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Expansion of the planetary mutual distance raised to any negative power by the method of symbolic differential operators. (English) Zbl 0883.70009

Summary: We present an approach to evaluate \(\Delta^{-s}\) necessary for the construction of high-order planetary theories. This approach is valid to be applied on very large scale digital computers with standard Poisson series programs, for high-order and high-degree planetary theories. We apply the method of symbolic differential operators for single variable functions, and the binomial theorem expansions, for the evaluation of \(\Delta^{-s}\). We utilize Laplace coefficients and their derivatives to carry out the development, without dealing with Newcomb operators or Hansen’s coefficients.

MSC:

70F15 Celestial mechanics
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References:

[1] Abu-El-Ata, N. and Chapront, J.: 1975, Astron. and Astrophys. 38, 57-66.
[2] Brouwer, D. and Clemence, G. M.: 1965, Methods of Celestial Mechanics, Academic Press. · Zbl 0132.23506
[3] Broucke, R. and Smith, G.: 1971, Cel. Mech. 4, 490. · doi:10.1007/BF01231405
[4] Duriez, L.: 1992, Le Developpment de la Fonction Perturbatrice, Publications de l’Université des Sciences et Techniques de Lille, UFR de mathématiques, Laboratoire d’Astronomie, Lille, France pp. 1-26.
[5] Iszak, I. G.: 1966, Reprint from International Astronomical Union No. 25, 230.
[6] Kamel, O. M. and Soliman, A. S.: 1990, Earth, Moon and Planets 49, 25-56. · Zbl 0698.70006 · doi:10.1007/BF00053996
[7] Meffroy, J.: 1967, Goddard Space Flight Center, Greenbelt. Maryland No X-641-67-442.
[8] Smart, W. M.: 1960, Celestial Mechanics, Longmans.
[9] Shook, C. A.: 1931, M.N., 91, 553.
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