Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 23h 37m 32.04280s[1] |
Declination | +44° 25′ 44.3723″[1] |
Apparent magnitude (V) | 5.80[2] (6.08 + 7.38)[3] |
Characteristics | |
Spectral type | B8V[4] |
U−B color index | -0.32[2] |
B−V color index | -0.06[2] |
Astrometry | |
Radial velocity (Rv) | −22.90±3.9[5] km/s |
Proper motion (μ) | RA: 14.20±0.30[1] mas/yr Dec.: −17.63±0.45[1] mas/yr |
Parallax (π) | 4.04 ± 0.52 mas[1] |
Distance | approx. 800 ly (approx. 250 pc) |
Orbit[6] | |
Period (P) | 351.22 yr |
Semi-major axis (a) | 0.41″ |
Eccentricity (e) | 0.39 |
Inclination (i) | 40.3° |
Longitude of the node (Ω) | 157.1° |
Periastron epoch (T) | B 2103.29 |
Argument of periastron (ω) (secondary) | 0.0° |
Details | |
Mass | 2.9[7] M☉ |
Surface gravity (log g) | 3.932±0.021[8] cgs |
Temperature | 12,157±100[8] K |
Rotational velocity (v sin i) | 158±13[8] km/s |
Age | 54[7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 222109 is a binary star system located in the northern constellation of Andromeda. It has a combined apparent visual magnitude of 5.80,[2] which allows it to be visible to the naked eye as a single star. The system has a combined spectral classification of B8V.[4] It is situated at a distance of approximately 800 light years from the Solar System,[1] and the two stars orbit each other with a period of 351.22 years. They are separated by a distance of 0.41″ and have an orbital eccentricity of 0.39.[3] Individually, the stars have apparent magnitudes of 6.08 and 7.38, respectively.[3]
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