1. (astronomy) the generalization that the speed of recession of distant galaxies (the red shift) is proportional to their distance from the observer; [syn: Hubble's law, Hubble law]
WordNet (r) 3.0 (2006):
Hubble law
n 1: (astronomy) the generalization that the speed of recession
of distant galaxies (the red shift) is proportional to
their distance from the observer [syn: Hubble's law,
Hubble law]