description HD 40307 c Overview
HD 40307 c is a super-Earth-mass exoplanet orbiting the K-type star HD 40307. It was announced in 2008 from radial-velocity observations and has an orbital period of approximately 9.6 days. The planet was part of the original set of three reported planets around the star, a system that helped establish the presence of multiple low-mass planets detected by the radial-velocity method. Its close orbit places it well inside the star's habitable zone.
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