A Mapping of Martian Water Vapor using OMEGA/Mars Express

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

The OMEGA imaging spectrometer aboard the Mars Express orbiter has been used to map the water vapor abundance over the martian surface, from the analysis of the 2.6-micron band of H2O. The study of this band, in the reflected sunlight range, allows a determination of the water vapor abundance which is, to first order, independent of the temperature profile. As a first result of this study, we present water vapor maps in the northern hemisphere at the time of the norther polar cap sublimation (Ls = 90-115 deg.),when the water vapor column density is maximum. Our measurements are compared with previous results by MAWD/Viking and TES/MGS. The authors acknowledge support from the Centre National de la Recherche Scientifique (CNRS) and from the Centre National d'Etudes Spatiales (CNES).

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