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About: KQ Puppis     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatPulsatingVariables, within Data Space : dbpedia.demo.openlinksw.com associated with source document(s)

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatB-typeMain-sequenceStarsyago:WikicatB-typeStarsyago:WikicatM-typeStarsyago:WikicatObjectsNamedWithVariableStarDesignationsyago:WikicatSpectroscopicBinariesyago:BinaryStar109221070yago:CelestialBody109239740yago:NaturalObject100019128yago:Object100002684yago:PhysicalEntity100001930staryago:Star109444100yago:Supergiant109450708yago:Thing100002452yago:Variable109468959yago:Whole100003553yago:WikicatA-typeSupergiantsyago:WikicatPulsatingVariables New Facet based on Instances of this Class

KQ Puppis (KQ Pup) is a spectroscopic binary variable star in the constellation Puppis. A red supergiant star and a hot main sequence star orbit each other every 9,742 days. Its apparent magnitude varies between 4.82 and 5.17. KQ Puppis has been catalogued as an outlying member of the open cluster Messier 47 (NGC 2422) and would be the brightest member of that cluster. Membership is uncertain as it appears to be more distant than the other stars in the cluster.