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The convection zone in a star like the Sun is located just beneath the photosphere. It is the layer where energy generated in the star's core is transported to the surface via convection currents, providing the energy needed for the star to shine.
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.
Convection currents can vary in thickness, typically ranging from a few centimeters to kilometers depending on the scale of the system in which they occur. In the Earth's mantle, for example, convection currents can be tens to hundreds of kilometers thick.
The temperature of gases in the convection zone increases as they rise towards the top. This is due to the process of convective heat transfer, where hotter gases move upwards and cooler gases move downwards, creating a cycle that leads to temperature increase towards the top of the convection zone.
No, nuclear fusion does not occur in the convection zone of a star. Fusion reactions primarily take place in the core region of a star, where the temperature and pressure are high enough to sustain the nuclear reactions that power the star. The convection zone is a region of the star where heat is transported through the movement of gas, but fusion does not occur there.
It is 20000 big times
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 portion of the sun in which energy moves from atom to atom in the form of waves is called the?
Sunspots and convection cells
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.
In the convection zone, hot plasma rises, cools as it nears the surface, and falls to be heated and rise again.
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.
The layer that surrounds the radiation zone of the sun is the convection zone. In this zone, energy is transferred by the movement of hot plasma rising and cooler plasma sinking, creating a convection current. This process allows energy to be transported from the core to the surface of the sun.
They are the Convection Zone, Radiative Zone, then the Core.
The convection zone in a star like the Sun is located just beneath the photosphere. It is the layer where energy generated in the star's core is transported to the surface via convection currents, providing the energy needed for the star to shine.
It goes out from the core into the radiation zone then into the convection zone where convection happens then it goes to the photosphere to become granules.
The convective zone,energy is transferred much faster that it is in the radiative zone.