The silicon-burning process remains exothermic beyond iron due to the fusion of alpha particles with heavier nuclei, which continues to release energy despite decreasing energy output with each step. While iron is the endpoint for significant energy release in stellar fusion, the binding energy of silicon and tin allows for energy generation through intermediate reactions. The binding energy per nucleon peaks at iron, but the addition of alpha particles, which have a lower binding energy, still results in net energy release up to tin-116. This process illustrates that energy can be produced even when the resulting nuclei have lower binding energy per nucleon than the starting materials. Ultimately, while the production of elements beyond nickel is minimal, the fusion process can still yield energy until reaching tin.