Analyzing the Setup
Imagine a frictionless horizontal surface where three blocks, A, B, and C, are placed in a straight line. The masses are mA=m, mB=2m, and mC=m.
Block A is fired towards block B with an initial speed of uA=9 m/s. The problem states that two distinct collisions will occur sequentially. First, an elastic collision between A and B. Then, a completely inelastic collision between B and C.
Our goal is to find the final velocity of block C after all the dust settles.
Phase 1
The Elastic Strike
When block A collides with the stationary block B, the collision is perfectly elastic. This means both momentum and kinetic energy are conserved.
Instead of writing out both conservation equations and solving the quadratic system, we can use the standard derived formula for the velocity of a stationary target after a 1D elastic collision:
Let's substitute our known values into this powerful tool:
Simplifying the mass ratio, we get:
So, after the first impact, block B is launched forward with a speed of 6 m/s.
Phase 2
The Inelastic Embrace
Now, block B is hurtling towards the stationary block C at 6 m/s. This second collision is completely inelastic.
In a completely inelastic collision, the objects stick together upon impact and move as a single combined mass. While kinetic energy is lost to deformation and heat, linear momentum is strictly conserved.
Let's set up the momentum conservation equation for the B−C system. The initial momentum is just the momentum of block B, and the final momentum is the momentum of the combined mass moving at a final velocity vf:
mBvB+mC(0)=(mB+mC)vf
Substituting the masses and the velocity of B we just found:
Dividing both sides by 3m, we find the final velocity:
Since block C is now stuck to block B, its final speed is exactly 4 m/s.
The Ninja Technique
System Momentum Conservation
While the step-by-step chronological method is fantastic for building physical intuition, there is a faster, more elegant way to solve this problem—a true "ninja technique" for competitive exams.
Notice that the entire surface is frictionless. This means there are zero external horizontal forces acting on the A+B+C system. Therefore, the total linear momentum of the entire three-block system must remain constant from the very beginning to the very end!
Let's calculate the initial momentum of the entire system before any collisions happen:
pinitial=mAuA+mB(0)+mC(0)=m(9)=9m
Now, what does the system look like at the very end? Block A has bounced back after the first collision, and blocks B and C are stuck together moving at vC. We need the final velocity of A, let's call it vA′. Using the elastic collision formula for the projectile:
vA′=mA+mBmA−mBuA=m+2mm−2m(9)=3m−m(9)=−3 m/s
Now, let's write the final momentum of the entire system:
pfinal=mAvA′+(mB+mC)vC
pfinal=m(−3)+(2m+m)vC=−3m+3mvC
Equating the initial and final total momentum:
Both methods yield the exact same result! The chronological method is safer, but the system momentum method is a beautiful demonstration of the deep conservation laws governing our universe.