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HD 86081 b image

HD 86081 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2006
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Meet Santamasa, officially known as HD 86081 b, a fascinating exoplanet that orbits the star HD 86081. Discovered back in 2006 using the radial velocity method with the keen eyes of the HIRES Spectrometer at the W. M. Keck Observatory, Santamasa is a world that invites curiosity and wonder. Although we don’t have exact distances in this description, this ground-based discovery showcases the power of Earth’s telescopes in exploring distant planetary systems. Santamasa isn’t just a name; it’s a gateway to imagining what alien skies might look like as this planet circles its host star. A remarkable find that reminds us how much there is to discover beyond our solar system!