A Thermodynamic and Kinetic Model of Metal Condensation: Implications for the Evolution of the Nebular Source Regions of Chondrites

Details A Thermodynamic and Kinetic Model of Metal Condensation: Implications for the Evolution of the Nebular Source Regions of Chondrites A Thermodynamic and Kinetic Model of Metal Condensation: Implications for the Evolution of the Nebular Source Regions of Chondrites

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1657p&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1657

Physics

Scientific paper

Modeling growth and simultaneous diffusional equilibration of the zoned
metal grains in CH chondrites reveals that the condensation zoning
profiles were substantially modified by diffusion while the grains were
growing in the nebula.

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