Resum
We consider the planar restricted three-body problem and the collinear equilibrium point L3, as an example of a center×saddle equilibrium point in a Hamiltonian with two degrees of freedom. We explore numerically the existence of symmetric and non-symmetric homoclinic orbits to L3, when varying the mass parameter μ. Concerning the symmetric homoclinic orbits (SHO), we study the multi-round, m-round, SHO for m ≥ 2. More precisely, given a transversal value of μ for which there is a 1-round SHO, say μ1, we show that for any m ≥ 2, there are countable sets of values of μ, tending to μ1, corresponding to m-round SHO. Some comments on related analytical results are also made. © Springer Science+Business Media B.V. 2009.
| Idioma original | Anglès |
|---|---|
| Pàgines (de-a) | 197-210 |
| Revista | Celestial Mechanics and Dynamical Astronomy |
| Volum | 105 |
| Número | 1 |
| DOIs | |
| Estat de la publicació | Publicada - 1 d’oct. 2009 |
Fingerprint
Navegar pels temes de recerca de 'Dynamical aspects of multi-round horseshoe-shaped homoclinic orbits in the RTBP'. Junts formen un fingerprint únic.Com citar-ho
- APA
- Author
- BIBTEX
- Harvard
- Standard
- RIS
- Vancouver