description HD 202206 b Overview
HD 202206 b is a very massive companion of the solar-type star HD 202206. Its measured minimum mass is about seventeen times the mass of Jupiter, placing it near the boundary between the most massive planets and brown dwarfs. The object was discovered through radial-velocity observations, which detect the motion induced in the host star. Because its true mass depends on the unknown orbital inclination, its classification has been discussed in the context of the planet-brown-dwarf transition.
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