Sigma Percentile
JEE Advanced 1985
LEVELJEE Advanced

Animated Solution for Physics - System of Particles: A ball of mass is projected vertically upwards from the ground with a velocity of . At the same time, another identical ball is dropped from a height of to fall freely along the same path as that followed by the first ball. After some time, the two balls collide and stick together and finally fall to the ground. Find the time of flight of the masses.

Enter Numerical Value:

Visualized Solution

Visualizing the Setup

  • Ball 1 is projected upwards from with .
  • Ball 2 is dropped from with .
  • They collide, stick together, and fall to the ground.

The Kinematic Trap

  • Solving for the exact collision time and then setting up a new equation for the combined mass is tedious.
  • We need a more elegant approach.

The Centre of Mass (COM)

  • During the collision, the forces are purely internal.
  • Internal forces do not affect the motion of the Centre of Mass.
  • We can track the COM as if the collision never happened!

Initial Position of COM

  • At , the masses are at and .

Initial Velocity of COM

  • At , the velocities are and .

Acceleration of COM

  • The only external force on the system is gravity.

The Combined Mass Trajectory

  • After the perfectly inelastic collision, the two balls stick together.
  • The combined mass is now physically located at the COM.
  • We just need to find when the COM hits the ground ().

The Equation of Motion

  • The COM must undergo a displacement of .
  • We use the second equation of motion:

Substituting Values

  • Substitute the known values into the equation:

Simplifying the Equation

  • Divide the entire equation by :

Solving the Quadratic

  • Apply the quadratic formula:

The Final Answer

  • Discard the negative root since time must be positive.

The Sigma Insight: Motion of Centre of Mass

Solution Diagram

The Trap of the Two-Part Problem

Imagine the scenario: two balls hurtling towards each other. One is fighting gravity, launched upwards at . The other is surrendering to it, dropped from a height of .
Inevitably, they collide. And not just a gentle bump—they crash and stick together, becoming a single, heavier mass that eventually plummets back to the earth.
If you try to solve this using standard kinematics, you are walking straight into a trap. You would first have to calculate the exact time they collide. Then, you'd need to find their individual velocities right before impact. After that, you'd apply the conservation of momentum to find the new velocity of the combined mass. Finally, you'd set up a whole new kinematic equation for the second phase of the journey.
It is exhausting, error-prone, and frankly, not the elegant way a physicist thinks.

The Elegance of the Centre of Mass

Enter the Centre of Mass (COM). This concept is like a cheat code for the universe.
When the two balls collide, the forces they exert on each other are massive. But here is the secret: those forces are strictly internal to the two-ball system. According to Newton's laws, internal forces cannot change the motion of the system's Centre of Mass.
From the moment the balls are released, right through the violent collision, and all the way until they hit the ground, the Centre of Mass moves as if nothing happened. It is completely oblivious to the collision!
So, instead of tracking two separate balls, we just track this one imaginary point.

Setting Up the Master Equation

Let's find out where this magical point starts. At , the first ball is at the ground () and the second is at (). Since their masses are identical, the COM is exactly in the middle.
Next, how fast is it moving initially? We use the same weighted average for velocity. The first ball is moving up at , and the second is dropped from rest ().
What about acceleration? The only external force acting on both balls is gravity. Therefore, the acceleration of the COM is simply the acceleration due to gravity.

The Final Execution

Here is the beautiful part. After the collision, the balls stick together. The combined mass is now physically located exactly at the Centre of Mass!
To find the total time of flight, we just need to find the time it takes for the Centre of Mass to hit the ground. Hitting the ground means the final position is , so the displacement is .
We deploy the second equation of motion for the Centre of Mass:
Substituting our values:
Let's clean this up by dividing the entire equation by :
Rearranging this into a standard quadratic form gives:
This doesn't factor nicely, so we bring out the quadratic formula:
Since time must be positive, we discard the negative root. The square root of is approximately .
And there it is. By shifting our perspective to the Centre of Mass, we bypassed the collision entirely and solved a complex two-part problem with a single, elegant equation.

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