Sigma Percentile
JEE Advanced 2024
LEVELJEE Advanced

Animated Solution for Physics - Gravitation: A particle of mass is under the influence of the gravitational field of a body of mass . The particle is moving in a circular orbit of radius with time period around the mass . Then, the particle is subjected to an additional central force, corresponding to the potential energy , where is a positive constant of suitable dimensions and is the distance from the center of the orbit. If the particle moves in the same circular orbit of radius in the combined gravitational potential due to and , but with a new time period , then is given by [G is the gravitational constant.]

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Visualized Solution

The Sigma Insight: Orbital Motion of a Satellite

Solution Diagram

The Gravitational Dance

Imagine a massive body of mass sitting quietly at the center of the universe. A much smaller particle of mass is caught in its gravitational embrace, revolving around it in a perfect circular orbit of radius .
Initially, what keeps this particle from flying off into deep space? It's the gravitational force acting as the centripetal force. We can express this mathematically by balancing the forces:
We know that the angular velocity is intimately connected to the time period by the relation . Substituting this into our force equation gives us a beautiful expression for the square of the initial time period:
Keep this equation safe; it will be our master key later on.

The Plot Twist

A New Potential
Now, the universe throws a curveball. The particle is suddenly subjected to an additional central force. We aren't given the force directly, but rather its potential energy:
To find the force, we must remember the fundamental relationship between conservative forces and potential energy: force is the negative gradient of potential energy (). Let's differentiate our new potential:
Notice the positive sign! In the language of central forces, a positive sign means the force is directed radially outwards. It is a repulsive force, actively trying to push the particle away from the central mass .

The Battle of Forces

The particle is now caught in a tug-of-war. Gravity pulls it inward, while this new mysterious force pushes it outward. However, the problem states a crucial constraint: the particle continues to move in the exact same circular orbit of radius .
For the radius to remain constant, the particle must adjust its speed so that the new net inward force perfectly provides the required centripetal force. Let's write the new force balance equation:
Substituting our known force expressions, we get:

The Mathematics of Time

Let's clean up this equation by dividing everything by and replacing the new angular velocity with , where is the new time period:
Look closely at the first term on the left side: . Does it look familiar? It is exactly the term we found in our very first step! We can replace it with :
Now we have a direct bridge connecting the new time period to the old time period . Let's divide the entire equation by to isolate the time periods:

The Grand Finale

We are asked to find the value of the expression . Let's rearrange our equation to match this form:
We are almost there! Remember that master key we saved in the first step? It's time to use it. Substitute into our equation:
The terms cancel out beautifully, and divides to leave in the denominator. The dust settles, revealing our final, elegant answer:
Because the net inward force decreased due to the repulsive potential, the particle had to slow down to maintain its orbit, resulting in a longer time period . This is a masterful demonstration of how forces dictate the rhythm of orbital mechanics!

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