
Gliese 667
Triple-star system in the constellation Scorpius

Triple-star system in the constellation Scorpius
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. 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. There is a 12th-magnitude star visually close to the other three, but it is a distant background star not gravitationally bound to the system. 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. This...
Read on Wikipedia · Image Scorpius_constellation_map.png: Torsten Bronger derivative work: Kxx (talk), CC BY-SA 3.0
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