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There are actually three types of wavelength shift:...
* Cosmological redshifts
* Doppler shifts...
* Gravitational redshifts
There are actually three types of wavelength shift:
* Cosmological redshifts, due to the expansion of the universe (the
"Hubble flow"). As an example, a cluster of galaxies at a distance of
50 megaparsecs (160 million light-years) has a recessional velocity
of about 3500 km/s, corresponding to a redshift z = (wavelength
shift)/(rest wavelength) = 0.012.
* Doppler shifts due to motion within the universe. As an example,
the galaxies that make up a cluster move within the cluster at speeds
of a few hundred km/s. These motions can be in any direction, so by
themselves they could produce either a blueshift or a redshift. As an
example, the galaxy M31 in Andromeda (part of the same cluster as the
Milky Way, and a mere 750 kiloparsecs away) is approaching us at 300
km/s. For our example cluster of galaxies at 50 megaparsecs, the
superposition of the motion of galaxies within the cluster on the
cosmological expansion gives a range of recessional velocities from
about 3200 to 3800 km/s. Doppler shifts of galaxies within clusters
are less important for more distant clusters, which have larger
cosmological redshifts.