The particles which must fuse or stick together in the nuclei of atoms during nuclear reactions in stars are atoms of hydrogen.
During a nuclear fusion reaction that occurs in stars, the nuclei of two atoms will combine to form a new atom with a release of energy.
This nuclear reaction usually occur in the core of a star, and the particles involved include the following;
The reaction equation can be represented as;
[tex]H \ + \ H \ --> He + \ energy[/tex]
Thus, we can conclude that, the particles which must fuse or stick together in the nuclei of atoms during nuclear reactions in stars are atoms of hydrogen.
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