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Xi Cygni
Star in the constellation Cygnus From Wikipedia, the free encyclopedia
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ξ Cygni (Latinised as Xi Cygni) is a spectroscopic binary star in the constellation Cygnus, made up of a K-type supergiant star (primary) and an A-type star (secondary). Its apparent magnitude is 3.73, making it readily visible to the naked eye, and it is located around 350 parsecs (1,100 ly) away.
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Characteristics
The system contains two stars which orbit every 18 years in a mildly eccentric orbit. The primary star is a supergiant with a spectral type of around K4, while the secondary is an A-type main-sequence star with a spectral type of A1.5. Stellar winds from the supergiant have been measured at around 50 km/s, but with variations in speed and individual line strengths.[5]
The distance to Xi Cygni is of about 350 parsecs (1,100 ly), based on parallax measurements.[1] At this distance, the apparent magnitude is diminished by 0.16 magnitudes.[6]
ξ Cygni is in the Kepler spacecraft's field of view but no planets have been detected.[7]
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Gallery
- H-alpha RGB amateur image of ξ Cygni, center star, at edge of NGC7000
- NGC 7000 (North America Nebula). ξ Cygni is the bright star on the left.
References
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