Ligeia Mare

E49257

Ligeia Mare is one of the largest known hydrocarbon seas on Saturn’s moon Titan, composed primarily of liquid methane and ethane.

AI illustration

How this image was made

AI-generated illustration of Ligeia Mare

This AI-generated illustration was produced by black-forest-labs/FLUX.2-dev (1024x1024) from a prompt written by openai/gpt-oss-120b from the entity's label + description.

Prompt

Generate an image of Ligeia Mare (Ligeia Mare is one of the largest known hydrocarbon seas on Saturn’s moon Titan, composed primarily of liquid methane and ethane.)

All labels observed (1)

Label Occurrences
Ligeia Mare canonical 5

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf extraterrestrial sea ⓘ
hydrocarbon sea ⓘ
surface feature on Titan ⓘ
associatedWithProcess Titan methane cycle ⓘ
evaporation and precipitation of hydrocarbons ⓘ
belongsToSystem Saturn system ⓘ
linked to: Saturn
celestialBody Titan ⓘ
chemicalEnvironment reducing ⓘ
composedPrimarilyOf liquid ethane ⓘ
liquid methane ⓘ
contains hydrocarbons ⓘ
coordinateSystem Titan planetocentric coordinates ⓘ
discoveredBy Cassini–Huygens mission ⓘ
linked to: Cassini–Huygens
environmentType cryogenic hydrocarbon environment ⓘ
featureType mare ⓘ
fluidType non-water liquid ⓘ
hasApproximateArea about 126000 square kilometers ⓘ
hasBathymetry measured depths by radar sounding ⓘ
hasNeighbor Kraken Mare ⓘ
Punga Mare ⓘ
hasScientificInterest climate and weather patterns on Titan ⓘ
potential habitability of hydrocarbon solvents ⓘ
hasShoreline complex coastline ⓘ
imagedIn radar wavelengths ⓘ
isLargerThan Lake Superior ⓘ
isOneOf largest known seas on Titan ⓘ
locatedIn northern hemisphere of Titan ⓘ
locatedInAtmosphericContext dense nitrogen–methane atmosphere of Titan ⓘ
locatedNear Titan’s north pole ⓘ
locatedOn Titan ⓘ
mappedBy Cassini radar altimetry ⓘ
linked to: Cassini–Huygens
maximumDepthEstimate hundreds of meters ⓘ
namedAfter Ligeia ⓘ
nameOrigin Ligeia from Greek mythology ⓘ
observedBy Cassini spacecraft ⓘ
linked to: Cassini–Huygens
observedUsing Cassini radar instrument ⓘ
linked to: Cassini–Huygens
orbitsWithPrimary Saturn ⓘ
partOf Titan northern polar lake district ⓘ
phaseOfMethane liquid methane at Titan surface conditions ⓘ
pressureCondition about 1.5 bar at Titan surface ⓘ
studiedFor comparative planetology of seas and lakes ⓘ
prebiotic chemistry ⓘ
surfaceGravityContext low gravity environment of Titan ⓘ
surfaceInteraction contact with Titan icy crust ⓘ
surfaceState liquid ⓘ
temperatureCondition cryogenic ⓘ
temperatureEstimate around 90 to 95 Kelvin ⓘ

How these facts were elicited

Referenced by (5)

Full triples — surface form annotated when it differs from this entity's canonical label.

Titan → majorSea → Ligeia Mare ⓘ
Punga Mare → hasNeighbor → Ligeia Mare ⓘ
Titan → sea → Ligeia Mare ⓘ
subject linked to: Titan (moon of Saturn)