| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 44m 16.60522s [1] |
| Declination | +37° 21′ 15.6771″ [1] |
| Apparent magnitude (V) | 4.90 [2] |
| Characteristics | |
| Spectral type | G8 III [2] |
| B−V color index | 0.931 [3] |
| Astrometry | |
| Radial velocity (Rv) | −23.62±0.21 [4] km/s |
| Proper motion (μ) |
RA: +72.660
[1]
mas/
yr Dec.: +35.708 [1] mas/ yr |
| Parallax (π) | 11.0063 ± 0.1188 mas [1] |
| Distance | 296 ± 3
ly (90.9 ± 1.0 pc) |
| Absolute magnitude (MV) | 0.19 [5] |
| Details | |
| Mass | 2.30 [3] M☉ |
| Radius | 12 [4] R☉ |
| Luminosity | 93.3 [3] L☉ |
| Surface gravity (log g) | 2.8 [4] cgs |
| Temperature | 4,920±61 [3] K |
| Metallicity [Fe/H] | −0.14 [4] dex |
| Rotational velocity (v sin i) | 2.8 [4] km/s |
| Age | 1.50 [3] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
15 Cygni is a single [7] star in the northern constellation Cygnus. With an apparent visual magnitude of 4.90, [2] it is a faint star but visible to the naked eye. The distance to 15 Cygni can be estimated from its annual parallax shift of 11.0 mas, [1] which yields a separation of some 296 light years. It is moving closer to the Sun with a heliocentric radial velocity of −23.6 km/s. [4]
This is an aging giant star with a stellar classification of G8 III, [2] having consumed the hydrogen at its core and evolved off the main sequence. It is a red clump giant, [8] which means it is generating energy via helium fusion at its core. The star is 1.50 billion years old with 2.3 times the mass of the Sun, [3] and has expanded to 12 times the Sun's radius. [4] It is radiating 93 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,920 K. [3]
References
- ^ a b c d e f Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv: 1804.09365. Bibcode: 2018A&A...616A...1G. doi: 10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ a b c d Keenan, Philip C.; McNeil, Raymond C. (1989), "The Perkins catalog of revised MK types for the cooler stars", Astrophysical Journal Supplement Series, 71: 245, Bibcode: 1989ApJS...71..245K, doi: 10.1086/191373.
- ^ a b c d e f g Luck, R. Earle (2015), "Abundances in the Local Region. I. G and K Giants", The Astronomical Journal, 150 (3): 88, arXiv: 1507.01466, Bibcode: 2015AJ....150...88L, doi: 10.1088/0004-6256/150/3/88, S2CID 118505114.
- ^ a b c d e f g Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 Hipparcos Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode: 2008AJ....135..209M, doi: 10.1088/0004-6256/135/1/209
- ^ Takeda, Yoichi; et al. (February 2005), "Stellar Parameters and Photospheric Abundances of Late-G Giants: Properties of the Targets of the Okayama Planet Search Program", Publications of the Astronomical Society of Japan, 57 (1): 109–125, Bibcode: 2005PASJ...57..109T, doi: 10.1093/pasj/57.1.109.
- ^ "15 Cyg". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-01-09.
- ^ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, arXiv: 0806.2878, Bibcode: 2008MNRAS.389..869E, doi: 10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ Alves, David R. (August 2000), "K-Band Calibration of the Red Clump Luminosity", The Astrophysical Journal, 539 (2): 732–741, arXiv: astro-ph/0003329, Bibcode: 2000ApJ...539..732A, doi: 10.1086/309278, S2CID 16673121.