Non-Newtonian Convection Modeling and the Possibility of Present Day Internal Activity on Ceres?

Details Non-Newtonian Convection Modeling and the Possibility of Present Day Internal Activity on Ceres? Non-Newtonian Convection Modeling and the Possibility of Present Day Internal Activity on Ceres?

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2017s&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2017

Computer Science

Scientific paper

Using a three-dimensional spherical shell convection model to understand
the internal activity of Ceres. Also, to analyze the geoid, topography
and heat flow from our models and compare it with observational data
from Dawn when it arrives at Ceres in 2015.

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