The discussion centers on the formation of the largest stars and smallest galaxies from primordial hydrogen. It suggests that the largest stars, exceeding 200 solar masses, were abundant but have long since exploded as supernovae. These early supernovae are crucial for explaining cosmic reionization and the creation of black hole seeds for quasars. The earliest structures, likely globular clusters, played a significant role in galaxy formation, with the Jeans mass influencing the collapse of protogalactic clouds. Ultimately, the formation of massive bodies is limited by isothermal collapse and subsequent fragmentation into smaller clouds, halting further growth.