radiators.
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.
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 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.
In the radiative zone of the sun, energy moves through the transfer of photons. Photons, which are massless particles of light, are created through nuclear fusion in the sun's core and gradually travel through the radiative zone, bouncing off particles in a zig-zag pattern until they reach the convective zone.
Hi! It's 13 Million* Fahrenheit to 3.6* Fahrenheit.
The radiative zone is hotter than the convection zone. In the radiative zone, energy is transferred through electromagnetic radiation, while in the convection zone, energy is transferred through the movement of hot gas or plasma.
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.
They are the Convection Zone, Radiative Zone, then the Core.
The radiative zone of the Sun is not visible to the human eye, so it does not have a color. It is located beneath the Sun's visible surface where energy is transported by photons through a process of radiative diffusion.
radiative zone
radiative zone
The core, the radiative zone, and the convective zone.
The radiative zone extends from the outer edge of the solar core to about 70% of the distance to the solar surface. It is approximately 200,000 kilometers thick.
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 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 layer of the Sun through which energy is transferred away from the core by radiation is called the radiative zone. In this zone, energy from the core travels outward as photons, which are absorbed and re-emitted multiple times by the particles in the dense solar plasma before reaching the convective zone.