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On the Motion of Short-Period Comets in the Neighbourhood of Jupiter

Published online by Cambridge University Press:  14 August 2015

V. M. Chepurova
V. M. Chepurova*
Affiliation:
Sternberg Astronomical Institute, Moscow, U.S.S.R.

Abstract

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An intermediate orbit is developed for studying the hyperbolic jovicentric motion of a comet in the vicinity of Jupiter, where the effect of Jupiter's oblateness may become significant. A comparison is made with some of the results obtained by other investigators on the motions of specific periodic comets.

Type
Part II/General Methods of Orbit Theory
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972 , pp. 62 - 65
Copyright
Copyright © Reidel 1972 

References

Aksenov, E. P., Grebenikov, E. A., and Demin, V. G.: 1961, Iskusstv. Sputniki Zemli No. 8, 64.Google Scholar
Aksenov, E. P., Grebenikov, E. A., and Demin, V. G.: 1963, Astron. Zh. 40, 363.Google Scholar
Chepurova, V. M.: 1970, Byull. Inst. Teor. Astron. 12, 216.Google Scholar
Dubyago, A. D.: 1950, Trudy Astron. Obs. Kazan No. 31.Google Scholar
Kamieński, M.: 1949, Bull. Acad. Polon. Sci. Lettres Ser. A 61.Google Scholar
Kamieński, M.: 1956, Acta Astron. 6, 153.Google Scholar
Kazimirchak-Polonskaya, E. I.: 1961, Trudy Inst. Teor. Astron. 7.Google Scholar