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About: Omega Fornacis     Goto   Sponge   NotDistinct   Permalink

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

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatB-typeMain-sequenceStarsyago:WikicatBayerObjectsyago:WikicatBinaryStarsyago:WikicatStarsyago:BinaryStar109221070yago:CelestialBody109239740yago:NaturalObject100019128yago:Object100002684yago:PhysicalEntity100001930staryago:Star109444100yago:Whole100003553yago:WikicatA-typeMain-sequenceStars New Facet based on Instances of this Class

Omega Fornacis, which is Latinized from ω Fornacis, is a wide binary star system in the southern constellation of Fornax. It has a blue-white hue and is faintly visible to the naked eye as a fifth-magnitude star. The system lies at a distance of approximately 470 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +10 km/s. The dual nature of this system was discovered in 1836 by John Herschel. As of 2013, the two components had an angular separation of 11.0″ along a position angle of 246°. This corresponds to a projected separation of 1,520 AU.