China’s Tianwen-1 orbiter caught a rare glimpse of 3I/ATLAS as it swept past Mars, revealing the hazy coma and tail of a comet born beyond our solar system. The interstellar object known as 3I/ATLAS just flew past Mars, and China’s Tianwen-1 mission managed to snap some pics with its high-resolution camera. According to the China [...]The post NASA’s Viking Mission to Mars appeared first on NASA Science.
An international team of researchers has demonstrated a new biosignature detection method for distinguishing between abiotic and biotic apatite mineral samples on Mars using instruments already aboard the Perseverance Rover, rather than returning samples to Earth.
The team said their mineral-based biosignature detection approach was successful in identifying samples with nearly 98% accuracy and allows for “deeper time” searches for signs of life, given the longer-lasting nature of minerals compared to biological materials. They also suggest their approach could broaden the capabilities of upcoming rover and life-hunting missions without adding new tools or sensors.
In a study detailing the team’s technique, Robert M. Hazen from the Carnegie Institution for Science and colleagues explained that searching for life and biosignatures beyond Earth “is a central objective of astrobiology.” They also note that this research is complemented by studies exploring the origin and early evolution of terrestrial life. Still, they add, although identifying biosignatures remains a key challenge, “robust mineral biosignatures remain limited.”
For example, most proposed biosignature missions focus on organic molecules or searching for fossils preserved in sedimentary environments or aquatic environments, including the subsurface oceans of some of the solar system’s moons. However, there are few, if any, proposed missions searching for signs of life preserved in mineral records, which the team notes “can retain records of biological activity over much longer geological timescales”
On Mars, NASA’s Perseverance rover has meticulously collected soil and rock samples deemed most likely to contain biosignatures. However, efforts to send a future sample-return mission to the red planet to retrieve samples are currently stalled and may never be completed.
According to the study authors, there are flight-ready instruments “already deployed on the “Perseverance” rover and planned for deployment on the “Rosalind Franklin” rover capable of searching for signs of life in place rather than returning the samples to labs on Earth. However, they add, “to fully exploit these mission-limited yet information-rich tools, it is essential to efficiently extract as much diagnostic value as possible from the data they generate.”
To search for mineral-based biosignatures, the team focused its research on Raman spectroscopy.
“Raman spectroscopy is particularly attractive because it provides bond-specific information on crystal structure and chemical substitution in a nondestructive manner,” they explain.
The team also notes that the Raman spectra acquired by the rover’s instruments “are highly comparable to those obtained under laboratory conditions,” increasing the robustness of any possible life signal.
“This consistency enables direct translation of laboratory reference datasets to planetary environments,” they write.
However, they add, Raman spectra from natural geological samples are often complex, including “overlapping vibrational modes, heterogeneous backgrounds, and chemistry-dependent band shifts.” Until now, this complexity has made interpreting samples based on individual spectral peaks or qualitative inspection inherently challenging.
“Identifying reliable biosignatures that can be detected by flight-ready instruments, such as Raman spectroscopy, remains a central challenge in astrobiology,” the researchers explain. “Developing robust mineralogical indicators of life therefore represents a critical and complementary approach for planetary exploration.”
To test their approach, the team focused on the mineral apatite. A ubiquitous phosphate, the team notes that apatite can be found “in terrestrial and extraterrestrial environments.” Although apatite is a major component of biological formations such as teeth and bones, it also forms naturally, providing an opportunity to search for biosignatures over much longer timescales if scientists can differentiate the two.
“Here, we integrate Raman spectroscopy with interpretable machine learning to distinguish biotic from abiotic apatite, a ubiquitous phosphate mineral in terrestrial and extraterrestrial environments,” the researchers write.
First, Hazen and colleagues compiled 331 Raman spectra samples. Critically, they included only specimens with known origin attributes: biogenic, abiogenic, or synthetic.
Next, they used this data to extract 21 “band-resolved features.” This was accomplished by training a random forest classifier to identify the “most diagnostic” features of each sample.
“Determining the origin of a sample involves assessing multiple independently varying features of a Raman spectrum, including band positions, widths, and relative intensities, the type of multivariate analysis well suited to machine learning,” the study authors explain.
After some comparative analysis, the team ultimately determined that a sample’s carbonate band and the width of the dominant phosphate band, “reflecting chemical composition and crystal structure, respectively,” were the strongest indicators of biological, natural, or synthetic origin.
After using their method to check the 311 samples, the team said the model successfully distinguished biotic from abiotic apatite “with classification accuracy exceeding 96%.” In fact, the team reported that their mineral-based biosignature detection method misidentified only one biotic apatite sample as abiotic and one abiotic sample as biological.
“Here, we show that biologically formed apatite can be distinguished from abiotic counterparts using interpretable machine learning applied to Raman spectra,” the study authors write.
When discussing the potential implications of their new mineral-based biosignature detection approach, the team noted that their findings establish a “broadly applicable and mission-relevant strategy for deep-time archives and future planetary missions.” More broadly, the researchers note that their findings highlight the “growing importance of combining flight-ready analytical instruments with AI” to fully leverage datasets already captured by Mars rovers and other “in situ” planetary missions.
“As planetary exploration increasingly shifts toward autonomous decision-making and target selection, the integration of interpretable AI with mineralogical biosignatures offers a powerful and extensible framework,” they write.
Beyond mineral-based biosignature detection strategies, the research team notes that future life hunting missions will “increasingly rely on the joint interpretation of mineralogical and organic spectroscopic signatures.” These include on-board py-GC-MS measurements, infrared spectroscopy, luminescence, laser-induced breakdown spectroscopy, X-ray fluorescence, and “other analytic methods.”
Future approaches will increasingly rely on AI to analyze these disparate datasets, which the authors note will allow for biologically mediated patterns to be distinguished from natural or synthetic backgrounds “in a physically and chemically consistent manner.”
“In this context, such an integrative and interpretable framework provides a pathway toward autonomous, mechanism-informed life detection across diverse planetary environments, advancing the broader goals of planetary science in understanding habitability, biosignature preservation, and the coevolution of geology and biology,” the authors conclude.
The study “Mineral biosignature identification from Raman spectroscopy using machine learning” was published in PNAS Nexus.
Christopher Plain is a Science Fiction and Fantasy novelist and Head Science Writer at The Debrief. Follow and connect with him on X, learn about his books at plainfiction.com, or email him directly at christopher@thedebrief.org.
If you still picture Mars as a monotonous red desert, it may be time for an update.
The European Space Agency's Mars Express orbiter has been capturing some of the Red Planet's most surreal landscapes, and its latest images reveal a sprawling field that looks like molten metal frozen across the floor of an ancient Mars crater.
The shimmering "waves" aren't metal at all, however. They are dark sand dunes dusted with seasonal frost, much of it carbon dioxide, or "dry ice," that settles on the surface during Martian winters, giving the dunes their uncanny chrome-like sheen, according to ESA.
The rest is a trick of light and contrast. Because the dark sand absorbs light and the white frost reflects it, the interplay transforms the landscape into something that looks more like a scene from a sci-fi movie than a windswept Martian plain.
Over thousands of years, Martian winds have sculpted this volcanic sand into dunes that now ripple through the floor of Kaiser Crater, a 129-mile-wide (207-kilometer-wide) impact basin in the planet's southern highlands. The bowl-shaped crater acts as a giant sand trap that prevents the sand from escaping, according to NASA.
The dunes themselves are darker than much of Mars' surface because they are made of fine, basaltic sand rich in volcanic minerals such as pyroxene and olivine, rather than the iron-oxide dust that gives the planet its familiar rusty-red appearance and its famous moniker, the Red Planet.
Because the crater floor remains visible between the ridges, scientists think there is a relatively limited sand supply shaping the field. Still, these ripples of sand are massive, extending for several kilometers and towering more than 100 meters (320 feet) above the surrounding terrain.
The landscape isn't just visually dramatic, it also preserves clues to a time when Mars was a very different world.
Today, Mars is wrapped in an atmosphere little more than a thin veil that is 100 times thinner than Earth's and slowly leaking into space. That makes it harder for winds to lift and transport sand than it is on our own planet. Yet the soaring dunes inside Kaiser Crater show that Martian winds have nonetheless been powerful enough to sculpt vast landscapes over time, perhaps during a period when the Martian atmosphere was thicker a few billion years ago.
The new image adds to a growing collection of striking Martian scenes captured by Mars Express, which has been orbiting the Red Planet since 2003. Just last month, the probe tracked a frenetic cluster of 30 dust devils swirling through the canyons of Mamers Valles, also in the northern hemisphere.
Over the spring and summer, the orbiter similarly spotlighted the planet's vast and complex geological history, from Shalbatana Vallis — carved by groundwater floods about 3.5 billion years ago into winding valleys that span the length of Italy — to a massive blanket of dark volcanic ash elsewhere on the world that has spread across a large chunk of the terrain over just the last 50 years, having either been redistributed by Martian winds or exposed as the overlying dust was blown away.
However desolate Mars may appear from afar, there is certainly no shortage of activity on its surface — or discoveries still waiting to be made.
5 min read
NASA’s Perseverance Mars rover has uncovered evidence that a 245-foot-thick (75-meter-thick) stack of ancient rock on the rim of Jezero Crater was built by repeated asteroid impacts. Referred to as the “Broom Point member” by the rover’s science team, this sequence of layered bedrock is likely more than 3.9 billion years old, making it among the oldest terrain ever examined by a Mars rover.
Released Wednesday in the Journal of Geophysical Research: Planets, the findings offer a window into one of the most tumultuous chapters in the history of the solar system.
“Since leaving Jezero, Perseverance has been exploring a brand-new frontier, both geographically and geologically — a chapter of Martian time that predates the crater itself,” said Ken Farley, Perseverance deputy project scientist at Caltech in Pasadena, California. “On Earth, our earliest geologic history has been fundamentally broken up, deformed, and erased by plate tectonics. Because Mars lacks plate tectonics to recycle its crust, this ancient record remains intact, giving us a rare glimpse into a geological time period that doesn’t exist on our own planet.”
After ascending the western rim of Jezero Crater in late 2024, Perseverance began examining surrounding locations with its science instruments. Their data at Broom Point revealed six distinct rock types, including breccias — rocks composed of angular fragments — alternating with layers of fine-grained, pulverized rock dust. Rock fragments within the breccias are pocked with gas-bubble cavities, indicating they were once molten.
The presence of tiny, dark, glassy beads within the layers offered an important clue about how these rocks formed. While volcanoes can produce similar glassy droplets, they rarely occur in such high abundance, pointing to asteroid impacts, instead, as the primary architect. In fact, the largest beads rival those flung out by the dinosaur-killing Chicxulub asteroid’s impact on Earth.
The repetition of these distinct rock types multiple times throughout this thick sequence of rock indicates that high-energy impact events happened again and again across this region of early Mars.
“The different rock layers are a record of variable-sized impacts occurring at different distances from where this rock sequence was accumulating,” said Alex Jones, a Ph.D. student in planetary geology at Imperial College London and lead author of the paper. “Some large impacts took place very far away, some small impacts nearby. Their debris all ended up landing here, constructing this thick section of rock.”
How these layers formed may suggest an interaction with water or ice. Several of the layers look like they may have been formed by fast, ground-hugging debris flows. On Earth, these powerful, fluidlike surges can occur when molten rock hits water or ice that instantly flashes into steam.
Some of Broom Point’s layers tilt at angles exceeding 80 degrees — nearly vertical — which is far too steep to be caused by the impact that created Jezero Crater.
Instead, scientists suspect a cosmic “one-two punch” shaped this landscape long ago. First, a colossal asteroid impact created the 1,200-mile-wide (1,900-kilometer-wide) Isidis Basin, one of the largest impact basins on Mars, upending and tilting the once-flat rock layers. Later, a second asteroid likely struck, forming Jezero Crater, which measures 28 miles (45 kilometers) across. This second impact fractured and uplifted the already-tilted rocks into the dramatic formations the rover sees today.
To pin down exactly when these events took place, the Perseverance team collected two core samples, dubbed “Bell Island” and “Main River.” If a future mission were to return them to Earth, laboratory dating could determine when and how often impacts were occurring on early Mars — and, by extension, the infant Earth, whose own early impact record has been erased by billions of years of plate tectonics.
“During this violent era, it wasn’t rain or snow falling from the sky, but an almost constant barrage of molten rock droplets and pulverized dust kicked up by asteroid impacts,” said Jones. “If we can pin down the ages of these layers, it would be like reading a cosmic weather report from 4 billion years ago.”
NASA’s Jet Propulsion Laboratory in Southern California, which is managed for the agency by Caltech, built and manages operations of the Perseverance rover on behalf of the agency’s Science Mission Directorate in Washington, as part of NASA’s Mars Exploration Program portfolio. Arizona State University leads the operations of the rover’s Mastcam-Z instrument, working in collaboration with Malin Space Science Systems in San Diego, on the design, fabrication, testing, and operation of the cameras. SuperCam is led by Los Alamos National Laboratory in New Mexico, where the instrument’s Body Unit was developed. The rover’s SHERLOC (Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals) instrument was built at NASA JPL, and its WATSON (Wide Angle Topographic Sensor for Operations and eNgineering) camera was built at Malin Space Science Systems.
For more information on NASA’s Perseverance, visit:
https://science.nasa.gov/mission/mars-2020-perseverance
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NASA’s Mars Perseverance rover seeks signs of ancient life and collects samples of rock and regolith for possible Earth return.
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NASA is teaming up with 37 companies to develop the next generation of technologies that could make long-term exploration of the Moon and Mars possible. NASA has chosen 41 proposals from 37 U.S. companies to help develop technologies needed for a sustained human presence on the Moon and eventual crewed missions to Mars. The companies [...]A new NASA orbital image captures Perseverance after completing a marathon across the surface of Mars. NASA’s Perseverance rover has completed the equivalent of a full marathon on Mars, reaching 26.2 miles (42.195 kilometers) after five years and four months of driving across the Red Planet. The milestone came on the 1,890th Martian day, or [...]
NASA's Curiosity rover has spotted a strange honeycomb texture on the surface of Mars. But what is it?
Almost 14 years since landing on the Red Planet, Curiosity is still hard at work exploring. And in new observations, Curiosity has revealed an image that is certainly ... peculiar.
Curiosity went to get a closer look at an area first observed from Mars orbit, and found what appears to be a honeycomb structure in on the planet's surface. Polygonal shapes, nearly identical to one another, make up a pattern almost like a Martian wallpaper or carpet.
But what is it? Why does it look like that? What is a honeycomb doing on Mars?
This is one of many mysteries we have yet to solve on Mars. While the team saw this area first from orbit around the planet, when the rover arrived and saw this structure they were surprised, they shared in a blog post.
In addition to the honeycomb texture, the area was littered with dark rocks and strewn around. But even these pebbles lack explanation. Did they "float" down from higher rock levels, did they launch out of Gale crater during some ancient collision or could they possibly even be meteorites from outside of Mars that ended up strewn across the surface? Researchers think any one of these explanations could be possible.
Previous, similar dark stones have been found on Mars with minerals like nickel that are common in meteorites and uncommon in Mars rocks. But are these similar? Perhaps part of a similar collision event? We don't yet know.
As researchers find new mysteries on Mars, they also continue to find new ways to investigate the unknown. With further study, they will explore both these strange honeycombs and the dark rocks scattered amongst them.
This week in stories we’re covering at The Debrief… Japan’s Hayabusa2 spacecraft just completed its flyby of the mysterious asteroid Torifune over the weekend, in a celestial rendezvous that nearly coincided with the Chinese Tianwen-2 mission’s successful capturing of new images of Earth’s “quasi-moon”. Equally intriguing are the unusual “polygon” structures NASA’s Curiosity rover just spotted and photographed on the Martian surface; what are they, and what caused them? And finally, bringing things back down to Earth a bit, scientists have revealed new details about an odd “reversal” that occurred deep within the Earth’s molten core, and what new findings suggest that could mean.
In addition to these stories, here’s a look at more of the stories we’re following right now at The Debrief…
An unusual discovery on the Red Planet has revealed an odd-looking series of polygon-shaped structures, documented in new images obtained by NASA’s Curiosity Rover.
The curious features were discovered after Curiosity was dispatched to an area of interest on the Martian terrain initially identified from orbital imagery obtained by the Mars Reconnaissance Orbiter (MRO).
Upon its arrival at the area, which the satellite imagery had conveyed as appearing light in coloration and apparently smooth-surfaced, Curiosity discovered something vastly different.
Writing at NASA’s Curiosity blog, Senior Research Scientist William Farrand of the Space Science Institute described the area in question as being “covered with polygonal structures like the top of a giant Martian honeycomb.”
Polygonal structures are a frequent occurrence in nature, as evidenced by the Curiosity team’s likening them to a “honeycomb” in appearance. Similar polygon-shaped features are often seen in geology, such as the famous Giant’s Causeway on Northern Ireland’s Antrim Coast, which consists of close to 40,000 interlocking basalt columns that bear a similar appearance to the features recently discovered on Mars by Curiosity.
This is also not the first time such features have been observed by Curiosity. Last May, NASA revealed similar discoveries of structural features resembling honeycomb or “waffle” patterns.
As Curiosity proceeded into the unusual area, imagery provided by the rover revealed additional polygonal features, albeit in a more eroded condition than the features it initially spotted.
“Littered about this unit are pebble to cobble-sized dark-toned rocks,” Farrand wrote, adding that among the unresolved questions researchers with the Curiosity team have “is whether these are bits of Mars that ‘floated’ down from higher in the stratigraphy, were ejected from distant impacts outside of Gale crater, or are meteorites from beyond Mars altogether.”
A potential clue arises from the presence of nickel Curiosity detected in some of the darker stones. This may be significant, since nickel is generally rare in Martian rocks.
The same can’t be said for meteorites, though, which often contain an abundance of nickel and other metals. On Earth, meteors that flash in vivid shades of green as they collide with Earth’s atmosphere do so when nickel and magnesium are present within these space rocks.
It remains unclear whether all the darker-colored stones discovered by Curiosity are possible fragments from a meteorite or if their appearance is due to other factors that remain undetermined.
“Further investigations should help in answering this question,” Farrand added.
On Monday, June 29, 2026, Curiosity continued its investigations of these unusual features with its APXS and MAHLI instruments, with further plans to conduct additional viewing of an area the Curiosity team has dubbed the Miraflores butte, which features a small knob-like prominence.
Additional viewing was planned for the nearby Cordillera mesa as well, although much of the rover’s work has remained focused on the unique polygon-shaped structures.
“After driving further towards the upper boundary of the light-toned, polygon-covered unit, the three-sol Friday plan included APXS and MAHLI measurements of another polygon ridge and one of the dark-toned cobbles,” Farrand’s update at the Curiosity blog noted.
This particular cobble, which the Curiosity team has dubbed “Cortadera,” was studied using the rover’s ChemCam instrument, which was also used in observations of the aforementioned features, and others in the nearby Martian terrain.
In the days ahead, Curiosity is expected to traverse another area where dark-colored materials are present based on previous orbital reconnaissance, which may provide additional clues about their origins, and the intriguing features in the area where the rover’s current investigations are focused.
Additional details can be found at NASA’s Curiosity blog.
Micah Hanks is the Editor-in-Chief and Co-Founder of The Debrief. A longtime reporter on science, defense, and technology with a focus on space and astronomy, he can be reached at micah@thedebrief.org. Follow him on X @MicahHanks, and at micahhanks.com.
This week in stories we’re covering at The Debrief, one of the Seven Wonders of the Ancient World has been rediscovered and is now rising from its ancient resting place in the Mediterranean. Meanwhile on Mars, NASA’s Mars Reconnaissance Orbiter (MRO) just spotted something in a hilly area of the Red Planet that you have to see; fortunately, the space agency has unveiled it all in stunning new images. And finally, this unusual object should have been “impossible” to create using Iron Age tools… so how did its ancient crafters make it?
Ready to dive deeper? Here’s a look at several of the top stories we’re covering right now at The Debrief…
Evidence for possible life on Mars in the ancient past continues to build, thanks to a recent discovery by NASA’s Perseverance rover that identified complex carbon in two mudstones.
As detailed in a recent paper published in Science Advances, Perseverance collected samples in the Jezero crater, a location that has continued to yield possible biosignatures of life on Mars in the ancient past.
In the same region, scientists reported potential evidence of microbial activity on ancient Mars, adding to a growing list of circumstantial evidence for one of the most intriguing possibilities in modern space exploration: the prospect that Earth may not have been the only planet in our Solar System that has held the potential to host life.
Among the study’s most significant findings is that complex macromolecular carbon was discovered alongside other potential biosignatures. Jezero Crater, a 28-mile-wide impact basin on the Martian surface, once contained flowing water roughly 3.5 billion years ago, making it one of the most promising locations in the search for ancient life. Water is essential to all known life on Earth, serving as a universal solvent and playing a critical role in biological processes.
“Jezero Crater was selected as a landing site due, in part, to its past evidence of aqueous activity and potential to preserve organic material,” co-lead author Kyle Uckert, a research scientist at NASA’s Jet Propulsion Laboratory, told The Debrief. “The Perseverance Rover’s exploration of Jezero Crater helps us understand the past habitability of Mars.”
Perseverance targeted a distinctive geological feature known as the Bright Angel outcrop, where the samples were collected. The outcrop consists of mudstones deposited in the dry bed of an ancient river that once flowed into Jezero Crater. Comparable sedimentary deposits on Earth are often associated with environments capable of preserving evidence of microbial life.
Determining the origin of the organic carbon preserved within these Martian rocks is key to understanding whether the Red Planet ever supported life.
Using its onboard Raman spectrometer, Perseverance mapped the distribution of the rocks’ organic matter. One sample contained organic carbon within a primary silicate-dominated matrix, while another preserved carbon within secondary carbonate and sulfate minerals.
Notably, the carbon appears to have remained remarkably well preserved despite billions of years of exposure to the harsh Martian environment. Researchers suggest its limited weathering may indicate that the material is resistant to radiation and oxidation—possibly because it is mixed with iron-rich regolith or protected by clay minerals—or that it was only recently exposed at the surface through erosion.
The researchers are quick to point out that their findings do not determine whether the carbon originated through biological or non-biological processes. Nevertheless, the discovery adds another intriguing piece of evidence to the ongoing search for ancient life on Mars.
“Macromolecular carbon may be delivered to Mars via meteorites, or may have formed through hydrothermal geologic processes,” Uckert said.
According to the researchers, determining the true origin of the carbon will ultimately require returning Martian samples to Earth, where they can be examined using far more sophisticated laboratory instruments than those carried aboard Perseverance.
“Further constraining the origin, distribution, and alteration history of the MMC observed in the Neretva Vallis mudstones requires high-resolution and high-sensitivity analyses in terrestrial laboratories, which can be facilitated by the return of the Cheyava Falls rock core, ‘Sapphire Canyon’ to Earth,” explained co-lead author Ashley Murphy, a postdoctoral research scientist at the Planetary Science Institute.
“The Perseverance Rover science payload is not designed to determine whether martian organic molecules were created by biologic or geologic processes, and our study is unable to make this distinction,” Uckert added.
The researchers say that future sample-return missions, combined with advanced laboratory analyses on Earth, may finally help resolve one of planetary science’s most enduring questions.
“The Perseverance Rover collects samples of scientifically compelling martian rocks for potential return to Earth,” Uckert concludes.“Using high-resolution terrestrial instruments to analyze these rock samples, particularly the Sapphire Canyon core collected on the Cheyava Falls rock, may provide more compelling evidence for a biologic or abiotic origin of this organic matter.”
The paper, “Spatially Distributed Complex Organic Matter Detected in an Ancient River Valley in Jezero Crater, Mars,” appeared in Science Advances on June 24, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
GOLDEN, Colorado — Scientists are engaged in research with an eye toward transforming the cold climes of Mars into a far more habitable place for Earthlings in the future.
One notion proposed is the dispersion of an aerosol meant to help warm up Mars' atmosphere. The idea is projected to be a first step toward terraforming the Red Planet. Also emerging recently as a new field of study is "applied astrobiology," which seeks to appraise what would be needed to create sustainable habitats and biospheres beyond Earth.
Scientists have drawn up a research blueprint for assessing the viability of warming the Red Planet, outlining what it might take to make Mars a place in space where life can thrive. Importantly, that roadmap does not presuppose that warming Mars is desirable. Rather, its purpose is to identify what is required for Mars to be warmed, what it would cost and what could go wrong.
Edwin Kite, an associate professor of geophysical sciences at the University of Chicago, detailed the plan here at a Space Resources Roundtable, which was held from June 2 to June 5 on the campus of the Colorado School of Mines.
Kite's talk showcased a mission concept prototype to validate aerosol dispersal to warm Mars' atmosphere as a first step toward terraforming the Red Planet.
"Creating sustainable habitats and biospheres beyond Earth is an enormous scientific and technical challenge, but it's one we'll have to surmount if we're going to extend life beyond Earth," Kite told Space.com.
"We do not yet know enough to create a biosphere from scratch," he added. "Applied astrobiology, like planetary science, requires contributions from many disciplines."
Kite said that relatively modest research investments can keep open the option of extending life beyond Earth as the scientific exploration of Mars continues.
The roadmap, Kite explained to Space.com, identifies several approaches to warming Mars. Solid-state greenhouse membranes, he said, offer the nearest-term benefits, with direct applications to moisture farming and life support at human bases on Mars.
Strengthening Mars' natural greenhouse effect might warm large regions of the globe, Kite noted, although many aspects remain to be worked out. Each approach carries scientific and technical risks that research must address, he added.
Whether Mars can support a biosphere, however, is unknown. But, if activated, a biosphere on Mars would help sustain large numbers of people in bases beyond Earth, sparking the conditions for a centuries-long process of atmospheric oxygen buildup.
The questions raised by the possibility of warming Mars are numerous. But the immediate unanswered questions are identifiable, Kite suggested, and can be addressed with a focused research campaign.
He acknowledged that a consensus on moving forward requires more data on two fronts: whether Mars could support life in the future, and whether there's life on Mars today.
An approach to warming Mars would be inherently modular, in that it could be done by many sites in parallel, Kite suggested. An aspect of the endeavor may well involve orbiting reflectors for warming intermediate-sized areas, such as human bases.
Kite is also a resident researcher at the Berkeley, California-based Astera Institute, which was founded to steer science and technology towards an abundant future. And he's a participating scientist on the mission of NASA's Curiosity Mars rover, which has been exploring the Red Planet since August 2012.
Being scoped out by Kite and fellow researchers is a potential technology demonstration on Mars, an automated payload that would test an aerosol release concept. It would discharge less than 2 pounds (about 1 kilogram) of sub-micron artificial particles and laser track that dispersal to an altitude of roughly 1,500 feet (500 meters), to confirm ascent of the plume into the skies of Mars.
Kite said that dispenser requirements are particularly challenging. For example, researchers will need to show that it works on Earth before launching a demonstration mission to Mars.
There has been "prototyping progress," Kite said, with an experimental setup designed and built for rapid deployment.
To trial-run the particle dispersal concept and plume tracking technology, the plan calls for use of NASA's Planetary Aeolian Laboratory (PAL) at Ames Research Center in California this year. PAL is a unique facility used to support experiments under different planetary atmospheric environments, including Earth, Mars and Saturn's largest moon, Titan.
To help evaluate the feasibility of terraforming Mars, Kite points to the need for better maps of subsurface water ice on that world; climate-monitoring orbiters to observe the planet's natural variability; the return of Red Planet samples to Earth for study; and international cooperation.
"Mars sample return will be done by China's space agency. The original plan for their Tianwen-3 mission was to grab some rocks from wherever and then head back to Earth," Kite said. "The new plan is to go around with a helicopter and collect rocks from a wide area. I'm hopeful that they share their Martian samples, allowing all the world's labs to have a crack at them."
Then there's the prospect of an International Mars Ice Mapper, Kite said, a proposed Mars orbiter that's been studied by NASA, the Japan Aerospace Exploration Agency (JAXA), the Canadian Space Agency (CSA) and the Italian Space Agency (ASI). However, that mission appears at this moment to have been shelved.
"It's a good idea and could always come back," said Kite. "We should search for deep aquifers using electromagnetic soundings — that's the best strategy. We don't know whether there's still liquid water deep underground. There are big gaps in our knowledge about Mars."
Kite reported that warming Mars with artificial aerosol appears feasible, backed by workshops about creating a "Green Mars" and applied astrobiology.
If early findings from aerosol release demonstrations on Mars prove positive, Kite said, those results would provide the quantitative basis for "government-scale programs" to evaluate whether extending habitable conditions beyond Earth is achievable, at what cost and on what timescale.
"Even under optimistic assumptions, warming at kilometer scale is at least a decade away, and wider environmental modification would require sustained investment over many decades beyond that," states the recent research paper, which Kite led.
"Relatively modest research investments would keep open the option of extending life beyond Earth as Mars’ scientific exploration continues," Kite and his colleagues concluded.
Flood-Related Surface Collapse at Osuga Valles, Mars: Unveiling the Dynamics of Martian Geomorphology
Recent research published in Communications Earth & Environment has spotlighted a remarkable phenomenon occurring on Mars — flood-related surface collapses in the Osuga Valles region. This discovery marks a transformative step in our understanding of Martian geomorphological activity, revealing dynamic processes previously undetected on the Red Planet. The comprehensive study led by Naor et al. deploys advanced remote sensing and modeling techniques to decipher the mechanisms behind these collapses, providing a fresh perspective on Mars’s hydrological past and present.
Osuga Valles, located in the northern hemisphere of Mars, has long intrigued planetary scientists due to its complex valley networks and evidence hinting at ancient water activity. The new findings reveal that these valleys are not merely relics of a bygone era but continue to undergo morphologic changes influenced by episodic flooding events. These floods, possibly triggered by subsurface ice melting or transient atmospheric phenomena, induce sudden collapses on the surface, reshaping the landscape at scales previously underestimated.
The investigation is centered around detailed analysis of high-resolution imagery combined with digital elevation models captured by Mars orbiters. These datasets allowed the researchers to identify distinct collapse features characterized by disrupted terrain, steep scarps, and chaotic blocky deposits. The spatial distribution and morphology indicate that these collapses originated from floodwaters undermining subsurface deposits, triggering a rapid failure of overlying strata.
What makes the Osuga Valles surface collapses particularly compelling is their implication for current Martian hydrology. The collapse events are believed to be linked to relatively recent flood episodes, suggesting the presence of liquid water or brines beneath the Martian surface. This challenges the longstanding notion of Mars as an entirely arid world and paves the way for hypotheses about transient hydrological cycles persisting in specific locales and under certain environmental conditions.
Moreover, the tectonic setting of the Osuga Valles region seems to facilitate these collapses. The valley system’s structural configuration, inclusive of fractures and faults, creates zones of mechanical weakness. When these structural features interface with floodwaters infiltrating subsurface layers, they act as conduits potentiating the collapse process. Thus, the interplay between geology and hydrology emerges as a critical driver of surface dynamics on Mars.
The authors also explore analogs from terrestrial environments—places where flooding induces surface collapse, such as in karst terrains or volcanic regions with subglacial lakes—to better interpret the Martian data. These Earth analogs provide a fertile framework for understanding how subsurface voids or weakened materials collapse under hydraulic pressure, refining our conceptual models applicable to Mars.
Advanced computational fluid dynamics simulations performed in the study reveal that the hydraulic pressures generated by transient floods are sufficient to disrupt sediment cohesion and trigger mass wasting events. The models incorporate variable sediment porosities, ice content, and fracture permeability, emphasizing how subtle changes in subsurface conditions can culminate in massive geomorphic transformations. This underscores the sensitivity of Martian surface processes to inundation events, even if these are limited in time and spatial extent.
In addition, the researchers analyzed mineralogical data from spectrometers aboard orbiters, detecting possible hydrated minerals and salts that corroborate the interaction between water and subsurface sediment. This mineralogical evidence supports the hypothesis of localized aqueous alteration driven by flood events, contributing to ongoing soil and sediment evolution in Osuga Valles.
The implications of these findings extend beyond geology and planetary science to astrobiology. The presence of liquid water, even transiently, opens up potential niches for microbial life or preserves biosignatures in subsurface refuges. Flood-related collapses could expose freshly altered materials, creating accessible targets for future rover missions endeavoring to seek signs of life or past habitability.
Technological advancements in orbital imaging and data analysis have thus unlocked a new era in Martian surface exploration. This study leverages these capabilities, illustrating how multidisciplinary approaches integrating geomorphology, hydrology, geochemistry, and computational modeling can unravel complex planetary phenomena. The Osuga Valles floods and collapses exemplify the dynamic and evolving nature of Mars, still shaped by aqueous forces despite its overall cold and dry climate.
Looking forward, these discoveries necessitate a revision in mission planning and surface hazard assessments. Understanding flood-related collapses aids in predicting surface stability and potential geomorphic hazards affecting landers or rovers. Moreover, unraveling the hydrologic cycles underlying these collapses could inform in situ resource utilization strategies, potentially enabling human exploration by identifying water reservoirs.
Furthermore, this research revitalizes the debate about Mars’s climatic variability and the possibility of episodic warming events facilitating surface liquid water. Such events might arise from volcanic outgassing, orbital shifts, or impact heating, temporarily altering atmospheric and subsurface conditions to create flood-triggering scenarios. Consequently, Osuga Valles may serve as a natural laboratory to study these transient climatic phenomena.
In summary, the study by Naor et al. dramatically expands our understanding of Martian surface processes by revealing active, flood-related collapses in Osuga Valles. By decoding the intricate linkages between subsurface hydrology, geological structure, and surface dynamics, it paints a picture of Mars as a planet where water still plays a crucial role in shaping landscapes. This breakthrough invites a new generation of explorations targeted at unraveling the mysteries of Mars’s watery past and its intermittent present.
The knowledge gained from these investigations not only transforms planetary science but also enriches comparative planetology, emphasizing how terrestrial analogs can illuminate extraterrestrial environments. As we decode Mars’s dynamic surface, the paradigm shifts from a static, desiccated world to one punctuated by active, fluid-driven geomorphology. The dynamic interplay between floods and collapses in Osuga Valles is a testament to this evolving narrative—a promise for thrilling discoveries yet to come.
Subject of Research: Flood-related surface collapses and geomorphologic processes on Mars, specifically in the Osuga Valles region.
Article Title: Flood-related surface collapse at Osuga Valles, Mars.
Article References:
Naor, R., Gulick, V.C., Spurling, R. et al. Flood-related surface collapse at Osuga Valles, Mars. Communications Earth & Environment (2026). https://doi.org/10.1038/s43247-026-03683-w
Image Credits: AI Generated
DOI: https://doi.org/10.1038/s43247-026-03683-w
Keywords: Mars geomorphology, flood-related collapse, Osuga Valles, Martian hydrology, subsurface water, geomorphic dynamics, remote sensing, planetary geology
Billions of years ago, Mars looked very different from the cold, dry world we see today. Scientists believe the Red Planet once had a warmer climate, liquid water and a thicker atmosphere. These conditions may have been suitable for simple forms of life. But did life ever actually exist on Mars? That remains one of […]
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A Martian meteorite fragment containing unexpected grains of mineral could hold clues to the Red Planet’s geological history, according to an international team of researchers.
Prior to the team’s new paper, which was published in Geochemical Perspectives Letters, the red mineral garnet had never been observed in any martian rock sample. Now, the meteorite discovery provides scientists with new clues to Mars‘ extreme past conditions, over its 4.5 billion-year history, which could include hidden magma sources or ancient impact events.
Although the gemstone garnet can come in many colors, it is best known for its dark red varieties, which were historically popular in ancient Egypt, Rome, and Victorian England. Beyond its beauty, the rock is important for the record it keeps of its birth, providing Earth’s geologists with information on our planet’s tectonic forces, ore-forming processes, and the fluid-rock interactions of the crust and mantle.
Similarly, the small grains of garnet discovered in the meteorite sample contain important data for reconstructing the forces that forged the Red Planet long ago.
“The findings add a striking new dimension to our understanding of the geology of Mars and open an exciting new window into the evolution of our planetary neighbour,” said co-author Professor James Darling.
“This discovery is going to expand our knowledge of the geologic processes that are possible on this planet,” said lead author Tanya Kizovski, Assistant Professor of Earth Sciences, from Brock University in Canada. “This new garnet-bearing rock type could give us clues to how Mars has changed throughout its history and new insights into the ancient environments that could have formed the garnet and related minerals.”
The garnet fragments were discovered in a tiny Martian meteorite sample held in the Royal Ontario Museum’s collection, designated NWA 8171, discovered in northwest Africa. Kizovski led the team in analyzing the sample’s mineral and chemical composition after identifying it as a unique piece within the collection.
“This little section of the meteorite looked really interesting, and the chemistry was a bit odd,” Kizovski said. “At first, we assumed it was a mineral called pyroxene, which is very common, but then we decided to take a second look.”
The international effort brought in researchers from Italy’s University di Trieste and the UK’s Open University, utilizing the Royal Ontario Museum’s laser equipment and the University of Portsmouth’s Electron Microscopy and Microanalysis Unit.
Having never been observed in any previous Martian sample, the researchers were surprised to identify garnet in the meteorite’s composition. From their analysis of the sample’s chemistry and mineralogy, the researchers began to consider how the unexpected garnet could have formed.
“Garnet is a classic example of a mineral often found in metamorphic rocks on Earth,” Kizovski said. “The process of metamorphism transforms igneous or sedimentary rocks into a new form through exposure to extreme heat, high pressure, or hot fluids.”
“On Mars, the heat and pressure needed to produce garnet through metamorphism could have come from the impact of a meteorite hitting the surface of Mars, magma rising up into the Martian crust, or both,” Kizovski continued.
While garnet provided geologists with some data about how it formed, this is not like the point of origin stamped on a manufactured good. It is possible that the garnet was deposited on Mars during an earlier meteorite impact, only to later travel through the solar system again, or that it was created by a heretofore unknown magma source on Mars.
Only further analysis of the garnet’s isotopic signatures will allow the researchers to determine whether the mineral formed on Mars or elsewhere. Unfortunately, to do so, the team would have to destroy a portion of this rare and precious sample, which measures only 0.8 by 0.5 millimeters to begin with.
“Measuring oxygen isotopes from the garnet-bearing rock type itself would help to confirm if it is Martian in origin or from an exotic meteorite impactor,” Kizovski said.
“Isotopes are a collection of atoms with equal numbers of protons and electrons, but different numbers of neutrons,” she added, “which was avoided thus far due to its rarity, as it may be the only garnet-bearing Martian rock we have for study.”
A few members of the team are continuing their study of the sample by comparing their findings to Martian data collected by rovers and orbital platforms. Further insights, they hope, may help them discover more about how the garnet could have formed, and what its presence means for the deeper history of the Red Planet.
The paper, “Expanding Mars’ Lithologic Diversity: Discovery of a Garnet-Bearing Clast in NWA 8171,” appeared in Geochemical Perspectives Letters on June 16, 2026.
Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.
Scientists have discovered a completely new type of rock from Mars and, for the first time, identified the mineral garnet in a Martian sample. The finding offers an exciting glimpse into the Red Planet’s distant past and could help researchers better understand how Mars evolved over the past 4.5 billion years. The discovery was made […]
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