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HD 42012 b image

HD 42012 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2017
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Orbiting the star HD 42012, this intriguing exoplanet, HD 42012 b, was discovered back in 2017 by a clever team using the radial velocity method at the Haute-Provence Observatory. While it might not have a flashy nickname yet, HD 42012 b is a fascinating world revealed through the subtle wobble it induces in its host star. This planet was found with the help of multiple instruments working in harmony on the ground, showcasing the power of teamwork in astronomy. Though it keeps its secrets well about size and composition, HD 42012 b invites us to imagine far-off landscapes and alien skies, all thanks to the patient observations made from Earth’s own picturesque mountain observatory.