Global Mineralogical and Aqueous Mars History Derived from OMEGA/Mars Express Data
Brown University · Laboratoire de Tribologie et Dynamique des Systèmes · +5 more institutions
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.
Citation impact
- FWCI
- 50.99
- Percentile
- 100%
- References
- 27
Authors
52- JBJean‐Pierre BibringCorresponding
Brown University, Laboratoire de Tribologie et Dynamique des Systèmes, Institut d'Astrophysique Spatiale, Observatoire Midi-Pyrénées
- YLYves Langevin
Brown University, Laboratoire de Tribologie et Dynamique des Systèmes, Institut d'Astrophysique Spatiale, Observatoire Midi-Pyrénées
- JFJohn F. Mustard
Brown University, Laboratoire de Tribologie et Dynamique des Systèmes, Institut d'Astrophysique Spatiale, Observatoire Midi-Pyrénées
- FPF. Poulet
Brown University, Laboratoire de Tribologie et Dynamique des Systèmes, Institut d'Astrophysique Spatiale, Observatoire Midi-Pyrénées
- RER. E. Arvidson
Washington University in St. Louis, Brown University, Laboratoire de Tribologie et Dynamique des Systèmes, Institut d'Astrophysique Spatiale, Observatoire Midi-Pyrénées
Topics & keywords
- Mars Exploration Program
- Astrobiology
- Weathering
- Geology
- Geochemistry
- Planet
- Physics