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Rho Pavonis, Latinized from ρ Pavonis, is a single, variable star in the southern constellation of Pavo. It is yellow-white in hue and faintly visible to the naked eye with an apparent visual magnitude that fluctuates around 4.86. The star is located at a distance of approximately 190 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +8 km/s. It is a candidate outlying member of the Tucana Association of co-moving stars.

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  • Rho Pavonis (en)
  • Rho Pavonis (pt)
  • Rho Pavonis (sv)
  • HD195961 (uk)
  • 孔雀座ρ (zh)
rdfs:comment
  • Rho Pavonis (107 Pavonis) é uma estrela na direção da constelação de Pavo. Possui uma ascensão reta de 20h 37m 35.24s e uma declinação de −61° 31′ 47.1″. Sua magnitude aparente é igual a 4.86. Considerando sua distância de 195 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.67. Pertence à classe espectral Fm delta Del. É uma estrela variável δ Scuti. (pt)
  • Rho Pavonis (ρ Pavonis, förkortat Rho Pav, ρ Pav), som är stjärnans Bayer-beteckning, är en ensam stjärna i den nordöstra delen av stjärnbilden Påfågeln. Den har en genomsnittlig skenbar magnitud på +4,88 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätningar i Hipparcos-uppdraget på ca 17,2 mas beräknas den befinna sig på ca 190 ljusårs (58 parsek) avstånd från solen. (sv)
  • 孔雀座ρ,又名CP-61 6495,HD 195961、SAO 254835、HR 7859,是孔雀座的一颗恒星,视星等为4.88,位于銀經334.83,銀緯-36.18,其B1900.0坐标为赤經20h 29m 12.4s,赤緯-61° -36.18′ 24″。 (zh)
  • HD195961 — хімічно пекулярна зоря спектрального класу F1, що має видиму зоряну величину в смузі V приблизно 4,9.Вона розташована на відстані близько 195,0 світлових років від Сонця. (uk)
  • Rho Pavonis, Latinized from ρ Pavonis, is a single, variable star in the southern constellation of Pavo. It is yellow-white in hue and faintly visible to the naked eye with an apparent visual magnitude that fluctuates around 4.86. The star is located at a distance of approximately 190 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +8 km/s. It is a candidate outlying member of the Tucana Association of co-moving stars. (en)
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