Statements (48)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
planetary ring system
|
| gptkbp:associated_with |
gptkb:Oberon
gptkb:Titania gptkb:Ariel Miranda Umbriel |
| gptkbp:colors |
dark and faint
|
| gptkbp:composedOf |
ice and rock particles
|
| gptkbp:culturalHeritage |
featured in science fiction
|
| gptkbp:distribution |
varies throughout the rings
|
| gptkbp:education |
used in astronomy education
|
| gptkbp:established |
gptkb:James_L._Elliot
|
| gptkbp:explores |
Voyager 2
|
| gptkbp:futurePlans |
potential for future missions
|
| https://www.w3.org/2000/01/rdf-schema#label |
the rings of Uranus
|
| gptkbp:impact |
affects the orbits of nearby moons
|
| gptkbp:location |
around_Uranus
|
| gptkbp:maxRange |
Epsilon ring
|
| gptkbp:mission |
gptkb:Uranus
|
| gptkbp:namedAfter |
gptkb:Uranus
|
| gptkbp:numberOfStudents |
13
|
| gptkbp:officialResidence |
faintness_and_distance_from_Earth
|
| gptkbp:publicAccess |
sparks curiosity about outer planets
|
| gptkbp:relatedTo |
gptkb:the_rings_of_Saturn
|
| gptkbp:releaseYear |
1977
|
| gptkbp:researchInterest |
various theories about formation
|
| gptkbp:resolution |
less than 1 kilometer
|
| gptkbp:ringName |
unknown
ongoing studies complex and variable requires advanced telescopes influenced by gravitational interactions compared to other planetary rings composed of narrow and broad rings due to composition and size focus on composition and dynamics important for understanding ring mechanics likely from moons or comets micrometers to meters possibly young present in the ring system theories include collision and debris capture unique among the solar system's rings |
| gptkbp:scientificName |
imaging systems
provides insight into planetary formation |
| gptkbp:visibility |
difficult_to_observe_from_Earth
|
| gptkbp:visitedBy |
Voyager 2
|
| gptkbp:width |
up to 100 kilometers
|