Perspective view of Hellas Basin taken with the High Resolution Stereo Camera on ESA’s Mars Express in January 2014, and released in July 2014. Credit: ESA/DLR/FU Berlin
Beyond the pretty picture is a tale of how snow behaved on the Martian surface, according to the European Space Agency. The vast basin is about half the size of Brazil.
The wrinkled view of that crater in front is a product of snowing and freezing that took place when the Martian surface was wetter, ESA said.
A map of the Hellas basin in the southern hemisphere of Mars, as well as the rocky Hellespontus Montes. Image taken by the High Resolution Stereo Camera on ESA’s Mars Express. Credit: NASA MGS MOLA Science Team/Freie Universitaet Berlin
Additionally, the high hill chain in the back (called Hellespontus Montes) is a remnant of how Hellas basin was formed, the agency said.
“This feature is a product of the final stages of the formation of the vast Hellas impact basin itself, most likely as the basin walls – which were first pushed outwards by the extraordinary forces at work during the formation of the basin – later collapsed and sank inwards to create the observed stair-stepped shape.”
The image was taken by ESA’s Mars Express spacecraft, which is just one of several robotic emissaries circling the Red Planet.
Source: European Space Agency
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