Animated Solution for Physics - System of Particles: A ball of mass 100 g is projected vertically upwards from the ground with a velocity of 49 m/s. At the same time, another identical ball is dropped from a height of 98 m 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 y=0 with u1=49 m/s.
Ball 2 is dropped from y=98 m with u2=0.
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 t=0, the masses are at 0 and 98 m.
ycm=m+mm(0)+m(98)
ycm=49 m
Initial Velocity of COM
At t=0, the velocities are 49 m/s and 0.
ucm=m+mm(49)+m(0)
ucm=24.5 m/s
Acceleration of COM
The only external force on the system is gravity.
acm=m+mm(−g)+m(−g)
acm=−g=−9.8 m/s2
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 (y=0).
The Equation of Motion
The COM must undergo a displacement of scm=−49 m.
We use the second equation of motion:
scm=ucmt+21acmt2
Substituting Values
Substitute the known values into the equation:
−49=24.5t+21(−9.8)t2
Simplifying the Equation
−49=24.5t−4.9t2
Divide the entire equation by 4.9:
−10=5t−t2⟹t2−5t−10=0
Solving the Quadratic
Apply the quadratic formula:
t=2(1)−(−5)±(−5)2−4(1)(−10)
t=25±65
The Final Answer
Discard the negative root since time must be positive.
65≈8.06
t≈25+8.06=6.53 s
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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 49 m/s. The other is surrendering to it, dropped from a height of 98 m.
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 t=0, the first ball is at the ground (y1=0) and the second is at 98 m (y2=98 m). Since their masses are identical, the COM is exactly in the middle.
ycm=m+mm(0)+m(98)=49 m
Next, how fast is it moving initially? We use the same weighted average for velocity. The first ball is moving up at 49 m/s, and the second is dropped from rest (0 m/s).
ucm=m+mm(49)+m(0)=24.5 m/s
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.
acm=−g=−9.8 m/s2
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 0, so the displacement is −49 m.
We deploy the second equation of motion for the Centre of Mass:
scm=ucmt+21acmt2
Substituting our values:
−49=24.5t−21(9.8)t2
−49=24.5t−4.9t2
Let's clean this up by dividing the entire equation by 4.9:
−10=5t−t2
Rearranging this into a standard quadratic form gives:
t2−5t−10=0
This doesn't factor nicely, so we bring out the quadratic formula:
t=2(1)−(−5)±(−5)2−4(1)(−10)
t=25±25+40=25±65
Since time must be positive, we discard the negative root. The square root of 65 is approximately 8.06.
t≈25+8.06=213.06=6.53 s
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.