Detection and stratigraphic mapping of spectrally distinct hydrated layers in equatorial regions of Mars

Details Detection and stratigraphic mapping of spectrally distinct hydrated layers in equatorial regions of Mars Detection and stratigraphic mapping of spectrally distinct hydrated layers in equatorial regions of Mars

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1255s&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1255

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We demonstrate the use of spectral and topographic data to map spectrally distinct rock units spatially, in elevation and in stratigraphy. Using hyperspectral data from NASA's CRISM and stereo-derived topographic data from ESA's HRSC we present the first results of a project to map geologic units containing hydrated minerals in equatorial regions of Mars (e.g. Valles Marineris, Xanthe Terra and Margaritifer Terra) and to correlate their stratigraphic position with existing formation theories.

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