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  2. Mantle convection - Wikipedia

    en.wikipedia.org/wiki/Mantle_convection

    Mantle convection is the very slow creep of Earth's solid silicate mantle as convection currents carry heat from the interior to the planet's surface. [ 2 ] [ 3 ] Mantle convection causes tectonic plates to move around the Earth's surface.

  3. Earth's internal heat budget - Wikipedia

    en.wikipedia.org/wiki/Earth's_internal_heat_budget

    This convective flow of the mantle drives the movement of Earth's lithospheric plates; thus, an additional reservoir of heat in the lower mantle is critical for the operation of plate tectonics and one possible source is an enrichment of radioactive elements in the lower mantle. [14] Earth heat transport occurs by conduction, mantle convection ...

  4. Earth's mantle - Wikipedia

    en.wikipedia.org/wiki/Earth's_mantle

    The temperature of the mantle increases rapidly in the thermal boundary layers at the top and bottom of the mantle, and increases gradually through the interior of the mantle. [22] Although the higher temperatures far exceed the melting points of the mantle rocks at the surface (about 1,500 K (1,200 °C; 2,200 °F) for representative peridotite ...

  5. Convection - Wikipedia

    en.wikipedia.org/wiki/Convection

    Mantle convection is the slow creeping motion of Earth's rocky mantle caused by convection currents carrying heat from the interior of the Earth to the surface. [33] It is one of 3 driving forces that causes tectonic plates to move around the Earth's surface.

  6. Convection (heat transfer) - Wikipedia

    en.wikipedia.org/wiki/Convection_(Heat_transfer)

    Simulation of thermal convection in the Earth's mantle. Hot areas are shown in red, cold areas are shown in blue. A hot, less-dense material at the bottom moves upwards, and likewise, cold material from the top moves downwards. Convection (or convective heat transfer) is the transfer of heat from

  7. Heat transfer - Wikipedia

    en.wikipedia.org/wiki/Heat_transfer

    Simulation of thermal convection in the Earth's mantle. Colors span from red and green to blue with decreasing temperatures. Colors span from red and green to blue with decreasing temperatures. A hot, less-dense lower boundary layer sends plumes of hot material upwards, and cold material from the top moves downwards.

  8. Slab (geology) - Wikipedia

    en.wikipedia.org/wiki/Slab_(geology)

    The slab affects the convection and evolution of the Earth's mantle due to the insertion of the hydrous oceanic lithosphere. [3] Dense oceanic lithosphere retreats into the Earth's mantle, while lightweight continental lithospheric material produces active continental margins and volcanic arcs, generating volcanism. [4]

  9. Earth's crustal evolution - Wikipedia

    en.wikipedia.org/wiki/Earth's_crustal_evolution

    An adiabat represents a change of temperature with pressure if no heat was lost through convection. Early mantle adiabats show crystallisation took place from the base; above approximately 25 GPa (deep mantle) perovskites would begin to crystallise, below 25 GPa (upper mantle) olivine would crystallise.