What are the key differences between GJ 3293 e and HAT-P-11b?

Compare GJ 3293 e and HAT-P-11b side by side on Lunoo to see detailed feature differences, AI scores, and expert analysis.

How are GJ 3293 e and HAT-P-11b scored?

GJ 3293 e has an AI score of 5.8/10 and HAT-P-11b has an AI score of 8.2/10. Scores are based on category fit, feature coverage, pricing signals, public reception, and recency.

GJ 3293 e vs HAT-P-11b 2026 - Compared

GJ 3293 e

HAT-P-11b

WINNER HAT-P-11b

HAT-P-11b edges ahead with a score of 7.5/10 compared to 5.3/10 for GJ 3293 e. While both are highly rated in their resp...

GJ 3293 e

5.34 Mediocre

Exoplanet

emoji_events WINNER

HAT-P-11b edges ahead with a score of 7.5/10 compared to 5.3/10 for GJ 3293 e. While both are highly rated in their respective fields, HAT-P-11b demonstrates a slight advantage in our AI ranking criteria. A detailed AI-powered analysis is being prepared for this comparison.

emoji_events Winner: HAT-P-11b

verified Confidence: Low

description Overview

GJ 3293 e

GJ 3293 e is an exoplanet orbiting the red dwarf star GJ 3293, which lies roughly 65 light-years from the Sun. It was identified through measurements of the star's motion using the radial-velocity method and is the outermost of the system's known planets, not the innermost. Its reported classification and orbital properties place it among the cooler, lower-mass planets found around nearby red dwar...

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...