Dynamic Temperature Fields under Mars Landing Sites and Implications for Supporting Microbial Life

Details Dynamic Temperature Fields under Mars Landing Sites and Implications for Supporting Microbial Life Dynamic Temperature Fields under Mars Landing Sites and Implications for Supporting Microbial Life

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010asbio..10..643u&link_type=abstract

Astrobiology, Volume 10, Issue 6, pp. 643-650.

Biology

5

Mars, Temperature, Lander, Liquid, Brine

Scientific paper

While average temperatures on Mars may be too low to support terrestrial life-forms or aqueous liquids, diurnal peak temperatures over most of the planet can be high enough to provide for both, down to a few centimeters beneath the surface for some fraction of the time. A thermal model was applied to the Viking 1, Viking 2, Pathfinder, Spirit, and Opportunity landing sites to demonstrate the dynamic temperature fields under the surface at these well-characterized locations. A benchmark temperature of 253 °K was used as a lower limit for possible metabolic activity, which corresponds to the minimum found for specific terrestrial microorganisms. Aqueous solutions of salts known to exist on Mars can provide liquid solutions well below this temperature. Thermal modeling has shown that 253 °K is reached beneath the surface at diurnal peak heating for at least some parts of the year at each of these landing sites. Within 40° of the equator, 253 °K beneath the surface should occur for at least some fraction of the year; and, within 20°, it will be seen for most of the year. However, any life-form that requires this temperature to thrive must also endure daily excursions to far colder temperatures as well as periods of the year where 253 °K is never reached at all.

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