The Arabia Terra is a vast hilly plain on Mars. Recently, the Mars Express spacecraft, which operates in orbit around the red planet, took a picture of this area. It shows how densely cratered it is.

In this new image ESA's Mars Express visits the highlands of Mars, exploring the innumerable craters peppering this ancient part of the red planet. Part of the particularly prominent Trouvelot Crater can be seen to the bottom-right. This image comprises data gathered by Mars Express's High Resolution Stereo Camera (HRSC) on 12 October 2024 (orbit 26233). It was created using data from the nadir channel, the field of view aligned perpendicular to the surface of Mars, and the colour channels of the HRSC. North is to the right. The ground resolution of the original image is approximately 18 m/pixel and the image is centred at about 15°N/255°E.
Credit: ESA/DLR/FU Berlin

Arabia Terra

Craters, craters, and yet more craters: this snapshot from ESA's Mars Express is packed full of them, each as fascinating as the last.

This view of the Red Planet – taken by Mars Express’s High Resolution Stereo Camera – shows a slice of Arabia Terra, a large plain in Mars’ ancient highlands. This part of Mars is known for being heavily pockmarked with craters, each formed as a space rock hurtled inwards to collide with the planet.

Ancient ground

The glut of craters seen here is no surprise. Arabia Terra is truly ancient. As a result, it’s had lots of time to add to its impressive crater collection – between 3.7 and 4.1 billion years, in fact.

The main image above shows just a few of these. Some are filled with strikingly dark material, others are home to lighter sands and rippling dunes, while yet others show signs of collapsing walls and worn-away rims.

The most prominent crater seen in the image, extending out of frame to the bottom-right, is Trouvelot Crater. This crater is around 130 km across, and shows signs of being very old: it has a rim that has long since started to crumble away, uneven interior “terraced” walls that have collapsed under their own weight over time, and several smaller overlapping and overlaid craters that have formed since the creation of Trouvelot Crater itself.

These, and other, features are all clearly labeled if you click on the image. Be sure to take a look to easily find features of interest and explore this intriguing landscape in detail.

Counting craters

This image shows Mars’s Trouvelot Crater and the surrounding plains of Arabia Terra in wider context. A large dotted square highlights the area of Mars featured in new images from the ESA Mars Express High Resolution Stereo Camera (HRSC), released in March 2026. The two smaller boxes within mark the precise patch of surface shown in the images, captured by Mars Express on 12 October 2024 (orbit 26233). The elevation of the surface, shown by the bright colours marking the surface of Mars, is indicated by the scale to the bottom-right.

Credit: NASA/USGS.; ESA/DLR/FU Berlin

Variety of relief forms

To the left of Trouvelot Crater sits another basin that appears to be even older and more eroded, with a wall that’s almost completely worn away. Trouvelot cuts through this crater, further indicating that this more deteriorated crater companion was there first.

The floor of this more ancient crater is nearly entirely covered in dark rock, which is rich in minerals such as magnesium, iron, pyroxine, and olivine (known as “mafic” rock, and often created by volcanism). These volcanic rocks may have been thrown up by crater-forming impacts, and later moved around as winds swept across the terrain and gravity pulled material down crater walls.

The other large craters seen here – and across Arabia Terra, beyond the edges of this frame – have similar dark deposits on their floors or walls, indicating that these processes are widespread across this part of Mars.

In Trouvelot Crater, the dark material has been shaped by wind into rippling dunes known as “barchan” dunes. These are characteristically sickle- or crescent-shaped and created when winds predominantly blow in one direction. Mars Express has spotted barchan dunes on Mars before, such as in the planet’s north polar region and near the large volcanic province of Tharsis.

Dark and volcanic

To the left of Trouvelot Crater sits another basin that appears to be even older and more eroded, with a wall that's almost completely worn away. Trouvelot cuts through this crater, further indicating that this more deteriorated crater companion was there first.

The floor of this more ancient crater is nearly entirely covered in dark rock, which is rich in minerals such as magnesium, iron, pyroxine and olivine (known as "mafic" rock, and often created by volcanism). These volcanic rocks may have been thrown up by crater-forming impacts, and later moved around as winds swept across the terrain and gravity pulled material down crater walls.

The other large craters seen here—and across Arabia Terra, beyond the edges of this frame—have similar dark deposits on their floors or walls, indicating that these processes are widespread across this part of Mars.

In Trouvelot Crater, the dark material has been shaped by wind into rippling dunes known as "barchan" dunes. These are characteristically sickle- or crescent-shaped, and created when winds predominantly blow in one direction. Mars Express has spotted barchan dunes on Mars before, such as in the planet's north polar region and near the large volcanic province of Tharsis.

Counting craters

Close-up image showing the dark rock covering the floor of Trouvelot Crater and its ancient companion, with even darker barchan dunes visible at the center-left of the image.

Credit: ESA/DLR/FU Berlin

From dark to light

Sitting amid the dark material in Trouvelot Crater is a sign that other processes have been at play here: a light-toned mound around 20 km long and covered in ridges and grooves.

Such mounds have been spotted elsewhere on Mars – in the nearby Becquerel crater, for example, as seen by Mars Express in 2013 and 2014. They typically show signs of minerals that have come into contact with, or formed in the presence of, water, and are usually far lighter than their surroundings.

Counting craters

Close-up image showing the light-toned mound at the upper left, standing out among the dark rock.

Credit: ESA/DLR/FU Berlin

Water is thought to play a key role in how the mounds themselves form, too, but this is still a topic of debate. The mounds may have formed in a lake or sea in Mars’ past. Alternatively, layers of light-toned rock may have gradually built up as water in and below the Martian surface (“groundwater”) swelled upwards to mix with wind-swept sediments on the crater floor.

This image was captured by one of eight instruments aboard Mars Express: the High Resolution Stereo Camera. The Mars orbiter has been exploring Mars’ many landscapes since it launched in 2003. It has mapped the planet’s surface at unprecedented resolution, in color, and in three dimensions for over two decades, returning insights that have drastically changed our understanding of our planetary neighbor.

Counting craters

Close-up image showing another crater that is visible in the lower left of the main image (to the left of Trouvelot Crater and the ancient companion that it intersects).

Credit: ESA/DLR/FU Berlin

Decades of Mars exploration

This image was captured by one of eight instruments aboard Mars Express: the High Resolution Stereo Camera. The Mars orbiter has been exploring Mars' many landscapes since it launched in 2003. It has mapped the planet's surface at unprecedented resolution, in color, and in three dimensions for over two decades, returning insights that have drastically changed our understanding of our planetary neighbor.