xi Cygni
{{short description|Star in the constellation Cygnus}}
{{Starbox begin
| name = ξ Cygni
}}
{{Starbox image
| image=
{{Location mark
|image=Cygnus constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=10|mark_link=ξ Cyg
|x=231|y=322
}}
|caption=Location of ξ Cygni (circled)
}}
{{Starbox observe
|epoch = J2000
|constell = Cygnus
}}
{{Starbox character
}}
{{Starbox astrometry
| parallax = 2.8363
| p_error = 0.1269
| parallax_footnote = {{cite Gaia DR3|2162316545207257600}}
}}
{{Starbox orbit
|period_unitless=6,750 ± 200 days
|eccentricity=0.25 ± 0.07
|inclination=~50
|axis_unitless=~{{solar radius|766}}
}}
{{Starbox detail
| component1 = Primary
| temperature = {{val|3,878|33|fmt=commas}}{{snd}}4,031
| gravity = 0.89
| metal_fe = −0.26
| radius = {{val|220.09|9.64|10.56}}
| luminosity = {{val|9889|964}}
| component2 = Secondary
| age_myr2 =
}}
{{Starbox catalog
| names = 62 Cygni, FK5 792, GC 29459, HIP 104060, HR 8079, HD 200905, SAO 50424
}}
{{Starbox reference
| Simbad = Xi+Cygni
}}
{{Starbox end}}
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 {{convert|350|pc|ly}} away.
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.
The distance to Xi Cygni is of about {{convert|350|pc|ly}}, based on parallax measurements. At this distance, the apparent magnitude is diminished by 0.16 magnitudes.
ξ Cygni is in the Kepler spacecraft's field of view but no planets have been detected.{{cite journal|bibcode=2013MNRAS.434.1422M|title=Atmospheric parameters of 169 F-, G-, K- and M-type stars in the Kepler field|journal=Monthly Notices of the Royal Astronomical Society|volume=434|issue=2|pages=1422|last1=Molenda-Żakowicz|first1=J.|last2=Sousa|first2=S. G.|last3=Frasca|first3=A.|last4=Uytterhoeven|first4=K.|last5=Briquet|first5=M.|last6=Van Winckel|first6=H.|last7=Drobek|first7=D.|last8=Niemczura|first8=E.|last9=Lampens|first9=P.|last10=Lykke|first10=J.|last11=Bloemen|first11=S.|last12=Gameiro|first12=J. F.|last13=Jean|first13=C.|last14=Volpi|first14=D.|last15=Gorlova|first15=N.|last16=Mortier|first16=A.|last17=Tsantaki|first17=M.|last18=Raskin|first18=G.|year=2013|doi=10.1093/mnras/stt1095|doi-access=free |arxiv = 1306.6011 |s2cid=59269553}}
Gallery
{{gallery |align=center
| File:XiCygni JeffJohnson.jpg|H-alpha RGB amateur image of ξ Cygni, center star, at edge of NGC7000
| File:NGC7000 North America Nebula.jpg|NGC 7000 (North America Nebula). ξ Cygni is the bright star on the left.
}}
References
{{reflist|refs=
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{{Stars of Cygnus}}
Category:Cygnus (constellation)
Category:Spectroscopic binaries