Origin and evolution of near earth asteroids

Celestial Mechanics and Dynamical Astronomy

Volumn 73, Issue 1-4, 1999, Pages 39-50

  Morbidelli, A ^a  

^a UNIVERSITÉ CÔTE D'AZUR   (France)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0003779342     PISSN: 09232958     EISSN: None     Source Type: Journal    
DOI: 10.1007/978-94-011-4527-5_4     Document Type: Article

References (36)

1. Arnold, J.R.: 1965, The origin of meteorites as small bodies II. The model, Ap. J, 141, 1536-1547.
2. Burns, J.A., Lamy, P.H. and Soter, S. : 1979, Radiation forces on small particles in the solar system, Icarus, 40, 1-48.
3. Farinella, P., Gonczi, R., Froeschlé, Ch. and Froeschlé, C.: 1993, The injection of asteroid fragments into resonance, Icarus, 101, 174-187.
4. Farinella, P., Froeschlé,Ch., Froeschlé, C., Gonczi, R., Hahn, G., Morbidelli, A. and Valsecchi, G.B.: 1994, Asteroids falling onto the Sun, Nature, 371, 315-317.
5. Farinella, P., Vokrouhlický, D. and W.K. Hartmann, W.K.: 1998, Meteorite delivery via Yarkovsky orbital drift, Icarus, 132, 378-387.
6. Farinella, P. and Vokrouhlicky, D.: 1998, Semimajor axis mobility of asteroidal fragments, Science, submitted.
7. Froeschlé, Ch. and Morbidelli, A.: 1994, The secular resonances in the solar system, I-in Asteroids, Comets, and Meteors, 1993 (A. Milani, M. Di Martino, A. Cellino, Eds.) Kluwer: Boston, 189-204.
8. Gladman B., F. Migliorini, F., A. Morbidelli, A., Zappalá, V., P. Michel, P., A. Cellino, A., Ch. Froeschlé, Ch., Levison, H., Bailey, M. and Duncan, M.: 1997, Dynamical lifetimes of objects injected into asteroid main belt resonances, Science, 277, 197-201.
9. Greenberg R. and Nolan, M.: 1989, Delivery of asteroids and meteorites to the inner solar system, in Asteroids II, eds. R.P. Binzel, T. Gehrels and M.S. Matthews (Tucson: Univ. Arizona Press), 778-804.
10. Greenberg R. and Nolan, M.: 1993, Dynamical relationships of near-Earth asteroids to main-belt asteroids, in Resources of Near-Earth space, J. Lewis et al. eds. (Tucson: Univ. Arizona Press), 473-492.
11. Kirkwood, D.: 1866, in Proceedings of the American Association for the Advancement of Science for 1866.
12. Levison, H.F. and Duncan, M.: 1994, The long term dynamical behaviour of short period comets, Icarus, 108, 18-36.
13. Menichella M., Paolicchi, P. and Farinella, P.: 1996, The main belt as a source of Near Earth-Asteroids, Earth, Moon and Planets, 72, 133-149.
14. Michel, P., Froeschlé, Ch. and Farinella, P.: 1996, Dynamical evolution of NEAs: close encounters, secular perturbations and resonances, Earth Moon and Planets, 72, 151-164.
15. Michel, P., and Froeschlé, Ch,: 1997, The location of secular resonances for semimajor axes smaller than 2 AU, Icarus, 128, 230-240.
16. Michel, P.: 1997, Effects of linear secular resonances in the region of semimajor axes smaller than 2 AU, Icarus, 129, 348-366.
17. Migliorini, F., P. Michel, P., Morbidelli, A., Nesvorný, D. and Zappalà, V.: 1998, Origin of Earth-crossing asteroids: the new scenario, Science, 281, 2022-2024.
18. Milani, A. and Knežević, Z.: 1994, Asteroid proper elements and the chaotic structure of the asteroid main belt, Icarus, 107, 219-254.
19. Moons M.: 1997, Review of the dynamics in the Kirkwood gaps, Cel. Mech., 65, 175-204.
20. Moons M. and Morbidelli, A.: 1995, Secular resonances inside mean-motion commensurabilities: the 4/1, 3/1, 5/2 and 7/3 cases, Icarus, 114, 33-50.
21. Morbidelli, A.: 1993, Asteroid secular resonant proper elements, Icarus, 105, 48-66.
22. Morbidelli, A. and Gladman, B.: 1998, Orbital and temporal distribution of meteorites originating in the asteroid belt, Meteoritics and Planet. Sci., 33, 999-1016.
23. Morbidelli A. and Nesvorný, D.: 1998, Numerous weak resonances drive asteroids towards terrestrial planets orbits, Icarus, submitted.
24. Morrison, D. Ed.: 1992, The Spaceguard Survey. Report of the NASA near-Earth object detection workshop, NASA, Washington, D.C.
25. Rubincam, D.P.: 1995, Asteroid orbit evolution due to thermal drag, JGR, 100, 1585-1594.
26. Öpik, E.J.: 1976, Interplanetary Encounters, Elsevier Press, New York. 155 pp.
27. Valsecchi, G.B., Morbidelli, A., Gonczi, R., Farinella, P., Froeschlé, Ch., Froeschlé, C.: 1995, The dynamics of objects in orbits resembling that of P/Encke, Icarus, 117, 45-61.
28. Wetherill, G.W.: 1976, Where do meteorites come from? A re-evaluation of the Earth-crossing Apollo objects as sources of chondritic meteorites, Geochimica et Cosmochimica Acta, 40, 1297-1317.
29. Wetherill, G.W.: 1979, Steady-state populations of Apollo-Amor objects, Icarus, 37, 96-112.
30. Wetherill, G.W.: 1985, Asteroidal sources of ordinary chondrites, Meteoritics, 20, 1-22.
31. Wetherill, G.W.: 1987, Dynamic relationship between asteroids, meteorites and Apollo-Amor objects, Phil. Trans. Royal Soc. London, 323, 323-337.
32. Wetherill, G.W.: 1988, Where do the Apollo objects come from? Icarus, 76, 1-18.
33. Williams, J. G., and Faulkner, J.: 1981, The position of secular resonance surfaces, Icarus, 46, 390-399.
34. Wisdom, J.: 1983, Chaotic behavior and the origin of the 3/1 Kirkwood gap, Icarus, 56, 51-74.
35. Wisdom, J. and Holman, M.: 1991, Symplectic maps for the N-body problem, Astron. J., 102, 1528-1538.
36. Zappalá, V., Cellino, A., Gladman, B., Manley, S. and Migliorini, F.: 1998, Note: asteroid showers on Earth after family break-up events, Icarus, 134, 176-179.