Matches in DBpedia 2016-04 for { <http://wikidata.dbpedia.org/resource/Q14020> ?p ?o }
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- Q14020 subject Q10595.
- Q14020 subject Q5894358.
- Q14020 subject Q7207584.
- Q14020 subject Q7465898.
- Q14020 subject Q7465903.
- Q14020 subject Q7724325.
- Q14020 subject Q8293947.
- Q14020 subject Q8461104.
- Q14020 subject Q8759509.
- Q14020 subject Q8790837.
- Q14020 abstract "Eta Boötis (η Boo, η Boötis) is a star in the constellation Boötes. It has the traditional names Muphrid and Saak, and the Flamsteed designation 8 Boötis. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.The name Muphrid is from the Arabic مفرد الرامح mufrid ar-rāmiħ "the (single) one of the lancer". In Chinese, 右攝提 (Yòu Niè Dī), meaning "the Right Conductor", refers to an asterism consisting of Eta Boötis, Tau Boötis and Upsilon Boötis. Consequently, Eta Boötis itself is known as 右攝提一 (Yòu Niè Dī yī, English: "the First Star of the Right Conductor"). In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Ramih al Ramih (رمح الرامح—rumḥ al rāmiḥ), which was translated into Latin as Lancea Lanceator, possibly meaning the lance of the lancer.This star is a subgiant that has begun the process of evolving from a main sequence star into a red giant. It has about 1.7 times the mass of the Sun and 2.7 times the Sun's radius. The estimated age of this star is about 2.7 billion years. Based on its spectra, Eta Boötis has a significant excess of elements heavier than helium. In fact the ratio of iron to hydrogen is considered close to the upper limit for dwarf stars in the galactic disk. The star is a suspected spectroscopic binary with a reported period of 494 days, but the companion was not confirmed through speckle interferometry. This measurement does not rule out a low mass stellar companion of spectral class M7.Eta Boötis appears close to the prominent star Arcturus (Alpha Bootis) in Earth's sky, and Arcturus is in fact its closest stellar neighbor, as both stars are nearly identical in distance from the Sun. The two stars are about 3.24 light years apart, and each would appear bright in the other's sky. Arcturus would appear as roughly magnitude -5.2 (about 120 times brighter than it appears from Earth, or close to twice the brightness of Venus) in the night sky of a hypothetical planet orbiting Eta Boötis, while Eta Boötis would appear at about magnitude -2.5 in the sky of a hypothetical planet orbiting Arcturus, or over twice the brightness of Sirius in our night sky.".
- Q14020 thumbnail Boötes_IAU.svg?width=300.
- Q14020 wikiPageExternalLink AladinPreview?-c=13+54+41.0787%2B18+23+51.781&ident=NSV+19993&submit=Aladin+previewer.
- Q14020 wikiPageExternalLink VizieR-S?CCDM%20J13547%2b1824A.
- Q14020 wikiPageExternalLink VizieR-S?GJ%20534.
- Q14020 wikiPageExternalLink muphrid.html.
- Q14020 wikiPageExternalLink stars.htm.
- Q14020 wikiPageWikiLink Q10595.
- Q14020 wikiPageWikiLink Q111116.
- Q14020 wikiPageWikiLink Q111130.
- Q14020 wikiPageWikiLink Q1145927.
- Q14020 wikiPageWikiLink Q1150541.
- Q14020 wikiPageWikiLink Q12985.
- Q14020 wikiPageWikiLink Q1504755.
- Q14020 wikiPageWikiLink Q180892.
- Q14020 wikiPageWikiLink Q207247.
- Q14020 wikiPageWikiLink Q2402863.
- Q14020 wikiPageWikiLink Q244393.
- Q14020 wikiPageWikiLink Q3450.
- Q14020 wikiPageWikiLink Q397.
- Q14020 wikiPageWikiLink Q3972970.
- Q14020 wikiPageWikiLink Q4703437.
- Q14020 wikiPageWikiLink Q48440.
- Q14020 wikiPageWikiLink Q499138.
- Q14020 wikiPageWikiLink Q50053.
- Q14020 wikiPageWikiLink Q50081.
- Q14020 wikiPageWikiLink Q555846.
- Q14020 wikiPageWikiLink Q560.
- Q14020 wikiPageWikiLink Q5894358.
- Q14020 wikiPageWikiLink Q6227.
- Q14020 wikiPageWikiLink Q654182.
- Q14020 wikiPageWikiLink Q677.
- Q14020 wikiPageWikiLink Q7207584.
- Q14020 wikiPageWikiLink Q7465898.
- Q14020 wikiPageWikiLink Q7465903.
- Q14020 wikiPageWikiLink Q7724325.
- Q14020 wikiPageWikiLink Q781947.
- Q14020 wikiPageWikiLink Q7850.
- Q14020 wikiPageWikiLink Q8293947.
- Q14020 wikiPageWikiLink Q845735.
- Q14020 wikiPageWikiLink Q8461104.
- Q14020 wikiPageWikiLink Q850950.
- Q14020 wikiPageWikiLink Q8667.
- Q14020 wikiPageWikiLink Q8759509.
- Q14020 wikiPageWikiLink Q8790837.
- Q14020 wikiPageWikiLink Q8928.
- Q14020 wikiPageWikiLink Q9262.
- Q14020 wikiPageWikiLink Q984158.
- Q14020 type Place.
- Q14020 type CelestialBody.
- Q14020 type Location.
- Q14020 type Place.
- Q14020 type Star.
- Q14020 type Thing.
- Q14020 comment "Eta Boötis (η Boo, η Boötis) is a star in the constellation Boötes. It has the traditional names Muphrid and Saak, and the Flamsteed designation 8 Boötis. Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified.The name Muphrid is from the Arabic مفرد الرامح mufrid ar-rāmiħ "the (single) one of the lancer".".
- Q14020 label "Eta Boötis".
- Q14020 depiction Boötes_IAU.svg.
- Q14020 name "Eta Boötis".