Ophir Chasma

E485881

Ophir Chasma is a large, steep-walled canyon on Mars forming part of the northern section of the vast Valles Marineris canyon system.

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Statements (48)

Predicate Object
instanceOf canyon
chasma
surface feature on Mars
connectedTo Candor Chasma NERFINISHED
Melas Chasma NERFINISHED
Tithonium Chasma NERFINISHED
containsGeologicalUnit dune fields
landslide aprons
layered deposits
massive bedrock
featureTypeInGazetteer chasma
formedByProcess crustal rifting
tectonic extension
hasAtmosphereAbove thin carbon-dioxide-dominated Martian atmosphere
hasCoordinateSystem planetocentric latitude/longitude
hasEnvironment cold desert
hasFloorCharacteristic chaotic terrain in parts
relatively flat floor in places
tectonically disrupted floor
hasMorphology canyon-like trough
hasScientificDiscipline geomorphology
planetary geology
hasSideCharacteristic landslide deposits
terraced walls
hasWallCharacteristic steep-walled
imagedByInstrument CTX NERFINISHED
HiRISE NERFINISHED
THEMIS NERFINISHED
isComponentOf equatorial canyon belt of Mars
locatedInHemisphere Martian southern hemisphere
Martian western hemisphere
locatedInRegion northern Valles Marineris
locatedOnPlanet Mars NERFINISHED
modifiedByProcess aeolian erosion
landsliding
mass wasting
namedAfter Ophir (biblical region) NERFINISHED
namingAuthority International Astronomical Union NERFINISHED
observedByMission Mariner 9 NERFINISHED
Mars Global Surveyor NERFINISHED
Mars Odyssey NERFINISHED
Mars Reconnaissance Orbiter NERFINISHED
Viking Orbiter NERFINISHED
partOf Valles Marineris NERFINISHED
partOfSystem Valles Marineris canyon system NERFINISHED
scientificInterest potential evidence for past water-related processes
records tectonic and erosional history of Valles Marineris
surfaceType rocky

Referenced by (1)

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

Valles Marineris hasSubfeature Ophir Chasma