HiRISE: High Resolution Imaging Science Experiment          The University of Arizona
Home  New Images  Catalog  Science in Motion  FAQ  HiBLOG  Outreach  Mobile  Themes  Tools  Contact  Search


Wrinkle Ridges in Western Elysium Planitia
Wrinkle Ridges in Western Elysium Planitia
Wrinkle Ridges in Western Elysium Planitia  (PSP_007896_1890)
Credit: NASA/JPL/University of Arizona

This image shows “wrinkle” ridges running north to south across the lava-covered plains of Elysium Planitia.

Wrinkle ridges are tectonic landforms produced by lateral compression, or shortening. They are typically snaking, irregular ridges that can branch apart and rejoin. The wrinkle ridges in this image are in some of the youngest lavas on Mars. The lavas erupted from a fissure at the head of the Athabasca Valles channel system between one million and two hundred million years ago.

In the main, it looks as if these ridges existed before lava flooded the region. For example, some parts of the ridge crests are not covered by lava, suggesting that they were already topographically high features. Similarly, the surface of the lava flow is jagged and rough (indicating that the flow-top crumpled) on either side of the wrinkle ridges, but relatively smooth between and immediately downstream (east) of the ridges. This suggests that the wrinkle ridges acted as obstacles, slowing the flow of the lava.

However, there are also hints that the wrinkle ridges deformed the lava flow after it had solidified. On the east face of the western wrinkle ridge and near the top (north) of the HiRISE image (it looks as if these ridges existed beforesee the subimage), the lava flow is broken at the base of the ridge. It seems likely that although the wrinkle ridges were largely formed before lava covered the region, they continued to be uplifted after the cessation of volcanism.


OBSERVATION TOOLBOX
Acquisition date:02 April 2008 Local Mars time: 3:03 PM
Latitude (centered):8.7 ° Longitude (East):150.7 °
Range to target site:280.3 km (175.2 miles)Original image scale range:28.0 cm/pixel
(with 1 x 1 binning) so objects ~84 cm across are resolved
Map projected scale:25 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:8.7 ° Phase angle:38.1 °
Solar incidence angle:46 °, with the Sun about 44 ° above the horizon Solar longitude:53.4 °, Northern Spring
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:25.0 °
For map projected products:
North azimuth:270°Sub solar azimuth199.314°

 

....................

IMAGE PRODUCT INFORMATION
Grayscale label description
Color product label
EDR products


SUBIMAGES IN THIS OBSERVATION

(7.4MB)

SCIENCE THEME
Tectonic Processes


RESOURCES
About color products (PDF)
IAS Viewer help
HiRISE Online Image Viewer


WALLPAPER
800x600
1024x768
1152x864
1280x960
1440x1080
1600x1200
1920x1440
2048x1536
2560x1600


REFERENCE SHEET
PDF Reference Sheet


Share on Facebook



P O S T S C R I P T

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.