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
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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