Pogson Scale

Pogson scale

[′päg·sən ‚skāl]
(astronomy)
An index of brightness used in star catologs; it is the ratio of 2.512 to 1 between the brightness of successive magnitudes.
McGraw-Hill Dictionary of Scientific & Technical Terms, 6E, Copyright © 2003 by The McGraw-Hill Companies, Inc.
The following article is from The Great Soviet Encyclopedia (1979). It might be outdated or ideologically biased.

Pogson Scale

 

a relation between the magnitudes m \ and m 2 of two stars and their brightnesses E1 and E2:

m2 — m1 = —2.5 log E2/E1

The value of —2.5 for the coefficient was proposed by the English astronomer N. R. Pogson in 1859. It was chosen so that a variation in brightness by a factor of 100 would correspond to a difference of five magnitudes (which is the mean difference between the brightest and faintest stars visible to the naked eye); thus faint stars have greater magnitudes.

The Pogson scale for visual observations is one example of the Weber-Fechner psychophysical law. In this case, the strength of the stimulus on the pupil of the observer’s eye is determined by the brightness of a particular star, while the intensity of the sensation is a function of the star’s magnitude.

The Great Soviet Encyclopedia, 3rd Edition (1970-1979). © 2010 The Gale Group, Inc. All rights reserved.
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