Variations in the semimajor axis of a planetary orbit during the accumulation process

Details Variations in the semimajor axis of a planetary orbit during the accumulation process Variations in the semimajor axis of a planetary orbit during the accumulation process

Dec 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986avest..20..328z&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 20, Oct.-Dec. 1986, p. 328-333. In Russian.

Statistics

Computation

Axes Of Rotation, Periodic Variations, Planetary Evolution, Planetary Orbits, Accumulations, Computational Astrophysics, Distance, Mass Distribution, Velocity Distribution

Scientific paper

The magnitude of the regular shift of the semimajor axis of a planetary orbit from its initial value is evaluated as well as that of the root mean square deviation due to interactions with the cluster's bodies. It is shown that the former value is small in comparison with the latter. The root mean square deviation for the earth is in the 0.01-0.3 AU range depending on the ratio of the average mass of the bodies in the cluster to the mass of the accumulating planet. The results are of interest in connection with accumulation processes in the preplanetary swarm in the primordial solar system.

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