A note on the cosmogony of the asteroidal belt

研究成果: 雜誌貢獻期刊論文同行評審

1 引文 斯高帕斯(Scopus)

摘要

Several arguments based on the orbital dynamics of the asteroids are used to support the idea that the original solar nebula might not necessarily be the Laplacian type of thin disk-like structure. The orbital distribution of the large asteroids is suggested to be a direct result of their accretions of condensed grains in eccentric orbits via the jet stream process.

原文???core.languages.en_GB???
頁(從 - 到)235-241
頁數7
期刊Astrophysics and Space Science
45
發行號1
DOIs
出版狀態已出版 - 11月 1976

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