HD 222109

HD 222109 is a binary star system located in the northern constellation of Andromeda. It has a combined apparent visual magnitude of 5.80, which allows it to be visible to the naked eye as a single star. The system has a combined spectral classification of B8V. It is situated at a distance of approximately 800 light years from the Solar System, 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. Individually, the stars have apparent magnitudes of 6.08 and 7.38, respectively.

HD 222109
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension 23h 37m 32.04280s
Declination +44° 25 44.3723
Apparent magnitude (V) 5.80 (6.08 + 7.38)
Characteristics
Spectral type B8V
U−B color index -0.32
B−V color index -0.06
Astrometry
Radial velocity (Rv)−22.90±3.9 km/s
Proper motion (μ) RA: 14.20±0.30 mas/yr
Dec.: −17.63±0.45 mas/yr
Parallax (π)4.04 ± 0.52 mas
Distanceapprox. 800 ly
(approx. 250 pc)
Orbit
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
Mass2.9 M
Surface gravity (log g)3.932±0.021 cgs
Temperature12,157±100 K
Rotational velocity (v sin i)158±13 km/s
Age54 Myr
Other designations
BD+43° 4508, HD 222109, HIP 116582, HR 8962, SAO 53202.
Database references
SIMBADdata
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