Can you explain the concept of nuclear reactions in stars and their contribution to stellar evolution?

Sample interview questions: Can you explain the concept of nuclear reactions in stars and their contribution to stellar evolution?

Sample answer:

Nuclear Reactions in Stars

Nuclear reactions are the fundamental processes that drive stellar evolution and provide the energy that powers stars. These reactions occur in the cores of stars, where immense gravitational pressure and temperature conditions foster the fusion of light elements into heavier ones.

Key Nuclear Reactions

  • Proton-Proton Chain (PP Chain): Dominant in stars with masses less than 1.5 solar masses. Hydrogen atoms fuse to form helium nuclei, releasing energy.
  • CNO Cycle: Occurs in more massive stars. Carbon, nitrogen, and oxygen isotopes catalyze the fusion of hydrogen into helium.
  • 3α Process: Fusion of three helium nuclei to form a carbon nucleus, releasing significant energy.

Contribution to Stellar Evolution

Nuclear reactions play a crucial role in stellar evolution by:

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