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Zeta Pavonis, Latinized from ζ Pavonis, is an orange-hued star in the southern constellation Pavo. Its apparent magnitude is 4.01, which is bright enough to be faintly visible to the naked eye. The annual parallax shift of this star is 14.93 mas as seen from Earth, which provides a distance estimate of approximately 420 light-years (130 parsecs) away from the Sun. It is moving closer to the Sun with a radial velocity of −16.30. Based upon its motion through space, this star appears to be a member of the Hyades Supercluster.

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rdf:type
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  • Zeta Pavonis (fr)
  • Zeta Pavonis (it)
  • Zeta Pavonis (pt)
  • Zeta Pavonis (sv)
  • Zeta Pavonis (en)
  • 孔雀座ζ (zh)
rdfs:comment
  • Zeta Pavonis (35 Pavonis) é uma estrela na direção da constelação de Pavo. Possui uma ascensão reta de 18h 43m 02.13s e uma declinação de −71° 25′ 39.8″. Sua magnitude aparente é igual a 4.01. Considerando sua distância de 210 anos-luz em relação à Terra, sua magnitude absoluta é igual a 4.39. Pertence à classe espectral K2III. (pt)
  • Zeta Pavonis (ζ Pav, förkortat Zeta Pav, ζ Pav) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den sydvästra delen av stjärnbilden Påfågeln. Den har en skenbar magnitud på 4,01 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 14,9 mas, beräknas den befinna sig på ett avstånd på ca 218 ljusår (ca 67 parsek) från solen. Den rör sig närmare solen med en radiell hastighet på -16,3 km/s. Sett utifrån dess rörelse genom rymden verkar stjärnan ingå i stjärnhopen Hyaderna. (sv)
  • 孔雀座ζ,又名CP-71 2353,HD 171759、SAO 257620、HR 6982,是孔雀座的一颗恒星,视星等为4.01,位于銀經323.49,銀緯-24.95,其B1900.0坐标为赤經18h 31m 21.1s,赤緯-71° -24.95′ 50″。 (zh)
  • Zeta Pavonis (ζ Pavonis / ζ Pav) est une étoile de la constellation australe du Paon. Sa magnitude apparente est de 4,00, et elle est donc visible à l'œil nu. D'après la mesure de sa parallaxe par le satellite Hipparcos, l'étoile est distante d'environ ∼218 a.l. (∼66,8 pc) de la Terre, et elle se rapproche du système solaire à une vitesse radiale héliocentrique de −16 km/s. Son mouvement à travers l'espace suggère qu'elle est membre du courant des Hyades. (fr)
  • Zeta Pavonis, Latinized from ζ Pavonis, is an orange-hued star in the southern constellation Pavo. Its apparent magnitude is 4.01, which is bright enough to be faintly visible to the naked eye. The annual parallax shift of this star is 14.93 mas as seen from Earth, which provides a distance estimate of approximately 420 light-years (130 parsecs) away from the Sun. It is moving closer to the Sun with a radial velocity of −16.30. Based upon its motion through space, this star appears to be a member of the Hyades Supercluster. (en)
  • Zeta Pavonis (ζ Pavonis / ζ Pav), è la sesta stella più luminosa della costellazione del Pavone. Dista dal sistema solare circa 218 anni luce e la sua magnitudine apparente è +4,01. È invisibile alle medie latitudini dell'emisfero boreale, più a nord del parallelo 29°N, mentre nell'emisfero australe diventa circumpolare più a sud della latitudine 29°S. (it)
foaf:name
  • ζ Pavonis (en)
foaf:depiction
  • 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
  • −0.12 (en)
appmag v
  • +4.01 (en)
b-v
  • +1.13 (en)
class
  • K0III (en)
constell
epoch
  • J2000 (en)
luminosity
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