Ceres: The Smallest and Closest Dwarf Planet
The dwarf planet Ceres as seen by the Hubble Space Telescope.
Credit: NASA, ESA, J. Parker (Southwest Research Institute), P. Thomas (Cornell University), L. McFadden (University of Maryland, College Park), and M. Mutchler and Z. Levay (STScI)

Ceres is a dwarf planet, the only one located in the inner reaches of the solar system; the rest lie at the outer edges, in the Kuiper Belt. While it is the smallest of the known dwarf planets, it is the largest object in the asteroid belt.

Unlike other rocky bodies in the asteroid belt, Ceres is an oblate spheroid, rounded with a rotational bulge around its equator. Scientists think Ceres may have an ocean and possibly an atmosphere. The recent arrival of a probe has unlocked some of the dwarf planet's secrets, but others remain hidden. [See more photos of the dwarf planet Ceres]

On March 6, 2015, NASA's Dawn Spacecraft became the first probe to orbit two bodies in the solar system. After leaving the asteroid Vesta, Dawn traveled to Ceres, an icy world that has tantalized scientists for years. While most asteroids are made of rock, Ceres revealed hints that it could contain water on its surface since 1991, though those hints remained unconfirmed for more than 20 years.

As Dawn drew closer to the giant asteroid, a bright spot on its surface grew clearer. After observing Ceres, 130 similar spots of varying brightness were found on the planet. The surface of Ceres is generally as reflective as freshly poured asphalt, while the spots ranged from the dull sheen of concrete to the startling brightness of ice floating on Earth's oceans. The brightest region lies in the 56-mile-wide (90 kilometers) Occator Crater, which contains the most famous collections of shining spots on the surface of Ceres.

Early speculation regarding the spots included the possibility of ice volcanoes on the dwarf planet. However, only a single "lonely mountain" rises from the surface. The pyramid-shaped mountain rises to an altitude of 21,120 feet (6,437 meters). The 4-mile high mountain stands solitary, with no evidence of volcanic or other geologic activity to suggest its puzzling origin.

A recent study of the spots found that they are made up of hydrated magnesium sulfates, the same material that makes up Epsom salt back on Earth. Most of the bright regions are associated with craters, suggesting that their formation could be related to impacts. These findings tie into earlier understanding of the formation of the dwarf planet.

Ceres has a density of 2.09 grams per cubic centimeter, leading scientists to conclude approximately a quarter of its weight is water. This would give the dwarf planet more fresh water than Earth contains. By comparison, Earth has a density of 5.52 grams per cubic centimeter.

Scientists think that water-ice serves as the mantle of the dwarf planet. The thin, dusty crust is thought to be composed of rock, while a rocky inner core lies at the center. Spectral observations of Ceres from Earth reveal that the surface contains iron-rich clays. Signs of carbonates have similarly been found, making Ceres one of the only bodies in the solar system known to contain these minerals, the other two being Earth and Mars. Formed by a process that involves heat and water, carbonates are considered good potential indicators of habitability. [The Search for Life on Mars (A Photo Timeline)

When large bodies crash into Ceres, they may scoop out a region of the crust, cutting into the icy mantle beneath to leave the ice closer to surface. When sunlight heats the outer layer, the ice could go from solid to gas through a process known as sublimation.

In 2014, the European Space Agency's Herschel Space Observatory detected plumes of water vapor escaping from the dwarf planet at a rate of 13 lbs. (6 kilograms) per second.

"This is the first clear-cut detection of water on Ceres and in the asteroid belt in general," said Michael Küppers of the European Space Agency, Villanueva de la Cañada, Spain. Küppers led the study of the vapor that appeared in Nature.

Ceres is thought to contain a thin outer layer of dust and rock over an icy layer.
Ceres is thought to contain a thin outer layer of dust and rock over an icy layer.

Astronomers in the late 18th century mathematically predicted the presence of a planet between Mars and Jupiter, eagerly turning their telescopes to the region in search of the missing body. On Jan. 1, 1801, Sicilian astronomer Giuseppe Piazzi discovered what was then considered a planet, naming it Ceres for the Roman goddess of corn and harvests.

Within a decade, four new objects were discovered in the same region, all also considered planets. Nearly 50 years passed before more, smaller bodies were found scattered between Mars and Jupiter — the components of the asteroid belt — and Ceres was demoted to the status of an asteroid.

In 2006, Ceres was promoted to the status of a dwarf planet; it did not reach full planetary status because it failed to gravitationally clear its neighborhood of debris, though it often retains its classification as an asteroid, as well. [Infographic: Dwarf Planets in the Solar System]

The largest object in the asteroid belt, Ceres makes up nearly a third of its mass. Even so, it remains the smallest known dwarf planet, only 590 miles (950 km) across — roughly the size of Texas. A day on Ceres lasts a little over 9 Earth-hours, while it takes 4.6 Earth-years to travel around the sun.

The close proximity and low mass of Ceres have led some scientists to suggest that it could serve as a potential site for manned landings and a launching point for manned deep space missions.

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Unlike most of the asteroid belt, Ceres contains a significant amount of ice. This could mean similar worlds in the early solar system could have been responsible for bringing water to Earth.

Under current solar system models, Earth would have formed primarily rocky. Any water it held on its surface would have been vaporized when a large protoplanet collided with it to form the moon. For a long time, scientists thought that comets might have delivered water to the reformed Earth as they collided with its surface. However, comet-studying probes have shown that the icy rocks don't contain the right kind of water for their siblings to be responsible for those deliveries. New studies have turned to objects known as main belt asteroids, rock and icy neighbors of Ceres.

"One quarter of the mass of Ceres is water, and three quarters is rock," Dawn scientist Chris Russell told Space.com in 2015.

"If we had just a few Ceres-type bodies colliding with the Earth, we can explain where the water came from."

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