Gravitational Redshift
Also known as: Einstein Shift · GR Redshift
Photons climbing out of a gravity well lose energy — their wavelength stretches and clocks at the bottom appear to tick slower.
Photons leave gravity well; wavelength stretches visibly.
Equivalent forms
A direct consequence of equivalence: gravity slows time, so light from below arrives redshifted with no need for the full machinery of GR.
Unit systems
Where it holds
Dimensional analysis
Predicted in Einstein's 1907 equivalence-principle paper, eight years before GR was complete. Pound-Rebka confirmed it in 1959 at Harvard using Mössbauer spectroscopy over a 22.5 m tower.
How much does light reddened climbing out of the Sun's gravity?
Light leaving the Sun loses energy climbing out of its gravitational well: Δλ/λ ≈ GM/(Rc^2) ≈ 2.12e-6. Solar absorption lines shift by ~0.6 km/s — measured to confirm GR.
- GPS frequency standards
- Tests of equivalence principle
- Black hole and neutron star spectroscopy
- Cosmological redshift contribution (alongside expansion)
- Gravitational redshift is NOT a Doppler effect — emitter and observer can be stationary
- It's the same effect that makes lower clocks tick slower
- Photons don't 'fight gravity' — spacetime geometry stretches their wavelength
Limiting cases
What if…
It blueshifts symmetrically: . Photons gain energy climbing in.
— significant non-perturbative redshift.
Energy conservation would fail: a photon could climb a tower, convert to mass, fall, convert back, and gain energy — a perpetual motion machine.
Sun's surface
- M:
- 1.989e+30
- r:
- 696000000
- G:
- 6.674e-11
White dwarf Sirius B
- M:
- 2e+30
- r:
- 5840000
- G:
- 6.674e-11