Formation of the Solar System: Birth of the Sun and Planets
The Sun ignited at the centre of a spinning disc of gas and dust, and within tens of millions of years the planets, moons, asteroids and comets had formed.
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The Sun ignited at the centre of a spinning disc of gas and dust, and within tens of millions of years the planets, moons, asteroids and comets had formed.
A layered rocky planet with an iron core, a silicate mantle and an early crust emerged, opening the Hadean Eon.
Debris from a collision between the proto-Earth and a planet-sized body gathered in orbit to form the Moon, which has accompanied Earth ever since.
Liquid water collected on Earth's cooling surface, forming the first oceans, which have persisted in some form ever since.
Large impacts formed many of the Moon's great basins; whether they came in a sudden late spike or as the tail of a steady decline is still debated.
Earth gained stable continental crust, oceans and widespread microbial life, setting the stage for the oxygenation of the atmosphere.
Simple single-celled microbes appeared, the ancestors of all living things; how non-living chemistry became life is still unresolved.
A proposed Neoarchean supercontinent whose existence is still debated; its suggested breakup after about 2.5 billion years ago is marked by large swarms of volcanic dykes.
Iron-rich sediments deposited in oxygen-poor oceans that now record the rise of oxygen and supply most of the world's iron ore.
Earth gained an oxygenated atmosphere, complex eukaryotic cells and multicellular life, ending with the first animals just before the Cambrian.
Repeated glaciations left tillites on several continents and coincided with the first lasting rise of atmospheric oxygen.
Free oxygen became a lasting part of Earth's atmosphere, transforming the chemistry of rocks, oceans and life.