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Physics · Ch 6 — Work, Energy and Power

Collisions in Two Dimensions

6.11.3

Collisions in Two Dimensions

The Core Idea: Why Two Dimensions Changes Everything

In the previous section, every collision happened along a single straight line. A ball hits a wall and bounces straight back; two gliders on an air track meet head-on. Real collisions are rarely that tidy. A car hits another at an intersection; a billiard ball is struck at an angle. In these cases, the velocities before and after the collision are vectors in a plane, not scalars on a line.

The fundamental laws — conservation of linear momentum and conservation of kinetic energy (for elastic collisions) — still hold. But now they give us two component equations (one for the xx-axis, one for the yy-axis) instead of one. That extra equation is what makes two-dimensional collisions richer and, in many cases, solvable only when we know enough of the final conditions.


Setting Up the Problem

Consider two particles, AA and BB, of masses m1m_1 and m2m_2. Particle AA moves with initial velocity v1i\mathbf{v}_{1i}; particle BB is initially at rest (v2i=0\mathbf{v}_{2i} = 0). This is the standard textbook scenario — one target stationary — and it captures the essential physics.

After the collision, both particles move off with velocities v1f\mathbf{v}_{1f} and v2f\mathbf{v}_{2f}. The collision is elastic, so both momentum and kinetic energy are conserved.

We choose a coordinate system that simplifies the algebra: let the initial velocity of AA define the xx-axis. So v1i=v1i i^\mathbf{v}_{1i} = v_{1i}\,\hat{\mathbf{i}}. After the collision, AA moves at an angle θ1\theta_1 above the xx-axis, and BB moves at an angle θ2\theta_2 below the xx-axis (or vice versa — the signs will come from the equations).

Note

This choice of axes is a trick, not a loss of generality. Because momentum is a vector, we are free to rotate our coordinate system to align with the initial motion. The physics is unchanged.


The Two Conservation Laws, Component by Component

Conservation of linear momentum gives two scalar equations:

  • xx-component: m1v1i=m1v1fcos⁡θ1+m2v2fcos⁡θ2m_1 v_{1i} = m_1 v_{1f} \cos\theta_1 + m_2 v_{2f} \cos\theta_2
  • yy-component: 0=m1v1fsin⁡θ1−m2v2fsin⁡θ20 = m_1 v_{1f} \sin\theta_1 - m_2 v_{2f} \sin\theta_2

The minus sign in the yy-equation appears because we have chosen θ2\theta_2 to be measured below the xx-axis, so its yy-component is negative.

Conservation of kinetic energy (elastic collision) gives the scalar equation:

12m1v1i2=12m1v1f2+12m2v2f2\frac{1}{2} m_1 v_{1i}^2 = \frac{1}{2} m_1 v_{1f}^2 + \frac{1}{2} m_2 v_{2f}^2

These three equations contain four unknowns: v1fv_{1f}, v2fv_{2f}, θ1\theta_1, θ2\theta_2. (The masses and v1iv_{1i} are known.) So the system is underdetermined — we need one more piece of information to get a unique answer. That extra information usually comes from the geometry of the impact: for example, the angle at which the particles strike each other, or the fact that the collision is "glancing" rather than head-on.

Watch out

A common mistake is to think that conservation laws alone give a unique answer in 2D. They don't. You always need one additional condition — often the impact parameter or the angle of the line of centres at the moment of contact.


The Special Case of Equal Masses

When m1=m2=mm_1 = m_2 = m, the equations simplify dramatically. The momentum equations become:

  • xx: v1i=v1fcos⁡θ1+v2fcos⁡θ2v_{1i} = v_{1f} \cos\theta_1 + v_{2f} \cos\theta_2
  • yy: 0=v1fsin⁡θ1−v2fsin⁡θ20 = v_{1f} \sin\theta_1 - v_{2f} \sin\theta_2

And the energy equation becomes:

v1i2=v1f2+v2f2v_{1i}^2 = v_{1f}^2 + v_{2f}^2

Now square the two momentum equations and add them:

v1i2=v1f2(cos⁡2θ1+sin⁡2θ1)+v2f2(cos⁡2θ2+sin⁡2θ2)+2v1fv2f(cos⁡θ1cos⁡θ2−sin⁡θ1sin⁡θ2)v_{1i}^2 = v_{1f}^2 (\cos^2\theta_1 + \sin^2\theta_1) + v_{2f}^2 (\cos^2\theta_2 + \sin^2\theta_2) + 2 v_{1f} v_{2f} (\cos\theta_1 \cos\theta_2 - \sin\theta_1 \sin\theta_2)

Using cos⁡2+sin⁡2=1\cos^2 + \sin^2 = 1 and the cosine addition formula cos⁡θ1cos⁡θ2−sin⁡θ1sin⁡θ2=cos⁡(θ1+θ2)\cos\theta_1 \cos\theta_2 - \sin\theta_1 \sin\theta_2 = \cos(\theta_1 + \theta_2), we get:

v1i2=v1f2+v2f2+2v1fv2fcos⁡(θ1+θ2)v_{1i}^2 = v_{1f}^2 + v_{2f}^2 + 2 v_{1f} v_{2f} \cos(\theta_1 + \theta_2)

But the energy equation says v1i2=v1f2+v2f2v_{1i}^2 = v_{1f}^2 + v_{2f}^2. For both to be true simultaneously, we must have:

2v1fv2fcos⁡(θ1+θ2)=02 v_{1f} v_{2f} \cos(\theta_1 + \theta_2) = 0

Since v1fv_{1f} and v2fv_{2f} are not zero (the particles do move after collision), the only possibility is:

cos⁡(θ1+θ2)=0\cos(\theta_1 + \theta_2) = 0

Therefore:

θ1+θ2=90∘\theta_1 + \theta_2 = 90^\circ

Important

For an elastic collision between two equal masses, one of which is initially at rest, the two particles always move off at right angles to each other.

This is a beautiful and testable result. If you shoot one billiard ball into a stationary one of the same mass, the two balls will always leave at 90∘90^\circ to each other — provided the collision is elastic and not head-on.

›Proof

The derivation above is the complete proof. The key step is squaring and adding the momentum components, then comparing with the energy equation. The cancellation forces cos⁡(θ1+θ2)=0\cos(\theta_1+\theta_2)=0.


The General Case: Unequal Masses

When m1≠m2m_1 \neq m_2, the algebra is messier but the logic is the same. The three equations (two momentum, one energy) still have four unknowns. The extra condition is often the impact parameter — the perpendicular distance between the line of motion of the incoming particle and the centre of the target particle. This parameter determines the angles θ1\theta_1 and θ2\theta_2.

The textbook does not derive a closed-form solution for the general case; instead, it emphasises the method:

  1. Write the momentum conservation equations in component form.
  2. Write the energy conservation equation. …