Statements (54)
Predicate | Object |
---|---|
gptkbp:instanceOf |
planetary ring system
|
gptkbp:age |
relatively young
|
gptkbp:associatedWith |
gptkb:Jupiter's_moons
Jupiter's_atmosphere Jupiter's_magnetosphere |
gptkbp:auxiliaryVessel |
gptkb:Gossamer_Rings
|
gptkbp:colors |
faint and translucent
mostly greyish |
gptkbp:composedOf |
dust particles
ice particles |
gptkbp:contains |
small moonlets
|
gptkbp:distribution |
very low density
|
gptkbp:established |
Voyager 1
|
gptkbp:explores |
gptkb:Galileo_spacecraft
|
gptkbp:firstPublished |
Pioneer 10
|
gptkbp:formed |
material from moons
|
gptkbp:historicalResearch |
ongoing studies
|
https://www.w3.org/2000/01/rdf-schema#label |
Jupiter's rings
|
gptkbp:influencedBy |
Jupiter's_gravity
|
gptkbp:interactsWith |
Jupiter's_magnetic_field
|
gptkbp:isTrainedIn |
gptkb:Halo_Ring
|
gptkbp:lighting |
very faint
|
gptkbp:locatedIn |
gptkb:Jupiter
|
gptkbp:material |
impacts on moons
|
gptkbp:numberOfStudents |
four
|
gptkbp:operationalRange |
constantly changing
|
gptkbp:orbitalInclination |
about 10 hours
|
gptkbp:peerage |
requires advanced telescopes
|
gptkbp:relatedTo |
gptkb:Saturn's_rings
|
gptkbp:releaseYear |
1979
|
gptkbp:researchInterest |
high due to unique characteristics
|
gptkbp:resolution |
about 30 kilometers
|
gptkbp:ringName |
complex and varied
varies significantly influenced by nearby moons still under investigation affected by solar radiation pressure best viewed during certain angles constantly replenished important for planetary science. includes micrometeoroid debris less than a million years not perfectly circular primarily water ice and silicate material less_prominent_than_Saturn's |
gptkbp:scientificName |
helps understand ring formation
|
gptkbp:sequel |
Main Ring
|
gptkbp:size |
varies from micrometers to centimeters
|
gptkbp:visibility |
difficult_to_see_from_Earth
|
gptkbp:visitedBy |
gptkb:New_Horizons_mission
gptkb:spacecraft gptkb:Hubble_Space_Telescope ultraviolet light |
gptkbp:width |
about 7,000 kilometers
|