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Small Solar System body

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Title: Small Solar System body  
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Subject: Solar System, Asteroid, IAU definition of planet, P/2010 A2, Hydrostatic equilibrium
Collection: Minor Planets
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Small Solar System body

951 Gaspra, 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. 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 may turn out to be dwarf planets.

Contents

  • Definition 1
  • See also 2
  • References 3
  • External links 4

Definition

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

References

  1. ^ RESOLUTION B5 - Definition of a Planet in the Solar System (IAU)

External links

  • Expected Science Return of Spatially-Extended In-Situ Exploration at Small Solar System Bodies
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