description HD 10180 h Overview
HD 10180 h is a Neptune-class exoplanet detected through the radial-velocity motion of the Sun-like star HD 10180, about 127 light-years from Earth. It has a minimum mass of roughly 65 Earth masses and takes about six years to complete an orbit, placing it in the outer region of this multi-planet system. Because the radial-velocity method measures a minimum mass rather than a direct bulk mass, the planet’s true mass depends on the system’s orbital inclination.
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How good is HD 10180 h?
HD 10180 h scores 6.62/10 (Fair) on Lunoo, making it rated in the Exoplanet category.
What are the best alternatives to HD 10180 h?
See our alternatives page for HD 10180 h for a ranked list with scores. Top alternatives include: 47 Ursae Majoris d, 55 Cancri b, 55 Cancri d.
How does HD 10180 h compare to 47 Ursae Majoris d?
See our detailed comparison of HD 10180 h vs 47 Ursae Majoris d with scores, features, and an AI-powered verdict.
Is HD 10180 h worth it in 2026?
With a score of 6.62/10, HD 10180 h is a solid option in Exoplanet. See all Exoplanet ranked.
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