Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Octans |
Right ascension | 23h 57m 32.8617s[1] |
Declination | −82° 10′ 11.30968″[1] |
Apparent magnitude (V) | 5.72±0.01[2] |
Characteristics | |
Spectral type | K0 III[3] |
U−B color index | +0.92[4] |
B−V color index | +1.05[4] |
Astrometry | |
Radial velocity (Rv) | 27.2±2.9[5] km/s |
Proper motion (μ) | RA: −22.246 mas/yr[1] Dec.: −23.235 mas/yr[1] |
Parallax (π) | 10.1771 ± 0.0345 mas[1] |
Distance | 320 ± 1 ly (98.3 ± 0.3 pc) |
Absolute magnitude (MV) | +0.87[6] |
Details[7] | |
Mass | 1.15±0.15 M☉ |
Radius | 10.54±0.28 R☉ |
Luminosity | 52.6±1.3 L☉ |
Surface gravity (log g) | 2.53±0.13 cgs |
Temperature | 4,788±58 K |
Metallicity [Fe/H] | −0.04±0.04 dex |
Rotational velocity (v sin i) | 2.8±1.1[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
γ2 Octantis, Latinized to Gamma2 Octantis (Gamma2 Oct), is a solitary[11] star in the southern circumpolar constellation Octans. It has an apparent magnitude of 5.72,[2] allowing it to be faintly seen with the naked eye. Parallax measurements place the object at a distance of 320 light years[1] and is currently receding with a heliocentric radial velocity of 27 km/s.[5]
Gamma2 Oct has a stellar classification of K0 III,[3] indicating that it is a red giant. At present it has 115% the mass of the Sun but has expanded to 10.54 times its girth.[7] It shines at 52.6 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,788 K,[7] giving it a yellow-orange glow. Gamma2 Oct has a poorly constrained metallicity 91% that of the Sun[7] and spins with a projected rotational velocity of about 3 km/s.[8]
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