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

Antoine Pommerol 1 Bernard Schmitt 1 The Omega Team
1 LPG - Laboratoire de Planétologie de Grenoble
Abstract : 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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Conference papers
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https://hal-insu.archives-ouvertes.fr/insu-00361641
Contributor : Béatrice Pibaret-Bourdon Connect in order to contact the contributor
Submitted on : Monday, February 16, 2009 - 12:05:33 PM
Last modification on : Tuesday, October 19, 2021 - 6:58:02 PM

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  • HAL Id : insu-00361641, version 1

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Antoine Pommerol, Bernard Schmitt, The Omega Team. Water-of-Hydration Near-IR Bands on Mars: Distinguishing Between the Effects of Hydration State and Surface Texture using OMEGA and TES Datasets. 39th Lunar and Planetary Science Conference, Mar 2008, League City, Texas, United States. pp.1861. ⟨insu-00361641⟩

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