Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Hydra |
Right ascension | 09h 38m 27.28962s[1] |
Declination | +04° 38′ 57.4461″[1] |
Apparent magnitude (V) | 4.68[2] |
Characteristics | |
Evolutionary stage | giant |
Spectral type | K3 III[2] |
B−V color index | +1.310±0.033[3] |
Astrometry | |
Radial velocity (Rv) | +44.61±0.23[4] km/s |
Proper motion (μ) | RA: −163.18[1] mas/yr Dec.: −50.88[1] mas/yr |
Parallax (π) | 11.04 ± 0.27 mas[1] |
Distance | 295 ± 7 ly (91 ± 2 pc) |
Absolute magnitude (MV) | −0.10[3] |
Details | |
Mass | 1.32[2] M☉ |
Radius | 24[4] R☉ |
Luminosity | 190.5[2] L☉ |
Surface gravity (log g) | 2.09±0.22[5] cgs |
Temperature | 4,188±33[2] K |
Metallicity [Fe/H] | −0.30±0.09[5] dex |
Rotational velocity (v sin i) | 3.0[4] km/s |
Age | 4.58[2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
2 Sextantis is a single[7] star that is now in the equatorial constellation Hydra, located around 295 light years away from the Sun. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.68.[2] This object is moving further from the Earth with a heliocentric radial velocity of +44.6 km/s.[4] It has a relatively high proper motion, traversing the celestial sphere at the rate of 0.173″ per year.[8]
This is a giant star with a stellar classification of K3 III,[2] which, at the age of 4.58[2] billion years old, has exhausted the hydrogen at its core and evolved away from the main sequence. The star has 1.32[2] times the mass of the Sun and has expanded to 24[4] times the Sun's radius. It is radiating 190.5[2] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,188 K.[2]
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