Certain neutron stars (extremely dense stars) are believed to be rotating at about 1.6 rev/s. If such a star has a radius of 48 km, what must be its minimum mass so that material on its surface remains in place during the rapid rotation?

Respuesta :

Answer:

Mass, [tex]M=4.24\times 10^9\ kg[/tex]

Explanation:

Given that,

Angular velocity of the star, [tex]\omega=1.6\ reav/s[/tex]

Radius of the star, r = 48 cm = 0.48 m

The centripetal force acting on the on the star is caused by the gravitational force such that,

[tex]\dfrac{GMm}{r^2}=\dfrac{mv^}{r}[/tex]

[tex]\dfrac{GM}{r}=v^2[/tex]

Since, [tex]v=r\omega[/tex]

[tex]M=\dfrac{r^3\omega^2}{G}[/tex]

[tex]M=\dfrac{(0.48)^3\times (1.6)^2}{6.67\times 10^{-11}}[/tex]

[tex]M=4.24\times 10^9\ kg[/tex]

So, the minimum mass so that material on its surface remains in place during the rapid rotation is [tex]4.24\times 10^9\ kg[/tex]

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