The Big Bang theory is the prevailing cosmological model for the observable universe from the earliest known periods through its subsequent large-scale evolution. According to this theory, the universe began as a hot, dense point and has been expanding and cooling ever since.
The cosmic microwave background (CMB) radiation is the afterglow of the Big Bang and is the oldest light in the universe. It provides crucial evidence supporting the Big Bang theory and helps us understand the early stages of the universe's evolution.
Dark matter is a form of matter that does not emit, absorb, or reflect light, making it invisible and detectable only through its gravitational effects on visible matter. It is believed to make up a significant portion of the total mass of the universe and plays a key role in the formation and structure of galaxies.
Dark energy is a mysterious force that is driving the accelerated expansion of the universe. Its nature is not well understood, but it is thought to constitute about 68% of the universe. The discovery of dark energy has led to a major shift in our understanding of the universe's ultimate fate.
Cosmology also involves the study of how galaxies form, evolve, and interact with each other over cosmic time. The distribution and properties of galaxies provide valuable insights into the underlying structure and dynamics of the universe.
Cosmologists explore various scenarios for the ultimate fate of the universe, including the possibilities of continued expansion, eventual contraction, or a "Big Freeze" as a result of dark energy's influence. Understanding the long-term evolution of the universe is a central concern in cosmology.