Application of the Brown-Shook model to the Kirkwood gaps and resonant asteroids

研究成果: 雜誌貢獻期刊論文同行評審

3 引文 斯高帕斯(Scopus)

摘要

The mathematical model developed by Brown and Shook is used to explain the absence of asteroids in the Kirkwood gaps as well as the existence of some resonant asteroids with orbital periods commensurable to that of Jupiter. In addition, this model can possibly explain the biased number distributions at the commensurable positions of both resonant gaps and clusters. However, this resonant model is probably not applicable to the Saturnian ring system due to the possible cosmogonic plasma process during its formation.

原文???core.languages.en_GB???
頁(從 - 到)73-79
頁數7
期刊Celestial Mechanics
9
發行號1
DOIs
出版狀態已出版 - 3月 1974

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