A Model Scenario for Kieserite-Dominated Evaporites in Juventae Chasma, Mars

Details A Model Scenario for Kieserite-Dominated Evaporites in Juventae Chasma, Mars A Model Scenario for Kieserite-Dominated Evaporites in Juventae Chasma, Mars

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2453a&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2453

Computer Science

Scientific paper

Taking evaporation as a prerequisite, we measured the "stairstep"
morphology and the volume of mound B to model the mineral assamblage to
reconstruct the amount of water needed to form mound B in its
composition as measured by CRISM and OMEGA.

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