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  1. Home
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  3. /Relativity Calculators
  4. /Time Dilation Calculator

Time Dilation Calculator

Last updated: March 18, 2026

Calculator

Results

Enter values to see results

Lorentz Factor (γ)

—

Dilated Time (t)

—

s

Time Difference (Δt)

—

s

β = v/c

—

Results

Enter values to see results

Lorentz Factor (γ)

—

Dilated Time (t)

—

s

Time Difference (Δt)

—

s

β = v/c

—

The Time Dilation Calculator computes how time intervals stretch for objects moving at relativistic speeds, one of the most remarkable predictions of Einstein's special theory of relativity. According to the time dilation formula $$t = \frac{t_0}{\sqrt{1 - v^2/c^2}} = \gamma\, t_0$$ a clock moving at velocity v relative to an observer ticks more slowly than a stationary clock. Here $$t_0$$ is the proper time measured by the moving clock, and $$t$$ is the dilated time measured by the stationary observer.

Time dilation is not merely a theoretical curiosity — it is confirmed by experiments with muon decay, atomic clocks on aircraft and satellites, and is essential for the accuracy of GPS navigation. Without relativistic corrections, GPS positions would drift by roughly 10 km per day. This calculator lets you explore how the Lorentz factor $$\gamma$$ grows as velocity approaches the speed of light, and how dramatically time stretches at ultra-relativistic speeds.

Visual Analysis

How It Works

In special relativity, time is not absolute. Two observers in relative motion measure different time intervals between the same pair of events. If a clock is at rest in a moving frame (the proper frame), it measures the proper time $$t_0$$. An observer in a different inertial frame sees that clock running slow by the Lorentz factor:

$$t = \gamma\, t_0 = \frac{t_0}{\sqrt{1 - \beta^2}}$$

where $$\beta = v/c$$ is the velocity as a fraction of the speed of light, and $$\gamma = (1 - \beta^2)^{-1/2}$$ is the Lorentz factor. Key properties of time dilation:

  • Reciprocal effect: Each observer sees the other's clock running slow. This is consistent because the two observers disagree on simultaneity.
  • γ at low speeds: For everyday velocities, $$\gamma \approx 1 + \frac{v^2}{2c^2}$$, so the effect is negligible. At 1000 km/h, γ differs from 1 by only about 4 parts in 1013.
  • γ diverges near c: As $$v \to c$$, $$\gamma \to \infty$$. At 99% of c, γ ≈ 7.09; at 99.99%, γ ≈ 70.7.
  • Proper time is minimum: The proper time (measured by the clock present at both events) is always the shortest time interval. All other observers measure longer intervals.

Experimental confirmations include the observation that cosmic-ray muons (with a rest-frame lifetime of 2.2 μs) survive the trip from the upper atmosphere to Earth's surface because their clocks run slow in our frame. The Hafele-Keating experiment (1971) flew atomic clocks around the world and measured time differences matching special and general relativistic predictions to within 10%.

Note that gravitational time dilation (from general relativity) is a separate effect not included here. Near massive bodies, clocks run slower in stronger gravitational fields.

Understanding Your Results

The Lorentz factor γ tells you how much time is stretched. A γ of 2 means the moving clock ticks at half the rate of the stationary clock — one second of proper time corresponds to two seconds for the observer. The time difference shows the extra elapsed time the stationary observer measures. At low velocities (β ≪ 1), γ is essentially 1 and time dilation is unmeasurable. The effect only becomes significant above about 10% of the speed of light (β > 0.1, γ ≈ 1.005).

Worked Examples

Muon Lifetime in Cosmic Rays

Inputs

proper time0.0000022
velocity296794533
input modems

Results

gamma7.0888
dilated time0.0000156
time difference0.0000134
beta0.99

A muon with a 2.2 μs rest-frame lifetime at 0.99c has a dilated lifetime of about 15.6 μs, allowing it to travel ~4.6 km and reach Earth's surface from the upper atmosphere.

GPS Satellite Clock

Inputs

proper time86400
velocity3874
input modems

Results

gamma1.0000000000835
dilated time86400.0000072
time difference0.0000072
beta0.00001292

A GPS satellite at 3.87 km/s experiences about 7.2 μs per day of special-relativistic time dilation. Combined with general-relativistic effects (~45 μs/day), GPS must correct for a net ~38 μs/day.

Frequently Asked Questions

Time dilation is the phenomenon where a clock moving relative to an observer ticks more slowly than a clock at rest relative to that observer. The relationship is $$t = \gamma t_0$$, where $$\gamma = 1/\sqrt{1 - v^2/c^2}$$. This is not an illusion or mechanical effect — it is a fundamental property of spacetime.

Proper time $$t_0$$ is the time interval measured by a clock that is present at both events (start and end). It is the time measured in the rest frame of the moving object. Proper time is always the shortest time interval between two events — all other observers measure a longer (dilated) time.

Yes, many times. Key experiments include: cosmic-ray muon survival (1940s–present), the Hafele-Keating experiment with atomic clocks on aircraft (1971), particle accelerator lifetime measurements, and ongoing GPS satellite corrections. All confirm special relativity to high precision.

Time dilation allows effective forward time travel: by traveling at high speed, you age less than people who remain stationary. A round trip at 0.99c for 1 year of proper time means 7 years pass on Earth. However, backward time travel is not permitted by special relativity.

The twin paradox imagines one twin traveling at high speed while the other stays home. The traveling twin ages less due to time dilation. The apparent paradox — why isn't the effect symmetric? — is resolved by noting the traveling twin must accelerate to turn around, breaking the symmetry between the two frames.

GPS satellites move at ~3.87 km/s and orbit at ~20,200 km altitude. Special relativity causes their clocks to lose ~7 μs/day, while general relativity (weaker gravity at altitude) causes them to gain ~45 μs/day. The net ~38 μs/day gain must be corrected, or position errors would accumulate at ~10 km/day.

Sources & Methodology

Einstein, A. (1905). On the Electrodynamics of Moving Bodies. Annalen der Physik, 17, 891–921. Hafele, J.C. & Keating, R.E. (1972). Science, 177, 166–170. Taylor, E.F. & Wheeler, J.A. (1992). Spacetime Physics, 2nd Ed. W.H. Freeman. NIST: https://physics.nist.gov/cuu/Constants/
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