Relaxation of Crustal Thickness Variations on Mars: Implications for Thermal Evolution

Details Relaxation of Crustal Thickness Variations on Mars: Implications for Thermal Evolution Relaxation of Crustal Thickness Variations on Mars: Implications for Thermal Evolution

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1357p&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1357

Physics

6

Scientific paper

A long wavelength crustal thickness variation on Mars, plausibly dating
from early crustal differentiation, constrains the thermal evolution,
particularly the amount of secular cooling of the mantle or rate of
convective heat transfer.

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