Hubble's law

American  

noun

Astronomy.

1. the law that the velocity of recession of distant galaxies from our own is proportional to their distance from us.

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Hubble's law British  

noun

1. astronomy a law stating that the velocity of recession of a galaxy is proportional to its distance from the observer

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Hubble's law Scientific  

/ hŭb′əlz /

1. A law of cosmology stating that the rate at which astronomical objects in the universe move apart from each other is proportional to their distance from each other. Current estimates of the value of this proportion, known as Hubble's constant, put its value at approximately 71 kilometers per second per megaparsec.

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Etymology

Origin of Hubble's law

First recorded in 1930–35; named after E. P. Hubble, discoverer of the relationship

Example Sentences

See Examples For:

Hubble's law

Pythagoras wasn’t the first person to derive the Pythagorean theorem, Edwin Hubble wasn’t the first to formulate Hubble’s law, and so on.

From Scientific American ● Apr. 2, 2020

First, we must reliably establish Hubble’s constant by measuring both the distance and the velocity of many galaxies in many directions to be sure Hubble’s law is truly a universal property of galaxies.

From Textbooks ● Oct. 13, 2016

In other words, the kind of relationship expressed by Hubble’s law can be explained by a uniform stretching of the “world” of the ants.

From Textbooks ● Oct. 13, 2016

The relationship between the velocity of recession of galaxies and their distance from Earth that we call Hubble's law was first formulated by Belgian cosmologist Georges Lemaître.

From Nature ● Mar. 22, 2012

By Hubble's law it appeared to be some 4 billion light-years away.

From Time Magazine Archive