Why does the sun shine?

Physics

Scientific paper

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Stellar Characteristics And Properties, Solar Physics, Radiation Mechanisms, Polarization

Scientific paper

In order to understand the fundamental properties of a star in radiative equilibrium, a simplified model is introduced which yields relations for physical quantities by elementary methods. In particular, the dependence of these quantities on the parameters of the star and on the fundamental constants of nature is exhibited. Numerical evaluation of these relations is in good agreement with observation and with more elaborate calculations.

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