HD 185269
HD 185269 is a stellar triple system approximately 170 light-years away in the constellation Cygnus. It is easily visible to binoculars, but not the naked eye.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 37m 11.7411s |
| Declination | +28° 29′ 59.5025″ |
| Apparent magnitude (V) | 6.67 |
| Characteristics | |
| Spectral type | G0IV |
| B−V color index | 0.58 |
| Astrometry | |
| Proper motion (μ) | RA: −31.499±0.045 mas/yr Dec.: −80.782±0.046 mas/yr |
| Parallax (π) | 19.2049 ± 0.0309 mas |
| Distance | 169.8 ± 0.3 ly (52.07 ± 0.08 pc) |
| Absolute magnitude (MV) | 3.29 |
| Absolute bolometric magnitude (Mbol) | 3.228 |
| Details | |
| Mass | 1.33 ± 0.07 M☉ |
| Surface gravity (log g) | 4.05 ± 0.22 cgs |
| Temperature | 5983 ± 62 K |
| Metallicity [Fe/H] | 0.10 ± 0.08 dex |
| Rotational velocity (v sin i) | 5.5 km/s |
| Age | 4.0 ± 1.0 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Exoplanet Archive | data |
The primary star is a third more massive and four times more luminous than the Sun. The spectrum of the star is G0IV. About 4.5 arcseconds away are the two other stars, which are much less massive than the Sun. The primary has a mass of 0.165 M☉, while the secondary has a mass of 0.154 M☉.
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