Sample records for icebreaker life mission

  1. The Icebreaker Mission to Search for Life on Mars

    NASA Technical Reports Server (NTRS)

    Stoker, C.; Mckay, C.; Brinckerhoff, W.; Davila, A.; Parro, V.; Quinn, R.

    2015-01-01

    The search for evidence of life on Mars is the ultimate motivation for its scientific exploration. The results from the Phoenix mission indicate that the high N. latitude ice-rich regolith at low elevations is likely to be a recently habitable place on Mars [Stoker et al., 2010]. The near-surface ice likely provided adequate water activity during periods of high obliquity, 3 to 10 Myr ago. Carbon dioxide and nitrogen are present in the atmosphere, and nitrates may be present in the soil. Together with iron in basaltic rocks and perchlorate in the soil they provide carbon and energy sources, and oxidative power to drive metabolism. Furthermore, the presence of organics is possible, as thermally reactive perchlorate would have prevented their detection by Viking and Phoenix. The Mars Icebreaker Life mission [McKay et al., 2013] focuses on the following science goals: (1) Search for biomolecular evidence of life; (2) Search for organic matter from either exogeneous or endogeneous sources using methods that are not effected by the presence of perchlorate; (3) Characterize oxidative species that produced reactivity of soils seen by Viking; and 4) Assess the habitability of the ice bearing soils. The Icebreaker Life payload (Figure 1) includes a 1-m rotary percussive drill that brings cuttings samples to the surface where they are delivered to three instruments (Fig. 1), the Signs of Life Detector (SOLID) [Parro et al., 2011] for biomolecular analysis, Laser Desorption Mass Spectrometer (LDMS) [??? 2015]) for broad spectrum organic analysis, and Wet Chemistry Laboratory (WCL) [Hecht et al., 2009] for detecting soluble species of nutrients and reactive oxidants. The Icebreaker payload fits on the Phoenix spacecraft and can land at the well-characterized Phoe-nix landing site in 2020 in a Discovery-class mission.

  2. The Icebreaker Life Mission to Mars: A Search for Biomolecular Evidence for Life

    NASA Technical Reports Server (NTRS)

    Mckay, Christopher P.; Stoker, Carol R.; Glass, Brian J.; Dave, Arwen I.; Davila, Alfonso F.; Heldmann, Jennifer L.; Marinova, Margarita M.; Fairen, Alberto G; Quinn, Richard C; Zacny, Kris A.; hide

    2012-01-01

    The search for evidence of life on Mars is the primary motivation for the exploration of that planet. The results from previous missions, and the Phoenix mission in particular, indicate that the ice-cemented ground in the north polar plains is likely to be the most recently habitable place that is currently known on Mars. The near-surface ice likely provided adequate water activity during periods of high obliquity, 5 Myr ago. Carbon dioxide and nitrogen is present in the atmosphere, and nitrates may be present in the soil. Perchlorate in the soil together with iron in basaltic rock provides a possible energy source for life. Furthermore, the presence of organics must once again be considered, as the results of the Viking GCMS are now suspect given the discovery of the thermally reactive perchlorate. Ground-ice may provide a way to preserve organic molecules for extended periods of time, especially organic biomarkers. The Mars Icebreaker Life mission focuses on the following science goals: 1. Search for specific biomolecules that would be conclusive evidence of life. 2. A general search for organic molecules in the ground ice. 3. Determine the processes of ground ice formation and the role of liquid water. 4. Understand the mechanical properties of the Mars polar ice-cemented soil. 5. Assess the recent habitability of the environment with respect to required elements to support life, energy sources, and possible toxic elements. And 6. Compare the elemental composition of the northern plains with mid-latitude sites. The Icebreaker Life payload has been designed around the Phoenix spacecraft and is targeted to a site near the Phoenix landing site. However, the Icebreaker payload could be supported on other Mars landing systems. Preliminary studies of the SpaceX Dragon lander show that it could support the Icebreaker payload for a landing either at the Phoenix site or at mid-latitudes. Duplicate samples could be cached as a target for possible return by a Mars Sample

  3. The Icebreaker Life Mission to Mars: a search for biomolecular evidence for life.

    PubMed

    McKay, Christopher P; Stoker, Carol R; Glass, Brian J; Davé, Arwen I; Davila, Alfonso F; Heldmann, Jennifer L; Marinova, Margarita M; Fairen, Alberto G; Quinn, Richard C; Zacny, Kris A; Paulsen, Gale; Smith, Peter H; Parro, Victor; Andersen, Dale T; Hecht, Michael H; Lacelle, Denis; Pollard, Wayne H

    2013-04-01

    The search for evidence of life on Mars is the primary motivation for the exploration of that planet. The results from previous missions, and the Phoenix mission in particular, indicate that the ice-cemented ground in the north polar plains is likely to be the most recently habitable place that is currently known on Mars. The near-surface ice likely provided adequate water activity during periods of high obliquity, ≈ 5 Myr ago. Carbon dioxide and nitrogen are present in the atmosphere, and nitrates may be present in the soil. Perchlorate in the soil together with iron in basaltic rock provides a possible energy source for life. Furthermore, the presence of organics must once again be considered, as the results of the Viking GCMS are now suspect given the discovery of the thermally reactive perchlorate. Ground ice may provide a way to preserve organic molecules for extended periods of time, especially organic biomarkers. The Mars Icebreaker Life mission focuses on the following science goals: (1) Search for specific biomolecules that would be conclusive evidence of life. (2) Perform a general search for organic molecules in the ground ice. (3) Determine the processes of ground ice formation and the role of liquid water. (4) Understand the mechanical properties of the martian polar ice-cemented soil. (5) Assess the recent habitability of the environment with respect to required elements to support life, energy sources, and possible toxic elements. (6) Compare the elemental composition of the northern plains with midlatitude sites. The Icebreaker Life payload has been designed around the Phoenix spacecraft and is targeted to a site near the Phoenix landing site. However, the Icebreaker payload could be supported on other Mars landing systems. Preliminary studies of the SpaceX Dragon lander show that it could support the Icebreaker payload for a landing either at the Phoenix site or at midlatitudes. Duplicate samples could be cached as a target for possible return by

  4. The Sample Handling System for the Mars Icebreaker Life Mission: from Dirt to Data

    NASA Technical Reports Server (NTRS)

    Dave, Arwen; Thompson, Sarah J.; McKay, Christopher P.; Stoker, Carol R.; Zacny, Kris; Paulsen, Gale; Mellerowicz, Bolek; Glass, Brian J.; Wilson, David; Bonaccorsi, Rosalba; hide

    2013-01-01

    The Mars icebreaker life mission will search for subsurface life on mars. It consists of three payload elements: a drill to retrieve soil samples from approx. 1 meter below the surface, a robotic sample handling system to deliver the sample from the drill to the instruments, and the instruments themselves. This paper will discuss the robotic sample handling system.

  5. The sample handling system for the Mars Icebreaker Life mission: from dirt to data.

    PubMed

    Davé, Arwen; Thompson, Sarah J; McKay, Christopher P; Stoker, Carol R; Zacny, Kris; Paulsen, Gale; Mellerowicz, Bolek; Glass, Brian J; Willson, David; Bonaccorsi, Rosalba; Rask, Jon

    2013-04-01

    The Mars Icebreaker Life mission will search for subsurface life on Mars. It consists of three payload elements: a drill to retrieve soil samples from approximately 1 m below the surface, a robotic sample handling system to deliver the sample from the drill to the instruments, and the instruments themselves. This paper will discuss the robotic sample handling system. Collecting samples from ice-rich soils on Mars in search of life presents two challenges: protection of that icy soil--considered a "special region" with respect to planetary protection--from contamination from Earth, and delivery of the icy, sticky soil to spacecraft instruments. We present a sampling device that meets these challenges. We built a prototype system and tested it at martian pressure, drilling into ice-cemented soil, collecting cuttings, and transferring them to the inlet port of the SOLID2 life-detection instrument. The tests successfully demonstrated that the Icebreaker drill, sample handling system, and life-detection instrument can collectively operate in these conditions and produce science data that can be delivered via telemetry--from dirt to data. Our results also demonstrate the feasibility of using an air gap to prevent forward contamination. We define a set of six analog soils for testing over a range of soil cohesion, from loose sand to basalt soil, with angles of repose of 27° and 39°, respectively. Particle size is a key determinant of jamming of mechanical parts by soil particles. Jamming occurs when the clearance between moving parts is equal in size to the most common particle size or equal to three of these particles together. Three particles acting together tend to form bridges and lead to clogging. Our experiments show that rotary-hammer action of the Icebreaker drill influences the particle size, typically reducing particle size by ≈ 100 μm.

  6. Reaching 1 m deep on Mars: the Icebreaker drill.

    PubMed

    Zacny, K; Paulsen, G; McKay, C P; Glass, B; Davé, A; Davila, A F; Marinova, M; Mellerowicz, B; Heldmann, J; Stoker, C; Cabrol, N; Hedlund, M; Craft, J

    2013-12-01

    The future exploration of Mars will require access to the subsurface, along with acquisition of samples for scientific analysis and ground-truthing of water ice and mineral reserves for in situ resource utilization. The Icebreaker drill is an integral part of the Icebreaker mission concept to search for life in ice-rich regions on Mars. Since the mission targets Mars Special Regions as defined by the Committee on Space Research (COSPAR), the drill has to meet the appropriate cleanliness standards as requested by NASA's Planetary Protection Office. In addition, the Icebreaker mission carries life-detection instruments; and in turn, the drill and sample delivery system have to meet stringent contamination requirements to prevent false positives. This paper reports on the development and testing of the Icebreaker drill, a 1 m class rotary-percussive drill and triple redundant sample delivery system. The drill acquires subsurface samples in short, approximately 10 cm bites, which makes the sampling system robust and prevents thawing and phase changes in the target materials. Autonomous drilling, sample acquisition, and sample transfer have been successfully demonstrated in Mars analog environments in the Arctic and the Antarctic Dry Valleys, as well as in a Mars environmental chamber. In all environments, the drill has been shown to perform at the "1-1-100-100" level; that is, it drilled to 1 m depth in approximately 1 hour with less than 100 N weight on bit and approximately 100 W of power. The drilled substrate varied and included pure ice, ice-rich regolith with and without rocks and with and without 2% perchlorate, and whole rocks. The drill is currently at a Technology Readiness Level (TRL) of 5. The next-generation Icebreaker drill weighs 10 kg, which is representative of the flightlike model at TRL 5/6.

  7. Coast Guard Polar Icebreaker Modernization: Background and Issues for Congress

    DTIC Science & Technology

    2016-11-10

    time between the end of Polar Star’s current intended service life and the entry into service of one or more new heavy polar icebreakers. There are...at least two options for bridging this time period: One would be to further extend the service life of Polar Star and/or repair and extend the...service life of Polar Sea. The other would be to charter (i.e., lease) one or more other icebreakers (perhaps foreign- owned ones), if such ships are

  8. Coast Guard Polar Icebreaker Modernization: Background and Issues for Congress

    DTIC Science & Technology

    2013-04-25

    Accountability Office, Coast Guard[:]Efforts to Identify Arctic Requirements Are Ongoing, but More Communication about Agency Planning Efforts Would...control, and communications capabilities. The flexibility and mobility of polar icebreakers would assist the Coast Guard in closing future mission...Sea to prevent foreign fishing in U.S. waters and overfishing —Capability to conduct search and rescue in Beaufort Sea for cruise line and natural

  9. Icebreaker: The Evaluation

    ERIC Educational Resources Information Center

    Peerbhoy, Denise; Bourke, Cathriona

    2007-01-01

    Objective: To document young people's and teachers' responses to "Icebreaker", a Theatre in Education (TIE) performance exploring themes of sexual health and relationships, in relation to "Healthy Arts"' objectives. Design: Data reported here were part of a wider evaluation of a government funded scheme. Setting: Data was…

  10. New U.S. icebreaker to advance Arctic Marine Science

    NASA Astrophysics Data System (ADS)

    Swift, Jim; Clough, Lisa; Berkson, Jonathan; DuPree, George; Falkner, Kelly

    The decades-long planning for a U.S. icebreaking vessel dedicated to Arctic marine science reached its goal with the entry into service of the UGCGC Healy, a polar research vessel operated by the U.S. Coast Guard for the U.S. science community. The ship is named for Captain Michael A. Healy, a legendary figure of Alaskan history who served as commanding officer of the U.S. Revenue Cutters Corwin (1884-1885) and Bear (1886-1895).Healy is 128 m long, 25 m wide, displaces 14,900 metric tons, and traverses up to 1.4 m ice at 1.65 m s-1, propelled by two 11.1-MW AC synchronous motors fed from DC diesel electric engines through cycloconverters. Thus, Healy is more powerful and somewhat larger than the German polar research vessel Polarstern or the Canadian icebreaker Louis S. St-Laurent. Healy's power system responds quickly to the load changes common in icebreaking. The ship has a conventional icebreaker bow. The hull provides a sea-kindly ride and more stable work conditions in open water than do the U.S. Coast Guard Polar-class icebreakers. The ship is designed to work in any Arctic season.

  11. Energizers and Icebreakers for All Ages and Stages.

    ERIC Educational Resources Information Center

    Foster, Elizabeth Sabrinsky

    This book is intended to assist group leaders, teachers, counselors, and peer helpers in the development of relationships and active learning. The first chapter, "Icebreakers," begins with an overview that explains the nature, purpose, and importance of these activities. Icebreakers are used to help group members learn about each other in a…

  12. Ice-Breaking as a Useful Teaching Policy for Both Genders

    ERIC Educational Resources Information Center

    Yeganehpour, Parisa

    2017-01-01

    These days focus of interest in English learning changes to productive skills, in Turkey. This research study assesses the teachers' point of view about using ice-breakers for adult Turkish EFL learners in upper-intermediate level. It also anticipates finding valuable information with applying ice-breaker activities as a useful teaching policy…

  13. Embracing life-the Bethlehem Schools' Project, an "icebreaker" and "a foot in the door".

    PubMed

    Hocking, Mary

    2018-01-01

    This workshop details a Partnership involving a High school, a Hospital (Calvary Health Care Bethlehem), La Trobe University and Palliative Care Victoria which seeks to support Community Capacity and resilience in dealing with Life-Limiting illness, death, dying and Loss. This alliance has produced an educational resource which may be used, not only as a tool to normalize death, but also as a means of exploring 'keys to well-being' at any stage of life, through any loss or challenge. This workshop features a template which has been trialled, adapted and evaluated in High School, workshop and Hospital induction settings within Australia. Responses thus far have been "overwhelmingly positive". Translating evidence of positive outcomes into Education & Health Care Systems, is a challenge-this workshop offers a means of approaching both. The conclusion of the workshop provides a number of insights: (I) engaging communities in discussions about well-being and harnessing the insights of youth is a palatable means of discussing well-being at end-of-life; (II) what we know, as a community about supporting people with life-limiting illness is applicable across the span of life-not just at the end; (III) just as it takes a village to raise a child-it takes a village to ensure a quality end-of life experience. What began as a one-off hospital immersion for Secondary School students has grown to become a sustainable educational resource, applicable across a number of domains-with the capacity to become an evidence-based means of increasing community EOL capacity. This workshop details the evolution of a community partnership, which produced an evaluated, sustainable, educational resource encouraging conversations about death and loss whilst emphasizing the essentials of well-being. It is a potential "foot in the door" of the education system and an "ice-breaker" for new staff/students to Palliative care.

  14. Coast Guard Polar Icebreaker Modernization: Background and Issues for Congress

    DTIC Science & Technology

    2014-02-11

    Efforts to Identify Arctic Requirements Are Ongoing, but More Communication about Agency Planning Efforts Would Be Beneficial, GAO-10- 870, September...icebreakers also have substantial command, control, and communications capabilities. The flexibility and mobility of polar icebreakers would assist...Fisheries enforcement in Bering Sea to prevent foreign fishing in U.S. waters and overfishing —Capability to conduct search and rescue in Beaufort Sea

  15. Coast Guard Polar Icebreaker Modernization: Background and Issues for Congress

    DTIC Science & Technology

    2013-07-24

    but More Communication about Agency Planning Efforts Would Be Beneficial, GAO-10- 870, September 2010, p. 53. Coast Guard Polar Icebreaker...and helicopters. Polar icebreakers also have substantial command, control, and communications capabilities. The flexibility and mobility of polar...Coast Guard —Fisheries enforcement in Bering Sea to prevent foreign fishing in U.S. waters and overfishing —Capability to conduct search and rescue in

  16. Building Community in the Classroom through Ice-Breakers and Parting Ways

    ERIC Educational Resources Information Center

    Eggleston, Tami; Smith, Gabie

    2004-01-01

    Many instructors are concerned with creating a community in the classroom. Although there are numerous published "ice-breakers," many of these techniques are not specific to psychology courses or have been used so much that the students see them as redundant and cliche. Icebreakers are better if they have relevance to a specific class, are…

  17. Open-Water Resistance and Seakeeping Characteristics of Ships with Icebreaking Bows

    DTIC Science & Technology

    1991-05-13

    of a Knuckled Forefoot on a Typical Icebreaker ...... ................... . 19 3-2. Lines Plan, T-AGS OCEAN (ICE) . * * .... . 23 3-3. Curve of...the ice. As the stem strikes the ice, initial failure of the ice occurs by simple crushing. Then the raked stem of the icebreaker rides up onto the ice...bossings, skegs, rudders, 18 and special stem forefoot shapes were not included in the shapes tested. To ensure that the parent and its variants

  18. Life sciences interests in Mars missions

    NASA Technical Reports Server (NTRS)

    Rummel, John D.; Griffiths, Lynn D.

    1989-01-01

    NASA's Space Life Sciences research permeates plans for Mars missions and the rationale for the exploration of the planet. The Space Life Sciences program has three major roles in Mars mission studies: providing enabling technology for piloted missions, conducting scientific exploration related to the origin and evolution of life, and protecting space crews from the adverse physiological effects of space flight. This paper presents a rationale for exploration and some of the issues, tradeoffs, and visions being addressed in the Space Life Sciences program in preparation for Mars missions.

  19. Extended mission life support systems

    NASA Technical Reports Server (NTRS)

    Quattrone, P. D.

    1985-01-01

    Extended manned space missions which include interplanetary missions require regenerative life support systems. Manned mission life support considerations are placed in perspective and previous manned space life support system technology, activities and accomplishments in current supporting research and technology (SR&T) programs are reviewed. The life support subsystem/system technologies required for an enhanced duration orbiter (EDO) and a space operations center (SOC), regenerative life support functions and technology required for manned interplanetary flight vehicles, and future development requirements are outlined. The Space Shuttle Orbiters (space transportation system) is space cabin atmosphere is maintained at Earth ambient pressure of 14.7 psia (20% O2 and 80% N2). The early Shuttle flights will be seven-day flights, and the life support system flight hardware will still utilize expendables.

  20. Designing a Maintainable and Sustainable Coast Guard Icebreaker for Arctic and Antarctic Operations

    DTIC Science & Technology

    2014-03-21

    03-2014 Technical June 2013-August 2013 Designing a Maintainable and Sustainable Coast Guard Icebreaker for Arctic and Antarctic Operations...of Engineering Designing a Maintainable and Sustainable Coast Guard Icebreaker for Arctic and Antarctic Operations Abstract The U.S. Coast Guard is...Pollution (MARPOL) of which Annex V prohibits the discharge of solid waste other than food refuge less than 25mm in diameter into the Antarctic Region [6

  1. Life sciences flight experiments program mission science requirements document. The first life sciences dedicated Spacelab mission, part 1

    NASA Technical Reports Server (NTRS)

    Rummel, J. A.

    1982-01-01

    The Mission Science Requirements Document (MSRD) for the First Dedicated Life Sciences Mission (LS-1) represents the culmination of thousands of hours of experiment selection, and science requirement definition activities. NASA life sciences has never before attempted to integrate, both scientifically and operationally, a single mission dedicated to life sciences research, and the complexity of the planning required for such an endeavor should be apparent. This set of requirements completes the first phase of a continual process which will attempt to optimize (within available programmatic and mission resources) the science accomplished on this mission.

  2. ICESCAPE Mission

    NASA Image and Video Library

    2010-07-08

    Dartmouth College's Chris Polashenski cuts a block of ice from below a melt pond on sea ice in the Chukchi Sea on July 9, 2010, for analysis upon return from the mission. The research is part of NASA's ICESCAPE mission onboard the U.S. Coast Guard icebreaker Healy to sample the physical, chemical and biological characteristics of the ocean and sea ice. Impacts of Climate change on the Eco-Systems and Chemistry of the Arctic Pacific Environment (ICESCAPE) is a multi-year NASA shipborne project. The bulk of the research will take place in the Beaufort and Chukchi Sea’s in summer of 2010 and fall of 2011. Photo Credit: (NASA/Kathryn Hansen)

  3. Icebreaker-3 Drill Integration and Testing at Two Mars-Analog Sites

    NASA Technical Reports Server (NTRS)

    Glass, B.; Bergman, D.; Yaggi, B.; Dave, A.; Zacny, K.

    2016-01-01

    A decade of evolutionary development of integrated automated drilling and sample handling at analog sites and in test chambers has made it possible to go 1 meter through hard rocks and ice layers on Mars. The latest Icebreaker-3 drill has been field tested in 2014 at the Haughton Crater Marsanalog site in the Arctic and in 2015 with a Mars lander mockup in Rio Tinto, Spain, (with sample transfer arm and with a prototype life-detection instrument). Tests in Rio Tinto in 2015 successfully demonstrated that the drill sample (cuttings) was handed-off from the drill to the sample transfer arm and thence to the on-deck instrument inlet where it was taken in and analyzed ("dirt-to-data").

  4. Using Appreciative Intelligence for Ice-Breaking: A New Design

    ERIC Educational Resources Information Center

    Verma, Neena; Pathak, Anil Anand

    2011-01-01

    Purpose: The purpose of this paper is to highlight the importance of applying appreciative intelligence and appreciative inquiry concepts to design a possibly new model of ice-breaking, which is strengths-based and very often used in any training in general and team building training in particular. Design/methodology/approach: The design has…

  5. The first dedicated life sciences Spacelab mission

    NASA Technical Reports Server (NTRS)

    Perry, T. W.; Rummel, J. A.; Griffiths, L. D.; White, R. J.; Leonard, J. I.

    1984-01-01

    JIt is pointed out that the Shuttle-borne Spacelab provides the capability to fly large numbers of life sciences experiments, to retrieve and rescue experimental equipment, and to undertake multiple-flight studies. A NASA Life Sciences Flight Experiments Program has been organized with the aim to take full advantages of this capability. A description is provided of the scientific aspects of the most ambitious Spacelab mission currently being conducted in connection with this program, taking into account the First Dedicated Life Sciences Spacelab Mission. The payload of this mission will contain the equipment for 24 separate investigations. It is planned to perform the mission on two separate seven-day Spacelab flights, the first of which is currently scheduled for early 1986. Some of the mission objectives are related to the study of human and animal responses which occur promptly upon achieving weightlessness.

  6. Kick-Start Your Class: Academic Icebreakers to Engage Students

    ERIC Educational Resources Information Center

    Johnson, LouAnne

    2012-01-01

    LouAnne Johnson's newest book is a collection of fun and simple educational icebreaker activities that get students excited and engaged from the very first minute of class. These activities are great to use with students at all levels, and many of the activities include variations and modifications for different groups. Research has shown that the…

  7. ICESCAPE Mission

    NASA Image and Video Library

    2010-07-03

    Teams of scientists set up equipment on sea ice not far from the U.S. Coast Guard icebreaker Healy in the Chukchi Sea on July 4, 2010, where they spent the day collecting data. The research is part of NASA's ICESCAPE oceanographic mission to sample the physical, chemical and biological characteristics of the ocean and sea ice. Impacts of Climate change on the Eco-Systems and Chemistry of the Arctic Pacific Environment (ICESCAPE) is a multi-year NASA shipborne project. The bulk of the research will take place in the Beaufort and Chukchi Sea’s in summer of 2010 and fall of 2011. Photo Credit: (NASA/Kathryn Hansen)

  8. Life support approaches for Mars missions

    NASA Astrophysics Data System (ADS)

    Drysdale, A. E.; Ewert, M. K.; Hanford, A. J.

    Life support approaches for Mars missions are evaluated using an equivalent system mass (ESM) approach, in which all significant costs are converted into mass units. The best approach, as defined by the lowest mission ESM, depends on several mission parameters, notably duration, environment and consequent infrastructure costs, and crew size, as well as the characteristics of the technologies which are available. Generally, for the missions under consideration, physicochemical regeneration is most cost effective. However, bioregeneration is likely to be of use for producing salad crops for any mission, for producing staple crops for medium duration missions, and for most food, air and water regeneration for long missions (durations of a decade). Potential applications of in situ resource utilization need to be considered further.

  9. 76 FR 17621 - Biotech Life Science Trade Mission to China

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-03-30

    ... DEPARTMENT OF COMMERCE International Trade Administration Biotech Life Science Trade Mission to... Commercial Service (CS) is organizing a Biotechnology Life Sciences trade mission to China on October 17-20... representatives from a variety of U.S. biotechnology and life science firms and trade organizations. The mission...

  10. 77 FR 35353 - Biotech Life Sciences Trade Mission to Australia

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-06-13

    ... DEPARTMENT OF COMMERCE International Trade Administration Biotech Life Sciences Trade Mission to... Commercial Service (CS) is organizing a Biotech Life Sciences trade mission to Australia, October 29-November.... biotechnology and life science firms. The goals of the trade mission to Australia are to (1) increase U.S...

  11. Life support approaches for Mars missions

    NASA Technical Reports Server (NTRS)

    Drysdale, A. E.; Ewert, M. K.; Hanford, A. J.

    2003-01-01

    Life support approaches for Mars missions are evaluated using an equivalent system mass (ESM) approach, in which all significant costs are converted into mass units. The best approach, as defined by the lowest mission ESM, depends on several mission parameters, notably duration, environment and consequent infrastructure costs, and crew size, as well as the characteristics of the technologies which are available. Generally, for the missions under consideration, physicochemical regeneration is most cost effective. However, bioregeneration is likely to be of use for producing salad crops for any mission, for producing staple crops for medium duration missions, and for most food, air and water regeneration for long missions (durations of a decade). Potential applications of in situ resource utilization need to be considered further. c2002 Published by Elsevier Science Ltd on behalf of COSPAR.

  12. Life support approaches for Mars missions.

    PubMed

    Drysdale, A E; Ewert, M K; Hanford, A J

    2003-01-01

    Life support approaches for Mars missions are evaluated using an equivalent system mass (ESM) approach, in which all significant costs are converted into mass units. The best approach, as defined by the lowest mission ESM, depends on several mission parameters, notably duration, environment and consequent infrastructure costs, and crew size, as well as the characteristics of the technologies which are available. Generally, for the missions under consideration, physicochemical regeneration is most cost effective. However, bioregeneration is likely to be of use for producing salad crops for any mission, for producing staple crops for medium duration missions, and for most food, air and water regeneration for long missions (durations of a decade). Potential applications of in situ resource utilization need to be considered further. c2002 Published by Elsevier Science Ltd on behalf of COSPAR.

  13. Spacelab life sciences 2 post mission report

    NASA Technical Reports Server (NTRS)

    Buckey, Jay C.

    1994-01-01

    Jay C. Buckey, M.D., Assistant Professor of Medicine at The University of Texas Southwestern Medical Center at Dallas served as an alternate payload specialist astronaut for the Spacelab Life Sciences 2 Space Shuttle Mission from January 1992 through December 1993. This report summarizes his opinions on the mission and offers suggestions in the areas of selection, training, simulations, baseline data collection and mission operations. The report recognizes the contributions of the commander, payload commander and mission management team to the success of the mission. Dr. Buckey's main accomplishments during the mission are listed.

  14. LIFE: Enceladus Sample Return Mission Concept for Searching Evidence of Life

    NASA Technical Reports Server (NTRS)

    Tsou, P.; Brownlee, D. E.; McKay, C. P.; Beegle, L. W.; Spilker, L.; Kanik, I.

    2011-01-01

    One of the most promising targets for the search for life other than Mars in our Solar System is the tiny Saturn moon Enceladus. The Cassini mission to the Saturian system detected an active region on Enceladus where small water particles and gas containing organic materials were being flung into space from a region near the south pole known as the tiger stripes. This discovery indicated that there is very likely a liquid subsurface ocean heated through tidal interactions as Enceladus orbits Saturn. On Earth, whenever there is an energy source, liquid water and organics, there is life; this makes Enceladus one of the prime candidates for a search for life missions. In this presentation, we describe LIFE (Life Investigation For Enceladus) sample return concept from Enceladus in the search for evidence of life.

  15. Spacelab Life Sciences 1 - Dedicated life sciences mission

    NASA Technical Reports Server (NTRS)

    Womack, W. D.

    1990-01-01

    The Spacelab Life Sciences 1 (SLS-1) mission is discussed, and an overview of the SLS-1 Spacelab configuration is shown. Twenty interdisciplinary experiments, planned for this mission, are intended to explore the early stages of human and animal physiological adaptation to space flight conditions. Biomedical and gravitational biology experiments include cardiovascular and cardiopulmonary deconditioning, altered vestibular functions, altered metabolic functions (including altered fluid-electrolyte regulation), muscle atrophy, bone demineralization, decreased red blood cell mass, and altered immunologic responses.

  16. ICESCAPE Mission

    NASA Image and Video Library

    2010-07-03

    Scientists on the sea ice in the Chukchi Sea off the north coast of Alaska disperse equipment on July 4, 2010, as they prepare to collect data on and below the ice. The research is part of NASA's ICESCAPE mission onboard the U.S. Coast Guard icebreaker Healy to sample the physical, chemical and biological characteristics of the ocean and sea ice. Impacts of Climate change on the Eco-Systems and Chemistry of the Arctic Pacific Environment (ICESCAPE) is a multi-year NASA shipborne project. The bulk of the research will take place in the Beaufort and Chukchi Sea’s in summer of 2010 and fall of 2011. Photo Credit: (NASA/Kathryn Hansen)

  17. ICESCAPE Mission

    NASA Image and Video Library

    2010-07-08

    Scientists and Coast Guard swimmers test the integrity a melt pond on sea ice in the Chukchi Sea on July 9, 2010, before drilling holes through which instruments can be deployed to collect data. The research is part of NASA's ICESCAPE mission onboard the U.S. Coast Guard icebreaker Healy to sample the physical, chemical and biological characteristics of the ocean and sea ice. Impacts of Climate change on the Eco-Systems and Chemistry of the Arctic Pacific Environment (ICESCAPE) is a multi-year NASA shipborne project. The bulk of the research will take place in the Beaufort and Chukchi Sea’s in summer of 2010 and fall of 2011. Photo Credit: (NASA/Kathryn Hansen)

  18. Life sciences experiments in the first Spacelab mission

    NASA Technical Reports Server (NTRS)

    Huffstetler, W. J.; Rummel, J. A.

    1978-01-01

    The development of the Shuttle Transportation System (STS) by the United States and the Spacelab pressurized modules and pallets by the European Space Agency (ESA) presents a unique multi-mission space experimentation capability to scientists and researchers of all disciplines. This capability is especially pertinent to life scientists involved in all areas of biological and behavioral research. This paper explains the solicitation, evaluation, and selection process involved in establishing life sciences experiment payloads. Explanations relative to experiment hardware development, experiment support hardware (CORE) concepts, hardware integration and test, and concepts of direct Principal Investigator involvement in the missions are presented as they are being accomplished for the first Spacelab mission. Additionally, discussions of future plans for life sciences dedicated Spacelab missions are included in an attempt to define projected capabilities for space research in the 1980s utilizing the STS.

  19. AURORA BOREALIS - Development of a New Research Icebreaker with Drilling Capability

    NASA Astrophysics Data System (ADS)

    Thiede, J.; Biebow, N.; Egerton, P.; Kunz-Pirrung, M.; Lembke-Jene, L.

    2007-12-01

    Polar research both on land and in the sea cannot achieve the needed progress without novel and state of the art technologies and infrastructure. In addition, we have the obligation to equip the upcoming young and courageous generation of polar researchers with the most modern and safest research platforms the 21st century can provide. This effort will require major investments, both in terms of generating new tools, as well as maintaining and renovating existing infrastructure. There are many different novel tools under development for polar research, we will concentrate on the presently largest one, the planning for a new type of research icebreaker, the AURORA BOREALIS with an all-season capability of operations in permanently ice-covered waters and with the possibility to carry out deep-sea drilling in ice-covered deep-sea basins. AURORA BOREALIS will be the most advanced Polar Research Vessel in the world with a multi-functional role of drilling in deep ocean basins and supporting climate and environmental research and decision support for stakeholder governments for the next 35 to 40 years. The vessel is planned as a large research icebreaker with 44,000 tons displacement and a length of up to 196 m, with about 50 Megawatt propulsion power. Advanced technological features will include azimuth propulsion systems, extensive instrumental and airborne ice- management support, and the routine operation of Remotely Operated Vehicles (ROV) and Autonomous Underwater Vehicles (AUVs) from two moon-pools. An unique feature of this icebreaker will be the drilling rig that will enable sampling of the ocean floor and sub-sea down to 5000 m water depth and 1000 m penetration at the most inhospitable places on earth. The possibility to flexibly equip the ship with laboratory and supply containers, and the variable arrangement of other modular infrastructure (in particular, winches, cranes, etc.), free deck- space, and separate protected deck areas, will allow the planned

  20. Systems Analysis of Life Support for Long-Duration Missions

    NASA Technical Reports Server (NTRS)

    Drysdale, Alan E.; Maxwell, Sabrina; Ewert, Michael K.; Hanford, Anthony J.

    2000-01-01

    Work defining advanced life support (ALS) technologies and evaluating their applicability to various long-duration missions has continued. Time-dependent and time-invariant costs have been estimated for a variety of life support technology options, including International Space Station (ISS) environmental control and life support systems (ECLSS) technologies and improved options under development by the ALS Project. These advanced options include physicochemical (PC) and bioregenerative (BIO) technologies, and may in the future include in-situ resource utilization (ISRU) in an attempt to reduce both logistics costs and dependence on supply from Earth. PC and bioregenerative technologies both provide possibilities for reducing mission equivalent system mass (ESM). PC technologies are most advantageous for missions of up to several years in length, while bioregenerative options are most appropriate for longer missions. ISRU can be synergistic with both PC and bioregenerative options.

  1. LIFE: Life Investigation For Enceladus A Sample Return Mission Concept in Search for Evidence of Life.

    PubMed

    Tsou, Peter; Brownlee, Donald E; McKay, Christopher P; Anbar, Ariel D; Yano, Hajime; Altwegg, Kathrin; Beegle, Luther W; Dissly, Richard; Strange, Nathan J; Kanik, Isik

    2012-08-01

    Life Investigation For Enceladus (LIFE) presents a low-cost sample return mission to Enceladus, a body with high astrobiological potential. There is ample evidence that liquid water exists under ice coverage in the form of active geysers in the "tiger stripes" area of the southern Enceladus hemisphere. This active plume consists of gas and ice particles and enables the sampling of fresh materials from the interior that may originate from a liquid water source. The particles consist mostly of water ice and are 1-10 μ in diameter. The plume composition shows H(2)O, CO(2), CH(4), NH(3), Ar, and evidence that more complex organic species might be present. Since life on Earth exists whenever liquid water, organics, and energy coexist, understanding the chemical components of the emanating ice particles could indicate whether life is potentially present on Enceladus. The icy worlds of the outer planets are testing grounds for some of the theories for the origin of life on Earth. The LIFE mission concept is envisioned in two parts: first, to orbit Saturn (in order to achieve lower sampling speeds, approaching 2 km/s, and thus enable a softer sample collection impact than Stardust, and to make possible multiple flybys of Enceladus); second, to sample Enceladus' plume, the E ring of Saturn, and the Titan upper atmosphere. With new findings from these samples, NASA could provide detailed chemical and isotopic and, potentially, biological compositional context of the plume. Since the duration of the Enceladus plume is unpredictable, it is imperative that these samples are captured at the earliest flight opportunity. If LIFE is launched before 2019, it could take advantage of a Jupiter gravity assist, which would thus reduce mission lifetimes and launch vehicle costs. The LIFE concept offers science returns comparable to those of a Flagship mission but at the measurably lower sample return costs of a Discovery-class mission.

  2. A life sciences Spacelab mission simulation

    NASA Technical Reports Server (NTRS)

    Mason, J. A.; Musgrave, F. S.; Morrison, D. R.

    1977-01-01

    The paper describes the purposes of a seven-day simulated life-sciences mission conducted in a Spacelab simulator. A major objective was the evaluation of in-orbit Spacelab operations and those mission control support functions which will be required from the Payload Operations Center. Tested equipment and procedures included experiment racks, common operational research equipment, commercial off-the-shelf equipment, experiment hardware interfaces with Spacelab, experiment data handling concepts, and Spacelab trash management.

  3. Exploration Life Support Critical Questions for Future Human Space Missions

    NASA Technical Reports Server (NTRS)

    Kwert, Michael K.; Barta, Daniel J.; McQuillan, Jeff

    2010-01-01

    Exploration Life Support (ELS) is a current project under NASA's Exploration Systems Mission Directorate. The ELS Project plans, coordinates and implements the development of advanced life support technologies for human exploration missions in space. Recent work has focused on closed loop atmosphere and water systems for long duration missions, including habitats and pressurized rovers. But, what are the critical questions facing life support system developers for these and other future human missions? This paper explores those questions and how progress in the development of ELS technologies can help answer them. The ELS Project includes the following Elements: Atmosphere Revitalization Systems, Water Recovery Systems, Waste Management Systems, Habitation Engineering, Systems Integration, Modeling and Analysis, and Validation and Testing, which includes the Sub-Elements Flight Experiments and Integrated Testing. Systems engineering analysis by ELS seeks to optimize overall mission architectures by considering all the internal and external interfaces of the life support system and the potential for reduction or reuse of commodities. In particular, various sources and sinks of water and oxygen are considered along with the implications on loop closure and the resulting launch mass requirements. Systems analysis will be validated through the data gathered from integrated testing, which will demonstrate the interfaces of a closed loop life support system. By applying a systematic process for defining, sorting and answering critical life support questions, the ELS project is preparing for a variety of future human space missions

  4. Zones of impact around icebreakers affecting beluga whales in the Beaufort Sea.

    PubMed

    Erbe, C; Farmer, D M

    2000-09-01

    A software model estimating zones of impact on marine mammals around man-made noise [C. Erbe and D. M. Farmer, J. Acoust. Soc. Am. 108, 1327-1331 (2000)] is applied to the case of icebreakers affecting beluga whales in the Beaufort Sea. Two types of noise emitted by the Canadian Coast Guard icebreaker Henry Larsen are analyzed: bubbler system noise and propeller cavitation noise. Effects on beluga whales are modeled both in a deep-water environment and a near-shore environment. The model estimates that the Henry Larsen is audible to beluga whales over ranges of 35-78 km, depending on location. The zone of behavioral disturbance is only slightly smaller. Masking of beluga communication signals is predicted within 14-71-km range. Temporary hearing damage can occur if a beluga stays within 1-4 km of the Henry Larsen for at least 20 min. Bubbler noise impacts over the short ranges quoted; propeller cavitation noise accounts for all the long-range effects. Serious problems can arise in heavily industrialized areas where animals are exposed to ongoing noise and where anthropogenic noise from a variety of sources adds up.

  5. AURORA BOREALIS - European Research Icebreaker With Drilling Capability

    NASA Astrophysics Data System (ADS)

    Biebow, N.; Lembke-Jene, L.; Kunz-Pirrung, M.; Thiede, J.

    2008-12-01

    The polar oceans are the least known areas of the globe, in although they hold the key to many of our climate´s secrets. How does the sea ice coverage and the sea water properties change? How do plants and animals survive under the most extreme conditions of the earth? Which information of past climate change can be read from the sediments at the sea-floor and how can the future changing climate be predicted? In order to answer such and further questions, for the moment a hypermodern research vessel, the AURORA BOREALIS, is planned, which can handle the cool summers and freezing winters of the polar oceans and which can drill deep into the sea floor. AURORA BOREALIS will be the most advanced Research Icebreaker in the world with a multi-functional role of drilling in deep ocean basins and supporting climate/environmental research and decision support for stakeholder governments for the next 35-40 years. It will have a high icebreaking capacity to penetrate autonomously (single ship operation) into the central Arctic Ocean with more than 2.5 meters of ice cover, during all seasons of the year. The new technological features will include dynamic positioning in closed sea- ice cover, satellite navigation and ice-management support and the deployment and operation of Remotely Operated Vehicles (ROV) and Autonomous Underwater Vehicles (AUVs) from the twin moon-pools. A unique feature of the vessel is the deep-sea drilling rig, which will enable sampling of the ocean floor and sub-sea up to 5000 m water and 1000 m penetration at the most inhospitable places on earth. The drilling capability will be deployed in both Polar Regions on the long run and AURORA BOREALIS will be the only vessel worldwide that could undertake this type of scientific investigation.

  6. Spacelab Life Science-1 Mission Onboard Photograph

    NASA Technical Reports Server (NTRS)

    1991-01-01

    The laboratory module in the cargo bay of the Space Shuttle Orbiter Columbia was photographed during the Spacelab Life Science-1 (SLS-1) mission. SLS-1 was the first Spacelab mission dedicated solely to life sciences. The main purpose of the SLS-1 mission was to study the mechanisms, magnitudes, and time courses of certain physiological changes that occur during space flight, to investigate the consequences of the body's adaptation to microgravity and readjustment to Earth's gravity, and to bring the benefits back home to Earth. The mission was designed to explore the responses of the heart, lungs, blood vessels, kidneys, and hormone-secreting glands to microgravity and related body fluid shifts; examine the causes of space motion sickness; and study changes in the muscles, bones and cells. The five body systems being studied were: The Cardiovascular/Cardiopulmonary System (heart, lungs, and blood vessels), the Renal/Endocrine System (kidney and hormone-secreting organs), the Immune System (white blood cells), the Musculoskeletal System (muscles and bones), and the Neurovestibular System (brain and nerves, eyes, and irner ear). The SLS-1 was launched aboard the Space Shuttle Orbiter Columbia (STS-40) on June 5, 1995.

  7. Improving Life-Cycle Cost Management of Spacecraft Missions

    NASA Technical Reports Server (NTRS)

    Clardy, Dennon

    2010-01-01

    This presentation will explore the results of a recent NASA Life-Cycle Cost study and how project managers can use the findings and recommendations to improve planning and coordination early in the formulation cycle and avoid common pitfalls resulting in cost overruns. The typical NASA space science mission will exceed both the initial estimated and the confirmed life-cycle costs by the end of the mission. In a fixed-budget environment, these overruns translate to delays in starting or launching future missions, or in the worst case can lead to cancelled missions. Some of these overruns are due to issues outside the control of the project; others are due to the unpredictable problems (unknown unknowns) that can affect any development project. However, a recent study of life-cycle cost growth by the Discovery and New Frontiers Program Office identified a number of areas that are within the scope of project management to address. The study also found that the majority of the underlying causes for cost overruns are embedded in the project approach during the formulation and early design phases, but the actual impacts typically are not experienced until late in the project life cycle. Thus, project management focus in key areas such as integrated schedule development, management structure and contractor communications processes, heritage and technology assumptions, and operations planning, can be used to validate initial cost assumptions and set in place management processes to avoid the common pitfalls resulting in cost overruns.

  8. Spacelab mission 4 - The first dedicated life sciences mission

    NASA Technical Reports Server (NTRS)

    Perry, T. W.; Reid, D. H.

    1983-01-01

    Plans for the first Spacelab-4 mission dedicated entirely to the life sciences, are reviewed. The thrust of the scientific mission scheduled for late 1985 will be to study the acute effects of weightlessness on living systems, particularly humans. The payload of the Spacelab compartment will contain 24 experiments of which approximately half will involve humans. Among the major areas of interest are cardiovascular and pulmonary function, vestibular function, renal and endocrine physiology, hematology, nitrogen balance, immunological function, the gravitational biology of plants, inflight fertilization of frogs' eggs and the effects of zero gravity on monkeys and rats. In selecting the array of experiments an effort was made to combine investigations with complementary scientific objectives to develop animal models of human biological problems.

  9. Life sciences - On the critical path for missions of exploration

    NASA Technical Reports Server (NTRS)

    Sulzman, Frank M.; Connors, Mary M.; Gaiser, Karen

    1988-01-01

    Life sciences are important and critical to the safety and success of manned and long-duration space missions. The life science issues covered include gravitational physiology, space radiation, medical care delivery, environmental maintenance, bioregenerative systems, crew and human factors within and outside the spacecraft. The history of the role of life sciences in the space program is traced from the Apollo era, through the Skylab era to the Space Shuttle era. The life science issues of the space station program and manned missions to the moon and Mars are covered.

  10. Future Marine Polar Research Capacities - Science Planning and Research Services for a Multi-National Research Icebreaker

    NASA Astrophysics Data System (ADS)

    Biebow, N.; Lembke-Jene, L.; Wolff-Boenisch, B.; Bergamasco, A.; De Santis, L.; Eldholm, O.; Mevel, C.; Willmott, V.; Thiede, J.

    2011-12-01

    Despite significant advances in Arctic and Antarctic marine science over the past years, the polar Southern Ocean remains a formidable frontier due to challenging technical and operational requirements. Thus, key data and observations from this important region are still missing or lack adequate lateral and temporal coverage, especially from time slots outside optimal weather seasons and ice conditions. These barriers combined with the obligation to efficiently use financial resources and funding for expeditions call for new approaches to create optimally equipped, but cost-effective infrastructures. These must serve the international science community in a dedicated long-term mode and enable participation in multi-disciplinary expeditions, with secured access to optimally equipped marine platforms for world-class research in a wide range of Antarctic science topics. The high operational and technical performance capacity of a future joint European Research Icebreaker and Deep-sea Drilling Vessel (the AURORA BOREALIS concept) aims at integrating still separately operating national science programmes with different strategic priorities into joint development of long-term research missions with international cooperation both in Arctic and Antarctica. The icebreaker is planned to enable, as a worldwide first, autonomous year-round operations in the central Arctic and polar Southern Ocean, including severest ice conditions in winter, and serving all polar marine disciplines. It will facilitate the implementation of atmospheric, oceanographic, cryospheric or geophysical observatories for long-term monitoring of the polar environment. Access to the biosphere and hydrosphere e.g. beneath ice shelves or in remote regions is made possible by acting as advanced deployment platform for instruments, robotic and autonomous vehicles and ship-based air operations. In addition to a report on the long-term strategic science and operational planning objectives, we describe foreseen

  11. Computer Simulation of Great Lakes-St. Lawrence Seaway Icebreaker Requirements.

    DTIC Science & Technology

    1980-01-01

    of Run No. 1 for Taconite Task Command ... ....... 6-41 6.22d Results of Run No. I for Oil Can Task Command ........ ... 6-42 6.22e Results of Run No...Port and Period for Run No. 2 ... .. ... ... 6-47 6.23c Results of Run No. 2 for Taconite Task Command ... ....... 6-48 6.23d Results of Run No. 2 for...6-53 6.24b Predicted Icebreaker Fleet by Home Port and Period for Run No. 3 6-54 6.24c Results of Run No. 3 for Taconite Task Command. ....... 6

  12. Exploration Life Support Technology Development for Lunar Missions

    NASA Technical Reports Server (NTRS)

    Ewert, Michael K.; Barta, Daniel J.; McQuillan, Jeffrey

    2009-01-01

    Exploration Life Support (ELS) is one of NASA's Exploration Technology Development Projects. ELS plans, coordinates and implements the development of new life support technologies for human exploration missions as outlined in NASA's Vision for Space Exploration. ELS technology development currently supports three major projects of the Constellation Program - the Orion Crew Exploration Vehicle (CEV), the Altair Lunar Lander and Lunar Surface Systems. ELS content includes Air Revitalization Systems (ARS), Water Recovery Systems (WRS), Waste Management Systems (WMS), Habitation Engineering, Systems Integration, Modeling and Analysis (SIMA), and Validation and Testing. The primary goal of the ELS project is to provide different technology options to Constellation which fill gaps or provide substantial improvements over the state-of-the-art in life support systems. Since the Constellation missions are so challenging, mass, power, and volume must be reduced from Space Shuttle and Space Station technologies. Systems engineering analysis also optimizes the overall architecture by considering all interfaces with the life support system and potential for reduction or reuse of resources. For long duration missions, technologies which aid in closure of air and water loops with increased reliability are essential as well as techniques to minimize or deal with waste. The ELS project utilizes in-house efforts at five NASA centers, aerospace industry contracts, Small Business Innovative Research contracts and other means to develop advanced life support technologies. Testing, analysis and reduced gravity flight experiments are also conducted at the NASA field centers. This paper gives a current status of technologies under development by ELS and relates them to the Constellation customers who will eventually use them.

  13. CELSS and regenerative life support for manned missions to MARS

    NASA Technical Reports Server (NTRS)

    Mcelroy, R. D.

    1986-01-01

    In the mid 1990's, the space station will become a point from which inter-planetary vehicles can be launched. The practicalities of a manned Mars mission are now being studied, along with some newer concepts for human life support. Specifically, the use of organisms such as plants and algae as the basis for life support systems is now being actively considered. A Controlled Ecological Life Support System (CELSS) is composed of several facilities: (1) to grow photosynthetic plants or algae which will produce food, oxygen and potable water, and remove carbon dioxide exhaled by a crew; (2) to process biomass into food; (3) to oxidize organic wastes into CO2; and (4) to maintain system operation and stability. Such a system, when compared to using materials stored at launch, may have distinct weight and cost advantages, depending upon crew size and mission duration, as well as psychological benefits for the crew. The use of the system during transit, as well as in establishing a re-visitable surface camp, will increase the attractiveness of the CELSS concept for life support on interplanetary missions.

  14. Exploration Life Support Critical Questions for Future Human Space Missions

    NASA Technical Reports Server (NTRS)

    Ewert, Michael K.; Barta, Daniel J.; McQuillan, Jeff

    2009-01-01

    Exploration Life Support (ELS) is a project under NASA s Exploration Technology Development Program. The ELS Project plans, coordinates and implements the development of advanced life support technologies for human exploration missions in space. Recent work has focused on closed loop atmosphere and water systems for a lunar outpost, including habitats and pressurized rovers. But, what are the critical questions facing life support system developers for these and other future human missions? This paper explores those questions and discusses how progress in the development of ELS technologies can help answer them. The ELS Project includes Atmosphere Revitalization Systems (ARS), Water Recovery Systems (WRS), Waste Management Systems (WMS), Habitation Engineering, Systems Integration, Modeling and Analysis (SIMA), and Validation and Testing, which includes the sub-elements Flight Experiments and Integrated Testing. Systems engineering analysis by ELS seeks to optimize the overall mission architecture by considering all the internal and external interfaces of the life support system and the potential for reduction or reuse of commodities. In particular, various sources and sinks of water and oxygen are considered along with the implications on loop closure and the resulting launch mass requirements.

  15. Spacelab Life Science-1 Mission Onboard Photograph

    NASA Technical Reports Server (NTRS)

    1995-01-01

    Spacelab Life Science -1 (SLS-1) was the first Spacelab mission dedicated solely to life sciences. The main purpose of the SLS-1 mission was to study the mechanisms, magnitudes, and time courses of certain physiological changes that occur during space flight, to investigate the consequences of the body's adaptation to microgravity and readjustment to Earth's gravity, and bring the benefits back home to Earth. The mission was designed to explore the responses of the heart, lungs, blood vessels, kidneys, and hormone-secreting glands to microgravity and related body fluid shifts; examine the causes of space motion sickness; and study changes in the muscles, bones, and cells. This photograph shows astronaut Rhea Seddon conducting an inflight study of the Cardiovascular Deconditioning experiment by breathing into the cardiovascular rebreathing unit. This experiment focused on the deconditioning of the heart and lungs and changes in cardiopulmonary function that occur upon return to Earth. By using noninvasive techniques of prolonged expiration and rebreathing, investigators can determine the amount of blood pumped out of the heart (cardiac output), the ease with which blood flows through all the vessels (total peripheral resistance), oxygen used and carbon dioxide released by the body, and lung function and volume changes. SLS-1 was launched aboard the Space Shuttle Orbiter Columbia (STS-40) on June 5, 1995.

  16. Feasibility of a Dragon-Derived Mars Lander for Scientific and Human-Precursor Missions

    NASA Technical Reports Server (NTRS)

    Karcz, John S.; Davis, Sanford S.; Allen, Gary A.; Glass, Brian J.; Gonzales, Andrew; Heldmann, Jennifer Lynne; Lemke, Lawrence G.; McKay, Chris; Stoker, Carol R.; Wooster, Paul Douglass; hide

    2013-01-01

    A minimally-modified SpaceX Dragon capsule launched on a Falcon Heavy rocket presents the possibility of a new low-cost, high-capacity Mars lander for robotic missions. We have been evaluating such a "Red Dragon" platform as an option for the Icebreaker Discovery Program mission concept. Dragon is currently in service ferrying cargo to and from the International Space Station, and a crew transport version is in development. The upcoming version, unlike other Earth-return vehicles, exhibits most of the capabilities necessary to land on Mars. In particular, it has a set of high-thrust, throttleable, storable bi-propellant "SuperDraco" engines integrated directly into the capsule that are intended for launch abort and powered landings on Earth. These thrusters provide the possibility of a parachute-free, fully-propulsive deceleration at Mars from supersonic speeds to the surface, a descent approach which would also scale well to larger future human landers. We will discuss the motivations for exploring a Red Dragon lander, the current results of our analysis of its feasibility and capabilities, and the implications of the platform for the Icebreaker mission concept. In particular, we will examine entry, descent, and landing (EDL) in detail. We will also describe the modifications to Dragon necessary for interplanetary cruise, EDL, and operations on the Martian surface. Our analysis to date indicates that a Red Dragon lander is feasible and that it would be capable of delivering more than 1000 kg of payload to sites at elevations three kilometers below the Mars Orbiter Laser Altimeter (MOLA) reference, which includes sites throughout most of the northern plains and Hellas.

  17. Parametric Analysis of Life Support Systems for Future Space Exploration Missions

    NASA Technical Reports Server (NTRS)

    Swickrath, Michael J.; Anderson, Molly S.; Bagdigian, Bob M.

    2011-01-01

    The National Aeronautics and Space Administration is in a process of evaluating future targets for space exploration. In order to maintain the welfare of a crew during future missions, a suite of life support technology is responsible for oxygen and water generation, carbon dioxide control, the removal of trace concentrations of organic contaminants, processing and recovery of water, and the storage and reclamation of solid waste. For each particular life support subsystem, a variety competing technologies either exist or are under aggressive development efforts. Each individual technology has strengths and weaknesses with regard to launch mass, power and cooling requirements, volume of hardware and consumables, and crew time requirements for operation. However, from a system level perspective, the favorability of each life support architecture is better assessed when the sub-system technologies are analyzed in aggregate. In order to evaluate each specific life support system architecture, the measure of equivalent system mass (ESM) was employed to benchmark system favorability. Moreover, the results discussed herein will be from the context of loop-closure with respect to the air, water, and waste sub-systems. Specifically, closure relates to the amount of consumables mass that crosses the boundary of the vehicle over the lifetime of a mission. As will be demonstrated in this manuscript, the optimal level of loop closure is heavily dependent upon mission requirements such as duration and the level of extra-vehicular activity (EVA) performed. Sub-system level trades were also considered as a function of mission duration to assess when increased loop closure is practical. Although many additional factors will likely merit consideration in designing life support systems for future missions, the ESM results described herein provide a context for future architecture design decisions toward a flexible path program.

  18. Biological life-support systems for Mars mission.

    PubMed

    Gitelson, J I

    1992-01-01

    Mars mission like the Lunar base is the first venture to maintain human life beyond earth biosphere. So far, all manned space missions including the longest ones used stocked reserves and can not be considered egress from biosphere. Conventional path proposed by technology for Martian mission LSS is to use physical-chemical approaches proved by the experience of astronautics. But the problem of man living beyond the limits of the earth biosphere can be fundamentally solved by making a closed ecosystem for him. The choice optimum for a Mars mission LSS can be substantiated by comparing the merits and demerits of physical-chemical and biological principles without ruling out possible compromise between them. The work gives comparative analysis of ecological and physical-chemical principles for LSS. Taking into consideration universal significance of ecological problems with artificial LSS as a particular case of their solution, complexity and high cost of large-scale experiments with manned LSS, it would be expedient for these works to have the status of an International Program open to be joined. A program of making artificial biospheres based on preceding experience and analysis of current situation is proposed.

  19. Drilling Polar Oceans with the European Research Icebreaker AURORA BOREALIS: the IODP Context

    NASA Astrophysics Data System (ADS)

    Lembke-Jene, Lester; Wolff-Boenisch, Bonnie; Azzolini, Roberto; Thiede, Joern; Biebow, Nicole; Eldholm, Olav; Egerton, Paul

    2010-05-01

    Polar oceans are characterized by extreme environmental conditions for humans and materials, and have remained the least accessible regions to scientists of the IODP. DSDP and ODP have for long faced specific technical and logistical problems when attempting to drill in ice-covered polar deep-sea basins. The Arctic Ocean and large areas of the high-latitude Southern Ocean remained largely un-sampled by ODP and remain one of the major scientific and technological challenges for IODP. Drilling in these regions has been discussed and anticipated for decades and the scientific rationales are reflected in the science plans of the international Nansen Arctic Drilling Program (NAD) or the Arctic Program Planning Group (APPG) of ODP/IODP, amongst others. More recently, the rationale to investigate the polar oceans in a holistic approach has been outlined by workshops, leading to strategic assessments of the scientific potential and new drilling proposals. The European Polar Board took the initiative to develop a plan for a novel and dedicated research icebreaker with technical capabilities hitherto unrealised. This research icebreaker will enable autonomous operations in the central Arctic Ocean and the Southern Ocean, even during the severest ice conditions in the deep winter, serving all marine disciplines of polar research including scientific drilling: The European Research Icebreaker and Deep-Sea Drilling Vessel AURORA BOREALIS. AURORA BOREALIS is presently planned as a multi-purpose vessel. The ship can be deployed as a research icebreaker in all polar waters during any season of the year, as it shall meet the specifications of the highest ice-class attainable (IACS Polar Code 1) for icebreakers. During the times when it is not employed for drilling, it will operate as the most technically advanced multi-disciplinary research vessel in the Arctic or polar Southern Ocean. AURORA BOREALIS will be a "European scientific flagship facility" (fully open to non

  20. Solid Waste Management Requirements Definition for Advanced Life Support Missions: Results

    NASA Technical Reports Server (NTRS)

    Alazraki, Michael P.; Hogan, John; Levri, Julie; Fisher, John; Drysdale, Alan

    2002-01-01

    Prior to determining what Solid Waste Management (SWM) technologies should be researched and developed by the Advanced Life Support (ALS) Project for future missions, there is a need to define SWM requirements. Because future waste streams will be highly mission-dependent, missions need to be defined prior to developing SWM requirements. The SWM Working Group has used the mission architecture outlined in the System Integration, Modeling and Analysis (SIMA) Element Reference Missions Document (RMD) as a starting point in the requirement development process. The missions examined include the International Space Station (ISS), a Mars Dual Lander mission, and a Mars Base. The SWM Element has also identified common SWM functionalities needed for future missions. These functionalities include: acceptance, transport, processing, storage, monitoring and control, and disposal. Requirements in each of these six areas are currently being developed for the selected missions. This paper reviews the results of this ongoing effort and identifies mission-dependent resource recovery requirements.

  1. Using Artificial Life to Assess the Typicality of Terrestrial Life: Implications for Human Mission Planetary Protection

    NASA Technical Reports Server (NTRS)

    Lupisella, Mark; Powers, Edward I. (Technical Monitor)

    2001-01-01

    The extent to which extraterrestrial life questions can be addressed, in the absence of an actual example, rests in some measure on the extent to which terrestrial life is representative of life in general since we will likely have to draw heavily, if not completely, from terrestrial life research. One example of a practical question involving extraterrestrial life that arises in preparing for a human mission to another planet such as Mars, is trying to assess and minimize the possible adverse effects of the presence of humans on possible indigenous extraterrestrial life-forms. This paper will present some key planetary protection challenges for a human Mars mission and then focus on one possible approach for assessing the extent to which terrestrial life is representative of biological phenomena in general, informing perhaps, the level of confidence we might have in applying terrestrial research - to extraterrestrial life issues. The approach involves appealing to the relatively new field of Artificial Life (A-Life) to: (1) use what might be the most basic minimal set of life-defining characteristics in (2) a large number of open-ended Artificial Life simulations to generate a "life possibility space" (3) the products of which can be examined for their plausibility within the context of relevant constraining knowledge, so that (4) the remaining possibility space can be examined for its variability relative to terrestrial life, where low variability might suggest that terrestrial life is representative of life in general, and high variability would indicate otherwise.

  2. Collecting winter data on U.S. Coast Guard icebreakers

    NASA Astrophysics Data System (ADS)

    Oyserman, Ben O.; Woityra, William C.; Bullerjahn, George S.; Beall, Benjamin F. N.; McKay, Robert Michael L.

    2012-03-01

    Winter research and monitoring of icebound rivers, lakes, and coastal seas to date has usually involved seagoing civilian scientists leading survey efforts. However, because of poor weather conditions and a lack of safe research platforms, scientists collecting data during winter face some difficult and often insurmountable problems. To solve these problems and to further research and environmental monitoring goals, new partnerships can be formed through integrating efforts of the U.S. Coast Guard (USCG) with citizen science initiatives. USCG and a research group at Ohio's Bowling Green State University are entering the third year of such a partnership, in which icebreaking operations in Lake Erie using USCG Cutter Neah Bay support volunteer data collection. With two additional USCG vessels joining the program this winter season, the partnership serves as a timely and useful model for worldwide environmental research and monitoring through citizen science and government collaboration.

  3. Life Support Filtration System Trade Study for Deep Space Missions

    NASA Technical Reports Server (NTRS)

    Agui, Juan H.; Perry, Jay L.

    2017-01-01

    The National Aeronautics and Space Administrations (NASA) technical developments for highly reliable life support systems aim to maximize the viability of long duration deep space missions. Among the life support system functions, airborne particulate matter filtration is a significant driver of launch mass because of the large geometry required to provide adequate filtration performance and because of the number of replacement filters needed to a sustain a mission. A trade analysis incorporating various launch, operational and maintenance parameters was conducted to investigate the trade-offs between the various particulate matter filtration configurations. In addition to typical launch parameters such as mass, volume and power, the amount of crew time dedicated to system maintenance becomes an increasingly crucial factor for long duration missions. The trade analysis evaluated these parameters for conventional particulate matter filtration technologies and a new multi-stage particulate matter filtration system under development by NASAs Glenn Research Center. The multi-stage filtration system features modular components that allow for physical configuration flexibility. Specifically, the filtration system components can be configured in distributed, centralized, and hybrid physical layouts that can result in considerable mass savings compared to conventional particulate matter filtration technologies. The trade analysis results are presented and implications for future transit and surface missions are discussed.

  4. 76 FR 42682 - China Biotech Life Sciences Trade Mission-Clarification and Amendment

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-07-19

    ... DEPARTMENT OF COMMERCE International Trade Administration China Biotech Life Sciences Trade... Life Science Trade Mission to China, 76 FR 17,621, Mar. 30, 2011, to clarify eligibility and amend the... representatives from a variety of U.S. biotechnology and life science firms and trade organizations. In response...

  5. Masked hearing thresholds of a beluga whale ( Delphinapterus leucas) in icebreaker noise

    NASA Astrophysics Data System (ADS)

    Erbe, C.; Farmer, D. M.

    An experiment is presented that measured masked hearing thresholds of a beluga whale at the Vancouver Aquarium. The masked signal was a typical beluga vocalization; the masking noise included two types of icebreaker noise and naturally occurring icecracking noise. Thresholds were measured behaviorally in a go/no-go paradigm. Results were that bubbler system noise exhibited the strongest masking effect with a critical noise-to-signal ratio of 15.4 dB. Propeller cavitation noise completely masked the vocalization for noise-to-signal ratios greater than 18.0 dB. Natural icecracking noise showed the least interference with a threshold at 29.0 dB. A psychophysical analysis indicated that the whale did not have a consistent decision bias.

  6. Space Station accommodation of life sciences in support of a manned Mars mission

    NASA Technical Reports Server (NTRS)

    Meredith, Barry D.; Willshire, Kelli F.; Hagaman, Jane A.; Seddon, Rhea M.

    1989-01-01

    Results of a life science impact analysis for accommodation to the Space Station of a manned Mars mission are discussed. In addition to addressing such issues as on-orbit vehicle assembly and checkout, the study also assessed the impact of a life science research program on the station. A better understanding of the effects on the crew of long duration exposure to the hostile space environment and to develop controls for adverse effects was the objective. Elements and products of the life science accommodation include: the identification of critical research areas; the outline of a research program consistent with the mission timeframe; the quantification of resource requirements; the allocation of functions to station facilities; and a determination of the impact on the Space Station program and of the baseline configuration. Results indicate the need at the Space Station for two dedicated life science lab modules; a pocket lab to support a 4-meter centrifuge; a quarantine module for the Mars Sample Return Mission; 3.9 man-years of average crew time; and 20 kilowatts of electrical power.

  7. Mission Life Thermal Analysis and Environment Correlation for the Lunar Reconnaissance Orbiter

    NASA Technical Reports Server (NTRS)

    Garrison, Matthew B.; Peabody, Hume

    2012-01-01

    Standard thermal analysis practices include stacking worst-case conditions including environmental heat loads, thermo-optical properties and orbital beta angles. This results in the design being driven by a few bounding thermal cases, although those cases may only represent a very small portion of the actual mission life. The NASA Goddard Space Flight Center Thermal Branch developed a procedure to predict the flight temperatures over the entire mission life, assuming a known beta angle progression, variation in the thermal environment, and a degradation rate in the coatings. This was applied to the Global Precipitation Measurement core spacecraft. In order to assess the validity of this process, this work applies the similar process to the Lunar Reconnaissance Orbiter. A flight-correlated thermal model was exercised to give predictions of the thermal performance over the mission life. These results were then compared against flight data from the first two years of the spacecraft s use. This is used to validate the process and to suggest possible improvements for future analyses.

  8. IceBreaker: Mars Drill and Sample Delivery System

    NASA Astrophysics Data System (ADS)

    Mellerowicz, B. L.; Paulsen, G. L.; Zacny, K.; McKay, C.; Glass, B. J.; Dave, A.; Davila, A. F.; Marinova, M.

    2012-12-01

    We report on the development and testing of a one meter class prototype Mars drill and cuttings sample delivery system. The IceBreaker drill consists of a rotary-percussive drill head, a sampling auger with a bit at the end having an integrated temperature sensor, a Z-stage for advancing the auger into the ground, and a sam-pling station for moving the augered ice shavings or soil cuttings into a sample cup. The drill is deployed from a 3 Degree of Freedom (DOF) robotic arm. The drill demonstrated drilling in ice-cemented ground, ice, and rocks at the 1-1-100-100 level; that is the drill reached 1 meter in 1 hour with 100 Watts of power and 100 Newton Weight on Bit. This cor-responds to an average energy of 100 Whr. The drill has been extensively tested in the Mars chamber to a depth of 1 meter, as well as in the Antarctic and the Arctic Mars analog sites. We also tested three sample delivery systems: 1) 4 DOF arm with a custom soil scoop at the end; 2) Pneumatic based, and 3) Drill based enabled by the 3 (DOF) drill deployment boom. In all approaches there is an air-gap between the sterilized drill (which penetrates subsurface) and the sample transfer hardware (which is not going to be sterilized). The air gap satisfies the planetary protection requirements. The scoop acquires cuttings sample once they are augered to the surface, and drops them into an in-strument inlet port. The system has been tested in the Mars chamber and in the Arctic. The pneumatic sample delivery system uses compressed gas to move the sample captured inside a small chamber inte-grated with the auger, directly into the instrument. The system was tested in the Mars chamber. In the third approach the drill auger captures the sample on its flutes, the 3 DOF boom positions the tip of the auger above the instrument, and then the auger discharges the sample into an instrument. This approach was tested in the labolatory (at STP). The above drilling and sample delivery tests have shown that drilling

  9. Ultra Reliable Closed Loop Life Support for Long Space Missions

    NASA Technical Reports Server (NTRS)

    Jones, Harry W.; Ewert, Michael K.

    2010-01-01

    Spacecraft human life support systems can achieve ultra reliability by providing sufficient spares to replace all failed components. The additional mass of spares for ultra reliability is approximately equal to the original system mass, provided that the original system reliability is not too low. Acceptable reliability can be achieved for the Space Shuttle and Space Station by preventive maintenance and by replacing failed units. However, on-demand maintenance and repair requires a logistics supply chain in place to provide the needed spares. In contrast, a Mars or other long space mission must take along all the needed spares, since resupply is not possible. Long missions must achieve ultra reliability, a very low failure rate per hour, since they will take years rather than weeks and cannot be cut short if a failure occurs. Also, distant missions have a much higher mass launch cost per kilogram than near-Earth missions. Achieving ultra reliable spacecraft life support systems with acceptable mass will require a well-planned and extensive development effort. Analysis must determine the reliability requirement and allocate it to subsystems and components. Ultra reliability requires reducing the intrinsic failure causes, providing spares to replace failed components and having "graceful" failure modes. Technologies, components, and materials must be selected and designed for high reliability. Long duration testing is needed to confirm very low failure rates. Systems design should segregate the failure causes in the smallest, most easily replaceable parts. The system must be designed, developed, integrated, and tested with system reliability in mind. Maintenance and reparability of failed units must not add to the probability of failure. The overall system must be tested sufficiently to identify any design errors. A program to develop ultra reliable space life support systems with acceptable mass should start soon since it must be a long term effort.

  10. Synchronous in-field application of life-detection techniques in planetary analog missions

    NASA Astrophysics Data System (ADS)

    Amador, Elena S.; Cable, Morgan L.; Chaudry, Nosheen; Cullen, Thomas; Gentry, Diana; Jacobsen, Malene B.; Murukesan, Gayathri; Schwieterman, Edward W.; Stevens, Adam H.; Stockton, Amanda; Yin, Chang; Cullen, David C.; Geppert, Wolf

    2015-02-01

    Field expeditions that simulate the operations of robotic planetary exploration missions at analog sites on Earth can help establish best practices and are therefore a positive contribution to the planetary exploration community. There are many sites in Iceland that possess heritage as planetary exploration analog locations and whose environmental extremes make them suitable for simulating scientific sampling and robotic operations. We conducted a planetary exploration analog mission at two recent lava fields in Iceland, Fimmvörðuháls (2010) and Eldfell (1973), using a specially developed field laboratory. We tested the utility of in-field site sampling down selection and tiered analysis operational capabilities with three life detection and characterization techniques: fluorescence microscopy (FM), adenine-triphosphate (ATP) bioluminescence assay, and quantitative polymerase chain reaction (qPCR) assay. The study made use of multiple cycles of sample collection at multiple distance scales and field laboratory analysis using the synchronous life-detection techniques to heuristically develop the continuing sampling and analysis strategy during the expedition. Here we report the operational lessons learned and provide brief summaries of scientific data. The full scientific data report will follow separately. We found that rapid in-field analysis to determine subsequent sampling decisions is operationally feasible, and that the chosen life detection and characterization techniques are suitable for a terrestrial life-detection field mission. In-field analysis enables the rapid obtainment of scientific data and thus facilitates the collection of the most scientifically relevant samples within a single field expedition, without the need for sample relocation to external laboratories. The operational lessons learned in this study could be applied to future terrestrial field expeditions employing other analytical techniques and to future robotic planetary exploration

  11. Environmental control and life support technologies for advanced manned space missions

    NASA Technical Reports Server (NTRS)

    Powell, F. T.; Wynveen, R. A.; Lin, C.

    1986-01-01

    Regenerative environmental control and life support system (ECLSS) technologies are found by the present evaluation to have reached a degree of maturity that recommends their application to long duration manned missions. The missions for which regenerative ECLSSs are attractive in virtue of the need to avoid expendables and resupply requirements have been identified as that of the long duration LEO Space Station, long duration stays at GEO, a permanently manned lunar base (or colony), manned platforms located at the earth-moon libration points L4 or L5, a Mars mission, deep space exploration, and asteroid exploration. A comparison is made between nonregenerative and regenerative ECLSSs in the cases of 10 essential functions.

  12. Impact of Planetary Protection and Contamination Control on a Life Detection or Sample Return Mission

    NASA Astrophysics Data System (ADS)

    Steininger, H.

    2018-04-01

    ExoMars as one of the few life detection missions can be an example of how planetary protection and contamination control influence of the development of flight hardware. A few lessons learned can be drawn from the mission even before launch.

  13. STS-40 Spacelab Life Sciences 1 (SLS-1): The first dedicated spacelab life sciences mission

    NASA Technical Reports Server (NTRS)

    1991-01-01

    Successful exploration of space depends on the health and well-being of people who travel and work there. For this reason, the National Aeronautics and Space Administration (NASA) has dedicated several Space Shuttle missions to examine how living and working in space affects the human body. Spacelab Life Sciences 1 (SLS-1) is the first of these missions. The main purpose of the SLS-1 mission is to study the mechanisms, magnitudes, and time courses of certain physiological changes that occur during space flight and to investigate the consequences of the body's adaptation to microgravity and readjustment to gravity upon return to Earth. How does space flight influence the heart and circulatory system, metabolic processes, the muscles and bones, and the cells? If responses to weightlessness are undesirable, how can they be prevented or controlled? Will the human body maintain its physical and chemical equilibrium during months aboard a space station and years-long missions to Mars? When crews return to Earth, what can they expect to experience as their bodies readjust to Earth's gravity? With the SLS-1 experiments, NASA is addressing some of these questions. Various aspects of the SLS-1 are discussed.

  14. Guidelines for NASA Missions to Engage the User Community as a Part of the Mission Life Cycle

    NASA Astrophysics Data System (ADS)

    Escobar, V. M.; Friedl, L.; Bonniksen, C. K.

    2017-12-01

    NASA continues to improve the Earth Science Directorate in the areas of thematic integration, stakeholder feedback and Project Applications Program tailoring for missions to transfer knowledge between scientists and projects. The integration of application themes and the implementation of application science activities in flight projects have evolved to formally include user feedback and stakeholder integration. NASA's new Flight Applied Science Program Guidelines are designed to bridge NASA Earth Science Directorates in Flight, Applied Sciences and Research and Development by agreeing to integrate the user community into mission life cycles. Thus science development and science applications will guide all new instruments launched by NASAs ESD. The continued integration with the user community has enabled socio-economic considerations into NASA Earth Science projects to advance significantly. Making users a natural part of mission science leverages future socio-economic impact research and provides a platform for innovative and more actionable product to be used in decision support systems by society. This presentation will give an overview of the new NASA Guidelines and provide samples that demonstrate how the user community can be a part of NASA mission designs.

  15. Ames Research Center Life Sciences Payload Project for Spacelab Mission 3

    NASA Technical Reports Server (NTRS)

    Callahan, P. X.; Tremor, J.; Lund, G.; Wagner, W. L.

    1983-01-01

    The Research Animal Holding Facility, developed to support rodent and squirrel monkey animal husbandry in the Spacelab environment, is to be tested during the Spacelab Mission 3 flight. The configuration and function of the payload hardware elements, the assembly and test program, the operational rationale, and the scientific approach of this mission are examined. Topics covered include animal life support systems, the squirrel monkey restraint, the camera-mirror system, the dynamic environment measurement system, the biotelemetry system, and the ground support equipment. Consideration is also given to animal pretests, loading the animals during their 12 hour light cycle, and animal early recovery after landing. This mission will be the first time that relatively large samples of monkeys and rats will be flown in space and also cared for and observed by man.

  16. Air-sea interaction regimes in the sub-Antarctic Southern Ocean and Antarctic marginal ice zone revealed by icebreaker measurements

    NASA Astrophysics Data System (ADS)

    Yu, Lisan; Jin, Xiangze; Schulz, Eric W.; Josey, Simon A.

    2017-08-01

    This study analyzed shipboard air-sea measurements acquired by the icebreaker Aurora Australis during its off-winter operation in December 2010 to May 2012. Mean conditions over 7 months (October-April) were compiled from a total of 22 ship tracks. The icebreaker traversed the water between Hobart, Tasmania, and the Antarctic continent, providing valuable in situ insight into two dynamically important, yet poorly sampled, regimes: the sub-Antarctic Southern Ocean and the Antarctic marginal ice zone (MIZ) in the Indian Ocean sector. The transition from the open water to the ice-covered surface creates sharp changes in albedo, surface roughness, and air temperature, leading to consequential effects on air-sea variables and fluxes. Major effort was made to estimate the air-sea fluxes in the MIZ using the bulk flux algorithms that are tuned specifically for the sea-ice effects, while computing the fluxes over the sub-Antarctic section using the COARE3.0 algorithm. The study evidenced strong sea-ice modulations on winds, with the southerly airflow showing deceleration (convergence) in the MIZ and acceleration (divergence) when moving away from the MIZ. Marked seasonal variations in heat exchanges between the atmosphere and the ice margin were noted. The monotonic increase in turbulent latent and sensible heat fluxes after summer turned the MIZ quickly into a heat loss regime, while at the same time the sub-Antarctic surface water continued to receive heat from the atmosphere. The drastic increase in turbulent heat loss in the MIZ contrasted sharply to the nonsignificant and seasonally invariant turbulent heat loss over the sub-Antarctic open water.Plain Language SummaryThe <span class="hlt">icebreaker</span> Aurora Australis is a research and supply vessel that is regularly chartered by the Australian Antarctic Division during the southern summer to operate in waters between Hobart, Tasmania, and Antarctica. The vessel serves as the main lifeline to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160002378','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160002378"><span>Requirements for Designing <span class="hlt">Life</span> Support System Architectures for Crewed Exploration <span class="hlt">Missions</span> Beyond Low-Earth Orbit</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Howard, David; Perry,Jay; Sargusingh, Miriam; Toomarian, Nikzad</p> <p>2016-01-01</p> <p>NASA's technology development roadmaps provide guidance to focus technological development on areas that enable crewed exploration <span class="hlt">missions</span> beyond low-Earth orbit. Specifically, the technology area roadmap on human health, <span class="hlt">life</span> support and habitation systems describes the need for <span class="hlt">life</span> support system (LSS) technologies that can improve reliability and in-situ maintainability within a minimally-sized package while enabling a high degree of <span class="hlt">mission</span> autonomy. To address the needs outlined by the guiding technology area roadmap, NASA's Advanced Exploration Systems (AES) Program has commissioned the <span class="hlt">Life</span> Support Systems (LSS) Project to lead technology development in the areas of water recovery and management, atmosphere revitalization, and environmental monitoring. A notional exploration LSS architecture derived from the International Space has been developed and serves as the developmental basis for these efforts. Functional requirements and key performance parameters that guide the exploration LSS technology development efforts are presented and discussed. Areas where LSS flight operations aboard the ISS afford lessons learned that are relevant to exploration <span class="hlt">missions</span> are highlighted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=sts078-305-022&hterms=work+life&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dwork%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=sts078-305-022&hterms=work+life&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dwork%2Blife"><span>Astronaut Richard M. Linnehan, <span class="hlt">mission</span> specialist, works out in the <span class="hlt">Life</span> and Microgravity Spacelab</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1996-01-01</p> <p>STS-78 ONBOARD VIEW --- Astronaut Richard M. Linnehan, <span class="hlt">mission</span> specialist, works out in the <span class="hlt">Life</span> and Microgravity Spacelab (LMS-1) Science Module aboard the Earth-orbiting Space Shuttle Columbia. With an almost 17-day <span class="hlt">mission</span> away from Earths gravity, crew members maintained an exercise regimen above and beyond their assigned LMS-1 duty assignments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160002244','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160002244"><span>Crater Morphology in the Phoenix Landing Ellipse: Insights Into Net Erosion and Ice Table Depth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Noe Dobrea, E. Z.; Stoker, C. R.; McKay, C. P.; Davila, A. F.; Krco, M.</p> <p>2015-01-01</p> <p><span class="hlt">Icebreaker</span> [1] is a Discovery class <span class="hlt">mission</span> being developed for future flight opportunities. Under this <span class="hlt">mission</span> concept, the <span class="hlt">Icebreaker</span> payload is carried on a stationary lander, and lands in the same landing ellipse as Phoenix. Samples are acquired from the subsurface using a drilling system that penetrates into materials which may include loose or cemented soil, icy soil, pure ice, rocks, or mixtures of these. To avoid the complexity of mating additional strings, the drill is single-string, limiting it to a total length of 1 m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26587241','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26587241"><span>The <span class="hlt">ice-breaker</span> effect: singing mediates fast social bonding.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pearce, Eiluned; Launay, Jacques; Dunbar, Robin I M</p> <p>2015-10-01</p> <p>It has been proposed that singing evolved to facilitate social cohesion. However, it remains unclear whether bonding arises out of properties intrinsic to singing or whether any social engagement can have a similar effect. Furthermore, previous research has used one-off singing sessions without exploring the emergence of social bonding over time. In this semi-naturalistic study, we followed newly formed singing and non-singing (crafts or creative writing) adult education classes over seven months. Participants rated their closeness to their group and their affect, and were given a proxy measure of endorphin release, before and after their class, at three timepoints (months 1, 3 and 7). We show that although singers and non-singers felt equally connected by timepoint 3, singers experienced much faster bonding: singers demonstrated a significantly greater increase in closeness at timepoint 1, but the more gradual increase shown by non-singers caught up over time. This represents the first evidence for an '<span class="hlt">ice-breaker</span> effect' of singing in promoting fast cohesion between unfamiliar individuals, which bypasses the need for personal knowledge of group members gained through prolonged interaction. We argue that singing may have evolved to quickly bond large human groups of relative strangers, potentially through encouraging willingness to coordinate by enhancing positive affect.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090020667','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090020667"><span>Development of <span class="hlt">Life</span> Support System Technologies for Human Lunar <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barta, Daniel J.; Ewert, Michael K.</p> <p>2009-01-01</p> <p>With the Preliminary Design Review (PDR) for the Orion Crew Exploration Vehicle planned to be completed in 2009, Exploration <span class="hlt">Life</span> Support (ELS), a technology development project under the National Aeronautics and Space Administration s (NASA) Exploration Technology Development Program, is focusing its efforts on needs for human lunar <span class="hlt">missions</span>. The ELS Project s goal is to develop and mature a suite of Environmental Control and <span class="hlt">Life</span> Support System (ECLSS) technologies for potential use on human spacecraft under development in support of U.S. Space Exploration Policy. ELS technology development is directed at three major vehicle projects within NASA s Constellation Program (CxP): the Orion Crew Exploration Vehicle (CEV), the Altair Lunar Lander and Lunar Surface Systems, including habitats and pressurized rovers. The ELS Project includes four technical elements: Atmosphere Revitalization Systems, Water Recovery Systems, Waste Management Systems and Habitation Engineering, and two cross cutting elements, Systems Integration, Modeling and Analysis, and Validation and Testing. This paper will provide an overview of the ELS Project, connectivity with its customers and an update to content within its technology development portfolio with focus on human lunar <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110013004','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110013004"><span><span class="hlt">Life</span> Support and Habitation Systems: Crew Support and Protection for Human Exploration <span class="hlt">Missions</span> Beyond Low Earth Orbit</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barta, Daniel J.; McQuillan, Jeffrey</p> <p>2011-01-01</p> <p>The National Aeronautics and Space Administration (NASA) has recently expanded its <span class="hlt">mission</span> set for possible future human exploration <span class="hlt">missions</span>. With multiple options there is interest in identifying technology needs across these <span class="hlt">missions</span> to focus technology investments. In addition to the Moon and other destinations in cis-lunar space, other destinations including Near Earth Objects and Mars have been added for consideration. Recently, technology programs and projects have been re-organizing to better meet the Agency s strategic goals and address needs across these potential future <span class="hlt">missions</span>. <span class="hlt">Life</span> Support and Habitation Systems (LSHS) is one of 10 Foundational Domains as part of the National Aeronautics and Space Administration s Exploration Technology Development Program. The chief goal of LSHS is to develop and mature advanced technologies to sustain human <span class="hlt">life</span> on <span class="hlt">missions</span> beyond Low Earth Orbit (LEO) to increase reliability, reduce dependency on resupply and increase vehicle self-sufficiency. For long duration exploration <span class="hlt">missions</span>, further closure of <span class="hlt">life</span> support systems is of interest. Focus includes key technologies for atmosphere revitalization, water recovery, waste management, thermal control and crew accommodations. Other areas of focus include technologies for radiation protection, environmental monitoring and fire protection. The aim is to recover additional consumable mass, reduce requirements for power, volume, heat rejection, crew involvement, and meet exploration vehicle requirements. This paper provides a brief description of the LSHS Foundational Domain as defined for fiscal year 2011.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040084463','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040084463"><span>Forward Contamination of the Moon and Mars: Implications for Future <span class="hlt">Life</span> Detection <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Glavin, Daniel P.; Dworkin, Jason P.; Lupisella, Mark; Kminek, Gerhard; Rummel, John D.</p> <p>2004-01-01</p> <p>NASA and ESA have outlined new visions for solar system exploration that will include a series of lunar robotic <span class="hlt">missions</span> to prepare for, and support a human return to the Moon, and future human exploration of Mars and other destinations. One of the guiding principles for exploration is to pursue compelling scientific questions about the origin and evolution of <span class="hlt">life</span>. The search for <span class="hlt">life</span> on objects such as Mars will require that all spacecraft and instrumentation be sufficiently cleaned and sterilized prior to launch to ensure that the scientific integrity of extraterrestrial samples is not jeopardized by terrestrial organic contamination. Under COSPAR's current planetary protection policy for the Moon, no sterilization procedures are required for outbound lunar spacecraft. Nonetheless, future in situ investigations of a variety of locations on the Moon by highly sensitive instruments designed to search for biologically derived organic compounds would help assess the contamination of the Moon by lunar spacecraft. These studies could also provide valuable "ground truth" data for Mars sample return <span class="hlt">missions</span> and help define planetary protection requirements for future Mars bound spacecraft carrying <span class="hlt">life</span> detection experiments. In addition, studies of the impact of terrestrial contamination of the lunar surface by the Apollo astronauts could provide valuable data to help refine future Mars surface exploration plans for a human <span class="hlt">mission</span> to Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017LPICo1989.8175W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017LPICo1989.8175W"><span>Analogies Among Current and Future <span class="hlt">Life</span> Detection <span class="hlt">Missions</span> and the Pharmaceutical/Biomedical Industries</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wainwright, N. R.; Steele, A.; Monaco, L.; Fries, M.</p> <p>2017-02-01</p> <p><span class="hlt">Life</span> detection goals and technologies are remarkably similar between several types of NASA <span class="hlt">missions</span> and the pharmaceutical and biotechnology industries. Needs for sensitivity, specificity, speed have driven techniques and equipment to common ends.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100040672','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100040672"><span><span class="hlt">Life</span> Support and Habitation Systems: Crew Support and Protection for Human Exploration <span class="hlt">Missions</span> Beyond Low Earth Orbit</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barta, Daniel J.; McQuillan, Jeffrey</p> <p>2010-01-01</p> <p><span class="hlt">Life</span> Support and Habitation Systems (LSHS) is one of 10 Foundational Domains as part of the National Aeronautics and Space Administration s proposed Enabling Technology Development and Demonstration (ETDD) Program. LSHS will develop and mature technologies to sustain <span class="hlt">life</span> on long duration human <span class="hlt">missions</span> beyond Low Earth Orbit that are reliable, have minimal logistics supply and increase self-sufficiency. For long duration exploration <span class="hlt">missions</span>, further closure of <span class="hlt">life</span> support systems is paramount, including focus on key technologies for atmosphere revitalization, water recovery, waste management, thermal control and crew accommodation that recover additional consumable mass, reduce requirements for power, volume, heat rejection, crew involvement, and which have increased reliability and capability. Other areas of focus include technologies for radiation protection, environmental monitoring and fire protection. Beyond LEO, return to Earth will be constrained. The potability of recycled water and purity of regenerated air must be measured and certified aboard the spacecraft. <span class="hlt">Missions</span> must be able to recover from fire events through early detection, use of non-toxic suppression agents, and operation of recovery systems that protect on-board Environmental Control and <span class="hlt">Life</span> Support (ECLS) hardware. Without the protection of the Earth s geomagnetic field, <span class="hlt">missions</span> beyond LEO must have improved radiation shielding and dosimetry, as well as warning systems to protect the crew against solar particle events. This paper will describe plans for the new LSHS Foundational Domain and <span class="hlt">mission</span> factors that will shape its technology development portfolio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930015528','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930015528"><span>Analysis of reentry into the White Sands Missile Range (WSMR) for the <span class="hlt">Life</span>Sat <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hametz, M.; Roszman, L.; Snow, F.; Cooley, J.</p> <p>1993-01-01</p> <p>This study investigates the reentry of the <span class="hlt">Life</span>Sat vehicles into the WSMR. The <span class="hlt">Life</span>Sat <span class="hlt">mission</span> consists of two reusable reentry satellites, each carrying a removable payload module, which scientists will use to study long-term effects of microgravity, Van Allen belt radiation, and galactic cosmic rays on living organisms. A series of <span class="hlt">missions</span> is planned for both low-Earth circular orbits and highly elliptic orbits. To recover the payload module with the specimens intact, a soft parachute landing and recovery at the WSMR is planned. This analysis examines operational issues surrounding the reentry scenario to assess the feasibility of the reentry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050176025','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050176025"><span>Field Simulation of a Drilling <span class="hlt">Mission</span> to Mars to Search for Subsurface <span class="hlt">Life</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stoker, C. R.; Lemke, L. G.; Cannon, H.; Glass, B.; Dunagan, S.; Zavaleta, J.; Miller, D.; Gomez-Elvira, J.</p> <p>2005-01-01</p> <p>The discovery of near surface ground ice by the Mars Odyssey <span class="hlt">mission</span> and the abundant evidence for recent Gulley features observed by the Mars Global Surveyor <span class="hlt">mission</span> support longstanding theoretical arguments for subsurface liquid water on Mars. Thus, implementing the Mars program goal to search for <span class="hlt">life</span> points to drilling on Mars to reach liquid water, collecting samples and analyzing them with instrumentation to detect in situ organisms and biomarker compounds. Searching for <span class="hlt">life</span> in the subsurface of Mars will require drilling, sample extraction and handling, and new technologies to find and identify biomarker compounds and search for living organisms. In spite of its obvious advantages, robotic drilling for Mars exploration is in its technological infancy and has yet to be demonstrated in even a terrestrial field environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070035921&hterms=life+cycles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dlife%2Bcycles','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070035921&hterms=life+cycles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dlife%2Bcycles"><span><span class="hlt">Life</span> Cycle of a <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bothwell, Mary</p> <p>2004-01-01</p> <p>A viewgraph presentation describing the the six phases of a space <span class="hlt">mission</span> is shown. The contents include: 1) What Does Planning Involve?; 2) Designing the Flight System; 3) Building the Flight System; 4) Testing the Flight System; 5) Flying the <span class="hlt">Mission</span>; and 6) Analyzing the Data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006cosp...36..554G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006cosp...36..554G"><span>ExoMars: ESA's <span class="hlt">mission</span> to search for signs of <span class="hlt">life</span> on the red planet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gardini, B.; Vago, J. L.; Baglioni, P.; Kminek, G.; Gianfiglio, G.</p> <p></p> <p>In the framework of its Aurora Exploration Program in 2011 the European Space Agency ESA plans to launch the ExoMars <span class="hlt">mission</span> ExoMars will deliver two science elements to the Martian surface a Rover carrying the Pasteur scientific payload and a small fixed surface station ---the Geophysics Environment Package GEP The Rover s scientific objectives are 1 To search for signs of past and present <span class="hlt">life</span> and 2 To characterise in the shallow subsurface the vertical distribution profile for water and geochemical composition The science goals of GEP are 1 to measure geophysics parameters necessary to understand the planet s long-term internal evolution and habitability and 2 to characterise the local environment and identify hazards to future human <span class="hlt">missions</span> Over its planned 6-month lifetime the Rover will travel a few kilometres searching for traces of past and present signs of <span class="hlt">life</span> It will do this by collecting and analysing samples from within surface rocks and from underground ---down to 2-m depth The very powerful combination of mobility with the capability to access locations where organic molecules might be well preserved is unique to this <span class="hlt">mission</span> ExoMars will have the right tools to try to answer the question of whether <span class="hlt">life</span> ever arose on the red planet The ExoMars <span class="hlt">mission</span> contains two other elements a Carrier and a Descent Module The Carrier will bring the Descent Module to Mars and release it from the hyperbolic arrival trajectory The Descent Module s objective is to safely deploy the Rover and the GEP ---developing a robust</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880033869&hterms=technologies+environmental&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtechnologies%2Benvironmental','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880033869&hterms=technologies+environmental&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtechnologies%2Benvironmental"><span>Environmental control and <span class="hlt">life</span> support system requirements and technology needs for advanced manned space <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Powell, Ferolyn T.; Sedej, Melaine; Lin, Chin</p> <p>1987-01-01</p> <p>NASA has completed an environmental control and <span class="hlt">life</span> support system (ECLSS) technology R&D plan for advanced <span class="hlt">missions</span> which gave attention to the drivers (crew size, <span class="hlt">mission</span> duration, etc.) of a range of manned <span class="hlt">missions</span> under consideration. Key planning guidelines encompassed a time horizon greater than 50 years, funding resource requirements, an evolutionary approach to goal definition, and the funding of more than one approach to satisfy a given perceived requirement. Attention was given to the ECLSS requirements of transportation and service vehicles, platforms, bases and settlements, ECLSS functions and average load requirements, unique drivers for various <span class="hlt">missions</span>, and potentially exploitable commonalities among vehicles and habitats.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1616323A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1616323A"><span>Arctic summer school onboard an <span class="hlt">icebreaker</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alexeev, Vladimir A.; Repina, Irina A.</p> <p>2014-05-01</p> <p>The International Arctic Research Center (IARC) of the University of Alaska Fairbanks conducted a summer school for PhD students, post-docs and early career scientists in August-September 2013, jointly with an arctic expedition as a part of NABOS project (Nansen and Amundsen Basin Observational System) onboard the Russian research vessel "Akademik Fedorov". Both the summer school and NABOS expedition were funded by the National Science Foundation. The one-month long summer school brought together graduate students and young scientists with specialists in arctic oceanography and climate to convey to a new generation of scientists the opportunities and challenges of arctic climate observations and modeling. Young scientists gained hands-on experience during the field campaign and learned about key issues in arctic climate from observational, diagnostic, and modeling perspectives. The summer school consisted of background lectures, participation in fieldwork and mini-projects. The mini-projects were performed in collaboration with summer school instructors and members of the expedition. Key topics covered in the lectures included: - arctic climate: key characteristics and processes; - physical processes in the Arctic Ocean; - sea ice and the Arctic Ocean; - trace gases, aerosols, and chemistry: importance for climate changes; - feedbacks in the arctic system (e.g., surface albedo, clouds, water vapor, circulation); - arctic climate variations: past, ongoing, and projected; - global climate models: an overview. An outreach specialist from the Miami Science Museum was writing a blog from the <span class="hlt">icebreaker</span> with some very impressive statistics (results as of January 1, 2014): Total number of blog posts: 176 Blog posts written/contributed by scientists: 42 Blog views: 22,684 Comments: 1,215 Number of countries who viewed the blog: 89 (on 6 continents) The 33-day long NABOS expedition started on August 22, 2013 from Kirkenes, Norway. The vessel ("Akademik Fedorov") returned to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=problem+AND+military+AND+university&pg=3&id=EJ738585','ERIC'); return false;" href="https://eric.ed.gov/?q=problem+AND+military+AND+university&pg=3&id=EJ738585"><span><span class="hlt">Life</span> at <span class="hlt">Mission</span> Creep U</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Dubrow, Greg; Moseley, Bryan; Dustin, Daniel</p> <p>2006-01-01</p> <p>The term "<span class="hlt">mission</span> creep" was originally coined nearly a hundred years ago to describe the gradual process by which a military <span class="hlt">mission</span>'s stated methods and goals change, and recently the term has been applied to incremental organizational changes. In this article, the term is used to describe what happens when a teaching-oriented college or…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5974796','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5974796"><span>The <span class="hlt">Life</span> <span class="hlt">Mission</span> Theory II. The Structure of the <span class="hlt">Life</span> Purpose and the Ego</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ventegodt, Soren; Andersen, Niels Jorgen; Merrick, Joav</p> <p>2003-01-01</p> <p>Pursuing your <span class="hlt">life</span> <span class="hlt">mission</span> is often very difficult, and many frustrations are experienced along the way. Major failures to bring out our potential can cause us considerable emotional pain. When this pain is unbearable, we are induced to shift from one intention and talent to another that better allows us to adapt and survive. Thus, we become set on a course that brings out a secondary or tertiary talent instead of the primary talent. This talent displacement may be expressed as a loss of our true nature or true self. The new purpose in <span class="hlt">life</span> now functions as the core of a new personality: the ego. The ego has a structure similar to that of the true self. It is anchored in a talent and it draws on subtalents. But the person who is centered in his or her ego is not as powerful or talented as the person he or she originally was, living the primary purpose of <span class="hlt">life</span>. This is because the original personality (the true self or “higher self”) is still there, active and alive, behind the ego. Symptoms, disorders, and diseases may be explained by the loss of energy, joy in <span class="hlt">life</span>, and intuitive competence because of inner conflicts, which may be alleviated or cured in the salutogenetic process of Antonovsky that helps patients find their sense of coherence or their primary purpose in <span class="hlt">life</span>. Many cases of reduced ability to function, physically as well as psychologically, socially or sexually, can also be explained and alleviated in this way. When a person discovers his true talent and begins to use it with dedication, privately as well as professionally, his <span class="hlt">life</span> will flourish and he may overcome even serious disease and great adversity in <span class="hlt">life</span>. The salutogenetic process can also be called personal development or “quality of <span class="hlt">life</span> as medicine”. It is important to note that the plan for personal development laid out by this theory is a plan not for the elimination of the ego, but for its cultivation. An existentially sound person still has a mental ego of course, but it is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14755108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14755108"><span>The <span class="hlt">life</span> <span class="hlt">mission</span> theory II. The structure of the <span class="hlt">life</span> purpose and the ego.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ventegodt, Søren; Andersen, Niels Jørgen; Merrick, Joav</p> <p>2003-12-11</p> <p>Pursuing your <span class="hlt">life</span> <span class="hlt">mission</span> is often very difficult, and many frustrations are experienced along the way. Major failures to bring out our potential can cause us considerable emotional pain. When this pain is unbearable, we are induced to shift from one intention and talent to another that better allows us to adapt and survive. Thus, we become set on a course that brings out a secondary or tertiary talent instead of the primary talent. This talent displacement may be expressed as a loss of our true nature or true self. The new purpose in <span class="hlt">life</span> now functions as the core of a new personality: the ego. The ego has a structure similar to that of the true self. It is anchored in a talent and it draws on subtalents. But the person who is centered in his or her ego is not as powerful or talented as the person he or she originally was, living the primary purpose of <span class="hlt">life</span>. This is because the original personality (the true self or "higher self") is still there, active and alive, behind the ego. Symptoms, disorders, and diseases may be explained by the loss of energy, joy in <span class="hlt">life</span>, and intuitive competence because of inner conflicts, which may be alleviated or cured in the salutogenetic process of Antonovsky that helps patients find their sense of coherence or their primary purpose in <span class="hlt">life</span>. Many cases of reduced ability to function, physically as well as psychologically, socially or sexually, can also be explained and alleviated in this way. When a person discovers his true talent and begins to use it with dedication, privately as well as professionally, his <span class="hlt">life</span> will flourish and he may overcome even serious disease and great adversity in <span class="hlt">life</span>. The salutogenetic process can also be called personal development or "quality of <span class="hlt">life</span> as medicine". It is important to note that the plan for personal development laid out by this theory is a plan not for the elimination of the ego, but for its cultivation. An existentially sound person still has a mental ego of course, but it is centered</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AcAau.106...63K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AcAau.106...63K"><span>A lander <span class="hlt">mission</span> to probe subglacial water on Saturn's moon Enceladus for <span class="hlt">life</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Konstantinidis, Konstantinos; Flores Martinez, Claudio L.; Dachwald, Bernd; Ohndorf, Andreas; Dykta, Paul; Bowitz, Pascal; Rudolph, Martin; Digel, Ilya; Kowalski, Julia; Voigt, Konstantin; Förstner, Roger</p> <p>2015-01-01</p> <p>The plumes discovered by the Cassini <span class="hlt">mission</span> emanating from the south pole of Saturn's moon Enceladus and the unique chemistry found in them have fueled speculations that Enceladus may harbor <span class="hlt">life</span>. The presumed aquiferous fractures from which the plumes emanate would make a prime target in the search for extraterrestrial <span class="hlt">life</span> and would be more easily accessible than the moon's subglacial ocean. A lander <span class="hlt">mission</span> that is equipped with a subsurface maneuverable ice melting probe will be most suitable to assess the existence of <span class="hlt">life</span> on Enceladus. A lander would have to land at a safe distance away from a plume source and melt its way to the inner wall of the fracture to analyze the plume subsurface liquids before potential biosignatures are degraded or destroyed by exposure to the vacuum of space. A possible approach for the in situ detection of biosignatures in such samples can be based on the hypothesis of universal evolutionary convergence, meaning that the independent and repeated emergence of <span class="hlt">life</span> and certain adaptive traits is wide-spread throughout the cosmos. We thus present a hypothetical evolutionary trajectory leading towards the emergence of methanogenic chemoautotrophic microorganisms as the baseline for putative biological complexity on Enceladus. To detect their presence, several instruments are proposed that may be taken aboard a future subglacial melting probe. The "Enceladus Explorer" (EnEx) project funded by the German Space Administration (DLR), aims to develop a terrestrial navigation system for a subglacial research probe and eventually test it under realistic conditions in Antarctica using the EnEx-IceMole, a novel maneuverable subsurface ice melting probe for clean sampling and in situ analysis of ice and subglacial liquids. As part of the EnEx project, an initial concept study is foreseen for a lander <span class="hlt">mission</span> to Enceladus to deploy the IceMole near one of the active water plumes on the moon's South-Polar Terrain, where it will search for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160012091','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160012091"><span>Guiding Requirements for Designing <span class="hlt">Life</span> Support System Architectures for Crewed Exploration <span class="hlt">Missions</span> Beyond Low-Earth Orbit</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perry, Jay L.; Sargusingh, Miriam J.; Toomarian, Nikzad</p> <p>2016-01-01</p> <p>The National Aeronautics and Space Administration's (NASA) technology development roadmaps provide guidance to focus technological development in areas that enable crewed exploration <span class="hlt">missions</span> beyond low-Earth orbit. Specifically, the technology area roadmap on human health, <span class="hlt">life</span> support and habitation systems describes the need for <span class="hlt">life</span> support system (LSS) technologies that can improve reliability and in-flight maintainability within a minimally-sized package while enabling a high degree of <span class="hlt">mission</span> autonomy. To address the needs outlined by the guiding technology area roadmap, NASA's Advanced Exploration Systems (AES) Program has commissioned the <span class="hlt">Life</span> Support Systems (LSS) Project to lead technology development in the areas of water recovery and management, atmosphere revitalization, and environmental monitoring. A notional exploration LSS architecture derived from the International Space has been developed and serves as the developmental basis for these efforts. Functional requirements and key performance parameters that guide the exploration LSS technology development efforts are presented and discussed. Areas where LSS flight operations aboard the ISS afford lessons learned that are relevant to exploration <span class="hlt">missions</span> are highlighted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150003840','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150003840"><span>Enviromnental Control and <span class="hlt">Life</span> Support Systems for Mars <span class="hlt">Missions</span> - Issues and Concerns for Planetary Protection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barta, Daniel J.; Anderson, Molly S.; Lange, Kevin</p> <p>2015-01-01</p> <p>Planetary protection represents an additional set of requirements that generally have not been considered by developers of technologies for Environmental Control and <span class="hlt">Life</span> Support Systems (ECLSS). Planetary protection guidelines will affect the kind of operations, processes, and functions that can take place during future human planetary exploration <span class="hlt">missions</span>. Ultimately, there will be an effect on <span class="hlt">mission</span> costs, including the <span class="hlt">mission</span> trade space when planetary protection requirements begin to drive vehicle deisgn in a concrete way. Planetary protection requirements need to be considered early in technology development and <span class="hlt">mission</span> programs in order to estimate these impacts and push back on requirements or find efficient ways to perform necessary functions. It is expected that planetary protection will be a significant factor during technology selection and system architecture design for future <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110007794','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110007794"><span>In Situ Biological Contamination Studies of the Moon: Implications for Planetary Protection and <span class="hlt">Life</span> Detection <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Glavin, Daniel P.; Dworkin, Jason P.; Lupisella, Mark; Williams, David R.; Kminek, Gerhard; Rummel, John D.</p> <p>2010-01-01</p> <p>NASA and ESA have outlined visions for solar system exploration that will include a series of lunar robotic precursor <span class="hlt">missions</span> to prepare for, and support a human return to the Moan, and future human exploration of Mars and other destinations, including possibly asteroids. One of the guiding principles for exploration is to pursue compelling scientific questions about the origin and evolution of <span class="hlt">life</span>. The search for <span class="hlt">life</span> on objects such as Mars will require careful operations, and that all systems be sufficiently cleaned and sterilized prior to launch to ensure that the scientific integrity of extraterrestrial samples is not jeopardized by terrestrial organic contamination. Under the Committee on Space Research's (COSPAR's) current planetary protection policy for the Moon, no sterilization procedures are required for outbound lunar spacecraft, nor is there a different planetary protection category for human <span class="hlt">missions</span>, although preliminary C SPAR policy guidelines for human <span class="hlt">missions</span> to Mars have been developed. Future in situ investigations of a variety of locations on the Moon by highly sensitive instruments designed to search for biologically derived organic compounds would help assess the contamination of the Moon by lunar spacecraft. These studies could also provide valuable "ground truth" data for Mars sample return <span class="hlt">missions</span> and help define planetary protection requirements for future Mars bound spacecraft carrying <span class="hlt">life</span> detection experiments. In addition, studies of the impact of terrestrial contamination of the lunar surface by the Apollo astronauts could provide valuable data to help refine future: Mars surface exploration plans for a human <span class="hlt">mission</span> to Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12469368','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12469368"><span>Reassessing the possibility of <span class="hlt">life</span> on venus: proposal for an astrobiology <span class="hlt">mission</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schulze-Makuch, Dirk; Irwin, Louis N</p> <p>2002-01-01</p> <p>With their similar size, chemical composition, and distance from the Sun, Venus and Earth may have shared a similar early history. Though surface conditions on Venus are now too extreme for <span class="hlt">life</span> as we know it, it likely had abundant water and favorable conditions for <span class="hlt">life</span> when the Sun was fainter early in the Solar System. Given the persistence of <span class="hlt">life</span> under stabilizing selection in static environments, it is possible that <span class="hlt">life</span> could exist in restricted environmental niches, where it may have retreated after conditions on the surface became untenable. High-pressure subsurface habitats with water in the supercritical liquid state could be a potential refugium, as could be the zone of dense cloud cover where thermoacidophilic <span class="hlt">life</span> might have retreated. Technology based on the Stardust <span class="hlt">Mission</span> to collect comet particles could readily be adapted for a pass through the appropriate cloud layer for sample collection and return to Earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AsBio...2..197S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AsBio...2..197S"><span>Reassessing the Possibility of <span class="hlt">Life</span> on Venus: Proposal for an Astrobiology <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schulze-Makuch, Dirk; Irwin, Louis N.</p> <p>2002-06-01</p> <p>With their similar size, chemical composition, and distance from the Sun, Venus and Earth may have shared a similar early history. Though surface conditions on Venus are now too extreme for <span class="hlt">life</span> as we know it, it likely had abundant water and favorable conditions for <span class="hlt">life</span> when the Sun was fainter early in the Solar System. Given the persistence of <span class="hlt">life</span> under stabilizing selection in static environments, it is possible that <span class="hlt">life</span> could exist in restricted environmental niches, where it may have retreated after conditions on the surface became untenable. High-pressure subsurface habitats with water in the supercritical liquid state could be a potential refugium, as could be the zone of dense cloud cover where thermoacidophilic <span class="hlt">life</span> might have retreated. Technology based on the Stardust <span class="hlt">Mission</span> to collect comet particles could readily be adapted for a pass through the appropriate cloud layer for sample collection and return to Earth.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19203238','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19203238"><span>Darwin--a <span class="hlt">mission</span> to detect and search for <span class="hlt">life</span> on extrasolar planets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cockell, C S; Léger, A; Fridlund, M; Herbst, T M; Kaltenegger, L; Absil, O; Beichman, C; Benz, W; Blanc, M; Brack, A; Chelli, A; Colangeli, L; Cottin, H; Coudé du Foresto, F; Danchi, W C; Defrère, D; den Herder, J-W; Eiroa, C; Greaves, J; Henning, T; Johnston, K J; Jones, H; Labadie, L; Lammer, H; Launhardt, R; Lawson, P; Lay, O P; LeDuigou, J-M; Liseau, R; Malbet, F; Martin, S R; Mawet, D; Mourard, D; Moutou, C; Mugnier, L M; Ollivier, M; Paresce, F; Quirrenbach, A; Rabbia, Y D; Raven, J A; Rottgering, H J A; Rouan, D; Santos, N C; Selsis, F; Serabyn, E; Shibai, H; Tamura, M; Thiébaut, E; Westall, F; White, G J</p> <p>2009-01-01</p> <p>The discovery of extrasolar planets is one of the greatest achievements of modern astronomy. The detection of planets that vary widely in mass demonstrates that extrasolar planets of low mass exist. In this paper, we describe a <span class="hlt">mission</span>, called Darwin, whose primary goal is the search for, and characterization of, terrestrial extrasolar planets and the search for <span class="hlt">life</span>. Accomplishing the <span class="hlt">mission</span> objectives will require collaborative science across disciplines, including astrophysics, planetary sciences, chemistry, and microbiology. Darwin is designed to detect rocky planets similar to Earth and perform spectroscopic analysis at mid-infrared wavelengths (6-20 mum), where an advantageous contrast ratio between star and planet occurs. The baseline <span class="hlt">mission</span> is projected to last 5 years and consists of approximately 200 individual target stars. Among these, 25-50 planetary systems can be studied spectroscopically, which will include the search for gases such as CO(2), H(2)O, CH(4), and O(3). Many of the key technologies required for the construction of Darwin have already been demonstrated, and the remainder are estimated to be mature in the near future. Darwin is a <span class="hlt">mission</span> that will ignite intense interest in both the research community and the wider public.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22897155','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22897155"><span>Effects of simulated space radiation on immunoassay components for <span class="hlt">life</span>-detection experiments in planetary exploration <span class="hlt">missions</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Derveni, Mariliza; Hands, Alex; Allen, Marjorie; Sims, Mark R; Cullen, David C</p> <p>2012-08-01</p> <p>The <span class="hlt">Life</span> Marker Chip (LMC) instrument is part of the proposed payload on the ESA ExoMars rover that is scheduled for launch in 2018. The LMC will use antibody-based assays to detect molecular signatures of <span class="hlt">life</span> in samples obtained from the shallow subsurface of Mars. For the LMC antibodies, the ability to resist inactivation due to space particle radiation (both in transit and on the surface of Mars) will therefore be a prerequisite. The proton and neutron components of the <span class="hlt">mission</span> radiation environment are those that are expected to have the dominant effect on the operation of the LMC. Modeling of the radiation environment for a <span class="hlt">mission</span> to Mars led to the calculation of nominal <span class="hlt">mission</span> fluences for proton and neutron radiation. Various combinations and multiples of these values were used to demonstrate the effects of radiation on antibody activity, primarily at the radiation levels envisaged for the ExoMars <span class="hlt">mission</span> as well as at much higher levels. Five antibodies were freeze-dried in a variety of protective molecular matrices and were exposed to various radiation conditions generated at a cyclotron facility. After exposure, the antibodies' ability to bind to their respective antigens was assessed and found to be unaffected by ExoMars <span class="hlt">mission</span> level radiation doses. These experiments indicated that the expected radiation environment of a Mars <span class="hlt">mission</span> does not pose a significant risk to antibodies packaged in the form anticipated for the LMC instrument.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920034049&hterms=science+important&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dscience%2Bimportant','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920034049&hterms=science+important&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dscience%2Bimportant"><span><span class="hlt">Life</span> sciences get important new data from Spacelab <span class="hlt">mission</span>. III</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schuiling, Roelof L.; Young, Steven</p> <p>1991-01-01</p> <p>An investigation of the effects of weightlessness on the human body is reported that was conducted on a flight of the Space Shuttle Columbia. Experiments are described regarding zero-gravity effects on the human perception of balance, the growth of lymphocytes, and general <span class="hlt">life</span>-sciences examinations of body mass, body fluid, pulmonary parameters, and echocardiograph imaging. Specific attention is given to the day-to-day operations of the <span class="hlt">mission</span>, and particular emphasis is given to the study of rodents and jellyfish reacting to microgravity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E1608Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E1608Q"><span>Research on <span class="hlt">Life</span> Science and <span class="hlt">Life</span> Support Engineering Problems of Manned Deep Space Exploration <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qi, Bin; Guo, Linli; Zhang, Zhixian</p> <p>2016-07-01</p> <p>Space <span class="hlt">life</span> science and <span class="hlt">life</span> support engineering are prominent problems in manned deep space exploration <span class="hlt">mission</span>. Some typical problems are discussed in this paper, including long-term <span class="hlt">life</span> support problem, physiological effect and defense of varying extraterrestrial environment. The causes of these problems are developed for these problems. To solve these problems, research on space <span class="hlt">life</span> science and space medical-engineering should be conducted. In the aspect of space <span class="hlt">life</span> science, the study of space gravity biology should focus on character of physiological effect in long term zero gravity, co-regulation of physiological systems, impact on stem cells in space, etc. The study of space radiation biology should focus on target effect and non-target effect of radiation, carcinogenicity of radiation, spread of radiation damage in <span class="hlt">life</span> system, etc. The study of basic biology of space <span class="hlt">life</span> support system should focus on theoretical basis and simulating mode of constructing the <span class="hlt">life</span> support system, filtration and combination of species, regulation and optimization method of <span class="hlt">life</span> support system, etc. In the aspect of space medical-engineering, the study of bio-regenerative <span class="hlt">life</span> support technology should focus on plants cultivation technology, animal-protein production technology, waste treatment technology, etc. The study of varying gravity defense technology should focus on biological and medical measures to defend varying gravity effect, generation and evaluation of artificial gravity, etc. The study of extraterrestrial environment defense technology should focus on risk evaluation of radiation, monitoring and defending of radiation, compound prevention and removal technology of dust, etc. At last, a case of manned lunar base is analyzed, in which the effective schemes of <span class="hlt">life</span> support system, defense of varying gravity, defense of extraterrestrial environment are advanced respectively. The points in this paper can be used as references for intensive study on key</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060043569&hterms=life+planets&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dlife%2Bplanets','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060043569&hterms=life+planets&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dlife%2Bplanets"><span>Assessment of in-flight anomalies of long <span class="hlt">life</span> outer plant <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hoffman, Alan R.; Green, Nelson W.; Garrett, Henry B.</p> <p>2004-01-01</p> <p>Thee unmanned planetary spacecraft to the outer planets have been controlled and operated successfully in space for an accumulated total of 66 years. The Voyager 1 and 2 spacecraft each have been in space for more than 26 years. The Galileo spacecraft was in space for 14 years, including eight years in orbit about Jupiter. During the flight operations for these <span class="hlt">missions</span>, anomalies for the ground data system and the flight systems have been tracked using the anomaly reporting tool at the Jet Propulsion Laboratory. A total of 3300 incidents, surprises, and anomaly reports have been recorded in the database. This paper describes methods and results for classifying and identifying trends relative to ground system vs. flight system, software vs. hardware, and corrective actions. There are several lessons learned from these assessments that significantly benefit the design and planning for long <span class="hlt">life</span> <span class="hlt">missions</span> of the future. These include the necessity for having redundancy for successful operation of the spacecraft, awareness that anomaly reporting is dependent on <span class="hlt">mission</span> activity not the age of the spacecraft, and the need for having a program to maintain and transfer operation knowledge and tools to replacement flight team members.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870008364','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870008364"><span>Manned Mars <span class="hlt">mission</span> environmental control and <span class="hlt">life</span> support subsystem</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hueter, Uwe</p> <p>1986-01-01</p> <p>A specific design is not presented, but the general philosophy regarding potential Environmental Control/<span class="hlt">Life</span> Support System (ECLSS) requirements, concepts, issues, and technology needs are discussed. The focus is on a manned Mars <span class="hlt">mission</span> occurring in the late 1990's. Discussions on the Trans-Mars Vehicle, the Mars Excursion Module (MEM), and a Martian base facility are covered. The functions, performance requirements, and design loads of a typical ECLSS are listed, and the issues and technology briefly discussed. Several ECLSS concepts and options are identified, and comparative weights and volumes are provided for these. Several aspects of the space station ECLSS are contrasted with the Mars element ECLSS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ACP....16.7899A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ACP....16.7899A"><span>Ship emissions measurement in the Arctic by plume intercepts of the Canadian Coast Guard <span class="hlt">icebreaker</span> Amundsen from the Polar 6 aircraft platform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aliabadi, Amir A.; Thomas, Jennie L.; Herber, Andreas B.; Staebler, Ralf M.; Leaitch, W. Richard; Schulz, Hannes; Law, Kathy S.; Marelle, Louis; Burkart, Julia; Willis, Megan D.; Bozem, Heiko; Hoor, Peter M.; Köllner, Franziska; Schneider, Johannes; Levasseur, Maurice; Abbatt, Jonathan P. D.</p> <p>2016-06-01</p> <p>Decreasing sea ice and increasing marine navigability in northern latitudes have changed Arctic ship traffic patterns in recent years and are predicted to increase annual ship traffic in the Arctic in the future. Development of effective regulations to manage environmental impacts of shipping requires an understanding of ship emissions and atmospheric processing in the Arctic environment. As part of the summer 2014 NETCARE (Network on Climate and Aerosols) campaign, the plume dispersion and gas and particle emission factors of effluents originating from the Canadian Coast Guard <span class="hlt">icebreaker</span> Amundsen operating near Resolute Bay, NU, Canada, were investigated. The Amundsen burned distillate fuel with 1.5 wt % sulfur. Emissions were studied via plume intercepts using the Polar 6 aircraft measurements, an analytical plume dispersion model, and using the FLEXPART-WRF Lagrangian particle dispersion model. The first plume intercept by the research aircraft was carried out on 19 July 2014 during the operation of the Amundsen in the open water. The second and third plume intercepts were carried out on 20 and 21 July 2014 when the Amundsen had reached the ice edge and operated under <span class="hlt">ice-breaking</span> conditions. Typical of Arctic marine navigation, the engine load was low compared to cruising conditions for all of the plume intercepts. The measured species included mixing ratios of CO2, NOx, CO, SO2, particle number concentration (CN), refractory black carbon (rBC), and cloud condensation nuclei (CCN). The results were compared to similar experimental studies in mid-latitudes. Plume expansion rates (γ) were calculated using the analytical model and found to be γ = 0.75 ± 0.81, 0.93 ± 0.37, and 1.19 ± 0.39 for plumes 1, 2, and 3, respectively. These rates were smaller than prior studies conducted at mid-latitudes, likely due to polar boundary layer dynamics, including reduced turbulent mixing compared to mid-latitudes. All emission factors were in agreement with prior</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780019030','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780019030"><span>Critical review of Ames <span class="hlt">Life</span> Science participation in Spacelab <span class="hlt">Mission</span> Development Test 3: The SMD 3 management study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Helmreich, R.; Wilhelm, J.; Tanner, T. A.; Sieber, J. E.; Burgenbauch, S.</p> <p>1978-01-01</p> <p>A management study was conducted to specify activities and problems encountered during the development of procedures for documentation and crew training on experiments, as well as during the design, integration, and delivery of a <span class="hlt">life</span> sciences experiment payload to Johnson Space Center for a 7 day simulation of a Spacelab <span class="hlt">mission</span>. Conclusions and recommendations to project management for current and future Ames' <span class="hlt">life</span> sciences projects are included. Broader issues relevant to the conduct of future scientific <span class="hlt">missions</span> under the constraints imposed by the environment of space are also addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007LPICo1353.3135S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007LPICo1353.3135S"><span>Searching for <span class="hlt">Life</span> in the Martian Subsurface: Results from the MARTE Astrobiological Drilling Experiment and Implications for Future <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stoker, C. R.</p> <p>2007-07-01</p> <p>Drilling for subsurface <span class="hlt">life</span> should be a goal of future Mars <span class="hlt">missions</span>. The approach is illustrated by MARTE: A search for subsurface <span class="hlt">life</span> in Rio Tinto, Spain explored a biosphere using reduced iron and sulfur minerals and demonstrated automated drilling, sample handling, and <span class="hlt">life</span> detection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980237901','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980237901"><span><span class="hlt">Life</span> and Microgravity Sciences Spacelab <span class="hlt">Mission</span>: Human Research Pilot Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Arnaud, Sara B. (Editor); Walker, Karen R. (Editor); Hargens, Alan (Editor)</p> <p>1996-01-01</p> <p>The <span class="hlt">Life</span> Sciences, Microgravity Science and Spacelab <span class="hlt">Mission</span> contains a number of human experiments directed toward identifying the functional, metabolic and neurological characteristics of muscle weakness and atrophy during space flight. To ensure the successful completion of the flight experiments, a ground-based pilot study, designed to mimic the flight protocols as closely as possible, was carried out in the head-down tilt bed rest model. This report records the rationales, procedures, preliminary results and estimated value of the pilot study, the first of its kind, for 12 of the 13 planned experiments in human research. The bed rest study was conducted in the Human Research Facility at Ames Research Center from July 11 - August 28, 1995. Eight healthy male volunteers performed the experiments before, during and after 17 days bed rest. The immediate purposes of this simulation were to integrate the experiments, provide data in a large enough sample for publication of results, enable investigators to review individual experiments in the framework of a multi-disciplinary study and relay the experience of the pilot study to the <span class="hlt">mission</span> specialists prior to launch.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100036597','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100036597"><span>In Situ Biological Contamination Studies of the Moon: Implications for Future Planetary Protection and <span class="hlt">Life</span> Detection <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Glavin, Daniel P.; Dworkin, Jason P.; Lupisella, Mark; Kminek, Gerhard; Rummel, John D.</p> <p>2010-01-01</p> <p>NASA and ESA have outlined visions for solar system exploration that will include a series of lunar robotic precursor <span class="hlt">missions</span> to prepare for, and support a human return to the Moon, and future human exploration of Mars and other destinations. One of the guiding principles for exploration is to pursue compelling scientific questions about the origin and evolution of <span class="hlt">life</span>. The search for <span class="hlt">life</span> on objects such as Mars will require that all spacecraft and instrumentation be sufficiently cleaned and sterilized prior to launch to ensure that the scientific integrity of extraterrestrial samples is not jeopardized by terrestrial organic contamination. Under the Committee on Space Research's (COSPAR's) current planetary protection policy for the Moon, no sterilization procedures are required for outbound lunar spacecraft, nor is there yet a planetary protection category for human <span class="hlt">missions</span>. Future in situ investigations of a variety of locations on the Moon by highly sensitive instruments designed to search for biologically derived organic compounds would help assess the contamination of the Moon by lunar spacecraft. These studies could also provide valuable "ground truth" data for Mars sample return <span class="hlt">missions</span> and help define planetary protection requirements for future Mars bound spacecraft carrying <span class="hlt">life</span> detection experiments. In addition, studies of the impact of terrestrial contamination of the lunar surface by the Apollo astronauts could provide valuable data to help refine future Mars surface exploration plans for a human <span class="hlt">mission</span> to Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006PhDT.......174A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006PhDT.......174A"><span>A simulation based optimization approach to model and design <span class="hlt">life</span> support systems for manned space <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aydogan, Selen</p> <p></p> <p>This dissertation considers the problem of process synthesis and design of <span class="hlt">life</span>-support systems for manned space <span class="hlt">missions</span>. A <span class="hlt">life</span>-support system is a set of technologies to support human <span class="hlt">life</span> for short and long-term spaceflights, via providing the basic <span class="hlt">life</span>-support elements, such as oxygen, potable water, and food. The design of the system needs to meet the crewmember demand for the basic <span class="hlt">life</span>-support elements (products of the system) and it must process the loads generated by the crewmembers. The system is subject to a myriad of uncertainties because most of the technologies involved are still under development. The result is high levels of uncertainties in the estimates of the model parameters, such as recovery rates or process efficiencies. Moreover, due to the high recycle rates within the system, the uncertainties are amplified and propagated within the system, resulting in a complex problem. In this dissertation, two algorithms have been successfully developed to help making design decisions for <span class="hlt">life</span>-support systems. The algorithms utilize a simulation-based optimization approach that combines a stochastic discrete-event simulation and a deterministic mathematical programming approach to generate multiple, unique realizations of the controlled evolution of the system. The timelines are analyzed using time series data mining techniques and statistical tools to determine the necessary technologies, their deployment schedules and capacities, and the necessary basic <span class="hlt">life</span>-support element amounts to support crew <span class="hlt">life</span> and activities for the <span class="hlt">mission</span> duration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=S92-40040&hterms=raft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Draft','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=S92-40040&hterms=raft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Draft"><span>STS-52 <span class="hlt">Mission</span> Specialist Veach in <span class="hlt">life</span> raft during JSC bailout exercises</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1992-01-01</p> <p>STS-52 Columbia, Orbiter Vehicle (OV) 102, <span class="hlt">Mission</span> Specialist (MS) Charles Lacy Veach, wearing launch and entry suit (LES) and launch and entry helmet (LEH), floats in a single person <span class="hlt">life</span> raft during emergency egress (bailout) training exercises in JSC's Weightless Environment Training Facility (WETF) Bldg 29 pool. SCUBA-equipped divers look on. The bailout exercises utilize the WETF's 25-foot deep pool as the ocean for this water landing simulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950015114','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950015114"><span>Power systems for future <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gill, S. P.; Frye, P. E.; Littman, Franklin D.; Meisl, C. J.</p> <p>1994-01-01</p> <p>A comprehensive scenario of future <span class="hlt">missions</span> was developed and applicability of different power technologies to these <span class="hlt">missions</span> was assessed. Detailed technology development roadmaps for selected power technologies were generated. A simple methodology to evaluate economic benefits of current and future power system technologies by comparing <span class="hlt">Life</span> Cycle Costs of potential <span class="hlt">missions</span> was developed. The methodology was demonstrated by comparing <span class="hlt">Life</span> Cycle Costs for different implementation strategies of DIPS/CBC technology to a selected set of <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15806741','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15806741"><span>Analysis of a spacecraft <span class="hlt">life</span> support system for a Mars <span class="hlt">mission</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Czupalla, M; Aponte, V; Chappell, S; Klaus, D</p> <p>2004-01-01</p> <p>This report summarizes a trade study conducted as part of the Fall 2002 semester Spacecraft <span class="hlt">Life</span> Support System Design course (ASEN 5116) in the Aerospace Engineering Sciences Department at the University of Colorado. It presents an analysis of current <span class="hlt">life</span> support system technologies and a preliminary design of an integrated system for supporting humans during transit to and on the surface of the planet Mars. This effort was based on the NASA Design Reference <span class="hlt">Mission</span> (DRM) for the human exploration of Mars [NASA Design Reference <span class="hlt">Mission</span> (DRM) for Mars, Addendum 3.0, from the world wide web: http://exploration.jsc.nasa.gov/marsref/contents.html.]. The integrated design was broken into four subsystems: Water Management, Atmosphere Management, Waste Processing, and Food Supply. The process started with the derivation of top-level requirements from the DRM. Additional system and subsystem level assumptions were added where clarification was needed. Candidate technologies were identified and characterized based on performance factors. Trade studies were then conducted for each subsystem. The resulting technologies were integrated into an overall design solution using mass flow relationships. The system level trade study yielded two different configurations--one for the transit to Mars and another for the surface habitat, which included in situ resource utilization. Equivalent System Mass analyses were used to compare each design against an open-loop (non-regenerable) baseline system. c2003 International Astronautical Federation. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017LPICo2042.4124C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017LPICo2042.4124C"><span>Enceladus <span class="hlt">Life</span> Finder (ELF): A Proposed <span class="hlt">Mission</span> to Assess the Habitability of a Plume-Bearing World</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cable, M. L.; Spilker, L. J.; Postberg, F.; Waite, J. H.; Kempf, S.; Clark, K.; Reh, K.; Sherwood, B.; Lunine, J. I.</p> <p>2017-11-01</p> <p>Enceladus is a uniquely accessible ocean world due to its plume emanating from the south polar terrain. Here we discuss the Enceladus <span class="hlt">Life</span> Finder <span class="hlt">mission</span> concept and its implications for this and other ocean worlds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130011629','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130011629"><span>Environmental Controls and <span class="hlt">Life</span> Support System (ECLSS) Design for a Multi-<span class="hlt">Mission</span> Space Exploration Vehicle (MMSEV)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stambaugh, Imelda; Baccus, Shelley; Buffington, Jessie; Hood, Andrew; Naids, Adam; Borrego, Melissa; Hanford, Anthony J.; Eckhardt, Brad; Allada, Rama Kumar; Yagoda, Evan</p> <p>2013-01-01</p> <p>Engineers at Johnson Space Center (JSC) are developing an Environmental Control and <span class="hlt">Life</span> Support System (ECLSS) design for the Multi-<span class="hlt">Mission</span> Space Exploration Vehicle (MMSEV). The purpose of the MMSEV is to extend the human exploration envelope for Lunar, Near Earth Object (NEO), or Deep Space <span class="hlt">missions</span> by using pressurized exploration vehicles. The MMSEV, formerly known as the Space Exploration Vehicle (SEV), employs ground prototype hardware for various systems and tests it in manned and unmanned configurations. Eventually, the system hardware will evolve and become part of a flight vehicle capable of supporting different design reference <span class="hlt">missions</span>. This paper will discuss the latest MMSEV ECLSS architectures developed for a variety of design reference <span class="hlt">missions</span>, any work contributed toward the development of the ECLSS design, lessons learned from testing prototype hardware, and the plan to advance the ECLSS toward a flight design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120016969','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120016969"><span>Environmental Controls and <span class="hlt">Life</span> Support System (ECLSS) Design for a Multi-<span class="hlt">Mission</span> Space Exploration Vehicle (MMSEV)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stambaugh, Imelda; Baccus, Shelley; Naids, Adam; Hanford, Anthony</p> <p>2012-01-01</p> <p>Engineers at Johnson Space Center (JSC) are developing an Environmental Control and <span class="hlt">Life</span> Support System (ECLSS) design for the Multi-<span class="hlt">Mission</span> Space Exploration Vehicle (MMSEV). The purpose of the MMSEV is to extend the human exploration envelope for Lunar, Near Earth Object (NEO), or Deep Space <span class="hlt">missions</span> by using pressurized exploration vehicles. The MMSEV, formerly known as the Space Exploration Vehicle (SEV), employs ground prototype hardware for various systems and tests it in manned and unmanned configurations. Eventually, the system hardware will evolve and become part of a flight vehicle capable of supporting different design reference <span class="hlt">missions</span>. This paper will discuss the latest MMSEV ECLSS architectures developed for a variety of design reference <span class="hlt">missions</span>, any work contributed toward the development of the ECLSS design, lessons learned from testing prototype hardware, and the plan to advance the ECLSS toward a flight design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980024344','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980024344"><span><span class="hlt">Life</span> Sciences Issues for a <span class="hlt">Mission</span> to Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>Session MP5 includes short reports on: (1) Cardiovascular Concerns for a Mars <span class="hlt">Mission</span>: Autonomic and Biomechanical Effects; (2) Reducing the Risk of Space Radiation Induced Bioeffects: Vehicle Design and Protectant Molecules; (3) Musculoskeletal Issues for Long Duration <span class="hlt">Mission</span>: Muscle Mass Preservation, Renal Stone Risk Factors, Countermeasures, and Contingency Treatment Planning; (4) Psychological Issues and Crew Selection for a Mars <span class="hlt">Mission</span>: Maximizing the Mix for the Long Haul; and (5) Issues in Crew Health, Medical Selection and Medical Officer (CMO) Training for a <span class="hlt">Mission</span> to Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017LPICo1989.8100S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017LPICo1989.8100S"><span>Affordable Precursor <span class="hlt">Missions</span> to Search for <span class="hlt">Life</span> and Pave the Way for Human Exploration of Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stoker, C. R.</p> <p>2017-02-01</p> <p>The goal of landing humans on Mars in the 2030s requires a precursor program to assess modern <span class="hlt">life</span> on Mars and assess the water resource of near surface ground ice. <span class="hlt">Missions</span> that address these issues are presented.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880014327','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880014327"><span>Manned Mars <span class="hlt">mission</span> accommodation: Sprint <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cirillo, William M.; Kaszubowski, Martin J.; Ayers, J. Kirk; Llewellyn, Charles P.; Weidman, Deene J.; Meredith, Barry D.</p> <p>1988-01-01</p> <p>The results of a study conducted at the NASA-LaRC to assess the impacts on the Phase 2 Space Station of Accommodating a Manned <span class="hlt">Mission</span> to Mars are documented. In addition, several candidate transportation node configurations are presented to accommodate the assembly and verification of the Mars <span class="hlt">Mission</span> vehicles. This study includes an identification of a <span class="hlt">life</span> science research program that would need to be completed, on-orbit, prior to <span class="hlt">mission</span> departure and an assessment of the necessary orbital technology development and demonstration program needed to accomplish the <span class="hlt">mission</span>. Also included is an analysis of the configuration mass properties and a preliminary analysis of the Space Station control system sizing that would be required to control the station. Results of the study indicate the Phase 2 Space Station can support a manned <span class="hlt">mission</span> to Mars with the addition of a supporting infrastructure that includes a propellant depot, assembly hangar, and a heavy lift launch vehicle to support the large launch requirements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004cosp...35.4173T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004cosp...35.4173T"><span>Biological <span class="hlt">life</span> support systems for martian <span class="hlt">missions</span>: some problems and prospects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tikhomirov, A. A.; Ushakova, S. A.; Kovaleva, N. P.; Lasseur, C.</p> <p></p> <p>Taking into account the experience of scientific researches obtained during experiments in the BIOS - 3 of the Institute of Biophysics of Siberian Branch of Russian Academy of Science (IBP SB RAS) and the MELISSA program (ESA), approaches in creation biological <span class="hlt">life</span> support systems for a flight period and a fixed-site base of Martian <span class="hlt">mission</span> are considered. Various alternate variants of designing of elements of BLSS based on use of Chlorella and/or Spirulina, and also greenhouses with higher plants for the flight period of Martian <span class="hlt">mission</span> are analyzed. For this purpose construction of BLSS ensuring full closure of matter turnover according to gas exchange and water and partial closure on the human's exometabolites is supposed. For the fixed site Martian station BLSS based on use of higher plants with a various degree of closure of internal mass exchange are suggested. Various versions of BLSS configuration and degree of closure of mass exchange depending on duration of Martian <span class="hlt">mission</span>, the diet type of a crew and some other conditions are considered. Special attention is given to problems of reliability and tolerance of matter turnover processes in BLSS which maintenance is connected, in particular, with additional oxygen reproduction inside a system. Technologies for realization of BLSS of various configurations are offered and justified. The auxiliary role of the physicochemical methods in BLSS functioning both for the flight period and for the crew stay on Mars is justified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089897&hterms=test+automation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtest%2Bautomation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089897&hterms=test+automation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dtest%2Bautomation"><span><span class="hlt">Mission</span> simulation as an approach to develop requirements for automation in Advanced <span class="hlt">Life</span> Support Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Erickson, J. D.; Eckelkamp, R. E.; Barta, D. J.; Dragg, J.; Henninger, D. L. (Principal Investigator)</p> <p>1996-01-01</p> <p>This paper examines <span class="hlt">mission</span> simulation as an approach to develop requirements for automation and robotics for Advanced <span class="hlt">Life</span> Support Systems (ALSS). The focus is on requirements and applications for command and control, control and monitoring, situation assessment and response, diagnosis and recovery, adaptive planning and scheduling, and other automation applications in addition to mechanized equipment and robotics applications to reduce the excessive human labor requirements to operate and maintain an ALSS. Based on principles of systems engineering, an approach is proposed to assess requirements for automation and robotics using <span class="hlt">mission</span> simulation tools. First, the story of a simulated <span class="hlt">mission</span> is defined in terms of processes with attendant types of resources needed, including options for use of automation and robotic systems. Next, systems dynamics models are used in simulation to reveal the implications for selected resource allocation schemes in terms of resources required to complete operational tasks. The simulations not only help establish ALSS design criteria, but also may offer guidance to ALSS research efforts by identifying gaps in knowledge about procedures and/or biophysical processes. Simulations of a planned one-year <span class="hlt">mission</span> with 4 crewmembers in a Human Rated Test Facility are presented as an approach to evaluation of <span class="hlt">mission</span> feasibility and definition of automation and robotics requirements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720008139','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720008139"><span>Space station (modular) <span class="hlt">mission</span> analysis. Volume 1: <span class="hlt">Mission</span> analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1971-01-01</p> <p>The <span class="hlt">mission</span> analysis on the modular space station considers experimental requirements and options characterized by low initial cost and incremental manning. Features that affect initial development and early operating costs are identified and their impacts on the program are assessed. Considered are the areas of experiment, <span class="hlt">mission</span>, operations, information management, and long <span class="hlt">life</span> and safety analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150022488','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150022488"><span>Development of Bioregenerative <span class="hlt">Life</span> Support for Longer <span class="hlt">Missions</span>: When Can Plants Begin to Contribute to Atmospheric Management?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wheeler, Raymond M.</p> <p>2015-01-01</p> <p>Through photosynthesis, plants can be used to generate oxygen and food for <span class="hlt">life</span> support in human exploration of space. Initial contributions of plants to <span class="hlt">life</span> support would likely occur through the production of supplemental, fresh foods. For plants to provide significant contributions to oxygen production, larger areas and significant lighting would be needed. An area of 10 m2 of plants with moderate lighting could provide about 13 of a human's oxygen needs. As <span class="hlt">mission</span> distances and durations increase, plant growing areas could be expanded to assume more of the human <span class="hlt">life</span> support needs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920012000','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920012000"><span>A lunar base reference <span class="hlt">mission</span> for the phased implementation of bioregenerative <span class="hlt">life</span> support system components</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dittmer, Laura N.; Drews, Michael E.; Lineaweaver, Sean K.; Shipley, Derek E.; Hoehn, A.</p> <p>1991-01-01</p> <p>Previous design efforts of a cost effective and reliable regenerative <span class="hlt">life</span> support system (RLSS) provided the foundation for the characterization of organisms or 'biological processors' in engineering terms and a methodology was developed for their integration into an engineered ecological LSS in order to minimize the mass flow imbalances between consumers and producers. These techniques for the design and the evaluation of bioregenerative LSS have now been integrated into a lunar base reference <span class="hlt">mission</span>, emphasizing the phased implementation of components of such a BLSS. In parallel, a designers handbook was compiled from knowledge and experience gained during past design projects to aid in the design and planning of future space <span class="hlt">missions</span> requiring advanced RLSS technologies. The lunar base reference <span class="hlt">mission</span> addresses in particular the phased implementation and integration of BLS parts and includes the resulting infrastructure burdens and needs such as mass, power, volume, and structural requirements of the LSS. Also, operational aspects such as manpower requirements and the possible need and application of 'robotics' were addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140003749','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140003749"><span>Modified ACES Portable <span class="hlt">Life</span> Support Integration, Design, and Testing for Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kelly, Cody</p> <p>2014-01-01</p> <p>NASA's next generation of exploration <span class="hlt">missions</span> provide a unique challenge to designers of EVA <span class="hlt">life</span> support equipment, especially in a fiscally-constrained environment. In order to take the next steps of manned space exploration, NASA is currently evaluating the use of the Modified ACES (MACES) suit in conjunction with the Advanced Portable <span class="hlt">Life</span> Support System (PLSS) currently under development. This paper will detail the analysis and integration of the PLSS thermal and ventilation subsystems into the MACES pressure garment, design of prototype hardware, and hardware-in-the-loop testing during the spring 2014 timeframe. Prototype hardware was designed with a minimal impact philosophy in order to mitigate design constraints becoming levied on either the advanced PLSS or MACES subsystems. Among challenges faced by engineers were incorporation of <span class="hlt">life</span> support thermal water systems into the pressure garment cavity, operational concept definition between vehicle/portable <span class="hlt">life</span> support system hardware, and structural attachment mechanisms while still enabling maximum EVA efficiency from a crew member's perspective. Analysis was completed in late summer 2013 to 'bound' hardware development, with iterative analysis cycles throughout the hardware development process. The design effort will cumulate in the first ever manned integration of NASA's advanced PLSS system with a pressure garment originally intended primarily for use in a contingency survival scenario.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830060824&hterms=animal+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Danimal%2Bscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830060824&hterms=animal+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Danimal%2Bscience"><span>The first dedicated <span class="hlt">life</span> sciences <span class="hlt">mission</span> - Spacelab 4</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cramer, D. R.; Reid, D. H.; Klein, H. P.</p> <p>1983-01-01</p> <p>The details of the payload and the experiments in Spacelab 4, the first Spacelab <span class="hlt">mission</span> dedicated entirely to the <span class="hlt">life</span> sciences, are discussed. The payload of Spacelab 4, carried in the bay of the Shuttle Orbiter, consists of 25 tentatively selected investigations combined into a comprehensive integrated exploration of the effects of acute weightlessness on living systems. The payload contains complementary designs in the human and animal investigations in order to validate animal models of human physiology in weightlessness. Animals used as experimental subjects will include squirrel monkeys, laboratory rats, several species of plants, and frog eggs. The main scientific objectives of the investigations include the study of the acute cephalic fluid shift, cardiovascular adaptation to weightlessness, including postflight reductions in orthostatic tolerance and exercise capacity, and changes in vestibular function, including space motion sickness, associated with weightlessness. Other scientific objective include the study of red cell mass reduction, negative nitrogen balance, altered calcium metabolism, suppressed in vitro lymphocyte reactivity, gravitropism and photropism in plants, and fertilization and early development in frog eggs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017496','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017496"><span>Investigation of Bio-Regenerative <span class="hlt">Life</span> Support and Trash-To-Gas Experiment on a 4 Month Mars Simulation <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Caraccio, Anne; Poulet, Lucie; Hintze, Paul E.; Miles, John D.</p> <p>2014-01-01</p> <p>Future crewed <span class="hlt">missions</span> to other planets or deep space locations will require regenerative <span class="hlt">Life</span> Support Systems (LSS) as well as recycling processes for <span class="hlt">mission</span> waste. Constant resupply of many commodity materials will not be a sustainable option for deep space <span class="hlt">missions</span>, nor will storing trash on board a vehicle or at a lunar or Martian outpost. The habitable volume will decline as the volume of waste increases. A complete regenerative environmentally controlled <span class="hlt">life</span> support system (ECLSS) on an extra-terrestrial outpost will likely include physico-chemical and biological technologies, such as bioreactors and greenhouse modules. Physico-chemical LSS do not enable food production and bio-regenerative LSS are not stable enough to be used alone in space. <span class="hlt">Mission</span> waste that cannot be recycled into the bio-regenerative ECLSS can include excess food, food packaging, clothing, tape, urine and fecal waste. This waste will be sent to a system for converting the trash into the high value products. Two crew members on a 120 day Mars analog simulation, in collaboration with Kennedy Space Centers (KSC) Trash to Gas (TtG) project investigated a semi-closed loop system that treated non-edible biomass and other logistical waste for volume reduction and conversion into useful commodities. The purposes of this study are to show the how plant growth affects the amount of resources required by the habitat and how spent plant material can be recycled. Real-time data was sent to the reactor at KSC in Florida for replicating the analog <span class="hlt">mission</span> waste for laboratory operation. This paper discusses the 120 day <span class="hlt">mission</span> plant growth activity, logistical and plant waste management, power and water consumption effects of the plant and logistical waste, and potential energy conversion techniques using KSCs TtG reactor technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140017444','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140017444"><span>Investigation of Bio-Regenerative <span class="hlt">Life</span> Support and Trash-to-Gas Experiment on a 4-Month Mars Simulation <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Caraccio, Anne; Poulet, Lucie; Hintze, Paul E.; Miles, John D.</p> <p>2014-01-01</p> <p>Future crewed <span class="hlt">missions</span> to other planets or deep space locations will require regenerative <span class="hlt">Life</span> Support Systems (LSS) as well as recycling processes for <span class="hlt">mission</span> waste. Constant resupply of many commodity materials will not be a sustainable option for deep space <span class="hlt">missions</span>, nor will stowing trash on board a vehicle or at a lunar or Martian outpost. The habitable volume will decline as the volume of waste increases. A complete regenerative environmentally controlled <span class="hlt">life</span> support system (ECLSS) on an extra-terrestrial outpost will likely include physico-chemical and biological technologies, such as bioreactors and greenhouse modules. Physico-chemical LSS do not enable food production and bio-regenerative LSS are not stable enough to be used alone in space. <span class="hlt">Mission</span> waste that cannot be recycled into the bio-regenerative ECLSS can include excess food, food packaging, clothing, tape, urine and fecal waste. This waste will be sent to a system for converting the trash into high value products. Two crew members on a 120 day Mars analog simulation, in collaboration with Kennedy Space Centers (KSC) Trash to Gas (TtG) project investigated a semi-closed loop system that treated non-edible biomass and other logistical waste for volume reduction and conversion into useful commodities. The purpose of this study is to show how plant growth affects the amount of resources required by the habitat and how spent plant material can be recycled. Real-time data was sent to the reactor at KSC in Florida for replicating the analog <span class="hlt">mission</span> waste for laboratory operation. This paper discusses the 120 day <span class="hlt">mission</span> plant growth activity, logistical and plant waste management, power and water consumption effects of the plant and logistical waste, and potential energy conversion techniques using KSCs TtG technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AdSpR..40.1741T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AdSpR..40.1741T"><span>Biological <span class="hlt">life</span> support systems for a Mars <span class="hlt">mission</span> planetary base: Problems and prospects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tikhomirov, A. A.; Ushakova, S. A.; Kovaleva, N. P.; Lamaze, B.; Lobo, M.; Lasseur, Ch.</p> <p></p> <p>The study develops approaches to designing biological <span class="hlt">life</span> support systems for the Mars <span class="hlt">mission</span> - for the flight conditions and for a planetary base - using experience of the Institute of Biophysics of the Siberian Branch of the Russian Academy of Sciences (IBP SB RAS) with the Bios-3 system and ESA's experience with the MELISSA program. Variants of a BLSS based on using Chlorella and/or Spirulina and higher plants for the flight period of the Mars <span class="hlt">mission</span> are analyzed. It is proposed constructing a BLSS with a closed-loop material cycle for gas and water and for part of human waste. A higher-plant-based BLSS with the mass exchange loop closed to various degrees is proposed for a Mars planetary base. Various versions of BLSS configuration and degree of closure of mass exchange are considered, depending on the duration of the Mars <span class="hlt">mission</span>, the diet of the crew, and some other conditions. Special consideration is given to problems of reliability and sustainability of material cycling in BLSS, which are related to production of additional oxygen inside the system. Technologies of constructing BLSS of various configurations are proposed and substantiated. Reasons are given for using physicochemical methods in BLSS as secondary tools both during the flight and the stay on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030064056','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030064056"><span>Mathematical Modeling of Food Supply for Long Term Space <span class="hlt">Missions</span> Using Advanced <span class="hlt">Life</span> Support</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cruthirds, John E.</p> <p>2003-01-01</p> <p>A habitat for long duration <span class="hlt">missions</span> which utilizes Advanced <span class="hlt">Life</span> Support (ALS), the Bioregenerative Planetary <span class="hlt">Life</span> Support Systems Test Complex (BIO-Plex), is currently being built at JSC. In this system all consumables will be recycled and reused. In support of this effort, a menu is being planned utilizing ALS crops that will meet nutritional and psychological requirements. The need exists in the food system to identify specific physical quantities that define <span class="hlt">life</span> support systems from an analysis and modeling perspective. Once these quantities are defined, they need to be fed into a mathematical model that takes into consideration other systems in the BIO-Plex. This model, if successful, will be used to understand the impacts of changes in the food system on the other systems and vice versa. The Equivalent System Mass (ESM) metric has been used to describe systems and subsystems, including the food system options, in terms of the single parameter, mass. There is concern that this approach might not adequately address the important issues of food quality and psychological impact on crew morale of a supply of fiesh food items. In fact, the mass of food can also depend on the quality of the food. This summer faculty fellow project will involve creating an appropriate mathematical model for the food plan developed by the Food Processing System for BIO-Plex. The desired outcome of this work will be a quantitative model that can be applied to the various options of supplying food on long-term space <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140012851','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140012851"><span>The Influence of Free Space Environment in the <span class="hlt">Mission</span> <span class="hlt">Life</span> Cycle: Material Selection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Edwards, David L.; Burns, Howard D.; de Groh, Kim K.</p> <p>2014-01-01</p> <p>The natural space environment has a great influence on the ability of space systems to perform according to <span class="hlt">mission</span> design specification. Understanding the natural space environment and its influence on space system performance is critical to the concept formulation, design, development, and operation of space systems. Compatibility with the natural space environment is a primary factor in determining the functional lifetime of the space system. Space systems being designed and developed today are growing in complexity. In many instances, the increased complexity also increases its sensitivity to space environmental effects. Sensitivities to the natural space environment can be tempered through appropriate design measures, material selection, ground processing, mitigation strategies, and/or the acceptance of known risks. The design engineer must understand the effects of the natural space environment on the space system and its components. This paper will discuss the influence of the natural space environment in the <span class="hlt">mission</span> <span class="hlt">life</span> cycle with a specific focus on the role of material selection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=S90-45229&hterms=raft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Draft','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=S90-45229&hterms=raft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Draft"><span>STS-37 <span class="hlt">Mission</span> Specialist (MS) Godwin floating in <span class="hlt">life</span> raft in JSC WETF pool</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1990-01-01</p> <p>STS-37 <span class="hlt">Mission</span> Specialist (MS) Linda M. Godwin, wearing launch and entry suit (LES) and launch and entry helmet (LEH), floats in a one-person <span class="hlt">life</span> raft during a training session in JSC's Weightless Environment Training Facility (WETF) Bldg 29 pool. She was simulating steps involved in emergency egress from a Space Shuttle. The WETF's 25-ft deep pool served as a simulated ocean into which a parachute landing might be made.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890040430&hterms=How+long+can+earth+support+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DHow%2Blong%2Bcan%2Bearth%2Bsupport%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890040430&hterms=How+long+can+earth+support+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DHow%2Blong%2Bcan%2Bearth%2Bsupport%2Blife"><span>Lunar and Mars <span class="hlt">missions</span> - Challenges for advanced <span class="hlt">life</span> support</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Duke, Michael B.</p> <p>1988-01-01</p> <p>The development of a suite of scenarios is a prerequisite to the studies that will enable an informed decision by the United States on a program to meet the recently announced space policy goal to expand human presence beyond earth orbit. NASA's Office of Exploration is currently studying a range of initiative options that would extend the sphere of human activity in space to Mars and include permanent bases or outposts on the moon and on Mars. This paper describes the evolutionary lunar base and the Mars expedition scenarios in some detail so that an evaluation can be made from the point of view of human support and opportunities. Alternative approaches in the development of lunar outposts are outlined along with Mars expeditionary scenarios. Human environmental issues are discussed, including: closed loop <span class="hlt">life</span> support systems; EVA systems; mobility systems; and medical support, physiological deconditioning, and psychological effects associated with long-duration <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....2504V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....2504V"><span>ESA's new <span class="hlt">mission</span> to search for signs of <span class="hlt">life</span> on Mars: ExoMars and its Pasteur scientific payload</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vago, J. L.; Gardini, B.; Kminek, G.; Exomars Study Team</p> <p>2003-04-01</p> <p>ESA has recently completed a study for an exobiology <span class="hlt">mission</span> to be launched in 2009. Its scientific objective is to search for signs of past and present <span class="hlt">life</span> on Mars. <span class="hlt">Life</span> as we know it relies, above all else, upon water. However, the present low ambient temperature and pressure conditions preclude the widespread existence of water on the Martian surface; except, maybe, in very localised environments, and then only episodically. Still, water/ice may lie at some depth underground. Additionally, because of the sterilizing/degrading effect of the Martian UV radiation spectrum, the search for <span class="hlt">life</span> indicators, whether for present or for extinct <span class="hlt">life</span>, should best be conducted below the surface. ESA's <span class="hlt">mission</span> will consist of two main elements: a dedicated communications satellite, and a 200-kg rover. The rover will carry the Pasteur scientific payload. The Pasteur Model Payload used for the study is equipped with a multispectral, stereoscopic camera; an electromagnetic subsurface sounder to identify water/ice deposits; a drill capable of reaching a depth of 2 m, and also of collecting specimens from within surface rocks; a sample preparation unit, an optical microscope; an oxidation sensor; and a variety of spectroscopic instruments. For the characterisation of organic substances, Pasteur also houses a gas chromatographer/mass spectrometer, and a novel device based on protein assay chip technology. Latitudinal bands between 10 and 45 deg, both N and S can be targeted for landing. Over its envisioned lifetime of 180 sols, the rover is designed to cover 30-50 km of ground track over typical Martian terrain. Operations beyond this period will depend on the amount of dust deposited on the rover's solar panels. This paper summarises the present ExoMars concept. Particular attention is devoted to <span class="hlt">mission</span>-imposed constraints having an influence on the science output: i.e. for instrument selection and operations, power generation, and landing sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000053505','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000053505"><span><span class="hlt">Mission</span> to the Solar System: Exploration and Discovery. A <span class="hlt">Mission</span> and Technology Roadmap</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gulkis, S. (Editor); Stetson, D. S. (Editor); Stofan, E. R. (Editor)</p> <p>1998-01-01</p> <p>Solar System exploration addresses some of humanity's most fundamental questions: How and when did <span class="hlt">life</span> form on Earth? Does <span class="hlt">life</span> exist elsewhere in the Solar System or in the Universe? - How did the Solar System form and evolve in time? - What can the other planets teach us about the Earth? This document describes a <span class="hlt">Mission</span> and Technology Roadmap for addressing these and other fundamental Solar System Questions. A Roadmap Development Team of scientists, engineers, educators, and technologists worked to define the next evolutionary steps in in situ exploration, sample return, and completion of the overall Solar System survey. Guidelines were to "develop aa visionary, but affordable, <span class="hlt">mission</span> and technology development Roadmap for the exploration of the Solar System in the 2000 to 2012 timeframe." The Roadmap provides a catalog of potential flight <span class="hlt">missions</span>. (Supporting research and technology, ground-based observations, and laboratory research, which are no less important than flight <span class="hlt">missions</span>, are not included in this Roadmap.)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C13E0658F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C13E0658F"><span>Under-Ice Operations with AUVS in High Latitudes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferguson, J.; Kaminski, C. D.</p> <p>2012-12-01</p> <p>In 2010 and 2011, ISE Explorer Autonomous Underwater Vehicles (AUV), built for Natural Resources Canada (NRCan), were deployed to Canada's high Arctic. The <span class="hlt">mission</span> was to undertake under-ice bathymetric surveys supporting Canada's submission under the United Nations Convention on the Law of the Sea (UNCLOS). During these deployments several under-ice records were broken and several new technologies were demonstrated. The NRCan AUV is a 5000 meter depth rated vehicle, with several innovative additions to make it suitable for arctic survey work. Most notable are a depth rated variable ballast system, a 1300 Hz long-range homing system, and under-ice charging and data transfer capabilities. The Explorer's range was extended to approximately 450 km by adding a hull section to accommodate extra batteries. The scientific payload onboard included a Seabird SBE49 Conductivity-Temperature-Depth (CTD) sensor, Knudsen singlebeam echosounder, and a Kongsberg Simrad EM2000 multibeam echosounder. In 2010, operations were conducted from an ice camp near Borden Island (78°14'N, 112°39'W) operating through an ice hole. Following several test <span class="hlt">missions</span>, the AUV spent 10 days surveying under ice before being successfully recovered. In total, close to 1100 km of under-ice survey was undertaken at depths to 3160 meters. A further set of operations was carried out in August and September 2011 from the Canadian <span class="hlt">Icebreaker</span> CCGS Louis St. Laurent operating with the American <span class="hlt">Icebreaker</span> USCGS Healy. Here the operations were much further north to latitudes of 88°30' N and to depths of 3500 meters. In this paper, the 2010 ice camp and the 2011 <span class="hlt">icebreaker</span> <span class="hlt">missions</span> are described, with an outline of technology developments that were undertaken, the preparations that were necessary for the success of the <span class="hlt">missions</span> and finally, the outcome of the <span class="hlt">missions</span> themselves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170009116','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170009116"><span>The Impact of <span class="hlt">Mission</span> Duration on a Mars Orbital <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Arney, Dale; Earle, Kevin; Cirillo, Bill; Jones, Christopher; Klovstad, Jordan; Grande, Melanie; Stromgren, Chel</p> <p>2017-01-01</p> <p>Performance alone is insufficient to assess the total impact of changing <span class="hlt">mission</span> parameters on a space <span class="hlt">mission</span> concept, architecture, or campaign; the benefit, cost, and risk must also be understood. This paper examines the impact to benefit, cost, and risk of changing the total <span class="hlt">mission</span> duration of a human Mars orbital <span class="hlt">mission</span>. The changes in the sizing of the crew habitat, including consumables and spares, was assessed as a function of duration, including trades of different <span class="hlt">life</span> support strategies; this was used to assess the impact on transportation system requirements. The impact to benefit is minimal, while the impact on cost is dominated by the increases in transportation costs to achieve shorter total durations. The risk is expected to be reduced by decreasing total <span class="hlt">mission</span> duration; however, large uncertainty exists around the magnitude of that reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050174596','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050174596"><span>Using Near Real-Time <span class="hlt">Mission</span> Data for Education and Public Outreach: Strategies from the <span class="hlt">Life</span> in the Atacama E/PO Effort</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Myers, E.; Coppin, P.; Wagner, M.; Fischer, K.; Lu, L.; McCloskey, R.; Seneker, D.; Cabrol, N.; Wettergreen, D.; Waggoner, A.</p> <p>2005-01-01</p> <p>The EventScope educational telepresence project has been involved with education and public outreach for a number of NASA-sponsored <span class="hlt">missions</span> including the Mars Exploration Rovers, the Odyssey <span class="hlt">Mission</span>, and the <span class="hlt">Life</span> in the Atacama project. However, during the second year of operations in the Atacama, a modified version of the EventScope public interface was used as the remote science operations interface. In addition, the EventScope lab hosted remote science operations. This intimate connection with the <span class="hlt">mission</span> operations allowed the EventScope team to bring the experience of the <span class="hlt">mission</span> to the public in near real-time. Playing to this strength, the lab developed strategies for releasing E/PO content as close to real-time as possible.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790008538','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790008538"><span>A critical review of the <span class="hlt">life</span> sciences project management at Ames Research Center for the Spacelab <span class="hlt">Mission</span> development test 3</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Helmreich, R. L.; Wilhelm, J. M.; Tanner, T. A.; Sieber, J. E.; Burgenbauch, S. F.</p> <p>1979-01-01</p> <p>A management study was initiated by ARC (Ames Research Center) to specify Spacelab <span class="hlt">Mission</span> Development Test 3 activities and problems. This report documents the problems encountered and provides conclusions and recommendations to project management for current and future ARC <span class="hlt">life</span> sciences projects. An executive summary of the conclusions and recommendations is provided. The report also addresses broader issues relevant to the conduct of future scientific <span class="hlt">missions</span> under the constraints imposed by the space environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860034825&hterms=craft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dcraft','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860034825&hterms=craft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dcraft"><span>The First Spacelab <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Craft, H.</p> <p>1984-01-01</p> <p>The role of the <span class="hlt">mission</span> manager in coordinating the payload with the space transportation system is studied. The establishment of the investigators working group to assist in achieving the <span class="hlt">mission</span> objectives is examined. Analysis of the scientific requirements to assure compatibility with available resources, and analysis of the payload in order to define orbital flight requirements are described. The training of payload specialists, launch site integration, and defining the requirements for the operation of the integrated payload and the payload operations control center are functions of the <span class="hlt">mission</span> manager. The experiences gained from the management of the Spacelab One <span class="hlt">Mission</span>, which can be implemented in future <span class="hlt">missions</span>, are discussed. Examples of material processing, earth observations, and <span class="hlt">life</span> sciences advances from the First Spacelab <span class="hlt">Mission</span> are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920014115','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920014115"><span>SLS-PLAN-IT: A knowledge-based blackboard scheduling system for Spacelab <span class="hlt">life</span> sciences <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kao, Cheng-Yan; Lee, Seok-Hua</p> <p>1992-01-01</p> <p>The primary scheduling tool in use during the Spacelab <span class="hlt">Life</span> Science (SLS-1) planning phase was the operations research (OR) based, tabular form Experiment Scheduling System (ESS) developed by NASA Marshall. PLAN-IT is an artificial intelligence based interactive graphic timeline editor for ESS developed by JPL. The PLAN-IT software was enhanced for use in the scheduling of Spacelab experiments to support the SLS <span class="hlt">missions</span>. The enhanced software SLS-PLAN-IT System was used to support the real-time reactive scheduling task during the SLS-1 <span class="hlt">mission</span>. SLS-PLAN-IT is a frame-based blackboard scheduling shell which, from scheduling input, creates resource-requiring event duration objects and resource-usage duration objects. The blackboard structure is to keep track of the effects of event duration objects on the resource usage objects. Various scheduling heuristics are coded in procedural form and can be invoked any time at the user's request. The system architecture is described along with what has been learned with the SLS-PLAN-IT project.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015IJAsB..14..511W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015IJAsB..14..511W"><span>On the abundance of extraterrestrial <span class="hlt">life</span> after the Kepler <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wandel, Amri</p> <p>2015-07-01</p> <p>The data recently accumulated by the Kepler <span class="hlt">mission</span> have demonstrated that small planets are quite common and that a significant fraction of all stars may have an Earth-like planet within their habitable zone. These results are combined with a Drake-equation formalism to derive the space density of biotic planets as a function of the relatively modest uncertainty in the astronomical data and of the (yet unknown) probability for the evolution of biotic <span class="hlt">life</span>, F b. I suggest that F b may be estimated by future spectral observations of exoplanet biomarkers. If F b is in the range 0.001-1, then a biotic planet may be expected within 10-100 light years from Earth. Extending the biotic results to advanced <span class="hlt">life</span> I derive expressions for the distance to putative civilizations in terms of two additional Drake parameters - the probability for evolution of a civilization, F c, and its average longevity. For instance, assuming optimistic probability values (F b~F c~1) and a broadcasting longevity of a few thousand years, the likely distance to the nearest civilizations detectable by searching for intelligent electromagnetic signals is of the order of a few thousand light years. The probability of detecting intelligent signals with present and future radio telescopes is calculated as a function of the Drake parameters. Finally, I describe how the detection of intelligent signals would constrain the Drake parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11987306','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11987306"><span>Human factor observations of the Biosphere 2, 1991-1993, closed <span class="hlt">life</span> support human experiment and its application to a long-term manned <span class="hlt">mission</span> to Mars.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Alling, Abigail; Nelson, Mark; Silverstone, Sally; Van Thillo, Mark</p> <p>2002-01-01</p> <p>Human factors are a key component to the success of long-term space <span class="hlt">missions</span> such as those necessitated by the human exploration of Mars and the development of bioregenerative and eventually self-sufficient <span class="hlt">life</span> support systems for permanent space outposts. Observations by participants living inside the 1991-1993 Biosphere 2 closed system experiment provide the following insights. (1) Crew members should be involved in the design and construction of their <span class="hlt">life</span> support systems to gain maximum knowledge about the systems. (2) Individuals living in closed <span class="hlt">life</span> support systems should expect a process of physiological and psychological adaptation to their new environment. (3) Far from simply being a workplace, the participants in such extended <span class="hlt">missions</span> will discover the importance of creating a cohesive and satisfying <span class="hlt">life</span> style. (4) The crew will be dependent on the use of varied crops to create satisfying cuisine, a social <span class="hlt">life</span> with sufficient outlets of expression such as art and music, and to have down-time from purely task-driven work. (5) The success of the Biosphere 2 first 2-year <span class="hlt">mission</span> suggests that crews with high cultural diversity, high commitment to task, and work democracy principles for individual responsibility may increase the probability of both <span class="hlt">mission</span> success and personal satisfaction. (6) Remaining challenges are many, including the need for far more comprehensive real-time modeling and information systems (a "cybersphere") operating to provide real-time data necessary for decision-making in a complex <span class="hlt">life</span> support system. (7) And, the aim will be to create a noosphere, or sphere of intelligence, where the people and their living systems are in sustainable balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=S96-08073&hterms=raft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Draft','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=S96-08073&hterms=raft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Draft"><span>Astronaut Daniel W. Bursch, <span class="hlt">mission</span> specialist, uses his helmet to bail out water from his <span class="hlt">life</span> raft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1996-01-01</p> <p>STS-77 TRAINING VIEW --- Astronaut Daniel W. Bursch, <span class="hlt">mission</span> specialist, uses his helmet to bail out water from his <span class="hlt">life</span> raft during emergency bailout training for crew members in the Johnson Space Centers (JSC) Weightless Environment Training Facility (WET-F). Bursch will join five other astronauts for nine days aboard the Space Shuttle Endeavour next month.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14696589','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14696589"><span>HUMEX, a study on the survivability and adaptation of humans to long-duration exploratory <span class="hlt">missions</span>, part I: lunar <span class="hlt">missions</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Horneck, G; Facius, R; Reichert, M; Rettberg, P; Seboldt, W; Manzey, D; Comet, B; Maillet, A; Preiss, H; Schauer, L; Dussap, C G; Poughon, L; Belyavin, A; Reitz, G; Baumstark-Khan, C; Gerzer, R</p> <p>2003-01-01</p> <p>The European Space Agency has recently initiated a study of the human responses, limits and needs with regard to the stress environments of interplanetary and planetary <span class="hlt">missions</span>. Emphasis has been laid on human health and performance care as well as advanced <span class="hlt">life</span> support developments including bioregenerative <span class="hlt">life</span> support systems and environmental monitoring. The overall study goals were as follows: (i) to define reference scenarios for a European participation in human exploration and to estimate their influence on the <span class="hlt">life</span> sciences and <span class="hlt">life</span> support requirements; (ii) for selected <span class="hlt">mission</span> scenarios, to critically assess the limiting factors for human health, wellbeing, and performance and to recommend relevant countermeasures; (iii) for selected <span class="hlt">mission</span> scenarios, to critically assess the potential of advanced <span class="hlt">life</span> support developments and to propose a European strategy including terrestrial applications; (iv) to critically assess the feasibility of existing facilities and technologies on ground and in space as testbeds in preparation for human exploratory <span class="hlt">missions</span> and to develop a test plan for ground and space campaigns; (v) to develop a roadmap for a future European strategy towards human exploratory <span class="hlt">missions</span>, including preparatory activities and terrestrial applications and benefits. This paper covers the part of the HUMEX study dealing with lunar <span class="hlt">missions</span>. A lunar base at the south pole where long-time sunlight and potential water ice deposits could be assumed was selected as the Moon reference scenario. The impact on human health, performance and well being has been investigated from the view point of the effects of microgravity (during space travel), reduced gravity (on the Moon) and abrupt gravity changes (during launch and landing), of the effects of cosmic radiation including solar particle events, of psychological issues as well as general health care. Countermeasures as well as necessary research using ground-based test beds and/or the International</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040092942&hterms=Elsevier&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DElsevier','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040092942&hterms=Elsevier&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DElsevier"><span>HUMEX, a study on the survivability and adaptation of humans to long-duration exploratory <span class="hlt">missions</span>, part I: lunar <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Horneck, G.; Facius, R.; Reichert, M.; Rettberg, P.; Seboldt, W.; Manzey, D.; Comet, B.; Maillet, A.; Preiss, H.; Schauer, L.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20040092942'); toggleEditAbsImage('author_20040092942_show'); toggleEditAbsImage('author_20040092942_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20040092942_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20040092942_hide"></p> <p>2003-01-01</p> <p>The European Space Agency has recently initiated a study of the human responses, limits and needs with regard to the stress environments of interplanetary and planetary <span class="hlt">missions</span>. Emphasis has been laid on human health and performance care as well as advanced <span class="hlt">life</span> support developments including bioregenerative <span class="hlt">life</span> support systems and environmental monitoring. The overall study goals were as follows: (i) to define reference scenarios for a European participation in human exploration and to estimate their influence on the <span class="hlt">life</span> sciences and <span class="hlt">life</span> support requirements; (ii) for selected <span class="hlt">mission</span> scenarios, to critically assess the limiting factors for human health, wellbeing, and performance and to recommend relevant countermeasures; (iii) for selected <span class="hlt">mission</span> scenarios, to critically assess the potential of advanced <span class="hlt">life</span> support developments and to propose a European strategy including terrestrial applications; (iv) to critically assess the feasibility of existing facilities and technologies on ground and in space as testbeds in preparation for human exploratory <span class="hlt">missions</span> and to develop a test plan for ground and space campaigns; (v) to develop a roadmap for a future European strategy towards human exploratory <span class="hlt">missions</span>, including preparatory activities and terrestrial applications and benefits. This paper covers the part of the HUMEX study dealing with lunar <span class="hlt">missions</span>. A lunar base at the south pole where long-time sunlight and potential water ice deposits could be assumed was selected as the Moon reference scenario. The impact on human health, performance and well being has been investigated from the view point of the effects of microgravity (during space travel), reduced gravity (on the Moon) and abrupt gravity changes (during launch and landing), of the effects of cosmic radiation including solar particle events, of psychological issues as well as general health care. Countermeasures as well as necessary research using ground-based test beds and/or the International</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1983AdSpR...3..143C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1983AdSpR...3..143C"><span>The first dedicated <span class="hlt">life</span> sciences <span class="hlt">mission</span> - Spacelab 4</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cramer, D. R.; Reid, D. H.; Klein, H. P.</p> <p></p> <p>Spacelab is a large versatile laboratory carried in the bay of the Shuttle Orbiter. The first Spacelab <span class="hlt">mission</span> dedicated entirely to <span class="hlt">Life</span> Sciences is known as Spacelab 4. It is scheduled for launch in late 1985 and will remain aloft for seven days. This payload consists of 25 tentatively selected investigations combined into a comprehensive integrated exploration of the effects of acute weightlessness on living systems. An emphasis is placed on studying physiological changes that have been previously observed in manned space flight. This payload has complementary designs in the human and animal investigations in order to validate animal models of human physiology in weightlessness. The experimental subjects include humans, squirrel monkeys, laboratory rats, several species of plants, and frog eggs. The primary scientific objectives include study of the acute cephalic fluid shift, cardiovascular adaptation to weightlessness, including postflight reductions in orthostatic tolerance and exercise capacity, and changes in vestibular function, including space motion sickness, associated with weightlessness. Secondary scientific objectives include the study of red cell mass reduction, negative nitrogen balance, altered calcium metabolism, suppressed in vitro lymphocyte reactivity, gravitropism and photropism in plants, and fertilization and early development in frog eggs. The rationale behind this payload, the selection process, and details of the individual investigations are presented in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089885&hterms=policy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dpolicy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089885&hterms=policy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dpolicy"><span>Refinement of planetary protection policy for Mars <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>DeVincenzi, D. L.; Stabekis, P.; Barengoltz, J.</p> <p>1996-01-01</p> <p>Under existing COSPAR policy adopted in 1984, <span class="hlt">missions</span> to Mars (landers, probes, and some orbiters) are designated as Category IV <span class="hlt">missions</span>. As such, the procedures for implementing planetary protection requirements could include trajectory biasing, cleanrooms, bioload reduction, sterilization of hardware, and bioshields. In 1992, a U.S. National Research Council study recommended that controls on forward contamination of Mars be tied to specific <span class="hlt">mission</span> objectives. The report recommended that Mars landers with <span class="hlt">life</span> detection instruments be subject to at least Viking-level sterilization procedures for bioload reduction, while spacecraft (including orbiters) without <span class="hlt">life</span> detection instruments be subject to at least Viking-level pre-sterilization procedures for bioload reduction but need not be sterilized. In light of this, it is proposed that the current policy's Category IV and its planetary protection requirements be divided into two sub-categories as follows: Category IVa, for <span class="hlt">missions</span> comprising landers and probes without <span class="hlt">life</span> detection experiments, which will meet a specified bioburden limit for exposed surfaces, and Category IVb, for landers and probes with <span class="hlt">life</span> detection experiments, which will require sterilization of landed systems. In addition, Category III orbiter <span class="hlt">mission</span> specifications are expanded to be consistent with these recommendations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010062154&hterms=science+policy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dscience%2Bpolicy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010062154&hterms=science+policy&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dscience%2Bpolicy"><span>Revision to Planetary Protection Policy for Mars <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>DeVincenzi, D. L.; Stabekis, P.; Barengoltz, J.; Morrison, David (Technical Monitor)</p> <p>1994-01-01</p> <p>Under existing COSPAR policy adopted in 1984, <span class="hlt">missions</span> to Mars (landers, probes, and some orbiters) are designated as Category IV <span class="hlt">missions</span>. As such, the procedures for implementing planetary protection requirements could include trajectory biasing, cleanrooms, bioload reduction, sterilization of hardware, and bioshields, i. e. requirements could be similar to Viking. However, in 1992, a U. S. National Academy of Sciences study recommended that controls on forward contamination of Mars be tied to specific <span class="hlt">mission</span> objectives. The report recommended that Mars landers with <span class="hlt">life</span> detection instruments be subject to at least Viking-level sterilization procedures for bioload reduction, while spacecraft (including orbiters) without <span class="hlt">life</span> detection instruments be subject to at least Viking-level pre sterilization procedures for bioload reduction but need not be sterilized. In light of this, it is proposed that the current policy's Category IV <span class="hlt">missions</span> and their planetary protection requirements be divided into two subcategories as follows: Category IV A, for <span class="hlt">missions</span> comprising landers and probes without <span class="hlt">life</span> detection experiments and some orbiters, which will meet a specified bioburden limit for exposed surfaces; Category IV B, for landers and probes with <span class="hlt">life</span> detection experiments, which will require complete system sterilization. For Category IV A <span class="hlt">missions</span>, bioburden specifications will be proposed and implementing procedures discussed. A resolution will be proposed to modify the existing COSPAR policy to reflect these changes. Similar specifications, procedures, and resolution for Category IV B <span class="hlt">missions</span> will be the subject of a later study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040014959&hterms=accounting+system&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Daccounting%2Bsystem','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040014959&hterms=accounting+system&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Daccounting%2Bsystem"><span>The Effect of <span class="hlt">Mission</span> Location on <span class="hlt">Mission</span> Costs and Equivalent System Mass</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fisher, John W.; Levri, Julie</p> <p>2002-01-01</p> <p>It is the goal of developers of advanced <span class="hlt">life</span> support researcher to develop technology that reduces the cost of <span class="hlt">life</span> support for future space <span class="hlt">missions</span> and thereby enables <span class="hlt">missions</span> that are currently infeasible or too expensive. Because the cost of propulsion dominates the cost of hardware emplacement in space and because the mass of a deliverable object controls its propulsive requirements, equivalent system mass (ESM) is used as a means for accounting for <span class="hlt">mission</span> costs. ESM is typically calculated by adding to the actual mass the equivalent amount of mass that must be added to a <span class="hlt">mission</span> due to other characteristics of a piece of hardware such as the item s volume or energy requirements. This approach works well for comparing different pieces of hardware when they go to the same location in space. However, different locations in <span class="hlt">mission</span> space such low Earth orbit, Mars surface, or full trip to Mars and return to low Earth orbit require vastly different amounts of propulsion. Moving an object from Earth surface to the Martian surface and returning it to Earth will require as much as 100 times the propulsion that is required to move the object to low Earth orbit only. This paper presents the case for including the effect that location can have on cost as a part of ESM and suggests a method for achieving this improvement of ESM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-9308442&hterms=veterinary&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dveterinary','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-9308442&hterms=veterinary&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dveterinary"><span>STS-58 <span class="hlt">Mission</span> Insignia</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1993-01-01</p> <p>Designed by members of the flight crew, the STS-58 insignia depicts the Space Shuttle Columbia with a Spacelab module in its payload bay in orbit around Earth. The Spacelab and the lettering Spacelab <span class="hlt">Life</span> Sciences ll highlight the primary <span class="hlt">mission</span> of the second Space Shuttle flight dedicated to <span class="hlt">life</span> sciences research. An Extended Duration Orbiter (EDO) support pallet is shown in the aft payload bay, stressing the scheduled two-week duration of the longest Space Shuttle <span class="hlt">mission</span> to date. The hexagonal shape of the patch depicts the carbon ring, a molecule common to all living organisms. Encircling the inner border of the patch is the double helix of DNA, representing the genetic basis of <span class="hlt">life</span>. Its yellow background represents the sun, energy source for all <span class="hlt">life</span> on Earth. Both medical and veterinary caducei are shown to represent the STS- 58 <span class="hlt">life</span> sciences experiments. The position of the spacecraft in orbit about Earth with the United States in the background symbolizes the ongoing support of the American people for scientific research intended to benefit all mankind.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012epsc.conf..501B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012epsc.conf..501B"><span>When the Viking <span class="hlt">Missions</span> Discovered <span class="hlt">Life</span> on the Red Planet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bianciardi, G.; Miller, J. D.; Straat, P. A.; Levin, G. V.</p> <p>2012-09-01</p> <p>The first (and only) dedicated <span class="hlt">life</span> detection experiments on another planet were performed by the Viking Landers of 1976. In the Viking Labeled Release (LR) experiment of Levin and Straat, injections of organic compounds into Martian soil samples caused radioactive gas to evolve approaching plateaus of 10,000 - 15,000 cpm over several sols (Martian days). These "actives" were run at lander sites 1 and 2 with similar results. In contrast, the LR response to the 160o C control sample soils was very low. In conjunction with the active experiment results this negative result from the controls satisfied the pre-<span class="hlt">mission</span> criteria for <span class="hlt">life</span>. However, a controversy immediately arose concerning a biologic interpretation of the data. In an attempt to resolve this issue in the current work, we have employed complexity analysis of the Viking LR data for the initial six sols, and of terrestrial LR pilot studies using bacteria-laden, active soil (Biol 5) and sterilized soil (Biol 6). . Measures of mathematical complexity permitted a deep analysis of signal structure. Martian LR active response data were strongly superimposable upon the terrestrial biological time series, forming a welldefined cluster; and the heat-treated control samples, terrestrial and Martian, also clustered together, but distant from the active group, suggesting that the LR had, indeed, detected biological activity on Mars. The results presente herein are a key subset of the details published earlier by the same authors (IJASS, 13 (1), 14-26, 2012).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080012584&hterms=human+resources+support&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dhuman%2Bresources%2Bsupport','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080012584&hterms=human+resources+support&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dhuman%2Bresources%2Bsupport"><span>Lunar Outpost <span class="hlt">Life</span> Support Trade Studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lange, Kevin E.; Anderson, Molly S.; Ewert, Michael K.; Barta, Daniel J.</p> <p>2008-01-01</p> <p>Engineering trade-off studies of <span class="hlt">life</span> support system architecture and technology options were conducted for potential lunar surface <span class="hlt">mission</span> scenarios within NASA's Constellation Program. The scenarios investigated are based largely on results of the NASA Lunar Architecture Team (LAT) Phase II study. In particular, the possibility of Hosted Sortie <span class="hlt">missions</span>, the high cost of power during eclipse periods, and the potential to reduce <span class="hlt">life</span> support consumables through scavenging, in-situ resources, and alternative EVA technologies were all examined. These trade studies were performed within the Systems Integration, Modeling and Analysis (SIMA) element of NASA's Exploration <span class="hlt">Life</span> Support (ELS) technology development project. The tools and methodology used in the study are described briefly, followed by a discussion of <span class="hlt">mission</span> scenarios, <span class="hlt">life</span> support technology options and results presented in terms of equivalent system mass for various regenerative <span class="hlt">life</span> support technologies and architectures. Three classes of repeated or extended lunar surface <span class="hlt">missions</span> were investigated in this study along with several <span class="hlt">life</span> support resource scenarios for each <span class="hlt">mission</span> class. Individual <span class="hlt">mission</span> durations of 14 days, 90 days and 180 days were considered with 10 <span class="hlt">missions</span> assumed for each at a rate of 2 <span class="hlt">missions</span> per year. The 14-day <span class="hlt">missions</span> represent a class of Hosted Sortie <span class="hlt">missions</span> where a pre-deployed and potentially mobile habitat provides <span class="hlt">life</span> support for multiple crews at one or more locations. The 90-day and 180-day <span class="hlt">missions</span> represent lunar outpost expeditions with a larger fixed habitat. The 180-day <span class="hlt">missions</span> assume continuous human presence and must provide <span class="hlt">life</span> support through eclipse periods of up to 122 hours while the 90-day <span class="hlt">missions</span> are planned for best-case periods of nearly continuous sunlight. This paper investigates system optimization within the assumptions of each scenario and addresses how the scenario selected drives the <span class="hlt">life</span> support system to different designs</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950011191','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950011191"><span>Re-engineering the <span class="hlt">mission</span> <span class="hlt">life</span> cycle with ABC and IDEF</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mandl, Daniel; Rackley, Michael; Karlin, Jay</p> <p>1994-01-01</p> <p>The theory behind re-engineering a business process is to remove the non-value added activities thereby lowering the process cost. In order to achieve this, one must be able to identify where the non-value added elements are located which is not a trivial task. This is because the non-value added elements are often hidden in the form of overhead and/or pooled resources. In order to be able to isolate these non-value added processes from among the other processes, one must first decompose the overall top level process into lower layers of sub-processes. In addition, costing data must be assigned to each sub-process along with the value the sub-process adds towards the final product. IDEF0 is a Federal Information Processing Standard (FIPS) process-modeling tool that allows for this functional decomposition through structured analysis. In addition, it illustrates the relationship of the process and the value added to the product or service. The value added portion is further defined in IDEF1X which is an entity relationship diagramming tool. The entity relationship model is the blueprint of the product as it moves along the 'assembly line' and therefore relates all of the parts to each other and the final product. It also relates the parts to the tools that produce the product and all of the paper work that is used in their acquisition. The use of IDEF therefore facilitates the use of Activity Based Costing (ABC). ABC is an essential method in a high variety, product-customizing environment, to facilitate rapid response to externally caused change. This paper describes the work being done in the <span class="hlt">Mission</span> Operations Division to re-engineer the development and operation <span class="hlt">life</span> cycle of <span class="hlt">Mission</span> Operations Centers using these tools.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780013230','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780013230"><span>An interstellar precursor <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jaffe, L. D.; Ivie, C.; Lewis, J. C.; Lipes, R. G.; Norton, H. N.; Stearns, J. W.; Stimpson, L.; Weissman, P.</p> <p>1977-01-01</p> <p>A <span class="hlt">mission</span> out of the planetary system, with launch about the year 2000, could provide valuable scientific data as well as test some of the technology for a later <span class="hlt">mission</span> to another star. Primary scientific objectives for the precursor <span class="hlt">mission</span> concern characteristics of the heliopause, the interstellar medium, stellar distances (by parallax measurements), low energy cosmic rays, interplanetary gas distribution, and mass of the solar system. Secondary objectives include investigation of Pluto. Candidate science instruments are suggested. Individual spacecraft systems for the <span class="hlt">mission</span> were considered, technology requirements and problem areas noted, and a number of recommendations made for technology study and advanced development. The most critical technology needs include attainment of 50-yr spacecraft lifetime and development of a long-<span class="hlt">life</span> NEP system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AIPC.1637..555L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AIPC.1637..555L"><span>A close examination of under-actuated attitude control subsystem design for future satellite <span class="hlt">missions</span>' <span class="hlt">life</span> extension</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lam, Quang M.; Barkana, Itzhak</p> <p>2014-12-01</p> <p>Satellite <span class="hlt">mission</span> <span class="hlt">life</span>, maintained and prolonged beyond its typical norm of their expectancy, are primarily dictated by the state of health of its Reaction Wheel Assembly (RWA), especially for commercial GEO satellites since torquer bars are no longer applicable while thruster assistant is unacceptable due to pointing accuracy impact during jet firing. The RWA is the primary set of actuators (as compared to thrusters for orbit maintenance and maneuvering) mainly responsible for the satellite <span class="hlt">mission</span> for accurately and precisely pointing its payloads to the right targets to conduct its <span class="hlt">mission</span> operations. The RWA consisting of either a set of four in pyramid or three in orthogonal is the primary set of actuators to allow the satellite to achieve accurate and precise pointing of the satellite payloads towards the desired targets. Future space <span class="hlt">missions</span> will be required to achieve much longer lives and are currently perceived by the GEO satellite community as an "expected norm" of 20 years or longer. Driven by customers' demands/goals and competitive market have challenged Attitude Control Subsystems (ACS) engineers to develop better ACS algorithms to address such an emerging need. There are two main directions to design satellite's under-actuated control subsystem: (1) Attitude Feedback with Zero Momentum Principle and (2) Attitude Control by Angular Velocity Tracking via Small Time Local Controllability concept. Successful applications of these control laws have been largely demonstrated via simulation for the rest to rest case. Limited accuracy and oscillatory behaviors are observed in three axes for non-zero wheel momentum while realistic loss of a wheel scenario (i.e., fully actuated to under-actuated) has not been closely examined! This study revisits the under-actuated control design with detailed set ups of multiple scenarios reflecting real <span class="hlt">life</span> operating conditions which have put current under-actuated control laws mentioned earlier into a re-evaluation mode</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA263030','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA263030"><span>Shelf-<span class="hlt">Life</span> Specifications for <span class="hlt">Mission</span> Readiness</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1993-03-01</p> <p>R applies to this item. Arthur D Little t.𔃻.., 4-48 NSN: 7930009353794 Name: Polish , Plastic Description: White lotion with a slight odor Intended...<span class="hlt">MISSION</span> READINESS TC•T I AR16 19931 Abstract The Navy disposes of tons of hazardous material as hazardous waste due to the expiration of excessively...of hazardous material as hazardous waste due to the expiration of excessively conservati’e shielf-Ihfe terms. In order to reduce this occurrence, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950022454','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950022454"><span>The influence of space flight on erythrokinetics in man. Space <span class="hlt">Life</span> Sciences <span class="hlt">Missions</span> 1 and 2. Experiment E261</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Alfrey, Clarence P.</p> <p>1995-01-01</p> <p>The purpose of this contract was to design and conduct experiments that would increase our understanding of the influence of space flight on erythrokinetics and the rapid change that occurs in the red blood cell mass during spaceflight. The experiment designated E261, was flown on Space <span class="hlt">Life</span> Science <span class="hlt">missions</span> SLS-1 and SLS-2 (STS 40 and STS 58). Unique features of this experiment included radionuclide tracer studies during flight and frequent in-flight blood samples specifically for the first three or four days of the <span class="hlt">mission</span>. Plasma volume measurements were made early and late in the <span class="hlt">missions</span>. Radioactive iron kinetics studies were initiated after one or three days in microgravity since the magnitude of the red blood cell mass decrease dictated that bone marrow production must be decreased very early in the flight. The schedule was designed to study the time course of the changes that occur during spaceflight and to possibly define a mechanism for the rapid reduction in red blood cell mass.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0290&hterms=Evolution+flies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DEvolution%2Bflies','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0290&hterms=Evolution+flies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DEvolution%2Bflies"><span>An experiment to fly on <span class="hlt">mission</span> STS-93 is prepared at <span class="hlt">Life</span> Sciences Building, CCAS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1999-01-01</p> <p>In the KSC <span class="hlt">Life</span> Sciences Building, Hangar L, Cape Canaveral Air Station, Mark Rupert, with BioServe Space Technologies, checks the canisters, or incubators, that will hold an experiment to fly on <span class="hlt">mission</span> STS-93. The incubators will hold a mix of fruit fly embryos and larvae to examine the effects of microgravity and space flight on the development of neural connections between specific motor neurons and their targets in muscle fibers. The incubators are part of a Commercial Generic Bioprocessing Apparatus (CGBA), which can start bioprocessing reactions by mixing or heating a sample and can also initiate multiple-step, sequential reactions in a technique called phased processing. The primary payload of <span class="hlt">mission</span> STS-93 is the Chandra X-ray Observatory, which will allow scientists from around the world to see previously invisible black holes and high-temperature gas clouds, giving the observatory the potential to rewrite the books on the structure and evolution of our universe. The target launch date for STS-93 is July 9, aboard Space Shuttle Columbia, from Launch Pad 39B.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0291&hterms=Evolution+flies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DEvolution%2Bflies','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0291&hterms=Evolution+flies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DEvolution%2Bflies"><span>An experiment to fly on <span class="hlt">mission</span> STS-93 is prepared at <span class="hlt">Life</span> Sciences Building, CCAS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1999-01-01</p> <p>In the KSC <span class="hlt">Life</span> Sciences Building, Hangar L, Cape Canaveral Air Station, Jake Freeman and Mark Rupert, with BioServe Space Technologies, check canisters, or incubators, that will hold fruit fly embryos and larvae for an experiment to fly on <span class="hlt">mission</span> STS-93. The experiment will examine the effects of microgravity and space flight on the development of neural connections between specific motor neurons and their targets in muscle fibers. The incubators are part of the Commercial Generic Bioprocessing Apparatus (CGBA), which can start bioprocessing reactions by mixing or heating a sample and can also initiate multiple-step, sequential reactions in a technique called phased processing. The primary payload of <span class="hlt">mission</span> STS-93 is the Chandra X-ray Observatory, which will allow scientists from around the world to see previously invisible black holes and high-temperature gas clouds, giving the observatory the potential to rewrite the books on the structure and evolution of our universe. The target launch date for STS-93 is July 9, aboard Space Shuttle Columbia, from Launch Pad 39B.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830031262&hterms=inverter+lifetime&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dinverter%2Blifetime','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830031262&hterms=inverter+lifetime&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dinverter%2Blifetime"><span>Results of the <span class="hlt">mission</span> profile <span class="hlt">life</span> test. [for J-series mercury ion engines</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bechtel, R. T.; Trump, G. E.; James, E. L.</p> <p>1982-01-01</p> <p>Seven J series 30-cm diameter thrusters have been tested in segments of up to 5,070 hr, for 14,541 hr in the <span class="hlt">Mission</span> Profile <span class="hlt">Life</span> Test facility. Test results have indicated the basic thruster design to be consistent with the lifetime goal of 15,000 hr at 2-A beam. The only areas of concern identified which appear to require additional verification testing involve contamination of mercury propellant isolators, which may be due to facility constituents, and the ability of specially covered surfaces to contain sputtered material and prevent flake formation. The ability of the SCR, series resonant inverter power processor to operate the J series thruster and autonomous computer control of the thruster/processor system were demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/486164','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/486164"><span>The Europa Ocean Discovery <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Edwards, B.C.; Chyba, C.F.; Abshire, J.B.</p> <p>1997-06-01</p> <p>Since it was first proposed that tidal heating of Europa by Jupiter might lead to liquid water oceans below Europa`s ice cover, there has been speculation over the possible exobiological implications of such an ocean. Liquid water is the essential ingredient for <span class="hlt">life</span> as it is known, and the existence of a second water ocean in the Solar System would be of paramount importance for seeking the origin and existence of <span class="hlt">life</span> beyond Earth. The authors present here a Discovery-class <span class="hlt">mission</span> concept (Europa Ocean Discovery) to determine the existence of a liquid water ocean on Europa and to characterize Europa`smore » surface structure. The technical goal of the Europa Ocean Discovery <span class="hlt">mission</span> is to study Europa with an orbiting spacecraft. This goal is challenging but entirely feasible within the Discovery envelope. There are four key challenges: entering Europan orbit, generating power, surviving long enough in the radiation environment to return valuable science, and complete the <span class="hlt">mission</span> within the Discovery program`s launch vehicle and budget constraints. The authors will present here a viable <span class="hlt">mission</span> that meets these challenges.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27492296','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27492296"><span>[Exploring the Experience of Dysmenorrhea and <span class="hlt">Life</span> Adjustments of Women Undergoing Traditional Chinese Medicine Treatment].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tsai, Min-Min; Yang, Fu-Chi; Lee, Shih-Min; Huang, Chiu-Mieh</p> <p>2016-08-01</p> <p>Previous studies of women with dysmenorrhea have focused on menstrual attitudes, the characteristics of menstrual pain, and self-care behavior. Traditional Chinese Medicine (TCM) studies on dysmenorrhea, on the other hand, have focused on the efficacy and safety of TCM treatments. Few studies have investigated how women perceive their own TCM-treatment experience of dysmenorrhea. The objective of this study was to explore the experience of dysmenorrhea and <span class="hlt">life</span> adjustments of women undergoing TCM treatment. A semi-structured interviewing guide was used to collect data. A total of 40 dysmenorrheal women participated in the study. Individual, in-depth interviews were conducted for about 60-90 minutes with each participant. Their speech tone, facial expressions, and gestures during the interview process were also observed and recorded. The findings were analyzed using content analysis via ATLAS. ti 5.2 software. The process that the participants used to adjust to dysmenorrhea were distinguished into four progressive stages: "tip of the iceberg", "<span class="hlt">ice-breaking</span>", "tug-of-war", and "blending-in". Initially, the participants perceived the symptoms of dysmenorrhea as the "tip of the iceberg". They attempted to hide / ignore the initial pain until the problem gradually worsened to the point that the symptoms began to significantly affect various aspects of <span class="hlt">life</span>. It was only then that the participants began to pay attention to the problem and to seek help from TCM practitioners, which we defined as the "<span class="hlt">ice-breaking</span>" stage. If they encountered unexpected situations with regard to the treatment regimen, the participants entered the "tug-of-war" stage, during which they struggled over whether to continue with TCM treatments. Afterward, the participants gradually achieved a "blending-in" of new ideas, which allowed them to identify the strategies that best facilitated adjustment and rebalancing. Eventually, the participants achieved a new <span class="hlt">life</span> balance. The outcomes of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060039478&hterms=pluto&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dpluto','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060039478&hterms=pluto&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dpluto"><span>(abstract) Follow-on <span class="hlt">Missions</span> for the Pluto Spacecraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Weinstein, Stacy; Salvo, Chris; Stern, Alan</p> <p>1994-01-01</p> <p>The Pluto Fast Flyby <span class="hlt">mission</span> development baseline consists of 2 identical spacecraft (120 - 165 kg) to be launched to Pluto/Charon in the late 1990s. These spacecraft are intended to fly by Pluto and Charon in order to perform various remote-sensing scientific investigations and have a <span class="hlt">mission</span> development cost less than $400M (FY92$) through launch plus 30 days. The long-<span class="hlt">life</span> (6 - 10 years) <span class="hlt">mission</span> duration and lightweight design make the Pluto spacecraft a good candidate for a number of other flyby <span class="hlt">missions</span> to objects in the outer Solar System, and some of these were investigated by JPL in cooperation with NASA Code SL's (Solar System Exploration) Outer Planets Science Working Group (OPSWG) in 1993. The JPL team looked at what it would mean to fly one of these <span class="hlt">missions</span> (if a third spacecraft were available) in terms of flight time, spacecraft modifications, and science payload resources; the OPSWG recommended science investigation modifications for the different targets based on the available resources. The <span class="hlt">missions</span> could, in many cases, utilize less capable launch vehicles, thereby reducing <span class="hlt">life</span>-cycle cost of the <span class="hlt">mission</span>. Examples of the sort of targets which were investigated and looked attractive in terms of flight time are: Uranus, Neptune, Uranus/Neptune dual-<span class="hlt">mission</span>, Trojan asteroids (624 Hektor, 617 Patroclus, others), 5145 Pholus (the reddest object known in the solar system), and Kuiper Belt objects (i.e., 1992 QB1) . This paper will present the results of this investigation in terms of potential science return, performance, and the potential for <span class="hlt">life</span>-cycle cost reductions through inheritance from Pluto Fast Flyby .</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120011664','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120011664"><span>Next Generation <span class="hlt">Life</span> Support Project: Development of Advanced Technologies for Human Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barta, Daniel J.</p> <p>2012-01-01</p> <p>Next Generation <span class="hlt">Life</span> Support (NGLS) is one of several technology development projects sponsored by the National Aeronautics and Space Administration s Game Changing Development Program. NGLS is developing <span class="hlt">life</span> support technologies (including water recovery, and space suit <span class="hlt">life</span> support technologies) needed for humans to live and work productively in space. NGLS has three project tasks: Variable Oxygen Regulator (VOR), Rapid Cycle Amine (RCA) swing bed, and Alternative Water Processing. The selected technologies within each of these areas are focused on increasing affordability, reliability, and vehicle self sufficiency while decreasing mass and enabling long duration exploration. The RCA and VOR tasks are directed at key technology needs for the Portable <span class="hlt">Life</span> Support System (PLSS) for an Exploration Extravehicular Mobility Unit (EMU), with focus on prototyping and integrated testing. The focus of the Rapid Cycle Amine (RCA) swing-bed ventilation task is to provide integrated carbon dioxide removal and humidity control that can be regenerated in real time during an EVA. The Variable Oxygen Regulator technology will significantly increase the number of pressure settings available to the space suit. Current spacesuit pressure regulators are limited to only two settings while the adjustability of the advanced regulator will be nearly continuous. The Alternative Water Processor efforts will result in the development of a system capable of recycling wastewater from sources expected in future exploration <span class="hlt">missions</span>, including hygiene and laundry water, based on natural biological processes and membrane-based post treatment. The technologies will support a capability-driven architecture for extending human presence beyond low Earth orbit to potential destinations such as the Moon, near Earth asteroids and Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1985AdSpR...5..147R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1985AdSpR...5..147R"><span>Orbit determination for ISRO satellite <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rao, Ch. Sreehari; Sinha, S. K.</p> <p></p> <p>Indian Space Research Organisation (ISRO) has been successful in using the in-house developed orbit determination and prediction software for satellite <span class="hlt">missions</span> of Bhaskara, Rohini and APPLE. Considering the requirements of satellite <span class="hlt">missions</span>, software packages are developed, tested and their accuracies are assessed. Orbit determination packages developed are SOIP, for low earth orbits of Bhaskara and Rohini <span class="hlt">missions</span>, ORIGIN and ODPM, for orbits related to all phases of geo-stationary <span class="hlt">missions</span> and SEGNIP, for drift and geo-stationary orbits. Software is tested and qualified using tracking data of SIGNE-3, D5-B, OTS, SYMPHONIE satellites with the help of software available with CNES, ESA and DFVLR. The results match well with those available from these agencies. These packages have supported orbit determination successfully throughout the <span class="hlt">mission</span> <span class="hlt">life</span> for all ISRO satellite <span class="hlt">missions</span>. Member-Secretary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11538980','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11538980"><span>Planetary protection program for Mars 94/96 <span class="hlt">mission</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rogovski, G; Bogomolov, V; Ivanov, M; Runavot, J; Debus, A; Victorov, A; Darbord, J C</p> <p>1996-01-01</p> <p>Mars surface in-situ exploration started in 1975 with the American VIKING <span class="hlt">mission</span>. Two probes landed on the northern hemisphere and provided, for the first time, detailed information on the martian terrain, atmosphere and meteorology. The current goal is to undertake larger surface investigations and many projects are being planned by the major Space Agencies with this objective. Among these projects, the Mars 94/96 <span class="hlt">mission</span> will make a major contributor toward generating significant information about the martian surface on a large scale. Since the beginning of the Solar System exploration, planets where <span class="hlt">life</span> could exist have been subject to planetary protection requirements. Those requirements accord with the COSPAR Policy and have two main goals: the protection of the planetary environment from influence or contamination by terrestrial microorganisms, the protection of <span class="hlt">life</span> science, and particularly of <span class="hlt">life</span> detection experiments searching extra-terrestrial <span class="hlt">life</span>, and not <span class="hlt">life</span> carried by probes and spacecrafts. As the conditions for <span class="hlt">life</span> and survival for terrestrial microorganisms in the Mars environment became known, COSPAR recommendations were updated. This paper will describe the decontamination requirements which will be applied for the MARS 94/96 <span class="hlt">mission</span>, the techniques and the procedures which are and will be used to realize and control the decontamination of probes and spacecrafts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820011414','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820011414"><span>OAO-3 end of <span class="hlt">mission</span> tests report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kalil, F.; Kull, F. J.; Mcintosh, R.; Ollendorf, S.; Margolies, D. L.; Gemmell, J.; Tasevoli, C. M.; Polidan, R. S.; Kochevar, H.; Chapman, C.</p> <p>1981-01-01</p> <p>Twelve engineering type tests were performed on several subsystems and experiment(s) of the OAO 3 spacecraft near its end of <span class="hlt">mission</span>. The systems tested include: Princeton experiment package (PEP), fine error system guidance, inertial reference unit, star trackers, heat pipes, thermal control coatings, command and data handling, solar array; batteries, and onboard processor/power boost regulator. Generally, the systems performed well for the 8 1/2 years <span class="hlt">life</span> of OAO 3, although some degradation was noted in the sensitivity of PEP and in the absorptivity of the skin coatings. Battery <span class="hlt">life</span> was prolonged during the <span class="hlt">life</span> of the <span class="hlt">mission</span> in large part by carefully monitoring the charge-discharge cycle with careful attention not to overcharge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003IAUSS...4E..26C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003IAUSS...4E..26C"><span>Attracting Students to Space Science Fields: <span class="hlt">Mission</span> to Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Congdon, Donald R.; Lovegrove, William P.; Samec, Ronald G.</p> <p></p> <p>Attracting high school students to space science is one of the main goals of Bob Jones University's annual <span class="hlt">Mission</span> to Mars (MTM). MTM develops interest in space exploration through a highly realistic simulated trip to Mars. Students study and learn to appreciate the challenges of space travel including propulsion <span class="hlt">life</span> support medicine planetary astronomy psychology robotics and communication. Broken into teams (Management Spacecraft Design Communications <span class="hlt">Life</span> Support Navigation Robotics and Science) they address the problems specific to each aspect of the <span class="hlt">mission</span>. Teams also learn to interact and recognize that a successful <span class="hlt">mission</span> requires cooperation. Coordinated by the Management Team the students build a spacecraft and associated apparatus connect computers and communications equipment train astronauts on the <span class="hlt">mission</span> simulator and program a Pathfinder-type robot. On the big day the astronauts enter the spacecraft as <span class="hlt">Mission</span> Control gets ready to support them through the expected and unexpected of their <span class="hlt">mission</span>. Aided by teamwork the astronauts must land on Mars perform their scientific <span class="hlt">mission</span> on a simulated surface of mars and return home. We see the success of MTM not only in successful <span class="hlt">missions</span> but in the students who come back year after year for another MTM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013237','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013237"><span>Ames Coronagraph Experiment: Enabling <span class="hlt">Missions</span> to Directly Image Exoplanets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Belikov, Ruslan</p> <p>2014-01-01</p> <p>Technology to find biomarkers and <span class="hlt">life</span> on other worlds is rapidly maturing. If there is a habitable planet around the nearest star, we may be able to detect it this decade with a small satellite <span class="hlt">mission</span>. In the 2030 decade, we will likely know if there is <span class="hlt">life</span> in our Galactic neighborhood (1000 nearest stars). The Ames Coronagraph Experiment is developing coronagraphic technologies to enable such <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040015097&hterms=ALS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DALS','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040015097&hterms=ALS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DALS"><span>The Effect of <span class="hlt">Mission</span> Location on <span class="hlt">Mission</span> Costs and Equivalent System Mass</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fisher, John W.; Levri, Julie A.; Jones, Harry W.</p> <p>2003-01-01</p> <p>Equivalent System Mass (ESM) is used by the Advanced <span class="hlt">Life</span> Support (ALS) community to quantify <span class="hlt">mission</span> costs of technologies for space applications (Drysdale et al, 1999, Levri et al, 2000). Mass is used as a cost measure because the mass of an object determines propulsion (acceleration) cost (i.e. amount of fuel needed), and costs relating to propulsion dominate <span class="hlt">mission</span> cost. <span class="hlt">Mission</span> location drives <span class="hlt">mission</span> cost because acceleration is typically required to initiate and complete a change in location. Total <span class="hlt">mission</span> costs may be reduced by minimizing the mass of materials that must be propelled to each distinct location. In order to minimize fuel requirements for <span class="hlt">missions</span> beyond low-Earth orbit (LEO), the hardware and astronauts may not all go to the same location. For example, on a Lunar or Mars <span class="hlt">mission</span>, some of the hardware or astronauts may stay in orbit while the rest of the hardware and astronauts descend to the planetary surface. In addition, there may be disposal of waste or used hardware at various <span class="hlt">mission</span> locations to avoid propulsion of mass that is no longer needed in the <span class="hlt">mission</span>. This paper demonstrates how using location factors in the calculation of ESM can account for the effects of various acceleration events and can improve the accuracy and value of the ESM metric to <span class="hlt">mission</span> planners. Even a <span class="hlt">mission</span> with one location can benefit from location factor analysis if the alternative technologies under consideration consume resources at different rates. For example, a <span class="hlt">mission</span> that regenerates resources will have a relatively constant mass compared to one that uses consumables and vents/discards mass along the way. This paper shows examples of how location factors can affect ESM calculations and how the inclusion of location factors can change the relative value of technologies being considered for development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160009303','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160009303"><span>Radiation Hardness Assurance (RHA) for Small <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Campola, Michael J.</p> <p>2016-01-01</p> <p>Varied <span class="hlt">mission</span> <span class="hlt">life</span> and complexity is growing for small spacecraft. Small <span class="hlt">missions</span> benefit from detailed hazard definition and evaluation as done in the past. Requirements need to flow from the system down to the parts level and aid system level radiation tolerance. RHA is highlighted with increasing COTS usage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=apollo&pg=4&id=EJ494031','ERIC'); return false;" href="https://eric.ed.gov/?q=apollo&pg=4&id=EJ494031"><span>Bonus: Apollo's Amazing <span class="hlt">Mission</span> and Spin-Offs from Space.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Learning, 1994</p> <p>1994-01-01</p> <p>Two posters examine the 1969 Apollo moon <span class="hlt">mission</span>. The first tracks the stages and path of the <span class="hlt">mission</span>, suggesting that students create their own diagrams or models. The second presents a puzzle that helps student understand how many items developed for the <span class="hlt">mission</span> are useful to today's everyday <span class="hlt">life</span>. (SM)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720021182','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720021182"><span>Apollo 15 <span class="hlt">Mission</span> Report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1971-01-01</p> <p>A detailed discussion is presented of the Apollo 15 <span class="hlt">mission</span>, which conducted exploration of the moon over longer periods, greater ranges, and with more instruments of scientific data acquisition than previous <span class="hlt">missions</span>. The topics include trajectory, lunar surface science, inflight science and photography, command and service module performance, lunar module performance, lunar surface operational equipment, pilot's report, biomedical evaluation, <span class="hlt">mission</span> support performance, assessment of <span class="hlt">mission</span> objectives, launch phase summary, anomaly summary, and vehicle and equipment descriptions. The capability of transporting larger payloads and extending time on the moon were demonstrated. The ground-controlled TV camera allowed greater real-time participation by earth-bound personnel. The crew operated more as scientists and relied more on ground support team for systems monitoring. The modified pressure garment and portable <span class="hlt">life</span> support system provided better mobility and extended EVA time. The lunar roving vehicle and the lunar communications relay unit were also demonstrated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910025385&hterms=reimburs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dreimburs*','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910025385&hterms=reimburs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dreimburs*"><span>The Spacelab J <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cremin, J. W.; Leslie, F. W.</p> <p>1990-01-01</p> <p>This paper describes Spacelab J (SL-J), its <span class="hlt">mission</span> characteristics, features, parameters and configuration, the unique nature of the shared reimbursable cooperative effort with the National Space Development Agency (NASDA) of Japan and the evolution, content and objectives of the <span class="hlt">mission</span> scientific experiment complement. The <span class="hlt">mission</span> is planned for launch in 1991. This long module <span class="hlt">mission</span> has 35 experiments from Japan as well as 9 investigations from the United States. The SL-J payload consists of two broad scientific disciplines which require the extended microgravity or cosmic ray environment: (1) materials science such as crystal growth, solidification processes, drop dynamics, free surface flows, gas dynamics, metallurgy and semiconductor technology; and (2) <span class="hlt">life</span> science including cell development, human physiology, radiation-induced mutations, vestibular studies, embryo development, and medical technology. Through an international agreement with NASDA, NASA is preparing to fly the first Japanese manned, scientific, cooperative endeavor with the United States.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150003005','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150003005"><span>Logistics Needs for Potential Deep Space <span class="hlt">Mission</span> Scenarios Post Asteroid Redirect Crewed <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lopez, Pedro, Jr.; Shultz, Eric; Mattfeld, Bryan; Stromgren, Chel; Goodliff, Kandyce</p> <p>2015-01-01</p> <p>The Asteroid Redirect <span class="hlt">Mission</span> (ARM) is currently being explored as the next step towards deep space human exploration, with the ultimate goal of reaching Mars. NASA is currently investigating a number of potential human exploration <span class="hlt">missions</span>, which will progressively increase the distance and duration that humans spend away from Earth. <span class="hlt">Missions</span> include extended human exploration in cis-lunar space which, as conceived, would involve durations of around 60 days, and human <span class="hlt">missions</span> to Mars, which are anticipated to be as long as 1000 days. The amount of logistics required to keep the crew alive and healthy for these <span class="hlt">missions</span> is significant. It is therefore important that the design and planning for these <span class="hlt">missions</span> include accurate estimates of logistics requirements. This paper provides a description of a process and calculations used to estimate mass and volume requirements for crew logistics, including consumables, such as food, personal items, gasses, and liquids. Determination of logistics requirements is based on crew size, <span class="hlt">mission</span> duration, and the degree of closure of the environmental control <span class="hlt">life</span> support system (ECLSS). Details are provided on the consumption rates for different types of logistics and how those rates were established. Results for potential <span class="hlt">mission</span> scenarios are presented, including a breakdown of mass and volume drivers. Opportunities for mass and volume reduction are identified, along with potential threats that could possibly increase requirements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0293&hterms=Evolution+flies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DEvolution%2Bflies','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0293&hterms=Evolution+flies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DEvolution%2Bflies"><span>An experiment to fly on <span class="hlt">mission</span> STS-93 is prepared at <span class="hlt">Life</span> Sciences Building, CCAS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1999-01-01</p> <p>In the KSC <span class="hlt">Life</span> Sciences Building, Hangar L, Cape Canaveral Air Station, Shawn Bengtson, with Lockheed Martin, checks population cages containing fruit flies. The larvae of the flies are part of an experiment that is a secondary payload on <span class="hlt">mission</span> STS-93. The experiment will examine the effects of microgravity and space flight on the development of neural connections between specific motor neurons and their targets in muscle fibers. That information could lead to understanding the effect of microgravity on human nervous system connectivity. The larvae will be contained in incubators that are part of a Commercial Generic Bioprocessing Apparatus (CGBA), which can start bioprocessing reactions by mixing or heating a sample and can also initiate multiple-step, sequential reactions in a technique called phased processing. The primary payload of <span class="hlt">mission</span> STS-93 is the Chandra X-ray Observatory, which will allow scientists from around the world to see previously invisible black holes and high-temperature gas clouds, giving the observatory the potential to rewrite the books on the structure and evolution of our universe. The target launch date for STS-93 is July 9, aboard Space Shuttle Columbia, from Launch Pad 39B.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0292&hterms=Science+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DScience%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=KSC-99PP-0292&hterms=Science+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DScience%2Blife"><span>An experiment to fly on <span class="hlt">mission</span> STS-93 is prepared at <span class="hlt">Life</span> Sciences Building, CCAS</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1999-01-01</p> <p>In the KSC <span class="hlt">Life</span> Sciences Building, Hangar L, Cape Canaveral Air Station, Dr. Haig Keshishian checks fruit fly larvae in a petri dish. The larvae are part of an experiment that is a secondary payload on <span class="hlt">mission</span> STS-93. The experiment will examine the effects of microgravity and space flight on the development of neural connections between specific motor neurons and their targets in muscle fibers. Dr. Keshishian, from Yale University, is the principle investigator for the experiment. The larvae will be contained in incubators that are part of a Commercial Generic Bioprocessing Apparatus (CGBA), which can start bioprocessing reactions by mixing or heating a sample and can also initiate multiple-step, sequential reactions in a technique called phased processing. The primary payload of <span class="hlt">mission</span> STS-93 is the Chandra X-ray Observatory, which will allow scientists from around the world to see previously invisible black holes and high- temperature gas clouds, giving the observatory the potential to rewrite the books on the structure and evolution of our universe. The target launch date for STS-93 is July 9, aboard Space Shuttle Columbia, from Launch Pad 39B.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012IJAsB..11..269E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012IJAsB..11..269E"><span>Raman spectroscopy and the search for <span class="hlt">life</span> signatures in the ExoMars <span class="hlt">Mission</span>*</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, Howell G. M.; Hutchinson, Ian B.; Ingley, Richard</p> <p>2012-10-01</p> <p>The survival strategies of extremophilic organisms in terrestrially stressed locations and habitats are critically dependent on the production of protective chemicals in response to desiccation, low wavelength radiation insolation, temperature and the availability of nutrients. The adaptation of <span class="hlt">life</span> to these harsh prevailing conditions involves the control of the substratal geology; the interaction between the rock and the organisms is critical and the biological modification of the geological matrix plays a very significant role in the overall survival strategy. Identification of these biological and biogeological chemical molecular signatures in the geological record is necessary for the recognition of the presence of extinct or extant <span class="hlt">life</span> in terrestrial and extraterrestrial scenarios. Raman spectroscopic techniques have been identified as valuable instrumentation for the detection of <span class="hlt">life</span> extra-terrestrially because of the use of non-invasive laser-based excitation of organic and inorganic molecules, and molecular ions with high discrimination characteristics; the interactions effected between biological organisms and their environments are detectable through the molecular entities produced at the interfaces, for which the vibrational spectroscopic band signatures are unique. A very important attribute of Raman spectroscopy is the acquisition of molecular experimental data non-destructively without the need for chemical or mechanical pre-treatment of the specimen; this has been a major factor in the proposal for the adoption of Raman instrumentation on robotic landers and rovers for planetary exploration, particularly for the forthcoming European Space Agency (ESA)/National Aeronautics and Space Administration (NASA) ExoMars <span class="hlt">mission</span>. In this paper, the merits of using Raman spectroscopy for the recognition of key molecular biosignatures from several terrestrial extremophile specimens will be illustrated. The data and specimens used in this presentation have</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993paal.work...13H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993paal.work...13H"><span>Planetary protection implementation on future Mars lander <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Howell, Robert; Devincenzi, Donald L.</p> <p>1993-06-01</p> <p>A workshop was convened to discuss the subject of planetary protection implementation for Mars lander <span class="hlt">missions</span>. It was sponsored and organized by the Exobiology Implementation Team of the U.S./Russian Joint Working Group on Space Biomedical and <span class="hlt">Life</span> Support Systems. The objective of the workshop was to discuss planetary protection issues for the Russian Mars '94 <span class="hlt">mission</span>, which is currently under development, as well as for additional future Mars lander <span class="hlt">missions</span> including the planned Mars '96 and U.S. MESUR Pathfinder and Network <span class="hlt">missions</span>. A series of invited presentations was made to ensure that workshop participants had access to information relevant to the planned discussions. The topics summarized in this report include exobiology science objectives for Mars exploration, current international policy on planetary protection, planetary protection requirements developed for earlier <span class="hlt">missions</span>, <span class="hlt">mission</span> plans and designs for future U.S. and Russian Mars landers, biological contamination of spacecraft components, and techniques for spacecraft bioload reduction. In addition, the recent recommendations of the U.S. Space Studies Board (SSB) on this subject were also summarized. Much of the discussion focused on the recommendations of the SSB. The SSB proposed relaxing the planetary protection requirements for those Mars lander <span class="hlt">missions</span> that do not contain <span class="hlt">life</span> detection experiments, but maintaining Viking-like requirements for those <span class="hlt">missions</span> that do contain <span class="hlt">life</span> detection experiments. The SSB recommendations were found to be acceptable as a guide for future <span class="hlt">missions</span>, although many questions and concerns about interpretation were raised and are summarized. Significant among the concerns was the need for more quantitative guidelines to prevent misinterpretation by project offices and better access to and use of the Viking data base of bio-assays to specify microbial burden targets. Among the questions raised were how will the SSB recommendations be integrated with existing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940008710','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940008710"><span>Planetary protection implementation on future Mars lander <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Howell, Robert; Devincenzi, Donald L.</p> <p>1993-01-01</p> <p>A workshop was convened to discuss the subject of planetary protection implementation for Mars lander <span class="hlt">missions</span>. It was sponsored and organized by the Exobiology Implementation Team of the U.S./Russian Joint Working Group on Space Biomedical and <span class="hlt">Life</span> Support Systems. The objective of the workshop was to discuss planetary protection issues for the Russian Mars '94 <span class="hlt">mission</span>, which is currently under development, as well as for additional future Mars lander <span class="hlt">missions</span> including the planned Mars '96 and U.S. MESUR Pathfinder and Network <span class="hlt">missions</span>. A series of invited presentations was made to ensure that workshop participants had access to information relevant to the planned discussions. The topics summarized in this report include exobiology science objectives for Mars exploration, current international policy on planetary protection, planetary protection requirements developed for earlier <span class="hlt">missions</span>, <span class="hlt">mission</span> plans and designs for future U.S. and Russian Mars landers, biological contamination of spacecraft components, and techniques for spacecraft bioload reduction. In addition, the recent recommendations of the U.S. Space Studies Board (SSB) on this subject were also summarized. Much of the discussion focused on the recommendations of the SSB. The SSB proposed relaxing the planetary protection requirements for those Mars lander <span class="hlt">missions</span> that do not contain <span class="hlt">life</span> detection experiments, but maintaining Viking-like requirements for those <span class="hlt">missions</span> that do contain <span class="hlt">life</span> detection experiments. The SSB recommendations were found to be acceptable as a guide for future <span class="hlt">missions</span>, although many questions and concerns about interpretation were raised and are summarized. Significant among the concerns was the need for more quantitative guidelines to prevent misinterpretation by project offices and better access to and use of the Viking data base of bioassays to specify microbial burden targets. Among the questions raised were how will the SSB recommendations be integrated with existing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E2092Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E2092Y"><span>Initial Sample Analyses inside a Capsule: A Strategy of <span class="hlt">Life</span> Detection and Planetary Protection for Ocean World Sample Return <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yano, Hajime; Takano, Yoshinori; Sekine, Yasuhito; Takai, Ken; Funase, Ryu; Fujishima, Kosuke; Shibuya, Takazo</p> <p>2016-07-01</p> <p>Planetary protection is considered to be one of the most crucial challenges to enable sample return <span class="hlt">missions</span> from "Ocean Worlds", internal oceans of icy satellites as potential deep habitat such as Enceladus and Europa, due to the risk of backward contamination of bringing back potential biology-related matters or at most, possible extraterrestrial living signatures to the Earth. Here we propose an innovative technological solution for both <span class="hlt">life</span> detection and planetary protection of such returned samples, namely by conducting all major <span class="hlt">life</span> signature searches, which are also a critical path of quarantine processes of planetary protection, inside the Earth return capsule, prior to open the canister and expose to the terrestrial environment. We plan to test the latest sample capture and recovery methods of preparing multiple aliquot chambers in the sample return capsule. Each aliquot chamber will trap, for instance, plume particles and ambient volatiles during the spacecraft flying through Enceladus plumes so that respective analyses can be performed focusing on volatiles and minerals (i.e., habitability for <span class="hlt">life</span>), organics (i.e., ingredients for <span class="hlt">life</span>), biosignatures (i.e., activity of <span class="hlt">life</span>) and for archiving the samples for future investigations at the same time. In-situ analysis will be conducted under complete containment through an optical interface port that allows pre-installed fiber optic cables to perform non-contact measurements and capillary tubing for extraction/injection of gas and liquids through metal barriers to be punctuated inside a controlled environment. Once primary investigations are completed, the interior of the capsule will be sterilized by gamma rays and UV irradiation. Post-sterilized aliquot chambers will be further analyzed under enclosed and ultraclean environment at BAL 2-3 facilities, rather than BSL4. We consider that this is an unique solution that can cope with severe requirements set for the Category-V sample returns for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998PhDT........50E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998PhDT........50E"><span>The masking of beluga whale (Delphinapterus leucas) vocalizations by <span class="hlt">icebreaker</span> noise</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Erbe, Christine</p> <p>1998-11-01</p> <p>This thesis examines the masking effect of underwater noise on beluga whale communication. As ocean water is greatly opaque for light but well conducting for sound, marine mammals rely primarily on their hearing for orientation and communication. Man-made underwater noise has the potential of interfering with sounds used by marine mammals. Masking to the point of incomprehensibility can have fatal results-for the individual, but ultimately for the entire species. As part of our understanding of whether marine mammals can cope with human impact on nature, this thesis is the first to study the interference of real ocean noises with complex animal vocalizations. At the Vancouver Aquarium, a beluga whale was trained for acoustic experiments, during which masked hearing thresholds were measured. Focus lay on noise created by <span class="hlt">icebreaking</span> ships in the Arctic. As experiments with trained animals are time and cost expensive, various techniques were examined for their ability to model the whale's response. These were human hearing tests, visual spectrogram discrimination, matched filtering, spectrogram cross-correlation, critical band cross-correlation, adaptive filtering and various types of artificial neural networks. The most efficient method with respect to similarity to the whale's data and speed, was a backpropagation neural net. Masked hearing thresholds would be of little use if they could not be related to accessible quantities in the wild. An ocean sound propagation model was applied to determine critical distances between a noise source, a calling whale and a listening whale. Colour diagrams, called maskograms, were invented to illustrate zones of masking in the wild. Results are that bubbler system noise with a source level of 194 dB re 1 μPa at 1 m has a maximum radius of masking of 15 km in a 3- dimensional ocean. Propeller noise with a source level of 203 dB re 1 μPa at 1 m has a maximum radius of masking of 22 km. A naturally occurring icecracking event</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140008285','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140008285"><span>Asteroid Crew Segment <span class="hlt">Mission</span> Lean Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gard, Joseph; McDonald, Mark</p> <p>2014-01-01</p> <p>Asteroid Retrieval Crewed <span class="hlt">Mission</span> (ARCM) requires a minimum set of Key Capabilities compared in the context of the baseline EM-1/2 Orion and SLS capabilities. These include: <span class="hlt">Life</span> Support & Human Systems Capabilities; <span class="hlt">Mission</span> Kit Capabilities; Minimizing the impact to the Orion and SLS development schedules and funding. Leveraging existing technology development efforts to develop the kits adds functionality to Orion while minimizing cost and mass impact.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910025530&hterms=life+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlife%2Bscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910025530&hterms=life+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlife%2Bscience"><span><span class="hlt">Life</span> sciences and Mars exploration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sulzman, Frank M.; Rummel, John D.; Leveton, Lauren B.; Teeter, Ron</p> <p>1990-01-01</p> <p>The major <span class="hlt">life</span> science considerations for Mars exploration <span class="hlt">missions</span> are discussed. Radiation protection and countermeasures for zero gravity are discussed. Considerations of crew psychological health considerations and <span class="hlt">life</span> support systems are addressed. Scientific opportunities presented by manned Mars <span class="hlt">missions</span> are examined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770010734','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770010734"><span>Space shuttle and <span class="hlt">life</span> sciences</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mason, J. A.</p> <p>1977-01-01</p> <p>During the 1980's, some 200 Spacelab <span class="hlt">missions</span> will be flown on space shuttle in earth-orbit. Within these 200 <span class="hlt">missions</span>, it is planned that at least 20 will be dedicated to <span class="hlt">life</span> sciences research, projects which are yet to be outlined by the <span class="hlt">life</span> sciences community. Objectives of the <span class="hlt">Life</span> Sciences Shuttle/Spacelab Payloads Program are presented. Also discussed are major space <span class="hlt">life</span> sciences programs including space medicine and physiology, clinical medicine, <span class="hlt">life</span> support technology, and a variety of space biology topics. The shuttle, spacelab, and other <span class="hlt">life</span> sciences payload carriers are described. Concepts for carry-on experiment packages, mini-labs, shared and dedicated spacelabs, as well as common operational research equipment (CORE) are reviewed. Current NASA planning and development includes Spacelab <span class="hlt">Mission</span> Simulations, an Announcement of Planning Opportunity for <span class="hlt">Life</span> Sciences, and a forthcoming Announcement of Opportunity for Flight Experiments which will together assist in forging a <span class="hlt">Life</span> Science Program in space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20130009125&hterms=Engineering+courses&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DEngineering%2Bcourses','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20130009125&hterms=Engineering+courses&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DEngineering%2Bcourses"><span>Re-Engineering the <span class="hlt">Mission</span> Operations System (MOS) for the Prime and Extended <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hunt, Joseph C., Jr.; Cheng, Leo Y.</p> <p>2012-01-01</p> <p>One of the most challenging tasks in a space science <span class="hlt">mission</span> is designing the <span class="hlt">Mission</span> Operations System (MOS). Whereas the focus of the project is getting the spacecraft built and tested for launch, the <span class="hlt">mission</span> operations engineers must build a system to carry out the science objectives. The completed MOS design is then formally assessed in the many reviews. Once a <span class="hlt">mission</span> has completed the reviews, the <span class="hlt">Mission</span> Operation System (MOS) design has been validated to the Functional Requirements and is ready for operations. The design was built based on heritage processes, new technology, and lessons learned from past experience. Furthermore, our operational concepts must be properly mapped to the <span class="hlt">mission</span> design and science objectives. However, during the course of implementing the science objective in the operations phase after launch, the MOS experiences an evolutional change to adapt for actual performance characteristics. This drives the re-engineering of the MOS, because the MOS includes the flight and ground segments. Using the Spitzer <span class="hlt">mission</span> as an example we demonstrate how the MOS design evolved for both the prime and extended <span class="hlt">mission</span> to enhance the overall efficiency for science return. In our re-engineering process, we ensured that no requirements were violated or <span class="hlt">mission</span> objectives compromised. In most cases, optimized performance across the MOS, including gains in science return as well as savings in the budget profile was achieved. Finally, we suggest a need to better categorize the Operations Phase (Phase E) in the NASA <span class="hlt">Life</span>-Cycle Phases of Formulation and Implementation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790023145&hterms=animal+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Danimal%2Bscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790023145&hterms=animal+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Danimal%2Bscience"><span>Experimental control requirements for <span class="hlt">life</span> sciences</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Berry, W. E.; Sharp, J. C.</p> <p>1978-01-01</p> <p>The <span class="hlt">Life</span> Sciences dedicated Spacelab will enable scientists to test hypotheses in various disciplines. Building upon experience gained in <span class="hlt">mission</span> simulations, orbital flight test experiments, and the first three Spacelab <span class="hlt">missions</span>, NASA will be able to progressively develop the engineering and management capabilities necessary for the first <span class="hlt">Life</span> Sciences Spacelab. Development of experiments for these <span class="hlt">missions</span> will require implementation of <span class="hlt">life</span>-support systems not previously flown in space. Plant growth chambers, animal holding facilities, aquatic specimen <span class="hlt">life</span>-support systems, and centrifuge-mounted specimen holding units are examples of systems currently being designed and fabricated for flight.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.9071N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.9071N"><span>The ENVISAT Atmospheric Chemistry <span class="hlt">mission</span> (GOMOS, MIPAS and SCIAMACHY) - Instrument status and <span class="hlt">mission</span> evolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niro, F.</p> <p>2009-04-01</p> <p>The ENVISAT ESA's satellite was launched on a polar orbit on March 2002. It carries on-board three atmospheric chemistry instruments: GOMOS, MIPAS and SCIAMACHY [1]. At the present time, although the <span class="hlt">mission</span> expected lifetime of 5 years has been already exceeded, all the payload modules are in good to excellent status. The only limiting factor is the available fuel that is used for orbit control manoeuvre. Recently a new strategy was proposed [2] that will allow to save fuel and to extend the <span class="hlt">mission</span> up to 2013. Following this strategy, the altitude of the orbit will be lowered by 17 km starting from end of 2010 and the inclination will be allowed to drift. The new orbit scenario will result in a new repeating cycle with a variation of the Mean Local Solar Time (MLST). This will have an impact on both the in-flight operations, on the science data and on the <span class="hlt">mission</span>. The simulations carried out for the atmospheric chemistry instruments show that the new orbit strategy will neither have a significant impact in the instrument operations nor on the quality of the science data. Therefore we expect that the atmospheric <span class="hlt">mission</span> will continue nominally until the end of the platform <span class="hlt">life</span> time, providing to the scientist a unique dataset of the most important geophysical parameters (e.g., trace gases, clouds, and aerosol) spanning a time interval of about 11 years. The aim of this paper is to review the overall ENVISAT atmospheric <span class="hlt">mission</span> status for the past, present and future. The evolution of the instrument performances since launch will be analyzed with focus on the <span class="hlt">life</span>-limited items monitoring. The tuning of the instrument in-flight operations decided to cope with instrument degradation or scientific needs will be described. The lessons learned on how to operate and monitor the instruments will be highlighted. Finally the expected evolution of the instrument performances until the ENVISAT end-of-<span class="hlt">life</span> will be discussed. [1] H. Nett, J. Frerick, T. Paulsen, and G</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010cosp...38..126D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010cosp...38..126D"><span>The ENVISAT Atmospheric Chemistry <span class="hlt">mission</span> (GOMOS, MIPAS and SCIAMACHY) -Instrument status and <span class="hlt">mission</span> evolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dehn, Angelika</p> <p></p> <p>The ENVISAT ESA's satellite was launched on a polar orbit on March 2002. It carries on-board three atmospheric chemistry instruments: GOMOS, MIPAS and SCIAMACHY [1]. At the present time, although the <span class="hlt">mission</span> expected lifetime of 5 years has been already exceeded, all the payload modules are in good to excellent status. The only limiting factor is the available fuel that is used for orbit control manoeuvre. A new strategy was proposed [2] that will allow to save fuel and to extend the <span class="hlt">mission</span> up to 2013. Following this strategy, the altitude of the orbit will be lowered by 17 km starting from end of 2010 and the inclination will be allowed to drift. The new orbit scenario will result in a new repeating cycle with a variation of the Mean Local Solar Time (MLST). This will have an impact on both the in-flight operations, on the science data and on the <span class="hlt">mission</span>. The simulations carried out for the atmospheric chemistry instruments show that the new orbit strategy will neither have a significant impact in the instrument operations nor on the quality of the science data. Therefore we expect that the atmospheric <span class="hlt">mission</span> will continue nominally until the end of the platform <span class="hlt">life</span> time, providing to the scientist a unique dataset of the most important geophysical parameters (e.g., trace gases, clouds, and aerosol) spanning a time interval of about 11 years. The aim of this paper is to review the overall ENVISAT atmospheric <span class="hlt">mission</span> status for the past, present and future. The evolution of the instrument performances since launch will be analyzed with focus on the <span class="hlt">life</span>-limited items monitoring. The tuning of the instrument in-flight operations decided to cope with instrument degradation or scientific needs will be described. The lessons learned on how to operate and monitor the instruments will be highlighted. Finally the expected evolution of the instrument performances until the ENVISAT end-of-<span class="hlt">life</span> will be discussed. [1] H. Nett, J. Frerick, T. Paulsen, and G. Levrini, "The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960001911','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960001911"><span>Spacelab <span class="hlt">Life</span> Sciences-1</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dalton, Bonnie P.; Jahns, Gary; Meylor, John; Hawes, Nikki; Fast, Tom N.; Zarow, Greg</p> <p>1995-01-01</p> <p>This report provides an historical overview of the Spacelab <span class="hlt">Life</span> Sciences-1 (SLS-1) <span class="hlt">mission</span> along with the resultant biomaintenance data and investigators' findings. Only the nonhuman elements, developed by Ames Research Center (ARC) researchers, are addressed herein. The STS-40 flight of SLS-1, in June 1991, was the first spacelab flown after 'return to orbit', it was also the first spacelab <span class="hlt">mission</span> specifically designated as a <span class="hlt">Life</span> Sciences Spacelab. The experiments performed provided baseline data for both hardware and rodents used in succeeding <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992STIN...9424995R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992STIN...9424995R"><span>PERCIVAL <span class="hlt">mission</span> to Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reed, David W.; Lilley, Stewart; Sirman, Melinda; Bolton, Paul; Elliott, Susan; Hamilton, Doug; Nickelson, James; Shelton, Artemus</p> <p>1992-12-01</p> <p>With the downturn of the world economy, the priority of unmanned exploration of the solar system has been lowered. Instead of foregoing all <span class="hlt">missions</span> to our neighbors in the solar system, a new philosophy of exploration <span class="hlt">mission</span> design has evolved to insure the continued exploration of the solar system. The 'Discovery-class' design philosophy uses a low cost, limited <span class="hlt">mission</span>, available technology spacecraft instead of the previous 'Voyager-class' design philosophy that uses a 'do-everything at any cost' spacecraft. The Percival <span class="hlt">Mission</span> to Mars was proposed by Ares Industries as one of the new 'Discovery-class' of exploration <span class="hlt">missions</span>. The spacecraft will be christened Percival in honor of American astronomer Percival Lowell who proposed the existence of <span class="hlt">life</span> on Mars in the early twentieth century. The main purpose of the Percival <span class="hlt">mission</span> to Mars is to collect and relay scientific data to Earth suitable for designing future manned and unmanned <span class="hlt">missions</span> to Mars. The measurements and observations made by Percival will help future <span class="hlt">mission</span> designers to choose among landing sites based on the feasibility and scientific interest of the sites. The primary measurements conducted by the Percival <span class="hlt">mission</span> include gravity field determination, surface and atmospheric composition, sub-surface soil composition, sub-surface seismic activity, surface weather patterns, and surface imaging. These measurements will be taken from the orbiting Percival spacecraft and from surface penetrators deployed from Mars orbit. The design work for the Percival <span class="hlt">Mission</span> to Mars was divided among four technical areas: Orbits and Propulsion System, Surface Penetrators, Gravity and Science Instruments, and Spacecraft Structure and Systems. The results for each of the technical areas is summarized and followed by a design cost analysis and recommendations for future analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940020513','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940020513"><span>PERCIVAL <span class="hlt">mission</span> to Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Reed, David W.; Lilley, Stewart; Sirman, Melinda; Bolton, Paul; Elliott, Susan; Hamilton, Doug; Nickelson, James; Shelton, Artemus</p> <p>1992-01-01</p> <p>With the downturn of the world economy, the priority of unmanned exploration of the solar system has been lowered. Instead of foregoing all <span class="hlt">missions</span> to our neighbors in the solar system, a new philosophy of exploration <span class="hlt">mission</span> design has evolved to insure the continued exploration of the solar system. The 'Discovery-class' design philosophy uses a low cost, limited <span class="hlt">mission</span>, available technology spacecraft instead of the previous 'Voyager-class' design philosophy that uses a 'do-everything at any cost' spacecraft. The Percival <span class="hlt">Mission</span> to Mars was proposed by Ares Industries as one of the new 'Discovery-class' of exploration <span class="hlt">missions</span>. The spacecraft will be christened Percival in honor of American astronomer Percival Lowell who proposed the existence of <span class="hlt">life</span> on Mars in the early twentieth century. The main purpose of the Percival <span class="hlt">mission</span> to Mars is to collect and relay scientific data to Earth suitable for designing future manned and unmanned <span class="hlt">missions</span> to Mars. The measurements and observations made by Percival will help future <span class="hlt">mission</span> designers to choose among landing sites based on the feasibility and scientific interest of the sites. The primary measurements conducted by the Percival <span class="hlt">mission</span> include gravity field determination, surface and atmospheric composition, sub-surface soil composition, sub-surface seismic activity, surface weather patterns, and surface imaging. These measurements will be taken from the orbiting Percival spacecraft and from surface penetrators deployed from Mars orbit. The design work for the Percival <span class="hlt">Mission</span> to Mars was divided among four technical areas: Orbits and Propulsion System, Surface Penetrators, Gravity and Science Instruments, and Spacecraft Structure and Systems. The results for each of the technical areas is summarized and followed by a design cost analysis and recommendations for future analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920003933','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920003933"><span>Space acceleration measurement system description and operations on the First Spacelab <span class="hlt">Life</span> Sciences <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Delombard, Richard; Finley, Brian D.</p> <p>1991-01-01</p> <p>The Space Acceleration Measurement System (SAMS) project and flight units are briefly described. The SAMS operations during the STS-40 <span class="hlt">mission</span> are summarized, and a preliminary look at some of the acceleration data from that <span class="hlt">mission</span> are provided. The background and rationale for the SAMS project is described to better illustrate its goals. The functions and capabilities of each SAMS flight unit are first explained, then the STS-40 <span class="hlt">mission</span>, the SAMS's function for that <span class="hlt">mission</span>, and the preparation of the SAMS are described. Observations about the SAMS operations during the first SAMS <span class="hlt">mission</span> are then discussed. Some sample data are presented illustrating several aspects of the <span class="hlt">mission</span>'s microgravity environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.G21C..01T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.G21C..01T"><span>GRACE Status at <span class="hlt">Mission</span> End</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tapley, B. D.; Flechtner, F. M.; Watkins, M. M.; Bettadpur, S. V.</p> <p>2017-12-01</p> <p>The twin satellites of the Gravity Recovery and Climate Experiment (GRACE) were launched on March 17, 2002 and have operated for nearly 16 years. The <span class="hlt">mission</span> objectives are to observe the spatial and temporal variations of the Earth's mass through its effects on the gravity field at the GRACE satellite altitude. The mass changes observed are related to both the changes within the solid earth and the change within and between the Erath system components. A significant cause of the time varying mass is water motion and the GRACE <span class="hlt">mission</span> has provided a continuous decade long measurement sequence which characterizes the seasonal cycle of mass transport between the oceans, land, cryosphere and atmosphere; its inter-annual variability; and the climate driven secular, or long period, mass transport signals. The fifth reanalysis on the <span class="hlt">mission</span> data set, the RL05 data, were released in mid-2013. With the planned launch of GRACE Follow-On in early 2018, plans are underway for a reanalysis that will be consistent with the GRACE FO processing standards. The <span class="hlt">mission</span> is entering the final phases of its operation <span class="hlt">life</span> with <span class="hlt">mission</span> end expected to occur in early 2018. The current <span class="hlt">mission</span> operations strategy emphasizes extending the <span class="hlt">mission</span> lifetime to obtain an overlap with the GRACE FO. This presentation will review the <span class="hlt">mission</span> status and the projections for <span class="hlt">mission</span> lifetime, describe the current operations philosophy and its impact on the science data, discuss the issues related to achieving the GRACE and GRACE FO connection and discuss issues related to science data products during this phase of the <span class="hlt">mission</span> period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/10191068','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/10191068"><span>Cycle <span class="hlt">life</span> testing of lithium-ion batteries for small satellite LEO space <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Mayer, S.T.; Feikert, J.H.; Kaschmitter, J.L.</p> <p>1993-08-16</p> <p>In 1990, Sony corporation announced their intention to manufacture a rechargeable lithium ion battery, based on the intercalation of lithium ions into a carbonaceous anode. The cells were first introduced for portable telephone use in June, 1991. (1) A 3.6V average cell voltage (4.1-2.75V range); (2) Excellent cycle <span class="hlt">life</span> (1200 @ 100% DOD); (3) Good capacity retention (70% after 6 months); (4) Wide temperature range performance ({minus}20 to +60{degrees}C); (5) Excellent Discharge rate (82% capacity at 30 min. discharge rate); (6) Excellent Charge rate (100% Charge in <3 hrs); and (7) High energy density (264 W*hr/1 and 120 Whr/kg formore » ``D`` size cell. These specifications show significant promise for application of these batteries in low earth orbit (LEO) small satellites, particularly when compared to existing NiH{sub 2} and NiCd technology. The very high energy density and specific energy will reduce power system volume and weight. The wide temperature range enables simpler thermal design, particularly for new, small, high power satellites. The materials used in the lithium ion batteries are relatively inexpensive and benign, so that we expect costs to come down substantially in the future. The specified cycle <span class="hlt">life</span> at 100% DOD is also 50% longer than most NiCds, so low DOD (depth of discharge) performance could be substantial. This study was undertaken to: (a) assess the feasibility for using lithium ion cells on small satellite LEO <span class="hlt">missions</span> and (b) verify the claims of the manufacturer. This was accomplished by performing a detailed autopsy and various depth of discharge and rate tests on the cells. Of special interest was the cycle <span class="hlt">life</span> performance of these cell at various depths of discharge DOD`s, to get an initial measure of the reduction in capacity fade with cycle conditions. Low DOD`s are used to extend the <span class="hlt">life</span> of all batteries used in a space application.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000109794','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000109794"><span>Sample Returns <span class="hlt">Missions</span> in the Coming Decade</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Desai, Prasun N.; Mitcheltree, Robert A.; Cheatwood, F. McNeil</p> <p>2000-01-01</p> <p>In the coming decade, several <span class="hlt">missions</span> will attempt to return samples to Earth from varying parts of the solar system. These samples will provide invaluable insight into the conditions present during the early formation of the solar system, and possibly give clues to how <span class="hlt">life</span> began on Earth. A description of five sample return <span class="hlt">missions</span> is presented (Stardust, Genesis, Muses-C. Mars Sample Return, and Comet Nucleus Sample Return). An overview of each sample return <span class="hlt">mission</span> is given, concentrating particularly on the technical challenges posed during the Earth entry, descent, and landing phase of the <span class="hlt">missions</span>. Each <span class="hlt">mission</span> faces unique challenges in the design of an Earth entry capsule. The design of the entry capsule must address the aerodynamic, heating, deceleration, landing, and recovery requirements for the safe return of samples to Earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870012670','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870012670"><span>Spacelab 3 <span class="hlt">Mission</span> Science Review</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fichtl, George H. (Editor); Theon, John S. (Editor); Hill, Charles K. (Editor); Vaughan, Otha H. (Editor)</p> <p>1987-01-01</p> <p>Papers and abstracts of the presentations made at the symposium are given as the scientific report for the Spacelab 3 <span class="hlt">mission</span>. Spacelab 3, the second flight of the National Aeronautics and Space Administration's (NASA) orbital laboratory, signified a new era of research in space. The primary objective of the <span class="hlt">mission</span> was to conduct applications, science, and technology experiments requiring the low-gravity environment of Earth orbit and stable vehicle attitude over an extended period (e.g., 6 days) with emphasis on materials processing. The <span class="hlt">mission</span> was launched on April 29, 1985, aboard the Space Shuttle Challenger which landed a week later on May 6. The multidisciplinary payload included 15 investigations in five scientific fields: material science, fluid dynamics, <span class="hlt">life</span> sciences, astrophysics, and atmospheric science.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880065118&hterms=pearson+human&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dpearson%2Bhuman','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880065118&hterms=pearson+human&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dpearson%2Bhuman"><span>Manned Mars <span class="hlt">Mission</span> program concepts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hamilton, E. C.; Johnson, P.; Pearson, J.; Tucker, W.</p> <p>1988-01-01</p> <p>This paper describes the SRS Manned Mars <span class="hlt">Mission</span> and Program Analysis study designed to support a manned expedition to Mars contemplated by NASA for the purposes of initiating human exploration and eventual habitation of this planet. The capabilities of the interactive software package being presently developed by the SRS for the <span class="hlt">mission</span>/program analysis are described, and it is shown that the interactive package can be used to investigate the impact of various <span class="hlt">mission</span> concepts on the sensitivity of mass required in LEO, schedules, relative costs, and risk. The results, to date, indicate the need for an earth-to-orbit transportation system much larger than the present STS, reliable long-<span class="hlt">life</span> support systems, and either advanced propulsion or aerobraking technology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012SPIE.8521E..02L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012SPIE.8521E..02L"><span>Stealth <span class="hlt">life</span> detection instruments aboard Curiosity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Levin, Gilbert V.</p> <p>2012-10-01</p> <p>NASA has often stated (e.g. MSL Science Corner1) that it's Mars Science Laboratory (MSL), "Curiosity," <span class="hlt">Mission</span> to Mars carries no <span class="hlt">life</span> detection experiments. This is in keeping with NASA's 36-year explicit ban on such, imposed immediately after the 1976 Viking <span class="hlt">Mission</span> to Mars. The space agency attributes the ban to the "ambiguity" of that <span class="hlt">Mission</span>'s Labeled Release (LR) <span class="hlt">life</span> detection experiment, fearing an adverse effect on the space program should a similar "inconclusive" result come from a new robotic quest. Yet, despite the NASA ban, this author, the Viking LR Experimenter, contends there are "stealth <span class="hlt">life</span> detection instruments" aboard Curiosity. These are <span class="hlt">life</span> detection instruments in the sense that they can free the Viking LR from the pall of ambiguity that has held it prisoner so long. Curiosity's stealth instruments are those seeking organic compounds, and the <span class="hlt">mission</span>'s high-resolution camera system. Results from any or all of these devices, coupled with the Viking LR data, can confirm the LR's <span class="hlt">life</span> detection claim. In one possible scenario, Curiosity can, of itself, completely corroborate the finding of <span class="hlt">life</span> on Mars. MSL has just successfully landed on Mars. Hopefully, its stealth confirmations of <span class="hlt">life</span> will be reported shortly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19760060113&hterms=physics+astrophysics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dphysics%2Bastrophysics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19760060113&hterms=physics+astrophysics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dphysics%2Bastrophysics"><span>Early Spacelab physics and astronomy <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chapman, R. D.</p> <p>1976-01-01</p> <p>Some of the scientific problems which will be investigated during the early Spacelab physics and astronomy <span class="hlt">missions</span> are reviewed. The Solar Terrestrial Programs will include the Solar Physics Spacelab Payloads (SPSP) and the Atmospheres, Magnetospheres and Plasmas in Space (AMPS) <span class="hlt">missions</span>. These <span class="hlt">missions</span> will study the sun as a star and the influence of solar phenomena on the earth, including sun-solar wind interface, the nature of the solar flares, etc. The Astrophysics Spacelab Payloads (ASP) programs are divided into the Ultraviolet-Optical Astronomy and the High Energy Astrophysics areas. The themes of astrophysics Spacelab investigations will cover the nature of the universe, the fate of matter and the <span class="hlt">life</span> cycles of stars. The paper discusses various scientific experiments and instruments to be used in the early Spacelab <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830025644','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830025644"><span>Spacelab <span class="hlt">mission</span> 1 experiment descriptions, third edition</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Craven, P. D. (Editor)</p> <p>1983-01-01</p> <p>Experiments and facilities selected for flight on the first Spacelab <span class="hlt">mission</span> are described. Chosen from responses to the Announcement of Opportunity for the Spacelab 1 <span class="hlt">mission</span>, the experiments cover five broad areas of investigation: atmospheric physics and Earth observations; space plasma physics; astronomy and solar physics; material sciences and technology; and <span class="hlt">life</span> sciences. The name of the principal investigator and country is listed for each experiment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AdSpR..56..479A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AdSpR..56..479A"><span>End-of-<span class="hlt">life</span> disposal of high elliptical orbit <span class="hlt">missions</span>: The case of INTEGRAL</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Armellin, Roberto; San-Juan, Juan F.; Lara, Martin</p> <p>2015-08-01</p> <p>Nowadays there is international consensus that space activities must be managed to minimize debris generation and risk. The paper presents a method for the end-of-<span class="hlt">life</span> (EoL) disposal of spacecraft in high elliptical orbits (HEO). The time evolution of HEO is strongly affected by Earth's oblateness and luni-solar perturbation, and this can cause in the long-term to extended interferences with low Earth orbit (LEO) protected region and uncontrolled Earth re-entry. An EoL disposal concept that exploits the effect of orbital perturbations to reduce the disposal cost is presented. The problem is formulated as a multiobjective optimization problem, which is solved with an evolutionary algorithm. To explore at the best the search space a semi-analytical orbit propagator, which allows the propagation of the orbit motion for 100 years in few seconds, is adopted. The EoL disposal of the INTErnational Gamma-Ray Astrophysics Laboratory (INTEGRAL) <span class="hlt">mission</span> is used as a practical test-case to show the effectiveness of the proposed methodology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-0500974&hterms=neuroscience&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dneuroscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-0500974&hterms=neuroscience&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dneuroscience"><span>STS-90 <span class="hlt">Mission</span> Insignia</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>The STS-90 crew patch reflects the dedication of the <span class="hlt">mission</span> to neuroscience in celebration of the decade of the brain. Earth is revealed through a neuron-shaped window, which symbolizes new perspectives in the understanding of nervous system development, structure and function, both here on Earth and in the microgravity environment of space. The Space Shuttle Columbia is depicted with its open payload bay doors revealing the Spacelab within. An integral component of the <span class="hlt">mission</span>, the laboratory/science module provided by the European Space Agency (ESA), signifies the strong international involvement in the <span class="hlt">mission</span>. The seven crew members and two alternate payload specialists, Chiaki Naito-Mukai and Alexander W. Dunlap, are represented by the nine major stars of the constellation Cetus (the whale) in recognition of the International Year of the Ocean. The distant stars illustrate the far reaching implications of the <span class="hlt">mission</span> science to the many sponsoring agencies, helping prepare for long-duration space flight aboard the International Space Station (ISS). The moon and Mars are depicted to reflect the crew's recognition that those two celestial bodies will be the next great challenges in human exploration of space and represent the key role that <span class="hlt">life</span> science research will play in supporting such <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870008363','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870008363"><span>Manned Mars <span class="hlt">mission</span> communication and data management systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>White, Ronald E.</p> <p>1986-01-01</p> <p>A manned Mars <span class="hlt">mission</span> will involve a small crew and many complex tasks. The productivity of the crew and the entire <span class="hlt">mission</span> will depend significantly on effective automation of these tasks and the ease with which the crew can interface with them. The technology to support a manned Mars <span class="hlt">mission</span> is available today; however, evolving software and electronic technology are enabling many interesting possibilities for increasing productivity and safety while reducing <span class="hlt">life</span> cycle cost. Some of these advanced technologies are identified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19710003598','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19710003598"><span>Apollo 13 <span class="hlt">Mission</span> Report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1970-01-01</p> <p>The Apollo 13 <span class="hlt">mission</span>, planned as a lunar landing in the Fra Mauro area, was aborted because of an abrupt loss of service module cryogenic oxygen associated with a fire in one of the two tanks at approximately 56 hours. The lunar module provided the necessary support to sustain a minimum operational condition for a safe return to earth. A circumlunar profile was executed as the most efficient means of earth return, with the lunar module providing power and <span class="hlt">life</span> support until transfer to the command module just prior to entry. Although the <span class="hlt">mission</span> was unsuccessful as planned, a lunar flyby and several scientific experiments were completed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120010672','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120010672"><span>NASA Advanced <span class="hlt">Life</span> Support Technology Testing and Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wheeler, Raymond M.</p> <p>2012-01-01</p> <p>Prior to 2010, NASA's advanced <span class="hlt">life</span> support research and development was carried out primarily under the Exploration <span class="hlt">Life</span> Support Project of NASA's Exploration Systems <span class="hlt">Mission</span> Directorate. In 2011, the Exploration <span class="hlt">Life</span> Support Project was merged with other projects covering Fire Prevention/Suppression, Radiation Protection, Advanced Environmental Monitoring and Control, and Thermal Control Systems. This consolidated project was called <span class="hlt">Life</span> Support and Habitation Systems, which was managed under the Exploration Systems <span class="hlt">Mission</span> Directorate. In 2012, NASA re-organized major directorates within the agency, which eliminated the Exploration Systems <span class="hlt">Mission</span> Directorate and created the Office of the Chief Technologist (OCT). <span class="hlt">Life</span> support research and development is currently conducted within the Office of the Chief Technologist, under the Next Generation <span class="hlt">Life</span> Support Project, and within the Human Exploration Operation <span class="hlt">Missions</span> Directorate under several Advanced Exploration System projects. These Advanced Exploration Systems projects include various themes of <span class="hlt">life</span> support technology testing, including atmospheric management, water management, logistics and waste management, and habitation systems. Food crop testing is currently conducted as part of the Deep Space Habitation (DSH) project within the Advanced Exploration Systems Program. This testing is focused on growing salad crops that could supplement the crew's diet during near term <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890013614','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890013614"><span>Human exploration <span class="hlt">mission</span> studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cataldo, Robert L.</p> <p>1989-01-01</p> <p>The Office of Exploration has established a process whereby all NASA field centers and other NASA Headquarters offices participate in the formulation and analysis of a wide range of <span class="hlt">mission</span> strategies. These strategies were manifested into specific scenarios or candidate case studies. The case studies provided a systematic approach into analyzing each <span class="hlt">mission</span> element. First, each case study must address several major themes and rationale including: national pride and international prestige, advancement of scientific knowledge, a catalyst for technology, economic benefits, space enterprise, international cooperation, and education and excellence. Second, the set of candidate case studies are formulated to encompass the technology requirement limits in the <span class="hlt">life</span> sciences, launch capabilities, space transfer, automation, and robotics in space operations, power, and propulsion. The first set of reference case studies identify three major strategies: human expeditions, science outposts, and evolutionary expansion. During the past year, four case studies were examined to explore these strategies. The expeditionary <span class="hlt">missions</span> include the Human Expedition to Phobos and Human Expedition to Mars case studies. The Lunar Observatory and Lunar Outpost to Early Mars Evolution case studies examined the later two strategies. This set of case studies established the framework to perform detailed <span class="hlt">mission</span> analysis and system engineering to define a host of concepts and requirements for various space systems and advanced technologies. The details of each <span class="hlt">mission</span> are described and, specifically, the results affecting the advanced technologies required to accomplish each <span class="hlt">mission</span> scenario are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19760006049','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19760006049"><span>Manned orbital systems concepts study. Book 3: Configurations for extended duration <span class="hlt">missions</span>. [<span class="hlt">mission</span> planning and project planning for space <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1975-01-01</p> <p><span class="hlt">Mission</span> planning, systems analysis, and design concepts for the Space Shuttle/Spacelab system for extended manned operations are described. Topics discussed are: (1) payloads, (2) spacecraft docking, (3) structural design criteria, (4) <span class="hlt">life</span> support systems, (5) power supplies, and (6) the role of man in long duration orbital operations. Also discussed are the assembling of large structures in space. Engineering drawings are included.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770036625&hterms=papers+scientists&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dpapers%2Bscientists','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770036625&hterms=papers+scientists&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dpapers%2Bscientists"><span><span class="hlt">Life</span> Sciences Laboratories for the Shuttle/Spacelab</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schulte, L. O.; Kelly, H. B.; Secord, T. C.</p> <p>1976-01-01</p> <p>Space Shuttle and Spacelab <span class="hlt">missions</span> will provide scientists with their first opportunity to participate directly in research in space for all scientific disciplines, particularly the <span class="hlt">Life</span> Sciences. Preparations are already underway to ensure the success of these <span class="hlt">missions</span>. The paper summarizes the results of the 1975 NASA-funded <span class="hlt">Life</span> Sciences Laboratories definition study which defined several long-range <span class="hlt">life</span> sciences research options and the laboratory designs necessary to accomplish high-priority <span class="hlt">life</span> sciences research. The implications and impacts of Spacelab design and development on the <span class="hlt">life</span> sciences <span class="hlt">missions</span> are discussed. An approach is presented based upon the development of a general-purposs laboratory capability and an inventory of common operational research equipment for conducting <span class="hlt">life</span> sciences research. Several <span class="hlt">life</span> sciences laboratories and their capabilities are described to demonstrate the systems potentially available to the experimenter for conducting biological and medical research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000020489&hterms=Science+projects&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DScience%2Bprojects','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000020489&hterms=Science+projects&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DScience%2Bprojects"><span>The Human Space <span class="hlt">Life</span> Sciences Critical Path Roadmap Project: A Strategy for Human Space Flight through Exploration-Class <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sawin, Charles F.</p> <p>1999-01-01</p> <p>The product of the critical path roadmap project is an integrated strategy for mitigating the risks associated with human exploration class <span class="hlt">missions</span>. It is an evolving process that will assure the ability to communicate the integrated critical path roadmap. Unlike previous reports, this one will not sit on a shelf - it has the full support of the JSC Space and <span class="hlt">Life</span> Sciences Directorate (SA) and is already being used as a decision making tool (e.g., budget and investigation planning for Shuttle and Space Station <span class="hlt">mission</span>). Utility of this product depends on many efforts, namely: providing the required information (completed risk data sheets, critical question information, technology data). It is essential to communicate the results of the critical path roadmap to the scientific community - this meeting is a good opportunity to do so. The web site envisioned for the critical path roadmap will provide the capability to communicate to a broader community and to track and update the system routinely.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AdSpR..38..752H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AdSpR..38..752H"><span>HUMEX, a study on the survivability and adaptation of humans to long-duration exploratory <span class="hlt">missions</span>, part II: <span class="hlt">Missions</span> to Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horneck, G.; Facius, R.; Reichert, M.; Rettberg, P.; Seboldt, W.; Manzey, D.; Comet, B.; Maillet, A.; Preiss, H.; Schauer, L.; Dussap, C. G.; Poughon, L.; Belyavin, A.; Reitz, G.; Baumstark-Khan, C.; Gerzer, R.</p> <p>2006-01-01</p> <p>Space exploration programmes, currently under discussion in the US and in Europe, foresee human <span class="hlt">missions</span> to Mars to happen within the first half of this century. In this context, the European Space Agency (ESA) has conducted a study on the human responses, limits and needs for such exploratory <span class="hlt">missions</span>, the so-called HUMEX study (ESA SP-1264). Based on a critical assessment of the limiting factors for human health and performance and the definition of the <span class="hlt">life</span> science and <span class="hlt">life</span> support requirements performed in the frame of the HUMEX study, the following major critical items have been identified: (i) radiation health risks, mainly occurring during the interplanetary transfer phases and severely augmented in case of an eruption of a solar particle event; (ii) health risks caused by extended periods in microgravity with an unacceptable risk of bone fracture as a consequence of bone demineralisation; (iii) psychological risks as a consequence of long-term isolation and confinement in an environment so far not experienced by humans; (iv) the requirement of bioregenerative <span class="hlt">life</span> support systems complementary to physico-chemical systems, and of in situ resource utilisation to reach a closure of the <span class="hlt">life</span> support system to the highest degree possible. Considering these constraints, it has been concluded that substantial research and development activities are required in order to provide the basic information for appropriate integrated risk managements, including efficient countermeasures and tailored <span class="hlt">life</span> support. Methodological approaches should include research on the ISS, on robotic precursors <span class="hlt">missions</span> to Mars, in ground-based simulation facilities as well as in analogue natural environments on Earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000085887','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000085887"><span>Mitigating Adverse Effects of a Human <span class="hlt">Mission</span> On Possible Martian Indigenous Ecosystems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lupisella, Mark L.</p> <p>2000-01-01</p> <p>Although human beings are, by most standards, the most capable agents to search for and detect extraterrestrial <span class="hlt">life</span>, we are also potentially the most harmful. While there has been substantial work regarding forward contamination with respect to robotic <span class="hlt">missions</span>, the issue of potential adverse effects on possible indigenous Martian ecosystems, such as biological contamination, due to a human <span class="hlt">mission</span> has remained relatively unexplored and may require our attention now as this presentation will try to demonstrate by exploring some of the relevant scientific questions, <span class="hlt">mission</span> planning challenges, and policy issues. An informal, high-level <span class="hlt">mission</span> planning decision tree will be discussed and is included as the next page of this abstract. Some of the questions to be considered are: To what extent could contamination due to a human presence compromise possible indigenous <span class="hlt">life</span> forms? To what extent can we control contamination? For example, will it be local or global? What are the criteria for assessing the biological status of Mars, both regionally and globally? For example, can we adequately extrapolate from a few strategic <span class="hlt">missions</span> such as sample return <span class="hlt">missions</span>? What should our policies be regarding our <span class="hlt">mission</span> planning and possible interaction with what are likely to be microbial forms of extraterrestrial <span class="hlt">life</span>? Central to the science and <span class="hlt">mission</span> planning issues is the role and applicability of terrestrial analogs, such as Lake Vostok for assessing drilling issues, and modeling techniques. Central to many of the policy aspects are scientific value, international law, public concern, and ethics. Exploring this overall issue responsibly requires an examination of all these aspects and how they interrelate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010020469&hterms=ethic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dethic','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010020469&hterms=ethic&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dethic"><span>Mitigating Adverse Effects of a Human <span class="hlt">Mission</span> on Possible Martian Indigenous Ecosystems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lupisella, M. L.</p> <p>2000-01-01</p> <p>Although human beings are, by most standards, the most capable agents to search for and detect extraterrestrial <span class="hlt">life</span>, we are also potentially the most harmful. While there has been substantial work regarding forward contamination with respect to robotic <span class="hlt">missions</span>, the issue of potential adverse effects on possible indigenous Martian ecosystems, such as biological contamination, due to a human <span class="hlt">mission</span> has remained relatively unexplored and may require our attention now as this presentation will try to demonstrate by exploring some of the relevant scientific questions, <span class="hlt">mission</span> planning challenges, and policy issues. An informal, high-level <span class="hlt">mission</span> planning decision tree will be discussed and is included as the next page of this abstract. Some of the questions to be considered are: (1) To what extent could contamination due to a human presence compromise possible indigenous <span class="hlt">life</span> forms? (2) To what extent can we control contamination? For example, will it be local or global? (3) What are the criteria for assessing the biological status of Mars, both regionally and globally? For example, can we adequately extrapolate from a few strategic <span class="hlt">missions</span> such as sample return <span class="hlt">missions</span>? (4) What should our policies be regarding our <span class="hlt">mission</span> planning and possible interaction with what are likely to be microbial forms of extraterrestrial <span class="hlt">life</span>? (5) Central to the science and <span class="hlt">mission</span> planning issues is the role and applicability of terrestrial analogs, such as Lake Vostok for assessing drilling issues, and modeling techniques. Central to many of the policy aspects are scientific value, international law, public concern, and ethics. Exploring this overall issue responsibly requires an examination of all these aspects and how they interrelate. A chart is included, titled '<span class="hlt">Mission</span> Planning Decision Tree for Mitigating Adverse Effects to Possible Indigenous Martian Ecosystems due to a Human <span class="hlt">Mission</span>'. It outlines what questions scientists should ask and answer before sending humans to Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000came.work..200L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000came.work..200L"><span>Mitigating Adverse Effects of a Human <span class="hlt">Mission</span> on Possible Martian Indigenous Ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lupisella, M. L.</p> <p>2000-07-01</p> <p>Although human beings are, by most standards, the most capable agents to search for and detect extraterrestrial <span class="hlt">life</span>, we are also potentially the most harmful. While there has been substantial work regarding forward contamination with respect to robotic <span class="hlt">missions</span>, the issue of potential adverse effects on possible indigenous Martian ecosystems, such as biological contamination, due to a human <span class="hlt">mission</span> has remained relatively unexplored and may require our attention now as this presentation will try to demonstrate by exploring some of the relevant scientific questions, <span class="hlt">mission</span> planning challenges, and policy issues. An informal, high-level <span class="hlt">mission</span> planning decision tree will be discussed and is included as the next page of this abstract. Some of the questions to be considered are: (1) To what extent could contamination due to a human presence compromise possible indigenous <span class="hlt">life</span> forms? (2) To what extent can we control contamination? For example, will it be local or global? (3) What are the criteria for assessing the biological status of Mars, both regionally and globally? For example, can we adequately extrapolate from a few strategic <span class="hlt">missions</span> such as sample return <span class="hlt">missions</span>? (4) What should our policies be regarding our <span class="hlt">mission</span> planning and possible interaction with what are likely to be microbial forms of extraterrestrial <span class="hlt">life</span>? (5) Central to the science and <span class="hlt">mission</span> planning issues is the role and applicability of terrestrial analogs, such as Lake Vostok for assessing drilling issues, and modeling techniques. Central to many of the policy aspects are scientific value, international law, public concern, and ethics. Exploring this overall issue responsibly requires an examination of all these aspects and how they interrelate. A chart is included, titled '<span class="hlt">Mission</span> Planning Decision Tree for Mitigating Adverse Effects to Possible Indigenous Martian Ecosystems due to a Human <span class="hlt">Mission</span>'. It outlines what questions scientists should ask and answer before sending humans to Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011epsc.conf.1508R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011epsc.conf.1508R"><span>Planetary protection and Mars: requirements and constraints on the 2016 and 2018 <span class="hlt">missions</span>, and beyond</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rummel, J.; Kminek, G.; Conley, C.</p> <p>2011-10-01</p> <p>The suite of <span class="hlt">missions</span> being planned currently by NASA and ESA as a partnership under the name "ExoMars" include an orbiter and an entry, descent, and landing demonstrator module (EDM) for the 2016 "ExoMars Trace Gas Orbiter" <span class="hlt">mission</span> (ExoMars TGO), as well as a highly capable rover to be launched in 2018 to address the original ExoMars objectives (including the Pasteur payload). This 2018 ExoMars rover is expected to begin a series of <span class="hlt">missions</span> leading to the first sample return <span class="hlt">mission</span> from Mars, also conducted jointly between NASA, ESA, and their partners (JMSR). Each of these <span class="hlt">missions</span> and <span class="hlt">mission</span> components has a role in enabling future Mars exploration, including the search for <span class="hlt">life</span> or <span class="hlt">life</span>-related compounds on Mars, and each of them has the potential to carry confounding biological and organic materials into sensitive environments on Mars. Accordingly, this suite of <span class="hlt">missions</span> will be subjected to joint planetary protection requirements applied by both ESA and NASA to their respective components, according to the COSPAR-delineated planetary protection policy to protect Mars from contamination, and eventually to provide for the protection of the Earth from potential <span class="hlt">life</span> returned in a martian sample. This paper will discuss the challenges ahead for <span class="hlt">mission</span> designers and the <span class="hlt">mission</span> science teams, and will outline some of the potential pitfalls involved with different <span class="hlt">mission</span> options.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5936573','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5936573"><span>The <span class="hlt">Life</span> <span class="hlt">Mission</span> Theory VII. Theory of Existential (Antonovsky) Coherence: A Theory of Quality of <span class="hlt">Life</span>, Health, and Ability for Use in Holistic Medicine</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ventegodt, Søren; Flensborg-Madsen, Trine; Andersen, Niels Jørgen; Merrick, Joav</p> <p>2005-01-01</p> <p>A theoretical framework of existential coherence is presented, explaining how health, quality of <span class="hlt">life</span> (QOL), and the ability to function were originally created and developed to rehabilitate human <span class="hlt">life</span> from an existential perspective. The theory is inspired by the work of Aaron Antonovsky and explains our surprising recent empirical findings—that QOL, health, and ability primarily are determined by our consciousness. The theory is a matrix of nine key elements in five layers: (1) coherence; (2) purpose and talent; (3) consciousness, love, and physicality/sexuality; (4) light and joy; and (5) QOL/meaning of <span class="hlt">life</span>. The layer above causes the layer below, with the layer of QOL again feeding the fundamental layer of coherence. The model holds the person responsible for his or her own degree of reality, happiness, and being present. The model implies that when a person takes responsibility in all nine “dimensions” of <span class="hlt">life</span>, he or she can improve and develop health, the ability to function, all aspects of QOL, and the meaning of <span class="hlt">life</span>. The theory of existential coherence integrates a wide range of QOL theories from Jung and Maslow to Frankl and Wilber. It is a nine-ray theory in accordance with Gurjieff's enneagram and the old Indian chakra system. It can be used in the holistic medical clinic and in existential coaching. Love is in the center of the model and rehabilitation of love in its broadest sense is, accordingly, the essence of holistic medicine. To know yourself, your purpose of <span class="hlt">life</span> (<span class="hlt">life</span> <span class="hlt">mission</span>) and talents, and taking these into full use and becoming coherent with <span class="hlt">life</span> inside and reality outside is what human <span class="hlt">life</span> is essentially about. The new model has been developed to integrate the existing knowledge in the complex field of holistic medicine. Its strength is that it empowers the holistic physician to treat the patient with even severe diseases and can also be used for existential rehabilitation, holistic psychiatry, and sexology. Its major weakness is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AsBio...9..581R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AsBio...9..581R"><span>Tardigrade Resistance to Space Effects: First Results of Experiments on the <span class="hlt">LIFE</span>-TARSE <span class="hlt">Mission</span> on FOTON-M3 (September 2007)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rebecchi, Lorena; Altiero, Tiziana; Guidetti, Roberto; Cesari, Michele; Bertolani, Roberto; Negroni, Manuela; Rizzo, Angela M.</p> <p>2009-08-01</p> <p>The Tardigrade Resistance to Space Effects (TARSE) project, part of the <span class="hlt">mission</span> <span class="hlt">LIFE</span> on FOTON-M3, analyzed the effects of the space environment on desiccated and active tardigrades. Four experiments were conducted in which the eutardigrade Macrobiotus richtersi was used as a model species. Desiccated (in leaf litter or on paper) and hydrated tardigrades (fed or starved) were flown on FOTON-M3 for 12 days in September 2007, which, for the first time, allowed for a comparison of the effects of the space environment on desiccated and on active animals. In this paper, we report the experimental design of the TARSE project and data on tardigrade survival. In addition, data on survival, genomic DNA integrity, Hsp70 and Hsp90 expressions, antioxidant enzyme contents and activities, and <span class="hlt">life</span> history traits were compared between hydrated starved tardigrades flown in space and those maintained on Earth as a control. Microgravity and radiation had no effect on survival or DNA integrity of active tardigrades. Hsp expressions between the animals in space and the control animals on Earth were similar. Spaceflight induced an increase of glutathione content and its related enzymatic activities. Catalase and superoxide dismutase decreased with spaceflight, and thiobarbituric acid reactive substances did not change. During the flight <span class="hlt">mission</span>, tardigrades molted, and females laid eggs. Several eggs hatched, and the newborns exhibited normal morphology and behavior.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960035771','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960035771"><span>Flight Dynamics <span class="hlt">Mission</span> Support and Quality Assurance Process</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Oh, InHwan</p> <p>1996-01-01</p> <p>This paper summarizes the method of the Computer Sciences Corporation Flight Dynamics Operation (FDO) quality assurance approach to support the National Aeronautics and Space Administration Goddard Space Flight Center Flight Dynamics Support Branch. Historically, a strong need has existed for developing systematic quality assurance using methods that account for the unique nature and environment of satellite Flight Dynamics <span class="hlt">mission</span> support. Over the past few years FDO has developed and implemented proactive quality assurance processes applied to each of the six phases of the Flight Dynamics <span class="hlt">mission</span> support <span class="hlt">life</span> cycle: systems and operations concept, system requirements and specifications, software development support, operations planing and training, launch support, and on-orbit <span class="hlt">mission</span> operations. Rather than performing quality assurance as a final step after work is completed, quality assurance has been built in as work progresses in the form of process assurance. Process assurance activities occur throughout the Flight Dynamics <span class="hlt">mission</span> support <span class="hlt">life</span> cycle. The FDO Product Assurance Office developed process checklists for prephase process reviews, <span class="hlt">mission</span> team orientations, in-progress reviews, and end-of-phase audits. This paper will outline the evolving history of FDO quality assurance approaches, discuss the tailoring of Computer Science Corporations's process assurance cycle procedures, describe some of the quality assurance approaches that have been or are being developed, and present some of the successful results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611806T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611806T"><span>The ODINUS <span class="hlt">Mission</span> Concept: a <span class="hlt">Mission</span> to the Ice Giant Planets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turrini, Diego; Politi, Romolo; Peron, Roberto; Grassi, Davide; Plainaki, Christina; Barbieri, Mauro; Massimo Lucchesi, David; Magni, Gianfranco; Altieri, Francesca; Cottini, Valeria; Gorius, Nicolas; Gaulme, Patrick; Schmider, François-Xavier; Adriani, Alberto; Piccioni, Giuseppe</p> <p>2014-05-01</p> <p>We present the scientific case and the <span class="hlt">mission</span> concept for the comparative exploration of the ice giant planets Uranus and Neptune and their satellites with a pair of twin spacecraft: ODINUS (Origins, Dynamics and Interiors of Neptunian and Uranian Systems). The ODINUS proposal was submitted in response to the call for white papers for the definition of the themes of the L2 and L3 <span class="hlt">mission</span> in the framework of the ESA Cosmic Vision 2015-2025 program. The goal of ODINUS is the advancement of our understanding of the ancient past of the Solar System and, more generally, of how planetary systems form and evolve. The <span class="hlt">mission</span> concept is focused on providing elements to answer to the scientific themes of the Cosmic Vision 2015-2025 program: What are the conditions for planetary formation and the emergency of <span class="hlt">life</span>? How does the Solar System work? What are the fundamental physical laws of the Universe? In order to achieve its goals, the ODINUS <span class="hlt">mission</span> concept proposed the use of two twin spacecraft to be put in orbit around Uranus and Neptune respectively, with selected flybys of their satellites. The proposed measurements aim to study the atmospheres and magnetospheres of the planets, the surfaces of the satellites, and the interior structure and composition of both satellites and planets. An important possibility for performing fundamental physics studies (among them tests of general relativity theory) is offered by the cruise phase. After the extremely positive evaluation of ESA Senior Survey Committee, who stated that 'the exploration of the icy giants appears to be a timely milestone, fully appropriate for an L class <span class="hlt">mission</span>', we discuss strategies to comparatively study Uranus and Neptune with future international <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840035232&hterms=Life+skies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DLife%2Bskies','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840035232&hterms=Life+skies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DLife%2Bskies"><span>Orbit and geometry constraints on the design and operation of a long-<span class="hlt">life</span> SIRTF <span class="hlt">mission</span>. [Shuttle Infrared Telescope Facility</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jackson, R. W.</p> <p>1984-01-01</p> <p>For a long-<span class="hlt">life</span> SIRTF <span class="hlt">mission</span>, the ability of the telescope to observe targets everywhere in the sky is an important requirement. For low-inclination orbits, a telescope aperture shade must be designed for Sun and Earth Limb avoidance angles of 50 deg to 60 deg to prevent unwanted radiation from entering the telescope. The minimum orbit inclination depends on the Earth Limb avoidance angle. About 30 percent of the sky will be prohibited for observations during any day in orbit, with about 100 days in orbit required to observe the entire sky.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930046927&hterms=indigenous&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dindigenous','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930046927&hterms=indigenous&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dindigenous"><span>Low cost manned Mars <span class="hlt">mission</span> based on indigenous propellant production</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bruckner, A. P.; Cinnamon, M.; Hamling, S.; Mahn, K.; Phillips, J.; Westmark, V.</p> <p>1993-01-01</p> <p>The paper describes a low-cost approach to the manned exploration of Mars (which involves an unmanned <span class="hlt">mission</span> followed two years later by a manned <span class="hlt">mission</span>) based on near-term technologies and in situ propellant production. Particular attention is given to the basic <span class="hlt">mission</span> architecture and its major components, including the orbital analysis, the unmanned segment, the Earth Return Vehicle, the aerobrake design, <span class="hlt">life</span> sciences, guidance, communications, power, propellant production, the surface rovers, and Mars science. Also discussed are the cost per <span class="hlt">mission</span> over an assumed 8-yr initiative.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100002027','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100002027"><span>Kepler: NASA's First <span class="hlt">Mission</span> Capable of Finding Earth-Size Planets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borucki, William J.</p> <p>2009-01-01</p> <p>Kepler, a NASA Discovery <span class="hlt">mission</span>, is a spaceborne telescope designed to search a nearby region of our galaxy for Earth-size planets orbiting in the habitable zone of stars like our sun. The habitable zone is that region around a start where the temperature permits water to be liquid on the surface of a planet. Liquid water is considered essential forth existence of <span class="hlt">life</span>. <span class="hlt">Mission</span> Phases: Six <span class="hlt">mission</span> phases have been defined to describe the different periods of activity during Kepler's <span class="hlt">mission</span>. These are: launch; commissioning; early science operations, science operations: and decommissioning</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040010358&hterms=Non+equivalent&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DNon%2Bequivalent','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040010358&hterms=Non+equivalent&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3DNon%2Bequivalent"><span>Equivalent Mass versus <span class="hlt">Life</span> Cycle Cost for <span class="hlt">Life</span> Support Technology Selection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Harry</p> <p>2003-01-01</p> <p>The decision to develop a particular <span class="hlt">life</span> support technology or to select it for flight usually depends on the cost to develop and fly it. Other criteria - performance, safety, reliability, crew time, and risk - are considered, but cost is always an important factor. Because launch cost accounts for most of the cost of planetary <span class="hlt">missions</span>, and because launch cost is directly proportional to the mass launched, equivalent mass has been used instead of cost to select <span class="hlt">life</span> support technology. The equivalent mass of a <span class="hlt">life</span> support system includes the estimated masses of the hardware and of the pressurized volume, power supply, and cooling system that the hardware requires. The equivalent mass is defined as the total payload launch mass needed to provide and support the system. An extension of equivalent mass, Equivalent System Mass (ESM), has been established for use in Advanced <span class="hlt">Life</span> Support. A crew time mass-equivalent and sometimes other non-mass factors are added to equivalent mass to create ESM. Equivalent mass is an estimate of the launch cost only. For earth orbit rather than planetary <span class="hlt">missions</span>, the launch cost is usually exceeded by the cost of Design, Development, Test, and Evaluation (DDT&E). Equivalent mass is used only in <span class="hlt">life</span> support analysis. <span class="hlt">Life</span> Cycle Cost (LCC) is much more commonly used. LCC includes DDT&E, launch, and operations costs. Since LCC includes launch cost, it is always a more accurate cost estimator than equivalent mass. The relative costs of development, launch, and operations vary depending on the <span class="hlt">mission</span> design, destination, and duration. Since DDT&E or operations may cost more than launch, LCC may give a more accurate cost ranking than equivalent mass. To be sure of identifying the lowest cost technology for a particular <span class="hlt">mission</span>, we should use LCC rather than equivalent mass.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160010586','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160010586"><span>Implementing Effective <span class="hlt">Mission</span> Systems Engineering Practices During Early Project Formulation Phases</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moton, Tryshanda</p> <p>2016-01-01</p> <p>Developing and implementing a plan for a NASA space <span class="hlt">mission</span> can be a complicated process. The needs, goals, and objectives of any proposed <span class="hlt">mission</span> or technology must be assessed early in the Project <span class="hlt">Life</span> Cycle. The key to successful development of a space <span class="hlt">mission</span> or flight project is the inclusion of systems engineering in early project formulation, namely during Pre-phase A, Phase A, and Phase B of the NASA Project <span class="hlt">Life</span> Cycle. When a space <span class="hlt">mission</span> or new technology is in pre-development, or "pre-Formulation", feasibility must be determined based on cost, schedule, and risk. Inclusion of system engineering during project formulation is key because in addition to assessing feasibility, design concepts are developed and alternatives to design concepts are evaluated. Lack of systems engineering involvement early in the project formulation can result in increased risks later in the implementation and operations phases of the project. One proven method for effective systems engineering practice during the pre-Formulation Phase is the use of a <span class="hlt">mission</span> conceptual design or technology development laboratory, such as the <span class="hlt">Mission</span> Design Lab (MDL) at NASA's Goddard Space Flight Center (GSFC). This paper will review the engineering process practiced routinely in the MDL for successful <span class="hlt">mission</span> or project development during the pre-Formulation Phase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160001262','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160001262"><span>The <span class="hlt">Life</span> Cycle Cost (LCC) of <span class="hlt">Life</span> Support Recycling and Resupply</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Harry W.</p> <p>2015-01-01</p> <p>Brief human space <span class="hlt">missions</span> supply all the crew's water and oxygen from Earth. The multiyear International Space Station (ISS) program instead uses physicochemical <span class="hlt">life</span> support systems to recycle water and oxygen. This paper compares the <span class="hlt">Life</span> Cycle Cost (LCC) of recycling to the LCC of resupply for potential future long duration human space <span class="hlt">missions</span>. Recycling systems have high initial development costs but relatively low durationdependent support costs. This means that recycling is more cost effective for longer <span class="hlt">missions</span>. Resupplying all the water and oxygen requires little initial development cost but has a much higher launch mass and launch cost. The cost of resupply increases as the <span class="hlt">mission</span> duration increases. Resupply is therefore more cost effective than recycling for shorter <span class="hlt">missions</span>. A recycling system pays for itself when the resupply LCC grows greater over time than the recycling LCC. The time when this occurs is called the recycling breakeven date. Recycling will cost very much less than resupply for long duration <span class="hlt">missions</span> within the Earth-Moon system, such as a future space station or Moon base. But recycling would cost about the same as resupply for long duration deep space <span class="hlt">missions</span>, such as a Mars trip. Because it is not possible to provide emergency supplies or quick return options on the way to Mars, more expensive redundant recycling systems will be needed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070019775','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070019775"><span>Ares V an Enabling Capability for Future Space Astrophysics <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stahl, H. Philip</p> <p>2007-01-01</p> <p>The potential capability offered by an Ares V launch vehicle completely changes the paradigm for future space astrophysics <span class="hlt">missions</span>. This presentation examines some details of this capability and its impact on potential <span class="hlt">missions</span>. A specific case study is presented: implementing a 6 to 8 meter class monolithic UV/Visible telescope at an L2 orbit. Additionally discussed is how to extend the <span class="hlt">mission</span> <span class="hlt">life</span> of such a telescope to 30 years or longer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100030350','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100030350"><span>Potential Lunar In-Situ Resource Utilization Experiments and <span class="hlt">Mission</span> Scenarios</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sanders, Gerald B.</p> <p>2010-01-01</p> <p>The extraction and use of resources on the Moon, known as In-Situ Resource Utilization (ISRU), can potentially reduce the cost and risk of human lunar exploration while also increasing science achieved. By not having to bring all of the shielding and <span class="hlt">mission</span> consumables from Earth and being able to make products on the Moon, <span class="hlt">missions</span> may require less mass to accomplish the same objectives, carry more science equipment, go to more sites of exploration, and/or provide options to recover from failures not possible with delivery of spares and consumables from Earth alone. The concept of lunar ISRU has been considered and studied for decades, and scientists and engineers were theorizing and even testing concepts for how to extract oxygen from lunar soil even before the Apollo 11 <span class="hlt">mission</span> to the Moon. There are four main areas where ISRU can significantly impact how human <span class="hlt">missions</span> to the Moon will be performed: <span class="hlt">mission</span> consumable production, civil engineering and construction, energy production, storage, and transfer, and manufacturing and repair. The area that has the greatest impact on <span class="hlt">mission</span> mass, hardware design and selection, and <span class="hlt">mission</span> architecture is <span class="hlt">mission</span> consumable production, in particular, the ability to make propellants, <span class="hlt">life</span> support consumables, and fuel cell reagents. <span class="hlt">Mission</span> consumable production allows for refueling and reuse of spacecraft, increasing power production and storage, and increased capabilities and failure tolerance for crew <span class="hlt">life</span> support. The other three areas allow for decreased <span class="hlt">mission</span> risk due to radiation and plume damage, alternative power systems, and failure recover capabilities while also enabling infrastructure growth over Earth delivered assets. However, while lunar ISRU has significant potential for mass, cost, and risk reduction for human lunar <span class="hlt">missions</span>, it has never been demonstrated before in space. To demonstrate that ISRU can meet <span class="hlt">mission</span> needs and to increase confidence in incorporating ISRU capabilities into <span class="hlt">mission</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910007724','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910007724"><span>Operational efficiency subpanel advanced <span class="hlt">mission</span> control</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Friedland, Peter</p> <p>1990-01-01</p> <p>Herein, the term <span class="hlt">mission</span> control will be taken quite broadly to include both ground and space based operations as well as the information infrastructure necessary to support such operations. Three major technology areas related to advanced <span class="hlt">mission</span> control are examined: (1) Intelligent Assistance for Ground-Based <span class="hlt">Mission</span> Controllers and Space-Based Crews; (2) Autonomous Onboard Monitoring, Control and Fault Detection Isolation and Reconfiguration; and (3) Dynamic Corporate Memory Acquired, Maintained, and Utilized During the Entire Vehicle <span class="hlt">Life</span> Cycle. The current state of the art space operations are surveyed both within NASA and externally for each of the three technology areas and major objectives are discussed from a user point of view for technology development. Ongoing NASA and other governmental programs are described. An analysis of major research issues and current holes in the program are provided. Several recommendations are presented for enhancing the technology development and insertion process to create advanced <span class="hlt">mission</span> control environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130010920','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130010920"><span>Assessing Habitability: Lessons from the Phoenix <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stoker, Carol R.</p> <p>2013-01-01</p> <p>The Phoenix <span class="hlt">mission</span>'s key objective was to search for a habitable zone. The Phoenix lander carried a robotic arm with digging scoop to collect soil and icy material for analysis with an instrument payload that included volatile mineral and organic analysis(3) and soil ionic chemistry analysis (4). Results from Phoenix along with theoretical modeling and other previous <span class="hlt">mission</span> results were used to evaluate the habitability of the landing site by considering four factors that characterize the environments ability to support <span class="hlt">life</span> as we know it: the presence of liquid water, the presence of an energy source to support metabolism, the presence of nutrients containing the fundamental building blocks of <span class="hlt">life</span>, and the absence of environmental conditions that are toxic to or preclude <span class="hlt">life</span>. Phoenix observational evidence for the presence of liquid water (past or present) includes clean segregated ice, chemical etching of soil grains, calcite minerals in the soil and variable concentrations of soluble salts5. The maximum surface temperature measured was 260K so unfrozen water can form only in adsorbed films or saline brines but warmer climates occur cyclically on geologically short time scales due to variations in orbital parameters. During high obliquity periods, temperatures allowing metabolism extend nearly a meter into the subsurface. Phoenix discovered 1%w/w perchlorate salt in the soil, a chemical energy source utilized by a wide range of microbes. Nutrient sources including C, H, N, O, P and S compounds are supplied by known atmospheric sources or global dust. Environmental conditions are within growth tolerance for terrestrial microbes. Summer daytime temperatures are sufficient for metabolic activity, the pH is 7.8 and is well buffered and the projected water activity of a wet soil will allow growth. In summary, martian permafrost in the north polar region is a viable location for modern <span class="hlt">life</span>. Stoker et al. presented a formalism for comparing the habitability of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940029027','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940029027"><span>Planetary protection issues and future Mars <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Devincenzi, D. L.; Klein, H. P.; Bagby, J. R.</p> <p>1991-01-01</p> <p>A primary scientific theme for the Space Exploration Initiative (SEI) is the search for <span class="hlt">life</span>, extant or extinct, on Mars. Because of this, concerns have arisen about Planetary Protection (PP), the prevention of biological cross-contamination between Earth and other planets during solar system exploration <span class="hlt">missions</span>. A recent workshop assessed the necessity for, and impact of, PP requirements on the unmanned and human <span class="hlt">missions</span> to Mars comprising the SEI. The following ground-rules were adopted: (1) Information needed for assessing PP issues must be obtained during the unmanned precursor <span class="hlt">mission</span> phase prior to human landings. (2) Returned Mars samples will be considered biologically hazardous until proven otherwise. (3) Deposition of microbes on Mars and exposure of the crew to martian materials are inevitable when humans land. And (4) Human landings are unlikely until it is demonstrated that there is no harmful effect of martian materials on terrestrial <span class="hlt">life</span> forms. These ground-rules dictated the development of a conservative PP strategy for precursor <span class="hlt">missions</span>. Key features of the proposed strategy include: to prevent forward-contamination, all orbiters will follow Mars Observer PP procedures for assembly, trajectory, and lifetime. All landers will follow Viking PP procedures for assembly, microbial load reduction, and bio-shield. And, to prevent back-contamination, all sample return <span class="hlt">missions</span> will have PP requirements which include fail-safe sample sealing, breaking contact chain with the martian surface, and containment and quarantine analysis in Earth-based laboratory. In addition to deliberating on scientific and technical issues, the workshop made several recommendations for dealing with forward and back-contamination concerns from non-scicntific perspectives.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070030241','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070030241"><span><span class="hlt">Life</span> Support System Technologies for NASA Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ewert, Michael K.</p> <p>2007-01-01</p> <p>The Lunar Mars <span class="hlt">Life</span> Support Test series successfully demonstrated integration and operation of advanced technologies for closed-loop <span class="hlt">life</span> support systems, including physicochemical and biological subsystems. Increased closure was obtained when targeted technologies, such as brine dewatering subsystems, were added to further process <span class="hlt">life</span> support system byproducts to recover resources. Physicochemical and biological systems can be integrated satisfactorily to achieve desired levels of closure. Imbalances between system components, such as differences in metabolic quotients between human crews and plants, must be addressed. Each subsystem or component that is added to increase closure will likely have added costs, ranging from initial launch mass, power, thermal, crew time, byproducts, etc., that must be factored into break even analysis. Achieving <span class="hlt">life</span> support system closure while maintaining control of total mass and system complexity will be a challenge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150019532','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150019532"><span>Water Recovery System Design to Accommodate Dormant Periods for Manned <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tabb, David; Carter, Layne</p> <p>2015-01-01</p> <p>Future manned <span class="hlt">missions</span> beyond lower Earth orbit may include intermittent periods of extended dormancy. Under the NASA Advanced Exploration System (AES) project, NASA personnel evaluated the viability of the ISS Water Recovery System (WRS) to support such a <span class="hlt">mission</span>. The <span class="hlt">mission</span> requirement includes the capability for <span class="hlt">life</span> support systems to support crew activity, followed by a dormant period of up to one year, and subsequently for the <span class="hlt">life</span> support systems to come back online for additional crewed <span class="hlt">missions</span>. Dormancy could be a critical issue due to concerns with microbial growth or chemical degradation that might prevent water systems from operating properly when the crewed <span class="hlt">mission</span> began. As such, it is critical that the water systems be designed to accommodate this dormant period. This paper details the results of this evaluation, which include identification of dormancy issues, results of testing performed to assess microbial stability of pretreated urine during dormancy periods, and concepts for updating to the WRS architecture and operational concepts that will enable the ISS WRS to support the dormancy requirement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080010623','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080010623"><span>Thermostable Shelf <span class="hlt">Life</span> Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perchonok, M. H.; Antonini, D. K.</p> <p>2008-01-01</p> <p>The objective of this project is to determine the shelf <span class="hlt">life</span> end-point of various food items by means of actual measurement or mathematical projection. The primary goal of the Advanced Food Technology Project in these long duration exploratory <span class="hlt">missions</span> is to provide the crew with a palatable, nutritious and safe food system while minimizing volume, mass, and waste. The Mars <span class="hlt">missions</span> could be as long as 2.5 years with the potential of the food being positioned prior to the crew arrival. Therefore, it is anticipated that foods that are used during the Mars <span class="hlt">missions</span> will require a 5 year shelf <span class="hlt">life</span>. Shelf <span class="hlt">life</span> criteria are safety, nutrition, and acceptability. Any of these criteria can be the limiting factor in determining the food's shelf <span class="hlt">life</span>. Due to the heat sterilization process used for the thermostabilized food items, safety will be preserved as long as the integrity of the package is maintained. Nutrition and acceptability will change over time. Since the food can be the sole source of nutrition to the crew, a significant loss in nutrition may determine when the shelf <span class="hlt">life</span> endpoint has occurred. Shelf <span class="hlt">life</span> can be defined when the food item is no longer acceptable. Acceptability can be defined in terms of appearance, flavor, texture, or aroma. Results from shelf <span class="hlt">life</span> studies of the thermostabilized food items suggest that the shelf <span class="hlt">life</span> of the foods range from 0 months to 8 years, depending on formulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20090006887','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20090006887"><span>Thermostabilized Shelf <span class="hlt">Life</span> Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perchonok, Michele H.; Catauro, Patricia M.</p> <p>2009-01-01</p> <p>The objective of this project is to determine the shelf <span class="hlt">life</span> end-point of various food items by means of actual measurement or mathematical projection. The primary goal of the Advanced Food Technology Project in these long duration exploratory <span class="hlt">missions</span> is to provide the crew with a palatable, nutritious and safe food system while minimizing volume, mass, and waste. The Mars <span class="hlt">missions</span> could be as long as 2.5 years with the potential of the food being positioned prior to the crew arrival. Therefore, it is anticipated that foods that are used during the Mars <span class="hlt">missions</span> will require a 5 year shelf <span class="hlt">life</span>. Shelf <span class="hlt">life</span> criteria are safety, nutrition, and acceptability. Any of these criteria can be the limiting factor in determining the food's shelf <span class="hlt">life</span>. Due to the heat sterilization process used for the thermostabilized food items, safety will be preserved as long as the integrity of the package is maintained. Nutrition and acceptability will change over time. Since the food can be the sole source of nutrition to the crew, a significant loss in nutrition may determine when the shelf <span class="hlt">life</span> endpoint has occurred. Shelf <span class="hlt">life</span> can be defined when the food item is no longer acceptable. Acceptability can be defined in terms of appearance, flavor, texture, or aroma. Results from shelf <span class="hlt">life</span> studies of the thermostabilized food items suggest that the shelf <span class="hlt">life</span> of the foods range from 0 months to 8 years, depending on formulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160008917','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160008917"><span>Terra <span class="hlt">Mission</span> Operations: Launch to the Present (and Beyond)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kelly, Angelita; Moyer, Eric; Mantziaras, Dimitrios; Case, Warren</p> <p>2014-01-01</p> <p>The Terra satellite, flagship of NASA's long-term Earth Observing System (EOS) Program, continues to provide useful earth science observations well past its 5-year design lifetime. This paper describes the evolution of Terra operations, including challenges and successes and the steps taken to preserve science requirements and prolong spacecraft <span class="hlt">life</span>. Working cooperatively with the Terra science and instrument teams, including NASA's international partners, the <span class="hlt">mission</span> operations team has successfully kept the Terra operating continuously, resolving challenges and adjusting operations as needed. Terra retains all of its observing capabilities (except Short Wave Infrared) despite its age. The paper also describes concepts for future operations. This paper will review the Terra spacecraft <span class="hlt">mission</span> successes and unique spacecraft component designs that provided significant benefits extending <span class="hlt">mission</span> <span class="hlt">life</span> and science. In addition, it discusses special activities as well as anomalies and corresponding recovery efforts. Lastly, it discusses future plans for continued operations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920032159&hterms=Professional+choice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DProfessional%2Bchoice','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920032159&hterms=Professional+choice&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DProfessional%2Bchoice"><span>A <span class="hlt">mission</span> design for International Manned Mars <span class="hlt">Mission</span> - From the 1991 International Space University (ISU) Design Project</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mendell, Wendell W.</p> <p>1991-01-01</p> <p>The International Space University (ISU) conducted a study of an international program to support human exploration of Mars as its annual Design Project activity during its 1991 summer session in Toulouse, France. Although an ISU Design Project strives to produce an in-depth analysis during the intense 10-week summer session, the International Mars <span class="hlt">Mission</span> (IMM) project was conducted in a manner designed to provide a learning experience for young professionals working in an unusual multidisciplinary and multinational environment. The breadth of the IMM study exceeds that of most Mars <span class="hlt">mission</span> studies of the past, encompassing political organization for long-term commitment, multinational management structure, cost analysis, <span class="hlt">mission</span> architecture, vehicle configuration, crew health, <span class="hlt">life</span> support, Mars surface infrastructure, <span class="hlt">mission</span> operations, technology evaluation, risk assessment, scientific planning, exploration, communication networks, and Martian resource utilization. The IMM Final Report has particular value for those seeking insight into the choices made by a multinational group working in an apolitical environment on the problems of international cooperation in space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150008892&hterms=life+mars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dlife%2Bmars','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150008892&hterms=life+mars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dlife%2Bmars"><span>Environmental Monitoring as Part of <span class="hlt">Life</span> Support for the Crew Habitat for Lunar and Mars <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jan, Darrell L.</p> <p>2010-01-01</p> <p>Like other crewed space <span class="hlt">missions</span>, future <span class="hlt">missions</span> to the moon and Mars will have requirements for monitoring the chemical and microbial status of the crew habitat. Monitoring the crew habitat becomes more critical in such long term <span class="hlt">missions</span>. This paper will describe the state of technology development for environmental monitoring of lunar lander and lunar outpost <span class="hlt">missions</span>, and the state of plans for future <span class="hlt">missions</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830007769','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830007769"><span>Controlled ecological <span class="hlt">life</span> support system: Transportation analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gustan, E.; Vinopal, T.</p> <p>1982-01-01</p> <p>This report discusses a study utilizing a systems analysis approach to determine which NASA <span class="hlt">missions</span> would benefit from controlled ecological <span class="hlt">life</span> support system (CELSS) technology. The study focuses on manned <span class="hlt">missions</span> selected from NASA planning forecasts covering the next half century. Comparison of various <span class="hlt">life</span> support scenarios for the selected <span class="hlt">missions</span> and characteristics of projected transportation systems provided data for cost evaluations. This approach identified <span class="hlt">missions</span> that derived benefits from a CELSS, showed the magnitude of the potential cost savings, and indicated which system or combination of systems would apply. This report outlines the analytical approach used in the evaluation, describes the <span class="hlt">missions</span> and systems considered, and sets forth the benefits derived from CELSS when applicable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS12B..03J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS12B..03J"><span>Scientific Discoveries in the Central Arctic Ocean Based on Seafloor Mapping Carried out to Support Article 76 Extended Continental Shelf Claims (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jakobsson, M.; Mayer, L. A.; Marcussen, C.</p> <p>2013-12-01</p> <p>Despite the last decades of diminishing sea-ice cover in the Arctic Ocean, ship operations are only possible in vast sectors of the central Arctic using the most capable polar-class <span class="hlt">icebreakers</span>. There are less than a handful of these <span class="hlt">icebreakers</span> outfitted with modern seafloor mapping equipment. This implies either fierce competition between those having an interest in using these <span class="hlt">icebreakers</span> for investigations of the shape and properties of Arctic Ocean seafloor or, preferably, collaboration. In this presentation examples will be shown of scientific discoveries based on mapping data collected during Arctic Ocean <span class="hlt">icebreaker</span> expeditions carried out for the purpose of substantiating claims for an extended continental shelf under United Nations Convention of the Law of the Sea (UNCLOS) Article 76. Scientific results will be presented from the suite of Lomonosov Ridge off Greenland (LOMROG) expeditions (2007, 2009, and 2012), shedding new light on Arctic Ocean oceanography and glacial history. The Swedish <span class="hlt">icebreaker</span> Oden was used in collaboration between Sweden and Denmark during LOMROG to map and sample portions of the central Arctic Ocean; specifically focused on the Lomonosov Ridge north of Greenland. While the main objective of the Danish participation was seafloor and sub-seabed mapping to substantiate their Article 76 claim, LOMROG also included several scientific components, with scientists from both countries involved. Other examples to be presented are based on data collected using US Coast Guard Cutter Healy, which for several years has carried out mapping in the western Arctic Ocean for the US continental shelf program. All bathymetric data collected with Oden and Healy have been contributed to the International Bathymetric Chart of the Arctic Ocean (IBCAO). This is also the case for bathymetric data collected by Canadian Coast Guard Ship Louis S. St-Laurent for Canada's extended continental shelf claim. Together, the bathymetric data collected during these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018LSSR...17....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018LSSR...17....1M"><span>A urine-fuelled soil-based bioregenerative <span class="hlt">life</span> support system for long-term and long-distance manned space <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maggi, Federico; Tang, Fiona H. M.; Pallud, Céline; Gu, Chuanhui</p> <p>2018-05-01</p> <p>A soil-based cropping unit fuelled with human urine for long-term manned space <span class="hlt">missions</span> was investigated with the aim to analyze whether a closed-loop nutrient cycle from human liquid wastes was achievable. Its ecohydrology and biogeochemistry were analysed in microgravity with the use of an advanced computational tool. Urine from the crew was used to supply primary (N, P, and K) and secondary (S, Ca and Mg) nutrients to wheat and soybean plants in the controlled cropping unit. Breakdown of urine compounds into primary and secondary nutrients as well as byproduct gases, adsorbed, and uptake fractions were tracked over a period of 20 years. Results suggested that human urine could satisfy the demand of at least 3 to 4 out of 6 nutrients with an offset in pH and salinity tolerable by plants. It was therefore inferred that a urine-fuelled <span class="hlt">life</span> support system can introduce a number of advantages including: (1) recycling of liquids wastes and production of food; (2) forgiveness of neglect as compared to engineered electro-mechanical systems that may fail under unexpected or unplanned conditions; and (3) reduction of supply and waste loads during space <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16379531','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16379531"><span>Venus, Mars, and the ices on Mercury and the moon: astrobiological implications and proposed <span class="hlt">mission</span> designs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schulze-Makuch, Dirk; Dohm, James M; Fairén, Alberto G; Baker, Victor R; Fink, Wolfgang; Strom, Robert G</p> <p>2005-12-01</p> <p>Venus and Mars likely had liquid water bodies on their surface early in the Solar System history. The surfaces of Venus and Mars are presently not a suitable habitat for <span class="hlt">life</span>, but reservoirs of liquid water remain in the atmosphere of Venus and the subsurface of Mars, and with it also the possibility of microbial <span class="hlt">life</span>. Microbial organisms may have adapted to live in these ecological niches by the evolutionary force of directional selection. <span class="hlt">Missions</span> to our neighboring planets should therefore be planned to explore these potentially <span class="hlt">life</span>-containing refuges and return samples for analysis. Sample return <span class="hlt">missions</span> should also include ice samples from Mercury and the Moon, which may contain information about the biogenic material that catalyzed the early evolution of <span class="hlt">life</span> on Earth (or elsewhere). To obtain such information, science-driven exploration is necessary through varying degrees of <span class="hlt">mission</span> operation autonomy. A hierarchical <span class="hlt">mission</span> design is envisioned that includes spaceborne (orbital), atmosphere (airborne), surface (mobile such as rover and stationary such as lander or sensor), and subsurface (e.g., ground-penetrating radar, drilling, etc.) agents working in concert to allow for sufficient <span class="hlt">mission</span> safety and redundancy, to perform extensive and challenging reconnaissance, and to lead to a thorough search for evidence of <span class="hlt">life</span> and habitability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120007779','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120007779"><span>Human Exploration <span class="hlt">Missions</span> - Maturing Technologies to Sustain Crews</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mukai, Chiaki; Koch, Bernhard; Reese, Terrence G.</p> <p>2012-01-01</p> <p>Human exploration <span class="hlt">missions</span> beyond low earth orbit will be long duration with abort scenarios of days to months. Providing crews with the essentials of <span class="hlt">life</span> such as clean air and potable water means recycling human metabolic wastes back to useful products. Individual technologies are under development for such things as CO2 scrubbing, recovery of O2 from CO2, turning waste water into potable water, and so on. But in order to fully evaluate and mature technologies fully they must be tested in a relevant, high-functionality environment; a systems environment where technologies are challenged with real human metabolic wastes. It is for this purpose that an integrated systems ground testing capability at the Johnson Space Center is being readied for testing. The relevant environment will include deep space habitat human accommodations, sealed atmosphere of 8 psi total pressure and 32% oxygen concentration, <span class="hlt">life</span> support systems (food, air, water), communications, crew accommodations, medical, EVA, tools, etc. Testing periods will approximate those of the expected <span class="hlt">missions</span> (such as a near Earth asteroid, Earth ]Moon L2 or L1, the moon, and Mars). This type of integrated testing is needed not only for research and technology development but later during the <span class="hlt">mission</span> design, development, test, and evaluation phases of preparing for the <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5369257','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5369257"><span>Cost-effectiveness of short-term neurosurgical <span class="hlt">missions</span> relative to other surgical specialties</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Punchak, Maria; Lazareff, Jorge A.</p> <p>2017-01-01</p> <p>Background: Short-term surgical relief efforts have helped close some gaps in the provision of surgical care in remote settings. We reviewed the published literature on short-term surgical <span class="hlt">missions</span> to compare their cost-effectiveness across subspecialties. Methods: PubMed was searched using the algorithm [“cost-effectiveness” AND “surgery” AND (“mission” OR “volunteer”)]. Articles detailing the cost-effectiveness of short-term surgical <span class="hlt">missions</span> in low and middle-income countries (LMIC) were included. Only direct <span class="hlt">mission</span> costs were considered, and all costs were converted into 2014 USD. Results: Eight articles, representing 27 <span class="hlt">missions</span> in 9 LMIC countries during 2006–2014, met our inclusion criteria. Latin America was the most frequently visited region. Per capita costs ranged from $259 for cleft lip/cleft palate (CL/CP) <span class="hlt">missions</span> to $2900 for a neurosurgery <span class="hlt">mission</span>. <span class="hlt">Mission</span> effectiveness ranged from 3 disability adjusted <span class="hlt">life</span> years (DALYs) averted per patient for orthopedic surgery <span class="hlt">missions</span> to 8.12 DALYs averted per patient for a neurosurgery <span class="hlt">mission</span>. CL/CP and general surgery <span class="hlt">missions</span> were the most cost-effective, averaging $80/DALY and $87/DALY, respectively. The neurosurgical, orthopedic, and hand surgery <span class="hlt">missions</span> averaged the highest costs/DALY averted, with the cost-effectiveness being $357/DALY, $435/DALY, and $445/DALY, respectively. All analyzed <span class="hlt">missions</span> were very cost effective. Conclusion: To date, this is the first study to assess the cost-effectiveness of short-term surgical <span class="hlt">missions</span> across surgical specialties. Neurosurgical <span class="hlt">missions</span> avert the largest number of healthy <span class="hlt">life</span> years compared to other specialties, and thus, could yield a greater long-term benefit to resource-poor communities. We recommend that further studies be carried out to assess the impact of surgical <span class="hlt">missions</span> in low-resource settings. PMID:28458951</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-9606423&hterms=friendship&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dfriendship','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-9606423&hterms=friendship&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dfriendship"><span>STS-78 <span class="hlt">Mission</span> Insignia</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1996-01-01</p> <p>The STS-78 patch links past with present to tell the story of its <span class="hlt">mission</span> and science through a design imbued with the strength and vitality of the 2-dimensional art of North America's northwest coast Indians. Central to the design is the space Shuttle whose bold lines and curves evoke the Indian image for the eagle, a native American symbol of power and prestige as well as the national symbol of the United States. The wings of the Shuttle suggest the wings of the eagle whose feathers, indicative of peace and friendship in Indian tradition, are captured by the U forms, a characteristic feature of Northwest coast Indian art. The nose of the Shuttle is the strong downward curve of the eagle's beak, and the Shuttle's forward windows, the eagle's eyes, represented through the tapered S forms again typical of this Indian art form. The basic black and red atoms orbiting the <span class="hlt">mission</span> number recall the original NASA emblem while beneath, utilizing Indian ovoid forms, the major <span class="hlt">mission</span> scientific experiment package LMS (<span class="hlt">Life</span> and Materials Sciences) housed in the Shuttle's cargo bay is depicted in a manner reminiscent of totem-pole art. This image of a bird poised for flight, so common to Indian art, is counterpointed by an equally familiar Tsimshian Indian symbol, a pulsating sun with long hyperbolic rays, the symbol of <span class="hlt">life</span>. Within each of these rays are now encased crystals, the products of this <span class="hlt">mission</span>'s 3 major, high-temperature materials processing furnaces. And as the sky in Indian lore is a lovely open country, home of the Sun Chief and accessible to travelers through a hole in the western horizon, so too, space is a vast and beckoning landscape for explorers launched beyond the horizon. Beneath the Tsimshian sun, the colors of the earth limb are appropriately enclosed by a red border representing <span class="hlt">life</span> to the Northwest coast Indians. The Indian colors of red, navy blue, white, and black pervade the STS-78 path. To the right of the Shuttle-eagle, the constellation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA564217','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA564217"><span>Technical Report on DOMICE Simulation Model</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-04-01</p> <p>Branch GPS Global Positioning System HHO home heating oil LCA Lake Carriers’ Association MAR USCG Domestic <span class="hlt">Icebreaking</span> <span class="hlt">Mission</span> Analysis...cargo types considered in the module. The module groups the four types of cargo into two broader categories, namely, Home Heating Oil ( HHO ) shipments...or Non- HHO shipments. Table 11. Cargo types. Types of Cargo Cargo Group Dry Bulk Non- HHO Liquid Bulk Perishable / Food Home Heating Oil HHO</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070030191','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070030191"><span>Future Opportunities for Dynamic Power Systems for NASA <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shaltens, Richard K.</p> <p>2007-01-01</p> <p>Dynamic power systems have the potential to be used in Radioisotope Power Systems (RPS) and Fission Surface Power Systems (FSPS) to provide high efficiency, reliable and long <span class="hlt">life</span> power generation for future NASA applications and <span class="hlt">missions</span>. Dynamic power systems have been developed by NASA over the decades, but none have ever operated in space. Advanced Stirling convertors are currently being developed at the NASA Glenn Research Center. These systems have demonstrated high efficiencies to enable high system specific power (>8 W(sub e)/kg) for 100 W(sub e) class Advanced Stirling Radioisotope Generators (ASRG). The ASRG could enable significant extended and expanded operation on the Mars surface and on long-<span class="hlt">life</span> deep space <span class="hlt">missions</span>. In addition, advanced high power Stirling convertors (>150 W(sub e)/kg), for use with surface fission power systems, could provide power ranging from 30 to 50 kWe, and would be enabling for both lunar and Mars exploration. This paper will discuss the status of various energy conversion options currently under development by NASA Glenn for the Radioisotope Power System Program for NASA s Science <span class="hlt">Mission</span> Directorate (SMD) and the Prometheus Program for the Exploration Systems <span class="hlt">Mission</span> Directorate (ESMD).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006epsc.conf...76V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006epsc.conf...76V"><span>Science objectives of ESA's ExoMars <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vago, J. L.; Gardini, B.; Baglioni, P.; Kminek, G.; Gianfiglio, G.; Exomars Project Team</p> <p></p> <p>ExoMars will deliver two science elements to the Martian surface: a Rover, carrying the Pasteur scientific payload; and a small, fixed surface station -the Geophysics & Environment Package (GEP). The ExoMars <span class="hlt">mission</span>'s scientific objectives are: 1) To search for signs of past and present <span class="hlt">life</span> on Mars; 2) To characterise the water/geochemical environment as a function of depth in the shallow subsurface; 3) To study the surface environment and identify hazards to future human <span class="hlt">missions</span>; and 4) To investigate the planet's deep interior to better understand Mars's evolution and habitability. Over its planned 6-month lifetime, the Rover will travel a few kilometres searching for traces of past and present signs of <span class="hlt">life</span>. It will do this by collecting and analysing samples from within surface rocks, and from underground -down to 2-m depth. The very powerful combination of mobility with the capability to access locations where organic molecules may be well preserved is unique to this <span class="hlt">mission</span>. The ExoMars <span class="hlt">mission</span> contains two other elements: a Carrier and a Descent Module. The Carrier will bring the Descent Module to Mars and release it from the hyperbolic arrival trajectory. The Descent Module's objective is to safely deploy the Pasteur Rover and the GEP -developing a robust European Entry, Descent and Landing System (EDLS) is another fundamental goal of this <span class="hlt">mission</span>. The <span class="hlt">mission</span>'s data relay capability will be provided by a NASA orbiter. The Pasteur Rover's mass is presently estimated at 190 kg, including the Pasteur scientific payload. The Pasteur payload contains: Panoramic Instruments: stereoscopic cameras, a ground-penetrating radar, and an IR spectrometer; Contact Instrument for studying surface rocks: a close-up imager and a Mössbauer spectrometer; a subsurface drill capable of reaching a depth of 2 m, and also of collecting specimens from exposed bedrock; a sample preparation and distribution unit; a microscope; an oxidation sensor; and a variety of analytical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010cosp...38.3389B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010cosp...38.3389B"><span>Alisse : Advanced <span class="hlt">life</span> support system evaluator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brunet, Jean; Gerbi, Olivier; André, Philippe; Davin, Elisabeth; Avezuela Rodriguez, Raul; Carbonero, Fernando; Soumalainen, Emilia; Lasseur, Christophe</p> <p></p> <p>Long duration <span class="hlt">missions</span>, such as the establishment of permanent bases on the lunar surface or the travel to Mars, require such an amount of <span class="hlt">life</span> support consumables (e.g. food, water and oxygen) that direct supply or re-supply from Earth is not an option anymore. Regenerative <span class="hlt">Life</span> Support Systems are therefore necessary to sustain long-term manned space <span class="hlt">mission</span> to increase recycling rates and so reduce the launched mass. The architecture of an Environmental Controlled <span class="hlt">Life</span> Support System widely depends on the <span class="hlt">mission</span> scenario. Even for a given <span class="hlt">mission</span> scenario, different architectures could be envisaged which need to be evaluated and compared with appropriate tools. As these evaluation and comparison, based on the single criterion of Equivalent System Mass, was not considered com-prehensive enough, ESA is developing a multi-criteria evaluation tool: ALISSE (Advanced <span class="hlt">Life</span> Support System Evaluator). The main objective of ALISSE, and of the work presented here, is the definition and implemen-tation of a metrics system, addressing the complexity of any ECLSS along its <span class="hlt">Life</span> Cycle phases. A multi-dimensional and multi-criteria (i.e. mass, energy, efficiency, risk to human, reliability, crew time, sustainability, <span class="hlt">life</span> cycle cost) approach is proposed through the development of a computing support platform. Each criterion being interrelated with the others, a model based system approach is used. ALISSE is expected to provide significant inputs to the ESA Concurrent Design Facility and, as a consequence, to be a highly valuable tool for decision process linked to any manned space <span class="hlt">mission</span>. Full contact detail for the contact author : Jean Brunet Sherpa Engineering General Manager Phone : 0033(0)608097480 j.brunet@sherpa-eng.com</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9821E..0QR','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9821E..0QR"><span>Overview of RICOR tactical cryogenic refrigerators for space <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riabzev, Sergey; Filis, Avishai; Livni, Dorit; Regev, Itai; Segal, Victor; Gover, Dan</p> <p>2016-05-01</p> <p>Cryogenic refrigerators represent a significant enabling technology for Earth and Space science enterprises. Many of the space instruments require cryogenic refrigeration to enable the use of advanced detectors to explore a wide range of phenomena from space. RICOR refrigerators involved in various space <span class="hlt">missions</span> are overviewed in this paper, starting in 1994 with "Clementine" Moon <span class="hlt">mission</span>, till the latest ExoMars <span class="hlt">mission</span> launched in 2016. RICOR tactical rotary refrigerators have been incorporated in many space instruments, after passing qualification, <span class="hlt">life</span> time, thermal management testing and flight acceptance. The tactical to space customization framework includes an extensive characterization and qualification test program to validate reliability, the design of thermal interfacing with a detector, vibration export control, efficient heat dissipation in a vacuum environment, robustness, mounting design, compliance with outgassing requirements and strict performance screening. Current RICOR development is focused on dedicated ultra-long-<span class="hlt">life</span>, highly reliable, space cryogenic refrigerator based on a Pulse Tube design</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170012500','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170012500"><span>Raman <span class="hlt">Life</span> Detection Instrument Development for Icy Worlds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thomson, Seamus; Allen, A'Lester; Gutierrez, Daniel; Quinn, Richard C.; Chen, Bin; Koehne, Jessica E.</p> <p>2017-01-01</p> <p>The objective of this project is to develop a compact, high sensitivity Raman sensor for detection of <span class="hlt">life</span> signatures in a flow cell configuration to enable bio-exploration and <span class="hlt">life</span> detection during future <span class="hlt">mission</span> to our Solar Systems Icy Worlds. The specific project objectives are the following: 1) Develop a Raman spectroscopy liquid analysis sensor for biosignatures; 2) Demonstrate applicability towards a future Enceladus or other Icy Worlds <span class="hlt">missions</span>; 3) Establish key parameters for integration with the ARC Sample Processor for <span class="hlt">Life</span> on Icy Worlds (SPLIce); 4) Position ARC for a successful response to upcoming Enceladus or other Icy World <span class="hlt">mission</span> instrument opportunities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.P24A..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.P24A..01M"><span>The Mars 2020 <span class="hlt">Mission</span>: The Next Step Forward in Mars Exploration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meyer, M. A.; Schulte, M. D.</p> <p>2014-12-01</p> <p>The next rover <span class="hlt">mission</span> to Mars represents the culmination of almost two decades of strategic <span class="hlt">missions</span> in the exploration of Mars. Our understanding of the Red Planet has evolved from a global frozen desert to a dynamic world that once was warmer, wetter, and could have supported microbial <span class="hlt">life</span>, and the series of <span class="hlt">missions</span> reflect this evolution, moving from global reconnaissance to seeking the signs of <span class="hlt">life</span>. The 2020 rover will be outfitted with seven sophisticated payload elements to conduct remote sensing and contact science, demonstrate exploration technology, and cache samples for potential return to Earth. The <span class="hlt">mission</span>'s capabilities exceed the threshold <span class="hlt">mission</span> detailed in the Mars 2020 Science Definition Team 2013 report1 and meets the NRC's 2011 Decadal Survey's requirements for the highest priority <span class="hlt">mission</span> of NASA's Planetary Science2. The instruments selected July 31, 2014, are able to determine elemental composition and mineralogy and detect organic compounds across spatial scales of meters to 100's of micrometers. The instrument suite includes a combination of a zooming, binocular, multi-spectral camera; a telescopic imager; two Raman spectrometers with different wavelength lasers (UV and Green); a visible/near-infrared spectrometer; a Laser-Induced Breakdown Spectrometer; an X-ray fluorescence spectrometer, a microscopic imager, and ground-penetrating radar. Their purpose is to enable the science team to establish the geological context of the landing site area, to assess whether past or present environments could support microbial <span class="hlt">life</span>, to search for potential biosignatures, and to use this information to identify samples for caching. To prepare for future human exploration, the payload includes the ability for in situ resource utilization, converting CO2 to O2, the ability to assess physical characteristics of the dust, and environmental monitoring of the temperature, pressure, humidity, wind, and radiation. The Mars 2020 <span class="hlt">mission</span> will pave a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19750041961&hterms=Biomedicine&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBiomedicine','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19750041961&hterms=Biomedicine&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DBiomedicine"><span><span class="hlt">Life</span> sciences payloads for Shuttle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dunning, R. W.</p> <p>1974-01-01</p> <p>The <span class="hlt">Life</span> Sciences Program for utilization of the Shuttle in the 1980's is presented. Requirements for <span class="hlt">life</span> sciences research experiments in space flight are discussed along with study results of designs to meet these requirements. The span of <span class="hlt">life</span> sciences interests in biomedicine, biology, man system integration, bioinstrumentation and <span class="hlt">life</span> support/protective systems is described with a listing of the research areas encompassed in these descriptions. This is followed by a description of the approach used to derive from the <span class="hlt">life</span> sciences disciplines, the research functions and instrumentation required for an orbital research program. Space Shuttle design options for <span class="hlt">life</span> sciences experiments are identified and described. Details are presented for Spacelab laboratories for dedicated <span class="hlt">missions</span>, mini-labs with carry on characteristics and carry on experiments for shared payload <span class="hlt">missions</span> and free flying satellites to be deployed and retrieved by the Shuttle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25999079','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25999079"><span>Thinking of serving nursing abroad: how technology assists nurses on <span class="hlt">mission</span> trips.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brown, Rachel M</p> <p>2015-06-01</p> <p>Advances in technology have assisted in the proliferation of short-term, faith-based international medical <span class="hlt">mission</span> trips. Many of these <span class="hlt">mission</span> trips include health care not only to local citizens but also building schools and churches and sharing the Gospel of Jesus Christ. Included in this article are my own personal experiences in short-term, faith-based medical <span class="hlt">missions</span>. A step-by-step guide is offered to help prepare inexperienced <span class="hlt">mission</span> participants gain insight into short-term <span class="hlt">mission</span> trips. Advanced planning, fundraising, collaboration, and being open to change are key elements to successful participation in these <span class="hlt">life</span>-changing <span class="hlt">missions</span>. Copyright © 2015 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030053087&hterms=planets+orbit+sun&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DWhy%2Bplanets%2Borbit%2Bsun','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030053087&hterms=planets+orbit+sun&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DWhy%2Bplanets%2Borbit%2Bsun"><span>Kepler <span class="hlt">Mission</span> to Detect Earth-like Planets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kondo, Yoji</p> <p>2003-01-01</p> <p>Kepler <span class="hlt">Mission</span> to detect Earth-like planets in our Milky Way galaxy was approved by NASA in December 2001 for a 4-5 year <span class="hlt">mission</span>. The launch is planned in about 5 years. The Kepler observatory will be placed in an Earth-trailing orbit. The unique feature of the Kepler <span class="hlt">Mission</span> is its ability to detect Earth-like planets orbiting around solar-type stars at a distance similar to that of Earth (from our Sun); such an orbit could provide an environment suitable for supporting <span class="hlt">life</span> as we know it. The Kepler observatory accomplishes this feat by looking for the transits of planetary object in front of their suns; Kepler has a photometric precision of 10E-5 (0.00001) to achieve such detections. Other ongoing planetary detection programs (based mostly on a technique that looks for the shifting of spectral lines of the primary star due to its planetary companions' motions around it) have detected massive planets (with masses in the range of Jupiter); such massive planets are not considered suitable for supporting <span class="hlt">life</span>. If our current theories for the formation of planetary systems are valid, we expect to detect about 50 Earth-like planets during Kepler's 4-year <span class="hlt">mission</span> (assuming a random distribution of the planetary orbital inclinations with respect to the line of sight from Kepler). The number of detection will increase about 640 planets if the planets to be detected are Jupiter-sized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040034187&hterms=planets+orbit+sun&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DWhy%2Bplanets%2Borbit%2Bsun','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040034187&hterms=planets+orbit+sun&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DWhy%2Bplanets%2Borbit%2Bsun"><span>Kepler <span class="hlt">Mission</span> to Detect Earth-like Planets</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kondo, Yoji</p> <p>2002-01-01</p> <p>Kepler <span class="hlt">Mission</span> to detect Earth-like planets in our Milky Way galaxy was approved by NASA in December 2001 for a 4-5 year <span class="hlt">mission</span>. The launch is planned in about 5 years. The Kepler observatory will be placed in an Earth-trailing orbit. The unique feature of the Kepler <span class="hlt">Mission</span> is its ability to detect Earth-like planets orbiting around solar-type stars at a distance similar to that of Earth (from our Sun); such an orbit could provide an environment suitable for supporting <span class="hlt">life</span> as we know it. The Kepler observatory accomplishes this feat by looking for the transits of planetary object in front of their suns; Kepler has a photometric precision of 10E-5 (0.00001) to achieve such detections. Other ongoing planetary detection programs (based mostly on a technique that looks for the shifting of spectral lines of the primary star due to its planetary companions' motions around it) have detected massive planets (with masses in the range of Jupiter); such massive planets are not considered suitable for supporting <span class="hlt">life</span>. If our current theories for the formation of planetary systems are valid, we expect to detect about 50 Earth-like planets during Kepler's 4-year <span class="hlt">mission</span> (assuming a random distribution of the planetary orbital inclinations with respect to the line of sight from Kepler). The number of detection will increase about 640 planets if the planets to be detected are Jupiter-sized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060022163&hterms=microbiology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmicrobiology','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060022163&hterms=microbiology&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dmicrobiology"><span>Planned Environmental Microbiology Aspects of Future Lunar and Mars <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ott, C. Mark; Castro, Victoria A.; Pierson, Duane L.</p> <p>2006-01-01</p> <p>With the establishment of the Constellation Program, NASA has initiated efforts designed similar to the Apollo Program to return to the moon and subsequently travel to Mars. Early lunar sorties will take 4 crewmembers to the moon for 4 to 7 days. Later <span class="hlt">missions</span> will increase in duration up to 6 months as a lunar habitat is constructed. These <span class="hlt">missions</span> and vehicle designs are the forerunners of further <span class="hlt">missions</span> destined for human exploration of Mars. Throughout the planning and design process, lessons learned from the International Space Station (ISS) and past programs will be implemented toward future exploration goals. The standards and requirements for these <span class="hlt">missions</span> will vary depending on <span class="hlt">life</span> support systems, <span class="hlt">mission</span> duration, crew activities, and payloads. From a microbiological perspective, preventative measures will remain the primary techniques to mitigate microbial risk. Thus, most of the effort will focus on stringent preflight monitoring requirements and engineering controls designed into the vehicle, such as HEPA air filters. Due to volume constraints in the CEV, in-flight monitoring will be limited for short-duration <span class="hlt">missions</span> to the measurement of biocide concentration for water potability. Once long-duration habitation begins on the lunar surface, a more extensive environmental monitoring plan will be initiated. However, limited in-flight volume constraints and the inability to return samples to Earth will increase the need for crew capabilities in determining the nature of contamination problems and method of remediation. In addition, limited shelf <span class="hlt">life</span> of current monitoring hardware consumables and limited capabilities to dispose of biohazardous trash will drive flight hardware toward non-culture based methodologies, such as hardware that rapidly distinguishes biotic versus abiotic surface contamination. As <span class="hlt">missions</span> progress to Mars, environmental systems will depend heavily on regeneration of air and water and biological waste remediation and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060012174','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060012174"><span>Solar Electric Propulsion for Primitive Body Science <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Witzberger, Kevin E.</p> <p>2006-01-01</p> <p>This paper describes work that assesses the performance of solar electric propulsion (SEP) for three different primitive body science <span class="hlt">missions</span>: 1) Comet Rendezvous 2) Comet Surface Sample Return (CSSR), and 3) a Trojan asteroid/Centaur object Reconnaissance Flyby. Each of these <span class="hlt">missions</span> launches from Earth between 2010 and 2016. Beginning-of-<span class="hlt">life</span> (BOL) solar array power (referenced at 1 A.U.) varies from 10 to 18 kW. Launch vehicle selections range from a Delta II to a Delta IV medium-class. The primary figure of merit (FOM) is net delivered mass (NDM). This analysis considers the effects of imposing various <span class="hlt">mission</span> constraints on the Comet Rendezvous and CSSR <span class="hlt">missions</span>. Specifically, the Comet Rendezvous <span class="hlt">mission</span> analysis examines an arrival date constraint with a launch year variation, whereas the CSSR <span class="hlt">mission</span> analysis investigates an Earth entry velocity constraint commensurate with past and current <span class="hlt">missions</span>. Additionally, the CSSR <span class="hlt">mission</span> analysis establishes NASA's New Frontiers (NF) Design Reference <span class="hlt">Mission</span> (DRM) in order to evaluate current and future SEP technologies. The results show that transfer times range from 5 to 9 years (depending on the <span class="hlt">mission</span>). More importantly, the spacecraft's primary propulsion system performs an average 5-degree plane change on the return leg of the CSSR <span class="hlt">mission</span> to meet the previously mentioned Earth entry velocity constraint. Consequently, these analyses show that SEP technologies that have higher thrust-to-power ratios can: 1) reduce flight time, and 2) change planes more efficiently.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19790014955','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19790014955"><span><span class="hlt">Mission</span> specification for three generic <span class="hlt">mission</span> classes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1979-01-01</p> <p><span class="hlt">Mission</span> specifications for three generic <span class="hlt">mission</span> classes are generated to provide a baseline for definition and analysis of data acquisition platform system concepts. The <span class="hlt">mission</span> specifications define compatible groupings of sensors that satisfy specific earth resources and environmental <span class="hlt">mission</span> objectives. The driving force behind the definition of sensor groupings is <span class="hlt">mission</span> need; platform and space transportation system constraints are of secondary importance. The three generic <span class="hlt">mission</span> classes are: (1) low earth orbit sun-synchronous; (2) geosynchronous; and (3) non-sun-synchronous, nongeosynchronous. These <span class="hlt">missions</span> are chosen to provide a variety of sensor complements and implementation concepts. Each <span class="hlt">mission</span> specification relates <span class="hlt">mission</span> categories, <span class="hlt">mission</span> objectives, measured parameters, and candidate sensors to orbits and coverage, operations compatibility, and platform fleet size.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24823800','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24823800"><span>Field trial of a dual-wavelength fluorescent emission (<span class="hlt">L.I.F.E</span>.) instrument and the Magma White rover during the MARS2013 Mars analog <span class="hlt">mission</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Groemer, Gernot; Sattler, Birgit; Weisleitner, Klemens; Hunger, Lars; Kohstall, Christoph; Frisch, Albert; Józefowicz, Mateusz; Meszyński, Sebastian; Storrie-Lombardi, Michael; Bothe, Claudia; Boyd, Andrea; Dinkelaker, Aline; Dissertori, Markus; Fasching, David; Fischer, Monika; Föger, Daniel; Foresta, Luca; Frischauf, Norbert; Fritsch, Lukas; Fuchs, Harald; Gautsch, Christoph; Gerard, Stephan; Goetzloff, Linda; Gołebiowska, Izabella; Gorur, Paavan; Groemer, Gerhard; Groll, Petra; Haider, Christian; Haider, Olivia; Hauth, Eva; Hauth, Stefan; Hettrich, Sebastian; Jais, Wolfgang; Jones, Natalie; Taj-Eddine, Kamal; Karl, Alexander; Kauerhoff, Tilo; Khan, Muhammad Shadab; Kjeldsen, Andreas; Klauck, Jan; Losiak, Anna; Luger, Markus; Luger, Thomas; Luger, Ulrich; McArthur, Jane; Moser, Linda; Neuner, Julia; Orgel, Csilla; Ori, Gian Gabriele; Paternesi, Roberta; Peschier, Jarno; Pfeil, Isabella; Prock, Silvia; Radinger, Josef; Ragonig, Christoph; Ramirez, Barbara; Ramo, Wissam; Rampey, Mike; Sams, Arnold; Sams, Elisabeth; Sams, Sebastian; Sandu, Oana; Sans, Alejandra; Sansone, Petra; Scheer, Daniela; Schildhammer, Daniel; Scornet, Quentin; Sejkora, Nina; Soucek, Alexander; Stadler, Andrea; Stummer, Florian; Stumptner, Willibald; Taraba, Michael; Tlustos, Reinhard; Toferer, Ernst; Turetschek, Thomas; Winter, Egon; Zanella-Kux, Katja</p> <p>2014-05-01</p> <p>Abstract We have developed a portable dual-wavelength laser fluorescence spectrometer as part of a multi-instrument optical probe to characterize mineral, organic, and microbial species in extreme environments. Operating at 405 and 532 nm, the instrument was originally designed for use by human explorers to produce a laser-induced fluorescence emission (<span class="hlt">L.I.F.E</span>.) spectral database of the mineral and organic molecules found in the microbial communities of Earth's cryosphere. Recently, our team had the opportunity to explore the strengths and limitations of the instrument when it was deployed on a remote-controlled Mars analog rover. In February 2013, the instrument was deployed on board the Magma White rover platform during the MARS2013 Mars analog field <span class="hlt">mission</span> in the Kess Kess formation near Erfoud, Morocco. During these tests, we followed tele-science work flows pertinent to Mars surface <span class="hlt">missions</span> in a simulated spaceflight environment. We report on the <span class="hlt">L.I.F.E</span>. instrument setup, data processing, and performance during field trials. A pilot postmission laboratory analysis determined that rock samples acquired during the field <span class="hlt">mission</span> exhibited a fluorescence signal from the Sun-exposed side characteristic of chlorophyll a following excitation at 405 nm. A weak fluorescence response to excitation at 532 nm may have originated from another microbial photosynthetic pigment, phycoerythrin, but final assignment awaits development of a comprehensive database of mineral and organic fluorescence spectra. No chlorophyll fluorescence signal was detected from the shaded underside of the samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920024965','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920024965"><span>Strategic considerations for support of humans in space and Moon/Mars exploration <span class="hlt">missions</span>. <span class="hlt">Life</span> sciences research and technology programs, volume 1</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1992-01-01</p> <p>During the next several decades, our nation will embark on human exploration in space. In the microgravity environment we will learn how human physiology responds to the absence of gravity and what procedures and systems are required to maintain health and performance. As the human experience is extended for longer periods in low Earth orbit, we will also be exploring space robotically. Robotic precursor <span class="hlt">missions</span>, to learn more about the lunar and Martian environments will be conducted so that we can send crews to these planetary surfaces to further explore and conduct scientific investigations that include examining the very processes of <span class="hlt">life</span> itself. Human exploration in space requires the ability to maintain crew health and performance in spacecraft, during extravehicular activities, on planetary surfaces, and upon return to Earth. This goal can only be achieved through focused research and technological developments. This report provides the basis for setting research priorities and making decisions to enable human exploration <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010106392&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dheat%2Bexchange','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010106392&hterms=heat+exchange&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dheat%2Bexchange"><span>Practical Considerations of Waste Heat Reuse for a Mars <span class="hlt">Mission</span> Advanced <span class="hlt">Life</span> Support System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levri, Julie; Finn, Cory; Luna, Bernadette (Technical Monitor)</p> <p>2000-01-01</p> <p>Energy conservation is a key issue in design optimization of Advanced <span class="hlt">Life</span> Support Systems (ALSS) for long-term space <span class="hlt">missions</span>. By considering designs for conservation at the system level, energy saving opportunities arise that would otherwise go unnoticed. This paper builds on a steady-state investigation of system-level waste heat reuse in an ALSS with a low degree of crop growth for a Mars <span class="hlt">mission</span>. In past studies, such a system has been defined in terms of technology types, hot and cold stream identification and stream energy content. The maximum steady-state potential for power and cooling savings within the system was computed via the Pinch Method. In this paper, several practical issues are considered for achieving a pragmatic estimate of total system savings in terms of equivalent system mass (ESM), rather than savings solely in terms of power and cooling. In this paper, more realistic ESM savings are computed by considering heat transfer inefficiencies during material transfer. An estimate of the steady-state mass, volume and crewtime requirements associated with heat exchange equipment is made by considering heat exchange equipment material type and configuration, stream flow characteristics and associated energy losses during the heat exchange process. Also, previously estimated power and cooling savings are adjusted to reflect the impact of such energy losses. This paper goes one step further than the traditional Pinch Method of considering waste heat reuse in heat exchangers to include ESM savings that occur with direct reuse of a stream. For example, rather than exchanging heat between crop growth lamp cooling air and air going to a clothes dryer, air used to cool crop lamps might be reused directly for clothes drying purposes. When thermodynamically feasible, such an approach may increase ESM savings by minimizing the mass, volume and crewtime requirements associated with stream routing equipment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150007234&hterms=europa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Deuropa','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150007234&hterms=europa&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Deuropa"><span>Jovian Tour Design for Orbiter and Lander <span class="hlt">Missions</span> to Europa</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Campagnola, Stefano; Buffington, Brent B.; Petropoulos, Anastassios E.</p> <p>2013-01-01</p> <p>Europa is one of the most interesting targets for solar system exploration, as its ocean of liquid water could harbor <span class="hlt">life</span>. Following the recommendation of the Planetary Decadal Survey, NASA commissioned a study for a flyby <span class="hlt">mission</span>, an orbiter <span class="hlt">mission</span>, and a lander <span class="hlt">mission</span>. This paper presents the moon tours for the lander and orbiter concepts. The total delta v and radiation dose would be reduced by exploiting multi-body dynamics and avoiding phasing loops in the Ganymede-to- Europa transfer. Tour 11-O3, 12-L1 and 12-L4 are presented in details and their performaces compared to other tours from previous Europa <span class="hlt">mission</span> studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160005781','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160005781"><span>Methods and Costs to Achieve Ultra Reliable <span class="hlt">Life</span> Support</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Harry W.</p> <p>2012-01-01</p> <p>A published Mars <span class="hlt">mission</span> is used to explore the methods and costs to achieve ultra reliable <span class="hlt">life</span> support. The Mars <span class="hlt">mission</span> and its recycling <span class="hlt">life</span> support design are described. The <span class="hlt">life</span> support systems were made triply redundant, implying that each individual system will have fairly good reliability. Ultra reliable <span class="hlt">life</span> support is needed for Mars and other long, distant <span class="hlt">missions</span>. Current systems apparently have insufficient reliability. The <span class="hlt">life</span> cycle cost of the Mars <span class="hlt">life</span> support system is estimated. Reliability can be increased by improving the intrinsic system reliability, adding spare parts, or by providing technically diverse redundant systems. The costs of these approaches are estimated. Adding spares is least costly but may be defeated by common cause failures. Using two technically diverse systems is effective but doubles the <span class="hlt">life</span> cycle cost. Achieving ultra reliability is worth its high cost because the penalty for failure is very high.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120016811','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120016811"><span>Ice Dragon: A <span class="hlt">Mission</span> to Address Science and Human Exploration Objectives on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stoker, Carol R.; Davila, A.; Sanders, G.; Glass, Brian; Gonzales, A.; Heldmann, Jennifer; Karcz, J.; Lemke, L.; Sanders, G.</p> <p>2012-01-01</p> <p>We present a <span class="hlt">mission</span> concept where a SpaceX Dragon capsule lands a payload on Mars that samples ground ice to search for evidence of <span class="hlt">life</span>, assess hazards to future human <span class="hlt">missions</span>, and demonstrate use of Martian resources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012LPICo1679.4176S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012LPICo1679.4176S"><span>Ice Dragon: A <span class="hlt">Mission</span> to Address Science and Human Exploration Objectives on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stoker, C.; Davilla, A.; Davis, S.; Glass, B.; Gonzales, A.; Heldmann, J.; Karcz, J.; Lemke, L.; Sanders, G.</p> <p>2012-06-01</p> <p>We present a <span class="hlt">mission</span> concept where a SpaceX Dragon capsule lands a payload on Mars that samples ground ice to search for evidence of <span class="hlt">life</span>, assess hazards to future human <span class="hlt">missions</span>, and demonstrate use of Martian resources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912931B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912931B"><span>Joint Europa <span class="hlt">Mission</span> (JEM) : A multi-scale study of Europa to characterize its habitability and search for <span class="hlt">life</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blanc, Michel; Prieto Ballesteros, Olga; Andre, Nicolas; Cooper, John F.</p> <p>2017-04-01</p> <p>Europa is the closest and probably the most promising target to perform a comprehensive characterization of habitability and search for extant <span class="hlt">life</span>. We propose that NASA and ESA join forces to design an ambitious planetary <span class="hlt">mission</span> we call JEM (for Joint Europa <span class="hlt">Mission</span>) to reach this objective. JEM will be assigned the following overarching goal: Understand Europa as a complex system responding to Jupiter system forcing, characterize the habitability of its potential biosphere, and search for <span class="hlt">life</span> in its surface, sub-surface and exosphere. Our observation strategy to address these goals will combine three scientific measurement sequences: measurements on a high-latitude, low-latitude Europan orbit providing a continuous and global mapping of planetary fields (magnetic and gravity) and of the neutral and charged environment during a period of three months; in-situ measurements at the surface, using a soft lander operating during 35 days, to search for bio-signatures at the surface and sub-surface and operate a geophysical station; measurements of the chemical composition of the very low exosphere and plumes in search for biomolecules. The implementation of these three observation sequences will rest on the combination of two science platforms equipped with the most advanced instrumentation: a soft lander to perform all scientific measurements at the surface and sub-surface at a selected landing site, and a carrier/relay/orbiter to perform the orbital survey and descent sequences. In this concept, the orbiter will perform science operations during the relay phase on a carefully optimized halo orbit of the Europa-Jupiter system before moving to its final Europan orbit. The design of both orbiter and lander instruments will have to accommodate the very challenging radiation mitigation and Planetary Protection issues. The proposed lander science platform is composed of a geophysical station and of two complementary astrobiology facilities dedicated to bio</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140009163','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140009163"><span>NASA Laboratory Analysis for Manned Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Krihak, Michael K.; Shaw, Tianna E.</p> <p>2014-01-01</p> <p>The Exploration Laboratory Analysis (ELA) project supports the Exploration Medical Capability Element under the NASA Human Research Program. ELA instrumentation is identified as an essential capability for future exploration <span class="hlt">missions</span> to diagnose and treat evidence-based medical conditions. However, <span class="hlt">mission</span> architecture limits the medical equipment, consumables, and procedures that will be available to treat medical conditions during human exploration <span class="hlt">missions</span>. Allocated resources such as mass, power, volume, and crew time must be used efficiently to optimize the delivery of in-flight medical care. Although commercial instruments can provide the blood and urine based measurements required for exploration <span class="hlt">missions</span>, these commercial-off-the-shelf devices are prohibitive for deployment in the space environment. The objective of the ELA project is to close the technology gap of current minimally invasive laboratory capabilities and analytical measurements in a manner that the <span class="hlt">mission</span> architecture constraints impose on exploration <span class="hlt">missions</span>. Besides micro gravity and radiation tolerances, other principal issues that generally fail to meet NASA requirements include excessive mass, volume, power and consumables, and nominal reagent shelf-<span class="hlt">life</span>. Though manned exploration <span class="hlt">missions</span> will not occur for nearly a decade, NASA has already taken strides towards meeting the development of ELA medical diagnostics by developing <span class="hlt">mission</span> requirements and concepts of operations that are coupled with strategic investments and partnerships towards meeting these challenges. This paper focuses on the remote environment, its challenges, biomedical diagnostics requirements and candidate technologies that may lead to successful blood-urine chemistry and biomolecular measurements in future space exploration <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20180002051','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20180002051"><span>Introduction to <span class="hlt">Life</span> Support Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perry, Jay</p> <p>2017-01-01</p> <p>This course provides an introduction to the design and development of <span class="hlt">life</span> support systems to sustain humankind in the harsh environment of space. The <span class="hlt">life</span> support technologies necessary to provide a respirable atmosphere and clean drinking water are emphasized in the course. A historical perspective, beginning with open loop systems employed aboard the earliest crewed spacecraft through the state-of-the-art <span class="hlt">life</span> support technology utilized aboard the International Space Station today, will provide a framework for students to consider applications to possible future exploration <span class="hlt">missions</span> and destinations which may vary greatly in duration and scope. Development of future technologies as well as guiding requirements for designing <span class="hlt">life</span> support systems for crewed exploration <span class="hlt">missions</span> beyond low-Earth orbit are also considered in the course.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29753408','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29753408"><span>A urine-fuelled soil-based bioregenerative <span class="hlt">life</span> support system for long-term and long-distance manned space <span class="hlt">missions</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Maggi, Federico; Tang, Fiona H M; Pallud, Céline; Gu, Chuanhui</p> <p>2018-05-01</p> <p>A soil-based cropping unit fuelled with human urine for long-term manned space <span class="hlt">missions</span> was investigated with the aim to analyze whether a closed-loop nutrient cycle from human liquid wastes was achievable. Its ecohydrology and biogeochemistry were analysed in microgravity with the use of an advanced computational tool. Urine from the crew was used to supply primary (N, P, and K) and secondary (S, Ca and Mg) nutrients to wheat and soybean plants in the controlled cropping unit. Breakdown of urine compounds into primary and secondary nutrients as well as byproduct gases, adsorbed, and uptake fractions were tracked over a period of 20 years. Results suggested that human urine could satisfy the demand of at least 3 to 4 out of 6 nutrients with an offset in pH and salinity tolerable by plants. It was therefore inferred that a urine-fuelled <span class="hlt">life</span> support system can introduce a number of advantages including: (1) recycling of liquids wastes and production of food; (2) forgiveness of neglect as compared to engineered electro-mechanical systems that may fail under unexpected or unplanned conditions; and (3) reduction of supply and waste loads during space <span class="hlt">missions</span>. Copyright © 2018 The Committee on Space Research (COSPAR). Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20000020680&hterms=ECG&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DECG','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20000020680&hterms=ECG&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DECG"><span>Bion-11 Spaceflight <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Skidmore, M.</p> <p>1999-01-01</p> <p>The Sensors 2000! Program, in support of the Space <span class="hlt">Life</span> Sciences Payloads Office at NASA Ames Research Center developed a suite of bioinstrumentation hardware for use on the Joint US/Russian Bion I I Biosatellite <span class="hlt">Mission</span> (December 24, 1996 - January 7, 1997). This spaceflight included 20 separate experiments that were organized into a complimentary and interrelated whole, and performed by teams of US, Russian, and French investigators. Over 40 separate parameters were recorded in-flight on both analog and digital recording media for later analysis. These parameters included; Electromyogram (7 ch), Electrogastrogram, Electrooculogram (2 ch), ECG/EKG, Electroencephlogram (2 ch), single fiber firing of Neurovestibular afferent nerves (7 ch), Tendon Force, Head Motion Velocity (pitch & yaw), P02 (in vivo & ambient), temperature (deep body, skin, & ambient), and multiple animal and spacecraft performance parameters for a total of 45 channels of recorded data. Building on the close cooperation of previous <span class="hlt">missions</span>, US and Russian engineers jointly developed, integrated, and tested the physiologic instrumentation and data recording system. For the first time US developed hardware replaced elements of the Russian systems resulting in a US/Russian hybrid instrumentation and data system that functioned flawlessly during the 14 day <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E.151B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E.151B"><span>Why we need asteroid sample return <span class="hlt">mission</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barucci, Maria Antonietta</p> <p>2016-07-01</p> <p>Small bodies retain evidence of the primordial solar nebula and the earliest solar system processes that shaped their evolution. They may also contain pre-solar material as well as complex organic molecules, which could have a major role to the development of <span class="hlt">life</span> on Earth. For these reasons, asteroids and comets have been targets of interest for <span class="hlt">missions</span> for over three decades. However, our knowledge of these bodies is still very limited, and each asteroid or comet visited by space <span class="hlt">mission</span> has revealed unexpected scientific results, e.g. the structure and nature of comet 67P/Churyumov-Gerasimenko (67P/C-G) visited by the Rosetta <span class="hlt">mission</span>. Only in the laboratory can instruments with the necessary precision and sensitivity be applied to individual components of the complex mixture of materials that forms a small body regolith, to determine their precise chemical and isotopic composition. Such measurements are vital for revealing the evidence of stellar, interstellar medium, pre-solar nebula and parent body processes that are retained in primitive material, unaltered by atmospheric entry or terrestrial contamination. For those reasons, sample return <span class="hlt">missions</span> are considered a high priority by a number of the leading space agencies. Abundant within the inner Solar System and the main impactors on terrestrial planets, small bodies may have been the principal contributors of the water and organic material essential to create <span class="hlt">life</span> on Earth. Small bodies can therefore be considered to be equivalent to DNA for unravelling our solar system's history, offering us a unique window to investigate both the formation of planets and the origin of <span class="hlt">life</span>. A sample return <span class="hlt">mission</span> to a primitive Near-Earth Asteroid (NEA) has been study at ESA from 2008 in the framework of ESA's Cosmic Vision (CV) programme, with the objective to answer to the fundamental CV questions "How does the Solar System work?" and "What are the conditions for <span class="hlt">life</span> and planetary formations?". The returned material</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title45-vol4/pdf/CFR-2010-title45-vol4-sec1388-3.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title45-vol4/pdf/CFR-2010-title45-vol4-sec1388-3.pdf"><span>45 CFR 1388.3 - Program criteria-<span class="hlt">mission</span>.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-10-01</p> <p>... statement. (c) The UAP's <span class="hlt">mission</span> and programs must reflect a <span class="hlt">life</span> span approach, incorporate an interdisciplinary approach and include the active participation of individuals with developmental disabilities and... collaborations and strategies to effect systemic change within the university and in State and local communities...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030111644&hterms=Alvera&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAlvera','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030111644&hterms=Alvera&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DAlvera"><span>Mars Analog Research and Technology Experiment (MARTE): A Simulated Mars Drilling <span class="hlt">Mission</span> to Search for Subsurface <span class="hlt">Life</span> at the Rio Tinto, Spain</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stoker, Carol; Lemke, Larry; Mandell, Humboldt; McKay, David; George, Jeffrey; Gomez-Alvera, Javier; Amils, Ricardo; Stevens, Todd; Miller, David</p> <p>2003-01-01</p> <p>The MARTE (Mars Astrobiology Research and Technology Experiment) project was selected by the new NASA ASTEP program, which supports field experiments having an equal emphasis on Astrobiology science and technology development relevant to future Astrobiology <span class="hlt">missions</span>. MARTE will search for a hypothesized subsurface anaerobic chemoautotrophic biosphere in the region of the Tinto River in southwestern Spain while also demonstrating technology needed to search for a subsurface biosphere on Mars. The experiment is informed by the strategy for searching for <span class="hlt">life</span> on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140010823','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140010823"><span>Kilowatt-Class Fission Power Systems for Science and Human Precursor <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mason, Lee S.; Gibson, Marc Andrew; Poston, Dave</p> <p>2013-01-01</p> <p>Nuclear power provides an enabling capability for NASA <span class="hlt">missions</span> that might otherwise be constrained by power availability, <span class="hlt">mission</span> duration, or operational robustness. NASA and the Department of Energy (DOE) are developing fission power technology to serve a wide range of future space uses. Advantages include lower mass, longer <span class="hlt">life</span>, and greater <span class="hlt">mission</span> flexibility than competing power system options. Kilowatt-class fission systems, designated "Kilopower," were conceived to address the need for systems to fill the gap above the current 100-W-class radioisotope power systems being developed for science <span class="hlt">missions</span> and below the typical 100-k We-class reactor power systems being developed for human exploration <span class="hlt">missions</span>. This paper reviews the current fission technology project and examines some Kilopower concepts that could be used to support future science <span class="hlt">missions</span> or human precursors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011723','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011723"><span>Kilowatt-Class Fission Power Systems for Science and Human Precursor <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mason, Lee; Gibson, Marc; Poston, Dave</p> <p>2013-01-01</p> <p>Nuclear power provides an enabling capability for NASA <span class="hlt">missions</span> that might otherwise be constrained by power availability, <span class="hlt">mission</span> duration, or operational robustness. NASA and the Department of Energy (DOE) are developing fission power technology to serve a wide range of future space uses. Advantages include lower mass, longer <span class="hlt">life</span>, and greater <span class="hlt">mission</span> flexibility than competing power system options. Kilowatt-class fission systems, designated "Kilopower," were conceived to address the need for systems to fill the gap above the current 100-Wclass radioisotope power systems being developed for science <span class="hlt">missions</span> and below the typical 100-kWe-class reactor power systems being developed for human exploration <span class="hlt">missions</span>. This paper reviews the current fission technology project and examines some Kilopower concepts that could be used to support future science <span class="hlt">missions</span> or human precursors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20100031721&hterms=development+chemistry&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Ddevelopment%2Bchemistry','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20100031721&hterms=development+chemistry&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Ddevelopment%2Bchemistry"><span>Development of a NASA 2018 Mars Landed <span class="hlt">Mission</span> Concept</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wilson, M. G.; Salvo, C. G.; Abilleira, F.; Sengstacken, A. J.; Allwood, A. G.; Backes, P. G.; Lindemann, R. A.; Jordan, J. F.</p> <p>2010-01-01</p> <p>Fundamental to NASA's Mars Exploration Program (MEP) is an ongoing development of an integrated and coordinated set of possible future candidate <span class="hlt">missions</span> that meet fundamental science and programmatic objectives of NASA and the Mars scientific community. In the current planning horizon of the NASA MEP, a landed mobile surface exploration <span class="hlt">mission</span> launching in the 2018 Mars launch opportunity exists as a candidate project to meet MEP in situ science and exploration objectives. This paper describes the proposed <span class="hlt">mission</span> science objectives and the <span class="hlt">mission</span> implementation concept developed for the 2018 opportunity. As currently envisioned, this <span class="hlt">mission</span> concept seeks to explore a yet-to-be-selected site with high preservation potential for physical and chemical biosignatures, evaluate paleoenvironmental conditions, characterize the potential for preservation of biosignatures, and access multiple sequences of geological units in a search for evidence of past <span class="hlt">life</span> and/or prebiotic chemistry at a site on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980024341','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980024341"><span>Biological <span class="hlt">Life</span> Support Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>Session MP2 includes short reports on: (1) Crew Regenerative <span class="hlt">Life</span> Support in Long Duration Space <span class="hlt">Missions</span>; (2) Bioconversion Systems for Food and Water on Long Term Space <span class="hlt">Missions</span>; (3) Novel Laboratory Approaches to Multi-purpose Aquatic Biogenerative Closed-Loop Food Production Systems; and (4) Artificial Neural Network Derived Plant Growth Models.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002cosp...34E..88H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002cosp...34E..88H"><span>HUMEX, a study on the survivability and adaptation of humans to long- duration exploratory <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horneck, G.</p> <p></p> <p>ESA has recently initiated a study of the human responses, limits and needs with regard to the stress environments of interplanetary and planetary <span class="hlt">missions</span>. Emphasis was laid on human health and performance care as well as Advanced <span class="hlt">Life</span> Support Developments including Bioregenerative <span class="hlt">Life</span> Support Systems and environmental monitoring. The overall study goals were as follows: (i) to define reference scenarios for a European participation in human exploration and to estimate their influence on the <span class="hlt">Life</span> Sciences and <span class="hlt">Life</span> Support requirements; (ii) for selected <span class="hlt">mission</span> scenarios, to critically assess the limiting factors for human health, wellbeing, and performance and to recommend relevant countermeasures; (iii) for selected <span class="hlt">mission</span> scenarios, to critically assess the potential of Advanced <span class="hlt">Life</span> Support Developments and to propose a European strategy including terrestrial applications; (iv) to critically assess the feasibility of existing facilities and technologies on ground and in space as testbeds in preparation for human exploratory <span class="hlt">missions</span> and to develop a test plan for ground and ISS campaigns; (v) to develop a roadmap for a future European strategy towards human exploratory <span class="hlt">missions</span>, including preparatory activities and terrestrial applications and benefits. A lunar base at the south pole where constant sunlight and potential water ice deposits could be assumed was selected as the moon scenario. the impact on human health, performance and well being has been investigated from the view point of the effects of microgravity (during space travel), reduced gravity (on the Moon) and abrupt gravity changes (during launch and landing), of the effects of cosmic radiation including solar particle events, of psychological issues as well as general health care. Countermeasures as well as necessary research using ground- based testbeds and/or the ISS have been defined. The need for highly intelligent autonomous diagnostic and therapy systems was considered as a driver also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980024353','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980024353"><span>The German/Russian MIR 1997 <span class="hlt">Mission</span>: An Overview</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1997-01-01</p> <p>Session TP4 includes short reports concerning: (1) <span class="hlt">Life</span> Science Experiments During the German-Russian Mir '97 <span class="hlt">Mission</span>; (2) Orthostatic Intolerance Following Microgravity: A Role for Autonomic Dysfunction; (3) Heart Rate Variability and Skin Blood Flow in Man During Orthostatic Stress in Weightlessness; (4) Effects of Microgravity and Lower Body Negative Pressure on Circulatory Drives from Excercising Calf Muscles; (5) The Mir Station in Its Second Decade: Crew Science Operation During Mir '97; (6) Metabolic WARD (Water, Sodium, Calcium, and Bone Metabolism) and Endocrinological Experiments During the Mir '97 <span class="hlt">Mission</span>; (7) Long-term Monitoring of the Spine-geometry During the Mir '97 <span class="hlt">Mission</span>: Introduction of a New Method; and (8) Effects of 20 days of Microgravity (German/Russian Mir '97 <span class="hlt">Mission</span>) on the Mechanical and Electromyographic Characteristics of Explosive Efforts of the Lower Limbs and of Cycloergometric Exercises of Mild to Sprint-Like Intensity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010018879&hterms=Science+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DScience%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010018879&hterms=Science+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DScience%2Blife"><span>Spacelab <span class="hlt">Life</span> Sciences Research Panel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sulzman, Frank; Young, Laurence R.; Seddon, Rhea; Ross, Muriel; Baldwin, Kenneth; Frey, Mary Anne; Hughes, Rod</p> <p>2000-01-01</p> <p>This document describes some of the <span class="hlt">life</span> sciences research that was conducted on Spacelab <span class="hlt">missions</span>. Dr. Larry Young, Director of the National Space Biomedical Research Institute, provides an overview of the <span class="hlt">Life</span> Sciences Spacelabs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H31F1268H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H31F1268H"><span>Water Cycle <span class="hlt">Missions</span> for the Next Decade</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Houser, P. R.</p> <p>2013-12-01</p> <p>The global water cycle describes the circulation of water as a vital and dynamic substance in its liquid, solid, and vapor phases as it moves through the atmosphere, oceans and land. <span class="hlt">Life</span> in its many forms exists because of water, and modern civilization depends on learning how to live within the constraints imposed by the availability of water. The scientific challenge posed by the need to observe the global water cycle is to integrate in situ and space-borne observations to quantify the key water-cycle state variables and fluxes. The vision to address that challenge is a series of Earth observation <span class="hlt">missions</span> that will measure the states, stocks, flows, and residence times of water on regional to global scales followed by a series of coordinated <span class="hlt">missions</span> that will address the processes, on a global scale, that underlie variability and changes in water in all its three phases. The accompanying societal challenge is to foster the improved use of water data and information as a basis for enlightened management of water resources, to protect <span class="hlt">life</span> and property from effects of extremes in the water cycle. A major change in thinking about water science that goes beyond its physics to include its role in ecosystems and society is also required. Better water-cycle observations, especially on the continental and global scales, will be essential. Water-cycle predictions need to be readily available globally to reduce loss of <span class="hlt">life</span> and property caused by water-related natural hazards. Building on the 2007 Earth Science Decadal Survey, NASA's Plan for a Climate-Centric Architecture for Earth Observations and Applications from Space , and the 2012 Chapman Conference on Remote Sensing of the Terrestrial Water Cycle, a workshop was held in April 2013 to gather wisdom and determine how to prepare for the next generation of water cycle <span class="hlt">missions</span> in support of the second Earth Science Decadal Survey. This talk will present the outcomes of the workshop including the intersection between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/986416-systematic-comprehensive-computational-model-stake-estimation-mission-assurance-applying-cyber-security-econometrics-system-cses-mission-assurance-analysis-protocol-maap','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/986416-systematic-comprehensive-computational-model-stake-estimation-mission-assurance-applying-cyber-security-econometrics-system-cses-mission-assurance-analysis-protocol-maap"><span>A Systematic Comprehensive Computational Model for Stake Estimation in <span class="hlt">Mission</span> Assurance: Applying Cyber Security Econometrics System (CSES) to <span class="hlt">Mission</span> Assurance Analysis Protocol (MAAP)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Abercrombie, Robert K; Sheldon, Frederick T; Grimaila, Michael R</p> <p>2010-01-01</p> <p>In earlier works, we presented a computational infrastructure that allows an analyst to estimate the security of a system in terms of the loss that each stakeholder stands to sustain as a result of security breakdowns. In this paper, we discuss how this infrastructure can be used in the subject domain of <span class="hlt">mission</span> assurance as defined as the full <span class="hlt">life</span>-cycle engineering process to identify and mitigate design, production, test, and field support deficiencies of <span class="hlt">mission</span> success. We address the opportunity to apply the Cyberspace Security Econometrics System (CSES) to Carnegie Mellon University and Software Engineering Institute s <span class="hlt">Mission</span> Assurance Analysismore » Protocol (MAAP) in this context.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020081349','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020081349"><span>The Stellar Imager (SI) <span class="hlt">Mission</span> Concept</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carpenter, Kenneth G.; Schrijver, Carolus J.; Lyon, Richard G.; Mundy, Lee G.; Allen, Ronald J.; Armstrong, Thomas; Danchi, William C.; Karovska, Margarita; Marzouk, Joe; Mazzuca, Lisa M.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20020081349'); toggleEditAbsImage('author_20020081349_show'); toggleEditAbsImage('author_20020081349_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20020081349_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20020081349_hide"></p> <p>2002-01-01</p> <p>The Stellar Imager (SI) is envisioned as a space-based, UV-optical interferometer composed of 10 or more one-meter class elements distributed with a maximum baseline of 0.5 km. It is designed to image stars and binaries with sufficient resolution to enable long-term studies of stellar magnetic activity patterns, for comparison with those on the sun. It will also support asteroseismology (acoustic imaging) to probe stellar internal structure, differential rotation, and large-scale circulations. SI will enable us to understand the various effects of the magnetic fields of stars, the dynamos that generate these fields, and the internal structure and dynamics of the stars. The ultimate goal of the <span class="hlt">mission</span> is to achieve the best-possible forecasting of solar activity as a driver of climate and space weather on time scales ranging from months up to decades, and an understanding of the impact of stellar magnetic activity on <span class="hlt">life</span> in the Universe. In this paper we describe the scientific goals of the <span class="hlt">mission</span>, the performance requirements needed to address these goals, the "enabling technology" development efforts being pursued, and the design concepts now under study for the full <span class="hlt">mission</span> and a possible pathfinder <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870008289','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870008289"><span>Manned Mars <span class="hlt">Missions</span>. Working group papers, volume 1, section 1-4</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Duke, Michael B. (Editor); Keaton, Paul W. (Editor)</p> <p>1986-01-01</p> <p>The papers presented by the working group on Manned Mars <span class="hlt">Missions</span> are given. The purpose is to update earlier Mars <span class="hlt">missions</span> study data, to examine the impact of new and emerging technologies on Mars <span class="hlt">mission</span> capabilities, and to identify technological issues that would be useful in projecting scientific and engineering research in the coming decades. The papers are grouped into nine sections, which are: (1) rationale; (2) transportation trades and issues; (3) <span class="hlt">mission</span> and configuration concepts; (4) surface infrastructure; (5) science investigations and issues; (6) <span class="hlt">life</span> science/medical issues; (7) subsystems and technology development requirements; (8) political and economic issues; and (9) impact on other programs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940020208','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940020208"><span>Power generation technology options for a Mars <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bozek, John M.; Cataldo, Robert L.</p> <p>1994-01-01</p> <p>The power requirements and resultant power system performances of an aggressive Mars <span class="hlt">mission</span> are characterized. The power system technologies discussed will support both cargo and piloted space transport vehicles as well as a six-person crew on the Martian surface for 600 days. The <span class="hlt">mission</span> uses materials transported by cargo vehicles and materials produced using in-situ planetary feed stock to establish a <span class="hlt">life</span>-support cache and infrastructure for the follow-on piloted lander. Numerous power system technical options are sized to meet the <span class="hlt">mission</span> power requirements using conventional and solar, nuclear, and wireless power transmission technologies for stationary, mobile surface, and space applications. Technology selections will depend on key criteria such as mass, volume, area, maturity, and application flexibility.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140002978','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140002978"><span>Photonics on the <span class="hlt">Mission</span> to Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Watson, Michael D.</p> <p>2013-01-01</p> <p>Human <span class="hlt">missions</span> to Mars present some unique challenges for photonics devices. These devices will have exposure to many different space environments. During assembly they will be exposed to the Earth orbiting environment. Upon departure they will need to function through the Earth's Van Allen Radiation Belt. While the general interplanetary environment is less challenging than the radiation belt, they will operate in this environment for 18 months, subject to sudden saturation from solar flares. These components must continue to function properly through these saturation events presenting quite a challenge to photonic components, both optical and electronic. At Mars, the orbital environment is more benign than the Earth's. Components used as part of the landing vehicles must also deal with the pervasive dust environment for 3 - 6 months. These assembly and <span class="hlt">mission</span> execution environments provide every form of space environmental challenges to photonic components. This paper will briefly discuss each environment and the expectations on the components for successful operation over the <span class="hlt">life</span> of the <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160010478','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160010478"><span>NASA Advanced Exploration Systems: Advancements in <span class="hlt">Life</span> Support Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shull, Sarah A.; Schneider, Walter F.</p> <p>2016-01-01</p> <p>The NASA Advanced Exploration Systems (AES) <span class="hlt">Life</span> Support Systems (LSS) project strives to develop reliable, energy-efficient, and low-mass spacecraft systems to provide environmental control and <span class="hlt">life</span> support systems (ECLSS) critical to enabling long duration human <span class="hlt">missions</span> beyond low Earth orbit (LEO). Highly reliable, closed-loop <span class="hlt">life</span> support systems are among the capabilities required for the longer duration human space exploration <span class="hlt">missions</span> assessed by NASA’s Habitability Architecture Team.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Environmental+AND+scanning&pg=6&id=EJ508777','ERIC'); return false;" href="https://eric.ed.gov/?q=Environmental+AND+scanning&pg=6&id=EJ508777"><span>The Comprehensive <span class="hlt">Mission</span> of Rural Community Colleges.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Cavan, John</p> <p>1995-01-01</p> <p>Reviews the comprehensive <span class="hlt">mission</span> of rural community colleges, arguing that they are major elements in the <span class="hlt">life</span> of their service areas and must meet community needs. Describes the role of rural college presidents and the importance of environmental scanning. Reviews challenges facing rural institutions in the future. (MAB)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008cosp...37..798E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008cosp...37..798E"><span>Urey onboard Exomars: Searching for <span class="hlt">life</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ehrenfreund, Pascale</p> <p></p> <p>Exomars is the flagship <span class="hlt">mission</span> of the European exploration program Aurora. The main goal of the Exomars <span class="hlt">mission</span> is to further characterize the environment on Mars and to search for <span class="hlt">life</span>. Data from recent Mars <span class="hlt">missions</span> indicate the presence of liquid water for a geologically relevant period of time. If <span class="hlt">life</span> arose during that period, evidence in the form of organic compounds might still be present on Mars today. A fundamental challenge ahead for the Exomars <span class="hlt">mission</span> is to search for extinct and extant <span class="hlt">life</span> using a sophisticated drill and innovative <span class="hlt">life</span> detection instruments. Urey: Mars Organic and Oxidant Detector has been selected for the Pasteur payload and is considered a key instrument to achieve the <span class="hlt">mission</span>'s scientific objectives. Urey will target several key classes of organic molecules such as amino acids, nucleobases, aminosugars as well as polycyclic aromatic hydrocrabon (PAHs) using state-of-the-art analytical methods. The sensitivity of Urey to detect organic compounds in the Martian regolith is unprecedented (part-per-trillions). Efficient extraction of organic molecules using a sub-critical water extractor and subsequent concentration through sublimation renders a sample that is best suited to be analyzed by the sensitive mµCE system. The capability of the mµCE component to distinguish chiral amino acids will give direct evidence for abiotic or biotic compound origin. Another Urey component, the Mars Oxidation Instument, will deploy chemoresistor oxidant sensors to take complementary measurements evaluating the survival potential of organic compounds in the environment. We report on the progress of instrument development and related field tests in the Atacama desert.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950016842','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950016842"><span>STS-61 <span class="hlt">mission</span> director's post-<span class="hlt">mission</span> report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Newman, Ronald L.</p> <p>1995-01-01</p> <p>To ensure the success of the complex Hubble Space Telescope servicing <span class="hlt">mission</span>, STS-61, NASA established a number of independent review groups to assess management, design, planning, and preparation for the <span class="hlt">mission</span>. One of the resulting recommendations for <span class="hlt">mission</span> success was that an overall <span class="hlt">Mission</span> Director be appointed to coordinate management activities of the Space Shuttle and Hubble programs and to consolidate results of the team reviews and expedite responses to recommendations. This report presents pre-<span class="hlt">mission</span> events important to the experience base of <span class="hlt">mission</span> management, with related <span class="hlt">Mission</span> Director's recommendations following the event(s) to which they apply. All <span class="hlt">Mission</span> Director's recommendations are presented collectively in an appendix. Other appendixes contain recommendations from the various review groups, including Payload Officers, the JSC Extravehicular Activity (EVA) Section, JSC EVA Management Office, JSC Crew and Thermal Systems Division, and the STS-61 crew itself. This report also lists <span class="hlt">mission</span> events in chronological order and includes as an appendix a post-<span class="hlt">mission</span> summary by the lead Payload Deployment and Retrieval System Officer. Recommendations range from those pertaining to specific component use or operating techniques to those for improved management, review, planning, and safety procedures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EOSTr..83R.322S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EOSTr..83R.322S"><span>Panel proposes solar system <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Showstack, Randy</p> <p></p> <p>A proposed probe to the Kuiper Belt and Pluto and another to Europa are among the priority Solar System exploration <span class="hlt">missions</span> that should be pursued by NASA over the next decade, according to an 11 July report by a steering group of the Space Studies Board of the U.S. National Research Council (NRC).The report, "New Frontiers in the Solar System: An Integrated Exploration Strategy," was requested by NASA, and proposes a set of new <span class="hlt">missions</span> and facilities to respond to key questions in four cross-cutting themes. The themes, which the report indicates form the basis for an integrated space exploration strategy are: the first billion years of Solar System history; volatiles and organics: the stuff of <span class="hlt">life</span>; the origin and evolution of habitable worlds; and processes: how planets work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050193848&hterms=satisfaction&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dsatisfaction','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050193848&hterms=satisfaction&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dsatisfaction"><span>Model implementation for dynamic computation of system cost for advanced <span class="hlt">life</span> support</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levri, J. A.; Vaccari, D. A.</p> <p>2004-01-01</p> <p><span class="hlt">Life</span> support system designs for long-duration space <span class="hlt">missions</span> have a multitude of requirements drivers, such as <span class="hlt">mission</span> objectives, political considerations, cost, crew wellness, inherent <span class="hlt">mission</span> attributes, as well as many other influences. Evaluation of requirements satisfaction can be difficult, particularly at an early stage of <span class="hlt">mission</span> design. Because launch cost is a critical factor and relatively easy to quantify, it is a point of focus in early <span class="hlt">mission</span> design. The method used to determine launch cost influences the accuracy of the estimate. This paper discusses the appropriateness of dynamic <span class="hlt">mission</span> simulation in estimating the launch cost of a <span class="hlt">life</span> support system. This paper also provides an abbreviated example of a dynamic simulation <span class="hlt">life</span> support model and possible ways in which such a model might be utilized for design improvement. c2004 COSPAR. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030025732','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030025732"><span>Satellite Servicing in <span class="hlt">Mission</span> Design Studies at the NASA GSFC</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Leete, Stephen J.</p> <p>2003-01-01</p> <p>Several NASA <span class="hlt">missions</span> in various stages of development have undergone one-week studies in the National Aeronautics and Space Administration (NASA) Goddard Space Flight Center (GSFC) Integrated <span class="hlt">Mission</span> Design Center (IMDC), mostly in preparation for proposals. The possible role of satellite servicing has been investigated for several of these <span class="hlt">missions</span>, applying the lessons learned from Hubble Space Telescope (HST) servicing, taking into account the current state of the art, projecting into the future, and implementing NASA long-range plans, and is presented here. The general benefits and costs of injecting satellite servicing are detailed, including components such as <span class="hlt">mission</span> timeline, mass, fuel, spacecraft design, risk abatement, <span class="hlt">life</span> extension, and improved performance. The approach taken in addressing satellite servicing during IMDC studies is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990018685','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990018685"><span>Surface Nuclear Power for Human Mars <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mason, Lee S.</p> <p>1999-01-01</p> <p>The Design Reference <span class="hlt">Mission</span> for NASA's human <span class="hlt">mission</span> to Mars indicates the desire for in-situ propellant production and bio-regenerative <span class="hlt">life</span> systems to ease Earth launch requirements. These operations, combined with crew habitation and science, result in surface power requirements approaching 160 kilowatts. The power system, delivered on an early cargo <span class="hlt">mission</span>, must be deployed and operational prior to crew departure from Earth. The most mass efficient means of satisfying these requirements is through the use of nuclear power. Studies have been performed to identify a potential system concept using a mobile cart to transport the power system away from the Mars lander and provide adequate separation between the reactor and crew. The studies included an assessment of reactor and power conversion technology options, selection of system and component redundancy, determination of optimum separation distance, and system performance sensitivity to some key operating parameters. The resulting system satisfies the key <span class="hlt">mission</span> requirements including autonomous deployment, high reliability, and cost effectiveness at a overall system mass of 12 tonnes and a stowed volume of about 63 cu m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002cosp...34E.192S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002cosp...34E.192S"><span>Analysis and control of macro - and microorganisms interactions for <span class="hlt">missions</span> of different duration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Somova, L.; Pechurkin, N.</p> <p></p> <p>In developing different t pes of <span class="hlt">life</span> support systems for use in space or extremey environments Earth, researchers should pay attention to the functional state and stability of such systems. Special attention has been given to the interactions between macro- and microorganisms. Microorganisms are considered the most suitable indicators of a system's health and its component links. We can divide all space <span class="hlt">missions</span> into types by which the behavior of man microbe interactions may be categorized: short <span class="hlt">missions</span> and long ones. For short <span class="hlt">missions</span> sanitary and hygiene procedures can be used to control the microflora of open and / or physico -chemical systems of <span class="hlt">life</span> support. F r more prolonged <span class="hlt">missions</span> hygieneo provisions may become inadequate and opportunistic infection occur rapidly. In general we should understand that the task of maintaining the heals of human being under conditions of stress is not only a question of sanitation and hygiene, but also a problem of the ecological balance within the habitat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040087004','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040087004"><span>Predicting <span class="hlt">Mission</span> Success in Small Satellite <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Saunders, Mark; Richie, Wayne; Rogers, John; Moore, Arlene</p> <p>1992-01-01</p> <p>In our global society with its increasing international competition and tighter financial resources, governments, commercial entities and other organizations are becoming critically aware of the need to ensure that space <span class="hlt">missions</span> can be achieved on time and within budget. This has become particularly true for the National Aeronautics and Space Administration's (NASA) Office of Space Science (OSS) which has developed their Discovery and Explorer programs to meet this need. As technologies advance, space <span class="hlt">missions</span> are becoming smaller and more capable than their predecessors. The ability to predict the <span class="hlt">mission</span> success of these small satellite <span class="hlt">missions</span> is critical to the continued achievement of NASA science <span class="hlt">mission</span> objectives. The NASA Office of Space Science, in cooperation with the NASA Langley Research Center, has implemented a process to predict the likely success of <span class="hlt">missions</span> proposed to its Discovery and Explorer Programs. This process is becoming the basis for predicting <span class="hlt">mission</span> success in many other NASA programs as well. This paper describes the process, methodology, tools and synthesis techniques used to predict <span class="hlt">mission</span> success for this class of <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990099585&hterms=tool+financial&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dtool%2Bfinancial','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990099585&hterms=tool+financial&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dtool%2Bfinancial"><span>Predicting <span class="hlt">Mission</span> Success in Small Satellite <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Saunders, Mark; Richie, R. Wayne; Moore, Arlene; Rogers, John</p> <p>1999-01-01</p> <p>In our global society with its increasing international competition and tighter financial resources, governments, commercial entities and other organizations are becoming critically aware of the need to ensure that space <span class="hlt">missions</span> can be achieved on time and within budget. This has become particularly true for the National Aeronautics and Space Administration's (NASA's) Office of Space Science (OSS) which has developed their Discovery and Explorer programs to meet this need. As technologies advance, space <span class="hlt">missions</span> are becoming smaller and more capable than their predecessors. The ability to predict the <span class="hlt">mission</span> success of these small satellite <span class="hlt">missions</span> is critical to the continued achievement of NASA science <span class="hlt">mission</span> objectives. The NASA Office of Space Science, in cooperation with the NASA Langley Research Center, has implemented a process to predict the likely success of <span class="hlt">missions</span> proposed to its Discovery and Explorer Programs. This process is becoming the basis for predicting <span class="hlt">mission</span> success in many other NASA programs as well. This paper describes the process, methodology, tools and synthesis techniques used to predict <span class="hlt">mission</span> success for this class of <span class="hlt">mission</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29048222','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29048222"><span>Correlations Between <span class="hlt">Life</span>-Detection Techniques and Implications for Sampling Site Selection in Planetary Analog <span class="hlt">Missions</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gentry, Diana M; Amador, Elena S; Cable, Morgan L; Chaudry, Nosheen; Cullen, Thomas; Jacobsen, Malene B; Murukesan, Gayathri; Schwieterman, Edward W; Stevens, Adam H; Stockton, Amanda; Tan, George; Yin, Chang; Cullen, David C; Geppert, Wolf</p> <p>2017-10-01</p> <p>We conducted an analog sampling expedition under simulated <span class="hlt">mission</span> constraints to areas dominated by basaltic tephra of the Eldfell and Fimmvörðuháls lava fields (Iceland). Sites were selected to be "homogeneous" at a coarse remote sensing resolution (10-100 m) in apparent color, morphology, moisture, and grain size, with best-effort realism in numbers of locations and replicates. Three different biomarker assays (counting of nucleic-acid-stained cells via fluorescent microscopy, a luciferin/luciferase assay for adenosine triphosphate, and quantitative polymerase chain reaction (qPCR) to detect DNA associated with bacteria, archaea, and fungi) were characterized at four nested spatial scales (1 m, 10 m, 100 m, and >1 km) by using five common metrics for sample site representativeness (sample mean variance, group F tests, pairwise t tests, and the distribution-free rank sum H and u tests). Correlations between all assays were characterized with Spearman's rank test. The bioluminescence assay showed the most variance across the sites, followed by qPCR for bacterial and archaeal DNA; these results could not be considered representative at the finest resolution tested (1 m). Cell concentration and fungal DNA also had significant local variation, but they were homogeneous over scales of >1 km. These results show that the selection of <span class="hlt">life</span> detection assays and the number, distribution, and location of sampling sites in a low biomass environment with limited a priori characterization can yield both contrasting and complementary results, and that their interdependence must be given due consideration to maximize science return in future biomarker sampling expeditions. Key Words: Astrobiology-Biodiversity-Microbiology-Iceland-Planetary exploration-Mars <span class="hlt">mission</span> simulation-Biomarker. Astrobiology 17, 1009-1021.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840010198','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840010198"><span>Space station needs, attributes and architectural options study. Volume 2: <span class="hlt">Mission</span> analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1983-01-01</p> <p>Space environment studies, astrophysics, Earth environment, <span class="hlt">life</span> sciences, and material sciences are discussed. Commercial communication, materials processing, and Earth observation <span class="hlt">missions</span> are addressed. Technology development, space operations, scenarios of operational capability, <span class="hlt">mission</span> requirements, and benefits analysis results for space-produced gallium arsenide crystals, direct broadcasting satellite systems, and a high inclination space station are covered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170002600','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170002600"><span>Dust Storm Impacts on Human Mars <span class="hlt">Mission</span> Equipment and Operations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rucker, M. A.</p> <p>2017-01-01</p> <p>Although it is tempting to use dust impacts on Apollo lunar exploration <span class="hlt">mission</span> equipment and operations as an analog for human Mars exploration, there are a number of important differences to consider. Apollo <span class="hlt">missions</span> were about a week long; a human Mars <span class="hlt">mission</span> will start at least two years before crew depart from Earth, when cargo is pre-deployed, and crewed <span class="hlt">mission</span> duration may be over 800 days. Each Apollo <span class="hlt">mission</span> landed at a different site; although no decisions have been made, NASA is investigating multiple human <span class="hlt">missions</span> to a single Mars landing site, building up capability over time and lowering costs by re-using surface infrastructure. Apollo <span class="hlt">missions</span> used two, single-use spacecraft; a human Mars <span class="hlt">mission</span> may require as many as six craft for different phases of the <span class="hlt">mission</span>, most of which would be re-used by subsequent crews. Apollo crews never ventured more than a few kilometers from their lander; Mars crews may take "camping trips" a hundred kilo-meters or more from their landing site, utilizing pressurized rovers to explore far from their base. Apollo <span class="hlt">mission</span> designers weren't constrained by human for-ward contamination of the Moon; if we plan to search for evidence of <span class="hlt">life</span> on Mars we'll have to be more careful. These differences all impact how we will mitigate and manage dust on our human Mars <span class="hlt">mission</span> equipment and operations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140009939','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140009939"><span>Logistics Reduction Technologies for Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Broyan, James L., Jr.; Ewert, Michael K.; Fink, Patrick W.</p> <p>2014-01-01</p> <p>Human exploration <span class="hlt">missions</span> under study are limited by the launch mass capacity of existing and planned launch vehicles. The logistical mass of crew items is typically considered separate from the vehicle structure, habitat outfitting, and <span class="hlt">life</span> support systems. Although mass is typically the focus of exploration <span class="hlt">missions</span>, due to its strong impact on launch vehicle and habitable volume for the crew, logistics volume also needs to be considered. NASA's Advanced Exploration Systems (AES) Logistics Reduction and Repurposing (LRR) Project is developing six logistics technologies guided by a systems engineering cradle-to-grave approach to enable after-use crew items to augment vehicle systems. Specifically, AES LRR is investigating the direct reduction of clothing mass, the repurposing of logistical packaging, the use of autonomous logistics management technologies, the processing of spent crew items to benefit radiation shielding and water recovery, and the conversion of trash to propulsion gases. Reduction of mass has a corresponding and significant impact to logistical volume. The reduction of logistical volume can reduce the overall pressurized vehicle mass directly, or indirectly benefit the <span class="hlt">mission</span> by allowing for an increase in habitable volume during the <span class="hlt">mission</span>. The systematic implementation of these types of technologies will increase launch mass efficiency by enabling items to be used for secondary purposes and improve the habitability of the vehicle as <span class="hlt">mission</span> durations increase. Early studies have shown that the use of advanced logistics technologies can save approximately 20 m(sup 3) of volume during transit alone for a six-person Mars conjunction class <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cosp...40E2501P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cosp...40E2501P"><span>The ODINUS <span class="hlt">Mission</span> Concept: a <span class="hlt">Mission</span> for the exploration the Ice Giant Planets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peron, Roberto</p> <p></p> <p>We present the scientific case and the <span class="hlt">mission</span> concept of a proposal for the the comparative exploration of the ice giant planets Uranus and Neptune and their satellites with a pair of twin spacecraft: ODINUS (Origins, Dynamics and Interiors of Neptunian and Uranian Systems). The ODINUS proposal was submitted in response to the call for white papers for the definition of the themes of the L2 and L3 <span class="hlt">mission</span> in the framework of ESA Cosmic Vision 2015-2025 program. The goal of ODINUS is the advancement of our understanding of the ancient past of the Solar System and, more generally, of how planetary systems form and evolve. The <span class="hlt">mission</span> concept is focused on providing elements to answer to the scientific themes of the Cosmic Vision 2015-2025 program: What are the conditions for planetary formation and the emergency of <span class="hlt">life</span>? How does the Solar System work? What are the fundamental physical laws of the Universe? In order to achieve its goals, ODINUS foresees the use of two twin spacecraft to be placed in orbit around Uranus and Neptune respectively, with selected flybys of their satellites. The proposed measurements aim to study the atmospheres and magnetospheres of the planets, the surfaces of the satellites, and the interior structure and composition of both satellites and planets. An important possibility for performing fundamental physics studies (among them tests of general relativity theory) is offered by the cruise phase. After the extremely positive evaluation of ESA Senior Survey Committee, who stated that ``the exploration of the icy giants appears to be a timely milestone, fully appropriate for an L class <span class="hlt">mission</span>'', we discuss strategies to comparatively study Uranus and Neptune with future international <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110016241','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110016241"><span>The Use of the Integrated Medical Model for Forecasting and Mitigating Medical Risks for a Near-Earth Asteroid <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kerstman, Eric; Saile, Lynn; Freire de Carvalho, Mary; Myers, Jerry; Walton, Marlei; Butler, Douglas; Lopez, Vilma</p> <p>2011-01-01</p> <p>Introduction The Integrated Medical Model (IMM) is a decision support tool that is useful to space flight <span class="hlt">mission</span> managers and medical system designers in assessing risks and optimizing medical systems. The IMM employs an evidence-based, probabilistic risk assessment (PRA) approach within the operational constraints of space flight. Methods Stochastic computational methods are used to forecast probability distributions of medical events, crew health metrics, medical resource utilization, and probability estimates of medical evacuation and loss of crew <span class="hlt">life</span>. The IMM can also optimize medical kits within the constraints of mass and volume for specified <span class="hlt">missions</span>. The IMM was used to forecast medical evacuation and loss of crew <span class="hlt">life</span> probabilities, as well as crew health metrics for a near-earth asteroid (NEA) <span class="hlt">mission</span>. An optimized medical kit for this <span class="hlt">mission</span> was proposed based on the IMM simulation. Discussion The IMM can provide information to the space program regarding medical risks, including crew medical impairment, medical evacuation and loss of crew <span class="hlt">life</span>. This information is valuable to <span class="hlt">mission</span> managers and the space medicine community in assessing risk and developing mitigation strategies. Exploration <span class="hlt">missions</span> such as NEA <span class="hlt">missions</span> will have significant mass and volume constraints applied to the medical system. Appropriate allocation of medical resources will be critical to <span class="hlt">mission</span> success. The IMM capability of optimizing medical systems based on specific crew and <span class="hlt">mission</span> profiles will be advantageous to medical system designers. Conclusion The IMM is a decision support tool that can provide estimates of the impact of medical events on human space flight <span class="hlt">missions</span>, such as crew impairment, evacuation, and loss of crew <span class="hlt">life</span>. It can be used to support the development of mitigation strategies and to propose optimized medical systems for specified space flight <span class="hlt">missions</span>. Learning Objectives The audience will learn how an evidence-based decision support tool can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=PHILOSOPHY+AND+HUMAN&pg=2&id=EJ1030106','ERIC'); return false;" href="https://eric.ed.gov/?q=PHILOSOPHY+AND+HUMAN&pg=2&id=EJ1030106"><span>A Strengthened Teaching <span class="hlt">Mission</span> in Preschool: Teachers' Experiences, Beliefs and Strategies</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Westman, Susanne; Bergmark, Ulrika</p> <p>2014-01-01</p> <p>This paper aimed to explore how preschool teachers' experience their strengthened teaching <span class="hlt">mission</span>, specifically when working with scientific exploration. The study was based on the philosophy of the <span class="hlt">life</span>-world, a branch of the phenomenological movement. <span class="hlt">Life</span>-world philosophy focuses on the concrete reality humans inhabit and is responsive to its…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=KSC-01PP-1087&hterms=1087&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3D%2526%25231087','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=KSC-01PP-1087&hterms=1087&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3D%2526%25231087"><span>STS-107 <span class="hlt">Mission</span> INSIGNIA</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2001-01-01</p> <p>JOHNSON SPACE CENTER, HOUSON, TEXAS -- STS-107 INSIGNIA -- This is the insignia for STS-107, which is a multi-discipline microgravity and Earth science research <span class="hlt">mission</span> with a multitude of international scientific investigations conducted continuously during the planned 16 days on orbit. The central element of the patch is the microgravity symbol flowing into the rays of the astronaut symbol. The <span class="hlt">mission</span> inclination is portrayed by the 39-degree angle of the astronaut symbol to the Earth's horizon. The sunrise is representative of the numerous experiments that are the dawn of a new era for continued microgravity research on the International Space Station and beyond. The breadth of science conducted on this <span class="hlt">mission</span> will have widespread benefits to <span class="hlt">life</span> on Earth and our continued exploration of space, illustrated by the Earth and stars. The constellation Columba (the dove) was chosen to symbolize peace on Earth and the Space Shuttle Columbia. The seven stars also represent the <span class="hlt">mission</span> crew members and honor the original astronauts who paved the way to make research in space possible. The Israeli flag is adjacent to the name of the payload specialist who is the first person from that country to fly on the Space Shuttle. The NASA insignia design for Space Shuttle flights is reserved for use by the astronauts and for other official use as the NASA Administrator may authorize. Public availability has been approved only in the form of illustrations by the various news media. When and if there is any change in this policy, which we do not anticipate, it will be publicly announced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010cosp...38.3331P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010cosp...38.3331P"><span>EXPOSE-R on <span class="hlt">Mission</span> on the ISS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Panitz, Corinna; Rabbow, Elke; Rettberg, Petra; Barczyk, Simon; Kloss, Maria; Reitz, Guenther</p> <p></p> <p>Currently EXPOSE-R is on <span class="hlt">mission</span>! This astrobiological exposure facility was accommodated at the universal workplace URM-D Zenith payload site, located outside the Russian Svezda Module of the International Space Station (ISS) by extravehicular activity (EVA) on March 10th 2009. It contains 3 trays accommodating 12 sample compartments with sample carriers in three levels either open to space vacuum or kept in a defined gas environment. In its 8 experiments of biological and chemical content, more than 1200 individual samples are exposed to solar ultraviolet (UV) radiations, vacuum, cosmic rays or extreme temperature variations. In their different experiments the involved scientists are studying the question of <span class="hlt">life</span>'s origin on Earth and the results of their experiments are contributing to different aspects of the evolution and distribution of <span class="hlt">life</span> in the Universe. Additionally integrated into the EXPOSE-R facility are several dosimeters monitoring the ionising and the solar UV-radiation during the <span class="hlt">mission</span> to deliver useful information to complement the sample analysis. In close cooperation with the DLR and the Technical University Munich (TUM), the Rheinisch -Westfülische Technischen Hochschule Aachen (RWTH Aachen) operates the experiment "Spores". a This is one of the 6 astrobiological experiments of the ROSE-Consortium" (Response of Or-ganisms to Space Environment) of the EXPOSE-R <span class="hlt">mission</span>. In these experiments spores of bacteria, fungi and ferns are being over layered or mixed with meteorite material. The analysis of the effect of the space parameters on different biological endpoints of the spores of the mi-croorganism Bacillus subtilis will be performed after the retrieval of the experiment scheduled for the end of 2010. Parallel to the space <span class="hlt">mission</span> an identical set of samples was accommodated into EXPOSE-R trays identical in construction to perform the <span class="hlt">Mission</span> Ground Reference (MGR) Test. Currently this MGR Test is carried out in the Planetary and Space</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AsBio...8..921S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AsBio...8..921S"><span>The 2005 MARTE Robotic Drilling Experiment in Río Tinto, Spain: Objectives, Approach, and Results of a Simulated <span class="hlt">Mission</span> to Search for <span class="hlt">Life</span> in the Martian Subsurface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stoker, Carol R.; Cannon, Howard N.; Dunagan, Stephen E.; Lemke, Lawrence G.; Glass, Brian J.; Miller, David; Gomez-Elvira, Javier; Davis, Kiel; Zavaleta, Jhony; Winterholler, Alois; Roman, Matt; Rodriguez-Manfredi, Jose Antonio; Bonaccorsi, Rosalba; Bell, Mary Sue; Brown, Adrian; Battler, Melissa; Chen, Bin; Cooper, George; Davidson, Mark; Fernández-Remolar, David; Gonzales-Pastor, Eduardo; Heldmann, Jennifer L.; Martínez-Frías, Jesus; Parro, Victor; Prieto-Ballesteros, Olga; Sutter, Brad; Schuerger, Andrew C.; Schutt, John; Rull, Fernando</p> <p>2008-10-01</p> <p>The Mars Astrobiology Research and Technology Experiment (MARTE) simulated a robotic drilling <span class="hlt">mission</span> to search for subsurface <span class="hlt">life</span> on Mars. The drill site was on Peña de Hierro near the headwaters of the Río Tinto river (southwest Spain), on a deposit that includes massive sulfides and their gossanized remains that resemble some iron and sulfur minerals found on Mars. The <span class="hlt">mission</span> used a fluidless, 10-axis, autonomous coring drill mounted on a simulated lander. Cores were faced; then instruments collected color wide-angle context images, color microscopic images, visible near infrared point spectra, and (lower resolution) visible-near infrared hyperspectral images. Cores were then stored for further processing or ejected. A borehole inspection system collected panoramic imaging and Raman spectra of borehole walls. <span class="hlt">Life</span> detection was performed on full cores with an adenosine triphosphate luciferin-luciferase bioluminescence assay and on crushed core sections with SOLID2, an antibody array-based instrument. Two remotely located science teams analyzed the remote sensing data and chose subsample locations. In 30 days of operation, the drill penetrated to 6 m and collected 21 cores. Biosignatures were detected in 12 of 15 samples analyzed by SOLID2. Science teams correctly interpreted the nature of the deposits drilled as compared to the ground truth. This experiment shows that drilling to search for subsurface <span class="hlt">life</span> on Mars is technically feasible and scientifically rewarding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19032053','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19032053"><span>The 2005 MARTE Robotic Drilling Experiment in Río Tinto, Spain: objectives, approach, and results of a simulated <span class="hlt">mission</span> to search for <span class="hlt">life</span> in the Martian subsurface.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Stoker, Carol R; Cannon, Howard N; Dunagan, Stephen E; Lemke, Lawrence G; Glass, Brian J; Miller, David; Gomez-Elvira, Javier; Davis, Kiel; Zavaleta, Jhony; Winterholler, Alois; Roman, Matt; Rodriguez-Manfredi, Jose Antonio; Bonaccorsi, Rosalba; Bell, Mary Sue; Brown, Adrian; Battler, Melissa; Chen, Bin; Cooper, George; Davidson, Mark; Fernández-Remolar, David; Gonzales-Pastor, Eduardo; Heldmann, Jennifer L; Martínez-Frías, Jesus; Parro, Victor; Prieto-Ballesteros, Olga; Sutter, Brad; Schuerger, Andrew C; Schutt, John; Rull, Fernando</p> <p>2008-10-01</p> <p>The Mars Astrobiology Research and Technology Experiment (MARTE) simulated a robotic drilling <span class="hlt">mission</span> to search for subsurface <span class="hlt">life</span> on Mars. The drill site was on Peña de Hierro near the headwaters of the Río Tinto river (southwest Spain), on a deposit that includes massive sulfides and their gossanized remains that resemble some iron and sulfur minerals found on Mars. The <span class="hlt">mission</span> used a fluidless, 10-axis, autonomous coring drill mounted on a simulated lander. Cores were faced; then instruments collected color wide-angle context images, color microscopic images, visible-near infrared point spectra, and (lower resolution) visible-near infrared hyperspectral images. Cores were then stored for further processing or ejected. A borehole inspection system collected panoramic imaging and Raman spectra of borehole walls. <span class="hlt">Life</span> detection was performed on full cores with an adenosine triphosphate luciferin-luciferase bioluminescence assay and on crushed core sections with SOLID2, an antibody array-based instrument. Two remotely located science teams analyzed the remote sensing data and chose subsample locations. In 30 days of operation, the drill penetrated to 6 m and collected 21 cores. Biosignatures were detected in 12 of 15 samples analyzed by SOLID2. Science teams correctly interpreted the nature of the deposits drilled as compared to the ground truth. This experiment shows that drilling to search for subsurface <span class="hlt">life</span> on Mars is technically feasible and scientifically rewarding.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060019173&hterms=advanced+performance+management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dadvanced%2Bperformance%2Bmanagement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060019173&hterms=advanced+performance+management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dadvanced%2Bperformance%2Bmanagement"><span>Developing Advanced Support Technologies for Planetary Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Berdich, Debra P.; Campbel, Paul D.; Jernigan, J. Mark</p> <p>2004-01-01</p> <p>The United States Vision for Space Exploration calls for sending robots and humans to explore the Earth s moon, the planet Mars, and beyond. The National Aeronautics and Space Administration (NASA) is developing a set of design reference <span class="hlt">missions</span> that will provide further detail to these plans. Lunar <span class="hlt">missions</span> are expected to provide a stepping stone, through operational research and evaluation, in developing the knowledge base necessary to send crews on long duration <span class="hlt">missions</span> to Mars and other distant destinations. The NASA Exploration Systems Directorate (ExSD), in its program of bioastronautics research, manages the development of technologies that maintain human <span class="hlt">life</span>, health, and performance in space. Using a systems engineering process and risk management methods, ExSD s Human Support Systems (HSS) Program selects and performs research and technology development in several critical areas and transfers the results of its efforts to NASA exploration <span class="hlt">mission</span>/systems development programs in the form of developed technologies and new knowledge about the capabilities and constraints of systems required to support human existence beyond Low Earth Orbit. HSS efforts include the areas of advanced environmental monitoring and control, extravehicular activity, food technologies, <span class="hlt">life</span> support systems, space human factors engineering, and systems integration of all these elements. The HSS Program provides a structured set of deliverable products to meet the needs of exploration programs. these products reduce the gaps that exist in our knowledge of and capabilities for human support for long duration, remote space <span class="hlt">missions</span>. They also reduce the performance gap between the efficiency of current space systems and the greater efficiency that must be achieved to make human planetary exploration <span class="hlt">missions</span> economically and logistically feasible. In conducting this research and technology development program, it is necessary for HSS technologists and program managers to develop a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160011154','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160011154"><span>The Role of Synthetic Biology in NASA's <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rothschild, Lynn J.</p> <p>2016-01-01</p> <p>The time has come to for NASA to exploit synthetic biology in pursuit of its <span class="hlt">missions</span>, including aeronautics, earth science, astrobiology and most notably, human exploration. Conversely, NASA advances the fundamental technology of synthetic biology as no one else can because of its unique expertise in the origin of <span class="hlt">life</span> and <span class="hlt">life</span> in extreme environments, including the potential for alternate <span class="hlt">life</span> forms. This enables unique, creative "game changing" advances. NASA's requirement for minimizing upmass in flight will also drive the field toward miniaturization and automation. These drivers will greatly increase the utility of synthetic biology solutions for military, health in remote areas and commercial purposes. To this end, we have begun a program at NASA to explore the use of synthetic biology in NASA's <span class="hlt">missions</span>, particular space exploration. As part of this program, we began hosting an iGEM team of undergraduates drawn from Brown and Stanford Universities to conduct synthetic biology research at NASA Ames Research Center. The 2011 team (http://2011.igem.org/Team:Brown-Stanford) produced an award-winning project on using synthetic biology as a basis for a human Mars settlement.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AIPC..746.1188M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AIPC..746.1188M"><span>Technical Feasibility Assessment of Lunar Base <span class="hlt">Mission</span> Scenarios</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Magelssen, Trygve ``Spike''; Sadeh, Eligar</p> <p>2005-02-01</p> <p>Investigation of the literature pertaining to lunar base (LB) <span class="hlt">missions</span> and the technologies required for LB development has revealed an information gap that hinders technical feasibility assessment. This information gap is the absence of technical readiness levels (TRL) (Mankins, 1995) and information pertaining to the criticality of the critical enabling technologies (CETs) that enable <span class="hlt">mission</span> success. TRL is a means of identifying technical readiness stages of a technology. Criticality is defined as the level of influence the CET has on the <span class="hlt">mission</span> scenario. The hypothesis of this research study is that technical feasibility is a function of technical readiness and technical readiness is a function of criticality. A newly developed research analysis method is used to identify the technical feasibility of LB <span class="hlt">mission</span> scenarios. A Delphi is used to ascertain technical readiness levels and CET criticality-to-<span class="hlt">mission</span>. The research analysis method is applied to the Delphi results to determine the technical feasibility of the LB <span class="hlt">mission</span> scenarios that include: observatory, science research, lunar settlement, space exploration gateway, space resource utilization, and space tourism. The CETs identified encompasses four major system level technologies of: transportation, <span class="hlt">life</span> support, structures, and power systems. Results of the technical feasibility assessment show the observatory and science research LB <span class="hlt">mission</span> scenarios to be more technical ready out of all the scenarios, but all <span class="hlt">mission</span> scenarios are in very close proximity to each other in regard to criticality and TRL and no one <span class="hlt">mission</span> scenario stands out as being absolutely more technically ready than any of the other scenarios. What is significant and of value are the Delphi results concerning CET criticality-to-<span class="hlt">mission</span> and the TRL values evidenced in the Tables that can be used by anyone assessing the technical feasibility of LB <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11540213','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11540213"><span>Regenerative <span class="hlt">life</span> support systems--why do we need them?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Barta, D J; Henninger, D L</p> <p>1994-11-01</p> <p>Human exploration of the solar system will include <span class="hlt">missions</span> lasting years at a time. Such <span class="hlt">missions</span> mandate extensive regeneration of <span class="hlt">life</span> support consumables with efficient utilization of local planetary resources. As <span class="hlt">mission</span> durations extend beyond one or two years, regenerable human <span class="hlt">life</span> support systems which supply food and recycle air, water, and wastes become feasible; resupply of large volumes and masses of food, water, and atmospheric gases become unrealistic. Additionally, reduced dependency on resupply or self sufficiency can be an added benefit to human crews in hostile environments far from the security of Earth. Comparisons of resupply and regeneration will be discussed along with possible scenarios for developing and implementing human <span class="hlt">life</span> support systems on the Moon and Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AIPC..813..173F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AIPC..813..173F"><span>A Nuclear Powered ISRU <span class="hlt">Mission</span> to Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finzi, Elvina; Davighi, Andrea; Finzi, Amalia</p> <p>2006-01-01</p> <p>Space exploration has always been drastically constrained by the masses that can be launched into orbit; Hence affordable planning and execution of prolonged manned space <span class="hlt">missions</span> depend upon the utilization of local. Successful in-situ resources utilization (ISRU) is a key element to allow the human presence on Mars or the Moon. In fact a Mars ISRU <span class="hlt">mission</span> is planned in the Aurora Program, the European program for the exploration of the solar system. Orpheus <span class="hlt">mission</span> is a technological demonstrator whose purpose is to show the advantages of an In Situ Propellant Production (ISPP). Main task of this work is to demonstrate the feasibility of a nuclear ISPP plant. The <span class="hlt">mission</span> designed has been sized to launch back form Mars an eventual manned module. The ISPP <span class="hlt">mission</span> requires two different: the ISPP power plant module and the nuclear reactor module. Both modules reach the escape orbit thanks to the launcher upper stage, after a 200 days cruising phase the Martian atmosphere is reached thanks to small DV propelled manoeuvres, aerobreaking and soft landing. During its operational <span class="hlt">life</span> the ISPP plant produces. The propellant is produced in one synodic year. 35000 kg of Ethylene are produced at the Martian equator. The resulting systems appear feasible and of a size comparable to other ISRU <span class="hlt">mission</span> designs. This <span class="hlt">mission</span> seems challenging not only for the ISPP technology to be demonstrated, but also for the space nuclear reactor considered; Though this seems the only way to allow a permanent human presence on Mars surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170006519','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170006519"><span>Human Mars Surface <span class="hlt">Mission</span> Nuclear Power Considerations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rucker, Michelle A.</p> <p>2018-01-01</p> <p>A key decision facing Mars <span class="hlt">mission</span> designers is how to power a crewed surface field station. Unlike the solar-powered Mars Exploration Rovers (MER) that could retreat to a very low power state during a Martian dust storm, human Mars surface <span class="hlt">missions</span> are estimated to need at least 15 kilowatts of electrical (kWe) power simply to maintain critical <span class="hlt">life</span> support and spacecraft functions. 'Hotel' loads alone for a pressurized crew rover approach two kWe; driving requires another five kWe-well beyond what the Curiosity rover’s Radioisotope Power System (RPS) was designed to deliver. Full operation of a four-crew Mars field station is estimated at about 40 kWe. Clearly, a crewed Mars field station will require a substantial and reliable power source, beyond the scale of robotic <span class="hlt">mission</span> experience. This paper explores the applications for both fission and RPS nuclear options for Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110011623','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110011623"><span>Altair Lander <span class="hlt">Life</span> Support: Design Analysis Cycles 4 and 5</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, Molly; Curley, Su; Rotter, Henry; Stambaugh, Imelda; Yagoda, Evan</p> <p>2011-01-01</p> <p><span class="hlt">Life</span> support systems are a critical part of human exploration beyond low earth orbit. NASA s Altair Lunar Lander team is pursuing efficient solutions to the technical challenges of human spaceflight. <span class="hlt">Life</span> support design efforts up through Design Analysis Cycle (DAC) 4 focused on finding lightweight and reliable solutions for the Sortie and Outpost <span class="hlt">missions</span> within the Constellation Program. In DAC-4 and later follow on work, changes were made to add functionality for new requirements accepted by the Altair project, and to update the design as knowledge about certain issues or hardware matured. In DAC-5, the Altair project began to consider <span class="hlt">mission</span> architectures outside the Constellation baseline. Selecting the optimal <span class="hlt">life</span> support system design is very sensitive to <span class="hlt">mission</span> duration. When the <span class="hlt">mission</span> goals and architecture change several trade studies must be conducted to determine the appropriate design. Finally, several areas of work developed through the Altair project may be applicable to other vehicle concepts for microgravity <span class="hlt">missions</span>. Maturing the Altair <span class="hlt">life</span> support system related analysis, design, and requirements can provide important information for developers of a wide range of other human vehicles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100038344','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100038344"><span>Altair Lander <span class="hlt">Life</span> Support: Design Analysis Cycles 4 and 5</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Anderson, Molly; Curley, Su; Rotter, Henry; Yagoda, Evan</p> <p>2010-01-01</p> <p><span class="hlt">Life</span> support systems are a critical part of human exploration beyond low earth orbit. NASA s Altair Lunar Lander team is pursuing efficient solutions to the technical challenges of human spaceflight. <span class="hlt">Life</span> support design efforts up through Design Analysis Cycle (DAC) 4 focused on finding lightweight and reliable solutions for the Sortie and Outpost <span class="hlt">missions</span> within the Constellation Program. In DAC-4 and later follow on work, changes were made to add functionality for new requirements accepted by the Altair project, and to update the design as knowledge about certain issues or hardware matured. In DAC-5, the Altair project began to consider <span class="hlt">mission</span> architectures outside the Constellation baseline. Selecting the optimal <span class="hlt">life</span> support system design is very sensitive to <span class="hlt">mission</span> duration. When the <span class="hlt">mission</span> goals and architecture change several trade studies must be conducted to determine the appropriate design. Finally, several areas of work developed through the Altair project may be applicable to other vehicle concepts for microgravity <span class="hlt">missions</span>. Maturing the Altair <span class="hlt">life</span> support system related analysis, design, and requirements can provide important information for developers of a wide range of other human vehicles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140016932','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140016932"><span>Asteroid Redirect Crewed <span class="hlt">Mission</span> Space Suit and EVA System Maturation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bowie, Jonathan; Buffington, Jesse; Hood, Drew; Kelly, Cody; Naids, Adam; Watson, Richard</p> <p>2015-01-01</p> <p>The Asteroid Redirect Crewed <span class="hlt">Mission</span> (ARCM) requires a Launch/Entry/Abort (LEA) suit capability and short duration Extra Vehicular Activity (EVA) capability from the Orion spacecraft. For this <span class="hlt">mission</span>, the pressure garment selected for both functions is the Modified Advanced Crew Escape Suit (MACES) with EVA enhancements and the <span class="hlt">life</span> support option that was selected is the Exploration Portable <span class="hlt">Life</span> Support System (PLSS) currently under development for Advanced Exploration Systems (AES). The proposed architecture meets the ARCM constraints, but much more work is required to determine the details of the suit upgrades, the integration with the PLSS, and the tools and equipment necessary to accomplish the <span class="hlt">mission</span>. This work has continued over the last year to better define the operations and hardware maturation of these systems. EVA simulations were completed in the Neutral Buoyancy Lab (NBL) and interfacing options were prototyped and analyzed with testing planned for late 2014. This paper discusses the work done over the last year on the MACES enhancements, the use of tools while using the suit, and the integration of the PLSS with the MACES.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140009938','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140009938"><span>Asteroid Redirect Crewed <span class="hlt">Mission</span> Space Suit and EVA System Maturation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bowie, Jonathan T.; Kelly, Cody; Buffington, Jesse; Watson, Richard D.</p> <p>2015-01-01</p> <p>The Asteroid Redirect Crewed <span class="hlt">Mission</span> (ARCM) requires a Launch/Entry/Abort (LEA) suit capability and short duration Extra Vehicular Activity (EVA) capability from the Orion spacecraft. For this <span class="hlt">mission</span>, the pressure garment that was selected, for both functions, is the Modified Advanced Crew Escape Suit (MACES) with EVA enhancements and the <span class="hlt">life</span> support option that was selected is the Exploration Portable <span class="hlt">Life</span> Support System (PLSS). The proposed architecture was found to meet the <span class="hlt">mission</span> constraints, but much more work is required to determine the details of the required suit upgrades, the integration with the PLSS, and the rest of the tools and equipment required to accomplish the <span class="hlt">mission</span>. This work has continued over the last year to better define the operations and hardware maturation of these systems. EVA simulations have been completed in the NBL and interfacing options have been prototyped and analyzed with testing planned for late 2014. For NBL EVA simulations, in 2013, components were procured to allow in-house build up for four new suits with mobility enhancements built into the arms. Boots outfitted with clips that fit into foot restraints have also been added to the suit and analyzed for possible loads. Major suit objectives accomplished this year in testing include: evaluation of mobility enhancements, ingress/egress of foot restraint, use of foot restraint for worksite stability, ingress/egress of Orion hatch with PLSS mockup, and testing with two crew members in the water at one time to evaluate the crew's ability to help one another. Major tool objectives accomplished this year include using various other methods for worksite stability, testing new methods for asteroid geologic sampling and improving the fidelity of the mockups and crew equipment. These tests were completed on a medium fidelity capsule mockup, asteroid vehicle mockup, and asteroid mockups that were more accurate for an asteroid type EVA than previous tests. Another focus was the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140009934','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140009934"><span>Potential <span class="hlt">Mission</span> Scenarios Post Asteroid Crewed <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lopez, Pedro, Jr.; McDonald, Mark A.</p> <p>2015-01-01</p> <p>A deep-space <span class="hlt">mission</span> has been proposed to identify and redirect an asteroid to a distant retrograde orbit around the moon, and explore it by sending a crew using the Space Launch System and the Orion spacecraft. The Asteroid Redirect Crewed <span class="hlt">Mission</span> (ARCM), which represents the third segment of the Asteroid Redirect <span class="hlt">Mission</span> (ARM), could be performed on EM-3 or EM-4 depending on asteroid return date. Recent NASA studies have raised questions on how we could progress from current Human Space Flight (HSF) efforts to longer term human exploration of Mars. This paper will describe the benefits of execution of the ARM as the initial stepping stone towards Mars exploration, and how the capabilities required to send humans to Mars could be built upon those developed for the asteroid <span class="hlt">mission</span>. A series of potential interim <span class="hlt">missions</span> aimed at developing such capabilities will be described, and the feasibility of such <span class="hlt">mission</span> manifest will be discussed. Options for the asteroid crewed <span class="hlt">mission</span> will also be addressed, including crew size and <span class="hlt">mission</span> duration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Department+AND+Defense&pg=6&id=EJ988147','ERIC'); return false;" href="https://eric.ed.gov/?q=Department+AND+Defense&pg=6&id=EJ988147"><span>Understanding the Importance of <span class="hlt">Life</span> <span class="hlt">Mission</span> when Advising Soldiers</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Wilson, Kristen; Smith, Natesha</p> <p>2012-01-01</p> <p>Since the military became an all-voluntary force (AVF), men and women have chosen to serve as a career, viewing it as a way to accomplish their <span class="hlt">life</span> goals. Whether these goals include advancing in rank or transitioning into civilian <span class="hlt">life</span>, service members find themselves needing additional training and/or education while serving. Although the…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960002976','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960002976"><span>Low Cost <span class="hlt">Mission</span> Operations Workshop. [Space <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1994-01-01</p> <p>The presentations given at the Low Cost (Space) <span class="hlt">Mission</span> Operations (LCMO) Workshop are outlined. The LCMO concepts are covered in four introductory sections: Definition of <span class="hlt">Mission</span> Operations (OPS); <span class="hlt">Mission</span> Operations (MOS) Elements; The Operations Concept; and <span class="hlt">Mission</span> Operations for Two Classes of <span class="hlt">Missions</span> (operationally simple and complex). Individual presentations cover the following topics: Science Data Processing and Analysis; Mis sion Design, Planning, and Sequencing; Data Transport and Delivery, and <span class="hlt">Mission</span> Coordination and Engineering Analysis. A list of panelists who participated in the conference is included along with a listing of the contact persons for obtaining more information concerning LCMO at JPL. The presentation of this document is in outline and graphic form.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080012646','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080012646"><span>Cluster: <span class="hlt">Mission</span> Overview and End-of-<span class="hlt">Life</span> Analysis</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pallaschke, S.; Munoz, I.; Rodriquez-Canabal, J.; Sieg, D.; Yde, J. J.</p> <p>2007-01-01</p> <p>The Cluster <span class="hlt">mission</span> is part of the scientific programme of the European Space Agency (ESA) and its purpose is the analysis of the Earth's magnetosphere. The Cluster project consists of four satellites. The selected polar orbit has a shape of 4.0 and 19.2 Re which is required for performing measurements near the cusp and the tail of the magnetosphere. When crossing these regions the satellites form a constellation which in most of the cases so far has been a regular tetrahedron. The satellite operations are carried out by the European Space Operations Centre (ESOC) at Darmstadt, Germany. The paper outlines the future orbit evolution and the envisaged operations from a Flight Dynamics point of view. In addition a brief summary of the LEOP and routine operations is included beforehand.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880006447','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880006447"><span>Space station accommodations for <span class="hlt">life</span> sciences research facilities. Phase 1: Conceptual design and programmatics studies for <span class="hlt">Missions</span> SAAX0307, SAAX0302 and the transition from SAAX0307 to SAAX0302. Volume 2: Study results</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1986-01-01</p> <p>Lockheed Missiles and Space Company's conceptual designs and programmatics for a Space Station Nonhuman <span class="hlt">Life</span> Sciences Research Facility (LSRF) are presented. Conceptual designs and programmatics encompass an Initial Orbital Capability (IOC) LSRF, a growth or follow-on Orbital Capability (FOC), and the transitional process required to modify the IOC LSFR to the FOC LSFR. The IOC and FOC LSFRs correspond to <span class="hlt">missions</span> SAAX0307 and SAAX0302 of the Space Station <span class="hlt">Mission</span> Requirements Database, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSM.P13A..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSM.P13A..02H"><span>The Europa Jupiter System <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hendrix, A. R.; Clark, K.; Erd, C.; Pappalardo, R.; Greeley, R. R.; Blanc, M.; Lebreton, J.; van Houten, T.</p> <p>2009-05-01</p> <p> formation and evolution of gas giant planets and their satellites will be better known. Most important, EJSM will shed new light on the potential for the emergence of <span class="hlt">life</span> in the celestial neighborhood and beyond. The EJSM <span class="hlt">mission</span> architecture provides opportunities for coordinated synergistic observations by JEO and JGO of the Jupiter and Ganymede magnetospheres, the volcanoes and torus of Io, the atmosphere of Jupiter, and comparative planetology of icy satellites. Each spacecraft could and would conduct "stand-alone" measurements, including the detailed investigation of Europa and Ganymede, providing significant programmatic flexibility. Although engineering advances are needed for JEO (radiation designs) and JGO, no new technologies will be required to execute either EJSM <span class="hlt">mission</span> element. The development schedule for the <span class="hlt">mission</span> is such that a technology developed by 2012 - 2013 could easily be incorporated if it enhances the <span class="hlt">mission</span> capability. Risk mitigation activities are under way to ensure that the radiation designs are implemented in the lowest-risk approach. The baseline <span class="hlt">mission</span> concepts include robust mass and power margins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cosp...40E2438P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cosp...40E2438P"><span>The Europa Clipper <span class="hlt">mission</span> concept</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pappalardo, Robert; Lopes, Rosaly</p> <p></p> <p>Jupiter's moon Europa may be a habitable world. Galileo spacecraft data suggest that an ocean most likely exists beneath Europa’s icy surface and that the “ingredients” necessary for <span class="hlt">life</span> (liquid water, chemistry, and energy) could be present within this ocean today. Because of the potential for revolutionizing our understanding of <span class="hlt">life</span> in the solar system, future exploration of Europa has been deemed an extremely high priority for planetary science. A NASA-appointed Science Definition Team (SDT), working closely with a technical team from the Jet Propulsion Laboratory (JPL) and the Applied Physics Laboratory (APL), recently considered options for a future strategic <span class="hlt">mission</span> to Europa, with the stated science goal: Explore Europa to investigate its habitability. The group considered several <span class="hlt">mission</span> options, which were fully technically developed, then costed and reviewed by technical review boards and planetary science community groups. There was strong convergence on a favored architecture consisting of a spacecraft in Jupiter orbit making many close flybys of Europa, concentrating on remote sensing to explore the moon. Innovative <span class="hlt">mission</span> design would use gravitational perturbations of the spacecraft trajectory to permit flybys at a wide variety of latitudes and longitudes, enabling globally distributed regional coverage of the moon’s surface, with nominally 45 close flybys at altitudes from 25 to 100 km. We will present the science and reconnaissance goals and objectives, a <span class="hlt">mission</span> design overview, and the notional spacecraft for this concept, which has become known as the Europa Clipper. The Europa Clipper concept provides a cost-efficient means to explore Europa and investigate its habitability, through understanding the satellite’s ice and ocean, composition, and geology. The set of investigations derived from these science objectives traces to a notional payload for science, consisting of: Ice Penetrating Radar (for sounding of ice-water interfaces</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920038364&hterms=food+category&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dfood%2Bcategory','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920038364&hterms=food+category&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dfood%2Bcategory"><span><span class="hlt">Life</span> support systems for Mars transit</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Macelroy, R. D.; Kliss, M.; Straight, C.</p> <p>1992-01-01</p> <p>The structural elements of <span class="hlt">life</span>-support systems are reviewed in order to assess the suitability of specific features for use during a Mars <span class="hlt">mission</span>. <span class="hlt">Life</span>-support requirements are estimated by means of an approximate input/output analysis, and the advantages are listed relating to the use of recycling and regeneration techniques. The technological options for regeneration are presented in categories such as CO2 reduction, organics removal, polishing, food production, and organics oxidation. These data form the basis of proposed <span class="hlt">mission</span> requirements and constraints as well as the definition of what constitutes an adequate reserve. Regenerative physical/chemical <span class="hlt">life</span>-support systems are championed based exclusively on the mass savings inherent in the technology. The resiliency and 'soft' failure modes of bioregenerative <span class="hlt">life</span>-support systems are identified as areas of investigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950005502','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950005502"><span>Modeling and <span class="hlt">life</span> prediction methodology for Titanium Matrix Composites subjected to <span class="hlt">mission</span> profiles</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mirdamadi, M.; Johnson, W. S.</p> <p>1994-01-01</p> <p>Titanium matrix composites (TMC) are being evaluated as structural materials for elevated temperature applications in future generation hypersonic vehicles. In such applications, TMC components are subjected to complex thermomechanical loading profiles at various elevated temperatures. Therefore, thermomechanical fatigue (TMF) testing, using a simulated <span class="hlt">mission</span> profile, is essential for evaluation and development of <span class="hlt">life</span> prediction methodologies. The objective of the research presented in this paper was to evaluate the TMF response of the (0/90)2s SCS-6/Timetal-21S subjected to a generic hypersonic flight profile and its portions with a temperature ranging from -130 C to 816 C. It was found that the composite modulus, prior to rapid degradation, had consistent values for all the profiles tested. A micromechanics based analysis was used to predict the stress-strain response of the laminate and of the constituents in each ply during thermomechanical loading conditions by using only constituent properties as input. The fiber was modeled as elastic with transverse orthotropic and temperature dependent properties. The matrix was modeled using a thermoviscoplastic constitutive relation. In the analysis, the composite modulus degradation was assumed to result from matrix cracking and was modeled by reducing the matrix modulus. Fatigue lives of the composite subjected to the complex generic hypersonic flight profile were well correlated using the predicted stress in 0 degree fibers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013382','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013382"><span>NASA Laboratory Analysis for Manned Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Krihak, Michael (Editor); Shaw, Tianna</p> <p>2014-01-01</p> <p>The Exploration Laboratory Analysis (ELA) project supports the Exploration Medical Capability Element under the NASA Human Research Program. ELA instrumentation is identified as an essential capability for future exploration <span class="hlt">missions</span> to diagnose and treat evidence-based medical conditions. However, <span class="hlt">mission</span> architecture limits the medical equipment, consumables, and procedures that will be available to treat medical conditions during human exploration <span class="hlt">missions</span>. Allocated resources such as mass, power, volume, and crew time must be used efficiently to optimize the delivery of in-flight medical care. Although commercial instruments can provide the blood and urine based measurements required for exploration <span class="hlt">missions</span>, these commercial-off-the-shelf devices are prohibitive for deployment in the space environment. The objective of the ELA project is to close the technology gap of current minimally invasive laboratory capabilities and analytical measurements in a manner that the <span class="hlt">mission</span> architecture constraints impose on exploration <span class="hlt">missions</span>. Besides micro gravity and radiation tolerances, other principal issues that generally fail to meet NASA requirements include excessive mass, volume, power and consumables, and nominal reagent shelf-<span class="hlt">life</span>. Though manned exploration <span class="hlt">missions</span> will not occur for nearly a decade, NASA has already taken strides towards meeting the development of ELA medical diagnostics by developing <span class="hlt">mission</span> requirements and concepts of operations that are coupled with strategic investments and partnerships towards meeting these challenges. This paper focuses on the remote environment, its challenges, biomedical diagnostics requirements and candidate technologies that may lead to successful blood/urine chemistry and biomolecular measurements in future space exploration <span class="hlt">missions</span>. SUMMARY The NASA Exploration Laboratory Analysis project seeks to develop capability to diagnose anticipated space exploration medical conditions on future manned <span class="hlt">missions</span>. To achieve</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990026747&hterms=indigenous+peoples&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dindigenous%2Bpeoples','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990026747&hterms=indigenous+peoples&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dindigenous%2Bpeoples"><span>Human Exploration of Mars: The Reference <span class="hlt">Mission</span> of the NASA Mars Exploration Study Team</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Connolly, John</p> <p>1998-01-01</p> <p>The Reference <span class="hlt">Mission</span> was developed over a period of several years and was published in NASA Special Publication 6107 in July 1997. The purpose of the Reference <span class="hlt">Mission</span> was to provide a workable model for the human exploration of Mars, which is described in enough detail that alternative strategies and implementations can be compared and evaluated. NASA is continuing to develop the Reference <span class="hlt">Mission</span> and expects to update this report in the near future. It was the purpose of the Reference <span class="hlt">Mission</span> to develop scenarios based on the needs of scientists and explorers who want to conduct research on Mars; however, more work on the surface-<span class="hlt">mission</span> aspects of the Reference <span class="hlt">Mission</span> is required and is getting under way. Some aspects of the Reference <span class="hlt">Mission</span> that are important for the consideration of the surface <span class="hlt">mission</span> definition include: (1) a split <span class="hlt">mission</span> strategy, which arrives at the surface two years before the arrival of the first crew; (2) three <span class="hlt">missions</span> to the outpost site over a 6-year period; (3) a plant capable of producing rocket propellant for lifting off Mars and caches of water, O, and inert gases for the <span class="hlt">life</span>-support system; (4) a hybrid physico-chemical/bioregenerative <span class="hlt">life</span>-support system, which emphasizes the bioregenerative system more in later parts of the scenario; (5) a nuclear reactor power supply, which provides enough power for all operations, including the operation of a bioregenerative <span class="hlt">life</span>-support system as well as the propellant and consumable plant; (6) capability for at least two people to be outside the habitat each day of the surface stay; (7) telerobotic and human-operated transportation vehicles, including a pressurized rover capable of supporting trips of several days' duration from the habitat; (7) crew stay times of 500 days on the surface, with six-person crews; and (8) multiple functional redundancies to reduce risks to the crews on the surface. New concepts are being sought that would reduce the overall cost for this exploration</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C13E0664H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C13E0664H"><span>FRAM-2012: Norwegians return to the High Arctic with a Hovercraft for Marine Geophysical Research</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hall, J. K.; Kristoffersen, Y.; Brekke, H.; Hope, G.</p> <p>2012-12-01</p> <p> became clear that to compensate for delayed rendezvous would take up substantially more <span class="hlt">icebreaker</span> time than initially agreed to. It was therefore decided that the hovercraft would remain in the Gakkel Ridge survey area while the <span class="hlt">icebreaker</span> would concentrate on its primary <span class="hlt">mission</span> objective, a Danish UNCLOS survey. The two vessels would rejoin for the return journey to Svalbard in early September. The hovercraft has made continuous ice thickness measurements along its track by a front-mounted electromagnetic survey instrument in combination with a sonic height measuring device. The poster will present the findings of the expedition, and a short video is under preparation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003ilu..book..149P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003ilu..book..149P"><span>The Search for Extraterrestrial <span class="hlt">Life</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peter, Ulmschneider</p> <p></p> <p>Looking at the nature, origin, and evolution of <span class="hlt">life</span> on Earth is one way of assessing whether extraterrestrial <span class="hlt">life</span> exists on Earth-like planets elsewhere (see Chaps. 5 and 6). A more direct approach is to search for favorable conditions and traces of <span class="hlt">life</span> on other celestial bodies, both in the solar system and beyond. Clearly, there is little chance of encountering nonhuman intelligent beings in the solar system. But there could well be primitive <span class="hlt">life</span> on Mars, particularly as in the early history of the solar system the conditions on Mars were quite similar to those on Earth. In addition, surprisingly favorable conditions for <span class="hlt">life</span> once existed on the moons of Jupiter. Yet even if extraterrestrial <span class="hlt">life</span> is not encountered in forthcoming space <span class="hlt">missions</span>, it would be of utmost importance to recover fossils of past organisms as such traces would greatly contribute to our basic understanding of the formation of <span class="hlt">life</span>. In addition to the planned <span class="hlt">missions</span> to Mars and Europa, there are extensive efforts to search for <span class="hlt">life</span> outside the solar system. Rapid advances in the detection of extrasolar planets, outlined in Chap. 3, are expected to lead to the discovery of Earth-like planets in the near future. But how can we detect <span class="hlt">life</span> on these distant bodies?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040021352&hterms=Football&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DFootball','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040021352&hterms=Football&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DFootball"><span>Compaction of Space <span class="hlt">Mission</span> Wastes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fisher, John; Pisharody, Suresh; Wignarajah, K.</p> <p>2004-01-01</p> <p>The current solid waste management system employed on the International Space Station (ISS) consists of compaction, storage, and disposal. Wastes such plastic food packaging and trash are compacted manually and wrapped in duct tape footballs by the astronauts. Much of the waste is simply loaded either into the empty Russian Progress vehicle for destruction on reentry or into Shuttle for return to Earth. This manual method is wasteful of crew time and does not transition well to far term <span class="hlt">missions</span>. Different wastes onboard spacecraft vary considerably in their characteristics and in the appropriate method of management. In advanced <span class="hlt">life</span> support systems for far term <span class="hlt">missions</span>, recovery of resources such as water from the wastes becomes important. However waste such as plastic food packaging, which constitutes a large fraction of solid waste (roughly 21% on ISS, more on long duration <span class="hlt">missions</span>), contains minimal recoverable resource. The appropriate management of plastic waste is waste stabilization and volume minimization rather than resource recovery. This paper describes work that has begun at Ames Research Center on development of a heat melt compactor that can be used on near term and future <span class="hlt">missions</span>, that can minimize crew interaction, and that can handle wastes with a significant plastic composition. The heat melt compactor takes advantage of the low melting point of plastics to compact plastic materials using a combination of heat and pressure. The US Navy has demonstrated successful development of a similar unit for shipboard application. Ames is building upon the basic approach demonstrated by the Navy to develop an advanced heat melt type compactor for space <span class="hlt">mission</span> type wastes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940000185&hterms=How+long+can+earth+support+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DHow%2Blong%2Bcan%2Bearth%2Bsupport%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940000185&hterms=How+long+can+earth+support+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DHow%2Blong%2Bcan%2Bearth%2Bsupport%2Blife"><span>Bioregenerative <span class="hlt">Life</span>-Support System For Long <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cullingford, Hatice S.</p> <p>1994-01-01</p> <p>Collection of four reports proposes integrated bioregenerative <span class="hlt">life</span>-support system that sustains tens of people isolated from Earth's oxygen and sunlight. System self-sufficient for year or more; continues beyond that period with replenishment of supplies. Used in long-term spaceflights, space stations, such planet bases as those on Earth's Moon or Mars, and submarine vehicles and installations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910030373&hterms=stallings+william&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dstallings%2Bwilliam','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910030373&hterms=stallings+william&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dstallings%2Bwilliam"><span>Multi-<span class="hlt">mission</span> space science data processing systems - Past, present, and future</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stallings, William H.</p> <p>1990-01-01</p> <p>Packetized telemetry that is consistent with the international Consultative Committee for Space Data Systems (CCSDS) has been baselined for future NASA <span class="hlt">missions</span> such as Space Station Freedom. Some experiences from past and present multimission systems are examined, including current experiences in implementing a CCSDS standard packetized data processing system, relative to the effectiveness of the multimission approach in lowering <span class="hlt">life</span> cycle cost and the complexity of meeting new <span class="hlt">mission</span> needs. It is shown that the continued effort toward standardization of telemetry and processing support will permit the development of multimission systems needed to meet the increased requirements of future NASA <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17511302','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17511302"><span>Biohazard potential of putative Martian organisms during <span class="hlt">missions</span> to Mars.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Warmflash, David; Larios-Sanz, Maia; Jones, Jeffrey; Fox, George E; McKay, David S</p> <p>2007-04-01</p> <p>Exploration Class <span class="hlt">missions</span> to Mars will require precautions against potential contamination by any native microorganisms that may be incidentally pathogenic to humans. While the results of NASA's Viking biology experiments of the 1970s have been generally interpreted as inconclusive for surface organisms, and attributed to active but nonbiological chemistries, the possibility of native surface <span class="hlt">life</span> has never been ruled out completely. It is possible that, prior to the first human landing on Mars, robotic craft and sample return <span class="hlt">missions</span> will provide enough data to know with certainty whether future human landing sites harbor extant <span class="hlt">life</span> forms. If native <span class="hlt">life</span> were found to exist, it would be problematic to determine whether any of its species might present a medical danger to astronauts. Therefore, it will become necessary to assess empirically the risk that the planet contains pathogens based on terrestrial examples of pathogenicity and to take a reasonably cautious approach to biohazard protection. A survey of terrestrial pathogens was conducted with special emphasis on those whose evolution has not depended on the presence of animal hosts. The history of the development and implementation of Apollo anti-contamination protocol and recommendations of the National Research Council's Space Studies Board regarding Mars were reviewed. Organisms can emerge in Nature in the absence of indigenous animal hosts and both infectious and non-infectious human pathogens are therefore theoretically possible on Mars. Although remote, the prospect of Martian surface <span class="hlt">life</span>, together with the existence of a diversity of routes by which pathogenicity has emerged on Earth, suggests that the probability of human pathogens on Mars, while low, is not zero. Still, since the discovery and study of Martian <span class="hlt">life</span> can have long-term benefits for humanity, the risk that Martian <span class="hlt">life</span> might include pathogens should not be an obstacle to human exploration. As a precaution, it is recommended that EVA</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950019664','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950019664"><span>The spacelab scientific <span class="hlt">missions</span>: A comprehensive bibliography of scientific publications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Torr, Marsha (Compiler)</p> <p>1995-01-01</p> <p>November 1993 represented the 10-year anniversary of the flight of Spacelab 1 <span class="hlt">mission</span>, with the first precursor <span class="hlt">mission</span> (OSTA-1) being launched 2 years earlier. Since that time, a total of 27 Shuttle <span class="hlt">missions</span> has been flown, using the Spacelab system as a facility for conducting scientific research in space. The <span class="hlt">missions</span> flown to date have allowed a total of approximately 500 Principle Investigator class investigations to be conducted in orbit. These investigations have constituted major scientific efforts in astronomy/astrophysics, atmospheric science, Earth observation, <span class="hlt">life</span> sciences, microgravity science, and space plasma physics. An initial survey of the scientific products gleaned from Spacelab <span class="hlt">missions</span> already flown was sent to the Principle Investigators. In that survey, information was gathered from the investigators on the scientific highlights of their investigations and statistical measurements of overall success -- such as papers published. This document is a compilation of the papers that have been published to date in referred literature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5956382','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5956382"><span>Clinical Holistic Medicine: Induction of Spontaneous Remission of Cancer by Recovery of the Human Character and the Purpose of <span class="hlt">Life</span> (the <span class="hlt">Life</span> <span class="hlt">Mission</span>)</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ventegodt, Søren; Morad, Mohammed; Hyam, Eytan; Merrick, Joav</p> <p>2004-01-01</p> <p>The recovery of the human character and purpose of <span class="hlt">life</span> with consciousness-based medicine seems to be able to induce spontaneous remissions in several diseases. On two different occasions, we observed breast tumors reduced to less than half their original diameters (clinically judged) during a holistic session, when working with the patients in accordance with the holistic process theory of healing, the <span class="hlt">life</span> <span class="hlt">mission</span> theory, and the theory of human character. One tumor was histologically diagnosed as malign breast cancer prior to the session, while the other was under examination. As both patients had the affected regions of the breast surgically removed immediately after the session, we are unable to determine if they were actually healed by the holistic treatment. We find it extremely interesting that the size of a tumor can be reduced dramatically within a few hours of holistic treatment, when the patient is highly motivated for personal development. The reduction of tumor size is in accordance with the holistic view that many types of cancer are caused by emotional and existential disturbances. From a holistic perspective, cancer can be understood as a simple disturbance of the cells, arising from the tissue holding on to a trauma with strong emotional content. This is called “a blockage”, where the function of the cells is changed from their original function in the tissue to a function of holding emotions. The reduction of the tumor in the two cases happened when old painful emotions were identified in the tissues, in and around the tumor, and processed into understanding; when the patients finally did let go of negative beliefs and attitudes that had kept the feeling(s) repressed to that part of the body, the tumor first softened and then disappeared, presumably by apoptosis. We believe that the consciousness-based/holistic medical toolbox has a serious additional offer to cancer patients, and we will therefore strongly encourage the scientific society to</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140016794','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140016794"><span>Recommendation of a More Effective Alternative to the NASA Launch Services Program <span class="hlt">Mission</span> Integration Reporting System (MIRS) and Implementation of Updates to the <span class="hlt">Mission</span> Plan</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dunn, Michael R.</p> <p>2014-01-01</p> <p>Over the course of my internship in the Flight Projects Office of NASA's Launch Services Program (LSP), I worked on two major projects, both of which dealt with updating current systems to make them more accurate and to allow them to operate more efficiently. The first project dealt with the <span class="hlt">Mission</span> Integration Reporting System (MIRS), a web-accessible database application used to manage and provide <span class="hlt">mission</span> status reporting for the LSP portfolio of awarded <span class="hlt">missions</span>. MIRS had not gone through any major updates since its implementation in 2005, and it was my job to formulate a recommendation for the improvement of the system. The second project I worked on dealt with the <span class="hlt">Mission</span> Plan, a document that contains an overview of the general <span class="hlt">life</span> cycle that is followed by every LSP <span class="hlt">mission</span>. My job on this project was to update the information currently in the <span class="hlt">mission</span> plan and to add certain features in order to increase the accuracy and thoroughness of the document. The outcomes of these projects have implications in the orderly and efficient operation of the Flight Projects Office, and the process of <span class="hlt">Mission</span> Management in the Launch Services Program as a whole.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-S93-26894.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-S93-26894.html"><span>Space <span class="hlt">Life</span> Sciences-2 (SLS-2) logo or patch</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1993-03-01</p> <p>S93-26894 (March 1993) --- Spacelab <span class="hlt">Life</span> Sciences 2, scheduled to fly as the major payload on the STS-58 <span class="hlt">mission</span>, is represented with this logo. As in the case of SLS-1, which flew in space in June of 1991, this Spacelab <span class="hlt">mission</span> will be devoted to <span class="hlt">life</span> sciences and will carry a crew of experts in the associated disciplines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150014778&hterms=ion+batteries&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dion%2Bbatteries','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150014778&hterms=ion+batteries&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dion%2Bbatteries"><span>Performance Testing of Yardney Li-Ion Cells and Batteries in Support of JPL's 2009 Mars Science Laboratory <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smart, M.C.; Ratnakumar, B.V.; Whitcanack, L. D.; Dewell, E. A.; Jones, L. E.; Salvo, C. G.; Puglia, F. J.; Cohen, S.; Gitzendanner, R.</p> <p>2008-01-01</p> <p>In 2009, JPL is planning to launch an unmanned rover <span class="hlt">mission</span> to the planet Mars. This <span class="hlt">mission</span>, referred to as the Mars Science Laboratory (MSL), will involve the use of a rover that is much larger than the previously developed Spirit and Opportunity Rovers for the 2003 Mars Exploration Rover (MER) <span class="hlt">mission</span>, that are currently still in operation on the surface of the planet after more than three years. Part of the reason that the MER rovers have operated so successfully, far exceeding the required <span class="hlt">mission</span> duration of 90 sols, is that they possess robust Li-ion batteries, manufactured by Yardney Technical Products, which have demonstrated excellent <span class="hlt">life</span> characteristics. Given the excellent performance characteristics displayed, similar lithium-ion batteries have been projected to successfully meet the <span class="hlt">mission</span> requirements of the up-coming MSL <span class="hlt">mission</span>. Although comparable in many facets, such as being required to operate over a wide temperature range (-20 to 40 C), the MSL <span class="hlt">mission</span> has more demanding performance requirements compared to the MER <span class="hlt">mission</span>, including much longer <span class="hlt">mission</span> duration (approx. 687 sols vs. 90 sols), higher power capability, and the need to withstand higher temperature excursions. In addition, due to the larger rover size, the MSL <span class="hlt">mission</span> necessitates the use of a much larger battery to meet the energy, <span class="hlt">life</span>, and power requirements. In order to determine the viability of meeting these requirements, a number of performance verification tests were performed on 10 Ah Yardney lithium-ion cells (MER design) under MSL-relevant conditions, including <span class="hlt">mission</span> surface operation simulation testing. In addition, the performance of on-going ground <span class="hlt">life</span> testing of 10 Ah MER cells and 8-cell batteries will be discussed in the context of capacity loss and impedance growth predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20060043611&hterms=history+Science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dhistory%2BScience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20060043611&hterms=history+Science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dhistory%2BScience"><span>Mars Science Laboratory (MSL) : the US 2009 Mars rover <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Palluconi, Frank; Tampari, Leslie; Steltzner, Adam; Umland, Jeff</p> <p>2003-01-01</p> <p>The Mars Science Laboratory <span class="hlt">mission</span> is the 2009 United States Mars Exploration Program rover <span class="hlt">mission</span>. The MSL Project expects to complete its pre-Phase A definition activity this fiscal year (FY2003), investigations in mid-March 2004, launch in 2009, arrive at Mars in 2010 during Northern hemisphere summer and then complete a full 687 day Mars year of surface exploration. MSL will assess the potential for habitability (past and present) of a carefully selected landing region on Mars by exploring for the chemical building blocks of <span class="hlt">life</span>, and seeking to understand quantitatively the chemical and physical environment with which these components have interacted over the geologic history of the planet. Thus, MSL will advance substantially our understanding of the history of Mars and potentially, its capacity to sustain <span class="hlt">life</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100033687','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100033687"><span>Impact of Water Recovery from Wastes on the Lunar Surface <span class="hlt">Mission</span> Water Balance</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fisher, John W.; Hogan, John Andrew; Wignarajah, Kanapathipi; Pace, Gregory S.</p> <p>2010-01-01</p> <p>Future extended lunar surface <span class="hlt">missions</span> will require extensive recovery of resources to reduce <span class="hlt">mission</span> costs and enable self-sufficiency. Water is of particular importance due to its potential use for human consumption and hygiene, general cleaning, clothes washing, radiation shielding, cooling for extravehicular activity suits, and oxygen and hydrogen production. Various water sources are inherently present or are generated in lunar surface <span class="hlt">missions</span>, and subject to recovery. They include: initial water stores, water contained in food, human and other solid wastes, wastewaters and associated brines, ISRU water, and scavenging from residual propellant in landers. This paper presents the results of an analysis of the contribution of water recovery from <span class="hlt">life</span> support wastes on the overall water balance for lunar surface <span class="hlt">missions</span>. Water in human wastes, metabolic activity and survival needs are well characterized and dependable figures are available. A detailed <span class="hlt">life</span> support waste model was developed that summarizes the composition of <span class="hlt">life</span> support wastes and their water content. Waste processing technologies were reviewed for their potential to recover that water. The recoverable water in waste is a significant contribution to the overall water balance. The value of this contribution is discussed in the context of the other major sources and loses of water. Combined with other analyses these results provide guidance for research and technology development and down-selection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920047001&hterms=design+concept+principles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Ddesign%2Bconcept%2Bprinciples','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920047001&hterms=design+concept+principles&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Ddesign%2Bconcept%2Bprinciples"><span>The Solar Probe <span class="hlt">mission</span> - <span class="hlt">Mission</span> design concepts and requirements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ayon, Juan A.</p> <p>1992-01-01</p> <p>The Solar Probe concept as studied by the Jet Propulsion Laboratory represents the first <span class="hlt">mission</span> to combine out-of-the-ecliptic scientific coverage with multiple, close solar encounters (at 4 solar radii). The scientific objectives of the <span class="hlt">mission</span> have driven the investigation and analysis of several <span class="hlt">mission</span> design concepts, all optimized to meet the science/<span class="hlt">mission</span> requirements. This paper reviews those <span class="hlt">mission</span> design concepts developed, the science objectives that drive the <span class="hlt">mission</span> design, and the principle <span class="hlt">mission</span> requirements associated with these various concepts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930068547&hterms=Tuskegee&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DTuskegee','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930068547&hterms=Tuskegee&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3DTuskegee"><span>Effect of <span class="hlt">mission</span> cycling on the fatigue performance of SiC-coated carbon-carbon composites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mahfuz, H.; Das, P. S.; Jeelani, S.; Baker, D. M.; Johnson, S. A.</p> <p>1993-01-01</p> <p>The effects of thermal and pressure cycling on the fatigue performance of carbon-carbon composites, and the influence of <span class="hlt">mission</span> cycling on these effects, were investigated by subjecting both virgin and <span class="hlt">mission</span>-cycled two-dimensional specimens of SiC-coated carbon-carbon composites to fatigue tests, conducted at room temperature in three-point bending, with a stress ratio of 0.2 and a frequency of 1 Hz. It was found that the fatigue strength of C-C composites is high (about 90 percent of the ultimate flexural strength), but decreased with the <span class="hlt">mission</span> cycling. The lowering of the fatigue strength with <span class="hlt">mission</span> cycling is attributed to the increase in interfacial bond strength due to thermal and pressure cycling of the material. The already high sensitivity of C-C composites to stress during cyclic loading increases further with the amount of <span class="hlt">mission</span> cycling. Results of NDE suggest that the damage growth in virgin C-C, in the high-cycle range, is slow at the initial stage of the cyclic <span class="hlt">life</span>, but propagates rapidly after certain threshold cycles of the fatigue <span class="hlt">life</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010cosp...38..515C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010cosp...38..515C"><span>Exomars <span class="hlt">Mission</span> Verification Approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cassi, Carlo; Gilardi, Franco; Bethge, Boris</p> <p></p> <p>According to the long-term cooperation plan established by ESA and NASA in June 2009, the ExoMars project now consists of two <span class="hlt">missions</span>: A first <span class="hlt">mission</span> will be launched in 2016 under ESA lead, with the objectives to demonstrate the European capability to safely land a surface package on Mars, to perform Mars Atmosphere investigation, and to provide communi-cation capability for present and future ESA/NASA <span class="hlt">missions</span>. For this <span class="hlt">mission</span> ESA provides a spacecraft-composite, made up of an "Entry Descent & Landing Demonstrator Module (EDM)" and a Mars Orbiter Module (OM), NASA provides the Launch Vehicle and the scientific in-struments located on the Orbiter for Mars atmosphere characterisation. A second <span class="hlt">mission</span> with it launch foreseen in 2018 is lead by NASA, who provides spacecraft and launcher, the EDL system, and a rover. ESA contributes the ExoMars Rover Module (RM) to provide surface mobility. It includes a drill system allowing drilling down to 2 meter, collecting samples and to investigate them for signs of past and present <span class="hlt">life</span> with exobiological experiments, and to investigate the Mars water/geochemical environment, In this scenario Thales Alenia Space Italia as ESA Prime industrial contractor is in charge of the design, manufacturing, integration and verification of the ESA ExoMars modules, i.e.: the Spacecraft Composite (OM + EDM) for the 2016 <span class="hlt">mission</span>, the RM for the 2018 <span class="hlt">mission</span> and the Rover Operations Control Centre, which will be located at Altec-Turin (Italy). The verification process of the above products is quite complex and will include some pecu-liarities with limited or no heritage in Europe. Furthermore the verification approach has to be optimised to allow full verification despite significant schedule and budget constraints. The paper presents the verification philosophy tailored for the ExoMars <span class="hlt">mission</span> in line with the above considerations, starting from the model philosophy, showing the verification activities flow and the sharing of tests</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.P14A..05G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.P14A..05G"><span>The Long, Bumpy Road to a Mars Aeronomy <span class="hlt">Mission</span> (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grebowsky, J. M.; Luhmann, J. G.; Bougher, S. W.; Jakosky, B. M.</p> <p>2013-12-01</p> <p>With the advent of the space age, early focus was put into characterizing the Earth's upper atmosphere with aeronomy <span class="hlt">missions</span>. These <span class="hlt">missions</span> were designed to study the upper atmosphere region of a planet where the ionosphere is produced with particular attention given to the composition, properties and motion of atmosphere constituents. In particular a very successful US series of Atmosphere Explorer aeronomy spacecraft (1963-1977) was implemented. This upper atmosphere region is the envelope that all energy from the sun must penetrate and is recognized as an inseparable part of a planet's entire atmosphere. Venus was the next planet to have its upper atmosphere/ionosphere deeply probed via the Pioneer Venus Orbiter (1978-1986) that carried a complement of instruments similar to some flown on the Atmosphere Explorers. The planet which humans have long set their imagination on, Mars, has yet to be subjected to the same detailed upper atmosphere perusal until now, with MAVEN. Not that attempts have been wanting. More than 30 spacecraft launches to Mars were attempted, but half were not successful and those that attained orbit came far short of attaining the same level of knowledge of the Martian upper atmosphere. Other countries had planned Mars aeronomy <span class="hlt">missions</span> that didn't bear fruit - e.g. Mars-96 and Nozomi and the US did studies for two <span class="hlt">missions</span>, Mars Aeronomy Orbiter and MUADEE, that never were implemented. This is about to change. NASA's Scout Program singled out two aeronomy <span class="hlt">missions</span> in its final competition and the selected <span class="hlt">mission</span>, MAVEN, will fly with the needed sophistication of instruments to finally probe and understand the top of Mars' atmosphere. Was this late selection of a NASA aeronomy <span class="hlt">mission</span> to Mars a philosophy change in US priorities or was it an accident of planning and budget constraints? Was it driven by the developing knowledge that Mars really had an early atmosphere environment conducive to <span class="hlt">life</span> and that an aeronomy <span class="hlt">mission</span> is indeed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10567E..0HD','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10567E..0HD"><span>Search for extraterrestrial planets: the DARWIN <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>d'Arcio, Luigi; Karlsson, Anders; Bavdaz, Marcos; Jagemann, Thomas</p> <p>2017-11-01</p> <p>The ESA Darwin <span class="hlt">mission</span> is primarily devoted to the detection of earth-like exoplanets and the spectroscopic characterization of their atmospheres for key tracers of <span class="hlt">life</span>. Darwin is implemented as a free-flying stellar interferometer operating in the 6.5-20 micron wavelength range, and passively cooled to 40 K. The stellar flux is suppressed by destructive interference (nulling) over the full optical bandwidth. The planetary signal is extracted from the zodiacal background signature by modulating the optical response of the interferometer. The Darwin <span class="hlt">mission</span> concept has evolved considerably in the past years. The original concept, based on six 1.5 m telescopes, has been replaced by more efficient designs using three to four three-meter class apertures. A novel 3D architecture is being evaluated, together with the conventional planar one, bearing the potential for significant volume and mass savings and enhanced straylight rejection. A number of technology development activities have been successfully completed, including optical metrology, optical delay lines, and single-mode infrared optical fibers. A second iteration of the Darwin System Assessment Study has been kicked off end 2005, aiming to consolidate the overall <span class="hlt">mission</span> architecture and the preliminary design of the Darwin <span class="hlt">mission</span> concept. This paper illustrates the current status of the Darwin <span class="hlt">mission</span>, with special emphasis on the optical configuration and the technology development programme in the area of optics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/5347439','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/5347439"><span>ETF <span class="hlt">Mission</span> Statement document. ETF Design Center team</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Not Available</p> <p>1980-04-01</p> <p>The <span class="hlt">Mission</span> Statement document describes the results, activities, and processes used in preparing the <span class="hlt">Mission</span> Statement, facility characteristics, and operating goals for the Engineering Test Facility (ETF). Approximately 100 engineers and scientists from throughout the US fusion program spent three days at the Knoxville <span class="hlt">Mission</span> Workshop defining the requirements that should be met by the ETF during its operating <span class="hlt">life</span>. Seven groups were selected to consider one major category each of design and operation concerns. Each group prepared the findings of the assigned area as described in the major sections of this document. The results of the operations discussed mustmore » provide the data, knowledge, experience, and confidence to continue to the next steps beyond the ETF in making fusion power a viable energy option. The results from the ETF <span class="hlt">mission</span> (operations are assumed to start early in the 1990's) are to bridge the gap between the base of magnetic fusion knowledge at the start of operations and that required to design the EPR/DEMO devices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040045251&hterms=food+analysis&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfood%2Banalysis','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040045251&hterms=food+analysis&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfood%2Banalysis"><span>System-level Analysis of Food Moisture Content Requirements for the Mars Dual Lander Transit <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levri, Julie A.; Perchonok, Michele H.</p> <p>2004-01-01</p> <p>In order to ensure that adequate water resources are available during a <span class="hlt">mission</span>, any net water loss from the habitat must be balanced with an equivalent amount of required makeup water. Makeup water may come from a variety of sources, including water in shipped tanks, water stored in prepackaged food, product water from fuel cells, and in-situ water resources. This paper specifically addresses the issue of storing required makeup water in prepackaged food versus storing the water in shipped tanks for the Mars Dual Lander Transit <span class="hlt">Mission</span>, one of the Advanced <span class="hlt">Life</span> Support Reference <span class="hlt">Missions</span>. In this paper, water mass balances have been performed for the Dual Lander Transit <span class="hlt">Mission</span>, to determine the necessary requirement of makeup water under nominal operation (i.e. no consideration of contingency needs), on a daily basis. Contingency issues are briefly discussed with respect to impacts on makeup water storage (shipped tanks versus storage in prepackaged food). The Dual Lander Transit <span class="hlt">Mission</span> was selected for study because it has been considered by the Johnson Space Center Exploration Office in enough detail to define a reasonable set of scenario options for nominal system operation and contingencies. This study also illustrates the concept that there are multiple, reasonable <span class="hlt">life</span> support system scenarios for any one particular <span class="hlt">mission</span>. Thus, the need for a particular commodity can depend upon many variables in the system. In this study, we examine the need for makeup water as it depends upon the configuration of the rest of the <span class="hlt">life</span> support system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997EOSTr..78Q..14C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997EOSTr..78Q..14C"><span><span class="hlt">Mission</span> for Mitchell</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carlowicz, Michael</p> <p></p> <p>In honor of a <span class="hlt">life</span> of pioneering efforts to use satellite altimetry for geophysical studies, the U.S. Navy announced on December 16, 1996, that it will dedicate its next satellite altimeter—the follow-on to Geosat—to deceased AGU member Jimmy Mitchell. The announcement was made during a special session dedicated to Mitchell's research at the AGU Fall Meeting.Mitchell first won renown at the Jet Propulsion Laboratory in the 1970s and 1980s while conducting research associated with Voyager <span class="hlt">missions</span>. But it was his work in later years at the Naval Research Laboratory at Stennis Space Center, Mississippi, that led the Navy to honor him with the satellite.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840010229','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840010229"><span>Space Station needs, attributes and architectural options. Volume 2, book 1, part 2, task 1: <span class="hlt">Mission</span> requirements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1983-01-01</p> <p><span class="hlt">Mission</span> areas analyzed for input to the baseline <span class="hlt">mission</span> model include: (1) commercial materials processing, including representative <span class="hlt">missions</span> for producing metallurgical, chemical and biological products; (2) commercial Earth observation, represented by a typical carry-on <span class="hlt">mission</span> amenable to commercialization; (3) solar terrestrial and resource observations including <span class="hlt">missions</span> in geoscience and scientific land observation; (4) global environment, including representative <span class="hlt">missions</span> in meteorology, climatology, ocean science, and atmospheric science; (5) materials science, including <span class="hlt">missions</span> for measuring material properties, studying chemical reactions and utilizing the high vacuum-pumping capacity of space; and (6) <span class="hlt">life</span> sciences with experiments in biomedicine and animal and plant biology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.P53A0997S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.P53A0997S"><span>Progress in <span class="hlt">Life</span> Marker Chip Technology for Detection of <span class="hlt">Life</span> on Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sims, M. R.; Cullen, D. C.; Laan, E.; Borst, G.; Prak, A.; Richter, L.; Gaubert, F.; Steele, A.; Parnell, J.; Sephton, M.</p> <p>2007-12-01</p> <p>Detection of <span class="hlt">Life</span> on Mars will rely on detection of biomarkers, physical or chemical structures that can be associated with <span class="hlt">Life</span>. As a possible payload for the ESA ExoMars rover <span class="hlt">mission</span> planned in 2013 and other future <span class="hlt">missions</span> a <span class="hlt">Life</span> Marker Chip instrument is being developed. This instrument uses immuno-assay techniques to detect the relevant biomarkers. This paper describes the typical targets it will search for, its operating principle and the status of development. 63 biomarker targets have been identified and assays have been developed for a limited subset. Assay development includes use of recombinant DNA techniques to generate the molecular receptors (antibodies). This type of instrument has applications in terrestrial research e.g. sub-glacial lakes as well as planetary exploration. Breadboard demonstrators have been built of the assay system and key components of the micro-fluidics. Results from these breadboards will be presented, along with plans for future development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170008272&hterms=alien&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dalien','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170008272&hterms=alien&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dalien"><span>Enceladus <span class="hlt">Life</span> Finder: the Search for <span class="hlt">Life</span> in a Habitable Moon</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Cable, Morgan L.; Clark, Karla; Lunine, Jonathan I.; Postberg, Frank; Reh, Kim; Spilker, Linda; Waite, J. Hunter</p> <p>2016-01-01</p> <p>Enceladus is one of the most intriguing bodies in the solar system. In addition to having one of the brightest and youngest surfaces, this small Saturnian moon was recently discovered to have a plume erupting from its south polar terrain and a global subsurface ocean. The Cassini <span class="hlt">Mission</span> discovered organics and nitrogen-bearing molecules in the plume, as well as salts and silicates that strongly suggest ocean water in contact with a rocky core. However, Cassini's instruments lack sufficient resolution and mass range to determine if these organics are of biotic origin. The Enceladus <span class="hlt">Life</span> Finder (ELF) is a Discovery-class <span class="hlt">mission</span> that would use two state-of-the-art mass spectrometers to target the gas and grains of the plume and search for evidence of <span class="hlt">life</span> in this alien ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.P51G1798R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.P51G1798R"><span>Planetary Protection Provisions for the Mars 2020 <span class="hlt">Mission</span>: Enabling Discovery by Constraining Contamination</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rummel, J. D.; Conley, C. A.</p> <p>2013-12-01</p> <p>The 2013-2022 NRC Decadal Survey named its #1 Flagship priority as a large, capable Mars rover that would be the first of a three-<span class="hlt">mission</span>, multi-decadal effort to return samples from Mars. More recently, NASA's Mars Program has stated that a Mars rover <span class="hlt">mission</span> known as 'Mars 2020' would be flown to Mars (in 2020) to accomplish a subset of the goals specified by the NRC, and the recent report of the Mars 2020 Science Definition Team (SDT) has recommended that the <span class="hlt">mission</span> accomplish broad and rigorous in situ science, including seeking biosignatures, acquiring a diverse set of samples intended to address a range of Mars science questions and storing them in a cache for potential return to Earth at a later time, and other engineering goals to constrain costs and support future human exploration. In some ways Mars 2020 will share planetary protection requirements with the Mars Science Laboratory <span class="hlt">mission</span> that landed in 2012, which included landing site constraints based on the presence of a perennial heat source (the MMRTG) aboard the lander/rover. In a very significant way, however, the presence of a sample-cache and the potential that Mars 2020 will be the first <span class="hlt">mission</span> in the chain that will return a sample from Mars to Earth. Thus Mars 2020 will face more stringent requirements aimed at keeping the <span class="hlt">mission</span> from returning Earth contamination with the samples from Mars. Mars 2020 will be looking for biosignatures of ancient <span class="hlt">life</span>, on Mars, but will also need to be concerned with the potential to detect extant biosignatures or <span class="hlt">life</span> itself within the sample that is eventually returned. If returned samples are able to unlock wide-ranging questions about the geology, surface processes, and habitability of Mars that cannot be answered by study of meteorites or current <span class="hlt">mission</span> data, then either the returned samples must be free enough of Earth organisms to be releasable from a quarantine facility or the planned work of sample scientists, including high- and low</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100023420','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100023420"><span><span class="hlt">Life</span> Science Research in Outer Space: New Platform Technologies for Low-Cost, Autonomous Small Satellite <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ricco, Antonio J.; Parra, Macarena P.; Niesel, David; McGinnis, Michael; Ehrenfreund, Pascale; Nicholson, Wayne; Mancinelli, Rocco; Piccini, Matthew E.; Beasley, Christopher C.; Timucin, Linda R.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20100023420'); toggleEditAbsImage('author_20100023420_show'); toggleEditAbsImage('author_20100023420_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20100023420_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20100023420_hide"></p> <p>2009-01-01</p> <p>We develop integrated instruments and platforms suitable for economical, frequent space access for autonomous <span class="hlt">life</span> science experiments and processes in outer space. The technologies represented by three of our recent free-flyer small-satellite <span class="hlt">missions</span> are the basis of a rapidly growing toolbox of miniaturized biologically/biochemically-oriented instrumentation now enabling a new generation of in-situ space experiments. Autonomous small satellites ( 1 50 kg) are less expensive to develop and build than fullsize spacecraft and not subject to the comparatively high costs and scheduling challenges of human-tended experimentation on the International Space Station, Space Shuttle, and comparable platforms. A growing number of commercial, government, military, and civilian space launches now carry small secondary science payloads at far lower cost than dedicated <span class="hlt">missions</span>; the number of opportunities is particularly large for so-called cube-sat and multicube satellites in the 1 10 kg range. The recent explosion in nano-, micro-, and miniature technologies, spanning fields from telecommunications to materials to bio/chemical analysis, enables development of remarkably capable autonomous miniaturized instruments to accomplish remote biological experimentation. High-throughput drug discovery, point-of-care medical diagnostics, and genetic analysis are applications driving rapid progress in autonomous bioanalytical technology. Three of our recent <span class="hlt">missions</span> exemplify the development of miniaturized analytical payload instrumentation: GeneSat-1 (launched: December 2006), PharmaSat (launched: May 2009), and O/OREOS (organism/organics exposure to orbital stresses; scheduled launch: May 2010). We will highlight the overall architecture and integration of fluidic, optical, sensor, thermal, and electronic technologies and subsystems to support and monitor the growth of microorganisms in culture in these small autonomous space satellites, including real-time tracking of their culture</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040015099','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040015099"><span>Equivalent Mass versus <span class="hlt">Life</span> Cycle Cost for <span class="hlt">Life</span> Support Technology Selection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Harry</p> <p>2003-01-01</p> <p>The decision to develop a particular <span class="hlt">life</span> support technology or to select it for flight usually depends on the cost to develop and fly it. Other criteria such as performance, safety, reliability, crew time, and technical and schedule risk are considered, but cost is always an important factor. Because launch cost would account for much of the cost of a future planetary <span class="hlt">mission</span>, and because launch cost is directly proportional to the mass launched, equivalent mass has been used instead of cost to select advanced <span class="hlt">life</span> support technology. The equivalent mass of a <span class="hlt">life</span> support system includes the estimated mass of the hardware and of the spacecraft pressurized volume, power supply, and cooling system that the hardware requires. The equivalent mass of a system is defined as the total payload launch mass needed to provide and support the system. An extension of equivalent mass, Equivalent System Mass (ESM), has been established for use in the Advanced <span class="hlt">Life</span> Support project. ESM adds a mass-equivalent of crew time and possibly other cost factors to equivalent mass. Traditional equivalent mass is strictly based on flown mass and reflects only the launch cost. ESM includes other important cost factors, but it complicates the simple flown mass definition of equivalent mass by adding a non-physical mass penalty for crew time that may exceed the actual flown mass. Equivalent mass is used only in <span class="hlt">life</span> support analysis. <span class="hlt">Life</span> Cycle Cost (LCC) is much more commonly used. LCC includes DDT&E, launch, and operations costs. For Earth orbit rather than planetary <span class="hlt">missions</span>, the launch cost is less than the cost of Design, Development, Test, and Evaluation (DDTBE). LCC is a more inclusive cost estimator than equivalent mass. The relative costs of development, launch, and operations vary depending on the <span class="hlt">mission</span> destination and duration. Since DDTBE or operations may cost more than launch, LCC gives a more accurate relative cost ranking than equivalent mass. To select the lowest cost</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950032174&hterms=coma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcoma','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950032174&hterms=coma&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dcoma"><span>Cometary coma chemical composition (C4) <span class="hlt">mission</span>. [Abstract only</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carle, G. C.; Clark, B. C.; Niemann, H. B.; Alexander, M.; Knocke, P. C.; O'Hara, B. J.</p> <p>1994-01-01</p> <p>Cometary <span class="hlt">missions</span> are of enormous fundamental importance for many different space science disciplines, including exobiology. Comets are presumed relics of the earliest, most primitive material in the solar nebula and are related to the planetesimals. They undoubtedly provided a general enrichment of volatiles to the inner solar system (contributing to atmospheres and oceans) and may have been key to the origin of <span class="hlt">life</span>. A Discovery class, comet rendezvous <span class="hlt">mission</span>, the Cometary Coma Chemical Composition (C4) <span class="hlt">Mission</span>, was selected for further study by NASA earlier this year. The C4 <span class="hlt">Mission</span> is a highly focused and usefully-limited subset of the Cometary Rendezvous Asteroid Flyby (CRAF) <span class="hlt">Mission</span>, concentrating exclusively on measurements which will lead to an understanding of the chemical composition and make-up of the cometary nucleus. The scientific goals of the Cometary Coma Chemical Composition (C4) <span class="hlt">Mission</span> are to rendezvous with a short-period comet and (1) to determine the elemental, chemical, and isotopic composition of the nucleus and (2) to characterize the chemical and isotopic nature of its atmosphere. Further, it is a goal to obtain preliminary data on the development of the coma (dust and gas composition) as a function of time and orbital position.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=jupiter&pg=2&id=EJ789704','ERIC'); return false;" href="https://eric.ed.gov/?q=jupiter&pg=2&id=EJ789704"><span><span class="hlt">Life</span> in the Universe</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Lowman, Paul D., Jr.</p> <p>2003-01-01</p> <p>The belief that <span class="hlt">life</span> exists in the universe is an optimism shared by many. With several manned <span class="hlt">missions</span> expected to be carried out in the future, the possibility of discovering <span class="hlt">life</span> in outer space will revolutionize the field of astrobiology. In this article, the author presents a summary of recent developments and discoveries made in the search…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DPS....4812312Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DPS....4812312Z"><span>Ongoing Mars <span class="hlt">Missions</span>: Extended <span class="hlt">Mission</span> Plans</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zurek, Richard; Diniega, Serina; Crisp, Joy; Fraeman, Abigail; Golombek, Matt; Jakosky, Bruce; Plaut, Jeff; Senske, David A.; Tamppari, Leslie; Thompson, Thomas W.; Vasavada, Ashwin R.</p> <p>2016-10-01</p> <p>Many key scientific discoveries in planetary science have been made during extended <span class="hlt">missions</span>. This is certainly true for the Mars <span class="hlt">missions</span> both in orbit and on the planet's surface. Every two years, ongoing NASA planetary <span class="hlt">missions</span> propose investigations for the next two years. This year, as part of the 2016 Planetary Sciences Division (PSD) <span class="hlt">Mission</span> Senior Review, the Mars Odyssey (ODY) orbiter project submitted a proposal for its 7th extended <span class="hlt">mission</span>, the Mars Exploration Rover (MER-B) Opportunity submitted for its 10th, the Mars Reconnaissance Orbiter (MRO) for its 4th, and the Mars Science Laboratory (MSL) Curiosity rover and the Mars Atmosphere and Volatile Evolution (MVN) orbiter for their 2nd extended <span class="hlt">missions</span>, respectively. Continued US participation in the ongoing Mars Express <span class="hlt">Mission</span> (MEX) was also proposed. These <span class="hlt">missions</span> arrived at Mars in 2001, 2004, 2006, 2012, 2014, and 2003, respectively. Highlights of proposed activities include systematic observations of the surface and atmosphere in twilight (early morning and late evening), building on a 13-year record of global mapping (ODY); exploration of a crater rim gully and interior of Endeavour Crater, while continuing to test what can and cannot be seen from orbit (MER-B); refocused observations of ancient aqueous deposits and polar cap interiors, while adding a 6th Mars year of change detection in the atmosphere and the surface (MRO); exploration and sampling by a rover of mineralogically diverse strata of Mt. Sharp and of atmospheric methane in Gale Crater (MSL); and further characterization of atmospheric escape under different solar conditions (MVN). As proposed, these activities follow up on previous discoveries (e.g., recurring slope lineae, habitable environments), while expanding spatial and temporal coverage to guide new detailed observations. An independent review panel evaluated these proposals, met with project representatives in May, and made recommendations to NASA in June 2016. In this</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060025034','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060025034"><span>Developing Advanced Human Support Technologies for Planetary Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Berdich, Debra P.; Campbell, Paul D.; Jernigan, J. Mark</p> <p>2004-01-01</p> <p>The United States Vision for Space Exploration calls for sending robots and humans to explore the Earth's moon, the planet Mars, and beyond. The National Aeronautics and Space Administration (NASA) is developing a set of design reference <span class="hlt">missions</span> that will provide further detail to these plans. Lunar <span class="hlt">missions</span> are expected to provide a stepping stone, through operational research and evaluation, in developing the knowledge base necessary to send crews on long duration <span class="hlt">missions</span> to Mars and other distant destinations. The NASA Exploration Systems Directorate (ExSD), in its program of bioastronautics research, manages the development of technologies that maintain human <span class="hlt">life</span>, health, and performance in space. Using a system engineering process and risk management methods, ExSD's Human Support Systems (HSS) Program selects and performs research and technology development in several critical areas and transfers the results of its efforts to NASA exploration <span class="hlt">mission</span>/systems development programs in the form of developed technologies and new knowledge about the capabilities and constraints of systems required to support human existence beyond Low Earth Orbit. HSS efforts include the areas of advanced environmental monitoring and control, extravehicular activity, food technologies, <span class="hlt">life</span> support systems, space human factors engineering, and systems integration of all these elements. The HSS Program provides a structured set of deliverable products to meet the needs of exploration programs. These products reduce the gaps that exist in our knowledge of and capabilities for human support for long duration, remote space <span class="hlt">missions</span>. They also reduce the performance gap between the efficiency of current space systems and the greater efficiency that must be achieved to make human planetary exploration <span class="hlt">missions</span> economically and logistically feasible. In conducting this research and technology development program, it is necessary for HSS technologists and program managers to develop a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19760087376&hterms=physiology+stress&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dphysiology%2Bstress','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19760087376&hterms=physiology+stress&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dphysiology%2Bstress"><span>Physiological and psychological stress limits for astronautics Observations during the Skylab I-III <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Burchard, E. C.</p> <p>1975-01-01</p> <p>The physiological and psychological factors of manned space flight had a particular significance in the Skylab <span class="hlt">missions</span> during which astronauts were subjected to a <span class="hlt">life</span> in a space environment for longer periods of time than on previous space <span class="hlt">missions</span>. The Skylab <span class="hlt">missions</span> demonstrated again the great adaptability of human physiology to the environment of man. The results of Skylab have indicated also approaches for enhancing the capability of man to tolerate the physiological and psychological stresses of space flight.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930057457&hterms=financial+considerations&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dfinancial%2Bconsiderations','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930057457&hterms=financial+considerations&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dfinancial%2Bconsiderations"><span>Towards a Mars base - Critical steps for <span class="hlt">life</span> support on the moon and beyond</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rummel, John D.</p> <p>1992-01-01</p> <p>In providing crew <span class="hlt">life</span> support for future exploration <span class="hlt">missions</span>, overall exploration objectives will drive the <span class="hlt">life</span> support solutions selected. Crew size, <span class="hlt">mission</span> tasking, and exploration strategy will determine the performance required from <span class="hlt">life</span> support systems. Human performance requirements, for example, may be offset by the availability of robotic assistance. Once established, exploration requirements for <span class="hlt">life</span> support will be weighed against the financial and technical risks of developing new technologies and systems. Other considerations will include the demands that a particular <span class="hlt">life</span> support strategy will make on planetary surface site selection, and the availability of precursor <span class="hlt">mission</span> data to support EVA and in situ resource recovery planning. As space exploration progresses, the diversity of <span class="hlt">life</span> support solutions that are implemented is bound to increase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040074336&hterms=stellar+black+holes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dstellar%2Bblack%2Bholes','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040074336&hterms=stellar+black+holes&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dstellar%2Bblack%2Bholes"><span>The Stellar Imager (SI)"Vision <span class="hlt">Mission</span>"</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carpenter, Ken; Danchi, W.; Leitner, J.; Liu, A.; Lyon, R.; Mazzuca, L.; Moe, R.; Chenette, D.; Karovska, M.; Allen, R.</p> <p>2004-01-01</p> <p>The Stellar Imager (SI) is a "Vision" <span class="hlt">mission</span> in the Sun-Earth Connection (SEC) Roadmap, conceived for the purpose of understanding the effects of stellar magnetic fields, the dynamos that generate them, and the internal structure and dynamics of the stars in which they exist. The ultimate goal is to achieve the best possible forecasting of solar/stellar magnetic activity and its impact on <span class="hlt">life</span> in the Universe. The science goals of SI require an ultra-high angular resolution, at ultraviolet wavelengths, on the order of 100 micro-arcsec and thus baselines on the order of 0.5 km. These requirements call for a large, multi-spacecraft (less than 20) imaging interferometer, utilizing precision formation flying in a stable environment, such as in a Lissajous orbit around the Sun-Earth L2 point. SI's resolution will make it an invaluable resource for many other areas of astrophysics, including studies of AGN s, supernovae, cataclysmic variables, young stellar objects, QSO's, and stellar black holes. ongoing <span class="hlt">mission</span> concept and technology development studies for SI. These studies are designed to refine the <span class="hlt">mission</span> requirements for the science goals, define a Design Reference <span class="hlt">Mission</span>, perform trade studies of selected major technical and architectural issues, improve the existing technology roadmap, and explore the details of deployment and operations, as well as the possible roles of astronauts and/or robots in construction and servicing of the facility.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19920007755','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19920007755"><span>STS-41 Space Shuttle <span class="hlt">mission</span> report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Camp, David W.; Germany, D. M.; Nicholson, Leonard S.</p> <p>1990-01-01</p> <p>The STS-41 Space Shuttle Program <span class="hlt">Mission</span> Report contains a summary of the vehicle subsystem activities on this thirty-sixth flight of the Space Shuttle and the eleventh flight of the Orbiter vehicle, Discovery (OV-103). In addition to the Discovery vehicle, the flight vehicle consisted of an External Tank (ET) (designated as ET-39/LWT-32), three Space Shuttle main engines (SSME's) (serial numbers 2011, 2031, and 2107), and two Solid Rocket Boosters (SRB's), designated as BI-040. The primary objective of the STS-41 <span class="hlt">mission</span> was to successfully deploy the Ulysses/inertial upper stage (IUS)/payload assist module (PAM-S) spacecraft. The secondary objectives were to perform all operations necessary to support the requirements of the Shuttle Backscatter Ultraviolet (SSBUV) Spectrometer, Solid Surface Combustion Experiment (SSCE), Space <span class="hlt">Life</span> Sciences Training Program Chromosome and Plant Cell Division in Space (CHROMEX), Voice Command System (VCS), Physiological Systems Experiment (PSE), Radiation Monitoring Experiment - 3 (RME-3), Investigations into Polymer Membrane Processing (IPMP), Air Force Maui Optical Calibration Test (AMOS), and Intelsat Solar Array Coupon (ISAC) payloads. The sequence of events for this <span class="hlt">mission</span> is shown in tabular form. Summarized are the significant problems that occurred in the Orbiter subsystems during the <span class="hlt">mission</span>. The official problem tracking list is presented. In addition, each Orbiter problem is cited in the subsystem discussion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004cosp...35..535H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004cosp...35..535H"><span>critcial human health issues in connection with future human <span class="hlt">missions</span> to mMars: the HUMEX study of ESA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horneck, G.; Humex Team</p> <p></p> <p>ESA has recently initiated a study of the human responses, limits and needs with regard to the stress environments of interplanetary and planetary <span class="hlt">missions</span>. Emphasis was laid on human health and performance care as well as Advanced <span class="hlt">Life</span> Support Developments including Bioregenerative <span class="hlt">Life</span> Support Systems and environmental monitoring. The overall study goals were as follows: (i) to define reference scenarios for a European participation in human exploration and to estimate their influence on the <span class="hlt">Life</span> Sciences and <span class="hlt">Life</span> Support requirements; (ii) for selected <span class="hlt">mission</span> scenarios, to critically assess the limiting factors for human health, wellbeing, and performance and to recommend relevant countermeasures; (iii) for selected <span class="hlt">mission</span> scenarios, to critically assess the potential of Advanced <span class="hlt">Life</span> Support Developments and to pro-pose a European strategy including terrestrial applications; (iv) to critically assess the feasibility of existing facilities and technologies on ground and in space as test-beds in preparation for human exploratory <span class="hlt">missions</span> and to develop a test plan for ground and ISS campaigns; (v) to develop a roadmap for a future European strategy towards human exploratory <span class="hlt">missions</span>, including preparatory activities and terrestrial applications and benefits. Two scenarios for a Mars <span class="hlt">mission</span> were selected: (i) with a 30 days stay on Mars, and (ii) with about 500 days stay on Mars. The impact on human health, perform-ance and well being has been investigated from the view point of (i) the effects of microgravity (during space travel), reduced gravity (on Mars) and abrupt gravity changes (during launch and landing), (ii) the effects of cosmic radiation including solar particle events, (iii) psychological issues as well as general health care. Coun-termeasures as well as necessary research using ground-based testbeds and/or the ISS have been defined. The need for highly intelligent autonomous diagnostic and therapy systems was emphasized. Advanced <span class="hlt">life</span> support</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19800057590&hterms=craft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dcraft','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19800057590&hterms=craft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dcraft"><span><span class="hlt">Mission</span> management - Lessons learned from early Spacelab <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Craft, H. G., Jr.</p> <p>1980-01-01</p> <p>The concept and the responsibilities of a <span class="hlt">mission</span> manager approach are reviewed, and some of the associated problems in implementing Spacelab <span class="hlt">mission</span> are discussed. Consideration is given to program control, science management, integrated payload <span class="hlt">mission</span> planning, and integration requirements. Payload specialist training, payload and launch site integration, payload flight/<span class="hlt">mission</span> operations, and postmission activities are outlined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960035765','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960035765"><span>Balancing Science Objectives and Operational Constraints: A <span class="hlt">Mission</span> Planner's Challenge</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Weldy, Michelle</p> <p>1996-01-01</p> <p>The Air Force minute sensor technology integration (MSTI-3) satellite's primary <span class="hlt">mission</span> is to characterize Earth's atmospheric background clutter. MSTI-3 will use three cameras for data collection, a mid-wave infrared imager, a short wave infrared imager, and a visible imaging spectrometer. <span class="hlt">Mission</span> science objectives call for the collection of over 2 million images within the one year <span class="hlt">mission</span> <span class="hlt">life</span>. In addition, operational constraints limit camera usage to four operations of twenty minutes per day, with no more than 10,000 data and calibrating images collected per day. To balance the operational constraints and science objectives, the <span class="hlt">mission</span> planning team has designed a planning process to e event schedules and sensor operation timelines. Each set of constraints, including spacecraft performance capabilities, the camera filters, the geographical regions, and the spacecraft-Sun-Earth geometries of interest, and remote tracking station deconflictions has been accounted for in this methodology. To aid in this process, the <span class="hlt">mission</span> planning team is building a series of tools from commercial off-the-shelf software. These include the <span class="hlt">mission</span> manifest which builds a daily schedule of events, and the MSTI Scene Simulator which helps build geometrically correct scans. These tools provide an efficient, responsive, and highly flexible architecture that maximizes data collection while minimizing <span class="hlt">mission</span> planning time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150014767&hterms=communication+commercial&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dcommunication%2Bcommercial','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150014767&hterms=communication+commercial&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dcommunication%2Bcommercial"><span>Qualification of Commercial XIPS(R) Ion Thrusters for NASA Deep Space <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Goebel, Dan M.; Polk, James E.; Wirz, Richard E.; Snyder, J.Steven; Mikellides, Ioannis G.; Katz, Ira; Anderson, John</p> <p>2008-01-01</p> <p>Electric propulsion systems based on commercial ion and Hall thrusters have the potential for significantly reducing the cost and schedule-risk of Ion Propulsion Systems (IPS) for deep space <span class="hlt">missions</span>. The large fleet of geosynchronous communication satellites that use solar electric propulsion (SEP), which will approach 40 satellites by year-end, demonstrates the significant level of technical maturity and spaceflight heritage achieved by the commercial IPS systems. A program to delta-qualify XIPS(R) ion thrusters for deep space <span class="hlt">missions</span> is underway at JPL. This program includes modeling of the thruster grid and cathode <span class="hlt">life</span>, environmental testing of a 25-centimeter electromagnetic (EM) thruster over DAWN-like vibe and temperature profiles, and wear testing of the thruster cathodes to demonstrate the <span class="hlt">life</span> and benchmark the model results. This paper will present the delta-qualification status of the XIPS thruster and discuss the <span class="hlt">life</span> and reliability with respect to known failure mechanisms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013470','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013470"><span>NASA Mars 2020 Rover <span class="hlt">Mission</span>: New Frontiers in Science</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Calle, Carlos I.</p> <p>2014-01-01</p> <p>The Mars 2020 rover <span class="hlt">mission</span> is the next step in NASAs robotic exploration of the red planet. The rover, based on the Mars Science Laboratory Curiosity rover now on Mars, will address key questions about the potential for <span class="hlt">life</span> on Mars. The <span class="hlt">mission</span> would also provide opportunities to gather knowledge and demonstrate technologies that address the challenges of future human expeditions to Mars.Like the Mars Science Laboratory rover, which has been exploring Mars since 2012, the Mars 2020 spacecraft will use a guided entry, descent, and landing system which includes a parachute, descent vehicle, and, during the provides the ability to land a very large, heavy rover on the surface of Mars in a more precise landing area. The Mars 2020 <span class="hlt">mission</span> is designed to accomplish several high-priority planetary science goals and will be an important step toward meeting NASAs challenge to send humans to Mars in the 2030s. The <span class="hlt">mission</span> will conduct geological assessments of the rover's landing site, determine the habitability of the environment, search for signs of ancient Martian <span class="hlt">life</span>, and assess natural resources and hazards for future human explorers. The science instruments aboard the rover also will enable scientists to identify and select a collection of rock and soil samples that will be stored for potential return to Earth in the future. The rover also may help designers of a human expedition understand the hazards posed by Martian dust and demonstrate how to collect carbon dioxide from the atmosphere, which could be a valuable resource for producing oxygen and rocket fuel.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140002765','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140002765"><span>Asteroid Redirect Crewed <span class="hlt">Mission</span> Space Suit and EVA System Architecture Trade Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Blanco, Raul A.; Bowie, Jonathan T.; Watson, Richard D.; Sipila, Stephanie A.</p> <p>2014-01-01</p> <p>The Asteroid Redirect Crewed <span class="hlt">Mission</span> (ARCM) requires a Launch/Entry/Abort (LEA) suit capability and short duration Extra Vehicular Activity (EVA) capability for Orion. The EVAs will involve a two-person crew for approximately four hours. Currently, two EVAs are planned with one contingency EVA in reserve. Providing this EVA capability is very challenging due to system level constraints and a new and unknown environment. The goal of the EVA architecture for ARCM is one that builds upon previously developed technologies and lessons learned, and that accomplishes the ARCM <span class="hlt">mission</span> while providing a stepping stone to future <span class="hlt">missions</span> and destinations. The primary system level constraints are to 1) minimize system mass and volume and 2) minimize the interfacing impacts to the baseline Orion design. In order to minimize the interfacing impacts and to not perturb the baseline Orion schedule, the concept of adding "kits" to the baseline system is proposed. These kits consist of: an EVA kit (converts LEA suit to EVA suit), EVA Servicing and Recharge Kit (provides suit consumables), the EVA Tools, Translation Aids & Sample Container Kit (the tools and mobility aids to complete the tasks), the EVA Communications Kit (interface between the EVA radio and the MPCV), and the Cabin Repress Kit (represses the MPCV between EVAs). This paper will focus on the trade space, analysis, and testing regarding the space suit (pressure garment and <span class="hlt">life</span> support system). Historical approaches and lessons learned from all past EVA operations were researched. Previous and current, successfully operated EVA hardware and high technology readiness level (TRL) hardware were evaluated, and a trade study was conducted for all possible pressure garment and <span class="hlt">life</span> support options. Testing and analysis was conducted and a recommended EVA system architecture was proposed. Pressure garment options that were considered for this <span class="hlt">mission</span> include the currently in-use ISS EVA Mobility Unit (EMU), all variations of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140003764','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140003764"><span>Asteroid Redirect Crewed <span class="hlt">Mission</span> Space Suit and EVA System Architecture Trade Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bowie, Jonathan T.; Blanco, Raul A.; Watson, Richard D.; Kelly, Cody; Buffington, Jesse; Sipila, Stephanie A.</p> <p>2014-01-01</p> <p>This paper discusses the Asteroid Redirect Crewed <span class="hlt">Mission</span> (ARCM) space suit and Extravehicular Activity (EVA) architecture trade study and the current state of the work to mature the requirements and products to the <span class="hlt">mission</span> concept review level. The <span class="hlt">mission</span> requirements and the resulting concept of operations will be discussed. A historical context will be presented as to present the similarities and differences from previous NASA <span class="hlt">missions</span>. That will set the stage for the trade study where all options for both pressure garment and <span class="hlt">life</span> support were considered. The rationale for the architecture decisions will then be presented. Since the trade study did identity risks, the subsequent tests and analyses that mitigated the risks will be discussed. Lastly, the current state of the effort will be provided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002iaf..confE.858D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002iaf..confE.858D"><span>Marco Polo : an Italian <span class="hlt">Mission</span> Scoring a lot of Records</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>di Pippo, Simonetta; Bracciaferri, Fabio M.</p> <p>2002-01-01</p> <p>The first astronaut of the European Astronaut Corps of Italian nationality, Roberto Vittori, will fly on a Soyuz capsule at the end of April 2002, opening a new era of space flight. The <span class="hlt">mission</span>, sponsored by the Italian Space Agency, has been developed in the framework of an ESA- ROSAVIAKOSMOS agreement, reached in order to give European astronauts additional possibilities to fly. It's the first <span class="hlt">mission</span> of this kind. In addition to that, this is the real first time in which a Soyuz <span class="hlt">mission</span> is in the hands of two cosmonauts, and one of them is non Russian. On the same flight, in fact, Mark Shuttleworth, the second tourist in the history of space activities, is going to fly, performing also a set of scientific experiments. Marco Polo is also the first <span class="hlt">mission</span> in which the two Agencies, ASI and ESA, are developing a joint commercialisation program, devoted to attire sponsors for improving research and development activities in the Human Spaceflight area. This will allow the two agencies to improve also the quality of <span class="hlt">life</span> on Earth. A comprehensive scientific program is also foreseen accompanying Vittori on board, mainly in the field of <span class="hlt">life</span> science. Experiments devoted to neurophysiology, arms rehabilitation, test of new materials for dressing in space, evaluation of the behaviour of the Nobel Prize Montalcini discovery named NGF (Nerve Growth Factor) will be performed on board. A R&D payload for Blood Pressure Measurements could have in the future commercial spin-off. In addition, a possible institutional sponsorship of the World Health Organization is under discussion. It will be the real first time in which a space <span class="hlt">mission</span> gets this kind of sponsorship, and this strictly related to the World Health Day this year, devoted in promoting health throughout movement, i.e. "Move for Health". The Italian Space Agency proposed a joint combination of the two slogans, coupling the "Move for Health" message with the Italian "Space for Health" one. This is because of the Marco</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800003723','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800003723"><span>Scientific need for a cometary <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Whipple, F. L.</p> <p>1979-01-01</p> <p>Known facts about comets are reviewed including their organic and inorganic content. Photographs are used to show the differences in the physical appearances of the three types of comets. Space <span class="hlt">missions</span> will provide the opportunity to determine the sequence of events that led to their formation and that of the solar system; how volatiles arrived on earth; and the basis for the existence of <span class="hlt">life</span> on earth; and the source of the outer planetary system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960000326','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960000326"><span>Space transfer concepts and analyses for exploration <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Woodcock, Gordon R.</p> <p>1992-01-01</p> <p>The current technical effort is part of the third phase of a broad-scoped and systematic study of space transfer concepts for human lunar and Mars <span class="hlt">missions</span>. The study addressed the technical issues relating to the First Lunar Outpost (FLO) habitation vehicle with emphasis in the structure, power, <span class="hlt">life</span> support system, and radiation environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160013216','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160013216"><span>Woven TPS Enabling <span class="hlt">Missions</span> Beyond Heritage Carbon Phenolic</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stackpoole, M.; Feldman, J.; Venkatapathy, E.</p> <p>2013-01-01</p> <p>WTPS is a new approach to producing TPS architectures that uses precisely engineered 3D weaving techniques to customize material characteristics needed to meet specific <span class="hlt">missions</span> requirements for protecting space vehicles from the intense heating generated during atmospheric entry. Using WTPS, sustainable, scalable, <span class="hlt">mission</span>-optimized TPS solutions can be achieved with relatively low <span class="hlt">life</span> cycle costs compared with the high costs and long development schedules currently associated with material development and certification. WTPS leverages the mature state-of-the-art weaving technology that has evolved from the textile industry to design TPS materials with tailorable performance. Currently, <span class="hlt">missions</span> anticipated encountering heat fluxes in the range of 1500 4000 Wcm2 and pressures greater than 1.5 atm are limited to using fully dense Carbon Phenolic. However, fully dense carbon phenolic is only mass efficient at higher heat fluxes greater than 4000 Wcm2), and current <span class="hlt">mission</span> designs suffer this mass inefficiency for lack of an alternative mid-density TPS. WTPS not only bridges this mid-density TPS gap but also offers a replacement for carbon phenolic, which itself requires a significant and costly redevelopment effort to re-establish its capability for use in the high heat flux <span class="hlt">missions</span> recently prioritized in the NRC Decadal survey, including probe <span class="hlt">missions</span> to Venus, Saturn and Neptune. This presentation will overview the WTPS concept and present some results from initial testing completed comparing WTPS architectures to heritage carbon phenolic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1113998C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1113998C"><span>The Europa Jupiter system <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, K.; Stankov, A.; Pappalardo, R. T.; Greeley, R.; Blanc, M.; Lebreton, J.-P.; van Houten, T.</p> <p>2009-04-01</p> <p> better known. Most important, EJSM would shed new light on the potential for the emergence of <span class="hlt">life</span> in the celestial neighborhood and beyond. The EJSM <span class="hlt">mission</span> architecture provides opportu-nities for coordinated synergistic observations by JEO and JGO of the Jupiter and Ganymede magnetospheres, the volcanoes and torus of Io, the atmosphere of Jupi-ter, and comparative planetology of icy satellites. Each spacecraft could and would conduct "stand-alone" measurements, including the detailed investigation of Europa and Ganymede, providing significant pro-grammatic flexibility. Although engineering advances are needed for JEO (radiation designs) and JGO, no new technologies would be required to execute either EJSM <span class="hlt">mission</span> element. The development schedule for the <span class="hlt">mission</span> is such that a technology developed by 2012 - 2013 could easily be incorporated if it enhances the <span class="hlt">mission</span> capability. Risk mitigation activities are under way to ensure that the radiation designs are implemented in the lowest-risk approach. The baseline <span class="hlt">mission</span> con-cepts include robust mass and power margins. The EJSM <span class="hlt">mission</span> architecture provides the opti-mal balance between science, risk, and cost using three guiding principles: achieve Decadal science; builds on lessons learned; and leverages international collabora-tions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140007369','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140007369"><span>Logistics Reduction Technologies for Exploration <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Broyan, James L., Jr.; Ewert, Michael K.; Fink, Patrick W.</p> <p>2014-01-01</p> <p>Human exploration <span class="hlt">missions</span> under study are very limited by the launch mass capacity of existing and planned vehicles. The logistical mass of crew items is typically considered separate from the vehicle structure, habitat outfitting, and <span class="hlt">life</span> support systems. Consequently, crew item logistical mass is typically competing with vehicle systems for mass allocation. NASA's Advanced Exploration Systems (AES) Logistics Reduction and Repurposing (LRR) Project is developing five logistics technologies guided by a systems engineering cradle-to-grave approach to enable used crew items to augment vehicle systems. Specifically, AES LRR is investigating the direct reduction of clothing mass, the repurposing of logistical packaging, the use of autonomous logistics management technologies, the processing of spent crew items to benefit radiation shielding and water recovery, and the conversion of trash to propulsion gases. The systematic implementation of these types of technologies will increase launch mass efficiency by enabling items to be used for secondary purposes and improve the habitability of the vehicle as the <span class="hlt">mission</span> duration increases. This paper provides a description and the challenges of the five technologies under development and the estimated overall <span class="hlt">mission</span> benefits of each technology.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950060044&hterms=philosophy+life&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dphilosophy%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950060044&hterms=philosophy+life&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dphilosophy%2Blife"><span>Environmental control and <span class="hlt">life</span> support system selection for the first Lunar outpost habitat</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Adams, Alan</p> <p>1993-01-01</p> <p>The planning for and feasibility study of an early human return <span class="hlt">mission</span> to the lunar surface has been undertaken. The First Lunar Outpost (FLO) <span class="hlt">Mission</span> philosophy is to use existing or near-term technology to achieve a human landing on the lunar surface in the year 2000. To support the crew the lunar habitat for the FLO <span class="hlt">mission</span> incorporates an environmental control/<span class="hlt">life</span> support system (ECLSS) design which meets the <span class="hlt">mission</span> requirements and balances fixed mass and consumable mass. This tradeoff becomes one of regenerable <span class="hlt">life</span> support systems versus open-loop systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820054265&hterms=reimburs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dreimburs*','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820054265&hterms=reimburs&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dreimburs*"><span>U.S. <span class="hlt">mission</span> plans for Spacelab</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sander, M. J.</p> <p>1982-01-01</p> <p><span class="hlt">Mission</span> configurations, instrumentation, and objectives for Spacelab sorties on board the Shuttle beginning in Sept. 1983 are reviewed. The first two flights will serve to verify the Spacelab systems and will be followed by operational status, including the fifth flight, which will be a reimbursible venture. Scientific investigations in the fields of atmospheric physics and environmental observation, space plasma physics, astronomy and solar physics, materials processing, and <span class="hlt">life</span> sciences will be performed using the habitable long module, instrument pallets, and/or an instrument igloo mounted in the payload bay. Instrumentation, such as the imaging spectrometric observatory, which was developed in the U.S., will originate in either the U.S. or Europe. Details of the first four Spacelab flights are presented, noting that the OSS-3 through -7 <span class="hlt">missions</span> will feature the first time that entire NASA payloads have returned to space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740019251','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740019251"><span>Applications Explorer <span class="hlt">Missions</span> (AEM): <span class="hlt">Mission</span> planners handbook</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smith, S. R. (Editor)</p> <p>1974-01-01</p> <p>The Applications Explorer <span class="hlt">Missions</span> (AEM) Program is a planned series of space applications <span class="hlt">missions</span> whose purpose is to perform various tasks that require a low cost, quick reaction, small spacecraft in a dedicated orbit. The Heat Capacity Mapping <span class="hlt">Mission</span> (HCMM) is the first <span class="hlt">mission</span> of this series. The spacecraft described in this document was conceived to support a variety of applications instruments and the HCMM instrument in particular. The maximum use of commonality has been achieved. That is, all of the subsystems employed are taken directly or modified from other programs such as IUE, IMP, RAE, and Nimbus. The result is a small versatile spacecraft. The purpose of this document, the AEM <span class="hlt">Mission</span> Planners Handbook (AEM/MPH) is to describe the spacecraft and its capabilities in general and the HCMM in particular. This document will also serve as a guide for potential users as to the capabilities of the AEM spacecraft and its achievable orbits. It should enable each potential user to determine the suitability of the AEM concept to his <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040088836&hterms=primates&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dprimates','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040088836&hterms=primates&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dprimates"><span>Bion 11 <span class="hlt">mission</span>: primate experiments</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ilyin, E. A.; Korolkov, V. I.; Skidmore, M. G.; Viso, M.; Kozlovskaya, I. B.; Grindeland, R. E.; Lapin, B. A.; Gordeev, Y. V.; Krotov, V. P.; Fanton, J. W.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20040088836'); toggleEditAbsImage('author_20040088836_show'); toggleEditAbsImage('author_20040088836_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20040088836_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20040088836_hide"></p> <p>2000-01-01</p> <p>A summary is provided of the major operations required to conduct the wide range of primate experiments on the Bion 11 <span class="hlt">mission</span>, which flew for 14 days beginning December 24, 1996. Information is given on preflight preparations, including flight candidate selection and training; attachment and implantation of bioinstrumentation; flight and ground experiment designs; onboard <span class="hlt">life</span> support and test systems; ground and flight health monitoring; flight monkey selection and transport to the launch site; inflight procedures and data collection; postflight examinations and experiments; and assessment of results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018LPICo2071.6033S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018LPICo2071.6033S"><span>Landing Sites for a Mars Sample Return <span class="hlt">Mission</span> in Arabia Terra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Salese, F.; Pondrelli, M.; Schmidt, G. W.; Mitri, G.; Pacifici, A.; Cavalazzi, B.; Ori, G. G.; Glamoclija, M.; Hauber, E.; Le Deit, L.; Marinangeli, L.; Rossi, A. P.</p> <p>2018-04-01</p> <p>We are characterizing the geology of several areas in Arabia Terra as possible Mars Sample Return <span class="hlt">mission</span> landing sites. Arabia Terra presents several interesting sites regarding the search for past traces of <span class="hlt">life</span> on Mars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMED51G0842L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMED51G0842L"><span>Exomars <span class="hlt">Mission</span> Achievements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lecomte, J.; Juillet, J. J.</p> <p>2016-12-01</p> <p>ExoMars is the first step of the European Space Agency's Aurora Exploration Programme. Comprising two <span class="hlt">missions</span>, the first one launched in 2016 and the second one to be launched in 2020, ExoMars is a program developed in a broad ESA and Roscosmos co-operation, with significant contribution from NASA that addresses the scientific question of whether <span class="hlt">life</span> ever existed on Mars and demonstrate key technologies for entry, descent, landing, drilling and roving on the Martian surface . Thales Alenia Space is the overall prime contractor of the Exomars program leading a large industrial team The Spacecraft Composite (SCC), consisting of a Trace Gas Orbiter (TGO) and an EDL (Entry Descend and Landing) Demonstrator Module (EDM) named Schiaparelli, has been launched on 14 March 2016 from the Baikonur Cosmodrome by a Proton Launcher. The two modules will separate on 16 October 2016 after a 7 months cruise. The TGO will search for evidence of methane and other atmospheric gases that could be signatures of active biological or geological processes on Mars and will provide communications relay for the 2020 surface assets. The Schiaparelli module will prove the technologies required to safely land a payload on the surface of Mars, with a package of sensors aimed to support the reconstruction of the flown trajectory and the assessment of the performance of the EDL subsystems. For the second Exomars <span class="hlt">mission</span> a space vehicle composed of a Carrier Module (CM) and a Descent Module (DM), whose Landing Platform (LP) will house a Rover, will begin a 7 months long trip to Mars in August 2020. In 2021 the Descent Module will be separated from the Carrier to carry out the entry into the planet's atmosphere and subsequently make the Landing Platform and the Rover land gently on the surface of Mars. While the LP will continue to measure the environmental parameters of the landing site, the Rover will begin exploration of the surface, which is expected to last 218 Martian days (approx. 230 Earth</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-9610973&hterms=Operations+Management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D90%26Ntt%3DOperations%2BManagement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-9610973&hterms=Operations+Management&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D90%26Ntt%3DOperations%2BManagement"><span>Data Management Coordinators Monitor STS-78 <span class="hlt">Mission</span> at the Huntsville Operations Support Center</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1996-01-01</p> <p>Launched on June 20, 1996, the STS-78 <span class="hlt">mission</span>'s primary payload was the <span class="hlt">Life</span> and Microgravity Spacelab (LMS), which was managed by the Marshall Space Flight Center (MSFC). During the 17 day space flight, the crew conducted a diverse slate of experiments divided into a mix of <span class="hlt">life</span> science and microgravity investigations. In a manner very similar to future International Space Station operations, LMS researchers from the United States and their European counterparts shared resources such as crew time and equipment. Five space agencies (NASA/USA, European Space Agency/Europe (ESA), French Space Agency/France, Canadian Space Agency /Canada, and Italian Space Agency/Italy) along with research scientists from 10 countries worked together on the design, development and construction of the LMS. This photo represents Data Management Coordinators monitoring the progress of the <span class="hlt">mission</span> at the Huntsville Operations Support Center (HOSC) Spacelab Payload Operations Control Center (SL POCC) at MSFC. Pictured are assistant <span class="hlt">mission</span> scientist Dr. Dalle Kornfeld, Rick McConnel, and Ann Bathew.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020039737&hterms=rooting&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Drooting','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020039737&hterms=rooting&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Drooting"><span>Exploring for Martian <span class="hlt">Life</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Farmer, Jack D.; Chang, Sherwood (Technical Monitor)</p> <p>1997-01-01</p> <p>Terrestrial <span class="hlt">life</span> appears to have arisen very quickly during late accretion, sometime between approximately 3.5 and 4.2 Ga. During this same time, liquid water appears to have been abundant at the surface of Mars and it is quite plausable that <span class="hlt">life</span> originated there as well. We now believe that the last common ancestor of terrestrial <span class="hlt">life</span> was a sulfur-metabolizing microbe that lived at high temperatures. Rooting of the RNA tree in thermophily probably reflects high temperature "bottle-necking" of the biosphere by giant impacts during late accretion, sometime after <span class="hlt">life</span> had originated. If high temperature bottle-necking is a general property of early biosphere development, Martian <span class="hlt">life</span> may have also developed in close association with hydrothermal systems. Several independent lines of evidence suggest that hydrothermal processes have played an important role during the geological history of Mars. Because hydrothermal deposits on Earth are known to capture and retain abundant microbial fossil information, they are considered prime targets in the search for an ancient Martian biosphere. An important step in planning for future landed <span class="hlt">missions</span> to Mars is the selection of priority targets for high resolution orbital mapping. Geotectonic terranes on Mars that provide a present focus for ongoing site selection studies include channels located along the margins of impact crater melt sheets, or on the slopes of ancient Martian volcanoes, chaotic and fretted terranes where shallow subsurface heat sources are thought to have interacted with ground ice, and the floors of calderas and rifted basins. Orbital <span class="hlt">missions</span> in 1996, 1998 and 2001 will provide opportunities for high resolution geological mapping at key sites in such terranes, as a basis for selecting targets for future landed <span class="hlt">missions</span> for exopaleontology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002cosp...34E1732S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002cosp...34E1732S"><span>Radiobiological foundation of crew radiation risk for mars <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shafirkin, A.</p> <p></p> <p>The results of a comprehensive clinico-physiological study of 250 dogs after 22 hours per day chronic exposure to gamma -radiation throughout their <span class="hlt">life</span> are presented. The exposure duration was 3 and 6 years. The dose rate varied between 25 and 150 cSv/year to simulate galactic cosmic ray dose of crew members during mars <span class="hlt">mission</span>. Several groups of the dogs received an additional acute dose of 10 and 50 cSv during a day three times per year to simulate stochastic irradiation caused by solar cosmic rays. Data on the status of regulatory systems of organism, exchange processes dynamics, organism reaction on additional functional loads are also presented. Organism reaction and dynamics of kinetic relations are considered in detail for most radiosensitive and regenerating tissue systems of the organism, namely, bloodforming system and spermatogenic epithelium. The results on <span class="hlt">life</span> span reduction of the dogs and dog race characteristics after the radiation exposure are discussed. Based on the results obtained in this study and in model experiments realized with big amount of small laboratory animals that were exposed to a wide dose range, using other published data, mathematical models were developed, e. g. a model of radiation damage forming as dependent on time with taking into account recovery processes, and a model of radiation mortality rate of mammals. Based on these models and analysis of radiation environment behind various shielding on the route to Mars, crew radiation risk was calculated for space <span class="hlt">missions</span> of various durations. Total radiation risk values for cosmonaut lifetime after the <span class="hlt">missions</span> were also estimated together with expected <span class="hlt">life</span> span reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cosp...40E..52A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cosp...40E..52A"><span>Radiobiological foundation of crew radiation risk for Mars <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aleksandr, Shafirkin; Grigoriev, Yurj</p> <p></p> <p>The results of a comprehensive clinico-physiological study of 250 dogs after 22 hours per day chronic exposure to gamma-radiation throughout their <span class="hlt">life</span> are presented. The exposure duration was 3 and 6 years. The dose rate varied between 25 and 150 cSv/year to simulate galactic cosmic ray dose of crew members during mars <span class="hlt">mission</span>. Several groups of the dogs received an additional acute dose of 10 and 50 cSv during a day three times per year to simulate stochastic irradiation caused by solar cosmic rays. Data on the status of regulatory systems of organism, exchange processes dynamics, organism reaction on additional functional loads are also presented. Organism reaction and dynamics of kinetic relations are considered in detail for most radiosensitive and regenerating tissue systems of the organism, namely, bloodforming system and spermatogenic epithelium. The results on <span class="hlt">life</span> span reduction of the dogs and dog race characteristics after the radiation exposure are discussed. Based on the results obtained in this study and in model experiments realized with big amount of small laboratory animals that were exposed to a wide dose range, using other published data, mathematical models were developed, e. g. a model of radiation damage forming as dependent on time with taking into account recovery processes, and a model of radiation mortality rate of mammals. Based on these models and analysis of radiation environment behind various shielding on the route to Mars, crew radiation risk was calculated for space <span class="hlt">missions</span> of various durations. Total radiation risk values for cosmonaut lifetime after the <span class="hlt">missions</span> were also estimated together with expected <span class="hlt">life</span> span reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150011990&hterms=ion+batteries&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dion%2Bbatteries','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150011990&hterms=ion+batteries&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dion%2Bbatteries"><span>Performance Testing of Yardney Li-Ion Cells and Batteries in Support of Future NASA <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Smart, M. C.; Ratnakumar, B. V.; Whitcanack, L. D.; Puglia, F. J.; Santee, S.; Gitzendanner, R.</p> <p>2009-01-01</p> <p>NASA requires lightweight rechargeable batteries for future <span class="hlt">missions</span> to Mars and the outer planets that are capable of operating over a wide range of temperatures, with high specific energy and energy densities. Due to the attractive performance characteristics, Li-ion batteries have been identified as the battery chemistry of choice for a number of future applications. For example, JPL is planning to launch another unmanned rover <span class="hlt">mission</span> to the planet Mars. This <span class="hlt">mission</span>, referred to as the Mars Science Laboratory (MSL), will involve the use of a rover that is much larger than the previously developed Spirit and Opportunity Rovers for the 2003 Mars Exploration Rover (MER) <span class="hlt">mission</span>, that are currently still in operation on the surface of the planet after more than five years. Part of the reason that the MER rovers have operated so successfully, far exceeding the required <span class="hlt">mission</span> duration of 90 sols, is that they possess robust Li-ion batteries, manufactured by Yardney Technical Products, which have demonstrated excellent <span class="hlt">life</span> characteristics. Given the excellent performance characteristics displayed, similar Li-ion batteries have been projected to successfully meet the <span class="hlt">mission</span> requirements of the up-coming MSL <span class="hlt">mission</span>. In addition to future <span class="hlt">missions</span> to Mars, Li-ion technology is attractive for a number of other future NASA applications which require high specific energy, rechargeable batteries. To ascertain the viability of using Li-ion batteries for these applications, a number of performance validation tests have been performed on both Yardney cells and batteries of various sizes. These tests include <span class="hlt">mission</span> simulation tests, charge and discharge rate characterization testing, cycle <span class="hlt">life</span> testing under various conditions, and storage testing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150007660','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150007660"><span>Advanced Stirling Radioisotope Generator <span class="hlt">Life</span> Certification Plan</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rusick, Jeffrey J.; Zampino, Edward J.</p> <p>2013-01-01</p> <p>An Advanced Stirling Radioisotope Generator (ASRG) power supply is being developed by the Department of Energy (DOE) in partnership with NASA for potential future deep space science <span class="hlt">missions</span>. Unlike previous radioisotope power supplies for space exploration, such as the passive MMRTG used recently on the Mars Curiosity rover, the ASRG is an active dynamic power supply with moving Stirling engine mechanical components. Due to the long <span class="hlt">life</span> requirement of 17 years and the dynamic nature of the Stirling engine, the ASRG project faced some unique challenges trying to establish full confidence that the power supply will function reliably over the <span class="hlt">mission</span> <span class="hlt">life</span>. These unique challenges resulted in the development of an overall <span class="hlt">life</span> certification plan that emphasizes long-term Stirling engine test and inspection when analysis is not practical. The ASRG <span class="hlt">life</span> certification plan developed is described.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840047766&hterms=economic+papers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deconomic%2Bpapers','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840047766&hterms=economic+papers&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deconomic%2Bpapers"><span>Analysis of heliographic <span class="hlt">missions</span> complementary to ISPM. [International Solar Polar <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Driver, J. M.</p> <p>1984-01-01</p> <p>Five concepts were formulated, analyzed, and compared for satisfying heliographic science <span class="hlt">mission</span> objectives both with and without a concurrent International Solar Polar <span class="hlt">Mission</span> (ISPM) Spacecraft. Key astrodynamic constraints and performance factors are known from literature for the Lagrange point <span class="hlt">mission</span> and the sun-synchronous earth orbit <span class="hlt">mission</span>, but are set forth in this paper for the three solar orbiting <span class="hlt">missions</span> concepts considered. Any of these five <span class="hlt">missions</span> should be doable at modest cost since no strong cost drivers were encountered in the analyses. The <span class="hlt">mission</span> to be flown depends on <span class="hlt">mission</span> capability to meet science measurement needs more than on strong economic factors. Each <span class="hlt">mission</span> offers special advantages for particular measurement emphasis. Based on selected qualitative <span class="hlt">mission</span> discriminators, an overall 'best <span class="hlt">mission</span>' was selected and described in some detail.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000064109','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000064109"><span>Ceramic Matrix Composites (CMC) <span class="hlt">Life</span> Prediction Method Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levine, Stanley R.; Calomino, Anthony M.; Ellis, John R.; Halbig, Michael C.; Mital, Subodh K.; Murthy, Pappu L.; Opila, Elizabeth J.; Thomas, David J.; Thomas-Ogbuji, Linus U.; Verrilli, Michael J.</p> <p>2000-01-01</p> <p>Advanced launch systems (e.g., Reusable Launch Vehicle and other Shuttle Class concepts, Rocket-Based Combine Cycle, etc.), and interplanetary vehicles will very likely incorporate fiber reinforced ceramic matrix composites (CMC) in critical propulsion components. The use of CMC is highly desirable to save weight, to improve reuse capability, and to increase performance. CMC candidate applications are <span class="hlt">mission</span> and cycle dependent and may include turbopump rotors, housings, combustors, nozzle injectors, exit cones or ramps, and throats. For reusable and single <span class="hlt">mission</span> uses, accurate prediction of <span class="hlt">life</span> is critical to <span class="hlt">mission</span> success. The tools to accomplish <span class="hlt">life</span> prediction are very immature and not oriented toward the behavior of carbon fiber reinforced silicon carbide (C/SiC), the primary system of interest for a variety of space propulsion applications. This paper describes an approach to satisfy the need to develop an integrated <span class="hlt">life</span> prediction system for CMC that addresses mechanical durability due to cyclic and steady thermomechanical loads, and takes into account the impact of environmental degradation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10983153','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10983153"><span>[The <span class="hlt">mission</span>].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ruiz Moreno, J; Blanch Mon, A</p> <p>2000-01-01</p> <p>After having made a historical review of the concept of <span class="hlt">mission</span> statement, of evaluating its importance (See Part I), of describing the bases to create a <span class="hlt">mission</span> statement from a strategic perspective and of analyzing the advantages of this concept, probably more important as a business policy (See Parts I and II), the authors proceed to analyze the <span class="hlt">mission</span> statement in health organizations. Due to the fact that a <span class="hlt">mission</span> statement is lacking in the majority of health organizations, the strategy of health organizations are not exactly favored; as a consequence, neither are its competitive advantage nor the development of its essential competencies. After presenting a series of <span class="hlt">mission</span> statements corresponding to Anglo-Saxon health organizations, the authors highlight two <span class="hlt">mission</span> statements corresponding to our social context. The article finishes by suggesting an adequate sequence for developing a <span class="hlt">mission</span> statement in those health organizations having a strategic sense.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMSA43A2132K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMSA43A2132K"><span>Measurement of LF Standard-Frequency Waves JJY along the track of Shirase, the Japanese Antarctic Research <span class="hlt">Icebreaker</span>, during JARE53-JARE54</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kitauchi, H.; Nozaki, K.; Ito, H.; Tsuchiya, S.; Imamura, K.; Nagatsuma, T.</p> <p>2013-12-01</p> <p>We first obtained a strong evidence of reception of the low frequency (LF) radio waves, 40 kHz and 60 kHz, of the call sign JJY by use of a newly developed, highly sensitive receiving system on board the Japanese Antarctic research <span class="hlt">icebreaker</span> Shirase offshore East Ongul Island, East Antarctica--about 14,000 km away from those transmitting stations in Japan. The measured data sets of the electric field intensity and phase of those signals are to be analysed to examine and/or improve numerical prediction methods of field strength for long-distance propagation of LF radio waves, contributing to the Recommendation 'Prediction of field strength at frequencies below about 150 kHz' made by International Telecommunication Union Radiocommunication Sector (ITU-R). The call sign JJY of standard frequency and time signals (SFTS) of LF 40 kHz and 60 kHz are emitted from the transmitting stations, respectively, Ohtakadoya-yama 37° 22‧ 21″ N, 140° 50‧ 56″ E in Fukushima Prefecture (eastern Japan) and Hagane-yama 33° 27‧ 56″ N, 130° 10‧ 32″ E in Saga/Fukuoka Prefecture (western Japan) by NICT. Those are widely used for calibrating frequency standard oscillators and radio-controlled clocks in Japan. Since low signal attenuation in LF radio band allows long distance communication, kilometre waves have been utilized for operations such as SFTS and military communications around the world. Therefore, there is a need to give guidance to engineers for the planning of radio services in LF band so as to avoid interference. ITU-R recommends the guidance 'Prediction of field strength at frequencies below about 150 kHz', in which a numerical prediction method is proposed to compute the electric field intensity, up to 16,000 km of long-distance propagation, away from the transmitting station. Since reliable data sets are limited for the long-distance propagation, in this study we tried to measure the field strength and phase of the LF SFTS JJY of 40 kHz and 60 kHz over 14</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008cosp...37.2998S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008cosp...37.2998S"><span>Active shielding for long duration interplanetary manned <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spillantini, Piero</p> <p></p> <p>The problem of protecting astronauts from the cosmic rays action in unavoidable and was therefore preliminary studied by many space agencies. In Europe, in the years 2002-2004, ESA supported two works on this thematic: a topical team in the frame of the ‘<span class="hlt">life</span> and physical sciences' and a study, assigned by tender, of the ‘radiation exposure and <span class="hlt">mission</span> strategies for interplanetary manned <span class="hlt">missions</span> to Moon and Mars'. In both studies it was concluded that, while the protection from solar cosmic rays can relay on the use of passive absorbers, for long duration <span class="hlt">missions</span> the astronauts must be protected from the much more energetic galactic cosmic rays during the whole duration of the <span class="hlt">mission</span>. This requires the protection of a large habitat where they could live and work, and not a temporary small volume shelter, and the use of active shielding is therefore mandatory. The possibilities offered by using superconducting magnets were discussed, and the needed R&D recommended. The technical development occurred in the meantime and the evolution of the panorama of the possible interplanetary <span class="hlt">missions</span> in the near future require to revise these pioneer studies and think of the problem at a scale allowing long human permanence in ‘deep' space, and not for a relatively small number of dedicated astronauts but also for citizens conducting there ‘normal' activities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013134','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013134"><span>Asteroid Redirect Crewed <span class="hlt">Mission</span> Space Suit and EVA System Architecture Trade Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bowie, Jonathan; Buffington, Jesse; Hood, Drew; Kelly, Cody; Naids, Adam; Watson, Richard; Blanco, Raul; Sipila, Stephanie</p> <p>2014-01-01</p> <p>The Asteroid Redirect Crewed <span class="hlt">Mission</span> (ARCM) requires a Launch/Entry/Abort (LEA) suit capability and short duration Extra Vehicular Activity (EVA) capability from the Orion spacecraft. For this <span class="hlt">mission</span>, the pressure garment selected for both functions is the Modified Advanced Crew Escape Suit (MACES) with EVA enhancements and the <span class="hlt">life</span> support option that was selected is the Exploration Portable <span class="hlt">Life</span> Support System (PLSS) currently under development for Advanced Exploration Systems (AES). The proposed architecture meets the ARCM constraints, but much more work is required to determine the details of the suit upgrades, the integration with the PLSS, and the tools and equipment necessary to accomplish the <span class="hlt">mission</span>. This work has continued over the last year to better define the operations and hardware maturation of these systems. EVA simulations were completed in the Neutral Buoyancy Lab (NBL) and interfacing options were prototyped and analyzed with testing planned for late 2014. This paper discusses the work done over the last year on the MACES enhancements, the use of tools while using the suit, and the integration of the PLSS with the MACES.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006cosp...36.2562B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006cosp...36.2562B"><span>Closure of regenerative <span class="hlt">life</span> support systems: results of the Lunar-Mars <span class="hlt">Life</span> Support Test Project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barta, D.; Henninger, D.; Edeen, M.; Lewis, J.; Smith, F.; Verostko, C.</p> <p></p> <p>Future long duration human exploration <span class="hlt">missions</span> away from Earth will require closed-loop regenerative <span class="hlt">life</span> support systems to reduce launch mass reduce dependency on resupply and increase the level of <span class="hlt">mission</span> self sufficiency Such systems may be based on the integration of biological and physiocochemical processes to produce potable water breathable atmosphere and nutritious food from metabolic and other <span class="hlt">mission</span> wastes Over the period 1995 to 1998 a series of ground-based tests were conducted at the National Aeronautics and Space Administration Johnson Space Center to evaluate the performance of advanced closed-loop <span class="hlt">life</span> support technologies with real human metabolic and hygiene loads Named the Lunar-Mars <span class="hlt">Life</span> Support Test Project LMLSTP four integrated human tests were conducted with increasing duration complexity and closure The first test LMLSTP Phase I was designed to demonstrate the ability of higher plants to revitalize cabin atmosphere A single crew member spent 15 days within an atmospherically closed chamber containing 11 2 square meters of actively growing wheat Atmospheric carbon dioxide and oxygen levels were maintained by control of the rate of photosynthesis through manipulation of light intensity or the availability of carbon dioxide and included integrated physicochemical systems During the second and third tests LMLSTP Phases II IIa four crew members spent 30 days and 60 days respectively in a larger sealed chamber Advanced physicochemical <span class="hlt">life</span> support hardware was used to regenerate the atmosphere and produce potable water</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950010820','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950010820"><span>A <span class="hlt">mission</span> planning concept and <span class="hlt">mission</span> planning system for future manned space <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wickler, Martin</p> <p>1994-01-01</p> <p>The international character of future manned space <span class="hlt">missions</span> will compel the involvement of several international space agencies in <span class="hlt">mission</span> planning tasks. Additionally, the community of users requires a higher degree of freedom for experiment planning. Both of these problems can be solved by a decentralized <span class="hlt">mission</span> planning concept using the so-called 'envelope method,' by which resources are allocated to users by distributing resource profiles ('envelopes') which define resource availabilities at specified times. The users are essentially free to plan their activities independently of each other, provided that they stay within their envelopes. The new developments were aimed at refining the existing vague envelope concept into a practical method for decentralized planning. Selected critical functions were exercised by planning an example, founded on experience acquired by the MSCC during the Spacelab <span class="hlt">missions</span> D-1 and D-2. The main activity regarding future <span class="hlt">mission</span> planning tasks was to improve the existing MSCC <span class="hlt">mission</span> planning system, using new techniques. An electronic interface was developed to collect all formalized user inputs more effectively, along with an 'envelope generator' for generation and manipulation of the resource envelopes. The existing scheduler and its data base were successfully replaced by an artificial intelligence scheduler. This scheduler is not only capable of handling resource envelopes, but also uses a new technology based on neuronal networks. Therefore, it is very well suited to solve the future scheduling problems more efficiently. This prototype <span class="hlt">mission</span> planning system was used to gain new practical experience with decentralized <span class="hlt">mission</span> planning, using the envelope method. In future steps, software tools will be optimized, and all data management planning activities will be embedded into the scheduler.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130011598','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130011598"><span>Lunar Simulants, Analogues, and Standards: Needs and Realities for <span class="hlt">Mission</span> Technologies Development</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sibille, Laurent</p> <p>2013-01-01</p> <p>Integration of In-Situ Resource Utilization (ISRU) capabilities into <span class="hlt">missions</span> present both challenges as well as benefits for future <span class="hlt">missions</span> to the Moon and Mars. However, since ISRU systems and capabilities have not flown, <span class="hlt">mission</span> planners have been hesitant to include ISRU capabilities in <span class="hlt">mission</span> critical roles, thereby significantly reducing the benefits that ISRU can provide in <span class="hlt">mission</span> mass and cost reductions. For ISRU systems to provide products and services to 'customers' such as <span class="hlt">life</span> support, propulsion, and power systems, close development of requirements, hardware, and operations between ISRU and these systems are required. To address these development and incorporation challenges, NASA and csA initiated a series of analog field test demonstrations at sites in Hawaii. Two tests completed in November of 2008 and February of 2010 have demonstrate all the critical steps in operating ISRU systems on the lunar surface at relevant <span class="hlt">mission</span> scales as well as integration with power and propulsion systems. The third field test planned for July 2012 will demonstrate that a <span class="hlt">mission</span> to the lunar poles to locate and characterize ice and other volatiles is possible in a highly integrated <span class="hlt">mission</span> with multiple space agencies. These analog field tests have shown that not only are ISRU systems feasible at relevant <span class="hlt">mission</span> scales, that they can be successfully integrated into <span class="hlt">mission</span> architectures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E.521E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E.521E"><span>The Search for <span class="hlt">Life</span> in the Solar System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ehrenfreund, Pascale</p> <p>2016-07-01</p> <p>To unravel the origins of <span class="hlt">life</span> on Earth and possibly elsewhere remains one of mankind's most important discoveries. Basic building blocks of <span class="hlt">life</span> are widespread in planetary systems in our Milky Way and other galaxies. Extraterrestrial material delivered to young terrestrial planetary surfaces in the early history of our solar system through asteroids, comets and meteorites may have provided significant raw material for the emergence of <span class="hlt">life</span> on Earth. Since August 2014 the comet rendezvous <span class="hlt">mission</span> Rosetta has monitored the evolution of comet 67P/Churyumov-Gerasimenko during its approach to the Sun and observed numerous volatiles and complex organic compounds on the comet surface. Several asteroid sample return <span class="hlt">missions</span> as well as the improved analyses of key meteorites increase our knowledge about the organic inventory that seeded the young planets. Prokaryotic, anaerobic bacteria, which are approximately 3.5 billion years old, represent the first evidence for <span class="hlt">life</span> on Earth. Since then, <span class="hlt">life</span> has evolved to high complexity and adapted to nearly every explored environment on our planet. Extreme <span class="hlt">life</span> on Earth has expanded the list of potentially habitable solar system environments. However, our neighbor planet Mars is the most promising target to search for <span class="hlt">life</span> within our solar system. Data from the Curiosity rover show regions that were habitable in the past, traces of organic carbon and active CH_4 in the Martian atmosphere at present. Recent discoveries such as the plumes from the southern polar region of Enceladus and plume activity on Europa strengthen the long-standing hypothesis that moons in our solar system contain substantial bodies of water and are probably habitable. Since decades, a fleet of robotic space <span class="hlt">missions</span> target planets, moons and small bodies to reveal clues on the origin of our solar system and <span class="hlt">life</span> beyond Earth. This lecture will review and discuss past, current and future space <span class="hlt">missions</span> investigating habitability and biosignatures in our</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AsBio...7..578P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AsBio...7..578P"><span>Searching for <span class="hlt">Life</span> on Mars: Selection of Molecular Targets for ESA's Aurora ExoMars <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parnell, John; Cullen, David; Sims, Mark R.; Bowden, Stephen; Cockell, Charles S.; Court, Richard; Ehrenfreund, Pascale; Gaubert, Francois; Grant, William; Parro, Victor; Rohmer, Michel; Sephton, Mark; Stan-Lotter, Helga; Steele, Andrew; Toporski, Jan; Vago, Jorge</p> <p>2007-08-01</p> <p>The European Space Agency's ExoMars <span class="hlt">mission</span> will seek evidence of organic compounds of biological and non-biological origin at the martian surface. One of the instruments in the Pasteur payload may be a <span class="hlt">Life</span> Marker Chip that utilizes an immunoassay approach to detect specific organic molecules or classes of molecules. Therefore, it is necessary to define and prioritize specific molecular targets for antibody development. Target compounds have been selected to represent meteoritic input, fossil organic matter, extant (living, recently dead) organic matter, and contamination. Once organic molecules are detected on Mars, further information is likely to derive from the detailed distribution of compounds rather than from single molecular identification. This will include concentration gradients beneath the surface and gradients from generic to specific compounds. The choice of biomarkers is informed by terrestrial biology but is wide ranging, and nonterrestrial biology may be evident from unexpected molecular distributions. One of the most important requirements is to sample where irradiation and oxidation are minimized, either by drilling or by using naturally excavated exposures. Analyzing regolith samples will allow for the search of both extant and fossil biomarkers, but sequential extraction would be required to optimize the analysis of each of these in turn.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17723091','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17723091"><span>Searching for <span class="hlt">life</span> on Mars: selection of molecular targets for ESA's aurora ExoMars <span class="hlt">mission</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Parnell, John; Cullen, David; Sims, Mark R; Bowden, Stephen; Cockell, Charles S; Court, Richard; Ehrenfreund, Pascale; Gaubert, Francois; Grant, William; Parro, Victor; Rohmer, Michel; Sephton, Mark; Stan-Lotter, Helga; Steele, Andrew; Toporski, Jan; Vago, Jorge</p> <p>2007-08-01</p> <p>The European Space Agency's ExoMars <span class="hlt">mission</span> will seek evidence of organic compounds of biological and non-biological origin at the martian surface. One of the instruments in the Pasteur payload may be a <span class="hlt">Life</span> Marker Chip that utilizes an immunoassay approach to detect specific organic molecules or classes of molecules. Therefore, it is necessary to define and prioritize specific molecular targets for antibody development. Target compounds have been selected to represent meteoritic input, fossil organic matter, extant (living, recently dead) organic matter, and contamination. Once organic molecules are detected on Mars, further information is likely to derive from the detailed distribution of compounds rather than from single molecular identification. This will include concentration gradients beneath the surface and gradients from generic to specific compounds. The choice of biomarkers is informed by terrestrial biology but is wide ranging, and nonterrestrial biology may be evident from unexpected molecular distributions. One of the most important requirements is to sample where irradiation and oxidation are minimized, either by drilling or by using naturally excavated exposures. Analyzing regolith samples will allow for the search of both extant and fossil biomarkers, but sequential extraction would be required to optimize the analysis of each of these in turn.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930015896','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930015896"><span>A survey of <span class="hlt">life</span> support system automation and control</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Finn, Cory K.</p> <p>1993-01-01</p> <p>The level of automation and control necessary to support advanced <span class="hlt">life</span> support systems for use in the manned space program is steadily increasing. As the length and complexity of manned <span class="hlt">missions</span> increase, <span class="hlt">life</span> support systems must be able to meet new space challenges. Longer, more complex <span class="hlt">missions</span> create new demands for increased automation, improved sensors, and improved control systems. It is imperative that research in these key areas keep pace with current and future developments in regenerative <span class="hlt">life</span> support technology. This paper provides an overview of past and present research in the areas of sensor development, automation, and control of <span class="hlt">life</span> support systems for the manned space program, and it discusses the impact continued research in several key areas will have on the feasibility, operation, and design of future <span class="hlt">life</span> support systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cosp...40E3019S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cosp...40E3019S"><span>Strategic Map for Enceladus Plume Biosignature Sample Return <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sherwood, Brent; Yano, Hajime</p> <p></p> <p>The discovery of jets emitting salty water from the interior of Saturn’s small moon Enceladus is one of the most astounding results of the Cassini <span class="hlt">mission</span> to date. The measured presence of organic species in the resulting plume, the finding that the jet activity is valved by tidal stretching at apochrone, and the modeled lifetime of E-ring particles, all indicate that the textbook conditions for habitability are met at Enceladus today: liquid water, biologically available elements, and source of energy, longevity of conducive conditions. Enceladus may be the best place in our solar system to search for direct evidence of biomarkers, and the plume provides a way to sample for and even return them to Earth for detailed analysis. It is straightforward to imagine a Stardust-like, fly-through, plume particle and gas collection and return <span class="hlt">mission</span> for Enceladus. An international team (<span class="hlt">LIFE</span>, <span class="hlt">Life</span> Investigation For Enceladus) has dedicated itself to pursuing such a flight project. Concept engineering and evaluation indicate that the associated technical, programmatic, regulatory, and cost issues are quite unlike the Stardust precedent however, not least because of such a mission’s Category-V, Restricted Earth Return, classification. The paper presents a strategic framework that systematically integrates the cultivation of science advocacy, resolution of diverse stakeholder issues, development of verifiable and affordable technical solutions, validation of cost estimation methods, alignment with other candidate astrobiology <span class="hlt">missions</span>, complementarity of international agency goals, and finally the identification of appropriate research and flight-<span class="hlt">mission</span> opportunities. Resolving and using this map is essential if we are to know the astrobiological state of Enceladus in our lifetime.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070036669','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070036669"><span>Advances in Radiation-Tolerant Solar Arrays for SEP <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>O'Neill, Mark J.; Eskenazi, Michael I.; Ferguson, Dale C.</p> <p>2007-01-01</p> <p>As the power levels of commercial communications satellites reach the 20 kWe and higher, new options begin to emerge for transferring the satellite from LEO to GEO. In the past electric propulsion has been demonstrated successfully for this <span class="hlt">mission</span> - albeit under unfortunate circumstances when the kick motor failed. The unexpected use of propellant for the electric propulsion (EP) system compromised the <span class="hlt">life</span> of that vehicle, but did demonstrate the viability of such an approach. Replacing the kick motor on a satellite and replacing that mass by additional propellant for the EP system as well as mass for additional revenue-producing transponders should lead to major benefits for the provider. Of course this approach requires that the loss in solar array power during transit of the Van Allen radiation belts is not excessive and still enables the 15 to 20 year <span class="hlt">mission</span> <span class="hlt">life</span>. In addition, SEP <span class="hlt">missions</span> to Jupiter, with its exceptional radiation belts, would mandate a radiation-resistant solar array to compete with a radioisotope alternative. Several critical issues emerge as potential barriers to this approach: reducing solar array radiation damage, operating the array at high voltage (>300 V) for extended times for Hall or ion thrusters, designing an array that will be resistant to micrometeoroid impacts and the differing environmental conditions as the vehicle travels from LEO to GEO (or at Jupiter), producing an array that is light weight to preserve payload mass fraction - and to do this at a cost that is lower than today's arrays. This paper will describe progress made to date on achieving an array that meets all these requirements and is also useful for deep space electric propulsion <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090036320&hterms=life+planets&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlife%2Bplanets','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090036320&hterms=life+planets&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlife%2Bplanets"><span>Starship <span class="hlt">Life</span> Support</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Harry W.</p> <p>2009-01-01</p> <p>The design and mass cost of a starship and its <span class="hlt">life</span> support system are investigated. The <span class="hlt">mission</span> plan for a multi generational interstellar voyage to colonize a new planet is used to describe the starship design, including the crew habitat, accommodations, and <span class="hlt">life</span> support. Only current technology is assumed. Highly reliable <span class="hlt">life</span> support systems can be provided with reasonably small additional mass, suggesting that they can support long duration <span class="hlt">missions</span>. Bioregenerative <span class="hlt">life</span> support, growing crop plants that provide food, water, and oxygen, has been thought to need less mass than providing stored food for long duration <span class="hlt">missions</span>. The large initial mass of hydroponics systems is paid for over time by saving the mass of stored food. However, the yearly logistics mass required to support a bioregenerative system exceeds the mass of food solids it produces, so that supplying stored dehydrated food always requires less mass than bioregenerative food production. A mixed system that grows about half the food and supplies the other half dehydrated has advantages that allow it to breakeven with stored dehydrated food in about 66 years. However, moderate increases in the hydroponics system mass to achieve high reliability, such as adding spares that double the system mass and replacing the initial system every 100 years, increase the mass cost of bioregenerative <span class="hlt">life</span> support. In this case, the high reliability half food growing, half food supplying system does not breakeven for 389 years. An even higher reliability half and half system, with three times original system mass and replacing the system every 50 years, never breaks even. Growing food for starship <span class="hlt">life</span> support requires more mass than providing dehydrated food, even for multigeneration voyages of hundreds of years. The benefits of growing some food may justify the added mass cost. Much more efficient recycling food production is wanted but may not be possible. A single multigenerational interstellar voyage to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890001552','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890001552"><span>Risk analysis of earth return options for the Mars rover/sample return <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1988-01-01</p> <p>Four options for return of a Mars surface sample to Earth were studied to estimate the risk of <span class="hlt">mission</span> failure and the risk of a sample container breach that might result in the release of Martian <span class="hlt">life</span> forms, should such exist, in the Earth's biosphere. The probabilities calculated refer only to the time period from the last midcourse correction burn to possession of the sample on Earth. Two extreme views characterize this subject. In one view, there is no <span class="hlt">life</span> on Mars, therefore there is no significant risk and no serious effort is required to deal with back contamination. In the other view, public safety overrides any desire to return Martian samples, and any risk of damaging contamination greater than zero is unacceptable. Zero risk requires great expense to achieve and may prevent the <span class="hlt">mission</span> as currently envisioned from taking place. The major conclusion is that risk of sample container breach can be reduced to a very low number within the framework of the <span class="hlt">mission</span> as now envisioned, but significant expense and effort, above that currently planned is needed. There are benefits to the public that warrant some risk. Martian <span class="hlt">life</span>, if it exists, will be a major discovery. If it does not, there is no risk.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMED54A..07I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMED54A..07I"><span>Lunar Exploration Island, NASA’s Return to the Moon in Second <span class="hlt">Life</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ireton, F. M.; Bleacher, L.; Day, B.; Hsu, B. C.; Mitchell, B. K.</p> <p>2009-12-01</p> <p>Second <span class="hlt">Life</span> is a metaverse—a massively multi-user virtual world (MMVR) community. With over 9 million users worldwide, there are 40,000-50,000 users on line at any one time. Second <span class="hlt">Life</span> hosts over 200 educational and institutional simulation locations termed “islands” or sims that are developed by users providing support for education and business endeavors. On-line tools are provided to construct structures and landforms simulating a real world in a virtual three-dimensional environment. Users develop a persona and are seen on screen as a human figure or avatar. Avatars move in Second <span class="hlt">Life</span> by walking, flying, or teleporting and interact with other users via text or voice chat. This poster details the design and creation of the Second <span class="hlt">Life</span> exhibit hall for NASA’s Lunar Precursor Robotics Program and the LRO/LCROSS <span class="hlt">missions</span>. The hall has been placed on the Lunar Exploration Island (LEI) in Second <span class="hlt">Life</span>. Avatars enter via teleportation to an orientation room with information about the project, a simulator map, and other information. A central hall of flight houses exhibits pertaining to the LRO/ LCROSS <span class="hlt">missions</span> and includes full size models of the two spacecraft and launch vehicle. Storyboards with information about the <span class="hlt">missions</span> interpret the exhibits while links to external websites provide further information on the <span class="hlt">missions</span>, both spacecraft instrument suites, and EPO directed to support the <span class="hlt">missions</span>. The sim includes several sites for meetings, a conference amphitheater with a stage and screen for video links such as live broadcasts of conferences and speakers. A link is provided to NASATV for live viewing LRO/LCROSS launch and impact activities and other NASA events. Recently visitors have viewed the Hubble servicing <span class="hlt">mission</span> and several shuttle launches as well as the LRO/LCROSS launch. Lunar Exploration Island in Second <span class="hlt">Life</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20180000025','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20180000025"><span>Monte Carlo Simulations of the Formation Flying Dynamics for the Magnetospheric Multiscale (MMS) <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schiff, Conrad; Dove, Edwin</p> <p>2011-01-01</p> <p>The MMS <span class="hlt">mission</span> is an ambitious space physics <span class="hlt">mission</span> that will fly 4 spacecraft in a tetrahedron formation in a series of highly elliptical orbits in order to study magnetic reconnection in the Earth's magnetosphere. The <span class="hlt">mission</span> design is comprised of a combination of deterministic orbit adjust and random maintenance maneuvers distributed over the 2.5 year <span class="hlt">mission</span> <span class="hlt">life</span>. Formal verification of the requirements is achieved by analysis through the use of the End-to-End (ETE) code, which is a modular simulation of the maneuver operations over the entire <span class="hlt">mission</span> duration. Error models for navigation accuracy (knowledge) and maneuver execution (control) are incorporated to realistically simulate the possible maneuver scenarios that might be realized These error models, coupled with the complex formation flying physics, lead to non-trivial effects that must be taken into account by the ETE automation. Using the ETE code, the MMS Flight Dynamics team was able to demonstrate that the current <span class="hlt">mission</span> design satisfies the <span class="hlt">mission</span> requirements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-9015178&hterms=vitruvian+man&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dvitruvian%2Bman','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-9015178&hterms=vitruvian+man&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dvitruvian%2Bman"><span>STS-40 <span class="hlt">Mission</span> Insignia</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1990-01-01</p> <p>The STS-40 patch makes a contemporary statement focusing on human beings living and working in space. Against a background of the universe, seven silver stars, interspersed about the orbital path of Columbia, represent the seven crew members. The orbiter's flight path forms a double-helix, designed to represent the DNA molecule common to all living creatures. In the words of a crew spokesman, ...(the helix) affirms the ceaseless expansion of human <span class="hlt">life</span> and American involvement in space while simultaneously emphasizing the medical and biological studies to which this flight is dedicated. Above Columbia, the phrase Spacelab <span class="hlt">Life</span> Sciences 1 defines both the Shuttle <span class="hlt">mission</span> and its payload. Leonardo Da Vinci's Vitruvian man, silhouetted against the blue darkness of the heavens, is in the upper center portion of the patch. With one foot on Earth and arms extended to touch Shuttle's orbit, the crew feels, he serves as a powerful embodiment of the extension of human inquiry from the boundaries of Earth to the limitless laboratory of space. Sturdily poised amid the stars, he serves to link scentists on Earth to the scientists in space asserting the harmony of efforts which produce meaningful scientific spaceflight <span class="hlt">missions</span>. A brilliant red and yellow Earth limb (center) links Earth to space as it radiates from a native American symbol for the sun. At the frontier of space, the traditional symbol for the sun vividly links America's past to America's future, the crew states. Beneath the orbiting Shuttle, darkness of night rests peacefully over the United States. Drawn by artist Sean Collins, the STS 40 Space Shuttle patch was designed by the crewmembers for the flight.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140004919','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140004919"><span>Woven TPS Enabling <span class="hlt">Missions</span> Beyond Heritage Carbon Phenolic</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stackpoole, Margaret M.; Venkatapathy, Ethiraj; Feldman, Jay D.</p> <p>2013-01-01</p> <p>NASAs Office of the Chief Technologist (OCT) Game Changing Division recently funded an effort to advance a Woven TPS (WTPS) concept. WTPS is a new approach to producing TPS architectures that uses precisely engineered 3D weaving techniques to customize material characteristics needed to meet specific <span class="hlt">missions</span> requirements for protecting space vehicles from the intense heating generated during atmospheric entry. Using WTPS, sustainable, scalable, <span class="hlt">mission</span>-optimized TPS solutions can be achieved with relatively low <span class="hlt">life</span> cycle costs compared with the high costs and long development schedules currently associated with material development and certification. WTPS leverages the mature state-of-the-art weaving technology that has evolved from the textile industry to design TPS materials with tailorable performance. Currently, <span class="hlt">missions</span> anticipated encountering heat fluxes in the range of 1500 4000 Wcm2 and pressures greater than 1.5 atm are limited to using fully dense Carbon Phenolic. However, fully dense carbon phenolic is only mass efficient at higher heat fluxes g(reater than 4000 Wcm2), and current <span class="hlt">mission</span> designs suffer this mass inefficiency for lack of an alternative mid-density TPS. WTPS not only bridges this mid-density TPS gap but also offers a replacement for carbon phenolic, which itself requires a significant and costly redevelopment effort to re-establish its capability for use in the high heat flux <span class="hlt">missions</span> recently prioritized in the NRC Decadal survey, including probe <span class="hlt">missions</span> to Venus, Saturn and Neptune. This presentation will overview the WTPS concept and present some results from initial testing completed comparing WTPS architectures to heritage carbon phenolic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060048545','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060048545"><span>The Stellar Imager (SI) "Vision <span class="hlt">Mission</span>"</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carpenter, K.; Danchi, W.; Leitner, J.; Liu, A.; Lyon, R.; Mazzuca, L.; Moe, R.; Chenette, D.; Schrijver, C.; Kilston, S.</p> <p>2004-01-01</p> <p>The Stellar Imager (SI) is a Vision <span class="hlt">Mission</span> in the Sun-Earth Connection (SEC) NASA Roadmap, conceived for the purpose of understanding the effects of stellar magnetic fields, the dynamos that generate them, and the internal structure and dynamics of the stars in which they exist. The ultimate goal is to achieve the best possible forecasting of solar/stellar activity and its impact on <span class="hlt">life</span> in the Universe. The science goals of SI require an ultra-high angular resolution, at ultraviolet wavelengths, on the order of 100 micro-arcsec and baselines on the order of 0.5 km. These requirements call for a large, multi-spacecraft (greater than 20) imaging interferometer, utilizing precision formation flying in a stable environment, such as in a Lissajous orbit around the Sun-Earth L2 point. In this paper, we present an update on the ongoing SI <span class="hlt">mission</span> concept and technology development studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040171818','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040171818"><span>The Stellar Imager (SI) "Vision <span class="hlt">Mission</span>"</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carpenter, K.; Danchi, W.; Leitner, J.; Liu, A.; Lyon, R.; Mazzuca, L.; Moe, R.; Chenette, D.; Schrijver, C.; Kilston, S.</p> <p>2004-01-01</p> <p>The Stellar Imager (SI) is a Vision <span class="hlt">Mission</span> in the Sun-Earth Connection (SEC) NASA Roadmap, conceived for the purpose of understanding the effects of stellar magnetic fields, the dynamos that generate them, and the internal structure and dynamics of the stars in which they exist. The ultimate goal is to achieve the best possible forecasting of solar/stellar activity and its impact on <span class="hlt">life</span> in the Universe. The science goals of SI require an ultra-high angular resolution, a t ultraviolet wavelengths, on the order of 100 micro-arcsec and baselines on the order of 0.5 km. These requirements call for a large, multi-spacecraft (>20) imaging interferometer, utilizing precision formation flying in a stable environment, such as in a Lissajous orbit around the Sun-Earth L2 point. In this paper, we present an update on the ongoing SI <span class="hlt">mission</span> concept and technology development studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010020468&hterms=extraterrestrial&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dextraterrestrial','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010020468&hterms=extraterrestrial&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dextraterrestrial"><span>Cooperative Robotics and the Search for Extraterrestrial <span class="hlt">Life</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lupisella, M. L.</p> <p>2000-01-01</p> <p>If we think tenuous abodes of <span class="hlt">life</span> may be hiding in remote extraterrestrial environmental niches, and if we want to assess the biological status of a given locale or entire planet before sending humans (perhaps because of contamination concerns or other motivations) then we face the challenge of robotically exploring a large space efficiently and in enough detail to have confidence in our assessment of the biological status of the environment in question. On our present schedule of perhaps two or so <span class="hlt">missions</span> per opportunity, we will likely need a different exploratory approach than singular stationary landers or singular rover <span class="hlt">missions</span> or sample return, because there appear to be fundamental limitations in these <span class="hlt">mission</span> profiles to obtain the many samples we will likely need if we want to have confidence in assessing the biological status of an environment in which <span class="hlt">life</span> could be hiding in remote environmental niches. Singular rover <span class="hlt">missions</span> can potentially accommodate sampling over a fairly large area, but are still limited by range and can be a single point of failure. More importantly, such <span class="hlt">mission</span> profiles have limited payload capabilities which are unlikely to meet the demanding requirements of <span class="hlt">life</span>-detection. Sample return has the advantage of allowing sophisticated analysis of the sample, but also has the severe limitations associated with only being able to bring back a few samples. This presentation will suggest two cooperative robotic approaches for exploration that have the potential to overcome these difficulties and facilitate efficient and thorough <span class="hlt">life</span>-detecting exploration of a large space. Given the two premises stated above, it appears at least two fundamental challenges have to be met simultaneously: (1) coverage of a large space and (2) bringing to bear a sophisticated suite of detection and experimental payloads on any specific location in order to address a major challenge in looking for extraterrestrial <span class="hlt">life</span>: namely, executing a wide variety</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20000085882','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20000085882"><span>Cooperative Robotics and the Search for Extraterrestrial <span class="hlt">Life</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lupisella, Mark L.</p> <p>2000-01-01</p> <p>If we think tenuous abodes of <span class="hlt">life</span> may be hiding in remote extraterrestrial environmental niches, and if we want to assess the biological status of a given locale or entire planet before sending humans (perhaps because of contamination concerns or other motivations) then we face the challenge of robotically exploring a large space efficiently and in enough detail to have confidence in our assessment of the biological status of the environment in question. On our present schedule of perhaps two or so <span class="hlt">missions</span> per opportunity, we will likely need a different exploratory approach than singular stationary landers or singular rover <span class="hlt">missions</span> or sample return, because there appear to be fundamental limitations in these <span class="hlt">mission</span> profiles to-obtain the many samples we will likely need if we want to have confidence in assessing the biological status of an environment in which <span class="hlt">life</span> could be hiding in remote environmental niches. Singular rover <span class="hlt">missions</span> can potentially accommodate sampling over a fairly large area, but are still limited by range and can be a single point of failure. More importantly, such <span class="hlt">mission</span> profiles have limited payload capabilities which are unlikely to meet the demanding requirements of <span class="hlt">life</span>-detection. Sample return has the advantage of allowing sophisticated analysis of the sample, but also has the severe limitations associated with only being able to bring back a few samples. This presentation will suggest two cooperative robotic approaches for exploration that have the potential to overcome these difficulties and facilitate efficient and thorough <span class="hlt">life</span>-detecting exploration of a large space. Given the two premises state above, it appears at least two fundamental challenges have to be met simultaneously: coverage of a large space and bringing to bear a sophisticated suite of detection and experimental payloads on any specific location in order to address a major challenge in looking for extraterrestrial <span class="hlt">life</span>: namely, executing a wide variety of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20010060339&hterms=chemical+engineering&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dchemical%2Bengineering','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20010060339&hterms=chemical+engineering&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dchemical%2Bengineering"><span>Cometary Coma Chemical Composition (C4) <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carle, Glenn C.; Clark, Benton C.; Knocke, Philip C.; OHara, Bonnie J.; Adams, Larry; Niemann, Hasso B.; Alexander, Merle; Veverka, Joseph; Goldstein, Raymond; Huebner, Walter; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20010060339'); toggleEditAbsImage('author_20010060339_show'); toggleEditAbsImage('author_20010060339_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20010060339_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20010060339_hide"></p> <p>1994-01-01</p> <p>Cometary exploration remains of great importance to virtually all of space science. Because comets are presumed to be remnants of the early solar nebula, they are expected to provide fundamental knowledge as to the origin and development of the solar system as well as to be key to understanding of the source of volatiles and even <span class="hlt">life</span> itself in the inner solar system. Clearly the time for a detailed study of the composition of these apparent messages from the past has come. A comet rendezvous <span class="hlt">mission</span>, the Cometary Coma Chemical Composition (C4) <span class="hlt">Mission</span>, is now being studied as a candidate for the new Discovery program. This <span class="hlt">mission</span> is a highly-focussed and usefully-limited subset of the Cometary Rendezvous Asteroid Flyby (CRAF) <span class="hlt">Mission</span>. The C4 <span class="hlt">mission</span> will concentrate on measurements that will produce an understanding of the composition and physical makeup of a cometary nucleus. The core science goals of the C4 <span class="hlt">mission</span> are 1) to determine the chemical, elemental, and isotopic composition of a cometary nucleus and 2) to characterize the chemical and isotopic nature of its atmosphere. A related goal is to obtain temporal information about the development of the cometary coma as a function of time and orbital position. The four short-period comets -- Tempel 1, Tempel 2, Churyumov-Gerasimenko, and Wirtanen -which all appear to have acceptable dust production rates, were identified as candidate targets. <span class="hlt">Mission</span> opportunities have been identified beginning as early as 1998. Tempel I with a launch in 1999, however, remains the baseline comet for studies of and planning the C4 <span class="hlt">mission</span>. The C4 <span class="hlt">mission</span> incorporates two science instruments and two engineering instruments in the payload to obtain the desired measurements. The science instruments include an advanced version of the Cometary Ice and Dust Experiment (CIDEX), a mini-CIDEX with a sample collection system, an X-ray Fluorescence Spectrometer and a Pyrolysis-Gas Chromatograph, and a simplified version of the Neutral</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008epsc.conf..855W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008epsc.conf..855W"><span>Selecting a landing site of astrobiological interest for Mars landers and sample return <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wills, D.; Monaghan, E.; Foing, B. H.</p> <p>2008-09-01</p> <p>Abstract The landscape of Mars, despite its apparent hostility to <span class="hlt">life</span>, is riddled with geological and mineralogical signs of past or present hydrological activity. As such, it is a key target for astrobiological exploration. There are, however, many factors that will need to be considered when planning in-situ and sample return <span class="hlt">missions</span>, if these <span class="hlt">missions</span> are indeed to adequately exploit the science potential of this intriguing world. These will not only take into account the environment of the landing site in terms of topography and ambient atmosphere etc., but also the geochemical make up of the surface regolith, evidence of hydrological processes and various other considerations. The knowledge base in all aspects of Martian science is being added to on an almost daily basis, and the aim of this work is to combine data and studies to nominate top priority landing locations for the search for evidence of <span class="hlt">life</span> on Mars. We report in particular on science and technical criteria and our data analysis for sites of astrobiological interest. This includes information from previous <span class="hlt">missions</span> (such as Mars Express, MGS, Odyssey, MRO and MER rovers) on mineralogical composition, geomorphology, evidence from past water history from imaging and spectroscopic data, and existence of in-situ prior information from landers and rovers (concerning evidences for volatiles, organics and habitability conditions). We discuss key <span class="hlt">mission</span> objectives, and assess what sort of sites should be targeted in the light of these. We consider the accessibility of chosen locations, taking into account difficulties presented in accessing the polar regions and other regions of high altitude. We describe what additional measurements are needed, and outline the technical and scientific operations requirements of such in-situ landers and sample return <span class="hlt">missions</span>. Approach In the first step of this study we focus on the science objectives of in-situ and sample return <span class="hlt">missions</span> to Mars. We investigate the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-9300933&hterms=animal+rights&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Danimal%2Brights','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-9300933&hterms=animal+rights&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Danimal%2Brights"><span>Spacelab Module for USML-1 <span class="hlt">Mission</span> in Orbiter Cargo Bay</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1992-01-01</p> <p>This is a photograph of the Spacelab module for the first United States Microgravity Laboratory (USML-1) <span class="hlt">mission</span>, showing logos of the Spacelab <span class="hlt">mission</span> on the left and the USML-1 <span class="hlt">mission</span> on the right. The USML-1 was one part of a science and technology program that opened NASA's next great era of discovery and established the United States' leadership in space. From investigations designed to gather fundamental knowledge in a variety of areas to demonstrations of new equipment, USML-1 forged the way for future USML <span class="hlt">missions</span> and helped prepare for advanced microgravity research and processing aboard the Space Station. Thirty-one investigations comprised the payload of the first USML-1 <span class="hlt">mission</span>. The experiments aboard USML-1 covered five basic areas: fluid dynamics, the study of how liquids and gases respond to the application or absence of differing forces; crystal growth, the production of inorganic and organic crystals; combustion science, the study of the processes and phenomena of burning; biological science, the study of plant and animal <span class="hlt">life</span>; and technology demonstrations. The USML-1 was managed by the Marshall Space Flight Center and launched aboard the Space Shuttle Orbiter Columbia (STS-50) on June 25, 1992.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790033644&hterms=animals+tests&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Danimals%2Btests','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790033644&hterms=animals+tests&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Danimals%2Btests"><span>Spacelab <span class="hlt">mission</span> development tests</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dalton, B. P.</p> <p>1978-01-01</p> <p>The paper describes Spacelab <span class="hlt">Mission</span> Development Test III (SMD III) whose principal scientific objective was to demonstrate the feasibility of conducting biological research in the <span class="hlt">Life</span> Sciences Spacelab. The test also provided an opportunity to try out several items of Common Operational Research Equipment (CORE) hardware being developed for operational use in Shuttle/Spacelab, such as rodent and primate handling, transportation units, and a 'zero-g' surgical bench. Operational concepts planned for Spacelab were subjected to evaluation, including animal handling procedures, animal logistics, crew selection and training, and a 'remote' ground station concept. It is noted that all the objectives originally proposed for SMD III were accomplished</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011epsc.conf.1705R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011epsc.conf.1705R"><span>3 EXPOSE <span class="hlt">Missions</span> - overview and lessons learned</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabbow, E.; Willnekcer, R.; Reitz, G.; Aman, A.; Bman, B.; Cman, C.</p> <p>2011-10-01</p> <p>The International Space Station ISS provides a variety of external research platforms for experiments aiming at the utilization of space parameters like vacuum, temperature oscillation and in particular extraterrestrial short wavelength UV and ionizing radiation which cannot be simulated accurately in the laboratory. Three <span class="hlt">Missions</span>, two past and one upcoming, will be presented. A family of astrobiological experimental ESA facilities called "EXPOSE" were and will be accommodated on these outside exposure platforms: on one of the external balconies of the European Columbus Module (EXPOSE-E) and on the URM-D platform on the Russian Zvezda Module (EXPOSE-R and EXPOSE-R2). Exobiological and radiation experiments, exposing chemical, biological and dosimetric samples to the harsh space environment are - and will be - accommodated on these facilities to increase our knowledge on the origin, evolution and distribution of <span class="hlt">life</span>, on Earth and possibly beyond. The biological experiments investigate resistance and adaptation of organisms like bacteria, Achaea, fungi, lichens, plant seeds and small animals like mosquito larvae to extreme environmental conditions and underlying mechanisms like DNA repair. The organic chemical experiments analyse chemical reactions triggered by the extraterrestrial environment, especially short wavelength UV radiation, to better understand prebiotic chemistry. The facility is optimized to allow exposure of biological specimen and material samples under a variety of conditions, using optical filter systems. Environmental parameters like temperature and radiation are regularly recorded and down linked by telemetry. Two long term <span class="hlt">missions</span> named according to their facility - EXPOSE-E and EXPOSE-R - are completed and a third <span class="hlt">mission</span> is planned and currently prepared. Operations of all three <span class="hlt">missions</span> including sample accommodation are performed by DLR. An overview of the two completed <span class="hlt">missions</span> will be given including lessons learned as well as an outlook</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020079822&hterms=Science+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DScience%2Blife','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020079822&hterms=Science+life&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DScience%2Blife"><span>Why, from a <span class="hlt">Life</span> Sciences Perspective, This <span class="hlt">Mission</span> to Mars?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McKay, Christopher P.; DeVincenzi, Donald (Technical Monitor)</p> <p>2002-01-01</p> <p>Mars may have had water and <span class="hlt">life</span> early in its history and this make it a key target for robotic and human exploration. Extensive human exploration of Mars will of necessity depend on <span class="hlt">life</span> support systems that rely on agricultural plants. If current concept for recreating, a biosphere on Mars are implemented this would involve widespread use of plants, particularly species from Arctic and alpine environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160008122','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160008122"><span>Extended <span class="hlt">Life</span> Testing of Duplex Ball Bearings</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mobley, Jeffrey; Robertson, Michael; Hodges, Charles</p> <p>2016-01-01</p> <p>Sierra Nevada Corporation’s Space Systems performed bearing <span class="hlt">life</span> testing for the Scan Mirror Motor/Encoder Assembly (SMMA), part of the Scan Mirror Assembly on-board the Aerosol Polarimetry Sensor (APS) on the NASA Glory Spacecraft. The baseline bearing <span class="hlt">life</span> test duration extended beyond the launch date for the Glory Spacecraft; a risk that the program was willing to undertake with the understanding that if any anomalies or failures occurred before the required <span class="hlt">life</span> was achieved, then the <span class="hlt">mission</span> objectives or operating profile could be modified on orbit to take those results into account. Even though the Glory Spacecraft failed to reach orbit during its launch in March of 2011, the bearing <span class="hlt">life</span> testing was continued through a mutual understanding of value between Sierra Nevada Corporation and our customer; with a revised goal of testing to failure rather than completing a required number of <span class="hlt">life</span> cycles. <span class="hlt">Life</span> testing thus far has not only exceeded the original <span class="hlt">mission</span> required <span class="hlt">life</span>, but has also exceeded the published test data for Cumulative Degradation Factor (CDF) from NASA/CR-2009-215681. Many lessons were learned along the way regarding long <span class="hlt">life</span> testing. The bearing <span class="hlt">life</span> test has been temporarily suspended due to test support equipment issues.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22535247-conceptual-solutions-concerning-decommissioning-dismantling-russian-civil-nuclear-powered-ships','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22535247-conceptual-solutions-concerning-decommissioning-dismantling-russian-civil-nuclear-powered-ships"><span>The conceptual solutions concerning decommissioning and dismantling of Russian civil nuclear powered ships</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kulikov, Konstantin N.; Nizamutdinov, Rinat A.; Abramov, Andrey N.</p> <p></p> <p>From 1959 up to 1991 nine civil nuclear powered ships were built in Russia: eight <span class="hlt">ice-breakers</span> and one lash lighter carrier (cargo ship). At the present time three of them were taking out of service: <span class="hlt">ice-breaker</span> 'Lenin' is decommissioned as a museum and is set for storage in the port of Murmansk, nuclear <span class="hlt">ice-breakers</span> 'Arktika' and 'Sibir' are berthing. The <span class="hlt">ice-breakers</span> carrying rad-wastes appear to be a possible source of radiation contamination of Murmansk region and Kola Bay because the ship long-term storage afloat has the negative effect on hull's structures. As the result of this under the auspices ofmore » the Federal Targeted Program 'Nuclear and Radiation Safety of Russia for 2008 and the period until 2015' the conception and projects of decommissioning of nuclear-powered ships are developed by the State corporation Rosatom with the involvement of companies of United Shipbuilding Corporation. In developing the principal provisions of conception of decommissioning and dismantling of <span class="hlt">icebreakers</span> the technical and economic assessment of dismantling options in ship-repairing enterprises of North-West of Russia was performed. The paper contains description of options, research procedure, analysis of options of decommissioning and dismantling of nuclear <span class="hlt">ice-breakers</span>, taking into account the principle of optimization of potential radioactive effect to personnel, human population and environment. The report's conclusions contain the recommendations for selection of option for development of nuclear <span class="hlt">icebreaker</span> decommissioning and dismantling projects. (authors)« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170007996','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170007996"><span>OSIRIS-REx Asterod Sample Return <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nakamura-Messinger, Keiki; Connolly, Harold C. Jr.; Messenger, Scott; Lauretta, Dante S.</p> <p>2017-01-01</p> <p>OSIRIS-REx is NASA's third New Frontiers Program <span class="hlt">mission</span>, following New Horizons that completed a flyby of Pluto in 2015 and the Juno <span class="hlt">mission</span> to Jupiter that has just begun science operations. The OSIRIS-REx <span class="hlt">mission</span>'s primary objective is to collect pristine surface samples of a carbonaceous asteroid and return to Earth for analysis. Carbonaceous asteroids and comets are 'primitive' bodies that preserved remnants of the Solar System starting materials and through their study scientists can learn about the origin and the earliest evolution of the Solar System. The OSIRIS-REx spacecraft was successfully launched on September 8, 2016, beginning its seven year journey to asteroid 101955 Bennu. The robotic arm will collect 60-2000 grams of material from the surface of Bennu and will return to Earth in 2023 for worldwide distribution by the Astromaterials Curation Facility at NASA Johnson Space Center. The name OSIRIS-REx embodies the <span class="hlt">mission</span> objectives (1) Origins: Return and analyze a sample of a carbonaceous asteroid, (2) Spectral Interpretation: Provide ground-truth for remote observation of asteroids, (3) Resource Identification: Determine the mineral and chemical makeup of a near-Earth asteroid (4) Security: Measure the non-gravitational that changes asteroidal orbits and (5) Regolith Explorer: Determine the properties of the material covering an asteroid surface. Asteroid Bennu may preserve remnants of stardust, interstellar materials and the first solids to form in the Solar System and the molecular precursors to the origin of <span class="hlt">life</span> and the Earth's oceans. Bennu is a potentially hazardous asteroid, with an approximately 1 in 2700 chance of impacting the Earth late in the 22nd century. OSIRIS-REx collects from Bennu will help formulate the types of operations and identify <span class="hlt">mission</span> activities that astronauts will perform during their expeditions. Such information is crucial in preparing for humanity's next steps beyond low Earthy orbit and on to deep space</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008ESASP.663E..33M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008ESASP.663E..33M"><span>Testing Crew Responses to Varied Higher Plant Presentations in the MARS-500 Day <span class="hlt">Mission</span> Simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marquit, J. D.; Bates, S. C.; Gushin, V. I.; Synchev, V. N.; Levinskikh, M. A.; Podolsky, I. G.; Marchant, C. C.; Bingham, G. E.</p> <p>2008-06-01</p> <p>Maintaining psychological and behavioral health of humans during long-duration space <span class="hlt">missions</span> is of great importance for the future success of space exploration as the hostile space environment adversely impacts the psychological, social, and physiological well-being of humans in space. Growing and tending plants has been proposed as a countermeasures for the negative impacts of long-duration space <span class="hlt">missions</span>[3] as interactions with plant <span class="hlt">life</span> on earth have been found to be beneficial to humans in other settings. Preliminary results from a pilot 14-day chamber study appear to support the notion that interactions with plant <span class="hlt">life</span> may act as a countermeasure for the negative impacts of <span class="hlt">life</span> in space. Additional data will be collected during the Mars 500-day Chamber Study at Institute of Biomedical Problems (IMBP).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20010038488','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20010038488"><span><span class="hlt">Life</span> Sciences Accomplishments 1994</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Burnell, Mary Lou (Editor)</p> <p>1993-01-01</p> <p>The NASA <span class="hlt">Life</span> and Biomedical Sciences and Applications Division (LBSAD) serves the Nation's <span class="hlt">life</span> sciences community by managing all aspects of U.S. space-related <span class="hlt">life</span> sciences research and technology development. The activities of the Division are integral components of the Nation's overall biological sciences and biomedical research efforts. However, NASA's <span class="hlt">life</span> sciences activities are unique, in that space flight affords the opportunity to study and characterize basic biological mechanisms in ways not possible on Earth. By utilizing access to space as a research tool, NASA advances fundamental knowledge of the way in which weightlessness, radiation, and other aspects of the space-flight environment interact with biological processes. This knowledge is applied to procedures and technologies that enable humans to live and work in and explore space and contributes to the health and well-being of people on Earth. The activities of the Division are guided by the following three goals: Goal 1) Use microgravity and other unique aspects of the space environment to enhance our understanding of fundamental biological processes. Goal 2) Develop the scientific and technological foundations for supporting exploration by enabling productive human presence in space for extended periods. Goal 3) Apply our unique <span class="hlt">mission</span> personnel, facilities, and technology to improve education, the quality of <span class="hlt">life</span> on Earth, and U.S. competitiveness. The Division pursues these goals with integrated ground and flight programs involving the participation of NASA field centers, industry, and universities, as well as interactions with other national agencies and NASA's international partners. The published work of Division-sponsored researchers is a record of completed research in pursuit of these goals. During 1993, the LBSAD instituted significant changes in its experiment solicitation and peer review processes. For the first time, a NASA Research Announcement (NRA) was released requesting</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770052459&hterms=craft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dcraft','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770052459&hterms=craft&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dcraft"><span>Early Spacelab <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pace, R. E., Jr.; Craft, H. G., Jr.</p> <p>1977-01-01</p> <p>NASA has issued payload flight assignments for the first three Spacelab <span class="hlt">missions</span>. The first two of these <span class="hlt">missions</span> will have dual objectives, that of verifying Spacelab system performance and accomplishing meaningful space research. The first of these <span class="hlt">missions</span> will be a joint NASA and ESA <span class="hlt">mission</span> with a multidisciplinary payload. The second <span class="hlt">mission</span> will verify a different Spacelab configuration while addressing the scientific disciplines of astrophysics. The third assigned <span class="hlt">mission</span> will concentrate on utilizing the capabilities of Spacelab to perform meaningful experiments in space applications, primarily space processing. The paper describes these <span class="hlt">missions</span> with their objectives, planned configuration and accommodation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982SPIE..284..158F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982SPIE..284..158F"><span><span class="hlt">Life</span> Science Research In Space: The Spacelab Era</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Farrell, R. M.; Cramer, D. B.; Reid, D. H.</p> <p>1982-02-01</p> <p>This manuscript summarizes the events leading to the first Spacelab <span class="hlt">mission</span> dedicated exclusively to <span class="hlt">life</span> sciences experimentation. This <span class="hlt">mission</span> is currently planned for a Space Shuttle flight in the 1984-1985 time frame. Following publication of a NASA Announce ment of Opportunity in 1978, approximately 400 proposals were received from researchers in universities, government laboratories, and industrial firms both in the U. S. and abroad. In 1979, 87 candidate experiments were selected for definition studies to identify the detailed resources which would need to be accommodated by the Spacelab. These proposals addressed problems encountered in man's previous space flight experience, such as space motion sickness, cardiovascular deconditioning, muscle wasting, calcium loss and a reduction in red cell mass. Additionally, experiments were selected in areas of bioengineering, behavior and performance, Plant physiology, and cell biology. Animal species (rodents and small primates) to be investigated will be housed in a specially-developed animal holding facility which will provide all <span class="hlt">life</span> support requirements for the animals. Human subjects will consist of a <span class="hlt">Mission</span> Specialist Astronaut and up to four Payload Specialists. Plant species will be housed in Plant Growth Units. A general purpose work station and biological containment facility will provide the working area for much of the in-space experimentation. A comprehensive array of flight qualified laboratory equipment will be made available by NASA to Principal Investigators for in-flight use by the Payload Specialists. This equipment includes microscopes, biotelemetry systems, cameras, centrifuges, refrigerators, and similar equipment. All of this equipment has been designed for use in weightlessness. The process to develop a primary payload of about 20 experiments is now underway for Spacelab <span class="hlt">mission</span> number four, the first dedicated <span class="hlt">life</span> sciences flight. Under the overall guidance of NASA Headquarters</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19780003214','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19780003214"><span><span class="hlt">Life</span> science payloads planning study. [for space shuttle orbiters and spacelab</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nelson, W. G.; Wells, G. W.</p> <p>1977-01-01</p> <p>Preferred approaches and procedures were defined for integrating the space shuttle <span class="hlt">life</span> sciences payload from experiment solicitation through final data dissemination at <span class="hlt">mission</span> completion. The payloads operations plan was refined and expended to include current information. The NASA-JSC facility accommodations were assessed, and modifications recommended to improve payload processing capability. Standard format worksheets were developed to permit rapid location of experiment requirements and a Spacelab <span class="hlt">mission</span> handbook was developed to assist potential <span class="hlt">life</span> sciences investigators at academic, industrial, health research, and NASA centers. Practical, cost effective methods were determined for accommodating various categories of live specimens during all <span class="hlt">mission</span> phases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000037.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-GSFC_20171208_Archive_e000037.html"><span>NICER <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2017-12-08</p> <p>This video previews the Neutron star Interior Composition Explorer (NICER). NICER is an Astrophysics <span class="hlt">Mission</span> of Opportunity within NASA’s Explorer program, which provides frequent flight opportunities for world-class scientific investigations from space utilizing innovative, streamlined and efficient management approaches within the heliophysics and astrophysics science areas. NASA’s Space Technology <span class="hlt">Mission</span> Directorate supports the SEXTANT component of the <span class="hlt">mission</span>, demonstrating pulsar-based spacecraft navigation. NICER is an upcoming International Space Station payload scheduled to launch in June 2017. Learn more about the <span class="hlt">mission</span> at nasa.gov/nicer NASA image use policy. NASA Goddard Space Flight Center enables NASA’s <span class="hlt">mission</span> through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s <span class="hlt">mission</span>. Follow us on Twitter Like us on Facebook Find us on Instagram</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840002104','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840002104"><span>Payload <span class="hlt">missions</span> integration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mitchell, R. A. K.</p> <p>1983-01-01</p> <p>Highlights of the Payload <span class="hlt">Missions</span> Integration Contract (PMIC) are summarized. Spacelab <span class="hlt">Missions</span> no. 1 to 3, OSTA partial payloads, Astro-1 <span class="hlt">Mission</span>, premission definition, and <span class="hlt">mission</span> peculiar equipment support structure are addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950010810','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950010810"><span><span class="hlt">Mission</span> operations management</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rocco, David A.</p> <p>1994-01-01</p> <p>Redefining the approach and philosophy that operations management uses to define, develop, and implement space <span class="hlt">missions</span> will be a central element in achieving high efficiency <span class="hlt">mission</span> operations for the future. The goal of a cost effective space operations program cannot be realized if the attitudes and methodologies we currently employ to plan, develop, and manage space <span class="hlt">missions</span> do not change. A management philosophy that is in synch with the environment in terms of budget, technology, and science objectives must be developed. Changing our basic perception of <span class="hlt">mission</span> operations will require a shift in the way we view the <span class="hlt">mission</span>. This requires a transition from current practices of viewing the <span class="hlt">mission</span> as a unique end product, to a '<span class="hlt">mission</span> development concept' built on the visualization of the end-to-end <span class="hlt">mission</span>. To achieve this change we must define realistic <span class="hlt">mission</span> success criteria and develop pragmatic approaches to achieve our goals. Custom <span class="hlt">mission</span> development for all but the largest and most unique programs is not practical in the current budget environment, and we simply do not have the resources to implement all of our planned science programs. We need to shift our management focus to allow us the opportunity make use of methodologies and approaches which are based on common building blocks that can be utilized in the space, ground, and <span class="hlt">mission</span> unique segments of all <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015IJNAO...7..708C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015IJNAO...7..708C"><span>A prediction method of ice breaking resistance using a multiple regression analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cho, Seong-Rak; Lee, Sungsu</p> <p>2015-07-01</p> <p>The two most important tasks of <span class="hlt">icebreakers</span> are first to secure a sailing route by breaking the thick sea ice and second to sail efficiently herself for purposes of exploration and transportation in the polar seas. The resistance of <span class="hlt">icebreakers</span> is a priority factor at the preliminary design stage; not only must their sailing efficiency be satisfied, but the design of the propulsion system will be directly affected. Therefore, the performance of <span class="hlt">icebreakers</span> must be accurately calculated and evaluated through the use of model tests in an ice tank before construction starts. In this paper, a new procedure is developed, based on model tests, to estimate a ship's ice breaking resistance during continuous <span class="hlt">ice-breaking</span> in ice. Some of the factors associated with crushing failures are systematically considered in order to correctly estimate her <span class="hlt">ice-breaking</span> resistance. This study is intended to contribute to the improvement of the techniques for ice resistance prediction with ice breaking ships.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DPS....4910108M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DPS....4910108M"><span>An Analog Rover Exploration <span class="hlt">Mission</span> for Education and Outreach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moores, John; Campbell, Charissa L.; Smith, Christina L.; Cooper, Brittney A.</p> <p>2017-10-01</p> <p>This abstract describes an analog rover exploration <span class="hlt">mission</span> designed as an outreach program for high school and undergraduate students. This program is used to teach them about basic <span class="hlt">mission</span> control operations, how to manage a rover as if it were on another planetary body, and employing the rover remotely to complete <span class="hlt">mission</span> objectives. One iteration of this program has been completed and another is underway. In both trials, participants were shown the different operation processes involved in a real-<span class="hlt">life</span> <span class="hlt">mission</span>. Modifications were made to these processes to decrease complexity and better simulate a <span class="hlt">mission</span> control environment in a short time period (three 20-minute-long <span class="hlt">mission</span> “days”). In the first run of the program, participants selected a landing site, what instruments would be on the rover - subject to cost, size, and weight limitations - and were randomly assigned one of six different <span class="hlt">mission</span> operations roles, each with specific responsibilities. For example, a Science Planner/Integrator (SPI) would plan science activities whilst a Rover Engineer (RE) would keep on top of rover constraints. Planning consisted of a series of four meetings to develop and verify the current plan, pre-plan the next day's activities and uplink the activities to the “rover” (a human colleague). Participants were required to attend certain meetings depending upon their assigned role. To conclude the <span class="hlt">mission</span>, students viewed the site to understand any differences between remote viewing and reality in relation to the rover. Another <span class="hlt">mission</span> is currently in progress with revisions from the earlier run to improve the experience. This includes broader roles and meetings and pre-selecting the landing site and rover. The new roles are: <span class="hlt">Mission</span> Lead, Rover Engineer and Science Planner. The SPI role was previously popular so most of the students were placed in this category. The meetings were reduced to three but extended in length. We are also planning to integrate this program</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940019405','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940019405"><span>Generic <span class="hlt">mission</span> planning concepts for space astronomy <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Guffin, O. T.; Onken, J. F.</p> <p>1993-01-01</p> <p>The past two decades have seen the rapid development of space astronomy, both manned and unmanned, and the concurrent proliferation of the operational concepts and software that have been produced to support each individual project. Having been involved in four of these <span class="hlt">missions</span> since the '70's and three yet to fly in the present decade, the authors believe it is time to step back and evaluate this body of experience from a macro-systems point of view to determine the potential for generic <span class="hlt">mission</span> planning concepts that could be applied to future <span class="hlt">missions</span>. This paper presents an organized evaluation of astronomy <span class="hlt">mission</span> planning functions, functional flows, iteration cycles, replanning activities, and the requirements that drive individual concepts to specific solutions. The conclusions drawn from this exercise are then used to propose a generic concept that could support multiple <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150021783','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150021783"><span>Scaling Impacts in <span class="hlt">Life</span> Support Architecture and Technology Selection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lange, Kevin</p> <p>2016-01-01</p> <p>For long-duration space <span class="hlt">missions</span> outside of Earth orbit, reliability considerations will drive higher levels of redundancy and/or on-board spares for <span class="hlt">life</span> support equipment. Component scaling will be a critical element in minimizing overall launch mass while maintaining an acceptable level of system reliability. Building on an earlier reliability study (AIAA 2012-3491), this paper considers the impact of alternative scaling approaches, including the design of technology assemblies and their individual components to maximum, nominal, survival, or other fractional requirements. The optimal level of <span class="hlt">life</span> support system closure is evaluated for deep-space <span class="hlt">missions</span> of varying duration using equivalent system mass (ESM) as the comparative basis. Reliability impacts are included in ESM by estimating the number of component spares required to meet a target system reliability. Common cause failures are included in the analysis. ISS and ISS-derived <span class="hlt">life</span> support technologies are considered along with selected alternatives. This study focusses on minimizing launch mass, which may be enabling for deep-space <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790037247&hterms=social+support&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsocial%2Bsupport','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790037247&hterms=social+support&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsocial%2Bsupport"><span>Developing closed <span class="hlt">life</span> support systems for large space habitats</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Phillips, J. M.; Harlan, A. D.; Krumhar, K. C.</p> <p>1978-01-01</p> <p>In anticipation of possible large-scale, long-duration space <span class="hlt">missions</span> which may be conducted in the future, NASA has begun to investigate the research and technology development requirements to create <span class="hlt">life</span> support systems for large space habitats. An analysis suggests the feasibility of a regeneration of food in <span class="hlt">missions</span> which exceed four years duration. Regeneration of food in space may be justified for <span class="hlt">missions</span> of shorter duration when large crews must be supported at remote sites such as lunar bases and space manufacturing facilities. It is thought that biological components consisting principally of traditional crop and livestock species will prove to be the most acceptable means of closing the food cycle. A description is presented of the preliminary results of a study of potential biological components for large space habitats. Attention is given to controlled ecosystems, Russian <span class="hlt">life</span> support system research, controlled-environment agriculture, and the social aspects of the <span class="hlt">life</span>-support system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120003213','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120003213"><span>The Importance of Meteorite Collections to Sample Return <span class="hlt">Missions</span>: Past, Present, and Future Considerations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Welzenbach, L. C.; McCoy, T. J.; Glavin, D. P.; Dworkin, J. P.; Abell, P. A.</p> <p>2012-01-01</p> <p>While much of the scientific community s current attention is drawn to sample return <span class="hlt">missions</span>, it is the existing meteorite and cosmic dust collections that both provide the paradigms to be tested by these <span class="hlt">missions</span> and the context for interpreting the results. Recent sample returns from the Stardust and Hayabusa <span class="hlt">missions</span> provided us with new materials and insights about our Solar System history and processes. As an example, Stardust sampled CAIs among the population of cometary grains, requiring extensive and unexpected radial mixing in the early solar nebula. This finding would not have been possible, however, without extensive studies of meteoritic CAIs that established their high-temperature, inner Solar System formation. Samples returned by Stardust also revealed the first evidence of a cometary amino acid, a discovery that would not have been possible with current in situ flight instrument technology. The Hayabusa <span class="hlt">mission</span> provided the final evidence linking ordinary chondrites and S asteroids, a hypothesis that developed from centuries of collection and laboratory and ground-based telescopic studies. In addition to these scientific findings, studies of existing meteorite collections have defined and refined the analytical techniques essential to studying returned samples. As an example, the fortuitous fall of the Allende CV3 and Murchison CM2 chondrites within months before the return of Apollo samples allowed testing of new state-of-the-art analytical facilities. The results of those studies not only prepared us to better study lunar materials, but unanticipated discoveries changed many of our concepts about the earliest history and processes of the solar nebula. This synergy between existing collections and future space exploration is certainly not limited to sample return <span class="hlt">missions</span>. Laboratory studies confirmed the existence of meteorites from Mars and raised the provocative possibility of preservation of ancient microbial <span class="hlt">life</span>. The laboratory studies in</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720020437','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720020437"><span><span class="hlt">Life</span> sciences payload definition and integration study. Volume 1: Management summary</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1972-01-01</p> <p>The objectives of a study program to determine the <span class="hlt">life</span> sciences payloads required for conducting biomedical experiments during space <span class="hlt">missions</span> are presented. The objectives are defined as: (1) to identify the research functions which must be performed aboard <span class="hlt">life</span> sciences spacecraft laboratories and the equipment needed to support these functions and (2) to develop layouts and preliminary conceptual designs of several potential baseline payloads for the accomplishment of <span class="hlt">life</span> research in space. Payload configurations and subsystems are described and illustrated. Tables of data are included to identify the material requirements for the space <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19830007070&hterms=animal+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Danimal%2Bscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19830007070&hterms=animal+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Danimal%2Bscience"><span>Ames Research Center <span class="hlt">life</span> sciences payload</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Callahan, P. X.; Tremor, J. W.</p> <p>1982-01-01</p> <p>In response to a recognized need for an in-flight animal housing facility to support Spacelab <span class="hlt">life</span> sciences investigators, a rack and system compatible Research Animal Holding Facility (RAHF) has been developed. A series of ground tests is planned to insure its satisfactory performance under certain simulated conditions of flight exposure and use. However, even under the best conditions of simulation, confidence gained in ground testing will not approach that resulting from actual spaceflight operation. The Spacelab <span class="hlt">Mission</span> 3 provides an opportunity to perform an inflight Verification Test (VT) of the RAHF. Lessons learned from the RAHF-VT and baseline performance data will be invaluable in preparation for subsequent dedicated <span class="hlt">life</span> sciences <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011688','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011688"><span>Implementation Options for the PROPEL Electrodynamic Tether Demonstration <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bilen, Sven G.; Johnson, C. Les; Gilchrist, Brian E.; Hoyt, Robert P.; Elder, Craig H.; Fuhrhop, Keith P.; Scadera, Michael; Stone, Nobie</p> <p>2014-01-01</p> <p>. The ETPS builds on prior work on long-<span class="hlt">life</span>, failure-resistant, conducting tethers and includes an instrument suite with demonstrated heritage capable of performing necessary diagnostics to measure performance against predictions for a given system size (to be determined) and boost rate. <span class="hlt">Mission</span> designs in other configurations and launch vehicle options are being developed such that the system can be demonstration should a flight opportunity be identified. We will report on past and ongoing implementation options for PROPEL.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19830003310','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19830003310"><span>OAO-3 end of <span class="hlt">mission</span> power subsystem evaluation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tasevoli, M.</p> <p>1982-01-01</p> <p>End of <span class="hlt">mission</span> tests were performed on the OAO-3 power subsystem in three component areas: solar array, nickel-cadmium batteries and the On-Board Processor (OBP) power boost operation. Solar array evaluation consisted of analyzing array performance characteristics and comparing them to earlier flight data. Measured solar array degradation of 14.1 to 17.7% after 8 1/3 years is in good agreement with theortical radiation damage losses. Battery discharge characteristics were compared to results of laboratory <span class="hlt">life</span> cycle tests performed on similar cells. Comparison of cell voltage profils reveals close correlation and confirms the validity of real time <span class="hlt">life</span> cycle simulation. The successful operation of the system in the OBP/power boost regulation mode demonstrates the excellent <span class="hlt">life</span>, reliability and greater system utilization of power subsystems using maximum power trackers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19860044074&hterms=interpersonal+training&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dinterpersonal%2Btraining','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19860044074&hterms=interpersonal+training&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dinterpersonal%2Btraining"><span>Psychological and interpersonal adaptation to Mars <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Harrison, A. A.; Connors, M. M.</p> <p>1985-01-01</p> <p>The crucial importance of a thorough understanding of the psychological and interpersonal dimensions of Mars flights is indicated. This is necessary both to reduce the chances that psychological problems or interpersonal frictions will threaten the success of Mars <span class="hlt">missions</span> and to enhance the quality of <span class="hlt">life</span> of the people involved. Adaptation to interplanetary flight will depend on an interplay of the psychological stresses imposed by the <span class="hlt">missions</span> and the psychological strengths and vulnerabilities of the crewmembers involved. Stresses may be reduced through environmental engineering, manipulating crew composition, and the structuring of situations and tasks. Vulnerabilities may be reduced through improving personnel selection procedures, training personnel in psychological and group dynamics, and providing mechanisms for emotional support. It is essential to supplement anecdotal evidence regarding the human side of space travel with the results of carefully conducted scientific research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19930013516','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19930013516"><span>Space transfer concepts and analysis for exploration <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Woodcock, Gordon R.</p> <p>1992-01-01</p> <p>The current technical effort is part of the third phase of a broad-scoped and systematic study of space transfer concepts for human lunar and Mars <span class="hlt">missions</span>. The study addressed the technical issues relating to the First Lunar Outpost (FLO) habitation vehicle with emphasis on the structure, power, <span class="hlt">life</span> support system, and radiation environment for a baseline habitat with specific alternatives for the baseline.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070031690','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070031690"><span>Electric Propulsion Requirements and <span class="hlt">Mission</span> Analysis Under NASA's In-Space Propulsion Technology Project</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Dudzinski, Leonard a.; Pencil, Eric J.; Dankanich, John W.</p> <p>2007-01-01</p> <p>The In-Space Propulsion Technology Project (ISPT) is currently NASA's sole investment in electric propulsion technologies. This project is managed at NASA Glenn Research Center (GRC) for the NASA Headquarters Science <span class="hlt">Mission</span> Directorate (SMD). The objective of the electric propulsion project area is to develop near-term and midterm electric propulsion technologies to enhance or enable future NASA science <span class="hlt">missions</span> while minimizing risk and cost to the end user. Systems analysis activities sponsored by ISPT seek to identify future <span class="hlt">mission</span> applications in order to quantify <span class="hlt">mission</span> requirements, as well as develop analytical capability in order to facilitate greater understanding and application of electric propulsion and other propulsion technologies in the ISPT portfolio. These analyses guide technology investments by informing decisions and defining metrics for technology development to meet identified <span class="hlt">mission</span> requirements. This paper discusses the <span class="hlt">missions</span> currently being studied for electric propulsion by the ISPT project, and presents the results of recent electric propulsion (EP) <span class="hlt">mission</span> trades. Recent ISPT systems analysis activities include: an initiative to standardize <span class="hlt">life</span> qualification methods for various electric propulsion systems in order to retire perceived risk to proposed EP <span class="hlt">missions</span>; <span class="hlt">mission</span> analysis to identify EP requirements from Discovery, New Frontiers, and Flagship classes of <span class="hlt">missions</span>; and an evaluation of system requirements for radioisotope-powered electric propulsion. Progress and early results of these activities is discussed where available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMIN11A3603B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMIN11A3603B"><span>Low Cost <span class="hlt">Missions</span> Operations on NASA Deep Space <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barnes, R. J.; Kusnierkiewicz, D. J.; Bowman, A.; Harvey, R.; Ossing, D.; Eichstedt, J.</p> <p>2014-12-01</p> <p>The ability to lower <span class="hlt">mission</span> operations costs on any long duration <span class="hlt">mission</span> depends on a number of factors; the opportunities for science, the flight trajectory, and the cruise phase environment, among others. Many deep space <span class="hlt">missions</span> employ long cruises to their final destination with minimal science activities along the way; others may perform science observations on a near-continuous basis. This paper discusses approaches employed by two NASA <span class="hlt">missions</span> implemented by the Johns Hopkins University Applied Physics Laboratory (JHU/APL) to minimize <span class="hlt">mission</span> operations costs without compromising <span class="hlt">mission</span> success: the New Horizons <span class="hlt">mission</span> to Pluto, and the Solar Terrestrial Relations Observatories (STEREO). The New Horizons spacecraft launched in January 2006 for an encounter with the Pluto system.The spacecraft trajectory required no deterministic on-board delta-V, and so the <span class="hlt">mission</span> ops team then settled in for the rest of its 9.5-year cruise. The spacecraft has spent much of its cruise phase in a "hibernation" mode, which has enabled the spacecraft to be maintained with a small operations team, and minimized the contact time required from the NASA Deep Space Network. The STEREO <span class="hlt">mission</span> is comprised of two three-axis stabilized sun-staring spacecraft in heliocentric orbit at a distance of 1 AU from the sun. The spacecraft were launched in October 2006. The STEREO instruments operate in a "decoupled" mode from the spacecraft, and from each other. Since STEREO operations are largely routine, unattended ground station contact operations were implemented early in the <span class="hlt">mission</span>. Commands flow from the MOC to be uplinked, and the data recorded on-board is downlinked and relayed back to the MOC. Tools run in the MOC to assess the health and performance of ground system components. Alerts are generated and personnel are notified of any problems. Spacecraft telemetry is similarly monitored and alarmed, thus ensuring safe, reliable, low cost operations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AdSpR..30.1607D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AdSpR..30.1607D"><span>Planetary protection requirements for orbiter and netlander elements of the CNES/NASA Mars sample return <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Debus, A.</p> <p></p> <p>In the framework of Mars exploration, particularly for <span class="hlt">missions</span> dedicated to the search for <span class="hlt">life</span> or for traces of ancient forms of <span class="hlt">life</span>, NASA and CNES have decided to join their efforts in order to build a Mars sample return <span class="hlt">mission</span>. Taking into account article IX of the OUTER SPACE TREATY (Treaty on principles governing the activities of states in the exploration and use of outer space, including the Moon and other celestial, referenced 610 UNTS 205 - resolution 2222(XXI) of December 1966, ratified in London / Washington January 27, 1967) and in order to comply with the COSPAR planetary protection recommendations, a common planetary protection program has to be established. Mars in-situ experimentations are limited by the size and the mass of the instruments necessary to perform exobiology investigations and, consequently, it appears that the best way to conduct such experiments is to bring back Mars samples to Earth. A sample return <span class="hlt">mission</span> enables the use of a very large number of instruments and analysis protocols, giving exobiologists the best chance to find living entities or organic compounds related to <span class="hlt">life</span>. Such a <span class="hlt">mission</span> is complicated from a planetary protection point of view, it combines constraints for the protection of both the Mars environment as well as Earth, including the preservation of samples to ensure the validity of exobiological experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018LPICo2071.6016O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018LPICo2071.6016O"><span>Impact Craters and Impactites as Important Targets for Mars Sample Return <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osinski, G. R.; Cockell, C. S.; Pontefract, A.; Sapers, H. M.; Tornabene, L. L.</p> <p>2018-04-01</p> <p>Research conducted over the past few years reveals that meteorite impact craters provide substrates and habitats for <span class="hlt">life</span>. We propose that craters and their products should be reconsidered as high priority targets for Mars Sample Return <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMED31B0624I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMED31B0624I"><span>Lunar Quest in Second <span class="hlt">Life</span>, Lunar Exploration Island, Phase II</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ireton, F. M.; Day, B. H.; Mitchell, B.; Hsu, B. C.</p> <p>2010-12-01</p> <p>Linden Lab’s Second <span class="hlt">Life</span> is a virtual 3D metaverse created by users. At any one time there may be 40,000-50,000 users on line. Users develop a persona and are seen on screen as a human figure or avatar. Avatars move through Second <span class="hlt">Life</span> by walking, flying, or teleporting. Users form communities or groups of mutual interest such as music, computer graphics, and education. These groups communicate via e-mail, voice, and text within Second <span class="hlt">Life</span>. Information on downloading the Second <span class="hlt">Life</span> browser and joining can be found on the Second <span class="hlt">Life</span> website: www.secondlife.com. This poster details Phase II in the development of Lunar Exploration Island (LEI) located in Second <span class="hlt">Life</span>. Phase I LEI highlighted NASA’s LRO/LCROSS <span class="hlt">mission</span>. Avatars enter LEI via teleportation arriving at a hall of flight housing interactive exhibits on the LRO/ LCROSS <span class="hlt">missions</span> including full size models of the two spacecraft and launch vehicle. Storyboards with information about the <span class="hlt">missions</span> interpret the exhibits while links to external websites provide further information on the <span class="hlt">mission</span>, both spacecraft’s instrument suites, and related EPO. Other lunar related activities such as My Moon and NLSI EPO programs. A special exhibit was designed for International Observe the Moon Night activities with links to websites for further information. The sim includes several sites for meetings, a conference stage to host talks, and a screen for viewing NASATV coverage of <span class="hlt">mission</span> and other televised events. In Phase II exhibits are updated to reflect on-going lunar exploration highlights, discoveries, and future <span class="hlt">missions</span>. A new section of LEI has been developed to showcase NASA’s Lunar Quest program. A new exhibit hall with Lunar Quest information has been designed and is being populated with Lunar Quest information, spacecraft models (LADEE is in place) and kiosks. A two stage interactive demonstration illustrates lunar phases with static and 3-D stations. As NASA’s Lunar Quest program matures further</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11538996','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11538996"><span>The Neurolab <span class="hlt">mission</span> and biomedical engineering: a partnership for the future.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liskowsky, D R; Frey, M A; Sulzman, F M; White, R J; Likowsky, D R</p> <p>1996-01-01</p> <p>Over the last five years, with the advent of flights of U.S. Shuttle/Spacelab <span class="hlt">missions</span> dedicated entirely to <span class="hlt">life</span> sciences research, the opportunities for conducting serious studies that use a fully outfitted space laboratory to better understand basic biological processes have increased. The last of this series of Shuttle/Spacelab <span class="hlt">missions</span>, currently scheduled for 1998, is dedicated entirely to neuroscience and behavioral research. The <span class="hlt">mission</span>, named Neurolab, includes a broad range of experiments that build on previous research efforts, as well as studies related to less mature areas of space neuroscience. The Neurolab <span class="hlt">mission</span> provides the global scientific community with the opportunity to use the space environment for investigations that exploit microgravity to increase our understanding of basic processes in neuroscience. The results from this premier <span class="hlt">mission</span> should lead to a significant advancement in the field as a whole and to the opening of new lines of investigation for future research. Experiments under development for this <span class="hlt">mission</span> will utilize human subjects as well as a variety of other species. The capacity to carry out detailed experiments on both human and animal subjects in space allows a diverse complement of studies that investigate functional changes and their underlying molecular, cellular, and physiological mechanisms. In order to conduct these experiments, a wide array of biomedical instrumentation will be used, including some instruments and devices being developed especially for the <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089879&hterms=neuroscience&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dneuroscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089879&hterms=neuroscience&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dneuroscience"><span>The Neurolab <span class="hlt">mission</span> and biomedical engineering: a partnership for the future</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liskowsky, D. R.; Frey, M. A.; Sulzman, F. M.; White, R. J.; Likowsky, D. R.</p> <p>1996-01-01</p> <p>Over the last five years, with the advent of flights of U.S. Shuttle/Spacelab <span class="hlt">missions</span> dedicated entirely to <span class="hlt">life</span> sciences research, the opportunities for conducting serious studies that use a fully outfitted space laboratory to better understand basic biological processes have increased. The last of this series of Shuttle/Spacelab <span class="hlt">missions</span>, currently scheduled for 1998, is dedicated entirely to neuroscience and behavioral research. The <span class="hlt">mission</span>, named Neurolab, includes a broad range of experiments that build on previous research efforts, as well as studies related to less mature areas of space neuroscience. The Neurolab <span class="hlt">mission</span> provides the global scientific community with the opportunity to use the space environment for investigations that exploit microgravity to increase our understanding of basic processes in neuroscience. The results from this premier <span class="hlt">mission</span> should lead to a significant advancement in the field as a whole and to the opening of new lines of investigation for future research. Experiments under development for this <span class="hlt">mission</span> will utilize human subjects as well as a variety of other species. The capacity to carry out detailed experiments on both human and animal subjects in space allows a diverse complement of studies that investigate functional changes and their underlying molecular, cellular, and physiological mechanisms. In order to conduct these experiments, a wide array of biomedical instrumentation will be used, including some instruments and devices being developed especially for the <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19770036652&hterms=training+plan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtraining%2Bplan','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19770036652&hterms=training+plan&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dtraining%2Bplan"><span>Operational plans for <span class="hlt">life</span> science payloads - From experiment selection through postflight reporting</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mccollum, G. W.; Nelson, W. G.; Wells, G. W.</p> <p>1976-01-01</p> <p>Key features of operational plans developed in a study of the Space Shuttle era <span class="hlt">life</span> science payloads program are presented. The data describes the overall acquisition, staging, and integration of payload elements, as well as program implementation methods and <span class="hlt">mission</span> support requirements. Five configurations were selected as representative payloads: (a) carry-on laboratories - medical emphasis experiments, (b) mini-laboratories - medical/biology experiments, (c) seven-day dedicated laboratories - medical/biology experiments, (d) 30-day dedicated laboratories - Regenerative <span class="hlt">Life</span> Support Evaluation (RLSE) with selected <span class="hlt">life</span> science experiments, and (e) Biomedical Experiments Scientific Satellite (BESS) - extended duration primate (Type I) and small vertebrate (Type II) <span class="hlt">missions</span>. The recommended operational methods described in the paper are compared to the fundamental data which has been developed in the <span class="hlt">life</span> science Spacelab <span class="hlt">Mission</span> Simulation (SMS) test series. Areas assessed include crew training, experiment development and integration, testing, data-dissemination, organization interfaces, and principal investigator working relationships.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100033369','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100033369"><span>CANADARM: 20 Years of <span class="hlt">Mission</span> Success Through Adaptation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hiltz, Michael; Rice, Craig; Boyle, Keith; Allison, Ronald</p> <p>2001-01-01</p> <p>As part of the National Aeronautics and Space Administration's Space Shuttle Transportation System, the Shuttle Remote Manipulator System has played a vital role in the success of 60 space <span class="hlt">missions</span>. This paper concludes that the robustness and success of the Canadarm over its 20 year <span class="hlt">life</span> can be attributed to the adaptations that have been made to it to meet the increased demands that have been placed on the system. Enhancements that have been made to the arm to improve its operational capabilities, reduce risk and extend its <span class="hlt">life</span> are examined in this paper. Potential future enhancements based on operational trends are also discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19760021478','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19760021478"><span>Long-<span class="hlt">life</span> <span class="hlt">mission</span> reliability for outer planet atmospheric entry probes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mccall, M. T.; Rouch, L.; Maycock, J. N.</p> <p>1976-01-01</p> <p>The results of a literature analysis on the effects of prolonged exposure to deep space environment on the properties of outer planet atmospheric entry probe components are presented. Materials considered included elastomers and plastics, pyrotechnic devices, thermal control components, metal springs and electronic components. The rates of degradation of each component were determined and extrapolation techniques were used to predict the effects of exposure for up to eight years to deep space. Pyrotechnic devices were aged under accelerated conditions to an equivalent of eight years in space and functionally tested. Results of the literature analysis of the selected components and testing of the devices indicated that no severe degradation should be expected during an eight year space <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20180002209','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20180002209"><span>A Planet for Goldilocks: The Search for Evidence of <span class="hlt">Life</span> Beyond Earth</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Batalha, Natalie M.</p> <p>2018-01-01</p> <p>A Planet for Goldilocks: The Search for Evidence of <span class="hlt">Life</span> Beyond Earth "Not too hot, not too cold" begins the prescription for a world that's just right for <span class="hlt">life</span> as we know it. Finding evidence of <span class="hlt">life</span> beyond Earth is one of the primary goals of science agencies around the world thanks in large part to NASA's Kepler <span class="hlt">Mission</span> which launched in 2009 with the objective of finding Goldilocks planets orbiting other stars like our Sun. Indeed, the space telescope opened our eyes to the terrestrial-sized planets that populate the galaxy as well as exotic worlds unlike anything that exists in the solar system. The <span class="hlt">mission</span> ignited the search for <span class="hlt">life</span> beyond earth via remote detection of atmospheric biosignatures on exoplanets. Most recently, our collective imagination was awakened by the discovery of Goldilocks worlds orbiting some of the nearest neighbors to the Sun, turning abstractions into destinations. Dr. Batalha will give an overview of the science legacy of the Kepler <span class="hlt">Mission</span> and other key discoveries. She'll give a preview of what's to come by highlighting the <span class="hlt">missions</span> soon to launch and those that are concepts taking shape on the drawing board.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=data+AND+governance&pg=7&id=EJ1163254','ERIC'); return false;" href="https://eric.ed.gov/?q=data+AND+governance&pg=7&id=EJ1163254"><span><span class="hlt">Mission</span> as Metaphor: Reconceptualizing How Leaders Utilize Institutional <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Zenk, Leslie R.; Seashore Louis, Karen R.</p> <p>2018-01-01</p> <p>Background/Context: Institutional <span class="hlt">missions</span> serve many purposes within universities, but most studies focus on how <span class="hlt">mission</span> points to direction, guidelines, or priorities. However, organizational <span class="hlt">missions</span> have been shown to have other functions such as instructing members about actions or behaviors that are acceptable. This paper therefore examines…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=MSFC-9262661&hterms=koi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26Nf%3DPublication-Date%257CBTWN%2B19900101%2B20180515%26N%3D0%26No%3D10%26Ntt%3Dkoi','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=MSFC-9262661&hterms=koi&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26Nf%3DPublication-Date%257CBTWN%2B19900101%2B20180515%26N%3D0%26No%3D10%26Ntt%3Dkoi"><span>Activities During Spacelab-J <span class="hlt">Mission</span> at Payload Operations and Control Center</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1992-01-01</p> <p>The group of Japanese researchers of the Spacelab-J (SL-J) were thumbs-up in the Payload Operations Control Center (POCC) at the Marshall Space Flight Center after the successful launch of Space Shuttle Orbiter Endeavour that carried their experiments. The SL-J was a joint <span class="hlt">mission</span> of NASA and the National Space Development Agency of Japan (NASDA) utilizing a marned Spacelab module. The <span class="hlt">mission</span> conducted microgravity investigations in materials and <span class="hlt">life</span> sciences. Materials science investigations covered such fields as biotechnology, electronic materials, fluid dynamics and transport phenomena, glasses and ceramics, metals and alloys, and acceleration measurements. <span class="hlt">Life</span> sciences included experiments on human health, cell separation and biology, developmental biology, animal and human physiology and behavior, space radiation, and biological rhythms. Test subjects included the crew, Japanese koi fish (carp), cultured animal and plant cells, chicken embryos, fruit flies, fungi and plant seeds, frogs, and frog eggs. The POCC was the air/ground communications channel between the astronauts and ground control teams during the Spacelab <span class="hlt">missions</span>. The Spacelab science operations were a cooperative effort between the science astronaut crew in orbit and their colleagues in the POCC. Spacelab-J was launched aboard the Space Shuttle Orbiter Endeavour on September 12, 1992.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.P11B2075S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.P11B2075S"><span>International Search for <span class="hlt">Life</span> in Ocean Worlds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sherwood, B.</p> <p>2015-12-01</p> <p>We now know that our solar system contains diverse "ocean worlds." One has abundant surface water and <span class="hlt">life</span>; another had significant surface water in the distant past and has drawn significant exploration attention; several contain large amounts of water beneath ice shells; and several others evince unexpected, diverse transient or dynamic water-related processes. In this century, humanity will explore these worlds, searching for <span class="hlt">life</span> beyond Earth and seeking thereby to understand the limits of habitability. Of our ocean worlds, Enceladus presents a unique combination of attributes: large reservoir of subsurface water already known to contain salts, organics, and silica nanoparticles originating from hydrothermal activity; and able to be sampled via a plume predictably expressed into space. These special circumstances immediately tag Enceladus as a key destination for potential <span class="hlt">missions</span> to search for evidence of non-Earth <span class="hlt">life</span>, and lead to a range of potential <span class="hlt">mission</span> concepts: for orbital reconnaissance; in situ and returned-sample analysis of plume and surface-fallback material; and direct sulcus, vent, cavern, and ocean exploration. Each <span class="hlt">mission</span> type can address a unique set of science questions, and would require a unique set of capabilities, most of which are not yet developed. Both the questions and the capability developments can be sequenced into a programmatic precedence network, the realization of which requires international cooperation. Three factors make this true: exploring remote oceans autonomously will cost a lot; the Outer Space Treaty governs planetary protection; and discovery of non-Earth <span class="hlt">life</span> is an epochal human imperative. Results of current planning will be presented in AGU session 8599: how ocean-world science questions and capability requirements can be parsed into programmatically acceptable <span class="hlt">mission</span> increments; how one <span class="hlt">mission</span> proposed into the Discovery program in 2015 would take the next step on this path; the Decadal calendar of</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150008746&hterms=interior+design&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dinterior%2Bdesign','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150008746&hterms=interior+design&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dinterior%2Bdesign"><span>Designing <span class="hlt">Mission</span> Operations for the Gravity Recovery and Interior Laboratory <span class="hlt">Mission</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Havens, Glen G.; Beerer, Joseph G.</p> <p>2012-01-01</p> <p>NASA's Gravity Recovery and Interior Laboratory (GRAIL) <span class="hlt">mission</span>, to understand the internal structure and thermal evolution of the Moon, offered unique challenges to <span class="hlt">mission</span> operations. From launch through end of <span class="hlt">mission</span>, the twin GRAIL orbiters had to be operated in parallel. The journey to the Moon and into the low science orbit involved numerous maneuvers, planned on tight timelines, to ultimately place the orbiters into the required formation-flying configuration necessary. The baseline GRAIL <span class="hlt">mission</span> is short, only 9 months in duration, but progressed quickly through seven very unique <span class="hlt">mission</span> phases. Compressed into this short <span class="hlt">mission</span> timeline, operations activities and maneuvers for both orbiters had to be planned and coordinated carefully. To prepare for these challenges, development of the GRAIL <span class="hlt">Mission</span> Operations System began in 2008. Based on high heritage multi-<span class="hlt">mission</span> operations developed by NASA's Jet Propulsion Laboratory and Lockheed Martin, the GRAIL <span class="hlt">mission</span> operations system was adapted to meet the unique challenges posed by the GRAIL <span class="hlt">mission</span> design. This paper describes GRAIL's system engineering development process for defining GRAIL's operations scenarios and generating requirements, tracing the evolution from operations concept through final design, implementation, and validation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040043715&hterms=food+analysis&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dfood%2Banalysis','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040043715&hterms=food+analysis&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dfood%2Banalysis"><span>A Probabilistic Risk Analysis (PRA) of Human Space <span class="hlt">Missions</span> for the Advanced Integration Matrix (AIM)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Harry W.; Dillon-Merrill, Robin L.; Thomas, Gretchen A.</p> <p>2003-01-01</p> <p>The Advanced Integration Matrix (AIM) Project u7ill study and solve systems-level integration issues for exploration <span class="hlt">missions</span> beyond Low Earth Orbit (LEO), through the design and development of a ground-based facility for developing revolutionary integrated systems for joint human-robotic <span class="hlt">missions</span>. This paper describes a Probabilistic Risk Analysis (PRA) of human space <span class="hlt">missions</span> that was developed to help define the direction and priorities for AIM. Risk analysis is required for all major NASA programs and has been used for shuttle, station, and Mars lander programs. It is a prescribed part of early planning and is necessary during concept definition, even before <span class="hlt">mission</span> scenarios and system designs exist. PRA cm begin when little failure data are available, and be continually updated and refined as detail becomes available. PRA provides a basis for examining tradeoffs among safety, reliability, performance, and cost. The objective of AIM's PRA is to indicate how risk can be managed and future human space <span class="hlt">missions</span> enabled by the AIM Project. Many critical events can cause injuries and fatalities to the crew without causing loss of vehicle or <span class="hlt">mission</span>. Some critical systems are beyond AIM's scope, such as propulsion and guidance. Many failure-causing events can be mitigated by conducting operational tests in AIM, such as testing equipment and evaluating operational procedures, especially in the areas of communications and computers, autonomous operations, <span class="hlt">life</span> support, thermal design, EVA and rover activities, physiological factors including habitation, medical equipment, and food, and multifunctional tools and repairable systems. AIM is well suited to test and demonstrate the habitat, <span class="hlt">life</span> support, crew operations, and human interface. Because these account for significant crew, systems performance, and science risks, AIM will help reduce <span class="hlt">mission</span> risk, and <span class="hlt">missions</span> beyond LEO are far enough in the future that AIM can have significant impact.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050167126','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050167126"><span>Palmer Quest: A Feasible Nuclear Fission "Vision <span class="hlt">Mission</span>" to the Mars Polar Caps</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carsey, F. D.; Beegle, L. W.; Nakagawa, R.; Elliott, J. O.; Matthews, J. B.; Coleman, M. L.; Hecht, M. H.; Ivaniov, A. B.; Head, J. W.; Milkovich, S.</p> <p>2005-01-01</p> <p>We are engaged in a NASA Vision <span class="hlt">Mission</span> study, called Palmer Quest after the American Antarctic explorer Nathaniel Palmer, to assess the presence of <span class="hlt">life</span> and evaluate the habitability of the basal domain of the Mars polar caps. We address this goal through four objectives: 1. Determine the presence of amino acids, nutrients, and geochemical heterogeneity in the ice sheet. 2. Quantify and characterize the provenance of the amino acids in Mars ice. 3. Assess the stratification of outcropped units for indications of habitable zones. 4. Determine the accumulation of ice, mineralogic material, and amino acids in Mars ice caps over the present epoch. Because of the defined scientific goal for the vision <span class="hlt">mission</span>, the Palmer Quest focus is astrobiological; however, the results of the study make us optimistic that aggressive multi-platform in-situ <span class="hlt">missions</span> that address a wide range of objectives, such as climate change, can be supported by variations of the approach used on this <span class="hlt">mission</span>. <span class="hlt">Mission</span> Overview: The Palmer Quest baseline</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012TJSAI..10.Tp23N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012TJSAI..10.Tp23N"><span><span class="hlt">Mission</span> X in Japan, an Education Outreach Program Featuring Astronautical Specialties and Knowledge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niihori, Maki; Yamada, Shin; Matsuo, Tomoaki; Nakao, Reiko; Nakazawa, Takashi; Kamiyama, Yoshito; Takeoka, Hajime; Matsumoto, Akiko; Ohshima, Hiroshi; Mukai, Chiaki</p> <p></p> <p>In the science field, disseminating new information to the public is becoming increasingly important, since it can aid a deeper understanding of scientific significance and increase the number of future scientists. As part of our activities, we at the Japan Aerospace Exploration Agency (JAXA) Space Biomedical Research Office, started work to focus on education outreach featuring space biomedical research. In 2010, we launched the <span class="hlt">Mission</span> X education program in Japan, named after “<span class="hlt">Mission</span> X: Train Like an Astronaut” (hereinafter called “<span class="hlt">Mission</span> X”), mainly led by NASA and European Space Agency (ESA). <span class="hlt">Mission</span> X is an international public outreach program designed to encourage proper nutrition and exercise and teaching young people to live and eat like astronauts. We adopted <span class="hlt">Mission</span> X's standpoint, and modified the program based on the originals to suit Japanese culture and the students' grade. Using astronauts as examples, this <span class="hlt">mission</span> can motivate and educate students to instill and adopt good nutrition and physical fitness as <span class="hlt">life</span>-long practices.Here we introduce our pilot <span class="hlt">mission</span> of the “<span class="hlt">Mission</span> X in Japan” education program, which was held in early 2011. We are continuing the education/public outreach to promote the public understanding of science and contribute to science education through lectures on astronautical specialties and knowledge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120013472','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120013472"><span>Human in the Loop Integrated <span class="hlt">Life</span> Support Systems Ground Testing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Henninger, Donald L.; Marmolejo, Jose A.; Seaman, Calvin H.</p> <p>2012-01-01</p> <p>Human exploration <span class="hlt">missions</span> beyond low earth orbit will be long duration with abort scenarios of days to months. This necessitates provisioning the crew with all the things they will need to sustain themselves while carrying out <span class="hlt">mission</span> objectives. Systems engineering and integration is critical to the point where extensive integrated testing of <span class="hlt">life</span> support systems on the ground is required to identify and mitigate risks. Ground test facilities (human-rated altitude chambers) at the Johnson Space Center are being readied to integrate all the systems for a <span class="hlt">mission</span> along with a human test crew. The relevant environment will include deep space habitat human accommodations, sealed atmosphere capable of 14.7 to 8 psi total pressure and 21 to 32% oxygen concentration, <span class="hlt">life</span> support systems (food, air, and water), communications, crew accommodations, medical, EVA, tools, etc. Testing periods will approximate those of the expected <span class="hlt">missions</span> (such as a near Earth asteroid, Earth-Moon L2 or L1, the moon, Mars). This type of integrated testing is needed for research and technology development as well as later during the <span class="hlt">mission</span> design, development, test, and evaluation (DDT&E) phases of an approved program. Testing will evolve to be carried out at the <span class="hlt">mission</span> level fly the <span class="hlt">mission</span> on the ground . <span class="hlt">Mission</span> testing will also serve to inform the public and provide the opportunity for active participation by international, industrial and academic partners.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20110023644','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20110023644"><span>Human-in-the-Loop Integrated <span class="hlt">Life</span> Support Systems Ground Testing</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Henninger, Donald L.; Marmolejo, Jose A.; Westheimer, David T.</p> <p>2011-01-01</p> <p>Human exploration <span class="hlt">missions</span> beyond low earth orbit will be long duration with abort scenarios of days to months. This necessitates provisioning the crew with all the things they will need to sustain themselves while carrying out <span class="hlt">mission</span> objectives. Systems engineering and integration is critical to the point where extensive integrated testing of <span class="hlt">life</span> support systems on the ground is required to identify and mitigate risks. Ground test facilities (human-rated altitude chamber) at the Johnson Space Center are being readied to integrate all the systems for a <span class="hlt">mission</span> along with a human test crew. The relevant environment will include deep space habitat human accommodations, sealed atmosphere of 8 psi total pressure and 32% oxygen concentration, <span class="hlt">life</span> support systems (food, air, water), communications, crew accommodations, medical, EVA, tools, etc. Testing periods will approximate those of the expected <span class="hlt">missions</span> (such as a near Earth asteroid, Earth-Moon L2 or L1, the moon). This type of integrated testing is needed for research and technology development as well as later during the <span class="hlt">mission</span> design, development, test, and evaluation (DDT&E) phases of an approved program. Testing will evolve to be carried out at the <span class="hlt">mission</span> level fly the <span class="hlt">mission</span> on the ground . <span class="hlt">Mission</span> testing will also serve to inform the public and provide the opportunity for active participation by international partners.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120006481','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120006481"><span>Reliability Impacts in <span class="hlt">Life</span> Support Architecture and Technology Selection</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lange Kevin E.; Anderson, Molly S.</p> <p>2012-01-01</p> <p>Quantitative assessments of system reliability and equivalent system mass (ESM) were made for different <span class="hlt">life</span> support architectures based primarily on International Space Station technologies. The analysis was applied to a one-year deep-space <span class="hlt">mission</span>. System reliability was increased by adding redundancy and spares, which added to the ESM. Results were thus obtained allowing a comparison of the ESM for each architecture at equivalent levels of reliability. Although the analysis contains numerous simplifications and uncertainties, the results suggest that achieving necessary reliabilities for deep-space <span class="hlt">missions</span> will add substantially to the <span class="hlt">life</span> support ESM and could influence the optimal degree of <span class="hlt">life</span> support closure. Approaches for reducing reliability impacts were investigated and are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JCos...2210219S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JCos...2210219S"><span>2013 - <span class="hlt">Life</span> is a Cosmic Phenomenon : The "Search for Water" evolves into the "Search for <span class="hlt">Life</span>"</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, William E.</p> <p>2013-03-01</p> <p>We propose that the 2013 data from the Kepler <span class="hlt">Mission</span> (giving a current estimate of the number of earth-like planets in the habitable zone of sun-like stars as 144 billion), has caused a consciousness change in human belief in the probability of <span class="hlt">life</span> off earth. This seems to have affected NASA's public statements which are now leaning to the more visionary <span class="hlt">mission</span> goal of the "Search for <span class="hlt">Life</span>" rather than the 1975-2012 focus of the "Search for Water". We propose that the first confirmed earth-like planet, expected to be announced later this year, be called "BORUCKI" in honour of the visionary USA scientist Bill Borucki, the father of the Kepler <span class="hlt">Mission</span>. We explore the 2013 status of the Hoyle-Wickramasinghe Model of Panspermia, its hypothesis, propositions, experiments and evidence. We use the Karl Popper model for scientific hypotheses (1). Finally we explore Sir Fred Hoyle's vision of a planetary microbe defense system we call the Hoyle Shield. We explore the subsystem components of the shield and assess some options for these components using break-though technologies already available.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA082175','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA082175"><span><span class="hlt">Icebreaking</span> Concepts.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1980-01-01</p> <p>Development, Report No 731343 Tests of 102 mm dia milling 160-190 1.1-1.3 Bonz, 1973 cutters 6n floating .ce Tesis of chain saw on floating ice 1430 9.9 tlonz... dia (urcular saws 140 (field) 2 3 Lecourt. I . I W Lewis. I Kotras and I C Roth (1973) Mechan- cutting floating ice 290-32) flab) 20-22 ical ire (utter...8217 3 . NUMBER OF PAGES 21 14. MONITORING AGENCY NAME & ADORESS(II different from Controlling Offlce) 1S. SECURITY CLASS. (of this report) Unclassified</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870010868','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870010868"><span>Manned Mars <span class="hlt">missions</span>: A working group report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Duke, Michael B. (Editor); Keaton, Paul W. (Editor)</p> <p>1986-01-01</p> <p>The discussions of the Working Group (based in large part on working papers, which will shortly be published separately) are summarized. These papers cover a broad range of subjects which need to be addressed in the formulation of such a formidable enterprise as a manned Mars program. Science objective and operations; Mars surface infrastructure and activities; <span class="hlt">mission</span> and system concepts and configurations; <span class="hlt">life</span> sciences; impacts on the space infrastructure; and costs, schedules, and organizations are addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100040617','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100040617"><span>Heritage Systems Engineering Lessons from NASA Deep Space <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barley, Bryan; Newhouse, Marilyn; Clardy, Dennon</p> <p>2010-01-01</p> <p>In the design and development of complex spacecraft <span class="hlt">missions</span>, project teams frequently assume the use of advanced technology systems or heritage systems to enable a <span class="hlt">mission</span> or reduce the overall <span class="hlt">mission</span> risk and cost. As projects proceed through the development <span class="hlt">life</span> cycle, increasingly detailed knowledge of the advanced and heritage systems within the spacecraft and <span class="hlt">mission</span> environment identifies unanticipated technical issues. Resolving these issues often results in cost overruns and schedule impacts. The National Aeronautics and Space Administration (NASA) Discovery & New Frontiers (D&NF) Program Office at Marshall Space Flight Center (MSFC) recently studied cost overruns and schedule delays for 5 <span class="hlt">missions</span>. The goal was to identify the underlying causes for the overruns and delays, and to develop practical mitigations to assist the D&NF projects in identifying potential risks and controlling the associated impacts to proposed <span class="hlt">mission</span> costs and schedules. The study found that optimistic hardware/software inheritance and technology readiness assumptions caused cost and schedule growth for all five <span class="hlt">missions</span> studied. The cost and schedule growth was not found to be the result of technical hurdles requiring significant technology development. The projects institutional inheritance and technology readiness processes appear to adequately assess technology viability and prevent technical issues from impacting the final <span class="hlt">mission</span> success. However, the processes do not appear to identify critical issues early enough in the design cycle to ensure project schedules and estimated costs address the inherent risks. In general, the overruns were traceable to: an inadequate understanding of the heritage system s behavior within the proposed spacecraft design and <span class="hlt">mission</span> environment; an insufficient level of development experience with the heritage system; or an inadequate scoping of the systemwide impacts necessary to implement an advanced technology for space flight applications</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850021223','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850021223"><span>Advanced Regenerative Environmental Control and <span class="hlt">Life</span> Support Systems: Air and Water Regeneration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schubert, F. H.; Wynveen, R. A.; Quattrone, P. D.</p> <p>1985-01-01</p> <p>Extended manned space <span class="hlt">missions</span> will require regenerative <span class="hlt">life</span> support techniques. Past manned <span class="hlt">missions</span> used nonregenerative expendables, except for a molecular sieve based carbon dioxide removal system aboard Skylab. The resupply penalties associated with expendables becomes prohibitive as crew size and <span class="hlt">mission</span> duration increase. The Space Station scheduled to be operational in the 1990's is based on a crew of four to sixteen and a resupply period of 90 days or greater. It will be the first major spacecraft to employ regenerable techniques for <span class="hlt">life</span> support. The techniques to be used in the requirements for the space station are addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850054760&hterms=regeneration&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dregeneration','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850054760&hterms=regeneration&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dregeneration"><span>Advanced regenerative environmental control and <span class="hlt">life</span> support systems - Air and water regeneration</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schubert, F. H.; Wynveen, R. A.; Quattrone, P. D.</p> <p>1984-01-01</p> <p>Extended manned space <span class="hlt">missions</span> will require regenerative <span class="hlt">life</span> support techniques. Past U.S. manned <span class="hlt">missions</span> used nonregenerative expendables, except for a molecular sieve-based carbon dioxide removal system aboard Skylab. The resupply penalties associated with expandables becomes prohibitive as crew size and <span class="hlt">mission</span> duration increase. The U.S. Space Station, scheduled to be operational in the 1990's, is based on a crew of four to sixteen and a resupply period of 90 days or greater. It will be the first major spacecraft to employ regenerable techniques for <span class="hlt">life</span> support. The paper uses the requirements for the Space Station to address these techniques.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950010813','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950010813"><span>Shared <span class="hlt">mission</span> operations concept</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Spradlin, Gary L.; Rudd, Richard P.; Linick, Susan H.</p> <p>1994-01-01</p> <p>Historically, new JPL flight projects have developed a <span class="hlt">Mission</span> Operations System (MOS) as unique as their spacecraft, and have utilized a <span class="hlt">mission</span>-dedicated staff to monitor and control the spacecraft through the MOS. NASA budgetary pressures to reduce <span class="hlt">mission</span> operations costs have led to the development and reliance on multimission ground system capabilities. The use of these multimission capabilities has not eliminated an ongoing requirement for a nucleus of personnel familiar with a given spacecraft and its <span class="hlt">mission</span> to perform <span class="hlt">mission</span>-dedicated operations. The high cost of skilled personnel required to support projects with diverse <span class="hlt">mission</span> objectives has the potential for significant reduction through shared <span class="hlt">mission</span> operations among <span class="hlt">mission</span>-compatible projects. Shared <span class="hlt">mission</span> operations are feasible if: (1) the <span class="hlt">missions</span> do not conflict with one another in terms of peak activity periods, (2) a unique MOS is not required, and (3) there is sufficient similarity in the <span class="hlt">mission</span> profiles so that greatly different skills would not be required to support each <span class="hlt">mission</span>. This paper will further develop this shared <span class="hlt">mission</span> operations concept. We will illustrate how a Discovery-class <span class="hlt">mission</span> would enter a 'partner' relationship with the Voyager Project, and can minimize MOS development and operations costs by early and careful consideration of <span class="hlt">mission</span> operations requirements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150023252','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150023252"><span>Evolution of Orion <span class="hlt">Mission</span> Design for Exploration <span class="hlt">Mission</span> 1 and 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gutkowski, Jeffrey P.; Dawn, Timothy F.; Jedrey, Richard M.</p> <p>2016-01-01</p> <p>The evolving <span class="hlt">mission</span> design and concepts of NASA's next steps have shaped Orion into the spacecraft that it is today. Since the initial inception of Orion, through the Constellation Program, and now in the Exploration <span class="hlt">Mission</span> frame-work with the Space Launch System (SLS), each <span class="hlt">mission</span> design concept and program goal have left Orion with a set of capabilities that can be utilized in many different <span class="hlt">mission</span> types. Exploration <span class="hlt">Missions</span> 1 and 2 (EM-1 and EM-2) have now been at the forefront of the <span class="hlt">mission</span> design focus for the last several years. During that time, different Design Reference <span class="hlt">Missions</span> (DRMs) were built, analyzed, and modified to solve or mitigate enterprise level design trades to ensure a viable <span class="hlt">mission</span> from launch to landing. The resulting DRMs for EM-1 and EM-2 were then expanded into multi-year trajectory scans to characterize vehicle performance and Earth-Moon geometry trends. This provides Orion's subsystems with stressing reference trajectories to help design their system. Now that Orion has progressed through the Preliminary and Critical Design Re-views (PDR and CDR) there is a general shift in the focus of <span class="hlt">mission</span> design from aiding the vehicle design to providing <span class="hlt">mission</span> specific products needed for pre-flight and real time operations. Some of the <span class="hlt">mission</span> specific products need-ed include analysis of steering law performance, inputs into navigational accura-cy assessments, abort options at any point in the <span class="hlt">mission</span> for each valid trajecto-ry in the launch window, recontact avoidance between the upper stage and Orion post nominal separation, etc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160001270','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160001270"><span>Evolution of Orion <span class="hlt">Mission</span> Design for Exploration <span class="hlt">Mission</span> 1 and 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gutkowski, Jeffrey P.; Dawn, Timothy F.; Jedrey, Richard M.</p> <p>2016-01-01</p> <p>The evolving <span class="hlt">mission</span> design and concepts of NASA’s next steps have shaped Orion into the spacecraft that it is today. Since the initial inception of Orion, through the Constellation Program, and now in the Exploration <span class="hlt">Mission</span> frame-work with the Space Launch System (SLS), each <span class="hlt">mission</span> design concept and pro-gram goal have left Orion with a set of capabilities that can be utilized in many different <span class="hlt">mission</span> types. Exploration <span class="hlt">Missions</span> 1 and 2 (EM-1 and EM-2) have now been at the forefront of the <span class="hlt">mission</span> design focus for the last several years. During that time, different Design Reference <span class="hlt">Missions</span> (DRMs) were built, analyzed, and modified to solve or mitigate enterprise level design trades to ensure a viable <span class="hlt">mission</span> from launch to landing. The resulting DRMs for EM-1 and EM-2 were then expanded into multi-year trajectory scans to characterize vehicle performance as affected by variations in Earth-Moon geometry. This provides Orion’s subsystems with stressing reference trajectories to help design their system. Now that Orion has progressed through the Preliminary and Critical Design Reviews (PDR and CDR), there is a general shift in the focus of <span class="hlt">mission</span> design from aiding the vehicle design to providing <span class="hlt">mission</span> specific products needed for pre-flight and real time operations. Some of the <span class="hlt">mission</span> specific products needed include, large quantities of nominal trajectories for multiple monthly launch periods and abort options at any point in the <span class="hlt">mission</span> for each valid trajectory in the launch window.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030000595','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030000595"><span>Thin-Film Solar Array Earth Orbit <span class="hlt">Mission</span> Applicability Assessment</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hoffman, David J.; Kerslake, Thomas W.; Hepp, Aloysius F.; Raffaelle, Ryne P.</p> <p>2002-01-01</p> <p>This is a preliminary assessment of the applicability and spacecraft-level impact of using very lightweight thin-film solar arrays with relatively large deployed areas for representative Earth orbiting <span class="hlt">missions</span>. The most and least attractive features of thin-film solar arrays are briefly discussed. A simple calculation is then presented illustrating that from a solar array alone mass perspective, larger arrays with less efficient but lighter thin-film solar cells can weigh less than smaller arrays with more efficient but heavier crystalline cells. However, a proper spacecraft-level systems assessment must take into account the additional mass associated with solar array deployed area: the propellant needed to desaturate the momentum accumulated from area-related disturbance torques and to perform aerodynamic drag makeup reboost. The results for such an assessment are presented for a representative low Earth orbit (LEO) <span class="hlt">mission</span>, as a function of altitude and <span class="hlt">mission</span> <span class="hlt">life</span>, and a geostationary Earth orbit (GEO) <span class="hlt">mission</span>. Discussion of the results includes a list of specific <span class="hlt">mission</span> types most likely to benefit from using thin-film arrays. NASA Glenn's low-temperature approach to depositing thin-film cells on lightweight, flexible plastic substrates is also briefly discussed to provide a perspective on one approach to achieving this enabling technology. The paper concludes with a list of issues to be addressed prior to use of thin-film solar arrays in space and the observation that with their unique characteristics, very lightweight arrays using efficient, thin-film cells on flexible substrates may become the best array option for a subset of Earth orbiting <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910067765&hterms=hack&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dhack','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910067765&hterms=hack&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dhack"><span>Nuclear electric propulsion <span class="hlt">mission</span> performance for fast piloted Mars <span class="hlt">missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hack, K. J.; George, J. A.; Dudzinski, L. A.</p> <p>1991-01-01</p> <p>A <span class="hlt">mission</span> study aimed at minimizing the time humans would spend in the space environment is presented. The use of nuclear electric propulsion (NEP), when combined with a suitable <span class="hlt">mission</span> profile, can reduce the trip time to durations competitive with other propulsion systems. Specifically, a split <span class="hlt">mission</span> profile utilizing an earth crew capture vehicle accounts for a significant portion of the trip time reduction compared to previous studies. NEP is shown to be capable of performing fast piloted <span class="hlt">missions</span> to Mars at low power levels using near-term technology and is considered to be a viable candidate for these <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3005285','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3005285"><span>Defining <span class="hlt">Life</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2010-01-01</p> <p>Abstract Any definition is intricately connected to a theory that gives it meaning. Accordingly, this article discusses various definitions of <span class="hlt">life</span> held in the astrobiology community by considering their connected “theories of <span class="hlt">life</span>.” These include certain “list” definitions and a popular definition that holds that <span class="hlt">life</span> is a “self-sustaining chemical system capable of Darwinian evolution.” We then act as “anthropologists,” studying what scientists do to determine which definition-theories of <span class="hlt">life</span> they constructively hold as they design <span class="hlt">missions</span> to seek non-terran <span class="hlt">life</span>. We also look at how constructive beliefs about biosignatures change as observational data accumulate. And we consider how a definition centered on Darwinian evolution might itself be forced to change as supra-Darwinian species emerge, including in our descendents, and consider the chances of our encountering supra-Darwinian species in our exploration of the Cosmos. Last, we ask what chemical structures might support Darwinian evolution universally; these structures might be universal biosignatures. Key Words: Evolution—Life—<span class="hlt">Life</span> detection—Biosignatures. Astrobiology 10, 1021–1030. PMID:21162682</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.P33A2127R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.P33A2127R"><span>Exploration of Icy Moons in the Outer Solar System: Updated Planetary Protection Requirements for <span class="hlt">Missions</span> to Enceladus and Europa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rummel, J. D.; Race, M. S.</p> <p>2016-12-01</p> <p>Enceladus and Europa are bodies with icy/watery environments and potential habitable conditions for <span class="hlt">life</span>, making both of great interest in astrobiological studies of chemical evolution and /or origin of <span class="hlt">life</span>. They are also of significant planetary protection concern for spacecraft <span class="hlt">missions</span> because of the potential for harmful contamination during exploration. At a 2015 COSPAR colloquium in Bern Switzerland, international scientists identified an urgent need to establish planetary protection requirements for <span class="hlt">missions</span> proposing to return samples to Earth from Saturn's moon Enceladus. Deliberations at the meeting resulted in recommended policy updates for both forward and back contamination requirements for <span class="hlt">missions</span> to Europa and Enceladus, including <span class="hlt">missions</span> sampling plumes originating from those bodies. These recently recommended COSPAR policy revisions and biological contamination requirements will be applied to future <span class="hlt">missions</span> to Europa and Encealadus, particularly noticeable in those with plans for in situ <span class="hlt">life</span> detection and sample return capabilities. Included in the COSPAR policy are requirementsto `break the chain of contact' with Europa or Enceladus, to keep pristine returned materials contained, and to complete required biohazard analyses, testing and/or sterilization upon return to Earth. Subsequent to the Bern meeting, additional discussions of Planetary Protection of Outer Solar System bodies (PPOSS) are underway in a 3-year study coordinated by the European Science Foundation and involving multiple international partners, including Japan, China and Russia, along with a US observer. This presentation will provide science and policy updates for those whose research or activities will involve icy moon <span class="hlt">missions</span> and exploration.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880035105&hterms=life+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dlife%2Bscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880035105&hterms=life+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dlife%2Bscience"><span>Telescience testbedding for <span class="hlt">life</span> science <span class="hlt">missions</span> on the Space Station</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rasmussen, D.; Mian, A.; Bosley, J.</p> <p>1988-01-01</p> <p>'Telescience', defined as the ability of distributed system users to perform remote operations associated with NASA Space Station <span class="hlt">life</span> science operations, has been explored by a developmental testbed project allowing rapid prototyping to evaluate the functional requirements of telescience implementation in three areas: (1) research planning and design, (2) remote operation of facilities, and (3) remote access to data bases for analysis. Attention is given to the role of expert systems in telescience, its use in realistic simulation of Space Shuttle payload remote monitoring, and remote interaction with <span class="hlt">life</span> science data bases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950023871&hterms=life+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dlife%2Bscience','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950023871&hterms=life+science&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dlife%2Bscience"><span>NASA <span class="hlt">Life</span> Sciences Program</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1995-01-01</p> <p>This <span class="hlt">Life</span> Science Program video examines the variety of projects that study both the physiological and psychological impacts on astronauts due to extended space <span class="hlt">missions</span>. The hazards of space radiation and microgravity effects on the human body are described, along with these effects on plant growth, and the performance of medical procedures in space. One research technique, which is hoped to provide help for future space travel, is the study of aquanauts and their <span class="hlt">life</span> habits underwater.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001xmm..pres....4.','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001xmm..pres....4."><span>Space <span class="hlt">Mission</span> : Y3K</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p></p> <p>2001-01-01</p> <p>ESA and the APME are hosting a contest for 10 - 15 year olds in nine European countries (Austria, Belgium, France, Germany, Italy, the Netherlands, Spain, Sweden and the United Kingdom). The contest is based on an interactive CD ROM, called Space <span class="hlt">Mission</span>: Y3K, which explores space technology and shows some concrete uses of that technology in enhancing the quality of <span class="hlt">life</span> on Earth. The CD ROM invites kids to join animated character Space Ranger Pete on an action-packed, colourful journey through space. Space Ranger Pete begins on Earth: the user navigates around a 'locker room' to learn about synthetic materials used in rocket boosters, heat shields, space suits and helmets, and how these materials have now become indispensable to everyday <span class="hlt">life</span>. From Earth he flies into space and the user follows him from the control room in the spacecraft to a planet, satellites and finally to the International Space Station. Along the way, the user jots down clues that he or she discovers in this exploration, designing an imaginary space community and putting together a submission for the contest. The lucky winners will spend a weekend training as "junior astronauts" at the European Space Centre in Belgium (20-22 April 2001). They will be put through their astronaut paces, learning the art of space walking, running their own space <span class="hlt">mission</span>, piloting a space capsule and re-entering the Earth's atmosphere. The competition features in various youth media channels across Europe. In the UK, popular BBC Saturday morning TV show, Live & Kicking, will be launching the competition and will invite viewers to submit their space community designs to win a weekend at ESC. In Germany, high circulation children's magazine Geolino will feature the competition in the January issue and on their internet site. And youth magazine ZoZitDat will feature the competition in the Netherlands throughout February. Space <span class="hlt">Mission</span>: Y3K is part of an on-going partnership between the ESA's Technology Transfer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150008906&hterms=project+structural&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dproject%2Bstructural','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150008906&hterms=project+structural&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dproject%2Bstructural"><span>Reliability and Qualification of Hardware to Enhance the <span class="hlt">Mission</span> Assurance of JPL/NASA Projects</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ramesham, Rajeshuni</p> <p>2010-01-01</p> <p>Packaging Qualification and Verification (PQV) and <span class="hlt">life</span> testing of advanced electronic packaging, mechanical assemblies (motors/actuators), and interconnect technologies (flip-chip), platinum temperature thermometer attachment processes, and various other types of hardware for Mars Exploration Rover (MER)/Mars Science Laboratory (MSL), and JUNO flight projects was performed to enhance the <span class="hlt">mission</span> assurance. The qualification of hardware under extreme cold to hot temperatures was performed with reference to various project requirements. The flight like packages, assemblies, test coupons, and subassemblies were selected for the study to survive three times the total number of expected temperature cycles resulting from all environmental and operational exposures occurring over the <span class="hlt">life</span> of the flight hardware including all relevant manufacturing, ground operations, and <span class="hlt">mission</span> phases. Qualification/<span class="hlt">life</span> testing was performed by subjecting flight-like qualification hardware to the environmental temperature extremes and assessing any structural failures, mechanical failures or degradation in electrical performance due to either overstress or thermal cycle fatigue. Experimental flight qualification test results will be described in this presentation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810055481&hterms=life+mars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlife%2Bmars','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810055481&hterms=life+mars&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlife%2Bmars"><span><span class="hlt">Life</span> on Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Soffen, G. A.</p> <p>1981-01-01</p> <p>The Viking biology experiments are examined. It is noted that the Viking <span class="hlt">missions</span> did not find a terrestrial type of <span class="hlt">life</span> at either of the two landing sites. This evidence may suggest that Mars is lifeless, but science demands a more rigorous proof; thus, it is still not known whether <span class="hlt">life</span> exists on Mars. It is suggested that the Martian polar regions must be explored before a conclusive answer is possible; the permanent polar caps of Mars are frozen water and would act as a 'cold finger' of the planet to trap organic molecules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960020461','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960020461"><span>STS-71, Space Shuttle <span class="hlt">Mission</span> Report</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Frike, Robert W., Jr.</p> <p>1995-01-01</p> <p>The STS-71 Space Shuttle Program <span class="hlt">Mission</span> Report summarizes the Payload activities and provides detailed data on the Orbiter, External Tank (ET), Solid Rocket Booster (SRB), Reusable Solid Rocket Motor (RSRM), and the Space Shuttle main engine (SSME) systems performance. STS-71 is the 100th United States manned space flight, the sixty-ninth Space Shuttle flight, the forty-fourth flight since the return-to-flight, the fourteenth flight of the OV-104 Orbiter vehicle Atlantis, and the first joint United States (U.S.)-Russian docking <span class="hlt">mission</span> since 1975. In addition to the OV-104 Orbiter vehicle, the flight vehicle consisted of an ET that was designated ET-70; three SSMEs that were designated 2028, 2034, and 2032 in positions 1, 2, and 3, respectively; and two SRBs that were designated Bl-072. The RSRMs that were an integral part of the SRBs were designated 360L045A for the left SRB and 360W045B for the right SRB. The STS-71 <span class="hlt">mission</span> was planned as a 1 0-day plus 1-day-extension <span class="hlt">mission</span> plus 2 additional days for contingency operations and weather avoidance. The primary objectives of this flight were to rendezvous and dock with the Mir Space Station and perform on-orbit joint U.S.-Russian <span class="hlt">life</span> sciences investigations, logistical resupply of the Mir Space Station, return of the United States astronaut flying on the Mir, the replacement of the Mir-18 crew with the two-cosmonaut Mir-19 crew, and the return of the Mir-18 crew to Earth. The secondary objectives were to perform the requirements of the IMAX Camera and the Shuttle Amateur Radio experiment-2 (SAREX-2).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-sts078-396-015.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-sts078-396-015.html"><span>AGHF, TRE and TVD experiment activity in the Spacelab during LMS-1 <span class="hlt">mission</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1996-07-09</p> <p>STS078-396-015 (20 June - 7 July 1996) --- Payload specialist Jean-Jacques Favier, representing the French Space Agency (CNES), prepares a sample for the Advanced Gradient Heating Facility (AGHF) while wearing instruments that measure upper body movement. The Torso Rotation Experiment (TRE) complements other vestibular studies that measure differences in the way human beings react physically to their surroundings in microgravity. This is a typical <span class="hlt">Life</span> and Microgravity Spacelab (LMS-1) <span class="hlt">mission</span> scene, with several experiments being performed. Astronaut Susan J. Helms, payload commander, assists Favier in the AGHF preparations. Astronaut Richard M. Linnehan (bottom right), <span class="hlt">mission</span> specialist, tests his muscle response with the Handgrip Dynamometer. Astronaut Thomas T. (Tom) Henricks (far background), <span class="hlt">mission</span> commander, offers assistance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12038481','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12038481"><span>Implementing planetary protection requirements for sample return <span class="hlt">missions</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rummel, J D</p> <p>2000-01-01</p> <p>NASA is committed to exploring space while avoiding the biological contamination of other solar system bodies and protecting the Earth against potential harm from materials returned from space. NASA's planetary protection program evaluates <span class="hlt">missions</span> (with external advice from the US National Research Council and others) and imposes particular constraints on individual <span class="hlt">missions</span> to achieve these objectives. In 1997 the National Research Council's Space Studies Board published the report, Mars Sample Return: Issues and Recommendations, which reported advice to NASA on Mars sample return <span class="hlt">missions</span>, complementing their 1992 report, The Biological Contamination of Mars Issues and Recommendations. Meanwhile, NASA has requested a new Space Studies Board study to address sample returns from bodies other than Mars. This study recognizes the variety of worlds that have been opened up to NASA and its partners by small, relatively inexpensive, <span class="hlt">missions</span> of the Discovery class, as well as the reshaping of our ideas about <span class="hlt">life</span> in the solar system that have been occasioned by the Galileo spacecraft's discovery that an ocean under the ice on Jupiter's moon Europa might, indeed, exist. This paper will report on NASA's planned implementation of planetary protection provisions based on these recent National Research Council recommendations, and will suggest measures for incorporation in the planetary protection policy of COSPAR. c2001 COSPAR Published by Elsevier Science Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160009360','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160009360"><span>On Beyond Star Trek, the Role of Synthetic Biology in Nasa's <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Rothschild, Lynn J.</p> <p>2016-01-01</p> <p>The time has come to for NASA to exploit the nascent field of synthetic biology in pursuit of its <span class="hlt">mission</span>, including aeronautics, earth science, astrobiology and notably, human exploration. Conversely, NASA advances the fundamental technology of synthetic biology as no one else can because of its unique expertise in the origin of <span class="hlt">life</span> and <span class="hlt">life</span> in extreme environments, including the potential for alternate <span class="hlt">life</span> forms. This enables unique, creative "game changing" advances. NASA's requirement for minimizing upmass in flight will also drive the field toward miniaturization and automation. These drivers will greatly increase the utility of synthetic biology solutions for military, health in remote areas and commercial purposes. To this end, we have begun a program at NASA to explore the use of synthetic biology in NASA's <span class="hlt">missions</span>, particularly space exploration. As part of this program, we began hosting an iGEM team of undergraduates drawn from Brown and Stanford Universities to conduct synthetic biology research at NASA Ames Research Center. The 2011 team (http://2011.igem.org/Team:Brown-Stanford) produced an award-winning project on using synthetic biology as a basis for a human Mars settlement and the 2012 team has expanded the use of synthetic biology to estimate the potential for <span class="hlt">life</span> in the clouds of other planets (http://2012.igem.org/Team:Stanford-Brown; http://www.calacademy.org/sciencetoday/igem-competition/). More recent projects from the Stanford-Brown team have expanded our ideas of how synthetic biology can aid NASA's <span class="hlt">missions</span> from "Synthetic BioCommunication" (http://2013.igem.org/Team:Stanford-Brown) to a "Biodegradable UAS (drone)" in collaboration with Spelman College (http://2014.igem.org/Team:StanfordBrownSpelman#SBS%20iGEM) and most recently, "Self-Folding Origami" (http://2015.igem.org/Team:Stanford-Brown), the winner of the 2015 award for Manufacturing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170010166','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170010166"><span>Need for Cost Optimization of Space <span class="hlt">Life</span> Support Systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jones, Harry W.; Anderson, Grant</p> <p>2017-01-01</p> <p>As the nation plans manned <span class="hlt">missions</span> that go far beyond Earth orbit to Mars, there is an urgent need for a robust, disciplined systems engineering methodology that can identify an optimized Environmental Control and <span class="hlt">Life</span> Support (ECLSS) architecture for long duration deep space <span class="hlt">missions</span>. But unlike the previously used Equivalent System Mass (ESM), the method must be inclusive of all driving parameters and emphasize the economic analysis of <span class="hlt">life</span> support system design. The key parameter for this analysis is <span class="hlt">Life</span> Cycle Cost (LCC). LCC takes into account the cost for development and qualification of the system, launch costs, operational costs, maintenance costs and all other relevant and associated costs. Additionally, an effective methodology must consider system technical performance, safety, reliability, maintainability, crew time, and other factors that could affect the overall merit of the <span class="hlt">life</span> support system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19940029151&hterms=chemical+warfare&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dchemical%2Bwarfare','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19940029151&hterms=chemical+warfare&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dchemical%2Bwarfare"><span>Advanced integrated <span class="hlt">life</span> support system update</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Whitley, Phillip E.</p> <p>1994-01-01</p> <p>The Advanced Integrated <span class="hlt">Life</span> Support System Program (AILSS) is an advanced development effort to integrate the <span class="hlt">life</span> support and protection requirements using the U.S. Navy's fighter/attack <span class="hlt">mission</span> as a starting point. The goal of AILSS is to optimally mate protection from altitude, acceleration, chemical/biological agent, thermal environment (hot, cold, and cold water immersion) stress as well as <span class="hlt">mission</span> enhancement through improved restraint, night vision, and head-mounted reticules and displays to ensure <span class="hlt">mission</span> capability. The primary emphasis to date has been to establish garment design requirements and tradeoffs for protection. Here the garment and the human interface are treated as a system. Twelve state-off-the-art concepts from government and industry were evaluated for design versus performance. On the basis of a combination of centrifuge, thermal manikin data, thermal modeling, and mobility studies, some key design parameters have been determined. Future efforts will concentrate on the integration of protection through garment design and the use of a single layer, multiple function concept to streamline the garment system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990019365','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990019365"><span>Mir <span class="hlt">Mission</span> Chronicle</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McDonald, Sue</p> <p>1998-01-01</p> <p>Dockings, module additions, configuration changes, crew changes, and major <span class="hlt">mission</span> events are tracked for Mir <span class="hlt">missions</span> 17 through 21 (November 1994 through August 1996). The international aspects of these <span class="hlt">missions</span> are presented, comprising joint <span class="hlt">missions</span> with ESA and NASA, including three U.S. Space Shuttle dockings. New Mir modules described are Spektr, the Docking Module, and Priroda.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007STIN...0730184D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007STIN...0730184D"><span>Reducing the Risk of Human <span class="hlt">Missions</span> to Mars Through Testing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Drake, Bret G.</p> <p>2007-07-01</p> <p>The NASA Deputy Administrator charted an internal NASA planning group to develop the rationale for exploration beyond low-Earth orbit. This team, termed the Exploration Blueprint, performed architecture analyses to develop roadmaps for how to accomplish the first steps beyond Low-Earth Orbit through the human exploration of Mars. Following the results of the Exploration Blueprint study, the NASA Administrator asked for a recommendation on the next steps in human and robotic exploration. Much of the focus during this period was on integrating the results from the previous studies into more concrete implementation strategies in order to understand the relationship between NASA programs, timing, and resulting budgetary implications. This resulted in an integrated approach including lunar surface operations to retire risk of human Mars <span class="hlt">missions</span>, maximum use of common and modular systems including what was termed the exploration transfer vehicle, Earth orbit and lunar surface demonstrations of long-<span class="hlt">life</span> systems, collaboration of human and robotic <span class="hlt">missions</span> to vastly increase <span class="hlt">mission</span> return, and high-efficiency transportation systems (nuclear) for deep-space transportation and power. The data provided in this summary presentation was developed to begin to address one of the key elements of the emerging implementation strategy, namely how lunar <span class="hlt">missions</span> help retire risk of human <span class="hlt">missions</span> to Mars. During this process the scope of the activity broadened into the issue of how testing in general, in various venues including the moon, can help reduce the risk for Mars <span class="hlt">missions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720019467','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720019467"><span>Skylab astronaut <span class="hlt">life</span> support assembly</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Brown, J. T.</p> <p>1972-01-01</p> <p>A comparative study was performed to define an optimum portable <span class="hlt">life</span> support system for suited operations inside and outside the Skylab Program. Emphasis was placed on utilization of qualified equipment, modified versions of qualified equipment, and new systems made up to state-of-the-art components. Outlined are the <span class="hlt">mission</span> constraints, operational modes, and evaluation ground rules by which the Skylab portable <span class="hlt">life</span> support system was selected and the resulting design.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26667195','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26667195"><span>[Medical Humanities--the Historical Significance and <span class="hlt">Mission</span> in Medical Education].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fujino, Akihiro</p> <p>2015-12-01</p> <p>In this paper we consider the significance and <span class="hlt">mission</span> of medical humanities in medical education from the following six viewpoints: (1) misunderstanding of the medical humanities; (2) its historical development; (3) the criteria for the ideal physician; (4) the contents of current Medical Humanities education; (5) the basic philosophy; and (6) its relation to medical professionalism. Medical humanities consists of the three academic components of bioethics, clinical ethics and medical anthropology, and it is a philosophy and an art which penetrate to the fundamental essence of medicine. The purpose of medical humanities is to develop one's own humanity and spirituality through medical practice and contemplation by empathizing with patients' illness narratives through spiritual self-awakening and by understanding the mutual healing powers of human relations by way of the realization of primordial <span class="hlt">life</span>. The basic philosophy is "the coincidence of contraries". The ultimate <span class="hlt">mission</span> of medical humanities is to cultivate physicians to educate themselves and have a <span class="hlt">life</span>-long philosophy of devotion to understanding, through experience, the coincidence of contraries.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050156211&hterms=HUMAN+RESOURCE+MANAGEMENT&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DHUMAN%2BRESOURCE%2BMANAGEMENT','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050156211&hterms=HUMAN+RESOURCE+MANAGEMENT&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DHUMAN%2BRESOURCE%2BMANAGEMENT"><span>Issues that Drive Waste Management Technology Development for Space <span class="hlt">Missions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fisher, John W.; Levri, Julie A.; Hogan, John A.; Wignarajah, Kanapathipillai</p> <p>2005-01-01</p> <p>Waste management technologies for space <span class="hlt">life</span> support systems are currently at low development levels. Manual compaction of waste in plastic bags and overboard disposal to earth return vehicles are the primary current waste management methods. Particularly on future <span class="hlt">missions</span>, continuance of current waste management methods would tend to expose the crew to waste hazards, forfeit recoverable resources such as water, consume valuable crew time, contaminate planetary surfaces, and risk return to Earth of extraterrestrial <span class="hlt">life</span>. Improvement of waste management capabilities is needed for adequate management of wastes. Improvements include recovery of water and other resources, conversion of waste to states harmless to humans, long-term containment of wastes, and disposal of waste. Current NASA requirements documents on waste management are generally not highly detailed. More detailed requirements are needed to guide the development of waste management technologies that will adequately manage waste. In addition to satisfying requirements, waste management technologies must also recover resources. Recovery of resources such as water and habitat volume can reduce <span class="hlt">mission</span> cost. This paper explores the drivers for waste management technology development including requirements and resource recovery.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002ESASP.518..247S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002ESASP.518..247S"><span>Astrobiological relevance and feasibility of a sample collection <span class="hlt">mission</span> to the atmosphere of Venus</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schulze-Makuch, Dirk; Irwin, Louis N.; Irwin, Troy</p> <p>2002-11-01</p> <p>The lower cloud level of the Venusian atmosphere is an environmental niche that could harbor microbial <span class="hlt">life</span>. Particularly the mode 3 particles that are enriched in this atmospheric layer are of astrobiological interest. We propose here a sample collection <span class="hlt">mission</span> to the atmosphere of Venus and evaluate three <span class="hlt">mission</span> options. The first option is a Stardust-type spacecraft used for sample collection, the second option is a Rotating Probe Tether System, and the third option is a Parachute Drop - Balloon Floatation System. Given the current state of technology, the result of our preliminary analysis is that the Parachute Drop - Balloon Floatation <span class="hlt">Mission</span> is the most feasible and practical option.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20020064472&hterms=Dunham&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D30%26Ntt%3DDunham','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20020064472&hterms=Dunham&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D30%26Ntt%3DDunham"><span>Kepler <span class="hlt">Mission</span>: a Discovery-Class <span class="hlt">Mission</span> Designed to Determine the Frequency of Earth-Size and Larger Planets Around Solar-Like Stars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Borucki, William; Koch, David; Lissauer, Jack; Basri, Gibor; Caldwell, John; Cochran, William; Dunham, Edward W.; Gilliland, Ronald; Caldwell, Douglas; Kondo, Yoji; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20020064472'); toggleEditAbsImage('author_20020064472_show'); toggleEditAbsImage('author_20020064472_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20020064472_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20020064472_hide"></p> <p>2002-01-01</p> <p>The first step in discovering the extent of <span class="hlt">life</span> in our galaxy is to determine the number of terrestrial planets in the habitable zone (HZ). The Kepler <span class="hlt">Mission</span> is designed around a 0.95 in aperture Schmidt-type telescope with an array of 42 CCDs designed to continuously monitor the brightness of 100,000 solar-like stars to detect the transits of Earth-size and larger planets. The photometer is scheduled to be launched into heliocentric orbit in 2007. Measurements of the depth and repetition time of transits provide the size of the planet relative to the star and its orbital period. When combined with ground-based spectroscopy of these stars to fix the stellar parameters, the true planet radius and orbit scale, hence the position relative to the HZ are determined. These spectra are also used to discover the relationships between the characteristics of planets and the stars they orbit. In particular, the association of planet size and occurrence frequency with stellar mass and metallicity will be investigated. At the end of the four year <span class="hlt">mission</span>, hundreds of terrestrial planets should be discovered in and near the HZ of their stars if such planets are common. Extending the <span class="hlt">mission</span> to six years doubles the expected number of Earth-size planets in the HZ. A null result would imply that terrestrial planets in the HZ occur in less than 1% of the stars and that <span class="hlt">life</span> might be quite rare. Based on the results of the current Doppler-velocity discoveries, detection of a thousand giant planets is expected. Information on their albedos and densities of those giants showing transits will be obtained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-S69-40023.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-S69-40023.html"><span><span class="hlt">MISSION</span> CONTROL CENTER (MCC) - CELEBRATION - CONCLUSION - APOLLO 11 <span class="hlt">MISSION</span> - MSC</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>1969-07-25</p> <p>S69-40023 (24 July 1969) --- Overall view of the <span class="hlt">Mission</span> Operations Control Room (MOCR) in the <span class="hlt">Mission</span> Control Center (MCC), Building 30, Manned Spacecraft Center (MSC), showing the flight controllers celebrating the successful conclusion of the Apollo 11 lunar landing <span class="hlt">mission</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20150005558&hterms=senior&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dsenior','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20150005558&hterms=senior&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dsenior"><span>JPL <span class="hlt">Mission</span> Bibliometrics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Coppin, Ann</p> <p>2013-01-01</p> <p>For a number of years ongoing bibliographies of various JPL <span class="hlt">missions</span> (AIRS, ASTER, Cassini, GRACE, Earth Science, Mars Exploration Rovers (Spirit & Opportunity)) have been compiled by the JPL Library. <span class="hlt">Mission</span> specific bibliographies are compiled by the Library and sent to <span class="hlt">mission</span> scientists and managers in the form of regular (usually quarterly) updates. Charts showing publications by years are periodically provided to the ASTER, Cassini, and GRACE <span class="hlt">missions</span> for supporting Senior Review/ongoing funding requests, and upon other occasions as a measure of the impact of the <span class="hlt">missions</span>. Basically the Web of Science, Compendex, sometimes Inspec, GeoRef and Aerospace databases are searched for the <span class="hlt">mission</span> name in the title, abstract, and assigned keywords. All get coded for journal publications that are refereed publications.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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