Saturn's A ring

E829228

Saturn's A ring is the planet's outermost bright main ring, composed primarily of countless icy particles and separated from the B ring by the Cassini Division.

Try in SPARQL Jump to: Statements Referenced by

Statements (40)

Predicate Object
instanceOf planetary ring
albedo high
belongsTo outer main rings of Saturn
boundedBy Encke Gap NERFINISHED
Keeler Gap NERFINISHED
brightness high
composition icy particles
water ice
discoveredBy Giovanni Domenico Cassini NERFINISHED
discoveryMethod telescopic observation
dynamicsInfluencedBy Saturn's moons NERFINISHED
gravitational resonances
hasAzimuthalAsymmetries yes
hasGap Encke Gap NERFINISHED
Keeler Gap NERFINISHED
hasStructure bending waves
density waves
ringlets
spiral density waves
innerBoundary Cassini Division NERFINISHED
innerRadius approximately 122,000 kilometers from Saturn's center
isOuterMost bright main ring of Saturn
locationInSystem outside Saturn's B ring
meanRadius approximately 136,770 kilometers from Saturn's center
namedAfter letter A
nomenclatureSystem historical order of discovery of Saturn's rings
observedBy Cassini spacecraft NERFINISHED
Voyager 1 NERFINISHED
Voyager 2 NERFINISHED
opticalDepth moderate
orbits Saturn NERFINISHED
outerBoundary Roche Division NERFINISHED
outerRadius approximately 136,800 kilometers from Saturn's center
particleSizeRange dust to meter-sized bodies
partOf ring system of Saturn
separatedFrom Saturn's B ring NERFINISHED
separationRegion Cassini Division NERFINISHED
shepherdedBy Daphnis NERFINISHED
Pan NERFINISHED
width approximately 14,600 kilometers

Referenced by (1)

Full triples — surface form annotated when it differs from this entity's canonical label.

Keeler Gap isDivisionOf Saturn's A ring