Scientific evidence that suggests that the two moons of Uranus, Miranda and Ariel, may harbour active oceans which could be possible evidence of life.
Both Miranda and Ariel are icy worlds with complex geological features, and they have been studied by spacecraft missions such as Voyager 2 and the Hubble Space Telescope. While these moons have some characteristics that could potentially make them habitable, such as subsurface oceans and sources of energy, there is currently no conclusive evidence of life on either of these moons.
Scientific exploration and investigation are ongoing, and new discoveries could potentially shed light on the possibility of life on these moons or elsewhere in our solar system and beyond.