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Evolution of the Edgeworth-Kuiper Belt

Published online by Cambridge University Press:  30 March 2016

S.I. Ipatov
S.I. Ipatov*
Affiliation:
Institute of applied mathematics, Miusskaya sq. 4, Moscow, 125047, Russia

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.

Type
II. Joint Discussions
Information
Highlights of Astronomy , Volume 12: Highlights of Astronomy. As presented at the XXIVth General Assembly of the IAU, 2000 , 2002 , pp. 247 - 248
Copyright
Copyright © Astronomical Society of Pacific 2002

References

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