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HD 134987 b image

HD 134987 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 1999
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HD 134987 b is a fascinating exoplanet orbiting the star HD 134987, discovered back in 1999 thanks to the clever use of the radial velocity method at the W. M. Keck Observatory with the trusty HIRES Spectrometer. This planet gleefully circles its star, revealing the secrets of distant worlds to Earth-bound astronomers. While it doesn’t have a catchy proper name just yet, HD 134987 b stands out as a great example of how ground-based technology can unveil planetary neighbors light-years away. Picture a world out there, silently dancing around its sun, inviting future explorers to imagine its landscapes and skies. It’s a reminder that our cosmic neighborhood is full of surprises waiting to be uncovered!