Question #90736
The radius R of collapsing spinning star drops to 1/3 its initial value wheres the mass M remains unchanged. The star spins as a rigid body and its rotational inertia I =2/5 MR^2. The ratio of the new rotational kinetic energy to the initial rotational kinetic energy is
1
Expert's answer
2019-06-12T15:24:26-0400

From the conservation of angular momentum:


Iω=IωI\omega=I'\omega'

25MR2ω=13225MR2ω\frac{2}{5}MR^2\omega=\frac{1}{3^2}\frac{2}{5}MR^2\omega'

ω=9ω\omega'=9\omega

I=19II'=\frac{1}{9}I

The ratio of the new rotational kinetic energy to the initial rotational kinetic energy is


0.5Iω20.5Iω2=9219=9\frac{0.5I'\omega'^2}{0.5I\omega^2}=9^2\frac{1}{9}=9


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