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The temperature in the radiative zone of the sun averages around 27 million degrees Fahrenheit.
The radiative zone in the sun can reach temperatures of several million degrees Celsius. Energy from nuclear fusion reactions in the core is transported through this region via photons before reaching the convective zone.
The three main layers of the sun's interior are the core, radiative zone, and convective zone. The core is where nuclear fusion reactions occur, producing the sun's energy. The radiative zone is where energy moves outward through radiation. The convective zone is where heat is carried to the surface through the movement of hot gas.
The convection zone of the sun surrounds the radiative zone, which is the region where energy generated by nuclear fusion in the core is transported outwards through the slow process of radiative diffusion. In the convection zone, energy is transported by the movement of hot plasma, creating convection currents.
The sun can be divided into three main regions: the core, the radiative zone, and the convective zone. The core is where nuclear fusion reactions occur, producing the sun's energy. The radiative zone is where energy is transported primarily through electromagnetic radiation. The convective zone is the outermost layer where energy is transferred through the motion of hot gas bubbles.
The two main parts of the Sun's core are the radiative zone and the convective zone. In the radiative zone, energy is transferred through radiation as photons bounce around and slowly move toward the surface. In the convective zone, energy is transported through the movement of hot plasma creating convection currents.