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  • Rule: asEquivalentb3sb3sifpdbprdf-labelfacetshttp://dbpedia.org/resource/inference/rules/dbpedia#http://dbpedia.org/resource/inference/rules/opencyc#http://dbpedia.org/resource/inference/rules/umbel#http://dbpedia.org/resource/inference/rules/yago#http://dbpedia.org/schema/property_rules#http://www.ontologyportal.org/inference/rules/SUMO#http://www.ontologyportal.org/inference/rules/WordNet#http://www.w3.org/2002/07/owl#ldpoplwebskos-transvirtrdf-labelvirtrdf-urlNone
    
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About: 30 Vulpeculae     Goto   Sponge   NotDistinct   Permalink

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

Type: Thingplacedbo:Locationyago:LivingThing100004258yago:NaturalObject100019128yago:Object100002684yago:Organism100004475yago:Animal100015388yago:BinaryStar109221070yago:CelestialBody109239740yago:Giant101323781staryago:WikicatFlamsteedObjectsyago:WikicatStarsyago:WikicatK-typeGiantsyago:Star109444100yago:Whole100003553yago:PhysicalEntity100001930schema:Placecelestial bodyyago:WikicatBinaryStars New Facet based on Instances of this Class

30 Vulpeculae is a binary star system in the northern constellation of Vulpecula, located mid-way between Epsilon Cygni and a diamond-shaped asterism in Delphinus. It is visible to the naked eye as a faint, orange-hued point of light with an apparent visual magnitude of 4.91. The system is located approximately 350 light years away from the Sun based on parallax, and is drifting further away with a mean radial velocity of +30 km/s. The system has a relatively high proper motion, traversing the celestial sphere at the rate of 0.186 arc seconds per annum.