Gravitational stirring of the asteroid belt by Jupiter zone bodies.

研究成果: 雜誌貢獻期刊論文同行評審

16 引文 斯高帕斯(Scopus)


Explores the scenario that the large random velocity (approx 5 km/s) among the asteroids is the result of dynamical interaction between the original population of the parent asteroids in near-circular orbits with some large planetesimals (JZB) scattered from the accretion zone of Jupiter. The statistical property of such a gravitational scattering process is evaluated using a Monte Carlo method. It is found that a few tens of JZB with individual masses reaching 3 X 1027 g would be needed to provide the necessary orbital velocity dispersion. -Author

頁(從 - 到)44-51
期刊Gerlands Beitrage zur Geophysik
出版狀態已出版 - 1987


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