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HD 221287 b image

HD 221287 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2007
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Meet Pipitea, officially known as HD 221287 b, a fascinating exoplanet orbiting the star HD 221287. Discovered in 2007 using the radial velocity method with the super-precise HARPS Spectrograph at the La Silla Observatory, this intriguing world captures the imagination of stargazers and scientists alike. Pipitea orbits its host star like a cosmic dance partner, revealed by the subtle wobbles HD 221287 makes under its gravitational spell. While its exact characteristics remain a mystery waiting to be unraveled, Pipitea serves as a shining example of how ground-based telescopes continue to unlock the secrets of distant planets, inviting us to dream about the vastness and variety of worlds beyond our solar system.