Layers in Candor Mensa
NASA/JPL-Caltech/UArizona
Layers in Candor Mensa
PSP_010027_1745  Science Theme: Sedimentary/Layering Processes
This image shows layered sedimentary deposits in Candor Mensa, a broad plateau of thickly stacked sedimentary rocks in Candor Chasma, part of the giant troughs of Valles Marineris.

Valles Marineris is a system of tectonic depressions formed by down-dropping faults; the floors are among the lowest points on the surface of Mars, and may have once held lakes. Some sites show evidence for streams or rivers. The troughs may have also been sites of volcanic activity.

Currently, the deep floors contain massive deposits of bright sedimentary rocks. Some of the deposits are several kilometers thick, and have diverse composition and appearance. They were probably formed by many different processes in different environments.

At this site, most of the bright rocks exhibit a scalloped, patterned texture. This is thought to be associated with low-density deposits undergoing wind erosion, although the process is still not well-understood. Despite this relatively uniform texture, some variations are evident. The southern (upper) part of the deposit is relatively uniform, while the central portion appears to have thin layers.

On close inspection, the layers near the center of the image are all composed of the same material; they are probably visible due to slight topographic steps caused by variations in the strength of the rock. The layers have been highlighted by a mantle of dark, wind-blown sand ripples, which cover the flat parts of the stepped structure. At low resolution, this gives the appearance of alternating light and dark layers.

In the northernmost part of the image, the sediments have an entirely different texture, ranging from massive to fractured. These sediments also show evidence of layering.

Interpretation of these sediments is complicated by younger mantling materials. In addition to the sand ripples (some of which may have hardened to rock), a relatively massive dark layer appears to cap or drape the deposit in many places, including the southern part of this image.



Written by: Colin Dundas  (12 November 2008)

This is a stereo pair with PSP_009038_1745.
 
Acquisition date
15 September 2008

Local Mars time
15:38

Latitude (centered)
-5.556°

Longitude (East)
286.756°

Spacecraft altitude
262.7 km (163.3 miles)

Original image scale range
27.2 cm/pixel (with 1 x 1 binning) so objects ~82 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
13.2°

Phase angle
48.8°

Solar incidence angle
59°, with the Sun about 31° above the horizon

Solar longitude
127.7°, Northern Summer

For non-map projected images
North azimuth:  93°
Sub-solar azimuth:  32.3°
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   (1144MB)

IRB color
map-projected   (520MB)

JP2 EXTRAS
Black and white
map-projected  (586MB)
non-map           (556MB)

IRB color
map projected  (189MB)
non-map           (484MB)

Merged IRB
map projected  (263MB)

Merged RGB
map-projected  (270MB)

RGB color
non map           (454MB)
ANAGLYPHS
Map-projected, reduced-resolution
Full resolution JP2 download
Anaglyph details page

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

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:
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.