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Length Contraction Calculator

The contracted length of a moving object as seen by an observer it passes, with the Lorentz factor and the speed in ordinary units.

Special relativity: an object moving at speed v is measured shorter along its direction of motion by the Lorentz factor γ = 1 ÷ √(1 − v²/c²).

Results update as you type
Results
Contracted length
43.589
Lorentz factor γ
Shortened by
Speed
Time dilation at this speed
Reviewed September 2026. Physics is the same everywhere: SI units in, with imperial equivalents in the results.
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About length contraction

How the length contraction calculator works

Special relativity: an object moving at speed v is measured shorter along its direction of motion by the Lorentz factor γ = 1 ÷ √(1 − v²/c²). At everyday speeds γ is 1 to a dozen decimal places; at 0.9 c a 100 m ship measures 43.6 m. The object itself notices nothing — in its own frame it is the observer who is contracted.

Formula: L = L₀ ÷ γ; γ = 1 ÷ √(1 − β²); β = v ÷ c

Worked examples

InputsContracted lengthNote
100 m ship at 0.9 c43.58943.59 m, γ = 2.294
At 0.5 c86.602586.60 m
A meter rule at 0.99 c0.14110.141 m

Frequently asked questions

Does the object really get shorter?

In the observer’s frame, yes — it is a real measurement, not an illusion — but in the object’s own frame nothing changes. Length, like simultaneity, depends on the frame it is measured in.

Does it contract in every direction?

No, only along the direction of motion. Width and height are unchanged, so a fast-moving sphere measures as a flattened ellipsoid.

Why is there no effect at everyday speeds?

γ − 1 is about ½ β²; at an airliner’s 250 m/s, β is 8 × 10⁻⁷ and the contraction of a 70 m aircraft is a few hundred-billionths of a meter.

How does this relate to time dilation?

Same factor, opposite way: moving clocks run slow by γ while moving lengths shrink by γ. Together they keep the speed of light the same for everyone.

Where these figures come from

Last checked: September 2026. Constants are the CODATA 2018 values; formulas are the standard textbook forms.