Relativityundergraduate

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.

Δλλ=GMrc2\frac{\Delta\lambda}{\lambda} = \frac{GM}{rc^2}
Live simulation
warming up the physics…

Photons leave gravity well; wavelength stretches visibly.

Equivalent forms

νrecνem=1rs/r11rs/r2\frac{\nu_{rec}}{\nu_{em}} = \sqrt{\frac{1 - r_s/r_1}{1 - r_s/r_2}}
zΔΦc2z \approx \frac{\Delta\Phi}{c^2}
A direct consequence of equivalence: gravity slows time, so light from below arrives redshifted with no need for the full machinery of GR.