The problem of a bouncing ball on an inclined plane is a classic test of your ability to decouple motion into independent axes. At first glance, the continuous bouncing might seem chaotic, but by choosing the right coordinate system, a beautiful mathematical pattern emerges.
Tilting Our Perspective
The secret to solving this problem elegantly lies in our choice of axes. Instead of using the standard horizontal and vertical axes, we align our coordinate system with the inclined plane. Let the x-axis point down the incline and the y-axis point perpendicular to it, away from the surface.
By doing this, the acceleration due to gravity, g, splits into two constant components:
- Down the incline: ax=gsinθ
- Perpendicular to the incline: ay=−gcosθ
When the ball is dropped and hits the incline for the first time, it has a purely vertical velocity, let's call it v0. In our tilted coordinate system, this initial velocity has components v0x=v0sinθ and v0y=−v0cosθ.
The First Bounce
A Fresh Start
The problem states that the bounces are perfectly elastic. In the language of physics, this means the impulsive normal force from the plane only affects the perpendicular component of velocity. The parallel component remains completely untouched!
So, immediately after the first bounce, the velocity components are:
- u1x=v0x=v0sinθ
- u1y=−v0y=v0cosθ
Now, the ball is in the air. The time it spends in the air before hitting the plane again depends
only on the
y-motion. Setting the net
y-displacement to zero, we find the time of flight
T1:
T1=∣ay∣2u1y=gcosθ2v0cosθ=g2v0
Notice something incredible? The time of flight is completely independent of the incline's angle θ!
During this time
T1, the ball is accelerating down the incline. The distance it covers,
R12, is given by the second equation of motion:
R12=u1xT1+21axT12
Substituting our values:
R12=(v0sinθ)(g2v0)+21(gsinθ)(g2v0)2=g4v02sinθ
The Second Bounce
Gaining Momentum
While the ball was in the air, gravity was constantly pulling it down the incline, increasing its
x-velocity. Just before the second bounce, its
x-velocity is:
v1x=u1x+axT1=v0sinθ+(gsinθ)(g2v0)=3v0sinθ
The y-velocity, right before impact, is back to −v0cosθ.
Upon the second elastic bounce, the y-velocity reverses again to v0cosθ, while the x-velocity remains 3v0sinθ. Because the initial y-velocity for this second jump is identical to the first jump, the time of flight T2 is exactly the same: T2=g2v0.
Now, let's calculate the distance of the second jump,
R23:
R23=u2xT2+21axT22
R23=(3v0sinθ)(g2v0)+21(gsinθ)(g2v0)2=g8v02sinθ
The Grand Finale
The Ratio
We have our two distances. The question asks for the ratio of
R12 to
R23.
R23R12=g8v02sinθg4v02sinθ=84=21
The ratio is 1:2.
If we were to calculate the distance of the third jump, R34, we would find it to be g12v02sinθ. The distances between successive bounces form a beautiful arithmetic progression: 1:2:3:4… This is a powerful generalized result that can save you immense time in competitive exams!