Global mineralogical and aqueous mars history derived from OMEGA/Mars express data

被引:1238
作者
Bibring, JP
Langevin, Y
Mustard, JF
Poulet, F
Arvidson, R
Gendrin, A
Gondet, B
Mangold, N
Pinet, P
Forget, F
机构
[1] Inst Astrophys Spatiale, F-91405 Orsay, France
[2] Brown Univ, Dept Geol Sci, Providence, RI 02912 USA
[3] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[4] Interact & Dynam Environm Surface, F-91405 Orsay, France
[5] Observ Midi Pyrenees, F-31400 Toulouse, France
[6] Univ Paris 06, Meteorol Dynam Lab, Paris, France
关键词
D O I
10.1126/science.1122659
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
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.
引用
收藏
页码:400 / 404
页数:5
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