Mars’ South Pole: 8-Meter CO₂ Ice, -193°F Patterns, Geysers, 66-Foot Avalanches, and Dune Shifts

December 30, 2024
2 mins read
Martian spring involves lots of cracking ice, which led to this 66-foot-wide (20-meter-wide) chunk of carbon dioxide frost captured in freefall by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter in 2015 NASA/JPL-Caltech/University of Arizona
Martian spring involves lots of cracking ice, which led to this 66-foot-wide (20-meter-wide) chunk of carbon dioxide frost captured in freefall by the HiRISE camera aboard NASA’s Mars Reconnaissance Orbiter in 2015 NASA/JPL-Caltech/University of Arizona

The European Space Agency’s (ESA) Mars Express orbiter has captured images of carbon dioxide ice formations at Mars’ south pole, revealing complex seasonal patterns at -193°F (-125°C). These observations, made in June 2022, show an 8-meter-thick layer of carbon dioxide ice persisting year-round at the planet’s south pole.

“Springtime on Earth has lots of trickling as water ice gradually melts. But on Mars, everything happens with a bang,” says Serina Diniega, planetary surface researcher at NASA’s Jet Propulsion Laboratory.

As light shines through carbon dioxide ice on Mars, it heats up its bottom layers, which, rather than melting into a liquid, turn into gas. The buildup gas eventually results in explosive geysers that toss dark fans of debris on to the surface.
NASA/JPL-Caltech/University of Arizona

Technical Analysis of Ice Formations

The Mars Express orbiter’s High Resolution Stereo Camera (HRSC) documented the Australe Scopuli region’s ice dynamics. NASA’s Mars Reconnaissance Orbiter (MRO), using its High-Resolution Imaging Science Experiment (HiRISE) camera, complemented these observations in September 2022.

The sublimation process – ice converting directly from solid to gas – creates distinct surface patterns. Gas pockets form beneath the ice as sunlight penetrates the translucent upper layers. When pressure builds, the gas bursts through, carrying dark dust upward. Wind patterns then distribute this dust across the surface.

Sometimes, after carbon dioxide geysers have erupted from ice-covered areas on Mars, they leave scour marks on the surface. When the ice is all gone by summer, these long scour marks look like the legs of giant spiders.
NASA/JPL-Caltech/University of Arizona

Seasonal Changes and Their Implications

Mars completed its latest orbit around the Sun on November 12, 2024, marking 687 Earth days. The planet’s thin atmosphere prevents liquid formation on its surface, resulting in ice sublimating directly into gas. This process produces specific geological features:

  • Gas geysers erupting through carbon dioxide ice
  • 66-foot-wide frost avalanches
  • Texas-sized ice cap formations with California-length troughs
  • Dune migration patterns affected by carbon dioxide frost
As temperatures rise, powerful winds kick up that carve deep troughs into the ice cap of Mars’ north pole. Some of these troughs are as long as California, and give the Martian north pole its trademark swirls. This image was captured by NASA’s now-inactive Mars Global Surveyor.
NASA/JPL-Caltech/MSSS

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Scientific Data Collection

The Mars Express mission, launched in 2003, has mapped the chemical composition of Mars’ atmosphere and studied its moons, Phobos and Deimos. The MRO, launched in 2005, continues monitoring seasonal changes.

Isaac Smith from York University notes the scale of polar formations: “These things are enormous. You can find similar troughs in Antarctica but nothing at this scale.”

Surrounded by frost, these Martian dunes in Mars’ northern hemisphere were captured from above by NASA’s Mars Reconnaissance Orbiter using its HiRISE camera on Sept. 8, 2022.
NASA/JPL-Caltech/University of Arizona

Current Research Focus

Scientists are studying the relationship between frost patterns and dune preservation. Recent research published in September details how carbon dioxide frost immobilizes polar sand dunes during winter months.

The University of Arizona operates the HiRISE camera, built by Ball Aerospace & Technologies Corp. JPL manages the Mars Reconnaissance Orbiter Project for NASA’s Science Mission Directorate.

Rahul Somvanshi

Rahul, possessing a profound background in the creative industry, illuminates the unspoken, often confronting revelations and unpleasant subjects, navigating their complexities with a discerning eye. He perpetually questions, explores, and unveils the multifaceted impacts of change and transformation in our global landscape. As an experienced filmmaker and writer, he intricately delves into the realms of sustainability, design, flora and fauna, health, science and technology, mobility, and space, ceaselessly investigating the practical applications and transformative potentials of burgeoning developments.

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