T94 Mineralogy of Diagenesis on Earth and Mars: In Honor of Nicholas J. Tosca, 2015 MSA Awardee
Monday, 2 November 2015
8:00 AM - 12:00 PM
Room 342
IN-SITU EVIDENCE FOR ALTERATION BY ACID FOG ON HUSBAND HILL, GUSEV CRATER, MARS
Paper number: T94-11
Program: Technical Sessions
Time: 10:40 AM – 10:55 AM
Authors
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Benton ClarkSpace Science Institute, Boulder, CO
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William FarrandSpace Science Institute, Boulder, CO
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Ken HerkenhoffUS Geological Survey, Flagstaff, AZ
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Richard V. MorrisNASA Johnson Space Center, Houston, TX
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Steven RuffArizona State University, Tempe, AZ
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Steven W. SquyresCornell University, Ithaca, NY
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R. YingstPlanetary Science Institute, Brunswick, ME
Abstract
The Mars Exploration Rover Spirit observed evidence of this process in the Columbia Hills of Gusev Crater. Spirit examined a set of geochemically similar but mineralogically distinct outcrops on Cumberland Ridge and the Husband Hill summit. The iron oxidation state (Fe3+/Fetotal) of the “Watchtower Class” exposures on Cumberland Ridge range from 0.43 to 0.94, across a distance of only ~30m. The outcrops’ microtextures exhibit knobby protuberances, whose size correlates directly with the iron oxidation state and abundance of nanophase Fe3+ oxides as measured by the Mössbauer Spectrometer, and the abundance of amorphous phases modeled through the deconvolution of Mini-TES thermal emission spectra. We propose that the knobby protuberances are agglomerations of preexisting grains, formed from the interaction of acid fog and the host rock. In this alteration scenario, acid fog condensed on the outcrop surfaces, dissolving material at the condensation-surface interface and forming a gel, which desiccated as the adsorbed water evaporated. Differences in condensation residence time, due to amount of insolation and/or winds, resulted in the oxidative, mineralogical, and microtextural variations Spirit observed on these targets.