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Formation of the Planets and Asteroids: Some Difficulties of Accretion Theories

Published online by Cambridge University Press:  25 April 2016

M. M. Komesaroff
M. M. Komesaroff*
Affiliation:
Division of Radiophysics, CSIRO, Sydney
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Extract

Figure 1 is a plot of spin angular momentum, J, against mass, m, for some of the main sequence stars, the planets and the asteroids.

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Publications of the Astronomical Society of Australia , Volume 5 , Issue 4 , 1984 , pp. 457 - 459
Copyright
Copyright © Astronomical Society of Australia 1984

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