MODULE:KNOWLEDGE-BASE
SIMULATION: ACTIVE
RETURN::Planetary Science

Rings & Moons

Ring Structure, Shepherds & Moon Systems

Saturn-Like Ring System

A, B, and C rings separated by the Cassini Division. Inner ring particles orbit faster than outer ones (Kepler's 3rd law). Shepherd moons sit at gap edges. Three named outer moons (Mimas, Tethys, Titan) orbit on dashed paths.

Why Rings Form

Rings form inside the Roche limit — the distance below which tidal forces overcome a body's self-gravity. Material there cannot coalesce into a moon, so it spreads into a flat orbiting sheet.

Possible origins: a moon torn apart on a decaying orbit, a comet captured and shredded, leftover material from formation, or impact debris from larger moons.

Despite their breadth (Saturn's rings span 280,000 km end-to-end), main rings are vertically thin — about 10 m. They are proportionally thinner than a sheet of paper at the scale of a football field.

Shepherd Moons & Gaps
Encke GapCleared and shepherded by Pan (~30 km moonlet)
Keeler GapCleared by Daphnis — visible 'wakes' on either edge
Cassini DivisionResonant gap from 2:1 orbital lock with Mimas
Resonant edgesOuter A ring edge held by 7:6 with Janus & Epimetheus
SpokesCharged dust grains lifted electrostatically — transient
ED: Ring Mining

Rings in Elite Dangerous come in four compositions: rocky, icy, metallic, and metal-rich. Composition determines what minerals you can extract.

Pristine reserves in metallic rings yield the rarest minerals. Hotspot scanning inside the ring reveals concentrated ore deposits.

The visual ring structure in ED is simplified — real planetary rings have complex banding, gaps, and spokes that change on timescales of hours to years.

Ring & Moon Reference
FeatureCompositionScaleNote
Saturn's A ringWater ice (98%) + traces~10 mOutermost main ring — bordered by Encke and Keeler gaps
Cassini DivisionMostly empty~4,800 kmCleared by 2:1 resonance with Mimas
Saturn's B ringWater ice — dense~10 mBrightest, densest main ring
Saturn's C ringWater ice — sparse~5 mThinner, more transparent inner ring
Pan & DaphnisRock + ice~30 km bodiesShepherd moons that maintain Encke and Keeler gaps
Jupiter's ringDust from impacts~30 kmTenuous, replenished by impacts on small inner moons
Uranus' ring systemDark carbonaceous13 narrow rings, kept thin by shepherd moons
Galilean moonsMixed rock/iceIo, Europa, Ganymede, Callisto in a 4:2:1 resonance chain