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If a body of mass m is raised to height ...

If a body of mass m is raised to height 2 R from the earth`s surface, then the change in potential energy of the body is (R is the radius of earth)

A

mgR

B

12 mgR

C

`2/3 mgR`

D

9 mgR

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The correct Answer is:
To find the change in potential energy of a body of mass \( m \) raised to a height of \( 2R \) from the Earth's surface, we can follow these steps: ### Step 1: Understand the initial and final positions - The initial position of the body is at the Earth's surface, which we can denote as height \( h_1 = 0 \). - The final position of the body is at a height \( h_2 = 2R \) from the Earth's surface. ### Step 2: Calculate the gravitational potential energy at the initial position The gravitational potential energy (U) at a distance \( r \) from the center of the Earth is given by the formula: \[ U = -\frac{G M m}{r} \] where: - \( G \) is the universal gravitational constant, - \( M \) is the mass of the Earth, - \( m \) is the mass of the body, - \( r \) is the distance from the center of the Earth. At the Earth's surface, the distance \( r_1 \) is equal to the radius of the Earth \( R \): \[ U_1 = -\frac{G M m}{R} \] ### Step 3: Calculate the gravitational potential energy at the final position At the height of \( 2R \), the distance \( r_2 \) from the center of the Earth is: \[ r_2 = R + 2R = 3R \] Thus, the gravitational potential energy at this height is: \[ U_2 = -\frac{G M m}{3R} \] ### Step 4: Calculate the change in potential energy The change in potential energy (\( \Delta U \)) is given by: \[ \Delta U = U_2 - U_1 \] Substituting the values we calculated: \[ \Delta U = \left(-\frac{G M m}{3R}\right) - \left(-\frac{G M m}{R}\right) \] This simplifies to: \[ \Delta U = -\frac{G M m}{3R} + \frac{G M m}{R} \] \[ \Delta U = G M m \left(-\frac{1}{3R} + \frac{1}{R}\right) \] \[ \Delta U = G M m \left(\frac{-1 + 3}{3R}\right) \] \[ \Delta U = G M m \left(\frac{2}{3R}\right) \] ### Step 5: Express in terms of \( g \) We know that \( g = \frac{G M}{R^2} \). Thus, we can express \( G M \) as \( g R^2 \): \[ \Delta U = \frac{2}{3R} \cdot g R^2 \cdot m \] \[ \Delta U = \frac{2}{3} g m R \] ### Final Answer The change in potential energy of the body when raised to a height of \( 2R \) from the Earth's surface is: \[ \Delta U = \frac{2}{3} g m R \]
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