Sigma Capricorni

Star in the constellation Capricornus From Wikipedia, the free encyclopedia

Sigma Capricorni is a solitary,[8] orange-hued star in the southern constellation of Capricornus,[7] 0.5 degree north of the ecliptic. Its name is a Bayer designation that is Latinized from σ Capricorni, and abbreviated Sigma Cap or σ Cap. This star is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of +5.31.[3] The star is about 950 ly (290 pc) 1,070 light years away from the Sun based on parallax, but is drifting closer with a radial velocity of −9.6 km/s.[5]

Quick facts Constellation, Right ascension ...
Sigma Capricorni
Location of σ Capricorni (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Capricornus[1]
Right ascension 20h 19m 23.604s[2]
Declination −19° 07 06.69[2]
Apparent magnitude (V) +5.31[3]
Characteristics
Spectral type K2 III[4]
U−B color index +1.56[3]
B−V color index +1.43[3]
Astrometry
Radial velocity (Rv)−9.64±0.16[5] km/s
Proper motion (μ) RA: +5.034 mas/yr[2]
Dec.: −10.825 mas/yr[2]
Parallax (π)3.4448±0.0987 mas[2]
Distance950 ± 30 ly
(290 ± 8 pc)
Absolute magnitude (MV)−2.38[1]
Details
Mass6.3±0.7[6] M
Radius67.5+4.2
−6.0
[5] R
Luminosity1,392±64[5] L
Temperature4,292+204
−127
[5] K
Age60.5±17.2[6] Myr
Other designations
σ Cap, CD−19°5776, FK5 3625, HD 193150, HIP 100195, HR 7761, SAO 163445, WDS J20194-1907A[7]
Database references
SIMBADdata
Close

This is an evolved, K-type giant star with a stellar classification of K2 III.[4] Having exhausted the supply of hydrogen at its core, it has expanded and now has around 67.5[5] times the girth of the Sun. The star is about 60.5[6] million years old with 6.3[6] times the mass of the Sun. It is radiating 1,392[5] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,292 K.[5]

A magnitude 9.43 visual companion is at an angular separation of 55.90 along a position angle of 179°, as of 2016.[9]

References

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