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- W1989107981 abstract "Abstract The Hamiltonian representing the average over the mean-motion angles (i.e. the secular part) of the three-body planetary problem is considered. An efficient algorithm constructing invariant tori for the trajectories in phase space is provided. To give a possible practical application, we consider a toy-model including the main terms of the secular part of a hypothetic Sun-Jupiter-Saturn system having eccentricities and inclinations equal to 1 20 of the true ones. The scheme of a KAM proof of the stability of the model is sketched. The proof is “computer assisted”." @default.
- W1989107981 created "2016-06-24" @default.
- W1989107981 creator A5016605837 @default.
- W1989107981 date "1998-11-01" @default.
- W1989107981 modified "2023-09-27" @default.
- W1989107981 title "Three-body planetary problem: study of KAM stability for the secular part of the Hamiltonian" @default.
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- W1989107981 doi "https://doi.org/10.1016/s0032-0633(98)00064-6" @default.
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