Closure of the Fe-S-Si Liquid Miscibility Gap at High Pressure and Its Implications for Planetary Core Formation

Details Closure of the Fe-S-Si Liquid Miscibility Gap at High Pressure and Its Implications for Planetary Core Formation Closure of the Fe-S-Si Liquid Miscibility Gap at High Pressure and Its Implications for Planetary Core Formation

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1298s&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1298

Computer Science

Scientific paper

We report melting experiments in the Fe-S-Si system conducted in a
multi-anvil apparatus at pressures between 10 and 27 GPa and
temperatures up to 2343 K. The results have important implications for
the differentiation processes of the planets and the composition of
their cores.

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