A new stretchable quantum-dot light-emitting diode (QLED) delivers incredibly high resolution while producing record brightness that can be clearly viewed even outside in direct sunlight.

In a recent paper published in Nature Nanotechnology, Korean researchers unveiled a new QLED material with applications far beyond televisions, stretching into many future daily-use technologies.

This new QLED can stretch in every direction, just like organic skin, making it extremely useful in future wearable applications and as a covering for soft robots. Unlike earlier attempts to make a stretchable QLED, this one doesn’t lose picture quality when it stretches, delivering high resolution and extreme brightness under tension.

QLED Explained

For most of us, QLEDs are familiar as one of the technologies available in modern televisions. Conventional QLED TVs use quantum dots—nanoscale semiconductor crystals—to help produce exceptionally bright and vivid colors. OLED displays, by comparison, use self-emissive pixels that can switch off individually, allowing them to produce deeper blacks. While OLEDs perform particularly well in dark viewing environments, the high brightness achievable with quantum-dot displays can make them especially well-suited for brightly lit environments.

Despite the technology’s suitability for the bright world around us rather than just darkened environments, major challenges remained in producing a stretchable version. Early attempts addressed the problem by allowing the wiring to stretch while the light-emitting pixels remained unchanged in size. This meant that as the material expanded, its effective resolution dropped because the same number of pixels became spread across a wider area, much like enlarging a low-resolution digital image.

Building on these efforts, some researchers attempted to replace conventional materials with more stretchable alternatives, but these tended to make achieving high resolutions and efficiently moving electrical charge through the material difficult. As a result, these systems produced dimmer, lower-resolution images, limiting their utility.

A New Process

The researchers developed a new fabrication approach to address some of the major problems facing stretchable QLED technology. Central to their innovation is the use of an elastic polymer incorporating MPA as a ligand, or bonding molecule. This approach improves charge injection efficiency while helping eliminate the image stretching and smearing that have affected previous stretchable displays.

Using this new process, the researchers produced a display with a resolution of about 16,000 pixels per inch, with features spaced at roughly 700 nanometers. Red, green, and blue emissive layers can also be precisely arranged, allowing the stretchable material to produce full-color images.

Testing a New QLED

In tests, the team’s new QLED proved to be a major advance. They successfully stretched the material to 1.65 times its original size with no damage to its light-emitting performance. Additionally, their stretchable QLEDs were the brightest ever tested at 53,300 nits, more than triple the brilliance of prior attempts.

Based on these tests, the researchers see numerous future applications for their material in extended reality devices, soft robots, electronic skin, wearable technologies, health care, and automotive displays. 

“We resolved both the drop in resolution and the limits on light-emitting performance, which had been the biggest challenges for stretchable displays, and secured core technology for commercialization,” concluded co-author Professor Moon Kee Choi of Ulsan National Institute of Science and Technology in Korea. “It will be used widely as a manufacturing platform for various next-generation soft devices, including wearables and electronic skin.”

The paper, “High-Resolution Intrinsically Stretchable Quantum-Dot Displays Through Thermally Assisted Intaglio Transfer Printing,” appeared in Nature Nanotechnology on September 14, 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.

The most powerful volcanic eruption of the last century occurred in 2022 with the Hunga volcano, and new research reveals it caused massive changes to the Pacific Ocean floor, according to an international team of researchers.

In a recent paper published in Nature Geoscience, researchers revealed the extent of the underwater caldera collapse, in which material equal to 1,500 Great Pyramids was displaced, and a massive tsunami was created.

According to the team, studying this volcanic event yields important new information for monitoring such calamities and highlights what is to be gained by increased mapping efforts. Close monitoring is an essential element of tsunami early warning systems, where time is of the essence in saving lives.

2022 Hunga Volcano Eruption

Beginning December 20, 2021, and reaching its climax on January 15, 2022, the Hunga volcano eruption was a devastating underwater event. It occurred north of Tonga, an archipelago in the Pacific, and its effects spread as far as Chile, Peru, and Russia. The volcano is part of the Tonga–Kermadec Arc, a major submarine feature with 74 underwater volcanoes and 20 caldera complexes.

A caldera is a large depression that can form when magma is expelled from beneath a volcano and the overlying ground collapses. As a result of the eruption, the caldera deepened from roughly 150 meters below sea level to as much as 850 meters. The event displaced an enormous amount of volcanic material—8.9 cubic kilometers—and generated waves and underwater flows that destroyed crucial telecommunications cables and contributed to massive tsunamis. Fortunately, the eruption was far less deadly than an event like the 2011 Japanese tsunami. While millions of dollars in damage occurred, the global death toll remained at seven, despite fatalities occurring as far away as Peru.

Volcanic Caldera

While some of the displaced material resulted from erosion produced by the event, most of it was newly erupted magma. Still, only about 30% of the total magma involved was displaced, leaving a significant amount behind.

Historically, undersea volcanic calderas have been linked to some of Earth’s most catastrophic eruptions. Some 30,000 people died in 1883 when Indonesia’s Krakatau erupted, generating tsunamis and incredibly powerful ocean currents.

The Hunga caldera is extremely steep and formed during a rapid collapse, the speed and scale of which helped produce a tsunami even larger near the volcano than the one generated by Krakatau in the nineteenth century. Even about 100 kilometers from the volcano, waves reached heights of 40 meters.

Exploring the Sea

Scientists often discuss how mysterious the seafloor remains, representing a largely unexplored frontier here on our own planet. Yet with Hunga, this was not the case, as the seafloor in the region had already been extensively mapped. Having such detailed maps from before an underwater volcanic eruption is extremely rare, making this a unique opportunity for scientists to study the impact of such an event.

By comparing these before-and-after datasets, the team can identify changes to the seafloor and better understand the threats such events pose to coastal communities and critical undersea infrastructure, including communications and energy links. By collecting repeated observations, scientists may eventually be able to develop better predictive models.

The researchers say this event illustrates the need for more extensive and repeated high-resolution seafloor mapping to better study these changes. They note that the southwest Pacific is particularly in need of improved mapping. By developing better mapping datasets, the team hopes to help mitigate the impacts of future—and potentially deadlier—events.

The paper, “Rapid Submarine Caldera Collapse During the 2022 Climactic Eruption of Hunga Volcano (Tonga),” appeared in Nature Geoscience on September 11, 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.

A new class of cosmic object observed by NASA’s Chandra X-ray Observatory could hold the key to unraveling two long-standing mysteries, astronomers say.

In a recent paper published in Nature Astronomy, researchers described these new cosmic objects as having high levels of ultraviolet radiation but low-intensity X-rays. 

In the NASA Chandra data, the team identified 84 of these strange objects, which they dubbed “hypersoft X-ray sources,” across six galaxies. The unexpected discovery could finally help answer puzzling questions related to star formation and the expansion of the universe.

Chandra Sees Something New

“We’ve never encountered a group of objects that act like this,” said lead author Mustafa Muhibullah of the University of Alabama. “Of course, the next step was to try to figure out what these things are.”

The new research used data from a publicly accessible Chandra archive provided by NASA, including the spiral Andromeda and Pinwheel galaxies and an additional four elliptical galaxies. Intriguingly, both older regions and active star-forming regions contained the new objects.

The team discovered the objects by comparing Chandra’s high- and low-energy X-ray images to identify sources that were disappearing. Their departure from high-energy X-ray images indicated the objects were producing only low-energy X-rays, which border ultraviolet light on the spectrum. This led the researchers to then identify the high-energy ultraviolet radiation coming from the objects.

Mystery Objects

Currently, the team cannot effectively determine what these objects are, but they do have some suspects, including black holes, neutron stars, or white dwarves pulling material from a companion. Such material would heat as it fell into one of the three suggested objects, theoretically producing the observed X-rays. While these types of binary systems have all been observed previously, this combination of ultraviolet radiation and low-energy X-rays hasn’t been associated with them.

Because the researchers found so many of these objects in just six galaxies, they suggest many more of these likely binary systems remain undiscovered across the universe. 

These objects were not previously identified for two reasons. The more obvious is how faint their X-ray signature is, which requires extremely sensitive equipment to detect. The other is that helium and hydrogen gas between stars absorbs the stronger ultraviolet radiation, obscuring these otherwise brilliant signals.

“By combing through the Chandra archive, we were able to eliminate what used to be a blind spot for telescopes,” said co-author Rosanne Di Stefano, Senior Astrophysicist with the Center for Astrophysics, Harvard & Smithsonian. “That’s how we found what appears to be a new class of cosmic objects with remarkable qualities.”

What Did Chandra See?

“These clandestine X-ray sources are actually among the most energetic objects in galaxies, and they could be solving two cosmic mysteries at once,” said Muhibullah.

One of the mysteries this may solve ties to the rate of universal expansion itself. Type Ia supernova observations have provided astrophysicists with essential data indicating that the universal expansion is accelerating. Although they suggest these supernovae likely come from white dwarf binary systems, astronomers have never observed a star turning into one to confirm the hypothesis.

“If we could find a way to spot these Type Ia supernova explosions before they go off, that would be really important,” said co-author Jimmy Irwin, also of the University of Alabama. “Right now, we study them after they’ve exploded, and astronomers have struggled to understand what is actually ignited.”

The other mystery is what removes electrons from the free-floating gas between some stars, which could have major ramifications for star formation and galactic life cycles. Hot, massive stars were previously identified as likely partially responsible, but they couldn’t account for the full extent by themselves. The research team says hyper-soft X-rays and intense ultraviolet radiation could be the missing culprit. 

Only continued observation and research can provide a definitive answer on the mystery objects that Chandra observed.

The paper, “Hypersoft X-Ray Sources as a Low-Energy Class of Luminous Cosmic Emitters,” appeared in Nature Astronomy on September 9, 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.

Stanford University scientists say experiments on ancient Chinese stone tools, including 15,000-year-old hand axes, have solved a longstanding mystery about the critical technological transition from rudimentary hand tools to more versatile ground-edged tools, suggesting these new technologies enabled uses beyond food harvesting.

The research team behind the new analysis said the discovery of ground-edged sickles and knives in Neolithic North China, likely used for fiber production and harvesting, combined with their replica-based experiments, highlights the growing technological capabilities of the transition between Paleolithic and Neolithic peoples.

“The combined experimental and archaeological evidence from the site of Peiligang indicates that the emergence of ground-edged tools marked a significant step in technological specialization from the Late Pleistocene to the Early Holocene,” the researchers write in a paper detailing the work.

Mysterious Technological Transition Hidden in 15,000-Year-Old Stone Tools

According to lead author Ran Chen and colleagues, archaeologists widely regard ground-edged cutting tools like the modern sickle as “technological hallmarks of early agriculture in North China.” However, they note, the functional foundations of this advanced toolmaking capability “remain insuf­ficiently tested.”

The research team also noted that most analyses of the transition from the Upper Paleolithic to the Early Neolithic (ca. 15,000–8,000 BP) in ancient China have viewed tools through “the lens of food production.”

“Within this framework, cutting tools, including early flakes and blades and later ground-edged sickles and knives, are often interpreted primarily as implements for harvesting cereals through cutting stems and leaves,” they explained.

The researchers said these earlier findings made them wonder whether this “food-focused perspective” could have led researchers to miss the broader range of plant resource exploitation possibilities in some of the 15,000-year-old stone tools previously discovered, prompting their replica-based experiments.

“The development of stone tool technology in North China provides a framework for reassessing this long-term relationship between plant use and technological change,” they explained.

Experiments Reveal Ground-Edged Tools Were Multifunctional Implements

To test their hypothesis, Chen and colleagues analyzed 140 stone artifacts previously collected from the Peiligang site in Henan Province, China. This included some 15,000-year-old Upper Paleolithic flaked stone tools and several more advanced Early Neolithic flaked and ground-edged stone tools.

Rather than test irreplaceable artifacts, the study authors created realistic experimental replicas.

Testing the effectiveness of the oldest, most rudimentary stone flake designs and the more technologically advanced ground-edged tools for harvesting seed-bearing grasses, the researchers found little measurable advantage between the two designs.

However, when the researchers compared the 15,000-year-old stone flake tools against ground-edged tools made thousands of years later, they found the more technologically advanced tools were “significantly more efficient at cutting thick-stemmed weeds and fiber-yielding plants.”

“Upper Paleolithic flaked tools were multifunctional implements used for processing diverse plant and animal materials, and Early Neolithic flakes continued to serve similarly flexible roles,” the study authors explain. “In contrast, Early Neolithic ground- edged tools show marked specialization in plant- related tasks.”

More Advanced Tools Emerged Through Broader Functional Demands

When discussing the experimental results, the team noted that their findings were supported by microfiber and starch residues found on some of the ancient tools, suggesting that “ground- edged sickles and knives were used not only for plant foods but also for harvesting and processing fibrous plants.”

“These findings indicate that ground- edged cutting tools emerged through broader functional demands, including fiber production, and potentially vegetation clearance, rather than cereal harvesting alone,” they explained.

Beyond the food-harvesting uses of ground-edged tools, Chen and colleagues said their identification of non-food plant labor like fiber production as an important driver of technological evolution and specialization “reframes the emergence of ground- edged tools as part of a broader technological and economic reorganization in early Holocene East Asia.”

“These findings identify nonfood plant work as an important contributor to the adoption of ground-edged cutting tools and show that tools conventionally linked to early agriculture were shaped by broader demands than food production alone,” they explained.

Finally, the study authors suggested that their analysis of 15,000-year-old Chinese stone tools could “invite renewed attention” to ancient fiber-based economies and nonfood plant use during forager–farmer transitions and in early farming societies beyond China.

The study “Plant fiber exploitation contributed to the emergence of ground-edged cutting tools in North China” was published in Proceedings of the National Academy of Sciences. 

Christopher Plain has spent the last six years as Associate News Editor and Head Science Reporter at The Debrief. Follow and connect with him on X, learn about his novels at plainfiction.com, or email him at christopher@thedebrief.org.

Long before pottery became a common art form, the southern Levant underwent major environmental changes that stripped vegetation from hillsides and caused large amounts of clay-rich soil to accumulate in the valleys.

Now, a new study led by Amos Frumkin at the Hebrew University of Jerusalem suggests this process may have exposed Neolithic communities to the effects of intense fire on clay. Frumkin refers to this as the natural kiln hypothesis.

The study, published in Geomorphology, examined evidence from ancient sediments, cave deposits, and charcoal remains and identified two separate periods when wildfire and erosion impacted the area.

The Hills That Burned Twice

The two periods are separated by more than 100,000 years; the first of them was the last interglacial, lasting from about 129,000 to 116,000 years ago. The second was the early Holocene, which lasted from about 11,000 to 7,000 years ago, a period that corresponds with the establishment of farming communities in the region. The most intense burning occurred between 9,500 and 8,200 years ago.

Both periods left similar evidence. Small charcoal particles in ancient lake sediments indicate periods of increased burning. Chemical signatures in cave formations show the loss of vegetation and soil that followed. Frumkin notes that the scale and timing of the fires point toward climatic causes rather than increased human use of fire, although people in the region already used fire on a limited scale.

A Natural Kiln

Once the vegetation disappeared, the hillsides could no longer retain soil when it rained. The terra rossa clay, therefore, washed down the slopes and collected in low-lying areas like the Jordan and Dead Sea valleys, building up in thick layers. Since this redeposited clay was very fertile, Neolithic settlements tended to cluster in these areas.

Pottery appeared in the region during the same time period. Earlier petrographic studies show that local redeposited terra rossa clay provided the material for Yarmukian pottery from the Jordan Valley, the same material that erosion deposited in Frumkin’s study.

“A wildfire is normally seen only as a catastrophe, but environmental disruption can also expose people to new materials and new possibilities,” said Frumkin. “Neolithic communities in the Jordan Valley may have watched fire transform the clay beneath and around their settlements and realized that this process could be reproduced deliberately. If so, one of humanity’s most important technologies may have emerged partly from people learning to imitate what they had already seen nature do.”

The 120,000-Year Comparison

This earlier period can serve as a comparison for this hypothesis. Vegetation also declined, and clay deposited heavily during the last interglacial period; however, pottery did not appear after that event. Frumkin sees this as an example of a natural limitation because the required materials were available 120,000 years earlier, but there were no settled, agricultural societies to identify and replicate the process.

The comparison suggests that environmental conditions alone were not enough to produce pottery. The innovation may have emerged when these conditions intersected with a society capable of recognizing the opportunity and reproducing what it observed.

Frumkin stresses that the hypothesis is still speculative. Although the fires, the clay deposits, and the earliest pottery all come from roughly the same period, current dating techniques cannot establish the exact order of events. Further excavations might search for fire-baked clay beneath the oldest pottery layers and test whether wildfires in the Jordan Valley reached the temperatures needed to harden clay. Finding any pottery that clearly predates the major fire episode would challenge this hypothesis.

Austin Burgess is a writer and researcher with a background in sales, marketing, and data analytics. He holds an MBA, a Bachelor of Science in Business Administration, and a data analytics certification. His work focuses on breaking scientific developments, with an emphasis on emerging biology, cognitive neuroscience, and archaeological discoveries.

Mercury has been slowly shrinking for billions of years. But scientists studying the smallest planet in the solar system may have overlooked just how dramatic that transformation has been because some of the evidence has literally been buried.

A new study suggests Mercury’s battered, crater-covered surface has concealed a significant fraction of the faults created as the planet cooled and contracted. After accounting for those hidden geological structures, researchers estimate Mercury may have shrunk by as much as 7.2 miles (11.6 kilometers) in radius—up to 30% more than previous estimates based on the same tectonic record.

The findings could alter models of how Mercury’s interior evolved and raise an interesting possibility beyond the planet itself. For instance, scientists may also be underestimating how much other rocky worlds, particularly the Moon, have contracted.

“Combined with the contractional strain map from Broquet and Andrews-Hanna (2026a), we show that radial contraction may have been underestimated by 10%–30%,” researchers write. “Our radial contraction correction should be considered as a lower bound.”

In the study published in Geophysical Research Letters, researchers led by Dr. Gaku Nishiyama of the German Aerospace Center (DLR) examined a longstanding mystery in Mercury’s geology.

As a rocky planet loses heat, its interior contracts. Much like the skin of a drying fruit, the planet’s rigid exterior must accommodate a shrinking interior, producing faults and enormous cliff-like features known as lobate scarps, along with wrinkle ridges and other shortening structures.

Scientists therefore use the crustal shortening recorded by these structures as a geological ruler to determine how much Mercury has contracted.

The problem is that those structures aren’t distributed across Mercury the way scientists might expect.

If cooling caused the entire planet to contract, the resulting deformation should be comparatively widespread. Instead, previous mapping has revealed regions filled with large scarps alongside enormous areas where surprisingly few contractional structures have been identified.

Dr. Nishiyama and his colleagues investigated whether at least part of that discrepancy could be an illusion created by Mercury’s extraordinarily battered surface.

Mercury’s Craters May Be Hiding Its Wrinkles

The researchers constructed a global map of Mercury’s surface roughness using topographic measurements acquired from NASA’s MESSENGER mission and a global digital terrain model produced from spacecraft imagery.

They then compared that roughness with previously cataloged tectonic structures.

Findings showed that fault scarps and other shortening structures were preferentially identified in smoother terrain, while rougher regions contained substantially fewer detectable structures. The relationship remained apparent across geographic scales extending to roughly 93 miles or about 150 kilometers.

That is counterintuitive because tectonic ridges themselves create topographic roughness. If roughness and plate movements were unrelated, areas with scarps might be expected to be slightly rougher than the surrounding terrain.

Instead, the researchers found the opposite.

One explanation is evident around relatively young impact craters such as Rachmaninoff. Large impacts blasted enormous quantities of debris across the surrounding landscape, producing thick blankets of material and secondary craters. In some locations, long tectonic structures appear to lose relief as they approach these deposits—consistent with the older structures being progressively hidden under impact material.

Other faults may still exist but become difficult to recognize against heavily cratered terrain. Once the surrounding topography becomes rough enough, a weathered ridge only a little higher than the background landscape can effectively disappear into the geological noise.

There is also a third possibility.

Heavily cratered regions may contain thick, porous layers of broken rock called regolith. During planetary contraction, some deformation could be absorbed as pores collapse rather than producing large faults visible from orbit. Alternatively, deformation could create faults too small for current observations to resolve. The researchers say available evidence cannot yet rule out that possibility.

Mercury Could Have Shrunk by More Than 7 Miles

Whatever mechanism is responsible, Dr. Nishiyama and his colleagues argue the relationship creates a systematic bias, where scientists see more evidence of contraction where Mercury’s surface makes that evidence easier to preserve and identify.

The team developed a correction using comparatively smooth regions, where tectonic structures appear less affected by this bias.

Applied to an earlier global estimate of 5.2 miles (8.3 kilometers) of radial contraction, the correction increased Mercury’s estimated shrinkage to roughly 7.2 miles or about 11.6 kilometers.

Depending on which tectonic structures are included, the researchers estimate surface roughness could have caused previous calculations to underestimate Mercury’s contraction by roughly 10% to 30%. They also caution that their corrected figure may itself represent a lower limit.

Ultimately, Mercury’s shrinking surface effectively records what has happened deep inside the planet.

The amount of contraction constrains how quickly Mercury lost heat, the thickness of its insulating regolith, the abundance of heat-producing elements, and even the composition and freezing history of its enormous metallic core. The revised estimate, for example, favors models involving a thinner regolith and lower sulfur content in Mercury’s core than some previous estimates.

Scientists may soon get a much sharper look.

The ESA-JAXA BepiColombo mission’s laser altimeter will eventually measure Mercury’s topography at scales as small as about 330 feet or 100 meters, possibly revealing geological relationships that MESSENGER could not resolve.

And Mercury may not be the only world whose geological record has been hiding in plain sight.

The Moon’s highlands are even rougher than Mercury’s cratered plains—by roughly 40% at the little-over 6-mile (10-kilometer) scale examined by the researchers. Yet evidence suggests the Moon contracted less than some thermal models estimate. If rough terrain similarly hides lunar faults, part of that difference might reflect structures scientists haven’t been able to see.

In other words, Mercury’s missing wrinkles may expose a wider problem in planetary geoscience. The more battered an ancient world becomes, the more effectively its later surface can erase the visible record of what happened before it.

“Investigating roughness alongside tectonic landforms may therefore refine our understanding of the lunar thermal evolution as well,” researchers conclude. “Mars could also be subject to this roughness effect, while topographic smoothing due to fluvial and aeolian processes may introduce more complex correlation between surface roughness and shortening structures.”

Study: Nishiyama, G., Broquet, A., Tosi, N., Preusker, F., Stark, A., Hussmann, H., & Hauber, E. “Underestimation of Planetary Contraction Due to Obscuration by Surface Roughness: The Case of Mercury.” Geophysical Research Letters 53, (2026). 

Tim McMillan is a retired law enforcement executive, investigative reporter and co-founder of The Debrief. His writing typically focuses on defense, national security, the Intelligence Community and topics related to psychology. You can follow Tim on Twitter: @LtTimMcMillan.  Tim can be reached by email: tim@thedebrief.org or through encrypted email: LtTimMcMillan@protonmail.com 

The first Denisovan radius ever discovered is offering scientists a rare new glimpse into one of humanity’s most mysterious ancient relatives, whose scarce fossil remains have left much of their story unknown.

In a recent paper published in Nature, the team described these unique remains, discovered in the Bianfu Cave in Southwest China, an important Paleolithic site.

While Denisovans have been discovered throughout Asia, this part of China has been a major gap in the record. Therefore, this site provides important information about what a complete Denisovan body would have been like, as well as intricate details about regional skull variations among these archaic hominins.

A New Technique

The researchers behind the new study developed a novel technique to make the most of the more than 60,000 bone fragments recovered from Bianfu Cave. While Zooarchaeology by Mass Spectrometry (ZooMS) has become an important tool in working with hominin fossils, using it on a find of this scale would be inefficient and expensive. 

Therefore, the team developed a morphological pre-screening and ZooMS identification technique, which greatly increased their efficiency in recovering hominin fragments from the site and could be applied to other Paleolithic sites in the future.

A total of 22 likely hominin bone fragments were identified in the pre-screening process, from which two parietal bone fragments and one proximal radial fragment were confirmed by ZooMS as belonging to hominins.

Denisovan Remains Uncovered

Two of these hominin remains were excavated from the same layer, dated between 148,000 and 143,000 years old, which also held four hominin teeth. The research team further examined two of those teeth, and a detailed analysis indicated they belonged to males. The third specimen was even older, from a layer dated between 167,000 and 150,00 years old.

By screening the fragments for amino acids, the team identified a variant of COL1A2 R996K unique to Denisovans as present, confirming the species identity of the remains. Other intriguing amino acids in the fragments included one shared by Denisovans, Neanderthals, and modern humans, as well as one that marks them as distinct from Homo erectus, which also occupied East Asia.

As the team closely examined the morphology of skulls excavated from Bianfu Cave, they identified a cranial thickness pattern remarkably similar to H. heidelbergensis and East Asian late Middle Pleistocene archaic Homo.

A New Understanding of Denisovans

After analyzing the morphology of the first Denisovan radius ever discovered, the researchers suggest it was likely oriented similarly to a Neanderthal’s, but with a shape and cross-sectional geometry closer to that found in modern humans.

The importance of the find lies not only in being the first example of its kind, but also in indicating biochemical demands and adaptations distinct from both Neanderthals and modern humans.

Besides Denisova Cave in Siberia, from which Denisovans draw their name, the team believes Bianfu Cave may hold the largest fossil record for the species. This could provide researchers with crucial new data, over a decade into the quest to understand the Denisovan species of Asia.

Based on the age of the layers in which the remains were found, the team says the Yunnan-Guizhou Plateau region, where the cave resides, may have been an ideal homing habitat at the time. The Earth would have been in a glacial period, during which the area’s relatively warm climate would have aided hominin survival.

The paper, “Ancient Proteins Identify Various Denisovan Remains from Southwest China,” appeared in Nature on September 9, 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 investigating a 66-million-year-old mystery have revealed that a bird feather embedded in fossilized dinosaur excrement suggests that the ancestors of modern birds who survived the dinosaur-killing asteroid that also wiped out all other ancient bird species benefited from the waterproofing properties of their feathers.

The newly analyzed bird feather fossil that provided the missing clues comes from an extinct bird group called Hesperornithiforms and not from the ancestor of modern birds, Neornithes.

However, the team said subtle differences between the species suggest previous theories crediting adaptation to water diving as the key to Neornithes’ survival were likely on the right track.

Survival of Modern Bird Ancestors Posed a 66-Million-Year-Old Mystery

When a huge piece of space rock slammed into Earth, killing off virtually all dinosaur species save the ancestors of modern birds, the event also left behind a 66-million-year-old mystery. How did these ancient avians survive this apocalyptic event, resulting in every bird species we see today?

Jingmai O’Connor, the associate curator of fossil reptiles at the Field Museum in Chicago, said her career has been spent analyzing fossils to try to answer this single, critical question. However, unlike the new poop-encased bird feathers, most were not so ‘naturally’ protected from the ravages of time.

“It’s such a beautiful, well-preserved feather, from such an unexpected source, and it’s exciting that it could help us answer this huge question in paleontology,” explained the lead author of a study detailing the new analysis. “As far as I know, no one has ever thought to look for feathers or to study feathers in coprolites, so this project was really exciting.”

Dinosaur Dropping Provided Effective Preservation Medium

Researchers discovered the ancient bird feather in 2016 in Montana. Although she initially suspected it could be a coprolite rock (fossilized feces), O’Connor said she couldn’t confirm the theory for a decade.

The situation changed when O’Connor and Nate Carroll, a co-author of the paper and paleontologist at the Carter County Museum in Ekalaka, Montana, gained access to the micro-CT scanner at USC’s medical campus in Los Angeles, California. According to O’Connor, that’s when “the full feathery fabric of this fossil feces” started to finally reveal itself.

“Every hour processing the data revealed another feather, another scale, another bone—in stunning 3D,” Carrol also recalled.

Along with multiple feathers and tiny fish scales, the ancient dinosaur poop, which may have come from a Tyrannosaurus Rex, also contained legs from a hesperonithiform bird.

O’Connor said hesperonithiforms were ancient aquatic birds with similarities to modern loons. Critically, these cousins of the modern bird ancestor group had evolved specialized feet to hunt for fish by diving deep into the water.

“The feathers showed adaptations for being underwater that we see in living aquatic birds,” O’Connor explained.

Notably, the team said this evolution likely cost ancient hesperonithiforms like the one that was consumed by a dinosaur the ability to fly.

Connection to Modern Birds Offers a Solution 

Although the bird group represented by the fossilized feather did not survive the dinosaur-killing asteroid, its connection to the ancestor of modern birds appears to support a previously proposed theory that adaptation to water may have helped Neornithes survive. O’Connor said she thinks that small differences in the feathers of the two ancient bird species hold the answer to a 66-million-year-old mystery.

“We think the types of feathers that these birds had, and/or the way they molted those feathers, may have been one of the underlying causes of the selectivity of the end-Cretaceous mass extinction,” the researcher explained, adding that this is “essentially why some birds died out and why others survived.”

Specifically, O’Connor pointed to the “smaller, fuzzy, primitive body feathers” found on the extinct bird “that we associate with dinosaurs and enantiornithines” alongside more modern-looking waterproof adaptations.

The team said that these evolutionary relics suggest that hesperornithiforms like the one that left behind its feathers were an evolutionary bridge between older bird groups and the Neornithes that survived the cosmic collision. Even more critically, the team said these earlier feather structures may not have retained heat as effectively as Neornithes feathers, allowing one species to survive the asteroid and another to die in the extreme cold that followed.

“The hesperornithiforms retain primitive feather types that may not have been as efficient for insulation as modern plumaceous feathers, and that could explain why they went extinct along with the enantiornithines,” O’Connor explained.

The study “Bird feathers from a Late Cretaceous coprolite” was published in Current Biology. 

Christopher Plain has spent the last six years as Associate News Editor and Head Science Reporter at The Debrief. Follow and connect with him on X, learn about his novels at plainfiction.com, or email him at christopher@thedebrief.org.

What may be the earliest known evidence of human drug use suggests that it occurred 25,000 years ago, according to findings by archaeologists that push back on earlier estimates by over 10,000 years.

In a recent paper published in Science Advances, an international team of researchers led by Professor Adam Brumm from Griffith University’s Australian Research Center for Human Evolution (ARCHE) discovered betel nut residue on ancient teeth in Indonesia. 

Betel nuts are an addictive stimulant popular throughout the Asia-Pacific region, which researchers previously believed only came into use about 3,500 years ago. Globally, archaeologists had believed psychoactive drugs had been tied to the rise of agriculture.

Betel Nuts: the First Drugs

Archaeologists typically point to Israel’s brewing of fermented alcoholic drinks, such as those made of barley, as the earliest use of psychoactive drugs, roughly 13,000 years ago.

“However, this theory fails to account for the possibility that very ancient drug-taking lies at the roots of our most commonly used psychoactive substances,” Professor Brumm said.

Betel nuts are only regionally popular in India and the South Pacific, but their use is almost ubiquitous among the 10% of the world’s population that lives there. The psychoactive effects of the stimulant include enhanced alertness and mild euphoria.

The betel nut is the seed of the Areca catechu palm. Locals burn its shell, then grind it into a fine powder and mix it with slaked lime, another powder made from quicklime and water. They mix these powders with other minor ingredients, wrap them in a betel leaf, and chew them to produce a mild altered state.

Research on the drug suggests that this processing releases Arecoline, the neuroactive alkaloid present in the betel nut, in a more bioavailable form. Modern usage is linked to cancer, gum disease, and tooth decay, making it a significant public health problem in regions where it is used.

A Prehistory of Betel Nut Usage Uncovered

The seeds were rarely preserved in archeological sites, creating a great deal of uncertainty about the drug’s early history.

Human remains used in the study came from Sulawesi, one of the islands that make up Indonesia. There, archeologists uncovered two hunter-gatherer skeletons: one dating to 7,600 to 6,300 years old and the other 25,000 to 16,000 years old.

These skeletons carried an unusual signal, which the team interpreted as related to ancient drug use. Their teeth had deep, rounded grooves that the researchers believe developed from the habit of sucking on whole betel nuts. Biochemical analysis further supported this interpretation by identifying Arecoline in the remains’ dental tissues.

“But our team conducted experiments in which we soaked betel nuts in artificial saliva and tested the resultant broths against a panel of cloned human receptors expressed in frog egg cells, including specialized proteins that act as molecular switches, regulating neural activity,” said lead author Professor Adam Brumm. “This showed that just sucking on intact betel nuts will release Arecoline in sufficient amounts to have a physiological effect, altering brain function.”

Rethinking Prehistory

This crude attempt to use the betel nuts as a drug likely produced a milder high, while also promoting periodontal disease. Given the poor state of the teeth in human remains previously found on the island, the team believes the betel nuts may have initially been used as a toothache remedy, though it was a poor choice for that purpose.

“Over time, however, sucking these hard, abrasive seeds wore down the foragers’ teeth so badly that in some cases the inner pulp chamber became completely exposed – this would have been extremely painful, caused difficulty eating, and greatly increased the rate of chronic tooth infection,” Professor Brumm said. “So while this habit may have been a remedy for toothache, years of prolonged nut-sucking eventually caused much worse dental health problems, creating a cycle of continued habitual use.”

Pushing back the use of these psychoactive substances so far significantly rewrites our understanding of human drug history.

“Emerging by up to 25,000 years ago in Sulawesi, thus long preceding the onset of agriculture, betel nut-sucking may be the earliest evidence for drug use anywhere in the world,” Professor Brumm concluded. “By identifying the ancient practice underlying betel-nut chewing as we know it, the study implies that some modern drug-taking behaviors are deeply rooted in forager traditions.”

The paper, “Betel Nut Sucking is the Earliest Recorded Evidence for the Habitual Use of a Neuroactive Plant Drug,” appeared in Science Advances on September 9, 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.

Defense aviation company Hermeus has announced the development of Ramjet-X, its next-generation ramjet propulsion test vehicle capable of carrying test payloads to high Mach speeds.

The company said Ramjet-X, designed to launch mid-flight from a carrier aircraft, offers the key advantages of competitive high-Mach test platforms while keeping costs low enough for a wider range of mission profiles.

Pre-flight testing of Ramjet-X is already underway, with its first official prototype test flights expected in 2027.

Ramjet-X Will Launch Mid-Flight from Quarterhorse

Most conventional jet engines can’t achieve supersonic speeds without dumping raw fuel into an afterburner and literally rocketing past the sound barrier. To travel at high Mach speeds without relying on rocket-style propulsion, engineers have turned to ramjet engines.

While ramjets are effective, they rely on the high-speed influx of air to operate. This limitation means aircraft equipped with this type of propulsion must be propelled to higher speeds by another craft or booster rocket before they can engage.

In an email to The Debrief, a Hermeus spokesperson explained that current options often rely on “large and expensive” boosters that are discarded after each test. Conversely, Ramjet-X relies on the company’s reusable aircraft to reach launch velocity.

“Ramjet-X is designed to be carried by Quarterhorse, which provides the speed and altitude required for deployment,” the company told The Debrief.

The company could not disclose what speed Quarterhorse must achieve before it can launch Ramjet-X. However, the spokesperson did note that the launch craft is designed to return to home base for future missions.

When asked about Ramjet-X’s specific operating velocity once it disengages from Quarterhorse and engages its ramjet propulsion system, the company could only say the vehicle will operate at “High-Mach speeds.”

Conventional ramjets use a combination of high-velocity air and fuel to achieve extreme velocities. Hermeus said they cannot disclose specifics about Rocket-X’s fuel requirements.

Mission Profiles and Repeatable Architecture

Because of the sensitive nature of potential future missions, Hermeus was cautious about sharing specifics of any planned missions. The company also couldn’t provide technical details on what a typical mission profile might look like.

However, a Hermeus spokesperson told The Debrief, the vehicle’s architecture “allows customers and partners to integrate payloads, sensors, communications and computer systems, autonomy, material samples, propulsion technologies, and other experimental hardware and software onto Ramjet-X for testing in representative sustained high-Mach conditions.”

Hermeus also highlighted the potential cost savings of a “repeatable platform, launch architecture, and flight-test infrastructure,” designed to dramatically lower costs without sacrificing versatility or reliability.

“Instead of relying on a large dedicated expendable booster to accelerate the test vehicle into its ramjet operating regime, the launch aircraft provides much of that energy and then returns to fly again,” the company told The Debrief. “This architecture allows Hermeus to fly more by reducing the cost of expendable launch hardware.”

“High-speed flight testing is extremely expensive, and you don’t get many shots at it,” Hermeus CEO Zach Shore explained.

“Another Order of Magnitude Reduction”

Hermeus said specific unit costs are not currently available. However, they said a projected cost per minute of high-Mach test time “is in the low $100k’s per minute.” For comparison, the company highlighted the historic and current costs of high-Mach flight testing.

“Most of the below comparisons are rocket-based but will give you an idea how costly high-Mach tests are and why Ramjet-X will fundamentally change the equation,” Hermeus told The Debrief.

Older examples include NASA’s X-43, which achieved around 21 seconds of high-Mach flight, and the Air Force’s X-51, which achieved around 350 seconds. Hermeus said both multi-year efforts cost around $450 million each in today’s dollars.

Current options include rocket-powered test flights aboard Rocket Lab’s HASTE, which Hermeus said run $10-20 million each, “not including the expendable cruise or glide vehicles.” The company also pointed to Stratolaunch Talon-A missions.

“Even though fully reusable, (they) are $10-12m per flight for a few min of on-condition time,” the company told The Debrief.

Conversely, Hermeus said its current projections of less than a million per minute offer potential customers “another order of magnitude reduction in the problem that matters most.”

“Ramjet-X is being designed around simplified manufacturing, rapid production, and expendability in meaningful quantities rather than the traditional model of building a small number of highly bespoke high-speed test articles as was done in other high-speed airbreathing flight test programs like X-43 and X-51,” the company told The Debrief. 

Development of Ramjet-X is already well underway

When detailing the newly announced Ramjet-X’s benefits, Shore noted that their system gives them a way to place new systems into sustained high-Mach environments “without building an expensive one-off test program every time.”

“Bringing speed, sustained flight, and scalability all into one system lowers the barriers to gathering extremely valuable data from these conditions and accelerates programs for both us and our customers,” the Hermeus CEO explained.

When announcing Ramjet-X, Hermeus said the vehicle’s ramjet engine is already undergoing extensive testing at its Florida-based HEAT facility. Future tests will occur at the company’s California headquarters, with the first flight tests planned for 2027. 

Christopher Plain has spent the last six years as Associate News Editor and Head Science Reporter at The Debrief. Follow and connect with him on X, learn about his novels at plainfiction.com, or email him at christopher@thedebrief.org.

A University of Cambridge-led research team has announced the discovery of a 560-million-year-old animal fossil preserved in three dimensions (3D) in a sheep field in the Norwegian Arctic.

The exceptionally rare Ediacaran Period fossil is the first of its kind in Europe in decades and gives scientists a unique window into a period of Earth’s history when the first complex life forms began to appear.

The discovery suggests the site could hide an entire lost ancient ecosystem that has remained hidden for hundreds of millions of years.

3D Fossil of 560-Million-Year-Old Lifeform ‘Unlike Animal Life Today’

When announcing the historic discovery, the Cambridge-led team noted that the fossil, called a Charnia, resembles a fern more than any animal life we would likely recognize today.

For example, Charnia has none of the organs we typically associate with animals. The archaic life form also lacks a mouth or visible means of locomotion. The closest modern comparison would be a sedentary jellyfish.

While previous efforts have identified ancient animal-life fossils from this period, the team noted that most are found as “flat impressions.” As a result, Professor Neil Davies from Cambridge’s Department of Earth Sciences said that many fossils from this period “occur as impressions where they’ve been squashed down under layers of rock,” like a flower pressed into a book.

“As a fossil record, the Ediacaran has several things working against it, primarily that most organisms were soft-bodied and skeletons hadn’t evolved yet, so that they are harder to preserve,” the team member and co-author of the study detailing the research explained.

Dr Veema agreed, while noting the difficulty in finding such rare specimens.

“Fossils need to be embedded within sedimentary rocks to be found, so if the rocks themselves are less common, then that makes the fossils harder to find,” the researcher explained. “Most Ediacaran fossils come from just a handful of locations, which makes it exciting to find them somewhere new.”

Fortunately, the newly identified 560-million-year-old life form was preserved in all three dimensions. The team said that discovering an ancient life form preserved in 3D is incredibly rare, particularly for soft-bodied organisms like Charnia. Finding one from this extremely ancient time, when animal life first began to appear, is even more unlikely, making the discovery unusually rare.

Well-Preserved Charnia Reveals Previously Unknown Details

560 million years ago, when this Charnia was still alive, evidence suggests that it was buried during an ancient underwater avalanche. This sudden submergence also filled the animal’s body with sediment. The researchers said these events caused the fossil to become preserved in 3D

For example, the research team identified small ridges along the animal’s branches. Called keels, these extremely subtle features had never been detected in other, flatter Charnia fossils.

Dr Yorick Veenma, from Cambridge’s Department of Earth Sciences and the lead author of the study detailing the team’s discovery, said finding a 3D fossil from this archaic time has provided them with an entirely new perspective.

“When you see the same species preserved in a different way, you start noticing properties you hadn’t seen before,” Dr. Veenma explained.

“There May Be a Whole Undiscovered Community of These Very Early Organisms”

Although scientists have found a few fossils from this period, they are often from the same handful of sites. However, this is the first time one has been found in Norway. Dr. Veema said this shows that discoveries can be made “in less familiar places.”

The researchers also successfully identified other components of the ancient ecosystem that this Charnia fossil called home. Future efforts may reveal that it was one small part of a larger, ‘lost’ ancient ecosystem supporting a variety of complex life forms.

“There may be a whole undiscovered community of these very early organisms preserved up there,” Davies explained. “Weird little umbrella-shaped blobs, things that don’t fit with what people know from elsewhere.”

“There are a whole host of different things that were not known before,” the researcher added.

The study “Charnia and other late Ediacaran macrofossils preserved in turbiditic deposits of the Indreelva Member (Finnmark, Norway)” was published in Paleontology.

Christopher Plain has spent the last six years as Associate News Editor and Head Science Reporter at The Debrief. Follow and connect with him on X, learn about his novels at plainfiction.com, or email him at christopher@thedebrief.org.