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About: NR Canis Majoris     Goto   Sponge   NotDistinct   Permalink

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

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatBinaryStarsyago:WikicatVariableStarsyago:WikicatObjectsNamedWithVariableStarDesignationsyago:WikicatStarsyago:BinaryStar109221070yago:CelestialBody109239740yago:NaturalObject100019128yago:Object100002684yago:PhysicalEntity100001930yago:WikicatHRObjectsyago:WikicatHenryDraperCatalogueObjectsstaryago:Star109444100yago:Thing100002452yago:Variable109468959yago:VariableStar109469152yago:Whole100003553yago:WikicatA-typeMain-sequenceStarsyago:WikicatDeltaScutiVariablesyago:WikicatF-typeMain-sequenceStarsyago:WikicatF-typeStars New Facet based on Instances of this Class

NR Canis Majoris is a binary star system in the southern constellation of Canis Major, located to the east of Sirius and Gamma Canis Majoris near the constellation border with Puppis. It has a yellow-white hue and is dimly visible to the naked eye with a combined apparent visual magnitude that fluctuates around 5.60. It is located at a distance of approximately 297 light years from the Sun based on parallax. The system is drifting closer to the Sun with a radial velocity of −29 km/s, and in about three million years it is predicted to approach within 14.1+4.7−4.0 ly. At that time, the star will become the brightest in the night sky, potentially reaching magnitude −0.88.