The Early Despinning of the Sun

Details The Early Despinning of the Sun The Early Despinning of the Sun

Dec 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969ap%26ss...5..444s&link_type=abstract

Astrophysics and Space Science, Volume 5, Issue 4, pp.444-447

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

It is shown that if the Sun passed through a T Tauri stage, then a mass loss of only 15% would be sufficient to despin the Sun to an angular velocity of 0 (10-5 rad/sec) at 107 years without the additional braking effect of an enhanced magnetic field. Thus the present Sun could have a core rotating at most ten times faster than its surface.

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