Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Andromeda |
Right ascension | 02h 22m 50.30316s[1] |
Declination | +41° 23′ 46.6540″[1] |
Apparent magnitude (V) | 5.81[2] |
Characteristics | |
Spectral type | F0 III–IV[3] |
B−V color index | 0.289±0.006[2] |
Variable type | suspected[4] |
Astrometry | |
Radial velocity (Rv) | −34.5±2.9[5] km/s |
Proper motion (μ) | RA: +74.938[1] mas/yr Dec.: −98.513[1] mas/yr |
Parallax (π) | 20.8673 ± 0.1336 mas[1] |
Distance | 156 ± 1 ly (47.9 ± 0.3 pc) |
Absolute magnitude (MV) | 2.45[2] |
Details | |
Mass | 1.69[6] M☉ |
Luminosity | 8.14[7] L☉ |
Temperature | 7,000[7] K |
Rotational velocity (v sin i) | 43±2[8] km/s |
Age | 890[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 14622 is a single[6][10] star in the northern constellation of Andromeda. It is dimly visible to the naked eye under good seeing conditions, having an apparent visual magnitude of 5.81.[2] Based upon an annual parallax shift of 20.9 mas,[1] it is located 156 light years away. The star is moving closer to the Earth with a heliocentric radial velocity of −35 km/s,[5] and is predicted to come within 96 light-years in around 812,000 years.[2]
The stellar classification of HD 14622 is F0 III–IV,[3] showing a mixed spectrum of an evolving subgiant and giant star; suggesting this is an intermediate-mass star that has used up its core hydrogen and is expanding. The star is suspected of being slightly variable, but this has not been conclusively proven.[4] It is around 890[6] million years old with 1.69[6] times the mass of the Sun. The star is radiating 8[7] times the Sun's luminosity from its photosphere at an effective temperature of approximately 7,000.[7]
GaiaDR2
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