Numerical experiments on planetesimal aggregation during the formation of the solar system

Details Numerical experiments on planetesimal aggregation during the formation of the solar system Numerical experiments on planetesimal aggregation during the formation of the solar system

Sep 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977pasau...3..169h&link_type=abstract

(Astronomical Society of Australia, Annual General Meeting, 11th, Clayton, Victoria, Australia, May 30-June 1, 1977.) Astronomic

Computer Science

Numerical Analysis

5

Numerical Analysis, Particle Motion, Planetary Evolution, Solar System, Gas Flow, Jet Flow, Jet Streams (Meteorology), Kinetic Theory, Mathematical Models

Scientific paper

A numerical analysis is undertaken to evaluate different hypotheses of planetary formation through the aggregation of small particles. It is found that the planetary jetstream configuration is produced when condensation and evolution of the bodies occur within a Prentice-Laplacian gas ring. Excess kinetic energy is damped out through collisions, and a gradual migration of planetesimals toward regions of higher density can then take place.

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