9 Cygni
{{short description|Star in the constellation Cygnus}}
{{Starbox begin}}
{{Starbox observe
|epoch=J2000
|constell=Cygnus
|ra={{RA|19|34|50.9285}}{{cite DR2}}
|appmag_v=5.39{{cite journal|bibcode=2002ApJS..143..513G|doi=10.1086/342942|title=Spectral Classification of the Hot Components of a Large Sample of Stars with Composite Spectra, and Implication for the Absolute Magnitudes of the Cool Supergiant Components|year=2002|last1=Ginestet|first1=N.|last2=Carquillat|first2=J. M.|journal=The Astrophysical Journal Supplement Series|volume=143|issue=2|pages=513–537|doi-access=free}} {{nowrap|(5.9 + 6.4){{cite web|url=http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6|title=Sixth Catalog of Orbits of Visual Binary Stars|publisher=United States Naval Observatory|access-date=2020-02-29|archive-date=2017-08-01|archive-url=https://web.archive.org/web/20170801102553/http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6|url-status=dead}}}}
}}
{{Starbox character
|type=Red clump + main sequence
}}
{{Starbox astrometry
|parallax=5.4904
|p_error=0.0892
}}
{{Starbox orbit
|period=4.56
|axis=0.030
|inclination=114.6
|node=29.3
|periastron=1985.56
|eccentricity=0.82
|periarg=45.5
}}
{{Starbox detail
|component1=9 Cyg A
|metal_fe={{val|-0.260|0.090}}
|component2=9 Cyg B
}}
{{Starbox catalog
|names={{odlist|BD=+29 3651|HIP=96302|HR=7441|SAO=87385}}{{cite simbad|title=* 9 Cyg|access-date=2020-02-28}}
|component1=9 Cyg A
|names1={{odlist|HD=184759}}
|component2=9 Cyg B
|names2={{odlist|HD=184760}}
}}
{{Starbox reference
|Simbad=9+Cyg
}}
{{Starbox end}}
9 Cygni is a binary star system in the northern constellation of Cygnus. 9 Cygni is its Flamsteed designation. The two stars have a combined magnitude of 5.39, so it can be seen with the naked eye under good viewing conditions. Parallax measurements made by Gaia put the star at a distance of around {{val|590|u=light-years}} ({{val|182|u=parsecs}}) away.
The two stars of 9 Cygni are a G-type giant and an A-type star. Both stars are over twice as massive as the Sun. They orbit once every 4.56 years, separated with a semi-major axis of {{val|0.030|u=arcseconds}}. However, the eccentricity is high, at 0.82. The primary is a red clump giant, a star on the cool end of the horizontal branch fusing helium in its core. The secondary star has begun to evolve off the main sequence; it is sometimes classified as a giant star and sometimes as a main-sequence star.
References
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