Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q1154120> ?p ?o }
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- Q1154120 subject Q17420444.
- Q1154120 subject Q5894358.
- Q1154120 subject Q6454106.
- Q1154120 subject Q7009295.
- Q1154120 subject Q7465898.
- Q1154120 subject Q7465903.
- Q1154120 subject Q8393112.
- Q1154120 subject Q8461112.
- Q1154120 subject Q8641743.
- Q1154120 subject Q8691170.
- Q1154120 abstract "Kruger 60 (DO Cephei) is a binary star system located 13.15 light-years from the Sun. These red dwarf stars orbit each other every 44.6 years.The larger, primary star is designated component A, while the secondary, smaller star is labeled component B. Component A has about 27% of the Sun's mass and 35% of the Sun's radius. Component B has about 18% of the Sun's mass and 24% of the Sun's radius. Component B is a flare star and has been given the variable star designation "DO Cephei". It is an irregular flare that typically doubles in brightness and then returns to normal over an 8-minute period.On average, the two stars are separated by 9.5 AUs, which is roughly the average distance of Saturn from the Sun. However, their eccentric mutual orbit causes their distance to vary between 5.5 AUs at periastron, to 13.5 at apastron.This system is orbiting through the Milky Way at a distance from the core that varies from 7–9 kpc with an orbital eccentricity of 0.126–0.130. The closest approach to the Sun will occur in about 88,600 years when this system will come within 1.95 parsecs.".
- Q1154120 wikiPageExternalLink Astro-Star-Dwarf-Krueger-60.htm.
- Q1154120 wikiPageWikiLink Q1045111.
- Q1154120 wikiPageWikiLink Q10468.
- Q1154120 wikiPageWikiLink Q111130.
- Q1154120 wikiPageWikiLink Q1351528.
- Q1154120 wikiPageWikiLink Q17420444.
- Q1154120 wikiPageWikiLink Q180892.
- Q1154120 wikiPageWikiLink Q1811.
- Q1154120 wikiPageWikiLink Q193.
- Q1154120 wikiPageWikiLink Q285400.
- Q1154120 wikiPageWikiLink Q350.
- Q1154120 wikiPageWikiLink Q48440.
- Q1154120 wikiPageWikiLink Q50053.
- Q1154120 wikiPageWikiLink Q525.
- Q1154120 wikiPageWikiLink Q531.
- Q1154120 wikiPageWikiLink Q555846.
- Q1154120 wikiPageWikiLink Q5893.
- Q1154120 wikiPageWikiLink Q5894358.
- Q1154120 wikiPageWikiLink Q6243.
- Q1154120 wikiPageWikiLink Q6454106.
- Q1154120 wikiPageWikiLink Q7009295.
- Q1154120 wikiPageWikiLink Q7465898.
- Q1154120 wikiPageWikiLink Q7465903.
- Q1154120 wikiPageWikiLink Q83481.
- Q1154120 wikiPageWikiLink Q8393112.
- Q1154120 wikiPageWikiLink Q845735.
- Q1154120 wikiPageWikiLink Q8461112.
- Q1154120 wikiPageWikiLink Q850950.
- Q1154120 wikiPageWikiLink Q8641743.
- Q1154120 wikiPageWikiLink Q8691170.
- Q1154120 type Place.
- Q1154120 type CelestialBody.
- Q1154120 type Location.
- Q1154120 type Place.
- Q1154120 type Star.
- Q1154120 type Thing.
- Q1154120 comment "Kruger 60 (DO Cephei) is a binary star system located 13.15 light-years from the Sun. These red dwarf stars orbit each other every 44.6 years.The larger, primary star is designated component A, while the secondary, smaller star is labeled component B. Component A has about 27% of the Sun's mass and 35% of the Sun's radius. Component B has about 18% of the Sun's mass and 24% of the Sun's radius. Component B is a flare star and has been given the variable star designation "DO Cephei".".
- Q1154120 label "Kruger 60".
- Q1154120 name "Kruger 60 A/B".