Hubbry Logo
HD 31134HD 31134Main
Open search
HD 31134
Community hub
HD 31134
logo
8 pages, 0 posts
0 subscribers
Be the first to start a discussion here.
Be the first to start a discussion here.
HD 31134
from Wikipedia
HD 31134
Location of HD 31134 on the map (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Camelopardalis[1]
Right ascension 04h 56m 07.07238s[2]
Declination +52° 52′ 11.0544″[2]
Apparent magnitude (V) 5.74±0.01[3]
Characteristics
Evolutionary stage main sequence[4]
Spectral type A2 Vs[5] or A1 Vp[6]
U−B color index +0.11[3]
B−V color index +0.09[3]
Astrometry
Radial velocity (Rv)−15.1±2.5[7] km/s
Proper motion (μ) RA: −3.418 mas/yr[2]
Dec.: +14.954 mas/yr[2]
Parallax (π)6.8897±0.1144 mas[2]
Distance473 ± 8 ly
(145 ± 2 pc)
Absolute magnitude (MV)+0.19[1]
Details
Mass2.74±0.05[4] M
Radius4.38±0.22[8] R
Luminosity103+13
−11
[4] L
Surface gravity (log g)3.85[9] cgs
Temperature8,690[9] K
Metallicity [Fe/H]−0.11[10] dex
Rotational velocity (v sin i)60±1[11] km/s
Age432[12] Myr
Other designations
AG+52°472, BD+52°898, GC 5988, HD 31134, HIP 22936, HR 1561, SAO 24919[13]
Database references
SIMBADdata

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.[3] Gaia DR3 parallax measurements place it 473 light years away.[2] It appears to be approaching the Solar System with a heliocentric radial velocity of −15.1 km/s.[7] 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.[1]

The object has a stellar classification of A2 Vs,[5] 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,[6] 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[4] 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[4] 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]

References

[edit]
Revisions and contributorsEdit on WikipediaRead on Wikipedia
Add your contribution
Related Hubs
User Avatar
No comments yet.