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GJ 411 b image

GJ 411 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2019
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GJ 411 b is a fascinating exoplanet orbiting the nearby red dwarf star GJ 411, discovered in 2019 thanks to the clever use of the radial velocity method at the Haute-Provence Observatory with the SOPHIE Spectrograph. This little world is one of our stellar neighbors, making it a prime target for curious astronomers eager to explore planets beyond our solar system. Although it’s a bit sweltering closer to its star than Earth is to the Sun, GJ 411 b’s discovery opens a window into the diverse types of planets that can circle cool stars in our galaxy. It’s a cosmic gem discovered right here from Earth’s ground-based observatories, reminding us how technology and curiosity combine to unveil the wonders of the universe.