How is energy primarily transported through the dense inner region of a star, known as the radiative zone?
Answer
By photons that are continually absorbed and re-emitted.
In the radiative zone, energy moves via photons which interact repeatedly with the plasma, being absorbed and re-emitted, resulting in an extremely slow journey outward.
Related Questions
What characterizes the true, complex nature of stellar emission beyond visible light?What fundamental process is identified as the engine driving the perpetual energy release in a star's core?For a star like our Sun residing on the main sequence, what is the primary fusion reaction occurring?What crucial physical state is maintained by the outward pressure generated from fusion balancing the inward crush of gravity?How is energy primarily transported through the dense inner region of a star, known as the radiative zone?What energy transport mechanism takes over in the outer, cooler, and less dense layers of a star?What is the significant difference in escape time between neutrinos and photons from the Sun's core?What factor primarily dictates the longevity and fuel consumption rate of a star?The conversion of mass directly into pure energy during stellar nucleosynthesis follows which mathematical principle?By analyzing a star’s spectral signature, what key characteristics can astrophysicists deduce?What non-radiant output is produced when a star undergoes significant structural changes like a core collapse?