An interpretation of the distribution of angular momentum in the solar system

Details An interpretation of the distribution of angular momentum in the solar system An interpretation of the distribution of angular momentum in the solar system

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976acasn..17..165d&link_type=abstract

Acta Astronomica Sinica, vol. 17, Dec. 1976, p. 165-175. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

1

Angular Momentum, Momentum Theory, Nebulae, Solar System, Gravitational Collapse, Momentum Transfer, Planetary Evolution, Stellar Evolution, Stellar Mass Ejection

Scientific paper

A scenario for the evolution of the solar system is described which accounts for the present distribution of angular momentum. Before entering the main sequence, the sun while undergoing gravitational contraction lost most of its angular momentum, but the bulk of matter ejected by the sun did not enter the nebulous disk. The planetary material already possessed enough angular momentum, and did not need the sun to transfer angular momentum to it.

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