K2-148b
K2-148b is a confirmed Super-Earth, probably rocky, closely orbiting a small orange dwarf star. It is the innermost of three Super-Earths around the star K2-148, which is in a wide binary pair with the M0.5V red dwarf EPIC 220194953. K2-148b is the smallest planet of the system, at about a third larger than Earth, and could be terrestrial in nature. However, the three planets do not exhibit significant transit timing variations, implying that they could have relatively low masses. The planet was validated in early 2018 by Hirano "et al." and is too hot for known life.
Kepler-124b
Kepler-124b is an extrasolar planet discovered in 2014. It is located from Earth, orbiting the unclassified star Kepler-124 in the constellation Cygnus. Within The Kepler-124 system (KOI-241) there are three known planets, Kepler-124b being both the smallest and closest to its parent star.