24 Cephei
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Cepheus |
| Right ascension | 22h 09m 48.43010s |
| Declination | +72° 20′ 28.3421″ |
| Apparent magnitude (V) | 4.79 |
| Characteristics | |
| Spectral type | G7 II-III |
| B−V color index | 0.898 |
| Astrometry | |
| Radial velocity (Rv) | −16.58 km/s |
| Proper motion (μ) | RA: +33.214 mas/yr Dec.: +2.679 mas/yr |
| Parallax (π) | 8.3965±0.1332 mas |
| Distance | 388 ± 6 ly (119 ± 2 pc) |
| Absolute magnitude (MV) | −0.519 |
| Details | |
| Mass | 3.50 M☉ |
| Radius | 13 R☉ |
| Luminosity | 209 L☉ |
| Surface gravity (log g) | 2.31±0.33 cgs |
| Temperature | 5,023±54 K |
| Metallicity [Fe/H] | −0.16±0.11 dex |
| Rotational velocity (v sin i) | 6.5 km/s |
| Age | 234 Myr |
| Other designations | |
| 24 Cep, BD+71° 1111, FK5 837, HD 210807, HIP 109400, HR 8468, SAO 10265 | |
| Database references | |
| SIMBAD | data |
24 Cephei is a single, yellow-hued star in the northern circumpolar constellation of Cepheus. With an apparent visual magnitude of 4.79, it is faintly visible to the naked eye. The distance to this star, based upon an annual parallax shift of 8.3965 mas, is around 388 light years. It is moving closer with a heliocentric radial velocity of −17 km/s.
Keenan and McNeil (1989) listed a stellar classification of G7 II-III for 24 Cep, matching the spectrum of an evolved G-type star with blended features of a bright giant and a giant star. Older sources list a class of G8 III, which would suggest an ordinary giant star. At the age of 234 million years, it has an estimated 3.5 times the mass of the Sun and has expanded to about 13 times the Sun's radius. The star is radiating 199 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,023 K. These coordinates are a source of X-ray emission.