Hydrothermal Geochemistry as the Source of Plume Gases on Enceladus: A Thermodynamic Evaluation

Details Hydrothermal Geochemistry as the Source of Plume Gases on Enceladus: A Thermodynamic Evaluation Hydrothermal Geochemistry as the Source of Plume Gases on Enceladus: A Thermodynamic Evaluation

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1251g&link_type=abstract

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

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Thermodynamic modeling indicates that hydrothermal systems that existed
at temperatures near 300°C and oxidation states corresponding to PPM
redox buffering could have produced fluids with compositions that are
consistent with the plume's chemistry.

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