Direct condensation of ferromagnesian liquids from cosmic gases

Details Direct condensation of ferromagnesian liquids from cosmic gases Direct condensation of ferromagnesian liquids from cosmic gases

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..317e&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 317.

Computer Science

3

Cosmic Gases, Liquid Phases, Condensation, Temperature Dependence, Chemical Composition, Silicates, Condensates, Solid Phases, Free Energy, Thermodynamic Equilibrium

Scientific paper

In order to investigate the condensation temperature of ferromagnesian liquids from cosmic gases and their coexisting solid condensates as well as changes in the compositions of coexisting solids and liquid with falling temperature, nonideal liquid solution models applicable to a much broader range of compositions than those restricted to CMAS must be incorporated into equilibrium condensation calculations. The authors have therefore rewritten their condensation program in order to use the same free-energy minimization technique, the same silicate liquid composition-activity relations, and the same thermodynamic data base for both pure solids and solid solution phases compatible with that liquid as are used in MELTS, a program written by Ghiorso and Sack (1995). The results running this rewritten program are reported here.

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