2004 mazda mx 5 specs - Surrounding the core is the radiative zone. This is a very dense region where energy is transported outwards through the slow process of radiative transfer. Photons produced in the core bounce around, constantly interacting with the dense plasma and gradually making their way towards the surface. The radiative zone extends out to about 70% of the **sun's** radius. This region is still extremely hot, but the temperature decreases as you move further away from the core. The radiative zone is crucial for the **sun's** energy transport. Because the plasma is so dense in this region, it takes a long time for photons to escape. Scientists estimate that it can take hundreds of thousands of years for a photon to travel from the core to the edge of the radiative zone. This slow process helps to regulate the **sun's** energy output and ensures that the **sun** shines steadily. The **sun's** structure is really fascinating, and the radiative zone plays a huge part in its overall function.
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