Haumea is a dwarf planet located in the Kuiper Belt, a region of the outer solar system. It was discovered in 2004 by a team of astronomers led by Mike Brown of the California Institute of Technology. Haumea is unique among the known dwarf planets due to its elongated shape, rapid rotation, and two small moons.
Haumea is approximately the same size as Pluto, with a diameter of about 1,500 kilometers. Its elongated shape is thought to be the result of a high-speed collision with another object in the distant past. This collision likely caused Haumea to spin rapidly, completing a full rotation in just under four hours. Haumea's surface is covered in a layer of crystalline water ice, giving it a bright and reflective appearance.
Haumea is known to have two small moons, Hi'iaka and Namaka, which were discovered in 2005 and 2006, respectively. These moons are thought to be fragments of Haumea resulting from the collision that gave the dwarf planet its unusual shape.