A convection zone is the final process of the sun's radius. Energy from the sun is carried outward to the surface by convection currents.
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In the radiative zone of a star, energy is transferred through electromagnetic radiation (photons) as it travels from the core to the convective zone. In contrast, in the convective zone, energy is transferred by the physical movement of hot gas or plasma through convection currents.
The three main parts of the Sun are the core, radiative zone, and convective zone. The core is where nuclear fusion occurs, producing the Sun's energy. The radiative zone is where energy is transported by electromagnetic radiation, and the convective zone is where energy is transported by convection currents.
The core, the radiative zone, and the convective zone.
Rainbow
The core, the radiative zone, and the convective zone.
they are in the convective zone
Convective zone.
From the Sun's core, energy moves through the radiative zone, across the tachocline (transition layer) to the convective zone, and then to the outer convective zone with its visible granulation.
The convective zone,energy is transferred much faster that it is in the radiative zone.
Energy travels through the convective zone of a star mainly through the process of convection, where hot plasma rises and cooler plasma sinks. This creates a continuous circulation of energy within the convective zone, helping to transport heat outward from the star's core to its surface.
The three main parts of the sun's interior are the core, where nuclear fusion occurs, the radiative zone, where energy is transported by photons, and the convective zone, where heat is transported through the motion of plasma.