Rho Capricorni
Star in the constellation Capricornus From Wikipedia, the free encyclopedia
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Star in the constellation Capricornus From Wikipedia, the free encyclopedia
Rho Capricorni (ρ Cap, ρ Capricorni) is a binary star[3] in the constellation Capricornus. Sometimes, this star is called by the name Bos, meaning the cow in Latin.[10] In Chinese, 牛宿 (Niú Su), meaning Ox (asterism), refers to an asterism consisting of β Capricorni, α2 Capricorni, ξ2 Capricorni, π Capricorni, ο Capricorni and ρ Capricorni.[11] Consequently, the Chinese name for ρ Capricorni itself is 牛宿六 (Niú Su liù, English: the Sixth Star of Ox.)[12]
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Capricornus |
Right ascension | 20h 28m 51.61448s[1] |
Declination | −17° 48′ 49.2693″[1] |
Apparent magnitude (V) | +4.78[2] (4.97 + 6.88)[3] |
Characteristics | |
Spectral type | F2 IV[2] + G1[4] |
Astrometry | |
Radial velocity (Rv) | +18.4[5] km/s |
Proper motion (μ) | RA: −14.98[1] mas/yr Dec.: −7.29[1] mas/yr |
Parallax (π) | 33.04 ± 0.46 mas[1] |
Distance | 99 ± 1 ly (30.3 ± 0.4 pc) |
Absolute magnitude (MV) | 2.52 + 4.56[4] |
Orbit[3] | |
Period (P) | 278 yr |
Semi-major axis (a) | 1.877″ |
Eccentricity (e) | 0.91 |
Inclination (i) | 113.3° |
Longitude of the node (Ω) | 162.0° |
Periastron epoch (T) | 1965.0 |
Argument of periastron (ω) (secondary) | 144.5° |
Details[6] | |
ρ Cap A | |
Mass | 1.52±0.04 M☉ |
Radius | 1.3[2] R☉ |
Luminosity | 9[7] L☉ |
Surface gravity (log g) | 4.02±0.03 cgs |
Temperature | 6,911±63 K |
Metallicity [Fe/H] | −0.20±0.05 dex |
Rotational velocity (v sin i) | 87.7[8] km/s |
Age | 1.74±0.15 Gyr |
Other designations | |
Database references | |
SIMBAD | ρ Cap |
ρ Cap A | |
ρ Cap B | |
ARICNS | ρ Cap A |
ρ Cap B |
This system is visible to the naked eye with a combined apparent visual magnitude of +4.78.[2] The pair orbit each other with a period of 278 years and an eccentricity of 0.91.[3] Based upon an annual parallax shift of 33.04 mas as seen from the Earth,[1] the system is located about 99 light years from the Sun. It is a thin disk population[6] star system that made its closest approach to the Sun about 1.6 million years ago when it came within 12.49 ly (3.830 pc).[13]
The primary member, component A, is a yellow-white hued, F-type subgiant with an apparent magnitude of 4.97[3] and a stellar classification of F2 IV.[2] This star has 1.5[6] times the mass of the Sun and 1.3 times the Sun's radius. It is radiating 9 times[7] as much luminosity of the Sun from its outer atmosphere at an effective temperature of 6,911 K.[6] The companion, component B, has a visual magnitude of 6.88.[3] The mass ratio is 0.539, meaning the secondary is only 53.9% as massive as the primary.[14]
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