Thermal History Calculations Versus Full Convection Models: Application to the Thermal Evolution of Mercury

Details Thermal History Calculations Versus Full Convection Models: Application to the Thermal Evolution of Mercury Thermal History Calculations Versus Full Convection Models: Application to the Thermal Evolution of Mercury

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1905r&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1905

Computer Science

Scientific paper

We present a suite of convection calculations with a constant viscosity
and dry, olivine rheology. By comparing our convective models with
previous calculations, we hope to resolve the inconsistencies in
previous thermal history models of Mercury.

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