Water-of-Hydration Near-IR Bands on Mars: Distinguishing Between the Effects of Hydration State and Surface Texture using OMEGA and TES Datasets

Details Water-of-Hydration Near-IR Bands on Mars: Distinguishing Between the Effects of Hydration State and Surface Texture using OMEGA and TES Datasets Water-of-Hydration Near-IR Bands on Mars: Distinguishing Between the Effects of Hydration State and Surface Texture using OMEGA and TES Datasets

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1861p&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Physics

Scientific paper

We analyze the origins of the 3 µm water-of-hydration band
strength spatial variations on the martian surface to discriminate the
effects of albedo, particle size and hydration state variations.

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