Time Dilation Relativity Calculator
Enter a velocity and proper time to calculate how much time passes for a stationary observer due to special relativistic time dilation.
Inputs
Duration experienced by the moving object
c = 299,792,458 m/s
Result
If a traveler experiences
—
a stationary observer measures
—
Lorentz Factor
—
γ
Time Ratio
—
Δt′ / Δt
Extra Time
—
Δt′ − Δt
Calculation Details
Velocity vs. Time Dilation Reference Table
| Velocity (v/c) | Lorentz Factor (γ) | Observer Time per Traveler Year | Extra Time per Year |
|---|
Observer time = γ × traveler time. At 0.1c, the effect is negligible (<0.5%). Near c, it grows without bound.
Gravitational Time Dilation (General Relativity)
This calculator covers velocity-based time dilation from special relativity. A separate but related effect — gravitational time dilation — comes from general relativity: clocks deeper in a gravitational well (closer to a massive body) run slower than clocks farther away. GPS satellites experience both effects simultaneously. The velocity effect makes satellite clocks run ~7 μs/day slower; the gravitational effect makes them run ~45 μs/day faster — for a net +38 μs/day correction applied in GPS firmware.
Summary
Enter a velocity and proper time to calculate how much time passes for a stationary observer due to special relativistic time dilation.
How it works
- Enter the proper time — the duration experienced by the moving traveler.
- Select the time unit (seconds, minutes, hours, days, or years).
- Enter the velocity as a fraction of the speed of light (e.g. 0.8 for 80% of c) or in m/s.
- The calculator computes the Lorentz factor γ = 1 / √(1 − v²/c²).
- Dilated time Δt' = γ × Δt is the duration measured by a stationary observer.
Use cases
- Verify textbook special relativity problems and homework exercises.
- Explore how close to the speed of light a spaceship must travel for meaningful time differences.
- Calculate aging differences for twin paradox thought experiments.
- Understand why muons created in the upper atmosphere reach Earth's surface.
- Compare relativistic time effects across different velocities for physics courses.
- Estimate onboard vs. mission-control elapsed time for hypothetical interstellar travel.