Answer:
Part a)
Initial angular speed of the star is
[tex]\omega = 7.27 \times 10^{-6} rad/s[/tex]
Part b)
Final angular speed of the star after it collapse is given as
[tex]\omega = 7.72 rad/s[/tex]
Explanation:
Part a)
As we know that angular speed is given as
[tex]\omega = \frac{2\pi}{T}[/tex]
now we have
[tex]\omega = \frac{2\pi}{10 (24 \times 3600)}[/tex]
[tex]\omega = 7.27 \times 10^{-6} rad/s[/tex]
Part b)
As we know that star collapses due to its own force
So here we can say that angular momentum is conserved here
So we have
[tex]I_1\omega_1 = I_2\omega_2[/tex]
[tex]\frac{2}{5}MR^2 (7.27 \times 10^{-6}) = \frac{2}{5}M(0.001R)^2\omega[/tex]
[tex]\omega = 7.72 rad/s[/tex]