Start around 13.8 billion years ago. NASA's cosmic history timeline has two beats students often merge into one.
First, cosmic inflation: space expanded extremely fast for a tiny fraction of a second. Then inflation stopped, and the energy driving it transferred to matter and light. That transition is what cosmologists call the Big Bang.
From there the story is concrete. One second in, the universe is a hot soup of light and particles. Minutes later, nucleosynthesis builds hydrogen, helium, and traces of heavier light elements. Roughly 380,000 years later, atoms form, the fog clears, and the cosmic microwave background (CMB) is released. That glow is the oldest light we can observe.
WMAP and later missions measured tiny temperature ripples in that background. Those ripples became the scaffolding for galaxies. The theory's strength is matching that timeline to observation.