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Small Solar System body

object in the Solar System that is neither a planet, nor a dwarf planet, nor a satellite

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Record originEnglish Wikipedia
Text licenseCC BY-SA 4.0
Source revisionApr 20, 2026
Entity authorityQ193275
Source-derived summary

A small Solar System body (SSSB) is an object in the Solar System that is neither a planet, a dwarf planet, nor a natural satellite. The term was first defined in 2006 by the International Astronomical Union (IAU) as follows: "All other objects, except satellites, orbiting the Sun shall be referred to collectively as 'Small Solar System Bodies'".

This encompasses all comets and all minor planets other than those that are dwarf planets. Thus SSSBs are: the comets; the classical asteroids, with the exception of the dwarf planet Ceres; the trojans; and the centaurs and trans-Neptunian objects, with the exception of the dwarf planets Pluto, Haumea, Makemake, Quaoar, Orcus, Sedna, Gonggong and Eris and others that may turn out to be dwarf planets.

Definition

The current definition was included in the 2006 IAU resolution that defined the term planet, demoting the status of Pluto to that of dwarf planet. In the context, it should be interpreted as, "All objects other than planets and dwarf planets orbiting the Sun shall be referred to collectively as 'Small Solar System Bodies'. The definition excludes interstellar objects traveling through the Solar System, such as the interstellar interlopers 1I/ʻOumuamua, 2I/Borisov, and 3I/ATLAS.

It is not presently clear whether a lower size bound will be established as part of the definition of small Solar System bodies in the future, or if it will encompass all material down to the level of meteoroids, the smallest macroscopic bodies in orbit around the Sun. (On a microscopic level there are even smaller objects such as interplanetary dust, particles of solar wind and free particles of hydrogen.)

Except for the largest, which are in hydrostatic equilibrium, natural satellites (moons) differ from small Solar System bodies not in size, but in their orbits. The orbits of natural satellites are not centered on the Sun, but around other Solar System objects such as planets, dwarf planets, and small Solar System bodies.

Some of the larger small Solar System bodies may be reclassified in future as dwarf planets, pending further examination to determine whether or not they are in hydrostatic equilibrium.

Editorial summary

“Small Solar System body” enters the record as object in the Solar System that is neither a planet, nor a dwarf planet, nor a satellite. Crown Archives preserves that source wording while asking what Small, Solar and System can confirm, complicate or overturn.

Editorial reviewA concise reference frame for defining the subject, testing terminology and identifying the institution closest to the evidence. The current lead gives the account dated anchors—2006—that can be checked directly. The selected authority fields contribute no independent date. Its strongest next move is a source search built around Small, Solar and System.
Editorial analysis

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“Small Solar System body” is worth following because a concise public description often conceals a longer documentary argument. Here, Small, Solar and System provides the most credible route into that argument.

Evidence profile

Named sources, stable identifiers and responsible institutions provide the strongest route from overview to verifiable evidence. The source revision retrieved here is dated Apr 20, 2026. The linked authority identifier is Q193275. None of the 0 selected statements returned an explicit reference. The first chronological checks are 2006.

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Source & attribution

This entry incorporates text from Small Solar System body” on English Wikipedia. Contributors are listed in the page history. Text is available under the Creative Commons Attribution-ShareAlike 4.0 License. Selected authority identifiers and statements are retrieved from Wikidata under CC0; their references and qualifiers remain part of the verification path.