Magmatic Transport of Carbon, Hydrogen and Nitrogen Constituents from Reduced Planetary Interiors

Details Magmatic Transport of Carbon, Hydrogen and Nitrogen Constituents from Reduced Planetary Interiors Magmatic Transport of Carbon, Hydrogen and Nitrogen Constituents from Reduced Planetary Interiors

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1020k&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Computer Science

Scientific paper

In the light of experimental data we argue that magma in reduced
environment at in area of the Fe-Si alloy stability could form melts
containing dissolved both oxidized, and reduced components of hydrogen
and carbon species.

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