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How does mantle convection drive plate tectonics?

Mantle convection is the slow creeping motion of Earth's solid silicate mantle, driven by internal heat from radiogenic decay and primordial formation. This convective movement directly causes tectonic plates to form, move, and be consumed at plate boundaries. Specifically, sinking dense oceanic crust at subduction zones acts as the strongest downward driver of plate motion, while seafloor spreading adds new crust at divergent margins.

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