description HD 50499 b Overview
HD 50499 b is a giant exoplanet orbiting the G-type star HD 50499. It was detected by radial-velocity measurements and has an orbital period of several years, placing it among the long-period planets found through extended stellar monitoring. Its wide orbit distinguishes it from close-in gas giants and makes the system useful for studying planetary companions that require many years of observations to characterize.
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