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Cryovolcanism

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Cryovolcanism

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A dwarf planet in the Kuiper belt beyond Neptune. It measures approximately 1,086 km in diameter, about the size of Saturn’s moon Dione or half the size of Pluto. Signs of water ice on its surface suggest that cryovolcanism may be occurring. It has one known moon, Weywot .

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The largest moons in our solar system are subjected to various processes. For example, tidal forces from their parent planet can lead to tidal heating, causing geological activity and volcanism. Impact cratering from collisions with asteroids or other objects can also occur. Additionally, some moons may experience geological processes such as tectonic activity, cryovolcanism (volcanic activity with water or ice instead of molten rock), and erosion caused by the moon's own atmosphere or external factors.

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Water cant just appear. All water is either recycled (such as it raining, going into lakes, and it being evaporated back into clouds), saved in places such as springs, and saved in polar glaciers. There is no way for new water to form on earth. The water that's on earth now, if hidden, or found, is the only water there is.

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