Cygnus X-1 is an astrophysical source renowned for its intense, persistent emissions of X-rays. It is classified as a high-mass X-ray binary system, consisting of a compact object orbiting a massive stellar companion. In this configuration, matter is stripped from the companion star and gravitationally funneled toward the compact object, forming an accretion disk. The extreme gravitational forces and friction generated as material spirals inward accelerate the plasma to near relativistic speeds. This accretion process converts gravitational potential energy into thermal energy, resulting in the powerful radiation detectable across the electromagnetic spectrum, with the X-ray emissions being the most signature characteristic of the system.