the radiative zone is hotter
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 convection zone.
In the radiative zone, energy moves from atom to atom in the form of electromagnetic waves, or radiation. Energy produced in the core moves through this zone by convection, the transfer of energy by moving liquids or gases.
The convective zone,energy is transferred much faster that it is in the radiative zone.
The convection zone.
They are the Convection Zone, Radiative Zone, then the Core.
The portion of the sun in which energy moves from atom to atom in the form of waves is called the?
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 convective zone,energy is transferred much faster that it is in the radiative zone.
The convective zone,energy is transferred much faster that it is in the radiative zone.
In the convection Zone!
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 is composed of highly compressed gas (mainly hydrogen and helium) where energy is transported by electromagnetic radiation rather than by convection. This zone lies between the core and the convective zone of a star like the sun.
The layer of the sun between the core and the convection zone is the radiative zone. In the radiative zone, energy moves outward primarily through the absorption and re-emission of photons by ionized atoms. This process takes place over millions of years as the energy slowly diffuses through this layer before reaching the convective zone.
It takes about 100,000 years for a photon to move from the core of the sun to the convection zone. Photons created in the core of the sun have to undergo a random walk through the dense radiative zone before finally reaching the less dense convection zone.
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.