Mars Express Team Celebrates 20 Years

A new mosaic of Mars marks 20 years since the launch of ESA's Mars Express, and reveals the planet’s color and composition in spectacular detail. The mosaic was created using data from the Mars Express High Resolution Stereo Camera (HRSC).

HRSC normally photographs Mars’s surface from an altitude of about 300 km – the closest the spacecraft gets to Mars in its elliptical orbit – with the resulting images covering areas about 50 km (≈31 miles) across. However, the mosaic presented here uses a slightly different approach. To view the planet more widely, HRSC gathered 90 images at higher altitudes (of 4,000 to 10,000 km, or ≈2,500 to 6,200 miles), thus capturing areas of around 2500 km (≈1,553 miles) wide. These images were then put together to form a full global view.

Such large-scale images are typically obtained to observe weather patterns on Mars – but even in the absence of atmospheric phenomena they offer wonderful views of the planet’s surface.

A Richer Color View

This new view highlights variation across Mars’s surface by enhancing local color and contrast.

Thanks to its nine imaging channels, HRSC can visualize Mars not only in three dimensions but also in color. However, the ever-changing opacity of the martian atmosphere makes it difficult to determine accurate surface colors from orbit. Dust scatters and reflects light, causing colors to shift between images and creating a patchwork-like effect when assembling a mosaic.

Until now, suppressing this effect during image processing has reduced variations in color between different parts of Mars. But to create this mosaic, the HRSC team instead color-referenced each constituent image to a color model derived from high-altitude observations, allowing them to preserve color variations and reveal a far richer color view of Mars than has been seen before.

Each Color a Different Material

While beautiful in its own right, the mosaic also provides fascinating information about Mars’s composition, revealing an unprecedented variety and detail of colors across its surface.

Mars is famous for its reddish color, which is caused by high levels of oxidized iron. However, large parts of the planet appear to be rather dark and blue-toned here. These are gray-black basaltic sands of volcanic origin that form far-reaching, dark layers of sand across Mars. They pile up as they move in the wind, creating imposing sand dunes and dune fields within impact craters.

Material weathered by water, on the other hand, tends to look lighter. The two most common water-weathered minerals on Mars, clay and sulfate minerals, appear particularly bright on such color composites; their presence was established by the OMEGA spectrometer on Mars Express. The presence of these minerals signals that liquid water existed on Mars for a long time, weathering and altering rock over time to form significant clay deposits such as Mawrth Vallis (a former outflow channel not shown in this view but previously observed by HRSC).

Sulfate minerals are visible here within the Valles Marineris canyon system, as seen most clearly in the annotated image above. Here, however, they are covered by a thin veneer of dark sand, but their impressive color variations can be seen on closer look. Unlike clay deposits, sulfate minerals indicate more acidic environmental conditions that would be less friendly to life.

Mars Express Marks Two Decades of Exploring Mars

Mars Express launched and has been orbiting the Red Planet since 2003 – 20 years ago! The orbiter is imaging Mars’ 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, the camera responsible for these images, has revealed much about Mars’ diverse surface features 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 in its two decades of life, creating a far fuller and more accurate understanding of our planetary neighbor than ever before. It was initially planned to last for one Martian year, or around 687 Earth days, but has continued to meet and exceed its objectives. As the mission has been extended until at least the end of 2026, we can anticipate many more beautiful and insightful snapshots of Mars in the years to come.

The mission’s High Resolution Stereo Camera (HRSC) was developed and is operated by the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR).

The development of the color model method and processing of the mosaic was performed by Greg Michael of the HRSC team at Freie Universität Berlin. The acquisition and planning of the high-altitude images were the responsibility of the camera operations team at the German Aerospace Center (DLR) at Berlin-Adlershof. On publication of the upcoming scientific paper on the mosaic, the georeferenced dataset will be made available through the ESA guest storage facility.

(Source: ESA news release. Images provided)