On some aspects of the stirring rate of planetesimal velocities by a protoplanet

Astronomy and Astrophysics – Astronomy

Scientific paper

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Celestial Mechanics, Planets And Satellites: Formation, Solar System: Formation

Scientific paper

We discuss some aspects of the evolution of the relative velocities of a swarm of planetesimals stirred by a protoplanet. We show that the prescriptions most commonly used in semi-analytical `oligarchic growth' models overestimate the relative velocities of planetesimals by a non-negligible factor. We discuss the probable origin of this discrepancy, proposing a correction factor that provides good agreement between these prescriptions and the results of numerical experiments. The proposed correction factor can be easily implemented in semi-analytical accretion models.

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