description GJ 1132 c Overview
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 transiting planet. Its properties are therefore inferred mainly from orbital and mass measurements.
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