Secular perturbations of a general second-order planetary theory developed with the aid of Poincare's canonical variables and von Zeipel's method

Details Secular perturbations of a general second-order planetary theory developed with the aid of Poincare's canonical variables and von Zeipel's method Secular perturbations of a general second-order planetary theory developed with the aid of Poincare's canonical variables and von Zeipel's method

Oct 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974crasm.279..671m&link_type=citations

Academie des Sciences (Paris), Comptes Rendus, Serie A - Sciences Mathematiques, vol. 279, no. 16, Oct. 14, 1974, p. 671-674. In

Mathematics

1

Celestial Mechanics, Many Body Problem, Orbit Perturbation, Planetology, Solar Orbits, Canonical Forms, Hamiltonian Functions, Secular Variations, Three Body Problem, Two Body Problem, Von Zeipel Method

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