description HIP 14810 d Overview
HIP 14810 d is the outer confirmed planet in the HIP 14810 system, orbiting a star broadly similar to the Sun. It was identified through radial-velocity measurements as part of a three-planet system announced in the late 2000s. Unlike the system’s inner planets, it has a substantially longer orbit and a mass in the giant-planet range rather than the super-Earth range. The system is used to study how multiple planets form and remain dynamically arranged around one star.
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