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Cosmic epoch · Cosmology

The Big Bang

Cosmology & UniverseEstablished Science

Definition

The hot, dense early state from which the observable Universe has been expanding for about 13.8 billion years.

Scientific overview

The Big Bang is not an explosion in space but an expansion of space itself from an extremely hot, dense beginning. The framework explains the expansion of the Universe, the abundances of the light elements, and the cosmic microwave background — three independent lines of evidence that together make it the foundation of modern cosmology.

Historical development

Georges Lemaître proposed an expanding Universe from a 'primeval atom' in 1927–1931; the discovery of the cosmic microwave background in 1965 confirmed the hot early state and settled the debate with the rival Steady State model.

Evidence

  • The observed expansion of the Universe
  • The cosmic microwave background
  • The primordial abundances of hydrogen, helium, and lithium

Open questions

  • What set the initial conditions?
  • What preceded the hot Big Bang, if anything?

Rests on

Predicts

Related discoveries & objects

Related scientists

Knowledge connections

Sources & references

The primary and reference sources this topic draws on.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.

  • Planck CollaborationESA Planck mission / Planck Collaboration

    Cosmic microwave background maps and the cosmological parameters of the ΛCDM model.