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  2. Mantle convection - Wikipedia

    en.wikipedia.org/wiki/Mantle_convection

    On Earth, the Rayleigh number for convection within Earth's mantle is estimated to be of order 10 7, which indicates vigorous convection. This value corresponds to whole mantle convection (i.e. convection extending from the Earth's surface to the border with the core). On a global scale, surface expression of this convection is the tectonic ...

  3. Earth's internal heat budget - Wikipedia

    en.wikipedia.org/wiki/Earth's_internal_heat_budget

    Controversy over the exact nature of mantle convection makes the linked evolution of Earth's heat budget and the dynamics and structure of the mantle difficult to unravel. [21] There is evidence that the processes of plate tectonics were not active in the Earth before 3.2 billion years ago, and that early Earth's internal heat loss could have ...

  4. Internal structure of Earth - Wikipedia

    en.wikipedia.org/wiki/Internal_structure_of_Earth

    The pressure at the bottom of the mantle is ≈140 GPa (1.4 Matm). [24] The mantle is composed of silicate rocks richer in iron and magnesium than the overlying crust. [25] Although solid, the mantle's extremely hot silicate material can flow over very long timescales. [26] Convection of the mantle propels the motion of the tectonic plates in the

  5. Convection (heat transfer) - Wikipedia

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

    In many real-life applications (e.g. heat losses at solar central receivers or cooling of photovoltaic panels), natural and forced convection occur at the same time (mixed convection). [4] Internal and external flow can also classify convection. Internal flow occurs when a fluid is enclosed by a solid boundary such as when flowing through a pipe.

  6. Thermal history of Earth - Wikipedia

    en.wikipedia.org/wiki/Thermal_history_of_Earth

    The catastrophe is defined as when the mean mantle temperature exceeds the mantle solidus so that the entire mantle melts. Using the geochemically preferred Urey ratio of U r = 1 / 3 {\displaystyle Ur=1/3} and the geodynamically preferred cooling exponent of beta = 1 / 3 {\displaystyle {\text{beta}}=1/3} the mantle temperature reaches the ...

  7. Convection - Wikipedia

    en.wikipedia.org/wiki/Convection

    Mantle convection occurs at rates of centimeters per year, and it takes on the order of hundreds of millions of years to complete a cycle of convection. Neutrino flux measurements from the Earth's core (see kamLAND ) show the source of about two-thirds of the heat in the inner core is the radioactive decay of 40 K , uranium and thorium.

  8. images.huffingtonpost.com

    images.huffingtonpost.com/2012-05-14-PA1.pdf

    %PDF-1.4 %âãÏÓ 6 0 obj > endobj xref 6 120 0000000016 00000 n 0000003048 00000 n 0000003161 00000 n 0000003893 00000 n 0000004342 00000 n 0000004557 00000 n 0000004733 00000 n 0000005165 00000 n 0000005587 00000 n 0000005635 00000 n 0000006853 00000 n 0000007332 00000 n 0000008190 00000 n 0000008584 00000 n 0000009570 00000 n 0000010489 00000 n 0000011402 00000 n 0000011640 00000 n ...

  9. Earth's mantle - Wikipedia

    en.wikipedia.org/wiki/Earth's_mantle

    The movements of the lithosphere and the underlying mantle are coupled since descending lithosphere is an essential component of convection in the mantle. The observed continental drift is a complicated relationship between the forces causing oceanic lithosphere to sink and the movements within Earth's mantle.