Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Tucana |
Right ascension | 00h 42m 28.37166s[1] |
Declination | −65° 28′ 04.9100″[1] |
Apparent magnitude (V) | +5.38[2] |
Characteristics | |
Spectral type | F6 V[3] |
U−B color index | +0.00[2] |
B−V color index | +0.50[2] |
Astrometry | |
Radial velocity (Rv) | 33.962±0.796[4] km/s |
Proper motion (μ) | RA: +53.07[1] mas/yr Dec.: +40.94[1] mas/yr |
Parallax (π) | 24.37 ± 0.27 mas[1] |
Distance | 134 ± 1 ly (41.0 ± 0.5 pc) |
Absolute magnitude (MV) | +2.75[5] |
Orbit[6] | |
Period (P) | 4.8202 d |
Eccentricity (e) | 0.02 |
Periastron epoch (T) | 2419299.11 JD |
Semi-amplitude (K1) (primary) | 26.1 km/s |
Details | |
ρ Tuc A | |
Mass | 1.66[7] M☉ |
Luminosity | 9.7[8] L☉ |
Surface gravity (log g) | 3.64±0.11[4] cgs |
Temperature | 6,034±54[4] K |
Metallicity [Fe/H] | −0.26[4] dex |
Rotational velocity (v sin i) | 23.5±1.2[5] km/s |
Age | 2.64[3] Gyr |
ρ Tuc B | |
Mass | 0.33[7] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Rho Tucanae (ρ Tuc, ρ Tucanae) is a binary star system in the southern constellation of Tucana. It is visible to the naked eye with a combined apparent visual magnitude of +5.38.[2] Based upon an annual parallax shift of 24.37 mas as seen from Earth, it is located 131 light years from the Sun.
This is a single-lined spectroscopic binary with a close, nearly circular orbit having a period of 4.82 days and an eccentricity of 0.02.[6] The primary member, component A, is a yellow-white hued F-type main sequence star with a stellar classification of F6 V.[3] It is around 2.6 billion years old and a member of the thin disk population.[3] The primary has about 1.66 times the mass of the Sun while the secondary is just 0.33 times the Sun's mass.[7]
vanLeeuwen2007
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