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Elastic Collisions in 1d

Physics Classical Mechanics • Momentum and Impulse

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Solve perfectly elastic collisions in one dimension. The calculator conserves both momentum and kinetic energy, computes final velocities, verifies relative velocity reversal, and animates the before/contact/after motion.

Sign convention: positive velocity is to the right and negative velocity is to the left. In a perfectly elastic collision, total momentum and total kinetic energy are conserved, and the relative velocity reverses: \(v_2-v_1=u_1-u_2\).
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Enter two masses and their signed initial velocities, then click “Calculate”.

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Frequently Asked Questions

What is a perfectly elastic collision?

A perfectly elastic collision is a collision in which both total momentum and total kinetic energy are conserved.

What are the 1D elastic collision formulas?

The final velocities are v1 = ((m1 - m2)u1 + 2m2u2)/(m1 + m2) and v2 = (2m1u1 + (m2 - m1)u2)/(m1 + m2).

Can final velocity be negative?

Yes. A negative final velocity means the object moves in the negative direction after the collision.

What does relative velocity reversal mean?

For a perfectly elastic collision in 1D, the speed of approach equals the speed of separation, written as u1 - u2 = v2 - v1.

What happens when equal masses collide elastically and one is initially at rest?

The moving object stops and the initially stationary object moves away with the original speed of the first object.

Does kinetic energy always stay the same?

In the ideal perfectly elastic model, yes. The calculator verifies this by comparing total kinetic energy before and after.

How is this different from an inelastic collision?

Momentum is conserved in both elastic and inelastic collisions, but kinetic energy is conserved only in a perfectly elastic collision.

What does the center-of-mass velocity show?

The center-of-mass velocity is the constant velocity of the system's center of mass when no external impulse acts.