Gravitational Time Dilation
Also known as: GR Time Dilation · Gravitational Redshift of Time
Gravity slows time. The deeper you are in a gravitational potential, the slower your clock runs compared to a distant observer.
Two clock dials: distant observer (orange) ticks at 1 Hz; local observer at radius r (blue) ticks slower by sqrt(1 - r_s/r). Slider controls r/r_s.
Equivalent forms
A single square root, parameterized by the Schwarzschild radius, encodes how gravity warps the flow of time near any spherical mass.
Unit systems
Where it holds
Dimensional analysis
Predicted in Einstein's 1915 general relativity. The Schwarzschild solution (1916) gave the exact form for spherical masses; Pound-Rebka (1959) verified it experimentally.
Why do GPS satellite clocks tick faster than ground clocks?
Clocks higher in a gravitational potential tick faster. For GPS at 20200 km altitude, the gravitational effect is +45 microseconds/day; velocity effect is −7 microseconds/day. Net +38 microseconds/day correction.
- GPS positioning (38 microseconds/day correction)
- Pulsar timing arrays for gravitational waves
- Black hole imaging (Event Horizon Telescope)
- Optical lattice clock geodesy (sensitive to 1 cm altitude changes)
- Gravitational time dilation is NOT a Doppler effect — it persists for static observers
- It depends on potential difference, not on local g
- Clocks don't 'know' they are dilated — locally each clock runs at 1 second per second
Limiting cases
What if…
A distant observer sees your clock slow to a halt at r_s; you yourself see nothing unusual locally as you cross.
Surface time dilation roughly doubles ; GPS correction would grow proportionally.
Inside the horizon, the t and r coordinates swap roles — 'time' becomes radial; no static observer exists.
GPS satellite vs Earth surface
- M:
- 5.972e+24
- r:
- 26571000
- G:
- 6.674e-11
- Surface:
- Orbit:
- (dtau/ microseconds/day
Clock near a stellar-mass black hole
- M:
- 2e+30
- r:
- 10000
- G:
- 6.674e-11
- dtau/