HD 24160
HD 24160 is a single star in the equatorial constellation of Eridanus. It has the Bayer designation g Eridani. It is visible to the naked eye with an apparent visual magnitude of 4.17. The distance to HD 24160 can be estimated from its annual parallax shift of 15.0 mas, yielding a separation of 217 light years. It is moving further from the Earth with a heliocentric radial velocity of +2 km/s. This object is a coronal member of the Ursa Major Moving Group of stars that share a common motion through space.
Location shown, annotated: g | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Eridanus |
Right ascension | 03h 49m 27.24527s |
Declination | −36° 12′ 34.8771″ |
Apparent magnitude (V) | 4.17 |
Characteristics | |
Spectral type | G7 III |
B−V color index | 0.927±0.045 |
Astrometry | |
Radial velocity (Rv) | +2.0±0.7 km/s |
Proper motion (μ) | RA: −44.841 mas/yr Dec.: −50.421 mas/yr |
Parallax (π) | 15.0389 ± 0.2211 mas |
Distance | 217 ± 3 ly (66.5 ± 1.0 pc) |
Absolute magnitude (MV) | 0.13 |
Details | |
Mass | 2.33 M☉ |
Radius | 11 R☉ |
Luminosity | 81.3 L☉ |
Surface gravity (log g) | 2.85±0.08 cgs |
Temperature | 4,948±45 K |
Metallicity [Fe/H] | +0.08±0.02 dex |
Age | 1.76 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
At the age of 1.76 billion years old, HD 24160 is an evolved G-type giant star with a stellar classification of G7 III, having consumed the hydrogen at its core and tracked away from the main sequence. It has 2.33 times the mass of the Sun and has expanded to about 11 times the Sun's radius. The star is radiating 81.3 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,948 K.