HiRISE: High Resolution Imaging Science Experiment                  The University of Arizona
Home  New Images  Catalog  Anaglyphs  Stereo Pairs  Science in Motion  FAQ  HiBLOG  Themes  Software  Contact  Search


Enigmatic Terrain in Hellas Basin (PSP_009548_1420)

Enigmatic Terrain in Hellas Basin
Enigmatic Terrain in Hellas Basin (PSP_009548_1420)
Credit: NASA/JPL/University of Arizona

Hellas Planitia is the low-lying plain on the floor of the Hellas Basin, an ancient impact crater over 2000 kilometers wide. This basin includes the lowest point on the surface of Mars.

A variety of unusual landforms occur on the floor of the basin due to the low elevation. One hypothesis is that Hellas may once have held lakes or seas, possibly with thick ice that might account for some of these features.

This image shows a small portion of western Hellas, in a region of enigmatic ridges. These ridges form an intricate pattern, enclosing kilometer-wide depressions. These strange features are still not well-understood; one possibility is that they formed in lake-bottom sediments when ice covering the lake touched bottom and shoved wet, loose material to the side. This HiRISE image reveals that the ridges contain many boulders; sediments deposited on the bottom of a lake might be fine-grained, although they may have hardened to rock later. The image also shows lineations, probably outcropping layers, running between the large ridges.

Because the resolution of HiRISE images is sufficient to see details such as the abundance of boulders and the presence of thin sedimentary layers, images of this and other poorly-understood terrains will be important in interpreting the geological and climatological history of Mars.

This observation is part of a stereo pair along with PSP_007834_1420.
Written by: Colin Dundas

OBSERVATION TOOLBOX
Acquisition date:09 August 2008 Local Mars time: 3:45 PM
Latitude (centered):-37.6 ° Longitude (East):49.5 °
Range to target site:280.0 km (175.0 miles)Original image scale range:56.0 cm/pixel
(with 2 x 2 binning) so objects ~168 cm across are resolved
Map projected scale:50 cm/pixel and north is upMap projection:EQUIRECTANGULAR
Emission angle:22.8 ° Phase angle:66.3 °
Solar incidence angle:81 °, with the Sun about 9 ° above the horizon Solar longitude:110.3 °, Northern Summer
For non-map projected products:
North azimuth:97 ° Sub-solar azimuth:49.3 °
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 azimuth218.4°
A N A G L Y P H   P R O D U C T S
Right observation:PSP_007834_1420Convergence angle17.5°

 

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

SCIENCE THEME
Glacial/Periglacial Processes

STEREO PAIR
PSP_007834_1420

IMAGE PRODUCT INFORMATION
Grayscale label description
Color product label
EDR products


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


TRANSLATE

U S A G E   P O L I C Y

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


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.