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ξ Pavonis, Latinised as Xi Pavonis, is a triple star system in the southern constellation of Pavo. It is visible to the naked eye as a faint star with a combined apparent visual magnitude of 4.35 The system is located approximately 440 light-years from the Sun based on parallax, and it is drifting further away with a radial velocity of +12 km/s.

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  • Xi Pavonis (pt)
  • Xi Pavonis (sv)
  • Xi Pavonis (en)
  • 孔雀座ξ (zh)
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  • Xi Pavonis (26 Pavonis) é uma estrela na direção da constelação de Pavo. Possui uma ascensão reta de 18h 23m 13.62s e uma declinação de −61° 29′ 38.1″. Sua magnitude aparente é igual a 4.35. Considerando sua distância de 420 anos-luz em relação à Terra, sua magnitude absoluta é igual a −1.71. Pertence à classe espectral M1III SB. (pt)
  • Xi Pavonis (ξ Pav, förkortat Xi Pav, ξ Pav) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den mellersta delen av stjärnbilden Påfågeln. Den har en skenbar magnitud på 4,35 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 7,0 mas, beräknas den befinna sig på ett avstånd på ca 470 ljusår (ca 140 parsek) från solen. (sv)
  • 孔雀座ξ,又名CP-61 6140,HD 168339、SAO 254226、HR 6855,是孔雀座的一颗恒星,视星等为4.36,位于銀經333.29,銀緯-20.4,其B1900.0坐标为赤經18h 14m 0.6s,赤緯-61° -20.4′ 21″。 (zh)
  • ξ Pavonis, Latinised as Xi Pavonis, is a triple star system in the southern constellation of Pavo. It is visible to the naked eye as a faint star with a combined apparent visual magnitude of 4.35 The system is located approximately 440 light-years from the Sun based on parallax, and it is drifting further away with a radial velocity of +12 km/s. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Pavo_constellation_map.svg
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absmag v
  • −1.16 (en)
appmag v
b-v
  • +1.46 (en)
class
  • K4III (en)
constell
eccentricity
epoch
  • J2000 (en)
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