Gliese 676

Gliese 676 is a 10th-magnitude wide binary system of red dwarfs that has an estimated minimum separation of 800 AU with an orbital period of greater than 20,000 years. It is located approximately 54 light years away in the constellation Ara. In 2009, a gas giant was found in orbit around the primary star, in addition to its confirmation in 2011 there was also a strong indication of a companion; the second gas giant was characterised in 2012, along with two much smaller planets.

Gliese 676 A/B
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ara
Right ascension 17h 30m 11.20s
Declination –51° 38 13.1
Apparent magnitude (V) 9.59
Characteristics
Spectral type M0V/M3V
Apparent magnitude (B) 11.05/14.8
Apparent magnitude (J) 6.711
Apparent magnitude (H) 6.082
Apparent magnitude (K) 5.825
B−V color index 1.46
Astrometry
Radial velocity (Rv)−39.82±0.14 km/s
Proper motion (μ) RA: −258.759±0.034 mas/yr
Dec.: −185.119±0.025 mas/yr
Parallax (π)62.5786 ± 0.0303 mas
Distance52.12 ± 0.03 ly
(15.980 ± 0.008 pc)
Absolute magnitude (MV)8.55
Details
Mass0.631±0.017/0.29 M
Radius0.617+0.028
−0.027
 R
Luminosity0.08892±0.00220 L
Temperature4,014+94
−90
 K
Metallicity [Fe/H]0.23±0.10 dex
Rotation41.2±3.8 d
Other designations
CD–51°10924, HIP 85647, LTT 6947/6948, NLTT 44859, NSV 8846
Database references
SIMBADdata
Exoplanet Archivedata
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