The description of the evolution of preplanetary bodies using kinetic theory

Details The description of the evolution of preplanetary bodies using kinetic theory The description of the evolution of preplanetary bodies using kinetic theory

Jul 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15..661z&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, July 1989, p. 661-666. In Russian. In Russian.

Statistics

Computation

Computational Astrophysics, Kinetic Theory, Planetary Evolution, Planetology, Gravitational Effects, Protoplanets, Saturn Rings, Stress Tensors

Scientific paper

The study of transport processes in a preplanetary disk using the approach of Goldreich and Tremaine (1978) is studied. This approach considers the dynamics of a system of inelastically colliding particles with regard to Saturn's rings. Expressions for the rates of the variation of the principal components of the stress tensor due to the gravitational interaction of bodies are obtained.

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