Collisional probability of planetesimals revolving in the solar gravitational field. III

Details Collisional probability of planetesimals revolving in the solar gravitational field. III Collisional probability of planetesimals revolving in the solar gravitational field. III

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...224..303i&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 224, no. 1-2, Oct. 1989, p. 303-315.

Statistics

Computation

52

Collision Rates, Hill Method, Probability Theory, Protoplanets, Solar Gravitation, Computational Astrophysics, Degrees Of Freedom, Planetary Orbits, Three Body Problem

Scientific paper

The rate of collisions of planetesimals on the protoplanet are
calculated, accounting for the effect of solar gravity. The numerical
scheme is based on Hill's equations which approximately describe the
three-body problem. The collisional rate is summarized in terms of the
normalized eccentricity and inclination of relative motion.

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