An Entity of Type: star, from Named Graph: http://dbpedia.org, within Data Space: dbpedia.org:8891

Pi Coronae Borealis, Latinized from π Coronae Borealis, is a solitary, orange-hued star in the northern constellation of Corona Borealis. Its apparent magnitude is 5.58, which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 13.40 mas as measured from Earth, it is located about 243 light years from the Sun. The star is moving closer to the Sun with a radial velocity of −5 km/s. It is most likely (98% chance) a member of the thin disk population.

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dbo:abstract
  • Pi de la Corona Boreal (π Coronae Borealis) és un estel en la constel·lació de la Corona Boreal de magnitud aparent +5,58. Es troba a 243 anys llum del Sistema Solar. (ca)
  • Pi Coronae Borealis (π CrB / 9 Coronae Borealis)​ es una estrella en la constelación de la Corona Boreal de magnitud aparente +5,58.Se encuentra a 243 años luz del Sistema Solar. (es)
  • Pi Coronae Borealis, Latinized from π Coronae Borealis, is a solitary, orange-hued star in the northern constellation of Corona Borealis. Its apparent magnitude is 5.58, which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 13.40 mas as measured from Earth, it is located about 243 light years from the Sun. The star is moving closer to the Sun with a radial velocity of −5 km/s. It is most likely (98% chance) a member of the thin disk population. This is an evolved G-type giant star with a stellar classification of G9 III:, where the ':' indicates some uncertainty about the classification. (Bartkevicius and Lazauskaite (1997) classify it as K0 III.) The star has 1.61 times the mass of the Sun and has expanded to about 10 times the Sun's radius. The abundance of iron is lower than in the Sun: the star is considered metal deficient. It is around 4.6 billion years old and is radiating 39 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,667 K. (en)
  • Pi Coronae Borealis (9 Coronae Borealis) é uma estrela na direção da constelação de Corona Borealis. Possui uma ascensão reta de 15h 43m 59.32s e uma declinação de +32° 30′ 57.0″. Sua magnitude aparente é igual a 5.57. Considerando sua distância de 249 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.16. Pertence à classe espectral G9III:. (pt)
  • Pi Coronae Borealis (π Coronae Borealis, förkortat Pi CrB, π CrB) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Norra kronan. Den har en skenbar magnitud på 5,58 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,4 mas, beräknas den befinna sig på ett avstånd på ca 243 ljusår (ca 75 parsek) från solen. Den rör sig närmare solen med en radiell hastighet på -5 km/s. och ingår troligen (98 procent sannolikhet) i Vintergatans tunna skiva. (sv)
  • 北冕座π,又名BD+32 2621,HD 140716、SAO 64870、HR 5855,是北冕座的一颗恒星,视星等为5.56,位于銀經51.87,銀緯52.44,其B1900.0坐标为赤經15h 40m 2.8s,赤緯+32° 52.44′ 53″。 (zh)
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  • +1.21 (en)
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  • G9 III: (en)
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  • J2000.0 (en)
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  • 2.700000 (xsd:double)
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  • 39 (xsd:integer)
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  • 1.610000 (xsd:double)
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  • −0.15 (en)
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  • −8.85 (en)
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  • Pi de la Corona Boreal (π Coronae Borealis) és un estel en la constel·lació de la Corona Boreal de magnitud aparent +5,58. Es troba a 243 anys llum del Sistema Solar. (ca)
  • Pi Coronae Borealis (π CrB / 9 Coronae Borealis)​ es una estrella en la constelación de la Corona Boreal de magnitud aparente +5,58.Se encuentra a 243 años luz del Sistema Solar. (es)
  • Pi Coronae Borealis (9 Coronae Borealis) é uma estrela na direção da constelação de Corona Borealis. Possui uma ascensão reta de 15h 43m 59.32s e uma declinação de +32° 30′ 57.0″. Sua magnitude aparente é igual a 5.57. Considerando sua distância de 249 anos-luz em relação à Terra, sua magnitude absoluta é igual a 1.16. Pertence à classe espectral G9III:. (pt)
  • Pi Coronae Borealis (π Coronae Borealis, förkortat Pi CrB, π CrB) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den mellersta delen av stjärnbilden Norra kronan. Den har en skenbar magnitud på 5,58 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 13,4 mas, beräknas den befinna sig på ett avstånd på ca 243 ljusår (ca 75 parsek) från solen. Den rör sig närmare solen med en radiell hastighet på -5 km/s. och ingår troligen (98 procent sannolikhet) i Vintergatans tunna skiva. (sv)
  • 北冕座π,又名BD+32 2621,HD 140716、SAO 64870、HR 5855,是北冕座的一颗恒星,视星等为5.56,位于銀經51.87,銀緯52.44,其B1900.0坐标为赤經15h 40m 2.8s,赤緯+32° 52.44′ 53″。 (zh)
  • Pi Coronae Borealis, Latinized from π Coronae Borealis, is a solitary, orange-hued star in the northern constellation of Corona Borealis. Its apparent magnitude is 5.58, which is bright enough to be faintly visible to the naked eye. Based upon an annual parallax shift of 13.40 mas as measured from Earth, it is located about 243 light years from the Sun. The star is moving closer to the Sun with a radial velocity of −5 km/s. It is most likely (98% chance) a member of the thin disk population. (en)
rdfs:label
  • Pi de la Corona Boreal (ca)
  • Pi Coronae Borealis (es)
  • Pi Coronae Borealis (en)
  • Pi Coronae Borealis (pt)
  • Pi Coronae Borealis (sv)
  • 北冕座π (zh)
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  • Pi Coronae Borealis (en)
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