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Orbits of Trojan Asteroids

Published online by Cambridge University Press:  14 August 2015

G. A. Chebotarev ,
N. A. Belyaev  and
R. P. Eremenko
G. A. Chebotarev
Affiliation:
Institute of Theoretical Astronomy, Leningrad, U.S.S.R.
N. A. Belyaev
Affiliation:
Institute of Theoretical Astronomy, Leningrad, U.S.S.R.
R. P. Eremenko
Affiliation:
Institute of Theoretical Astronomy, Leningrad, U.S.S.R.

Abstract

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In this paper the orbital evolution of Trojan asteroids are studied by integrating numerically the equations of motion over the interval 1660–2060, perturbations from Venus to Pluto being taken into account. The comparison of the actual motion of Trojans in the solar system with the theory based on the restricted three-body problem are given.

Information

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 62: The Stability of the Solar System , 1974 , pp. 63 - 69
Copyright
Copyright © Reidel 1974 

References

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