Gamma1 Octantis

Yellow-hued giant star in the constellation Octans From Wikipedia, the free encyclopedia

Gamma1 Octantis, Latinized from γ1 Octantis, is a single,[13] yellow-hued star in the constellation which includes the southern celestial pole, Octans. Its apparent visual magnitude is 5.10,[2] meaning that in good conditions it is bright enough to be faintly visible to the naked eye.

Right ascension23h 52m 06.47318s[1]
Declination−82° 01 07.7636[1]
Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
γ1 Octantis
Location of γ1 Octantis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Octans
Right ascension 23h 52m 06.47318s[1]
Declination −82° 01 07.7636[1]
Apparent magnitude (V) 5.10[2]
Characteristics
Evolutionary stage red clump[3]
Spectral type G7III[4]
U−B color index +0.60[5]
B−V color index +0.92[5]
Astrometry
Radial velocity (Rv)+15.4±0.1[6] km/s
Proper motion (μ) RA: −45.670[1] mas/yr
Dec.: −15.666[1] mas/yr
Parallax (π)12.1790±0.0552 mas[1]
Distance268 ± 1 ly
(82.1 ± 0.4 pc)
Absolute magnitude (MV)0.55[2]
Details
Mass1.81[7] M
Radius10.3[8] R
Luminosity60[8] L
Surface gravity (log g)2.64[7] cgs
Temperature5,017[8] K
Metallicity [Fe/H]−0.34[9] dex
Rotational velocity (v sin i)1.8[10] km/s
Other designations
γ1 Oct, 86 G. Octantis, CPD−82°905, FK5 3997, GC 33107, HD 223647, HIP 117689, HR 9032, SAO 258989[11][12]
Database references
SIMBADdata
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Distance and proper motion

Based upon an annual parallax shift of 12.2 mas which is taken during opposing points of the Earth's orbit of the sun (with compensation for its eccentricity),[1] the star is about 268 light years away. Its (proper) motion has a net vector at present of receding from the Sun, at +15.4 km/s.[6]

Characteristics

This is an evolved G-type giant star with a stellar classification of G7 III.[4] It is a red clump star,[3] which means it is generating energy through helium fusion at its core. The star has an estimated 1.81 times the mass of the Sun[7] and it has expanded to over 10 times the Sun's radius and is radiating 60 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 5,017 K.[8]

References

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