Non-equilibrium condensation of refractory metals in a primordial solar nebula

Details Non-equilibrium condensation of refractory metals in a primordial solar nebula Non-equilibrium condensation of refractory metals in a primordial solar nebula

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002asthe..95..173t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 95, No. 4, p. 173 - 178 (2002)

Astronomy and Astrophysics

Astronomy

Solar Nebula

Scientific paper

We investigated non-equilibrium condensation of refractory metals in the primordial solar nebula theoretically, in relation to the origin of refractory metal nuggets in chondrites. On the basis of the nucleation theory, we performed numerical simulations of the non-equilibrium condensation of refractory metals and found that the condensation temperatures decrease considerably from the values in equilibrium condensation. We found that the cooling time should be longer than 1×105 years in the primordial solar nebula for the formation of sub-micron size or larger refractory metal nuggets.

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