Mineralogical and Geochemical Trends of the Murray Mudstones, Gale Crater: A Combined Sample Analysis at Mars-Evolved Gas Analyzer and Chemistry and Mineralogy Instrument Assessment

Sutter, B ; McAdam, A C ; Rampe, E B ; Archer, P D ; Ming, D W ; Mahaffy, P R ; Navarro-Gonzalez, R ; Stern, J C ; Eigenbrode, J L ; Franz,H B

关键词: MINERALOGY;    GEOCHEMISTRY;    MONTMORILLONITE;    MARS CRATERS;    METEORITE CRATERS;    MARS SURFACE;    CHEMICAL ANALYSIS;    GAS DETECTORS;    HEMATITE;    MAGNETITE;    GAS ANALYSIS;    MARS SCIENCE LABORATORY;    CURIOSITY ROVER;    IRON;    SULFUR;   

RP-ID  :  JSC-E-DAA-TN64825

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来源: NASA Technical Reports Server

【 摘 要 】

The Murray formation is predominantly composed of lacustrine mudstone that forms the basal layer of Aeolis Mons (informally Mt. Sharp) in Gale Crater, Mars. The Murray formation has distinct iron and sulfur mineralogical variation within its stratigraphy detectable by the Chemistry Mineralogy (Che-Min) instrument consisting of magnetite/hematite in the lower Murray and higher hematite, CaSO4, and smectite content in the upper Murray. The objectives of this work were to evaluate the Sample Analysis at Mars Evolved Gas Analyzer (SAM-EGA) data to 1) Determine what SAM-EGA-detectable phases correlate or do not correlate with the Murray mineralogical composition detected by CheMin and 2) Utilize CheMin/SAM results to propose possible formation scenarios for the observed Murray mudstone mineralogy.