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The past orbit of comet Halley and its meteor stream

Published online by Cambridge University Press:  12 April 2016

A. Hajduk*
Affiliation:
Astronomical Institute of the Slovak Academy of Sciences, 842 28 Bratislava, Czechoslovakia

Abstract

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The present paper studies the structural features of the meteor streams associated with Comet Halley deduced from the observations of its meteor showers, as check points of orbital elements in a deeper history of the comet orbit. Libration of the argument of perihelion of the comet and the corresponding displacement of the nodes, as recognized in the distribution of condensations within the stream, allows to estimate the maximum lifetime of the comet in the inner Solar System at about 2 × 105 years.

Type
Section VII. Comet P/Halley and Future Missions to Comets
Copyright
Copyright © Cambridge University Press 1985

References

Kamieński, M.: 1961, Acta Astronomica 11, 223229.Google Scholar
Kozai, Y.: 1979, IAU Symp. 81, 231237.Google Scholar
McIntosh, B.A. and Hajduk, A.: 1983, Mon. Not. Roy. Astron. Soc. 205, 931943.CrossRefGoogle Scholar
Yatoushita, S.: 1972, Astron. Astrophys. 20, 205214.Google Scholar
Yeomans, D.K. and Kiang, T.: 1981, Mon. Not. Roy. Astron. Soc. 197, 633646.Google Scholar