Kinetic analysis of the stability of interstellar carbon in the preplanetary cloud

Details Kinetic analysis of the stability of interstellar carbon in the preplanetary cloud Kinetic analysis of the stability of interstellar carbon in the preplanetary cloud

Apr 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989geokh......467m&link_type=abstract

Geokhimiia (ISSN 0016-7525), April 1989, p. 467-477. In Russian.

Physics

Carbon, Interstellar Matter, Reaction Kinetics, Thermodynamics, Water Vapor, Cosmochemistry, Planetary Nebulae, Solar System

Scientific paper

The stability of interstellar carbon in the preplanetary cloud is analyzed from the thermodynamic and kinetic standpoints. It is shown that the reaction with water vapor is the principal contributor to the gasification of elementary carbon in the preplanetary cloud and that this process could take place in regions of the nebula with temperatures above 1000-1200 K. Some cosmochemical implications are examined.

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