Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data
550
SURFACE
Extraterrestrial Environment
SPIRIT ROVER
DIVERSITY
Mars
GUSEV CRATER
DUST
551
Ferric Compounds
01 natural sciences
Time
[SDU] Sciences of the Universe [physics]
MERIDIANI
0103 physical sciences
Mars Express
Minerals
Omega
IDENTIFICATION
Atmosphere
Sulfates
Silicates
Water
Carbon Dioxide
15. Life on land
Phyllosilicates
EVOLUTION
CLIMATE
[SDU]Sciences of the Universe [physics]
13. Climate action
Clay
Aluminum Silicates
CRUST
DOI:
10.1126/science.1122659
Publication Date:
2006-04-21T22:24:13Z
AUTHORS (52)
ABSTRACT
Global mineralogical mapping of Mars by the Observatoire pour la Mineralogie, l'Eau, les Glaces et l'Activité (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.
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