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If the graviational potential at the sur...

If the graviational potential at the surface of the earth is assumed to be zero, then the potential at infinity is given by

A

0

B

`prop`

C

`-(GM)/( R)`

D

`+(GM)/( R)`

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The correct Answer is:
To solve the question, we need to find the gravitational potential at infinity when the gravitational potential at the surface of the Earth is assumed to be zero. ### Step-by-Step Solution: 1. **Understanding Gravitational Potential**: The gravitational potential \( V \) at a distance \( r \) from a mass \( M \) is given by the formula: \[ V = -\frac{GM}{r} \] where \( G \) is the gravitational constant. 2. **Potential at the Surface of the Earth**: Let \( M \) be the mass of the Earth and \( R \) be the radius of the Earth. The gravitational potential at the surface of the Earth (\( V_R \)) is: \[ V_R = -\frac{GM}{R} \] According to the question, we assume this potential to be zero: \[ V_R = 0 \] 3. **Revising the Potential Scale**: If we set \( V_R = 0 \), we can define a new potential scale. Let’s denote the new potential at the surface as \( V'_R \): \[ V'_R = V_R + \frac{GM}{R} = 0 + \frac{GM}{R} = \frac{GM}{R} \] 4. **Potential at Infinity**: The gravitational potential at infinity (\( V_{\infty} \)) in the original scale is: \[ V_{\infty} = 0 \] In the new scale, we denote this as \( V'_{\infty} \): \[ V'_{\infty} = V_{\infty} + \frac{GM}{R} = 0 + \frac{GM}{R} = \frac{GM}{R} \] 5. **Final Result**: Therefore, the potential at infinity in the new scale, where the potential at the surface of the Earth is zero, is: \[ V'_{\infty} = \frac{GM}{R} \] ### Conclusion: The gravitational potential at infinity, when the potential at the surface of the Earth is assumed to be zero, is given by: \[ \frac{GM}{R} \]

To solve the question, we need to find the gravitational potential at infinity when the gravitational potential at the surface of the Earth is assumed to be zero. ### Step-by-Step Solution: 1. **Understanding Gravitational Potential**: The gravitational potential \( V \) at a distance \( r \) from a mass \( M \) is given by the formula: \[ V = -\frac{GM}{r} ...
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