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New semi-analytic theory of the four outer planets

Published online by Cambridge University Press:  25 May 2016

J.L. Simon*
Affiliation:
Bureau des longitudes 77, avenue Denfert-Rochereau 75014, Paris France

Extract

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A planetary theory of the planets Jupiter, Saturn, Uranus and Neptune is presented here. It is a classical planetary theory where the perturbations are computed in the form of Poisson series of only one angular variable. It is built with modern values of the planetary masses and fitted to the numerical integration DE245 of the Jet Propulsion Laboratory (Standish, 1994). Its validity time span is of several thousand of years.

Type
Part II - Planets and Moon: Theory and Ephemerides
Copyright
Copyright © Kluwer 1996 

References

Bretagnon, P. (1982) Astron. Astrophys., Vol. no. 114, p. 278288.Google Scholar
Bretagnon, P., Francou, G. (1987) Astron. Astrophys., Vol. no. 202, p. 309315.Google Scholar
McCarthy, D.D. (1992), IERS Standards (1992) IERS Technical Note. 13, Observatoire de Paris Google Scholar
Simon, J.L. (1983) Astron. Astrophys., Vol. no. 120, p. 197202.Google Scholar
Simon, J.L., Bretagnon, P. (1984) Astron. Astrophys., Vol. no. 138, p. 169178.Google Scholar
Simon, J.L., Joutel, F. (1988) Astron. Astrophys., Vol. no. 205, p. 328334.Google Scholar
Simon, J.L., Joutel, F., Bretagnon, P. (1992) Astron. Astrophys., Vol. no. 265, p. 308323.Google Scholar
Standish, E.M. (1982) Astron. Astrophys., Vol. no. 114, p. 297302.Google Scholar
Standish, E.M. (1994), Private Communication .Google Scholar