Gravitational redshift

/ˌɡrævɪˈteɪʃənəl ˈrɛdˌʃɪft/ noun

Definition

The increase in wavelength (shift toward red) of electromagnetic radiation as it climbs out of a gravitational field, caused by gravitational time dilation. Light loses energy as it escapes from massive objects, making it appear redder to distant observers.

Etymology

Combines 'gravitational' (Latin 'gravitas') with 'redshift' (coined in early 20th century astronomy from the shift toward the red end of the spectrum). Einstein predicted this effect in 1907, and it was first observed in laboratory tests in 1959 by Pound and Rebka.

Kelly Says

Gravitational redshift means that identical atomic clocks run slower in stronger gravitational fields—GPS satellites must correct for this effect because their clocks run 45 microseconds per day faster than Earth-based clocks! Without accounting for gravitational redshift, GPS would be off by about 10 kilometers per day.

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