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The Big Bang theory predicts that the early universe was a very hot place and that as it expands, the gas within it cools. Thus the universe should be filled with radiation that is literally the remnant heat left over from the Big Bang, called the “cosmic microwave background", or CMB.
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Big Bang Chronology, the chronology of the Universe, probably the past and future of the universe according to the big bang cosmology. Explains how the universe has developed according to dominant models since the Planck age, using the parameters of cosmological coordinates. It is estimated that the expansion of the Universe started 13.8 billion years ago. [1] To summarize the chronology of the universe, it is appropriate to divide it into 4 main parts.
The History of the Universe - the gravitational waves hypothesis arises from cosmic inflation that expands faster than light immediately after the big bang.
In the very early stages of the universe, from the Planck era to cosmic inflation, or from the first picoseconds of cosmic time, this period is beyond the current understanding of experimental theory of change in the physics of change.
In the early universe, from the quark age to the photon age, or the first 380,000 years of cosmic time, familiar forces and fundamental problems arose, but the universe remained in the plasma state from 380,000 to 150 million years in the ensuing "dark age". In this case, although the universe was complete, it had not yet formed on large scales.
Nearly 150 million years of stellar evolution, galaxy formation and evolution, and the massive ordered structure, including the formation of galaxy clusters and superclusters, has survived to the present day. It took about 5 billion (9 Gya) years for our galaxy to form as a thin disk. [2] It took about 9.2 millennia (4.6 Gya) years for our solar system to form. It took about 9.8 billion (4 Gya) years for life to arise with this formation.
After the cessation of formation in the distant future, there are several types for the final part of the universe.
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