Low- to medium-temperature phase equilibria in a gas of solar composition

Details Low- to medium-temperature phase equilibria in a gas of solar composition Low- to medium-temperature phase equilibria in a gas of solar composition

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983e%26psl..65....7s&link_type=abstract

Earth and Planetary Science Letters (ISSN 0012-821X), vol. 65, no. 1, Oct. 1983, p. 7-16. Research supported by the Naturvetensk

Other

15

Gas Composition, Mineralogy, Planetary Evolution, Solar System, Abundance, Chemical Composition, Equilibrium, Solid Solutions, Vapor Phases

Scientific paper

Solar-composition gas mineral assemblages are calculated for 423-1023 K and 1-10 to the -8th bar pressures, yielding the modal percent variation of all condensates and the chemical compositions of ideal and nonideal coexisting solid solutions. The major mineral assemblage that is stable over most of the pressure and temperature field is gamma- and alpha-Fe-Ni alloys + olivine + orthopyroxene + clinopyroxene + plagioclase + ilmenite. Compositions of the plagioclase, olivine, orthopyroxene, ilmenite, and garnet, are found to be potential cosmobarometers and cosmothermometers.

Affiliated with

Also associated with

No associations

Rating

Low- to medium-temperature phase equilibria in a gas of solar composition does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Low- to medium-temperature phase equilibria in a gas of solar composition, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Low- to medium-temperature phase equilibria in a gas of solar composition will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1192976