High Pressure, Near-Liquidus Phase Relations in Fe-C-S Systems and Implications for Composition, Structure, and Process of Formation of Metallic Cores in Planetary Bodies

Details High Pressure, Near-Liquidus Phase Relations in Fe-C-S Systems and Implications for Composition, Structure, and Process of Formation of Metallic Cores in Planetary Bodies High Pressure, Near-Liquidus Phase Relations in Fe-C-S Systems and Implications for Composition, Structure, and Process of Formation of Metallic Cores in Planetary Bodies

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009lpi....40.2008d&link_type=abstract

40th Lunar and Planetary Science Conference, (Lunar and Planetary Science XL), held March 23-27, 2009 in The Woodlands, Texas, i

Physics

Scientific paper

We present new high pressure, near-liquidus phase relation experiments
in Fe-C-S systems. Our experiments shed light on to the evolution and
formation of metallic cores in differentiated planetary bodies in the
presence of both carbon and sulfur.

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