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      Igneous mineralogy at Bradbury Rise: The first ChemCam campaign at Gale crater : IGNEOUS MINERALOGY AT BRADBURY RISE

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          The operated Markov´s chains in economy (discrete chains of Markov with the income)

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            Mars Science Laboratory Mission and Science Investigation

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              Martian fluvial conglomerates at Gale crater.

              Observations by the Mars Science Laboratory Mast Camera (Mastcam) in Gale crater reveal isolated outcrops of cemented pebbles (2 to 40 millimeters in diameter) and sand grains with textures typical of fluvial sedimentary conglomerates. Rounded pebbles in the conglomerates indicate substantial fluvial abrasion. ChemCam emission spectra at one outcrop show a predominantly feldspathic composition, consistent with minimal aqueous alteration of sediments. Sediment was mobilized in ancient water flows that likely exceeded the threshold conditions (depth 0.03 to 0.9 meter, average velocity 0.20 to 0.75 meter per second) required to transport the pebbles. Climate conditions at the time sediment was transported must have differed substantially from the cold, hyper-arid modern environment to permit aqueous flows across several kilometers.
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                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res. Planets
                Wiley
                21699097
                January 2014
                January 2014
                January 08 2014
                : 119
                : 1
                : 30-46
                Affiliations
                [1 ]LMCM; UMR-CNRS 7202, MNHN; Paris France
                [2 ]CNRS-UMR 7359 GeoRessources; Universite de Lorraine; Nancy France
                [3 ]CNRS-UMR 7277 IRAP; Universite de Toulouse; Toulouse France
                [4 ]Los Alamos National Laboratory; Los Alamos New Mexico USA
                [5 ]Institute of Meteoritics; University of New Mexico; Albuquerque New Mexico USA
                [6 ]CNRS-UMR 6112; LPG Nantes; Nantes France
                [7 ]U.S. Geological Survey; Flagstaff Arizona USA
                [8 ]CNRS-UMR 5275; ISTerre, Universite de Grenoble; Grenoble France
                [9 ]Department of Earth Sciences; Brock University; St. Catharines Ontario Canada
                [10 ]Department of Astronomy; Mount Holyoke College; South Hadley Massachusetts USA
                [11 ]Division of Geological and Planetary Sciences; California Institute of Technology; Pasadena California USA
                [12 ]SRC; University of Leicester; Leicester UK
                [13 ]Space Science Institute; Boulder Colorado USA
                Article
                10.1002/2013JE004472
                aabbcbfe-c01a-4c01-85c0-2225f55a4e5e
                © 2014

                http://doi.wiley.com/10.1002/tdm_license_1.1

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