Answer:
0.2 milisecond
Step-by-step explanation:
Let the mass of sun is M
mass of star = 2 M
initial radius of the star, R = radius of sun = 7 x 10^5 km
initial time period, T = 10 days
final radius, R' = 10 km
mass remains same.
As no external torque is acting on the star so its angular momentum remains constant.
So, Angular momentum before collapsing = Angular momentum after collapsing
I x ω = constant
![(2)/(5)(2M)* R^(2)* (2\pi )/(T)=(2)/(5)(2M)* R'^(2)* (2\pi )/(T')](https://img.qammunity.org/2020/formulas/physics/high-school/rbwcjlqwqmen8nutyuf2cjht0hctahfjyd.png)
![(R^(2))/(T)=(R'^(2))/(T')](https://img.qammunity.org/2020/formulas/physics/high-school/rz9wj7a29rw5e5zgeoebi7suxi319r65q6.png)
![T'=(R'^(2)T)/(R^(2))](https://img.qammunity.org/2020/formulas/physics/high-school/hq3rz0y5bxqcceh4jbimfyvziiisa6443y.png)
![T'=(10* 10*10)/(7*10^(5)* 7* 10^(5))](https://img.qammunity.org/2020/formulas/physics/high-school/5kwtoxv5e30lcsq4nncedfwfwja5i4jaob.png)
T' = 2.04 x 10^-9 days
T' = 0.2 milisecond