The Big Bang
How expansion and cooling transformed the early universe from a hot plasma into a transparent cosmos of atoms—and what its oldest light can tell us.
THE SERIES COMPANION
The sources behind the story.
Research, visual credits, and how each film is made.
24 films · Episodes and full chapters
How expansion and cooling transformed the early universe from a hot plasma into a transparent cosmos of atoms—and what its oldest light can tell us.
How the first stars formed from primordial gas, ended the cosmic dark ages, and began changing the universe around them.
Rotation curves, gravitational lensing, galaxy clusters, and the cosmic web reveal the effects of dark matter, while its identity remains unknown.
How stars and stellar explosions build the chemical elements, and why the heaviest nuclei require processes beyond ordinary fusion.
The complete first chapter brings together the early universe, the first stars, dark matter, and the stellar origins of the elements.
From a collapsing cloud to a young Sun and a disk of forming planets, with meteorites preserving the chronology of the Solar System’s birth.
What lunar samples and the Earth–Moon system reveal about the giant impact that most likely formed the Moon—and which details remain unsettled.
How the early Earth cooled, developed a crust and oceans, and left fragments of its first 500 million years in ancient zircon crystals.
How seafloor spreading, magnetic stripes, earthquakes, and subduction revealed a planet whose surface is continually rebuilt.
The complete second chapter follows the formation of the Solar System, the Moon-forming impact, the early Earth, and plate tectonics.
The early Earth’s chemical ingredients, energy gradients, membranes, and catalysts—and the settings in which nonliving chemistry could begin to acquire life’s capabilities.
RNA copying, chemical cycles, metabolism, and dividing compartments illuminate possible routes toward the first cells, along with the gaps experiments have yet to close.
How cells translate genetic information into proteins, why RNA sits at the heart of the ribosome, and what today’s shared genetic code reveals about its origins.
What the shared machinery of living cells reveals about LUCA, the last universal common ancestral population, and the deep split between bacteria and archaea.
The complete third chapter follows the chemistry of the early Earth through RNA, the genetic code, and the common ancestry of cellular life.
How microbes built Earth’s first ecosystems by using chemical energy and sunlight, cycling nutrients, and changing the chemistry of rock, water, and air.
Why oxygen accumulated long after oxygen-producing photosynthesis began, and how the Great Oxidation Event transformed the atmosphere, oceans, climate, and life.
The ancient partnership between an archaeon and a bacterium that gave rise to mitochondria, explored through living relatives, genomes, and competing models of the merger.
How meiosis reshuffles inheritance, what sexual reproduction costs, and the leading explanations for why sex persists across complex life.
How a cyanobacterium became a chloroplast, how photosynthetic partnerships spread through other cells, and how cells began forming multicellular bodies.
The evidence for the Cryogenian ice ages, the feedbacks that froze and thawed Earth, and the refuges where life may have endured.
The complete fourth chapter connects microbial ecosystems, oxygenation, mitochondria, sex, chloroplasts, multicellularity, and Snowball Earth.
The Ediacaran seafloor, from the fronds of Mistaken Point to mobile grazers, early reefs, and burrows, records the emergence of large and increasingly active organisms.
The Cambrian transformation of marine ecosystems: deeper burrows, skeletons, jointed legs, eyes, and predators, seen through Chengjiang and Burgess Shale fossils.
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BEHIND THE SERIES
Developed and directed by Anders Lunde, with AI-assisted research and production, text-to-speech narration, and custom scientific animation.
How the films are made →