Science & Exploration <\/p>\n
03\/07\/2024 7480 views 39 likes <\/p>\n
A fascinating feature takes centre stage in this new image from ESAs Mars Express: a dark, uneven scar slicing through marbled ground at the foot of a giant volcano. <\/p>\n
This scar, known as Aganippe Fossa, is a patchy, roughly 600-km-long feature known as a graben: a ditch-like groove with steep walls on either side. <\/p>\n
Aganippe Fossa cuts across the lower flank of one of Marss largest volcanoes, Arsia Mons. Mars Express regularly observesArsia Mons and its nearby companions in the region of Tharsis, where several of Marss behemoth volcanoes are found. This includesOlympus Mons, the tallest volcano in the Solar System (visible in the context map associated with this new image, as is Arsia Mons). <\/p>\n
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. <\/p>\n
Werestill 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 Marss crust to stretch and crack. <\/p>\n
In this view, Mars ExpresssHigh 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. <\/p>\n
These terrains are characteristic of Arsia Monss ring-shaped aureole, a 100 000-square-kilometre 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. <\/p>\n
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. <\/p>\n
Mars Express has been orbiting the Red Planet since 2003. It is imaging Marss 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. <\/p>\n
The spacecrafts HRSC, responsible for these images, has revealed much about Marss diverse surface in the past 20 years. Its images show everything fromwind-sculpted ridges and groovestosinkholes on the flanks of colossal volcanoestoimpact 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 neighbour than ever before. <\/p>\n
The Mars Express High Resolution Stereo Camera(HRSC) was developed and is operated by the German Aerospace Center (Deutsches Zentrum fr Luft- und Raumfahrt; DLR). <\/p>\n
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ESA - A snaking scar on Mars - European Space Agency<\/a><\/p>\n","protected":false},"excerpt":{"rendered":" Science & Exploration 03\/07\/2024 7480 views 39 likes A fascinating feature takes centre stage in this new image from ESAs Mars Express: a dark, uneven scar slicing through marbled ground at the foot of a giant volcano. This scar, known as Aganippe Fossa, is a patchy, roughly 600-km-long feature known as a graben: a ditch-like groove with steep walls on either side Continue reading