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Eris

Artist's vision of Eris

Eris is a dwarf planet in the outer reaches of our Solar system.

It was first sighted in 2005 and is currently 97 astronomical units away, putting it at more than twice the distance of Pluto. Following its discovery there was debate amongst astronomers as to whether the new object would be a planet, but the discussion eventually led to Pluto being de-classified as a proper planet in 2006.

Although we cannot yet be sure, we think that Eris is an icy, rocky object that is about three-quarters the size of our Moon. Like other dwarf planets, Eris's orbit is tilted by 44° to the orbits of the main planets.

Having an inclined orbit suggests that it did not form in the same way as the planets, and is simply a large lump of rock that was somehow captured into its highly eccentric 557 year orbit around the Sun.

Eris has one known moon, called Dysnomia, which is around 150km across and orbits the dwarf planet every 15.8 days.

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