The Effects of Obliquity on Geothermal Gradients and Methane Hydrate Stability Zones on Mars

Details The Effects of Obliquity on Geothermal Gradients and Methane Hydrate Stability Zones on Mars The Effects of Obliquity on Geothermal Gradients and Methane Hydrate Stability Zones on Mars

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2454r&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2454

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Scientific paper

This work models the location of the methane hydrate stability zone
using geothermal gradients on Mars. By examining the system kinetics,
the potential volume of hydrate dissociated through temperature changes
with obliquity can be better understood.

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