Sigma Columbae

Star in the constellation Columba From Wikipedia, the free encyclopedia

Sigma Columbae is a solitary,[10] yellow-white hued star in the southern constellation of Columba. Its name is a Bayer designation that is Latinized from σ Columbae, and abbreviated Sigma Col or σ Col. This star is faintly visible to the naked eye with an apparent visual magnitude of 5.51.[3] Based upon an annual parallax shift of 2.3 mas as seen from Earth,[2] this star is located at a distance of approximately 1,420 light years from the Sun.

Quick facts Constellation, Right ascension ...
Sigma Columbae
Location of σ Columbae (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Columba[1]
Right ascension 05h 56m 20.943s[2]
Declination −31° 22 56.780[2]
Apparent magnitude (V) 5.51[3]
Characteristics
Spectral type F2 III[4]
B−V color index +0.39[3]
Astrometry
Radial velocity (Rv)+19.4±2.9[5] km/s
Proper motion (μ) RA: +0.692 mas/yr[2]
Dec.: +6.510 mas/yr[2]
Parallax (π)2.2952±0.0438 mas[2]
Distance1,420 ± 30 ly
(436 ± 8 pc)
Absolute magnitude (MV)−2.98[1]
Details
Mass3.79[6] M
Luminosity1,312[7] L
Surface gravity (log g)2.02[6] cgs
Temperature6,820[8] K
Metallicity [Fe/H]−0.91[6] dex
Rotational velocity (v sin i)73.4±3.7[8] km/s
Age400[6] Myr
Other designations
σ Col, CD−31°2848, FK5 2454, GC 7499, HD 40248, HIP 28098, HR 2092, SAO 196330[9]
Database references
SIMBADdata
Close

At an age of about 400 million years,[6] the spectrum of this star suggests this is an evolved F-type giant with a stellar classification of F2 III.[4] It is spinning with a projected rotational velocity of about 74 km/s,[8] which is giving the star an oblate shape with an equatorial bulge that is 10% larger than the polar radius.[11] It has 3.79[6] times the mass of the Sun and is radiating 1,312[7] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 6,820 K.[8]

References

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