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Star in the constellation Cygnus
Eta Cygni (η Cygni) is a
star in the northern
constellation of
Cygnus . It is visible to the naked eye with an
apparent visual magnitude of 3.889.
[2] The star lies along the main body of the constellation, about midway between
Gamma Cygni and
Albireo .
[8] Based upon an annual
parallax shift of 24.17
mas ,
[1] it is located 135
light years from the
Sun .
At an age of about 3.3
[6] billion years, this is an
evolved
red clump
[9]
giant star with a
stellar classification of K0 III.
[3] It is presently on the
horizontal branch and is generating energy through the nuclear fusion of helium at its core. The star has about 1.59
[6] times the
mass of the Sun and has expanded to 11
[4] It radiates 52.5 times the
solar luminosity from its
outer atmosphere at an
effective temperature of 4,783 K.
[6]
Eta Cygni has five visual companions,
[10] of which only component B appears to be physically associated. This magnitude 12.0 star lies at an
angular separation of 7.80
arc seconds along a
position angle of 206°, as of 2007.
[11]
References
^
a
b
c
d
e
f van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics , 474 (2): 653–664,
arXiv :
0708.1752 ,
Bibcode :
2007A&A...474..653V ,
doi :
10.1051/0004-6361:20078357 ,
S2CID
18759600 .
^
a
b
c
d Oja, T. (August 1986), "UBV photometry of stars whose positions are accurately known. III", Astronomy and Astrophysics Supplement Series , 65 (2): 405–409,
Bibcode :
1986A&AS...65..405O .
^
a
b Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics , 11 : 29–50,
Bibcode :
1973ARA&A..11...29M ,
doi :
10.1146/annurev.aa.11.090173.000333 .
^
a
b
c Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal , 135 (1): 209–231,
Bibcode :
2008AJ....135..209M ,
doi :
10.1088/0004-6256/135/1/209 ,
S2CID
121883397 .
^ Cardini, D. (January 2005), "Mg II chromospheric radiative loss rates in cool active and quiet stars", Astronomy and Astrophysics , 430 : 303–311,
arXiv :
astro-ph/0409683 ,
Bibcode :
2005A&A...430..303C ,
doi :
10.1051/0004-6361:20041440 ,
S2CID
12136256 .
^
a
b
c
d
e
f Luck, R. Earle (September 2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal , 150 (3): 23,
arXiv :
1507.01466 ,
Bibcode :
2015AJ....150...88L ,
doi :
10.1088/0004-6256/150/3/88 ,
S2CID
118505114 , 88.
^
"eta Cyg" .
SIMBAD .
Centre de données astronomiques de Strasbourg . Retrieved 2017-02-19 .
^ Marett-Crosby, Michael (2013),
Twenty-Five Astronomical Observations That Changed the World: And How To Make Them Yourself , The Patrick Moore Practical Astronomy Series,
Springer Science & Business Media , p. 231,
ISBN
978-1461468004 .
^ Puzeras, E.; et al. (October 2010), "High-resolution spectroscopic study of red clump stars in the Galaxy: iron-group elements", Monthly Notices of the Royal Astronomical Society , 408 (2): 1225–1232,
arXiv :
1006.3857 ,
Bibcode :
2010MNRAS.408.1225P ,
doi :
10.1111/j.1365-2966.2010.17195.x ,
S2CID
44228180 .
^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal , 122 (6): 3466–3471,
Bibcode :
2001AJ....122.3466M ,
doi :
10.1086/323920 .
^ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems",
Monthly Notices of the Royal Astronomical Society , 389 (2): 869–879,
arXiv :
0806.2878 ,
Bibcode :
2008MNRAS.389..869E ,
doi :
10.1111/j.1365-2966.2008.13596.x ,
S2CID
14878976 .
External links
Kaler, James B. (September 7, 2012),
"Eta Cygni" , Stars , University of Illinois, retrieved 2017-02-19 .