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- 50_Persei abstract "50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.50. Located around 21.00 parsecs (68.5 ly) distant, it is a White main-sequence star of spectral type F7V, a star that is currently fusing its core hydrogen. The star is an RS Canum Venaticorum variable, meaning that it is a close binary star whose components have star-spots, which cause variations in brightness.".
- 50_Persei wikiPageID "41515817".
- 50_Persei wikiPageRevisionID "588740951".
- 50_Persei constell Perseus_(constellation).
- 50_Persei name "50".
- 50_Persei type "F7V".
- 50_Persei subject Category:F-type_main-sequence_stars.
- 50_Persei subject Category:Flamsteed_objects.
- 50_Persei subject Category:Objects_named_with_variable_star_designations.
- 50_Persei subject Category:Perseus_(constellation).
- 50_Persei subject Category:RS_Canum_Venaticorum_variables.
- 50_Persei type CelestialBody.
- 50_Persei type Star.
- 50_Persei type PhysicalBody.
- 50_Persei comment "50 Persei is a star in the constellation Perseus. Its apparent magnitude is 5.50. Located around 21.00 parsecs (68.5 ly) distant, it is a White main-sequence star of spectral type F7V, a star that is currently fusing its core hydrogen. The star is an RS Canum Venaticorum variable, meaning that it is a close binary star whose components have star-spots, which cause variations in brightness.".
- 50_Persei label "50 Persei".
- 50_Persei label "50 Persei".
- 50_Persei label "卷舌增五".
- 50_Persei sameAs 50_Persei.
- 50_Persei sameAs m.0zwrdqw.
- 50_Persei sameAs Q8179459.
- 50_Persei sameAs Q8179459.
- 50_Persei wasDerivedFrom 50_Persei?oldid=588740951.
- 50_Persei isPrimaryTopicOf 50_Persei.