Meet GJ 667 C g, a fascinating world orbiting the modest red dwarf star GJ 667 C, discovered back in 2013 using the trusty HARPS spectrograph at the La Silla Observatory. This exoplanet was found through the radial velocity method, which measures the star’s tiny wobbles caused by the planet’s gravitational tug. GJ 667 C g orbits in the star’s habitable zone—a cosmic sweet spot where conditions might just be right for liquid water. While not officially named, this intriguing planet sparks imaginations about what kind of environment it may have. It’s a cool target for future exploration and a reminder of the exciting diversity of worlds beyond our solar system, tucked away in the southern skies.
