The Big Bang Theory is the prevailing cosmological model for the observable universe from the earliest known periods through its subsequent large-scale evolution.
Several lines of evidence support the Big Bang Theory, including the cosmic microwave background radiation, the abundance of light elements, and the large-scale structure of the universe.
The discovery of cosmic microwave background radiation in 1964 provided strong evidence for the Big Bang. This radiation is the residual heat from the early universe and is detected uniformly in all directions.
The Big Bang Theory accurately predicts the abundance of elements such as hydrogen, helium, and lithium in the universe. The observed ratios of these light elements align with the predictions of the theory.
Observations of the large-scale distribution of galaxies and the expansion of the universe also support the Big Bang Theory. The redshift of distant galaxies indicates that the universe is expanding, consistent with the predictions of the theory.
According to the Big Bang Theory, the universe has undergone several key phases, including cosmic inflation, the formation of subatomic particles, the formation of atoms, the formation of galaxies and stars, and the evolution of the universe to its current state.
The Big Bang Theory provides a comprehensive and well-supported framework for understanding the origin and evolution of the universe. Its predictions and evidence have been instrumental in shaping our current understanding of cosmology and the nature of the cosmos.
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