description HD 3167 b Overview
HD 3167 b is a transiting super-Earth orbiting the K-type star HD 3167. It completes an orbit in roughly 23 hours and has a radius about 1.6 times that of Earth, placing it among the short-period rocky or volatile-rich planets found by transit surveys. Its bright host star and repeated transits make it a useful target for measuring planetary composition and studying whether a close-in atmosphere can survive intense stellar irradiation.
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