About: VZ Camelopardalis     Goto   Sponge   NotDistinct   Permalink

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VZ Camelopardalis is a single, variable star in the northern circumpolar constellation of Camelopardalis. It has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude that fluctuates around 4.92. The star is located at a distance of approximately 500 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +12 km/s. It was considered a member of the Hyades Supercluster, but in 1990 this was brought into question.

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  • VZ Camelopardalis (en)
  • VZ Camelopardalis (sv)
  • 六甲四 (zh)
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  • VZ Camelopardalis (VZ Cam) är en stjärna i stjärnbilden Giraffen. VZ Camelopardalis är en röd jättestjärna med en magnitud på +4,92 och den ligger på ungefär 473 ljusårs avstånd. VZ Camelopardalis är en variabel stjärna som varierar mellan magnituderna +4,80 och +4,96 på 23,7 dygn. (sv)
  • 鹿豹座VZ,又名BD+82 201,HD 55966、SAO 1179、HR 2742,是鹿豹座的一颗恒星,视星等为4.96,位于銀經131.42,銀緯28.18,其B1900.0坐标为赤經7h 10m 3.1s,赤緯+82° 28.18′ 16″。 (zh)
  • VZ Camelopardalis is a single, variable star in the northern circumpolar constellation of Camelopardalis. It has a reddish hue and is faintly visible to the naked eye with an apparent visual magnitude that fluctuates around 4.92. The star is located at a distance of approximately 500 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +12 km/s. It was considered a member of the Hyades Supercluster, but in 1990 this was brought into question. (en)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/VZCamLightCurve.png
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absmag v
  • −1.00 (en)
appmag v
class
  • M4IIIa (en)
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