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Developing high accuracy numerical theories of motion of outer satellites of Jupiter and Saturn

Published online by Cambridge University Press:  04 August 2017

L. E. Bykova  and
V. V. Shikhalev
L. E. Bykova
Affiliation:
Tomsk University, Lenin prospect, 36, 634010, Tomsk, USSR
V. V. Shikhalev
Affiliation:
Tomsk University, Lenin prospect, 36, 634010, Tomsk, USSR

Abstract

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The effect of different perturbing factors on the rectangular coordinates of outer satellites of Jupiter (VI-XII) and Saturn (VI-IX) is investigated by the numerical integration of the equations of motion. The effect of relativistic terms in the equations of motion is considered among other perturbations. The effect of weak perturbations is compared with the accuracy of modern observations of satellites.

Type
Motions of Natural Bodies in the Solar System
Information
Symposium - International Astronomical Union , Volume 114: Relativity in Celestial Mechanics and Astrometry , 1986 , pp. 135 - 140
Copyright
Copyright © Reidel 1986 

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