The thermal stability of near-surface ground ice on Mars

Details The thermal stability of near-surface ground ice on Mars The thermal stability of near-surface ground ice on Mars

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992natur.356...43p&link_type=abstract

Nature (ISSN 0028-0836), vol. 356, March 5, 1992, p. 43-45. Research supported by NASA and California Space Institute.

Physics

81

Ground Water, Ice, Mars Surface, Surface Water, Thermal Stability, Surface Temperature, Thermal Conductivity, Viking Spacecraft

Scientific paper

Results of thermal calculations are presented which show that observed geographic variations in the thermal and reflectance properties of Martian soils significantly affect subsurface temperatures. The results indicate that in certain regions, ground-ice deposits could exist much closer to the surface and much closer to the equator than previously thought. These deposits could be a valuable resource for future human exploration.

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