Epoch J2000.0 Equinox J2000.0 (ICRS)
|Right ascension||19h 30m 43.286s|
|Declination||+27° 57′ 34.84″|
|Apparent magnitude (V)||3.18|
|Right ascension||19h 30m 43.295s|
|Declination||+27° 57′ 34.62″|
|Apparent magnitude (V)||5.82|
|Right ascension||19h 30m 45.3954s|
|Declination||+27° 57′ 54.995″|
|Apparent magnitude (V)||5.09|
|B−V color index||1.074|
|V−R color index||0.92|
|B−V color index||0.09|
|V−R color index||0.09|
|U−B color index||-0.30|
|B−V color index||-0.06|
|Radial velocity (Rv)||-24.07 km/s|
|Proper motion (μ)||RA: -7.17 mas/yr
Dec.: -6.15 mas/yr
|Parallax (π)||7.51 ± 0.33[a] mas|
|Distance||430 ± 20 ly
(133 ± 6 pc)
|Absolute magnitude (MV)||−2.45|
|Absolute magnitude (MV)||−0.25|
|Radial velocity (Rv)||-18 km/s|
|Proper motion (μ)||RA: -1.95 mas/yr
Dec.: -0.98 mas/yr
|Parallax (π)||8.16 ± 0.25[a] mas|
|Distance||400 ± 10 ly
(123 ± 4 pc)
|Period (P)||213.859 yr|
|Semi-major axis (a)||0.536″|
|Longitude of the node (Ω)||170.4°|
|Periastron epoch (T)||B1997.995|
|Argument of periastron (ω)
|Luminosity (bolometric)||1,200 L☉|
|Luminosity (bolometric)||230 L☉|
|Mass||3.7 ± 0.8 M☉|
|Luminosity (bolometric)||230 ± 90 L☉|
|Surface gravity (log g)||4.00 ± 0.15 cgs|
|Temperature||13200 ± 600 K|
|Age||4×107 to 2×108  years|
|Position (relative to Albireo A)|
|Epoch of observation||2006|
|Angular distance||35.3″ |
|Position angle||54° |
|AlbireoA: β¹ Cygni, BD+27 3410, HR 7417, HD 183912/183913, HIP 95947, SAO 87301, FK5 732, MCA 55 Aac, NSV 12105|
|AlbireoB: β² Cygni, STF 4043B, BD+27 3411, HD 183914, HIP 95951, HR 7418, SAO 87302|
Albireo is the traditional name for the double star also designated Beta Cygni (β Cygni, abbreviated Beta Cyg, β Cyg), although the International Astronomical Union now regards the name as only applying to the brightest component. Despite being designated 'beta', it is fainter than Gamma Cygni, Delta Cygni, and Epsilon Cygni and is the fifth brightest point of light in the constellation of Cygnus. Appearing to the naked eye to be a single star of magnitude 3, viewing through even a low magnification telescope resolves it into its two components. The brighter yellow star (actually itself a very close binary system) makes a striking colour contrast with its fainter blue companion.
The system's traditional name Albireo is a result of misunderstanding and mistranslation. It is thought that it originated in the Greek name ornis for the constellation of Cygnus, which became urnis in Arabic. When translated into Latin, this name was thought to refer to the plant Sisymbrium officinale, and so was translated into a Latin name for this plant, ireo. The phrase ab ireo was later treated as a misprint of an Arabic term and transcribed as al-bireo.
In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Albireo for β¹ Cygni. It is now so entered in the IAU Catalog of Star Names.
Medieval Arabic-speaking astronomers called Beta Cygni minqār al-dajājah (English: the hen's beak). The term minqār al-dajājah (منقار الدجاجة) or Menchir al Dedjadjet appeared in the catalogue of stars in the Calendarium of Al Achsasi Al Mouakket, which was translated into Latin as Rostrum Gallinǣ, meaning the hen's beak.
Since Cygnus is the swan, and Beta Cygni is located at the head of the swan, it is sometimes called the "beak star". With Deneb, Gamma Cygni (Sadr), Delta Cygni, and Epsilon Cygni (Gienah), it forms the asterism called the Northern Cross.
When viewed with the naked eye, it appears to be a single star. However, in a telescope it readily resolves into a double star, consisting of Beta Cygni A (amber, apparent magnitude 3.1), and Beta Cygni B (blue-green, apparent magnitude 5.1). Separated by 35 seconds of arc, the two components provide one of the best contrasting double stars in the sky due to their different colors. It is not known whether the two components are orbiting around each other in a physical binary system. If they are, their orbital period is probably at least 100,000 years.
Beta Cygni A
The spectrum of Beta Cygni A was found to be composite when it was observed as part of the Henry Draper Memorial project in the late 19th century, leading to the supposition that it was itself double. This was supported by observations from 1898 to 1918 which showed that it had a varying radial velocity. In 1923, the components now called Beta Cygni Aa and Beta Cygni Ac were identified in the Henry Draper Catalogue as HD 183912 and HD 183913 respectively. In 1976 speckle interferometry was used to resolve the pair at the 2.1-meter telescope at the Kitt Peak National Observatory. It is also listed in the Washington Double Star Catalog. An orbit for the pair has since been computed using interferometric measurements, but as only approximately a quarter of the orbit has been observed, the orbital parameters must be regarded as preliminary. The period of this orbit is 213 years. The current angular separation between the components is around 0.4 arcseconds, too close to be visually resolved except with instruments of at least 20" in aperture with exceptionally stable atmospheric conditions.
Beta Cygni B
Beta Cygni B is a fast-rotating Be star, with an equatorial rotational velocity of at least 250 kilometers per second. Its surface temperature has been spectroscopically estimated to be about 13,200 K.
- The primary and secondary have different formal Hipparchos parallaxes. They are thought to be physically related and so at the same distance from Earth in astronomical terms, hence one or both derived distances are somewhat in error.
- , Hipparcos catalogue; CDS.
- Binary Star Differential Photometry Using the Adaptive Optics System at Mount Wilson Observatory, Theo ten Brummelaar, Brian D. Mason, et al., Astronomical Journal 119, #5 (May 2000), pp. 2403–2414. doi:10.1086/301338. Bibcode: 2000AJ....119.2403T . See tables 4, 5, 6, and 8. Luminosity from Lbol=102(4.75−Mbol)/5.
- , Hipparcos catalogue; CDS.
- HD 183914 -- Emission-line Star, database entry, SIMBAD. Accessed on line July 9, 2008.
- Ginestet, N.; Carquillat, J. M. (2002). "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". The Astrophysical Journal Supplement Series. 143 (2): 513. Bibcode:2002ApJS..143..513G. doi:10.1086/342942.
- UBV observations of visual double stars, T. E. Lutz, Publications of the Astronomical Society of the Pacific 83 (August 1971), pp. 488–490. Bibcode: 1971PASP...83..488L .
- NAME ALBIREO -- Star in double system , database entry, SIMBAD. Accessed on line July 9, 2008.
- Entry, WDS identifier 19307+2758, Sixth Catalog of Orbits of Visual Binary Stars, William I. Hartkopf & Brian D. Mason, U.S. Naval Observatory. Accessed on line July 9, 2008. (19307+2758)
- Albireo, Stars, Jim Kaler. Accessed on line October 23, 2013.
- Table 1, Physical Parameters of Southern B- and Be-Type Stars, R. S. Levenhagen and N. V. Leister, The Astronomical Journal 127, #2 (February 2004), pp. 1176–1180, doi:10.1086/381063, Bibcode: 2004AJ....127.1176L .
- Entry, HD 183914, Catalogue of Stellar Diameters (CADARS); CDS ID II/224.
- Entry, The Washington Double Star Catalog, identifier 19307+2758, discoverer identifier STFA 43. Accessed on line July 9, 2008. Archived 8 September 2008 at the Wayback Machine.
- Speckle observations with PISCO in Merate: IV. Astrometric measurements of visual binaries in 2005, M. Scardia et al., Astronomische Nachrichten 329, #1 (2008), pp. 54–68. Bibcode: 2008AN....329...54S . doi:10.1002/asna.200710834.
- "IAU Catalog of Star Names". Retrieved 28 July 2016.
- p. 24, The names of the stars and constellations compiled from the Latin, Greek and Arabic, W. H. Higgins, Leicester: Samuel Clarke, 1882.
- p. 194, Allen.
- "IAU Working Group on Star Names (WGSN)". Retrieved 22 May 2016.
- "Bulletin of the IAU Working Group on Star Names, No. 1" (PDF). Retrieved 28 July 2016.
- p. 196, Star-names and Their Meanings, Richard Hinckley Allen, New York, G. E. Stechert, 1899.
- Knobel, E. B. (June 1895). "Al Achsasi Al Mouakket, on a catalogue of stars in the Calendarium of Mohammad Al Achsasi Al Mouakket". Monthly Notices of the Royal Astronomical Society. 55 (8): 429. Bibcode:1895MNRAS..55..429K. doi:10.1093/mnras/55.8.429.
- p. 416, In Quest of the Universe, Theo Koupelis and Karl F. Kuhn, 5th ed., Sudbury, Massachusetts: Jones & Bartlett Publishers, 2007, ISBN 0-7637-4387-9.
- Northern Cross, entry, The Internet Encyclopedia of Science, David Darling. Accessed on line July 24, 2008.
- p. 46, The Monthly Sky Guide, Ian Ridpath, Wil Tirion, Cambridge University Press, 2006, ISBN 0-521-68435-8.
- note 145, p. 99, "Spectra of bright stars photographed with the 11-inch Draper Telescope as part of the Henry Draper Memorial", Antonia C. Maury and Edward C. Pickering, Annals of the Astronomical Observatory of Harvard College 28 (1897), pp. 1-128, Bibcode: 1897AnHar..28....1M .
- "The Variable Velocity of β Cygni", W. W. Campbell, Publications of the Astronomical Society of the Pacific 31, #179, pp. 38-39, Bibcode: 1919PASP...31...38C .
- freestarcharts dot com
- p. 251, "The Henry Draper Catalogue: 19h and 20h", Annie J. Cannon & Edward C. Pickering, Annals of the Astronomical Observatory of Harvard College 98 (1923), Bibcode: 1923AnHar..98....1C . See note re HD 183912,3,4 on this page.
- Speckle interferometric measurements of binary stars. VI, H. A. McAlister and E. M. Hendry, Astrophysical Journal Supplement Series 48 (March 1982), pp. 273–278. Bibcode: 1982ApJS...48..273M . doi:10.1086/190778.
- Webb, T. W.; McAlister, H. A.; Worley, C. E.; Burnham, S. W.; Aitken, R. G. (1980). "Albireo as a Triple Star". Sky and Telescope. 59: 210. Bibcode:1980S&T....59..210W.
- Photo by Richard Yandrick; August 30, 2005
- A picture of Albireo by Stefan Seip
- Albireo at Pete Roberts' Fuzzy Blobs site
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