CCalclabhub

Relativity

How To Calculate Time Dilation

Time dilation is the special relativity result that a moving clock ticks more slowly. The effect is tiny at everyday speeds and dramatic once you get close to the speed of light.

Quick Answer

t = t0 / sqrt(1 - v^2/c^2), where the reciprocal of the root is the Lorentz factor

t
The time measured by the stationary observer
t0
The proper time, measured by the moving clock
v
The speed of the moving clock
c
The speed of light, 299,792,458 metres per second

Divide the velocity by the speed of light, square it, subtract from one and take the square root, then divide the proper time by that root. One second at 90 percent of light speed stretches to 2.294157 seconds, a Lorentz factor of 2.294157.

What Is Time Dilation?

Time dilation says that the interval between two events depends on who is measuring. A clock carried by a moving observer ticks more slowly than the same clock left behind, and both observers are correct in their own frames.

The effect is described by the Lorentz factor, which is one over the square root of one minus the velocity squared over the speed of light squared. At rest the factor is exactly one and there is no dilation at all.

The growth is not linear. Half the speed of light gives a factor of 1.154701, but ninety percent gives 2.294157, and ninety nine percent gives 7.0888. The curve bends sharply upward as the velocity approaches light speed.

Nothing with mass can reach the speed of light, because the factor grows without bound and the energy needed grows with it. The calculator clamps the velocity just below light speed to keep the result finite.

Proper time is the time measured by a clock that is present at both events. A passenger on a fast ship measures proper time; the observer left at the origin measures the longer dilated time.

Muons created in the upper atmosphere are the classic laboratory evidence. Their proper lifetime is about 2.2 microseconds, yet they reach the ground because their internal clocks run slow from our point of view.

The same factor governs length contraction. A fast ship is shortened along its direction of travel by exactly the same ratio, which keeps the speed of light constant for every observer.

Satellite navigation needs this correction. A GPS satellite orbits at about 1.2922 percent of light speed, which stretches each day by roughly 7.1712 microseconds before the general relativistic correction is added.

The effect is symmetric. Each observer sees the other's clock running slow, and the apparent paradox is resolved only when the two clocks are brought back together and one of them has accelerated.

Time dilation is measured directly and routinely. Atomic clocks flown on aircraft agree with the prediction to a fraction of a percent, and particle accelerators see unstable particles live far longer than their rest-frame lifetime.

General relativity adds a second effect. Deeper in a gravitational field a clock runs slower, so a clock on the ground and one in orbit disagree for two reasons that partly cancel in the case of the GPS satellites.

The muon evidence is worth spelling out. Created at about fifteen kilometres altitude with a lifetime of 2.2 microseconds, a muon at light speed covers only 660 metres before decaying. Detectors at sea level count far more of them than that non-relativistic fraction would allow.

The twin paradox is not a paradox. The travelling twin has to accelerate to leave, to turn around and to stop, so the two situations are not symmetric, and only the traveller comes back younger.

Formula

t = t0 / sqrt(1 - v^2/c^2)

Formula page →

The time seen by a stationary observer for a clock moving at v.

SymbolMeaning
tDilated time
t0Proper time
vVelocity
cSpeed of light

gamma = 1 / sqrt(1 - v^2/c^2)

Formula page →

The multiplier applied to time, length and relativistic mass.

SymbolMeaning
gammaLorentz factor
vVelocity
cSpeed of light

How To Calculate Time Dilation

  1. 1

    Divide the velocity by the speed of light

    This fraction is often written as beta. At ninety percent of light speed beta is 0.9, which is the only number the rest of the formula needs.

  2. 2

    Square beta and subtract it from one

    0.9 squared is 0.81, and one minus 0.81 is 0.19. This is the quantity under the square root.

  3. 3

    Take the square root

    The square root of 0.19 is about 0.43589, and its reciprocal is the Lorentz factor.

  4. 4

    Take the reciprocal

    One divided by 0.43589 is 2.294157, which is the Lorentz factor at ninety percent of light speed.

  5. 5

    Multiply the proper time by the factor

    One second of proper time becomes 2.294157 seconds for the stationary observer, which is the dilation.

Examples

Example 1: One year of proper time at ninety percent of light speed

Proper time
31557600
Velocity
90%
StepCalculationResult
Beta0.90.9
Beta squared0.9 x 0.90.81
One minus beta squared1 - 0.810.19
Square rootsqrt(0.19)0.43589
Lorentz factor1 / 0.435892.294157
Dilated time31557600 x 2.29415772398088.9432

Result: A spacecraft travelling at ninety percent of light speed experiences one year, or 72398088.9432 seconds of dilated time, for every 31,557,600 seconds that pass back home. The crew is about 40840488.9432 seconds, or one year and three months, younger than everyone who stayed behind.

Example 2: A muon travelling at ninety nine point eight percent of light speed

Proper time
0.0000022
Velocity
99.8%
StepCalculationResult
Beta0.9980.998
Beta squared0.998 x 0.9980.996004
One minus beta squared1 - 0.9960040.003996
Square rootsqrt(0.003996)0.063215
Lorentz factor1 / 0.06321515.8193
Dilated lifetime0.0000022 x 15.81930.0000348

Result: The muon's own clock says 0.0000022 seconds, but a laboratory observer measures a lifetime of 0.0000348 seconds, about sixteen times longer. That extension is why muons created high in the atmosphere reach the ground.

Example 3: A GPS satellite orbiting for one day

Proper time
86400
Velocity
1.2922%
StepCalculationResult
Beta0.0129220.012922
Beta squared0.012922 x 0.0129220.000167
One minus beta squared1 - 0.0001670.999833
Square rootsqrt(0.999833)0.999917
Lorentz factor1 / 0.9999171.000083
Dilated time86400 x 1.00008386407.1712

Result: One day aboard a GPS satellite stretches to 86407.1712 seconds as seen from the ground, a difference of 7.1712 microseconds per day. Ignoring it would put navigation positions out by kilometres within a single day.

Calculator

Dilated time in seconds

2.2942

Lorentz factor
2.2942
Velocity in metres per second
269,813,212
Extra seconds gained
1.2942

Values update as you type. This calculator covers the single scenario its formula assumes — see Common Mistakes for what it leaves out.

Prefer a full-width tool? Open the Time Dilation calculator page.

Common Mistakes

  • Using kilometres per second against the constant in metres

    The speed of light is 299,792,458 metres per second. Feeding 300000 or 3 x 10^5 without matching units changes the answer by orders of magnitude.

  • Forgetting to square the velocity fraction

    The formula needs v squared over c squared, not v over c. Using 0.9 instead of 0.81 puts a negative number under the square root.

  • Entering a velocity above the speed of light

    The formula has no real answer once v exceeds c, so the calculator clamps the fraction just below one. A value above one is a sign the inputs need checking.

  • Swapping proper time and dilated time

    Proper time is the shorter interval measured by the moving clock. Multiplying by the factor in the wrong direction halves the effect instead of doubling it.

  • Applying the factor to only one clock

    Time dilation affects every process on the moving object equally, including electronics, chemistry and biology, not just the clock you are watching.

  • Ignoring gravity in orbit

    Special relativity covers motion only. Clocks in orbit also run faster because gravity is weaker up there, and the net GPS correction is the sum of both effects.

FAQ

What is time dilation in one sentence?

A moving clock runs slower than a stationary one, by a factor of one over the square root of one minus the velocity squared over the speed of light squared.

How small is the effect at everyday speeds?

Vanishingly small. At a hundred kilometres per hour the Lorentz factor differs from one by less than one part in a hundred billion trillion.

Does time dilation mean time travel?

It means travel into the future only. A fast-moving traveller ages less than the people left behind, but cannot return to a point earlier than their own departure.

What is proper time?

The interval measured by a clock that is present at both events, which is always the shortest interval any observer can record.

Why is the Lorentz factor infinite at light speed?

Because the square root goes to zero, and dividing by zero is undefined. Only massless particles travel at light speed.

Do astronauts actually age less?

Yes, but by milliseconds over a six month stay because orbital speeds are a tiny fraction of the speed of light. The effect is real but far too small to notice.

References

  1. [1]Wikipedia, Time dilation — https://en.wikipedia.org/wiki/Time_dilation
  2. [2]Wikipedia, Lorentz factor — https://en.wikipedia.org/wiki/Lorentz_factor
  3. [3]Wikipedia, Proper time — https://en.wikipedia.org/wiki/Proper_time