| 1. There are many galaxies outside of our own. |
| 2. These galaxies are all receding from us if we go to large-enough distances. |
| 3. The velocity of recession is proportional to the distance from us. |
Thus, this work early in this century altered forever our perception of the Universe. It established both that the Universe was a much larger place than previously thought, and that it was not static but was expanding.
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Because of this relation, we shall commonly refer to the redshift of a distant object rather than its distance or its recessional velocity. The recessional velocity is related to the redshift by the relativistic formula
It also is often useful to solve this equation for the velocity in terms of the redshift. The result is
These formulas are called "relativistic" because they were derived using the special theory of relativity so they are valid for all velocities, including very large ones approaching the speed of light. These expressions reduce to the much simpler nonrelativistic form
but only for low velocities (that is, ones that are small compared with the speed of
light; they may still be large by ordinary standards!). If velocities are
more than a few percent of the speed of light, the more complicated relativistic
formula must be used. Otherwise we would make a serious error for large redshifts.
Once the velocity is related to the redshift by the above formulas,
it can then be related approximately to a distance using the
Hubble Law, as we describe in the next section.
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