Approximately 13.72 billion years ago, the first star formed in the observable universe. Gravitational collapse of a gaseous nebula composed primarily of hydrogen and helium created this primordial star. Thermonuclear fusion of hydrogen into helium in the star's core generated energy that enabled it to shine. This event initiated stellar evolution, a process of stellar birth, life, and death. The first star and subsequent stars became building blocks for galaxies, star clusters, and other large-scale structures in the observable universe.