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29 Cygni

From Wikipedia, the free encyclopedia
A-type main sequence star in the constellation Cygnus
This article is about b3 Cygni. For other stars with thisBayer designation, seeb Cygni.
29 Cygni
Location of 29 Cygni (circled in red)
Observation data
Epoch J2000      Equinox J2000
ConstellationCygnus
Right ascension20h 14m 32.03235s[1]
Declination+36° 48′ 22.7009″[1]
Apparent magnitude (V)4.94 - 4.97[2]
Characteristics
Evolutionary stagemain sequence[3][4]
Spectral typeA2 V[5]
B−Vcolor index0.151±0.018[6]
Variable typeδ Sct[7]
Astrometry
Radial velocity (Rv)−17.30±2.80[6] km/s
Proper motion (μ)RA: +68.391[1]mas/yr
Dec.: +70.446[1]mas/yr
Parallax (π)24.5456±0.0724 mas[1]
Distance132.9 ± 0.4 ly
(40.7 ± 0.1 pc)
Absolute magnitude (MV)1.78[6]
Details
Mass1.67–1.75[4] M
Radius1.942±0.055[8] R
Luminosity25.2+3.7
−3.1
[3] L
Surface gravity (log g)4.14±0.08[8] cgs
Temperature8,774±113[9] K
Rotational velocity (v sin i)65[3] km/s
Age28+15
−14
or119+37
−10
[10] Myr
Other designations
b3 Cygni,29 Cyg,V1644 Cygni,BD+36°3955,HD 192640,HIP 99770,HR 7736,SAO 69678,WDS J20145+3648A,2MASS J20143203+3648225[11]
Database references
SIMBADdata
Exoplanet Archivedata

29 Cygni is a single[12]star in the northernconstellation ofCygnus. It is dimly visible to the naked eye as a white-hued star with anapparent visual magnitude of 4.93.[6] The distance to 29 Cyg, as estimated from an annualparallax shift of24.5 mas, is 133 light years. The star is moving closer to the Earth with a heliocentricradial velocity of −17 km/s.[6] It is a member of the 30–50 million year oldArgus Association of co-moving stars.[13]

A yellow-lightlight curve for V1644 Cygni, adapted from Gies and Percy (1977)[14]

This is anA-type main-sequence star with astellar classification of A2 V.[5] Rodríguez et al. (2000) classify it as aDelta Scuti variable with afrequency of 0.0267 cycles per day.[7] It is aLambda Boötis[15] classchemically peculiar star and the first such star to be classified as apulsating variable.[4] 29 Cyg is multi-periodic,[16] small-amplitude variable with a magnitude change of about 0.02 and a dominant period of 39 minutes.[4] Amagnetic field has been detected with an averaged quadratic field of(194.5±230.7)×10−4 T.[17] The star has a moderate rate of rotation,[4] showing aprojected rotational velocity of 65 km/s.[3] It has 1.67 to 1.75 themass of the Sun,[4] 1.942 times theSun's radius,[8] is radiating 25 times theSun's luminosity from itsphotosphere[3] at aneffective temperature of roughly 8,774 K.[9]

29 Cygni is listed inmultiple star catalogs as having several companions within4, including the yellow 7th magnitude HD 192661. All are background objects not physically associated with 29 Cygni itself.[18][1] The naked-eye starsb1 Cygni andb2 Cygni, respectively about one and two degrees away, also lie at different distances to 29 Cygni.

Substellar companion

[edit]
Direct imaging of 29 Cygni b by theSubaru Telescope.

In 2022, asuperjovian planet,HIP 99770 b, was discovered by direct imaging andastrometry. Its spectral class is between L7 and L9.5, corresponding to a surface temperature of 1,400±100K.[19]

The 29 Cygni planetary system[20]
Companion
(in order from star)
MassSemimajor axis
(AU)
Orbital period
(years)
EccentricityInclinationRadius
b13.1+4.8
−5.2
 MJ
15.7+3.5
−1.0
47+14
−4
0.31+0.06
−0.12
[10]
151.3+8.4
−12.0
°
1.056 RJ

References

[edit]
  1. ^abcdefVallenari, A.; et al. (Gaia collaboration) (2023)."Gaia Data Release 3. Summary of the content and survey properties".Astronomy and Astrophysics.674: A1.arXiv:2208.00211.Bibcode:2023A&A...674A...1G.doi:10.1051/0004-6361/202243940.S2CID 244398875. Gaia DR3 record for this source atVizieR.
  2. ^Samus, N. N.; Durlevich, O. V.; 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.
  3. ^abcdeZorec, J.; Royer, F. (2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities",Astronomy & Astrophysics,537: A120,arXiv:1201.2052,Bibcode:2012A&A...537A.120Z,doi:10.1051/0004-6361/201117691,S2CID 55586789, A120.
  4. ^abcdefCasas, R.; et al. (May 2009), "Asteroseismological Modeling of the Multiperiodic λ Bootis Star 29 Cygni",The Astrophysical Journal,697 (1):52–534,Bibcode:2009ApJ...697..522C,doi:10.1088/0004-637X/697/1/522,hdl:10481/41210,S2CID 120924176
  5. ^abCowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications",Astronomical Journal,74:375–406,Bibcode:1969AJ.....74..375C,doi:10.1086/110819.
  6. ^abcdeAnderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation",Astronomy Letters,38 (5): 331,arXiv:1108.4971,Bibcode:2012AstL...38..331A,doi:10.1134/S1063773712050015,S2CID 119257644.
  7. ^abRodríguez, E.; et al. (June 2000), "A revised catalogue of delta Sct stars",Astronomy and Astrophysics Supplement,144 (3):469–474,Bibcode:2000A&AS..144..469R,doi:10.1051/aas:2000221,hdl:10261/226673.
  8. ^abcStassun, Keivan G.; Oelkers, Ryan J.; Paegert, Martin; Torres, Guillermo; Pepper, Joshua; De Lee, Nathan; Collins, Kevin; Latham, David W.; Muirhead, Philip S.; Chittidi, Jay; Rojas-Ayala, Bárbara; Fleming, Scott W.; Rose, Mark E.; Tenenbaum, Peter; Ting, Eric B. (2019-10-01), "The Revised TESS Input Catalog and Candidate Target List",The Astronomical Journal,158 (4): 138,arXiv:1905.10694,Bibcode:2019AJ....158..138S,doi:10.3847/1538-3881/ab3467,ISSN 0004-6256
  9. ^abPrugniel, Ph.; Vauglin, I.; Koleva, M. (2011), "The atmospheric parameters and spectral interpolator for the MILES stars",Astronomy and Astrophysics,531: A165,arXiv:1104.4952,Bibcode:2011A&A...531A.165P,doi:10.1051/0004-6361/201116769
  10. ^abWinterhalder, T. O.; Kammerer, J.; Lacour, S.; Mérand, A.; Nowak, M.; Stolker, T.; Balmer, W. O.; Marleau, G.-D.; Abuter, R.; Amorim, A.; Asensio-Torres, R.; Berger, J.-P.; Beust, H.; Blunt, S.; Bonnefoy, M. (2025-06-27), "Orbit and atmosphere of HIP 99770 b through the eyes of VLTI/GRAVITY",Astronomy & Astrophysics,700: A4,arXiv:2507.00117,Bibcode:2025A&A...700A...4W,doi:10.1051/0004-6361/202554766,ISSN 0004-6361
  11. ^"29 Cyg".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved2019-01-13.
  12. ^De Rosa, R. J.; et al. (2014), "The VAST Survey - III. The multiplicity of A-type stars within 75 pc",Monthly Notices of the Royal Astronomical Society,437 (2): 1216,arXiv:1311.7141,Bibcode:2014MNRAS.437.1216D,doi:10.1093/mnras/stt1932,S2CID 88503488.
  13. ^Malo, Lison; et al. (January 2013), "Bayesian Analysis to Identify New Star Candidates in Nearby Young Stellar Kinematic Groups",The Astrophysical Journal,762 (2): 50,arXiv:1209.2077,Bibcode:2013ApJ...762...88M,doi:10.1088/0004-637X/762/2/88,S2CID 118497872, 88.
  14. ^Gies, Douglas R.; Percy, John R. (February 1977)."Photometric variability of 29 Cygni".The Astronomical Journal.82 (2):166–168.Bibcode:1977AJ.....82..166G.doi:10.1086/112023.
  15. ^Murphy, Simon J.; et al. (October 2015), "An Evaluation of the Membership Probability of 212 λ Boo Stars. I. A Catalogue",Publications of the Astronomical Society of Australia,32 e036: 43,arXiv:1508.03633,Bibcode:2015PASA...32...36M,doi:10.1017/pasa.2015.34,S2CID 59405545, e036
  16. ^Mkrtichian, D. E.; et al. (October 2007), "Multimode Pulsations of the λ Bootis Star 29 Cygni: The 1995 and 1996 Multisite Campaigns",The Astronomical Journal,134 (4): 1713,Bibcode:2007AJ....134.1713M,doi:10.1086/521434.
  17. ^Bychkov, V. D.; et al. (August 2003), "Catalogue of averaged stellar effective magnetic fields. I. Chemically peculiar A and B type stars",Astronomy and Astrophysics,407 (2):631–642,arXiv:astro-ph/0307356,Bibcode:2003A&A...407..631B,doi:10.1051/0004-6361:20030741,S2CID 14184105.
  18. ^Mason, Brian D.; Wycoff, Gary L.; Hartkopf, William I.; Douglass, Geoffrey G.; Worley, Charles E. (2001), "The 2001 US Naval Observatory Double Star CD-ROM. I. The Washington Double Star Catalog",The Astronomical Journal,122 (6): 3466,Bibcode:2001AJ....122.3466M,doi:10.1086/323920.
  19. ^Currie, Thayne; et al. (2023), "Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star",Science,380 (6641):198–203,arXiv:2212.00034,doi:10.1126/science.abo6192,PMID 37053312
  20. ^Bovie, Danielle; Currie, Thayne; Morsy, Mona El; Lacy, Brianna; Kuzuhara, Masayuki; Chilcote, Jeffrey; Tobin, Taylor; Guyon, Olivier; Groff, Tyler (2025-09-02), "Multi-band Spectral and Astrometric Characterization of the HIP 99770 b Planet with SCExAO/CHARIS and Gaia",The Astronomical Journal,arXiv:2509.02665.
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