description HD 10180 g Overview
HD 10180 g is a proposed exoplanet candidate orbiting the Sun-like star HD 10180, located about 127 light-years from Earth. It was identified from radial-velocity measurements and was announced in 2010 as part of a possible system containing as many as nine planets. The object was described as a cold giant planet and as a possible member of the system's habitable-zone region, although its candidate status is important.
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