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The work done to increases the radius of...

The work done to increases the radius of orbit of a satellite of mass 'm' revolving around a planet of mass `M` from orbit of radius `R` into another orbit of radius `3R` is

A

`(2GMm)/(3R)`

B

`(GMm)/(3R)`

C

`(GMm)/(6R)`

D

`(GMMm)/(24R)`

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The correct Answer is:
To solve the problem of finding the work done to increase the radius of orbit of a satellite from radius \( R \) to \( 3R \), we can follow these steps: ### Step 1: Understand the Total Energy of a Satellite in Orbit The total mechanical energy \( E \) of a satellite in a circular orbit of radius \( r \) around a planet of mass \( M \) is given by the formula: \[ E = -\frac{GMm}{2r} \] where \( G \) is the gravitational constant, \( m \) is the mass of the satellite, and \( r \) is the radius of the orbit. ### Step 2: Calculate the Total Energy at Radius \( R \) Using the formula for total energy, we can calculate the energy when the satellite is at radius \( R \): \[ E(R) = -\frac{GMm}{2R} \] ### Step 3: Calculate the Total Energy at Radius \( 3R \) Next, we calculate the total energy when the satellite is at radius \( 3R \): \[ E(3R) = -\frac{GMm}{2(3R)} = -\frac{GMm}{6R} \] ### Step 4: Find the Change in Total Energy The work done \( W \) to move the satellite from radius \( R \) to radius \( 3R \) is equal to the change in total energy: \[ W = E(3R) - E(R) \] Substituting the values we calculated: \[ W = \left(-\frac{GMm}{6R}\right) - \left(-\frac{GMm}{2R}\right) \] This simplifies to: \[ W = -\frac{GMm}{6R} + \frac{GMm}{2R} \] ### Step 5: Simplify the Expression To combine the terms, we need a common denominator: \[ W = \frac{GMm}{2R} - \frac{GMm}{6R} = \frac{GMm \cdot 3}{6R} - \frac{GMm}{6R} = \frac{(3 - 1)GMm}{6R} = \frac{2GMm}{6R} \] Thus, we have: \[ W = \frac{GMm}{3R} \] ### Final Answer The work done to increase the radius of orbit of the satellite from \( R \) to \( 3R \) is: \[ W = \frac{GMm}{3R} \] ---

To solve the problem of finding the work done to increase the radius of orbit of a satellite from radius \( R \) to \( 3R \), we can follow these steps: ### Step 1: Understand the Total Energy of a Satellite in Orbit The total mechanical energy \( E \) of a satellite in a circular orbit of radius \( r \) around a planet of mass \( M \) is given by the formula: \[ E = -\frac{GMm}{2r} \] where \( G \) is the gravitational constant, \( m \) is the mass of the satellite, and \( r \) is the radius of the orbit. ...
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