A-type main sequence star in the constellation Cygnus
29 Cygni Location of 29 Cygni (circled in red)
Observation dataEpoch J2000 Equinox J2000 Constellation Cygnus Right ascension 20h 14m 32.03235s [ 1] Declination +36° 48′ 22.7009″[ 1] Apparent magnitude (V)4.94 - 4.97[ 2] Characteristics Evolutionary stage main sequence [ 3] [ 4] Spectral type A2 V[ 5] B−Vcolor index 0.151± 0.018[ 6] Variable type δ 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] Distance 132.9 ± 0.4 ly (40.7 ± 0.1 pc ) Absolute magnitude (MV )1.78[ 6] Details Mass 1.67–1.75[ 4] M ☉ Radius 1.942± 0.055[ 8] R ☉ Luminosity 25.2+3.7 −3.1 [ 3] L ☉ Surface gravity (log g ) 4.14± 0.08[ 8] cgs Temperature 8,774± 113[ 9] K Rotational velocity (v sin i )65[ 3] km/s Age 28+15 −14 or 119+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 SIMBAD data Exoplanet Archive data
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 of 24.5 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 within 4′ , 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]
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