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HD 63765 b image

HD 63765 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2009
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HD 63765 b, charmingly named Yvaga, is a fascinating exoplanet orbiting the star HD 63765. This distant world was discovered back in 2009 using the radial velocity method, thanks to the keen eye of the HARPS Spectrograph stationed at the La Silla Observatory in Chile. Imagine a planet that reveals itself not by direct sight but by the subtle wobble it induces in its host star! Yvaga orbits relatively close to its sun, making it an intriguing target for scientists studying planetary systems beyond our own. While we haven't quite figured out all its secrets, Yvaga's discovery showcases the magic of modern astronomy, unveiling new worlds from the precision of ground-based telescopes. A true cosmic neighbor in the vast expanse, waiting to be better understood!