Animated Solution for Physics - Gravitation: Two bodies, each of mass M, are kept fixed with a separation 2L. A particle of mass m is projected from the mid-point of the line joining their centres, perpendicular to the line. The gravitational constant is G. The correct statement(s) is (are)
Select Answer:
* Multiple Correct
Visualized Solution
Visualizing the Setup
Two bodies of mass M are fixed at a distance 2L apart.
A particle of mass m is placed at the midpoint C, which is at a distance L from both masses.
The particle is projected perpendicular to the line joining the two masses with velocity v.
Conservation of Mechanical Energy
The gravitational force is a conservative force.
Therefore, the total mechanical energy E of the particle remains constant throughout its motion.
E=K+U=constant
The Escape Condition
To escape the gravitational field, the particle must reach infinity (r→∞).
At infinity, the gravitational potential energy U∞=0.
For minimum escape velocity, the kinetic energy at infinity is also zero: K∞=0.
Thus, the total mechanical energy at infinity is E∞=0.
Gravitational Potential at Midpoint
The gravitational potential Vc at the midpoint C is the sum of potentials due to both masses M:
Vc=V1+V2=−LGM−LGM
Vc=−L2GM
Initial Potential Energy
The initial gravitational potential energy Uc of the mass m at the midpoint is:
Uc=m⋅Vc
Uc=−L2GMm
Setting Up Energy Conservation
Using the conservation of mechanical energy:
Einitial=Efinal
Kc+Uc=K∞+U∞
21mv2−L2GMm=0
Solving for Escape Velocity
Rearranging the equation to solve for v2:
21mv2=L2GMm
v2=L4GM
Final Escape Velocity
Taking the square root on both sides:
v=L4GM
v=2LGM
Conclusion
The correct options are (b) and (d).
Minimum escape velocity: v=2LGM
Total mechanical energy remains constant throughout the motion.
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The Sigma Insight: Gravitational Potential and Potential Energy
Solution Diagram
Analyzing the Setup
Imagine standing in deep space, watching a fascinating cosmic dance. We have two massive bodies, each of mass M, anchored firmly at a distance of 2L from one another.
Exactly at the midpoint of the line connecting these two giants, we place a tiny test particle of mass m. This midpoint, which we will call point C, lies at a distance of exactly L from both of the larger masses.
Now, we give this tiny particle a sudden kick, projecting it with an initial velocity v in a direction perpendicular to the line joining the two fixed masses. Our quest is to determine the minimum initial velocity required for this particle to break free from the gravitational embrace of these two massive bodies and escape to infinity.
The Master Principle
Conservation of Energy
Before diving into the mathematics, let us step back and appreciate the physics at play. The only force acting on our test particle is gravity.
Because the gravitational force is a conservative force, the total mechanical energy of the particle—which is the sum of its kinetic energy (K) and gravitational potential energy (U)—must remain absolutely constant at every single point along its trajectory.
E=K+U=constant
This fundamental truth immediately validates statement (d): the energy of the mass m remains constant throughout its motion.
Defining the Escape Condition
What does it truly mean to "escape" a gravitational field? To escape means to travel infinitely far away from the source masses, where their gravitational pull drops to zero.
By definition, we set the gravitational potential energy at infinity to be zero:
U∞=0
For the particle to escape with the absolute minimum initial velocity, it should just barely reach infinity. This means that upon arriving at infinity, its kinetic energy will also have dwindled to zero:
K∞=0
Thus, the total mechanical energy of the particle at infinity is exactly zero:
E∞=K∞+U∞=0
Since energy is conserved, the total mechanical energy at our starting point C must also be exactly zero!
Calculating Gravitational Potential and Potential Energy
Let us find the gravitational potential Vc at the midpoint C. Since potential is a scalar quantity, we can simply sum the potentials contributed by each of the two fixed masses:
Vc=V1+V2=−LGM−LGM=−L2GM
Now, we can easily find the initial gravitational potential energy Uc of our test mass m at this midpoint by multiplying its mass by the potential:
Uc=m⋅Vc=−L2GMm
The negative sign here is beautiful—it signifies that the particle is trapped in a gravitational potential well, bound to the two massive bodies.
Applying Energy Conservation to Solve for Velocity
Now, we bring everything together using our energy conservation equation:
Einitial=Efinal
Kc+Uc=K∞+U∞
Substituting our expressions for kinetic and potential energy, we get:
21mv2−L2GMm=0
Let's rearrange this equation to solve for the velocity v:
21mv2=L2GMm
Notice how the mass of the test particle, m, appears on both sides of the equation. It cancels out beautifully! This tells us a profound physical truth: the escape velocity is completely independent of the mass of the escaping object itself.
v2=L4GM
Taking the square root on both sides, we find the minimum escape velocity:
v=2LGM
This perfectly matches statement (b).
Conclusion
Through the elegant application of energy conservation, we have shown that:
1. The minimum initial velocity required for the mass m to escape is indeed 2LGM, making statement (b) correct.
2. The total mechanical energy of the mass m remains constant throughout its motion because gravity is a conservative force, making statement (d) correct.