|
gptkbp:instanceOf
|
gptkb:bar
|
|
gptkbp:altitudeOfHazeLayer
|
up to 500 km
|
|
gptkbp:block
|
visible light
|
|
gptkbp:cause
|
seasonal weather patterns
polar vortex
dune formation
methane storms
superrotation
surface erosion
|
|
gptkbp:clouds
|
methane clouds
|
|
gptkbp:component
|
nitrogen
methane
|
|
gptkbp:contains
|
gptkb:argon
gptkb:helium
gptkb:hydrogen_cyanide
hydrogen
carbon dioxide
water vapor
ammonia
carbon monoxide
acetylene
benzene
ethane
propane
complex organic molecules
nitriles
cyanoacetylene
carbonyl sulfide
cyanide compounds
diacetylene
ethene
hydrocarbon smog
methylacetylene
organic aerosols
tholin particles
trace hydrocarbons
|
|
gptkbp:discoveredBy
|
gptkb:Gerard_P._Kuiper
|
|
gptkbp:discoveredIn
|
1944
|
|
gptkbp:enables
|
hydrocarbon lakes
methane rain
|
|
gptkbp:haze
|
orange photochemical haze
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Titan's atmosphere
|
|
gptkbp:locatedOn
|
gptkb:Titan
|
|
gptkbp:minimumPressure
|
about 1.5 bar
|
|
gptkbp:pressureAtSurface
|
higher than Earth's
|
|
gptkbp:studiedBy
|
gptkb:Cassini-Huygens_mission
|
|
gptkbp:supports
|
methane cycle
|
|
gptkbp:temperature
|
about 94 K
|
|
gptkbp:thickerThan
|
gptkb:Earth's_atmosphere
|
|
gptkbp:bfsParent
|
gptkb:Ultraviolet_Imaging_Spectrograph
gptkb:Huygens_Aerosol_Collector_and_Pyrolyser
gptkb:Huygens_Descent_Imager/Spectral_Radiometer
gptkb:Huygens_aerosol_collector_and_pyrolyzer
gptkb:Titan_Wind_Tunnel
|
|
gptkbp:bfsLayer
|
7
|