Time Dilation Calculator

Enter a proper time and a relative velocity to find the Lorentz factor (γ = 1 / √(1 − v²/c²)) and the dilated time Δt = γΔt₀ that a stationary observer measures.

Quick Facts

Time dilation formula
Δt = Δt₀ / √(1 − v²/c²)
Δt₀ is the proper time on the moving clock; Δt is the longer interval measured by a stationary observer.
Lorentz factor
γ = 1 / √(1 − v²/c²)
Always ≥ 1; stays near 1 at everyday speeds, then rises sharply as v approaches c.
Speed of light
c = 299,792,458 m/s
v must stay strictly below c for any object with mass, or the formula is undefined.

Your Results

Calculated
Lorentz Factor (γ)
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γ = 1 / √(1 − v²/c²)
Dilated Time (Δt)
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Time elapsed for the stationary observer
Extra Time Elapsed
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Δt − Δt₀, the time "gained" in the stationary frame
Velocity (β = v/c)
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Relative velocity as a fraction of light speed

Ready

Enter a proper time and a relative velocity below the speed of light, then press Calculate.

How Time Dilation Is Calculated

Time dilation is a direct consequence of Einstein's special theory of relativity: a clock moving relative to an observer runs slower, from that observer's point of view, than an identical clock at rest with them. The proper time (Δt₀) is the interval measured by a clock traveling with the moving object itself — for example, the elapsed time on an astronaut's wristwatch. The dilated time (Δt) is the longer interval measured by a stationary observer watching that clock go by. The two are related by Δt = Δt₀ / √(1 − v²/c²) = γΔt₀, where v is the relative velocity between the two frames and c is the speed of light in a vacuum (299,792,458 m/s).

The Lorentz factor (γ)

The quantity γ = 1 / √(1 − v²/c²) is called the Lorentz factor. It depends only on the ratio β = v/c, not on the direction of motion, and it is always greater than or equal to 1. At everyday speeds — cars, planes, even orbital spacecraft — β is a tiny fraction of a percent, so γ is indistinguishable from 1 and the dilation is far too small to notice without atomic clocks. As v climbs toward c, γ grows nonlinearly: at β = 0.6 (60% of c), γ = 1.25; at β = 0.99, γ ≈ 7.09; at β = 0.9999, γ ≈ 70.7. Because γ blows up as β → 1, no object with mass can ever reach or exceed the speed of light — the formula becomes undefined (division by zero) exactly at v = c.

Proper time vs. dilated time in practice

This calculator takes the proper time Δt₀ (the time the moving object experiences) and the relative velocity v, then computes γ and the dilated time Δt that a stationary observer would measure. The effect is real and measured routinely: cosmic-ray muons created in the upper atmosphere travel at roughly 0.998c and, thanks to time dilation, survive long enough in their own decaying "clock" to reach the ground — without dilation, their short particle lifetime would let them travel only a fraction of that distance. Particle accelerators push electrons and protons to γ factors in the thousands, and the effect has been confirmed directly with atomic clocks flown on aircraft. Note that this tool covers kinematic (velocity-based) time dilation only; time dilation caused by gravity — relevant to GPS satellites and clocks at different altitudes — follows a different formula from general relativity.

Frequently Asked Questions

What is time dilation?
Time dilation is the difference in elapsed time measured by two observers moving relative to each other. In special relativity, a clock moving at velocity v relative to an observer ticks slower, from that observer's perspective, by the Lorentz factor γ = 1 / √(1 − v²/c²).
What is the formula for time dilation?
The special-relativistic time dilation formula is Δt = Δt₀ / √(1 − v²/c²), where Δt₀ is the proper time measured in the moving object's own frame, Δt is the dilated time measured by a stationary observer, v is the relative velocity, and c is the speed of light (about 299,792,458 m/s).
Why can't the velocity reach or exceed the speed of light in this formula?
As v approaches c, the term (1 − v²/c²) under the square root approaches zero, so the Lorentz factor grows without bound. At v = c the formula divides by zero, and for v greater than c the term under the square root turns negative. This is one reason special relativity treats c as an absolute speed limit for any object with mass.
Is this the same as gravitational time dilation?
No. This calculator computes kinematic (velocity-based) time dilation from special relativity. Gravitational time dilation, which causes clocks to run slower in stronger gravitational fields such as near a planet, follows a different formula from general relativity — see our Gravitational Time Dilation Calculator for that case.