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Surface brightness
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==Relationship to physical units== The surface brightness in magnitude units is related to the surface brightness in physical units of [[solar luminosity]] per square [[parsec]] by{{Citation needed|date=April 2023}} <math display="block">S(\mathrm{mag/arcsec^2}) = M_{\odot} + 21.572-2.5\log_{10} S (L_{\odot}/\mathrm{pc}^2),</math> where <math>M_{\odot}</math> and <math> L_{\odot} </math> are the [[absolute magnitude]] and the luminosity of the Sun in chosen [[Photometric system|color-band]]<ref>Absolute magnitudes of the Sun in different color-bands can be obtained from {{harvtxt|Binney|Merrifield|1998}} or [http://www.ucolick.org/~cnaw/sun.html Absolute Magnitude of the Sun in Several Bands] {{webarchive|url=https://web.archive.org/web/20070718015507/http://www.ucolick.org/~cnaw/sun.html |date=2007-07-18 }}</ref> respectively. Surface brightness can also be expressed in [[candela per square metre]] using the formula [value in cd/m<sup>2</sup>] = {{val|10.8e4}} Γ 10<sup>(β0.4Γ[value in mag/arcsec<sup>2</sup>])</sup>.
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