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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. [16] 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.
Gliese 667 Cb; Gliese 667 Cc; Τ. Template:Gliese 667 This page was last edited on 14 May 2023, at 12:13 (UTC). Text is available under the Creative Commons ...
Gliese 581e; Gliese 649 b; Gliese 667 Cb; Gliese 667 Cc; Gliese 674 b; Gliese 676 Ab; Gliese 676 Ac; Gliese 685 b; Gliese 777 b; Gliese 777 c; Gliese 806 c; Gliese 832 b;
1 Merge from Gliese 667 Cb. ... 2 Semimajor axis of Gliese 667 Cc. 1 comment. 3 ... 4 comments. 5 candidate for a diagram. 8 comments. 6 Map. 2 comments. 7 Planet ...
This page was last edited on 2 February 2021, at 19:51 (UTC).; Text is available under the Creative Commons Attribution-ShareAlike 4.0 License; additional terms may apply.