Eris

2,326 kmmean diameter

Updated

2,326km
Visual creditscaleofspace.org / CC BY-NC 4.0

Details

Eris is a distant dwarf planet in the scattered disk beyond Neptune. Its discovery helped trigger the 2006 planet-definition debate, and its tiny moon Dysnomia lets astronomers measure its mass.

Eris is close to Pluto in diameter but more massive, a comparison made possible by tracking its moon Dysnomia. Its 2005 announcement sharpened the question of whether similarly sized trans-Neptunian objects should all count as planets. The resulting 2006 IAU definition placed Eris, Pluto and Ceres in the dwarf-planet category.

Key facts

Category
Dwarf planets
Object class
Dwarf planet
Mass
~0.0028 Earth masses
Host
Sun
Scale fact
2,326 kmmean diameter
Estimated age
~4.5 billion years
Composition
Rock and ice
Embed

Size neighbors

Objects near Eris on the scale

On the logarithmic size axis, Eris falls between Haumea and Pluto. 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 Eris

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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