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Theta Octantis
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Theta Octantis
Theta Octantis
Location of θ Octantis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Octans[1]
Right ascension 00h 01m 35.70158s[2]
Declination −77° 03′ 56.6092″[2]
Apparent magnitude (V) 4.78[1]
Characteristics
Evolutionary stage red clump[3]
Spectral type K3III[4]
U−B color index +1.41[5]
B−V color index +1.27[5]
Astrometry
Radial velocity (Rv)+22.48±0.17[6] km/s
Proper motion (μ) RA: −57.30[2] mas/yr
Dec.: −177.06[2] mas/yr
Parallax (π)15.02±0.18 mas[2]
Distance217 ± 3 ly
(66.6 ± 0.8 pc)
Absolute magnitude (MV)0.66[1]
Details
Mass1.20[7] M
Radius15.84+0.42
−1.02
[6] R
Luminosity79.2±1.5[6] L
Surface gravity (log g)2.16[7] cgs
Temperature4,325+147
−55
[6] K
Rotational velocity (v sin i)< 1.0[8] km/s
Other designations
θ Oct, CPD−77°1596, FK5 904, GC 33321, HD 224889, HIP 122, HR 9084, SAO 258207[9]
Database references
SIMBADdata

θ Octantis, Latinized as Theta Octantis, is a single[10] star in the southern circumpolar constellation of Octans, near the constellation border with Hydrus. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.78.[1] The star is located approximately 217 light years from the Sun based on parallax,[2] and is drifting further away with a radial velocity of +22.5 km/s.[6]

This is an aging giant star with a stellar classification of K3III,[4] having exhausted the supply of hydrogen at its core then cooled and expanded. It has been catalogued as a red clump giant,[3] which would indicate it is on the horizontal branch and is undergoing core helium fusion. At present it has 16[6] times the radius of the Sun. This star has 1.20[7] times the mass of the Sun and is radiating 79[6] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,325 K.[6]

References

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