Isolated grain condensation behavior: Computation methods and first results

Details Isolated grain condensation behavior: Computation methods and first results Isolated grain condensation behavior: Computation methods and first results

Feb 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982plap.nasa...36l&link_type=abstract

In its Planetary Atmospheres Program p 36-47 (SEE N82-22112 12-88)

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Applications Programs (Computers), Computer Programs, Condensates, Planetary Atmospheres, Planetary Evolution, Enstatite, Low Pressure, Meteorites, Minerals, Novae

Scientific paper

A set of efficient programs for calculation of condensation behavior in a system with either solar or carbon-rich elemental composition was developed to treat the course of condensation at very low pressures. These programs were applied to the problem of condensation at very low pressures. The minerals produced in the stellar and nova-related processes under study, including carriers of important volatile elements such as carbon and nitrogen, are candidates for accretion into meteorite parent bodies and planets, and may still be discernible in the enstatite chondrites.

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