convection cells
The heat generated in the core of the sun is transported to the surface through a process called radiative and convective heat transfer. Energy in the form of photons moves outward through the radiative zone, and in the convective zone, hot plasma rises to the surface carrying heat with it.
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.
The layers of the sun from inside out are the core, radiative zone, convective zone, photosphere, chromosphere, and corona. The core is the densest layer, with a density of about 150 g/cm3. As you move outward, the density decreases, with the corona being the least dense layer.
Energy is generated in the core of the sun through nuclear fusion where hydrogen atoms are converted into helium. This energy then moves through the radiative zone via photons, which are energy particles that bounce around and slowly make their way to the photosphere. The energy eventually reaches the photosphere where it is released as sunlight.
Energy moves from the core of the Sun to its surface primarily through a process called radiative transfer, where photons are absorbed and re-emitted by particles in the dense plasma of the Sun's interior. This process takes a long time, often thousands to millions of years, as photons slowly migrate outward. Once they reach the convective zone, energy is transported more rapidly by convection currents, where hot plasma rises to the surface, cools, and then sinks back down. Finally, the energy is radiated into space as sunlight.
Convection currents move in the Mantle.
This layer is the mantle.
The upper mantle contains convection currents that move the tectonic plates.
Convection currents occur in the mantle, which is the middle layer of the Earth. The heat generated from the core causes the molten rock in the mantle to move in a circular pattern, creating convection currents.
The asthenosphere, which is a partially molten layer in the upper mantle, has convection currents that cause tectonic plates to move due to the heat-driven circulation of rock material. These convection currents are responsible for the continuous motion of tectonic plates on the Earth's surface.
Convection can happen in any state of matter in which the matter is free to move - such as a liquid, a gas, a plasma, a superfluid, a liquid crystal, etc.
In a star, energy from fusion moves outward from the core through radiation and convection. In the core, where fusion takes place, high-energy photons are generated and slowly diffuse outwards. In the outer layers, energy is carried by convection, where hot plasma rises and cooler plasma sinks, creating a cycle that transports energy towards the surface of the star.
Yes. Convection currents move hot materials to other places.
The layer of the Earth where convection currents occur is the mantle. These currents are generated by the heat from the Earth's core, causing movement in the semi-fluid mantle material. The movement of these convection currents is one of the driving forces behind the movement of tectonic plates on the Earth's surface.
Plates move because of the intense heat in the Earth's core. The heat causes molten rock in the mantle layer to move.
How does a convection current move rock
Yes, heat can move through air by conduction, convection, and radiation. Conduction is the transfer of heat between molecules in direct contact, convection is the transfer of heat by the movement of air, and radiation is the transfer of heat through electromagnetic waves.