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  • Articles  (35)
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  • 1
    Publication Date: 2016-05-05
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hamilton, Douglas P -- England -- Nature. 2016 May 4;533(7602):187-8. doi: 10.1038/nature17896.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy, University of Maryland, College Park, Maryland 20742-2421, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/27144360" target="_blank"〉PubMed〈/a〉
    Keywords: Astronomical Phenomena ; Astronomy/*methods ; Gravitation ; *Models, Theoretical ; *Solar System
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    Electronic ISSN: 1476-4687
    Topics: Biology , Chemistry and Pharmacology , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2015-03-18
    Description: Vertebrates have a unique 3D body shape in which correct tissue and organ shape and alignment are essential for function. For example, vision requires the lens to be centred in the eye cup which must in turn be correctly positioned in the head. Tissue morphogenesis depends on force generation, force transmission through the tissue, and response of tissues and extracellular matrix to force. Although a century ago D'Arcy Thompson postulated that terrestrial animal body shapes are conditioned by gravity, there has been no animal model directly demonstrating how the aforementioned mechano-morphogenetic processes are coordinated to generate a body shape that withstands gravity. Here we report a unique medaka fish (Oryzias latipes) mutant, hirame (hir), which is sensitive to deformation by gravity. hir embryos display a markedly flattened body caused by mutation of YAP, a nuclear executor of Hippo signalling that regulates organ size. We show that actomyosin-mediated tissue tension is reduced in hir embryos, leading to tissue flattening and tissue misalignment, both of which contribute to body flattening. By analysing YAP function in 3D spheroids of human cells, we identify the Rho GTPase activating protein ARHGAP18 as an effector of YAP in controlling tissue tension. Together, these findings reveal a previously unrecognised function of YAP in regulating tissue shape and alignment required for proper 3D body shape. Understanding this morphogenetic function of YAP could facilitate the use of embryonic stem cells to generate complex organs requiring correct alignment of multiple tissues.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4720436/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4720436/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Porazinski, Sean -- Wang, Huijia -- Asaoka, Yoichi -- Behrndt, Martin -- Miyamoto, Tatsuo -- Morita, Hitoshi -- Hata, Shoji -- Sasaki, Takashi -- Krens, S F Gabriel -- Osada, Yumi -- Asaka, Satoshi -- Momoi, Akihiro -- Linton, Sarah -- Miesfeld, Joel B -- Link, Brian A -- Senga, Takeshi -- Castillo-Morales, Atahualpa -- Urrutia, Araxi O -- Shimizu, Nobuyoshi -- Nagase, Hideaki -- Matsuura, Shinya -- Bagby, Stefan -- Kondoh, Hisato -- Nishina, Hiroshi -- Heisenberg, Carl-Philipp -- Furutani-Seiki, Makoto -- P30 EY001931/EY/NEI NIH HHS/ -- R01 EY014167/EY/NEI NIH HHS/ -- R01 EY016060/EY/NEI NIH HHS/ -- R01EY014167/EY/NEI NIH HHS/ -- Medical Research Council/United Kingdom -- England -- Nature. 2015 May 14;521(7551):217-21. doi: 10.1038/nature14215. Epub 2015 Mar 16.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Biology and Biochemistry, University of Bath, Bath BA2 7AY, UK. ; Department of Developmental and Regenerative Biology, Medical Research Institute, Tokyo Medical and Dental University (TMDU), Tokyo 113-8510, Japan. ; IST Austria, Am Campus 1, A-3400 Klosterneuburg, Austria. ; Department of Genetics and Cell Biology, Research Institute for Radiation Biology and Medicine, Hiroshima University, Hiroshima 734-8553, Japan. ; Department of Molecular Biology, School of Medicine, Keio University, Tokyo 160-8582, Japan. ; Japan Science and Technology Agency (JST), ERATO-SORST Kondoh Differentiation Signaling Project, Kyoto 606-8305, Japan. ; Department of Cell Biology, Neurobiology, and Anatomy, Medical College of Wisconsin, Milwaukee, Wisconsin 53226, USA. ; Division of Cancer Biology, Nagoya University Graduate School of Medicine, Nagoya 466-8550, Japan. ; Kennedy Institute of Rheumatology, Nuffield Department of Orthopaedics, Rheumatology and Musculoskeletal Sciences, University of Oxford, Oxford OX3 7FY, UK. ; 1] Japan Science and Technology Agency (JST), ERATO-SORST Kondoh Differentiation Signaling Project, Kyoto 606-8305, Japan [2] Graduate School of Frontier Bioscience, Osaka University, Osaka 565-0871, Japan [3] Faculty of Life Sciences, Kyoto Sangyo University, Kyoto 603-8555, Japan. ; 1] Department of Biology and Biochemistry, University of Bath, Bath BA2 7AY, UK [2] Japan Science and Technology Agency (JST), ERATO-SORST Kondoh Differentiation Signaling Project, Kyoto 606-8305, Japan.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/25778702" target="_blank"〉PubMed〈/a〉
    Keywords: Actomyosin/metabolism ; Adaptor Proteins, Signal Transducing/genetics/metabolism ; Animals ; Body Size/*genetics ; Embryo, Nonmammalian/anatomy & histology/embryology/metabolism ; Fish Proteins/genetics/*metabolism ; GTPase-Activating Proteins/metabolism ; Genes, Essential/genetics ; Gravitation ; Humans ; Morphogenesis/*genetics ; Mutation/genetics ; Organ Size/genetics ; Oryzias/*anatomy & histology/*embryology/genetics ; Phenotype ; Protein-Serine-Threonine Kinases/genetics/metabolism ; Signal Transduction ; Spheroids, Cellular/cytology/metabolism
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  • 3
    Publication Date: 2013-03-16
    Description: Determining the atmospheric structure and chemical composition of an exoplanet remains a formidable goal. Fortunately, advancements in the study of exoplanets and their atmospheres have come in the form of direct imaging--spatially resolving the planet from its parent star--which enables high-resolution spectroscopy of self-luminous planets in jovian-like orbits. Here, we present a spectrum with numerous, well-resolved molecular lines from both water and carbon monoxide from a massive planet orbiting less than 40 astronomical units from the star HR 8799. These data reveal the planet's chemical composition, atmospheric structure, and surface gravity, confirming that it is indeed a young planet. The spectral lines suggest an atmospheric carbon-to-oxygen ratio that is greater than that of the host star, providing hints about the planet's formation.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Konopacky, Quinn M -- Barman, Travis S -- Macintosh, Bruce A -- Marois, Christian -- New York, N.Y. -- Science. 2013 Mar 22;339(6126):1398-401. doi: 10.1126/science.1232003. Epub 2013 Mar 14.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Dunlap Institute for Astronomy and Astrophysics, University of Toronto, 50 St. George Street, Toronto, ON M5S 3H4, Canada. konopacky@di.utoronto.ca〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/23493423" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Carbon Monoxide ; *Evolution, Planetary ; Extraterrestrial Environment ; Gravitation ; *Planets ; Spectrum Analysis ; *Water
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    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 4
    Publication Date: 2012-06-30
    Description: We have detected in Cassini spacecraft data the signature of the periodic tidal stresses within Titan, driven by the eccentricity (e = 0.028) of its 16-day orbit around Saturn. Precise measurements of the acceleration of Cassini during six close flybys between 2006 and 2011 have revealed that Titan responds to the variable tidal field exerted by Saturn with periodic changes of its quadrupole gravity, at about 4% of the static value. Two independent determinations of the corresponding degree-2 Love number yield k(2) = 0.589 +/- 0.150 and k(2) = 0.637 +/- 0.224 (2sigma). Such a large response to the tidal field requires that Titan's interior be deformable over time scales of the orbital period, in a way that is consistent with a global ocean at depth.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Iess, Luciano -- Jacobson, Robert A -- Ducci, Marco -- Stevenson, David J -- Lunine, Jonathan I -- Armstrong, John W -- Asmar, Sami W -- Racioppa, Paolo -- Rappaport, Nicole J -- Tortora, Paolo -- New York, N.Y. -- Science. 2012 Jul 27;337(6093):457-9. doi: 10.1126/science.1219631. Epub 2012 Jun 28.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Dipartimento di Ingegneria Meccanica e Aerospaziale, Universita La Sapienza, via Eudossiana 18, 00184 Rome, Italy. luciano.iess@uniroma1.it〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/22745254" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment ; Gravitation ; Ice ; *Saturn ; Spacecraft ; *Water
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  • 5
    Publication Date: 2010-03-13
    Description: Precise radio tracking of the spacecraft Cassini has provided a determination of Titan's mass and gravity harmonics to degree 3. The quadrupole field is consistent with a hydrostatically relaxed body shaped by tidal and rotational effects. The inferred moment of inertia factor is about 0.34, implying incomplete differentiation, either in the sense of imperfect separation of rock from ice or a core in which a large amount of water remains chemically bound in silicates. The equilibrium figure is a triaxial ellipsoid whose semi-axes a, b, and c differ by 410 meters (a-c) and 103 meters (b-c). The nonhydrostatic geoid height variations (up to 19 meters) are small compared to the observed topographic anomalies of hundreds of meters, suggesting a high degree of compensation appropriate to a body that has warm ice at depth.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Iess, Luciano -- Rappaport, Nicole J -- Jacobson, Robert A -- Racioppa, Paolo -- Stevenson, David J -- Tortora, Paolo -- Armstrong, John W -- Asmar, Sami W -- New York, N.Y. -- Science. 2010 Mar 12;327(5971):1367-9. doi: 10.1126/science.1182583.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Dipartimento di Ingegneria Aerospaziale ed Astronautica, Universita La Sapienza, via Eudossiana 18, 00184 Rome, Italy. luciano.iess@uniroma1.it〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20223984" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment ; Gravitation ; Ice ; *Saturn ; Spacecraft ; Water
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  • 6
    Publication Date: 2010-09-11
    Description: Plants and animals produce modular developmental units in a periodic fashion. In plants, lateral roots form as repeating units along the root primary axis; however, the developmental mechanism regulating this process is unknown. We found that cyclic expression pulses of a reporter gene mark the position of future lateral roots by establishing prebranch sites and that prebranch site production and root bending are periodic. Microarray and promoter-luciferase studies revealed two sets of genes oscillating in opposite phases at the root tip. Genetic studies show that some oscillating transcriptional regulators are required for periodicity in one or both developmental processes. This molecular mechanism has characteristics that resemble molecular clock-driven activities in animal species.〈br /〉〈br /〉〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2976612/" target="_blank"〉〈img src="https://static.pubmed.gov/portal/portal3rc.fcgi/4089621/img/3977009" border="0"〉〈/a〉   〈a href="https://www.ncbi.nlm.nih.gov/pmc/articles/PMC2976612/" target="_blank"〉This paper as free author manuscript - peer-reviewed and accepted for publication〈/a〉〈br /〉〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Moreno-Risueno, Miguel A -- Van Norman, Jaimie M -- Moreno, Antonio -- Zhang, Jingyuan -- Ahnert, Sebastian E -- Benfey, Philip N -- R01 GM043778/GM/NIGMS NIH HHS/ -- R01 GM043778-19/GM/NIGMS NIH HHS/ -- R01 GM043778-20/GM/NIGMS NIH HHS/ -- R01 GM043778-21/GM/NIGMS NIH HHS/ -- R01-GM043778/GM/NIGMS NIH HHS/ -- New York, N.Y. -- Science. 2010 Sep 10;329(5997):1306-11. doi: 10.1126/science.1191937.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Biology and Institute for Genome Sciences and Policy Center for Systems Biology, Duke University, Durham, NC 27708, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20829477" target="_blank"〉PubMed〈/a〉
    Keywords: Arabidopsis/cytology/*genetics/*growth & development/metabolism ; Arabidopsis Proteins/genetics/metabolism ; Gene Expression Profiling ; *Gene Expression Regulation, Plant ; Gene Regulatory Networks ; Genes, Plant ; Genes, Reporter ; Gravitation ; Indoleacetic Acids/metabolism/pharmacology ; Meristem/*genetics/*growth & development/metabolism ; Oligonucleotide Array Sequence Analysis ; Phthalimides/pharmacology ; Plant Roots/cytology/genetics/*growth & development ; Promoter Regions, Genetic ; Signal Transduction ; Temperature ; Time Factors ; Transcription Factors/genetics/metabolism ; Transcription, Genetic
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  • 7
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    Nature Publishing Group (NPG)
    Publication Date: 2010-07-31
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kwok, Roberta -- England -- Nature. 2010 Jul 29;466(7306):540-1. doi: 10.1038/466540a.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20671681" target="_blank"〉PubMed〈/a〉
    Keywords: Earth (Planet) ; Gravitation ; *Meteoroids ; *Minor Planets ; *Moon ; Time Factors ; Water/analysis
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  • 8
    Publication Date: 2010-01-16
    Description: Wetlands are the largest individual source of methane (CH4), but the magnitude and distribution of this source are poorly understood on continental scales. We isolated the wetland and rice paddy contributions to spaceborne CH4 measurements over 2003-2005 using satellite observations of gravity anomalies, a proxy for water-table depth Gamma, and surface temperature analyses TS. We find that tropical and higher-latitude CH4 variations are largely described by Gamma and TS variations, respectively. Our work suggests that tropical wetlands contribute 52 to 58% of global emissions, with the remainder coming from the extra-tropics, 2% of which is from Arctic latitudes. We estimate a 7% rise in wetland CH4 emissions over 2003-2007, due to warming of mid-latitude and Arctic wetland regions, which we find is consistent with recent changes in atmospheric CH4.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Bloom, A Anthony -- Palmer, Paul I -- Fraser, Annemarie -- Reay, David S -- Frankenberg, Christian -- New York, N.Y. -- Science. 2010 Jan 15;327(5963):322-5. doi: 10.1126/science.1175176.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉School of GeoSciences, University of Edinburgh, Edinburgh, UK.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20075250" target="_blank"〉PubMed〈/a〉
    Keywords: Archaea/metabolism ; Atmosphere/*chemistry ; *Crops, Agricultural/growth & development ; Geography ; Gravitation ; Methane/*analysis/biosynthesis ; *Oryza/growth & development ; Seasons ; Spacecraft ; Temperature ; Tropical Climate ; *Wetlands
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  • 9
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2010-03-13
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Sohl, Frank -- New York, N.Y. -- Science. 2010 Mar 12;327(5971):1338-9. doi: 10.1126/science.1186255.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Institute of Planetary Research, German Aerospace Center (DLR), Rutherfordstrasse 2, 12489 Berlin, Germany. frank.sohl@dlr.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/20223976" target="_blank"〉PubMed〈/a〉
    Keywords: Extraterrestrial Environment ; Gravitation ; Ice ; *Saturn ; Spacecraft ; Water
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  • 10
    Publication Date: 2010-11-13
    Description: Animals have developed a range of drinking strategies depending on physiological and environmental constraints. Vertebrates with incomplete cheeks use their tongue to drink; the most common example is the lapping of cats and dogs. We show that the domestic cat (Felis catus) laps by a subtle mechanism based on water adhesion to the dorsal side of the tongue. A combined experimental and theoretical analysis reveals that Felis catus exploits fluid inertia to defeat gravity and pull liquid into the mouth. This competition between inertia and gravity sets the lapping frequency and yields a prediction for the dependence of frequency on animal mass. Measurements of lapping frequency across the family Felidae support this prediction, which suggests that the lapping mechanism is conserved among felines.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Reis, Pedro M -- Jung, Sunghwan -- Aristoff, Jeffrey M -- Stocker, Roman -- New York, N.Y. -- Science. 2010 Nov 26;330(6008):1231-4. doi: 10.1126/science.1195421. Epub 2010 Nov 11.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Civil and Environmental Engineering, Massachusetts Institute of Technology (MIT), Cambridge, MA 02139, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21071630" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Biomechanical Phenomena ; Cats/*physiology ; Drinking/*physiology ; Felidae/physiology ; Gravitation ; Models, Biological ; Movement ; Physical Processes ; Tongue/*physiology
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  • 11
    Publication Date: 2009-02-21
    Description: Thin layers of phytoplankton are important hotspots of ecological activity that are found in the coastal ocean, meters beneath the surface, and contain cell concentrations up to two orders of magnitude above ambient concentrations. Current interpretations of their formation favor abiotic processes, yet many phytoplankton species found in these layers are motile. We demonstrated that layers formed when the vertical migration of phytoplankton was disrupted by hydrodynamic shear. This mechanism, which we call gyrotactic trapping, can be responsible for the thin layers of phytoplankton commonly observed in the ocean. These results reveal that the coupling between active microorganism motility and ambient fluid motion can shape the macroscopic features of the marine ecological landscape.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Durham, William M -- Kessler, John O -- Stocker, Roman -- New York, N.Y. -- Science. 2009 Feb 20;323(5917):1067-70. doi: 10.1126/science.1167334.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Civil and Environmental Engineering, Massachusetts Institute of Technology (MIT), Cambridge, MA 02139, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/19229037" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Biomechanical Phenomena ; Cell Shape ; Chlamydomonas/cytology/*physiology ; *Ecosystem ; Flagella ; Gravitation ; Movement ; Phytoplankton/cytology/*physiology ; *Water ; *Water Movements
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  • 12
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2006-12-23
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉New York, N.Y. -- Science. 2006 Dec 22;314(5807):1850-1.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/17185567" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Birds ; Cosmic Radiation ; Electric Conductivity ; Gravitation ; Helium/chemistry ; Humans ; Influenza A Virus, H5N1 Subtype ; Influenza in Birds/epidemiology/virology ; Influenza, Human/epidemiology/virology ; Microbiology ; RNA Interference ; *Science ; Temperature
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  • 13
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2005-04-02
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Alexander, R McNeill -- New York, N.Y. -- Science. 2005 Apr 1;308(5718):58-9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉School of Biology, University of Leeds, Leeds LS2 9JT, UK. r.m.alexander@leeds.ac.uk〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15802589" target="_blank"〉PubMed〈/a〉
    Keywords: Biomechanical Phenomena ; Energy Metabolism ; Gravitation ; Humans ; Models, Anatomic ; Oxygen Consumption ; *Robotics ; *Walking/physiology
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  • 14
    Publication Date: 2005-02-19
    Description: Passive-dynamic walkers are simple mechanical devices, composed of solid parts connected by joints, that walk stably down a slope. They have no motors or controllers, yet can have remarkably humanlike motions. This suggests that these machines are useful models of human locomotion; however, they cannot walk on level ground. Here we present three robots based on passive-dynamics, with small active power sources substituted for gravity, which can walk on level ground. These robots use less control and less energy than other powered robots, yet walk more naturally, further suggesting the importance of passive-dynamics in human locomotion.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Collins, Steve -- Ruina, Andy -- Tedrake, Russ -- Wisse, Martijn -- New York, N.Y. -- Science. 2005 Feb 18;307(5712):1082-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Mechanical Engineering, University of Michigan, Ann Arbor, MI 48104, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15718465" target="_blank"〉PubMed〈/a〉
    Keywords: Algorithms ; Biomechanical Phenomena ; Electric Power Supplies ; Energy Metabolism ; Gait ; Gravitation ; Humans ; Motion ; Oxygen Consumption ; *Robotics ; *Walking
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  • 15
    Publication Date: 2005-05-28
    Description: Radio Doppler data from the Galileo spacecraft's encounter with Amalthea, one of Jupiter's small inner moons, on 5 November 2002 yield a mass of (2.08 +/- 0.15) x 10(18) kilograms. Images of Amalthea from two Voyager spacecraft in 1979 and Galileo imaging between November 1996 and June 1997 yield a volume of (2.43 +/- 0.22) x 10(6) cubic kilometers. The satellite thus has a density of 857 +/- 99 kilograms per cubic meter. We suggest that Amalthea is porous and composed of water ice, as well as rocky material, and thus formed in a cold region of the solar system, possibly not at its present location near Jupiter.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Anderson, John D -- Johnson, Torrence V -- Schubert, Gerald -- Asmar, Sami -- Jacobson, Robert A -- Johnston, Douglas -- Lau, Eunice L -- Lewis, George -- Moore, William B -- Taylor, Anthony -- Thomas, Peter C -- Weinwurm, Gudrun -- New York, N.Y. -- Science. 2005 May 27;308(5726):1291-3.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109-8099, USA. john.d.anderson@jpl.nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15919987" target="_blank"〉PubMed〈/a〉
    Keywords: Gravitation ; Ice ; *Jupiter ; Pressure ; Spacecraft ; *Water
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  • 16
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2005-12-24
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉New York, N.Y. -- Science. 2005 Dec 23;310(5756):1885.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/16373543" target="_blank"〉PubMed〈/a〉
    Keywords: Animals ; Birds ; Cosmic Radiation ; Environmental Microbiology ; Gravitation ; Humans ; Physical Phenomena ; Physics ; Rna ; Research/*trends
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2004-09-09
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Fortney, Jonathan J -- New York, N.Y. -- Science. 2004 Sep 3;305(5689):1414-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Planetary Systems Branch, NASA Ames Research Center, Moffett Field, CA 94035, USA. jfortney@arc.nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15353790" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Evolution, Planetary ; Gravitation ; *Helium ; *Hydrogen ; *Jupiter ; Mathematics ; Models, Structural ; Pressure ; *Saturn ; Spacecraft ; Temperature
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2003-04-12
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Dehant, Veronique -- New York, N.Y. -- Science. 2003 Apr 11;300(5617):260-1.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/12690177" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; Evolution, Planetary ; Gravitation ; *Mars ; Pressure ; Temperature
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    Publication Date: 2003-03-08
    Description: The solar tidal deformation of Mars, measured by its k2 potential Love number, has been obtained from an analysis of Mars Global Surveyor radio tracking. The observed k2 of 0.153 +/- 0.017 is large enough to rule out a solid iron core and so indicates that at least the outer part of the core is liquid. The inferred core radius is between 1520 and 1840 kilometers and is independent of many interior properties, although partial melt of the mantle is one factor that could reduce core size. Ice-cap mass changes can be deduced from the seasonal variations in air pressure and the odd gravity harmonic J3, given knowledge of cap mass distribution with latitude. The south cap seasonal mass change is about 30 to 40% larger than that of the north cap.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Yoder, C F -- Konopliv, A S -- Yuan, D N -- Standish, E M -- Folkner, W M -- New York, N.Y. -- Science. 2003 Apr 11;300(5617):299-303. Epub 2003 Mar 6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. Charles.F.Yoder@jpl.nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/12624177" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Dry Ice ; Gravitation ; *Mars ; Mathematics ; Pressure ; Rotation ; Temperature
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2003-05-06
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Lawler, Andrew -- New York, N.Y. -- Science. 2003 May 2;300(5620):727.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/12730573" target="_blank"〉PubMed〈/a〉
    Keywords: Evolution, Planetary ; Extraterrestrial Environment ; Gravitation ; Ice ; *Moon ; *Space Flight
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2003-07-12
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Stone, Richard -- New York, N.Y. -- Science. 2003 Jul 11;301(5630):152.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/12855780" target="_blank"〉PubMed〈/a〉
    Keywords: Biological Evolution ; England ; Fossils ; Gravitation ; History, 17th Century ; Natural History/history ; Physics/history ; Science/*history
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  • 22
    Publication Date: 2002-12-03
    Description: The evolution of gravitationally unstable protoplanetary gaseous disks has been studied with the use of three-dimensional smoothed particle hydrodynamics simulations with unprecedented resolution. We have considered disks with initial masses and temperature profiles consistent with those inferred for the protosolar nebula and for other protoplanetary disks. We show that long-lasting, self-gravitating protoplanets arise after a few disk orbital periods if cooling is efficient enough to maintain the temperature close to 50 K. The resulting bodies have masses and orbital eccentricities similar to those of detected extrasolar planets.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Mayer, Lucio -- Quinn, Thomas -- Wadsley, James -- Stadel, Joachim -- New York, N.Y. -- Science. 2002 Nov 29;298(5599):1756-9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Astronomy, University of Washington, Seattle, WA 98195, USA. lucio@physik.unizh.ch〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/12459581" target="_blank"〉PubMed〈/a〉
    Keywords: Computer Simulation ; *Evolution, Planetary ; Gases ; Gravitation ; Hydrogen ; Jupiter ; *Planets
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2002-12-03
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kerr, Richard A -- New York, N.Y. -- Science. 2002 Nov 29;298(5599):1698-9.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/12459562" target="_blank"〉PubMed〈/a〉
    Keywords: Computer Simulation ; *Evolution, Planetary ; Gases ; Gravitation ; *Jupiter ; *Saturn
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2001-02-07
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kerr, R A -- New York, N.Y. -- Science. 2000 Mar 10;287(5459):1727-8.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10755919" target="_blank"〉PubMed〈/a〉
    Keywords: *Evolution, Planetary ; *Extraterrestrial Environment ; Geologic Sediments ; Gravitation ; *Mars ; *Water
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  • 25
    Publication Date: 2001-04-03
    Description: Loading of the lithosphere of Mars by the Tharsis rise explains much of the global shape and long-wavelength gravity field of the planet, including a ring of negative gravity anomalies and a topographic trough around Tharsis, as well as gravity anomaly and topographic highs centered in Arabia Terra and extending northward toward Utopia. The Tharsis-induced trough and antipodal high were largely in place by the end of the Noachian Epoch and exerted control on the location and orientation of valley networks. The release of carbon dioxide and water accompanying the emplacement of approximately 3 x 10(8) cubic kilometers of Tharsis magmas may have sustained a warmer climate than at present, enabling the formation of ancient valley networks and fluvial landscape denudation in and adjacent to the large-scale trough.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Phillips, R J -- Zuber, M T -- Solomon, S C -- Golombek, M P -- Jakosky, B M -- Banerdt, W B -- Smith, D E -- Williams, R M -- Hynek, B M -- Aharonson, O -- Hauck , S A 2nd -- New York, N.Y. -- Science. 2001 Mar 30;291(5513):2587-91. Epub 2001 Mar 15.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉McDonnell Center for the Space Sciences and Department of Earth and Planetary Sciences, Washington University, St. Louis, MO 63130, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/11283367" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Carbon Dioxide ; *Evolution, Planetary ; Extraterrestrial Environment ; Gravitation ; *Mars ; *Water
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2001-10-06
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Stevenson, D J -- New York, N.Y. -- Science. 2001 Oct 5;294(5540):71-2.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA. djs@gps.caltech.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/11588243" target="_blank"〉PubMed〈/a〉
    Keywords: Evolution, Planetary ; Extraterrestrial Environment ; Gravitation ; Ice ; *Jupiter
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 2001-12-12
    Description: Using topography collected over one martian year from the Mars Orbiter Laser Altimeter on the Mars Global Surveyor (MGS) spacecraft, we have measured temporal changes in the elevation of the martian surface that correlate with the seasonal cycle of carbon dioxide exchange between the surface and atmosphere. The greatest elevation change (1.5 to 2 meters) occurs at high latitudes ( above 80 degrees ), whereas the bulk of the mass exchange occurs at lower latitudes (below 75 degrees N and below 73 degrees S). An unexpected period of sublimation was observed during northern hemisphere autumn, coincident with dust storms in the southern hemisphere. Analysis of MGS Doppler tracking residuals revealed temporal variations in the flattening of Mars that correlate with elevation changes. The combined changes in gravity and elevation constrain the average density of seasonally deposited carbon dioxide to be 910 +/- 230 kilograms per cubic meter, which is considerably denser than terrestrial snow.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Smith, D E -- Zuber, M T -- Neumann, G A -- New York, N.Y. -- Science. 2001 Dec 7;294(5549):2141-6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Laboratory for Terrestrial Physics, NASA/Goddard Space Flight Center, Greenbelt, MD 20771, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/11739951" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Carbon Dioxide ; *Dry Ice ; Extraterrestrial Environment ; Gravitation ; *Mars ; Seasons ; Temperature
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  • 28
    Publication Date: 2000-03-10
    Description: Topography and gravity measured by the Mars Global Surveyor have enabled determination of the global crust and upper mantle structure of Mars. The planet displays two distinct crustal zones that do not correlate globally with the geologic dichotomy: a region of crust that thins progressively from south to north and encompasses much of the southern highlands and Tharsis province and a region of approximately uniform crustal thickness that includes the northern lowlands and Arabia Terra. The strength of the lithosphere beneath the ancient southern highlands suggests that the northern hemisphere was a locus of high heat flow early in martian history. The thickness of the elastic lithosphere increases with time of loading in the northern plains and Tharsis. The northern lowlands contain structures interpreted as large buried channels that are consistent with northward transport of water and sediment to the lowlands before the end of northern hemisphere resurfacing.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Zuber, M T -- Solomon, S C -- Phillips, R J -- Smith, D E -- Tyler, G L -- Aharonson, O -- Balmino, G -- Banerdt, W B -- Head, J W -- Johnson, C L -- Lemoine, F G -- McGovern, P J -- Neumann, G A -- Rowlands, D D -- Zhong, S -- New York, N.Y. -- Science. 2000 Mar 10;287(5459):1788-93.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA. zuber@mit.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10710301" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Evolution, Planetary ; *Extraterrestrial Environment ; Geologic Sediments ; Gravitation ; *Mars ; Temperature ; Water
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  • 29
    Publication Date: 1999-12-22
    Description: Interstellar dust grains intercepted by the dust detectors on the Ulysses and Galileo spacecrafts at heliocentric distances from 2 to 4 astronomical units show a deficit of grains with masses from 1 x 10(-17) to 3 x 10(-16) kilograms relative to grains intercepted outside 4 astronomical units. To divert grains out of the 2- to 4-astronomical unit region, the solar radiation pressure must be 1.4 to 1.8 times the force of solar gravity. These figures are consistent with the optical properties of spherical or elongated grains that consist of astronomical silicates or organic refractory material. Pure graphite grains with diameters of 0.2 to 0.4 micrometer experience a solar radiation pressure force as much as twice the force of solar gravity.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Landgraf, M -- Augustsson, K -- Grun, E -- Gustafson, B A -- New York, N.Y. -- Science. 1999 Dec 17;286(5448):2319-22.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉NASA Johnson Space Center, Mailcode SN2, Houston, TX 77058, USA. mlandgra@esoc.esa.de〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10600737" target="_blank"〉PubMed〈/a〉
    Keywords: *Cosmic Dust ; Gravitation ; Magnetics ; Solar System
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 1998-03-28
    Description: The Mars Global Surveyor (MGS) spacecraft achieved a 45-hour elliptical orbit at Mars on 11 September 1997 after an 11-month cruise from Earth. The mission is acquiring high-quality global observations of the martian surface and atmosphere and of its magnetic and gravitational fields. These observations will continue for one martian year.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Albee, A L -- Palluconi, F D -- Arvidson, R E -- New York, N.Y. -- Science. 1998 Mar 13;279(5357):1671-2.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉California Institute of Technology, Pasadena, CA, 91125, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9497277" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; Atmospheric Pressure ; *Extraterrestrial Environment ; Gravitation ; Magnetics ; *Mars ; Spacecraft
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  • 31
    Publication Date: 1998-06-11
    Description: Radio Doppler data from a single encounter (C3) of the Galileo spacecraft with Callisto, the outermost Galilean moon of Jupiter, indicated that Callisto was probably undifferentiated. Now, similar data from a second encounter (C9) corroborate this conclusion, but more accurate data from a third encounter (C10) indicate that the rock and ice within Callisto have partially, but not completely, separated. Callisto may be differentiated into a rock-metal core less than 25 percent of Callisto's radius, an outer layer of clean ice less than 350 km thick, and a middle layer of mixed rock and ice. Models in which ice and rock are mixed all the way to the center of Callisto are also consistent with the data.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Anderson, J D -- Schubert, G -- Jacobson, R A -- Lau, E L -- Moore, W B -- Sjogren, W L -- New York, N.Y. -- Science. 1998 Jun 5;280(5369):1573-6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California 91109-8099, USA.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9616114" target="_blank"〉PubMed〈/a〉
    Keywords: Ferrous Compounds ; Geologic Sediments ; Gravitation ; Hot Temperature ; *Ice ; Iron ; *Jupiter ; *Metals
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 1998-09-04
    Description: Lunar Prospector is providing a global map of the composition of the moon and analyzing the moon's gravity and magnetic fields. It has been in a polar orbit around the moon since 16 January 1998. Neutron flux data show that there is abundant H, and hence probably abundant water ice, in the lunar polar regions. Gamma-ray and neutron data reveal the distribution of Fe, Ti, and other major and trace elements on the moon. The data delineate the global distributions of a key trace element-rich component of lunar materials called KREEP and of the major rock types. Magnetic mapping shows that the lunar magnetic fields are strong antipodal to Mare Imbrium and Mare Serenitatis and has discovered the smallest known magnetosphere, magnetosheath, and bow shock complex in the solar system. Gravity mapping has delineated seven new gravity anomalies and shown that the moon has a small Fe-rich core of about 300 km radius.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Binder, A B -- New York, N.Y. -- Science. 1998 Sep 4;281(5382):1475-6.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Lunar Research Institute, 1180 Sunrise Drive, Gilroy, CA 95020, USA. abinder@mail.arc.nasa.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9727967" target="_blank"〉PubMed〈/a〉
    Keywords: *Elements ; Extraterrestrial Environment ; Gravitation ; Hydrogen ; Magnetics ; *Moon ; *Spacecraft ; Spectrum Analysis ; Water
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 1998-06-20
    Description: 〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Kargel, J S -- New York, N.Y. -- Science. 1998 May 22;280(5367):1211-2.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉U.S. Geological Survey, Flagstaff, AZ 86001, USA. jkargel@flagmail.wr.usgs.gov〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9634401" target="_blank"〉PubMed〈/a〉
    Keywords: Evolution, Planetary ; Gravitation ; Ice ; *Jupiter ; Oceans and Seas ; *Salts ; Spectrophotometry, Infrared ; *Water
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 1997-10-23
    Description: A stellar-occultation light curve for Triton shows asymmetry that can be understood if Triton's middle atmosphere is distorted from spherical symmetry. Although a globally oblate model can explain the data, the inferred atmospheric flattening is so large that it could be caused only by an unrealistic internal mass distribution or highly supersonic zonal winds. Cyclostrophic winds confined to a jet near Triton's northern or southern limbs (or both) could also be responsible for the details of the light curve, but such winds are required to be slightly supersonic. Hazes and clouds in the atmosphere are unlikely to have caused the asymmetry in the light curve.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Elliot, J L -- Stansberry, J A -- Olkin, C B -- Agner, M A -- Davies, M E -- New York, N.Y. -- Science. 1997 Oct 17;278(5337):436-9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Department of Earth, Atmospheric, and Planetary Sciences and Department of Physics, Building 54-422, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139-4307, USA. jle@mit.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/9334297" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; *Extraterrestrial Environment ; Gravitation ; *Neptune ; Optics and Photonics ; Temperature
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    American Association for the Advancement of Science (AAAS)
    Publication Date: 1979-11-30
    Description: On the earth, or in level flight, a blindfolded subject being rotated at constant velocity about his recumbent long body axis experiences illusory orbital motion of his body in the opposite direction. By contrast, during comparable rotation in the free-fall phase of parabolic flight, no body motion is perceived and all sense of external orientation may be lost; when touch and pressure stimulation is applied to the body surface, a sense of orientation is reestablished immediately. The increased gravitoinertial force period of a parabola produces an exaggeration of the orbital motion experienced in level flight. These observations reveal an important influence of touch, pressure, and kinesthetic information on spatial orientation and provide a basis for understanding many of the postural illusions reported by astronauts in space flight.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Lackner, J R -- Graybiel, A -- New York, N.Y. -- Science. 1979 Nov 30;206(4422):1105-8.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/493998" target="_blank"〉PubMed〈/a〉
    Keywords: Acceleration ; *Aerospace Medicine ; Eye Movements ; Gravitation ; Humans ; Illusions ; Kinesis/physiology ; *Orientation ; Posture ; Pressure ; Touch/physiology
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