Titania
Titania's surface – a mixture of cratered terrain (including some craters that are partly submerged) and systems of interconnected valleys hundreds of kilometers long but with few impact basins – has clearly been reworked over the past few billion years. According to one theory, Titania was once hot enough to be liquid; the surface cooled and hardened, then the interior froze and expanded, cracking the surface and resulting in the valley systems seen today.
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