In a groundbreaking study co-authored by a Texas A&M University scientist, researchers have revealed new insights into the geological history of Mars’ Jezero Crater, the landing site of NASA’s Perseverance rover. Their findings suggest that the crater’s floor is composed of a diverse array of iron-rich volcanic rocks, providing a window into the planet’s distant past and the closest chance yet to uncover signs of ancient life.
Research scientist Dr. Michael Tice, who studies geobiology and sedimentary geology in the Texas A&M College of Arts and Sciences, is part of an international team exploring the surface of Mars. He and his co-authors published their findings in Science Advances. “By analyzing these diverse volcanic rocks, we’ve gained valuable insights into the processes that shaped this region of Mars,” Tice said. “This enhances our understanding of the planet’s geological history and its potential to have supported life.”
Unlocking Mars’ volcanic history
Perseverance, NASA’s most advanced robotic explorer, landed in the Jezero Crater on Feb. 18, 2021, as part of the Mars 2020 Mission’s search for signs of ancient microbial life on the Red Planet. The rover is collecting core samples of Martian rock and regolith (broken rock and soil) for possible future analysis on Earth. Meanwhile, scientists like Tice are using the rover’s high-tech tools to analyze Martian rocks to determine their chemical composition and detect compounds that could be signs of past life. The rover also has a high-resolution camera system that provides detailed images of rock texture and structures. But Tice said the technology is so advanced compared to that of past NASA rovers that they are gathering new information at unprecedented levels.
The history of rocks on Mars
“We’re not just looking at pictures — we’re getting detailed chemical data, mineral compositions and even microscopic textures,” Tice said. “It’s like having a mobile lab on another planet.” Tice and his co-authors analyzed the rock formations within the crater to better understand Mars’ volcanic and hydrological history. The team used the Planetary Instrument for X-ray Lithochemistry (PIXL), an advanced spectrometer, to analyze the chemical composition and textures of rocks in the Máaz formation, a key geological area within Jezero Crater. PIXL’s high-resolution X-ray capabilities allow for unprecedented detail in studying the elements in the rocks.
Tice noted the importance of the technology in revolutionizing Martian exploration. “Every rover that has ever gone to Mars has been a technological marvel, but this is the first time we’ve been able to analyze rocks in such high resolution using X-ray fluorescence. It has completely changed the way we think about the history of rocks on Mars,” he said.
What the rocks reveal
The team’s analysis revealed two distinct types of volcanic rocks. The first type, dark-toned and rich in iron and magnesium, contains intergrown minerals such as pyroxene and plagioclase feldspar, with evidence of altered olivine. The second type, a lighter-toned rock classified as trachy-andesite, includes plagioclase crystals within a potassium-rich groundmass. These findings indicate a complex volcanic history involving multiple lava flows with varying compositions.
To determine how these rocks formed, researchers conducted thermodynamic modeling — a method that simulates the conditions under which the minerals solidified. Their results suggest that the unique compositions resulted from high-degree fractional crystallization, a process where different minerals separate from molten rock as it cools. They also found signs that the lava may have mixed with iron-rich material from Mars’ crust, changing the rocks’ composition even more.
Life on Mars?
“The processes we see here — fractional crystallization and crustal assimilation — happen in active volcanic systems on Earth,” said Tice. “It suggests that this part of Mars may have had prolonged volcanic activity, which in turn could have provided a sustained source for different compounds used by life.” This discovery is crucial for understanding Mars’ potential habitability. If Mars had an active volcanic system for an extended period, it might have also maintained conditions suitable for life for long portions of Mars’ early history.
“We’ve carefully selected these rocks because they contain clues to Mars’ past environments,” Tice said. “When we get them back to Earth and can analyze them with laboratory instruments, we’ll be able to ask much more detailed questions about their history and potential biological signatures.” Tice said that given the astounding level of technology on Perseverance, more discoveries are ahead. “Some of the most exciting work is still ahead of us. This study is just the beginning. We’re seeing things that we never expected, and I think in the next few years, we’ll be able to refine our understanding of Mars’ geological history in ways we never imagined.”
Source: Texas A&M University.
Image credit: NASA/JPL-Caltech/ASU.
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