Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Centaurus [1] |
Right ascension | 12h 42m 35.45s [2] |
Declination | −48° 48′ 47.2″ [2] |
Apparent magnitude (V) | +4.66 [1] |
Characteristics | |
Evolutionary stage | red clump [3] |
Spectral type | K0III [4] [5] |
U−B color index | +1.01 |
B−V color index | +1.09 |
Astrometry | |
Radial velocity (Rv) | −11.7±0.8 [1] km/s |
Proper motion (μ) | RA: −123.84±0.16 [2] mas/yr Dec.: −30.17±0.13 [2] mas/yr |
Parallax (π) | 17.11±0.22 mas [2] |
Distance | 191 ± 2 ly (58.4 ± 0.8 pc) |
Absolute magnitude (MV) | +0.99±0.028 [6] |
Details | |
Mass | 1.71 [7] M☉ |
Radius | 11.61+0.23 −0.19 [8] R☉ |
Luminosity | 60.8±2.0 [8] L☉ |
Surface gravity (log g) | 2.61 [6] cgs |
Temperature | 4,682±26 [7] K |
Metallicity [Fe/H] | 0.19 [6] dex |
Age | 2.61 [7] Gyr |
Other designations | |
w Cen, CD−48°7608, GC 17282, HD 110458, HIP 62012, HR 4831, SAO 223614 [9] | |
Database references | |
SIMBAD | data |
HD 110458 is a single [10] star in the southern constellation of Centaurus. It has the Bayer designation w Centauri, while HD 110458 is the star's identifier in the Henry Draper Catalogue . The star has an orange hue and is faintly visible to the naked eye with an apparent visual magnitude of +4.66. [1] It is located at a distance of approximately 191 light years from the Sun based on parallax, [2] but is drifting closer with a radial velocity of −12 km/s. [1] Based on its space motion, in 1972 O. J. Eggen listed it as a probable member of the Hyades group. [11]
The stellar classification of HD 110458 is K0III, [4] [5] which indicates this is an aging giant star that has exhausted the supply of hydrogen at its core. It is estimated to be 2.6 [7] billion years old with 1.7 [7] times the mass of the Sun and has expanded to 11.6 [8] times the girth of the Sun. The star is radiating 61 [8] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,682 K. [7]