Landslides in Valles Marineris
NASA/JPL-Caltech/UArizona
Landslides in Valles Marineris
ESP_089701_1660  Science Theme: Landscape Evolution
This image shows part of several long, lobe-shaped deposits of sediment in the Coprates Chasma region of Valles Marineris. These deposits formed when rocks in very steep terrain became unstable and collapsed, forming a landslide.

The landslide flowed downhill and created these lobe-shaped deposits. The deposits have ridges along their perimeter called levees or flank ridges. Flank ridges are observed within landslide deposits on the Earth and are generally believed to form through progressive downhill movement of the landslide over a long period of time. In other words, the middle part of the landslide continues to flow downhill after the sides of the landslide have stopped moving.

A closer look at the sides of the flank ridges reveals that they are composed of many different layers of sediment, from fine-grained, sandy layers to coarse, bouldery layers. This stratification suggests that the landslide was formed by multiple collapses of rock, rather than though one catastrophic collapse. Thus, the flank ridges and stratification within them indicate that this area experienced a period of numerous overlapping slope collapses and downhill movement of landslides.

Written by: Chris Okubo  (19 March 2026)

This is a stereo pair with ESP_090400_1660.
 
Acquisition date
14 September 2025

Local Mars time
15:41

Latitude (centered)
-13.740°

Longitude (East)
303.373°

Spacecraft altitude
261.9 km (162.8 miles)

Original image scale range
52.4 cm/pixel (with 2 x 2 binning) so objects ~157 cm across are resolved

Map projected scale
50 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
0.5°

Phase angle
62.8°

Solar incidence angle
62°, with the Sun about 28° above the horizon

Solar longitude
140.0°, Northern Summer

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  33.2°
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Black & white is 5 km across; enhanced color about 1 km
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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:
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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.