Location of 56 Cygni (circled) in front of the Pelican Nebula | |
| Observation data Epoch J2000 Equinox ICRS | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 20h 50m 04.93165s |
| Declination | +44° 03′ 33.4916″ |
| Apparent magnitude (V) | 5.06 |
| Characteristics | |
| Evolutionary stage | main sequence |
| Spectral type | A6 V |
| B−V color index | 0.198±0.002 |
| Astrometry | |
| Radial velocity (Rv) | −21.5±3.5 km/s |
| Proper motion (μ) | RA: +123.197 mas/yr Dec.: +132.062 mas/yr |
| Parallax (π) | 24.2284±0.0747 mas |
| Distance | 134.6 ± 0.4 ly (41.3 ± 0.1 pc) |
| Absolute magnitude (MV) | 2.00 |
| Details | |
| Mass | 1.89 M☉ |
| Radius | 1.92 R☉ |
| Luminosity | 12.8 L☉ |
| Surface gravity (log g) | 4.15±0.07 cgs |
| Temperature | 7,895±127 K |
| Rotational velocity (v sin i) | 73 km/s |
| Age | 394 Myr |
| Other designations | |
| 56 Cyg, BD+43°3739, FK5 3666, HD 198639, HIP 102843, HR 7984, SAO 50121, WDS J20501+4404 | |
| Database references | |
| SIMBAD | data |
56 Cygni is a single star in the northern constellation of Cygnus, located 135 light years from Earth. It is visible to the naked eye as a white-hued star with an apparent visual magnitude of 5.06. The star is moving closer to the Earth with a heliocentric radial velocity of −21.5. It has a relatively high proper motion, traversing the celestial sphere at an angular rate of 0.181″/yr. According to Eggen (1998), this is a member of the Hyades Supercluster.
This is an A-type main-sequence star with a stellar classification of A6 V. Cowley et al. (1969) classified it as a Delta Delphini star, which is a type of suspected Am star. The star is around 394 million years old with a projected rotational velocity of 73 km/s. It has 1.9 times the mass of the Sun and is radiating 13 times the Sun's luminosity from its photosphere at an effective temperature of 7,895 K.
56 Cygni has a visual companion: a magnitude 11.9 star at an angular separation of 55.4″ along a position angle of 48°, as of 2015.