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      Martian aeolian activity at the Bagnold Dunes, Gale Crater: The view from the surface and orbit : Aeolian Activity at the Bagnold Dunes

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

          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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            Mars Reconnaissance Orbiter's High Resolution Imaging Science Experiment (HiRISE)

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              Mars Global Surveyor Thermal Emission Spectrometer experiment: Investigation description and surface science results

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                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res. Planets
                Wiley-Blackwell
                21699097
                October 2017
                October 2017
                : 122
                : 10
                : 2077-2110
                Article
                10.1002/2017JE005263
                b302d27e-9492-4188-acb9-a4cb10f2c006
                © 2017

                http://doi.wiley.com/10.1002/tdm_license_1.1

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