Statements (95)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Ring_of_Honor
gptkb:star |
| gptkbp:age |
young
|
| gptkbp:associated_with |
gptkb:Neptune's_moons
|
| gptkbp:characterized_by |
faintness
|
| gptkbp:color |
dark
|
| gptkbp:composed_of |
dust
dust particles rocky material ice particles |
| gptkbp:diameter |
10 meters
less than 10 meters |
| gptkbp:discovered_by |
gptkb:Voyager_2
|
| gptkbp:discovery_year |
gptkb:1989
|
| gptkbp:formed |
likely from moon collisions
|
| gptkbp:gravity_effect |
affects nearby moons
|
| gptkbp:has_function |
constantly changing
|
| https://www.w3.org/2000/01/rdf-schema#label |
Neptune's rings
|
| gptkbp:image |
gptkb:Voyager_2
|
| gptkbp:influenced_by |
Neptune's gravity
|
| gptkbp:inner_ring |
Galle ring
|
| gptkbp:interacts_with |
Neptune's magnetic field
|
| gptkbp:is_a_phenomenon_that |
shepherd moons
|
| gptkbp:is_located_near |
gptkb:Neptune
|
| gptkbp:is_observed_in |
gptkb:Hubble_Space_Telescope
|
| gptkbp:is_visible_from |
difficult to observe
|
| gptkbp:named_after |
gptkb:Neptune
|
| gptkbp:orbital_period |
approximately 16 hours
varies with distance from Neptune |
| gptkbp:outer_ring |
gptkb:Adams_ring
|
| gptkbp:population_density |
low
|
| gptkbp:research |
difficult to see
due to distance from Earth |
| gptkbp:research_importance |
study of planetary formation
helps understand planetary ring systems |
| gptkbp:research_interest |
due to unique characteristics
|
| gptkbp:ring_age |
young
less than a few hundred million years |
| gptkbp:ring_brightness |
faint
|
| gptkbp:ring_characteristics |
distinct from other planets
|
| gptkbp:ring_color_variations |
observed under different lighting conditions
|
| gptkbp:ring_composition |
not fully understood
varies with distance from planet |
| gptkbp:ring_density_variations |
not uniform throughout
|
| gptkbp:ring_dust |
contributes to ring structure
|
| gptkbp:ring_dynamics |
gptkb:complex
influenced by nearby moons |
| gptkbp:ring_dynamics_research |
provides insights into gravitational interactions
|
| gptkbp:ring_dynamics_study |
important for understanding planetary systems
important for planetary science |
| gptkbp:ring_erosion |
occurs over time
|
| gptkbp:ring_exploration |
part of planetary missions
|
| gptkbp:ring_formation |
possibly from moon collisions
|
| gptkbp:ring_formation_theories |
varied and debated
still under investigation |
| gptkbp:ring_future_research |
promises new discoveries.
|
| gptkbp:ring_gravity |
influences nearby objects
|
| gptkbp:ring_impact_on_moons |
affects their orbits
|
| gptkbp:ring_interaction |
with solar wind
|
| gptkbp:ring_material |
water ice
primarily water ice |
| gptkbp:ring_name |
gptkb:5
dark blue five Galle, Adams, Leverrier, Arago, and others dark and bluish |
| gptkbp:ring_observation |
requires advanced technology
|
| gptkbp:ring_observation_challenges |
due to distance from Earth
|
| gptkbp:ring_observation_history |
limited to recent decades
notable since Voyager 2 |
| gptkbp:ring_observation_techniques |
include radar and imaging
|
| gptkbp:ring_observation_tools |
include space telescopes
|
| gptkbp:ring_opacity |
low
varies with location |
| gptkbp:ring_origin |
gptkb:unknown
|
| gptkbp:ring_particle_size |
varies from micrometers to meters
|
| gptkbp:ring_particles |
reflect sunlight
|
| gptkbp:ring_research |
ongoing
|
| gptkbp:ring_research_goals |
understand formation and evolution
|
| gptkbp:ring_research_importance |
helps understand other ring systems
|
| gptkbp:ring_research_methods |
include computer simulations
|
| gptkbp:ring_shape |
irregular
|
| gptkbp:ring_size |
varies significantly
|
| gptkbp:ring_spectroscopy |
used to analyze composition
|
| gptkbp:ring_structure |
gptkb:complex
not uniform |
| gptkbp:ring_temperature |
cold
|
| gptkbp:ring_variability |
changes over time
|
| gptkbp:ring_visibility |
best during certain alignments
best during certain conditions |
| gptkbp:ring_width |
varies
varies significantly |
| gptkbp:size |
varies
|
| gptkbp:bfsParent |
gptkb:Voyager_2
|
| gptkbp:bfsLayer |
4
|