The scattered disc is a disc of distant objects in the outer Solar System. It includes some icy minor planets, ranging from about 30 AU from the sun. Scattered disc objects are known as SDOs.
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| - The scattered disc is a disc of distant objects in the outer Solar System. It includes some icy minor planets, ranging from about 30 AU from the sun. Scattered disc objects are known as SDOs.
- The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets known as scattered disc objects (SDOs), a subset of the broader family of trans-Neptunian objects (TNOs). The scattered disc objects have orbital eccentricities ranging as high as 0.8, inclinations as high as 40° and perihelia greater than 30 astronomical units (AU). These extreme orbits are believed to be the result of gravitational "scattering" by the gas giants, and the objects continue to be subject to perturbation by the planet Neptune.
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| abstract
| - The scattered disc is a disc of distant objects in the outer Solar System. It includes some icy minor planets, ranging from about 30 AU from the sun. Scattered disc objects are known as SDOs.
- The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets known as scattered disc objects (SDOs), a subset of the broader family of trans-Neptunian objects (TNOs). The scattered disc objects have orbital eccentricities ranging as high as 0.8, inclinations as high as 40° and perihelia greater than 30 astronomical units (AU). These extreme orbits are believed to be the result of gravitational "scattering" by the gas giants, and the objects continue to be subject to perturbation by the planet Neptune. While the nearest distance to the Sun approached by scattered objects is about 30–35 AU, their orbits can extend well beyond 100 AU. This makes scattered objects "among the most distant and cold objects in the Solar System". The innermost portion of the scattered disc overlaps with a torus-shaped region of orbiting objects known as the Kuiper belt, but its outer limits reach much farther away from the Sun and farther above and below the ecliptic than the belt proper. Due to its unstable nature, astronomers now consider the scattered disc to be the place of origin for most periodic comets observed in the Solar System, with the centaurs, a population of icy bodies between Jupiter and Neptune, being the intermediate stage in an object's migration from the disc to the inner Solar System. Eventually, perturbations from the giant planets send such objects towards the Sun, transforming them into periodic comets. Many Oort cloud objects are also believed to have originated in the scattered disc.
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![[RDF Data]](/fct/images/sw-rdf-blue.png)