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  • Rule: ActivityStreamsMapasEquivalentb3sb3sifpdbprdf-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-transurn:det:rdf:labelvirtrdf-labelvirtrdf-urlNone
    
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About: HD 60532     Goto   Sponge   NotDistinct   Permalink

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

Type: Thingplacedbo:Locationschema:Placecelestial bodyyago:WikicatStarsyago:WikicatSubgiantStarsyago:CelestialBody109239740yago:NaturalObject100019128yago:Object100002684yago:PhysicalEntity100001930yago:WikicatHRObjectsyago:WikicatHenryDraperCatalogueObjectsyago:WikicatHipparcosObjectsstaryago:Star109444100yago:Whole100003553yago:WikicatDurchmusterungObjectsyago:WikicatF-typeMain-sequenceStarsyago:WikicatF-typeStars New Facet based on Instances of this Class

HD 60532 is a white (F-type) main sequence star located approximately 84 light-years away in the constellation of Puppis, taking its primary name from its Henry Draper Catalogue designation. It is calculated to be 1.44 times more massive than the Sun. The star is only 59% as old as the Sun (2.7 Gyr) and has metallicity of only 38% that of the Sun. In 2008, two extrasolar planets were discovered in orbit around it.