A.5.11 (HL)—Length contraction

Syllabus
First assessment 2025
Objective
Level
HL

Calculate Length Contraction

HL only

Use the contraction equation

If L0L_0 is the proper length measured in the object’s rest frame, an observer who sees the object moving at speed vv measures L=L0/γL=L_0/\gamma, with γ=1/1v2/c2\gamma=1/\sqrt{1-v^2/c^2}.

Select the proper length

Find the frame in which the object is at rest; that frame measures L0L_0. Calculate γ\gamma, then divide the proper length by γ\gamma. The endpoints must be measured simultaneously in the observer’s frame.

Check the result

Since γ1\gamma\ge1, a moving observer measures LL0L\le L_0. At low speed the contraction is negligible; as vv approaches cc, the measured length along the direction of motion becomes substantially smaller.

Worked example from local Question Bank row 30450

A rocket's proper length is L0=450mL_0=450\,\mathrm{m} and γ=5/3\gamma=5/3. An observer who sees it moving measures

L=L0γ=4505/3=270mL=\frac{L_0}{\gamma}=\frac{450}{5/3}=270\,\mathrm{m}

Only the dimension parallel to the relative motion is contracted.

Common trap

Do not contract a length perpendicular to the motion, and do not multiply by γ\gamma when the requested quantity is the moving-frame length.

A.5.11 (HL) Exam Analysis

HL only

Assessment in practice

2–3 marks
How it is assessed

Questions ask you to calculate a moving space station’s length or compare a spaceship measurement with an Earth-frame distance. The evidence rewards finding γ and applying the division in the correct direction.

Command terms

Calculate

What earns marks

Identify L0 as the object’s rest-frame length, calculate γ = 1/√(1 − v²/c²), and use L = L0/γ for the moving observer. State that the measurement is along the direction of motion and check that L is no greater than L0.

Watch for

Multiplying the proper length by γ or applying contraction to a direction perpendicular to the relative motion.

Representative question

Question 1

[Maximum number: 2]

Calculate the length of the space station according to observer B, with reference to special relativity.