Murray formation

E803492

The Murray formation is a sedimentary rock unit on Mars within Gale Crater, studied by the Curiosity rover for its record of ancient lake and habitable environments.

All labels observed (1)

Label Occurrences
Murray formation canonical 3

How this entity was disambiguated

Statements (47)

Predicate Object
instanceOf geologic formation ⓘ
sedimentary rock unit ⓘ
age Hesperian ⓘ
analyzedFor geochemistry ⓘ
mineralogy ⓘ
sedimentology ⓘ
composedPrimarilyOf fine-grained sandstone ⓘ
mudstone ⓘ
siltstone ⓘ
contains drill targets ⓘ
multiple stratigraphic members ⓘ
containsEvidenceOf concretions ⓘ
cross-bedding ⓘ
diagenetic alteration ⓘ
hematite ⓘ
laminated bedding ⓘ
long-lived liquid water ⓘ
low-energy depositional environments ⓘ
mudcracks ⓘ
nodules ⓘ
silica enrichment ⓘ
stratified lake deposits ⓘ
sulfate minerals ⓘ
depositionalEnvironment deltaic to lacustrine settings ⓘ
lake bottom ⓘ
exploredSince 2014 ⓘ
hostRockFor organic-matter detections by Curiosity ⓘ
interpretedAs lacustrine sedimentary sequence ⓘ
locatedIn Gale Crater ⓘ
locatedOn Mars ⓘ
namedAfter Bruce C. Murray ⓘ
observedByInstrument APXS ⓘ
CheMin ⓘ
ChemCam ⓘ
DAN ⓘ
MAHLI ⓘ
Mastcam ⓘ
overlies Bradbury group ⓘ
partOf Mount Sharp ⓘ
partOfMission Mars Science Laboratory mission ⓘ
records ancient lake environments ⓘ
habitable environments ⓘ
significance key record of ancient Martian habitability ⓘ
studiedBy Curiosity rover ⓘ
thickness hundreds of meters ⓘ
underlies Siccar Point group ⓘ
Vera Rubin Ridge ⓘ

How these facts were elicited

Referenced by (3)

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

Vera Rubin Ridge → isStratigraphicallyAbove → Murray formation ⓘ
Aeolis Mons → contains → Murray formation ⓘ
Mount Sharp → hasStratigraphicSequence → Murray formation ⓘ