Caloris Basin

E100918

Caloris Basin is one of the largest and youngest impact basins in the Solar System, forming a prominent multi-ringed geological feature on the planet Mercury.

All labels observed (2)

Label Occurrences
Caloris Basin canonical 1
Caloris Planitia (interior plains) 1

How this entity was disambiguated

Statements (36)

Predicate Object
instanceOf impact basin
planetary surface feature
alsoKnownAs Caloris Basin
surface form: Caloris Planitia (interior plains)
diameter approximately 1550 kilometers
discoveredBy Mariner 10
formedBy large asteroid or comet impact
furtherImagedBy MESSENGER
surface form: MESSENGER spacecraft
geologicalAge Late Heavy Bombardment era
hasAlbedoCharacteristic high-reflectance interior plains
hasAntipodalRegion weird terrain of Mercury
hasCoordinateSystemReference Mercury planetocentric coordinates
hasFeature concentric rings
radial graben
smooth plains fill
hasGeologicalType multi-ring basin
hasInteriorPlains volcanic plains
hasScientificInterest key target for future Mercury missions
hasSurroundingRing mountainous annulus
hasTectonicStructures extensional troughs
wrinkle ridges
influencedBy Mercury thermal and tidal history
influences Mercury global tectonics
interiorPlainsComposition basaltic lava flows (inferred)
isOneOf largest impact basins in the Solar System
youngest large impact basins in the Solar System
locatedIn Solar System
locatedOn Mercury
nameGivenBy International Astronomical Union
nameMeaning Caloris means heat in Latin
observedIn infrared wavelengths
visible wavelengths
surfaceAge relatively young compared to surrounding highlands
surroundedBy low-reflectance material
usedFor studies of Mercury volcanism
studies of impact basin formation
studies of planetary tectonics

How these facts were elicited

Referenced by (2)

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

Mercury surfaceFeature Caloris Basin
Caloris Basin alsoKnownAs Caloris Basin
this entity surface form: Caloris Planitia (interior plains)