|
gptkbp:instance_of
|
gptkb:star
|
|
gptkbp:age
|
estimated to be 100 million to 1 billion years
|
|
gptkbp:appearance
|
bright and reflective
|
|
gptkbp:average_temperature
|
very cold
|
|
gptkbp:color
|
varies from white to brown
|
|
gptkbp:color_variation
|
yes
|
|
gptkbp:composed_of
|
ice particles
rocky debris
|
|
gptkbp:contains
|
moonlets
|
|
gptkbp:diameter
|
up to 1 kilometer
|
|
gptkbp:discovered_by
|
gptkb:Christiaan_Huygens
|
|
gptkbp:emergency_services
|
yes
|
|
gptkbp:financial_stability
|
in the short term
|
|
gptkbp:gravity_effect
|
affects nearby moons
|
|
gptkbp:has_function
|
yes
|
|
gptkbp:has_gaps
|
yes
|
|
gptkbp:has_ice
|
yes
|
|
gptkbp:has_natural_feature
|
in the solar system
|
|
gptkbp:has_rock
|
yes
|
|
gptkbp:has_shepherd_moons
|
yes
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
rings of Saturn
|
|
gptkbp:influenced_by
|
gptkb:Saturn's_moons
|
|
gptkbp:influences
|
Saturn's atmosphere
|
|
gptkbp:is_observed_in
|
gptkb:Cassini_spacecraft
gptkb:Voyager_1
gptkb:Voyager_2
|
|
gptkbp:is_part_of
|
gptkb:Saturn_system
|
|
gptkbp:is_visible_from
|
with a telescope
during equinoxes
from space missions
|
|
gptkbp:largest_ring
|
A Ring
|
|
gptkbp:made_of
|
dust particles
|
|
gptkbp:orbit_type
|
gptkb:Saturn
|
|
gptkbp:orbital_inclination
|
about 27 degrees
|
|
gptkbp:origin
|
formed from asteroids
formed from comets
formed from debris of moons
|
|
gptkbp:population_density
|
varies across rings
|
|
gptkbp:research
|
ongoing research
|
|
gptkbp:research_importance
|
helps understand planetary formation
|
|
gptkbp:ring_name
|
gptkb:E_Ring
gptkb:F_Ring
gptkb:G_Ring
gptkb:H_Ring
yes
over 30 distinct rings
B Ring
C Ring
D Ring
|
|
gptkbp:rotation_period
|
depends on ring location
|
|
gptkbp:smallest_ring
|
gptkb:F_Ring
|
|
gptkbp:width
|
up to 282,000 kilometers
|
|
gptkbp:bfsParent
|
gptkb:Pioneer_11
gptkb:Galileo_Galilei
gptkb:The_Solar_System
|
|
gptkbp:bfsLayer
|
4
|