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A star produces its energy through the process of **nuclear fusion**. In deep inside the core of stars, enough protons collide into each other with enough speed and form a helium nucleus, generating a tremendous amount of energy at the same time. This process is called nuclear fusion.
The energy produced by nuclear fusion is what makes stars shine. The outflow of energy from the central regions of the star provides the pressure necessary to keep the star from collapsing under its own weight, and the energy by which it shines.
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