On the transport of bodies within and from the asteroid belt

Meteoritics and Planetary Science

Volumn 35, Issue 2, 2000, Pages 331-340

  Franklin, Fred ^a   Lecar, Myron ^a  

^a HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

ASTEROID; METEORITE;

EID: 0034163922     PISSN: 10869379     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1945-5100.2000.tb01778.x     Document Type: Article

References (21)

1. BELL J., DAVIS D., HARTMANN W. K. AND GAFFEY M. (1989) Asteroids: The big picture. In Asteroids II (eds. R. Binzel, T. Gehrels and M. Matthews), pp. 921-945. Univ. Arizona Press, Tucson, Arizona, USA.
2. DAVIS D., WEIDENSCHILLING S., FARINELLA P. PAOLICCHI P. AND BINZEL R. (1989) Asteroid collisional history: Effects on sizes and spins. In Asteroids II (eds. R. Binzel, T. Gehrels and M. Matthews), pp. 805-826. Univ. Arizona Press, Tucson, Arizona, USA.
3. CAMERON A. G. W (1995) The first ten million years of the solar nebula. Meteoritics 30, 133-161.
4. 6. Astron. Astrophys. 179, 294-303.
5. GRADIE J., CHAPMAN C. AND TEDESCO E. (1989) Distribution of taxonomic classes and the compositional structure of the asteroid belt. In Asteroids II (eds. R. Binzel, T. Gehrels and M. Matthews), pp. 316-335. Univ. Arizona Press, Tucson, Arizona, USA.
6. HAYASHI C. (1981) Formation of the Planets. In Fundamental Problems in the Theory of Stellar Evolution (eds. D. Sugimoto, D. Q. Lamb and D. N. Schramm), pp. 113-128. D. Reidel, Dordrecht, the Netherlands.
7. KENYON S. AND HARTMANN L. (1995) Pre-main sequence evolution in the Taurus-Auriga molecular cloud. Astrophys. J. Suppl. 101, 117-171.
8. KNEZEVIĆ Z., MILANI A., FARINELLA P., FROESCHLÉ CH. AND FROESCHLÉ CL. (1991) Secular resonances from 2 to 50 AU. Icarus 93, 316-330.
9. LEMAÎTRE A. AND DUBRU P. (1991) Secular resonances in the primitive solar nebula. Cel. Mech. 52, 57-78.
10. LECAR M. AND FRANKLIN F. (1973) On the original distribution of the Asteroids. I. Icarus 20, 422-436.
11. LECAR M. AND FRANKLIN F. (1997) The solar nebula, secular resonances, gas drag and the asteroid belt. Icarus 129, 134-146
12. MILANI A., CARPINO M., HAHN G. AND NOBILI A. (1989) Dynamics of planet crossing asteroids: Classes of orbital behavior. Icarus 78, 212-269.
13. 6 and 3:1 resonances: Implications for V-type near Earth asteroids and HED meteroites. Meteorit. Planet. Sci. 32, 903-916.
14. NAGASAWA M., TANAKA H. AND IDA S. (2000) Orbital evolution of asteroids during depletion of the solar nebula. Astron. J. (in press).
15. PETIT J-M., MORBIDELLI A. AND VALSECCHI G. (1999) Large scattered planetesimals and the excitation of the small body belts. Icarus 141, 367-387.
16. VEVERKA J. ET AL (1997) NEAR's flyby of 253 Mathilde: Images of a C asteroid. Science 278, 2109-2114.
17. WARD W. R. (1980) Scanning secular resonances: A cosmogonical broom? (abstract). Lunar Planet. Sci. 11, 1199-1201.
18. WARD W. R. (1981) Solar nebula dispersal and the stability of the planetary system I. Scanning secular resonance theory. Icarus 47, 234-264.
19. WARD W. R., COLOMBO G. AND FRANKLIN F. (1976) Solar spin-down, secular resonance and the orbit of Mercury. Icarus 28, 441-452.
20. WETHERILL G. W. (1988) Where do the Apollo objects come from? Icarus 76, 1-18.
21. WISDOM J. L. (1983) Chaotic behavior and the origin of the 3:1 Kirkwood gap. Icarus 56, 51-74.