Comparison of analytical and physical modeling of planetesimal accumulation

Mathematics – Probability

Scientific paper

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Astronomical Models, Planetary Evolution, Planetary Mass, Protoplanets, Kinetic Theory, Mass Distribution, Probability Theory, Size Distribution

Scientific paper

Three cases for which the analytic solutions to the planetary embryo coagulation equation are known, namely those of constant coagulation rate, of rate proportional to the sum of the masses of the two colliding bodies, and of rate proportional to the product of their masses, are presently used to test the mathematical validity of the Wetherill and Stewart (1989) physical model for the evolution of planetary embryos' mass distribution. In all cases, excellent agreement is found between numerical physical modeling results and those of the analytic solutions. The treatment of the runaway case can proceed via extension of the efforts of Trubnikov (1971).

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