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On the Stability of the Solar System as Hierarchical Dynamical System

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Abstract

The Stability of the Solar System as hierarchical dynamical system is investigated with analytical methods i) by using the topological stability criterion of the general 3-body problem for 3-body subsystems ii) by exploiting the hierarchical arrangement of the whole system to develop a new perturbation theory containing as smallness parameters both mass and distance ratios. At the first order in these parameters we get, for the inner Solar System, a minimum lifetime of ~108y. Most of the results presented here are discussed in detail in Milani and Nobili (1982,1983a,1983b) which we shall refer to as Paper I, II and III, respectively.

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© 1984 D. Reidel Publishing Company, Dordrecht, Holland

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Milani, A., Nobili, A.M. (1984). On the Stability of the Solar System as Hierarchical Dynamical System. In: Berger, A. (eds) The Big Bang and Georges Lemaître. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-6487-7_19

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  • DOI: https://doi.org/10.1007/978-94-009-6487-7_19

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-6489-1

  • Online ISBN: 978-94-009-6487-7

  • eBook Packages: Springer Book Archive

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