A.5.4 (HL)—Galilean velocity addition
- Syllabus
- First assessment 2025
- Objective
- —
- Level
- HL
Use the classical addition rule
If an object has velocity u in frame S and frame S′ moves at velocity v relative to S, the velocity measured in S′ is u′=u−v. Both u and v are signed velocities along the chosen axis.
Calculate in two steps
Choose the positive direction, write the velocity of the object and the relative frame velocity with signs, then subtract. If the object and S′ move in the same direction, the relative speed is reduced; if they move in opposite directions, the signed relative velocity has greater magnitude.
Check the model
Galilean addition assumes inertial frames, common time, and non-relativistic speeds. It can predict a resultant speed greater than c, which signals that special relativity—not the arithmetic—is required for a high-speed light problem.
Worked example from local Question Bank row 31297
In the classical model, two spacecraft moving in opposite directions at 0.80c have signed velocities u=−0.80c and v=+0.80c.
u′=u−v=−0.80c−0.80c=−1.60c
The magnitude 1.60c shows why Galilean addition cannot describe relativistic relative velocity; the sign only gives direction in S′.
Common trap
Do not subtract speed magnitudes before deciding the direction. The sign of u′ tells you the object’s direction in S′; dropping signs can reverse the physical interpretation.
Questions ask for the speed of a signal or the travel time seen by an observer after combining velocities. The evidence rewards a correct relative-velocity expression and a clearly shown substitution.
State / Calculate
Choose a positive direction and write u′ = u − v before substituting. Use signed velocities, keep c in the units where it is given, show the subtraction, and interpret the sign of u′ as the direction in the moving frame.
Treating velocity magnitudes as unsigned and losing the direction of the relative motion.
Representative question
State, using Galilean relativity, the speed of the radio signal relative to Q .
Choose the model
State the inertial reference frame first. Galilean relativity uses x′=x−vt, t′=t and u′=u−v. Special relativity uses the two postulates, Lorentz transformations and u′=(u−v)/(1−uv/c²).
Track what changes and what is invariant
In special relativity, use γ=1/√(1−v²/c²), the invariant interval (Δs)²=(cΔt)²−(Δx)², proper time, proper length, Δt=γΔt0 and L=L0/γ. Separate measurements of space and time can change between frames, while the interval and vacuum light speed do not.
Read the evidence
On a space–time diagram, world-line angle gives tanθ=v/c, frame axes determine simultaneity, and no world line exceeds the light line. Muon survival provides experimental evidence: time dilation explains the longer Earth-frame lifetime, while length contraction explains the shorter atmospheric distance in the muon frame.
Final retrieval check
For every calculation, identify the frame, select the proper quantity if one is given, keep signed velocities and units consistent, and check the result against c, γ≥1, or the invariant interval. The syllabus requires applying the transformations and equations, not deriving them.