Shangri-La dune fields on Titan
E198121
The Shangri-La dune fields on Titan are vast equatorial expanses of dark, organic-rich sand dunes on Saturn’s largest moon, considered a prime site for studying prebiotic chemistry and targeted for exploration by NASA’s Dragonfly mission.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Shangri-La dune fields on Titan canonical | 1 |
Statements (42)
| Predicate | Object |
|---|---|
| instanceOf |
dune field
ⓘ
planetary surface feature ⓘ |
| atmosphericContext | dense nitrogen-rich atmosphere of Titan ⓘ |
| atmosphericPressureApprox | about 1.5 bar ⓘ |
| belongsToCategory | Titan dune fields ⓘ |
| considered | prime site for astrobiology research on Titan ⓘ |
| contrastsWith | brighter icy terrains on Titan ⓘ |
| discoveredBy |
Cassini–Huygens
ⓘ
surface form:
Cassini–Huygens mission
|
| explorationGoal |
assess habitability
ⓘ
investigate organic chemistry ⓘ study surface-atmosphere interactions ⓘ |
| hasAppearance | dark ⓘ |
| hasComposition | organic-rich sand ⓘ |
| hasExtent | vast area spanning hundreds of kilometers ⓘ |
| hasHostBody |
Saturn
ⓘ
surface form:
Saturn’s moon Titan
|
| hasMorphology |
linear dunes
ⓘ
longitudinal dunes ⓘ |
| hasOrientation | dunes generally aligned east–west ⓘ |
| hasPrimaryConstituent |
hydrocarbon particles
ⓘ
organic aerosols ⓘ |
| isEnvironmentFor | prebiotic chemistry studies ⓘ |
| isOneOf | largest dune fields on Titan ⓘ |
| locatedIn | equatorial region of Titan ⓘ |
| locatedOn | Titan ⓘ |
| namedAfter |
Shangri-La
ⓘ
surface form:
mythical land Shangri-La
|
| observedBy |
Cassini–Huygens
ⓘ
surface form:
Cassini spacecraft
|
| observedUsing |
Cassini–Huygens
ⓘ
surface form:
Cassini RADAR instrument
Cassini–Huygens ⓘ
surface form:
Cassini imaging science subsystem
|
| orbits | Saturn ⓘ |
| partOf | surface of Titan ⓘ |
| relevantTo |
comparative planetology of dunes
ⓘ
organic geochemistry on icy worlds ⓘ |
| scientificInterest |
testing models of sand formation on Titan
ⓘ
understanding transport of organic material on Titan ⓘ |
| shapedBy | Titan atmospheric winds ⓘ |
| similarTo | terrestrial sand seas ⓘ |
| studiedIn |
Cassini radar altimetry
ⓘ
surface form:
Cassini RADAR global mosaics
|
| surfaceGravity | low gravity environment of Titan ⓘ |
| surfaceProcessType | aeolian ⓘ |
| surfaceTemperatureApprox | around 94 K ⓘ |
| targetedBy | NASA Dragonfly mission ⓘ |
| willBeExploredBy | Dragonfly rotorcraft lander ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.