The Mystery of Aganippe Fossa

Aganippe Fossa cuts across the lower flank of one of Mars’s largest volcanoes, Arsia Mons. Mars Express regularly observes Arsia Mons and its nearby companions in the region of Tharsis, where several of Mars’s behemoth volcanoes are found. This includes Olympus Mons, the tallest volcano in the Solar System (visible in the context map associated with this new image, as is Arsia Mons).

Arsia Mons itself measures 435 km in diameter and rises more than 9 km above the surrounding plains. For context, the highest dormant volcano on Earth, Ojos del Salado on the Argentina-Chile border, tops out at under 7 km.

This image shows Aganippe Fossa, a snaking groove found at the foot of Mars’s giant Arsia Mons volcano, in a wider context. The area outlined by the larger white box indicates the area imaged by the High Resolution Stereo Camera aboard ESA’s Mars Express orbiter on December 13, 2023, during orbit 25189, while the smaller white box shows the part of the surface featured in these new images. Credit: NASA/MGS/MOLA Science Team

Seeping Lava

We’re still unsure of how and when Aganippe Fossa came to be, but it seems likely that it was formed as magma rising underneath the colossal mass of the Tharsis volcanoes caused Mars’s crust to stretch and crack.

In this view, Mars Express’s High Resolution Stereo Camera (HRSC) captures two different kinds of terrain: so-called hummocky terrain, which comprises many irregularly shaped mounds and valleys all clustered together, and lobate terrain, which is formed of gently sloping cliffs and rocky debris.

This color-coded topographic image shows Aganippe Fossa, a snaking groove found at the foot of Mars’s giant Arsia Mons volcano. It was created from data collected by ESA’s Mars Express on December 13, 2023, and is based on a digital terrain model of the region, from which the topography of the landscape can be derived. Lower altitude parts of the surface are shown in blues and purples, while higher altitude regions show up in whites and reds, as indicated on the scale to the top right. Credit: ESA/DLR/FU Berlin

These terrains are characteristic of Arsia Mons’s ring-shaped ‘aureole’, a 100,000-square-kilometer disc around the base of the volcano, possibly associated with ancient glaciers. Intriguingly, this aureole has only built up on the northwestern flank of the volcano, likely due to prevailing winds from the opposite direction controlling where ice settled over time.

Windblown dust and sand have also shaped this patch of Mars, creating interesting zebra-like patterns to the right of the frame as darker material is deposited on lighter ground (or vice versa!). The surface here also shows evidence of lava flows, dating from when the volcano was active.

This stereoscopic image shows Aganippe Fossa, a snaking groove found at the foot of Mars’s giant Arsia Mons volcano. The anaglyph offers a three-dimensional view when viewed using red-green or red-blue glasses. Credit: ESA/DLR/FU Berlin

Exploring Mars

Mars Express has been orbiting the Red Planet since 2003. It is imaging Mars’s surface, mapping its minerals, identifying the composition and circulation of its tenuous atmosphere, probing beneath its crust, and exploring how various phenomena interact in the Martian environment.

The spacecraft’s HRSC, responsible for these images, has revealed much about Mars’s diverse surface in the past 20 years. Its images show everything from wind-sculpted ridges and grooves to sinkholes on the flanks of colossal volcanoes to impact craters, tectonic faults, river channels, and ancient lava pools. The mission has been immensely productive over its lifetime, creating a far fuller and more accurate understanding of our planetary neighbor than ever before.

The High Resolution Stereo Camera (HRSC) on the Mars Express spacecraft is a sophisticated imaging system designed to study Mars in high detail. Launched by the