Crater Ejecta in Utopia Region
NASA/JPL/University of Arizona

Crater Ejecta in Utopia Region
PSP_010100_2165  Science Theme: Glacial/Periglacial Processes


Wallpaper
800  
1024  
1152  
1280  
1440  
1600  
1920  
2048  
2560  

HiFlyer
PDF, 11 x 17 in  

This image of a crater in the Utopian region can be described as what happens when heat produced from an impact comes into contact with Mars’ icy surface.

Since the surface temperature of Mars is well below the freezing point of water, Mars’ soil is a mixture of soil and permafrost. When this impact occurred, a great deal of energy in the form of heat was released onto the surface, creating a melted feature in the bright icy soil. This melting and then refreezing of the ice (as the impact cooled) caused what is known as a periglacial formation. This is depicted towards the middle of the image where the ejecta blanket lays.

This is likely a geologically newer surface since the only impacts disrupting the image are a few small craters that are mostly towards the bottom left-hand side of the full image. The fact the ejecta blanket is still intact and not fully collapsed supports the idea that is it a newer surface feature as it has not been affected by erosional processes.

Note: this caption was written by student Laura Woodbury.Written by: Laura Woodbury/Circe Verba   (20 May 2009)



 Image Products: All image links are drag & drop for HiView, or click to download
JPEG
Grayscale: map projected  non-map
IRB color: map projected  non-map
Merged IRB: map projected
Merged RGB: map projected
RGB color: non-map projected

JP2 DOWNLOAD
Grayscale: map-projected (497.6 MB)
IRB color: map-projected (262.4 MB)

JP2 EXTRAS
Grayscale: map-projected  (240.2 MB),
non-map  (166.1 MB)

IRB color: map projected  (81.9 MB)
non-map  (214.0 MB)

Merged IRB: map projected  (151.1 MB)
Merged RGB: map-projected  (145.3 MB)
RGB color: non map-projected  (199.2 MB)
Additional Image Information
Grayscale label   Color label
Merged IRB label   Merged RGB label
EDR products

About color products (PDF)
HiView main page
HiRISE Online Image Viewer

 Observation Toolbox
Acquisition date:21 September 2008 Local Mars time: 3:28 PM
Latitude (centered):36.3 degrees Longitude (East):87.7 degrees
Range to target site:296.0 km (185.0 miles)Original image scale range:from 29.6 cm/pixel (with 1 x 1 binning) to 59.2 cm/pixel (with 2 x 2 binning)
Map projected scale:25 cm/pixel and North is upMap projection:EQUIRECTANGULAR
Emission angle:2.7 degrees Phase angle:45.9 degrees
Solar incidence angle:49 degrees, with the Sun about 41 degrees above the horizon Solar longitude:130.4 degrees, Northern Summer
For non-map projected products:
North azimuth:97 degrees Sub-solar azimuth:358.5 degrees
For map-projected products
North azimuth:270 degreesSub solar azimuth:173.7 degrees

    Nearby observations

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
Postscript
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.