Dynamical behaviour of Near-Earth asteroids in the terrestrial planet region : The role of secular resonances

Planetary and Space Science

Volumn 46, Issue 8, 1998, Pages 905-910

  Michel, Patrick ^a  

^a UNIVERSITÉ CÔTE D'AZUR   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0009241066     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0032-0633(98)00036-1     Document Type: Article

References (17)

1. Bretagnon, P. (1974) Termes à longues périodes dans le système solaire. Astron. Astrophys. 30, 141-154.
2. Bottke, W. F., Nolan, M. C., Melosh, H. J., Vickery, A. M. and Greenberg, R. (1996) Origin of the Spacewatch small Earth-approaching asteroids. Icarus 122, 406-427.
3. Froeschlé, Ch. and Morbidelli, A. (1994) The secular resonances in the Solar System. In Asteroids, Comets, Meteors 1993, ed. A. Milani, M. Di Martino and A. Cellino, pp. 189-204. Kluwer Academic, Dordecht, The Netherlands.
4. Froeschlé, Ch., Farinella, P., Gonczi, R., Hahn, G. and Morbidelli, A. (1995) Secular resonances and the dynamics of Mars-crossing and near-Earth asteroids. Icarus 117, 45-61.
5. Gladman, B. J., Burns, J. A., Duncan, M. J. and Levison, H. F. (1995) The dynamical evolution of lunar impact ejecta. Icarus 118, 302-321.
6. Kozai, Y. (1962) Secular perturbations of asteroids with high inclination and eccentricity. Astron. Journal 67, 591-598.
7. Michel, P. (1997) Effects of linear secular resonances in the region of semimajor axes smaller than 2AU. Icarus 129, 348-366.
8. Michel, P. and Froeschlé, Ch. 1(1997) The location of secular resonances for semimajor axes smaller than 2 AU. Icarus 128, 230-240.
9. Michel, P. and Thomas, F. (1996) The Kozai resonance for nearEarth asteroids with semimajor axes smaller than 2 AU. Astron. Astrophys. 307, 310-318.
10. Michel, P., Farinella, P. and Froeschlé, Ch. (1996a) The orbital evolution of the asteroid Eros and implications for collision with the Earth. Nature 380, 689-691.
11. Michel, P., Froeschlé, Ch. and Farinella, P. (1996b) Dynamical evolution of two near-Earth asteroids to be explored by spacecraft : (433) Eros and (4660) Neureus. Astron. Astrophys. 313, 993-1007.
12. Milani, A., Carpino, M., Hahn, G. and Nobili, A. M. (1989) Dynamics of planet-crossing asteroids : classes of orbital behavior, project Spaceguard. Icarus 78, 212-269.
13. Morbidelli, A. and Henrard, J. (1991) Secular resonances in the asteroid belt : theoretical perturbation approach and the problem of their location. Celest. Mech. 51, 131-167.
14. Öpik, E. J. (1976) Interplanetary Encounters, Elsevier Scientific Publishing Company, Amsterdam/Oxford/New York.
15. Rabinowitz, D. L. (1997) Are main belt asteroids a sufficient source for the Earth approaching asteroids? Part I. Predicted vs observed orbital distributions. Icarus 127, 33-54.
16. Rabinowitz, D. L., Gehrels, T., Scotti, J. V., McMillan, R. S., Perry, M. L., Wisniewski, W., Larson, S. M., Howell, E. S. and Mueller, B. E. A. (1993) Evidence for a near-Earth asteroid belt. Nature 363, 704-706.
17. Williams, J. G. (1969) Secular perturbations in the Solar System. Ph.D. dissertation, University of California, Los Angeles, 1969.