Ceres

940 kmmean diameter

Updated

940km
Visual creditDawn 2015 / NASA / JPL-Caltech / MPS / DLR / IDA / Daniel Macháček / Public domainSource: Wikimedia Commons

Details

Ceres is the largest object in the asteroid belt and the smallest recognized dwarf planet. NASA’s Dawn mission showed that its brightest spots are salt deposits left by briny water rising from below, showing that Ceres is a water-rich world with a geologically recent past.

Dawn found that Ceres has a differentiated interior and a water-rich crust containing ice, hydrated salts, rock and clathrates. In Occator crater, bright sodium-carbonate deposits record brines that reached the surface or shallow subsurface after the impact.

Some deposits and flow features are geologically recent, and Dawn data leave open the possibility of activity continuing below the surface. Any liquid today is probably limited to brine reservoirs deep below the surface.

Key facts

Category
Dwarf planets
Object class
Dwarf planet
Mass
~0.00016 Earth masses
Host
Sun
Scale fact
940 kmmean diameter
Estimated age
~4.56 billion years
Composition
Rock and water ice
Temperature
~167 K mean surface
Embed

Size neighbors

Objects near Ceres on the scale

On the logarithmic size axis, Ceres falls between 4 Vesta and Tethys. The band uses nearby Dwarf planet records.

Shared physical scale
1,820km
Ceres940 km
Makemake1,430 km
Haumea2,322 km
Eris2,326 km
Pluto2,380 km

Sources

References for Ceres

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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