Eta Columbae

Star in the constellation Columba From Wikipedia, the free encyclopedia

Eta Columbae is a solitary[7] star near the southern boundary of the constellation Columba.[8] Its name is a Bayer designation that is Latinized from η Columbae, and abbreviated Eta Col or η Col. This star is visible to the naked eye, having an apparent visual magnitude of 3.96.[2] Based upon an annual parallax shift of 7.40 mas,[1] it lies at a distance of approximately 441 light-years (135 pc) from the Sun. It is drifting further away with a line of sight velocity component of +17 km/s.[4]

Quick facts Constellation, Right ascension ...
η Columbae
Location of η Columbae (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension 05h 59m 08.805s[1]
Declination −42° 48 54.48[1]
Apparent magnitude (V) 3.96[2]
Characteristics
Spectral type G8/K1 II[3] or K0 III[4]
U−B color index +1.08[2]
B−V color index +1.14[2]
Astrometry
Radial velocity (Rv)+17.0[4] km/s
Proper motion (μ) RA: +118.897 mas/yr[1]
Dec.: −11.038 mas/yr[1]
Parallax (π)7.4021±0.1207 mas[1]
Distance441 ± 7 ly
(135 ± 2 pc)
Absolute magnitude (MV)−2.10[5]
Details
Mass4.70±0.04[1] M
Radius35.6±0.9[1] R
Luminosity564+18
16
[1] L
Surface gravity (log g)1.799±0.013[1] cgs
Temperature4,715+4
5
[1] K
Metallicity [Fe/H]−0.01[4] dex
Other designations
η Col, CD−42°2266, FK5 229, HD 40808, HIP 28328, HR 2120, SAO 217650[6]
Database references
SIMBADdata
Close

This is an orange-hued[8] K-type giant star with a stellar classification of K0 III,[4] or possibly a bright giant with a crossover class of G8/K1 II.[3] It has an estimated 4.7 times the mass of the Sun and has expanded to 35.6 times the Sun's radius. This star is radiating 564 times the solar luminosity from its photosphere at an effective temperature of 4,715 K.[1]

References

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