The journey

Eight thresholds, one future, 60 lessons

Each threshold is a moment when the universe crossed into a new kind of complexity: stars, elements, planets, life, minds, farms, machines. The last chapter looks past the present. Read them in order, or jump to the one you are curious about.

Threshold 1: The Big Bang · 13.8 billion years ago · 13.8 billion years ago to the first atoms

  1. 1.1
    Was the Big Bang an explosion?

    The Big Bang was not a blast at a point in empty space. It was the whole universe, everywhere at once, hot and dense and beginning to expand.

    Draft
  2. 1.2
    The first three minutes

    How quarks became protons and neutrons, and how the first nuclei formed before the universe was twenty minutes old.

    Draft
  3. 1.3
    Why is the night sky dark?

    A dark night sky is evidence that the universe has a finite age and is expanding.

    Draft
  4. 1.4
    The afterglow

    The cosmic microwave background, the oldest light there is, and what its faint ripples tell us.

    Draft
  5. 1.5
    How we know

    The three pillars of evidence for the Big Bang, and how each one could have proved it wrong.

    Draft
  6. 1.6
    The Dark Ages and the first light

    A hundred million years of darkness, and then the first stars switch on.

    Draft
  7. 1.7
    Open questions

    Dark matter, dark energy and inflation: what the standard model of cosmology cannot yet explain.

    Draft

Threshold 2: Stars light up · 13.6 billion years ago · About 13.6 billion years ago onward

  1. 2.1
    Gravity versus pressure

    How a cloud of gas collapses, heats and ignites.

    Draft
  2. 2.2
    What a star is

    Fusion in the core balanced against gravity: the equilibrium that lets a star shine for billions of years.

    Planned
  3. 2.3
    The lives of stars, sorted by mass

    Why a star's mass decides everything: how long it lives, how it dies and what it leaves behind.

    Draft
  4. 2.4
    Galaxies

    Cities of stars, dark matter and the cosmic web.

    Planned
  5. 2.5
    Reading starlight

    Spectra, distances and the cosmic distance ladder: how we measure things we can never visit.

    Planned
  6. 2.6
    The Sun, a typical star

    Our own star as an ordinary star, with Aditya-L1 as India's eye on it.

    Planned
  7. 2.7
    One chart for every star

    The Hertzsprung–Russell diagram, which organises every star by brightness and temperature.

    Planned

Threshold 3: New chemical elements · 13.5 billion years ago · From the first supernovae onward

  1. 3.1
    Where the elements come from

    Stellar nucleosynthesis: how stars build carbon, oxygen and iron.

    Draft
  2. 3.2
    Making gold

    Supernovae and neutron-star mergers, the violent events that make the heaviest elements.

    Planned
  3. 3.3
    The periodic table as a history book

    Every element has an origin story; the periodic table arranged by where each one was made.

    Planned
  4. 3.4
    Why carbon?

    Bonding, chains and rings: why carbon chemistry is the chemistry of complexity.

    Planned
  5. 3.5
    Molecules in space

    Dust, ice and organic molecules between the stars.

    Planned
  6. 3.6
    From quarks to the Higgs

    The fundamental particles and the four forces that shape matter.

    Draft
  7. 3.7
    Are you really made of stardust?

    The famous claim, tested element by element.

    Planned

Threshold 4: Earth and the solar system · 4.57 billion years ago · 4.57 billion years ago onward

  1. 4.1
    From nebula to planets

    How the solar system assembled from a disc of gas and dust.

    Draft
  2. 4.2
    Earth's violent birth

    The Moon-forming impact and the magma ocean.

    Planned
  3. 4.3
    Core, mantle, crust

    Differentiation: how the Earth sorted itself into layers.

    Draft
  4. 4.4
    Plate tectonics and the Himalaya

    The engine of a living planet, told through the Indian plate and the rise of the Himalaya.

    Planned
  5. 4.5
    Oceans and air

    Where the water and the atmosphere came from.

    Planned
  6. 4.6
    Deep time

    Radiometric dating: how we know the age of a rock.

    Planned
  7. 4.7
    Earth as a system

    Rock, water, air and life as one connected machine.

    Planned

Threshold 5: Life on Earth · 3.5 billion years ago · At least 3.5 billion years ago onward

  1. 5.1
    What is life?

    Definitions of life, and the last universal common ancestor of everything alive today.

    Planned
  2. 5.2
    How chemistry became biology

    The hypotheses and evidence for the origin of life.

    Draft
  3. 5.3
    Evolution by natural selection

    The mechanism, stated precisely, and the evidence that it works.

    Planned
  4. 5.4
    The Great Oxidation Event

    How microbes remade the planet's atmosphere.

    Planned
  5. 5.5
    The complex cell

    Endosymbiosis and the origin of the eukaryotic cell.

    Planned
  6. 5.6
    The Cambrian explosion

    Animal body plans appear in the fossil record.

    Planned
  7. 5.7
    Mass extinctions

    Five great dyings and the age of reptiles.

    Planned
  8. 5.8
    Mammals in the shadows

    How small mammals survived the dinosaurs and inherited the Earth.

    Draft

Threshold 6: Collective learning · 300,000 years ago · About 7 million years ago to 12,000 years ago

  1. 6.1
    Primates and hominins

    The family tree from the first primates to the hominins.

    Draft
  2. 6.2
    From habilis to sapiens

    Homo habilis, Homo erectus and the arrival of our species.

    Draft
  3. 6.3
    Fire, tools and cooking

    Stone tools, controlled fire and the cooking hypothesis.

    Planned
  4. 6.4
    Language and symbolic thought

    The evidence for language and the first art.

    Planned
  5. 6.5
    Collective learning

    Why humans, alone among species, accumulate knowledge across generations.

    Planned
  6. 6.6
    Out of Africa, into India

    The peopling of the world, including the early routes into the subcontinent.

    Planned
  7. 6.7
    Foraging lifeways

    How people lived for most of human history.

    Planned

Threshold 7: Agriculture · 12,000 years ago · About 12,000 years ago to 1500 CE

  1. 7.1
    Why farm?

    Climate, population and the Holocene: why farming began where and when it did.

    Draft
  2. 7.2
    Domestication

    How wheat, rice, cattle and dogs were remade by people, and people by them.

    Planned
  3. 7.3
    Villages to cities

    Surplus, hierarchy, writing and the first states.

    Draft
  4. 7.4
    The Indus Valley civilisation

    Cities, water engineering and a script still unread.

    Planned
  5. 7.5
    The price of farming

    Disease, inequality and shorter lives: what agriculture cost.

    Planned
  6. 7.6
    Empires and exchange

    Agrarian empires, the Silk Road and the Indian Ocean world.

    Planned

Threshold 8: The modern revolution · 275 years ago · About 1500 CE to the present

  1. 8.1
    The Columbian Exchange

    1492 and the joining of the world's biological and human systems.

    Planned
  2. 8.2
    The Scientific Revolution

    A new way of knowing: evidence, instruments and doubt.

    Planned
  3. 8.3
    Fossil fuels and the Industrial Revolution

    Coal, steam and the release of stored sunlight.

    Planned
  4. 8.4
    The Great Acceleration

    Population, energy and information since 1950.

    Planned
  5. 8.5
    The Anthropocene

    Humans as a geological force.

    Planned

What comes next · The present to the deep future

  1. 9.1
    The next century: climate

    What the climate models say, what is settled, what is not, and what is still up to us.

    Planned
  2. 9.2
    Energy after fossil fuels

    Sun, wind, atoms and storage: the transition that decides what the next century looks like.

    Planned
  3. 9.3
    Machines that learn

    Artificial intelligence, and whether it counts as a new kind of collective learning.

    Planned
  4. 9.4
    Editing life

    Biotechnology, from vaccines to gene editing, and what it means to steer evolution on purpose.

    Planned
  5. 9.5
    Leaving Earth

    Space as a place to live, and the physics that makes it hard.

    Planned
  6. 9.6
    The deep future

    From the year 3000 to the death of the Sun and the fate of the universe.

    Planned