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A body of mass m taken from the earth's...

A body of mass m taken from the earth's surface to the height equal to the twice the earth radius R of the earth . The change in potential energy of the body will be

A

`2mgR`

B

`(2)/(3) m g R`

C

`3 mg R`

D

`(mgR)/(3)`

Text Solution

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The correct Answer is:
To find the change in potential energy of a body of mass \( m \) taken from the Earth's surface to a height equal to twice the Earth's radius \( R \), we can follow these steps: ### Step-by-Step Solution: 1. **Identify Initial and Final Positions**: - The initial position of the body is at the Earth's surface, which is at a distance \( R \) from the center of the Earth. - The final position of the body is at a height equal to twice the Earth's radius, which means it is at a distance of \( R + 2R = 3R \) from the center of the Earth. 2. **Calculate Initial Potential Energy**: - The formula for gravitational potential energy \( U \) at a distance \( r \) from the center of the Earth is given by: \[ U = -\frac{GMm}{r} \] - Therefore, the initial potential energy \( U_i \) at distance \( R \) is: \[ U_i = -\frac{GMm}{R} \] 3. **Calculate Final Potential Energy**: - The final potential energy \( U_f \) at distance \( 3R \) is: \[ U_f = -\frac{GMm}{3R} \] 4. **Find Change in Potential Energy**: - The change in potential energy \( \Delta U \) is given by: \[ \Delta U = U_f - U_i \] - Substituting the values we calculated: \[ \Delta U = \left(-\frac{GMm}{3R}\right) - \left(-\frac{GMm}{R}\right) \] - Simplifying this expression: \[ \Delta U = -\frac{GMm}{3R} + \frac{GMm}{R} \] - Finding a common denominator (which is \( 3R \)): \[ \Delta U = -\frac{GMm}{3R} + \frac{3GMm}{3R} = \frac{2GMm}{3R} \] 5. **Express in Terms of Acceleration Due to Gravity**: - We know that the acceleration due to gravity \( g \) at the surface of the Earth is given by: \[ g = \frac{GM}{R^2} \] - Rearranging gives \( GM = gR^2 \). - Substituting this into our expression for \( \Delta U \): \[ \Delta U = \frac{2(gR^2)m}{3R} = \frac{2g m R}{3} \] ### Final Result: Thus, the change in potential energy of the body is: \[ \Delta U = \frac{2}{3} mgR \]

To find the change in potential energy of a body of mass \( m \) taken from the Earth's surface to a height equal to twice the Earth's radius \( R \), we can follow these steps: ### Step-by-Step Solution: 1. **Identify Initial and Final Positions**: - The initial position of the body is at the Earth's surface, which is at a distance \( R \) from the center of the Earth. - The final position of the body is at a height equal to twice the Earth's radius, which means it is at a distance of \( R + 2R = 3R \) from the center of the Earth. ...
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