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The gravitational potential energy of a ...

The gravitational potential energy of a body at a distance r from the center of the earth is U. The force at that point is :

A

`U/r^(2)`

B

`U/r`

C

`Ur`

D

`Ur^(2)`

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To solve the problem, we need to find the gravitational force acting on a body at a distance \( r \) from the center of the Earth, given that the gravitational potential energy at that distance is \( U \). ### Step-by-Step Solution: 1. **Understand Gravitational Potential Energy**: The gravitational potential energy \( U \) of a mass \( m \) at a distance \( r \) from the center of the Earth (mass \( M \)) is given by the formula: \[ U = -\frac{GMm}{r} \] where \( G \) is the universal gravitational constant. 2. **Relate Force to Potential Energy**: The gravitational force \( F \) can be derived from the gravitational potential energy. The force is related to the potential energy by the negative gradient of potential energy: \[ F = -\frac{dU}{dr} \] 3. **Differentiate the Potential Energy**: To find the force, we differentiate \( U \) with respect to \( r \): \[ F = -\frac{d}{dr}\left(-\frac{GMm}{r}\right) \] This simplifies to: \[ F = \frac{GMm}{r^2} \] 4. **Express Force in Terms of Potential Energy**: We can express \( F \) in terms of \( U \). From the expression for \( U \): \[ U = -\frac{GMm}{r} \] Rearranging gives: \[ GMm = -Ur \] Substituting this back into the force equation gives: \[ F = \frac{-Ur}{r^2} = -\frac{U}{r} \] 5. **Final Expression for Force**: Thus, we find that the gravitational force \( F \) at a distance \( r \) from the center of the Earth is: \[ F = -\frac{U}{r} \] ### Conclusion: The force at that point is given by: \[ F = -\frac{U}{r} \]
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