This paper describes the discovery of the dwarf planet Makemake in 2005. Makemake is the second brightest object in the Kuiper Belt after Pluto and is the third brightest trans-Neptunian object after Pluto and Eris. The paper discusses the discovery process, the characteristics of Make
Makemake is a dwarf planet orbiting the Sun in the Kuiper belt, a disc of icy bodies beyond the orbit of Neptune. It is the fourth largest dwarf planet and trans-Neptunian object in the Solar System, having a diameter 60% that of Pluto. It was discovered on March 31, 2005, by American astronomers Michael E. Brown, Chad Trujillo, and David Rabinowitz at Palomar Observatory. As one of the largest objects found by this team, the discovery of Makemake contributed to the reclassification of Pluto as a dwarf planet in 2006.