Perseverance rover finds light-colored rocks in Jezero crater, offering new clues about Mars' wet past

The rocks were determined to be kaolinite, which is found in tropical regions on Earth.
UPDATED DEC 3, 2025
Kaolinite rocks on Mars’ surface shows the dry, dusty planet could have featured a rain-heavy climate billions of years ago. (Image Credit: NASA)
Kaolinite rocks on Mars’ surface shows the dry, dusty planet could have featured a rain-heavy climate billions of years ago. (Image Credit: NASA)

A study published in Communications Earth & Environment suggests that certain pale rocks spotted on Mars, seen as bright, light-toned specks against the planet’s rusty terrain, are evidence that Mars once hosted moist oases with a humid atmosphere and substantial rainfall. These rocks were spotted by NASA’s Perseverance rover and were determined to be kaolinite, a white, aluminum-rich clay.

NASA's Perseverance (Mars 2020) rover uses its drill to core a rock sample and will store it for future missions, in the area known as Jezero crater on the planet Mars. (Photo illustration by NASA via Getty Images)
NASA's Perseverance (Mars 2020) rover uses its drill to core a rock sample and will store it for future missions, in the area known as Jezero crater on the planet Mars. (Image Source: NASA via Getty Images)

These are formed on Earth when all other minerals from rocks and sediments are swept off by millions of years of water and rain, according to Purdue University. “Elsewhere on Mars, rocks like these are probably some of the most important outcrops we’ve seen from orbit because they are just so hard to form,” said Briony Horgan, professor of planetary science in the Department of Earth, Atmospheric, and Planetary Sciences in Purdue’s College of Science. The sheer amount of water required for such formations led the scientists to conclude that the Red Planet might have experienced rainfall for millions of years. 

The Echus Chasma, one of the largest water source regions on Mars, pictured from ESA's Mars Express. (Image Source: ESA via Getty Images)
The Echus Chasma, one of the largest water source regions on Mars, pictured from ESA's Mars Express. (Representative Image Source: Getty Images | Photo by ESA)

Kaolinite clay on Earth is commonly found in environments that have tropical climates, like rainforests. Finding such a rock in a barren and dry place like Mars is a strong indication of a wet past. The fragments of kaolinite, which were as small as pebbles to as big as boulders, were initially examined by the Mars rover’s SuperCam and Mastcam-Z instruments and compared to similar rocks on Earth. These fragments might prove to be crucial in not just tracing Mars' past environmental stages but also help figure out how it became barren. 

Scientists were stunned on May 30 when a rock that NASA’s Curiosity Mars rover drove over cracked open to reveal something never seen before on the Red Planet: yellow sulfur crystals (Image Source: NASA/JPL)
Scientists were stunned on May 30 when a rock that NASA’s Curiosity Mars rover drove over cracked open to reveal something never seen before on the Red Planet: yellow sulfur crystals (Representative Image Source: NASA/JPL)

According to Horgan, what's really mysterious about the kaolinite is the absence of major outcropping near where the rocks could have originated, even though they can be found everywhere on the path Perseverance has followed since landing at the Jezero crater four years ago. “They’re clearly recording an incredible water event, but where did they come from?” Horgan said. “Maybe they were washed into Jezero’s lake by the river that formed the delta, or maybe they were thrown into Jezero by an impact, and they’re just scattered there. We’re not totally sure.” There is evidence of a lake that is around twice the size of Lake Tahoe in the crater, and major outcroppings of kaolinite have been spotted in other areas of Mars.

This illustration shows Jezero Crater — the landing site of the Mars 2020 Perseverance rover (Image Source: NASA/JPL-Caltech)
This illustration shows Jezero Crater — the landing site of the Mars Perseverance rover (Image Source: NASA/JPL-Caltech)

These spots are still out of reach and are yet to be investigated by the rover to get more insight into the rocks. "Until we can actually get to these large outcroppings with the rover, these small rocks are our only on-the-ground evidence for how these rocks could have formed,” Horgan stated. "And right now the evidence in these rocks really points toward these kinds of ancient warmer and wetter environments." The Martian kaolinite samples were compared to rock samples near San Diego, California, and in South Africa, and the rocks were a close match.

These dark, narrow, 100 meter-long streaks called recurring slope lineae flowing downhill on Mars are inferred to have been formed by contemporary flowing water (Image Source: NASA/JPL/University of Arizona)
These dark, narrow, 100-meter-long streaks called recurring slope lineae flowing downhill on Mars are inferred to have been formed by contemporary flowing water (Representative Image Source: NASA/JPL/University of Arizona)

Martian rocks are like a time capsule and can hold information about the planet from billions of years ago. No life can survive without water, and its presence on Mars opens a multitude of opportunities to explore.

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