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Gravitational potential energy of body o...

Gravitational potential energy of body of mass `m` at a height of `h` above the surface of earth (M = mass of earth , R = radius of earth) is

A

`(GMm)/(h)`

B

`(GMm)/((R+h))`

C

`(-GM)/((R+h))`

D

`-(GMm)/((R+h))`

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The correct Answer is:
To find the gravitational potential energy (U) of a body of mass \( m \) at a height \( h \) above the surface of the Earth, we can use the formula for gravitational potential energy in the context of gravitational fields. ### Step-by-Step Solution: 1. **Understand the Gravitational Potential Energy Formula**: The gravitational potential energy \( U \) of a mass \( m \) in a gravitational field created by a mass \( M \) (in this case, the Earth) at a distance \( r \) from the center of the mass \( M \) is given by the formula: \[ U = -\frac{G M m}{r} \] where \( G \) is the universal gravitational constant. 2. **Identify the Distance from the Center of the Earth**: When the body is at a height \( h \) above the surface of the Earth, the distance \( r \) from the center of the Earth to the body is: \[ r = R + h \] where \( R \) is the radius of the Earth. 3. **Substitute \( r \) into the Potential Energy Formula**: Substitute \( r = R + h \) into the gravitational potential energy formula: \[ U = -\frac{G M m}{R + h} \] 4. **Final Expression**: Thus, the gravitational potential energy of the body of mass \( m \) at a height \( h \) above the surface of the Earth is: \[ U = -\frac{G M m}{R + h} \] ### Conclusion: The gravitational potential energy of a body of mass \( m \) at a height \( h \) above the surface of the Earth is given by: \[ U = -\frac{G M m}{R + h} \]

To find the gravitational potential energy (U) of a body of mass \( m \) at a height \( h \) above the surface of the Earth, we can use the formula for gravitational potential energy in the context of gravitational fields. ### Step-by-Step Solution: 1. **Understand the Gravitational Potential Energy Formula**: The gravitational potential energy \( U \) of a mass \( m \) in a gravitational field created by a mass \( M \) (in this case, the Earth) at a distance \( r \) from the center of the mass \( M \) is given by the formula: \[ U = -\frac{G M m}{r} ...
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