| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Camelopardalis |
| Right ascension | 05h 44m 08.44597s[1] |
| Declination | +61° 28′ 35.5255″[1] |
| Apparent magnitude (V) | 6.168[2] |
| Characteristics | |
| Spectral type | G5 III:[2] |
| B−V color index | 0.881[2] |
| Astrometry | |
| Radial velocity (Rv) | −2.47±0.17[1] km/s |
| Proper motion (μ) | RA: −11.312[1] mas/yr Dec.: +0.766[1] mas/yr |
| Parallax (π) | 7.5250 ± 0.0371 mas[1] |
| Distance | 433 ± 2 ly (132.9 ± 0.7 pc) |
| Absolute magnitude (MV) | 0.95[3] |
| Details | |
| Mass | 2.13[2] M☉ |
| Radius | 9.84[1] R☉ |
| Luminosity | 60.255[1] L☉ |
| Surface gravity (log g) | 3.15±0.18[4] cgs |
| Temperature | 5,183±51[4] K |
| Metallicity [Fe/H] | −0.01±0.05[4] dex |
| Age | 1.50[2] Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
23 Camelopardalis is a star in the northern circumpolar constellation of Camelopardalis, located 433 light years away from the Sun.[1] It is just visible to the naked eye as a dim, yellow-hued star with an apparent visual magnitude of 6.17.[2] The object is moving closer to the Sun with a heliocentric radial velocity of −2.5 km/s.[1]
With a stellar classification of G5 III:,[2] 23 Camelopardalis appears to be an aging giant star that has exhausted the hydrogen at its core and evolved away from the main sequence, although the ':' denotes some uncertainty about the classification. It is a red clump giant,[6] which indicates it is on the horizontal branch and is generating energy through helium fusion at its core. The star is 1.5[2] billion years old with more than double[2] the mass of the Sun and almost 10[1] times the Sun's radius. It is radiating 60[1] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,183 K.[4]
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