Thermodynamic Modeling of Evaporation Processes of Lunar and Meteorite Substance


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Abstract

The paper suggests a thermodynamic approach to modeling the evaporation of lunar and meteorite matter. Comparison of the results of model calculations and experimental data demonstrates the high accuracy of the developed approach to description of thermodynamic properties of melts of lunar and meteorite substance and its behavior at evaporation. The observed relations of melt evaporation are consistent with the thermodynamic values characterizing the residual melts.

About the authors

S. I. Shornikov

Vernadsky Institute of Geochemistry and Analytical Chemistry (GEOKhI), Russian Academy of Sciences

Author for correspondence.
Email: sergey.shornikov@gmail.com
Russian Federation, Moscow, 119991

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