Nuclear fusion is the process that powers the sun and other stars. Essentially, it involves the combination of lighter atomic nuclei to form a heavier nucleus. During this process, a tremendous amount of energy is released. This energy release occurs because the mass of the resulting nucleus is slightly less than the sum of the original nuclei. This difference in mass is converted into energy according to Einstein's equation,
\[ E = mc^2 \].
This is the principle behind nuclear fusion.
- Fusion happens naturally in stars due to the extremely high temperatures and pressures found in their cores.
- Scientists are working to replicate fusion on Earth as a potential source of clean energy.
Replicating these conditions on Earth is incredibly challenging, requiring advanced technology and materials capable of withstanding extreme conditions.