Collisions in one dimension

Two billiard balls meet head-on. One stops dead, the other rolls off with the exact speed the first one had — a result so clean it looks like a magic trick, until you realise it falls straight out of two conservation laws you already know. Every collision along a straight line, whether it is a cricket ball caught by a fielder, a bumper car crash, or a proton striking a nucleus, obeys the same two rules: momentum is always conserved, and kinetic energy is conserved only if the collision is elastic. This section builds the general formula for a one-dimensional elastic collision from those two laws, reads off three physically important special cases, and works through the perfectly inelastic limit where two bodies stick together and some kinetic energy is deliberately "lost" to heat, sound, and deformation.

The core insight

In any isolated one-dimensional collision momentum is always conserved, while kinetic energy is conserved only if the collision is elastic, and solving the two conservation equations together gives the general elastic final-velocity formulas that reduce to intuitive results for equal, very heavy, and very light colliding bodies.

The core idea

A collision is a brief, strong interaction between two bodies — brief enough that external forces (like friction or gravity acting during the contact) can be ignored. Two facts anchor everything that follows.

Momentum is conserved in every collision. As long as the two-body system is isolated from external forces, the total linear momentum before and after the collision is the same, regardless of what type of collision it is:

m1u1+m2u2=m1v1+m2v2m_1u_1 + m_2u_2 = m_1v_1 + m_2v_2

where: m1,m2m_1, m_2 are the masses, u1,u2u_1, u_2 are the initial velocities, and v1,v2v_1, v_2 are the final velocities, all measured along the same line (with sign for direction).

Kinetic energy is conserved only in an elastic collision. An elastic collision conserves both momentum and total kinetic energy:

12m1u12+12m2u22=12m1v12+12m2v22\frac{1}{2}m_1u_1^2 + \frac{1}{2}m_2u_2^2 = \frac{1}{2}m_1v_1^2 + \frac{1}{2}m_2v_2^2

An inelastic collision conserves momentum but not kinetic energy — some of it converts to heat, sound, and permanent deformation. The extreme case, a perfectly inelastic collision, is where the two bodies stick together and move off with one common final velocity vv. The figure below shows the equal-mass elastic case: the moving ball transfers its entire velocity to the stationary one and stops, which is exactly the "billiard ball" result from the overview.

Figure
Before and after view of an elastic head-on collision between two equal balls, showing the velocity completely transferring from the moving ball to the stationary one
Equal-mass elastic collision: velocities exchange completely before m u = 6 m at rest after m stopped, v1 = 0 m v2 = 6

The general one-dimensional elastic collision formula (derived below) lets you find v1v_1 and v2v_2 for any masses and initial speeds:

v1=(m1−m2)u1+2m2u2m1+m2,v2=(m2−m1)u2+2m1u1m1+m2v_1 = \frac{(m_1-m_2)u_1 + 2m_2u_2}{m_1+m_2}, \qquad v_2 = \frac{(m_2-m_1)u_2 + 2m_1u_1}{m_1+m_2}

Setting u2=0u_2 = 0 (target at rest) gives three named special cases: m1=m2m_1 = m_2 gives v1=0v_1 = 0, v2=u1v_2 = u_1 (complete velocity exchange). m1≫m2m_1 \gg m_2 gives v1≈u1v_1 \approx u_1, v2≈2u1v_2 \approx 2u_1 (the heavy body barely slows; the light body is flung forward at nearly double the incoming speed). m1≪m2m_1 \ll m_2 gives v1≈−u1v_1 \approx -u_1, v2≈0v_2 \approx 0 (the light body bounces straight back, like a ball off a wall; the heavy body barely moves). For a perfectly inelastic collision, momentum conservation alone (with v1=v2=vv_1 = v_2 = v) gives the common final velocity:

v=m1u1+m2u2m1+m2v = \frac{m_1u_1 + m_2u_2}{m_1+m_2}

and the kinetic energy lost is ΔK=Ki−Kf\Delta K = K_i - K_f, converted to heat, sound, and deformation.

Derivation AThe general elastic collision formulas

The goal is to solve the momentum-conservation equation and the kinetic-energy-conservation equation together, for two bodies of mass m1,m2m_1, m_2 colliding elastically along a line with initial velocities u1,u2u_1, u_2, and extract closed-form expressions for the final velocities v1v_1 and v2v_2 purely in terms of the masses and initial velocities, without guessing the answer first.

Step 1. Write both conservation laws with the unknowns v1,v2v_1, v_2 on one side. Momentum: m1(u1−v1)=m2(v2−u2)m_1(u_1-v_1) = m_2(v_2-u_2). Kinetic energy: m1(u12−v12)=m2(v22−u22)m_1(u_1^2-v_1^2) = m_2(v_2^2-u_2^2), after multiplying the energy equation through by 22 and rearranging so masses group with their own before-and-after terms.

Step 2. Factor the energy equation using a2−b2=(a−b)(a+b)a^2-b^2=(a-b)(a+b). The left side becomes m1(u1−v1)(u1+v1)m_1(u_1-v_1)(u_1+v_1) and the right side becomes m2(v2−u2)(v2+u2)m_2(v_2-u_2)(v_2+u_2).

Step 3. Divide the Step 2 equation by the Step 1 equation term by term (both sides of Step 1 are nonzero for a genuine collision). The factors m1(u1−v1)m_1(u_1-v_1) and m2(v2−u2)m_2(v_2-u_2) cancel top and bottom, leaving the compact relative-velocity relation u1+v1=v2+u2u_1+v_1 = v_2+u_2, or equivalently u1−u2=v2−v1u_1-u_2 = v_2-v_1 — the relative speed of approach before impact equals the relative speed of separation after impact, for an elastic collision specifically.

Step 4. Use this relation to eliminate one unknown. From Step 3, v2=u1+v1−u2v_2 = u_1 + v_1 - u_2. Substitute into the momentum equation m1u1+m2u2=m1v1+m2v2m_1u_1+m_2u_2 = m_1v_1+m_2v_2 and solve for v1v_1: m1u1+m2u2=m1v1+m2(u1+v1−u2)m_1u_1+m_2u_2 = m_1v_1 + m_2(u_1+v_1-u_2), which rearranges to v1(m1+m2)=(m1−m2)u1+2m2u2v_1(m_1+m_2) = (m_1-m_2)u_1+2m_2u_2, giving v1=(m1−m2)u1+2m2u2m1+m2v_1 = \dfrac{(m_1-m_2)u_1+2m_2u_2}{m_1+m_2}.

Step 5. Substitute this v1v_1 back into v2=u1+v1−u2v_2 = u_1+v_1-u_2 and simplify to get the matching expression v2=(m2−m1)u2+2m1u1m1+m2v_2 = \dfrac{(m_2-m_1)u_2+2m_1u_1}{m_1+m_2}. As a check, setting m1=m2m_1=m_2 collapses these to v1=u2v_1=u_2 and v2=u1v_2=u_1 — the bodies simply exchange velocities, matching the worked example below.

Worked example

A ball of mass 2 kg2\ \text{kg} moving at 6 m/s6\ \text{m/s} collides elastically, head-on, with an identical 2 kg2\ \text{kg} ball at rest. Find both final velocities, and then check what happens if the second ball's mass is tripled to 6 kg6\ \text{kg} instead.

Step 1. Identify the case. Here m1=m2=2 kgm_1=m_2=2\ \text{kg}, u1=6 m/su_1=6\ \text{m/s}, u2=0u_2=0 — the equal-mass special case, so we expect complete velocity exchange.

Step 2. Apply the general formulas. v1=(m1−m2)u1+2m2u2m1+m2=0+04=0 m/sv_1 = \dfrac{(m_1-m_2)u_1+2m_2u_2}{m_1+m_2} = \dfrac{0+0}{4} = 0\ \text{m/s}, and v2=(m2−m1)u2+2m1u1m1+m2=0+2(2)(6)4=244=6 m/sv_2 = \dfrac{(m_2-m_1)u_2+2m_1u_1}{m_1+m_2} = \dfrac{0+2(2)(6)}{4} = \dfrac{24}{4} = 6\ \text{m/s}.

Step 3. Interpret. The first ball stops completely and the second moves off at 6 m/s6\ \text{m/s} — the incoming ball's entire velocity is transferred, exactly as the equal-mass rule predicts.

Answer: v1=0 m/sv_1 = 0\ \text{m/s}, v2=6 m/sv_2 = 6\ \text{m/s}.

Competitive stretch

Now keep m1=2 kgm_1=2\ \text{kg}, u1=6 m/su_1=6\ \text{m/s}, u2=0u_2=0, but make the target heavier: m2=6 kgm_2=6\ \text{kg}. Using the same formulas, v1=(2−6)(6)+08=−248=−3 m/sv_1 = \dfrac{(2-6)(6)+0}{8} = \dfrac{-24}{8} = -3\ \text{m/s} and v2=0+2(2)(6)8=248=3 m/sv_2 = \dfrac{0+2(2)(6)}{8} = \dfrac{24}{8} = 3\ \text{m/s}. The incoming ball rebounds backward at 3 m/s3\ \text{m/s} (negative sign, reversed direction) while the heavier target moves forward at 3 m/s3\ \text{m/s} — a preview of the m1≪m2m_1 \ll m_2 trend, though here the mass ratio is only 1:31:3, not extreme enough for the full v1≈−u1v_1 \approx -u_1, v2≈0v_2 \approx 0 approximation to kick in yet.

Common traps

  • Assuming kinetic energy is conserved in every collision — only elastic collisions conserve it; momentum is conserved in all collisions (isolated system).
  • Mixing up the three special cases — m1=m2m_1=m_2, m1≫m2m_1\gg m_2, and m1≪m2m_1\ll m_2 give distinctly different outcomes and must be matched to the actual mass ratio, not applied by memory alone.
  • Dropping the sign on a rebound velocity — when the light body bounces back off a heavy one, v1v_1 is negative, and that sign must carry through any energy or further-motion calculation.
  • Thinking "perfectly inelastic" means the final kinetic energy is zero — the combined body still moves (unless total momentum is exactly zero) and only the conservation of kinetic energy fails, not motion itself.

Ask the tutor: Want to work through a few more one-dimensional collisions with different mass ratios, or see how the coefficient of restitution generalises the elastic and inelastic cases together?

Why does relative velocity of approach equal relative velocity of separation only for elastic collisions?

That relation, u1−u2=v2−v1u_1-u_2 = v_2-v_1, comes directly from combining momentum and kinetic-energy conservation, as shown in the derivation above — it only holds when both quantities are conserved, which is the definition of an elastic collision. In an inelastic collision kinetic energy is not conserved, so the algebra that produced that neat relative-velocity relation breaks down, and the bodies separate more slowly than they approached (or, in the perfectly inelastic case, do not separate at all).

Does it matter which body I call body 1 and which I call body 2?

No, as long as you are consistent. The formulas are symmetric under swapping the labels: if you relabel body 1 as body 2 and vice versa, the formula for v1v_1 becomes the formula for v2v_2 and vice versa. What genuinely matters is getting the sign of each velocity right relative to one chosen positive direction along the line of motion — that convention, not the numbering, is where marks are usually lost.

If momentum is always conserved, why do we say kinetic energy is "lost" in an inelastic collision?

"Lost" here means lost from the kinetic energy of the two bodies' overall motion — it has not vanished, by the law of conservation of energy overall. It has converted into other forms: heat generated by internal friction during impact, sound waves radiating away, and permanent deformation (bent metal, a dented panel) that stores energy in the bodies' internal structure. Momentum only tracks motion of the centre of mass, so it is untouched by where that energy goes; kinetic energy tracks the bodies' bulk motion specifically, so it visibly drops.

Before this

Where this leads