Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
Right ascension | 04h 21m 51.80623s[1] |
Declination | +56° 30′ 22.7351″[1] |
Apparent magnitude (V) | 5.92±0.01[2] |
Characteristics | |
Evolutionary stage | main sequence star[3] |
Spectral type | A3 V[4] or A2 IV-V[5] |
U−B color index | +0.08[6] |
B−V color index | +0.11[6] |
Astrometry | |
Radial velocity (Rv) | −13±5[7] km/s |
Proper motion (μ) | RA: −14.793 mas/yr[1] Dec.: +7.466 mas/yr[1] |
Parallax (π) | 10.4168 ± 0.0907 mas |
Distance | 313 ± 3 ly (96.0 ± 0.8 pc) |
Absolute magnitude (MV) | +0.98[8] |
Details | |
A | |
Mass | 1.9±0.1[9] M☉ |
Radius | 2.64+0.11 −0.10[10] R☉ |
Luminosity | 54.7+1.0 −0.9[1] L☉ |
Surface gravity (log g) | 3.88±0.14[11] cgs |
Temperature | 8,414+176 −173[3] K |
Metallicity [Fe/H] | −0.25[12] dex |
Rotational velocity (v sin i) | 130±8[5] km/s |
Age | 640[11] Myr |
B | |
Mass | 1.30±0.04[9] M☉ |
Temperature | 6,492±109[9] K |
Metallicity [Fe/H] | −0.50[9] dex |
Rotational velocity (v sin i) | 20[9] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 27322, also known as HR 1342, is a binary star located in the northern circumpolar constellation Camelopardalis. The visible component is faintly visible to the naked eye as a white-hued point of light with an apparent magnitude of 5.92.[2] The object is located relatively close at a distance of 313 light-years based on Gaia DR3 parallax measurements,[1] and it is drifting closer with a heliocentric radial velocity of approximately −13 km/s.[7] At its current distance, HD 27322's brightness is diminished by 0.24 magnitudes due to interstellar extinction[14] and it has an absolute magnitude of +0.98.[8]
HD 27322 A has a stellar classification of A3 V,[4] indicating that it is an ordinary A-type main-sequence star that is generating energy via hydrogen fusion at its core. Abt & Morell (1995) gave a hotter and slightly more evolved classification of A2 IV-V,[5] indicating that it is an A-type star with a luminosity class intermediate between a main sequence star and a subgiant. At the age of 640 million years,[11] HD 27322 A has completed 79.5% of its main sequence lifetime.[3] It has 1.9 times the mass of the Sun[9] and 2.64 times the radius of the Sun.[10] It radiates 54.7 times the luminosity of the Sun[1] from its photosphere at an effective temperature of 8,414 K.[3] HD 27322 A is metal deficient with an iron abundance 56% that of the Sun's ([Fe/H] = −0.25)[12] and it spins rapidly with a projected rotational velocity of 130 km/s.[5]
The object was generally classified as a solitary star.[15] However, evidence of HD 27322 being a binary first arose when an X-ray emission with a luminosity of 3.22×1020 W was detected around the star.[16] A-type stars are expected to be X-ray quiet, so it might be coming from a hidden companion. A 2016 spectroscopic survey detected a companion around HD 27322.[9] It has 1.3 times the mass of the Sun and it has an effective temperature of 6,492 K.[9] HD 27322 B is metal deficient with a [Fe/H] of −0.5 and it spins modestly with a projected rotational velocity of 20 km/s.[9]
GaiaDR3
was invoked but never defined (see the help page).Oja1991
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