SPHEREx: Mapping the Entire Sky in Infrared for Unprecedented Cosmic Insights

NASA’s SPHEREx (Spectrophotometer for the Exploration of the History of the Universe, Era of Reionization, and Ice) space telescope has successfully created the first comprehensive 102-color infrared map of the entire sky, utilizing observations collected from May to December 2025. While these 102 infrared wavelengths are invisible to the human eye, their widespread presence in the universe enables scientists to tackle significant questions, such as understanding monumental events on Earth. The milliseconds following the Big Bang profoundly influenced the 3D distribution of billions of galaxies. Furthermore, this invaluable data will aid in studying the evolution of galaxies over the universe’s 13.8 billion-year history and analyzing the distribution of essential life ingredients within our Milky Way galaxy.



This infrared image from SPHEREx features color emissions from stars (blue, green, and white), hot hydrogen gas (blue), and cosmic dust (red). Image credit: NASA/JPL-Caltech.

The Earth completes approximately 14.5 rotations in a single day. Spherex travels from north to south, crossing over both poles.

Each day, SPHEREx captures around 3,600 images along a defined circular path in the sky. As time progresses and the planets orbit the sun, SPHEREx’s observational field shifts accordingly.

After six months, the observatory managed to explore the cosmos, capturing a full 360 degrees of the sky.

NASA’s Jet Propulsion Laboratory in Southern California oversees this mission, which commenced sky mapping in May and achieved its inaugural all-sky mosaic in December.

Over its two-year primary mission, SPHEREx plans to conduct three additional all-sky scans, merging these maps to enhance measurement sensitivity.

Dr. Sean Domagal Goldman, director of the Astrophysics Division at NASA Headquarters, remarked, “It’s astounding that SPHEREx has gathered such a wealth of data in just six months. This information, combined with data from other missions, provides deeper insights into the universe.”

“We essentially have 102 new maps of the entire sky, each featuring distinct wavelengths and delivering unique information about celestial objects.”

“Astronomers will find valuable insights here, as NASA’s mission will facilitate answers to fundamental questions regarding the universe’s beginnings and its evolution, ultimately shedding light on our position within it.”

“SPHEREx is a medium-sized astrophysics mission delivering groundbreaking science,” stated Dave Gallagher, director of NASA’s Jet Propulsion Laboratory.

“This remarkable project exemplifies how bold ideas can transform into reality, unlocking immense potential for groundbreaking discoveries.”

Every one of the 102 colors detected by SPHEREx corresponds to a wavelength of infrared light, each of which conveys unique information about galaxies, stars, planet-forming regions, and other cosmic phenomena.

For instance, dense dust clouds in our galaxy, where stars and planets are born, shine brightly at specific wavelengths but remain completely invisible at others.

This separation of light into its component wavelengths is known as spectroscopy.

While prior missions, including NASA’s Wide-Field Infrared Surveyor, have mapped the entire sky, none have achieved the same diversity of colors as SPHEREx.

In contrast, the NASA/ESA/CSA James Webb Space Telescope can perform spectroscopy at significantly longer wavelengths than SPHEREx, but its field of view is thousands of times smaller.

The diversity of colors combined with a wide observational field is what renders SPHEREx exceptionally powerful.

“The true superpower of SPHEREx lies in its ability to capture the entire sky in 102 colors approximately every six months,” declared SPHEREx Project Manager Beth Fabinski, Ph.D., of NASA’s Jet Propulsion Laboratory.

“It’s incredible how much information we can collect in a short timeframe.”

“This makes us akin to telescopic mantis shrimps, equipped with an extraordinary polychromatic visual detection system capable of observing a vast area around us.”

Source: www.sci.news

Study Reveals How Dinosaurs’ Free-Range Parenting Transformed the Mesozoic Era

University of Maryland paleontologist Thomas R. Holtz Jr. has explored how dinosaurs adapted to their ancient environments and the differences between those worlds and our own for decades. His recent research suggests that crucial factors may have been overlooked in comparing ancient dinosaurs with modern mammals.

Some sauropod dinosaurs, Alamosaurus sanjuanensis, formed herds divided by age. Image credit: DiBgd.

“Many people view dinosaurs as the Mesozoic equivalent of mammals since both groups were the dominant land animals of their respective eras,” says Holtz.

“However, a crucial difference relates to their reproductive and child-rearing strategies, which scientists haven’t fully considered when comparing these worlds.”

“The methods by which animals raise their young significantly influence their ecosystems. Understanding these differences can help scientists reevaluate ecological diversity,” he explains.

“Young mammals often receive extensive care from their mothers until they are nearly fully grown.”

“In essence, mammal offspring fulfill similar ecological roles as their parents; they consume similar food and interact within the same environment because adults handle most of the responsibilities.”

“You could say mammals have ‘helicopter’ parents—particularly helicopter mothers,” he continues.

“For example, mother tigers continue to hunt for cubs that are nearly their size.”

“Even young elephants, among the largest animals in the Serengeti at birth, rely on their mothers for years.”

“Humans exhibit similar behavior, caring for our children until they reach adulthood.”

“Conversely, dinosaurs exhibited different parenting behaviors. They offered some parental care, but their young were relatively independent.”

“After a short period, from a few months to a year, young dinosaurs left their parents to roam independently, often cautious of one another.”

Dr. Holtz notes that adult crocodiles, closely related to dinosaurs, demonstrate a similar trend.

Crocodiles guard their nests and protect their young for a limited duration; however, within a few months, the young disperse and lead independent lives, taking years to reach adulthood.

“Dinosaurs could be likened to ‘latchkey kids,'” Holtz states.

“Fossil evidence shows that juvenile skeletons were often found together, with no adults nearby.”

“These juveniles congregated in groups of similar ages, learning to feed themselves and fend for their safety.”

This parenting style suited the fact that dinosaurs laid eggs and produced relatively large chicks at once.

By producing multiple offspring at a time and reproducing more frequently than mammals, dinosaurs increased the chances of their lineage’s survival without significant resource investment.

“The key takeaway is that this early separation between parents and offspring, alongside size differences, likely had significant ecological implications,” Holtz noted.

“The dietary needs of dinosaurs shifted as they matured, as did their vulnerabilities to predators and their mobility.”

“Even though adult and juvenile dinosaurs belong to the same biological species, they occupy distinctly different ecological niches.”

“Therefore, they can be regarded as different ‘functional species.’

For instance, a juvenile Brachiosaurus, comparable in size to a sheep, couldn’t access food 10 meters above ground like its adult counterparts.

Juveniles faced different predators, feeding in different locations and avoiding fully grown adults.

As young Brachiosaurus grow from dog-sized to horse-sized to giraffe-sized, their ecological roles evolve significantly.

“This understanding has transformed how scientists perceive ecological diversity,” Holtz emphasized.

Typically, scientists argue that modern mammals inhabit more diverse ecosystems because of the coexistence of varied species.

However, if young dinosaurs are counted as separate functional species and their numbers recalculated, the total functional species in dinosaur fossil assemblages likely exceeds that of mammalian fossil assemblages.

How did ancient ecosystems accommodate all these functional roles? Dr. Holtz proposes two potential explanations.

First, the Mesozoic era featured unique environmental conditions, such as warmer temperatures and elevated carbon dioxide levels.

These factors likely enhanced plant productivity, generating more food energy to sustain larger populations.

Secondly, dinosaurs may have had lower metabolic rates than similarly sized mammals, demanding less food for survival.

“Our world might actually be less productive in terms of plant resources than the age of dinosaurs,” claims Holtz.

“A more robust food chain could support greater functional diversity.”

“If dinosaurs’ physiological demands were lower, their ecosystems might have accommodated far more functional species than found in mammalian systems.”

Dr. Holtz emphasizes that his theory doesn’t necessarily imply that dinosaur ecosystems were vastly more diverse than those of mammals, but rather that diversity may have existed in forms that have yet to be identified by scientists.

He intends to further explore similar patterns within the context of dinosaur functional diversity across different life stages to gain deeper insights into their world and its evolution into our contemporary ecosystem.

“We shouldn’t merely consider dinosaurs as scaled and feathered versions of mammals,” Holtz concludes.

“They are remarkable creatures in their own right, and the full scope of their existence is still being uncovered.”

This research will be detailed in Holtz’s paper, set to appear in the Italian Journal of Geosciences.

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Thomas R. Holtz Jr. et al. 2026. Raising Babies: A Preliminary Investigation into Ontogenetic Niche Partitioning in Dinosaurs and Long-term Maternal Care in Mammals within Their Ecosystems. Italian Journal of Geosciences 145; doi: 10.3301/IJG.2026.09

Source: www.sci.news

Scientists Uncover Largest Protoplanetary Disk Ever Detected Around Young Star

IRAS 23077+6707: A Turbulent Protoplanetary Disk – Located approximately 1,000 light-years away, this young star exhibits an unexpectedly chaotic and turbulent surrounding protoplanetary disk, with material fragments extending farther than what astronomers have previously observed in similar systems. For more details, check the study here.



This Hubble image showcases the protoplanetary disk surrounding IRAS 23077+6707. Image credit: NASA / ESA / STScI / K. Monsch, CfA / J. DePasquale, STScI.

Protoplanetary disks, rich in dust and gas, form around young stars and serve as primary locations for planet formation.

The disk surrounding IRAS 23077+6707 spans approximately 644 billion km (400 billion miles), making it about 40 times the diameter of our solar system, reaching to the outer Kuiper belt.

This vast disk obscures the star, which scientists suggest could be a massive star or potentially a binary star system.

Not only is this disk the largest known for planet formation, but its unique characteristics also make it exceptionally rare.

“It’s uncommon to capture such fine detail in protoplanetary disks. The new Hubble images suggest that planetary nurseries might be much more dynamic and chaotic than we previously thought,” explained Dr. Christina Monsch, an astronomer at Harvard University and the Smithsonian Center for Astrophysics.

“Observing this disk nearly head-on reveals its delicate upper layers and asymmetrical features,” she added.

Both the NASA/ESA Hubble Space Telescope and the NASA/ESA/CSA James Webb Space Telescope have glimpsed similar structures, but IRAS 23077+6707 allows for unmatched visibility of its substructure in visible light.

This unique perspective makes it an exceptional laboratory for studying planet formation and the environments in which it occurs.

Edge-on, these disks resemble hamburgers, with bright upper and lower layers of glowing dust and gas, separated by a dark central lane.

In addition to its significant height, the new images reveal that vertical filament-like structures only appear on one side of the disk, indicating an uneven distribution of material.

“We were astonished by how asymmetric this disk appeared,” noted Dr. Joshua Bennett Lovell from the Harvard University & Smithsonian Center for Astrophysics.

“Hubble provides us with an exceptional view of the chaotic processes involved in the formation of disks and new planets. This process remains poorly understood, but these insights allow for fresh study opportunities.”

All planetary systems originate from a disk of gas and dust surrounding young stars. Over time, gas is absorbed by the star while planets form from the remaining material.

IRAS 23077+6707 might act as an extended analog to the early Solar System, with an estimated disk mass between 10 to 30 times that of Jupiter, providing sufficient material for multiple gas giant planets.

This and other discoveries make IRAS 23077+6707 an extraordinary case for examining planetary system formation.

“Theoretically, IRAS 23077+6707 could support a vast planetary system,” Dr. Monch stated.

“While planet formation may differ in such expansive conditions, the fundamental processes are likely akin to those in smaller systems.”

“At this point, we have more questions than answers, but these new images serve as a valuable foundation for understanding how planets evolve in diverse environments.”

Findings are set to be published in the Astrophysical Journal and can be accessed here.

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Christina Monche et al. 2025. Hubble reveals the complex multiscale structure of the edge-on protoplanetary disk IRAS 23077+6707. APJ in press. arXiv: 2510.11819

Source: www.sci.news

Ancient DNA Study Uncovers ‘Beach-Headed Woman’ from Southern England: New Insights into Early History

The skeletal remains of the individual known as ‘Beachy Head Woman’ were rediscovered in 2012 within the collection of Eastbourne Town Hall. Since then, her story has garnered significant public interest. Radiocarbon dating reveals that she lived between 129 and 311 AD during the Roman occupation of Britain. Over the last decade, researchers have sought to uncover her geographic origins and ancestry. Initially believed to originate from sub-Saharan Africa or the Mediterranean, groundbreaking DNA research now indicates she shares strong genetic connections with the local population of Roman-occupied Britain and modern-day Britons.



A depiction of Beachy Head Woman’s face. Image credit: Face Lab, Liverpool John Moores University.

The journey of Beachy Head Woman began with her rediscovery in 2012, although uncertainty still surrounds her life. Radiocarbon dating placed her death between 129 and 311 AD, during the Roman occupation of Britain.

Analysis of her remains suggests she was aged between 18 and 25 at the time of death and stood just over 1.5 meters tall. A healed leg wound implies she endured a serious but non-fatal injury during her life.

Dietary analysis of her bones indicates a high seafood diet, revealing insights into her lifestyle.

“Using advanced DNA technology, we have made significant strides in uncovering the origins of this individual,” stated researcher Dr. William Marsh from the Natural History Museum in London.

“Our findings show that her genetic ancestry is most closely aligned with other individuals from the local population of Roman Britain,” he added.

The Beachy Head Woman’s remains were unearthed from a collection at Eastbourne Town Hall. Initial findings indicated that her skeleton was discovered at Beachy Head, a nearby geographic landmark, during the 1950s, though details of the excavation remain elusive.

Interest in Beachy Head Woman intensified when initial morphometric analyses suggested potential sub-Saharan African origins. This captivating narrative was exhibited at Eastbourne Museum, capturing widespread media attention.

In 2017, unpublished DNA findings implied a Mediterranean origin, possibly from Cyprus, rather than Africa. However, these conclusions are drawn from limited data, leaving many questions about Beachy Head Woman’s life unanswered.

“As our scientific knowledge continues to expand, it is our mission as researchers to seek further answers,” commented Dr. Selina Brace, also from the Natural History Museum in London.

“Thanks to technological advancements over the past decade since Beachy Head Woman’s reemergence, we are thrilled to share new comprehensive data and insights into her life,” she concluded.

For more details, you can refer to the team’s paper published this month in the Archaeology Journal.

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Andy Walton et al. Beachy Head Woman: Uncovering her origins using multi-proxy anthropological and biomolecular approaches. Archaeology Journal, published online on December 17, 2025. doi: 10.1016/j.jas.2025.106445

Source: www.sci.news

Unlock Your Creativity: Tips to Enhance Your Life and Well-Being

Fotografia Inc./Getty Images

To lead longer, healthier, and happier lives, we often hear advice like reducing sugar, exercising, quitting smoking, eating vegetables, taking supplements, managing stress, and getting quality sleep. However, one fun health tip remains overlooked: engaging in the arts.

Recent decades have highlighted the positive impact of creativity on overall health. Global initiatives are integrating arts into healthcare, showing remarkable outcomes: from music reducing the need for sedatives during surgeries to dance programs aiding Parkinson’s patients in walking.

Art isn’t just for illness recovery. Crafting, singing, acting, dancing, reading, writing, and painting promote well-being in our daily lives, regardless of our health concerns. In my upcoming book, Art Cure, I assert these activities qualify as “health behaviors,” akin to exercise, nutrition, and sleep. Discover how to incorporate more art into your life starting in 2026.

As an epidemiologist, analyzing cohort studies is part of my routine. These extensive datasets reveal the long-term benefits of art engagement on various health outcomes, collected from diverse populations worldwide.

The findings are compelling. Regular art participants report greater happiness and life satisfaction. Children engaged in the arts are less likely to face depression as they enter adolescence. Additionally, older adults attending cultural events significantly reduce their risk of developing depression over the next few years, as highlighted in this research: The risk of depression is nearly halved.

You may question whether art engagement impacts health independently from wealth or overall lifestyle. Advanced statistical methods account for such variables, including genetics and early life experiences, ensuring valid results still support the link between art and health.

These benefits extend beyond psychological health; children involved in musical activities develop better social skills as they transition to schooling. Conversely, fewer youths participate in artistic endeavors, increasing the risk of anti-social behavior. Furthermore, seniors attending cultural events have been shown to be 32% less likely to feel lonely after a decade.

Live Events: A Path to Enhanced Creativity

Sean Gardner/Getty Images

The positive outcomes intensify with age. My research team at University College London analyzed data from around 100,000 individuals across 16 countries, finding that hobbies like gardening, baking, sewing, and journaling promote: Self-reported health improvements as we age. Engaging in these activities yields benefits such as enhanced balance, lower pain levels, improved sleep quality, better cognitive function, reduced frailty, and a lower risk of chronic diseases like diabetes. In fact, many studies reveal those involved in the arts could live longer compared to their less-engaged counterparts.

How do these surprising health benefits manifest? Psychological, social, and behavioral factors contribute, but intriguing biological mechanisms are emerging. Studies indicate regular art participants show lower blood pressure, heart rates, cholesterol levels, reduced inflammation, improved immune function, and lower body mass index.

Recent advancements in measuring biological age allow scientists to explore how healthy habits influence our aging process. Research combining data on cardiovascular, respiratory, circulatory health, and gene expression patterns suggests that creatively engaging might keep us biologically younger. Individuals participating in dance, music, or visual arts often demonstrate more youthful brain characteristics.

It’s essential to clarify that engaging with art isn’t a cure-all. Factors like accessibility and misconceptions about its health benefits can limit participation. Nonetheless, evidence consistently indicates that dedicating time to enjoyable, creative activities is a valuable health investment for this year. Furthermore, promoting art is also altruistic; economists suggest that arts activities deliver over £18.6 billion in societal value annually.


Artistic activities involving screens often serve as the ultra-processed foods of the art domain.

So, how can we all enhance our artistic consumption in 2026? This question is explored throughout my upcoming book, Art Cure, which offers daily strategies for leveraging art to meet your health objectives. Think about art as you do food: don’t binge on it, as quick fixes yield short-lived benefits. Instead, find your equivalent to “5 servings a day” of fruits and vegetables. Dedicate just 10 minutes daily to creative writing or 15 minutes each evening to a craft. Effortlessly swap out activities; trade your dinner date for a live performance, replace gym workouts with dance classes, and read poetry on your commute instead of news articles.

Diversity in your artistic experiences is crucial; explore various creative forms to maximize health benefits. Each unique encounter offers different sensory joys and health advantages. Aim for a moderate level of novelty—something outside your norm but likely enjoyable. Make your artistic engagement genuine rather than virtual; screen-based activities can dilute the essence of art.

Lastly, be a mindful creator. In our fast-paced lives, it’s tempting to think of art as a quick solution. However, art’s beauty lies in its complexity and individuality. These rich and dynamic experiences should be afforded the time they deserve in our lives. Ultimately, art not only enhances our well-being but also evokes feelings of elation and upliftment, proving it is undeniably good for us.

This article is part of a series on simple changes you can implement to enhance your health in the coming year.
Read the full series here

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Source: www.newscientist.com

Alpine Communities Confront Uncertain Future Following 2025 Glacier Collapse

Landslide in Bratten, Switzerland

Bratten, Switzerland: Landslide Devastation in May 2025

Alexandre Agrusti/AFP via Getty Images

In May 2025, the picturesque village of Bratten in the Swiss Alps was tragically destroyed by a massive glacier collapse. Thanks to meticulous monitoring, nearly all residents were safely evacuated.

The initial warning signs emerged on May 14, when the Swiss avalanche warning service reported a minor rockfall in the area. Trained observers, who typically have other full-time roles, were on alert for signs of potential danger.

Detailed investigations followed, utilizing images from cameras installed on the glacier after a previous avalanche in the 1990s. “The angles provided crucial insights into shifts in the mountain,” explained Mylène Jacquemart from ETH Zurich, Switzerland.

On May 18 and 19, 300 residents were evacuated, but one individual, a 64-year-old man, resisted leaving his home.

On May 28, the situation escalated as the glacier suffered a catastrophic collapse. “This was an enormous rock avalanche,” Jacquemart stated.

The glacier had accumulated debris from previous years, and when a rockfall occurred, it triggered the collapse of 3 million cubic meters of ice, along with 6 million cubic meters of rock, ravaging a significant portion of the village. Regrettably, the man who opted to remain was killed.

Contrary to some media reports suggesting advanced surveillance technology monitored the glacier, Jacquemart clarified, “The observer’s office didn’t have an elaborate alarm system; a simple red light indicated a problem.”

However, Jacquemart emphasized that Switzerland’s monitoring system ensures effective communication and distinct accountability regarding evacuation decisions.

Satellite Image of the Landslide Area on May 30

European Union, Copernicus Sentinel 2 imagery

What contributed to this disaster? The likelihood of rockfalls exacerbated by climate change is a pressing concern. As global warming causes Alpine glaciers to retreat, the incidence of rockfalls is on the rise. Switzerland’s average temperature has increased by nearly 3 degrees since the pre-industrial era, resulting in melting permafrost that allows water to infiltrate cracks in the rocks.

“There’s a clear connection between climate change and the increase in rockfalls,” Jacquemart remarks. “Dramatic transformations are occurring in high-altitude regions, and the consequences are alarming.”

Yet, Jacquemart advises against attributing the Bratten tragedy solely to recent warming phenomena. The slow geological adjustment to post-Ice Age conditions could also be a factor, she notes.

The immediate future remains unclear for Bratten’s residents. Local authorities declared that the village cannot be reconstructed on unstable ground. Plans are underway for rebuilding, but the area remains susceptible to further landslides, and establishing protective measures demands significant financial resources.

“Communities in mountainous regions worldwide, from the Alps to the Andes and the Himalayas, face increasing threats from the intensity and frequency of mountain-related disasters,” stated Kamal Kishore, United Nations Secretary-General for Disaster Risk Reduction, in a recent statement. “Their livelihoods, cultural heritage, and way of life are under severe threat.”

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Source: www.newscientist.com

How Long He Abstains: The Impact of Male Ejaculation Timing on IVF Success

How Simple Interventions Boost IVF Success Rates

Christoph Burgstedt/Science Photo Library

Men are encouraged to ejaculate within 48 hours prior to IVF egg retrieval to enhance their chances of achieving a viable pregnancy. This recommendation comes from the first clinical trial exploring the effects of varying ejaculation intervals on fertility treatment outcomes.

During the final stages of an IVF cycle, a woman receives a “trigger” injection that matures the developing egg. This crucial injection occurs 36 hours before the eggs are harvested and fertilized.

For optimal sperm health during fertilization, men are often advised to ejaculate between two to seven days before providing their sperm sample for IVF. According to Dr. David Miller from the University of Leeds, who was not involved in the study, “There is an ideal timeframe for ejaculation when sperm quality peaks.”

This two-to-seven-day range is quite broad. Prolonged storage of sperm in the testes exposes them to various environmental toxins, particularly free oxygen radicals from metabolic processes and pollution. This exposure can lead to DNA damage and deterioration of sperm quality, warns Dr. Richard Paulson, also not involved in the trial. Conversely, too short a period between ejaculations may decrease sperm count.

Until now, solid clinical evidence supporting the idea that shorter intervals between ejaculations improve pregnancy outcomes has been lacking, though some studies hint at this. For instance, a 2024 meta-analysis observed that ejaculating less than four days apart correlated with improved semen quality in infertile men. Moreover, another study indicated that intervals under four hours resulted in lesser DNA-damaged sperm and enhanced sperm motility.

To investigate this concept further, Professor Yang Yu from the First Hospital of Jilin University in Changchun, China, conducted a study with 453 men undergoing conventional IVF. One group ejaculated roughly 36 hours prior to the final sperm sample, while another group ejaculated between 48 hours and seven days before.

Results revealed that the ongoing pregnancy rate was significantly higher in the short abstinence group: 46% versus 36% in the longer abstinence group. “While these findings are encouraging, it’s essential to note that they don’t completely represent ultimate treatment outcomes such as live birth rates,” Miller states. Nonetheless, the shorter abstinence group exhibited lower miscarriage rates, suggesting a potential for more live births.

Professor Paulson highlighted that the study provided intriguing insights but also noted its weaknesses, including the inclusion of both fresh and frozen embryos. IVF success rates can vary significantly between these two types. He also pointed out that the data showed a fertility decline in the short abstinence group while simultaneously seeing an increase in ongoing pregnancies. This suggests that fewer couples conceived, but those who did were more likely to continue past 12 weeks, warranting more detailed analysis. “Extraordinary claims necessitate extraordinary evidence that meticulously accounts for all potential variables,” he commented.

Future studies may also disclose whether more frequent ejaculation improves pregnancy outcomes for couples not undergoing IVF. “This trial offers strong evidence that shorter periods of abstinence contribute to better sperm quality,” asserts Dr. Jackson Kirkman-Brown from the University of Birmingham, UK.

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Source: www.newscientist.com

How Lab-Grown Lichens Could Revolutionize Habitat Construction on Mars

Synthesized lichen that shines bright blue under ultraviolet light.

As I explore the fascinating world of lichens, I often find myself captivated by their unique growths on tree branches, rocky outcrops, and gravestones. Although I have encountered numerous lichens during my research on symbiosis, discovering them in a laboratory flask swirling in an incubator was a novel experience. Recently, I’ve begun to contemplate the insights lichens can provide, not just about our past but about the potential for our future.

The green liquid in the incubator may not resemble typical lichen, as this is actually a synthetic alternative. According to Rodrigo Ledesma Amaro, director at the Bezos Center for Sustainable Protein, this co-culture comprises fungi (yeast) and cyanobacteria. Much like natural lichens, the fungal component acts as a structural host while cyanobacteria leverage sunlight, water, and carbon dioxide to create sugars during photosynthesis.

What drives the creation of such “potion”? As Ledesma-Amaro explains, genetically edited yeast can produce useful products—food, fuels, and medications—which can be created sustainably through photosynthesis. Today’s synthetic lichens present exciting opportunities within the biotechnology sector. They hold potential for repairing infrastructures, mitigating climate change, and even crafting habitats on Mars.

“Synthetic lichens replicate the symbiotic nature of natural lichens but grow significantly faster,” says Ledesma-Amaro. Their use of yeast facilitates large-scale production of valuable compounds, like caryophyllene—a vital ingredient in pharmaceuticals, cosmetics, and fuel. Notably, alternative synthetic lichens could be engineered for carbon capture and storage, while ongoing research pursues their use in revitalizing aging concrete structures worldwide. The future application of lichens could even extend beyond Earth, with NASA exploring ways to cultivate engineered lichens on the Moon and Mars for building purposes.

The Science of Symbiosis

Though unassuming, lichens exemplify the essence of symbiosis, where diverse species coexist harmoniously. Typically, lichens consist of fungal partners that host photobionts—algae or bacteria—that produce food through photosynthesis while the fungus shelters them. This arrangement enables lichens to thrive in extreme conditions, fostering scientific interest in creating synthetic counterparts.

Lichens demonstrate two key benefits: their interdependent nature allows them to accomplish more together than individually, and their resilience enables survival in harsh environments. In some regions like Svalbard, where around 700 lichen species exist, they tolerate frigid temperatures, salinity, and other extreme conditions. Curious scientists continue to explore how these organisms endure aridity and temperature fluctuations.

Lichens represent a fascinating life form sustained through a symbiotic relationship.

Jose B. Luis/naturepl.com

Researchers propose that lichen resilience stems from biomolecules formed by filamentous fungi, which provide protection to the entire community. Moreover, their slow growth allows them to persist with minimal resources. Together, these qualities offer lichens unique advantages over single-species organisms.

Space Lichens: The Future of Exploration

These attributes have sparked interest from NASA due to lichens’ ability to withstand simulated and real space conditions. For instance, lichens like Cirquinaria girosa survived outside the International Space Station for over 18 months. Their capacity for growth within rocks and survival in space conditions has intrigued scientists and advocates alike.

Kongrui Jin, a biomaterials engineer at Texas A&M University, recognizes the potential of lichens in future space habitats. Proposals for extraterrestrial homes often use inflatable structures, reducing the need to transport materials from Earth. However, opportunities exist to produce building materials directly from Martian regolith using lichen-based solutions.

Lichens have survived in space, proving their resilience and adaptability.

ESA

“We aim to merge these fungi with photosynthetic species like cyanobacteria,” Jin elaborates. “This combination can convert sunlight into organic nutrients while binding Martian soil particles into cohesive structures.” The biomaterials produced could be utilized with 3D printing technology for constructing habitats.

Jin’s research illustrates the potential of lichens in transforming Martian regolith into conducive building materials. They also offer routes toward producing biominerals and biopolymers, leading some futurists to envision them as key players in terraforming Mars. Yet even without strict planetary protection measures, lichens will need shielding from the harsh Martian surface conditions to flourish.

The Future of Architecture with Lichens

While colonizing other planets remains a distant goal, the application of lichens offers immediate benefits on Earth. They can aid in bundling rubble for construction, notably in rebuilding after natural or human-made disasters. Furthermore, incorporating methods that sequester carbon in concrete production could significantly lessen its environmental impact.

Jin and her colleagues successfully demonstrated that integrating lichen-based combinations of fungi and cyanobacteria can grow in concrete, precipitating calcium carbonate to repair structural cracks efficiently. “This method shows much higher survival rates compared to other microbes in challenging conditions,” she states. These synthetic lichens can extract nitrogen from the air, negating the need for external nutrient supplementation.

Meanwhile, Khakhar is exploring ways to enhance lichen growth by selecting and modifying fast-growing microorganisms. His lab is developing synthetic lichens similar to Jin’s, paving the way for sustainable production of building materials through biomanufacturing, termed “mycomaterials.”

My journey into the world of symbiosis reveals that lichens embody complex ecosystems—a vivid lesson in interdependence and their futuristic potential in shaping our materials. The next time you encounter a lichen adorning a tree or tombstone, take a moment to reflect on the incredible possibilities these organisms hold for our future.

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Source: www.newscientist.com

Stunning Space Photos of 2025: From Supernovae to Moon Landings

Supernova remnant SNR 0509-67.5

Exploring Supernova Remnant SNR 0509-67.5 with the VLT

Credit: ESO/P. Das et al. Background stars (Hubble): K. Noll et al.

Researchers captured a stunning two-tone sphere, evidence of a rare double-massive explosion, using the European Southern Observatory’s Very Large Telescope in Chile.

Astronomers from the University of New South Wales in Australia theorize that this magnificent gas and dust formation emerged when a white dwarf star, once akin to our sun, absorbed helium from a companion star and detonated. The initial explosion transpired approximately 300 years ago, potentially dazzling the Southern Hemisphere night sky, if not for the Sun’s obstruction from Earth.

Dramatic Explosion of SpaceX’s Starship

Photo by: James Temple

This year has been pivotal for SpaceX as CEO Elon Musk aims to send astronauts to Mars with the company’s Starship, the world’s largest and most powerful rocket. After a successful orbital test flight in August, three previous launches ended in catastrophic explosions, referred to by SpaceX as “unplanned rapid disintegration.” James Temple captured the spectacular display of flames during Starship’s seventh unsuccessful attempt in January.

SpaceX’s Dragon Spacecraft After Splashdown

Credit: NASA/Keegan Barber

Aside from its Starship endeavors, SpaceX made strides this year by successfully ferrying astronauts to and from the International Space Station (ISS), stepping in for NASA’s unready rockets. The stunning photograph captures the moment when SpaceX’s Dragon capsule splashed down near a pod of dolphins, carrying two astronauts who had spent nine months aboard the ISS after the Boeing Starliner spacecraft was rendered unsafe for return.

Historic Lunar Photos by Firefly Aerospace’s Blue Ghost Lander

Credit: Firefly Aerospace

In March, Firefly Aerospace’s Blue Ghost lander made history as the second commercial spacecraft to successfully land on the moon and the first to do so in an upright position, after previously tipping over. After a 45-day journey, it settled in the smooth volcanic terrain of Mare Crisium, capturing a selfie of its shadow against the sunlight, with Earth appearing as a distant dot.

Spectacular View of the Trifid and Lagoon Nebulae

Credit: NSF-DOE Vera C. Rubin Observatory

The newly operational Vera C. Rubin Observatory, one of the most advanced telescopes in the world, will conduct daily scans of the night sky for the next decade. One of its early images depicts the Trifid Nebula, a stellar nursery located about 5,000 light-years away, visible as a pink and blue cloud in the upper right corner, contrasted by the Lagoon Nebula—another stellar formation situated 4,000 light-years from Earth. This breathtaking image was compiled from 678 individual snapshots taken during a seven-hour session.

Stunning Composite of September’s Lunar Eclipse Over Tokyo

Credit: Kyodo News (via Getty Images)

The astronomical community eagerly anticipated September’s lunar eclipse, where the moon traverses through the Earth’s shadow, adopting a distinctive red hue similar to sunsets. This striking composite visual captures the moon’s transition as it soared across the Tokyo skyline.

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Source: www.newscientist.com

How Europa’s Thick Ice May Obstruct the Hunt for Ocean Life

Europa’s Ice: A Thick Shell Over a Salty Ocean

Claudio Caridi / Alamy

Europa, one of Jupiter’s intriguing moons, features a liquid ocean possibly encased beneath a thick layer of ice, estimated to be six times the depth of Antarctica’s icy crust, complicating our efforts to detect any potential lifeforms.

This moon is a leading candidate in the search for extraterrestrial life, primarily due to its significant volume of liquid water.

Previously, estimates regarding the thickness of Europa’s ice have varied dramatically—ranging from under 10 kilometers to nearly 50 kilometers. Researchers initially believed certain defects in the ice might permit nutrient exchange between the surface and the ocean below.

Now, a research team, led by Stephen Levin from the California Institute of Technology, has analyzed data collected by the Juno spacecraft, which has been orbiting Jupiter since 2016.

On September 29, 2022, Juno came within 360 kilometers of Europa, utilizing its microwave radiometer to scan the surface and perform the first direct measurements of the ice layer. Levin noted that this instrument assessed the heat emitted by Europa’s icy exterior, enabling the measurement of ice temperatures at various depths and detecting temperature fluctuations resulting from imperfections in the ice sheet.

The researchers estimate that the most accurate thickness of the ice sheet is approximately 29 kilometers, aligning with the higher range of previous estimates while presenting a possible thickness that could range from 19 kilometers to 39 kilometers.

Crucially, their findings indicate that the fissures, pores, and other imperfections likely extend only a few hundred meters beneath the surface, with pore diameters measuring only a few centimeters.

“This indicates that the observed defects in the microwave radiometers are insufficiently deep or expansive to facilitate significant nutrient transport between the ocean and the surface,” asserts Levin.

Nonetheless, this does not diminish the potential for life on Europa. Levin further explains, “Though the observed pores and cracks are too minute and shallow to transport nutrients, alternative transportation mechanisms may exist.”

There may also be unexplored regions of the moon where conditions differ, he adds.

Researchers including Ben Montet from the University of New South Wales in Sydney, express concerns that the ice thickness could hinder life’s search. “While this protection may sustain life for extended durations, it complicates our ability to penetrate the ice and study the ocean beneath,” he notes.

He argues that life could exist without a direct link between Europa’s surface and its subterranean ocean, though such a connection would enhance the chances of discovering life. Helen Maynard-Casley of the Australian Nuclear Science and Technology Agency emphasizes that without that transport link, “you’re essentially confined to whatever was in the ocean initially.”

NASA has plans to launch the Europa Clipper spacecraft in 2024, aiming to embark on its mission to Jupiter’s moons in 2030. This spacecraft is expected to provide clearer insights into Europa’s icy layer, according to Maynard-Casley.

Explore the Mysteries of the Universe: Cheshire, England

Join leading scientists for an engaging weekend as you unravel the mysteries of the universe alongside a tour of the legendary Lovell Telescope.

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Source: www.newscientist.com

Breakthrough Gene Therapy for Huntington’s Disease Demonstrates Promising Results in 2025

Huntington’s Disease: A Gradual Destruction of Brain Cells.

Science Photo Library/Alamy

This year marks a watershed moment in addressing Huntington’s disease, a rare yet impactful form of dementia. Researchers have achieved a groundbreaking milestone with an experimental gene therapy that effectively slows the advancement of this debilitating condition for the first time ever. This represents a significant breakthrough in the search for viable treatments.

According to Sarah Tabrizi from University College London, “This is a monumental step forward,” referencing the successes observed in late-stage trials earlier this year. “We now understand that Huntington’s disease is potentially treatable, presenting us with a tremendous opportunity.”

Huntington’s disease stems from a genetic mutation that causes the normally benign huntingtin protein to cluster into harmful aggregates within the brain. This accumulation leads to gradual deterioration of brain cells, hindering movement, cognitive function, and emotional well-being. Currently, no approved treatments halt the progression of symptoms, and care primarily focuses on supporting affected individuals.

The novel treatment, dubbed AMT-130, directly targets these abnormal proteins by delivering genetic instructions to brain cells, instructing them to produce molecules that inhibit protein formation.

In a recent investigation, Tabrizi and her team administered high doses of AMT-130 to 17 patients with Huntington’s disease. They evaluated changes in cognitive, motor, and daily functioning over a three-year period compared to a control group. Preliminary results released by the drug’s manufacturer, biotechnology firm uniQure, indicate a remarkable 75% average slowdown in symptom progression.

“Huntington’s disease treatment has faced numerous challenges in recent years,” stated Sarah O’Shea at Mount Sinai in New York, who was not involved in the study. “This accomplishment is significant, not just in delaying the disease’s progression but also because it arrives at a crucial time when hope is desperately needed.”

Nevertheless, this innovative treatment does come with its own set of challenges. Tabrizi explained that the 12- to 18-hour surgical procedure required to deliver the treatment deep within the brain is only accessible in a limited number of facilities in select countries, including the U.S. and U.K. Additionally, if approved, the treatment is likely to be prohibitively expensive. “Will it be accessible to all? Achieving that will be a challenge,” she remarked.

To navigate these hurdles, Tabrizi and her team are developing an alternative therapy that involves injecting the fluid around the spinal cord. “We’re currently conducting a Phase I study, and the first patient was treated in November 2024,” Tabrizi noted, with safety results expected by July 2026.

Meanwhile, uniQure’s executives revealed in September plans to submit AMT-130 for FDA approval in early 2026. However, the submission timeline is now uncertain, as the FDA has expressed concerns regarding the study plan and the control group, which consists of *non-treatment* patients drawn from a database.

The absence of a proper control group complicates the ability to discern the placebo effect on results. Still, given the surgical nature of the treatment, establishing such a group poses significant challenges.

“We firmly believe that AMT-130 holds substantial potential to benefit patients and are dedicated to collaborating with the FDA to expedite access to this treatment for families in need across the U.S.,” stated Matt Kapusta, CEO of uniQure.

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Source: www.newscientist.com

Scientists Warn: Cannabis Reclassification Could Unlock Vast Research Opportunities

A long-awaited change in drug policy could pave the way for scientists to explore the benefits and risks of marijuana, the most widely used federally prohibited substance.

On Thursday, President Donald Trump signed an executive order aimed at reclassifying marijuana from a Schedule I substance to a Schedule III substance, a move initiated during the Biden administration.

“Decades of federal drug control policy have overlooked the medical applications of marijuana,” states the order. “This oversight hampers scientists and manufacturers in conducting essential safety and efficacy studies to inform healthcare providers and patients.”

This reclassification is expected to enhance research into medical marijuana, without federally legalizing the substance. However, marijuana use in the U.S. is rising significantly. Gallup data suggests that 15% of adults may smoke marijuana in 2023 and 2024, an increase from 7% in 2013.

The poll did not differentiate between medical and recreational use, revealing the highest usage (19%) among 18- to 34-year-olds—an age group that has exhibited concerning psychological side effects from cannabis use. A recent study published in the journal Pediatrics indicated that even infrequent use was linked to increased psychological distress and lower academic performance in teens.

Medical marijuana is often prescribed for chronic pain relief, to manage nausea and vomiting in cancer patients undergoing chemotherapy, and to stimulate appetite in individuals with specific medical conditions. It remains uncertain how rescheduling cannabis will impact funding for recreational cannabis research.

Scientists like Ziva Cooper are hopeful that reclassification will transform public health through in-depth marijuana research.

“Studying cannabis, also known as marijuana, for both its therapeutic and side effects has been very challenging,” said Cooper, director of the Center for Cannabis and Cannabinoids at UCLA. “The rapid evolution of this industry often outpaces consumer behavior and research developments.”

“It’s challenging to study, and as a scientist committed to public health, it’s tough to keep up with the shifting landscape.”

Schedule I is the most restrictive category within U.S. drug scheduling recognized by the Drug Enforcement Agency (DEA), applying to substances with “no currently accepted medical use and high abuse potential,” such as ecstasy and heroin. Schedule III substances, which include ketamine and anabolic steroids, are classified as having a “moderate to low potential for physical and psychological dependence.”

Even in cannabis-friendly regions, Cooper acknowledges that he faces similar research obstacles as those in states like Idaho, where cannabis use is prohibited.

“Researchers are unable to test readily available products; they can only inquire about basic characteristics of the cannabis available at compounding pharmacies visible from their lab,” Cooper said. “This creates limitations on sourcing the cannabis for research.”

Need for Thorough Research on Marijuana’s Benefits and Risks

Last year, the National Institutes of Health allocated $75 million for cannabinoid research, a slight increase from $70 million in 2023. Moreover, $217 million was directed towards cannabinoid studies, with $53 million specifically for cannabidiol (CBD), a non-psychoactive cannabinoid.

Dr. Brooke Wurster, medical director of the master’s in medical cannabis science and business program at Thomas Jefferson University, pointed out that bureaucratic challenges often confine cannabis research to observational studies rather than the rigorous clinical trials required for pharmaceuticals, resulting in mixed findings.

For instance, a study published in 2024 in the journal Current Alzheimer’s Research found a 96% reduced risk of subjective cognitive decline among recreational cannabis users aged 45 and older compared to non-users. In contrast, 2025 research in the JAMA Network Open indicated that heavy cannabis users aged 22-36 exhibited memory impairments.

A recent study in Biomedicine suggested cannabinoids as a “promising” alternative for opioid use in chronic pain management, emphasizing an urgent need for large-scale randomized controlled trials. Meanwhile, a study last year found that JAMA Network Open reported increased medical visits for cannabis-related disorders among older Medicare beneficiaries from 2017 to 2022.

The reclassification will enable researchers to examine and prepare specific marijuana formulations, Wurster noted. Even in states with medical cannabis programs, cannabis quality and potency can vary significantly across dispensaries.

“We can comprehensively monitor immediate symptoms, blood levels, and long-term effects,” she explained. “All the essential elements required for drug research mandated by the federal government.”

While cannabis has medical benefits for some individuals, Jonathan Caulkins, H. Guyford Steever Professor of Operations Research and Public Policy at Carnegie Mellon University, cautioned that administrative barriers alone do not account for cannabis not being a “miracle cure” for conditions like cancer and Alzheimer’s.

“Studies conducted in countries like Canada, France, and Israel are not under the same restrictions,” Caulkins stated. “We should not assume U.S. law is the sole reason cannabis hasn’t emerged as a definitive treatment option.”

Wurster emphasized that these changes bring new responsibilities for the medical community, as smoked and inhaled products may not be safe for all individuals.

“We still need to comprehend the best methods for delivering appropriate medications and guidance to the right patients,” she cautioned. “Available products are frequently unregulated and present significant mental health risks, particularly among young users, as well as cardiovascular concerns, necessitating greater caution.”

A Major Shift in Cannabis Policy After 55 Years

The regulatory barriers that researchers face have roots extending back over fifty years. Under the Nixon administration, the Controlled Substances Act of 1970 categorized marijuana as a Schedule I drug.

Almost six decades later, much regarding marijuana’s medicinal potential remains undiscovered. Currently, from a legal standpoint, it is viewed merely as a substance of abuse, Wurster noted.

Susan Ferguson, director of the Institute on Addiction, Drugs and Alcohol at the University of Washington School of Medicine, anticipates that obtaining cannabis research licenses will soon become easier for scientists. Presently, researchers can broadly license drugs classified from Schedule II to V, while those exploring Schedule I substances must secure individual licenses for each.

“This necessitates a detailed written protocol,” she explained. “It involves DEA personnel visiting to review research and experimental strategies, which complicates the process considerably.”

Ferguson believes that reclassifying marijuana would “open the floodgates” for clinical research. Participants may be more willing to engage in Schedule III studies than in those involving Schedule I drugs.

Ferguson compared cannabis to alcohol and tobacco, which, although common, are not benign. Due to medical research, their risks are well documented.

“We have yet to conduct that level of research on cannabis,” Ferguson concluded. “Ultimately, we aim to inform people more comprehensively about the risks and benefits associated with its use.”

Source: www.nbcnews.com

Massive Jellyfish Larger Than a Bus Discovered in Shallow Waters: What You Need to Know

Imagine a colossal deep-sea predator in the ocean’s depths. It’s likely there’s a giant squid nearby, perhaps being pursued by an even larger sperm whale.

Yet, numerous enigmatic giant hunters roam the dark abyss, many still shrouded in mystery from science. Meet the Stydiomedusa gigantea, a name derived from Greek that means “giant jellyfish of the underworld.”

This impressive jellyfish is typically a deep crimson shade, showcasing smooth, rounded bells (or “caps”) that exceed 1 meter (3 ft) in diameter, adorned with a wavy margin.

Four ribbon-like arms extend back up to 10 meters (33 feet). To visualize, if one of these jellies were resting in a London double-decker bus, it could easily tap the driver on the shoulder.

The giant phantom jellyfish belongs to the Urumidae family, which also includes more common species like the moon jellyfish.

A giant phantom jellyfish was captured in the Bellingshausen Sea off Antarctica in February 2025 – Photo credit: ROV SuBastian / Schmidt Ocean Institute

Unlike its relatives, the phantom jellyfish is devoid of stinging cells needed to paralyze prey. Instead, it relies on its long arms to capture small fish and zooplankton, guiding them into its mouth.

Specimens of the giant phantom jellyfish were first collected in the late 19th century, and the species received its official name in 1910.

Despite its size, only about 100 encounters with the phantom jellyfish have been documented over the years.

Rare sightings have occurred globally, spanning the Atlantic, Pacific, Indian, and Southern Oceans, primarily at extreme depths where they might roam over 6 km (4 miles) below the surface.

https://www.youtube.com/watch?v=9bzQYKm3xTA" title="Giant Phantom Jellyfish Video

In 2025, researchers from the Schmidt Ocean Institute aboard the R/V Falcor were exploring the Southern Ocean following the recent calving of a giant iceberg, unveiling vast ocean regions previously inaccessible to scientists.

Using remotely operated vehicles like the Subastian, they uncovered a thriving ecosystem beneath the ice, teeming with animals such as octopuses and giant sea spiders.

They also captured stunning footage of giant phantom jellyfish gracefully floating in the water.

Interestingly, many of these elusive jellyfish are spotted by tourists rather than researchers. Luxury Antarctic cruise ships often come equipped with personal deep submersibles, allowing vacationers to venture beneath the waves.

Fortunate passengers have encountered giant phantom jellyfish, leaving behind ghostly footage on their smartphones as they resurface.

Scientific studies published in 2023 documented sightings primarily occurring near the West Antarctic Peninsula at depths ranging from 80 to 280 meters (262 to 918 ft).

For context, that’s roughly the height between Big Ben and the Empire State Building.

The reason these giant phantom jellies venture so close to the surface of Antarctica’s frigid waters remains an unsolved puzzle.


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Stunning Close-Up of Arp 4 Captured by Hubble Space Telescope

Discover the latest stunning image captured by the NASA/ESA Hubble Space Telescope, showcasing Arp 4, an intriguing visual pair of galaxies located in the constellation Cetus.



The Hubble image captures the galaxy pair Arp 4. Image credits: NASA / ESA / Hubble / J. Dalcanton, Dark Energy Survey / DOE / FNAL / DECam / CTIO / NOIRLab / NSF / AURA.

For more details, explore Arp 4, which features the bright spiral galaxy MCG-02-05-050a alongside the larger spiral galaxy MCG-02-05-050.

Located within the constellation Cetus, this galaxy pair was first discovered by Dutch-Canadian astronomer Sidney van den Bergh in 1959.

Arp 4 stands as the fourth entry in Halton Arp’s Atlas of Peculiar Galaxies and belongs to the section focusing on “Galaxies with Low Surface Brightness.”

“The term ‘Arp 4’ derives from the Atlas of Peculiar Galaxies compiled by astronomer Halton Arp during the 1960s,” Hubble astronomers explained.

“These ‘unusual galaxies’ were chosen for photography to illustrate their distinct and non-standard shapes, providing insights into galaxy evolution.”

Hubble’s mission has transformed our understanding of galaxies, revealing captivating examples from Arp’s Atlas, including Arp 4.

The initial galaxies in this catalog, including Arp 4, exhibit low surface brightness, rendering them faint and challenging to observe.

“The larger galaxy, cataloged as MCG-02-05-050, features fragmented arms and a dim disk, perfectly fitting this description,” the astronomers noted.

“In contrast, its smaller counterpart, MCG-02-05-050a, is considerably brighter and more dynamic as a spiral galaxy.”

“Crucially, these galaxies are not in close proximity,” the researchers emphasized.

“The prominent blue galaxy, MCG-02-05-050, lies 65 million light-years from Earth.”

“Meanwhile, the brighter, smaller galaxy MCG-02-05-050a is positioned at an impressive 675 million light-years, over ten times farther away.”

This positioning likely suggests that MCG-02-05-050a is the more substantial of the two, while MCG-02-05-050 is relatively smaller.

“This visual pairing is simply an unlikely coincidence,” the astronomers added.

“Despite the absence of a physical connection, we can enjoy the unique sight of Arp 4 as an enthralling duo adorning our night sky.”

Source: www.sci.news

New Bird Species Discovered in Papua New Guinea: A Breakthrough in Avian Research

Ornithologists have utilized camera traps to document a newly identified species of jewel bubbler in the lush karst forests of Papua New Guinea’s Southern Fold Mountains.



Camera trap images showcasing the holotype and two paratypes of Ptilorrhoa urrissia taken during a detailed 3-month sampling in a high-density array over 0.5 ha. The holotype (ac, marked ‘h’ in image a) and a paratype (a and d, marked ‘p’ in image a), an adult female and juvenile with female-type plumage, were photographed together on January 1, 2020. The shown image is from a sequence of 20 photos captured within 87 seconds. A putative adult male paratype (e) was photographed on March 8, 2020, from under 40 meters. Image credit: Woxvold et al., doi: 10.1111/ibi.70016.

The newly identified species falls under the genus Ptilorrhoa, known for small birds in the family Cinclosomatidae.

Commonly referred to as jewel bubblers, these unique birds are endemic to New Guinea.

According to Ian Wachsvold, an ornithologist with the Australian Museum Research Institute, “Jewel bubblers are a group of ground-dwelling, insectivorous passerines found exclusively in New Guinea and nearby land-bridge islands.”

“These birds are characterized by their plump bodies, short wings, black masks, and white throat or cheek patches, with many species having soft feathers adorned with blue or maroon markings.”

“Typically vocal but shy, they dwell deep within the forests, making them more often heard than seen.”

“Currently, there are four recognized species, with three found across much of New Guinea, differentiated mainly by their altitude – Ptilorrhoa caerulescens lives in lowland areas, while Ptilorrhoa castanonota resides in hills and low mountains; Ptilorrhoa leucosticta prefers dense forests.”

“The fourth species, the brown-headed jewel bubbler (Ptilorrhoa geislerorum), has been recorded in two geographically separated regions: the hills and lowlands of northeastern Papua New Guinea, and a recently discovered population presumed to be this species located far west of Yapen Island.”

In 2017, Dr. Wachsvold and Leo Regula from Lihir Gold Ltd. initiated a biennial camera trap monitoring program for ground-dwelling birds and mammals on the Igif Ridge (Uri [mount] Uricia in the local Fasu language), a limestone forested anticline situated on the southeastern fringe of the Agogo Mountains in the Southern Highlands Province of Papua New Guinea.

Throughout this research, distinctive, undescribed jewel bubblers were captured on camera.

“During over 1,800 camera days, we recorded 10 images of the bird across three sequences (trigger events) using two cameras set approximately 600 meters apart,” the researchers noted.

“In November 2018, we attempted to set up mist nets to capture these birds but were unsuccessful.”

“Camera trap surveillance was repeated in 2019, 2021, and 2024, accumulating a total of 94 photographs (22 sequences) and seven 30-second videos (4 sequences) featuring at least three to six birds, with 11 cameras monitoring an area of 16 hectares.”

Analysis of museum specimens alongside field photographic evidence confirms that the bird in question distinctly differs from other known Ptilorrhoa species.

Pyroroa urrissia),” they stated.

Pyroroa urrissia appears to be a resident species in the Yagif Ridge area, with birds photographed consistently over a span of ten consecutive months (June through March) across seven years.

The total number of newly detected species during the sampling period probably comprises fewer than ten birds.

“This species tends to be observed alone, in pairs, or in small family groups of three to four,” the researchers highlighted.

“Data indicates a similar social organization to other jewel bubblers worldwide. The Pyroroa urrissia duo is frequently photographed together, with most records (all but 3 sequences of one male) gathered from a 7 ha area; most likely indicating two breeding events involving a resident pair and their offspring.”

“We hypothesize that the Igif Ridge supports a fragmented population occupying an isolated low mountain lacking higher altitude support for Ptilorrhoa leucosticta,” they add.

“Potentially suitable habitats may be restricted to regions between Mt Bosabi and Mt Karimui in southern Papua New Guinea.”

To date, no songs have been distinctly attributed to any Ptilorrhoa species aside from Ptilorrhoa castanonota, although the team did encounter vocalizations on the Igif Ridge.

The new species appears to produce softer calls compared to other species such as Ptilorrhoa caerulescens and Ptilorrhoa castanonota, while showing behavioral similarities to Ptilorrhoa leucosticta.

“Jewel bubblers on the Igif Ridge are threatened by multiple factors,” scientists warn.

“Known native predators include at least three marsupials, such as the New Guinea quoll (Dasyrus albopuntatus), the woolly three-striped dasher (Myoichthys leucula), and certain Murexia species. Furthermore, the Papuan eagle (Harpyopsis novaeguineae), goshawk (Accipiter poliocephalus), and the great owl (Tito tenebricosa) prey on the ground, possibly targeting adult birds or their young.”

“Invasive predators represent an additional significant risk, especially for ground-nesting species like the jewel bubbler.”

“Domestic cats (Felis catus) have been photographed on Igif Ridge thrice in 2021 and 2024.”

“Dogs (Canis lupus familiaris) are frequently spotted in the area, often accompanying hunters or loitering opportunistically.”

“Lastly, climate change poses a severe threat to tropical montane birds, particularly those like Pyroroa urrissia that have limited dispersal capabilities and no access to high-altitude environments on Igif Ridge.”

The findings of this significant discovery were published in a study in the journal Toki on November 26, 2025.

_____

Ian A. Wachsvold et al. A newly identified species of jewel bubbler (Cinclosomatidae: Ptilorrhoa) from Papua New Guinea’s Southern Fold Mountains. Toki, published online November 26, 2025. doi: 10.1111/ibi.70016

Source: www.sci.news

Scientists Uncover 1.4 Billion-Year-Old Salt Crystals with Ancient Bubbles

In a groundbreaking study, researchers uncovered ancient gases and fluids trapped within 1.4 billion-year-old rock salt crystals in northern Ontario, Canada. Their analysis reveals that oxygen and carbon dioxide concentrations during the Mesoproterozoic Era (1.8 billion to 800 million years ago) were suppressed to just 3.7% of current levels, while carbon dioxide was found to be ten times pre-industrial levels. These findings indicate a period of climatic stability, suggesting atmospheric oxygen levels temporarily exceeded the needs of early animals long before their emergence.

Examples of primary halite, mixed halite, and secondary halite rock inclusion aggregates. Image credit: Park et al., doi: 10.1073/pnas.2513030122.

Scientists have long recognized that liquid inclusions within rock salt crystals preserve samples of Earth’s primordial atmosphere.

However, accurately measuring these inclusions has presented significant challenges. These inclusions encompass both air bubbles and saline water, with gases like oxygen and carbon dioxide interacting differently in liquids compared to air.

“It’s astonishing to crack open a sample of air that is over a billion years older than the dinosaurs,” said Justin Park, a graduate student at Rensselaer Polytechnic Institute.

“Our carbon dioxide measurements are unprecedented,” stated Morgan Schaller, a professor at Rensselaer Polytechnic Institute.

“For the first time, we can trace this era of Earth’s history with remarkable precision. These are authentic samples of ancient air.”

Measurements indicate that Mesoproterozoic atmospheric oxygen levels sat at 3.7%, mirroring today’s levels. This high oxygen concentration was sufficient to support the existence of complex multicellular life, which would not arise for hundreds of millions of years.

Conversely, carbon dioxide was found to be ten times more abundant than present levels, effectively counterbalancing the “weak young sun” and fostering the climate conditions seen today.

One pivotal question arises: if oxygen levels were adequate for animal life, why did evolution take so long?

“This sample represents a snapshot in geological time,” Park explained.

“It may reflect a brief oxygenation event during this lengthy period, humorously dubbed the ‘billion boring years.'”

“This era in Earth’s history was marked by low oxygen levels, geological stability, and minimal evolutionary change.”

“Despite its moniker, direct observational data from this time is crucial for understanding the emergence of complex life and the evolution of our atmosphere.”

Prior indirect estimates suggested low carbon dioxide levels for this epoch, contradicting evidence of a lack of significant glaciation during the Mesoproterozoic.

The team’s direct measurements of elevated carbon dioxide, alongside temperature estimates from the salt, imply that Mesoproterozoic climate conditions were milder and more akin to today’s climate than previously assumed.

“Algae began to flourish during this period, continuing to play a vital role in global oxygen production today,” Professor Schaller remarked.

“The relatively elevated oxygen levels may directly result from the increasing prevalence and complexity of algae.”

“The insights we gained could represent an exciting moment in what is otherwise regarded as a billion years of monotony.”

The team’s research paper has been published today in the Proceedings of the National Academy of Sciences.

_____

Justin G. Park et al.. 2025. Bringing the Boring Billion to Life: Direct constraints from 1.4 Ga fluid inclusions reveal a favorable climate and oxygen-rich atmosphere. PNAS 122 (52): e2513030122; doi: 10.1073/pnas.2513030122

Source: www.sci.news

NASA’s Parker Solar Probe Discovers 3I/ATLAS Comet: Key Findings and Insights

Scientists utilized the WISPR (Wide Field Imager for Solar Exploration) instrument on NASA’s Parker Solar Probe to capture stunning images of the interstellar comet 3I/ATLAS between October 18 and November 5, 2025.

WISPR captures the interstellar comet 3I/ATLAS. Image credit: NRL / NASA / JHUAPL / Guillermo Stenborg, JHUAPL.

Discovered on July 1, 2025, by the NASA-funded ATLAS survey telescope in Rio Hurtado, Chile, 3I/ATLAS, also known as C/2025 N1 (ATLAS) and A11pl3Z, originated from the constellation Sagittarius.

This remarkable interstellar comet approached Mars on October 3 at a distance of just 0.194 AU and reached its perihelion, the closest point to the Sun, on October 30.

On December 19, 3I/ATLAS made its nearest pass to Earth, coming within 270 million kilometers (168 million miles) of our planet.

The spectacular images of 3I/ATLAS were obtained by the WISPR instrument aboard NASA’s Parker Solar Probe during a critical observation window from October 18 to November 5.

“The Parker Solar Probe captured around 10 images of the comet daily,” stated WISPR team members.

“During this observation period, the spacecraft accelerated away from the Sun following its 25th solar flyby on September 15.”

“These initial images are currently undergoing calibration and processing, revealing the comet’s movement behind the Sun from Parker’s vantage point.”

“At that time, the comet was located about 209 million kilometers (130 million miles) from the Sun, just beyond Mars’ orbit.”

“These images offer a rare opportunity to study the comet when it was too close to the Sun for ground-based observations.”

The WISPR team is diligently working to finalize the data by eliminating stray light and adjusting for varying exposure times between images, enhancing the comet’s visibility.

“The final images will significantly advance our understanding of this intriguing interstellar visitor,” researchers concluded.

Source: www.sci.news

New Study Examines Paleolithic Shift: Transition from Neanderthals to Anatomically Modern Humans

The transition from the Middle to Upper Paleolithic, occurring approximately 50,000 to 38,000 years ago, was a pivotal period characterized by the decline and extinction of Neanderthals alongside the emergence and expansion of anatomically modern humans, known as Homo sapiens. Paleoanthropologists at the University of Cologne have created a high-resolution model of population dynamics to reconstruct this significant transition on the Iberian Peninsula. Their ensemble simulations investigated Neanderthal survival, the arrival of modern humans, and the potential for interbreeding.

This image shows a Neanderthal and a human child. Image credit: Neanderthal Museum.

During this critical transition from the Middle Paleolithic to the Upper Paleolithic, Neanderthal populations experienced a steady decline across Europe, particularly in the Iberian Peninsula, leading to their eventual extinction.

Simultaneously, anatomically modern humans spread throughout Europe, marking a significant shift in human history.

This era was further defined by dramatic climate fluctuations, featuring alternating cold and warm periods. Rapid warming events occurred within centuries, contrasting with gradual cooling phases, known as the Dansgaard-Eschger phenomenon, which were punctuated by severe cooling caused by iceberg releases into the North Atlantic (Heinrich phenomenon).

The precise timing of Neanderthal extinction and the arrival of modern humans remains uncertain, leaving open the possibility of interactions between the two species.

Genetic analyses of archaeological bones compared to modern populations indicate admixture events in eastern Europe during the early phases of modern human migration.

Given the uncertainty of these dates, it remains possible that the two populations on the Iberian Peninsula may have intermixed at a later time, though this has yet to be substantiated.

In this innovative study, Professor Yaping Hsiao and his colleagues from the University of Cologne utilized numerical models to exploratory simulate potential encounters between Neanderthals and modern humans on the Iberian Peninsula.

These models considered ongoing climate changes while simulating the populations of both groups, along with their interactions and connectivity.

“By running the model multiple times with varying parameters, we can assess the plausibility of different scenarios, such as the early extinction of Neanderthals, small at-risk populations, or prolonged survival leading to admixture,” explained Professor Hsiao.

“However, for the majority of the simulations, the two groups did not converge.”

Across all scenarios, the populations exhibited high sensitivity to climate change.

Mixing between the two species was plausible if both populations could maintain stability over an extended period.

At a low probability (1%), a small fraction of the total population—approximately 2-6%—could possess genes from both groups by the end of the simulation.

This admixture likely occurred in the northwestern region of the Iberian Peninsula, where modern humans may have arrived early enough to interact with still-surviving Neanderthal populations.

“By integrating climate, demography, and cultural factors, our dynamic model provides a comprehensive framework that enhances our interpretation of the archaeological and genomic records,” stated Professor Gerd Christian Weniger from the University of Cologne.

For further details, refer to a paper that will be published in the online journal PLoS ONE.

_____

Y. Xiao et al. 2025. Pathways at the Crossroads of Iberia: Dynamic Modeling of the Middle to Upper Paleolithic Transition. PLoS ONE 20 (12): e0339184; doi: 10.1371/journal.pone.0339184

Source: www.sci.news

New Scientist Reveals Changes to UK Freedom of Information Laws in 2025

Peter Kyle’s Landmark Request for ChatGPT Logs Stuns Observers

In early 2025, I sent an email that I never expected would set a legal precedent for the UK government’s approach to AI chatbot interactions. However, that’s precisely what unfolded.

It all began in January when I came across an interview with Peter Kyle, then UK Technology Secretary. In the interview with Politics Home, Kyle disclosed that he frequently converses with ChatGPT, hinting that he actively engages with the technology his department is responsible for regulating.

This revelation piqued my curiosity. Could I obtain his chat history? Freedom of Information (FOI) laws are typically used to request emails and documents from public authorities, yet past court rulings suggest that certain personal data, like search queries, are not released under these laws. I was particularly interested in how chatbot conversations are classified.

Ultimately, the answer leaned towards the former. Most of Kyle’s interactions with ChatGPT were deemed private and exempt from FOI regulations. However, interactions that occurred in an official capacity were subject to disclosure.

In March, the Department of Science, Industry, and Technology (DSIT) provided several conversations between Kyle and the chatbot. This revelation formed the basis of an exclusive article detailing his exchanges.

The publication of these chat logs took data protection and FOI experts by surprise. “I’m astonished you obtained them,” remarked Tim Turner, a Manchester-based data protection expert. Others were simply left speechless.

When this article was released, we emphasized that this represented a world first, capturing global attention around the accessibility of AI chatbot conversations.

International researchers from countries like Canada and Australia reached out to me for advice on how to file similar requests with their government ministers. For example, subsequent FOI requests in April revealed that Ferrill Clarke, the then UK Artificial Intelligence Secretary, had never used ChatGPT in an official capacity, despite promoting its advantages. However, many inquiries were met with denials as governments increasingly cited legal exceptions to FOI.

I observed a noticeable shift in the UK government’s approach to FOI, especially regarding AI utilization. In a subsequent request for DSIT’s internal responses to this article—comprising emails and Microsoft Teams messages—my FOI application was denied, citing the process as laborious and time-consuming.

Despite considering asking the government to utilize ChatGPT for summarizing the relevant information, I ultimately chose not to pursue it.

This release was pivotal as governments swiftly adapt to AI technologies. The UK government has acknowledged that civil servants use tools such as ChatGPT in their daily operations, claiming that this adoption can save up to two weeks annually due to enhanced efficiency. However, it’s critical to note that AI does not always deliver impartial summaries and can produce inaccuracies or “hallucinations.” Thus, transparency in how these technologies are employed is essential for accountability, whether the implications are positive or negative.

Topic: Politics / 2025 News Review

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Source: www.newscientist.com

NASA Astronomers Classify Near-Earth Asteroids: Latest Findings – Sciworthy

Researchers exploring the solar system’s history focus on a diverse range of comets and asteroids, particularly those classified as Near-Earth Objects (NEOs). These celestial bodies not only offer insights into the origins of water and organic materials but also continue to impact planets across the solar system, including Mars, Earth, Venus, and Mercury. Their close proximity to Earth facilitates detection and observation with smaller telescopes, increasing the potential for successful interceptions, potentially involving rovers and landers.

An international research team has recently classified and identified 39 new NEOs between February 2021 and September 2024, utilizing two advanced telescopes: Itaparica Observatory (OASI) in Brazil, along with the 2.15-meter Jorge Sahade telescope at Complejo Astronomico El Leoncito (CASLEO) in Argentina.

The research team used these telescopes to study variations in the brightness of NEOs over time. Since NEOs are essentially blocks of ice or rock that reflect sunlight rather than emit light, their visibility from Earth is influenced by the angle between Earth and the Sun along with their size, shape, and structure. By measuring the periodic changes in brightness, scientists calculated the rotation rates of these objects.

The diameters of the 39 NEOs varied from 0.1 to 10 kilometers (0.06 to 6 miles), with most ranging between 0.5 to 3 kilometers (0.3 to 2 miles). Their shapes ranged from nearly spherical to elongated, cigar-like forms. The team successfully determined the rotation periods for 26 of these NEOs, noting that the shortest rotation cycle was just over two hours while the longest approached 20 hours. Notably, 16 of these NEOs rotated in under 5 hours, suggesting that many are fast-rotating bodies.

The study established that a rotation period exceeding 2.2 hours is the upper limit for small NEOs known as rubble pile asteroids, which are loose formations held together by self-gravity. Beyond this threshold, centrifugal forces could destabilize them. Conversely, those NEOs under 250 meters (820 feet) tend to be more solid, dubbed monoliths. The findings indicated that smaller and medium-sized NEOs exhibit varied structures and formation histories.

Using advanced imaging techniques through telescope lenses that filter specific light wavelengths, the researchers analyzed the chemical composition of 34 NEOs. They employed 2 additional filters alongside 4 filters designed for green and red wavelengths, including near-infrared wavelengths. Their results revealed that 50% of the NEOs are silica-based, resembling many terrestrial rocks, with 23.5% comprising carbon-rich materials, approximately 9% metals, and around 6% basaltic elements. The remaining composition was a mixture of carbon and silicates as well as calcium and aluminum.

While the chemical analysis largely aligned with previous findings, the researchers found a lack of olivine—a mineral typically prevalent in smaller asteroids. This absence can be attributed to the fact that most sampled NEOs exceeded 200 meters (660 feet), surpassing the typical size for olivine-rich asteroids.

This research enriches our understanding of NEOs and their physical and chemical properties. The team advocates for an integrated research approach that leverages technology and multi-telescope observations to effectively characterize small celestial objects. Future studies should prioritize close monitoring of NEOs, especially those approaching their rotation threshold, and employ radar observations to confirm the existence of potential binary pairs. By analyzing reflected visible and near-infrared light, researchers can further unveil the chemical makeup of the asteroid surfaces.


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Source: sciworthy.com

2025’s Most Captivating Animal Photography Showcase

Please wait a moment

Wenjian Sun et al. 2025

Remarkably, the rat is observed attempting to resuscitate its unconscious cage mate by pulling its tongue and clearing the airway. In studies, researchers found that certain rodents, when interacting with anesthetized mice, exhibited caring behaviors such as pawing, grooming, and biting unresponsive individuals. This discovery indicates that empathetic behavior may be more prevalent in the animal kingdom than previously thought.

How high can you shoot?

Claryana Araújo-Wang/Botos do Cerrado Research Project/CetAsia Research Group

The male Amazon river dolphin (Inia geofrensis) was caught on camera urinating while rolling onto its back. This behavior is thought to communicate with other dolphins, similar to how land mammals employ scent marking. Other males might be drawn to the urine that falls into the water, interpreting it as a message.

Stay away!

David Ongley

This beautiful wren can be seen perched cautiously on a branch (Marlus cyaneus), evading the cuckoo—a notorious brood parasite. Scientists have discovered that over 20 bird species utilize similar “call” calls to alert nearby birds, as cuckoos secretly lay their eggs in other birds’ nests to shirk their parenting responsibilities.

Ali tries origami

Dr Chris Reid, Macquarie University

The weaving ant (Oecophila smaragdina) is depicted rolling up a piece of lined paper, using teamwork to lock it together in a long chain. Each ant grasps the abdomen of the ant in front, enabling the construction of nests from rolled leaves. Studies show that individual ants can pull nearly 60 times their body weight, while teams of 15 can generate forces exceeding 100 times their combined weight.

Never seen before

ROV Subastian/Schmidt Ocean Institute

For the first time, a living giant squid (Mesonihoteutis hamiltonii) was captured on film. While these mollusks are believed to grow up to 7 meters, the squid filmed was just a baby measuring 30 centimeters. This rare footage was obtained by a vessel from the Schmidt Ocean Institute while streaming live from the depths of the Southern Ocean near the South Sandwich Islands.

That’s my arm!

Sumire Kawashima, Yuzuru Ikeda/Ryukyu University

This octopus appears fooled into believing that a fake arm made of white gel is its own. While it’s well-known that humans can be tricked in a similar manner, scientists have discovered that octopuses share this intriguing behavior as well.

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Source: www.newscientist.com

Did Black Holes Exist in the Early Universe? Exploring the Evidence

Gas ball with a black hole

A New Discovery: Gas Balls with Black Holes at Their Centers

Shutterstock / Nazarii_Neshcherenskyi

The early universe is rich with enigmatic star-like gas balls powered by central black holes, a discovery that has astounded astronomers and may clarify some of the most significant mysteries unveiled by the James Webb Space Telescope (JWST).

Upon initiating its observations of the universe’s first billion years, JWST uncovered compact, red galaxies that exhibited extraordinary brightness—galaxies unlike those found in our local universe. Previous interpretations suggested that these “small red dots” (LRDs) were either supermassive black holes engulfed in dust or densely packed star galaxies; however, these theories inadequately explained the light signals detected by JWST.

Recently, astronomers suggested that LRDs might actually be dense gas clusters with a black hole at their core, termed “black hole stars.” According to Anna de Graaf from Harvard University, as matter falls into a black hole, it emits immense gravitational energy, causing the surrounding gas to radiate light like stars. While this energy is distinct from nuclear fusion typical in stars, it results in a luminous mass of dense gas potentially billions of times brighter than our sun, according to de Graaf.

Despite some early evidence supporting this idea, a consensus remained elusive. Now, de Graaf and colleagues have reviewed the most extensive sample of LRDs since JWST’s launch, encompassing over 100 galaxies, and propose that these entities are best classified as black hole stars. “Although the term black hole star is still debated, there’s growing agreement within the scientific community that we’re observing accreting black holes enveloped by dense gas,” de Graaf noted.

When examining the spectrum of light emitted by an LRD, the observed patterns more closely resemble those from a uniform surface (blackbody) characteristic of stars, contrasting with the intricate and varied spectra from galaxies emitting light produced by a combination of stars, dust, gas, and central black holes.

“The black hole star concept has intrigued scientists for a while and, despite initial skepticism, is proving to be a viable explanation,” states Gillian Bellovary of the American Museum of Natural History. “Using a star-like model simplifies the framework for interpreting observations without necessitating extraordinary physics.”

In September, de Graaf’s team also identified another single LRD displaying a striking peak in the light frequency spectrum, which they dubbed “the cliff.” “We discovered spectral characteristics unexplainable by existing models,” de Graaf explained. “This pushes us to reevaluate our understanding and explore alternative theories.”

Presently, many astronomers agree that LRDs likely operate like vast star formations; however, de Graaf cautions that substantiating the black hole hypothesis presents challenges. “The core is hidden within a dense, optically thick envelope, obscuring what’s inside,” de Graaf explains. “Their brightness leads us to suspect they harbor black holes.”

A potential method to affirm their nature as black holes involves studying the temporal changes in emitted light, observing whether they fluctuate akin to known black holes in our universe, as noted by Western Hanki from Cambridge University. “We note brightness variances over brief intervals, yet there’s scant evidence of such variations in most LRD cases.”

While JWST’s observational timeframe is limited, scrutinizing long-lived light fluctuations from LRDs may yield insights. A new study by Sun Fengwu and his team at Harvard recently uncovered a gravitational lens, an LRD that bends light around a massive galaxy between us and the object. This lens generated four distinct images of the original LRD, mimicking observations over 130 years and suggesting brightness variations similar to known pulsating stars, aligning with the hypothesis of black hole stars. Sun and his team opted not to comment for this article.

Although utilizing gravitational lenses to observe LRDs at different times is clever, Bellovary notes that other factors might account for brightness changes. “The data may not suffice to validate their conclusion. While I’m not dismissing their claims, I think there may be alternative explanations for the observed variations.”

If it turns out these galaxies are indeed black hole stars, de Graaf warns we’ll need to devise a new model addressing their origin and what they evolve into, given the absence of equivalent systems in our local universe. “This could represent a new growth phase for supermassive black holes,” she concludes. “The nature of these events and their significance to the final mass of black holes remains an open question.”

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Rising Hopes for Alien Discovery in 2025: What Happened to the Excitement?

Artist's impression of K2-18b exoplanet

Artist’s Impression of Exoplanet K2-18b

A. Smith/N. Mandusudhan

The quest for extraterrestrial life intensified this year when scientists detected intriguing signals from exoplanets containing molecules associated with life on Earth. Although subsequent attempts to confirm these findings were unsuccessful, exoplanet researchers believe the resulting discussions provided valuable insights for future alien detection efforts.

In April, Nick Madhusudan and his team at the University of Cambridge announced they observed “the first hints of another world, possibly inhabited.” These signals originated from K2-18b, an exoplanet approximately eight times the mass of Earth and located 124 light-years away within its star’s habitable zone, as observed with the James Webb Space Telescope (JWST).

The infrared radiation emitted by K2-18b suggests its atmosphere may contain dimethyl sulfide (DMS), a molecule known to be produced solely by living organisms, particularly marine phytoplankton, here on Earth.

As expected, this discovery generated significant buzz within both media and the scientific community. However, many researchers advised caution, emphasizing that the DMS signal was weak and required additional observations and rigorous analysis for confirmation.

Now, several months later, most astronomers concur that there is currently no evidence of DMS or any biomolecules in K2-18b’s atmosphere. Should they exist, they remain undetectable. “We only know for certain that methane and carbon dioxide are present in the atmosphere of this planet,” explains Lewis Wellbanks from Arizona State University.

Claims of discovering extraterrestrial life were premature, according to Wellbanks. “It’s been shown repeatedly that this information is inaccurate. New observations indicate that those gases are not present,” he asserted.

Yet, the data spike initially attributed to DMS still requires clarification, says Jake Taylor at Oxford University. “We observed a spike—a physical phenomenon. At this point, we still don’t know what it signifies.”

Identifying the molecules responsible for these spikes requires further exploration planned for the JWST next year. Scientists can only ascertain what’s present in a planet’s atmosphere by analyzing the starlight filtering through it during the planet’s transit across its host star. This occurs four times each Earth year.

Despite the controversy surrounding this discovery, Taylor notes it also fostered positive outcomes. “This has been a significant learning experience for the entire exoplanet community. We are reassessing our definitions and statistical methods, which has been tremendously beneficial,” he states.

“This experience teaches us to calibrate our expectations,” says Wellbanks. “It’s a reminder that relying on data manipulation to validate a claim is challenging. As one wise person noted, there are lies, damned lies, and statistics. This whole DMS saga falls into that category.”

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Enhance Your Brain Detox: Effective Tips for Strengthening the Glymphatic System

X-ray image of a skull showing a colored brain and neurons

When neurons in the brain are active, they generate waste products.

Credit: Nick Veasey/Science Photo Library/Alamy

As we embrace the joy of the Christmas season, many are already thinking about detox plans for the new year, such as reducing movie watching or cutting back on alcohol. This leads to an interesting query: can we apply similar detox methods to our brains? After the festivities, how can we clear away any cognitive clutter?

The brain is naturally equipped to detoxify itself daily, flushing out accumulated metabolic waste that could be harmful. But can we assist in this vital process, potentially shielding ourselves from age-related cognitive decline and dementia?

Let’s delve into the glymphatic system, a newly uncovered pathway responsible for detoxification. This system effectively “sucks” away undesirable proteins and waste from the spaces between neurons, channeling them into cerebrospinal fluid (CSF).

“CSF circulates much like water in a dishwasher,” explains Maha Alattar from Virginia Commonwealth University.

This fluid systematically drains waste into lymph nodes, eventually allowing it to exit the body through the veins.

While the connection between the glymphatic and lymphatic systems is still not fully understood, researchers are increasingly focused on ways to optimize the glymphatic process. Enhancing this system could prove pivotal in combating cognitive decline and promoting healthy aging. Accumulation of metabolic waste in the brain is linked to symptoms such as declining cognitive function, increasing the risk of dementia and expediting Alzheimer’s and Parkinson’s disease symptoms.

“The glymphatic system is fascinating,” says Nandakumar Narayanan from the University of Iowa Health Care. “Numerous innovative research efforts aim to better understand and quantify glymphatic functions, shedding light on human health and disease.”

Enhancing the Brain’s Waste Removal System

Are there ways we can enhance this waste disposal mechanism? Recent studies indicate that lifestyle changes may significantly impact its efficiency.

“The most proven method to boost glymphatic clearance is sleep,” notes Dr. Lila Landovsky from the University of Tasmania.

The glymphatic system is predominantly inactive during waking hours but reaches peak activity during sleep. For instance, in mice, CSF flow surges by about 60% while they sleep, enabling the removal of beta-amyloid, a protein linked to Alzheimer’s disease.

Though studies have yet to definitively establish that glymphatic activation directly prevents dementia, “the hypothesis is strengthened by evident links between factors that impair glymphatic clearance—such as sleep disturbances and sedentary behavior—and an increased risk for neurodegenerative conditions,” states Landowski.

The position in which we sleep could also affect glymphatic function. In 2015, Helen Benveniste and her team found that sleeping on one’s side improved glymphatic clearance in mice more effectively than sleeping on the back or stomach. While this has not yet been tested in humans, many types of dementia show strong associations with sleep disorders, suggesting sleep positions may be important in our fight against dementia.

Additional Strategies to Enhance Brain Detox

Emerging evidence suggests that other lifestyle choices, such as regular exercise, may also bolster glymphatic function. In April, a study involving 37 adults highlighted that only participants who completed a 12-week stationary cycling program experienced noticeable increases in glymphatic drainage, as observed through brain imaging.

“Research in mice indicates that glymphatic clearance can roughly double after five weeks of regular exercise in comparison to sedentary mice,” says Landowski. “However, short-term studies in mice have yet to be performed.”

Further examination of the glymphatic system may uncover additional methods to enhance its function. Lymphatic vessels connected to CSF are located deep in the neck, making direct manipulation challenging, but researchers led by Ko Young Gu at the Korea Institute of Science and Technology have identified another lymphatic network directly beneath the skin of monkeys and mice’s facial and neck areas.

In experiments, gentle downward stroking of the face and neck in mice tripled CSF flow, effectively rejuvenating older animals’ flow to a more youthful state.

Similar vessels have been detected in human cadavers, suggesting that facial and neck massages could potentially enhance CSF flow, aiding in glymphatic clearance. Nonetheless, more research is needed to substantiate these claims and verify whether this enhanced flow can shield against neurodegenerative disorders.

Promising Evidence Supporting Yoga and Breathing Techniques

One exercise that should not be overlooked is yoga breathing. Hamid Jalillian from the University of California, Irvine, notes that diaphragmatic breathing has robust evidence supporting its ability to increase CSF velocity, effectively activating a glymphatic “rinse cycle.”

Diaphragmatic breathing is characterized by keeping the chest relatively still while moving the abdomen outward and lowering the diaphragm as you inhale through your nose. Conclude the cycle by exhaling through pursed lips while retracting your belly.

Unexplored Potential

Despite the enthusiasm surrounding the glymphatic system, our comprehension of its intricate workings is still developing. Not everyone is convinced we possess enough knowledge to prescribe specific interventions at this time. “We are far from being able to accurately predict how a specific intervention, like exercise, will influence the glymphatic system. There are limited studies in both mice and small human populations, but nothing large-scale and conclusive,” cautions Narayanan.

Nevertheless, there is a sense of optimism. “The potential is immense, but these studies require meticulous and thorough execution,” he concludes.

For now, I’ll concentrate on essential routines—prioritizing quality sleep and regular exercise. These habits are crucial for overall health, but should glymphatic research hold true, they may soon play an even more critical role in keeping my brain clear, not just in the new year, but for years to come.

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Source: www.newscientist.com

Struggling to Connect with Your Emotions? You Might Have Alexithymia.

Finding the right words to express ourselves can be challenging at times. If you frequently encounter emotions that seem elusive, you might be experiencing symptoms of alexithymia.

Individuals with alexithymia struggle not only to articulate their emotions but may also find it hard to differentiate between feelings and bodily sensations.

For instance, when you see someone you once admired while walking down the street, you might feel your chest tighten and your heart race. These physical responses could signify nervousness or excitement.

Unlike those without alexithymia, who can quickly identify their emotions, those with the condition may need to search their memories or the contextual clues before they can name their feelings.

Since recognizing emotions is crucial for effective emotion regulation, alexithymia can hinder the management of intense feelings, whether negative or positive.

This trait is a personality aspect rather than a specific disorder or syndrome. While the precise cause remains unclear, research has indicated that both genetic and environmental factors may play a role.

Approximately 13 percent of the population may experience some form of alexithymia, with studies suggesting a higher prevalence in men than in women .

Struggling to accurately identify your emotions can lead to issues like anxiety, relationship challenges, and isolation – Photo credit: Getty

Additionally, alexithymia is linked to common traits associated with neurological disorders that may emerge following trauma or brain injury, such as experiences after a stroke or epilepsy.

A review conducted by psychologists in 2018 highlighted that alexithymia overlaps considerably with autism, with one in two individuals on the autism spectrum potentially facing alexithymia.

While no cure exists for this condition, it has been proposed that improving emotional awareness through practice may be possible.

This involves engaging with exercises that connect physical sensations to specific emotions, as well as expanding our “emotional vocabulary” to better articulate our inner experiences.


This article addresses the question “Am I alexithymic?” as posed by Lochlan Booth from Durham.

If you have any inquiries, please reach out via email at: questions@sciencefocus.com or send us a message facebook, ×or Instagram Page (don’t forget to include your name and location).

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How One Man Thrived for 555 Days Without a Heart

The chronicles of medical history demonstrate that the human body is remarkably resilient. Numerous documented cases illustrate this, including that of a French man who was discovered alive in 2007 with 90 percent of his brain missing.

This 44-year-old man was leading a typical life when it was revealed that he had severe hydrocephalus, a condition where cerebrospinal fluid replaces brain tissue.

His case exemplifies biological redundancy and adaptability, as remaining tissues compensate for lost functions (primarily through neuroplasticity).

Similar adaptations can occur with paired organs, like the lungs, kidneys, and testicles. When one organ fails, the remaining one can assume both functions.










In many instances, even after critical organ loss, advanced medical techniques can keep individuals alive.

For instance, a young American man carried a functioning artificial heart in his backpack for 555 days awaiting a transplant after his own was removed.

In some “pneumothorax cases,” surgeons can remove a patient’s heart and lungs, substituting them with a life support system known as extracorporeal membrane oxygenation (ECMO).

There are instances of individuals living without several organs.

The chronicles of medical history illustrate the incredible resilience of the human body – Image courtesy of Robin Boyden

Some patients with stomach cancer may need multiple digestive organs removed, including the full stomach, spleen, pancreas, small intestine, and colon.

Survival is possible in these situations through a combination of enzyme supplements, a tailored diet, parenteral nutrition, and sometimes insulin supplementation.

Additional internal organs that can be lived without include the gallbladder, bladder, thyroid, and appendix.

While it’s uncertain if there’s a maximum number of organs one can live without simultaneously, losing several organs in a single incident often leads to death due to blood loss, infection, or severe trauma.


This article is in response to Miriam Russell of Hull’s inquiry: “How many organs can you live without?”

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Newly Found Spider Web Traverses Two Countries, Hosting 100,000 Creatures

For those with arachnophobia, it might be best to look away, as scientists have unearthed the largest spider colony in the world.

The nest spans 106 square meters (1,140 square feet) and is believed to host up to 111,000 spiders—roughly half the size of a tennis court.

Recently, researchers published their findings in Underground Biology, revealing that two distinct species of spiders formed this massive colony.

This remarkable spider colony is situated in the Sulfur Caves of the Vromoner Valley, straddling the Greece-Albania border.

The nest resides in a permanently dark section of the cave, extending 50 meters (164 feet) from the entrance through a narrow, low-ceilinged passage. It comprises a multilayered patchwork of individual funnels that merge to create a spongy mass.

Researchers estimate the colony houses around 69,000 spiders, including Tegenaria domestica (commonly known as the barn funnel weaver or common house spider) and approximately 42,000 of The Vagrant of Prineligone species.

While these two species often coexist nearby, they typically do not share close quarters.

In fact, barn funnel weavers usually prey on smaller creatures, including The Vagrant of Prineligone. A truce between the two is unlikely, as the low light within the cave hinders the spiders’ vision.

Tegenaria domestica hides in a funnel-shaped nest and emerges when prey approaches – Credit: Getty

Instead, the spiders primarily feed on non-stinging midges, which swarm thickly in proximity to their colonies. These midges thrive on nutrients provided by natural springs and sustained by the sulfur-rich river navigating through the cave.

DNA analysis indicates that these spiders are genetically distinct from their surface relatives, highlighting adaptations to their unique environment.

Conversely, a sulfur-rich diet significantly diminishes the variety of gut microbiota.

Both factors imply that these spiders do not intermingle with their cousins found above ground.

The colony was initially discovered in 2022 by a group of cavers from the Czech Speleological Society during their exploration of the area.

A team of researchers followed up in 2024, estimating the spider population by counting the web funnels and collecting specimens for further analysis.

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Hubble Observes the Collision of Two Planetesimals near Fomalhaut

Fomalhaut, the 18th brightest star visible in the night sky, is orbited by the compact light source Fomalhaut b, which has been previously interpreted as either a dusty exoplanet or debris from a collision of two planetesimals. While such collisions are seldom witnessed, their remnants can be captured in images. Recent observations from the NASA/ESA Hubble Space Telescope indicate that a second point source is expected to appear around Fomalhaut in 2023, reminiscent of Fomalhaut b’s appearance two decades ago. Astronomer Paul Karas from the University of California, Berkeley, and his team suggest this new source is a dust cloud resulting from a recent collision between two planetesimals.



This Hubble image shows the debris ring and dust clouds CS1 and CS2 around Fomalhaut. Image credit: NASA / ESA / P. Kalas, University of California, Berkeley / J. DePasquale, STScI.

Fomalhaut is an A-type star located a mere 25 light-years away in the constellation Austrinus Pisces.

The name Fomalhaut originates from its Arabic name, Hum Al Hat, which translates to “fish mouth.”

This star is twice as massive and 20 times more luminous than the Sun, encircled by a ring of dust and debris.

In 2008, astronomers utilized Hubble to identify a potential planet surrounding Fomalhaut, marking it as the first star system where a potential planet was detected using visible light.

The object termed Fomalhaut b presently resembles a dust cloud that appears akin to a planet, resulting from a planetesimal impact.

During new Hubble observations aimed at locating Fomalhaut b, Dr. Karas and his colleagues were astonished to discover a second point of light positioned similarly around the star.

This new object has been dubbed Stellar Frequency Source 2 (cs2), while the original object is now referred to as cs1.

“This is definitely the first instance we’ve observed a point of light spontaneously appearing in an exoplanetary system,” remarked Dr. Karas.

“Hubble images up to now have not shown this. What we’re witnessing is a violent collision between two massive bodies creating an enormous debris cloud, unlike anything else currently seen in our solar system. It’s incredible.”

The proximity of these two debris clouds remains a puzzle for astronomers.

If asteroid and planetesimal collisions were random, cs1 and cs2 should ideally be found in unrelated positions.

However, they are intriguingly located close together along the inner edge of Fomalhaut’s outer debris disk.

Another enigma is the occurrence of these two events in such a brief timespan.

“Previous theories indicated that impacts should occur roughly once every 100,000 years or more. Yet, we’ve observed two impacts in just 20 years,” Dr. Karas noted.

“If you had movies from the past 3,000 years and fast-forwarded them to make a year just a fraction of a second, imagine how many flashes you’d see during that period.”

“The Fomalhaut planetary system will continue to provide insights into these collisions.”

Collisions are crucial for the evolution of planetary systems, yet they are infrequent and challenging to study.

Dr. Mark Wyatt, an astronomer at the University of Cambridge, stated: “The intrigue of this observation lies in its ability to assist researchers in estimating the size of the impactor and the number of objects present in the disk. This data is nearly impossible to obtain through other methods.”

“We estimate that the planetesimals destroyed to form CS1 and CS2 were only around 30 km in diameter, suggesting there are approximately 300 million such objects orbiting the Fomalhaut system.”

“This system effectively serves as a natural laboratory for studying the behavior of planetesimals during collisions, enabling us to learn about their composition and formation.”

For further details, see this result. Featured in this week’s Science diary.

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Paul Kalas and colleagues. 2025. Second planetesimal impact in the Fomalhaut system. Science published online on December 18, 2025. doi: 10.1126/science.adu6266

Source: www.sci.news

NASA’s New Leader, Jared Isaacman, Outlines His Key Priorities

Jared Isaacman, a billionaire entrepreneur, has outlined his priorities for NASA on his inaugural day as the agency’s new leader.

Sworn in as NASA’s 15th administrator on Thursday, Isaacman was officially appointed the same day President Donald Trump endorsed an executive order instructing NASA to return astronauts to the Moon by 2028, initiate the development of a permanent lunar outpost by 2030, and establish a framework for future exploration of Mars.

This order is expected to offer Isaacman and NASA a strategic roadmap.

“In the next three years, we will once again land American astronauts on the Moon, but this time we aim to create the necessary infrastructure for their extended stay,” Isaacman stated in an interview with NBC News following his swearing-in.

He assumes this role during a pivotal moment for NASA, as the Trump administration urges the agency to land astronauts on the Moon before any Chinese astronauts arrive there.

“A new space race is upon us,” Isaacman remarked.

The next stage of NASA’s Moon return initiative, known as Artemis, could kick off as soon as February. The Artemis II mission will send four astronauts on a 10-day lunar orbit to test the Space Launch System rocket and Orion spacecraft.

The following Artemis III mission is anticipated to have astronauts land close to the lunar south pole.

U.S. District Judge Timothy Kelly (left) swears in Jared Isaacman (right) as NASA’s 15th administrator in Washington, D.C., on Thursday, with Isaacman’s parents, Donald and Sandra Murray, present.Bill Ingalls/NASA (via Getty Images)

Under Isaacman’s leadership, NASA is anticipated to pursue increased commercialization. SpaceX and Blue Origin will be crucial to the agency’s lunar return efforts, and Isaacman indicated that additional private space firms will back the agency’s aspirations for the Moon.

President Trump’s space policy executive order advocates for the creation of a “dynamic commercial space economy driven by American free enterprise” and details plans to reduce the International Space Station while establishing a commercial space station by 2030.

Additionally, the order emphasizes nuclear power in space. Following direction from Transportation Secretary Sean Duffy, who served as NASA’s acting administrator before Isaacman’s confirmation, the initiative aims to develop a nuclear reactor ready for launch to the Moon by 2030.

Isaacman highlighted the importance of nuclear power for explorations beyond the Moon, particularly for future Mars missions.

However, one significant challenge he will encounter as administrator is translating the White House’s vision into action with a constrained budget.

Current funding for the U.S. government is set to last until January 30; afterward, NASA may face substantial budget reductions, especially for science operations.

Despite these immediate hurdles, Isaacman remains optimistic about the agency’s capacity to align with the administration’s goals.

“Whether it’s $25 billion or $20 billion, it’s a significant sum that the agency receives every year,” he remarked. “We possess exceptional talent to tackle numerous challenging, nearly impossible tasks simultaneously.”

“This is an opportunity for the president’s space policy to revisit the Moon, establish infrastructure there, and invest in future technologies like nuclear power in anticipation of Mars missions,” Isaacman stated. “With the resources at hand and the president’s dedication to space policy in the White House, I’m confident we can achieve our objectives.”

Source: www.nbcnews.com

Quantum Computers Prove More Valuable Than Anticipated by 2025

Quantum Computers Could Shed Light on Quantum Behavior

Galina Nelyubova/Unsplash

Over the past year, I consistently shared the same narrative with my editor: Quantum computers are increasingly pivotal for scientific breakthroughs.

This was the primary intent from the start. The ambition to leverage quantum computers for deeper insights into our universe has been part of its conception, even referenced in Richard Feynman’s 1981 address. In his discussion about effectively simulating nature, he suggested: “Let’s construct the computer itself using quantum mechanical components that adhere to quantum laws.”

Currently, this vision is being brought to life by Google, IBM, and a multitude of academic teams. Their devices are now employed to simulate reality on a quantum scale. Below are some key highlights.

This year’s advancements in quantum technology began for me with two studies in high-energy particle physics that crossed my desk in June. Separate research teams utilized two unique quantum computers to mimic the behavior of particle pairs within quantum fields. One utilized Google’s Sycamore chip, crafted from tiny superconducting circuits, while the other, developed by QuEra, employed a chip based on cryogenic atoms regulated by lasers and electromagnetic forces.

Quantum fields encapsulate how forces like electromagnetism influence particles across the universe. Additionally, there’s a local structure that defines the behaviors observable when zooming in on a particle. Simulating these fields, especially regarding particle dynamics—where particles exhibit time-dependent behavior—poses challenges akin to producing a motion picture of such interactions. These two quantum computers addressed this issue for simplified versions of quantum fields found in the Standard Model of particle physics.

Jad Halime, a researcher at the University of Munich who was not a part of either study, remarked that enhanced versions of these experiments—simulating intricate fields using larger quantum computers—could ultimately clarify particle behaviors within colliders.

In September, teams from Harvard University and the Technical University of Munich applied quantum computers to simulate two theoretical exotic states of matter that had previously eluded traditional experiments. Quantum computers adeptly predicted the properties of these unusual materials, a feat impossible by solely growing and analyzing lab crystals.

Google’s new superconducting quantum computer, “Willow,” is set to be utilized in October. Researchers from the company and their partners leveraged Willow to execute algorithms aimed at interpreting data obtained from nuclear magnetic resonance (NMR) spectroscopy, frequently applied in molecular biochemical studies.

While the team’s demonstration using actual NMR data did not achieve results beyond what conventional computers can handle, the mathematics underlying the algorithm holds the promise of one day exceeding classical machines’ capabilities, providing unprecedented insights into molecular structures. The speed of this development hinges on advancements in quantum hardware technology.

Later, a third category of quantum computer made headlines. Quantinuum’s Helios-1, designed with trapped ions, successfully executed simulations of mathematical models relating to perfect electrical conductivity, or superconductivity. Superconductors facilitate electricity transfer without loss, promising highly efficient electronics and potentially enhancing sustainable energy grids. However, currently known superconductors operate solely under extreme conditions, rendering them impractical. Mathematical models elucidating the reasons behind certain materials’ superconducting properties are crucial for developing functional superconductors.

What did Helios-1 successfully simulate? Henrik Dreyer from Quantinuum provided insights, stating that it is likely the most pivotal model in this domain, capturing physicists’ interests since the 1960s. Although this simulation didn’t unveil new insights into superconductivity, it established quantum computers as essential players in physicists’ ongoing quest for understanding.

A week later, I was on another call with Sabrina Maniscalco discussing metamaterials with the quantum algorithm firm Algorithmiq. These materials can be finely tuned to possess unique attributes absent in naturally occurring substances. They hold potential for various applications, ranging from basic invisibility cloaks to catalysts accelerating chemical reactions.

Maniscalco’s team worked on metamaterials, a topic I delved into during my graduate studies. Their simulation utilized an IBM quantum computer built with superconducting circuits, enabling the tracking of how metamaterials manipulate information—even under conditions that challenge classical computing capabilities. Although this may seem abstract, Maniscalco mentioned that it could propel advancements in chemical catalysts, solid-state batteries, and devices converting light to electricity.

As if particle physics, new states of matter, molecular analysis, superconductors, and metamaterials weren’t enough, a recent tip led me to a study from the University of Maryland and the University of Waterloo in Canada. They utilized a trapped ion quantum computer to explore how particles bound by strong nuclear forces behave under varying temperatures and densities. Some of these behaviors are believed to occur within neutron stars—poorly understood cosmic entities—and are thought to have characterized the early universe.

While the researchers’ quantum computations involved approximations that diverged from the most sophisticated models of strong forces, the study offers evidence of yet another domain where quantum computers are emerging as powerful discovery tools.

Nevertheless, this wealth of examples comes with important caveats. Most mathematical models simulated on quantum systems require simplifications compared to the most complex models; many quantum computers are still prone to errors, necessitating post-processing of computational outputs to mitigate those inaccuracies; and benchmarking quantum results against top-performing classical computers remains an intricate challenge.

In simpler terms, conventional computing and simulation techniques continue to advance rapidly, with classical and quantum computing researchers engaging in a dynamic exchange where yesterday’s cutting-edge calculations may soon become routine. Last month, IBM joined forces with several other companies to launch a publicly accessible quantum advantage tracker. This initiative ultimately aims to provide a leaderboard showcasing where quantum computers excel or lag in comparison to classical ones.

Even if quantum systems don’t ascend to the forefront of that list anytime soon, the revelations from this past year have transformed my prior knowledge into palpable excitement and eagerness for the future. These experiments have effectively transitioned quantum computers from mere subjects of scientific exploration to invaluable instruments for scientific inquiry, fulfilling tasks previously deemed impossible just a few years prior.

At the start of this year, I anticipated primarily focusing on benchmark experiments. In benchmark experiments, quantum computers execute protocols showcasing their unique properties rather than solving practical problems. Such endeavors can illuminate the distinctions between quantum and classical computers while underscoring their revolutionary potential. However, transitioning from this stage to producing computations useful for active physicists appeared lengthy and undefined. Now, I sense this path may be shorter than previously envisioned, albeit with reasonable caution. I remain optimistic about uncovering more quantum surprises in 2026.

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Source: www.newscientist.com

The U.S. Conquered Avian Influenza in 2025, Yet the Battle Continues

Millions of chickens culled due to threat of bird flu

Emily Elkonin/Bloomberg via Getty Images

This year, the United States has seen its first reported death from bird flu, stirring apprehension regarding the possibility of a human pandemic. Although the virus’s spread has been contained sufficiently to conclude the emergency measures, health experts caution that vigilance remains crucial.

“The pandemic persists,” stated Megan Davis from Johns Hopkins University in Maryland. “The virus’s lethality hasn’t diminished.”

The predominant strain causing human infections is a subtype of avian influenza named H5N1, which was first detected in poultry in China back in 1996. After a resurgence in 2021, it wreaked havoc on bird populations worldwide and infected various mammals, including foxes, seals, and cats.

H5N1 is not well-equipped to infect humans and has not shown transmission capability between humans. However, it remains a grave concern; nearly half of the approximately 1,000 recorded global infections have ended in death since 2003. These fatalities are likely concentrated in severe cases, with many milder instances undocumented. Nonetheless, potential risks remain for the human population, especially if the virus adapts to enable human-to-human transmission, Davis emphasized.

Health experts expressed concern when H5N1 was identified among dairy cows in the U.S. in March 2024—the first confirmed case in this type of livestock. This not only placed the virus closer to human populations, particularly farm workers, but it also provided a prime opportunity for the virus to evolve and spread among humans. Each time it infects a new mammal, the pathogen stands to acquire mutations that could facilitate human transmission, according to Davis.

Since that time, H5N1 has been found in 1,080 herds across 19 states while monitoring a chicken farm. From February to mid-December 2022, around 1,950 birds were reported sick across the U.S., prompting the culling of nearly 200 million birds.

Subsequent outbreaks on farms triggered a significant uptick in human cases. As of December 2025, 71 individuals had tested positive for avian influenza in the United States; all knew of their infections through close contact with infected livestock or poultry. Out of these, three were infected by different animal sources, and although the cause for the remaining three cases remains unknown, there is no evidence suggesting they were transmitted from other humans.

Most affected individuals exhibited mild symptoms, such as conjunctivitis, and recovered fully. However, one person with pre-existing health conditions succumbed to the H5N1 virus in Louisiana, marking the first recorded bird flu-related death in the nation.

Since that incident, the United States has largely managed to curb the virus’s spread. The most recent positive testing for H5N1 occurred in February, according to Emily Hilliard, a representative for the U.S. Department of Health and Human Services. However, a man in Washington state later tested positive and died from a different strain of avian influenza, H5N5, after contact with infected birds in November .

“Somewhat reassuringly, retrospective analyses of fatal H5N5 instances have not indicated further human cases, although the potential for H5 viruses to incite a pandemic continues to loom, particularly given their capacity to affect mammals, including humans, and mammals’ potential for reciprocal transmission,” Davis pointed out. The CDC is actively monitoring the situation and asserts the threat to public health is currently low.

Cases of H5N1 in dairy cows have also significantly dwindled, with reports from the U.S. Department of Agriculture (USDA) citing only two flocks testing positive between November and mid-December.

These reductions ultimately led the CDC to conclude its emergency response to bird flu in early July, stated Hilliard. This response, which commenced in April 2024, enabled the agency to allocate additional resources and staff toward surveillance and containment efforts, she explained.

Several factors may have contributed to the decrease in cases. Notably, the Department of Agriculture implemented the National Milk Testing Strategy in December 2024, mandating dairy facilities to furnish raw milk samples for H5N1 testing. “Testing is central to any management program,” asserted Davis. “Without knowledge regarding its location, [H5N1] it would be impossible to enforce enhanced protective measures or request that farms enact quarantines.”

In February, USDA rolled out a $1 billion initiative aimed at reducing H5N1 occurrences within poultry farms, with increased funding earmarked for vaccine research and biosecurity protocols. One focus was to bolster defenses against wildlife. “The vast majority of [bird flu] outbreaks in poultry and livestock have been linked to contact with infected wild birds,” noted a USDA spokesperson. By curbing H5N1 spread on farms, according to Davis, the fact that most infections affect dairy workers likely contributed to lowering human transmission as well.

However, seasonal fluctuations could also play a role. “We experienced a drop during summer but subsequently witnessed a surge in cases during fall and winter,” remarked Davis. “Currently observing the migratory season, we are likely to see an increment in cases.”

This may account for the more than 200,000 increase in H5N1 detections among backyard and commercial poultry flocks, as migratory birds are known to spread the virus to farms during their seasonal flights, representing a rise of 130 percent between September and October. “What we haven’t seen is a considerable number of human cases,” Davis clarified. However, she added that it remains uncertain whether this is attributed to improved safety protocols or diminished monitoring of farm workers.

“It’s encouraging to observe the decline in cases,” stated Davis. “Nevertheless, we still have work to accomplish.”

Topics:

  • bird flu/
  • 2025 News Review

Source: www.newscientist.com

Space-Based Data Centers Are Still a Long Way Off.

Starcloud aims to establish a 4km x 4km data center satellite

star cloud

Is the overwhelming need for massive data centers by AI manageable through extraterrestrial solutions? Tech firms are considering low-Earth orbit as a viable option, although experts warn that substantial engineering and unresolved challenges currently hinder progress.

The explosive demand and investment in generative AI platforms like ChatGPT have sparked an unparalleled need for computing resources, requiring vast land areas as well as electricity levels comparable to those consumed by millions of households. Consequently, many data centers are increasingly relying on unsustainable energy sources such as natural gas, with tech companies expressing concerns that renewable energy sources cannot meet their skyrocketing power needs or stability requirements for reliable operations.

In response, executives like Elon Musk and Jeff Bezos are advocating for the launch of data centers into orbit, where they could benefit from continuous sunlight, surpassing that of terrestrial solar panels. Bezos, founder of Amazon and owner of Blue Origin, stated earlier this year: It is anticipated that gigawatt-class data centers could be operational in space within 10 to 20 years.

Google is moving forward with its vision for a space data center through its pilot initiative, Project Suncatcher, which plans to launch two prototype satellites equipped with TPU AI chips by 2027 to experiment with their functionality in orbit. However, one of the most notable advancements in space data processing occurred this year with the launch of a solitary H100 graphics processing unit by StarCloud, an Nvidia-backed company. Nevertheless, this is significantly less computing power than what modern AI systems require; OpenAI is estimated to utilize around a million of such chips.

For data centers to function effectively in orbit, many unresolved issues must be tackled. “From an academic research standpoint, [space data centers] are still far from being production-ready,” remarks Benjamin Lee from the University of Pennsylvania, USA.

According to Lee, one of the major hurdles is the extensive scale required to meet AI’s computational needs. This involves not only the power demands from solar panels—requiring substantial surface area—but also the challenge of dissipating heat produced by the chips, the only feasible cooling method in a vacuum. “We can’t use cold air and evaporative cooling like we do on Earth,” Lee explained.

“Square kilometers will be occupied independently for energy generation and cooling,” he added. “These structures expand rapidly. When discussing capacity in the range of 1,000 megawatts, it essentially equates to a considerable area in orbit.” Indeed, StarCloud plans to construct a data center of 5,000 megawatts over 16 square kilometers, roughly 400 times the area of the solar panels on the International Space Station.

Lee believes that several promising technologies could help mitigate these requirements. Krishna Muralidharan from the University of Arizona is investigating thermoelectric devices that can convert heat into electricity, enhancing the efficiency of chips functioning in space. “It’s not a matter of feasibility; it’s a challenge,” Muralidharan stated. “For now, we can temporarily rely on large thermal panels, but ultimately we will require more sophisticated solutions.”

Additionally, space presents unique challenges unlike those found on Earth. For instance, there is a significant presence of high-energy radiation that can impact computer chips, leading to errors and disrupted calculations. “Everything will slow down,” Lee cautioned. “A chip positioned in space might perform worse compared to one on Earth due to the need for recalibration and error correction.”

To function at this scale, Muralidharan noted that thousands of satellites need to operate in tandem, necessitating highly precise laser systems for communication both between data centers and with Earth, where atmospheric interference can distort signals. Despite this, Muralidharan remains optimistic, believing these challenges are surmountable. “The real question is not if, but when,” he asserts.

Another point of uncertainty is whether AI will still necessitate such extensive computational resources by the time the data centers are in place. This is particularly relevant if anticipated advancements in AI do not align with the growing computing power we are beginning to observe. “It’s evident that training requirements may peak or stabilize, which would likely cause the demand for large-scale data centers to follow suit,” Lee explained.

Yet, even in such a scenario, Muralidharan suggests potential applications for space-based data centers, such as facilitating space exploration beyond Earth and monitoring terrestrial phenomena.

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Source: www.newscientist.com

Most High-Achieving Adults Do Not Begin as Child Prodigies.

The award-winning athlete may have been a late bloomer when it came to enhancing their abilities

Michael Steele/Getty Images

A review has revealed that international chess masters, Olympic gold medalists, and Nobel Prize-winning scientists were seldom child prodigies. In many cases, early childhood achievements and rigorous training do not lead to elite performance as adults.

This investigation, based on 19 studies involving nearly 35,000 high achievers, indicates that most adults who dominate global rankings in their respective fields engaged in various activities during their youth, gradually honing their expertise.

The findings challenge the popular notion that reaching top performance internationally necessitates rigorous training in early childhood, according to Arne Gullich from RPTU Kaiserslautern in Germany. “Understanding that many world-class performers were not exceptionally outstanding in their formative years implies that extraordinary early achievements are not a precondition for sustained elite performance.”

Numerous studies have examined the intensity of training for children in specific domains like music or sports; competitive performance in these areas during adolescence or early adulthood. However, research on older elite athletes shows a different pattern. For instance, 82% of junior athletes at the international level do not become international adult athletes, and 72% of senior athletes at the international level never reached junior international status.

The life stories of notable global experts further indicate that the correlation between childhood and adult success may not be as significant as perceived. For instance, while composer Wolfgang Amadeus Mozart, golfer Tiger Woods, chess prodigy Gyukesh Donmaraj, and mathematician Terence Tao were undeniable child prodigies, others like composer Ludwig van Beethoven, basketball legend Michael Jordan, chess player Viswanathan Anand, and scientist Charles Darwin were not recognized as such.

The studies analyzed by Gurich and colleagues included examinations of the life journeys of Olympic athletes, Nobel laureates in science, the top ten chess players globally, renowned classical music composers, and international leaders across various disciplines.

In numerous fields, early successes and later elite performers exhibited stark differences. In fact, only around 10% of individuals who excelled as youngsters maintained that level into adulthood, with a similar percentage of those who thrived as young adults continuing to excel later in life.

The researchers compared their findings with data from 66 studies on the training experiences of young athletes and “sub-elite” athletes — those who have achieved notable local recognition but are not world-class. They observed that common traits attributed to high-achieving youth, such as early specialization and rapid advancement, are often lacking or even reversed in adults who perform at the highest levels.

This may stem from the fact that gaining exposure to a diverse range of activities in early childhood cultivates adaptable learning skills, enabling children to discover the pursuits that resonate best with them. “Essentially, they identify the best match for their interests and enhance their learning potential for future endeavors,” Gullich notes.

Additionally, a less rigorous training schedule during childhood and adolescence can help mitigate the risk of burnout and injuries that might hinder long-term careers. “There’s a danger of becoming entrenched in an area that you no longer find enjoyable, which could lead you to seek a change,” Gullich adds.

This review addresses an enduring research gap by clearly differentiating between early success and prolonged elite performance. According to David Feldon from Utah State University, there remains a propensity to push children towards intense focus on acquiring and practicing specific skills. “This undoubtedly fosters expertise and yields immediate benefits,” he explains. “However, it remains uncertain whether this will be advantageous over a lifetime.”

For Feldon, who also coaches youth wrestling, the implications of this review are essential for those guiding children’s skill development. “It’s about not just nurturing exceptional expertise but doing so in a healthy and constructive manner that fosters improvement in a broader context, rather than simply achieving narrow targets.”

As a result, programs aimed at quick identification and acceleration of young talents may overlook many potential future leaders, as they often prioritize immediate success over sustained excellence. Gullich emphasizes, “Do elite training programs, gifted programs, and scholarship initiatives typically cater to very young age groups with a singular focus? Given recent evidence, it is more beneficial to inspire young people to engage in at least one or possibly two other disciplines over several years.”

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Source: www.newscientist.com

2025: A Landmark Year for Online Safety Laws—Will They Be Effective?

The evolving experience of young people on the internet.

Linda Raymond/Getty Images

In 2025, numerous countries will implement new internet access restrictions aimed at protecting children from harmful content, with more expected to follow in 2026. However, do these initiatives genuinely safeguard children, or do they merely inconvenience adults?

The UK’s Online Safety Act (OSA), which took effect on July 25, mandates that websites prevent children from accessing pornography or content that promotes self-harm, violence, or dangerous activities. While intended to protect, the law has faced backlash due to its broad definition of “harmful content,” which resulted in many small websites closing down as they struggled to meet the regulatory requirements.

In Australia, a new policy prohibits those under 16 from using social media, even with parental consent, as part of the Online Safety Amendment (Social Media Minimum Age) Act 2024. This legislation, effective immediately, grants regulators the authority to impose fines up to A$50 million on companies that fail to prevent minors from accessing their platforms. The European Union is considering similar bans. Meanwhile, France has instituted a law requiring age verification for websites with pornographic material, facing protests from adult website operators.

Indicators suggest that such legislation may indeed be effective. The UK’s regulatory body, Ofcom, recently fined AVS Group, which runs 18 adult websites, £1 million for not implementing adequate measures to restrict children’s access. Other companies are being urged to enhance their efforts to comply with these new regulations.

Concerns surrounding the use of technology for age verification are growing, with some sites utilizing facial recognition tools that can be tricked with screenshots of video game characters. Moreover, VPNs allow users to masquerade as being from regions without strict age verification requirements. Following the onset of the OSA, search attempts for VPNs have surged, with reports indicating as much as a 1800% increase in daily registrations following the law’s implementation. The most prominent adult site experienced a 77% decline in UK visitors in the aftermath of the OSA, as users changed their settings to appear as if they were located in countries where age verification isn’t enforced.

The Children’s Commissioner for England emphasized that these loopholes need to be addressed and has made recommendations for age verification measures to prevent children from using VPNs. Despite this, many argue that such responses address symptoms rather than the root of the problem. So, what is the appropriate course of action?

Andrew Coun, a former member of Meta and TikTok’s safety and moderation teams, opines that harmful content isn’t deliberately targeted at children. Instead, he argues that algorithms aim to maximize engagement, subsequently boosting ad revenue. This creates skepticism regarding the genuine willingness of tech companies to protect kids, as tighter restrictions could harm their profits.

“It’s exceedingly unlikely that they will prioritize compliance,” he remarked, noting the inherent conflict between their interests and public welfare. “Ultimately, profits are a primary concern, and they will likely fulfill only the minimum requirements to comply.”

Graham Murdoch, a researcher at Loughborough University, believes the surge in online safety regulations will likely yield disappointment, as policymaking typically lags behind the rapid advancements of technology firms. He advocates for the establishment of a national internet service complete with its own search engine and social platforms, guided by a public charter akin to that of the BBC.

“The Internet should be regarded as a public service because of the immense value it offers to everyday life,” Murdoch stated. “We stand at a pivotal moment; if decisive action isn’t taken soon, returning to our current trajectory will be impossible.”

Topics:

Source: www.newscientist.com

How Virtual Reality Farming Will Transform the Future of Food Supply

Agriculture has long been a skilled and high-pressure profession, but modern farmers encounter challenges that even our grandparents could not have imagined.

In the UK, extreme weather is severely impacting agricultural lands. A recent survey revealed that 84% of farmers have witnessed a drop in crop yields or livestock production. This decline stems from a mix of heavy rain, drought, and extreme heat. Coupled with labor shortages, escalating machinery costs, and the demand to produce more food with fewer resources, the outlook for British agriculture appears increasingly uncertain.

As these issues escalate, innovations have surged. One of the most surprising solutions isn’t a cutting-edge tractor, miracle fertilizer, or genetically enhanced supercrops. Instead, it’s virtual reality (VR). This immersive technology, typically associated with gaming, is gradually becoming essential for the agricultural sector.

Here are five ways VR can pave the way for resilient farms and safeguard the food supply for an expanding population.

Life-saving VR Simulator

Operating a tractor is a daily task on the farm, but it can be daunting for new drivers. Tractors may be slow, but they can pose serious risks.

Rural roadways are infamous for narrow lanes, mud, hidden ditches, overgrown hedges, and blind turns, all of which can lead to serious accidents. Statistics indicate higher accident risks.

To combat this, researchers at Nottingham Trent University have developed a tractor-specific VR hazard perception test. Utilizing 360-degree footage from a tractor’s perspective, learners can experience real-life scenarios. Farmers report these situations as highly dangerous: hidden bikes, potholes, tight corners, and vehicles that regard 14-ton tractors as mere obstacles.

In trials with over 100 drivers, many, particularly those with past accidents, struggled to recognize hazards in time. It’s evident that traditional training doesn’t suffice, as tractors have distinct turning radii, slower speeds, and unique blind spots compared to cars.

There’s hope that this VR training could become a standard educational tool in universities and young farmers’ clubs, ensuring safer driving practices before they venture onto the roads.

Hone Your Skills in VR

VR is also training the next generation of vineyard workers safely, minimizing the risk of harming the vines. The Maara Tech project in New Zealand has created a system enabling trainees to practice vine cutting indoors, even on rainy days. Pruning in wet conditions carries significant risks, exposing fresh cuts to moisture, which can lead to fungal diseases.

Researchers at Eurecat, a European R&D center collaborating with several universities on agricultural innovations, have advanced this concept further. They’ve developed VR pruning shears equipped with sensors that guide users on the correct pressure, angle, and technique. It’s not just about speed; precision is crucial.

Accurate cuts result in healthier grapes, leading to superior quality and fewer errors. Since this training is virtual, new workers can build their confidence and help alleviate seasonal labor shortages.

Mindfulness with VR Headsets

Agriculture is not just physically demanding; it’s also mentally taxing. When adverse weather ruins planting schedules, drought devastates fields, and costs soar, even the most resilient farmers can reach their breaking point.

It’s perhaps unsurprising that 95% of farmers under 40 believe that mental health issues are the biggest hidden struggle they face in agriculture.

In response, researchers at the University of East Anglia have initiated the Rural Mind Project, employing a 360-degree VR experience to immerse healthcare professionals, policymakers, and support workers in real farming scenarios—addressing issues like isolation, anxiety due to weather, and financial pressures.

This initiative goes beyond fostering empathy; it aims to facilitate tangible change. VR training is equipping practitioners to recognize rural-specific stressors, find effective support strategies, and dismantle the stigma associated with seeking help.

Unlike conventional therapy, where the presence of a psychiatrist may induce anxiety, farmers can practice coping methods in a tranquil virtual setting designed for rural challenges. Initial feedback suggests VR may reach individuals who would typically avoid seeking assistance.

While it’s not a complete solution, it’s a promising step towards making mental health care as accessible as checking the weather forecast.

Learn the Ropes Without the Mess

Not only does VR help in understanding farm life, but it also provides the younger generation a head start without the mess, fertilizers, or early wake-ups.

Through the DIVE4Ag project at Oregon State University, schoolchildren can embark on virtual field trips via their gadgets, exploring dairy farms, urban gardens, and aquaculture facilities.

Meanwhile, at Lala Lajpat Rai University of Veterinary and Animal Science in India, the AR/VR Experience Center offers agricultural students interactive lessons on crop cultivation, animal care, and modern production methods.

As immersive VR education gains traction, it sparks excitement and confidence, motivating the upcoming generation to consider agricultural careers long before stepping onto a physical farm.

Stepping into the Metaverse

If VR can train farmers effectively, support their mental well-being, and educate them about agriculture, why not extend these benefits to animals? In Turkey, one adventurous dairy farmer has started using VR goggles on his cows while they are comfortably housed in a barn, allowing them to view lush pastures accompanied by soft classical music.

The goal was to create a serene atmosphere to reduce stress and potentially enhance milk output. Early results have been remarkable, as average production climbed from 22 to 27 liters per cow per day.

This approach might seem quirky, but managing cows indoors during extreme climates allows for better control over their feeding, milking, and overall health, suggesting that the future of farming may indeed lie where livestock engage with the metaverse.

From safer tractor operations to calming cows using VR, this technology is demonstrating its value beyond mere gaming. It offers a glimpse into the future of agriculture. EIT Food showcases these innovations, merging visionary concepts with practical solutions to illustrate how immersive technology can make agriculture smarter, safer, and more sustainable for all.

Source: www.sciencefocus.com

Intestinal Parasites Found in Roman Soldiers Stationed at Hadrian’s Wall

Third-century baths and sanitary facilities at Vindolanda, a Roman stronghold near Hadrian’s Wall in England

Vindolanda Trust

Although the Romans were recognized for their sophisticated sanitation systems, those stationed in major forts in northern England likely endured numerous digestive illnesses caused by parasites.

The Vindolanda Fortress, situated close to Hadrian’s Wall and inhabited by Roman soldiers from the 1st to 4th century AD, was likely not suitable for individuals with sensitive stomachs, as excavations of waste pits at this location indicate.

Piers Mitchell and his team from the University of Cambridge collected and examined nearly 60 sediment samples from the communal toilets believed to have been utilized in the 3rd century.

Utilizing microscopy, they discovered the eggs of two intestinal parasites: roundworms and whipworms. Additionally, they identified a one-celled parasite called duodenal giardia through specific antibodies that bind exclusively to proteins found in this organism.

All three parasites can lead to gastrointestinal issues, which can be particularly severe for children, the elderly, and immunocompromised individuals.

“Even with our efforts to implement Roman conveniences like baths and toilets, we still faced diarrhea and intestinal parasitic diseases,” Mitchell remarked.

Structures such as toilets, baths, aqueducts, and fountains primarily served to enhance air quality and maintain visible cleanliness, he explains. “They lacked microscopes and therefore were unaware of many infections that plagued them.”

Whipworm eggs discovered in a sewer pipe in Vindolanda

Marissa Ledger

Excavations at another nearby fort, occupied in the 1st century AD and believed to have defensive ditches, also revealed roundworms and whipworms.

“The contents of the sewage drains consist of mixed fecal matter from various individuals utilizing the toilets, making it difficult to determine the infection rate among soldiers,” Mitchell states. “However, the presence of parasite eggs along the sewer drains implies that a considerable number of individuals using the facilities were likely infected.”

Roundworms and whipworms are also found throughout the Roman Empire; giardia, however, has only been identified in the Roman contexts in Turkey and Italy, according to Mitchell.

If asked whether he would like a glass of water during the time the fort was operational, he would certainly decline. “They might say, ‘How about a beer instead?'”

Exploring Hadrian’s Wall and Roman Innovations: England

Embark on an immersive walking tour tracing the paths of the Romans along Hadrian’s Wall, one of Britain’s most iconic ancient sites and a UNESCO World Heritage gem.

Topic:

  • Archaeology/
  • Infectious disease

Source: www.newscientist.com

Jurassic Dinosaur Fossils Illuminate the Evolution of Flight

Paleontologists studied fossils that are 160 million years old. Anchiornis Huxley, a non-avian theropod dinosaur, was unearthed from the Late Jurassic Tianjishan Formation in northeastern China. The preserved feathers indicated that these dinosaurs had lost their flying capability. This rare find offers insights into the functions of organisms that existed 160 million years ago and their role in the evolution of flight among dinosaurs and birds.

This fossil of Anchiornis Huxley has nearly complete feathers and coloration preserved, allowing for detailed identification of feather morphology. Image credit: Kiat et al., doi: 10.1038/s42003-025-09019-2.

“This discovery has significant implications, suggesting that the evolution of flight in dinosaurs and birds was more intricate than previously understood,” said paleontologist Yosef Kiat from Tel Aviv University and his team.

“It is possible that some species had rudimentary flight abilities but lost them as they evolved.”

“The lineage of dinosaurs diverged from other reptiles approximately 240 million years ago.”

“Shortly after (on an evolutionary timeline), many dinosaurs began developing feathers, unique structures that are lightweight and strong, made of protein, and primarily used for flight and thermoregulation.”

About 175 million years ago, feathered dinosaurs, known as Penaraputra, emerged as distant ancestors of modern birds; they are the only dinosaur lineage that survived the mass extinction marking the end of the Mesozoic Era 66 million years ago.

As far as we know, the Pennaraputra group developed feathers for flight, but some may have lost that capability due to changing environmental conditions, similar to modern ostriches and penguins.

In this study, the researchers examined nine specimens of a feathered pennaraptorian dinosaur species called Anchiornis Huxley.

This rare paleontological find, along with hundreds of similar fossils, had its feathers remarkably preserved due to the unique conditions present during their fossilization.

Specifically, the nine fossils analyzed were selected because they retained the color of their wing feathers: white with black spots on the tips.

“Feathers take about two to three weeks to grow,” explains Dr. Kiat.

“Once they reach their final size, they detach from the blood vessels that nourished them during growth and become dead material.”

“Over time, birds shed and replace their feathers in a process known as molting, which is crucial for flight.” He notes that birds that depend on flight molt in an organized and gradual manner, maintaining symmetry and allowing them to continue flying during the process.

Conversely, the molting of flightless birds tends to be more random and irregular.

“Molting patterns can indicate whether a winged creature was capable of flight.”

By examining the color of the feathers preserved in dinosaur fossils from China, researchers could reconstruct the wing structure, which featured series of black spots along the edges.

Additionally, newly grown feathers, which had not fully matured, were identifiable by their deviation in black spot patterns.

A detailed analysis of the new feathers in nine fossils revealed an irregular molting process.

“Based on our understanding of contemporary birds, we identified a molting pattern suggesting these dinosaurs were likely flightless,” said Dr. Kiat.

“This is a rare and particularly intriguing discovery. The preservation of feather color offers a unique opportunity to explore the functional characteristics of ancient organisms alongside body structures found in fossilized skeletons and bones.”

“While feather molting might seem like a minor detail, it could significantly alter our understanding of the origins of flight when examined in fossils,” he added.

Anchiornis Huxley‘s inclusion in the group of feathered dinosaurs that couldn’t fly underscores the complexity and diversity of wing evolution.”

The findings were published in the journal Communication Biology.

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Y. Kiat et al. 2025. Wing morphology of Anchiornis Huxley and the evolution of molting strategies in paraavian dinosaurs. Communication Biology August 1633. doi: 10.1038/s42003-025-09019-2

Source: www.sci.news

Asteroid Collision Near a Nearby Star Unravels Cosmic Mystery

Composite image of Fomalhaut’s dust belt (center hidden). The inset displays dust cloud cs1 taken in 2012 together with dust cloud cs2 from 2023.

NASA, ESA, Paul Karas/University of California, Berkeley

Around the star Fomalhaut, asteroids are involved in collisions that generate massive dust clouds. This is the first time astronomers are witnessing these events, offering insights into the early days of our solar system.

Fomalhaut has had its share of unusual findings. In 2008, Paul Kalas, based on observations from the Hubble Space Telescope in 2004 and 2005, reported a potential giant planet orbiting the young star. Over the years, however, the nature of this peculiar object, dubbed Fomalhaut b, has sparked heated debates. It could either be a planet slightly larger than Jupiter or simply a cloud of debris.

Now, Kalas and his team have revisited Fomalhaut using Hubble. “In 2023, we utilized the same equipment as before, and Fomalhaut b was undetectable. It was effectively gone,” says Kalas, “What appeared was a new Fomalhaut b.”

This new bright feature, named Fomalhaut CS2 (short for “circumstellar light source”), cannot be a planet, as it would have been identified earlier. The leading theory is that it represents a dust cloud resulting from the collision of two large asteroids or planetesimals, each approximately 60 kilometers in diameter. The disappearance of Fomalhaut b implies that it may have been a similar dust cloud all along.

“These sources exhibit noise and instability, so we’re still far from drawing definitive conclusions,” notes David Kipping at Columbia University. “Yet, all existing evidence aligns well with a broader narrative of collisions between protoplanets in nascent systems.”

Interestingly, it’s unexpected to observe such a significant break twice. “The hypothesis suggests that we shouldn’t witness such impacts more than once every 100,000 years, if not even more infrequently. And yet, for some unexplained reason, we seem to observe it twice within 20 years,” Kalas explains. “Fomalhaut lights up like a holiday tree and it’s astounding.”

This might indicate that collisions among planetesimals are occurring more frequently than previously thought, particularly around relatively young stars like Fomalhaut. Kalas and his team plan to conduct further observations over the next three years utilizing both Hubble and the more powerful James Webb Space Telescope (JWST) to track the behavior of Fomalhaut CS2 and attempt to pick up faint signals from Fomalhaut b.

This presents a rare opportunity to witness these collisions first-hand. “To comprehend these violent phenomena, we no longer need to rely solely on theoretical models; we can observe them in real time,” Kalas states. Further observations may enlighten us not only about young planetary systems generally but also about our own early solar system’s position in the cosmic landscape.

“We have long pondered whether the collisions that formed our moon are typical of what occurs throughout the universe, and now we have strong evidence suggesting they are indeed common,” Kipping remarked. “Perhaps we are not as unique as some may assume.”

Exploring the Mysteries of the Universe: Cheshire, England

Join a weekend with some of science’s brightest minds as you delve into the mysteries of the universe, featuring a tour of the renowned Lovell Telescope.

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Source: www.newscientist.com

Europa Clipper Presents a Distinct View of 3I/ATLAS

Utilizing the Ultraviolet Spectroscopy (UVS) instrument onboard NASA’s Europa Clipper spacecraft, scientists have made significant observations of 3I/ATLAS. This interstellar object is the third and only confirmed of its kind to have been detected entering our solar system from beyond it. While many telescopes on Earth and Mars struggled to track such interstellar visitors due to their proximity to the Sun, Europa Clipper was able to gather data from a distinct position as it advanced towards Jupiter.

This composite image of interstellar comet 3I/ATLAS was captured on November 6, 2025, by the UVS instrument aboard NASA’s Europa Clipper spacecraft from a distance of around 164 million kilometers (103 million miles). Image Credit: NASA/JPL-Caltech/SwRI.

Scheduled to launch in 2024 and reach the Jupiter system by 2030, Europa Clipper will orbit Jupiter and conduct 49 flybys of its icy moon, Europa.

The UVS instrument specializes in collecting ultraviolet light to analyze the composition of Europa’s atmospheric gases and the materials on its icy surface.

Dr. Curt Retherford, principal investigator for Europa-UVS and a research scientist at the Southwest Research Institute, remarked, “This unexpected opportunity to observe another target on its journey to Jupiter has us very excited.”

“Our observations offer a distinctive and detailed view of the comet.”

Discovered on July 1, 2025, by the NASA-funded ATLAS survey telescope in Rio Hurtado, Chile, 3I/ATLAS was traveling at a heliocentric distance of 4.51 astronomical units (AU) with an eccentricity of 6.13 at that time.

Within a week of its discovery, the Jet Propulsion Laboratory’s analysts had determined its trajectory through the solar system.

The Europa Clipper team quickly identified that their spacecraft could view 3I/ATLAS in November 2025, especially after Earth-based observations were largely obstructed by the Sun’s position and Mars observations became optimal.

During this period, the spacecraft provided crucial data between the Mars observations in September and upcoming Earth-based exams.

With the comet’s trajectory aligning between Europa Clipper and the Sun, the UVS team was able to observe it from a distinctive angle.

Comets feature a dust tail that trails behind and a plasma tail that extends away from the Sun.

The Europa-UVS’s unique sunward perspective enabled a rare downstream view of the comet’s two tails, primarily observing from behind the tail and toward the comet’s core and coma.

“We anticipate that this new perspective, together with data from Earth-based assets and other spacecraft, will enhance our understanding of the tail’s shape,” stated Dr. Thomas Greathouse, co-principal investigator for the Europa-UVS study.

The UVS instrument identified signatures associated with oxygen, hydrogen, and dust, reinforcing evidence of significant outgassing activity from 3I/ATLAS shortly after its closest approach to the Sun.

“Europa-UVS excels at measuring fundamental transitions of atoms and molecules,” remarked Dr. Retherford.

“We can observe gas being expelled from the comet, along with water molecules splitting into hydrogen and oxygen atoms.”

This capability allows Europa Clipper to closely analyze and measure these atomic species, offering deeper insights into the comet’s processes and composition.

“By understanding the chemical makeup of comets and how readily these gases are ejected, we can better comprehend their origins and evolution as they traverse from distant parts of the galaxy to our solar system,” explained Dr. Tracy Becker, co-principal investigator for Europa and UVS, also at the Southwest Research Institute.

“What chemical processes occur? How can we grasp the origins of comets within our solar system?”

“Are these processes akin to our theories about the formation of the solar system? That’s a key question.”

Source: www.sci.news

US Lab Closure Will Significantly Hinder Climate Research

National Center for Atmospheric Research in Boulder, Colorado

Matthew Jonas/MediaNews Group/Boulder Daily Camera (via Getty Images)

The decision by the Trump administration to shut down the premier center for atmospheric research could jeopardize weather forecasting and climate modeling, increasing the risks posed by global warming.

In a statement to USA Today, White House official Russ Vought mentioned that the National Center for Atmospheric Research (NCAR) is viewed as a source of “climate change concerns” and will be disbanded. The plan includes the discontinuation of Green New Fraud Research, with “essential capacities” like weather modeling and supercomputing to be relocated.

NCAR’s models provide vital support for reports from the United Nations’ Intergovernmental Panel on Climate Change, which are crucial for countries in establishing measures to lower carbon emissions and adapt to severe weather.

“Ceasing operations would amplify uncertainty regarding our climate future and hinder our preparation efforts,” asserts Michael Meredith from the British Antarctic Survey. “It’s difficult to view this as anything other than silencing the messenger.”

Established in 1960 to advance atmospheric science, NCAR employs 830 individuals conducting research that spans “from the ocean floor to the core of the sun.” According to its unofficial motto, it manages programs monitoring everything from floods and wildfires to space weather.

NCAR developed the GPS dropsonde, a device equipped with sensors that is deployed into hurricanes, significantly enhancing our understanding of tropical cyclones. This has started a revolution in weather research. The researchers also designed a wind shear warning system for airports, saving numerous lives by preventing crashes.

However, one of its major contributions lies in providing data, modeling, and supercomputing resources to other researching entities. Weather Underground, one of the pioneers in offering localized weather forecasts online in the 1990s, credits its founding on the software and weather data developed by NCAR, according to meteorologist Jeff Masters.

NCAR is responsible for developing and managing weather research and forecasting models that are extensively utilized for daily forecasts and regional climate studies. They will continue to collaborate with the National Oceanic and Atmospheric Administration to enhance weather modeling aimed at predicting extreme storms.

If this critical work faces disruption, it could lead to a decline in the accuracy of weather apps and TV news forecasts at a time when abnormal weather patterns are increasingly frequent. Masters likens the situation to “halting weapons research and development on the eve of World War II.”

“Without knowledge of impending dangers, more lives will be at stake,” he warns.

NCAR oversees the Community Earth System Model (CESM), the first global climate model developed specifically for universities. CESM facilitates diverse research efforts, from estimating current global carbon emissions to predicting upcoming changes in ocean currents, heat wave frequency, and ice melt.

“This model is arguably the most utilized globally,” states Richard Rood at the University of Michigan.

Twice a year, NCAR organizes user meetings to gather insights on improving the model, which can be operated on a server or downloaded for local modifications. The closure may jeopardize the ongoing maintenance and development of CESM and its bug fixes.

Colin Carlson from Yale University was among numerous scientists who took to social media to highlight NCAR’s importance. He utilizes climate models to predict the requirements for cholera and yellow fever vaccines as the climate evolves and anticipates dengue fever outbreaks in Florida. “We need NCAR to perform our roles effectively,” Carlson emphasized in a recent post.

NCAR also operates a modified C-130 cargo plane and a Gulfstream business jet designed for research purposes, reaching the stratosphere and facilitating the operation of King Air propeller planes that study cloud physics.

From 2009 to 2011, the Gulfstream jet successfully conducted its inaugural comprehensive flight, traversing from the North to South Poles multiple times and reaching altitudes between 150 meters and 9000 meters. Their investigation measured CO2 and other atmospheric gases. They also gathered data on solar corona during the 2017 solar eclipse.

Rood noted that the aircraft assists in monitoring air pollution and calibrating satellite instruments.

The research conducted by NCAR on aerosols is crucial for understanding geoengineering effects, especially proposals aimed at mitigating abrupt climate changes through aerosol diffusion to shield sunlight.

“Elimination of such climate research will lead to decisions regarding geoengineering and tipping points being made in a blind manner,” Rood cautioned.

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Source: www.newscientist.com