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About: W Mensae     Goto   Sponge   NotDistinct   Permalink

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

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatObjectsNamedWithVariableStarDesignationsyago:CelestialBody109239740yago:NaturalObject100019128yago:Object100002684yago:PhysicalEntity100001930staryago:Star109444100yago:Supergiant109450708yago:Thing100002452yago:Variable109468959yago:Whole100003553yago:WikicatExtragalacticStarsyago:WikicatF-typeSupergiantsyago:WikicatRCoronaeBorealisVariables New Facet based on Instances of this Class

W Mensae (W Men) is an unusual yellow supergiant star in the Large Magellanic Cloud in the southern constellation Mensa. It is an R Coronae Borealis variable and periodically decreases in brightness by several magnitudes. W Men is very distant, being located in the neighboring galaxy Large Magellanic Cloud, where it lies on the southern metal-deficient edge. Despite its high luminosity, the star has a maximum apparent brightness of +13.8m, too dim to be visible in a small telescope. Its radius has been calculated to be 61 times that of the Sun.