Possible Sulfates in the Northeast Syrtis Major Region
Possible Sulfates in the Northeast Syrtis Major Region
ESP_041893_1975  Science Theme: Composition and Photometry
A variety of diverse morphological features are present in this image located in the southeastern area of the Nili Fossae region and just northeast of Syrtis Major.

This particular region has been studied intensely due to the presence of volcanics from Syrtis Major and impact ejecta from the Isidis Basin. The region is rich in unaltered mafic deposits, in contact with diverse altered deposits rich in clays, carbonates, and sulfates. These deposits make the Nili Fossae region one of the most colorful regions on Mars, which is most distinctive in infrared color composites (IRB). HiRISE IRB color aids in chemical and mineral-type mapping, especially when correlated with other MRO instruments such as CRISM.

In this infrared color close-up image, we can see a mesa, along with aeolian (wind-blown) dunes and yellow-colored deposits. A mesa is a flat, steep-sloped hill, which was likely eroded by a combination of wind-driven and landslide processes. These are often formed due to differing rock compositions, which vary in their resistance to erosion, e.g., a weaker and softer rock, such as sediments, lies beneath a stronger and more resistant rock. The flat top surfaces of mesas, termed the “cap” rock, are relatively erosion-resistant rock types, such as igneous lavas or intrusive sills. The looser, yellowish deposits that underlie the cap rock contrast nicely with the purplish-blue cap rock.

Another closeup shows an area just north of the mesa that is particularly distinct in this IRB color. Based on a corresponding CRISM image providing spectral data, there is some exposed bedrock in the area that likely contains salt-bearing rocks.

Written by: Kayle Hansen, Livio Tornabene, and Elizabeth Silber (narration: Tre Gibbs)  (16 September 2015)

This is a stereo pair with ESP_041115_1975.
Acquisition date
04 July 2015

Local Mars time

Latitude (centered)

Longitude (East)

Spacecraft altitude
278.5 km (173.1 miles)

Original image scale range
28.1 cm/pixel (with 1 x 1 binning) so objects ~84 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection

Emission angle

Phase angle

Solar incidence angle
39°, with the Sun about 51° above the horizon

Solar longitude
8.0°, Northern Spring

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North azimuth:  97°
Sub-solar azimuth:  348.5°
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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.