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HD 44131 is a star in the equatorial constellation of Orion, positioned near the eastern constellation border with Monoceros. It has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.91. The star is located at a distance of approximately 465 light years from the Sun based on parallax, and it is drifting further away with a radial velocity of +48.6 km/s. Based on radial velocity variations, it is a candidate spectroscopic binary system and a preliminary orbital solution was published in 1991 with a period of 9.29 yr. However, these velocity variations may be due to other causes.

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  • HD 44131 (en)
  • HD 44131 (it)
  • HD 44131 (sv)
  • HD 44131 (zh)
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  • HD 44131 è una stella gigante rossa di magnitudine 4,93 situata nella costellazione di Orione. Dista 506 anni luce dal sistema solare. (it)
  • HD 44131,又名BD-02 1564,SAO 133118、HR 2275,是一颗恒星,视星等为4.9,位于銀經211.97,銀緯-8.34,其B1900.0坐标为赤經6h 14m 59.1s,赤緯-2° -8.34′ 7″。 (zh)
  • HD 44131 is a star in the equatorial constellation of Orion, positioned near the eastern constellation border with Monoceros. It has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.91. The star is located at a distance of approximately 465 light years from the Sun based on parallax, and it is drifting further away with a radial velocity of +48.6 km/s. Based on radial velocity variations, it is a candidate spectroscopic binary system and a preliminary orbital solution was published in 1991 with a period of 9.29 yr. However, these velocity variations may be due to other causes. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Orion_constellation_map.svg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Red_circle.svg
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absmag v
  • −0.86 (en)
appmag v
b-v
  • +1.60 (en)
class
  • M1III (en)
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