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Submitted on December 16, 2004
Accepted on February 9, 2005
Mars Surface Diversity as Revealed by the OMEGA/Mars Express Observations
Jean-Pierre Bibring 1*, Yves Langevin 1, Aline Gendrin 1, Brigitte Gondet 1, François Poulet 1, Michel Berthé 1, Alain Soufflot 1, Ray Arvidson 2, Nicolas Mangold 3, John Mustard 4, Pierre Drossart 5, Michel Berthé 6, Jean-Pierre Bibring 6, Stéphane Erard 6, Olivier Forni 6, Aline Gendrin 6, Brigitte Gondet 6, François Poulet 6, Alain Soufflot 6, Michel Combes 5, Pierre Drossart 5, Thérèse Encrenaz 5, Thierry Fouchet 5, Riccardo Merchiorri 5, GianCarlo Belluci 3, Francesca Altieri 3, Vittorio Formisano 3, Guillaume Bonello 7, Fabricio Capaccioni 7, Pricilla Cerroni 7, Angioletta Coradini 7, Sergio Fonti 8, Volodia Kottsov 9, Nikolai Ignatiev 9, Vassili Moroz 9, Dimitri Titov 9, Ludmilla Zasova 9, Nicolas Mangold 10, Patrick Pinet 11, Sylvain Douté 12, Bernard Schmitt 12, Christophe Sotin 13, Ernst Hauber 14, Harald Hoffmann 14, Ralf Jaumann 14, Uwe Keller 15, Ray Arvidson 16, Jack Mustard 17, Tom Duxbury 18, François Forget 19
1 Institut d'Astrophysique Spatiale, Bâtiment 121, 91405 Orsay Campus, France. 2 Earth and Planetary Sciences, Washington University, St Louis, Missouri 63130, USA. 3 IDES, Bâtiment 509, 91405 Orsay Campus, France. 4 Geological Sciences, Brown University, Providence, Rhode Island 02912, USA. 5 LESIA, Observatoire de Paris, Meudon, France. 6 IAS, Orsay Campus, France. 7 IAS-INAF, Rome, Italy. 8 University of Lecce, Italy, Italy. 9 IKI, Moscow, Russia. 10 IDES, Orsay Campus, France. 11 Observatoire Midi-Pyrénées, Toulouse, France. 12 Laboratoire de Planétologie, Grenoble, France. 13 Planétologie, Université de Nantes, France. 14 DLR, Berlin, Germany. 15 MPAE, Lindau, Germany. 16 Earth and Planetary Sciences, Washington University, Saint-Louis, Missouri, USA. 17 Geological Sciences, Brown University, Providence, RI, USA. 18 JPL, Pasadena, California, USA. 19 LMD, Université Paris 6, Paris, France.
The OMEGA investigation, on board the ESA/Mars Express mission,is mapping the surface composition of Mars, at a 0.3 to 5 kmresolution, by means of VIS-NIR hyperspectral reflectance imagery.The data acquired during the first nine months of the missionalready reveal a diverse and complex surface mineralogy, offeringkey insights to the evolution of Mars. OMEGA has identifiedand mapped mafic iron-bearing silicates of both the northernand southern crust; localized concentrations of hydrated phyllosilicatesand sulfates, and no carbonates; ices and frosts, with a water-icecomposition of the north polar perennial cap, as for the southcap, covered by a thin CO2 - ice veneer.
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