Classical Perturbation Theory in Celestial Mechanics. The Equations of Planetary Motion

Author:

Boccaletti Dino,Pucacco Giuseppe

Publisher

Springer Berlin Heidelberg

Reference45 articles.

1. In any case, what makes these periodic solutions so precious for us is that they are, so to speak, the only breach through which we can try to penetrate into a place so far deemed inaccessible“. H. Poincaré: Les Méthodes Nouvelles de la Mécanique Céleste (Gauthiers-Villars, Paris, 1892), Vol. 1, p. 82.

2. For C1 Hamiltonians, the point has been established by Pugh and Robinson. See C. Pugh, C. Robinson: The C1 closing lemma, including Hamiltonians. Erg. Theory and Dyn. Syst. 3, 261–313 (1977).

3. For a demonstration of this statement and for a further deepening of the subject, the reader is referred to C. L. Siegel, J. K. Moser: Lectures on Celestial Mechanics (Springer, 1971), Sect. 21, of which our exposition is an incomplete summary.

4. L. A. Pars: A Treatise on Analytical Dynamics (Heinemann, 1964) Sects. 30.7, 30.8.

5. V. Szebehely: Theory of Orbits (Academic Press, 1967) Sect. 8.6.

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