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- S_Persei abstract "S Persei is a red supergiant or hypergiant located in the Double Cluster in Perseus, north of the cluster NGC 869. It is a representative of the semiregular variables, whose periods of variation are subject to more irregularities than those of Mira variable red supergiants. Many of the visually bright (5th - 7th magnitude) variable stars belong to this class of semiregulars, as these stars are extremely large and luminous, and hence visible across long distances. S Persei is as much as 1000 times the sun's diameter.".
- S_Persei wikiPageID "19023665".
- S_Persei wikiPageRevisionID "585722522".
- S_Persei absmagV "-6.36".
- S_Persei appmagV "9.23".
- S_Persei bV "2.65".
- S_Persei class "M3Iaev-M4.5I".
- S_Persei constell Perseus_(constellation).
- S_Persei dec "+58° 31' 11.45"".
- S_Persei distLy "8200".
- S_Persei distPc "2510".
- S_Persei epoch "J2000".
- S_Persei hasPhotoCollection S_Persei.
- S_Persei luminosity "88000".
- S_Persei parallax "1.66".
- S_Persei propMoDec "-0.29".
- S_Persei propMoRa "-2.7".
- S_Persei ra "8571.709".
- S_Persei radialV "-39.71".
- S_Persei radius "780".
- S_Persei temperature "~3,500".
- S_Persei variable Semiregular_variable_star.
- S_Persei subject Category:Henry_Draper_Catalogue_objects.
- S_Persei subject Category:M-type_supergiants.
- S_Persei subject Category:Objects_named_with_variable_star_designations.
- S_Persei subject Category:Objects_within_10_kly_of_Earth.
- S_Persei subject Category:Perseus_(constellation).
- S_Persei type CelestialBody109239740.
- S_Persei type NaturalObject100019128.
- S_Persei type Object100002684.
- S_Persei type ObjectsNamedWithVariableStarDesignations.
- S_Persei type PhysicalEntity100001930.
- S_Persei type Star109444100.
- S_Persei type SupergiantStars.
- S_Persei type Whole100003553.
- S_Persei type CelestialBody.
- S_Persei type Star.
- S_Persei type PhysicalBody.
- S_Persei comment "S Persei is a red supergiant or hypergiant located in the Double Cluster in Perseus, north of the cluster NGC 869. It is a representative of the semiregular variables, whose periods of variation are subject to more irregularities than those of Mira variable red supergiants. Many of the visually bright (5th - 7th magnitude) variable stars belong to this class of semiregulars, as these stars are extremely large and luminous, and hence visible across long distances.".
- S_Persei label "S Persei".
- S_Persei label "S Persei".
- S_Persei label "S Persei".
- S_Persei label "S Персея".
- S_Persei label "英仙座S".
- S_Persei sameAs S_Persei.
- S_Persei sameAs S_Persei.
- S_Persei sameAs m.04j9m9p.
- S_Persei sameAs Q2083066.
- S_Persei sameAs Q2083066.
- S_Persei sameAs S_Persei.
- S_Persei wasDerivedFrom S_Persei?oldid=585722522.
- S_Persei isPrimaryTopicOf S_Persei.
- S_Persei name "S Persei".