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V538 Aurigae is a single star in the northern constellation of Auriga. With an apparent visual magnitude of 6.23, this star requires good dark sky conditions to view with the naked eye. It is located at a distance of 40.0 light-years (12.3 pc) from Sun based on parallax. The star is drifting further away with a radial velocity of 0.9 km/s. It is a member of the Local Association, and is most likely a thin disk star.

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  • V538 Aurigae (es)
  • HD 37394 (it)
  • V538 Aurigae (nl)
  • V538 Aurigae (en)
  • HD 37394 (zh)
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  • HD 37394, nota nella nomenclatura delle stelle variabili come V538 Aurigae (V538 Aur), è una stella nana arancione nella sequenza principale di magnitudine 6,23 situata nella costellazione dell'Auriga. Dista 40 anni luce dal sistema solare. (it)
  • V538 Aurigae is een oranje dwerg met een spectraalklasse van K1.V. De ster bevindt zich 40,02 lichtjaar van de zon. (nl)
  • HD 37394,又名BD+53 934,SAO 25319、HR 1925,是一颗恒星,视星等为6.23,位于銀經158.38,銀緯11.95,其B1900.0坐标为赤經5h 33m 13.4s,赤緯+53° 11.95′ 26″。 (zh)
  • V538 Aurigae (V538 Aur) es un sistema estelar en la constelación de Auriga, el cochero.De acuerdo a la nueva reducción de los datos de paralaje de Hipparcos, está a 40,0 años luz del Sistema Solar. La estrella primaria, Gliese 211 (HR 1925 / HD 37394),​ tiene magnitud aparente +6,23.Es una enana naranja de tipo espectral K1V con una temperatura efectiva de 5293 ± 109 K.​Su luminosidad equivale a algo menos de la luminosidad solar.​Tiene un radio un 18% más pequeño que el del Sol​ y gira sobre sí misma con una velocidad de rotación proyectada de 4 km/s.​Igualmente posee menos masa que el Sol, aproximadamente 0,91 masas solares.​No se ha detectado exceso en el infrarrojo ni a 24 μm ni a 70 μm,​ lo que en principio descarta la presencia de un disco de polvo a su alrededor.Evidencia actividad (es)
  • V538 Aurigae is a single star in the northern constellation of Auriga. With an apparent visual magnitude of 6.23, this star requires good dark sky conditions to view with the naked eye. It is located at a distance of 40.0 light-years (12.3 pc) from Sun based on parallax. The star is drifting further away with a radial velocity of 0.9 km/s. It is a member of the Local Association, and is most likely a thin disk star. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/V538AurLightCurve.png
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