|
gptkbp:instanceOf
|
planetary ring system
|
|
gptkbp:age
|
100 million to 4.5 billion years
|
|
gptkbp:albedo
|
0.6
|
|
gptkbp:component
|
water ice
rocky debris
|
|
gptkbp:consistsOf
|
gptkb:B_ring
gptkb:C_ring
gptkb:D_ring
gptkb:E_ring
gptkb:F_ring
gptkb:G_ring
A ring
|
|
gptkbp:contains
|
dust
shepherd moons
rock fragments
ice chunks
micrometer to meter-sized particles
|
|
gptkbp:diameter
|
273,600 km
|
|
gptkbp:discoveredBy
|
gptkb:Galileo_Galilei
|
|
gptkbp:discoveredIn
|
1610
|
|
gptkbp:distanceFromEarth
|
7,000 km to 80,000 km from Saturn's center
|
|
gptkbp:features
|
most extensive ring system in Solar System
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Saturnian ring system
|
|
gptkbp:inclination
|
1.0° to Saturn's equator
|
|
gptkbp:influencedBy
|
Saturn's moons
Saturn's gravity
|
|
gptkbp:innermostRing
|
gptkb:D_ring
|
|
gptkbp:location
|
gptkb:Saturnian_system
|
|
gptkbp:mass
|
~3 × 10^19 kg
|
|
gptkbp:namedAfter
|
gptkb:Saturn
|
|
gptkbp:notableFeature
|
gptkb:Cassini_Division
gptkb:Encke_Gap
gptkb:Keeler_Gap
|
|
gptkbp:observedBy
|
gptkb:Hubble_Space_Telescope
ground-based telescopes
|
|
gptkbp:orbitType
|
gptkb:Saturn
|
|
gptkbp:origin
|
material from Saturn's formation
remnants of a destroyed moon
|
|
gptkbp:outermostRing
|
gptkb:E_ring
|
|
gptkbp:shepherdMoons
|
gptkb:Titan
gptkb:Prometheus
gptkb:Pandora
gptkb:Pan
gptkb:Daphnis
|
|
gptkbp:studiedBy
|
gptkb:Voyager_1
gptkb:Voyager_2
gptkb:Cassini_spacecraft
|
|
gptkbp:thickness
|
about 10 meters
|
|
gptkbp:visibleToNakedEye
|
yes
|
|
gptkbp:bfsParent
|
gptkb:Huygens_Gap
|
|
gptkbp:bfsLayer
|
7
|