Sulfates in the North Polar Region of Mars Detected by OMEGA/Mars Express

The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) imaging spectrometer observed the northern circumpolar regions of Mars at a resolution of a few kilometers. An extended region at 240°E, 85°N, with an area of 60 kilometers by 200 kilometers, exhibits absorpti...

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Veröffentlicht in:Science (American Association for the Advancement of Science) 2005-03, Vol.307 (5715), p.1584-1586
Hauptverfasser: Langevin, Yves, Poulet, François, Bibring, Jean-Pierre, Gondet, Brigitte
Format: Artikel
Sprache:eng
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Zusammenfassung:The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) imaging spectrometer observed the northern circumpolar regions of Mars at a resolution of a few kilometers. An extended region at 240°E, 85°N, with an area of 60 kilometers by 200 kilometers, exhibits absorptions at wavelengths of 1.45, 1.75, 1.94, 2.22, 2.26, and 2.48 micrometers. These signatures can be unambiguously attributed to calcium-rich sulfates, most likely gypsum. This region corresponds to the dark longitudinal dunes of Olympia Planitia. These observations reveal that water alteration played a major role in the formation of the constituting minerals of northern circumpolar terrains.
ISSN:0036-8075
1095-9203
DOI:10.1126/science.1109091