Data Reveals Thick, Water-Rich Clay Layers on Mars, Shifting Exploration Priorities
Data Reveals Thick, Water-Rich Clay Layers on Mars, Shifting Exploration Priorities

Breakthrough Discovery: Thick Martian Clay Layers Could Preserve Evidence of Life

November 11, 2025  Jet Propulsion Laboratory, Pasadena, CA

The enduring question, “Are we alone in the universe?” has just found a compelling new focal point, not in the distant stars, but on our planetary neighbor, Mars. A comprehensive new analysis of data from NASA’s Perseverance rover and the ESA’s ExoMars Trace Gas Orbiter has revealed the presence of vast, deep, and remarkably pristine clay-rich sedimentary layers buried within the Jezero Crater and stretching across the Martian northern plains. This discovery, announced today by an international consortium of scientists, is being hailed as the most promising sign yet that the Red Planet may have once harbored life, and more importantly, that the evidence for it has been perfectly preserved for billions of years, waiting for us to find it. These are not mere surface stains; they are geological tomes, and we are on the cusp of learning to read them.

The significance of clay, or phyllosilicates, to astrobiologists cannot be overstated. Clay minerals are the product of the chemical weathering of rock in the presence of neutral-pH water over long, stable periods. Unlike the highly acidic or salty environments evidenced by other minerals on Mars, the conditions that form clays are benign, even hospitable, to life as we know it. On Earth, clays are known to form in calm, watery environments like lakebeds and slow-flowing rivers—exactly the kind of environments thought to have existed in Jezero Crater, an ancient lakebed with a clear river delta. But the new data suggests the story is far grander and deeper than previously imagined. Dr. Janice Bishop, a senior scientist at the SETI Institute and a key author of the report, explains, “What we’re seeing now is not just a shallow layer. We are looking at sedimentary deposits hundreds of meters thick. This implies a body of water that was not only persistent but potentially global in nature, an ocean in the northern lowlands, with a climate stable enough for hundreds of thousands, perhaps millions of years. That is a timescale more than sufficient for life to emerge and flourish.”

The breakthrough came from correlating two distinct streams of data. The Perseverance rover, which has been trundling across the Jezero delta floor, has been using its onboard spectrometer to analyze rock composition up close. Simultaneously, the ExoMars Orbiter, circling the planet from above, has been using its FREND (Fine Resolution Epithermal Neutron Detector) instrument to map hydrogen, a proxy for water, in the shallow subsurface. The combination was revelatory. The rover’s ground-truth data confirmed the presence of specific, complex smectite clays, while the orbiter revealed that these clay deposits extend far beyond the rover’s path, forming a continuous, water-rich layer beneath the dusty surface. This “clay horizon” appears to be a global or near-global feature, buried and protected from the harsh surface radiation that sterilizes the top layers of Martian soil. This protection is the second critical element of the discovery. The surface of Mars is bombarded by solar and cosmic radiation, which breaks down organic molecules over time. A sample on the surface would have its biological signatures erased within a few million years. However, a sample buried just a few meters underground could be preserved for billions of years.

The thick, overlying layers of rock and dust have acted as a perfect geological seal, creating a natural time capsule from Mars’s Noachian period, over 3.5 billion years ago, when the planet was wetter and warmer. Dr. Arun Misra, a planetary geologist at the University of Tokyo involved in the data analysis, states, “It’s like finding a library where all the books have been sealed in a vault. The surface of Mars has been scoured and sandblasted for eons, but these deep clay layers are pristine. They haven’t been cooked by volcanoes or oxidized by the atmosphere. They are quite simply the most promising biological records we have ever encountered on another world.”

The implications for the search for past life, or biosignatures, are profound. Clays are not just a benign environment; they are actively excellent at trapping and preserving organic matter. Their layered, charged structure acts like a molecular-scale sponge, absorbing and protecting lipids, proteins, and even fragile cellular structures from degradation. On Earth, some of the oldest evidence of microbial life has been found preserved in ancient clay deposits. The scientists hypothesize that if microbial life did exist in the standing waters of ancient Mars, its microscopic remains and chemical byproducts would almost certainly have been trapped and concentrated within these specific clay layers. The challenge, and the next great step, is getting physical access to these buried treasures. Perseverance is equipped with a drill, but it can only collect samples from the surface and very shallow subsurface. The most pristine, radiation-protected clays lie deeper.

This is where the future of Martian exploration comes into sharp focus. The discovery has immediately elevated the priority of a proposed “Deep Drill” mission, a rover specifically designed to drill several meters into the Martian crust to retrieve sealed core samples. The cache of samples being collected by Perseverance is intended for eventual return to Earth by a subsequent NASA-ESA mission in the early 2030s. However, those samples are primarily from surface-level rocks. The new findings are creating a powerful scientific consensus that the next logical step, after the Mars Sample Return campaign, must be a mission capable of accessing this deep clay horizon. Professor Lena Petrova, the lead European scientist on the ExoMars team, emphasizes the urgency, “This data changes the roadmap. We have now identified the address. The question is no longer ‘where should we look?’ but ‘how fast can we get there and dig?’ A deep-drilling mission is no longer a fringe idea; it is a strategic imperative for astrobiology. The potential for finding a definitive biosignature in those cores is, in my professional opinion, higher than it has ever been.”

Of course, caution remains the watchword in science. The discovery of a perfect repository for life does not guarantee that life was ever present to be stored within it. Abiotic processes can create complex organic molecules, and the bar for declaring the discovery of extraterrestrial life is, rightly, set astronomically high. The mission now is to prove a positive. Yet, the shift in perspective is palpable. For decades, the search for life on Mars has been a hopeful scavenger hunt across a desiccated landscape. Today, it feels more like a targeted archaeological dig, with a detailed map in hand. We have moved from asking “Could Mars have been habitable?” to actively identifying the specific shelves in the planetary archive most likely to hold the answer. The thick clay layers of Mars are no longer just a geological curiosity; they are a silent promise, a sealed chapter in the story of life in our solar system, and humanity has just been handed the key.