On the classical expansion of the perturbing function in individual orbital elements
Publikation: Beitrag in Fachzeitschrift › Forschungsartikel › Beigetragen › Begutachtung
Beitragende
- Lohrmann Observ, Inst Planetare Geodaesie
Abstract
Starting from the classical expansion of the perturbing function in the three-body problem, the transformation to individual orbital elements is performed in principle up to any degree in small parameters. Some corrections to the results presented in the well-known article by Yuasa on secular perturbations of asteroids are given. Consequences for the expansion of the indirect part of the perturbing function are discussed.
Details
Originalsprache | Englisch |
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Seiten (von - bis) | 147-152 |
Seitenumfang | 6 |
Fachzeitschrift | Celestial mechanics & dynamical astronomy |
Jahrgang | 74 |
Ausgabenummer | 3 |
Publikationsstatus | Veröffentlicht - Juli 1999 |
Peer-Review-Status | Ja |
Externe IDs
Scopus | 0043140190 |
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Schlagworte
Schlagwörter
- asteroid motion, perturbing function, asteroid proper elements, ASTEROID PROPER ELEMENTS