Verona Rupes

E502405

Verona Rupes is an enormous, possibly the tallest known, cliff on Uranus’s moon Miranda, plunging several kilometers from its rim to the surface below.

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Statements (31)

Predicate Object
instanceOf cliff
geological formation
surface feature on a natural satellite
approximateHeight 5 km to 20 km (estimates vary)
astronomicalBodyTypeOfHost moon Miranda NERFINISHED
astronomicalBodyTypeOfPrimary planet Uranus NERFINISHED
belongsTo Miranda’s complex tectonic terrain
characterizedAs enormous cliff
classification planetary scarp
comparativeScale often cited as possibly the tallest cliff in the Solar System
compositionContext likely associated with water-ice rich crust
discoveredBy Voyager 2 spacecraft imaging
environment airless, extremely cold surface of Miranda
etymology named after Verona, setting of Shakespeare’s play Romeo and Juliet
featureType rupes (scarp)
freeFallTimeFromTop several minutes due to Miranda’s low gravity (order of 10 minutes)
hostBodyOrbits Uranus in a prograde, inclined orbit
imagedBy Voyager 2 NERFINISHED
knownFrom remote sensing imagery
locatedIn Uranus system NERFINISHED
locatedInRegion southern hemisphere of Miranda (approximate)
locatedOn Miranda
namingTheme Shakespearean characters and places on Miranda
notableFor being one of the tallest known cliffs in the Solar System
orbitsWith Uranus NERFINISHED
relativeLocationDescription sheer cliff dropping from rim to lower surrounding terrain
scientificInterest evidence for Miranda’s tectonic and possibly resurfacing history
solarSystemBodyType feature on an icy moon
solarSystemRegion outer Solar System
surfaceDrop several kilometers
surfaceGravityContext low gravity environment of Miranda

Referenced by (1)

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

Miranda notableCliff Verona Rupes