The ancient history of our planet’s impact events is coming into focus, thanks to researchers who have triangulated similarly aged impacts on Earth, the Moon, and the asteroid 4 Vesta in a new study.

The lunar meteorite NWA 12593 correlates not only with impact events observed across three locations in our solar system but also contains evidence of three separate impact events that occurred at different times.

The findings, revealed in a recent paper published in Geology, show that scientists are using this new impact data to fill in the volatile early-Earth period when life began.

Early Earth Impacts

The Archean period, roughly 4 to 2.5 billion years ago, was a consequential time from which our earliest fossil records date, corresponding to around 3.5 billion years ago. Researchers believe that life likely first arose at this time, yet it may have faced adversity from bombardment by space rocks between 3.2 and 3.5 billion years ago, although scientists disagree on how intense this impact activity was.

Our planet’s geological activity eventually destroys evidence of the ancient past through erosion, subduction, and burial, continually reshaping the surface. Yet those early years are essential to understanding the origins of water, atmospheres, and life on Earth. 

“On Earth, the first fossil evidence of life shows up around 3.5 billion years ago, meaning that life is emerging and evolving before then. The question that we often have, even going back further, is what was the impact record when life was emerging?” said lead author Carolyn Crow, a planetary scientist at the University of Colorado Boulder.

“It is important for understanding how life is taking hold, how life is emerging,” Crow added. “The cadence of these catastrophic events is an important part of the equation.”

A Neighbor Remembers

While Earth’s surface is constantly renewed by geological processes, our nearest significant neighbor, the Moon, is much more stable, retaining its geological record for longer periods. Because of this, lunar meteorites provide a resource for scientists to understand the impact of Earth and the inner solar system by matching them to known impacts on our planet and in the asteroid belt.

For the recent study, the team focused on a lunar meteorite discovered in northwest Africa, designated NWA 12593, and identified three separate impact events in a single sample. 

Radiometric dating traced the oldest to 3.5 million years ago, intriguingly close to the time of the earliest known fossils. Extraordinary in power, this impact produced the mineral zirconia by melting the lunar surface into a lava-like flow. Without the precise laboratory conditions required to produce stable cubic zirconia, only traces of mineral remained in the sample.

According to the team, the first impact aligns with previously known impact events on Earth, and the fourth-largest object in the asteroid belt, 4 Vesta. It’s extremely rare to find such corresponding evidence between three bodies, providing important data on this time of frequent collisions.

“It’s not very common, which is why we’re very excited about it,” says Crow. “It’s pretty rare to have all three records line up like this.”

Later Impacts

Evidence of later impacts included breccia composed of large, angular, broken mineral fragments cemented together. The team believes the breccia resulted from a second impact that struck the melt sheet formed by the first.

“Breccias are similar to what you would see if you went and chipped out a chunk of concrete. You would see all these little rocks, and then it’s fused together by the cement,” says Crow. “But the meteorite is fused together by the impact process. You get all these chunks of different kinds of rocks that the impact hit into. These all get mixed up, and then it gets fused together like your concrete sidewalk.”

As for the third impact, the evidence for this is the meteorite’s mere presence on Earth; an event that occurred some time after the first would have ejected the lunar breccia, the researchers say, allowing it to eventually land on our planet.

In total, the sample reveals an intriguing impact history, preserving a record of bombardment that provides solid evidence for a flurry of activity in the inner solar system during a violent chapter in the early history of our Solar System.

The paper, “Three-Body Evidence of Ca. 3.7 Ga to 3.2 Ga Bombardment Across the Inner Solar System,” appeared in Geology on May 12, 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.

An unexpected human behavioral tendency to prefer turning counterclockwise rather than clockwise has been uncovered by a team of researchers in Spain and Japan, and its cause remains unknown.

In a recent paper published in Nature Communications, the team sought to identify patterns in individual human behavior among large crowds and determine which factors influence them. Surprisingly, the team found that counterclockwise turning is the overwhelmingly common behavioral preference, regardless of gender or culture, with only age making a slight difference.

An Unexpected Behavior

The team’s work could have ramifications not only for psychology but also for architecture, engineering, and design, enabling more intuitive layouts. Work on the project began at Spain’s University of Navarra, before experiments continued at the University of Tokyo in Japan.

The University of Navarra team discovered the phenomenon entirely by accident while researching social distancing during the COVID-19 pandemic. Initially, their interest was in monitoring how effectively the recommended six-foot spacing could be maintained in public spaces. They observed how humans moved through spaces, such as museums, without a set route. While closely monitoring crowd video, they were surprised to witness the counterclockwise trend emerge.

“When analyzing the experiments, my colleagues realized by chance that in 32 out of 33 experimental trials, as people moved and turned, they noticeably preferred to turn counterclockwise,” said co-author Professor Claudio Feliciani from the University of Tokyo’s Department of Aeronautics and Astronautics.

“This was completely unexpected as, at least instinctively, when people walk around randomly, you imagine people turn as their needs suit them with little sign of an overall preference,” Feliciani added. “But there was a definite, measurable tendency for people to turn counterclockwise over clockwise, all things being equal.”

Exploring Internationally

With their curiosity piqued, the University of Navarro team sought to test their findings against further observations to determine which factors might be influencing the behavior. They decided to seek international follow-up observations. This brought them into contact with Claudio Feliciani, whose presence in Tokyo would allow the project to test how the trend played out across cultures, and among other factors. 

For the second stage of the project, Feliciani and his team developed a series of experiments targeting age, handedness, gender, group size, and cultural influence. They observed pedestrian test subjects in both constrained and open environments.

“Of all these things, the only thing that stood out was that kids tend to have a stronger bias for the counterclockwise direction, so probably age plays a role in making the effect weaker or stronger,” said Feliciani. “Our results may appear as a minor, insignificant discovery, but in nature, most phenomena related to locomotion show that animals mostly walk without directional preference.”

“The strong bias found in people hints to some asymmetry at the biomechanical level,” Feliciani added.

Unknown Behavioral Causes

With the international project having confirmed the counterclockwise trend, the researchers are now moving on to more granular exploration of the phenomenon at the individual level. They hope that this more individualized research will yield some information on what biomechanical factors may be driving the behavior.

“It likely does not come from the eyes, because we tried to patch people’s left or the right eyes and the bias was still there,” Feliciani said. “And some people asked us if it might be large-scale phenomena like the Coriolis force or Earth’s magnetic field, but this seems unlikely given what we have managed to point to so far. “

Both lead investigator Iñaki Echeverría Huarte and Feliciani say that the Coriolis effect has become something of a joke among the team, and that they are invariably asked about it when presenting their findings.

“As a curious aside, a friend and collaborator in Argentina was intrigued enough to run some similar experiments when he heard about this,” Huarte told The Debrief of the team’s research in an email. “He tells me that, with no proper scientific confirmation yet, the counterclockwise rotation still seems to be there in the southern hemisphere too.

“There are some interesting parallels to certain sports,” Feliciani concluded. “Some running and driving competitions are always, but inexplicably, taken on courses that run counterclockwise. But that’s an investigation for another time.”

The paper, “Individual Locomotor Bias Drives Counterclockwise Motion in Pedestrian Crowds,” appeared in Nature Communications on June 10, 2026.

Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.

The mystery of the Greenland shark’s incredible longevity may finally be unraveling, as a team of international researchers has completed the first comprehensive genome map of the creature.

Native to the cold waters between Greenland, Iceland, and Canada, Greenland sharks boast one of the longest vertebrate lifespans on Earth, approaching 400 years. In a recent paper published in the Proceedings of the National Academy of Sciences, researchers led by Shigeharu Kinoshita of the University of Tokyo have identified some of the genetic basis of that extraordinary lifespan, which they say future researchers may exploit to treat cancer and age-related illnesses.

Greenland Sharks Longevity

As genetic sequencing technology has improved and costs have fallen, there has been a major increase in the number of sequences from long-lived species for comparative analysis. Discoveries have included identifying increases in genes related to the immune system and growth hormone receptors in rockfish and bat species noted for their longevity.

With an entire lifecycle in slow motion, Greenland sharks’ longevity can be traced to their prolonged development: they take 150 years to reach sexual maturity, growing only 1 centimeter per year. Despite being one of the slowest swimmers in the ocean, the species undertakes large-scale migrations spanning over 1,000 kilometers.

Genome Mapping

Large genome sizes, like those of the Greenland shark, pose enormous mapping challenges, full of many repetitive sequences. Despite their importance for management and conservation, few whale and shark species have been sequenced due to the difficulty involved. To fill data gaps in the genetic causes of longevity, aquatic species evolution, and the risks of biodiversity loss, the team chose the Greenland shark as their subject.

The University of Tokyo-led team mapped roughly 5.9 billion DNA base pairs, accounting for 96.7% of the shark’s genome. Among the discoveries were the identification of specific genetic features likely related to the Greenland shark’s longevity. 

In their paper, they wrote of discovering “genetic traits associated with cancer, immune response function, genome stability, and cardiac function, deep-sea adaptations, and population size dynamics,” in the new research.

Longevity Results

One of the most crucial of these traits is how the shark appears to mitigate the genetic strain that contributes to aging by stabilizing the building blocks of chromosomes. Chromatin is a structure consisting of DNA, RNA, and proteins, which makes up chromosomes.

In the Greenland shark, the histone H1.0 protein, which binds DNA in chromatin, undergoes an amino acid substitution that may enhance stability and reduce the effects of aging.

Another genetic tool aiding the shark’s longevity is the presence of 59 copies of the FTH1b gene, which researchers discovered on pseudochromosome 33, far above the number seen in other shark or fish species. This helps regulate ferroptosis, a form of programmed cell death, thereby mitigating cell damage. Since the gene controls iron storage and ferroptosis is iron-dependent, the researchers say this multiplication of FTH1b could prevent oxidative cell damage.

Beyond those specific expressions, researchers also found expansion of entire gene families associated with DNA repair, immune functions, and cancer resistance.

Although limited to a single species, the research does advance general understanding of the genetic factors involved in extended lifespans. However, it will be up to future researchers to identify how this new information can be applied to human concerns.

The paper, “The Greenland Shark Genome: Insights into Lifespan Extremes and Population Dynamics,” appeared in Earth and Planetary Science Letters on May 19, 2026.

Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.

A meteorite discovered in Africa could be evidence of a lost protoplanet that once orbited our Sun, according to researchers at the University of Colorado at Boulder.

In a recent paper published in Earth and Planetary Science Letters, the team revealed evidence of an ancient protoplanet that may have been as large as Mars based on simulations of how the meteorite sample may have formed.

The four-and-a-half-billion-year-old world carried an unexpected geological makeup, which the researchers say casts doubt on common assumptions regarding planetary evolution.

Protoplanetary Demise

According to the UC Boulder team, the massive protoplanetary body collided with another object four and a half billion years ago, shattering it completely. This is the first definitive evidence of a lost protoplanet in our solar system, based on analysis of the angrite meteorite NWA 12774, a shard of that planetary embryo recovered from the Sahara Desert.

“It’s incredible to think there was once a world this large,” said lead author Aaron Bell, an assistant research professor in the Department of Earth Science at CU Boulder. “We only know it existed because a few fragments of it happened to land on Earth. These meteorites preserved evidence of a completely different pathway through which early planets developed.”

A Rare Meteorite Sample

Angrites, a rare type of volcanic rock, serve as a record of our solar system’s distant past. These rocks began forming only a few million years after the solar system’s birth, making them valuable evidence of this early era. However, they are extremely rare and difficult to find.

NWA 12774 is one of only 68 angrite samples identified among more than 80,000 meteorites cataloged by scientists. Given its rarity, the discovery could potentially reshape how researchers understand these ancient rocks.

Until now, scientists had assumed that angrites originated from relatively small asteroids less than 124 miles (200 kilometers) wide, based largely on their chemical composition. Large rocky planets such as Earth and Mars contain significant amounts of silicon dioxide, while angrites contain very little of the compound.

Unexpected Meteorite Discovery

Researchers began to reconsider those assumptions when they identified clinopyroxene in the meteorite sample. This mineral, commonly found in Earth’s crust and mantle, appeared unusually rich in aluminum, suggesting that it formed under significant pressure deep within a planetary body.

To investigate this unusual characteristic of NWA 12774, the University of Colorado Boulder team recreated the conditions under which the sample could have formed. Their analysis revealed that pressures of at least 17.5 kilobars were required to produce the aluminum-rich clinopyroxene found in the meteorite. For comparison, one kilobar is roughly equivalent to the pressure at the deepest part of Earth’s oceans, near the bottom of the Mariana Trench.

Rethinking Meteorite Origins

The researchers’ discovery proved that at least this particular angrite sample could not have formed inside a small meteorite, as a body with a radius of at least 621 miles would be required to generate the pressure needed to produce the crystals. 

Additional evidence suggested the parent body may have been even larger. The crystals’ sharp edges and delicate internal structures indicate they likely formed at relatively shallow depths beneath the surface. Reconciling both the high-pressure conditions and the shallow formation depth suggests that the parent body may have ranged in size from the Moon to Mars.

“There are many meteorites sitting in drawers that haven’t been thoroughly studied, so there were likely more of these protoplanets we don’t know about,” Bell said.

Exactly what happened to this ancient world remains uncertain, but researchers believe it was likely destroyed in a massive collision early in the solar system’s history. Fragments of that lost protoplanet may have later contributed material to other bodies, potentially including Earth itself.

“The materials that formed the angrite parent body are fundamentally different from the ingredients of Earth and Mars,” Bell concluded. “It points to a distinct and separate evolutionary path in planetary formation in the early history of our solar system.”

The paper, “High-Pressure Clinopyroxene in Northwest Africa 12774 and New Geobarometric Evidence for a Planetary Embryo-Sized Angrite Parent Body,” appeared in Earth and Planetary Science Letters on July 1, 2026.

Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.

Scientists have uncovered the genetic secrets behind a novel energy-use strategy that allows a deep-sea “giant” to survive without food for over five years, in one of nature’s most stunning survival stories.

Supergiant bathynomids, also known as giant isopods, present a bizarre biological paradox: they exhibit pronounced body gigantism as megafaunal species yet inhabit a deep-sea habitat with extremely sparse nutrient availability.

In a recent paper in Cell, researchers from the Institute of Oceanology of the Chinese Academy of Sciences (IOCAS) revealed how these large deep-sea creatures subsist on such limited food, using a novel genetic strategy unique to bathynomids.

A Complex Genetic Approach

The IOCAS team employed a multi-omic strategy to address the problem, combining genomics with other disciplines, such as morphology, physiology, behaviorology, and metagenomics. Doing so led to a novel discovery: that supergiant bathynomids don’t have just one, but two techniques to manage their limited access to nutrients.

First, isopods have a massive stomach that can store vast amounts of nutrients for later use. Second, they have an exceptionally low basal metabolic rate (BMR), which is genetically driven.

To diversify their research, the team focused on two species that occupy different depths. At around 300 meters, the Bathynomus doederleini is the shallower of the two, while the Bathynomus jamesi is found at 898 meters. Despite the difference in depth, both are technically considered “deep-sea” inhabitants, as the boundary is defined at 200 meters.

A Powerful Stomach

Roughly two-thirds of a bathynomid’s body is stomach—a figure far beyond that of related intertidal and shallow water species. The contents of those enormous stomachs are also unusual, filled with a mud-like mixture of highly digested food. This finely ground nutrient sludge has a low proportion of digestive bacteria, but a high amount of lipid-storing Chlamydiae. 

With a bacterial ratio leaning toward preservation rather than just digestion, this creates a food reserve that can be slowly digested and utilized as the creatures lower their BMR to endure long periods between feedings.

Genetic Findings

Another major finding was that bathynomids benefit not only from vertically transferred genes between parents and offspring, but from the horizontally transferred ND1 gene they acquired from an exogenous symbiotic bacterium. Intriguingly, the transfer defied typical horizontal transfer limitations, achieving an ultra-high level of expression in the bathynomid genome. 

These isopods use epigenetic histone modifications to regulate energy-related gene expression, thereby improving efficiency, conservation, and control. An example of this is histone acetylation regulating ND1 expression at an ultra-high level, which the team investigated in a laboratory test. Researchers suspected this gene was essential to energy metabolism, as it is a component of Complex I in the electron transport chain.

ND1 Genetic Tests

Using zebrafish, nematodes, and human 293T cells, the IOCAS team tested the gene’s impact on energy usage. At normal temperatures, the team found that ND1 actually decreased starvation tolerance by increasing energy metabolism. Yet when the team lowered temperatures to reflect those found in a typical deep sea environment, they found the opposite effect, with ND1 decreasing mitochondrial activity and energy metabolism rates, to improve zebrafish starvation tolerance an astounding 37%.

The IOCAS team concluded that ND1 provides a solution to the long-standing paradox of bathynomid gigantism in the context of their nutrient-poor environment. By fine-tuning the degree of metabolic depression, the gene can adjust the mitochondrial metabolic network to preserve energy during extended periods without sustenance.

Never before has such a strategy for energy efficiency, combining horizontal gene transfer and epigenetic optimization, been identified in a deep-sea megafaunal species.

“Our work not only deciphers the mystery of ultra-long starvation tolerance in deep-sea isopods,” said lead author Yuan Jianbo, “but also provides an important paradigm for understanding how life balances growth and survival in extreme environments.”

The paper, “Deep-Sea Megafauna Co-Opts Microbial Energy Metabolism Genes to Withstand Ultra-Long Starvation,” appeared in Cell on June 5, 2026.

Ryan Whalen covers science and technology for The Debrief. He holds an MA in History and a Master of Library and Information Science with a certificate in Data Science. He can be contacted at ryan@thedebrief.org, and follow him on Twitter @mdntwvlf.

A novel phase of matter has been achieved by a team of American researchers, finally realizing a theoretical quantum prediction using nanoscale building blocks, a breakthrough that could pave the way for room-temperature quantum computing.

Researchers at Brown University and the University of Michigan College of Engineering revealed how they briefly stabilized the novel state of matter in a nanoparticle superlattice in a recent paper published in the journal Science. They say their work provides a new method for engineering classes of materials with custom-shaped nanoparticles, which could be applied to quantum computers and other quantum applications.

Quantum Blocks

“Our work is a little bit like kids playing with LEGO blocks,” said co-author Ou Chen, an associate professor of chemistry at Brown. “We synthesize unique nanoscale building blocks and stack them into interesting structures. In this case, we were able to stabilize these theorized transitional structures and demonstrate important quantum optical properties.”

Most metals form in one of two primary groups of crystal structures. The first is face-centered cubic (FCC), the tightest packing arrangement for spherical particles, typically forming a cube with a single particle at each corner and at the center of each face. The other type is body-centered cubic (BCC), a more loosely packed structure in which single particles are still present at the corners, but instead of each face being centered on a particle, one sits at the center of the entire arrangement.

For the most part, atoms form one of these structures as they arrange into a metal, yet at high temperatures, some metals can switch from one structure to another. When it reaches 912° Celsius, Iron will transition from BCC to FCC. One explanation proposed for the transition is the Nishiyama-Wassermann pathway, which suggests that, due to the lower symmetry of the transition phases between FCC and BCC, these phases are fleeting.

Testing the In-Between States

The American team behind the recent research decided to test this idea, fabricating one of those low symmetries in between phases with silver nanoparticles 

“Materials scientists have cared about how to control the amount of FCC and BCC in their metals for a long time, but the transitions between these phases have been hard to study because they are so unstable,” said co-author Tim Moore, an assistant research scientist at the University of Michigan. “Being able to observe these structures is a fundamental breakthrough in materials science, and it gives us greater control over nanomaterial engineering.”

At the heart of the team’s work was the truncated octahedron, or “mecon,” a 14-sided polyhedron formed by cutting off the vertices of a diamond, producing an intermediate shape between a cube and sphere.

As the team synthesized silver nanoparticles, they varied the heat level during production, resulting in a spectrum of shapes ranging from cubic to spherical, which were coated with long, sticky molecules that bound the particles. They found that the sticky molecules were required for the particles to assemble themselves into the intermediate shapes predicted by the Nishiyama-Wassermann pathway.

Near Quantum Behavior 

Once the particles self-assembled into variously shaped nanoparticle superlattices, the team tested their behavior with computer simulations and physical observations.

The superlattices show evidence of a process known as deep-strong light-matter coupling, in which silver electrons vibrate in unison with light waves, becoming so hybridized they could no longer be treated independently. The similarity of this state to quantum entanglement leaves the team hopeful that their superlattice can be applied to quantum work in the future. 

Crucially, this action occurs at room temperature, whereas in previous instances it occurred only at very cold temperatures. This means the work could be useful for developing quantum technologies, which have been limited by the extreme cold required.

“One of the major challenges in quantum computing is maintaining coherent quantum states without requiring extremely low temperatures,” Chen told The Debrief in an email. “Our work suggests that carefully engineered nanoparticle superlattices may provide a scalable materials platform where strong and coherent light–matter interactions can persist at room temperature.”

Quantum Applications

“In the long term, such systems could potentially be used to create or manipulate quantum states for applications in quantum information science, including quantum communication, sensing, or photonic quantum technologies,” Chen said. “However, it is important to emphasize that this research is still at the fundamental physics and materials discovery stage. We are not yet building a room-temperature quantum computer, but rather exploring new material platforms that may help enable future quantum technologies.”

As research continues, the team is focused on more precisely controlling the superlattices’ quantum optical properties.

“Specifically, we are interested in: Engineering nanoparticle architectures that produce even stronger and more controllable light–matter coupling; Exploring how structural order, particle shape, and lattice symmetry influence quantum optical behavior,” Chen explained, “and Integrating these materials with photonic and optoelectronic platforms for potential quantum-device applications.

“More broadly,” Chen concluded, “we see this work as opening a new direction where nanoscale self-assembly can be used to engineer emergent quantum optical properties that do not exist in the individual nanoparticles alone.”

The paper, “Stabilizing In-Transition Phases of Superlattices Through Shape Control of Silver Nanocrystals,” appeared in Science on May 28, 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.