Miranda has experienced geological activity that was likely caused by tidal heating when this little moon was in orbital resonance with its neighbour Umbriel. The image was taken during Voyager 2's flyby of the Uranus system in … Miranda is one of the smallest bodies in the solar system to be self-rounded under its own gravity. Miranda's surface may be mostly water ice, with the low density body also likely silicate rock and organic compounds in its interior.
The surface of Uranus' moon Miranda (seen here) is pocked with craters, but humans might be able to find a way to settle it.
Miranda's surface has patchwork regions of broken terrain indicating intense geological activity in the moon's past, and is criss-crossed by huge canyons. The Voyager 2 spacecraft is the only mission to fly close enough to image Miranda.
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