Discipline

Cosmology

Lessons across the journey that lean on cosmology, in the order they appear in the story.

  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.

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  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.

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  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.

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  4. 1.4
    The afterglow

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

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  5. 1.5
    How we know

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

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  6. 1.6
    The Dark Ages and the first light

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

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  7. 1.7
    Open questions

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

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  8. 2.1
    Gravity versus pressure

    How a cloud of gas collapses, heats and ignites.

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  9. 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.

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  10. 2.4
    Galaxies

    Cities of stars, dark matter and the cosmic web.

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  11. 2.5
    Reading starlight

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

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  12. 3.1
    Where the elements come from

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

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  13. 3.2
    Making gold

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

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  14. 3.5
    Molecules in space

    Dust, ice and organic molecules between the stars.

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  15. 3.7
    Are you really made of stardust?

    The famous claim, tested element by element.

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  16. 9.5
    Leaving Earth

    Space is one of the most valuable things we do, and almost all of its value points back at Earth.

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  17. 9.6
    The deep future

    Earth has about a billion years of biosphere left, not five, and that is only the first paragraph.

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