|
gptkbp:instanceOf
|
dwarf planet
|
|
gptkbp:associatedWith
|
gptkb:Pluto
|
|
gptkbp:atmosphere
|
nitrogen
0.96
|
|
gptkbp:classification
|
plutoid
|
|
gptkbp:countryOfOrigin
|
Greek_goddess_of_strife_and_discord
|
|
gptkbp:crew
|
25.9 hours
|
|
gptkbp:diameter
|
approximately 2,326 kilometers
|
|
gptkbp:established
|
gptkb:Mike_Brown
|
|
gptkbp:firstAppearance
|
2005
|
|
gptkbp:gameMechanics
|
0.8 m/s²
|
|
gptkbp:has
|
no
|
|
gptkbp:hasCategories
|
dwarf planets
|
|
gptkbp:hasCitations
|
very low
|
|
gptkbp:hasDeveloped
|
no
|
|
gptkbp:hasPersonalityTrait
|
no
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Eris
|
|
gptkbp:isAccessibleBy
|
no
|
|
gptkbp:isAssociatedWith
|
scientific interest
the_discovery_of_other_trans-Neptunian_objects
|
|
gptkbp:isATypeOf
|
gptkb:trans-Neptunian_object
|
|
gptkbp:isConsidered
|
a significant object in the solar system.
the largest known dwarf planet
|
|
gptkbp:isIntegratedWith
|
yes
|
|
gptkbp:isNamedAfter
|
Eris,_the_Greek_goddess
|
|
gptkbp:isNotableFor
|
its_large_size_and_distance_from_the_Sun
|
|
gptkbp:isPartOf
|
yes
dwarf planet characteristics
|
|
gptkbp:isSetIn
|
gptkb:Haumea
|
|
gptkbp:isStudiedIn
|
astronomers
|
|
gptkbp:isSuitableFor
|
Sedna
|
|
gptkbp:isVisitedBy
|
no
|
|
gptkbp:keyFunction
|
the debate over planet classification
|
|
gptkbp:location
|
Scattered disc
|
|
gptkbp:mission
|
Dysnomia
|
|
gptkbp:orbitalInclination
|
0.44
557.5 years
44.04°
|
|
gptkbp:releaseYear
|
January 5, 2005
Palomar Observatory
|
|
gptkbp:surface
|
ice and rock
-243 °C
|
|
gptkbp:symbol
|
Erisian symbol
|
|
gptkbp:type
|
neutral color spectrum
|
|
gptkbp:userInterface
|
craters and icy plains
|
|
gptkbp:wasEstablishedIn
|
no
|
|
gptkbp:weight
|
approximately 1.66×10^22 kg
|