Water-of-Hydration Near-IR Bands on Mars: Distinguishing Between the Effects of Hydration State and Surface Texture using OMEGA and TES Datasets - INSU - Institut national des sciences de l'Univers Access content directly
Conference Papers Year : 2008

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

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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Dates and versions

insu-00361641 , version 1 (16-02-2009)

Identifiers

  • HAL Id : insu-00361641 , version 1

Cite

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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