Eta Circini

Star in the constellation Circinus From Wikipedia, the free encyclopedia

Eta Circini, Latinized from η Circini, is the Bayer designation for a solitary[8] star located in the southern constellation of Circinus. It is faintly visible to the naked eye with an apparent visual magnitude of 5.17.[3] The distance to this star, as determined from an annual parallax shift of 11.8 mas, is around 277 light years.

Quick facts Constellation, Right ascension ...
η Circini
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Circinus[1]
Right ascension 15h 04m 48.18757s[2]
Declination −64° 01 52.8641[2]
Apparent magnitude (V) 5.17[3]
Characteristics
Evolutionary stage red giant branch[2]
Spectral type G8 III[4]
B−V color index +0.93[3]
Astrometry
Radial velocity (Rv)44.8±0.8[5] km/s
Proper motion (μ) RA: +102.058[2] mas/yr
Dec.: 8.499[2] mas/yr
Parallax (π)11.7561±0.0661 mas[2]
Distance277 ± 2 ly
(85.1 ± 0.5 pc)
Absolute magnitude (MV)+0.52[1]
Details
Mass2.9[2] M
Radius10[2] R
Luminosity78[2] L
Surface gravity (log g)2.70[2] cgs
Temperature5,250[2] K
Metallicity [Fe/H]−0.37±0.02[6] dex
Age414[2] Myr
Other designations
η Cir, CPD−63°3493, HD 132905, HIP 73776, HR 5593, SAO 253005[7]
Database references
SIMBADdata
Close

This is an evolved G-type giant star with a stellar classification of G8 III.[4] It is radiating an estimated 78 times the solar luminosity from its outer atmosphere at an effective temperature of 5,250 K.[6]

References

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