Statements (45)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
ring system
|
| gptkbp:age |
a few million years old
|
| gptkbp:associated_with |
Jupiter's_magnetic_field
|
| gptkbp:composedOf |
dust particles
four main rings |
| gptkbp:contains |
micrometers to centimeters
|
| gptkbp:depth |
gptkb:Saturn's_ring_system
|
| gptkbp:diameter |
approximately 7,000 kilometers
|
| gptkbp:established |
Voyager 1
|
| gptkbp:features |
the evolution of planetary systems
Jupiter's_atmosphere |
| gptkbp:first_appearance |
1979
|
| gptkbp:formed |
material ejected from moons
|
| gptkbp:has_a |
gaps and clumps
|
| gptkbp:has_a_focus_on |
planetary scientists
|
| https://www.w3.org/2000/01/rdf-schema#label |
Jupiter's ring system
|
| gptkbp:impact |
Jupiter's_intense_radiation_environment
|
| gptkbp:includes |
the Main ring
the Amalthea gossamer ring the_Halo_ring the_Thebe_gossamer_ring |
| gptkbp:influenced |
Jupiter's_gravity
|
| gptkbp:is_a_dish_that |
1 kilometer thick
|
| gptkbp:is_a_subject_of |
space exploration
planetary geology astrobiology |
| gptkbp:is_characterized_by |
its faintness and complexity
the complexity of planetary systems. |
| gptkbp:is_essential_for |
planetary formation processes
|
| gptkbp:is_integrated_with |
changing structures
|
| gptkbp:is_located_in |
gptkb:Jupiter
|
| gptkbp:is_part_of |
celestial mechanics
the solar system's ring systems Jupiter's_complex_system_of_moons_and_rings |
| gptkbp:is_studied_in |
gptkb:the_rings_of_Saturn
planetary atmospheres spacecraft missions extraterrestrial materials |
| gptkbp:is_used_in |
gptkb:the_rings_of_Uranus
|
| gptkbp:isRecognizedFor |
dust from its moons
|
| gptkbp:maintainedBy |
collisions with small meteoroids
|
| gptkbp:prominence |
gptkb:the_rings_of_Saturn
|
| gptkbp:visibility |
powerful telescopes
|
| gptkbp:visitedBy |
gptkb:Hubble_Space_Telescope
|
| gptkbp:was_a_result_of |
collisions between moons and meteoroids
|