Sava Vallis

E419819

Sava Vallis is a Martian valley that serves as one of the main ancient river channels feeding into Jezero Crater, a site of significant interest for studying past water activity on Mars.

All labels observed (1)

Label Occurrences
Sava Vallis canonical 1

How this entity was disambiguated

Statements (25)

Predicate Object
instanceOf Martian valley
ancient river channel
valley
associatedWith past water activity on Mars
connectedTo Jezero Crater watershed
contributesTo deltaic deposits in Jezero Crater
evidenceType fluvial erosion features
feedsInto Jezero Crater NERFINISHED
formedBy ancient surface runoff
hasGeologicalSignificance potential transport of sediments into Jezero Crater
hasNameLanguage Latinized nomenclature for Martian feature
locatedOn Mars
mappedBy orbital imaging of Mars
notableFor evidence of ancient fluvial processes
observedUsing Mars Reconnaissance Orbiter imagery
partOf Martian fluvial system
planetaryBody Mars
relatedToMissionTarget Mars 2020 Perseverance rover landing site region
relevantTo reconstruction of ancient Martian climate
search for past habitable environments on Mars
roleInSystem main inlet channel to Jezero Crater
scientificInterest study of Martian paleohydrology
studiedInDiscipline astrobiology
planetary geology
surfaceFeatureType valley network

How these facts were elicited

Referenced by (1)

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

Jezero Crater hasInflowChannels Sava Vallis