Towards combined modelling of planetary accretion and differentiation

Details Towards combined modelling of planetary accretion and differentiation Towards combined modelling of planetary accretion and differentiation

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1140g&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1140

Computer Science

Scientific paper

Results confirm that late formed planetsimals do not experience silicate melting and avoid thermal alteration. However they also indicate that even for cool bodies a more complex thermal structure develops than the previously proposed onion-shell model. In early formed bodies accretion and iron core growth occur almost simultaneously and magma oceans develop in the interior of these bodies, which tend to form first close to the coremantle boundary and migrate upwards with growing internal pressure.

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