description HD 10180 f Overview
HD 10180 f is a super-Earth or mini-Neptune candidate orbiting the Sun-like star HD 10180, approximately 127 light-years from Earth. It belongs to a compact, multi-planet system identified through radial-velocity measurements made with the HARPS instrument. The planet was included in the system announced in 2010 and is classified as a cool, Neptune-class object rather than a small rocky planet.
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