MHT CET · Physics · Rotational Motion
A body is situated on the surface of the earth becomes weightless at equator when the rotational kinetic energy of the earth reaches a critical value ' \(K\) '. The value of \(K\) is given by [ \(\mathrm{g}\) = gravitational acceleration on earth's surface, \(M=\) mass of the earth and \(\mathrm{R}=\) radius of the earth]
- A \(\frac{1}{2} \mathrm{MgR}\)
- B \(\frac{1}{3} \mathrm{MgR}\)
- C \(\frac{1}{4} \mathrm{MgR}\)
- D \(\frac{1}{5} \mathrm{MgR}\)
Answer & Solution
Correct Answer
(D) \(\frac{1}{5} \mathrm{MgR}\)
Step-by-step Solution
Detailed explanation
A body will become weightless at equator if \(R \omega^2=g\) or \(\omega^2=\frac{g}{R}\) Kinetic energy of the earth, \(\mathrm{K}=\frac{1}{2} \mathrm{I} \omega^2\)
For a solid sphere, \(\mathrm{I}=\frac{2}{5} \mathrm{MR}^2\)
(M is mass of the earth)
\(\therefore \mathrm{K}=\frac{1}{2} \times \frac{2}{5} \mathrm{MR}^2 \times \frac{\mathrm{g}}{\mathrm{R}}=\frac{1}{5} \mathrm{MgR}\)
For a solid sphere, \(\mathrm{I}=\frac{2}{5} \mathrm{MR}^2\)
(M is mass of the earth)
\(\therefore \mathrm{K}=\frac{1}{2} \times \frac{2}{5} \mathrm{MR}^2 \times \frac{\mathrm{g}}{\mathrm{R}}=\frac{1}{5} \mathrm{MgR}\)
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