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Ice moons in the outer solar system could have oceans that boil as water reaches the triple point where solid, liquid and gaseous water can coexist. The new models help us understand how surface features of moons like Mimas, Miranda or Titania are formed by internal processes. 🌌🌊❄️

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#IceMoons #OuterSolarSystem #BoilingOceans #PlanetaryScience #Astrobiology