Science, Tech, Math › Science Explore the Dwarf Planet Haumea Share Flipboard Email Print Lexicon / Wikimedia Commons / Public Domain Science Astronomy An Introduction to Astronomy Important Astronomers Solar System Stars, Planets, and Galaxies Space Exploration Chemistry Biology Physics Geology Weather & Climate By Carolyn Collins Petersen Astronomy Expert M.S., Journalism and Mass Communications, University of Colorado - Boulder B.S., Education, University of Colorado Carolyn Collins Petersen is an astronomy expert and the author of seven books on space science. She previously worked on a Hubble Space Telescope instrument team. our editorial process Facebook Facebook Carolyn Collins Petersen Updated January 31, 2020 There's an odd little world in the outer solar system called 136108 Haumea, or Haumea (for short). It orbits the Sun as part of the Kuiper Belt, far beyond the orbit of Neptune and in the same general region as Pluto. Planet searchers have been observing that region for years now, looking for other worlds. It turns out there are many of them out there, but none have been found (yet) as weird as Haumea. It's less like a sedately orbiting planet and more like a wildly spinning top. It lopes around the Sun once every 285 years, whirling madly, end over end. The motion tells planetary scientists Haumea was sent into that propeller-like orbit by a collision with another body sometime in the past. Stats For a tiny world out in the middle of nowhere, Haumea presents some striking statistics. It's not very big and its shape is oblong, like a fat cigar that is 1920 kilometers long, about 1,500 km wide and 990 kilometers thick. It spins on its axis once every four hours. Its mass is about a third of Pluto's, and planetary scientists classify it as a dwarf planet, similar to Pluto. It's more properly listed as a plutoid due to its ice-rock composition and its position in the solar system in the same region as Pluto. It has been observed for decades, although not recognized as a world until its "official" discovery in 2004 and the announcement in 2005. Mike Brown, of CalTech, was set to announce his team's discovery when they were beaten to the punch by a Spanish team who claimed to have seen it first. However, the Spanish team apparently accessed Brown's observing logs just before Brown was set to make his announcement and they claim to have "discovered" Haumea first. The International Astronomical Union (IAU) credited the observatory in Spain for the discovery, but not the Spanish team. Brown was given the right to name Haumea and its moons (which his team discovered later). Collision Family The fast, spinning motion that flips Haumea around as it orbits the Sun is the result of a long-ago collision between at least two objects. It's actually a member of what's called a "collisional family," which contains objects all created in an impact that took place very early in the solar system's history. The impact shattered the colliding objects and might also have removed much of primordial Haumea's ice, leaving it a large, rocky body with a thin layer of ice. Some measurements indicate that there is water ice on the surface. It appears to be fresh ice, meaning it was deposited within the past 100 million years or so. Ices in the outer solar system are darkened by ultraviolet bombardment, so fresh ice on Haumea implies some kind of activity. However, no one is sure what that would be. More studies are needed to understand this spinning world and its bright surface. Moons and Possible Rings Small as Haumea is, it's large enough to have moons (satellites that orbit around it). Astronomers spotted two of them, called 136108 Haumea I Hi'iaka and 136108 Hamuea II Namaka. They were found in 2005 by Mike Brown and his team using the Keck Observatory on Maunakea in Hawai'i. Hi'iaka is the outermost of the two moons and is only 310 kilometers across. It appears to have an icy surface and it might be a fragment of the original Haumea. The other moon, Namaka, orbits closer to Haumea. It's only about 170 kilometers across. Hi'iaka orbits Haumea in 49 days, while Namaka takes only 18 days to go once around its parent body. In addition to the small moons, Haumea is thought to have at least one ring surrounding it. No observations have conclusively confirmed this but eventually, astronomers should be able to detect traces of it. Etymology Astronomers who discover objects get the pleasure of naming them, according to guidelines set up by the International Astronomical Union. In the case of these distant worlds, the IAU's rules suggest that objects in the Kuiper Belt and beyond should be named after mythological beings associated with creation. So, the Brown team went to Hawaiian mythology and selected Haumea, who is the goddess of the island of Hawai'i (from where the object was discovered using the Keck telescope). The moons are named after Haumea's daughters. Further Exploration It's not too likely that a spacecraft would be sent to Haumea in the near future, so planetary scientists will continue to study it using ground-based telescopes and space-based observatories such as Hubble Space Telescope. There have been some preliminary studies aimed at developing a mission to this distant world. It would take astronauts nearly 15 years to arrive there. So far, there are no concrete plans for a Haumea mission, although it would certainly be an interesting world to study up close!