Intrinsic brightness
Astronomers use the term intrinsic brightness 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's apparent brightness might be 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. A star's intrinsic brightness is measured by its absolute magnitude.
This article is issued from Wikipedia - version of the 2/17/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.