NFT token detail for exoplanet GJ 676 A d. Only at exoplanetary.systems

GJ 676 A d is a sub_neptune exoplanet discovered in 2012 using the Radial Velocity method at La Silla Observatory. The 3.6 m ESO Telescope was employed with the instruments of the HARPS Spectrograph.

GJ 676 A d image

GJ 676 A d

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Discovery Details

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2012
Facility: La Silla Observatory
Instrument: HARPS Spectrograph
Telescope: 3.6 m ESO Telescope

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More planets in the GJ 676 A system

GJ 676 A b thumbnail GJ 676 A b GJ 676 A c thumbnail GJ 676 A c GJ 676 A e thumbnail GJ 676 A e
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.