| Full text | |
| Author(s): |
Total Authors: 2
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| Affiliation: | [1] Univ Estadual Paulista UNESP, Dept Estat Matemat Aplicada & Computacao, Inst Geociencias & Ciencias Exatas, BR-13506900 Rio Claro, SP - Brazil
Total Affiliations: 1
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| Document type: | Journal article |
| Source: | CELESTIAL MECHANICS & DYNAMICAL ASTRONOMY; v. 115, n. 1, p. 59-79, JAN 2013. |
| Web of Science Citations: | 3 |
| Abstract | |
An analytical expansion of the disturbing function arising from direct planetary perturbations on the motion of satellites is derived. As a Fourier series, it allows the investigation of the secular effects of these direct perturbations, as well as of every argument present in the perturbation. In particular, we construct an analytical model describing the evection resonance between the longitude of pericenter of the satellite orbit and the longitude of a planet, and study briefly its dynamic. The expansion developed in this paper is valid in the case of planar and circular planetary orbits, but not limited in eccentricity or inclination of the satellite orbit. (AU) | |
| FAPESP's process: | 10/52715-5 - Direct planetary perturbations on satellite motions |
| Grantee: | Julien Henri Pierre Frouard |
| Support Opportunities: | Scholarships in Brazil - Post-Doctoral |