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Evolution of the Edgeworth-Kuiper Belt
Published online by Cambridge University Press: 30 March 2016
Abstract
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Due to gravitational interactions with large trans-neptunian objects (TNOs) several percent of TNOs can change their semimajor axes by more that 1 AU during last 4 Gyr. Now about 30000 1-km former TNOs can be Jupiter crossers and about 20% of Earth-crossing objects can be former TNOs which now move in Jupiter-crossing orbits.
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- II. Joint Discussions
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- Copyright © Astronomical Society of Pacific 2002
References
Ipatov, S.I.
1998, in “Planetary systems: thelong view”, ed. Celnikier, L.M. and Van, Tran Thanh (Editions Frontières), 157
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