Lee–Lincoln scarp
E824739
The Lee–Lincoln scarp is a geologic fault scarp on the Moon located in the Taurus–Littrow valley, explored by the Apollo 17 mission.
Statements (31)
| Predicate | Object |
|---|---|
| instanceOf |
geologic feature
ⓘ
lunar fault scarp ⓘ |
| ageCharacteristic | relatively young lunar tectonic feature ⓘ |
| associatedWith | tectonic activity on the Moon ⓘ |
| country | none (extraterrestrial feature) ⓘ |
| documentedIn |
Apollo 17 mission reports
ⓘ
Apollo 17 surface photographs ⓘ Lunar Reconnaissance Orbiter images ⓘ |
| evidenceFor | recent lunar tectonic activity ⓘ |
| exploredBy | Apollo 17 mission NERFINISHED ⓘ |
| featureOf | Mare Serenitatis region NERFINISHED ⓘ |
| formedBy | compressional tectonics ⓘ |
| hasNearbyFeature |
Camelot crater
NERFINISHED
ⓘ
Nansen crater NERFINISHED ⓘ North Massif NERFINISHED ⓘ Sculptured Hills NERFINISHED ⓘ Shorty crater NERFINISHED ⓘ South Massif NERFINISHED ⓘ |
| locatedIn | Taurus–Littrow valley NERFINISHED ⓘ |
| locatedOn | Moon NERFINISHED ⓘ |
| namedAfter |
Gene Cernan
NERFINISHED
ⓘ
Harrison H. Schmitt NERFINISHED ⓘ |
| observedDuring |
Apollo 17 EVA 2
NERFINISHED
ⓘ
Apollo 17 EVA 3 NERFINISHED ⓘ |
| orientation | roughly north–south trending ⓘ |
| partOf | Taurus–Littrow landing site NERFINISHED ⓘ |
| relatedTo | lunar graben and fault systems ⓘ |
| studiedBy | lunar geologists ⓘ |
| surfaceType | steep slope ⓘ |
| visitedBy |
Eugene A. Cernan
NERFINISHED
ⓘ
Harrison H. Schmitt NERFINISHED ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.