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υ Gruis, Latinised as Upsilon Gruis, is a double star in the southern constellation of Grus. The apparent magnitude is 5.61, which is bright enough to be viewed with the naked eye. Located around 87 parsecs (280 ly) distant, the white-hued primary is an A-type main-sequence star of spectral type A1V, a star that is currently fusing its core hydrogen. it is spinning rapidly with a projected rotational velocity of 320 km/s. The companion is a magnitude 8.24 star at an angular separation of 0.90″ from the primary along a position angle of 205°, as of 2009.

AttributesValues
rdf:type
rdfs:label
  • Upsilon Gruis (pt)
  • Upsilon Gruis (en)
  • Ypsilon Gruis (sv)
  • 天鶴座υ (zh)
rdfs:comment
  • υ Gruis, Latinised as Upsilon Gruis, is a double star in the southern constellation of Grus. The apparent magnitude is 5.61, which is bright enough to be viewed with the naked eye. Located around 87 parsecs (280 ly) distant, the white-hued primary is an A-type main-sequence star of spectral type A1V, a star that is currently fusing its core hydrogen. it is spinning rapidly with a projected rotational velocity of 320 km/s. The companion is a magnitude 8.24 star at an angular separation of 0.90″ from the primary along a position angle of 205°, as of 2009. (en)
  • Upsilon Gruis (85 Gruis) é uma estrela na direção da constelação de Grus. Possui uma ascensão reta de 23h 06m 53.60s e uma declinação de −38° 53′ 32.3″. Sua magnitude aparente é igual a 5.62. Considerando sua distância de 294 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.84. Pertence à classe espectral A0V. (pt)
  • Ypsilon Gruis (υ Gruis, förkortat Ypsilon Gru, υ Gru) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den nordöstra delen av stjärnbilden Tranan. Den har en skenbar magnitud på 5,61 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 11,5 mas, beräknas den befinna sig på ett avstånd på ca 280 ljusår (ca 87 parsek) från solen. (sv)
  • 天鶴座υ,又名CD-3914936,HD 218242、SAO 214313、HR 8790,是天鶴座的一颗恒星,视星等为5.61,位于銀經357.92,銀緯-65.25,其B1900.0坐标为赤經23h 1m 19.6s,赤緯-39° -65.25′ 59″。 (zh)
foaf:name
  • υ Gruis (en)
dcterms:subject
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Wikipage revision ID
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absmag v
  • +0.92 (en)
appmag v
b-v
  • +0.01 (en)
class
  • A1V (en)
constell
epoch
luminosity
p error
parallax
prop mo dec
  • +6.40 (en)
prop mo ra
  • +34.31 (en)
radial v
  • +16 (en)
radius
rotational velocity
temperature
has abstract
  • υ Gruis, Latinised as Upsilon Gruis, is a double star in the southern constellation of Grus. The apparent magnitude is 5.61, which is bright enough to be viewed with the naked eye. Located around 87 parsecs (280 ly) distant, the white-hued primary is an A-type main-sequence star of spectral type A1V, a star that is currently fusing its core hydrogen. it is spinning rapidly with a projected rotational velocity of 320 km/s. The companion is a magnitude 8.24 star at an angular separation of 0.90″ from the primary along a position angle of 205°, as of 2009. (en)
  • Upsilon Gruis (85 Gruis) é uma estrela na direção da constelação de Grus. Possui uma ascensão reta de 23h 06m 53.60s e uma declinação de −38° 53′ 32.3″. Sua magnitude aparente é igual a 5.62. Considerando sua distância de 294 anos-luz em relação à Terra, sua magnitude absoluta é igual a 0.84. Pertence à classe espectral A0V. (pt)
  • Ypsilon Gruis (υ Gruis, förkortat Ypsilon Gru, υ Gru) som är stjärnans Bayerbeteckning, är en dubbelstjärna belägen i den nordöstra delen av stjärnbilden Tranan. Den har en skenbar magnitud på 5,61 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 11,5 mas, beräknas den befinna sig på ett avstånd på ca 280 ljusår (ca 87 parsek) från solen. (sv)
  • 天鶴座υ,又名CD-3914936,HD 218242、SAO 214313、HR 8790,是天鶴座的一颗恒星,视星等为5.61,位于銀經357.92,銀緯-65.25,其B1900.0坐标为赤經23h 1m 19.6s,赤緯-39° -65.25′ 59″。 (zh)
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