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Verona Rupes

Coordinates:18°18′S347°48′E / 18.3°S 347.8°E /-18.3; 347.8
From Wikipedia, the free encyclopedia
Tallest cliff in the solar system

18°18′S347°48′E / 18.3°S 347.8°E /-18.3; 347.8

Verona Rupes
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Verona Rupes, right of center,[1] photographed byVoyager 2 in January 1986.
Feature typeScarp
LocationMiranda
Coordinates18°18′S347°48′E / 18.30°S 347.80°E /-18.30; 347.80[2]
Diameter116.0 km (72.1 mi)
Peak
  • 5–15 km (3.1–9.3 mi)[3]
  • 5–10 km (3.1–6.2 mi)[4]
  • 20 km (12 mi)[5]
DiscovererVoyager 2
EponymVerona, the setting forRomeo and Juliet

Verona Rupes is the tallest knowncliff onMiranda, a moon ofUranus, and plausibly holds the record for the highest cliff in theSolar System. It was discovered by theVoyager 2 space probe in January 1986. Its name was adopted by theInternational Astronomical Union (IAU) in 1988, named after the city ofVerona, which is the setting for several plays byWilliam Shakespeare.[2] It may have been created by a major impact that caused the moon to disrupt and reassemble,[6][7] or by the crust rifting.[8] Given Miranda's low gravity, it would take about 12 minutes to fall from the top, reaching the bottom at a speed of about 200 km/h.[5]

There are many estimates about the cliff's height. It was thought its height was between 5 and 10 km (3 and 6 mi)[4] high, while another places it at a higher altitude of 20 km (12 mi),[5] potentially making it the tallest known cliff in theSolar System. One study estimated that the "true" height of Verona Rupes is around 5 to 15 km (3 to 9 mi) when not accounting for oblique viewing caused byparallax, gradually getting more shallow towards the terminator.[3] It may be presumed that the scarp extends beyond theterminator, into the northern hemisphere, where theVoyager 2 probe could not see.[9] The scarp's slope with regard to the dark limb that extends past the terminator is estimated to be around 25 to 30 degrees.[3]

References

[edit]
  1. ^"PIA00044: Miranda high resolution of large fault". JPL, NASA. Retrieved2007-07-23.
  2. ^ab"Verona Rupes".Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  3. ^abc"1991LPI....22.1341S Page 1341".adsabs.harvard.edu. Retrieved2024-08-04.
  4. ^abThomas, P.C. (1988). "Radii, shapes, and topography of the satellites of Uranus from limb coordinates".Icarus.73 (3):427–441.Bibcode:1988Icar...73..427T.doi:10.1016/0019-1035(88)90054-1.
  5. ^abc"APOD: 2016 November 27 - Verona Rupes: Tallest Known Cliff in the Solar System".apod.nasa.gov. Retrieved2018-02-20.
  6. ^"Miranda".USGS. 2003-05-08. Archived fromthe original on July 4, 2003. Retrieved2006-11-28.
  7. ^Chaikin, Andrew (2001-10-16)."Birth of Uranus' provocative moon still puzzles scientists".space.com. Imaginova Corp. p. 1. Archived fromthe original on July 9, 2008. Retrieved2007-07-23.
  8. ^Chaikin, Andrew (2001-10-16)."Birth of Uranus' provocative moon still puzzles scientists".space.com. Imaginova Corp. p. 2. Retrieved2007-07-23.
  9. ^Plescia, J. B. (1988-03-01)."Cratering history of Miranda: Implications for geologic processes".Icarus.73 (3):442–461.doi:10.1016/0019-1035(88)90055-3.ISSN 0019-1035.
  • Listed in approximately increasing distance fromUranus
Inner
Major (spheroid)
Outer (irregular)
Caliban group (3)
Margaret (1)
Other retrograde moons (6)
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