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Dynamical Evolution of Trans-Neptunian Objects in High-Eccentricity Orbits

Published online by Cambridge University Press:  30 March 2016

V.V. Emel’yanenko
V.V. Emel’yanenko*
Affiliation:
South Ural University, Lenina 76, Chelyabinsk 454080, Russia

Abstract

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The evolution of near-parabolic orbits with perihelia in the trans-neptunian region has been studied, considering the action of planetary, Galactic and stellar perturbations for the age of the Solar System. This investigation has led to the conclusion that the observed trans-neptunian objects in high-eccentricity orbits might originate from the inner core of the Oort cloud.

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. 223 - 224
Copyright
Copyright © Astronomical Society of Pacific 2002

References

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