Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Scorpius |
Right ascension | 17h 18m 57.16483s[1] |
Declination | −34° 59′ 23.1416″[1] |
Apparent magnitude (V) | 5.91/7.20/10.20[2] |
Characteristics | |
Spectral type | K3V + K5V + M1.5V[2][3] |
U−B color index | 0.83/???/1.17 |
B−V color index | 1.03/???/1.57 |
Variable type | A: suspected B: unknown C: flare star[citation needed] |
Astrometry | |
Radial velocity (Rv) | 6.13±0.30[4] km/s |
Proper motion (μ) | RA: 1131.517 mas/yr[4] Dec.: −215.569 mas/yr[4] |
Parallax (π) | 138.0663 ± 0.0283 mas[4] |
Distance | 23.623 ± 0.005 ly (7.243 ± 0.001 pc) |
Absolute magnitude (MV) | 7.07/8.02/11.03 |
Details | |
GJ 667 AB | |
Mass | 0.73 / 0.69[5] M☉ |
Radius | 0.76 / 0.70[2] R☉ |
Metallicity [Fe/H] | –0.59[6] dex |
GJ 667 C | |
Mass | 0.327±0.008[7] M☉ |
Radius | 0.337±0.014[7] R☉ |
Luminosity | 0.01439±0.00035[7] L☉ |
Temperature | 3,443+75 −71[7] K |
Metallicity [Fe/H] | –0.59 ± 0.10[8] dex |
Rotation | 103.9±0.7 days[9] |
Age | 6.10±2.2[10] Gyr |
Orbit[11] | |
Companion | Gliese 667 B |
Period (P) | 42.15 yr |
Semi-major axis (a) | 1.81″ |
Eccentricity (e) | 0.58 |
Inclination (i) | 128° |
Longitude of the node (Ω) | 313° |
Periastron epoch (T) | 1975.9 |
Argument of periastron (ω) (secondary) | 247° |
Other designations | |
Database references | |
AB | |
A | |
B | |
C | |
Cb | |
Cc | |
Ce | |
Cf | |
Exoplanet Archive | Gliese 667 C |
ARICNS | Gliese 667 A |
B | |
C |
Gliese 667 (142 G. Scorpii) is a triple-star system in the constellation Scorpius lying at a distance of about 7.2 parsecs (23 light-years) from Earth. All three of the stars have masses smaller than the Sun. There is a 12th-magnitude star close to the other three, but it is not gravitationally bound to the system. To the naked eye, the system appears to be a single faint star of magnitude 5.89.
The system has a relatively high proper motion, exceeding 1 second of arc per year.
The two brightest stars in this system, GJ 667 A and GJ 667 B, are orbiting each other at an average angular separation of 1.81 arcseconds with a high eccentricity of 0.58. At the estimated distance of this system, this is equivalent to a physical separation of about 12.6 AU, or nearly 13 times the separation of the Earth from the Sun. Their eccentric orbit brings the pair as close as about 5 AU to each other, or as distant as 20 AU, corresponding to an eccentricity of 0.6.[note 1][12] This orbit takes approximately 42.15 years to complete and the orbital plane is inclined at an angle of 128° to the line of sight from the Earth. The third star, GJ 667 C, orbits the GJ 667 AB pair at an angular separation of about 30", which equates to a minimum separation of 230 AU.[8][13] GJ 667 C also has a system of two confirmed super-Earths and a number of additional doubtful candidates, though the innermost, GJ 667 Cb, may be a gas dwarf; GJ 667 Cc, and the controversial Cf and Ce, are in the circumstellar habitable zone.[14]
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