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- Scattered_disc abstract "The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets, a subset of the broader family of trans-Neptunian objects. The scattered-disc objects (SDOs) have orbital eccentricities ranging as high as 0.8, inclinations as high as 40°, and perihelia greater than 30 astronomical units (4.5×109 km; 2.8×109 mi). 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.Although the closest scattered-disc objects approach the Sun at about 30–35 AU, their orbits can extend well beyond 100 AU. This makes scattered objects among the most distant and coldest objects in the Solar System. The innermost portion of the scattered disc overlaps with a torus-shaped region of orbiting objects traditionally called the Kuiper belt, but its outer limits reach much farther away from the Sun and farther above and below the ecliptic than the Kuiper belt proper.Because of its unstable nature, astronomers now consider the scattered disc to be the place of origin for most periodic comets 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.".
- Scattered_disc thumbnail Eris_and_dysnomia2.jpg?width=300.
- Scattered_disc wikiPageID "2719753".
- Scattered_disc wikiPageRevisionID "602291435".
- Scattered_disc hasPhotoCollection Scattered_disc.
- Scattered_disc subject Category:Scattered_disc_and_detached_objects.
- Scattered_disc subject Category:Trans-Neptunian_region.
- Scattered_disc comment "The scattered disc (or scattered disk) is a distant region of the Solar System that is sparsely populated by icy minor planets, a subset of the broader family of trans-Neptunian objects. The scattered-disc objects (SDOs) have orbital eccentricities ranging as high as 0.8, inclinations as high as 40°, and perihelia greater than 30 astronomical units (4.5×109 km; 2.8×109 mi).".
- Scattered_disc label "Disco diffuso".
- Scattered_disc label "Disco disperso".
- Scattered_disc label "Disco disperso".
- Scattered_disc label "Disque des objets épars".
- Scattered_disc label "Dysk rozproszony".
- Scattered_disc label "Scattered disc".
- Scattered_disc label "Scattered disk object".
- Scattered_disc label "Scattered disk".
- Scattered_disc label "Рассеянный диск".
- Scattered_disc label "قرص متفرق".
- Scattered_disc label "散乱円盤天体".
- Scattered_disc label "離散盤".
- Scattered_disc sameAs Rozptýlený_disk.
- Scattered_disc sameAs Scattered_disk.
- Scattered_disc sameAs Αντικείμενο_διεσκορπισμένου_δίσκου.
- Scattered_disc sameAs Disco_disperso.
- Scattered_disc sameAs Disque_des_objets_épars.
- Scattered_disc sameAs Piringan_tersebar.
- Scattered_disc sameAs Disco_diffuso.
- Scattered_disc sameAs 散乱円盤天体.
- Scattered_disc sameAs 산란_분포대.
- Scattered_disc sameAs Scattered_disk_object.
- Scattered_disc sameAs Dysk_rozproszony.
- Scattered_disc sameAs Disco_disperso.
- Scattered_disc sameAs m.07zwmq.
- Scattered_disc sameAs Q180380.
- Scattered_disc sameAs Q180380.
- Scattered_disc wasDerivedFrom Scattered_disc?oldid=602291435.
- Scattered_disc depiction Eris_and_dysnomia2.jpg.
- Scattered_disc isPrimaryTopicOf Scattered_disc.