Radiation and Heat Practice Test

Convection is heat transport by the bulk movement of material. In the Earth’s mantle, hot material near the core becomes less dense and slowly rises, while cooler, denser material near the surface sinks. Over immense timescales these buoyant motions set up circulation currents that carry heat upward through the mantle. The mantle isn’t a nice, everyday fluid, but it’s an extremely viscous, plastic solid that flows very slowly, so convection behaves like a slow, fluid movement that transfers heat effectively. Radiation or heating through a vacuum wouldn’t explain the large-scale, directional heat transfer observed; the key idea is the moving mantle material carrying heat with it, not just radiation. This motion of mantle material aligns with how convection drives processes like plate tectonics.