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HD 141399 c image

HD 141399 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2014
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HD 141399 c is an intriguing exoplanet orbiting the star HD 141399, discovered in 2014 using the clever radial velocity method. This ingenious technique involves spotting the star's tiny wobbles caused by the gravitational tug of its planet, much like detecting a dance partner’s steps in the dark! HD 141399 c resides far beyond our solar system, observed from multiple ground-based observatories wielding an array of instruments, making it a fascinating product of international collaboration. While details like its exact distance or size play hide-and-seek, its discovery adds another chapter to our cosmic story, inspiring us to keep searching the skies for new worlds and adventures. Think of HD 141399 c as a whisper from the distant universe inviting us to dream big!