Liquid CO₂ May Have Shaped Mars’ Ancient Terrain, Not Just Water, Study Suggests

December 21, 2024
1 min read
Caption:At left: Steel is seen to corrode into siderite (FeCO3) when immersed in subcritical liquid carbon dioxide (LCO2). At right: Samples of albite (a plagioclase feldspar) and a sandstone core are observed to form red rhodochrosite (MnCO3) when exposed to supercritical CO2 in the presence of a water solution with potassium chloride and manganese chloride, with particularly strong reaction near the interface of the two solutions. In both experiments, water saturation is provided by floating LCO2 on the water. Under the lower pressure conditions characteristic of early Mars, the water would float on the LCO2. Credits:Photos courtesy of Todd Schaef/PNNL (left) and Earl Mattson/Mattson Hydrology (right).
Caption:At left: Steel is seen to corrode into siderite (FeCO3) when immersed in subcritical liquid carbon dioxide (LCO2). At right: Samples of albite (a plagioclase feldspar) and a sandstone core are observed to form red rhodochrosite (MnCO3) when exposed to supercritical CO2 in the presence of a water solution with potassium chloride and manganese chloride, with particularly strong reaction near the interface of the two solutions. In both experiments, water saturation is provided by floating LCO2 on the water. Under the lower pressure conditions characteristic of early Mars, the water would float on the LCO2. Credits:Photos courtesy of Todd Schaef/PNNL (left) and Earl Mattson/Mattson Hydrology (right).

A new study published in Nature Geoscience proposes that liquid carbon dioxide, alongside water, may have shaped Mars’ ancient surface features and mineral composition.

The perspective article, led by Michael Hecht, principal investigator of the MOXIE instrument aboard the NASA Mars Rover Perseverance and research scientist at MIT’s Haystack Observatory and former associate director, challenges the long-held assumption that water alone created Mars’ dry river channels and lake beds. “Understanding how sufficient liquid water was able to flow on early Mars to explain the morphology and mineralogy we see today is probably the greatest unsettled question of Mars science,” states Hecht.

The research draws parallels from Earth’s carbon sequestration studies, where mineral alterations occur in liquid CO2 environments, sometimes showing rapid alteration processes. These findings suggest similar processes could have occurred on Mars, potentially explaining the presence of carbonates, phyllosilicates, and sulfates observed on the planet‘s surface.

The study outlines three scenarios for liquid CO2’s presence on Mars: stable surface liquid, basal melting under CO2 ice, and subsurface reservoirs. The feasibility of each scenario depends on the actual inventory of CO2 at the time and surface temperatures.


More Stories


However, the researchers acknowledge key differences between Earth’s carbon sequestration conditions – where liquid CO2 exists above room temperature at high pressures – and Mars’ colder, lower-pressure environment. They emphasize the need for laboratory testing under Mars-like conditions to verify these chemical reactions.

“There is likely no one right answer, and we are merely suggesting another possible piece of the puzzle,” Hecht adds, maintaining scientific caution while presenting this alternative hypothesis.

This research opens new avenues for understanding Mars’ geological history, suggesting a more complex interplay between different liquids in shaping the Red Planet’s surface features and mineral deposits.

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.

Leave a Reply

Your email address will not be published.

Representative Image. Nuna Child Car Seats. Photo Source: Nuna Baby
Previous Story

Nuna Recalls 608,786 Rava Car Seats Over Harness Defect—Is Your Child’s Safety at Risk?

Representative Image. Summer solstice 2010. Photo Source: Vicki (CC BY-NC-ND 2.0)
Next Story

Australia’s Summer Solstice 2024: Which Capital City Enjoys the Longest Daylight Hours?

Latest from Astronomy

Representative Image. Mars exploration sol 383. Photo Source: NASA/JPL-Caltech/ASU/Thomas Thomopoulos

CIA Mars Report: Remote Viewing Ancient Pyramids

The CIA’s “Mars Exploration May 22, 1984” report, declassified in 2017, details remote viewing sessions claiming to observe Mars from one million years ago. Project Stargate, operating from Fort Meade, Maryland (1977-1995),

Don't Miss

Huntington's Mutation

Huntington’s Mutation Remains Harmless Until 150 CAG Repeats

A major breakthrough in Huntington’s disease research has