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PHYSICS / GENERAL RELATIVITY

Gravitational Time Dilation Calculator

Estimate the stationary-clock rate and proper elapsed time outside a spherical non-rotating mass.

  • 01 Calculated in this tab
  • 02 Values stay in this browser tab
  • 03 Use boundary

Conversion input

Known value

Filter by unit name, symbol, or code. Your current selections remain available.

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METHOD / WORKED EXAMPLE

Understand Gravitational Time Dilation

Estimate the stationary-clock rate and proper elapsed time outside a spherical non-rotating mass. Inputs remain visible so the physical model and units can be checked instead of treated as a black box.

WORKED DEFAULT

Check the calculation with the default inputs

At Earth’s mean radius, an 86,400 s distant interval differs by only a tiny fraction under this ideal spherical model.

  1. Read the measured inputsM, r, t_∞
  2. Apply the physical modeldτ/dt = sqrt(1 - 2GM/(rc^2)).
  3. Check domain and unitsThe clock is stationary outside an isolated spherical, non-rotating, uncharged mass.

READ THE RESULT

Interpret the output in context

A factor below one means the local stationary clock accumulates less proper time than the far-away coordinate interval.

ASSUMPTIONS AND LIMITS

Know where the model stops

  • Radius is measured from the modeled center.
  • The observer at infinity defines the coordinate-time reference.

The clock is stationary outside an isolated spherical, non-rotating, uncharged mass.

Use internally consistent units and retain extra precision when carrying the result into another calculation.

COMMON QUESTIONS

Gravitational Time Dilation Calculator FAQs

Which model does Gravitational Time Dilation Calculator use?

Evaluate the Schwarzschild stationary-clock factor at the supplied areal radius and multiply it by distant elapsed time. This is gravitational, not velocity-based special-relativistic dilation. The calculator evaluates only the stated idealized equation and supplied values. It does not infer missing conditions, choose an experimental convention, or certify a measurement. Keep every quantity in the displayed unit and verify the model against the physical setup before relying on the result.

How should I interpret the Gravitational Time Dilation Calculator result?

A factor below one means the local stationary clock accumulates less proper time than the far-away coordinate interval. Near weak fields the factor is extremely close to one. Numerical precision does not imply experimental accuracy. Compare the output with scale, sign, limiting cases, and an independent source, then account for uncertainty in measured inputs and constants before using it in laboratory, engineering, or safety-sensitive work.

What is outside the scope of Gravitational Time Dilation Calculator?

The clock is stationary outside an isolated spherical, non-rotating, uncharged mass. It excludes rotation, altitude paths, moving clocks, multipoles, and combined relativistic effects. The result is educational and is not a simulation, calibration, engineering approval, or safety determination. More complete models may require geometry, material response, boundary conditions, relativistic frames, dispersion, losses, uncertainty propagation, or numerical field solutions not represented by these inputs.

Use boundary

Calculation path

Evaluate the Schwarzschild stationary-clock factor at the supplied areal radius and multiply it by distant elapsed time. The page evaluates the displayed equation from your supplied values and presents both symbolic and substituted KaTeX working so the arithmetic can be checked.

Calculation path

dτ/dt = sqrt(1 - 2GM/(rc^2)).