Copernican System of lunar stratigraphy

E373199

The Copernican System of lunar stratigraphy is the youngest major geologic time division on the Moon, characterized by relatively fresh impact craters with bright ray systems and minimal space weathering.

All labels observed (1)

Label Occurrences
Copernican System of lunar stratigraphy canonical 1

How this entity was disambiguated

Statements (30)

Predicate Object
instanceOf lunar geologic time system
stratigraphic system
appliesTo Moon
associatedWith high optical maturity contrast between rays and background
post-mare impact cratering
characterizedBy bright crater ray systems
minimal space weathering of surface materials
relatively fresh impact craters
contrastedWith older, more weathered lunar terrains
definedBy lack of significant ray degradation
presence of high-albedo crater rays
distinguishedFrom Eratosthenian System by presence of bright rays
follows Eratosthenian System of lunar stratigraphy
hasBoundaryCriterion craters with rays that are still optically bright
hasDeposits fresh impact ejecta
hasKeyIndicator persistence of bright rays over large distances
sharp crater morphologies
hasRelativeAge youngest lunar surface units
hasSurfaceFeatureState minimal smoothing by regolith processes
hasSurfaceProperty relatively high albedo compared to older units
hasWeatheringState limited micrometeorite gardening effects
limited solar wind darkening
includes their associated ray systems
young rayed craters
isYoungestDivisionOf major lunar geologic time divisions
partOf lunar geologic timescale
usedFor correlating young lunar surface units
relative dating of lunar impact craters
usedIn lunar geologic mapping
lunar stratigraphy

How these facts were elicited

Referenced by (1)

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

Kepler (lunar crater) belongsTo Copernican System of lunar stratigraphy