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HD 3167 c vs Kepler-11f

HD 3167 c HD 3167 c
VS
Kepler-11f Kepler-11f
Kepler-11f WINNER Kepler-11f

Kepler-11f edges ahead with a score of 7.4/10 compared to 6.8/10 for HD 3167 c. While both are highly rated in their res...

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emoji_events WINNER
Kepler-11f

Kepler-11f

6.81 Fair
Exoplanet

psychology AI Verdict

Kepler-11f edges ahead with a score of 7.4/10 compared to 6.8/10 for HD 3167 c. While both are highly rated in their respective fields, Kepler-11f demonstrates a slight advantage in our AI ranking criteria. A detailed AI-powered analysis is being prepared for this comparison.

emoji_events Winner: Kepler-11f
verified Confidence: Low

description Overview

HD 3167 c

HD 3167 c is a transiting sub-Neptune orbiting the K-type star HD 3167. Discovered in 2016 through transit observations, it has an orbital period of about 29.8 days and a radius roughly three times that of Earth. Its orbit is strongly misaligned with the star's equatorial plane and is often described as nearly polar, contrasting with the much shorter, more aligned orbit of the system's inner plane...
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Kepler-11f

Kepler-11f is one of six known transiting planets orbiting the Sun-like star Kepler-11. Announced in 2011, it belongs to an unusually compact system in which five planets orbit closer to their star than Mercury does to the Sun. Transit timing variations allowed researchers to estimate planetary masses and densities, making the system important for studying the structures and formation of low-densi...
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