Intrinsic brightness

Intrinsic brightness

Astronomers use the term intrinsic brightness (also termed absolute magnitude) to refer to how bright a star would be without the effects of distance or absorption due to interstellar dust or gas. While a bright distant star might have "apparent brightness" less than a nearby dim star, due to the inverse square law for brightness, astronomers can discuss its intrinsic brightness meaning how bright the stars would be at a common distance.


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