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Chi Cygni information


χ Cygni
Location of χ Cygni (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 19h 50m 33.92439s[1]
Declination +32° 54′ 50.6097″[1]
Apparent magnitude (V) 3.3 – 14.2[2]
Characteristics
Spectral type S6+/1e = MS6+[3] (S6,2e – S10,4e[4])
U−B color index −0.30 – +0.98[5]
B−V color index +1.56 – +2.05[5]
Variable type Mira[2]
Astrometry
Radial velocity (Rv)+1.60[6] km/s
Proper motion (μ) RA: -20.16[1] mas/yr
Dec.: -38.34[1] mas/yr
Parallax (π)5.53 ± 1.10 mas[1]
Distance553 ly
(169[7] pc)
Absolute magnitude (MV)−3.2 – +7.7[8]
Details
Mass2.1+1.5
−0.7
[7] M
Radius348 – 480[7] R
Luminosity6,000 – 9,000[7] L
Surface gravity (log g)0.49[9] cgs
Temperature2,441 – 2,742[7] K
Metallicity [Fe/H]-1.00[9] dex
Other designations
χ Cyg, Chi Cyg, HD 187796, BD+32°3593, HIP 97629, HR 7564, SAO 68943
Database references
SIMBADdata

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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Chi Cygni

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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...

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35 HD 84810 Star 4.07 3.48 Delta Cephei Quadruple star system 4.24 3.3 Chi Cygni Star 4.97 3.5 R Hydrae Star 5.68 5.38 Uranus Planet 6.53 2.0 Mira Binary...

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S5. The non-standard designation S10 has only been used for the star Chi Cygni when at an extreme minimum. The basic classification is usually followed...

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Mira variable

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days) Distance (in parsecs) Reference Mira 2.0 10.1 332 92+12 −9 [1] Chi Cygni 3.3 14.2 408 180+45 −30 [2] R Hydrae 3.5 10.9 380 224+56 −37 [3] R Carinae...

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notices that Algol's brightness varies 1686 — Gottfried Kirch notices that Chi Cygni's brightness varies 1718 — Edmund Halley discovers stellar proper motions...

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John Goodricke gave the correct explanation of its variability in 1784. Chi Cygni was identified in 1686 by G. Kirch, then R Hydrae in 1704 by G. D. Maraldi...

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technology involved some significant events. Gottfried Kirch notices that Chi Cygni's brightness varies. John Ray begins publication of his Historia Plantarum...

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Y.; Bechis, K. P. (November 1977). "Variable 2.5 mm CO emission from chi Cygni and Mira". Astrophysical Journal. 218 (L27–L30): L27. Bibcode:1977ApJ...

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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...

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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...

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