A Study of the Thermal Evolution of Mars via Viscoelastic Relaxation of Large Craters

Details A Study of the Thermal Evolution of Mars via Viscoelastic Relaxation of Large Craters A Study of the Thermal Evolution of Mars via Viscoelastic Relaxation of Large Craters

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2712k&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2712

Physics

Scientific paper

We constrain Mars’ heat flux by simulating deformation of large
craters. Our results reveal a secular cooling of Mars and a regional
variation consistent with higher heat fluxes closer to the Crustal
Dichotomy boundary persisting to the mid-Noachian.

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