A Model for Sulfur Speciation and Sulfur Isotope Fractionation During Magmatic Degassing on Earth and Mars

Details A Model for Sulfur Speciation and Sulfur Isotope Fractionation During Magmatic Degassing on Earth and Mars A Model for Sulfur Speciation and Sulfur Isotope Fractionation During Magmatic Degassing on Earth and Mars

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.1238d&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.1238

Physics

1

Scientific paper

Our model results suggest that (1) H2S and S2 are the main S gases
exsolved from martian magmas, (2) degassing fractionation cannot explain
the range in δ34S of martian meteorites, and (3) the δ34S
value of the bulk martian surface is ~0 to +2‰.

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