Posted by Lindsay on Friday, December 23, 2011 at 1:25pm.
Look up the contraction ratio Rsun/Rearth. It is about 100
For an exact answe, you will need the radii or diameters of the sun and the earth, to calculate the contraction ratio Rinitial/Rfinal. It is approximatley 100, but you need a more precise vlaue
Remember that angular momentum, I*w, is conserved. That means that M*R^2/P stays the same, where P is the rotation period.
I*w = Constant*M*R^2/P
You can forget about the Mass m and the constant. They stay the same.
Since R decreases by about 100, P must decrease by a factor of about 10^4. That will make the new period about 29.2 days/10^4 = 4 minutes
For the ratio of kinetic energies, remember that for a rotating sphere, KE = (1/2)I*w^2
The KE ratio will be about
(Iw)final*wfinal/[(Iw)initial*winitial]
wfinal/winitial = 10^4
The increase in KE comes from work done by gravity during contraction.
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