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56 Orionis is a single, variable star in the equatorial constellation of Orion. It has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude that fluctuates around 4.76. The star is located at a distance of approximately 1,130 light years from the Sun based on parallax. It is drifting further away with a radial velocity of +11 km/s. The star has a peculiar velocity of 19.0+2.9−3.1 km/s relative to its neighbors, and may be a runaway star. It has one reported visual companion, designated component B, with magnitude 13.5 and angular separation 42.9″.

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  • 56 Orionis (en)
  • 56 Orionis (fr)
  • 56 Orionis (it)
  • 56 Orionis (sv)
  • 参宿增廿二 (zh)
rdfs:comment
  • 56 Orionis (en abrégé 56 Ori) est une étoile variable de la constellation d'Orion, située à 1 130 al (~350 pc) de la Terre. Elle est de couleur orange et faiblement visible à l'œil nu avec une magnitude apparente de 4,76. (fr)
  • 56 Orionis è una stella gigante brillante arancione di magnitudine 4,76 situata nella costellazione di Orione. Dista 1113 anni luce dal sistema solare. (it)
  • 56 Orionis, som är stjärnans Flamsteed-beteckning är en ensam stjärna i den mellersta delen av stjärnbilden Orion. Den har en genomsnittlig skenbar magnitud på ca 4,76 och är svagt synlig för blotta ögat där ljusföroreningar ej förekommer. Baserat på parallax enligt Gaia Data Release 2 på ca 2,9 mas, beräknas den befinna sig på ett avstånd på ca 1 130 ljusår (ca 350 parsek) från solen. Den rör sig bort från solen med en heliocentrisk radialhastighet av ca 11 km/s. Stjärnan har en egenrörelse på 19,0+2,9−3,1 km/s i förhållande till dess grannar, och kan vara en flyktstjärna. (sv)
  • 獵戶座56,又名BD+01 1151,HD 39400、SAO 113220、HR 2037,是獵戶座的一颗恒星,视星等为4.78,位于銀經204.41,銀緯-12.22,其B1900.0坐标为赤經5h 47m 14.8s,赤緯+1° -12.22′ 51″。 (zh)
  • 56 Orionis is a single, variable star in the equatorial constellation of Orion. It has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude that fluctuates around 4.76. The star is located at a distance of approximately 1,130 light years from the Sun based on parallax. It is drifting further away with a radial velocity of +11 km/s. The star has a peculiar velocity of 19.0+2.9−3.1 km/s relative to its neighbors, and may be a runaway star. It has one reported visual companion, designated component B, with magnitude 13.5 and angular separation 42.9″. (en)
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