Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q2310758> ?p ?o }
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- Q2310758 subject Q5894358.
- Q2310758 subject Q7009767.
- Q2310758 subject Q8284795.
- Q2310758 subject Q8293947.
- Q2310758 abstract "Beta Muscae (β Muscae, β Mus) is a binary star in the southern circumpolar constellation of Musca. With a combined apparent visual magnitude of 3.07, it is the second brightest star (or star system) in the constellation. Judging by the parallax results, it is located at a distance of roughly 330–350 light-years (100–110 parsecs) from the Earth.This is a binary star system with a period of about 194 years at an orbital eccentricity of 0.6. As of 2007, the two stars had an angular separation of 1.206 arcseconds at a position angle of 35°. The components are main sequence stars of similar size and appearance. The primary component, β Muscae A, has an apparent magnitude of 3.51, a stellar classification of B2 V, and about 7.35 times the Sun's mass. The secondary component, β Muscae B, has an apparent magnitude of 4.01, a stellar classification of B3 V, and is about 6.40 times the mass of the Sun.This is a confirmed member of the Scorpius-Centaurus Association, which is a group of stars with similar ages, locations, and trajectories through space, implying that they formed together in the same molecular cloud. Beta Muscae is considered a runaway star system as it has a high peculiar velocity of 43.9 km s−1 relative to the normal galactic rotation. Runaway stars can be produced through several means, such as through an encounter with another binary star system. Binary systems form a relatively small fraction of the total population of runaway stars.".
- Q2310758 thumbnail Musca_IAU.svg?width=300.
- Q2310758 wikiPageExternalLink betamus.html.
- Q2310758 wikiPageWikiLink Q10435.
- Q2310758 wikiPageWikiLink Q1067416.
- Q2310758 wikiPageWikiLink Q111130.
- Q2310758 wikiPageWikiLink Q124313.
- Q2310758 wikiPageWikiLink Q1253791.
- Q2310758 wikiPageWikiLink Q1329496.
- Q2310758 wikiPageWikiLink Q1357788.
- Q2310758 wikiPageWikiLink Q165074.
- Q2310758 wikiPageWikiLink Q1666400.
- Q2310758 wikiPageWikiLink Q179600.
- Q2310758 wikiPageWikiLink Q180892.
- Q2310758 wikiPageWikiLink Q2.
- Q2310758 wikiPageWikiLink Q208474.
- Q2310758 wikiPageWikiLink Q2105737.
- Q2310758 wikiPageWikiLink Q22066400.
- Q2310758 wikiPageWikiLink Q2703.
- Q2310758 wikiPageWikiLink Q272447.
- Q2310758 wikiPageWikiLink Q3450.
- Q2310758 wikiPageWikiLink Q37640.
- Q2310758 wikiPageWikiLink Q45059.
- Q2310758 wikiPageWikiLink Q499138.
- Q2310758 wikiPageWikiLink Q50053.
- Q2310758 wikiPageWikiLink Q555846.
- Q2310758 wikiPageWikiLink Q5894358.
- Q2310758 wikiPageWikiLink Q6440.
- Q2310758 wikiPageWikiLink Q7009767.
- Q2310758 wikiPageWikiLink Q8284795.
- Q2310758 wikiPageWikiLink Q8293947.
- Q2310758 wikiPageWikiLink Q984158.
- Q2310758 type Place.
- Q2310758 type CelestialBody.
- Q2310758 type Location.
- Q2310758 type Place.
- Q2310758 type Star.
- Q2310758 type Thing.
- Q2310758 comment "Beta Muscae (β Muscae, β Mus) is a binary star in the southern circumpolar constellation of Musca. With a combined apparent visual magnitude of 3.07, it is the second brightest star (or star system) in the constellation. Judging by the parallax results, it is located at a distance of roughly 330–350 light-years (100–110 parsecs) from the Earth.This is a binary star system with a period of about 194 years at an orbital eccentricity of 0.6.".
- Q2310758 label "Beta Muscae".
- Q2310758 depiction Musca_IAU.svg.
- Q2310758 name "Beta Muscae".