Misplaced Pages

49 Librae

Article snapshot taken from[REDACTED] with creative commons attribution-sharealike license. Give it a read and then ask your questions in the chat. We can research this topic together.
Star in the constellation Libra
49 Librae
Observation data
Epoch J2000      Equinox J2000
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
Distance95.3 ± 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
Mass1.4 M
Radius1.86+0.05
−0.04 R
Luminosity4.74±0.03 L
Surface gravity (log g)4.14 cgs
Temperature6,237 K
Metallicity –0.02 dex
Rotational velocity (v sin i)9.6±1.0 km/s
Age12 Gyr
49 Lib B
Mass0.45 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
SIMBADdata

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

  1. ^ 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.
  2. ^ 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.
  3. ^ 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.
  4. ^ 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.
  5. 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.
  6. 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.
  7. "49 Lib". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2013-11-06.
  8. 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.
  9. 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.
Constellation of Libra
Stars
Bayer
Flamsteed
Variable
HR
HD
Other
Exoplanets
Star clusters
Galaxies
NGC
Other
Category
Categories:
49 Librae Add topic