A determination of secular terms in first-order planetary theory. (English) Zbl 0662.70014
The secular terms of the first-order planetary Hamiltonian is determined, by two methods, in terms of the variables of H. Poincaré, neglecting powers higher than the second in the eccentricity-inclination.
References:
[1] | Anolik, M. V. Krassinsky, B. A., and Pius, L. J.: 1969, Trudy Inst. Theor. Astron. Leningrad 14, 3-47. |
[2] | Bretagnon, P.: 1974, Astron. Astrophys. 30, 141-154. |
[3] | Brouwer, D., Van Woerkom, A. J. J.: 1950, Astron. Papers 13, Part 2, 81-107. |
[4] | Kamel, O. M. and Bakry, A. A.: 1981, Astrophys. Space Sci. 87, 3. · Zbl 0478.70010 · doi:10.1007/BF00654020 |
[5] | Kamel, O. M.: 1970, M.Sc. Thesis, Faculty of Sciences, Cairo University, Giza, Egypt, Chapter IV. |
[6] | Kamel, O. M.: 1988, Earth, Moon and Planets 43, 271 (this issue). · Zbl 0662.70009 · doi:10.1007/BF00117099 |
This reference list is based on information provided by the publisher or from digital mathematics libraries. Its items are heuristically matched to zbMATH identifiers and may contain data conversion errors. In some cases that data have been complemented/enhanced by data from zbMATH Open. This attempts to reflect the references listed in the original paper as accurately as possible without claiming completeness or a perfect matching.