Orbital evolution of asteroids in the 5:3 conmensurability
This paper deals with the orbital evolution of 25 fictitious asteroids generated in the space zone corresponding to means motions in the 5:3 commensurability with Jupiter. Regarding the extension of the gap from a₁=3.63 UA. to a₂=3.76 UA. The eccentricities for t = 0 vary from 0.0 to 0.4. The solar...
Guardado en:
| Autores principales: | , |
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| Formato: | Articulo Comunicacion |
| Lenguaje: | Español |
| Publicado: |
1992
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/145397 |
| Aporte de: |
| Sumario: | This paper deals with the orbital evolution of 25 fictitious asteroids generated in the space zone corresponding to means motions in the 5:3 commensurability with Jupiter. Regarding the extension of the gap from a₁=3.63 UA. to a₂=3.76 UA. The eccentricities for t = 0 vary from 0.0 to 0.4. The solar system model used includes perturbations from Venus to Saturn. The numerical integration of the equations of motion were performed with the N-Body Program by Schubart and Stumpff, for an integration time of 5x10⁴ years. The results can be analyzed considering the behaviour observed according to the initial eccentricities. |
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