description HD 114762 b Overview
HD 114762 b is a long-period companion detected from radial-velocity measurements of the star HD 114762 and reported by Latham and colleagues in 1989. The signal implies a minimum mass of about 11 Jupiter masses, but radial velocity alone does not determine the orbital inclination, so its true mass may be higher. It is therefore discussed as an early exoplanet candidate near the planet-brown-dwarf boundary.
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How good is HD 114762 b?
HD 114762 b scores 6.26/10 (Fair) on Lunoo, making it rated in the Exoplanet category.
What are the best alternatives to HD 114762 b?
See our alternatives page for HD 114762 b for a ranked list with scores. Top alternatives include: Upsilon Andromedae c, HD 86264 b, Tau Boötis b.
How does HD 114762 b compare to Upsilon Andromedae c?
See our detailed comparison of HD 114762 b vs Upsilon Andromedae c with scores, features, and an AI-powered verdict.
Is HD 114762 b worth it in 2026?
With a score of 6.26/10, HD 114762 b is a solid option in Exoplanet. See all Exoplanet ranked.
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