Chloride Salt Deposits within a Channel in Terra Sirenum
NASA/JPL-Caltech/UArizona
Chloride Salt Deposits within a Channel in Terra Sirenum
PSP_009318_1465  Science Theme: Composition and Photometry
This image shows a series of knobs, channels and inverted channels in the ancient Southern highlands of Mars.

The inverted channels, which now appear as sinuous ridges, are filled with a fractured light-toned material that is also apparent in the knobs and nearby bedrock. Previous analyses of the infrared data from TES and THEMIS of similar materials in Terra Sirenum and elsewhere on Mars suggest that these light-toned materials are deposits of chloride salts such as sodium chloride (ordinary rock salt).

Salt deposits are key targets in the search for ancient life on Mars, because they represent places where bodies of liquid water may have ponded and evaporated. The salt forms an ideal setting in which to preserve signs of biological activity. The clear association of the salt with the sinuous channels visible here suggests that the material was precipitated from brines that once flowed through these channels. The fractured surface of the deposits is consistent with cracking by desiccation (rapid drying) of the thick salts as they were deposited.



Written by: Paul Geissler and Livio Tornabene  (27 August 2008)

This is a stereo pair with ESP_017243_1465.
 
Acquisition date
22 July 2008

Local Mars time
15:30

Latitude (centered)
-33.421°

Longitude (East)
205.481°

Spacecraft altitude
255.1 km (158.5 miles)

Original image scale range
51.4 cm/pixel (with 2 x 2 binning) so objects ~154 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
6.7°

Phase angle
81.3°

Solar incidence angle
77°, with the Sun about 13° above the horizon

Solar longitude
102.2°, Northern Summer

For non-map projected images
North azimuth:  96°
Sub-solar azimuth:  48.0°
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   (171MB)

IRB color
map-projected   (83MB)

JP2 EXTRAS
Black and white
map-projected  (85MB)
non-map           (82MB)

IRB color
map projected  (27MB)
non-map           (74MB)

Merged IRB
map projected  (147MB)

Merged RGB
map-projected  (139MB)

RGB color
non map           (68MB)
ANAGLYPHS
Map-projected, reduced-resolution
Full resolution JP2 download
Anaglyph details page

DIGITAL TERRAIN MODEL (DTM)
DTM 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.