火星探测计划
地质学
绕极星
极地的
石膏
火星人
天体生物学
地形
矿物学
地貌学
古生物学
海洋学
地理
物理
天文
地图学
作者
Y. Langevin,F. Poulet,Jean‐Pierre Bibring,B. Gondet
出处
期刊:Science
[American Association for the Advancement of Science (AAAS)]
日期:2005-02-18
卷期号:307 (5715): 1584-1586
被引量:498
标识
DOI:10.1126/science.1109091
摘要
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.
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