T111 When Water Meets Rock: Aqueous Alteration in the Solar System I
Monday, 20 October 2014
8:00 AM - 12:00 PM
301
INTERPRETING AQUEOUS ALTERATION ON EARTH AND ON MARS USING FIELD ANALYSES, LABORATORY EXPERIMENTS, AND MODELING
Paper number: T111-4
Program: Technical Sessions
Time: 8:50 AM – 9:10 AM
Authors
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Seth R. GaineyUniversity of Nevada, Las Vegas, Las Vegas, NV
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Michael H. SteinerUniversity of Nevada, Las Vegas, Las Vegas, NV
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Renee E. SchofieldUniversity of Nevada, Las Vegas, Las Vegas, NV
Abstract
Here we are using a combination of laboratory synthesis and dissolution experiments and reactive transport modeling to interpret the origin of Mawrth Vallis. Mawrth Vallis is one of many locations on Mars in which a sequence of Al-rich clay minerals overlies Fe, Mg-rich clay minerals, and possible formation mechanisms include weathering or a change in environmental conditions such as oxidation state. Dissolution experiments indicate that nontronite dissolves more rapidly than montmorillonite and kaolinite under very acidic conditions, suggesting that a mixture of these minerals would become enriched in montmorillonite and kaolinite over geological time. Dissolution of nontronite in brines occurs much more slowly than in dilute solutions, and reactive transport modeling of clay minerals relevant to Mawrth Vallis indicates the mineral sequences that occur and the duration of time required. Synthesis experiments indicate the importance of conditions such as oxidation state, pH, and water: rock ratio of reacting solutions to secondary mineral formation.