Special Relativity: Length Contraction

April 12, 2026

Problem

A spaceship has a rest length of L₀ = 100 m. When traveling at v = 0.9c relative to a stationary observer, its observed length contracts to L = L₀/γ = L₀√(1 − v²/c²). Calculate the contracted length and animate the ship shrinking as speed increases.

Explanation

Length contraction is time dilation's spatial twin: just as moving clocks run slow, moving objects are shortened in their direction of motion as measured by a stationary observer. A 100-meter spaceship traveling at 0.9c appears to be only 43.6 meters long to someone standing on Earth.

L=L0γ=L01v2c2L = \dfrac{L_{0}}{\gamma} = L_{0}\sqrt{1 - \dfrac{v^{2}}{c^{2}}}

For v=0.9cv = 0.9c: L=10010.81=1000.19=100×0.4359=43.6L = 100\sqrt{1 - 0.81} = 100\sqrt{0.19} = 100 \times 0.4359 = 43.6 m.

The ship isn't "crushed" — nothing happens to it in its own frame. The passengers measure their ship as 100 m long. But measurements made by the Earth observer (who sees the ship moving) yield a shorter length. It's a property of spacetime itself, not a mechanical effect.

Symmetry and consistency

Just as with time dilation, length contraction is symmetric: the ship's passengers see Earth (and everything on it) contracted in the direction of motion. Earth looks "squished" to them by the same factor γ.

This seems contradictory but isn't — the two observers disagree about what counts as "simultaneous" (they measure the front and back of the object at different events), and this disagreement exactly accounts for the apparent paradox.

Connection to time dilation via the muon

The cosmic-ray muon example connects both effects beautifully:

Earth's perspective: The muon's clock runs slow (time dilation). Its lifetime is stretched by γ ≈ 15.8, giving it enough time to travel ~10 km and reach the ground.

Muon's perspective: The muon's clock runs normally (2.2 μs). But the atmosphere is length-contracted from 10 km to ~630 m. The muon only needs to travel 630 m, which it can easily do in 2.2 μs at 0.998c. Both frames agree: the muon reaches the ground.

Common mistakes

  • Thinking the contraction is visible to the eye. What you'd actually see with a camera is more complex — the Penrose-Terrell rotation effect makes objects look rotated, not simply squished, because of the finite speed of light from different parts of the object reaching your eye at different times.
  • Applying contraction in the perpendicular direction. Length contraction only occurs along the direction of motion. A ship moving horizontally contracts horizontally but NOT vertically.

Try it in the visualization

Drag the speed slider and watch the ship visually contract. At rest, it's 100 m. At 0.9c, it's 43.6 m. At 0.99c, it's only 14.1 m. The ruler below shows the measurement. Toggle "muon view" to see length contraction from the muon's frame, where the atmosphere shrinks instead of the muon's lifetime stretching.

Interactive Visualization

Parameters

0.90
100.00
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Special Relativity: Length Contraction | MathSpin