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The theory of the motion of Halley Comet

Published online by Cambridge University Press:  04 August 2017

E.L. Akim ,
Ju.F. Koljuka ,
V.V. Savtchenko ,
V.A. Stepanianz ,
N.M. Ivanov  and
V.F. Tikhonov
E.L. Akim
Affiliation:
Flight Central Center, Moscow, USSR Institute of applied Mathematics, Moscow, USSR
Ju.F. Koljuka
Affiliation:
Flight Central Center, Moscow, USSR Institute of applied Mathematics, Moscow, USSR
V.V. Savtchenko
Affiliation:
Flight Central Center, Moscow, USSR Institute of applied Mathematics, Moscow, USSR
V.A. Stepanianz
Affiliation:
Flight Central Center, Moscow, USSR Institute of applied Mathematics, Moscow, USSR
N.M. Ivanov
Affiliation:
Flight Central Center, Moscow, USSR Institute of applied Mathematics, Moscow, USSR
V.F. Tikhonov
Affiliation:
Flight Central Center, Moscow, USSR Institute of applied Mathematics, Moscow, USSR

Abstract

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The theory of the motion of Halley comet has been built using ground optical positional observations of 1682, 1759, 1835, 1910 and 1982–84. The orbital elements of the comet and two coefficients characterizing non-gravitational perturbations were determined precisely as a result of the statistical treatment of the observations. The estimations of the accuracy of the theory and the data describing its agreement with the observations are presented. The theory has been applied to ballistic-navigational calculations for the Soviet Vega project.

Type
Motions of Natural Bodies in the Solar System
Information
Symposium - International Astronomical Union , Volume 114: Relativity in Celestial Mechanics and Astrometry , 1986 , pp. 93 - 97
Copyright
Copyright © Reidel 1986