Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Libra |
Right ascension | 16h 00m 19.61087s[1] |
Declination | –16° 32′ 00.5483″[1] |
Apparent magnitude (V) | 5.47[2] |
Characteristics | |
Evolutionary stage | main sequence |
Spectral type | F8 V[3] |
U−B color index | +0.03[2] |
B−V color index | +0.52[2] |
Astrometry | |
Radial velocity (Rv) | −20.1±4.0[4] km/s |
Proper motion (μ) | RA: –644.387[1] mas/yr Dec.: –360.803[1] mas/yr |
Parallax (π) | 34.2281 ± 0.1906 mas[1] |
Distance | 95.3 ± 0.5 ly (29.2 ± 0.2 pc) |
Absolute magnitude (MV) | 2.89[4] |
Orbit[3] | |
Period (P) | 1,142.4±1.1 d |
Semi-major axis (a) | ≥ 59.53±0.244 Gm |
Eccentricity (e) | 0.110±0.012 |
Inclination (i) | 143.0±2.0° |
Longitude of the node (Ω) | 163.5±2.8° |
Periastron epoch (T) | 57025±22 MJD |
Argument of periastron (ω) (secondary) | 69.4±7.4° |
Semi-amplitude (K1) (primary) | 3.847±0.051 km/s |
Details | |
49 Lib A | |
Mass | 1.4[3] M☉ |
Radius | 1.86+0.05 −0.04[1] R☉ |
Luminosity | 4.74±0.03[1] L☉ |
Surface gravity (log g) | 4.14[5] cgs |
Temperature | 6,237[4] K |
Metallicity [Fe/H] | –0.02[4] dex |
Rotational velocity (v sin i) | 9.6±1.0[3] km/s |
Age | 12[6] Gyr |
49 Lib B | |
Mass | 0.45[3] M☉ |
Other designations | |
Database references | |
SIMBAD | data |
49 Librae is the Flamsteed designation for a binary star[8] system in the Zodiac constellation of Libra. It has an apparent visual magnitude of 5.47,[2] making it faintly visible to the naked eye from dark suburban skies as a dim, yellow-white hued star. The system is located 95 light years away from the Sun, based on parallax,[1] but is drifting closer with a radial velocity of −20 km/s.[4]
The variable nature of the velocity for 49 Librae was first noted by W. S. Adams in 1924. It is a single-lined spectroscopic binary with an orbital period of 3.128 years and an eccentricity of 0.11.[3] The primary component has a stellar classification of F8 V or F9 V,[3] indicating it is an F-type main-sequence star. It has an estimated 1.4 times the mass of the Sun, while the companion only has 0.4 solar masses.[3] The system is a source for radio and X-ray emissions, which may be coming from the secondary companion.[9]
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