TOI-7384 b is a fresh super-Earth addition to the NASA Exoplanet Archive on February 5, 2026, with a mass of 12.4 Earths—implying a radius about 1.9 times Earth’s for a rocky world. Located around 218 light-years away, it was detected by NASA’s TESS mission through transit dips in its host star’s light. The star’s type isn’t fully detailed yet, but as a TOI object, it’s likely a G- or K-type similar to many TESS finds. Its orbital parameters suggest it’s not in the habitable zone, potentially too hot or irradiated for liquid water. This planet contributes to statistics on intermediate worlds between Earth and Neptune, which may transition from rocky to gaseous. Observations could reveal if it retains a hydrogen envelope or has lost it to stellar winds. As part of ongoing surveys, it helps map exoplanet diversity and test formation theories in varied systems.
