SolarExplorer

Trans-Neptunian & Belt Realms

Dwarf Planets

Worlds large enough to be rounded by their own gravity, yet sharing their orbital neighborhood with other cosmic bodies. Step into the realm of Pluto, Ceres, Eris, Haumea, and Makemake.

Pluto

Kuiper Belt King

Reclassified as a dwarf planet in 2006, Pluto features nitrogen-ice glaciers, nitrogen atmosphere hazes, and a heart-shaped glacier named Sputnik Planitia. It shares a binary orbit with its giant moon Charon.

1,188 km
39.5 AU
248 Years
5 (Charon)

Ceres

Asteroid Belt Giant

The only dwarf planet inside the inner Solar System, Ceres accounts for a third of the main asteroid belt's total mass. NASA's Dawn mission discovered mysterious bright sodium carbonate spots in Occator crater.

473 km
2.77 AU
4.6 Years
0

Eris

Massive Remote World

Discovered in 2005, Eris is 27% more massive than Pluto. Its discovery sparked the official IAU definition of a planet. Eris has an extremely reflective surface covered in methane ice and is orbited by moon Dysnomia.

1,163 km
67.7 AU
558 Years
1 (Dysnomia)

Haumea

Spinning Ellipsoid

Haumea spins so rapidly (a day lasts under 4 hours) that centripetal force distorts it into an elongated triaxial ellipsoid. In 2017, astronomers discovered a ring system orbiting Haumea.

~816 km
43.1 AU
284 Years
2 (Hiʻiaka)

Makemake

Icy Easter World

Named after the Rapa Nui creator god, Makemake is the second brightest Kuiper Belt object after Pluto. It is covered in frozen methane and ethane snow and is orbited by a dark moon nicknamed MK2.

~715 km
45.8 AU
305 Years
1 (S/2015 1)