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HD 177830 c image

HD 177830 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2010
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HD 177830 c is an intriguing exoplanet orbiting the star HD 177830, discovered back in 2010 thanks to the sharp eyes of the HIRES Spectrometer at the W. M. Keck Observatory. This planet revealed itself through the subtle wobbles in its star’s motion, spotted by the radial velocity method. Though it doesn’t yet have a catchy nickname, HD 177830 c holds its own as part of a fascinating star system located far beyond our solar neighborhood. Imagine a distant world dancing around its star, silently showcasing the wonders of the cosmos. Thanks to pioneering ground-based technology, astronomers continue to peel back the mysteries of such planets, turning the great expanse of space into an exciting playground for discovery.