Core Formation by Percolation of Iron-rich Liquids

Details Core Formation by Percolation of Iron-rich Liquids Core Formation by Percolation of Iron-rich Liquids

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1329h&link_type=abstract

37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1329

Computer Science

Scientific paper

Experimental and numerical modeling evidence supports the hypothesis
that core formation in planetesimals and planets can occur by the
percolation of iron-rich liquids through a deforming, solid silicate
layer that compacts as the liquid core grows.

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