In a new study, planetary scientists found strong similarities between soils found in Gale Crater on Mars and those of Canada’s Newfoundland, a cold subarctic climate.
X-ray amorphous material comprises 15-73 wt.% of sedimentary rocks and eolian sediments in Gale Crater. This material is variably siliceous and iron rich but aluminum poor. The presence of volatiles is consistent with the existence of incipient weathering products. To better understand the implications of this material for past aqueous conditions on Mars, Feldman et al. investigated X-ray amorphous material formation and longevity within terrestrial iron rich soils with varying ages and environmental conditions using bulk and selective dissolution methods, X-ray diffraction, and transmission electron microscopy. Image credit: M. Kornmesser / ESO.
Scientists often use soil to depict environmental history, as the minerals present can tell the story of landscape evolution through time.
Understanding more about how these materials formed could help answer long-standing questions about historical conditions on the red planet.
The soils and rocks of Gale Crater provide a record of Mars’ climate between 3 and 4 billion years ago, during a time of relatively abundant water on the planet — and the same time period that saw life first appear on Earth.
“Gale Crater is a paleo lakebed — there was obviously water present. But what were the environmental conditions when the water was there?” said Dr. Anthony Feldman, a soil scientist and geomorphologist at Desert Research Institute.
“We’re never going to find a direct analog to the Martian surface, because conditions are so different between Mars and Earth. But we can look at trends under terrestrial conditions and use those to try to extrapolate to Martian questions.”
NASA’s Curiosity Rover has been investigating Gale Crater since 2011, and has found a plethora of soil materials known as X-ray amorphous materials.
These components of the soil lack the typical repeating atomic structure that defines minerals, and therefore can’t be easily characterized using traditional techniques like X-ray diffraction.
When X-rays are shot at crystalline materials like a diamond, for example, the X-rays scatter at characteristic angles based on the mineral’s internal structure.
However, X-ray amorphous material does not produce these characteristic fingerprints.
This X-ray diffraction method was used by the Curiosity Rover to demonstrate that X-ray amorphous material comprised between 15 and 73% of the soil and rock samples tested in Gale Crater.
“You can think of X-Ray amorphous materials like Jello. It’s this soup of different elements and chemicals that just slide past each other,” Dr. Feldman said.
Curiosity also conducted chemical analyses on the soil and rock samples, finding that the amorphous material was rich in iron and silica but deficient in aluminum.
Beyond the limited chemical information, scientists don’t yet understand what the amorphous material is, or what its presence implies about Mars’ historical environment.
Uncovering more information about how these enigmatic materials form and persist on Earth could help answer persistent questions about the red planet.
Dr. Feldman and his colleagues visited three locations in search of similar X-ray amorphous material: the Tablelands of Gros Morne National Park in Newfoundland, Northern California’s Klamath Mountains, and western Nevada.
These three sites had serpentine soils that the researchers expected to be chemically similar to the X-ray amorphous material at Gale Crater: rich in iron and silicon but lacking in aluminum.
The three locations also provided a range of rainfall, snowfall, and temperature that could help provide insight into the type of environmental conditions that produce amorphous material and encourage its preservation.
At each site, the research team examined the soils using X-ray diffraction analysis and transmission electron microscopy, which allowed them to see the soil materials at a more detailed level.
The subarctic conditions of Newfoundland produced materials chemically similar to those found in Gale Crater that also lacked in crystalline structure. The soils produced in warmer climates like California and Nevada did not.
“This shows that you need the water there in order to form these materials,” Dr. Feldman said.
“But it needs to be cold, near-freezing mean annual temperature conditions in order to preserve the amorphous material in the soils.”
Amorphous material is often considered to be relatively unstable, meaning that at an atomic level, the atoms haven’t yet organized into their final, more crystalline forms.
“There’s something going on in the kinetics — or the rate of reaction — that is slowing it down so that these materials can be preserved over geologic time scales,” Dr. Feldman said.
“What we’re suggesting is that very cold, close to freezing conditions, is one particular kinetic limiting factor that allows for these materials to form and be preserved.”
“This study improves our understanding of the climate of Mars.”
“The results suggest that the abundance of this material in Gale Crater is consistent with subarctic conditions, similar to what we would see in, for instance, Iceland.”
The team’s work appears in the journal Communications Earth and Environment.
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A.D. Feldman et al. 2024, Fe-rich X-ray amorphous material records past climate and persistence of water on Mars. Commun Earth Environ 5, 364; doi: 10.1038/s43247-024-01495-4
This article is based on a press-release from Desert Research Institute.
Source : Breaking Science News