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GJ 1132 c vs Kepler-138d

GJ 1132 c GJ 1132 c
VS
Kepler-138d Kepler-138d
Kepler-138d WINNER Kepler-138d

Kepler-138d edges ahead with a score of 8.3/10 compared to 6.2/10 for GJ 1132 c. While both are highly rated in their re...

GJ 1132 c

GJ 1132 c

5.70 Mediocre
Exoplanet
VS
emoji_events WINNER
Kepler-138d

Kepler-138d

7.64 Good
Exoplanet

psychology AI Verdict

Kepler-138d edges ahead with a score of 8.3/10 compared to 6.2/10 for GJ 1132 c. While both are highly rated in their respective fields, Kepler-138d demonstrates a slight advantage in our AI ranking criteria. A detailed AI-powered analysis is being prepared for this comparison.

emoji_events Winner: Kepler-138d
verified Confidence: Low

description Overview

GJ 1132 c

GJ 1132 c is a super-Earth-mass exoplanet associated with GJ 1132, a red dwarf star. It was announced in 2018 as one of several planets reported in the system and is described as orbiting near the outer edge of the host star's habitable zone. Unlike GJ 1132 b, the better-known inner planet in the system, GJ 1132 c does not pass across the star from Earth's line of sight, so it is not observed as a...
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Kepler-138d

Kepler-138d is a transiting exoplanet orbiting the M-dwarf star Kepler-138 approximately 200 light-years from Earth. It is the outermost of three known planets in the system, completing an orbit every 23.1 days. Categorized as a super-Earth, its mass and radius suggest a low bulk density. Researchers propose that this low density implies a substantial volatile envelope, leading to classifications...
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