HD 142 b vs Mu Arae e
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HD 142 b
HD 142 b is a gas-giant exoplanet orbiting HD 142, a solar-type star in the constellation Phoenix. It was detected through the radial-velocity method and has an orbital period of approximately 350 days, close to the length of Earth's year. The planet is part of a multi-planet system and was among the early companions identified around Sun-like stars.
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Mu Arae e
Mu Arae e is an outer planet in the multi-planet system surrounding Mu Arae, a Sun-like star roughly 50 light-years from Earth. It has a mass in the Jupiter range and was identified from changes in the star's radial velocity. The planet was reported as part of the system's early four-planet interpretation in 2004. Its outer orbit distinguishes it from the shorter-period planets closer to Mu Arae.
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