Step 1: Weight reduction due to rotation.
The centrifugal force due to the Earth's rotation at the equator is given by \( F_{\text{centrifugal}} = m \omega^2 R \), where \( \omega \) is the angular velocity of the Earth's rotation, \( R \) is the radius of the Earth, and \( m \) is the mass. The apparent weight will be reduced by this centrifugal force.
Step 2: Weight comparison.
The apparent weight at the equator is reduced by \( \frac{1}{25} \), which means
\[
\frac{m g - m \omega^2 R}{m g} = \frac{1}{25} \Rightarrow 1 - \frac{\omega^2 R}{g} = \frac{1}{25}
\]
Solving for \( \omega \), we get:
\[
\omega = 7.91 \times 10^{-4} \, \text{rad/s}
\]
Step 3: Conclusion.
The correct answer is (B), \( 7.91 \times 10^{-4} \, \text{rad/s} \).