Spatial distribution of small particles in the gravitational field of a massive body in the case of inelastic collisions

Details Spatial distribution of small particles in the gravitational field of a massive body in the case of inelastic collisions Spatial distribution of small particles in the gravitational field of a massive body in the case of inelastic collisions

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979sogru..95..589k&link_type=abstract

Akademiia Nauk Gruzinskoi SSR, Soobshcheniia, vol. 95, Sept. 1979, p. 589-592. In Russian.

Astronomy and Astrophysics

Astrophysics

Astrophysics, Gravitational Fields, Particle Density (Concentration), Planetary Evolution, Protoplanets, Solar System, Astronomical Models, Inelastic Collisions, Spatial Distribution

Scientific paper

A scenario of planetary evolution in the solar system is proposed. Small
dust particles moving in the gravitational field of a protoplanet lose
energy due to inelastic collisions, are captured by the protoplanet into
elliptical orbit, and form a swarm. This paper presents some results for
the case of totally inelastic collisions.

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