Asteroid orbits in mixed resonances: Some numerical experiments

Planetary and Space Science

Volumn 49, Issue 8, 2001, Pages 793-797

  Vakhidov, Akmal A ^a  

^a DRESDEN UNIVERSITY OF TECHNOLOGY   (Germany)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0035399818     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0032-0633(01)00030-7     Document Type: Article

References (9)

1. Ferraz-Mello, S., 1999. Slow and fast diffusion in asteroid-belt resonances: a review. Celestial Mech. Dyn. Astronom. 73, 25-37.
2. Hanslmeier, A., Dvorak, R., 1984. Numerical integration with Lie-series. Astronom. Astrophys. 132, 203-207.
3. Michel, P., 1997. Effects of linear secular resonances in the region of semimajor axes smaller than 2AU. Icarus 129, 348-366.
4. Michel, P., Froeschle, C., 1997. The location of linear secular resonances for semimajor axes smaller than 2AU. Icarus 128, 230-240.
5. Morbidelli, A., Nesvorny, D., 1999. Numerous weak resonances drive asteroids toward terrestrial planets orbits. Icarus 139, 295-308.
6. Nesvorny, D., Morbidelli, A., 1998. Three-body mean-motion resonances and the chaotic structure of the asteroid belt. Astronom. J. 116, 3029-3037.
7. Quinlan, G.D., Tremaine, S., 1990. Symmetric multistep methods for the numerical integration of planetary orbits. Astronom. J. 100, 1694-1700.
8. Sidlichovsky, M., 1999. On stable chaos in the asteroid belt. Celestial Mech. Dyn. Astronom. 73, 77-86.
9. Tupikova, I.V., Vakhidov, A.A., Soffel, M., 1999. Explicit semianalytical theory of asteroid motion. Celestial Mech. Dyn. Astronom. 73, 87-96.