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Create the page "Hubble?s law" on this wiki! See also the search results found.
- ....<ref>See [[Planck (spacecraft)#2015 data release|the Planck Collaboration's 2015 data release]].</ref> # the [[physical law|universality of physical laws]] – that the laws of physics don't cha41 KB (6,072 words) - 19:16, 4 February 2018
- | z = 547 ± 5 km/[[second|s]]<ref name="ned" /> ...l galaxy]])<ref name=harris10b/> and distance (10–16 million [[light-year]]s).<ref name="tonryetal2001"/><ref name="ned-dist"/><ref name=ferrarese07/><r29 KB (4,015 words) - 12:30, 5 February 2018
- ...81A&A....95..188N |doi=}}</ref> is the [[hypothesis]] that the [[redshift]]s of cosmologically distant objects (in particular [[galaxies]] and [[quasars ...[[cosmic distance ladder|cosmic distance]] from the Earth (see [[Hubble's Law]]). This is referred to as [[cosmological redshift]]. Ruling out errors in22 KB (3,040 words) - 20:16, 4 February 2018
- ...energy when electromagnetic radiation is red-shifted, as given by [[Planck's relation]], due to the electromagnetic radiation propagating in opposition where <math>G</math> denotes Newton's [[gravitational constant]], <math>M</math> the [[mass]] of the gravitating22 KB (3,270 words) - 20:15, 4 February 2018
- ...;5; and the imaging survey has been involved in the detection of [[quasar]]s beyond a redshift ''z'' = 6. ...esolution of 2048×2048 [[pixel]]s, totaling approximately 120 [[Megapixel]]s.<ref>{{cite web | title = Key Components of the Survey Telescope | publishe25 KB (3,589 words) - 12:34, 5 February 2018