Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Columba |
Right ascension | 05h 56m 20.94287s[1] |
Declination | −31° 22′ 56.7846″[1] |
Apparent magnitude (V) | 5.51[2] |
Characteristics | |
Spectral type | F2 III[3] |
B−V color index | +0.39[2] |
Astrometry | |
Radial velocity (Rv) | +19.4±2.9[4] km/s |
Proper motion (μ) | RA: +0.08[1] mas/yr Dec.: +6.04[1] mas/yr |
Parallax (π) | 1.96 ± 0.24 mas[1] |
Distance | approx. 1,700 ly (approx. 510 pc) |
Absolute magnitude (MV) | −2.98[5] |
Details | |
Mass | 3.79[6] M☉ |
Luminosity | 1,312[7] L☉ |
Surface gravity (log g) | 2.02[6] cgs |
Temperature | 6,820[8] K |
Metallicity [Fe/H] | −0.91[6] dex |
Rotational velocity (v sin i) | 73.4±3.7[8] km/s |
Age | 400[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Sigma Columbae, Latinized from σ Columbae, is a solitary,[10] yellow-white hued star in the southern constellation of Columba. It is faintly visible to the naked eye with an apparent visual magnitude of 5.51.[2] Based upon an annual parallax shift of 1.96 mas as seen from Earth,[1] this star is located roughly 1,700 light years from the Sun.
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.[3] 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]