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・ Ring Rock
・ Ring Round the Moon
・ Ring Route
・ Ring Route (Nagoya Expressway)
・ Ring saw
・ Ring Settlements
・ Ring shout
・ Ring signature
・ Ring singularity
・ Ring size
・ Ring species
・ Ring spectrum
・ Ring spinning
・ Ring strain
・ Ring structure
Ring system (astronomy)
・ Ring the Alarm
・ Ring the Alarm (album)
・ Ring the Alarm (disambiguation)
・ Ring the Alarm (Fu-Schnickens song)
・ Ring the Bell (horse)
・ Ring Them Bells
・ Ring theory
・ Ring Tone Transfer Language
・ Ring toss
・ Ring Tour 2009
・ Ring traveller
・ Ring Trilogy
・ Ring True Foundation
・ Ring Up the Curtain


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Ring system (astronomy) : ウィキペディア英語版
Ring system (astronomy)

A ring system is a disc or ring orbiting an astronomical object that is composed of solid material such as dust and moonlets, and is a common component of satellite systems around giant planets. A ring system around a planet is also known as a planetary ring system.
The most prominent planetary rings in the Solar System are those around Saturn, but the other three giant planets (Jupiter, Uranus and Neptune) also have ring systems. Recent evidence suggests that ring systems may be found around other types of astronomical objects, including minor planets, moons, and brown dwarfs.
== Ring systems of planets ==

There are three ways that thicker planetary rings (the rings around planets) have been proposed to have formed: from material of the protoplanetary disk that was within the Roche limit of the planet and thus could not coalesce to form moons; from the debris of a moon that was disrupted by a large impact; or from the debris of a moon that was disrupted by tidal stresses when it passed within the planet's Roche limit. Most rings were thought to be unstable and to dissipate over the course of tens or hundreds of millions of years, but it now appears that Saturn's rings might be quite old, dating to the early days of the Solar System.
Fainter planetary rings can form as a result of meteoroid impacts with moons orbiting around the planet or, in case of Saturn's E-ring, the ejecta of cryovolcanic material.
The composition of ring particles varies; they may be silicate or icy dust. Larger rocks and boulders may also be present, and in 2007 tidal effects from eight 'moonlets' only a few hundred meters across were detected within Saturn's rings.
Sometimes rings will have "shepherd" moons, small moons that orbit near the inner or outer edges of rings or within gaps in the rings. The gravity of shepherd moons serves to maintain a sharply defined edge to the ring; material that drifts closer to the shepherd moon's orbit is either deflected back into the body of the ring, ejected from the system, or accreted onto the moon itself.

抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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