Dynamical lifetimes of objects injected into asteroid belt resonances

被引:343
作者
Gladman, BJ
Migliorini, F
Morbidelli, A
Zappala, V
Michel, P
Cellino, A
Froeschle, C
Levison, HF
Bailey, M
Duncan, M
机构
[1] ARMAGH OBSERV, COLL HILL, NORTH IRELAND
[2] OSSERV ASTRON TORINO, I-10025 TURIN, ITALY
[3] SW RES INST, BOULDER, CO 80302 USA
[4] QUEENS UNIV, DEPT ANAT, KINGSTON, ON K7L 3N6, CANADA
关键词
D O I
10.1126/science.277.5323.197
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Numerical simulations of particles placed in orbital resonances in the main asteroid belt show that the typical dynamical lifetimes of objects that could become near-Earth asteroids or meteorites are only a few million years, with the majority destroyed by being transferred to Jupiter-crossing orbits or being driven into the sun. Particles that fortuitously migrate to the terrestrial planet region may be pushed to high-inclination orbits by resonances but are still dynamically eliminated on time scales of similar to 10 million years, These shorter lifetimes may require a reassessment of our qualitative understanding about near-Earth asteroids and meteorite delivery.
引用
收藏
页码:197 / 201
页数:5
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