The H2O Sorption Properties of a Martian Dust Analog

Details The H2O Sorption Properties of a Martian Dust Analog The H2O Sorption Properties of a Martian Dust Analog

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.1395j&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

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Scientific paper

Palagonitic dust is a geologically reasonable hydrated phase on the
surface of Mars. Its presence as dust may account for the presence of
the 3 μm absorption band as seen by OMEGA and CRISM at the martian
surface for the entire planet.

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