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In order to shift a body of mass m from ...

In order to shift a body of mass `m` from a circular orbit of radius `3R` to a higher orbit of radius `5R` around the earth, the work done is

A

`(3GMm)/(5R)`

B

`(GMm)/(2R)`

C

`2/15(GMm)/R`

D

`(GMm)/(5R)`

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The correct Answer is:
To find the work done in shifting a body of mass \( m \) from a circular orbit of radius \( 3R \) to a higher orbit of radius \( 5R \) around the Earth, we can follow these steps: ### Step 1: Understand the Potential Energy in Circular Orbits The gravitational potential energy \( U \) of a body of mass \( m \) in a circular orbit around the Earth is given by the formula: \[ U = -\frac{GMm}{r} \] where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( r \) is the radius of the orbit. ### Step 2: Calculate Initial Potential Energy For the initial orbit at radius \( 3R \): \[ U_i = -\frac{GMm}{3R} \] ### Step 3: Calculate Final Potential Energy For the final orbit at radius \( 5R \): \[ U_f = -\frac{GMm}{5R} \] ### Step 4: Calculate the Change in Potential Energy The work done \( W \) by an external agent to shift the body from the initial orbit to the final orbit is equal to the change in potential energy: \[ W = U_f - U_i \] Substituting the values we calculated: \[ W = \left(-\frac{GMm}{5R}\right) - \left(-\frac{GMm}{3R}\right) \] \[ W = -\frac{GMm}{5R} + \frac{GMm}{3R} \] ### Step 5: Simplify the Expression To simplify the expression, we need a common denominator. The least common multiple of \( 5R \) and \( 3R \) is \( 15R \): \[ W = \left(-\frac{3GMm}{15R}\right) + \left(\frac{5GMm}{15R}\right) \] \[ W = \frac{2GMm}{15R} \] ### Final Answer Thus, the work done to shift the body from a circular orbit of radius \( 3R \) to a higher orbit of radius \( 5R \) is: \[ W = \frac{2GMm}{15R} \] ---

To find the work done in shifting a body of mass \( m \) from a circular orbit of radius \( 3R \) to a higher orbit of radius \( 5R \) around the Earth, we can follow these steps: ### Step 1: Understand the Potential Energy in Circular Orbits The gravitational potential energy \( U \) of a body of mass \( m \) in a circular orbit around the Earth is given by the formula: \[ U = -\frac{GMm}{r} \] where \( G \) is the gravitational constant, \( M \) is the mass of the Earth, and \( r \) is the radius of the orbit. ...
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