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Epsilon Columbae

ε Columbae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba
Right ascension 05h 31m 12.75540s
Declination −35° 28′ 13.8730″
Apparent magnitude (V) 3.87
Characteristics
Spectral type K1 II/III or K1 IIIa
U−B color index +1.08
B−V color index +1.14
Astrometry
Radial velocity (Rv) −4.9 km/s
Proper motion (μ) RA: +27.90 mas/yr
Dec.: −34.72 mas/yr
Parallax (π) 12.39 ± 0.42mas
Distance 263 ± 9 ly
(81 ± 3 pc)
Details
Luminosity 223 L
Surface gravity (log g) 2.05 cgs
Temperature 4,573 K
Metallicity [Fe/H] −0.03 dex
Other designations
ε Col, CD−35° 2348, FK5 2413, HD 36597, HIP 25859, HR 1862, SAO 195924.
Database references
SIMBAD data

Epsilon Columbae is a star in the southern constellation of Columba. It is visible to the naked eye, having an apparent visual magnitude of 3.87. Based upon an annual parallax shift of 12.39, it is located roughly 263 light years from the Sun.

This is an orange-huedK-type giant star with a stellar classification of K1 II/III. The star radiates 223 times the solar luminosity from its outer atmosphere at an effective temperature of 4,573 K. It has a peculiar velocity of 30.0±3.9 km/s, making it a candidate runaway star system. Based upon changes in the star's movement, it has an orbiting stellar companion of unknown type.


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Wikipedia

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