Dwarf planet
Ceres
The largest body in the asteroid belt and the only dwarf planet of the inner solar system — a wet, salty, partially differentiated world.

Vital statistics
01
Overview
Ceres is the largest body in the asteroid belt — and the only dwarf planet inside Neptune's orbit. Discovered by Giuseppe Piazzi on January 1, 1801, it was briefly considered the eighth planet before astronomers realised it shared its orbit with thousands of similar objects. NASA's Dawn mission settled into orbit around Ceres in March 2015, returning detailed maps and discovering bright salt deposits, possible cryovolcanic features, and evidence for a subsurface brine reservoir. Ceres holds roughly a quarter of the entire asteroid belt's mass.
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Composition
A rocky core wrapped in a thick mantle of water ice and hydrated minerals, possibly with a remaining liquid-brine layer just beneath the surface. About 25% of Ceres by mass is water — more fresh-water ice than all of Earth's. The crust is a complex mixture of clays, carbonates, and salts. Ceres is partially differentiated: dense rocky material settled toward the centre but not enough to form a metallic core like Earth's.
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Atmosphere
Ceres has an extremely tenuous water-vapour exosphere, detected by the Herschel Space Observatory in 2014. The vapour likely originates from sublimation of surface ice and possible cryovolcanic outgassing rather than a sustained atmosphere. ESA observed plumes coming from two specific surface points, supporting the idea that Ceres is geologically active even today.
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Surface
Ceres is heavily cratered but missing the giant impact basins seen on similar-sized icy moons — its weak surface relaxes over geological time. The Occator crater, 92 km wide, contains the most famous "bright spots": sodium-carbonate salt deposits left behind when subsurface brine reached the surface and the water sublimated away. The Ahuna Mons cryovolcano stands 4 km tall — the only confirmed cryovolcano in the asteroid belt. Surface temperatures range from -105 °C average to lows below -130 °C in permanently shadowed crater floors.
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Exploration
NASA's Dawn spacecraft, having already orbited the asteroid Vesta from 2011-2012, arrived at Ceres in March 2015 and remained until its hydrazine ran out in October 2018. Dawn used ion propulsion — the first spacecraft ever to orbit two distinct extra-terrestrial bodies. It mapped the entire surface at multiple altitudes (the lowest at just 35 km), characterised the bright spots and cryovolcanic features, and confirmed evidence for a subsurface brine layer. Dawn now sits in a stable orbit around Ceres as a derelict.
Did you know?
Ceres was originally classified as a planet for 50 years, then reclassified as an asteroid, then re-classified again as a dwarf planet in 2006.
Ceres contains more water — mostly as ice — than all of Earth's freshwater combined.
You could orbit Ceres at walking speed if you ran fast enough; escape velocity is just 510 m/s.
Occator crater's bright spots are sodium carbonate, the most reflective salts in the solar system.
Ahuna Mons is unique: a 4-km cryovolcano made of frozen water-ice "lava" instead of molten rock.
Some scientists argue Ceres meets the criteria to be considered a candidate for life — it has water, energy from radiogenic heating, and complex organic chemistry.
Dawn's ion engine used 1/10 the propellant of a chemical engine to complete the same mission.
Timeline
- 18011801
Giuseppe Piazzi discovers Ceres on January 1, briefly the "eighth planet".
- 1850s1850s
Discovery of more main-belt objects forces Ceres' reclassification as an asteroid.
- 20062006
IAU reclassifies Ceres again — this time as a dwarf planet.
- 20142014
Herschel detects water-vapour plumes outgassing from the surface.
- 20152015
NASA's Dawn enters orbit around Ceres on March 6 — first dwarf-planet orbiter.
- 20182018
Dawn mission ends after running out of hydrazine; remains in stable orbit.
- 20242024
Reanalysis of Dawn data confirms a global subsurface brine layer beneath Ceres' crust.