Constraints on the Stabilities of Observed Martian Secondary Mineral Phases from Geothermal Gradient Models

Details Constraints on the Stabilities of Observed Martian Secondary Mineral Phases from Geothermal Gradient Models Constraints on the Stabilities of Observed Martian Secondary Mineral Phases from Geothermal Gradient Models

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2340h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2340

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Scientific paper

We attempt to place thermal constraints on the stability of exposed
secondary mineral phases on Mars based on heat flow and geothermal
gradients modeled at the time of mineral formation and burial.

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