If the Earth were to suddenly contract to $\frac{1}{n}$ th of its present radius without any change in its mass, the duration of the new day will be nearly
From the conservation of momentum, we have $I_{1} \omega_{1}=I_{2} \omega_{2}$ Thus, we get $\frac{2}{5} M R^{2}\left(\frac{2 \pi}{T_{1}}\right)$ $=\frac{2}{5} M \frac{R^{2}}{n^{2}}\left(\frac{2 \pi}{T_{2}}\right)$ Hence, we get $T_{2}=\frac{T_{1}}{n^{2}}=\frac{24}{n^{2}} h$
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Top Questions on System of Particles & Rotational Motion
The system of particles refers to the extended body which is considered a rigid body most of the time for simple or easy understanding. A rigid body is a body with a perfectly definite and unchangeable shape.
The distance between the pair of particles in such a body does not replace or alter. Rotational motion can be described as the motion of a rigid body originates in such a manner that all of its particles move in a circle about an axis with a common angular velocity.
The few common examples of rotational motion are the motion of the blade of a windmill and periodic motion.