Regional Martian Crustal Heat Flow from Mars Odyssey Gamma-Ray Spectrometry

Details Regional Martian Crustal Heat Flow from Mars Odyssey Gamma-Ray Spectrometry Regional Martian Crustal Heat Flow from Mars Odyssey Gamma-Ray Spectrometry

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1371h&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1371

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Scientific paper

Using radiogenic elemental abundances derived from Gamma-Ray
Spectrometer (GRS) observations, we estimate the crustal component of
martian heat flow for specific geologic features and regions, both
present day and at the time of formation.

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