By conservation of angular momentum:
\[ I_1 \omega_1 = I_2 \omega_2 \]
Moment of inertia of a sphere:
\[ I = \frac{2}{5} M R^2 \]
Angular velocity relation:
\[ \omega = \frac{2 \pi}{T} \]
\[ \frac{2}{5} M R^2 \cdot \frac{2 \pi}{T_1} = \frac{2}{5} M \left( \frac{3}{4} R \right)^2 \cdot \frac{2 \pi}{T_2} \]
Simplifying:
\[ \frac{1}{T_1} = \frac{9}{16} \cdot \frac{1}{T_2} \]
\[ T_2 = \frac{16}{9} \cdot T_1 \]
Substituting $T_1 = 24$ hours:
\[ T_2 = \frac{9}{16} \cdot 24 = \frac{27}{2} = 13 \, \text{hours} \, 30 \, \text{minutes}. \]
Step 1: Apply Conservation of Angular Momentum
Initial angular momentum \( L \) must equal final angular momentum \( L' \):
\( L = L' \rightarrow I \cdot \omega = I' \cdot \omega' \).
Since radius reduces to \( \frac{3}{4}r \), moment of inertia becomes \( I' = \frac{2}{5} m \left(\frac{3}{4}r\right)^2 = \frac{9}{16}I \).
So, \( I \cdot \omega = \frac{9}{16}I \cdot \omega' \).
Thus, \( \omega' = \frac{16}{9} \omega \).
Step 2: Relating Angular Velocity and Time Period
The period \( T \) of Earth's rotation is related to angular velocity by:
\( \omega = \frac{2\pi}{T} \).
Therefore,
\( \omega' = \frac{2\pi}{T'} = \frac{16}{9} \omega \).
Hence, \( \frac{2\pi}{T'} = \frac{16}{9} \cdot \frac{2\pi}{T} \).
It leads to:
\( T' = \frac{9}{16} T \).
Given \( T = 24 \) hours, then:
\( T' = \frac{9}{16} \times 24 = 13.5 \) hours.
Final Check
The new duration of Earth's day is 13.5 hours.
Hence, the answer is 13 hours 30 minutes.
A black body is at a temperature of 2880 K. The energy of radiation emitted by this body with wavelength between 499 nm and 500 nm is U1, between 999 nm and 1000 nm is U2 and between 1499 nm and 1500 nm is U3. The Wien's constant, b = 2.88×106 nm-K. Then,

What will be the equilibrium constant of the given reaction carried out in a \(5 \,L\) vessel and having equilibrium amounts of \(A_2\) and \(A\) as \(0.5\) mole and \(2 \times 10^{-6}\) mole respectively?
The reaction : \(A_2 \rightleftharpoons 2A\)