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The Possible Orbital Evolution of the Near-Earth Asteroids

Published online by Cambridge University Press:  07 August 2017

E.I. Timoshkova
E.I. Timoshkova*
Affiliation:
Institute of Theoretical Astronomy, Leningrad 191187, USSR

Abstract

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The subject of this paper is a study of a possible orbital evolution for near-Earth asteroids. The investigation is fulfilled in the frame of the restricted circular three body problem. It is based on the calculations of the Jacobi constant. The osculating elements of some real Apollo-Amor-Aten asteroids are used as the starting parameters. The comparison with the results of other authors is given.

Type
Part III - The Asteroidal Belt
Information
Symposium - International Astronomical Union , Volume 152: Chaos, Resonance and Collective Dynamical Phenomena in the Solar System , 1992 , pp. 175 - 178
Copyright
Copyright © Kluwer 1992 

References

Hahn, G., Lagerkvist, C., Lindgren, M. and Dahlgren, M.:1989 in Lagerkvist, C. I. et al., eds., Asteroids, Comets, Meteors III, Uppsala, p.95.Google Scholar
Kozai, Y.:1980, Icarus 41, 1.Google Scholar
Steel, D.I. and Baggaley, W.J.:1985, Mon. Not. R. Astr. Soc. 212 (4), 817.CrossRefGoogle Scholar
Szebehely, V.:1979 in Szebehely, V., ed., Instabilities in Dynamical Systems Reidel, Dordrecht, p.115.Google Scholar
Vashkovjak, M.A.:1980, Inst. Appl. Math. USSR Academy of Sciences, Preprint No. 93.Google Scholar
Ephemerides of Minor Planets for 1991, Nauka, Institute of Theoretical Astronomy, Leningrad.Google Scholar