Dwarf planets are celestial bodies that orbit the sun and are similar to planets in terms of their composition and size, but have not cleared their orbital path of other debris. They are smaller than the eight recognized planets in our solar system, such as Pluto and Eris. The classification of dwarf planets was introduced by the International Astronomical Union in 2006 to differentiate them from traditional planets. These bodies are interesting to study because they offer insights into the formation and evolution of our solar system, as well as the dynamics of celestial bodies in space. Research on dwarf planets includes studying their surfaces, compositions, atmospheres, and orbits to better understand their characteristics and place in the solar system.