Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Camelopardalis |
Right ascension | 12h 49m 06.6701s[1] |
Declination | +83° 25′ 04.221″[1] |
Apparent magnitude (V) | 5.92[2] |
Characteristics | |
Spectral type | A0V + A2V[3] |
B−V color index | 0.015±0.004[2] |
Astrometry | |
Radial velocity (Rv) | +1.0[4] km/s |
Proper motion (μ) | RA: −24.013(47) mas/yr[1] Dec.: 18.235(46) mas/yr[1] |
Parallax (π) | 8.0261 ± 0.0401 mas[1] |
Distance | 406 ± 2 ly (124.6 ± 0.6 pc) |
Orbit[5] | |
Period (P) | 3.2865 d |
Eccentricity (e) | 0.0405±0.005 |
Longitude of the node (Ω) | 211.05±0.04° |
Periastron epoch (T) | JD 2424226.669 |
Argument of periastron (ω) (primary) | 211.1° |
Semi-amplitude (K1) (primary) | 108.34±1.05 km/s |
Semi-amplitude (K2) (secondary) | 128.86±1.07 km/s |
Details | |
Ba | |
Radius | 2.88[6] R☉ |
Rotational velocity (v sin i) | 15±12[6] km/s |
Bb | |
Radius | 2.44[6] R☉ |
Rotational velocity (v sin i) | 13±12[6] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 112014 is a star system[7] in the northern constellation of Camelopardalis. It is dimly visible as a point of light with an apparent visual magnitude of 5.92.[2] The distance to this system is approximately 406 light years based on parallax measurements.[1]
The stars HD 112028 and HD 112014 were identified as a double star by F. G. W. Struve in 1820, and are listed as WDS 12492+8325 A and B, respectively, in the Washington Double Star Catalog.[8] The binary nature of component B, or HD 112014, was discovered by J. S. Plaskett in 1919. It is a double-lined spectroscopic binary with an orbital period of 3.29 days and an eccentricity (ovalness) of 0.04.[5] They are separated by 0.0759 AU (11.35 Gm).[6] Both components are A-type main-sequence stars.[3]
Gaia DR3
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