LMC star clusters are groups of stars located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way. These clusters are important for studying stellar evolution, as they contain stars of similar age and composition. The LMC hosts both open clusters, which are loosely bound and contain younger stars, and globular clusters, which are tightly bound and older. The LMC is home to several well-known star clusters, such as NGC 1866 and NGC 2070, the latter of which includes the famous Tarantula Nebula. Observing these clusters helps astronomers understand the formation and development of galaxies, as well as the life cycles of stars.