The European Space Agency has released a new aerial video tracking part of Mars’ southern highlands, offering a slow, up-close look at one of the planet’s most cratered regions. The footage focuses on Flagelug Crater and its surrounding terrain, and is built entirely on real spacecraft data, rather than artistic reconstruction. This video, created using images and elevation measurements from the Mars Express mission, shows how deeply scarred and rugged this part of Mars remains. Subtle lighting, added haze, and controlled camera movement give the landscape a sense of scale without drastically changing it. What emerges is not a spectacle, a measured visual record formed not by imagination but by geology, time, and careful processing.
ESA’s high-resolution imaging turns Mars’ orbital data into a three-dimensional landscape
video by european space agency It uses data from a high-resolution stereo camera aboard Mars Express. The source material comes from a Mars map image mosaic compiled from individual orbital passes. This mosaic is centered around 20 degrees south latitude and 17 degrees east longitude. Camera data was integrated with a digital terrain model to transform flat images into images with depth. The result is a three-dimensional surface that reflects real height changes over hundreds of kilometers.
Camera movement follows a measured fixed path
Each second of video consists of 50 separate frames, each rendered separately. The camera follows a predetermined path across the landscape, and its movement is very smooth and consistent. Vertical relief is exaggerated by a factor of 3 to make the land shape more visible. If this correction is not done, many slopes and depressions will appear flatter than they really are from the spatial view.
Haze is added to reflect atmospheric limits
Mars has a thin atmosphere, but its influence still shapes how the surface looks from a distance. In the video, a soft fog gradually increases over 250 kilometers. This serves two purposes. This reflects how dust and light are scattered on Mars, hiding the edges of the terrain model. The transition to the horizon feels natural, not choppy or artificial.
Graben structure reveals ancient crustal deformation
The elevated road begins along a long ditch-like terrain between two steep cliffs known as Scylla Scopulus and Charybdis Scopulus. This geological formation is a graben, which is formed when the Earth’s crust peels away. It is about 75 kilometers long and about 1 kilometer deep. Scale only becomes apparent when the camera moves steadily along its length.
A large impact crater dominates the surrounding plains
To the left of the first path is the Bakhuisen crater, which is approximately 150 kilometers wide. As the camera moves north, the Hlajerg crater comes into view. The basin spans approximately 240 kilometers and is located in a terrain dense with impacts of all sizes. Parts of the floor rise abruptly, and the steepest parts reach a height of about 1 kilometer.