description HD 74156 b Overview
HD 74156 b is a gas-giant exoplanet orbiting the G-type star HD 74156. It is the inner known planet in a system with two reported giant planets and was detected by observing the host star's radial-velocity changes. The planet follows an eccentric orbit, meaning its distance from the star changes substantially during each revolution. It is historically significant in exoplanet research because its 2001 discovery contributed to the early evidence that planetary systems can differ widely from the Solar System.
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