Astronomy:Delta Cygni

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Short description: Third-magnitude star in the constellation Cygnus
Delta Cygni
Location of δ Cygni (circled)
Observation data
Equinox J2000.0]] (ICRS)
Constellation Cygnus[1]
Right ascension  19h 44m 58.47854s[2]
Declination +45° 07′ 50.9161″[2]
Apparent magnitude (V) 2.87[3]
Characteristics
Spectral type A0 IV[4] (B9 III + F1 V[5])
U−B color index −0.10[6]
B−V color index −0.02[6]
Variable type Suspected[7]
Astrometry
Radial velocity (Rv)−20.1[8] km/s
Proper motion (μ) RA: +44.07[2] mas/yr
Dec.: +48.66[2] mas/yr
Parallax (π)19.77 ± 0.48[2] mas
Distance165 ± 4 ly
(51 ± 1 pc)
Absolute magnitude (MV)−0.74[1]
Orbit[9]
PrimaryA
CompanionB
Period (P)780.27 yr
Semi-major axis (a)3.0″
Eccentricity (e)0.4670
Details[10]
Mass2.93 M☉
Radius4.81±0.36[11] R☉
Luminosity155 L☉
Surface gravity (log g)3.4±0.25[11] cgs
Temperature10400±400[11] K
Rotational velocity (v sin i)142[11] km/s
Other designations
Fawaris, δ Cyg, 18 Cygni, 18 Cyg, BD+44°3234, GC 27347, HD 186882, HIP 97165, HR 7528, SAO 48796, WDS J19450+4508AB[12]
Database references
SIMBADdata

Delta Cygni is a binary star system of a combined third-magnitude in the northern constellation of Cygnus. It is part of the Northern Cross asterism whose brightest star is Deneb. Its name is a Bayer designation that is Latinized from δ Cygni, and abbreviated Delta Cyg or δ Cyg. Based upon parallax measurements obtained during the Hipparcos mission, Delta Cygni is located roughly 165 light-years (51 parsecs) distant from the Sun.[2]

Delta Cygni's two components are designated Delta Cygni A (officially named Fawaris /fəˈwɛərɪs/)[13] and B. More widely separated is a faint third component, a 12th magnitude star that is moving along with the others. Together they form a triple star system.[14]

Nomenclature

δ Cygni (Latinised to Delta Cygni) is the binary's Bayer designation. The designations of the two components as Delta Cygni A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU).[15]

Traditionally, Delta Cygni had no proper name.[14] It belonged to the Arabic asterism al-Fawāris (الفوارس), meaning "the Riders" in indigenous Arabic,[16] together with Zeta, Epsilon, and Gamma Cygni, the transverse of the Northern Cross. In 2016, the IAU organized a Working Group on Star Names (WGSN)[17] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems.[18] It approved the name Fawaris for the component Delta Cygni A on 1 June 2018 and it is now so included in the List of IAU-approved Star Names.[13]

In Chinese, 天津 (Tiān Jīn), meaning Celestial Ford, refers to an asterism consisting of Delta Cygni, Gamma Cygni, 30 Cygni, Alpha Cygni (Deneb) and Nu, Tau, Upsilon, Zeta and Epsilon Cygni.[19] Consequently, the Chinese name for Delta Cygni itself is 天津二 (Tiān Jīn èr, English: the Second Star of Celestial Ford).[20]

Properties

The primary, Delta Cygni A, is a blue-white giant star of spectral class B9,[5] with a temperature of 10,400 K.[11] It is nearing the end of its main-sequence life stage with a luminosity 155 times that of the Sun,[10] a radius of 4.81 solar radii,[11] and a mass approximately 2.93 solar masses. Like many hot stars, it spins rapidly, at least 135 kilometers per second at the equator, about 60 times that of the Sun.[10]

The close companion Delta Cygni B is a yellow-white F-type main-sequence star of the sixth magnitude (6.33) with a luminosity about 6 times that of the Sun, and a mass about 1.5 times the Sun's. The two stars orbit each other at an average distance of 157 AU and a period of 780 years.[14]

The much more distant third companion is an orange (class K) twelfth magnitude star, and only two thirds as massive.[14]

The two main stars together appear with a spectral type of A0 IV.[4] As seen from Earth, the entire triple star system of Delta Cygni shines at a combined apparent magnitude of 2.87.[3] Both δ Cygni A and B have been suspected to vary in brightness. δ Cygni A was reported in 1951 as varying between magnitudes 2.85 and 2.89, and δ Cygni B was reported in 1837 to vary between magnitudes 6.3 and 8.5. The variability of the stars has not been confirmed.[7]

Pole Star

Main article: Astronomy:Pole star

Delta Cygni is a visible star located within 3° of the precessional path traced across the celestial sphere by the Earth's North pole. For at least four centuries around 11,250 AD it will probably be considered a pole star, a title currently held by Polaris which is just 0.5° off of the precessional path.

Preceded by Pole Star Succeeded by
Deneb ~11,000 AD
to
~11,500 AD 		Vega

References

  1. ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012). "XHIP: An extended hipparcos compilation". Astronomy Letters 38 (5): 331. doi:10.1134/S1063773712050015. Bibcode: 2012AstL...38..331A  XHIP record for this object at VizieR.
  2. ↑ 2.0 2.1 2.2 2.3 2.4 van Leeuwen, F. (November 2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V. 
  3. ↑ 3.0 3.1 Malagnini, M. L.; Morossi, C. (November 1990). "Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars". Astronomy and Astrophysics Supplement Series 85 (3): 1015–1019. Bibcode: 1990A&AS...85.1015M. 
  4. ↑ 4.0 4.1 Zorec, J. et al. (July 2009). "Fundamental parameters of B supergiants from the BCD system. I. Calibration of the (λ_1, D) parameters into Teff". Astronomy and Astrophysics 501 (1): 297–320. doi:10.1051/0004-6361/200811147. Bibcode: 2009A&A...501..297Z. 
  5. ↑ 5.0 5.1 Edwards, T. W. (April 1976). "MK classification for visual binary components". Astronomical Journal 81: 245–249. doi:10.1086/111879. Bibcode: 1976AJ.....81..245E. 
  6. ↑ 6.0 6.1 Johnson, H. L. et al. (1966). "UBVRIJKL photometry of the bright stars". Communications of the Lunar and Planetary Laboratory 4 (99): 99. Bibcode: 1966CoLPL...4...99J. 
  7. ↑ 7.0 7.1 Samus, N. N. et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S 1: B/GCVS. Bibcode: 2009yCat....102025S. 
  8. ↑ Evans, D. S. (June 20–24, 1966). Batten, Alan Henry; Heard, John Frederick. eds. "The Revision of the General Catalogue of Radial Velocities". Determination of Radial Velocities and Their Applications, Proceedings from IAU Symposium No. 30 30: 57. Bibcode: 1967IAUS...30...57E. 
  9. ↑ Malkov, O. Yu. et al. (October 2012). "Dynamical masses of a selected sample of orbital binaries". Astronomy & Astrophysics 546: 5. doi:10.1051/0004-6361/201219774. A69. Bibcode: 2012A&A...546A..69M. 
  10. ↑ 10.0 10.1 10.2 Challouf, M. et al. (2014). "Improving the surface brightness-color relation for early-type stars using optical interferometry⋆". Astronomy & Astrophysics 570: A104. doi:10.1051/0004-6361/201423772. Bibcode: 2014A&A...570A.104C. 
  11. ↑ 11.0 11.1 11.2 11.3 11.4 11.5 Gordon, Kathryn D. et al. (2019). "Angular Sizes, Radii, and Effective Temperatures of B-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal 873 (1): 91. doi:10.3847/1538-4357/ab04b2. Bibcode: 2019ApJ...873...91G. 
  12. ↑ "del Cyg". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=del+Cyg. 
  13. ↑ 13.0 13.1 "Naming Stars". IAU.org. https://www.iau.org/public/themes/naming_stars/. 
  14. ↑ 14.0 14.1 14.2 14.3 Kaler, James B.. "Delta Cygni". Stars. University of Illinois. http://stars.astro.illinois.edu/sow/deltacyg.html. 
  15. ↑ Hessman, F. V.; et al. (2010). "On the naming convention used for multiple star systems and extrasolar planets". arXiv:1012.0707 [astro-ph.SR].
  16. ↑ Allen, R. H. (1963). Star Names: Their Lore and Meaning (Reprint ed.). New York, NY: Dover Publications Inc.. p. 193, 197. ISBN ((978-0-486-21079-7)). https://archive.org/details/starnamestheirlo00alle/page/193. 
  17. ↑ "IAU Working Group on Star Names (WGSN)". International Astronomical Union. https://www.iau.org/science/scientific_bodies/working_groups/280/. 
  18. ↑ "WG Triennial Report (2015-2018) - Star Names". 2018. p. 5. https://www.iau.org/static/science/scientific_bodies/working_groups/280/wg-starnames-triennial-report-2015-2018.pdf. 
  19. ↑ (in Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
  20. ↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 4 日



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