An Inverted Channel in Flammarion Crater
NASA/JPL-Caltech/UArizona
An Inverted Channel in Flammarion Crater
ESP_089631_2065  Science Theme: Fluvial Processes
Topographic inversion is a process where geologic features that were once low-lying, like impact craters or riverbeds, become elevated over time, like mesas or ridges. In this process, a crater or channel is filled with lava or sediment that becomes lithified.

If this infill is more resistant to erosion than the surrounding landscape, the less-resistant material can be eroded away by wind or water. The former crater or valley fill, being more resistant, remains elevated as the landscape around it lowers. The original low-lying feature becomes a mesa or ridge.

In this image, an ancient river network and nearby impact craters have undergone topographic inversion. Impact craters contain round mesas within them, and the stream channel is defined by a network of ridges. Studies of ancient stream channels and impact craters (and their inverted counterparts, like mesas and ridges) help scientists understand when and where liquid water was present on the surface of Mars and the potential for the past existence of habitable environments on the planet.

Written by: Chris Okubo  (18 December 2025)
 
Acquisition date
09 September 2025

Local Mars time
15:30

Latitude (centered)
26.029°

Longitude (East)
48.929°

Spacecraft altitude
283.1 km (175.9 miles)

Original image scale range
from 28.6 cm/pixel (with 1 x 1 binning) to 57.1 cm/pixel (with 2 x 2 binning)

Map projected scale
25 cm/pixel and North is up

Map projection
Equirectangular

Emission angle
6.1°

Phase angle
55.7°

Solar incidence angle
50°, with the Sun about 40° above the horizon

Solar longitude
137.3°, Northern Summer

For non-map projected images
North azimuth:  97°
Sub-solar azimuth:  5.9°
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Black & white is 5 km across; enhanced color about 1 km
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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.