Redshift is the phenomenon where the light from a star or galaxy appears “shifted” toward the red end of the spectrum. This happens when the source is moving away from us, stretching the light waves and making their wavelength longer.
Think of a runner on a track. If the runner is moving away from you, each step you see takes a bit longer to reach you. In the same way, as a galaxy moves away, each crest of its light wave takes a little longer to arrive, so the wavelength increases.
The key relationship is:
\$z = \dfrac{\Delta \lambda}{\lambda_{\text{emit}}}\$
where:
If a galaxy is moving away at a speed \$v\$ that is much less than the speed of light \$c\$, the redshift can be approximated by:
\$z \approx \dfrac{v}{c}\$
| Galaxy | Recessional Velocity (km/s) | Redshift \$z\$ |
|---|---|---|
| Andromeda (M31) | -300 (approaching) | -0.001 |
| Messier 87 (M87) | 13,000 | 0.043 |
| NGC 1300 | 12,000 | 0.040 |
Redshift tells us how fast galaxies are moving away from us, which in turn helps us understand the expansion of the Universe. The farther a galaxy is, the larger its redshift, showing that the Universe is stretching over time.