PIA09632: Gullies on Gorgonum Chaos Mesas


Gullies on Gorgonum Chaos Mesas

Caption:

Click here for larger version of PIA09632
Click on image for larger version

This HiRISE image ( PSP_001948_1425 ) 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); scene is approximately 4 km across). 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.

Observation Toolbox
Acquisition date: 12 December 2006
Local Mars time: 3:43 PM
Degrees latitude (centered): -37.1°
Degrees longitude (East): 189.5°
Range to target site: 254.9 km (159.3 miles)
Original image scale range: 25.5 cm/pixel (with 1 x 1 binning) so objects ~76 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 Autumn

Background Info:

NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, is the prime contractor for the project and built the spacecraft. The High Resolution Imaging Science Experiment is operated by the University of Arizona, Tucson, and the instrument was built by Ball Aerospace and Technology Corp., Boulder, Colo.

Cataloging Keywords:

Name Value Additional Values
Target Mars
System
Target Type Planet
Mission Mars Reconnaissance Orbiter (MRO)
Instrument Host Mars Reconnaissance Orbiter
Host Type Orbiter
Instrument High Resolution Imaging Science Experiment (HiRISE)
Detector
Extra Keywords Grayscale, Infrared, Map, Water
Acquisition Date
Release Date 2007-03-21
Date in Caption 2006-12-12
Image Credit NASA/JPL/Univ. of Arizona
Source photojournal.jpl.nasa.gov/catalog/PIA09632
Identifier PIA09632