Couldn't find element LayerAd

Error finding content

Haumea, Icy Dwarf Planet in Kuiper Belt: Discovery and Composition - Windows to the Universe

Shop Windows to the Universe

Warnings: The True Story of How Science Tamed the Weather by Mike Smith tells the story of our storm warning system. See our online store book collection.
This is an artist's impression of the dwarf planet Haumea and its two moons Hi'iaka and Namaka. Notice how Haumea's rapid rotation has stretched it into an elliptical (not spherical) shape.
Click on image for full size
Images courtesy of NASA, ESA, and A. Feild (STScI).

Haumea (dwarf planet)

Haumea is a dwarf planet in our Solar System. Haumea is the fifth object officially classified as a dwarf planet; the previous four are Pluto, Eris, Ceres, and Makemake. The International Astronomical Union announced Haumea's official status as a dwarf planet in September 2008.

Haumea is a large Kuiper Belt Object (KBO) that orbits far from the Sun on the frozen fringes of our Solar System. Because it is so far away, Haumea takes 285 years to orbit the Sun once! On average, Haumea is about 10% further from the Sun than Pluto, though both of these dwarf planets move closer to and further from the Sun as they go around.

Haumea is smaller than both Pluto and Eris. Haumea is not spherical. Haumea rotates so rapidly that it has been stretched into the shape of an ellipsoid (3D ellipse). This strange body measures 1,960 km (1,218 miles) along its longest axis, but only about half that - 996 km (619 miles) - along its shortest.

The "days" are really short on Haumea. This odd object spins around in less than four hours! That is the shortest rotation period of any known Solar System object larger than 100 km. Haumea is also relatively dense, tipping the scales at 2.6 to 3.3 g/cm3. That probably means it is made mostly of rock, which is somewhat odd since most KBOs have quite a bit of ice (which is less dense) in them. Haumea has known moons, both discovered in 2005. They are named Hi'iaka and Namaka.

Astronomers have a theory that links Haumea's rapid rotation, odd shape, and strange composition. They believe Haumea collided with another large object sometime in the distant past. The collision set Haumea spinning, giving it its odd shape. Outer layers of lightweight ice would have been more easily knocked loose by the collision, leaving behind denser rocks. Haumea's moons may also be leftover debris from the collision.

In Hawaiian mythology, Haumea is the goddess of fertility and childbirth. Her children include Hi'iaka and Namaka, as well as the Hawaiian volcano and fire goddess Pele.

There is some controversy concerning who should be credited with the discovery of Haumea. A group led by Mike Brown of the California Institute of Technology noticed Haumea in December 2004 on images taken in May 2004. Another group, led by Josť Luis Ortiz Moreno at the Sierra Nevada Observatory in Spain, filed a notification of the discovery of Haumea in July 2005. They had spotted the dwarf planet on images taken in March 2003. It isn't yet clear which group will eventually be given official recognition for the discovery.

Haumea was called 2003 EL61 before it received its official, permanent name. It was formerly nicknamed "Santa" by Brown's group due to its discovery near Christmas in 2004.

Last modified October 8, 2008 by Randy Russell.

Shop Windows to the Universe Science Store!

The Winter 2010 issue of The Earth Scientist, which includes articles on meteor cratering, classroom glaciers, podcasts in the classroom, and pyro-cumulonimbus clouds, is available in our online store.

Windows to the Universe Community



You might also be interested in:

Traveling Nitrogen Classroom Activity Kit

Check out our online store - minerals, fossils, books, activities, jewelry, and household items!...more

Dwarf Planets

In 2006 the International Astronomical Union (IAU) approved a new classification scheme for planets and smaller objects in our Solar System. Their scheme includes three classes of objects: "small solar...more


Pluto is a frigid ball of ice and rock that orbits far from the Sun on the frozen fringes of our Solar System. Considered a planet, though a rather odd one, from its discovery in 1930 until 2006, it was...more

Eris - a dwarf planet

Eris is a dwarf planet that was discovered in 2005. Eris is a trans-Neptunian object (TNO) that orbits the Sun on the frozen fringes of our Solar System beyond the Kuiper Belt. Eris takes 557 years to...more

Makemake: a Dwarf Planet

Makemake is a dwarf planet in our Solar System. Makemake was discovered on March 31, 2005 by a team of astronomers led by Mike Brown of the California Institute of Technology. The International Astronomical...more

Trans-Neptunian Objects (TNO)

There are many icy and rocky planetoids on the outer edge of our Solar System. As a group, all bodies that orbit, on average, further from the Sun than the 8th planet Neptune are called Trans-Neptunian...more

Elliptical Orbits

When one object is in orbit around another object, the orbit is usually an elliptical orbit. For example, all of the planets in our Solar System move around the Sun in elliptical orbits. An ellipse is...more

Density Definition Page

Density is a measure of how much mass is contained in a given unit volume (density = mass/volume). It is usually expressed in kg/m^3, so you would say that a cube 2 meters on each side with a mass of 16...more

Windows to the Universe, a project of the National Earth Science Teachers Association, is sponsored in part by the National Science Foundation and NASA, our Founding Partners (the American Geophysical Union and American Geosciences Institute) as well as through Institutional, Contributing, and Affiliate Partners, individual memberships and generous donors. Thank you for your support! NASA AGU AGI NSF