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]
{{
cite web}}
: CS1 maint: postscript (
link)
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]
{{
cite web}}
: CS1 maint: postscript (
link)