Hydrothermal Alteration in a Late Hesperian Impact Crater on Mars

Details Hydrothermal Alteration in a Late Hesperian Impact Crater on Mars Hydrothermal Alteration in a Late Hesperian Impact Crater on Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1209m&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1209

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Scientific paper

The 45-km-diameter Majuro Crater shows an alluvial fan containing
phyllosilicates. Observations suggest alteration occurred during the
Hesperian by hydrothermal circulation due to the impact heat coupled to
snow precipitation.

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