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Gliese 667 Cc (also known as GJ 667 Cc, HR 6426 Cc, or HD 156384 Cc) [2] is an exoplanet orbiting within the habitable zone of the red dwarf star Gliese 667 C, which is a member of the Gliese 667 triple star system, approximately 23.62 light-years (7.24 parsecs; 223.5 trillion kilometres) away in the constellation of Scorpius.
The largest star in the system, Gliese 667 A (GJ 667 A), is a K-type main-sequence star of stellar classification K3V. [2] It has about 73% [5] of the mass of the Sun and 76% [2] of the Sun's radius, but is radiating only around 12-13% of the luminosity of the Sun. [15] The concentration of elements other than hydrogen and helium, what astronomers term the star's metallicity, is much lower ...
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Gliese 667 Cb is an exoplanet orbiting the star Gliese 667 C, a member of the Gliese 667 triple-star system. It is the most massive planet discovered in the system and is likely a super-Earth or a mini-Neptune. Orbital-stability analysis indicates that it cannot be more than twice its minimum mass.
Pages in category "Gliese 667" The following 4 pages are in this category, out of 4 total. This list may not reflect recent changes. ...
The combined catalogue is now commonly referred to as the Gliese–Jahreiß (GJ) catalog. [4] This catalogue was published with two tables: Table 1 uses the designations GJ NNNN for entries numbered 1000–1294 for confirmed nearby stars; Table 2 uses the designations GJ NNNN for entries numbered 2001–2159 for suspected nearby stars. [ 5 ]
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