Rubin Ridge on Mars

E44739

Rubin Ridge on Mars is a geologic feature on the Martian surface named in honor of pioneering astronomer Vera Rubin, recognized for her groundbreaking work on galaxy rotation and dark matter.

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All labels observed (1)

Label Occurrences
Rubin Ridge on Mars canonical 2

Statements (46)

Predicate Object
instanceOf geologic feature
ridge
alsoKnownAs Vera Rubin Ridge
associatedWith dark matter research legacy of Vera Rubin
search for past habitable environments on Mars
composition sedimentary rocks
contextWithinMission intermediate waypoint on Curiosity ascent of Mount Sharp
discoveredBy orbital imaging prior to Curiosity landing
exploredBy Curiosity rover
featureType sedimentary rock ridge
hasStratigraphicPosition overlies Murray formation units of Mount Sharp
underlies younger units higher on Mount Sharp
honors Vera Rubin
hosted multiple Curiosity drill targets
investigatedFor mineralogy
potential habitability indicators
stratigraphy
locatedIn Gale Crater
locatedInHemisphere Martian southern hemisphere
locatedOn Mars
mappedBy Mars Reconnaissance Orbiter
surface form: Mars Reconnaissance Orbiter CRISM spectrometer

Mars Reconnaissance Orbiter
surface form: Mars Reconnaissance Orbiter HiRISE camera
namedAfter Vera Rubin
namedBy International Astronomical Union
notableFor distinctive color and texture compared to surrounding terrain
evidence of past water-related processes
observedByInstrument APXS on Curiosity rover
CheMin
surface form: CheMin on Curiosity rover

ChemCam
surface form: ChemCam on Curiosity rover

DAN on Curiosity rover
MAHLI
surface form: MAHLI on Curiosity rover

Mastcam
surface form: Mastcam on Curiosity rover

SAM on Curiosity rover
partOf Curiosity rover traverse route
Gale Crater stratigraphic sequence
Gale Crater
surface form: Mount Sharp
planet Mars
region Gale Crater
surface form: Aeolis region of Mars
scientificGoalAtSite characterize mineralogy related to red and gray color variations
search for organic molecules in drilled samples
scientificInterest ancient environmental conditions in Gale Crater
long-term climate history of Mars
showsEvidenceOf erosional processes
layered sedimentary bedding
studiedByMission Mars Science Laboratory
surface rocky

Referenced by (2)

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

Vera Rubin hasHonorificName Rubin Ridge on Mars
Vera hasNamesake Rubin Ridge on Mars
subject surface form: Vera Rubin