description HD 160691 d Overview
HD 160691 d is a gas-giant exoplanet associated with the mu Arae system around the nearby G-type star HD 160691. It is one of several reported companions detected through radial-velocity measurements, a technique that infers a planet from the periodic motion of its host star. Its relatively long orbital period places it among the more distant members of the system. The object is of interest because mu Arae was an early, closely studied example of a compact multi-planet system around a Sun-like star.
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