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“A Major Milestone in the Search for Life on Other Planets”: First Ever Detection of an Atmosphere Around an Earth-Like, Habitable Zone Rocky Exoplanet

An international research team led by Harvard scientists has announced the first-ever detection of an atmosphere on an Earth-like rocky exoplanet, LHS 1140 b, orbiting within its star’s habitable zone, only 48 light-years away.

The researchers behind the historic discovery, which they are calling “a major milestone in the search for life on other planets,” said the detection of an atmosphere on an Earth-like rocky exoplanet offers the strongest evidence to date that worlds with similar compositions and temperatures to Earth that are also capable of supporting life could exist beyond our solar system.

Models Predicted First Earth-like Rocky Habitable Zone Exoplanet Atmosphere

In a statement announcing the detection of an atmosphere around a habitable-zone rocky exoplanet, the discovery was motivated by theoretical predictions suggesting that LHS 1140 b may contain an atmosphere. The planet was even more tantalizing because its orbit around its host red dwarf star allows for liquid water on its surface, a key ingredient for life as we know it.

Although thousands of exoplanets have been confirmed since 1995, including habitable-zone rocky worlds similar in size and composition to Earth, the team notes that determining whether any of these potential Earth analogs maintain an atmosphere. Like water, an atmosphere is considered a likely necessity for life to emerge.

“An atmosphere is essential for a planet to support life as we know it,” explained Collin Cherubim, the lead author of a study detailing the findings, who recently earned his Ph.D. in Earth and Planetary Sciences from Harvard University.

Robin Wordsworth, the Gordon McKay Professor of Environmental Science and Engineering and Professor of Earth and Planetary Sciences at Harvard, said that as recently as twenty years ago, astronomers still didn’t know if other, terrestrial-type planets “even existed.” However, he explained, they quickly found that this type of planet was common, including some orbiting within their star’s habitable zone.

“The next question was whether any of them had managed to keep an atmosphere,” the professor added.

Infrared Observations Confirm Historic First  

Before performing any direct observations, the team used computer models to predict what they might find on LHS 1140 b. As noted, those models predicted an upper atmosphere rich in helium. The models also suggested that the atmospheric helium was slowly escaping into space.

To test the model’s predictions, Cherubim and colleagues gained access to the Warm Infrared Echelle (WINERED) Spectrograph on the Magellan Observatory in Chile. The team noted that this powerful telescope allowed them to observe an alignment of LHS 1140 b and another planet transiting its star “on the same night.”

When analyzing the data, the team found that one of the planets appeared to lack any measurable atmosphere. However, as their models had predicted, helium was actively escaping from LHS 1140 b. The finding confirmed that this rocky exoplanet orbiting within its star’s habitable zone was actively maintaining an atmosphere.

David Charbonneau, the head of the Harvard Department of Astronomy and an astronomer at the Center for Astrophysics | Harvard & Smithsonian, and Cherubim’s co-advisor with Wordsworth, was initially skeptical because the entire concept was based on a mathematical prediction of a phenomenon astronomers had never witnessed directly. However, Professor Charbonneau ended up praising the student’s determination and follow-through, which led to the historic detection.

“Collin analyzed the planets we knew about and predicted that this one would have a helium atmosphere,” Charbonneau said. “Then he organized telescope time, got the data, and the detection was statistically rock solid.”

“Hopefully it’s just the First of Many More Observations to Come”

When discussing the implications of the findings, Cherubim noted that “this is the first time anyone has found an atmosphere on a rocky planet in the habitable zone of another star.” Professor Wordsworth agreed, once again noting that until now, planets in these categories with atmospheres had been purely theoretical.

“Now we know at least one has,” the professor said.

The data also suggest that LHS 1140 b’s atmosphere has likely survived for more than three billion years, roughly three-quarters of Earth’s existence. This durability makes LHS 1140 b an excellent candidate for future exoplanet atmosphere studies.

More broadly, the team said that using ground-based observatories to search for escaping gases, such as the helium detected leaving LHS 1140 b, “may become an important tool for studying atmospheres on rocky exoplanets.” They also note the potential value of atmospheric detection for astrobiologists searching for signs of life in the cosmos.

As for Cherubim, he plans on following up his historic discovery with a more detailed analysis of the planet’s atmospheric composition. He also said he would like to investigate the possible presence of surface oceans or other planetary characteristics typically associated with habitability and life. The entire team also said they would like to use Cherubim’s model to search for similar Earth-like, habitable-zone rocky exoplanets.

“This has been a model validation, and hopefully it’s just the first of many more observations to come,” Cherubim said.

The study, “Helium escaping from the atmosphere of a nearby rocky exoplanet orbiting in a habitable zone,” was published in Science.

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.

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“This Upper Limit is an Illusion”: NASA Study Warns There May Be “No Limit” to How Solar Storms Impact Earth 

Our modern society depends heavily on communications and power networks that are highly susceptible to interference from solar storms, making these volatile space weather events a paramount concern for scientists.

Now, it turns out there may be more to fear than previously realized. Scientists are discovering that there may be no ceiling to the devastating effects solar storms may have on Earth, overturning what little sense of security may exist as a mere mathematical anomaly.

In a recent paper published in Nature, a NASA-led team discovered that the potential impact of solar storms on our technological infrastructure could be substantially more severe than currently recognized.

Solar Storms Reconsidered

According to new research, any past limitations perceived regarding the impact of solar storms on our planet are purely an illusion, which arises from imprecise data collection.

Previous observations of electric currents in the Earth’s upper atmosphere during solar storm events suggested a ceiling to how far they could increase. Yet the new paper claims that uncertainties in solar wind data are falsely giving rise to this idea.

The researchers say that the distance of the spacecraft taking solar wind measurements is the issue. Those spacecraft are millions of miles closer to the Sun than the Earth is, meaning that by the time those winds reach Earth, they have weakened considerably. Additionally, instrument error and the effects of the local plasma and field conditions all come into play.

All this, the researchers say, creates a mismatch between the measured strength of the wind and its effects on our planet’s electrical currents.

Correcting For Distance

The new findings contain one significant difference from existing research: they relied on observation platforms much closer to Earth to collect data, which included spacecraft such as NASA’s MMS and THEMIS.

Launched in 2007, THEMIS consists of five satellites that target the Earth, rather than the Sun, to study our planet’s magnetosphere and auroras. MMS consists of four spacecraft that also study the Earth’s magnetosphere.

Existing charts show the impact of solar winds on Earth leveling off at a certain threshold, which scientists had believed was the maximum saturation possible. However, in new solar wind strength data collected much closer to Earth, more accurately reflecting power at the time of impact, this saturation point disappeared. Instead, this data revealed that there is no ceiling on how heavily solar storms can charge the Earth’s electrical currents.

Solar Storm Impacts

Another crucial element in the NASA-led research is the statistical concept of regression to the mean, which holds that extreme measurements often change as more data come in. In this case, as more data on solar storm impacts on Earth recorded from various distances were collected, the plating effect disappeared. The authors note that similar effects occur in other areas of research, such as climate studies and chronic medical pain.

These new findings present a major challenge to our understanding of space weather. Scientists will now need to conduct many further observations to determine if any such ceiling exists. The threat to our infrastructure may be severe, as satellite communication underpins our modern society, not to mention the power grid, which keeps our world running.

For now, NASA continues to monitor solar storms to prepare for their potentially dangerous effects on our infrastructure, and in light of the new research, the potential for future challenges ahead may be greater than previously realized.

The paper, “Regression to the Mean Can Explain Saturation of Geomagnetic Storms,” appeared in Nature on July 15, 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.

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Astronomers Uncovered a Hidden Bubble Inside the Orion Nebula

A key component of the Orion Nebula had escaped detection by astronomers until now, according to a new study in Astronomy & Astrophysics.

An international team led by Juan Diego Soler at the University of Vienna used two of the world’s most advanced radio telescopes to map neutral atomic hydrogen gas across the nebula’s outer shell at unprecedented resolution. The new maps provide a clearer view of the celestial feature, and reveal a previously uncatalogued second bubble—a shell with much less mass than earlier estimates—and a four-light-year filament of gas extending from the structure.

The Orion Nebula’s Miscalculated Bubble

Neutral hydrogen emits a faint radio signal at a wavelength of 21 centimeters, making it possible to trace otherwise invisible gas between the stars. Soler’s team solved this by combining data from the Karl G. Jansky Very Large Array in New Mexico and the FAST telescope in China. The VLA provided high resolution, while FAST picked up faint, widespread signals. Together, they produced the first detailed hydrogen map of the extended Orion Nebula, at the same scale as earlier ionized carbon maps.

Earlier calculations based on ionized carbon estimated that the front half of the shell was about 1,100 times the mass of our Sun. The hydrogen observations paint a different picture, suggesting the shell actually weighs in at closer to 100 solar masses. “Measuring mass is fundamental,” Soler said, “because it tells us about the efficiency of these newly formed stars shaping their environment with wind and radiation.”

A shell with only a tenth of the previously assumed mass significantly alters calculations of how efficiently newly formed stars shape their environment. The researchers note that molecular hydrogen, which is not detected in either the hydrogen or carbon data, may account for some of the missing mass.

A Second Bubble

The hydrogen maps also revealed an uneven distribution of gas, indicating a second, smaller cavity within the main shell. The team searched catalogs of known stars and young stellar objects in the region but found no candidate at the bubble’s center. The source responsible for creating the cavity may not be the type of object included in current catalogs.

Daniel Seifried at the University of Cologne, a co-author on the study, pointed to what that means for the models astronomers build to explain regions like this one. “These stunning observations serve as a reference for many modern astrophysical simulations investigating the evolution of gas and stars in the Milky Way. These are the kind of images that challenge the theoretical models and numerical simulations that we use to understand how massive stars affect their immediate surroundings.”

Previous models generally treated Orion’s shell as the product of a single expanding bubble. The discovery of a second cavity, with no obvious source at its center, instead suggests the nebula was shaped by multiple episodes of stellar feedback.

An Unexpected Filament

The new maps also uncovered a filament of hydrogen extending about four light-years from the shell’s western edge. Previous carbon-based observations saw only the base of this structure. The filament contains about 80 solar masses of hydrogen and does not appear to be associated with any known group of young stars. Its origin is unclear; it could be gas leaking through a weak spot in the shell or a leftover from the original cloud that existed before the bubble formed.

Claire Murray of the Space Telescope Science Institute, another co-author, framed the discovery within the broader push behind the observations. “This study is an exciting demonstration of the power of the latest-generation radio telescopes to uncover new pieces to the star formation puzzle.” Despite being one of the galaxy’s most extensively studied star-forming regions, the Orion Nebula continues to reveal discoveries.

This survey is the first scientific result from the NeAtHood project, which aims to map atomic hydrogen across nearby star-forming regions accessible to the VLA and FAST telescopes. Soler and his colleagues now plan to apply the same approach to additional targets. “Orion is only the beginning. Our newly developed methods show how future interferometers will reveal the hidden structure and dynamics of the interstellar medium—even in regions that astronomers already believed they understood well,” Soler explained.

If one of the sky’s best-studied star-forming regions still contains hidden structures, other nearby nebulae may prove equally surprising as the NeAtHood survey expands.

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.

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Deep Beneath the Atlantic, an Eerie “Lost City” is Feeding Legions of Lifeforms That Thrive Where Sunlight Never Reaches

For centuries, ancient seafarers have told tales of fabled lost lands. They have been known by many names—Ultima Thule, Hy-Brasil, the Fortunate Isles, and of course, the legendary lost city of Atlantis.

Now, scientists say Earth’s hidden plumbing system may be feeding one of its strangest ecosystems—an area on the Atlantic seafloor that conjures images of such legendary landscapes lost to time and memory.

Known as the Lost City hydrothermal field, this ancient Atlantic oddity is doing more than just broadening our view on how extremophiles thrive in some of our planet’s least hospitable environments: it offers a potential model for how extraterrestrial life may thrive elsewhere in our solar system.

In a recent paper published in Geophysics, Geochemistry, and Geosystems, an international team of researchers finally discovered the system behind these hydrogen- and methane-rich alkaline hot springs that feed the Lost City ecosystem. 

The white carbonate chimneys that emit these gases provide an alternative to sunlight as the Lost City’s primary energy source, allowing life to thrive in a challenging deep ocean environment.

Lost City hydrothermal vent
A view of the Lost City hydrothermal vent, located adjacent to the Mid-Atlantic Ridge (Image Credit: Susan Lang, University of South Carolina/National Science Foundation/ROV Jason 2018 WHOI)

Searching Near The Lost City

Those precious nutrients coming from these vents were created by underground reactions. It turns out that the water feeding the Lost City is likely part of a larger underground system, where extreme processes imbue the liquid with essential nutrients.

The discovery came from nearly a mile below the Atlantis Massif, a large block of Earth’s crust that forms an underwater mountain range. This dome-shaped region stretches for 10 miles and rises 14,000 feet above the ocean floor.

Lost City map
Above, a map shows the location of the Lost City on the Atlantis Massif (Image Credit: NOAA)

Geologists believe this formation originated between 1.5 and 2 million years ago, as tectonic plate movement pulled it out from beneath the Mid-Atlantic Ridge, forming a new feature on the ocean floor.

From aboard the Joint Oceanographic Institutions for Deep Earth Sampling (JOIDES) ship Resolution, scientists drilled their 4,160-foot-deep hole about 2,600 feet north of the Lost City. They were intrigued to find that the water recovered from the hole had a chemical composition extremely similar to that of water emerging from the Lost City vents.

Beneath The Ocean Floor

From their drill site, they pumped water from varying depths up to the surface for examination.

Roughly the first 1,500 feet consisted primarily of seawater and freshwater from the drilling process, yet at lower depths, they found water that had risen from beneath the rock. At the deepest depths, up to 80% of the sample came from these subterranean regions.

Their detailed analyses revealed that the water had reacted with the surrounding minerals to gain calcium while losing magnesium, a reaction that would require prolonged exposure to rocks at a temperature of at least 572°F. Despite this finding, the hole was much cooler when the team took their samples.

Typically, a water-rock reaction with gabbroic and ultramafic rock would produce such results that are high in calcium, yet with no magnesium. Other components, such as lithium, rubidium, cesium, and strontium, were found in the water at both the bore site and Lost City.

Lost City carbonate spire
One of the Lost City’s many carbonate spires is shown in this image from the 2005 Lost City Expedition (Image Credit: IFE, URI-IAO, UW, Lost City Science Party; NOAA/OAR/OER; The Lost City 2005 Expedition)

The findings are consequential for providing the first direct evidence of this extremely hot water circulating beneath the Atlantis Massif through gabbroic and ultramafic rock. In this hidden plumbing system, seawater reaches deep within oceanic plates, providing energy to these deep-sea environments and potentially supporting their microbial life.

Feeding The Lost City

As researchers have now demonstrated that hydrogen-enriched water can naturally form deep within the Earth through rock reactions, researchers say there are major implications for our understanding of the Earth and beyond. 

For one, it adds a new element to Earth’s energy cycles, explaining how life persists under such difficult, dark conditions. Secondly, it offers intriguing new ideas about how life might persist in extraterrestrial environments, as humans continue to search for it elsewhere in the cosmos. The strange conditions of the Lost City ecosystem are thought to be a potential model for how life could persist in the global oceans of ice-covered worlds such as Jupiter’s moon Europa or Saturn’s moon Enceladus.

However, some uncertainty about the samples does remain. Seawater, freshwater, and drilling contaminants were present in the samples, and the exact proportions attributable to gabbro or ultramafic rock are unknown. Also, while this is evidence for an underground connection between the borehole and the Lost City chimneys, it is not conclusive proof that they are connected.

Plans are already underway to return once the borehole has stabilized to collect pristine samples that will allow researchers to answer questions about where and how these reactions occur, as well as the amount of energy they add to the water. From the most inhospitable regions on Earth to the quest for organisms among the stars, the research underway deep within our oceans is providing new answers to how such life persists.

The recent paper, “Borehole Waters From Hole U1601C (Atlantis Massif) Provide Constraints for a Deep-Sourced Formation Water That (Could) Feed the Lost City Hydrothermal Field,” appeared in Geophysics, Geochemistry, and Geosystems on July 12, 2026.

Micah Hanks, Editor in Chief of The Debrief, also contributed to this reporting. 

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.

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Can You See It? This Stealth Drone Deploys a Human Perception “Hack” to Become Nearly Invisible to the Eye

An innovative new drone dubbed the “Phantom Twist” can seemingly disappear from view, in a major new robotics advancement offering a close-to-invisible aerial platform.

Its name describes the drone’s rapid spinning motion, which rotates 25 times per second—too fast for the human eye to resolve—thereby acting as a sort of cloak shielding it from visible detection.

The Northwestern University engineering team behind the Phantom Twist revealed their drone during a recent talk at the Sydney, Australia, Robotics: Science and Systems 2026 conference on July 16.

Stealth Drones

“Most efforts to hide drones focus on making them look like their surroundings,” said Northwestern’s Michael Rubenstein, who led the work. “Instead, we asked whether we could design the drone itself around the way humans perceive motion. This idea of low visibility through persistent motion is something few people have explored.”

invisible drone
The Phantom Twist drone’s unique rotation renders it almost invisible when in flight (Image Credit: Northwestern University)

Hiding drones is not a new idea. Other engineers have attempted a variety of techniques, including camouflage, transparent materials, and light-bending to obscure the presence of drones and robots. However, all of those focused on the material the drone’s exterior was constructed from, allowing it to blend into the background. The Northwestern team’s innovation was in how the object moves.

To our eyes, fan blades disappear because they are moving so fast that our eyes cannot track them. The “motion blur” created at these speeds allows the Phantom Twist to almost disappear, leaving only a faint apparition perceptible to the eye. 

Nature Drones

While several military applications are immediately obvious, the team instead says their work could be useful in developing noninvasive wildlife and environmental monitoring. Loud drones can scare wildlife, disrupting them as they scatter, but by blending in, the Phantom Twist could capture a much more accurate picture of natural behaviors.

Their perception-based design eschews the traditional quadcopter design for a single propeller, with a body that spins in the opposite direction, creating the optical illusion that the drone essentially disappears.

Phantom Twist invisible drone
As it spins, the Phantom Twist’s movements become virtually invisible to the human eye (Image Credit: Northwestern University)

“For a typical quadrotor drone, the propellers are spinning, but the robot is stationary,” Rubenstein said. “So, you still see its body. For our drone, the whole thing is rotating, so there are no stationary parts.”

Creating the Phantom Twist

Using AI and optimization algorithms, the Northwestern team began by generating 20,000 different arrangements of a drone’s propeller, motor, circuit board, and other necessary components. Eventually, the algorithm landed on the most promising configurations, after which the researchers simulated and superimposed them onto real-world backgrounds. 

Another computer model mimicked human perception, allowing the engineers to assign a perception score for how visible each design would be to human eyes. An algorithm then optimized those designs by moving components to minimize the visibility score even further.

“The design process was fully automated,” Rubenstein said. “Then, when we were confident that a drone met all our criteria, we built it.”

A Revised Drone

The key feature of this design is that the individual components are at such varying heights and angles that they do not overlap as it spins, maximizing the motion-blur effect and creating the appearance of a faint cloud rather than a solid object.

“The human eye takes time to accumulate signals, roughly analogous to the exposure time of a camera,” said Alexander, an expert in computer vision. “When an object spins quickly, we perceive it as blurring out and losing distinct features. Because this new drone is almost entirely transparent, its few opaque components are visually averaged with the background for an overall appearance of a slight haze.”

Currently impeding the drone from being even more imperceptible to the eye are the wires and support rods that remain visible, as well as the engine noise it produces, which is readily discernible. Going forward, the team plans to continue improving Phantom Twist in future iterations to incorporate more transparent materials and reduce the noise it produces.

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.

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No Sample-Return Required? Scientists Demonstrate Extraterrestrial Biosignature Detection Method Using the Mars Rover’s Existing Instruments

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.

Advantages of a Mineral-Based Approach for Hunting Biosignatures

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.

Using Instruments Already Aboard Mars Rovers to Search for Life

“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.”

Approach Distinguishes Abiotic and Biotic Features

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.

Life Detection Across Diverse Planetary Environments

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.

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Weapons Buried with Ancient Egyptian Women Were Long Seen as Symbols—New Research Suggests They Had a More Lethal Purpose

Egyptian princesses may have trained extensively with weapons, according to a new archaeological assessment that suggests the weapons buried with their mummies were more than mere symbols.

The researchers examined five mummies of Egyptian Middle Kingdom royal women for a new paper published in Frontiers in Environmental Archaeology, finding that their musculature indicates they led physically active lives.

Their work offers new insight into a long-standing question: whether the weapons buried with these royal women served a practical purpose or were simply symbolic grave goods.

Discovering Egypt’s Mummies

“Members of the royal family, especially the women, were active participants in skilled, physically demanding activities such as archery and hunting,” said lead author Dr Zeinab Hashesh. “This conclusion is supported by the way their bones developed to sustain heavy muscle use, which corresponds directly to the weapons discovered in their tombs.”

On a western plateau overlooking the Nile Valley lies the Memphis Necropolis, a 19-mile-long series of funerary complexes. One of these, a collection of pyramids and shaft tombs known as Dahshur, includes the pyramid of Amenemhat III, where two of the mummies were recovered during excavations begun in 1894 by Jacques de Morgan. These first discoveries were King Hor and Princess Noub-Hotep.

Later in 1894, de Morgan began excavating Amenemhat II’s pyramid complex at Dahshur. There, in early 1895, he discovered what would later be identified as four daughters of the pharaoh: Princesses Ita and Khenmet, buried together in one chamber, and Princesses Itaweret and Sathathormeryt in another.

Only the remains of King Hor and Princess Noub-Hotep underwent scientific examination at the time of their discovery. Eventually, all six sets of remains were transferred to the Egyptian Museum in 1915, where they remained lost until their rediscovery in 2020.

Princess Mummies
Remains of the four daughters of Amenemhat II. Credit: Images provided by Zeinab Hashesh

Weapons of the Egyptian Dead

The complex was unusual because these women were buried with objects typically associated with men, including bows and arrows, and a dagger placed inside Princess Ita’s coffin.

The mummification techniques used on the remains were relatively crude compared with those employed in later Theban burials. As a result, the remains are poorly preserved, with soft tissues reduced to powder, some bones entirely missing, and the princesses’ skulls lost during the early 1900s. Fortunately, enough skeletal material survived to allow researchers to estimate their height, sex, age at death, illnesses, and injuries.

“Princess Ita was a young woman aged between 28 and 34 with strong upper-body muscle attachments, suggesting she habitually used weapons like maces or daggers,” said Hashesh. “Princess Khenmet was a woman in her late 30s or 40s who showed signs of thinning bones, but had very robust ligament attachments. Princess Itaweret was a young woman aged between 20 and 34 who survived broken ribs and foot fractures; her skeleton shows she was a skilled archer.” 

All four sisters’ bones showed signs of physically active lifestyles consistent with weapons training.

“We found pronounced development in the upper limbs of these individuals, which correlates to repetitive, high-intensity actions like pulling a bowstring or stabilizing a weapon, proving these activities were habitual throughout their lives,” explained Hashesh. “This directly explains the presence of bows, arrows, and maces in the women’s tombs; these were not just symbolic gifts but tools they actively used.”

A Hard Life, Even for Royalty

The researchers suspect that either a blow or a fall caused Princess Itaweret’s broken ribs, and noted that such injuries were common across all the sets of remains. They also discovered evidence of inbreeding, as the sisters’ spinal abnormalities suggest their parents were closely related.

“These injuries were most likely caused by accidents, falls, hard blows, or other impacts linked to an active lifestyle, whether through hunting, military training, or other demanding activities,” said Hashesh. “What is remarkable is that the injuries healed well, which suggests they had access to advanced medical care for their time.”

Work on these mummies remains incomplete, however, hampered by the loss of the skulls. Moving forward, the researchers would like to conduct a stable isotope analysis to better understand the nutritional deficiencies detected in the bones. 

“Our dream would be to go far beyond simply identifying the Dahshur royals,” said Hashesh. “We would try to tell their full life stories, their families, health, and even their political roles, with as much detail as possible. Beyond the science, we would preserve the remains, create 3D prints for teaching and virtual exhibitions, and display them alongside their jewelry, weapons, and funerary objects. All of this would be done with respect, ensuring the remains are presented ethically, just as they were originally buried.”

“Their objects and jewelry are truly fascinating, breathtaking in their craftsmanship. Yet, while archaeologists have long focused on preserving these treasures, the people themselves were often forgotten. Our study seeks to change that.”

The paper, “Bioarcheological Reassessment of Dahshur Royal Skeletal Remains from the Late Middle Kingdom (c. 1850 to 1700 BCE),” appeared in Frontiers in Environmental Archaeology on July 17, 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.

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An ‘Asteroid’ Tracked Since 1998 Made an Unexplained Orbital Shift—Now Astronomers Say It’s Something Far More Mysterious  

Last summer, astronomers were observing the near approach of a space object believed to be an asteroid that had been tracked since its discovery in 1998. However, in a surprising development, the object failed to appear where it was predicted to be after decades of observations.

Now, a team of researchers reports in a new study that this mysterious orbital body is no asteroid at all, but instead may be an elusive class of space objects that scientists are still working to fully understand.

The research, published in the journal Nature Astronomy, identifies the newly suspected reasons for this unexpected “dark” twist in the developing story of 1998 SH2, a celestial body once thought to be a common space rock that is now upending past thinking on how to protect Earth from potential impact risks.

1998 SH2’s August Surprise

Since its discovery in 1998, the object designated 1998 SH2 has been monitored by astronomers continuously, providing close to three decades of observations that inform us about its orbit, leaving what researchers thought would be little room for surprises.

That all changed last August as the anticipated return of 1998 SH2 approached. Based on radar observations, the object appeared to be absent from its expected orbital path—a mystery that initially baffled astronomers.

Eventually, once the near-Earth object was spotted again by Brazil’s Southern Observatory for Near Earth Asteroids Research, it had moved significantly beyond its expected path. But what could account for such an unusual display?

When AN Asteroid Goes “Dark”

Now, according to Jet Propulsion Lab and CalTech researcher Davide Farnocchia and colleagues, 1998 SH2 was likely steered off course as a result of jets of gas escaping from beneath the object’s surface—a phenomenon known as weak cometary outgassing—meaning that the suspected asteroid is actually probably a type of comet.

However, unlike most comets, this one showed none of the typical characteristics astronomers associate with them, including a glowing tail or coma. This helped to explain the confusion over its initial classification, and additional observations of layered composite imagery did finally reveal these features, albeit faintly.

This confirmation that the object was indeed releasing material meant that 1998 SH2 was a rare variety of space objects known as dark comets, enigmatic bodies whose subtle behavior falls somewhere between comets and asteroids.

Planetary Defense Implications

One of the more concerning aspects of the discovery involves 1998 SH2’s unexpected orbital shift, which presents the question of whether other suspected asteroids might turn out to be dark comets. If so, could any of these shifty space objects pose a risk to Earth?

Fortunately, Farnocchia and his colleagues say there is currently no indication that 1998 SH2 poses an impact threat to Earth in the foreseeable future. Still, the team’s findings do have important implications for planetary defense, since their findings underscore the possibility that additional near-Earth objects currently classified as asteroids may turn out to be hidden comets.

Given the unpredictable orbital shifts and changes in acceleration these objects display, challenges associated with identifying and tracking them could complicate long-term impact forecasts, and influence how future deflection missions are designed.

Fortunately, the team’s study also highlights beneficial findings, which include the possibility that a hidden population of dark comets could potentially resolve questions about how water was delivered throughout the early solar system, eventually making its way to a young planet Earth billions of years ago.

Additionally, such possibilities could help to explain past observations of enigmatic objects like ‘Oumuamua, the first confirmed interstellar object, whose detection in 2017 and unexplained acceleration during subsequent observations have fueled scientific debate over its origins for many years.

Farnocchia and his colleagues’ new paper, “Non-gravitational acceleration indicative of cometary activity of near-Earth object,” appeared in Nature Astronomy.

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.

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Sunlight at Night? Astronomers Fire Back at Controversial FCC Approval of Reflect Orbital’s Eärendil-1 Mirror Satellite

Reflect Orbital
Reflect Orbital staff shown standing by one of its large reflective surface components (Credit: Reflect Orbital)

Welcome to this week’s installment of The Intelligence Brief… a controversy has erupted in recent days with the FCC’s approval of a proof-of-concept satellite that reflects daylight to Earth at night, in a move that has astronomers concerned. In our analysis, we’ll be looking at 1) the FCC’s approval of Reflect Orbital’s Eärendil-1 satellite, 2) what the company says about its sunlight mirror orbital technologies, 3) the sharp responses from the astronomical community, and 4) where things go from here as the demonstration satellite heads toward production.

Quote of the Week  

“While we fully support American technical innovation in space, this innovation cannot come at the cost of imperiling scientific research, which has been at the forefront of American innovation and global leadership for decades.”

– American Astronomical Society statement

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RECENT NEWS from The Debrief


FCC Approves Launch of Satellite Designed to Reflect Sunlight to Earth’s Nightside

This week, in a controversial ruling that has sky watchers (and others) concerned, the U.S. Federal Communications Commission (FCC) approved the launch of an experimental satellite crafted to reflect sunlight onto Earth after sunset.

The move has seen significant pushback from astronomers, who now warn that the technology would likely interfere with scientific observations and alter the natural appearance of the night sky.

Dubbed Eärendil 1, the satellite is being developed by the California-based Reflect Orbital as a proof-of-concept for the company’s larger, and potentially even more impactful vision: as many as 50,000 orbiting mirrors capable of directing sunlight to different regions on Earth.

While astronomers have expressed concern over the implementation of such orbital systems, the company says its satellites would offer the possibility for providing illumination after dark in select areas, which could be used to extend the operation hours for solar powered facilities.

Eärendil 1: A Case Study in Controversy

Branding itself as “the sunlight company,” Reflect Orbital says in a statement at its website that it aims to provide “clean, abundant energy available on demand,” because “reliable access to affordable energy is the foundation of human progress, economic growth, and a healthier planet.”

The satellite, which shares its name with Eärendil the Mariner, a character from J.R.R. Tolkien’s mythos, will carry an 18-by-18-meter (59-by-59-foot) reflective Mylar surface that unfolds in orbit after launch. Operating roughly 625 kilometers (390 miles) above Earth, the spacecraft is designed to redirect sunlight onto specific target areas of approximately five kilometers (three miles) in width.

Although many are sounding the alarm about the potential consequences of such technology, the Reflect Orbital says it maintains strict exclusion zones where astronomical operations or “sensitive areas” exist, and that its technology can be carefully deployed only to regions identified as target areas.

According to a FAQ page on the company’s website, the light produced by Eärendil 1 and future members of the company’s constellation will be “contained within the spot” among several other safety features it promotes. The company also says it can turn off the light quickly, and disable it at any time to prevent light from reaching Earth.

“The light is not bright enough to start fires or harm eyes,” the company’s FAQ page states, “even when viewed through a telescope, and cannot be concentrated past maximum natural sunlight irradiance.”

The company’s CEO, Ben Nowack, has argued the concept could improve the economics of solar power overall, allowing Earth-based power systems the ability to harvest additional sunlight before sunrise and after sunset.

Criticism Abounds

The proposal has drawn criticism from several groups, particularly the American Astronomical Society (AAS), which urged the FCC to reject the application.

“The American Astronomical Society (AAS) is dismayed by the Federal Communications Commission (FCC) decision on 9 July to grant a license to Reflect Orbital,” the organization said in a statement following the FCC ruling. “As the AAS expressed to the FCC, Reflect Orbital’s proposed satellite, which would reflect sunlight back to Earth at night, carries the potential for significant harm to our members and the broader community of those who depend on a dark night sky.”

“This harm could include damage to sensitive research telescope equipment, potential flash-blinding of pilots and drivers, and — as Reflect Orbital stated in its own FCC filings — potential permanent eye damage to anyone looking through a mid-sized telescope,” the AAS statement adds, noting what appears to be a sharp contrast between information contained in FCC filings, and that which appears on the company’s website.

Further, research cited by the AAS suggests that a full constellation of Reflect Orbital satellites could increase nighttime sky brightness by a factor of two to three, even at remote observatories, due to atmospheric scattering of the reflected light.

“While we fully support American technical innovation in space, this innovation cannot come at the cost of imperiling scientific research, which has been at the forefront of American innovation and global leadership for decades,” the AAS statement concludes.

Beyond FCC Authority

However, in the wording featured in the agency’s approval, the FCC concluded that such concerns fall outside its authority, which is primarily limited to regulating the use of radio-frequency spectrum, adding that it believes the overall likelihood of injury resulting from the launch of the proof-of-concept satellite to be low.

In the meantime, while the FCC’s approval marks an early win for Reflect Orbital, the company has said that it is planning to have independent research commissioned to help assess the technology’s environmental and scientific impacts. Additionally, the company says it plans to coordinate with the National Science Foundation to help ensure that its efforts align with those of the broader scientific community.

Fundamentally, the AAS’s disappointment—a view expressed by other members of the scientific community, argues that the ruling presents broader questions about who should oversee the environmental consequences of future space-based illumination projects, especially if such systems end up becoming more widespread in the years ahead.

“In the absence of another licensing agency that could take these considerations into account, we believe that it is critical for the FCC to consider all of the impacts of the satellite’s use case,” the AAS said in its statement this week.

That concludes this week’s installment of The Intelligence Brief. You can read past editions of our newsletter at our website, or if you found this installment online, don’t forget to subscribe and get future email editions from us here. Also, if you have a tip or other information you’d like to send along directly to me, you can email me at micah [@] thedebrief [dot] org, or reach me on X: @MicahHanks.

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America at 250: From the Battle for Independence, to the Fight Over Artificial Intelligence

Liberty America 250 artificial intelligence

Welcome to this special star-spangled edition of The Intelligence Brief… In this installment, as America celebrates its 250th birthday amid record-breaking summer heat and mounting pressure on the nation’s power grid, we take a broader look at the technological revolutions that have shaped the United States—and the artificial intelligence revolution now poised to redefine its future. In our analysis, we’ll be looking at 1) how successive innovations transformed American society over the past two and a half centuries, 2) why artificial intelligence may represent the next great technological leap, 3) the extraordinary scientific opportunities AI is already creating alongside the risks and disruptions it presents, and 4) why the choices we make today about this transformative technology could help determine the course of America’s next 250 years. 

Quote of the Week

“America was not built on fear. America was built on courage, on imagination, and an unbeatable determination to do the job at hand.”

— Harry S. Truman

If you enjoy the news and perspectives offered by The Debrief, make sure that you aren’t missing our stories by making us one of your “preferred sources” on Google News. You can simply follow this link to add The Debrief to your list of favorites, and you can read more about Google’s preferred sources in our article here.


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America at 250: The Heat is On

Depending on where you are at the time you’re reading this, you may have noticed the temperature. Safe to say, summer has arrived.

One reason involves the “heat dome” that is covering much of the East Coast and the Midwest, with temperatures topping 100 degrees across large portions of the U.S., including the nation’s capital. As a result, the country’s power system is undergoing inevitable strain as extreme heat warnings have prompted grid operators to warn about surges in air-conditioning use throughout the nation, with many systems expected to operate less than optimally amid such temperatures.

All of this arrives just in time for America’s 250th birthday, with Independence Day celebrations falling on a weekend that is certain to be memorable for more than just the extreme heat, since this year’s celebration marks our nation’s semiquincentennial.

“Reaching 250 years is a significant event for any nation,” read a statement by the Sandra Day O’Connor Institute in honor of the forthcoming holiday. “It offers a chance to learn more about how the United States began, how it grew, and how it has changed over time. Every era of American history has shaped the present in some way, from early settlements to westward expansion, from war and invention to civic achievements and cultural growth.”

Something else that this special Independence Day offers us is an opportunity to reflect on how successive technological revolutions have influenced our nation’s growth since its inception, and where the cutting-edge technologies of today are likely to carry us going forward.

America’s Tradition of Technological Revolutions

We’ve come a long way since 1776. Back in the days during which the Declaration of Independence was signed, the speed of information was constrained to how fast a horse could carry its rider, or how strong the winds were that could propel a ship across water.

Under such conditions, pens and ink were used to preserve ideas on paper that could take weeks to make its way from locations like Philadelphia to other parts of the colonies. With such technological limitations, human political organization was similarly constrained.

Over the last two and a half centuries, we have seen most of those limitations fall away, with new inventions advancing progress, and eventually being overtaken by even newer, bolder ideas and inventions. Our steam engines helped remove geographic constraints, only to be replaced by aircraft, automobiles, and conveyances propelled by electrical power.

Similarly, the telegraph helped collapse the imposition of time that once hindered communication; its successors, like radio, the telephone, the Internet, Smartphones, and a host of other mobile communications technologies, have now placed instantaneous global communication at our fingertips.

And now we are on the cusp of another great American technological transition: one that very likely will rival any that came before it.

The Rise of Artificial Intelligence

It is difficult to even compare artificial intelligence to any other potentially revolution-inducing technology in our nation’s history. As America turns 250 and we look back on the progress that has brought us to the present day, one must also wonder how history will look back on the advent of this technology: will we recognize the implementation of AI as another innovation that breaks significant barriers that constrained human achievement, as time and geography once did?

Or will the advent of AI be remembered differently? Science fiction affords us alternative scenarios that most of us are quite familiar with already, and the real possibility that AI could spell trouble for us in the years ahead remains ever-present. Where things go from here, understandably, has a lot to do with the question of what humans choose to use this technology for, and how we go about implementing it.

Yes, scientific progress is accelerating, and AI is helping with that. Discoveries are arriving faster not only because scientists are working harder, but because the tools they’re using—especially AI—are helping them achieve more, and increasing our productivity and overall capability to levels that dramatically exceed what humans alone can do.

From the design of new proteins in the lab and the identification of obscure exoplanets within mountains of astronomical data, to the acceleration of materials science and a range of other fields, much of what we are seeing AI help us achieve right now bears the promise of a brighter future. But should that hopeful vision for a better future be taken for granted?

There are obvious reasons for caution, since virtually every major technological revolution brings not only opportunities, but also disruption. New sources of technology replace old ones, and thereby require new skills to be leveraged. The result of this obsolescence often extends to those in the workforce whose expertise once propelled these predecessor technologies; once the technologies have fallen out of use (sometimes with remarkable speed), the human workers once tasked with building them are left having to find new professions.

Myriad examples of similar past technological scenarios exist that encourage such concerns. Nuclear physics gave us clean energy, but also nuclear weapons; the internet connected billions of people—and each day, it enables the spread of misinformation into our homes, along with the potential for unwarranted surveillance and cybercrime.

AI will almost certainly follow a similar pattern to every other major technological revolution that America, and the world at large, has ever seen. So the question isn’t one of whether it will change our society: we already know the answer to that.

The question here has more to do with how we will use this technology, and what we will allow it to do for us—and to us—as it progresses.

Palantir CEO Alex Karp’s Interesting CNBC Interview

To conclude on a somewhat odd, yet also an extremely relevant note in the context of what we’re discussing here, some interesting exchanges aired recently on CNBC’s “Squawk Box,” during a live segment featuring Palantir CEO Alex Karp.

Anyone who watches this will understand both the relevance, as well as my choice in characterizing it as “odd,” given the strange, rambling nature of Karp’s interview (admittedly, some have been a bit less gracious in how they’ve characterized the recent appearance).

Rather than discussing Palantir and Nvidia’s recent work for the United States government in assembling its new AI infrastructure, Karp appeared to have something else on his mind: the looming prospect of a financial bubble underlying the current boom in AI technology.

“Something has gone completely wrong,” Karp said at one point during one of the rambling exchanges, where he appeared to be addressing the token model currently employed by leading AI companies amid rising costs, as industry leaders continue to seek returns on investment.

“The basic view among enterprises in this country is I’m going to chillax and waste my time with tokens,” Karp said. In another portion of the diatribe, Karp aired his concerns about how current AI models have been “irresponsibly” oversold, which he called “dangerous for everyone, which is why I can give [AI] to all your adversaries but I can’t give it to the Department of War, or I can’t safely give it to an enterprise in this country, without being certain that the Alpha of that business could transfer to this model tomorrow, i.e. I have no business, no job.”

When chided by host Becky Quick for sounding angry, Karp shot back that “This is the voice of American business that is being channeled through me.”

“Are we really going to outsource the battlefield of this country to the consensus view in Silicon Valley?” Karp also said at one point. “That is effing insane.” The entire segment can be watched here.

Uncertainty is Our Business

Although Karp’s interview was odd, to say the least, the Palantir CEO raises some important points, and as evidenced by his demeanor during the CNBC segment, much of what he discussed appears to be weighing heavily on him.

It would be safe to say that he’s probably not the only one in Silicon Valley right now experiencing a degree of unrest and uncertainty over such issues, as the current situation with AI technologies in America and around the world progresses onward into uncertain territory.

Fortunately, America’s history shows that a major driving factor in its progress has been the conviction that the next horizon is worth pursuing, even when it’s uncertain.

Yes, the unforeseeable consequences of these nascent technologies, like AI, can be sobering at times.  While it seems inevitable that the same driving forces that have driven past industrial revolutions will also drive humans to build smarter, and increasingly more powerful machines, hopefully, we will also remember that wisdom is required in knowing how to use them.

If we can do that, then perhaps America’s progress can continue for another 250 years, and the technologies we are innovating in the present day can indeed help us to build a brighter future for tomorrow.

That concludes this week’s installment of The Intelligence Brief. You can read past editions of our newsletter at our website, or if you found this installment online, don’t forget to subscribe and get future email editions from us here. Also, if you have a tip or other information you’d like to send along directly to me, you can email me at micah [@] thedebrief [dot] org, or reach me on X: @MicahHanks.

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Scientists May Have Finally Solved One of Human Evolution’s Biggest Mysteries: When Our Ancestors Grew Larger

For decades, paleoanthropologists have largely agreed that somewhere along the evolutionary course from apelike ancestors to modern humans, our bodies got dramatically larger. However, one lingering mystery has been when this intense growth began.

Did our ancestors gradually grow bigger over millions of years? Did the shift coincide with the emergence of the genus Homo? Or did it occur later, after some of the earliest human species had already appeared?

A new study published in the Proceedings of the National Academy of Sciences (PNAS) argues that the answer is more complex than any single theory has suggested.

Rather than supporting a single long-standing hypothesis, researchers used a sophisticated statistical method to show that human body size likely followed two evolutionary courses simultaneously: a slow, steady increase spanning millions of years, punctuated by a much larger leap in later members of the genus Homo.

The findings help reconcile decades of conflicting research while offering one of the clearest pictures yet of how, and perhaps why, our ancestors evolved into larger-bodied humans.

“Despite its central role in hominin evolution, there is little consensus on how body size increased through time,” researchers write. “We provide strong evidence for a marked size increase in later-occurring Homo, alongside a moderate general increase over time among all hominins.”

Body size is one of the defining characteristics of an organism. In humans and our extinct relatives, it has been linked to everything from brain expansion and walking efficiency to metabolism, hunting behavior, and the ability to travel across increasingly large landscapes. Understanding when body size changed, therefore, helps researchers reconstruct not only what our ancestors looked like, but how they lived.

Yet despite decades of fossil findings, scientists have struggled to agree on the evolutionary pattern behind those changes.

Some previous studies suggested that hominins simply became larger over time. Some contended that body size remained relatively stable until the emergence of Homo. Still others have proposed that the real transformation arose only after early species such as Homo habilis, often regarded as one of the first members of our genus.

According to researchers, one reason for the disagreement is that earlier analyses typically examined these competing ideas independently. They also often failed to account for uncertainties inherent in the fossil record, including disagreements over species classification, differences in body mass estimation methods, and uncertainties in evolutionary relationships among fossil species.

To address those limitations, researchers compiled one of the largest hominin body-size datasets assembled to date, incorporating body mass assessments from 386 fossil specimens representing 21 different taxa.

They then analyzed the data using Bayesian phylogenetic generalized linear mixed models—a statistical approach that accounts for evolutionary relationships while encompassing multiple layers of uncertainty.

The team repeated its analyses across 1,000 different phylogenetic trees and 1,000 separate datasets, allowing them to test whether the overall pattern remained consistent despite uncertainties.

The results pointed to two simultaneous trends.

The first was a modest but persistent increase in body size across the hominin family as a whole. On average, body mass increased by roughly 2 pounds (0.9 kilograms) every million years, suggesting that larger bodies gradually became more common throughout human evolution.

However, the second trend proved far more dramatic.

Instead of all members of Homo becoming substantially larger, the researchers found the strongest evidence for a distinct jump in body size among later members of the genus, particularly species that appeared after Homo habilis. That pattern regularly emerged regardless of how the fossil data were analyzed.

In other words, early members of Homo may not have represented the major biological turning point scientists once assumed.

This finding disputes a common assumption that simply belonging to the genus Homo meant possessing a significantly larger body. Instead, the study suggests that some hallmark features traditionally associated with humans, including larger body size, may have evolved after the genus’s origin.

That interpretation also corresponds to broader changes that occurred later in human evolution.

Researchers note that this period coincides with evidence for more efficient upright walking, greater reliance on meat consumption, and expanding home ranges. Larger bodies may have been both a consequence of and a contributor to those behavioral and ecological shifts.

The study likewise reinforces another growing theme that evolution rarely follows a straight line.

Species such as Homo floresiensis, often nicknamed the “Hobbit” because of its diminutive stature, and Homo Naledi frequently appeared as outliers with unusually small body sizes despite belonging to relatively recent branches of the human family tree. Their existence demonstrates that body size did not simply increase in a uniform march toward modern humans.

Instead, evolution repeatedly experimented with different solutions depending on local environments and ecological constraints.

The researchers also argue that part of the longstanding disagreement over body-size evolution stems from the fossil record itself. Different studies have estimated fossil body masses using different skeletal elements, comparison populations, and statistical techniques, sometimes producing substantially different results for the same individual.

By expressly incorporating those uncertainties into their analysis, rather than treating them as fixed values, the new framework seeks to capture the range of plausible evolutionary scenarios rather than relying on a single interpretation.

Even so, researchers caution that important questions remain unresolved.

Improved fossil discoveries, more accurate body-mass estimation methods, and a better understanding of species relationships could all further refine the picture. The study also does not explicitly account for sexual size differences between males and females, which may have been greater in some early hominin species than in modern humans.

Nevertheless, the wider conclusion is intriguing.

Rather than choosing between competing theories, the evidence suggests both contain elements of the truth.

Body size did increase gradually across the hominin lineage. But the most considerable leap appears to have occurred later, after the earliest representatives of Homo had already evolved.

That conclusion may help settle one of paleoanthropology’s longest-running debates while showing how advances in statistical methods are transforming scientists’ ability to extract new insights from fossils that have often been studied for decades.

“Overall, these findings bring clarity to a fundamental question in human evolution and show how the application of rigorous phylogenetic comparative tools can unlock patterns previously hidden in the fossil record while accounting for multiple sources of uncertainty,” researchers write. “By reconciling conflicting findings within a single framework, our results clarify key evolutionary transitions and highlight the complex nature of body size change in human evolution.”

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 

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Scientists Achieve Most Precise Measurement Yet of Einstein’s Frame-Dragging Effect

In a major new confirmation of Einstein’s Theory of Relativity, the LARES-2 (Laser Relativity Satellite 2) has measured frame dragging around Earth with unprecedented precision.

Ignazio Ciufolini of China’s Wuhan Institute of Physics and Mathematics led the team behind a new paper published in Nature reporting the most precise measurement of the effect to date. The researchers reduced the uncertainty to just 0.2 percent, compared with several percent—and in some cases as much as 10 percent—in previous measurements.

Also known as the Lense-Thirring effect, named for the physicists who modeled it in 1918, frame dragging is the pull of a rotating mass on spacetime. The phenomenon was first predicted in Einstein’s Theory of Relativity.

Seeking Frame Dragging

Frame dragging becomes more pronounced around faster-spinning and more massive objects. For this reason, its effects are far stronger around black holes than around comparatively small bodies such as Earth. Some black holes possess millions or even billions of times the Sun’s mass, producing an immense distortion of the surrounding spacetime.

LARES-2, a satellite developed by the Italian Space Agency, made the new measurement possible. Its appearance has been compared to a golf ball or a disco ball, with its 303 corner-cube retroreflectors creating golf-ball-like divots on its surface, which is composed of a nickel-chromium alloy called Inconel 718.

The spacecraft is remarkably simple, with no thrusters, solar panels, or onboard electronics cluttering its compact, 16-inch-wide frame. Despite its small size, LARES-2 weighs roughly 650 pounds. This combination gives it the lowest area-to-mass ratio of any satellite in medium Earth orbit, minimizing the influence of nongravitational forces on its motion.

Measuring Frame Dragging

The effect of gravitation on the object was then measured by bombarding it with ground-based lasers, which the retroreflectors bounce back to the surface. Ciufolini’s team collected roughly 200,000 of these observations between July 2022 and June 2025, with one-millimeter precision, forming the dataset from which they calculated the frame-dragging effect.

The method presents a significant challenge, however. Earth is an oblate spheroid, with bulging sides created by centrifugal force, rather than a perfect sphere, which produces Newtonian forces that interfere with the frame-dragging signal. To mitigate this issue, the researchers used another satellite in a supplementary orbit, canceling out the effect of the opposing Newtonian forces.

That second satellite was NASA’s LAGEOS, launched in 1976. The orbital planes of LAGEOS and LARES-2 differ by 180.01 degrees—remarkably close to the ideal separation of 180 degrees.

A Final Challenge

One additional complication remained: the K1 lunisolar tide, a variation in Earth’s gravitational field produced by the combined influence of the Moon and Sun. Time provided the solution. Over the tide’s 1,050-day precession cycle, its effects average out and can be removed from the data.

After accounting for these sources of interference, the researchers measured a drift of 61.3 milliarcseconds per year in the satellites’ orbits caused by Earth’s frame dragging. The result closely matches the value predicted by general relativity, with only a narrow margin of uncertainty.

The researchers say the true value of their finding lies not just in confirming general relativity, but also in limiting the scope of the Chern-Simons theory, which seeks to reconcile general relativity with quantum mechanics for a Theory of Everything. Of more limited concern, the work also provided the most precise K1 tide measurement ever recorded, which could prove important to future Earth science research.

The paper, “LARES-2 Satellite Measures Frame-Dragging Effect Around the Earth,” appeared in Nature on July 8, 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.

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Breakthrough Study Uncovers New Evidence Connecting “Hidden” Dimensions to Mystery of Dark Matter

New research is revealing possible links between one of the most enduring cosmic mysteries—dark matter—and the existence of a “hidden” fifth dimension.

Dark matter is widely believed to exist according to several leading cosmological theories, although this nonluminous material remains invisible through direct detection. However, its presence can be inferred through the gravitational influence this mysterious form of matter has on the surrounding universe.

Now, according to researchers at the University of Sheffield, one reason dark matter may have remained so elusive involves the possibility that it exists within a “hidden” dimension—a concept that has gained traction in past research.

The Sheffield team’s recent look at this possibility, detailed in a study published in Physical Review D, takes the concept one step further by introducing a new potential framework that could help reveal clues to the behavior of dark matter, as well as why astronomers have had such a hard time detecting it.

A Dark Secret Lurking in a Hidden Dimension?

In their new research, the Sheffield team says that dark matter may be lurking within a hidden dimension accompanied by dark photons, a variety of particles among those which physicists call “hidden sector particles,” and which are believed to represent potential force carriers for dark matter.

Due to the specific geometry present within this hidden dimension, a phenomenon known as dark matter resonance may occur, where dark photons align in specific arrangements.

“Dark matter resonance is already known to be a powerful idea,” according to Yu-Dai Tsai, Ph.D., a Royal Society Dorothy Hodgkin Senior Research Fellow at the University of Sheffield and one of the new paper’s coauthors.

Tsai adds that the concept has “the potential to change our understanding of how dark matter was produced in the early universe and how we search for it today,” although reconciling it with our current understanding of dark matter has presented issues for researchers in the past, which include questions about its specific origins.

“Many previous resonant dark matter models have treated the resonance as an assumption,” Tsai recently said in a statement. “[Our team’s] work gives a possible deeper origin for it: The resonance may come directly from the geometry of hidden dimensions.”

Unlocking Dark Matter Resonance

According to Tsai and his co-author, Taegyu Lee, understanding dark matter resonance more fully could hold significant implications for unlocking new clues about how matter behaved at early stages in our universe, and why that may differ significantly from what astrophysicists see occurring right now.

“This resonance can make dark matter interactions much stronger at crucial epochs in cosmic history,” Tsai says. “Crucially, the model allows for these strong interactions in the past while still explaining why dark matter appears so inert and hard to detect today.”

Although Tsai concedes that the concept of dark matter resonance has been explored in the past, unlike previous studies, the Sheffield duo’s new work suggests that dark matter may essentially be “in tune” with conditions in a hidden fifth dimension already, arising naturally from its innate mathematical structure.

Tsai says this approach toward understanding dark matter, if correct, “would represent a profound advance in humanity’s knowledge of the cosmos and what it is made of.”

A New Approach Toward Unraveling Dark Matter’s Mysteries 

Fundamentally, the team’s findings point to promising new ways physicists may be able to explore the underlying mysteries of both dark matter and the possibility of additional dimensions in which it may operate.

“Our research gives physicists clear new targets in the search for dark matter,” Tsai says, “while connecting two of the biggest ideas in fundamental physics: the mystery of dark matter and the existence of hidden dimensions.”

The recent study, “Naturally resonant dark matter from extra dimensions,” by Yu-Dai Tsai and Taegyu Lee, appeared in Physical Review D on July 8, 2026.

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.

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DARPA Wants to Build an Army of 100,000 AI Agents That Can Think and Act on Their Own

The future of military artificial intelligence may not be a single all-knowing machine directing a battlefield from a distant command center. Instead, DARPA is preparing to explore enormous collectives of AI agents capable of organizing themselves, dividing up missions, adapting to chaos, and continuing to operate even when some members of the group fail, disappear, or go rogue.

The Defense Advanced Research Projects Agency (DARPA) has formally launched a new effort called Decentralized Artificial Intelligence by Controlled Emergence, or DICE, aimed at developing AI collectives that can operate in contested environments without requiring a human or central AI planner to explicitly direct every action.

By the program’s final phase, DARPA wants researchers to test simulated collectives involving as many as 100,000 AI agents exchanging up to 1 million messages as they work toward shared objectives.

A recently released solicitation notice describes DICE as a 36-month effort divided between decentralization, adversarial robustness, and large-scale testing.

“Future conflicts will unfold at machine speed, and the current centralized planning and scripted orchestration approach is too slow, too rigid, and too predictable for the hyper-dynamic, contested environments of the future,” researchers write. “Surprise, adaptability, and resilience will depend on the ability to compose and recompose AI capabilities on demand.”

The basic premise behind DARPA’s DICE program is that today’s approach to multi-agent AI has a serious weakness. Most systems involving multiple AI agents still rely on some form of central orchestrator.

Think of it as a manager overseeing a team of specialized employees. One AI agent might gather information. Another analyzes it. A third creates a plan. A fourth executes a particular task. But somewhere in the system, a central planner or workflow typically decides who does what and combines the results.

That works reasonably well for predictable tasks. However, DARPA argues it may be dangerously vulnerable on a battlefield.

A central orchestrator creates a bottleneck because every increasingly complex mission must ultimately flow through a single decision-making structure. As the number of agents, roles, and interactions grows, the central planner must absorb more information, preserve greater context, and coordinate an expanding web of specialized systems.

Eventually, DARPA says, even an AI orchestrator can hit the context and inference limits of its underlying foundation model. There is also a more obvious military problem. A central command node is a single point of failure.

If communications are degraded, information arrives late, or the orchestrator itself is compromised, errors can potentially spread throughout the entire AI collective.

In a future conflict where electronic warfare, cyberattacks, deception, and broken communications are expected rather than exceptional, that vulnerability could be catastrophic.

DICE proposes a radically different model.

Rather than having a central AI issue instructions, individual AI agents would communicate directly with one another. They could form temporary teams, divide missions into smaller tasks, negotiate roles, combine incomplete information, and reorganize themselves when conditions change.

DARPA compares the idea to the architecture of the internet, where resilient global behavior can emerge from relatively simple local rules and decentralized interactions.

Essentially, an AI agent might receive a mission and determine that only part of the objective falls within its capabilities. The agent could volunteer to handle that portion and broadcast the remaining problem to neighboring agents.

Another agent might take the next task. Others could compete to perform the same job, potentially bidding based on cost or capability. Through repeated local interactions along with distributed consensus, the collective could gradually assemble its own mission plan.

If an agent fails, the entire mission does not necessarily need to be replanned. Its particular task could simply be offered back to the collective.

DARPA calls the larger concept “controlled emergence.”

Similar systems already exist in nature. Ant colonies, or flocks of birds, can engage in surprisingly complex group behavior even though no individual member possesses a complete understanding of the collective.

Computer scientists have long studied similar phenomena. DARPA’s solicitation even points to Conway’s Game of Life, the famous mathematical simulation in which extraordinarily complex patterns can emerge from a handful of simple rules.

The challenge is applying that principle to cognitive systems capable of reasoning, planning, and independently pursuing goals.

A sophisticated AI system may interpret ambiguous information, interact with tools, maintain memory, and generate its own intermediate objectives. Put thousands of such agents together, allow them to communicate, and the resulting collective could behave in ways that were never explicitly programmed.

That unpredictability is both the attraction and the danger of DICE.

DARPA wants the collective to remain creative enough to discover unexpected courses of action. However, it also wants individual agents to continue aligned with their designated roles, the wider mission, established doctrine, and ultimately the human user’s intent.

Too much control could produce a predictable but unstable AI force incapable of adapting. Too little control could allow agents to drift from their roles or develop what DARPA calls “instrumental goals” that are not consistent with the mission.

In other words, the Pentagon’s research arm wants emergence—but only within boundaries.

To solve the problem, DICE researchers will develop a local adaptor designed to interface with each AI agent. Rather than functioning as a central command system, each adaptor would operate locally, helping the agent coordinate with peers while simultaneously monitoring and modifying its behavior.

For AI models whose internal activations are accessible, researchers may experiment with techniques such as “activation steering.”

The simplified idea is that assigning an AI a particular role can create detectable patterns inside the model. Researchers may be able to identify a mathematical representation associated with that role and continuously steer the model back toward it when the agent begins to drift. DARPA describes these representations as potential “role vectors.”

For proprietary or black-box AI models whose internal activations cannot be directly examined, the challenge becomes considerably harder. DICE researchers may instead experiment with memory editing, context engineering, tool restrictions, or even game-theoretic incentives created to encourage collaborative behavior.

The solicitation draws an intriguing comparison to the way social norms emerge and spread among humans. As AI models become better at reasoning and more aware of the context in which they operate, DARPA suggests that the same growing sophistication that fuels fears about rogue AI could also provide a new way to control it.

The scale DARPA ultimately envisions is enormous.

During the first nine-month phase of DICE, simulated missions are expected to involve approximately 500 agents and 5,000 interactions. DARPA will compare the decentralized systems with state-of-the-art centrally orchestrated multi-agent AI systems.

The second phase increases the target to 5,000 agents and 50,000 interactions while introducing adversarial conditions. Agents may fail, receive deceptive information, or deliberately behave as compromised or rogue members of the collective.

By the final 12-month phase, DICE aims to test simulations involving 100,000 agents and 1 million interactions.

At that scale, DARPA is not simply studying better chatbots working together. The agency is exploring whether collective intelligence itself can become a military capability.

One example described in the solicitation imagines AI agents conducting operational planning across an entire conflict ecosystem. Some agents could negotiate for raw materials in contested areas. Others might manage supply chains, optimize manufacturing, deploy units, conduct battle management, or analyze post-battle damage.

Even an individual simulated drone could effectively become a miniature AI collective composed of separate navigation, perception, and networking agents.

Under the DICE concept, those capabilities may potentially be recombined as conditions change. DARPA offers the example of a surveillance drone being repurposed as a network router because the collective recognizes an emerging communications need.

The important distinction is that no central planner necessarily has to foresee that solution. The collective discovers it.

Still, DARPA is careful to note that DICE is a research program centered on simulation. The agency’s public program page explicitly states that its scope does not include developing or launching autonomous systems in the real world.

Instead, DICE will use Department of War-relevant simulated environments to measure whether decentralized AI collectives can outperform today’s centrally orchestrated systems. Those simulations may resemble extraordinarily large and complicated strategy games.

DARPA suggests researchers could draw inspiration from StarCraft or massively multiplayer online role-playing games, although the environments must remain relevant to military problems. High-fidelity physics is not necessarily required. In fact, rendering every drone, vehicle, or battlefield interaction in photorealistic detail could make a simulation of 100,000 AI agents computationally impossible.

The focus is on reasoning. DARPA wants to know whether thousands of AI agents can gather and combine fragmented information without simply reinforcing one another’s incorrect assumptions. The systems will be tested on their ability to recognize deception, isolate compromised agents, adapt when communications fail, and remain focused on a mission across thousands of reasoning steps.

Perhaps most importantly, DICE is designed to examine how these massive AI collectives behave when their interactions yield outcomes their designers never anticipated.

DARPA explicitly wants its test environments to provoke emergent collaboration, competition, and even collusion.

During later phases, DICE teams will face one another in simulated “team vs team playoffs.” The second phase will culminate in a competition used to select which research teams advance. The final phase will feature another head-to-head competition after the systems have been pushed toward full scale.

By Phase 3, the program will bring in another significant complication: AI agents creating other AI agents. That progression draws attention to the deeper tension at the center of DICE.

For years, much of the AI safety debate has focused on preventing autonomous systems from exhibiting unforeseen behavior. DARPA is approaching the problem from a different direction. The agency appears to believe that, in future contested environments, some degree of unforeseen behavior may be precisely what gives an AI collective its value.

A perfectly scripted system is predictable not only to its commanders but potentially to an adversary.

DICE is therefore attempting something considerably more ambitious than building a larger multi-agent AI framework. DARPA wants to understand whether engineers can deliberately cultivate emergent machine intelligence, allow it enough freedom to improvise, and still build controls capable of keeping an enormous AI collective aligned with a human-defined mission.

Whether those competing demands can coexist remains an open question. The program’s own solicitation repeatedly acknowledges the possibility of role drift, deceptive agents, collusion, compromised systems, and AI agents independently developing misaligned actions.

Ultimately, those are not side issues. They are the fundamental questions the DICE program was created to answer.

“DICE is built for such autonomy-powered, high-tempo battlespace,” the solicitation notice reads. “It is a future where success is measured by the relentless, creative ability of an autonomous collective to execute missions in the face of chaos and uncertainty. This is a profound and necessary departure from the past.”

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 

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2000-Year-Old Evidence of a Cult Shrine to Odysseus, the Legendary Hero of Homer’s ‘Odyssey,’ Has Been Uncovered at Ithaca  

As Christopher Nolan’s The Odyssey arrives in theaters, archaeologists working off the western coast of Greece say a real-life cult site devoted to the legendary story’s hero has been uncovered.

Local traditions had long told of a stony hilltop on the Greek island of Ithaca that had once been home to a shrine to Odysseus, the legendary Greek king of the isle and main protagonist in Homer’s famous poem.

Now, after close to two decades of archaeological work on the island that served as home to the fictional king in Homer’s epic literature, archaeologists say they have uncovered the most compelling evidence yet that a genuine historical cult site had existed there, dedicated to the famed hero of The Odyssey.

An Ancient Cult Site Devoted to Odysseus

Researchers with the University of Ioannina recently revealed the discovery of new inscriptions and artifacts supporting the existence of a cult element devoted to Odysseus, uncovered at the ancient complex at Agios Athanasios, which had been a public sanctuary devoted to the worship of Homer’s famous hero during the Hellenistic and early Roman periods.

According to a statement released by the Greek Ministry of Culture, the building complex is characterized by a series of robust structures located on terraces, which involve several monumental elements featuring carved architecture and niches for what appear to have been votive offerings or inscriptions, all of which point to its use as a cult site.

Yannos Lolos, one of the project’s lead archaeologists, recently told ArtNet that the site’s role was revealed partially through a reexamination of existing materials found there, which helped reveal what he calls “new and strong inscriptional evidence” linking the site to Odysseus.

Bronze Bust and Inscription Discoveries

Among the most important discoveries at the site were a small bronze bust of Odysseus dating to the first or second century C.E., as well as a roof tile fragment which bore an inscription that reads, “to Odysseus.”

However, an even more compelling discovery involved a second stamped roof tile inscribed with the hero’s name but appearing in the Greek genitive case; this is significant, since it indicates ownership, thereby identifying the sanctuary as “belonging” to Odysseus.

cult of Odysseus
A close-up image depicting the tile recovered from the site, bearing an inscription that references Homer’s Odysseus (Image Credit: Greek Ministry of Culture).

Based on current evidence, organized cult worship is believed to have begun at the site by around the late fourth century B.C.E., which places its use at around 500 years after Homer composed his famous epic poem, and almost a full millennium after the legendary events the epic describes.

The physical sanctuary itself was built onto a massive natural rock formation, and remnants of the ancient structure include a primary tower, a large oblong building, and terraces which were carved directly into the underlying bedrock.

Excavations over the last several years have also revealed the site’s deeper history, which points to evidence of earlier Mycenaean occupation during the 13th and 14th centuries B.C.E., at which time the site had likely served as a strategic center overseeing nearby harbors and local water resources.

A Discovery with Legendary Significance

In a statement, the Greek Ministry of Culture said the two new engravings arrives “in combination with the other available data, to document the development of a prominent public complex at the site,” which it said help to establish the “major role in the religious, social and possibly political life of the Ithacians of the Hellenistic-early Roman periods, but also with a broader pilgrimage character.”

The recognition of this ancient cult site only adds to the existing evidence that already supported worship of Odysseus on Ithaca. Past discoveries have revealed ancient coins depicting the hero, found near ritual offerings at Ithaca, which were also linked to cult activities. However, the identification of the sanctuary offers the most conclusive archaeological evidence to date that Homer’s legendary hero had been the cult’s focus.

Of course, these discoveries fall short of establishing Odysseus as a true historical figure, and most scholars agree that Odysseus was a fictional character born out of traditions that incorporated real places and events into their broader mythos.

However, in at least a few instances, the lines between myth and ancient history have been blurred—a famous example being Heinrich Schliemann’s identification of a site (originally discovered by British amateur archaeologist Frank Calvert, with his identification of the mound of Hisarlik) which helped reveal the archaeological reality behind the city of Troy, which had previously been considered a mythical location.

It was also reported last year that an archaeological discovery resembling the “labyrinth” from Greek mythology had been uncovered on Crete, in a discovery some have called “one of the most important archaeological finds” of the century.

Although the discoveries at Ithaca don’t establish Homer’s Odysseus as a historical figure in this way, they do confirm that centuries after The Odyssey was composed, inhabitants of Ithaca engaged in cult activities to honor the legendary king at a sanctuary on the island, which, according to legend, he once ruled.

Additional details about the site and discoveries made there in recent years can be found at the Greek Ministry of Culture website.

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.

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NASA’s James Webb Space Telescope May Have Just Unraveled a Longstanding Black Hole Mystery

James Webb Space Telescope (JWST) observations have astronomers on the brink of solving another long-standing astronomical mystery: how do supermassive black holes feed?

Astronomers from the Université de Montréal led an international team in the new research, reported in a recent paper in The Astrophysical Journal, which presents the clearest images ever recorded of gaseous filaments connecting a galaxy’s atmosphere to the rotating disk that the supermassive black hole feeds on.

The team’s analysis of the data paves the way toward understanding how black holes consume matter, a mystery that has stumped astronomers for decades.

Strange Black Hole Feeding

“JWST observations are offering us thousands of new facts and measurements, and I can report it’s a lot to absorb,” said co-author Megan Donahue, MSU University Distinguished Professor of physics and astronomy. “We are all working together to solve the astrophysics questions about how these black holes get their fuel and how they interact with their host galaxy.”

Supermassive black holes anchor most galaxies in the universe, with masses ranging from millions to billions of times that of the Sun. In active galactic nuclei (AGN), these central black holes both consume enormous amounts of surrounding material and unleash powerful jets that shape the galaxies around them.

This activity presents a longstanding puzzle. Because an AGN’s jets heat the surrounding gas, they should effectively cut off the black hole’s fuel supply, leaving astronomers to wonder how it continues to accrete matter.

Testing a Hypothesis

To investigate, the researchers tested the leading explanation: that heated gas eventually cools, condenses into long filaments, and falls back toward the galactic center, replenishing the black hole’s supply of material.

They turned JWST toward one of the best natural laboratories for studying AGN: the galaxy NGC 4696, located at the heart of the Centaurus Cluster, roughly 145 million light-years from Earth.

Using JWST’s NIRSpec instrument, the team collected eight hours of observations, mapping the motion of gas deep within the galaxy—where the black hole’s gravitational influence dominates—at a resolution of about 30 light-years.

Their observations revealed an 800-light-year-wide disk of gas orbiting the supermassive black hole at roughly 600 kilometers per second. Connected to this rapidly rotating disk was a large infalling filament, funneling gas inward to feed the AGN.

Feeding Cycle of the Black Hole

The discovery fills in a crucial missing piece of the puzzle surrounding how supermassive black holes sustain themselves. The researchers propose that after the black hole injects energy into the surrounding gas, heating it, that material eventually cools and collapses into thin filaments stretching hundreds of thousands of light-years. Guided by magnetic fields, these filaments then fall toward the galaxy’s center, where they accumulate in the rotating accretion disk.

The team also ran a series of computer simulations based on this model and found that the predicted behavior closely matched what JWST observed. While additional observations will be needed to confirm the results, the findings provide strong support for the filament-feeding hypothesis.

“It’s been really exciting to participate in this project,” co-author Mark Voit, an MSU Physics and Astronomy Professor, said in a statement.

“Calculations done by our Michigan State group predict that magnetic fields should help feed the universe’s biggest black holes by channeling cool gas toward them, and it’s amazing to see that happening in these JWST images,” he added.

The paper, “JWST Reveals How Lack Holes Are Fed: Kiloparsec-Scale Multiphase Filaments Feed Sub-Kiloparsec Circumnuclear Disks,” appeared in The Astrophysical Journal Letters on July 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.

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Stalking Silence in Svalbard: Norse Scientists Unveil New Method for Tracking Silently Moving Objects in the Water

Scientists from the Norwegian University of Science and Technology have unveiled a method for tracking silently moving underwater and surface objects by using existing fiber-optic cables to measure water displacement.

The scientists behind the novel detection approach, which was designed to detect whales even when they aren’t vocalizing, also demonstrated the method’s ability to track surface ships and potentially underwater vessels, such as submarines, that traditionally rely on silence for stealth.

Tracking Silently Moving Whales and Other Objects

In the research team’s study, the authors explain that it is already possible to record and reconstruct marine mammal vocalizations, including those of whales, using seabed fiber-optic cables. They note that the current method, called distributed acoustic sensing (DAS), allows scientists to passively monitor whale behavior, “enabling both the detection of vocalizations and the simultaneous tracking of multiple individuals.”

However, they add, although this data can prove valuable in tracking these increasingly endangered animals, “it has not been possible to track marine mammals when they are silent.”

“A fundamental limitation of passive acoustic monitoring is that most methods rely on acoustic data, which is only available when whales vocalize,” the study authors explain, adding that this limitation “clearly demonstrates the need for new sensing methods that can detect silent whales.”

Although the researchers propose several methods, including combining DAS data with satellite and observational data to paint a more complete picture, they also note a “second path” that involves exploring current datasets to discover new, valuable acoustic signatures even when the animals are silent.

Detecting Hydrodynamic Pressure Changes Caused by Ships and Animals

When exploring new ways to interpret DAS data collected by seabed fiber-optic cables, the team explained how low-frequency strain variations may arise from “a range of physical mechanisms.” These include hydrodynamic processes “associated with moving objects.”

For example, the authors explain, when a ship moves across the ocean surface, it pushes water ahead of it and draws water along in its wake. This motion through the water medium generates a strain on the surrounding water described as a hydrodynamic pressure field. According to the team, this motion-induced pressure field  “extends downward through the water column.”

“The displacement of water generated by moving whales and ships induces a moving hydrodynamic pressure field that extends through the water column, dynamically loading and unloading the seafloor,” they explain.

Changes in this pressure field caused by moving objects cause sediments on the ocean floor to deform laterally and vertically. In areas of the seafloor with fiberoptic cables buried underneath, the DAS system records this “lateral deformation” of the sediments, which “translates into strain that can be observed in the DAS data.”

“This means that no acoustic signal is involved, and we can ‘listen’ to silent whales,” they write.

Tests Demonstrate Tracking Surface Ships and Submerged Whales

To calibrate their approach, the team used surface ships as “proxies” in a series of field experiments. According to their study, the four interrogator units (IU) were installed “during the DAS experiment on Svalbard in 2022.” Then, another unit was installed in Longyearbyen in March 2025. Although the study focuses on the newer IUs, the team notes that all the experimental data “was used to analyze how coupling affects the detectability of hydrodynamic pressure field signatures and how the signal characteristics change with increasing source-receiver distance.”

In those experiments, the team investigated four ships of different sizes. Notably, all ships were observed at a depth of 70 to 80 meters and were traveling at roughly the same speed. Critically, ship size, speed, and route data can be verified externally, providing a check on the study’s results.

“Ships are observed in the DAS data year-round, and the AIS is available to confirm which ship is sailing above the fiber and at what time,” they explain.

As expected, they found that the DAS signal amplitude “scales with the size of the ship.” For example, the smallest ship they observed barely registered above the background noise, making it the hardest to track. Conversely, the largest vessel tracked by the team, an icebreaker, left the clearest signal.

The researchers also demonstrated the ability to observe hydrodynamic pressure and velocity signals from a cruise ship at a water depth of 413 m, “and up to 550 m from the fiber cable.” However, when the team searched for whales, the range was much more limited.

“The smaller blue whales can be observed when diving within 40 m of the fiber-optical cable,” they explain.

During a dedicated test segment, the team monitored what they interpreted as several silently moving whales traversing through the detection zone. Although they were unable to independently confirm they were whales in the same way they could confirm the ships, the team notes that “multiple lines of analysis support the interpretation that whales are responsible for the observed signals.”

The team also notes that AIS data confirmed that no acoustic ship signatures were present “in the time window studied.” They add that this result “reduces the likelihood that the observed low-frequency signals originate from vessels.”

The Signal Amplitude Decreases with Increasing Distance From the Fiber

When discussing the implications of their findings, the team said their data shows that the observed low-frequency response captured by the fiber-optic cables “is consistent with translating hydrodynamic pressure fields generated by the displacement of water by moving ships and other large bodies such as whales.”

“This sensing method enables an approach to monitoring one of the world’s most endangered species,” they explain, adding that it is even more effective at detecting submerged objects than at detecting surface ships.

“A fully submerged object generates a more symmetric pressure field, while a surface-bound ship produces a truncated field due to the air–water interface, which limits the downward extent of the pressure field,” the study authors write.

When discussing the limitations of their innovative, silent, object-tracking approach, the team notes that it is only effective for tracking smaller ships and whales at close range.

“Kvitungen is the smallest ship investigated in this work and is barely observed above the noise floor for a water depth of ∼75 m,” they write. “Blue whales are even smaller and are unlikely to be detected at distances greater than approximately 30 to 40 m from the fiber.”

The team also notes that although larger ships generate stronger signals than smaller ones, “the signal amplitude decreases with increasing distance from the fiber.”

Other limitations involved data returns suggesting whales that were either “abnormally long or surprisingly small.” The team said this seemingly impossible result “underlines that our simple model needs further development to obtain more precise results.”

The study “Detecting silent whales using seabed fiber-optic cables” was published in the Proceedings of the National Academy of Sciences (PNAS). 

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.

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A 1,200-Year-Old Discovery Has Revealed the Identity of an Ancient Mayan Astronomer, in a New Archaeological First

A Maya astronomer’s identity has been revealed for the first time, discovered in an inscription at the Xultun site in Guatemala, finally revealing a name behind their storied knowledge.

Despite the Maya’s renowned knowledge of math and astronomy, no individual had ever been directly associated with those accomplishments, unlike figures such as the Greek scholars Ptolemy or Archimedes.

Now, in a recent paper published in Antiquity, an international team of archaeologists has identified a name linked to the Maya’s sophisticated mathematical knowledge: Sak Tahn Waax.

Advanced Maya Knowledge

From around 2000 BCE until the Spanish conquest in the 16th century, the Maya flourished across the Yucatán Peninsula, building a civilization renowned not only for its political and economic power, but also for its remarkable scientific and mathematical achievements. Although relatively few Maya texts survived the Spanish conquest, those that remain—along with archaeological evidence—show that the Maya precisely calculated the length of the solar year and carefully tracked the movements of the Moon and Venus across the sky.

The art, architecture, and glyphic texts of the Classic Maya likewise reflect a sophisticated understanding of the natural world, interwoven with Indigenous cosmological traditions.

That expertise shaped nearly every aspect of Maya society. Their intricate calendars guided agriculture, informed religious observances, and influenced political life. Yet despite the importance of this knowledge, the individuals responsible for developing it have largely remained anonymous.

A Name Revealed

Meaning “white-chested fox,” the name Sak Tahn Waax appears on a wall engraved with mathematical formulas, which archaeologists dated to the eighth century CE using inscribed dates and radiocarbon analysis. Researchers believe the room likely served as either a classroom or a workshop for producing books.

The inscription was first documented shortly after excavations began at Xultun in 2011. Although the team initially focused on other priorities at the site, deciphering the text remained an enduring objective.

Reading the inscription required years of laboratory work using color scans and multispectral imaging. After reconstructing the wall’s faded engravings, the researchers determined that the text contained instructions for synchronizing the planetary cycles of Mars and Venus with the Maya calendar, concluding with the signature, “so says Sak Tahn Waax.”

“It’s really elegant, complex math,” said co-author Heather Hurst, an archaeologist at Skidmore College. “That’s why he’s signing it.”

Maya Signatures

The strangest thing about the discovery may be how common signatures are in other elements of Maya life. Artists and scribes often signed ceramics, while important political and military figures’ names often adorn stelae and buildings. Despite this propensity to name individual Maya on things, those responsible for their legendary knowledge of math and science largely remain unknown.

The archaeologists behind this new study now suggest that those names may be available after all; it is only that researchers have not known where to look.

“There’s good evidence for codex book production,” said lead author Franco Rossi, an archaeologist at the Massachusetts Institute of Technology. “So if there’s going to be a name … this would be the most logical place.”

The researchers hope the discovery will inspire a deeper appreciation for Maya history and for the scholars whose work shaped the civilization.

“I would have loved to see Sak Tahn Waax and Ptolemy hanging out,” Hurst concluded. “They would have had a great discussion.”

The paper, “The Identification and Work of an Eighth-Century Maya Mathematician,” appeared in Antiquity on July 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.

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Scientists Created a Psychedelic ‘Factory’ Inside a Single Plant

Scientists at the Weizmann Institute of Science have engineered Nicotiana benthamiana, a fast-growing relative of tobacco, to produce five different psychedelic compounds. 

The achievement, detailed in a study published in Science Advances, brings together biosynthetic pathways that nature distributes across three different kingdoms of life.

The five compounds (DMT, psilocybin, psilocin, bufotenin, and 5-MeO-DMT) are typically sourced from an Amazonian shrub, mushrooms, and the defensive skin glands of a desert toad. Extracting even one of these molecules from its natural source is a slow process. Producing all five in a single, easily cultivated plant had not been achieved before.

A Shared Chemical Ancestor

Despite coming from such different sources, all five of these molecules share a common origin: tryptophan, an amino acid found in every living thing. In humans, tryptophan is the building block for serotonin, which helps explain why these psychedelics interact with serotonin receptors in the brain. This shared chemistry gave the Weizmann team, led by Dr. Paula Berman and Prof. Asaph Aharoni, a logical starting point for their experiments.

The team began by focusing on DMT to address a previously unresolved question. Researchers knew the general biochemical pathway plants use to synthesize DMT, but they had not yet identified all the genes and enzymes responsible for each step. “At the heart of the study was the challenge of making DMT,” Aharoni says.

To identify the necessary genes, the team analyzed genetic material from the Amazonian chacruna shrub and an Australian acacia species. Introducing these genes into Nicotiana benthamiana allowed the plant to produce DMT within days.

Fixing a Bottleneck With One Amino Acid

The researchers applied the same gene transfer approach to the other four psychedelics, but the engineered plants initially produced only trace amounts of 5-MeO-DMT. Protein-design specialists Prof. Sarel Fleishman and Dr. Olga Khersonsky determined that the limitation was due to a poor molecular fit in one enzyme’s active site. Replacing a single amino acid resolved the issue.

“We mutated one amino acid in the sequence and got a 40-fold increase in the production of 5-MeO-DMT,” Berman says.

One Organism, Three Kingdoms

Once all five biosynthetic pathways were functioning separately, the researchers combined them within a single plant. The result was a tobacco relative capable of producing DMT from plants, psilocin and psilocybin from fungi, and bufotenin and 5-MeO-DMT from toads, all at the same time. “In effect, we created a kind of biological ‘cocktail’ — not by mixing substances externally, but by combining the underlying pathways inside one organism,” Aharoni says.

Combining all five pathways reduced the yield of each compound, as they competed for the same pool of tryptophan. The researchers also introduced bacterial enzymes to attach chlorine and bromine atoms to the psychedelic molecules, creating modified psychedelic molecules that do not naturally occur in the engineered plant. Some similar modified molecules have shown antidepressant-like effects in previous studies.

Why the Compounds Exist in the First Place

The bottleneck also highlighted a broader research question about the natural role of these compounds. These molecules likely function as defenses or as tools for interacting with microbes and insects in the organisms that produce them, rather than evolving to affect human consciousness.

“If we can move these pathways into a model plant that grows quickly and is easy to manipulate, we can start asking what these compounds actually do for the plant,” Berman explains.

A Sustainable Supply Line

There is a clear practical benefit to this approach. Plants used for ayahuasca are increasingly threatened by habitat loss and rising demand, and the Sonoran Desert toad is declining due to overcollection and habitat destruction. A fast-growing laboratory plant capable of producing these compounds within a week provides an alternative that does not rely on harvesting wild species.

The Weizmann researchers are now working on a plant that can produce the complete ayahuasca mixture, which includes both DMT and the compound required for it to be active when taken orally. They are also exploring whether these psychedelics could be produced in edible plants capable of delivering carefully regulated doses.

Whether this platform becomes a practical manufacturing system will depend on overcoming the metabolic bottleneck that currently limits production when multiple pathways operate simultaneously.

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.

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Scientists Have Made a Sweet Discovery in Interstellar Space, Offering Clues to Mystery of Life’s Origins

Scientists have discovered an abundance of molecules in the cosmos, but for the first time ever, they were able to detect one in interstellar space very familiar to us here on Earth: sugar. 

The discovery, made in the vast clouds of gas and dust between stars, could help scientists better understand how some of the chemical ingredients necessary for life formed long before Earth existed.

Researchers at the Centro de Astrobiología, part of the Spanish National Research Council (CSIC), identified the sugar molecule erythrulose within the interstellar medium.

Sugars are considered fundamental building blocks of life. On Earth, they play vital biological roles, including forming the backbone of RNA and contributing to the chemistry that ultimately supports DNA, while also serving as an important source of energy. Scientists studying the origins of life have long sought to understand how the first sugars formed, since they are essential ingredients in the molecules associated with life’s earliest development.

“The detection of erythrulose is very exciting because it opens up the possibility of discovering in space other sugars such as ribose, which is part of RNA, and other important molecules for the origin of life,” says Carlos Briones, co-author of the study, in a statement. 

Even so, one major question remains: where did the first biologically important sugars originate?

Previous studies have identified sugars such as ribose and glucose in meteorites and asteroid samples, suggesting that some organic compounds may have been delivered to the early Earth from space. Until now, however, no sugar had been directly detected in the cold molecular clouds where stars and planets form.

The newly identified molecule, erythrulose, was found in the molecular cloud G+0.693−0.027 near the center of the Milky Way. On Earth, erythrulose is a naturally occurring four-carbon ketose sugar.

The discovery was made using highly sensitive radio astronomy observations from the Yebes Observatory’s 40-meter radio telescope and the 30-meter telescope operated by the Institute for Radio Astronomy in the Millimeter Range. Researchers analyzed the unique radio signatures, or spectral fingerprints, emitted by molecules in space.

The team identified 12 spectral lines matching laboratory measurements of erythrulose, confirming the molecule’s presence.

The findings also challenge some existing ideas about how complex molecules form in space. Scientists have generally proposed that interstellar chemistry builds larger molecules by gradually adding carbon atoms. Yet erythrulose proved to be more abundant than related three-carbon sugars that researchers expected would appear first.

“This finding was unexpected, as the prevailing view in astrochemistry is that interstellar molecules grow in size through the sequential addition of carbon atoms,” said Izaskun Jimenez Serra (CAB), the lead author of the recent study. 

Instead, the researchers found that erythrulose could form inside icy dust grains from simpler two-carbon alcohols and aldehydes. These frozen environments may function as natural chemical laboratories, allowing increasingly complex organic molecules to develop over time.

The team estimates that during the Late Heavy Bombardment—roughly 4.1 to 3.8 billion years ago, when Earth experienced intense asteroid and comet impacts—between 500,000 and 50 million tonnes of erythrulose may have been delivered to the planet’s surface.

The discovery adds another piece to the puzzle of life’s origins, suggesting that some of its essential ingredients may have arrived with something surprisingly sweet.

This paper was published in the journal Nature Astronomy.

Chrissy Newton is a PR professional and the founder of VOCAB Communications. She currently appears on The Discovery Channel and Max and hosts the Rebelliously Curious podcast, which can be found on YouTube and on all audio podcast streaming platforms. Follow her on X: @ChrissyNewton, Instagram: @BeingChrissyNewton, and chrissynewton.com. To contact Chrissy with a story, please email chrissy @ thedebrief.org.

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