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Mantle Convection

/ˈmæn.tl̩ kənˈvɛk.ʃən/noun
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Mantle convection is the process by which heat from the Earth's core causes the semi-fluid mantle to circulate in slow, massive currents, driving the movement of tectonic plates and shaping the planet's surface over geological time. This phenomenon not only explains phenomena like earthquakes and mountain formation but also influences long-term climate patterns through its role in volcanic activity and carbon cycling in modern earth sciences.

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