χ Cyg, Chi Cyg, HD 187796, BD+32°3593, HIP 97629, HR 7564, SAO 68943
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Chi Cygni (Latinised from χ Cygni) is a Mira variable star in the constellation Cygnus, and also an S-type star. It is around 500 light years away.
χ Cygni is an asymptotic giant branch star, a very cool and luminous red giant nearing the end of its life. It was discovered to be a variable star in 1686 and its apparent visual magnitude varies from as bright as 3.3 to as dim as 14.2, corresponding to a brightness factor of over 20,000. It is only visible to the naked eye for a short period near each maximum.
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ChiCygni (Latinised from χ Cygni) is a Mira variable star in the constellation Cygnus, and also an S-type star. It is around 500 light years away. χ...
35 HD 84810 Star 4.07 3.48 Delta Cephei Quadruple star system 4.24 3.3 ChiCygni Star 4.97 3.5 R Hydrae Star 5.68 5.38 Uranus Planet 6.53 2.0 Mira Binary...
S5. The non-standard designation S10 has only been used for the star ChiCygni when at an extreme minimum. The basic classification is usually followed...
John Goodricke gave the correct explanation of its variability in 1784. ChiCygni was identified in 1686 by G. Kirch, then R Hydrae in 1704 by G. D. Maraldi...
technology involved some significant events. Gottfried Kirch notices that ChiCygni's brightness varies. John Ray begins publication of his Historia Plantarum...
Chi2 Orionis (Chi2 Ori / χ2 Orionis / χ2 Ori) /kaɪ.tuːˈɒraɪ/ is a B-type supergiant star in the constellation of Orion. It has an apparent visual magnitude...
431..773R. doi:10.1051/0004-6361:20042039. ISSN 0004-6361. Data about NML Cygni (IRC +40448) is found here at VizieR. Zhang, B.; Reid, M. J.; Menten, K...
Project A-Ko C-Ko is the Fourth Princess from the Lepton Kingdom of Alpha Cygni and the long-lost daughter of the Fifth Queen. Alessandra Bellagamba Puss...
Meynet, Georges (2014-03-21). "The puzzle of the CNO abundances of {\alpha} Cygni variables resolved by the Ledoux criterion?". Monthly Notices of the Royal...
discovered, it had the highest proper motion of any star known, replacing 61 Cygni in that department. Later it dropped to second place after the discovery...
David F. (September 2015). "A SPECTROSCOPIC ANALYSIS OF THE K0 III BINARY ϵ CYGNI". The Astrophysical Journal. 810 (2): 117. doi:10.1088/0004-637X/810/2/117...
89 and 7.07 in 87 days. This star has been found to display an inverse P Cygni profile, where cold infalling gas on to the star creates redshifted hydrogen...
Vernet, D.; Kaiser, R.; Guerin, W. (2020). "Intensity interferometry of P Cygni in the H α emission line: Towards distance calibration of LBV supergiant...
doi:10.1093/mnras/4.19.168. Bessel, F. W. (1838b). "On the parallax of 61 Cygni". Monthly Notices of the Royal Astronomical Society. 4 (17): 152–161. Bibcode:1838MNRAS...
to the Sun. He also discovered the proper motion of the double star 61 Cygni. The asteroid 1000 Piazzia and a Moon's crater have been christened with...