Universe Evolution

The evolution of the universe refers to how the cosmos has changed over time since its beginning approximately 13.8 billion years ago with the Big Bang. Initially, the universe was a hot, dense point that rapidly expanded, cooling and allowing particles to form. Over billions of years, these particles coalesced into stars, galaxies, and larger structures. The universe continues to expand, driven by mysterious forces like dark energy. Understanding this evolution helps us grasp the origin of matter, the formation of celestial bodies, and the ongoing development of the universe we observe today.