Ceres is a dwarf planet located within the asteroid belt in the main solar system. It is the largest body in this belt and is primarily composed of a mix of rock and water ice, suggesting a geological history involving significant thermal activity. Its surface exhibits varying topography, including large basins and possible evidence of past cryovolcanic processes. The body maintains a distinct orbital path, and its study provides critical insights into the composition and evolutionary processes of celestial bodies that formed in the early solar system.