Length Contraction Calculator

Enter the proper length (L₀) of an object and its relative velocity (v) to calculate the observed (contracted) length as seen by a stationary observer. The Length Contraction Calculator applies the Lorentz contraction formula from special relativity, also showing the Lorentz factor (γ) and the velocity as a fraction of the speed of light.

m

The length of the object measured in its own rest frame.

km/s

Velocity of the moving object relative to the observer. Max is the speed of light (~299,792 km/s).

Results

Observed (Contracted) Length

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Lorentz Factor (γ)

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Velocity as Fraction of c (v/c)

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Length Difference (ΔL)

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Contraction Percentage

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Observed Length vs. Contracted Portion

Frequently Asked Questions

What is length contraction?

Length contraction is a phenomenon predicted by Einstein's special theory of relativity. An object moving at a significant fraction of the speed of light appears shorter along its direction of motion when measured by a stationary observer, compared to its length measured in its own rest frame. The effect is also known as Lorentz contraction.

What is the length contraction formula?

The formula is L = L₀ × √(1 − v²/c²), where L is the observed (contracted) length, L₀ is the proper length (rest length), v is the relative velocity of the object, and c is the speed of light (~299,792,458 m/s). This can also be written as L = L₀ / γ, where γ is the Lorentz factor.

What is the Lorentz factor (γ)?

The Lorentz factor, denoted γ (gamma), is defined as γ = 1 / √(1 − v²/c²). It quantifies how much time, length, and relativistic mass change at a given velocity. At low speeds γ ≈ 1 and effects are negligible; as velocity approaches c, γ approaches infinity.

What is proper length (L₀)?

Proper length is the length of an object measured in the reference frame where the object is at rest. It is the maximum possible length of the object — any observer moving relative to the object will measure a shorter length due to relativistic contraction.

At what speeds does length contraction become noticeable?

Length contraction is only significant at speeds that are a substantial fraction of the speed of light (roughly above 10% of c, or ~30,000 km/s). At everyday speeds — even the fastest spacecraft — the contraction is so tiny it is immeasurable. For example, at 90% of c, an object contracts to about 44% of its rest length.

Can an object travel faster than the speed of light?

No. According to special relativity, no object with mass can reach or exceed the speed of light (c ≈ 299,792 km/s). As velocity approaches c, the energy required becomes infinite. If v = c were entered, the contracted length would be zero and the Lorentz factor would be undefined (infinite), which is physically impossible for a massive object.

What is the ladder (pole-barn) paradox related to length contraction?

The ladder paradox is a classic thought experiment in special relativity. A ladder moving at relativistic speed appears short enough to fit inside a barn that would be too small for it at rest — yet from the ladder's reference frame, the barn appears contracted instead. This apparent paradox is resolved by the relativity of simultaneity: the two ends of the ladder don't pass through the barn doors at the same time in both frames.

Does length contraction affect all dimensions of an object?

No. Length contraction only occurs along the axis of motion (the direction of travel). The dimensions perpendicular to the direction of motion remain unchanged. So a sphere moving at relativistic speed would appear as a flattened disk when measured by a stationary observer.

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