Ius Chasma

E478303

Ius Chasma is a large, steep-walled canyon on Mars that forms part of the vast Valles Marineris rift system.

All labels observed (1)

Label Occurrences
Ius Chasma canonical 2

How this entity was disambiguated

Statements (45)

Predicate Object
instanceOf canyon
chasma
surface feature on Mars
adjacentTo Melas Chasma
Ophir Chasma
Tithonium Chasma
astronomicalBodyType canyon
belongsToBody Mars
catalogedIn USGS Gazetteer of Planetary Nomenclature
coordinateFrame Mars IAU coordinate system
formationProcess crustal rifting
tectonic extension
geologicalContext rift system
tectonic trough
hasAtmosphereAbove thin Martian atmosphere
hasCharacteristic large
steep-walled
hasCoordinateSystem planetocentric coordinates
hasEnvironment cold and dry
hasFeature faulted and fractured terrain
landslides and mass-wasting deposits
layered rock outcrops
steep canyon walls
hasScientificInterest potential past water-related processes
records tectonic and erosional history of Mars
imagedByInstrument CTX
HiRISE
linked to: HiRISE instrument

THEMIS
linked to: THEMIS instrument
isComponentOf Noctis Labyrinthus–Valles Marineris system
linked to: Noctis Labyrinthus
locatedInHemisphere Martian southern hemisphere
locatedInRegion equatorial region of Mars
locatedOnPlanet Mars
memberOf Valles Marineris rift system
linked to: Valles Marineris
namedAfter Ius (Latin word related to law or right)
observedBy Mariner 9 spacecraft
linked to: Mariner 9

Mars Global Surveyor
Mars Reconnaissance Orbiter
Viking Orbiter
partOf Martian canyon system
Valles Marineris
Valles Marineris canyon complex
linked to: Valles Marineris
studiedInDiscipline geomorphology
planetary geology
surfaceFeatureOf Martian crust
surfaceType rocky

How these facts were elicited

Referenced by (2)

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

Valles Marineris hasSubfeature Ius Chasma
Melas Chasma hasNearbyFeature Ius Chasma