Sigma Centauri

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Template:Short description

σ Centauri
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Centaurus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 3.91[2]
Characteristics
Spectral type B3 V[3]
U−B Template:Engvar −0.805[2]
B−V Template:Engvar −0.202[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[4] km/s
Proper motion (μ) RA: −32.36[1] mas/yr
Dec.: −12.51[1] mas/yr
Parallax (π)7.92±0.18 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−1.60[5]
Details
MassScript error: No such module "val".[3] Template:Solar mass
Radius4.5[6] Template:Solar radius
Luminosity1,101[7] Template:Solar luminosity
Temperature15,744[7] K
Rotational velocity (v sin i)169[4] km/s
AgeScript error: No such module "val".[3] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
σ Cen, CD−49°7115, FK5 464, HD 108483, HIP 60823, HR 4743, SAO 223454.[8]
Database references
SIMBADdata

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Sigma Centauri, Latinized from σ Centauri, is the Bayer designation for a solitary[9] star in the southern constellation of Centaurus. It is visible to the naked eye with an apparent visual magnitude of 3.91.[2] A visual companion at an angular separation of Script error: No such module "val". along a position angle of Script error: No such module "val". was detected in 2010 using interferometry,[10] but its association with Sigma Centauri remains undetermined as of 2013.[11] The distance to Sigma Centauri, based upon an annual parallax shift of 7.92 mas,[1] is around 412 light years.

This is a B-type main sequence star with a stellar classification of B3 V.[3] It is a helium-rich star, the most massive type of chemically peculiar star.[12] Sigma Centauri has around 6.8 times the mass of the Sun and 4.5 times the Sun's radius.[6] It has a relatively high rate of spin with a projected rotational velocity of 169 km/s,[4] and is around 25 million years old.[3] The star radiates 1,101 times the solar luminosity from its outer atmosphere at an effective temperature of 15,744 K.[7] It is a member of the Lower Centaurus Crux component of the Scorpius–Centaurus association.[4]

References

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Template:Stars of Centaurus