Astrophysics (index)

Hubble Constant

(rate of expansion of the universe)

The Hubble Constant (H0) characterizes the rate of expansion of the universe. Hubble's Law is a theory that the universe is expanding such that the velocity at which an object is moving away from another is proportional to the distance between them, i.e.,

v = cd

where v is velocity, d is distance, and constant c (H0) is the Hubble Constant. Estimates are in the range of 50-90 (km/s)/Mpc with current estimates very close to 70. This expansion is called the Hubble Expansion.

Observation has revealed evidence that the universe's expansion is not constant. One might say "the Hubble constant changes with time", but for much work, this issue can (or must) be set aside, and even when it is relevant, the term Hubble constant is often used specifically to mean the current rate of expansion.

The Hubble Parameter (h) is a dimensionless variant on the constant, where

H0 = h × 100 km s-1Mpc-1

h calculates to 0.7.

The term Hubble Flow is used for the apparent motion of astronomical objects due to this expansion.

The terms are named for Edwin Hubble, who in the early 20th century established that galaxies are more-distant Milky Way-like objects, and later that the distant ones can be seen to be receding from us, suggesting an expanding universe.


Referenced by:
Alcock-Paczyński Effect
Big Bang
Comoving Units
Cosmic Time
Dark Flow
Luminosity Function (LF)
Peculiar Velocity
Redshift (z)
Scale Factor
Sunyaev-Zel'dovich Effect (SZ Effect)