description HD 142 c Overview
HD 142 c is a confirmed outer giant planet orbiting the star HD 142, a nearby solar-type star. Its existence was inferred from long-term radial-velocity monitoring, which revealed a second, slower signal after the inner planet HD 142 b had been identified. HD 142 c has a multi-year orbital period and a minimum mass in the giant-planet range. The system provides a case for examining how massive planets are arranged around a star similar to the Sun.
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