About Ceres
Ceres is the largest body in the asteroid belt, the only dwarf planet in the inner Solar System, and the first asteroid ever discovered — found by Giuseppe Piazzi on the first night of the 19th century, 1 January 1801. It was originally classified as a planet, then reclassified as an asteroid in the 1850s, and finally as a dwarf planet in 2006 alongside Pluto, Haumea, Makemake and Eris.
NASA’s Dawn spacecraft (2015-2018) orbited Ceres and revealed a remarkable world. Bright salt deposits — sodium carbonate and ammonium chloride — inside Occator Crater originate from cryovolcanic brine that reached the surface as recently as 2 million years ago. Gravity data indicate a 40 km thick upper crust, a muddy subsurface reservoir, and a still-extant deep brine layer between the rocky mantle and crust. Ceres is therefore both an asteroid and an ocean world.
Physical Properties
Orbit
Missions to Ceres
1 spacecraft tracked on Space Launch Live.
Gallery
Hand-picked mission imagery of Ceres sourced from NASA and partner archives. Click any photo for full resolution and source attribution.
Imagery on this page is provided by the original mission teams. Full attribution terms: Image Rights & Credits.
Sources & Further Reading
- NASA — official mission / factsheet page
- Wikipedia — extensive cross-referenced article
- NASA Dawn Mission
- NASA u2014 Ceres
- JPL Small-Body Database u2014 1 Ceres
Numerical values (radius, mass, orbital elements, temperatures) are drawn from NASA NSSDC Planetary Fact Sheets, JPL Horizons, and the JPL Small-Body Database. Last refreshed: 2026-06-08 01:37:02.