description HD 72659 b Overview
HD 72659 b is a gas-giant exoplanet orbiting the solar-type star HD 72659. It was detected through radial-velocity measurements and completes one orbit in roughly 3.6 years. The planet has a minimum mass several times that of Jupiter, so the term Jupiter analog refers mainly to its broad orbital scale and giant-planet nature rather than to an exact match with Jupiter. It is studied as an example of a long-period planet around a Sun-like star.
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