Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Capricornus |
Right ascension | 20h 19m 23.60402s[1] |
Declination | −19° 07′ 06.6967″[1] |
Apparent magnitude (V) | +5.31[2] |
Characteristics | |
Spectral type | K2 III[3] |
U−B color index | +1.56[2] |
B−V color index | +1.43[2] |
Astrometry | |
Radial velocity (Rv) | −9.64±0.16[1] km/s |
Proper motion (μ) | RA: +8.07[4] mas/yr Dec.: −11.31[4] mas/yr |
Parallax (π) | 3.0609 ± 0.1194 mas[1] |
Distance | 1,070 ± 40 ly (330 ± 10 pc) |
Absolute magnitude (MV) | −2.38[5] |
Details | |
Mass | 6.3±0.7[6] M☉ |
Radius | 67.5+4.2 −6.0[1] R☉ |
Luminosity | 1,392±64[1] L☉ |
Temperature | 4292+204 −127[1] K |
Age | 60.5±17.2[6] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Sigma Capricorni, Latinized from σ Capricorni, is a solitary[8] star in the southern constellation of Capricornus,[7] 0.5 degree north of the ecliptic. It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of +5.31.[2] The star is about 1,070 light years away from the Sun based on parallax, but is drifting closer with a radial velocity of −9.6 km/s.[1]
This object is an evolved, K-type giant star with a stellar classification of K2 III.[3] Having exhausted the supply of hydrogen at its core, it has expanded and now has around 67.5[1] 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[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,292 K.[1]
A magnitude 9.43 visual companion is at an angular separation of 55.90″ along a position angle of 179°, as of 2016.[9]
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