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Big Bang

Physical theory

The Big Bang is a physical theory that describes how the universe expanded from an initial state of high density and temperature. Various cosmological models based on the Big Bang concept explain a broad range of phenomena, including the abundance of light elements, the cosmic microwave background (CMB) radiation, and large-scale structure. The uniformity of the universe, known as the horizon and flatness problems, is explained through cosmic inflation: a phase of accelerated expansion during the earliest stages. Detailed measurements of the expansion rate of the universe place the Big Bang singularity at an estimated 13.787±0.02 billion years ago, which is considered the age of the universe. A wide range of empirical evidence strongly favors the Big Bang event, which is now widely accepted.

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Timeline
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  • 1912Vesto Slipher measured the first Doppler shift of a "spiral nebula."
  • 1922Alexander Friedmann introduced the concept of an expanding universe with the Friedmann equations.
  • 1924Edwin Hubble's measurement of the great distance to the nearest spiral nebulae showed they were other galaxies.
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