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ν Pavonis, Latinized as Nu Pavonis, is a possible triple star system in the southern constellation of Pavo. It is visible to the naked eye as a faint star that varies in apparent visual magnitude from 4.60 to 4.64 over a period of 0.85584 days. The system lies approximately 440 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +17 km/s. It is a possible member of the Wolf 630 group of co-moving stars.

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  • Nu Pavonis (it)
  • Nu Pavonis (en)
  • Nu Pavonis (pt)
  • Ny Pavonis (sv)
  • 孔雀座ν (zh)
rdfs:comment
  • Nu Pavonis (ν Pavonis, ν Pav) è una stella tripla gerarchica situata nella costellazione del Pavone. Anche in virtù della sua velocità peculiare di 17,0 km/s rispetto ai sistemi vicini, si ritiene che questo sistema stellare possa far parte del gruppo di stelle fuggitive denominato Wolf 630. Situata a circa 440 anni luce dal sistema solare, la sua magnitudine apparente, che varia da +4,60 a +4,64 su un periodo di 0,85584 giorni, fa sì che questa stella sia visibile a occhio nudo nell'emisfero australe. (it)
  • Nu Pavonis (33 Pavonis) é uma estrela na direção da constelação de Pavo. Possui uma ascensão reta de 18h 31m 22.43s e uma declinação de −62° 16′ 41.5″. Sua magnitude aparente é igual a 4.63. Considerando sua distância de 479 anos-luz em relação à Terra, sua magnitude absoluta é igual a 2.55. Pertence à classe espectral B8III. (pt)
  • Ny Pavonis (ν Pavonis, förkortat Ny Pav, ν Pav), som är stjärnans Bayer-beteckning, är en ensam stjärna i den västra delen av stjärnbilden Påfågeln. Den har en genomsnittlig skenbar magnitud på +4,62 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätningar i Hipparcos-uppdraget på ca 7,0 mas beräknas den befinna sig på ca 460 ljusårs (142 parsek) avstånd från solen. (sv)
  • 孔雀座ν,又名CP-62 5879,HD 169978、SAO 254273、HR 6916,是孔雀座的一颗恒星,视星等为4.64,位于銀經332.82,銀緯-21.56,其B1900.0坐标为赤經18h 22m 2s,赤緯-62° -21.56′ 30″。 (zh)
  • ν Pavonis, Latinized as Nu Pavonis, is a possible triple star system in the southern constellation of Pavo. It is visible to the naked eye as a faint star that varies in apparent visual magnitude from 4.60 to 4.64 over a period of 0.85584 days. The system lies approximately 440 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +17 km/s. It is a possible member of the Wolf 630 group of co-moving stars. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/NuPavLightCurve.png
  • 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
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b-v
  • −0.11 (en)
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  • B7III (en)
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