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HD 23127 is a star in the southern constellation of Reticulum. With an apparent visual magnitude of +8.58 it is not visible to the naked eye, but can be viewed with a good pair of binoculars. The star is located at a distance of 307 light years from the Sun based on parallax, and is drifting further away with a radial velocity of ~22 km/s. It has an absolute magnitude of 3.62.

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  • HD 23127 (de)
  • HD 23127 (en)
  • HD 23127 (pl)
  • HD 23127 (pt)
  • HD 23127 (ru)
  • HD 23127 (sv)
  • HD 23127 (zh)
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  • HD 23127 ist ein etwa 322 Lichtjahre entfernter Hauptreihenstern im Sternbild Reticulum. Er besitzt eine scheinbare Helligkeit von 8,6 mag. Im Jahre 2007 veröffentlichten O’Toole et al. die Entdeckung eines Exoplaneten, der diesen Stern umkreist und mit HD 23127 b bezeichnet wird. (de)
  • HD 23127 – gwiazda położona w gwiazdozbiorze Sieci w odległości około 290,6 lat świetlnych od Ziemi. Jej typ widmowy to G2V, a masa jest większa o 13% od masy Słońca. Jest ona żółtym karłem. W 2007 roku odkryto planetę HD 23127 b okrążającą tę gwiazdę po bardzo ekscentrycznej orbicie. (pl)
  • HD 23127 é uma estrela na constelação de Reticulum. Tem uma magnitude aparente de 8,58, sendo invisível a olho nu. Com base em medições de paralaxe pela sonda Gaia, está localizada a aproximadamente 305 anos-luz (94 parsecs) da Terra. Esta é uma estrela de classe G da sequência principal com um tipo espectral de G2V, sendo maior e mais luminosa que o Sol, apesar de ter a mesma classificação. Em 2007, foi descoberto um planeta extrassolar Júpiter excêntrico ao seu redor. (pt)
  • HD 23127 är en gul stjärna i huvudserien i stjärnbilden Rombiska nätet. Stjärnan har visuell magnitud +8,55 och kräver fältkikare för att observeras. Den befinner sig på ett avstånd av ungefär 320 ljusår (sv)
  • HD 23127是一颗位于网罟座的恒星,距离地球大约320光年。用肉眼不能观测到它,但用较好的双筒望远镜就容易看到它。 (zh)
  • HD 23127 — звезда в созвездии Сетки на расстоянии около 320 светового года от нас. Вокруг звезды обращается, как минимум, одна планета. (ru)
  • HD 23127 is a star in the southern constellation of Reticulum. With an apparent visual magnitude of +8.58 it is not visible to the naked eye, but can be viewed with a good pair of binoculars. The star is located at a distance of 307 light years from the Sun based on parallax, and is drifting further away with a radial velocity of ~22 km/s. It has an absolute magnitude of 3.62. (en)
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