Title of article :
Coordinated analyses of Antarctic sediments as Mars analog materials using reflectance spectroscopy and current flight-like instruments for CheMin, SAM and MOMA
Author/Authors :
Bishop، نويسنده , , Janice L. and Franz، نويسنده , , Heather B. and Goetz، نويسنده , , Walter and Blake، نويسنده , , David F. and Freissinet، نويسنده , , Caroline and Steininger، نويسنده , , Harald and Goesmann، نويسنده , , Fred and Brinckerhoff، نويسنده , , William B. and Getty، نويسنده , , Stephanie and Pinnick، نويسنده , , Veronica T. and Mahaffy، نويسنده , , Paul R. and Dyar، نويسنده , , M. D، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2013
Pages :
17
From page :
309
To page :
325
Abstract :
Coordinated analyses of mineralogy and chemistry of sediments from the Antarctic Dry Valleys illustrate how data obtained using flight-ready technology of current NASA and ESA missions can be combined for greater understanding of the samples. Mineralogy was measured by X-ray diffraction (XRD) and visible/near-infrared (VNIR) reflectance spectroscopy. Chemical analyses utilized a quadrupole mass spectrometer (QMS) to perform pyrolysis-evolved gas analysis (EGA) and gas chromatography–mass spectrometry (GC/MS) both with and without derivatization, as well as laser desorption–mass spectrometry (LD/MS) techniques. These analyses are designed to demonstrate some of the capabilities of near-term landed Mars missions, to provide ground truthing of VNIR reflectance data acquired from orbit by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on MRO and to provide detection limits for surface-operated instruments: the Chemistry and Mineralogy (CheMin) and Sample Analysis at Mars (SAM) instrument suites onboard Mars Science Laboratory (MSL) and the Mars Organic Molecule Analyzer (MOMA) onboard ExoMars-2018. The new data from this study are compared with previous analyses of the sediments performed with other techniques. Tremolite was found in the oxic region samples for the first time using the CheMin-like XRD instrument. The NIR spectral features of tremolite are consistent with those observed in these samples. Although the tremolite bands are weak in spectra of these samples, spectral features near 2.32 and 2.39 μm could be detected by CRISM if tremolite is present on the martian surface. Allophane was found to be a good match to weak NIR features at ∼1.37–1.41, 1.92, and 2.19 μm in spectra of the oxic region sediments and is a common component of immature volcanic soils. Biogenic methane was found to be associated with calcite in the oxic region samples by the SAM/EGA instrument and a phosphoric acid derivative was found in the anoxic region sample using the SAM/MTBSTFA technique.
Keywords :
Mars , Surface , Mineralogy , organic chemistry , Spectroscopy
Journal title :
Icarus
Serial Year :
2013
Journal title :
Icarus
Record number :
2379887
Link To Document :
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