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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
Abstract
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