Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 20h 29m 23.73561s [1] |
Declination | +30° 22′ 06.7968″ [1] |
Apparent magnitude (V) | 4.02 [2] |
Characteristics | |
Evolutionary stage | supergiant [3] |
Spectral type | F5Ib-II [3] |
B−V color index | +0.38 [2] |
Variable type | constant [3] |
Astrometry | |
Radial velocity (Rv) | −18.20 [4] km/s |
Proper motion (μ) |
RA: 6.89
[1]
mas/
yr Dec.: −0.87 [1] mas/ yr |
Parallax (π) | 4.24 ± 0.16 mas [1] |
Distance | 770 ± 30
ly (236 ± 9 pc) |
Absolute magnitude (MV) | −3.32 [5] |
Details | |
Mass | 5.3±0.4 [6] M☉ |
Radius | 27.01+2.51 −1.01 [7] R☉ |
Luminosity | 1,197±90 [7] L☉ |
Surface gravity (log g) | 2.32±0.08 [6] cgs |
Temperature | 6533+126 −283 [7] K |
Metallicity [Fe/H] | 0.00±0.07 [6] dex |
Rotational velocity (v sin i) | 9.5±2.0 [3] km/s |
Age | 85 [6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
41 Cygni is a single [9] star in the northern constellation of Cygnus, located near the southern border with Vulpecula. It is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of 4.02. [2] The star lies at a distance of around 770 light years from the Sun, based on parallax, and is drifting closer with a radial velocity of −18 km/s. [4]
This is a sharp-lined supergiant star [10] with a stellar classification of F5Ib-II. [3] It is 85 [6] million years old with 5.3 [6] times the mass of the Sun and is spinning with a projected rotational velocity of 9.5 km/s. [3] Having exhausted the supply of hydrogen at its core, the star has expanded to 27 [7] times the Sun's radius. It is radiating about 1,200 [7] times the Sun's luminosity from its swollen photosphere at an effective temperature of 6,533 K. [7]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Cygnus |
Right ascension | 20h 29m 23.73561s [1] |
Declination | +30° 22′ 06.7968″ [1] |
Apparent magnitude (V) | 4.02 [2] |
Characteristics | |
Evolutionary stage | supergiant [3] |
Spectral type | F5Ib-II [3] |
B−V color index | +0.38 [2] |
Variable type | constant [3] |
Astrometry | |
Radial velocity (Rv) | −18.20 [4] km/s |
Proper motion (μ) |
RA: 6.89
[1]
mas/
yr Dec.: −0.87 [1] mas/ yr |
Parallax (π) | 4.24 ± 0.16 mas [1] |
Distance | 770 ± 30
ly (236 ± 9 pc) |
Absolute magnitude (MV) | −3.32 [5] |
Details | |
Mass | 5.3±0.4 [6] M☉ |
Radius | 27.01+2.51 −1.01 [7] R☉ |
Luminosity | 1,197±90 [7] L☉ |
Surface gravity (log g) | 2.32±0.08 [6] cgs |
Temperature | 6533+126 −283 [7] K |
Metallicity [Fe/H] | 0.00±0.07 [6] dex |
Rotational velocity (v sin i) | 9.5±2.0 [3] km/s |
Age | 85 [6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
41 Cygni is a single [9] star in the northern constellation of Cygnus, located near the southern border with Vulpecula. It is visible to the naked eye as a faint, yellow-white hued star with an apparent visual magnitude of 4.02. [2] The star lies at a distance of around 770 light years from the Sun, based on parallax, and is drifting closer with a radial velocity of −18 km/s. [4]
This is a sharp-lined supergiant star [10] with a stellar classification of F5Ib-II. [3] It is 85 [6] million years old with 5.3 [6] times the mass of the Sun and is spinning with a projected rotational velocity of 9.5 km/s. [3] Having exhausted the supply of hydrogen at its core, the star has expanded to 27 [7] times the Sun's radius. It is radiating about 1,200 [7] times the Sun's luminosity from its swollen photosphere at an effective temperature of 6,533 K. [7]