Cosmogony of the asteroidal belt

Hannes Alfvén, Wing Huén Ip, Martin D. Burkenroad

研究成果: 雜誌貢獻期刊論文同行評審

5 引文 斯高帕斯(Scopus)

摘要

WE have to derive the state of partial corotation in a way which, by being very simple, stresses its character as a basic state in cosmic plasma dynamics. We also substitute the mass density (m, a) for the number density (n, a) in the plot of asteroids, as a function of their semimajor axis a. This gives a better definition to the limits of the main belt, and demonstrates more clearly that the asteroids-like the Saturnian rings-have condensed from a partially corotating plasma.

原文???core.languages.en_GB???
頁(從 - 到)634-636
頁數3
期刊Nature
250
發行號5468
DOIs
出版狀態已出版 - 1974

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