description HD 192310 b Overview
HD 192310 b is a planet with a minimum mass in the Neptune range orbiting the nearby K-type star HD 192310. Its existence was inferred from precise radial-velocity measurements, including observations made with the Keck and HARPS instruments, and was reported in 2011. The system also contains another known planet. Because radial velocity measures only minimum mass, the planet's true mass depends on its orbital inclination.
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