Image:Miranda scarp rotated.jpg
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[edit] Summary
Description |
Miranda High Resolution of Large Fault 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. The Voyager project is managed for NASA by the Jet Propulsion Laboratory. |
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January 24, 1986 |
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NASA/JPL |
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Permission (Reusing this image) |
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Template:NASA-image
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Date/Time | Dimensions | User | Comment | |
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current | 14:14, 11 January 2008 | 1,016×1,002 (78 KB) | Rubble pile (Talk | contribs) | ({{Information |Description= |Source=NASA |Date=1986 |Location= |Author= |Permission=Public domain |other_versions= }}) |
14:12, 11 January 2008 | 1,002×1,016 (72 KB) | Rubble pile (Talk | contribs) | ({{Information |Description=Verona Rupes on Miranda (rotated) |Source=NASA |Date= |Location= |Author= |Permission=Public domain |other_versions= }}) |
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