Jupiter-family comets are a group of comets that have short orbital periods and are thought to originate from the Kuiper Belt or the scattered disc in the outer solar system. These comets have orbits that are influenced by the gravitational pull of Jupiter, resulting in periodic returns to the inner solar system. Jupiter-family comets typically have orbital periods of less than 20 years and are characterized by bright, active nuclei when they approach the Sun. They are a valuable research target for studying the composition and dynamics of cometary nuclei, as well as the processes involved in the formation and evolution of the solar system.