Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Camelopardalis [1] |
Right ascension | 07h 01m 21.41899s [2] |
Declination | +70° 48′ 29.8635″ [2] |
Apparent magnitude (V) | 5.69±0.01 [3] |
Characteristics | |
Evolutionary stage | red giant branch [4] |
Spectral type | K4 III [5] |
U−B color index | +1.52 [3] |
B−V color index | +1.34 [3] |
Astrometry | |
Radial velocity (Rv) | −17.8±0.2 [6] km/s |
Proper motion (μ) | RA: +13.101 mas/yr [2] Dec.: −15.749 mas/yr [2] |
Parallax (π) | 6.3572±0.0481 mas [2] |
Distance | 513 ± 4 ly (157 ± 1 pc) |
Absolute magnitude (MV) | −0.27 [1] |
Details | |
Mass | 1.32±0.82 [7] M☉ |
Radius | 30.43 [8] R☉ |
Luminosity | 203±3 [2] L☉ |
Surface gravity (log g) | 1.99 [9] cgs |
Temperature | 4,396±122 [10] K |
Metallicity [Fe/H] | +0.01 [9] dex |
Age | 292 [2] Myr |
Other designations | |
AG+70°299, BD+70°430, GC 9152, HD 50885, HIP 33827, HR 2581, SAO 6041, WDS J07014+7049A [11] | |
Database references | |
SIMBAD | data |
HD 50885, also known as HR 2581, is a star located in the northern circumpolar constellation Camelopardalis, the giraffe. It has an apparent magnitude of 5.69, [3] making it faintly visible to the naked eye if viewed under ideal conditions. Based on parallax measurements from Gaia DR3, the object is estimated to be 513 light years distant. [2] It appears to be approaching the Solar System with a heliocentric radial velocity of −17.8 km/s . [6]
This is a solitary, [12] evolved red giant star with a stellar classification of K4 III. [5] It is currently on the red giant branch, [4] fusing a hydrogen shell around an inert helium core. It has 1.32 times the mass of the Sun [7] but has expanded to 30.4 times its girth. [8] It radiates 203 times the luminosity of the Sun [2] from its photosphere at an effective temperature of 4,396 K . [10] HD 50885 has an iron abundance only 102% that of the Sun, placing it at solar metallicity. [9]
There is an optical companion located 119″ away along a position angle of 357°. [13] This object was first noticed by Robert S. Ball in 1879 [14]