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Length Contraction Calculator (relativistic L = L₀/γ)

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Understanding the length contraction calculator — concept and principle

This calculator applies special relativity to find how much shorter a moving object is measured along its direction of motion. It gives the contracted length, the shortening, the length as a percentage of the proper length and the Lorentz factor. It is used in physics courses and to explore what happens near the speed of light.

Relativistic length contractionA 100 m ship at 0.9 cProper length100 mSpeed0.9 cL = 100 × √(1 − 0.9²) = 100 × 0.43589Measured length43.589 mγ2.29416Shortened by56.41 m
Only the length along the motion shrinks, and only for observers who see the ship moving.

How it is calculated

L = L₀ √(1 − v²/c²) = L₀ ÷ γ

γ = 1 ÷ √(1 − v²/c²)

Shortening = L₀ (v/c)² ÷ (1 + √(1 − v²/c²))

The principle

Special relativity says the speed of light is the same for every observer. To keep it so, observers moving relative to each other must disagree about times and lengths. Measuring a moving object's length means marking both ends at the same moment, and observers disagree about what "the same moment" is. The result is that a moving object is shorter along its motion by the factor γ. Widths across the motion do not change. The shortening formula used here avoids rounding loss at everyday speeds, where the effect is far smaller than an atom.

Worked example

Default inputs: L₀ = 100 m, speed 90% of c.

  1. v/c = 0.9, so √(1 − 0.81) = √0.19 = 0.43589.
  2. γ = 1 ÷ 0.43589 = 2.29416.
  3. L = 100 × 0.43589 = 43.589 m, which is 43.589% of the proper length.
  4. Shortening = 100 − 43.589 = 56.41 m.
How Contracted length (m) changes with Proper length at rest (m)How Contracted length changes with Prope…020406080100255075100125150200Example: 43.589Proper length at rest (m)
Each point is the calculator re-run with only “Proper length at rest (m)” changed; the gold point is the default example. Change the inputs above and this chart follows your numbers.
Proper length at rest (m)Contracted length (m)
2510.8972
5021.7945
7532.6917
10043.589
12554.4862
15065.3835
20087.178

How to read the result

Contraction is negligible at everyday speeds and only becomes large close to c: at 50% of c the length is still about 87%, while at 99% it is about 14%. The proper length is always the longest measured length. Fast muons reaching the ground from the upper atmosphere are a classic test: in their frame, the atmosphere is contracted.

Common mistakes

Keep in mind: The formula applies to inertial frames in special relativity. Accelerating objects and gravity need more careful treatment.

Frequently asked questions

Would a moving object look shorter in a photograph?

Not simply; light-travel-time effects make it appear rotated or distorted rather than just contracted.

How fast must something go to halve its length?

About 86.6% of the speed of light, where γ = 2.

Does the moving object notice anything?

No. In its own frame it has its proper length.

How is this linked to time dilation?

Both use the same γ; moving clocks run slow by the same factor that lengths contract.

Sources: OpenStax, University Physics Volume 3 (2016), section 5.4 "Length Contraction"

Checked 9 Nov 2026. OpenStax, University Physics Volume 3 (2016), §5.4 “Length Contraction” (eq. 5.4 L = L₀√(1 − v²/c²); muon example at 0.950c; Example 5.5: γ = 30.00, 4.300 ly → 0.1433 ly). c exact (2019 SI).

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