We use cookies to distinguish you from other users and to provide you with a better experience on our websites. Close this message to accept cookies or find out how to manage your cookie settings.
Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.
We propose here the first results of the semi analytical method of Henrard(1990) applied to the calculation of proper elements for the asteroids.
Henrard, J.: 1990, “A Semi-Numerical Perturbation Method for Separable Hamiltonian Systems”, Celest. Mech. and Dyn. Astr.49, 43–67Google Scholar
Knezevic, : 1988, “Asteroid Mean Orbital Elements”, Bull. Obs. Astron. Belgrade139, 1–6Google Scholar
Knezevic, : 1989, “Asteroid long-periodic perturbations: the second order Hamiltonian”, Celest. Mech. and Dyn. Astr.46, 147–158CrossRefGoogle Scholar
Kozai, Y.: 1985, “Stability of Asteroid Motions”, in Resonances in the Motion of Planets, Satellites and Asteroids, Ferraz-Mello, S., Sessin, W., ed(s)., 117–127, Universidade de Sao Paulo, Sao paulo, BresilGoogle Scholar
Lemaitre, A., Morbidelli, A.: 1992?, “Calculation of Proper Elements for high inclined asteroidal orbits by Henrard's semi - analytical Perturbation Method”, Celest. Mech. and Astr. Dyn., in preparationGoogle Scholar
Milani, A., Knezevic, Z.: 1990, “Secular Perturbation Theory and Calculation of Asteroid Proper Elements”, Celest. Mech. and Dyn. Astr.49, 347–411CrossRefGoogle Scholar
Williams, J.G.: 1969, “Secular Perturbations in the Solar System”, Ph.D. Dissertation, University of California, Los AngelesGoogle Scholar
Yuasa, M.: 1973, “Theory of Secular Perturbations of asteroids Including Terms of Higher Orders and Higher Degrees”, Publ. Astron. Soc. Japan25, 399–445Google Scholar