The history of Earth

The Earth is about 4.5 billion years old. In 1956 the geochemist Clair Patterson measured this age at 4.55 billion years1. His method rests on uranium, which slowly turns into lead at a known rate. By measuring the lead that the uranium in a sample has produced, one calculates the time elapsed since the sample formed. Patterson made this measurement in meteorites and in ocean sediments, which mix the lead of the whole planet; both give the same age, so the Earth was born at the same time as the meteorites1.

The oldest known piece of the Earth is a grain of zircon, a very resistant mineral, found in Western Australia. It crystallised 4.4 billion years ago, 150 million years after the Earth formed. Zircon grains survive the erosion of their original rock and end up in rocks younger than themselves; this one was found in such a rock. In 2014 Valley and colleagues located the grain's lead atoms one by one and checked that they had stayed in place. Had they moved, the measurement of its age would have been wrong2.

Almost all rocks dating from 4.4 to 4.02 billion years ago have disappeared. In 2014 Marchi and colleagues attributed this disappearance to asteroid impacts, which they simulated3. In their model, repeated impacts melt the surface rock, stir it and bury it under flows of molten rock. The largest collisions there also boil away the oceans already present, until about 4 billion years ago3. The oldest precisely dated rock, the Acasta gneiss in north-western Canada, dates from the end of this period. According to Reimink and colleagues, in 2016, it is 4.02 billion years old, to within 2 million years4.

Today the Earth's crust is divided into plates that move: this is plate tectonics. From 3.9 to 3.4 billion years ago, the crust was still a single, motionless piece. Tarduno and colleagues established this in 2023 from zircons from South Africa5. These zircons contain tiny grains of magnetite, a mineral that becomes magnetised as it cools, all the more strongly as the Earth's magnetic field is intense at that moment. The intensity of this field depends on latitude. The magnetite grains dating from 3.9 to 3.4 billion years ago almost all carry the same magnetisation. Tarduno and colleagues deduce that the original rocks of these zircons did not change latitude during this period. Zircons from Western Australia, measured earlier, show the same intensity5. Plate tectonics therefore began after 3.4 billion years ago. Before this result, estimates of that date ranged from the Hadean to the Proterozoic5.

The editors of Genes.media sort the events of this site's timeline onto one of two pages, according to what characterises them best. Those that concern the planet above all, its formation, its air and its climate, are on this page. The build-up of oxygen in the air is one of them, although bacteria caused it. The others are on the page "The history of life".

References for this introduction

  1. Patterson (1956), Geochimica et Cosmochimica Acta · Age of meteorites and the earthdoi:10.1016/0016-7037(56)90036-9
  2. Valley et al. (2014), Nature Geoscience · Hadean age for a post-magma-ocean zircon confirmed by atom-probe tomographydoi:10.1038/ngeo2075
  3. Marchi et al. (2014), Nature · Widespread mixing and burial of Earth's Hadean crust by asteroid impactsdoi:10.1038/nature13539
  4. Reimink et al. (2016), Nature Geoscience · No evidence for Hadean continental crust within Earth's oldest evolved rock unitdoi:10.1038/ngeo2786
  5. Tarduno et al. (2023), Nature · Hadaean to Palaeoarchaean stagnant-lid tectonics revealed by zircon magnetismdoi:10.1038/s41586-023-06024-5

18 milestones kept out of 200, grouped into 8 chapters

Hadean4.54 Ga → 4.03 Ga

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Mesoarchean3.2 Ga → 2.8 Ga

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Paleoproterozoic2.5 Ga → 1.6 Ga

  • 04
    The Great Oxidation Event~2.4 billion years ago

    Oxygen accumulated in the Earth's atmosphere and stayed there for the first time about 2.4 billion years ago, after hundreds of millions of years in which iron, volcanic gases and rock absorbed it as fast as microbes produced it.

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Mesoproterozoic1.6 Ga → 1 Ga

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Neoproterozoic1 Ga → 539 Ma

  • 06
    Snowball Earth~717 to 635 million years ago

    Snowball Earth is the name of two glaciations of the Cryogenian period, between 717 and 635 million years ago, during which ice sheets reached the sea at every latitude, the tropics included.

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Paleozoic539 Ma → 252 Ma

  • 07
    The Late Palaeozoic Ice Age~360 to 260 million years ago

    The Late Palaeozoic Ice Age is the span of about a hundred million years, late in the Palaeozoic era of 539 to 252 million years ago, during which ice sheets spread repeatedly over much of Gondwana, formed by today's southern continents.

  • 08
    Pangaea~335 to 175 million years ago

    Pangaea was a supercontinent that united nearly all the land in a single mass from pole to pole, surrounded by a single ocean, Panthalassa, with an interior a thousand kilometres from any coast, from 335 to 175 million years ago.

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Mesozoic252 Ma → 66 Ma

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Cenozoic66 Ma → 2026

  • 11
    The Freezing of Antarctica~34 million years ago

    Atmospheric carbon dioxide fell, about 34 million years ago, below the level at which ice can survive an Antarctic summer, and an ice sheet spread across the continent in about eight hundred thousand years.

  • 12
    The Quaternary Ice Ages~2.6 million to 11,700 years ago

    Ice sheets have grown and melted over North America and northern Europe dozens of times during the last 2.6 million years, to the rhythm of the Milankovitch cycles, slow variations in the Earth's orbit and axis.

  • 13
    The Industrial Revolution1750 to 1950 CE

    The Industrial Revolution, from 1750, returned to the atmosphere within decades carbon buried over hundreds of millions of years, and corals and tree rings recorded the industrial warming year by year.

  • 14
    James Hutton and Deep Time1788 CE

    James Hutton examined two sets of rock layers meeting at right angles at Siccar Point, on the Scottish coast, in 1788, and inferred from them a sequence of events too long for any short chronology, which is the idea of deep time.

  • 15
    The Great Accelerationsince 1950 CE

    The Great Acceleration is the sharp and simultaneous rise, after 1950, of some two dozen measures of human activity and of the Earth's response, from population and energy to carbon dioxide and plastics.

  • 16
    The Age of the Earth1956 CE

    Clair Patterson obtained 4.55 billion years for the age of the Earth in 1956, by measuring the lead in meteorites and in deep-ocean sediment.

  • 17
    Seafloor Spreading and Magnetic Stripes1963 to 1968 CE

    Sea-floor spreading, in which rock forms at the mid-ocean ridges and is carried away on both sides, was demonstrated between 1963 and 1968 from magnetic stripes that mirror one another on either side of those ridges.

  • 18
    The EPICA Dome C Ice Core2004 CE

    The EPICA Dome C ice core, three kilometres of Antarctic ice read layer by layer since 2004, contains bubbles of ancient air sealed as the snow compacted, and gives past temperature and carbon dioxide side by side.

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