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The Hubble–Reynolds law models the surface brightness of elliptical galaxies as

$I(R)=\frac{I_0}{(1+R/R_H{)}^2}$

Where $I(R)$ is the surface brightness at radius $R$, $I_0$ is the central brightness, and $R_H$ is the radius at which the surface brightness is diminished by a factor of 1/4. It is asymptotically similar to the de Vaucouleurs law which is a special case of the Sérsic law for elliptical galaxies.

The law is named for the astronomers Edwin Hubble and John Henry Reynolds.

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