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- Intrinsic_brightness abstract "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.".
- Intrinsic_brightness wikiPageID "14837254".
- Intrinsic_brightness wikiPageRevisionID "601785133".
- Intrinsic_brightness hasPhotoCollection Intrinsic_brightness.
- Intrinsic_brightness subject Category:Observational_astronomy.
- Intrinsic_brightness comment "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.".
- Intrinsic_brightness label "Absolute Helligkeit".
- Intrinsic_brightness label "Intrinsic brightness".
- Intrinsic_brightness sameAs Absolute_Helligkeit.
- Intrinsic_brightness sameAs m.03gzpcj.
- Intrinsic_brightness sameAs Q15230792.
- Intrinsic_brightness sameAs Q15230792.
- Intrinsic_brightness wasDerivedFrom Intrinsic_brightness?oldid=601785133.
- Intrinsic_brightness isPrimaryTopicOf Intrinsic_brightness.