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Rho Tucanae (ρ Tuc, ρ Tucanae) is a binary star system in the southern constellation of Tucana. It is visible to the naked eye with a combined apparent visual magnitude of +5.38. Based upon an annual parallax shift of 24.37 mas as seen from Earth, it is located 131 light years from the Sun.

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  • Rho Tucanae (es)
  • Rho Tucanae (en)
  • Rho Tucanae (pt)
  • Rho Tucanae (sv)
  • 鳥喙五 (zh)
rdfs:comment
  • Rho Tucanae (62 Tucanae) é uma estrela na direção da constelação de Tucana. Possui uma ascensão reta de 00h 42m 28.30s e uma declinação de −65° 28′ 05.3″. Sua magnitude aparente é igual a 5.38. Considerando sua distância de 133 anos-luz em relação à Terra, sua magnitude absoluta é igual a 2.33. Pertence à classe espectral F6V. (pt)
  • Rho Tucanae (ρ Tuc, förkortat Rho Tuc, ρ Tuc) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den mellersta delen av stjärnbilden Tukanen. Den har en kombinerad skenbar magnitud på 5,38 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 24,4 mas, beräknas den befinna sig på ett avstånd på ca 134 ljusår (ca 41 parsek) från solen. (sv)
  • 杜鵑座ρ,又名CP-66 47,HD 4089、SAO 248237、HR 187,是杜鵑座的一颗恒星,视星等为5.39,位于銀經304.43,銀緯-51.63,其B1900.0坐标为赤經0h 38m 12s,赤緯-66° -51.63′ 3″。 (zh)
  • Rho Tucanae (ρ Tuc / HD 4089 / HR 187) es un sistema estelar de magnitud aparente +5,39​ situado en la constelación de Tucana. Se encuentra a 133 años luz del Sistema Solar. Rho Tucanae es una binaria espectroscópica cuya componente principal es una estrella blanco-amarilla de tipo espectral F6V, semejante a Tabit (π3 Orionis) o γ Serpentis.Con una temperatura efectiva de 6223 K,​ su luminosidad es aproximadamente 6 veces superior a la luminosidad solar.Gira sobre sí misma con una velocidad de rotación proyectada de 23,5 km/s, siendo su período de rotación igual o inferior a 5 días.​Su metalicidad —abundancia relativa de elementos más pesados que el helio— es muy similar a la solar ([Fe/H] = -0,03).Diversos estudios estiman su masa entre 1,32​ y 1,57 masas solares​ y su edad se sitúa en to (es)
  • Rho Tucanae (ρ Tuc, ρ Tucanae) is a binary star system in the southern constellation of Tucana. It is visible to the naked eye with a combined apparent visual magnitude of +5.38. Based upon an annual parallax shift of 24.37 mas as seen from Earth, it is located 131 light years from the Sun. (en)
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  • Rho Tucanae (en)
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absmag v
  • +2.75 (en)
age gyr
appmag v
  • +5.38 (en)
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