Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Camelopardalis |
Right ascension | 04h 56m 07.07238s[1] |
Declination | +52° 52′ 11.0544″[1] |
Apparent magnitude (V) | 5.74±0.01[2] |
Characteristics | |
Evolutionary stage | main sequence star[3] |
Spectral type | A2 Vs[4] or A1 Vp[5] |
U−B color index | +0.11[2] |
B−V color index | +0.09[2] |
Astrometry | |
Radial velocity (Rv) | −15.1±2.5[6] km/s |
Proper motion (μ) | RA: −3.418 mas/yr[1] Dec.: +14.954 mas/yr[1] |
Parallax (π) | 6.8897 ± 0.1144 mas[1] |
Distance | 473 ± 8 ly (145 ± 2 pc) |
Absolute magnitude (MV) | +0.19[7] |
Details | |
Mass | 2.74±0.05[3] M☉ |
Radius | 4.38±0.22[8] R☉ |
Luminosity | 103+13 −11[3] L☉ |
Surface gravity (log g) | 3.85[9] cgs |
Temperature | 8,690[9] K |
Metallicity [Fe/H] | −0.11[10] dex |
Rotational velocity (v sin i) | 60±1[11] km/s |
Age | 432[12] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 31134, also designated as HR 1561, is a solitary star[14] located in the northern circumpolar constellation Camelopardalis, the giraffe. It is faintly visible to the naked eye as a white-hued star with an apparent magnitude of 5.74.[2] Gaia DR3 parallax measurements place it 473 light years away.[1] It appears to be approaching the Solar System with a heliocentric radial velocity of −15.1 km/s.[6] At its current distance, HD 31134's brightness is diminished by 0.35 magnitudes due to interstellar dust.[15] It has an absolute magnitude of +0.19.[7]
The object has a stellar classification of A2 Vs,[4] indicating that it is an A-type main-sequence star with sharp or narrow absorption lines due to slow rotation. Two sources remove the s prefix and instead list it as an ordinary dwarf star[16][17] while one lists it as a more evolved giant star.[18] Abt and Morell (1995) list it as a slightly hotter peculiar Ap star,[5] but it is now considered unlikely to be chemically peculiar.[19] It has 2.74 times the mass of the Sun and an enlarged radius of 4.38 R☉.[8] It radiates 103 times the luminosity of the Sun[3] from its photosphere at an effective temperature of 8,690 K.[9] HD 31134 is a rather evolved star, having completed 97.6% of its main sequence lifetime[3] at the age of 432 million years.[12] Consistent with its spectrum, it spins modestly with a projected rotational velocity of 60 km/s.[11]
GaiaDR3
was invoked but never defined (see the help page).Oja1991
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