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Tau Cygni

Tau Cygni AB
Diagram showing star positions and boundaries of the Cygnus constellation and its surroundings
Cercle rouge 100%.svg

Location of τ Cygni (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cygnus
Right ascension 21h 14m 47.4916s
Declination +38° 02′ 43.141″
Apparent magnitude (V) 3.80 / 6.69
Characteristics
Spectral type F2 IV + G0 V
U−B color index +0.03 / +0.09
B−V color index +0.38 / +0.60
Astrometry
Radial velocity (Rv) -21.1 km/s
Proper motion (μ) RA: 195.75 mas/yr
Dec.: 410.03 mas/yr
Parallax (π) 47.80 ± 0.61 mas
Distance 68.2 ± 0.9 ly
(20.9 ± 0.3 pc)
Orbit
Period (P) 810 days
Semi-major axis (a) 0.796 mas
Eccentricity (e) 0.43
Inclination (i) 92.6°
Longitude of the node (Ω) 78.7°
Periastron epoch (T) 2453139.5
Argument of periastron (ω)
(secondary)
90°
Details
τ Cyg A
Mass 1.65 M
Radius 2.48 R
Surface gravity (log g) 3.87 cgs
Temperature 6,600 K
Metallicity [Fe/H] 0.05 dex
τ Cyg B
Mass 1.03 M
Radius 0.93 R
Surface gravity (log g) 4.52 cgs
Temperature 5,670 K
Other designations
τ Cygni, 65 Cygni, BD+37°4240, HD 202444, HIP 104887, HR 8130, SAO 71121, GC 29723, CCDM J21148+3803AB.
Database references
SIMBAD data

Tau Cygni (τ Cyg) is a binary star system in the constellation Cygnus, approximately 69 light years away from Earth. This visual binary system has a period of 49.6 years.

The main star, 4th magnitude GJ 822.1 A, is a yellowish white subgiant star of the spectral type F2IV. It therefore has a surface temperature of 6,000 to 7,500 kelvins and is larger, hotter, and several times as bright as the Sun. Its companion, 6th magnitude GJ 822.1 B, is a yellow main sequence star of the spectral type G0V. It is similar to the Sun in size, surface temperature, and luminosity.



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