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An Investigation of the Motion of Periodic Comet Borrelly from 1904 to 1967

Published online by Cambridge University Press:  14 August 2015

L. M. Belous
L. M. Belous*
Affiliation:
Northwestern Extramural Polytechnic Institute, Leningrad, U.S.S.R.

Abstract

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The motion of P/Borrelly has been investigated using all precise published positions and taking into account the perturbations by Venus to Pluto. Nongravitational forces have been found to influence the motion of the comet considerably, formerly as a secular deceleration, more recently as a secular acceleration. By linking the seven apparitions 1904–1960, with allowance for the nongravitational effects, we have obtained a set of elements which represents 802 observations with a mean error of 1′.89.

Type
Part III/Motions of the Short-Period Comets
Information
Symposium - International Astronomical Union , Volume 45: The Motion, Evolution of Orbits and Origin of Comets , 1972 , pp. 190 - 194
Copyright
Copyright © Reidel 1972 

References

Fayet, G.: 1914, Ann. Obs. Paris Mem. 30, A1.Google Scholar
Fayet, G.: 1925, J. Obs. 8, 109.Google Scholar
Kazimirchak-Polonskaya, E. I.: 1967, Trudy Inst. Teor. Astron. 12, 39.Google Scholar
Marsden, B. G.: 1968, Astron. J. 73, 367.Google Scholar
Schaumasse, A.: 1931, J. Obs. 14, 147.Google Scholar
Vsekhsvyatskij, S. K.: 1958, Fizicheskie Kharakteristiki Komet , Moscow.Google Scholar