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Strange Surfaces in Nilosyrtis Region (PSP_010536_2190)

Strange Surfaces in Nilosyrtis Region
Strange Surfaces in Nilosyrtis Region (PSP_010536_2190)
Credit: NASA/JPL/University of Arizona

This image shows a part of the Nilosyrtis region of Mars, along the “dichotomy boundary” which separates the southern highlands from the low-lying northern plains.

In this region, the boundary is actually a broad region of hills, knobs and mesas, with strange and exotic textures observed on the surface. This is among the northernmost parts of the boundary region; it is thought that under different climate conditions, ice is deposited from the atmosphere here, potentially forming significant glaciers.

Evidence for large-scale glacial flow is not obvious at this site, but many of the enigmatic surface textures may be related to deposition and removal of ice. The variety of textures includes areas with dense patterns of cracks, lumpy and pitted regions, and areas of small, pitted hummocks. Downslope-trending ridges in some places could indicate ice flow but may be due to more complex processes.

Many of the subtle breaks in slope in the area correspond to changes in the surface texture. The formation of many of these features is still not well understood in detail, but it is likely that much of this texture is due to deposition and removal of ice, some of which could still be preserved under a lag deposit of dust and rocks. For instance, polygonal fracture patterns commonly occur in ice-rich ground on both Earth and Mars. Similar textures occur in many parts of the Martian mid-latitudes and indicate past processes which have reworked much of the surface.


Written by: Colin Dundas

OBSERVATION TOOLBOX
Acquisition date:25 October 2008 Local Mars time: 3:23 PM
Latitude (centered):38.5 ° Longitude (East):61.7 °
Range to target site:309.4 km (193.4 miles)Original image scale range:31.0 cm/pixel
(with 1 x 1 binning) so objects ~93 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:19.0 ° Phase angle:70.4 °
Solar incidence angle:51 °, with the Sun about 39 ° above the horizon Solar longitude:147.2 °, Northern Summer
For non-map projected products:
North azimuth:98 ° Sub-solar azimuth:350.9 °
F O R   M A P   P R O J E C T E D   P R O D U C T S
North azimuth:270°Sub solar azimuth165.7°
A N A G L Y P H   P R O D U C T S
Left observation:PSP_009824_2190Convergence angle15.1°

 

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All of the images produced by HiRISE and accessible on this site are within the public domain: there are no restrictions on their usage by anyone in the public, including news or science organizations. We do ask for a credit line where possible: Image: NASA/JPL/University of Arizona


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For information about NASA and agency programs on the Web, visit: http://www.nasa.gov. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, Calif., manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems is the prime contractor for the project and built the spacecraft. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona. The image data were processed using the U.S. Geological Survey’s ISIS3 software.