A mapping of martian water sublimation during early northern summer using OMEGA/Mars Express

Thérèse Encrenaz (1, 2, 3) , Riccardo Melchiorri (1, 2, 3) , Thierry Fouchet (1, 2, 3) , Pierre Drossart (1, 2, 3) , Emmanuel Lellouch (1, 2, 3) , Brigitte Gondet (4) , Jean-Pierre Bibring (4) , Yves Langevin (4) , Dmitry V. Titov (5) , Nikolai Ignatiev (6) , François Forget (7)

1 LESIA - Laboratoire d'études spatiales et d'instrumentation en astrophysique
2 Ingénieurs, Techniciens et Administratifs
3 Pôle Planétologie du LESIA
4 IAS - Institut d'astrophysique spatiale
5 MPI - Max Planck Institute
6 IKI - Space Research Institute of the Russian Academy of Sciences
7 LMD - Laboratoire de Météorologie Dynamique (UMR 8539)

The OMEGA imaging spectrometer aboard Mars Express has been used to map the water vapor abundance over the martian surface, from the analysis of the 2.6 mum band of H2O. As a preliminary result of this study, we present water vapor maps in the northern hemisphere at the time of the northern polar cap sublimation (Ls = 94-112 deg). The maps show a mean H2O mixing ratio of about 2-3× 10^-4 at a latitude of 40N, and in the range of 5 × 10^-4-10^-3 at 60N-80N latitudes. The corresponding mean H2O column densities are about 25 pr-mum at 40N and between 40 and 60 pr-mum at 60N-80N, with uncertainties of about 30 percent. Our results are in agreement with previous results by MAWD/Viking and TES/MGS for latitudes up to 60N, but seem to indicate lower values at high latitude. However they are still globally consistent in view of our error bars.

Domaines: Astrophysique [astro-ph]; Planète et Univers [physics]

Thérèse Encrenaz, Riccardo Melchiorri, Thierry Fouchet, Pierre Drossart, Emmanuel Lellouch, et al.. A mapping of martian water sublimation during early northern summer using OMEGA/Mars Express. Astronomy and Astrophysics - A&A, 2005, 441, pp.L9-L12. ⟨10.1051/0004-6361:200500171⟩. ⟨hal-03732534⟩