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HD 217107 c image

HD 217107 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2005
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HD 217107 c is an intriguing exoplanet orbiting the star HD 217107, discovered back in 2005 using the radial velocity method at the Lick Observatory with the trusty Hamilton Echelle Spectrograph. This gas giant plays a slower cosmic dance far from its host star, making it quite the contrast to its closer-in sibling, HD 217107 b. While it circles quietly in the outer reaches of its system, HD 217107 c offers a peek into the diverse family of planets beyond our solar neighborhood. It’s a great reminder that the universe is full of surprises, with worlds both near and far waiting to be explored and understood — proving that even distant giants have their own stories to tell!