← Back to Cryptoplanets

GJ 367 d image

GJ 367 d

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2023
FOR_SALE
GJ 367 d orbits the red dwarf star GJ 367, discovered in 2023 using the trusty HARPS Spectrograph at the La Silla Observatory. This intriguing exoplanet, found through the radial velocity method, is part of a star system that has captured astronomers' attention with its mysterious charm. While details about GJ 367 d’s size and atmosphere remain a cosmic puzzle, it promises to be an exciting world lurking far beyond our solar system. Its discovery highlights the power of ground-based observatories in unveiling new planetary neighbors, making GJ 367 d a fresh gem in the ever-growing collection of exoplanets that remind us how vast and varied our galaxy truly is. Keep looking up—there’s always a new wonder awaiting!