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Under some circumstances, a star can collapse into an extremely dense object made mostly of neutrons and called a neutron star. The density of a neutron star is roughly 10^14 times as great as that of ordinary solid matter. Suppose we represent the star as a uniform, solid, rigid sphere, both before and after the collapse. The star's initial radius was 7.0×10^5 km (comparable to our sun); its final radius is 18km .

User Anvy Zhang
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Answer:

The angular speed of the neutron star is 3130.5 rad/s.

Step-by-step explanation:

Given that,

Initial radius
r_(1)=7*10^(5)\ km

Final radius
r_(2)=18 km

Density of a neutron
\rho= 10^(14)

Equal masses of two stars
m_(1)=m_(2)

Suppose, If the original star rotated once in 35 days, find the angular speed of the neutron star

Time period of original star T = 35 days = 3024000 s

We need to calculate the initial angular speed of original star

Using formula of angular star


\omega=(2\pi)/(T)

Put the value into the formula


\omega_(1)=(2\pi)/(3024000)


\omega_(1)=0.00207*10^(-3)\ rad/s

Let the initial moment of inertia of the star is


I_(1)=m_(1)r_(1)^2

Final moment of inertia of the star is


I_(2)=m_(2)r_(2)^2

From the conservation of angular momentum


I_(1)\omega_(1)=I_(2)\omega_(2)


\omega_(2)=(I_(1)\omega_(1))/(I_(2))


\omega_(2)=(m_(1)r_(1)^2\omega_(1))/(m_(2)r_(2)^2)

Put the value into the formula


\omega_(2)=((7.0*10^(5))^2*0.00207*10^(-3))/(18^2)


\omega_(2)=3130.5\ rad/s

Hence, The angular speed of the neutron star is 3130.5 rad/s.

User TimB
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