Inside the world’s newest data centers, energy-guzzling computations proceed round the clock as AI chatbots and other generative AI tools tackle tasks from the frivolous to the weighty: assembling imagery for social media, proffering relationship advice, analyzing medical images to diagnose cancer, creating code for developers or detecting financial scams for banks.

Just as the popularity of AI tools has skyrocketed in recent years, so have the associated environmental costs. Data centers now consume 414 terawatt-hours per year, or about 1.5 percent of global electricity use, according to the International Energy Agency — an amount that grew by 12 percent annually for five years before jumping to 17 percent in 2025. By 2030, the agency projects that demand for electricity by data centers will more than double. Much of the increasing demand for electricity is being met by fossil fuels, while experts also worry about the use of local water resources to cool data centers in drought-struck regions.

Use of AI to generate text or imagery probably accounts for a mere sliver of any given person’s environmental footprint. And experts stress that the onus is on tech companies to reduce AI’s resource consumption, from creating smarter, energy-saving algorithms to building more efficient hardware.

Yet there are simple actions people can take to ensure that their AI usage has as little environmental impact as possible — from carefully considering where AI is needed to tailoring prompts to minimize the amount of computation required.

“Individual choices are not meaningless, and some are more powerful than people realize,” says computer scientist Ivana Drobnjak of University College London.

Energy-hungry bots

It is notoriously tricky to estimate the energy expended on processing an individual chatbot query. Google, for example, estimates that its chatbot Gemini consumes around 0.24 watt-hours to respond to a median-length text query — equivalent to the electricity needed to watch TV for less than nine seconds. It also uses about 0.26 milliliters of water and emits the equivalent of 0.03 grams of carbon dioxide (driving a gas-powered car for a mile would emit about 400 grams). Small individually, these expenditures build up for those individuals and companies that use AI tools a lot.

The reason AI models consume so much energy lies partly in the processors that power them, such as the graphic processing units (GPUs) that consume significantly more energy than the central processing units (CPUs) that fuel simpler tasks like web searches and email. It also has to do with the models that underlie most popular generative AI tools, including the large language models (LLMs) that power AI chatbots and assistants.

These are based on a particular design called transformer architecture. This allows LLMs to train on vast swaths of language patterns in text and, from this, compute hundreds of billions or trillions of parameters. These parameters can then be used to generate new strings of text, by predicting which words are likely to follow one other.

A transformer-based LLM is computationally intensive because for each new word it generates in response to a user’s query, it runs the query and the words that have been written so far through the model, performing billions of calculations each time.

Tech companies note that LLMs have become more energy-efficient over time; according to Google’s 2025 calculations, the 0.24 watt-hours that Gemini consumes on a median-length text prompt represents a 33-fold decrease compared with the model’s energy consumption the previous year.

In any case, even small amounts of energy add up quickly given the scale of AI use. Based on 2025 numbers from tech company OpenAI, Drobnjak estimated in May that, at that point, around 3.2 billion queries are being sent every day to its chatbot ChatGPT. Users are asking AI tools to process and produce vast quantities of text, images and video. Some are having lengthy conversations with chatbots. And, increasingly, people are creating their own “AI agents” that themselves send queries to AI chatbots.

So what can users do to minimize the resources spent on their AI use? Experts have some tips.

Don’t give up on search

As a first, simple measure to save energy, users should carefully consider whether they truly need AI for a given task. “Asking ChatGPT ‘What should I wear today?’ or ‘How is the weather?’ is like taking a Concorde to travel to your supermarket,” says Günter Klambauer, an AI expert at Johannes Kepler University in Austria.

The same goes for web search engines that use AI to automatically generate a response to a query alongside the actual search results, such as Google’s AI overviews or Bing’s Copilot search. “If you’re just looking for a particular article, turning that off could be powerful from a saving-energy perspective,” says Udit Gupta, an expert in electrical and computer engineering at Cornell Tech in New York City. Selecting “Web results only” in one’s browser or including “-ai” in the wording of your web search can do the trick.

Smaller models use less energy

People and businesses that use AI tools a lot for specific tasks like translating or summarizing could consider shifting to smaller language models that are specialized to these tasks. Because these are trained more narrowly and perform fewer computations, they expend less energy than the massive, all-purpose LLMs on the same tasks.

In one 2025 study published by UNESCO, Drobnjak tested the benefits of using small models — such as one called opus-mt-en-es for English-Spanish translations, and other models for summarization and query-answering — in lieu of the model Llama 3.1 developed by Meta. Though these smaller models are often less user-friendly than more popular AI models, they’re freely available from the AI platform Hugging Face. The small models consumed between 15 and 50 times less energy while producing higher-quality outputs on the tasks for which they were designed, the study found.

The shift away from larger models resulted in a 90 percent decrease in energy use overall, making this the most powerful single energy-saving strategy Drobnjak tested in her study. As Gupta puts it, “You don’t need to use a trillion-parameter model for editing an email.”

Less chatty chatbots

Because LLMs perform so many computations for every consecutive word they produce, it helps to choose models that produce less text in general. AI systems expert Mosharaf Chowdhury of the University of Michigan, who has been measuring the electricity usage of LLMs that have been made publicly available, has learned that models that are “chattier” by nature tend to consume more energy.

For instance, one version of the model Qwen developed by Chinese company Alibaba Cloud consumes significantly more energy when it’s in “problem solving with reasoning mode,” where it produced roughly 10 times as many words in response to a prompt compared to its “text conversation” mode. So some experts recommend using reasoning mode only for complex questions and otherwise sticking with a chatbot’s standard mode.

Simply asking AI chatbots to “be brief” or giving them a word limit can also save energy. In the UNESCO paper, Drobnjak and her colleagues found they could reduce the energy consumption of the Llama model by 50 percent when they instructed it to halve its output. By contrast, keeping the prompt itself short had less significant savings — just 5 percent for a prompt that was half the length of the original query.

“The size of the output is what determines and drives the energy expenditure the most,” Drobnjak says. She has collaborated with the city of San Francisco to develop energy-saving tips for AI users, which include being as specific as possible and adding instructions like “five bullets max.”

Go low-res and batch video

Similar recommendations apply for generating images and video, which can consume orders of magnitude more energy than generating text, as they involve iterating millions of pixels many times over, each time processing the entire image anew, says Drobnjak. Such tools are highly popular: Nearly 40 percent of teens ages 13 to 17 surveyed in a recent study by the Pew Research Center use AI to create or edit images or videos.

Drobnjak recommends generating images or videos only when necessary and only at the resolution necessary. “One option is to just start in low resolution,” she says, “and if the algorithm is in the right direction, you then start increasing resolution.” She also notes that editing existing images is always less computationally intensive than generating new ones from scratch.

And when generating multiple images, it helps to do so in a single session or batch, which is more efficient than doing so in multiple separate requests.

These actions may seem like a drop in a bucket, and in many respects they are, experts say. But small things add up. While waiting for tech companies, scientists and policymakers to find ways of reducing AI’s overall environmental impact, “the individual who knows to reach for the right tool can make a real difference,” Drobnjak says. “AI is [consuming] so much energy that we have to look at it from every angle.”

Editor’s note: This story was updated on July 21, 2026, to clarify that the energy use of individuals who use AI tools a lot is cumulative, not necessarily huge, as was originally stated.

This article originally appeared in Knowable Magazine, a nonprofit publication dedicated to making scientific knowledge accessible to all. Sign up for Knowable Magazine's newsletter.

Millions of people across Europe and North America will witness a solar eclipse on Wednesday, Aug. 12, but the event will vary greatly depending on the location. A narrow corridor stretching from Greenland to northeastern Spain will experience a total solar eclipse, much of Europe will enjoy a deep partial eclipse, and parts of North America will see a smaller partial eclipse.

Want to know what you can expect to see from where you are? Here's an overview of the event from various locations, along with the exact viewing times for the Aug. 12 solar eclipse.

Remember, it's important to wear certified solar eclipse glasses during all partial phases of the eclipse. Totality ‪—‬ when the sun's face is completely blocked by the moon ‪—‬ is the only time it's safe to remove your eclipse glasses. (It’s not too late to order last-minute eclipse glasses if you don’t have a pair on hand.)

If you're in the path of totality

If you're fortunate enough to be inside the 180-mile-wide (290 kilometers) path of totality — the path of the dark shadow of the moon — in eastern Greenland, western Iceland or northeastern Spain, you'll experience the moon completely covering the sun for up to 2 minutes, 18 seconds. The sky will darken to twilight, bright stars and planets may appear in the daytime sky, and the sun's spectacular corona (its wispy outer atmosphere) will become visible. Here’s a handy guide to all the gear you’ll need to get the most out of totality.

The closer you are to the centerline of the path, the longer totality will last. But the most important consideration is to stay within the boundaries of the path, because it has a hard edge. Madrid, for example, is barely outside the path and will see a 99.99% partial eclipse — and no totality whatsoever. The partial phases last an hour on each side of totality.

Here's when totality will occur in various locations for the Aug. 12 total solar eclipse:

• Scoresby Sund, Greenland: 4:35 p.m. WGST (up to 2 minutes, 17 seconds)
• Reykjavik, Iceland: 5:48 p.m. GMT (60 seconds)
• León, Spain: 8:28 p.m. CEST (1 minute, 45 seconds)
• Soria, Spain: 8:29 p.m. CEST (1 minute, 43 seconds)
• S'Arenal, Mallorca, Spain: 8:31 p.m. CEST (1 minute, 36 seconds)

If you're in North America

Viewers in North America will see a modest partial eclipse, with the biggest eclipse seen from northern and eastern Canada, Alaska and the northeastern U.S. The farther northeast you are, the deeper the eclipse will appear. Eclipse glasses are essential at every stage of the two-hour event, because there will be no totality. Here are the times of maximum eclipse in various locations:

• Iqaluit, Nunavut: 1:24 p.m. EDT (61% eclipse)
• St. John's, Newfoundland and Labrador: 3:00 p.m. NDT (53%)
• Fairbanks, Alaska: 8:27 a.m. AKDT (37%)
• Anchorage, Alaska: 8:21 a.m. AKDT (28%)
• Bangor, Maine: 1:53 p.m. EDT (23%)
• Quebec City: 1:46 p.m. EDT (24%)
• Montreal: 1:45 p.m. EDT (18%)
• Boston: 1:55 p.m. EDT (16%)
• New York: 1:54 p.m. EDT (9%)

If you want to watch totality from outside the path, there are many live stream options available, including planned streams from NASA and the European Space Agency.

If you're elsewhere in Europe and North Africa

Most of Europe and far northwestern Africa will see a spectacular deep partial eclipse, with more than 90% of the sun covered in many western cities. Although the eclipse will never become total, it will still be an impressive sight, though solar eclipse glasses will be required throughout the event. Here are the times of maximum eclipse in some major cities:

• Madrid: 8:32 p.m. CEST (99.9%)
• Barcelona: 8:29 p.m. CEST (99.8%)
• Algiers, Algeria: 7:33 p.m. CET (96%)
• Nice, France: 8:24 p.m. CEST (95%)
• Lisbon, Portugal: 7:36 p.m. WEST (94%)
• Dublin, Ireland: 7:10 p.m. BST (94%)
• Cardiff, Wales: 7:13 p.m. BST (93%)
• Belfast, Northern Ireland: 7:08 p.m. BST (93%)
• Paris: 8:17 p.m. CEST (92%)
• Tangier, Morocco: 7:40 p.m. WEST (92%)
• London: 7:13 p.m. BST (91%)
• Edinburgh, Scotland: 7:05 p.m. BST (91% eclipse)

To check exactly what you'll see and when, enter your location on an interactive map of the eclipse, which will give you a schedule for when the eclipse begins, peaks and ends where you are.

Bolstering a type of bacteria that lives in the uterus may help counter age-related changes that can make it harder to get pregnant, a new study suggests.

While fertility decline is often linked to changes in egg number or quality, the uterus also becomes less receptive to an implanting embryo with age. The new research suggests that changes in the bacteria living there may be part of the reason.

In experiments, treating aged mice and lab-grown human uterine cells with a specific species of Lactobacillus, a group of bacteria often found in the uterus, reduced signs of aging in the uterine lining and improved embryo implantation. This improvement was also seen with a specific byproduct of Lactobacillus.

The findings, published Thursday (Aug. 6) in the journal Cell Host & Microbe, suggest that the uterine microbiome could be a promising target for treating age-related infertility. However, experts who were not involved in the study cautioned that the research is still preliminary.

"This is an interesting and promising approach, but we still don't know whether these findings will translate into meaningful improvements in human fertility," said Dr. Alex Robles, a fertility specialist at Columbia University Fertility Center who was not involved in the study.

"The microbiome can be influenced by many factors, including genetics, diet, geography, environmental exposures and other lifestyle practices," he told Live Science in an email, "which is why it's important to validate these findings across diverse populations before developing broadly applicable treatments."

To explore whether and how the uterine microbiome changes with age, the study researchers analyzed samples of the endometrium — tissue from the lining of the uterus — from 149 women ages 20 to 45 who were undergoing fertility treatment in China. The older women had lower levels of beneficial Lactobacillus bacteria, particularly L. gasseri and L. crispatus. These bacteria are generally associated with a healthy reproductive tract.

"One finding that surprised us was that overall microbial diversity did not change markedly across the different age groups," study co-author Dr. Rong Li, deputy director of the Department of Obstetrics and Gynecology at Peking University Third Hospital in Beijing, said in a statement. "Instead, the major differences involved particular bacterial species."

Later, 93 of the women underwent in vitro fertilization (IVF), and of those, 56 became pregnant. Those who became pregnant had higher levels of Lactobacillus in their uterine lining than those who did not get pregnant. That said, the pregnancy rates were similar across women of different ages who underwent IVF.

To better understand the effect of these bacteria on the uterus, the team isolated five Lactobacillus species and tested how they interacted with uterine cells. L. gasseri stood out because it attached strongly to uterine cells, and this attachment was associated with reduced inflammation and lower damage from oxidative stress. The bacterium also produced large amounts of exopolysaccharides (EPS), a type of sugar molecule.

The researchers then purified these sugars into a postbiotic they call LG-EPS. Unlike probiotics, postbiotics are products of bacterial cells and thus do not contain live bacteria.

Then, the researchers ran tests in older female mice (roughly equivalent to a middle-aged woman) to see whether introducing L. gasseri or LG-EPS to the vaginal canal could affect the aging uterus. After four weeks of daily vaginal treatment with either the bacterium or the postbiotic, the mice had fewer signs of uterine aging, less inflammation and higher embryo implantation rates than the untreated animals did. (That said, the team did not measure how much of each treatment actually reached the uterus.)

When they tried the same test with a modified strain of L. gasseri that could not make EPS, they found that many of these benefits disappeared. That suggested that the exopolysaccharides were responsible for much of the benefit. LG-EPS also reduced signs of aging in artificially aged human uterine cells, improving their ability to support embryo implantation.

Further experiments suggested that the postbiotic works by modifying a signaling pathway that helps control cell growth and tissue repair. This pathway was overactive in aged mice and uterine cells, but treatment helped to normalize its activity. Blocking a key protein in the same pathway eliminated the treatment's effects.

Robles said postbiotic treatments could be especially interesting because they may be easier to manufacture than treatments containing live bacteria. "If confirmed in future studies, these treatments could potentially be used alongside IVF to improve the uterine environment before embryo transfer," he suggested.

But he cautioned that the study should not prompt people to try over-the-counter probiotics or other supplements as ad hoc fertility treatments.

"The reproductive tract is a delicate ecosystem, and introducing or eliminating certain bacteria could have unintended consequences," Robles said. "We do not fully understand what constitutes a 'healthy' uterine microbiome. As such, any intervention should be approached with caution."

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

Your favorite stretchy workout clothes may be much easier to recycle one day, thanks to a new type of elastic yarn that is as strong and stretchy as today's spandex-containing fabrics.

The yarn, described in a July 25 study in the journal ACS Materials Letters, is built entirely from polyethylene, the plastic used in milk jugs and single-use grocery bags. By contrast, most of today's stretchy fabrics blend spandex, a bouncy-but-weak polyurethane fiber, with a tougher fiber like polyester or nylon.

That combination gives clothes their stretch and durability. But because the fibers are chemically different, it's difficult and costly to separate them for recycling, and chemicals used to break down the fabrics are toxic. The result is that almost none of this material is recycled. An estimated 80% of textiles sold in the U.S. contain spandex, and most end up incinerated or in a landfill, study co-author Svetlana Boriskina, a research scientist in the Department of Mechanical Engineering at MIT, said in a statement.

To solve that problem, the MIT team turned to polyethylene, one of the world's most widely recycled plastics. For the yarn's stretchy core, the researchers created a soft, springy version of polyethylene akin to a rubber band. Around that core, they wound a second, stiffer polyethylene fiber, more like a fishing line, coiling it tightly the way a spring or a twisted phone cord is coiled. Because both materials come from the same plastic family, they don't need to be separated before they're recycled.

In laboratory tests, the researchers melted a spool of the yarn and respun it into new yarn 10 separate times. Each time, they tested its strength, and the recycled yarn performed just as well as the original in every case. In head-to-head tests, the new yarn even outperformed commercial spandex-polyester yarn in maximum load, meaning it could bear more force before breaking, according to the study.

The team has already shown that these lightweight polyethylene fibers can be engineered for other perks, too ‪—‬ like cooling, moisture wicking and stain resistance ‪—‬ building on their earlier work spinning polyethylene into wearable fabric. Even buttons, zippers and buckles could eventually be made from compatible plastics, so a whole garment could be melted down and remade without being taken apart first.

Scientists are preparing for an interstellar rescue of humanity's most distant spacecraft, Voyager 1, after fixing up its twin from billions of miles away.

According to a NASA statement released Aug. 4, a clever power-saving maneuver known as the "Big Bang" helped the agency avoid having to shut off another one of the Voyager 2 probe's three remaining science instruments later this year. The Big Bang procedure involves selectively shutting off some high-power instruments on the Voyager probes while switching on lower-power alternatives, all while keeping the spacecraft warm enough to operate in the frigid environment of interstellar space.

"The idea is to swap out a group of powered devices all at once — hence the nickname — turning some things off, and replacing them with lower-power alternatives, to keep the spacecraft warm enough to continue gathering science data," representatives from NASA's Jet Propulsion Laboratory, which manages the mission, wrote in an April blog post.

NASA carefully ran tests on Voyager 2 before implementing the procedure in May and June. Now, sharing the results of those tests in the Aug. 4 statement, NASA reports a successful power transfer that should keep Voyager 2 running a while longer.

"The savings should provide power to keep its three instruments operating for at least an extra year," NASA wrote of the Big Bang.

But power is dwindling on both nuclear-powered spacecraft, and Voyager 1 is in worse shape than its twin. Mission scientists were forced to turn off one of Voyager 1's last remaining science instruments in April.

Voyager 1's turn for a life-extending Big Bang will happen within a few months, to keep science operating there as long as possible, agency officials added.

Going out with a bang

Scientists decided to do the "Big Bang" on Voyager 2 first because it is in better health, and closer to Earth, than Voyager 1. Voyager 1 is nearly 171 astronomical units (AU, where 1 AU is the average distance between Earth and the sun) from our planet, while Voyager 2 is about 143 AU away. Both spacecraft are crucial for revealing clues about the region outside the heliopause ‪—‬ the sphere of influence the sun exerts upon our solar system ‪—‬ as they are the only working spacecraft at such a distance.

That distance is no small factor. In November, Voyager 1 will reach a milestone "light day" from Earth — when it takes 24 hours for a radio signal to travel one way from our planet to the spacecraft. Both spacecraft will also turn 50 years old in 2027, assuming they keep working.

Both Voyager probes launched in 1977, with Voyager 2 getting an opportunity for a "grand tour" of our solar system. An alignment of the outer planets — Jupiter, Saturn, Uranus and Neptune — that occurs only once every 176 years allowed both Voyager probes to maneuver from one planet to the next with minimal fuel usage.

Voyager 2 flew by all four planets, finishing its Neptune encounter in 1989, while Voyager 1 was tasked with flying above the plane, or "ecliptic," of our solar system after its closest approach to Saturn in 1981. As each spacecraft finished its close-up imaging of these planets, some instruments were shut off to extend their mission for as long as possible. But as the two spacecraft aged, more instruments needed to go quiet.

Plutonium, which the spacecraft rely on for power, has a natural decay rate, with the spacecraft now losing roughly 4 watts of power a year, according to NASA. In recent years, power supplies have turned critically low on both spacecraft. Voyager 2 would have needed to shut off one of its remaining three science instruments later this year if measures were not taken, and Voyager 1 was in slightly worse shape after an unexpected power drop in February occurred following a planned maneuver in deep space. Only two of Voyager 1's 10 science instruments remain powered after the latest was shut down in April.

Artificial intelligence (AI) has helped uncover new weaknesses in two cryptographic systems, including a simplified version of the Advanced Encryption Standard (AES) that underpins much of today's internet. While these headline-grabbing findings don't put anyone's passwords or bank accounts at immediate risk, experts say the research could mark the beginning of a new era in which AI becomes a powerful assistant for discovering flaws in the mathematical foundations of digital security.

In a blog post published July 28, representatives from Anthropic's Frontier Red Team said Claude Mythos Preview independently developed new cryptanalytic techniques against two different targets: a version of AES-128, one of the world's most widely used encryption algorithms, and HAWK, an experimental post-quantum digital signature scheme currently being evaluated as part of the U.S. National Institute of Standards and Technology's (NIST) effort to standardize cryptography for the quantum computing age.

It's tempting to interpret this news as AI cracking one of the internet's most important encryption algorithms, but the reality is less dramatic. Nonetheless, experts say the achievement could mark the start of a new age of digital security.

The power of encryption

AES protects huge amounts of everyday digital life, from encrypted websites and messaging apps to Wi-Fi networks and financial transactions. But the version Anthropic attacked wasn't the full AES-128 algorithm used in those systems. Instead, the researchers studied a seven-round version of AES, a deliberately weakened variant long used by cryptographers to test new attack techniques.

The full AES-128 algorithm uses 10 rounds of encryption, while Anthropic's research focused on a seven-round version. In a self-published study that has not been peer-reviewed, scientists Milad Nasr and Nicholas Carlini said Claude found a faster way to recover the encryption key from that simplified version, making the best-known attack between 200 and 800 times faster. However, the study stressed that the technique does not work against the full version of AES used to protect real-world systems.

The more significant result may instead involve HAWK. Unlike AES, which has protected data for more than two decades, HAWK is a relatively new digital signature scheme designed to resist attacks from future quantum computers. It's one of the remaining candidates in NIST's additional post-quantum signature standardization process, meaning it is still being scrutinized by researchers before its widespread deployment.

In a separate study, Anthropic scientists Zygimantas Straznickas and Stephen A. Weis found that Claude spotted a mathematical property that researchers hadn't previously exploited. Combined with existing attack techniques, this property made it much easier to recover HAWK's secret key.

Thomas Espitau ‪—‬ head of research at PQShield, a cybersecurity company that specializes in post-quantum cryptography, and a cryptographer who has published research on HAWK ‪—‬ described the work as "one of the most, if not the most significant, cryptanalytic result of the year."

"To say it plainly, this is great work, and it is exactly what the NIST process is designed to produce," Espitau told Live Science. "Candidate schemes exist to be attacked before they are deployed, not after."

Espitau said the attack combined previously known techniques with one missing mathematical insight that Claude identified, substantially reducing HAWK's estimated security margin. He believes the work demonstrates how AI could increasingly help researchers evaluate the strength of cryptographic systems before they are adopted.

"This development illustrates how AI can act as a powerful accelerator in cryptanalysis," he said. "Claude Mythos Preview identified the exploitation of the sign-flip symmetry, providing the final piece of a puzzle that the research community had been assembling."

Building defensive measures

However, not everyone thinks the announcement means AI suddenly outsmarted human cryptographers.

"There is nothing you need to change," Roberta Faux, head of cryptography at cybersecurity and quantum encryption company Arqit, told Live Science. "Both Anthropic and the outside cryptographers agree that you don't need to change your key sizes or switch your cryptography."

Instead, Faux said the bigger story is AI's ability to apply expert-level cryptanalysis across thousands of algorithms that relatively few researchers have had time to examine.

"The interesting prospect is not a model outdueling the world's best lattice theorist on one problem but a model applying solid, roughly expert-level analysis at scale to the several thousand ciphers nobody ever had the human-hours to examine," she said.

Faux also cautioned against attributing the HAWK breakthrough solely to AI.

"The HAWK attack used no exotic ingredients; it simply competently assembled tools that were already lying around," she said. "A post-quantum candidate is seriously scrutinized by maybe a few dozen people on the planet, so beating two years of review mostly reveals how thin that layer of review is."

For consumers, the immediate implications are reassuring. The encryption protecting online banking, shopping, messaging and cloud storage has not suddenly become obsolete. But for the researchers designing the next generation of cryptography, Anthropic's work hints that AI could soon help cryptographers test tomorrow's encryption schemes more quickly and more thoroughly than has previously been possible.

New images captured by the world's most powerful solar telescope have revealed something that was hiding in plain sight on the sun for 150 years: thousands of tiny whirlpools twisting across our star's surface. The ultra-detailed observations could help to explain some of the sun's most violent behavior as well as hint at the answer to a long-standing solar mystery.

The new time-lapse footage offers the first direct proof of a long-predicted phenomenon called Kelvin-Helmholtz instability. The effect itself isn't new to science; it's named for physicists Lord Kelvin and Hermann von Helmholtz, who described it in the 19th century. The physicists found that whenever two fluids slide past each other at different speeds, the friction between them, or shear, rolls into spiraling patterns. However, this is the first time this effect has been seen on the sun, where that shear plays out between neighboring streams of solar plasma.

Researchers captured the swirls using the U.S. National Science Foundation's Daniel K. Inouye Solar Telescope in Hawaii and then compared the images against computer simulations of the sun's visible surface, called the photosphere. The findings were published Aug. 5 in the journal Nature.

The resulting time-lapse footage from the telescope is unlike anything solar physicists have captured before. It shows dozens of tiny vortices clustering along the edges of magnetic regions, some accompanied by delicate, dark stripes known as striations, according to a statement from the National Science Foundation. The telescope's resolution is sharp enough to pick out structures just tens of miles across — a scale so fine that the vortices had gone completely undetected until now.

When the researchers lined the images up against their simulations, the match was close enough ‪—‬ down to the average spacing between vortices ‪—‬ to confirm that they'd finally caught the instability in action.

Beyond the impressive visuals, researchers think these swirls may serve an important function. By constantly twisting and mixing the sun's magnetic-field lines, these vortices may play a part in building up the energy behind solar flares and coronal mass ejections.

The effect also might help to explain the long-standing mystery of why the sun's outer atmosphere, or corona, reaches temperatures of around 2 million degrees Fahrenheit (around 1 million degrees Celsius) while its surface remains hundreds of thousands of degrees cooler, Thomas Rimmele, chief technologist at the National Solar Observatory, said in the statement.

The team now plans to use computer programs to automatically track these vortices across future observations. This will help them measure exactly how much these swirls contribute to heating the corona and driving the explosive space weather that can disrupt satellites, communications and power grids on Earth.

See how much you know about the sun with our sun quiz!

The U.S. Food and Drug Administration (FDA) has approved a new seasonal flu vaccine that uses mRNA as its base.

Moderna, the vaccine's maker, announced Wednesday (Aug. 5) that a vaccine advisory committee to the FDA unanimously agreed that the shot is safe and effective for preventing illness from seasonal influenza. The shot, called mFlusiva or mRNA-1010, has been approved for people ages 50 and older.

Similar to mRNA vaccines against COVID-19, the vaccine uses the genetic molecule mRNA to encode instructions for cells in the body. In this case, it prompts the cells to build hemagglutinin (HA), a protein found on the surface of influenza viruses. Flu viruses use this protein to infiltrate human cells, and it's the same protein targeted by conventional flu vaccines. Following vaccination with mFlusiva, the immune system learns to recognize the HA protein on targeted flu strains, thereby improving its ability to block the viruses from infecting cells.

The HA protein poses a major challenge for conventional flu vaccines because it mutates very rapidly as the viruses multiply and spread — and these existing vaccines take months to manufacture. That's one reason the resulting shots aren't always a great match for the flu viruses that end up circulating in any given year. A benefit of the mRNA platform is that vaccines can be produced very quickly and thus made to better match the season's dominant strains.

mFlusiva's approval was based in part on a late-stage clinical trial involving over 40,000 people ages 50 and up who were vaccinated for the 2024-2025 Northern Hemisphere flu season. Half received the mRNA-based shot, and half received a standard dose of a conventional flu vaccine (as opposed to the higher-dose option available to older adults in the U.S.).

Of the 40,000 participants, about 970 got sick with flu, including 2% of the mRNA group and 2.8% of the standard group. That means the mRNA vaccine was 26.6% more protective than the conventional vaccine against illness from flu in this trial.

mFlusiva also offered superior protection against each of the three flu subtypes included in the vaccine. And in participants ages 65 and up, the vaccine was 27.4% more protective, overall.

More people in the mRNA group experienced side effects like injection-site pain, headache, fatigue and achiness, compared with the standard group, but these effects were mostly short-lived and mild to moderate in severity. These side effects were consistent with what was seen in earlier trials of the vaccine.

An additional trial involved a group of adults ages 65 and older and directly compared mFlusiva to an existing high-dose flu vaccine, which is approved only for older adults in the U.S. The findings suggested that the mRNA vaccine generated superior immune protection than the conventional option, based on antibody levels.

These results led the FDA advisory committee to decide that the vaccine's benefits outweigh its risks, and the agency ultimately approved it. For adults ages 50 to 64, the vaccine earned standard approval, and for adults 65 and up, it earned "accelerated approval," meaning further trials will be conducted to confirm the benefit of the shot over the high-dose option for this population.

"Flu remains a significant public health challenge, and mFLUSIVA provides an important new option for America's seniors," Moderna CEO Stéphane Bancel said in a statement.

The approval appears to mark a shift in the government's stance on mRNA vaccines.

Under the second Trump administration, the federal government has been broadly retracting its support for mRNA vaccines, directly canceling hundreds of millions of dollars in funds for research and development and indirectly sending a chilling effect through the mRNA field, experts previously told Live Science. Even Moderna has been pulling back from investments, citing opposition from the U.S. market. Health Secretary Robert F. Kennedy Jr. has repeatedly voiced his opposition to mRNA technology.

When Moderna initially filed for mFlusiva's approval in February, the FDA declined to review the application — but then changed its mind one week later. The exact motivation for this reversal was unclear to experts.

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

In the dead of night on Wednesday (Aug. 5), part of a defunct SpaceX rocket slammed into the moon at more than 5,000 mph (8,000 km/h) — and a Korean lunar satellite has just shared the first images of the aftermath.

A series of photos snapped by South Korea's Danuri lunar orbiter on Wednesday reveal a small, blackened crater at the alleged site where a used Falcon 9 upper stage crashed into the lunar surface around 2:35 a.m. ET. The crash occurred near Einstein crater, on the northwestern limb of the moon, close to the terminator zone where lunar day and night meet. The photos were shared by the Korea AeroSpace Administration on social media on Thursday (Aug. 6).

Because this region was on the sunlit side of the moon at the time, the initial flare from the crash was not visible from Earth; however, scientists at the European Southern Observatory's Very Large Telescope in Chile reported seeing evidence of a debris plume lifting off of the lunar surface shortly after the collision, according to the CBC. (At this time, no photos of the debris plume have been released).

A preprint study shared earlier this week predicted that the crash would create a new crater on the moon measuring roughly 90 feet (27 meters) wide and up to 16 feet (5 m) deep — a dent too small to be seen from Earth, even with a good telescope. No measurements of the newfound crater have been shared yet, but they are likely to arrive in the coming days as other lunar orbiters, such as NASA’s Lunar Reconnaissance Orbiter, and Earth-based observatories get a chance to examine the crash site.

What caused the crash?

The pesky piece of space junk that hit the moon on Wednesday is the second (or upper) stage of one of SpaceX's Falcon 9 rockets that launched into space on Jan. 15, 2025. It was carrying a pair of lunar landers: the Blue Ghost lander developed by private company Firefly Aerospace, which successfully touched down on the moon in March 2025; and the Hakuto-R lander developed by Japanese company ispace, which lost contact with Earth and crash-landed on the moon in June 2025.

Unlike Falcon 9's first (or lower) stages, which can return to Earth for reuse, the rocket's second stages are discarded in orbit. This rocket piece spent nearly a year drifting in an elliptical orbit around our planet before a combination of solar radiation and the moon's gravitational pull nudged it away from us, according to Live Science's sister site Space.com. In May this year, independent astronomer Bill Gray first predicted the crash and when and where the collision would occur, before other experts confirmed his calculations.

The 4.4-ton (4 metric tons) rocket part is estimated to have struck the moon at roughly 5,400 mph (8,700 km/h). While many times faster than the speed of sound, that’s still much slower than the average meteoroid strike on the moon, making the crash that much harder to see.

More to come

This is not the first time that human-made objects have impacted the moon, nor will it be the last. Studying these crashes can lead to important insights about the moon’s composition.

For example, the 2009 crash of a Centaur rocket's upper stage near the moon's south pole was analyzed by NASA's Lunar Crater Observation and Sensing Satellite mission, which revealed subsurface ice in the area. As a result, the lunar south pole is now the most coveted location for missions that aim to establish a permanent human presence on the moon.

Studying human-made impacts like these will also be essential for managing the potential risks to future astronauts and missions, like the permanent moon base NASA hopes to build.

"Now that we're in an era where we're going to have more and more astronauts going back to the moon, perhaps permanently, we also want to understand how much of a risk these artificial impacts pose," Benjamin Fernando, a postdoctoral researcher at Los Alamos National Laboratory and co-author of a recent study on the impact, told CBC.

"It presents a different set of hazards than say the Apollo astronauts faced on the lunar surface from the average background meteoroids that are striking the moon every day. And what we want to try and do with this event is understand both the direct [and indirect] hazards."

Physicists have built a crystal out of an "einstein" tile — an elusive shape mathematicians spent years searching for — and found that it bends light in a way no ordinary crystal can.

In the new study, published July 29 in the journal Nature Communications, researchers arranged this never-repeating tile shape into a pattern of nanoscale holes. This structure, known as a photonic crystal, is designed to control the way light moves through it. When the team shined a laser at it, the crystal produced a swirling, pinwheel-shaped scattering pattern that responded differently depending on which direction the incoming light was spinning.

The tile solves what mathematicians call the "einstein problem," a decades-old puzzle asking whether a single shape could cover a flat surface endlessly without ever repeating its pattern. (The name is a pun on "ein stein," German for "one stone," not a reference to Albert Einstein).

In the 1970s, mathematician Roger Penrose showed that two different shapes, used together like floor tiles, could cover a surface without the pattern ever repeating. Then, in 2023, geometry enthusiast David Smith and collaborators finally found one: a 13-sided shape that they nicknamed the "Smith hat"

Yuto Moritake, an experimental physicist at the University of Tokyo, first came across the hat tile in a popular science book in 2024. Moritake specializes in photonic crystals — materials patterned with repeating structures (often much thinner than a human hair) that bend and steer light for uses like lasers and optical sensors. Almost all photonic crystals rely on patterns that repeat in a regular grid. Moritake wondered what would happen if he swapped that repetition for the hat tile's never-repeating arrangement.

"I decided to include it in our photonic crystal structure," Moritake told Live Science, describing it as the starting point for the project.

To build the structure, Moritake and his colleagues used two precision manufacturing techniques, called electron beam lithography and etching, to punch hundreds of thousands of tiny holes — each just 100 nanometers in radius, or roughly 500 times thinner than a human hair — into a thin film of silicon nitride. This ceramic material is commonly used in computer chips. The holes were arranged according to the hat tile's pattern, covering a chip roughly half a millimeter across ‪—‬ about the width of a pencil tip.

When the team shined a laser at the finished chip, the light scattered, or diffracted, into a pinwheel-shaped pattern that appeared on a screen. Moritake first photographed the colorful pattern using his iPhone's long-exposure mode. The setting captured faint light over several seconds. Then, he switched to specialized cameras for more precise measurements.

The pattern was made up of well-defined bright spots, called Bragg peaks, that stayed in the same positions no matter where on the chip the laser hit. That consistency confirmed that the structure had the kind of long-range, predictable order found in a quasicrystal — a class of material whose atoms (or, in this case, holes) follow an orderly pattern that never repeats, unlike the repeating grids found in ordinary crystals such as table salt or diamonds.

Because the hat tile itself has no mirror symmetry — meaning it doesn't look the same as its own reflection, similar to how a left hand differs from a right hand — the scattering pattern it produced was also asymmetrical in this way. Scientists call this property chirality.

That chirality led to the study's biggest surprise. Light can be circularly polarized, meaning it spins either clockwise or counterclockwise as it travels, like a corkscrew. When Moritake tested the structure with both types of spinning light, he found a subtle difference in how each direction scattered off the crystal. Ordinary quasicrystals, which do have mirror symmetry, cannot produce this kind of effect.

"This structure can have some kind of circular polarization dependence," Moritake said, adding that the effect — made only possible by the tile’s asymmetry — was not something he initially expected to find .

Now, Moritake wants to apply this never-repeating pattern to control light traveling inside a photonic chip, rather than light that simply bounces off its surface. This could lead to future uses in optical communications and optical computing ‪—‬ technologies that use light instead of electricity to transmit or process information, Moritake said.

See how much you know about Albert Einstein with our Albert Einstein quiz!

A German startup has debuted the world's first diamond-based quantum computing system to exceed 10 qubits.

The machine, built by engineers at Saxon Q, is a nitrogen-vacancy (NV) quantum computer, meaning it uses defects in synthetic diamonds as quantum bits (qubits) to perform quantum operations. Qubits can be manipulated to represent the 0s and 1s of data, as well as quantum states that are superpositions of both the 0s and the 1s.

The hardware is currently available in rack-mounted systems featuring up to 128 qubits, with 512-qubit configurations available for delivery next year. According to the company's road map, the goal is to scale to 10,000 qubits and beyond after 2030.

Although the technology existed before this debut, scientists have found it difficult to build systems beyond 10 qubits due to the difficulty of creating nitrogen vacancy qubits.

Although Live Science saw a technical white paper outlining how the technology works, there didn't appear to be any published research demonstrating a functional quantum computer based on the NV architecture operating with more than 10 qubits before this launch. It's still unclear exactly how well the firm's quantum computers stack up against other platforms.

Quantum mechanics and flawed diamonds

In the 1970s, scientists discovered that certain diamonds shone with a brilliant red light when illuminated in a specific way. Subsequent research determined that the optical shift was caused by annealing radiation damage that attracted isolated substitutional nitrogen atoms. In other words, nature occasionally produces a diamond that has a nitrogen atom where a carbon atom should be.

The unintegrated nitrogen atoms are drawn to the vacancy in the otherwise perfectly ordered carbon atoms inside the diamond. Although these flawed diamonds occur rarely in nature, scientists can create diamonds with nitrogen vacancies in laboratories.

Functionally, the single nitrogen atoms inside the vacancies act as if they were "trapped," and their electrons can "spin" independently of the electrons inside the surrounding carbon atoms.

Scientists exploit this "spin" feature by using special lasers to put the nitrogen atom's electrons in a specific state they measure as "zero." They can then use microwave pulses to precisely manipulate the electrons into numerous configurations, including quantum states that binary "bits" can't achieve.

Marius Grundmann, a professor of experimental physics at Leipzig University and co-founder of Saxon Q, said the breakthrough that allowed his firm to push past the 10-qubit barrier was a materials discovery.

When the Saxon Q team creates the vacancy inside its lab-grown diamonds, they co-implant sulfur. Per Grundman, “That's the key technology point. Because the sulfur lifts the chemical potential to a point that it's negatively charged. The sulfur supplies the electron; the sulfur also makes the vacancy attached to the nitrogen with a very high yield."

In other words, by co-implanting sulfur atoms, the Saxon Q researchers can express greater control over the individual qubits. Once the qubits are set with lasers and subjected to microwave pulses, they're ready for error correction. In a statement, Saxon Q representatives said the qubits achieved a 99.92% fidelity rate — fewer than one error per 1,000 operations — before error correction.

However, Grundmann told Live Science that the latest numbers as of July 22 showed 99.98% fidelity in single-qubit operations. That's comparable to state-of-the-art error correction results reported by other quantum computing labs, such as those from IBM and MIT, although it wasn't possible to independently verify the results.

Room-temperature quantum computing

It's difficult to compare Saxon Q's diamond-based NV systems with more established quantum computing platforms, such as superconducting qubits. Most recent research on NV systems has focused on quantum sensing applications, though at least one preprint study discusses hybrid NV/superconducting systems.

"We have a fully functioning quantum computer," Grundmann told Live Science. According to Grundmann, the company's quantum computers are on a par with those using other modalities. "We have a quantum computer that can execute quantum code that you can reach via the network, and it is a multiuser, multitasking, multicore system," he said.

If the Saxon Q systems ultimately prove comparable to existing solid-state quantum computing architectures, they'd be among the first generation of room-temperature quantum computers to reach performance similar to systems that require cryogenics and on-site monitoring.

The ease of setup is notable. Saxon Q's devices can be slotted into a standard computer rack and plugged directly into alternating-current power.

This provides a clear near-term advantage for clients who want to run algorithms on a quantum system without operating through the cloud. Grundmann said this could be especially important in edge computing scenarios, such as autonomous driving or robotics, where cloud communication could produce unacceptable latency.

Research comparing solid-state quantum systems indicates that superconducting quantum computers would typically operate faster than diamond-based NV systems. It's unclear, however, what the trade-off between processing speed and cloud latency would be or whether it could be addressed through scaling.

The current challenge to scaling diamond-based NV quantum computers beyond the 512-qubit range is the size of the chips. Saxon Q's current chips are limited to supporting either eight or 16 qubits. For more powerful systems, scientists will need to squeeze hundreds ‪—‬ or even thousands ‪—‬ of qubits onto a single array to support operations requiring hundreds of thousands or millions of qubits.

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

A fleet of telescopes around the world just captured the first shocking moments of a supernova explosion in the most detailed-ever observations of their kind.

The explosive event was first spotted by China's Einstein Probe space telescope as a flash of X-rays in March. Ground-based telescopes jumped in within the hour and quickly identified the flash as a supernova, a powerful explosion of a massive dying star. Before long, a big team of observatories was on the job, including the wide-field Vera C. Rubin Observatory, which began its ambitious 10-year survey of the sky in late June.

With this fleet of telescopes, astronomers charted how the light of the supernova, located 500 million light-years away, changed over time. They reported their results in two papers published July 14 in The Astrophysical Journal Letters.

Each science team verified the "shock breakout" ‪—‬ the point when a supernova emits its first light from the explosion as a huge shock wave. The recently detected supernova is only the second stellar explosion in the past 20 years in which a shock wave was observed, because these events tend to be short — only seconds to hours, the researchers noted.

They classified the stellar explosion as a Type Ic broad-lined (Ic-BL) supernova, meaning that the blast included jets with material moving close to light speed. This type of supernova is often associated with gamma-ray bursts, which are extremely powerful flashes of high-energy radiation from space. However, the recently detected supernova presented some surprises: Its shock breakout was the faintest seen in an Ic-BL supernova, and no gamma-ray bursts were observed.

"Follow-up observations using the most sensitive facilities found no evidence" of the gamma-ray bursts, Brendan O'Connor, an astrophysicist at Carnegie Mellon University and co-author on one of the studies, said in a statement. "One possibility is that the jet was 'choked,' either by the surface of the star or by circumstellar material surrounding the star."

Telescopes of the world unite

The Rubin telescope, located in Chile, happened to spot the explosion because it was viewing that particular patch of the sky at the time, known as the COSMOS Deep Drilling Field.

"Thanks to Rubin's rapid cadence and unprecedented sensitivity, continued observations are expected to provide detailed, long-term records of the supernova as it evolves for years to come," the science teams said in the statement. The Rubin Observatory will spend the next decade mapping the entire southern sky many times over, creating a time-lapse movie of the cosmos expected to reveal millions of supernovas, asteroids, comets, and other transient events.

As Rubin spots events in the sky, the Dark Energy Spectroscopic Instrument on the National Science Foundation's Nicholas U. Mayall 4-meter Telescope at Kitt Peak National Observatory in Arizona is tasked with springing into action for follow-up observations. The instrument confirmed the recently detected explosion as an Ic-BL supernova.

When the scientists dove into 10 years of data from the 570-megapixel Department of Energy Dark Energy Camera on the National Science Foundation's Víctor M. Blanco 4-meter Telescope in Chile, they found a "blue source" just where the supernova later occurred, revealing clues about what the star system and its environment looked like before it exploded.

Meanwhile, a team led by Jillian Rastinejad, an astronomer at the University of Maryland, College Park and co-author of the second study, used the Gemini Multi-Object Spectrographs on two telescopes — Gemini North in Hawaii and Gemini South in Chile — to investigate the explosion, among other observatories. Those telescopes also confirmed the explosion as an Ic-BL supernova, without the jets, and the astronomers obtained archival details on the star's structure and environment before their demise.

"Our observations allowed us to study the physics of three pieces of this explosion: the X-ray shock breakout, the accompanying supernova, and the interaction of the supernova with material previously cast out by the dying star," Rastinejad explained in the statement. "With this information we were able to map out the structure of the material surrounding the star and understand the star's violent lifestyle before it collapsed."

The star was about 20 times the mass of the sun and was classified as a Wolf-Rayet — a star that used up most of its hydrogen early in its life. Just before the star exploded, it periodically ejected massive chunks of hydrogen and helium, leaving behind only carbon and oxygen. These chunks of material generated shells that were visible in telescopes as individual events, including the first X-ray shock.

"This is the first time we've mapped out the pre-explosion environment of a star that has been stripped of hydrogen and helium," said Gokul Srinivasaragavan, an astronomer on Rastinejad's team who was a doctoral student at the University of Maryland at the time of the study. "Going forward, I'm excited to observe more shock breakout events in similar detail to test if all stripped stars have a similar ‘lifestyle' prior to collapse and what, if any, differences we see."

Every total solar eclipse travels from west to east, because the moon and Earth move in the same direction — counterclockwise, or from west to east. Earth rotates eastward once every 24 hours, and the moon also travels eastward as it orbits our planet. Because the moon's shadow moves across Earth faster than the planet rotates beneath it, the path of totality (the route of the moon's umbra, the darkest part of its inner shadow) always sweeps from west to east.

But if you've looked at maps of the Aug. 12, 2026, total solar eclipse, you may have noticed something puzzling. At first glance, the eclipse appears to do the exact opposite. The path seems to begin in far northern Siberia, near the North Pole, before heading toward eastern Greenland, making it look as though the moon's shadow were traveling from east to west. It then appears to curve over western Iceland and northern Spain. So what's going on?

The apparent reversal from Siberia to Greenland is an illusion. It's created by geometry, but it's also a result of viewing the eclipse on a flat map instead of on a globe. The moon's shadow follows a smooth arc across Earth's curved surface and never changes direction, as shown by this animation. This eclipse passes so close to the North Pole that the distortion caused by map projections makes the track appear to bend back on itself, when in reality, the shadow is simply sweeping over the top of the world.

"The path of this eclipse also has a strong north-south component, the combined effect of Earth's rotation and the tilt of both Earth's axis and the Moon's orbit," experts at NASA's Scientific Visualization Studio explained. "Combined with Earth's rotation, the umbra's eastern motion during the first half of its travel is effectively canceled out."

This causes the shadow to sweep over the Arctic in a broad curve, instead of following the more familiar west-to-east path. On a flat map, that curved route can make it look as though the eclipse briefly reverses direction, even though it never actually does.

The moon's shadow has two parts — the narrow umbra, where observers experience totality, and the much broader penumbra, where only a partial eclipse is visible. The widths of these shadows depend on the moon's distance from Earth, while their speed is influenced by the moon's orbit, Earth's rotation and the geometry of the eclipse.

If you are among the millions of people who will be in the moon's penumbra on Aug. 12, make sure to always wear a pair of certified solar eclipse glasses (or use a solar filter on your telescope or binoculars) to view the partial eclipse. It is never safe to look directly at the sun, except during the moment of totality, when the sun is 100% covered.

If you aren't in the right spot for the total solar eclipse, fear not. A near-total lunar eclipse will be visible over most of North America just two weeks later, and there are plenty of other summer skywatching highlights to watch for.

An ichthyosaur fossil found in Australia's outback may preserve a rare snapshot of a prehistoric food chain. Around 100 million years ago, the enormous marine reptile swallowed a flying pterosaur before being attacked by a giant ocean predator, new research suggests.

The fossil set, nicknamed "BOB" or "Bag of Bones," belonged to a 20- to 23-foot-long (6 to 7 meters) ichthyosaur, an animal that belonged to a group of dolphin-shaped marine reptiles that lived alongside the dinosaurs during the Mesozoic era, from about 250 million to 90 million years ago. But in a new study, researchers discovered fragments of a pterosaur's jaw — along with fish and cephalopod remains — preserved inside the animal's body cavity.

The finding is the first confirmed evidence that ichthyosaurs ate pterosaurs, an extinct group of flying reptiles that ruled the ancient skies, according to the new study, published July 28 in the journal Gondwana Research.

The fossils may also hint at the ichthyosaur's violent end. Its skeleton — discovered in 2019 in Queensland's outback — contains shattered bones, missing ribs and large crushing injuries. Researchers think the gruesome wounds may have been inflicted by Kronosaurus queenslandicus, a colossal crocodile-like apex predator that lived 120 million to 100 million years ago in the ancient Eromanga Sea in Australia.

A rare prehistoric meal

Fossilized stomach contents are a rare find because they can be preserved only under very specific conditions.

"Rapid burial after death is essential to prevent decay and scattering of remains," study co-author Matt White, a research associate at the University of New England in Australia, told Live Science in an email. "The animal must have died soon after its last meal so stomach acids don't fully digest the prey."

Researchers used advanced neutron imaging to peer inside BOB's stomach contents without breaking any of the fossilized formations. The scans revealed hidden bones and helped scientists determine that the remains were likely associated with the ichthyosaur's digestive system.

White said that advances in imaging technology are making it possible to uncover evidence that would previously have remained hidden inside fossils.

"Scanning techniques have also improved, which has enabled us to see inside specimens and reveal what they potentially ate," White said. The methods can also reveal "the shape of various organs" and internal bone structures, he added.

The pterosaur remains were found near the front of the ichthyosaur's body cavity rather than in their expected position as digested prey, which White and his colleagues think may be because the ichthyosaur struck the seafloor headfirst shortly after its last meal, shifting some of its stomach contents forward.

"We believe the animal died in the water column — perhaps from a pliosaur (Kronosaurus) attack or natural causes — and then sank," White said. "It impacted the seafloor with its rostrum, and connected soft tissues kept most of the body in sequence."

Reconstructing an ancient ecosystem

The fossil offers a rare glimpse into the food web of the ancient Eromanga Sea, which covered much of central Australia during the early Cretaceous period around 145 million to 100 million years ago.

Although ichthyosaurs are known to have eaten fish and squidlike animals, evidence that they ate pterosaurs, a common predator of the ancient skies, has been elusive. The new fossil suggests that at least some ichthyosaurs may have fed on flying reptiles that landed on the water or died and floated to the surface.

"Such discoveries yield valuable information about trophic interactions and allow us to reconstruct ancient ecosystems in greater detail," White said.

A camera drone operator captured footage of a humpback whale giving birth off the north coast of New South Wales in what is thought to be a world first.

Alexander Forrest, a commercial drone pilot for the Organisation for the Rescue and Research of Cetaceans in Australia (ORRCA), was conducting aerial observations of migrating humpback whales (Megaptera novaeangliae) on July 28. ORRCA is a nonprofit organization focused on the rescue, conservation and welfare of marine mammals.

During the survey, Forrest noticed a whale swimming slightly behind her pod and going unusually slowly. Then, he saw her give birth.

"It's incredibly rare to see a moment like this in the ocean. It's a very rarely documented encounter," Forrest told Live Science. "It's the first drone video as far as we know of a full humpback whale live birth. It gives critical inside moments in the first moments of a calf's life, and also discovers the behaviour of a new humpback whale mother and her freshly newborn calf."

An ORRCA spokesperson said that this is only the fourth time the phenomenon of a humpback whale giving birth had been filmed, in general. Scientists also have footage of other whale births, including a gray whale (Eschrichtius robustus) birth filmed off the coast of California and a sperm whale (Physeter macrocephalus) recorded giving birth in the Caribbean.

The drone video shows the newborn whale surface from blood-reddened water for its first breath. The mother then turns back to reunite with it. The scene was filmed around 0.4 miles (700 meters) from the shore at Kingscliff in northeastern New South Wales.

The birth is "a symbol of one of the strongest conservation efforts in history, returning humpback whales from near extinction to nearly 50,000 on the New South Wales coast," Forrest said. Gathering data on this humpback whale population is critical to "discovering more about where they birth, what happens when they birth, and what those early moments look like."

The footage will now be analyzed so that a report on the observation can be peer-reviewed and published in a scientific journal. Notably, the mother whale was trailing behind her pod when she gave birth, a detail biologists will compare with observations of other birthing whales that were accompanied by members of their pod. For instance, the 2023 drone footage of the sperm whale giving birth showed that she had 10 adult females near her that formed a protective circle and took turns lifting the calf up so it could breathe at the water's surface.

Throughout their first weeks, calves stay close to their mothers and learn critical behaviors, such as breathing at the surface.

"Humpback whales seem to have an incredible maternal bond with their offspring," Forrest said. "There is an 11-month period where this calf will be raised and feeding on very nutrient-rich milk until it is a yearling and can fend for itself."

A newborn humpback whale calf weighs 1 to 1.5 tons (900 to 1,360 kilograms) and measures roughly 10 to 16 feet (3 to 5 meters) in length. While feeding on its mother's milk, the calf will gain 100 pounds (45 kg) a day and develop the strength and food storage it needs for its first migration. Humpback whales undertake one of the longest migrations of any mammal, travelling up to 5,000 miles (8,000 kilometers) each way between the cold waters of the poles to warm tropical breeding grounds.

In the past 20 years, an increasing number of bacterial infections caught by children have been resistant to antibiotics, a new study finds.

The research, published in July in the journal JAMA Pediatrics, looked back at the past two decades, as well as looked forward, to predict how resistance rates might change in the decade to come. By 2035, some critical antibiotics will be met with "steep increases" in resistance among common bacteria, such as Acinetobacter baumannii and Klebsiella, the analysis found.

Antibiotic resistance contributed to 840,000 deaths among children under 5 in 2021, global estimates suggest, so if resistance continues to increase, that number could grow.

"These forecasts are warning scenarios, not inevitable outcomes," said study co-author Dr. Yanhong Jessika Hu, a clinical epidemiologist and public health researcher at Murdoch Children's Research Institute (MCRI) in Australia. "The projections broadly assume that historical patterns continue without a major change in direction," Hu told Live Science in an email.

If significant action is taken, that trajectory could be altered, she said.

"Resistance increased across all regions"

Antibiotic resistance is sometimes called "a silent pandemic," as it poses a formidable threat without stirring as much concern as other health crises, such as viral outbreaks. Resistance has gained attention in recent years, but the data on how it has affected children is patchy, said study co-author Dr. Penelope Bryant, a clinician-researcher at MCRI, Royal Children's Hospital Melbourne, and the University of Melbourne.

"It's perceived as being a lesser problem in children," Bryant told Live Science. "It's not a theoretical problem; it's real, and it's happening. But I think the visibility is just substantially less than in adults."

That's partly because many resistance-tracking efforts combine adult and pediatric data, and the adult data ends up obscuring trends in children, Hu said. "Adult findings cannot simply be applied to children because children have different infection patterns, antibiotic exposure and treatment options," she noted.

Meanwhile, studies aimed only at children tend to vary in the age groups and clinical settings they include, making direct comparisons difficult, Hu said. This lack of granularity hinders efforts to counter resistant infections in children through changes in policy or clinical protocols. Children also have fewer antibiotic options than adults do at baseline, which makes preserving those options even more important, Bryant added.

To help fill the gap, the researchers turned to the Antimicrobial Testing Leadership and Surveillance database, which contains clinical samples from children and teens ages 0 to 18 across 82 countries. These bacterial samples were collected between 2004 and 2022 from a variety of medical settings, including hospital wards, intensive care units and outpatient clinics. The included countries ranged from high-income, such as the U.K. and the U.S., to low-income, such as Malawi and Uganda.

The analysis included over 106,000 bacterial samples and assessed which antibiotics these germs were resistant to. The antibiotics were grouped based on the World Health Organization's Access, Watch, Reserve (AWaRe) system: "Access" antibiotics target few bacteria and are recommended as the first choice for most bacterial infections, "Watch" antibiotics have broader effects and should be used selectively for more-resistant infections, and "Reserve" antibiotics are considered last-resort options to use when all alternatives have failed.

"Resistance increased across all regions, showing that this is not only a problem in lower-income countries," Hu said. "However, the highest resistance levels and some of the steepest increases were seen in lower-resource settings."

A wake-up call

Part of the analysis zoomed in on eight bacteria that are considered "critical" or "high" priority by the WHO, meaning they impose a particularly high healthcare burden due to their resistance. Across these germs, resistance rates were similar across high- and low-income countries in 2004, but those trends diverged by 2022.

Overall, resistance to Access antibiotics declined across the study period, but that improvement wasn't the same across all settings. In high-resource countries, resistance to Access drugs fell from 48% to 29% among the eight bacteria, while it rose slightly — from 44% to 47% — in low-income settings. These percentages correspond to the number of bacterial samples from each year that showed resistance to at least one Access drug.

The decline seen in some countries is "almost certainly because of the large investment that high-income countries have put into controlling MRSA," Bryant said, referencing methicillin-resistant Staphylococcus aureus. MRSA can cause painful skin infections as well as life-threatening complications, like sepsis.

Modeling future trends, the team predicts that resistance to Access antibiotics will stabilize or decline across most regions by 2035. However, resistance against Watch antibiotics rose between 2004 and 2022 and is projected to continue increasing. Among the eight critical and high-priority bacteria, it rose from 14% to 24% in high-income countries and from 16% to 48% in low-income nations.

Resistance to Reserve drugs also increased among these germs, rising from 9% to 25% in high-income countries and from 4% to 37% in low-income ones.

While the model predicted "steep increases" in Watch resistance, it projected slower increases in Reserve resistance over the next decade, by comparison. These trends were driven largely by increases in low-income settings, but high-income settings were not spared.

"With low-income countries, the problem is amplified because of poor sanitation and because of unregulated access to antibiotics," Bryant noted. Easy access to over-the-counter antibiotics makes it more likely for the medicines to be misused, which ultimately pressures more bacteria to evolve resistance.

This analysis gives a snapshot of how antibiotic resistance is affecting kids now and how it might do so in the future. However, the data it's based on has some limitations. For instance, the samples collected from each country aren't necessarily representative of the entire nation; they came from only certain participating medical centers and each country contributed different numbers and types of samples. So "the results should therefore not be interpreted as precise national prevalence estimates," Hu cautioned.

"But it's the first large dataset, really, to look specifically at children," Bryant said. And "it gives us an idea that things are getting worse."

The team has made their analysis freely available to other researchers on the website AMR in Kids, where "AMR" stands for antimicrobial resistance. Future steps include surveying resistant infections in children in a more representative way, as well as modeling how different intervention strategies could help drive down the rates.

"I'm hopeful that this is a little bit of a sort of wake-up call around children, that it really isn't a problem just in adults," Bryant said.

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

Each year, tons of soil, silt and rocks flow into reservoirs in the U.S. and get stuck there, creating a "ticking time bomb" that threatens lives and livelihoods. According to a new study, around a fifth of the world's reservoirs are currently at high risk of filling with sediment, and by 2060, half could be inoperable as a result.

The sediment takes up space meant for water, putting additional pressure on structures that were not built to contain large quantities of sand and sludge. As the reservoir fills with the material instead of water, sediment-filled reservoirs pose a serious threat to water security and the safety of people living near or downstream of them — and as the climate changes, scientists expect the problem to worsen.

"We are losing storage space in our reservoirs faster from sediment accumulation than we gain space from new dam construction," Amy East, a geologist at the U.S. Geological Survey, told Live Science.

What is dam sedimentation?

Dam sedimentation is not a uniquely U.S. problem. Rain pulls sediment down slopes into waterways. Normally, this sediment would travel through the river system, shaping the water flow, creating habitats, and fortifying coastal wetlands and estuaries against erosion. In many parts of the world, this sediment is also a vital natural fertilizer for crops. But after a river is dammed, this sediment can collect in the reservoir.

A 2023 study published in the journal Science found that sediment buildup was the greatest threat to global water storage in existing reservoirs — even more than drought.

New research, which includes smaller reservoirs, has offered a more nuanced and concerning picture. In the study, published June 5 in the journal Nature Sustainability, researchers assessed the state of reservoir sedimentation globally. They looked at more than 550,000 reservoirs, most of which spanned less than 0.4 square miles (1 square kilometre). They found that almost 1 in 5 of reservoirs globally are at high risk of filling up with sediment.

The researchers found that sedimentation is eating into global reservoir storage capacity at about 7.3% every decade. There are 16 global hotspots that are at high risk of reservoir sedimentation, threatening water supplies to more than 2 billion people and impacting more than a quarter of global irrigated land. One of these hotspots includes the western U.S.

The authors found that sedimentation risk was especially pronounced in regions with dense small-reservoir networks supporting key crop systems.

"Without intervention, we project that, by 2060, more than half of all reservoirs could become functionally inoperable," the authors wrote. This includes more than half of all small reservoirs and more than a third of large reservoirs globally.

Where is it a problem in the U.S.?

North America has the second largest number of reservoirs, after Asia, according to the global survey. And at 7.8%, its sedimentation rate is higher than the global average, ranking it third after Oceania (9.9%) and South America (8.1%),

The U.S. is home to many small dams, said Matthias Kondolf, a geomorphologist at the University of California, Berkeley who wasn't involved in the study. "All the focus tends to be on the big dams, and these many, many small ones have been neglected," he told Live Science.

From the 1940s to 1970s, there was a big push by the U.S. government to build "farm ponds," he said. In western Oklahoma, for example, "all these dams are now filling up with sediment, and there's nothing in place to assess the safety of these features, which have now become threats."

Some of these dams have already failed, following large storms as the ageing dams were not able to cope with the volume of water. A 2018 study found that since 1980, there have been on average 24 dam failures a year in the U.S.

Reservoirs in some regions are more at risk than others. The western U.S. is a natural hotspot because it has a steeper topography, meaning more sediment naturally ends up in watersheds, East, who wasn't involved in the new research, said.

And in areas where human activities like farming or logging disrupt the landscape, rainfall is likely to drag even more sediment into reservoirs, East said. "Those types of land use can create sediment-producing hotspots almost anywhere."

In California, for example, more than half of small reservoirs in maize-growing areas are filling up with sediment at a rate of more than 10% a year, which threatens local maize production.

The threat to water security will be particularly acute in places struggling with wildfires, such as the western U.S. After fires, rain washes the debris and sediment into watersheds. A 2024 study in California found that most of this post-fire sediment erosion occurred upstream of reservoirs, rather than in places where sediment would move downstream directly to the ocean.

The dam-sedimentation situation is likely to get worse as the climate changes, researchers said. As the climate changes, there will be more extreme weather events, such as droughts and wildfires, adding more sediment to watersheds. Dams are designed to cope with the pressure of water, not sediment which exerts more force on dam walls. Moreover, in seismically active areas, the sediment vibrates at a different frequency than the concrete of the dam, which creates further impact against the structure. Additionally, the dams are just getting older.

"What do we do 50 or 100 years from now when we have all these reservoirs across the landscape filled with sediment, sitting there as ticking time bombs?" Kondolf said.

What can be done about it?

For a reservoir to be sustainable long-term, the amount of sediment entering it and leaving it should be the same.

"A big part of preventing reservoir sedimentation problems is upstream soil conservation in the watershed," East said. Interventions include ensuring that land use, such as agriculture or timber harvesting, follow best practice to reduce the amount of sediment washing off the landscapes.

If sediment is already in the dam, it can be difficult to manage and expensive to remediate, Kondolf said. Some dams, such as Fall Creek Dam in Oregon, have mechanisms that enable engineers to release sediment. But in the past, reservoirs were not designed to manage sediment and little thought was given to how to decommission them.

"This is one of those issues that falls in the cracks between different agencies and responsibilities," Kondolf said. Some larger facilities fall under the remit of the federal government. Other dams fall under state governments. California, for example, recently launched a state-sponsored program to future-proof the state's dams.

But smaller dams often get overlooked, Kondolf said.

One option is to remove the dams entirely. For example, sediment-related concerns contributed to the decision to remove the Elwha and Glines Canyon dams in Washington. The Elwha River later carried most of the sediment to its river mouth.

For smaller dams with a relatively small amount of sediment, "you just blow up the dam and let the sediment work its way downstream", Kondolf said.

There are other technological solutions, but they are expensive, such as retrofitting dams to enable them to pass sediment; creating a bypass to route sediment-heavy water around the dam; and mechanical dredging.

Another option is to empty the reservoir of water and let the river cut a channel through the sediment, Kondolf said.

However, released dam sediment brings its own risks. If not managed carefully, sediment can flood the river system and disrupt downstream ecosystems.

"The economics of managing reservoir sediment long-term were not generally incorporated into dam design and planning in the last century when many western-U.S. water projects began," East said. This has "pushed the cost burden on future generations."

But the reality is that reservoirs around the country are filling with sediment. It is reducing their ability to store water and potentially endangering the communities living downstream of them — and unless addressed, the problem will only get worse.

Researchers have designed a material that can "program" the way it releases heat, paving the way for more efficient energy systems and, potentially, devices that store information using heat instead of electricity.

The design, described in a June 25 study in the journal Laser & Photonics Reviews, sidesteps a nearly 160-year-old rule of physics linking how materials absorb and emit heat. Under ordinary conditions, a material that's good at absorbing heat from one direction is equally good at emitting heat in that direction. This rule of reciprocity, first described by physicist Gustav Kirchhoff in the 19th century, has limited engineers' ability to control incoming heat independently from and outgoing heat.

In the new study, the researchers designed a theoretical device that could direct heat radiation in different directions and remember that setting even after the power was switched off.

The new device pairs two materials that don't normally work together. Using a magnetic field, the team broke the natural symmetry in a layer of indium arsenide ‪—‬ a material that absorbs and emits infrared light ‪—‬ so that radiation traveling in one direction behaves differently than radiation traveling the other way.

On top of that layer sits a grating made of germanium-antimony-tellurium (GST) — a phase-changing substance that can switch between two distinct physical structures and stay in whichever structure it's set to until it's deliberately switched again. Once the GST is set into position, it locks the directional difference of radiation in place and holds it there without needing continuous power, which is what lets the device's heat-directing behavior be "programmed."

"I was impressed by the elegant combination of magneto-optical nonreciprocity with a nonvolatile phase-change material," Juejun Hu, a professor of materials science and engineering at MIT who wasn't involved in the study, told Live Science in an email.

That's significant because earlier attempts at this kind of directional control typically worked only at steep angles, which made them impractical. It's "particularly noteworthy" that this device functions when radiation arrives just 3 degrees off an otherwise-straight line, making it far easier to fit into real-world optical systems, Hu said.

The researchers compared their design to computer memory, since it holds onto its programmed state after the power is cut. However, the device stores a material state rather than heat itself, Hu told Live Science. GST simply keeps its amorphous or crystalline structure without power, which preserves the programmed response.

For now, the device exists only on paper; it hasn't been built or tested. Still, Hu thinks it's realistic, since it relies on well-established materials and manufacturing methods. However, the GST layer is thick enough that switching it back and forth repeatedly would be difficult, though other materials could fix this problem. Once that hurdle is surpassed, Hu expects the first real-world use to be infrared sensing, where compact, direction-selective heat absorption is most directly useful.

The brain preservation paradox — the discovery of well-preserved human brains among otherwise skeletal remains — has puzzled archaeologists and pathologists alike for decades. Now, new research finally provides a scientific explanation for this longstanding mystery.

"We found that brain preservation isn't a rare anomaly, it's a novel chemical pathway," first study author Alexandra Seviour, a doctoral researcher of paleobiology at the University of Oxford, told Live Science in an email about the new work, published June 19 in the Journal of Proteome Research. "Under the right conditions, preservation actually arises from decay itself: the same reactions that degrade tissue can also weld the breakdown products together into something far tougher."

Despite being one of the first tissues to begin decomposing after death, human brains are surprisingly prolific in archaeology: more than 4,400 preserved brains have been discovered among human remains spanning the last 12,000 years, according to earlier work published by Seviour.

Mummification, freezing, and even saponification (where body fat turns into a greasy substance called grave wax) can all preserve soft tissues, sometimes for millennia. Usually, these processes conserve the structures of multiple body parts, including the internal organs and skin. But bizarrely, around one-third of the archaeological brains recovered don't fit this model, and a shrunken mass of protein is the only surviving tissue left among a cluster of bones.

The bulk of these unexplained brains were found in waterlogged, oxygen-poor (hypoxic) ground — anything from riverbeds and lake shores, to flooded caves and sunken shipwrecks. "Water, being nature's solvent, is typically associated with decomposition, not preservation, " Seviour said. "So the surprise is really the selectivity." In other words: Why is it only the brain which survives under these conditions?

Burying mice

Seviour's team hypothesized that this specific burial environment, combined with the brain's unique structure and chemistry, divert the normal decay pathway away from total breakdown — instead stabilizing the brain's proteins via a different chemical sequence. To test this theory, they buried mouse carcasses in four different water and oxygen conditions and evaluated their decay pathways over a period of six months.

"At 24 hours, 72 hours, one week, six weeks, three months, and six months, we dissected the brains and analysed them using high-resolution mass spectrometry to see exactly which proteins were still present and in what state," Seviour explained. "We were looking for which specific peptides survived and which vanished, and what chemical marks were left on the survivors."

Overall, their analysis yielded more than 1.26 million protein decay trajectories, enabling the team to draw patterns about how and when the chemistry diverged under the different conditions. Early analysis showed that the initial steps of decay were fairly similar, but that after a few weeks, oxygen levels became the controlling factor, with more oxygen leading to faster and more widespread decay. Conversely, wet, low-oxygen conditions favored the formation of toughened protein structures, which resisted further decomposition and preserved the remaining brain tissue.

The solution comes down to free radicals — extremely reactive particles with a single, unpaired electron. Abundant oxygen initiates a chain-like free radical chemical sequence in the brain proteins, which quickly degrades the entire protein structure, Seviour said. However, in hypoxic conditions, there is simply not sufficient oxygen for this same cascade to occur; instead, intermediates in the sequence form crosslinks with other neighboring parts of the brain protein, creating tough and insoluble aggregates that resist decay.

Brain tissue is particularly well-adapted to this localized and self-limiting pathway, Seviour added: it's rich in metals that promote free-radical chemistry, packed with membranes where radicals can accumulate, and contains many "redox-active" amino acids that can absorb free radicals to form crosslinks. The physical barrier of the skull also likely plays a part, restricting the exchange of fluid and oxygen compared with the rest of the body, the researchers said.

Richard Evershed, an organic geochemist at the University of Bristol who was not part of the study, was impressed by the team's comprehensive analysis. Evershed believes it would be fascinating to expand this to other proteins found in the archaeological record.

"Comparing more tissues — other organs and muscles — would be really useful to get an idea whether what was happening in the brain was special compared to what was happening elsewhere, and also to resolve questions regarding proteins preserved in other environments in archaeology such as pots or dental calculus," Evershed told Live Science.

But the implications of the work extend beyond archaeology. "For medicine, the more unexpected finding is that the molecular fingerprint of these decay-resistant peptides closely resembles the fingerprint seen in neurodegenerative diseases like Alzheimer's," Seviour said. One interesting future direction will therefore be to explore how far this similarity extends and whether preserved brains could ultimately help scientists understand the progression of these devastating diseases.

See how much you know about the most complex organ in the human body with our brain quiz!

Scientists have confirmed that a flowering plant native to the mountains in southwest China is carnivorous, supporting a prediction made by Charles Darwin more than 150 years ago.

The species, Saxifraga candelabrum, grows at elevations above 8,200 feet (2,500 meters) in the Hengduan Mountains, which connect the southeast portions of the Tibetan Plateau to the Yunnan-Guizhou Plateau.

The plant has stems and branches covered in sticky hairs that can trap small insects, predominantly nonbiting midges. However, scientists were unsure if these insects were being ingested by the plant. In a new study, researchers showed that S. candelabrum can digest and absorb nutrients from insects after capturing them, proving that the plant is carnivorous. The scientists published their findings Tuesday (Aug. 4) in the journal Nature Communications.

This is the first demonstrated case of carnivory in the saxifrage plant group, said study co-author Douglas Soltis, a distinguished professor of biology at the Florida Museum of Natural History.

Other carnivorous plants typically grow in moist, boggy soils, but S. candelabrum is found in dry alpine areas, Soltis told Live Science in an email. "These are all nitrate poor soils — that's why this carnivorous habit has evolved a number of times" to supplement the plants in vital nutrients, he said.

In 1875, Darwin theorized that two species closely related to S. candelabrum that also have sticky hairs — S. rotundifolia and S. umbrosa — may be carnivorous, based on their ability to catch insects. But the 19th-century naturalist couldn't show that the plants digested their prey or reused the nutrients in insect tissues — two conditions that are key to confirming carnivory in plants. Without these conditions, a species is considered simply "protocarnivorous," meaning it catches and kills insects or other small animals but doesn't digest or absorb them, according to the study.

"Although untested at the time, Darwin’s hypothesis provided an important inspiration for our study," study co-author Hang Sun, a researcher in the Chinese Academy of Sciences' Kunming Institute of Botany, told Live Science in an email.

The researchers conducted field observations and herbarium surveys of S. candelabrum, which revealed that mature plants with more numerous and longer branches had an average of 71 trapped insects on them. In the herbarium surveys, the team found that 43 out of 45 specimens had caught insects, suggesting that insect-trapping is a widespread phenomenon in this species.

Next, the study's authors showed that S. candelabrum possesses phosphatase, a digestive enzyme commonly found in carnivorous plants. They did this by labeling the phosphatase enzymes with fluorescent molecules to visualize them under a specialized microscope, a technique known as fluorescence tagging.

To determine if S. candelabrum digests and absorbs nutrients from insects, the researchers labeled fruit flies with a stable form of nitrogen before feeding them to the plants. This led to a marked rise in stable nitrogen in S. candelabrum and in a different, known carnivorous species, which the team used as a control group. By contrast, a non-carnivorous plant that formed a second control group did not show an increase in stable nitrogen, indicating that S. candelabrum is carnivorous.

Finally, the researchers performed a genetic analysis, which revealed that S. candelabrum has genes in common with known carnivorous plants that are linked to prey attraction, digestion and nutrient absorption. Together, the results showed that S. candelabrum evolved carnivorous traits to cope with its nutrient-poor environment, adapting its hairs — which were initially used for herbivore defense — into insect traps, according to the study.

Larger insects, which S. candelabrum requires for pollination, rarely get stuck to the hairs, the researchers noted in the study, suggesting that the species has perfectly balanced its needs through evolution.

Other Saxifraga species and plants belonging to the same lineage could turn out to be carnivorous, too.

"Many members of the Saxifragaceae, which includes genera other than Saxifraga, have sticky glandular hairs and are often covered with insects," Soltis said. "I would not be surprised if other members of the family are also carnivorous — as Darwin predicted."

The study broadens the scope of carnivorous plant research, Sun said. "Carnivory may therefore be far more widespread among flowering plants than previously recognized," he said.

Charles Darwin quiz: Test your knowledge on the 'father of evolution'

An abandoned part of a SpaceX Falcon 9 rocket is projected to crash into the moon at 2:35 a.m. EDT on Aug. 5 — and two new studies suggest the event may be visible in telescopes from parts of North and South America, providing both amateur and professional astronomers with a rare, real-time viewing opportunity. Both studies are available as preprints on the arXiv server.

The impending Aug. 5 impactor is the truck-sized spent upper stage of a Falcon 9 rocket. In 2005, the rocket boosted two privately owned landers into orbit around the moon, before leaving its upper stage in an elliptical orbit around Earth, according to OrbitalRadar.com.

A report earlier this year estimated that the collision would occur near the moon's Einstein crater, with the rocket grinding into the lunar surface at a speed of 5,436 mph (8,748 km/h). Although that sounds fast, it's about six times slower than a natural impactor, like an asteroid, would hit.

What can you see with a telescope?

The initial impact flash of the collision — which will last less than a second and be hidden on the sunlit side of the moon — will likely be invisible to casual skywatchers, according to one of the new studies. The brightest estimates for the impact put it at 20 times dimmer than Saturn. The resulting crater likely won't be visible from Earth, as the study estimates that the hole is relatively small and shallow ‪—‬ about 90 feet (27 meters) wide and up to 16 feet (5 m) deep.

More promising for Earthbound skywatchers is the plume of regolith (and potentially water vapor) the impact will loft. The plume will likely reach several miles in height, with computer-based simulations from the second study showing it may tower up to 31 miles (50 km) high. This will make it visible over the moon's limb as a cloud, with the debris spreading up to 112 miles (180 km) from the impact site.

The plume will hang above the lunar surface much longer than the flash ‪—‬ for up to 400 seconds, or close to seven minutes; during this time, it will scatter sunlight toward Earth. Even then, the plume will be too faint to be observed with the naked eye, William Jo, a graduate research assistant at the University of Texas at Austin and co-author of the second study, told Live Science in an email. Viewers will need a good backyard telescope to see it.

"Where the science is"

Although the event will be dim and occur on the sunlit portion of the moon, skywatchers are gearing up to watch it. Benjamin Fernando, a postdoctoral researcher at Los Alamos National Laboratory and co-author of the first study, told Live Science in an email that there "will be an observing campaign involving professional and amateur astronomers from around the world."

In particular, he said, folks in South America and continental North America — where it will be night, with the moon high above the horizon — will have the best chance of seeing it, although you will need at least a 4-inch (10 centimeters) telescope.

However, Jo was less optimistic. "I don't think it would be an easy task for an amateur astronomer," he said, but if they know exactly where to point their telescope and tackle atmospheric refraction, they might see the plume. Nonetheless, he urged well-equipped observers to try observing the plume, as that is "where the science is."

This science, Jo said, would help researchers understand how everything delivered to or disposed of on the moon will ultimately affect the lunar surface. "This would be useful for studying disposal methods for upper stages, maybe how far ejecta will travel, and whether or not the ejecta will hit sensitive instruments, or in the far future lunar bases," he added.

Previous collisions of human-made objects on the moon have likewise led to some major scientific insights. For example, the 2009 crash of a Centaur rocket's upper stage was analyzed by NASA's Lunar Crater Observation and Sensing Satellite mission, which revealed subsurface ice near the lunar south pole. As a result, the lunar south pole is now considered the most coveted location for moon missions that aim to establish a permanent human presence on Earth's satellite.

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

Editor's note: This is a developing story and may be updated.

Michigan has reported two deaths in its ongoing Cyclospora outbreak, a wave of parasitic infections that has affected over 11,000 people in the state.

Since early May, 193 people in Michigan have been hospitalized with cases of Cyclospora cayetanensis infection, called cyclosporiasis. The parasite can enter the body when someone consumes food or water contaminated with the organism, and the cases in Michigan have been linked to iceberg lettuce sourced from central Mexico.

These two deaths are the first reported in the Michigan outbreak, as well as the first deaths documented in any of the ongoing Cyclospora outbreaks in the United States.

Multiple outbreaks have been detected in the country in recent months, but not all have been linked to a specific source of exposure, such as lettuce. Since May, the Centers for Disease Control and Prevention has confirmed over 6,700 cases of cyclosporiasis acquired within the U.S. (In some states, case counts are typical of what's usually seen this time of year, while in others, case counts are higher than normal.)

Regarding the deaths in Michigan, "according to medical records, both individuals had significant underlying health conditions that may have been impacted by cyclosporiasis and dehydration," the state's Department of Health and Human Services (HHS) said in a statement. "No additional information will be provided on these two cases."

Cases of cyclosporiasis range from mild to severe, with severe cases being more likely in young children, older adults, and people with weakened immune systems. Symptoms include loss of appetite, fatigue, low-grade fever, vomiting and diarrhea. The infection is treated with antibiotics, which block the parasite's ability to multiply.

In mild cases, the infection can sometimes resolve on its own, but without treatment, the symptoms can linger for over a month. Severe and prolonged infections can raise the risk of dehydration due to vomiting and diarrhea. Severe dehydration can then cause various complications, such as electrolyte imbalances and hypovolemia (severe fluid loss).

While these complications can be dangerous — causing kidney failure or shock, for instance — cyclosporiasis is not usually life-threatening. For instance, over 2,200 cases were reported in the U.S. between 2011 and 2015, but there were no associated deaths.

"Death resulting from cyclosporiasis is uncommon in the United States," Michigan HHS representatives noted in the statement.

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

At the end of a glacier deep in East Antarctica's Taylor Valley, there is a haunting waterfall that oozes red brine like a bleeding wound in the ice. Scientists explained the brine's gory hue several years ago, finding that it is exceptionally rich in iron. And now, they may have identified the salty water's origin.

Microbes in the crimson waterfall, called Blood Falls, suggest the brine is composed of ancient seawater that was trapped in a pool beneath the glacier when ocean levels fell and the glacier advanced. However, it's unclear exactly when that happened, researchers noted. Previous studies had already proposed a seawater origin for the brine, based on various chemical signatures and bacteria detected in the liquid, but the new results add molecular and genetic evidence to the mix of clues.

"Findings in this study reveal a dominance of marine eukaryotic lineages in the Blood Falls area" compared with the broader region, known as the McMurdo Dry Valleys, the authors wrote in the study, published Monday (Aug. 3) in the journal Nature Geoscience. "This marine signal is less prominent but still detectable in the prokaryotic structure," the researchers added.

Eukaryotes' cells contain a membrane-bound nucleus and other closed internal compartments. Prokaryotes, by contrast, are single-celled organisms whose DNA floats around freely in the cell, unbounded by a membrane.

To characterize the types of microorganisms present within Blood Falls, the researchers used a suite of genetic techniques to analyze 167 samples of water, sediment and air from around the falls and the broader McMurdo Dry Valleys.

Some researchers argue that Blood Falls' water does not originate from seawater, and suggest the marine bacteria and chemical signatures that point to seawater may have instead reached the falls from the ocean via intense winds, which are common in the McMurdo Dry Valleys. By analyzing samples from various sites in the Dry Valleys, the team behind the new study compared microorganisms from the wider region with those at Blood Falls to determine if Blood Falls has a distinct microbial assemblage potentially left over from ancient conditions.

The researchers found that the crimson brine and associated red-tinted sediments at Blood Falls shared a higher proportion of eukaryotes with nearby oceanic samples than other sites in the Dry Valleys did. Whereas Blood Falls had a little over 9% of its eukaryotes in common with the ocean, the Dry Valleys showed only about 1% similarity, according to the study. The remaining eukaryotes and most of the prokaryotes identified in the paper had freshwater and terrestrial origins.

The results also showed that the air near Blood Falls contained only a tiny proportion of marine microorganisms, suggesting that present-day winds can't fully explain the microbial composition of Blood Falls, the researchers wrote.

Therefore, an ancient seawater origin is the most likely explanation for the microorganisms found at Blood Falls today, the team concluded. Winds may have played a role in shaping the community in the past, but now, their influence is probably insignificant, the team added.

The brine that feeds Blood Falls may have become entrapped more than 1 million years ago, during a warm period with higher sea levels and less ice cover than there is now, previous estimates suggested. However, further work, including more comprehensive genetic profiling and mapping of microorganisms, is needed to pinpoint when Taylor Valley's glacier grew to cover the brine, the researchers wrote.

Antarctica quiz: Test your knowledge on Earth's frozen continent

A poop transplant — otherwise known as a fecal microbiota transplant (FMT) — may help adults with long-term insomnia sleep better, a small study suggests.

After the transplant, study participants' gut bacteria became more diverse than an untreated group of people with insomnia. Their sleep efficiency, meaning the percentage of time they spent asleep while in bed, also increased, researchers reported July 22 in the Journal of Internal Medicine.

If future studies confirm that FMT is safe and effective for the treatment of insomnia, it could become another tool against the sleep disorder, joining sleeping pills and cognitive behavioral therapy (CBT).

The findings "are aligned with a recent body of work over the last five years indicating that the gut microbiome may play a role in sleep-wake regulation," said Dr. David Gozal, a pediatric sleep specialist at Marshall University in West Virginia who wasn't involved in this study.

However, "these results should be regarded as promising proof-of-concept evidence rather than confirmation that FMT is ready for routine treatment of insomnia," Kenji Hashimoto, a forensic mental health researcher at Chiba University in China who wasn't involved with the study, told Live Science in an email.

Improving sleep with "poop pills"

The study included 80 adult women and men with chronic insomnia from seven hospitals in China; the participants did not have other health problems, such as migraine or obstructive sleep apnea, that could interfere with the results.

Half of the participants took antibiotics for two days to clear out some of their existing gut bacteria. Then, they swallowed 60 FMT capsules chockfull of gut bacteria from healthy donors who had been confirmed to be good sleepers. These bacteria were isolated from fecal samples from the donors. Two weeks later, this group took a booster dose of 20 capsules.

The other half of the participants instead took placebo pills in place of the antibiotics and FMT capsules.

The researchers used an overnight sleep assessment called a polysomnography, which records brain waves, eye movements, heart rate, oxygen levels and breathing patterns, to assess the participants. The results showed that sleep efficiency in the FMT group jumped from 79% before the transplant to 93% one month after treatment, on average. The placebo group's sleep efficiency barely changed, shifting from about 85% to 87%.

Additionally, the treated group woke up less throughout the night. Their time spent awake after initially falling asleep fell from 79 to 17 minutes, while the same metric increased from 37 to 42 minutes in the placebo group.

On questionnaires, the FMT group continued reporting better sleep from two all the way to six months after treatment.

It is "encouraging" that FMT treatment seemed to improve sleep not only on objective tests, but also in how the participants themselves rated their insomnia, added Harriët Schellekens, a neuroscientist and microbiome researcher at University College Cork in Ireland, who wasn't involved in the work.

Gut-sleep connection

The results also suggest that the treatment is safe. In the FMT group, only three out of 40 participants had side effects, and they were mild, such as nausea and transient fever.

However, experts noted several caveats. The trial was small and limited to relatively healthy adults in China, so the results may not apply broadly. Sleep was measured only once after treatment, at the one‑month mark, Hashimoto said. And because the treatment combined antibiotics with FMT, it's unclear how much of the benefit came from the donor microbes alone, Schellekens and Hashimoto noted.

Hashimoto added that the study focused exclusively on the gut microbiota. "Microbial communities in other body sites, particularly the oral and nasal cavities, may also influence sleep regulation through immune, metabolic, and neural pathways and through oral-gut-brain or nasal-gut-brain communication," he said.

The gut and brain communicate in various ways, including via chemicals made by gut microbes that travel to the brain via the bloodstream, Hashimoto explained. These chemicals may steer inflammation, stress responses and the body's sleep-wake control.

Shifts in certain microbes can alter these gut chemicals and gut barrier function in ways that ripple out to the brain and change sleep patterns, Gozal said. Conversely, disrupted sleep can reshape the microbiome. "The question is, what came first?" he said — a disordered microbiome driving insomnia, or insomnia reshaping the microbiome and worsening symptoms.

In the study, the mix of gut microbes in the FMT group shifted between the start and end of the study, but the placebo group's microbiomes stayed the same. Several types of bacteria became more abundant after FMT, while others decreased, suggesting that FMT reshapes the gut microbiome.

Not everyone responded to the treatment, and they mostly differed in what their gut microbiota looked like before FMT, not after. That suggests that a person's initial microbial makeup may help determine how well they respond to the treatment.

Gozal said he would have liked the study to measure the chemicals made by gut microbes before treatment and then show how those same chemicals changed after FMT.

More research is needed to understand the biological mechanisms underlying the improvements, Schellekens said. For now, "FMT remains an experimental approach for insomnia and is not something that should be used outside carefully controlled clinical studies."

The study's researchers did not respond to a request for comment by the time of publication.

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

How much do you know about sleep and dreams? Find out with our sleep quiz!

Ancient slingstones found in northeastern Spain may be evidence of a local uprising against Roman rule in the first century B.C.

Archaeologists think the lead sling "bullets" were fired by Roman soldiers after an ambush orchestrated by the local Indigenous Ceretani (also spelled Cerretani) people, who by this time had spent almost 200 years resisting Roman expansion in Iberia.

The findings, which were unearthed during an archaeological survey of the area, reinforce that "the Roman conquest of the Iberian Peninsula was neither a brief nor a peaceful process," researchers explained in a statement from the Autonomous University of Barcelona.

The ancient Roman historian Cassius Dio (who lived from around A.D. 150 to 235) wrote that the Ceretani revolt took place in 39 B.C., but it was generally thought to have occurred farther west. The new finds, however, pinpoint an ancient Roman military camp in what's now Cerdanya, a region of the eastern Pyrenees on the Spanish side of the modern border with France. At the time, this location was in Ceretani territory.

Roman expansion

The archaeological team found the sling bullets last year among the remains of the camp at Collet de Jovell, an alpine pass in the region. The bullets were poured from lead (it was easier than collecting stones), and two were emblazoned with the letters CND, which stood for the Roman governor of the province of Hispania at that time, Gnaeus Domitius Calvinus. These letters help date the ambush to exactly 39 B.C., when he was in office.

The archaeologists also unearthed the distinctive iron studs that Roman legionaries wore on their sandals, called clavi caligae; Roman fibulae, or brooches for fastening clothing; and several Roman coins that reinforced the team's dating of the site.

The Romans started expanding in Iberia, known to them as Hispania, after first landing on the Mediterranean coast in 218 B.C., during the Second Punic War with Carthage. But they were opposed by the Ceretani and other Indigenous peoples.

The two sides battled for centuries. But the Ceretani revolt in 39 B.C. failed to oust the invaders and was followed by severe Roman repression of the local people, according to the statement.

The Romans suffered, too ‪—‬ the governor ordered that some of his troops be punished for running away when the Ceretani ambushed the camp.

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

Aspen trees could provide a natural buffer against wildfires, as new research shows that areas of forest where these trees dominate burn less intensely than those made of conifers.

The findings suggest that planting more of the right kinds of trees, such as trembling aspen (Populus tremuloides, also known as quaking aspen), could be an effective strategy for protecting communities as devastating wildfires become more common and intense in a warming world, researchers reported June 15 in the journal Forest Ecology and Management.

Individual aspen trees burn easily because of their thin bark, but large "stands" ‪—‬ contiguous communities of trees that are uniform in species, age and structure ‪—‬ of them are more resistant to fire than stands of conifers and can act like a firebreak.

The reasons for aspen stands' resilience are not certain. However, researchers think it likely stems from a combination of factors, including the high moisture content in the aspens' leaves and the undergrowth, the trees' lack of highly flammable resin, and the leaves' height, which makes it harder for fire to spread to the canopy and leap from tree to tree.

Flavie Pelletier, who conducted the research as part of her doctorate at McGill University in Montreal, wanted to see whether aspen stands have been able to maintain their fire-resistant properties as climate change makes fire seasons more intense and destructive.

She combined new maps of dominant tree species in forests across Canada with satellite maps of wildfires from three recent years, including 2023, which was the country's most destructive wildfire season ever recorded. She noted which tree species tended to be inside the fire zone and which were more common at the edges. She found that aspen trees were more than twice as common at the perimeters of fires than inside them, while conifers like spruce and pine were equally present in both locations.

Having more aspen trees in a particular area also decreased the amount of forest that burned each day during a fire, so it also appears to help slow the spread of the fire. Notably, the trees still resisted fire spread even in the spring, before their leaves had fully sprouted.

"This is proof that aspen has an impact on fire perimeter formation and can slow fire progression," she told Live Science.

Anthony Taylor, a forest management specialist at the University of New Brunswick, said the study, with its use of large datasets on real fires, does a good job of analyzing and quantifying a phenomenon that Indigenous peoples and foresters have understood for a long time.

"The idea that deciduous trees burn less has been known for millennia, but knowing something through experience is different than testing it," he told Live Science.

Changing practices

The research supports the idea that planting aspen or other deciduous trees around vulnerable communities can help protect them from fires. Taylor said this buffer strategy is being considered or implemented in many areas.

A single line of trees will not do the trick. The stands must be deep enough to stop the flames from blowing over the top — probably 300 to 1,000 feet (100 to 300 meters), Taylor said.

Aspens can also play a role in fire control at larger scales. Pelletier first became interested in this topic when she learned that forestry companies often spray the forests they manage with the herbicide glyphosate to kill deciduous trees like aspen so they can grow monocultures of more economically valuable conifers, leaving those forests at much higher risk of fires. She hopes her work will help convince the companies and regulators to change their practices.

"There needs to be less of a war on aspen in commercial forests," she said. In the long term, it would actually benefit the companies, because it would reduce the risk of losing large numbers of trees to fire, even if it slightly reduces the value of the forest in the short term.

Taylor agrees that in places like New Brunswick, a province with a large forestry sector, officials should be promoting more mixed and hardwood forests, and less of the softwood monocultures that the forestry industry relies on.

"That would go a long way to making our landscape more resilient to wildfire," he said. "And that's what would have been here anyway, before we started converting the forests to a more industrial forest."

LONDON — In the packed halls of the recent Alzheimer's Association International Conference in mid-July, over 10,000 experts in brain research discussed strategies to beat dementia. But in one room, attendees gathered to watch a video from a nonscientist named Isabel Beltre, whose life was transformed by a recent trial.

Beltre was one of 1,200 participants ages 60 to 77 who took part in the Latin American Initiative for Lifestyle Intervention to Prevent Cognitive Decline (LatAm-FINGERS), the first trial to test a culturally adapted lifestyle intervention to prevent cognitive decline in Latin America. Rather than attempting to treat dementia after it has developed, the trial tackled risk factors that raise the likelihood of the condition, like smoking and a sedentary lifestyle.

In her native Spanish, Beltre thanked both God and the project for its impact on her life. There was a celebratory air in the conference room as the trial's results were released. The lifestyle interventions, which included exercise programs and brain training, had statistically improved participants' thinking skills, compared with a control group who received only bare-bones support, like general health advice.

Trials like LatAm-FINGERS — including a related U.S.-based trial called the POINTER study — ultimately aim to cut rates of dementia around the world. The LatAm trial is the most successful of these trials to date, raising hopes that this approach could help to prevent dementia en masse.

Whether that promise pans out remains to be seen, though, experts told Live Science.

The lifestyle factors that increase dementia risk

When it comes to dementia prevention, few guidelines are as influential as those written by the Lancet Commission, an expert-led review of the available evidence on dementia. Three editions of this review have provided comprehensive overviews of risk factors; the most recent, published in 2024, identified 14 factors, including smoking, infrequent social contact, and a lack of physical activity.

The commission estimated that, together, the identified risk factors contribute to 45% of dementia cases at a population level.

Long before the 2024 report, Dr. Miia Kivipelto, a professor of clinical geriatrics at the Karolinska Institute in Sweden, wanted to tackle these risk factors at the individual and population level in her work as a medical doctor and epidemiologist.

"I felt that I wanted to move on to interventions to really show that if you do something, you can change the risk," Kivipelto told Live Science.

The many contributing factors that lead to cognitive decline, and ultimately dementia, couldn't be tackled in isolation, Kivipelto realized. She designed a trial in her native Finland, called the Finnish Geriatric Intervention Study to Prevent Cognitive Impairment and Disability (FINGER) study, that would aim to tackle many risks simultaneously.

The two-year project recruited 1,260 participants ages 60 to 77 and divided them into two groups. The first group received general health advice, such as tips on healthy eating and exercise, at the start of the study and then again after six and 12 months.

The other group additionally received a multipart intervention consisting of meetings with nutritionists to discuss personalized meal plans, brain training, exercise programs, social activities, and metabolic and vascular tests. These programs lasted throughout the study period, with the brain training alone including 144 sessions over 12 months of the study.

At the end, the two groups' cognitive skills, such as thinking speed and memory, were tested; the trial did not track dementia rates, only overall cognition. In both groups, these skills improved by the end of the study. But the headline finding was that in the group given the comprehensive intervention, overall brain function was judged to be 25% stronger than in the control group.

What did that difference mean in concrete terms? It turns out, the improvement was relatively small.

It was calculated in terms of a statistical measure called a z-score, which represented the extent of the improvement in brain-function test scores in each group. In the end, the difference in z-scores between the two groups was just 0.04 points, which a 2021 review defined as "small."

However, Kivipelto maintained that the improvement is significant. "It's as big as anti-amyloid treatments," she said.

Several drugs approved by the U.S Food and Drug Administration for the treatment of Alzheimer's disease target amyloid, a protein that forms unruly tangles in the brain. These drugs have been reported to marginally slow the disease's progression, but statistically, their overall effect is small.

Targeting those most at risk of dementia

Despite criticism of the trial's moderate effects, Kivipelto's FINGER intervention has since been repeated all over the world, including by the U.S.-based POINTER study, and, most recently, LatAm-FINGERS.

Dr. Gill Livingston, a psychiatrist at University College London who led the 2024 Lancet Commission report, told Live Science that the data from these trials shows that dementia interventions need to be tailored to the risks the participants actually face.

In the POINTER study, 70% of the participants had a college degree, compared with roughly 43% of the wider U.S. population. "People who are usually in randomized controlled trials are usually highly educated people who are very interested in health," Livingston noted. "And that means they're at less risk of developing dementia, and therefore, less can be done to help them" through lifestyle interventions.

The difference between the test group and the control group in the POINTER study was even smaller than in the original FINGER trial — just 0.029 points.

LatAm-FINGERS tried to maximize flexibility in its approach by better tailoring its interventions to its study participants, said study first author Dr. Lucía Crivelli, a neuropsychologist at the neurology center FLENI in Argentina. Dietary advice reflected the produce available in each region. Exercise programs considered local environmental factors; for example, sessions were held outside, avoiding hot gyms during the sweltering summers in Ecuador and Mexico.

The trial recruited volunteers across Argentina, Brazil, Bolivia, Chile, Colombia, Costa Rica, Ecuador, Mexico, Peru, Puerto Rico, the Dominican Republic and Uruguay. The participants were less highly educated than the POINTER cohort had been; 37% had no education beyond a high school diploma, compared to just 5% in the POINTER study. That likely made the study participants more representative of people who might benefit from the trial's interventions.

When Crivelli announced the results of the trial at the conference, a large cheer filled the room. The intervention had achieved a difference of 0.11 points between the test and control groups' z-scores — more than twice the difference seen in the FINGER trial.

That difference corresponded to a relative 55% improvement in overall brain function in the test group compared to the control group at the end of the study.

What made the difference?

Crivelli, Kivipelto and Livingston all pointed to one key factor in explaining the project's relative success. "In Latin America, there are more modifiable risk factors," Kivipelto summarized.

The study participants had lower academic attainment and higher cardiometabolic risk factors, such as high BMI, than the participants in previous studies. The trial had reaped the rewards of delivering the intervention to people who needed it most, experts concluded.

But the approach wasn't perfect. said Dr. Claudia Suemoto, a neuroscientist at the University of São Paulo who presented a detailed breakdown of the trial's results. They found that the intervention didn't improve men's overall cognitive ability, compared with the control group. Only women benefited.

The difference may be that men simply didn't engage in the trial as much as women did, Suemoto's data suggested. Livingston pointed to the trials' exercise classes as an example of an activity that men may not be as likely to participate in, although that's an assumption rather than being based on the trial data.

Can we really prevent dementia?

The LatAm-FINGERS results show that addressing the dementia risk factors that people face is the most effective way to prevent dementia, Livingston said.

And Livingston is leaning into the idea. She's planning a dementia prevention trial in the U.K. that will ask participants about their risk factors and then give them tailored interventions based on the risks they can realistically avoid.

"We ask them to choose which ones they want," Livingston said. "If somebody doesn't want to stop drinking or smoking, then they're not going to."

While LatAm-FINGERS has been the most successful of the FINGER trials to date, it's still unclear whether such projects actually reduce dementia rates.

Only two previous prevention trials have attempted to measure dementia incidence, and neither saw a notable change in their test group. That said, neither trial included cognitive training interventions like FINGER did; they instead focused on cardiovascular risk factors, such as low exercise rates and high body weight.

Measuring changes in dementia rates requires trials much longer than two years, and they also need massive recruitment. Implementing an intensive study like LatAM-FINGERS in the wider community "is not practical," Crivelli said. Instead, she said the study's interventions would need to be distilled into their essential parts so that they could be implemented at scale.

Kivipelto is optimistic that advances in Alzheimer's screening, including new blood-based tests, could provide an early biological measure to show that FINGERS-style interventions can help stave off dementia. This would be an indirect measure but wouldn't require as long a trial as tracking dementia rates.

Some of the risk factors the Lancet Commission identified, like air pollution, can't be modified at an individual level, Livingston noted. A combination of personal and governmental change could address this, she said, as it has in the realm of infectious-disease prevention.

While the scientific field still has uncertainty about the scale of change that trials like FINGERS can bring about, Beltre has little doubt about the trial's impact.

While she previously relied on help from family members like her grandson to complete everyday activities, she said, "I do everything myself now."

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

See how much you know about the most complex organ in the human body with our brain quiz!

Skywatchers across North America and Europe should mark Wednesday, Aug. 12 on their calendars. From a daytime solar eclipse to the peak of the Perseid meteor shower beneath a moonless sky, the date offers an exceptionally rare combination of celestial events within a 24-hour period. Add brilliant Venus and the glowing band of the Milky Way after sunset, and the result is a full day of astronomy that could become one of the standout skywatching opportunities of the year.

The first spectacle arrives during daylight as the moon partially covers the sun across Alaska, eastern Canada and parts of the northeastern U.S. A dramatic total solar eclipse will be visible along a narrow path stretching across eastern Greenland, western Iceland and northern Spain — and that's where eclipse chasers will be. However, about 779 million people in North America, Europe and North Africa will see at least a 10% partial eclipse, according to Time and Date.

Northern Canada will experience North America's deepest partial eclipse, with parts of Nunavut in the Canadian Arctic seeing up to 93% of the sun covered, according to Time And Date; large eastern cities like Toronto, Ottawa and Quebec will see between 8% and 24% coverage. The best views in the U.S. will be from Alaska and the Northeast, with Fairbanks, Alaska, seeing 37% of the sun covered, and Boston seeing 16%.

In Europe, London will see a 91% eclipse and Paris will get 92%. No matter your viewing location, it's important to use ISO 12312-2 certified solar eclipse glasses throughout the entire partial eclipse. Also remember to fit binoculars, telescopes and cameras with solar filters before pointing them at the sun. (Here’s a great selection of gear that will help you safely watch the eclipse from anywhere).

After sunset, the day's second major event begins. Brilliant Venus will be easy to spot as it reaches dichotomy, the point at which the planet appears half illuminated. Through a small telescope or large stargazing binoculars, skywatchers should see Venus resembling a tiny half-moon as it moves closer to Earth.

Once darkness falls, the day's third and fourth major events will begin. The annual Perseid meteor shower will peak during the overnight hours of Aug. 12-13, and this year's display benefits from one crucial advantage: a new moon. With no moonlight washing out faint meteors, observers under truly dark skies could see between 50 and 75 meteors per hour, while even suburban locations should enjoy frequent "shooting stars," according to The Planetary Society.

The best time to look is from midnight to 2 a.m. local time, when the sky is darkest and the constellation Perseus is highest in the sky. As a final bonus, those under dark, rural skies will see the Milky Way arch overhead, providing one of the finest views of our home galaxy all year.

A daytime solar eclipse, a moon-free Perseid meteor shower, a dazzling Venus and spectacular views of the Milky Way make Aug. 12 a great opportunity for anyone with an interest in the night sky. If skies are clear, it could be the single greatest day and night for skywatching in years.

See how much you know about the sun with our sun quiz!

Happy Shark Week, science fans! To mark the occasion, we had a flurry of fishy features this week, including a first look at the secret lives of whale sharks, as seen from cameras on the animals' fins, and the discovery of a "demon cavefish" beneath a World War II chemical weapons facility in Alabama.

This week, we also saw the first drone footage of the birth of a humpback whale.

Meanwhile, off the coast of Spain, the orcas are at it again, sinking yet another ship along the Iberian coast. And speaking of boats, as cargo ships continue to stall near the Strait of Hormuz, scientists have warned of an imminent biological "superspreader" event once the key shipping route reopens.

We also have an update of our own: Live Science has launched Live Science Pro, a paid membership that gives you access to our exclusive features, analyses, interviews, book excerpts and opinion pieces, all without ads And to celebrate, we're offering an introductory price of only $3 for the first three months! You can subscribe here.

Earth registers coldest temperature

Antarctica just experienced minus 119 F, Earth's coldest temperature since 2012 — here's why

While the Northern Hemisphere battled heat waves and wildfires, Antarctica just experienced the lowest temperature recorded on Earth in over a decade. High-altitude research station Concordia, located in the icy continent's interior, logged a low of minus 119.4 degrees Fahrenheit (minus 84.1 degrees Celsius) on July 18, just shy of the coldest temperature ever recorded at the station.

"Even here, where extreme cold is expected, temperatures below minus 84 C are remarkable and highlight how variable Antarctic weather can still be," Gabriele Carugati, the station leader at Concordia for Italy's National Antarctic Research Program, told Live Science from the station.

Discover more planet Earth news

—Magnitude 6.8 earthquake traps shoppers as mall collapses in Japan —‬ here's why the seismic event was unusual

—Colossal scars of 60 million-year-long continental collision streak across warped mountains in Pakistan — Earth from space

—Mice on 'godforsaken' frozen volcanoes eat toxic plants to survive conditions 'not remotely compatible with long-term human survival'

Life's Little Mysteries

Why do cats have 'leg whiskers'?

Cats are known for having whiskers on their faces. But if you look closely, you'll see they also have them on their legs. So what are these leg whiskers for? And how do they differ from the ones on their face?

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

Geoglyphs from lost Amazonian civilization

Lasers reveal hundreds of geoglyphs made by a mysterious civilization in the Amazon rainforest thousands of years ago

A significant portion of the Amazon rainforest remains unexplored, and even from above, it's almost impossible to see through the trees' thick canopies to find out what lies beneath. However, thanks to modern laser scanning technology, scientists have peered through this wall of leaves ‪—‬ and what they've found may offer new insight into lost human civilizations.

A new lidar survey has revealed hundreds of earthworks made by the Aquiry people, who arose 2,500 years ago in Brazil. So what can these structures teach us about this mysterious lost civilization?

Discover more archaeology news

—Relief fragment with vanquished enemies: A 3,400-year-old depiction of an Egyptian pharaoh crushing western Asian soldiers under his royal chariot

—Ancient human relative cannibalized both adults and children in a cave in Spain 850,000 years ago, fossils reveal

—Archaeologists find 2,800-year-old burial of person clutching sea turtle vessel in El Salvador

Also in science news this week

—A unique antibody system may help explain bats' unusual tolerance of viruses

—Scientists may have found a clue to prevent muscles from aging, study hints

—'Feynman and followers, you guys are off': Physicists disprove decades-old Richard Feynman theory on 'silly' sprinklers

—A strange string of a dozen galaxies keeps surprising astronomers with its missing dark matter

—Scientists discover 2 new 'ghost' lineages that contributed DNA to modern humans

Science Spotlight

Inflammation may trigger persistent 'out-of-body' experiences, emerging research hints

We're increasingly learning about the role of chronic inflammation in a range of diseases, from autoimmune conditions like rheumatoid arthritis to neurodegenerative diseases like Alzheimer's. However, scientists may have now added a new surprising side effect to this immune response: "out-of-body" experiences.

It's been known for a while that trauma can trigger altered states of consciousness, but exactly what was causing this psychiatric response was unclear. Now, scientists have found that stress triggered by trauma may dial up chronic inflammation, which could, in turn, trigger these dissociative disorders.

Something for the weekend

If you're looking for things to keep you busy over the weekend, here's a selection from our best interviews, explainers, skywatching guides and crosswords that we published this week.

—America's gun violence epidemic, through the eyes of a Chicago trauma surgeon [Interview]

—'World models' are the future of AI, but how do they work? [Explainer]

—Which solar eclipse viewing method is right for you? [Skywatching]

—Live Science crossword puzzle #54: Egyptian pharaoh who died at 18 — 6 down [Crossword]

Science in motion

Chinese rocket hit by rare midair lightning strike moments after launch as onlookers gasp in horror

It's like something from a movie: Seconds after China's Long March 3B rocket launched on July 23, the spacecraft was struck by lightning. Hundreds of spectators watched in shock as at least 100 million volts of electricity hit the craft and surged around its fuselage and through its exhaust plume, before shooting down to Earth.

Despite the strike, the uncrewed rocket safely reached space and successfully deployed its payload into orbit.

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 private mission to rescue an ailing NASA space telescope may now need a rescue of its own. The LINK spacecraft — designed by private company Katalyst Space to boost the orbit of NASA’s ageing Swift Observatory — is reportedly spinning unexpectedly in the weeks after its launch, so much so that stabilizing the spacecraft will likely delay the telescope rescue.

Katalyst’s LINK spacecraft launched July 3 from a mid-air Northrop Grumman Pegasus XL rocket mounted aboard a modified Lockheed Martin L-1011 airliner. The spacecraft lifted off after less than a year of development, on a mission to catch NASA's nearly 22-year-old Neil Gehrels Swift Observatory before the telescope falls back to Earth.

While teams at NASA and Katalyst are working hard to stabilize the new LINK spacecraft, the next few weeks will be a delicate balance of getting LINK ready before Swift falls back to Earth (which is expected to occur this autumn), while not putting Swift at undue risk.

NASA administrator Jared Isaacman said there’s still time. "We are not giving up yet," he wrote late Thursday (July 30) on X. "This remains a very cool, very low-cost, high-potential, high-reward mission, and another step toward a more autonomous future where missions like this routinely upgrade, repair, service, and boost satellites."

LINK was supposed to rendezvous with Swift about a month after its early-July launch, but now it looks like late August is the earliest possible date, according to the latest update. That’s because the $30-million LINK began spinning in recent days after electrical power issues affected two of the devices that control the spacecraft’s orientation, known as reaction control system (RCS) wheels. Only one of the three RCS is working properly.

As of Thursday (July 30), Katalyst’s mission blog said engineers reduced the rotation with engine fires from the spacecraft, and that work is ongoing to stabilize the spacecraft. LINK is now spinning at four degrees a second, instead of the previous nine.

"Over the last 48 hours, the Katalyst team has worked to reduce LINK’s rotation while assessing current spacecraft functionality and its control system," Katalyst representatives wrote.

All the troubleshooting has delayed LINK’s expected arrival near NASA's Swift Observatory — a legacy telescope designed to detect gamma-ray outbursts — into late August. Time is of the essence, as Swift is expected to fall too far for help by autumn. The observatory has already reduced its science work to stay as streamlined as possible, so that drag doesn’t pull it into the atmosphere this summer.

Swift must stay above a minimum rescue altitude of 185 miles (298 kilometers) for the mission to succeed, agency models suggest. For comparison, the International Space Station typically operates at about 250 miles (400 kilometers) in altitude.

NASA has noted that other systems on LINK are working well. "The spacecraft remains power positive and in communication with the Katalyst team," NASA officials wrote in a Tuesday (July 28) update. Assuming LINK’s attitude stabilizes and the spacecraft is healthy enough, teams "will then evaluate revised plans to approach and capture Swift," NASA stated.

Katalyst’s ultimate goal is to refuel and reboost Swift so that the observatory, worth roughly $450 million today when accounting for inflation, will be able to continue its mission. (The mission cost $250 million in 2004, which is much cheaper than the $10 billion James Webb Space Telescope that launched almost five years ago.)

Swift was initially mainly tasked with looking at gamma-ray bursts, which are huge explosions that happen after a dying and massive star collapses into a black hole. Swift has gathered many observations of these bursts, but it also looks at other stellar changes (like supernovas or X-ray flares) as well as moving objects like comets and asteroids.

Its science remains valuable, a recent NASA statement noted. "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."

If successful, the rescue mission could give Swift many more years — potentially decades — to continue surveying the cosmos, as long as its science instruments continue to function.

Scientists at IBM and partner institutions say they've reached "quantum advantage" in a trio of experiments demonstrating quantum computing capabilities that even the fastest classical supercomputers can't match.

In a purported major milestone for quantum computing, the experiments show how these machines could perform useful computational tasks, such as computing chemical reactions, within minutes. By comparison, a supercomputer would take years.

In a statement, IBM representatives said these experiments show that quantum computers can provide trusted solutions more efficiently, more cheaply or more accurately than any classical computing method.

Trust and verification

At a July 28 news conference, representatives from IBM, Algorithmiq, Qedma, and the University of Chicago described three experiments demonstrating quantum advantage over classical computers in three different challenges.

Each used IBM's Quantum Heron R3 superconducting quantum computer system running novel error mitigation techniques. The experiments focused on both demonstrating and verifying quantum advantage.

The first study, conducted in partnership with Qedma, investigated the Floquet transverse-field Ising model, a system physicists use to study how a material's magnetic properties evolve when rhythmically driven by external pulses. This is an extremely difficult problem for classical computers because the model's math becomes exponentially more difficult to process as the problem scales. Scientists published the study, which has not been peer-reviewed, on the arXiv preprint server July 27.

But quantum computers can perform deeper computations using the Floquet transverse-field Ising model than their classical counterparts due to quirks of quantum mechanics that allow quantum bits (qubits) to represent not just the 1s and 0s of binary data but also a superposition of the two values, so that calculations can run in parallel.

When physicists use a classical supercomputer to run the model ‪—‬ in this case, the Fugaku supercomputer in Kobe, Japan ‪—‬ they have some trust that the results will be computed correctly and without significant error.

Quantum computers, by contrast, are far more prone to error. They're extremely sensitive to any form of noise, including interference from Earth's magnetic field. One of the chief challenges in quantum computing is finding ways to mitigate the errors caused by this noise.

Scientists can compare a classical supercomputer's results with those of a quantum computer using the Floquet transverse-field Ising model, but only to a certain point. When the classical computer reaches the limit of its ability to compute complex problems, the quantum computer still has plenty of runway left.

But, as IBM principal research scientist Abhinav Kandala explained in an interview with Live Science, the problem lies in trusting the results.

"You want to perform computations that outperform classical, right? But you've relied on classical results for the longest time," he said. "So when you now begin to outperform, or you go beyond classical, how do you know you had the right result? This is a question that's independent of application. For any computation that you want to do, you want to [ask], 'OK, is this really something that I can trust?"

The experiment was designed to create a trusted stack that essentially allowed scientists to verify the quantum computer's results. They used Qedma's quantum error suppression and error mitigation (QESEM) software to provide consistent results, and then compared those results against the Fugaku supercomputer's.

Once the results matched, they cranked up the difficulty until the classical computer could not keep up. Then, to replicate the results, they brought in additional quantum computers.

The team ran the same experiment on multiple quantum computers. To ensure they were getting enough errors to test the error mitigation strategy, Kandala said, they purposely injected each system with different levels of artificial noise and corruption.

"We measured the same circuit on five different quantum computers," Kandala told Live Science, including a superconducting quantum computer from IBM Boston and another at IBM Pittsburgh.

They also ran the experiments on two of Quantinuum's quantum computers, using the same error mitigation techniques. In each measurement, the noise and corruption injected into the system was different, but the computational results were consistent.

Quantum building blocks

In the second experiment, conducted by IBM and Algorithmiq, researchers applied the Floquet transverse-field Ising model to a different set of problems and used a different method for error mitigation. As the researchers scaled the problem on both the classical and quantum computers, the classical systems began to produce inconsistent results. The quantum systems, by contrast, maintained consistency at measured intervals, thus demonstrating verifiable outputs, the team reported in a preprint paper posted to arXiv July 28.

The third study, uploaded to arXiv July 28 and conducted in partnership with the University of Chicago, approached quantum advantage from a different angle. Researchers designed a system of "Clifford gates," a type of circuit that is intentionally easy for classical computers to simulate. Then, they made the circuits progressively harder for classical systems to solve by injecting them with more difficult gates called T gates.

The nature of the experiment allowed physicists to guarantee error mitigation at complexities beyond what a classical supercomputer could handle. Any computations run through the circuit ‪—‬ even those that would be impossible for a classical computer ‪—‬ would be trustworthy by design.

Based on these three technical papers and other press information provided by IBM, it appears that each of the experiments demonstrated a clear quantum advantage over classical computers. Whether it will stay that way, however, remains to be seen.

There have been numerous reports of laboratories achieving "quantum supremacy," "quantum utility" and "quantum advantage" over the past few years — each, essentially, claiming to have surpassed the abilities of classical computing. However, most of those achievements ended up being topped. It isn't possible for physicists to imagine every possible mathematical method for conducting classical computations when they test quantum computers against state-of-the-art supercomputers.

IBM and its partners said they expect classical computer scientists to try disproving their claims.

"The classical back-and-forth ‪—‬ that'll keep going on, I think," Kandala said. "And that should; that's how science progresses. And that's precisely [why we have] the Quantum Advantage Tracker, a benchmark for measuring quantum advantage. "A lot of these problems have been on the tracker for a while now," Kandala said, "and I'm sure getting the papers out will get more eyes on it."

LONDON ‪—‬ New blood tests for Alzheimer's disease aim to catch the condition in its earliest stages. Scientists hope that, someday, by spotting very early signs of dementia and enabling earlier treatments, these tests could significantly improve patients' prognoses.

But how well do current blood tests work for that purpose?

At the Alzheimer's Association International Conference in London on July 12-15, Live Science spoke with researchers and clinicians who study and use blood tests for Alzheimer's disease. Here's their take on the current state of these tests and their practicality for real-world use

Scientists' big hopes for the tests

People diagnosed with Alzheimer's disease face an incurable condition, but their outlook is marginally more hopeful than it was 10 years ago. That's because the first "disease-modifying" drugs for Alzheimer's, which target the disease's causes rather than its symptoms, have been approved in recent years.

These drugs, which include the lab-made antibodies lecanemab and donanemab, only slow, rather than stop, the progression of the disease. However, researchers hope these medicines could be the precursors to more effective treatments.

Alzheimer's disease researchers hotly debate the exact causes of the condition, but they are united on the idea that early intervention is likely to produce the best possible outcome for patients. The aim is to remove disease-linked proteins before they can damage the brain.

That's why new blood tests for Alzheimer's disease, some of which have been approved in the past year, are exciting so many scientists. These tests, which measure chemical signals of the disease circulating through the bloodstream, are currently paired with other clinical exams to provide an accurate Alzheimer's diagnosis for patients with early symptoms, such as subtle changes to memory or personality.

The hope is that if these patients could be identified at this stage, they could access clinical trials and treatments when they might be the most helpful.

What do Alzheimer's blood tests measure?

The U.S. Food and Drug Administration (FDA) has approved two blood tests for Alzheimer's disease: Roche's Elecsys pTau181 assay and Fujirebio's Lumipulse G pTau217/ß-Amyloid 1-42 Plasma Ratio test.

An additional test from Roche (the Elecsys pTau217 test) has received a basic safety certification in the European Union and U.K., which allows it to be sold but is not equivalent to FDA approval. This test is not approved in the U.S. yet. A second test from Fujirebio (the Lumipulse G pTau 217 Plasma assay) is in the same boat.

Plus, there are a host of other tests made in specific clinical laboratories; these are not FDA-approved but they are available in certain specialist clinics.

All of these tests in varying stages of approval measure "a core part of the pathology of Alzheimer's disease in the brain," said Dr. Sebastian Palmqvist, a clinical neurologist at Lund University in Sweden. These include two proteins that build up in the brains of Alzheimer's patients: tau and amyloid.

The Elecsys tests and the FDA-approved Lumipulse test measure levels of tau in the blood, while the other Lumipulse test measures the ratio of tau to amyloid. Both measurements can be used to indirectly assess the presence of amyloid plaques, sticky deposits in the brain that are associated with the disease's progression.

It's important to note that the blood tests alone aren't diagnostics for Alzheimer's disease, said Dr. Jemma Hazan, an old-age psychiatrist at University College London. Instead, "the test is telling you whether you have certain abnormal proteins in your brain." This, she said, makes it important to use the test in a setting where patients can be properly directed to the next steps of diagnosis and treatment.

How are Alzheimer's disease blood tests used?

Currently in the U.S., Alzheimer's blood tests are approved for use only for adults ages 55 and older who have signs of cognitive impairment, like memory problems. Palmqvist said these tests are best used by specialists with knowledge of dementia, such as doctors in memory clinics. They aren't approved for use by primary care doctors in the U.S.

"The clinicians working there [at memory clinics] have many, many years of experience of interpreting these types of biomarkers," he explained.

Before the advent of these blood tests, memory clinics had to rely solely on expensive brain scanning technology or invasive lumbar punctures to identify physical signs of Alzheimer's disease. The new tests greatly simplify diagnosis, Palmqvist said, but they still need to be used in combination with other tests.

So currently, if a patient receives a positive blood test, they must undergo further cognitive testing, brain scans or invasive biomarker analyses to confirm the diagnosis.

While for now the blood tests are best used by specialists, data that Palmqvist presented at the conference suggested that access to a blood test result may improve a primary care physician’s diagnostic accuracy to levels closer to a memory clinic specialist's. That hints that the test may eventually be usable in primary care, without more invasive diagnostics.

How well do the approved Alzheimer's tests work?

In clinical trials, the approved Lumipulse test had a sensitivity of 97.6% and a specificity of 90.8%. Sensitivity refers to the percentage of people who do have amyloid in their brains that test positive — so it's the rate of true positives. Specificity refers to the percentage of healthy people who test negative, meaning true negatives.

However, the test was recalled in February because it returned an unusually high percentage of false-positive results when it was used in the real world, compared to clinical trials. Palmqvist said there's now a newer version of the same test that avoids this problem.

Analyses comparing pTau217 and pTau181, the two tau biomarkers that Roche uses in its tests, have concluded that pTau217 is a more accurate indicator of Alzheimer's disease. That means it more closely matches results from gold-standard amyloid brain scans.

Dr. Ashton Harper, global medical affairs lead for neurosciences at Roche Diagnostics, said the Roche pTau217 test correctly spotted Alzheimer's-linked proteins 96.1% of the time and accurately ruled out that pathology 94.7% of the time in trials. By comparison, pTau181 — the Roche test approved in the U.S. — correctly identified Alzheimer's pathology 83.6% of the time and ruled out pathology in healthy brains 72.2% of the time.

Patients who take this more-accurate test are given one of three possible results based on two cutoff points, Harper said. If their tau level comes back above the upper cutoff — giving a positive result — clinicians can be "highly certain" that the patient has disease-linked amyloid in their brain, he said.

Below the lower of the two cutoffs, clinicians can be confident that their patient doesn't have any disease-linked amyloid in their brain. If the reading comes back in between the two cutoffs, though, the result is uncertain.

Current guidelines set by the Alzheimer’s Association require that patients end up in that gray area no more than 20% of the time, and the pTau217 test meets that requirement, Harper said. As with patients who get a positive test result, patients who receive these uncertain results are also advised to undergo further testing, such as scans or cognitive tests.

There are other reasons a person without Alzheimer's disease might get a positive test result; rare cases of severe kidney disease, for example, can artificially inflate the test's readings.

Harper said early data suggests that Roche's pTau217 test is roughly as accurate at detecting Alzheimer's disease proteins in cognitively unimpaired people as it is in those with symptoms. This may someday open the door to prevent Alzheimer's in patients who have not yet developed symptoms, he suggested, clarifying that Roche's test is not intended for that use yet.

How do Alzheimer's tests actually affect patients' care?

In the U.S., these tests can help patients get a diagnosis more quickly, but treatment options for the condition remain limited.

The approved antibody drugs are available through both private and government insurers, but they still cost the patient thousands of dollars each month. And again, these drugs only slow, rather than stop, the progression of the disease.

Researchers hope that early treatment with the drugs will enhance their effectiveness, but as of yet, there's no published data to back this idea up.

In the U.K., disease-modifying drugs like the antibodies have not been approved by the U.K.'s National Health Service (NHS) yet. Because the drugs only modestly slow Alzheimer's progression, ultimately, the NHS determined that they were too costly to cover without clearer signs of efficacy. That means British patients cannot access the drug for free.

Still, Hazan said a positive test could be beneficial for patients.

"Diagnostic accuracy is important in its own right so that people feel more certain about the diagnosis and also there are management implications," Hazan said. While they can't access antibody drugs, patients do have access to drugs that help ease the condition's cognitive and behavioral symptoms, as well as non-pharmacological treatments like behavior management.

Diagnosed patients can also access one of the many clinical trials for the condition. It's estimated that 50,000 patients are needed to populate these ongoing trials worldwide.

Hazan and Palmqvist agreed that, despite the blood tests' accuracy, they should not be used to preventively screen for Alzheimer's in people with no symptoms. That's because testing in a wider population, where fewer people will have Alzheimer's disease, naturally increases the number of false-positive results, even while the assay itself retains the same level of accuracy. This could lead many healthy people to be incorrectly diagnosed with Alzheimer's disease, which would cause stress for patients and have significant financial implications for healthcare systems.

Newer tests that are still in development may help reduce the likelihood of false positives by measuring only a subset of tau protein that comes directly from the brain rather than from the rest of the body, Palmqvist said. But for now, mass screening remains a goal, rather than a reality, for these blood-based Alzheimer's diagnostics.

"I think that's the next frontier," Palmqvist said.

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

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Astronomers may have just found a first-of-its-kind phenomenon buried in the shadow of one of the Milky Way's most famous stellar explosions: two stars that died in separate supernovas, after spending millions of years orbiting each other.

Using 16 years of data from NASA's Fermi Gamma-ray Space Telescope, researchers detected high-energy gamma rays coming from a faint, previously overlooked supernova remnant called G189.6+3.3, which sits right beside the well-studied remnant IC 443 (nicknamed the Jellyfish Nebula). Their analysis suggests that the two remnants aren't just neighbors by coincidence. Instead, they may be the leftover wreckage of a binary star system, making this the first confirmed case of two supernova remnants traced to the same stellar pair.

The findings were published July 21 in the journal Nature Communications.

"We weren't really looking for a binary supernova remnant," study first author Miltiadis Michailidis, an astrophysicist and postdoctoral fellow at Stanford University, told Live Science. The team originally set out to characterize G189.6+3.3, which had long been overshadowed by its brighter neighbor. IC 443 is one of the best-studied remnants in the galaxy and among the first ever confirmed to accelerate protons — one of the key ingredients thought to produce cosmic rays, the high-energy particles that constantly strike Earth's atmosphere.

By combining Fermi's gamma-ray data with X-ray, radio, ultraviolet and optical observations, the team teased out G189.6+3.3's faint signal and found something strange: Instead of glowing uniformly, its northern half was dominated by accelerated protons, while its southern half was dominated by electrons. It's the first time such a clean split has been spotted within a single remnant.

The explanation, they found, came down to the environment: The northern edge of the remnant presses against a dense cloud of hydrogen gas, which gives fast-moving protons something to collide with, thereby producing gamma rays, Michailidis said. The southern half lacks that dense material, letting a different, electron-driven process take over instead. Ultraviolet observations showed that the northern shock wave had slowed after slamming into the cloud, backing up that interpretation.

Earlier work had already shown that IC 443 interacts with the same cloud, which implies that both remnants sit at roughly the same distance from Earth. To rule out coincidence, the researchers simulated 1 million hypothetical binary star systems and calculated how often two unrelated remnants would wind up this close together purely by chance. Depending on the method used, the odds came out to somewhere between 1 in 1,000 and 1 in 100. In other words, it's highly likely that the two supernova remnants are related.

The team also estimated when each star likely exploded, finding that the two blasts were probably separated by tens of thousands of years. That finding is consistent with one star in a binary pair going supernova first, with its companion following suit long afterward.

Rather than relying purely on computer models, astronomers can use this real-world system to test long-standing theories about how massive binary stars live, interact and eventually explode.

Michailidis said the team's next step is to search for similar binary remnant pairs elsewhere in the galaxy, to understand why this system has stood alone until now. He pointed to one particular payoff: Measuring the distance between two remnants' explosion centers can reveal how much energy a supernova actually released — a quantity that, until now, astronomers could only estimate from theory. "Now we can actually test it," he said.

Traces of two "ghost lineages" of extinct human populations lie hidden within our genome, a new study reveals.

One of these ghost lineages left its DNA scattered in all present-day people. The other, a "super-archaic" lineage, dates back nearly 2 million years, researchers reported Thursday (July 30) in the journal Science.

"These extinct populations may have lived hundreds of thousands — or even more than a million — years ago, yet traces of their genetic legacy remain preserved in our genomes today," study co-author Priya Moorjani, a human evolutionary geneticist at the University of California, Berkeley, told Live Science.

For decades, experts have found DNA evidence that our species, Homo sapiens, once mated with now-extinct relatives such as Neanderthals and Denisovans. Most people not of sub-Saharan ancestry living today possess about 1% to 2.4% Neanderthal ancestry, and Asians and Oceanians (people from the island nations of the Pacific Ocean) harbor about 0.1% to 6% Denisovan ancestry.

But scientists have suspected that modern humans may have interbred with other now-extinct human groups that have not been identified yet. However, the scarcity of ancient DNA samples makes it challenging to identify what these unidentified groups, often called ghost lineages, might have contributed to our species.

"Ancient DNA has transformed our understanding of human evolution, but it can only tell us about populations for which DNA has been preserved," Moorjani said. "DNA survives only under very specific conditions — typically in cold, dry environments — which means that much of our evolutionary history, particularly in Africa, other tropical regions, and at very deep timescales, remains inaccessible."

Looking for "long-extinct ancestors"

In the new study, Moorjani and her colleagues reasoned that everyone's genome contains a record of their ancestry. They investigated whether it was possible to uncover signs of "long-extinct ancestors preserved within the genomes of present-day people," Moorjani said.

The researchers developed a new technique to scan and compare more than 500 complete genomes of present-day humans from around the world. Using this data, they reconstructed the complete genealogies of each spot in each person's genome, developing family trees of the people's ancestors that mapped out every time genetic lineages diverged and merged. They focused on ancestors who had profound genetic differences from modern humans ‪—‬ a sign they evolutionarily split from the modern human lineage a long time ago.

"Most regions of our genome share a common ancestor relatively recently in our evolutionary history," Moorjani said. "Occasionally, however, we find stretches of DNA whose common ancestor lies much farther back in time, indicating they originated from a long-separated human lineage."

Unlike previous approaches, this new method does not require DNA samples from fossils in order to spot ancient genetic sequences in the modern-human genome. "We no longer have to wait for extraordinary fossil preservation to learn about extinct human populations," Moorjani said. "Instead, the genomes of living people contain traces of these ancient ancestors, and genealogical methods allow us to recover some of that hidden history."

The researchers experimentally tested the new method, which correctly identified Neanderthal and Denisovan ancestors in modern-human genomes. However, it also uncovered previously unknown instances of interbreeding with now-extinct groups.

The researchers said one ghost lineage's DNA was found in all modern humans. This finding suggested that the lineage interbred with modern humans in Africa more than 50,000 years ago, before the most recent migration of H. sapiens out of Africa and into the rest of the world.

"Previous publications suggested that there might be ghost ancestry — ancestry from unknown archaic lineages in modern humans — but they hadn't concluded whether this unknown ancestry is present only in Africans or not, and when this introgression event happened," study co-author Yulin Zhang, a computational biologist at UC Berkeley, said in a statement. "We were actually able to find and map genomic locations in modern humans that are from this ghost lineage and show that this ghost ancestry is in all modern humans, not only in Africans."

This newfound lineage's DNA constitutes about 0.5% to 1% of the genomes of modern humans, comparable to the amount of Neanderthal DNA in many people living today. The scientists estimated that this ghost lineage diverged from the ancestors of modern humans about the same time Neanderthals and Denisovans did, about 800,000 years ago.

Ghost candidates

One possible candidate for the ghost lineage is Homo heidelbergensis, the researchers wrote in the study. This human species lived from about 700,000 to 200,000 years ago in Africa and Europe.

"I agree with their speculation that this ghost could have been the species Homo heidelbergensis, which was present in Africa as recently as 300,000 years ago," Chris Stringer, a paleoanthropologist at the Natural History Museum in London who was not involved in the study, told Live Science.

The scientists also found evidence that people from Oceania inherited traces of a "super-archaic" human lineage that diverged from the ancestors of modern humans about 1.8 million years ago, before the emergence of the common ancestor of modern humans, Neanderthals and Denisovans. This super-archaic DNA, on average, made up about 0.002% of the Oceanian genomes investigated and appeared within regions of Denisovan DNA, suggesting that the super-archaic DNA got into modern humans through interbreeding with Denisovans.

The age of this super-archaic DNA suggests it may have come into Denisovans, and then modern humans, from Homo erectus, the longest surviving human species to date, Fernando Villanea, a population geneticist at the University of Colorado Boulder who was not involved in the study, told Live Science. That could make sense, because H. erectus skulls found in Yunxian, China, share some features with Denisovan fossils, Villanea added. But to date, only a limited amount of H. erectus genetic material has been analyzed.

The study's findings highlight that modern humans are the product of multiple species and that "hybridization is the norm and not the exception," Villanea said. "We see hybridization being a common trait in the evolution of many other species, and these findings help us reframe our scientific thinking away from a mentality of human exceptionalism."

The DNA segments from these newfound lineages are spread throughout the human genome, but they are most numerous in parts of the genome associated with the immune system and metabolic function. Moorjani said this makes sense, as the need to adapt to new germs and sources of food has been one of the strongest drives in human evolution. Interbreeding with other now-extinct human groups allowed modern humans to acquire potentially beneficial DNA.

"This work reinforces a fundamental shift in how we think about human evolution," Moorjani said. "Rather than a simple branching tree, human history is increasingly emerging as a complex web of populations connected by repeated episodes of divergence, migration and mixing."

Stringer agreed, adding that this new technique provides "indirect ways of reconstructing parts of the genomes of more primitive species like H. erectus and H. heidelbergensis."

In the future, the scientists hope to use their new method to detect signs of more ghost lineages, "particularly those from regions such as Africa and South Asia that remain underrepresented in ancient-DNA studies," Moorjani said. The new technique can also help researchers "study evolutionary history in other species where fossil DNA is scarce or absent," she added.

See how much you know about early humans with our human evolution quiz!

Whale sharks may be the biggest fish in the ocean, but their feeding habits have remained mysterious. Now, new camera footage from the backs of these gentle giants has captured them doing something scientists rarely get to see: hunting for food far below the surface.

The footage reveals that whale sharks (Rhincodon typus) spend far more time feeding underwater than scientists realized and that they use a surprising variety of foraging techniques that had never been documented before.

The videos show whale sharks filtering food while cruising through open water, gliding downward as they feed during dives, climbing back toward the surface with their mouths still open, and cruising just above the seafloor to feed. Slow, steady underwater feeding turned out to be one of the sharks' most common activities.

Philip Motta, a professor emeritus of biology at the University of South Florida who was not involved in the study, said the videos provide "very valuable" new information on the variability of whale shark feeding behaviors, which have been poorly documented to date.

Cameras reveal whale shark feeding

Before this study, whale sharks had been studied from boats, from planes and by divers swimming alongside them. But those methods shared a blind spot: They could only follow the sharks when they were near the surface.

Earlier research had hinted that whale sharks spend a lot of time feeding out of view, at varying depths. In a 2020 study, researchers estimated that whale sharks may forage at these depths for up to 20% of the day and feed at the surface for less than 1% of their time.

In the new study, scientists strapped cameras directly onto the whale sharks, offering a rare shark's-eye view beneath the waves.

They deployed camera tags on 10 whale sharks at Ningaloo Reef in Western Australia and gathered more than 22 hours of footage from the sharks' own perspective. They combined that footage with a review of 106 previously published studies to build the most comprehensive catalog of whale shark behavior to date. Ultimately, they cataloged 36 distinct behaviors ‪—‬ 12 were related to feeding, and of those, six had never been recorded before. The findings were published July 21 in the journal Marine Biology.

Whale sharks can grow to 60 feet (18 meters) in length. And yet, this enormous fish survives on tiny prey ‪—‬ like krill, fish eggs and plankton ‪—‬ in tropical waters that are notoriously poor in nutrients. The ability to switch between so many feeding techniques may help to explain the long-standing puzzle of how such a large species can survive in these nutrient-poor waters.

However, even with a shark's-eye view, the cameras captured only part of the story. Whale sharks are known to dive hundreds of feet below the surface, where sunlight disappears and conventional cameras can no longer record.

"The most important new discoveries could be what these gentle giants are doing when they perform really deep dives," Motta said.

Shark quiz: How much do you know about these iconic ocean superstars?

Two Chilean mummies have provided scientists with the earliest known smallpox genomes found in the Americas, dating between 1492 and 1631.

The genomes are the first-ever DNA evidence that proves European colonization introduced smallpox to the Americas, according to a paper that published Thursday (July 30) in the journal Science.

Smallpox, an infection caused by the variola virus, was one of the deadliest diseases in the world until it was completely eradicated in 1980. While the disease has been found in 3,000-year-old Egyptian mummies, the first documented outbreak in the Americas was in 1518, during the Spanish conquest of the Caribbean. The virus then spread rapidly throughout Central and South America.

Experts have estimated that the disease caused the deaths of three to four million Indigenous people with no prior immunity to the disease. The combination of smallpox, violence, slavery and other diseases wiped out about 90% of the original inhabitants of the Americas by 1600.

While historians and scientists have long understood the toll of the disease, the story of smallpox's spread comes primarily from historical records, which were written by European colonizers and may not have fully captured transmission among Indigenous peoples. There's also a lot scientists don't know about the specific viral strains responsible for the pandemic because of the lack of ancient smallpox DNA evidence in the Americas.

In the new study, the researchers identified ancient smallpox virus DNA from the bones of two mummified Indigenous Inca individuals from northern Chile: an adult female and an adult male who lived between 1492 and 1631.

"None of us expected to find variola virus DNA from the sample that they collected, so it was completely a surprise," study co-author Shigeki Nakagome, a geneticist at Trinity College Dublin, told Live Science. The research team was not targeting ancient pathogens but rather looking to understand human population history in the region. "I don't think there was any historical record documenting smallpox in this particular community, so no one expected the smallpox evidence."

Analysis of the two ancient viral genomes showed them to be almost identical, suggesting the two individuals were likely infected during the same outbreak or by the same circulating strain.

Comparing the genomes of ancient and modern variola viruses, the researchers found that the genome matched an extinct lineage that split from another European strain around 1296, but that predates modern strains. That means the variola virus found in the mummies is an evolutionary step between medieval European strains and modern strains, proving that Europeans brought smallpox to the Americas.

"We provide the first molecular evidence of smallpox introduction to the Americas through colonization," Nakagome said.

"This paper is really lovely because we know from the historical record that smallpox had a huge impact on Indigenous populations in the Americas," Anne Stone, an anthropologist at Arizona State University who was not involved in the study, told Live Science. "This paper gives us the first description of the pathogen during the colonial period," she said, adding that it corroborates the "historical record that a smallpox epidemic went through [the Americas]."

The genome also showed that, through a series of mutations, the genes that enable variola to infect species other than humans — genes present in related viruses that infect animals, like mpox or cowpox — were inactivated, Bruno Romero González, a computational biologist at Trinity College Dublin and lead author of the study, told Live Science. Over time, this ancient variola strain became less able to infect animals. "Because of that, variola started to focus on targeting only humans," Romero González said, ultimately adapting to become more successful in infecting people.

The researchers hope that more samples of ancient variola virus are found throughout the Americas, to complete the picture of smallpox's evolution and movement.

Studying ancient DNA can also give scientists insight into how modern day diseases might behave, Stone said. Understanding the evolution of this pathogen is particularly important because Mpox is in the same group and closely related, she said. Studies have suggested Mpox might behave similarly to the historical variola virus, in that it seems to mutate to adapt to human hosts. "It's always useful to study ancient pathogens," Stone said, "helping us learn how these pathogens adapt to us."

The study adds to growing evidence for smallpox on ancient Indigenous skeletons, including two 16th-century toddlers buried in Peru whose bones have lesions suggestive of smallpox infection.

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Archaeologists excavating in the famous prehistoric Hohle Fels cave in Germany have uncovered two bird figurines carved from mammoth ivory. ‪‪The thumbnail-size carvings add to the existing ‬‬evidence that ice age humans had a sophisticated artistic sense 40,000 years ago.

"The figurines demonstrate that the earliest artists were skilled ivory-carvers, who could depict delicate motifs in miniature form," Nicholas Conard, an archaeologist at the University of Tübingen in Germany and director of excavations at Hohle Fels, said in a July 29 statement.

When the birds were found in 2025, they were lying just 5 feet (1.5 meters) from each other in a layer dating back 40,000 years, according to the statement. The sculptures bring the total number of bird figurines from Hohle Fels up to three; a small water bird was found there in 2001.

Hohle Fels was occupied by early Homo sapiens during the Aurignacian period of prehistory (43,000 to 28,000 years ago), following the decline and disappearance of Neanderthals from Europe. At that time, humans launched a creative explosion, creating the world's first musical instruments, jewelry and small sculptures. The Venus of Hohle Fels, a 41,000-year-old statuette of a woman with exaggerated breasts and buttocks discovered in the cave in 2008, is generally considered the oldest figurative sculpture in Europe. Archaeologists have also found figurines of animals and an ivory rope-making tool at Hohle Fels, a German name that means "hollow rock" in English.

At roughly thumbnail-size, the two new bird carvings are significantly smaller than the figurines found previously at Hohle Fels. Despite their tiny dimensions, "the carvings are not highly stylized but instead include many specific and unique features," Conard said. "The artist has recorded detailed observations that allow us to consider which kind of bird is represented and what the bird could be doing."

One bird appears to be lying on the ground, possibly brooding over its eggs. This position suggests the bird is a ptarmigan, a game bird that is related to chickens and grouse and whose bones have been discovered in the prehistoric layers at Hohle Fels. The second bird has spread wings that are suggestive of flight or posturing in courtship, according to the statement. This bird may also be a ptarmigan, or possibly a bird of prey.

The two tiny ptarmigans raise many new questions about early humans in Europe, Conard said. They are among the earliest evidence of modern humans in Europe, suggesting art was a major feature of early human life. Archaeologists do not know what meaning the carvings held for the Aurignacian people who lived at Hohle Fels, but the objects may have been personal talismans or a symbol of a specific group of people.

Hohle Fels is unique among ice age cave sites because, to date, it is the only one with bird figurines. This may reflect people's keen observations of the natural world around them.

"Our region and landscape have always been the home of a vast range of birds," Stefanie Kölbl, managing director of the Museum of Prehistory and Ice Age Art, said in the statement. "Their calls signaled warnings, and the residents of the region often used their hollow bones and even mammoth ivory to make flutes that produced magical sounds."

The figurines are on display at the Museum of Prehistory and Ice Age Art in Blaubeuren, Germany, through April 4, 2027.

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Bats have long posed an immunological mystery: They can harbor viruses that cause severe diseases in other animals, including humans, yet they rarely show signs of illness. Now, scientists have discovered a big clue as to why that is.

Researchers uncovered an unusual feature of bat immunity that could help to explain how these mammals evade infections. Vesper bats, the world's largest family of bats, may possess two separate genetic systems for producing the building blocks of antibodies, the immune proteins that latch onto germs. This configuration has never been found before in mammals.

"It was really surprising," study co-author Hannah Frank, an associate professor of ecology and evolutionary biology at Tulane University, told Live Science. "The only other vertebrates we see something similar in are fish."

The findings, published Wednesday (July 29) in the journal Science Advances, could open new avenues for studying viral infections and the evolution of immunity.

"The study provides a novel view into the evolution and diversity of adaptive immunity in bats," said Daniel Becker, an associate professor of biology at the University of Oklahoma who was not involved in the study. "The duplication seen in vesper bats is really intriguing and suggests that we need more immunological study of this globally distributed family of bats," Becker told Live Science in an email.

'More diversity in their antibodies'

Antibodies are Y-shaped proteins that help the immune system recognize and neutralize foreign invaders, including viruses, as well as other threats, like toxins. Each antibody contains two "heavy chains" and two "light chains," structures that work together to recognize and bind to specific features of viruses, bacteria or other targets.

The tips of the Y shape are responsible for recognizing the targets, while other parts of the antibody help determine how the immune system responds — by blocking pathogens from infecting cells or flagging them for destruction by other immune cells, for instance.

In humans and most other mammals, the genes that build antibody heavy chains are organized into a single region of the genome, called a locus. Cells create a wide range of antibodies by mixing and matching the proteins encoded in different segments of that locus.

But when Frank and her team examined 26 bat species, they found two complete heavy-chain loci located on different chromosomes. The team then showed that both sets of genes were functional and actively used by immune cells to build antibodies. The finding was initially surprising enough that the researchers considered whether it could be an error in how they'd assembled the bats' genomes after sequencing them.

However, Frank's collaborator and former graduate student Dr. Taylor Pursell thought the finding might be genuine, rather than an experimental fluke.

"She said, 'No, Hannah; this is really weird ‪—‬ like, this doesn't happen,'" Frank recalled. "And I said, 'Oh my God; you're right. This is not just an experimental annoyance. This is actually super cool.'"

Using genetic analysis, the team found that one of the two loci contained a larger and more varied collection of gene segments that could be used to create a broad, ready-made repertoire of antibodies. The other had fewer of these building blocks but appeared to rely more heavily on a process called somatic hypermutation, in which antibody-producing cells make small genetic changes after encountering a pathogen.

Those changes can help antibodies become more "customizable" to whatever threatens the immune system, Frank said.

She compared this system to the different layers of defense seen in the 1998 Disney movie "Mulan." Upon seeing invaders at the Great Wall of China, guards raised an alarm to alert others without yet knowing the specific threat; this is like the innate immune system, the body's first, broad line of defense. The adaptive immune system is more like the heroine Mulan: highly targeted and capable of responding to a specific enemy, but slower to develop.

These two layers of immune defense are not unique to bats, but bats' two antibody systems may provide an additional layer of protection.

From each loci, bats can create a "cache of trainable, customizable cells," Frank said. This degree of customization could help the bats immune system ward off a wider range of threats than other mammals can.

"This extra set of genes gives the animals more diversity in their antibodies," said Michael Letko, a molecular virologist at Washington State University who was not involved in the study. "This study suggests bats have more diversity to start with, which may allow for faster and more effective responses from the start of an infection," Letko told Live Science in an email.

Letko added that the genetic analysis in the study was impressive and lends credibility to the results. "It is hard to dispute the validity of information solidly founded on the genetic organization of these bats," he said.

That interpretation remains a hypothesis, though; Frank and her team will need to study how these two systems behave when bats are exposed to viruses before they can determine exactly what advantages they provide.

"We think this discovery is an important piece of the puzzle," Frank said in a statement. "It doesn't fully explain why bats are such effective viral reservoirs, but it reveals a level of immune variety we didn't know existed and gives us an entirely new direction to explore."

Past studies of bat immunity have found that hotter body temperatures and a larger number of virus-filled packages in stem cells could also help bats' tolerate viruses better.

Understanding how bats tolerate viruses could help scientists predict which kinds of bats are most likely to affect human health and how we can mitigate those risks, Becker noted. Separately, bats have a notably low incidence of tumors and cancer, Letko said, and he wonders if their unique immune systems might hold clues as to why.

While bats are often viewed through the lens of the infectious diseases they carry, their story is far more complex, Frank said.

"Let's learn from the guys who've been evolving with them [viruses] for millions and millions of years," Frank said. "But let's try not to villainize them for surviving for millions and millions of years."

Using laser scanning technology to peer beneath the dense canopy of the Amazon rainforest, archaeologists have discovered hundreds of ancient earthworks that were made by a complex, enigmatic society over two millennia ago, a new study finds.

This ancient civilization, called the Aquiry, arose 2,500 years ago in Brazil. Based on the large number of earthworks, called geoglyphs, the Aquiry may have had 3 million people before the society collapsed, the researchers suggested in the study.

"The cultures and societies that composed the Aquiry shared a common worldview and constructed ceremonial centers in a variety of monumental geometric forms, characterized by deep ditches and high outer embankments, commonly known as Amazonian geoglyphs," Martti Pärssinen, an archaeologist at the University of Helsinki, told Live Science in an email.

In the new study, published Wednesday (July 29) in the journal Nature, Pärssinen and co-authors presented findings from their survey of nearly 1,740 square miles (4,500 square kilometers) of Amazonian rainforest, which revealed 396 new geoglyphs and allowed them to approximate the geographical extent of the Aquiry civilization.

Pärssinen has been investigating geometric earthworks in Brazil's Acre state for more than two decades. In a 2021 study, he officially introduced the name Aquiry for the multicultural ancient civilization, named after the Acre River, which flows from Peru and Bolivia through the present-day states of Acre and Amazonas in Brazil. Aquiry means "river of caimans" in the language spoken by the Indigenous Arawakan people.

Because of the dense canopy of trees in the rainforest, archaeological investigation in the area has been limited. Most of the evidence for the Aquiry civilization comes from lidar and airborne laser scanning of monumental geoglyphs that were constructed between 600 B.C. and A.D. 850, according to the study. People lived in multifamily longhouses around the earthworks, and they farmed crops like maize and squash.

"According to native oral traditions, the Aquiry centers were built to foster relations among communities" and with significant otherworldly beings, Pärssinen said. These centers also served as venues for gatherings and political decision-making, and they enabled chiefs to display their generosity, he added.

To date, archaeologists have identified around 1,700 known geoglyphs in the area. But the researchers think the total is significantly higher, with more than 20,000 Aquiry earthworks waiting to be found in places that haven't yet been surveyed. And based on an estimate of 300 people needed to build and maintain each geoglyph on average, the researchers estimated that the Aquiry civilization likely peaked at 1.25 million to 3 million people between A.D. 100 and 300.

Similar geoglyphs dating to between 200 B.C. and A.D. 500 have been found in Peru. Known as the Nazca Lines, these earthworks are shaped like animals, humans, plants and fantastical figures, in addition to having geometric motifs. The Nazca were an interconnected regional society of precolonial farmers who were able to survive in a forbidding geographic region, but they lived roughly 1,050 miles (1,700 kilometers) from the Aquiry.

"The Nazca geoglyphs represent a different phenomenon and were probably unrelated to the Aquiry civilization," Pärssinen said. "Nevertheless, in both cases, the straight roads and lines, as well as the geometric forms and motifs, are best appreciated from the air."

The presence of thousands of geoglyphs in the southwest Amazon region is leading archaeologists to rethink assumptions about precolonial civilizations and urban development — but it's also bringing up questions about the fate of the Aquiry.

"We do not know why the geoglyphs were suddenly abandoned between A.D. 850 and 950," Pärssinen said. "The available evidence points to a relatively rapid collapse" that may be related to the disappearance of other major precolonial powers, he said, "including the Classic Maya in Central America and the Tiwanaku and Wari civilizations in the Andes."

How much do you know about the first people to reach the Americas? Find out with our First Americans quiz!

Hundreds of spectators who attended the recent launch of a Chinese rocket witnessed a truly shocking sight when a bolt of lightning struck the ascending vehicle in midair.

Stunning photos show the exact moment the zigzagging beam of electricity surged around the rocket's fuselage and through its exhaust plume before shooting down toward Earth's surface.

Despite being hit with at least 100 million volts of electricity, the uncrewed rocket safely reached space and successfully deployed its payload in orbit.

The stricken spacecraft, a Long March 3B rocket, lifted off from Xichang Satellite Launch Center in southwest China on July 23 at around 8 p.m. local time, Live Science's sister site Space.com reported. But around 30 seconds after leaving the ground, the rocket was suddenly hit by lightning, which illuminated the sky in the blink of an eye.

Video footage from the launch (see below) shows a large crowd of people with raincoats and umbrellas collectively gasping as lightning hits the rocket and then loudly cheering as the spacecraft continues its climb, unimpeded by the electrical discharge.

A translated statement from the state-owned China Aerospace Science and Technology Corp. released later the same day said the mission was a "complete success" and that the Long March 3B correctly deployed its payload, the Tianlian-2 (06) satellite, a geostationary relay satellite that will help support China's Tiangong space station.

However, the statement did not mention the lightning strike.

Modern spacecraft are designed to have highly conductive shells that divert massive electrical charges around their exteriors without impacting critical interior infrastructure or any crew they might be carrying. This works similarly to a Faraday cage, a protective enclosure that prevents certain types of electromagnetic radiation from entering or exiting. Similar designs are also used in commercial planes, which are struck by lightning at least once per year, on average, according to the National Weather Service.

Despite this, rockets normally launch only in good weather to minimize the risk.

Previous incidents

It is unclear exactly how many rockets have been struck by lightning throughout the history of spaceflight, but there have been several notable examples.

Perhaps the most famous incident was during NASA's Apollo 12 mission, which successfully landed a trio of astronauts — Charles Conrad, Alan Bean and Richard Gordon — on the lunar surface in November 1969. Shortly after liftoff, the Saturn V rocket carrying the astronauts was struck by lightning twice as it climbed into the atmosphere. Some nonessential instruments and sensors experienced "permanent effects" from the strikes, according to one recently released report. However, these issues did not stop the spacecraft from safely ferrying the astronauts to the moon and back.

Most recently, in 2019, a Russian Soyuz rocket was struck by lightning while carrying a communications satellite into low Earth orbit, Ars Technica reported.

Lightning can also hit rockets on the launchpad, which is what happened in the lead-up to the Artemis I mission in 2022. The uncrewed Space Launch System rocket, which launched NASA's first moon mission in 50 years, was struck by lightning during a "wet dress rehearsal" around seven months before launch. However, strikes like these are exceedingly rare nowadays, as most launchpads are surrounded by towers designed to attract lightning away from standing rockets, according to The Institution of Engineering and Technology.

Although these spacecraft remained relatively unscathed, the same cannot be said for an Atlas-Centaur rocket (dubbed AC-67) that was destroyed in 1987 after being struck by lightning 48 seconds after lifting off from Cape Canaveral, Florida. A NASA report later revealed that the electrical discharge had triggered a "single-word memory alteration" in the rocket's navigational computer, which caused it to veer sideways and completely break apart.

While millions around the world grappled with extreme heat this month, a research station in Antarctica recorded Earth's coldest temperature since 2012.

The high-altitude research station, named Concordia, logged a low of minus 119.4 degrees Fahrenheit (minus 84.1 degrees Celsius) on July 18, according to data from the station.

Concordia is located in the interior of the Antarctic continent, which is currently in the dead of winter with no sunlight. Temperatures at the station regularly fall below minus 112 F (minus 80 C) this time of year ‪—‬ so the new reading isn't unprecedented, but it's still significant.

"Even here, where extreme cold is expected, temperatures below minus 84 C are remarkable and highlight how variable Antarctic weather can still be," Gabriele Carugati, the station leader at Concordia for Italy's National Antarctic Research Program (PNRA), told Live Science over a video call from the station.

The French Polar Institute Paul-Émile Victor, which runs Concordia with the PNRA, sent Live Science raw data from July 18, which showed the temperature dropping to minus 84.1 C twice, at 6:25 a.m. and 6:34 a.m. local time.

The extreme chill at Concordia stands in sharp contrast to the sweltering heat that many countries are currently experiencing. North America and Europe have been battling heat waves this summer, with Western Europe recording the hottest June on record. Meanwhile, wildfires are raging in Canada, the U.S., France, Spain and other countries.

Globally, average temperatures are going up as humans pump more heat-trapping greenhouse gases into the atmosphere. However, Earth's weather systems are complex, and climate change doesn't mean that everywhere gets hotter all of the time.

"Climate change describes the long-term global trends, while individual weather events can still [bring] exceptional cold," Carugati said. "Antarctica is influenced by complex atmospheric processes, so an extreme low temperature at one location does not contradict the broader picture of global warming."

"Astronauts of ice"

Concordia is considered the most remote and extreme research station in the world. Built on top of a 10,800-foot-thick (3,300 meters) ice cap, the station is used for a variety of purposes, including seismic observations, astronomy and the modeling of Earth's past climates, according to the French Polar Institute Paul-Émile Victor.

"Concordia is a special place because it sits at over 3,200 meters [10,500 feet] above sea level on the Antarctic Plateau, and more than 1,000 kilometers [600 miles] from the coast," Carugati said. "During winter, there is no sunlight for months, the atmosphere is extremely dry and stable, and under clear skies, heat continuously escapes to space because there are no clouds, allowing temperatures to fall to extraordinary levels."

Concordia's environment is so harsh and isolated that the station is also used to improve our understanding of the physical, mental and social challenges astronauts experience in space. Carugati noted that the only person at the station who is not researching the environment is a European Space Agency biomedical doctor, who is studying the researchers who work there, nicknamed "astronauts of ice."

Planes can't fly to Concordia once winter sets in, and it's around 370 miles (600 kilometers) from the nearest research station. That technically makes crews more isolated than astronauts on the International Space Station, which orbits about 250 miles (400 km) above Earth, according to the European Space Agency.

What is the coldest temperature ever recorded?

The coldest temperature ever recorded at Concordia was minus 120.5 F (minus 84.7 C), logged in the winter of 2010, according to the Italian Antarctic Meteo-Climatological Observatory. However, another high-altitude research station in East Antarctica has the all-time record for the coldest temperature ever recorded on Earth. Russia's Vostok weather station, the nearest station to Concordia, recorded a temp of minus 128.6 F (minus 89.2 C) in July 1983, according to the World Meteorological Organization.

Satellite data suggests that temperatures can drop as low as minus 144 F (98 C) in East Antarctica, according to a 2018 study published in the journal Geophysical Research Letters. However, even though Antarctica is the coldest and driest continent, it's not immune to global warming.

Major glaciers and the ice sheet they support are at risk in West Antarctica, with the Antarctic Peninsula — which extends out of the western side of the continent — experiencing the most rapid warming. A study published in February in the journal Frontiers in Environmental Science found that decisions made on greenhouse gas emissions today will determine how much the peninsula will change in the coming centuries, with sea ice, ice shelves and glaciers, along with the penguins that live on them, at risk of disappearing.

Concordia sits on the largest ice sheet on Earth. This sheet in East Antarctica is more stable than the smaller sheet of West Antarctica, but it is still vulnerable to rising temperatures. An unprecedented Antarctic winter heat wave in March 2024 saw temperatures near Concordia rise to a record high of 15.1 F (minus 9.4 C) ‪—‬ about 32 F (18 C) warmer than the previous March maximum. This East Antarctic heat wave was amplified by global warming, according to a study published in April in the journal npj Climate and Atmospheric Science.

Earth recently entered an El Niño, the warm phase of a multiyear natural climate pattern, which could bring unprecedented temperature extremes to an already-warming world. Carbon Brief, a U.K. based outlet that reports on climate news and policy, has predicted that 2026 is likely to be the second-warmest year on record, behind 2024, with the intensifying El Niño increasing the likelihood that 2027 will be the warmest year ever recorded.

For now, at Concordia, the researchers are continuing their work in the blistering cold of Antarctica's winter. Carugati noted that the latest extreme-temperature data will inform forecasts and long-term climate monitoring.

"Extreme observations like this help scientists better understand atmospheric processes and improve the climate models," he said.

Betelgeuse, the bright reddish star that marks Orion's shoulder, has kept skywatchers company for thousands of years — and it may have had company of its own the whole time.

Astronomers say they've captured the clearest image yet of a faint star orbiting tightly around Betelgeuse, in what they're calling the strongest evidence so far that the famous red supergiant isn't flying solo. The find was announced by the European Southern Observatory (ESO) on Tuesday (July 28) and detailed in a new paper in the journal Astronomy & Astrophysics.

Betelgeuse, usually one of the top 10 brightest stars visible from Earth, naturally swells and shrinks as it pulses across a cycle of 400 days, according to NASA, which causes the star to wax and wane in brightness. But for decades, scientists have puzzled over an extra pattern: a slower dimming and brightening outside of this 400-day cycle that repeats roughly every six years.

Two independent teams — one led by astrophysicist Morgan MacLeod of Harvard University, the other by Jared Goldberg, a postdoctoral fellow at the City University of New York — each modeled that long-term wobble using decades of brightness and velocity data, and converged on the same explanation: the pattern comes from a hidden companion star, orbiting so close to Betelgeuse's bloated surface that it's nearly impossible to see.

However, their calculations suggested that there might be a moment, in December 2024, when that companion would swing far enough away from Betelgeuse that we might be able to photograph it.

So that December, a team led by Paris Observatory astronomer Miguel Montargès trained the European Southern Observatory's Very Large Telescope on Betelgeuse. They then spent months combing through the data, and the effort paid off: they found what looks to be this companion star, now nicknamed Betelgeuse B.

"The fact that we can still discover a nearby companion, more massive and brighter than the Sun, around such a well-studied star is remarkable," Montargès said in an ESO statement. "These are among the best moments in science: seeing something new, unexpected."

One surprise: the companion turned out to be beefier than expected. Scientists had guessed it was roughly as massive as our sun, but the new images suggest it's actually two to three times heavier — which also makes it brighter and easier to spot than predicted.

However, the researchers say they need one more image of this star. To be certain that the companion is really there, we still need to observe it in one year on the other side of the star, but there is very little space left for doubt,"adds Montargès.

If confirmed, the discovery could reshape how astronomers think about Betelgeuse's fate. As a red supergiant, it's in the final stage of its life and will eventually end in a supernova explosion — though pinning down exactly when is notoriously difficult, says Montargès. "The question is … whether this companion is going to have an impact on the evolution of the red supergiant," Montargès said.

Monkeys use some of the same basic mental strategies as people do to perceive abstract relationships between shapes, a new study suggests.

The findings challenge the idea that humans crossed a sharp evolutionary divide when they learned to recognize geometric properties like symmetry, parallel lines and right angles, the researchers say.

"While humans do come up with geometric descriptions that are more abstract than what nonhumans can do, there's still some overlap, some similarity in the kinds of geometric intuitions you see in humans and those of non-primates," study co-author Jessica Cantlon, a professor of developmental neuroscience and psychology at Carnegie Mellon University, told Live Science. "So there's a thread of continuity that runs through geometric reasoning between humans and nonhumans."

The research, published July 20 in the journal PNAS, adds to a long-standing scientific debate over whether humans possess entirely unique forms of abstract thought or unusually sophisticated versions of abilities found elsewhere in the animal kingdom.

"For decades, cognitive scientists have searched for the 'special ingredient' that distinguishes human intelligence from that of other animals," Elizabeth Brannon, a professor of psychology at the University of Pennsylvania who was not involved in the research, told Live Science in an email. "This study provides compelling evidence that, at least for geometric reasoning, the difference between humans and other primates is more quantitative than qualitative."

In other words, the study suggested that baboons and macaques don't lack the ability to reason about geometry. Instead, they just aren't as proficient at it as humans, meaning that humans didn't evolve a new unique skill in understanding geometry.

A geometric matching game

The researchers tested eight adult monkeys: four rhesus macaques (Macaca mulatta) and four olive baboons (Papio anubis). The olive baboons participated through the Primate Portal, a touch-screen system installed at Seneca Park Zoo in Rochester, New York. One baboon, Kalamata, was especially enthusiastic.

"Every day he came to the touch screen," Jialin Li, a doctoral student at Carnegie Mellon University and first author of the study, told Live Science. "He just sat there and worked for two hours, three hours straight, completing thousands of trials. That's just amazing."

The macaques participated separately at Carnegie Mellon University, having prior experience with matching tests in other experiments.

The researchers then compared the animals' performance with that of 58 U.S. preschoolers ages 3 to 6, and 79 adults from the Tsimané, an Indigenous farmer-forager society in Bolivia whose members received little formal education. A separate experiment in the larger project involving rotating shapes also included 21 U.S. adults.

In all of the study's cohorts, the participants played a game known as a match-to-sample task.

"[The participants] see a sample shape first," Li said. "For example, it's a square. Then they need to tap the square to make sure that they are looking at it. When they tap it, there will be two shape choices that come up: one on the left and one on the right. They need to choose which shape matches with the sample shape."

The researchers made the choice shapes half the area of the sample shape, thus preventing the participants from solving the task by simply matching overall size or pixel count. In another version of the test, they rotated the choice shapes, thereby forcing the participants to identify the underlying form despite its changed orientation.

Correct answers earned the monkeys fruit-flavored cereal pellets, preschoolers collected stickers that could later be exchanged for prizes, and adults received verbal feedback. Incorrect answers triggered a "bonk" sound and a short timeout from the game.

Despite their limited formal education, the adult group had little trouble with the game, but the monkeys and the children had to put considerable thought into their choices.

"We often think that this matching task will be super easy for humans," Li said. "But actually, young kids were struggling in completing the task in telling the shapes apart, which makes them more similar to monkeys."

Ultimately, the children and monkeys could find the matches, Cantlon said, but only after taking a long time to think about the problem.

The researchers then used computer models to investigate which visual properties best predicted participants' decisions. One model represented simple details, such as edges and lines. Another represented more complex information about a shape's overall form. A third encoded discrete geometric properties, such as equal sides, equal angles, symmetry and parallelism — an approach the researchers described as "symbolic."

According to Cantlon and Li, the term "symbolic" does not mean the monkeys were mentally applying rules such as "a square has four equal sides." Much of the apparent symbolic effect could be explained by the ability to recognize a shape regardless of its orientation, known as rotation invariance.

If abstract geometry depended on a uniquely human symbolic system, only the human participants would have shown evidence of using that thought process. Instead, both monkeys and humans appeared to rely on a mixture of complex visual information and symbolic-like features. Adult humans generally performed the best, followed by preschoolers and monkeys, but their results overlapped. This finding suggests that the differences were quantitative, meaning humans are simply better at the same underlying kind of geometric reasoning rather than possessing an entirely unique ability., Monkeys relied roughly three times more strongly on the symbolic model when the shapes were rotated than when they remained upright.

Brandon said one of the study's most intriguing findings is that what looks like uniquely human symbolic reasoning for understanding geometry may actually grow out of flexible, abstract ways of representing information that are shared by humans and other primates.

Ancient roots of geometry

The results do not mean that monkeys understand formal mathematics, Brannon cautioned. "Human mathematical reasoning extends far beyond recognizing geometric regularities — it includes language, formal proof, recursive reasoning and cultural transmission."

Rather, this study provides evidence that some of the building blocks of mathematical thought have deeper evolutionary roots than previously recognized, she said.

Giorgio Vallortigara, a professor of neuroscience at the University of Trento in Italy who was not involved in the study, agrees with Brannon and her colleagues' conclusions.

Vallortigara explained in an email to Live Science that previous studies have often focused on how animals understand the geometry of their surroundings, such as navigating spaces. What makes these findings different is that they show animals can also reason about the geometric properties of individual objects.

Comparing species can help scientists trace the origins of geometry before language or arbitrary symbols became involved, Vallortigara said. It may also reveal whether similar abilities depend on mechanisms inherited from a common ancestor or evolved independently in animals with different nervous systems.

Li and Cantlon are now breaking down shapes into components such as angles, side lengths and numbers of sides to identify which properties are the hardest for monkeys and humans to understand. Cantlon described the follow-up as "a deconstructed geometry task."

The research could also help educators understand the geometric intuitions children bring into the classroom, Cantlon said, allowing lessons to build upon those abilities rather than treating geometry as something learned entirely from scratch.

"Evolution rarely invents entirely new mechanisms from scratch," Brannon said. "More often, it refines, recombines and extends existing ones."

What do you know about chimpanzees and great apes? Test your smarts with our primate quiz!

An ecological "superspreader" event may be imminent as more than 1,500 ships continue to idle in the closed Strait of Hormuz, with the potential to cause serious impacts for human health and global marine ecosystems, scientists warn.

In a study published July 22 in the journal Biological Invasions, scientists explain how the hundreds of stranded commercial vessels sitting idle on both sides of the strait are being colonized by marine microbes, algae, seaweed, barnacles and other invertebrates. The problem is that once these ships start moving again, these organisms will be spread all around the world.

"The unprecedented scale and duration of this spring and summer mass lay-up of large commercial ships has created ideal conditions for a marine invasive species 'super-spreader' event," Mario Tamburri, a professor at the University of Maryland Center for Environmental Science and first author of the study, said in a statement.

The Iran War is already having devastating impacts around the world. After the U.S. and Israel launched strikes on Iran on Feb. 28, Tehran retaliated by restricting shipping traffic through the Strait of Hormuz ‪—‬ a critical shipping route that connects the Persian Gulf and the Gulf of Oman and facilitates the transport of 20% of the world's oil supply, according to the U.S. Energy Information Administration.

But the economic impacts of the waterway's prolonged closure are only part of the story.

While it's common for cargo ships to linger for a day or two at most ports, the study authors say these organisms — which are arriving from all over the world and are now mixing and spreading among the other stationary vessels — really begin to flourish after about 10 days of inactivity.

When ships are idle for longer than 10 days, these organisms start to colonize "aggressively" as the special coatings that protect ships from contamination start to work less effectively, the researchers write. And once these organisms are brought into new environments, they can wreak havoc on local ecosystems.

"Marine invasions are hard to predict but it is possible for several species to establish themselves in new habitats and with some causing significant environmental and economic impacts," Tamburri told Live Science in an email.

Tamburri pointed to the example of zebra mussels (Dreissena polymorpha) in the Great Lakes. The mollusks, which are native to Europe and Asia, are thought to have been introduced to the U.S. in the 1980s via water discharged from large European cargo ships, according to the U.S. Geological Survey.

The impacts of these invasive animals are widespread: They filter out algae that native species need for food and attach to native mussels, preventing them from moving, feeding or reproducing, according to the National Park Service (NPS). They also clog pipes and water supply systems, which cost millions of dollars to fix.

Each female zebra mussel can produce thousands of eggs, so once populations are established, there is "very little" that can be done to remove them, the NPS notes.

In addition to outcompeting native species for space and resources, invasive species can spread disease.

"One of the less perceptible concerns from biological invasions is the potential spread of infective stages of parasites and diseases that are either entrained within ship ballast tanks or associated with organisms attached to ship hulls," April Blakeslee, an associate professor of biology at East Carolina University, told Live Science in an email. Parasites and diseases introduced by ships could then spill over to native species, which could affect ecologically and/or commercially valuable species, or possibly pose concerns for human health, Blakeslee added.

In other words, these species could spread diseases with the potential to infect local wildlife and humans, as well as fisheries and aquaculture.

Tamburri said the areas most at risk are first ports of call with similar temperatures and salt levels to the Gulf region, particularly ports in India, Singapore, Greece, Spain, the Netherlands and several ports in the Middle East.

So what can be done to stop this "superspreading" event before it happens? According to the researchers, cleaning ships in the water before they leave the Gulf region could significantly reduce the spread of these organisms. Estimating the risks posed by specific ships before departure and setting up monitoring networks and early detection systems at high-risk ports may also limit the damage.

"While the human and economic consequences of events like the war in the Middle East will always remain the highest priority, ecological impacts cannot be overlooked," the researchers wrote.

Chinese researchers have revealed a new technology that could soon enable drones to charge mid-flight using high-powered lasers.

The scientists built a prototype of the system using a model of a drone and attached a receiver that works similarly to a solar cell. Fixed to the underside of the wing, the receiver successfully converted the energy from the laser beam into electricity to power the aircraft’s propellers.

The breakthrough was made by researchers at the Civil Aviation University of China and Tsinghua University, with details outlined in a new study published on 29 July in the journal Matter & Light.

"Previous studies largely focused on the materials or the device itself," study senior author Jianhua Han, a researcher at the Civil Aviation University of China, said in a statement. "We wanted to think beyond the laboratory, to how the system could actually be integrated into an aircraft, cooled during operation, and made compatible with flight. It isn’t just a materials science problem; it’s an engineering one."

Wirelessly charging drones

The receiver is what's known as a perovskite laser cell-thermoelectric (PLC-TE) tandem device optimized to turn laser light into electricity.

Perovskite is a highly efficient material used in cutting-edge solar cells, noteworthy for its crystal structure that allows it to capture more wavelengths of the light spectrum than silicon. For this reason, it’s prized as a future solar material, with some research indicating it could even be used to convert ambient indoor light into usable electricity.

When hit with a green laser, the receiver converted 38.49% of the light into electricity — well above the 34% peak results for perovskite-silicon tandem cells as recorded by the U.S. Department of Energy (DOE).

In initial testing, the researchers discovered an unwelcome side effect of using the laser: the drone was being heated to extreme temperatures, reducing its overall efficiency.

"When we tested the device under a high-power laser, the thermal camera showed temperatures of 80 to 90 degrees Celsius [176 to 194 degrees Fahrenheit]," said Han. "That was much higher than we expected and made us realise that heat buildup was a far more serious problem than we had imagined."

To combat this, the researchers introduced nanocrystals made from antimony triselenide — an abundant semiconductor material — into the PLC-TE design. This plays the role of a thermal barrier, preventing the device from releasing too much heat.

In addition to their cooling innovation, the constant airflow generated by the drone’s propeller helped further regulate the temperature of the receiver’s cool side.

Overcoming battery life barriers

"Imagine a future where drones inspecting forests, monitoring disasters, or delivering packages no longer need to land frequently to replace batteries,” said Han. "As drones take on longer missions, battery life has become one of the biggest barriers."

The researchers specifically identified reconnaissance, logistics, and disaster relief as key areas where drones powered by lasers could one day be used. But they also said more needs to be done to develop real-time tracking systems that precisely target the PLC-TE on in-flight drones before the system could be used in the wild.

Going forward, the researchers will test how the device functions on a real lightweight drone in outdoor conditions.

The promise of indefinite flight has made wireless power tests a focus for militaries around the world. If achieved, reconnaissance and weapons-carrying unmanned aerial vehicles (UAVs) could operate in radically different environments than those they are currently restricted to, with regular refuelling requirements.

For example, the most commonly used hand-launched unmanned aerial vehicle (UAV), the AeroVironment RQ-11 Raven, can fly for a maximum flight time of 60 to 90 minutes before needing to charge.

In June 2025, the U.S. Defense Advanced Research Projects Agency (DARPA) successfully beamed 800 watts of power over a distance of 5.3 miles (8.6 kilometers), as part of its Persistent Optical Wireless Energy Relay (POWER) program.

Private companies such as PowerLight Technologies, in collaboration with the U.S. Department of Defense, have said they could deliver kilowatts of energy to in-flight drones operating at altitudes of up to 5,000 feet (1,500 meters).

"Demon cavefish" have been discovered lurking in caverns beneath a contaminated U.S. Army base in Alabama, a new study has found.

Biologists have named the pale, eyeless creatures Demogorgonichthys arcanus, after the monstrous Demogorgons from Netflix's "Stranger Things" and the underworld demon of Greek mythology from which the Demogorgon name derives. They are likely among the rarest fishes in the world.

The find came as a shock to scientists because the cavefish's home, Bobcat Cave, has been extensively studied in recent decades. The subterranean system is part of U.S. Army site Redstone Arsenal, which was historically a center for chemical weapons production. Bobcat Cave is regularly subject to water quality monitoring and part of efforts to save endangered Alabama Cave Shrimp (Palaemonias alabamae), which also call the cave home.

In a new study, published July 6 in the journal Scientific Reports, researchers described the cavefish find as a "discovery in plain sight." Study lead author Matthew Niemiller, who directs the cave biology lab at The University of Alabama in Huntsville, encountered the cavefish by chance during a routine survey of Bobcat Cave's largest chamber, known as the Shrimp Room, in early 2025.

"I slipped in the mud at the back of the Shrimp Room and fell into a deeper pool," Niemiller told Live Science in an email. "During my graceful plummet, I disturbed a cavefish and crayfish underneath a rock ledge."

Niemiller quickly snapped photos of the animals using an underwater camera before silt clouded his view of them. It wasn't until several days later, when he checked the photos, that he noticed the cavefish looked different from southern cavefish (Typhlichthys subterraneus), a known species within the cave.

"The new cavefish had a pronounced hump behind the head, a longer, flatter snout, and unbranched fin rays," Niemiller said. "We returned a few days later, before a storm system forecasted to dump several inches of rain moved into the area. On the next trip, we confirmed that nearly half of the cavefish we observed were this new species."

Niemiller studied the cavefish with colleagues at Auburn University, The University of Alabama and Mississippi State University, with students performing much of the lab work. Genetic analysis revealed that demon cavefish didn't fit within any known cavefish group. Notably, demon cavefish carry unique disabling mutations for rhodopsin, a light-sensitive protein that would otherwise support dim light vision. Niemiller noted that this mattered for two reasons.

"First, it's a great example of 'use it or lose it' at the molecular level," he said. "In total darkness, vision is useless, so natural selection stops maintaining the gene, and mutations simply accumulate. Second, and more importantly, the specific way this fish's rhodopsin is broken is different from how it's broken in the related cavefish it lives alongside. That's strong evidence they lost their vision independently."

Demon cavefish and southern cavefish seemingly losing the ability to see independently is an example of how evolution can lead different species to converge on the same physical characteristics when they're suitable for an environment.

The conditions in Bobcat Cave have likely been influenced by the history of the military base above it. Redstone Arsenal made various chemical weapons during World War II. At the end of the war, vast quantities of chemical munitions were buried at the site, along with chemical weapons from overseas, like British mustard gas and nerve agents and other toxic weapons recovered from Nazi Germany. The site is the subject of ongoing investigations, clean-ups and storage.

Researchers have found that the cave contains elevated levels of trace metals compared to what would normally be found in such a habitat. However, Niemiller noted that the restricted-access status of the military installation does limit disturbance in the cave.

A bigger concern for the demon cavefish is that surface water connects to the cave's groundwater, so the life in the cave is also exposed to runoff, sediment and contaminants linked to the nearby city of Huntsville. As demon cavefish are, as far as we know, restricted to a single cave, they are very vulnerable to extinction.

The researchers concluded that demon cavefish would meet the criteria for becoming a "critically endangered" species, under the International Union for Conservation of Nature (IUCN) Red List — a framework for determining a species' conservation status. It's unknown how many demon cavefish live within the cave, and it's likely that many of them will be in places that are inaccessible to researchers.

"Like other cavefish, these animals probably spend much of their lives down in the water-filled aquifer below the cave, beyond where we can observe them, so any single survey is a snapshot, not a census," Niemiller said. "What we can say with some confidence is that it's known from just one cave system, it's rarely encountered, and by every measure we use, it qualifies as critically imperiled."

Fortunately for the cavefish, Bobcat Cave is already known for being a home for endangered Alabama Cave Shrimp. Since 1990, the cave has been a focus for water quality monitoring, shrimp surveys, and other biological investigations that should also help the newfound species.

"What protects the shrimp's water protects the fish's water too," Niemiller said.

July’s full Buck Moon, the second full moon of summer in the Northern Hemisphere, will turn full on Wednesday (July 29). It will be the final full moon before a flurry of solar and lunar activity — notably, a total solar eclipse caused by the new moon on August 12, and a partial lunar eclipse during the following full moon on August 28.

Named for the new antlers that emerge from male deer during summer, July’s full moon is also known as the Thunder Moon and Hay Moon, according to Time and Date. The Anishinaabeg people call it Miin Giizis, or Berry Moon, according to the Center for Native American Studies.

The Buck Moon will be at its fullest at 10:37 a.m. EDT on Wednesday — however, it will also look bright and full on Tuesday and Thursday night. From North America, the best time to see it will be at moonrise in the southeast during dusk on Wednesday evening. The exact time of moonrise will depend on your location. A full moon looks most dramatic as it first appears above the eastern horizon shortly after sunset, with Rayleigh scattering making it loom orange — the same light-scattering phenomenon that makes the sky blue and sunsets red.

July's full moon is one of the lowest full moons of the year as seen from the Northern Hemisphere because it occurs relatively soon after the June solstice. A full moon always sits opposite the sun, so the path of July's full moon mirrors the sun's path in February.

You can easily enjoy the full moon with the naked eye, but a good backyard telescope or pair of stargazing binoculars can help you zoom in on famous structures, such as craters and Apollo landing sites. And if you want to take stunning photos of the moon, here’s everything you need to know.

Two weeks after theBuck Moon, the new moon will slide directly between Earth and the sun, causing a total solar eclipse. Observers along a narrow path of totality in eastern Greenland, western Iceland and northern Spain will see the moon block the sun for a few minutes, revealing the solar corona.

A deep partial solar eclipse will be visible across Europe, with a small partial solar eclipse observed over Canada and the northeastern U.S.. The largest eclipse in Canada will be 93% in northeastern Nunavut, while northeastern Maine in the U.S. will see 29% of the sun covered by the moon. Solar eclipse glasses must be worn at all times to safely view the partial phases.

The next full moon, the Sturgeon Moon, will rise on August 27 and be partially eclipsed by Earth overnight. More than 96% of the moon will pass into Earth's shadow as seen from Europe, Africa, North America and South America.

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

A powerful earthquake struck southwestern Japan Tuesday afternoon local time, collapsing part of a shopping mall, toppling a stone wall at the centuries-old Kumamoto Castle, and sending more than 150,000 people to evacuation shelters, the BBC reported.

The quake, which the U.S. Geological Survey (USGS) measured as a magnitude 6.8, hit at 4:27 p.m. local time near Kumamoto, a city of more than 700,000 people located on the island of Kyushu in southern Japan.

Thousands of homes lost power, and roads buckled across the region. The second floor of a shopping center collapsed, trapping shoppers inside, according to the BBC report; some of these people were evacuated and later hospitalized. A brief tsunami warning was issued and lifted within an hour.

The USGS measurement is different from the magnitude 7.1 reported by the Japan Meteorological Agency, "primarily because the agencies are reporting different magnitude types," the USGS reported. While Japan is looking at local magnitude, the USGS measured the moment magnitude, which is derived from the physical size of the fault rupture and gives the "most reliable estimate of earthquake size" for large earthquakes, since local-magnitude scales can lose accuracy once a rupture grows big enough, the USGS reported.

These measurements are helpful, as "different magnitude types capture different characteristics of earthquake source processes," the USGS noted. Local magnitude, for example, reflects how strongly the ground shook nearby, while moment magnitude reflects the total energy released across the fault.

Why this quake is scientifically interesting

Japan sits atop one of the most active plate boundaries on Earth, where the Philippine Sea Plate dives beneath the Eurasia Plate. That process, known as subduction, is responsible for the massive, tsunami-generating earthquakes that periodically strike offshore Japan, and it's been studied intensively for decades.

But Tuesday's earthquake didn't occur at the boundary itself. Instead, the rupture happened within the Eurasia Plate, more than 60 miles (100 kilometers) inland from where the plates meet, Jeffrey Park, a theoretical seismologist at Yale University, told Live Science. Roughly 90% of earthquakes happen at plate boundaries, where the constant grinding of two plates builds up stress until a fault gives way. Quakes that strike farther inside a plate — sometimes called intraplate earthquakes — are rarer and less understood, though scientists suspect that stress transmitted through the plate can reactivate old, dormant faults far from the boundary that produced it.

According to Park, the fault in Tuesday's earthquake moved in a way that suggests the plate tore horizontally as it was twisted by subduction occurring at an angle.

The USGS describes this event as shallow strike-slip faulting: the two sides of the fracture slid past each other horizontally, rather than one side thrusting up and over the other. This faulting style, combined with the shallow depth of just 6 miles (10 kilometers) down, points to the same type of rupture behind Kyushu’s deadly 2016 Kumamoto earthquake sequence.

That inland location is also why the quake didn't generate a damaging tsunami, despite the brief precautionary warning. Tsunamis are produced when a big event ‪—‬ such as an earthquake, volcanic eruption or landslide ‪—‬ displaces water; the force from that displacement then propagates as a wave.

Tuesday's rupture stayed entirely on land, so it never pushed the seafloor up the way offshore quakes do. That's why the tsunami risk stayed low, even with the brief precautionary warning. Still, an inland quake isn't automatically off the hook: if the shaking triggers a landslide that spills into the sea, that alone can generate a tsunami.

The depth mattered just as much as the location. The quake was shallow enough to concentrate its energy near the surface, which Park said explains the structural damage.

"Because it is shallow it will cause more structural damage than a similar-sized event that might occur deeper and offshore," he told Live Science in an email.

Earthquake country

Several earthquakes have already clustered in the area, and numerous aftershocks are expected over the coming days. Japan experiences roughly 1,500 earthquakes annually, making it one of the most seismically active countries on the planet — a byproduct of sitting at the junction of several tectonic plates.

To protect itself, Japan has spent decades — and learned from painful lessons from disasters like the 2011 Tohoku earthquake and tsunami — engineering a response system built for exactly this scenario.

Bullet trains are programmed to halt automatically the instant seismic sensors detect a major earthquake, a safeguard Park pointed to as a defining feature of the country's earthquake readiness. That automatic shutdown extends to other transit and utility systems, part of a broader early-warning network that alerts the public within seconds of a quake's detection, giving people crucial time to take cover before shaking arrives.

Japan's investment in its infrastructure may help to explain why, even after a magnitude 7 event near a city of 700,000, Japan's death toll and damage have historically been far lower than those from comparable quakes elsewhere in the world.

Search-and-rescue efforts are continuing in Kumamoto, with CNN reporting that between 20 and 30 employees remained unaccounted for at the Aeon Mall in Kashima Town, where the building’s second floor had collapsed. Firefighters were also working to reach the site and contain nearby fires.

In a string of a dozen small galaxies hung in the sky like a row of cosmic fairy lights, astronomers have discovered a small, ghostly galaxy without any dark matter. The rare discovery offers additional evidence that violent galactic collisions can knock this invisible substance loose from visible matter.

Dark matter acts like cosmic glue, accumulating in "halos" in which galaxies form. It makes up about 85% of all the matter in the cosmos, meaning all the stars and other celestial objects we see account for a small fraction of the universe's mass. And as astronomer Vera Rubin observed, despite its invisible nature, dark matter seems essential to explain the apparent movement of stars around their galactic centers.

Yet in a study published June 16 in The Astrophysical Journal, astronomers report that a dwarf galaxy called DF9 may be devoid of dark matter, joining a couple of other apparently dark-matter-devoid dwarfs (DF2 and DF4) previously discovered in the same string of tiny, faint galaxies.

"The most surprising aspect is that this finding indicates that an entire trail of galaxies including DF2, DF4, and DF9 formed together in an extreme event producing galaxies not alike any we've ever seen before — the first of its kind," Michael Keim, an astrophysicist at Yale's Graduate School of Arts and Sciences and the study's first author, told Live Science via email. "As a result, they have a ghostly appearance, bright clusters of stars, and a lack of dark matter."

Following a trail of galactic crumbs

To study DF9, the researchers used the Keck Cosmic Web Imager at the W. M. Keck Observatory atop the dormant Mauna Kea volcano in Hawaii. The dwarf galaxy is situated within a long trail of a dozen similarly small, diffuse galaxies in the NGC 1052 field, nearly 70 light-years from Earth.

To calculate the mass of DF9, the researchers measured the motion of its stars by analyzing changes in their wavelengths. The analysis revealed that DF9 has a measly mass of approximately 100 million suns, which is consistent with its visible mass in stars. If it contained the expected amount of dark matter, it would be exponentially heavier, harboring a mass of more than 10 billion suns, the researchers said in a statement.

As revealed over the past decade, at least two of DF9’s nearby galactic siblings also appear to lack dark matter.

"If DF2, DF4, and DF9 were the only galaxies known, one would not conclude there is any need for dark matter," the researchers wrote in the paper. These three galaxies do not display a mass-based discrepancy based on their visible and invisible matter; their mass, determined by the gravitational motion of their stars, matches their mass as measured by the light emitted from these same stars.

But this is hardly typical among most observed galaxies, especially the tiniest ones. Counterintuitively, low-mass dwarf galaxies such as these often have the highest fraction of dark matter. Because they are not as massive, they have lower escape velocities, allowing supernovas and other "feedback mechanisms," like intense black hole winds, to eject their gas more easily. This mass expulsion typically results in dark matter halos around galaxies that are 100 times more massive than all of a dwarf galaxy's stars, the researchers said.

Dark matter deficiency is linked to a violent past

The team likened this lineup of dwarf galaxies to a miniature version of the Bullet Cluster, located nearly 4 billion light-years from Earth. The collision of two galaxy clusters that created the Bullet Cluster is considered the most energetic event known since the Big Bang, astronomers say, and the massive mashup is responsible for separating the system's gas from its dark matter.

Violent galaxy mergers are widespread in space, suggesting such galaxies without dark matter also may be more common throughout the cosmos than once thought.

"The Bullet Dwarf event in which DF9 is thought to have formed is named after the famous Bullet Cluster wherein the gas of two entire clusters of galaxies was separated out in a similar manner as this 'Bullet Dwarf' collision, so indeed this can occur at much larger scales," Keim explained via email. "But collisions between giant clusters are far less frequent than collisions of individual galaxies."

Yet being able to glimpse DF9 and its linearly laid-out counterparts still required an element of fortune. "High-speed collisions are, nevertheless, somewhat rare," Keim added. "DF9 is 67 million light years away from Earth; based on cosmological simulations, we would expect just 7 or so similar collisions to have occurred within that distance."

Additionally, celestial bodies are always in flux, so finding galaxies devoid of dark matter is difficult for other reasons. For example, they may exist in dense regions, where they are harder to view through the obscuring dust, gas and starlight surrounding them. Or, they may merge with other galaxies that do have dark matter.

The strange separation between dark matter and visible matter in the galaxies of the NGC 1052 field warrants further study, the researchers said. Finding any leftover gas from the collision would provide the "smoking gun" evidence for the collisional origin of this faint string of galaxies.

The astronomers are conducting follow-ups with other observatories, including the new MOTHRA facility, the "world's largest all-lens telescope," which is under construction in Chile. With an array of 1,140 telephoto lenses, "its line mapping sensitivity on large scales — like that of the trail — will be at least an order of magnitude deeper than any other facility," Keim added.

Scientists may have found a way to rejuvenate key cells that help rebuild muscle in the body and thus preserve muscle into old age, they report in a new mouse study.

It is "really exciting stuff," Matthew Krause, a muscle physiologist at the University of Windsor in Ontario, said of the results. It could have clinical applications down the road if shown to work in humans, as well, added Krause, who was not involved in the research.

The body loses muscle with age and with chronic conditions that compromise people's mobility. To find a potential treatment for this muscle atrophy, the scientists behind the new study looked to "satellite cells." These stem cells are located around skeletal muscle fibers and play an important role in muscle regeneration.

Muscles incur microscopic damage with use, and this damage calls satellite cells into action. They proliferate to rebuild muscle fibers, by either merging into the torn muscle cells or forming new muscle cells. With age, satellite cells activate less efficiently and muscles become weak. But the new study, published July 24 in the journal Scientific Reports, suggests that it may be possible to rescue satellite cells from dormancy.

When muscles tear during exercise, a protein called hepatocyte growth factor (HGF) gets released. This is the signal that binds to receptors on satellite cells and activates them. Previously, studies from the same team showed that HGF works less well in old lab mice because its structure is chemically altered by a compound called peroxynitrite, and this makes it harder for HGF to plug into its receptor on satellite cells. This chemical alteration is known as nitration.

Peroxynitrite is produced through the reaction of unstable nitrogen and oxygen molecules, called radicals, said study co-author Ryuichi Tatsumi, a muscle physiologist at Kyushu University in Japan. These radicals are produced during normal metabolism, but their levels increase with age, he explained.

As a result, satellite cells cannot be activated efficiently to trigger muscle growth, even if the amount of HGF itself does not decline. Tatsumi and colleagues showed this in a previous study in rats.

In the new study, the scientists tested two compounds to see if they could counter this effect in lab mice. They used an experimental setup in which mice couldn't use their muscles as normal, so they weakened; such muscle disuse is known to increase HGF nitration around muscle cells.

Both of the tested compounds are known to protect proteins from damage caused by highly reactive chemicals by intercepting the reaction before it can take place. In experiments, the team treated HGF with each compound before exposing it to peroxynitrite. They found that, compared with untreated HGF, HGF treated with either compound showed substantially lower levels of nitration. This preserved its ability to activate satellite cells grown in lab dishes.

At high concentrations, one of the compounds — lipoic acid trisulfide (LASSS) — not only prevented nitration but also markedly increased HGF's ability to plug into its receptor. That suggests LASSS may chemically modify HGF in a way that could boost its effects.

To see if these observations carried over to living animals, the researchers gave lab mice LASSS in their drinking water. Although these were young mice, they were prevented from bearing weight on their hind limbs for five days, so they experienced short-term muscle disuse. Compared with untreated animals, the mice given LASSS had substantially lower HGF nitration around their muscle cells.

It's "pretty remarkable" that providing LASSS by mouth was sufficient to produce this effect, Krause said. He noted, however, that the researchers did not measure muscle atrophy or try administering LASSS to old mice to see the effects on the muscle. Longer experiments would be needed to observe those changes, he told Live Science.

The compound could also be tested in other forms of muscle wasting, Krause suggested. For example, severe chronic diseases like cancer can cause cachexia, a wasting syndrome marked by dramatic weight and muscle loss.

In general, protein nitration has been linked to several age-related disorders, including Alzheimer's disease, in which nitrated proteins accumulate in the brain. Understanding how to protect proteins from this kind of chemical damage could have implications beyond muscle biology, Tatsumi said.

However, further studies are still needed to assess the effectiveness and safety of LASSS in older animals. Experiments involving aging animals are expensive and can take a lot of time, Tatsumi said, but he is optimistic that this understanding will help address a range of age-related disorders with this same underlying biology.

"That is our big wish," he told Live Science. "I think, in the near future, we can do that."