Quasars are extremely bright astronomical objects powered by supermassive black holes at the centers of galaxies, surrounded by active accretion disks primarily composed of hydrogen and helium. The immense electromagnetic radiation emitted by quasars results from gravitational compression and friction within the accretion disk, which efficiently converts mass into energy. This process can convert up to 10% of the disk's mass into energy, making quasars visible across vast distances. As galaxies mature, their supermassive black holes may enter a dormant state once their accretion disks are depleted, but they can be reactivated through galactic mergers. Ultimately, while black holes can theoretically evaporate over time, they do not recycle matter back into the universe.