Sorted Boulders
NASA/JPL-Caltech/UArizona
Sorted Boulders
ESP_021862_1175  Science Theme: Rocks and Regolith
Fields of boulders are sometimes found in high latitude patches, distinct from neighboring smooth and relatively rock-free plains.

The origins of these boulder fields is not entirely clear, but may be the result of a thinner soil layer overlying the eroding bedrock. They may also be the result of a number of more ancient geologic processes. For example, glacial bulldozing of surface rocks can push and drop rocks gathered from some distance away. Some volcanic flows may generate a rough and broken rocky surface, later mantled with soil.

Unusual to this boulder field is the sorting of these rocks into small rings, arcs, and clusters. On Earth, sorting of rocks is common in frozen climates, though usually on a smaller scale. Rock sorting can result from cyclic freezing and thawing of water in the soil.

Alternatively, in a deeply cold environment such as Mars, permanently subfreezing temperature still undergo seasonal heating and cooling which may be capable of driving extremely slow convection cycles in the ice-rich soil. These cycles then collect rocks and boulders at the surface in areas where the finer soil is downwelling into the soil subsurface.

Written by: Mike Mellon  (20 April 2011)
 
Acquisition date
26 March 2011

Local Mars time
15:14

Latitude (centered)
-62.189°

Longitude (East)
104.116°

Spacecraft altitude
249.2 km (154.9 miles)

Original image scale range
24.9 cm/pixel (with 1 x 1 binning) so objects ~75 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
0.3°

Phase angle
49.4°

Solar incidence angle
49°, with the Sun about 41° above the horizon

Solar longitude
262.2°, Northern Autumn

For non-map projected images
North azimuth:  98°
Sub-solar azimuth:  32.2°
JPEG
Black and white
map projected  non-map

IRB color
map projected  non-map

Merged IRB
map projected

Merged RGB
map projected

RGB color
non-map projected

JP2
Black and white
map-projected   (546MB)

IRB color
map-projected   (233MB)

JP2 EXTRAS
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map-projected  (206MB)
non-map           (365MB)

IRB color
map projected  (65MB)
non-map           (255MB)

Merged IRB
map projected  (139MB)

Merged RGB
map-projected  (135MB)

RGB color
non map           (247MB)
ADDITIONAL INFORMATION
B&W label
Color label
Merged IRB label
Merged RGB label
EDR products
HiView

NB
IRB: infrared-red-blue
RGB: red-green-blue
About color products (PDF)

Black & white is 5 km across; enhanced color about 1 km
For scale, use JPEG/JP2 black & white map-projected images

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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:
NASA/JPL-Caltech/UArizona

POSTSCRIPT
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. The HiRISE camera was built by Ball Aerospace and Technology Corporation and is operated by the University of Arizona.