Planets become layered during their formation due to processes like differentiation, where denser materials sink toward the center while lighter materials rise to the surface. As a planet accumulates mass from dust and gas, heat generated from gravitational compression and radioactive decay causes melting, allowing for the movement of materials. This results in distinct layers, such as a metallic core, a silicate mantle, and a crust, each with different compositions and properties. The layering is further influenced by factors like temperature, pressure, and the specific materials present during formation.
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