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ReportsSummer Evolution of the North Polar Cap of Mars as Observed by OMEGA/Mars Express
The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) visible-infrared imaging spectrometer extensively observed regions of Mars with latitudes above 70°N in late 2004 (heliocentric longitude from Ls 93° to Ls 127°). The extent of water ice at the surface and the size of ice grains were monitored as a function of time. Bright, small-grained frost, which initially covered a large fraction of the polar cap, waned in favor of large-grained ice. In outlying regions, dominated by large-grained ice, the albedo increased over the period. Evaluating the dust content was model dependent. However, contamination of ice by dust was low.
1 Institut d'Astrophysique Spatiale, CNRSUniversité Paris Sud, 91405 Orsay, France.
2 Laboratoire de Planétologie de Grenoble, CNRSUniversité Joseph Fourier, 38400 Grenoble, France. * To whom correspondence should be addressed. E-mail: yves.langevin{at}ias.u-psud.fr
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Science. ISSN 0036-8075 (print), 1095-9203 (online)