GJ 1132 b (Gliese 1132 b) is an extra-solar planet orbiting
M-type starGJ 1132 (Gliese 1132), ~13 parsecs
from Earth,
and somewhat close to Earth-size (an exo-Earth),
i.e., 1.7 Earth-masses and 1.1 Earth radii.
It is a transiting planet discovered by the MEarth Project in 2015.
It has been of interest for being sufficiently close to observe,
and though not in the habitable zone, it was initially thought
to be cool enough (plausibly as low as 409 K) to retain
an atmosphere, which could be investigated using
transmission spectroscopy.
However, further study reveals it to be warmer and unlikely to have
much of an atmosphere.
GJ 1132 b characteristics: