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  • 1
    Publication Date: 2005-02-19
    Description: The Observatoire pour la Mineralogie, l'Eau, les Glaces, et l'Activite (OMEGA) visible-infrared imaging spectrometer extensively observed regions of Mars with latitudes above 70 degrees N in late 2004 (heliocentric longitude from Ls 93 degrees to Ls 127 degrees ). The extent of water ice at the surface and the size of ice grains were monitored as a function of time. Bright, small-grained frost, which initially covered a large fraction of the polar cap, waned in favor of large-grained ice. In outlying regions, dominated by large-grained ice, the albedo increased over the period. Evaluating the dust content was model dependent. However, contamination of ice by dust was low.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Langevin, Y -- Poulet, F -- Bibring, J-P -- Schmitt, B -- Doute, S -- Gondet, B -- New York, N.Y. -- Science. 2005 Mar 11;307(5715):1581-4. Epub 2005 Feb 17.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Institut d'Astrophysique Spatiale, CNRS-Universite Paris Sud, 91405 Orsay, France. yves.langevin@ias.u-psud.fr〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15718426" target="_blank"〉PubMed〈/a〉
    Keywords: Carbon Dioxide ; Extraterrestrial Environment ; *Ice ; *Mars ; Seasons ; Spacecraft ; Spectroscopy, Near-Infrared ; Spectrum Analysis ; Water
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
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  • 2
    Publication Date: 2006-04-22
    Description: Global mineralogical mapping of Mars by the Observatoire pour la Mineralogie, l'Eau, les Glaces et l'Activite (OMEGA) instrument on the European Space Agency's Mars Express spacecraft provides new information on Mars' geological and climatic history. Phyllosilicates formed by aqueous alteration very early in the planet's history (the "phyllocian" era) are found in the oldest terrains; sulfates were formed in a second era (the "theiikian" era) in an acidic environment. Beginning about 3.5 billion years ago, the last era (the "siderikian") is dominated by the formation of anhydrous ferric oxides in a slow superficial weathering, without liquid water playing a major role across the planet.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Bibring, Jean-Pierre -- Langevin, Yves -- Mustard, John F -- Poulet, Francois -- Arvidson, Raymond -- Gendrin, Aline -- Gondet, Brigitte -- Mangold, Nicolas -- Pinet, P -- Forget, F -- Berthe, Michel -- Gomez, Cecile -- Jouglet, Denis -- Soufflot, Alain -- Vincendon, Mathieu -- Combes, Michel -- Drossart, Pierre -- Encrenaz, Therese -- Fouchet, Thierry -- Merchiorri, Riccardo -- Belluci, Giancarlo -- Altieri, Francesca -- Formisano, Vittorio -- Capaccioni, Fabricio -- Cerroni, Pricilla -- Coradini, Angioletta -- Fonti, Sergio -- Korablev, Oleg -- Kottsov, Volodia -- Ignatiev, Nikolai -- Moroz, Vassili -- Titov, Dimitri -- Zasova, Ludmilla -- Loiseau, Damien -- Pinet, Patrick -- Doute, Sylvain -- Schmitt, Bernard -- Sotin, Christophe -- Hauber, Ernst -- Hoffmann, Harald -- Jaumann, Ralf -- Keller, Uwe -- Arvidson, Ray -- Duxbury, Tom -- Forget, Francois -- Neukum, G -- New York, N.Y. -- Science. 2006 Apr 21;312(5772):400-4.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Institut d'Astrophysique Spatiale (IAS), Batiment 121, 91405 Orsay Campus, France.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/16627738" target="_blank"〉PubMed〈/a〉
    Keywords: Aluminum Silicates ; Atmosphere ; Carbon Dioxide ; Extraterrestrial Environment ; Ferric Compounds ; *Mars ; *Minerals ; Silicates ; Sulfates ; Time ; *Water
    Print ISSN: 0036-8075
    Electronic ISSN: 1095-9203
    Topics: Biology , Chemistry and Pharmacology , Computer Science , Medicine , Natural Sciences in General , Physics
    Location Call Number Expected Availability
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