About: HD 194012

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HD 194012 (HR 7793; Gliese 789) is a star in the equatorial constellation Delphinus. It has an apparent magnitude of 6.15, making it visible to the naked eye under ideal conditions. The star is relatively close at a distance of only 85 light years but is receding with a heliocentric radial velocity of 4.5 km/s. A 2010 paper has identified a candidate substellar companion 12.78″ away along a position angle of 67.9°. HD 194012 has been examined for infrared excess suggesting a debris disk but none was found.

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  • HD 194012 (HR 7793; Gliese 789) is a star in the equatorial constellation Delphinus. It has an apparent magnitude of 6.15, making it visible to the naked eye under ideal conditions. The star is relatively close at a distance of only 85 light years but is receding with a heliocentric radial velocity of 4.5 km/s. HD 194012 has a stellar classification of F7 V, indicating that it is an ordinary F-type main-sequence star. It has 121% the mass of the Sun and is estimated to be a billion years old, spinning with a projected rotational velocity of 5 km/s. The star's diameter is 118% that of the Sun and shines with a luminosity of 1.9 L☉ from its photosphere at an effective temperature of 6,301 K, giving a yellow white hue. HD 194012's metallicity is calculated to be 87% that of the Sun. A 2010 paper has identified a candidate substellar companion 12.78″ away along a position angle of 67.9°. HD 194012 has been examined for infrared excess suggesting a debris disk but none was found. (en)
  • HD 194012,又名BD+14 4275,SAO 106042、HR 7793,是一颗恒星,视星等为6.17,位于銀經56.82,銀緯-12.71,其B1900.0坐标为赤經20h 18m 12.4s,赤緯+14° -12.71′ 51″。 (zh)
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  • HD 194012,又名BD+14 4275,SAO 106042、HR 7793,是一颗恒星,视星等为6.17,位于銀經56.82,銀緯-12.71,其B1900.0坐标为赤經20h 18m 12.4s,赤緯+14° -12.71′ 51″。 (zh)
  • HD 194012 (HR 7793; Gliese 789) is a star in the equatorial constellation Delphinus. It has an apparent magnitude of 6.15, making it visible to the naked eye under ideal conditions. The star is relatively close at a distance of only 85 light years but is receding with a heliocentric radial velocity of 4.5 km/s. A 2010 paper has identified a candidate substellar companion 12.78″ away along a position angle of 67.9°. HD 194012 has been examined for infrared excess suggesting a debris disk but none was found. (en)
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  • HD 194012 (en)
  • HD 194012 (zh)
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