NFT token detail for exoplanet GJ 667 C b. Only at exoplanetary.systems
GJ 667 C b 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 667 C b
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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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GJ 667 C b orbits the vibrant star GJ 667 C, a cool red dwarf nestled in the constellation of Scorpius. Discovered in 2012 using the radial velocity method with the HARPS Spectrograph at Chile’s La Silla Observatory, this exoplanet adds to the intriguing family of worlds circling this star. While details about GJ 667 C b’s exact size and temperature remain exciting topics for astronomers, what’s clear is that this planet offers a fascinating glimpse into the diversity of planetary systems beyond our own. Its discovery showcases the power of ground-based astronomy to unveil hidden cosmic neighbors, making GJ 667 C b a charming reminder of our ever-expanding celestial neighborhood.
