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Angular momentum problem

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This is an old revision of this page, as edited by 177.40.147.126 (talk) at 17:02, 29 May 2013 (Asked for a reliable source to back up the claim that the Sun does not, in fact, hold the majority of the solar system's angular momentum.). The present address (URL) is a permanent link to this revision, which may differ significantly from the current revision.

The angular momentum problem is a problem in astrophysics by which the angular momentum of a protoplanetary disk is misappropriated when compared to models during stellar birth. The Sun and other stars are predicted by models to be rotating considerably faster than they actually are. The Sun, for example, only accounts for about 0.3 percent of the total angular momentum of the solar system[citation needed] while about 60% is attributed to Jupiter.[1]

References

  1. ^ "The Angular Momentum Problem". Lifeng.lamost.org. Retrieved 2013-03-29.