File:Miranda scarp 90 deg counterclockwise.jpg
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[edit]DescriptionMiranda scarp 90 deg counterclockwise.jpg |
English: This high-resolution image of Miranda was acquired by Voyager 2 on Jan. 24, 1986, when the spacecraft was 36,250 kilometers (22,500 miles) from the Uranian moon. In this clear-filter, narrow-angle image, Miranda displays a dramatically varied surface. Well shown at this resolution of 660 meters (2,160 feet) are numerous ridges and valleys -- a topography that was probably produced by compressional tectonics. Cutting across the ridges and valleys are many faults. The largest fault scarp, or cliff, is seen below and right of center; it shows grooves probably made by the contact of the fault blocks as they rubbed against each other (leaving what are known as slickensides). Movement of the down-dropped block is shown by the offset of the ridges. The fault may be 5 km (3 mi) high, or higher than the walls of the Grand Canyon on Earth.
NOTE: This image is rotated at 90 degrees counterclockwise so the scarp is vertical. |
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Date | |||||||
Source | http://photojournal.jpl.nasa.gov/catalog/PIA00044 | ||||||
Author | NASA/JPL | ||||||
Permission (Reusing this file) |
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Other versions | File:Miranda_scarp.jpg |
This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA00044. This tag does not indicate the copyright status of the attached work. A normal copyright tag is still required. See Commons:Licensing. Other languages:
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current | 11:23, 25 June 2024 | 1,002 × 1,016 (72 KB) | PlanetUser (talk | contribs) | {{Information |Description = {{en|This high-resolution image of Miranda was acquired by Voyager 2 on Jan. 24, 1986, when the spacecraft was 36,250 kilometers (22,500 miles) from the Uranian moon. In this clear-filter, narrow-angle image, Miranda displays a dramatically varied surface. Well shown at this resolution of 660 meters (2,160 feet) are numerous ridges and valleys -- a topography that was probably produced by compressional tectonics. Cutting across the ridges and valleys are many faul... |
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