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. No planetary companions have yet been detected orbiting these stars.

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dbpprop: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. No planetary companions have yet been detected orbiting these stars.
dbpprop:appmagV
  • 5.22 (xsd:double)
dbpprop:bV
  • +0.570
dbpprop:class
  • F9V (G0V/K1V)
dbpprop:constell
dbpprop:dec
dbpprop:epoch
  • J2000
dbpprop:gravity
  • 4.6 (xsd:double)
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dbpprop:mass
  • 1.07/0.71
dbpprop:metal
  • [Fe/H]=−0.11
dbpprop:pError
  • 0.54 (xsd:double)
dbpprop:parallax
  • 66.76 (xsd:double)
dbpprop:propMoDec
  • −143.98
dbpprop:propMoRa
  • 202.86 (xsd:double)
dbpprop:ra
dbpprop:radialV
  • -47.2 (xsd:double)
dbpprop:temperature
  • 6000 (xsd:integer)
dbpprop:uB
  • +0.029
dbpprop:variable
  • Spectroscopic binary
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rdfs:comment
  • 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. No planetary companions have yet been detected orbiting these stars.
rdfs:label
  • HD 176051
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