High manganese concentrations in rocks at Gale crater, Mars
Résumé
The surface of Mars has long been considered a relatively oxidizing environment, an idea
supported by the abundance of ferric iron phases observed there. However, compared to iron, manganese
is sensitive only to high redox potential oxidants, and when concentrated in rocks, it provides a more specific
redox indicator of aqueous environments. Observations from the ChemCam instrument on the Curiosity
rover indicate abundances of manganese in and on some rock targets that are 1–2 orders of magnitude
higher than previously observed on Mars, suggesting the presence of an as-yet unidentified manganese-rich
phase. These results show that the Martian surface has at some point in time hosted much more highly
oxidizing conditions than has previously been recognized
Domaines
Planète et Univers [physics]
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