Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q1367410> ?p ?o }
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- Q1367410 subject Q10650.
- Q1367410 subject Q7217188.
- Q1367410 subject Q7724320.
- Q1367410 subject Q8293947.
- Q1367410 subject Q8759509.
- Q1367410 subject Q8790837.
- Q1367410 abstract "Iota Pegasi (24 Peg, HD 210027) is a star located within the constellation Pegasus. It is about 38 light-years from Earth. It is a spectroscopic binary system.Iota Pegasi A is a yellowish-white star somewhat brighter than the sun. It and the dimmer Iota Pegasi B orbit each other with a period of about 10 days. In about four billion years from now, component A will evolve off the main sequence into a giant. In the process it will overflow its Roche lobe and begin to transfer mass onto the secondary. This may cause the secondary to acquire enough mass to become the primary component. After both stars have passed through the giant star stage, the end result will be a pair of co-orbiting white dwarfs in about eight billion years.".
- Q1367410 wikiPageExternalLink 0000224.000.html.
- Q1367410 wikiPageExternalLink sim-id?protocol=html&Ident=HD+210027&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id.
- Q1367410 wikiPageExternalLink S032003.html.
- Q1367410 wikiPageWikiLink Q10650.
- Q1367410 wikiPageWikiLink Q162797.
- Q1367410 wikiPageWikiLink Q2.
- Q1367410 wikiPageWikiLink Q50053.
- Q1367410 wikiPageWikiLink Q5871.
- Q1367410 wikiPageWikiLink Q7217188.
- Q1367410 wikiPageWikiLink Q7724320.
- Q1367410 wikiPageWikiLink Q8293947.
- Q1367410 wikiPageWikiLink Q848485.
- Q1367410 wikiPageWikiLink Q8759509.
- Q1367410 wikiPageWikiLink Q8790837.
- Q1367410 wikiPageWikiLink Q8864.
- Q1367410 type Place.
- Q1367410 type CelestialBody.
- Q1367410 type Location.
- Q1367410 type Place.
- Q1367410 type Star.
- Q1367410 type Thing.
- Q1367410 comment "Iota Pegasi (24 Peg, HD 210027) is a star located within the constellation Pegasus. It is about 38 light-years from Earth. It is a spectroscopic binary system.Iota Pegasi A is a yellowish-white star somewhat brighter than the sun. It and the dimmer Iota Pegasi B orbit each other with a period of about 10 days. In about four billion years from now, component A will evolve off the main sequence into a giant.".
- Q1367410 label "Iota Pegasi".
- Q1367410 name "Iota Pegasi".