A large diversity of hydrated minerals formed from interaction with hydrothermal fluids in Noctis Labyrinthus, Mars.

Details A large diversity of hydrated minerals formed from interaction with hydrothermal fluids in Noctis Labyrinthus, Mars. A large diversity of hydrated minerals formed from interaction with hydrothermal fluids in Noctis Labyrinthus, Mars.

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1067t&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1067

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The processes that formed hydrated minerals on Mars remain unconstrained. A suite of minerals including all mineralogical classes known on Mars (clays, sulfates and oxides) has been identified in Noctis Labyrinthus. The particular mineralogical association and proximity to settings of volcanic activity suggests coeval formation in a unique local hydrothermal environment.

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