Norman Robert Pogson
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- magnitude
In 1850 the English astronomer Norman Robert Pogson proposed the system presently in use. One magnitude is defined as a ratio of brightness of 2.512 times; e.g., a star of magnitude 5.0 is 2.512 times as bright as one of magnitude 6.0. Thus, a difference of five magnitudes corresponds to…
Read MoreIn 1850 the English astronomer Norman Robert Pogson proposed the system presently in use. One magnitude is defined as a ratio of brightness of 2.512 times; e.g., a star of magnitude 5.0 is 2.512 times as bright as one of magnitude 6.0. Thus, a difference of five magnitudes corresponds to…
Read More - photometry
In 1856 Norman Robert Pogson suggested that this ratio should be used to define the scale of magnitude, so that a brightness difference of one magnitude was a ratio of 2.512 in intensity and a five-magnitude difference was a ratio of (2.51188)5, or precisely 100. Steps in…
Read MoreIn 1856 Norman Robert Pogson suggested that this ratio should be used to define the scale of magnitude, so that a brightness difference of one magnitude was a ratio of 2.512 in intensity and a five-magnitude difference was a ratio of (2.51188)5, or precisely 100. Steps in…
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