Clay mineral diversity and abundance in sedimentary rocks of Gale crater, Mars
Résumé
Clay minerals provide indicators of the evolution of aqueous conditions and possible habitats for life on ancient
Mars. Analyses by the Mars Science Laboratory rover Curiosity show that ~3.5–billion year (Ga) fluvio-lacustrine
mudstones in Gale crater contain up to ~28 weight % (wt %) clay minerals. We demonstrate that the species of clay
minerals deduced from x-ray diffraction and evolved gas analysis show a strong paleoenvironmental dependency.
While perennial lake mudstones are characterized by Fe-saponite, we find that stratigraphic intervals associated
with episodic lake drying contain Al-rich, Fe3+-bearing dioctahedral smectite, with minor (3 wt %) quantities of
ferripyrophyllite, interpreted as wind-blown detritus, found in candidate aeolian deposits. Our results suggest that
dioctahedral smectite formed via near-surface chemical weathering driven by fluctuations in lake level and atmospheric
infiltration, a process leading to the redistribution of nutrients and potentially influencing the cycling of
gases that help regulate climate.
Domaines
Planétologie
Origine : Fichiers produits par l'(les) auteur(s)
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