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Investigation of the Orbital Stability of Minor Planets with Cometary Eccentricities

Published online by Cambridge University Press:  14 August 2015

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

Abstract

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The evolution of the orbits of 19 asteroids of particular interest has been studied over the interval 1660–2060, perturbations by Venus to Pluto being taken into account. Information was obtained about the encounters with Venus, the Earth, and Mars. A few approaches of Hidalgo to Jupiter were noted. In distinction to the orbits of short-period comets, the orbits of the 19 asteroids are stable throughout the 400-yr interval.

Type
Part VI/Relationship With Meteors and Minor Planets
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972 , pp. 431 - 436
Copyright
Copyright © Reidel 1972 

References

Belyaev, N. A.: 1967, Byull. Inst. Teor. Astron. 10, 696.Google Scholar
Chebotarev, G. A., Belyaev, N. A., and Eremenko, R. P.: 1970, Byull. Inst. Teor. Astron. 12, 82.Google Scholar
Chebotarev, G. A. and Shmakova, M. Ya.: 1970, Byull. Inst. Teor. Astron. 12, 104.Google Scholar
Gehrels, T., Roemer, E., Taylor, R. C., and Zellner, B. H.: 1970, Astron. J. 75, 186.CrossRefGoogle Scholar
Kresák, L.: 1969, Bull. Astron. Inst. Czech. 20, 177.Google Scholar
Marsden, B. G.: 1970, Astron. J. 75, 206.Google Scholar