Chaotic Terrain and Its Constraints on the Surface Heat Flux of Mars

Details Chaotic Terrain and Its Constraints on the Surface Heat Flux of Mars Chaotic Terrain and Its Constraints on the Surface Heat Flux of Mars

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1345s&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1345

Mathematics

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Scientific paper

Geological analysis of Aram Chaos on Mars suggests that this chaotic
terrain could have formed by the collapse of an underground lake. We
show how this concept can be used to constrain the surface heat flux
during the Hesperian.

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