Student Image of the Week: Debris Apron South of Euripus Mons
Student Image of the Week: Debris Apron South of Euripus Mons
PSP_003639_1345  Science Theme: Fluvial Processes


This image was suggested by Andras Sik's SUPERNOVA astronomy and space research class at the Alternative Secondary School of Economics in Budapest, Hungary.

They write: "In the fretted terrains and in the eastern region of the Hellas Basin rim, many plateaus can be found surrounded by a skirt-like debris cover. These debris aprons can extend to 15-25 kilometers long; they have a convex shape, steep front slopes and differ from gravitational talus or fluvial fans. (There may be) ice cores and/or ice cement in the apron material, therefore the closest terrestrial analogs are periglacial rock (terrains). This HiRISE image shows a small part of Euripus Mons' debris apron [at a] very high resolution so its detailed surface morphology can be investigated and compared to field observations of terrestrial rock glaciers."

Euripus Mons is located to the east of Hellas impact basin in the Southern mid-latitudes of Mars.

The overall wavy, curved surface pattern of this debris apron suggests that material flowed out from the isolated flat-top ridge. This mass movement of debris probably involved ice flow (possibly forming rock glaciers) and potentially liquid water.

A closer view of the upper portion of the image (see subimage; 718 x 588; 1MB), reveals that rough sharp scalloped ridges are particularly prominent. This scalloping may have resulted from sublimation of ice below the surface.

At full resolution, polygonal features can be observed (see subimage; 722 x 596; 1.2MB), which are characteristic of periglacial terrains. These polygons form by the contraction and expansion of the ground due to freezing and thawing of ice just below the surface during seasonal changes.

All of these features provides evidence that ice was or is present just below the surface at this location. This apron is not pockmarked with craters, suggesting it is relatively young in age.

Written by: Alix Davatzes  (26 September 2007)
Acquisition date
06 May 2007

Local Mars time

Latitude (centered)

Longitude (East)

Spacecraft altitude
251.5 km (156.3 miles)

Original image scale range
25.2 cm/pixel (with 1 x 1 binning) so objects ~75 cm across are resolved

Map projected scale
25 cm/pixel and North is up

Map projection

Emission angle

Phase angle

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

Solar longitude
233.0°, Northern Autumn

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  17.2°
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

Black and white
map-projected   (923MB)

IRB color
map-projected   (396MB)

Black and white
map-projected  (343MB)
non-map           (627MB)

IRB color
map projected  (129MB)
non-map           (467MB)

Merged IRB
map projected  (246MB)

Merged RGB
map-projected  (238MB)

RGB color
non map           (457MB)
B&W label
Color label
Merged IRB label
Merged RGB label
EDR products

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

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/University of Arizona

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.