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Eta Octantis
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Eta Octantis
η Octantis
Location of η Octantis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Octans
Right ascension 10h 59m 13.7578s[1]
Declination −84° 35′ 38.018″[1]
Apparent magnitude (V) 6.18±0.01[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type A1 Va[4]
U−B color index +0.12[5]
B−V color index +0.11[5]
Astrometry
Radial velocity (Rv)−1.7±0.6[6] km/s
Proper motion (μ) RA: −65.747 mas/yr[1]
Dec.: −8.273 mas/yr[1]
Parallax (π)9.1133±0.02 mas[1]
Distance357.9 ± 0.8 ly
(109.7 ± 0.2 pc)
Absolute magnitude (MV)+1.08[7]
Details
Mass2.37±0.03[3] M
Radius2.6±0.1[8] R
Luminosity45.3+3.1
−3.0
[3] L
Surface gravity (log g)4.1[9] cgs
Temperature9,500[9] K
Metallicity [Fe/H]−0.01[10] dex
Rotational velocity (v sin i)152±13[11] km/s
Age547[10] Myr
Other designations
η Oct, 11 G. Octantis[12], CPD−83°386, FK5 1664, GC 15164, HD 96124, HIP 53702, HR 4312, SAO 258600[13]
Database references
SIMBADdata

Eta Octantis, Latinized from η Octantis, is a solitary star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 6.19,[2] making it faintly visible to the naked eye. The object is situated at a distance of 358 light years[1] but is approaching the Solar System with a heliocentric radial velocity of −1.7 km/s.[6]

Eta Octantis has a stellar classification of A1 Va,[4] indicating that it is an ordinary A-type main sequence star. At present it has 2.37 times the Sun's mass[3] and 2.6 times the Sun's radius.[8] It shines with a luminosity of 45 L[3] from its photosphere at an effective temperature of 9,500 K, giving a white hue.[9] Eta Octantis is a rapidly rotating star, with a projected rotational velocity of 152 km/s,[11] and is estimated to be 547 million years old,[10] having completed 72% of its main sequence lifetime.[3]

References

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