Channels East of Olympus Mons
NASA/JPL/University of Arizona
Channels East of Olympus Mons
PSP_005401_1960  Science Theme: Volcanic Processes
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These channels emerge from a fracture system called the Gordii Fossae to the East of Olympus Mons, the largest volcano in the solar system.

The channels bear superficial resemblance to features formed by floods of water. It is most likely that the channels were first carved by water and then coated with lava. However, it is possible that they are purely volcanic in origin. This puzzle will be solved by investigating a number of similar channels across Mars.

The hills are part of the Sulci Gordii, a series of knobs that form an apron around the eastern part of Olympus Mons. It is likely that these hills resulted from a giant landslide as part of the volcano collapsed under its own weight. The lumpy landslide deposit is now partially buried under younger lava flows, many of which seem to have been erupted from fractures around Olympus Mons.
Written by: Laszlo Kestay   (24 November 2010)

This is a stereo pair with PSP_005546_1960.

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Acquisition date:21 September 2007 Local Mars time:14:12
Latitude (centered):16.000° Longitude (East):232.925°
Range to target site:276.8 km (173.0 miles)Original image scale range:27.7 cm/pixel (with 1 x 1 binning) so objects ~83 cm across are resolved
Map projected scale:25 cm/pixel and North is upMap projection:Equirectangular
Emission angle:6.2° Phase angle:41.6°
Solar incidence angle:46°, with the Sun about 44° above the horizon Solar longitude:317.6°, Northern Winter

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