Evidence for Enhanced Hydration and Water Ice Stability at Tropical Latitudes on Mars

Details Evidence for Enhanced Hydration and Water Ice Stability at Tropical Latitudes on Mars Evidence for Enhanced Hydration and Water Ice Stability at Tropical Latitudes on Mars

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agufm.p21b0153b&link_type=abstract

American Geophysical Union, Fall Meeting 2005, abstract #P21B-0153

Physics

5422 Ices

Scientific paper

New spectroscopic observations performed by the OMEGA instrument on board Mars Express show evidence for a small region of enhanced hydration on the northern scarp of Olympus Mons. Day and night measurements of surface temperatures in this region indicate that the soil has an high thermal inertia and exhibits the lowest daytime temperatures in the area. Thermodynamic modeling suggests that water ice in this region is stable during most of the Martian year due to the saturation of the atmosphere.

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