Imagine you are observing a straight-line track where two objects are moving. The first object, with mass m1, is cruising along with a velocity v1i^. Ahead of it is a second object, mass m2, moving with velocity v2i^. They are on a direct collision course!
This is a classic 1D collision problem. The i^ simply tells us that all the action is happening along the x-axis.
The Power of Momentum Conservation
When these two bodies collide, they exert forces on each other. However, if we consider both bodies together as a single system, these collision forces are purely internal.
Since there are no external horizontal forces acting on our system, the total linear momentum must remain perfectly conserved. This is our master key to unlocking the problem.
We can write the momentum conservation equation as:
m1v1+m2v2=m1v3+m2v4
Simplifying the Algebra
Now, the problem gives us some fantastic clues to simplify our lives. We are told that m2=0.5m1.
To make the algebra cleaner and avoid decimals, let's set m2=m. This immediately means m1=2m.
We are also given a relationship for the final velocity of the first mass: v3=0.5v1.
Let's carefully substitute these relationships into our momentum equation:
(2m)v1+(m)v2=(2m)(0.5v1)+(m)v4
The Final Reveal
Look closely at the equation we just built. Every single term contains the mass
m. This is a beautiful moment in physics where the specific mass value doesn't matter, only the ratio does! We can safely divide the entire equation by
m:
2v1+v2=2(0.5v1)+v4
Simplifying the right side,
2×0.5 is just
1:
2v1+v2=v1+v4
Our goal is to isolate
v1. Let's subtract
v1 from both sides:
v1+v2=v4
Finally, moving
v2 to the other side gives us our answer:
v1=v4−v2
And there we have it! By simply trusting the conservation of momentum and carefully substituting our given ratios, we've arrived at the exact expression for v1. This perfectly matches option (d).