TOI-2094 b is a super-Earth exoplanet orbiting a quiet red dwarf M-type star 163 light-years from Earth. Nearly twice our planet’s size with a mass of 4.27 Earth masses, it completes its orbit every 18.8 days at 0.136 AU, positioning it on the outer edge of the habitable zone. Its equilibrium temperature hovers around a crisp 276 Kelvin, offering tantalizing possibilities for liquid water beneath the right atmosphere. With a density hinting at a rocky or volatile-rich makeup, this world reveals how terrestrial-like planets can form around cooler stars. It stands as a steadfast beacon in the eternal archive of the universe, expanding our sense of wonder about potential life-friendly realms across the galaxy.
