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gptkbp:instance_of
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gptkb:star
|
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gptkbp:associated_with
|
Uranus's moons
|
|
gptkbp:color
|
dark
|
|
gptkbp:composed_of
|
dust
rocky material
ice particles
|
|
gptkbp:diameter
|
up to 10 meters
|
|
gptkbp:discovered_by
|
gptkb:James_L._Elliot
|
|
gptkbp:discovery_year
|
gptkb:1977
|
|
gptkbp:gravity_effect
|
affects nearby moons
|
|
https://www.w3.org/2000/01/rdf-schema#label
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Uranus's rings
|
|
gptkbp:is_located_near
|
gptkb:Uranus
|
|
gptkbp:is_observed_in
|
gptkb:Voyager_2
|
|
gptkbp:is_visible_from
|
not easily visible from Earth
|
|
gptkbp:orbital_period
|
approximately 0.5 days
|
|
gptkbp:population_density
|
low density
|
|
gptkbp:research_importance
|
study of planetary formation
insight into moon formation
understanding of ring dynamics
|
|
gptkbp:ring_dynamics
|
complex interactions with moons
|
|
gptkbp:ring_formation_theories
|
collisional debris
remnants of moon formation
|
|
gptkbp:ring_name
|
gptkb:Lambda_ring
gptkb:13
Epsilon ring
Alpha ring
Beta ring
Delta ring
Eta ring
Gamma ring
Iota ring
Kappa ring
Mu ring
Zeta ring
Nu ring
|
|
gptkbp:ring_observation_challenges
|
distance from Earth
faintness of rings
light scattering effects
|
|
gptkbp:ring_particle_color
|
dark and reddish
|
|
gptkbp:ring_particle_composition
|
mostly water ice
|
|
gptkbp:ring_particle_size
|
varies from micrometers to meters
|
|
gptkbp:ring_structure
|
narrow and well-defined
|
|
gptkbp:ring_system_age
|
possibly young
|
|
gptkbp:ring_system_origin
|
gptkb:unknown
|
|
gptkbp:topics
|
gptkb:space_exploration
gptkb:astronomy
astrophysics
planetary science
|
|
gptkbp:width
|
up to 100 kilometers
|
|
gptkbp:bfsParent
|
gptkb:Voyager_ship
|
|
gptkbp:bfsLayer
|
6
|