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.

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Statements (47)

Predicate Object
instanceOf geologic formation
sedimentary rock unit
age Hesperian NERFINISHED
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 NERFINISHED
locatedOn Mars NERFINISHED
namedAfter Bruce C. Murray NERFINISHED
observedByInstrument APXS NERFINISHED
CheMin NERFINISHED
ChemCam NERFINISHED
DAN NERFINISHED
MAHLI NERFINISHED
Mastcam NERFINISHED
overlies Bradbury group NERFINISHED
partOf Mount Sharp NERFINISHED
partOfMission Mars Science Laboratory mission NERFINISHED
records ancient lake environments
habitable environments
significance key record of ancient Martian habitability
studiedBy Curiosity rover NERFINISHED
thickness hundreds of meters
underlies Siccar Point group NERFINISHED
Vera Rubin Ridge NERFINISHED

Referenced by (2)

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

Aeolis Mons contains Murray formation
Vera Rubin Ridge isStratigraphicallyAbove Murray formation