Deciphering the Hydration State of the Martian Surface from Near-Infrared Spectroscopy

Details Deciphering the Hydration State of the Martian Surface from Near-Infrared Spectroscopy Deciphering the Hydration State of the Martian Surface from Near-Infrared Spectroscopy

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1890p&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1890

Computer Science

1

Scientific paper

We characterize the hydration state of Mars’ surface through
comparison between laboratory simulations and remote-sensing data. The
relative strength of the 1.9- and 3-µm features indicates the
presence of an hydroxylated phase in the surface dust.

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