HD 176051 is a spectroscopic binary star system located approximately 49 light years away from Earth, in the constellation Lyra. The pair orbit with a period of 22,423 days (61.4 years) and an eccentricity of 0.25. Compared to the Sun, they have a somewhat lower proportion of elements more massive than helium. Their individual masses are estimated at 1.07 and 0.71 solar masses.

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dbpedia-owl:abstract
  • HD 176051 is a spectroscopic binary star system located approximately 49 light years away from Earth, in the constellation Lyra. The pair orbit with a period of 22,423 days (61.4 years) and an eccentricity of 0.25. Compared to the Sun, they have a somewhat lower proportion of elements more massive than helium. Their individual masses are estimated at 1.07 and 0.71 solar masses.
  • HD 176051 — двойная звезда, которая находится в созвездии Лира на расстоянии около 49 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета.
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  • 0 (xsd:integer)
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  • J2000
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  • Spectroscopic binary
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  • HD 176051 is a spectroscopic binary star system located approximately 49 light years away from Earth, in the constellation Lyra. The pair orbit with a period of 22,423 days (61.4 years) and an eccentricity of 0.25. Compared to the Sun, they have a somewhat lower proportion of elements more massive than helium. Their individual masses are estimated at 1.07 and 0.71 solar masses.
  • HD 176051 — двойная звезда, которая находится в созвездии Лира на расстоянии около 49 световых лет от нас. Вокруг звезды обращается, как минимум, одна планета.
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  • HD 176051
  • HD 176051
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