CICLOPS: Cassini Imaging Central Laboratory for OPerationS

Miranda's Geologic History (variety of terrain)
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Miranda reveals a complex geologic history in this view, acquired by Voyager 2 on Jan. 24, 1986, around its close approach to the Uranian moon.

At least three terrain types of different age and geologic style are evident at this resolution of about 700 meters (2,300 feet). Visible in this clear-filter, narrow-angle image are, from left: (1) an apparently ancient, cratered terrain consisting of rolling, subdued hills and degraded medium-sized craters (2) a grooved terrain with linear valleys and ridges developed at the expense of, or replacing, the first terrain type: and (3) a complex terrain seen along the terminator, in which intersecting curvilinear ridges and troughs are abruptly truncated by the linear, grooved terrain. Voyager scientists believe this third terrain type is intermediate in age between the first two.

The Voyager Project is managed for NASA by the Jet Propulsion Laboratory, Pasadena, Calif.

Acquired: January 1986
  Miranda's Geologic History (variety of terrain)
PIA 00141

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Alliance Member Comments
Dragon_of_Luck_Mah_Jonng1971 (Nov 24, 2013 at 6:45 PM):
I suppose that at the grooved terrain of Miranda shown here happened ( is happening ? ) a kind of activity similar to the one on Enceladus and Europa, but not on the same scale.

The image of Saturn seen from above is amazing !

Greetings from the Dragon_of_Luck

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