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.
Name | Value | Additional Values |
---|---|---|
Target | Miranda | |
System | Uranus | |
Target Type | Satellite | |
Mission | Voyager | |
Instrument Host | Cassini Orbiter | Voyager 2 |
Host Type | Orbiter | Flyby Spacecraft |
Instrument | Imaging Science Subsystem (ISS) | |
Detector | Narrow Angle Camera | |
Extra Keywords | Grayscale, Visual | |
Acquisition Date | ||
Release Date | 1996-01-29 | |
Date in Caption | 1986-01-24 | |
Image Credit | NASA/JPL | |
Source | photojournal.jpl.nasa.gov/catalog/PIA00044 | |
Identifier | PIA00044 |