The Big Bang theory is the prevailing cosmological model for the observable universe. It states that the universe originated from a single, extremely dense and hot point, and has been expanding and cooling ever since.
The cosmic microwave background (CMB) radiation is the afterglow of the Big Bang. It is a faint glow of light that fills the universe and provides crucial evidence for the Big Bang theory.
Dark matter and dark energy are two mysterious components that make up the majority of the universe's mass-energy content. Dark matter is invisible and detectable only through its gravitational effects, while dark energy is thought to be responsible for the accelerated expansion of the universe.
Cosmology studies the formation and evolution of galaxies, including how they are distributed in the universe and how they have changed over cosmic time.
Cosmologists develop mathematical models to describe the universe's behavior and predict its future. These models often include concepts such as inflation, cosmic inflation, and the multiverse.
Observational cosmology involves using telescopes and other instruments to study the universe and gather data that can be used to test cosmological theories and models.
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