As per the question,
Mass of the spherical star=M
Radius of the spherical star= R
Radius of the other star"=10^{-5}R"
rotational speed of the first star"\\omega_1= 1\/25 rev\/day"
rotational speed of the second star "\\omega_2=?"
Now, applying the conservation of angular momentum,
"I_1\\omega_1=I_2\\omega_2"
"\\Rightarrow \\omega_2=\\dfrac{I_1\\omega_1}{I_2}=\\dfrac{10^{10}}{25}=4\\times 10^8 rev\/day"
"\\omega_2=4.6\\times 10^3 rev\/sec"
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