A Channel Cut into an Impact Crater
NASA/JPL/University of Arizona
A Channel Cut into an Impact Crater
ESP_023825_1855  Science Theme: Volcanic Processes
Greek  Italian  Portuguese  Spanish 


800  1024  
1152  1280  
1440  1600  
1920  2048  


PDF, 11 x 17 in  


This image shows an impact crater in the eastern part of Elysium Planitia. The region is a smooth plain along the equator of Mars, between the rugged Southern highlands and the Elysium volcanic rise.

The plains have been repeatedly covered by lava flows that have filled in most of the low areas, resulting in a remarkably flat region. This particular crater has been surrounded by the youngest large lava flow known on Mars, the Athabasca Valles flood lava.

The lavas have flowed into the crater, through the lowest point in its rim, forming a leveed channel. The bottom of the crater is covered with sand dunes, so it is difficult to tell how much lava poured inside this crater. What is preserved here is one step in the process that has erased many other craters in Elysium Planitia as lava filled craters and other topographic lows.

Written by: Laszlo Kestay   (14 September 2011)

This is a stereo pair with ESP_023535_1855.

Click to share this post on Twitter Click to share this post on Facebook Click to share this post on Google+ Click to share this post on Tumblr

 Image Products: All image links are drag & drop for HiView, or click to download
B&W: map projected  non-map

IRB color: map projected  non-map

Merged IRB: map projected

Merged RGB: map projected

RGB color: non-map projected

B&W: map-projected (498MB)

IRB color: map-projected (213MB)
B&W: map-projected  (218MB),
non-map  (212MB)

IRB color: map projected  (55MB)
non-map  (156MB)

Merged IRB: map projected  (139MB)

Merged RGB: map-projected  (133MB)

RGB color: non map-projected  (146MB)
Map-projected reduced-resolution (PNG)
Full resolution JP2 download
View anaglyph details page

B&W label
Color label
Merged IRB label
Merged RGB label
EDR products

About color products (PDF)
HiView main page

 Observation Toolbox
Acquisition date:26 August 2011 Local Mars time:14:01
Latitude (centered):5.343° Longitude (East):138.871°
Range to target site:308.4 km (192.8 miles)Original image scale range:30.9 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:28.6° Phase angle:60.1°
Solar incidence angle:32°, with the Sun about 58° above the horizon Solar longitude:351.1°, Northern Winter

Context map

Usage Policy
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
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.