| http://www.w3.org/ns/prov#value | - In the case of solar-like stars, as simulated here, the outermost zone is convective and turbulent: heat is transferred by the motion of matter, in the same way as air moves in a house heated by convection heaters.The inner zone is stratified and stable: it is a radiative zone in which energy is pushed outwards mainly by photons (light).
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