Pliva Vallis
E424256
Pliva Vallis is an ancient Martian valley system interpreted as a former river channel that once drained water from Jezero Crater.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Pliva Vallis canonical | 1 |
Statements (27)
| Predicate | Object |
|---|---|
| instanceOf |
Martian valley
ⓘ
ancient river channel ⓘ |
| associatedWith |
Jezero Crater
ⓘ
surface form:
Jezero Crater delta system
|
| connectedTo | Jezero Crater ⓘ |
| considered | potential former outflow channel from Jezero Crater ⓘ |
| drainsFrom | Jezero Crater ⓘ |
| evidenceFor |
ancient Martian hydrologic activity
ⓘ
past surface water on Mars ⓘ |
| formedBy | fluvial erosion ⓘ |
| formedIn | Martian past ⓘ |
| hasMorphology |
sinuous channel
ⓘ
valley network ⓘ |
| hasScientificInterest |
record of Martian surface hydrology
ⓘ
record of ancient Martian climate ⓘ |
| interpretedAs | former river channel ⓘ |
| locatedOn | Mars ⓘ |
| mentionedIn | Mars fluvial geomorphology studies ⓘ |
| observedBy |
Mars Global Surveyor
ⓘ
Mars Reconnaissance Orbiter ⓘ |
| observedUsing | orbital imagery ⓘ |
| partOf | Martian fluvial systems ⓘ |
| planetaryBody | Mars ⓘ |
| relevantTo |
astrobiology on Mars
ⓘ
paleolake in Jezero Crater ⓘ |
| studiedInContextOf | Mars 2020 Perseverance rover landing site ⓘ |
| surfaceFeatureOf | Martian highlands and lowlands transition region ⓘ |
| usedAs | constraint on Jezero Crater paleolake level ⓘ |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.