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Gliese 667 Cc

A super-Earth in the habitable zone of a red dwarf in a triple-star system.

Gliese 667 Cc is a super-Earth orbiting in the habitable zone of the red dwarf Gliese 667 C, part of the Gliese 667 triple-star system about 23.6 light-years away in Scorpius. It was found with the radial velocity method and is sometimes called the first confirmed potentially habitable exoplanet.

It has a minimum mass of about 3.7 Earth masses and an estimated equilibrium temperature of 277 K.

Quick Facts

Type
Super-Earth
Host
Gliese 667 C
Constellation
Scorpius
Distance
~23.6 light-years
Minimum mass
~3.7 Earth masses

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