Mars 2, 83-96, 2006 | doi:10.1555/mars.2006.0006
Received March 27, 2006 | Accepted November 7, 2006 | Published December 14, 2006
We describe the response of icy martian soil to a localized heat source using analytical and numerical models. Our motivation is to understand the implications of a landing failure in which a radioisotope power source is deposited along with terrestrial microbes within or near icy regolith, resulting in the production of liquid water and the proliferation of microbes.
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