About: HD 10800

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HD 10800, also known as HR 512 or Gliese 67.1, is a triple star located in the southern circumpolar constellation Octans. It has a combined apparent magnitude of 5.87, allowing it to be faintly seen with the naked eye. The system is relatively close at a distance of 88.1 light years but is drifting closer with a heliocentric radial velocity −1.1 km/s.

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dbo:abstract
  • HD 10800, also known as HR 512 or Gliese 67.1, is a triple star located in the southern circumpolar constellation Octans. It has a combined apparent magnitude of 5.87, allowing it to be faintly seen with the naked eye. The system is relatively close at a distance of 88.1 light years but is drifting closer with a heliocentric radial velocity −1.1 km/s. The system has a blended spectral classification of G1 V, indicating an ordinary G-type main-sequence star. The primary is a spectroscopic binary consisting of a G-type and K-type star circling around each other in 19 days. HD 10800B has a class of G2 V, the same spectral class as our own Sun. The AB pair take 1.7 years to orbit each other. (en)
  • HD 10800,又名CP-83 27,SAO 258271、HR 512,是一颗恒星,视星等为5.87,位于銀經301.23,銀緯-34,其B1900.0坐标为赤經1h 40m 33.8s,赤緯-83° -34′ 2″。 (zh)
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  • HD 10800,又名CP-83 27,SAO 258271、HR 512,是一颗恒星,视星等为5.87,位于銀經301.23,銀緯-34,其B1900.0坐标为赤經1h 40m 33.8s,赤緯-83° -34′ 2″。 (zh)
  • HD 10800, also known as HR 512 or Gliese 67.1, is a triple star located in the southern circumpolar constellation Octans. It has a combined apparent magnitude of 5.87, allowing it to be faintly seen with the naked eye. The system is relatively close at a distance of 88.1 light years but is drifting closer with a heliocentric radial velocity −1.1 km/s. (en)
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  • HD 10800 (en)
  • HD 10800 (zh)
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