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The heat emitted from a star is generated through the fusion of hydrogen to form helium in its core, leading to the outward flow of energy in the form of electromagnetic radiation.
The source of the heat emitted from a star is the fusion of hydrogen to form helium. This process occurs in the core of the star and releases a tremendous amount of energy, which then moves outward through the star's layers to its outer surface.
The energy emitted from a star is in the form of electromagnetic radiation, including visible light, heat, ultraviolet light, and radio waves. This energy transfer is vital for maintaining the star's temperature and brightness.
Stefan-Boltzmann law describes the energy flux from a star, showing that the power radiated by a star is proportional to the fourth power of its absolute temperature.
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