Mars Express Spots ‘Spiders’ at Outskirts of Martian ‘Inca City’

ESA’s Mars Express spacecraft have spotted the telltale traces of ‘spiders’ scattered across the southern polar region of Mars.

This image of the Martian Inca City was captured by the High Resolution Stereo Camera onboard ESA’s Mars Express orbiter on February 27, 2024. Image credit: ESA / DLR / FU Berlin.
This image of the Martian Inca City was captured by the High Resolution Stereo Camera onboard ESA’s Mars Express orbiter on February 27, 2024. Image credit: ESA / DLR / FU Berlin.


According to members of the Mars Express team, the so-called Martian 'spiders' aren't actually arachnids but rather formations resulting from the interplay of sunlight and carbon dioxide layers accumulated during winter on Mars.

Sunlight triggers the transformation of carbon dioxide ice beneath these layers into gas, which accumulates and eventually ruptures the overlying ice sheets. As the gas rushes upwards during the Martian spring, it carries dark material to the surface, fracturing ice layers up to a meter thick.

The gas, laden with dark dust, erupts through cracks in the ice, resembling tall fountains or geysers before settling back down, leaving behind dark spots ranging from 45 meters to 1 kilometer across. These spots, displaying characteristic 'spider-shaped' patterns beneath the ice, serve as indicators of potential subterranean spider-like formations.

These dark spots are visible throughout Mars Express images, particularly concentrated within the dark region adjacent to a Mars area known as Inca City, named for its striking resemblance to linear ridges reminiscent of Inca ruins.

Formally termed Angustus Labyrinthus, Inca City was first identified by NASA's Mariner 9 probe in 1972. Its formation remains a subject of speculation, with theories ranging from petrified sand dunes to seepage of magma or sand through fractured Martian rock, or even the presence of glacial-related structures known as 'eskers.'

The circular 'walls' of Inca City, spanning 86 kilometers (53.5 miles) in diameter, suggest its location within a crater likely formed by the impact of a celestial body on Mars's surface. This impact event likely triggered fault lines to propagate across the surrounding plain, subsequently filled with lava that has eroded over time.


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