Mineralogy and Stratigraphy of Light Toned Deposits in Ophir Chasma, Mars

Details Mineralogy and Stratigraphy of Light Toned Deposits in Ophir Chasma, Mars Mineralogy and Stratigraphy of Light Toned Deposits in Ophir Chasma, Mars

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..491w&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.491

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Scientific paper

We studied the mineralogy, geomorphology and layering attitude of Light Toned Deposits (LTD) in Ophir Chasma, Mars, using visible and short wave infrared data (SWIR) from the imaging spectrometers OMEGA and CRISM together with panchromatic and color imagery, digital elevation models and anaglyphs from HRSC, Themis, CTX, MOC and HiRISE. Previous investigations of the light-toned deposits (LTD) in Valles Marineris on the regional scale based SWIR data from OMEGA or CRISM include [1,2]. Thermal infrared data from TES [3] was used by [4]. LTDs in other chasms have been investigated in detail by [5-12].

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