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HD 177830 b image

HD 177830 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 1999
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Meet HD 177830 b, a fascinating world orbiting the star HD 177830, discovered back in 1999 using the clever radial velocity method at the W. M. Keck Observatory, home to the impressive HIRES Spectrometer. This planet doesn't just quietly orbit its star; it dances in space, revealing clues about its existence through subtle stellar wobbles. While we don't have its exact distance from Earth here, HD 177830 b represents the excitement of hunting for worlds beyond our solar system using ground-based telescopes. It's a reminder of how much we can learn about far-off planets by studying the light from their stars and the gentle gravitational tugs they receive from their unseen companions. A cosmic partner in the grand galactic ballroom!