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If g be the acceleration due to gravity ...

If g be the acceleration due to gravity of the earth's surface, the gain is the potential energy of an object of mass m raised from the surface of the earth to a height equal to the radius R of the earth is

A

(1/2) m g R

B

2 m g R

C

m g R

D

(1/4) m g R

Text Solution

AI Generated Solution

The correct Answer is:
To solve the problem of finding the gain in potential energy of an object of mass \( m \) raised from the surface of the Earth to a height equal to the radius \( R \) of the Earth, we can follow these steps: ### Step 1: Understand the Initial and Final Positions - The object is initially at the surface of the Earth, which we can denote as height \( h_1 = 0 \). - The object is raised to a height equal to the radius of the Earth, so the final height is \( h_2 = R \). ### Step 2: Calculate the Initial Potential Energy The potential energy \( U \) at a distance \( r \) from the center of the Earth is given by the formula: \[ U = -\frac{GMm}{r} \] where: - \( G \) is the gravitational constant, - \( M \) is the mass of the Earth, - \( m \) is the mass of the object, - \( r \) is the distance from the center of the Earth. At the surface of the Earth, the distance \( r \) is equal to the radius \( R \): \[ U_1 = -\frac{GMm}{R} \] ### Step 3: Calculate the Final Potential Energy When the object is raised to a height equal to the radius of the Earth, the distance from the center of the Earth becomes \( r = 2R \): \[ U_2 = -\frac{GMm}{2R} \] ### Step 4: Calculate the Gain in Potential Energy The gain in potential energy \( \Delta U \) is the difference between the final and initial potential energies: \[ \Delta U = U_2 - U_1 \] Substituting the values from Steps 2 and 3: \[ \Delta U = \left(-\frac{GMm}{2R}\right) - \left(-\frac{GMm}{R}\right) \] This simplifies to: \[ \Delta U = -\frac{GMm}{2R} + \frac{GMm}{R} \] \[ \Delta U = \frac{GMm}{R} - \frac{GMm}{2R} \] \[ \Delta U = \frac{GMm}{2R} \] ### Step 5: Relate \( GM/R^2 \) to \( g \) We know that the acceleration due to gravity \( g \) at the surface of the Earth is given by: \[ g = \frac{GM}{R^2} \] Thus, we can express \( GM \) as: \[ GM = gR^2 \] ### Step 6: Substitute \( GM \) in the Gain in Potential Energy Now, substituting \( GM \) in the expression for \( \Delta U \): \[ \Delta U = \frac{gR^2 m}{2R} = \frac{gRm}{2} \] ### Final Answer The gain in potential energy of the object when raised to a height equal to the radius of the Earth is: \[ \Delta U = \frac{gRm}{2} \]
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