Examinando por Autor "House, C. H."

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Acceso Abierto
Detection of Reduced Sulfur on Vera Rubin Ridge by Quadratic Discriminant Analysis of Volatiles Observed During Evolved Gas Analysis.
(American Geophysical Union: Advancing Earth and Space Science, 2020-06-10) Wong, K. H.; Lewis, J.; Knudson, C. A.; Millan, M.; McAdam, A. C.; Eigenbrode, J. L.; Andrejkovičová, S.; Gómez, F.; Navarro González, R.; House, C. H.; Universidad Nacional Autónoma de México (UNAM); Navarro González, R. [0000-0002-6078-7621]; Knudson, C. A. [0000-0003-3875-2200]; Andrejkovicova, S. [0000-0001-8429-6926]; Gómez, F. [0000-0001-9977-7060]; McAdam, A. [0000-0001-9120-2991]; House, C. [0000-0002-4926-4985]; Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
The Mars Science Laboratory mission investigated Vera Rubin ridge, which bears spectral indications of elevated amounts of hematite and has been hypothesized as having a complex diagenetic history. Martian samples, including three drilled samples from the ridge, were analyzed by the Sample Analysis at Mars instrument suite via evolved gas analysis‐mass spectrometry (EGA‐MS). Here, we report new EGA‐MS data from Martian samples and describe laboratory analogue experiments. Analyses of laboratory analogues help determine the presence of reduced sulfur in Martian solid samples, which could have supported potential microbial life. We used evolved carbonyl sulfide (COS) and carbon disulfide (CS2) to identify Martian samples likely to contain reduced sulfur by applying a quadratic discriminant analysis. While we report results for 24 Martian samples, we focus on Vera Rubin ridge samples and select others for comparison. Our results suggest the presence of reduced sulfur in the Jura member of Vera Rubin ridge, which can support various diagenetic history models, including, as discussed in this work, diagenetic alteration initiated by a mildly reducing, sulfite‐containing groundwater.
Acceso Abierto
Extraformational sediment recycling on Mars
(Geo Science World, 2020-10-06) Edgett, K. S.; Branham, S. G.; Bennett, A.; Edgard, L. A.; Edwards, C. S.; Fairén, A.; Fedo, C. M.; Fey, D. M.; Garvin, J. B.; Grotzinger, J. P.; Gupta, S.; Henderson, M. J.; House, C. H.; Mangold, N.; McLennan, S. M.; Newsom, H. E.; Rowland, S. K.; Siebach, K. L.; Thompson, L.; Van Bommel, S. J.; Wiens, R. C.; Williams, R. M. E.; Yingst, R. A.; European Research Council (ERC); 0000-0003-1206-1639; 0000-0001-6415-1332; 0000-0001-7197-5751; Unidad de Excelencia Científica María de Maeztu Centro de Astrobiología del Instituto Nacional de Técnica Aeroespacial y CSIC, MDM-2017-0737
Extraformational sediment recycling (old sedimentary rock to new sedimentary rock) is a fundamental aspect of Earth’s geological record; tectonism exposes sedimentary rock, whereupon it is weathered and eroded to form new sediment that later becomes lithified. On Mars, tectonism has been minor, but two decades of orbiter instrument–based studies show that some sedimentary rocks previously buried to depths of kilometers have been exposed, by erosion, at the surface. Four locations in Gale crater, explored using the National Aeronautics and Space Administration’s Curiosity rover, exhibit sedimentary lithoclasts in sedimentary rock: At Marias Pass, they are mudstone fragments in sandstone derived from strata below an erosional unconformity; at Bimbe, they are pebble-sized sandstone and, possibly, laminated, intraclast-bearing, chemical (calcium sulfate) sediment fragments in conglomerates; at Cooperstown, they are pebble-sized fragments of sandstone within coarse sandstone; at Dingo Gap, they are cobble-sized, stratified sandstone fragments in conglomerate derived from an immediately underlying sandstone. Mars orbiter images show lithified sediment fans at the termini of canyons that incise sedimentary rock in Gale crater; these, too, consist of recycled, extraformational sediment. The recycled sediments in Gale crater are compositionally immature, indicating the dominance of physical weathering processes during the second known cycle. The observations at Marias Pass indicate that sediment eroded and removed from craters such as Gale crater during the Martian Hesperian Period could have been recycled to form new rock elsewhere. Our results permit prediction that lithified deltaic sediments at the Perseverance (landing in 2021) and Rosalind Franklin (landing in 2023) rover field sites could contain extraformational recycled sediment.