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GJ 676 A d image

GJ 676 A d

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2012
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GJ 676 A d is an intriguing exoplanet orbiting the star GJ 676 A, discovered back in 2012 using the clever radial velocity technique. This cosmic detective work was carried out with the HARPS Spectrograph stationed at the La Silla Observatory, nestled in the clear skies of Chile. Though we don’t know its exact size or composition, GJ 676 A d is part of a fascinating planetary system that continues to captivate astronomers and stargazers alike. It orbits its host star like a dancer in a stellar waltz, quietly reminding us that the galaxy is packed with worlds just waiting to be explored. GJ 676 A d certainly sparks the imagination of anyone curious about life beyond our own solar system.