Elastic Collision Equations- Physics Guide

What Is an Elastic Collision?

An elastic collision is a collision where both momentum and kinetic energy are conserved. That's it. No energy gets lost to heat, sound, or deformation.

In the real world, perfectly elastic collisions don't exist. But in physics problems, we treat collisions between billiard balls, gas molecules, and certain atomic particles as elastic because the math works out cleanly.

If energy gets lost during impact, you're looking at an inelastic collision instead. Know the difference before you start solving problems.

The Two Conservation Laws You Need

Every elastic collision problem requires you to satisfy two equations simultaneously:

Conservation of Momentum

p₁ + p₂ = p₁' + p₂'

In expanded form:

m₁v₁ + m₂v₂ = m₁v₁' + m₂v₂'

Where:

Conservation of Kinetic Energy

KE₁ + KE₂ = KE₁' + KE₂'

In expanded form:

½m₁v₁² + ½m₂v₂² = ½m₁v₁'² + ½m₂v₂'²

You need both equations. Most students forget the kinetic energy equation and end up with the wrong answer.

One-Dimensional Elastic Collision Formulas

For head-on collisions in a single line, you can use derived formulas instead of solving two equations from scratch.

Final Velocity Equations

v₁' = [(m₁ - m₂)/(m₁ + m₂)] × v₁ + [(2m₂)/(m₁ + m₂)] × v₂

v₂' = [(2m₁)/(m₁ + m₂)] × v₁ + [(m₂ - m₁)/(m₁ + m₂)] × v₂

These look ugly, but they collapse into simpler cases depending on the masses involved.

Special Case: Equal Masses

When m₁ = m₂, the equations simplify dramatically:

v₁' = v₂

v₂' = v₁

The objects basically swap velocities. This is why pool balls scatter the way they do.

Special Case: Heavy Target at Rest

When m₂ >> m₁ and m₂ is stationary:

v₁' ≈ -v₁ (the light object bounces back)

v₂' ≈ 0 (the heavy object barely moves)

Think of a tennis ball bouncing off a brick wall.

Special Case: Light Target at Rest

When m₁ >> m₂ and m₂ is stationary:

v₁' ≈ v₁ (the heavy object keeps moving, barely slowed)

v₂' ≈ 2v₁ (the light object flies off with double the initial speed)

This is what happens when a moving bowling ball hits a ping pong ball.

Two-Dimensional Elastic Collisions

Things get trickier when objects collide at angles. You now have x and y components to track.

You need three equations instead of two:

The general approach:

m₁v₁ₓ + m₂v₂ₓ = m₁v₁ₓ' + m₂v₂ₓ'

m₁v₁ᵧ + m₂v₂ᵧ = m₁v₁ᵧ' + m₂v₂ᵧ'

½m₁(v₁ₓ² + v₁ᵧ²) + ½m₂(v₂ₓ² + v₂ᵧ²) = ½m₁(v₁ₓ'² + v₁ᵧ'²) + ½m₂(v₂ₓ'² + v₂ᵧ'²)

Break velocities into components first, then solve. Most textbook problems give you angles to work with—use them.

How to Solve Elastic Collision Problems

Here's the practical process:

Step 1: Identify Known Values

Write down every mass and velocity you know. Label initial and final states clearly.

Step 2: Choose Your Approach

For one-dimensional problems, you can either:

The formulas are faster. The simultaneous equations are more flexible if you're given partial information.

Step 3: Set Up Your Equations

Write out:

m₁v₁ + m₂v₂ = m₁v₁' + m₂v₂'

½m₁v₁² + ½m₂v₂² = ½m₁v₁'² + ½m₂v₂'²

Substitute your known values. Leave unknowns as variables.

Step 4: Solve

For two unknowns, two equations is enough. Solve algebraically. Don't plug numbers in until the end—you'll make fewer mistakes.

Step 5: Check Your Work

Verify that momentum and kinetic energy are actually conserved in your answer. If they don't match within rounding error, you messed up somewhere.

Elastic vs. Inelastic vs. Perfectly Inelastic

Students mix these up constantly. Here's the breakdown:

Collision Type Momentum Kinetic Energy Real Example
Elastic Conserved Conserved Billiard balls, gas molecules
Inelastic Conserved Lost Car crashes, baseball and glove
Perfectly Inelastic Conserved Lost Objects stick together after impact

The key difference: only elastic collisions conserve kinetic energy. Everything else loses some to deformation or heat.

Common Mistakes to Avoid

Where Elastic Collisions Actually Matter

You won't use these equations to calculate billiard ball trajectories in daily life. But they show up in:

The formulas stay the same regardless of scale. Masses change, but the conservation laws don't.