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HD 34445 d image

HD 34445 d

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2017
FOR_SALE
HD 34445 d is an intriguing exoplanet orbiting the star HD 34445, spotted back in 2017 using the trusty radial velocity method from several observatories on good old Earth. This planet is part of a distant star system that teases astronomers with its subtle gravitational wobbles, detected by a mix of instruments working together in harmony. Although it doesn’t boast a flashy proper name, HD 34445 d invites curiosity as a member of an extrasolar family far from our solar neighborhood. Imagine a world circling a star beyond our view, discovered through the clever dance of light and motion, showcasing how ground-based telescopes continue to unravel the secrets of the cosmos one wobbly star at a time!