Tau Octantis
Star in the southern constellation of Octans From Wikipedia, the free encyclopedia
Tau Octantis, Latinized from τ Octantis, is a solitary[11] star in the southern circumpolar constellation Octans. It has an apparent magnitude of 5.50,[2] allowing it to be faintly seen with the naked eye. The object is located at a distance of 480 light years[1] but is receding with a heliocentric radial velocity of 31 km/s.[5]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Octans |
Right ascension | 23h 28m 03.7855s[1] |
Declination | −87° 28′ 55.967″[1] |
Apparent magnitude (V) | 5.50[2] |
Characteristics | |
Spectral type | K2 III[3] |
U−B color index | +1.43[4] |
B−V color index | +1.27[4] |
Astrometry | |
Radial velocity (Rv) | 31.0±1.4[5] km/s |
Proper motion (μ) | RA: +16.782 mas/yr[1] Dec.: +11.957 mas/yr[1] |
Parallax (π) | 6.8009 ± 0.0574 mas[1] |
Distance | 480 ± 4 ly (147 ± 1 pc) |
Absolute magnitude (MV) | −0.36[2] |
Details | |
Mass | 1.14[6] M☉ |
Radius | 24[7] R☉ |
Luminosity | 223[8] L☉ |
Surface gravity (log g) | 1.63[6] cgs |
Temperature | 4,422[8] K |
Metallicity [Fe/H] | +0.12[9] dex |
Rotational velocity (v sin i) | <1[10] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Tau Octantis has a stellar classification of K2 III, indicating that the object is a red giant. It has 114% the mass of the Sun[6] but is 223 times as luminous.[8] However, an enlarged radius of 24 R☉ yields an effective temperature of 4,422 K,[8] giving it an orange glow. Tau Octantis has an iron abundance 132% that of the Sun and is believed to be a member of the old disk population.[9] Currently, it spins with a projected rotational velocity less than 1 km/s.[10]
References
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