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Delta1 Gruis, Latinized from δ1 Gruis, is a candidate binary star system in the constellation Grus. With a peak apparent visual magnitude of 3.97, it is bright enough to be seen with the naked eye at night. The distance to this system, as determined using an annual parallax shift of 10.54 mas as seen from the Earth, is around 309 light years. It is gradually moving away from the Sun with a radial velocity of +4.9 km/s.

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rdfs:label
  • Delta1 Gruis (en)
  • Delta1 Gruis (it)
  • Delta1 Gruis (fr)
  • Delta1 Gruis (pt)
  • Delta1 Gruis (sv)
  • 天鶴座δ1 (zh)
rdfs:comment
  • Delta1 Gruis (en abrégé δ1 Gru) est une étoile de la constellation de la Grue. Sa magnitude apparente est de 3,97. (fr)
  • Delta1 Gruis (δ1 Gruis, δ1 Gruis) è una stella della costellazione della Gru. Di magnitudine apparente +3,97, dista 309 anni luce dal sistema solare. Condivide la lettera δ della nomenclatura di Bayer con , con la quale forma una binaria ottica in cielo; tuttavia le due stelle non sono legate gravitazionalmente tra loro, visto che hanno un differente moto proprio nello spazio. (it)
  • Delta1 Gruis (δ1 Gruis, förkortat Delta1 Gru, δ1 Gru) som är stjärnans Bayerbeteckning, är en trolig dubbelstjärna belägen i den mellersta delen av stjärnbilden Tranan. Den har en skenbar magnitud på 3,97 och är synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallaxmätning inom Hipparcosuppdraget på ca 10,5 mas, beräknas den befinna sig på ett avstånd på ca 309 ljusår (ca 95 parsek) från solen. (sv)
  • Delta1 Gruis (42 Gruis) é uma estrela na direção da constelação de Grus. Possui uma ascensão reta de 22h 29m 16.15s e uma declinação de −43° 29′ 44.0″. Sua magnitude aparente é igual a 3.97. Considerando sua distância de 296 anos-luz em relação à Terra, sua magnitude absoluta é igual a −0.82. Pertence à classe espectral G6/G8III. (pt)
  • 天鶴座δ1,又名CD-4414931,HD 213009、SAO 231154、HR 8556,是天鶴座的一颗恒星,视星等为3.97,位于銀經353.77,銀緯-57.05,其B1900.0坐标为赤經22h 23m 17.6s,赤緯-44° -57.05′ 23″。 (zh)
  • Delta1 Gruis, Latinized from δ1 Gruis, is a candidate binary star system in the constellation Grus. With a peak apparent visual magnitude of 3.97, it is bright enough to be seen with the naked eye at night. The distance to this system, as determined using an annual parallax shift of 10.54 mas as seen from the Earth, is around 309 light years. It is gradually moving away from the Sun with a radial velocity of +4.9 km/s. (en)
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  • Delta1 Gruis (en)
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absmag v
  • −0.91 (en)
appmag v
b-v
  • +1.03 (en)
class
  • G6/8 III (en)
constell
epoch
equinox
  • J2000.0 (en)
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parallax
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