Lamba - the cosmological constant
Albert Einstein
Current cosmological models are based on the field equations of Albert Einstein, which include the cosmological constant. The cosmological constant has important influence on the large scale dynamics of the cosmos.
Vesto Slipher
Alexander Friedmann
Georges Lemaitre
Edwin Hubble
In 1912, Vesto Slipher, discovered the redshift of light from distant galaxies. This was later to be interpreted as galaxies receding from Earth.
In 1922, Alexander Friedmann, using the field equations of Albert Einstein, provided theoretical evidence for the expanding universe.
In 1927, Georges Lemaitre, reached a conclusion similar to Friemann, however, on a theoretical basis. Lemaitre also proposed observational evidence for Hubble's law: The linear relationship between distance to galaxies and their recessional velocity.
Lastly, in 1929, Edwin Hubble, confirmed Lemaitre's findings.
If we assume the cosmological principle, that the spatial distribution of matter is homogeneous and isotropic, we find that galaxies are moving away from each other.