HD 23089

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HD 23089
Observation data
Epoch J2000      Equinox J2000
Constellation Camelopardalis[1]
Right ascension 03h 46m 02.33087s[2]
Declination +63° 20 42.1639[2]
Apparent magnitude (V) 4.79[3]
Characteristics
Spectral type G2II-III + B9V[4]
U−B color index +0.24[3]
B−V color index +0.79[3]
R−I color index 0.53
Astrometry
Radial velocity (Rv)-2.4[5] km/s
Proper motion (μ) RA: -0.94[2] mas/yr
Dec.: -8.41[2] mas/yr
Parallax (π)4.08±0.66 mas[2]
Distanceapprox. 800 ly
(approx. 250 pc)
Absolute magnitude (MV)−2.70  −1.50[6]
Orbit[6]
Period (P)6,124±3 d
Eccentricity (e)0.678±0.003
Inclination (i)87±4°
Periastron epoch (T)MJD45850±3
Argument of periastron (ω)
(secondary)
136.5±0.6°
Semi-amplitude (K1)
(primary)
15.87±0.08 km/s
Semi-amplitude (K2)
(secondary)
17.6±0.34 km/s
Details
HD 23089 A
Mass5.0±0.24[6] M
Radius41±7.3[6] R
Luminosity1,150[6] L
Surface gravity (log g)2.88[7] cgs
Temperature5,250[6] K
Metallicity [Fe/H]−0.28[7] dex
HD 23089 B
Mass4.5±0.21[6] M
Radius5.3±0.9[6] R
Luminosity708[6] L
Temperature13,000±300[6] K
Rotational velocity (v sin i)18[8] km/s
Other designations
BD+62°604, HD 23089, HIP 17587, HR 1129, SAO 12891
Database references
SIMBADdata

HD 23089 is a spectroscopic binary[6] star in the northern constellation of Camelopardalis. Based on stellar parallax measurements made by Hipparcos, the system is about 800 ly (250 pc) away from the Sun.[2]

The system consists of a cooler giant star and hotter main sequence companion.[4] The pair orbit each other every 6,124 days, on an orbit that is relatively eccentric, at 0.678. Unpublished speckle observations suggest that the orbit is tilted towards the Earth's line of sight, and it has a relatively high inclination of about 87 degrees.[6]

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