GJ 3991

GJ 3991
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Hercules
Right ascension 17h 09m 31.544s
Declination +43° 40′ 52.77″
Apparent magnitude (V) 13.671
Characteristics
Spectral type M3.5V
Apparent magnitude (B) 13.46
Apparent magnitude (R) 11.511
Apparent magnitude (J) 7.380
Apparent magnitude (H) 6.76
Apparent magnitude (K) 6.485
Astrometry
Radial velocity (Rv)−27.87 km/s
Proper motion (μ) RA: +332.032 mas/yr
Dec.: −274.501 mas/yr
Parallax (π)131.5996±0.4285 mas
Distance24.78 ± 0.08 ly
(7.60 ± 0.02 pc)
Absolute magnitude (MV)12.41
Orbit
Period (P)14.7136±0.0005 days
(0.0402836±0.0000014 yr)
Semi-major axis (a)0.015+0.01
−0.05
"
(0.1102 AU)
Eccentricity (e)0.068±0.004
Argument of periastron (ω)
(primary)
175.0±3.0°
Semi-amplitude (K1)
(primary)
50.6±0.2 km/s
Details
GJ 3991 A
Mass0.20 M
Temperature3250±50 K
Metallicity [Fe/H]0.20±0.06 dex
GJ 3991 B
Mass0.50 M
Temperature~4900 K
Age>6? Gyr
Other designations
GJ 3991, HIP 83945, G 203-47, WD 1708+437, USNO 752
Database references
SIMBADdata

GJ 3991 (also known as Gliese 3991 and G 203-47) is a binary star system located 24.2 light-years away in the constellation Hercules. It consists of a red dwarf star with 20–30% the mass of the Sun, and a white dwarf star roughly 50% the mass of the sun. The two components orbit each other in a tight orbit only 0.11 astronomical units from each other, with an orbital period of only 14.71 days. Due to their small separation, the two objects have never been visually resolved and are merely predicted from the radial velocity changes of GJ 3991, making the system a spectroscopic binary.