Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lyra |
Right ascension | 19h 10m 14.354s[1] |
Declination | +46° 57′ 26.14″[1] |
Apparent magnitude (V) | 13.435 (13.88 / 14.63)[2] |
Characteristics | |
LHS 6343 A | |
Spectral type | M4V[3] / T1.5[4] |
B−V color index | 1.57 ± 0.07[2] |
LHS 6343 B | |
Spectral type | M5V[3] |
B−V color index | 1.60 ± 0.07[2] |
Astrometry | |
Proper motion (μ) | RA: -76.59[5] mas/yr Dec.: -176.78[5] mas/yr |
Distance | 119.4 ± 3.6[2] ly (36.6 ± 1.1[2] pc) |
Orbit[6] | |
Period (P) | 12.7137941 ± 0.0000002 d |
Semi-major axis (a) | 0.0797 ± 0.0008 AU |
Eccentricity (e) | 0.030 ± 0.002 |
Inclination (i) | 90.45 ± 0.03° |
Periastron epoch (T) | JD 2455008.07259 ± 0.00001 |
Argument of periastron (ω) (secondary) | 320 ± 4° |
Semi-amplitude (K1) (primary) | 9.69 ± 0.02 km/s |
Details | |
LHS 6343 A | |
Mass | 0.358 ± 0.011[6] M☉ |
Radius | 0.373 ± 0.005[6] R☉ |
Surface gravity (log g) | 4.851 ± 0.008[2] cgs |
Temperature | 3431 ± 21[6] K |
Metallicity [Fe/H] | 0.04 ± 0.08[2] dex |
Rotation | 13.137 ± 0.011[2] |
LHS 6343 B | |
Mass | 0.292 ± 0.013[6] M☉ |
Radius | 0.394 ± 0.012[6] R☉ |
Temperature | 3354 ± 17[6] K |
Metallicity [Fe/H] | 0.04 ± 0.08[2] dex |
LHS 6343 C | |
Mass | 62.1 ± 1.2[6] MJup |
Radius | 0.783 ± 0.011[6] RJup |
Luminosity | 6.91×10−6[7] L☉ |
Surface gravity (log g) | 5.35 ± 0.02[2] cgs |
Temperature | 1130 ± 50[7] K |
Age | 5 ± 1[7] Gyr |
Other designations | |
Database references | |
SIMBAD | LHS 6343 |
LHS 6343 A | |
LHS 6343 B | |
LHS 6343 C |
LHS 6343 is a star system in the northern constellation of Lyra. It appears exceedingly faint with a combined apparent magnitude of 13.435.[2] Based on its stellar properties, the system is thought to be about 119.4 light-years (36.6 parsecs) away.[2]
LHS 6343 is a binary star with two red dwarfs, designated LHS 6343 A and B, respectively. A brown dwarf orbits LHS 6343 A at a close distance, and periodically transits it.[2] The brown dwarf, designated LHS 6343 C, is located within the brown dwarf desert, a zone around stars where very few brown dwarfs have been discovered.[2]
The system was in the field of view of the Kepler spacecraft,[2] and was monitored continuously for possible planets transiting the star, although the transits were found to be caused by LHS 6343 C.[2]