Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Libra |
Right ascension | 16 00 19.61087 |
Declination | –16° 32′ 00.5483″ |
Apparent magnitude (V) | 5.47 |
Characteristics | |
Evolutionary stage | main sequence |
Spectral type | F8 V |
U−B color index | +0.03 |
B−V color index | +0.52 |
Astrometry | |
Radial velocity (Rv) | −20.1±4.0 km/s |
Proper motion (μ) | RA: –644.387 mas/yr Dec.: –360.803 mas/yr |
Parallax (π) | 34.2281 ± 0.1906 mas |
Distance | 95.3 ± 0.5 ly (29.2 ± 0.2 pc) |
Absolute magnitude (MV) | 2.89 |
Orbit | |
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 M☉ |
Radius | 1.86+0.05 −0.04 R☉ |
Luminosity | 4.74±0.03 L☉ |
Surface gravity (log g) | 4.14 cgs |
Temperature | 6,237 K |
Metallicity | –0.02 dex |
Rotational velocity (v sin i) | 9.6±1.0 km/s |
Age | 12 Gyr |
49 Lib B | |
Mass | 0.45 M☉ |
Other designations | |
49 Lib, BD–16°4196, FK5 1419, GJ 3931, HD 143333, HIP 78400, HR 5954, SAO 159625, WDS J16003-1632A | |
Database references | |
SIMBAD | data |
49 Librae is the Flamsteed designation for a binary star system in the Zodiac constellation of Libra. It has an apparent visual magnitude of 5.47, 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, but is drifting closer with a radial velocity of −20 km/s.
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. The primary component has a stellar classification of F8 V or F9 V, 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. The system is a source for radio and X-ray emissions, which may be coming from the secondary companion.
References
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ Nicolet, B. (October 1978), "Photoelectric photometric Catalogue of homogeneous measurements in the UBV System", Astronomy and Astrophysics Supplement Series, 34: 1–49, Bibcode:1978A&AS...34....1N.
- ^ Willmarth, Daryl W.; et al. (August 2016), "Spectroscopic Orbits for 15 Late-type Stars" (PDF), The Astronomical Journal, 152 (2): 13, Bibcode:2016AJ....152...46W, doi:10.3847/0004-6256/152/2/46, S2CID 53648490, 46.
- ^ Nordström, B.; et al. (November 2007), "The Geneva-Copenhagen survey of the Solar neighbourhood. II. New uvby calibrations and rediscussion of stellar ages, the G dwarf problem, age-metallicity diagram, and heating mechanisms of the disk", Astronomy & Astrophysics, 475 (2): 519–537, arXiv:0707.1891, Bibcode:2007A&A...475..519H, doi:10.1051/0004-6361:20077221, S2CID 119054949.
- Balachandran, Suchitra (May 1, 1990), "Lithium depletion and rotation in main-sequence stars", Astrophysical Journal, Part 1, 354: 310–332, Bibcode:1990ApJ...354..310B, doi:10.1086/168691.
- Fuhrmann, K.; Chini, R. (January 2, 2017), "Bright Times for an Ancient Star", The Astrophysical Journal, 834 (2): 114, Bibcode:2017ApJ...834..114F, doi:10.3847/1538-4357/834/2/114, S2CID 125888005.
- "49 Lib". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-11-06.
- Abt, Helmut A. (January 2009), "MK Classifications of Spectroscopic Binaries", The Astrophysical Journal Supplement, 180 (1): 117–118, Bibcode:2009ApJS..180..117A, doi:10.1088/0067-0049/180/1/117, S2CID 122811461.
- Lazio, T. Joseph W.; et al. (January 2010), "A Blind Search for Magnetospheric Emissions from Planetary Companions to Nearby Solar-Type Stars", The Astronomical Journal, 139 (1): 96–101, arXiv:0910.3938, Bibcode:2010AJ....139...96L, doi:10.1088/0004-6256/139/1/96, S2CID 118537554.
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