A team of conservationists has discovered and restored the tombstone of Sebastian, a formerly enslaved man who died free in 1729.

"That discovery is likely one of the oldest gravestones of a free Black person in America," Michelle Wu, the mayor of Boston, said in a July 4 speech. "It's been there all along. We just had to go look and share the story."

The stone marker is inscribed with Sebastian's chosen name, Boston, and features an image common in 17th- and early 18th-century tombstones in New England: the death's head. The symbol includes a stylized skull flanked by wings, which were possibly intended to symbolize spiritual resurrection.

On the tombstone, a simple, five-line inscription reads:

In 18th-century American writing, the word "the" was often abbreviated with a Y-shaped letter form called a "thorn" representing the "th" sound. Tombstones also frequently abbreviated "deceased" and the month. Somewhat confusingly, before 1752, the American colonies regularly used the Julian calendar, as did Britain, in which the new year started on March 25. Boston's year of death is listed on the tombstone as 1728, but his February 28 death was actually in 1729 in our modern Gregorian calendar.

Kelly Thomas, the director of the Historic Burying Grounds Initiative for the Boston Parks and Recreation Department, told WBZ News Radio that she identified the gravestone during a restoration project at the Granary Burying Ground, the city's third-oldest cemetery. Established in 1660, the cemetery includes over 5,000 graves, including the final resting places of Declaration of Independence signers Samuel Adams and John Hancock; the U.S. Revolutionary War officer Paul Revere; and Crispus Attucks, a sailor of mixed African and Indigenous ancestry who is thought to be the first American killed in the Boston Massacre.

"I was reviewing the photos of headstones, and then I noticed that the stone only had one name," rather than a first and last name, Thomas told WBZ News Radio, suggesting that Boston was either enslaved or free when he died. Based on a search of historical records, Thomas determined that Boston's enslaved name was Sebastian and that he also went by Bastian.

A surprising amount of information was recorded about Boston and his wife, Jane Lake. In 1701, they had their daughter, also named Jane, baptized at First Church in Boston, where they regularly attended worship services. But while the two were married with children, they were also both enslaved and lived in different households, historian Gloria Whiting wrote in a 2016 study.

Boston was likely freed in the early 18th century, some time after the 1702 death of John Waite, who had held him in slavery. By 1708, a list of free Black people included the name Boston, and he had gained a reputation in the city as a hardworking handyman, according to Whiting's study. He had been freed for roughly 30 years when he died in 1729 and was well-known enough to have an obituary published for him in the New-England Weekly Journal, a rare occurrence for enslaved or freed Black people in colonial America.

Wu also said that, in recent weeks, archaeologists in Boston had discovered musket balls and gun flints from the infamous Battle of Bunker Hill that took place on June 17, 1775. The battle was fought by British Crown forces and New England troops in the first stage of the American Revolutionary War.

See if you know what these mysterious artifacts are with our archaeological fragments quiz!

The fragile and battered remains of an infant who lived about 6,000 years in Mesopotamia may be the oldest documented case of child abuse from the Middle East and one of the oldest known cases of its kind in the world, a new study finds.

Researchers unearthed the infant's remains in Syria, but at the time the infant died, sometime between 4200 and 3900 B.C., it was buried in Tell Brak, one of the world's earliest cities. It's possible that the difficulties associated with early urbanization played a role in the child's abuse, the researchers noted.

The team determined that, based on the infant's tooth development, the child was 6 to 9 months old at death. An analysis of the remains, which were interred in a children's burial ground within a Late Copper Age workshop district, revealed that the infant had four fractured ribs near the breastbone. The right thigh bone had abnormal growth, while both sides of the skull bore active, porous lesions. These injuries point to the bones being subject to intense and repetitive external forces, and the nature of the lesions don't fit easily with an accidental fall, the researchers said.

"Ribs shouldn't break" in such a small child, study co-author Aleksandra Grzegorska, a bioarchaeologist at the University of Warsaw, told Live Science. Although rib fractures are relatively common in adults, they suggest child abuse in young infants, she said.

In the study, published May 21 in the International Journal of Osteoarchaeology, Grzegorska and her colleagues systematically ruled out other explanations for the injuries, including rickets, scurvy, birth trauma and violent coughing from illnesses such as tuberculosis. Vitamin deficiencies were unlikely, the researchers noted, given that ancient Mesopotamia had ample sunlight and fresh produce due to the fertile land between the two rivers. Birth-related fractures typically heal within weeks in infants, and bone density and growth measurements for the baby matched those of its peers from that time, indicating that the child didn't have an underlying skeletal condition.

To gauge how unusual the injuries were, the team compared the infant to other children excavated from the same burial area. None of the other youngsters with substantial rib preservation showed similar fractures, making the infant's injuries an outlier in the local population.

It appears that the infant likely experienced "caregiver-induced violence," Grzegorska said. This term is used because the evidence can't identify who caused the harm or confirm intent, Grzegorska said. "We don't want to point fingers at any specific individual," she said, noting that in many ancient cultures, multiple family members, not just parents, helped raise children.

Other clues that might shed light on the infant's injuries are missing from this case, she added. Unlike modern clinicians, bioarchaeologists can't interview a living patient or bystander, or examine soft tissue that might reveal more about the abuse. The partially healed state of the fractures suggest the infant survived for some time after the injuries were inflicted, Grzegorska found — an indication that the trauma was not immediately fatal.

Around the time the infant died, Tell Brak was transforming into a city, so the authors suggested that the stresses of early urbanization and possibly less support from extended kin could have contributed to the violence. Centuries after the infant died, upheavals related to city building appear to have led to mass deaths that were likely caused by violent conflict, Grzegorska noted.

Documented cases of child abuse remain exceptionally rare in the archaeological record, with only a handful previously identified in places such as Egypt, France and Lithuania.

For the first time, a physicist has experimentally watched time emerge from within an isolated quantum system — by creating a “mini-universe.” This bizarre experiment raises an intriguing question: If the universe has nothing outside it, where does time come from?

In a new study published June 11 in the journal Physical Review Research, Giovanni Barontini, an experimental physicist at the University of Birmingham in the U.K., used a cloud of ultracold atoms to build his mini-universe. The system was so well isolated from its surroundings that, like the universe itself, it had nothing external to use as a clock. He split that system in two and ignored one half — what he called the "dark sector" — to show that time could arise entirely from within the system.

The result offers the first experimental look on why the universe has time at all. "When you put everything together, things really start to make sense," Barontini told Live Science. "How time inside the system was speeding up or slowing down, or even stopping — this was quite surprising, how well everything came together. Very neatly, in a way. Which is something that doesn't happen that often in experiments."

The work is an experimental verification of ideas that have been floating around in quantum cosmology and thermodynamics for decades. This is not a bombshell claim that time is an illusion, but it is the first time anyone has put those ideas to a direct, quantitative test in the lab.

A universe with nothing outside

Barontini set out to look at a problem that physicists have puzzled over for nearly 60 years. The Wheeler-DeWitt equation — a central equation in quantum gravity, the field that seeks to unify Einstein’s theory of gravity with quantum mechanics — describes the universe as a whole system with no external time parameter. There is no cosmic clock ticking away outside the universe. So where does our experience of time come from?

One influential idea, called relational time, says that time doesn't exist as a fundamental ingredient of reality. Instead, it emerges from relationships inside the universe, with one part of the system acting as a clock for another. But this idea had never been tested directly in the lab.

Barontini's inspiration came from watching his son play with building toys. "I thought that it's something very similar to what we do in our labs," he told Live Science. "We play with very expensive toys. We create our own small samples of reality."

In his lab, that sample is a Bose-Einstein condensate — a state of matter that forms only at near absolute zero. In a Bose-Einstein condensate, thousands of atoms slow to a near standstill and blur together into a single quantum object, behaving as one.

The dark side of time

To mimic a universe with nothing outside it, Barontini placed the condensate in a trap and divided it down the middle with a thin sheet of laser light. He watched one half, the "bright sector," closely and deliberately ignored the other half, which he called the "dark sector."

The atoms in the bright sector sloshed back and forth in the trap, periodically spilling over the barrier and back again. Barontini called the moments when atoms flooded into the bright sector the "Big Bang" and the times when they drained out the "Big Crunch" (the nickname for one theory of how the universe will end, with the universe collapsing in on itself). Then, he tracked how entropy — a measure of disorder, or how spread out energy is within a system — was exchanged between the two halves as atoms crossed the barrier.

Instead of using laboratory time to order events, he built an "entropic time" — a clock defined entirely by how much entropy was flowing between the two halves of the system. If entropy was flowing, time was ticking. If no entropy was exchanged, time stopped. "The entropy exchange between the two systems could be transformed into an internal time variable," Barontini said.

Time speeds up, slows down and stops

What surprised Barontini most was how cleanly everything fit together. The internal, entropic time reliably ordered events in the bright sector. It matched the sequence seen in laboratory time, but it flowed at a different rate.

When entropy was flooding between the sectors, entropic time ran fast. When the exchange slowed, so did the clock. And when the two halves reached equilibrium (no more entropy flowing), the internal clock stopped altogether.

"Time was speeding up or slowing down, or even stopping, depending on what the system was doing," Barontini said.

He then went a step further: Using this internal time, he derived a version of the Schrödinger equation and showed it accurately reproduced what he saw in the experiment. "This was quite surprising, how well everything came together," he said — "very neatly, in a way, which is something that doesn't happen that often in experiments."

Both time itself and the arrow of time — why time flows in one direction rather than the other — may arise from the same source: an observer giving up information. When Barontini chose not to look at the dark sector, he gave up knowledge of that half of the system. That act of ignorance, encoded in entropy, is what gave rise to time in the other half.

"Both time and the arrow of time — maybe they just are born from ignorance," Barontini said. "To have time and to observe, you have to give up some degrees of freedom."

Barontini sees this as just the beginning. The same cold-atom tool kit that generated a miniature Big Bang and Big Crunch in his trap could, in principle, be engineered to simulate far more exotic phenomena, such as black hole analogues, the conditions of the early universe, and what will happen at the moment of the Big Crunch itself.

"These are things we can do very simply, using the tools we already have to engineer our systems," he said.

The study is a proof of concept ‪—‬ a first demonstration that controlled quantum systems can serve as a test bed for some unanswered questions in physics. For now, those questions remain open.

Archaeologists in Italy have unearthed the royal tomb of a pre-Roman "warrior-prince" along with the remains of his chariot and weapons. The tomb was just one part of an extensive sixth-century B.C. burial ground and reveals new information about the funerals of elite rulers from this mysterious civilization.

The funerary complex was found in the municipality of Sirolo, a small town on the Adriatic Sea on Italy's east coast, according to a translated July 1 statement from the Superintendency of Archaeology, Fine Arts and Landscape for the Provinces of Ancona, Pesaro and Urbino.

In the sixth century B.C., an Italic group called the Piceni or Picentes lived in the area, bordered to the north by the Etruscans. The Piceni left few written records, so much of what is known about the enigmatic group comes from archaeological excavations. In 2020, a "princely tomb" complete with an iron-wheeled chariot, a cache of weapons and a helmet was discovered in the Pini cemetery. Now, archaeologists have found a second one.

At the center of a monumental circular palisade, researchers unearthed a large male burial with a wooden "currus" — a two-wheeled chariot that had been buried intact with the nobleman around 2,500 years ago. The warrior prince was also buried with a helmet and an ax, as well as several bronze vessels sealed with ceramic lids and filled with organic remains, which may represent the traces of a funeral banquet or food offerings for the afterlife.

Next to the warrior prince was the tomb of a woman who was buried with textiles, shoes and numerous "fibulae" — ancient metal safety pins that likely fastened her clothing and burial shroud. An enormous fibula with a hunk of amber had been placed on or near her head, possibly as part of her hairstyle or a headdress. This burial is not far from the "Queen's Tomb" in the Pini necropolis, where, in 1989, archaeologists discovered a Piceni woman buried with two chariots, two mules and a large quantity of personal belongings.

While royal burials had been discovered in the Sirolo area for decades, the newly discovered cemetery surprised archaeologists because of its unprecedented shape. Previously discovered burial grounds in the territory of the Piceni were ringed with a ditch, symbolizing the separation of the dead from the living. But the newly discovered cemetery was ringed with a wooden palisade instead of a ditch, and it had been placed on a slight hill, possibly to emphasize its monumental character and symbolic value, according to the statement.

This is the the first time that archaeologists have observed "an entire aristocratic nucleus" of the Piceni, and the discovery can provide "new perspectives on the structure of the elites that led to the great Piceni center," archaeologist Stefano Finocchi, the director of the new excavation, said in the statement.

Although many of the artifacts are still being analyzed, the quantity and quality of the grave goods already recovered reveal that the "ruling groups integrated into a dense network of relationships connecting the central Adriatic with the principal centers of central Italy," Finocchi said.

From Augustus to Nero, see how much you know about ancient Rome's famous leaders with our Roman emperor quiz!

The European Space Agency's (ESA) Euclid space telescope has spotted 31 previously unknown quasars dating to the universe's earliest chapter, including the two oldest ever found.

The discoveries, described July 6 in the journal Astronomy & Astrophysics, more than double the number of known quasars from that primordial era and could help astronomers unravel one of cosmology's biggest mysteries: how supermassive black holes grew so enormous so quickly after the Big Bang.

"It's a big step towards understanding these fascinating objects on a more fundamental level," Antonio La Marca, an ESA research fellow on the Euclid team, said in a statement.

Quasars are among the brightest objects in the universe. They form when gas and dust spiral into a galaxy's central supermassive black hole, heating up and releasing enormous amounts of energy that can outshine the galaxy itself. Each of the two most ancient quasars detected in the new study shone with the light of a trillion suns, according to the researchers.

Euclid spotted the quasars while surveying the distant universe. Twelve of them have redshifts of 7 or higher, meaning their light has traveled for more than 13 billion years and dates to the universe's first 770 million years. Two of the objects, with redshifts of 7.77 and 7.69, are the most ancient quasars ever identified, shining just 670 million years after the Big Bang, when the universe was only about 5% of its current age.

"These early quasars date back to the Universe's infancy," Daming Yang, an astronomer at Leiden University in the Netherlands and first author of the new study, said in the statement. "By finding and studying them, we can better understand how these enormous systems formed and grew so quickly — one of the greatest mysteries in astrophysics."

Finding quasars from the early universe has long been difficult because they are rare and incredibly distant. Until now, astronomers had identified only the brightest examples, making it difficult to understand the broader population during this early era. Euclid's wide-field survey is changing that by detecting fainter quasars across huge swaths of the sky.

The latest discoveries represent only a fraction of what the telescope is expected to find during its six-year mission, which will cover more than one-third of the total sky once complete. Mounted with a pair of instruments that see in visible and near-infrared light, Euclid is currently assembling the largest-ever 3D map of the universe. Scientists expect the survey to uncover hundreds of similarly ancient quasars, providing an unprecedented look at how the universe's earliest galaxies and supermassive black holes evolved.

Euclid has also taken some time to study the nearby universe, revealing more than 60 million individual stars packed into the Milky Way's center in a sparkling image released in late June.

Black hole quiz: How supermassive is your knowledge of the universe?

This ethereal satellite snap shows beautiful, "painting-like" folds within an ancient underwater structure in the Bahamas.

The Great Bahama Bank (GBB) is a massive submerged platform stretching around 330 miles (530 kilometers) across a shallow ocean channel between Andros Island and the Exuma islands, according to Britannica. The crescent-shaped bank surrounds a darkly colored ocean drop-off known as "The Tongue of the Ocean," which plunges to depths of 6,500 feet (2,000 meters), according to NASA's Earth Observatory.

The photographed section of the GBB is around 23 miles (37 km) across and features a series of submerged sandbanks — most of which are covered with dense seagrass beds — that lie between 7 and 40 feet (2 to 12 m) below the ocean's surface.

The varying water depth and seagrass concentration cause multiple hues of green and blue to shine across the sandbanks, which have been carved into smooth, folding ribbons by ocean currents over thousands of years.

"The varying colors and curves remind us of graceful strokes on a painting," Earth Observatory representatives wrote.

This section of the GBB was first photographed in 2001 by the Landsat 7 satellite and has often appeared on lists of the most iconic aerial images of our planet.

"There are many nice seagrass and sand patterns worldwide, but none like this anywhere on Earth," Serge Andréfouet, an oceanographer at the French National Research Institute for Sustainable Development who first shared the 2001 image, told the Earth Observatory. "I am not surprised it is still a favorite, especially for people who see it for the first time."

The sandbanks are like giant underwater dunes carved out by ocean currents.

"Tides and ocean currents in the Bahamas sculpted the sand and seaweed beds into these multicolored, fluted patterns in much the same way that winds sculpted the vast sand dunes in the Sahara Desert," Earth Observatory representatives wrote in 2001.

The GBB lies atop a roughly 3-mile-thick (5 km) bed of limestone dating to the age of the dinosaurs, more than 65 million years ago. This hefty mass, made up of the remains of long-dead coral reefs, is so large that Earth's crust directly below the GBB has "sagged under the weight," according to the University of Texas at Austin's Marine Science Institute.

Before the end of the last ice age, around 12,000 years ago, this limestone slab had risen to more than 400 feet (120 m) above sea level and only resubmerged as global sea levels rose due to the melting of glaciers, according to the Marine Science Institute.

The Bahamas has more than 3,000 islands and smaller cays and is home to several other intriguing oceanographic features, including deep tidal channels off the coast of Great Exuma Island (which once harbored famous pirate ships) and a series of aurora-like sandbanks that appear to shine along the nation's northernmost islands.

See more Earth from space

Scientists say they have built a "synthetic cell" that can eat, grow and divide in a way that's remarkably similar to living cells.

The research, released to the preprint database bioRxiv July 2, has not been peer-reviewed yet. It introduces SpudCell, a new type of artificial cell, and marks a striking step toward creating living cells from scratch. But for study co-author Kate Adamala, a synthetic biologist at the University of Minnesota, that's far from the most interesting part of the work.

"I do not believe [SpudCell] is alive," Adamala told Live Science. Instead, she describes the system as a framework that could generate "all the chemicals we need for our civilization with biology." The thought is that SpudCell could serve as a tiny factory, pumping out medicines, fertilizers, plastics or any number of other compounds.

The work's announcement has sparked some controversy, with some scientists seeing it as a ploy to gain media attention for the simultaneous launch of the author's nonprofit Biotic, which aims to raise money to further develop the SpudCell platform. Adamala does not take umbrage to that criticism, as she is keen to bring more attention and funding to her field. If a synthetic cell can be perfected, she thinks, it could help humanity generate chemicals without relying as heavily on petroleum products.

"I feel this incredible stressful urgency that if we don't get to work on it now, then we're going to run out of time," she said, referring to the climate crisis. "We need to highlight that bioengineering can offer a solution. That's why I'm doing it."

A synthetic cell and a big promise

According to the preprint, Adamala and her team produced a lifelike system that closely resembles a living cell. To do so, they combined 36 purified enzymes and a fatty membrane with a pared-back genome about 50 times smaller than that of an average bacterial cell. By mixing these human-made elements together, the scientists generated a cell that could feed, grow, and divide — so, in essence, they created a full cell cycle in a petri dish.

"We built a cell-like system that is fully chemically defined, so there are no unknown building blocks in it," Adamala said. "It's capable of doing things that people up until now used to think only natural living cells can do." They call the system "SpudCell" because it looks similar to a potato, The New York Times reported. The name is also a nod to the Sputnik satellite, per CNN.

The concept of recreating the cell cycle in a dish is not entirely new. The J. Craig Venter Institute's 2016 "minimal cell" paper flirted with the concept by stripping as many genes from a bacterium as possible to leave only a minimal cell that could still replicate. However, the new study is the first time scientists have achieved feeding, growing and division using a "bottom-up" approach.

The work marks "a great advancement," said Mauro Rinaldi, a lecturer in biotechnology and biochemistry at the University of Hull in the U.K. who was not involved in the work. "It moves the needle because one of the key things about cells is division."

But there are important caveats. For one, the cells cannot yet create their own energy as our cells do with mitochondria. They also rely on externally provided fats, sugars and enzymes. The cells cannot make their own ribosomes, the machinery that turns genetic instructions into working parts of the cell. That means it relies on proteins being delivered from the outside.

Another difference is that SpudCell's genome is spread out over bits of DNA called plasmids, rather than being neatly packaged in chromosomes. It does not possess the skeleton that cells typically use to neatly split DNA during cell division, so consequently, the division of SpudCell's DNA to its daughter cells can be somewhat haphazard.

"The description of the results leaves me with substantial technical questions regarding the nature and the robustness of the findings," said Cees Dekker, a biophysicist at the Delft University of Technology in the Netherlands who was not involved in the work. "[Its] approach uses some ingenious engineering tricks as shortcuts to achieve complex functions such as growth, but a major challenge remains to create a truly autonomous cell that executes all these functions without external help," he said.

Dekker is among the scientists who would have preferred that the research made the news after being published in a peer-reviewed scientific journal. "If these findings are solid, that great media attention is definitely warranted; if peer review would, however, reveal weaknesses or issues, all the current media reporting is premature," he argued.

From cell to manufacturing platform

Adamala sees SpudCell as a blank slate for engineering. "We believe that if we make a cell from scratch, that's fully engineerable," she said.

Cells have long been used to produce chemicals for human use. Millions of people use synthetic insulin made in bacteria and yeast cells, for example. But cells resist making chemicals that could be harmful to them, and through evolution, they've developed systems to prevent them from doing so. A SpudCell-like system could circumvent those natural hurdles, Adamala and her colleagues think.

That kind of platform could also be useful for making newer generations of medicines, such as those based on mRNA or peptides. These drugs use molecular building blocks, like amino acids or nucleotides, that have been chemically tweaked to make the molecules more stable or harder for the body to break down. SpudCell could be engineered to produce such modified components directly, rather than scientists having to synthesize them in traditional chemistry labs. This could potentially shorten development timelines and lower costs, the team thinks.

Adamala and her colleagues also envision the cells being used as easily shippable laboratories. They could be dried out, shipped, stored without refrigeration, and then activated on-site to make chemicals, vaccines or proteins when and where they are needed.

But there's still a long road ahead. For now, SpudCell is only a proof of principle, and many hurdles must be addressed before it could become an industrial platform.

"[SpudCell] is not an engineering platform that can give you any useful product, but it's step one," Adamala said. "It's probably at least a couple of decades from now when we can actually scale it up to the point where we can replace all the petrochemicals with biology, but I do believe it's doable."

Adamala hopes the nonprofit Biotic will help funnel donations from philanthropists directly to research. "Biotic is a funding agency that is going to globally fund this work," she said.

While the technology is promising, "it needs to go through peer review," Rinaldi said. "I expect a lot of the hype and some of the terms that they're using to go away after a couple of years have passed."

Deep in a limestone cave on Turkey's Mediterranean coast, archaeologists have uncovered evidence that Neanderthals and the modern humans who moved in later left behind surprisingly similar traces of their daily lives — evidence that they hunted the same animals, crafted the same stone tools and collected the same type of seashells.

The findings, published Monday (July 6) in the journal PNAS, feed into some of the biggest questions in human evolution: How similar were the cultures of Neanderthals and Homo sapiens, given that we're so closely related? And did we share information with one another?

A series of archaeological finds over the past few decades, including the new paper's finding that the two had similar cultural practices, suggests that Neanderthals and H. sapiens behaved far more similarly in the Middle East than once assumed.

The new evidence comes from Üçağızlı II Cave (pronounced Ooch-ah-UHZ'-luh), on a stretch of coastline just north of Syria that served as a prehistoric corridor between the Levant (an area of land east of the Mediterranean) and Eurasia. Although the team found only teeth and a partial jawbone within the cave, they were able to distinguish between the remains of Neanderthals and H. sapiens by analyzing the internal structure of the fossilized teeth. Meanwhile, they dated the sediment at the site using optically stimulated luminescence, a technique that reveals how long ago buried mineral grains last saw sunlight.

The team found that the Neanderthals had lived within the cave between approximately 77,000 and 59,000 years ago, while H. sapiens stayed there between about 59,000 and 47,000 years ago. Despite the different time periods, the layers from both of these periods show "substantially uniform hunting-gathering strategies and lithic technology," showing how similar the Neanderthals and H. sapiens were in their hunting-gathering strategies and stone-tool use, the team wrote in the study.

What's more, Neanderthals and H. sapiens got raw materials, such as flint, from the same local sources and hunted the same prey: wild goats (Capra aegagrus), fallow deer (Dama mesopotamica), roe deer (Capreolus capreolus) and wild boar (Sus scrofa). Layer after layer also turned up 29 shells of a small marine snail, Columbella rustica, carried into the cave not for food but seemingly as ornaments. Some were pierced as if meant to be strung, and one shell dating to the Neanderthal occupation showed signs of deliberate heating that altered its color.

"Our findings indicate a deep level of cultural interaction," study co-author Naoki Morimoto, paleoanthropologist at Kyoto University, said in a statement. "These two distinct but closely related human groups were not just adapting to the same environment: they were probably sharing symbolic preferences."

That pattern breaks from findings at Mandrin Cave in France, where Neanderthals and modern humans are thought to have alternated occupation in distinct pulses from about 56,800 and 41,500 years ago, but did not leave evidence of a continuous culture. Instead, it echoes evidence from Tinshemet Cave in Israel, where researchers recently reported similar signs of shared behavior between the two groups tens of thousands of years earlier, from about 130,000 to 80,000 years ago.

Üçağızlı II Cave in Turkey and Tinshemet Cave in Israel suggest that even though there was a "biological" turnover as the caves went from being occupied by Neanderthal groups to modern humans, there weren't major cultural turnovers, too.

"Rather, we hypothesize that the two human species that coexisted in the region were in contact and shared cultural aspects," the researchers wrote in the study.

"A fascinating region"

Sites like these are forcing a rethink of how these two types of human were culturally related to each other, April Nowell, a Paleolithic archaeologist at the University of Victoria in Canada who was not involved in the new study, told Live Science in an email. "By demonstrating cultural continuity and elevated levels of interaction, sites such as Tinshemet and Üçağızlı II are changing what we thought we knew about Neandertals, Homo sapiens and other contemporary Homo groups … a fascinating region just got even more so!" she said.

But that cultural continuity only heightens the mystery of how modern humans and Neanderthals interacted, with Neanderthals eventually going extinct around 40,000 years ago. Two types of human can't occupy the same ecological niche indefinitely, Nowell noted, and some research into Neanderthal cognition suggests Neanderthals were less-flexible thinkers than modern humans, with more limited capacity for language and less of the kind of self-awareness and creativity that may have given H. sapiens an edge. (However, there is pushback against the idea that Neanderthals weren't as cognitively complex as H. sapiens.)

If the archaeological record at sites like Üçağızlı II shows this much overlap in behavior, Nowell said, the real differences between the two may be ones the fossil record simply hasn't revealed yet.

The authors noted that many big questions remain, including when and where these shared cultural practices took place and whether these cultural similarities happened because modern humans mated with Neanderthals.

Ongoing and future excavations at sites like Üçağızlı II Cave may help to answer these questions and build a "more comprehensive picture of human evolution and cultural development during the Late Pleistocene," the team wrote in the study.

How much do you know about our closest relatives? Find out with our Neanderthal quiz!

Scientists uncovered a link between mild heart trouble and microscopic signs of brain damage that may raise the risk of memory problems down the line.

The new study, published Monday (July 6) in The Journal of Neuroscience, did not prove that the heart issues directly caused memory problems. But it "adds to the overall picture that preserving healthy brain-heart communication is key for healthy aging," said Dr. Jan Scheitz, a consultant stroke neurologist and head of the Brain-Heart Lab at the Charité University Hospital in Germany, who was not involved in the study.

"A healthy lifestyle that protects the cardiovascular system will not only benefit the heart but also the brain," he told Live Science in an email.

The work could one day help doctors identify patients at risk of memory problems early on through routine heart-function tests, said study co-author Dr. Xia Zhang, a doctoral researcher at the Max Planck Institute for Human Cognitive and Brain Sciences in Germany.

"The broader implication is that the brain may show subtle tissue-level changes related to cardiac dysfunction before we see obvious brain shrinkage or clinical dementia," Zhang told Live Science in an email.

Early warning signs

Researchers already knew that heart and brain function are closely interconnected. Heart diseases such as heart failure, atrial fibrillation and heart attack impair communication between the heart and the brain. This can contribute to thinking problems and dementia by restricting blood flow to the brain and causing chronic inflammation.

So far, though, scientists have only studied changes in the brain in people already diagnosed with heart conditions. They haven't necessarily assessed the changes that take place earlier on.

In the new study, researchers followed 73 patients who had sought care for heart-related symptoms at the Heart Center Leipzig in Germany, some of whom had confirmed coronary artery disease and/or heart failure. They also assessed 95 people without any heart-related symptoms. The researchers measured heart function at the start of the study. Then, about 3.5 years later, they performed cognitive testing and an MRI scan of the brain to take a snapshot of its structure.

Among all 168 study participants, those whose hearts pumped blood less efficiently at the start of the study showed greater signs of tissue damage in their gray matter years later. This was true regardless of whether or not they had diagnosed heart failure.

The cognitive tests were given only to the heart-disease patients, and they assessed attention, executive function, learning and memory. Only memory showed a link to weaker heart pumping. The participants with weaker heart pumping showed more microscopic damage in memory-related brain regions, and those brain changes correlated with worse memory scores.

The degree of brain damage also correlated with the levels of stress hormones released by the heart, but this link was only seen in patients who already had heart failure.

"What surprised us most" was that subtle reductions in the heart's ability to pump were tied to later brain changes, even in patients who did not meet clinical criteria for heart failure, Zhang said.

One limitation of the study is that the researchers didn't take MRI scans at the start. That means "we do not know whether some changes were already present at the beginning of the study period," Scheitz noted. This is something that Zhang and her colleagues plan to test in future studies.

"The next step for the field is replication in larger cohorts with multiple time points, so that cardiac function, brain microstructure, and cognition can be followed more precisely over time," she said.

The brain damage flagged in the 73 patients happened in parts of the brain that are important for memory and are vulnerable in Alzheimer's disease. "These regions helped identify a possible brain pathway through which poorer cardiac function may contribute to later memory problems," Zhang said.

However, until this idea is tested directly in future studies, it is too soon to say if the heart function-related brain changes seen on the MRI scans point to a higher risk of Alzheimer's, Zhang cautioned. The team did not measure proteins related to Alzheimer's, so they cannot conclude that the patients with measurable brain changes are developing Alzheimer's disease.

The study also did not directly test the effect of exercise on heart and brain health, but the findings may help explain why regular exercise is often linked to better brain health and cognitive aging, Zhang said.

"Regular exercise supports cardiovascular function, vascular health, and cerebral blood-flow regulation," she said, "all of which may help protect brain tissue over time."

This article is for informational purposes only and is not meant to offer medical advice.

What do you know about the body's hardest-working muscle? Find out with our heart quiz!

Scientists have found evidence that gravitational waves from a spectacular black hole collision carry signals from the very edge of the newly formed black hole. If confirmed by future observations, the discovery could provide an entirely new way to investigate what happens in the immediate vicinity of a black hole without ever observing it directly.

In a new study, the researchers analyzed an exceptionally strong gravitational wave event known as GW250114. They identified a "direct wave," a subtle feature of the total gravitational wave signal predicted by theory but never previously detected in real data. The signal appears to contain information from extremely close to the black hole's event horizon, the boundary beyond which nothing, not even light, can escape.

The findings, published June 24 in the journal Nature, suggest that gravitational wave observatories may eventually allow astronomers to probe regions that have remained inaccessible since black holes were first predicted by Albert Einstein's theory of general relativity.

Listening to the edge of a black hole

Although astronomers have photographed the glowing material surrounding some supermassive black holes and have detected dozens of black hole mergers through gravitational waves, the event horizon itself has remained frustratingly difficult to study.

Unlike ordinary light, gravitational waves are tiny ripples in space-time produced when massive objects accelerate. They pass almost undisturbed through the universe, carrying information about violent cosmic events that would otherwise remain hidden.

According to study co-author Sizheng Ma, a postdoctoral researcher at the Perimeter Institute for Theoretical Physics in Canada, the newly identified signal offers a rare glimpse of what happens immediately after two black holes collide.

"When two black holes merge, they violently shake space-time itself," Ma told Live Science. "For a brief moment, the region very close to the newly formed black hole's horizon is swept into a fast, fading swirl."

Ma explained that the direct wave is the portion of the gravitational wave signal produced near the horizon and carries the imprint of that motion outward through space.

"That is why it is so interesting," he said. "It may let us 'listen' to what happens near the horizon, a region we cannot see directly with light."

A remarkable black hole collision

The team focused on GW250114, a black hole merger detected on Jan. 14, 2025, by the two Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors in Hanford, Washington, and Livingston, Louisiana.

"Our earlier theoretical work predicted that black hole mergers should produce a direct-wave signal from the near-horizon region," Ma said. "The big question was whether this effect could actually be seen in real data."

GW250114 turned out to provide exactly the conditions needed to test that prediction.

"It was strong enough, clean enough, and close enough to the theoretical situation where this signal should be visible," he said.

To search for the elusive feature, the researchers first removed the best-understood part of the gravitational wave signal, which comes from the newly formed black hole settling down after the merger. Then, they examined the remaining data to determine whether it consisted only of detector noise or contained another physical signal.

"What we found was striking," Ma said. "The remaining signal followed the expected rhythm and fading pattern of a wave shaped by the region very close to the final black hole's horizon."

The team concluded that the leftover signal matches the behavior expected for a direct wave predicted by previous theoretical studies.

A new way to explore extreme gravity

The researchers stressed that their findings do not reveal what lies inside a black hole. Instead, they're providing a new observational tool for investigating the region immediately outside the event horizon.

"The gravitational wave data appear to carry an imprint from very close to the newly formed black hole's horizon — the famous point of no return," Ma said.

He explained that the measurements are consistent with space-time near the horizon being rapidly dragged around by the spinning black hole while the signal fades because of the intense gravitational field.

"For us, the exciting message is that gravitational waves may be giving us a new way to study the edge of a black hole using real observational data," Ma said.

Ma believes the method could eventually become useful for exploring ideas such as quantum gravity — which seeks to unite Einstein's theory of gravity with quantum mechanics — or the black hole information paradox, the longstanding puzzle of whether information that falls into a black hole is truly lost. However, it cannot test those questions directly yet.

"If quantum effects, or any deviations from the standard black-hole picture, leave a measurable imprint there, then direct waves could, in principle, help us search for them in the future," he said.

More observations will be needed

The researchers cautioned that the discovery is based on a single gravitational wave event. While GW250114 provided exceptionally favorable conditions, much stronger evidence will come only if similar signals are found in many additional black hole mergers.

"There are two main directions," Ma said. "The first is theory."

Current models capture the essential physics but remain simplified, and more realistic descriptions of black hole mergers will be needed.

"The second is observation," he added. "This result comes from one exceptionally loud and clean event, so the strongest confirmation would come from seeing the same kind of pattern in other black hole mergers."

As gravitational wave observatories continue to improve and detect increasing numbers of mergers, researchers hope to determine whether direct waves are a universal feature of black hole collisions.

"If the pattern appears repeatedly in the way general relativity predicts," Ma said, "direct waves could become a new way to study black hole horizons or the regions very close to them, and to test Einstein's theory in one of the most extreme environments in the universe."

If future observations confirm the team's results, scientists may have gained something they have sought for decades: a direct observational window into the very edge of a black hole.

See how much you know about black holes with our black hole quiz!

The patient: A 63-year-old woman in Massachusetts

The symptoms: The patient went to the emergency department after experiencing nausea and vomiting for about a month, along with decreased appetite. She told doctors that she'd also experienced a burning pain in her upper abdomen and right side of her torso, which wrapped around to her back. She'd tried treating these symptoms with two common over-the-counter medications for acid reflux, but the treatments didn't help.

In the year prior, the patient had started taking semaglutide, a type of drug known as a GLP-1 receptor agonist — the same class of drug as Ozempic. These injected drugs are used to treat type 2 diabetes and assist in chronic weight management; in this case, the woman had a history of type 2 diabetes and obesity. Since starting the medication, she'd lost about 40 pounds (18 kilograms), but notably, that weight loss had accelerated over the previous month, she noted.

What happened next: Doctors took a CT scan of the patient's abdomen and pelvis. This revealed that the bile ducts, which move bile from the liver to the gallbladder and small intestine, were slightly dilated. The woman also had "heavy stool burden" but no signs of obstructions in her bowels, and her stomach was slightly stretched out due to carrying "semisolid material."

To take a closer look, the medical team then used magnetic resonance cholangiopancreatography, a noninvasive scan that examines the bile ducts, gallbladder, pancreas and pancreatic ducts. The scan confirmed that the bile ducts were dilated and revealed a mass in the stomach that appeared to be trapped air. The doctors then examined the upper digestive tract, from the esophagus to the top of the small intestine, with an endoscope.

The diagnosis: The endoscopy revealed a large mass in the woman's stomach, known as a gastric bezoar. These masses are tightly packed blobs of partially digested or undigested materials.

The treatment: Semaglutide and other GLP-1 agonists typically cause delayed gastric emptying, which means they slow the rate at which the stomach empties its contents into the intestines. The woman was taken off that medication upon hospital admission.

The next step with a bezoar is to try and dissolve the mass while it's still in the stomach — and evidence suggests a good way to do this is to give the patient soda.

"Existing evidence, largely from case series and anecdotal experiences, supports the administration of 3 liters [0.8 gallons] of cola, either orally or through a nasogastric tube, within a 12-hour window," doctors noted in a report of the case. "It is not well understood whether acidity, carbonation, or another mechanism accounts for dissolution of the bezoar."

Due to the patient's history of diabetes, she was given diet cola. She also didn't enjoy carbonated beverages, so the typical prescription of 3 liters of soda was cut down to 1.5 liters (0.4 gallons). On the second day after starting this treatment, the patient noted a "tugging" sensation in her abdomen followed by relief of her nausea and abdominal discomfort. An endoscopic exam revealed that the bezoar was no longer stuck in her stomach.

The woman then transitioned to a typical diet in the hospital, and by the time she was discharged, she had no nausea, vomiting or abdominal pain. She did not restart semaglutide but was prescribed acid reflux medication to take daily. She reported that her appetite increased after hospital discharge and her weight rebounded a bit over the following months. Her abdominal symptoms had not returned within a few months of discharge.

What makes the case unique: Gastric bezoars are fairly rare, the report noted. They are found in less than 0.5% of endoscopies of the upper digestive tract. Common symptoms of the condition, such as pain, nausea, vomiting and abdominal discomfort, also appear in many more-common disorders, so they don't necessarily point to the presence of a bezoar in all cases.

The most common type of gastric bezoar is formed of plant fibers and called a "phytobezoar." Eating lots of certain foods, such as persimmons, pineapples, raisins or celery, can raise the risk of phytobezoars because the plants contain a high concentration of indigestible components, such as cellulose, lignins and certain tannins.

However, various medical conditions, procedures and drugs can also raise the risk of bezoars. These include anatomical changes related to bariatric or other gastric surgeries, autonomic nerve damage, and medications that cause delayed gastric emptying, such as GLP-1s. In the woman's case, semaglutide was likely to blame for her bezoar, and discontinuing the treatment helped resolve the problem.

The cola she consumed also helped. Although that course of treatment sounds strange on paper, it is the preferred first-line treatment over using a scope to physically break up the bezoar in the patient's stomach.

"Bezoars formed from food material may be initially managed with oral administration of cola in patients in a clinically stable condition," the report said. "This intervention is generally cost-effective and is associated with a lower risk of complications than invasive procedures."

For more intriguing medical cases, check out our Diagnostic Dilemma archives.

This article is for informational purposes only and is not meant to offer medical advice.

This article was first published Oct. 15, 2025.

Astronomers have reconstructed the "skeleton" of the cosmos in unprecedented detail, thanks to the largest-ever survey conducted by the James Webb Space Telescope (JWST). The resulting map reveals how galaxies have evolved since the universe's infancy around 13 billion years ago and how they fall together in a vast structure called the cosmic web.

The cosmic web is the largest known structure in existence, home to countless galaxy clusters and clusters of clusters. It is the framework of the universe, a scaffolding of gas filaments, stars, voids and sheets of dark matter that trace the entire large-scale organization of the cosmos.

In a paper published May 6 in The Astrophysical Journal, an international team of astronomers, led by researchers from the University of California, Riverside (UCR), utilized a treasure trove of JWST data to reveal how the universe has evolved.

How to sculpt a universe from scratch

The new research shows how intrinsic and extrinsic factors influence the formation and death of stars — and, therefore, galaxies and galactic clusters — throughout vast swathes of cosmic time.

Yet in what may seem like a wistful twist, the peak era of star formation is many billions of years behind us. The new research offers additional evidence of how the universe's structural framework facilitated this transition.

"We show how the cosmic web helped shape galaxy growth before, during, and after that peak era," study co-author and UCR astronomer Hossein Hatamnia told Live Science via email. "At earlier times, dense regions appear to be sites of rapid galaxy growth, while at later times dense environments are associated with the shutdown of star formation."

Such revelations come courtesy of COSMOS-Web, the grandest JWST survey yet: a 255-hour program spanning a contiguous area of the sky about the size of three full moons.

Compared with the previous COSMOS2020 survey, shared in 2021 and conducted by the Hubble Space Telescope and other facilities, the JWST-derived COSMOS-Web boasts better redshift precision and includes more galaxies — including fainter, lower-mass and more-distant objects. (Redshift is a measure of cosmic distance and time based on how light shifts to redder wavelengths as it crosses the universe.)

Compared with the JWST-derived image below, which shows a slice of the cosmos as it appeared 11.5 billion years ago, previous cosmic maps were sparser, more diffuse, and lacking in cosmic structures.

Additionally, the older COSMOS2020 survey tended to overestimate the depth in especially dense cosmic regions, where galaxies grow earlier and larger, and underestimate the depth of the least-dense spatial regions, the researchers said.

Revealing celestial birth and death

Yet JWST's cosmic map preserves the relative contrast across cosmic regions. It also shows that "massive galaxies in dense environments are more likely to be quiescent" — dying and quenched of their star-forming potential.

This may be because those galaxies are too massive, the team theorized. Once the dark matter halos that anchor galaxies grow to 1 trillion solar masses, they energize gas and prevent it from forming new stars. Additionally, active supermassive black holes quench star formation by energizing gas with their lethal, near-light-speed jets.

Such "mass-related" star-killing mechanisms dominated up to around 7 billion years ago — around half the age of the universe, the team found.

In the more recent universe, star formation is dominantly quenched by the environment around galaxies, which may strip them of material or prevent cold gas from accumulating and coalescing into stars.

Thanks to JWST's capabilities, the large-scale structure and evolution of the universe have been made clearer than ever, resolving blurry blobs into dim, ancient galaxies.

"The jump in depth and resolution is truly significant, and we can now see the cosmic web at a time when the universe was only a few hundred million years old, an era that was essentially out of reach before JWST," co-author Bahram Mobasher, a distinguished professor of physics and astronomy at UCR, concluded in a statement.

The catalog of 164,000 galaxies used to build the map of the cosmic web is publicly available.

This article was first published May 18, 2026.

This small, abstract sculpture of a woman, carved from milky-white marble, is known as The Stargazer because her head is tilted back and her eyes appear to stare skyward. Only about 30 figurines of this type have ever been found; all of them date to about 3000 B.C. and were crafted by a culture that left no written records of the figurines' meaning, according to art historian Amanda Mikolic.

This particular stargazer figurine was once owned by philanthropist Nelson Rockefeller, a member of the wealthy industrial family and vice president of the United States under Gerald Ford. It is now in the collection of the Cleveland Museum of Art (CMA).

The marble figurine is roughly 6.8 inches (17.2 centimeters) tall and weighs about 1 pound (454 grams). Clearly carved into human form but lacking a mouth, the statuette likely represents a woman, with the incised lines below the waist representing her pubic triangle. Her large, oval head is tilted back, and her tiny, dot-like eyes look upward.

Most stargazer figurines that have been discovered in western Anatolia (present-day Turkey) were broken at the neck before being buried in the ground millennia ago, making the CMA example one of the finest and most complete stargazer statuettes ever found.

But the meaning of the woman portrayed in The Stargazer figurine is unclear, since the culture that created it did not leave any written language explaining their art.

The figurine cannot stand on its own, suggesting that it was meant to be held or placed flat, according to Mikolic. "Deliberately rendered as female, she may be associated with fertility and abundance," she wrote. The statuette may be part of a trend of simplistic female figurines in the Mediterranean area linked to female fertility and the life cycle, such as the Cycladic figurines, according to The Getty, which has a stargazer figurine in its collection.

Regardless of the woman's specific meaning, "she must have been an important devotional object to some long-lost culture," Arielle Kozloff, former curator of ancient art at the CMA, wrote in the CMA Members Magazine.

Abstract female figurines like The Stargazer and other Neolithic examples are known to have inspired early-20th-century cubist masters, Kozloff wrote. This gives her "a sense of timelessness," according to Mikolic, "encouraging the viewer to think of humankind’s place and role in a larger cosmos."

For more stunning archaeological discoveries, check out our Astonishing Artifacts archives.

Can you put together last week's Astonishing Artifact?

A simple method to thicken Arctic sea ice has shown promising results in its very first field experiment, performed in Cambridge Bay, Nunavut, Canada.

Researchers are considering several controversial geoengineering techniques to slow the catastrophic melt of Arctic sea ice, including stratospheric aerosol injection, which involves shooting tiny sulfur particles into the sky to blot out the sun. But in a new study, scientists evaluated the merits of a much safer and more straightforward approach: pumping seawater onto existing sea ice in winter and letting it freeze into a reinforcing layer.

Known as sea ice thickening, this method has been used by Nordic and Arctic communities for decades, and ice hockey rinks employ a similar technique to keep their ice sturdy, two of the study's authors told Live Science in an email.

"Practical applications [that already exist] include building ice roads and creating platforms for offshore oil exploration," said Edward Blanchard-Wrigglesworth, a research associate professor in the University of Washington's Department of Atmospheric Sciences, and Andrea Ceccolini, an honorary professor at University College London and the CEO of the startup Real Ice, which studies artificial sea ice thickening methods and receives funding from the U.K. government.

Modeling work hints that sea ice thickening could become a climate adaptation tool for Arctic communities by limiting coastal erosion near towns, facilitating travel and supporting animal migrations and hunting.

Now, researchers have assessed the method's efficacy in the field for the first time. Their results, published May 22 in the journal Earth's Future, indicate that both the thickness and brightness of sea ice can be enhanced significantly on small scales — making the ice more reflective, and therefore more resilient to melting.

In the experiment, the team set up eight test areas and three control sites in Cambridge Bay during the winter of 2024 to 2025. Using submersible pumps that each consume less power than a toaster, they flooded the test areas either once or twice with up to 8 inches (20 centimeters) of seawater, while the control sites were never flooded. In spring, one control site was used for a melt pond drainage experiment, which involved drilling small holes in the ice to remove meltwater and expose the brighter ice underneath.

Overall, the test areas grew up to 12.6 inches (32 cm) thicker than the control sites by the end of winter, which is roughly equivalent to the ice thinning that has happened in the Arctic over the past 50 years, according to the study. Test areas that were flooded twice showed greater thickening than those flooded once. And in the melt period from late May to September, sea ice in the test areas appeared brighter and had slower melt rates, remaining thicker than the ice in the control sites. The melt pond drainage experiment also resulted in brighter sea ice than the other control sites.

When water is pumped onto sea ice, it saturates the snow that sits on top of the ice. "The snow-water mixture freezes into a new layer of ice, while the reduction in snow insulation allows colder atmospheric temperatures to accelerate natural ice growth from below," Blanchard-Wrigglesworth and Ceccolini explained.

Thicker sea ice is usually brighter than thin sea ice, which boosts the amount of sunlight that is reflected back into space. "The broader implication is that these effects could enhance the Arctic's reflectivity through both increased surface brightness and longer-lasting sea ice," the researchers said. "If similar results could eventually be achieved at larger scales, increased Arctic albedo could contribute to regional cooling, with potential knock-on benefits such as slowing permafrost thaw and reducing ice loss from Greenland."

However, there is still a big question mark over how scalable and economically viable sea ice thickening is, given that it requires people and machines working in the field. According to a 2016 study, 10 million wind-powered pumps would be needed to cover just 10% of the Arctic Ocean, and 100 million to cover the entire Arctic. "It is reasonable to ask whether such an endeavor is financially feasible or even logistically possible," the authors of that study wrote.

Yearly sea ice extent in the Arctic has shrunk by 20% since 1979, and this loss is accelerating with global warming. Therefore, if we want Arctic sea ice thickening to work at a large scale, "the pumps must be deployed almost immediately, while there is still a sufficient area of sea ice over which to flood," researchers wrote in a 2021 study.

The ecological and social impacts of Arctic sea ice thickening are not well understood, and further research will delay deployment, meaning it might be too late to roll out sea ice thickening by the time scientists have the data they need to ensure its safety and feasibility.

For these reasons and others, including governance issues and high maintenance needs, "sea-ice thickening is simply not feasible for use at a scale and at a rate that would be meaningful for sea ice protection," researchers wrote in a review published last year.

Deployment on anything but local scales would be challenging, Blanchard-Wrigglesworth and Ceccolini agreed. Nevertheless, the researchers said their most recent winter trials, which have yet to be published, showed encouraging results. In those trials, the sea ice in test areas grew 20 inches (50 cm) thicker than in control sites, The Guardian reported.

"We expect to have a clearer picture once the current melt season is complete," the researchers told Live Science. "In parallel, we are developing underwater robotic technology that could support autonomous deployments. Earlier this year, we conducted the first Arctic field tests of a prototype re-icing drone in Finland."

The drone is currently being refined in collaboration with the BioRobotics Institute in Pisa, Italy, according to The Guardian.

Artificial Intelligence (AI) is continuing to have a disruptive impact on ever more parts of humanity. But what does it mean in the long run? A new paper, available in pre-print on arXiv from Austrian researcher Sergey Ivliev, extrapolates what the wide scale adoption of AI means for the future of humanity in space — and in particular what it means for the ultimate question of whether we're truly alone in the galaxy or not.

A framework for much of the search for extraterrestrial intelligence came from famous physicist Enrico Fermi, who simply asked "Where is everybody?" at a lunchtime discussion at Los Alamos in the 1950s. Though never officially published, Fermi's lunch partners from that day have passed down an oral history of that conversation that has cemented it into the Search for Extraterrestrial Intelligence (SETI), at least until Michael Hart formally laid out the argument and mathematics for the underlying question in a paper in 1975.

There are plenty of potential answers to the Fermi Paradox, many of which can be found floating around the internet — and some are likely more valid than others. But Ivliev, a Ph.D. in Mathematical Economics and founder of environmental project consultancies such as Peatland Ecosystems and Vlinder, suggests a new resolution: the Quiet Expansion filter.

The central argument of the paper is that there aren't thousands of alien mega-structures lighting up the night sky because once a civilization reaches the threshold of Autonomous AI-Cosmoindustry (AICI), "loud", resource-hungry empires motivated by prestige or romance become irrational. However, this does not mean expansion stops; instead, it shifts to a "quiet" mode driven by rational goals like survival diversification, knowledge preservation, and scientific observation.

The AICI threshold is reached when a civilization possesses a self-sustaining off-planet industrial and computational system capable of designing, manufacturing, repairing and launching space hardware through AI-mediated autonomy. We're already taking tentative steps in this direction with the advent of space-based data centers, but true AICI —where a civilization can extend its infrastructure beyond its home planet without continuous biological intervention — is leaps and bounds beyond our current capabilities.

In this vein, Ivliev is drawing on work done by astrophysicists Sergey Popov, who noted that a truly rational AI system would reject human-like motivations for space travel — such as romance, conquest, or prestige. Instead, AI would view space expansion as simple risk management.

To an AI, putting all your eggs in one basket — whether that basket is a single planet, solar system, or even galaxy, can lead to a single point of failure. Therefore, expansion is highly logical as a way of mitigating the risk posed by that single point of failure. At the point where we have reached AICI, the cost for sending a 10kg interstellar probe to another star at 1% of the speed of light is roughly 4.5x10^13 Joules — a tiny fraction of the overall energy budget of such a civilization.

One key aspect is that the 10 kg probe doesn't contain any actual people — it simply holds the "seeds" to restart life elsewhere in case a catastrophe happens back in the home system. It would contain a civilization's knowledge, and possibly some of its biological material, enabling a sufficiently advanced AI to rebuild the entire civilization from scratch. This is the "Quiet Expansion" where an AI sends low-mass and hard to detect "seed systems" instead of moving millions of biological entities around in massive interstellar space ships.

There are some additional constraints on this method of expansion, including selecting promising exoplanets discovered by remote sensing and deploying minimal local resources to maintain themselves until needed. Additionally, the AI would restrict self-replication of the probes in order to avoid any "grey goo" scenario with a probe attempting to take over entire swathes of the galaxy.

This has obvious implications for why we've never found "loud" technosignatures. In this scenario, a "null" result of being unable to find the thermal signature of a Kardashev-III scale civilization doesn't mean a galaxy is empty. It just means that the successful civilizations are residing in a "quiet" state in case its back-up plans are needed.

But there's another, more ominous implication from this framework. If interstellar backups are cheap to make, and we haven't found any in our own backyard, that means either we're one of the first civilizations to make it to that point or the transition from a planetary industrial society to a space-based one is a narrow path to tread. Admittedly the probes such civilizations would send out are probably hard to find even in our own solar systems, but if we're unable to, it means we're ending uncharted territory — and might just run into a filter that had silenced the rest of the galaxy. That's a sobering thought, but one to keep in mind as we start to advance our own AI capabilities.

The original version of this article was published on Universe Today.

Are you a UFO fanatic? Find out with our extraterrestrials quiz!

NASA has marked the 250th birthday of the U.S. with a striking new collection of cosmic images from its Chandra X-ray Observatory, presenting four deep-space objects in red, white and blue.

The image set combines X-ray data from Chandra — which has been orbiting Earth since 1999 — with observations from NASA’s Hubble and James Webb Space Telescopes (JWST), as well as multiple ground-based observatories. Together, the images showcase some of the universe’s most dramatic environments, from the remains of an exploded star to a massive galaxy cluster shaped by dark matter — each rendered in patriotic colors.

Arguably the image most reminiscent of Fourth of July fireworks is that of Cassiopeia A, a famous supernova remnant about 11,000 light-years away in the constellation Cassiopeia (top left). Chandra’s X-ray data, shown in blue and purple, reveal the blast wave from a massive stellar explosion and trace elements such as iron, calcium and oxygen. Meanwhile, infrared data from JWST has been overlaid in red and white, highlighting the expanding shell of debris and cosmic dust. It’s all the result of a massive star that exploded about 340 years ago, according to NASA.

On the top-right is NGC 3603, a giant nebula 20,000 light-years away in the Carina spiral arm of the Milky Way. Here it appears as a glowing field of highly active, newly formed stars. Chandra’s X-ray observations reveal the light coming from the nebula, while Hubble data in optical, infrared and ultraviolet light show its glittering array of stars, as well as dust and gas. NGC 3603 is the largest nebula seen in visible light in our galaxy.

NGC 4736, also known as M94, is something else entirely. Pictured bottom-right, it’s a spiral galaxy about 19 million light-years from Earth in the constellation Canes Venatici. Its famed for the faint arms outside of its oval-shaped core region — known as a "starburst ring," where new stars are forming. It’s shown here with Chandra’s X-ray data layered with visible-light imagery captured by ground-based astrophotographers.

The final image features ZwCl 0024+1652 (bottom-left), a distant galaxy cluster where Hubble data has helped astronomers infer the presence of dark matter. About five billion light-years away in the constellation Pisces, Chandra’s X-rays reveal a vast reservoir of superheated gas in ZwCl 0024+1652 — shown in red — that contains more mass than the cluster’s galaxies combined.

The release of the new photos also includes novel sonifications for NGC 3603, NGC 4736 and ZwCl 0024+1652, transforming astronomical data into sound. The project allows audiences to experience space through both sight and hearing.

See more space photos of the week:

With violent conflicts happening across the world right now, war feels like a permanent condition. But have humans ever lived without war?

The answer depends on how you define "war." If war means a fight between two governments, then yes, there have been peaceful periods "because for nearly 99% of human history, there were no governments," said Ian Morris, a historian at Stanford University and author of "War! What Is It Good For? Conflict and the Progress of Civilization from Primates to Robots" (Farrar, Straus and Giroux, 2014).

Violence, on the other hand, has always been with us. If the question becomes "Have people ever lived without violence?" then "the answer is pretty clearly no — people have always fought and killed each other," Morris told Live Science in an email.

The theory of a peaceful prehistory

According to a review of studies published in 2022, war was rare or nonexistent in early human history when people lived as nomadic hunter gatherers. Peter Stearns, a professor emeritus of history at George Mason University and author of "Peace in World History" (Routledge, 2014), agrees with this idea. There was "little or no war in hunting and gathering [cultures] before the rise of agriculture," he told Live Science in an email.

This idea is based on archaeological records. Researchers examining ancient human bones from around the world have looked for skeletal evidence of war injuries, for instance of multiple individuals with unhealed wounds from stabbing, slicing and blunt force trauma who were buried in mass graves. However, they found little evidence of war injuries before 8000 B.C. After that, when humans began transitioning from nomadic life to permanent settlements, such injuries appeared widely.

This doesn't mean that lethal violence was absent in prehistoric societies. Researchers in Kenya found 27 skeletons dating to 10,000 years ago at the archaeological site of Nataruk; these skeletons show signs of violent death, which some anthropologists interpret as evidence of intergroup violence among early hunter-gatherers. And at Jebel Sahaba, a prehistoric cemetery in Sudan, archaeologists unearthed 13,000-year-old remains bearing signs of intergroup attacks.

But these cases of interpersonal violence don't count as war, because of how researchers usually define it. "Researchers who focus on war as a specific category of violence usually define it by saying it has to be violence organized by a government or else collective violence that kills more than a certain number of people," Morris said. "Prehistoric societies rarely had formal governments and hunter-gatherer bands rarely had more than a few dozen members, so if you define war as a conflict run by a government or one that kills >100 people, then by definition there can't have been wars in [early] prehistory."

David Christian, a historian and professor emeritus in the Department of History and Archaeology at Macquarie University in Australia, echoed this idea. "For much of human history communities were so small that it is not clear if we can equate violence with war," he told Live Science in an email. "I guess we can say that humans have always been capable of violence and as communities got larger that violence began to take on forms that we might want to describe as 'war.'"

Peace between rival powers

Once large kingdoms and empires appeared, war became very common. A doctoral thesis written by Jared Morgan McKinney, now an assistant professor of international security studies at Air War College in Alabama, focused on periods of peace between major powers. He concluded that war was basically the norm throughout history and that famous "peaceful" eras, like the Pax Romana (Roman Peace), usually just meant one powerful group had beaten everyone else into submission.

But there were exceptions. "Wars are expensive and risky," said Peter Frankopan, a professor of global history at the University of Oxford. "So in many periods in history, stability and peace have been achieved by rivals, adversaries and neighbors being able to match each other's capabilities."

McKinney's thesis identified several periods when rival powers managed to avoid war.

From around 1400 to 1200 B.C., the big powers of the ancient Middle East — mainly Egypt and the Hittite Empire, an ancient civilization in modern-day Turkey — went through two unusually long stretches without major wars. Peace was possible because the "Great Kings" recognized one another as equals and settled their territorial and political differences through formal treaties rather than war.

For most of their history, Rome and Persia were at war. Then, from roughly A.D. 387 to around 501, the two superpowers mostly stopped fighting. Historians call this the "Long Fifth Century" and have put forward many explanations for this period of peace, including that both sides faced serious outside threats that made fighting less affordable and that the two sides developed a language of "brotherhood" that acknowledged each other as equals rather than enemies, McKinney wrote in his thesis.

Between roughly A.D. 1000 and 1200, the rich Song dynasty in China secured peace with its militant northern neighbors ‪—‬ the Liao and the Jin‪ —‬ by paying them regularly to keep the peace. Although these monetary gifts (or bribes) looked like weakness, the payments were tiny compared with what China was earning through trade, according to McKinney.

Another example, according to Morris, is the "long peace" between China, Korea and Japan between about 1600 and 1850. While European states spent those centuries competing for power and territory through war, the East Asian states lived in relative peace. "In Europe, we've tended to be a lot more aggressive and competitive — which gives the impression that war is a 'natural state' of being," Frankopan said.

A notable period of relative peace in North America was the Long Peace among the Iroquois nations, McKinney told Live Science in an email. For roughly three centuries, from about 1450 to 1777, five (and later six) Native American nations who had previously engaged in violent and costly conflict forged a peaceful relationship known as the "Haudenosaunee Confederacy" or "League of Five Nations."

In South America, McKinney pointed to the South American Long Peace. This refers to the absence of major interstate wars between sovereign nations in South America ever since 1935.

"War is 'normal' in history," McKinney said. But, as these examples show, "patterns have exceptions."

Can you identify these historical objects of war? Test your smarts with our weapons of the world quiz.

Want to speed up your recovery after an injury or a workout? Some influencers are fans of shots of BPC-157 and TB-500 for that. Want scar-free, youthful skin and thick hair? Reddit posts rave about GHK-Cu and KPV. Want to build beautiful, bulky biceps? Some fitness influencers swear shots of ipamorelin will do wonders. This is the world of peptides — an assortment of chemicals that promise to boost your body and health — and people are self-injecting them in a growing wellness trend.

Promoted by bodybuilders and influencers, supporters of the "Make America Healthy Again" movement and Silicon Valley early adopters, peptides promise results that leave people better than well, fitter than fit. Yet despite getting glowing reviews on social media, most peptides have limited clinical evidence to support health benefits, whether it's helping to heal a rotator cuff injury, improving libido or building muscles. There's not much information out there on the drugs' effectiveness and even less on their safety.

In 2023 the Food and Drug Administration banned several peptides, including BPC-157, GHK-Cu, KPV and ipamorelin, from being produced in the U.S. by compounding pharmacies — facilities that legally make non-FDA-approved medications for individual use — because of "significant safety risks." Many peptides are imported from outside of the country, and many made here are marketed for research use only. People who desperately want the promise contained in the tiny vials seek them out on online on legally dubious gray markets.

But accessing the shots might soon get easier. On the podcast The Joe Rogan Experience on February 27, Robert F. Kennedy, Jr., secretary of the Department of Health and Human Services, proposed legalizing the compounding of 14 peptides — and the FDA seems poised to grant his wish. Earlier this week the agency released plans to hold a meeting with independent advisers in July to review whether some U.S. pharmacies should be allowed to manufacture certain peptides, including BPC-157, TB-500 and KPV.

If the lift on peptides happens, a flood of people could start using the drugs, regardless of any safety concerns.

A Peptide by Many Names

A peptide is a chain of two or more amino acids — building blocks of proteins. The body's cells can produce numerous peptides, which perform various tasks or serve as signaling molecules.

Insulin is a peptide. So is human growth hormone — and semaglutide, the active ingredient in glucagonlike peptide 1 (GLP-1) receptor agonist drugs such as Ozempic and Wegovy. (GLP-1s are FDA-approved for managing type 2 diabetes and for weight loss). Buzzy new injections such as BPC-157 and GHK-Cu — touted for tissue repair — are derivations or synthetic versions of naturally occurring peptides. The public and online health retailers are starting to use "peptides" as a catchall term for any chemical taken for well-being, energy, exercise recovery, and more, says Luke Turnock, a criminologist who studies how people use enhancement drugs at the University of Lincoln in England.

And while people are using them as treatments, peptides aren't often described as drugs. "'Drug' has a certain stigma or negative connotation attached to it," Turnock says. The popularity of peptides has its roots in the bodybuilding and powerlifting communities, he explains, where "drug" has historically been tied to steroids — which are generally banned for professional athletes.

The term "peptides," meanwhile, stresses the natural origin of the molecules, says Flynn McGuire, who studies sports medicine at the University of Utah. "Because it's 'natural,' it is better or different, even though they're just drugs," McGuire says.

A Surge in Popularity

In the past few years, orthopedic surgeon Omar Rahman has seen a spike in interest in peptides. "I'm seeing more patients asking about peptides, often driven by the longevity and wellness space," says Rahman, who practices at Pacific Coast Sports Medicine in Los Angeles.

Because peptides encompass many products — some available by prescription, others on the gray market — the exact number of people trying them is hard to pin down. The subreddit r/peptides currently has more than 70,000 weekly visitors, and the related subreddit r/biohackers, which frequently hosts conversations on peptides, has more than 600,000. A scroll through TikTok offers pages of people sharing their "stacks" — combinations of injections people take to meet their personal goals, from muscle-building and exercise recovery to increased brainpower or a better tan.

"The real cultural tipping point in my mind seems to have been around 2022, when the GLP-1s really blew up," says Turnock, who is researching the peptide boom. He says injecting drugs became "normalized" when GLP-1 drugs approved to treat diabetes, such as Ozempic, were also shown to be effective for weight loss — and eventually became an approved treatment for obesity.

Some are turning to peptides because they feel doctors aren't giving them the help they need, says Dan Cushman, a sports medicine doctor at the University of Utah. Injuries to certain tissues, such as tendons, "are very slow to heal" with conventional treatments, he says. Mainstream treatment can also be expensive and painful. To someone desperate for relief, peptides might seem worth a try.

Peptide use is also linked to a growing interest in health autonomy, Turnock says. This is the idea "that doctors, if they're not prescribing what you ask for or they're not offering you these solutions, are acting as a barrier to your good health."

Stacking Up

McGuire, Cushman and colleagues published a review last year on one peptide they encountered frequently: BPC-157. The peptide is promoted as a way to stimulate multiple cellular pathways involved in blood vessel formation, cell growth, muscle repair and inflammation. Their review, however, found that most of the evidence of such health effects was from rodent studies, and only three small pilot studies had looked at BPC-157 use in humans.

In a regimen called the "Wolverine" stack, many people combine BPC-157 with injections of TB-500, another peptide that is supposed to promote healing but has even less research behind it. The "Wolverine" stack is named after the rapidly healing X-Men character. Add injections of GHK-Cu and KPV, and the stack is called "glow" or "KLOW." People claim that GHK-Cu increases wound healing, decreases scarring and helps regenerate collagen — and that KPV, derived from a hormone naturally found in the body, reduces inflammation. GHK-Cu is found in blood plasma and is an FDA-approved ingredient in topical antiaging cosmetics — but it is currently banned as an injectable because of safety concerns, such as the risk of immune reactions caused by impurities.

For muscle-building, the peptides ipamorelin and CJC-1295 are advertised as stimulating growth hormone release. Both have little clinical evidence behind them, however. Some people stack ipamorelin with GLP-1 drugs to try to lose fat while building muscle, though the effects of taking these injections together have not been studied.

Use at Your Own Risk

Clinical trial data for most of these peptides are thin. Not only are the effects anecdotal, but so are the doses. FDA-approved drugs, Cushman says, have been tested and reviewed not just for their efficacy but also for their safety. There is very little existing information on most of these peptides, he says, let alone on what happens if they are combined.

In many cases, the provenance of these peptides is even grayer than the gray market would suggest. "Patients are accessing peptides through online vendors, wellness clinics and compounding pharmacies," Rahman says. "That variability in sourcing is one of the biggest concerns, particularly when it comes to purity, dosing consistency and overall quality control."

The FDA does not allow production of BPC-157, GHK-Cu, KPV and ipamorelin in the U.S., for example, by compounding pharmacies because of safety concerns, so people are ordering them from overseas — usually from China. Some are buying peptides labeled as "for research only." Not all are stuck in the legal gray areas; other peptides are available from compounding pharmacies.

In Kennedy's February remarks about his aim to allow compounding of more than a dozen peptides in the U.S., he suggested that peptides made within the country would be safer than ones acquired abroad.

"Americans deserve to know the quality of the products they are buying and deserve drugs that have been proven to be safe and effective," an HHS spokesperson told Scientific American in response to questions about Kennedy's comment and the timing of the lift. "The FDA's goal is to ensure that patients can obtain FDA-approved products, and when those aren't available or can't work because of a patient's unique situation, are made by licensed U.S. pharmacies."

But even if Kennedy's plan to make some peptides easier to compound in the U.S. is enacted, it does not necessarily mean the drugs are safe or effective. The FDA does not approve or review drugs from compounding pharmacies — it just monitors the active ingredients the facilities use.

If peptides become more readily available in the U.S. market, Cushman predicts, more "people are going to just start trying [them]" — whether there are data to back them up or not. The public may experience any benefits — and perils — of peptides before scientists quantify them in the clinic.

This article was first published at Scientific American. © ScientificAmerican.com. All rights reserved. Follow on TikTok and Instagram, X and Facebook.

This week's science news was all about goings on in space, with reports that the James Webb Space Telescope (JWST) picked up a signal from a mysterious, never-before-seen substance on Pluto and Titan.

The space telescope detected a specific absorption line in the spectra of these worlds' atmospheres, revealing the characteristic trace of a unique and unknown molecule. It's unclear exactly what the molecule could be, and the mystery is made even more compelling by the fact that the environments of Pluto and Titan are very distinct.

Farther afield, the JWST's predecessor, the Hubble Space Telescope, spotted "impossible" light from a galaxy we shouldn't even be able to see. And in the busy skies surrounding our own planet, scientists are dreaming up a scheme to drop a giant "airbag" that could protect us from solar storms, sending spacecraft into orbit to save doomed telescopes, and also giving answers to why metal sticks together in space.

And just in time for Independence Day weekend, the sun has launched a string of eruptions to Earth that will likely paint the night skies with colorful auroras.

China's 'Great Green Wall' grows faster than natural forests

66 billion trees have been planted in China's Great Green Wall — and they appear to be growing faster than natural forests

China is no stranger to engineering projects designed to bring its environment to heel; we've recently covered the Asian powerhouse's attempts to tame nature through the creation of atmospheric rivers, the world's biggest dam and water transfers. But these are hardly China's only forays into sculpting its natural environment, with the country having planted more than 66 billion trees along its northern borders to halt the advance of the Gobi and Taklamakan deserts.

Now, new research has revealed a startling detail about the trees in this "Great Green Wall": they're growing significantly faster than natural forests. Exactly why remains a mystery, but, as Live Science contributor Brian Owens reveals, it could be due to a stronger response from the trees to rising atmospheric carbon dioxide.

Discover more planet Earth news

—'It sounds so impossible': Student studying fungus that makes users hallucinate tiny people may be on the verge of a scientific breakthrough

—'Uncharted territory': Record high ocean temperatures confirmed for June as El Niño strengthens its grip

—Study suggests life on Earth has around 1.8 billion years left — but the biosphere might evolve to survive even longer

Life's Little Mysteries

Are CAPTCHAs obsolete in the age of AI?

Are you a robot? It used to be a question that only humans could answer — by clicking on traffic lights or strings of warped and grainy characters, or Completely Automated Public Turing tests to tell Computers and Humans Apart (CAPTCHAs). But what happens now that autonomous artificial intelligence (AI) agents can ace some of these trials without detection? Have they made CAPTCHAs obsolete?

—If you enjoyed this, sign up for our Life's Little Mysteries newsletter

Medici murder mystery solved

Ancient-DNA analysis solves 500-year-old mystery of what killed 2 Medici brothers

The Medici family ruled Renaissance Tuscany with an iron fist, fulfilling their ruthless ambitions with methods so underhand that the name of their most famous advisor, Niccolò Machiavelli, became a synonym for skulduggery.

So, when two brothers from the infamous family died under mysterious circumstances, it was believed for 500 years that they were murdered, possibly by arsenic poisoning. Now, science has revealed the true culprit behind the medieval cold case, and it's not what we expected.

Discover more archaeology news

—Ancient ring discovered underground in Scotland could be a Stonehenge-like monument

—500-year-old freeze-dried potato snacks discovered in Inca storage room in Peru

—2,000-year-old scrolls buried by Mount Vesuvius eruption finally deciphered with help from AI

Also in science news this week

—Chinese supercomputer leapfrogs best US machines to be ranked world's fastest

—The hantavirus outbreak is over, WHO declares

—Rise in cancer in younger adults may be explained by faster 'biological aging,' early study hints

—Dead-end bitcoin mining wastes as much energy as Switzerland's entire hydropower generation capacity

—CERN shuts down Large Hadron Collider until 2030, upgrading the atom smasher to its most powerful form yet

—Scientists figured out how to shrink huge ultrafast lasers so they fit on a tiny chip ‪‪—‬ the 'holy grail' of the field

Science Spotlight

Japan's bold experiment to curb antibiotic misuse has been a huge success. Could it work in the US?

Antibiotic resistance is a growing threat in the U.S., with more than 2.8 million Americans developing antimicrobial-resistant infections each year. The solutions to this worrying trend can be very complex— such as moving agricultural systems away from their overreliance on antibiotics, or preventing the rapid spread of superbugs through international travel.

But stopping doctors from overprescribing antibiotics is one of the easiest strategies in the battle against this "silent pandemic." And it turns out that Japan has already fought it with some success, driving down antibiotic overuse with an innovative new policy. To investigate further and ask what notes the U.S. should be taking, Live Science's health editor Nicoletta Lanese visited Japan and reported back on their investigation.

Something for the weekend

If you're looking for things to keep you busy over the weekend, here are a smattering of our best expert opinion pieces, alongside a crossword, an interview and a quiz, that we published this week.

— Computer scientists are rushing to tame AI's voracious appetite for energy [Opinion]

—'It's more than a hope, it's a guarantee': The Vera C. Rubin Observatory's 10-year movie of the universe is about to 'blow our minds,' chief scientist Tony Tyson says [Interview]

—Live Science crossword puzzle #50: Longest-serving president in US history — 1 across [Crossword]

—Ancient empires quiz: Can you match these lands to the historical powers that ruled them? [Quiz]

Science photo of the week

Bull's-eye! Enormous 'bow and arrow' galaxy is unlike anything radio astronomers have ever seen

If you ask me, it looks more like a rusty anchor, or a blurry deep-sea fish. But whichever way you see it, the newly discovered "bow and arrow" galaxy — or, more formally, the RAD-Bow-And-Arrow Radio Galaxy (RAD-BAARG) — is an oddball unlike any other recorded.

The galaxy's unique structure is likely the result of gravity, which is warping RAD-BAARG into a funhouse mirror version of its former self as it falls into a nearby galaxy cluster. A shock front from this plunge surrounds the galaxy as it moves through hot gas.

Follow Live Science on social media

Want more science news? Follow our Live Science WhatsApp Channel for the latest discoveries as they happen. It's the best way to get our expert reporting on the go, but if you don't use WhatsApp we're also on Facebook, X (formerly Twitter), Flipboard, Instagram, TikTok, Bluesky and LinkedIn.

A hefty "super Earth" lurking in one of the closest star systems to our planet may be much better suited to supporting extraterrestrial life than scientists initially thought, a new study suggests. The alien world's relative proximity to Earth, and the nature of its home star, make it a prime candidate for follow-up observations, researchers say.

The exoplanet, dubbed GJ 3378b, was discovered in 2024 and orbits a red dwarf star around 25 light-years from our planet. The alien world circles its star every 21.5 days at a distance around 10 times closer than Earth orbits the sun, which would make it completely inhospitable in our solar system. But because the red dwarf emits around 90% less radiation than the sun does, GJ 3378b is slap bang in the middle of this star system’s "habitable zone," where liquid water could exist on the exoplanet's surface.

Researchers initially thought that GJ 3378b was around five times more massive than Earth. If the planet is rocky like ours, it would qualify as a "super Earth" — often considered the best candidates for sustaining extraterrestrial life. However, it was hard to tell if this world had a solid surface or was actually a mini gas giant. And even if it was rocky, its immense size would probably mean that its atmospheric pressure would be crushing, making it less likely to harbor life.

But in a new study, published June 30 in The Astrophysical Journal, researchers recalculated the exoplanet's size, using the Habitable-zone Planet Finder instrument attached to the Hobby-Eberly Telescope at the McDonald Observatory in Texas. This device measures subtle wobbles in the host star, caused by the gravitational tug of orbiting planets, and can be used to calculate the planet’s mass and trajectory.

This revealed that GJ 3378b is actually only 2.3 times more massive than Earth, which almost guarantees it is a rocky world and means it could have an atmosphere with a similar pressure to our own, raising the chances that extraterrestrial lifeforms could thrive there.

While researchers have found several other exoplanets that could harbor life, the fact that GJ 3378b is so close to us makes it particularly intriguing, as it will be easier to confirm whether it is truly habitable.

"This one’s exciting," study first author Paul Robertson, an astronomer at the University of California, Irvine, said in a statement. "25 light-years sounds like a long way, but the Milky Way is about 100,000 light-years across, so in that respect it’s our next-door neighbor."

Before we get too carried away, there is still no evidence that GJ 3378b has an atmosphere or liquid water. Its proximity to its home star may mean that any atmosphere it once had was stripped away by stellar winds, similar to how solar radiation likely stripped Mars of its atmosphere and ancient oceans.

Therefore, more observations are needed. But if an atmosphere is detected, GJ 3378b would likely jump to near the front of the queue of exoplanets that researchers want to study further.

"If a planet in the habitable zone has a proper atmosphere, we can justify further research looking for biosignatures, liquid water or other signs of life," study co-author Gogod James, an undergraduate student at UC Irvine, said in the statement.

The fact that GJ 3378b orbits a red dwarf also makes it more appealing for future study because this is the most common star type in the Milky Way, so experts are keen to learn more about these stars' planetary systems and potential to nurture life.

"About 70% of stars in our galaxy are red dwarfs, so they represent the standard," study co-author Michael Endl, an astronomer at the McDonald Observatory and the University of Texas at Austin, said in another statement. "It’s really important that we understand the planet population around these stars."

When you click to enter a website or try to log in or fill out a form, you may be asked to identify motorcycles from a grid of grainy images, decipher a string of convoluted characters, or click a box that states "I am not a robot."

These tests are called CAPTCHAs, which stands for "Completely Automated Public Turing test to tell Computers and Humans Apart." As their name suggests, they are meant to help a website distinguish if an action is coming from a human or a bot, since the aforementioned tasks are theoretically easy for a human and difficult for automated software to perform. This, in turn, blocks bots from spamming comments, downloading files, taking over accounts, or executing any other action on a website.

But as computer models increasingly gain the ability to solve CAPTCHAs, thanks to advancing artificial intelligence (AI) — and with puzzles getting weirder and more difficult for humans to complete — does this mean CAPTCHAs are still useful?

CAPTCHAs were introduced in the late 1990s to address "a very simple, but very difficult problem," Andreas Plesner, a computer scientist at ETH Zurich, told Live Science. "If I don't interact with a person physically … is it a computer? Or is it human?" Some of the first CAPTCHAs, still common on websites today, were composed of distorted text, since text-reading software at that time had trouble interpreting warped words.

But over time, text-reading software improved and new types of CAPTCHAs were developed. For instance, reCAPTCHA, one of the most popular CAPTCHA services, has an image-based test that asks users to identify objects such as traffic lights, motorcycles or bicycles from a grid of Google Street View photos. This was developed after Google acquired the service in 2009.

"The bet was that recognizing objects in messy, real-world photos was still a uniquely human skill," Ng Chong, chief of information technology and director of United Nations University's Campus Computing Centre in Tokyo, told Live Science in an email.

As time went on, CAPTCHA design continued to advance. In 2014, Google came out with reCAPTCHA v2, which analyzed computer mouse behavior by asking people to click a checkbox to test if a user was human. If the behavior is deemed suspicious, determined by factors like how a user interacts with the site beforehand or the timing of their click, the street-image grid pops up as an additional puzzle.

However, more recently, technology has improved to a point where image recognition is no longer a human-specific skill. As early as 2016, researchers found that low-cost deep learning technologies could solve reCAPTCHAv2 around 70% of the time. By 2024, Plesner and his colleagues developed an AI model that could solve the puzzles correctly 100% of the time. Earlier in 2026, Chong noted that he built a tool that could mimic human-like browsing behavior and sometimes bypass reCAPTCHA v2 without triggering the image grid at all. When the grid was triggered, the tool used AI to solve it within a few tries.

"When both the challenge and the behavioral layer are defeated by commodity tools running on a single laptop, the fundamental premise of CAPTCHA, that there are tasks humans can do but machines can't, stops holding," Chong wrote.

Looking ahead

So does that mean CAPTCHAs are completely obsolete? Not quite. Although the model Plesner and his colleagues developed breezed past reCAPTCHAv2, "there were a lot of the safety measures that were not tied to being able to solve it, but more tied to how you solve it," he said. For example, while conducting their research, Plesner noted that his team used a virtual private network (VPN) that changed IP addresses for each test, since a single IP address with a high volume of solved CAPTCHAs faced tasks with increasing difficulty, or got blocked entirely.

Modern CAPTCHAs focus on these background clues and tactics, rather than the puzzle itself. This includes Google's reCAPTCHA v3, Friendly CAPTCHA, hCAPTCHA and Cloudflare's Turnstile, among others, which run without sending a puzzle at all. They instead look at whether the action is coming from a real attested device (rather than from automated code), whether an IP address has had a high volume of automated requests in the past, how a user navigates a webpage, what the user's cookie history is, and a slew of other factors to determine possible malicious intent.

As the tug-of-war continues, CAPTCHA puzzles are still widespread. After all, they’ve been the status quo for decades, are easy to set up and are relatively cost-effective, Chong said. But these tasks have some other drawbacks. Although bots can increasingly solve the puzzles with ease, CAPTCHAs can be a headache to get through for humans and can be seen as discriminatory against those with disabilities, notably visual disabilities, as a researcher noted in a 2022 conference paper.

The crescendoing complexity of CAPTCHA puzzles has even been the subject of parody, with developer Neal Agarwal creating a free satirical game called "I'm Not a Robot." Users must solve a series of increasingly convoluted verification checks — scoring a point for each stage they pass, which eventually transcend into the absurd.

So, as machines get smarter, the answer may not be to find more difficult puzzles. "If a CAPTCHA can only be solved by someone with a Ph.D. in mathematics, then it's not very useful," Plesner said. "The internet needs to be used by everyone."

Can you match these ancient devices to their pictures? Find out with our computing quiz!

The diminutive, now-extinct humans known as the "hobbits" were scavengers who dined on dwarf elephants after Komodo dragons took the best cuts, archaeologists have discovered. The finding upends the assumption that Homo floresiensis, a human species that arrived on the Indonesian island of Flores at least 700,000 years ago, hunted big game.

First discovered in 2003, H. floresiensis has been nicknamed the hobbit because of its small size, averaging around 3 feet, 6 inches (106 centimeters) tall, along with its small brain, large teeth and big feet. But archaeologists also found stone tools, animal bones with cut marks, and charred bones that seemed to add up to sophisticated behavior common within our genus, Homo. The hobbits disappeared around 50,000 years ago as Homo sapiens began spreading around Southeast Asia.

But in a study published Friday (July 3) in the journal Science Advances, an international team of researchers questions whether the behavior of H. floresiensis was really as advanced as previously assumed.

The researchers looked at fossil bones of Stegodon florensis insularis, an extinct dwarf species of elephant relative discovered at Liang Bua cave, where bones from H. floresiensis and stone tools have also been found, to determine whether the cut marks were from hunting Stegodon meat or from scavenging the remains of the feasts of the only other carnivore on the island: the Komodo dragons (Varanus komodensis).

To distinguish the hobbit cut marks from Komodo dragon tooth marks, the researchers first conducted an experiment, feeding a goat carcass to a captive Komodo dragon at Zoo Atlanta. Then, they recovered the goat skeleton and painstakingly documented all of the marks, pits, notches and furrows the Komodo dragon's teeth made in the bones. The tooth marks were concentrated in areas with substantial amounts of goat flesh, the researchers wrote in the study, suggesting the Komodo dragon had a preference for meaty areas.

The researchers then investigated the ancient Stegodon bones for evidence of cut marks made by H. floresiensis' stone tools and tooth marks from Komodo dragons. They found 54 cut marks on the Stegodon bones and nearly twice as many Komodo dragon tooth marks. More importantly, they discovered that the Komodo dragon marks were focused on meaty areas, while the human cut marks were made primarily in areas without a lot of meat, suggesting H. floresiensis did not hunt and kill the Stegodon.

The overall patterns of cut marks and tooth marks suggest "a combination of mostly primary access by Komodo dragons and secondary access by H. floresiensis where both predators consumed Stegodon," the researchers wrote. And the hobbits likely ate this meat raw, according to the researchers, as they found no evidence on the Stegodon bones that they had been cooked. Nor did they find any evidence of burning on over 4,000 mouse bones from the site, suggesting the previous evidence of charring was actually natural manganese staining.

A lack of hunting and fire-making technology suggests that the hobbits were not as behaviorally sophisticated as previously thought and raises questions about their ancestry, the researchers said.

It's possible that the ancestor of H. floresiensis branched from the Homo genus before humans accomplished the control of fire and hunting, study first author E. Grace Veatch, a paleoanthropologist at the University of Tübingen in Germany, told Live Science in an email.

One hypothesis for the origin of the hobbits is island dwarfism, which occurs when a large species' average body size evolves to be smaller over generations due to the limited availability of natural resources. Another theory is that hobbits descended from an earlier Homo species that was already small-bodied.

"I think our study highlights the importance of considering behavior in these debates," Veatch said. "Our study suggests that H. floresiensis evolved from a hominin population that did not require these dietary strategies [of hunting and cooking], such as a form of early Homo."

But the new study has not entirely settled the debate about the hobbits' ancestry, because very little is known about the behavior of early hominins in Southeast Asia, such as Homo erectus on Java and other areas of Sunda or Sundaland, a landmass between the South China Sea and the Indian Ocean that has been exposed off and on over the past 2.6 million years.

If H. floresiensis really did branch off from H. erectus, that would suggest many evolutionary changes occurred.

"Taking place on an island that was cut off from contact with the Sunda mainland, this evolution from Homo erectus to Homo floresiensis may have involved not just profound anatomical transformations, such as reduced body size and brain volume, but also behavioural adaptations," Adam Brumm, an archaeologist at Griffith University in Australia who was not involved in the study, told Live Science in an email.

"Flores was clearly a wild card in the story of early human evolution, the sort of place where almost anything could have happened — including, potentially, the loss of deeply-rooted hominin behaviours, such as hunting and fire use," Brumm added.

Where H. floresiensis fits in with the rest of the Homo genus is still an open question, Veatch said. "Importantly, this study highlights the contribution of taphonomy [the study of what happens to organic remains after death] to speak to these larger questions about ancestry."

What do you know about early humans? Test your knowledge with our human origins quiz!

The enigmatic Scythians, a diverse group of nomadic tribes known for their ferocity in battle, were organized around elite dynasties of powerful men and women over 2,500 years ago, a new DNA study finds. The results reveal that social inequality arose in these nomadic groups around 900 B.C., during the Iron Age.

Most of what archaeologists know about the Scythians comes from ancient Greek and Roman accounts of the accomplished equestrians and from their large, mound-shaped tombs, called kurgans, that dot the Eurasian steppe grassland. The Scythians' tattooed mummies and intricate, animal-themed jewelry were as well-known in ancient times as their women warriors, who may have inspired the myth of the Amazons. But the Scythians left no written records of their own and were likely absorbed by other cultural groups after suffering several military defeats around 200 B.C.

In a study published Friday (July 3) in the journal Science Advances, researchers sequenced DNA from 85 Iron Age Scythians to better understand how these geographically spread-out groups were related and how their society was politically structured. They discovered that elite family dynasties ruled the nomadic groups from centralized locations, revealing the origin of social inequality among the Scythians.

The researchers generated genomes from the skeletons of 38 elite and 47 non-elite people buried in kurgan tombs across 20 archaeological sites between 900 and 200 B.C. The non-elite tombs were smaller than the elite tombs, and they lacked the impressive weapons and gold artifacts of the elite tombs.

Based on DNA, the researchers discovered that elite people were 11 times more likely to be related to each other than they were to be related to non-elite people, suggesting there was a powerful extended family group that ruled the steppe nomads.

Among the elite, they discovered two pairs of biological brothers, a brother and a sister, and a parent and child. In one case, the two brothers were buried at different sites some distance apart. They also found two elite grandfathers and grandsons buried in different cemeteries. But the elite people were still buried closer together than the non-elite people were.

"It is possible that this indicates some degree of geographic centralization of the elite burials being on average closer to each other," study co-author Ainash Childebayeva, a genetic anthropologist at the University of Texas at Austin, told Live Science in an email. "For example, in Siberia there is an area known as the 'Valley of the Kings' that contains many large mounds that are likely elite of the similar time period as in our study."

The researchers also investigated the historical claim by Greek authors such as Herodotus that women held high-status positions.

"An important observation from our study was the noticeable presence of elite women," study first author Ayshin Ghalichi, an archaeogeneticist at the Max Planck Institute for Evolutionary Anthropology in Germany, said in a statement. "Nearly half of the elite individuals in our dataset were female, indicating that women held high social status within Iron Age Scythian society."

Mysterious "Golden Man"

DNA evidence also solved a long-standing question about the "Golden Man." This skeleton of a teenager, discovered in 1969 in a kurgan in Kazakhstan, was found with more than 4,000 gold ornaments and a silver bowl with an inscription that has never been deciphered. Although the skeleton's sex could not be determined based on the bones, experts assumed the person was a powerful male warrior, even though women held nearly equal power among the Scythians.

"Although the data we were able to generate is low coverage, we found that the individual was a lot more likely to be genetically male than female," Childebayeva said, but "we did not identify any relatedness for the Golden Man."

The young age of the Golden Man – 17 based on his bones – and his elite burial status together provide clear evidence of elite dynastic rule, Childebayeva noted. An additional example that is "even more striking" comes from the pairing of a grandfather and his 1-year-old grandson, both buried in elite kurgans, Childebayeva said. These burials of elite children reinforce the conclusion that Iron Age steppe nomads inherited their social status.

"The results presented here further our understanding of the rise of social inequality and differentiation among ancient Eurasian nomadic groups and highlight the practices of the earliest nomadic groups of Central Eurasia in the first millennium BCE," the researchers wrote in the study.

Can you identify these historical objects of war? Test your smarts with our weapons of the world quiz!

Fourth of July celebrations across the United States this weekend could be accompanied by light shows in the night skies, as a string of powerful solar eruptions appear set to strike Earth.

The sun has been especially hyperactive over the past few days — firing off 10 M-class solar flares over 24 hours that have been accompanied by multiple coronal mass ejections (CMEs), which are set to slam into Earth on July 3 and July 5.

CMEs are large, fast-moving clouds of magnetized plasma and solar radiation that occasionally get flung into space with solar flares when kinks in the sun's magnetic field snap. If CMEs smash into Earth, they cause disturbances in Earth's magnetic field, called geomagnetic storms, that can trigger partial radio blackouts and produce vibrant aurora displays farther away from Earth's magnetic poles than usual.

"Machine-Gun Sun! More than 5 storms on their way to Earth and 3 of them offer good chances for aurora views," Tamitha Skov, a space weather physicist at Millersville University of Pennsylvania, wrote in a July 2 post on the social platform X. "NOAA and NASA model predictions do not show all the storms yet (it's hard to keep up with the rapid-fire storm launches!) but the first should hit before noon July 3 UTC."

The CMEs are expected to give a glancing blow to our planet, creating conditions for a moderate (G2) geomagnetic storm, according to the National Oceanic and Atmospheric Administration's (NOAA) Space Weather Prediction Center. It's also possible that these storms will strengthen to become strong (G3), depending on how they interact with Earth's magnetic field.

Auroras resulting from G3-class geomagnetic storms are often visible in northern parts of Washington, Idaho, Montana, Wyoming, North Dakota, South Dakota, Minnesota, Wisconsin, Michigan, New York and Maine, according to NOAA. Skywatchers farther south in Oregon, Nebraska, Iowa, Illinois, Indiana, Ohio, Pennsylvania, Massachusetts, Connecticut, Rhode Island, Vermont and New Hampshire will also have a chance of catching the light show. In any case, skywatchers interested in seeing or photographing the auroras will need to get as far from artificial light sources as possible.

The weekend storms might not be the last activity we see from the sun in the coming days, as two gigantic sunspots currently pimpling its face are displaying "beta-gamma-delta" magnetic fields — the most tangled and unstable type. This means these sunspots harbor the potential to launch powerful X-class flares, according to spaceweather.com.

The last few years have seen a record number of powerful X-class flares explode from the sun's surface, hitting Earth with several major solar storms, including 2024's Mother's Day storm. This record comes partly from improvements to scientists' solar monitoring technologies, but also due to the sun reaching its 11-year peak in sunspot production, or solar maximum, in 2024.

Following this peak, the sun has now entered a period known as the "battle zone," a relatively understudied solar phase where instabilities across our star's newly flipped magnetic field ramp up the production of solar holes, gigantic, highly-tangled sunspots and subsequent geomagnetic storms.

The worst-case scenario for a solar storm is a superstorm like the 1859 Carrington Event, which released roughly the same energy as 10 billion 1-megaton atomic bombs. After slamming into Earth, the powerful stream of solar particles set telegraph systems around the world on fire and caused auroras brighter than the light of the full moon to appear as far south as the Caribbean.

The Carrington Event unleashed a roughly X45 magnitude solar flare that remains a record, yet it's likely far from the worst the sun can muster — with ancient tree rings harboring evidence of even more powerful blasts that occurred long before humans existed.

On a dark mountaintop in Chile, the world's largest digital camera has begun filming its masterpiece.

This Tuesday (June 30), scientists with the Vera C. Rubin Observatory announced that the facility's ambitious Legacy Survey of Space and Time (LSST) officially began. Every night for the next 10 years, the observatory's car-size LSST Camera will capture a 3,200-megapixel image of the southern sky — then another, then another, slowly filling in a mosaic of the universe 30 seconds at a time.

"In a sense, we're taking a digital color motion picture of the universe," Tony Tyson, a professor of cosmology at the University of California Davis and LSST's chief scientist and former founding director of the Rubin Observatory, told Live Science.

Strafing across the sky in stop-motion, the survey is expected to spot between 7 million and 8 million changes among the stars each night — from flashing supernovas and streaking comets to colliding galaxies and dim, tumbling asteroids. Within minutes of each exposure, alerts to any peculiar changes will become publicly available for astronomers and space enthusiasts around the world to study.

"Rubin is an automated facility, so scientists don't come here to use it," Tyson said. "But tens of trillions of observations is enough data for everybody in the world."

Tyson is hoping the firehose of data will unmask theinvisible 95% of the universe that is composed of dark matter and dark energy.

While there are still some technical bugs to work out — and the looming threat of ultra-bright corporate satellites to contend with — Tyson and his colleagues are ready to roll out the survey, "gradually increasing our sky area and image quality" over the next few months, he added.

Live Science spoke with Tyson about the LSST and what it may find in the coming years.

Brandon Specktor: You're about to spend 10 years observing the southern sky with the largest digital camera ever. What will a typical night of the survey look like?

Tony Tyson: In a sense, we're making a digital color motion picture of the universe. We'll take thousands of 30-second exposures every night. Within two minutes of the shutter closing on an exposure, we will process all the data, [compare] it from the archival sky of that piece of the sky, and — if something explodes, or pops off, or moves in the sky in a way we don't understand — issue an alert. The alerts go to the world.

I made the decision early on to make the data available to everyone. The alerts will also go to eight data brokers, which specialize in things like cosmology, supernovae, etc., and the public can sign up to the feed from their favorite brokers.

BS: Which feed will you be watching most closely?

TT: My most interesting data broker is one which will come up with a classification of "unknown." I'm more interested in the unknown, unclassifiable things that go on in the universe. But there's a sort of a live stream of catalog information that's going to be available to people — and we're excited for writing up a lot of new discoveries.

My hope at this time is that we will discover something unexpected that will revolutionize astronomy. I think it's more than a hope, I think it's a guarantee.

BS: What kind of revolution would that be? Is there one big question you hope Rubin will answer?

TT: I'm a cosmologist, so my hope is that we'll get closer to understanding the physics of dark energy and dark matter.

But to be frank, I think we'll be remembered 100 years from now for something else in addition. And discovering something totally new in the time domain, something that blows our minds, that we did not expect — some kind of new object that's out there. There's examples of this in radio astronomy with the FRBs [fast radio bursts], for example. And I think that that's going to be how we will be remembered.

BS: The Rubin Observatory observes in optical light. Are there any strange optical phenomena you have your eye on?

TT: There's already a pretty strong hint, actually, that there is a population of very faint bursting objects that just pop off. The ones we know about are typically pretty bright — supernovae, which last for a long time, and gamma-ray bursts, which are bright but they don't last very long. But there's a big question mark in this unique area that we're going to explore, of faint things that are very short-lived. And there's evidence now from a team in Japan that there is a population of very faint things that explode just once. They don't repeat. And so I'm keeping my eye on that.

BS: What are the Rubin Observatory's main science goals?

TT: There's a lot of areas of science that we can address — and that was really the main selling point for us with the agencies. For one, we'll be looking at cosmology and the history of the expansion of the universe. Just by itself, we will have enough data to measure key parameters in cosmology to eliminate models of dark matter and dark energy, which is exciting.

Another area is looking at new kinds of stars in our galaxy, so we can look at the history of our galaxy and the history of star formation in our galaxy. At even lower redshift, an interesting area is looking at both comets and potentially Earth-threatening asteroids. Every night we detect about a thousand new asteroids.

And we will be able to uniquely look for those, if we can get rid of the interfering low-Earth-orbiting satellites, which really make that impossible. And so I've been unfortunately sidetracked into worrying a lot about that in the recent year.

BS: Are you talking about companies like Reflect Orbital, which essentially want to put giant mirrors in low Earth orbit? We've written about how satellites like that could totally compromise the LSST.

Yes. There's a proposed class of extremely ultra-bright satellites that are going to be launched that are incompatible with the LSST science, totally incompatible. The skies will no longer be dark for anybody, anywhere.

Reflect Orbital is one example. The other example is these orbiting AI [artificial intelligence] computational centers, which will be exceedingly bright. We've met with all these companies. They say that they feel our pain, but their board of directors or their investors say that they're going to go forward.

I've been working with SpaceX, though. They're really trying very hard to eliminate some of these effects, but nothing is perfect. It's going to be tough.

BS: So if these companies are moving forward, what are you going to do?

What I'm trying to do is work very closely with Congress and the American Astronomical Society and other bodies — the United Nations, the FCC [Federal Communications Commission] — to see what we can do.

I'm inherently an optimist. I think the Reflect Orbital is a failed business model, but they're going to try doing it anyway. So they'll put a lot of junk up there for a while.

BS: I truly wish you the best with that. But since you're an optimist, let's end on something positive. You've championed this observatory for more than 20 years — first as its founding director and now its chief scientist. How does it feel now that the LSST is finally operational?

It's quite gratifying, after all this time, to have something that actually works. It's a hugely complicated system, and nothing so complicated as that works perfectly all the time.

I was the original founding director, I am now the chief scientist, and it is my day job to worry about what's going wrong with this or that. And there's a laundry list of things that we're worried about. But it's working, and it's working quite well. And so that's quite gratifying.

Editor's Note: This interview has been condensed and edited for clarity. The article was updated with a new headline on July 6 at 1 p.m. ET.

Astronomers have spotted an ancient galaxy shining through the cosmic fog of the early universe, revealing a detailed view that was thought to be impossible.

Using NASA's Hubble Space Telescope, along with data from the James Webb Space Telescope (JWST) and the European Southern Observatory's Very Large Telescope (VLT), researchers detected "ionizing" ultraviolet photons — energetic light capable of stripping electrons from hydrogen atoms — coming from the galaxy, called MXDFz4.4. It's the earliest such detection on record, arriving only around 250 million years after the end of a major cosmic transition called the Epoch of Reionization, the researchers explained in a study published June 23 in The Astrophysical Journal.

For hundreds of millions of years after the Big Bang, the space between galaxies was filled with a fog of neutral hydrogen gas that blocked this kind of light. Over time, radiation from the first stars and galaxies ionized that gas, clearing the fog and letting light travel freely across the universe — a process astronomers are still working to fully understand.

"This was thought to be impossible," Ilias Goovaerts, a postdoctoral fellow at the Space Telescope Science Institute (STScI) in Baltimore and first author of the new study, said to Live Science. "What’s really special about this galaxy is that it’s getting through so much of the intergalactic medium [the ionized plasma between galaxies]. It’s the furthest away so it has the most intergalactic medium to get through."

What makes MXDFz4.4 unusual is its combination of size and star-formation rate. The galaxy is roughly 100 times smaller by area than the Milky Way, yet it forms stars around 10 times faster, packing a large number of massive young stars into a compact space. According to Goovaerts, that crowding effect helps the galaxy punch clear channels through its surrounding gas, letting ionizing light escape both the galaxy and, eventually, the murky space between galaxies. The team estimates that somewhere between half and all of the galaxy's ionizing light is escaping.

The discovery, made in October, came about somewhat by chance. While preparing an unrelated funding proposal just days before a major deadline, Goovaerts examined an existing, deep Hubble image to check whether anyone had looked for this kind of signal there before. Within a couple of hours, he had a promising signal. "It was very, very quick from us having the idea to me going, okay, there’s something here and this is exciting," Goovaerts said. "We were excited from day one, but then it took months for it to mature and to extract all the properties about the galaxy."

The finding relied on an unusually rich set of observations: an extremely deep Hubble image taken from 40 hours of observations; JWST imaging across many wavelengths, used to characterize the galaxy's stars and star-formation history; and one of the deepest spectra ever taken of a single patch of sky, gathered over roughly six days of observing time with the VLT's Multi-Unit Spectroscopic Explorer instrument. That spectrum confirmed the galaxy's distance through its Lyman-alpha emission line — which serves as a "hydrogen fingerprint," or a glow given off by excited hydrogen gas, that astronomers can use to measure cosmic distance and time.

No other galaxy from this early period had previously shown detectable ionizing light, making MXDFz4.4 one of a kind so far, study co-author Marc Rafelski, deputy mission head for the Hubble Space Telescope at STScI, noted in the statement. .

Researchers say bursts of vigorous star formation like the one seen in MXDFz4.4 may have played an important role in clearing the early universe's hydrogen fog and that more galaxies like it are likely still waiting to be found.

James Webb Space Telescope quiz: How well do you know the world's most powerful telescope?

The hantavirus outbreak that struck a cruise ship in April, killing three people and sparking fears of further spread, is over, the World Health Organization (WHO) has announced.

"Today, the final contact of a person exposed to hantavirus on the cruise ship MV Hondius completed their quarantine period, tested negative and returned home. No further cases have been reported since the 25th of May," Tedros Adhanom Ghebreyesus, the WHO's director-general, said in his opening remarks at a news conference Thursday (July 2). "We are therefore very pleased to say that WHO considers the outbreak of hantavirus over."

The total number of cases linked to the outbreak was 13. All those affected were either passengers or crew on the ship.

The outbreak began aboard the Dutch-flagged cruise ship MV Hondius after it departed southern Argentina on April 1. It involved the Andes virus, the only known hantavirus that can spread between people.

Hantaviruses are rodent-borne viruses that are found in the Americas, Europe and Asia and spread to humans relatively rarely, usually via contact with the urine, droppings or saliva of infected rodents. The Andes virus, however, has sparked short chains of human-to-human transmission in the past.

Before public health authorities were informed of the cases on MV Hondius, several dozen people disembarked the vessel on the island of St. Helena. To find them, authorities launched an international contact-tracing operation, tracking down more than 650 contacts in total who were then followed by health authorities in 33 countries and territories, according to the WHO.

Additionally, health authorities coordinated the monitoring, care and transport of the remaining passengers and crew aboard MV Hondius.

Of these contacts, those considered at the highest risk of infection were then quarantined and monitored for up to 42 days, because sometimes, hantavirus symptoms don't show up until weeks after exposure to the virus. Depending on their jurisdiction and degree of exposure, some contacts quarantined at home while others stayed in specialized facilities.

The initial unchecked travel of some contacts, alongside the virus's long incubation period, prompted concern from the public that the cluster of cases could explode into an enormous outbreak, or even a global pandemic. Many infectious-disease experts emphasized that the Andes virus does not spread easily between people and that the containment effort was going well, so the risk of a large outbreak was low. Still, some experts raised concerns that the international travel of contacts could trigger pockets of the deadly disease, and some argued that the Andes virus does have "pandemic potential."

Now, with the final contact having completed their quarantine period and no further cases reported, the WHO has declared the outbreak over. All of the contacts who were repatriated to the U.S. completed their quarantine period by June 21.

"WHO will continue working with governments and partners to advance our understanding of this outbreak and of hantavirus more generally," Tedros said. "We are also coordinating a study involving 21 countries to understand how the disease develops, which will support the development of diagnostics, therapeutics and vaccines for future outbreaks."

Besides rigorous contact tracing, the WHO credited the coordinated actions of national public health bodies as being vital to preventing the further spread of the disease. These measures included the response of the Spanish government, which created a safe zone on the island of Tenerife for the ship's remaining passengers to disembark before they were repatriated under quarantine.

As the hantavirus outbreak concludes, there's an ongoing Ebola outbreak in the Democratic Republic of the Congo and an outbreak of the Marburg virus in Uganda. These and future outbreaks will require similarly robust international cooperation, the WHO emphasized.

"The outbreaks of hantavirus, Ebola and Marburg all show why there is no alternative to international cooperation in the face of international threats," Tedros said. "No country alone can fight."

This article is for informational purposes only and is not meant to offer medical advice.

June global sea surface temperatures have climbed to record highs, prompting concerns over extreme weather, flooding, sea level rise and stress to global ocean ecosystems.

The record, announced by the European Union's Copernicus Earth observation program on July 1, surpassed the previous record set in June 2024, with experts warning that more temperature records will likely be set over the coming months.

"Current conditions could indicate the beginning of a new phase, leading, once more, to uncharted territory," Carlo Buontempo, director of the Copernicus Climate Change Service at the European Centre for Medium-Range Weather Forecasts (ECMWF), said in a statement. "With ocean temperatures at these levels and El Niño on the horizon, we are likely to see more temperature records fall in the coming months.”

The record temperature was set on June 21, when the Copernicus Climate Change Service recorded global ocean surface temperatures of 20.86 degrees Celsius (69.55 degrees Fahrenheit), beating the record temperature of 20.83 C (69.49 F) set in 2023 and 2024. This measurement was corroborated by the Copernicus Marine Service, an independent dataset that reported temperatures of 21.0 C (69.8 F).

The recent sea surface heating did not occur evenly across the globe. In some areas, such as the Mediterranean, temperatures in June were up to 8 C (14.4 F) higher than average for the period from 1990 to 2020, as per data recorded on June 29, according to the European Space Agency.

The most significant rises in temperature were set in the Mediterranean, the Baltic Sea, bands across the Pacific and off the coasts of Northern Canada.

Warmer ocean temperatures have wide-ranging impacts. "Higher ocean temperatures keep the atmosphere warm for longer, provide extra energy to storms and increase evaporation, thus enhancing the potential for extreme precipitation and flooding," Copernicus Climate Change Service representatives said in the statement. "Ocean warming also contributes to sea level rise and ice melt, and stresses marine ecosystems."

According to data from the Copernicus Climate Change Service, the newly declared El Niño in the Pacific Ocean — the warm phase of a natural climate cycle. This El Niño is likely to reach levels that have not been seen in decades, with more temperature records expected to be set over the coming months as this Pacific heat is injected into an already warming world.

The service added that it remains to be seen whether these temperature spikes are temporary or indicative of longer term trends.

A mysterious wavelength of light is missing from the dwarf planet Pluto and Saturn's supersized moon Titan, new James Webb Space Telescope (JWST) observations show. The surprising discovery hints that these worlds harbor an unknown molecule that has not been seen in any other solar system world or exoplanet so far.

Every element or molecule in the universe absorbs unique wavelengths of electromagnetic radiation. Therefore, one of the main ways astronomers study distant worlds — both inside and outside the solar system — is by closely examining the light that reflects off them and searching for dark "absorption lines" that correspond to the wavelengths of known chemical compounds.

For example, molecular oxygen absorbs light at 230 nanometers, so if the electromagnetic spectrum of a faraway exoplanet has an absorption line at this frequency, researchers can be confident that its atmosphere contains oxygen, according to a 2021 study.

JWST has proved to be exceptionally good at capturing electromagnetic spectra and identifying specific chemicals in exoplanet atmospheres, around distant stars and within primitive galaxies. It has even identified a molecule on one alien world that could point to extraterrestrial life.

In a new study, uploaded June 11 to the preprint server arXiv, researchers analyzed JWST data from Pluto and Titan, focusing on very small wavelengths that have been relatively unexplored until now. This revealed a specific absorption line at around 5.11 micrometers in both worlds' spectra. (These findings have not been published in a peer-reviewed journal yet.)

The team pored through similar studies on other planetary spectra but "did not find any band referenced in these publications that corresponds to the location of the observed absorption in Titan and Pluto," the researchers wrote in the paper.

A molecular mystery

The discovery is even stranger because there are very few similarities between Pluto and Titan that could explain why they share a molecule not found anywhere else.

Titan is the largest of Saturn's many moons and is even larger than Mercury. It is also the only solar system world, other than Earth, that is known to have liquid rivers and oceans on its surface. Pluto, on the other hand, is a completely frozen world that's around half the size of Titan and roughly four times farther from the sun than Saturn's satellite is.

Both worlds do have similar atmospheres that are rich in methane and nitrogen. However, the researchers are confident that the molecule responsible for the 5.11-micrometer absorption line is located on both worlds' surfaces, not in their atmospheres.

Pluto's absorption line is around three times thicker than Titan's, meaning the mystery molecule is likely much more abundant on the dwarf planet. But on Titan, the molecule seems to be unevenly distributed, with a stronger absorption line on its trailing side — the hemisphere opposite to its forward momentum around Saturn — than on its leading side.

The researchers proposed that it could be benzene — a ring-shaped hydrocarbon — mixed with an unknown molecule, or some form of acetylene or ketene ice. However, much more work is needed to prove that any of these potential candidates are responsible for absorbing this specific wavelength, they wrote.

NASA's Dragonfly spacecraft, which is set to launch no earlier than 2028 and fly through Titan's atmosphere in 2034, could eventually shed more light on the situation. The helicopter-like craft's onboard spectrograph could identify the mystery molecule on Saturn's moon, which would also help reveal if it is viable on Pluto, the researchers suggested. But in the meantime, we'll have to wait to unravel this curious cosmic conundrum.

See how well you know our planetary neighborhood with our solar system quiz!

While scanning one of Scotland's richest prehistoric landscapes, archaeologists uncovered evidence of what may be a newfound stone or timber circle buried beneath a peat moorland. The find may add another monument to a ceremonial structure that has fascinated researchers for more than a century.

The possible circle lies beneath the surface of Machrie Moor on Scotland's Isle of Arran, a landscape already famous for its towering standing stones, burial monuments and ceremonial sites dating to between roughly 3500 and 1500 B.C. Researchers from Historic Environment Scotland identified the possible circle using geophysical survey equipment, which is wheeled aboveground and detects subtle magnetic changes underground without disturbing any archaeological remains.

The discovery emerged from a survey designed to test how well modern archaeological instruments work in peat-covered landscapes, but instead the project revealed the unexpected subterranean circle.

"We know that there is a lot of archaeology yet to uncover at Machrie Moor, but the discovery of a new circle completely surpassed our expectations," Nick Hannon, senior heritage recording manager at Historic Environment Scotland, said in a statement released June 30.

While Stonehenge is the world's most famous prehistoric circle, it is only one monument among hundreds built across Britain and mainland Europe during the Neolithic and Bronze ages. Machrie Moor is among the best-preserved examples of these ritual landscapes, with six ceremonial circles already identified since the 1980s.

In fact, the archaeologists found there was more to learn about some of the previously known circles. At Machrie Moor Circle 2, for instance, the team identified a ring of anomalies suggesting the circle may have had 14 stones instead of the seven or eight previously reconstructed.

The circles also share a striking orientation: They align with a notch at the head of nearby Machrie Glen where the midsummer sun would have risen, which suggesting astronomical observations may have played a role in ceremonies held there.

Archaeological anomalies

Unlike the circles that had already been discovered at the site, the newly detected monument has not been excavated yet. Instead, researchers identified a ring of magnetic anomalies ‪—‬ subtle disturbances in the soil that often indicate archaeological features such as pits or postholes.

According to the survey report, the feature consists of 12 circular, pit-like anomalies arranged in a circle approximately 92 feet (28 meters) across. The pits are spaced around 21 feet (6.5 m) apart, with two unusually wide gaps that the researchers say could represent the locations of two additional pits that are now decayed. If so, the monument may have originally contained 14 posts or standing stones.

"There is no indication that any of these anomalies contain a stone" at this time, the researchers noted in the report, so the circle could have been built from either timber posts or standing stones that were later removed.

Previous excavations have already revealed that several of the other stone circles at Machrie Moor were originally built as timber circles before the wooden posts were replaced with stones around 2000 B.C. Human cremations and bodily burials were later placed within some of the circles, suggesting the monuments' functions changed over time.

"It is likely that the newly-discovered circle dates from a similar period as the other circles still standing," representatives of Historic Environment Scotland said in the statement.

See how much you know about Stonehenge with our Stonehenge quiz!

An 11-year-old boy in Ontario, Canada, has died after being bitten by a rabid bat that was resting on his face as he slept. The boy had no obvious bite or scratch marks and didn't show symptoms for the first 19 days after the incident, his doctors report.

While on vacation with his parents at a cottage in northern Ontario in 2024, the boy was woken up in the night by a bat on his nose and mouth, according to a report published in the Canadian Medical Association Journal on June 29. His father caught the bat in a cooking pot and released it outside, and because the child had no visible injuries and the bat did not seem to be particularly aggressive, his parents decided not to seek a medical assessment, the report noted.

A few weeks later, the child began to experience tingling, numbness and swelling on the right side of his face. When he was examined at his local hospital his vital signs appeared to be normal, aside from an elevated heart rate and white blood cell count.

The next day, the boy's symptoms worsened: he lost feeling in the right side of his face and his speech was beginning to slur. While waiting in hospital, he developed a fever, confusion, hallucinations and difficulty swallowing, followed by excessive production of saliva.

After four days in intensive care at McMaster Children's Hospital in Hamilton, Ontario, the child tested positive for rabies, and after five days his brain stem reflexes were absent, indicating a total loss of brain stem function. Seventeen days after admission, following a consultation between his family and medical experts, he was taken off life support and died.

Rabies is a viral disease that primarily affects the central nervous system, according to the CDC. It is mainly spread through bites and scratches from infected animals, with bats accounting for the majority of cases in North America, according to the boy's doctors.

"Bats pose a particular risk because bites or scratches may be small and are easily overlooked, and patients may not recollect or recognize a bat exposure," the medical team wrote in their report.

According to a report in the Journal of Virology in 2013, silver-haired bats (Lasionycteris noctivagans), are responsible for the majority of rabies cases in Canada. Skunks, foxes and raccoons also often carry the disease.

The rabies virus must travel to the brain before symptoms can occur, but once a patient develops symptoms the infection is almost 100% fatal, with most deaths occurring within one to two weeks of symptom development. However, prompt treatment after exposure — including wound cleaning, antibody administration and a series of vaccines — is nearly always effective at preventing the disease, according to the CDC.

Rabies in humans is very rare in North America, with fewer than 10 deaths reported in the U.S. every year, according to the CDC. In Canada, only 28 human fatalities have been reported since 1924, according to the Canadian Veterinary Medical Association. Even so, the boy's doctors have emphasized the importance of prompt medical attention following exposure to bats and other animals that could carry the disease.

"Early recognition of exposure and timely PEP [postexposure prophylaxis] remain the only effective means of rabies prevention," they wrote. "Any direct human contact with a bat, even in the absence of a visible bite or scratch, is an indication for PEP."

They added that rabid bats do not always display the classic symptoms commonly associated with rabies, such as aggressive behavior and frothing at the mouth. "Any direct human contact with [a] bat is considered high risk," they added.

This article is for informational purposes only and is not meant to offer medical advice.

Editor's note: This article was updated at 06:53 EDT on July 3 with news that the mission has launched and reached orbit.

A rescue spacecraft set to speed toward a NASA telescope to prevent it from falling into Earth's atmosphere has launched into orbit.

The first-of-its-kind mission reached orbit after launching at 4:36 a.m. EDT (0836 GMT) Friday (July 3) from the Marshall Islands, carrying a robot-arm spacecraft named Link into the sky aboard a modified Lockheed Martin L-1011 airliner. In midair, a Northrop Grumman Pegasus XL rocket fired Link into orbit, where it will now rendezvous with NASA's Neil Gehrels Swift Observatory, a gamma-ray telescope that has been slowly falling toward Earth and headed for an untimely demise.

The launch follows two consecutive scrubs that caused delays to the mission on July 2 and 3, the first due to weather conditions and the second a software fault. Now that Link has reached orbit, mission engineers are working to acquire a signal from the craft to confirm that its solar panels have deployed and its power systems are working, NASA wrote in an update.

Link was developed by private company Katalyst Space for $30 million. Katalyst's goal is to meet up with the falling Swift Observatory, which launched in 2004, and pull it to a higher orbit, using Link's robotic arms and thrusters. Swift is still scientifically useful but is rapidly losing altitude due to the natural drag of Earth's atmosphere. Without help, Swift will likely meet its demise later this year, scientists say.

"This is a high-risk, high-reward mission," Shawn Domagal-Goldman, director of NASA's Astrophysics Division, said in a statement. "We have much to gain by attempting this boost, which is more affordable than trying to replace Swift's capabilities, and allows NASA to advance the nation's satellite servicing industry, for the benefit of all."

Swift cost $250 million in 2004, which is roughly $450 million today when accounting for inflation — a relatively cheap observatory compared with the $10 billion James Webb Space Telescope. The Swift mission was originally designed to study gamma-ray bursts ‪—‬ cosmic explosions that occur when a massive, dying star collapses into a black hole. Swift has made many observations of these bursts in the past 20-plus years while also watching for other signs of stellar activity, like X-ray flares or supernova explosions, as well as transient objects, like comets and asteroids.

In sum, Swift helps us see how the universe is changing over short periods.

"Swift is NASA's multitool when it comes to studying the cosmos," S. Bradley Cenko, Swift's principal investigator and an astrophysicist at NASA's Goddard Space Flight Center, said in the statement. "It observes the sky using a wide range of light, and rapidly points at short-lived outbursts, alerting other facilities in space and on the ground to help coordinate follow-up observations."

High-risk rescue mission

The rescue mission comes with several challenges. Swift was not designed to be serviced when it launched, making the logistics of the mission something of a puzzle. Moreover, NASA only gave the contract to Katalyst in September, after high solar activity in recent years ballooned Earth's atmosphere and unexpectedly accelerated the spacecraft's fall due to increased drag. This meant the mission had to be ready for space in less than a year after the usual punishing requirements of design, build and testing.

Katalyst accepted the challenge because the company hopes to do this kind of work more often. "If we're going to build an enduring presence beyond Earth, we need the capability to manipulate our environment in space," Katalyst CEO Ghonhee Lee said in the statement. "That means deploying robotic spacecraft that can reposition, repair, refuel, and refit satellites after launch."

Unless Swift altered its operations plan, however, the spacecraft would have been irrecoverable in July. So, to give Link as much time as possible to rescue Swift, the operations team at Penn State's Eberly College of Science made some changes.

For example, Swift's science was minimized so that the spacecraft looks at targets only if the telescope is put in a "streamlined position" to minimize drag, NASA explained. Power consumption has also been slashed to let Swift's solar panels fly "in a more aerodynamic orientation," which also reduces the drag that is making the spacecraft fall into the atmosphere.

These changes will allow Swift to stay above the minimum rescue altitude of 185 miles (298 kilometers) until autumn, agency models suggest. Katalyst will use that time to do the usual spacecraft "commissioning" on Link to make sure all systems are well. It will take Link about a month to rendezvous with Swift, according to NASA.

Following those steps, Link will approach Swift for evaluation, and Katalyst will use Link's robotic arms to latch onto the NASA observatory. Link will then use its propulsion system to gradually bring Swift's orbit to about 370 miles (595 km) ‪—‬ well above the pathway of the International Space Station, which orbits roughly 250 miles (400 km) over Earth.

NASA did not say how much longer Swift would be able to keep observing, should it reach its new altitude safely. However, figures from the European Space Agency suggest that spacecraft at an altitude of 310 miles (500 km) reenter the atmosphere within about 25 years. This would suggest that as long as Swift's instruments hold out, scientists would have many years of observations to look forward to.

Two brothers from the wealthy and powerful Medici family died of malaria and were not poisoned as a rumor had suggested, archaeologists have confirmed based on a DNA analysis of the brothers' skeletons. The analysis also revealed a unique, mutated strain of malaria that may hold the key to understanding the evolution of the disease in Europe.

The Medici family rose to power in the 15th century by creating the largest bank in Europe. The family used their extraordinary wealth to fund Renaissance artists and to start a political dynasty that eventually included numerous dukes, four popes and two queens of France.

In the 16th century, Cosimo I took over all of Tuscany as grand duke. But within a span of 25 years, at least five of his family members died from high fevers. This gave rise to a rumor that some of them had been poisoned with arsenic by another family member, although most people believed they died of malaria.

To get to the bottom of the 500-year-old Medici cold case, an international group of researchers tested the bones of two of Cosimo I's sons: Cardinal Giovanni de' Medici and Grand Duke Francesco I de' Medici, for the DNA of Plasmodium falciparum, the parasite that causes the deadliest form of malaria and that is transmitted by mosquitoes.

The researchers extracted ancient DNA from the bones of Cardinal Giovanni, who died in 1562 at age 19 in the same month as his mother and younger brother Garzia, and from Grand Duke Francesco I, who died at age 46 in 1587 along with his wife. The team's study was published online June 17 in the journal iScience.

Because of the almost simultaneous deaths of Grand Duke Francesco I and his wife, a rumor circulated that another brother had poisoned them over a long-standing feud. But the Medicis were known to have frequented their family villas in marshy and swampy areas of Tuscany, where malaria was prevalent well into the 20th century.

Researchers found evidence of P. falciparum in the bones of both Medici brothers, confirming reports from court physicians at the time that described the brothers as sick with "tertian fever," a type of high fever that returns every three days and is a hallmark of malaria. The medical reports also revealed the brothers were treated with bloodletting.

"Now we can say with scientific certainty that malaria, not poisoning, killed Grand Duke Francesco de Medici," study co-author Valentina Giuffra, a medical historian at the University of Pisa, said in a statement.

But the ancient-DNA study held two additional surprises.

The Grand Duke's bones were positive not only for P. falciparum but also for Plasmodium malariae, a different parasite species that also causes malaria in humans, suggesting that both species contributed to the severe illness that killed him and his wife.

Cardinal Giovanni, on the other hand, had only P. falciparum, but the specific strain that infected him was previously unknown. The strain is similar to those found in ancient and early modern Europe, but with two mutations the researchers had never seen before, they wrote in the study.

"The study of ancient DNA offers us an opportunity not only to diagnose malaria in the remains of individuals from the past, but it also offers us a window for understanding the evolution of malaria species, Plasmodium falciparum in this case, which can help scientists better understand how the pathogen adapts over time," study first author Alexander Ochoa, an evolutionary biologist at Yale University, said in the statement.

Further analysis of the brothers' bones is needed to determine the evolutionary relationship between the strains of malaria they carried, the researchers wrote in the study.

What do you know about the bones in your body? Test your knowledge with our human skeleton quiz.

The first dinosaur found in Antarctica belonged to a group that included the largest animals ever to walk the planet, a new study finds.

A backbone from the 82 million-year-old giant was discovered more than 40 years ago, but at the time, researchers assumed it came from an ancient marine reptile. Now a new study, published June 29 in the journal Acta Palaeontologica Polonica, has revealed that it was actually a titanosaur — the group of long-necked sauropods that included the largest land animals on record.

"At first glance this appears to be an unremarkable fossil, but it holds an important place in the history of Antarctic exploration as the first dinosaur fossil found on the continent," study first author Paul Barrett, a paleontologist at the Natural History Museum in London, said in a statement.

While this fossil now holds the record for the first dinosaur fossil found in Antarctica, other dinosaur fossils were identified on the continent after its discovery, so it's not the only known Antarctic dinosaur. In fact, researchers have identified a variety of dinosaurs on Antarctica, with another sauropod fossil identified as a titanosaur in 2011.

The newly identified dinosaur was around 20 to 23 feet (6 to 7 meters) long. That's very small compared with the largest-known titanosaurs, which could grow up to 123 feet (37.5 m) long. However, as the fossil is just a fragment of a vertebra, researchers are unable to narrow down which species the Antarctic titanosaur belonged to, and it's possible that the individual was only a juvenile when it died.

Mike Thomson, a British Antarctic Survey geologist, found the fossil during an expedition to James Ross Island in 1985. The island, which has been the site of multiple dinosaur discoveries, is located off the northeastern Antarctic Peninsula, south of the 600-mile-wide (965 kilometers) Drake Passage that separates South America from Antarctica.

Antarctica is well known for its icy landscapes, but when titanosaurs roamed Earth, the continent was still attached to South America and full of temperate forests. Antarctica's dinosaurs were so far south that they would have lived in constant twilight during the winter months, according to a news article published by the Natural History Museum.

The authors of the new study identified the dinosaur using high-resolution CT scans, which enabled them to look inside the fossil. Dating back to the Cretaceous period (143 million to 66 million years ago), the titanosaur lived in the last age of the non-avian dinosaurs, before an enormous asteroid hit what is now Mexico's Yucatan Peninsula 66 million years ago and wiped them out.

The Antarctic titanosaur helps researchers better understand how dinosaurs spread across Earth's southern continents, which at the time were combined into a supercontinent called Gondwana. The presence of titanosaurs on Antarctica suggests that they may have used Antarctica to travel from what is now South America to New Zealand.

Other dinosaurs identified on Antarctica include small herbivores, armored ankylosaurs and bipedal predators like Imperobator, which would have shared the forests with the newly identified titanosaur. While researchers are beginning to piece together Antarctica's ancient ecosystems, they still have a lot to learn about the dinosaurs that lived there.

"There are likely many more dinosaurs to be discovered on the continent," Barrett said. "As climate change causes ice to retreat we may indeed find further evidence of this past biodiversity."

Researchers have proposed creating a novel satellite constellation, dubbed StormWall, that could shield Earth from the worst effects of solar "superstorms" that we are otherwise unable to mitigate. The innovative idea, which would essentially create a giant airbag in front of our planet, could prevent trillions of dollars in potential damage and is "quite feasible," experts say.

Over the past few years, we have been bombarded by dozens of solar storms as the sun reached the most active phase of its roughly 11-year solar cycle, called solar maximum. These events are often triggered by large clouds of incoming plasma, or coronal mass ejections (CMEs), which often follow powerful explosions on the sun's surface known as solar flares. Such storms frequently paint vibrant auroras across our skies, but their effects are not always benign.

Every century or so, the sun spits out a supercharged storm, such as the Carrington Event of 1859, that is several orders of magnitude stronger than a typical CME. If such a storm were to hit us today, it could wipe out every satellite orbiting Earth, dose astronauts with lethal levels of radiation, damage power grids and even knock out the internet.

Currently, the only way we can prepare for the next superstorm is to get better at forecasting them and design our spacecraft and ground-based infrastructure to deal with their arrival as best as possible. However, a new study published June 2 in the journal Space Weather presents a more proactive approach.

In the new paper, researchers propose launching six bus-sized satellites into a geosynchronous orbit, around 22,500 miles (36,000 kilometers) above Earth. At this altitude — far above the International Space Station and most other satellites — the mini spacecraft swarm would sit and wait for the next "big one." If and when such a storm were spotted, the satellites would empty giant canisters of gas around the edge of Earth's invisible magnetic shield, or magnetosphere, creating a giant wall of plasma that would cushion and divert an incoming CME.

The team’s simulations show that this plasma wall could cut the intensity of a superstorm down by more than half. This would not completely shield us, but it could help avoid any worst-case scenarios, similar to having an airbag during a car crash, study co-author Daniel Welling, a space physicist at the University of Michigan, told Science magazine. "It's as if you could install an airbag in the magnetosphere," he said.

Because we currently have no way to defend ourselves against these storms, the researchers argue that such a system is vital and should be constructed as soon as possible.

"It's like people in a village who see a river flooding — maybe they can predict when that will happen, but probably what's even better is if they could build a storm wall. That's what we're proposing here," study first author Brian Walsh, a plasma physicist and space weather expert at Boston University, said in a statement. The only difference is that "it would help all people on the planet," he added.

Protecting the planet

StormWall was inspired by Earth's natural response to a solar storm. When CMEs impact our planet, they temporarily weaken the magnetosphere — known as a geomagnetic disturbance — allowing solar radiation to flood the upper atmosphere and trigger auroras. But this also causes oxygen ions to rise into the magnetosphere, where they accumulate on the sun-facing side of our planet, creating a bubble that helps shield us from incoming radiation while the magnetosphere is compromised.

The idea of StormWall is to create this protective barrier before the storm arrives so that the geomagnetic disturbance is not as strong as it otherwise would be. To do this, the proposed satellites would dump around a dozen oil trucks' worth of a reactive gas — such as barium, lithium, sodium or calcium — into the magnetosphere. This gas would accumulate on the sun-facing edge of the magnetosphere and quickly become ionized by the sun, creating a massive plasma barrier that would not only push back against an incoming CME but also help divert it around our planet.

To demonstrate StormWall's potential effectiveness, the team simulated how the satellites would have impacted the May 2024 solar storm (also known as the Mother's Day storm), which occurred when a series of CMEs struck our planet in quick succession, triggering the most powerful geomagnetic disturbance since 2003. They found that the satellites could have reduced the intensity of the resulting geomagnetic disturbance by as much as 84%.

"When you apply some really serious physics to it, it does work," Walsh said. "And the amount of mass we need, the launch capacities — it's all within our capabilities."

One of the most surprising aspects of the new proposal is the amount of gas being released by the satellites: It equates to only around one-millionth the weight of a typical CME, yet this can cut a solar storm's power in half — so the "scheme punches far above its weight," according to Spaceweather.com.

"I definitely would want this"

Some concerns need to be addressed before StormWall could become a reality. For example, similar geoengineering projects — most of which have been proposed to tackle the effects of human-caused climate change — have been criticized for the inadvertent impacts they may have on our planet.

However, while follow-up studies will be needed to make sure it is safe, the researchers are confident that the ionized gas would not affect Earth's magnetosphere or upper atmosphere in any way. Once deployed, the plasma wall would quickly dissipate and be blown clear of our planet by solar wind.

There is also the issue of money. The StormWall satellites, with their massive gas canisters, would be among the heaviest spacecraft ever launched and would likely require massive rockets, such as SpaceX's Starship, to put them into geosynchronous orbit. While a proper cost analysis has yet to be completed, this would likely cost billions of dollars.

However, considering the potential damages from solar storms, the researchers argue that StormWall would be well worth the money. The May 2024 solar storm, for example, cost U.S. farmers around $500 million due to malfunctions with GPS equipment. And that's just a drop in the bucket compared with what a Carrington-level storm would cost; the study researchers estimate that such a superstorm could cause up to $3.4 trillion in damage.

Another issue is that StormWall is a one-and-done solution. Once the gas canisters are empty, they need to be refilled or completely replaced, which would create a substantial additional cost. But again, if the benefits significantly outweigh the cost, this would be a no-brainer.

Even when taking all of these challenges into account, several experts believe StormWall is not only a good idea but also achievable on a relatively short timescale.

The proposal is "highly innovative and appears to be quite feasible in the near term," Allison Jaynes, a space physicist at the University of Iowa who was not involved in the study, told Science magazine.

And given that there are currently no viable alternatives, it would help put people at ease about the next superstorm.

"If I knew that a 100-year disturbance was coming and it would knock out power grids, I definitely would want this," David Sibeck, chief of heliophysics at NASA's Goddard Space Flight Center, told Science magazine.

Life on Earth could continue for another 1.8 billion years, according to new research. This figure, which is based on complex climate models, is far longer than many previous studies indicated.

As the sun evolves, it is getting brighter. Our star is currently producing about a third more energy than it did at the dawn of the solar system 4.5 billion years ago. And it will continue to get hotter until it eventually dies in about 5 billion years.

Scientists have wondered for decades how long life on Earth will manage to cling to existence as the sun brightens. In 1982, James Lovelock and colleagues estimated that Earth's photosynthetic biosphere — which includes all plants and forms the basis for most of the planet’s biology — would end about 100 million years from now. Successive studies have pushed back the deadline for the death of all life on Earth.

In the new study, published May 28 in the journal JGR Atmospheres, researchers suggest that plant life could continue about 1.8 billion years into the future. That nears the time when Earth would lose its oceans to space, either through radiation splitting water atoms or runaway evaporation, in about 2 billion years.

"We were trying to show that life on Earth — complex vegetation — could survive longer into the future than previous studies had shown," study co-author Jacob Haqq-Misra, an astrobiologist at space exploration charity Blue Marble Space, told Live Science.

The boundaries of life

Life on Earth relies on photosynthesis, the process used by plants, algae and some bacteria to turn sunlight into energy. The mechanism chemically converts carbon dioxide and water into sugars and oxygen. It requires both CO₂ and sunlight.

But at certain temperatures, plants' photosynthetic machinery shuts down. Eventually, the sun will warm Earth to the point that plants are no longer able to photosynthesize, which would in turn cause entire food webs to collapse and all life to perish.

Another issue is that as the sun dies and it gets brighter, there will be less carbon dioxide in the atmosphere, effectively starving plants.

"The Earth has stayed pretty hospitable in terms of surface temperature for most of the last 4 billion years because it has a built-in thermostat" by storing CO₂ in rocks and releasing it during volcanic eruptions, Robert Graham, a planetary science researcher at the University of Chicago, who was not involved in the research, told Live science.

When it is hotter, the planet pulls more carbon dioxide out of the atmosphere and stores it in rocks underground, Graham said. This offsets the warming to keep the temperature stable but means that the carbon dioxide isn't accessible to plants.

Climate models and extreme plants

In the new study, Haqq-Misra and colleague Eric Wolf, a research scientist at Blue Marble Space, used 29 climate models to estimate what would happen to Earth's vegetative biosphere under different scenarios. They used the two extreme cases as limits — when Earth is too hot for life but the CO₂ was stable; and when there is not enough CO_2, but the temperature was stable. They then looked at the range of CO₂ and sunlight conditions in between those extremes. This enabled them to include situations in which Earth was very efficient at pulling carbon from the atmosphere when temperatures started rising.

They also included information about a variety of plants. Some plants can survive on a much lower ratio of atmospheric CO₂ than others. The study included plants that have a special photosynthetic process (known as crassulacean acid metabolism), such as succulents and orchids. These plants can sustain themselves on relatively tiny amounts of CO₂. The same is true of some marine plants, which can dissolve and access carbon in the ocean system.

Other experts were impressed by the findings.

"Haqq-Misra and Wolf have used a sophisticated 3D climate model to show that Earth's climate may remain hospitable to plant life significantly longer into the future than predicted" by simpler models, said Graham, who authored one of those earlier studies. "It's an advance over previous work and suggests that complex biospheres like that of Earth are more resilient to environmental change from stellar brightening than previously suggested."

Looking to the future

Andrew Rushby, an astrobiologist at Birkbeck University of London who was not involved in the research, told Live Science that the paper updated the concept of the lifetime of the biosphere. However, he cautioned that the results remained "broad estimates."

"It is not possible for us to predict or know the possible evolutionary adaptations that the photosynthetic biosphere may undergo in response to increasing solar output and lower [atmospheric CO₂], especially over billions of years," he said.

In their paper, the authors wrote that "limits posed by thermal stress or starvation may only reflect our observations of the biosphere today rather than hard limits on how the biosphere may evolve." There is also no way of knowing how life might adapt to new circumstances.

Haqq-Misra said that he found the results comforting. "Earth's system is resilient, and we are part of something that could have a much, much longer future," he said.

The results could also help scientists figure out what the thresholds could be on other planets. "Part of the challenge is starting with these Earth-based models, and then generalizing the physics as much as possible to be able to simulate a wider range of atmospheres," he said.

How much do you know about our blue planet? Test your terran knowledge with our Earth quiz!

Network latency in bitcoin mining is driving massive energy waste ‪—‬ the annual equivalent of the total generation capacity of Switzerland's entire hydroelectric power system, scientists say. This wasted energy results from inefficiencies in the mining process and increasing competition among bitcoin miners.

In a new study published May 26 in the journal PNAS Nexus, the researchers aimed to provide a theoretical model to measure patterns within the networks powering bitcoin's distributed ledger system.

But they also calculated that in 2025, around 16,000 megawatts was wasted by fruitless bitcoin mining attempts, where competing mining efforts exert massive computational power to obtain the same units of bitcoin. This is roughly equivalent to the total generation capacity of Switzerland's 701 hydropower plants, according to statistics from the Swiss Federal Office of Energy.

It's important to note that this figure differs from the total energy consumed by bitcoin mining activity, estimated by researchers to stand at an annual level of 138 terawatt-hours, as of June 2024. This is higher than the annual energy consumption of several developed countries including Norway and the Netherlands.

Energy-guzzling crypto

Concerns around the environmental impact of bitcoin and other proof-of-work blockchain technologies have abounded in recent years.

In 2021, for example, bitcoin mining's water usage, primarily for liquid-cooled computer equipment, equated to more than the domestic water use of 300 million people in rural sub-Saharan Africa, according to a 2023 U.N. report.

Bitcoin is underpinned by a distributed ledger system, called a blockchain, which operates on a "proof-of-work" model. For a new unit of the digital currency to be generated, computing power must be used to solve a digital puzzle. In theory, the first entity to successfully "solve" the problem adds a new "block" of transactions to the ongoing chain and is granted a set quantity of bitcoin in return.

However, due to the explosion of interest in bitcoin as a financial trading asset, the competition for who can be the first to complete a block and claim the rewards has become incredibly fierce. A solution to the puzzle is based on computational power, with specialized hardware providing a greater advantage in speed. It has driven commercial entities to invest in building specialized data centers dedicated to such mining operations.

Because the race to be the first to mine a block is so competitive, the difference between first and second place can be just tiny fractions of a second. This often results in "accidental forks" — where two competing blocks are registered at almost exactly the same time.

In this scenario, the block with the longest chain of subsequent blocks built on top of it will eventually become a verified and legitimate part of the blockchain — earning its miners the bitcoin reward — while the competing block will be seen as invalid and worth nothing.

The energy needed to solve the proof of work and generate these "orphaned blocks" in the first place — as well as any subsequent blocks built on top of them before the winner is decided — is ultimately wasted.

"Despite their indication of a distributed network, accidental forks are an inefficiency of the Bitcoin protocol that leads to wasted computational resources (and thus energy), increasing the cost of network operations and its environmental impact to maintain a given level of security," the researchers wrote in the study.

According to the Crypto Carbon Ratings Institute (CCRI), a cryptocurrency analysis firm, bitcoin is the most dominant cryptocurrency by far, with a market capitalisation of more than $1.1 trillion — more than 80% larger than the next most popular currency, Ethereum. However, instead of proof-of-work, Ethereum uses a different form of consensus mechanism to establish block authorship, called "proof-of-stake," which is significantly less computationally intensive.

While other cryptocurrencies apart from bitcoin also use proof-of-work methods, bitcoin is around twice as large as its next nearest rival in this category, making it orders of magnitude more power-hungry.

Who rules the pool

Whereas previous models for analyzing fork rates treated all miners in the network as equal, this study considered elements such as network latency and geographic distribution, aiming to provide a "null model" — a baseline which can be used as a starting point to inform future analysis.

The model also allowed the researchers to quantify other notable trends, such as the distribution of "mining pools" — consortiums in which mining operators pool their efforts to maximize their potential success. They identified a decline in the dominance of Chinese mining pools from 2022 following the country's ban on bitcoin mining while also discovering high levels of consolidation at the upper level of the bitcoin mining industry.

The report found that just three mining pools produce over 50% of new bitcoin blocks. This is a problem because it risks a "51% attack," whereby unscrupulous miners enter fraudulent information into the blockchain by ensuring that they always produce the longest chain and, therefore, become validated.

This level of consolidation distorts the market for processing fees that bitcoin users pay to have their transactions included in the next block, the researchers added, and could thus allow miners to arbitrarily delay the inclusion of specific transactions.

The patient: A man in his 20s in Edinburgh, U.K.

The symptoms: The man visited an eye clinic after noticing floaters — small, dark shapes drifting across his field of vision — along with brief flashes of light in his right eye for six days. He was otherwise healthy and had no history of eye disease, physical trauma to the eye, or drug use. He had mild nearsightedness, for which he wore glasses.

What happened next: Doctors performed a thorough eye exam while the patient wore glasses, finding that his corrected vision measured 6/6 in both eyes, the metric equivalent of 20/20. His eye pressure was also normal.

However, a closer examination of the patient's retinas, the light-sensitive layer lining the back of the eye, revealed significant damage in both eyes, according to a report of the case.

In the right eye, doctors found multiple retinal tears and bruising, as well as a retinal dialysis, a rare type of tear in which the retina begins to separate from its outer edge where it connects to other tissues of the eye. Without treatment, retinal dialysis can progress to full retinal detachment and cause permanent vision loss. The left eye also had bruising and six small, horseshoe-shaped retinal tears: three at the top and three on the side of the retinal tissue.

Since these injuries are typically caused by sudden trauma to the eye ‪—‬ from a punch or sports injury, for instance ‪—‬ doctors revisited the patient's history and asked whether anything unusual had happened involving his eyes.

The patient, described in the case report as a "hesitant historian," later disclosed that he had been using a percussive massage gun directly on and around his eyes for the past three months. He had bought the device himself and used it weekly for several minutes at a time without medical guidance, in an effort to relieve a "feeling of tiredness" in his eyes.

The diagnosis: Doctors concluded that the patient's retinal injuries were most likely caused by this improper use of the massage gun, according to the case report. These devices deliver rapid, high-frequency pulses of pressure that are intended to relieve muscle tension. However, they can cause severe damage to delicate tissues like those found in the eyes.

The eye is filled with a gel-like fluid that helps it maintain its shape. The case report authors suggested that, each time the device put the eye under pressure, it may have briefly distorted the eye's shape. Over time, this repeated stress may have placed strain on the retina, eventually leading to the small tears.

This pattern of injury was also different from what's seen in typical retinal dialysis cases, they noted. The condition most often occurs in the lower, outer part of the retina, along its bottom edge. In this patient, however, the injury was found in the retina's upper region, which his doctors said may reflect repeated forward pressure from the device rather than a conventional lateral impact, such as blow to the head.

The treatment: Around 8% to 15% of retinal dialysis cases can progress to retinal detachment, which can lead to vision loss. In this case, however, the patient's vision was preserved.

The retinal tears in both eyes were treated with laser therapy; targeted laser burns create scar tissue that helps seal the retina in place and thus prevent fluid from seeping underneath. The right eye's retinal dialysis was treated with "barrier laser therapy," which similarly creates a protective scar around the affected area to reduce the risk of progression.

At a follow-up six months later, the patient's condition remained stable, with no further damage or cataract formation (clouding of the eye's lens). Doctors reported that the positive outcome was "likely due to the patient's prompt presentation soon after noticing symptoms and the immediate initiation of treatment."

What makes the case unique: Eye injuries linked to massage guns are rarely reported. The small number of cases that appear in the medical literature suggest they can sometimes cause serious or permanent damage.

In one such case, a 69-year-old man developed severe eye complications, including lens dislocation and glaucoma (a sudden rise in eye pressure) after using a massage gun near his eye for several weeks. In another case, a 38-year-old woman developed a dense traumatic cataract — a type of cataract that forms due to physical injury — and severe vision loss after using a similar device over her temple and eye region.

The Edinburgh man's case is the first to report retinal dialysis and multiple retinal tears linked to massage gun use. Such injuries are usually associated with high-energy trauma, such as road traffic accidents, sports injuries or a direct blow to the eye, or they occur in people with underlying risk factors, including severe nearsightedness or age-related eye changes, the case report authors noted.

In this case, the young man had none of these known risk factors. The extent of the damage in the absence of these risk factors raises concerns about the effects of improper use of massage guns near the eyes, his doctors concluded.

Massage guns are widely sold for at-home use, but there are currently no standardized safety guidelines for using them on or near sensitive areas, such as the eyes. The authors of the case report said the man's case highlights the need for clearer manufacturer warnings and greater awareness of the potential risks of improper massage gun use.

For more intriguing medical cases, check out our Diagnostic Dilemma archives.

This article is for informational purposes only and is not meant to offer medical advice.

Can you guess the diagnosis in these strange medical cases? Find out with our diagnostic dilemma quiz!

The Large Hadron Collider (LHC), the world's largest and most powerful atom smasher, has entered a planned four-year shutdown that will upgrade it to its most capable form yet.

The particle accelerator was switched off Monday (June 29) and is scheduled to come back online in 2030 as the High-Luminosity Large Hadron Collider (HiLumi LHC), with improvements that will allow it to smash together roughly 10 times more particles than its original design. That data could help spark new discoveries in fundamental physics and shed light on the nature of dark matter, antimatter and the early universe.

"This is a very important moment," HiLumi LHC project chief Markus Zerlauth told Agence France-Presse. "From Monday, we will be entering a new phase."

Since its first successful proton collision in 2009, the LHC has allowed physicists to test theories about particle physics and the Standard Model of the subatomic world. It was essential to the discovery of the Higgs boson in 2012, which helped explain how tiny fundamental particles acquire mass. The collider covers a 17-mile (27 kilometers) loop at the border between France and Switzerland near Geneva.

The current shutdown is the third long-term, planned pause in the collider's operations. The first, a two-year shutdown beginning in 2013, consolidated connections between superconducting magnets and boosted the energy of the colliding proton beams. A second pause, from 2018 to 2022, involved a series of upgrades, replacements and preventive maintenance.

In the current period of dormancy, dubbed Long Shutdown 3 (LS3), specialists will install upgrades to boost the collider's luminosity by a factor of 10. That will increase the number of particle collisions, roughly tripling the number of times particles will smack into each other compared with the existing setup. Once the final version of the particle accelerator is online, it will run until the end of its operational lifespan in the 2040s and will be earmarked for replacement by a new, higher-energy particle accelerator in the years that follow.

"It really is an opportunity to explore the universe in a way we haven't done before," Mark Thomson, director general of CERN (the European Organization for Nuclear Research), where the LHC is housed, told New Scientist.

That jump means that experiments will produce much more data, which will allow scientists to study known phenomena, such as the Higgs boson, in more detail and increase the odds of observing rare events. For example, the HiLumi LHC is expected to produce about 380 million Higgs bosons over its lifetime of a decade or so, compared with the 55 million it's made to date. The data could help scientists solve problems with the Standard Model, which currently doesn't incorporate dark matter or dark energy, the primary forms of mass and energy in the universe.

"The LS3 represents a huge and complex logistical and engineering undertaking," Jean-Philippe Tock, head of the LS3 coordination team, said in a statement. "In the LHC alone, 1.2 km [0.75 miles] of magnets and components will be removed and replaced with new equipment, and across the whole complex, dozens of projects are planned, involving thousands of engineers, physicists, technicians and support personnel."

While the LHC won't be smashing any particles together during the shutdown period, researchers will continue to analyze data already collected during experiments during the prior operational window.

Though the LHC's primary purpose is fundamental physics research, technologies used to upgrade the collider could find their way into everyday life. For example, some instruments and techniques originally developed at CERN are now being used in medical imaging, sensors and art restoration.

Two lumps of potato discovered in a roughly 500-year-old Inca storage room in Peru are a rare find: freeze-dried potatoes predating the Spanish invasion, a new study finds.

These freeze-dried potatoes, known as chuño, were once a backbone of the Inca Empire's food supply and a product so fragile that they almost never turn up at archaeological sites.

The new discovery, made along Peru's arid south coast, is only the second time chuño has been recovered from an Inca site, researchers reported in the new study. It is concrete evidence that the empire directed one of its most important food sources hundreds of miles from the Andes, down to the Pacific Ocean.

Chuño is made by repeatedly exposing potatoes to nighttime frost and daytime sun until nearly all their moisture has evaporated, leaving a lightweight, long-lasting vegetable that can be stored for decades. This technique works only at high elevations where hard frost occurs regularly, so chuño had to be produced in the mountains and then transported using llama caravans, often hundreds of kilometers, to feed people living elsewhere in the empire.

The Inca used the same drying method to preserve meat, producing a product called "charki" — the source of the English word "jerky," study principal investigator Lidio Valdez, an adjunct professor in the Department of Anthropology and Archaeology at the University of Calgary, told Live Science in an email.

In the new study, published May 1 in the Journal of Field Archaeology, Valdez and study co-author Katrina Bettcher, an independent archaeologist, reported that the chuño was found alongside an Inca pottery fragment and a broken spindle whorl, a tool used to spin fibers, such as raw wool, into yarn or thread.

The discovery happened during the 2024 field season at Tambo Viejo, an Inca provincial center in the Acarí Valley, where an archaeological team had worked for several years. Inside a small storage room, the team uncovered a clay pot sunk into the dirt floor, its top half long gone. As researchers scooped soil out of the broken pot, they reached its bottom.

"Almost at the base of the vessel, the two samples of freeze-dried potatoes were found," Valdez said. "They showed me without knowing what they were, and right away I said: chuño!"

Potatoes are roughly 80% water, and they typically rot within a week at lower, warmer elevations — making them a poor food choice for long-distance storage. Valdez said freeze-drying was likely discovered long before the Inca rose to power in the 15th century, perhaps when potatoes that were accidentally exposed to frost at a high elevation became dried out and people realized the result was still edible.

Because chuño can be made only above roughly 11,800 feet (3,600 meters), the samples at Tambo Viejo must have traveled down from the highlands, most likely via a llama caravan along the Inca road network, Valdez said.

"Chuño being a light product probably also made its transportation easier," he added.

The two freeze-dried potatoes survived thanks to the Acarí Valley's extremely dry conditions, which help preserve organic remains that would otherwise decay — the same conditions that have previously yielded naturally mummified guinea pigs (Cavia porcellus) in Valdez’s previous work at the site.

Beyond its archaeological importance, the ancient preservation method has lessons for today. "We still have so much to learn from the people of the past," Valdez said. "Food security is a main concern, even in our times; yet we waste food, perhaps more than at any time in human history."

Relatively few Inca sites along Peru's coast have been systematically excavated, and Valdez expects more evidence of chuño — and the long supply lines that carried it — to surface as archaeologists keep digging.

Do you know where pumpkins and blueberries come from? Find out with our fruits and vegetables quiz!

Trees in China that were planted as part of huge reforestation projects appear to grow faster than those in natural forests, a new study finds. This is possibly because the reforestation trees are responding more strongly to the rising atmospheric carbon dioxide, scientists say.

China is quickly turning green. The country has planted 66 billion trees since 1978, with plans for 34 billion more by the middle of this century, as part of its "Great Green Wall" to slow the spread of the Gobi and Taklamakan deserts.

These new forests absorb large amounts of CO₂, but it is unclear exactly how they differ from natural ones, study first author Yuhang Luo, a landscape ecologist at Peking University in Shenzhen, China, told Live Science.

Luo and his colleagues set out to study how differences between natural and planted forests, including species diversity, tree density and age, might affect how the forests respond to rising CO₂ and climate change.

"Planted forests are widely used in climate mitigation strategies, but most global ecosystem models do not distinguish between forest types or represent age-related dynamics adequately," Luo said. "So we felt it was important to clarify how these factors interact — not just for scientific understanding, but also for improving the models and assumptions that underpin real-world forest policy and carbon accounting."

Planted forests are those purposefully created by humans, such as those in the Great Green Wall. Natural forests, on the other hand, grow without human intervention.

The researchers used satellite data to track leaf area index, a measure of canopy density and a key driver of carbon uptake, to determine how fast the different forest types grew, and found a striking difference: Planted forests increased their leaf area 66% faster than natural ones.

Most of that difference was due to planted forests being, on average, much younger than the natural ones — and young trees grow faster than old ones. But even when comparing forests of similar age and growing conditions, the planted ones still grew 4.6% faster, and the difference was even more pronounced in mixed and evergreen forests.

This is largely due to how planted forests are managed. They tend to feature fast-growing species like eucalyptus and poplar and are often actively managed, with people removing competing vegetation and even fertilizing them. These interventions reduce competition for light, water, and nutrients, amplifying the fertilization effect of rising atmospheric CO₂.

This discrepancy peaks in planted forests when trees are around 30 to 40 years old and then declines noticeably after age 40. In contrast, natural forests grow more slowly but steadily, so have an advantage over the long term.

"Planted forests can be a powerful short-term tool for carbon uptake, but this advantage is temporary," Luo said. "For long-term carbon storage and resilience, natural forests remain irreplaceable."

Kevin Dsouza, who worked on reforestation models during his postdoctoral research at the University of Waterloo and was not involved in the new study, said the results make intuitive sense, as the sprawling leaves of young, fast-growing trees could lead to increased carbon take-up. But he is not sure that leaf area is the best measurement for tracking growth and carbon sequestration.

"It's not a bad proxy, but it doesn't give you the full picture," he said. "The canopy is just the top of the tree and the carbon is stored in all sorts of different places like wood, bark, roots and soil."

Another study of Chinese forests found that natural forests actually accumulate more carbon above ground than planted ones in their early years, Dsouza pointed out, so these results should be considered carefully alongside other factors.

Luo said the findings show that most global climate models are missing something when it comes to understanding how various forest types play a role in carbon sequestration and climate change.

"Land use management works in more subtle and specific ways than we had assumed," he said. "It is not just about planting more trees. It is also about when you plant them, what species you choose, and how you manage them over time."

Luo hopes these findings will help guide reforestation efforts, to ensure we get the most benefit from planting new forests to help mitigate the effects of climate change.

"Our work offers a more practical guide for forest-based climate action: when to plant, what to plant, how long the benefits last, and what current models are getting wrong. We hope that helps people make better decisions," he said.

Editor's note: A picture caption in this article was corrected at 5:16 ET on July 1 to say 66 billion trees had been planted.

A breakthrough in photonic chips could make large, costly, ultrafast lasers dramatically smaller, leading to portable and affordable imaging, diagnostic and information-processing devices, researchers say.

By using a decades-old overlooked laser architecture, scientists managed to fit an ultrafast laser onto a tiny photonic chip — a chip that uses light, rather than electricity, for computing operations.

In a new study published June 3 in the journal Nature, the team demonstrated that a tiny laser on the photonic chip could deliver 1.05 nanojoules of energy in 147-femtosecond (147 quadrillionths of a second) bursts — thereby competing with the output of laboratory-class ultrafast lasers.

Ultrafast lasers are used in a variety of applications, from precision manufacturing and eye surgery to biological imaging and atomic clocks, but the systems needed to power them tend to take up whole tabletops in labs or factories. Yet the powerful output of these laser pulses made them difficult to miniaturise onto photonic chips.

"For more than twenty years, a high-pulse-energy femtosecond laser on chip was widely regarded as a holy grail of integrated photonics," Tobias Kippenberg, a photonics professor at the Swiss Federal Institute of Technology(EPFL), said in a statement.

"Our result shows that it is not only possible, but that it can be achieved with a surprisingly elegant architecture that the integrated-photonics community had overlooked."

Forward-thinking breakthrough comes from looking back

Photonic chips manipulate light by using microscopic structures called waveguides — usually in the form of optical fibers or etched cavities — to carry information. They aren't particularly novel, and can be found in fiber-optic communications, medical sensors and lidar systems.

But photonic chips have previously struggled when handling high-powered, ultrafast lasers. That's because they need to contain light to extremely small waveguides, leading the light to interact strongly with itself and destabilizing the laser pulses.

To tackle this problem, the researchers looked at a laser architecture called the Mamyshev oscillator, created in 1998 by Pavel V. Mamyshev, a physicist and engineer at Bell Labs.

This oscillator, which has received little attention in the world of photonic chips, works by placing a nonlinear waveguide between two optical filters. This causes a high-intensity laser pulse to expand into a broader range of colors that can then pass through both filters while weaker light, which can cause laser destabilization, is blocked out. This technique essentially means that a high-intensity laser pulse can be maintained.

Because the Mamyshev oscillator doesn't require extra components to manufacture on a chip, it presents an attractive design for use on photonic chips. And although the laser cavity needed to direct an ultrafast laser is 16.5 inches (42 centimeters) long, it can be folded to occupy around the same area as a match head. This can't be done with conventional fiber-optic-based lasers, often used in photonic chips.

That takes care of the size, but the cost of ultrafast laser systems is another challenge. But because photonic chips can be fabricated using silicon wafers in the same fashion as computer chips, more than 1,000 laser cavities could potentially be produced in a single batch, the researchers said. As such, photonic chips with ultrafast laser capabilities could be produced at scale, in turn reducing manufacturing costs and even expanding their use.

Photonic chips capable of handling ultrafast lasers could, in the future, lead to portable tools for tasks like detecting pollutants or performing advanced medical diagnostics in the field, the researchers noted in the study. The technology also opens the door to smaller atomic clocks that can benefit navigation and future communications.

This eye-catching satellite snap shows off a sprawling mass of petrified lava surrounding the jet-black slopes of a potentially dangerous volcano in the heart of the Sahara. A smaller volcanic "skull" lurks near the shadowy peak's base.

Toussidé (also known as Tarso Toussidé) is a "potentially active" stratovolcano located within the Tibesti Mountains, which cover around 40,000 square miles (100,000 square kilometers) of northern Chad and southern Libya. The dark peak stands 10,712 feet (3,265 meters) above sea level, making it the second-tallest mountain in the Tibesti region.

The name Toussidé roughly translates to "which killed the local people with fire" in the language of the nearby Indigenous people, hinting at a destructive and deadly history. However, according to the Smithsonian Institution's Global Volcanism Program, there is no evidence that the volcano has erupted during the Holocene — the current geological epoch, which began around 12,000 years ago. It is unclear if it has actually killed anyone.

The dark blob surrounding the volcano is known as a massif. It is made up of layers of overlapping magmatic rock left by multiple ancient lava flows that effusively erupted, or slowly poured from, the volcano's summit.

The shadowy structure, which is up to 20 miles (32 kilometers) across at its widest point, stands out against the surrounding sand-covered plateau, which has been carved into a network of crisscrossing canyons by eons of wind blasting, according to NASA's Earth Observatory.

Just southeast of the massif (in the upper right of the photo), there is a small, white circle containing several dark patches. This is Trou au Natron — a roughly 3,300-foot-deep (1,000 m) volcanic crater, or caldera, which looks eerily like a giant skull when viewed directly from above.

The cranium-like caldera likely formed during an explosive eruption more than 120,000 years ago. It was once filled with a giant salt lake that was home to ancient algae and other microorganisms. When the lake dried out, around the start of the Holocene, the receding water left behind a thick layer of white salt surrounding a pair of eyelike volcanic cones.

Toussidé is one of the youngest mountains in the Tibesti range, which formed by similar effusive eruptions long before the stratovolcano was born. The entire region likely once matched the massif's dark hue before being relentlessly bombarded by sand and wind. In another 100,000 years or so, the massif may blend in with the surrounding plateau, according to the Earth Observatory.

While the shadowy volcano has remained dormant for several millennia, it occasionally puffs out steam from small vents, or fumaroles, near its summit, suggesting that it is still technically active, according to the European Space Agency. However, geologists have not properly assessed its eruptive potential.

Nearly 2,000 years ago, Mount Vesuvius buried a vast collection of scrolls in ash and scorched them into solid black lumps. Now, without unrolling them, researchers have virtually read two of them —‬ and uncovered what may be a work by a well-known Stoic philosopher.

The breakthrough comes from the Vesuvius Challenge, an international research effort to digitally read the scrolls that were preserved when Pompeii and Herculaneum were buried by ash and pumice in A.D. 79. Papyrologists, who study and preserve the ancient manuscripts, announced June 25 that they had digitally unwrapped the surviving portion of one scroll, known as PHerc. 1667, revealing roughly 5 feet (1.5 meters) of continuous Greek text across 20 columns. Researchers also recovered more than 70 columns of text from a second scroll, PHerc. 172.

"For nearly two millennia, many of these texts have been physically preserved but intellectually inaccessible," Brent Seales, Vesuvius Challenge co-founder and a computer scientist at the University of Kentucky, said in a statement. "Today ‪—‬ after years of interdisciplinary work combining advanced imaging, artificial intelligence, academic research and an innovation contest ‪—‬ we are finally able to read them."

Over the past few years, Seales and his team have used a synchrotron to essentially X-ray inside the scrolls and detect the ink ancient Romans used to write. The letters are then studied by papyrologists, who translate the text.

Part of PHerc. 1667 was physically opened in the 1980s, but overlapping layers obscured the writing so badly that the scroll was given a readability score of zero, Federica Nicolardi, a papyrologist at the University of Naples Federico II, said in the statement.

The handwriting and text of PHerc. 1667 suggest the scroll dates to the second or third century B.C., making it one of the oldest scrolls in the Herculaneum collection. This early date means it could not have been authored by Philodemus of Gadara, the first-century-B.C. Epicurean philosopher whose writings dominated the Herculaneum library.

Experts think the text reads more like a Stoic treatise on ethics and human behavior, and it specifically mentions Aristocreon, the nephew and pupil of the influential Stoic philosopher Chrysippus. Very little of Chrysippus' own writing has survived, so if the attribution holds up, it would be a significant addition to the historical record of early Stoic thought.

In a separate discovery, researchers identified a new book title within scroll PHerc. 139. The end of the scroll references Philodemus' eighth book of "On Gods." While this treatise had previously been known to exist, the new discovery reveals the work extended across at least eight volumes. Experts plan to reexamine other texts in the Herculaneum collection for additional volumes that may belong to the same series.

More than 600 Herculaneum scrolls remain unopened. It's thought that the villa was once owned by the father-in-law of Julius Caesar.

How much do you know about the Roman town destroyed by Mount Vesuvius? Find out by taking our Pompeii quiz!

About a decade ago, the Japanese government spotted a worrying pattern: Pediatricians were doling out a ton of antibiotics, well beyond what should be needed to treat the bacterial infections coming through their doors.

Antibiotics treat bacterial infections, not those caused by viruses, fungi or parasites. Yet doctors were often sending young patients home with antibiotics for illnesses unlikely to be bacterial. Treating nonbacterial infections with antibiotics can fuel antimicrobial resistance (AMR) and the rise of superbugs by unnecessarily exposing bacteria to the drugs, pressuring those bacteria to evolve strategies to survive. Resistant bacteria can then spread their adaptations to others, thereby compounding the problem.

In the long run, resistance could make common infections impossible to treat with existing drugs, raising the risk of serious illness and death across the population.

When pediatricians in Japan did treat bacterial infections, they were overusing the antibiotics that are likely to fuel resistance — "broad-spectrum" drugs that target many bacteria at once. When compared against 35 other high-income countries in 2015, Japan ranked dead last in the appropriateness of antibiotic choices for kids under 5.

One way to slow the development of AMR is to get antibiotic prescriptions under control. So Japan focused on one of its biggest sources of problematic antibiotic use: pediatric outpatient clinics.

"The clinics are a particular problem," said Dr. Yusuke Okubo, chief of clinical epidemiology and health services research at the National Center for Child Health and Development, a research center and hospital in Tokyo. Looking at Japan's overall antibiotic use, "90% of prescriptions are [from] outpatient clinics, not hospitals," Okubo told me. (Outpatient practices account for a similar proportion of antibiotic prescriptions in the U.S.)

A large proportion of problematic prescriptions were being written for children under 3 years old, especially those with upper respiratory tract infections, which nine times out of 10 are caused by viruses, Okubo said. The stomach bug gastroenteritis was another biggie for overprescription, despite most often being caused by a virus.

Government officials hatched an idea: What if each time a pediatrician chose not to prescribe an antibiotic in these cases, they earned a small financial reward — a tip for making a better choice? Each tip would be small, amounting to about $5 per claim at today's exchange rate, but could translate to thousands of extra dollars of annual income for individual clinics. That's no small matter for Japanese pediatricians, who Okubo estimates earn roughly $90,000 to $100,000 a year.

This incentive program, rolled out in 2018, has proved a success, so much so that it's since been expanded to cover more patients, more clinics and a wider variety of diseases. But what made the program work? I went to Japan to find out what systemic and cultural factors contributed to the program's success. Ultimately, I wanted to see whether other countries, like the U.S., could learn from this nationwide experiment.

The quietly rising threat of resistance

With bacteria, as with animals, it's survival of the fittest. When exposed to antibiotics, a percentage of bacteria die, while others survive. That surviving population has traits that help them withstand the drug's effects, which are encoded in "resistance genes." Bacteria can transfer those genes to the next generation by multiplying, as well as physically pass those genes to nearby bacteria. Plus, they can pick up new resistance genes through random DNA mutations.

All antibiotics come with the risk of pressuring bacteria to evolve resistance — it's an inherent feature of the drugs. However, broad-spectrum drugs carry the greatest risk, because they place pressure on a wider variety of bacteria than narrow-spectrum drugs do. The 2015 cross-country comparison found that Japanese doctors prescribed antibiotics with the lowest risk of resistance only 35% of the time, meaning most antibiotic prescriptions were for broader-spectrum drugs.

It's sometimes necessary to use broad-spectrum drugs — such as when an infection is resistant to narrow-spectrum options — but using broad-spectrum antibiotics when they're not needed hastens the development of AMR. So does using antibiotics for nonbacterial infections. In both scenarios, you're introducing evolutionary pressure that could have otherwise been avoided.

Globally, resistance is rising among common disease-causing bacteria; it's far outpacing the development of alternatives to antibiotics. In 2021, resistant bacterial infections directly caused 1.14 million deaths worldwide and contributed to another 3.57 million deaths. Those numbers could climb dramatically by 2050 if swift action isn't taken now.

Common pathogens already show high rates of resistance in Japan, and resistant germs contribute to thousands of deaths each year, with most occurring among older adults. People over 65 make up about 30% of Japan's population. As that percentage grows in the coming years, AMR-related illness may also increase, health officials worry.

Japan's youngest residents are also at risk, though, as resistant bacteria can sometimes pass from mothers to newborns at birth and can cause serious complications, like sepsis. Resistance has also been detected among respiratory bugs that frequently infect kids, such as Mycoplasma pneumoniae, said Dr. Takemi Murai, deputy head of the Infectious Diseases Division at Nagano Children's Hospital in Azumino. "There have been outbreaks of Mycoplasma that are resistant to antibiotics," he said.

Yet not long ago, the unrestrained use of antibiotics was a mainstay of Japanese medicine. (I'll dig into the myriad reasons why in later installments of this series.)

National insurance data sampled from 2005 showed that 60% of patients in Japan with nonbacterial upper respiratory tract infections were prescribed antibiotics, mostly broad-spectrum ones like third-generation cephalosporins, macrolides and quinolones. Most of those prescriptions came from clinics.

Something had to shift.

Tips for appropriate treatment

In 2016, Japan got serious about reducing its antibiotic misuse, releasing its first National Action Plan on Antimicrobial Resistance. It aligned with a global plan from the World Health Organization, which aimed to raise awareness of AMR and optimize the use of antimicrobials, including antibiotics, among its member states.

Two of Japan's big goals were to slash overall antibiotic use by 33% and broad-spectrum antibiotic use by 50% by 2020. The country came very close to hitting those ambitious targets by the deadline, and doing so was no small feat. The tipping program was just one of a slew of initiatives introduced to improve AMR awareness and antibiotic use.

Prior to the incentive's introduction, Japan's Ministry of Health, Labour and Welfare (MHLW) — whose role is somewhat analogous to the U.S. Department of Health and Human Services — rolled out educational campaigns for doctors and patients and wrote a manual for antibiotic use, with the first edition directed primarily at outpatient doctors. It emphasized that most acute respiratory tract infections and acute diarrheal diseases don't require antibiotics.

Among kids, children under 5 saw the highest antibiotic prescription rates, often receiving the drugs for respiratory infections. Data showed this overprescription problem was the worst in children under 3 being assessed for upper respiratory infections or acute gastroenteritis. The government's solution? Pay doctors extra to withhold antibiotics when faced with cases that don't warrant them.

"If the clinicians provide more appropriate medical services, we add additional payment," said Dr. Takuma Kato, a counselor at the Permanent Mission of Japan to the United Nations who previously worked on the incentive program for MHLW. In this case, they pay "a little bit more" when doctors don't give patients antibiotics for illnesses that are likely viral, he said.

A "little bit more" is accurate. Each tip is 800 yen, equivalent to about $7.20 when the program launched in April 2018 and about $5 at today's exchange rate.

Here's how it works: A caregiver brings in their sick infant or toddler for an initial visit, and the pediatrician determines the child likely has an acute upper respiratory tract infection or gastroenteritis. These illnesses are typically caused by viruses, so the doctor decides not to provide an antibiotic. The doctor explains this rationale to the caregiver and provides guidance for home care. If the appointment checks those boxes, the clinic can claim an extra 800 yen when they seek reimbursement.

Because mild viral infections typically resolve on their own in a few days, a strategy called "watchful waiting" can help clarify if a bacterium is actually at fault. So if a doctor does prescribe an antibiotic at the first visit, they'll often encourage the caregiver to bring the child back if their condition remains the same or worsens within a few days. The incentive and this "waiting" strategy go hand in hand.

There are a few technicalities. For example, the children being assessed must have no underlying conditions that might complicate their case, such as a weakened immune system. If children test positive on a formal diagnostic test for influenza or COVID-19, the incentive cannot be claimed. To qualify for the incentive, clinics must specialize in pediatrics and use a "comprehensive" payment system, meaning patients pay a standardized amount for the whole appointment rather than the itemized "fee for service" that is ubiquitous in the U.S.

Despite this fine print, the perk is pretty appealing for the clinics that claim it. "I think pediatric doctor associations are really happy," Okubo said.

Doctors say "small incentives add up"

The Japanese government generally incentivizes doctors to adjust their behaviors, rather than penalizing them for poor practices, Okubo said.

"It's a constructive message from the government: 'You changed your behavior, so we'll pay something,'" Okubo said. "This constructive approach motivates physicians, especially pediatricians, to apply their common sense to their actual practice."

This system is readily accepted by Japanese doctors, who have historically held a lot of political power, Kato noted. Just like in the U.S., their professional groups, such as the Japan Medical Association, lobby the government and typically push against policy proposals that they view as potential threats to their bottom line.

By contrast, an incentivizing approach is "very, very welcome, especially by the doctors' associations," said Dr. Norio Ohmagari, director of disease control and prevention at the National Center for Global Health and Medicine, part of the Japan Institute for Health Security (JIHS) in Tokyo. Ohmagari also leads the AMR Clinical Reference Center, which collaborates with the WHO on AMR countermeasures.

Doctors I asked confirmed that they like the incentive, namely because it boosts their profits.

"I apply for the pediatric antibiotic appropriate use support premium each time" it's applicable, said Dr. Yusuke Shibata, who runs the Shibata Pediatric Clinic in Asakusa, a historic district in Tokyo's Taito ward. "I appreciate the premium, as pediatric clinics already have low profits" compared with clinics that care for adults, Shibata told me in an email after I visited his clinic.

For first visits with kids under 6, clinics are paid a base rate of 6,040 to 7,210 yen, or about $38 to $45 at current exchange rates. An extra 800 yen (about $5) increases that fee by more than 10% — "a huge amount," Okubo emphasized.

Shibata estimates that his clinic sees about 30 to 40 patients with an acute respiratory infection or diarrhea each week, depending on the season. He can potentially claim the incentive for the first visit with each of these patients, assuming they don't have any conditions that would disqualify the claim.

On the high end, Shibata estimates that he might claim the incentive 180 times in a single busy month, which would total 144,000 yen, or about $900.

Dr. Atsushi Miyahara, who runs the Karugamo Clinic in the Setagaya ward in Tokyo, said he was already conservative about using antibiotics so the incentive rewards him for sticking with his status quo.

Fifteen years ago, when Miyahara opened his clinic, he noticed that other physicians prescribed a lot of antibiotics, and he questioned the practice due to the potential to fuel resistance. He provides his patients with informational flyers that explain the risks of resistance and how avoiding unnecessary prescriptions can reduce that risk. When antibiotics are needed, he predominantly uses narrow-spectrum drugs that pose a relatively low risk of resistance.

Miyahara said the local government and medical associations announced the antibiotic incentive when it was launched, and he felt its introduction has been very positive. It's increased his revenue and encouraged him to continue his stewardship practices. He estimates that for every 50 of his first visits with patients, he claims the incentive 10 to 15 times, so it applies to at least 20% of those visits.

The incentive's impact

Because some pediatric clinics qualified and others didn't — due to fee-for-service clinics being excluded — Okubo and his colleagues could directly measure whether the policy worked.

To assess the incentive's effects in its first year, the researchers looked at insurance claims from over 10,000 medical facilities from just before and after the policy's introduction. About 3,000 of the facilities qualified and claimed the incentive 316,770 times, totaling 253 million yen ($2.29 million at the time). These eligible clinics saw a 17.8% reduction in their total antibiotic use over a year without any negative effects for patients, such as higher hospitalization rates.

To see if those effects lasted, the team drew years of data from over 165,000 young children who went to either eligible or ineligible clinics. Within the first month of the policy's implementation, the former group of children saw a nearly 45% reduction in total antibiotic prescriptions, compared with the other kids. Cumulatively over the next four years, their overall antibiotic use and broad-spectrum-antibiotic use was 20% and 24% lower, respectively.

The decrease in antibiotic prescriptions did not come with an uptick in hospitalizations or healthcare costs, although there was a slight increase in the total number of doctor's visits. But that's what you'd expect as doctors track an infection over time, Okubo explained, meaning they likely employed the watchful-waiting strategy and had parents bring their kids back in if they didn't improve quickly.

Okubo's team has continued to track pediatricians' antibiotic use, and he noted that they're seeing "spillover effects" among age groups not covered by the incentive. In the under-20 age group, outpatient antibiotic prescriptions fell by 50% between 2011 and 2022. He thinks the incentive is a key driver of this trend, directly reducing prescriptions for the youngest kids while also triggering ripple effects in older groups. (This research will soon be published in a peer-reviewed journal.)

That said, there's room to improve doctors' selection of antibiotics when they are used, as the ratio of broad- to narrow-spectrum drugs is still too high. "Total antibiotic use was reduced, but its quality should be improved further," Okubo said.

The incentive's evolution

While the 800-yen tip has proved significant to clinicians, the incentive represents a very small slice of overall government healthcare spending, which totaled 468 billion yen ($3.1 billion) in 2022.

"This program is not large compared to the whole budget," Dr. Kosuke Sasaki, who works in the MHLW's health insurance bureau, told me. The program's budget has no upper limit, so if the number of claims from clinics increased, there isn't a cap on how many could be paid out. "The number of doctors using this program has increased while the number of antibiotic prescriptions has decreased since the start," Sasaki's colleague Dr. Tomonori Aoki added, noting that the government isn't concerned about how to pay that rising bill.

The program's measurable impact and low price tag may explain its growth over the years.

Every two years, Japan's Ministry of Finance hands the MHLW its slice of the government budget, and MHLW then revises the pricing for drugs, medical devices and healthcare services. The antibiotic incentive falls under this revision process and has been expanded several times.

During its first revision in 2020, the incentive was extended to children under 6. In 2022, ear, nose and throat specialists (ENTs) newly qualified for the incentive; like pediatricians, they treat many acute infections in kids and tend to overuse antibiotics, insurance data suggested. That same year, doctors could start claiming the fee for ear infections and sinus infections.

"I see a tendency for pediatric clinics to avoid prescribing antibiotics, but I do see some ENT clinics prescribing antibiotics carelessly," Shibata, the clinic owner in Asakusa, Tokyo, told me. So ENTs seem to be a logical next target.

In 2024, a separate, facility-level incentive was introduced as a complement to the 800-yen incentive. It encourages clinics to submit data to a government database that tracks antibiotic use. If first-line, narrow-spectrum antibiotics make up a certain percentage of the clinic's overall prescriptions, that clinic earns extra money, Okubo explained.

Ultimately, the 800-yen incentive helped put AMR on the radar of doctors who didn't take it as seriously as experts like Kato, who told me "AMR is kind of my life's work." Kato and researchers like Okubo see the program as a success, although they pointed to room for improvement in antibiotic selection. Ministry officials like Sasaki and Aoki said the program is easy to implement and makes a difference. Clinic doctors like Shibata and Miyahara appreciate the incentive and use it consistently. All in all, at just $5 a claim, the incentive has been remarkably effective.

In speaking with experts in Japan and the U.S., I've learned that U.S. doctors have historically faced the same pressures and showed similar lapses in antibiotic use that Japanese doctors have. However, the U.S. does not have an incentive program like Japan's. Should it launch one?

In the next installment of this series, I'll explore a central feature of this problem: the motivations behind pediatricians' antibiotic misuse. What are they, and do those motivations differ between doctors in the U.S. and Japan? Answers to those questions will help determine whether a similar incentive might have the same impact in both places.

A Chinese system has become the world’s most powerful supercomputer, surpassing American machines for the first time since 2021.

LineShine, installed at China’s National Supercomputing Center in Shenzhen, clinched the top spot in the 67^th TOP500 ranking of the world’s most powerful supercomputers. The new system has already been used in a range of fields, giving developers another route to achieve supercomputing power.

The machine, which came online in the first half of 2026, can reach speeds of 2.198 exaFLOPS — where 1 exaFLOP is 1 quintillion (10¹⁸) floating-point operations, or mathematical calculations, per second (FLOPs) — making it the only supercomputer on the planet to exceed 2 exaFLOPS per second. It's also the first time China has hosted the world's fastest supercomputer since 2017.

A FLOP is a type of calculation used to benchmark computing performance. Exascale supercomputers can perform more than 1 quintillion of these operations every second. In comparison, home computers can perform roughly 5 trillion FLOPS.

According to TOP500, LineShine can achieve speeds about 22% faster than El Capitan, a supercomputer housed at Lawrence Livermore National Lab in California that had previously held the top spot since November 2024.

The system’s computing power is the result of "a comprehensive breakthrough in a series of core technological barriers," according to a translated statement from China's National Supercomputing Center.

Unlike many other supercomputers, LineShine uses only central processing units (CPUs) to perform calculations. Other systems rely on both CPUs and graphics processing units(GPUs), which run many jobs simultaneously by dividing tasks among smaller, specialized cores.

Since 2018, the U.S. government has restricted exports of semiconductor chips to China, including GPUs. However, startups such as DeepSeek have wrangled other technological advancements to train artificial intelligence (AI) models with fewer and less powerful GPUs than comparable systems such as ChatGPT.

LineShine "represents a historic leap forward for China's supercomputing field, breaking through foreign technological blockades and building an independent and controllable software and hardware system," the statement read.

The system has already been used on projects in multiple research areas, including atmospheric science, drug discovery and AI, according to the National Supercomputing Center. In general, supercomputers perform extremely complex calculations at speeds much faster than traditional computers can handle, allowing them to solve problems that would otherwise take too long or cost too much to address.

The fastest supercomputers utilize a range of different designs and processors, showing that high-performance computing doesn’t rely on any one single method.

"The list demonstrates that there is no single dominant technology path to leadership-class computing; instead, vendors are pursuing a variety of CPU, GPU, APU, and custom-accelerator approaches coupled with different interconnect and system designs," TOP500 representatives said in a statement.

Following LineShine and El Capitan, two supercomputers at U.S. national laboratories and one in Germany claimed spots three through five on the TOP500 list. Machines in Italy, Switzerland, Japan and the U.S. round out the top 10.

Can you match these ancient devices to their pictures? Find out with our computing quiz!

Homer's "Iliad" and "Odyssey" have inspired countless books, movies and works of art in the nearly three millennia since the epic tales were first written. This small, bronze sculpture, once attached to an ancient box, shows how the Greek epics influenced the aesthetics of the enigmatic Etruscans.

The Sleep and Death cista handle, which is in the collection of the Cleveland Museum of Art, features a set of bronze figurines welded to form a decorative handle for a cista ‪—‬ a small, cylindrical, lidded box used for a variety of purposes in ancient Egypt, Greece, Rome and Etruria, an ancient region in central Italy.

The handle is roughly 7.3 inches long and 7.2 inches tall (18.5 by 18.3 centimeters). The figurines represent Hypnos (the Greek god of sleep) and Thanatos (the Greek god of nonviolent death) bending to lift the body of Sarpedon, one of Zeus' sons who fought in the legendary Trojan War.

Sarpedon fought on the side of Troy, leading his men into battle against the formidable Greeks, according to Book XVI of the "Iliad." The Greek hero Patroclus entered the fray wearing Achilles' armor to trick the Trojans into thinking the greatest Greek warrior had joined the fight and scare off the Trojans. Sarpedon met Patroclus on the battlefield, and even though Zeus wanted to save his son, Sarpedon was mortally wounded. The Greeks stripped Sarpedon's body of his armor, but Zeus commanded Apollo to retrieve the corpse and deliver it to twin brothers Hypnos and Thanatos, "who bear men swiftly away" (translation by A. S. Kline).

The ancient sculptor of this piece "succeeded brilliantly in capturing the pathos and emotion in a scene from Homer's 'Iliad,'" Michael Bennett, former curator of Greek and Roman art at the Cleveland Museum of Art, said in a video. And on a technical level, the piece is much more detailed than a typical Etruscan handle; this one appears to be almost ergonomically designed, as Sarpedon's limply falling hair can be used as a finger grip, according to Bennett.

But the reason the Etruscans adapted the visual aesthetic of Homeric epic to many of their artworks, such as sculptures and wall paintings, is still unclear.

Because the Etruscan language is only partly understood, most information about this civilization, which arose around 900 B.C., comes from outside sources, such as the Greek historian Herodotus, who was writing several centuries later. Herodotus believed the Etruscans came from Lydia in Asia Minor, not too far south of Troy. Coupled with the later legend that Aeneas, a Trojan hero, wandered to Italy after the war and helped found Rome, some experts, such as linguist Robert Beekes, believe the Etruscans may derive from the Trojans or groups that fought on the Trojan side. However, a 2021 genetic study found the Etruscans may have been local.

The Etruscans may have used scenes from the Trojan War to decorate their vases and bronze boxes because they felt kinship with the antagonists in the "Iliad." But they also might have adopted the aesthetics because the Trojan War was a popular theme in Greek art at the time, and vases and other works decorated in this style reached the Etruscans through extensive trade networks. The Etruscans then put their own spin on the stories of the Trojan War, focusing in particular on scenes of death and brutality, classical archaeologist Larissa Bonfante argued in "Etruscan Myths" (2006, British Museum Press).

For more stunning archaeological discoveries, check out our Astonishing Artifacts archives.

Can you put together last week's Astonishing Artifact?

June's full moon, the Strawberry Moon, will rise Monday (June 29) as seen from North America and Europe. As it does, it will be the lowest-hanging and one of the smallest full moons of the year.

The moon will officially become full at 7:56 p.m. EDT on June 29. It will appear nearly full and brightly illuminated Sunday (June 28) and Tuesday (June 30) as well, but the best time to catch it is when it appears on the southeastern horizon at dusk on Monday. At that time, it will be visible on the horizon and remain unusually low in the sky for viewers in the Northern Hemisphere.

Full moons that occur close to the summer solstice, which happened on June 21 this year, follow a lower path across the southern horizon. That's because the solstice places the sun at its northernmost point on the ecliptic (the path of the sun through the daytime sky), so the full moon near that time appears low in the southern sky. Because a full moon, by definition, sits opposite the sun in Earth's sky, it mirrors the sun's path from approximately six months earlier.

Observers in the Southern Hemisphere will experience the opposite effect, with the Strawberry Moon climbing high overhead and becoming the year's highest-rising full moon.

Anyone can see the full moon without specialist equipment. But a decent backyard telescope or pair of binocualrs can help you zoom in on lunar landmarks, like craters and mountains. If you've got a good camera, here's how to take the best photos of the moon.

A low-hanging 'micromoon'

June's full moon will be the second-smallest full moon of 2026, occurring when the moon is 252,442 miles (406,267 kilometers) from Earth — just 63 miles (102 km) closer than the year's most distant full moon, the Blue Moon of May 31, at 252,505 miles (406,369 km). According to Time and date.com, that makes it a micromoon, minimoon or apogee moon.

The Strawberry Moon's name comes from Native American traditions associated with the seasonal harvesting of strawberries and other ripening fruits. According to Almanac, several tribes used other names linked to summer harvests, including the Berries Ripen Moon, Blooming Moon, Green Corn Moon, Hoer Moon, Birth Moon, Egg Laying Moon and Hatching Moon. European names include the Honey Moon and Mead Moon.

As the Strawberry Moon rises into summer skies, look out for a yellowish, bright star to its upper right. That's Antares, a red supergiant star and the brightest in the constellation Scorpius.

Following the Strawberry Moon, the next full moon — known as the Buck Moon — will rise on July 29, setting the stage for both a total solar eclipse and a partial lunar eclipse in August.

How much do you know about the moon? Test your lunar smarts with our moon quiz!

During several recent conversations, people have told me that they've stopped checking their phones in the morning. Not because nothing was happening, but because everything was. They described the feeling as standing under a waterfall of perpetual bad news.

This experience is far from an isolated one. According to Reuters Institute's 2025 Digital News Report, 69% of Canadians at least occasionally avoid the news now.

Globally, 40% report they at least sometimes or often do the same, the highest figure ever recorded. People shared consistent reasons for this: the news put them in a bad mood, they felt overwhelmed and powerless to act.

As a researcher in developmental psychology, focusing on social development and psychological well-being, I argue that news fatigue is not laziness, weakness or a generational decline in civic interest. It's the predictable response of a human brain meeting an environment it was never designed to navigate.

Wired for bad news

Long before smartphones or even the printing press, our cognitive architecture was shaped by a single problem: stay alive long enough to reproduce. Our ancestors whose attention drifted past the rustle in the grass left fewer descendants than those who froze, looked and listened.

The brain that paid attention to threats was the brain that survived.

This is the foundation of what psychologists call the negativity bias, one of the most replicated findings in cognitive science. Across decades of research, the human mind has been shown to weigh negative information more heavily than positive, attend to it faster and remember it longer.

A predator nearby mattered more than a beautiful sunset. The cost of missing a real threat was death, while the cost of overreacting was a few minutes of wasted vigilance. The asymmetry made this bias adaptive.

Here is the problem: the human brain has not changed since then. We are the same species as we were thousands of years ago. What's changed is the size of the world it's asked to scan for threats.

Scanning the whole world

For most of human history, the threats our nervous system processed were local. A neighbouring tribe. A drought. The illness of a child we personally knew. Information about distant places would barely arrive, and if it did, it was mainly irrelevant.

In 2026, the same neurological system is being asked to absorb a war in one region, a financial shock in another, a climate disaster in a third and a violent crime in a fourth, all before lunchtime.

A study published in the scientific journal Nature Human Behaviour examined more than 105,000 real news headlines viewed nearly six million times. Each additional negative word increased click-through rates, while positive words had the opposite effect.

Recent studies suggest people around the world demonstrate measurably stronger physiological responses to negative news than to positive news. The body is reacting before the mind has decided whether the threat is relevant.

Some researchers have introduced a clinical framework for what happens in this instance called Problematic News Consumption (PNC) — a pattern of news engagement that results in preoccupation, dysregulation and disruption to daily functioning. In their 2022 study, the researchers found that 17% of American adults qualified as having severe levels of PNC. Among that group, 61% reported feeling unwell quite a bit or very much, compared with 6% of those who didn't.

For minority populations, news fatigue may be even more consequential.

Repeatedly witnessing harm directed at our own groups, even when we're not the immediate target, can have a significant psychological impact on people from the same group affiliation. For racialized communities, such as immigrants, the cognitive load could be even heavier, and the option to simply stop watching is much harder to exercise when the news is about their country of origin.

Looking away is not the fix

What's the solution to news fatigue? Well, it's not avoidance. A democracy depends on informed citizens.

Many adults already cite the spread of misleading information as a major source of stress. Withdrawing from accurate, trustworthy information only deepens the problem. We're wired to pay more attention to bad news, and that kind of content will find its way to us one way or another.

The fix is to manage the consumption and the sources.

Several approaches can help manage news fatigue and protect mental health. Containing news consumption to defined windows of time reduces the sense of being overwhelmed. Choosing depth over volume also matters: one carefully reported long-form article will inform you better than bursts of random, unreliable and emotionally loaded posts on Instagram.

There is also value in distinguishing between information and action — research on perceived control and stress consistently shows that the gap between awareness and agency is one of the strongest predictors of psychological distress. Identifying what you can actually do about what you read in the news, however small, regulates that response.

Finally, be wary of "rage bait" — intentionally provocative messages or content designed to boost engagement on social media platforms by eliciting negative reactions. Recognizing that certain content creators want to provoke rather than reflect reality creates useful cognitive distance.

The news will not become less "heavy." But our relationship with it can become more deliberate. Our brains were not built for this scale of input. They were, however, built to learn to adapt.

This edited article is republished from The Conversation under a Creative Commons license. Read the original article.

Earth may survive the fiery death of the sun, even as our star engulfs the innermost planets, a new study using state-of-the-art models suggests.

The findings offer a potential alternative fate for our planet, which was thought to face certain death as the sun engulfs it in a thermonuclear inferno billions of years from now. As a yellow dwarf star, the sun is expected to have a relatively calm, 10 billion-year life. But in about 5 billion years, it will run out of hydrogen to fuse in its core and begin fusing hydrogen in its shell, causing it to expand enormously into a red giant star and then an even larger "AGB star," before it ultimately dies as a white dwarf.

Now, in a Letter to the Editor published June 19 in the journal Astronomy & Astrophysics, astronomers used stellar evolution models and observed a nearby dying star to reassess Earth's ultimate, potentially fiery fate.

Solar tug of war

When the sun enters its later life stages, Earth will be at the mercy of two competing forces — a fate shared by countless worlds throughout the unimaginably immense span of cosmic time.

As the sun expands to potentially hundreds of times its current size, the increased tidal forces will pull Earth toward our rapidly ballooning, sputtering star. Yet the surging sun will also lose its puffed-up outer layers into space through stellar wind. As it sheds much of its mass and becomes lighter, its gravitational grip will weaken, allowing our planet to escape outward into the depths of the solar system, the models show.

"The fate of Earth depends on a delicate balance between these two effects," Mats Esseldeurs, a doctoral candidate at KU Leuven's Institute of Astronomy in Belgium and first author of the study, said in a statement. "If tidal interactions dominate, Earth is engulfed. If mass loss dominates, Earth escapes to a wider orbit."

Previous research only muddies the issue. Studies have made different assumptions about solar mass loss, tidal forces and planetary interactions that may occur as the inner solar system evolves. As a result, it's uncertain if Earth will survive both of the sun's giant phases before our star shrivels into a tiny-but-dense stellar corpse called a white dwarf.

In a glimmer of hope, astronomers have discovered intact worlds around white dwarfs. On the other hand, some white dwarf systems are littered with the rocky remnants of their destroyed planetary children. So the researchers observed the formerly sunlike, dying giant star L2 Puppis, located 200 light-years away in the "poop deck" constellation Puppis, to glimpse our solar future. L2 Puppis may be losing up to one-millionth of a solar mass per year, according to previous estimates, expelling a dusty disk that's thought to harbor a planet 12 to 16 times the mass of Jupiter.

Additionally, the researchers performed state-of-the-art gravitational calculations "based on the internal structure and dynamics of evolved stars," modeling the orbital evolution of the inner solar system and the sun's lifespan from its infancy to its final phase as a "burned out" white dwarf.

So long, Mercury and Venus

Based on observations of L2 Puppis' mass loss, combined with the updated stellar evolution models, the researchers projected that Earth will survive as it shifts to just outside the expanding sun's radius.

"The largest uncertainty no longer comes from the tidal calculations, but from how much mass the future sun will lose," Esseldeurs said in the statement. "Observations of sun-like giant stars currently point towards Earth's survival, but we need better observations before we can be certain."

But even if Earth survives, our solar system siblings will not be spared; the simulations suggest Mercury and Venus will be engulfed by the hellish blaze of our dying star.

Additional stellar observations and improved models will help elucidate our planet's fate. For example, the European Space Agency's PLATO mission, a space telescope that aims to search for Earth-like planets around sunlike stars, will launch next year. It will likely detect planets around aging stars, thus providing a more accurate account of this potentially doomed population.

See how much you know about the sun with our sun quiz!