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Kepler-47b vs HAT-P-11b

Kepler-47b Kepler-47b
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HAT-P-11b HAT-P-11b
Kepler-47b WINNER Kepler-47b

Kepler-47b edges ahead with a score of 8.3/10 compared to 8.2/10 for HAT-P-11b. While both are highly rated in their res...

emoji_events WINNER
Kepler-47b

Kepler-47b

7.64 Good
Exoplanet
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psychology AI Verdict

Kepler-47b edges ahead with a score of 8.3/10 compared to 8.2/10 for HAT-P-11b. While both are highly rated in their respective fields, Kepler-47b demonstrates a slight advantage in our AI ranking criteria. A detailed AI-powered analysis is being prepared for this comparison.

emoji_events Winner: Kepler-47b
verified Confidence: Low

description Overview

Kepler-47b

Kepler-47b is a transiting circumbinary exoplanet located in the Kepler-47 system, which was announced in 2012. It was part of the first system discovered to host multiple planets orbiting a binary star pair. The planet completes an orbit around the two host stars approximately every 49 days. It is slightly larger than Uranus, placing it in the Neptune-class category of exoplanets.
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HAT-P-11b

HAT-P-11b is a Neptune-sized exoplanet discovered by the HATNet survey, orbiting the orange dwarf star HAT-P-11. It was one of the first small exoplanets to have water vapor successfully detected in its atmosphere, achieved via observations by the Hubble Space Telescope. The planet has a highly eccentric orbit for a hot Neptune, and it serves as an important target for studying the atmospheric com...
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