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1. Star

   Linked via "radiative zone"

   Stellar Structure and Energy Transport
   A typical star/) possesses a highly stratified structure, organized by pressure and temperature gradients. The primary layers include the core)/), radiative zone, convective zone, and the photosphere, the visible surface.
   The Core

2. Star

   Linked via "radiative zone"

   Energy produced in the core)/) propagates outward through two primary mechanisms:
   Radiation: In the radiative zone, energy is transported via photons. The opacity)/) of the plasma dictates the efficiency of this process. In lower-mass stars/), the opacity)/) is dominated by electron scattering, whereas in hotter, more massive [stars](/entries/star-(luminous-sphero…