The "Cosmic Web" is a large-scale structure of the universe, consisting of galaxies and galaxy clusters interconnected by vast filaments of dark matter and gas. This intricate network resembles a web, with denser regions where galaxies are concentrated and voids where few galaxies exist. The Cosmic Web helps scientists understand the distribution of matter in the universe and the formation of galaxies. The formation of the Cosmic Web is influenced by the gravitational pull of dark matter, which is invisible and makes up a significant portion of the universe's mass. As the universe expands, matter clumps together, creating the web-like structure observed today. This model is essential for studying the evolution of the universe and the behavior of cosmic structures.