description HD 69830 d Overview
HD 69830 d is an extrasolar planet orbiting the K-type orange dwarf star HD 69830, located approximately 41 light-years away in the constellation Puppis. Discovered in 2006 through radial velocity measurements, it is the outermost of three confirmed Neptune-mass planets within the system. The planet completes its orbit in approximately 197 days, positioning it near the inner edge of the host star's estimated habitable zone. It is considered a significant subject in planetary science due to the system's unique asteroid belt and planetary architecture.
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