Dwarf planet 2026-11-05
A dwarf planet, in the International Astronomical Union's 2006 Solar-system definition, is a body that orbits the Sun, has enough self-gravity to assume a nearly round hydrostatic equilibrium shape, has not cleared its orbital neighborhood, and is not a natural satellite. The classification combines a body's physical shape with its dynamical environment; it is not defined by size alone.[ref]
Definition of a Planet in the Solar System by the International Astronomical Union. Adopted planet-definition resolution, category 2 and its four criteria
Pluto illustrates why both aspects matter: it is rounded but belongs to the trans-Neptunian population rather than being dynamically dominant in its orbital region. Ceres provides another example, in the asteroid belt. A rounded Moon does not become a dwarf planet, because the satellite exclusion is explicit. Under this terminology, planet and dwarf planet are distinct categories.[ref]
Definition of a Planet in the Solar System by the International Astronomical Union. Adopted categories and accompanying classification of Pluto and Ceres
Clearing does not mean that literally no other object shares the region. It concerns orbital dominance over the surrounding population. Nor does the rounding requirement supply one universal diameter threshold: resistance to deformation depends on composition, internal structure and rotation. Observations of shape and mass therefore address one part of the definition, while orbital-population information addresses another. The cited resolution is explicitly about the Solar system; applying the same wording to an exoplanet population requires an additional convention.
Small Solar System body 2026-11-05
A Small Solar System body is an object orbiting the Sun that is neither a planet nor a dwarf planet nor a natural satellite, in the classification adopted by the International Astronomical Union in 2006. The category includes most asteroids, most trans-Neptunian objects and comets. The definition is tied to the Solar system; it is not a general classification of every small astronomical object.[ref]
The categories encode physical distinctions. A dwarf planet has enough self-gravity to assume a nearly round equilibrium figure but has not cleared its orbital neighborhood. A Small Solar System body does not satisfy both planetary shape and orbital-clearing conditions. A natural satellite is classified separately even if it is small and irregular.
For example, Ceres lies in the asteroid belt but is a dwarf planet, whereas Vesta is classified as an asteroid. Merely being in the asteroid belt therefore does not determine which formal category an object occupies.[ref]
Ceres: Facts by NASA. Dwarf-planet classification
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