alt label |
|
||||||
---|---|---|---|---|---|---|---|
dcterms modified | ![]() ![]() |
||||||
broader |
|
||||||
definition | The speed with which a galaxy cluster recedes from us is directly proportional to its distance. It can be stated as v = H_{0}d, where v is the recessional velocity, H_0 the Hubble-Lemaitre constant, and d the distance. | ||||||
narrower |
|
||||||
type |
|
||||||
contributor | AAS_Frey.Katie_Admin original |