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 ⓘ