Linked from

The 15 pages that link to Planetary rings, each with the reason it gives.

• Roche limitRelated: Ring particles inside a planet's Roche limit may fail to accrete into a moon.

• SaturnNarrower topic: Saturn’s bright rings are the best-known example of this planetary structure.

• OccultationRelated: Changes in starlight during occultations can map rings too faint to image directly.

• Voyager programNarrower topic: Voyager observations revealed ring structures at Jupiter, Saturn, Uranus, and Neptune.

• Hill sphereRelated: A planet's Hill sphere helps delimit the region where ring material can remain associated with it.

• Tidal disruptionNarrower topic: A ring can persist where tides inhibit particles from assembling into a larger satellite.

• Rings of SaturnNarrower topic: Saturn’s system is the brightest and most extensive example of planetary rings.

• Poynting–Robertson effectRelated: Radiation drag can influence fine ring grains, alongside plasma and gravitational forces.

• Stellar occultationRelated: Brief dips in starlight can reveal narrow rings and constrain their optical depth.

• Trojan asteroidCompared with: Rings orbit a planet directly, whereas Trojan asteroids orbit the Sun alongside a planet.

• ExomoonCompared with: Rings can produce transit features that may be confused with signals attributed to moons.

• Irregular satelliteRelated: Collisions and material shed by small satellites can contribute dust to planetary rings.

• Rings of NeptuneNarrower topic: Neptune’s rings are a faint, dusty example of this broader structure.

• Geometric albedoBroader topic: Ring particles show phase-dependent brightness that informs reflectance and scattering models.

• Extraterrestrial vortexCompared with: A ring may look like a rotating structure but consists of orbiting particles, not a fluid vortex.