Monster Moose Reading.

ERIC Educational Resources Information Center

Finney, Frank

Monster Moose (MM) Reading is a program specifically aimed at improving children's language, beginning reading, and self-concept development through the creation and utilization of student-authored reading materials which feature a series of wordless picture books about a magical moose. The MM Program is based on the following general principles…

Transgressive Hybrids as Hopeful Monsters.

PubMed

Dittrich-Reed, Dylan R; Fitzpatrick, Benjamin M

2013-06-01

The origin of novelty is a critical subject for evolutionary biologists. Early geneticists speculated about the sudden appearance of new species via special macromutations, epitomized by Goldschmidt's infamous "hopeful monster". Although these ideas were easily dismissed by the insights of the Modern Synthesis, a lingering fascination with the possibility of sudden, dramatic change has persisted. Recent work on hybridization and gene exchange suggests an underappreciated mechanism for the sudden appearance of evolutionary novelty that is entirely consistent with the principles of modern population genetics. Genetic recombination in hybrids can produce transgressive phenotypes, "monstrous" phenotypes beyond the range of parental populations. Transgressive phenotypes can be products of epistatic interactions or additive effects of multiple recombined loci. We compare several epistatic and additive models of transgressive segregation in hybrids and find that they are special cases of a general, classic quantitative genetic model. The Dobzhansky-Muller model predicts "hopeless" monsters, sterile and inviable transgressive phenotypes. The Bateson model predicts "hopeful" monsters with fitness greater than either parental population. The complementation model predicts both. Transgressive segregation after hybridization can rapidly produce novel phenotypes by recombining multiple loci simultaneously. Admixed populations will also produce many similar recombinant phenotypes at the same time, increasing the probability that recombinant "hopeful monsters" will establish true-breeding evolutionary lineages. Recombination is not the only (or even most common) process generating evolutionary novelty, but might be the most credible mechanism for sudden appearance of new forms.

[A case of double monster--duplicitas anterior with diprosopia].

PubMed

Meyer, R

1983-01-01

Report on a delivery of a double monster, duplicitas anterior with diprosopia. The course of delivery is compared with literature. The exclusion of malformations in early pregnancy is possible and necessary. Perinatal mortality can be reduced by abortion in time. The psychic burden of women concerned needs a special regard.

Face Time

ERIC Educational Resources Information Center

Waters, John K.

2008-01-01

It was the perfect Halloween project. Each class would construct a three-dimensional "monster" out of common classroom materials (construction paper, cardboard boxes, tape, markers, glue, string, etc.), then write down instructions for building the monster and send them off to another class in the district, or in some other district, or even some…

Monster Paintings

ERIC Educational Resources Information Center

Huggler, Silvia

2010-01-01

In this article, the author describes a unit on monsters wherein students were charged with painting an imaginary character and, in so doing, demonstrated mastery of expression, organization of space, control of paint media, and application of the elements of art. Students discovered how color and line could be used to convey expression. The media…

Monster Figures and Unhappy Endings in Inuit Literature.

ERIC Educational Resources Information Center

McGrath, Robin

1988-01-01

Examines the incidence of frightening figures and unhappy endings in traditional and modern Inuit stories and identifies purpose for these elements. Monsters and unhappy endings apparently are tools to help children come to terms with Eskimo environment and values. Studies the conclusions and implications for Indian education. (TES)

The Birth of "Frankenstein"

ERIC Educational Resources Information Center

Howard, Jennifer

2008-01-01

Nobody shouts "It's alive!" in the novel that gave birth to Frankenstein's monster. "Frankenstein, or the Modern Prometheus," does not feature mad scientists messing around with beakers in laboratories, nor does it deliver any bug-eyed assistants named Igor. Hollywood has given people those stock images, but the story of the monster and his maker…

Galileo, Gauss, and the Green Monster

ERIC Educational Resources Information Center

Kalman, Dan; Teague, Daniel J.

2013-01-01

Galileo dropped cannonballs from the leaning tower of Pisa to demonstrate something about falling bodies. Gauss was a giant of mathematics and physics who made unparalleled contributions to both fields. More contemporary (and not a person), the Green Monster is the left-field wall at the home of the Boston Red Sox, Fenway Park. Measuring 37 feet…

Tele-Collaborative Projects: Monsters.com?

ERIC Educational Resources Information Center

LeLoup, Jean; Ponterio, Robert

2003-01-01

Examines a collaborative language learning project that brought together elementary and middle school students in France, Canada, and a Basque school to communicate about monsters--a topic of concern to any child who has heard a fairy tale or watched a Disney movie. The Internet is used as the medium of interaction, allowing more students to…

Neoliberal Exclusion and the Fantasy of Competition: What Are Children Learning from "Monsters University?"

ERIC Educational Resources Information Center

Greeley, Luke

2018-01-01

The Disney/Pixar film, "Monsters University" (2013) was a tremendous financial success. As a film written entirely about college students and their quest for social and economic attainment, but marketed primarily to children and adolescents, its messages about the purpose of college and the college experience deserve close examination…

Monsters that Eat People--Oh My! Selecting Literature to Ease Children's Fears

ERIC Educational Resources Information Center

Mercurio, Mia Lynn; McNamee, Abigail

2008-01-01

What should families and teachers look for when they choose picture books to help young children overcome their fears of imaginary monsters, dark places, thunderstorms, and dogs? This article provides criteria for assessing picture books and suggests ways to read them in ways that support children's development. (Contains 4 tables.)

Monsters under the Bed: Critically Investigating Early Years Writing

ERIC Educational Resources Information Center

Melrose, Andrew

2012-01-01

"Monsters Under the Bed" is an essential text focussing on critical and contemporary issues surrounding writing for "early years" children. Containing a critically creative and a creatively critical investigation of the cult and culture of the child and childhood in fiction and non-fictional writing, it also contains a wealth of ideas and critical…

Are We Postmodern Yet? Reading "Monster" with 21st-Century Ninth Graders

ERIC Educational Resources Information Center

Groenke, Susan Lee; Youngquist, Michelle

2011-01-01

When the authors taught Walter Dean Myers's postmodern young adult novel "Monster" to ninth graders, they assumed the students would like the text, as its format and style resemble that of popular television crime shows. The authors also assumed the students would be savvy readers of the text, capable of understanding and integrating postmodern…

Cetus

NASA Astrophysics Data System (ADS)

Murdin, P.

2000-11-01

(the Sea Monster or Whale; abbrev. Cet, gen. Ceti; area 1231 sq. deg.) An equatorial constellation which lies between Aquarius and Taurus, and culminates at midnight in October. It is named after the sea monster from which Perseus rescued Andromeda in Greek mythology, though it is sometimes identified as a whale. Its brightest stars were cataloged by Ptolemy (c. AD 100-175) in the Almagest....

[The monster and the city].

PubMed

Calvo Albizu, A

1996-01-01

"Negative aesthetic categories" and, specifically, the idea of monsters and monstrosity, are used in this discussion of urban phenomena and their relation to modern art. The reflection on monstrosity as a metaphor for the city draws upon such disparate sources as Greek philosophers, Freudian theory, and recent art criticism. It compares dictionary definitions of monster to a general concept of cities, judging the modern metropolis to be "excessively large or extraordinary," "disfigured and ugly," and even "cruel" and "perverse" as demonstrated in social pathologies such as terrorism that breed in cities. The relationship between monstrosity and the city is evident in a variety of artistic manifestations and can be seen in the work of planners, architects, and artists. The examination opens up promising areas for future research in greater depth.

Manipulation of orthogonal neural systems together in electrophysiological recordings: the MONSTER approach to simultaneous assessment of multiple neurocognitive dimensions.

PubMed

Kappenman, Emily S; Luck, Steven J

2012-01-01

Event-related potentials (ERPs) are a powerful tool in understanding and evaluating cognitive, affective, motor, and sensory processing in both healthy and pathological samples. A typical ERP recording session takes considerable time but is designed to isolate only 1-2 components. Although this is appropriate for most basic science purposes, it is an inefficient approach for measuring the broad set of neurocognitive functions that may be disrupted in a neurological or psychiatric disease. The present study provides a framework for more efficiently evaluating multiple neural processes in a single experimental paradigm through the manipulation of functionally orthogonal dimensions. We describe the general MONSTER (Manipulation of Orthogonal Neural Systems Together in Electrophysiological Recordings) approach and explain how it can be adapted to investigate a variety of neurocognitive domains, ERP components, and neural processes of interest. We also demonstrate how this approach can be used to assess group differences by providing data from an implementation of the MONSTER approach in younger (18-30 y of age) and older (65-85 y of age) adult samples. This specific implementation of the MONSTER framework assesses 4 separate neural processes in the visual domain: (1) early sensory processing, using the C1 wave; (2) shifts of covert attention, with the N2pc component; (3) categorization, with the P3 component; and (4) self-monitoring, with the error-related negativity. Although the MONSTER approach is primarily described in the context of ERP experiments, it could also be adapted easily for use with functional magnetic resonance imaging.

Monster Magic: A Reading Activities Idea Book for Use with Children. A Fun with Reading Book.

ERIC Educational Resources Information Center

Fowler, Zinita

Intended as a usable resource for librarians and teachers in planning and implementing a program for young library users and students, this book was developed to stimulate children to use the library. The introduction contains opening comments--including an explanation of how the theme of "monster magic" inspires creativity, specific goals, and a…

The Gonzo Scientist. Slaying monsters for science.

PubMed

Bohannon, John

2008-06-20

Slaying Monsters for Science John Bohannon The first scientific conference held in Azeroth, the online universe of the role-playing game World of Warcraft, went off virtually without a hitch. Although the participants all died during the final day's social event - a massive raid on an enemy fort - they agree that this event is a glimpse at the future of scientific exchange.

360-degree b/w Monster

NASA Image and Video Library

1997-07-10

This 360 degree "monster" panorama was taken by the deployed Imager for Mars Pathfinder (IMP) on Sol 3. All three petals, the perimeter of the deflated airbags, deployed rover Sojourner, forward and backward ramps and prominent surface features are visible. The IMP stands 1.8 meters over the Martian surface. The curvature and misalignment of several sections are due to image parallax. http://photojournal.jpl.nasa.gov/catalog/PIA00662

Monster in My Closet: An Exploratory Study of the Relationship between Parent-Child Co-Sleeping and Nighttime Fears of Preschool Children

ERIC Educational Resources Information Center

Chang, I. Joyce; Pettit, Rebecca W.; Kennedy, Gregory

2004-01-01

Children's nighttime fears, such as monsters in the closet, have been a common issue for the American. In children's cognitive development, vivid imagination has been recognized as a cause of fear, but not all children around the globe share this common experience. This qualitative, exploratory study examined the relationship between parent-child…

Cloacal evaporative cooling: a previously undescribed means of increasing evaporative water loss at higher temperatures in a desert ectotherm, the Gila monster Heloderma suspectum.

PubMed

DeNardo, Dale F; Zubal, Tricia E; Hoffman, Ty C M

2004-02-01

The Gila monster Heloderma suspectum is an active forager in an environment that, at times, can be extremely hot and arid. Thus, Gila monsters face extreme thermostatic and hydrostatic demands. For a desert ectotherm routinely risking dehydration, evaporative water loss (EWL) is typically viewed as detrimental. Yet evaporation simultaneously dehydrates and cools an animal. We explored EWL in Gila monsters by measuring cutaneous, ventilatory and cloacal EWL at five ambient temperatures between 20.5 degrees C and 40 degrees C. Our results show that Gila monsters have high EWL rates relative to body mass. Cutaneous EWL underwent a consistent, temperature-dependent increase over the entire range of test temperatures (Q(10)=1.61, with EWL ranging from 0.378 to 0.954 mg g(-1) h(-1)). Ventilatory EWL did not show a significant temperature-dependent response, but ranged from 0.304 to 0.663 mg g(-1) h(-1). Cloacal EWL was extremely low and relatively constant between 20.5 degrees C and 35 degrees C, but rose dramatically above 35 degrees C (Q(10) >8.3 x 10(7), from 0.0008 at 35 degrees C to 7.30 mg g(-1) h(-1) at 40 degrees C). This steep rise in cloacal EWL coincided with an increasing suppression of body temperature relative to ambient temperature. Dehydration to 80% of initial body mass led to a delay in the onset and an attenuation of the dramatic increase in cloacal EWL. These results emphasize the potential value of EWL for thermoregulation in ectotherms and demonstrate for the first time the role of the cloaca in this process.

Good grief: bereavement literature for young adults and A Monster Calls.

PubMed

Day, Giskin

2012-12-01

Recent years have seen a proliferation of critically acclaimed novels for young adults dealing with bereavement. This is part of a 'bereavement turn'--a contemporary cultural movement to examine publicly our attitudes to death and grieving. This paper examines the narrative strategies in Patrick Ness's award-winning novel A Monster Calls to look at the ways in which the psychic burden of the impending loss of a parent through cancer is managed. The book draws on conventions of children's literature to create a sense of familiarity that helps to balance the emotional stress of the story. The Kübler-Ross stages of grief serve as a heuristic that helps the story deliver catharsis in spite of its inevitably traumatic subject matter. A Monster Calls is an important addition to the canon of fictional pathography.

Monsters or Good Guys: The Mediating Role of Emotions in Transforming a Young Child's Encounter with Nature

ERIC Educational Resources Information Center

Green, Carrie

2016-01-01

Nature-play inspires a sense of awe and wonder in young children, however, the uncertainty of elements in nature can also bring about fear and anxiety. Using sensory tours as a data collection method, this qualitative study explores the emotions of a four-year-old during his exploration of an imaginary "monster castle" in the forest, and…

Fleeing from Frankenstein's Monster and Meeting Kafka on the Way: Algorithmic Decision-Making in Higher Education

ERIC Educational Resources Information Center

Prinsloo, Paul

2017-01-01

In the socio-technical imaginary of higher education, algorithmic decision-making offers huge potential, but we also cannot deny the risks and ethical concerns. In fleeing from Frankenstein's monster, there is a real possibility that we will meet Kafka on our path, and not find our way out of the maze of ethical considerations in the nexus between…

Meal consumption is ineffective at maintaining or correcting water balance in a desert lizard, Heloderma suspectum.

PubMed

Wright, Christian D; Jackson, Marin L; DeNardo, Dale F

2013-04-15

Many xeric organisms maintain water balance by relying on dietary and metabolic water rather than free water, even when free water may be available. For such organisms, hydric state may influence foraging decisions, since meal consumption is meeting both energy and water demands. To understand foraging decisions it is vital to understand the role of dietary water in maintaining water balance. We investigated whether meal consumption was sufficient to maintain water balance in captive Gila monsters (Heloderma suspectum) at varying levels of dehydration. Gila monsters could not maintain water balance over long time scales through meal consumption alone. Animals fed a single meal took no longer to dehydrate than controls when both groups were deprived of free water. Additionally, meal consumption imparts an acute short-term hydric cost regardless of hydration state. Meal consumption typically resulted in a significant elevation in osmolality at 6 h post-feeding, and plasma osmolality never fell below pre-feeding levels despite high water content (~70%) of meals. These results failed to support our hypothesis that dietary water is valuable to Gila monsters during seasonal drought. When considered in conjunction with previous research, these results demonstrate that Gila monsters, unlike many xeric species, are heavily reliant on seasonal rainfall and the resulting free-standing water to maintain water balance.

"What is the Use of a Book without Pictures?" An Exploration of the Impact of Illustrations on Reading Experience in "A Monster Calls"

ERIC Educational Resources Information Center

Aggleton, Jen

2017-01-01

This article examines the effect of Jim Kay's illustrations on the experience of reading "A Monster Calls" by Patrick Ness. The author compares the responses of six Key Stage Three children (11-14 years old), three of whom were given an illustrated version of the text, and three a non-illustrated version. The children with an illustrated…

[From teratology to mythology: ancient legends].

PubMed

Stahl, A; Tourame, P

2010-12-01

The mythology of the Greeks and Romans is full of monsters of fiction: giants, cyclops, centaurs, hydras, Gorgons… The accounts of travelers, reproduced in the Natural History of Pline l'Ancien reported the existence, in distant countries, of men with a dog's head (baboons), of men with a single tall foot (sciapode), beings whose face is embedded in the chest (or acephala blemmyes), to which must be added a wide variety of men with no mouth, no nose, or equipped with giant ears or feet turned backwards, as well as hermaphrodites. Teratology reports on monstrous births, which have constituted the factual basis from which the imagination conceived adults whose morphology corresponds to the monsters of legend. Newborns sirenomelia were behind the legend of sciapode and sirens. Cyclopia have inspired the legend of the cyclops. Anencephaly probably explains the description of headless or blemmyes. The genesis of the legend of baboons may have multiple origins: firstly the existence of people suffering from congenital hypertrichosis, on the other hand, the influence of Egyptian mythology where the god Anubis has a dog's head. The acardiac fetus may explain some monstrous forms, features the work of Hieronymus Bosch. The significance of the monsters of legend, their genesis, their persistence through the ages is complex. By approaching teratology, we added a new field of exploration of real monsters of antiquity and Middle Ages. Copyright © 2010. Published by Elsevier SAS.

Sex Chromosomes and Karyotype of the (Nearly) Mythical Creature, the Gila Monster, Heloderma suspectum (Squamata: Helodermatidae)

PubMed Central

Pokorná, Martina Johnson; Rovatsos, Michail; Kratochvíl, Lukáš

2014-01-01

A wide variety of sex determination systems exist among squamate reptiles. They can therefore serve as an important model for studies of evolutionary transitions among particular sex determination systems. However, we still have only a limited knowledge of sex determination in certain important lineages of squamates. In this respect, one of the most understudied groups is the family Helodermatidae (Anguimorpha) encompassing the only two venomous species of lizards which are potentially lethal to human beings. We uncovered homomorphic ZZ/ZW sex chromosomes in the Gila monster (Heloderma suspectum) with a highly heterochromatic W chromosome. The sex chromosomes are morphologically similar to the ZZ/ZW sex chromosomes of monitor lizards (Varanidae). If the sex chromosomes of helodermatids and varanids are homologous, female heterogamety may be ancestral for the whole Anguimorpha group. Moreover, we found that the karyotype of the Gila monster consists of 2n = 36 chromosomes (14 larger metacentric chromosomes and 22 acrocentric microchromosomes). 2n = 36 is the widely distributed chromosomal number among squamates. In his pioneering works representing the only previous cytogenetic examination of the family Helodermatidae, Matthey reported the karyotype as 2n = 38 and suggested a different chromosomal morphology for this species. We believe that this was probably erroneously. We also discovered a strong accumulation of telomeric sequences on several pairs of microchromosomes in the Gila monster, which is a trait documented relatively rarely in vertebrates. These new data fill an important gap in our understanding of the sex determination and karyotype evolution of squamates. PMID:25119263

Water supplementation affects the behavioral and physiological ecology of Gila monsters (Heloderma suspectum) in the Sonoran Desert.

PubMed

Davis, Jon R; DeNardo, Dale F

2009-01-01

In desert species, seasonal peaks in animal activity often correspond with times of higher rainfall. However, the underlying reason for such seasonality can be hard to discern because the rainy season is often associated with shifts in temperature as well as water and food availability. We used a combination of the natural climate pattern of the Sonoran Desert and periodic water supplementation to determine the extent to which water intake influenced both the behavioral ecology and the physiological ecology of a long-lived desert lizard, the Gila monster (Heloderma suspectum) (Cope 1869). Water-supplemented lizards had lower plasma osmolality (i.e., were more hydrated) and maintained urinary bladder water reserves better during seasonal drought than did control lizards. During seasonal drought, water-supplemented lizards were surface active a significantly greater proportion of time than were controls. This increased surface activity can lead to greater food acquisition for supplemental Gila monsters because tail volume (an index of caudal lipid stores) was significantly greater in supplemented lizards compared with controls in one of the two study years.

Taming the monsters of tomorrow

NASA Astrophysics Data System (ADS)

Kupferschmidt, Kai

2018-01-01

In Mary Shelley's novel, the scientist Victor Frankenstein fears that creating a female companion to his unhappy monster could lead to a "race of devils" that could drive humanity extinct. Today, some scientists worry about scientific advances in the real world that could kill all of humanity, or at least end civilization as we know it. Some two dozen researchers at three academic centers are studying these "existential risks"—including labmade viruses, armies of nanobots, and artificial intelligence—and what can be done about them. But critics say their scenarios are far-fetched and distract from real existential dangers, including climate change and nuclear war.

Beauty and the beast: Superconformal symmetry in a monster module

NASA Astrophysics Data System (ADS)

Dixon, L.; Ginsparg, P.; Harvey, J.

1988-06-01

Frenkel, Lepowsky, and Meurman have constructed a representation of the largest sporadic simple finite group, the Fischer-Griess monster, as the automorphism group of the operator product algebra of a conformal field theory with central charge c=24. In string terminology, their construction corresponds to compactification on a Z 2 asymmetric orbifold constructed from the torus R 24/∧, where ∧ is the Leech lattice. In this note we point out that their construction naturally embodies as well a larger algebraic structure, namely a super-Virasoro algebra with central charge ĉ=16, with the supersymmetry generator constructed in terms of bosonic twist fields.

Does urbanization influence the spatial ecology of Gila monsters in the Sonoran Desert?

USGS Publications Warehouse

Kwiatkowski, M.A.; Schuett, G.W.; Repp, R.A.; Nowak, E.M.; Sullivan, B.K.

2008-01-01

To assess whether urbanization influences the spatial ecology of a rare and protected venomous reptilian predator, the Gila monster Heloderma suspectum, we compared home range (HR) size and movement parameters at three sites varying in degree of urbanization in the Sonoran Desert. We predicted that the urban population of H. suspectum would exhibit smaller HRs, avoid human structures and show less movement. Multivariate analysis indicated that males generally exhibited larger HRs and had higher movement rates and activity levels than females at all three sites. Contrary to our predictions, however, HR size and movement parameters did not vary across the sites in relation to the level of urbanization. At the urban site, individuals often crossed narrow roads and regularly used artificial structures as refuges for extended periods. Furthermore, the population sex ratio at the urban site was female-biased, consistent with the expectation that occupation of larger HRs and higher movement rates results in higher mortality for males in urbanized areas. Gila monsters did not appear to alter certain aspects of their spatial ecology in response to low levels of human activity but additional work will be required to assess population viability and possible effects in the long term and with higher levels of urbanization.

Language Arts

ERIC Educational Resources Information Center

Fisher, Carol J.

1978-01-01

Presents ideas and activities for teaching basic skills including vocabulary building, learning science from the microclimates, using tape recorders to teach reading, and using monsters to teach metrics. (JMB)

Monster Movies?

ERIC Educational Resources Information Center

Vaughn, Susan

1971-01-01

A library hooks onto junior teens' interest in horror films and expands it to their favorite film personalities, the history of horror film, and film techniques and criticism. (28 references) (Author)

Brain and Addiction

MedlinePlus

... build your own monster neuron. CSI Web Adventures Test your forensics knowledge—find clues to unlock the mysteries of drug abuse. Blog Posts Say What? "Habituation" February 05, 2018 / The NIDA ...

Mast cell chymase reduces the toxicity of Gila monster venom, scorpion venom, and vasoactive intestinal polypeptide in mice

PubMed Central

Akahoshi, Mitsuteru; Song, Chang Ho; Piliponsky, Adrian M.; Metz, Martin; Guzzetta, Andrew; Åbrink, Magnus; Schlenner, Susan M.; Feyerabend, Thorsten B.; Rodewald, Hans-Reimer; Pejler, Gunnar; Tsai, Mindy; Galli, Stephen J.

2011-01-01

Mast cell degranulation is important in the pathogenesis of anaphylaxis and allergic disorders. Many animal venoms contain components that can induce mast cell degranulation, and this has been thought to contribute to the pathology and mortality caused by envenomation. However, we recently reported evidence that mast cells can enhance the resistance of mice to the venoms of certain snakes and that mouse mast cell–derived carboxypeptidase A3 (CPA3) can contribute to this effect. Here, we investigated whether mast cells can enhance resistance to the venom of the Gila monster, a toxic component of that venom (helodermin), and the structurally similar mammalian peptide, vasoactive intestinal polypeptide (VIP). Using 2 types of mast cell–deficient mice, as well as mice selectively lacking CPA3 activity or the chymase mouse mast cell protease-4 (MCPT4), we found that mast cells and MCPT4, which can degrade helodermin, can enhance host resistance to the toxicity of Gila monster venom. Mast cells and MCPT4 also can limit the toxicity associated with high concentrations of VIP and can reduce the morbidity and mortality induced by venoms from 2 species of scorpions. Our findings support the notion that mast cells can enhance innate defense by degradation of diverse animal toxins and that release of MCPT4, in addition to CPA3, can contribute to this mast cell function. PMID:21926462

Clues cue the smooze: rhyme, pausing, and prediction help children learn new words from storybooks

PubMed Central

Read, Kirsten

2014-01-01

Rhyme, which is ubiquitous in the language experiences of young children, may be especially facilitative to vocabulary learning because of how it can support active predictions about upcoming words. In two experiments, we tested whether rhyme, when used to help children anticipate new words would make those words easier to learn. Two- to 4-year-old children heard rhyming stanzas naming novel monsters under three conditions: A non-rhyme condition in which novel monster names appeared as unrhymed elements within a rhymed stanza, a non-predictive rhyme condition in which the novel names were the rhymed element in the first line of a stanza, and a predictive rhyme condition in which the monster name came as the rhymed element in the last line of the stanza after a description of the features that distinguished him. In tests of retention and identification children showed greatest novel name learning in the predictive rhyme condition in both between-subjects (Experiment 1) and within-subjects (Experiment 2) comparisons. Additionally, when parents acted as the storybook readers in Experiment 2, many of them distinctly paused before target words in the predictive rhyme condition and for their children a stronger predictive rhyme advantage surfaced. Thus rhyme is not only facilitative for learning, but when the novel vocabulary is specifically in a position where it is predictable from the rhymes, it is most accessible. PMID:24600431

Phobias

MedlinePlus

... claustrophobia for the fear of confined spaces. No matter what specific phobia you have, it's likely to ... professional. Childhood fears, such as fear of the dark, of monsters or of being left alone, are ...

Monsters, dreams and madness: Commentary on 'The arms of the chimeras'.

PubMed

Reis, Bruce

2016-04-01

Considering Freudian and Post-Freudian approaches to the intersubjective Beatrice Ithier puts the work of Michel de M'Uzan and Thomas Ogden in comparison. To this comparison I add a consideration of the work of Christopher Bollas. The highly creative clinical approaches these three theorists take is shown to be informed by their elaborations of the Freudian notion of unconscious communication and by new approaches to the issue of identity. Attention is paid to differentiating traumatic from fanciful chimeras; and to the experience of the analyst undergoing the sorts of transformations requisite to entering this psychic space marked by fluid exchanges of being and becoming, wherein analyst becomes patient, new subjects are created through shared dreams, and through which monsters appear. Copyright © 2016 Institute of Psychoanalysis.

Caffeine

MedlinePlus

... most of their caffeine from soft drinks and energy drinks. (In addition to caffeine, these also can have ... SoBe No Fear 8 ounces 83 mg Monster energy drink 16 ounces 160 mg Rockstar energy drink 8 ...

People and Oceans.

ERIC Educational Resources Information Center

NatureScope, 1988

1988-01-01

Discusses people's relationship with oceans, focusing on ocean pollution, use, and protective measures of the sea and its wildlife. Activities included are "Mythical Monsters"; "Globetrotters"; "Plastic in the Sea"; and "Sea of Many Uses." (RT)

Modular constraints on conformal field theories with currents

NASA Astrophysics Data System (ADS)

Bae, Jin-Beom; Lee, Sungjay; Song, Jaewon

2017-12-01

We study constraints coming from the modular invariance of the partition function of two-dimensional conformal field theories. We constrain the spectrum of CFTs in the presence of holomorphic and anti-holomorphic currents using the semi-definite programming. In particular, we find the bounds on the twist gap for the non-current primaries depend dramatically on the presence of holomorphic currents, showing numerous kinks and peaks. Various rational CFTs are realized at the numerical boundary of the twist gap, saturating the upper limits on the degeneracies. Such theories include Wess-Zumino-Witten models for the Deligne's exceptional series, the Monster CFT and the Baby Monster CFT. We also study modular constraints imposed by W -algebras of various type and observe that the bounds on the gap depend on the choice of W -algebra in the small central charge region.

BOOK REVIEW: Symmetry and the Monster: One of the Greatest Quests of Mathematics

NASA Astrophysics Data System (ADS)

Szabo, R. J.

2007-04-01

The book Symmetry and the Monster: One of the Greatest Quests of Mathematics describes historical events leading up to the discovery of the Monster sporadic group, the largest simple sporadic group. It also expounds the significance and deep relationships between this group and other areas of mathematics and theoretical physics. It begins, in the prologue, with a nice overview of some of the mathematical drama surrounding the discovery of the Monster and its subsequent relationship to number theory (the so-called Moonshine conjectures). From a historical perspective, the book traces back to the roots of group theory, Galois theory, and steadily runs through time through the many famous mathematicians who contributed to group theory, including Lie, Killing and Cartan. Throughout, the author has provided a very nice and deep insight into the sociological and scientific problems at the time, and gives the reader a very prominent inside view of the real people behind the mathematics. The book should be an enjoyable read to anyone with an interest in the history of mathematics. For the non-mathematician the book makes a good, and mostly successful, attempt at being non-technical. Technical mathematical jargon is replaced with more heuristic, intuitive terminology, making the mathematical descriptions in the book fairly easy going. A glossary\\hspace{0.25pc} of\\hspace{0.25pc} terminology for noindent the more scientifically inclined is included in various footnotes throughout the book and in a comprehensive listing at the end of the book. Some more technical material is also included in the form of appendices at the end of the book. Some aspects of physics are also explained in a simple, intuitive way. The author further attempts at various places to give the non-specialist a glimpse into what mathematical proof is all about, and explains the difficulties and technicalities involved in this very nicely (for instance, he mentions the various 100+ page articles that appeared in the hey-day of finite group theory, indicating the enormous technical nature of the subject). The book nicely paints a dramatic landscape leading up to the discovery of the Monster group, and the problems that remain to this day in trying to understand its significance. One can really take from this book a feel of the mathematics leading up to its appearance, and the importance of the classification problem which was responsible for this. One also really gets an appreciation of the efforts and commitments of the mathematicians who contributed to the subject. All in all, this book achieves a nice balance between providing a beautiful historical account of group theory, and explaining the classification problem for finite groups in a way that is accessible to non-scientists. This should prove to be a good read for both the layperson interested in mathematics or mathematical physics, and also both mathematicians and physicists alike.

Mentors and Monsters.

ERIC Educational Resources Information Center

Osa, Nancy

2003-01-01

Discusses the author's investigation and participation in "Friendshipment" - a humanitarian aid shipment to Cuba sponsored by the ecumenical group Pastors for Peace. Researches the involvement of teenagers in "Friendshipment." Describes how her involvement and research led to her book, "Cuba 15." (SG)

Black Holes: The making of a monster

NASA Astrophysics Data System (ADS)

Mayer, Lucio

2017-04-01

The biggest black holes in the Universe were in place soon after the Big Bang. Explaining how they formed so rapidly is a daunting challenge, but the latest simulations give clues to how this may have occurred.

There's a Green Glob in Your Classroom.

ERIC Educational Resources Information Center

Dugdale, Sharon

1983-01-01

Discusses computer games (called intrinsic models) focusing on mathematics rather than on unrelated motivations (flashing lights or sounds). Games include "Green Globs," (equations/linear functions), "Darts"/"Torpedo" (fractions), "Escape" (graphing), and "Make-a-Monster" (equivalent fractions and…

Men, monsters and the modern universe.

NASA Astrophysics Data System (ADS)

Lovi, G.; Tirion, W.

This book is intended to introduce to the constellations in a memorable way and to start looking at the sky's most easily observable objects with nothing more than the eyes or a pair of binoculars or a small telescope.

Differences between the events preceding spina bifida and anencephaly.

PubMed

James, W H

1981-02-01

It is usually held that there is a time continuum in the formation of monoxygotic (MZ) twins which is indexed by their placentation, running from dichorionic to monochorionic diamniotic to monochorionic monoamniotic and conjoined pairs. There is good evidence that this continuum is characterised by a continuum of predisposition to anencephaly, slightly raised in dichorionic pairs but very high in some sorts of conjoined pairs. Although MZ twins, especially monoamniotic and conjoined pairs, are peculiarly liable to anencephaly, they are not particularly susceptible to spina bifida. Among twin pairs concordant for anencephaly or spina bifida, there are strikingly few concordant in the sense of one twin having anencephaly and the other spina bifida, in contrast with the numbers of pairs concordant for the same malformation. The prevalence of anencephaly in double monsters varies with the type of monster, being high in diprosopus. These findings may be explained by the timing of embryonic events.

Differences between the events preceding spina bifida and anencephaly.

PubMed Central

James, W H

1981-01-01

It is usually held that there is a time continuum in the formation of monoxygotic (MZ) twins which is indexed by their placentation, running from dichorionic to monochorionic diamniotic to monochorionic monoamniotic and conjoined pairs. There is good evidence that this continuum is characterised by a continuum of predisposition to anencephaly, slightly raised in dichorionic pairs but very high in some sorts of conjoined pairs. Although MZ twins, especially monoamniotic and conjoined pairs, are peculiarly liable to anencephaly, they are not particularly susceptible to spina bifida. Among twin pairs concordant for anencephaly or spina bifida, there are strikingly few concordant in the sense of one twin having anencephaly and the other spina bifida, in contrast with the numbers of pairs concordant for the same malformation. The prevalence of anencephaly in double monsters varies with the type of monster, being high in diprosopus. These findings may be explained by the timing of embryonic events. PMID:7019447

A Numerical Study on the Streams of Star Debris after Tidal Disruption

NASA Astrophysics Data System (ADS)

Camacho Olachea, Priscila; Ramirez-Ruiz, Enrico; Law-Smith, Jamie

2017-01-01

Lurking at the centers of most galaxies are gigantic star and gas devouring monsters. These monsters are supermassive black holes (SMBHs), some of which are larger than our solar system and ten billion times as massive as our own Sun. The vast majority of stars in the universe live for tens of billions of years, eventually dying from old age as the nuclearreactions that power them become progressively less effective. But for every ten thousand stars that die peacefully, one star will be brutally torn apart by the extreme tidal forces present as it passes near a SMBH. My recent work has been to develop computational tools necessary to study the fates of stars disrupted by SMBHs. In this research project I presentthe results of my numerical study aimed at understanding the streams of star debris that result after disruption.

[Extraordinary news of a curious apothecary. Monsters and wonders in the Florentine diary of Luca Landucci].

PubMed

Ciseri, Lorenzo Montemagno

This article offers a new reading of the well-known diary kept by the Florentine apothecary Luca Landucci between 1450 and 1516, examining its accounts of prodigies and other "monstrous" occurrences from a modern scientific point of view. Particular consideration is given to descriptions of a variety of birth defects observed in various Italian cities at the time, providing explanations for each case based on the latest medical theories. A detailed analysis is provided for a case of cranioschisis recorded in Volterra in 1474, a case of Opitz syndrome occurring in Venice in 1489, the birth of conjoined twins in Padua in the same year, conjoined triplets born to a 60-year-old woman in Venice, the well-publicized account of the 1512 Ravenna monster and, finally, the thoraco-acephalus tetramelus adolescent that Landucci personally observed in Florence in 1513.

Medusan Monster or Ingenuous Model?

ERIC Educational Resources Information Center

Baxter, Cecil, Jr.; Corcoran, James

1972-01-01

The resignation of the president of the Seattle Community College District resulted in the creation of a new form of administrative leadership. An executive committee consisting of the three campus presidents took over and the advantages and disadvantages are listed. (RN)

Further Adventures of Dr. Sony's Mad Monster Machine, or Cutting the Studio Umbilical Cord

ERIC Educational Resources Information Center

Steffin, Sherwin

1977-01-01

We must reexamine our often total reliance on the studio as the only source for instructional television production. The porta-pak provides an alternative. Tips are provided for successful field production. (Author/STS)

Modeling and monitoring the hydrological effects of the Sand Engine.

NASA Astrophysics Data System (ADS)

Schaars, Frans; Hoogmoed, Merel; van Vliet, Frank; Stuyfzand, Pieter; Groen, Michel; van der Made, Kees-Jan; Caljé, Ruben; Auken, Esben; Bergsted Pedersen, Jesper

2013-04-01

Since 1887, Dunea Water Company produces high quality drinking water using the dune area at Monster (Province of South Holland, the Netherlands). Annually, 8 billion liters of water is produced here using artificial recharge and recovery with shallow wells and infiltration lakes. The dunes are an important step in producing drinking water serving as an underground buffer, leveling fluctuating in temperature and quality and removing bacteria and viruses from the infiltrated water in a natural way. Since space is limited in the Netherlands, the drinking water production of Dunea is closely matched with surrounding land uses and natural constraints. This prevents groundwater nuisance, upconing and intrusion of salt water and, in this case, movement of a nearby groundwater pollution. This is especially true in the Monster area where the dunes are fairly low and small; the coast is less than 350 meters from the recovery wells. The coast of Monster was identified as a weak link in the coastal defense of The Netherlands. Because of this, two coastal defense projects were carried out between 2009 and 2011. The first project involved creating an extra dune ridge in front of existing dunes which leads to intrusion of a large volume of seawater. Directly after completion, the Sand Engine was constructed. This hook shaped sand peninsula will supply the coast with sand for the coming decades due to erosion and deposition along the coast. These two large coastal defense projects would obviously influence the tightly balanced hydrological system of Monster. Without hydrological intervention, the drinking water production would no longer be sustainable in this area. To study the effects of these projects and to find a solution to combine coastal defense and drinking water supply, field research and effect (geochemical) modeling were used interactively. To prevent negative effects it was decided to construct interception wells on top of the new dune ridge (28 in total). A comprehensive monitoring system was built to keep track of the salt groundwater and the groundwater heads. The zero measurement included groundwater heads, water samples, but also geophysical methods such as SkyTEM and CVES. We will also show the monitoring system we use to keep track of the groundwater heads and salt water intrusion in the future.

Craniofacial duplication (diprosopus) in a twin.

PubMed

Changaris, D G; McGavran, M H

1976-07-01

A fused, double-faced (diprosopus), anencephalic monster was born prematurely as one of twins after 30 weeks of gestation. We will describe the autopsy findings and summarize the literature concerning the diprosopus defect. Factors other than fetal environment may contribute to its pathogenesis.

The Disabled: Media's Monster.

ERIC Educational Resources Information Center

Bogdan, Robert; And Others

1982-01-01

From the early nineteenth century to the present, horror, gangster, and adventure films, television, the comics, and newspapers have shown physical and mental disabilities to connote murder, violence, and danger. Such false portrayals have promoted negative public attitudes toward people with disabilities. (Author/MJL)

First Look at Milky Way Monster in High-Energy X-ray Light

NASA Image and Video Library

2012-10-23

These images, taken by NASA black-hole hunter, NuSTAR, are the first, focused high-energy X-ray views of the area surrounding the supermassive black hole, called Sagittarius A*, at the center of our galaxy.

Global Positioning System Navigation Algorithms

DTIC Science & Technology

1977-05-01

Historical Remarks on Navigation In Greek mythology , Odysseus sailed safely by the Sirens only to encounter the monsters Scylla and Charybdis...TNED 000 00 1(.7 BIBLIOGRAPHY 1. Pinsent, John. Greek Mythology . Paul Hamlyn, London, 1969. 2. Kline, Morris. Mathematical Thought from Ancient to

NASA AIRS Instrument Captures Data on Monster Winter Storm Affecting 30 States

NASA Image and Video Library

2011-02-02

This visible image from NASA Aqua satellite Jan. 31 shows thickening clouds along a developing intense front in the plains and Midwestern states that will produce excessive snow, freezing rain, sleet, and wind in those areas.

Standards: The Philosophical Monster in the Classroom.

ERIC Educational Resources Information Center

Jervis, Kathe; McDonald, Joseph

1996-01-01

In 1993 Columbia University's National Center for Restructuring Education collaborated with three educational reform organizations to encourage teacher dialogue about assessment reform via the Four Seasons Project. This article profiles three participating schools that use theory, ritual, textmaking, and networking to help teachers reconcile…

The paper monster. Corporate compliance and the board.

PubMed

Hinrichsen, C A; Capobianco, C; Diamond, M

2001-02-01

Fraud and abuse lawsuits and settlements are getting bigger, and the DOJ shows no signs of letting up on its scrutiny of health care organizations. That's why a strong compliance program is your best defense, and it all starts with the board.

Pre-schoolers Learn at Home.

ERIC Educational Resources Information Center

Smith, Penny

1985-01-01

Reviews: "ArithMagic (Counting, Addition, Subtraction)" which uses graphics to illustrate/review basic arithmetic concepts; "The Sweet Shop" which uses graphics (and a character called Mr. Jellybean) to teach arithmetic concepts; and "Math Magic," a monster-filled arcade game that teaches addition and subtraction.…

Space-to-Ground: Tracking a Monster: 09/08/2017

NASA Image and Video Library

2017-09-07

Three crew members said farewell to the station...the station had eyes on a monstrous storm...and what kind of weather can you have in space? NASA's Space to Ground is your weekly update on what's happening aboard the International Space Station.

Assessment of a Mobile Game ("MobileKids Monster Manor") to Promote Physical Activity Among Children.

PubMed

Garde, Ainara; Umedaly, Aryannah; Abulnaga, S Mazdak; Robertson, Leah; Junker, Anne; Chanoine, Jean Pierre; Ansermino, J Mark; Dumont, Guy A

2015-04-01

The majority of children in North America are not meeting current physical activity guidelines. The purpose of this study was to evaluate the impact of a mobile phone game ("MobileKids Monster Manor") as a tool to promote voluntary physical activity among children. The game integrates data from an accelerometer-based activity monitor (Tractivity(®); Kineteks Corp., Vancouver, BC, Canada) wirelessly connected to a phone and was developed with the involvement of a team of young advisors (KidsCan Initiative: Involving Youth as Ambassadors for Research). Fifty-four children 8-13 years old completed a week of baseline data collection by wearing an accelerometer but receiving no feedback about their activity levels. The 54 children were then sequentially assigned to two groups: One group played "MobileKids Monster Manor," and the other received daily activity feedback (steps and active minutes) via an online program. The physical activity (baseline and intervention weeks) was measured using the activity monitor and compared using two-way repeated-measures analysis of variance (intervention×time). Forty-seven children with a body mass index (BMI) z-score of 0.35±1.18 successfully completed the study. Significant (P=0.01) increases in physical activity were observed during the intervention week in both the game and feedback groups (1191 and 796 steps/day, respectively). In the game group, greater physical activity was demonstrated in children with higher BMI z-score, showing 964 steps/day more per BMI z-score unit (P=0.03; 95 percent confidence interval of 98 to 1829). Further investigation is required to confirm that our game design promotes physical activity.

From Mathematical Monsters to Generalized Scale Invariance in Geophysics: Highlights of the Multifractal Saga

NASA Astrophysics Data System (ADS)

Schertzer, D. J.; Tchiguirinskaia, I.; Lovejoy, S.

2013-12-01

Fractals and multifractals are very illustrative of the profound synergies between mathematics and geophysics. The book ';Fractal Geometry of Nature' (Mandelbrot, 1982) brilliantly demonstrated the genericity in geophysics of geometric forms like Cantor set, Peano curve and Koch snowflake, which were once considered as mathematical monsters. However, to tame the geophysical monsters (e.g. extreme weather, floods, earthquakes), it was required to go beyond geometry and a unique fractal dimension. The concept of multifractal was coined in the course of rather theoretical debates on intermittency in hydrodynamic turbulence, sometimes with direct links to atmospheric dynamics. The latter required a generalized notion of scale in order to deal both with scale symmetries and strong anisotropies (e.g. time vs. space, vertical vs. horizontal). It was thus possible to show that the consequences of intermittency are of first order, not just 'corrections' with respect to the classical non-intermittent modeling. This was in fact a radical paradigm shift for geophysics: the extreme variability of geophysical fields over wide ranges of scale, which had long been so often acknowledged and deplored, suddenly became handy. Recent illustrations are the possibility to track down in large date sets the Higgs boson of intermittence, i.e. a first order multifractal phase transition leading to self-organized criticality, and to simulate intermittent vector fields with the help of Lie cascades, based for instance on random Clifford algebra. It is rather significant that this revolution is no longer limited to fundamental and theoretical problems of geophysics, but now touches many applications including environmental management, in particular for urban management and resilience. These applications are particularly stimulating when taken in their full complexity.

Outliers and Extremes: Dragon-Kings or Dragon-Fools?

NASA Astrophysics Data System (ADS)

Schertzer, D. J.; Tchiguirinskaia, I.; Lovejoy, S.

2012-12-01

Geophysics seems full of monsters like Victor Hugo's Court of Miracles and monstrous extremes have been statistically considered as outliers with respect to more normal events. However, a characteristic magnitude separating abnormal events from normal ones would be at odd with the generic scaling behaviour of nonlinear systems, contrary to "fat tailed" probability distributions and self-organized criticality. More precisely, it can be shown [1] how the apparent monsters could be mere manifestations of a singular measure mishandled as a regular measure. Monstrous fluctuations are the rule, not outliers and they are more frequent than usually thought up to the point that (theoretical) statistical moments can easily be infinite. The empirical estimates of the latter are erratic and diverge with sample size. The corresponding physics is that intense small scale events cannot be smoothed out by upscaling. However, based on a few examples, it has also been argued [2] that one should consider "genuine" outliers of fat tailed distributions so monstrous that they can be called "dragon-kings". We critically analyse these arguments, e.g. finite sample size and statistical estimates of the largest events, multifractal phase transition vs. more classical phase transition. We emphasize the fact that dragon-kings are not needed in order that the largest events become predictable. This is rather reminiscent of the Feast of Fools picturesquely described by Victor Hugo. [1] D. Schertzer, I. Tchiguirinskaia, S. Lovejoy et P. Hubert (2010): No monsters, no miracles: in nonlinear sciences hydrology is not an outlier! Hydrological Sciences Journal, 55 (6) 965 - 979. [2] D. Sornette (2009): Dragon-Kings, Black Swans and the Prediction of Crises. International Journal of Terraspace Science and Engineering 1(3), 1-17.

Diversions: Hilbert and Sierpinski Space-Filling Curves, and beyond

ERIC Educational Resources Information Center

Gough, John

2012-01-01

Space-filling curves are related to fractals, in that they have self-similar patterns. Such space-filling curves were originally developed as conceptual mathematical "monsters", counter-examples to Weierstrassian and Reimannian treatments of calculus and continuity. These were curves that were everywhere-connected but…

College Men and Jealousy

ERIC Educational Resources Information Center

Knox, David; Breed, Rhonda; Zusman, Marty

2007-01-01

Cultural meanings (e.g. the green eyed monster) and research interests have traditionally focused on female jealousy. In contrast, this research focused on male jealousy. Two-hundred ninety-one undergraduates at a large southeastern university completed a confidential, anonymous forty-four-item questionnaire on jealousy. Men reacted differently…

Steampunk: Full Steam Ahead

ERIC Educational Resources Information Center

Campbell, Heather M.

2010-01-01

Steam-powered machines, anachronistic technology, clockwork automatons, gas-filled airships, tentacled monsters, fob watches, and top hats--these are all elements of steampunk. Steampunk is both speculative fiction that imagines technology evolved from steam-powered cogs and gears--instead of from electricity and computers--and a movement that…

Marching Monsters: Sculpture in Motion.

ERIC Educational Resources Information Center

Wolfe, George

1984-01-01

With a grant from the National Endowment for the Arts, teenage art club members made a 20-foot float called "Bad Seed," which they entered in a parade spoofing the Mardi Gras. It had a purple volcano drooling chartreuse lava while giving birth to a huge dragon. (RM)

HIV/AIDS and Children in the English Speaking Caribbean.

ERIC Educational Resources Information Center

Dicks, Barbara A., Ed.

This collection of papers addresses the HIV/AIDS situation among English-speaking children in the Caribbean. Papers include: "Preface" (C. James Hospedales); "Introduction"; (Barbara A. Dicks); "HIV/AIDS: Challenging a Monster" (Brendan Bain); "HIV/AIDS in Caribbean Children and Adolescents" (Noreen Jack);…

"Can You Hear Me Now, Ms. Monster?": Anger, "Thumos," and First-Year Composition

ERIC Educational Resources Information Center

Baecker, Diann

2007-01-01

There are not many English words for "anger." There's "wrath" and "ire," although no one uses "ire" anymore and hardly anyone "wrath." There's "frustration," "resentment," and "indignation," but they don't have the emotional intensity of "anger," a word that…

Fossilized venom: the unusually conserved venom profiles of Heloderma species (beaded lizards and gila monsters).

PubMed

Koludarov, Ivan; Jackson, Timothy N W; Sunagar, Kartik; Nouwens, Amanda; Hendrikx, Iwan; Fry, Bryan G

2014-12-22

Research into snake venoms has revealed extensive variation at all taxonomic levels. Lizard venoms, however, have received scant research attention in general, and no studies of intraclade variation in lizard venom composition have been attempted to date. Despite their iconic status and proven usefulness in drug design and discovery, highly venomous helodermatid lizards (gila monsters and beaded lizards) have remained neglected by toxinological research. Proteomic comparisons of venoms of three helodermatid lizards in this study has unravelled an unusual similarity in venom-composition, despite the long evolutionary time (~30 million years) separating H. suspectum from the other two species included in this study (H. exasperatum and H. horridum). Moreover, several genes encoding the major helodermatid toxins appeared to be extremely well-conserved under the influence of negative selection (but with these results regarded as preliminary due to the scarcity of available sequences). While the feeding ecologies of all species of helodermatid lizard are broadly similar, there are significant morphological differences between species, which impact upon relative niche occupation.

The DELTA MONSTER: An RPV designed to investigate the aerodynamics of a delta wing platform

NASA Technical Reports Server (NTRS)

Connolly, Kristen; Flynn, Mike; Gallagher, Randy; Greek, Chris; Kozlowski, Marc; Mcdonald, Brian; Mckenna, Matt; Sellar, Rich; Shearon, Andy

1989-01-01

The mission requirements for the performance of aerodynamic tests on a delta wind planform posed some problems, these include aerodynamic interference; structural support; data acquisition and transmission instrumentation; aircraft stability and control; and propulsion implementation. To eliminate the problems of wall interference, free stream turbulence, and the difficulty of achieving dynamic similarity between the test and actual flight aircraft that are associated with aerodynamic testing in wind tunnels, the concept of the remotely piloted vehicle which can perform a basic aerodynamic study on a delta wing was the main objective for the Green Mission - the Delta Monster. The basic aerodynamic studies were performed on a delta wing with a sweep angle greater than 45 degrees. These tests were performed at various angles of attack and Reynolds numbers. The delta wing was instrumented to determine the primary leading edge vortex formation and location, using pressure measurements and/or flow visualization. A data acquisition system was provided to collect all necessary data.

Coping with the Green-Eyed Monster: Conceptualizing and Measuring Communicative Responses to Romantic Jealousy.

ERIC Educational Resources Information Center

Guerrero, Laura K.; And Others

1995-01-01

Examines communicative responses to romantic jealousy. Finds 12 superordinate categories and 67 tactics in communicative responses to jealousy. Develops measures for six types of interactive responses (integrative communication, distributive communication, active distancing, general avoidance/denial, expression of negative affect, and violent…

Sentence Processing in an Artificial Language: Learning and Using Combinatorial Constraints

ERIC Educational Resources Information Center

Amato, Michael S.; MacDonald, Maryellen C.

2010-01-01

A study combining artificial grammar and sentence comprehension methods investigated the learning and online use of probabilistic, nonadjacent combinatorial constraints. Participants learned a small artificial language describing cartoon monsters acting on objects. Self-paced reading of sentences in the artificial language revealed comprehenders'…

The Pedagogy of Monsters: Scary Disturbances in a Doctoral Research Preparation Course

ERIC Educational Resources Information Center

Lesko, Nancy; Simmons, Jacqueline A.; Quarshie, Antoinette; Newton, Nicki

2008-01-01

Background/Context: Although doctoral education is an important component of research universities, few investigations of doctoral education exist. Furthermore, with the push in education and in other disciplines to help beginning researchers understand multiple paradigmatic, epistemological, and theoretical orientations that define fields of…

Fueling the Flames of the Green-Eyed Monster: The Role of Ruminative Thought in Reaction to Romantic Jealousy.

ERIC Educational Resources Information Center

Carson, Christine L.; Cupach, William R.

2000-01-01

Examines factors predicted to influence individuals' responses to romantic jealousy. Details a study in which undergraduate students completed scales measuring relationship-specific linking, relationship-specific rumination, possessiveness, trust, and communicative responses to jealousy. Suggests that jealous rumination is an important cognitive…

Monsters in the Closet: Spyware Awareness and Prevention

ERIC Educational Resources Information Center

Cordes, Christofer Sean

2005-01-01

Spyware is the general term that describes a collection of technologies that help external parties in "gathering information about a person or organization without their knowledge." In addition to the minor annoyances spyware generates, such as redirected pages, redirected searches, and pop-up ads, a spyware infection can have more malicious…

Internet Investigations: Mixing Talent with Teachers and Telecommunications.

ERIC Educational Resources Information Center

Brown, Mark E.; Riley, Tracy L.

1998-01-01

Describes how teams of grade 4-9 gifted students investigated unsolved mysteries like Bigfoot, aliens and UFOs, the Loch Ness Monster, and Stonehenge to develop Internet and research skills. Highlights student observations on difficulties encountered using the Internet for research, notes student evaluation of the workshop, and provides addresses…

Monsters, Lovers and Former Friends: Exploring Relationships with Mathematics via Personification

ERIC Educational Resources Information Center

Zazkis, Dov

2015-01-01

Personification is the attribution of human qualities to non-human entities. The method of eliciting personification, which requires participants to attribute human qualities to non-human entities, takes advantage of a naturally occurring means through which (some) people discuss the emotional relationship they have with those entities. Eliciting…

Hunting for Monsters: Visual Arts Curriculum as Agonistic Inquiry

ERIC Educational Resources Information Center

Kalin, Nadine M.; Barney, Daniel T.

2014-01-01

This article explores the possibilities of placing curriculum design in close proximity with participatory contemporary art projects that potentially activate our capacities and willingness to re-vision the future of art education. In this curricular questing we have been drawn toward art that encompasses participatory forms--chiefly relational…

Harnessing the Talents of a "Loose and Baggy Monster."

ERIC Educational Resources Information Center

Myers, Jan; Sacks, Ruth

2001-01-01

Voluntary agencies' responses to change are moving toward use of business tools and techniques. However, these must be considered within the context of the nonprofit sector. Volunteer management could benefit from reciprocal learning--sharing its unique knowledge with the for-profit sector while learning from it. (Contains 38 references.) (SK)

Hollis Sigler: Artist, Teacher, and Activist

ERIC Educational Resources Information Center

Smith-Shank, Deborah L.

2007-01-01

Hollis Sigler was an artist, teacher, and activist. Her works seductively invite us to consider fantasies and challenge to confront the monsters. Sigler's narrative artwork after 1991 focused almost exclusively on issues relating to her and her family's history with breast cancer. It purposefully calls into question the capricious nature of life…

Leadership in the Age of Accountability

ERIC Educational Resources Information Center

Guskey, Thomas R.

2007-01-01

Many school leaders today, not to mention many teachers, view "accountability" as a loathsome political monster. Looming over educators, insensitive to the many problems they face, it wields the carrot of rewards in one hand and the club of sanctions in the other. Some educators even blame accountability for perverting their noble…

Rebuilding and Modeling of a Thermal Radiation Source

DTIC Science & Technology

1994-08-01

ATTN: Charles Brookly L. Meredith 330 Alleghany St. W. Wiederman Frostburg, MD 21532 A. Wong LTC Hassell Transmet Corporation JTCG-ME, LaGrange ATrN...far ABC-Schutz W. Babbage ATTN: W. Rehmann B. Bogartz Technical Library I. Smith Humboltstrale/Postfach 1142 I. Tate 3042 MOnster, Germany M. King

"Cthulhuic Literacy": Teaching Secondary English with a Dose of Lovecraft

ERIC Educational Resources Information Center

Cole, David R.

2014-01-01

This paper suggests how the "weird fiction" of H.P. Lovecraft might be mobilised within secondary English classrooms to examine aspects of visual literacy, literary style, narrative form and intertextuality. The approach that is outlined is characterised, after Lovecraft's famous monster, as a "Cthulhuic literacy" and is…

Portraying Monsters: Framing School Bullying through a Macro Lens

ERIC Educational Resources Information Center

Horton, Paul

2016-01-01

This article critically considers the discourse on school bullying through the conceptual framework of lenses and argues that a macro lens has been utilised by school bullying researchers to bring into focus the characteristics of the individuals involved and the types of actions used. By considering earlier understandings of bullying, the article…

Of Zombies, Monsters and Song: The Third Academic Identities Conference

ERIC Educational Resources Information Center

Grant, Barbara M.; Burford, James; Bosanquet, Agnes; Loads, Daphne

2014-01-01

This essay is a response to the third biennial conference showcasing research and scholarship on academic identities held at the University of Auckland, New Zealand in July 2012. The first conference, with the theme of "academic identities in crisis", was held at the University of Central Lancashire in 2008; the second, "academic…

Slaying the Writing Monsters: Scaffolding Reluctant Writers through a Writing Workshop Approach

ERIC Educational Resources Information Center

Gair, Marina

2015-01-01

Drawing on four years of anecdotal data and student feedback on course evaluations, this paper provides a retrospective account of the author's experience with teacher candidates in an elementary writing instruction course as first-time authors of children's books, in particular focusing on a writing workshop approach as an effective pedagogical…

Do Monsters Dream? Young Children's Understanding of the Fantasy/Reality Distinction

ERIC Educational Resources Information Center

Sharon, Tanya; Woolley, Jacqueline D.

2004-01-01

Young children are often thought to confuse fantasy and reality. This study took a second look at preschoolers' fantasy/reality differentiation. We employed a new measure of fantasy/reality differentiation--a property attribution task--in which children were questioned regarding the properties of both real and fantastical entities. We also…

Slayers of Monster-Watermelons Found in the Mental Health Patch.

ERIC Educational Resources Information Center

Ginter, Earl J.

1989-01-01

Comments on Hershenson, Power, and Seligman's position on mental health counseling theory and also on the evaluation of their article by Blocher. Criticizes Hershenson et al.'s models, claiming they fail to provide a clear image of how theory plays a role in present and future endeavors of mental health counselors. (Author/ABL)

Straw Godzilla: Engaging the Academy and Research Ethics in Artistic Research Projects

ERIC Educational Resources Information Center

Bolt, Barbara; Vincs, Robert

2015-01-01

In Australia, the university ethics approval process is guided by the "National Statement on Ethical Conduct in Human Research." The "National Statement" does not provide a hurdle to be overcome or avoided, nor is it a Godzilla-like monster that must be slain for "truth" to survive. Rather the "National…

Manual for a Summer Reading Program.

ERIC Educational Resources Information Center

Medina, Sue O.

This manual provides suggestions for materials and projects to carry out a summer reading program for children based on a monster theme. The planning process outlined may be used as a "how-to" guide for developing summer reading programs on other themes as well. In addition to general guidelines, the manual provides information on the following…

Tourism and wilderness: dancing with the messy monster

Treesearch

Ralf Buckley

2000-01-01

Currently, tourism offers one of the best prospects for conserving remaining areas of unprotected wilderness in most parts of the world. Tourism produces environmental impacts, and in heavily-visited protected areas these impacts may be a significant threat to conservation values and a major management issue; along with other anthropogenic impacts such as weeds, pests...

The WoW Factor

ERIC Educational Resources Information Center

Demski, Jennifer

2009-01-01

For a growing group of educators, the online role-playing game World of Warcraft, Blizzard Entertainment's massively popular massively multiplayer online role-playing game (MMORPG), is a place to go to relax, network, and discover potential learning strategies-- and slay a few monsters if they get in the way. The online role-playing game World of…

Befriending the Two-Headed Monster: Personal, Social and Emotional Development in Schools in Challenging Times

ERIC Educational Resources Information Center

Harris, Belinda

2008-01-01

Schools in the UK and beyond continue to experience the damaging effects of "top down," "one size fits all" "outcome-based" educational reforms. Educators struggle to meet the dual demands of a punishing performativity- and accountability-driven regime alongside the personal, social, emotional and learning needs of…

Boston University-Chelsea Match Endures

ERIC Educational Resources Information Center

Gehring, John

2004-01-01

When the Tobin Bridge was built in 1950, splitting Chelsea in half and leveling homes in its wake, middle-class families began leaving for greener pastures. The "Iron Monster" became a symbol of the city's decline. By the 1980s, Chelsea was grappling with a familiar litany of urban ills. Only half its students were graduating from high…

Angel on My Shoulder: "Angels in America," "In America," "Monster," "American Idol," and "The Apprentice"

ERIC Educational Resources Information Center

Beck, Bernard

2004-01-01

Culture offers people suggestions for dealing with life's vicissitudes, and people find different suggestions in different cultures. In a multicultural society, they have a variety of alternatives to choose among: ethnicities, regionalisms, lifestyles, religious movements, occupations, hobbies, and more. In American society, the groups that are…

Monster High as a Virtual Dollhouse: Tracking Play Practices across Converging Transmedia and Social Media

ERIC Educational Resources Information Center

Wohlwend, Karen E.

2017-01-01

Background: Today, children play in transmedia franchises that bring together media characters, toys, and everyday consumer goods with games, apps, and websites in complex mergers of childhood cultures, digital literacies, consumer practices, and corporate agendas. Recent research on youth videogames and virtual worlds suggests the productive…

Slaying the Food Monster: Help for Bulimics.

ERIC Educational Resources Information Center

Snyder, Francine; Levy, Karen Gorbitz

1984-01-01

Bulimia is an eating disorder often referred to as the binge-purge syndrome. The bulimic usually functions well at work and often holds a top-level position. Reasons for bulimia include feelings of inadequacy, societal pressures to be thin, and high parental expectations. Low self-esteem is a common characteristic of the bulimic. (RM)

Pearls and pitfalls in the horror cinema.

PubMed

Pascuzzi, R M

1998-01-01

Observations on the neurologic signs and symptoms of Count Dracula, Wolfman, and Frankenstein's Monster are presented as viewed by a specialist in neuromuscular disease. Key clinical features of these horror movie figures illustrate a variety of pearls in the diagnosis of a variety of neurologic disorders, including porphyria, lead poisoning, osteosclerotic myeloma, and myasthenia gravis.

Indigenous Systems within the African-American Community

ERIC Educational Resources Information Center

Marbley, Aretha Faye; Rouson, Leon

2011-01-01

For the African-American family, life ain't been no crystal stair. The African-American family has trotted for over 400 years through a wilderness of racism, poverty, discrimination of all kinds, crossing seas of monsters and forests of demons. Yet, despite the numerous obstacles and attacks that society has mounted against it since slavery, the…

That Way Be Monsters: Myths and Bugaboos about Teaching Personal Writing.

ERIC Educational Resources Information Center

Bloom, Lynn Z.

Many traditionally held academic views of personal writing have myths embedded in them. These myths include: (1) anything written in the first person singular is autobiographical; (2) personal writing can only exist in an expressionist classroom and is often uncritical and unproblematic; (3) student personal writing is a dying genre, and college…

"Battleship Numberline": A Digital Game for Improving Estimation Accuracy on Fraction Number Lines

ERIC Educational Resources Information Center

Lomas, Derek; Ching, Dixie; Stampfer, Eliane; Sandoval, Melanie; Koedinger, Ken

2011-01-01

Given the strong relationship between number line estimation accuracy and math achievement, might a computer-based number line game help improve math achievement? In one study by Rittle-Johnson, Siegler and Alibali (2001), a simple digital game called "Catch the Monster" provided practice in estimating the location of decimals on a…

Pedagogy of the Living Dead: Using Students' Prior Knowledge to Explore Perspective

ERIC Educational Resources Information Center

Nail, Allan

2009-01-01

One reason zombie films are so frightening, and perhaps so popular, is because zombies represent a unique type of monster. Rather than frightening people because they are so alien to the world as people understand it, zombies are horrifying in how closely they resemble people. Zombies are people and represent the potential of zombie…

What Kind of Car Am I? An Exercise to Sensitize Students to Social Class Inequality

ERIC Educational Resources Information Center

Tiemann, Kathleen A.; Davis, Karen; Eide, Terri L.

2006-01-01

Americans are said to have a love affair with cars. Recent magazine articles have addressed automobiles as objects of status and desire and how particular cars have become American icons. The popularity of "Car Talk" on National Public Radio and television shows like "Monster Garage" and "Overhaulin'" also suggest…

Tales of the Supernatural. [Lesson Plan].

ERIC Educational Resources Information Center

2000

Monsters have haunted the literary imagination from earliest times (e.g., the Cyclops, Grendel, etc.), but a particular interest in horror and the Gothic form dates back to the 18th and early 19th centuries. Taking their name from the Gothic architecture that often served as a backdrop to the action, these novels present supernatural events in…

Keep trophy records honest: Identifying whitetail/mule deer hybrids

Treesearch

Jim Heffelfinger; Renee Prive; David Paetkau; Carlos Alcala-Galvan; Roy Lopez; Irv Kornfield; Eldon Buckner

2012-01-01

Humans have always been fascinated by hybrids. Consider such classic monsters as Wolfman, Dracula, and Mothmanor heroes such as Spiderman, Batman, and Catwoman. This trend pre-dates Hollywood by millennia; the "Minotaur" in Greek mythology was half man and half bull. Our fascination with creatures that are half one thing and half another extends to wildlife....

Synchronic Etymologies of Ethnonyms as Cause of the Traditional Belief in Monstrous Races.

ERIC Educational Resources Information Center

Wittlin, Curt J.

A psychological basis for belief in human monsters is provided by the possibility of human aberrations, instinctive human fear and fascination for such prodigies, and the existence of barbaric tales ridiculing foreigners. The role of language as a cause for such belief is investigated, specifically in terms of folk etymologies for more or less…

Frankenstein's Validity Monster: The Value of Keeping Politics and Science Separated

ERIC Educational Resources Information Center

Borsboom, Denny; Wijsen, Lisa D.

2016-01-01

The distinction between facts and moral values is highly desirable: science and politics should keep to their own territories. Traditionally speaking, science can be seen as an ivory tower, which attempts to do its job in isolation of external influences. Politics does not mandate methods of scientific research or standards of justification;…

Perseus

NASA Astrophysics Data System (ADS)

Murdin, P.

2000-11-01

(abbrev. Per, gen. Persei; area 615 sq. deg.) A northern constellation which lies between Andromeda and Auriga, and culminates at midnight in early November. It is named after the hero in Greek mythology who beheaded the Gorgon Medusa and rescued Andromeda from being sacrificed to the sea monster Cetus. Its brightest stars were cataloged by Ptolemy (c. AD 100-175) in the Almagest....

Andromeda

NASA Astrophysics Data System (ADS)

Murdin, P.

2000-11-01

(abbrev. And, gen. Andromedae; area 722 sq. deg.) A northern constellation that lies between Perseus and Pegasus, and culminates at midnight in early October. It is named after the daughter of King Cepheus and Queen Cassiopeia in Greek mythology, who was rescued by Perseus from being sacrificed to the sea monster Cetus, and is usually shown on early celestial charts as a chained maiden. Its brigh...

Monsters, Microbiology and Mathematics: The Epidemiology of a Zombie Apocalypse

ERIC Educational Resources Information Center

Verran, J.; Crossley, M.; Carolan, K.; Jacobs, N.; Amos, M.

2014-01-01

The aim of this learning exercise was to harness current interest in zombies in order to educate audiences about the epidemiology of infectious disease. Participants in the activity were provided with an outbreak scenario, which they then used as the basis of play-based activities. By considering the mode and speed of transmission, size of…

What's Hot, What's Not 2013

ERIC Educational Resources Information Center

Raths, David

2013-01-01

With the exception of a plague of locusts, it seems as if the past five years have thrown every imaginable challenge at IT--from the incredible shrinking budget to BYOD and now the MOOC monster. For those of a superstitious bent, these were probably just appetizers to the crises that will inevitably accompany a year featuring the number 13 (cue…

Ted Hughes: The Development of a Children's Poet

ERIC Educational Resources Information Center

Lockwood, Michael

2009-01-01

This article looks at how Ted Hughes' poetry for children developed over more than 30 years of publication. It traces the movement from his earlier, more conventional rhyming poems, such as "Meet My Folks!" (1961) and "Nessie the Mannerless Monster" (1964), to the mature, free verse "animal poems" for older readers of "Season Songs" (1976c),…

My Tongue on Your Theory: The Bittersweet Reminder of Every-Thing Unnameable

ERIC Educational Resources Information Center

Holmes, Rachel

2016-01-01

Across research in UK Higher Education, the most immanent demands for quality have taken the shape of the Research Assessment Exercise and the Research Excellence Framework (REF). The theorist, Martin, is cautious of the relationship academics have engendered with the process of the REF, asking are we actually creating a Frankenstein monster,…

Disrupting Complacency: Helping Students Find Their Voices through Inquiry, Literature, and Technology

ERIC Educational Resources Information Center

Seglem, Robyn; Bonner, Sarah

2016-01-01

This article highlights an inquiry project in an eighth-grade ELA class in a rural middle school. Using the novel "Monster" by Walter Dean Myers, we encouraged students to form questions relating the text to the larger world. To begin the unit, students participated in three anchor activities over a three-week period. Students blogged…

Videos for Teachers: Successful Teaching Strategies in Middle and High School Classrooms. [CD-ROM].

ERIC Educational Resources Information Center

Teachers Network, New York, NY.

This CD-ROM presents six videos that feature veteran middle and high school teachers in action in their classrooms. Each video offers links to supplemental education resources, including innovative lesson plans. The six videos are: "Monsters and Myths" (a humanities unit for middle school students); "The Bleeding Edge" (a thematic…

The Big Glamorous Monster (or Lady Gaga's Adventures at Sea): Improving Student Writing through Dramatic Approaches in Schools

ERIC Educational Resources Information Center

Lee, Bridget Kiger; Enciso, Patricia

2017-01-01

Drawing on assets-oriented, sociocultural theories of imagination and learning, the authors argue that the improvisational qualities and expanded resources of dramatic approaches to teaching make a positive difference in the quality of and persistence in students' story writing. The authors describe findings from a controlled quasi-experimental…

The FrankensTEin Monster

ERIC Educational Resources Information Center

Blodget, Alden

2009-01-01

In budget meetings trustees tend to dehumanize teachers by looking at them as FTEs (full-time equivalents) instead of as flesh-and-blood people doing impossibly difficult jobs, a transformation that makes it easier to talk about reducing their number. So I created a model to try to humanize the FTE by looking at the number of hours a teacher needs…

Taming the Data Monster: Collecting and Analyzing Classroom Data to Improve Student Progress

ERIC Educational Resources Information Center

Kabot, Susan; Reeve, Christine E.

2016-01-01

Faced with increasing demands for accountability, teachers are having to base their instructional decisions and choice of interventions on data on student performance. This book shows how to make this otherwise daunting task much more manageable by means of case studies and countless evidence-based forms and graphs. Although this book often refers…

Monsters, Bananas and Seaweed: Active Participation and Young Children's Understanding of False Belief.

ERIC Educational Resources Information Center

Szarkowicz, Diane Louise

This study investigated the effect of active participation in a story reading on children's understanding of false belief. Children, ages 38-63 months, were assigned to a participation or non-participation group. Participating children engaged in a book-reading process using puppets to respond to the story. Non-participating children were read the…

The Siren Song That Keeps Us Coming Back: Multicultural Resources for Teaching Classical Mythology.

ERIC Educational Resources Information Center

Earthman, Elise Ann

1997-01-01

Notes the presence of references to classical mythology throughout modern culture, and offers an annotated list of 43 works of contemporary fiction, poetry, and drama that use mythological sources and that can help close the gap between today's students and the gods and goddesses, heroes and monsters of long ago. (SR)

Windigo Ways: Eating and Excess in Louise Erdrich's "The Antelope Wife"

ERIC Educational Resources Information Center

Tharp, Julie

2003-01-01

The cautionary figure of windigo has lurked at the edges of Louise Erdrich's writing since her first collection of poems in 1984. In "The Antelope Wife" it finally emerges into full view. A windigo is defined as a cannibalistic monster set loose by human greed, envy, and jealousy. Traditional Ojibwe windigo stories usually focus on the starving…

This Gun for Hire: The Fascination of Movie Assassins

ERIC Educational Resources Information Center

Beck, Bernard

2005-01-01

The main characters in a movie can serve individuals in many different ways, but the usual way is to appear good. In whatever form, stories of individuals are a useful part of popular culture when they offer models of how individuals might save themselves or be saved. However, there are other ways. Villains, monsters, and enemies can be at the…

Decolonizing Constructions of Childhood and History: Interrupting Narratives of Avoidance to Children's Questions about Social Injustice

ERIC Educational Resources Information Center

Diversi, Marcelo; Moreira, Claudio

2012-01-01

Together, we the authors, wonder, write, imagine, suffer, and criticize the support of the Belo Monte Monster Dam in the Rio Xingu, in the heart of the Amazon, by two of our personal heroes and fellow Brazilians: Lula, former president and iconic founder of the Workers' Party, and, Dilma Rousseff, our presidenta guerilheira. Using our…

The Monster Sound Pipe

ERIC Educational Resources Information Center

Ruiz, Michael J.; Perkins, James

2017-01-01

Producing a deep bass tone by striking a large 3 m (10 ft) flexible corrugated drainage pipe immediately grabs student attention. The fundamental pitch of the corrugated tube is found to be a semitone lower than a non-corrugated smooth pipe of the same length. A video (https://youtu.be/FU7a9d7N60Y) of the demonstration is included, which…

Scaring the Monster Away: What Children Know about Managing Fears of Real and Imaginary Creatures

ERIC Educational Resources Information Center

Sayfan, Liat; Lagattuta, Kristin Hansen

2009-01-01

Children around 4, 5, and 7 years old (N = 48) listened to scenarios depicting a child alone or accompanied by another person (mother, father, friend) who encounters an entity that looks like a real or an imaginary fear-inducing creature. Participants predicted and explained each protagonist's fear intensity and suggested coping strategies.…

Bodacious Berry, Potency Wood and the Aging Monster: Gender and Age Relations in Anti-Aging Ads

ERIC Educational Resources Information Center

Calasanti, Toni

2007-01-01

This paper situates age discrimination within a broader system of age relations that intersects with other inequalities, and then uses that framework to analyze internet advertisements for the anti-aging industry. Such ads reinforce age and gender relations by positing old people as worthwhile only to the extent that they look and act like those…

Incarceration, Identity Formation, and Race in Young Adult Literature: The Case of "Monster" versus "Hole in My Life"

ERIC Educational Resources Information Center

Engles, Tim; Kory, Fern

2013-01-01

English teachers can heighten awareness of the factors that influence racial disparities in arrest and incarceration rates by working with literature that dramatizes the differences between white and nonwhite experiences within the US criminal justice system. Tim Engles and Fern Kory demonstrate some methods for doing so by juxtaposing two…

A Derridaean Reading of the Zone of Proximal Development (ZPD): The Monster in the Play of "Differance"

ERIC Educational Resources Information Center

Flint, Kevin J.

2009-01-01

The institutional machine of contemporary activity theory currently appears to be constrained by centring on the structure of mediated activity first voiced by Vygotsky. As a centring, such a principle, it is argued, continually restores the equilibrium of the institutional machine in alignment with its possible development in the polysemy of…

Historical Research and Narrative Inquiry: Striking Similarities, Notable Differences

ERIC Educational Resources Information Center

Craig, Cheryl J.

2005-01-01

When Theseus sailed from Athens to the island of Crete to slay the Minotaur, a fearsome monster whose food was human flesh and whose home was the labyrinth, Ariadne, the daughter of the Cretan King Minos, gave her new found love, Theseus, a ball of thread to assist him in maneuvering his way through the great maze of winding passages. "Unwind it…

Brief Report: Effects of Tact Training on Emergent Intraverbal Vocal Responses in Adolescents with Autism

ERIC Educational Resources Information Center

May, Richard J.; Hawkins, Emma; Dymond, Simon

2013-01-01

The present study evaluated the emergence of intraverbal responses following tact training with three adolescents diagnosed with autism spectrum disorders. Participants were taught to tact the name of a cartoon character (e.g., "What is the name of this monster?" ["Simon"]) and that character's preferred food (e.g., "What food does this monster…

"American Chimera: The Ever-Present Domination of Whiteness, Patriarchy, and Capitalism…A Parable"

ERIC Educational Resources Information Center

Montoya, Roberto; Matias, Cheryl E.; Nishi, Naomi W. M.; Sarcedo, Geneva L.

2016-01-01

In Greek mythology, the Chimera is a fire-breathing monster with three heads: one of a lion, one of a horned goat, and one of a powerful dragon. Of similar construction is the presence of three structures in US society, whiteness, patriarchy, and capitalism, which are overwhelmingly represented, valued, and espoused when examining areas of…

Knowledge and Skill Requirements for Marketing Jobs in the 21st Century

ERIC Educational Resources Information Center

Schlee, Regina Pefanis; Harich, Katrin R.

2010-01-01

This study examines the skills and conceptual knowledge that employers require for marketing positions at different levels ranging from entry- or lower-level jobs to middle- and senior-level positions. The data for this research are based on a content analysis of 500 marketing jobs posted on Monster.com for Atlanta, Chicago, Los Angeles, New York…

Vanquishing the Hydra-Headed Monster: The Struggle To Establish the Classical Curriculum in New South Wales Schools, 1788-1850.

ERIC Educational Resources Information Center

Mooney, Christopher

1997-01-01

Gives a detailed examination of classical education in New South Wales prior to 1850. Describes how the emphasis on teaching the classical tradition, prevalent in British educational institutions, ensured its presence in the new colonial schools, but not with the same priority due to the need for more utilitarian subjects. (DSK)

The Monster and Lover?Girl: Mapping Complex Relations in Preschool Children's Digital Video Productions

ERIC Educational Resources Information Center

McClure, Marissa

2013-01-01

In this article, I propose that research which focuses on young children's experiences with the interactivity of new media not only furthers findings about young children's digital lives but also enriches the conclusion that children's engagement with artmaking--in general and in traditional ways--is richly complex, affective, and…

The Monsters in My Head: Posttraumatic Stress Disorder and the Child Survivor of Sexual Abuse

ERIC Educational Resources Information Center

Putman, Stacie E.

2009-01-01

Posttraumatic stress disorder (PTSD) is 1 of several possible outcomes of child sexual victimization. There is a growing body of literature regarding the prevalence of PTSD among children who have been sexually victimized. Using specific case examples, this article looks at the nature and scope of the problem, diagnostic criteria according to the…

Defense Against National Vulnerabilities in Public Data

DTIC Science & Technology

2017-02-28

ingestion of subscription based precision data sources ( Business Intelligence Databases, Monster, others).  Flexible data architecture that allows for... Architecture Objective: Develop a data acquisition architecture that can successfully ingest 1,000,000 records per hour from up to 100 different open...data sources.  Developed and operate a data acquisition architecture comprised of the four following major components:  Robust website

Always Feed the Clowns and Other Tips for Building Better Partnerships between School Librarians and Providers of Educational Programs

ERIC Educational Resources Information Center

Edwards, Jason

2015-01-01

Jason Edwards travels to schools and libraries across the nation performing educational enrichment programs, such as his Monster Hunt Library Skills-Building Adventure Program, for librarians and students. In this article, he shares tips that he has gleaned that may help librarian/programmer partnerships function more smoothly. Three of the…

History effects in visual search for monsters: search times, choice biases, and liking.

PubMed

Chetverikov, Andrey; Kristjansson, Árni

2015-02-01

Repeating targets and distractors on consecutive visual search trials facilitates search performance, whereas switching targets and distractors harms search. In addition, search repetition leads to biases in free choice tasks, in that previously attended targets are more likely to be chosen than distractors. Another line of research has shown that attended items receive high liking ratings, whereas ignored distractors are rated negatively. Potential relations between the three effects are unclear, however. Here we simultaneously measured repetition benefits and switching costs for search times, choice biases, and liking ratings in color singleton visual search for "monster" shapes. We showed that if expectations from search repetition are violated, targets are liked to be less attended than otherwise. Choice biases were, on the other hand, affected by distractor repetition, but not by target/distractor switches. Target repetition speeded search times but had little influence on choice or liking. Our findings suggest that choice biases reflect distractor inhibition, and liking reflects the conflict associated with attending to previously inhibited stimuli, while speeded search follows both target and distractor repetition. Our results support the newly proposed affective-feedback-of-hypothesis-testing account of cognition, and additionally, shed new light on the priming of visual search.

Monster potential meets potential monster: pros and cons of deploying genetically modified microalgae for biofuels production.

PubMed

Flynn, K J; Mitra, A; Greenwell, H C; Sui, J

2013-02-06

Biofuels production from microalgae attracts much attention but remains an unproven technology. We explore routes to enhance production through modifications to a range of generic microalgal physiological characteristics. Our analysis shows that biofuels production may be enhanced ca fivefold through genetic modification (GM) of factors affecting growth rate, respiration, photoacclimation, photosynthesis efficiency and the minimum cell quotas for nitrogen and phosphorous (N : C and P : C). However, simulations indicate that the ideal GM microalgae for commercial deployment could, on escape to the environment, become a harmful algal bloom species par excellence, with attendant risks to ecosystems and livelihoods. In large measure, this is because an organism able to produce carbohydrate and/or lipid at high rates, providing stock metabolites for biofuels production, will also be able to attain a stoichiometric composition that will be far from optimal as food for the support of zooplankton growth. This composition could suppress or even halt the grazing activity that would otherwise control the microalgal growth in nature. In consequence, we recommend that the genetic manipulation of microalgae, with inherent consequences on a scale comparable to geoengineering, should be considered under strict international regulation.

Monster potential meets potential monster: pros and cons of deploying genetically modified microalgae for biofuels production

PubMed Central

Flynn, K. J.; Mitra, A.; Greenwell, H. C.; Sui, J.

2013-01-01

Biofuels production from microalgae attracts much attention but remains an unproven technology. We explore routes to enhance production through modifications to a range of generic microalgal physiological characteristics. Our analysis shows that biofuels production may be enhanced ca fivefold through genetic modification (GM) of factors affecting growth rate, respiration, photoacclimation, photosynthesis efficiency and the minimum cell quotas for nitrogen and phosphorous (N : C and P : C). However, simulations indicate that the ideal GM microalgae for commercial deployment could, on escape to the environment, become a harmful algal bloom species par excellence, with attendant risks to ecosystems and livelihoods. In large measure, this is because an organism able to produce carbohydrate and/or lipid at high rates, providing stock metabolites for biofuels production, will also be able to attain a stoichiometric composition that will be far from optimal as food for the support of zooplankton growth. This composition could suppress or even halt the grazing activity that would otherwise control the microalgal growth in nature. In consequence, we recommend that the genetic manipulation of microalgae, with inherent consequences on a scale comparable to geoengineering, should be considered under strict international regulation. PMID:24427510

Monsters, Monkeys, & Mandalas: Art Therapy with Children Experiencing the Effects of Trauma and Fetal Alcohol Spectrum Disorder (FASD)

ERIC Educational Resources Information Center

Gerteisen, June

2008-01-01

Fetal Alcohol Spectrum Disorder (FASD) is an umbrella term that describes the range of effects associated with the diagnoses of Fetal Alcohol Effects (FAE) and Fetal Alcohol Syndrome (FAS). FASD itself is not a diagnosis, but rather encompasses a wide range of symptomatic behaviors that occur in an individual whose mother drank alcohol during…

Prisoners of Childhood? Child Abuse and the Development of Heroes and Monsters in "Ender's Game"

ERIC Educational Resources Information Center

Gross, Melissa

2007-01-01

Alice Miller's work provides a theoretical framework to assess the effects of child abuse and its relationship to the development of creativity, hatred, and violence in the novel "Ender's Game." Analysis focuses on the extent to which children are manipulated in order to meet the needs of adults, the presence of behaviors such as the repression of…

"Your Vagina Is Not Supposed to Be This Scary Monster": Young Heterosexual Women's Recommendations for Improving Sexual Satisfaction and Implications for Sexuality Education

ERIC Educational Resources Information Center

Blunt-Vinti, Heather D.; Stokowski, Sarah E.; Bouza, Brooke M.

2018-01-01

Sexual satisfaction is an important component of sexuality, yet rarely discussed in sexuality education. In an effort to better understand young adult women's experiences and thoughts about sexual pleasure and satisfaction, we conducted interviews with heterosexual young women (N = 30, ages 18-25) attending college, asking their recommendations on…

The gene complement of the ancestral bilaterian - was Urbilateria a monster?

PubMed Central

2009-01-01

Expressed sequence tag analyses of the annelid Pomatoceros lamarckii, recently published in BMC Evolutionary Biology, are consistent with less extensive gene loss in the Lophotrochozoa than in the Ecdysozoa, but it would be premature to generalize about patterns of gene loss on the basis of the limited data available. See research article http://www.biomedcentral.com/1471-2148/9/240. PMID:19939290

"The Trampoline Tree and the Swamp Monster with 18 Heads": Outdoor Play in the Foundation Stage and Foundation Phase

ERIC Educational Resources Information Center

Waller, Tim

2007-01-01

This paper considers pedagogy and outdoor play in the early years. The particular focus is on the specific features and benefits of outdoor play in the Foundation Stage (England) and Foundation Phase (Wales). The paper will draw on current international literature and evidence from outdoor learning constructed in an ongoing research project in two…

Microarray analysis of a salamander hopeful monster reveals transcriptional signatures of paedomorphic brain development

PubMed Central

2010-01-01

Background The Mexican axolotl (Ambystoma mexicanum) is considered a hopeful monster because it exhibits an adaptive and derived mode of development - paedomorphosis - that has evolved rapidly and independently among tiger salamanders. Unlike related tiger salamanders that undergo metamorphosis, axolotls retain larval morphological traits into adulthood and thus present an adult body plan that differs dramatically from the ancestral (metamorphic) form. The basis of paedomorphic development was investigated by comparing temporal patterns of gene transcription between axolotl and tiger salamander larvae (Ambystoma tigrinum tigrinum) that typically undergo a metamorphosis. Results Transcript abundances from whole brain and pituitary were estimated via microarray analysis on four different days post hatching (42, 56, 70, 84 dph) and regression modeling was used to independently identify genes that were differentially expressed as a function of time in both species. Collectively, more differentially expressed genes (DEGs) were identified as unique to the axolotl (n = 76) and tiger salamander (n = 292) than were identified as shared (n = 108). All but two of the shared DEGs exhibited the same temporal pattern of expression and the unique genes tended to show greater changes later in the larval period when tiger salamander larvae were undergoing anatomical metamorphosis. A second, complementary analysis that directly compared the expression of 1320 genes between the species identified 409 genes that differed as a function of species or the interaction between time and species. Of these 409 DEGs, 84% exhibited higher abundances in tiger salamander larvae at all sampling times. Conclusions Many of the unique tiger salamander transcriptional responses are probably associated with metamorphic biological processes. However, the axolotl also showed unique patterns of transcription early in development. In particular, the axolotl showed a genome-wide reduction in mRNA abundance across loci, including genes that regulate hypothalamic-pituitary activities. This suggests that an axolotls failure to undergo anatomical metamorphosis late in the larval period is indirectly associated with a mechanism(s) that acts earlier in development to broadly program transcription. The axolotl hopeful monster provides a model to identify mechanisms of early brain development that proximally and ultimately affect the expression of adult phenotypes. PMID:20584293

First NATO/SIBCA Exercise in Sampling of Chemical Warfare Agents (Eerste NATO/SIBCA-oefening in monstername van chemische strijdmiddelen).

DTIC Science & Technology

1998-01-01

TNO-rapport PML1997-A81 Eerste NATO/SIBCA-oefening in monster- name van chemische strijdmiddelen TNO Prins Maurits Laboratorium Lange Kleiweg...27 Aantal pagina’s : 53 (incl. bijlagen, excl. RDP & distributielijst) Aantal bijlagen : 4 TNO Prins Maurits Laboratorium is onderdeel...van de hoofdgroep TNO Defensieonderzoek waartoe verder behoren: TNO Fysisch en Elektronisch Laboratorium TNO Technische Menskunde Nederlandse

National Science Resources Center Project to Improve Science Teaching in Elementary Schools. Appendix D. Science for Children, an Agenda for Action. Appendix E. Science for Children, Resources for Teachers

DTIC Science & Technology

1988-12-01

activities in chemistry tivities for the Visually Impaired/Science and physics: The Acid Test, How Dense?, The Cookie Monster, and The Sugar...baking powder. assembling a Grade(s): 3,4,5,6 gas generator, and learning how dough rises. Adult supervision is necessary for $6.95 these activities. 86

Geometric interpretation of vertex operator algebras.

PubMed Central

Huang, Y Z

1991-01-01

In this paper, Vafa's approach to the formulation of conformal field theories is combined with the formal calculus developed in Frenkel, Lepowsky, and Meurman's work on the vertex operator construction of the Monster to give a geometric definition of vertex operator algebras. The main result announced is the equivalence between this definition and the algebraic one in the sense that the categories determined by these definitions are isomorphic. PMID:11607240

LP-LPA: A link influence-based label propagation algorithm for discovering community structures in networks

NASA Astrophysics Data System (ADS)

Berahmand, Kamal; Bouyer, Asgarali

2018-03-01

Community detection is an essential approach for analyzing the structural and functional properties of complex networks. Although many community detection algorithms have been recently presented, most of them are weak and limited in different ways. Label Propagation Algorithm (LPA) is a well-known and efficient community detection technique which is characterized by the merits of nearly-linear running time and easy implementation. However, LPA has some significant problems such as instability, randomness, and monster community detection. In this paper, an algorithm, namely node’s label influence policy for label propagation algorithm (LP-LPA) was proposed for detecting efficient community structures. LP-LPA measures link strength value for edges and nodes’ label influence value for nodes in a new label propagation strategy with preference on link strength and for initial nodes selection, avoid of random behavior in tiebreak states, and efficient updating order and rule update. These procedures can sort out the randomness issue in an original LPA and stabilize the discovered communities in all runs of the same network. Experiments on synthetic networks and a wide range of real-world social networks indicated that the proposed method achieves significant accuracy and high stability. Indeed, it can obviously solve monster community problem with regard to detecting communities in networks.

A monster in the Milky Way

NASA Image and Video Library

2017-12-08

This image shows the star-studded center of the Milky Way towards the constellation of Sagittarius. The crowded center of our galaxy contains numerous complex and mysterious objects that are usually hidden at optical wavelengths by clouds of dust — but many are visible here in these infrared observations from Hubble. However, the most famous cosmic object in this image still remains invisible: the monster at our galaxy’s heart called Sagittarius A*. Astronomers have observed stars spinning around this supermassive black hole (located right in the center of the image), and the black hole consuming clouds of dust as it affects its environment with its enormous gravitational pull. Infrared observations can pierce through thick obscuring material to reveal information that is usually hidden to the optical observer. This is the best infrared image of this region ever taken with Hubble, and uses infrared archive data from Hubble’s Wide Field Camera 3, taken in September 2011. Credit: NASA, ESA, and G. Brammer NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Museum Monsters and Victorious Viruses: Improving Public Understanding of Emerging Biomedical Research

PubMed Central

Diamond, Judy; Jee, Benjamin; Matuk, Camilla; McQuillan, Julia; Spiegel, Amy N.; Uttal, David

2015-01-01

Although microbes directly impact everyone's health, most people have limited knowledge about them. In this article, we describe a museum and media public education campaign aimed at helping diverse audiences better understand emerging knowledge about microbes and infectious disease. Funded primarily by the Science Education Partnership (SEPA) program of the National Institutes of Health, this campaign involved crosscutting programs designed to extend impacts throughout a broad public audience. PMID:26392634

Meteor Beliefs Project: Meteoric imagery in SF, Part II - H. P. Lovecraft's The Colour Out Of Space

NASA Astrophysics Data System (ADS)

McBeath, Alastair; Gheorghe, Andrei Dorian

2005-12-01

A brief biography of American horror-fiction writer H. P. Lovecraft (1890-1937) precedes details from his story `The Colour Out Of Space', concerning a deadly life-form brought to Earth in a meteorite. This allows a comparison with details from the 1965 film derived from this tale, `Die, Monster, Die!', featuring the great horror actor Boris Karloff in one of his last, best roles.

Sea monsters & whirlpools: Navigating between examination and reflection in medical education.

PubMed

Hodges, Brian David

2015-03-01

The 16th International Ottawa Conference/Canadian Conference on Medical Education (2014) featured a keynote deconstructing the rising discourse of competence-as-reflection in medical education. This paper, an elaborated version of the presentation, is an investigation into the theoretical roots of the diverse forms of reflective practice that are being employed by medical educators. It also raises questions about the degree to which any of these practices is compatible with assessment.

USSR Report, Political and Sociological Affairs.

DTIC Science & Technology

1984-03-13

capitalism is doomed and has no future, and the more convicing and impressive is the march of true socialism, the more intense becomes the heat of...and curse those base monsters- socialists." It is true that soon the trickery of this sham student of eastern magicians was exposed. However, her...spiritual food. Over 30 million Americans believe in "miracles" of astrology and 1,200 newspapers print horoscopes . According to the American press

Dragon-Kings, Black-Swans and Prediction (Invited)

NASA Astrophysics Data System (ADS)

Sornette, D.

2010-12-01

Extreme fluctuations or events are often associated with power law statistics. Indeed, it is a popular belief that "wild randomness'' is deeply associated with distributions with power law tails characterized by small exponents. In other words, power law tails are often seen as the epitome of extreme events (the "Black Swan'' story). Here, we document in very different systems that there is life beyond power law tails: power laws can be superseded by "dragon-kings'', monster events that occur beyond (or changing) the power law tail. Dragon-kings reveal hidden mechanisms that are only transiently active and that amplify the normal fluctuations (often described by the power laws of the normal regime). The goal of this lecture is to catalyze the interest of the community of geophysicists across all fields of geosciences so that the "invisible gorilla" fallacy may be avoided. Our own research illustrates that new statistics or representation of data are often necessary to identify dragon-kings, with strategies guided by the underlying mechanisms. Paradoxically, the monsters may be ignored or hidden by the use of inappropriate analysis or statistical tools that amount to cut a mamooth in small pieces, so as to lead to the incorrect belief that only mice exist. In order to stimulate further research, we will document and discuss the dragon-king phenomenon on the statistics of financial losses, economic geography, hydrodynamic turbulence, mechanical ruptures, avalanches in complex heterogeneous media, earthquakes, and epileptic seizures. The special status of dragon-kings open a new research program on their predictability, based on the fact that they belong to a different class of their own and express specific mechanisms amplifying the normal dynamics via positive feedbacks. We will present evidence of these claims for the predictions of material rupture, financial crashes and epileptic seizures. As a bonus, a few remarks will be offered at the end on how the dragon-king phenomenon allows us to understand the present World financial crisis as underpinned in two decades of successive financial and economic bubbles, inflating the mother of all bubbles with new monster dragon-kings at the horizon. The consequences in terms of a new "normal" are eye-opening. Ref: D. Sornette, Dragon-Kings, Black Swans and the Prediction of Crises, International Journal of Terraspace Science and Engineering 1(3), 1-17 (2009) (http://arXiv.org/abs/0907.4290) and (http://ssrn.com/abstract=1470006)

Representation of the serial killer on the Italian Internet.

PubMed

Villano, P; Bastianoni, P; Melotti, G

2001-10-01

The representation of serial killers was examined from the analysis of 317 Web pages in the Italian language to study how the psychological profiles of serial killers are described on the Italian Internet. The correspondence analysis of the content of these Web pages shows that in Italy the serial killer is associated with words such as "monster" and "horror," which suggest and imply psychological perversion and aberrant acts. These traits are peculiar for the Italian scenario.

Structure-Function Relationship of Hydrophiidae Postsynaptic Neurotoxins

DTIC Science & Technology

1992-03-11

monster venom concluded that gila toxin is an arginine esterase with kallikrein-like activity causing lethality and gyration in mice. However, it is not a...Fractionation of Lapemis venom ............ 49 Fig 3-4 Fractionation of Gila Toxin ............... 50 Fig 3-5 Fibrinogenolytic Activity of Gila toxin...Sequence of 8 kD Fragment of Lapemis PLA ..... 8 7 Tab 3-9 Enzyme Activity of Native and Metal Pl . 88 Tab 3-10 Amino Acid Analysis of Lapemis 9 kD prorein

Research and application of multi-agent genetic algorithm in tower defense game

NASA Astrophysics Data System (ADS)

Jin, Shaohua

2018-04-01

In this paper, a new multi-agent genetic algorithm based on orthogonal experiment is proposed, which is based on multi-agent system, genetic algorithm and orthogonal experimental design. The design of neighborhood competition operator, orthogonal crossover operator, Son and self-learning operator. The new algorithm is applied to mobile tower defense game, according to the characteristics of the game, the establishment of mathematical models, and finally increases the value of the game's monster.

Studies in Battle Command

DTIC Science & Technology

1995-01-01

gulars i ttl . te i ewa, le nce r ss i a enstown. enstown, h d nt f t pture orge. tely, l ander t ri , odore ac uncey, ed erate. id...triumph, or another such attack, would finally smash us, and then will come the monster catastrophe--a horrible compound of Afghanistan and Corunna...compromise or compound of all of these.“5 On I6 May, while Pemberton vacillated (much to the disgust of his subordi- nates), Grant simplified the

Monsters of Muenster: Lessons from the Apocalyptic Narrative of the Anabaptist Kingdom

DTIC Science & Technology

2017-12-01

physical; it could be a psychological separation created by social tension and suspicion of non-members.58 Tension with the surrounding society based...injustice against divine moral standards and at calling God’s people to stand up against these injustices with an all- powerful God behind them.102...has the potential to have a conflict with the wider society . Apocalyptic groups turn to violence when they believe their violent acts are in

Preparation and Analysis of Samples for the Third Round Robin Verification Exercise

DTIC Science & Technology

1992-07-01

Hooge 34 Lid instituuts Advies Raad PML Prof. dr. U.A. Th. Brinkman 35 Directeur van het Medisch Biologisch Laboratorium TNO Proft dr. W.R.F. Notten 36...1991 werd uitgevoerd, heeft het Prins Maurits Laboratorium TNO de monsters aangemaakt die bestonden uit rubber, verf en beton. Deze materialen, die...Maurits Laboratorium TNO Chemische Research Prof. dr. G. Dijksrra 10 HBur. NBC-DMKIJOMATIKIO In. A.A.M. Slagveer 11 Lid van de Contact Cominissie NBC

Common Violations of the United States Code in Economic Crime Investigations. The Fraud, Waste and Abuse Monster.

DTIC Science & Technology

1983-11-15

person- nel in understanding the elements of the offense and the evidence necessary to establish or negate probable cause. For the benefit of OCONUS...gift, favor, entertainment, hospitality, transportation, loan, or other tangible benefit for which less than fair market value is paid. c...influenced. He may even refuse the offer, yet the offense is complete. Nor need the thing of value personally benefit the public official. However, the

World Epidemiology Review, Number 110.

DTIC Science & Technology

1978-10-18

Campaign Against Rhinoceros Beetle (DAILY NATION, 26 Sep 78) 43 LAOS Briefs Nong Bok Pest Eradication 44 Meuang Chanthabouli Pest Eradication...CAMPAIGN AGAINST RHINOCEROS BEETLE Nairobi DAILY NATION in English 26 Sep 78 p 5 [Text] A TINY pest hos become a big problem at the Coast. The... Rhinoceros Beetle (that’s it pictured on the right) is, in its own small way, trying to cause as much damage as the monster it’s named after is sometimes

Mary Wollstonecraft Shelley's Frankenstein, or the modern Prometheus: a psychological study of unrepaired shame.

PubMed

Severino, Sally K; Morrison, Nancy K

2013-01-01

Mary Wollstonecraft Shelley's modern Prometheus shows us the eternal punishment of unrepaired shame--eternal entrapment within the shame triangle of victim, perpetrator and rescuer. This paper describes how Shelley's insight--that lack of love creates a monster living in shame--is being confirmed by neuroscience and how this is exemplified in two characters--the creature and Victor Frankenstein. Additionally, it delineates how pastoral counselors can help those suffering from unrepaired shame

FRankenstein becomes a cyborg: the automatic recombination and realignment of fold recognition models in CASP6.

PubMed

Kosinski, Jan; Gajda, Michal J; Cymerman, Iwona A; Kurowski, Michal A; Pawlowski, Marcin; Boniecki, Michal; Obarska, Agnieszka; Papaj, Grzegorz; Sroczynska-Obuchowicz, Paulina; Tkaczuk, Karolina L; Sniezynska, Paulina; Sasin, Joanna M; Augustyn, Anna; Bujnicki, Janusz M; Feder, Marcin

2005-01-01

In the course of CASP6, we generated models for all targets using a new version of the "FRankenstein's monster approach." Previously (in CASP5) we were able to build many very accurate full-atom models by selection and recombination of well-folded fragments obtained from crude fold recognition (FR) results, followed by optimization of the sequence-structure fit and assessment of alternative alignments on the structural level. This procedure was however very arduous, as most of the steps required extensive visual and manual input from the human modeler. Now, we have automated the most tedious steps, such as superposition of alternative models, extraction of best-scoring fragments, and construction of a hybrid "monster" structure, as well as generation of alternative alignments in the regions that remain poorly scored in the refined hybrid model. We have also included the ROSETTA method to construct those parts of the target for which no reasonable structures were generated by FR methods (such as long insertions and terminal extensions). The analysis of successes and failures of the current version of the FRankenstein approach in modeling of CASP6 targets reveals that the considerably streamlined and automated method performs almost as well as the initial, mostly manual version, which suggests that it may be a useful tool for accurate protein structure prediction even in the hands of nonexperts. 2005 Wiley-Liss, Inc.

Late Jurassic low latitude of Central Iran: paleogeographic and tectonic implications

NASA Astrophysics Data System (ADS)

Mattei, Massimo; Muttoni, Giovanni; Cifelli, Francesca

2014-05-01

The individual blocks forming present-day Central Iran are now comprised between the Zagros Neo-Tethys suture to the south and the Alborz Palaeo-Tethys suture to the north. At the end of the Palaeozoic, the Iranian blocks rifted away from the northern margin of Gondwana as consequence of the opening of the Neo-Tethys, and collided with Eurasia during the Late Triassic, giving place to the Eo-Cimmerian orogeny. From then on, the Iranian block(s) should have maintained European affinity. Modern generations of apparent polar wander paths (APWPs) show the occurrence in North American and African coordinates of a major and rapid shift in pole position (=plate shift) during the Middle-Late Jurassic. This so-called monster polar shift is predicted also for Eurasia from the North Atlantic plate circuit, but Jurassic data from this continent are scanty and problematic. Here, we present paleomagnetic data from the Kimmeridgian-Tithonian (Upper Jurassic) Garedu Formation of Iran. Paleomagnetic component directions of primary (pre-folding) age indicate a paleolatitude of deposition of 10°N ± 5° that is in excellent agreement with the latitude drop predicted for Iran from APWPs incorporating the Jurassic monster polar shift. We show that paleolatitudes calculated from these APWPs, used in conjunction with simple zonal climate belts, better explain the overall stratigraphic evolution of Iran during the Mesozoic.

Prevalence of Musculoskeletal Symptoms, Excessive Daytime Sleepiness, and Fatigue in the Crewmembers of a U.S. Navy Ship

DTIC Science & Technology

2015-04-01

C., & Oria, M. (Eds.). (2008). Use of dietary supplements by military personnel. Washington, D.C.: National Academies Press. Gregg, M. A...the workers is job stress (i.e., the harmful physical and emotional responses that occur when the requirements of the job do not match the...Monster 160 Red Bull 80 Rock Star 160 NOS 250 5-Hour Energy 200 AMP 75 Sparks 170 No Fear 174 The preworkout supplements reported by two

Cryptozoology Society

NASA Astrophysics Data System (ADS)

Richman, Barbara T.

Reports of Loch Ness monsters, Bigfoot, and the Yeti spring u p from time to time, sparking scientific controversy about the veracity of these observations. Now an organization has been established to help cull, analyze, and disseminate information on the alleged creatures. The International Society of Cryptozoology, formed at a January meeting at the U.S. National Museum of Natural History of the Smithsonian Institution, will serve as the focal point for the investigation, analysis, publication, and discussion of animals of unexpected form or size or of unexpected occurrences in time or space.

Dual-Hierarchy Graph Method for Object Indexing and Recognition

DTIC Science & Technology

2014-07-01

from examples would be too late for the prey. Mythical monsters in movies or cartoons can look quite scary even though we have never seen their...uniform, at 25 blocks per parent, but depends on the number of SIFT features in the parent blocks. If we have more features we create more children for...method mentioned above to these descriptors to derive the 3D structure and pose of the object. In effect , we replace the previous “spatial verification

KSC-04PD-0606

NASA Technical Reports Server (NTRS)

2004-01-01

KENNEDY SPACE CENTER, FLA. -- Looking like a prehistoric monster crunching on its prey, the Caterpillar excavator and 48-inch shear attachment tear down Launch Umbilical Tower No. 1 (LUT-1) stored in the Industrial Area of KSC. The LUT-1 was part of the launch system used for Apollo-Saturn V, launching Apollo 8, Apollo 11, Skylab manned missions and the Apollo-Soyuz Test Project. The shear is one used in the deconstruction of the Twin Towers in New York City after 9/11.

KSC-04PD-0605

NASA Technical Reports Server (NTRS)

2004-01-01

KENNEDY SPACE CENTER, FLA. -- Looking like a prehistoric monster crunching on its prey, the Caterpillar excavator and 48-inch shear attachment tear down Launch Umbilical Tower No. 1 (LUT-1) stored in the Industrial Area of KSC. The LUT-1 was part of the launch system used for Apollo-Saturn V, launching Apollo 8, Apollo 11, Skylab manned missions and the Apollo-Soyuz Test Project. The shear is one used in the deconstruction of the Twin Towers in New York City after 9/11.

KSC-04PD-0609

NASA Technical Reports Server (NTRS)

2004-01-01

KENNEDY SPACE CENTER, FLA. -- Looking like a prehistoric monster crunching on its prey, the Caterpillar excavator and 48-inch shear attachment tear down Launch Umbilical Tower No. 1 (LUT-1) stored in the Industrial Area of KSC. The LUT-1 was part of the launch system used for Apollo-Saturn V, launching Apollo 8, Apollo 11, Skylab manned missions and the Apollo-Soyuz Test Project. The shear is one used in the deconstruction of the Twin Towers in New York City after 9/11.

The bear that never was

USGS Publications Warehouse

Smith, T.S.; Amstrup, Steven C.; Herrero, Stephen

2005-01-01

From campfire stories to sensational books detailing gory attacks, Alaska's bears have long been maligned as deadly marauders capable of acquiring a taste for human flesh. Tall tales make for good storytelling but force bad reputations on the bears. When myth is compared to fact, the three North American's leading bear experts show that Alaska's three bear species are not the huge, unpredictable monsters they often are made out to be. Here, Smith, Amstrup, and Herrero examine the conventional wisdom people often hear regarding bears in the Great Land.

Proceedings of the NASTRAN (Tradename) Users’ Colloquium (18th) Held in Portland, Oregon on 23-27 April 1990

DTIC Science & Technology

1990-04-01

Maxwell (Texas A&M University-) 4. ACCURACY OF THE QUAD& THICK SHELL ELEMENT ’........... .. 3.0 by William R. Case, Tiffany D. Bowles, Al ia K. Croft and...Computer Literacy: Mainframe Monsters and Pacman. Symposium on Advances and Trends in Structures and Dynamics, Washington, D.C., October 1984. 4. Woodward...No. 1, 1985. 5. Wilson, E.L., and M. Holt: CAL-80-Computer Assisted Learning of Structural Engineering. Symposium on Advances and Trends in

BUILDING THE FORCE OF THE FUTURE: A NEW CALL TO ATTRACT, HIRE AND RETAIN THE BEST AND BRIGHTEST TO AIR FORCE CIVIL SERVICE

DTIC Science & Technology

2015-10-25

Graduation Requirements Advisors: Dr . Gregory F. Intoccia and Dr . Patricia Lessane Maxwell Air Force Base, Alabama 25 October 2015 DISTRIBUTION A...support while I was diverting much of my free time and attention to this graduate program. I appreciate my research advisors Dr . Greg Intoccia and Dr ...underutilized USAJOBS, the federal government job search engine, as compare to LinkedIn , Career Builders and Monster. Only 8.8 percent of the

KSC-04pd0609

NASA Image and Video Library

2004-03-24

KENNEDY SPACE CENTER, FLA. -- Looking like a prehistoric monster crunching on its prey, the Caterpillar excavator and 48-inch shear attachment tear down Launch Umbilical Tower No. 1 (LUT-1) stored in the Industrial Area of KSC. The LUT-1 was part of the launch system used for Apollo-Saturn V, launching Apollo 8, Apollo 11, Skylab manned missions and the Apollo-Soyuz Test Project. The shear is one used in the deconstruction of the Twin Towers in New York City after 9/11.

KSC-04pd0606

NASA Image and Video Library

2004-03-24

KENNEDY SPACE CENTER, FLA. -- Looking like a prehistoric monster crunching on its prey, the Caterpillar excavator and 48-inch shear attachment tear down Launch Umbilical Tower No. 1 (LUT-1) stored in the Industrial Area of KSC. The LUT-1 was part of the launch system used for Apollo-Saturn V, launching Apollo 8, Apollo 11, Skylab manned missions and the Apollo-Soyuz Test Project. The shear is one used in the deconstruction of the Twin Towers in New York City after 9/11.

KSC-04pd0605

NASA Image and Video Library

2004-03-24

KENNEDY SPACE CENTER, FLA. -- Looking like a prehistoric monster crunching on its prey, the Caterpillar excavator and 48-inch shear attachment tear down Launch Umbilical Tower No. 1 (LUT-1) stored in the Industrial Area of KSC. The LUT-1 was part of the launch system used for Apollo-Saturn V, launching Apollo 8, Apollo 11, Skylab manned missions and the Apollo-Soyuz Test Project. The shear is one used in the deconstruction of the Twin Towers in New York City after 9/11.

Tarasca: ritual monster of Spain.

PubMed

Gilmore, David D

2008-09-01

Let us now revisit our original assumptions. First, we note that for the participants in Hacinas Carnival the Tarasca is a figure of fun and joy, but it also exudes a strain of aggressive misogyny that many female residents, not to mention tourists, find somewhat unsettling. In the spirit of feminist currents in Spain, a group of young women protested in 1992 to town officials and, when rebuffed, sought to build their own female monster, which they intended to use to attack boys and men. While their plan was never carried out, and indeed met with stiff opposition from officialdom and, especially, from older women, some of the younger, more modern girls find the Tarasca appalling, and they told me so without compunction. Accordingly, today the festival tends to polarize the sexes as well as the generations. Also, many children are frightened by the gigantic mock-up with its snapping teeth and foul breath, and many of them burst into tears at the roaring of the demons. But despite these negatives--or perhaps because of them--the Tarasca breaks down boundaries between things normally kept separate in the mind: humor and terror, man and beast, order and disorder, old and young, life and death, and so on. In so collapsing opposites, the Tarasca causes people to pause and to think about and question everyday reality in the non-Carnival universe. All these observations of course support the structural arguments of our four theorists above and in particular seem to corroborate Bloch's concept (1992) of the regenerative power of "rebounding violence." However, there are three specific features here that need psychological amplification beyond simply confirming the work of previous theorists. We must first note that like most grotesque fantasies, the Hacinas monster combines disparate organic "realities" into a bizarre and monstrous image that by its very oddness and the resulting "cognitive mismatch" captures people's attention and sparks the imagination, especially that of children (Konner 2002, 222). The Pentecostal beastie combines equine, reptilian, and bird-like features with a giraffe's neck, an elephant's bulk, an impossible number of legs, the usual human malevolence, and the satyr's insatiable lust. The monster also combines cognitive antitheses in a way that reinforces cultural biases while at the same time undermining them--a typical paradox of the Monstrous in ritual and art (Andriano 1999). In the Hacinas festival the integrated themes are those of bodily mutilation, sexual abuse, cannibalism, death, and decay. All these themes come together in certain compelling Iberian traditions: misogyny, costumed parading, religious revitalization, ritual displacement of aggression onto external objects, spontaneous street theatre. All forms of aggression are visually embodied in the image of the mystic beast, as happens every day in the classic Spanish bullfight pitting man against raw nature (Mitchell 1991). Peremptory male sexuality both parodied and glorified, women both raped and rescued, children both terrified and liberated. As Bloch has argued in the aptly titled Prey into Hunter (1992), the narrative of the Tarasca rite, turning victim into victimizer, enables the community to "absorb the vitality" of the external threat and thereby to regenerate itself and to transcend everyday reality. We may make a third, psychoanalytic, observation. As with all such fabulous and scary images, the Tarasca provokes regressive responses that probably go back to the primary organization of the mind before the advent of speech. In this childhood environment, sensations are limited to visions and primary emotions, and the world is experienced largely through the eyes and mouth. Psychoanalysts of childhood have called this the phase of oral/visual primacy. It may explain the locus of aggression in typical monster imagery: the rending teeth, the gnashing jaws, the cavernous belly. It would also help us understand the terror at being devoured by a giant predator during the ritual or, as Bloch puts it (1992, 101), "the horrifying possibility of being consumed" as an essential aspect of ritual process. The snapping mouth as well as other incorporative morphological features of the Hacinas monster, for example, the bulging belly, give an animated shape to primordial fear, with its dynamic mixture of oral, erotic, and self-identity themes. This is exactly what Bloch refers to as the "consuming" threat, the evil that "bites" and "eats" before succumbing to the power of the good. The Tarasca exemplifies both childhood anxieties and the residual fears of adults; and so the festival evokes passionate intensity in all age groups. As Turner might have put it, the "pressure points" that find expression in Hacinas are those between sexual desire and guilt, terror and curiosity, good and evil, purity and corruption; the tensions are those between old and young, death and re-birth (emerging anew from the Tarasca's belly). All of these themes are probably universally encountered and thus constitute the "core" of rituals everywhere by "reenacting the creation ot moral life" (Bloch 1992, 47). Although the Tarasca frightens children and makes them bawl and run away, it also stimulates their cognitive growth and offers ultimately a sense of safety provided by a united and victorious community. Some child psychologists such as Denyse Beaudet (1990) and Jean Piaget (1962, 229) have surmised as much. Piaget says that unconstrained mental operations caused by shock or disorientation provide Spieltaum: an imaginary playground where youngsters experiment with ideas. Bruno Bettelheim says that such creativity permits children to give anxieties tangible form: these can then be distanced and defeated (1976, 120). This projective process, beginning in infancy, of course continues in adulthood, not only in dreams and fantasy but in community rituals, where it reaches apotheosis as Bloch has so persuasively argued. Finally, we must address the misogynist theme that is so marked in the Spanish festival. Many anthroooloeists have noted the theme of the treacherous siren in Spanish folklore, a theme that corresponds to the female models carried aloft on the Tarasca's spine in Granada, Toledo, and other places. One observer, Stanley Brandes, was impressed with the pervasiveness of this specific male anxiety in the Andalusian town of Monteros. In his book on male folklore, Metaphors of Masculinity (1980), Brandes records a number of popular aphorisms that warn men to protect their fragile manhood from duplicitous females or suffer emasculation (one urges men literally to keep their penises in their pants or be castrated). In my own fieldwork in Seville Province, I found the eating/castration theme paramount in male folklore and I have recorded numerous Carnival ditties warning men and boys against the vagina dentata and other forms of female sexual aggression (Gilmore 1987; 1998). Literary scholar Louise Vasvari (1991, 3) refers to the "gastro-genital equivalence" symbolism of Spanish versification, which she identifies in writings dating back to the Middle Ages. Given all this evidence, we may conclude that with its defining misogynist theme and its female/monster imagery, the Spanish Tarasca embodies a dread of feminine sexuality that colors the Spanish male subculture. In particular, in the Hacinas case, the misogynist element combines a devouring theme along with the castration threat in the attack on the boys' genitals and in the liquid thrown onto the crotch, symbolizing, one may conjecture, semen and blood. While these themes are probably universal, their annual apotheosis in visual tropes, public rites, monster effigies, and masques may be specific to Spain. Both appalling in its ferocity and ennobling in its ultimate function as sacrificial object, the Tarasca is one of countless projections of universal human mental shadows as an embodiment, a visual metaphor, as James Fernandez has shown in his classic paper on the role of tropes in culture (1986). Like the other monsters of the world, the Tarascas of Spain are man-eaters and rapists, both lascivious females and priapic males; their toothy (and in Hacinas smelly) oral symbolism is at the same time lurid and hypnotic to the crowds that fight them. As an aspect of local pride, the beast calls forth reverence as well as repugnance. Frightening and also endearing, the Tarasca embodies the human imagination in all its whimsy, grotesqueness, and terror.

A re-examination of paleomagnetic results from NA Jurassic sedimentary rocks: Additional evidence for proposed Jurassic MUTO?

NASA Astrophysics Data System (ADS)

Housen, B. A.

2015-12-01

Kent and Irving, 2010; and Kent et al, 2015 propose a monster shift in the position of Jurassic (160 to 145 Ma) paleopoles for North America- defined by results from igneous rocks. This monster shift is likely an unrecognized true polar wander occurrence. Although subject to inclination error, results from sedimentary rocks from North America, if corrected for these effects, can be used to supplement the available data for this time period. Steiner (2003) reported results from 48 stratigraphic horizons sampled from the Callovian Summerville Fm, from NE New Mexico. A recalculated mean of these results yields a mean direction of D = 332, I = 39, n=48, k = 15, α95 = 5.4°. These data were analyzed for possible inclination error-although the dataset is small, the E-I results yielded a corrected I = 53. This yields a corrected paleopole for NA at ~165 Ma located at 67° N and 168° E.Paleomagnetic results from the Black Hills- Kilanowski (2002) for the Callovian Hulett Mbr of the Sundance Fm, and Gregiore (2001) the Oxfordian-Tithonian Morrison Fm (Gregiore, 2001) have previously been interpreted to represent Eocene-aged remagnetizations- due to the nearly exact coincidence between the in-situ pole positions of these Jurassic units with the Eocene pole for NA. Both of the tilt-corrected results for these units have high latitude poles (Sundance Fm: 79° N, 146° E; Morrison Fm: 89° N, 165° E). An E-I analysis of these data will be presented- using a provisional inclination error of 10°, corrected paleopoles are: (Sundance Fm: 76° N, 220° E; Morrison Fm: 77° N, 266° E). The Black Hills 165 Ma (Sundance Fm) and 145 Ma (Morrison Fm) poles, provisionally corrected for 10° inclination error- occur fairly close to the NA APWP proposed by Kent et al, 2015- using an updated set of results from kimberlites- the agreement between the Sundance Fm and the Triple-B (158 Ma) pole would be nearly exact with a slightly lesser inclination error. The Summerville Fm- which is thought to be ~ coeval with the Sundance Fm- is significantly offset from this newer NA path, but a larger inclination error for this unit would produce a better agreement. Thus, pending more precise estimates of inclination error from these units, middle-late Jurassic sedimentary rocks from NA do support the existence of a MUTO (Monster Unknown True polar wander Occurrence) during Jurassic time.

Partial duplication of head--a rare congenital anomaly.

PubMed

Hemachandran, Manikkapurath; Radotra, Bishan Dass

2004-10-01

Duplication of notochord results in rare congenital anomalies like double headed monsters, with or without trunk/limb duplication, depending upon the extent of notochordal abnormality. Here we describe the morphological abnormalities in a case of partial duplication of cranial structures with fusion of the two. Autopsy findings suggest that the bifurcation of the neural tube took place around 4th to 6th week of gestation. There are only few reports in English literature describing the autopsy findings of such an anomaly, which is termed as Diprosopus triophthalmus in the modern literature.

Two-dimensional RCFT's without Kac-Moody symmetry

NASA Astrophysics Data System (ADS)

Hampapura, Harsha R.; Mukhi, Sunil

2016-07-01

Using the method of modular-invariant differential equations, we classify a family of Rational Conformal Field Theories with two and three characters having no Kac-Moody algebra. In addition to unitary and non-unitary minimal models, we find "dual" theories whose characters obey bilinear relations with those of the minimal models to give the Moonshine Module. In some ways this relation is analogous to cosets of meromorphic CFT's. The theory dual in this sense to the Ising model has central charge 47/2 and is related to the Baby Monster Module.

VLA observations of radio sources in interacting galaxy pairs in poor clusters

NASA Technical Reports Server (NTRS)

Batuski, David J.; Hanisch, Robert J.; Burns, Jack O.

1992-01-01

Observations of 16 radio sources in interacting galaxies in 14 poor clusters were made using the Very Large Array in the B configuration at lambda of 6 and 2 cm. These sources had been unresolved in earlier observations at lambda of 21 cm, and were chosen as a sample to determine which of three models for radio source formation actually pertains in interacting galaxies. From the analysis of this sample, the starburst model appears most successful, but the 'central monster' model could pertain in some cases.

"MONSTROUS MOONSHINE" and Physics

NASA Astrophysics Data System (ADS)

Pushkin, A. V.

The report presents some results obtained by the author on the quantum gravitation theory. Algebraic structure of this theory proves to be related to the commutative nonassociative Griess algebra. The theory symmetry is the automorphism group of Griess algebra: "Monster" simple group. Knowledge of the theory symmetry allows to compute observed physical values in the `zero' approximation. The report presents such computed results for values {m_{p}}/{m_{c}} and α, for the latter the `zero' approximation accuracy, controlled by the theory, being one order of magnitude higher than the accuracy of modern measurements.

Subduing the green-eyed monster: bridging the psychopharmacological and psychosocial treatment perspective in understanding pathological jealousy.

PubMed

Samad, Farah Deena Abdul; Sidi, Hatta; Kumar, Jaya; Das, Srijit; Midin, Marhani; Hatta, Nurul Hazwani

2017-07-04

Human being is not spared from a broad-ranged emotional state, including being jealous. Jealousy has both affective-cognitive and behavioural-evaluative dimension where the person perceives, or experiences a real threat on a valued relationship. As this complex emotion becomes irrational and not amenable to reason, it later transforms into a dangerously 'green-eyed monster'. This perilous situation which is viewed as pathological jealousy is a form of delusion, which is maintained by a fixed and false reasoning in an originally entrusted intimate relationship. Pathological jealousy is equally prevailing among both gender, and with a greater ubiquitous among the geriatric population. The role of dopamine hyperactivity in the fronto-parietal-temporal region was implicated, with the anatomical mapping of the ventromedial prefrontal cortex (vmPFC), cingulate gyrus (CG), and amygdala involvement in the context of the disease's neurobiology. The etiology of pathological jealousy includes major psychiatric disorders, i.e. delusional disorder, schizophrenia, mood disorder, organic brain syndrome, and among others, the drug-induced psychosis. The role of relationship issues and psychodynamic perspective, i.e. psychological conflicts with dependence on a romantic partner, and low self-esteem are involved. Pathological jealousy inherits high-risk forensic psychiatry entanglement, which may warrant intensive intervention, including hospital admission and antipsychotic treatment. Treatment options include an early recognition, managing underlying neuropsychiatric disorders, psycho education, cognitive psychotherapy, and choosing an effective psychopharmacological agent. The management strategy may also resort to a geographical intervention, i.e. separation between both persons to complement the biological treatment. Copyright© Bentham Science Publishers; For any queries, please email at epub@benthamscience.org.

The 'Tully monster' is a vertebrate.

PubMed

McCoy, Victoria E; Saupe, Erin E; Lamsdell, James C; Tarhan, Lidya G; McMahon, Sean; Lidgard, Scott; Mayer, Paul; Whalen, Christopher D; Soriano, Carmen; Finney, Lydia; Vogt, Stefan; Clark, Elizabeth G; Anderson, Ross P; Petermann, Holger; Locatelli, Emma R; Briggs, Derek E G

2016-04-28

Problematic fossils, extinct taxa of enigmatic morphology that cannot be assigned to a known major group, were once a major issue in palaeontology. A long-favoured solution to the 'problem of the problematica', particularly the 'weird wonders' of the Cambrian Burgess Shale, was to consider them representatives of extinct phyla. A combination of new evidence and modern approaches to phylogenetic analysis has now resolved the affinities of most of these forms. Perhaps the most notable exception is Tullimonstrum gregarium, popularly known as the Tully monster, a large soft-bodied organism from the late Carboniferous Mazon Creek biota (approximately 309-307 million years ago) of Illinois, USA, which was designated the official state fossil of Illinois in 1989. Its phylogenetic position has remained uncertain and it has been compared with nemerteans, polychaetes, gastropods, conodonts, and the stem arthropod Opabinia. Here we review the morphology of Tullimonstrum based on an analysis of more than 1,200 specimens. We find that the anterior proboscis ends in a buccal apparatus containing teeth, the eyes project laterally on a long rigid bar, and the elongate segmented body bears a caudal fin with dorsal and ventral lobes. We describe new evidence for a notochord, cartilaginous arcualia, gill pouches, articulations within the proboscis, and multiple tooth rows adjacent to the mouth. This combination of characters, supported by phylogenetic analysis, identifies Tullimonstrum as a vertebrate, and places it on the stem lineage to lampreys (Petromyzontida). In addition to increasing the known morphological disparity of extinct lampreys, a chordate affinity for T. gregarium resolves the nature of a soft-bodied fossil which has been debated for more than 50 years.

Pipsqueak Star Unleashes Monster Flare

NASA Image and Video Library

2017-12-08

NASA release date May 9, 2008 An artist depicts the incredibly powerful flare that erupted from the red dwarf star EV Lacertae. Credit: Casey Reed/NASA To read more about this image go to: www.nasa.gov/topics/universe/features/pipsqueak_star.html NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Afraid of medical care school-aged children's narratives about medical fear.

PubMed

Forsner, Maria; Jansson, Lilian; Söderberg, Anna

2009-12-01

Fear can be problematic for children who come into contact with medical care. This study aimed to illuminate the meaning of being afraid when in contact with medical care, as narrated by children 7-11 years old. Nine children participated in the study, which applied a phenomenological hermeneutic analysis methodology. The children experienced medical care as "being threatened by a monster," but the possibility of breaking this spell of fear was also mediated. The findings indicate the important role of being emotionally hurt in a child's fear to create, together with the child, an alternate narrative of overcoming this fear.

"Juice Monsters": Sub-Ohm Vaping and Toxic Volatile Aldehyde Emissions.

PubMed

Talih, Soha; Salman, Rola; Karaoghlanian, Nareg; El-Hellani, Ahmad; Saliba, Najat; Eissenberg, Thomas; Shihadeh, Alan

2017-10-16

An emerging category of electronic cigarettes (ECIGs) is sub-Ohm devices (SODs) that operate at ten or more times the power of conventional ECIGs. Because carcinogenic volatile aldehyde (VA) emissions increase sharply with power, SODs may expose users to greater VAs. In this study, we compared VA emissions from several SODs and found that across device, VAs and power were uncorrelated unless power was normalized by coil surface area. VA emissions and liquid consumed were correlated highly. Analyzed in light of EU regulations limiting ECIG liquid nicotine concentration, these findings suggest potential regulatory levers and pitfalls for protecting public health.

Dinosaurs, Chameleons, Humans, and Evo-Devo Path: Linking Étienne Geoffroy's Teratology, Waddington's Homeorhesis, Alberch's Logic of "Monsters," and Goldschmidt Hopeful "Monsters".

PubMed

Diogo, Rui; Guinard, Geoffrey; Diaz, Raul E

2017-05-01

Since the rise of evo-devo (evolutionary developmental biology) in the 1980s, few authors have attempted to combine the increasing knowledge obtained from the study of model organisms and human medicine with data from comparative anatomy and evolutionary biology in order to investigate the links between development, pathology, and macroevolution. Fortunately, this situation is slowly changing, with a renewed interest in evolutionary developmental pathology (evo-devo-path) in the past decades, as evidenced by the idea to publish this special, and very timely, issue on "Developmental Evolution in Biomedical Research." As all of us have recently been involved, independently, in works related in some way or another with evolution and developmental anomalies, we decided to join our different perspectives and backgrounds in the present contribution for this special issue. Specifically, we provide a brief historical account on the study of the links between evolution, development, and pathologies, followed by a review of the recent work done by each of us, and then by a general discussion on the broader developmental and macroevolutionary implications of our studies and works recently done by other authors. Our primary aims are to highlight the strength of studying developmental anomalies within an evolutionary framework to understand morphological diversity and disease by connecting the recent work done by us and others with the research done and broader ideas proposed by authors such as Étienne Geoffroy Saint-Hilaire, Waddington, Goldschmidt, Gould, and Per Alberch, among many others to pave the way for further and much needed work regarding abnormal development and macroevolution. © 2016 Wiley Periodicals, Inc.

Assessing the Impact of an Interactive Mobile Game on Tobacco-Related Attitudes and Beliefs: The Truth Campaign's "Flavor Monsters".

PubMed

Rath, Jessica M; Williams, Valerie; Rubenstein, Rebecca; Smith, Lexi; Vallone, Donna

2015-12-01

Given that over 97 percent of American teens play videogames, it is not surprising that many "games for health" target youth. Although tobacco use is the leading cause of preventable death in the United States, few digital games focus on preventing this behavior. The aims of this study were twofold: (1) to determine if youth will play a game with tobacco-related information and themes and (2) to explain the relationship between the truth(®) (Legacy, Washington, DC) campaign's "Flavor Monsters" gameplay and shifts in game-related tobacco knowledge, attitudes, and beliefs. First, two versions of the game, with different amounts of tobacco-related content, were developed to examine the influence of tobacco-related content on player engagement, length of play, awareness of the truth brand, and receptivity to the game. No statistically significant differences were found for engagement (P=0.81), length of play (P=0.10), or awareness of the truth brand (P=0.67). Using an online survey through a preexisting online panel of 13-24 year olds, a longitudinal (n=693) design was used whereby exposure to messages varied naturally over time. Because of the large number of anti-tobacco industry attitude questions, we created an Anti-Tobacco Industry (ATI) Index based on the results of a factor analysis. Although gameplay was not a predictor of lower levels of intention to smoke, level mastered was a significant positive predictor of ATI Index attitudes score at 3 months, controlling for baseline ATI Index score, age, gender, and ever cigarette use (P=0.002). Longitudinal findings indicate a cumulative and enduring effect, suggesting that anti-tobacco content can be successfully integrated within a mobile game to help increase anti-tobacco attitudes.

Early evolution of the venom system in lizards and snakes.

PubMed

Fry, Bryan G; Vidal, Nicolas; Norman, Janette A; Vonk, Freek J; Scheib, Holger; Ramjan, S F Ryan; Kuruppu, Sanjaya; Fung, Kim; Hedges, S Blair; Richardson, Michael K; Hodgson, Wayne C; Ignjatovic, Vera; Summerhayes, Robyn; Kochva, Elazar

2006-02-02

Among extant reptiles only two lineages are known to have evolved venom delivery systems, the advanced snakes and helodermatid lizards (Gila Monster and Beaded Lizard). Evolution of the venom system is thought to underlie the impressive radiation of the advanced snakes (2,500 of 3,000 snake species). In contrast, the lizard venom system is thought to be restricted to just two species and to have evolved independently from the snake venom system. Here we report the presence of venom toxins in two additional lizard lineages (Monitor Lizards and Iguania) and show that all lineages possessing toxin-secreting oral glands form a clade, demonstrating a single early origin of the venom system in lizards and snakes. Construction of gland complementary-DNA libraries and phylogenetic analysis of transcripts revealed that nine toxin types are shared between lizards and snakes. Toxinological analyses of venom components from the Lace Monitor Varanus varius showed potent effects on blood pressure and clotting ability, bioactivities associated with a rapid loss of consciousness and extensive bleeding in prey. The iguanian lizard Pogona barbata retains characteristics of the ancestral venom system, namely serial, lobular non-compound venom-secreting glands on both the upper and lower jaws, whereas the advanced snakes and anguimorph lizards (including Monitor Lizards, Gila Monster and Beaded Lizard) have more derived venom systems characterized by the loss of the mandibular (lower) or maxillary (upper) glands. Demonstration that the snakes, iguanians and anguimorphs form a single clade provides overwhelming support for a single, early origin of the venom system in lizards and snakes. These results provide new insights into the evolution of the venom system in squamate reptiles and open new avenues for biomedical research and drug design using hitherto unexplored venom proteins.

Gods, daemons and banshees on the journey to the magic scroll: the use of myth as a framework for reflective practice in nurse education.

PubMed

Morgan, S

1996-04-01

This paper reports the use of a mythic journey scenario within a student nurse groupwork session. This approach was introduced as a means to facilitate personal and interpersonal sharing and self-knowledge. These processes are held as important for the development of critical reflective process as a cornerstone of contemporary nursing practice. The use of myth invoked a coherent and supportive student environment within which previously reticent students appeared confident enough to contribute and explore their educational experience in nursing. The mythic allegoric process also identified some poignant themes and enemies, common across the student body. Monsters no less!

Detection and Analysis of Six Lizard Adenoviruses by Consensus Primer PCR Provides Further Evidence of a Reptilian Origin for the Atadenoviruses

PubMed Central

Wellehan, James F. X.; Johnson, April J.; Harrach, Balázs; Benkö, Mária; Pessier, Allan P.; Johnson, Calvin M.; Garner, Michael M.; Childress, April; Jacobson, Elliott R.

2004-01-01

A consensus nested-PCR method was designed for investigation of the DNA polymerase gene of adenoviruses. Gene fragments were amplified and sequenced from six novel adenoviruses from seven lizard species, including four species from which adenoviruses had not previously been reported. Host species included Gila monster, leopard gecko, fat-tail gecko, blue-tongued skink, Tokay gecko, bearded dragon, and mountain chameleon. This is the first sequence information from lizard adenoviruses. Phylogenetic analysis indicated that these viruses belong to the genus Atadenovirus, supporting the reptilian origin of atadenoviruses. This PCR method may be useful for obtaining templates for initial sequencing of novel adenoviruses. PMID:15542689

Detection and analysis of six lizard adenoviruses by consensus primer PCR provides further evidence of a reptilian origin for the atadenoviruses.

PubMed

Wellehan, James F X; Johnson, April J; Harrach, Balázs; Benkö, Mária; Pessier, Allan P; Johnson, Calvin M; Garner, Michael M; Childress, April; Jacobson, Elliott R

2004-12-01

A consensus nested-PCR method was designed for investigation of the DNA polymerase gene of adenoviruses. Gene fragments were amplified and sequenced from six novel adenoviruses from seven lizard species, including four species from which adenoviruses had not previously been reported. Host species included Gila monster, leopard gecko, fat-tail gecko, blue-tongued skink, Tokay gecko, bearded dragon, and mountain chameleon. This is the first sequence information from lizard adenoviruses. Phylogenetic analysis indicated that these viruses belong to the genus Atadenovirus, supporting the reptilian origin of atadenoviruses. This PCR method may be useful for obtaining templates for initial sequencing of novel adenoviruses.

Chimaera and its modern virus-like descendants.

PubMed

Ulrich, R; Gerlich, W H; Krüger, D H

1996-01-01

Chimaera was a monster in ancient Greek mythology combining elements from different animal species in its body. Modern molecular biology enabled the generation of harmless but useful chimaeras consisting of elements from different nonrelated viruses. The objective is that the resulting chimaeras form highly immunogenic virus-like particles (VLPs). Such chimaeric VLPs can be used as highly efficient carriers for sequential and conformational B cell epitopes and T cell epitopes. Most VLPs are readily produced in heterologous hosts and are easy to purify. This article deals with various systems of VLPs described in this topical issue of Intervirology and makes comparisons with chimaeric replication-competent viruses, recombinant virus vectors expressing foreign proteins, and DNA vaccines.

The monster sound pipe

NASA Astrophysics Data System (ADS)

Ruiz, Michael J.; Perkins, James

2017-03-01

Producing a deep bass tone by striking a large 3 m (10 ft) flexible corrugated drainage pipe immediately grabs student attention. The fundamental pitch of the corrugated tube is found to be a semitone lower than a non-corrugated smooth pipe of the same length. A video (https://youtu.be/FU7a9d7N60Y) of the demonstration is included, which illustrates how an Internet keyboard can be used to estimate the fundamental pitches of each pipe. Since both pipes have similar end corrections, the pitch discrepancy between the smooth pipe and drainage tube is due to the corrugations, which lower the speed of sound inside the flexible tube, dropping its pitch a semitone.

Governor Pio Pico, the monster of California...no more: lessons in neuroendocrinology.

PubMed

Login, Ivan S; Login, Jessica

2010-01-01

We hypothesize that Pio Pico, the last Mexican Governor of California, had acromegaly between at least ages 43 to 57, from 1844 to 1858, before Pierre Marie published the clinical description of acromegaly in 1886. Pico's probable growth hormone-secreting pituitary tumor likely infarcted spontaneously after 1858. The tumor infarction resulted in burnt-out acromegaly and probably restored normal pituitary function. Pearce Bailey published the first account of pituitary tumor infarction only in 1898. Pico's undiagnosed, misunderstood, profoundly acromegalic appearance was widely misinterpreted, leading to pervasive, degrading, and highly prejudicial comments. This landmark case study in neuroendocrinology provides the opportunity to re-examine elements of 19th century California and American history.

Heart rate, blood pressure and repolarization effects of an energy drink as compared to coffee.

PubMed

Brothers, R Matthew; Christmas, Kevin M; Patik, Jordan C; Bhella, Paul S

2017-11-01

The goal of this study was to investigate the impact of energy drinks on haemodynamic and cardiac physiology. Comparisons were made to coffee as well as water consumption. In Protocol #1 the caffeine content was normalized to body weight to represent a controlled environment. Heart rate, blood pressure and cardiac QTc interval were assessed in 15 participants, on 4 days, prior to and for 6·5 h postconsumption of (i) energy drink (2 mg caffeine per kg body weight; low dose), (ii) energy drink (3 mg caffeine per kg body weight; medium dose), (iii) coffee (2 mg caffeine per kg body weight) and (iv) 250 ml water. In Protocol #2, the beverages were consumed in volumes that they are purchased to represent real-life conditions. The aforementioned measurements were repeated in 15 participants following (i) 1 16 oz can of energy drink (16 oz Monster), (ii) 1 24 oz can of energy drink (24 oz Monster), (iii) 1 packet of Keurig K-Cup Starbucks coffee (coffee) and (iv) 250 ml water. The order of the beverages was performed in a randomized double-blinded fashion. For both protocols, QTc interval, heart rate and systolic blood pressure were unchanged in any condition (P>0·05). Diastolic blood pressure and mean blood pressure were slightly elevated in Protocol #1 (P<0·05, main effect of time) with no difference between beverages (P<0·05, interaction of beverage × time); however, they were unaffected in Protocol #2 (P>0·05). These findings suggest that acute consumption of these commonly consumed beverages has no negative effect on cardiac QTc interval. © 2016 Scandinavian Society of Clinical Physiology and Nuclear Medicine. Published by John Wiley & Sons Ltd.

Monsters in the sky. I mostri del cielo

DOE Office of Scientific and Technical Information (OSTI.GOV)

Maffei, P.

1980-01-01

The book treats astronomical objects and phenomena which remain unexplained or unproven by current investigators. Specific objects discussed include comets, satellite clouds surrounding the earth, tektites, the planet Vulcan (within the orbit of Mercury), Planet X (beyond Pluto), the Gum Nebula, planetary nebulae, supernovae, supernova remnants, transient X-ray sources, the possible extinction of the dinosaurs by an X-ray explosion and super-supernovae. Attention is also given to the star Eta Carinae, black holes, BL Lacertae objects, active galaxies, Markarian galaxies, N and compact galaxies, Seyfert galaxies, quasars, redshift anomalies, Stephan's quintet of galaxies, and intergalactic black holes or black dwarfs whichmore » may account for the mass necessary to bind together clusters of galaxies.« less

Julius Caesar Arantius (Giulio Cesare Aranzi, 1530-1589) and the hippocampus of the human brain: history behind the discovery.

PubMed

Bir, Shyamal C; Ambekar, Sudheer; Kukreja, Sunil; Nanda, Anil

2015-04-01

Julius Caesar Arantius is one of the pioneer anatomists and surgeons of the 16th century who discovered the different anatomical structures of the human body. One of his prominent discoveries is the hippocampus. At that time, Arantius originated the term hippocampus, from the Greek word for seahorse (hippos ["horse"] and kampos ["sea monster"]). Arantius published his description of the hippocampus in 1587, in the first chapter of his work titled De Humano Foetu Liber. Numerous nomenclatures of this structure, including "white silkworm," "Ammon's horn," and "ram's horn" were proposed by different scholars at that time. However, the term hippocampus has become the most widely used in the literature.

Elliptic genera and 3d gravity

DOE Office of Scientific and Technical Information (OSTI.GOV)

Benjamin, Nathan; Cheng, Miranda C. N.; Kachru, Shamit

Here, we describe general constraints on the elliptic genus of a 2d supersymmetric conformal field theory which has a gravity dual with large radius in Planck units. We give examples of theories which do and do not satisfy the bounds we derive, by describing the elliptic genera of symmetric product orbifolds of K 3, product manifolds, certain simple families of Calabi–Yau hypersurfaces, and symmetric products of the “Monster CFT”. We discuss the distinction between theories with supergravity duals and those whose duals have strings at the scale set by the AdS curvature. Under natural assumptions, we attempt to quantify themore » fraction of (2,2) supersymmetric conformal theories which admit a weakly curved gravity description, at large central charge.« less

Elliptic genera and 3d gravity

DOE PAGES

Benjamin, Nathan; Cheng, Miranda C. N.; Kachru, Shamit; ...

2016-03-30

Here, we describe general constraints on the elliptic genus of a 2d supersymmetric conformal field theory which has a gravity dual with large radius in Planck units. We give examples of theories which do and do not satisfy the bounds we derive, by describing the elliptic genera of symmetric product orbifolds of K 3, product manifolds, certain simple families of Calabi–Yau hypersurfaces, and symmetric products of the “Monster CFT”. We discuss the distinction between theories with supergravity duals and those whose duals have strings at the scale set by the AdS curvature. Under natural assumptions, we attempt to quantify themore » fraction of (2,2) supersymmetric conformal theories which admit a weakly curved gravity description, at large central charge.« less

[The banishment of the marvellous. Hermaphrodites and sexual mutants in Enlightenment Spain].

PubMed

Vásquez, Francisco; Cleminson, Richard

2011-01-01

This article presents a historical synthesis in order to trace how the collective belief in the existence of hermaphrodites and sex-changes was slowly eroded in the changing medical and cultural context of Enlightenment Spain. In order to explain this change, three interlinked processes are outlined. First, the naturalization of the monster and the disappearance of the "marvellous" in Enlightenment science. Second, the consolidation of modern legal or forensic science and the rise of the medical specialist as the relevant authority in the determination of sexual identity. Third, the emergence of the notion of fundamental biological differences between the sexes. The article concludes by discussing the consequences of these shifts for early nineteenth-century Spanish medicine.

Lost Toy? Monsters Under the Bed? Contributions of Temperament and Family Factors to Early Internalizing Problems in Boys and Girls

PubMed Central

Marakovitz, Susan E.; Wagmiller, Robert L.; Mian, Nicholas D.; Briggs-Gowan, Margaret J.; Carter, Alice S.

2016-01-01

This study was designed to examine the contribution of multiple risk factors to early internalizing problems and to investigate whether family and ecological context moderated the association between child temperament and internalizing outcomes. A sample of 1,202 mothers of 2- and 3-year-old children completed a survey of child social-emotional functioning, family environment, and violence exposure. Child temperament, maternal affective symptoms, and family expressiveness were associated with child anxiety and depression problems. Violence exposure was related only to child anxiety. When maternal affective symptoms were elevated, inhibited girls but not boys were rated as more anxious and youngsters with heightened negative emotionality were rated as more depressed. Family expressiveness moderated the association between inhibited temperament and anxiety symptoms. PMID:21391020

Filming the freak show. Non-normative bodies on screen.

PubMed

Brodesco, Alberto

2014-01-01

The article focuses on four films that display the exhibition for profit of non- normative bodies in a context that is variously called freak show, sideshow, monster show, odditorium. Freaks (Tod Browning, 1932), The Ape Woman (La donna scimmia, Marco Ferreri, 1964), Elephant Man (David Lynch, 1980) and Black Venus (Venus noire, Abdellatif Kechiche, 2010) are reflexive movies that tell stories of abnormal bodies and of people who buy a ticket to see them. They inquire the fictional nature of "freakness"--a cultural and historical artefact, a social construction, a frame of mind and a set of practices--and draw attention to the continuity between the world of the freak shows and the scientific and medical milieus. The article finally considers the new visibility of the corporeal freak in contemporary voyeuristic television programs.

Monsters and babies from the first/IRAS survey

DOE Office of Scientific and Technical Information (OSTI.GOV)

Van Bruegel, W J M

Radio continuum emission at cm wavelengths is relatively little affected by extinction. When combined with far-infrared (FIR) surveys this provides for a convenient and unbiased method to select (radio-loud) AGN and starbursts deeply embedded in gas and dust-rich galaxies. Such radio-selected FIR samples are useful for detailed investigations of the complex relationships between (radio) galaxy and starburst activity, and to determine whether ULIRGs are powered by hidden quasars (monsters) or young stars (babies). We present the results of a large program to obtain identifications and spectra of radio-sleected, optically faint IRAS/FSC objects using the FIRST/VLA 20 cm survey (Becker, Whitemore » and Helfand 1995). These objects are all radio-'quiet' in the sense that their radio power/FIR luminosities follow the well-known radio/FIR relationship for star forming galaxies. We compare these results to a previous study by our group of a sample of radio-'loud' IRAS/FSC ULIRGs selected from the Texas 365 MHz survey (Douglas et al. 1996). Many of these objects also show evidence for dominant, A-type stellar populations, as well as high ionization lines usually associated with AGN. These radio-loud ULIRGs have properties intermediate between those of starbursts and quasars, suggesting a possibile evolutionary connection. Deep Keck spectroscopic observations of three ULIRGs from these samples are presented, including high signal-to-noise spectropolarimetry. The polarimetry observations failed to show evidence of a hidden quasar in polarized (scattered) light in the two systems in which the stellar light was dominated by A-type stars. Although observations of a larger sample would be needed to allow a general conclusion, our current data suggest that a large fraction of ULIRGs may be powered by luminous starbursts, not by hidden, luminous AGN (quasars). While we used radio-selected FIR sources to search for evidence of a causal AGN/starburst connection, we conclude our presentation with a dramatic example of an AGN/starburst object from an entirely unrelated quasar survey selected at the opposite, blue end of the spectrum.« less

Leibniz on the unicorn and various other curiosities.

PubMed

Ariew, R

1998-11-01

I discuss some of Leibniz's pronouncements about fringe phenomena--various monsters; talking dogs; genies and prophets; unicorns, glossopetrae, and other games of nature--in order to understand better Leibniz's views on science and the role these curiosities play in his plans for scientific academies and societies. However, given that Leibniz's sincerity has been called into question in twentieth-century secondary literature, I begin with a few historiographical remarks so as to situate these pronouncements within the Leibnizian corpus. What emerges is an image of Leibniz as a sober, cautious interpreter, a skeptic one might say but one who is prepared to concede the possibility of many strange phenomena. Leibniz expects these fringe phenomena to take their place among the natural curiosities catalogued as part of a hoped for empirical database intended as means toward the perfection of the sciences.

Diet-derived microRNAs: unicorn or silver bullet?

PubMed

Witwer, Kenneth W; Zhang, Chen-Yu

2017-01-01

In ancient lore, a bullet cast from silver is the only effective weapon against monsters. The uptake of active diet-derived microRNAs (miRNAs) in consumers may be the silver bullet long sought after in nutrition and oral therapeutics. However, the majority of scientists consider the transfer and regulation of consumer's gene activity by these diet-derived miRNAs to be a fantasy akin to spotting a unicorn. Nevertheless, groups like Dr. Chen-Yu Zhang's lab in Nanjing University have stockpiled breathtaking amounts of data to shoot down these naysayers. Meanwhile, Dr. Ken Witwer at John Hopkins has steadfastly cautioned the field to beware of fallacies caused by contamination, technical artifacts, and confirmation bias. Here, Dr. Witwer and Dr. Zhang share their realities of dietary miRNAs by answering five questions related to this controversial field.

From first galaxies to QSOs - feeding the baby monsters

NASA Astrophysics Data System (ADS)

Danese, L.; Shankar, F.; Granato, G. L.; Silva, L.; Bressan, A.; de Zotti, G.; Salucci, P.; Cirasuolo, M.

We present a physical model for the coevolution of massive spheroidal galaxies and active nuclei at their centers. Supernova heating is increasingly effective in slowing down the star formation and in driving gas outflows in smaller and smaller dark matter halos. Thus the more massive protogalaxies virializing at early times are the sites of faster star formation. The correspondingly higher radiation drag causes a faster angular momentum loss by the gas and induces a larger accretion rate onto the central black hole. In turn, the kinetic energy of the outflows powered by the active nuclei can unbind the residual gas in a time shorter for larger halos. The model accounts for a broad variety of dynamical, photometric and metallicity properties of early-type galaxies, for the MBH-σ relation and for the local supermassive black-hole mass function.

The content of recurrent dreams in young adolescents

PubMed Central

Gauchat, Aline; Séguin, Jean R.; McSween-Cadieux, Esther; Zadra, Antonio

2015-01-01

Studies on children’s recurrent dreams have been largely anecdotal and based on adults’ recollections of dreams experienced during childhood. We collected 102 reports of recurrent dreams from a sample of young adolescents aged between 11 and 15 years and scored the narratives using a range of content measures, including in relation to the threat simulation theory (TST) of dreaming. The most frequently reported themes involved confrontations with monsters or animals, followed by physical aggressions, falling and being chased. Recurrent dreams were more likely to include negative content elements than positive elements. Only half of the recurrent dreams contained threatening elements and their analysis provided mixed support for the TST. Differences between the content of recurrent dreams reported by young adolescent versus adults are discussed as are possible sex effects and key issues that remain to be addressed by future research. PMID:26366465

Nest guarding by female Agassiz's desert tortoise (Gopherus agassizii) at a wind-energy facility near Palm Springs, California

USGS Publications Warehouse

Agha, Mickey; Lovich, Jeffrey E.; Ennen, Joshua R.; Wilcox, Ethan

2013-01-01

We observed behavior consistent with nest-guarding in Agassiz's desert tortoise (Gopherus agassizii) at two nests in a large wind-energy-generation facility near Palm Springs, California, locally known as the Mesa Wind Farm. As researchers approached the nests, female desert tortoises moved to the entrance of their burrows and positioned themselves sideways, directly over their nests. One female stretched her limbs outward and wedged herself into the burrow (her plastron directly above the nest). Guarding of nests is rarely observed in Agassiz's desert tortoise but can occur as a result of attempted predation on eggs by Gila monsters (Heloderma suspectum) or in direct response to the perceived threat posed by researchers. This is the first report of nest-guarding for G. agassizii in the Sonoran Desert ecosystem of California.

GRB 130427A: A Nearby Ordinary Monster

NASA Technical Reports Server (NTRS)

Maselli, A.; Melandri, A.; Nava, L.; Mundell, C. G.; Kawai, N.; Campana, S.; Covino, S.; Cummings, J. R.; Cusumano, G.; Evans, P. A.;

Universal RCFT correlators from the holomorphic bootstrap

NASA Astrophysics Data System (ADS)

Mukhi, Sunil; Muralidhara, Girish

2018-02-01

We elaborate and extend the method of Wronskian differential equations for conformal blocks to compute four-point correlation functions on the plane for classes of primary fields in rational (and possibly more general) conformal field theories. This approach leads to universal differential equations for families of CFT's and provides a very simple re-derivation of the BPZ results for the degenerate fields ϕ 1,2 and ϕ 2,1 in the c < 1 minimal models. We apply this technique to compute correlators for the WZW models corresponding to the Deligne-Cvitanović exceptional series of Lie algebras. The application turns out to be subtle in certain cases where there are multiple decoupled primaries. The power of this approach is demonstrated by applying it to compute four-point functions for the Baby Monster CFT, which does not belong to any minimal series.

GRB 130427A: a nearby ordinary monster.

PubMed

Maselli, A; Melandri, A; Nava, L; Mundell, C G; Kawai, N; Campana, S; Covino, S; Cummings, J R; Cusumano, G; Evans, P A; Ghirlanda, G; Ghisellini, G; Guidorzi, C; Kobayashi, S; Kuin, P; La Parola, V; Mangano, V; Oates, S; Sakamoto, T; Serino, M; Virgili, F; Zhang, B-B; Barthelmy, S; Beardmore, A; Bernardini, M G; Bersier, D; Burrows, D; Calderone, G; Capalbi, M; Chiang, J; D'Avanzo, P; D'Elia, V; De Pasquale, M; Fugazza, D; Gehrels, N; Gomboc, A; Harrison, R; Hanayama, H; Japelj, J; Kennea, J; Kopac, D; Kouveliotou, C; Kuroda, D; Levan, A; Malesani, D; Marshall, F; Nousek, J; O'Brien, P; Osborne, J P; Pagani, C; Page, K L; Page, M; Perri, M; Pritchard, T; Romano, P; Saito, Y; Sbarufatti, B; Salvaterra, R; Steele, I; Tanvir, N; Vianello, G; Wiegand, B; Weigand, B; Wiersema, K; Yatsu, Y; Yoshii, T; Tagliaferri, G

2014-01-03

Long-duration gamma-ray bursts (GRBs) are an extremely rare outcome of the collapse of massive stars and are typically found in the distant universe. Because of its intrinsic luminosity (L ~ 3 × 10(53) ergs per second) and its relative proximity (z = 0.34), GRB 130427A reached the highest fluence observed in the γ-ray band. Here, we present a comprehensive multiwavelength view of GRB 130427A with Swift, the 2-meter Liverpool and Faulkes telescopes, and by other ground-based facilities, highlighting the evolution of the burst emission from the prompt to the afterglow phase. The properties of GRB 130427A are similar to those of the most luminous, high-redshift GRBs, suggesting that a common central engine is responsible for producing GRBs in both the contemporary and the early universe and over the full range of GRB isotropic energies.

Demonizing in children's television cartoons and Disney animated films.

PubMed

Fouts, Gregory; Callan, Mitchell; Piasentin, Kelly; Lawson, Andrea

2006-01-01

The purpose of this study was to assess the prevalence of demonizing in the two major media that young children use (television and movies). Two content analyses were conducted using the animated feature films (n = 34) of the Walt Disney Company and after-school cartoons (n = 41). Each was coded for the modeling of the use of "evil" words when referring to a person, e.g., monster, devil, demon, wicked. Seventy-four percent of the Disney films contained "evil" references, with an average of 5.6 references per film. Forty-four percent of the after-school cartoons contained "evil" references, with an average of one per cartoon. The results are discussed within the context of children's repeated exposure to popular animated movies and cartoons and their learning to demonize people who engage in perceived "bad" behaviors.

Exploring Gendered Notions: Gender, Job Hunting and Web Searches

NASA Astrophysics Data System (ADS)

Martey, R. M.

Based on analysis of a series of interviews, this chapter suggests that in looking for jobs online, women confront gendered notions of the Internet as well as gendered notions of the jobs themselves. It argues that the social and cultural contexts of both the search tools and the search tasks should be considered in exploring how Web-based technologies serve women in a job search. For these women, the opportunities and limitations of online job-search tools were intimately related to their personal and social needs, especially needs for part-time work, maternity benefits, and career advancement. Although job-seeking services such as Monster.com were used frequently by most of these women, search services did not completely fulfill all their informational needs, and became an — often frustrating — initial starting point for a job search rather than an end-point.

Images of cloning and stem cell research in editorial cartoons in the United States.

PubMed

Giarelli, Ellen

2006-01-01

Through semiotic analysis of manifest and latent meanings in editorial cartoons, the author uncovers how cloning and stem cell research are represented in a popular mass medium. She identified 86 editorial cartoons published in the United States between 2001 and 2004 that referred to cloning and 20 that referred to stem cell research. Cartoonists portrayed people individually 224 times and 4 times in groups of more than 10. Men were portrayed in 64% of cartoons. Stem cell research was depicted as having a potential positive value, and cloning was depicted negatively. Some major messages are that cloning will lead to the mass production of evil, cloning creates monsters, and politics will influence who or what will be cloned. Analyzing popular images can allow access to public understanding about genetic technology and evaluation of public beliefs, preconceptions, and expectations as the public is educated on the use and value of services.

Jealousy and the threatened self: getting to the heart of the green-eyed monster.

PubMed

DeSteno, David; Valdesolo, Piercarlo; Bartlett, Monica Y

2006-10-01

Several theories specifying the causes of jealousy have been put forth in the past few decades. Firm support for any proposed theory, however, has been limited by the difficulties inherent in inducing jealousy and examining any proposed mediating mechanisms in real time. In support of a theory of jealousy centering on threats to the self-system, 2 experiments are presented that address these past limitations and argue for a model based on context-induced variability in self-evaluation. Experiment 1 presents a method for evoking jealousy through the use of highly orchestrated social encounters and demonstrates that threatened self-esteem functions as a principal mediator of jealousy. In addition to replicating these findings, Experiment 2 provides direct evidence for jealousy as a cause of aggression. The ability of the proposed theory of jealousy to integrate other extant findings in the literature is also discussed. 2006 APA, all rights reserved

The Black Hole Safari: Big Game Hunting in 30+ Massive Galaxies

NASA Astrophysics Data System (ADS)

McConnell, Nicholas J.; Ma, Chung-Pei; Janish, Ryan; Gebhardt, Karl; Lauer, Tod R.; Graham, James R.

2015-01-01

The current census of the most massive black holes in the local universe turns up an odd variety of galaxy hosts: central galaxies in rich clusters, second- or lower-ranked cluster members, and compact relics from the early universe. More extensive campaigns are required to explore the number density and environmental distribution of these monsters. Over the past three years we have collected a large set of stellar kinematic data with sufficient resolution to detect the gravitational signatures of supermassive black holes with MBH > 109 MSun. This Black Hole Safari targets enormous galaxies at the centers of nearby galaxy clusters, as well as their similarly luminous counterparts in weaker galaxy groups. To date we have observed more than 30 early-type galaxies with integral-field spectrographs on the Keck, Gemini North, and Gemini South telescopes. Here I present preliminary stellar kinematics from 10 objects.

The content of recurrent dreams in young adolescents.

PubMed

Gauchat, Aline; Séguin, Jean R; McSween-Cadieux, Esther; Zadra, Antonio

2015-12-01

Studies on children's recurrent dreams have been largely anecdotal and based on adults' recollections of dreams experienced during childhood. We collected 102 reports of recurrent dreams from a sample of young adolescents aged between 11 and 15years and scored the narratives using a range of content measures, including in relation to the threat simulation theory (TST) of dreaming. The most frequently reported themes involved confrontations with monsters or animals, followed by physical aggressions, falling and being chased. Recurrent dreams were more likely to include negative content elements than positive elements. Only half of the recurrent dreams contained threatening elements and their analysis provided mixed support for the TST. Differences between the content of recurrent dreams reported by young adolescent versus adults are discussed as are possible sex effects and key issues that remain to be addressed by future research. Copyright © 2015 Elsevier Inc. All rights reserved.

Modelling third harmonic ion cyclotron acceleration of deuterium beams for JET fusion product studies experiments

NASA Astrophysics Data System (ADS)

Schneider, M.; Johnson, T.; Dumont, R.; Eriksson, J.; Eriksson, L.-G.; Giacomelli, L.; Girardo, J.-B.; Hellsten, T.; Khilkevitch, E.; Kiptily, V. G.; Koskela, T.; Mantsinen, M.; Nocente, M.; Salewski, M.; Sharapov, S. E.; Shevelev, A. E.; Contributors, JET

2016-11-01

Recent JET experiments have been dedicated to the studies of fusion reactions between deuterium (D) and Helium-3 (3He) ions using neutral beam injection (NBI) in synergy with third harmonic ion cyclotron radio-frequency heating (ICRH) of the beam. This scenario generates a fast ion deuterium tail enhancing DD and D3He fusion reactions. Modelling and measuring the fast deuterium tail accurately is essential for quantifying the fusion products. This paper presents the modelling of the D distribution function resulting from the NBI+ICRF heating scheme, reinforced by a comparison with dedicated JET fast ion diagnostics, showing an overall good agreement. Finally, a sawtooth activity for these experiments has been observed and interpreted using SPOT/RFOF simulations in the framework of Porcelli’s theoretical model, where NBI+ICRH accelerated ions are found to have a strong stabilizing effect, leading to monster sawteeth.

Retrogressive development: transcendental anatomy and teratology in nineteenth-century Britain.

PubMed

Bates, Alan W H

2014-01-01

In 1855 the leading British transcendental anatomist Robert Knox proposed a theory of retrogressive development according to which the human embryo could give rise to ancestral types or races and the animal embryo to other species within the same family. Unlike monsters attributed to the older theory of arrested development, new forms produced by retrogression were neither imperfect nor equivalent to a stage in the embryo's development. Instead, Knox postulated that embryos contained all possible specific forms in potentia. Retrogressive development could account for examples of atavism or racial throwbacks, and formed part of Knox's theory of rapid (saltatory) species change. Knox's evolutionary theorizing was soon eclipsed by the better presented and more socially acceptable Darwinian gradualism, but the concept of retrogressive development remained influential in anthropology and the social sciences, and Knox's work can be seen as the scientific basis for theories of physical, mental and cultural degeneracy.

Scylla and Charybdis observed from space

NASA Astrophysics Data System (ADS)

Alpers, Werner; Salusti, Ettore

1983-02-01

Scylla and Charybdis are, in Greek mythology, two immortal and irresistible monsters who beset the narrow waters separating the Italian peninsula from Sicily. They give poetic expressions to exceptional oceanographic features encountered in the Strait of Messina. Recently, the SEASAT satellite has added new information on the oceanography of this strait. For the first time, experimental evidence is presented that internal waves are generated in the Strait of Messina. The generation mechanism is linked to tidal currents washing over the shallow sill within the strait. The experimental data originate from a synthetic aperture radar (SAR) image obtained from the SEASAT satellite on Sept, 15, 1978, and from subsequent in situ measurements carried out from the Italian research vessel Bannock in Nov. 1980. The circular wave pattern visible on the SEASAT SAR image is interpreted in terms of internal solitons. Furthermore, the SEASAT SAR image also reveals `tagli,' special types of tidal bores, encountered in the Strait of Messina.

Brand Suicide? Memory and Liking of Negative Brand Names

PubMed Central

Guest, Duncan; Estes, Zachary; Gibbert, Michael; Mazursky, David

2016-01-01

Negative brand names are surprisingly common in the marketplace (e.g., Poison perfume; Hell pizza, and Monster energy drink), yet their effects on consumer behavior are currently unknown. Three studies investigated the effects of negative brand name valence on brand name memory and liking of a branded product. Study 1 demonstrates that relative to non-negative brand names, negative brand names and their associated logos are better recognised. Studies 2 and 3 demonstrate that negative valence of a brand name tends to have a detrimental influence on product evaluation with evaluations worsening as negative valence increases. However, evaluation is also dependent on brand name arousal, with high arousal brand names resulting in more positive evaluations, such that moderately negative brand names are equally as attractive as some non-negative brand names. Study 3 shows evidence for affective habituation, whereby the effects of negative valence reduce with repeated exposures to some classes of negative brand name. PMID:27023872

Brand Suicide? Memory and Liking of Negative Brand Names.

PubMed

Guest, Duncan; Estes, Zachary; Gibbert, Michael; Mazursky, David

2016-01-01

Negative brand names are surprisingly common in the marketplace (e.g., Poison perfume; Hell pizza, and Monster energy drink), yet their effects on consumer behavior are currently unknown. Three studies investigated the effects of negative brand name valence on brand name memory and liking of a branded product. Study 1 demonstrates that relative to non-negative brand names, negative brand names and their associated logos are better recognised. Studies 2 and 3 demonstrate that negative valence of a brand name tends to have a detrimental influence on product evaluation with evaluations worsening as negative valence increases. However, evaluation is also dependent on brand name arousal, with high arousal brand names resulting in more positive evaluations, such that moderately negative brand names are equally as attractive as some non-negative brand names. Study 3 shows evidence for affective habituation, whereby the effects of negative valence reduce with repeated exposures to some classes of negative brand name.

NORTICA—a new code for cyclotron analysis

NASA Astrophysics Data System (ADS)

Gorelov, D.; Johnson, D.; Marti, F.

2001-12-01

The new package NORTICA (Numerical ORbit Tracking In Cyclotrons with Analysis) of computer codes for beam dynamics simulations is under development at NSCL. The package was started as a replacement for the code MONSTER [1] developed in the laboratory in the past. The new codes are capable of beam dynamics simulations in both CCF (Coupled Cyclotron Facility) accelerators, the K500 and K1200 superconducting cyclotrons. The general purpose of this package is assisting in setting and tuning the cyclotrons taking into account the main field and extraction channel imperfections. The computer platform for the package is Alpha Station with UNIX operating system and X-Windows graphic interface. A multiple programming language approach was used in order to combine the reliability of the numerical algorithms developed over the long period of time in the laboratory and the friendliness of modern style user interface. This paper describes the capability and features of the codes in the present state.

Clinical problem solving: monster on the hook--case problems in neurosurgery.

PubMed

Muh, Carrie R; Boulis, Nicholas M; Chandler, William F; Barkan, Ariel L; Mosunjac, Marina B; Oyesiku, Nelson M

2011-03-01

Nonfunctioning and functioning pituitary tumors can present in numerous ways. They may be difficult to diagnose correctly and, even with proper treatment, may lead to complications. We present the case of a patient who presented with a large, invasive sellar mass and underwent both medical and surgical treatment for this lesion. The patient's course did not progress as was expected from his initial workup. The patient's history, physical examination, laboratory values, pathologic specimens, and radiologic findings are discussed. His management before, during, and after medical therapy and surgery is reviewed by pituitary experts from 2 different institutions. Aspects of diagnosis and management of sellar lesions are presented and reviewed in the literature. Neurosurgeons frequently treat patients with sellar lesions and should remember that despite modern laboratory, pathologic, and radiologic techniques, the diagnosis and treatment of these lesions is not always clear.

When Supermassive Black Holes Wander

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2018-05-01

Are supermassive black holes found only at the centers of galaxies? Definitely not, according to a new study in fact, galaxies like the Milky Way may harbor several such monsters wandering through their midst.Collecting Black Holes Through MergersIts generally believed that galaxies are built up hierarchically, growing in size through repeated mergers over time. Each galaxy in a major merger likely hosts a supermassive black hole a black hole of millions to billions of times the mass of the Sun at its center. When a pair of galaxies merges, their supermassive black holes will often sink to the center of the merger via a process known as dynamical friction. There the supermassive black holes themselves will eventually merge in a burst of gravitational waves.Spatial distribution and velocities of wandering supermassive black holes in three of the authors simulated galaxies, shown in edge-on (left) and face-on (right) views of the galaxy disks. Click for a closer look. [Tremmel et al. 2018]But if a galaxy the size of the Milky Way was built through a history of many major galactic mergers, are we sure that all its accumulated supermassive black holes eventually merged at the galactic center? A new study suggests that some of these giants might have escaped such a fate and they now wander unseen on wide orbits through their galaxies.Black Holes in an Evolving UniverseLed by Michael Tremmel (Yale Center for Astronomy Astrophysics), a team of scientists has used data from a large-scale cosmological simulation, Romulus25, to explore the possibility of wandering supermassive black holes. The Romulus simulations are uniquely suited to track the formation and subsequent orbital motion of supermassive black holes as galactic halos are built up through mergers over the history of the universe.From these simulations, Tremmel and collaborators find an end total of 316 supermassive black holes residing within the bounds of 26 Milky-Way-mass halos. Of these, roughly a third are wanderers within 10 kpc of the halo center (roughly the size of the Milky Ways disk).These wandering supermassive black holes were kicked onto wide orbits during the merger of their host galaxy with the main halo; Tremmel and collaborators find that their orbits are often tilted, lying outside of the galactic disk. Because these black holes travel through relatively deserted regions, they accumulate little mass and are rarely perturbed in their journeys, wandering for billions of years.Finding MonstersCumulative fraction of simulated Milky-Way-mass halos as a function of the number of supermassive black holes they host. All of the halos host at least one SMBH within 10 kpc from halo center, but the majority host more than that. [Tremmel et al. 2018]Tremmel and collaborators simulations suggest that, regardless of its merger history, a Milky-Way-mass halo will end up with an average of 5 supermassive black holes within 10 kpc of the galaxy center, and an average of 12 within its larger virial radius! This means there could be a number of supermassive black holes just like the enormous Sgr A* at our galaxys core wandering the Milky Way unseen.So how can we find these invisible monsters? We already have some observational evidence in the form of offset and dual active galactic nuclei of non-central supermassive black holes in distant galaxies. As for nearby, our best bet is to look for tidal disruption events, the burps of emission that occur when an otherwise invisible black hole encounters a star or a cloud of gas.CitationMichael Tremmel et al 2018 ApJL 857 L22. doi:10.3847/2041-8213/aabc0a

A design approach for small vision-based autonomous vehicles

NASA Astrophysics Data System (ADS)

Edwards, Barrett B.; Fife, Wade S.; Archibald, James K.; Lee, Dah-Jye; Wilde, Doran K.

2006-10-01

This paper describes the design of a small autonomous vehicle based on the Helios computing platform, a custom FPGA-based board capable of supporting on-board vision. Target applications for the Helios computing platform are those that require lightweight equipment and low power consumption. To demonstrate the capabilities of FPGAs in real-time control of autonomous vehicles, a 16 inch long R/C monster truck was outfitted with a Helios board. The platform provided by such a small vehicle is ideal for testing and development. The proof of concept application for this autonomous vehicle was a timed race through an environment with obstacles. Given the size restrictions of the vehicle and its operating environment, the only feasible on-board sensor is a small CMOS camera. The single video feed is therefore the only source of information from the surrounding environment. The image is then segmented and processed by custom logic in the FPGA that also controls direction and speed of the vehicle based on visual input.

Poverty, violence, and family disorganization: Three "Hydras" and their role in children's street movement in Bangladesh.

PubMed

Reza, Md Hasan

2016-05-01

The increasing number of children running away from home in Bangladesh is a major concern, and in need of critical attention. This yearlong study explores why children leave home with a sample of street children in Dhaka, Bangladesh. Purposive sampling from three locations in Dhaka yielded a sample of 75 homeless children aged 10-17. For each participant, a 60-90min in-depth qualitative interview was conducted multiple times. While the dominant explanations rely on poverty or abuse, the findings of this study reveal that the cause is actually three heads of a Hydra monster: poverty, abuse, and family disorganization and their interactions. It shows that the primary reasons for children breaking from their family are all interrelated. The findings from this study are likely to add knowledge regarding the issues and may lead to preventative interventions for street children and their families. Copyright © 2016 Elsevier Ltd. All rights reserved.

Einstein in Hollywood: Capturing the Scientific Minds of Movie Buffs

NASA Astrophysics Data System (ADS)

Young, Chadwick

2010-10-01

The film industry captures the minds of most students today. Americans spend one-half of their leisure time watching television, and students may often neglect their studies to catch the latest episode of Desperate Housewives or the new release of Leatherheads. Science teachers are challenged to compete with these seemingly unconquerable forces. One alternative to battling the influence of multimedia in its onslaught against the scientific minds of our youth is to embrace these monsters and tame them. By relating what the students know best (who kissed who in Walk the Line) with what they know least (thermodynamics, e.g.), teachers form connections in the minds of their students that will last for many years. In this session, the presenter will demonstrate an inquiry-based method employing clips from popular movies to learn physics. He will show movie clips from several different areas of physics, examine the particular clips in light of those physical principles, and discuss how to use the clips in the classroom.

BPS algebras, genus zero and the heterotic Monster

NASA Astrophysics Data System (ADS)

Paquette, Natalie M.; Persson, Daniel; Volpato, Roberto

2017-10-01

In this note, we expand on some technical issues raised in (Paquette et al 2016 Commun. Number Theory Phys. 10 433-526) by the authors, as well as providing a friendly introduction to and summary of our previous work. We construct a set of heterotic string compactifications to 0  +  1 dimensions intimately related to the Monstrous moonshine module of Frenkel, Lepowsky, and Meurman (and orbifolds thereof). Using this model, we review our physical interpretation of the genus zero property of Monstrous moonshine. Furthermore, we show that the space of (second-quantized) BPS-states forms a module over the Monstrous Lie algebras mg —some of the first and most prominent examples of Generalized Kac-Moody algebras—constructed by Borcherds and Carnahan. In particular, we clarify the structure of the module present in the second-quantized string theory. We also sketch a proof of our methods in the language of vertex operator algebras, for the interested mathematician.

Monster Clusters in the Young Universe? Weak-lensing Masses of SPT-CL J0205-5829 and MOO1014+0038 with HST Observations

NASA Astrophysics Data System (ADS)

Feilx Kim, Seojin; Jee, Myungkook James

2018-01-01

Measuring High-z clusters’ masses is very important as the cluster abundance is extremely sensitive to the cosmological parameters. However, deriving their masses from the intracluster medium properties (i.e., Sunyaev-Zel’dovich or X-ray observations) is not the best method because of their departure from the hydrostatic equilibrium. Fortunately, the “See Change” Hubble Space Telescope program offers a rare opportunity to measure them using weak gravitational lensing. We study SPT-CL J0205-5829 (z=1.322) and MOO1014+0038 (z=1.24) discovered in the SPT-SZ and MaDCoW Surveys, respectively. Previous non-lensing based approaches suggest that both targets might be extremely massive clusters. After carefully addressing various possible systematics from the Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3) images, we successfully detect clear weak lensing signals. We present their 2-dimensional mass maps and compare our weak-lensing masses with previous ICM-based results.

[Monsters of Phlegon--hermaphrodites, sex-changers and other strange beings in Phlegon's marvellous stories].

PubMed

Pataricza, Dóra

2010-01-01

The 1st-2nd century greek writer, Phlegon was a representative of the genre "paradoxography". In his book entitled Peri thaumasion (Book of wonders) he collected 35 extraordinary stories among which he described hermaphrodites, sex-changers and strange births. Phlegon's stories are only a part of the more than 79 ancient writings from Greek and Roman literature that describe children born with congenital defects. The article discusses the aspects of hermaphroditism in ancient times as well as ancient teratology. These stories might have had a core of truth. Although it is extremely difficult to identify a single potential cause for it, already ancient writers tried to give an explanation. With the help of modern teratology sciences many teratogenous causes can be partly identified. A part of the most probable factors among these were the same as today: malnutrition, viruses, alcohol, vitamin deficiencies etc., but lead poisoning has also be taken into account as a principal cause.

Improving Children’s Knowledge of Fraction Magnitudes

PubMed Central

Fazio, Lisa K.; Kennedy, Casey A.; Siegler, Robert S.

2016-01-01

We examined whether playing a computerized fraction game, based on the integrated theory of numerical development and on the Common Core State Standards’ suggestions for teaching fractions, would improve children’s fraction magnitude understanding. Fourth and fifth-graders were given brief instruction about unit fractions and played Catch the Monster with Fractions, a game in which they estimated fraction locations on a number line and received feedback on the accuracy of their estimates. The intervention lasted less than 15 minutes. In our initial study, children showed large gains from pretest to posttest in their fraction number line estimates, magnitude comparisons, and recall accuracy. In a more rigorous second study, the experimental group showed similarly large improvements, whereas a control group showed no improvement from practicing fraction number line estimates without feedback. The results provide evidence for the effectiveness of interventions emphasizing fraction magnitudes and indicate how psychological theories and research can be used to evaluate specific recommendations of the Common Core State Standards. PMID:27768756

"Ordinary men" or "evil monsters"? An action systems model of genocidal actions and characteristics of perpetrators.

PubMed

Hollows, Kerrilee; Fritzon, Katarina

2012-10-01

This study aimed to address the limitations of the existing genocide literature with the development of an empirically based classification system. Using Shye's (1985) action systems model, it was hypothesized that four types of perpetrators would exist and would be distinguishable by differences in the sources and target of individual criminal actions. Court transcripts from 80 perpetrators sentenced by the international courts were subject to content analysis and revealed 39 offense action variables, 17 perpetrator characteristic variables, and 6 perpetrator motive variables. A smallest space analysis using the Jaccard coefficient of association was conducted on the offense variables. The results supported the proposed framework, producing four distinct types of genocidal perpetrators. Correlational analyses were then conducted to examine the relationships between each of the perpetrator types and the remaining variables. The results of those correlations provided further support for the proposed framework. The implications of these findings are discussed. PsycINFO Database Record (c) 2012 APA, all rights reserved.

Mast Cells and IgE can Enhance Survival During Innate and Acquired Host Responses to Venoms*

PubMed Central

GALLI, STEPHEN J.; STARKL, PHILIPP; MARICHAL, THOMAS; TSAI, MINDY

2017-01-01

Mast cells and immunoglobulin E (IgE) antibodies are thought to promote health by contributing to host responses to certain parasites, but other beneficial functions have remained obscure. Venoms provoke innate inflammatory responses and pathology reflecting the activities of the contained toxins. Venoms also can induce allergic sensitization and development of venom-specific IgE antibodies, which can predispose some subjects to exhibit anaphylaxis upon subsequent exposure to the relevant venom. We found that innate functions of mast cells, including degradation of venom toxins by mast cell–derived proteases, enhanced survival in mice injected with venoms from the honeybee, two species of scorpion, three species of poisonous snakes, or the Gila monster. We also found that mice injected with sub-lethal amounts of honeybee or Russell’s viper venom exhibited enhanced survival after subsequent challenge with potentially lethal amounts of that venom, and that IgE antibodies, FcεRI, and probably mast cells contributed to such acquired resistance. PMID:28790503

Time to Redefine Organic Agriculture: Can’t GM Crops Be Certified as Organics?

PubMed Central

Husaini, Amjad M.; Sohail, Muhammad

2018-01-01

The challenges of sustainable food production without damaging the environment for a growing human population have increased considerably. The current agricultural practices involving chemical fertilizers and even organic farming are not sustainable in the long run and can have deleterious effects on the environment. Thus, new, innovative solutions need to be identified and propagated for tackling this. Among such innovations, that can complement conventional as well as organic farming methods, are genetic modification (GM) and aquaculture. Yet, GM technologies often face resistance from civil groups owing to an ‘unknown’ fear, akin to Frankenstein’s monster. How real is this fear? Our discussion rests on basic questions like, why can’t ‘organics’ include GM crops that do not require chemical inputs for cultivation, and can GM crops like Golden rice qualify to be ‘organic’ if cultivated through organic practices? Do we need to rethink organic agriculture in the context of the present and future challenges of 21st century? PMID:29692789

Time to Redefine Organic Agriculture: Can't GM Crops Be Certified as Organics?

PubMed

Husaini, Amjad M; Sohail, Muhammad

2018-01-01

The challenges of sustainable food production without damaging the environment for a growing human population have increased considerably. The current agricultural practices involving chemical fertilizers and even organic farming are not sustainable in the long run and can have deleterious effects on the environment. Thus, new, innovative solutions need to be identified and propagated for tackling this. Among such innovations, that can complement conventional as well as organic farming methods, are genetic modification (GM) and aquaculture. Yet, GM technologies often face resistance from civil groups owing to an 'unknown' fear, akin to Frankenstein's monster. How real is this fear? Our discussion rests on basic questions like, why can't 'organics' include GM crops that do not require chemical inputs for cultivation, and can GM crops like Golden rice qualify to be 'organic' if cultivated through organic practices? Do we need to rethink organic agriculture in the context of the present and future challenges of 21st century?

Sonoran Desert: Fragile Land of Extremes

USGS Publications Warehouse

Produced and Directed by Wessells, Stephen

2003-01-01

'Sonoran Desert: Fragile Land of Extremes' shows how biologists with the U.S. Geological Survey work with other scientists in an effort to better understand native plants and animals such as desert tortoises, saguaro cacti, and Gila monsters. Much of the program was shot in and around Saguaro National Park near Tucson, Arizona. Genetic detective work, using DNA, focuses on understanding the lives of tortoises. Studies of saguaros over many decades clarify how these amazing plants reproduce and thrive in the desert. Threats from fire, diseases in tortoises, and a growing human population motivate the scientists. Their work to identify how these organisms live and survive is a crucial step for the sound management of biological resources on public lands. This 28-minute program, USGS Open-File Report 03-305, was shot entirely in high definition video and produced by the USGS Western Ecological Research Center and Southwest Biological Science Center; produced and directed by Stephen Wessells, Western Region Office of Communications.

Rogue Waves in the Ocean

NASA Astrophysics Data System (ADS)

Waseda, Takuji

2010-03-01

Giant episodic ocean waves that suddenly soar like a wall of water out of an otherwise calm sea are not just a legend. Such waves—which in the past have been called “abnormal,” “exceptional,” “extreme,” and even “vicious killer” waves—are now commonly known as “rogue waves” or “freak waves.” These waves have sunk or severely damaged 22 supercarriers in the world and caused the loss of more than 500 lives in the past 40 years. The largest wave registered by reliable instruments reached 30 meters in height, and the largest wave recorded by visual observation reached about 34 meters, equivalent to the height of an eight-story building. Tales of seafarers from Christopher Columbus to the passengers of luxury cruise ships had long been undervalued by scientists, but in the past 10 or so years, those historical notes and modern testimonies have been scientifically dissected to reveal the nature of these monster waves.

Chasing the Late Jurassic APW Monster Shift in Ontario Kimberlites

NASA Astrophysics Data System (ADS)

Kent, D. V.; Muttoni, G.; Gee, J. S.; Kjarsgaard, B. A.

2012-12-01

A 30° gap was recognized in a composite APW path when global poles from predominantly igneous rocks were assembled in North American coordinates using plate reconstructions (Kent & Irving 2010 JGR). The 'monster shift' occurred between a 160-190 Ma cluster of mean poles at 75-80°N 90-110°E to a 140-145 Ma grouping centered at 60-65°N ~200°E. There are hardly any intermediate igneous poles whereas the rather divergent directions from the Late Jurassic Morrison Formation published by Steiner & Helsley (1975 GSA Bulletin) are subject to adjustments for Colorado Plateau rotation and sedimentary inclination error, neither of which are precisely known for this redbed unit sampled in Colorado. On the other hand, similar large rapid swings have been recognized in the Late Jurassic APW path for Adria (Channell et al. 2010 Paleo3), suggesting a global phenomena. In an effort to fill the data gap between ~145 and 160 Ma, we sampled accessible outcrops/subcrops of kimberlites in the Timiskaming area of Ontario, Canada, that are associated with high precision U-Pb perovskite ages (Heamon & Kjarsgaard 2000 EPSL). We report initial results from two of the intrusions: the 153.6±2.4 Ma Peddie kimberlite from outcrop and the Triple B kimberlite that was accessible by trenching and is assumed to be the same age as the nearby 153.7±1.8 Ma Seed kimberlite as delineated by aeromagnetic surveys and borings. Systematic progressive thermal demagnetization indicated in each unit a dominant characteristic component with unblocking temperatures to 575° that presumably reflect a magnetite carrier that will be checked by further rock magnetic experiments. Samples from the Peddie kimberlite had stable downward (normal polarity) magnetizations whose mean direction gives a paleopole at 73°N 184°E. In contrast, samples from the Triple B kimberlite have upward (reverse polarity) magnetizations with a well-grouped direction whose (north) paleopole is 78°N 197°E, proximal to the Peddie pole. The normal and reverse polarities suggest that sufficient time elapsed between emplacement of the Triple B and Peddie to give an opportunity to average secular variation. The combined ~154 Ma Triple B and Peddie pole encouragingly lies about halfway between igneous poles from North America nearest in age: the 169 Ma Moat volcanics and the 142 Ma Ithaca kimberlites. However, preliminary paleomagnetic results from some of the other sampled kimberlite bodies are more problematical and require further paleomagnetic and geochronological work.

Dance of Two Monster Black Holes

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2016-03-01

This past December, researchers all over the world watched an outburst from the enormous black hole in OJ 287 an outburst that had been predicted years ago using the general theory of relativity.Outbursts from Black-Hole OrbitsOJ 287 is one of the largest supermassive black holes known, weighing in at 18 billion solar masses. Located about 3.5 billion light-years away, this monster quasar is bright enough that it was first observed as early as the 1890s. What makes OJ 287 especially interesting, however, is that its light curve exhibits prominent outbursts roughly every 12 years.Diagram illustrating the orbit of the secondary black hole (shown in blue) in OJ 287 from 2000 to 2023. We see outbursts (the yellow bubbles) every time the secondary black hole crosses the accretion disk (shown in red, ina side view) surrounding the primary (the black circle). [Valtonen et al. 2016]What causes the outbursts? Astronomers think that there is a second supermassive black hole, ~100 times smaller, inspiraling as it orbits the central monster and set to merge within the next 10,000 years. In this model, the primary black hole of OJ 287 is surrounded by a hot accretion disk. As the secondary black hole orbits the primary, it regularly punches through this accretion disk, heating the material and causing the release of expanding bubbles of hot gas pulled from the disk. This gas then radiates thermally, causing the outbursts we see.Attempts to model this scenario using Newtonian orbits all fail; the timing of the secondary black holes crossings through the accretion disk (as measured by when we see the outbursts) can only be explained by a model incorporating general-relativistic effects on the orbit. Careful observations and precise timing of these outbursts therefore provide an excellent test of general relativity.Watching a Predicted CrossingThe model of OJ 287 predicted another disk crossing in December 2015, so professional and amateur astronomers around the world readied more than two dozen ground-based optical telescopes and the Swift/XRT satellite to observe OJ 287 in this time frame. The outburst occurred right on schedule, peaking on 5 December 2015, and the results of the observing campaign are now presented in a study led by Mauri Valtonen (University of Turku).Optical photometry of OJ 287 from October to December 2015, showing the outburst that resulted from the secondary black hole crossing the disk. [Valtonen et al. 2016]Because the secondary black holes orbit is affected by the spin of the primary black hole, Valtonen and collaborators were able to use the timing of the outburst to measure the spin of OJ 287s primary black hole to remarkably high precision. They find that its Kerr parameter is 0.313 0.01 which means its spinning at about a third of the maximum rate allowed by general relativity.The outburst timing also confirmed several general-relativistic properties of the system, including its loss of energy to gravitational waves. Remarkably, the energy lost as the secondary black hole punches through the accretion disk is still ten thousand times smaller than the amount of energy it loses through gravitational waves!The observations from this outburst have provided important black-hole measurements and tests of general relativity which are especially relevant in this new era of gravitational wave detections. And we may be able to perform still more tests on the secondarys next pass through the disk, which should occur in 2019.BonusCheck out this awesome animation of the orbits in a system similar to OJ 287! The secondarys orbit precesses around the primary due to general-relativistic effects. The sound you hearis an audio representation of the increasing frequency as the two black holes inspiral. You can find more information about this animation here. [Steve Drasco Curt Cutler]CitationM. J. Valtonen et al 2016 ApJ 819 L37. doi:10.3847/2041-8205/819/2/L37

More information than you ever wanted: does Facebook bring out the green-eyed monster of jealousy?

PubMed

Muise, Amy; Christofides, Emily; Desmarais, Serge

2009-08-01

The social network site Facebook is a rapidly expanding phenomenon that is changing the nature of social relationships. Anecdotal evidence, including information described in the popular media, suggests that Facebook may be responsible for creating jealousy and suspicion in romantic relationships. The objectives of the present study were to explore the role of Facebook in the experience of jealousy and to determine if increased Facebook exposure predicts jealousy above and beyond personal and relationship factors. Three hundred eight undergraduate students completed an online survey that assessed demographic and personality factors and explored respondents' Facebook use. A hierarchical multiple regression analysis, controlling for individual, personality, and relationship factors, revealed that increased Facebook use significantly predicts Facebook-related jealousy. We argue that this effect may be the result of a feedback loop whereby using Facebook exposes people to often ambiguous information about their partner that they may not otherwise have access to and that this new information incites further Facebook use. Our study provides evidence of Facebook's unique contributions to the experience of jealousy in romantic relationships.

Radio Identifications of UGC Galaxies - Starbursts and Monsters

NASA Astrophysics Data System (ADS)

Condon, J. J.; Broderick, J. J.

1995-11-01

Radio identifications of galaxies in the Uppsala General Catalogue of Galaxies with delta < +82 degrees were made from the Green Bank 1400 MHz sky maps. Every source having peak flux density S(P) >= 150 mJy in the approximately 12 arcmin FWHM map point-source response and position < 5 arcmin in both coordinates from the optical position of any UGC galaxy was considered a candidate identification to ensure that very extended (up to 1 Mpc) and asymmetric sources would not be missed. Maps in the literature or new 1.49 GHz VLA C-array maps made with 18 arcsec FWHM resolution were used to confirm or reject candidate identifications. The maps in this directory include both confirmed identifications and candidates rejected because of confusion or low flux density. For more information on this study, please see the following reference: Condon, J. J., and Broderick, J. J., 1988, AJ, 96, 30. The images and related TeX file come from the NRAO CDROM "Images From the Radio Universe" (c. 1992 National Radio Astronomy Observatory, used with permission).

Dogs and Monsters: Moral Status Claims in the Fiction of Dean Koontz.

PubMed

Smith, Stephen W

2016-03-01

This article explores conceptions of moral status in the work of American thriller author Dean Koontz. It begins by examining some of the general theories of moral status used by philosophers to determine whether particular entities have moral status. This includes both uni-criterial theories and multi-criterial theories of moral status. After this examination, the article argues for exploring bioethics conceptions in popular fiction. Popular fiction is considered a rich source for analysis because it provides not only a good approximation of the beliefs of ordinary members of the moral community, but also explores important issues in a context where ordinary individuals are likely to encounter them. Following on from this, the article then explores theories of moral status in the context of Koontz's novels. In particular, the article focuses on the novel Watchers and Koontz's Frankenstein series. Through these works, Koontz indicates that entities have moral status for a variety of reasons and thus presumably, he is a proponent of multi-criterial theories of moral status. The article concludes with an examination of what this might mean for our understanding of moral status claims generally.

Bidirectional tornado modes on the Joint European Torus

DOE Office of Scientific and Technical Information (OSTI.GOV)

Sandquist, P.; Sharapov, S. E.; Lisak, M.

In discharges on the Joint European Torus [P. H. Rebut and B. E. Keen, Fusion Technol. 11, 13 (1987)] with safety factor q(0)<1 and high-power ion cyclotron resonance heating (ICRH), monster sawtooth crashes are preceded by frequency sweeping 'tornado modes' in the toroidal Alfven eigenmode frequency range. A suite of equilibrium and spectral magnetohydrodynamical codes is used for explaining the observed evolution of the tornado mode frequency and for identifying temporal evolution of the safety factor inside the q=1 radius just before sawtooth crashes. In some cases, the tornado modes are observed simultaneously with both positive and negative toroidal modemore » numbers. Hence, a free energy source other than the radial gradient of the energetic ion pressure exciting these modes is sought. The distribution function of the ICRH-accelerated ions is assessed with the SELFO code [J. Hedin et al., Nucl. Fusion 42, 527 (2002)] and energetic particle drive due to the velocity space anisotropy of ICRH-accelerated ions is considered analytically as the possible source for excitation of bidirectional tornado modes.« less

The effects of energy beverages in counteracting the symptoms of mild hypoxia at legal general aviation altitudes

NASA Astrophysics Data System (ADS)

Bull, Daniel Mark

The purpose of this thesis was to conduct preliminary research, in the form of a pilot study, concerning the natural effects of hypoxia compared to the effects of hypoxia experienced after the consumption of an energy beverage. The study evaluated the effects of hypoxia on FAA certificated pilots at a simulated legal general aviation altitude, utilizing the normobaric High Altitude Lab (HAL) located at Embry Riddle Aeronautical University, Daytona Beach, Florida. The researcher tested 11 subjects, who completed three simulated flight tasks within the HAL using the Frasca International Mentor Advanced Aviation Training Device (AATD). The flight tasks were completed after consuming Red BullRTM, MonsterRTM , or a placebo beverage. The researcher derived three test variables from core outputs of the AATD: lateral deviations from the glide slope, vertical deviations from the localizer, and airspeed deviations from the target speed of 100 knots. A repeated-measures ANOVA was carried out to determine effects of the beverages on the test variables. While results were non-significant, the researcher concluded that further research should be conducted with a larger sample.

A Monster CME Obscuring a Demon Star Flare

NASA Astrophysics Data System (ADS)

Moschou, Sofia-Paraskevi; Drake, Jeremy J.; Cohen, Ofer; Alvarado-Gomez, Julian D.; Garraffo, Cecilia

2017-12-01

We explore the scenario of a coronal mass ejection (CME) being the cause of the observed continuous X-ray absorption of the 1997 August 30 superflare on the eclipsing binary Algol (the Demon Star). The temporal decay of the absorption is consistent with absorption by a CME undergoing self-similar evolution with uniform expansion velocity. We investigate the kinematic and energetic properties of the CME using the ice cream cone model for its three-dimensional structure in combination with the observed profile of the hydrogen column density decline with time. Different physically justified length scales were used that allowed us to estimate lower and upper limits of the possible CME characteristics. Further consideration of the maximum available magnetic energy in starspots leads us to quantify its mass as likely lying in the range 2× {10}21 {--} 2× {10}22 g and kinetic energy in the range 7× {10}35 {--} 3× {10}38 erg. The results are in reasonable agreement with extrapolated relations between flare X-ray fluence and CME mass and kinetic energy derived for solar CMEs.

Star formation in Herschel's Monsters versus semi-analytic models

NASA Astrophysics Data System (ADS)

Gruppioni, C.; Calura, F.; Pozzi, F.; Delvecchio, I.; Berta, S.; De Lucia, G.; Fontanot, F.; Franceschini, A.; Marchetti, L.; Menci, N.; Monaco, P.; Vaccari, M.

2015-08-01

We present a direct comparison between the observed star formation rate functions (SFRFs) and the state-of-the-art predictions of semi-analytic models (SAMs) of galaxy formation and evolution. We use the PACS Evolutionary Probe Survey and Herschel Multi-tiered Extragalactic Survey data sets in the COSMOS and GOODS-South fields, combined with broad-band photometry from UV to sub-mm, to obtain total (IR+UV) instantaneous star formation rates (SFRs) for individual Herschel galaxies up to z ˜ 4, subtracted of possible active galactic nucleus (AGN) contamination. The comparison with model predictions shows that SAMs broadly reproduce the observed SFRFs up to z ˜ 2, when the observational errors on the SFR are taken into account. However, all the models seem to underpredict the bright end of the SFRF at z ≳ 2. The cause of this underprediction could lie in an improper modelling of several model ingredients, like too strong (AGN or stellar) feedback in the brighter objects or too low fallback of gas, caused by weak feedback and outflows at earlier epochs.

Hubble Hones In on a Hypergiant's Home

NASA Image and Video Library

2017-12-08

This beautiful Hubble image reveals a young super star cluster known as Westerlund 1, only 15,000 light-years away in our Milky Way neighborhood, yet home to one of the largest stars ever discovered. Stars are classified according to their spectral type, surface temperature, and luminosity. While studying and classifying the cluster’s constituent stars, astronomers discovered that Westerlund 1 is home to an enormous star. Originally named Westerlund 1-26, this monster star is a red supergiant (although sometimes classified as a hypergiant) with a radius over 1,500 times that of our sun. If Westerlund 1-26 were placed where our sun is in our solar system, it would extend out beyond the orbit of Jupiter. Most of Westerlund 1’s stars are thought to have formed in the same burst of activity, meaning that they have similar ages and compositions. The cluster is relatively young in astronomical terms —at around three million years old it is a baby compared to our own sun, which is some 4.6 billion years old. Credit: ESA/Hubble & NASA

[Was cannibalism practiced in ancient Gaul? Critognatus, the leader of the Celts, in the focus of Caesar's propaganda].

PubMed

Moog, Ferdinand Peter

2011-01-01

Critognatus, the leader of the Celts, is mentioned only once in the extant ancient literature, namely in Caesar's description of the siege of Alesia in BG VII 77.2-78.2. Here he is portrayed as a determined patriot who wants to encounter the Roman invader bravely and at the risk of all available means. Nevertheless, crafty Caesar succeeds in stamping him by propagandistic pinches to an evil monster and cannibal. On the one hand Caesar falls back on current Roman prejudices towards the Gauls. On the other hand, the endocannibalism practised among Celts to a certain extent as a cult action seems to have played a rôle. Caesar's propagandistic methods are transparent and at the same time so effective that the label of an ogre sticks to Critognatus until the present day. Caesar's portrayal aims above all at the justification of his Gallic War which he wages against uncivilized and inhuman opponents who are a menace to Rome and even to the culture itself.

The Green Monster: Stokes's 1944 Modern Clinical Syphilology.

PubMed

Jackson, Robert

2010-01-01

There is much information on the life and accomplishments of John Hinchman Stokes (1885-1961), the dermatologist and syphilologist. There is little detailed information on his 1944 classic text on syphilis, Modern Clinical Syphilology. To review and critique this book. A careful review of the book, his life, and the accomplishments that were undertaken in relation to the age in which he lived. The book is indeed a goldmine of information of all aspects of syphilis from pre-World War I (1905) until the late (1944) World War II era. The factors that make it a classic are as follows: (1) the disease had a specific cause; (2) Stokes's 25-year obsession with the disease; (3) there was no effective simple cure for most of the time he was studying it; (4) Stokes was an obsessive, intelligent, well-trained physician; (5) he lived in a well-developed, reasonably stable country; and (6) he was able to see how the disease could be adequately treated with penicillin and compare these events with those in the prepenicillin era.

In Search of a Cure for Sepsis: Taming the Monster in Critical Care Medicine.

PubMed

Okeke, Emeka B; Uzonna, Jude E

2016-01-01

In spite of over half a century of research, sepsis still constitutes a major problem in health care delivery. Although advances in research have significantly increased our knowledge of the pathogenesis of sepsis and resulted in better prognosis and improved survival outcome, sepsis still remains a major challenge in modern medicine with an increase in occurrence predicted and a huge socioeconomic burden. It is generally accepted that sepsis is due to an initial hyperinflammatory response. However, numerous efforts aimed at targeting the proinflammatory cytokine network have been largely unsuccessful and the search for novel potential therapeutic targets continues. Recent studies provide compelling evidence that dysregulated anti-inflammatory responses may also contribute to sepsis mortality. Our previous studies on the role of regulatory T cells and phosphoinositide 3-kinases in sepsis highlight immunological approaches that could be explored for sepsis therapy. In this article, we review the current and emerging concepts in sepsis, highlight novel potential therapeutic targets and immunological approaches for sepsis treatment and propose a biphasic treatment approach for management of the condition. © 2016 S. Karger AG, Basel.

EVIDENCE OF MAGNETIC FIELD SWITCH-OFF IN COLLISIONLESS MAGNETIC RECONNECTION

DOE Office of Scientific and Technical Information (OSTI.GOV)

Innocenti, M. E.; Lapenta, G.; Goldman, M.

2015-09-10

The long-term evolution of large domain particle-in-cell simulations of collisionless magnetic reconnection is investigated following observations that show two possible outcomes for collisionless reconnection: toward a Petschek-like configuration or toward multiple X points. In the present simulation, a mixed scenario develops. At earlier time, plasmoids are emitted, disrupting the formation of Petschek-like structures. Later, an almost stationary monster plasmoid forms, preventing the emission of other plasmoids. A situation reminiscent of Petschek’s switch-off then ensues. Switch-off is obtained through a slow shock/rotational discontinuity compound structure. Two external slow shocks (SS) located at the separatrices reduce the in-plane tangential component of themore » magnetic field, but not to zero. Two transitions reminiscent of rotational discontinuities (RD) in the internal part of the exhaust then perform the final switch-off. Both the SS and the RD are characterized through analysis of their Rankine–Hugoniot jump conditions. A moderate guide field is used to suppress the development of the firehose instability in the exhaust.« less

Rogue waves in the ocean - review and progress

NASA Astrophysics Data System (ADS)

Pelinovsky, Efim; Kharif, Christian; Slunyaev, Alexey

2010-05-01

Rogue waves in the ocean and physical mechanisms of their appearance are discussed. Theyse waves are among waves naturally observed by people on the sea surface that represent inseparable feature of the Ocean. Rogue waves appear from nowhere, cause danger and disappear at once. They may occur at the surface of a relatively calm sea, reach not very high amplitudes, but be fatal for ships and crew due to their unexpectedness and abnormal features. The billows appear suddenly exceeding the surrounding waves twice and more, and obtained many names: abnormal, exceptional, extreme, giant, huge, sudden, episodic, freak, monster, rogue, vicious, killer, mad- or rabid-dog waves; cape rollers, holes in the sea, walls of water, three sisters… Freak monsters, though living for seconds, were able to arouse superstitious fear of the crew, cause damage, death of heedless sailors or the whole ship. All these epithets are full of human fear and feebleness. The serious studies of the phenomenon started about 20-30 years ago and have been intensified during the recent decade. The research is being conducted in different fields: in physics (search of physical mechanisms and adequate models of wave enhancement and statistics), in geoscience (determining the regions and weather conditions when rogue waves are most probable), and in ocean and coastal engineering (estimations of the wave loads on fixed and drifting floating structures). Thus, scientists and engineers specializing in different subject areas are involved in the solution of the problem. The state-of-art of the rogue wave study is summarized in our book [Kharif, Ch., Pelinovsky, E., and Slunyaev, A. Rogue Waves in the Ocean. Springer, 2009] and presented in given review. Firstly, we start with a brief introduction to the problem of freak waves aiming at formulating what is understood as rogue or freak waves, what consequences their existence imply in our life, why people are so worried about them. Then we discuss existing observations and measurements of freak waves. Two approaches to the rogue wave description (deterministic and statistical) are presented. Briefly, the physical mechanisms that have been already suggested as possible explanations of the freak wave phenomenon are: i) wave-current interaction; ii) geometrical (spatial) focusing; iii) focusing due to dispersion (spatio-temporal focusing); iv) focusing due to modulational instability; v) soliton collision; vi) atmospheric action. In conclusion we emphasize that most of the developed theories are applicable to other physical phenomena starting from ocean waves of different nature and ending with nonlinear optics (for instance optical rogue waves in fibers) and astrophysical plasma processes. The recent trends in study of the oceanic rogue waves are discussed as well.

Thalidomide and the Titanic: reconstructing the technology tragedies of the twentieth century.

PubMed

Annas, G J; Elias, S

1999-01-01

The Titanic has become a metaphor for the disastrous consequences of an unqualified belief in the safety and invincibility of new technology. Similarly, the thalidomide tragedy stands for all of the "monsters" that can be inadvertently or negligently created by modern medicine. Thalidomide, once banned, has returned to the center of controversy with the Food and Drug Administration's (FDA's) announcement that thalidomide will be placed on the market for the treatment of erythema nodosum leprosum, a severe dermatological complication of Hansen's disease. Although this indication is very restricted, thalidomide will be available for off-label uses once it is on the market. New laws regarding abortion and a new technology, ultrasound, make reasonable the approval of thalidomide for patients who suffer from serious conditions it can alleviate. In addition, the FDA and the manufacturer have proposed the most stringent postmarketing monitoring ever used for a prescription drug, including counseling, contraception, and ultrasonography in the event of pregnancy. The Titanic/thalidomide lesson for the FDA and public health is that rules and guidelines alone are not sufficient to guarantee safety. Continuous vigilance will be required to ensure that all reasonable postmarketing monitoring steps are actually taken to avoid predictable and preventable teratogenic disasters.

Structural Aberrations in T-Even Bacteriophage V. Effects of Canavanine on the Maturation and Utilization of Specific Gene Products

PubMed Central

Bolin, Rex W.; Cummings, Donald J.

1974-01-01

Previous results have shown that when a T-even bacteriophage-infected cell was exposed to l-canavanine followed by an exposure to l-arginine, a monster phage particle, termed a lollipop, was formed. l-Canavanine was necessary for the induction event but l-arginine was required for the maturation of the particle. We now describe the effects of canavanine on the maturation of certain T4 proteins and their role in the induction of lollipops. The cleavage reactions of the head proteins P22, P23, P24, and IPIII are prevented by l-canavanine as shown by the accumulation of the precursor proteins and the failure of the cleaved products to appear. l-Canavanine also prevents the appearance of P12 (tailplate protein) and P20 (head protein) indicating that these proteins may undergo a proteolytic cleavage during normal assembly. The formation of P10 (tailplate protein) and P18 (tail sheath protein) is also affected by l-canavanine. The data suggest that P23 in conjunction with P20 plays a major role in the determination of the length of the phage head. Images PMID:4833614

'Here There Be Monsters': the public's perception of paedophiles with particular reference to Belfast and Leicester.

PubMed

McCartan, Kieran

2004-10-01

This research study sought to investigate the public perception of paedophiles. It was undertaken in Belfast (Northern Ireland) and Leicester (England) in an attempt to determine whether or not regional variations existed in relation to the public's perception of paedophiles. In doing this, the study sought to test four hypotheses; (1) That the press affects the public's perception of paedophiles; (2) that the public's perception of paedophiles is not congruent with legal and clinical definitions; (3) that the Sarah Payne case has helped to reinforce the public's perception of a predatory paedophile; and (4) that the public's perception is based on fear and irrationality. These hypotheses were tested via the distribution of a questionnaire to an opportunistic sample on the streets of Belfast and Leicester. Although the results did not support the hypotheses, they did yield some very interesting information. The study indicated that the public is quite well-informed about paedophilia; its recurrence rates, practices and in particular the influence of the media. Furthermore, the study indicated quite significant differences between the cities of Belfast and Leicester. In conclusion, the results indicated that a moral panic connected to paedophilia is very present in our contemporary society.

Loch ness, special operations executive and the first surgeon in paradise: Robert Kenneth Wilson (26.1.1899-6.6.1969).

PubMed

Watters, David A K

2007-12-01

Lieutenant Colonel Robert Kenneth Wilson (1899-1969) was a surgeon who fought in both world wars and joined the Special Operations Executive parachuting behind enemy lines into Holland, France and Borneo, the last mission being with Australian forces (Semut II). He was an expert on firearms and gave opinion on ballistics at the Old Bailey during the 1930s. He also wrote a definitive text on automatic pistols with editions published in 1943 and 1975. He was an Edinburgh Fellow (1926), who had a practice in general surgery and gynaecology in Queen Anne Street during the 1930s. He took the famous 1934 'surgeon's photo' of the Loch Ness monster that was not admitted to be a hoax until 1994. After World War II, he became the first surgical specialist to work in the public service of the then Territory of Papua and New Guinea (1950-1956), where he wrote several papers on surgical topics. He married Gwen (1924), the daughter of Henrietta Gulliver, an Australian painter. They had two sons, Richard and Phillip. After practice he retired to Melbourne where he died of carcinoma oesophagus.

Visual perception during mirror-gazing at one's own face in patients with depression.

PubMed

Caputo, Giovanni B; Bortolomasi, Marco; Ferrucci, Roberta; Giacopuzzi, Mario; Priori, Alberto; Zago, Stefano

2014-01-01

In normal observers, gazing at one's own face in the mirror for a few minutes, at a low illumination level, produces the apparition of strange faces. Observers see distortions of their own faces, but they often see hallucinations like monsters, archetypical faces, faces of relatives and deceased, and animals. In this research, patients with depression were compared to healthy controls with respect to strange-face apparitions. The experiment was a 7-minute mirror-gazing test (MGT) under low illumination. When the MGT ended, the experimenter assessed patients and controls with a specifically designed questionnaire and interviewed them, asking them to describe strange-face apparitions. Apparitions of strange faces in the mirror were very reduced in depression patients compared to healthy controls. Depression patients compared to healthy controls showed shorter duration of apparitions; minor number of strange faces; lower self-evaluation rating of apparition strength; lower self-evaluation rating of provoked emotion. These decreases in depression may be produced by deficits of facial expression and facial recognition of emotions, which are involved in the relationship between the patient (or the patient's ego) and his face image (or the patient's bodily self) that is reflected in the mirror.

A new monster from southwest Oregon forests: Cryptomaster behemoth sp. n. (Opiliones, Laniatores, Travunioidea)

PubMed Central

Starrett, James; Derkarabetian, Shahan; Richart, Casey H.; Cabrero, Allan; Hedin, Marshal

2016-01-01

Abstract The monotypic genus Cryptomaster Briggs, 1969 was described based on individuals from a single locality in southwestern Oregon. The described species Cryptomaster leviathan Briggs, 1969 was named for its large body size compared to most travunioid Laniatores. However, as the generic name suggests, Cryptomaster are notoriously difficult to find, and few subsequent collections have been recorded for this genus. Here, we increase sampling of Cryptomaster to 15 localities, extending their known range from the Coast Range northeast to the western Cascade Mountains of southern Oregon. Phylogenetic analyses of mitochondrial and nuclear DNA sequence data reveal deep phylogenetic breaks consistent with independently evolving lineages. We use discovery and validation species delimitation approaches to generate and test species hypotheses, including a coalescent species delimitation method to test multi-species hypotheses. For delimited species, we use light microscopy and SEM to discover diagnostic morphological characters. Although Cryptomaster has a small geographic distribution, this taxon is consistent with other short-range endemics in having deep phylogenetic breaks indicative of species level divergences. Herein we describe Cryptomaster behemoth sp. n., and provide morphological diagnostic characters for identifying Cryptomaster leviathan and Cryptomaster behemoth. PMID:26877685

Monsters and the case of L. Joseph: André Feil's thesis on the origin of the Klippel-Feil syndrome and a social transformation of medicine.

PubMed

Belykh, Evgenii; Malik, Kashif; Simoneau, Isabelle; Yagmurlu, Kaan; Lei, Ting; Cavalcanti, Daniel D; Byvaltsev, Vadim A; Theodore, Nicholas; Preul, Mark C

2016-07-01

André Feil (1884-1955) was a French physician best recognized for his description, coauthored with Maurice Klippel, of patients with congenital fusion of cervical vertebrae, a condition currently known as Klippel-Feil syndrome. However, little is known about his background aside from the fact that he was a student of Klippel and a physician who took a keen interest in describing congenital anomalies. Despite the relative lack of information on Feil, his contributions to the fields of spinal disease and teratology extended far beyond science to play an integral role in changing the misguided perception shrouding patients with disfigurements, defects, deformities, and so-called monstrous births. In particular, Feil's 1919 medical school thesis on cervical abnormalities was a critical publication in defying long-held theory and opinion that human "monstrosities," anomalies, developmental abnormalities, and altered congenital physicality were a consequence of sinful behavior or a reversion to a primitive state. Indeed, his thesis on a spinal deformity centering on his patient, L. Joseph, was at the vanguard for a new view of a patient as nothing less than fully human, no matter his or her physicality or appearance.

Prime Astroarchaeological Researches near Mountain Monastyri in the Western Altai

NASA Astrophysics Data System (ADS)

Marsadolov, L.; Dmitrieva, N.

2009-08-01

On the Western Altai, 50 km southward from the city of Ust-Kamenogorsk, at the same latitude as the Ak-Baur sanctuary, another interesting complex of ancient objects was examined in 2006-2007. This complex consists of a grotto, ``spotty'' stone and platforms with holes. In the grotto anthropomorphic and geometric drawings madein red ochre were found. The centre of the composition schematically represents human figures with joined hands. One kilometer to the west from the complex there is a sharp-pointed mountain Zhangiztas. In its bottom part a ``zoomorphic'' ledge is visible; it reminds a sideview of a ``head with the opened mouth and tongue''. Observing the sunset on the days of equinox, one can watch the Sun ``setting down'' on the top of Mt. Zhangistas, then ``sliding'' along the right-side slope and finally ``rolling into the mouth''; in other words, it is ``swallowed by a monster''. The ``zoomorphic'' peculiarity of the mountain outliers (monad nocks) of the Monastyri complex as a whole and of their separate rocky juts was comprehended in the antiquity; the evidence for it is the presence of manmade holes near them; these holes might have an astronomical meaning.

Snake oil and venoms for medical research

NASA Astrophysics Data System (ADS)

Wolpert, H. D.

2011-04-01

Some think that using derivatives of snake venom for medical purposes is the modern version of snake oil but they are seriously misjudging the research potentials of some of these toxins in medicines of the 2000's. Medical trials, using some of the compounds has proven their usefulness. Several venoms have shown the possibilities that could lead to anticoagulants, helpful in heart disease. The blood clotting protein from the taipan snake has been shown to rapidly stop excessive bleeding. The venom from the copperhead may hold an answer to breast cancer. The Malaysian pit viper shows promise in breaking blood clots. Cobra venom may hold keys to finding cures for Parkinson's disease and Alzheimer's. Rattlesnake proteins from certain species have produced blood pressure medicines. Besides snake venoms, venom from the South American dart frog, mollusks (i.e. Cone Shell Snail), lizards (i.e. Gila Monster & Komodo Dragon), some species of spiders and tarantulas, Cephalopods, mammals (i.e. Platypus & Shrews), fish (i.e. sting rays, stone fish, puffer fish, blue bottle fish & box jelly fish), intertidal marine animals (echinoderms)(i.e. Crown of Thorn Star Fish & Flower Urchin) and the Honeybee are being investigated for potential medical benefits.

Two Major Bile Acids in the Hornbills, (24R,25S)-3α,7α,24-Trihydroxy-5β-cholestan-27-oyl Taurine and Its 12α-Hydroxy Derivative.

PubMed

Satoh, Rika; Ogata, Hiroaki; Saito, Tetsuya; Zhou, Biao; Omura, Kaoru; Kurabuchi, Satoshi; Mitamura, Kuniko; Ikegawa, Shigeo; Hagey, Lee R; Hofmann, Alan F; Iida, Takashi

2016-06-01

Two major bile acids were isolated from the gallbladder bile of two hornbill species from the Bucerotidae family of the avian order Bucerotiformes Buceros bicornis (great hornbill) and Penelopides panini (Visayan tarictic hornbill). Their structures were determined to be 3α,7α,24-dihydroxy-5β-cholestan-27-oic acid and its 12α-hydroxy derivative, 3α,7α,12α,24-tetrahydroxy-5β-cholestan-27-oic acid (varanic acid, VA), both present in bile as their corresponding taurine amidates. The four diastereomers of varanic acid were synthesized and their assigned structures were confirmed by X-ray crystallographic analysis. VA and its 12-deoxy derivative were found to have a (24R,25S)-configuration. 13 additional hornbill species were also analyzed by HPLC and showed similar bile acid patterns to B. bicornis and P. panini. The previous stereochemical assignment for (24R,25S)-VA isolated from the bile of varanid lizards and the Gila monster should now be revised to the (24S,25S)-configuration.

Harnessing the uncertainty monster: Putting quantitative constraints on the intergenerational social discount rate

NASA Astrophysics Data System (ADS)

Lewandowsky, Stephan; Freeman, Mark C.; Mann, Michael E.

2017-09-01

There is broad consensus among economists that unmitigated climate change will ultimately have adverse global economic consequences, that the costs of inaction will likely outweigh the cost of taking action, and that social planners should therefore put a price on carbon. However, there is considerable debate and uncertainty about the appropriate value of the social discount rate, that is the extent to which future damages should be discounted relative to mitigation costs incurred now. We briefly review the ethical issues surrounding the social discount rate and then report a simulation experiment that constrains the value of the discount rate by considering 4 sources of uncertainty and ambiguity: Scientific uncertainty about the extent of future warming, social uncertainty about future population and future economic development, political uncertainty about future mitigation trajectories, and ethical ambiguity about how much the welfare of future generations should be valued today. We compute a certainty-equivalent declining discount rate that accommodates all those sources of uncertainty and ambiguity. The forward (instantaneous) discount rate converges to a value near 0% by century's end and the spot (horizon) discount rate drops below 2% by 2100 and drops below previous estimates by 2070.

Coronary artery disease: new insights into the pathophysiology, prevalence, and early detection of a monster menace.

PubMed

Slater, James; Rill, Velisar

2004-04-01

Coronary artery disease (CAD) is the leading cause of morbidity and mortality in the United States and other industrialized countries. In the undeveloped world a similar epidemic is brewing. A new pathophysiologic paradigm has emerged, which assigns the mediators of inflammation a much larger role in the disease process. This paradigm has helped explain the unpredictable nature of many adverse consequences of CAD. The long latent phase of the disease, and often sudden initial presentation, make efforts at early detection extremely important. Considerable work has been devoted to identify, as well as influence, predisposing risk factors for developing arteriosclerosis. Novel markers of inflammation, like C-reactive protein, have been identified and compared to traditional risk factors. In addition, new imaging modalities introduce the possibility of screening for subclinical disease. Electron beam and multidetector computed tomography (CT) scanners, as well as other techniques, are emerging as powerful tools to detect early disease presence and allow intervention to take place before major clinical events occur. Advances in our understanding of the pathophysiology of CAD, and our ability to image the stages of silent disease will go hand in hand to revolutionize our approach to prevention and treatment of this deadly malady.

Coronary artery disease: new insights into the pathophysiology, prevalence and early detection of a monster menace.

PubMed

Slater, James; Rill, Velisar

2003-04-01

Coronary artery disease (CAD) is the leading cause of morbidity and mortality in the United States and industrialized countries. In the undeveloped world a similar epidemic is brewing. A new pathophysiologic paradigm has emerged, which assigns the mediators of inflammation a much larger role in the disease process. This paradigm has helped explain the unpredictable nature of many adverse consequences of CAD. The long latent phase of the disease and often sudden initial presentation make efforts at early detection extremely important. Considerable work has been devoted to identify as well as influence predisposing risk factors for developing arteriosclerosis. Novel markers of inflammation, like C-reactive protein, have been identified and compared to traditional risk factors. In addition, new imaging modalities introduce the possibility of screening for sub-clinical disease. Electron-beam and spiral CT scanners, as well as other techniques, are emerging as powerful tools to detect early disease presence and allow intervention to take place before major clinical events occur. Advances in our understanding of the pathophysiology and our ability to image the stages of silent disease will go hand in hand to revolutionize our approach to prevention and treatment of this deadly disease.

Monsters in the dark and other scary things: preschoolers' self-reports.

PubMed

Loxton, Helene

2009-06-01

This study attempted to obtain normative data regarding the content and frequency of expressed fears of a culturally diverse group of 152 South African preschool children (aged 5-7 years). The study employed four measuring instruments: a biographical questionnaire, the Goodenough-Harris Drawing Test, and individual drawings of feared objects by participants in conjunction with semi-structured interviews. The data analysis included descriptive statistics based on the themes that emerged from the children's drawings and interviews. Fear of animals was the most commonly expressed fear. Other high-frequency fear categories that emerged were fear of the dark, night and bad dreams; fantasy people; real people; and physical harm. For the group as a whole, the results largely support the existing body of literature. Participants expressed between one and nine fears (f = 429; mean = 2.8). This study contributed to a better understanding of both an under-researched psychological phenomenon, fear, and of an under-researched target group of young children. This knowledge is important in order for significant others, such as parents and caregivers, to understand and effectively mediate potentially stressful experiences of young children in their respective capacities.

eXtragalactic astronomy: the X-games of adaptive optics

NASA Astrophysics Data System (ADS)

Lai, Olivier

2000-07-01

Observing active nuclei, Ultra-Luminous Infrared Galaxies, starburst and merging galaxies, is both a challenge and a requirement for adaptive optics. It is a requirement, because models needed to explain the high infrared flux and the physics of these monsters need constraints that come, in part, from the fine details gleaned on high angular resolution images, and it is a challenge because, being distant, these objects are usually faint in apparent visual magnitude, meaning that the wavefront sensors have to operate in a photon starved regime. Many observations have been controversial in the past, and it is always difficult to tell an artifact such as astigmatism from an inner bar. The importance of observing the point spread function is therefore even more crucial than on bright objects, as PSF reconstruction methods 'a la Veran' break down when the photon noise dominates the statistics of the wave front, or when locking the loop on extended objects. Yet, while some cases have been controversial, some very clear and profound results have been obtained in the extragalactic domain, such as the detection of host galaxy to quasars and star formation studies. It turns out that the fundamental prerequisite to such success stories is a stable, well understood and well calibrated PSF.

Thalidomide and the Titanic: reconstructing the technology tragedies of the twentieth century.

PubMed Central

Annas, G J; Elias, S

1999-01-01

The Titanic has become a metaphor for the disastrous consequences of an unqualified belief in the safety and invincibility of new technology. Similarly, the thalidomide tragedy stands for all of the "monsters" that can be inadvertently or negligently created by modern medicine. Thalidomide, once banned, has returned to the center of controversy with the Food and Drug Administration's (FDA's) announcement that thalidomide will be placed on the market for the treatment of erythema nodosum leprosum, a severe dermatological complication of Hansen's disease. Although this indication is very restricted, thalidomide will be available for off-label uses once it is on the market. New laws regarding abortion and a new technology, ultrasound, make reasonable the approval of thalidomide for patients who suffer from serious conditions it can alleviate. In addition, the FDA and the manufacturer have proposed the most stringent postmarketing monitoring ever used for a prescription drug, including counseling, contraception, and ultrasonography in the event of pregnancy. The Titanic/thalidomide lesson for the FDA and public health is that rules and guidelines alone are not sufficient to guarantee safety. Continuous vigilance will be required to ensure that all reasonable postmarketing monitoring steps are actually taken to avoid predictable and preventable teratogenic disasters. PMID:9987477

A "WISE BOSS": Finding The Cosmic Monsters in the Mid-Infrared Lochs

NASA Astrophysics Data System (ADS)

Ross, Nicholas; Hamann, F. W.; Alexandroff, R.; Brandt, W. N.; Strauss, M. A.; Dey, A.; Richards, G. T.; Worseck, G.; Zakamska, N. L.; Eisenstein, D.; Ge, J.; Glikman, E.; Greene, J. E.; Haggard, D.; Krolik, J. H.; Myers, A. D.; Petitjean, P.; Streblyanska, A.; Schawinski, K.; Shen, Y.; Villforth, C.; McMahon, R.

2013-01-01

Mid-infrared photometry of QSOs provide an important constraint on the presence of hot dust in the vicinity of the active nucleus. However, assembling large statistical MIR samples of quasars at the height of the ``quasar epoch'' ( 2.5) has, up until now, been challenging due to either wide but relatively shallow optical quasar surveys, or deep but narrow mid-IR data. The SDSS-III Baryon Oscillation Spectroscopic Survey (BOSS) is the state-of-the-art in optical wide-field spectroscopy, and has over 150,000 quasars confirmed, with the majority of the quasar data at z=2.2-3.5. We combine these data with the all-sky mid-infrared coverage from the Wide-Field Infrared Survey Explorer (WISE), and initially concentrate on BOSS quasars with ``extreme'' colors, e.g. r-[22]>14, and those detected only in the redder WISE bands, a.k.a. "the W1W2drops". We find that these selections identify a heterogeneous sample within the BOSS quasar data, but also provide a key tool for finding interesting populations including the 2.5 Type II QSO population. We relate these very red BOSS quasars to the recent discoveries of the ``hyper-LIRG" and ``Hot Dust Obscured Galaxy'' (or Hot DOG) population.

Phylogenetics links monster larva to deep-sea shrimp.

PubMed

Bracken-Grissom, Heather D; Felder, Darryl L; Vollmer, Nicole L; Martin, Joel W; Crandall, Keith A

2012-10-01

Mid-water plankton collections commonly include bizarre and mysterious developmental stages that differ conspicuously from their adult counterparts in morphology and habitat. Unaware of the existence of planktonic larval stages, early zoologists often misidentified these unique morphologies as independent adult lineages. Many such mistakes have since been corrected by collecting larvae, raising them in the lab, and identifying the adult forms. However, challenges arise when the larva is remarkably rare in nature and relatively inaccessible due to its changing habitats over the course of ontogeny. The mid-water marine species Cerataspis monstrosa (Gray 1828) is an armored crustacean larva whose adult identity has remained a mystery for over 180 years. Our phylogenetic analyses, based in part on recent collections from the Gulf of Mexico, provide definitive evidence that the rare, yet broadly distributed larva, C. monstrosa, is an early developmental stage of the globally distributed deepwater aristeid shrimp, Plesiopenaeus armatus. Divergence estimates and phylogenetic relationships across five genes confirm the larva and adult are the same species. Our work demonstrates the diagnostic power of molecular systematics in instances where larval rearing seldom succeeds and morphology and habitat are not indicative of identity. Larval-adult linkages not only aid in our understanding of biodiversity, they provide insights into the life history, distribution, and ecology of an organism.

Phylogenetics links monster larva to deep-sea shrimp

PubMed Central

Bracken-Grissom, Heather D; Felder, Darryl L; Vollmer, Nicole L; Martin, Joel W; Crandall, Keith A

2012-01-01

Mid-water plankton collections commonly include bizarre and mysterious developmental stages that differ conspicuously from their adult counterparts in morphology and habitat. Unaware of the existence of planktonic larval stages, early zoologists often misidentified these unique morphologies as independent adult lineages. Many such mistakes have since been corrected by collecting larvae, raising them in the lab, and identifying the adult forms. However, challenges arise when the larva is remarkably rare in nature and relatively inaccessible due to its changing habitats over the course of ontogeny. The mid-water marine species Cerataspis monstrosa (Gray 1828) is an armored crustacean larva whose adult identity has remained a mystery for over 180 years. Our phylogenetic analyses, based in part on recent collections from the Gulf of Mexico, provide definitive evidence that the rare, yet broadly distributed larva, C. monstrosa, is an early developmental stage of the globally distributed deepwater aristeid shrimp, Plesiopenaeus armatus. Divergence estimates and phylogenetic relationships across five genes confirm the larva and adult are the same species. Our work demonstrates the diagnostic power of molecular systematics in instances where larval rearing seldom succeeds and morphology and habitat are not indicative of identity. Larval–adult linkages not only aid in our understanding of biodiversity, they provide insights into the life history, distribution, and ecology of an organism. PMID:23145324

Propagation optical quarks after an uniaxial crystal: the experiment

NASA Astrophysics Data System (ADS)

Egorov, Yu. A.; Konovalenko, V. L.; Zinovev, A. O.; Anischenko, P. M.; Glumova, M. V.

2013-12-01

There is a lots of different papers reporting about the propagation of the different types of an optical beams in a uniaxial crystals are known by that time. This beams are: Lager-Gaussian and Bessel- Gaussian beams. It is common for all this types of beams, that if propagation axis and crystal axis coincides, and accident beam had a circular polarization, are can get type spiral type degenerated umbilici, which corresponds to the charge 2 optical vortex in the orthogonal polarized beam component, generated by crystal [1] (Fig 1). This generation accurse due to total angular momentum conservation law symmetry axis of the crystal. One to the changing of the spin momentum which is associated with the beam polarization, this leads to the orbital momentum changes that associated with topological charge of formed orthogonal circular component. Double charged optical vortex could be easily perturbed by tilting beam axis with respect to the crystal axis. If the tilt angles are small (<0.1°) central umbilici splits on two lemons and the surrounding ring umbilici splits on two pairs of monster-star. The further increasing of the tilt angle leads to the topological charge of circular components becomes, equal, and additional orbital moment correspond to the beam mass center displacement.

ET versus Alien : Popular Attitudes to bringing back Biological Material from Space

NASA Astrophysics Data System (ADS)

Evans, D.

The general public tend to react to radical scientific innovation in extreme ways, seeing them alternatively as a passport to utopia or a ticket to hell. The possible discovery of alien life forms has generated both types of reaction, as a brief survey of Hollywood movies shows. In this fanciful world, alens are either the friendly beings of ET and Close Encounters, who show us a way to improve ourselves, or the frightening monsters of Alien and Independence Day, who are bent on our destruction. Yet most astrobiologists would agree that both types of scenario are extremely unlikely. If we do encounter other life forms, the scientific consensus is that such life is vastly more likely to be microbial than to be an advanced, intelligent multicellular species. The public focus on the improbable stories of Hollywood means that they are little prepared to engage in sensible dialogue about plans for sample return missions from Mars and other planets. Unless scientific organisations take steps to encourage a more realistic understanding of the kinds of life we are most likely to encounter in space, we risk seeing public debate on these matters degenerate into the same hysteria and idiocy as that which has surrounded the use of GM foods and stem cell research.

Dreams as a source of supernatural agent concepts.

PubMed

McNamara, Patrick; Bulkeley, Kelly

2015-01-01

We present a theory of the creativity of dreams as well as psychopathology of religious delusions with respect to production of fundamental forms of religious cognition-specifically supernatural agent (SA) cognitions. We suggest that dream cognitions are particularly efficient at producing highly memorable and impactful experiences with SAs because dreams involve three processes that are prerequisites for the generation of god concepts: (1) mental simulations of alternative realities, (2) theory of mind attributions to the extra-natural dream characters and divine beings, and (3) attribution of ultimate value (exemplified by 'good spirit beings'), and dis-value (exemplified by demonic monsters) to the supernatural dream characters. Because prefrontal cortex is deactivated during rapid eye movements (REM) sleep agentic impulses and internally generated ideas are not reliably attributed to Self or dreamer. Instead an exaggerated degree of agency is attributed to these supernatural dream characters who are then embedded in stories in dreams and in myths of waking life which explain their supernatural abilities. These dream-based SAs are salient characters that are processed in sleep-related memory systems according to rules of Lleweelyn's ancient art of memory model and therefore more easily remembered and reflected upon during waking life. When REM sleep intrudes into waking consciousness, as is the case with some forms of schizophrenia, religious delusions are more likely to emerge.

Crew Earth Observations (CEO) taken during Expedition Six

NASA Image and Video Library

2003-04-04

ISS006-E-43366 (4 April 2003) --- This view featuring Baitoushan Volcano, China and North Korea, was photographed by an Expedition 6 crewmember on the International Space Station (ISS). One of the largest known Holocene eruptions occurred at Baitoushan Volcano (also known as Changbaishan in China and P’aektu-san in Korea) about 1000 A.D., with erupted material deposited as far away as northern Japan – a distance of approximately 1200 kilometers. The eruption also created the 4.5 kilometer diameter, 850 meters deep summit caldera of the volcano that is now filled with the waters of Lake Tianchi (or Sky Lake). This oblique photograph was taken during the winter season, and snow highlights frozen Lake Tianchi along with lava flow lobes along the southern face of the volcano. Baitoushan last erupted in 1702 and is considered a dormant volcano. Gas emissions were reported from the summit and nearby hot springs in 1994, but no evidence of renewed activity of the volcano was observed. The Chinese-Korean border runs directly through the center of the summit caldera, and the mountain is considered sacred by the dominantly Korean population living near the volcano. Lake Tianchi is a popular resort destination, both for its natural beauty and alleged sightings of unidentified creatures living in its depths (similar to legendary Loch Ness Monster in Scotland).

Call it a monster for lack of anything else: narrative insight in psychosis.

PubMed

Roe, David; Hasson-Ohayon, Ilanit; Kravetz, Shlomo; Yanos, Phil T; Lysaker, Paul H

2008-12-01

Individuals diagnosed with schizophrenia often appear to be unaware of having an illness or actively reject their diagnostic label. It is unclear, however, how this lack of awareness relates to important outcomes. Broadening the definition of awareness to include "narrative insight" may clarify this issue. The objective of this study was to identify profiles of narrative insight and test how these relate to standardized measure of insight. Sixty-five individuals with schizophrenia spectrum disorders participated in an assessment that included the Scale of Unawareness of Mental Disorder (SUMD) and an in-depth semi-structured interview. Qualitative analysis revealed 5 central themes related to insight on the basis of which each interview was then rated. Cluster analysis of these ratings resulted in 4 profiles of narrative insight: (1) accepts illness/rejects label, (2) rejects illness/searches for a name (3) passive insight of illness and label, and (4) integrative insight. The SUMD differentiated between individuals assigned to profile 2 who showed low insight to their illness and those assigned to the other profiles of narrative insight, but could not differentiate between them. Results support the claim that illness narratives are multifaceted and that traditional measures of insight may not be sensitive to different ways in which people understand their illness.

Behemoth Black Hole Found in an Unlikely Place

NASA Image and Video Library

2016-04-06

This computer-simulated image shows a supermassive black hole at the core of a galaxy. The black region in the center represents the black hole’s event horizon, where no light can escape the massive object’s gravitational grip. The black hole’s powerful gravity distorts space around it like a funhouse mirror. Light from background stars is stretched and smeared as the stars skim by the black hole. Credits: NASA, ESA, and D. Coe, J. Anderson, and R. van der Marel (STScI) More info: Astronomers have uncovered a near-record breaking supermassive black hole, weighing 17 billion suns, in an unlikely place: in the center of a galaxy in a sparsely populated area of the universe. The observations, made by NASA’s Hubble Space Telescope and the Gemini Telescope in Hawaii, may indicate that these monster objects may be more common than once thought. Until now, the biggest supermassive black holes – those roughly 10 billion times the mass of our sun – have been found at the cores of very large galaxies in regions of the universe packed with other large galaxies. In fact, the current record holder tips the scale at 21 billion suns and resides in the crowded Coma galaxy cluster that consists of over 1,000 galaxies.

Call It a Monster for Lack of Anything Else

PubMed Central

Roe, David; Hasson-Ohayon, Ilanit; Kravetz, Shlomo; Yanos, Phil T.; Lysaker, Paul H.

2011-01-01

Individuals diagnosed with schizophrenia often appear to be unaware of having an illness or actively reject their diagnostic label. It is unclear, however, how this lack of awareness relates to important outcomes. Broadening the definition of awareness to include “narrative insight” may clarify this issue. The objective of this study was to identify profiles of narrative insight and test how these relate to standardized measure of insight. Sixty-five individuals with schizophrenia spectrum disorders participated in an assessment that included the Scale of Unawareness of Mental Disorder (SUMD) and an in-depth semi-structured interview. Qualitative analysis revealed 5 central themes related to insight on the basis of which each interview was then rated. Cluster analysis of these ratings resulted in 4 profiles of narrative insight: (1) accepts illness/rejects label, (2) rejects illness/searches for a name (3) passive insight of illness and label, and (4) integrative insight. The SUMD differentiated between individuals assigned to profile 2 who showed low insight to their illness and those assigned to the other profiles of narrative insight, but could not differentiae between them. Results support the claim that illness narratives are multifaceted and that traditional measures of insight may not be sensitive to different ways in which people understand their illness. PMID:19077852

From cutting nature and its joints to measuring it: new kinds and new kinds of people in biology.

PubMed

McOuat, G

2001-12-01

In the received version of the development of science, natural kinds are established in the preliminary stages (natural history) and made more precise by measurement (exact science). By examining the move from nineteenth- to twentieth-century biology, this paper unpacks the notion of species as 'natural kinds' and grounds for discourse, questioning received notions about both kinds and species. Life sciences in the nineteenth century established several 'monster-barring' techniques to block disputes about the precise definition of species. Counterintuitively, precision and definition brought dispute and disrupted exchange. Thus, any attempt to add precision was doomed to failure. By intervening and measuring, the new experimental biology dislocated the established links between natural kinds and kinds of people and institutions. New kinds were built in new places. They were made to measure from the very start. This paper ends by claiming that there was no long-standing 'species problem' in the history of biology. That problem is a later construction of the 'modern synthesis', well after the disruption of 'kinds' and kinds of people. Only then would definitions and precision matter. A new, non-linguistic, take on the incommensurability thesis is hinted at. Copyright 2001 Elsevier Science Ltd. All rights reserved.

[Theriac: medicine and antidote].

PubMed

Parojcic, Dusanka; Stupar, Dragan; Mirica, Milica

2003-06-01

Theriac was an ancient multi-ingredient preparation; originating as a cure for the bites of serpents, mad dogs and wild beasts, it later became an antidote to all known poisons. The name theriac (treacle), (Greek theriake, Latin theriaca, French thériaque) was derived from the Greek for wild beast - theriakos. The first formula was created by Mithridates Vl, King of Pontus, a skillful ruler but a monster of cruelty, who, living in such a fear of being poisoned, took a great interest in toxicology. In the 1st century AD, Nero's personal physician Andromachus improved the formula of Antidotum Mithridatium by adding flesh of vipers, which was commonly believed to be the best antidote against snakebite, and by increasing the proportion of opium. It became known as Theriac of Andromachus, and contained 64 ingredients including various minerals, herbals, poisons and animal flesh and blood, all combined with honey in the form of electuarium. Later it became the cure-all medicine which, accumulating all the simples into one form, was supposed to be a universal panacea against all diseases. In the Middle Ages this famous electuarium become a patent medicine and entered official dispensaries and pharmacopoeias. The most famous and expensive Theriac in Europe was that of Venice. It was not until the l8th century that it was excluded from medical use.

Jewish views on abortion.

PubMed

Jakobovits, I

1968-01-01

In Jewish law right and wrong, good and evil, are absolute values which transcend time, place, and environment. They defy definition by human intuition or expediency. Jewish law derives from the Divine revelation at Mount Sinai as expounded by sages faithful to, and authorized by, its writ. The Talmud rules that if a woman is in hard travail, and her life must be saved, the child must be aborted and extracted. The mother's life comes first. The fetus is not a human life until it is born. But 19th century Rabbinical works state that it is immoral to destroy a monster child. Modern rabbis are unanimous in condemning abortion, feticide, or infanticide as an unconscionable attack on human life. However, Jewish law allows abortion if the pregnancy will cause severe psychological damage to the mother. No civilized society could survive without laws which occasionally cause some suffering or personal anguish. One human life is worth a million lives, because each life is infinite in value. In cases of rape or incest Jewish law still does not sanction abortion. Man's procreative responsibilities are serious and carry rights and obligations which would be upset by liberalized abortion laws. If a person kills a person who is mortally wounded, the killer is guilty of a moral offense.

Evolutionary developmental pathology and anthropology: A new field linking development, comparative anatomy, human evolution, morphological variations and defects, and medicine.

PubMed

Diogo, Rui; Smith, Christopher M; Ziermann, Janine M

2015-11-01

We introduce a new subfield of the recently created field of Evolutionary-Developmental-Anthropology (Evo-Devo-Anth): Evolutionary-Developmental-Pathology-and-Anthropology (Evo-Devo-P'Anth). This subfield combines experimental and developmental studies of nonhuman model organisms, biological anthropology, chordate comparative anatomy and evolution, and the study of normal and pathological human development. Instead of focusing on other organisms to try to better understand human development, evolution, anatomy, and pathology, it places humans as the central case study, i.e., as truly model organism themselves. We summarize the results of our recent Evo-Devo-P'Anth studies and discuss long-standing questions in each of the broader biological fields combined in this subfield, paying special attention to the links between: (1) Human anomalies and variations, nonpentadactyly, homeotic transformations, and "nearest neighbor" vs. "find and seek" muscle-skeleton associations in limb+facial muscles vs. other head muscles; (2) Developmental constraints, the notion of "phylotypic stage," internalism vs. externalism, and the "logic of monsters" vs. "lack of homeostasis" views about human birth defects; (3) Human evolution, reversions, atavisms, paedomorphosis, and peromorphosis; (4) Scala naturae, Haeckelian recapitulation, von Baer's laws, and parallelism between phylogeny and development, here formally defined as "Phylo-Devo parallelism"; and (5) Patau, Edwards, and Down syndrome (trisomies 13, 18, 21), atavisms, apoptosis, heart malformations, and medical implications. © 2015 Wiley Periodicals, Inc.

Death by information overload.

PubMed

Hemp, Paul

2009-09-01

The value of information in the knowledge economy is indisputable, but so is its capacity to overwhelm consumers of it. HBR contributing editor Hemp reports on practical ways for individuals and organizations to avoid getting too much of a good thing. Ready access to useful information comes at a cost: As the volume increases, the line between the worthwhile and the distracting starts to blur. And ready access to you--via e-mail, social networking, and so on--exacerbates the situation: On average, Intel executives get 300 e-mails a day, and Microsoft workers need 24 minutes to return to work after each e-mail interruption. Clearly, productivity is taking a hit. Technological aids can help, such as e-mail management software for you, a message-volume regulation system for your organization, or even more-sophisticated solutions being developed by Microsoft, IBM, and others. Yet, battling technological interruptions on their own turf only goes so far. You also need to change your mind-set, perhaps by seeking help from personal-productivity experts or by simply accepting that you can't respond to every distraction that flits across your screen. Similarly, organizations must change their cultures, for instance by establishing clear e-communication protocols. In the end, only a multipronged approach will help you and your organization subdue the multiheaded monster of information overload. The secret is to manage the beast while still respecting it for the beautiful creature it is.

Dreams as a source of supernatural agent concepts

PubMed Central

McNamara, Patrick; Bulkeley, Kelly

2015-01-01

We present a theory of the creativity of dreams as well as psychopathology of religious delusions with respect to production of fundamental forms of religious cognition—specifically supernatural agent (SA) cognitions. We suggest that dream cognitions are particularly efficient at producing highly memorable and impactful experiences with SAs because dreams involve three processes that are prerequisites for the generation of god concepts: (1) mental simulations of alternative realities, (2) theory of mind attributions to the extra-natural dream characters and divine beings, and (3) attribution of ultimate value (exemplified by ‘good spirit beings’), and dis-value (exemplified by demonic monsters) to the supernatural dream characters. Because prefrontal cortex is deactivated during rapid eye movements (REM) sleep agentic impulses and internally generated ideas are not reliably attributed to Self or dreamer. Instead an exaggerated degree of agency is attributed to these supernatural dream characters who are then embedded in stories in dreams and in myths of waking life which explain their supernatural abilities. These dream-based SAs are salient characters that are processed in sleep-related memory systems according to rules of Lleweelyn’s ancient art of memory model and therefore more easily remembered and reflected upon during waking life. When REM sleep intrudes into waking consciousness, as is the case with some forms of schizophrenia, religious delusions are more likely to emerge. PMID:25852602

The Monster at the Heart of our Galaxy

NASA Astrophysics Data System (ADS)

Ghez, Andrea

2015-08-01

Learn about new developments in the study of black holes. Through the capture and analysis of twenty years of high-resolution imaging, Dr. Ghez and her team have moved the case for a supermassive black hole at the center of our galaxy from a possibility to a certainty. This was made possible with the first measurements of stars’ orbiting at high speeds around a galactic nucleus. Further advances in state-of-the-art of high-resolution imaging technology on the world’s largest telescopes have greatly expanded the power of using stellar orbits to characterize black holes. Recent observations have revealed an environment around the black hole that is quite unexpected (young stars where there should be none; a lack of old stars where there should be many; and a puzzling new class of objects). Continued measurements of the motions of stars have solved many of the puzzles posed by these perplexing populations of stars. This work on the orbits of stars, along with observations of the dining habits of the black hole, is providing insight into how black holes grow and the role that they play in regulating the growth of their host galaxies. Future measurements of stellar orbits at the Galactic Center hold the promise of improving our understanding of gravity through tests of Einstein’s General Theory of Relativity in an unexplored regime.

Acute effects of a glucose energy drink on behavioral control.

PubMed

Howard, Meagan A; Marczinski, Cecile A

2010-12-01

There has been a dramatic rise in the consumption of glucose energy drinks (e.g., Amp, Monster, and Red Bull) in the past decade, particularly among high school and college students. However, little laboratory research has examined the acute objective and subjective effects of energy drinks. The purpose of this study was to investigate the acute effects of a glucose energy drink (Red Bull) on cognitive functioning. Participants (N = 80) were randomly assigned to one of five conditions: 1.8 ml/kg energy drink, 3.6 ml/kg energy drink, 5.4 ml/kg energy drink, placebo beverage, or no drink. Participants completed a well-validated behavioral control task (the cued go/no-go task) and subjective measures of stimulation, sedation, and mental fatigue both before and 30 minutes following beverage administration. The results indicated that compared with the placebo and no drink conditions, the energy drink doses decreased reaction times on the behavioral control task, increased subjective ratings of stimulation and decreased ratings of mental fatigue. Greatest improvements in reaction times and subjective measures were observed with the lowest dose and improvements diminished as the dose increased. The findings suggest that energy drink consumption can improve cognitive performance on a behavioral control task, potentially explaining the dramatic rise in popularity of these controversial new beverages. PsycINFO Database Record (c) 2010 APA, all rights reserved.

Mass media, 'monsters' and mental health clients: the need for increased lobbying.

PubMed

Cutcliffe, J R; Hannigan, B

2001-08-01

A review of the limited empirical and theoretical literature indicates that current mass media representations of mental health service users appear to emphasize violence, dangerousness and criminality. This is despite the empirical evidence that indicates a decline over the last 40 years in the number of homicides carried out by people identified as suffering from mental health problems. Such inappropriate representations do much to increase stigma, ostracism, harassment and victimization of these individuals by the public. Furthermore, it can be argued that there is another repercussion of these representations and that is the subsequent government position/policy and the resulting legislation concerning care of people with mental health problems. Consequently, this paper argues that there is a clear need for psychiatric/mental health (P/MH) nurses to become more mindful of the wider, socio-political environment in which their practice occurs, particularly if psycho-social approaches to practice are adopted in their fullest sense, and as a result increase their political lobby. Such increased lobbying should occur on behalf of, and in collaboration with, service users, and accordingly the authors describe a range of activities under the broad headings of pro-active and reactive lobbying. Furthermore, it is incumbent upon P/MH nurse educationalists to prepare aspirant P/MH nurses for this lobbying role and equip them with the skills necessary to do so.

Future Extragalactic Surveys

NASA Astrophysics Data System (ADS)

Blain, Andrew

2007-12-01

The technology for mega-pixel mm/submm-wave cameras is being developed, and 10,000-pixel cameras are close to being deployed. These parameters correspond to degree-sized fields, and challenge the optical performance of current telescopes. Next-generation cameras will enable a survey of a large fraction of the sky, to detect active and star-forming dust-enshrouded galaxies. However, to avoid being limited by confusion, and finding only `monsters' it is necessary to push to large telescopes and short wavelengths. The CCAT project will enable the necessary performance to survey the sky to detect ultraluminous galaxies at z>2, each of which can then be imaged in detail with ALMA. The combination of image quality, collecting area and field-of-view will also enable CCAT to probe much deeper, to detect all the sources in legacy fields from the Spitzer and Herschel Space Telescopes. Unlike ALMA, CCAT will still be limited to detecting `normal' galaxies at z 3-5; however, by generating huge catalogs, CCAT will enable a dramatic increase in ALMA's efficiency, and almost completely remove the need for ALMA to conduct its own imaging survey. I will discuss the nature of galaxy surveys that will be enabled by CCAT, the issues of prioritizing and executing follow-up imaging spectroscopy with ALMA, and the links with the forthcoming NASA WISE mission, and future space-based far-infrared missions.

Problems with mitigation translocation of herpetofauna.

PubMed

Sullivan, Brian K; Nowak, Erika M; Kwiatkowski, Matthew A

2015-02-01

Mitigation translocation of nuisance animals is a commonly used management practice aimed at resolution of human-animal conflict by removal and release of an individual animal. Long considered a reasonable undertaking, especially by the general public, it is now known that translocated subjects are negatively affected by the practice. Mitigation translocation is typically undertaken with individual adult organisms and has a much lower success rate than the more widely practiced conservation translocation of threatened and endangered species. Nonetheless, the public and many conservation practitioners believe that because population-level conservation translocations have been successful that mitigation translocation can be satisfactorily applied to a wide variety of human-wildlife conflict situations. We reviewed mitigation translocations of reptiles, including our own work with 3 long-lived species (Gila monsters [Heloderma suspectum], Sonoran desert tortoises [Gopherus morafkai], and western diamond-backed rattlesnakes [Crotalus atrox]). Overall, mitigation translocation had a low success rate when judged either by effects on individuals (in all studies reviewed they exhibited increased movement or increased mortality) or by the success of the resolution of the human-animal conflict (translocated individuals often returned to the capture site). Careful planning and identification of knowledge gaps are critical to increasing success rates in mitigation translocations in the face of increasing pressure to find solutions for species threatened by diverse anthropogenic factors, including climate change and exurban and energy development. © 2014 Society for Conservation Biology.

Revisiting the monster: the mass profile of the galaxy cluster Abell 3827 using dynamical and strong lensing constrains

NASA Astrophysics Data System (ADS)

Rodrigo Carrasco Damele, Eleazar; Verdugo, Tomas

2018-01-01

The galaxy cluster Abell 3827 is one of the most massive clusters know at z ≦ 0.1 (Richness class 2, BM typeI, X-ray LX = 2.4 x 1044 erg s-1). The Brightest Cluster Galaxy (BCG) in Abell 3827 is perhaps the most extreme example of ongoing galaxy cannibalism. The multi-component BCG hosts the stellar remnants nuclei of at least four bright elliptical galaxies embedded in a common assymetric halo extended up to 15 kpc. The most notorious characteristic of the BCG is the existence of a unique strong gravitational lens system located within the inner 15 kpc region. A mass estimation of the galaxy based on strong lensing model was presented in Carrasco et al (2010, ApJL, 715, 160). Moreover, the exceptional strong lensing lens system in Abell 3827 and the location of the four bright galaxies has been used to measure for the first time small physical separations between dark and ordinary matter (Williams et al. 2011, MNRAS, 415, 448, Massey et al. 2015, MNRAS, 449, 3393). In this contribution, we present a detailed strong lensing and dynamical analysis of the cluster Abell 3827 based on spectroscopic redshift of the lensed features and from ~70 spectroscopically confirmed member galaxies inside 0.5 x 0.5 Mpc from the cluster center.

Taming the green-eyed monster: temporal responsivity to cognitive behavioural and cognitive analytic therapy for morbid jealousy.

PubMed

Kellett, Stephen; Totterdell, Peter

2013-03-01

Credible evaluations of the psychological treatment of morbid jealousy are rare. The aim of this study was to evaluate temporal responsivity to cognitive behavioural therapy (CBT) and cognitive analytic therapy (CAT) for morbid jealousy. The methodology involved matched A/B single-case experimental designs (SCED) with extended follow-up, in which two patients and their partners completed daily jealousy target symptom items across the phases of the study. Patients also completed traditional psychometric outcome measures at assessment, post-therapy, and at final follow-up. Both patients received the same number of assessment (n = 3), treatment (n = 13), and follow-up (n = 1) sessions.  Autoregressive Integrated Moving Average (ARIMA) models of the patients' daily target symptom jealousy SCED data indicate the effectiveness of the CAT intervention and the ineffectiveness of the CBT intervention, but both therapies produced large effect sizes. The partner of the CBT patient felt less controlled following therapy, whilst the partner of CAT patient did not perceive any change to his partner. The discussion calls for a stronger evidence base for the psychological treatment of morbid jealousy to be constructed and debates the routine measurement of outcomes for partners of morbidly jealous patients. Measuring outcomes for partners of jealous patients is indicated.   CAT shows promise as an intervention for morbid jealousy. The evidence base for the treatment of morbid jealousy requires further development. © 2011 The British Psychological Society.

Constructing identities in the media: newspaper coverage analysis of a major UK Clostridium difficile outbreak.

PubMed

Burnett, Emma; Johnston, Bridget; Corlett, Joanne; Kearney, Nora

2014-07-01

To examine how a major Clostridium difficile outbreak in the UK was represented in the media. Clostridium difficile is a serious health care-associated infection with significant global prevalence. As major outbreaks have continued to occur worldwide over the last few decades, it has also resulted in increasing media coverage. Newspaper journalists are, however, frequently criticized for sensationalized and inaccurate reporting and alarming the public. Despite such criticisms, nothing is known about how the media frame Clostridium difficile related coverage. Qualitative interpretive descriptive study. An interpretive analysis of newspaper articles from the national press that reported about the outbreak from the first day of coverage over 3 weeks (12 June-3 July 2008). Twenty-eight newspaper articles were included in the study from tabloids, broadsheets, a regional and a Sunday newspaper. Monster and war metaphors were frequently adopted to portray the severity of Clostridium difficile and the impact it can have on patient safety. In addition, the positioning of the affected patients, their families, healthcare professionals and the Government produced representations of victims, villains and heroes. This subsequently evoked notions of vulnerability, blame and conflict. The media are and will remain critical convectors of public information and, as such, are hugely influential in risk perceptions and responses. Rather than simply dismissing media coverage, further understanding around how such stories in specific contexts are constructed and represented is needed so that it can help inform future communication and management strategies. © 2013 John Wiley & Sons Ltd.

A mess of stars

NASA Image and Video Library

2015-08-10

Bursts of pink and red, dark lanes of mottled cosmic dust, and a bright scattering of stars — this NASA/ESA Hubble Space Telescope image shows part of a messy barred spiral galaxy known as NGC 428. It lies approximately 48 million light-years away from Earth in the constellation of Cetus (The Sea Monster). Although a spiral shape is still just about visible in this close-up shot, overall NGC 428’s spiral structure appears to be quite distorted and warped, thought to be a result of a collision between two galaxies. There also appears to be a substantial amount of star formation occurring within NGC 428 — another telltale sign of a merger. When galaxies collide their clouds of gas can merge, creating intense shocks and hot pockets of gas and often triggering new waves of star formation. NGC 428 was discovered by William Herschel in December 1786. More recently a type Ia supernova designated SN2013ct was discovered within the galaxy by Stuart Parker of the BOSS (Backyard Observatory Supernova Search) project in Australia and New Zealand, although it is unfortunately not visible in this image. This image was captured by Hubble’s Advanced Camera for Surveys (ACS) and Wide Field and Planetary Camera 2 (WFPC2). A version of this image was entered into the Hubble’s Hidden Treasures Image Processing competition by contestants Nick Rose and the Flickr user penninecloud. Links: Nick Rose’s image on Flickr Penninecloud’s image on Flickr

Rewinding Frankenstein and the body-machine: organ transplantation in the dystopian young adult fiction series Unwind.

PubMed

Wohlmann, Anita; Steinberg, Ruth

2016-12-01

While the separation of body and mind (and the entailing metaphor of the body as a machine) has been a cornerstone of Western medicine for a long time, reactions to organ transplantation among others challenge this clear-cut dichotomy. The limits of the machine-body have been negotiated in science fiction, most canonically in Mary Shelley's Frankenstein (1818). Since then, Frankenstein's monster itself has become a motif that permeates both medical and fictional discourses. Neal Shusterman's contemporary dystology for young adults, Unwind, draws on traditional concepts of the machine-body and the Frankenstein myth. This article follows one of the young protagonists in the series, who is entirely constructed from donated tissue, and analyses how Shusterman explores the complicated relationship between body and mind and between self and other as the teenager matures into an adult. It will be shown that, by framing the story of a transplanted individual along the lines of a coming-of-age narrative, Shusterman inter-relates the acceptance of a donor organ with the transitional space of adolescence and positions the quest for embodied selfhood at the centre of both developments. By highlighting the interconnections between medical discourse and a literary tradition, the potential contribution of the series to the treatment and understanding of post-transplant patients will be addressed. Published by the BMJ Publishing Group Limited. For permission to use (where not already granted under a licence) please go to http://www.bmj.com/company/products-services/rights-and-licensing/.

Kalkipyrone B, a marine cyanobacterial γ-pyrone possessing cytotoxic and anti-fungal activities

PubMed Central

Bertin, Matthew J; Demirkiran, Ozlem; Navarro, Gabriel; Moss, Nathan A; Lee, John; Goldgof, Gregory M; Vigil, Edgar; Winzeler, Elizabeth A; Valeriote, Fred A; Gerwick, William H

2015-01-01

Bioassay-guided fractionation of two marine cyanobacterial extracts using the H-460 human lung cancer cell line and the OVC-5 human ovarian cancer cell line led to the isolation of three related α-methoxy-β, β’-dimethyl-γ-pyrones each containing a modified alkyl chain, one of which was identified as the previously reported kalkipyrone and designated kalkipyrone A. The second compound was an analog designated kalkipyrone B. The third was identified as the recently reported yoshipyrone A, also isolated from a marine cyanobacterium. Kalkipyrone A and B were obtained from a field-collection of the cyanobacterium Leptolyngbya sp. from Fagasa Bay, American Samoa, while yoshipyrone A was isolated from a field-collection of cyanobacteria (cf. Schizothrix sp.) from Panama. One-dimensional and two-dimensional NMR experiments were used to determine the overall structures and relative configurations of the kalkipyrones, and the absolute configuration of kalkipyrone B was determined by 1H NMR analysis of diastereomeric Mosher’s esters. Kalkipyrone A showed good cytotoxicity to H-460 human lung cancer cells (EC50 = 0.9 µM), w M), while kalkipyrone B and yoshipyrone A were less active (EC50 = 9.0 µM and > 10 µM, respectively). Both kalkipyrone A and B showed moderate toxicity to Saccharomyces cerevisiae ABC16-Monster strain (IC50 = 14.6 and 13.4 µM, respectively), whereas yoshipyrone A was of low toxicity to this yeast strain (IC50 = 63.8 µM). PMID:26632528

Is it the Monster “Teratoma” or Simply Meningomyelocele: Our Experience of “Histological Surprise”

PubMed Central

Singh, Suyash; Sardhara, Jayesh; Sharma, Pradeep; Srivastava, Arun Kumar; Das, Kuntal Kanti; Bhaisora, Kamlesh S.; Mehrotra, Anant; Jaiswal, Awadhesh Kumar; Behari, Sanjay; Kumar, Raj

2017-01-01

Teratomas are one of the most common tumors in newborn with excellent prognosis arises from totipotent primordial germ cells harboring two or three germ cell layers. The tumor has been titled “Great masquerade.” The teratomas of sacrococcygeal region present with lower limb weakness, urinary or bowel obstruction, and swelling at lower back or intrauterine mass in ultrasound or complicated delivery. A 2-month-old male child presented with complaints of swelling over lumbosacral region with discharging punctum since birth. Sagittal T2-weighted magnetic resonance imaging (MRI) of the spine showed myelocele at L5 level forming placode with central defect at L4-S1 and low-lying tethered cord up to L4–L5. The patient was operated, and histopathology surprisingly came to be mature teratoma. We followed the patient with serum beta human chorionic gonadotropin and alpha-fetoprotein markers and MRI. Literature supports complete surgical removal, including coccyx and tumor base. Mature teratoma is considered as benign disease thus even subtotal excision is appropriate but with aggressive follow-up. The difference in recurrence following total compared to subtotal resection is considered insignificant. In this article, we have discussed the management of teratoma in detail. Teratoma with meningomyelocele is a rare entity. There is still dilemma in managing cases and prognosticating parents in such patients. The provisional diagnosis of teratoma should also be considered when child presents as midline sacrococcygeal mass. PMID:28904585

Cyclopia: from Greek antiquity to medical genetics.

PubMed

Kalantzis, George C; Tsiamis, Costas B; Poulakou-Rebelakou, Effie L

2013-01-01

Cyclops are among the best-known monsters of Greek mythology, also mentioned in art and literature. According to the most recent scientific knowledge, the malformations caused by defective development of the anterior brain and midline mesodermal structures include cyclopia (synophthalmos), ethmocephaly, cebocephaly and arrhinencephaly. These severe forebrain lesions often are accompanied by severe systemic malformations, and affected infants rarely survive. Neither true cyclopia nor synophthalmos are compatible with life because an anomalous development of the brain is involved. Thus, it is difficult to assume that ancient Greeks drew their inspiration from an adult patient suffering from cyclopia. Cyclops appear for the first time in literature in Homer's Odyssey (8th-7th century BC) and one of them, Polyphemus, is blinded by the hero of the epic poem. The description of the creature is identical with patients suffering from cyclopia; eyes are fused and above the median eye there is a proboscis, which is the result of an abnormal development of the surface ectodermal structures covering the brain. The next literature appearance of Cyclops is at the end of 7th century BC in "Theogonia", written by Hesiodus. Another interesting description is made by Euripides in his satyr play entitled 'Cyclops' (5th century BC). In conclusion, though it is not certain whether Homer's description of Cyclops was based on his personal experience or the narration of his ancestors, there is no doubt that the ophthalmological disease, cyclopia, was named after this mythical creature.

NASA Spitzer 12th Anniversary Space Calendar

NASA Image and Video Library

2015-08-20

NASA Spitzer Space Telescope celebrated its 12th anniversary with a new digital calendar showcasing some of the mission most notable discoveries and popular cosmic eye candy. The digital calendar is online at http://www.jpl.nasa.gov/images/spitzer/20150820/Spitzer12thAnniversaryCalendar.pdf The calendar follows the life of the mission, with each month highlighting top infrared images and discoveries from successive years -- everything from a dying star resembling the eye of a monster to a star-studded, swirling galaxy. The final month includes a brand new image of the glittery star-making factory known as the Monkey Head nebula. Spitzer, which launched into space on August 25, 2003, from Cape Canaveral, Florida, is still going strong. It continues to use its ultra-sensitive infrared vision to probe asteroids, comets, exoplanets (planets outside our solar system) and some of the farthest known galaxies. Recently, Spitzer helped discover the closest known rocky exoplanet to us, named HD219134b, at 21 light-years away. In fact, Spitzer's exoplanet studies continue to surprise the astronomy community. The telescope wasn't originally designed to study exoplanets, but as luck -- and some creative engineering -- would have it, Spitzer has turned out to be a critical tool in the field, probing the climates and compositions of these exotic worlds. This pioneering work began in 2005, when Spitzer became the first telescope to detect light from an exoplanet. http://photojournal.jpl.nasa.gov/catalog/PIA19872

Elegant spiral hides a hungry monster

NASA Image and Video Library

2015-10-12

NGC 4639 is a beautiful example of a type of galaxy known as a barred spiral. It lies over 70 million light-years away in the constellation of Virgo and is one of about 1500 galaxies that make up the Virgo Cluster. In this image, taken by the NASA/ESA Hubble Space Telescope, one can clearly see the bar running through the bright, round core of the galaxy. Bars are found in around two thirds of spiral galaxies, and are thought to be a natural phase in their evolution. The galaxy’s spiral arms are sprinkled with bright regions of active star formation. Each of these tiny jewels is actually several hundred light-years across and contains hundreds or thousands of newly formed stars. But NGC 4639 also conceals a dark secret in its core — a massive black hole that is consuming the surrounding gas. This is known as an active galactic nucleus (AGN), and is revealed by characteristic features in the spectrum of light from the galaxy and by X-rays produced close to the black hole as the hot gas plunges towards it. Most galaxies are thought to contain a black hole at the centre. NGC 4639 is in fact a very weak example of an AGN, demonstrating that AGNs exist over a large range of activity, from galaxies like NGC 4639 to distant quasars, where the parent galaxy is almost completely dominated by the emissions from the AGN.

The monster in the mirror: reasons for wanting to change appearance.

PubMed

Vandervoort, Julianne; Aimé, Annie; Green-Demers, Isabelle

2015-03-01

Many adults are dissatisfied with their body, regardless of their weight, and weight loss is commonly perceived as an effective solution to this dissatisfaction. The main purpose of this study was to examine the reasons for wanting to modify one's bodily appearance (shape and weight), and to compare these reasons by sex, age, and weight group. The sample consisted of 796 French-speaking Canadian adults (100 men, 696 women; M age = 27.00 years, SD = 7.88, range 18-64; M body mass index = 24.99 kg/m(2), SD = 6.37, range 12.6-66.5 kg/m(2)) who were asked online whether or not they wanted to change their appearance and if so, why. Answers were subjected to a content analysis wherein recurrent themes were grouped and labeled. Most participants (83.2%) wanted to change their appearance. Women, participants with a higher BMI, and older participants were significantly more likely to report this desire. The three most frequently evoked reasons were body dissatisfaction, well-being, and health/shape. The results suggest that body dissatisfaction constitutes the primary motive for change for both men and women of all ages, especially for those who are of healthy weight or underweight. Women and younger adults seem to be under the impression that in changing their appearance they will be more comfortable in their own skin. Men, older adults, and overweight adults, on the other hand, are more preoccupied by their health/shape and seldom relate their appearance to their psychological balance.

The ULIRG Monster Mash: The Evolution of Massive Mergers Since z~1

NASA Astrophysics Data System (ADS)

Rothberg, Barry; Fischer, Jacqueline; Pirzkal, Nor; Rodrigues, Myriam

2018-01-01

Theoretical models and observations in the local Universe indicate there is a clear progression from merger-induced star-formation (SF) to QSO activity via Ultraluminous Infrared Galaxies (ULIRGs), systems with L8-1000 µm ≥ 1012 LSun. Not all mergers are ULIRGs, but all local ULIRGs are mergers, and likely the progenitors of QSO host galaxies. At earlier epochs, this relationship is less well accepted. Here, we first present an overview of how the dynamical properties of local (z < 0.4) ULIRGs are statistically indistinguishable from Radio Loud and Radio Quiet QSOs. Then, transition to the critical redshift range 0.4 < z < 1.0, where the star-formation rates, gas fractions, and masses of galaxies are believed to be significantly higher than in the local universe. ULIRGs at these redshifts begin to dominate the SF activity and are responsible for up to 70% of the co-moving IR density. We use rest-frame UV & optical imaging and spectra to apply the same techniques used for local ULIRGs to a sample of "classically" selected (i.e via integrated 12, 25, 60 and 100μm fluxes) systems at 0.4 < z < 1.0. Although, in general, galaxies at z > 0.4 are not the same as those in the local Universe, these intermediate redshift ULIRGs are dynamically similar, but more powerful, than their local counterparts. Furthermore, they show evidence of merging, while containing a powerful AGN hosted within a massive galaxy.

THEMIS Images as Art #45

NASA Technical Reports Server (NTRS)

2005-01-01

Welcome to the second annual THEMIS ART MONTH. From Jan. 31 through March 4 we will be showcasing images for their aesthetic value, rather than their science content. Portions of these images resemble things in our everyday lives, from animals to letters of the alphabet. We hope you enjoy our fanciful look at Mars!

One wonders what sort of creature needs to be kept back by this large strand of barbed wire...or perhaps this is the scar on the top of some giant Frankenstein's monster's head?

Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.

THEMIS Images as Art #39

NASA Technical Reports Server (NTRS)

2005-01-01

Welcome to the second annual THEMIS ART MONTH. From Jan. 31 through March 4 we will be showcasing images for their aesthetic value, rather than their science content. Portions of these images resemble things in our everyday lives, from animals to letters of the alphabet. We hope you enjoy our fanciful look at Mars!

We often envision fictional Martians as bug-eyed monsters, but today we move beyond that to just plain bugs being depicted in this nighttime IR image.

Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time.

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.

Galaxies at High Redshift

NASA Astrophysics Data System (ADS)

Bauer, F. E.

2014-10-01

Recent years have seen tremendous progress in finding and charactering star-forming galaxies at high redshifts across the electromagnetic spectrum, giving us a more complete picture of how galaxies evolve, both in terms of their stellar and gas content, as well as the growth of their central supermassive black holes. A wealth of studies now demonstrate that star formation peaked at roughly half the age of the Universe and drops precariously as we look back to very early times, and that their central monsters apparently growth with them. At the highest-redshifts, we are pushing the boundaries via deep surveys at optical, X-ray, radio wavelengths, and more recently using gamma-ray bursts. I will review some of our accomplishments and failures. Telescope have enabled Lyman break galaxies to be robustly identified, but the UV luminosity function and star formation rate density of this population at z = 6 - 8 seems to be much lower than at z = 2 - 4. High escape fractions and a large contribution from faint galaxies below our current detection limits would be required for star-forming galaxies to reionize the Universe. We have also found that these galaxies have blue rest-frame UV colours, which might indicate lower dust extinction at z > 5. There has been some spectroscopic confirmation of these Lyman break galaxies through Lyman-α emission, but the fraction of galaxies where we see this line drops at z > 7, perhaps due to the onset of the Gunn-Peterson effect (where the IGM is opaque to Lyman-α).

The eyes of Tullimonstrum reveal a vertebrate affinity.

PubMed

Clements, Thomas; Dolocan, Andrei; Martin, Peter; Purnell, Mark A; Vinther, Jakob; Gabbott, Sarah E

2016-04-28

Tullimonstrum gregarium is an iconic soft-bodied fossil from the Carboniferous Mazon Creek Lagerstätte (Illinois, USA). Despite a large number of specimens and distinct anatomy, various analyses over the past five decades have failed to determine the phylogenetic affinities of the 'Tully monster', and although it has been allied to such disparate phyla as the Mollusca, Annelida or Chordata, it remains enigmatic. The nature and phylogenetic affinities of Tullimonstrum have defied confident systematic placement because none of its preserved anatomy provides unequivocal evidence of homology, without which comparative analysis fails. Here we show that the eyes of Tullimonstrum possess ultrastructural details indicating homology with vertebrate eyes. Anatomical analysis using scanning electron microscopy reveals that the eyes of Tullimonstrum preserve a retina defined by a thick sheet comprising distinct layers of spheroidal and cylindrical melanosomes. Time-of-flight secondary ion mass spectrometry and multivariate statistics provide further evidence that these microbodies are melanosomes. A range of animals have melanin in their eyes, but the possession of melanosomes of two distinct morphologies arranged in layers, forming retinal pigment epithelium, is a synapomorphy of vertebrates. Our analysis indicates that in addition to evidence of colour patterning, ecology and thermoregulation, fossil melanosomes can also carry a phylogenetic signal. Identification in Tullimonstrum of spheroidal and cylindrical melanosomes forming the remains of retinal pigment epithelium indicates that it is a vertebrate; considering its body parts in this new light suggests it was an anatomically unusual member of total group Vertebrata.

Tracking a Superstorm

NASA Image and Video Library

2017-12-08

Oct. 29, 2012 – A day before landfall, Sandy intensified into a Category 2 superstorm nearly 1,000 miles wide. Credit: NASA's Goddard Space Flight Center and NASA Center for Climate Simulation Video and images courtesy of NASA/GSFC/William Putman -- A NASA computer model simulates the astonishing track and forceful winds of Hurricane Sandy. Hurricane Sandy pummeled the East Coast late in 2012’s Atlantic hurricane season, causing 159 deaths and $70 billion in damages. Days before landfall, forecasts of its trajectory were still being made. Some computer models showed that a trough in the jet stream would kick the monster storm away from land and out to sea. Among the earliest to predict its true course was NASA’s GEOS-5 global atmosphere model. The model works by dividing Earth’s atmosphere into a virtual grid of stacked boxes. A supercomputer then solves mathematical equations inside each box to create a weather forecast predicting Sandy’s structure, path and other traits. The NASA model not only produced an accurate track of Sandy, but also captured fine-scale details of the storm’s changing intensity and winds. Watch the video to see it for yourself. For more information, please visit: gmao.gsfc.nasa.gov/research/atmosphericassim/tracking_hur... NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Strange-face Illusions During Interpersonal-Gazing and Personality Differences of Spirituality.

PubMed

Caputo, Giovanni B

Strange-face illusions are produced when two individuals gaze at each other in the eyes in low illumination for more than a few minutes. Usually, the members of the dyad perceive numinous apparitions, like the other's face deformations and perception of a stranger or a monster in place of the other, and feel a short lasting dissociation. In the present experiment, the influence of the spirituality personality trait on strength and number of strange-face illusions was investigated. Thirty participants were preliminarily tested for superstition (Paranormal Belief Scale, PBS) and spirituality (Spiritual Transcendence Scale, STS); then, they were randomly assigned to 15 dyads. Dyads performed the intersubjective gazing task for 10 minutes and, finally, strange-face illusions (measured through the Strange-Face Questionnaire, SFQ) were evaluated. The first finding was that SFQ was independent of PBS; hence, strange-face illusions during intersubjective gazing are authentically perceptual, hallucination-like phenomena, and not due to superstition. The second finding was that SFQ depended on the spiritual-universality scale of STS (a belief in the unitive nature of life; e.g., "there is a higher plane of consciousness or spirituality that binds all people") and the two variables were negatively correlated. Thus, strange-face illusions, in particular monstrous apparitions, could potentially disrupt binding among human beings. Strange-face illusions can be considered as 'projections' of the subject's unconscious into the other's face. In conclusion, intersubjective gazing at low illumination can be a tool for conscious integration of unconscious 'shadows of the Self' in order to reach completeness of the Self. Copyright © 2017 Elsevier Inc. All rights reserved.

Acardiac twin with externalized intestine adherent to placenta: unusual manifestation of omphalocele.

PubMed

Emery, Shawn Clark; Vaux, Keith K; Pretorius, Dolores; Masliah, Eliezer; Benirschke, Kurt

2004-01-01

TRAP (twin reversed arterial perfusion) syndrome produces an acardiac twin (acardiac monster, acardius, acardiacus, chorioangiopagus parasiticus, etc.). Acardiacs result from monozygotic multiple births in which three anatomic anomalies occur: (1) a fetus' cardiac development is disturbed; (2) artery-artery anastomosis carries blood from a normal ("pump") twin to the acardiac; (3) vein-vein anastomosis carries blood from the acardiac back to the normal twin. Whether reversal of blood flow in the acardiac results from or causes cardiac dysmorphogenesis has not been resolved. Acardiac twins demonstrate a complex constellation of malformations usually thought to result from reversed blood flow; omphalocele is particularly common. We report monochorionic monoamnionic male twins in which an acardiac twin demonstrated externalized intestines adherent to the placenta. The twins were delivered from a 30-year-old primigravida mother by cesarean section without maternal complications at 33 w. The mother has no significant past medical history. The macerated acardius had a 4-cm long attenuated umbilical cord with indeterminate number of vessels. Structures rostral to the thorax were absent save for one poorly developed hand and arm. The abdomen contained loose mesenchyme and no organs. The entire intestine (21 cm) along with two testes was located in a sac on the surface of the placenta. No histopathologic anomalies of formed structures were identified aside from spatial relationships and incomplete development. The normal twin required no intensive care and is doing well. To our knowledge, this is the first report of externalized intestine, which may represent an unusual consequence of omphalocele.

Preventing Rape of the Observatory: Thoughts on the Urgency of Preserving Historic Astronomical Artifacts

NASA Astrophysics Data System (ADS)

Bell, T. E.

2005-12-01

"What good is this century-old monster refractor? Sell it and use the money to buy a brand new go-to reflector useful for teaching students and advancing astronomy." So argues logic that is endangering an increasing number of university observatories around the U.S. (if not the rest of the world), even up to the Yerkes Observatory and its 40-inch Clark, world's largest refractor by the acknowledged world's best lens-makers. While most non-historians readily accept the value of preserving our cultural heritage in rare and precious documents (such as the Declaration of Independence), artifacts (such as Stradivarius violins), and institutions (such as the birthplaces of U.S. Presidents), they tend not to think of astronomical observatories as part of cultural heritage-with a result that history is crumbling apace to the wrecking ball. In early October, the Antique Telescope Society convened a special 60-minute session discussing philosophical why's and practical how's of preserving astronomical assets (including historically significant telescopes, observatory buildings, auxiliary equipment used to make observations or calculate results, and libraries of books and papers). This paper will summarize the discussion's key insights - including the assessing and assigning of value to old vs. new telescopes, and the roles of politics, funding and fund-raising, publicity (positive and negative), education, use as a form of preservation, innovative solutions by private collectors (including "half-way houses" for homeless instruments), restoration vs. renovation, special problems facing very large telescopes, and lessons learned from both failures and success.

[Energy drinks: an unknown risk].

PubMed

Petit, Aymeric; Levy, Fanny; Lejoyeux, Michel; Reynaud, Michel; Karila, Laurent

2012-05-01

The term "energy drink" designates "any product in the form of a drink or concentrated liquid, which claims to contain a mixture of ingredients having the property to raise the level of energy and vivacity". The main brands, Red Bull, Dark Dog, Rockstar, Burn, and Monster, are present in food stores, sports venues, and bars among other soft drinks and fruit juices. Their introduction into the French market raised many reluctances, because of the presence of taurine, caffeine and glucuronolactone. These components present in high concentrations, could be responsible for adverse effects on health. The association of energy drinks and spirits is widely found among adolescents and adults who justify drinking these mixed drinks by their desire to drink more alcohol while delaying drunkenness. Given the importance of the number of incidents reported among the energy drinks consumers, it seemed appropriate to make a synthesis of available data and to establish causal links between the use of these products and the development of health complications. For a literature review, we selected scientific articles both in English and French published between 2001 and 2011 by consulting the databases Medline, Embase, PsycINFO and Google Scholar. The words used alone or in combination are "energy dinks", "caffeine", "taurine", "toxicity", "dependence". An occasional to a moderate consumption of these drinks seems to present little risk for healthy adults. However, excessive consumption associated with the use of alcohol or drugs in amounts that far exceed the manufacturers recommended amount, could be responsible for negative consequences on health, particularly among subjects with cardiovascular disease.

M by Fritz Lang (Germany, 1931) Phenomenology of Evil: a serial killer and his social group.

PubMed

Secchi, Cesare

2015-10-01

In 1931 an unknown murderer of little girls (Peter Lorre) is terrorizing the city of Berlin. We see him entice a new victim, the little Elsie Beckmann, who is coming home from school: whistling a tune by Grieg, he buys her a balloon from a blind beggar. When her corpse is discovered, the police undertake a major mobilization aimed at seeking the serial killer in the criminal underworld; meanwhile, the ever more terrified population starts to see the dangerous murderer in everyone. Since the roundups and incursions into the seediest parts of town disturb the gangsters' activities, the leaders of organized crime, headed by Schränker (Gustav Gründgens), take it upon themselves also to hunt down the solitary child-killer, engaging the community of beggars. Every corner of the city is catalogued and sifted by the dual activity of the police and the gangsters. The 'monster', a former psychiatric patient, mild and harmless in manner, is finally tracked down via two parallel routes: the clue of a cigarette packet enables Inspector Lohmann (Otto Wernicke) to track down the serial killer's address, while the blind beggar recognizes the whistled tune. The murderer is identified by a 'slap' from a young criminal which leaves an M marked in chalk on a shoulder of the man's overcoat. Thus he is caught and undergoes a kind of trial at the hands of the gangsters who tie him up in order to lynch him, but they are interrupted by the arrival of the forces of law and order. Copyright © 2015 Institute of Psychoanalysis.

The donor organ as an 'object a': a Lacanian perspective on organ donation and transplantation medicine.

PubMed

Zwart, Hub

2014-11-01

Bioethical discourse on organ donation covers a wide range of topics, from informed consent procedures and scarcity issues up to 'transplant tourism' and 'organ trade'. This paper presents a 'depth ethics' approach, notably focussing on the tensions, conflicts and ambiguities concerning the status of the human body (as something which constitutes a whole, while at the same time being a set of replaceable elements or parts). These will be addressed from a psychoanalytical (Lacanian) angle. First, I will outline Lacan's view on embodiment as such. Subsequently, I will argue that, for organ recipients, the donor organ becomes what Lacan refers to as an object a, the 'partial object' of desire, the elusive thing we are deprived of, apparently beyond our grasp. Within the recipient's body an empty space emerges, a kind of 'vacuole', once occupied by a faltering organ (now removed). This space can only be filled by a 'gift' from the other, by an object a. Once implanted, however, this implant becomes an 'extimate' object: something both 'external' and 'intimate', both 'embedded' and 'foreign', and which is bound to remain an object of concern for quite some time, if not for life. A Lacanian analysis allows us, first of all, to address the question what organ transplantation has in common with other bodily practices involving bodily parts procured from others, such as cannibalism. But it also reveals the basic difference between the two, as well as the distance between the 'fragmented body' of Frankenstein's 'monster'--as an aggregate of replaceable parts--and the multiple organ recipients (the 'puzzle people') of today.

Atomic force microscopy for cellular level manipulation: imaging intracellular structures and DNA delivery through a membrane hole.

PubMed

Afrin, Rehana; Zohora, Umme Salma; Uehara, Hironori; Watanabe-Nakayama, Takahiro; Ikai, Atsushi

2009-01-01

The atomic force microscope (AFM) is a versatile tool for imaging, force measurement and manipulation of proteins, DNA, and living cells basically at the single molecular level. In the cellular level manipulation, extraction, and identification of mRNA's from defined loci of a cell, insertion of plasmid DNA and pulling of membrane proteins, for example, have been reported. In this study, AFM was used to create holes at defined loci on the cell membrane for the investigation of viability of the cells after hole creation, visualization of intracellular structure through the hole and for targeted gene delivery into living cells. To create large holes with an approximate diameter of 5-10 microm, a phospholipase A(2) coated bead was added to the AFM cantilever and the bead was allowed to touch the cell surface for approximately 5-10 min. The evidence of hole creation was obtained mainly from fluorescent image of Vybrant DiO labeled cell before and after the contact with the bead and the AFM imaging of the contact area. In parallel, cells with a hole were imaged by AFM to reveal intracellular structures such as filamentous structures presumably actin fibers and mitochondria which were identified with fluorescent labeling with rhodamine 123. Targeted gene delivery was also attempted by inserting an AFM probe that was coated with the Monster Green Fluorescent Protein phMGFP Vector for transfection of the cell. Following targeted transfection, the gene expression of green fluorescent protein (GFP) was observed and confirmed by the fluorescence microscope. Copyright (c) 2009 John Wiley & Sons, Ltd.

Pestilence, riots, lynchings and desecration of corpses. The sleep of reason produces monsters.

PubMed

Sabbatani, Sergio; Fiorino, Sirio

2016-06-01

Vampirism has been a component of Central European and Balkan folklore since the Middle Ages and was often believed to be responsible for the transmission of serious infectious diseases such as plague and tuberculosis/consumption. Vampirism was believed to be spread within the same family or village and if the rite of the so-called second burial after death was not performed. The practice of "second burial" entailed exhumation of the body and the removal of the shroud from the mouth of the corpse, and a search for evidence if the corpse had chewed the cloth. If the shroud was chewed, a handful of earth or a brick was put into the body's mouth so that the vampire could no longer harm others. In some cases, the corpse was decapitated and an awl, made of ash, was thrust into its chest. Furthermore, the limbs were nailed down to prevent its movements. Remarkably, these beliefs were not restricted to the popular classes, but were also debated by theologians, political scientists at the height of the eighteenth century (Enlightenment). In the Habsburg Empire, this question attained such important political, social as well as health connotations as to force the Empress Maria Theresa to entrust an ad hoc study to her personal physician Gerard van Swieten with a view to determining what was true about the apparitions of vampires that occurred throughout central Europe and in the Balkans. The result of this investigation led to a ban on the "second burial" rites. Despite this prohibition, the practice of necrophilia on the bodies of suspected people continued, and both a cultured and popular literature on vampirism continued to flourish well into the nineteenth century.

The green eyed monster in the bottle: Relationship contingent self-esteem, romantic jealousy, and alcohol-related problems.

PubMed

DiBello, Angelo M; Rodriguez, Lindsey M; Hadden, Benjamin W; Neighbors, Clayton

2015-10-01

Previous research suggests that both jealousy and relationship contingent self-esteem (RCSE) are related to alcohol use and alcohol-related problems. No work, however, has examined these two constructs together as they relate to motives for alcohol use and alcohol-related problems. The current study aims to build upon emerging literature examining different types of jealousy (i.e., emotional, cognitive, and behavioral), relationship quality (i.e., satisfaction, commitment, closeness), RCSE, and alcohol use. More specifically, the current study aimed to examine the associations between RCSE and drinking to cope and RCSE and alcohol-related problems, in the context of the different types of jealousy. Moreover, the current study aimed to assess whether the associations between RCSE, jealousy, and drinking outcomes vary as a function of relationship quality. Two hundred and seventy seven individuals (87% female) at a large southern university participated in the study. They completed measures of RCSE, relationship satisfaction, commitment, closeness, and jealousy as well as alcohol-related outcomes. Using PROCESS, moderated mediational analyses were used to evaluate different types of jealousy as mediators of the association between RCSE and drinking to cope/alcohol-related problems. Further, we aimed to examine whether relationship quality moderated the association between RCSE and jealousy in predicting alcohol-related variables. Results indicated that cognitive jealousy mediated the association between both RCSE and drinking to cope and RCSE and alcohol-related problems. Further, relationship satisfaction, commitment, and closeness were all found to moderate the association between RSCE and cognitive jealousy such that at lower, but not higher levels of satisfaction, commitment, and closeness, cognitive jealousy mediated the association between RCSE and drinking to cope and RCSE and alcohol-related problems. Copyright © 2015. Published by Elsevier Ltd.

MONSTER IN THE DARK: THE ULTRALUMINOUS GRB 080607 AND ITS DUSTY ENVIRONMENT

DOE Office of Scientific and Technical Information (OSTI.GOV)

Perley, D. A.; Morgan, A. N.; Miller, A. A.

2011-02-15

We present early-time optical through infrared photometry of the bright Swift gamma-ray burst (GRB) 080607, starting only 6 s following the initial trigger in the rest frame. Complemented by our previously published spectroscopy, this high-quality photometric data set allows us to solve for the extinction properties of the redshift 3.036 sightline, giving perhaps the most detailed information to date on the ultraviolet continuum absorption properties of any sightline outside our Local Group. The extinction properties are not adequately modeled by any ordinary extinction template (including the average Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud curves), partially because themore » 2175 A feature (while present) is weaker by about a factor of two than when seen under similar circumstances locally. However, the spectral energy distribution is exquisitely fitted by the more general Fitzpatrick and Massa parameterization of Local-Group extinction, putting it in the same family as some peculiar Milky Way extinction curves. After correcting for this (considerable, A{sub V} = 3.3 {+-} 0.4 mag) extinction, GRB 080607 is revealed to have been among the most optically luminous events ever observed, comparable to the naked-eye burst GRB 080319B. Its early peak time (t{sub rest} < 6 s) indicates a high initial Lorentz factor ({Gamma}>600), while the extreme luminosity may be explained in part by a large circumburst density. Only because of its early high luminosity could the afterglow of GRB 080607 be studied in such detail in spite of the large attenuation and great distance, making this burst an excellent prototype for the understanding of other highly obscured extragalactic objects, and of the class of 'dark' GRBs in particular.« less

Hubble Sees a "Mess of Stars"

NASA Image and Video Library

2015-08-14

Bursts of pink and red, dark lanes of mottled cosmic dust, and a bright scattering of stars — this NASA/ESA Hubble Space Telescope image shows part of a messy barred spiral galaxy known as NGC 428. It lies approximately 48 million light-years away from Earth in the constellation of Cetus (The Sea Monster). Although a spiral shape is still just about visible in this close-up shot, overall NGC 428’s spiral structure appears to be quite distorted and warped, thought to be a result of a collision between two galaxies. There also appears to be a substantial amount of star formation occurring within NGC 428 — another telltale sign of a merger. When galaxies collide their clouds of gas can merge, creating intense shocks and hot pockets of gas, and often triggering new waves of star formation. NGC 428 was discovered by William Herschel in December 1786. More recently a type of supernova designated SN2013ct was discovered within the galaxy by Stuart Parker of the BOSS (Backyard Observatory Supernova Search) project in Australia and New Zealand, although it is unfortunately not visible in this image. This image was captured by Hubble’s Advanced Camera for Surveys (ACS) and Wide Field and Planetary Camera 2 (WFPC2). Image credit: ESA/Hubble and NASA and S. Smartt (Queen's University Belfast), Acknowledgements: Nick Rose and Flickr user pennine cloud NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

The ‘Tully monster’ is a vertebrate

NASA Astrophysics Data System (ADS)

McCoy, Victoria E.; Saupe, Erin E.; Lamsdell, James C.; Tarhan, Lidya G.; McMahon, Sean; Lidgard, Scott; Mayer, Paul; Whalen, Christopher D.; Soriano, Carmen; Finney, Lydia; Vogt, Stefan; Clark, Elizabeth G.; Anderson, Ross P.; Petermann, Holger; Locatelli, Emma R.; Briggs, Derek E. G.

2016-04-01

Problematic fossils, extinct taxa of enigmatic morphology that cannot be assigned to a known major group, were once a major issue in palaeontology. A long-favoured solution to the ‘problem of the problematica’, particularly the ‘weird wonders’ of the Cambrian Burgess Shale, was to consider them representatives of extinct phyla. A combination of new evidence and modern approaches to phylogenetic analysis has now resolved the affinities of most of these forms. Perhaps the most notable exception is Tullimonstrum gregarium, popularly known as the Tully monster, a large soft-bodied organism from the late Carboniferous Mazon Creek biota (approximately 309-307 million years ago) of Illinois, USA, which was designated the official state fossil of Illinois in 1989. Its phylogenetic position has remained uncertain and it has been compared with nemerteans, polychaetes, gastropods, conodonts, and the stem arthropod Opabinia. Here we review the morphology of Tullimonstrum based on an analysis of more than 1,200 specimens. We find that the anterior proboscis ends in a buccal apparatus containing teeth, the eyes project laterally on a long rigid bar, and the elongate segmented body bears a caudal fin with dorsal and ventral lobes. We describe new evidence for a notochord, cartilaginous arcualia, gill pouches, articulations within the proboscis, and multiple tooth rows adjacent to the mouth. This combination of characters, supported by phylogenetic analysis, identifies Tullimonstrum as a vertebrate, and places it on the stem lineage to lampreys (Petromyzontida). In addition to increasing the known morphological disparity of extinct lampreys, a chordate affinity for T. gregarium resolves the nature of a soft-bodied fossil which has been debated for more than 50 years.

Visual perception during mirror gazing at one's own face in schizophrenia.

PubMed

Caputo, Giovanni B; Ferrucci, Roberta; Bortolomasi, Marco; Giacopuzzi, Mario; Priori, Alberto; Zago, Stefano

2012-09-01

In normal observers gazing at one's own face in the mirror for some minutes, at a low illumination level, triggers the perception of strange faces, a new perceptual illusion that has been named 'strange-face in the mirror'. Subjects see distortions of their own faces, but often they see monsters, archetypical faces, faces of dead relatives, and of animals. We designed this study to primarily compare strange-face apparitions in response to mirror gazing in patients with schizophrenia and healthy controls. The study included 16 patients with schizophrenia and 21 healthy controls. In this paper we administered a 7 minute mirror gazing test (MGT). Before the mirror gazing session, all subjects underwent assessment with the Cardiff Anomalous Perception Scale (CAPS). When the 7minute MGT ended, the experimenter assessed patients and controls with a specifically designed questionnaire and interviewed them, asking them to describe strange-face perceptions. Apparitions of strange-faces in the mirror were significantly more intense in schizophrenic patients than in controls. All the following variables were higher in patients than in healthy controls: frequency (p<.005) and cumulative duration of apparitions (p<.009), number and types of strange-faces (p<.002), self-evaluation scores on Likert-type scales of apparition strength (p<.03) and of reality of apparitions (p<.001). In schizophrenic patients, these Likert-type scales showed correlations (p<.05) with CAPS total scores. These results suggest that the increase of strange-face apparitions in schizophrenia can be produced by ego dysfunction, by body dysmorphic disorder and by misattribution of self-agency. MGT may help in completing the standard assessment of patients with schizophrenia, independently of hallucinatory psychopathology. Copyright © 2012 Elsevier B.V. All rights reserved.

Behemoth Black Hole Found in an Unlikely Place

NASA Image and Video Library

2017-12-08

This computer-simulated image shows a supermassive black hole at the core of a galaxy. The black region in the center represents the black hole’s event horizon, where no light can escape the massive object’s gravitational grip. The black hole’s powerful gravity distorts space around it like a funhouse mirror. Light from background stars is stretched and smeared as the stars skim by the black hole. Credits: NASA, ESA, and D. Coe, J. Anderson, and R. van der Marel (STScI) More info: Astronomers have uncovered a near-record breaking supermassive black hole, weighing 17 billion suns, in an unlikely place: in the center of a galaxy in a sparsely populated area of the universe. The observations, made by NASA’s Hubble Space Telescope and the Gemini Telescope in Hawaii, may indicate that these monster objects may be more common than once thought. Until now, the biggest supermassive black holes – those roughly 10 billion times the mass of our sun – have been found at the cores of very large galaxies in regions of the universe packed with other large galaxies. In fact, the current record holder tips the scale at 21 billion suns and resides in the crowded Coma galaxy cluster that consists of over 1,000 galaxies. More: www.nasa.gov/feature/goddard/2016/behemoth-black-hole-fou... NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

An associative account of how the obesogenic environment biases adolescents' food choices.

PubMed

Watson, P; Wiers, R W; Hommel, B; Ridderinkhof, K R; de Wit, S

2016-01-01

Adolescents and children are the targets of much food advertising, the majority of which is for unhealthy snacks. Although the effects of advertising on food preferences and consummatory behavior are well documented, our understanding of the underlying mechanisms is still limited. The present study investigates an associative (ideomotor) mechanism by which exposure to rewarding (snack) outcomes may activate behavior that previously resulted in these rewards. Specifically, we used a computerized task to investigate whether exposing adolescents to food pictures directly, or to Pavlovian cues predictive of those food pictures, would bias their subsequent responses towards the presented/signaled food. Furthermore, we assessed whether this effect was particularly pronounced with palatable, high-calorie snacks (crisps and chocolate) relative to low-calorie snacks (tomatoes and cucumber). In two experiments, adolescents learnt that certain key presses would yield particular food pictures - some high calorie and others low calorie - before learning Pavlovian associations between cues (cartoon monsters) and these same food pictures. Subsequently, in a response-priming test, we examined the extent to which the food pictures and Pavlovian cues spontaneously primed the previously associated response. The results show that we replicated, in adolescents, previous demonstrations of ideomotor response priming in adults: food pictures biased responding towards the response that previously yielded them, and this effect transferred to the Pavlovian cues. Furthermore, the priming effect was significantly stronger for high-calorie rewards than for low-calorie. These findings indicate that the ideomotor mechanism plays an important role in the detrimental effect of our obesogenic environment, with its plethora of unhealthy food reminders, on adolescents' food-related choices. Copyright © 2015 Elsevier Ltd. All rights reserved.

The ‘Tully monster’ is a vertebrate

DOE Office of Scientific and Technical Information (OSTI.GOV)

McCoy, Victoria E.; Saupe, Erin E.; Lamsdell, James C.

Abstract Problematic fossils, extinct taxa of enigmatic morphology that cannot be assigned to a known major group, were once a major issue in palaeontology. A long-favoured solution to the 'problem of the problematica'(1), particularly the 'weird wonders'(2) of the Cambrian Burgess Shale, was to consider them representatives of extinct phyla. A combination of new evidence and modern approaches to phylogenetic analysis has now resolved the affinities of most of these forms. Perhaps the most notable exception is Tullimonstrum gregarium(3), popularly known as the Tully monster, a large soft-bodied organism from the late Carboniferous Mazon Creek biota (approximately 309-307 million yearsmore » ago) of Illinois, USA, which was designated the official state fossil of Illinois in 1989. Its phylogenetic position has remained uncertain and it has been compared with nemerteans(4,5), polychaetes(4), gastropods(4), conodonts(6), and the stem arthropod Opabinia(4). Here we review the morphology of Tullimonstrum based on an analysis of more than 1,200 specimens. We find that the anterior proboscis ends in a buccal apparatus containing teeth, the eyes project laterally on a long rigid bar, and the elongate segmented body bears a caudal fin with dorsal and ventral lobes(3-6). We describe new evidence for a notochord, cartilaginous arcualia, gill pouches, articulations within the proboscis, and multiple tooth rows adjacent to the mouth. This combination of characters, supported by phylogenetic analysis, identifies Tullimonstrum as a vertebrate, and places it on the stem lineage to lampreys (Petromyzontida). In addition to increasing the known morphological disparity of extinct lampreys(7-9), a chordate affinity for T. gregarium resolves the nature of a soft-bodied fossil which has been debated for more than 50 years« less

The making of a monster: postnatal ontogenetic changes in craniomandibular shape in the great sabercat Smilodon.

PubMed

Christiansen, Per

2012-01-01

Derived sabercats had craniomandibular morphologies that in many respects were highly different from those of extant felids, and this has often been interpreted functionally as adaptations for predation at extreme gape angles with hypertrophied upper canines. It is unknown how much of this was a result of intraspecific postnatal ontogeny, since juveniles of sabercats are rare and no quantitative study has been made of craniomandibular ontogeny. Postnatal ontogenetic craniomandibular shape changes in two morphologically derived sabercats, Smilodon fatalis and S. populator, were analysed using geometric morphometrics and compared to three species of extant pantherines, the jaguar, tiger, and Sunda clouded leopard. Ontogenetic shape changes in Smilodon usually involved the same areas of the cranium and mandible as in extant pantherines, and large-scale modularization was similar, suggesting that such may have been the case for all felids, since it followed the same trends previously observed in other mammals. However, in other respects Smilodon differed from extant pantherines. Their crania underwent much greater and more localised ontogenetic shape changes than did the mandibles, whereas crania and mandibles of extant pantherines underwent smaller, fewer and less localised shape changes. Ontogenetic shape changes in the two species of Smilodon are largely similar, but differences are also present, notably those which may be tied to the presence of larger upper canines in S. populator. Several of the specialized cranial characters differentiating adult Smilodon from extant felids in a functional context, which are usually regarded as evolutionary adaptations for achieving high gape angles, are ontogenetic, and in several instances ontogeny appears to recapitulate phylogeny to some extent. No such ontogenetic evolutionary adaptive changes were found in the extant pantherines. Evolution in morphologically derived sabercats involved greater cranial ontogenetic changes than among extant felids, resulting in greatly modified adult craniomandibular morphologies.

Ambush frequency should increase over time during optimal predator search for prey.

PubMed

Alpern, Steve; Fokkink, Robbert; Timmer, Marco; Casas, Jérôme

2011-11-07

We advance and apply the mathematical theory of search games to model the problem faced by a predator searching for prey. Two search modes are available: ambush and cruising search. Some species can adopt either mode, with their choice at a given time traditionally explained in terms of varying habitat and physiological conditions. We present an additional explanation of the observed predator alternation between these search modes, which is based on the dynamical nature of the search game they are playing: the possibility of ambush decreases the propensity of the prey to frequently change locations and thereby renders it more susceptible to the systematic cruising search portion of the strategy. This heuristic explanation is supported by showing that in a new idealized search game where the predator is allowed to ambush or search at any time, and the prey can change locations at intermittent times, optimal predator play requires an alternation (or mixture) over time of ambush and cruise search. Thus, our game is an extension of the well-studied 'Princess and Monster' search game. Search games are zero sum games, where the pay-off is the capture time and neither the Searcher nor the Hider knows the location of the other. We are able to determine the optimal mixture of the search modes when the predator uses a mixture which is constant over time, and also to determine how the mode mixture changes over time when dynamic strategies are allowed (the ambush probability increases over time). In particular, we establish the 'square root law of search predation': the optimal proportion of active search equals the square root of the fraction of the region that has not yet been explored.

The effect of hydration state and energy balance on innate immunity of a desert reptile.

PubMed

Moeller, Karla T; Butler, Michael W; Denardo, Dale F

2013-05-04

Immune function is a vital physiological process that is often suppressed during times of resource scarcity due to investments in other physiological systems. While energy is the typical currency that has been examined in such trade-offs, limitations of other resources may similarly lead to trade-offs that affect immune function. Specifically, water is a critical resource with profound implications for organismal ecology, yet its availability can fluctuate at local, regional, and even global levels. Despite this, the effect of osmotic state on immune function has received little attention. Using agglutination and lysis assays as measures of an organism's plasma concentration of natural antibodies and capacity for foreign cell destruction, respectively, we tested the independent effects of osmotic state, digestive state, and energy balance on innate immune function in free-ranging and laboratory populations of the Gila monster, Heloderma suspectum. This desert-dwelling lizard experiences dehydration and energy resource fluctuations on a seasonal basis. Dehydration was expected to decrease innate immune function, yet we found that dehydration increased lysis and agglutination abilities in both lab and field studies, a relationship that was not simply an effect of an increased concentration of immune molecules. Laboratory-based differences in digestive state were not associated with lysis or agglutination metrics, although in our field population, a loss of fat stores was correlated with an increase in lysis. Depending on the life history of an organism, osmotic state may have a greater influence on immune function than energy availability. Thus, consideration of osmotic state as a factor influencing immune function will likely improve our understanding of ecoimmunology and the disease dynamics of a wide range of species.

The effect of hydration state and energy balance on innate immunity of a desert reptile

PubMed Central

2013-01-01

Introduction Immune function is a vital physiological process that is often suppressed during times of resource scarcity due to investments in other physiological systems. While energy is the typical currency that has been examined in such trade-offs, limitations of other resources may similarly lead to trade-offs that affect immune function. Specifically, water is a critical resource with profound implications for organismal ecology, yet its availability can fluctuate at local, regional, and even global levels. Despite this, the effect of osmotic state on immune function has received little attention. Results Using agglutination and lysis assays as measures of an organism’s plasma concentration of natural antibodies and capacity for foreign cell destruction, respectively, we tested the independent effects of osmotic state, digestive state, and energy balance on innate immune function in free-ranging and laboratory populations of the Gila monster, Heloderma suspectum. This desert-dwelling lizard experiences dehydration and energy resource fluctuations on a seasonal basis. Dehydration was expected to decrease innate immune function, yet we found that dehydration increased lysis and agglutination abilities in both lab and field studies, a relationship that was not simply an effect of an increased concentration of immune molecules. Laboratory-based differences in digestive state were not associated with lysis or agglutination metrics, although in our field population, a loss of fat stores was correlated with an increase in lysis. Conclusions Depending on the life history of an organism, osmotic state may have a greater influence on immune function than energy availability. Thus, consideration of osmotic state as a factor influencing immune function will likely improve our understanding of ecoimmunology and the disease dynamics of a wide range of species. PMID:23642164

Is it turquoise + fuchsia = purple or is it turquoise + fuchsia = blue?

NASA Astrophysics Data System (ADS)

Beretta, Giordano B.; Moroney, Nathan M.

2011-01-01

The first step in communicating color is to name it. The second step is color semiotics. The third step is introducing structure in the set of colors. In color education at all levels, this structure often takes the form of formulæ, like red + green = yellow, or turquoise + red = black. In recent times, Johannes Itten's color theory and its associated color wheel have been very influential, mostly through its impact on Bauhaus, although a number of color order systems and circles have been introduced over the centuries. Students get confused when they are trying to formulate the color name arithmetic using the structure of color order systems and concepts like complementary colors and opponent colors. Suddenly turquoise + fuchsia = purple instead of blue; purple and violet become blurred, and finally the student's head explodes under the epistemological pressures of Itten, Albers, Goethe, Runge, Newton, da Vinci, and all the other monsters of color structure. In this contribution we propose a systematic presentation of structure in color, from color theories to color naming. We start from the concept of color perception introduced by da Vinci and work ourselves through color measurement, color formation, and color naming, to develop the basis for a robust system based on table lookup and interpolation. One source of confusion is that color naming has been quite loose in color theory, where for example red can be used interchangeably with fuchsia, and blue with turquoise. Furthermore, common color terms are intermingled with technical colorant terms, for example cyan and aqua or fuchsia and magenta. We present the evolution of a few color terms, some of which have experienced a radical transition over the centuries, and describe an experiment showing the robustness of crowd-sourcing for color naming.

Beyond the Event Horizon: Education with Black Holes

NASA Astrophysics Data System (ADS)

Silva, Sarah; Cominsky, L.; Plait, P.; SSU E/PO Group

2006-09-01

The Sonoma State University NASA Education and Public Outreach Program (SSU E/PO), in collaboration with the Denver Museum of Nature & Science (DMNS), NOVA, Thomas Lucas Productions (TLP), the National Science Foundation and E/PO groups across NASA's Astrophysics Division, is creating a series of educational and outreach products for both formal and informal educational settings. The formal (in-class) products are closely tied with the informal (museum and television) products. An NSF-funded digital planetarium show titled "Black Holes: The Other Side of Infinity" was created by DMNS and TLP and is currently showing at several venues, with more planned. Through funding from the Swift and GLAST missions, SSU has developed an accompanying educator workshop and guide to train museum personnel in the use of black hole educational materials so that they can give professional development workshops to local teachers. In addition, SSU E/PO has worked with TLP and NOVA to create a television program ("Monster of the Milky Way") will premiere in the fall of 2006 with accompanying online educational materials. The educator guide materials include activities from NASA Astrophysics missions such as GLAST, Swift, XMM-Newton, and Gravity Probe-B, as well as from the Center for Science Education at Space Sciences Laboratory and the HEASARC education programs. We are also creating an online educational resource for use by anyone who wants to find information about black holes. It will have interactive features, including a possible museum kiosk where visitors can explore black holes. All products that are developed as a part of this program include integrated evaluation and assessment. The planetarium show has already had formative evaluation and is in the process of summative evaluation. The workshops include evaluation and follow-up work with the participating educators.

Teratology in cultural documents and today.

PubMed

Schumacher, Gert-Horst

2004-12-01

Teratology is the science of congenital malformations. The incidence of birth defects amounts to 2-3%, but it doubles postnatal owing to the fact that many dysfunctions are not discernible at birth. Congenital malformations were already known in ancient cultures, records from Assyrian and Babylonian astrologists as well as from physicians and philosophers of the Hippocratic era are testifying it. In medieval times they were recognized as supernatural phenomenons, terata, from what the term TERATOLOGY derived. In the eyes of the superstitious people affected stillborns were regarded as monster, symbol of devil or miracle. The foundation of anatomy as a science by Vesalius marked the beginning of a reorientation. In the 17th century, when the age of enlightenment began, ideas concerning the origin of birth defects became more objective. Original studies dealing with congenital malformations became common in the 18th century. Fundamental discoveries made by microscopy placed Teratology on a truly scientific basis. Significant impetus was grown to teratological research with the discovery of Gregg (1941) that German measles (rubella virus) of pregnant women caused birth defects in the embryo and the contergan disaster (1959--1962). Congenital malformations originate from genetic factors (single gene defects and chromosomal aberrations) and environmental factors, such as radiation, drugs, chemicals, and infectious agents. The susceptibility of teratogen depends on the period of embryonal development, which is classified into gametogenesis, blastogenesis, embryogenesis and fetogenesis. The Food and Drug Administration of the USA published guidelines for teratogenetic testing (1966). There are in-vivo and in-vitro-test programmes, the latter became of increasing importance owing to the large number of chemicals to be tested and the activities of opponents against animal experiments. Although great advances were made, the problem remained to transfer results from in-vivo and in-vitro tests to the constitution of man without risk.

Vision of Space Exploration Possibilities and limits of a human space conquest.

NASA Astrophysics Data System (ADS)

Zelenyi, Lev

Few generations of a schoolboys, which later become active and productive space researchers, have been brought up on a science fiction books. These books told us about travels to other Galaxies with velocities larger then velocity of light, meetings with friendly aliens (necessarily with communistic mentalities in Soviet Union books), star wars with ugly space monsters (in the western hemisphere books), etc. Beginning of Space age (4/10/1957) opened the door to a magic box, full of scientific discoveries, made mostly by robotic satellites and spacecraft. However, already the first human space trips clearly demonstrated that space is vigorously hostile to a human beings. Space medicine during the years since Gagarin flight, made an outstanding progress in supporting human presence at orbital stations, but the radiation hazards and problem of hypomagnetism are still opened and there is no visible path to their solution. So the optimistic slogan of 60-ies “Space is Our Place” is not supported by an almost half a century practice. Space never will be a comfortable place for soft and vulnerable humans? There is a general consensus that man will be on Mars during this century (or even its first part). This is very difficult but task it seems to be realistic after the significant advance of modern technologies will be made. But, is there any real need for humans to travel beyond the Mars orbit or to the inner regions of the Solar system? Will the age of Solar system exploration comes to its logical as it was described by Stanislav Lem in his famous book “Return from stars”? The author of this talk has more questions than answers, and thinks that PEX1 Panel on Exploration is just a right place to discuss these usually by passed topics.

Batch manufacturing: Six strategic needs

DOE Office of Scientific and Technical Information (OSTI.GOV)

Ash, R.H.; Chappell, D.A.

1995-08-01

Since the advent of industrial digital control systems in the mid-1970s, industry has had the promise of integrated, configurable digital batch control systems to replace the morass of electromechanical devices like relays and stepping switches, recorders, and indicators which comprised the components of previous generations of batch control systems - the {open_quotes}monolithic monsters{close_quotes} of the 1960s and earlier. To help fulfill that promise, there have been many wide-ranging proprietary automation solutions for batch control since 1975, many of them technically excellent. However, even the best examples suffered from the lack of a common language and unifying concept permitting separate systemsmore » to be interconnected and work together. Today, some 20 years after the digital revolution began, industry has microprocessors, memory chips, data highways, and other marvelous technology to help automate the control of discontinuous processes. They also are on the way to having an accepted standard for batch automation, ISA S88. Batching systems are at once conceptually simple but executionally complex. The notion of adding ingredients one at a time to a vat, mixing, and then processing into final form is as old as the stone age. Every homemaker on earth, male or female, is familiar with how to follow a recipe to create some sumptuous item of culinary delight. Food recipes, so familiar and ubiquitous, are really just microcosms of the S88 recipe standard. They contain the same components: (1) Header (name and description of item being prepared, sometimes serving size); (2) Formula (list and amount of ingredients); (3) Equipment requirements (pans, mixing and cooking equipment); (4) Procedure (description of order of ingredient addition, mixing and other processing steps, baking/cooling time, and other processing steps); and (5) Other information (safety, cautions, and other miscellaneous instructions).« less

New Panorama Reveals More Than a Thousand Black Holes

NASA Astrophysics Data System (ADS)

2007-03-01

By casting a wide net, astronomers have captured an image of more than a thousand supermassive black holes. These results give astronomers a snapshot of a crucial period when these monster black holes are growing, and provide insight into the environments in which they occur. The new black hole panorama was made with data from NASA's Chandra X-ray Observatory, the Spitzer Space Telescope and ground-based optical telescopes. The black holes in the image are hundreds of millions to several billion times more massive than the sun and lie in the centers of galaxies. X-ray, IR & Optical Composites of Obscured & Unobscured AGN in Bootes Field X-ray, IR & Optical Composites of Obscured & Unobscured AGN in Bootes Field Material falling into these black holes at high rates generates huge amounts of light that can be detected in different wavelengths. These systems are known as active galactic nuclei, or AGN. "We're trying to get a complete census across the Universe of black holes and their habits," said Ryan Hickox of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Mass. "We used special tactics to hunt down the very biggest black holes." Instead of staring at one relatively small part of the sky for a long time, as with the Chandra Deep Fields -- two of the longest exposures obtained with the observatory -- and other concentrated surveys, this team scanned a much bigger portion with shorter exposures. Since the biggest black holes power the brightest AGN, they can be spotted at vast distances, even with short exposures. Scale Chandra Images to Full Moon Scale Chandra Images to Full Moon "With this approach, we found well over a thousand of these monsters, and have started using them to test our understanding of these powerful objects," said co-investigator Christine Jones, also of the CfA. The new survey raises doubts about a popular current model in which a supermassive black hole is surrounded by a doughnut-shaped region, or torus, of gas. An observer from Earth would have their view blocked by this torus by different amounts, depending on the orientation of the torus. According to this model, astronomers would expect a large sample of black holes to show a range of absorption of the radiation from the nuclei. This absorption should range from completely exposed to completely obscured, with most in-between. Nuclei that are completely obscured are not detectable, but heavily obscured ones are. "Instead of finding a whole range, we found nearly all of the black holes are either naked or covered by a dense veil of gas," said Hickox. "Very few are in between, which makes us question how well we know the environment around these black holes." This study found more than 600 obscured and 700 unobscured AGN, located between about six to 11 billion light years from Earth. They were found using an early application of a new search method. By looking at the infrared colors of objects with Spitzer, AGN can be separated from stars and galaxies. The Chandra and optical observations then verify these objects are AGN. This multi-wavelength method is especially efficient at finding obscured AGN. "These results are very exciting, using two NASA Great Observatories to find and understand the largest sample of obscured supermassive black holes ever found in the distant universe", said co-investigator Daniel Stern, of NASA's Jet Propulsion Laboratory in Pasadena, Calif. The Chandra image is the largest contiguous field ever obtained by the observatory. At 9.3 square degrees, it is over 40 times larger than the full moon seen on the night sky and over 80 times larger than either of the Chandra Deep Fields. This survey, taken in a region of the Bootes constellation, involved 126 separate pointings of 5,000-second Chandra exposures each. The researchers combined this with data obtained from Spitzer, and Kitt Peak's 4-meter Mayall and the MMT 6.5-meter optical telescopes, both located outside Tuscon, Ariz., from the same patch of sky. NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the agency's Science Mission Directorate. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center, Cambridge, Mass. Additional information and images are available at: http://chandra.harvard.edu and http://chandra.nasa.gov

Exploring Jets from a Supermassive Black Hole

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2018-06-01

What are the feeding and burping habits of the supermassive black holes peppering the universe? In a new study, observations of one such monster reveal more about the behavior of its powerful jets.Beams from BehemothsAcross the universe, supermassive black holes of millions to billions of solar masses lie at the centers of galaxies, gobbling up surrounding material. But not all of the gas and dust that spirals in toward a black hole is ultimately swallowed! A large fraction of it can instead be flung out into space again, in the form of enormous, powerful jets that extend for thousands or even millions of light-years in opposite directions.M87, shown in this Hubble image, is a classic example of a nearby (55 million light-years distant) supermassive black hole with a visible, collimated jet. Its counter-jet isnt seen because relativistic effects make the receding jet appear less bright. [The Hubble Heritage Team (STScI/AURA) and NASA/ESA]What causes these outflows to be tightly beamed collimated in the form of jets, rather than sprayed out in all directions? Does the pressure of the ambient medium the surrounding gas and dust that the jet is injected into play an important role? In what regions do these jets accelerate and decelerate? There are many open questions that scientists hope to understand by studying some of the active black holes with jets that live closest to us.Eyes on a Nearby GiantIn a new study led by Satomi Nakahara (The Graduate University for Advanced Studies in Japan), a team of scientists has used multifrequency Very Long Baseline Array (VLBA) and Very Long Array (VLA) images to explore jets emitted from a galaxy just 100 million light-years away: NGC 4261.This galaxys (relatively) close distance as well as the fact that were viewing it largely from the side, so we can clearly see both of its polar jets allows us to observe in detail the structure and intensity of its jets as a function of their distance from the black hole. Nakahara and collaborators observations span the enormous radial distance of a thousand to a billion times the radius of the black hole, or about 54 light-days to more than a million light-years.Scale for ChangeThe width of the jet as a function of radial distance from the black hole, for NGC 4261 (red) compared to the few other jets from nearby supermassive black holes that weve measured. NGC 4261s jets transition from parabolic to conical at around 10,000 times the radius of the black hole (RS). [Nakahara et al. 2018]The authors observations of NGC 4261s jets indicate that a transition occurs at 10,000 times the radius of the black hole (thats a little over a light-year from the black hole). At this point, the jets structures change from parabolic (becoming more tightly beamed) to conical (expanding freely). Around the same location, Nakahara and collaborators also see the radiation profile of one of the jets change, suggesting the physical conditions in the jets transition here as well.This is the first time weve been able to examine jet width this closely for both of the jets emitted from a supermassive black hole. The fact that the structure changes at the same distance for both jets indicates that the shape of these powerful streams is likely governed by global properties of the environment surrounding the galaxys nucleus, or properties of the jets themselves, rather than by a local condition.The authors next hope to pin down velocities inside NGC 4261s jets to determine where the jets accelerate and decelerate. This nearby powerhouse is clearly going to be a useful laboratory in the future, helping to unveil the secrets of more distant, feeding monsters.BonusCurious what these hungry supermassive black holes look like? Check out this artists imagining of NGC 4261, which shows how it feeds from a large, swirling accretion disk and emits fast-moving, collimated jets. [Original video credit to Dana Berry, Space Telescope Science Institute]CitationSatomi Nakahara et al 2018 ApJ 854 148. doi:10.3847/1538-4357/aaa45e

Locomotion in Extinct Giant Kangaroos: Were Sthenurines Hop-Less Monsters?

PubMed Central

Janis, Christine M.; Buttrill, Karalyn; Figueirido, Borja

2014-01-01

Sthenurine kangaroos (Marsupialia, Diprotodontia, Macropodoidea) were an extinct subfamily within the family Macropodidae (kangaroos and rat-kangaroos). These “short-faced browsers” first appeared in the middle Miocene, and radiated in the Plio-Pleistocene into a diversity of mostly large-bodied forms, more robust than extant forms in their build. The largest (Procoptodon goliah) had an estimated body mass of 240 kg, almost three times the size of the largest living kangaroos, and there is speculation whether a kangaroo of this size would be biomechanically capable of hopping locomotion. Previously described aspects of sthenurine anatomy (specialized forelimbs, rigid lumbar spine) would limit their ability to perform the characteristic kangaroo pentapedal walking (using the tail as a fifth limb), an essential gait at slower speeds as slow hopping is energetically unfeasible. Analysis of limb bone measurements of sthenurines in comparison with extant macropodoids shows a number of anatomical differences, especially in the large species. The scaling of long bone robusticity indicates that sthenurines are following the “normal” allometric trend for macropodoids, while the large extant kangaroos are relatively gracile. Other morphological differences are indicative of adaptations for a novel type of locomotor behavior in sthenurines: they lacked many specialized features for rapid hopping, and they also had anatomy indicative of supporting their body with an upright trunk (e.g., dorsally tipped ischiae), and of supporting their weight on one leg at a time (e.g., larger hips and knees, stabilized ankle joint). We propose that sthenurines adopted a bipedal striding gait (a gait occasionally observed in extant tree-kangaroos): in the smaller and earlier forms, this gait may have been employed as an alternative to pentapedal locomotion at slower speeds, while in the larger Pleistocene forms this gait may have enabled them to evolve to body sizes where hopping was no longer a feasible form of more rapid locomotion. PMID:25333823

Anyone Else Think This Looks Like the Cookie Monster?

NASA Image and Video Library

2017-12-08

NASA image acquired August 29, 2012 Ok, so maybe it's just me. But the superposition of younger craters on older craters (in this case two smaller craters upon the rim of an older crater) can result in landforms that appear to resemble more familiar shapes to human eyes. More generally, the Law of Superposition allows scientists to determine which surface features pre- and postdate others, leading to a better understanding of the geological history of different regions of Mercury's surface. This image was acquired as a high-resolution targeted observation. Targeted observations are images of a small area on Mercury's surface at resolutions much higher than the 200-meter/pixel morphology base map. It is not possible to cover all of Mercury's surface at this high resolution, but typically several areas of high scientific interest are imaged in this mode each week. The MESSENGER spacecraft is the first ever to orbit the planet Mercury, and the spacecraft's seven scientific instruments and radio science investigation are unraveling the history and evolution of the Solar System's innermost planet. Visit the Why Mercury? section of this website to learn more about the key science questions that the MESSENGER mission is addressing. During the one-year primary mission, MESSENGER acquired 88,746 images and extensive other data sets. MESSENGER is now in a yearlong extended mission, during which plans call for the acquisition of more than 80,000 additional images to support MESSENGER's science goals. Go here to read more about the MESSENGER mission: www.nasa.gov/mission_pages/messenger/main/index.html Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

A comparison of sports and energy drinks--Physiochemical properties and enamel dissolution.

PubMed

Jain, Poonam; Hall-May, Emily; Golabek, Kristi; Agustin, Ma Zenia

2012-01-01

The consumption of sports and energy drinks by children and adolescents has increased at an alarming rate in recent years. It is essential for dental professionals to be informed about the physiochemical properties of these drinks and their effects on enamel. The present study measured the fluoride levels, pH, and titratable acidity of multiple popular, commercially available brands of sports and energy drinks. Enamel dissolution was measured as weight loss using an in vitro multiple exposure model consisting of repeated short exposures to these drinks, alternating with exposure to artificial saliva. The relationship between enamel dissolution and fluoride levels, pH, and titratable acidity was also examined. There was a statistically significant difference between the fluoride levels (p = 0.034) and pH (p = 0.04) of the sports and energy drinks studied. The titratable acidity of energy drinks (11.78) was found to be significantly higher than that of sports drinks (3.58) (p < 0.001). Five of the energy drinks (Red Bull Sugar Free, Monster Assault, Von Dutch, Rockstar, and 5-Hour Energy) were found to have the highest titratable acidity values among the brands studied. Enamel weight loss after exposure to energy drinks was significantly higher than it was after exposure to sports drinks. The effect of titratable acidity on enamel weight loss was found to vary inversely with the pH of the drinks. The findings indicated that energy drinks have significantly higher titratable acidity and enamel dissolution associated with them than sports drinks. Enamel weight loss after exposure to energy drinks was more than two times higher than it was after exposure to sports drinks. Titratable acidity is a significant predictor of enamel dissolution, and its effect on enamel weight loss varies inversely with the pH of the drink. The data from the current study can be used to educate patients about the differences between sports and energy drinks and the effects of these drinks on tooth enamel.

The Starburst-AGN connection: quenching the fire and feeding the monster

NASA Astrophysics Data System (ADS)

Melnick, Jorge; Telles, Eduardo; De Propris, Roberto; Chu, Zhang-Hu

2015-10-01

The merger of two spiral galaxies is believed to be one of the main channels for the production of elliptical and early-type galaxies. In the process, the system becomes an (ultra) luminous infrared galaxy, or (U)LIRG, that morphs to a quasar, to a K+A galaxy, and finally to an early-type galaxy. The time scales for this metamorphosis are only loosely constrained by observations. In particular, the K+A phase should follow immediately after the quasi stellar object (QSO) phase during which the dust and gas remaining from the (U)LIRG phase are expelled by the active galactic nucleus (AGN). An intermediate class of QSOs with K+A spectral signatures, the post-starburst QSOs (PSQ), may represent the transitional phase between QSOs and K+As. We have compiled a sample of 72 bona fide z < 0.5 PSQ from the SDSS DR7 QSO catalogue. We find the intermediate age populations in this sample to be on average significantly weaker and metal poorer than their putative descendants, the K+A galaxies. The typical spectral energy distribution of PSQ is well fitted by three components: starlight; an obscured power-law; and a hot dust component required to reproduce the mid-IR fluxes. From the slope and bolometric luminosity of the power-law component we estimate typical masses and accretion rates of the AGN, but we find little evidence of powerful radio-loud or strong X-ray emitters in our sample. This may indicate that the power-law component originates in a nuclear starburst rather than in an AGN, as expected if the bulk of their young stars are still being formed, or that the AGN is still heavily enshrouded in dust and gas. We find that both alternatives are problematic and that more and better optical, X-ray, and mm-wave observations are needed to elucidate the evolutionary history of PSQ.

Hurricane Patricia

NASA Image and Video Library

2017-12-08

Composite image of category 5 Hurricane Patricia, off the Pacific coast of Mexico, from 06:00 UTC on Friday, 23 October 2015. At 8 a.m. EDT on October 23, 2015, the National Hurricane Center said that Hurricane Patricia had grown into a monster hurricane. In fact, it is the strongest eastern north pacific hurricane on record. At 8 a.m. EDT (1200 UTC) on Oct. 23, the eye of Hurricane Patricia was located near latitude 17.3 North, longitude 105.6 West. That's about 145 miles (235 km) southwest of Manzanillo, Mexico and about 215 miles (345 km) south of Cabo Corrientes, Mexico. Patricia was moving toward the north-northwest near 12 mph (19 kph) and a turn toward the north is expected later this morning, followed by a turn toward the north-northeast this afternoon. On the forecast track, the core of Patricia will make landfall in the hurricane warning area today, October 23, 2015 during the afternoon or evening. Maximum sustained winds remain near 200 mph (325 kph) with higher gusts. The National Hurricane Center (NHC) said that Patricia is a category 5 hurricane on the Saffir-Simpson Hurricane Wind Scale. Some fluctuations in intensity are possible today, but Patricia is expected to remain an extremely dangerous category 5 hurricane through landfall. Hurricane force winds extend outward up to 30 miles (45 km) from the center and tropical storm force winds extend outward up to 175 miles (280 km). The estimated minimum central pressure is 880 millibars. Copyright: 2015 EUMETSAT. Infrared data from the geostationary satellites of EUMETSAT and NOAA overlays a computer-generated model of the Earth, containing NASA's Blue Marble Next Generation imagery NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Hubble Sees Elegant Spiral Hiding a Hungry Monster

NASA Image and Video Library

2017-12-08

NGC 4639 is a beautiful example of a type of galaxy known as a barred spiral. It lies over 70 million light-years away in the constellation of Virgo and is one of about 1,500 galaxies that make up the Virgo Cluster. In this image, taken by the NASA/ESA Hubble Space Telescope, one can clearly see the bar running through the bright, round core of the galaxy. Bars are found in around two-thirds of spiral galaxies, and are thought to be a natural phase in their evolution. The galaxy’s spiral arms are sprinkled with bright regions of active star formation. Each of these tiny jewels is actually several hundred light-years across and contains hundreds or thousands of newly formed stars. But NGC 4639 also conceals a dark secret in its core — a massive black hole that is consuming the surrounding gas. This is known as an active galactic nucleus (AGN), and is revealed by characteristic features in the spectrum of light from the galaxy and by X-rays produced close to the black hole as the hot gas plunges towards it. Most galaxies are thought to contain a black hole at the center. NGC 4639 is in fact a very weak example of an AGN, demonstrating that AGNs exist over a large range of activity, from galaxies like NGC 4639 to distant quasars, where the parent galaxy is almost completely dominated by the emissions from the AGN. Image credit: ESA/Hubble & NASA NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Hurricane Patricia

NASA Image and Video Library

2017-12-08

This full-disk image from NOAA’s GOES-13 satellite was captured at 14:45 UTC (10:45 a.m. EDT) and shows Hurricane Patricia off the coast of Mexico on September 23, 2015. At 8 a.m. EDT on October 23, 2015, the National Hurricane Center said that Hurricane Patricia had grown into a monster hurricane. In fact, it is the strongest eastern north pacific hurricane on record. At 8 a.m. EDT (1200 UTC) on Oct. 23, the eye of Hurricane Patricia was located near latitude 17.3 North, longitude 105.6 West. That's about 145 miles (235 km) southwest of Manzanillo, Mexico and about 215 miles (345 km) south of Cabo Corrientes, Mexico. Patricia was moving toward the north-northwest near 12 mph (19 kph) and a turn toward the north is expected later this morning, followed by a turn toward the north-northeast this afternoon. On the forecast track, the core of Patricia will make landfall in the hurricane warning area today, October 23, 2015 during the afternoon or evening. Maximum sustained winds remain near 200 mph (325 kph) with higher gusts. The National Hurricane Center (NHC) said that Patricia is a category 5 hurricane on the Saffir-Simpson Hurricane Wind Scale. Some fluctuations in intensity are possible today, but Patricia is expected to remain an extremely dangerous category 5 hurricane through landfall. Hurricane force winds extend outward up to 30 miles (45 km) from the center and tropical storm force winds extend outward up to 175 miles (280 km). The estimated minimum central pressure is 880 millibars. NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

The Making of a Monster: Postnatal Ontogenetic Changes in Craniomandibular Shape in the Great Sabercat Smilodon

PubMed Central

Christiansen, Per

2012-01-01

Derived sabercats had craniomandibular morphologies that in many respects were highly different from those of extant felids, and this has often been interpreted functionally as adaptations for predation at extreme gape angles with hypertrophied upper canines. It is unknown how much of this was a result of intraspecific postnatal ontogeny, since juveniles of sabercats are rare and no quantitative study has been made of craniomandibular ontogeny. Postnatal ontogenetic craniomandibular shape changes in two morphologically derived sabercats, Smilodon fatalis and S. populator, were analysed using geometric morphometrics and compared to three species of extant pantherines, the jaguar, tiger, and Sunda clouded leopard. Ontogenetic shape changes in Smilodon usually involved the same areas of the cranium and mandible as in extant pantherines, and large-scale modularization was similar, suggesting that such may have been the case for all felids, since it followed the same trends previously observed in other mammals. However, in other respects Smilodon differed from extant pantherines. Their crania underwent much greater and more localised ontogenetic shape changes than did the mandibles, whereas crania and mandibles of extant pantherines underwent smaller, fewer and less localised shape changes. Ontogenetic shape changes in the two species of Smilodon are largely similar, but differences are also present, notably those which may be tied to the presence of larger upper canines in S. populator. Several of the specialized cranial characters differentiating adult Smilodon from extant felids in a functional context, which are usually regarded as evolutionary adaptations for achieving high gape angles, are ontogenetic, and in several instances ontogeny appears to recapitulate phylogeny to some extent. No such ontogenetic evolutionary adaptive changes were found in the extant pantherines. Evolution in morphologically derived sabercats involved greater cranial ontogenetic changes than among extant felids, resulting in greatly modified adult craniomandibular morphologies. PMID:22235326

Plant chimeras: The good, the bad, and the 'Bizzaria'.

PubMed

Frank, Margaret H; Chitwood, Daniel H

2016-11-01

Chimeras - organisms that are composed of cells of more than one genotype - captured the human imagination long before they were formally described and used in the laboratory. These organisms owe their namesake to a fire-breathing monster from Greek mythology that has the head of a lion, the body of a goat, and the tail of a serpent. The first description of a non-fictional chimera dates back to the middle of the seventeenth century when the Florentine gardener Pietro Nati discovered an adventitious shoot growing from the graft junction between sour orange (Citrus aurantium) and citron (Citrus medica). This perplexing chimera that grows with sectors phenotypically resembling each of the citrus progenitors inspired discussion and wonder from the scientific community and was fittingly named the 'Bizzaria'. Initially, the 'Bizzaria' was believed to be an asexual hybrid that formed from a cellular fusion between the grafted parents; however, in-depth cellular analyses carried out centuries later demonstrated that the 'Bizzaria', along with other chimeras, owe their unique sectored appearance to a conglomeration of cells from the two donors. Since this pivotal discovery at the turn of the twentieth century, chimeras have served both as tools and as unique biological phenomena that have contributed to our understanding of plant development at the cellular, tissue, and organismal level. Rapid advancements in genome sequencing technologies have enabled the establishment of new model species with novel morphological and developmental features that enable the generation of chimeric organisms. In this review, we show that genetic mosaic and chimera studies provide a technologically simple way to delve into the organismal, genetic, and genomic inner workings underlying the development of diverse model organisms. Moreover, we discuss the unique opportunity that chimeras present to explore universal principles governing intercellular communication and the coordination of organismal biology in a heterogenomic landscape. Copyright © 2016 Elsevier Inc. All rights reserved.

The Sleeping Monster: NuSTAR Observations of SGR 1806-20, 11 Years After the Giant Flare

NASA Astrophysics Data System (ADS)

Younes, George; Baring, Matthew G.; Kouveliotou, Chryssa; Harding, Alice; Donovan, Sophia; Göğüş, Ersin; Kaspi, Victoria; Granot, Jonathan

2017-12-01

We report the analysis of five Nuclear Spectroscopic Telescope Array (NuSTAR) observations of SGR 1806-20 spread over a year from 2015 April to 2016 April, more than 11 years following its giant flare (GF) of 2004. The source spin frequency during the NuSTAR observations follows a linear trend with a frequency derivative \\dot{ν }=(-1.25+/- 0.03)× {10}-12 Hz s-1, implying a surface dipole equatorial magnetic field B≈ 7.7× {10}14 G. Thus, SGR 1806-20 has finally returned to its historical minimum torque level measured between 1993 and 1998. The source showed strong timing noise for at least 12 years starting in 2000, with \\dot{ν } increasing one order of magnitude between 2005 and 2011, following its 2004 major bursting episode and GF. SGR 1806-20 has not shown strong transient activity since 2009, and we do not find short bursts in the NuSTAR data. The pulse profile is complex with a pulsed fraction of ˜ 8 % with no indication of energy dependence. The NuSTAR spectra are well fit with an absorbed blackbody, {kT}=0.62+/- 0.06 {keV}, plus a power law, {{Γ }}=1.33+/- 0.03. We find no evidence for variability among the five observations, indicating that SGR 1806-20 has reached a persistent and potentially its quiescent X-ray flux level after its 2004 major bursting episode. Extrapolating the NuSTAR model to lower energies, we find that the 0.5-10 keV flux decay follows an exponential form with a characteristic timescale τ =543+/- 75 days. Interestingly, the NuSTAR flux in this energy range is a factor of ˜2 weaker than the long-term average measured between 1993 and 2003, a behavior also exhibited in SGR 1900+14. We discuss our findings in the context of the magnetar model.

Fishing in the Shadow of Angkor Wat:The effect of dams, climate change and fishing pressure on the Tonle Sap floodpulse ecosystem, Cambodia

NASA Astrophysics Data System (ADS)

Hannah, L.; Teh, L.; KC, K. B.; Elliott, V.; Fraser, E. D. G.; Phen, C.

2016-12-01

The Tonle Sap floodpulse lake is the epicenter of immense human, physical and biological change. The giant Mekong catfish, giant barb and other 'river monsters' once typical of the Tonle Sap are now vanishingly rare. The fishing villages and ecosystem of the Tonle Sap exemplify changes experienced in floodpulse systems and smallholder fisheries around the world. Much existing fishery theory focuses on well-capitalized, single-species temperate marine fisheries, such as salmon fisheries. In contrast, tropical fisheries are low-capital, multi-species and often freshwater. The Tonle Sap is the largest of these tropical freshwater fisheries. Fishing pressure includes gear of all types and sizes, resulting in take of a wide range of species and virtually all size classes. New fisheries theory is needed to describe these fisheries and their possible responses to change. Threats to the Tonle Sap include a failing monsoon, upstream dams, high fishing pressure and climate change. We have developed a theory of 'indiscriminate fisheries' to describe the fishing in the Tonle Sap and its consequences, and have collected three years of field data on the fishery and ecosystem to understand how indiscriminate fisheries may respond to global and local change. Our findings suggest that large individiual fish biomass is being traded for large collective biomass in the fishery, resulting in high-volume, low value catch. The economic and social consequences of these changes are declining per capita catch and value, accompanied by a shift from private to community management. The resulting system is likely to experience more fluctuation in catch value and to be more vulnerable to environmental perturbations caused by dams and climate change. These finding raise serious questions about the future of tropical floodpulse fisheries and the smallholder fishing families that depend upon them.

Panoramic Views of the Landing site from Sagan Memorial Station

NASA Technical Reports Server (NTRS)

1997-01-01

Each of these panoramic views is a controlled mosaic of approximately 300 IMP images covering 360 degrees of azimuth and elevations from approximately 4 degrees above the horizon to 45 degrees below it. Simultaneous adjustment of orientations of all images has been performed to minimize discontinuities between images. Mosaics have been highpass-filtered and contrast-enhanced to improve discrimination of details without distorting relative colors overall.

TOP IMAGE: Enhanced true-color image created from the 'Gallery Pan' sequence, acquired on sols 8-10 so that local solar time increases nearly continuously from about 10:00 at the right edge to about 12:00 at the left. Mosaics of images obtained by the right camera through 670 nm, 530 nm, and 440 nm filters were used as red, green and blue channels. Grid ticks indicate azimuth clockwise from north in 30 degree increments and elevation in 15 degree increments.

BOTTOM IMAGE: Anaglyphic stereoimage created from the 'monster pan' sequence, acquired in four sections between about 8:30 and 15:00 local solar time on sol 3. Mosaics of images obtained through the 670 nm filter (left camera) and 530 and 440 nm filters (right camera) were used where available. At the top and bottom, left- and right-camera 670 nm images were used. Part of the northern horizon was not imaged because of the tilt of the lander. This image may be viewed stereoscopically through glasses with a red filter for the left eye and a cyan filter for the right eye.

NOTE: original caption as published in Science Magazine

Mars Pathfinder is the second in NASA's Discovery program of low-cost spacecraft with highly focused science goals. The Jet Propulsion Laboratory, Pasadena, CA, developed and manages the Mars Pathfinder mission for NASA's Office of Space Science, Washington, D.C. JPL is a division of the California Institute of Technology (Caltech).

Gemini IFU, VLA, and HST observations of the OH megamaser galaxy IRAS F23199+0123: the hidden monster and its outflow

NASA Astrophysics Data System (ADS)

Hekatelyne, C.; Riffel, Rogemar A.; Sales, Dinalva; Robinson, Andrew; Gallimore, Jack; Storchi-Bergmann, Thaisa; Kharb, Preeti; O'Dea, Christopher; Baum, Stefi

2018-03-01

We present Gemini Multi-Object Spectrograph (GMOS) Integral field Unit (IFU), Very Large Array (VLA), and Hubble Space Telescope (HST) observations of the OH megamaser (OHM) galaxy IRAS F23199+0123. Our observations show that this system is an interacting pair, with two OHM sources associated with the eastern (IRAS 23199E) member. The two members of the pair present somewhat extended radio emission at 3 and 20 cm, with flux peaks at each nucleus. The GMOS-IFU observations cover the inner ˜6 kpc of IRAS 23199E at a spatial resolution of 2.3 kpc. The GMOS-IFU flux distributions in Hα and [N II] λ6583 are similar to that of an HST [N II]+Hα narrow-band image, being more extended along the north-east-south-west direction, as also observed in the continuum HST F814W image. The GMOS-IFU Hα flux map of IRAS 23199E shows three extranuclear knots attributed to star-forming complexes. We have discovered a Seyfert 1 nucleus in this galaxy, as its nuclear spectrum shows an unresolved broad (full width at half-maximum ≈2170 km s-1) double-peaked Hα component, from which we derive a black hole mass of M_{BH} = 3.8^{+0.3}_{-0.2}× 106 M⊙. The gas kinematics shows low velocity dispersions (σ) and low [N II]/Hα ratios for the star-forming complexes and higher σ and [N II]/Hα surrounding the radio emission region, supporting interaction between the radio plasma and ambient gas. The two OH masers detected in IRAS F23199E are observed in the vicinity of these enhanced σ regions, supporting their association with the active nucleus and its interaction with the surrounding gas. The gas velocity field can be partially reproduced by rotation in a disc, with residuals along the north-south direction being tentatively attributed to emission from the front walls of a bipolar outflow.

Is a 'one size fits all' taphonomic model appropriate for the Mazon Creek Lagerstätte?

NASA Astrophysics Data System (ADS)

Clements, Thomas; Purnell, Mark; Gabbott, Sarah

2017-04-01

The Late Carboniferous Mazon Creek Lagerstätte (Illinois, USA) is a world renowned fossil deposit with a huge diversity of preserved flora and fauna. It is widely considered to represent the most complete Late Carboniferous river delta ecosystem because researchers have identified that the deposit preserves organisms from multiple habitats including coastal swamps, brackish lagoons and oceanic environments. Often these fossils have exquisite soft tissue preservation yielding far more information that the 'normal' skeletal fossil record, while some soft bodied animals, such as the notorious Tully Monster (Tullimonstrum gregarium), are only known from this locality. However, constraining a 'one-size fits all' taphonomic model for the Mazon Creek is difficult because of our poor understanding of sideritic concretionary formation or preservation (i.e. the presence of large numbers of unfossiliferous concretions), the large geographical area, the influences of fresh, brackish and saline waters during burial and the subsequent complicated diagenetic processes. To determine the preservational pathways of Mazon Creek fossils, we have compiled data of the mode of preservation of morphological characters for all major groups of fossil organisms found in this Lagerstätte. This data can be used to test for variance in mode of preservation between taxa and also between specific tissue types. Furthermore, experimental decay data is used to constrain the impact of decay prior to fossilisation. Our analysis indicates that there are variations in preservation potential of specific characters shared by taxa. Modes of preservation, however, seem to be consistent across the majority of taxa dependant on locality. This quantitative approach is being utilised as part of a larger ongoing investigation which combines taphonomy with geochemical analysis of siderite concretions from across the vast geographical area of the Mazon Creek. Together this approach will allow us to elucidate the preservation pathways of organisms and will lead to better understanding of taphonomic biases operating in this Lagerstätte.

Communicating Science

NASA Astrophysics Data System (ADS)

Russell, Nicholas

2009-10-01

Introduction: what this book is about and why you might want to read it; Prologue: three orphans share a common paternity: professional science communication, popular journalism, and literary fiction are not as separate as they seem; Part I. Professional Science Communication: 1. Spreading the word: the endless struggle to publish professional science; 2. Walk like an Egyptian: the alien feeling of professional science writing; 3. The future's bright? Professional science communication in the age of the internet; 4. Counting the horse's teeth: professional standards in science's barter economy; 5. Separating the wheat from the chaff: peer review on trial; Part II. Science for the Public: What Science Do People Need and How Might They Get It?: 6. The Public Understanding of Science (PUS) movement and its problems; 7. Public engagement with science and technology (PEST): fine principle, difficult practice; 8. Citizen scientists? Democratic input into science policy; 9. Teaching and learning science in schools: implications for popular science communication; Part III. Popular Science Communication: The Press and Broadcasting: 10. What every scientist should know about mass media; 11. What every scientist should know about journalists; 12. The influence of new media; 13. How the media represents science; 14. How should science journalists behave?; Part IV. The Origins of Science in Cultural Context: Five Historic Dramas: 15. A terrible storm in Wittenberg: natural knowledge through sorcery and evil; 16. A terrible storm in the Mediterranean: controlling nature with white magic and religion; 17. Thieving magpies: the subtle art of false projecting; 18. Foolish virtuosi: natural philosophy emerges as a distinct discipline but many cannot take it seriously; 19. Is scientific knowledge 'true' or should it just be 'truthfully' deployed?; Part V. Science in Literature: 20. Science and the Gothic: the three big nineteenth-century monster stories; 21. Science fiction: serious literature of ideas or low-grade entertainment?; 22. Science in British literary fiction; 23. Science on stage: the politics and ethics of science in cultural and educational contexts.

Evolution of unusual morphologies in Lentibulariaceae (bladderworts and allies) and Podostemaceae (river-weeds): a pictorial report at the interface of developmental biology and morphological diversification.

PubMed

Rutishauser, Rolf

2016-04-01

Various groups of flowering plants reveal profound ('saltational') changes of their bauplans (architectural rules) as compared with related taxa. These plants are known as morphological misfits that appear as rather large morphological deviations from the norm. Some of them emerged as morphological key innovations (perhaps 'hopeful monsters') that gave rise to new evolutionary lines of organisms, based on (major) genetic changes. This pictorial report places emphasis on released bauplans as typical for bladderworts (Utricularia, approx. 230 secies, Lentibulariaceae) and river-weeds (Podostemaceae, three subfamilies, approx. 54 genera, approx. 310 species). Bladderworts (Utricularia) are carnivorous, possessing sucking traps. They live as submerged aquatics (except for their flowers), as humid terrestrials or as epiphytes. Most Podostemaceae are restricted to rocks in tropical river-rapids and waterfalls. They survive as submerged haptophytes in these extreme habitats during the rainy season, emerging with their flowers afterwards. The recent scientific progress in developmental biology and evolutionary history of both Lentibulariaceae and Podostemaceae is summarized. Lentibulariaceae and Podostemaceae follow structural rules that are different from but related to those of more typical flowering plants. The roots, stems and leaves - as still distinguishable in related flowering plants - are blurred ('fuzzy'). However, both families have stable floral bauplans. The developmental switches to unusual vegetative morphologies facilitated rather than prevented the evolution of species diversity in both families. The lack of one-to-one correspondence between structural categories and gene expression may have arisen from the re-use of existing genetic resources in novel contexts. Understanding what developmental patterns are followed in Lentibulariaceae and Podostemaceae is a necessary prerequisite to discover the genetic alterations that led to the evolution of these atypical plants. Future molecular genetic work on morphological misfits such as bladderworts and river-weeds will provide insight into developmental and evolutionary aspects of more typical vascular plants. © The Author 2015. Published by Oxford University Press on behalf of the Annals of Botany Company.

Time Restored - The Harrison Timekeepers and R.T. Gould, the Man Who Knew (Almost) Everything

NASA Astrophysics Data System (ADS)

Betts, Jonathan

2006-09-01

This is the story of Rupert T. Gould (1890-1948), the polymath and horologist. A remarkable man, Lt Cmdr Gould made important contributions in an extraordinary range of subject areas throughout his relatively short and dramatically troubled life. From antique clocks to scientific mysteries, from typewriters to the first systematic study of the Loch Ness Monster, Gould studied and published on them all. With the title The Stargazer, Gould was an early broadcaster on the BBC's Children's Hour when, with his encyclopaedic knowledge, he became known as The Man Who Knew Everything. Not surprisingly, he was also part of that elite group on BBC radio who formed The Brains Trust, giving on-the-spot answers to all manner of wide ranging and difficult questions. With his wide learning and photographic memory, Gould awed a national audience, becoming one of the era's radio celebrities. During the 1920s Gould restored the complex and highly significant marine timekeepers constructed by John Harrison (1693-1776), and wrote the unsurpassed classic, The Marine Chronometer, its History and Development . Today he is virtually unknown, his horological contributions scarcely mentioned in Dava Sobel's bestseller Longitude. The TV version of Longitude, in which Jeremy Irons played Rupert Gould, did at least introduce Gould's name to a wider public. Gould suffered terrible bouts of depression, resulting in a number of nervous breakdowns. These, coupled with his obsessive and pedantic nature, led to a scandalously-reported separation from his wife and cost him his family, his home, his job, and his closest friends. In this first-ever biography of Rupert Gould, Jonathan Betts, the Royal Observatory Greenwich's Senior Horologist, has given us a compelling account of a talented but flawed individual. Using hitherto unknown personal journals, the family's extensive collection of photographs, and the polymath's surviving records and notes, Betts tells the story of how Gould's early life, his naval career, and his celebrity status came together as this talented Englishman restored part of Britain's--and the world's--most important technical heritage: John Harrison's marine timekeepers.

Viperous fangs: development and evolution of the venom canal.

PubMed

Zahradnicek, Oldrich; Horacek, Ivan; Tucker, Abigail S

2008-01-01

Fangs are specialised long teeth that contain either a superficial groove (Gila monster, Beaded lizard, some colubrid snakes), along which the venom runs, or an enclosed canal (viperid, elapid and atractaspid), down which the venom flows inside the tooth. The fangs of viperid snakes are the most effective venom-delivery structures among vertebrates and have been the focus of scientific interests for more than 200 years. Despite this interest the questions of how the canal at the centre of the fang forms remains unresolved. Two different hypotheses have been suggested. The mainstream hypothesis claims that the venom-conducting canal develops by the invagination of the epithelial wall of the developing tooth germ. The sides of this invagination make contact and finally fuse to form the enclosed canal. The second hypothesis, known as the "brick chimney", claims the venom-conducting canal develops directly by successive dentine deposition as the tooth develops. The fang is thus built up from the tip to the base, without any folding of the tooth surface. In an attempt to cast further light on this subject the early development of the fangs was followed in a pit viper, Trimeresurus albolabris, using the expression of Sonic hedgehog (Shh). We demonstrate that the canal is indeed formed by an early folding event, resulting from an invagination of epithelial cells into the dental mesenchyme. The epithelial cells proliferate to enlarge the canal and then the cells die by apoptosis, forming an empty tube through which the poison runs. The entrance and discharge orifices at either end of the canal develop by a similar invagination but the initial width of the invagination is very different from that in the middle of the tooth, and is associated with higher proliferation. The two sides of the invaginating epithelium never come into contact, leaving the orifice open. The mechanism by which the orifices form can be likened to that observed in reptiles with an open groove along their fangs, such as the boomslang. It is thus tempting to speculate that the process of orifice formation in viperids represents the ancestral pleisomorphic state, and that enclosed canals developed by a change in the shape and size of the initial invagination.

Monsters on the move: A search for supermassive black holes undergoing gravitational wave recoil

NASA Astrophysics Data System (ADS)

Jadhav, Yashashree; Robinson, Andrew; Lena, Davide

2018-01-01

There is compelling evidence that supermassive black holes (SMBH) reside at the centers of all large galaxies and are the gravitational ‘engines’ of Active Galactic Nuclei (AGN). Furthermore, galaxy mergers are thought to have played a fundamental role in the growth and evolution of the largest galaxies in the nearby universe. A galaxy merger is expected to lead to the formation of an SMBH binary, which itself eventually coalesces through the emission of gravitational waves. Such events fall outside the frequency range accessible to the LIGO/VIRGO gravitational wave detectors, but they can be detected via electromagnetic signatures. Numerical relativity simulations show that, depending on the initial spin-orbit configuration of the binary, the merged SMBH receives a gravitational recoil kick that may reach several 1000km/s. This recoil in turn causes the merged SMBH to oscillate for up to ~1 Gyr in the gravitational potential well of the galaxy. During this time, the recoiling SMBH may be observed as a ‘displaced’ AGN. Such events provide a strong test of gravitational physics and the formation and merger frequencies of binary SMBH. As a result of residual oscillations, displacements ~10 – 100pc may be expected even in nearby elliptical galaxies and can be measured as spatial offsets in high resolution optical or infrared images. We present the results of a preliminary study, in which isophotal analysis was conducted for a sample of 96 galaxies to obtain the photocenter of the galaxies using Hubble Space Telescope (HST) archival optical or infrared WFC2/PC, ACS or NICMOS images. The position of the nuclear point source (AGN) was also measured to obtain a displacement vector. This initial sample reveals 18 candidates that show a significant displacement. Of these, 14 are hosted by core ellipticals, while the rest have a cuspy light profile. As galactic and nuclear dust structures may interfere with the isophotal analysis, we are currently obtaining new WFC3 NIR images for selected candidates, in order to confirm the measured displacements. Preliminary results from these new images will also be presented.

Anatomical Network Comparison of Human Upper and Lower, Newborn and Adult, and Normal and Abnormal Limbs, with Notes on Development, Pathology and Limb Serial Homology vs. Homoplasy

PubMed Central

Diogo, Rui; Esteve-Altava, Borja; Smith, Christopher; Boughner, Julia C.; Rasskin-Gutman, Diego

2015-01-01

How do the various anatomical parts (modules) of the animal body evolve into very different integrated forms (integration) yet still function properly without decreasing the individual’s survival? This long-standing question remains unanswered for multiple reasons, including lack of consensus about conceptual definitions and approaches, as well as a reasonable bias toward the study of hard tissues over soft tissues. A major difficulty concerns the non-trivial technical hurdles of addressing this problem, specifically the lack of quantitative tools to quantify and compare variation across multiple disparate anatomical parts and tissue types. In this paper we apply for the first time a powerful new quantitative tool, Anatomical Network Analysis (AnNA), to examine and compare in detail the musculoskeletal modularity and integration of normal and abnormal human upper and lower limbs. In contrast to other morphological methods, the strength of AnNA is that it allows efficient and direct empirical comparisons among body parts with even vastly different architectures (e.g. upper and lower limbs) and diverse or complex tissue composition (e.g. bones, cartilages and muscles), by quantifying the spatial organization of these parts—their topological patterns relative to each other—using tools borrowed from network theory. Our results reveal similarities between the skeletal networks of the normal newborn/adult upper limb vs. lower limb, with exception to the shoulder vs. pelvis. However, when muscles are included, the overall musculoskeletal network organization of the upper limb is strikingly different from that of the lower limb, particularly that of the more proximal structures of each limb. Importantly, the obtained data provide further evidence to be added to the vast amount of paleontological, gross anatomical, developmental, molecular and embryological data recently obtained that contradicts the long-standing dogma that the upper and lower limbs are serial homologues. In addition, the AnNA of the limbs of a trisomy 18 human fetus strongly supports Pere Alberch's ill-named "logic of monsters" hypothesis, and contradicts the commonly accepted idea that birth defects often lead to lower integration (i.e. more parcellation) of anatomical structures. PMID:26452269

Archetypal Dreams: the Quantum Theater of Robert Wilson

NASA Astrophysics Data System (ADS)

Dietrich, Dawn Yvette

1992-01-01

My topic is situated within the larger framework of interdisciplinary study currently exploring the impact of new physics on various "soft" disciplines and sciences. Aligning myself with thinkers like Fritjof Capra and N. Katherine Hayles, who argue that quantum mechanics has brought about a new paradigm for the conceptualization of the physical world and our relation to it, I demonstrate that there is a connection, a kind of cultural translation, which relates contemporary physics to some avant-garde theater. Specifically, I center my research on American theater designer, Robert Wilson, who, recognized for his manipulation of the formal elements of stagecraft, owes much to the reconstruction of principles governing space and time. Taken further, I maintain that it is through the paradigm established from relativity theory and quantum mechanics that Wilson experiments with the elementary "forces" of the theater itself. This "restructuring" occurs through the dramatist's conceptions of space and time and the relation of those properties to both performers and spectators. Unlike most conventional theater, but as in many contemporary visual arts, time is manipulated through spatial metaphors and events take place in an amplified space--effecting a kind of dramatic space/time. Through manipulation of scale, the exploration of discontinuous time, and segregated stage zones, Wilson demonstrates that theater time is fluid and that it is not necessary for dramatic action to take place within the unified stage space delineated by the proscenium itself. Unlike conventional theater, where the stage is constructed with one perspective in mind, Wilson's theatrical mise-en-scene--a kind of new "perceptual field"--requires "imaginative watching"; that is, more perceptual discrimination from the audience who must sort and organize the visual material, highlighting the essential while reconfiguring the incidental. And this is where the myth is born, where archetypal dreams stir the psyche through the symbolic forms of the stage. Robert Wilson confronts audiences with moonlit forests, rising pyramids, angels, monsters and shooting stars--mythic apparitions which connect to our deepest sense of time, while lodging this "quantum" theater within the postmodernist paradigm which has transformed the way in which we perceive ourselves in relation to the world.

Fault-Related Sanctuaries

NASA Astrophysics Data System (ADS)

Piccardi, L.

2001-12-01

Beyond the study of historical surface faulting events, this work investigates the possibility, in specific cases, of identifying pre-historical events whose memory survives in myths and legends. The myths of many famous sacred places of the ancient world contain relevant telluric references: "sacred" earthquakes, openings to the Underworld and/or chthonic dragons. Given the strong correspondence with local geological evidence, these myths may be considered as describing natural phenomena. It has been possible in this way to shed light on the geologic origin of famous myths (Piccardi, 1999, 2000 and 2001). Interdisciplinary researches reveal that the origin of several ancient sanctuaries may be linked in particular to peculiar geological phenomena observed on local active faults (like ground shaking and coseismic surface ruptures, gas and flames emissions, strong underground rumours). In many of these sanctuaries the sacred area is laid directly above the active fault. In a few cases, faulting has affected also the archaeological relics, right through the main temple (e.g. Delphi, Cnidus, Hierapolis of Phrygia). As such, the arrangement of the cult site and content of relative myths suggest that specific points along the trace of active faults have been noticed in the past and worshiped as special `sacred' places, most likely interpreted as Hades' Doors. The mythological stratification of most of these sanctuaries dates back to prehistory, and points to a common derivation from the cult of the Mother Goddess (the Lady of the Doors), which was largely widespread since at least 25000 BC. The cult itself was later reconverted into various different divinities, while the `sacred doors' of the Great Goddess and/or the dragons (offspring of Mother Earth and generally regarded as Keepers of the Doors) persisted in more recent mythologies. Piccardi L., 1999: The "Footprints" of the Archangel: Evidence of Early-Medieval Surface Faulting at Monte Sant'Angelo (Gargano, Italy). European Union of Geophysics Congress, Strasbourg, March 1999. Piccardi L., 2000: Active faulting at Delphi (Greece): seismotectonic remarks and a hypothesis for the geological environment of a myth. Geology, 28, 651-654. Piccardi L., 2001: Seismotectonic Origin of the Monster of Loch Ness. Earth System Processes, Joint Meeting of G.S.A. and G.S.L., Edinburgh, June 2001.

T. rex and Godzilla: Finding Science in Science Fiction

NASA Astrophysics Data System (ADS)

Engelmann, G. F.; Chure, D. J.

2017-12-01

Works of fiction act as a powerful vehicle for inculcating an intuitive understanding (or misunderstanding) of scientific concepts in the audience. They can communicate information about scientific phenomena or how science is done. These entertainments can contribute to scientific literacy of the public and provide valuable outreach opportunities, but scientific accuracy is rarely even a minor consideration in developing fictional stories. Science educators can still make use of popular fiction to promote science education and outreach. Varied approaches have focused on the physical science in classic space operas, but historical sciences can make use of public interest in fictional tales involving prehistoric creatures and settings. Dinosaurs like T. rex inspire awe and widespread popular appeal that can nurture an interest in fossils but also serves as a gateway to all the other sciences on which paleontology depends, and to the scientific endeavor itself. But the portrayal of dinosaurs has met with negative criticism of details that is not likely to be productive of further discussion and learning. Perhaps it is not so important that authors and film makers didn't get it right; that "correctness" of terms and reconstructions is less important than the opportunity to improve public understanding of how science works; to cultivate a habit of critical thinking and an analytical approach to interpreting the world. Dinosaurs and other long extinct creatures can provide examples of how we know what we know; what kind of evidence is available and how it can be interpreted; how creative framing of hypotheses allows imaginative conjectures to be constrained by observations. They can open informative discussions of how scientists work in gathering data and developing and testing hypotheses. For example, how do paleontologists find fossils? Monsters, unrealistic fantasy creatures like Godzilla, have great charismatic appeal, and can prompt discussions of the obstacles posed by physical laws to the actual existence of such phenomena, such as the effects of such large scale on mass and inertia. Alternatively, one could undertake a scientifically constrained flight of fancy that considers what properties would be needed to make such fantastic beasts possible. Imagination and creativity can bring real science to fiction.

Anatomical Network Comparison of Human Upper and Lower, Newborn and Adult, and Normal and Abnormal Limbs, with Notes on Development, Pathology and Limb Serial Homology vs. Homoplasy.

PubMed

Diogo, Rui; Esteve-Altava, Borja; Smith, Christopher; Boughner, Julia C; Rasskin-Gutman, Diego

2015-01-01

How do the various anatomical parts (modules) of the animal body evolve into very different integrated forms (integration) yet still function properly without decreasing the individual's survival? This long-standing question remains unanswered for multiple reasons, including lack of consensus about conceptual definitions and approaches, as well as a reasonable bias toward the study of hard tissues over soft tissues. A major difficulty concerns the non-trivial technical hurdles of addressing this problem, specifically the lack of quantitative tools to quantify and compare variation across multiple disparate anatomical parts and tissue types. In this paper we apply for the first time a powerful new quantitative tool, Anatomical Network Analysis (AnNA), to examine and compare in detail the musculoskeletal modularity and integration of normal and abnormal human upper and lower limbs. In contrast to other morphological methods, the strength of AnNA is that it allows efficient and direct empirical comparisons among body parts with even vastly different architectures (e.g. upper and lower limbs) and diverse or complex tissue composition (e.g. bones, cartilages and muscles), by quantifying the spatial organization of these parts-their topological patterns relative to each other-using tools borrowed from network theory. Our results reveal similarities between the skeletal networks of the normal newborn/adult upper limb vs. lower limb, with exception to the shoulder vs. pelvis. However, when muscles are included, the overall musculoskeletal network organization of the upper limb is strikingly different from that of the lower limb, particularly that of the more proximal structures of each limb. Importantly, the obtained data provide further evidence to be added to the vast amount of paleontological, gross anatomical, developmental, molecular and embryological data recently obtained that contradicts the long-standing dogma that the upper and lower limbs are serial homologues. In addition, the AnNA of the limbs of a trisomy 18 human fetus strongly supports Pere Alberch's ill-named "logic of monsters" hypothesis, and contradicts the commonly accepted idea that birth defects often lead to lower integration (i.e. more parcellation) of anatomical structures.

Cardiopulmonary Response to Videogaming: Slaying Monsters Using Motion Sensor Versus Joystick Devices.

PubMed

Sherman, Jeffrey D; Sherman, Michael S; Heiman-Patterson, Terry

2014-10-01

Replacing physical activity with videogaming has been implicated in causing obesity. Studies have shown that using motion-sensing controllers with activity-promoting videogames expends energy comparable to aerobic exercise; however, effects of motion-sensing controllers have not been examined with traditional (non-exercise-promoting) videogames. We measured indirect calorimetry and heart rate in 14 subjects during rest and traditional videogaming using motion sensor and joystick controllers. Energy expenditure was higher while subjects were playing with the motion sensor (1.30±0.32 kcal/kg/hour) than with the joystick (1.07±0.26 kcal/kg/hour; P<0.01) or resting (0.91±0.24 kcal/kg/hour; P<0.01). Oxygen consumption during videogaming averaged 15.7 percent of predicted maximum for the motion sensor and 11.8 percent of maximum for the joystick. Minute ventilation was higher playing with the motion sensor (10.7±3.5 L/minute) than with the joystick (8.6±1.8 L/minute; P<0.02) or resting (6.7±1.4 L/minute; P<0.001), predominantly because of higher respiratory rates (15.2±4.3 versus 20.3±2.8 versus 20.4±4.2 beats/minute for resting, the joystick, and the motion sensor, respectively; P<0.001); tidal volume did not change significantly. Peak heart rate during gaming was 16.4 percent higher than resting (78.0±12.0) for joystick (90.1±15.0; P=0.002) and 17.4 percent higher for the motion sensor (91.6±14.1; P=0.002); mean heart rate did not differ significantly. Playing with a motion sensor burned significantly more calories than with a joystick, but the energy expended was modest. With both consoles, the increased respiratory rate without increasing tidal volume and the increased peak heart rate without increasing mean heart rate are consistent with psychological stimulation from videogaming, rather than a result of exercise. We conclude that using a motion sensor with traditional videogames does not provide adequate energy expenditure to provide cardiovascular conditioning.

Varanoid Tooth Eruption and Implantation Modes in a Late Cretaceous Mosasaur.

PubMed

Liu, Min; Reed, David A; Cecchini, Giancarlo M; Lu, Xuanyu; Ganjawalla, Karan; Gonzales, Carol S; Monahan, Richard; Luan, Xianghong; Diekwisch, Thomas G H

2016-01-01

Erupting teeth are some of the oldest witnesses of developmental processes in the vertebrate fossil record and provide an important resource for vertebrate cladistics. Here, we have examined a mosasaur jaw fragment from central Texas using ultrathin ground section histology and 3D tomographic imaging to assess features critical for the cladistic placement of mosasaurs among varanoids vs. snakes: (i) the orientation of replacement teeth compared to the major tooth axis, (ii) the occurrence of resorption pits, and (iii) the mode of tooth implantation/attachment to the tooth bearing element (TBE). The replacement tooth studied here developed in an inclined position slightly distal of the deciduous parent tooth, similar to another varanoid squamate, the Gila monster Heloderma suspectum. Ground sections and tomographs also demonstrated that the replacement tooth attachment apparatus was entirely intact and that there was no evidence of mechanical deformation. Sections and tomographs further illustrated that the replacement tooth was located within a bony crypt and the inclination of the crypt matched the inclination of the replacement tooth. These preparations also revealed the presence of a resorption pit within the boundaries of the deciduous tooth that surrounded the developing replacement tooth. This finding suggests that developing mosasaur teeth developed within the walls of resorption pits similar to varanoid tooth germs and unlike developing snake teeth which are surrounded by fibrous connective tissue integuments. Finally, mosasaurs featured pseudo-thecodont tooth implantation with teeth anchored within a socket of mineralized tissue by means of a mineralized periodontal ligament. Together, these data indicate that the moderate inclination of the erupting mosasaur tooth studied here is neither a result of postmortem displacement nor a character representative of snakes, but rather a shared character between Mosasaurs and other varanoids such as Heloderma. In conjunction with the presence of resorption pits and the evidence for pseudothecodont tooth implantation, the tooth eruption and implantation characters described in the present study either place mosasaurs among the varanoids or suggest convergent evolution mechanisms between both clades, with mosasaurs evolving somewhat independently from a common varanoid ancestor.

Varanoid Tooth Eruption and Implantation Modes in a Late Cretaceous Mosasaur

PubMed Central

Liu, Min; Reed, David A.; Cecchini, Giancarlo M.; Lu, Xuanyu; Ganjawalla, Karan; Gonzales, Carol S.; Monahan, Richard; Luan, Xianghong

2016-01-01

Erupting teeth are some of the oldest witnesses of developmental processes in the vertebrate fossil record and provide an important resource for vertebrate cladistics. Here, we have examined a mosasaur jaw fragment from central Texas using ultrathin ground section histology and 3D tomographic imaging to assess features critical for the cladistic placement of mosasaurs among varanoids vs. snakes: (i) the orientation of replacement teeth compared to the major tooth axis, (ii) the occurrence of resorption pits, and (iii) the mode of tooth implantation/attachment to the tooth bearing element (TBE). The replacement tooth studied here developed in an inclined position slightly distal of the deciduous parent tooth, similar to another varanoid squamate, the Gila monster Heloderma suspectum. Ground sections and tomographs also demonstrated that the replacement tooth attachment apparatus was entirely intact and that there was no evidence of mechanical deformation. Sections and tomographs further illustrated that the replacement tooth was located within a bony crypt and the inclination of the crypt matched the inclination of the replacement tooth. These preparations also revealed the presence of a resorption pit within the boundaries of the deciduous tooth that surrounded the developing replacement tooth. This finding suggests that developing mosasaur teeth developed within the walls of resorption pits similar to varanoid tooth germs and unlike developing snake teeth which are surrounded by fibrous connective tissue integuments. Finally, mosasaurs featured pseudo-thecodont tooth implantation with teeth anchored within a socket of mineralized tissue by means of a mineralized periodontal ligament. Together, these data indicate that the moderate inclination of the erupting mosasaur tooth studied here is neither a result of postmortem displacement nor a character representative of snakes, but rather a shared character between Mosasaurs and other varanoids such as Heloderma. In conjunction with the presence of resorption pits and the evidence for pseudothecodont tooth implantation, the tooth eruption and implantation characters described in the present study either place mosasaurs among the varanoids or suggest convergent evolution mechanisms between both clades, with mosasaurs evolving somewhat independently from a common varanoid ancestor. PMID:27242535

Hubble Helps Find Smallest Known Galaxy Containing a Supermassive Black Hole

NASA Image and Video Library

2017-12-08

This is an illustration of a supermassive black hole, weighing as much as 21 million suns, located in the middle of the ultradense galaxy M60-UCD1. The dwarf galaxy is so dense that millions of stars fill the sky as seen by an imaginary visitor. Because no light can escape from the black hole, it appears simply in silhouette against the starry background. The black hole's intense gravitational field warps the light of the background stars to form ring-like images just outside the dark edges of the black hole's event horizon. Combined observations by the Hubble Space Telescope and Gemini North telescope determined the presence of the black hole inside such a small and dense galaxy. More info: Astronomers using data from NASA’s Hubble Space Telescope and ground observation have found an unlikely object in an improbable place -- a monster black hole lurking inside one of the tiniest galaxies ever known. The black hole is five times the mass of the one at the center of our Milky Way galaxy. It is inside one of the densest galaxies known to date -- the M60-UCD1 dwarf galaxy that crams 140 million stars within a diameter of about 300 light-years, which is only 1/500th of our galaxy’s diameter. If you lived inside this dwarf galaxy, the night sky would dazzle with at least 1 million stars visible to the naked eye. Our nighttime sky as seen from Earth’s surface shows 4,000 stars. The finding implies there are many other compact galaxies in the universe that contain supermassive black holes. The observation also suggests dwarf galaxies may actually be the stripped remnants of larger galaxies that were torn apart during collisions with other galaxies rather than small islands of stars born in isolation. “We don’t know of any other way you could make a black hole so big in an object this small,” said University of Utah astronomer Anil Seth, lead author of an international study of the dwarf galaxy published in Thursday’s issue of the journal Nature. Seth’s team of astronomers used the Hubble Space Telescope and the Gemini North 8-meter optical and infrared telescope on Hawaii’s Mauna Kea to observe M60-UCD1 and measure the black hole’s mass. The sharp Hubble images provide information about the galaxy’s diameter and stellar density. Gemini measures the stellar motions as affected by the black hole’s pull. These data are used to calculate the mass of the black hole. Black holes are gravitationally collapsed, ultra-compact objects that have a gravitational pull so strong that even light cannot escape. Supermassive black holes -- those with the mass of at least one million stars like our sun -- are thought to be at the centers of many galaxies. The black hole at the center of our Milky Way galaxy has the mass of four million suns. As heavy as that is, it is less than 0.01 percent of the Milky Way’s total mass. By comparison, the supermassive black hole at the center of M60-UCD1, which has the mass of 21 million suns, is a stunning 15 percent of the small galaxy’s total mass. “That is pretty amazing, given that the Milky Way is 500 times larger and more than 1,000 times heavier than the dwarf galaxy M60-UCD1,” Seth said. One explanation is that M60-UCD1 was once a large galaxy containing 10 billion stars, but then it passed very close to the center of an even larger galaxy, M60, and in that process all the stars and dark matter in the outer part of the galaxy were torn away and became part of M60. The team believes that M60-UCD1 may eventually be pulled to fully merge with M60, which has its own monster black hole that weighs a whopping 4.5 billion solar masses, or more than 1,000 times bigger than the black hole in our galaxy. When that happens, the black holes in both galaxies also likely will merge. Both galaxies are 50 million light-years away. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore conducts Hubble science operations. STScI is operated for NASA by the Association of Universities for Research in Astronomy, Inc., in Washington. For images and more information about Hubble, visit: www.nasa.gov/hubble NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Comets Kick up Dust in Helix Nebula

NASA Technical Reports Server (NTRS)

2007-01-01

This infrared image from NASA's Spitzer Space Telescope shows the Helix nebula, a cosmic starlet often photographed by amateur astronomers for its vivid colors and eerie resemblance to a giant eye.

The nebula, located about 700 light-years away in the constellation Aquarius, belongs to a class of objects called planetary nebulae. Discovered in the 18th century, these colorful beauties were named for their resemblance to gas-giant planets like Jupiter.

Planetary nebulae are the remains of stars that once looked a lot like our sun. When sun-like stars die, they puff out their outer gaseous layers. These layers are heated by the hot core of the dead star, called a white dwarf, and shine with infrared and visible colors. Our own sun will blossom into a planetary nebula when it dies in about five billion years.

In Spitzer's infrared view of the Helix nebula, the eye looks more like that of a green monster's. Infrared light from the outer gaseous layers is represented in blues and greens. The white dwarf is visible as a tiny white dot in the center of the picture. The red color in the middle of the eye denotes the final layers of gas blown out when the star died.

The brighter red circle in the very center is the glow of a dusty disk circling the white dwarf (the disk itself is too small to be resolved). This dust, discovered by Spitzer's infrared heat-seeking vision, was most likely kicked up by comets that survived the death of their star. Before the star died, its comets and possibly planets would have orbited the star in an orderly fashion. But when the star blew off its outer layers, the icy bodies and outer planets would have been tossed about and into each other, resulting in an ongoing cosmic dust storm. Any inner planets in the system would have burned up or been swallowed as their dying star expanded.

So far, the Helix nebula is one of only a few dead-star systems in which evidence for comet survivors has been found.

This image is made up of data from Spitzer's infrared array camera and multiband imaging photometer. Blue shows infrared light of 3.6 to 4.5 microns; green shows infrared light of 5.8 to 8 microns; and red shows infrared light of 24 microns.

Influence of solar flare X-rays on the habitability on the Mars

NASA Astrophysics Data System (ADS)

Jain, Rajmal; Awasthi, Arun K.; Tripathi, Sharad C.; Bhatt, Nipa J.; Khan, Parvaiz A.

2012-08-01

We probe the lethality of X-rays from solar flares to organisms on Mars based on the observations of 10 solar flares. We, firstly, estimate the doses produced by the strong flares observed by the RHESSI and GOES missions during the descending phase of sunspot cycle 23. Next, in order to realize the dependence of dose on flux and steepness of spectra, we model the incident spectra over a wide range of spectral index to estimate dose values and compare them with the observed doses. We calculate the distribution of surficial spectra visible to organisms on the martian surface by employing attenuation of X-rays due to CO2 column densities distribution over the South Pole. The surficial flux distribution after folding with the opacity of water enables us to estimate the dose distribution over the South Pole. The dose measured from the surficial spectrum produced by the observed 10 flares corresponding to the latitudes 50-60°, 60-70°, 70-80° and 80-90°S varies in the range of 6.39 × 10-9-1.80 × 10-6; 4.89 × 10-10-5.21 × 10-8; 5.10 × 10-11-5.20 × 10-9 and 4.42 × 10-10-4.89 × 10-12 gray (1 gray = 104 erg/g) respectively. Comparing the measured as well as the modeled doses with those proposed to be lethal for various organisms by Smith and Scalo (Smith, D.S., Scalo, J. [2007]. Planet. Space Sci. 55, 517-527); we report that the habitability of life on the South Pole remains unaffected even by the strongest solar flare occurred during descending phase of solar cycle 23. Further, the monthly integrated energy released by the solar flares in the most productive month viz. October 2003 and January 2005 from the GOES soft X-ray observations is estimated to be 8.43 and 3.32 × 1032 ergs respectively, which is almost equal in order to the typical energy released by a single strong X-class flare. Therefore, we propose the life near the South Pole region on the Mars remain uninfluenced by X-ray emission even during monster phenomena of energy release on the Sun and/or Star.

Medusae Fossae Formation

NASA Technical Reports Server (NTRS)

2002-01-01

(Released 10 April 2002) The Science This THEMIS visible image was acquired near 7o S, 172o W (188o E) and shows a remarkable martian geologic deposit known as the Medusae Fossae Formation. This Formation, seen here as the raised plateau in the upper two-thirds of the image, is a soft, easily eroded deposit that extends for nearly 1,000 km along the equator of Mars. In this region the deposit has been heavily eroded by the wind to produce a series of linear ridges called yardangs. These parallel ridges point in direction of the prevailing winds that carved them, and demonstrate the power of martian winds to sculpt the dry landscape of Mars. The Medusae Fossae Formation has been completely stripped from the surface in the lower third of the image, revealing a harder layer below that is more resistant to wind erosion. The easily eroded nature of the Medusae Fossae Formation suggests that it is composed of weakly cemented particles, and was most likely formed by the deposition of wind-blown dust or volcanic ash. Several ancient craters that were once completely buried by this deposit are being exposed, or exhumed, as the overlying Medusae Formation is removed. Very few impact craters are visible on this Formation, indicating that the surface seen today is relatively young, and that the processes of erosion are likely to be actively occurring. The Story Medusa of Greek mythology fame, the name-giver to this region, had snaky locks of hair that could turn a person to stone. Wild and unruly, this monster of the underworld could certainly wreak havoc on the world of the human imagination. As scary as she was, Medusa would have no advantage over the fierce, masterful winds blowing across Mars, which once carved the streaky, terrain at the top of this image. Wild and whipping, these winds have slowly eroded away the 'topsoil,' revealing ancient craters and other surface features they once covered. The loosely cemented particles of this 'topsoil' are likely made up of dust or volcanic ash, and are thus more susceptible to windblown erosion. The Martian winds have actually been strong and relentless enough over time to strip the land in the bottom of this image of the material that once covered it, leaving it hard and bare to the eye.

Consumption of energy beverage is associated with attenuation of arterial endothelial flow-mediated dilatation.

PubMed

Higgins, John P; Yang, Benjamin; Herrin, Nikki E; Yarlagadda, Santi; Le, George T; Ortiz, Brandon L; Ali, Asif; Infanger, Stephen C

2017-02-26

To investigate whether consumption of an energy drink will acutely impair endothelial function in young healthy adults. Energy drinks are being consumed more and more worldwide, and have been associated with some deaths in adolescents and young adults, especially when consumed while exercising. After fasting and not smoking for at least 8 h prior, eleven medical students (9 males) received an electrocardiogram, blood pressure and pulse check, and underwent baseline testing (BL) of endothelial function using the technique of endothelium-dependent flow mediated dilatation (FMD) with high-resolution ultrasound (according to recommended guidelines of the University of Wisconsin Atherosclerosis Imaging Research Program Core Laboratory). The subjects then drank an energy beverage (EB), a 24-oz can of Monster Energy, and the above was repeated at 90 min after consumption. The relative FMD (%) was calculated as the ratio between the average post-cuff release and the baseline diameter. Each image was checked for quality control, and each artery diameter was measured from the media to media points by two experts, 3 measurements at the QRS complex, repeated on 3 separate beats, and then all were averaged. Subjects characteristics averages (given with standard deviations) include: Age 24.5 ± 1.5 years, sex 9 male and 2 female, weight 71.0 ± 9.1 kg, height 176.4 ± 6.0 cm, BMI 22.8 ± 2.7 kg/m 2 . The hemodynamics were as follows, BL vs EB group respectively (mean ± SD): Heart rate 65.2 ± 11.3 vs 68.2 ± 11.8 beats per minute, systolic blood pressure 114.0 ± 10.4 mmHg vs 114.1 ± 10.4 mmHg, diastolic blood pressure 68.8 ± 9.3 mmHg vs 70.6 ± 7.1 mmHg; all were not significantly different. However after drinking the EB, a significantly attenuated peak FMD response was measured (mean ± SD): BL group 5.9% ± 4.6% vs EB group 1.9% ± 2.1%; P = 0.03). Given the increased consumption of energy beverages associated with exercise in young adults, more research is needed. Energy beverage consumption has a negative impact on arterial endothelial function in young healthy adults.

in the wind clothes dance on a line. Performative inquiry: A (re)search methodology. Possibilities and absences within a space-moment of imagining a universe

NASA Astrophysics Data System (ADS)

Fels, Lynn Margaret

in the wind clothes dance on a line is the conceptualization and articulation of performative inquiry as a research methodology within the field of education. Performative inquiry invites innovative and non-linear investigations, playing upon the multiple realities and interpretations of co-evolving worlds realized and recognized through creative action and interaction between researcher/teacher and participants/students within individual and shared, existing and imagined environments through motivating (im)pulse(s) of inquiry. Performative inquiry is elusively and momentarily balanced on the "edge of chaos" within the interstices of enactivism, complexity, interpretation, and performance. In articulating an ecological-cognitive reading of performance, I am in company with curricular theorists who envision curriculum as a journey and expression of students' and teachers' shared investigations within co-evolving landscapes of action and interaction. in the wind clothes dance on a line is a playful response to current conversations among researchers seeking recognition and articulation of arts-based processes as legitimate site(s) and praxis of research. Performative inquiry offers researchers---in drama education, in particular, and in education, in general---a theoretical and practical venue to investigate their fields of inquiry through an integrated vehicle of body, mind and imagination. This dissertation is informed by a three year science education research project (1995--1997) conducted with science educator, Karen Meyer. Our research investigated the teaching and learning of science education through drama and storytelling, culminating in a performance piece, Light Sound Movin' Around: What Are Monsters Made Of? Follow-up interviews with pre-service teachers speak eloquently to the possibility and power of performative inquiry as a research tool and learning vehicle in science education. in the wind clothes dance on a line has been imagined "in the air" through moments realized and recognized during the science education research project and through my work as a performing arts educator. And it is these moments that set the clothes dancing in the wind. in the wind clothes dance on a line is a conceptual piece, a performative work through which the reader will hopefully realize and recognize his or her own imaginings and understandings of possible universes within education.

Can personality traits predict pathological responses to audiovisual stimulation?

PubMed

Yambe, Tomoyuki; Yoshizawa, Makoto; Fukudo, Shin; Fukuda, Hiroshi; Kawashima, Ryuta; Shizuka, Kazuhiko; Nanka, Shunsuke; Tanaka, Akira; Abe, Ken-ichi; Shouji, Tomonori; Hongo, Michio; Tabayashi, Kouichi; Nitta, Shin-ichi

2003-10-01

The "Pockemon shock" is the most famous accident in the history of the broadcasting industry in Japan. Based on the experiences of this unfortunate accident from famous animation program "Pocket Monster", this study focused on the psychology and psychosomatics of the patients. A head-mounted display was used as the three-dimensional image presentation device and "Descent", a free software shooting game, was used as the software. Ten healthy adult male volunteers were used in this experiment after obtaining their informed consent. The oxygen metabolic change in the anterior lobe of the brain was measured by near infrared spectroscopy and recorded on an electrocardiogram. The mental scaling tendency of the object was analyzed using the type A behavior pattern and the hostility scaling. The Cook and Medley hostility (HO) scale from the Minnesota multiphasic personality inventory (MMPI) was also used in this experiment. From this scaling methodology, the paranoid scale, cynicism scale, lie scale, social support quality and social support quantity were calculated. All measured time series data were kept in the normal range, and no fatal arrhythmia or epilepsy were observed during experiments. In some cases, the brain oxygen metabolism may completely differ for the objects of Type A and Type B behavior patterns. On the whole, correlation did not become significant in type A scaling and hostility scaling. In a comparison of the percent changes of the HF in HRV with lie scaling, significant negative correlation was observed. The social support quantity was calculated from Cook and Medley, and significant negative correlations were observed with percent changes of LF/HF in HRV. The lie scale and social support quantity are opposite scaling. The sympathetic nervous system and parasympathetic nervous system have an opposite function also. Therefore, our results showed an interesting phenomenon, when considering the relationship between the autonomic function and the pathophysiological reaction to the audiovisual stimulations. As for the photo sensitive epilepsy, it was reported to be only 5-10% for all patients. Therefore, 90% or more of the cause could not be determined in patients who started a morbid response. The results in this study suggest that the autonomic function was connected to the mental tendency of the objects. By examining such directivity, it is expected that subjects, which show morbid reaction to an audiovisual stimulation, can be screened beforehand.

Doing battle with "the monster:" how high-risk heterosexuals experience and successfully manage HIV stigma as a barrier to HIV testing.

PubMed

Gwadz, Marya; Leonard, Noelle R; Honig, Sylvie; Freeman, Robert; Kutnick, Alexandra; Ritchie, Amanda S

2018-04-20

Annual HIV testing is recommended for populations at-risk for HIV in the United States, including heterosexuals geographically connected to urban high-risk areas (HRA) with elevated rates of HIV prevalence and poverty, who are primarily African American/Black or Hispanic. Yet this subpopulation of "individuals residing in HRA" (IR-HRA) evidence low rates of regular HIV testing. HIV stigma is a recognized primary barrier to testing, in part due to its interaction with other stigmatized social identities. Guided by social-cognitive and intersectionality theories, this qualitative descriptive study explored stigma as a barrier to HIV testing and identified ways IR-HRA manage stigma. In 2012-2014, we conducted in-depth qualitative interviews with 31 adult IR-HRA (74% male, 84% African American/Black) with unknown or negative HIV status, purposively sampled from a larger study for maximum variation on HIV testing experiences. Interviews were audio-recorded and professionally transcribed verbatim. Data were analyzed using a systematic content analysis approach that was both theory-driven and inductive. Stigma was a primary barrier to HIV testing among IR-HRA. In the context of an under-resourced community, HIV stigma was experienced as emerging from, and being perpetuated by, health care organizations and educational institutions, as well as community members. Participants noted it was "better not to know" one's HIV status, to avoid experiencing HIV-related stigma, which could interact with other stigmatized social identities and threaten vital social relationships, life chances, and resources. Yet most had tested for HIV previously. Factors facilitating testing included health education to boost knowledge of effective treatments for HIV; understanding HIV does not necessitate ending social relationships; and tapping into altruism. In the context of economic and social inequality, HIV stigma operates on multiple, intersecting layers. IR-HRA struggle with an aversion to HIV testing, because adopting another stigmatized status is dangerous. They also find ways to manage stigma to engage in testing, even if not at recommended levels. Findings highlight strategies to reduce HIV stigma at the levels of communities, institutions, and individuals to improve rates of annual HIV testing necessary to eliminate HIV transmission and reduce HIV-related racial and ethnic health disparities among IR-HRA.

Fueling nuclear activity in disk galaxies: Starbursts and monsters

NASA Astrophysics Data System (ADS)

Heller, Clayton H.; Shlosman, Isaac

1994-03-01

We study the evolution of the gas distribution in a globally unstable galactic disk with a particular emphasis on the gasdynamics in the central kiloparsec and the fueling activity there. The two-component self-gravitating disk is embedded in a responsive halo of comparable mass. The gas and stars are evolved using a three-dimensional hybrid smoothed particle hydrodynamics/N-body code and the gravitational interactions are calculated using a hierarchical TREE algorithm. A massive 'star formation' is introduced when the gas becomes Jeans unstable and locally exceeds the critical density of approximately 100 solar mass pc-3. The newly formed OB stars deposit energy in the gas by means of radiation-driven winds and supernovae. This energy is partially thermalized (efficiency of a few percent); the rest is radiated away. Models without star formation are evolved for a comparison. The effect of a massive object at the disk center is studied by placing a 'seed' black hole (BH) of 5 x 107 solar mass with an accretion radius of 20 pc. The tendency of the system to form a massive object 'spontaneously' is tested in models without the BH. We find that for models without star formation the bar- or dynamical friction-driven inflows lead to (1) domination of the central kpc by a few massive clouds that evolve into a single object probably via a cloud binary system, with and without a 'seed' BH, (2) accretion onto the BH which has a sporadic character, and (3) formation of remnant disks around the BH with a radius of 60-80 pc which result from the capture and digestion of clouds. For models with star formation, we find that (1) the enrgy input into the gas induces angular momentum loss and inflow rates by a factor less than 3, (2) the star formation is concentrated mainly at the apocenters of the gaseous circulation in the stellar bar and in the nuclear region, (3) the nuclear starburst phase appears to be very luminous approximately 1045-1046 erg/s and episodic with a typical single burst duration of aproximately 107 yr, and (4) the starburst phase coincides with both the gas becoming dynamically important and the catastrophic growth of the BH. It ends with the formation of cold residual less than 1 kpc radius gas disks. Models without the 'seed' BH form less than 1 kpc radius fat disks which dominate the dynamics. Gaseous bars follow, drive further inflow, and may fission into a massive cloud binary system at the center.

Welcoming a monster to the world: Myths, oral tradition, and modern societal response to volcanic disasters

NASA Astrophysics Data System (ADS)

Cashman, Katharine V.; Cronin, Shane J.

2008-10-01

Volcanic eruptions can overwhelm all senses of observers in their violence, spectacle and sheer incredibility. When an eruption is catastrophic or unexpected, neither individuals nor communities can easily assimilate the event into their world view. Psychological studies of disaster aftermaths have shown that trauma can shake the very foundations of a person's faith and trigger a search - supernatural, religious, or scientific - for answers. For this reason, the ability to rapidly comprehend a traumatic event by "accepting" the catastrophe as part the observer's world represents an important component of community resilience to natural hazards. A relationship with the event may be constructed by adapting existing cosmological, ancestral, or scientific frameworks, as well as through creative and artistic expression. In non-literate societies, communal perceptions of an event may be transformed into stories that offer myth-like explanations. As these stories make their way into oral traditions, they often undergo major changes to allow transmission through generations and, in some cases, to serve political or religious purposes. Disaster responses in literate societies are no different, except that they are more easily recorded and therefore are less prone to change over time. Here we explore ways in which the language, imagery and metaphor used to describe volcanic events may link disparate societies (both present and past) in their search for understanding of volcanic catastrophes. Responses to modern eruptions (1980 Mount St Helens, USA, and 1995-present Soufriere Hills, Montserrat) provide a baseline for examining the progression to older historic events that have already developed oral traditions (1886 Tarawera, New Zealand) and finally to oral traditions many hundreds of years old in both the Pacific Northwest US and New Zealand (NZ). We see that repeated volcanism over many generations produces rich webs of cosmology and history surrounding volcanoes. NZ Maori have incorporated volcanoes into the lineage of tribes and individuals, thus good and bad outcomes from volcanism are part of long-term cycles of reciprocity and equilibrium that link modern Maori to their ancestors. In both regions, cosmologies and mythologies not only document the attempts of past cultures to recover from the impacts of volcanic disasters, but also provide a means by which following generations can understand, contextualize, and therefore recover from, future volcanic catastrophes. We further suggest that such local traditions can provide a valuable community education tool as well as an important means of aiding the psychosocial recovery of individuals and communities after volcanic disasters.

Real Science, Real Learning: Bridging the Gap Between Scientists, Educators and Students

NASA Astrophysics Data System (ADS)

Lewis, Y.

2006-05-01

Today as never before, America needs its citizens to be literate in science and technology. Not only must we only inspire a new generation of scientists and engineers and technologists, we must foster a society capable of meeting complex, 21st-century challenges. Unfortunately, the need for creative, flexible thinkers is growing at a time when our young students are lagging in science interest and performance. Over the past 17 years, the JASON Project has worked to link real science and scientists to the classroom. This link provide viable pipeline to creating the next generation scientists and researchers. Ultimately, JASON's mission is to improve the way science is taught by enabling students to learn directly from leading scientists. Through partnerships with agencies such as NOAA and NASA, JASON creates multimedia classroom products based on current scientific research. Broadcasts of science expeditions, hosted by leading researchers, are coupled with classroom materials that include interactive computer-based simulations, video- on-demand, inquiry-based experiments and activities, and print materials for students and teachers. A "gated" Web site hosts online resources and provides a secure platform to network with scientists and other classrooms in a nationwide community of learners. Each curriculum is organized around a specific theme for a comprehensive learning experience. It may be taught as a complete package, or individual components can be selected to teach specific, standards-based concepts. Such thematic units include: Disappearing Wetlands, Mysteries of Earth and Mars, and Monster Storms. All JASON curriculum units are grounded in "inquiry-based learning." The highly interactive curriculum will enable students to access current, real-world scientific research and employ the scientific method through reflection, investigation, identification of problems, sharing of data, and forming and testing hypotheses. JASON specializes in effectively applying technology in science education by designing animated interactive visualizations that promote student understanding of complex scientific concepts and systems (Rieber, 1990, 1996). JASON's experience in utilizing the power of simulation technology has been widely recognized for its effectiveness in exciting and engaging students in science learning by independent evaluations of JASON's multimedia science curriculum (Ba et al., 2001; Goldenberg et al., 2003). The data collected indicates that JASON's science products have had a positive impact on students' science learning, have positively influenced their perceptions of scientists and of becoming scientists, and have helped diverse students grasp a deeper understanding of complex scientific content, concepts and technologies.

Rogue wave variational modelling through the interaction of two solitary waves

NASA Astrophysics Data System (ADS)

Gidel, Floriane; Bokhove, Onno

2016-04-01

The extreme and unexpected characteristics of Rogue waves have made them legendary for centuries. It is only on the 1st of January 1995 that these mariners' tales started to raise scientist's curiosity, when such a wave was recorded in the North Sea; a sudden wall of water hit the Draupner offshore platform, more than twice higher than the other waves, providing evidence of the existence of rogue or freak waves. Since then, studies have shown that these surface gravity waves of high amplitude (at least twice the height of the other sea waves [Dyste et al., 2008]) appear in non-linear dispersive water motion [Drazin and Johnson, 1989], at any depth, and have caused a lot of damage in recent years [Nikolkina and Didenkulova, 2011 ]. So far, most of the studies have tried to determine their probability of occurrence, but no conclusion has been achieved yet, which means that we are currently unenable to predict or avoid these monster waves. An accurate mathematical and numerical water-wave model would enable simulation and observation of this external forcing on boats and offshore structures and hence reduce their threat. In this work, we aim to model rogue waves through a soliton splash generated by the interaction of two solitons coming from different channels at a specific angle. Kodama indeed showed that one way to produce extreme waves is through the intersection of two solitary waves, or one solitary wave and its oblique reflection on a vertical wall [Yeh, Li and Kodama, 2010 ]. While he modelled Mach reflection from Kadomtsev-Petviashvili (KP) theory, we aim to model rogue waves from the three-dimensional potential flow equations and/or their asymptotic equivalent described by Benney and Luke [Benney and Luke, 1964]. These theories have the advantage to allow wave propagation in several directions, which is not the case with KP equations. The initial solitary waves are generated by removing a sluice gate in each channel. The equations are derived through a variational approach, based on Luke's variational principle [Luke, 1967], and its dynamical equivalent from Miles [Miles, 1977], that describe incompressible and inviscid potential flows with free surface, through the variations of the Lagrangian. This Lagrangian, obtained from Bernouilli's equations, can be expressed in a Hamiltonian form, for which robust time integrators have been derived [Gagarina et al., 2015]. A Galerkin finite element method is then used to solve the system numerically, and we aim to compare our simulations to exact solutions of the KP-equation.

The Role of Healthcare Professionals in Encouraging Parents to See and Hold Their Stillborn Baby: A Meta-Synthesis of Qualitative Studies

PubMed Central

Kingdon, Carol; O’Donnell, Emer; Givens, Jennifer; Turner, Mark

2015-01-01

Background Globally, during 2013 there were three million recorded stillbirths. Where clinical guidelines exist some recommend that professionals do not encourage parental contact. The guidance is based on quantitative evidence that seeing and holding the baby is not beneficial for everyone, but has been challenged by bereaved parents' organisations. We aim to inform future guideline development through a synthesis of qualitative studies reporting data relevant to the research question; how does the approach of healthcare professionals to seeing and holding the baby following stillbirth impact parents views and experiences? Methods/Findings Using a predetermined search strategy of PubMed and PsychINFO we identified robust qualitative studies reporting bereaved parental views and/or experiences relating to seeing and holding their stillborn baby (final search 24 February, 2014). Eligible studies were English language, reporting parental views, with gestational loss >20weeks. Quality was independently assessed by three authors using a validated tool. We used meta-ethnographic techniques to identify key themes and a line of argument synthesis. We included 12 papers, representing the views of 333 parents (156 mothers, 150 fathers, and 27 couples) from six countries. The final themes were: "[Still]birth: Nature of care is paramount", "Real babies: Perfect beauties, monsters and spectres", and "Opportunity of a lifetime lost." Our line-of-argument synthesis highlights the contrast between all parents need to know their baby, with the time around birth being the only time memories can be made, and the variable ability that parents have to articulate their preferences at that time. Thus, we hypothesised that how health professionals approach contact between parents and their stillborn baby demands a degree of active management. An important limitation of this paper is all included studies originated from high income, westernised countries raising questions about the findings transferability to other cultural contexts. We do not offer new evidence to answer the question "Should parents see and hold their stillborn baby?", instead our findings advance understanding of how professionals can support parents to make appropriate decisions in a novel, highly charged and dynamic situation. Conclusions Guidelines could be more specific in their recommendations regarding parental contact. The role of healthcare professionals in encouraging parents to see and hold their stillborn baby is paramount. Parental choice not to see their baby, apprehension, or uncertainty should be continuously revisited in the hours after birth as the opportunity for contact is fleeting and final. PMID:26154302

[Pathological nighttime fears in children: Clinical specificities and effective therapeutics].

PubMed

Ducasse, D; Denis, H

2015-09-01

Pathological nighttime fears in children have been little studied. However, this disorder is commonly encountered in medical consultations and is discomforting and dysfunctional for both the child and the family. Most nighttime fears are part and parcel of normal development, and emanate from increasingly sophisticated cognitive development in the growing child. Thus, most children report a variety of coping strategies generally helpful in reducing their anxiety, which resolves spontaneously in the growing child. Nevertheless, in about 10% of children, nighttime fears are related to one or more anxiety disorders according to Diagnostic and Statistical Manual of Mental Disorders criteria. Then, it is estimated that severe nighttime fears and sleep problems occur in 20-30% of children. This problem is not transient and has to be treated. This study aims to review clinical features of nighttime fears and possible treatments for these patients and their families. This systematic review follows the preferred reporting items for systematic reviews and meta-analysis (PRISMA) statement guidelines. Two databases (Medline and Web of Science) were searched combining the search terms: nighttime fears AND children. English and French languages were imposed. There were no publication date or publication status limitations. Pathological nighttime fears are responsible for emotional (crying, panic, tantrums at bedtime, loss of confidence, self-disparaging negative statements, and feeling of social embarrassment) and behavioral (wandering alone in the house at night, calls for parental or sibling comfort, bed sharing with parents or siblings, light source at night, refusal to go to the toilet alone at night) disturbances. This leads to a poor quality of sleep interfering with school learning, and also affects social development and family functioning. A full assessment has to be made to eliminate organic causes, have a baseline functioning, and search for comorbid anxiety diseases. The treatments which have proved effective are some cognitive-behavioral techniques: systematic desensitization (with relaxation or emotive imagery), reinforcement (gain of points and techniques of self statement), and cognitive techniques (reinforcing self-statements, reducing the aversive aspects of being in the dark, involving reality-testing statements, and active control are preferred in children older than 6 years, whereas the "anti-monster letter" and the techniques using a doll are preferred in children under 6 years old). The modelling technique seems to be appropriate at any age. We have explained the clinical features of pathological nighttime fears and the way to assess this disease, and we have pointed out the treatments whose effectiveness has been evaluated in this indication. Copyright © 2014 L’Encéphale, Paris. Published by Elsevier Masson SAS. All rights reserved.

Feeding the Monster

NASA Astrophysics Data System (ADS)

2005-10-01

Near-infrared images of the active galaxy NGC 1097, obtained with the NACO adaptive optics instrument on ESO's Very Large Telescope, disclose with unprecedented detail a complex central network of filamentary structure spiralling down to the centre of the galaxy. These observations provide astronomers with new insights on how super-massive black holes lurking inside galaxies get fed. "This is possibly the first time that a detailed view of the channelling process of matter, from the main part of the galaxy down to the very end in the nucleus is released," says Almudena Prieto (Max-Planck Institute, Heidelberg, Germany), lead author of the paper describing these results. Located at a distance of about 45 million light-years in the southern constellation Fornax (the Furnace), NGC 1097 is a relatively bright, barred spiral galaxy seen face-on. At magnitude 9.5, and thus just 25 times fainter than the faintest object that can be seen with the unaided eye, it appears in small telescopes as a bright, circular disc. NGC 1097 is a very moderate example of an Active Galactic Nucleus (AGN), whose emission is thought to arise from matter (gas and stars) falling into oblivion in a central black hole. However, NGC 1097 possesses a comparatively faint nucleus only, and the black hole in its centre must be on a very strict "diet": only a small amount of gas and stars is apparently being swallowed by the black hole at any given moment. Astronomers have been trying to understand for a long time how the matter is "gulped" down towards the black hole. Watching directly the feeding process requires very high spatial resolution at the centre of galaxies. This can be achieved by means of interferometry as was done with the VLTI MIDI instrument on the central parts of another AGN, NGC 1068 (see ESO PR 17/03), or with adaptive optics [1]. Thus, astronomers [2] obtained images of NGC 1097 with the adaptive optics NACO instrument attached to Yepun, the fourth Unit Telescope of ESO's VLT. These new images probe with unprecedented detail the presence and extent of material in the very proximity of the nucleus. The resolution achieved with the images is about 0.15 arcsecond, corresponding to about 30 light-years across. For comparison, this is only 8 times the distance between the Sun and its nearest star, Proxima Centauri. ESO PR Photo 33b/05 ESO PR Photo 33b/05 Filamentary Structures in NGC 1097 [Preview - JPEG: 400 x 570 pix - 275k] [Normal - JPEG: 800 x 1140 pix - 900k] [Full Res - JPEG: 1422 x 2026 pix - 2.6M] Caption: ESO PR Photo 33b/05: The left image shows the same central region as imaged in PR Photo 33a/05 but this time as seen in the J-Ks colour. It clearly shows the nucleus, the central spiral arms extending up to 1,300 light-years from the centre, and the star-forming ring. The right image shows the same but after a masking process has been applied to suppress the central stellar light of the galaxy. The central spiral arms are now seen as dark channels, some extending up to the star-forming ring. North is up and East is to the left. As can be seen in last year's image (see ESO PR Photo 35d/04), NGC 1097 has a very strong bar and a prominent star-forming ring inside it. Interior to the ring, a secondary bar crosses the nucleus almost perpendicular to the primary bar. The newly released NACO near-infrared images show in addition more than 300 star-forming regions, a factor four larger than previously known from Hubble Space Telescope images. These "HII regions" can be seen as white spots in ESO PR Photo 33a/05. At the centre of the ring, a moderate active nucleus is located. Details from the nucleus and its immediate surroundings are however outshone by the overwhelming stellar light of the galaxy seen as the bright diffuse emission all over the image. The astronomers therefore applied a masking technique that allowed them to suppress the stellar light (see ESO PR Photo 33b/05). This unveils a bright nucleus at the centre, but mostly a complex central network of filamentary structures spiralling down to the centre. "Our analysis of the VLT/NACO images of NGC 1097 shows that these filaments end up at the very centre of the galaxy", says co-author Juha Reunanen from ESO. "This network closely resembles those seen in computer models", adds co-worker Witold Maciejewski from the University of Oxford, UK. "The nuclear filaments revealed in the NACO images are the tracers of cold dust and gas being channelled towards the centre to eventually ignite the AGN." The astronomers also note that the curling of the spiral pattern in the innermost 300 light-years seem indeed to confirm the presence of a super-massive black hole in the centre of NGC 1097. Such a black hole in the centre of a galaxy causes the nuclear spiral to wind up as it approaches the centre, while in its absence the spiral would be unwinding as it moves closer to the centre. An image of NGC 1097 and its small companion, NGC 1097A, was taken in December 2004, in the presence of Chilean President Lagos with the VIMOS instrument on ESO's Very Large Telescope (VLT). It is available as ESO PR Photo 35d/04. More information This ESO Press Photo is based on research published in the October issue of Astronomical Journal, vol. 130, p. 1472 ("Feeding the Monster: The Nucleus of NGC 1097 at Subarcsecond Scales in the Infrared with the Very Large Telescope", by M. Almudena Prieto, Witold Maciejewski, and Juha Reunanen).

EarthLabs - Investigating Hurricanes: Earth's Meteorological Monsters

NASA Astrophysics Data System (ADS)

McDaris, J. R.; Dahlman, L.; Barstow, D.

2007-12-01

Earth science is one of the most important tools that the global community needs to address the pressing environmental, social, and economic issues of our time. While, at times considered a second-rate science at the high school level, it is currently undergoing a major revolution in the depth of content and pedagogical vitality. As part of this revolution, labs in Earth science courses need to shift their focus from cookbook-like activities with known outcomes to open-ended investigations that challenge students to think, explore and apply their learning. We need to establish a new model for Earth science as a rigorous lab science in policy, perception, and reality. As a concerted response to this need, five states, a coalition of scientists and educators, and an experienced curriculum team are creating a national model for a lab-based high school Earth science course named EarthLabs. This lab course will comply with the National Science Education Standards as well as the states' curriculum frameworks. The content will focus on Earth system science and environmental literacy. The lab experiences will feature a combination of field work, classroom experiments, and computer access to data and visualizations, and demonstrate the rigor and depth of a true lab course. The effort is being funded by NOAA's Environmental Literacy program. One of the prototype units of the course is Investigating Hurricanes. Hurricanes are phenomena which have tremendous impact on humanity and the resources we use. They are also the result of complex interacting Earth systems, making them perfect objects for rigorous investigation of many concepts commonly covered in Earth science courses, such as meteorology, climate, and global wind circulation. Students are able to use the same data sets, analysis tools, and research techniques that scientists employ in their research, yielding truly authentic learning opportunities. This month-long integrated unit uses hurricanes as the story line by which students investigate the different interactions involved in hurricane generation, steering, and intensification. Students analyze a variety of visualization resources looking for patterns in occurrence and to develop an understanding of hurricane structure. They download archived data about past hurricanes and produce temporal and spatial plots to discover patterns in hurricane life cycles. They investigate the relationship between hurricane wind speed and factors such as barometric pressure and sea surface temperature by conducting spreadsheet analyses on archived data. They also conduct hands-on laboratory experiments in order to understand the physical processes that underpin energy transfer in convection, condensation, and latent heat. These activities highlight Earth science as a vital, rich, invigorating course, employing state-of-the-art technologies and in-depth labs with high relevance for our daily lives and the future.

Transport and Dynamics in Toroidal Fusion Systems

DOE Office of Scientific and Technical Information (OSTI.GOV)

Sovinec, Carl

The study entitled, "Transport and Dynamics in Toroidal Fusion Systems," (TDTFS) applied analytical theory and numerical computation to investigate topics of importance to confining plasma, the fourth state of matter, with magnetic fields. A central focus of the work is how non-thermal components of the ion particle distribution affect the "sawtooth" collective oscillation in the core of the tokamak magnetic configuration. Previous experimental and analytical research had shown and described how the oscillation frequency decreases and amplitude increases, leading to "monster" or "giant" sawteeth, when the non-thermal component is increased by injecting particle beams or by exciting ions with imposedmore » electromagnetic waves. The TDTFS study applied numerical computation to self-consistently simulate the interaction between macroscopic collective plasma dynamics and the non-thermal particles. The modeling used the NIMROD code [Sovinec, Glasser, Gianakon, et al., J. Comput. Phys. 195, 355 (2004)] with the energetic component represented by simulation particles [Kim, Parker, Sovinec, and the NIMROD Team, Comput. Phys. Commun. 164, 448 (2004)]. The computations found decreasing growth rates for the instability that drives the oscillations, but they were ultimately limited from achieving experimentally relevant parameters due to computational practicalities. Nonetheless, this effort provided valuable lessons for integrated simulation of macroscopic plasma dynamics. It also motivated an investigation of the applicability of fluid-based modeling to the ion temperature gradient instability, leading to the journal publication [Schnack, Cheng, Barnes, and Parker, Phys. Plasmas 20, 062106 (2013)]. Apart from the tokamak-specific topics, the TDTFS study also addressed topics in the basic physics of magnetized plasma and in the dynamics of the reversed-field pinch (RFP) configuration. The basic physics work contributed to a study of two-fluid effects on interchange dynamics, where "two-fluid" refers to modeling independent dynamics of electron and ion species without full kinetic effects. In collaboration with scientist Ping Zhu, who received separate support, it was found that the rule-of-thumb criteria on stabilizing interchange has caveats that depend on the plasma density and temperature profiles. This work was published in [Zhu, Schnack, Ebrahimi, et al., Phys. Rev. Lett. 101, 085005 (2008)]. An investigation of general nonlinear relaxation with fluid models was partially supported by the TDTFS study and led to the publication [Khalzov, Ebrahimi, Schnack, and Mirnov, Phys. Plasmas 19, 012111 (2012)]. Work specific to the RFP included an investigation of interchange at large plasma pressure and support for applications [for example, Scheffel, Schnack, and Mirza, Nucl. Fusion 53, 113007 (2013)] of the DEBS code [Schnack, Barnes, Mikic, Harned, and Caramana, J. Comput. Phys. 70, 330 (1987)]. Finally, the principal investigator over most of the award period, Dalton Schnack, supervised a numerical study of modeling magnetic island suppression [Jenkins, Kruger, Hegna, Schnack, and Sovinec, Phys. Plasmas 17, 12502 (2010)].« less

When family drawings reveal vulnerabilities and resilience.

PubMed

Ireland, Rachel; Weisbart, Cindy; Dubowitz, Howard; Rowe, Jeffrey; Stein, Martin T

2009-10-01

Sonia's mother was concerned about her 9-year old daughter's aggression, defiant behavior, and distractibility. When she was 4-years, she kicked her bother and he lost a tooth as a result of the trauma. At this time, her pediatrician was concerned about hyperactivity, impulsivity, and defiance of authority and recommended a psychological evaluation. Sonia's father refused an evaluation and responded by physically abusing his wife while demanding a transfer to a new physician. Sonia's mother left her husband at this time and moved away with Sonia. Spousal abuse occurred frequently before the separation, and Sonia may have been physically abused as well.Currently, Sonia is in third grade where she is underperforming in many areas. She enjoys drawing and reading, but struggles to sit quietly and stay on task. Her teacher reports frequent vocal and physical disruptions. Homework takes an inordinate amount of time to complete. She does not have a sustained friendship; her mother feels that this is because other kids do not like being bossed by Sonia. Her mother is concerned about Sonia's behavior especially the unremorseful disruptive behavior toward her younger brother and grandmother.Sonia was born after an uneventful full-term pregnancy without evidence of maternal smoking, drugs, alcohol, or medications. Motor and social developmental milestones were achieved at the appropriate time. Language milestones were achieved early; her mother recalls that Sonia learned to read at the age of 3 years.Sonia's medical history is significant for obesity, seasonal allergic rhinitis, and delayed sleep onset with prolonged awakenings associated with nightmares. Her mother reports that Sonia "worries about everything," including thoughts that her brother will turn into a monster. When an argument occurs at home, she "gets scared," bites her nails, and cries. Sonia currently lives with her mother, 2 younger brothers, step-father, and grandparents. Family history is significant for drug abuse by her father and mental illness in the father's family.While conducting an interview with her mother, Sonia was asked to draw a picture of her family. Instead, she illustrated a book detailing her past experience in words accompanying each drawing. She described how she watched her father physically abuse her mother and her persistent fear of danger when conflict occurred at home. Although spelling was poor, her vocabulary, sequencing, and illustrations demonstrated above age-level skills for written expression and drawing. Examples of the writing that accompanied the drawings include: "I hate when my parents fight. I get scared and feel sick to my tummy like I want to throw up. I just hate that feeling!" "My mom told me she had a 'boyfriend.' These words were the most horrible I ever heard. Soon a nightmare began. Nightmares make me very, very scared."

Fires Rage Near Malibu, California

NASA Image and Video Library

2017-12-08

According to the NBCnews.com, Southern California firefighters were battling a growing, brush-fueled wildfire early Friday that had reached the beach in Ventura County and was pushing toward the upscale city of Malibu, officials said. Dubbed the Springs Fire, this "monster" of a wildfire has been made worse by howling Santa Ana winds and unusually dry vegetation. As of 2 am local time in California on Friday the 3rd, it was within "seven or eight miles" of Malibu, Ventura County Fire Department spokesman Bill Nash said. Weather conditions are not cooperating in the containment of this fire. The Weather Channel has predicted dry winds from offshore that will bring gusts of 40 to 50 miles per hour to the Southern California region on Friday the 3rd which could easily spread the fire. A complication to the winds is the extremely dry plant life left from a season in which only about five inches of rain fell in the area. The Springs Fire grew to 10,000 acres and was ten percent contained as of early Friday morning, according to the California Department of Forestry and Fire Prevention. Evacuations took place Thursday, and as of Friday morning 15 homes had been damaged. More than 2,000 homes and 100 commercial properties were under threat from the fire and those numbers could grow with weather conditions today (May 3). Currently the fire is burning in a rural area outside of Malibu, but it doesn't have to go very far to get to some expensive homes and more populated areas. It's current direction has it burning down the mountainside toward Malibu. Firefighters expect to receive help from tankers and helicopters in the air Friday morning, according to a release from the Ventura County Fire Department. The cause of the fire remained under investigation Friday. There had been no lightning or other natural fire-starting phenomenon in the area when the blaze began, Nash said. This natural-color satellite image was collected by the Moderate Resolution Imaging Spectroradiometer (MODIS) aboard the Aqua satellite on May 02, 2013. Actively burning areas, detected by MODIS’s thermal bands, are outlined in red. NASA image courtesy Jeff Schmaltz LANCE/EOSDIS MODIS Rapid Response Team, GSFC. Caption by Lynn Jenner with information from NBCnews.com NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

Molecular Characterization of a Lizard Adenovirus Reveals the First Atadenovirus with Two Fiber Genes and the First Adenovirus with Either One Short or Three Long Fibers per Penton

PubMed Central

Pénzes, Judit J.; Menéndez-Conejero, Rosa; Condezo, Gabriela N.; Ball, Inna; Papp, Tibor; Doszpoly, Andor; Paradela, Alberto; Pérez-Berná, Ana J.; López-Sanz, María; Nguyen, Thanh H.; van Raaij, Mark J.; Marschang, Rachel E.; Harrach, Balázs; Benkő, Mária

2014-01-01

ABSTRACT Although adenoviruses (AdVs) have been found in a wide variety of reptiles, including numerous squamate species, turtles, and crocodiles, the number of reptilian adenovirus isolates is still scarce. The only fully sequenced reptilian adenovirus, snake adenovirus 1 (SnAdV-1), belongs to the Atadenovirus genus. Recently, two new atadenoviruses were isolated from a captive Gila monster (Heloderma suspectum) and Mexican beaded lizards (Heloderma horridum). Here we report the full genomic and proteomic characterization of the latter, designated lizard adenovirus 2 (LAdV-2). The double-stranded DNA (dsDNA) genome of LAdV-2 is 32,965 bp long, with an average G+C content of 44.16%. The overall arrangement and gene content of the LAdV-2 genome were largely concordant with those in other atadenoviruses, except for four novel open reading frames (ORFs) at the right end of the genome. Phylogeny reconstructions and plesiomorphic traits shared with SnAdV-1 further supported the assignment of LAdV-2 to the Atadenovirus genus. Surprisingly, two fiber genes were found for the first time in an atadenovirus. After optimizing the production of LAdV-2 in cell culture, we determined the protein compositions of the virions. The two fiber genes produce two fiber proteins of different sizes that are incorporated into the viral particles. Interestingly, the two different fiber proteins assemble as either one short or three long fiber projections per vertex. Stoichiometry estimations indicate that the long fiber triplet is present at only one or two vertices per virion. Neither triple fibers nor a mixed number of fibers per vertex had previously been reported for adenoviruses or any other virus. IMPORTANCE Here we show that a lizard adenovirus, LAdV-2, has a penton architecture never observed before. LAdV-2 expresses two fiber proteins—one short and one long. In the virion, most vertices have one short fiber, but a few of them have three long fibers attached to the same penton base. This observation raises new intriguing questions on virus structure. How can the triple fiber attach to a pentameric vertex? What determines the number and location of each vertex type in the icosahedral particle? Since fibers are responsible for primary attachment to the host, this novel architecture also suggests a novel mode of cell entry for LAdV-2. Adenoviruses have a recognized potential in nanobiomedicine, but only a few of the more than 200 types found so far in nature have been characterized in detail. Exploring the taxonomic wealth of adenoviruses should improve our chances to successfully use them as therapeutic tools. PMID:25056898

Survivor Interviews from the Sept. 29, 2009 tsunami on Samoa and American Samoa

NASA Astrophysics Data System (ADS)

Richmond, B. M.; Dudley, W. C.; Buckley, M. L.; Jaffe, B. E.; Fanolua, S.; Chan Kau, M.

2009-12-01

Thirty-one video interviews were carried out on the islands of Tutuila, American Samoa and Upolu, Samoa with survivors of, and responders to, the September 29, 2009 tsunami event. Those interviewed included local residents caught by the waves while attempting to flee to higher ground, those who intentionally ran into the water to save others, individuals who recognized the potential tsunami hazard due to the severity of the earthquake and attempted to warn others, first-responders, aid workers, tourism managers, and others. The frank, often emotional, responses provide unfiltered insight into the level of preparedness of local residents, level of training of first responders, and challenges faced by aid workers. Among the important observations voiced by interviewees were: (1) recent tsunami education briefings and school drills were critical in preventing greater loss of life; (2) those who had not received training about the tsunami hazard were unaware that a tsunami could follow a strong earthquake; (3) first responders were not adequately trained or prepared for the specific impacts of a tsunami; (4) initial medical procedures did not adequately address the levels of bacterial contamination; and (5) survivors, first responders and aid workers suffer from post traumatic stress disorder as a result of the event and its aftermath. Valuable scientific data can also be gained from first-hand accounts. Several interviews describe waves “bending,” “funneling,” and one spoke of the waves coming together as a “monster that jumped up from the channel spitting boulders.” In the village of Fagasa on the north coast of Tutuila, American Samoa, the assumed transport direction of large boulders by scientists was dramatically revised based on first-hand accounts of the original position of the boulders. The single most common message was that hazard education played a key role in saving lives in both Samoa and American Samoa. It is critically important to understand the reaction and response of individuals from different cultures to tsunami events in order to better design mitigation, education, response and recovery programs that best fit local communities. It is hoped that the analysis of these and other post-tsunami interviews will be used in that effort. Interviews were carried out in high-definition (1080i) video so as to capture the emotional impact of first-person, eye-witness accounts. Interviews will be translated in Samoa and English and transcribed with video time-code thus making them suitable for quality media production for use in local, regional, and international tsunami education programs. Additional observations gleaned from the interviews, as well as preliminary analysis based on specific location and demographic will also be presented.

A Tornado on the Sun

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2015-10-01

On 7 November, 2012 at 08:00 UT, an enormous tornado of plasma rose from the surface of the Sun. It twisted around and around, climbing over the span of 10 hours to a height of 50 megameters roughly four times the diameter of the Earth! Eventually, this monster tornado became unstable and erupted violently as a coronal mass ejection (CME).Now, a team of researchers has analyzed this event in an effort to better understand the evolution of giant solar tornadoes like this one.Oscillating AxisIn this study, led by Irakli Mghebrishvili and Teimuraz Zaqarashvili of Ilia State University (Georgia), images taken by the Solar Dynamics Observatorys Atmospheric Imaging Assembly were used to track the tornados motion as it grew, along with a prominence, on the solar surface.The team found that as the tornado evolved, there were several intervals during which it moved back and forth quasi-periodically. The authors think these oscillations were due to one of two effects when the tornado was at a steady height: either twisted threads of the tornado were rotating around each other, or a magnetic effect known as kink waves caused the tornado to sway back and forth.Determining which effect was at work is an important subject of future research, because the structure and magnetic configuration of the tornado has implications for the next stage of this tornados evolution: eruption.Eruption from InstabilitySDO/AIA 3-channel composite image of the tornado an hour before it erupted in a CME. A coronal cavity has opened above the tornado; the top of the cavity is indicated by an arrow. [NASA/SDO/AIA; Mghebrishvili et al. 2015]Thirty hours after its formation, the tornado (and the solar prominence associated with it) erupted as a CME, releasing enormous amounts of energy. In the images from shortly before that moment, the authors observed a cavity open in the solar corona above the tornado. This cavity gradually expanded and rose above the solar limb until the tornado and prominence erupted into the space that had been opened.Based on these observations, the authors hypothesize that the eruption could be explained using the following model:A tornado and a related solar prominence forms.Magnetic field lines within it are gradually twisted by the tornados rotation, until the tornado becomes unstable to the kink instability (a magnetic instability).The tornado then destabilizes the entire prominence, which expands upwards and erupts into a CME through something known as the magnetic breakout model.If solar tornadoes such as this one generally cause instabilities of prominences, they could be used to predict when a related CME is about to happen providing important information for space weather predictions.CitationIrakli Mghebrishvili et al 2015 ApJ 810 89. doi:10.1088/0004-637X/810/2/89

Chandra Data Reveal Rapidly Whirling Black Holes

NASA Astrophysics Data System (ADS)

2008-01-01

A new study using results from NASA's Chandra X-ray Observatory provides one of the best pieces of evidence yet that many supermassive black holes are spinning extremely rapidly. The whirling of these giant black holes drives powerful jets that pump huge amounts of energy into their environment and affects galaxy growth. A team of scientists compared leading theories of jets produced by rotating supermassive black holes with Chandra data. A sampling of nine giant galaxies that exhibit large disturbances in their gaseous atmospheres showed that the central black holes in these galaxies must be spinning at near their maximum rates. People Who Read This Also Read... NASA’s Swift Satellite Catches First Supernova in The Act of Exploding Black Holes Have Simple Feeding Habits Jet Power and Black Hole Assortment Revealed in New Chandra Image Erratic Black Hole Regulates Itself "We think these monster black holes are spinning close to the limit set by Einstein's theory of relativity, which means that they can drag material around them at close to the speed of light," said Rodrigo Nemmen, a visiting graduate student at Penn State University, and lead author of a paper on the new results presented at American Astronomical Society in Austin, Texas. The research reinforces other, less direct methods previously used which have indicated that some stellar and supermassive black holes are spinning rapidly. According to Einstein's theory, a rapidly spinning black hole makes space itself rotate. This effect, coupled with gas spiraling toward the black hole, can produce a rotating, tightly wound vertical tower of magnetic field that flings a large fraction of the inflowing gas away from the vicinity of the black hole in an energetic, high-speed jet. Computer simulations by other authors have suggested that black holes may acquire their rapid spins when galaxies merge, and through the accretion of gas from their surroundings. "Extremely fast spin might be very common for large black holes," said co-investigator Richard Bower of Durham University. "This might help us explain the source of these incredible jets that we see stretching for enormous distances across space." One significant connection consequence of powerful, black-hole jets in galaxies in the centers of galaxy clusters is that they can pump enormous amounts of energy into their environments, and heat the gas around them. This heating prevents the gas from cooling, and affects the rate at which new stars form, thereby limiting the size of the central galaxy. Understanding the details of this fundamental feedback loop between supermassive black holes and the formation of the most massive galaxies remains an important goal in astrophysics. NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the agency's Science Mission Directorate. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center in Cambridge, Mass.

'A WONDERFULL MONSTER BORNE IN GERMANY': HAIRY GIRLS IN MEDIEVAL AND EARLY MODERN GERMAN BOOK, COURT AND PERFORMANCE CULTURE.

PubMed

Katritzky, M A

2014-09-24

Human hirsuteness, or pathological hair growth, can be symptomatic of various conditions, including genetic mutation or inheritance, and some cancers and hormonal disturbances. Modern investigations into hirsuteness were initiated by nineteenth-century German physicians. Most early modern European cases of hypertrichosis (genetically determined all-over body and facial hair) involve German-speaking parentage or patronage, and are documented in German print culture. Through the Wild Man tradition, modern historians routinely link early modern reception of historical hypertrichosis cases to issues of ethnicity without, however, recognising early modern awareness of links between temporary hirsuteness and the pathological nexus of starvation and anorexia. Here, four cases of hirsute females are reconsidered with reference to this medical perspective, and to texts and images uncovered by my current research at the Herzog August Library and German archives. One concerns an Italian girl taken to Prague in 1355 by the Holy Roman Empress, Anna von Schweidnitz. Another focuses on Madeleine and Antonietta Gonzalez, daughters of the 'Wild Man' of Tenerife, documented at German courts in the 1580s. The third and fourth cases consider the medieval bearded Sankt Kümmernis (also known as St Wilgefortis or St Uncumber), and the seventeenth-century Bavarian fairground performer Barbara Urslerin. Krankhafter menschlicher Hirsutismus kann aufgrund unterschiedlicher Ursachen auftreten, zu denen u.a. genetische Veländerungen und Vererbung, verschiedene Krebserkrankungen und hormonelle Störungen gehören. Die moderne Hirsutismus-Forschung ist im 19. Jh. von deutschen Forschern initiiert worden. Die meisten europäischen frühneuzeitlichen Erscheinungen von Hypertrichose (dem genetisch bedingten Haarwuchs am gesamten Körper und im Gesicht) gehen auf deutschsprachige Eltern oder Förderer zurück und sind in Deutschland in den Druck gelangt. Bei Untersuchungen des Motivs des Wilden Mannes zieht die aktuelle geschichtswissenschaftliche Forschung in der Regel Verbindungslinien zwischen der frühneuzeitlichen Wahrnehmung von Hypertrichose-Fällen und Fragen der Ethnizität, ohne jedoch zu beachten, dass in der Frühen Neuzeit die Verbindung zwischen temporärem Hirsutismus und der krankhaften Verknüpfung von Unterernährung und Anorexie bekannt war. Im vorliegenden Beitragwerden vier Fälle von an Hirsutismus erkrankten Frauen neu analysiert, unter Einbezug dieser medizinischen Perspektive und unter Beachtung von Texten und Abbildungen, die meine jüngsten Forschungen in der Herzog August Bibliothek und an deutschen Archiven ans Licht gefördert haben. Die hier betrachteten Fälle betreffen ein italienisches Mädchen, das 1355 von Anna von Schweidnitz, Kaiserin des Hl. Römischen Reichs, nach Prag gebracht wurde; Madeleine und Antonietta Gonzalez, die Töchter des 'Wilden Manns' von Teneriffa, die in den 1580er Jahren an deutschen Höfen bezeugt sind; die bärtige Sankt Kümmernis (Wilgefortis), und die bayerische Jahrmarktkünstlerin Barbara Urslerin.

‘A Wonderfull Monster Borne in Germany’: Hairy Girls in Medieval and Early Modern German Book, Court and Performance Culture*

PubMed Central

Katritzky, MA

2014-01-01

Human hirsuteness, or pathological hair growth, can be symptomatic of various conditions, including genetic mutation or inheritance, and some cancers and hormonal disturbances. Modern investigations into hirsuteness were initiated by nineteenth-century German physicians. Most early modern European cases of hypertrichosis (genetically determined all-over body and facial hair) involve German-speaking parentage or patronage, and are documented in German print culture. Through the Wild Man tradition, modern historians routinely link early modern reception of historical hypertrichosis cases to issues of ethnicity without, however, recognising early modern awareness of links between temporary hirsuteness and the pathological nexus of starvation and anorexia. Here, four cases of hirsute females are reconsidered with reference to this medical perspective, and to texts and images uncovered by my current research at the Herzog August Library and German archives. One concerns an Italian girl taken to Prague in 1355 by the Holy Roman Empress, Anna von Schweidnitz. Another focuses on Madeleine and Antonietta Gonzalez, daughters of the ‘Wild Man’ of Tenerife, documented at German courts in the 1580s. The third and fourth cases consider the medieval bearded Sankt Kümmernis (also known as St Wilgefortis or St Uncumber), and the seventeenth-century Bavarian fairground performer Barbara Urslerin. Krankhafter menschlicher Hirsutismus kann aufgrund unterschiedlicher Ursachen auftreten, zu denen u.a. genetische Veränderungen und Vererbung, verschiedene Krebserkrankungen und hormonelle Störungen gehören. Die moderne Hirsutismus-Forschung ist im 19. Jh. von deutschen Forschern initiiert worden. Die meisten europäischen frühneuzeitlichen Erscheinungen von Hypertrichose (dem genetisch bedingten Haarwuchs am gesamten Körper und im Gesicht) gehen auf deutschsprachige Eltern oder Förderer zurück und sind in Deutschland in den Druck gelangt. Bei Untersuchungen des Motivs des Wilden Mannes zieht die aktuelle geschichtswissenschaftliche Forschung in der Regel Verbindungslinien zwischen der frühneuzeitlichen Wahrnehmung von Hypertrichose-Fällen und Fragen der Ethnizität, ohne jedoch zu beachten, dass in der Frühen Neuzeit die Verbindung zwischen temporärem Hirsutismus und der krankhaften Verknüpfung von Unterernährung und Anorexie bekannt war. Im vorliegenden Beitrag werden vier Fälle von an Hirsutismus erkrankten Frauen neu analysiert, unter Einbezug dieser medizinischen Perspektive und unter Beachtung von Texten und Abbildungen, die meine jüngsten Forschungen in der Herzog August Bibliothek und an deutschen Archiven ans Licht gefördert haben. Die hier betrachteten Fälle betreffen ein italienisches Mädchen, das 1355 von Anna von Schweidnitz, Kaiserin des Hl. Römischen Reichs, nach Prag gebracht wurde; Madeleine und Antonietta Gonzalez, die Töchter des ‘Wilden Manns’ von Teneriffa, die in den 1580er Jahren an deutschen Höfen bezeugt sind; die bärtige Sankt Kümmernis (Wilgefortis), und die bayerische Jahrmarktkünstlerin Barbara Urslerin. PMID:25598545

Strong Winds over the Keel

NASA Astrophysics Data System (ADS)

2009-02-01

The latest ESO image reveals amazing detail in the intricate structures of one of the largest and brightest nebulae in the sky, the Carina Nebula (NGC 3372), where strong winds and powerful radiation from an armada of massive stars are creating havoc in the large cloud of dust and gas from which the stars were born. ESO PR Photo 05a/09 The Carina Nebula ESO PR Video 05a/09 Pan over the Carina Nebula ESO PR Video 05b/09 Carina Nebula Zoom-in The large and beautiful image displays the full variety of this impressive skyscape, spattered with clusters of young stars, large nebulae of dust and gas, dust pillars, globules, and adorned by one of the Universe's most impressive binary stars. It was produced by combining exposures through six different filters from the Wide Field Imager (WFI), attached to the 2.2 m ESO/MPG telescope at ESO's La Silla Observatory, in Chile. The Carina Nebula is located about 7500 light-years away in the constellation of the same name (Carina; the Keel). Spanning about 100 light-years, it is four times larger than the famous Orion Nebula and far brighter. It is an intensive star-forming region with dark lanes of cool dust splitting up the glowing nebula gas that surrounds its many clusters of stars. The glow of the Carina Nebula comes mainly from hot hydrogen basking in the strong radiation of monster baby stars. The interaction between the hydrogen and the ultraviolet light results in its characteristic red and purple colour. The immense nebula contains over a dozen stars with at least 50 to 100 times the mass of our Sun. Such stars have a very short lifespan, a few million years at most, the blink of an eye compared with the Sun's expected lifetime of ten billion years. One of the Universe's most impressive stars, Eta Carinae, is found in the nebula. It is one of the most massive stars in our Milky Way, over 100 times the mass of the Sun and about four million times brighter, making it the most luminous star known. Eta Carinae is highly unstable, and prone to violent outbursts, most notably the false supernova event in 1842. For just a few years, Eta Carinae became the second brightest star in the night sky and produced almost as much visible light as a supernova explosion (the usual death throes of a massive star), but it survived. Eta Carinae is also thought to have a hot companion that orbits around it in 5.54 years, in an elliptical orbit. Both stars have strong winds, which collide, leading to interesting phenomena. In mid-January 2009, the companion was at its closest distance to Eta Carinae. This event, which may provide a unique insight into the wind structure of the massive stars, has been followed by a flotilla of instruments on several of ESO's telescopes.

[Peter Simon Pallas (1741-1811). The structure of the organic world and the notion of species. On the bicentenary of the death of P. S. Pallas].

PubMed

Bednarczyk, Andrzej

2010-01-01

An attempt has been made in the current paper to dispel two myths concerning Peter Simon Pallas, myths which have led historians of biology to distort the picture of some of the general biological ideas developed by that eminent naturalist of the Age of Enlightenment. The first point dealt with in the paper involves the myth that Pallas had allegedly drafted a 'tree of life' diagram, one of the many graphic representations of this kind to appear in later times, illustrating the structure of the organic world. The tree, of which Pallas merely left a short description (but not a depiction), took--in the articles of authors who wrote about it--a variety of graphic forms (largely dependent on the authors' pictorial inventiveness), with all the authors assuring the readers that they illustrated their reasoning with the help of Pallas's tree of life, but never mentioning that it was they themseIves who had drawn it. The current paper presents a juxtaposition of a number of such diagrams, drawn by different authors: the great diversity of the diagrams is sufficient proof that the existence of one, original 'Pallas tree' is just a myth. Another aspect of the myth has to do with the view that the tree supposedly illustrated phylogenetic dependencies - in fact, Pallas described affinity relationships between groups in the animal world. The present paper investigates how the 'tree of life' myth has developed, and reveals the mechanism that has most likely led to the myth being perpetuated in writings on the history of biology. The second issue discussed in the current paper relates to the myth of how Pallas's general views on biology allegedly evolved. The naturalist was supposed to have moved from transformism (characteristic of early stages of his work) to the idea of the immutability of species, formed in the period of his full scientific maturity. The current paper proves, inter alia on the basis of little known and not easily accessible writings by the scholar, that Pallas espoused the Age of Enlightenment's deism, an important element of which was the idea of the immutability of species, to which Pallas steadfastly subscribed. On the other hand, the analysis presented in the paper has revealed that Pallas seemed to consider the problem of species on two planes: that of free-roaming wild species, which remained absolutely immutable, and that of domesticated species, which did manifest some mutability, largely sustained by human effort but never transgressing species boundaries. It was also--and only--under domestication that monsters appeared. Pallas did contemplate, not without much hesitation, teratogenesis as a possible mechanism behind speciation, but--given the lethal character of monstrous modifications--he did not treat it as the real mechanism of speciation.

[French validation of the Revised Paranormal Belief Scale].

PubMed

Bouvet, R; Djeriouat, H; Goutaudier, N; Py, J; Chabrol, H

2014-09-01

For the last decades, many researchers have focused on paranormal beliefs. Beliefs in the existence of paranormal phenomena would be common and studies conducted in westernized countries have highlighted a high prevalence of individuals believing in the existence of such phenomena. Tobacyk and Milford (1984) developed the Revised Paranormal Belief Scale (RPBS) for assessing beliefs in paranormal phenomena. This 26-item self-reported questionnaire, measuring beliefs in phenomena such as witchcraft or superstition, is one of the most widely used questionnaires to assess such beliefs. While studies focusing on paranormal beliefs tend to develop, there is no French self-report instrument to assess this construct. Researchers have tried to identify specific variables that might be linked to such beliefs, and some have focused on personalities of individuals who believe in the paranormal. Schizotypy has been reported to be significantly and positively correlated with paranormal beliefs. The aim of this study was a) to validate the French version of the RPBS and b) to explore the relationship between Schizotypal Personality Disorder traits and paranormal beliefs. After being recruited using the Internet and social networks (e.g. facebook), a sample of 313 participants (mean [SD] age=31.12 [11.62]; range 18-58years) completed the Schizotypal Personality Questionnaire (SPQ-B), assessing Schizotypal Personality Disorder traits and the Revised Paranormal Belief Scale assessing paranormal beliefs. Confirmatory factor analysis (CFA) was conducted to test the proposed 7-factor structure of the RPB developed by Tobacyk. Several adjustment indices were used to evaluate the model. As the first model did not fit the original one, others models were tested. Our findings indicated that a seven-factor solution, excluding 2 items, best described the item structure: (1) spiritualism, (2) superstition, (3) witchcraft, (4) precognition, (5) traditional religious belief, (6) psi, (7) and extraordinary life forms. Relationships between paranormal beliefs and Schizotypal Personality Disorder traits were also explored. Correlations between some subscales of the SPQ-B and some dimensions of the RPBS were found. The "cognition-perception" subscale was strongly correlated with the "witchcraft", "spirituality", "precognition" and "psi" subscales. Nevertheless, this subscale was lightly correlated with the "traditional religious belief" and "extraordinary life forms" dimensions. No correlation was found between the others dimensions of schizotypy as "disorganized" and "interpersonal" and dimensions of paranormal beliefs. The initial model developed by Tobacyk and Milford did not fit the data from the French population. The low internal consistencies regarding both superstition and extraordinary life forms dimensions highlighted some cultural differences that have to be acknowledged. This result emphasizes that beliefs in some extraordinary life forms as Loch Ness monster are not an important dimension to take into account in a French population. Our findings also indicate that the RPBS is a valid and reliable instrument for assessing paranormal beliefs in a French population. Our findings also highlight that such beliefs are associated with Schizotypal Personality Disorder traits. Developing research on the association between Schizotypal Personality Disorder traits and such beliefs appears of prime importance. Future studies focusing on features associated with paranormal beliefs are also warranted. Copyright © 2014 L’Encéphale, Paris. Published by Elsevier Masson SAS. All rights reserved.

Seeking care as a system.

PubMed

Berwick, Donald M; Luo, Eva

2010-01-01

Kim, aged 3 years, lies asleep, waiting for a miracle. Outside her room, the nurses on the night shift pad softly through the half-lighted corridors, stopping to count breaths, take pulses, or check the intravenous pumps. In the morning, Kim will have her heart fixed. She will be medicated and wheeled into the operating suite. Machines will take on the functions of her body: breathing and circulating blood. The surgeons will place a small patch over a hole within her heart, closing off a shunt between her ventricles that would, if left open, slowly kill her. Kim will be fine if the decision to operate on her was correct; if the surgeon is competent; if that competent surgeon happens to be trained to deal with the particular anatomic wrinkle that is hidden inside Kim's heart; if the blood bank cross-matched her blood accurately and delivered it to the right place; if the blood gas analysis machine works properly and on time; if the suture does not snap; if the plastic tubing of the heart-lung machine does not suddenly spring loose; if the recovery room nurses know that she is allergic to penicillin; if the "oxygen" and "nitrogen" lines in the anesthesia machine have not been reversed by mistake; if the sterilizer temperature gauge is calibrated so that the instruments are in fact sterile; if the pharmacy does not mix up two labels; and if when the surgeon says urgently, "Clamp, right now," there is a clamp on the tray. If all goes well, if ten thousand "ifs" go well, then Kim may sing her grandchildren to sleep some day. If not, she will be dead by noon tomorrow. If Kim were an astronaut, strapped into her seat at the top of some throbbing rocket, the crowd assembled would hold their breath in the morning Florida sun. "How can it possibly work?" they would whisper. "How many parts are there in that machine? A million? What if one fails? My toaster fails. Please let it all work right." The machine would bellow smoke, the gantry fall away, and slowly the monster would rise, Kim on top. If it worked, they would cheer. "A miracle," they would shout, in awe that the millions of tiny lines of effort, the millions of tiny lines of cause and effect, from job shops in Ohio and laboratories in Pasadena, criss-crossing through time and space, could converge so magnificently in a massive, gleaming rocket launched exactly right. Perfect. If it failed, they would cry. So would the rocket's makers, who had done their very best. No one wanted it to end this way. Poor Kim. What was the trouble? What went wrong? Why? The lines of cause will converge around Kim in the morning as she wheels toward the operating room. Thousands upon thousands of elements weaving a basket to hold her safely, all hope. No crowd holds its breath tonight; but wouldn't they if they knew? From: Berwick DM. Controlling variation in health care: a consultation from Walter Shewhart. Medical Care 1991; 29: 1212-1225.

Celestial Fireworks from Dying Stars

NASA Astrophysics Data System (ADS)

2011-04-01

This image of the nebula NGC 3582, which was captured by the Wide Field Imager on the MPG/ESO 2.2-metre telescope at ESO's La Silla Observatory in Chile, shows giant loops of gas bearing a striking resemblance to solar prominences. These loops are thought to have been ejected by dying stars, but new stars are also being born within this stellar nursery. These energetic youngsters emit intense ultraviolet radiation that makes the gas in the nebula glow, producing the fiery display shown here. NGC 3582 is part of a large star-forming region in the Milky Way, called RCW 57. It lies close to the central plane of the Milky Way in the southern constellation of Carina (The Keel of Jason's ship, the Argo). John Herschel first saw this complex region of glowing gas and dark dust clouds in 1834, during his stay in South Africa. Some of the stars forming in regions like NGC 3582 are much heavier than the Sun. These monster stars emit energy at prodigious rates and have very short lives that end in explosions as supernovae. The material ejected from these dramatic events creates bubbles in the surrounding gas and dust. This is the probable cause of the loops visible in this picture. This image was taken through multiple filters. From the Wide Field Imager, data taken through a red filter are shown in green and red, and data taken through a filter that isolates the red glow characteristic of hydrogen are also shown in red. Additional infrared data from the Digitized Sky Survey are shown in blue. The image was processed by ESO using the observational data identified by Joe DePasquale, from the United States [1], who participated in ESO's Hidden Treasures 2010 astrophotography competition [2]. The competition was organised by ESO in October-November 2010, for everyone who enjoys making beautiful images of the night sky using astronomical data obtained using professional telescopes. Notes [1] Joe searched through ESO's archive and identified datasets that he used to compose his image of NGC 3582, which was the tenth highest ranked entry in the competition, out of almost 100 entries. His original work can be seen here. [2] ESO's Hidden Treasures 2010 competition gave amateur astronomers the opportunity to search through ESO's vast archives of astronomical data, hoping to find a well-hidden gem that needed polishing by the entrants. To find out more about Hidden Treasures, visit http://www.eso.org/public/outreach/hiddentreasures/. More information ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 15 countries: Austria, Belgium, Brazil, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

NGC 4945: The Milky Way's not-so-distant Cousin

NASA Astrophysics Data System (ADS)

2009-09-01

ESO has released a striking new image of a nearby galaxy that many astronomers think closely resembles our own Milky Way. Though the galaxy is seen edge-on, observations of NGC 4945 suggest that this hive of stars is a spiral galaxy much like our own, with swirling, luminous arms and a bar-shaped central region. These resemblances aside, NGC 4945 has a brighter centre that likely harbours a supermassive black hole, which is devouring reams of matter and blasting energy out into space. As NGC 4945 is only about 13 million light-years away in the constellation of Centaurus (the Centaur), a modest telescope is sufficient for skygazers to spot this remarkable galaxy. NGC 4945's designation comes from its entry number in the New General Catalogue compiled by the Danish-Irish astronomer John Louis Emil Dreyer in the 1880s. James Dunlop, a Scottish astronomer, is credited with originally discovering NGC 4945 in 1826 from Australia. Today's new portrait of NGC 4945 comes courtesy of the Wide Field Imager (WFI) instrument at the 2.2-metre MPG/ESO telescope at the La Silla Observatory in Chile. NGC 4945 appears cigar-shaped from our perspective on Earth, but the galaxy is actually a disc many times wider than it is thick, with bands of stars and glowing gas spiralling around its centre. With the use of special optical filters to isolate the colour of light emitted by heated gases such as hydrogen, the image displays sharp contrasts in NGC 4945 that indicate areas of star formation. Other observations have revealed that NGC 4945 has an active galactic nucleus, meaning its central bulge emits far more energy than calmer galaxies like the Milky Way. Scientists classify NGC 4945 as a Seyfert galaxy after the American astronomer Carl K. Seyfert, who wrote a study in 1943 describing the odd light signatures emanating from some galactic cores. Since then, astronomers have come to suspect that supermassive black holes cause the turmoil in the centre of Seyfert galaxies. Black holes gravitationally draw gas and dust into them, accelerating and heating this attracted matter until it emits high-energy radiation, including X-rays and ultraviolet light. Most large, spiral galaxies, including the Milky Way, host a black hole in their centres, though many of these dark monsters no longer actively "feed" at this stage in galactic development. More information ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Surface Curvature in Island Groups and Discontinuous Cratonic Structures

NASA Astrophysics Data System (ADS)

McDowell, M. S.

2002-05-01

The Canadian Archipelago includes eight major islands and a host of smaller ones. They are separated by water bodies, of varying widths attributable to glacial activity and ocean currents. Land form varies from relatively rugged mountains (~2000 m) in eastern, glacial, islands, to low lying western, similar to the continental topography adjacent. The Arctic region is thought to have been low average elevation before the Pleistocene. To a picture puzzler, it all looks like it fit together. Experimentally cutting apart the islands from large scale maps shows that the rough edges match fairly well. However, when those independent pieces are sutured together, without restraint, as in free air, the fit is far better. Far more importantly, they consistently form a noticeably concave surface. This tendency is not at all apparent in flat surface or computer screen manipulation; the pieces need to be "hand joined" or on a molded surface to allow the assembly to freely form as it will. Fitting together the coastlines above 60 \\deg north, from 120 \\deg west to 45 \\deg east, and comparing the resulting contracted area to the original, obtains an 8 percent area reduction. The curvature "humps" a trial planar section of 15 cms by 1.6 cm, a substantial difference in the radius of curvature. If you rashly suggest applying that formula globally, the resulting sphere would have a surface area of 4.7 x108,(down from 5 x108), and therefore radius of 6117 km, down from 6400, which is a rather preposterous conclusion. As nobody would believe it, I tested the idea elsewhere. The Huronian succession of six named cratons is adjacent on the south. I cut this map apart, too, and fit it together, once again getting a curvature, this time more pronounced. I am trying it with the Indonesian Archipelago, although this area has volcanic complications, and with Precambrian Basins in western Australia and Nimibia, Africa. Indications are - an essentially similar pattern of fit, but non uniform distance separations, perhaps related to geologic time scale. What could this mean? 1) Two-dimensional expansion of an original Precambrian craton can be justified as rupture in some non explosive way (apparently not volcanic or quake action) with resulting cracks subsequently filled in from below. The cause of the initial cracking is problematic - consider an eggshell: a good whack on the outside, or a good chick on the inside, could make it happen. But 2) the tightened arc? The propensity to "curl up"? Is there something freaky about connecting flat map projections to make this happen, or has it really been there all along and we never realized it? If this is applied in reverse, curvature flattening further with time, the significance could be interesting. For idle speculation, the Atlantic mid-ocean ridge is calculated opening at 3cms/year. That's 3 km in 100,000 years. At that rate it would have taken 2.2 x 109 to open the Canadian archipelago this far. Which puts it almost into the Archean, matching Slave Province, not Wopmay, associated with the Huronian. So what WAS the early sea floor spreading rate? Monster speculations. Scientific research has created a fortress of opinion on Archean land masses and how they grew. This study proposes a phenomenon that has the advantage of measurability, one we can literally get our hands on, in our effort to know.

An Active Black Hole in a Compact Dwarf

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2016-05-01

A new type of galaxy has just been added to the galaxy zoo: a small, compact, and old elliptical galaxy that shows signs of a monster black hole actively accreting material in its center. What can this unusual discovery tell us about how compact elliptical galaxies form?A New Galactic BeastCompact elliptical galaxies are an extremely rare early-type dwarf galaxy. Consistent with their name, compact ellipticals are small, very compact collections of ancient stars; these galaxies exhibit a high surface brightness and arent actively forming stars.Optical view of the ancient compact elliptical galaxy SDSS J085431.18+173730.5 (center of image) in an SDSS color composite image. [Adapted from Paudel et al. 2016]Most compact ellipticals are found in dense environments, particularly around massive galaxies. This has led astronomers to believe that compact ellipticals might form via the tidal stripping of a once-large galaxy in interactions with another, massive galaxy. In this model, once the original galaxys outer layers are stripped away, the compact inner bulge component would be left behind as a compact elliptical galaxy. Recent discoveries of a few isolated compact ellipticals, however, have strained this model.Now a new galaxy has been found to confuse our classification schemes: the first-ever compact elliptical to also display signs of an active galactic nucleus. Led by Sanjaya Paudel (Korea Astronomy and Space Science Institute), a team of scientists discovered SDSS J085431.18+173730.5 serendipitously in Sloan Digital Sky Survey data. The team used SDSS images and spectroscopy in combination with data from the Canada-France-Hawaii Telescope to learn more about this unique galaxy.Puzzling CharacteristicsSDSS J085431.18+173730.5 presents an interesting conundrum. Ancient compact ellipticals are supposed to be devoid of gas, with no fuel left to trigger nuclear activity. Yet SDSS J085431.18+173730.5 clearly shows the emission lines that indicate active accretion onto a supermassive black hole of ~2 million solar masses, according to the authors estimates. Paudel and collaboratorsshow that this mass is consistent with the low-mass extension of the known scaling relation between central black-hole mass and brightness of the host galaxy.Central black hole mass vs. bulge K-band magnitude. SDSS J085431.18+173730.5 (red dot) falls right on the low-mass extension of the observed scaling relation. It has similar properties to M32, another compact elliptical galaxy. [Adapted from Paudel et al. 2016]To add to the mystery, SDSS J085431.18+173730.5 has no nearby neighbors: like the few other isolated compact ellipticals recently discovered, there are no massive galaxies in the immediate vicinity that could have led to its tidal stripping. So how was this puzzling ancient galaxy formed?The authors of this study support a previously proposed flyby scenario: isolated compact ellipticals may simply be tidally stripped systems that ran away from their hosts. Paudel and collaborators suggest that SDSS J085431.18+173730.5 might have long ago interacted with NGC 2672 a galaxy group located a whopping 6.5 million light-years away before being flung out to its current location.Further studies of this unique galaxys emission profile, as well as efforts to learn about its underlying stellar population and central kinematics, will hopefully help us to better understand not only the origins of this galaxy, but how all compact ellipticals form and evolve.CitationSanjaya Paudel et al 2016 ApJ 820 L19. doi:10.3847/2041-8205/820/1/L19

The Double Firing Burst

NASA Astrophysics Data System (ADS)

2008-09-01

Astronomers from around the world combined data from ground- and space-based telescopes to paint a detailed portrait of the brightest explosion ever seen. The observations reveal that the jets of the gamma-ray burst called GRB 080319B were aimed almost directly at the Earth. Uncovering the disc ESO PR Photo 28/08 A Gamma-Ray Burst with Two Jets Read more on this illuminating blast in the additional story. GRB 080319B was so intense that, despite happening halfway across the Universe, it could have been seen briefly with the unaided eye (ESO 08/08). In a paper to appear in the 11 September issue of Nature, Judith Racusin of Penn State University, Pennsylvania (USA), and a team of 92 co-authors report observations across the electromagnetic spectrum that began 30 minutes before the explosion and followed it for months afterwards. "We conclude that the burst's extraordinary brightness arose from a jet that shot material almost directly towards Earth at almost the speed of light - the difference is only 1 part in 20 000," says Guido Chincarini, a member of the team. Gamma-ray bursts are the Universe's most luminous explosions. Most occur when massive stars run out of fuel. As a star collapses, it creates a black hole or neutron star that, through processes not fully understood, drives powerful gas jets outward. As the jets shoot into space, they strike gas previously shed by the star and heat it, thereby generating bright afterglows. The team believes the jet directed toward Earth contained an ultra-fast component just 0.4 degrees across (this is slightly smaller than the apparent size of the Full Moon). This jet is contained within another slightly less energetic jet about 20 times wider. The broad component is more typical of other bursts. "Perhaps every gamma-ray burst has a narrow jet, but astronomers miss it most of the time," says team member Stefano Covino. "We happened to view this monster down the barrel of the very narrow and energetic jet, and the chance for this nearly head-on alignment to occur is only about once a decade," added his colleague Cristiano Guidorzi. GRB 080319B was detected by the NASA/STFC/ASI Swift satellite towards the constellation of Boötes, the "Herdsman". A host of ground-based telescopes reacted promptly to study this new object in the sky, including ESO's Very Large Telescope, which was the first to provide the distance of the object, 7.5 billion light-years. The visible light from the burst was detected by a handful of wide-field cameras worldwide that are mounted on telescopes constantly monitoring a large fraction of the sky. One of these was the TORTORA camera mounted on the 0.6-m REM telescope at ESO's La Silla Observatory (ESO 26/07). TORTORA's rapid imaging provides the most detailed look yet at the visible light associated with the initial blast of a gamma-ray burst. "We've been waiting a long time for this one," says TORTORA senior scientist Grigory Beskin of Russia's Special Astrophysical Observatory. The data collected simultaneously by TORTORA and the Swift satellite allowed astronomers to explain the properties of this burst.

ALMA Explores How Supermassive Black Holes Talk to Their Galaxies

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2017-03-01

We believe that supermassive black holes evolve in tandem with their host galaxies but how do the two communicate? Observations from the Atacama Large Millimeter/submillimeter Array (ALMA) have revealed new clues about how a monster black hole talks to its galaxy.A Hubble image of the central galaxy in the Phoenix cluster. [Adapted from Russell et al. 2017]Observing FeedbackActive galactic nuclei (AGN), the highly luminous centers of some galaxies, are thought to radiate due to active accretion onto the supermassive black hole at their center.Its long been suspected that the radiation and outflowing material which often takes the form of enormous bipolar radio jets emitted into the surroundings influence the AGNs host galaxy, affecting star formation rates and the evolution of the galaxy. This AGN feedback has been alternately suggested to trigger star formation, quench it, and truncate the growth of massive galaxies.The details of this feedback process, however, have yet to be thoroughly understood in part because its difficult to obtain detailed observations of how AGN outflows interact with the galactic gas surrounding them. Now, a team of scientists led by Helen Russell (Institute of Astronomy in Cambridge, UK) has published the results of a new, high-resolution look at the gas in a massive galaxy in the center of the Phoenix cluster.Many Uses for FuelThe Phoenix cluster, a nearby (z = 0.596) group of star-forming galaxies, is the most luminous X-ray cluster known. The central galaxy in the cluster is especially active: it hosts a starburst of 500800 solar masses per year, the largest starburst found in any galaxy below a redshift of z= 1.The star formation in this galaxy is sustained by an enormous reservoir of cold molecular gas roughly 20 billion solar masses worth. This reservoir also powers the galaxys central black hole, fueling powerful radio jets that extend into the hot atmosphere of the galaxy and blow a giant bubble into the hot gas at each pole.ALMA observations of the molecular gas in the central galaxy of the Phoenix cluster. The bubbles blown by the radio jets are indicated by the dashed white contours. Extended filaments of molecular gas can be seen to wrap around these cavities. [Adapted from Russell et al. 2017]ALMA Spots FilamentsALMAs observations of this reservoir show that extended filaments of molecular gas wrap around the peripheries of the radio bubbles. These filaments span 1020 kpc ( 3060 thousand light-years) and have a mass of several billion solar masses. The velocity gradients along them are smooth, suggesting that the gas is moving in an ordered flow around the bubble.Russell and collaborators suggest that these observations indicate that the clouds of molecular gas were either lifted by the radio bubbles as they inflated, or they formed in place via instabilities caused by the inflating bubbles.Either way, the data provide clear confirmation that the jets from the black hole affect the location and motion of the cold gas in the surrounding galaxy. This is a beautiful pieceof direct evidence showing how supermassive black holes might be communicating with their galaxies.CitationH. R. Russell et al 2017 ApJ 836 130. doi:10.3847/1538-4357/836/1/130

Making Supermassive Black Holes Spin

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2016-12-01

Where does the angular momentum come from that causes supermassive black holes (SMBHs) to spin on their axes and launch powerful jets? A new study of nearby SMBHs may help to answer this question.High-mass SMBHs are thought to form when two galaxies collide and the SMBHs at their centers merge. [NASA/Hubble Heritage Team (STScI)]High- vs. Low-Mass MonstersObservational evidence suggests a dichotomy between low-mass SMBHs (those with 106-7 M) and high-mass ones (those with 108-10 M). High-mass SMBHs are thought to form via the merger of two smaller black holes, and the final black hole is likely spun up by the rotational dynamics of the merger. But what spins up low-mass SMBHs, which are thought to build up very gradually via accretion?A team of scientists led by Jing Wang (National Astronomical Observatories, Chinese Academy of Sciences) have attempted to address this puzzle by examining the properties of the galaxies hosting low-mass SMBHs.A Sample of Neighboring SMBHsWang and collaborators began by constructing a sample of radio-selected nearby Seyfert 2 galaxies: those galaxies in which the stellar population and morphology of the host galaxy are visible to us, instead of being overwhelmed by continuum emission from the galaxys active nucleus.An example of a galaxy with a concentrated, classical bulge (M87; top) and a one with a disk-like pseudo bulge (Triangulum Galaxy; bottom). The authors find that for galaxies hosting low-mass SMBHs, those with more disk-like bulges appear to have more powerful radio jets. [Top: NASA/Hubble Heritage Team (STScI), Bottom: Hewholooks]From this sample, the authors then selected 31 galaxies that have low-mass SMBHs at their centers, as measured using the surrounding stellar dynamics. Wang and collaborators cataloged radio information revealing properties of the powerful jets launched by the SMBHs, and they analyzed the host galaxies properties by modeling their brightness profiles.Spin-Up From Accreting GasBy examining this sample, the authors discovered an intriguing relationship: the radio power of jets launched by an SMBH appears to be dependent upon its host galaxys bulge surface brightness. Specifically, Wang and collaborators found that more powerful radio emission comes from SMBHs associated with less-concentrated bulges, i.e. those that are more disk-like.The authors findings allow them to rule out many common explanations for the radio-loudness of such galaxies with small SMBH masses. Instead, they argue that the tendency for galaxies with more disk-like bulges to host SMBHs with more powerful jets is evidence that low-mass SMBHs are spun up by the accretion of surrounding gas.In this scenario, the angular momentum of gas with significant disk-like rotational dynamics provides the spin to the SMBH, and this rotational energy can then be extracted to launch the powerful jets. If this explanation is correct, it strengthens the dichotomy between low-mass and high-mass SMBHs, supporting the idea that the two categories of black holes are indeed formed and spun up via completely different mechanisms.CitationJ. Wang et al 2016 ApJL 833 L2.doi:10.3847/2041-8205/833/1/L2

ALMA Examines a Distant Quasar Host

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2017-04-01

The dust continuum (top) and the [CII] emission (bottom) maps for the region around J1120+0641. [Adapted from Venemans et al. 2017]A team of scientists has used the Atacama Large Millimeter/submillimeter Array (ALMA) to explore the host galaxy of the most distant quasar known. Their observations may help us to build a picture of how the first supermassive black holes in the universe formed and evolved.Faraway Monsters and Their GalaxiesWe know that quasars the incredibly luminous and active centers of some distant galaxies are powered by accreting, supermassive black holes. These monstrous powerhouses have been detected out to redshifts of z 7, when the universe was younger than a billion years old.Though weve observed over a hundred quasars at high redshift, we still dont understand how these early supermassive black holes formed, or whether the black holes and the galaxies that host them co-evolved. In order to answer questions like these, however, we first need to gather information about the properties and behavior of various supermassive black holes and their host galaxies.A team of scientists led by Bram Venemans (Max-Planck Institute for Astronomy, Germany) recently used the unprecedented sensitivity and angular resolution of ALMA as well as the Very Large Array and the IRAM Plateau de Bure Interferometer to examine the most distant quasar currently known, J1120+0641, located at a redshift of z = 7.1.A High-Resolution LookThe teams observations of the dust and gas emission from the quasars host galaxy revealed a number of intriguing things:The red and blue sides of the [CII] emission line are shown here as contours, demonstrating that theres no ordered rotational motion of the gas on kpc scales. [Adapted from Venemans et al. 2017]The majority of the galaxys emission is very compact. Around 80% of the observed flux came from a region of only 11.5 kpc in diameter.Despite the fact that the 2.4-billion-solar-mass black hole at the galaxys center is accreting at a high rate, the heating in the galaxy is dominated not by the black holes accretion, but by star formation.Theres no sign of the expected structure of a rotating disk on kpc scales.The authors estimate a dynamical mass of the host galaxy of 43 billion solar masses and the black hole at the galaxys center makes up 6% of that. This ratio is roughly 10x higher than the black-hole-to-bulge mass ratio in local early-type galaxies.In the very central region, the black hole accounts for around 20% of the galaxys dynamical mass, and gas and dust likely accounts for most of the remainder. This doesnt leave much room for massive stars in the center of the galaxy.ALMAs capabilities have enabled these first efforts to spatially resolve the host galaxy of the most distant quasar known, resulting new and unexpected information. The authors now look hopefully to the future, when even longer baselines of ALMA may allow us a still-higher-resolution look at this distant quasar, possibly providing answers to some of the questions it has raised.CitationBram P. Venemans et al 2017 ApJ 837 146. doi:10.3847/1538-4357/aa62ac

Blast from the Past Gives Clues About Early Universe

NASA Astrophysics Data System (ADS)

2009-10-01

Astronomers using the National Science Foundation's Very Large Array (VLA) radio telescope have gained tantalizing insights into the nature of the most distant object ever observed in the Universe -- a gigantic stellar explosion known as a Gamma Ray Burst (GRB). The explosion was detected on April 23 by NASA's Swift satellite, and scientists soon realized that it was more than 13 billion light-years from Earth. It represents an event that occurred 630 million years after the Big Bang, when the Universe was only four percent of its current age of 13.7 billion years. This explosion provides an unprecedented look at an era when the Universe was very young and also was undergoing drastic changes. The primal cosmic darkness was being pierced by the light of the first stars and the first galaxies were beginning to form. The star that exploded in this event was a member of one of these earliest generations of stars," said Dale Frail of the National Radio Astronomy Observatory. Astronomers turned telescopes from around the world to study the blast, dubbed GRB 090423. The VLA first looked for the object the day after the discovery, detected the first radio waves from the blast a week later, then recorded changes in the object until it faded from view more than two months later. "It's important to study these explosions with many kinds of telescopes. Our research team combined data from the VLA with data from X-ray and infrared telescopes to piece together some of the physical conditions of the blast," said Derek Fox of Pennsylvania State University. "The result is a unique look into the very early Universe that we couldn't have gotten any other way," he added. The scientists concluded that the explosion was more energetic than most GRBs, was a nearly-spherical blast, and that it expanded into a tenuous and relatively uniform gaseous medium surrounding the star. Astronomers suspect that the very first stars in the Universe were very different -- brighter, hotter, and more massive -- from those that formed later. They hope to find evidence for these giants by observing objects as distant as GRB 090423 or more distant. "The best way to distinguish these distant, early-generation stars is by studying their explosive deaths, as supernovae or Gamma Ray Bursts," said Poonam Chandra, of the Royal Military College of Canada, and leader of the research team. While the data on GRB 090423 don't indicate that it resulted from the death of such a monster star, new astronomical tools are coming that may reveal them. "The Atacama Large Millimeter/submillimeter Array (ALMA), will allow us to pick out these very-distant GRBs more easily so we can target them for intense followup observations. The Expanded Very Large Array, with much greater sensitivity than the current VLA, will let us follow these blasts much longer and learn much more about their energies and environments. We'll be able to look back even further in time," Frail said. Both ALMA and the EVLA are scheduled for completion in 2012. Chandra, Frail and Fox worked with Shrinivas Kulkarni of Caltech, Edo Berger of Harvard University, S. Bradley Cenko of the University of California at Berkeley, Douglas C.-J. Bock of the Combined Array for Research in Millimeter-wave Astronomy in California, and Fiona Harrison and Mansi Kasliwal of Caltech. The scientists described their research in a paper submitted to the Astrophysical Journal Letters.

Stars Just Got Bigger - A 300 Solar Mass Star Uncovered

NASA Astrophysics Data System (ADS)

2010-07-01

Using a combination of instruments on ESO's Very Large Telescope, astronomers have discovered the most massive stars to date, one weighing at birth more than 300 times the mass of the Sun, or twice as much as the currently accepted limit of 150 solar masses. The existence of these monsters - millions of times more luminous than the Sun, losing weight through very powerful winds - may provide an answer to the question "how massive can stars be?" A team of astronomers led by Paul Crowther, Professor of Astrophysics at the University of Sheffield, has used ESO's Very Large Telescope (VLT), as well as archival data from the NASA/ESA Hubble Space Telescope, to study two young clusters of stars, NGC 3603 and RMC 136a in detail. NGC 3603 is a cosmic factory where stars form frantically from the nebula's extended clouds of gas and dust, located 22 000 light-years away from the Sun (eso1005). RMC 136a (more often known as R136) is another cluster of young, massive and hot stars, which is located inside the Tarantula Nebula, in one of our neighbouring galaxies, the Large Magellanic Cloud, 165 000 light-years away (eso0613). The team found several stars with surface temperatures over 40 000 degrees, more than seven times hotter than our Sun, and a few tens of times larger and several million times brighter. Comparisons with models imply that several of these stars were born with masses in excess of 150 solar masses. The star R136a1, found in the R136 cluster, is the most massive star ever found, with a current mass of about 265 solar masses and with a birthweight of as much as 320 times that of the Sun. In NGC 3603, the astronomers could also directly measure the masses of two stars that belong to a double star system [1], as a validation of the models used. The stars A1, B and C in this cluster have estimated masses at birth above or close to 150 solar masses. Very massive stars produce very powerful outflows. "Unlike humans, these stars are born heavy and lose weight as they age," says Paul Crowther. "Being a little over a million years old, the most extreme star R136a1 is already 'middle-aged' and has undergone an intense weight loss programme, shedding a fifth of its initial mass over that time, or more than fifty solar masses." If R136a1 replaced the Sun in our Solar System, it would outshine the Sun by as much as the Sun currently outshines the full Moon. "Its high mass would reduce the length of the Earth's year to three weeks, and it would bathe the Earth in incredibly intense ultraviolet radiation, rendering life on our planet impossible," says Raphael Hirschi from Keele University, who belongs to the team. These super heavyweight stars are extremely rare, forming solely within the densest star clusters. Distinguishing the individual stars - which has now been achieved for the first time - requires the exquisite resolving power of the VLT's infrared instruments [2]. The team also estimated the maximum possible mass for the stars within these clusters and the relative number of the most massive ones. "The smallest stars are limited to more than about eighty times more than Jupiter, below which they are 'failed stars' or brown dwarfs," says team member Olivier Schnurr from the Astrophysikalisches Institut Potsdam. "Our new finding supports the previous view that there is also an upper limit to how big stars can get, although it raises the limit by a factor of two, to about 300 solar masses." Within R136, only four stars weighed more than 150 solar masses at birth, yet they account for nearly half of the wind and radiation power of the entire cluster, comprising approximately 100 000 stars in total. R136a1 alone energises its surroundings by more than a factor of fifty compared to the Orion Nebula cluster, the closest region of massive star formation to Earth. Understanding how high mass stars form is puzzling enough, due to their very short lives and powerful winds, so that the identification of such extreme cases as R136a1 raises the challenge to theorists still further. "Either they were born so big or smaller stars merged together to produce them," explains Crowther. Stars between about 8 and 150 solar masses explode at the end of their short lives as supernovae, leaving behind exotic remnants, either neutron stars or black holes. Having now established the existence of stars weighing between 150 and 300 solar masses, the astronomers' findings raise the prospect of the existence of exceptionally bright, "pair instability supernovae" that completely blow themselves apart, failing to leave behind any remnant and dispersing up to ten solar masses of iron into their surroundings. A few candidates for such explosions have already been proposed in recent years. Not only is R136a1 the most massive star ever found, but it also has the highest luminosity too, close to 10 million times greater than the Sun. "Owing to the rarity of these monsters, I think it is unlikely that this new record will be broken any time soon," concludes Crowther. Notes [1] The star A1 in NGC 3603 is a double star, with an orbital period of 3.77 days. The two stars in the system have, respectively, 120 and 92 times the mass of the Sun, which means that they have formed as stars weighing, respectively, 148 and 106 solar masses. [2] The team used the SINFONI, ISAAC and MAD instruments, all attached to ESO's Very Large Telescope at Paranal, Chile. [3] (note added on 26 July 2010) The "bigger" in the title does not imply that these stars are the biggest observed. Such stars, called red supergiants, can have radii up to about a thousand solar radii, while R136a1, which is blue, is about 35 times as large as the Sun. However, R136a1 is the star with the greatest mass known to date. More information This work is presented in an article published in the Monthly Notices of the Royal Astronomical Society ("The R136 star cluster hosts several stars whose individual masses greatly exceed the accepted 150 Msun stellar mass limit", by P. Crowther et al.). The team is composed of Paul A. Crowther, Richard J. Parker, and Simon P. Goodwin (University of Sheffield, UK), Olivier Schnurr (University of Sheffield and Astrophysikalisches Institut Potsdam, Germany), Raphael Hirschi (Keele University, UK), and Norhasliza Yusof and Hasan Abu Kassim (University of Malaya, Malaysia). ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory and VISTA, the world's largest survey telescope. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Young and Exotic Stellar Zoo

NASA Astrophysics Data System (ADS)

2005-03-01

Summary Super star clusters are groups of hundreds of thousands of very young stars packed into an unbelievably small volume. They represent the most extreme environments in which stars and planets can form. Until now, super star clusters were only known to exist very far away, mostly in pairs or groups of interacting galaxies. Now, however, a team of European astronomers [1] have used ESO's telescopes to uncover such a monster object within our own Galaxy, the Milky Way, almost, but not quite, in our own backyard! The newly found massive structure is hidden behind a large cloud of dust and gas and this is why it took so long to unveil its true nature. It is known as "Westerlund 1" and is a thousand times closer than any other super star cluster known so far. It is close enough that astronomers may now probe its structure in some detail. Westerlund 1 contains hundreds of very massive stars, some shining with a brilliance of almost one million suns and some two-thousand times larger than the Sun (as large as the orbit of Saturn)! Indeed, if the Sun were located at the heart of this remarkable cluster, our sky would be full of hundreds of stars as bright as the full Moon. Westerlund 1 is a most unique natural laboratory for the study of extreme stellar physics, helping astronomers to find out how the most massive stars in our Galaxy live and die. From their observations, the astronomers conclude that this extreme cluster most probably contains no less than 100,000 times the mass of the Sun, and all of its stars are located within a region less than 6 light-years across. Westerlund 1 thus appears to be the most massive compact young cluster yet identified in the Milky Way Galaxy. PR Photo 09a/05: The Super Star Cluster Westerlund 1 (2.2m MPG/ESO + WFI) PR Photo 09b/05: Properties of Young Massive Clusters Super Star Clusters Stars are generally born in small groups, mostly in so-called "open clusters" that typically contain a few hundred stars. From a wide range of observations, astronomers infer that the Sun itself was born in one such cluster, some 4,500 million years ago. In some active ("starburst") galaxies, scientists have observed violent episodes of star formation (see, for example, ESO Press Photo 31/04), leading to the development of super star clusters, each containing several million stars. Such events were obviously common during the Milky Way's childhood, more than 12,000 million years ago: the many galactic globular clusters - which are nearly as old as our Galaxy (e.g. ESO PR 20/04) - are indeed thought to be the remnants of early super star clusters. All super star clusters so far observed in starburst galaxies are very distant. It is not possible to distinguish their individual stars, even with the most advanced technology. This dramatically complicates their study and astronomers have therefore long been eager to find such clusters in our neighbourhood in order to probe their structure in much more detail. Now, a team of European astronomers [1] has finally succeeded in doing so, using several of ESO's telescopes at the La Silla observatory (Chile). Westerlund 1 ESO PR Photo 09a/05 ESO PR Photo 09a/05 The Super Star Cluster Westerlund 1 (2.2m MPG/ESO + WFI) [Preview - JPEG: 400 x 472 pix - 58k] [Normal - JPEG: 800 x 943 pix - 986k] [Full Res - JPEG: 1261 x 1486 pix - 2.4M] Caption: ESO PR Photo 09a/05 is a composite image of the super star cluster "Westerlund 1" from 2.2-m MPG/ESO Wide-Field Imager (WFI) observations. The image covers a 5 x 5 arcmin sky region and is based on observations made in the V-band (550 nm, 2 min exposure time, associated to the blue channel), R-band (650nm, 1 min, green channel) and I-band (784nm, 18 sec, red channel). Only the central CCD of WFI was used, as the entire cluster fits comfortably inside it. The foreground stars appear blue, while the hot massive members of the cluster look orange, and the cool massive ones come out red. The open cluster Westerlund 1 is located in the Southern constellation Ara (the Altar). It was discovered in 1961 from Australia by Swedish astronomer Bengt Westerlund, who later moved from there to become ESO Director in Chile (1970 - 74). This cluster is behind a huge interstellar cloud of gas and dust, which blocks most of its visible light. The dimming factor is more than 100,000 - and this is why it has taken so long to uncover the true nature of this particular cluster. In 2001, the team of astronomers identified more than a dozen extremely hot and peculiar massive stars in the cluster, so-called "Wolf-Rayet" stars. They have since studied Westerlund 1 extensively with various ESO telescopes. They used images from the Wide Field Imager (WFI) attached to the 2.2-m ESO/MPG as well as from the SUperb Seeing Imager 2 (SuSI2) camera on the ESO 3.5-m New Technology Telescope (NTT). From these observations, they were able to identify about 200 cluster member stars. To establish the true nature of these stars, the astronomers then performed spectroscopic observations of about one quarter of them. For this, they used the Boller & Chivens spectrograph on the ESO 1.52-m telescope and the ESO Multi-Mode Instrument (EMMI) on the NTT. An Exotic Zoo These observations have revealed a large population of very bright and massive, quite extreme stars. Some would fill the solar system space within the orbit of Saturn (about 2,000 times larger than the Sun!), others are as bright as a million Suns. Westerlund 1 is obviously a fantastic stellar zoo, with a most exotic population and a true astronomical bonanza. All stars identified are evolved and very massive, spanning the full range of stellar oddities from Wolf-Rayet stars, OB supergiants, Yellow Hypergiants (nearly as bright as a million Suns) and Luminous Blue Variables (similar to the exceptional Eta Carinae object - see ESO PR 31/03). All stars so far analysed in Westerlund 1 weigh at least 30-40 times more than the Sun. Because such stars have a rather short life - astronomically speaking - Westerlund 1 must be very young. The astronomers determine an age somewhere between 3.5 and 5 million years. So, Westerlund 1 is clearly a "newborn" cluster in our Galaxy! The Most Massive Cluster ESO PR Photo 09b/05 ESO PR Photo 09b/05 Properties of Young Massive Clusters [Preview - JPEG: 400 x 511 pix - 20k] [Normal - JPEG: 800 x 1021 pix - 122k] Caption: ESO PR Photo 09b/05 shows the properties of young massive clusters in our Galaxy and in the Large Magellanic Clouds, as well as of Super Star Clusters in star-forming galaxies. The diagram shows the mass and radius of these clusters and also the position of Westerlund 1 (indicated Wd 1). Westerlund 1 is incredibly rich in monster stars - just as one example, it contains as many Yellow Hypergiants as were hitherto known in the entire Milky Way! "If the Sun were located at the heart of Westerlund 1, the sky would be full of stars, many of them brighter than the full Moon", comments Ignacio Negueruela of the Universidad de Alicante in Spain and member of the team. The large quantity of very massive stars implies that Westerlund 1 must contain a huge number of stars. "In our Galaxy, explains Simon Clark of the University College London (UK) and one of the authors of this study, "there are more than 100 solar-like stars for every star weighing 10 times as much as the Sun. The fact that we see hundreds of massive stars in Westerlund 1 means that it probably contains close to half a million stars, but most of these are not bright enough to peer through the obscuring cloud of gas and dust". This is ten times more than any other known young clusterin the Milky Way. Westerlund 1 is presumably much more massive than the dense clusters of heavy stars present in the central region of our Galaxy, like the Arches and Quintuplet clusters. Further deep infrared observations will be required to confirm this. This super star cluster now provides astronomers with a unique perspective towards one of the most extreme environments in the Universe. Westerlund 1 will certainly provide new opportunities in the long-standing quest for more and finer details about how stars, and especially massive ones, do form. ... and the Most Dense The large number of stars in Westerlund 1 was not the only surprise awaiting Clark and his colleagues. From their observations, the team members also found that all these stars are packed into an amazingly small volume of space, indeed less than 6 light-years across. In fact, this is more or less comparable to the 4 light-year distance to the star nearest to the Sun, Proxima Centauri! It is incredible: the concentration in Westerlund 1 is so high that the mean separation between stars is quite similar to the extent of the Solar System. "With so many stars in such a small volume, some of them may collide", envisages Simon Clark. "This could lead to the formation of an intermediate-mass black hole more massive than 100 solar masses. It may well be that such a monster has already formed at the core of Westerlund 1." The huge population of massive stars in Westerlund 1 suggests that it will have a very significant impact on its surroundings. The cluster contains so many massive stars that in a time span of less than 40 million years, it will be the site of more than 1,500 supernovae. A gigantic firework that may drive a fountain of galactic material! Because Westerlund 1 is at a distance of only about 10,000 light-years, high-resolution cameras such as NAOS/CONICA on ESO's Very Large Telescope can resolve its individual stars. Such observations are now starting to reveal smaller stars in Westerlund 1, including some that are less massive than the Sun. Astronomers will thus soon be able to study this exotic galactic zoo in great depth. More information The research presented in this ESO Press Release will soon appear in the leading research journal Astronomy and Astrophysics ("On the massive stellar population of the Super Star Cluster Westerlund 1" by J.S. Clark and colleagues). The PDF file is available at the A&A web site. A second paper ("Further Wolf-Rayet stars in the starburst cluster Westerlund 1", by Ignacio Negueruela and Simon Clark) will also soon be published in Astronomy and Astrophysics. It is available as astro-ph/0503303. A Spanish press release issued by Universidad de Alicante is available on the web site of Ignacio Negueruela.

An Eagle of Cosmic Proportions

NASA Astrophysics Data System (ADS)

2009-07-01

Today ESO has released a new and stunning image of the sky around the Eagle Nebula, a stellar nursery where infant star clusters carve out monster columns of dust and gas. Located 7000 light-years away, towards the constellation of Serpens (the Snake), the Eagle Nebula is a dazzling stellar nursery, a region of gas and dust where young stars are currently being formed and where a cluster of massive, hot stars, NGC 6611, has just been born. The powerful light and strong winds from these massive new arrivals are shaping light-year long pillars, seen in the image partly silhouetted against the bright background of the nebula. The nebula itself has a shape vaguely reminiscent of an eagle, with the central pillars being the "talons". The star cluster was discovered by the Swiss astronomer, Jean Philippe Loys de Chéseaux, in 1745-46. It was independently rediscovered about twenty years later by the French comet hunter, Charles Messier, who included it as number 16 in his famous catalogue, and remarked that the stars were surrounded by a faint glow. The Eagle Nebula achieved iconic status in 1995, when its central pillars were depicted in a famous image obtained with the NASA/ESA Hubble Space Telescope. In 2001, ESO's Very Large Telescope (VLT) captured another breathtaking image of the nebula in the near-infrared, giving astronomers a penetrating view through the obscuring dust, and clearly showing stars being formed in the pillars. The newly released image, obtained with the Wide-Field Imager camera attached to the MPG/ESO 2.2-metre telescope at La Silla, Chile, covers an area on the sky as large as the full Moon, and is about 15 times more extensive than the previous VLT image, and more than 200 times more extensive than the iconic Hubble visible-light image. The whole region around the pillars can now be seen in exquisite detail. The "Pillars of Creation" are in the middle of the image, with the cluster of young stars, NGC 6611, lying above and to the right. The "Spire" - another pillar captured by Hubble - is at the centre left of the image. Finger-like features protrude from the vast cloud wall of cold gas and dust, not unlike stalagmites rising from the floor of a cave. Inside the pillars, the gas is dense enough to collapse under its own weight, forming young stars. These light-year long columns of gas and dust are being simultaneously sculpted, illuminated and destroyed by the intense ultraviolet light from massive stars in NGC 6611, the adjacent young stellar cluster. Within a few million years - a mere blink of the universal eye - they will be gone forever. More information ESO, the European Southern Observatory, is the foremost intergovernmental astronomy organisation in Europe and the world's most productive astronomical observatory. It is supported by 14 countries: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Italy, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope, the world's most advanced visible-light astronomical observatory. ESO is the European partner of a revolutionary astronomical telescope ALMA, the largest astronomical project in existence. ESO is currently planning a 42-metre European Extremely Large optical/near-infrared Telescope, the E-ELT, which will become "the world's biggest eye on the sky".

Chandra Sees Remarkable Eclipse of Black Hole

NASA Astrophysics Data System (ADS)

2007-04-01

A remarkable eclipse of a supermassive black hole and the hot gas disk around it has been observed with NASA's Chandra X-ray Observatory. This eclipse has allowed two key predictions about the effects of supermassive black holes to be tested. Just as eclipses of the Sun and moon give astronomers rare opportunities to learn about those objects, an alignment in a nearby galaxy has provided a rare opportunity to investigate a supermassive black hole. Illustrations of Black Hole Eclipse Illustrations of Black Hole Eclipse The supermassive black hole is located in NGC 1365, a galaxy 60 million light years from Earth. It contains a so called active galactic nucleus, or AGN. Scientists believe that the black hole at the center of the AGN is fed by a steady stream of material, presumably in the form of a disk. Material just about to fall into a black hole should be heated to millions of degrees before passing over the event horizon, or point of no return. The disk of gas around the central black hole in NGC 1365 produces copious X-rays but is much too small to resolve directly with a telescope. However, the disk was eclipsed by an intervening cloud, so observation of the time taken for the disk to go in and out of eclipse allowed scientists to estimate the size of the disk. Black Hole Animation Black Hole Animation "For years we've been struggling to confirm the size of this X-ray structure," said Guido Risaliti of the Harvard-Smithsonian Center for Astrophysics (CfA) in Cambridge, Mass, and the Italian Institute of Astronomy (INAF). "This serendipitous eclipse enabled us to make this breakthrough." The Chandra team directly measured the size of the X-ray source as about seven times the distance between the Sun and the Earth. That means the source of X-rays is about 2 billion times smaller than the host galaxy and only about 10 times larger than the estimated size of the black hole's event horizon, consistent with theoretical predictions. Chandra X-ray Image of NGC 1365 Chandra X-ray Image of NGC 1365 "Thanks to this eclipse, we were able to probe much closer to the edge of this black hole than anyone has been able to before," said co-author Martin Elvis from CfA. "Material this close in will likely cross the event horizon and disappear from the universe in about a hundred years, a blink of an eye in cosmic terms." In addition to measuring the size of this disk of material, Risaliti and his colleagues were also able to estimate the location of the dense gas cloud that eclipsed the X-ray source and central black hole. The Chandra data show that this cloud is one hundredth of a light year from the black hole's event horizon, or 300 times closer than generally thought. "AGN include the brightest objects in the Universe and are powerful probes of the early universe. So, it's vital to understand their basic structure," said Risaliti. "It turns out that we still have work to do to understand these monsters." A series of six Chandra observations of NGC 1365 were made every two days over a period of two weeks in April 2006. During five of the observations, high energy X-rays from the central X-ray source were visible, but in the second one - corresponding to the eclipse - they were not. NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the agency's Science Mission Directorate. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center, Cambridge, Mass. Additional information and images are available at: http://chandra.harvard.edu and http://chandra.nasa.gov

New Discoveries Fill the Quasar Gap

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2017-04-01

Quasars active and luminous galactic centers can be difficult to find at some high redshifts due to their camouflaging color. A team of scientists has now come up with a way to detect these distant monsters in spite of their disguise.Quasar CamouflageThe color track of quasars between 5 z 6 in the commonly used i z and r i bands. Each dot on the red line marks a 0.1 difference in redshift. The contours show the colors of M dwarfs, from early type to late type. Quasars at a redshift of 5.3 z 5.7 are clearly contaminated by M dwarfs, making them difficult to identify. [Adapted from Yang et al. 2017]One of the key ways we can study the early universe is by building a large sample of high-redshift quasars. In particular, we believe that reionization of the universe is just completing around z 6. Quasars near this redshift are crucial tools for probing the post-reionization epoch and exploring the evolution of the intergalactic medium, quasar evolution, and early supermassive black hole growth.But quasars at this redshift are difficult to detect! The problem is contamination: quasars at this distance are the same color in commonly used optical bands as cool M-dwarf stars. As a result, surveys searching for quasars have often just cut out that entire section of the color space in order to avoid this contamination.This means that theres a huge gap in our sample of quasars around z 5.5: of the more than 300,000 quasars known, only 30 have been found in the redshift range of 5.3 z 5.7.The addition of new colorcolor selection criteria using infrared bands (bottom two plots) allows the authors to differentiate quasars (blue) from M dwarfs (grey), which isnt possible when only the traditional optical colorcolor selection criteria are used (top plot). [Adapted from Yang et al. 2017]A New ApproachIn a recent publication led by Jinyi Yang (Peking University, China and Steward Observatory, University of Arizona), a team of scientists has demonstrated a new technique for finding these missing quasars. The team uses this technique to perform the first systematic survey of luminous quasars at a redshift near z = 5.5.Instead of relying only on the conventional color space in broad optical bands, Yang and collaborators selected candidates by also looking at their colors in near-infrared and mid-infrared bands. The team used observations from the Sloan Digital Sky Survey, the UKIRT Infrared Deep Sky Surveys Large Area Survey, the VISTA Hemisphere Survey, and the Wide Field Survey Explorer.Examining the quasar candidates in these color spaces allowed the authors to more clearly differentiate between the M dwarfs and the quasars, so that they could select only the candidates that clearly fell in the regions dominated by quasars in all three spaces. Yang and collaborators then performed spectroscopic follow-up on their candidates to confirm them.Gap Quasars UncoveredThe authors found 21 new high-redshift quasars (red), including 15 in the range of 5.3 z 5.7. [Adapted from Yang et al. 2017]The team found a total of 21 new quasars from their main sample, with 15 new quasars discovered specifically in the redshift range of 5.3 z 5.7. This nearly doubles the number of known quasars at z 5.5!This initial success has more applications in the future; upcoming surveys will provide an even larger sample to examine for z 5.5 quasars. The team demonstrated that their pipeline can be applied to such surveys by testing it on some preliminary data from the UKIRT Hemisphere Survey. In just this initial test they already discovered another z 5.5 quasar, demonstrating that theyll have little difficultly finding more once the complete data set is released.CitationJinyi Yang et al 2017 AJ 153 184. doi:10.3847/1538-3881/aa6577

Did Triton Destroy Neptune's First Moons?

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2017-11-01

Neptunes moon system is not what we would expect for a gas giant in our solar system. Scientists have now explored the possibility that Neptune started its life with an ordinary system of moons that was later destroyed by the capture of its current giant moon, Triton.An Odd SystemOur current understanding of giant-planet formation predicts a period of gas accretion to build up the large size of these planets. According to models, the circumplanetary gas disks that surround the planets during this time then become the birthplaces of the giant planets satellite systems, producing systems of co-planar and prograde (i.e., orbiting in the same direction as the planets rotation) satellites similar to the many-moon systems of Jupiter or Saturn.Tritons orbit is tilted relative to the inner Neptunian satellite orbits. [NASA, ESA, and A. Feild (STScI)]Neptune, however, is quirky. This gas giant has surprisingly few satellites only 14 compared to, say, the nearly 70 moons of Jupiter and most of them are extremely small. One of Neptunes moons is an exception to this, however: Triton, which contains 99.7% of the mass of Neptunes entire satellite system!Tritons orbit has a number of unusual properties. The orbit is retrograde Triton orbits in the opposite direction as Neptunes rotation which is unique behavior among large moons in our solar system. Tritons orbit is also highly inclined, and yet the moons path is nearly circular and lies very close to Neptune.The distribution of impact velocities in the authors simulations for primordial satellite interactions with Triton, in three cases of different satellite mass ratios. In the low-mass case a third of the mass ratio of the Uranian satellite system 88% of simulations ended with Triton surviving on its high-inclination orbit. The survival rate was only 12% in the high-mass case. [Adapted from Rufu et al. 2017]How did this monster of a satellite get its strange properties, and why is Neptunes system so odd compared to what we would expect for a gas giants satellites? Two scientists, Raluca Rufu (Weizmann Institute of Science, Israel) and Robin Canup (Southwest Research Institute), propose an explanation in which Triton long ago wreaked havoc on a former system of satellites around Neptune.Destruction After CaptureRufu and Canup explore the scenario in which Neptune once had an ordinary, prograde system of moons around it that resembled those of the other gas giants. Triton, the authors suggest, may have been a former Kuiper belt object that was then captured by Neptune. The ensuing interactions between retrograde Triton and Neptunes original, prograde satellite system may have then resulted in the destruction of this original system, leaving behind only Triton and Neptunes other current satellites.Nereid, a small irregular moon of Neptune, orbits at an average distance of more than 15 times that of Triton. Models of Tritons orbital evolution must also account for the preservation of satellites like this one. [NASA]Using N-body simulations that model a newly captured Triton and a likely primordial prograde system of moons, Rufu and Canup show that if the moons have a mass ratio similar to that of Uranuss system or smaller, Tritons interactions with it have a substantial likelihood of reproducing the current Neptunian satellite system. They even demonstrate that the interactions decrease Tritons initial semimajor axis quickly enough to prevent smaller, outer satellites like Nereid from being kicked out of the system.If the authors picture is correct, then it neatly explains why Neptunes satellite system looks so unusual compared to Jupiters or Saturns which means that our models of how primordial systems of moons form around gas giants still holdstrong.CitationRaluca Rufu and Robin M. Canup 2017 AJ 154 208. doi:10.3847/1538-3881/aa9184

Closer to the Monster

NASA Astrophysics Data System (ADS)

2004-05-01

Trailblazing VLT Interferometer Studies of the Central Region in Active Galaxy NGC 1068 [1] Summary Fulfilling an old dream of astronomers, observations with the Very Large Telescope Interferometer (VLTI) at the ESO Paranal Observatory (Chile) have now made it possible to obtain a clear picture of the immediate surroundings of the black hole at the centre of an active galaxy. The new results concern the spiral galaxy NGC 1068, located at a distance of about 50 million light-years. They show a configuration of comparatively warm dust (about 50°C) measuring 11 light-years across and 7 light-years thick, with an inner, hotter zone (500°C), about 2 light-years wide. These imaging and spectral observations confirm the current theory that black holes at the centres of active galaxies are enshrouded in a thick doughnut-shaped structure of gas and dust called a "torus". For this trailblazing study, the first of its kind of an extragalactic object by means of long-baseline infrared interferometry, an international team of astronomers [2] used the new MIDI instrument in the VLTI Laboratory. It was designed and constructed in a collaboration between German, Dutch and French research institutes [3]. Combining the light from two 8.2-m VLT Unit Telescopes during two observing runs in June and November 2003, respectively, a maximum resolution of 0.013 arcsec was achieved, corresponding to about 3 light-years at the distance of NGC 1068. Infrared spectra of the central region of this galaxy were obtained that indicate that the heated dust is probably of alumino-silicate composition. The new results are published in a research paper appearing in the May 6, 2004, issue of the international research journal Nature. PR Photo 13/04: The central region in active galaxy NGC 1068 NGC 1068 - a typical active galaxy Active galaxies are among the most spectacular objects in the sky. Their compact nuclei (AGN = Active Galaxy Nuclei) are so luminous that they can outshine the entire galaxy; "quasars" constitute extreme cases of this phenomenon. These cosmic objects show many interesting observational characteristics over the whole electromagnetic spectrum, ranging from radio to X-ray emission. There is now much evidence that the ultimate power station of these activities originate in supermassive black holes with masses up to thousands of millions times the mass of our Sun, cf. e.g., ESO PR 04/01. The one in the Milky Way galaxy has only about 3 million solar masses, cf. ESO PR 17/02. The black hole is believed to be fed from a tightly wound accretion disc of gas and dust encircling it. Material that falls towards such black holes will be compressed and heated up to tremendous temperatures. This hot gas radiates an enormous amount of light, causing the active galaxy nucleus to shine so brightly. NGC 1068 (also known as Messier 77) is among the brightest and most nearby active galaxies. Located in the constellation Cetus (The Whale) at a distance of about 50 million light-years, it looks like a rather normal, barred spiral galaxy. The core of this galaxy, however, is very luminous, not only in optical, but also in ultraviolet and X-ray light. A black hole with a mass equivalent to about 100 million times the mass of our Sun is required to account for the nuclear activity in NGC 1068. The VLTI observations ESO PR Photo 13/04 ESO PR Photo 13/04 The central region of NGC 1068 [Preview - JPEG: 852 x 400 pix - 187k] [Normal - JPEG: 1703 x 800 pix - 552k] Caption: ESO PR Photo 13/04 illustrates the new insight into the central region of the active galaxy NGC 1068, at increasing magnification. Image a (left) A colour composite of NGC 1068, obtained with the Hubble Space Telescope (HST); showing stellar light in blue, oxygen ionized by the active nucleus in yellow, and inonized hydrogen in red. Image b (middle) is a VLTI image by MIDI at wavelength 8.7 µm, penetrating the dust cloud and showing the central structures in great detail. Image c (right) is a sketch of the dust structure of the innermost region. It contains a central hot component (at least 500°C; yellow), marginally resolved by the VLTI observations in the North-South direction (i.e. in the vertical direction in this image). It is surrounded by a larger warm component (~50°, red) that is well resolved. The arrows at the upper left indicate the directions of the two VLTI baselines and the corresponding resolution (image sharpness) at the central observed wavelength (10.5 µm). On the nights of June 14 to 16, 2003, a team of European astronomers [2] conducted a first series of observations to verify the scientific potential of the newly installed MIDI instrument on the VLTI. They also studied the active galaxy NGC 1068. Already at this first attempt, it was possible to see details near the centre of this object, cf. ESO PR 17/03. MIDI is sensitive to light of a wavelength near 10 µm, i.e. in the mid-infrared spectral region ("thermal infrared"). With distances between the contributing telescopes ("baselines") of up to 200 m, MIDI can reach a maximum angular resolution (image sharpness) of about 0.01 arcsec. Equally important, by combining the light beams from two 8.2-m VLT Unit Telescopes, MIDI now allows, for the first time, to perform infrared interferometry of comparatively faint objects outside our own galaxy, the Milky Way. With its high sensitivity to thermal radiation, MIDI is ideally suited to study material in the highly obscured regions near a central black hole and heated by its ultraviolet and optical radiation. The energy absorbed by the dust grains is then re-radiated at longer wavelengths in the thermal infrared spectral region between 5 and 100 µm. The central region in NGC 1068 Additional interferometric observations were secured in November 2003 at a baseline of 42 m. Following a careful analysis of all data, the achieved spatial resolution (image sharpness) and the detailed spectra have allowed the astronomers to study the structure of the central region of NGC 1068. They detect the presence of an innermost, comparatively "hot" cloud of dust, heated to about 500°C and with a diameter equal to or smaller than the achieved image sharpness, i.e. about 3 light-years. It is surrounded by a cooler, dusty region, with a temperature of about 50°C, measuring 11 light-years across and about 7 light-years thick. This is most likely the predicted central, disc-shaped cloud that rotates around the black hole. The comparative thickness of the observed structure (the thickness is ~ 65% of the diameter) is of particular relevance in that it can only remain stable if subjected to a continuous injection of motion ("kinetic") energy. However, none of the current models of central regions in active galaxies provide a convincing explanation of this. The MIDI spectra, covering the wavelength interval from 8 - 13.5 µm, also provide information about the possible composition of the dust grains. The most likely constituent is calcium aluminum-silicate (Ca2Al2SiO7), a high-temperature species that is also found in the outer atmospheres of some super-giant stars. Still, these pilot observations cannot conclusively rule out other types of non-olivine dust. Outlook These are the first-ever long-baseline imaging and spectral inteferometric observations of an extragalactic object in the thermal infrared. They open the door to a completely new field in astronomy: the study of gas and dust structures surrounding and feeding the heaviest black holes in the universe. Says Dutch astronomer Walter Jaffe from the Leiden Observatory and first author of the research paper about the MIDI observations: "Already these first results show that we are far from understanding what really goes on near those monster objects. MIDI and the VLTI will offer for years to come the best combination for astronomers from all over the world to carry out these exciting studies."

Satellite Views Powerful Winter Storm Battering Mid-Atlantic and New England

NASA Image and Video Library

2014-02-13

The monster winter storm that brought icing to the U.S. southeast moved northward along the Eastern Seaboard and brought snow, sleet and rain from the Mid-Atlantic to New England on February 13. A new image from NOAA's GOES satellite showed clouds associated with the massive winter storm stretch from the U.S. southeast to the northeast. Data from NOAA's GOES-East satellite taken on Feb. 13 at 1455 UTC/9:45 a.m. EST were made into an image by NASA/NOAA's GOES Project at NASA's Goddard Space Flight Center in Greenbelt, Md. The clouds and fallen snow data from NOAA's GOES-East satellite were overlaid on a true-color image of land and ocean created by data from the Moderate Resolution Imaging Spectroradiometer or MODIS instrument that flies aboard NASA's Aqua and Terra satellites.The image showed that the clouds associated with the storm were blanketing much of the U.S. East Coast. At 3:11 a.m. EST, a surface map issued by the National Weather Service or NWS showed the storm's low pressure area was centered over eastern North Carolina. Since then, the low has continued to track north along the eastern seaboard. By 11 a.m. EST, precipitation from the storm was falling from South Carolina to Maine, according to National Weather Service radar. By 11 a.m. EST, the Washington, D.C. region snow and sleet totals ranged from 3" in far eastern Maryland to over 18" in the northern and western suburbs in Maryland and Virginia. NWS reported that snow, sleet and rain were still falling and more snow is expected as the back side of the low moves into the region. The New York City region remained under an NWS Winter Storm Warning until 6 a.m. on Friday, February 14 and the National Weather Service expects minor coastal impacts Thursday into Friday afternoon. New England was also being battered by the storm. At 10:56 a.m. EST, Barnstable, Mass. on Cape Cod was experiencing rain and winds gusting to 28 mph. An NWS wind advisory is in effect for Cape Cod until 7 p.m. EST. Further north, Portland, Maine was experiencing heavy snow with winds from the northeast at 6 mph. The National Weather Service in Gray, Maine noted "Significant snowfall is likely for much of western Maine and New Hampshire as this storm passes by. There will be a mix or changeover to sleet and freezing rain over southern and coastal sections tonight...before all areas end as a period of snow Friday (Feb. 14) morning." On February 13 at 10 a.m. EST, NOAA's National Weather Service noted "An abundance of Atlantic moisture getting wrapped into the storm will continue to fuel widespread precipitation...which should lift through the Mid-Atlantic States and Northeast Thursday into Friday. A wide swath of heavy snow accumulations are expected with this storm...but air [moving] off the warmer ocean water should change snow over to rain along the coastal areas. Also...a narrow axis of sleet and freezing rain will be possible within the transition zone...which is expected to set up near the I-95 corridor." For updates on local forecasts, watches and warnings, visit NOAA's www.weather.gov webpage. GOES satellites provide the kind of continuous monitoring necessary for intensive data analysis. Geostationary describes an orbit in which a satellite is always in the same position with respect to the rotating Earth. This allows GOES to hover continuously over one position on Earth's surface, appearing stationary. As a result, GOES provide a constant vigil for the atmospheric "triggers" for severe weather conditions such as tornadoes, flash floods, hail storms and hurricanes. For updated information about the storm system, visit NOAA's WPC website: www.hpc.ncep.noaa.gov/ For more information about GOES satellites, visit: www.goes.noaa.gov/ or goes.gsfc.nasa.gov/ Credit: NASA/GSFC/Jeff Schmaltz/MODIS Land Rapid Response Team NASA image use policy. NASA Goddard Space Flight Center enables NASA’s mission 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 mission. Follow us on Twitter Like us on Facebook Find us on Instagram

VLBA Reveals Closest Pair of Supermassive Black Holes

NASA Astrophysics Data System (ADS)

2006-05-01

Astronomers using the National Science Foundation's Very Long Baseline Array (VLBA) radio telescope have found the closest pair of supermassive black holes ever discovered in the Universe -- a duo of monsters that together are more than 150 million times more massive than the Sun and closer together than the Earth and the bright star Vega. The VLBA The VLBA CREDIT: NRAO/AUI/NSF "These two giant black holes are only about 24 light-years apart, and that's more than 100 times closer than any pair found before," said Cristina Rodriguez, of the University of New Mexico (UNM) and Simon Bolivar University in Venezuela. Black holes are concentrations of mass with gravity so strong that not even light can escape them. The black hole pair is in the center of a galaxy called 0402+379, some 750 million light-years from Earth. Astronomers presume that each of the supermassive black holes was once at the core of a separate galaxy, then the two galaxies collided, leaving the black holes orbiting each other. The black holes orbit each other about once every 150,000 years, the scientists say. "If two black holes like these were to collide, that event would create the type of strong gravitational waves that physicists hope to detect with instruments now under construction," said Gregory Taylor, of UNM. The physicists will need to wait, though: the astronomers calculate that the black holes in 0402+379 won't collide for about a billion billion years. "There are some things that might speed that up a little bit," Taylor remarked. An earlier VLBA study of 0402+379, an elliptical galaxy, showed the pair of radio-wave-emitting objects near its core. Further studies using the VLBA and the Hobby-Eberly Telescope in Texas, revealed that the pair of objects is indeed a pair of supermassive black holes. "We needed the ultra-sharp radio 'vision' of the VLBA, particularly at the high radio frequencies of 22 and 43 GigaHertz, to get the detail needed to show that those objects are a pair of black holes," Taylor said. The VLBA is a continent-wide system of ten radio-telescope antennas. It provides the greatest ability to see fine detail, called resolving power, of any telescope in astronomy. "Astronomers have thought for a long time that close pairs of black holes should result from galaxy collisions," Rodriguez said. Still, finding them has proven difficult. Until now, the closest confirmed pairs of supermassive black holes were at least 4,500 light-years apart. Pairs of smaller black holes, each only a few times the mass of the Sun, have been found in our own Milky Way Galaxy, but 0402+379 harbors the pair of supermassive black holes that are the closest to each other yet found. Galactic collisions are common throughout the Universe, and astronomers think that the binary pairs of supermassive black holes that result can have important effects on the subsequent evolution of the galaxies. In a number of predicted scenarios, such giant pairs of black holes will themselves collide, sending gravitational waves out through the Universe. Such gravitational waves could be detected with a proposed joint space mission between NASA and the European Space Agency, the Laser Interferometer Space Antenna. "Such black-hole collisions undoubtedly are important processes, and we need to understand them. Finding ever-closer pairs of supermassive black holes is the first step in that process. Even finding one such system has dramatically changed our expectations, and informed us about what to look for," Taylor said. Taylor and his collaborators are currently using the VLBA to carry out the largest survey of compact radio-emitting objects ever undertaken, in the hope of finding more such pairs. Rodriguez and Taylor worked with Robert Zavala of the U.S. Naval Observatory, Allison Peck of the SubMillimeter Array of the Harvard- Smithsonian Center for Astrophysics, Lindsey Pollack of the University of California at Santa Cruz, and Roger Romani of Stanford University. Their results have been accepted for publication in the Astrophysical Journal. The National Radio Astronomy Observatory is a facility of the National Science Foundation, operated under cooperative agreement by Associated Universities, Inc.

Black Hole Paradox Solved By NASA's Chandra

NASA Astrophysics Data System (ADS)

2006-06-01

Black holes are lighting up the Universe, and now astronomers may finally know how. New data from NASA's Chandra X-ray Observatory show for the first time that powerful magnetic fields are the key to these brilliant and startling light shows. It is estimated that up to a quarter of the total radiation in the Universe emitted since the Big Bang comes from material falling towards supermassive black holes, including those powering quasars, the brightest known objects. For decades, scientists have struggled to understand how black holes, the darkest objects in the Universe, can be responsible for such prodigious amounts of radiation. Animation of a Black Hole Pulling Matter from Companion Star Animation of a Black Hole Pulling Matter from Companion Star New X-ray data from Chandra give the first clear explanation for what drives this process: magnetic fields. Chandra observed a black hole system in our galaxy, known as GRO J1655-40 (J1655, for short), where a black hole was pulling material from a companion star into a disk. "By intergalactic standards J1655 is in our backyard, so we can use it as a scale model to understand how all black holes work, including the monsters found in quasars," said Jon M. Miller of the University of Michigan, Ann Arbor, whose paper on these results appears in this week's issue of Nature. Gravity alone is not enough to cause gas in a disk around a black hole to lose energy and fall onto the black hole at the rates required by observations. The gas must lose some of its orbital angular momentum, either through friction or a wind, before it can spiral inward. Without such effects, matter could remain in orbit around a black hole for a very long time. Illustration of Magnetic Fields in GRO J1655-40 Illustration of Magnetic Fields in GRO J1655-40 Scientists have long thought that magnetic turbulence could generate friction in a gaseous disk and drive a wind from the disk that carries angular momentum outward allowing the gas to fall inward. Using Chandra, Miller and his team provided crucial evidence for the role of magnetic forces in the black hole accretion process. The X-ray spectrum, the number of X-rays at different energies, showed that the speed and density of the wind from J1655's disk corresponded to computer simulation predictions for magnetically-driven winds. The spectral fingerprint also ruled out the two other major competing theories to winds driven by magnetic fields. "In 1973, theorists came up with the idea that magnetic fields could drive the generation of light by gas falling onto black holes," said co-author John Raymond of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. "Now, over 30 years later, we finally may have convincing evidence." Evidence for Wind in the GRO J1655-40 Spectrum Evidence for Wind in the GRO J1655-40 Spectrum This deeper understanding of how black holes accrete matter also teaches astronomers about other properties of black holes, including how they grow. "Just as a doctor wants to understand the causes of an illness and not merely the symptoms, astronomers try to understand what causes phenomena they see in the Universe," said co-author Danny Steeghs also of the Harvard-Smithsonian Center for Astrophysics. "By understanding what makes material release energy as it falls onto black holes, we may also learn how matter falls onto other important objects." In addition to accretion disks around black holes, magnetic fields may play an important role in disks detected around young sun-like stars where planets are forming, as well as ultra-dense objects called neutron stars. NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the agency's Science Mission Directorate. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center, Cambridge, Mass. Additional information and images can be found at: http://chandra.harvard.edu and http://chandra.nasa.gov

Milky Way Monster Stars in Cosmic Reality Show

NASA Astrophysics Data System (ADS)

2003-01-01

The longest X-ray look yet at the supermassive black hole at the Milky Way's center has given astronomers unprecedented access to its life and times. The new data from NASA's Chandra X-ray Observatory revealed that our galaxy's central black hole is a frequent bad actor, prone to numerous outbursts and occasional large explosions. The observations of the black hole, a.k.a. Sagittarius A* or Sgr A*, occurred over a two-week period for a total exposure time of 164 hours. During this time Sgr A* flared up in X-ray intensity half a dozen or more times. Astronomers also found evidence that suggests it had an even more boisterous past. These discoveries will help to unlock the secrets of how Sgr A* grows and how it interacts with its environment "We are getting a look at the everyday life of a supermassive black hole like never before," said Frederick K. Baganoff of the Massachusetts Institute of Technology in Cambridge, who presented these new results on behalf of an international team at a press conference today at the American Astronomical Society meeting in Seattle. "We see it flaring on an almost daily basis." Sagittarius A* More images of Sagittarius A* The cause of the flares is not understood, but the rapidity with which they rise and fall indicates that they are occurring near the event horizon, or point of no return, around the black hole. Even when it flares, the intensity of the X-ray emission from the vicinity of the black hole is relatively weak, which suggests that Sgr A*, weighing in at 3 million times the mass of the Sun, is a starved black hole. "Although it appears to snack often, this black hole is definitely on a severe diet," says Baganoff. "This could be because explosive events in the past blew away much of the gas from the neighborhood of the black hole." Indeed, evidence for such events - which astronomers are viewing 26,000 years later due to the time it takes light to travel to Earth from the center of the Galaxy - can be found in the image. A faint streak of X-rays about 1 light-year long has been discovered 1.5 light years from Sgr A*. The streak points at Sgr A*, suggesting that it may be a jet of particles expelled at nearly the speed of light from just outside the event horizon of the black hole. The intensity and size of this jet indicate that the flaring activity has been occurring for many years. Labeled image of Sagittarius A* Jet Labeled image of Sagittarius A* Jet On a much larger scale, huge lobes of 20-million-degree-Centigrade gas extending over dozens of light years on either side of the black hole have also been discovered. "These lobes show that enormous explosions have occurred several times over the last ten thousand years," said Mark Morris of UCLA, lead author of a second paper on Sgr A*, who also participated in the press conference. Sangwook Park, of Penn State University in University Park, and Michael Muno, of MIT, were lead authors of two other papers presented at the meeting. These papers focused on the extraordinarily rich region around the central black hole, where they detected more than 2,000 X-ray sources. Other members of the team include Mark Bautz and George Ricker of MIT, Niel Brandt, Patrick Broos, George Chartas, Eric Feigelson, Gordon Garmire, and Leisa Townsley of Penn State, Yoshitomo Maeda of the Institute of Space and Astronautical Science in Japan, and Christian Howard of UCLA. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program, and TRW, Inc., Redondo Beach, Calif., is the prime contractor for the spacecraft. The Smithsonian's Chandra X-ray Center controls science and flight operations from Cambridge, Mass., for the Office of Space Science at NASA Headquarters, Washington. Images and additional information about this result are available at: http://chandra.harvard.edu and http://chandra.nasa.gov

Neptune's Stormy Disposition

NASA Technical Reports Server (NTRS)

1998-01-01

Using powerful ground-and space-based telescopes, scientists have obtained a moving look at some of the wildest, weirdest weather in the solar system.

Combining simultaneous observations of Neptune made with the Hubble Space Telescope and NASA's Infrared Telescope Facility on Mauna Kea, Hawaii, a team of scientists led by Lawrence A. Sromovsky of the University of Wisconsin-Madison has captured the most insightful images to date of a planet whose blustery weather -- monster storms and equatorial winds of 900 miles per hour -- bewilders scientists.

Blending a series of Hubble images, Sromovsky's team constructed a time-lapse rotation movie of Neptune, permitting scientists to watch the ebb and flow of the distant planet's weather. And while the observations, presented here at a meeting of the American Astronomical Society's Division of Planetary Science, are helping scientists tease out clues to the planet's stormy weather, they also are deepening some of Neptune's mysteries, said Sromovsky.

The weather on Neptune, the eighth planet from the sun, is an enigma to begin with. The mechanism that drives its near-supersonic winds and giant storms has yet to be discerned.

On Earth, weather is driven by energy from the sun as it heats the atmosphere and oceans. On Neptune, the sun is 900 times dimmer and scientists have yet to understand how Neptune's weather-generating machinery can be so efficient.

'It's an efficient weather machine compared to Earth,' said Sromovsky. 'It seems to run on almost no energy.'

In an effort to dissect the distant planet's atmosphere and monitor its bizarre weather, Sromovsky and his colleagues obtained a series of measurements and images over the span of three of Neptune's rotations.

From those observations, Sromovsky said it is possible to measure Neptune's circulation and view a 'strange menagerie of variable, discrete cloud features and zonal bands' of weather. Moreover, the new observations enabled Sromovsky's team to probe some of the deeper features of the atmosphere and to map Neptune's cloud tops.

'We can show some clouds are higher than others, that altitudes vary,' he said. Knowing something about the topography of Neptune's clouds, provides a direct way to measure Neptune's powerful winds.

A looming mystery, he said, is the fate of huge dark spots, possibly giant storms. When the planetary probe Voyager visited Neptune in 1989, it detected the Great Dark Spot, a pulsating feature nearly the size of the Earth itself. Two years ago, Hubble observations showed the spot had disappeared, and that another, smaller spot had emerged. But instead of growing to a large-scale storm like the Great Dark Spot, the new spot appears to be trapped at a fixed latitude and may be declining in intensity, said Sromovsky, a senior scientist at UW-Madison's Space Science and Engineering Center.

'They behave like storms, and the Great Dark Spot was an exaggerated features we haven't seen on any other planet. They seem to come and go, and rather than an exciting development of these dark spots, they dissipate.'

Another strange aspect of the distant planet's weather are distinct bands of weather that run parallel to the Neptunian equator. The weather bands encircle the planet and, in some respects, may be similar to the equatorial region of the Earth where tropical heat provides abundant energy to make clouds.

'We can see regions of latitude where Neptune consistently generates bright clouds,' said Sromovsky. The regions are both above and below the planet's equator, but he added that it was uncertain what their explanation is in terms of atmospheric circulation.

Sromovsky said that compared to the look provided by the Voyager spacecraft, Neptune is a different place: 'The character of Neptune is different from what it was at the time of Voyager. The planet seems stable, yet different.'

Sromovsky's Hubble observations were made with Wide Field Planetary Camera 2 and the Near Infrared Camera and Multi-Object Spectrometer. The different instruments allowed observations to be made in a variety of wavelengths, each providing a different set of information about Neptune's clouds, their structures and how they circulate.

A Connection Between Corona and Jet

NASA Astrophysics Data System (ADS)

Kohler, Susanna

2017-03-01

The structure immediately around a supermassive black hole at the heart of an active galaxy can tell us about how material flows in and out of these monsters but this region is hard to observe! A new study provides us with clues of what might be going on in these active and energetic cores of galaxies.In- and OutflowsIn active galactic nuclei (AGN), matter flows both in and out. As material flows toward the black hole via its surrounding accretion disk, much of this gas and dust can then be expelled from the vicinity via highly collimated jets.Top: The fraction of X-rays that is reflected decreases as jet power increases. Bottom: the distance between the corona and the reflecting part of the disk increases as jet power increases. [Adapted from King et al. 2017]To better understand this symbiosis between accretion and outflows, we examine whats known as the corona the hot, X-ray-emitting gas thats located in the closest regions around the black hole. But because the active centers of galaxies are generally obscured by surrounding gas and dust, its difficult for us to learn about the structure of these inner regions near the black hole.Where are the X-rays of the corona produced: in the inner accretion flow, or at the base of the jet? How far away is this corona from the disk? And how does the coronas behavior relate to that of the jet?Reflected ObservationsTo address some of these questions, a group of scientists led by Ashley King (Einstein Fellow at Stanford University) has analyzed X-ray observations from NuSTAR and XMM-Newton of over 40 AGN. The team examined the reflections of the X-rays off of the accretion disk and used two measurements to learn about the structure around the black hole:the fraction of the coronas X-rays that are reflected by the disk, andthe time lag between the original and reflected X-rays, which reveals the distance from the corona to the reflecting part of the disk.A visualization of the authors model for an AGN. The accretion disk is red, corona is green, and jet is blue. The corona shines on the disk, causing the inner regions (colored brighter) to fluoresce, reflecting the radiation. As the accretion rate increases from the top to the bottom panel, the jet power increases and the dominant reflective part of the disk moves outward due to the ionization of the inner region (which puffs up into a torus). [Adapted from King et al. 2017]King and collaborators find two interesting relationships between the corona and the jet: there is an inverse correlation between jet power and reflection fraction, and there is a correlation between jet power and the distance of the corona from the reflecting part of the disk the disk. These observations indicate that there is a relationship between changes in the corona and jet production in AGN.Modeling the CoronaThe authors use these observations to build a self-consistent model of an AGNs corona. In their picture, the corona is located at the base of the jet and movesmildly relativistically away from the disk, propagating into the large-scale jets.As the velocity of the corona increases, more of its radiation is relativistically beamed away from the accretion disk, which decreases the fraction of X-rays that are reflected explaining the inverse correlation between jet power and reflection fraction.At the same time, the increased mass accretion further ionizesthe inner disk region, pushing the dominant reflection region to further out in the disk which explains the correlation between jet power and the distance from corona to reflection region.King and collaborators show that this model is fully consistent with the X-ray observations of the 40 AGN they examined. Future X-ray observations of the strongest radio jet sources will help us to further pin down whats happening at the heart of active galaxies.CitationAshley L. King et al 2017 ApJ 835 226. doi:10.3847/1538-4357/835/2/226

Chandra Discovers Light Echo from the Milky Way's Black Hole

NASA Astrophysics Data System (ADS)

2007-01-01

Like cold case investigators, astronomers have used NASA's Chandra X-ray Observatory to uncover evidence of a powerful outburst from the giant black hole at the Milky Way's center. A light echo was produced when X-ray light generated by gas falling into the Milky Way's supermassive black hole, known as Sagittarius A* (pronounced "A-star"), was reflected off gas clouds near the black hole. While the primary X-rays from the outburst would have reached Earth about 50 years ago, the reflected X-rays took a longer path and arrived in time to be recorded by Chandra. Variability in Chandra Images of Light Echo Variability in Chandra Images of Light Echo "This dramatic event happened before we had satellites in space that could detect it," said Michael Muno of the California Institute of Technology in Pasadena. "So, it's remarkable that we can use Chandra to dig into the past and see this monster black hole's capacity for destruction." Previously, scientists have used Chandra to directly detect smaller and more recent outbursts from the black hole. This latest outburst revealed by the X-ray echo was about 1,000 times brighter and lasted well over 1,000 times longer than any of the recent outbursts observed by Chandra. Theory predicts that an outburst from Sagittarius A* would cause X-ray emission from the clouds to vary in both intensity and shape. Muno and his team found these changes for the first time, thus ruling out other interpretations. The latest results corroborate other independent, but indirect, evidence for light echoes generated by the black hole in the more distant past. Illustrations of Light Echo Illustrations of Light Echo Scientists have long known that Sagittarius A*, with a mass of about 3 million suns, lurked at the center for Milky Way. However, the black hole is incredibly faint at all wavelengths, especially in X-rays. "This faintness implies that stars and gas rarely get close enough to the black hole to be in any danger," said co-author Frederick K. Baganoff of the Massachusetts Institute of Technology in Cambridge. "The huge appetite is there, but it's not being satisfied." During the outburst, the area close to the black hole would have been about 100,000 times brighter than it is currently. If such an outburst had occurred more recently, it likely would have been detected by an X-ray instrument, or would have produced similar features in other nearby clouds. Chandra X-ray Image of Sagittarius A* Chandra X-ray Image of Sagittarius A* "Our data show it has been 50 years or so since the black hole had its last decent meal," said Muno. "This is nothing like the feasting that black holes in other galaxies sometimes enjoy, but it gives unique knowledge about the feeding habits of our closest supermassive black hole." The details of how Sagittarius A* feeds remain unclear. For example, one possibility is that the black hole grows by pulling in matter from the winds of nearby young stars. Also, if there is a disk of material swirling around Sagittarius A*, it might be unstable in such a way that material migrates toward the black hole's edge in clumps, emitting X-rays before disappearing from the universe forever. The theoretical work is still being developed. Studying this light echo is also important because it illuminates and probes the poorly understood molecular clouds near the center of the galaxy. In particular, it gives information about the dense cores of these clouds where new stars may be forming. Variability in the X-ray emission between three Chandra observations in 2002, 2004 and 2005 argues against an alternate source for the light echo, which is that it came from a neutron star or black hole pulling matter away from a binary companion. This explanation is not favored because the data show the outburst would have been unusually long and bright for such a binary. These results were presented at the American Astronomical Society meeting in Seattle, Wash., and will appear in an upcoming issue of The Astrophysical Journal Letters. NASA's Marshall Space Flight Center, Huntsville, Ala., manages the Chandra program for the agency's Science Mission Directorate. The Smithsonian Astrophysical Observatory controls science and flight operations from the Chandra X-ray Center, Cambridge, Mass. Additional information and images are available at: http://chandra.harvard.edu and http://chandra.nasa.gov

ESO PR Highlights in 2005

NASA Astrophysics Data System (ADS)

2006-01-01

2005 was the year of Physics. It was thus also in part the year of astronomy and this is clearly illustrated by the numerous breakthroughs that were achieved, in particular using ESO's telescopes. One of the highlights was without any doubt the confirmation of the first image of an exoplanet , around the star 2M1207 (see ESO PR 12/05). ESO's telescopes also found a Neptune-mass exoplanet around a small star ( PR 30/05) - a discovery that proves crucial in the census of other planetary systems, and imaged a tiny companion in the close vicinity of the star GQ Lupi, a very young object still surrounded by a disc, with an age between 100,000 and 2 million years ( PR 09/05). Moreover, using a new high-contrast adaptive optics camera on the VLT, the NACO Simultaneous Differential Imager, or NACO SDI, astronomers were able for the first time to image a companion 120 times fainter than its star , very near the star AB Doradus A. This companion appears to be almost twice as heavy as theory predicts it to be ( PR 02/05). ESO's telescopes proved very useful in helping to solve a 30-year old puzzle . Astronomers have for the first time observed the visible light from a short gamma-ray burst (GRB). Using the 1.5m Danish telescope at La Silla (Chile), they showed that these short, intense bursts of gamma-ray emission most likely originate from the violent collision of two merging neutron stars ( PR 26/05). Additional evidence came from witnessing another event with the VLT ( PR 32/05). Also in this field, astronomers found the farthest known gamma-ray burst with ESO's VLT, observing an object with a redshift 6.3, i.e. that is seen when the Universe was less than 900 million years old ( PR 22/05). On July 4, NASA's Deep Impact spacecraft plunged onto Comet 9P/Tempel 1 with the aim to create a crater and expose pristine material from beneath the surface. For two days before and six days after, all major ESO telescopes have been observing the comet, in a coordinated fashion and in very close collaboration with the space mission' scientific team, in what was perhaps the most comprehensive ground-observing campaign of a celestial object. On this occasion, a dedicated Deep Impact at ESO web site was created, reporting on all the developments. This was not the sole contribution of ESO to the study of the solar system . The NACO SDI instrument was used to obtain outstanding images of Titan, the satellite of Saturn ( PHOT 04/05) and NACO also allowed astronomers to discover the first triple asteroid - two small asteroids orbiting a larger one known since 1866 as 87 Sylvia ( PR 21/05). 2005 was also a very important year for sub-millimetric astronomy at ESO. In July, APEX , the 12-m Atacama Pathfinder Experiment's telescope had first light ( PR 18/05) and since then, has been performing regular science observations ( PR 25/05). Moreover, two major contracts have been signed for ALMA , the Atacama Large Millimeter Array project, among which the largest-ever European industrial contract for a ground-based astronomy project ( PR 31/05 and 34/05). ESO's Very Large Telescope (VLT) proves to be a very efficient science machine that reached in April 2005, the count of more than 1000 scientific papers (see ESO PR 11/05) and the trend does not seem to change, as about 350 papers were published in 2005 based on data collected with the VLT. This efficiency was also recognised worldwide as ESO received the ComputerWorld Honors Program 21st Century Achievement Award in the Science Category ( PR 16/05). The interferometric mode of the VLT (VLTI) was able to observe with unprecedented detail the environment of two stars ( PR 29/05). The VLTI has also seen another extension of its already impressive capabilities by combining interferometrically the light from two relocatable 1.8-m Auxiliary Telescopes ( PR 06/05). ESO PR Highlights 2005 In 2005 again, many nice, amazing astronomical images have been obtained with ESO's telescopes: the super star cluster Westerlund 1 ( PR 08/05), the blob in the LMC ( PHOT 12/05), dream galaxies ( PHOT 24/05), a colossal cosmic eye ( PHOT 31/05), a monster being fed (PHOT 33/05), a perturbed family ( PHOT 34/05), and a cosmic Christmas ghost ( PHOT 42/05). All this, in addition to some images of the observatories ( PR 33/05 and PHOT 43/05). These developments are described in ESO's Press Releases, most with Press Photos, cf. the 2005 PR Index. Some of last year's ESO PR highlights may be accessed directly via the first clickable image above while some of the Press Photos are available via the second clickable image.

NEWS: A trip to CERN

NASA Astrophysics Data System (ADS)

Ellison, A. D.

2000-07-01

Two years ago John Kinchin and myself were lucky enough to attend the Goldsmith's particle physics course. As well as many interesting lectures and activities, this course included a visit to CERN. To most physics teachers CERN is Mecca, a hallowed place where gods manipulate and manufacture matter. The experience of being there was even better. Alison Wright was an enthusiastic and very knowledgeable host who ensured the visit went smoothly and we all learned a lot. While we were there, John and I discussed the possibility of bringing a party of A-level students to see real physics in action. In February of this year we managed it. 33 students from two schools, Boston Grammar School and Northampton School for Boys, and four staff left England and caught the 2 am ferry to France. Many hours and a few `short cuts' later we arrived at our hotel in St Genis, not far from CERN. The first day was spent sight-seeing in Lausanne and Geneva. The Olympic museum in Lausanne is well worth a visit. Unfortunately, the famous fountain in Geneva was turned off, but then you can't have everything. The following morning we turned up at CERN late due to the coach's brakes being iced up! We were met once again by Alison Wright who forgave us and introduced the visit by giving an excellent talk on CERN, its background and its reason for existing. At this point we met another member of our Goldsmith's course and his students so we joined forces once again. We then piled back into the coach to re-cross the border and visit ALEPH. ALEPH is a monster of a detector 150 m below ground. We divided into four groups, each with a very able and knowledgeable guide, and toured the site. The size and scale of the detector are awesome and the students were suitably impressed. We repeated the speed of sound experiment of two years ago at the bottom of a 150 m concrete shaft (320 m s-1), posed for a group photo in front of the detector (figure 1) and returned to the main site for lunch in the canteen. Over lunch we mixed with physicists of many different nationalities and backgrounds. Figure 1 Figure 1. In the afternoon we visited Microcosm, the CERN visitors centre, and the LEP control room and also the SPS. Here the students learned new applications for much of the physics of standing waves and resonance that they had been taught in the classroom. Later that night, we visited a bowling alley where momentum and collision theory were put into practice. The following morning we returned to CERN and visited the large magnet testing facility. Here again physics was brought to life. We saw superconducting magnets being assembled and tested and the students gained a real appreciation of the problems and principles involved. The afternoon was rounded off by a visit to a science museum in Geneva - well worth a visit, as some of us still use some of the apparatus on display. Friday was our last full day so we visited Chamonix in the northern Alps. In the morning, we ascended the Aiguille de Midi - by cable car. Twenty minutes and 3842 m later we emerged into 50 km h-1 winds and -10 °C temperature, not counting the -10 °C wind chill factor. A crisp packet provided an unusual demonstration of the effects of air pressure (figure 2). Figure 2 Figure 2. The views from the summit were very spectacular though a few people experienced mild altitude sickness. That afternoon the party went to the Mer de Glace. Being inside a 3 million year-old structure moving down a mountain at 3 cm per day was an interesting experience, as was a tot of whisky with 3 million year-old water. Once again the local scenery was very photogenic and the click and whirr of cameras was a constant background noise. Saturday morning saw an early start for the long drive home. Most students - and some staff - took the opportunity to catch up on their sleep. Thanks are due to many people without whom the trip would never have taken place. Anne Craige, Stuart Williams, Christine Sutton and Andrew Morrison of PPARC, but most especially Alison Wright of CERN and John Kinchin of Boston Grammar School who did all the hard work and organization. The week gave students a unique chance to see the principles of physics being applied in many different ways and I am sure this has reinforced their knowledge and understanding. Some students also took the opportunity to practise their language skills. The only remaining question is: what next? I'll have to think about it in the summer when I have some slack time. Hmm, SLAC, that gives me an idea....

Chandra Finds Surprising Black Hole Activity In Galaxy Cluster

NASA Astrophysics Data System (ADS)

2002-09-01

Scientists at the Carnegie Observatories in Pasadena, California, have uncovered six times the expected number of active, supermassive black holes in a single viewing of a cluster of galaxies, a finding that has profound implications for theories as to how old galaxies fuel the growth of their central black holes. The finding suggests that voracious, central black holes might be as common in old, red galaxies as they are in younger, blue galaxies, a surprise to many astronomers. The team made this discovery with NASA'S Chandra X-ray Observatory. They also used Carnegie's 6.5-meter Walter Baade Telescope at the Las Campanas Observatory in Chile for follow-up optical observations. "This changes our view of galaxy clusters as the retirement homes for old and quiet black holes," said Dr. Paul Martini, lead author on a paper describing the results that appears in the September 10 issue of The Astrophysical Journal Letters. "The question now is, how do these black holes produce bright X-ray sources, similar to what we see from much younger galaxies?" Typical of the black hole phenomenon, the cores of these active galaxies are luminous in X-ray radiation. Yet, they are obscured, and thus essentially undetectable in the radio, infrared and optical wavebands. "X rays can penetrate obscuring gas and dust as easily as they penetrate the soft tissue of the human body to look for broken bones," said co-author Dr. Dan Kelson. "So, with Chandra, we can peer through the dust and we have found that even ancient galaxies with 10-billion-year-old stars can have central black holes still actively pulling in copious amounts of interstellar gas. This activity has simply been hidden from us all this time. This means these galaxies aren't over the hill after all and our theories need to be revised." Scientists say that supermassive black holes -- having the mass of millions to billions of suns squeezed into a region about the size of our Solar System -- are the engines in the cores of bright active galaxies, often referred to as Active Galactic Nuclei, or AGN. Many astronomers think that all galaxies have central, supermassive black holes, yet only a small percent show activity. What is needed to power the AGN is fuel in the form of a nearby reservoir of gas and dust. Galaxy clusters contain hundreds to thousands of galaxies. They are the largest known structures in the universe and serve as a microcosm for the mechanics of the Universe at large. The galaxies in clusters are often old, reddish elliptically shaped galaxies, distinct from blue, spiral galaxies like our own. These old galaxies also do not have many young stars. The theory now in question is that as galaxies enter into clusters at high speeds, they are stripped of their interstellar gas, much as a strong wind strips leaves from a tree. Galaxies may also collide with one another and use up all of their gas in one huge burst of star formation triggered by this interaction. These processes remove most, if not all, of the gas that isn't locked up in stars. As they no longer have the raw material to form new stars, the stellar population slowly gets old and the Galaxy appears red. No gas is left to fuel an AGN. Previous surveys of galaxy clusters with optical telescopes have found that about only one percent of the galaxies in a cluster have AGN. This latest Chandra observation if typical, however, bumps the count up to about 5 percent. The team found six red galaxies with high X-ray activity during a nearly 14-hour Chandra observation of a galaxy cluster named Abell 2104, over 700 million light years from Earth. Based on previous optical surveys, only one was expected. "If we relied on optical data alone, we would have missed these hidden monsters," said co-author Dr. John Mulchaey. Only one of the six AGN, in fact, had the optical spectral properties typical of AGN activity. "The presence of these AGN indicate that supermassive black holes have somehow retained a fuel source, despite the harsh treatment galaxies suffer in clusters, and are now coming out of retirement," said Martini. This could imply that galaxies are better at holding onto a supply of gas and dust than previously thought, particularly deep down at their cores near the supermassive black hole. This gas and dust may also be the same material that obscures the AGN at other wavelengths. The presence of so many AGN could also contribute to the radio and infrared radiation from the clusters, which until now was thought to be almost exclusively a product of star formation. Thus, scientists may be overestimating the amount of star formation taking place in clusters. The Carnegie group has begun a study of other galaxy clusters with Chandra. Martini and Kelson are postdoctoral researchers at the Carnegie Observatories in Pasadena; Mulchaey is a staff astronomer. NASA's Marshall Space Flight Center in Huntsville, Ala., manages the Chandra program, and TRW, Inc., Redondo Beach, Calif., is the prime contractor. The Smithsonian's Chandra X-ray Center controls science and flight operations from Cambridge, Mass.

ESO Highlights in 2008

NASA Astrophysics Data System (ADS)

2009-01-01

As is now the tradition, the European Southern Observatory looks back at the exciting moments of last year. 2008 was in several aspects an exceptionally good year. Over the year, ESO's telescopes provided data for more than 700 scientific publications in refereed journals, making ESO the most productive ground-based observatory in the world. ESO PR Highlights 2008 ESO PR Photo 01a/09 The image above is a clickable map. These are only some of the press releases issued by ESO in 2008. For a full listing, please go to ESO 2008 page. Austria signed the agreement to join the other 13 ESO member states (ESO 11/08 and 20/08), while the year marked the 10th anniversary of first light for ESO's "perfect science machine", the Very Large Telescope (ESO 16/08 and 17/08). The ALMA project, for which ESO is the European partner, had a major milestone in December, as the observatory was equipped with its first antenna (ESO 49/08). Also the Atacama Pathfinder Experiment (APEX) telescope impressed this year with some very impressive and publicly visible results. Highlights came in many fields: Astronomers for instance used the Very Large Telescope (VLT) to discover and image a probable giant planet long sought around the star Beta Pictoris (ESO 42/08). This is now the eighth extrasolar planet to have been imaged since the VLT imaged the first extrasolar planet in 2004 (three of eight were imaged with VLT). The VLT also enabled three students to confirm the nature of a unique planet (ESO 45/08). This extraordinary find, which turned up during their research project, is a planet about five times as massive as Jupiter. This is the first planet discovered orbiting a fast-rotating hot star. The world's foremost planet-hunting instrument, HARPS, located at ESO's La Silla observatory, scored a new first, finding a system of three super-Earths around a star (ESO 19/08). Based on the complete HARPS sample, astronomers now think that one Sun-like star out of three harbours short orbit, low-mass planets. With the VLT and another recent instrument, CRIRES, astronomers have also been able to study planet-forming discs around young Sun-like stars in unsurpassed detail, clearly revealing the motion and distribution of the gas in the inner parts of the disc, possibly implying the presence of giant planets (ESO 27/08). As the result of an impressive 16-year long study, that combines data obtained with ESO's New Technology Telescope and the VLT, a team of German astronomers has produced the most detailed view ever of the surroundings of the monster lurking at our Galaxy's heart -- a supermassive black hole (ESO 46/08). Combining data from APEX and the VLT, another team studied the violent flares coming from this region (ESO 41/08). The flares are the likely signatures of material being torn apart by the black hole. Making such science discoveries doesn't happen without the best technological tools. ESO is constantly upgrading its battery of instruments and telescopes on Cerro Paranal, home of the VLT. For example, the PRIMA instrument for the VLT Interferometer (VLTI) recently saw first light (ESO 29/08). When fully operational, PRIMA will boost the capabilities of the VLTI to see sources much fainter than any previous interferometers, and determine positions on the sky better than any other existing astronomical facility. The Multi-Conjugate Adaptive Optics Demonstrator (MAD) prototype, mounted on the VLT, provided astronomers with the sharpest image of the full disc of planet Jupiter ever taken from the Earth's surface (ESO 33/08). The future VISTA telescope on Paranal also received its record-curved 4.1-metre mirror, paving the way for unique surveys of the southern sky in the infrared (ESO 10/08). In preparation for other instruments of the future, staff at ESO joined with quantum optics specialists to develop a new calibration system for ultra-precise spectrographs (ESO 26/08). Given the presence of such state-of-the-art technology, it is perhaps no surprise that the crucial scenes from the latest James Bond sequel were filmed at Paranal (even though the director was really more interested in blowing up the Residencia, the lodge where staff and visitors can relax after working at one of the world's most advanced ground-based astronomical observatories). In March, a movie crew of 300 people, including the principal actors, were shooting at Paranal (ESO 007/08 and 38/08). On the outreach side, ESO's series of video podcasts, the ESOcast, premiered with the first three episodes. More than two thousand new and historic ESO images were put online in the ESO image archive as well as more than 300 hundred videos, mostly in High Definition. The work to digitise ESO's heritage will continue in 2009. Doubtless just as many exciting results will be presented this year too. Especially as 2009 has been officially declared the International Year of Astronomy (IYA) by the UN, UNESCO and the International Astronomical Union. The Year is coordinated from the global IYA Secretariat hosted by ESO. In addition ESO leads a number of global and regional activities.

Biggest Star in Our Galaxy Sits within a Rugby-Ball Shaped Cocoon

NASA Astrophysics Data System (ADS)

2003-11-01

VLT Interferometer Gives Insight Into the Shape of Eta Carinae Summary Ever since 1841, when the until then inconspicuous southern star Eta Carinae underwent a spectacular outburst, astronomers have wondered what exactly is going on in this unstable giant star. However, due to its considerable distance - 7,500 light-years - details of the star itself were beyond observation. This star is known to be surrounded by the Homunculus Nebula , two mushroom-shaped clouds ejected by the star, each of which is hundreds of times larger than our solar system. Now, for the first time, infrared interferometry with the VINCI instrument on ESO's Very Large Telescope Interferometer (VLTI) enabled an international team of astronomers [1] to zoom-in on the inner part of its stellar wind. For Roy van Boekel , leader of the team, these results indicate that " the wind of Eta Carinae turns out to be extremely elongated and the star itself is highly unstable because of its fast rotation." PR Photo 32a/03 : The Immediate Surroundings of Eta Carinae (NAOS-CONICA/YEPUN). PR Photo 32b/03 : The Highly Unstable Star Eta Carinae (Artist's Impression) A monster in the southern sky ESO PR Photo 32a/03 ESO PR Photo 32a/03 [Preview - JPEG: 549 x 400 pix - 60k [Normal - JPEG: 1098 x 800 pix - 566k] Caption : The image to the left in PR Photo 32a/03 shows the mushroom-shaped clouds, known as the Homunculus Nebula , that surround the massive star Eta Carinae (Credit: NASA/ESA HST). To the right is an image obtained with the VLT NACO adaptive-optics camera that reveals the structure of the star's immediate surroundings. The central region displays a complex morphology of luminous objects. Eta Carinae , the most luminous star known in our Galaxy, is by all standards a real monster: it is 100 times more massive than our Sun and 5 million times as luminous. This star has now entered the final stage of its life and is highly unstable. It undergoes giant outbursts from time to time; one of the most recent happened in 1841 and created the beautiful bipolar nebula known as the Homunculus Nebula (see ESO PR Photo 32a/03 ). At that time, and despite the comparatively large distance - 7,500 light-years - Eta Carinae briefly became the second brightest star in the night sky, surpassed only by Sirius. Eta Carinae is so big that, if placed in our solar system, it would extend beyond the orbit of Jupiter. This large size, though, is somewhat arbitrary. Its outer layers are continually being blown into space by radiation pressure - the impact of photons on atoms of gas. Many stars, including our Sun, lose mass because of such "stellar winds", but in the case of Eta Carinae , the resulting mass loss is enormous (about 500 Earth-masses a year) and it is difficult to define the border between the outer layers of the star and the surrounding stellar wind region. Now, VINCI and NAOS-CONICA, two infrared-sensitive instuments on ESO's Very Large Telescope (VLT) at the Paranal Observatory (Chile), have probed the shape of the stellar wind region for the first time. Looking down into the stellar wind as far as possible, the astronomers could infer some of the structure of this enigmatic object. The astronomer team [1] first used the NAOS-CONICA adaptive optics camera [2], attached to the 8.2-m VLT YEPUN telescope, to image the hazy surroundings of Eta Carinae , with a spatial resolution comparable to the size of the solar system, cf. PR Photo 32a/03 . This image shows that the central region of the Homunculus nebula is dominated by an object that is seen as a point-like light source with many luminous "blobs" in the immediate vicinity. Towards the limit In order to obtain an even sharper view, the astronomers then turned to interferometry. This technique combines two or more telescopes to achieve an angular resolution [3] equal to that of a telescope as large as the separation of the individual telescopes (cf. ESO PR 06/01 and ESO PR 23/01 ). For the study of the rather bright star Eta Carinae the full power of the 8.2-m VLT telescopes is not required. The astronomers thus used VINCI, the VLT INterferometer Commissioning Instrument [4], together with two 35-cm siderostat test telescopes that served to obtain "First Light" with the VLT Interferometer in March 2001 (see ESO PR 06/01 ). The siderostats were placed at selected positions on the VLT Observing Platform at the top of Paranal to provide different configurations and a maximum baseline of 62 meters. During several nights, the two small telescopes were pointed towards Eta Carinae and the two light beams were directed towards a common focus in the VINCI test instrument in the centrally located VLT Interferometric Laboratory. It was then possible to measure the angular size of the star (as seen in the sky) in different directions. Pushing the spatial resolution of this configuration to the limit, the astronomers succeeded in resolving the shape of the outer layer of Eta Carinae . They were able to provide spatial information on a scale of 0.005 arcsec, that is about 11 AU (1650 million km) at the distance of Eta Carinae , corresponding to the full size of the orbit of Jupiter. Scaled down to terrestial dimensions, this achievement compares to making the distinction between an egg and a billiard ball at a distance of 2,000 kilometers. A most unusual shape ESO PR Photo 32b/03 ESO PR Photo 32b/03 [Preview - JPEG: 400 x 500 pix - 28k [Normal - JPEG: 800 x 999 pix - 302k] Caption : PR Photo 32b/03 is an artist's impression of the unstable star Eta Carinae , based on the new knowledge gained from measurements with the VLT Interferometer (VLTI). The inner elongated shape is the central star, as it would be visible in the absence of the stellar wind. The larger rugby-ball shape indicates the region where the strong stellar wind becomes opaque to VINCI. The longer axis of the system is found to coincide with the direction of the bipolar outflow, both on large and small scales. The VLTI observations brought the astronomers a surprise. They indicate that the wind around Eta Carinae is amazingly elongated: one axis is one-and-a-half times longer than the other! Moreover, the longer axis is found to be aligned with the direction in which the much larger mushroom-shaped clouds (seen on less sharp images) were ejected. Spanning a scale from 10 to 20-30,000 AU, the star itself and the Homunculus Nebula are thus closely aligned in space . VINCI was able to detect the boundary where the stellar wind from Eta Carinae becomes so dense that it is no longer transparent. Apparently, this stellar wind is much stronger in the direction of the long axis than of the short axis. According to mainstream theories, stars lose most mass around their equator. This is because this is where the stellar wind gets "lifting" assistance from the centrifugal force caused by the star's rotation. However, if this were so in the case of Eta Carinae , the axis of rotation (through the star's poles) would then be perpendicular to both mushroom-shaped clouds. But it is virtually impossible that the mushroom clouds are positioned like spokes in a wheel, relative to the rotating star. The matter ejected in 1841 would then have been stretched into a ring or torus. For Roy van Boekel , " the current overall picture only makes sense if the stellar wind of Eta Carinae is elongated in the direction of its poles . This is a surprising reversal of the usual situation, where stars (and planets) are flattened at the poles due to the centrifugal force . The next supernova? Such an exotic shape for Eta Carinae-type stars was predicted by theoreticians. The main assumption is that the star itself, which is located deep inside its stellar wind, is flattened at the poles for the usual reason. However, as the polar areas of this central zone are then closer to the centre where nuclear fusion processes take place, they will be hotter. Consequently, the radiation pressure in the polar directions will be higher and the outer layers above the polar regions of the central zone will get more "puffed up" than the outer layers at the equator. Assuming this model is correct, the rotation of Eta Carinae can be calculated. It turns out that it should spin at over 90 percent of the maximum speed possible (before break-up). Eta Carinae has experienced large outbursts other than the one in 1841, most recently around 1890. Whether another outburst will happen again in the near future is unknown, but it is certain that this unstable giant star will not settle down. At the present, it is losing so much mass so rapidly that nothing will be left of it after less than 100,000 years. More likely, though, Eta Carinae will destroy itself long before that in a supernova blast that could possibly become visible in the daytime sky with the naked eye. This may happen "soon" on the astronomical time-scale, perhaps already within the next 10-20,000 years. More information The research presented in this Press Release was published as a Letter to the Editor in the European astronomy journal Astronomy and Astrophysics ("Direct measurement of the size and shape of the present-day stellar wind of Eta Carinae", by Roy van Boekel et al. , A&A 410, L37-L40). Notes [1]: The team is composed of Roy van Boekel (ESO and the University of Amsterdam, The Netherlands), Pierre Kervella, Francesco Paresce and Markus Schöller (ESO), Wolfgang Brandner , Tom Herbst and Rainer Lenzen (MPI for Astronomy, Heidelberg, Germany), Alex de Koter and Rens Waters (University of Amsterdam, The Netherlands), John Hillier (University of Pittsburgh, USA), and Anne-Marie Lagrange (Observatoire de Grenoble, France). [2]: The Nasmyth Adaptive Optics System (NAOS) has been developed by a French Consortium including the Office National d'Etudes et de Recherches Aérospatiales (ONERA), the Laboratoire d'Astrophysique de Grenoble (LAOG) and Observatoire de Paris (DESPA and DASGAL), in collaboration with ESO. The CONICA Near-Infrared CAmera has been developed by the Max-Planck-Institut für Astronomie (MPIA, Heidelberg) and the Max-Planck-Institut für Extraterrestrische Physik (MPE, Garching), with an extensive ESO collaboration. See ESO PR 25/01. [3]: The achievable angular resolution is inversely proportional to the aperture of a telescope for single telescope observation, and to the length of the "baseline" between two telescopes for an interferometric observation. However, interferometric observations with two telescopes will improve the resolution only in the direction parallel to this baseline, while the resolution in the perpendicular direction will remain that of a single telescope. Nevertheless, the use of other telescope pairs with different baseline orientations "adds" resolution in other directions. [4]: The VINCI instrument was built under ESO contract at the Observatoire de Paris (France) and the camera in this instrument was delivered by the Max-Planck-Institute für Extraterrestrische Physik (Garching, Germany). The IR detector and the IRACE detector electronics were supplied by ESO.

Mega starbirth cluster is biggest, brightest and hottest ever seen

NASA Astrophysics Data System (ADS)

2003-10-01

Artist’s impression of the Lynx Arc hi-res Size hi-res: 4519 kb Credits: European Space Agency, NASA and Robert A.E. Fosbury (European Space Agency/Space Telescope-European Coordinating Facility, Germany) Artist’s impression of the Lynx Arc This illustration shows an artist’s impression of the so-called Lynx arc, a newly identified distant super-cluster that contains a million blue-white stars twice as hot as similar stars in our Milky Way galaxy. The Lynx arc is one million times brighter than the well-known Orion Nebula, a nearby prototypical ‘starbirth’ region visible with small telescopes. The stars in the Lynx arc are more than twice as hot as the Orion Nebula’s central stars, with surface temperatures up to 80 000°C. Though there are much bigger and brighter star-forming regions than the Orion Nebula in our local Universe, none are as bright as the Lynx arc, nor do they contain such large numbers of hot stars. The stars are so hot that a very large fraction of their light is emitted in the ultraviolet that makes the gas glow with the green and red colours illustrated here. The so-called Lynx Arc is one million times brighter than the well-known Orion Nebula, a nearby prototypical 'starbirth' region visible with small telescopes. The newly identified super-cluster contains a million blue-white stars that are twice as hot as similar stars in our Milky Way galaxy. It is a rarely glimpsed example of the early days of the Universe where furious firestorms of starbirth blazed across the skies. The spectacular cluster's opulence is dimmed when seen from Earth only by the fact that it is 12 000 million light years away. The discovery of this unique and tantalising object was the result of a systematic study of distant clusters of galaxies carried out with major X-ray, optical and infrared telescopes, including the NASA/ESA Hubble Space Telescope, ROSAT and the Keck Telescopes. Bob Fosbury, of the European Space Agency's Space Telescope-European Coordinating Facility in Germany, and a team of international co-authors report the discovery in the 20 October 2003 issue of the Astrophysical Journal. The mega-cluster of stars appears as a puzzling red arc behind a distant galaxy cluster 5400 million light-years away in the northern constellation of Lynx. The arc is the stretched and magnified image of a mysterious celestial object about 12 000 million light-years away (at a redshift of 3.36), far beyond the cluster of galaxies. This means that the remote source existed when the Universe was less than 2000 million years old. Fosbury and colleagues first tried to identify the arc by analysing the light from the object, but the team was not able to recognise the pattern of colours in the spectral signature of the remote object. While looking for matches with the colour spectrum, Fosbury realised that the light was related to that of the nearby Orion Nebula, a star-forming region in our own Milky Way. However where the Orion Nebula is powered by only four hot and bright blue stars, the Lynx Arc must contain around a million such stars! Furthermore, the spectrum shows that the stars in the Lynx Arc are more than twice as hot as the Orion Nebula's central stars, with surface temperatures up to 80 000°C. Though there are much bigger and brighter star-forming regions than the Orion Nebula in our local Universe, none are as bright as the Lynx Arc, nor do they contain such large numbers of hot stars. Even the most massive, normal nearby stars are no hotter than around 40 000°C. However, stars forming from the original, pristine gas in the early Universe can be more massive and consequently much hotter - perhaps up to 120 000°C. The earliest stars may have been as much as several hundred solar masses, but the chemical make-up of the Universe today prevents stars from forming beyond about 100 solar masses. Such 'primordial' super-hot stars are thought to be the first luminous objects to condense after the Big Bang cooled. Astronomers believe that these first 'monster' stars formed considerably earlier than the Lynx Arc - up to 1800 million years earlier. "This remarkable object is the closest we have come so far to seeing what such primordial objects might look like when our telescopes become powerful enough to see them," says Fosbury. The desire to find and study the first luminous objects in the Universe is the main scientific drive behind the construction of the NASA/ESA/CSA James Webb Space Telescope, scheduled for launch in 2011. Notes for editors The team is composed of R. A. E. Fosbury (European Space Agency/Space Telescope-European Coordinating Facility, Germany), M. Villar-Martín and A. Humphrey (University of Hertfordshire, UK), M. Lombardi and P. Rosati (European Southern Observatory, Germany), D. Stern (Institute of Geophysics and Planetary Physics, USA), R. N. Hook (ST-ECF/STScI, USA), B. P. Holden and S. A. Stanford (University of California, USA), G. K. Squires (SIRTF Science Center, USA), M. Rauch (The Observatories of the Carnegie Institution of Washington, USA) and W. L. W. Sargent (California Institute of Technology, USA). For broadcasters, animations of the discovery, interviews and general Hubble Space Telescope background footage are available from the ESA Television Service, see http://television.esa.int, and from http://www.spacetelescope.org/video/heic0312_vnr.html

Background Information on the Very Long Baseline Array

NASA Astrophysics Data System (ADS)

A continent-wide radio telescope system offering the greatest resolving power of any astronomical instrument operational today Overview: The National Science Foundation's VLBA is a system of ten identical radio-telescope antennas controlled from a common headquarters and working together as a single instrument. The radio signals received by each individual antenna contribute part of the information used to produce images of celestial objects with hundreds of times more detail than Hubble Space Telescope images. Scientific Areas: The VLBA can contribute to any astronomical research area where quality, high-resolution radio images will advance knowledge of the field. In its first five years of full operation, the VLBA has produced dramatic new information in these areas: * Stars: With the VLBA, astronomers have tracked gas motions in the atmosphere of a star other than the Sun for the first time; made the first maps of the magnetic field of a star other than the Sun; and studied the violent dances of double-star pairs in which one of the pair is a superdense neutron star or a black hole. * Protostars, star formation, and protoplanetary disks: The VLBA has provided scientists with some of the best views yet of very young stars and the complex regions in which they are born. VLBA images have shown outflows of gas from young stars and disks of material orbiting these new stars - material that later may form planetary systems. * Supernovae and Supernova Remnants: The VLBA has directly measured the expansion of a shell of exploded debris from the supernova SN 1993J, in the galaxy M81, some 11 million light-years from Earth. This has allowed scientists to learn new details about the explosion itself and its surroundings as well as calculate the distance to the supernova by using the VLBA data in conjunction with information from optical telescopes. VLBA images have shown regions of shocked gas in supernova remnants. * The Milky Way: Radio waves from extragalactic objects, such as quasars, are affected by variations in the interstellar medium of the Milky Way. By measuring these effects with the VLBA, scientists are gaining valuable information about this tenuous component of our own Galaxy. Similar studies can tell about the distribution of hydrogen gas in our Galaxy. The great resolving power of the VLBA will allow astronomers to directly measure the distance to the Milky Way's center, some 30,000 light-years away, and has detected the tiny apparent shift in its position caused by our Solar System's motion around that center. The Solar System takes more than 200 million years to complete an orbit of the Galaxy's center, but the VLBA can detect that motion in less than a month! * Other Galaxies and Active Galactic Nuclei: The sharp radio "vision" of the VLBA has allowed scientists to study other galaxies in unprecedented detail. Numerous VLBA studies have focused on active galactic nuclei - the "monsters" at the hearts of many galaxies thought to harbor supermassive black holes at their cores. The black hole is thought to be surrounded by a rotating disk of material being sucked into it, and jets of subatomic particles accelerated to nearly the speed of light by the gravitational energy of the black hole. VLBA studies have given strong support to this "standard model" of an active galactic nucleus, showing the accretion disk in several such systems, and even measuring motions in one such disk. VLBA observations also have provided strong evidence that the material in the jets may be a mixture of matter and antimatter. * Cosmology: The VLBA's resolving power has allowed the farthest direct distance measurements yet made, of galaxies up to 23 million light- years away. Farther still, the VLBA is being used to study gravitational lenses in attempts to use such lens systems to accurately measure extremely great distances, and thus to refine estimates of the size and age of the universe. VLBA observations also are being used to detect possible structure in extremely distant objects, to learn about the nature of the universe when it was but a fraction of its current age. Operations: The VLBA is operated from the National Radio Astronomy Observatory's (NRAO) Array Operations Center (AOC) in Socorro, New Mexico. The staff of the AOC also supports the Very Large Array, a system of 27 antennas 50 miles west of Socorro. The NRAO is a facility of the National Science Foundation, and its instruments, including the VLBA, are available to the scientific community on a peer-reviewed basis. Scientists whose observing proposals are successful can obtain extensive assistance from NRAO astronomers and technical staff in preparing for their observations and in processing their data after the observations. Through this process, numerous graduate students now are using the VLBA for their dissertation research. History: Construction of the VLBA began in 1986, and the last observing station was completed in 1993. Astronomical observations with the partially-completed system began in 1987. All 10 VLBA stations were used for observing the first time in May of 1993. The official opening of the VLBA was held in Socorro, NM, on August 20, 1993. The total cost of constructing the VLBA was $85 million. Stations: The VLBA has stations at: St. Croix, U.S. Virgin Islands; Hancock, New Hampshire; North Liberty, Iowa; Fort Davis, Texas; Los Alamos, New Mexico; Pie Town, New Mexico; Kitt Peak, Arizona; Owens Valley, California; Brewster, Washington; and Mauna Kea, Hawaii. Technical Data: The VLBA's 240-ton dish antennas are 25 meters (82 feet) in diameter. They are equipped with receivers capable of detecting signals at frequencies ranging from 300 MegaHertz to 86 GigaHertz in non-continuous bands. During observations, data is collected at each station and recorded on magnetic tape. Each 18,000-foot reel of this tape holds 750 GBytes of data. Following observation, the tapes are shipped to Socorro. In Socorro, the VLBA Correlator, a special-purpose digital machine that combines the signals from all antennas, can perform 750 billion mathematical operations per second. The VLBA can produce images with a resolution of less than a thousandth of a second of arc. Such resolution is the equivalent of being able to stand in New York and read a newspaper in Los Angeles. The VLBA routinely works with other radio telescopes elsewhere in the world and in space.

Exciting Message from a Dying Monster Star

NASA Astrophysics Data System (ADS)

1996-03-01

SEST Discovers First Extra-galactic SiO Maser With the help of a new and more sensitive receiver, recently installed on the 15-metre Swedish-ESO Submillimetre Telescope (SEST) at the European Southern Observatory on the La Silla mountain in Chile, a team of European astronomers [1] has succeeded in discovering the first extra-galactic silicon-monoxide (SiO) maser . It is located in the atmosphere of the largest known star in the Large Magellanic Cloud, a satellite galaxy to the Milky Way. This observational feat now opens new, exciting possibilities for the study of individual stars in other galaxies in the Local Group. The continued search for extra-galactic SiO masers is a joint project of European and Australian astronomers, to be carried on with even more advanced instruments that will become available in the near future. What is a maser ? The fact that masers exist in the Universe is one of the most unexpected discoveries made by astronomers in this century. They function according to the same principles as the better known lasers . Lasers (Light Amplified Stimulated Emission Radiators) are becoming more and more common in our daily life, for instance to read discs in CD players and to cut steel plates. Inside a laser, molecules act as an enormously powerful amplifier for light of a specific wavelength (`colour') [2]. However, this only happens when we subject the molecules to special conditions, much unlike those they would normally experience in nature. Nevertheless, exotic places do exist in the Universe where conditions are similar to those in lasers. In the 1960s, astronomers discovered that some celestial objects emit abnormally strong radio waves at a particular wavelength. In the beginning, they thought that this emission was coming from an unknown molecule they called `Mysterium'. Later it turned out that it originated in already known, and rather ordinary, OH-molecules of oxygen and hydrogen. In some places in space, these molecules experience the same conditions as in lasers. However, the emission that is amplified in this case is not visible light as in lasers, but rather microwave radiation [3]. They are therefore known under the name masers or Microwave Amplified Stimulated Emission Radiators. This radiation is not visible to the human eye or optical astronomical detectors, but must be captured with astronomical radio telescopes. Later, silicon-monoxide (SiO) masers were discovered in which the molecules that amplify the microwave emission are made up of equal proportions of silicon (Si) and oxygen (O). The discovery of the first extra-galactic SiO maser In May 1995, new state-of-the-art receivers were installed on the Swedish-ESO Submillimetre Telescope (SEST) , a radio dish measuring 15 metres across at the ESO La Silla Observatory in Chile. The great technical improvement of the receivers and the excellent quality of this observing site and of the telescope itself make it one of the world's most powerful instruments for this type of research. And indeed, immediately after the installation of the new receivers, the first observations bore fruit. The astronomers decided to look with the telescope at the Large Magellanic Cloud (LMC), a satellite galaxy to the Milky Way galaxy in which we live. On a dark night in the Southern Hemisphere, one can easily spot the LMC with the naked eye as a little `cloud', seen in the direction of the southern constellation of Doradus (The Goldfish). Although much smaller than the Milky Way, it still contains many millions of stars. The astronomers chose to observe the largest known star in the LMC and they registered its microwave radiation for no less than 26 hours. Most of the observing was done during daytime, which is possible with this type of instrument: at microwave wavelengths, the sky appears dark even during the day. The astronomers were delighted to see the star shining at microwave wavelengths, cf. ESO Press Photo 16/96. The measured wavelength leaves no doubt that this is radiation from a SiO maser in the atmosphere of the star. If it would not have been a maser, it would have been far too weak to have been detected. Although we know several hundred masers of this type in the Milky Way, this is the first discovery of a SiO maser in another galaxy than our own . Since then, the observations have been continued in collaboration with Australian astronomers, using radio telescopes at Parkes and Mopra on that continent. A most unusual star When Swedish astronomer Bengt Westerlund and his colleagues first observed this LMC maser star in 1981 with optical telescopes, they thought that it was a rather normal, cool and not particularly bright star. However, a few years later, the Dutch-British-USA InfraRed Astronomical Satellite (IRAS) revealed its true nature. The IRAS measurements showed that the star radiates most of its light in the form of infrared radiation [4], making it one of the most powerful stars in the LMC; in fact, it emits about half a million times more energy than the Sun. On this occasion, it was given the designation IRAS 04553-6825 , the number indicating its position in the sky. IRAS 04553-6825 is unusual in other ways. It is some fifty times as heavy as our Sun, and it is the biggest known star in the LMC: if it were to take the place of our Sun, it would fill the solar system out to the planet Neptune, thirty times the distance from the Earth to the Sun. It is rather cool when compared to other stars - although it still has a temperature of about 2,000 C - and it therefore has a very red colour [5]. This Press Release is accompanied by ESO Press Photo 15/96 which demonstrates that while the star is hardly visible in blue light, it shines brightly in red and infrared light. Stars like IRAS 04553-6825 are known as red supergiants. It has been unofficially dubbed `The Monster', and having reached the end of a short and hectic life, it is now dying. The nuclear reactions deep inside are undergoing important changes at an ever-increasing rate and in the course of this process the star has swollen to its present, enormous size. Moreover, IRAS 04553-6825 is now blowing away its atmosphere. It loses material at a prodigious rate: each month, the equivalent of one Earth mass disappears into the surrounding space, at velocities of up to 25 kilometers per second. Were the mass-loss to continue in this way, the star would soon evaporate completely. It may never get that far, though. There is little doubt that, much before, it will end its life by exploding as a bright supernova. In February 1987, another star in the LMC exploded as a supernova, becoming as bright as the combined light of all the stars in the entire LMC. In fact, IRAS 04553-6825 might already have exploded some time ago, but due to the finite velocity of light - it takes the light 170,000 years to travel the distance from the LMC to us - the message about its fiery death may not have reached us yet. Our Sun is not expected to die this way; the death as a brilliant supernova is reserved for much heavier stars. Stellar dust and the existence of life Billions of years ago, the silicate-rich minerals that now make up most of the rocks and sand on Earth surrounded another dying star, similar to IRAS 04553-6825 . These minerals contain the silicon-oxide molecules which were then illuminated by the light of the red supergiant star and had shone brightly as SiO masers before they condensed into dust and were blown away into space. After many millions, perhaps even billions of years, they finally ended up in the rocks of planet Earth. Not only rocks and sand, but all things we use in daily life ultimately owe their existence to stars like IRAS 04553-6825 , ranging from the food we eat to the air we breathe, from the bicycle we drive to the brain in our head. This is because massive stars such as IRAS 04553-6825 produce heavy elements like oxygen, iron and carbon. We consist of these elements, and almost everything we use is made up of these elements as well. IRAS 04553-6825 is now blowing away matter from its atmosphere and thereby enriches the Universe with heavy elements. The outflowing gas gradually cools, and at a certain distance from the star it begins to condense into dust grains, a process that resembles the formation of droplets in clouds in the Earth's atmosphere. In particular, the SiO molecules in the atmosphere end up in dust grains in this way. The gas and dust expelled by IRAS 04553-6825 is then mixed with the material in the space between the stars. From this material, new stars form. Around some of these young stars planets will form. It is not excluded that some of these planets may be similar to the Earth, and may even harbour life. On the accompanying ESO Press Photo 15/96 , we see huge nebulae near the maser star; they are interstellar gas clouds that shine by the light of the embedded stars. IRAS 04553-6825 was born a few million years ago of the material in one of these nebulae. Now the rapidly outflowing material from this star (the stellar wind) is mixing with the gas cloud. This may trigger the formation of new stars a bit further away in the brightest parts of the nebulae. Dying stars like IRAS 04553-6825 are the main factories of dust in the Universe. It is an interesting thought that without these stars, there would be no dust. Without dust, there would be no planets. Without planets, there would be no life. We therefore owe our very existence to the mass-loss from these big, cool, dying stars. What does the study of SiO masers tell us ? We do not yet fully understand the processes by which a star like IRAS 04553-6825 loses its material into space. The mechanism that is responsible for the mass loss must be active near the surface of the star. However, mass-losing stars are very difficult to observe in visible light, because they quickly become obscured by the dust forming in their own stellar wind. Blue and yellow light is more absorbed than red light and therefore penetrates less through this dust. The absorbed energy is re-radiated by the dust as infrared radiation; this is why IRAS 04553-6825 shines so brightly in the infrared spectral region, resulting in its detection by IRAS. SiO maser radiation originates from close to the stellar surface, where the matter is being ejected by the star. The maser radiation is intense, and we can observe it because the surrounding dust is nearly transparent at microwave wavelengths. By observing the SiO maser radiation we can therefore study how the star expels its material. SiO masers emit the amplified radiation at a specific wavelength. However, if the molecules are moving towards us or away from us, we receive this radiation at a slightly different wavelength. This is the usual Doppler effect, analogous to the change in sound pitch you hear when a train or an ambulance approaches and then recedes. By measuring very accurately the wavelength of a SiO maser, it is therefore possible to determine with high precision the velocity of the material. With modern instruments, an accuracy of about 100 metres per second may be reached. This may not seem very much, but there are no other methods to measure the velocity in a star inside a dense dust cloud with such a precision. Moreover, when compared with the velocity of the outflowing material - typically between one and thirty kilometres per second - this accuracy is still quite sufficient to study the motion of the material close to the stellar surface in great detail. Future observations In the future, the 26-hour observation of the first extra-galactic SiO maser is expected to be followed by the discovery of many other SiO masers in galaxies in the Local Group, especially as the instrumentation continues to improve. By combining several telescopes into an array, the observational limit may be pushed to stars at a distance of about 2 million light-years, i.e. just about to the distance of the Andromeda nebula, a galaxy that is similar to the Milky Way. Plans for this are being elaborated in Australia with the Australia Telescope (a combination of many single radio telescopes like at Mopra), as well as within ESO. When more SiO masers in the LMC will have been discovered, we will be able to study how the mass loss differs from star to star. This will help us to learn how the mass loss depends on the overall characteristics of the star, for instance its brightness or its mass. Strangely enough, it is easier to do this type of study with stars in another galaxy, despite the fact that they are much more distant than the maser stars in the Milky Way. The main reason is that it is very difficult to measure distances to individual stars in our own galaxy. And if the distance to a star is not known, many other characteristics of the star will not be known either, e.g. its total energy production (intrinsic brightness) or its mass. However, as we know the distance to the LMC, about 170,000 light-years, we also know the distance to all the maser stars, which will be detected in this small galaxy. SiO masers are extremely powerful velocity indicators for celestial objects. We can therefore use them, not only to measure the motion of the molecules in the atmospheres of stars, but also to measure the velocities of the stars themselves. A study of the velocities of many SiO masers in the Milky Way indicates how the stars move through our galaxy. From this we gain a better understanding of how the Milky Way was formed; this is one of the great mysteries present-day astronomers are very eager to solve. And in the future, we may extend this type of study to other nearby galaxies. There is indeed a great potential for important new knowledge in this exciting area of modern astronomical research ! Notes: [1] The team consists of Jacco Th. van Loon and Albert A. Zijlstra (ESO/Garching), Lars-Ake Nyman (ESO/La Silla), and Valentin Bujarrabal (Observatorio Astronomico Nacional, Madrid, Spain). [2] Depending on the wavelength (and therefore on the energy it carries), electromagnetic radiation may take form of long and short radio waves, microwave radiation, infrared radiation, visible light, ultraviolet radiation, X-rays or gamma-rays. [3] Microwave radiation is for instance used to cook meals in microwave ovens. The heating effect occurs when the radiation energy is absorbed by the water molecules in the food. [4] Infrared radiation is what we experience as `heat': we feel it, but we cannot see it. [5] Stars with different temperatures have different colours. The Sun has a temperature of about 5,500 C and looks yellow, while hotter stars look blue and cooler stars are red. Analogously, when a metal bar is heated, it first will glow reddish, then become yellow, and eventually it will shine bluish.

Messages from the Abyss

NASA Astrophysics Data System (ADS)

2003-10-01

VLT Observes Infrared Flares from Black Hole at Galactic Centre [1] Summary An international team of astronomers led by researchers at the Max-Planck Institute for Extraterrestrial Physics (MPE) in Garching (Germany) [2] has discovered powerful infrared flares from the supermassive black hole at the heart of the Milky Way . The signals, rapidly flickering on a scale of minutes, must come from hot gas falling into the black hole, just before it disappears below the "event horizon" of the monster. The new observations strongly suggest that the Galactic Centre black hole rotates rapidly . Never before have scientists been able to study phenomena in the immediate neighbourhood of a black hole in such a detail. The new result is based on observations obtained with the NACO Adaptive Optics instrument on the 8.2-m VLT YEPUN telescope and is published in this week's edition of the research journal Nature. PR Photo 29a/03 : A powerful flare from the black hole at the galactic centre. PR Photo 29b/03 : Light curve of the flare . PR Video 01/03 : A powerful flare from the black hole at the galactic centre . Flashes of light from disappearing matter ESO PR Photo 29a/03 ESO PR Photo 29a/03 [Preview - JPEG: 650 x 400 pix - 118k [Normal - JPEG: 1300 x 800 pix - 370k] ESO PR Video Clip 01/03 [MPEG] ESO PR Video Clip 01/03 [MPEG Video; 29X k] Captions : PR Photo 29a/03 and PR Video Clip 01/03 show the detection of a powerful flare from the centre of the Milky Way galaxy. These and other adaptive optics (AO) images (with resolution 0.040 arcsec in the near-infrared H-band at wavelength 1.65 µm) of the central region of the Milky Way were obtained with the NACO imager on the 8.2-m VLT YEPUN telescope at the ESO Paranal Observatory on May 9, 2003. The image covers a sky area of about 1 x 1 arcsec, corresponding to about 45 light-days at the distance of the Galactic Centre. The time (in minutes from the beginning of the data set at 6h59m24s (UT) on May 9, 2003) is shown at the upper right of each image. North is up and East to the left. The position of the 15-year orbiting star S2 (cf. ESO Press Release 17/02 ) is marked by a cross and the astrometric location of the black hole is indicated by a circle. The scene was the usual one in the VLT Control Room at the Paranal Observatory in the early morning of May 9, 2003. Groups of astronomers from different nations were sitting in front of the computer screens, pointing the four giant telescopes in different directions and recording the sparse photons from the remotest corners of the Universe. There were the usual brief exchanges of information, numbers, wavelengths, strange acronyms, but then suddenly something happened at the YEPUN desk.... " What is that star doing there? " exclaimed Rainer Schödel , one of the MPE scientists in the team working with the NACO Adaptive Optics instrument [3] that delivers razor-sharp images. He and Reinhard Genzel, leader of the team and MPE Director, were observing the Milky Way Centre, when they saw the "new" object on the screen in front of them. The astronomers were puzzled and then became excited - something unusual must be going on, there at the centre of our galaxy! And then, a few minutes later, the "star" disappeared from view. Now the scientists had little doubt - they had just witnessed, for the first time, a powerful near-infrared flare from exactly the direction of the supermassive black hole at the heart of the Milky Way , cf. PR Photo 29a/03 and PR Video Clip 01/03 . " We had been looking for infrared emission from that black hole for more than a decade " recalls another team member, Andreas Eckart of the Cologne University. " We were certain that the black hole must be accreting matter from time to time. As this matter falls towards the surface of the black hole, it gets hotter and hotter and starts emitting infrared radiation ". But no such infrared radiation had been seen until that night at the VLT. This was the wonderful moment of breakthrough. Never before had anybody witnessed the last "scream" from matter in the deadly grip of a black hole, about to pass the point of no return towards an unknown fate. At the border ESO PR Photo 29b/03 ESO PR Photo 29b/03 [Preview - JPEG: 400 x 516 pix - 87k [Normal - JPEG: 800 x 1032 pix - 219k] Captions : PR Photo 29b/03 displays the "light curve" of a light flare from the galactic centre, as observed in the K-band (wavelength 2.2 µm) on June 16, 2003. This and a second flare discovered about 24 hours earlier show variability on a time scale of a few minutes and appear to show larger variations (arrows) with a 17-minute periodicity. The rapid variability implies that the infrared emission comes from just outside (the event horizon of) the black hole. If the periodicity is a fundamental property of the motion of gas orbiting the black hole, the Galactic Centre black hole must rotate with about half the maximum spin rate allowed by General Relativity. The present observations thus probe the space-time structure in the immediate vicinity of that event horizon. A careful analysis of the new observational data, reported in this week's issue of the Nature magazine, has revealed that the infrared emission originates from within a few thousandths of an arcsecond [4] from the position of the black hole (corresponding to a distance of a few light-hours) and that it varies on time scales of minutes ( PR Photo 29b/03 ). This proves that the infrared signals must come from just outside the so-called "event horizon" of the black hole, that is the "surface of no return" from which even light cannot escape. The rapid variability seen in all data obtained by the VLT clearly indicates that the region around this horizon must have chaotic properties - very much like those seen in thunderstorms or solar flares [5]. " Our data give us unprecedented information about what happens just outside the event horizon and let us test the predictions of General Relativity " explains Daniel Rouan , a team member from Paris-Meudon Observatory. " The most striking result is an apparent 17-minute periodicity in the light curves of two of the detected flares. If this periodicity is caused by the motion of gas orbiting the black hole, the inevitable conclusion is that the black hole must be rotating rapidly ". Reinhard Genzel is very pleased: " This is a major breakthrough. We know from theory that a black hole can only have mass, spin and electrical charge. Last year we were able to unambiguously prove the existence and determine the mass of the Galactic Centre black hole ( ESO Press Release 17/02 ). If our assumption is correct that the periodicity is the fundamental orbital time of the accreting gas, we now have also measured its spin for the first time . And that turns out to be about half of the maximum spin that General Relativity allows ". He adds: " Now the era of observational black hole physics has truly begun !" More information The results described in this ESO press release are presented in a report published today in the research journal "Nature" ("Near-IR Flares from Accreting Gas around the Supermassive Black Hole in the Galactic Centre", by Reinhard Genzel and co-authors).

Ultrabass Sounds of the Giant Star xi Hya

NASA Astrophysics Data System (ADS)

2002-05-01

First Observations of Solar-type Oscillations in a Star Very Different from the Sun Summary About 30 years ago, astronomers realised that the Sun resonates like a giant musical instrument with well-defined periods (frequencies). It forms a sort of large, spherical organ pipe. The energy that excites these sound waves comes from the turbulent region just below the Sun's visible surface. Observations of the solar sound waves (known as " helioseismology ") have resulted in enormous progress in the exploration of the interior of the Sun, otherwise hidden from view. As is the case on Earth, seismic techniques can be applied and the detailed interpretation of the observed oscillation periods has provided quite accurate information about the structure and motions inside the Sun, our central star. It has now also become possible to apply this technique to some solar-type stars. The first observations concerned the northern star eta Bootis (cf. ESO PR 16/94 ). Last year, extensive and much more accurate observations with the 1.2-m Swiss telescope at the ESO La Silla Observatory proved that Alpha Centauri , a solar "twin", behaves very much like the Sun (cf. ESO PR 15/01 ), and that some of the periods are quite similar to those in the Sun. These new observational data were of a superb quality, and that study marked a true break-through in the new research field of " asteroseismology " (seismology of the stars) for solar-type stars. But what about other types of stars, for instance those that are much larger than the Sun? Based on an extremely intensive observing project with the same telescope, an international group of astronomers [1] has found that the giant star xi Hya ("xi" is the small greek letter [2]; "Hya" is an abbreviation of "Hydrae") behaves like a giant sub-ultra-bass instrument . This star is located in the constellation Hydra (the Water-Monster) at a distance of 130 light-years, it has a radius about 10 times that of the Sun and its luminosity is about 60 times larger. The new observations demonstrate that xi Hya oscillates with several periods of around 3 hours. xi Hya is now approaching the end of its life - it is about to expand its outer envelope and to become a "red giant star" . It is quite different from stars like the Sun, which are only halfway through their active life. xi Hya is considerably more massive than any other star in which solar-like oscillations have so far been detected. This observational feat allows to study for the first time with seismic techniques the interior of such a highly evolved star. It paves the way for similar studies of different types of stars. A new chapter of stellar astrophysics is now opening as asteroseismology establishes itself as an ingenious method that is able to revolutionise our detailed understanding of stellar interiors and the overall evolution of stars . PR Photo 13a/02 : Oscillation frequencies in the Giant Star xi Hya PR Photo 13b/02 : Non-radial oscillations of xi Hya (computer graphics) PR Audio Clip 01/02 : Listen to the sound of xi Hya (RealMedia and MP3) The difficult art of asteroseismology Helioseismology (seismology of the Sun) is based on measurements of the changing radial velocity of the solar upper atmospheric layers (the "surface") by means of the well-known Doppler effect, as this surface moves up and down during acoustic oscillations. The corresponding amplitudes are very small, with velocities of up to 15 - 20 cm/sec, and the typical period is around 5 minutes. Therefore the phenomenon was first known as the "five-minute oscillations". Intensity measurements have also been tried, but the noise level is larger than for velocity data due to the presence of "granulation" (moving cells of hot gas) on the solar surface. In the case of larger and brighter stars like the giant stars, the corresponding amplitudes and periods increase. For instance, theoretical predictions for the giant star xi Hya have indicated that velocity amplitudes of about 7 m/sec and periods of the order of 3 - 4 hours could be expected. Observations of such oscillations are much more difficult, because the demands on the performance of the spectrograph increase dramatically, as this timescale is similar to that of variations of conditions in the Earth's atmosphere during the observing night. Spurious instrumental effects, like mechanical flexure, would be detrimental to such demanding observations. However, the experience from the search for exoplanets orbiting other stars - by observing the periodic change in velocity of the parent star due to the weak pull of the orbiting planet over even longer timescales - has proven to be very useful. Indeed, asteroseismology has benefitted greatly from the development of accurate techniques now employed in the search for exoplanets . The observations of the giant star xi Hya An international team of astronomers [1] observed xi Hya with the Swiss 1.2-m Euler telescope at the ESO La Silla Observatory (Chile). They used the CORALIE spectrograph, which is well known for numerous discoveries of exoplanets (cf. PR 07/01 ), and recently for the detection of 7-min acoustic oscillations in the solar-twin star Alpha Centauri A (cf. PR 15/01 ). The same technique that delivered superb observations of Alpha Centauri A was employed to investigate the oscillations of xi Hya . The sound waves make the surface of the star oscillate periodically in and out, and the CORALIE spectrograph measures the velocities of the up-down motion. As xi Hya is a giant, these waves need more time to propagate through the stellar interior up to the stellar surface than they do in a solar-like star. Thus, the generated oscillations of the surface are slower. An observing campaign lasting no less than one full month, taking about two measurements every hour was necessary to detect the tiny movements of the surface of xi Hya . The detected oscillations have periods of about 3 hours, and have speeds of only up to 2 metres per second . This is somewhat smaller than expected, but the predictions for these amplitudes were very uncertain as the conditions in xi Hya are so very different from those in the Sun. First results for xi Hya ESO PR Photo 13a/02 ESO PR Photo 13a/02 [Preview - JPEG: 492 x 400 pix - 68k] [Normal - JPEG: 983 x 800 pix - 168k] Caption : PR Photo 13a/02 shows the "frequency spectrum" of the giant star xi Hya , as deduced on the basis of extensive velocity measurements with the 1.2-m Leonhard Euler telescope at the ESO La Silla Observatory (Chile). The abscissa unit is microHertz; 100 µHz corresponds to a period of 10,000 seconds (2.78 hours). PR Audio Clip 01/02 : Listen to the sound of xi Hya ! This 15-sec audio clip was produced by mixing the 16 strongest frequencies in the observed sound spectrum ( PR Photo 13a/02 ) with the correct, relative amplitudes. In order to render the signal audible, all frequencies were multiplied by a factor of one million. Note that quality loudspeakers are required to fully appreciate this rich and complex signal, especially the underlying bass tones. Several beat frequencies are obviously present. Available in RealMedia (requires RealPlayer software) and MP3 (264k) formats. PR Photo 13a/02 shows the frequency spectrum of xi Hya , based on these extensive observations. The "power peaks" indicate the frequencies of the oscillation of the stellar atmosphere. The broad distribution means that several different sound waves are clearly present. This is the first time such a spectrum has ever been obtained for a giant star. A first analysis showed the presence of about one dozen significant frequencies and correspondingly, periods . Among those, four have amplitudes above 1 metre per second. In addition to these twelve frequencies, others appear to have been detected as well, but with less certainty and their reality must be confirmed by a subsequent, more detailed study. The "sound of xi Hya" has been synthesized in PR Audio Clip 01/02 . Stellar models A good model of the star is necessary before the observed oscillation frequencies (periods) can be properly interpreted. Current models of the Sun are accurate and represent a typical main-sequence star at midlife, and the oscillations are well understood. The sound spectrum corresponding to the full disk - i.e., what we would observe if the Sun were as distant as other stars and we would therefore see it as a light point in the sky - shows a regular pattern in which the observed frequencies are separated by two different and constant intervals, the "large" and the "small" separations. It is much more difficult to "model" the interior of a giant star as the core has changed a lot during the evolution of the star. The nuclear fuel has been exhausted, the stellar core has contracted and the envelope has expanded substantially [3]. The resulting sound spectrum has therefore also changed considerably. Now there is only a small group of oscillating modes that display the same regular pattern as seen in the Sun. They are the radial modes , pressure modes that correspond to a radial expansion and contraction of the star (up and down motion of the surface). The modes in the Sun are sound waves for which most of the oscillation energy is concentrated in the outer parts of the Sun. In stars as highly evolved as xi Hya , they partly take on the character of gravity modes in the interior of the star. Gravity modes are oscillations that move matter up and down in the gravity field, under the influence of buoyancy, with only small changes of the pressure. This is the same effect that makes an air-filled ball pop to the surface when released under water. Gravity modes are normally trapped in the stable interior inside the upper (convective) envelope of a star. So far gravity modes have not been detected in the Sun. In a giant star, however, there is a chance to see some, because some of the oscillations have a mixed character : they behave like gravity modes in the interior and like sound waves in the envelope. The nature of the oscillations observed in xi Hya ESO PR Photo 13b/02 ESO PR Photo 13b/02 [Preview - JPEG: 400 x 461 pix - 112k] [Normal - JPEG: 800 x 922 pix - 232k] Caption : PR Photo 13b/02 is a computer-generated illustration of one possible non-radial oscillation mode in the giant star xi Hya . The blue parts contain particles in the upper stellar atmosphere moving away from the stellar centre, hence they cause a "blue-shift" (towards shorter wavelengths) in the spectrum for the observer. At the same time, particles in the red parts move towards the stellar centre and cause a "red-shift" (towards longer wavelengths). Particles in the white regions do not move during the oscillation cycle. Half an oscillation cycle later, the red parts will have become blue and vice versa. The high-resolution spectra of xi Hya were also used to determine improved values of the fundamental parameters of this star: its temperature is 4950 ± 100 K, the mass is 3.31 ± 0.17 times that of the Sun, and the age is 276 ± 21 million years [3]. These values may be refined in a subsequent, more extensive analysis. With this improved model for xi Hya , the astronomers calculated the frequencies of all oscillations likely to be observed. As in the Sun, the radial modes are expected to be the dominating ones. In fact, three out of the four modes actually observed in xi Hya coincide within the errors with the predicted radial modes. The fourth mode seems not to be radial, but agrees with a non-radial mode with 2 or 3 wave peaks and valleys over the surface. PR Photo 13b/02 provides a graphical illustration of this in the case of a star seen almost equator-on. Some of the observed lower-amplitude modes must be mixed non-radial modes , since more modes are detected than can be accounted for by the radial modes of the models alone. Future plans Moving directly from stars of about one solar mass to the giant star xi Hya is a rather great leap. With the CORALIE and HARPS instruments (the latter soon to be installed on the ESO 3.6-m telescope at La Silla), an entire sequence of stars at different evolutionary stages will be observed next: from newly born to middle-aged stars like the Sun, and also old ones that are near retirement. The new observations of xi Hya show that this is now technically feasible. Once more stars have been observed, changes in the interior structure and composition can be followed and current theories of the internal stellar structure can be verified and improved. Clearly, asteroseismology is bound to have a major impact on the understanding of stellar evolution . The detection of oscillations in the giant star xi Hya also has implications for the target selection of several space missions aiming at seismic measurements: the Canadian MOST mission, the French-led European COROT mission (with launch expected in 2005), and some that are still under consideration, as the Danish Rømer mission (now in the detailed design phase) and the ESA Eddington mission. The present observations have proven that these space missions will be able to observe oscillations in a wide range of stars, and thus will constitute a major new source of detailed information about the interior of stars, not accessible from the ground. More information The results described in this Press Release are about to be submitted to the research journal Astronomy & Astrophysics (Letters) by the present team. Notes [1]: The team consists of Conny Aerts and Thomas Maas (Dept. of Physics and Astronomy, Catholic University of Leuven, Belgium), Fabien Carrier, Michel Burnet, Jose de Medeiros and Francois Bouchy (Geneva Observatory, Switzerland), Søren Frandsen, Dennis Stello, Hans Kjeldsen, Teresa C. Teixeira, Frank Pijpers, Jørgen Christensen-Dalsgaard and Hans Bruntt (Dept. of Physics and Astronomy, Aarhus University; and Theoretical Astrophysics Center, Aarhus University, Denmark). [2]: Some HTML-browsers support character entities for greek letters - "xi" is then represented by "ξ" . [3]: In astrophysical terms, xi Hya is currently in the hydrogen shell-burning phase, having left the main sequence some time ago and now near the sub-giant/giant border.

Toward Open Science at the European Scale: Geospatial Semantic Array Programming for Integrated Environmental Modelling

NASA Astrophysics Data System (ADS)

de Rigo, Daniele; Corti, Paolo; Caudullo, Giovanni; McInerney, Daniel; Di Leo, Margherita; San-Miguel-Ayanz, Jesús

2013-04-01

Interfacing science and policy raises challenging issues when large spatial-scale (regional, continental, global) environmental problems need transdisciplinary integration within a context of modelling complexity and multiple sources of uncertainty [1]. This is characteristic of science-based support for environmental policy at European scale [1], and key aspects have also long been investigated by European Commission transnational research [2-5]. Parameters ofthe neededdata- transformations ? = {?1????m} (a.5) Wide-scale transdisciplinary modelling for environment. Approaches (either of computational science or of policy-making) suitable at a given domain-specific scale may not be appropriate for wide-scale transdisciplinary modelling for environment (WSTMe) and corresponding policy-making [6-10]. In WSTMe, the characteristic heterogeneity of available spatial information (a) and complexity of the required data-transformation modelling (D- TM) appeal for a paradigm shift in how computational science supports such peculiarly extensive integration processes. In particular, emerging wide-scale integration requirements of typical currently available domain-specific modelling strategies may include increased robustness and scalability along with enhanced transparency and reproducibility [11-15]. This challenging shift toward open data [16] and reproducible research [11] (open science) is also strongly suggested by the potential - sometimes neglected - huge impact of cascading effects of errors [1,14,17-19] within the impressively growing interconnection among domain-specific computational models and frameworks. From a computational science perspective, transdisciplinary approaches to integrated natural resources modelling and management (INRMM) [20] can exploit advanced geospatial modelling techniques with an awesome battery of free scientific software [21,22] for generating new information and knowledge from the plethora of composite data [23-26]. From the perspective of the science-policy interface, INRMM should be able to provide citizens and policy-makers with a clear, accurate understanding of the implications of the technical apparatus on collective environmental decision-making [1]. Complexity of course should not be intended as an excuse for obscurity [27-29]. Geospatial Semantic Array Programming. Concise array-based mathematical formulation and implementation (with array programming tools, see (b) ) have proved helpful in supporting and mitigating the complexity of WSTMe [40-47] when complemented with generalized modularization and terse array-oriented semantic constraints. This defines the paradigm of Semantic Array Programming (SemAP) [35,36] where semantic transparency also implies free software use (although black-boxes [12] - e.g. legacy code - might easily be semantically interfaced). A new approach for WSTMe has emerged by formalizing unorganized best practices and experience-driven informal patterns. The approach introduces a lightweight (non-intrusive) integration of SemAP and geospatial tools (c) - called Geospatial Semantic Array Programming (GeoSemAP). GeoSemAP (d) exploits the joint semantics provided by SemAP and geospatial tools to split a complex D- TM into logical blocks which are easier to check by means of mathematical array-based and geospatial constraints. Those constraints take the form of precondition, invariant and postcondition semantic checks. This way, even complex WSTMe may be described as the composition of simpler GeoSemAP blocks, each of them structured as (d). GeoSemAP allows intermediate data and information layers to be more easily an formally semantically described so as to increase fault-tolerance [17], transparency and reproducibility of WSTMe. This might also help to better communicate part of the policy-relevant knowledge, often difficult to transfer from technical WSTMe to the science-policy interface [1,15]. References de Rigo, D., 2013. Behind the horizon of reproducible integrated environmental modelling at European scale: ethics and practice of scientific knowledge freedom. F1000 Research. To appear as discussion paper. Funtowicz, S. O., Ravetz, J. R., 1994. Uncertainty, complexity and post-normal science. Environmental Toxicology and Chemistry 13 (12), 1881-1885. http://dx.doi.org/10.1002/etc.5620131203 Funtowicz, S. O., Ravetz, J. R., 1994. The worth of a songbird: ecological economics as a post-normal science. Ecological Economics 10 (3), 197-207. http://dx.doi.org/10.1016/0921-8009(94)90108-2 Funtowicz, S. O., Ravetz, J. R., 2003. Funtowicz, S., Ravetz, J. (2003). Post-normal science. International Society for Ecological Economics, Internet Encyclopaedia of Ecological Economics Ravetz, J., 2004. The post-normal science of precaution. Futures 36 (3), 347-357. http://dx.doi.org/10.1016/S0016-3287(03)00160-5 van der Sluijs, J. P., 2012. Uncertainty and dissent in climate risk assessment: A Post-Normal perspective. Nature and Culture 7 (2), 174-195. http://dx.doi.org/10.3167/nc.2012.070204 Ulieru, M., Doursat, R., 2011. Emergent engineering: a radical paradigm shift. International Journal of Autonomous and Adaptive Communications Systems 4 (1), 39-60. http://dx.doi.org/10.1504/IJAACS.2011.037748 Turner, M. G., Dale, V. H., Gardner, R. H., Dec. 1989. Predicting across scales: Theory development and testing. Landscape Ecology 3 (3), 245-252. http://dx.doi.org/10.1007/BF00131542 Zhang, X., Drake, N. A., Wainwright, J., 2004. Scaling issues in environmental modelling. In: Wainwright, J., Mulligan, M. 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Dancing around the Black Hole

NASA Astrophysics Data System (ADS)

2001-08-01

ISAAC Finds "Cool" Young Stellar Systems at the Centres of Active Galaxies Summary Supermassive Black Holes are present at the centres of many galaxies, some weighing hundreds of millions times more than the Sun. These extremely dense objects cannot be observed directly, but violently moving gas clouds and stars in their strong gravitational fields are responsible for the emission of energetic radiation from such "active galaxy nuclei" (AGN) . A heavy Black Hole feeds agressively on its surroundings . When the neighbouring gas and stars finally spiral into the Black Hole, a substantial fraction of the infalling mass is transformed into pure energy. However, it is not yet well understood how, long before this dramatic event takes place, all that material is moved from the outer regions of the galaxy towards the central region. So how is the food for the central Black Hole delivered to the table in the first place? To cast more light on this central question, a team of French and Swiss astronomers [1] has carried out a series of trailblazing observations with the VLT Infrared Spectrometer And Array Camera (ISAAC) on the VLT 8.2-m ANTU telescope at the ESO Paranal Observatory. The ISAAC instrument is particularly well suited to this type of observations. Visible light cannot penetrate the thick clouds of dust and gas in the innermost regions of active galaxies, but by recording the infrared light from the stars close to the Black Hole , their motions can be studied. By charting those motions in the central regions of three active galaxies (NGC 1097, NGC 1808 and NGC 5728), the astronomers were able to confirm the presence of "nuclear bars" in all three. These are dynamical structures that "open a road" for the flow of material towards the innermost region. Moreover, the team was surprised to discover signs of a young stellar population near the centres of these galaxies - stars that have apparently formed quite recently in a central gas disk. Such a system is unstable, however, and will soon disrupt. At some moment, many of those young stars may get too close to the monster in the centre and suffer an unhappy fate... PR Photo 25a/01 : The active galaxy NGC 1097 (R-band image) PR Photo 25b/01 : The active galaxy NGC 1808 (H-band image) PR Photo 25c/01 : The active galaxy NGC 5728 (K-band image) PR Photo 25d/01 : Schematic drawing of the various structural components mentioned in the text. PR Photo 25e/01 : ISAAC spectrum (2.3 µm) of the central region of NGC 1808 PR Photo 25f/01 : Stellar motions at the centre of NGC 1808 Central black holes in galaxies ESO PR Photo 25a/01 ESO PR Photo 25a/01 [Preview - JPEG: 400 x 489 pix - 39k] [Normal - JPEG: 800 x 977 pix - 296k] ESO PR Photo 25b/01 ESO PR Photo 25b/01 [Preview - JPEG: 400 x 499 pix - 40k] [Normal - JPEG: 800 x 997 pix - 168k] ESO PR Photo 25c/01 ESO PR Photo 25c/01 [Preview - JPEG: 400 x 488 pix - 47k] [Normal - JPEG: 800 x 975 pix - 384k] Caption : Photos of three active galaxies that were observed with ISAAC during the present programme. They show NGC 1097 (R-band; Photo 25a/01) and the central areas of NGC 1808 (H-band; Photo 25b/01) and NGC 5728 (K-band; Photo 25c/01). The bar-like structures and the luminous centres where the Black Holes are located are well visible - they are discussed in the text. The distances to these galaxies are approximately 55, 35 and 120 million light-years, respectively; the local scales are indicated in the photos. Technical information about these photos is available below. Recent research with space- and ground-based astronomical telescopes indicate that there are very heavy Black Holes at the centres of most galaxies. There is also general agreement among scientists that many of the closest neighbours of our own Milky Way Galaxy, for example the large spiral Andromeda Galaxy and the peculiar Centaurus A galaxy (cf. ESO PR 04/01 ), do contain central black holes with masses from millions to billions of solar masses [2]. Black Holes have an extremely intense gravitational field and as light can not escape from them, they are dark and invisible. Indeed, with presently available observational tools, they cannot be detected directly, only by effects resulting from interaction with their immediate surroundings. A small fraction of the black holes in galaxies are thus revealed by the spectacular activity they trigger in the central part of their hosts. Attracted by that heavy object, enormous quantities of gas (mostly hydrogen) spiral inwards towards the black hole. A disk-shaped structure forms in which the gas moves ever faster around the black hole while enormous amounts of energy are radiated at all wavelengths [3]. Getting the food to the Black Hole A great debate is now going on among scientists about how exactly the black holes are "fed". How is the gas first transported into the disk to fuel the seemingly insatiable supermassive black hole? It is still not well understood how the gas is moved from the outside to within a distance of 1000 light-years of the centre. Various violent processes have been mentioned in this context, like the merger of galaxies. A fine example of such an event was recently observed at the distant quasar HE 1013-2136 with the ESO Very Large Telescope, cf. ESO PR 13/01. The role of "nuclear bars" ESO PR Photo 25d/01 ESO PR Photo 25d/01 [Preview - JPEG: 364 x 400 pix - 89k] [Normal - JPEG: 727 x 800 pix - 264k] Caption : PR Photo 25d/01 is a schematic drawing of the various components of a double-barred galaxy, as mentioned in the text. Another possibility to move the gas inwards is the presence of bar-like structures at the centres of some galaxies, so-called "nuclear bars" . They look like small versions of the well-known, beautiful large-scale bar-like structures seen in galaxies like NGC 1365 (cf. ESO PR Photos 08a-e/99 ), but the responsible dynamical processes may possibly be somewhat different. Photo 25d/01 shows the various components that are discussed here in a schematic way. Acting as a gravitational brush, a bar that is thousands of light-years long efficiently "sweeps" the gas in that galaxy towards its core. When sufficient material has collected there, that matter may become dynamically "decoupled", forming a smaller bar at the centre of the larger "primary" bar. Such a "nuclear bar" may then, at least in theory, take over and let the gas move further inwards towards the central black hole. Until now, nuclear bars have mostly been seen on detailed images as small, elongated structures embedded within the larger primary bars - such structures may ressemble a "Russian doll". In addition, nuclear bars have been detected indirectly due to their gravitational effects, by means of very accurate measurements of the motions of the gas in the central region in a few galaxies. A first observational campaign by a team of French and Swiss astronomers [1] with the ESO Very Large Telescope (VLT) has now brought new, important insights about these nuclear bars. ISAAC spectra of the innermost regions of three active galaxies ESO PR Photo 25e/01 ESO PR Photo 25e/01 [Preview - JPEG: 400 x 424 pix - 40k] [Normal - JPEG: 800 x 847 pix - 256k] ESO PR Photo 25f/01 ESO PR Photo 25f/01 [Preview - JPEG: 400 x 241 pix - 40k] [Normal - JPEG: 800 x 401 pix - 112k] Caption : PR Photo 25e/01 is a reproduction of a long-slit ISAAC spectrum of the central region of the active galaxy NGC 1808 . It is in the 2.3 µm spectral region and the wavelength increases towards right. Several strong, vertical bands are seen; they are caused by CO-molecules in the atmospheres of the stars in this area. The bright band at the centre corresponds to the nucleus of the galaxy within which the central black hole is located. The characteristic S-shape is a result of the rotation of the stars around this centre, due to the Doppler effect. Technical information about this photo is available below. In the left half of PR Photo 25f/01 , the measured velocities (ordinate) of the stars near the centre of NGC 1808 are plotted at different distances from the nucleus (abscissa). The right half shows the corresponding curve after "removal" of the effect from the rotation - the remaining spread is a direct measure of the "velocity dispersion" and the individual stellar motions. As can be clearly seen, the width of the "band" decreases towards the centre, indicating the presence of a "dynamically cool" central stellar system. For more details, see the text. The scientists embarked upon a project with the goal of investigating in detail the motions of stars in the central regions of some active, comparatively "nearby" galaxies. As the innermost regions of such galaxies are usually quite dusty, the observations were carried out in infrared light that penetrates the dust clouds much better than does visible light. Thanks to its high efficiency and excellent imaging quality and spectral resolution, the VLT Infrared Spectrometer And Array Camera (ISAAC) is superbly suited for such work. Several galaxies with active centres were selected for the first observing runs in 1999 and 2000, among these NGC 1097, NGC 1808 and NGC 5728 that are shown in PR Photos 25a-c/01 . Infrared spectra were obtained in the 2.3 µm wavelength region in which a number of molecular spectral bands are seen, cf. PR Photo 25e/01 . They are caused by carbon monoxide ( 12 CO) molecules in the atmospheres of the stars located near the centres of the galaxies. Stellar motions By measuring the exact wavelengths of these molecular bands, it is possible to determine (from the Doppler effect), first, the mean velocity of the stars ( PR Photo 25f/01 ; left) and, secondly, the spread in this velocity (known as the "velocity dispersion" ; right). The first value reflects the general speed with which the stars move around the central black hole. The second indicates the extent to which the individual stellar motions deviate from that mean value. The comparison with the flight of a swarm of bees is useful: the mean velocity tells how fast the swarm moves forward as a whole - this is the ordered motion of the group. The second value instead indicates how much (or how fast) the individual bees move around inside the swarm - this is the spread in random velocities among the bees. Dynamical temperature is another concept defined by velocity dispersion. A warm gas is a gas where the molecules swarm around at high random speeds, while the molecules in a cold gas have low velocity dispersion. Astronomers often borrow this terminology and refer to stellar systems with low velocity dispersions as "dynamically cool systems". Confirming the "nuclear bars"... When "mapped" over the entire central area of a galaxy, these stellar velocity values provide detailed information about the gravitational field, and thus the mass distribution in the innermost region of the galaxy. The ISAAC observations did confirm the presence of "nuclear bars" in NGC 1097, NGC 1808 and NGC 5728. They also showed that these bars are truly "decoupled" stellar systems - their motions are only determined by the mass distribution in that area. ...and discovering a "dynamically cool" stellar system! However, the astronomers were very surprised to discover that in all three galaxies, the velocity dispersion is decreasing towards the centre, exactly contrary to what is predicted by simple models . The likely reason is the presence in the central region of a "newborn" system of stars whose individual velocities have not yet had time to "heat up". The project leader, Eric Emsellem explains: "Slower individual stellar motions correspond to a lower 'dynamical temperature' of the stellar system in this innermost region. We interpret this as evidence for a recent infall of gas that was induced by the nuclear bar. This has created a new gaseous disk at the centre of the galaxy, which has given birth to new stars. They all move around the black hole with more or less the same circular velocity as the gas from which they were born" . Agreement between observations and models This interesting scenario is supported by recent, extensive model computations by the team. In these computer models, large numbers of "stars" (mass points) move in a model galaxy with both a large and a nuclear bar, as observed in the three galaxies. Herve Wozniak refers to them as "self-consistent N-body simulations" and explains why the team is enthusiastic: "When our models also include star formation in the gas in the central region, a new, "dynamically cool" component of young stars emerges and mixes with the old stellar population" . He goes on: "The light from those young stars is superposed on that from the older ones in that area. Because of this, the overall "velocity dispersion" in the central region is then smaller than what it is further out. This is exactly as we observed in the ISAAC spectra obtained in the present programme" . Eric Emsellem points out that such a "dynamically cold" system is unstable and cannot last very long . "Soon it will "heat up" due to complex dynamical processes. It is quite possible that some of these stars will eventually end up as food for the hungry Black Hole.." Prospects With these new high-resolution infrared observations of the structure and the objects in the innermost regions of active galaxies, ISAAC and the VLT are paving the way for future studies of the processes that take place in the immediate neighbourhood of the central black holes. More active galaxies will now be observed with this method and it will be interesting to see if the presently discovered "cool" and young stellar systems represent a common phenomenon or not. More information The first stages of the research project reported in this Press Release are described in a scientific article ("Dynamics of embedded bars and the connection with AGN" by E. Emsellem et al.) that appeared in the European research journal Astronomy & Astrophysics (Vol. 368, p. 52). Two other articles about the new models and the implied properties of the central stellar population of young stars will follow. Notes [1]: The team consists of Eric Emsellem (Principal Investigator, Centre de Recherche Astronomique de Lyon, France), Didier Greusard and Daniel Friedli (Geneva Observatory, Switzerland), Francoise Combes (DEMIRM, Paris, France), Herve Wozniak (Marseille Observatory, France), Emmanuel Pecontal (Centre de Recherche Astronomique de Lyon, France) and Stephane Leon (University of Cologne, Germany). [2]: Black Holes represent an extreme physical phenomenon; if the Earth were to become one, it would measure no more than a few millimetres across. The gravitational field around a black hole is so intense that even light can not escape from it. [3]: On its most energetic and dramatic scale, this scenario results in a quasar , a type of object first discovered in 1963. In this case, the highly energetic centre of a galaxy completely outshines the outer structures and the "quasi-stellar object" appears star-like in smaller telescopes. Technical information about the photos PR Photo 25a/01 with NGC 1097 is a reproduction from the ESO LV archive, extracted via the Hypercat facility. It is based on a 2-hour photographic exposure in the R-band (Kodak IIIa-F emulsion + RG630 filtre) with the ESO 1-m Schmidt Telescope at La Silla and covers a field of about 35 x 35 arcmin 2. On this and the following photos, North is up and East is left. PR Photo 25b/01 of the central region of NGC 1808 was reproduced from an H-band (1.6 µm) image obtained with the IRAC2 camera (now decommissioned) at the MPG/ESO 2.2-m telescope on La Silla. The exposure time was 50 sec and the field measures 2.0 x 2.1 arcmin 2 (original pixel size = 0.52 arcsec). PR Photo 25c/01 of the central region of NGC 5728 was obtained at the 3.5-m Canada-France-Hawaii Telescope (CFHT) and the Adaptive-Optics PUEO instrument; the K-band (2.3 µm) exposure lasted 60 sec and the field measures 38 X 38 arcsec 2. PR Photo 25e/01 shows a raw, long-slit IR-spectrum in the 2.3 µm wavelength region, obtained with ISAAC along the major axis of this galaxy.

First Results from the UT1 Science Verification Programme

NASA Astrophysics Data System (ADS)

1998-11-01

Performance verification is a step which has regularly been employed in space missions to assess and qualify the scientific capabilities of an instrument. Within this framework, it was the goal of the Science Verification program to submit the VLT Unit Telescope No. 1 (UT1) to the scrutiny that can only be achieved in an actual attempt to produce scientifically valuable results. To this end, an attractive and diversified set of observations were planned in advance to be executed at the VLT. These Science Verification observations at VLT UT1 took place as planned in the period from August 17 to September 1, 1998, cf. the September issue of the ESO Messenger ( No. 93, p. 1 ) and ESO PR 12/98 for all details. Although the meteorological conditions on Paranal were definitely below average, the telescope worked with spectacular efficiency and performance throughout the entire period, and very valuable data were gathered. After completion of all observations, the Science Verification Team started to prepare all of the datasets for the public release that took place on October 2, 1998. The data related to the Hubble Deep Field South (now extensively observed by the Hubble Space Telescope) were made public world-wide, while the release of other data was restricted to ESO member states. With this public release ESO intended to achieve two specific goals: offer to the scientific community an early opportunity to work on valuable VLT data, and in the meantime submit the VLT to the widest possible scrutiny. With the public release, many scientists started to analyse scientifically the VLT data, and the following few examples of research programmes are meant to give a sample of the work that has been carried out on the Science Verification data during the past two months. They represent typical investigations that will be carried out in the future with the VLT. Many of these will be directed towards the distant universe, in order to gather insight on the formation and evolution of galaxies, galaxy clusters, and large scale structure. Others will concentrate on more nearby objects, including stars and nebulae in the Milky Way galaxy, and some will attempt to study our own solar system. The following six research programmes were presented at the Press Conference that took place at the ESO Headquarters in Garching (Germany) today. Deep Galaxy Counts and Photometric Redshifts in the HDF-S NIC3 Field The goal of this programme was to verify the capability of the VLT by obtaining the deepest possible ground-based images and using multicolour information to derive the redshifts (and hence the distances) of the faintest galaxies. The space distribution, luminosity and colour of these extreme objects may provide crucial information on the initial phases of the evolution of the universe. The method is known as photometric redshift determination . The VLT Test Camera was used to collect CCD images for a total of 16.6 hours in five spectral filters (U, B, V, R and I) in the so-called HDF-S NIC3 field. This is a small area (about 1 arcmin square) of the southern sky where very deep observations in the infrared bands J, H and K (1.1, 1.6 and 2.2µm, respectively) have been obtained by the Hubble Space Telescope (HST). The observations were combined and analyzed by a team of astronomers at ESO and the Observatory of Rome (Italy). Galaxies were detected in the field down to magnitude ~ 27-28. In most colours, the planned limiting values of the fluxes were successfully reached. ESO PR Photo 48a/98 ESO PR Photo 48a/98 [Preview - JPEG: 800 x 856 pix - 144k] [High-Res - JPEG: 3000 x 3210 pix - 728k] PR Photo 48a/98 shows some examples of photometric redshift determination for faint galaxies in the HDF-S NIC3 field. The filled points are the fluxes measured in the five colors observed with the VLT Test Camera (U, B, V, R and I) and in the infrared H spectral band with the NICMOS instrument on the Hubble Space Telescope. The curves constitute the best fit to the points obtained from a library of more than 400,000 synthetic spectra of galaxies at various redshifts (Fontana et al., in preparation). For most of these very faint sources, it is not possible to collect enough photons to measure the recession velocity (the redshift) by spectroscopy, even with an 8-m telescope. The redshifts and the main galaxy properties are then determined by comparing the colour observations with synthetic spectra (see PR Photo 48a/98 ). This has been done for more than one hundred galaxies in the field brighter than magnitude 26.5. Around 20 are found to be at redshifts larger than 2. The brighter ones are excellent candidates for future detailed studies with the UT1 instruments FORS1 and ISAAC. The scientists involved in this study are: Sandro D'Odorico, Richard Hook, Alvio Renzini, Piero Rosati, Rodolfo Viezzer (ESO) and Adriano Fontana, Emanuele Giallongo, Francesco Poli (Rome Observatory, Italy). A Gravitational Einstein Ring Because the gravitational pull of matter bends the path of light rays, astronomical objects - stars, galaxies and galaxy clusters - can act like lenses, which magnify and severely distort the images of galaxies behind them, producing weird pictures as in a hall of mirrors. In the most extreme case, where the foreground lensing galaxy and the background galaxy are perfectly lined up, the image of the background galaxy is stretched into a ring. Such an image is known as an Einstein ring , because the correct formula for the bending of light was first described by the famous phycisist Albert Einstein . ESO PR Photo 48b/98 ESO PR Photo 48b/98 [Preview - JPEG: 800 x 1106 pix - 952k] [High-Res - JPEG: 3000 x 4148 pix - 5.4Mb] ESO PR Photo 48c/98 ESO PR Photo 48c/98 [Preview - JPEG: 800 x 977 pix - 272k] [High-Res - JPEG: 3000 x 3664 pix - 1.4Mb] PR Photo 48b/98 (left) shows a new, true colour image of an Einstein ring (upper centre of photo), first discovered at ESO in 1995. The ring, which is the stretched image of a galaxy far out in the Universe, stands out clearly in green, and the red galaxy inside the ring is the lens. The discovery image was very faint, but this new picture, taken with the VLT during the Science Verification Programme allows a much clearer view of the ring because of the great light-gathering capacity of the telescope and, not least, because of the superb image quality. In Photo 48c/98 (right), four images illustrate the deduced model of the lensing effect. In the upper left, the observed ring has been enlarged and the image of the lensing galaxy removed by image processing. Below it is a model of the gravitational field (potential) around this galaxy along with the "true" image of the background galaxy shown. At the lower right is the resulting gravitationally magnified and distorted image of the background galaxy, which to the upper right has been de-sharpened to the same image quality as the observed image. The similarity between the two is most convincing. The picture shows a new, true colour image of an Einstein ring, first discovered at ESO in 1995. The ring, which is the stretched image of a galaxy far out in the Universe, stands out clearly in green, and the red galaxy inside the ring is the lens. The discovery image was very faint, but this new picture, taken with the VLT during the Science Verification Programme allows a much clearer view of the ring because of the great light-gathering capacity the telescope and, not least, because of the superb image quality. Gravitational lensing provides a very useful tool with which to study the Universe. As "weighing scales", it provides a measure of the mass within the lensing body, and as a "magnifying glass", it allows us to see details in objects which would otherwise be beyond the reach of current telescopes. This new detailed picture has allowed a much more accurate measurement of the mass of the lensing galaxy, revealing the presence of vast quantities of "unseen" matter, five times more than if just the light from the galaxy is taken into account. This additional material represents some of the Universe's dark matter . The gravitational lens action is also magnifying the background object by a factor of ten, providing an unparalleled view of this very distant galaxy which is in a stage of active star-formation. The scientists involved in this study are : Palle Møller (ESO), Stephen J. Warren (Blackett Laboratory, Imperial College, UK), Paul C. Hewett (Institute of Astronomy, Cambridge, UK) and Geraint F. Lewis (Dept. of Physics and Astronomy, University of Victoria, Canada). An Extremely Red Galaxy One of the main goals of modern cosmology is to understand when and how the galaxies formed. In the very last years, many high-redshift (i.e. very distant) galaxies have been found, suggesting that some galaxies were already assembled, when the Universe was much younger than now. None of these high-redshift galaxies have ever been found to be a bona-fide red elliptical galaxy . The VLT, however, with its very good capabilities for infrared observations, is an ideal instrument to investigate when and how the red elliptical galaxies formed. The VLT Science Verification images have provided unique multicolour information about an extremely red galaxy that was originally (Treu et al., 1998, A&A Letters, Vol. 340, p. 10) identified on the Hubble Deep Field South (HDF-S) Test Image. This galaxy is shown in PR Photo 48d/98 that is an enlargment from ESO PR Photo 35b/98. It was detected on Near-IR images and also on images obtained in the optical part of the spectrum, at the very faint limit of magnitude B ~ 29 in the blue. However, this galaxy has not been detected in the near-ultraviolet band. ESO PR Photo 48d/98 ESO PR Photo 48d/98 [Preview - JPEG: 800 x 594 pix - 264k] [High-Res - JPEG: 3000 x 2229 pix - 1.8Mb] ESO PR Photo 48e/98 ESO PR Photo 48e/98 [Preview - JPEG: 800 x 942 pix - 96k] [High-Res - JPEG: 3000 x 3533 pix - 576k] PR Photo 48d/98 (left) shows the very red galaxy (at the arrow) in the Hubble Deep Field South , discussed here. Photo 48e/98 (right) is the spectrum of a typical elliptical galaxy, redshifted to z = 1.8 and compared with the brightness of the galaxy in different wavebands (crosses), as measured during the VLT SV programme and the Hubble Deep Field South Test Program (the cross to the right). The arrow indicates the upper limit by the VLT SV in the ultraviolet band. It can be seen that these observations are fully consistent with the object being an old, elliptical galaxy at the high redshift of z=1.8 , i.e. at an epoch, when the Universe was much younger than now. The new ISAAC instrument at VLT UT1 will be able to obtain an infrared spectrum of this galaxy and thus to affirm or refute this provisional conclusion. The colours measured at the VLT and on the HST Test Image are very well matched by those of an old elliptical galaxy at redshift z ~ 1.8 ; see Photo 48e/98 . All the available evidence is thus consistent with this object being an elliptical galaxy with the highest-known redshift for this galaxy type. A preliminary analysis of Hubble Deep Field South data, just released, seems to support this hypothesis. If these conclusions are confirmed by direct measurement of its spectrum, this galaxy must already have been "old" (i.e. significantly evolved) when the Universe had an age of only about one fifth of its present value. A spectroscopic confirmation is still outstanding, but is now possible with the ISAAC instrument at VLT UT1. A positive result would demonstrate that elliptical galaxies can form very early in the history of the Universe. The scientists involved in this study are: Massimo Stiavelli, Tommaso Treu (also Scuola Normale Superiore, Italy), Stefano Casertano, Mark Dickinson, Henry Ferguson, Andrew Fruchter, Crystal Martin (STSci, Baltimore, USA), Piero Rosati and Rodolfo Viezzer (ESO), Marcella Carollo (Johns Hopkins University, Baltimore, USA) and Henry Tieplitz (NASA, Goddard Space Flight Center, Greenbelt, USA). Lyman-alpha Companions and Extended Nebulosity around a Quasar at Redshift z=2.2 In current theories of galaxy formation, luminous galaxies we see to-day were built up through repeated merging of smaller protogalactic clumps. Quasars, prodigious sources pouring out 100 to 1000 times as much light as an entire galaxy, have been used as markers of galaxy formation activity and have guided astronomers in their hunting of primeval galaxies and large-scale structures at high redshift. A supermassive black-hole, swallowing stars, gas and dust, is thought to be the engine powering a quasar and the interaction of the galaxy hosting the black-hole with neighboring galaxies is expected to play a key role in "feeding the monster". At intermediate redshift, a large fraction of radio-loud quasars and radio galaxies inhabit rich clusters of galaxies, whereas radio-quiet quasars are rarely found in very rich environments. Furthermore, tidal interaction between quasars and their nearby companions is also the favoured explanation for the presence of large gaseous nebulosities associated with radio-loud quasars and radio galaxies. At high redshift, searches for Lyman-alpha quasar companions and emission-line nebulosities show strong similarities with those seen at lower redshift, although the detection rate is lower. ESO PR Photo 48f/98 ESO PR Photo 48f/98 [Preview - JPEG: 800 x 977 pix - 184k] [High-Res - JPEG: 3000 x 3662 pix - 1.1Mb] ESO PR Photo 48g/98 ESO PR Photo 48g/98 [Preview - JPEG: 800 x 966 pix - 328k] [High-Res - JPEG: 3000 x 3621 pix - 1.8Mb] PR Photo 48f/98 (left) is a false-colour reproduction of a B-band image of the field around the radio-weak quasar J2233-606 in the Hubble Deep Field South (HDF-S) . Photo 48g/98 (right) represents emission from the same direction at a wavelength that corresponds to Lyman-alpha emission at the redshift ( z = 2.2 ) of the quasar. Three Lyman-alpha candidate companions are indicated with arrows. Note also the extended nebulosity around the quasar. A search for Lyman-alpha companions to the radio-weak quasar J2233-606 in the Hubble Deep Field South (HDF-S) was conducted during the VLT UT1 SV programme in a small field of 1.2 x 1.3 arcmin 2 , centered on the quasar. Candidate Lyman-alpha companions were identified by subtracting a broad-band B (blue) image, that traces the galaxy stellar populations, from a narrow-band image, spectrally centered on the redshifted, narrow Lyman-alpha emission line of the quasar ( z = 2.2 ). Three Lyman-alpha candidate companions were discovered at angular distances of 15 to 23 arcsec, or 200 to 300 kpc (650,000 to 1,000,000 light-years) at the distance corresponding to the quasar redshift. The emission lines are very strong, relative to the continuum emission of the galaxies - this could be a consequence of the strong ionizing radiation field of the quasar. These companions to the quasar may trace a large-scale structure which would extend over larger distances beyond the observed, small field. Even more striking is the presence of a very extended nebulosity whose size (120 kpc x 160 kpc) and Lyman-alpha luminosity (3 x 10 44 erg/cm 2 /s) are among the largest observed around radio galaxies and radio-loud quasars, but rarely seen around a radio-weak quasar. Tidal interaction between the northern, very nearby companion and the quasar is clearly present: the companion is embedded in the quasar nebulosity, most of its gas has been stripped and lies in a tail westwards of the galaxy. The scientists involved in this study are: Jacqueline Bergeron (ESO), Stefano Cristiani, Stephane Arnouts, Gianni Fasano (Padova, Italy) and Patrick Petitjean (Institut d'Astrophysique, Paris, France). Very Distant Galaxy Clusters During the past years, it has become possible to detect and subsequently study progressively more distant clusters of galaxies. For this research programme, UT1 Science Verification data were used, in combination with data obtained with the SOFI instrument at the ESO New Technology Telescope (NTT) at La Silla, to confirm the existence of two very distant galaxy clusters at redshift z ~ 1 , that had originally been detected in the ESO Imaging Survey. This redshift corresponds to an epoch when the age of the Universe was only two-thirds of the present. ESO PR Photo 48h/98 ESO PR Photo 48h/98 [Preview - JPEG: 800 x 917 pix - 896k] [High-Res - JPEG: 3000 x 3438 pix - 6.0Mb] PR Photo 48h/98 (left) is a colour composite that shows the now confirmed cluster EIS0046-2930 . The image has been produced by combining the V (green-yellow), R (red) and I (Near-IR) exposures with the Test Camera obtained during the VLT-UT1 Science Verification. The yellow-orange galaxies are the cluster members and the bluer objects are galaxies belonging to the general field population. The cluster center is at the location of the largest (yellow-orange) cluster galaxy to the left of the center of the image. The field measures 90 x 90 arcsec. This was achieved by the detection of a spatial excess density of galaxies, with measured colour equal to that of elliptical galaxies at this redshift, as established by counts in the respective sky areas. The field of one these clusters is shown in PR Photo 48h/98 . These new data show that the VLT will most certainly play a major role in the studies of the cluster galaxy population in such distant systems. This will contribute to shed important new light on the evolution of galaxies. Furthermore, the VLT clearly has the potential to identify and confirm the reality of many more such clusters and thereby to increase considerably the number of known objects. This will be important in order to determine more accurate values of the basic cosmological constants, and thus for our understanding of the evolution of the Universe as a whole. The presentation was made by Lisbeth Fogh Olsen (Copenhagen Observatory, Denmark, and ESO) on behalf of the scientists involved in this study. Icy Planets in the Outer Solar System Observations with large optical telescopes during the past years have begun to cast more light on the still very little known, distant icy planets in the outer solar system. Until November 1998, about 70 of these have been discovered outside the orbit of Neptune (between 30 and 50 AU, or 4,500 to 7,500 million km, from the Sun). They are accordingly referred to as Trans-Neptunian Objects (TNOs) . Those found so far are believed to represent the "tip of the iceberg" of a large population of such objects belonging to the so-called Kuiper Belt . This is a roughly disk-shaped region between about 50 and 120 AU (about 7,500 to 18,000 million km) from the Sun, in which remnant bodies from the formation of the solar system are thought to be present. From their measured brightness and the distance, it is found that most known TNOs have diameters of the order of a few hundred kilometres. About half of those known move in elongated Pluto-like orbits, the others move somewhat further out in stable, circular orbits. During the two-week Science Verification programme, approximately 200 minutes were spent on a small observing programme aimed at obtaining images of some TNOs in different wavebands (B, V, R and I). Since this programme was primarily designed as a back-up to be executed during less favourable atmospheric conditions, some of the observations could not be used. However, images of three faint TNOs were recorded during an excellent series of 1-10 min exposures. From these data, it was possible to measure quite accurate magnitudes (and thus approximate sizes) and to determine their colours. One of them, 1996 TL66, was among the bluest TNOs ever observed. It is believed that this is because its surface has undergone recent transformation, possibly due to collisions with other objects or the breaking-off of small pieces from the surface, in both cases revealing "fresh" layers below. The combination of all available exposures made it possible to look for faint and tenous atmospheres around these TNOs, but none were found. These results show that it is possible, with little effort and even under quite unfavourable observing conditions, to obtain valuable information with the VLT about icy objects in the outer solar system. Of even greater interest will be future spectroscopic observations with FORS and ISAAC that will allow to study the surface composition in some detail, with the potential of providing direct information about (nearly?) pristine material from the early phases of the solar system. The scientists involved in this study are: Olivier Hainaut, Hermann Boehnhardt, Catherine Delahodde and Richard West (ESO) and Karen Meech (Institute of Astronomy, Hawaii, USA). How to obtain ESO Press Information ESO Press Information is made available on the World-Wide Web (URL: http://www.eso.org ). ESO Press Photos may be reproduced, if credit is given to the European Southern Observatory.

hwhap_Ep15_Astronaut Photography

NASA Image and Video Library

2017-10-19

>> HOUSTON, WE HAVE A PODCAST. WELCOME TO THE OFFICIAL PODCAST OF THE NASA JOHNSON SPACE CENTER, EPISODE 15: ASTRONAUT PHOTOGRAPHY. I’M GARY JORDAN AND I’LL BE YOUR CO-HOST TODAY, ALONG WITH MEGAN SUMNER, PUBLIC AFFAIRS OFFICER FOR THE ASTRONAUT OFFICE. MEGAN, HOW YOU DOING? >> I’M DOING GOOD. HOW ARE YOU, GARY? >> DOING GREAT. SO MEGAN, TODAY’S EPISODE IS A LITTLE BIT DIFFERENT, BECAUSE WE HAD A CONVERSATION WITH FOUR-- THAT’S RIGHT, FOUR-- ASTRONAUTS IN SPACE. WE TALKED WITH RANDY “KOMRADE” BRESNIK, JOE ACABA, MARK “SABOT” VANDE HEI, AND PAOLO NESPOLI. ALL OF THEM ARE ASTRONAUTS ABOARD THE INTERNATIONAL SPACE STATION FOR EXPEDITION 53, WHICH STARTED BACK IN SEPTEMBER AFTER PEGGY WHITSON, JACK FISCHER, AND FYODOR YURCHIKHIN DEPARTED THE STATION. KOMRADE AND NESPOLI WERE ALREADY UP THERE, AND THEY WERE LATER JOINED BY ACABA AND SABOT, AS WELL AS ALEXANDER MISURKIN. >> THAT’S RIGHT, AND WE TALKED TO ALL FOUR OF THEM LIVE, SO WE BROUGHT IN SOME SOCIAL MEDIA QUESTIONS REAL TIME FOR THE ASTRONAUTS TO ANSWER. >> YES, THANKS TO YOU. WE TALKED ABOUT ASTRONAUT PHOTOGRAPHY, FOR THE MOST PART-- HOW THEY TAKE PICTURES OF EARTH, AND WHAT THEY SEE, AND THE SORT OF EMOTIONS THAT THAT VIEW BRINGS UP. BUT WE ALSO TALKED A LITTLE BIT ABOUT THE SPACEWALKS GOING ON THIS MONTH, AND EDUCATION IN SPACE, AS WELL AS LIFE IN SPACE. SO WITH NO FURTHER DELAY, LET’S GO LIGHTSPEED AND JUMP RIGHT AHEAD TO OUR TALK WITH THE EXPEDITION 53 CREW. ENJOY. [ MUSIC ] >> T MINUS FIVE SECONDS AND COUNTING-- MARK. [ INDISTINCT RADIO CHATTER ] >> HOUSTON, WE HAVE A PODCAST. [ MUSIC ] >> HELLO NASA TV, FACEBOOK LIVE, USTREAM-- WHEREVER YOU ARE WATCHING. WELCOME TO A VERY SPECIAL EPISODE OF “HOUSTON, WE HAVE A PODCAST.” SO IF YOU’RE UNFAMILIAR WITH THE PODCAST, THIS IS WHERE WE BRING IN NASA EXPERTS-- SCIENTISTS, ENGINEERS, ASTRONAUTS-- ALL TO TELL YOU THE COOLEST STUFF ABOUT WHAT’S GOING ON HERE AT NASA. SO TODAY WE HAVE A VERY SPECIAL EPISODE. OF COURSE, YOU CAN SEE US ON CAMERA, AND THIS IS USUALLY AN AUDIO PODCAST. BUT ALSO, WE’RE GOING TO BE TALKING TO SPACE. THIS IS NOT THE FIRST TIME WE’VE DONE THAT. WE’VE DONE IT ABOUT TWO MONTHS AGO WITH JACK FISCHER ABOARD THE INTERNATIONAL SPACE STATION. AND WE’RE GOING TO DO IT AGAIN WITH SOME ASTRONAUTS, EXCEPT NOT WITH JUST ONE. WE’RE GOING TO DO IT WITH FOUR ASTRONAUTS: RANDY “KOMRADE” BRESNIK, MARK “SABOT” VANDE HEI, JOE ACABA, AND PAOLO NESPOLI. SO I’M NOT GOING TO DO THIS ALONE, OF COURSE. SAME AS ALWAYS, SAME AS BEFORE, I HAVE A CO-HOST WITH ME-- NASA PUBLIC AFFAIRS OFFICER FOR THE ASTRONAUT OFFICE, MEGAN SUMNER. MEGAN, THANKS FOR BEING HERE. >> THANKS, HAPPY TO BE HERE. EXCITED TO TALK TO THEM. >> AWESOME. SO, I MEAN, PUBLIC AFFAIRS OFFICER FOR THE ASTRONAUT OFFICE. NOT THE ONLY ROLE YOU’VE HAD HERE AT NASA, RIGHT? >> MM-HMM, YEAH. I’VE PREVIOUSLY ACTUALLY MANAGED OUR SOCIAL MEDIA ACCOUNTS HERE-- THE JOHNSON SPACE CENTER ACCOUNTS, AND THE INTERNATIONAL SPACE STATION ACCOUNTS, AND NOW I AM WORKING SUPPORTING THE ASTRO OFFICE FOR APPEARANCES THAT THEY GO OUT AND DO, AND ALSO THE MEDIA SUPPORT. WE HAVE MEDIA COME AND TALK TO THEM BEFORE THEIR MISSIONS, AND DO INTERVIEWS AND MEDIA VISITS AND THINGS LIKE THAT. >> FANTASTIC. AND SO, I THINK THAT’S THE REASON YOU’RE THE PERFECT PERSON TO HAVE AS A CO-HOST WITH ME TODAY IS JUST BECAUSE, FIRST OF ALL, YOU KNOW THE ASTRONAUTS THAT WE’RE TALKING TO TODAY. YOU’VE ACTUALLY WORKED WITH SOME OF THEM IN THE PAST, RIGHT? >> YEAH, SO JOE AND MARK, WHO WE’LL BE TALKING TO TODAY, WERE ACTUALLY THE FIRST TWO ASTRONAUTS THAT I GOT TO WORK WITH IN THIS ROLE AS THE PUBLIC AFFAIRS OFFICER FOR THE ASTRONAUT OFFICE, SO I’M REALLY EXCITED TO GET TO ACTUALLY TALK TO THEM IN SPACE. >> AWESOME. BUT THEN ALSO, YOU RAN THE SOCIAL MEDIA ACCOUNTS HERE AT THE JOHNSON SPACE CENTER FOR A WHILE, SO THAT’S ANOTHER PART OF THIS IS WE ARE ON FACEBOOK LIVE SO IF YOU HAVE ANY QUESTIONS THAT YOU’D LIKE TO SEND UP TO THE CREW, MEGAN IS GOING TO BE MONITORING THOSE QUESTIONS REAL TIME. SHE’S GOT HER PHONE RIGHT NEXT TO HER AND WE’LL BE ASKING SOME OF THOSE QUESTIONS TO OUR FOUR ASTRONAUTS TODAY. SO THE TOPIC OF TODAY’S CONVERSATION IS ASTRONAUT PHOTOGRAPHY. SO WHAT’S THAT ALL ABOUT? >> OH, MAN, THE ASTRONAUTS TAKE THE MOST AMAZING PICTURES FROM THE SPACE STATION AND IT'S JUST AN AMAZING VIEW THAT MOST OF US WILL NEVER GET TO SEE IN OUR LIFETIME. AND THANKFULLY, THEY ARE WILLING TO SHARE THAT VIEW WITH US THROUGH SOCIAL MEDIA. EASILY THEY CAN SHARE IT OUT TO THE WHOLE WORLD OF WHAT THAT’S LIKE. AND NOT ONLY THAT, BUT THEY’RE SHARING WITH US WHAT THEY’RE DOING IN SPACE AND A LITTLE GLIMPSE INTO THEIR LIFE, THE SCIENCE THEY’RE DOING, ALL THE WORK THEY’RE DOING ON BOARD. SO IT’S SO COOL TO BE ABLE TO SEE THAT PERSPECTIVE. >> ABSOLUTELY. I’M VERY EXCITED FOR THIS TOPIC BECAUSE IT IS ONE OF THE MORE VISUAL THINGS THAT WE GET TO SEE OF WHAT THE ASTRONAUTS DO ON THE INTERNATIONAL SPACE STATION. OBVIOUSLY, THEY’RE DOING SCIENCE ALL THE TIME AND WE HAVE CREW MEMBERS THAT ARE CONSTANTLY WORKING VARIOUS EXPERIMENTS. AND JUST RECENTLY, THEY'VE BEEN GOING OUT AND DOING A FEW SPACEWALKS SO THEY HAVE MAINTENANCE TASKS THAT THEY REGULARLY DO. BUT RIGHT NOW, WE’RE ACTUALLY GOING TO BE TALKING ABOUT ASTRONAUT PHOTOGRAPHY. AND ACTUALLY RIGHT NEXT TO US WE HAVE SOME OF THE EQUIPMENT THAT THEY PRACTICE ON WHENEVER THEY’RE DOING SOME OF THE-- TO ACTUALLY PRACTICE FOR TAKING PHOTOS OF THE EARTH. SO IT LOOKS LIKE OUR ASTRONAUTS ARE ACTUALLY GETTING SET-UP HERE, JUST LIKE THEY DO FOR ANY PUBLIC AFFAIRS EVENT. SO WE’RE GOING TO BE TALKING WITH MISSION CONTROL SOON AND GETTING THAT STARTED. SO IF YOU HAVE ANY QUESTIONS, PLEASE FEEL FREE TO ASK THEM BELOW. >> YUP, YUP, WE’RE TAKING YOUR QUESTIONS ON FACEBOOK LIVE. I’LL BE WATCHING AND ASKING THE CREW, SO GET YOUR QUESTION IN THERE AND WATCH ALONG SO YOU CAN HEAR IF THEY GET A CHANCE TO ANSWER IT. >> ABSOLUTELY. ALL RIGHT, LOOKS LIKE OUR FOUR ASTRONAUTS ARE GETTING SET UP RIGHT NOW. LET’S THINK, I MEAN, SO WE HAVE-- WE CAN TALK ABOUT SOME OF THE EXTRAVEHICULAR ACTIVITIES THAT THEY’VE BEEN DOING, SOME OF THE SPACEWALKS AS WELL, BUT A LITTLE BIT ABOUT OUR CREW-- RANDY BRESNIK AND JOE ACABA AND PAOLO NESPOLI HAVE BEEN THERE BEFORE. FOR MARK VANDE HEI THIS IS HIS FIRST SPACEFLIGHT, SO WE’LL GET TO TALK TO HIM ABOUT HIS EXPERIENCE AS BEING A NEWCOMER. ACTUALLY, THREE OF THE ASTRONAUTS WE’VE TALKED TO ON THE PODCAST BEFORE-- RANDY BRESNIK, MARK VANDE HEI, AND JOE ACABA-- ALL EACH INDIVIDUAL EPISODES TO SHARE THEIR EXPERIENCES OF WHAT THEY’VE DONE ABOARD. PAOLO NESPOLI, THIS’LL BE THE FIRST TIME TALKING WITH HIM, SO THAT’LL BE A PLEASURE AS WELL. AND HE SHARED SOME FANTASTIC IMAGERY OF ITALY AND JUST DIFFERENT PARTS OF THE EARTH, SO CAN’T WAIT TO SEE WHAT WE’RE DOING THERE. SO LET’S CONNECT WITH MISSION CONTROL, HOUSTON, AND TALK TO OUR FOUR ASTRONAUTS. AGAIN, SEND YOU QUESTIONS BELOW ON FACEBOOK LIVE. >> STATION, THIS IS HOUSTON. ARE YOU READY FOR THE EVENT? >> HOUSTON, WE’RE READY FOR THE EVENT. >> JSC PAO, PLEASE CALL STATION FOR A VOICE CHECK. >> STATION, THIS IS GARY JORDAN AND MEGAN SUMNER IN THE PUBLIC AFFAIRS OFFICE. HOW DO YOU HEAR US? >> GARY, WE GOT YOU LOUD AND CLEAR. MEGAN, GOOD AFTERNOON TO YOU, TOO. >> ALL RIGHT, WELL THIS IS AN ABSOLUTE PLEASURE TO BE TALKING TO ALL FOUR OF YOU TODAY. I THOUGHT FOR SURE I’D AT LEAST GET TO TALK TO ONE ASTRONAUT, BUT THANK YOU SO MUCH FOR ALL FOUR OF YOU TAKING THE TIME TO TALK TO US TODAY. SO FOR-- A LOT OF YOU HAVE BEEN ON THE PODCAST ALREADY, SO AGAIN, WELCOME BACK. BUT TODAY, WE’RE GOING TO BE DOING A LIVE EVENT SO WE REALLY WANTED TO BRING IN SOME QUESTIONS FROM SOCIAL MEDIA AND HOPING YOU CAN ANSWER THOSE REAL TIME. BUT JUST TO START OFF, BECAUSE THERE ARE FOUR OF YOU, IF YOU CAN JUST SORT OF GIVE A QUICK INTRODUCTION TO ALL OF YOU SO OUR LISTENERS KIND OF KNOW WHO YOU ARE. >> ALL RIGHT, WE’VE GOT EXPEDITION 53 SPACE STATION COMMANDER RANDY BRESNIK. >> EXPEDITION 52, 53 FLIGHT ENGINEER, PAOLO NESPOLI FROM THE EUROPEAN SPACE AGENCY. >> AND EXPEDITION 53 AND 54 FLIGHT ENGINEER, JOE ACABA. >> EXPEDITION 53 AND 54 FLIGHT ENGINEER, MARK VANDE HEI. >> THAT’S AWESOME. WELCOME TO ALL OF YOU. THANKS FOR BEING WITH US TODAY. SO WE’LL START WITH KOMRADE AND PAOLO, YOU GUYS HAVE BEEN UP THERE THE LONGEST, SO JUST HOW HAVE THE-- HOW’S THE MISSION BEEN GOING SO FAR? WHAT ARE SOME OF THE HIGHLIGHTS? >> I THINK CERTAINLY HIGHS FOR US WERE GETTING TO WORK WITH THE PREVIOUS CREW AND THE SPACE NINJA, PEGGY WHITSON, LEARNING FROM THEM TO BE ABLE TO TAKE OVER AND RUN SPACE STATION WHEN WE HAD OUR NEW CREW SHOW UP FOR EXPEDITION 53. WE GOT TO HAVE A DRAGON COME UP HERE AND BRING A WHOLE BUNCH OF SCIENCE THAT WE GOT TO WORK WITH FOR A WHOLE MONTH. CERTAINLY THE PAST WEEK HAS BEEN REAL EXCITING BECAUSE WE DID TWO EVAs THAT ARE REALLY TURN THE STATION BACK TO GOOD CONFIGURATION WITH A ROBOTIC ARM, AND SOME CAMERA WORK, AND PREPARING STUFF FOR ROBOTIC TASKS IN THE FUTURE. SO WE’VE GOT A LOT OF STUFF GOING ON INSIDE AND GOING ON OUTSIDE, AND SO IT’S BEEN A REALLY EXCITING EXPEDITION SO FAR AND WE STILL ARE ONLY ABOUT HALFWAY THROUGH. >> WELL NOT MUCH TO ADD TO KOMRADE HAS ALREADY SAID. I MEAN, WE’RE DOING A LOT OF ACTIVITIES HERE. IT’S ALWAYS CRAZY. LIKE, YOU CAN WAKE UP IN THE MORNING, START WORKING WITH SOMETHING, AND SPIN AROUND, AND WORK WITH SOME SCIENCE, AND THEN SPIN AROUND AGAIN, AND WORK WITH THE ROBOTIC ARM. WE’VE BEEN DOING ALMOST ALL OF IT RIGHT NOW. WE HAVE, WHAT, 200 MORE ACTIVITIES, 250, SOMETHING LIKE THAT. I MEAN, AND WE ARE DOING ALL OF THEM. >> FANTASTIC. SO TODAY, I MEAN, I’M SURE THERE’S A LOT OF DIFFERENT TOPICS THAT WE COULD TALK ABOUT, BUT REALLY WANTED TO FOCUS ON ASTRONAUT PHOTOGRAPHY TODAY BECAUSE YOU GUYS HAVE SUCH A UNIQUE PERSPECTIVE OF THE EARTH AND YOU GET SOME TIME SOMETIMES TO GO AND TAKE PHOTOS OF THE EARTH AND MAYBE JUST KIND OF WATCH THE EARTH GO BY. SO I GUESS SINCE, KOMRADE, YOU’RE HOLDING THE MIC, IF YOU WANT TO SHARE SOME EXPERIENCES FROM JUST LOOKING OUT THE WINDOW AND JUST KIND OF WHAT THAT FEELING IS LIKE? WHAT IT’S LIKE TO WATCH THE EARTH GO BY? >> I MEAN, IT’S REALLY HUMBLING BECAUSE IT’S SUCH A BEAUTIFUL THING AND THEY’RE SO-- SO FAR, BEEN SO FEW OF US THAT HAVE HAD A CHANCE TO SEE IT. AND YOU DON’T LOOK AT THE EARTH AND COME-- NOT BE CHANGED. YOU CERTAINLY FEEL A PART OF THE EARTH. YOU REALIZE THAT EVERY EXPERIENCES YOU’VE EVER HAD, EVERY PERSON YOU’VE EVER KNOWN IS DOWN ON THAT LITTLE BLUE MARBLE. AND WHEN YOU SEE THE CURVE, YOUR MIND KNOWS HOW BIG THE EARTH IS AND REALIZE WHEN YOU GO AROUND IT IN 90 MINUTES YOU’RE BACK TO ESSENTIALLY THE SAME SPOT. AND THE FACT THAT WE CAN DO THAT AND SEE THAT YOU JUST FEEL COMPELLED TO SHARE IT. I’LL HAND THE MIC OVER TO SABOT OVER HERE BECAUSE HE’S ONLY BEEN UP HERE ABOUT A MONTH, BUT TO GET HIS IMPRESSIONS ON WHAT IT WENT FROM SEEING IT FOR THE FIRST TIME TO NOW TRANSLATING THAT INTO PHOTOGRAPHY TO TRY AND SHARE THAT WITH OTHERS. >> THE THING THAT IMPRESSED ME THE MOST WHEN I FIRST LOOKED OUT THE CUPOLA TO SEE THE EARTH WAS HOW CLOSE THE RECOGNIZABLE FEATURES OF THE EARTH SEEM TO SPACE. FOR EXAMPLE, SEEING ITALY AND IN THE SAME VIEW SEEING THE BLACKNESS OF SPACE. IT MAKES IT SEEM LIKE EVERYBODY ON THE EARTH IS REALLY, REALLY CLOSE TO SPACE WITHOUT EVER REALIZING IT. FROM OUR PERSPECTIVE, THERE’S JUST A THIN LAYER OF ATMOSPHERE THAT ALL OF HUMANITY’S LIVING IN AND OUTSIDE OF THAT IS SPACE. SO IT’S IMPRESSIVE TO ME HOW CLOSE WE REALLY ARE ALL TO WHAT WE SEE AS OUTER SPACE. FROM A PHOTOGRAPHY PERSPECTIVE, I THINK THAT’S AN IMPORTANT PERSPECTIVE FOR EVERYBODY TO HAVE, SO MY FAVORITE THING TO DO IS TO TRY TO CAPTURE THOSE PICTURES THAT SHOW BOTH THE SPACE AND PLACES THAT WE RECOGNIZE AND CALL HOME ON THE PLANET. >> ABSOLUTELY. AND KOMRADE, I KNOW YOU’VE SHARED SOME JUST THE PERSPECTIVE OF THE EARTH COMPARED TO SOME OTHER IMAGES, YOU KNOW, BEING ON THE EARTH, TOO. AND THOSE ARE AN ABSOLUTE PLEASURE TO SEE. BUT I KNOW WE HAVE SOME ACTUAL QUESTIONS COMING IN FROM SOME OF OUR LISTENERS RIGHT NOW. >> YEAH. THAT’S AMAZING. I CAN’T EVEN IMAGINE WHAT IT’S LIKE TO ACTUALLY SEE THAT VIEW IN PERSON, BUT NEXT BEST THING OF COURSE IS TO BE ABLE TO SEE IT THROUGH PICTURES AND VIDEOS THAT YOU GUYS ARE TAKING. AND THE WHOLE WORLD REALLY APPRECIATES THAT. WE’VE GOT SOME AWESOME QUESTIONS COMING IN. LOTS OF PEOPLE ARE INTERESTED IN PHOTOGRAPHY IN SPACE AND YOU GUYS ON THE SPACE STATION. SO JACE ON FACEBOOK WANTS TO KNOW, “THERE ARE SO MANY CAMERAS ON THE SPACE STATION, HOW DO YOU DECIDE WHICH CAMERA TO USE? AND CAN YOU TELL US A LITTLE BIT ABOUT THE EQUIPMENT YOU DO HAVE UP THERE?” >> YES, SO WE DO HAVE-- FOR STILL PHOTOGRAPHY, WE ESSENTIALLY HAVE A NIKON CAMERA. RIGHT NOW, WE HAVE SEVERAL D4. EACH ONE OF US GETS HIS OWN, PLUS WE HAVE A COUPLE PLACED STRATEGICALLY. SOME OF THEM ARE DEDICATED FOR SPECIAL PHOTOGRAPHY LIKE MACRO PHOTOGRAPHY. WE NEED TO DO A LOT OF MACRO PHOTOGRAPHY FOR EQUIPMENT HERE. SOME WE JUST DEDICATED TO TAKE-- THERE WAS A MICRO-- A MICRO SHOT, RIGHT? >> YEAH. >> TRY ONE WITH A TELE LENS HERE. SOME, LIKE THIS ONE, WE REALLY USE WHEN WE ARE POINTING AT EARTH AND WE HAVE SOME WINDOWS THAT HAVE A SPECIAL CAPABILITY OF LETTING US TAKE PICTURES WITH THIS LENS. AND THEN, WE HAVE-- WE ALSO HAVE A RED DRAGON CAMERA THAT WE USE FOR CINEMATOGRAPHY. WE HAVE VIDEO CAMERAS THAT ALLOWS US TO TAKE HD PHOTOS. I MEAN, I WOULD SAY THAT FROM A POINT OF VIEW OF CAMERAS, LENSES, SET-UP, WE ARE ALL SET HERE. WE HAVE EVERYTHING THAT YOU CAN IMAGINE. IT’S JUST WHAT IS MISSING A LITTLE BIT IS THE TIME BECAUSE IT TAKES TIME TO BE THERE AT THE WINDOW. IT’S NOT THAT YOU JUST GO THERE AND YOU CAN TAKE A PICTURE AND LEAVE. IF YOU WANT TO HAVE SOMETHING THAT REALLY MAKES SENSE YOU NEED TO HAVE TO BE THERE AND STAY THERE AND UNDERSTAND-- BECAUSE IT’S A VERY QUICK CHANGING ENVIRONMENT HERE. YOU HAVE TO THINK THAT WE ARE FLYING AROUND EARTH AT ABOUT 4 MILES PER SECOND AND THINGS CHANGE REALLY DRAMATICALLY AND REALLY QUICKLY. AND NOT ONLY THAT, YOU DON’T ALWAYS PASS OVER THE SAME PLACE WITH THE SAME CONDITIONS, ACTUALLY ALMOST NEVER. SO ALL THE CONDITIONS CHANGE CONTINUOUSLY-- THE SUN, THE CLOUD COVERAGE, THE SEASONS. I MEAN, THE COLORS, THE MOON, MAKES A LOT OF CHANGES DURING THE NIGHT. SO IT’S BEEN A QUITE INTERESTING TIME HERE IN TRYING TO TAKE ALL OF THIS ARMADA OF EQUIPMENT THAT WE HAVE AND TRY TO MAKE IT DO WHAT WE WANT IT TO DO. NOT ALWAYS HAPPENS, BUT SOMEBODY WILL GET REALLY GREAT, GREAT THINGS SOMETIMES. >> YEAH, SOUNDS LIKE THERE’S A PARTICULAR TECHNIQUE TO TAKE THE ABSOLUTE BEST [PICTURES THAT YOU CAN. AND FROM WHAT YOU’RE SAYING, YOU HAVE TO BE THERE FOR QUITE SOME TIME. AND THIS IS JUST SOMETHING THAT I’VE ALWAYS BEEN INTERESTED IN IN ASKING, BUT I’M SURE THE CUPOLA IS JUST A HOT PLACE TO BE ON THE SPACE STATION TO GET THOSE PHOTOS. SO HOW DO YOU SHARE YOUR TIME? AND WHO GETS TO-- TO SEE WHO GETS TO GO IN THE CUPOLA? >> WELL, PAOLO’S THE BIGGEST SO HE ALWAYS GETS THE FIRST-- HE GETS THE FIRST GO. THERE’S A LOT OF TIME IN THE DAY, BUT WE’RE REALLY BUSY AND SO IF SOMEBODY HAS AN INTEREST, THEY KNOW SOMETHING’S COMING UP THEY WANT TO SEE, THEY LET US ALL KNOW AND WE RESPECT THAT AND LET THEM HAVE THAT SPACE. BUT SOMETIMES, THINGS MIGHT COME UP IN THE MIDDLE OF THE NIGHT, SO IT’S AT TIMES WE’RE ALL IN THERE BECAUSE SOMETHING IS SO COOL AND WE ALL WANT TO SEE IT. AND SOMETIMES, YOU’RE IN THERE BY YOURSELF JUST ENJOYING IT. AND SOMETIMES, YOU DON’T TAKE PICTURES. I’M NOT THE GREATEST PHOTOGRAPHER SO I JUST ENJOY GOING AND LOOKING OUT THE WINDOW. BUT EVERY NOW AND THEN, WE WRESTLE FOR IT AND-- BUT WE MAKE IT WORK. >> NICE. ALL RIGHT, THIS ONE’S FOR JOE TOO FOR YOU, I HAVE TO ASK FROM FACEBOOK, JESSICA SAYS, “MY FIRST GRADERS WOULD LIKE TO KNOW WHAT YOUR FAVORITE PART ABOUT SPACE IS? JOE WAS MY MIDDLE SCHOOL TEACHER AND NOW I’M A TEACHER.” THAT’S PRETTY COOL. >> WOW! THAT’S VERY COOL. HELLO, JESSICA. GLAD THAT YOU’RE FOLLOWING US. THERE ARE SO MANY COOL THINGS ABOUT BEING IN SPACE. ONE OF THEM IS, OF COURSE, FLOATING AROUND. THESE GUYS ARE COOL AND THE RELATIONSHIPS THAT WE FORM ARE REALLY, REALLY COOL. SO I WOULD SAY BEING ABLE TO DO THIS AND JUST KIND OF HANG OUT IN ANY DIRECTION YOU WANT, YOU KIND OF FEEL LIKE A SUPERHERO, SO THAT’S PRETTY COOL. BUT AGAIN, LOOKING BACK AT THE EARTH IS SIMPLY AMAZING. SO JESSICA, I HOPE YOUR FIRST GRADERS GET INSPIRED TO KEEP STUDYING HARD, STUDYING THE STEM FIELDS, AND HOPEFULLY THEY’LL BE DOING MORE THAN WE’RE DOING TODAY ON THE SPACE STATION AND MAYBE THEY’LL BE VISITING OTHER PLANETS. SO THANKS A LOT. >> THANKS, JOE. AND I JUST HAVE TO MENTION, THAT SHE MENTIONED IN THAT COMMENT THAT YOU WERE A FORMER CLASSROOM TEACHER AND YOU’RE UP THERE. FOLLOWING YOU WE’LL HAVE RICKY ARNOLD, WHO IS ALSO A FORMER CLASSROOM TEACHER. AND AS PART OF THAT, WE’RE REALLY TALKING A LOT ABOUT EDUCATION AND HOW IT RELATES TO THE SPACE STATION. SO YOU CAN GO LOOK UP STEM ON STATION AND THERE’S A WEBSITE OUT THERE, AND EDUCATORS CAN FIND A LOT OF COOL RESOURCES THERE. >> ABSOLUTELY. >> ALL RIGHT, I GOT ANOTHER QUESTION ON FACEBOOK. THIS IS FROM JACE, “WERE YOU ABLE TO OPERATE PROFESSIONAL CAMERAS BEFORE BECOMING ASTRONAUTS, OR DID YOU LEARN ABOUT PHOTOGRAPHY DURING TRAINING? >> I NEVER TOUCHED A PROFESSIONAL CAMERA UNTIL I BECAME AN ASTRONAUT. AND THAT’S BEEN ONE OF THE REALLY NEAT OPPORTUNITIES ABOUT BEING AN ASTRONAUT IS THE-- LIKE THE VERY FANCY CAMERAS LIKE THE RED CAMERA THAT PAOLO MENTIONED. IT’S PRETTY IMPRESSIVE ARRAY OF EQUIPMENT AND THE GREAT TRAINERS TO HELP US LEARN HOW TO USE THEM. >> SO SABOT, I MEAN, YOU’VE BEEN UP THERE-- THIS IS YOUR FIRST SPACE FLIGHT AND YOU HAVE A UNIQUE PERSPECTIVE BEING A FIRST TIME FLYER, BUT ESPECIALLY I WAS WATCHING YOU ON YOUR SPACEWALK AND YOU GOT A COUPLE MOMENTS TO-- DURING THE SPACEWALK LOOK DOWN AT THE EARTH. SO CAN YOU SORT OF DESCRIBE THAT EXPERIENCE? >> IT’S HARD TO TAKE IT ALL IN. IT’S SO MASSIVE. IT’ EVERYWHERE. THE THINGS THAT STUCK OUT IN MY MIND WERE SEEING-- AT NIGHT, SEEING FLASHES OF LIGHTENING THAT WENT ON FOR ABOUT FIVE MINUTES. THE BRIGHT SUNLIGHT, IT WAS VERY IMPRESSIVE. IN FACT, I’LL NEVER FORGET WHEN-- ON THE VERY FIRST SPACEWALK WHEN RANDY OPENED THE HATCH THE AIRLOCK JUST LIT UP BECAUSE OF ALL THE REFLECTED LIGHT COMING FROM THE EARTH INTO THE AIRLOCK. AND THE AIRLOCK’S A VERY CONFINED PLACE. IT DOESN’T HAVE-- IT’S WELL LIT, BUT IT’S NOT LIT LIKE THE SUN, AND SO IT CHANGED THE FEELING OF THE AIRLOCK DRAMATICALLY WHEN THAT HATCH OPENED UP AND THEN IT REALLY FELT REAL TO ME. >> THAT’S AWESOME. ALL RIGHT, ANOTHER QUESTION. COLIN ON FACEBOOK WANTS TO KNOW, “IF YOU GUYS TAKE SPACE SELFIES UP THERE?” MAYBE YOU GOT TO TAKE ONE ON YOUR SPACEWALK. >> [ INDISTINCT ]. >> GO AHEAD, GO AHEAD. >> YEAH, I JUST POSTED SOMETHING FROM OUR LAST SPACEWALK ON TUESDAY WITH THE SPACE SELFIE AND TRIED TO EXPLAIN TO PEOPLE BECAUSE YOU GOT THESE BIG INFLATED GLOVES ON AND YOU’RE TRYING TO TAKE THIS CAMERA. AND IT’S LIKE IF YOU WENT TO YOUR OVEN, AND GRABBED YOUR OVEN MITTS, AND THEN GRABBED YOUR CAMERA AND TRIED TO TAKE THE SELFIE. THAT’S WHAT IT’S KIND OF LIKE IN SPACE TRYING TO DO THAT, AND LINE IT UP, AND FEEL FOR THE BUTTON, AND GET THE SHOT. SO YOU END UP TRYING TO SQUEEZE IT A FEW TIMES. HOPEFULLY YOU SEE MAYBE THE SHUTTER ACTUALLY TOOK THE PICTURE. AND THEN YOU COME BACK INSIDE LATER ON AND GO, “HEY, DID I GET ANYTHING?” >> AMAZING. HEY, SO PAOLO, WE WERE KIND OF LOOKING AT SOME OF YOUR PHOTOS ON TWITTER, JUST THE ONES THAT YOU’RE SHARING. I SEE A LOT OF AMAZING PICTURES OF ITALY, BUT ONE THAT REALLY STUCK OUT IN MY MIND WAS A PICTURE OF MADAGASCAR AND THE LOGGING GOING ON THERE. JUST FROM THE PERSPECTIVE THAT YOU SEE OF THE EARTH, WHAT SORTS OF IDEAS OF HUMAN INFLUENCE DO YOU SEE FROM 250 MILES ABOVE THE EARTH? >> WELL, WHEN YOU COME UP HERE AND YOU LOOK OUT OF THE WINDOW, AND MOST OF THE TIME YOU SEE OCEAN AND CLOUDS, AND THEN SOMETIMES YOU EVEN HAVE DIFFICULTIES ON SEEING THE ACTUAL GROUND, THE CONTINENTS. AND THEN LITTLE BY LITTLE YOU START ACQUIRING THIS ACUITY, YOU LITERALLY START SEEING DETAILS. AND AT THE BEGINNING, THE HUMAN PRESENCE IS NOT SO EVIDENT, AND THEN IT BECOMES MORE AND MORE AND MORE EVIDENT, UP TO THE POINT THAT WHEN YOU GO THERE AND IT’S NIGHT YOU ESSENTIALLY SEE THE PLANET LIT UP, ALL THE CONTINENT’S LIT UP LIKE A CHRISTMAS TREE. AND IN SOME OF THE PLACES IN EUROPE AND THE UNITED STATES ARE THE PRESENCE OF THE HUMAN BEINGS. IT’S INCREDIBLE. AND THEN, YOU START FOCUSING ON OTHER THINGS, LIKE YOU SEE RIVERS, YOU SEE HOW THERE’S A SHAPE. YOU SEE HOW THINGS HAVE CHANGED, HOW AS HUMAN BEINGS HAVE TRYING TO MODEL NATURE ACCORDING TO OUR NEEDS AND NOT OURSELF ACCORDING TO THE NEEDS OF NATURE. AND THIS CHANGE BECOMES REALLY APPARENT. THERE IN THAT PICTURE THAT YOU’RE REFERRING TO, YOU SEE ESSENTIALLY ALL THE RED DIRT THAT IS WASHING OVER ON THE OCEAN. NOT ANYMORE KEPT BY THE FOREST BY THE PLANTS-- BY THE PLANTS THERE IN MADAGASCAR. AND THIS IS SO EVIDENT IT’S REALLY CLEAR FROM UP HERE THAT WE ARE A MAJOR FORCE INTO THIS PLANET AND WE ARE CHANGING NATURE. IS THAT GOOD, IS THAT BAD? I’M NOT SURE ABOUT IT. FOR SURE WE PROBABLY NEED TO PAY ATTENTION TO WHAT WE ARE DOING IF WE WANT TO KEEP THE ENVIRONMENT AS IT IS TODAY OR YESTERDAY. >> WOW, THAT’S REALLY INTERESTING. SIMILAR TO THAT, NATALIE IS ASKING, “IF YOU’VE OBSERVED A CHANGE IN COLOR OF THE SUNRISES AND SUNSETS DUE TO THE WILDFIRES ACROSS NORTH AMERICA?” OR MAYBE IF YOU’VE BEEN ABLE TO SEE ANYTHING, ANY OF THE WILDFIRES?” >> WE’VE SEEN THE WILDFIRES WHEN WE WERE OVER IN OREGON AND WASHINGTON LAST MONTH. UNFORTUNATELY, THE WAY OUR DAY CYCLE WORKS, WE’RE NOT GOING OVER CALIFORNIA WHERE A TIME WHERE WE’RE TYPICALLY LOOKING OUTSIDE DURING DAYLIGHT. SO NONE OF US HAVE REALLY SEEN THE NORTHERN CALIFORNIA WILDFIRES THAT MUCH YET. YOU CAN SEE CERTAINLY THE SMOKE OBSCURES THE LOOK DOWN, BUT HAVEN’T SEEN ANY CHANGES TO THE OVERALL ATMOSPHERE OR THE COLOR OF THE SUN BECAUSE IT’S JUST NOT THAT MANY-- THAT MUCH PARTICULATE WHEN YOU’RE LOOKING AT IT AT A GLOBAL SCALE. >> SO KOMRADE, KIND OF SIMILAR QUESTION. RECENTLY, AGAIN, WE WERE LOOKING AT A LOT OF THE PHOTOS THAT YOU’RE SHARING ON SOCIAL MEDIA, BUT RECENTLY THERE’VE BEEN QUITE A FEW HURRICANES THAT HAVE HIT THE UNITED STATES, PUERTO RICO, A LOT OF THE CARIBBEAN ISLANDS AND YOU SHARED YOUR PERSPECTIVE OF THAT VIEW. CAN YOU-- I MEAN, THE PICTURES CAN TELL ONE STORY, BUT JUST FROM YOUR PERSPECTIVE, WHAT WAS IT LIKE SEEING IT FROM THE SPACE STATION, THE HURRICANES? >> CERTAINLY, THE FORMATION OF WEATHER CAN BE A REAL BEAUTIFUL THING AND HURRICANES HAVE THEIR OWN SHAPE AND DO AMAZING THINGS WITH THE CLOUDS. BUT IT’S WHEN YOU REALIZE THE DESTRUCTIVE POWER UNDERNEATH IT IT CEASES BEING AS BEAUTIFUL. AND CERTAINLY, THE FIRST ONE FOR US WAS HURRICANE HARVEY THAT WENT RIGHT OVER OUR FAMILIES, AND OUR HOMES, AND OUR FRIENDS, AND MISSION CONTROL DOWN THERE IN HOUSTON. AND SO, THAT WAS-- YOU SAY, “TOO CLOSE TO HOME.” WELL, THAT WAS AT HOME SO THAT WAS TOO CLOSE TO HOME FOR US. SO THEN THE PARADE OF HURRICANES AFTER THAT WAS JUST DISHEARTENING BECAUSE THERE WERE JUST SO MANY, AND SO MANY PEOPLE AFFECTED, AND SO MUCH DEVASTATION THAT IT-- WE WERE TAKING PICTURES TO HOPEFULLY HELP THE RESEARCHERS THAT ARE USING THOSE TO FIGURE OUT HOW HURRICANES FORM, HOW THEY CONTINUE TO MANIFEST THEMSELVES, WHAT WE CAN DO TO PROTECT OURSELVES. AND THEN, IT WAS TAKING PICTURES AFTERWARDS, HIGH RESOLUTION PHOTOGRAPHY, MAPPING THE AREAS TO SHOW WHERE THERE WAS FLOODING OR DESTRUCTION THAT WE DIDN’T KNOW ABOUT AT THAT POINT BECAUSE THERE STILL WASN’T COMMUNICATION OR CAMERA CREWS WERE ABLE TO GO OUT AND PICTURE STUFF. PICKING UP AT 24:00 SO IT WAS AN UNFORTUNATE PROJECT THAT WE ENDED UP DOING, BUT HOPEFULLY THE WORK WE DID UP HERE TRANSLATES INTO SOME SCIENCE, AND WE’RE ABLE TO TRANSLATE IT INTO ACTUAL PRACTICAL STUFF THAT’LL HELP PEOPLE IN THE FUTURE. >> I WOULD THINK IT DID. IT’S SUCH A UNIQUE PERSPECTIVE. >> YEAH, ABSOLUTELY. SEEING THE HURRICANES AND THE FLOODING AND ALL OF THAT FROM SPACE IS JUST REALLY AN OUTSIDE PERSPECTIVE THAT YOU JUST CAN’T SEE WHEN YOU ARE RIGHT HERE NEXT TO IT. SO IT’S VERY INTERESTING. AND SIMILAR TO THAT, NATALIE WANTS TO KNOW IF YOU COULD TALK TO US ABOUT THE WORF RACK, WHAT TYPES OF PHOTOS DO YOU TAKE FROM THERE, AND HOW DO YOU USE PHOTOGRAPHY FOR SCIENCE. >> YEAH, SO WE HAVE VARIOUS PROJECTS THAT WE’LL DO, AND ACTUALLY THE WORF RACK IS RIGHT HERE BENEATH US. IT’S ONE OF THE BEST WINDOWS THAT WE HAVE ON THE SPACE STATION. IT’S VERY WELL PROTECTED, SO VERY PRISTINE, AND WE CAN GET SOME REALLY COOL PHOTOS. UNFORTUNATELY FOR US, IT’S USUALLY COVERED UP, SO WE DON’T GET AN OPPORTUNITY TO USE IT TOO OFTEN. BUT THERE’S A LOT OF SCIENCE THAT GOES ON. I KNOW WHEN I WAS HERE LAST TIME, WE HAD THE EARTHCAM PROJECT GOING ON WHERE MIDDLE SCHOOL CHILDREN WERE TAKING PHOTOS AND LEARNING ABOUT THOSE DIFFERENT PARTS OF THE WORLD. WE WERE ALSO USING IT FOR AGRICULTURAL PURPOSES TO MAP DIFFERENT THINGS, SO IT’S A MULTIPURPOSE WINDOW, AND IT IS JUST A VERY UNIQUE PERSPECTIVE THAT YOU CAN GET FROM HERE. AND THEN YOU CAN PUT THE CAMERAS AT DIFFERENT ANGLES, YOU CAN DO THE DIFFERENT TIMES OF THE YEAR, DIFFERENT TIMES OF THE DAY. SO IT HAS A LOT OF FLEXIBILITY. IT’S PRETTY COOL. >> [ INDISTINCT ] >> THERE’S ALSO-- I KNOW WE’VE DONE-- THERE’S AN EXPERIMENT THAT’S BEEN GOING ON WITH ANALYZING THE SPECTRUM OF METEORS THAT ARE FALLING TOWARDS THE EARTH AND USING DIFFRACTION GRATINGS WITH THE LENS. SO THERE’S SOME REALLY INTERESTING SCIENCE THAT CAN COME OUT OF PHOTOGRAPHY. >> SO SABOT AND JOE, BOTH OF YOU HAVE BEEN EDUCATORS IN THE PAST, AND-- JOE JUST BEING A MIDDLE SCHOOL TEACHER, AND SABOT WITH-- AT WEST POINT. BUT IS THERE SORT OF AN EDUCATION PERSPECTIVE THAT YOU CAN DO FROM SHARING YOUR VIEW OF THE EARTH? OR MAYBE SOME OTHER EXPERIMENTS YOU’RE DOING ONBOARD THE STATION THAT YOU CAN USE TO SHARE WITH OTHERS. >> WELL, I THINK AS AN EDUCATOR, ONE OF THE MOST IMPORTANT TOOLS THAT YOU CAN HAVE IS SHARING EXPERIENCES AND REAL LIFE EXPERIENCES. SO AS MUCH AS WE CAN DO THAT TO HELP TEACHERS THAT ARE OUT THERE AND PROVIDE THEM MORE TOOLS TO DO THEIR JOB. SINCE WE’VE BEEN HERE, IT’S BEEN NON-STOP. IT’S KIND OF LIKE THE BEGINNING OF THE SCHOOL YEAR, WHERE YOU’RE KIND OF GETTING ON YOUR FEET, GETTING THE BALL ROLLING. BUT THEN WE HAD DRAGON, AND THEN WE HAD TWO SPACEWALKS ALREADY, SO TO BE HONEST WITH YOU, THAT’S THE KIND OF EXPERIENCE THAT WE WANT TO SHARE. AND HOPEFULLY BY DOING THAT AND BY RECORDING THAT, WHETHER IT’S WITH PHOTOS, VIDEO-- WE CAN SHARE THAT EXPERIENCES WITH TEACHERS WHO CAN THEN SHARE THAT WITH THEIR STUDENTS. >> THAT’S AWESOME. IT’S SO INTERESTING TO SO MANY OF US DOWN HERE, SO WE APPRECIATE BEING ABLE TO HEAR ABOUT THE AWESOME WORK YOU GUYS ARE DOING. I HAVE TO MENTION, KOMRADE, I’M GETTING A LOT OF COMMENTS ON FACEBOOK ABOUT YOUR SHIRT-- PEOPLE REALLY LOVE IT, SO I HAD TO TELL YOU THAT. JOSEPH WANTS TO KNOW, “WHAT’S THE MOST AMAZING PHOTO YOU TOOK?” SO DOES ANYBODY HAVE A FAVORITE PICTURE YET SO FAR? >> IT’S-- IT’S RELATIVELY EASY UP HERE TO DO TIME LAPSES, WHICH MEANS A LOT OF PHOTOS. AND THEY CAN GO GOOD OR TOTALLY BAD. I MEAN, I’VE DONE THOUSAND PICTURE COMPLETELY WASTED. THANK GOD IT’S NOT FILM ANYMORE AND ELECTRONS DON’T COST TOO MUCH. BUT I GOT A COUPLE OF TIME LAPSES PRETTY GOOD. THE ONE THAT I THINK WAS PROBABLY THE BEST IS ONE OF THE AURORA IN THE NORTH. SO IT WAS AURORA BOREALIS. AND I CAN-- I DON’T KNOW THAT NIGHT WHAT HAPPENED, BUT THE SPACE OF THE AURORA, THE COLORS TOWARD THE GROUND, AND THE SHADOWS WENT ALL THE WAY DOWN UNDER US. AND THIS WAS, TO ME, INCREDIBLE, ALL THAT SEQUENCE OF PICTURES. >> AND I THINK PAOLO MENTIONED EARLIER ABOUT THE EARTH IS EVER CHANGING. FOR ME, TO PICK OUT ONE AFTER JUST THE FEW MONTHS WE’VE BEEN HERE IS IMPOSSIBLE. IT’S EVERY DAY THERE’S ONE OR TWO THAT I GO, “WOW, THAT WAS JUST SO AMAZING. I’M SO FORTUNATE TO BE ABLE TO HAVE SEEN THAT.” AND THAT’S A LOT OF THE STUFF THAT WE’RE TRYING TO POST AND SHARE WITH YOU GUYS, BECAUSE EVERY DAY IS FULL OF AMAZING PICTURES. AND MY FOLDER OF AMAZING PICTURES FROM SPACE JUST KEEPS GROWING DAILY. >> I’D SAY MY FAVORITE PHOTO SO FAR IS ONE OF, FRANKLY, ITALY AND THE ALPS THAT WE HAPPENED-- I THINK KOMRADE DREW MY ATTENTION TO IT, GOT ME TO LOOK DOWN DURING THE SPACEWALK, AND I SNAPPED A COUPLE PICTURES. THE CAMERA DID A LOT OF GREAT WORK FOR ME, BECAUSE ALL I COULD REALLY DO IN THAT SITUATION WAS PRESS THE BUTTON. AND THE PICTURES TURNED OUT GREAT-- REALLY BRIGHTLY LIT JAPANESE MODULE OF THE SPACE STATION IN THE FOREGROUND, AND ITALY AND THE ALPS IN THE BACKGROUND. >> [ INDISTINCT ]. >> YEAH, AND IF I COULD JUST ADD, PROBABLY ONE OF MY FAVORITES WAS TAKEN JUST A FEW MINUTES AGO. AND KOMRADE AND I HAD A CONFERENCE THAT WAS SCHEDULED WITH SOME OF OUR FLIGHT DIRECTORS LOOKING AT THE UPCOMING SPACEWALK, AND ASKED OF ME, “WHERE ARE WE RIGHT NOW?” HE’S LIKE, “I THINK THAT’S SOUTH AMERICA.” AND I SAID, “WELL, IS PUERTO RICO GOING TO BE COMING UP?” AND HE’S LIKE, “WOW, THERE IT IS RIGHT THERE.” SO WE GRABBED CAMERAS RIGHT AWAY, AND IT WAS JUST A BEAUTIFUL DAY. I KNOW PEOPLE ARE STILL RECOVERING OVER IN PUERTO RICO, SO HOPEFULLY I CAN GET THESE PICTURES OUT AND THEY CAN SEE HOW BEAUTIFUL THEIR ISLAND LOOKS FROM UP HERE. BUT IT WAS PRETTY COOL TO TAKE THAT TODAY. >> WOW, GOOD TIMING. THAT IS AWESOME. WE CAN’T WAIT TO SEE THOSE PICTURES, AND I KNOW THE PEOPLE IN PUERTO RICO WILL BE REALLY, REALLY ANXIOUS TO SEE THAT. ALL RIGHT, SO WE’VE GOT A COUPLE QUESTIONS ABOUT THE EXPOSURE TIMES ON YOUR CAMERAS. CAN YOU GUYS TALK A LITTLE BIT ABOUT THAT? >> TYPICALLY FOR DAYTIME EARTH OBS, WE’RE SHOOTING, A LOT OF TIMES, SHUTTER PRIORITY AND WE’RE SHOOTING FOR ONE OVER THE FOCAL LENGTH. SO IF YOU’VE GOT A 400MM LENS LIKE THIS BIG MONSTER, YOU’RE SHOOTING 1/400 AND LETTING THE CAMERA TAKE CARE OF THE APERTURE. NIGHTTIME IS CERTAINLY DIFFERENT. DEPENDS ON WHETHER OR NOT WE’VE GOT MOON OR WE DON’T. AT THAT POINT, WE’RE SETTING UP THE CAMERAS ON ARMS SO THAT WE’RE NOT JIGGLING THEM, LIKE A TRIPOD ON THE GROUND. AND WE’RE SHOOTING ANYWHERE FROM A SECOND, TO TWO SECOND, UP TO EVEN-- PAOLO WAS SHOOTING THIS WEEK A TENTH OF A SECOND BECAUSE IT WAS SO BRIGHT WITH THE MOON OVER THE GROUND. SO YOU KIND OF ADJUST FOR THE CONDITIONS TO BE ABLE TO GET THE SHOTS ON THE TIME OF DAY. >> GREAT, THANKS. ALL RIGHT, JESSICA IS SAYING, “HI FROM CHICAGO. CAN YOU RECALL A TIME WHEN YOU SAW SOMETHING FROM UP THERE THAT WAS IMPOSSIBLE TO BE CAPTURED ON CAMERA, OR SOMETHING THAT JUST DOESN’T DO JUSTICE ON CAMERA THAT YOU WISH TO SHARE?” >> IT’S REALLY INTERESTING, BECAUSE YOU NEVER KNOW WHAT YOU’RE GOING TO GET. AND ACTUALLY, YOU NEVER KNOW WHAT YOU’RE GOING TO SEE, TO START WITH. MORE OR LESS YOU CAN PREDICT, BUT THE CONDITION CHANGES SO DRASTICALLY THAT YOU CAN WAIT FOR THE WHOLE DAY FOR A PASS OVER ITALY, FOR EXAMPLE, JUST TO DISCOVER THAT IT’S COMPLETELY COVERED BY CLOUDS. YOU DON’T EVEN SEE WHERE IT IS. OR THE OPPOSITE. OR YOU’RE DOING SOMETHING, YOU’RE THERE DOING EXERCISE. WE HAVE THE CUPOLA RIGHT THERE WHERE WE’RE DOING EXERCISE. YOU’RE THERE DOING A SET OF SOMETHING AND SUDDENLY, AN ISLAND APPEARS OUT OF THE BLUE AND IS INCREDIBLE COLORS. [ LAUGHTER ] I JUST LOST THE QUESTION. WHAT WAS THE QUESTION? >> [ INDISTINCT ]. >> AH, YES. SO THERE ARE A LOT OF THINGS THAT CANNOT BE-- I MEAN, THE CAMERA CANNOT TRANSLATE, AND-- BECAUSE IT’S VERY DIFFICULT TO SEE THE LIGHT. FOR EXAMPLE, I FIND IT VERY DIFFICULT TO TAKE PICTURES WHEN THE SUN GOES DOWN, BECAUSE THERE IS THIS HUGE BRIGHT SUN THERE AND YOU’RE TRYING TO CAPTURE SOMETHING ELSE AND YOU CANNOT DO IT. SO IN SPACE, THERE ARE HUGE CONTRASTS BETWEEN THE FULL DAY AND THE FULL NIGHT. THERE IS NOTHING IN THE MIDDLE THERE, AND IT’S VERY DIFFICULT TO TRANSITION. FOR EXAMPLE, WHEN WE DO A NIGHTTIME TIME LAPSES AND WE SET UP THE CAMERA FOR NIGHT, AS SOON AS WE GET THE SUN, JUST A LITTLE BIT OF SUN OUT IT’S TOTALLY WASHED OUT. AND I WOULD LOVE, FOR EXAMPLE, TO SHOW THIS TRANSITION AS WE SEE IT WITH THE EYE THAT ADJUSTS CONTINUOUSLY. THIS TRANSITION FROM NIGHT TO DAY, THIS IS SOMETHING THAT I STILL HAVEN’T FIGURED OUT A WAY TO DO IT. MAYBE WE’LL THINK ABOUT IT AND WE’LL WORK ON IT. >> WELL, KOMRADE, THAT KIND OF MAKES ME THINK OF-- I KNOW VERY SOON-- I THINK ON OCTOBER 23rd YOU WANT TO DO A SORT OF AROUND THE WORLD IN 90 MINUTES AND THEN KIND OF SHARE YOUR PERSPECTIVE OF A GREAT PASS OVER A LOT OF POPULATED CITIES AND VARIOUS FEATURES OF THE EARTH. CAN YOU TALK ABOUT WHAT YOUR PLANS ARE FOR THAT, WHAT YOU’RE GOING TO DO OVER THOSE 90 MINUTES? >> WELL, IT’S NOT JUST ME. IT’S GOING TO END UP BEING A CREW PROJECT. AND THE THOUGHT WAS TO SHOW EVERYBODY ON THE GROUND WHAT IT’S LIKE, AND THE FEATURES THAT CAPTURE OUR ATTENTION DURING EACH MINUTE OF THOSE 90 MINUTES IN ONE REVOLUTION OF THE EARTH, WHETHER IT’S DAY OR NIGHT. AND IDEALLY PEOPLE ARE ENGAGED AND THEY CAN THEN ADD TO THE PROJECT AND THE CONVERSATION-- WHAT WAS GOING ON ON THE GROUND AT THAT MOMENT THEMSELVES-- AND KIND OF CREATE THIS MOMENT IN TIME WHERE WE CIRCLE THE GLOBE, AND WHAT WAS THE WORLD DOING AT THAT MOMENT? AND SO WE’LL BE TRYING TO TAKE THOSE PICTURES. I THINK WE HAVEN’T QUITE SETTLED ON A DATE YET, BUT YES, IT’LL BE AFTER WE FINISH OUR LAST EVAs, AND SOMETHING THAT WE HOPE IS A GLOBAL PROJECT THAT’LL INCLUDE MOST OF THE WORLD’S POPULATION THAT WE CAN GET IN A SINGLE PASS, AND REALLY SHOW OFF, SHOWCASE ONE REVOLUTION OF OUR PLANET. >> CAN’T WAIT TO SEE WHAT YOU HAVE PLANNED FOR THAT. WELL, GENTLEMEN, THANK YOU SO MUCH FOR TAKING THE TIME TO COME ON THE PODCAST TODAY AND SHARE YOUR PERSPECTIVE OF EARTH. IT’S JUST SO UNIQUE-- LITERALLY NO ONE ELSE ON THIS PLANET HAS THAT PERSPECTIVE. SO THANK YOU SO MUCH FOR TAKING THE TIME TO DO THAT. AND I KNOW THIS IS THE END OF THE DAY FOR YOU, TOO, SO AGAIN, APPRECIATE ALL FOUR OF YOU PARTICIPATING IN THIS. SO JUST WANT TO WISH YOU THE BEST OF LUCK ON THE REST OF YOUR MISSION, AND GODSPEED. CAN’T WAIT TIL YOU GUYS GET HOME. >> THANK YOU VERY MUCH, GARY. WE’LL LOOK FORWARD TO THE NEXT TIME WE GET TO TALK TO YOU, AND READY-- BREAK. >> STATION, THIS IS HOUSTON ACR. THAT CONCLUDES THE EVENT. >> THANK YOU TO ALL THE PARTICIPANTS FROM JSC PAO. STATION, WE ARE NOW RESUMING OPERATIONAL AUDIO COMMUNICATION. >> AW, FANTASTIC. HOW ‘BOUT THAT, MEGAN? >> THAT WAS AMAZING! >> FOUR ASTRONAUTS. WE GOT TO SEE THEIR PERSPECTIVE OF THE PLANET. AND I KNOW WE WERE THROWN SOME IMAGES-- THOSE WERE ACTUAL IMAGES THAT THEY TOOK WHILE THEY WERE ACTUALLY-- SOME OF THE STILL PHOTOGRAPHY THAT THE CAMERA THEY ACTUALLY SHOWED WHILE THEY WERE UP THERE, BUT THEN SOME OF THOSE TIME LAPSES THAT PAOLO WAS TALKING ABOUT, TOO. ABSOLUTELY JUST SUCH A UNIQUE PERSPECTIVE. >> YEAH, IT’S SO COOL TO TALK TO THEM AND TO HEAR A LITTLE BIT ABOUT THEIR EXPERIENCE. AND OF COURSE, YOU CAN SEE ALL THOSE PICTURES ON THEIR SOCIAL MEDIA SITES. AND JUST AMAZING PICTURES THEY’VE TAKEN. >> YEAH, LET’S GO THROUGH THEM. SO WHO CAN WE FOLLOW ON THE STATION? >> ALL RIGHT, SO ALL FOUR OF THOSE GUYS WE JUST TALKED TO ARE ALL ON TWITTER, SO YOU CAN FOLLOW THEM ALL ON TWITTER. KOMRADE IS @ASTROKOMRADE. JOE IS @ASTROACABA. SABOT IS @ASTRO_SABOT. PAOLO IS @ASTRO_PAOLO. AND YOU CAN FOLLOW ALL THE ASTRONAUTS AT @NASA_ASTRONAUTS. AND ALSO, KOMRADE AND PAOLO ARE ALSO ON INSTAGRAM. SO IF YOU LIKE INSTAGRAM, YOU CAN LOOK THEM UP ON INSTAGRAM AND SEE ALL THEIR PICTURES. >> THAT’S RIGHT, YEAH. AND WE TRY TO KIND OF CONSOLIDATE THAT INTO THAT ASTRONAUTS ACCOUNT, TOO, SO YOU CAN JUST SEE EVERYONE’S PICTURES. AND THEY ARE SOME AMAZING PHOTOS. AGAIN, THESE PHOTOS THAT WE’RE SHARING WITH YOU, A LOT OF THEM WERE ACTUALLY SHARED ON THEIR TWITTER ACCOUNT, SO YOU CAN FOLLOW ALONG ON THAT JOURNEY. AND I KNOW THAT EACH OF THEM HAVE A COUPLE MONTHS LEFT, SO THERE’S PLENTY OF IMAGES TO SEE OVER THESE NEXT COUPLE OF MONTHS. IF YOU HAVE A QUESTION ABOUT ASTRONAUT PHOTOGRAPHY OR ANYTHING NASA RELATED, JUST GO ON YOUR FAVORITE SOCIAL MEDIA NETWORK AND USE THE HASHTAG #ASKNASA. IF YOU WANT TO ASK US SPECIFICALLY A QUESTION ON “HOUSTON, WE HAVE A PODCAST” JUST MENTION US IN THAT #ASKNASA QUESTION. #HWHAP I THINK IS THE ONE WE LIKE TO USE FOR HWHAP JUST SO YOU CAN LIMIT ALL THOSE CHARACTERS, ESPECIALLY FOR TWITTER. BUT IF YOU’RE NOT FOLLOWING “HOUSTON,WE HAVE A PODCAST” ALREADY, SHAMELESS PLUG. I’D SAY GO AND SUBSCRIBE ON WHATEVER PODCAST AVENUE YOU LISTEN TO. I KNOW WE’RE ON iTUNES, SOUNDCLOUD, AND NASA.GOV. WE JUST RECENTLY GOT ON GOOGLE PLAY, SO WHATEVER MEDIUM YOU LIKE TO LISTEN TO YOUR PODCASTS AT. SO I THINK THAT’LL DO IT FOR US HERE. AGAIN, IF YOU HAVE ANY QUESTIONS, USE THE HASHTAG #NASA, AND BE SURE TO SUBSCRIBE TO “HOUSTON, WE HAVE A PODCAST.” AND WE’LL SEE YOU NEXT TIME, HOPEFULLY THE NEXT TIME WE’RE ON CAMERA TALKING TO SPACE. >> YEAH. >> I HOPE SO. SO SUBSCRIBE TO “HOUSTON, WE HAVE A PODCAST.” WE’LL SEE YOU NEXT TIME. [ MUSIC ] [ INDISTINCT RADIO CHATTER ] >> WELCOME TO SPACE. >> HEY, THANKS FOR STICKING AROUND. SO I THINK WE PLUGGED MOST OF THE THINGS THAT WE WANTED TO TALK ABOUT, ALL THE ASTRONAUT ACCOUNTS THAT YOU CAN FOLLOW, AND NASA ASTRONAUTS, AND WHERE YOU CAN SUBSCRIBE TO “HOUSTON, WE HAVE A PODCAST,” WHICH, IF YOU’RE LISTENING TO THIS RIGHT NOW, CONGRATULATIONS-- YOU DID A GOOD JOB. BUT THIS PODCAST WAS RECORDED ON OCTOBER 13, 2017. THANKS TO ALEX PERRYMAN, JOHN STOLL, TOMMY [ INDISTINCT ], PAULA VARGAS, CHARLES CLENDANIEL, GREG WISEMAN, BILL STAFFORD, JOSH VALCARCEL, ROB NAVIAS, AND OF COURSE MEGAN SUMNER. THANKS AGAIN TO KOMRADE, SABOT, JOE ACABA, AND PAOLO NESPOLI FOR COMING ON THE SHOW. WE’LL BE BACK NEXT WEEK.

Houston, We Have a Podcast. Episode 41 The Space Launch System Part.1

NASA Image and Video Library

2018-04-20

Production Transcript for Ep41 The Space Launch System Part.1.mp3 Gary Jordan (Host): Houston, we have a podcast. Welcome to the official podcast of the NASA Johnson Space Center Episode 41, the Space Launch System part one. I'm Gary Jordan, and I'll be your host today. On this podcast, we bring in the experts, NASA scientists, engineers, astronauts, all to let you know the coolest information right here at NASA. So, today, we're talking about the most powerful rocket since the Saturn V moon rocket. It's called NASA's Space Launch System. So, we've got two guests from Marshall Space Flight Center in Huntsville, Alabama here with us today to tell us a little bit about the rocket, the payloads it will carry. Don't worry. We'll define what a payload is. And then, where it's going to go. Spoiler alert, it will bring people big stuff and little stuff all farther than we've ever gone before. Wait. Why did I do that? That totally ruins the, oh wait. Never mind. It doesn't ruin anything. This is a really good topic, jam packed with information. So much information that we're going to do this in two parts. This is part one. So, with us today are David Smith and Paul Bookout. David is the Vice President for Advanced Programs at Victory Solutions in Huntsville, Alabama. He has a long career in aerospace engineering and is a Subject Matter Expert on rocket architecture and how payloads fit inside the rocket. He wrote the SLS mission planner's guide which gives payload developers a general idea of the capabilities of the rocket and some technical specifications, so they can determine how their payloads might fit inside of it. He looks after some of the big payloads. Our other guest is Dr. Paul Bookout, EM-1 Secondary Payloads Integration Manager who manages integration of five CubeSats in the giant rocket as well as the avionics that will control deployment of the 13 small satellite payloads on the first mission of SLS and Orion called Exploration Mission-1, EM-1. He spends his time managing the little payloads, not much bigger than a shoebox, that goes inside of a skyscraper-sized rocket. So, we're going to be talking about just how powerful this monster rocket is, its unique capabilities, and what it will be used for, where it is in its development, its first mission with the Orion crew vehicle, and then look ahead to the future to missions to the moon, to Mars, and throughout the solar system. So, we are go for launch with Mr. David Smith and Dr. Paul Bookout for the Space Launch System Program. T minus five, four, three, two, one, zero, and liftoff of Episode 41 of Houston, We Have a Podcast. Always wanted to do that. Feel like I just ruined it. You know what? Let's just start. [ Music ] Host: T minus five second and counting. Mark. [ Music ] Host: There she goes. Host: Houston, we have a podcast. [ Music ] Host: All right. Paul and David, thanks so much for coming on the podcast today. We talked about Orion on a few episodes so far but really haven't had the privilege to talk about he giant rocket that Orion is going to be on, the SLS. And, we have you guys here from Marshall to actually talk to us about this rocket. So, thank you very much for coming on. David Smith: Sure. David Smith: Thank you for having us. Host: Our pleasure. Host: All right. Just to sort of back up, we have Paul Bookout and David Smith, so you guys want to talk a little bit about each one, so we can identify your voices. Paul Bookout: David, go ahead. David Smith: Well, sure. I'm just an engineer. My associate Dr. Bookout is a doctor. Host: Okay. David Smith: But, we both work together on trying to find innovative ways to associate payloads with the capability of SLS which is going to be the world's largest rocket. So, I kind of look at the larger payloads, and Dr. Bookout looks at maybe some of the other kind, smaller payloads that can fit in the niches that are left over. Paul Bookout: Well, thank you Vice President David. David Smith: Yes. Paul Bookout: I appreciate you talking about introducing myself. So, what we have is secondary payloads. Again, we're just trying to understand the whole utilization of SLS since it's going to be the most powerful rocket built since the Saturn V. It's going to have a lot more capability, so we want to utilize it to its fullest. Host: Okay. So, you said there's going to be, basically, we're going to utilize the rocket to its maximum potential. We got this big rocket, and we're going to test it. But, while we test it, let's put some cool stuff on it. Paul Bookout: Exactly. Host: So, let's back up and talk about just SLS. What is SLS? What is this giant rocket that we're talking about? Paul Bookout: SLS is America's rocket. It's the next NASA's launch vehicle that's going to be able to put humans back to the moon and further out into deep space. Of course, a lot of it's built on shuttle hardware heritage. The SLS rocket's made up of the solar rocket boosters, a main core, an upper stage, and then the crew Orion spacecraft with a co-manifest payload or a primary payload. And, David will talk a little bit more about that later. So, of course, this is NASA's first exploration class launch vehicle since Saturn V, so we're going to be putting humans back to the moon, out to deep space, and eventually, you know, to Mars systems. It has a very large mass lift capability and also volume, so some of these larger probes that are satellites or probes that are going to outer planets that they'll be able to arrive at their destination in just a few years instead of maybe eight to ten years. [00:05:24] You're cutting that trip down to one or two years. So, it's a lot of savings there. Host: So, that's a really important part to kind of hone in on is just the versatility of this rocket. You're talking about a giant rocket that can take people, giant payloads, faster, farther. That's pretty much the whole summary of the SLS, right? Paul Bookout: Yes. Definitely. Host: So, what's, what does it take to be human rated? So, I guess the difference between something that's not a rocket and something that is. Paul Bookout: Of course, it goes through the whole development process, starts at the beginning. You have to have safety emission assurances involved from the very beginning. Just an overview, you have to have, like redundant systems. If something goes wrong with one system, there's another system to kick in to back up to still make the vehicle safe. There's safety reviews throughout the whole process. We do additional testing, a lot more testing than other commercial launch vehicles do just to make sure that the vehicle is safe for humans. Host: That's really the main thing, right? Paul Bookout: Yeah. [00:06:33] Host: The safety. But, then, also the redundancy because I guess redundancy is cost. Redundancy is weight. So, you have to factor that into a rocket where you can just say, "Oh, if it fails, you know, with the primary systems, it fails." But, at least the only thing we lose is this piece of hardware. And, not to say that that's not a bad thing, but. Paul Bookout: Right. Host: It's very different from human life. So, I guess, absolutely, you need to be considerate of that. Paul Bookout: Right. And, there is a tradeoff, as you was saying. Additional systems, more mass, and that's mass that is being taken away from your primary payloads. Host: Yeah. Paul Bookout: And lift capability, but we need that to be safe. Host: You know what? I actually always wanted to ask this question, but you said primary payloads. I get this question all the time from folks not in NASA, and it's just, we use this term all the time, but what, to you, is a payload? [00:07:22] Paul Bookout: A payload is anything that goes up on top of the rocket that's lifted into space. It can be a satellite. I can be probes. Of course, the Orion spacecraft, once it's on the rocket, it can have its own second co-manifested payload along with it. So, just anything, really, that's launched into space. Host: Does a person count as a payload. Paul Bookout: We don't like to refer to. [ Laughter ] Host: It doesn't humanize it as much, right? Paul Bookout: No, it doesn't. No. Host: So, I guess, for example, going back to that co-manifest thing, the Orion. The Orion would be the payload. That would be the primary thing that you want to bring into orbit. Paul Bookout: Correct. Host: But, then, there's something that is, something called co-manifested which means it's not the primary thing, but it's also part of the part that you want to lift the mission. Paul Bookout: Correct. Host: Okay. Paul Bookout: For example, on the second generation of the SLS rocket, it will have capability of launching a co-manifest payload along with Orion, and it could be anywhere from additional probe going out into the moon, or it can be call separation bus, propulsion system that's launched. And, then, when a habitat is launched, then they can be combined and go to the moon. So, it's, allows us to build capabilities out in space, too, with co-manifested payloads. Host: Okay. Paul Bookout: Along with Orion. Host: Is that one of the things you're working on? Or, you're working on, I guess, secondary payload? Paul Bookout: Yes. I'm mainly focused in on secondary payloads. Host: So, what's secondary payloads? Paul Bookout: Okay. Secondary payloads, or they call auxiliary payloads. Host: Okay. Paul Bookout: They're payloads that do not drive the primary mission of the, of that launch. For example, on EM-1, we have secondary payloads on that. That's EM-1, Exploration Mission-1. Host: Okay. Paul Bookout: First launch of SLS rocket. David Smith: Yeah. Paul Bookout: We have 13 payloads on that, and I'll talk a little bit more about that later. But, the primary requirements they have is for secondary payloads in general is do no harm to the vehicle and minimal impact. So, the do no harm aspect is that we have to fly safe. The whole system, deployment system and everything, is designed to be safe. Like, all the CubeSats are turned off during launch. They have to have, like, redundant systems, as in two separation switches that allow them to turn on. Because, if one fails while we're being launched, it could turn on the systems. So, we have two there. Host: Oh, okay. Paul Bookout: To back that up, to keep it safe. And then, minimal requirements, of course, if the rocket is ready to launch and the secondary payload's not ready yet, it's going to launch. Because it does not affect the primary mission of the payload, of the launch. Host: Right. Paul Bookout: Of that. Host: Well, that puts a lot of constraints on you, then, huh? Paul Bookout: Yes, yes it does. Host: Because, not only do you have to worry about these, and I guess we can kind of hone in on the CubeSats a little bit later. But, you have to worry about the CubeSats, but now you have to add something else to it. Now, you have to add these redundant systems. And then, there's no guarantee that if you're not ready, that's okay. We're going to go without you. Paul Bookout: Right. Exactly. SLS is, the first rocket's not going to be the only configuration of SLS. And, of course, SLS is Space Launch System. We, the first launch is going to be called Block 1. Then, we're going to be stepping up to Block 1B which means we're going to be adding a different upper stage. Right now, we're utilizing an existing Boeing ULA upper stage to use on this mission, mainly to save initial money so we can develop the core stage. And, once the core stage has been developed, then we can have additional funds to start developing the new upper stage or exploration upper stage. Host: Okay. Paul Bookout: Okay? And, that's going to be the Block 1B configuration. And, Block 1B will have actually two configurations. It'll be a crew which was, as we talked about before, the Orion spacecraft with a co-manifested payload. The other configuration will be the Block 1B cargo where that would be your primary payloads. So, the only payload will be that major payload. Host: Okay. So, when you say "Block", you're looking at the entire rocket configuration. Paul Bookout: Correct. Host: And, Block 1 is this configuration with the ULE booster, right? Paul Bookout: Right. Host: Okay. And then, Block 1B has the NASA booster on top. Paul Bookout: Correct. Host: Instead of the ULA, but then you can do crew or cargo on that one. Paul Bookout: Exactly. Host: Whereas, EM-1 you don't, and EM-1, we can get into this later, is, you're not going to have crew on it, right? That's not part of the test. That's for one of the later missions. Paul Bookout: Correct. Host: I see. So, really, the blocks are kind of the stages of developing the rocket into its full capability of. Paul Bookout: Right. Host: Of this eventual Mars lander. That's awesome. So, now, you're using these commercial elements. You're using ULA in Block 1 and the leftover solid rocket boosters until, eventually, 1B, 1B crew, you get to Block 2. Now, you have the configuration. New boosters. You got the NASA upper stage. You got all of these configurations, and now you can go to, where can you go? David Smith: Well. Host: Is it just to Mars? David Smith: Well, you really need Block 2, ultimately, to fulfill a human settlement on the lunar surface as well. Host: Really? David Smith: You need a kind of lift capability. But, if you want to assemble an architecture, because it'll take multiple flights of a Block 2 to assemble a human architecture capable of transiting to Mars, you'll need four to five Block 2 flights at a time to assemble that stack that can go to Mars. Host: So, what's, I guess, how much more power does Block 2 provide you that, I guess, Block 1B would not? David Smith: Well, it nominally, you're talking another 25 tons or so. So, it could bring a second Orion vehicle in comparison because Orion weighs about 25 tons. So, it, really, from a lift standpoint, is maybe a fifth more powerful than the Block 1B, and it gives you that extra diameter, potentially for the payload ferrying that would allow, you know, the smaller the diameter of the ferrying, the taller a lander needs to be. And, think about a lander on the surface of the moon or Mars, if it's three or four stories, that's a lot of vertical height an astronaut has to overcome every time they're taking stuff back and forth. Host: That's right. David Smith: So, we're, the larger the diameter, the shorter can be the squatter, can be the easier it is to manipulate items on and off a lander. Whether it's on the moon or Mars. Host: Okay. Wow. So, then, you're talking about once this Block 2 configuration is done with the new solid rocket boosters, you can actually have a wider payload go on top of the rocket. David Smith: Right. Well, there's a nuclear thermal propulsion that's out there that has the potential of getting people to Mars a lot sooner. It needs a much larger diameter because it used hydrogen as a fuel. Hydrogen is very bulky because it isn't very dense. And so, if we were ever to use a new kind of propulsion that would lower the time to get to Mars, you need a Block 2 vehicle. A smaller rocket will never allow you to do nuclear thermal propulsion. Host: Okay. Let's go back to some of these other configurations. I kind of want to get a sense of the look and feel of this rocket. We sort of talked about it, but to just sort of go into detail. If I was looking at let's just say the Block 1 configuration, the one that's actually going to go for EM-1, what does that look like? How tall is it? What's the weight of it? How much power? David Smith: Right. So, roughly Block 1 and 1B are somewhat similar. Host: Okay. David Smith: They're going to be about the same height as the Saturn V. Host: Oh. David Smith: Which means it's a big rocket, but part of that's because we can't really exceed the vehicle assembly building limitations that are at the Cape. So, you want to make it as big as you can, so you can put as much fuel in it as you can. Basically, the thrust of the Block 1 vehicle which is similar to the Block 1B for the solid rocket motors is about 3.6 million pounds each. Those only fly for about two minutes. Then, you have the core engines. There's four space shuttle era type SSMEs that each have about 512,000 pounds of thrust. You multiply that by four. They operate for about eight minutes. Together, you get about a total thrust of about 8.8 million pounds which gives you an escape velocity of over 22,000 miles an hour. The core stage itself is about 2/3 the length of a football field which is pretty tremendous. One single stage of this vehicle's about 2/3 of a football stadium. And, which is around 212 feet, and the Block 1B ferrying that we talked about, the 8.4-meter diameter ferrying, could accommodate up to three school buses inside its volume. So, that's pretty incredible when you think about the size of what can be lofted in a single vehicle like that. In comparison, the Block 1 vehicle, you know, can throw 70 tons to lower earth orbit where the shuttle can only do 28 tons to low earth orbit. So, it's about three times more powerful than the shuttle. Host: Wow. So, you're talking, you're comparing it to the Saturn V in terms of its size but talking about these efficient engines. What makes, what is it about the engines that's more efficient that's giving you this extra power? David Smith: Well, they, you know, the shuttle engines were rated at 100% thrust originally, and I think they got them up to 109%. So, they actually got them to work 9% more efficiently at the end of the shuttle program. We're taking these up to 11% more thrust, and maybe even 13% more thrust. So, you're really pushing these engines to their limit, and the, it's really coupling their efficiency now at 113% thrust with the reliability of the shuttle system. Host: Unbelievable. The engine itself is called an RS25, right? Paul Bookout: Yes. Host: That's what it's called. And, these are the engines that were on the shuttle. Now, you're pretty much just putting it on the SLS, but it sounds like there's a good reason for that. It's because you've flown the shuttle so many times, improved the capability of it past its, like, total 100% thrust ratio. Now, you're going, you're going past the 100%. So, basically, is like why would we, why would we do something else? We worked so hard on this one. This one is, like, extremely efficient. Why would we, and we can make it even more efficient. That's the logic behind it? Paul Bookout: Well, right. Initially, of course, we have about, I believe, 16 space shuttle main engines or these RS25s left over from the shuttle program. So, we're utilizing the existing hardware to save cost while we're developing the core stage. You know, the first part of the SLS. Host: Yeah. Paul Bookout: And, as you mentioned, we are updating the engines, getting more capability out of them. So, to that point, we can do four per, so we can do about four launches, four rocket, or four engines on each launch. So, we can do about four launches with the current RS25s. Host: Okay. And, that, is that for one of the later configurations? Paul Bookout: That's correct. Host: Okay. Paul Bookout: Yeah. Host: Is it the Block 2? Paul Bookout: The Block 2. Host: Block 2? Paul Bookout: Block 2 and beyond. Host: Oh, okay. I see. I see where the whole idea of staging this whole thing comes from, right? Paul Bookout: Correct. Host: You've got, you're using the leftover solid rocket boosters, and you're using this commercial upper stage. And, it's just basically getting to this point where you're going to maximize the efficiency of the rocket. Paul Bookout: Right. Host: Unbelievable. So, three school buses inside of the 1B configuration, right? That's, is it about the weight of three school buses? Is like taking three school buses to space? David Smith: No, it would be, it would be more than that. Host: More than that? David Smith: I mean, nominally, if you went to the moon, we're going to take, the Block 1B could take roughly 40 tons to lunar vicinity which is, which is pretty incredible. Host: Wow, and just in terms of not only, like, quantity, you're talking three school buses. But, also size. David Smith: Yeah, and mass. Host: Also weight. David Smith: Right. Host: You know, you got all of these, all these different components. So, I guess we can kind of focus in on now that we kind of understand the rocket and the evolution of the rocket, let's go to that first, that first test flight, EM-1. We've talked about EM-1 on the podcast before, especially from testing Orion and that. But, really haven't focused in on what is it about, what is it about EM-1 that we're testing SLS for? So, let's start with that. What are we going to test, and I guess we can kind of start with the overview of EM-1 for those who haven't listened to it before. Paul Bookout: Right. So, EM-1 is, of course, going to be the first launch of the SLS rocket. Its primary segments are, of course, solid rocket motors which are a heritage from shuttle hardware. Shuttle had four segments, where EM-1 is going to have five segment motors. Then, of course, the core stage which is heritage off the shuttle external tank but made longer for additional capability of fuel. And, we're also using the main engines from the shuttle program with updated technology and ratings to get more power out of those four rockets on there. So, that makes up the primary lift capability of the SLS rocket. On top of that, we have an interim cryogenic propulsion stage, which, or second stage, upper stage, that we're utilizing from Boeing, existing hardware for EM-1 mission. And then, of course, in addition to adaptors, then there will be the Orion spacecraft, which is the primary mission of EM-1 is to test out the SLS rocket. Then, also, to test out the Orion spacecraft with its trajectory and telemetries and communications. It's going to be on about a 25 1/2 day mission to distant retrograde orbit. That really means just go way past the moon and come back. Host: Yeah. Paul Bookout: You know, a 25 1/2 day trip. Of course, and, you know, we're doing all this because, again, for the safety aspects. We want to test the vehicle out and Orion spacecraft before we put humans in it. Host: Right. Paul Bookout: So, we want to make sure it's safe, make sure everything works. And, that's that safety aspect, that human rated part of a launch vehicle. Host: So, the human rated part is the Orion can go to 25.5 days, or is this going past what it's expected to possibly operate at? David Smith: I think that's a nominal timeframe for the Orion with crew. So, this is pretty much, I think, its extreme capability. Host: Yeah. David Smith: But, you know, part of it is testing just the systems period. You always, for human rating, you always want to test it far in, you know, far from what the humans will actually experience so that you have a safety factor that's sufficient for human use. Host: Oh, yeah. Because if you're going to be operating on, say, 16 day missions, you don't really want to, okay. Well, let's just test 16. Paul Bookout: Exactly. Host: You really want to go kind of further out and see, all right. Let's see how far this puppy can go. David Smith: And, I think part of this mission's objective is to bring it in at a lunar return velocity to test that heat shield. Host: Yeah. David Smith: You can't do it from low earth orbit. You got to kind of go out and bring it in fast, so. Host: So, what's the difference with EFT-1? That was one of the first test flights we did where we didn't go all the way out to the moon, but we did kind of a, this large apogee so that we can get up to, I think it was some, like 25,000 miles. Or, maybe it was a little slower than that. The difference is between EFT-1 and EM-1. David Smith: I think, I think it was very close to what they would experience in a lunar return, but it's not the actual lunar return. Host: I see. David Smith: Right, so you want to be able to stage it. You want to go out in orbit. You want to test the time that you're out in orbit. That was a very short mission, maybe five or six hours. Now, we're talking 25 days. Well, all the equipment still work when it's, you know, soaked in a cold temperature, hot temperature, all those days. And, now, you're coming in. Will it all work when it comes to the right moment. So, this really puts the pedal to the metal. Host: That's right. So, what is it? I guess the relationship between what are you guys looking at for SLS versus Orion on this particular mission, EM-1? Paul Bookout: So, for SLS, again, we want to test all the systems, make sure they're fully functional. We'll be checking out redundant systems indirectly, of course. And, communications with the vehicle, since it's the first time the vehicle's being launched. We're all, we're talking with the vehicle all the way up. Host: Yeah. Paul Bookout: So, we want to make sure all those ground systems are ready to support, actually, human flight mission. So, it's just not the vehicle. It's the overall architecture of everything that goes into supporting a launch that we want to verify and check out. Host: Oh, that's right. Now, we're preparing to go into fly deep space missions. So, not only is it, all right, let's test the hardware, but let's test to operational aspect. Paul Bookout: Exactly. Host: Let's test what it's going to take to actually do these missions from the broadest perspective possible. David Smith: And, that includes, even, just bringing the, you know, the pieces are being built all over the place. Host: Yeah. David Smith: And, tested all over the place. So, just bringing them together at the cape and making sure they can be integrated in a safe and timely fashion for launch. That, in itself, is a really important objective. We're talking about such a large rocket. Paul Bookout: Yeah, so this is the first time all those components going to be coming together, and there's going to be hiccups along the way. And, we just need to understand how this vehicle goes together and make sure we do it correctly. Host: So, you say the vehicle's going to be talking to you guys throughout its flight. What is it going to be telling you? What kinds of data are you really looking for that's really going to tell you that this thing is working how we're expecting it to work? David Smith: Well, remember, you're talking to payload guys, so, you know, we're more interested in seeing what the payload's going to experience. Host: Yeah. David Smith: But, think about this. When it launches on the pad, it has an incredible noise issue coming off that mobile launch platform. That's why, if you remember, they had these things called rainbirds, the big sprinklers that start spraying as soon as the engines go to try to mitigate that noise. Host: Right. David Smith: The payload is particularly sensitive to it. Obviously, the vehicle itself is sensitive to that noise as well. So, acoustic mitigation is one of the most important things at launch. Then, we have a thermal issue, right? We go up to max Q, max dynamic pressure. We have a certain heating that is, occurs on the outside of the vehicle. And, before, we got to get through all that heating before we can make sure that the crew is going to be safe, that we can take the shielding off the Orion and so forth. So, we're going to be testing all those environmental concerns as we go forward, and of course, the jettisoning of, you know, the SRBs off the core stage. Then, the ICPS in Orion off the core stage. And then, of course, then, the Orion off the ICPS. All these jettison events, and there's quite a few of them, are extremely important, and we need to test those. Each one has its associated thermal and acoustic issues. So, we're going to test each one of those as it goes forward. Paul Bookout: Since this is the first launch of SLS rocket, we don't really understand the full environments that it's going to be launched in. As David mentioned, the thermal, interior thermal, acoustic, vibration. It's the first time we're going to launch it. So, what we're also have is a lot of instrumentation on this vehicle to be able to measure the actual vibration levels and everything else. So, we can, once we go back to designing and looking at what we call safety factors, reducing those so we can have more margin on the vehicle and means that goes into more mass lift capabilities. So, we're trying to understand the overall characteristics of the vehicle itself. So, in addition, for secondary payload, or payloads in general, we can give them more of an accurate environment that they will see during launch. As in, how much vibration they'll feel, how much thermal environments that they'll see. So, when they start designing their payloads for, to run the ride on this vehicle, they can have more of an accurate environment. And, maybe not have, make it a lot more efficient design. Host: Okay. So, then, what data are you going off of now based on, you guess you haven't launched the SLS. So, what are you assuming, or where are you getting the data from? David Smith: We have, we started off with assuming, at least for the payloads, that we would provide an ELV, and expendable launch vehicle class environment. Host: Okay. David Smith: So, if you've flown on Atlas or Delta, you should expect nothing worse than that. Host: Okay. David Smith: That's our starting point. Host: Oh, okay. David Smith: Now, what Paul's going into is we're going to try to characterize is that really true? So, the first flight's important. Are we in? Are we out? What do we have to do? Is there more foam that you got to put in the payload section to mitigate the noise? That's what we're trying to figure out. But, we should be within an ELV class is what we're projecting right now. Host: Okay. So, then, I'm assuming you're going to have some actual science on board EM-1, right? Because you're testing, you're testing the structure of EM-1. You're testing the rocket. But then, you have this mission. Why not take advantage of it? Is there anything else going on the EM-1? Paul Bookout: Oh, definitely. Host: Okay, good. Paul Bookout: Yes. We have, we'll have 13 secondary payloads that we're going to be launching on EM-1. Host: Wow. Paul Bookout: That'll, that is located in the Orion stage adapter. That's the segment that connects the SLS rocket to the Orion spacecraft. So, it's a small ring about five feet high. About 18 or so feet in diameter. And, along the inner circumference of that is where we are mounting these 13 secondary payloads. Host: Oh, so I guess they have to be kind of small, right? That's not a lot of space compared to the, what's in the ferrying. Paul Bookout: Correct. So, on EM-1, we have 13 CubeSats. CubeSats are defined as a, we call a 1U, which is about ten by ten by ten-centimeter cube. Host: Okay. Paul Bookout: So, what we're having on EM-1 is allowing them to go up to what we call a 6U. So, it's a CubeSat that's about the, a little bit larger than the size of a shoebox, a large shoebox. Host: Okay. Paul Bookout: And, that's kind of the dimensions of these 6U CubeSats that we're having on EM-1. David Smith: Which is the most common CubeSat, really, today, right? Paul Bookout: Correct. Exactly. So, we have multiple missions that these payloads are going to be doing. So, we've got one destination is to the moon. We have Lunar Flashlight which is out of Jet Propulsion Laboratory, and their primary mission is to search for ice deposits and resources on the moon using a laser. Host: Ooh. Paul Bookout: Okay. And, the second one is Lunar IceCube which is Morehead State University up in Kentucky. And, they're going to also be searching for water of all forms and volatiles on the moon using infrared spectrometer. These are some big words that I can't even define, so. [ Laughter ] LunaH-Map is from Arizona State University, and they're going to be creating high fidelity map of near surface hydrogen in craters on the moon. Lunar IR is from Lockheed Martin in Colorado, and they're going to be performing advanced infrared imagery of lunar surface. We've got one that's going to the sun facility, and it's called CuSP. It's from Southwest Research Institute here in Texas, and it's going to be measuring particles and magnetic fields of space weather between us and the sun. We have one that's going around the Earth. It's called EQUULEUS. It's a Japanese payload, and we actually have three international payloads on this mission. And, I'll touch on those others. Host: Awesome. Paul Bookout: So, again, EQUULEUS is from JAXA. It's the University of Tokyo supporting that. I mean, it's imaging the Earth's plasma sphere for a better understanding of Earth radiation environment. And also, it's going to be initially on the far side of the moon and detecting any meteor crater flashes that may impact the far side of the moon. Host: Wow. Paul Bookout: So, they'll be out there for about two months or so and just hopefully they'll be able to catch something. Some of the other missions are BioSentinel. It's from Ames Research Center, and they're going to be using baker's yeast to see the effects of radiation on actual live items, you know, live yeast. And, then, ArgoMoon, which is the European Space Agency, is built in Italy. It's going to be observing the interim cryogenic propulsion stage. That's upper stage is going to be deployed. Look at that upper stage, and then it's going to go on some additional missions. And, it's going to look at the upper stage to see what kind of effects the environment has during liftoff on the upper stage. Because, until now, we, once the upper stage is launched, we usually don't get a chance to look the conditions of that. This will give us some feedback and see what the upper stage has went through, if there's any damage or anything. Host: It sounds like these CubeSats are all over the place. Paul Bookout: Yes. Yeah. I've got a couple more here. Host: Oh, really. Paul Bookout: I haven't got to my two favorite yet. So. Host: Oh, we're standing by. Paul Bookout: Okay. Centennial Challenge. That was a challenge that NASA set up called Cube Quest, and it's to help develop communications for these smaller CubeSats. There's two challenges. One was a lunar challenge to around the lunar surface and for longevity. And, the other one was a deep space mission which was a CubeSat, as it says, going out into deep space to see how far and long and what burst rates and clarity that you can have in your signals. So, there's total prizes for everything through all the development and final missions. It's up to $5 million. Host: Wow. Paul Bookout: So, that's a lot of money. Host: Yeah. Paul Bookout: Spread out over those. So, you did, you asked what my two favorite payloads are. Host: Oh, yeah. Paul Bookout: Let me tell you. One of them is NEA Scout. That's developed at Marshall Spaceflight Center. What's unique about that is NEA Scout means Near Earth Asteroid. So, they're going to be going to a near earth asteroid. But, the exciting thing about it is that they're going to be using solar cell to get there for their propulsion system. So, this is the first time a solar cell will be used to, for propulsion out into deep space. There have been other missions in low earth orbit to check out the technology and feasibility of solar cells, but this is the first time going out to deep space. And, for a CubeSat that's a little bit larger than a shoebox, it will be deploying the cell that will be 40 by 40 feet. Host: Whoa. Paul Bookout: So, that's huge. Host: Wait, and a little CubeSat. Paul Bookout: In a little CubeSat. Host: And, it deploys a 40 foot. Paul Bookout: Yes. Host: Oh, wow. Paul Bookout: Yeah, so that solar cell is very thin material. Host: Yeah. It must be to fold up into, like, this ten-centimeter cube thing. Paul Bookout: Exactly. Host: So, so, the solar. Paul Bookout: You said ten centimeters. 6U CubeSat is 10 by 20 by 30. Host: Oh, because this is 6U. Paul Bookout: 6U, correct. Host: Oh, okay. Okay. Okay. So, solar sails, though, this is, it basically unfurls this 40-foot sail, and is it the one where the high-power laser that pushes it? Paul Bookout: No. Paul Bookout: That's different. Paul Bookout: This is going to ride the solar winds. Paul Bookout: Ride the solar winds. Paul Bookout: Solar particles will be pushing it along. It'll do actually a fly by the near-earth asteroid as it comes up. It'll be taking images all the way around as it passes. Host: Okay. Wow. Paul Bookout: So, and my ultimate favorite one is. Host: Yeah, we didn't get the last one. Paul Bookout: Is actually the one that I'm the Secondary Payload Integration Manager for. Host: Oh. Paul Bookout: So, it's one of my CubeSats. Host: So, it's an unbiased favorite, then. Paul Bookout: Yes. Host: Okay. Paul Bookout: Yeah, still. It's called OMOTENASHI. It's another Japanese CubeSat. Host: Okay. Paul Bookout: And, their mission is to land on the moon. Host: Oh. Paul Bookout: Can you imagine a small little CubeSat, you know, a little bit larger than a shoebox, land on the moon? Of course, and the big thing about it is that they're going to be using a solid rocket motor to slow down to be able to land on the moon. So, that's one of the things on EM-1 that we're offering that previous commercial launch vehicles and that don't offer propulsion systems for secondary payload to be able to utilize that. That's one thing EM-1 and SLS is allowing. So, that's a huge deal. Host: Yeah. Paul Bookout: For those. So, if OMOTENASHI is successful at landing on the moon, they'll be the fourth nation in the world to have actually land and do some science on the moon. Host: Wow. Paul Bookout: You know. Host: So, what kind of science? Paul Bookout: Well, because, again, they're still a small payload, so they can't get large science instruments to the moon, when they land, actually land on the moon, all that will be left is about the size of a sandwich box. Because they have to get rid of all the extra weight to be able to slow down enough to be able to land. And, they'll probably so some soil impact measurements, as in how soft vibration, shock, as it's landing on the moon. And, I, so, and they're only going to be able to do it for about 30 minutes or so. Again, because of the size, what we're limiting them to. Host: Yeah. Paul Bookout: They can't get the mechanics, orbital mechanics and velocities and everything. I'm sorry. Host: So, it's, it's kind of general on where you can land, then? It's just like, it's just going to land. It's not going to land in a targeted spot, I guess? Paul Bookout: Correct. They know the general vicinity where it's going to land. Host: Okay. Paul Bookout: But, they can't have ultimate control, like any of the other landers that have larger systems, propulsion systems, to slow them down. So, they would be actually, once the solar motor fires, they'll still be traveling at about 60 miles an hour when they impact the moon. So, they're going to inflate these impact balloons to actually bounce, similar to what they've done on Mars, some of the Mars Rovers. Host: Okay. Paul Bookout: So, it'll come and impact moon and bounce and then finally rest on the moon. Host: Okay. Paul Bookout: And, do about 30 minutes of impact soil measurements. Host: Wow. How would that be, though? I'm imagining, I mean, landing at 60 miles an hour. That's, you know. Paul Bookout: Well. Host: That's not slow, but at the same time, it's the moon, right? It's. Paul Bookout: Right. Yes, but then again, you're not going directly into it. You know, you're coming in at an angle, too. Host: At an angle. Paul Bookout: So, it's not a fully impact. Host: Okay. Great. Paul Bookout: Direct impact, so. Host: So, you got all these CubeSats going around the Earth, around the upper stage, around the moon, on the moon, to deep space. Where do you deploy, how does that work? Where do you deploy everything? It's not just like you just let everything go at all. It has to be pretty controlled because each one has a very specific mission. Paul Bookout: Right. We've created what we call bus stops. Host: Oh. Paul Bookout: They're basically different aspects of the trajectory of the upper stage. So, the first bus stop is when you're in between the two radiation belts or Van Allen belts. Bus stop two is when you've passed all the radiation belts. Bus stop three is half way between the Earth and the moon. Bus stop four is the closest proximity to the moon, and bus stop five is when you're going into a heliosynchronous or sun orbit. And, that's where the upper stage will be disposed into the sun orbit. So, when a payload says, "Hey, I want to get off at 200,000 miles away from the Earth." Well, okay, where is that exactly? So, that's why we kind of created these bus stops. Host: I see. Paul Bookout: They can get off anywhere they want to, but it helps us relate to the areas where they want off. So, most of them are wanting off at stop one. About seven or eight of them. Because they need to get out and start changing their trajectory as soon as possible. Again, we're offering propulsion systems, but they're not large enough to have really change their directions further on. So, a little change at first makes a big change later. Host: Yeah. Paul Bookout: So, they want to get off to be able to do that, make those little changes. Most of the payloads that are going to lunar orbit, what they're wanting to do is slow down because the ICPS, you know, is launching Orion into this distant retrograde orbit. And, you know, way past the moon. Host: Yeah. Paul Bookout: So, it has a lot of velocity heading that way, and if the payloads don't slow down, they'll just go flying past the moon. The moon can't, doesn't have enough gravity to pull them back into an orbit. And, some of them, even though they are going to the moon, they'll actually fly past the moon, and it may take a month or so for them to come back, to slow down enough to come back and get hooked into the moon's gravity and start orbiting the moon. Host: Oh, wow. Paul Bookout: So, it's not a direct flight into the moon orbit, just because they don't have the propulsion systems large enough to be able to do that. Host: So, is it fair to say they're all going to be in a very similar orbit, or are they all going to kind of go their respective directions? Paul Bookout: They're going to do their respective ways. Host: Okay. Paul Bookout: Some of them wants to do in the crater, so they're going to be going to the pole system, up to the poles to look see if there's ice up in there. And, some of them will just be doing a regular geosynchronous type of orbit. Host: Okay. Paul Bookout: Type thing. Host: All right. Paul Bookout: We talked about where these, what the payloads are and where they're going to want to get off. To be able to allow them to get off, again, we have to have a deployment system where, again, some of the primary requirements for EM-1 was or SLS is to do no harm and to have minimal impact to the vehicle. Host: Yes. Paul Bookout: Well, to do that latter one, what we've come up with a system is that we will receive an energy, the avionics unit for deploying the secondary payloads will receive an energy pulse for, from Orion. Or, I'm sorry. Will receive an energy pulse from the upper stage once Orion has already left and the upper stage has gone through its disposal maneuvers. That means burning off extra fuel and everything making it safe. Right before it shuts down, it will turn on the avionics unit for deploying the secondary payloads. Then, the upper stage turns off. So, we wake up, and we've got our own internal battery system. And, each payload is inside of a dispenser, and so, the dispenser operates as the, has a spring-loaded lid. And, the payloads inside are installed by compressing the spring. So, when the, when it's time for that particular payload to be deployed, we get an energy pulse from the avionics unit sent to the dispenser to open the door. The door flings open, and then the secondary payload is pushed out by springs. So, that's how they're deployed. Host: Okay. So, like a, so, like an SLS jack in the box. [laughter] Paul Bookout: If you will. Host: That's what I'm imagining. Obviously, it's going to shoot out. Paul Bookout: We have pulled those analogies before, but I'll let you state it. Host: And then, I guess there's, you get this power pulse that's going to, I guess, be directed to whatever seven is going to be part of bus stop one, and whatever the next ones for bus stop two. Paul Bookout: Correct. Host: Okay. Paul Bookout: And, they'll be deployed, if there's multiple at a particular bus stop, they'll be deployed a minute or two away from each other, after each other because we don't want to be able to deploy one and then deploy another one right behind it. Host: Yeah. Paul Bookout: And then, they have recontact. Host: So, I'm trying to imagine the way everything is situated in my head, and at this part of the flight when you're starting to deploy these secondary payloads, what does, what does the rocket, I guess, or what does the piece that's actually flying, what does it look like? I guess you have Orion and then there's this deployment system, and then there's, is it the upper stage behind it? Paul Bookout: Okay. So, once we've launched. Host: Yeah. Paul Bookout: After about two minutes, the solar rocket motors are. David Smith: Jettisoned. Paul Bookout: Jettisoned. And then, the core stage lifts the rest of the vehicle up into orbit. And, after that time, when the core stage is spent, then it'll be jettisoned. And then, you'll have your upper stage and your Orion spacecraft which of course the secondary payloads are still in part of that. And then, then, it'll go into what they call a translunar injection that's basically the upper stage will ignite and put Orion into its mission profile going past the moon. Host: So, at this point, right before it ignites, it's still in, I guess, Earth orbit, and the translunar injection gets it to the moon. Paul Bookout: Correct. Host: Okay. Paul Bookout: Okay. So, once the upper stage has spent its fuel, the Orion spacecraft will separate, okay? From the upper stage. So, it'll go through on to its mission. And then, about 30 minutes later, 20, 30 minutes later, the secondary payloads will start their deployment. Host: I see. Okay. Paul Bookout: So, Orion is well away and actually speeding faster away from the upper stage. Host: Yeah. Paul Bookout: The upper stage, once it goes through its disposal maneuver, is actually flying kind of, you would say, backwards, engine first, towards the moon. Host: Oh. Paul Bookout: So, the secondary payloads will be ejected out the other direction. So. Host: Okay. So, so. Paul Bookout: So, when they're deployed, the ICPS won't run back into them. Host: That's right. Paul Bookout: Okay. So, they'll be deployed in the other direction. Host: But, now, Orion is going in, it's doing its own thing. Paul Bookout: Correct. Host: Because it did its job. It delivered Orion. That's the primary payload. Now, it's off. But, the secondary payloads are still part of this upper stage. They haven't gone with Orion. They're totally separate. Paul Bookout: Correct. They have their own. Host: So, it's like, they're kind of doing, they're going. Paul Bookout: Yeah. Host: Different ways. Interesting. Paul Bookout: Yeah, they have their own mission profiles going in all different directions. Host: Okay. Okay. I don't know why that wasn't clear to me before but thank you. All right. So, I guess kind of backing up from there, you're talking about the solid rocket boosters are disposed. The core stage is disposed. Where are all these pieces going? Paul Bookout: Okay. Depending on their mission profile, all the secondary payloads are going to end of missions at different places. Some of them will be actually crashing into the moon, and that's common where the other countries and their lunar missions depositing on the moon. Some will, one or two will burn up in Earth's atmosphere as it comes back. Some of the other ones that are going out into deep space, of course, just keep going. The CuSP, which is going to solar. I'm sorry. CuSP, which is going to the sun's vicinity will just stay out there and eventually be pulled into the sun. Host: Okay. Host: So, that's all the secondary payloads. Paul Bookout: Correct. And, for each mission, each payload that's launched on U.S. rockets, they all have to have an end of mission plan. What are they going to do to end their mission, not just to be left out there as space junk. Because that's, we're having, sorry. We're starting to have a lot of problems with, as you know, there's a lot of space junk around Earth. Host: Oh, yeah. Paul Bookout: And, you don't want that same situation around other planets, too. Host: That's fair. That's fair. And, that's why, that's part of the, I mean, this is going back, but Cassini, right? That was the whole. It did its thing, and instead of just letting it be. It had a controlled entry into Saturn so that it didn't contaminate any other. Paul Bookout: Exactly. Yes. Host: Any other bodies. Yes, yes, of course. Paul Bookout: And, it doesn't matter what size you are. Host: Yeah. Paul Bookout: Even these small CubeSats have to have an end of mission. Host: Have to have an end of mission. Paul Bookout: Yes. Host: Awesome. But, I did want to go back to some of the earlier parts of the mission, right after launch. You know, you're talking about solid rocket boosters separating being. David Smith: Those go into the ocean. Host: Ocean? Okay. David Smith: Still, but they're not recovered this time. Host: Oh, okay. David Smith: You know, for shuttle, they were recovered. This time, it's too difficult. They're too large. So, they're just going to sink. Host: Okay. [00:48:19] David Smith: The external tank is, it can't go into orbit, so it's kind of lofted in such a way that it'll break up over the Indian Ocean safely. Host: Ah. David Smith: So, it's a very large tank. You know, this is much larger than the external tank of shuttle, so it's very important that it break up safely. So, that's, that's why you need the upper stage to actually bring the payload up into a circular orbit around the Earth. Otherwise, the payload would go down with the core module as well. Host: Okay. Okay. And, what about the, I guess, the upper stage. You said it's going to be doing this deployment, but then, after it deploys [inaudible]. David Smith: It's heliocentric. It goes into a sun, heliocentric disposal. Host: Sun heliocentric disposal. David Smith: So, it kind of goes away, and we should, hopefully, not see it again. Host: Okay. All right. That's a very nice summary of EM-1, and I feel like there's so much more to talk about. I kind of wanted to get into, you know, where are we now with SLS, all the history of it. So, I think we should take a break and just sort of let this one be Episode 41. We'll come back, and we'll do Episode 42 and just sort of get into the process behind building the SLS and then the journeys of where it's going to go and beyond. So, guys, thank you so much for coming on. We'll take a break. I'll see you in a few minutes. And, for everyone else, I guess we'll see you for the next episode. David Smith: All right. David Smith: Great, thank you. Look forward to it. Paul Bookout: Thank you. [ Music ] Houston, go ahead. [ Inaudible Comment ] [inaudible] for all mankind. Not because they are easy, but because they are hard. Welcome to space [echo]. Host: Hey, thanks for sticking around. So, the best places to follow development and delivery of the rocket as we test the major components and deliver it piece by piece to the Kennedy Space Center are on the social media channels on the web for the Space Launch System. So, first the website. You can go to www.nasa.gov/ guess what? SLS. That's where you can get the latest, the greatest on the Space Launch System. On Twitter, it's @nasa underscore SLS. On Facebook, it's NASASLS, that's one word. Or, this is one of the things that actually David Smith wrote. You can actually search SLS Mission Planner's Guide. And, it's a document that you can find on the web. You can download it, and it actually has a lot of great information on just the whole scope of the Space Launch System. We're really looking forward to the first launch of SLS and Orion from the Kennedy in a couple years. Sounds like we're well on our way to the pad, and we'll be launching astronauts back to the moon in just a few short years. If you have questions on SLS and its development, use the hashtag asknasa on your favorite platform. Just go to the Johnson accounts. Those are the ones we look at. The NASA Johnson Space Center accounts on Facebook, Twitter, and Instagram. You can send an idea or a question, and we'll make sure to mention it's for, or just make sure to mention it's for Houston, We Have a Podcast, and we'll bring it up in a later episode. Or, maybe address it in an entire episode. The whole episode will be dedicated to the question. Who knows? So, this podcast was recorded on March 20, 2018. Thanks to Alex Perryman, Rachel Craft, Laura Reshawn [assumed spelling], Kelly Humphries, Pat Ryan, Tyler Martin, Bev Perry, and all the folks at the Marshall Spaceflight Center for coming on to help to put this together. Thanks again to Dr. Paul Bookout and Mr. David Smith for coming on the show. We'll be back next week with part two.

Houston, We Have a Podcast. Ep42 The Space Launch System Part.2(2)

NASA Image and Video Library

2018-04-27

Production Transcript for Ep42 The Space Launch System Part.2.mp3 Gary Jordan (Host): Houston, we have a podcast. Welcome to the official podcast of the NASA Johnson Space Center, Episode 42: The Space Launch System, Part 2. I'm Gary Jordan, and I'll be your host today. So in this podcast, we bring in the experts -- NASA scientists, engineers, and astronauts -- all to let you know the coolest information about what's going on right here at NASA. So today, we're talking about the most powerful rocket since the Saturn V moon rocket, NASA's Space Launch System. We've got two guests from the Marshall Space Flight Center in Huntsville, Alabama here with us today to tell us about the rocket, the payloads it can carry, and where it will go. Spoiler alert: It will bring people, big stuff, and little stuff all farther than we've ever gone before. See, I did it again. You had a second chance for Part 2, and you blew it, Gary. If you're slightly confused, it's because this is Part 2 of our two-part episode on NASA's Space Launch System. There's still some good stuff in here, but if you want the full story, just go back and listen to Part 1. So continuing our conversation with us today are David Smith and Paul Bookout. David is the Vice President for Advanced Programs and Victory Solutions in Huntsville, Alabama. He has a long career in aerospace engineering and is a subject matter expert on rocket architecture and how payloads will fit into the rocket. He wrote the SLS Mission Planner's Guide, which gives payload developers a general idea of the capabilities of the rocket and some technical specifications so they can determine how their payloads might fit inside. He looks after the big payloads. Our other guest today is Dr. Paul Bookout, EM1 Secondary Payloads Integration Manager, who manages the integration of five CubeSats in the giant rocket as well the avionics that will control the deployment of all 13 small satellite payloads on the first mission of SLS and Orion called Exploration Mission 1, EM1. He spends his time managing the little payloads, not much bigger than a shoebox, on a skyscraper-sized rocket. So we're going to talk about just how powerful this monster rocket is, its unique capabilities, what it'll be used for, where it is in its development, its first mission with the Orion crew vehicle, and then look ahead to the future to the Moon, to Mars, and throughout the solar system. In this particular episode, we talk a lot about propulsion on this rocket, especially comparing solid and liquid fuel for the rockets. So at a very high level, the key differences are cost and control. Solid rocket fuel systems are generally simpler in design, cost effective, and they produce a large amount of thrust. But once the fuel is ignited, you can't really turn it off. Liquid fuel systems provide more flexibility. You can regulate the thrust through system throttle settings, but liquid fuel systems can be more costly. Very smart engineers have assessed the best way to use these two fuels and, for the SLS, they've come up with a combined design of solid and liquid fuel system. Solid fuel boosters and liquid fuel, the main engines to work in tandem to get you off the ground and moving fat, and then liquid fuel carries, or the liquid fuel engines will carry you where you need to go. So we're go for launch with Mr. David Smith and Dr. Paul Bookout for the Space Launch System program, T minus 5, 4, 3, 2, 1, 0, and liftoff of Episode 42 of Houston We Have a Podcast. Boom, nailed it. [ Music ] Okay. Paul and David, thanks for sticking around. This is going to be Part 2. We're sort of continuing our conversation, and we were talking a little bit during this I guess intermission, but one of the main things that we forgot to touch on was it takes eight minutes to do the first part of this launch. That's the solid rocket boosters and the core stage-- David Smith: Ignition to disposal of those stages. Host: Yes. Yeah, but I guess up to this point, all you need is some sort of injection burn, and you can pretty much go anywhere in the solar system. Is that right? David Smith: That's right. >> So it just depend, you just define what kind of injection burn, and you can go anywhere. David Smith: Well, it's the injection burn, and then the characteristic energy, which is the acceleration to get to that location. You know, it's a curve, so-- Host: Yeah. David Smith: If you go farther out, the less mass you can bring with that injection burn. So it is, it's the timing of the injection burn and the trajectory. But also, the farther away you go in the solar system, obviously, the less mass you can carry. So that's all kind of combined together. Host: That's right. And so for EM1, the injection burn is going to be translunar, right? David Smith: Correct. Host: But you can also do Mars injection burn, or Jupiter injection burn, or, like, anything after this eight minutes, it's just, you can just define it? David Smith: That's right. Yep. Host: So that's really the main thing about this vehicle is after eight minutes, you're ready to go wherever you want, and the fact that it's human rated, and the fact that you can bring really large payloads, right. I guess that, we'll start off with that. So we're building this rocket to pretty much go anywhere, but what are the sorts of missions we're looking at for the future for SLS? David Smith: Yeah, the first missions that are being considered are translunar and perhaps making something that has a, kind of a complicated acronym, LOP-G, Lunar Orbiting Platform/Gateway. What it really is is like a service plaza on a toll road. So think of Saturn V as the rocket that went out and surveyed everything and, you know, there were no roads, and it kind of established these, you know, these paths to go to the Moon, okay. Now, SLS is going to take that survey information and hopefully make this Lunar Orbiting Platform into a service plaza where, what do you get there? Well, you get a safe place for the crew. You can refuel landers that can go to the Moon. You can have a navigational way station. You can have a communication way station. You have a place for internationals to come by and make sure they got everything together before they go to the Moon. This gateway, in fact, gives you universal, total access to any spot on the lunar surface. Apollo is just equatorial. This station will give you access to any place on the Moon. So it has a lot of really great attributes, but it's a different kind of thing. Unlike the Space Station, which is purely science, this Lunar Orbiting Platform is probably going to be a lot more utilitarian and allow a lot more understanding and exploitation of the Moon and the lunar surface, which is, in fact, what we need that experience so that we can actually do the same thing for Mars. So it's three days away versus nine months away with Mars. So that, that's our first stage. It seems in the 2020's, we're going to be putting that together one piece at a time. So the first piece might be an EM2 mission that delivers a solar electric propulsion system that essentially is the way that this station keeps in its place. So it's just a little bit of impulse in this halo orbit around the Moon. You can stay there with very little power using a xenon solar electric propulsion system. The second part might be a habitation module. This isn't where the crew are going to, they're not going to live here full time. Again, it's a way station, so it's a place they can hang out, refresh themselves, get food, change clothing, who knows on their way to the Moon. Then, they're going to have an air lock that allows them to do servicing on perhaps landers and other kind of equipment that comes into that gateway. And then, also, a place for logistics modules to come to resupply this service plaza so that, for the long term, it can service people going to and from the Moon. So that's probably the first part, and that looks like that would be something that would be in the early 2020's, and that's where the current administration seems to be focusing us is on doing lunar first to be prepared for Mars later. Host: Okay. It's kind of like a small truck stop. David Smith: It is. David Smith: It is-- David Smith: Think of it as, yeah. [laughs] Yeah. And it should be kind of looked at that way as it's a way station to greater and better things, either the Moon or Mars. Host: Yeah. That's right. You can shower. You can, [laughs] you can service it. It's got a-- David Smith: Get your eggs and steak. Host: Yeah. David Smith: You know, get your car repaired. Refuel. Get some gas. Tow truck is even there to maybe save you if you have a probably on the Moon. So really, it's a good deal. It's kind of like a lighthouse and service plaza all put into one. Host: But not only will the SLS get us there. It's actually going to get the LOP-G there, right? It'll actually-- David Smith: It'll assemble it. David Smith: It'll assemble it. Host: In pieces. Now-- David Smith: Yeah. David Smith: If we were to do it the best way, instead of doing it in smaller pieces -- and by the way, it's going to do this just using the trunk section underneath the Orion. So the co-manifested payload is what these little elements of the station are going to be. If we were, if we could, it'd be best to just make one giant chunk and put in the, into a fairing, but the way I think the program is unfolding, to use crew to start with, is to bring the station in pieces that the crew can assemble at that location. Host: So going back to the previous episode, Episode 41 -- if you haven't listened to it, go back -- and that was the first part of our conversation, but going back to this co-manifested payload, we're talking about primary payloads, co manifested, secondary. What's the co manifested? David Smith: Yeah, the co manifested, again, is the ten-ton capability that is the trunk space underneath Orion that's going to fly on the Block 1B SLS. So in contrast, if you took off the Orion and its trunk space and put a large fairing on top, you get a primary payload that could be 40 tons the Moon. So it's ten tons the Moon is co manifested, or it's maybe 40 tons the Moon as a primary payload. And the secondary payloads are payloads of opportunity. They kind of fit in little, tiny spaces that are left over. They aren't filled up with other kinds of stuff. Host: And that's where Paul comes in-- Paul Bookout: Yes. Host: Right? [laughter] Paul Bookout: That's my world. Host: That's right. David Smith: So after Lunar Orbiting Platform-Gateway, one of the early missions that's been envisioned is taking a probe to the Europa, the moon, icy moon of Jupiter. What's so neat about this mission is that SLS, is we have to loft this payload and get it to Jupiter in two-and-a-half years, where a current ELV -- Atlas, Delta, even a Falcon 9 Heavy -- couldn't do that in more than seven years. So we're going to cut five years off a trip. Now, what does that mean? Well, one, it means that you're getting quicker returns to the science community. You're helping people not spend their whole career on one science mission. You have younger people come in, work on a mission, do it quicker. And if it costs $100 million a year to maintain a cadre of ground controllers watching this thing, think of the money that you're saving over time if you can eliminate five years of that mission. Plus, the risk of that hardware traveling through space. So this is a real enabler for Europa. In fact, SLS is the only vehicle that can bring it there in that kind of time. Host: Unbelievable. Is it a bigger payload because it's a, it's SLS, or is it just-- David Smith: Well-- Host: It gets it there faster? David Smith: In this case, Atlas could fly the same mass of payload, which is very large, by the way, but it would take over seven years. Host: I see. David Smith: So it had to take a whole bunch of gravity assists around the Earth and Venus to get it there where SLS can send it there directly. Now, to your point is the New Horizons mission, which was the mission to Pluto, I think it was 120-kilogram payload that was finally delivered there after like ten years. In that case, SLS couldn't get you there any faster, but it could double the payload to over 250 kilograms of delivered payload to Pluto. So it just depends on the trajectory and the position of the planets when you do this, on what value you have, but the fact you can do it quick is a unique attribute that only SLS can bring right now. Host: [laughs] Unbelievable what this rocket is capable of. And I kind of wanted to go back and kind of visit the rocket itself, where, the history of it. Where did we start with some, building some of these pieces, and kind of where are we now? So if we can just sort of start at the beginning, whenever SLS was proposed, and we're going to hammer in the first nail, I guess. It's a little bit more complicated than that, but where did this all begin? Paul Bookout: Yes. Of course, the primary design was based off of the shuttle heritage. You know, we're taking components that the shuttle used, the propulsion aspects of it -- the [inaudible] motors, the external tank, and the space shuttle main engines -- and utilizing, upgrading, making more powerful the, those components and assembling the core stage. So that's kind of where the history of where SLS is coming from. So we want to use that existing technology, again, upgrade it, make it better. Also, the manufacturing facilities that go into making these components are in existence, so we want to still utilize that, save money, save schedule to move forward with the SLS rocket. Host: Okay, and so it's kind of, that makes sense, right, because it's, you have, okay, this is a core stage that works. These are components of the shuttle that worked. Let's just sort of fit it and to meet these requirements of building a giant rocket that can take payloads anywhere in the solar system. Paul Bookout: Exactly. Host: And humans too. It's human rated, which is a huge component of this whole thing. Paul Bookout: Definitely. Host: So it's, where is it being built? Is it one location? Paul Bookout: No. Actually, overall, there's 44, over 44 states-- Host: Oh, wow. Paul Bookout: That different components are going to be, are being built in. So this is America's rocket. Host: Yeah. [laughs] Paul Bookout: So it's not just NASA's. It's being built all over. You know, there's more than 1000 contractors working on this, in addition, of course, into, in addition to NASA. The core stage, which is the prime or contractor is Boeing, they're building that in Michoud, which is outside of New Orleans. The engine prime is Aerojet Rocketdyne. They're being developed, or manufactured, or refurbished down at the Stennis Space Center. And then, when they're done, they'll be shipped to Michoud for integration with the core stage. And then, that core stage with the main engines would be sent back to Stennis for testing because Stennis is the primary testing facility for NASA-- Host: I see. Paul Bookout: For rockets. The boosters is the Orbital ATK. They're actually manufactured just north of Salt Lake City in Utah. And it's kind of ironic that the, it's very close to the Golden Spike, where the east and west railroads met when they were building the transcontinental railroad, was very close to that because the motor segments are used in the rail system to ship down to KSC from ATK, Orbital ATK out in Utah. Host: Oh, okay. All right. Paul Bookout: So-- Host: I like that. Paul Bookout: A little history there. [laughs] And the upper stage, of course, where, as Boeing ULA, which is a direct purchase from them for that. And that's being built in Decatur, Alabama. Host: Wow. All over the place is absolutely correct, so-- Paul Bookout: And again, those are just the primary elements. All the subsystems to that are spread out all over the United States. Host: So what is currently built, and then what's on the ticket to be built? David Smith: Well, right now, the core has been built three times so far. The weld confidence article to make sure that friction stir welding is appropriate because it's the world's tallest, biggest weld fixture-- Host: Oh, wow. David Smith: Down at Michoud, so we had to test that first. Then, they're building test articles. And then, the flight hardware. The test articles right now are up at Marshall, so there's this new barge -- actually, it's the same barge they used for shuttle Pegasus. They had to make it a lot longer, so they cut out the middle and put in a new middle section. And that just shipped up, the core section up to Marshall, where it's going under, undergoing static testing. The engine section's already been completed. The testing of that's been completed. And the intertank, the sections between the hydrogen and oxygen tank, has just arrived at Marshall Space Flight Center for testing. The hydrogen and the oxygen tanks will arrive later this year for testing at Marshall too, all for static testing, where they're put under a load to simulate their launch conditions. So this is the largest structural testing campaign since shuttle in the 1970's, and, you know, since this is probably a 50-year rocket, this is really laying the foundation for that kind of generational spacecraft capability that we're building for the Moon and beyond. The upper stage, the exploration upper stage, the NASA one is currently being worked on in design phase, but the ICPS that Paul talked about earlier, the interim cryogenic propulsion stage, is finished and down, already been tested and shipped down to KSC. The engines, the new engine controllers are hot fire tested at Stennis already, and I might even hear a sound of that in a minute. And the boosters, as we talked about, were built in Utah but had full, two full-scale static firing tests at the Orbital ATK facility so far. Core stage and booster avionics testing are undergoing at Marshall right now in specialized, in a specialized, integrated avionics test lab. So the testing is going forward. It's really quite a test campaign. Working on EM1 right at the moment, but, in parallel, getting ready for, I'm sorry, Block 1 to start with, and, in parallel, working on Block 1B for the EM2 mission maybe in 2022. Host: So I'm, I want to understand the full scope. That's, there's a lot of different elements, a lot of different parts of the testing. What are some of the main things that you really want to test? It sounds like structure is one of those things, and how do you do that? How do you test the structure? David Smith: There's a new static test facility at Marshall that's been developed where you essentially set them up vertically, and then you put a load down on the stage, and you do it in many different angles to make sure you can understand not only is it going straight in flight, but if starts experiencing some kind of skew because of the engines, so it undergoes quite a bit of testing that way. That's obviously, the structural modes are the most important. And when we talk about human spaceflight hardware, what that really means for structure is that you test it to a factor of 1.4. So it means there's a 40% margin on the capability of that structure, which is not something that expendable launch vehicles have to worry about. So our rockets are generally a little heavier, a little stiffer, a little more capable, but we do that to provide more margin for the crew in case of emergency. So that's the biggest part of that structural test that's going on right now at Marshall. Host: That goes back to your point, Paul, about one of the main parts of testing this and building SLS is the fact that it is human rated and you have these extra constraints for making sure that safety is and redundancy is one of the primary concerns of building this rocket. Paul Bookout: Exactly, yes. Host: Unbelievable. So the other part is the engines too. You're actually firing the engines. And it's a hot fire test. What's that? David Smith: Well, that's, the shuttle engines are going, they're installed into a test [inaudible] at Stennis. They're put through the same paces as if they were being launched in the vehicle. And remember, some of these engines haven't been test fired in eight years, seven, eight years. Host: Right. David Smith: So it's real important to make sure that they're still, still have the quality that we are looking for at the same time they have a new engine controller. So the controller, the computer that runs these engines have been upgraded from the shuttle days. So it's the first time those two have been mated together. So real important testing. We have I think up to 15 of those engines in inventory, so they're going to be going through those until they, at, probably in the mid-'20's, replacing with a new build of the shuttle engine. So right now, we're still going through the old engines with the new controllers installed. Host: Actually, we do have some audio from that that I really want to play. It's, this is the hot fire test at Stennis, so if you're listening right now, be prepared because it's going to be very loud. [ Engine Sounds ] Host: So that was the hot fire test, and what, you're looking at what components? Are you looking at temperature? Are you looking at propulsion, efficiency? What are the main things that you really want to get out of this test? David Smith: Well, I think the biggest one is, how's the turbo machinery going? You know, if you have turbine blades going at like 3000 rpm and you're spitting out all that fuel at the same time, how is that working out? Is it meeting all the parameters? Is, like you said, that's the temperature? How does it run through its life cycle for that eight-minute burn? That's a long time to run an engine. Host: Yeah. David Smith: So especially, you know, before we launch, you know, the shuttle only had three of these engines firing. Now, we're going to have four of them. So again, that's a unique configuration. So making sure, [inaudible] how these engines will play together will be an important part of the test as well. Host: Did you ever get to see any of these tests in person -- structural tests, hot fire tests, anything like that? David Smith: Yes. Host: Is it really, really loud? David Smith: Well, the Stennis tests, you can get really close to it-- Host: Oh, really? David Smith: Because, you know, it has the flume that comes out the side. And you can get close to a cyclone fence. In fact, you can taste the exhaust because, you know, oxygen and hydrogen comes together and forms water. Host: Right. David Smith: So that, and you have the sprinkler system that's cooling it down. So you get both the sound, right, you get the visual of the flames, and then you get the taste. [laughs] So I don't think you can do that anywhere else. You certainly can't get the taste at Kennedy, so Stennis is really a remarkable opportunity when they do those test fires there. Host: Does it -- I'm imagining like a hot shower or something, just like really-- David Smith: Well, remember, Stennis is pretty humid because it's in Mississippi, so-- Host: Oh, yeah. David Smith: It's going to feel like a hot shower, but, [laughs] yeah. Host: Okay, so I'm, a curious thing -- how does a hot fire test taste? David Smith: Yeah, it has a taste to it. Host: [laughs] So what about the flight hardware for EM1? Where are some of those components? Paul Bookout: Right now, the Orion stage adapter, that's where the 13 CubeSets are going to be housed during launch on EM1. Host: Oh, yeah. Paul Bookout: It's currently at Marshall Space Flight Center. And at the end of, beginning, I'm sorry, of April, it's planned to ship down on the Super Guppy, which is a large carrier aircraft, down to KSC for processing. And once it's down there when we're about six months to launch, that's when the secondary payloads will be integrated into that before stacked on the vehicle. The interim cryogenic propulsion stage, of course, is finished. It was, again, up in Decatur and is already down at KSC doing other final preps on that. The launch vehicle stage adapter, which is being developed at Marshall by Lockheed Martin, they, the primary structure is complete, and they're doing spray foam insulation on the vehicle right now. Again, that's also to help with acoustics aspects of the inside of that, inside of the LVSA. Host: Oh, that's right. Paul Bookout: The core stage, of course, the major components, as David said, the tank, the different tanks will be set up, sent up here for testing. And once they're done testing, they'll be sent back down to Michoud and assembled. And then, the main engines will come over from Stennis and assembled into the full core. That's the liquid oxygen, liquid hydrogen inner tank and the engines. Then, it'll be sent back over to Stennis. As David mentioned earlier, each engine, it would be separately tested, but then all four of these will be tested as, in flight configuration down there at Stennis. So we're running them through the full cycle of, as we're integrating. We're testing as we're putting it together. Host: That's right. Paul Bookout: So we understand that, as we assembled it, is it still operating the way we expected it to? Host: So then, will you, will it be built at Kennedy because that's when it's going to be launched? David Smith: Assembled. Host: I'm sorry, yeah. David Smith: It's built in Michoud, tested at Stennis, and then assembled at Kennedy. Host: Assembled at Kennedy. Paul Bookout: So the solid rocket motors, again, all the segment are, the five segments -- total of ten, five on each side -- have already been cast. They're in final prep for shipping down to KSC on the rail system. And then, just at, similar to shuttle program, once they've reached KSC, they'll be stacked in the VAB one segment at a time, and then the core stage will come in and be connected in the center between them. Then, you have your upper stage or the ICPS, where, I'm sorry, you'll have your LVSA, launch vehicle stage adapter. Then, you'll have your Orion -- let me just start over. Once the core has been installed, then you'll have the launch vehicle stage adapter installed. Then, you'll have your upper stage or the ICPS. And then, on top of that, you'll have the Orion stage adapter where the secondary payloads are. And then, Orion will come in and make, complete the stack. Host: All in this, in the Vertical Assembly Building? Paul Bookout: Yes. Yeah. Remember, it will built to assemble the Saturn V rocket, and-- Host: Yeah. Paul Bookout: We're about that same size, so [laughs] there's plenty of room in there. Host: That's right. It's, going back to that, actually, I don't think we've talked about it on the podcast. The Vertical Assembly Building is, as you can probably tell from the way that this is being assembled, it's gigantic. But it's so big, right, that it has its own weather system that you have to kind of worry about, right? Is that right? David Smith: Yeah, it's-- Paul Bookout: Yes. David Smith: Tall enough where, you know, everything that gets up in there can form its, it could rain a little bit sometimes-- Paul Bookout: Yes. Form clouds up there. David Smith: Yes. Host: Wow. And then, the, you have these giant doors that's going to open, and then you'll just sort of roll the rocket out. David Smith: But one big change is, if you recall, so it's really interesting. You know, a lot of that building was not changed from Saturn V. They only used two of the bays. There's four for shuttle. So they took out the platforms that were for Saturn and put in some shuttle platforms. But for Saturn, excuse me, for Block 1B, they had to do a lot more changes to that. So they had to replace all the platforms for that, and they actually removed a whole bunch of Saturn V, your equipment that had been left, abandoned in place. So it's, that building has really changed from what it was during the shuttle era. Host: So it's really been reconstructed to fit the SLS. That's really the main-- David Smith: Yes. Host: The thing that's going on right now in the VAB. Is it-- David Smith: Right. Host: Is it completed, or is it still going on? David Smith: The platforms are completed. Paul Bookout: Completed. David Smith: For [inaudible] 1, Block 1. Paul Bookout: For Block 1, okay. Host: Right. Paul Bookout: Yeah. And, you know, for SLS, there's still a lot of work at KSC being performed too. It's just not the launch vehicle and all of its hardware for EM1. It's KSC has to go through a redesign on a lot of their components. As David just said, the VAB and all the platforms to be able to reach the hardware where you're stacking SLS. Also, the crawler transporter that takes the mobile launch platform, which has the SLS rocket on -- originally, the Saturn V rocket -- has to be upgraded to fit the SLS rocket. So, in addition, out at the launch pad, they're redoing the flame trenches, re-bricking them because it's going to have a lot more powerful rockets since the S, you know, since the shuttle program. In addition, they're, they have to have a lot bigger water suspension system, you know, because at a lot more power than what shuttle was going through. David Smith: Called rainbirds after the sprinklers. Big rainbirds. Host: Rainbirds. David Smith: Yeah, they kind of go, click, click, click, click, click, on the lawn, but this time, they do it on the engines and stuff. Host: Oh. [laughs] Paul Bookout: So, you know, the water suspension, suppression system is to help with not just the heat but, also, the sound that these rockets, engines, and solid rocket motors, when they ignite, they're very loud. They send out a shock wave. And if you didn't have the water there to suppress or dilute that sound, that would just bounce back off the hard surface up into the vehicle and could damage the vehicle. So it's just not for flame. It's also to protect the vehicle from itself on the acoustics. Host: Okay. That's the, so that's the suppression system? Paul Bookout: Correct. The water that you usually see that starts a couple seconds right before ignition. Host: Actually, I think we do have some audio of that. I don't think this one's quite as loud as a hot fire test, but let's listen to that. This is what the suppression is going to sound like. [ Engine Sounds ] Host: And those are the, that's the clicks, right? That's the, I guess it's basically just like a giant-- David Smith: Sprinkler system. Host: Sprinkler system. Yeah, yeah, yeah. Paul Bookout: Yes. Host: Rocket-size sprinkler system. So you're going to take it from the VAB, and I wanted to get, circle back on that because I think I was calling it Vertical -- is it Vehicle Assembly? David Smith: Vehicle Assembly. Host: Vehicle? So I was getting that wrong. It's Vehicle Assembly Building. You bring it out to a launch pad, and is it going to launch on the same pad that the Saturn V was launching? David Smith: Yes. Host: Okay, so that's 39-- David Smith: In fact, I think -- well, I'm not sure if it's A or B-- Host: A or B. David Smith: But the one that we, that NASA kept, they totally revamped the equipment underneath that concrete mound. Host: Yeah. David Smith: And it's, there's a lot of [inaudible] and electrical equipment that's there in, the remnants from Saturn V, there's still a rubber room. If you know, that's where the, if someone was trapped at the pad, you'd have a safe place in there. So that's still in that same area, which they've now made a historic area, which is kind of interesting. But they, for the first time in 50 years, have to clean out all the old equipment, totally revamp that launch pad for SLS. So it's brand new and ready to go. It's really impressive. Host: So the, what's being suppressed over at this launch pad by that suppression system, is it, is the solid rocket boosters, right, and then are the engines firing at the same time? David Smith: Yes. David Smith: These RS-25-- Paul Bookout: Correct. Host: Engines? Paul Bookout: So-- Host: Everything's all at once? Paul Bookout: Right. Actually, the -- sorry. Actually, the main engines ignite first because we want to make sure all of those are operational and working at peak efficiency because once you start the solid rocket motors, you got to launch because you can't turn off solid rocket motors. So you want to make sure your other four engines are operating nominally, and then you ignite your solid rocket motors. Host: So we've done some testing with the, with these, the main engines, right? The RS-25's? Paul Bookout: Correct. Yes. Also, we have done full-scale testing of the solid rocket motors out there at Orbital ATK in Utah, where they actually constrain him, lay him on the ground sideways, and constrain him, and actually fire, do test fires out there at Utah. Host: Ooh, I've seen that. They actually had a HDR video I think of that -- high dynamic range or something. Paul Bookout: Yes. Host: Yeah, and it was super cool to see. But then, also, just the test itself, actually-- Paul Bookout: Yeah, I've been out there for a couple launches, and it's kind of unique because, with shuttle launch, you listen to the sound, and it's, you know, launching, so it's, after just a few seconds, it, the sound's gone. Where solid rocket motor is, it's operates for two minutes, so you're sitting there feeling that whole sound, you know, [laughs] for two minutes, and it's a really exciting experience to be out there. Host: How did it feel? Did it feel like you were at a loud concert, or even worse than that? Paul Bookout: Well, you're usually about a mile or so away. Host: A mile, okay. Paul Bookout: So, you know, just for safety reasons and everything. Host: That's, yeah. Paul Bookout: So you kind of get to see it off in the distance a little bit, but, yeah, you still feel it and hear it, yeah. And it's kind of unique because you see the smoke, the engines fire off, and the smoke coming out, and then, a couple seconds later, that's when you feel it. So-- Host: How about the RS-25's? Do you feel those too, or not as much? Were out at the RS-25 test? David Smith: Yeah, yeah. Well, the static firing, yeah, you feel it in your, you can get close for that, and you feel it in your stomach. I mean, it's very visceral, the shaking of your, of that sound, so, yeah, you won't forget it once you've had it. Host: That was the sound we played earlier, right? David Smith: Right. Host: Okay. I think the one we still have is the solid rocket booster, I think. Okay, let's play that one. This is the one that Paul was talking, the one out in Utah. >> T minus 10, 9, 8, 7, 6, 5, 4, 3, 2, 1, fire. [ Engine Sounds ] Host: Okay, so that was the test from out in Utah, and if you really, if you turned up the volume on your, on the podcast, you can really feel it. I listened to some of, I would listen to this in the car or hook it up to a nice speaker because you can really feel it there. So those, that's all of those -- the solid rocket boosters, the RS-25, and the suppression systems. So let's go back to the stages and sort of recap the, I guess the stages of all of these engines firing. What's that look like? David Smith: Right. So, you know, the term "stage" means that you have a single entity that provides an impulse for a period of time and then is thrown away. Host: Okay. David Smith: So in the olden days, so that would be Saturn, you know, you'd say Saturn was a three-stage vehicle, right. It had the first stage, the second stage, and then third stage was the injection stage that took, you know, Apollo and the land to the Moon. For both shuttle and for SLS, we really don't, can't call it three stages because these stages work together, which is kind of like they're two-and-a-half stages. So what that means is the core, and, as Paul said, the core starts a little bit earlier, but they're essentially the same time. The core and the booster, the solid rocket motors, boosters, excuse me, turn on at the same time. So they're ignited, and that's the one-and-a-half stage-- Host: Okay. David Smith: Because what happens? After two minutes, the boosters fall off and the core continues, so that's the half stage, in a sense, the boosters. Now, the core continues. And then, finally, the core is expended after eight minutes. It's disposed of in the ocean. And then, you have the upper stage -- in this case, the second of the one-and-a, two-and-a-half stages -- fires to get you to your destination. So you could still call it a three-stage system, but because some of the stages work together they're not really separate stages. So it gets a little confusing. So that's why you really don't hear, that's why people use the term "upper stage" these days and not "third stage" or "second stage" [laughs] because even the expendable vehicles have multiple solids on them, and so they have the same issues. So that's the difference in staging today. And it's more effective to do it this way as well. Host: It's more effective, I guess is it from the perspective of, oh, you can turn this off, you want to make sure everything's working? Is it I guess more reliable? That's why it's more effective? David Smith: Well, it's more effective because you use the power where you need it. At, you know, at sea level, you need the most thrust, so you combine everything together to get you out of the gravity well of Earth. So there's an efficiency with that system that, you know, is improved, is an improvement upon what was done for Saturn and other rockets before then? Host: Okay. So how about the, we're talking about different configurations too -- Block 1, Block 1B -- and how they're going to be different and just sort of evolve. Paul, I think you said you had some secondary payloads I think on 1B. Paul Bookout: Yes, that we're planning for. Host: That we're planning for, okay. Paul Bookout: So, you know, currently, on commercial launch vehicles, CubeSets usually don't have propulsion sets, and they're really going to low Earth orbit or geosynchronous orbit. Host: Yeah. Paul Bookout: And they're pretty much just deployed in those locations, so they don't need a secondary or propulsion system to get to where they need to. On EM1, this is the first opportunity for a secondary payload to be able to have propulsion systems and going to get access to deep space because we're giving them the initial thrust or velocity to get out going to the Moon or into deep space. They only need smaller propulsion system to change their trajectory or where they want to go. So it's, you know, this will be the game changer for secondary payloads. I mean, this is first-time opportunity for these small, little, shoe-size, shoebox-size payloads to be able to get out into deep space. Host: Yeah, and do some great stuff -- orbiting the Moon, land on the Moon. You got some-- Paul Bookout: Right. Host: Great stuff happening in some of these-- Paul Bookout: Right. Host: Secondary payloads. Paul Bookout: As I mentioned in Part 1, EM1's kind of discovering that, well, they really want to be a little bit bigger so they can have a little bit larger propulsion system. So instead of getting off at we call bus stop one right in the middle of the Van Allen belt, they'd like to get off at bus stop two or a little bit past so they don't have to worry about the radiation effects on their systems as much. But they can't do it because they don't have the propulsion system big enough to change their direction that they want to go. So on EM2, because it's a more powerful rocket, there's opportunity for additional mass allocations for secondary payloads. The mass allocation is the mass that's left over that the primary or co-manifested payload doesn't need the full capability of the rocket, so we can use that additional up mass for secondary payloads. So we're offering actually from a 6U- up to a 12U- and even a 27U-size secondary payload. That's huge for secondary payloads wanting to be able to get out into deep space. This allows them to have more power systems, more advanced telemetry, communications, and especially larger propulsion systems so they can get out into different destinations and do all this great science that they want to do in these smaller, less expensive packages. Host: Actually, that blends in nicely to drawing comparisons with SLS to other heavy-lift rockets because SLS is going to be gigantic and take these very, very large payloads. What's the difference between SLS capabilities and some other heavy lift rockets like Delta IV Heavy or Falcon Heavy? Why wouldn't you use just the heavy rockets? Why do you need SLS? Paul Bookout: Existing commercial rockets, they're not destinations going into deep space. They're mainly going into low Earth orbit or geosynchronous orbit. So for a secondary payload to get out into deep space, they'd have to be pretty big, you know, to have a propulsion system larger than a 27U. So the uniqueness of flying on SLS if you want to get out into deep space is that you don't have to have a huge satellite or, and propulsion system. SLS is providing that initial kick or velocity to get you out in the general direction you want to go. And then, you'd have a smaller propulsion system to be able to get out there. So overall, it's a lot less expensive. And again, SLS is giving these small CubeSets the opportunity to get onto deep space. Host: And also, the fact that it's human rated, right. The fact that you can actually put people on it and bring them far into space, right? Paul Bookout: Right. Host: Kind of a big thing. Paul Bookout: Definitely, yes. Host: Is it the only one that's rated for human, for deep space? David Smith: Well, it's the only launch vehicle today that's being designed specifically for that. There's-- Host: I see. David Smith: You could make the argument that a Boeing CST-100 capsule flying on a Falcon, excuse me, on a Atlas is a human-rated system. It's not really. It's an amalgam. And by the way, that's aimed at LEO. So they-- Host: I see. David Smith: You know, it, yes, we are the only ones that are being, designing specifically for that, and it's for safety reasons. Host: So it has to really meet these standards. It has to be redundant. It has to, and the SLS is the big, deep-space rocket that has the standards, has the capabilities, and is going to get you farther. David Smith: Right. Host: Ultimately. Paul Bookout: Exactly. And, you know, to be that safe vehicle for launching humans into space, deep space, you know, we have to have these built-in, redundant systems. We have to do all these testing throughout the whole build of the system. You know, of course, that's a little penalty that we have to have additional mass to be able to have this redundancy, have this extra safety aspects of this vehicle. So that, of course, goes right in against being able to have a larger mass, up mass capability. But we're doing this for human exploration, not robotics exploration, so we're, we have to take those extra steps to make it safe. Host: That's right. So what's the benefit of having this large up mass versus just launching a bunch of rockets with smaller masses? David Smith: Right. We, what's often not fully appreciated is, for human spaceflight, for long duration, you can put together a whole bunch of little modules for humans, but think about it like this: Every time you put together a module, it has to have a hatch. Maybe it has to have two. It has to have a life support system. It has to have a power system, a thermal system. It has to be able to operate autonomously until another small module is joined to it. So you can make a lunar orbiting platform or a Mars deep-space transport out of many small modules brought up over time for that many vehicles, but the problem is it becomes sub optimized. You end up paying maybe 50% more mass for all the structure you don't really have to have. Plus, now, you have many duplicative subsystems for many modules that have to all function flawlessly together and have to wait in space while other modules come up over time and to be joined together. So when you think about this, coming up with this giant, origami-type space station that's deployed over years from many small modules compared to one flight or maybe two flights bringing up a very large module that does everything in one reliable, tested on the ground type of human habitation system, it becomes almost a no-brainer, right. [laughs] If you want to make sure your people are alive over time, you really want that kind of system. Only SLS right now is sized to do that. Other guys can certainly deliver those pieces, but they'd be a lot smaller and you'd have these issues that we just talked about. Host: That's right. And I guess it kind of opens up some opportunities for just, because you can have a larger up mass, because you have more space within the fairing to put things-- David Smith: Right. Host: Now, you have a lot less constraints because even -- I'm going to go back to James Webb, right. James Webb is a wonderful telescope, but it was constrained by what it can-- David Smith: The volume of the fairing. Host: Yeah, so it had to come up with this folding technique to pretty much fit inside the fairing. Otherwise, you couldn't launch the satellite. But I guess you can design, you have a little bit more freedom of design with something a little bit larger, right? David Smith: Or if you wanted to scale up the James Webb design, let's say that was the perfect design for telescopes-- Host: Yeah. David Smith: You could make a telescope that's five times larger with the large fairing that, you know, larger fairings that SLS could fly. So it opens up a whole, either you can have a non-origami type, folding-out type telescope, and it's all great, or, if you want to still do that, it gets you something even larger. So the scale is, the current fairing is, in some cases, the ten-meter fairing would be five times larger than the largest existing fairing today-- Host: Whoa. David Smith: If we could produce that. And that's, you know, we're talking a seven-story building could fit inside that ten, you know, [laughs] that long, the long, ten-meter, diameter, meter, diameter fairing. Host: All right. Just launch my house into space and just-- David Smith: There you go. Host: Kind of get a nice view. David Smith: Well, it'd be your condo building that it would launch-- Host: [laughs] Condo building. David Smith: Not your house. David Smith: Even bigger. Host: Yes. Host: So I kind of wanted to end with just sort of a scope of, we're kind of setting up a scene for what this rocket is capable of. Looking towards the future, and, David, you kind of pointed towards this, was this is a 50-year rocket, right. This is something that we're planning on using for a long time for many missions. How do you see this rocket being used? Like, take us into the future. What is this rocket going to give us? David Smith: So, you know, obviously, the lunar orbiting platform would be the first step. Let's-- Host: Yeah. David Smith: Improve the technologies in our backyard we call the Moon. We use those technologies then to extrapolate a system that can go to Mars safely and start, you know, bringing Mars into this human ring of habitation in our solar system. Some of the more exciting things in tandem are these robotic missions. There's the idea that we can send, because we can go so fast, we, so fast into the deeper reaches of the solar system, that within a five-year mission, we can send out a telescope that could go 200 astronomical units out from the Sun, and actually come back and aim at the Sun, and use the Sun as a gravitational lens to see exoplanets on the other side of the Sun. So we could make the world's largest telescope by having one lens on one side of the Sun and using the Sun's gravity as the other lens, and now seeing planets like we could've never seen them before, all because SLS can send that telescope out in a time frame that we can actually operation a mission, versus, you know, remember, Voyager took 30 years to get outside to, close to the heliosphere. So, you know, it's a, it's such a game changer that the real issue with SLS is we haven't thought about all the stuff we can do with it yet, you know. It kind of bends our imagination in a new way that we haven't been thinking of. Another example is interstellar probe. Again, sending something beyond the heliosphere now. You know, instead of the Voyager drifting out there over 30 to 40 years, we can send something out there in 20 years to break the barrier and see what's on the other side of the heliosphere. And we can do that in an active manner versus we're just getting little pulses from Voyager now still coming back. We can be much more active in that. So a lot of places like JPL are investigating the capability of SLS in ways that we never even thought of recently. So we're just on the very edge of discovering what we can do with the system. Host: Unbelievable. And this just kind of opens up the plan for exploring beyond low Earth orbit, right. You've said the first step for human exploration is going towards the Moon, but now you have a bunch of Moon missions. You kind of develop your skills. You got this Lunar Orbital Platform, the gateway that's going to bring us, the truck stop [laughs] that we call it-- David Smith: Right. Host: Is going to take us further out. And I'm guessing this will be used for the future human missions too beyond this first step. David Smith: Well, if we go to, we talked about I think in the earlier episode, nuclear thermal propulsion. Host: Yeah. David Smith: If we're able to employ that for human transport, we can reduce times to where we can send people maybe even ultimately beyond Mars. So, but only SLS with its capability to loft both mass and volume, when the nuclear, this nuclear thermal propulsion requires large amounts of hydrogen, which requires volume, only the SLS can give us that capability to even see if some of these technologies are usable, versus just relying on the same old technologies as the last 50 years. So we have so much promise in front of us with this. Host: Unbelievable. You guys are getting me all excited for what's to come. I just want to take a time machine, and jump, you know, 20 years into the future, and just see this rocket has done. Paul Bookout: Yep, you're not the only one. David Smith: [laughter] Take us with you. Host: Yeah, that's-- David Smith: We want to be there too. Host: Unbelievable. Hey, David and Paul, thank you so much for coming on, and kind of describing the SLS, and really spending so much time so we can do this in two episodes because there's so much to this story. And honestly, this was the first time that I've actually gone into this much detail for the rocket, so I really appreciate you getting on. And for the listeners, please listen to Parts 1 and 2 and get the whole story of what this rocket is all about. Guys, thanks again for coming on. Houston, we have a podcast. David Smith: You're welcome. Paul Bookout: Thank you very much for having us. Host: Welcome to the official podcast of the NASA Johnson Space Center, Episode 2, Can You Hear Me Now? I'm Gary Jordan, and I'll be your host today. In this podcast, we're bringing in the experts -- NASA scientists, engineers, astronauts, pretty much all the folks that have the coolest information, the stuff that you really want to know. [inaudible] We're talking everything from extraterrestrial [inaudible] to the unknown [inaudible]. So today, we're talking space communication networks with Bill Foster. He's a ground controller-- Hey, thanks for sticking around and listening to the whole full story of the Space Launch System. This was Episode 42, Part 2. If you haven't listened to Part 1, go back. You can listen to some of the more components about EM1 and then just some general ideas about what SLS was. Otherwise, you can go to some social media channels and website. We'll start with the website -- www.NASA.gov/SLS. That's where you can get the latest and greatest. Otherwise, you can follow some social media accounts on Twitter. It's @NASA underscore SLS. On Facebook, it's NASA SLS. Or you can actually go on the web and search "SLS Mission Planner's Guide," and it's a document on the web that you can download and just learn everything about the rocket, some of the constraints. And that was actually one of the things that Mr. David Smith worked on. So we're really looking forward to the launch of the first SLS. Glad you were able to join us on today's podcast to listen about the rocket and some of the missions and capabilities of the Space Launch System. If you have any questions, just use the #askNASA on your favorite platform for the NASA Johnson Space Center accounts on Facebook, Twitter, and Instagram. You can submit a question or an idea for an episode that you want us to cover here on the podcast. Just make sure to mention it's for this podcast, Houston We Have a Podcast. This episode was recorded on March 20th, 2018 thanks to Alex Perryman, Rachel Craft, Laura Reshawn [phonetic], Kelly Humphries, Pat Ryan, Tyler Martin, Bev Perry, and all the folks at the Marshall Space Flight Center for helping to put this together. Thanks again to Dr. Paul Bookout and Mr. David Smith for coming on the show. [inaudible