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Ceres

HST image of Ceres

Ceres is a dwarf planet that orbits within the asteroid belt.

It is made of the same rocky minerals as asteroids, but is much larger and rounder.

Ceres was discovered way back in 1801 by the Italian astronomer Giuseppe Piazzi, although the image here was taken by the Hubble Space Telescope (HST).

Ceres orbits the Sun every 4.6 years and is about 930 kilometres (580 miles) across. This is about half the size of our own Moon. It seems to have a cratered surface made up of water-bearing minerals, and there are some indications of a very thin atmosphere.

Dwarf Planet Data Sheet show »« hide
Facts and FiguresCeresPlutoHaumeaMakemakeEris
Orbital distance (AU)12.7739.543.145.867.7
Orbital Inclination10.6°17.1°28.2°29°44°
Radius (KM)4871,1371,4367501,300
Mass (Earth Masses)20.000160.002130.00070.00070.003
Year Length (Earth Years)4.6248.5283.3309.9557
Day Length (Earth Days)0.386.390.16UnknownUnknown
Surface Gravity (g)30.0030.040.0440.050.08
Surface Temperatureabout -105°Cabout -230°Cabout -240°Cabout -243°Cabout -240°C
Number of moons03201
Notes: 1 1 AU (or Astronomical Unit) = 149,600,000 KM and is the mean distance from the Earth to the Sun
2 1 Earth Mass = 5,980,000,000,000,000,000,000,000 KG : 3 1 g = 9.8 m/s2