One of the central concepts in cosmology is the Big Bang theory, which proposes that the universe originated from a single, incredibly dense and hot point about 13.8 billion years ago. This event marked the beginning of the expansion of the universe and the creation of all matter and energy.
The cosmic microwave background radiation is a key piece of evidence supporting the Big Bang theory. It is a faint glow of light that fills the universe and is a remnant of the intense heat from the early universe.
Cosmologists study the presence and effects of dark matter and dark energy, which are thought to make up the majority of the universe's mass and energy. Although these components cannot be directly observed, their influence on the dynamics of the cosmos is significant.
Observational cosmology involves the use of telescopes and other instruments to study the properties and behavior of celestial objects, such as galaxies, stars, and cosmic phenomena like supernovae and black holes.