HD 155876

HD 155876
HD 155876

Location of HD 155876 in the constellation Hercules
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules
Right ascension 17h 12m 07.9117s
Declination +45° 39′ 57.216″
Apparent magnitude (V) 9.52
Characteristics
A
Evolutionary stage main sequence
Spectral type M3
B
Evolutionary stage main sequence
Spectral type M4
Astrometry
Radial velocity (Rv)−30.9±0.5 km/s
Proper motion (μ) RA: +348.59±5.68 mas/yr
Dec.: −1624.84±6.80 mas/yr
Parallax (π)156.66±1.37 mas
Distance20.8 ± 0.2 ly
(6.38 ± 0.06 pc)
Absolute magnitude (MV)+10.31
Orbit
Period (P)12.9512±0.0096 yr
Semi-major axis (a)0.7620±0.0015
Eccentricity (e)0.7430±0.008
Inclination (i)149.14±0.25°
Longitude of the node (Ω)160.0±1.3°
Periastron epoch (T)1991.032±0.011
Argument of periastron (ω)
(secondary)
99.0±1.0°
Details
A
Mass0.379±0.035 M
Radius0.37±0.07 R
Luminosity0.018 L
Temperature3,422±100 K
Metallicity [Fe/H]−0.31±0.17 dex
B
Mass0.369±0.035 M
Radius0.37±0.07 R
Temperature3,422±100 K
Metallicity [Fe/H]−0.31±0.17 dex
Other designations
BD+45°2505, GJ 661, HD 155876, HIP 84140, WDS J17121+4540, KUI 79, Furuhjelm 46
A: LFT 1326, LHS 433, LTT 15095, NLTT 44362
B: LFT 1327, LHS 434, LTT 15096, NLTT 44363
Database references
SIMBADThe system
A
B

HD 155876, also known as Gliese 661, is a nearby binary star system, consisting of two very similar red dwarfs, located in the constellation Hercules.

The star's duplicity was discovered by the Dutch astronomer Gerard Kuiper in 1934 in a systematic survey for duplicity of the known stars within about 25 parsecs from the Sun, carried out with the 36-inch telescope of the Lick Observatory. HD 155876 is the nearest "true" (i. e. not brown dwarf) star system in Hercules, however, there is brown dwarf in this constellation, located closer: WISE 1741+2553.