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L = L₀ / γ = L₀ · √(1 − v²/c²) (Lorentz factor γ = 1/√(1 − v²/c²))
Calculate contracted length from proper length and velocity.
Length of the object in its own rest frame (meters).
Length observed in the moving frame (meters).
Velocity as a fraction of the speed of light (0 to 0.999999).
Select the velocity unit.
Unit for length values.
Decimal places in results.
📋 Length Contraction Reference Formula, key values & real-world examples
Key Formula & Values
L = L₀ / γ = L₀ · √(1 − v²/c²)
γ = 1/√(1 − v²/c²)
c (speed of light)299,792,458 m/s
γ at 0.5c1.1547 → L = 0.866 L₀
γ at 0.9c2.294 → L = 0.436 L₀
γ at 0.99c7.089 → L = 0.141 L₀
γ at 0.999c22.37 → L = 0.0447 L₀
Contraction Factors
0.1c0.995 L₀
0.2c0.980 L₀
0.3c0.954 L₀
0.4c0.917 L₀
0.5c0.866 L₀
0.6c0.800 L₀
0.7c0.714 L₀
0.8c0.600 L₀
0.9c0.436 L₀
0.99c0.141 L₀
Real-World Examples
Particle acceleratorsBunches appear flattened
Muon experimentAtmospheric path contracted
Cosmic raysExtended range explained
GPS satellitesRelativistic corrections
Heavy-ion collisionsLorentz-contracted nuclei
Source: CERN, NIST, NASA
Note: Length contraction occurs only along the direction of motion. Perpendicular dimensions are unaffected. The contraction is not an illusion — it is a real physical effect measured in the observer's frame. The proper length L₀ is the maximum length, measured in the object's rest frame. This is the Lorentz-Fitzgerald contraction.
📌 Quick Reference: L = 0.866 L₀ at 0.5c  |  L = 0.436 L₀ at 0.9c  |  L = 0.141 L₀ at 0.99c  |  c = 299,792,458 m/s

What Is Length Contraction?

Length contraction (also called Lorentz contraction or Lorentz-Fitzgerald contraction) is a relativistic effect predicted by Albert Einstein's special theory of relativity (1905). It states that an object moving at relativistic speed is measured to be shorter in the direction of motion compared to its length at rest.

This effect is not a mechanical compression — it is a fundamental property of spacetime geometry. Length contraction and time dilation are two sides of the same relativistic coin.

Key characteristics of length contraction:

  • Direction-dependent: Contraction occurs only along the direction of relative motion. Perpendicular dimensions are unaffected.
  • Proper length (L₀): The maximum length, measured in the object's rest frame.
  • Contracted length (L): The length measured by an observer in relative motion, always ≤ L₀.
  • Symmetry: Each observer sees the other's objects contracted — the effect is reciprocal.
  • Real effect: Contraction is not an optical illusion; it is a genuine physical measurement.

The Length Contraction Formula

The formula for length contraction is:

L = L₀ / γ

where the Lorentz factor is: γ = 1 / √(1 − v²/c²)

Equivalently: L = L₀ · √(1 − v²/c²)

At low velocities (v ≪ c), γ ≈ 1 and length contraction is negligible. As v approaches c, γ increases without bound, meaning length contracts toward zero as v → c.

Key Contraction Values

The following table shows how the contraction factor changes with velocity:

  • 0.1c → L = 0.995 L₀ (0.5% contraction)
  • 0.5c → L = 0.866 L₀ (13.4% contraction)
  • 0.9c → L = 0.436 L₀ (56.4% contraction)
  • 0.99c → L = 0.141 L₀ (85.9% contraction)
  • 0.999c → L = 0.0447 L₀ (95.5% contraction)

At 0.5c, a 10-meter object measures 8.66 meters. At 0.99c, it measures only 1.41 meters.

Real-World Applications

Length contraction has been experimentally verified and is essential in many fields:

  • Particle accelerators: At CERN, particle bunches moving at 0.999999c appear flattened in the laboratory frame. This affects collision dynamics and detector design.
  • Muon experiment: Muons created in the upper atmosphere have a lifetime of 2.2 μs at rest, which would allow them to travel only ~660 m. Because of length contraction (and time dilation), they reach the ground from ~10 km altitude.
  • Heavy-ion collisions: At RHIC and LHC, lead nuclei are Lorentz-contracted into "pancakes" at collision energy.
  • GPS satellites: Relativistic corrections include length contraction effects to maintain timing accuracy.

Why Use This Calculator?

  • Solve for any variable: Calculate L, L₀, or v depending on what's unknown.
  • Multiple velocity units: Enter velocity as a fraction of c, or in m/s or km/s.
  • Step-by-step solution: See exactly how the calculation is performed.
  • Visual comparison: See proper length and contracted length side by side.
  • Free & private: No registration, no data storage — all calculations are done in your browser.

❓ Length Contraction Calculator FAQ

What is length contraction?

Length contraction is the relativistic effect where a moving object is measured to be shorter in the direction of motion compared to its length at rest. It becomes significant only at velocities approaching the speed of light.

What is the length contraction formula?

The formula is L = L₀ / γ = L₀ · √(1 − v²/c²), where L is the contracted length, L₀ is the proper length (rest length), v is the relative velocity, and c is the speed of light.

What is proper length?

Proper length (L₀) is the length of an object measured in its own rest frame — the frame in which the object is stationary. It is the maximum possible length of the object.

Does length contraction occur in all directions?

No. Length contraction occurs only along the direction of relative motion. Dimensions perpendicular to the motion are unaffected. For example, a moving sphere becomes an oblate spheroid (flattened along the direction of motion).

Is length contraction real or just an illusion?

It is a real physical effect, not an optical illusion. It is a consequence of the relativity of simultaneity — different observers disagree on which events are simultaneous, and this leads to different measured lengths.

Why can't we notice length contraction in everyday life?

Length contraction only becomes significant at velocities near the speed of light. At everyday speeds (e.g., a car at 100 km/h), the contraction is less than the diameter of a single atom — utterly imperceptible.

What is the Lorentz-Fitzgerald contraction?

Lorentz-Fitzgerald contraction is another name for length contraction. It was originally proposed by George FitzGerald and Hendrik Lorentz to explain the Michelson-Morley experiment, before Einstein derived it from first principles in special relativity.

Does length contraction affect GPS?

Yes, indirectly. GPS satellites move at about 3.9 km/s relative to Earth, giving γ ≈ 1.00000000008. The length contraction is tiny but relativistic corrections (including both special and general relativistic effects) are essential for GPS accuracy.

How accurate is this calculator?

This calculator uses the exact special relativistic length contraction formula. Results are accurate to the precision you select. For velocities very close to c, extremely high precision is needed to see the effect.

Is this calculator free?

Yes, this calculator is completely free to use. No registration or personal data storage is required.