Mutual gravitational influence of beyond-Neptune bodies

Details Mutual gravitational influence of beyond-Neptune bodies Mutual gravitational influence of beyond-Neptune bodies

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..617i&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 617.

Physics

Kuiper Belt, Solar Orbits, Neptune (Planet), Gravitational Effects, Collisions, Algorithms

Scientific paper

Previous investigation results on disks of bodies have indicated that the eccentricities of the largest bodies of the disk are smaller than the average eccentricity, and that these bodies can increase their semimajor axis due to gravitational interaction with those smaller bodies, which decrease theis semimajor axes. The same may be true of the Kuiper belt, in which some bodies have migrated to the orbit of Neptune; a fraction of large bodies may therefore be larger for the central part of the Kuiper belt than for the inner part.

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