File:Miranda scarp.jpg

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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.
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Source http://photojournal.jpl.nasa.gov/catalog/PIA00044
Author NASA/JPL
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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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This image or video was catalogued by Jet Propulsion Laboratory of the United States National Aeronautics and Space Administration (NASA) under Photo ID: PIA00044.

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Date/TimeThumbnailDimensionsUserComment
current12:06, 3 May 2010Thumbnail for version as of 12:06, 3 May 20101,016 × 1,002 (74 KB)Jeandré du Toit (talk | contribs)Reverted to version as of 16:03, 6 April 2005 per [http://en.wikipedia.org/wiki/File_talk:Miranda_scarp.jpg]
08:18, 7 December 2007Thumbnail for version as of 08:18, 7 December 20071,002 × 1,016 (72 KB)WolfmanSF (talk | contribs)rotate photo 90 deg. counterclockwise so scarp is vertical
16:03, 6 April 2005Thumbnail for version as of 16:03, 6 April 20051,016 × 1,002 (74 KB)Bricktop (talk | contribs)NASA image

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