ESA - Mars Express Mission patch.
14 December 2017
Mars Express
Which way is up in space? Planets are usually shown with the north pole at the top and the south pole at the bottom. In this remarkable image taken by ESA’s Mars Express, the Red Planet is seen with north at the bottom, and the equator at the top.
The image was taken on 19 June for calibrating the high-resolution stereo camera, while Mars Express was flying from north to south. The camera’s nine channels – one downward-pointing, four colour and four stereo – panned over the surface to record a large area with the same illumination conditions. At the same time, the camera was shifted to the horizon, instead of just pointing to the surface as in routine imaging.
North to south
The result is this rare wide-angle view of the planet, with the illuminated horizon near the equator at the top of the image, and the shadowed north pole at the bottom.
The northern polar cap was composed of water ice and dust at the time of imaging, at the beginning of spring. The carbon dioxide ice present in winter had already evaporated from the solid form to a gas. Similarly, water-ice also evaporates, injecting a large amount of water into the atmosphere that is circulated to the south by atmospheric motions. When the seasons change back, carbon dioxide frost and water-ice build up again.
Panning south, the view soaks up sights of some of the planet’s largest volcanoes in the Tharsis region. Tharsis covers an area larger than Europe, and rises some 5 km above the planet’s average elevation, with volcanoes towering 10–22 km in height.
The largest volcanic giant, Olympus Mons, is out of view in this scene, leaving Alba Mons to take centre stage in the top half of the image, with a diameter of more than 1000 km.
Mars global context
Alba Mons lies at the edge of the Tharsis uplift, and a number of parallel linear features can be seen around it, their formation tied to the tectonic stresses of the Tharsis bulge. As the region swelled with magma in the planet’s first billion years of history the crust was stretched apart. Later, when subsurface magma chambers were discharged, subsidence of the crust also generated fractures.
Further towards the horizon, the 15 km-high Ascraeus Mons comes into view, on this occasion covered by hazy clouds.
Thin layers of clouds can also be seen several tens of kilometres above the horizon.
Mars topography
Other volcanoes can also be seen to the left of Ascraeus Mons, including Uranius Mons, Ceraunius Tholus and Tharsis Tholus.
Although average in size by martian standards, with diameters between about 60 km and 150 km, and towering between about 5 km and 8 km above the surrounding terrain, they rival many of Earth’s volcanoes: Mauna Kea is the tallest volcano on Earth at 10 km when measured from its oceanic base to summit, with only 4200 m above sea level.
Related links:
Mars Express: http://www.esa.int/Our_Activities/Space_Science/Mars_Express
Mars Express overview: http://www.esa.int/Our_Activities/Space_Science/Mars_Express_overview
Mars Express in-depth: http://sci.esa.int/marsexpress
ESA Planetary Science archive (PSA): http://www.rssd.esa.int/PSA
High Resolution Stereo Camera: http://berlinadmin.dlr.de/Missions/express/indexeng.shtml
HRSC data viewer: http://hrscview.fu-berlin.de/
Behind the lens... http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Behind_the_lens
Frequently asked questions: http://www.esa.int/Our_Activities/Space_Science/Mars_Express/Frequently_asked_questions
Images, Text, Credits: ESA/NASA/MGS/MOLA Science Team, FU Berlin.
Best regards, Orbiter.ch
