Cratered Dunes and Yardangs in the Medusae Fossae Formation
NASA/JPL/UArizona
Cratered Dunes and Yardangs in the Medusae Fossae Formation
PSP_010453_1675  Science Theme: Aeolian Processes
This image shows cratered dunes and yardangs in the Medusae Fossae Formation, located in the Martian mid-latitudes and is characterized by wind-sculpted landforms. The composition of the Medusae Fossae is unclear but may include indurated (hardened) volcanic ash deposits or remnant dust-ice mixtures that formed during a different Martian climate.

The bottom half of the image reveals dunes that have apparently become cemented. The dune field is heavily cratered and both the dunes and craters exhibit much erosion and degradation indicating that they are relatively old in age. Most craters do not have visible ejecta deposits (most likely due to erosion and/or mantling (being covered)) and have superposed smaller dunes and ripples that also indicate that the craters and thus the dunes on which they lie are old in age.

Sharp ridges formed from wind abrasion, or yardangs, are visible in the upper half of the image. Yardangs typically form in dry, desert environments with strong prevailing winds that are unidirectional and carry an abrasive sediment load. Abrasive winds erode the surface into parallel elongate landforms, or ridges, that are often three or more times longer than they are wide.

When viewed from above, these landforms often resemble the hull of a boat. Yardangs typically form in easily-eroded material, most likely sedimentary rock or volcanic ash deposits that contain some amount of sand. Yardangs are found on both Earth and Mars.



Written by: Maria Banks  (14 January 2009)

This is a stereo pair with PSP_009609_1675.
 
Acquisition date
19 October 2008

Local Mars time
15:48

Latitude (centered)
-12.597°

Longitude (East)
178.082°

Spacecraft altitude
263.5 km (163.8 miles)

Original image scale range
28.0 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
Equirectangular

Emission angle
20.6°

Phase angle
45.9°

Solar incidence angle
63°, with the Sun about 27° above the horizon

Solar longitude
144.0°, Northern Summer

For non-map projected images
North azimuth:  98°
Sub-solar azimuth:  31.4°
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   (916MB)

IRB color
map-projected   (431MB)

JP2 EXTRAS
Black and white
map-projected  (461MB)
non-map           (442MB)

IRB color
map projected  (174MB)
non-map           (370MB)

Merged IRB
map projected  (217MB)

Merged RGB
map-projected  (222MB)

RGB color
non map           (350MB)
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/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.