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HD 52265 b image

HD 52265 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2000
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HD 52265 b, charmingly nicknamed Cayahuanca, is a fascinating exoplanet orbiting the star HD 52265. Discovered back in 2000 using the radial velocity method with the HIRES Spectrometer at the W. M. Keck Observatory, this distant world has captured the imagination of astronomers. Although Cayahuanca orbits its star in close proximity, making it a bit of a cosmic hotshot, it remains a mystery wrapped in starlight. The planet’s discovery on Earth’s celestial doorstep reminds us how much there is to explore beyond our solar system. Next time you gaze at the night sky, think about Cayahuanca, a planet discovered from a ground-based telescope halfway across the world, quietly orbiting its star in the vastness of space.