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About: U Scorpii     Goto   Sponge   NotDistinct   Permalink

An Entity of Type : yago:WikicatRecurrentNovae, within Data Space : dbpedia.org associated with source document(s)

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatNovaeyago:WikicatObjectsNamedWithVariableStarDesignationsyago:CelestialBody109239740yago:NaturalObject100019128yago:Nova109374493yago:Object100002684yago:PhysicalEntity100001930staryago:Star109444100yago:Whole100003553yago:WikicatRecurrentNovae New Facet based on Instances of this Class

U Scorpii (U Sco) is a recurrent nova system; one of 10 known recurring novae in the Milky Way galaxy. Located near the northern edge of the constellation Scorpius it normally has a magnitude of 18, but reaches a magnitude of about 8 during outbursts. Outbursts have been observed in 1863, 1906, 1936, 1979, 1987, 1999, 2010, and 2022. Originally identified in 1863 by English astronomer N.R. Pogson, U Scorpii was the third recurrent nova to be identified, in the years preceding World War II by Helen L. Thomas.