Heat Transfer: Radiation, Conduction, Convection

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The transfer of heat from the inner core to the surface of the plant is a vital progression of earth cooling. Recent scientific evidence has allowed for processes of conduction, convection and radiation to be better comprehended in their function of heat transfer and their contribution to the earth cooling process observing their importance in maintaining the earth’s equilibrium. The contrivance of conduction dominates the lithosphere. It holds the process that heat can move through solid without deforming its shape. Heat allows the atoms and molecules within these solids to vibrate aggressively cooling them. Conduction allows for the slow cooling of the lithosphere over a long period of time increasing the thickness. Isostasy therefore plays a key role in the process of conduction as the thicker the lithosphere becomes over time, its surface therefore descends to lower levels. Evidence of conduction can be been through the elevation of the mid ocean ridge is extremely high, comparable to the low lying abyssal plains distinctly illustrates this through studies of lithospheric samples where the mid oceanic ridge is younger and thinner than samples found at the abyssal plains which was much older and thicker. Conversely, convection primarily occurs due to buoyancy forces are able to overcome viscous resistance within the Earth’s interior. Materials in the mantle are heated through an internal source of the inner core thus expanding and rising upward toward the surface before flowing outward simultaneously cooling therefore decreasing in density and sinking in the formation of a current. This process occurs within the earth’s mantle, the transmission of scientific research in recent years has allowed the verification of the convection mechanism as an important form of heat transfer through the movement of tectonic plates. Convection allows for the transfer of

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