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ν Gruis, Latinised as Nu Gruis, is a solitary, yellow-hued star in the southern constellation of Grus. It is visible to the naked eye with an apparent visual magnitude of 5.47. The distance to this star, as determined using an annual parallax shift of 11.6 mas as seen from the Earth, is 280 light years. It is drifting further away with a heliocentric radial velocity of +11 km/s.

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rdf:type
rdfs:label
  • Nu Gruis (fr)
  • Nu Gruis (en)
  • Nu Gruis (pt)
  • Ny Gruis (sv)
  • 天鶴座ν (zh)
rdfs:comment
  • Nu Gruis est une étoile de la constellation de la Grue. Sa magnitude apparente est de 5,48. Située à environ 285 années-lumière, il s'agit d'une géante rouge de type spectral G8III, une étoile qui a consommé tout l'hydrogène de son cœur et qui a gonflé. Nu Gruis est une étoile seule. Elle possède un compagnon optique, dont la proximité avec Nu Gruis n'est que fortuite, qui est une étoile de magnitude apparente 12,5, non visible même à l'aide de jumelles. (fr)
  • Nu Gruis (41 Gruis) é uma estrela na direção da constelação de Grus. Possui uma ascensão reta de 22h 28m 39.18s e uma declinação de −39° 07′ 53.0″. Sua magnitude aparente é igual a 5.47. Considerando sua distância de 262 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.94. Pertence à classe espectral G8III. (pt)
  • Ny Gruis (ν Gruis, förkortat Ny Gru, ν Gru) som är stjärnans Bayerbeteckning, är en ensam stjärna belägen i den norra delen av stjärnbilden Tranan. Den har en skenbar magnitud på 5,47 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 11,4 mas, beräknas den befinna sig på ett avstånd på ca 285 ljusår (ca 87 parsek) från solen. (sv)
  • 天鶴座ν,又名CD-3914723,HD 212953、SAO 213850、HR 8552,是天鶴座的一颗恒星,视星等为5.47,位于銀經1.71,銀緯-58.04,其B1900.0坐标为赤經22h 22m 47.6s,赤緯-39° -58.04′ 16″。 (zh)
  • ν Gruis, Latinised as Nu Gruis, is a solitary, yellow-hued star in the southern constellation of Grus. It is visible to the naked eye with an apparent visual magnitude of 5.47. The distance to this star, as determined using an annual parallax shift of 11.6 mas as seen from the Earth, is 280 light years. It is drifting further away with a heliocentric radial velocity of +11 km/s. (en)
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  • Nu Gruis (en)
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absmag v
  • +0.76 (en)
appmag v
b-v
  • +0.95 (en)
class
  • G9 III (en)
constell
epoch
equinox
  • J2000.0 (en)
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