Minor planets are small, irregularly shaped celestial bodies that orbit a star, typically residing within the solar system. These objects vary widely in size and composition, ranging from tiny dust particles to bodies comparable in size to small moons. Many minor planets are classified as asteroids, which are primarily composed of rock and metal, and they are often found concentrated in the main belt between the orbits of the two largest planets. The understanding of these objects is crucial for understanding the early formation and evolution of the solar system, as their compositions and orbits reflect primordial material that has not undergone significant planetary differentiation. Detecting and studying these bodies provides insight into fundamental processes of accretion, gravitational dynamics, and planetary formation.