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  • 1
    Publication Date: 2005-02-01
    Description: We detected light emissions in the nightside martian atmosphere with the SPICAM (spectroscopy for the investigation of the characteristics of the atmosphere of Mars) ultraviolet (UV) spectrometer on board the Mars Express. The UV spectrum of this nightglow is composed of hydrogen Lyman alpha emission (121.6 nanometers) and the gamma and delta bands of nitric oxide (NO) (190 to 270 nanometers) produced when N and O atoms combine to produce the NO molecule. N and O atoms are produced by extreme UV photodissociation of O2, CO2, and N2 in the dayside upper atmosphere and transported to the night side. The NO emission is brightest in the winter south polar night because of continuous downward transport of air in this region at night during winter and because of freezing at ground level.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Bertaux, Jean-Loup -- Leblanc, Francois -- Perrier, Severine -- Quemerais, E -- Korablev, Oleg -- Dimarellis, E -- Reberac, A -- Forget, F -- Simon, P C -- Stern, S A -- Sandel, Bill -- SPICAM Team -- New York, N.Y. -- Science. 2005 Jan 28;307(5709):566-9.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Service d'Aeronomie du CNRS/Institut Pierre-Simon Laplace (IPSL), BP.3, 91371, Verrieres-le-Buisson, France. bertaux@aerov.jussieu.fr〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15681381" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; Carbon Dioxide ; Extraterrestrial Environment ; Hydrogen ; *Mars ; *Nitric Oxide ; Nitrogen ; Oxygen ; Seasons ; Spacecraft ; Spectrophotometry, Ultraviolet ; Temperature ; Ultraviolet Rays
    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
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  • 3
    Publication Date: 2011-10-01
    Description: The vertical distribution of water vapor is key to the study of Mars' hydrological cycle. To date, it has been explored mainly through global climate models because of a lack of direct measurements. However, these models assume the absence of supersaturation in the atmosphere of Mars. Here, we report observations made using the SPICAM (Spectroscopy for the Investigation of the Characteristics of the Atmosphere of Mars) instrument onboard Mars Express that provide evidence of the frequent presence of water vapor in excess of saturation, by an amount far surpassing that encountered in Earth's atmosphere. This result contradicts the widespread assumption that atmospheric water on Mars cannot exist in a supersaturated state, directly affecting our long-term representation of water transport, accumulation, escape, and chemistry on a global scale.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Maltagliati, L -- Montmessin, F -- Fedorova, A -- Korablev, O -- Forget, F -- Bertaux, J-L -- New York, N.Y. -- Science. 2011 Sep 30;333(6051):1868-71. doi: 10.1126/science.1207957.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Laboratoire Atmospheres, Milieux, Observations Spatiales (LATMOS), 78280 Guyancourt, France. luca.maltagliati@latmos.ipsl.fr〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/21960630" target="_blank"〉PubMed〈/a〉
    Keywords: Atmosphere ; Extraterrestrial Environment ; *Mars ; Spacecraft ; Spectrum Analysis ; *Steam
    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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