About: Pi Boötis

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Pi Boötis, Latinized from π Boötis, is a probable triple star system in the northern constellation of Boötes. It is visible to the naked eye with a combined apparent visual magnitude of 4.50. Based upon an annual parallax shift of 10.67 mas as seen from Earth, it is located roughly 310 light years from the Sun. Pi Boötis has the Chinese traditional star name 左攝提二 (Zuǒ shè tí èr)

Attributes	Values
rdf:type	Thing place dbo:Location schema:Place celestial body yago:WikicatB-typeMain-sequenceStars yago:WikicatBayerObjects yago:WikicatStars yago:BinaryStar109221070 yago:CelestialBody109239740 yago:NaturalObject100019128 yago:Object100002684 yago:PhysicalEntity100001930 yago:WikicatHenryDraperCatalogueObjects yago:WikicatHipparcosObjects star yago:Star109444100 yago:Whole100003553 yago:WikicatA-typeMain-sequenceStars yago:WikicatDoubleStars yago:WikicatDurchmusterungObjects yago:WikicatFlamsteedObjects
rdfs:label	Pi Bootis (es) Pi Bootis (fr) Pi Boötis (en) Pi1 Boötis (pt) Пи Волопаса (ru) Pi Bootis (sv) 左攝提二 (zh) HD129174 (uk)
rdfs:comment	Pi1 Boötis (29 Boötis) é uma estrela binária na direção da constelação de Boötes. Possui uma ascensão reta de 14h 40m 43.56s e uma declinação de +16° 25′ 05.9″. Sua magnitude aparente é igual a 4.49. Considerando sua distância de 317 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.45. Pertence à classe espectral B9p MnHg. (pt) Pi Bootis (π Bootis, förkortad Pi Boo, π Boo), som är stjärnans Bayer-beteckning, är sannolikt en trippelstjärna i södra delen av stjärnbilden Björnvaktaren. Den har en kombinerad skenbar magnitud av 4,50 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 10,7 mas, beräknas den befinna sig på ett avstånd av ca 310 ljusår (90 parsek) från solen. (sv) Пи Волопаса (лат. π Boötis), 29 Волопаса (лат. 29 Boötis) — кратная звезда в созвездии Волопаса на расстоянии приблизительно 288 световых лет (около 88,1 парсеков) от Солнца. (ru) HD129174 (π1 Волопаса) — хімічно пекулярна зоря спектрального класуB9 й має видиму зоряну величину в смузі V приблизно 4,9.Вона знаходиться у сузір'ї Волопаса й розташована на відстані близько 317,3 світлових років від Сонця. (uk) 牧夫座π，又名BD+17 2768，HD 129174、SAO 101138、HR 5475，是牧夫座的一颗恒星，视星等为4.94，位于銀經15.64，銀緯62.54，其B1900.0坐标为赤經14h 36m 1.5s，赤緯+16° 62.54′ 49″。 (zh) Pi Bootis (π Bootis / π Boo / 29 Bootis) es un sistema estelar de magnitud aparente +4,91 situado en la constelación de Bootes.En chino recibe el nombre de Zuochetier 左攝提二 (Zuǒ shè tí èr). Se encuentra a 309 años luz del Sistema Solar. La componente secundaria, π2 Bootis (HD 129175 / HR 5476), es una estrella blanca de la secuencia principal de tipo A6V.Con una temperatura estimada de 8.100 K, es 34 veces más luminosa que el Sol.Tiene una masa 2,3 veces mayor que la masa solar y rota a una velocidad de al menos 140 km/s. (es) Pi Bootis (π Boötis / π Boo), est une étoile triple probable de la constellation boréale du Bouvier. Elle est visible à l’œil nu vavec une magnitude apparente combinée de 4,50. En se basant sur une parallaxe annuelle de 10,67 mas, elle est localisée à environ ∼310 a.l. (∼95 pc) du Soleil. Pi Bootis possède le nom traditionnel chinois 左攝提二 (Zuǒ shè tí èr).[réf. nécessaire] (fr) Pi Boötis, Latinized from π Boötis, is a probable triple star system in the northern constellation of Boötes. It is visible to the naked eye with a combined apparent visual magnitude of 4.50. Based upon an annual parallax shift of 10.67 mas as seen from Earth, it is located roughly 310 light years from the Sun. Pi Boötis has the Chinese traditional star name 左攝提二 (Zuǒ shè tí èr) (en)
foaf:name	Pi Boötis (en)
dct:subject	A-type main-sequence stars B-type giants Bayer objects Boötes Bright Star Catalogue objects Double stars Durchmusterung objects Flamsteed objects Henry Draper Catalogue objects Hipparcos objects Mercury-manganese stars Triple stars
Wikipage page ID	2903562 (xsd:integer)
Wikipage revision ID	1079518357 (xsd:integer)
Link from a Wikipage to another Wikipage	B-type star Boötes Stellar classification A-type main-sequence stars B-type giants Bayer objects Boötes Bright Star Catalogue objects Double stars Durchmusterung objects Flamsteed objects Henry Draper Catalogue objects Hipparcos objects Mercury-manganese stars Triple stars Constellation Chemically peculiar star Light year Stellar evolution Stellar spectrum Stellar parallax A-type main-sequence star Latinisation of names Arcsecond Astronomical Unit Sun Position angle Spectroscopic binary Apparent visual magnitude Giant star Traditional Chinese star names Boötes (constellation) Milliarcsecond HgMn star Projected separation Triple star
Link from a Wikipage to an external page	http://stars.astro.illinois.edu/sow/piboo.html http://aladin.u-strasbg.fr/AladinPreview%3F-c=14+40+43.5668%2B16+25+05.967&ident=HD+129174&submit=Aladin+previewer http://webviz.u-strasbg.fr/viz-bin/VizieR-S%3FCCDM%20J14407%2b1625A http://webviz.u-strasbg.fr/viz-bin/VizieR-S%3FHR%205475
sameAs	Pi Boötis Pi Boötis Pi Boötis Pi Boötis Pi Boötis Pi Boötis Pi Boötis

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