Open Access Articles- Top Results for Small Solar System body

Small Solar System body

File:951 Gaspra.jpg
951 Gaspra, here photographed by the Galileo probe, is a small Solar System body in the asteroid belt whose length is about 18 km.

A small Solar System body (SSSB) is an object in the Solar System that is neither a planet, nor a dwarf planet, nor a satellite.[note 1] The term was first defined in 2006 by the International Astronomical Union.

All other objects, except satellites, orbiting the Sun shall be referred to collectively as "Small Solar System Bodies" ... These currently include most of the Solar System asteroids, most Trans-Neptunian Objects (TNOs), comets, and other small bodies.[1]

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


File:TheTransneptunians 73AU.svg
Distribution of centaurs and trans-Neptunian objects.

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.

The orbits of the vast majority of small Solar System bodies are located in two distinct areas, namely the asteroid belt and the Kuiper belt. These two belts possess some internal structure related to perturbations by the major planets (particularly Jupiter and Neptune, respectively), and have fairly loosely defined boundaries. Other areas of the Solar System also encompass small bodies in smaller concentrations. These include the near-Earth asteroids, centaurs, comets, and scattered disc objects.

See also


  1. ^ The formally correct typography for common nouns such as "small Solar System bodies" and "trans-Neptunian objects" is sentence case,[citation needed] rather than title case as used by the IAU in this instance.


External links