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The Study of Planetary Secular Perturbations*

Published online by Cambridge University Press:  12 April 2016

Zhang Jia-xiang
Zhang Jia-xiang*
Affiliation:
Purple Mountain Observatory, Academia Sinica, Nanjing, China

Summary

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The methods of the first-order planetary secular perturbations are discussed in this paper. On the basis of Gauss' method, some concrete applicable formulae are derived. And then, orbital evolutions of the nine major planets in solar system during about 2,100,000 years are investigated numerically. The method applied here is in principle suitable for the orbits of arbitrary eccentricities and inclinations.

Type
Part I - Satellites and Planets
Information
International Astronomical Union Colloquium , Volume 74: Dynamical Trapping and Evolution in the Solar System , 1983 , pp. 61 - 71
Copyright
Copyright © Reidel 1983

Footnotes

*

This paper has been published in Acta Astronomica Sinica, Vol. 23 (1982), No.1, 56, in Chinese.

References

1 Smart, W.M., Celestial Mechanics, 198–231.Google Scholar
2 Plummer, H.C., Dynamical Astronomy, 207–2l7.Google Scholar