Hubble's law, also known as the Hubble–Lemaître law, is the observation in physical cosmology that galaxies are moving away from Earth at speeds proportional...

Hubble confirmed in 1929 that the recessional velocity of a galaxy increases with its distance from Earth, a behavior that became known as Hubble's law...

the notion of an expanding universe is known as Hubble's law, published in work by physicist Edwin Hubble in 1929, which discerned that galaxies are moving...

proof that the universe was expanding and was not a static object. After Hubble's discovery was published, Einstein abandoned the cosmological constant....

galaxies. The ratio between these quantities gives the Hubble rate, in accordance with Hubble's law. Typically, the distance is measured using a standard...

original discoverer. Examples include Hubble's law, which was derived by Georges Lemaître two years before Edwin Hubble; the Pythagorean theorem, which was...

slope of about 500 km/s/Mpc. This correlation would come to be known as Hubble's law and would serve as the observational foundation for the expanding universe...

with the formulation of his eponymous Hubble's law. Milton Humason worked on those observations with Hubble. These observations corroborated Alexander...

itself was originally formalised by Father Georges Lemaître in 1927. Hubble's law of the expansion of the universe provided foundational support for the...

emitted by the object, known as the object's cosmological redshift. Hubble's law is the relationship between a galaxy's distance and its recessional velocity...

expanding away faster than the speed of light, at rates estimated by Hubble's law. The expansion rate appears to be accelerating, which dark energy was...

observed redshifts of the galaxies in the cluster. The deviation from the Hubble's law relationship between distance and redshift is altered, and this leads...

as "Hubble's law", but in 2018 the International Astronomical Union (IAU) adopted a resolution recommending that it be referred to as the "Hubble-Lemaître...

galaxy types Hubble's law, a statement in physical cosmology Hubble (crater), a lunar crater 2069 Hubble, a main-belt asteroid C/1937 P1 (Hubble), a long-period...

and always have been, receding from us at superluminal speeds. Hubble's law Hubble horizon Particle horizon Edward Robert Harrison (2003). Masks of...

never reach us in a finite amount of time. The Hubble velocity of an object is given by Hubble's law, v = x H . {\displaystyle v=xH.} Replacing v {\displaystyle...

their distance from Earth. This fact is now known as Hubble's law, though the numerical factor Hubble found relating recessional velocity and distance was...

literally. Benford's law Hilt's law Stigler's law of eponymy Goodhart's law Hubble's law Titius–Bode law Dermott's law Amdahl's law (maximum possible speed-up...

The actual measured velocity is the sum of the velocity predicted by Hubble's law plus a possible small velocity flowing in a common direction. Very large...

universe, this gives a nearly linear distance–redshift relation due to Hubble's law. At larger distances, since the expansion rate of the universe has changed...

universe. Hubble later used Leavitt's Law, together with galactic redshifts, to establish that the universe is expanding (see Hubble's law). Henrietta...

provide measurements of the Hubble parameter and angular diameter distance, respectively. The angular diameter distance and Hubble parameter can include different...

redshifts of the galaxies due to the expansion of the universe according to Hubble's law. A summarized timeline of important events in the field of cosmic voids...

of the universe, in contrast to other methods that typically involve Hubble's law and the age of the oldest stars in globular clusters. It is possible...

The Doppler effect and Hubble's law can be combined to form the equation z = v Hubble c {\displaystyle z={\frac {v_{\text{Hubble}}}{c}}} , where c is the...

is receding from us. The relationship is roughly linear, according to Hubble's law. It is relatively easy to measure redshift, but finding the distance...

to universes described by the FLRW metric, a de Sitter universe has a Hubble Law that is not only consistent through all space, but also through all time...

constant characterizing the "resistance of the space". To correspond to Hubble's law, the constant R 0 {\displaystyle R_{0}} must be several gigaparsecs....

{1-\Omega _{\mathrm {m} }}}}}} where w is defined above, H0 is Hubble's constant and Ωm is the present value of the density of all the matter in...

physical laws and physical constants. In regard to configurations such as the distribution of matter, almost all will differ from our Hubble volume. However...