A planetary ring is a ring of dust and other small particles orbiting around a planet in a flat disc-shaped region. The most spectacular and famous planetary rings are those around Saturn, but the other three gas giants of the solar system (Jupiter, Uranus, Neptune) possess ring systems of their own.
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Overview
There are three ways that planetary rings have been proposed to have formed: from material of the proto-planetary disc 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 are thought to be unstable and to dissipate over the course of tens or hundreds of millions of years, but it appears that Saturn's rings might be quite old, dating to the early days of the Solar system.[1] The composition of ring particles varies; they may be silicate or icy dust. Larger rocks and boulders are 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 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. Several of Jupiter's small innermost moons, namely Metis and Adrastea, are within Jupiter's ring system and are also within Jupiter's Roche limit. It is possible that these rings are composed of material that is being pulled off of these two bodies by Jupiter's tidal forces, possibly facilitated by impacts of ring material on their surfaces. A moon inside the Roche limit is held together only by its mechanical strength rather than by its gravity, and so loose material on its surface would simply "fall off" to join the rings. Neptune's rings are very unusual in that they first appeared to be composed of incomplete arcs in Earth-based observations, but Voyager 2's images showed them to be complete rings with bright clumps. It is thought that the gravitational influence of the shepherd moon Galatea and possibly other as-yet undiscovered shepherd moons are responsible for this clumpiness. Pluto is not known to have any ring systems. However, some astronomers think that the New Horizons probe might find a ring system when it visits in 2015.[2] It is also predicted that Phobos, a moon of Mars, will break up and form into a planetary ring in about 50 million years due to its low orbit.[3][4] After the impact of Theia and before the coalescence of the Moon, it is generally assumed that the Earth had a ring system.
See also
External links
Notes
- ^ Saturn's Rings May Be Old Timers. NASA (News Release 2007-149) (December 12, 2007). Retrieved on 2007-12-13.
- ^ Steffl, Andrew J.; S. Alan Stern. "First Constraints on Rings in the Pluto System". astro-ph/0608036.
- ^ Holsapple, K. A. (12 2001). "Equilibrium Configurations of Solid Cohesionless Bodies". Icarus 154 (2): 432-448. doi:10.1006/icar.2001.6683. Retrieved on 2007-12-13.
- ^ Gürtler, J. & Dorschner, J: "Das Sonnensystem", Barth (1993), ISBN 3-335-00281-4
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| Rings of Jupiter • Rings of Saturn • Rings of Uranus • Rings of Neptune |
| See also: gas torus |
| The Solar System |
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| <imagemap>
Image:Solar System XXVII.png
circle 0 0 90 35 The Sun
circle 112 18 6 Mercury
circle 153 18 8 Venus
circle 203 8 4 The Moon circle 194 18 8 Earth
circle 239 13 3 Phobos and Deimos circle 233 18 8 Mars
circle 271 18 8 Ceres rect 256 0 288 35 The asteroid belt
circle 316 18 15 Jupiter circle 329 5 6 Moons of Jupiter
circle 372 18 10 Saturn circle 381 7 6 Moons of Saturn
circle 418 18 9 Uranus circle 427 10 6 Moons of Uranus
circle 471 10 3 Moons of Neptune circle 462 18 12 Neptune
circle 508 13 3 Moons of Pluto circle 504 18 8 Pluto rect 492 0 527 35 The Kuiper Belt
circle 544 14 3 Dysnomia circle 540 18 8 Eris rect 528 0 567 35 The Scattered Disc rect 568 0 597 35 The Oort Cloud desc none
</imagemap> |
| The Sun · Mercury · Venus · Earth · Mars · Ceres · Jupiter · Saturn · Uranus · Neptune · Pluto · Eris |
| Planets · Dwarf planets · Moons: Terrestrial · Martian · Jovian · Saturnian · Uranian · Neptunian · Plutonian · Eridian |
| Small bodies: Meteoroids · Asteroids/Asteroid moons (Asteroid belt) · Centaurs · TNOs (Kuiper belt/Scattered disc) · Comets (Oort cloud) |
| See also astronomical objects, the solar system's list of objects, sorted by radius or mass, and the Solar System Portal |
