MHT CET · Physics · Gravitation

The difference in the acceleration due to gravity at the pole and equator is ( \(g=\) acceleration due to gravity, \(R=\) radius of earth, \(\theta=\) latitude, \(\omega=\) angular velocity, \(\cos 0^{\circ}=1, \cos 90^{\circ}=0\) )

A \(R \omega^2 \cos ^2 \theta\)
B \(R \omega^2\)
C \(\frac{R \omega^2}{g^2}\)
D \(\omega \cos ^2 \theta\)

Verified Solution

Answer & Solution

Correct Answer

(B) \(R \omega^2\)

Step-by-step Solution

Detailed explanation

Acceleration due to gravity at a place of latitude \(\theta\) due to rotation of earth is \(g^{\prime}=g-R \omega^2 \cos ^2 \theta\)
At equator, \(\theta=0, \cos 0=1\)
\(\therefore g^{\prime}=g_e=g-R \omega^2\)
At poles, \(\theta=90, \cos 90=0\)
\(\therefore g^{\prime}=g_p=g\)
\(\therefore g_p-g_e=g-\left(g-R \omega^2\right)=R \omega^2\)

Apply the relevant identity from the chapter and substitute the values established in the previous step, keeping the original constraint in view.

Use the simplified expression to isolate the unknown, then plug the result back into the question setup to confirm the working is internally consistent.

Cross-check against a boundary or limiting case. Both the dimensional balance and the qualitative behaviour at the extreme should agree with the candidate answer.

Combine the steps above to identify the correct option. The remaining choices each fail at least one of the consistency, dimensional, or boundary checks.

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