Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Aquarius [1] |
A | |
Right ascension | 22h 38m 45.57462s [2] |
Declination | −20° 37′ 16.0874″ [2] |
Apparent magnitude (V) | 9.08 [3] |
B | |
Right ascension | 22h 38m 45.28128s [4] |
Declination | −20° 36′ 51.8102″ [4] |
Apparent magnitude (V) | 11.49 [5] |
Characteristics | |
A | |
Evolutionary stage | main sequence |
Spectral type | M2.0V [6] |
Variable type | UV Cet+BY Dra [7] |
B | |
Evolutionary stage | main sequence |
Spectral type | M3.5V [6] |
Variable type | UV Cet+BY Dra [8] |
Astrometry | |
A | |
Radial velocity (Rv) | −8.70±0.69 [9] km/s |
Proper motion (μ) | RA: +449.207 mas/yr [2] Dec.: −79.046 mas/yr [2] |
Parallax (π) | 112.3859±0.0555 mas [2] |
Distance | 29.02 ± 0.01 ly (8.898 ± 0.004 pc) |
Absolute magnitude (MV) | 9.39 [3] |
B | |
Radial velocity (Rv) | −5.95±3.96 [4] km/s |
Proper motion (μ) | RA: +424.590 mas/yr [4] Dec.: −66.983 mas/yr [4] |
Parallax (π) | 112.9867 ± 0.0387 mas [4] |
Distance | 28.867 ± 0.010 ly (8.851 ± 0.003 pc) |
Orbit [10] | |
Primary | A |
Companion | C |
Period (P) | 4.0831962(29) d |
Semi-major axis (a) | 0.005607±0.000036″ |
Eccentricity (e) | 0.00520±0.00047 |
Inclination (i) | 51.95±0.42° |
Longitude of the node (Ω) | 111.64±0.22° |
Periastron epoch (T) | 2437145.575±0.037 JD |
Argument of periastron (ω) (secondary) | 307.5±3.0° |
Semi-amplitude (K1) (primary) | 46.138±0.011 km/s |
Semi-amplitude (K2) (secondary) | 58.275±0.023 km/s |
Orbit [6] | |
Primary | B |
Companion | D |
Period (P) | 1.795±0.017 d |
Eccentricity (e) | 0 (assumed) |
Periastron epoch (T) | 2456160.5611±0.0268 JD |
Semi-amplitude (K1) (primary) | 21.4±0.5 km/s |
Details | |
A | |
Mass | 0.5503±0.0095 [10] M☉ |
Radius | 0.56 [10] R☉ |
Temperature | 3416 [11] K |
Metallicity [Fe/H] | 0.08 [11] dex |
Rotation | 4.083 d [10] [a] |
Rotational velocity (v sin i) | 5.4±0.6 [10] km/s |
C | |
Mass | 0.4357±0.0075 [10] M☉ |
Radius | 0.45 [10] R☉ |
Rotation | 4.083 d [10] [a] |
Rotational velocity (v sin i) | 4.4±0.6 [10] km/s |
B | |
Mass | 0.29±0.06 [6] M☉ |
D | |
Mass | ≥0.056±0.007 [6] M☉ |
Other designations | |
BD−21 6267, GJ 867, CCDM J22388-2037AB | |
A: FK Aqr, CPD−21 8162, HD 214479, HIP 111802, SAO 191294, LTT 9128, NLTT 54421 [9] | |
B: FL Aqr, L 717-22, LP 876-81, LTT 9127, NLTT 54420 [5] | |
Database references | |
SIMBAD | A |
B |
Gliese 867 is a quadruple star system located 29 light-years (8.9 parsecs ) away in the constellation Aquarius. It is composed of two binary sub-systems, Gliese 867 A & B, also known by their variable star designations FK Aquarii and FL Aquarii. Gliese 867 is the third-nearest quadruple system, after Gliese 570 and Mu Herculis, [12] and the nearest such system where the primary star is a red dwarf. [6] There are two closer quintuple systems, V1054 Ophiuchi and Xi Ursae Majoris, the former composed entirely of red dwarfs. [12]
GJ 867 A (FK Aqr A) | |||||||||||
Period = 4.1 d | |||||||||||
GJ 867 C (FK Aqr B) | |||||||||||
Sep = 216 au | |||||||||||
GJ 867 B (FL Aqr A) | |||||||||||
Period = 1.8 d | |||||||||||
GJ 867 D (FL Aqr B) | |||||||||||
Hierarchy of orbits in the Gliese 867 system
Gliese 867 A & B are separated by 24.5 arcseconds, corresponding to a projected distance of 216 AU. Both are spectroscopic binaries. [6] Gliese 867 A & B are both flare stars and BY Draconis variables. [7] [8] They have been known to be flare stars since 1978. [13]
Gliese 867 A, also known as FK Aquarii, is a close binary orbiting every 4.1 days. The companion star is also called Gliese 867 C. [6] Both stars are red dwarfs around half the mass of the Sun. [10] The system has been known to be a spectroscopic binary since 1965, at that time referred to by its Durchmusterung designation BD−21°6267A. [16] It has also been characterized by astrometry from the Gaia space telescope. [17]
Both stars are magnetically active, and have strong dipolar magnetic fields resembling those found in lower-mass, fully convective red dwarfs. The primary star is the most massive red dwarf known to host this type of magnetic field as of 2024. [10]
Gliese 867 B, also known as FL Aquarii, is a close binary orbiting every 1.8 days. It was found to be a spectrosopic binary in 2014. The primary star is a red dwarf, while the companion, Gliese 867 D, has a minimum mass of only 61±7 Jupiter masses, and so may be a brown dwarf. [6]