S1, E3: Continuing the story of the early universe by exploring various highlights; the formation of the first atoms at 370,000 years; the accretion of hydrogen and helium gas into protogalaxies; the collapse of the gas into ever denser balls.

S1, E3: Continuing the story of the early universe by exploring various highlights; the formation of the first atoms at 370,000 years; the accretion of hydrogen and helium gas into protogalaxies; the collapse of the gas into ever denser balls.