Quasars are extremely luminous objects powered by supermassive black holes (SMBHs) that are actively accreting matter, emitting significant light in the process. They are typically found at great distances, indicating they were more common in the early universe when SMBHs were growing rapidly. The accretion occurs from a disk of matter, although the exact structure and dynamics of these disks remain unclear. Not all galaxies host SMBHs, and while many do, the Milky Way's black hole is relatively small compared to those powering quasars. The mechanisms behind the feeding process of quasars and how it eventually ceases are still subjects of ongoing research.