The article discusses the fascinating Martian phenomenon of araneidoform terrain, which appears when frozen carbon dioxide melts, revealing spider-like landforms. These formations, sometimes over a kilometer wide, lack complete understanding regarding their formation processes. JPL is actively researching to simulate Martian conditions for further study. Additionally, strong spring winds impact the north polar cap's spiral pattern and create deep canyons over time. Chasma Boreale, a major canyon in this region, is highlighted as exceptionally large. The seasonal change also causes sand dunes to move as thawing occurs, making spring on Mars a dynamic and noisy event.
When the frozen carbon dioxide has all melted in the summer, distinctive marks are revealed on the Martian landscape. These are known as \
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