Gullies on Gorgonum Chaos Mesas
NASA/JPL-Caltech/UArizona
Gullies on Gorgonum Chaos Mesas
PSP_001948_1425  Science Theme: Fluvial Processes
This observation shows part of Gorgonum Chaos, a large cluster of chaotic terrain found in the Southern Hemisphere.

Many regions of chaotic terrain are found at the head of large outflow channels that were scoured by ancient floods. Gorgonum Chaos is one region that is not associated with an outflow channel.

Chaotic terrain can form when subsurface volatiles (such as water) are catastrophically released and the overlying surface collapses. It is not known whether isolated chaotic terrain—such as that shown in this image—formed in the same way that the chaotic terrain near the outflow channels did. Wind erosion might play a role in their formation.

Gorgonum Chaos is an especially interesting area because gullies thought to have been eroded by liquid water are located on its mesas (see subimage). The gullies have a wide range of orientations and many appear to emanate from a distinct layer in the mesas (see subimage).

It is not known why gullies form on one slope rather than another, but insolation (amount of sunlight received), availability of water, and regional slope are possible contributing factors.



Written by: Kelly Kolb  (21 March 2007)
 
Acquisition date
26 December 2006

Local Mars time
15:43

Latitude (centered)
-37.052°

Longitude (East)
189.529°

Spacecraft altitude
254.3 km (158.1 miles)

Original image scale range
25.5 cm/pixel (with 1 x 1 binning) so objects ~77 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
3.7°

Phase angle
73.5°

Solar incidence angle
70°, with the Sun about 20° above the horizon

Solar longitude
156.4°, Northern Summer

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  35.4°
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   (976MB)

IRB color
map-projected   (473MB)

JP2 EXTRAS
Black and white
map-projected  (356MB)
non-map           (627MB)

IRB color
map projected  (131MB)
non-map           (488MB)

Merged IRB
map projected  (232MB)

Merged RGB
map-projected  (234MB)

RGB color
non map           (447MB)
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.