High Temperatures Above 90 Degrees Reported Northeast of New England

LAS VEGAS – The severe heatwave plaguing the Southwest is anticipated to move eastward in the coming days, with temperatures surpassing 90 degrees Fahrenheit expected in the northeast, particularly in parts of New England later this week.

Around 15 million individuals are currently facing extreme heat advisories in eastern California, Nevada, Arizona, and western Texas. Triple-digit temperatures are projected to become widespread throughout the area by Wednesday.

In southern Nevada, temperatures this week may rise up to 12°F above the seasonal average, as reported by the National Weather Service. Nearby Arizona is predicted to see highs reaching 115°F across its southern and central regions.

As the week progresses, this heat will extend into the Midwest and Great Lakes, leading to the region’s first significant heat wave this weekend.

The Weather Service has indicated that record high temperatures are possible from Northern and Eastern Colorado to Nebraska and South Dakota on Thursday, affecting parts of the Great Basin and western South Dakota.

Research indicates that climate change may contribute to more frequent, intense, and prolonged heat waves.

Warm temperatures combined with high humidity will affect the East Coast this weekend and into next week. In major cities like New York City, Boston, and Washington, DC, the thermal index (the combined effect of temperature and humidity on how hot it feels) is expected to reach the mid-90s or higher.

“Starting early next week, we will see a stretch of prolonged hot and humid weather beginning Sunday and lasting through at least mid-week,” according to the New York branch of the Weather Bureau, as noted in a post on X.

Meanwhile, extreme heat is forecasted to persist across southwestern desert regions, including Death Valley, for the remainder of the week, as per the weather services.

Source: www.nbcnews.com

Honda Announces Successful Test of Its Reusable Rocket

Honda’s newest initiative is literally reaching new heights.

On Wednesday, the Japanese automaker revealed that it has successfully developed its own “experimental reusable rocket,” which has completed a landing. According to company representatives, the roughly 21-foot tall booster achieved an altitude of 890 feet before landing vertically.

These test flights indicate that the global landscape of space operations is expanding towards the commercial sector, moving beyond a handful of government agencies.

While Honda has not yet shared specific plans on how it aims to commercialize its rocket technology or the intended applications of its boosters, the initiative is part of Honda’s commitment to “sustainable transport.”

“We view rocket research as a substantial endeavor that leverages Honda’s technological capabilities,” stated Toshihiro Mibe, Honda’s global CEO in a statement.

The test launch and landing occurred on Tuesday at a Honda facility located in Taika Town, Hokkaido Prefecture. The flight duration was 56.6 seconds, with the rocket landing within approximately 15 inches of the designated target area.

Honda aims to achieve a suborbital launch by 2029. This type of flight does not achieve a complete orbit around Earth, but reaches the edge of space at altitudes exceeding 65 miles.

Although Honda initially announced its foray into the space industry in 2021, details about ongoing projects or potential applications remain scarce. The company indicated that this endeavor builds on other Honda initiatives, including efforts related to automated driving systems.

“We are witnessing an exponential increase in data consumption, and the proliferation of satellites has raised expectations for utilizing data systems in space,” noted a company representative in a news release. “Considering this trend, the demand for satellite launch rockets is anticipated to rise significantly in the coming years.”

Reusable rockets are increasingly viewed as a method to enhance the sustainability and cost-efficiency of space launches. US company SpaceX continues to lead the industry with its reusable Falcon 9 rocket, while also developing a next-generation booster known as Starship, which is expected to be fully reusable.

Source: www.nbcnews.com

Australian Moths Navigate 1000 km Journeys Using the Stars as Their Compass

Bogong moths seek refuge in cooler caves during the summer

Ajay Narendra/Macquarie University, Australia

Traveling distances exceeding 1,000 kilometers to escape the summer heat, Australia’s moths have been identified as the first invertebrates to utilize stars for navigation on long migrations.

Every spring, billions of bogong moths (Agrotis infusa) embark from various regions of southern Australia, surviving the winter as caterpillars by feeding on vegetation before retreating to the cool caves of Australia’s Alpine regions. Once in the caves, they enter a state of dormancy known as estivation until they return to breeding grounds.

The recent decline of these moth populations has led to inquiries about their navigation methods in reaching high-altitude caves, as noted by Andrea Aden from the Francis Crick Institute in London.

Previous studies have demonstrated their ability to use Earth’s electromagnetic fields but only in conjunction with visible landmarks. Aden and her team sought to explore other potential cues that moths might use for navigation.

“When you venture into the Australian bush at night, one of the most striking visual markers is the Milky Way,” she explains. “We know that diurnal migratory birds rely on the sun, so testing whether moths use the starry sky seemed like a logical step.”

To investigate, the team employed light traps to capture moths during migration and transported them to a laboratory. There, they were placed in a Perspex arena with images of a night sky projected overhead. Moths were free to choose their flight direction based on the sky images while the Earth’s magnetic field was neutralized using a Helmholtz coil.

Experiments revealed that moths did utilize a stellar compass, according to team member Eric Warrant from Lund University, Sweden. “When the tethered moths were placed under a realistic starry sky, they oriented themselves towards their migratory direction,” he states. “They achieved this solely with the assistance of these stars, independent of other visual cues and the magnetic field.”

Caption: Aestivating moths in alpine caves during summer (roughly 17,000 per square meter, with millions in each cave) Copyright: Eric Warrant

Eric Warrant

When the simulated starry sky was rotated 180 degrees, the moth flew in the opposite direction. Randomizing the star placements in the image left them disoriented.

In a subsequent experiment, very thin electrodes were implanted in the moth’s brain, revealing changes in neural activity as the projected starfield was rotated.

While dung beetles are known to maintain a consistent bearing using the Milky Way, no other insect species has previously demonstrated this level of celestial navigation.

“The bogong moth is the first invertebrate documented with the ability to navigate long distances using stars as a compass—a phenomenon previously recognized only in certain birds and humans,” Warrant states. “This capability is truly remarkable.”

Another insect recognized for its extensive migrations, the Monarch butterfly (Danaus plexippus), primarily relies on the sun supplemented by the environment.

Cody Freas from Macquarie University in Sydney, Australia, emphasized the incredible efficiency of insect navigation, stating, “Stellar navigation showcases the remarkable visual acuity found in nocturnal insects, enabling them to utilize various cues (Sun, Moon, Stars) even in low-light conditions,” adds Freas.

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Source: www.newscientist.com

Rapamycin May Boost Lifespan More Significantly with Reduced Caloric Intake

An illustration depicting the drug rapamycin (red) inhibiting the protein complex MTORC1, influencing cell functionality

Science Photo Library/Getty Images

The drug rapamycin shows effects on life extension that are nearly comparable to calorie restriction, based on the largest study exploring the lifespan of various vertebrate species.

Researchers are probing if lifestyle changes like diet and exercise can enhance longevity while mitigating aging-related health issues. For instance, calorie restriction, when balanced with nutritional needs, has demonstrated extensions of lifespan in non-human animals of up to 40%.

“In our field, we have long recognized that calorie restriction often yields positive results,” says Matt Kaeberlein, who was not involved in the recent research from Washington University in Seattle.

Another area of interest lies with potential anti-aging medications, such as rapamycin, initially developed as an immunosuppressant. The combination of rapamycin with the cancer treatment trametinib has shown a 30% increase in mouse lifespan earlier this year.

Currently, Zahida Sultanova from the University of East Anglia, along with her collaborators, is reviewing data from 167 studies on lifespan interventions across eight vertebrate species, such as fish, mice, rats, and rhesus monkeys, though not in humans.

The findings indicated that dietary restrictions, regardless of whether they primarily involve calorie reduction or intermittent fasting, extend the lifespan of all eight species, regardless of sex. Rapamycin appears to produce effects similar to these. They also examined the type 2 diabetes medication metformin, which has been suggested as a potential longevity stimulant, but found no benefits regarding lifespan.

However, Sultanova advises against individuals self-prescribing rapamycin based on these findings. “High doses of rapamycin can have side effects, as it is designed to suppress the immune system,” she states, noting that studies in mice have indicated it might affect reproduction. Nonetheless, early data from a recent trial suggest low-dose rapamycin is relatively safe for healthy elderly individuals.

Kaeberlein also warns against using medication or limiting calories solely to combat aging, as this could be linked to physical debilitation and mental health issues. “We must better understand the ratio of risks to rewards in humans before making such decisions,” he states. “Rapamycin might be beneficial for certain individuals, and ongoing research aims to clarify who those individuals are.”

Other medications similar to rapamycin, termed Rapalogs, might offer even more promising options with fewer adverse effects for lifespan extension, claims Sultanova.

Kaeberlein adds that while these results align with existing literature, “the effect sizes observed in shorter lifespans typically surpass those in longer ones, so caution is warranted when comparing across species.”

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Source: www.newscientist.com

We’ve Unveiled the Appearance of Denisovans!

The human skull from Harbin, China, is currently identified as Denisovan

Hebei Geo University

Denisovans, an enigmatic group of ancient humans, were initially recognized solely through their DNA, but now they have a distinct appearance.

With molecular data, Qiaomei Fu and her team at the Institute for Vertebrate Paleontology and Paleoanthropology have validated long-held suspicions among researchers.

This aligns with additional evidence that Denisovans were robust and heavyset. “I believe we observe individuals weighing around 100 kg of lean body mass: a truly massive individual,” stated Bens Viola, who was not part of the research team from the University of Toronto, Canada.

Denisovans were first discovered in 2010 in the Denisova Cave in Siberia’s Altai Mountains, where researchers found fragments of an unknown ancient hominin’s finger bone. The preserved DNA concluded that it was neither modern humans (Homo sapiens) nor Neanderthals (Homo neanderthalensis), but rather an entirely new species.

Moreover, genetic findings indicated that Denisovans interbred with contemporary humans. Today, populations in Southeast Asia and Melanesia carry up to 5% of Denisovan DNA, signifying their earlier presence in Asia.

Following these revelations, researchers commenced their quest for Denisovan fossils in both fieldwork and museum collections. Several fossils have since been discovered, with a notable mandible found in the Baishaya Karst Cave on the Tibetan Plateau, confirmed through fossil and DNA protein analysis from surrounding sediments. Recently, a jawbone recovered from the Peng Channel off Taiwan’s coast was also confirmed as Denisovan through preserved proteins.

Nevertheless, there remained frustrating gaps, as all confirmed Denisovan fossils obtained via molecular evidence were small, leading to limited insight. Conversely, more complete fossils from Asia were considered candidate Denisovan remains, yet none yielded molecular evidence.

Fu and her team aimed to extract preserved DNA or proteins from the human skull discovered in Harbin, northeastern China. This skull, kept under wraps for decades, was first described in 2021 and is notably large and robust, characterized by prominent brow ridges and brain size similar to modern humans. It has been dubbed Homo longi—or Dragon Man—by its discoverer.

“My impression is that this specimen is representative of what we would expect Denisovan to be, in both size and context,” Viola remarked.

Fu noted that recovering preserved molecules from the Harbin skull was an arduous task. While her team struggled to obtain DNA from the bones, they successfully retrieved 95 proteins, including three variants unique to Denisovans.

Seeking further evidence, Fu turned to dental calculus, a hardened plaque that forms on teeth, which yielded mitochondrial DNA inherited from its maternal lineage. Although she described the quantity as “small,” it was sufficient to confirm the specimen as Denisovan.

“It’s an astonishing outcome, and the efforts made were commendable,” said Saman Subroun from the National Research Centre in Burgos, Spain. “I believe many researchers tend to overlook dental calculus in genetic studies.”

With the identification of the robust Harbin skull as Denisovan, the long-suspected notion of their substantial size is now validated.

“There was a clue,” Brown noted.

The reason for their size remains unclear. Neanderthals’ robust build is linked to the cold climates of Europe and West Asia where they thrived. While Denisovan sites, including Denisova Cave and the Tibetan Plateau, were also cold, others were tropical. “We need to contemplate the implications of this,” Viola stated.

It’s possible that Denisovans varied over time. The fragments from Denisova Cave suggest two distinct groups existed: one from 217,000 to 106,000 years ago and another from 84,000 to 52,000 years ago. The Harbin skull dates back at least 146,000 years, with Fu discovering that its proteins and mitochondrial DNA align with the older group. Nevertheless, we’ve yet to locate any large Denisovan fossils in contemporary times, leaving their full appearance uncertain.

“Numerous different groups inhabited the landscape independently, often isolated from each other for tens of thousands of years,” Viola remarked. We should not presume they all bore a similar appearance.

Topic:

  • Denisovan/
  • Ancient humans

Source: www.newscientist.com

Farmers Worldwide Struggle to Adapt to Climate Change

Climate change will lessen the availability of most staple crops, including corn

Jon Rehg/Shutterstock

Despite farmers’ best efforts to adapt, increasing global temperatures have the potential to significantly impact the world’s essential crops. Comprehensive analysis indicates that by the century’s end, for every degree of warming, global food supply may drop by nearly 121 kcal per person per day.

In a 3°C warming scenario—aligned with current trends—”It might mean skipping breakfast for everyone,” notes Andrew Hartgren from the University of Illinois, Urbana-Champaign.

Hartgren and his team gathered data on the yields of six major staple crops globally, which account for over two-thirds of the world’s calories. “This represents one of the largest datasets currently available for high-resolution crop yields,” he states. They also incorporated local weather information from 54 different countries.

The researchers utilized this data to forecast how various crops would respond to climate changes and how farmers might adapt. “We examined historical data on how farmers have reacted to weather fluctuations,” Hartgren explains. This approach enabled the team to assess how different agricultural strategies might mitigate losses, like crop variety adjustments, enhancing irrigation, or increasing fertilizer use.

Except for rice, which thrives under warmer nighttime conditions, higher temperatures generally lead to considerable yield reductions. For instance, global corn yields are anticipated to decline by about 12% to 28% by the century’s end, contingent upon whether greenhouse gas emissions are moderate or extremely high compared to projections without climate change.

These statistics illustrate how farmers adjust to rising temperatures and the implications of potentially beneficial effects of climate change, like elevated carbon dioxide levels fertilizing crops. Both factors are significant. Without adjustments, for example, crop losses could reach a third by the century’s end under extreme warming scenarios, yet this won’t mitigate the majority of losses. “In a warmer future, the corn belt will still be relevant,” Hartgren asserts.

Wolfram Schlenker of Harvard University emphasizes that agricultural adaptations seldom completely offset crop losses due to climate change, with previous studies from specific regions suggesting similar conclusions. “The major strength of their research is its global perspective, compiling data from numerous countries,” he remarks.

The global approach reveals some fascinating patterns. For example, researchers observed that the most significant projected crop losses are not concentrated in low-income nations but rather in comparatively affluent agricultural hubs like the Midwest and Europe. “They aren’t inherently better suited than poorer countries,” Schlenker notes.

Michael Roberts from the University of Hawaii Manoa states that these findings align with the conclusions of a smaller study. However, he highlights considerable uncertainties, such as the extent of future climate change and the complexities of global food systems’ responses.

“What’s alarming is our lack of knowledge,” Roberts adds. “There’s significant uncertainty, much of which is negative. Losses could range from non-existent to catastrophic, potentially causing massive famines. It’s a sobering thought for many.”

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Source: www.newscientist.com

Morse Code Messages Encased in Ice Bubbles

ICE can provide a method for long-term message storage in cold climates

Anton Petrus/Getty Images

Messages can be preserved in ice for millennia simply by altering the shape and positioning of the internal bubbles present.

Mengjie Song and his team at China’s Beijing University of Technology were exploring ice formation when they discovered that it influences the size and shape of bubbles encapsulated within. For instance, they found that freezing a layer of water between plastic sheets resulted in either oval or needle-shaped foam, depending on the freezing rate.

The researchers assigned specific bubble sizes, shapes, and positions to represent characters in Morse and binary code. By controlling the freezing rate of water, they created ice that conveyed messages through the embedded bubbles.

Transforming this ice image to grayscale revealed that white areas indicated the presence of bubbles, while black areas indicated the absence of them. This allowed computers to identify the size and location of bubbles for message decoding.

Currently, the amount of information that can be stored in conventional ice cubes is minimal with existing technology. However, Song suggests that by manipulating foam in materials like plastic, greater capacities could be achieved.

He mentions that beyond the novelty of reading messages embedded in ice cubes used in beverages, this research has diverse potential applications. “The strength of this study lies in its capability to sustain information over extended periods in frigid environments like the Arctic and Antarctic,” Song notes.

He envisions a future where bubbles could safely contain ozone for food preservation or act as carriers for slow-release medications. He is particularly intrigued by how bubbles can inhibit ice formation on airplane wings and how this knowledge could inform behavior in lunar environments.

However, Qiang Tang from the University of Sydney is more skeptical about the practical implications of this research, asserting that significant information can be long-term stored on hard drives and paper.

He comments, “This represents a novel method for conveying messages, but from a security and encryption standpoint, I see little value in it—unless, of course, a polar bear has something to communicate,” he adds.

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Source: www.newscientist.com

28 Years Later: Danny Boyle’s Long-Awaited Zombie Sequel Triumphs

Infection after 28 years

Miya Mizuno/Sony

28 Years Later

Written by Danny Boyle and Alex Garland

In theaters from June 20th

Here’s a piece of scriptwriting advice: simplify the plot while adding complexity to the characters.

The narrative of 28 Years Later can be summarized in a few sentences. This long-awaited third chapter of the series that began in 2002 with 28 Days Later revolves around a neurotoxic virus that has spread uncontrollably across Europe, turning people into an army of infected (which some might call zombies, though the term isn’t explicitly used). The infection ultimately becomes contained within the UK, safeguarded by the International Fleet to prevent anyone from escaping the island.

A young boy named Spike (played by newcomer Alfie Williams) resides in the relative safety of a small northern island linked to the mainland by a causeway that is passable only at low tide. At 12 years old—an age his father thinks makes him ready—Spike ventures onto the mainland in search of adventure. He navigates through the possibly long-abandoned woods. While there may not be much tracking after 28 years, the film showcases Spike skillfully battling slow-moving zombies and avoiding the much quicker ones, all while providing some context for these encounters.

Upon his return, despite his mother (Jodie Comer) being bedridden with an unknown illness, Spike is hailed as a hero, while his father, Jamie (Aaron Taylor-Johnson), seeks comfort with another woman. Determined, Spike sneaks out to find the only doctor he knows about to help his mother.

Let’s throw in a twist. However, introducing a twist often implies that there isn’t one. Author Alex Garland, who set the rules of the world in 28 Days Later, stays true to his vision. The world is thriving yet shadowed by the remnants of an earlier outbreak, where some zombies have mutated, growing larger and posing new challenges. These are not just recycled dangers but add complexity within Spike’s idyllic yet troubled village.

Visually, the film offers a unique experience. Boyle incorporates elements reminiscent of Laurence Olivier’s Henry V wartime newsreels and original footage of the 28 Weeks Later outbreak, providing a contemplative layer to the community’s defenses. It evokes a sense of folk horror, nodding to films like Apocalypse Now and Alien 3. Yet, despite its depth, the film remains accessible, conveying themes of loss, disillusionment, and personal growth through the relatable actions of its characters.

The budget is reasonable (estimated between $60 million and $75 million), with a keen eye for casting (like Christopher Fulford as Spike’s grandfather, who brings depth to a tragic backstory). Don’t be mistaken: 28 Years Later is filled with clever nods and callbacks that will engage fans. However, there is no unnecessary complexity. No contrived MacGuffins, pointless quests, or mystical items. Spike’s journey, portrayed expertly by Alfie Williams, is a relatable and poignant evolution, where he learns that to grow into manhood, he must let go.

The acclaim for 28 Days Later back in 2002 still resonates, as does its 2007 sequel 28 Weeks Later, which was equally impressive. The crown for this genre, at least for now, belongs to 28 Years Later.

Boyle and Garland have triumphantly revisited the territory they first explored over two decades ago.

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Source: www.newscientist.com

Forget Super Intelligence – Let’s Address “Silly” AI First

Should politicians prioritize AI to aid in galaxy colonization, or should they safeguard individuals from the excessive influence of powerful tech? While the former seems more appealing, it’s not the primary concern.

Among the Silicon Valley elite, the emergence of super-intelligent AI is viewed as an imminent reality, with tech CEOs enthusiastically anticipating a golden age of progress in the 2030s. This perspective has permeated both Westminster and Washington, as think tanks encourage politicians to prepare to leverage the approaching AI capabilities. The Trump administration even backed a $500 billion initiative for a super AI data center.

While this sounds thrilling, the so-called “silly intelligence” is already creating issues, akin to the lofty aspirations of super intelligence. A pressing question in the AI sector revolves around whether the vast array of online content essential for training AI constitutes copyright infringement.

Arguments exist on both sides. Proponents assert that AI is not infringing when learning from existing content. New Scientist highlights that simply reading these words should enable AI to learn in the same fashion. Conversely, industry giants like Disney and Universal are opposing this view. They are suing AI company Midjourney for generating replicas of copyrighted images, from Darth Vader to his minions. Ultimately, only the law can reconcile this issue.

We are approaching a world where machines can cause death with minimal human oversight.

The ongoing conflict in Ukraine presents another pressing AI-related dilemma. Sam Altman from OpenAI warns about the potential dangers of advanced AI, noting that fatal, unintelligent AI already exists. The war has progressed towards a scenario where machines could effectively cause harm with minimal human oversight.

Politicians seem to have underestimated this threat. The United Nations convened its first meeting in 2014 to discuss the regulation of “killer robots.” If leaders expect time to resolve their challenges, they may be gravely mistaken.

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Source: www.newscientist.com

Top Non-Pharmacological Therapies for Alleviating Knee Osteoarthritis Pain

Knee braces appear to effectively alleviate the symptoms of osteoarthritis impacting the joints

Tom Werner/Getty Images

Knee braces and water-based exercises are among the most effective techniques for alleviating pain and stiffness associated with knee osteoarthritis. High-quality evidence is necessary before these methods can be universally recommended in clinical practice, as indicated by reviews of 12 non-pharmacological therapies.

This condition arises from the deterioration of cartilage, which cushions the edges of bones, leading to inflammation, discomfort, and stiffness. Pain relief medications and anti-inflammatory drugs can ease these symptoms, but side effects may occur, so healthcare providers often recommend physical therapy, such as shoe inserts to reduce knee pressure, tape for joint support, or laser therapy aimed at encouraging cartilage repair.

However, it remains uncertain how these treatments compare to one another. “Many reviews of treatments focus solely on the efficacy of individual therapies,” states Sarah Kingsbury, who was not part of the recent research conducted at the University of Leeds in the UK.

To address this gap, Yuan Luo from China’s First People’s Hospital and colleagues evaluated data from 139 randomized controlled trials examining 12 approved or experimental physiotherapy approaches for knee osteoarthritis. These trials included over 9,600 adults suffering from this condition.

Some studies compared two or three physical therapies, while others investigated one therapy against either a placebo or no treatment at all. Participants typically underwent treatment for several weeks before completing a symptom assessment.

Based on their findings, researchers concluded that knee braces effectively diminish pain and stiffness, emerging as the top method for enhancing mobility, followed by water-based exercise. “When you’re walking in a pool, you engage your muscles without stressing the joints in the same way walking in a park would,” says Kingsbury.

The ranking of efficacy for the other tested treatments is as follows: high-energy laser therapy, which delivers high-energy sound waves into the knee; low-energy laser therapy, which applies electrical stimulation to knee nerves; taping the knee; electromagnetic stimulation; ultrasound treatment; and wearing insoles.

Due to various factors, the findings are insufficiently robust to change clinical practices, Kingsbury notes. Many studies involved fewer than 50 participants, resulting in a limited sample size that can undermine confidence in the results. Additionally, treatment durations varied widely, from one week to less than a few months, which may skew perceptions of effectiveness.

Another limitation is that these studies did not juxtapose physical therapy with drug treatments or evaluate the efficacy of combining pharmaceutical and non-pharmaceutical interventions, Kingsbury points out.

Despite these limitations, the reviews offer valuable insights regarding the most effective approaches, she suggests. “Establishing this ranking is useful and crucial. It allows us to possibly exclude the least effective 6 to 10 therapies, enabling us to focus on strengthening the evidence surrounding a few selected treatments.”

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Source: www.newscientist.com

Research Reveals How This Easy Snack Habit Can Lower Your Cholesterol

Consuming 50g of almonds (approximately 45 nuts) each day can boost your cholesterol levels and provides numerous metabolic advantages.

This information comes from a recent study conducted by Oregon State University (OSU). The findings were published in Nutritional research.

Researchers engaged 77 adults aged 35-60 in a 12-week clinical trial, where participants snacked daily on either 320 calories of almonds or crackers.

All subjects had metabolic syndrome, characterized by various risk factors for chronic illnesses such as heart disease and type 2 diabetes. This includes conditions like excess abdominal fat, elevated blood pressure, high blood sugar levels, low “good” cholesterol, and high triglyceride levels.

Professor Emily Ho, a co-author of the study and director of the Linus Pauling Institute at OSU, noted in BBC Science Focus that almond consumption reduces cholesterol levels, particularly LDL cholesterol (“bad” cholesterol), enhances gut health, decreases inflammation, and improves gut microbiota.

“The control group that consumed crackers didn’t show the same positive outcomes,” she stated. “Eating almonds did not lead to weight gain; in fact, there was a minor reduction in waist circumference and an improvement in vitamin E levels among participants, which is vital for the population.”

Vitamin E is an essential nutrient crucial for the proper functioning of various organs, nerves, and muscles, as well as for reducing blood clotting; however, many individuals in the UK and the US fail to consume sufficient amounts of vitamin E in their diets.

Participants who consumed almonds daily experienced numerous benefits for their metabolic health – Credit: Limpido via Getty

“Almonds are packed with various bioactive compounds, including essential vitamins and minerals like vitamin E and magnesium, along with fiber and numerous polyphenols that possess antioxidant and anti-inflammatory properties. They are truly nutritious snacks.”

She emphasized that substituting your usual snack with a handful of almonds can yield substantial health benefits, especially when included in a balanced and varied diet.

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About our experts

Emily Ho is a prominent professor at Oregon State University and director of the Linus Pauling Institute. Her research focuses on antioxidants, gene expression, and dietary chemoprevention strategies, particularly investigating the role of antioxidant nutrients such as zinc in maintaining DNA integrity and the development of cancer.

Source: www.sciencefocus.com

Bogong Moths May Be Using Stars to Navigate Their 600-Mile Journey

“To our knowledge, Bogon Moss is the first species identified to navigate using stars,” said Andrea Aden, a postdoctoral researcher at the Francis Crick Institute in London, who contributed to this research.

The researchers uncovered the stellar navigation abilities of moths by capturing wild bogon moths and suspending them with fine tungsten rods inside a small cylindrical “flight simulator.”

With its back affixed to the rod, the moth flapped its wings within the simulator, allowing it to turn as if it were flying in a natural environment.

“It can rotate freely,” noted David Dreyer, a researcher at Lund University and a co-author of the study. “You can choose the direction you wish to fly.”

The researchers created a magnetic vacuum to neutralize the moth’s internal magnetic compass, allowing them to focus on other sensory inputs.

Images of the night sky were projected onto the top of the flight simulator.

During trials, researchers manipulated the rotation of the sky, noting that the moth adjusted its flight patterns to adapt and establish new headings. However, the moths became disoriented when presented with randomized, fragmented sky images within the simulator.

“The moths were entirely confused,” Dreyer explained. “For us, this served as compelling evidence that they indeed utilize stars for navigation.”

In additional experiments, researchers drilled a small opening in the moths’ brains, inserted a glass tube into a neuron, and recorded the electrical impulses triggered by star projections. They discovered that electrical activity peaked when a specific angle of the sky was depicted. Conversely, there was little response to randomly generated patterns.

According to the findings, Bogon Moss possesses limited vision and likely perceives only a select few of the brightest stars. The researchers suspect that these moths navigate by the Milky Way.

“They probably perceive the Milky Way much more vividly and luminously than we do,” stated Warrant.

Furthermore, Warrant proposes that moths likely utilize olfactory cues as they approach alpine caves.

“They are probably detecting compounds emitted from the cave—odorous markers that act as olfactory beacons leading them there,” he mentioned, adding that these smells resemble the scent of decaying meat.

These moths have a lifespan of about a year, spending a dormant summer in the cave before returning to their original location.

Ken Rohman, a professor at the University of North Carolina’s Department of Biology, noted that although he did not participate in the research, he found the study compelling, with experiments that were both thoughtful and rigorously controlled.

“One of the remarkable aspects of this study is how moths manage such extensive navigation with a relatively small brain,” said Roman, who studies animal migrations. “This highlights the ingenuity driven by natural selection.”

Bogon Moss is currently at risk and was listed by the United Nations for the Conservation of Nature in 2021. The authors assert that these new insights could assist in preventing the decline of the species.

“Moth populations have dramatically decreased in recent years, particularly due to the droughts and wildfires experienced in Australia in 2020,” added Aden. “Understanding that they rely on vision as part of their navigational toolkit can inform conservation strategies, especially concerning light pollution in urban settings.”

Source: www.nbcnews.com

Asteroid 2024 YR4: On a Collision Course with the Moon, Possible Effects on Earth

Asteroid 2024 YR4 may create the largest lunar impact in the past 5,000 years

Mark Garlic/Science Photo Library/Getty Images

Originally believed to be on a collision path with Earth, asteroid 2024 YR4 still poses some level of threat to our planet. There remains a chance that such celestial bodies could impact the moon, potentially resulting in a catastrophic explosion that could flood Earth with debris capable of damaging satellites.

Astronomers have been monitoring this building-sized asteroid since its detection in December 2024. Initial forecasts heightened the risk of a collision with Earth in 2032, suggesting the impact could unleash enough energy to obliterate a city; fortunately, it now appears 2024 YR4 will likely miss us.

Nonetheless, the likelihood of a lunar impact is gradually increasing, currently estimated at 4.3% based on observations made before the asteroid moved out of our telescopes’ view until 2028. Paul Wiegelt from the University of Western Ontario and his team suggest that such a collision could inflict significant damage on Earth’s satellites.

“We were somewhat taken aback by the amount of debris that could potentially reach Earth,” Wiegert remarked. “In reality, Earth is a surprisingly small target from the moon’s vantage point. Thus, while impacts on Earth are infrequent, gravitational forces can draw in that material under certain conditions.”

Wiegert and his colleagues calculated that 2024 YR4 could create a crater over a kilometer wide on the moon, marking the largest lunar impact in at least the last 5,000 years, albeit still small compared to typical craters. By ejecting debris into space and simulating their trajectories tens of thousands of times, they concluded that this event could lead to collision rates for Earth’s satellites comparable to those observed over years or even days.

While these collisions may not entirely disable a satellite, they could cause significant anomalies due to electrical disruptions. Accurately modeling their potential damage proves challenging, Wiegert noted.

If luck is not on our side, the impact of fragmented materials could be particularly severe, according to Mark Burchell at the University of Kent in the UK. “If they impact a spacecraft’s coolant pipe or an exposed sensor, the loss of critical functions occurs suddenly,” he explained. “Once damaged, satellites cannot be repaired. Even minor issues can lead to serious problems.”

Wiegert emphasized that this scenario should provoke global space agencies to consider deflecting asteroids on a collision course with the moon, similar to efforts aimed at protecting Earth. A NASA Planetary Defense Coordination Agency representative stated that while it is crucial to identify Near-Earth Objects (NEOs) posing potential risks, it is “premature to speculate on possible response options” for a potential 2024 collision.

Depending on how events unfold, swift action could be necessary. When 2024 YR4 reappears in Earth’s telescopic view in 2028, we should be able to refine the precision of its orbital path, Wiegert commented. As chances for a lunar impact rise, it offers a four-year window for decision-making on any necessary actions.

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Source: www.newscientist.com

Discover the First Image from the Vera C. Rubin Observatory: Why You Can’t Miss the Clock Party!

Vera C. Rubin Observatory

Rubin Observatory/NSF/AURA/A. Pizzaro D

I’ve never attended a watch party, unless you include a gathering with my two friends for the Taylor Swift: ERAS Tour (which featured themed snacks). But now, it seems watch parties are evolving beyond just movie releases. In fact, I’m gearing up to join a watch party for my new telescope in just a few days.

I was fortunate enough to be part of one of the first public groups to tour the Bella C. Rubin Observatory in Chile, a visit organized by New Scientist. Now, just two years later, I’m eagerly anticipating the first image that will be captured by this colossal telescope, scheduled for release on June 23rd.

The Vera C. Rubin Observatory stands as a marvel of engineering. It’s set to perform sky scans across the Southern Hemisphere within merely three nights. Over a decade, the observatory will conduct scans for ten nights as part of its legacy survey of space-time known as the LSST. This project promises to revolutionize our understanding of astronomy, unraveling longstanding mysteries, including those related to dark matter, and revealing new enigmas.

Clearly, the images and videos produced by the telescope will be breathtaking. To fully appreciate their detail, watching on a phone screen won’t suffice. Even a desktop display falls short. To capture the full glory of a single image, one would need to utilize 400 Ultra HD TVs, as per the LSST UK consortium. Consequently, the team is encouraging partner institutions worldwide to organize watch parties for a more immersive viewing experience.

The specifics of each watch party vary depending on the hosting institution, which may include planetariums, museums, or universities. For instance, events will take place at the Perth Observatory in Australia and at City University in Hong Kong. Numerous locations across the United States, including the Detroit Observatory in Michigan, will host watch parties where attendees can enjoy science demos and hear from local experts. A common thread across all these events is the live release of the first images and videos captured by the Vera C. Rubin Observatory at 11 AM EDT (11 PM GMT), with everyone tuning in to the live stream.

Processing the intricate details of each image can be a time-consuming endeavor. Not only is there the requirement to zoom out and appreciate the telescope’s expansive field of view, but also to zoom in on galaxies in unprecedented detail. Images produced by Rubin will offer greater resolution than those from the James Webb Space Telescope, covering similar sky areas with 45 moon-like objects while JWST operates with roughly three years of data. Additionally, a time-lapse video capturing how the sky evolves over time has been recorded by Rubin.

You’ll indeed be able to view the images online, as well as in issues of New Scientist once they’re published or shared on social media. However, if you want to celebrate this moment in a community setting, consider visiting this interactive map to discover a watch party near you—or, why not host one yourself? While you may miss the full definition on your home screen, you can still experience some of the thrill of witnessing the unveiling of these images and videos alongside others.

I’m excited to attend a local event, hoping to capture the sense of wonder I felt when I first stood inside the observatory and marveled at its grandeur. It’s a scale that helps us better understand our place in the cosmos, even when contrasted with the vastness of the universe.

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Source: www.newscientist.com

The Hidden Dangers of Dogs: What You Need to Know

Mosquitoes are notorious as some of the most lethal creatures on the planet, causing up to 1 million deaths annually due to the diseases they carry, such as malaria and dengue.

However, in the UK, we have 36 native mosquito species that rarely pose a significant threat, thus they do not constitute a part of the three-way tie for the deadliest creature in Britain.

One contender is the dog. Recently, Prime Minister Rishi Snack placed the American XL bully dog on the list of banned breeds after a rise in fatalities associated with dog attacks.

Statistics indicate an average of about three deaths annually. However, in 2022, ten individuals in England and Wales lost their lives due to dog bites. This unfortunate trend can largely be attributed to negligent ownership, particularly with the inclination to breed larger, more powerful dogs.

Small creatures can also be deadly. Therefore, bees and hornets are contenders for the title as well, as 0.5% of the population is allergic to stings, which can lead to fatal anaphylaxis, resulting in two to nine deaths in the UK each year.



The ultimate threat may be less apparent. Picture a serene scene with grazing cattle that cause approximately 4,000 accidents yearly in the UK.

Around five fatalities result from these incidents, primarily affecting the agricultural community, but pedestrians are also at risk. Cows, being prey animals, are instinctively protective of their calves.

Most mishaps occur when natural boundaries are disregarded. Cows can injure individuals by knocking them over or trampling them. It’s advisable to keep dogs on a leash and maintain a respectful distance from herds.

This article responds to the inquiry (Adrianna Gardner, Chelmsford) “What is the deadliest creature in the UK?”

Feel free to email us your questions at questions@sciencefocus.com or reach out through our Facebook, Twitter, or Instagram (please include your name and location).

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New Research Reveals the Ancient Origins of Fish Biofluorescence

Biofluorescence, the process of absorbing high-energy light and re-emitting it as low-energy wavelengths, has been observed in various vertebrate and invertebrate lineages, particularly among fish. Research conducted by the American Museum of Natural History indicates that fish biofluorescence can be traced back at least 112 million years and has evolved over 100 times, predominantly in fish inhabiting coral reefs.



Phylogenesis of teleosts showing ancestral state reconstruction (absence/present) of biological fluorescence. Image credit: Carr et al., doi: 10.1038/s41467-025-59843-7.

“Researchers have long known that biological fluorescence is prevalent in marine creatures, including sea turtles and corals, particularly among fish,” stated PhD Emily Kerr, a student at the American Museum of Natural History.

“To truly grasp the reasons and methods behind this unique adaptation, we need to explore the evolutionary background and the variety of biofluorescence currently utilized for camouflage, predation, or reproduction.”

In a first study published in the journal Natural Communication, Carr and colleagues investigated all known biological fluorescent extents, focusing on a species of bony fish, which comprises the largest living vertebrate group today.

This research identified 459 biological fluorescent species, including 48 previously unrecognized as biologically fluorescent.

The researchers discovered that biological fluorescence has evolved over 100 times in marine teleost fish, dating back to approximately 112 million years ago, with the initial occurrence found in eels.

Furthermore, fish species residing in or near coral reefs developed biological fluorescence approximately ten times faster than their non-reef counterparts, leading to a surge in fluorescent species following the mass extinction event around 66 million years ago that wiped out non-avian dinosaurs.

“This pattern coincides with the emergence of modern coral reefs and the rapid infiltration of fish into these environments, particularly after a significant loss of coral diversity due to the Cretaceous extinction,” Kerr explained.

“These relationships imply that the rise of contemporary coral reefs may have spurred the diversification of fluorescence in reef-associated teleost fish.”

Among the 459 documented biological fluorescent extents indicated in this study, the majority are linked to coral reefs.

In a second survey published in the journal PLOS 1, Kerr and co-authors employed a specialized photographic system with ultraviolet and blue excitation lights, alongside emission filters, to analyze the wavelengths emitted by fish from the ichthyology collection at the American Museum of Natural History.

These specimens, collected over the past 15 years during museum expeditions to locations like the Solomon Islands, Greenland, and Thailand, had shown fluorescence previously; however, the full spectrum of biological fluorescence emissions remained unexplored.

This study unveiled a broader diversity in the colors emitted by teleost fish, with some displaying at least six distinct fluorescence emission peaks across various wavelengths, surpassing prior reports.

“The unexpected variation observed among a wide array of these fluorescent fish suggests that they may utilize highly diverse and intricate signaling systems based on species-specific fluorescent emission patterns.”

“As these studies illustrate, biological fluorescence is extensive and remarkably phenotypically diverse among marine fish.”

“Our goal is to enhance our understanding of how fluorescence operates within these varied marine ecosystems and its role in evolutionary diversification.”

“The multitude of fluorescence emission wavelengths identified in this study could significantly impact the discovery of new fluorescent molecules that are routinely employed in biomedical applications, including the diagnosis and treatment of fluorescence-related ailments.”

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Carr et al. 2025. The extensive evolution of repeated biological fluorescence in marine fish. Nat Commun 16, 4826; doi:10.1038/s41467-025-59843-7

Carr et al. 2025. Marine fish display exceptional variability in biological fluorescence emission spectra. PLOS 1 20 (6): E0316789; doi: 10.1371/journal.pone.0316789

Source: www.sci.news

Alma Identifies Molecular Activity in the Largest Known Oort Cloud Comet

Astronomers from the Atacama Large Millimeter/Submillimeter Array (Alma) have made observations of comet C/2014 UN271 (Bernardinelli-Bernstein).



Artist depiction of Comet C/2014 UN271. Image credits: NSF/AUI/NSF/NRAO/M.WEISS.

C/2014 UN271 was identified by astronomers Pedro Berner Dinnelli and Gary Bernstein through images captured in 2014 as part of dark energy research.

The comet spans approximately 140 km (85 miles) in diameter, making it over ten times larger than any known comet.

To date, little has been understood about the behavior of such cold, remote celestial bodies.

Recent findings from Alma revealed the intricate and dynamic jets of carbon monoxide gas erupting from the comet’s nucleus, offering the first direct evidence of what drives its activity in relation to the sun.

“With these measurements, we can understand how this massive, icy world functions,” stated Dr. Nathan Ross, an astronomer affiliated with a U.S. university and NASA’s Goddard Space Flight Center.

“We are observing explosive outgassing patterns that raise new inquiries about the comet’s evolution as it journeys deeper into the inner solar system.”

Alma observed C/2014 UN271 by detecting light from carbon monoxide gas in its atmosphere and thermal radiation when the comet was still distant from the sun.

Thanks to Alma’s exceptional sensitivity and resolution, scientists were able to focus on the very faint signals emitted from such cold and far-off objects.

Building on previous Alma observations that characterized the comet’s substantial nucleus size, the new findings measured the thermal signal to accurately assess the size of the comet and the dust surrounding its nucleus.

Their measurements for the nucleus size and dust mass are in line with earlier Alma observations, affirming it as the largest cloud comet ever identified.

Alma’s precision in measuring these signals enabled this research, providing a clearer understanding of this distant, icy giant.

“This discovery not only represents the first detection of molecular outgassing in a record-setting comet but also offers a rare glimpse into the chemical and dynamic processes of objects from the farthest reaches of the solar system,” the astronomer added.

“As C/2014 UN271 approaches the sun, we anticipate more frozen gases will start to evaporate, revealing further insights into the comet’s primitive composition and the early solar system.”

“Such discoveries help address fundamental questions about the origins of Earth and its waters, as well as the formation of life-supporting environments elsewhere.”

The team’s research paper was published in Astrophysics Journal Letters.

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Nathan X. Ross et al. 2025. Initial detection of molecular activity in the largest known OORT cloud comet: Alma Imaging of The Sun at C/2014 UN271 (Bernardinelli-Bernstein). apjl 986, L22; doi: 10.3847/2041-8213/add526

Source: www.sci.news

Triassic Sauropodomorph Dinosaurs Endured Severe Bone Infections

A team of paleontologists from the University of Zurich has identified chronic instances of osteomyelitis (bone tissue infection) in Plateosaurus trossingensis, one of the well-known dinosaurs from the late Triassic period in Europe.



Diagram of Plateosaurus trossingensis skeletons featured in the Theoprati exhibition at the Museum of Natural History, University of Zurich. Image credits: Dupuy et al., doi: 10.1186/s13358-025-00368-3.

Plateosaurus trossingensis inhabited Europe around 220 million years ago during the late Triassic epoch.

These ancient creatures were approximately 8 m (26 feet) long and primarily walked on their hind legs.

In a recent study, paleontologist Jordan Bestwick and colleagues analyzed the skeleton of Plateosaurus trossingensis from the Klettgau Layer in Switzerland.

They discovered significant osteomyelitis in the dinosaur’s upper arm and right shoulder.

“Osteomyelitis affects various living animals, including humans, birds, and reptiles,” noted Dr. Bestwick.

“The condition has been documented in several dinosaur groups, including sauropods, leading us to assess and compare numerous specimens, including Plateosaurus.

“The impacted bones in the shoulders and upper arms displayed notably rough internal and external textures, altered shapes, and even fusion, which are broad indicators of osteomyelitis.”

Researchers find their discoveries particularly intriguing since this case represents the oldest recorded instance of osteomyelitis in dinosaurs, dating back to about 220 million years ago, and the extent of the infection was unusually large.

“Earlier studies highlighted localized infections, such as in toe bones or adjacent vertebrae,” Dr. Bestwick explained.

“It’s exceptionally rare to observe infections in a shoulder and the entirety of an upper arm.”

“While the initial cause of the infection remains unknown, it likely plagued the animal for a prolonged period, potentially rendering its right arm nonfunctional.”

These findings are detailed in a paper published in the Swiss Journal of Palaeontology.

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sfj dupuis et al. 2025. Osteology and histology of a Plateosaurus trossingensis (Dinosaur: Sauropodomorpha) from the Upper Triassic in Switzerland with advanced chronic pathology. Swiss J Palaeontol 144, 27; doi:10.1186/s13358-025-00368-3

Source: www.sci.news

The ancient creature boasted “goblin-like” teeth and a customizable tail.

Artistic reconstruction of Borguamondor

Karen Townsend

An extinct creature uncovered in North America offers fresh insights into the region’s life around 75 million years ago.

The creature has been described as “looking like a goblin jumping out of a rock,” according to Hank Woolley of the Los Angeles County Natural History Museum. This species, known as Monstaurus, is part of a group of reptiles that thrived during the late Cretaceous period. Woolley notes it could have been “around 3 to 4 feet from tail to tip.” “Best to stay away,” he warns.

Woolley named the species Borguamondor. The first part of the name derives from a Lord of the Rings character, while the second part is inspired by an invented Elvish word, referring to its bone armor — a trait shared with its relatives, modern Gira Monsters (Healoderma Sumpectum).

Remarkably preserved fossils were found in Utah two decades ago by Joseph Sertich. Initially, the Smithsonian Tropical Research Institute believed it was a prehistoric lizard. Sertich recalls, “I found a collection of scattered bones in a low, flat sandy area,” including the skull, vertebrae, jawbone, and parts of a hip bone.

Sertich encouraged Woolley to investigate the fossils at the museum in 2022. B. Amondor represents an extinct species of lizard known as the Monstaurus. They found evidence that some could shed their tails when injured, making it the oldest known example of this defensive strategy that modern lizards employ.

bones belonging to Borguamondor

Utah Natural History Museum/Bureau of Land Management

According to researchers, B. Amondor dined on small mammals, frogs, snakes, insects, and “things not primarily plants,” even considering dinosaur eggs as part of its “round-length” diet. Its habitat was likely a wetland ecosystem, quite hot and humid, resembling the modern-day U.S. Gulf Coast rather than the arid landscape we see today.

Randall Nydam from Midwest University in Illinois, though not involved in this research, emphasizes the cautionary aspect of the story, reflecting on the vulnerabilities of such formidable “monsters,” both ancient and modern. “We must also acknowledge that they are long gone,” he states, “vanished due to changing circumstances.”

Continuing the dialogue about B. Amondor, Sertich believes people should broaden their understanding of these creatures. “Imagining North America’s primal tropical forests should portray nightmare lizard-hunting dinosaurs navigating the underbrush and scaling trees,” he suggests.

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Source: www.newscientist.com

UK to Brace for Summers Over 40°C in the Next Decade, Warn Officials

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It’s probable that extreme temperatures will persist during the UK’s summer months.

AFP via Henry Nichols/Getty Images

According to the Met Office, the UK must swiftly adapt to summer temperatures exceeding 40°C (104°F). This warning from the nation’s National Weather Service highlights the alarming rate of rising summer temperatures due to climate change.

In July 2022, Lincolnshire, eastern England, recorded an unprecedented temperature of 40.3°C (104.5°F), the highest for that month. Experts state that climate change has amplified the likelihood of such heatwaves by at least tenfold.

Furthermore, researchers caution that these extremes are part of a worrying trend. Under the guidance of Jillian Kay, the Met Office has utilized climate models to simulate over 2,500 UK summers to evaluate the potential for extreme heat under current climatic conditions.

The findings reveal a 50% chance of surpassing 40°C within the next 12 years, particularly affecting the southern and eastern regions of England, which are at higher risk for intense heat. The frequency of such extreme temperatures has surged dramatically in recent decades, increasing six times since the 1980s and nearly tripling since 2000.

Additionally, there is a 1% chance of temperatures breaching 42°C (107.6°F) annually, with the highest projected temperature for the UK under present conditions reaching 46.6°C (115.9°F), though such an extreme is described as “very rare,” according to Kay.

The simulations also provide meteorologists insights into the atmospheric conditions conducive to extreme heat in the UK. A primary scenario involves a persistent heatwave affecting Europe, with hot air moving across the southern and eastern coasts of England. Recently, the Met Office issued a warning of another heatwave forecasted for the UK due to the intense warmth persisting across the continent.

As temperatures rise, these heatwaves are becoming increasingly enduring. In the scorching summer of 1976, daytime temperatures surpassed 28°C (82.4°F) for two consecutive weeks. Today, under current climate conditions, similar temperatures can persist for over a month. Simulations indicate that exceeding 40°C could be feasible for 3-4 days even under existing conditions.

“We could experience temperatures a few degrees higher than the 40°C seen in July 2022, and we must be ready,” Kay emphasizes. The UK faced considerable challenges managing brief instances of heat above 40°C during that heatwave. More than 1,200 additional deaths were reported, rail travel was disrupted, schools closed, and wildfires raged throughout the country.

Kay urged public authorities, especially public health leaders, to “stress-test” systems to effectively handle such extreme temperatures. “The Met Office and similar entities have long predicted that climate change would lead to more intense and frequent heatwaves,” she states. “Our research confirms exactly that.”

Prolonged heatwaves pose significant risks. They not only strain the ecosystem but also dry out soil, wilt plants, and threaten animal life, while putting immense stress on human health, particularly when daytime and nighttime temperatures remain elevated for long durations. Extended heatwaves increase the risk of heart attacks and strokes. This risk is particularly acute in regions less accustomed to sustained heat, like the UK, where air conditioning is uncommon.

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Source: www.newscientist.com

Bright Seifert Galaxy’s Ultra-Massive Black Hole Exhibits Signs of “Overeating”

In a new research paper published in Monthly Notices of the Royal Astronomical Society, astronomers from the University of Leicester explain for the first time how the “excessive diet” of fresh material in black holes has led to emissions reaching nearly a third of the speed of light.



This image illustrates Seyfert Galaxy PG1211+143. Image credits: Centre Donna Astromyk destrasbourg/Sinbad/SDSS.

The intense outflow of ionized gases has raised significant concerns at the ESA’s XMM-Newton X-ray observatory since its initial detection by University of Leicester astronomers in 2001, now recognized as a distinctive trait of the luminous active galactic nuclei (AGNs).

Professor Ken Pound and Dr. Kim Page from Leicester remarked:

“The black hole’s size increases with its mass, with a solar mass black hole having a radius of about 3 km.”

“Stellar mass black holes are prevalent across galaxies, often forming from the dramatic collapse of massive stars; however, ultra-massive black holes can be found in the nuclei of almost all galaxies except the smallest external ones.”

In 2014, astronomers undertook a five-week investigation of an ultra-massive black hole in the distant Seyfert Galaxy PG1211+143, located approximately 1.2 billion light-years from the constellation Coma Berenices.

Utilizing ESA’s XMM-Newton Observatory, they observed counter-inflows, accumulating at least 10 Earth masses near the black hole.

In their latest study, they detected a powerful new outflow traveling at 0.27 times the speed of light, initiated shortly thereafter. The gravitational energy released as material is drawn into the black hole is heated to millions of degrees, producing an overwhelming radiant pressure.

“Establishing a direct causal relationship between significant, temporary inflows and the resulting outflows offers an exciting perspective for observing the growth of supermassive black holes through continuous monitoring of the hot relativistic winds linked with new material accretion,” stated Professor Pound.

“PG1211+143 has been the focus of University of Leicester X-ray astronomers using ESA’s XMM-Newton Observatory since its launch in December 1999.”

“Initial findings surprisingly revealed a counterflow of rapid movements, reaching 15% of the speed of light (0.15c), affecting stellar formation (and consequently the growth) of the host galaxy.”

“Subsequent observations have shown that such winds are a common characteristic of bright AGNs.”

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Ken Pounds & Kim Page. 2025. Observations of the Eddington-style outflow from the bright Seyfert Galaxy PG1211+143. mnras 540(3): 2530-2534; doi: 10.1093/mnras/staf637

Source: www.sci.news

Cryopreserved Seastar Larvae May Facilitate the Recovery of Key Species

Giant pink star larvae resumed development after freezing at -200°C

Patrick Webster

In a groundbreaking achievement, researchers have successfully frozen and revived sea star larvae, marking a significant advance in conservation efforts aimed at restoring an endangered keystone species.

Since 2013, Coastal Star Wasting Syndrome has been devastating populations of sunflower stars (Pycnopodia helianthoides) and giant pink stars (Pisaster brevispinus) along the North American west coast. The decline of these predators has resulted in a major surge in sea urchins, decimating 97% of the kelp forests in Northern California.

Currently, the sunflower star is considered functionally extinct in California, sparking extensive efforts to cultivate these creatures for eventual reintroduction into their natural habitat.

In January 2025, a giant pink star was birthed at the Pacific Aquarium in Long Beach, California. Just two days later, its larvae were dispatched to the San Diego Zoo Wildlife Alliance, where they were immersed in liquid nitrogen and stored at -200°C. The following month, they were transported approximately 700 kilometers north to the Sunflower Star Institute in Monterey Bay.

Upon careful thawing, the giant pink star larvae resumed their development, settling on the seabed and transitioning into a boy shape. “No one has ever successfully frozen a sea star at the larval stage and achieved this,” researchers noted.

Sunflower Stars play an important role in the Kelp forest ecosystem

Pat Webster

The successful cultivation of cryopreserved larvae represents a significant milestone for conservationists, as it opens up avenues for reintroducing genetically diverse sunflower stars back into California’s waters. “The larval cycle of the giant pink star closely resembles that of the sunflower stars,” explained Bank, “after which we will move forward with sunflower star rearing.”

Over the past 15 years, marine ecosystems in the North Pacific have faced a growing tide of environmental challenges. “It’s a daunting narrative involving climate change, ocean heat waves, and ecosystem collapse,” remarked Andrew Kim from the Sunflower Star Institute. “However, within Pycnopodia, there lies hope for recovery.”

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Source: www.newscientist.com

Biotechnology Firms Seek to Develop the “ChatGPT of Biology”: Does It Deliver?

Basecamp researchers gather genetic data in Malta

Greg Funnell

A British biotech firm, Basecamp Research, has spent recent years gathering extensive genetic data from microorganisms inhabiting extreme environments worldwide, uncovering 10 billion new species among over a million scientifically recognized entities. This vast database of planetary biodiversity aims to assist in training “biology chats” to address inquiries regarding life on Earth, although its effectiveness remains uncertain.

Jorg Overmann from the Leibniz Institute DSMZ, which houses one of the world’s most extensive collections of microbial cultures, asserts that while an increase in known genetic sequences is beneficial, it likely won’t lead to significant discoveries in drug development or chemistry without deeper insights into the organisms from which they originated. “In the end, I’m skeptical that a better understanding of unique features will be achieved merely through brute force in the sequencing domain,” he remarks.

Recent years have seen a surge in machine learning models aimed at identifying patterns and predicting relationships within vast biological datasets. The most well-known of these is Alphafold, which can predict the 3D structure of proteins using only genetic data, and was awarded the 2024 Nobel Prize in Chemistry at Google DeepMind.

This “genometric biology” approach has grown significantly, but according to Francis Din at the University of California, Berkeley, progress has been limited. One reason for this is the underrepresentation of biodiversity data. “Current biological models are primarily trained with datasets that favor well-studied species (e.g., E. coli, mice, humans), leading to poor prediction capabilities for traits associated with sequences from other branches of the Tree of Life,” she explains.

Basecamp researchers aim to bridge this biodiversity gap. Their expanding database now includes samples from over 120 locations across 26 countries, as detailed in a report by the company. Jonathan Finn, the company’s Chief Science Officer, notes that their sampling efforts target extreme environments that have yet to be thoroughly examined, spanning from the icy depths of the Arctic Ocean to the warm jungle hot springs. “Most of the samples we’re prioritizing are prokaryotic: bacteria, microorganisms, and their viruses,” Finn states. “We are also aware that some fungi are present.”

Genetic analyses of these samples have illuminated gene variations that are broadly shared across the Tree of Life. Based on this research, the company estimates that their data encompasses over a million species of genetic information not found in public genomic databases utilized for training AI models. This includes around 9.8 billion newly identified genes, increasing the overall known gene count tenfold, each potentially encoding useful proteins, according to the researchers.

“By providing these models with richer data, we enhance our understanding of biological mechanisms,” Finn explains. “We aim to create a ChatGPT for Biology.”

It’s estimated that Earth hosts trillions of microorganism species, many of which remain poorly characterized. Thus, it’s not unexpected that the company has identified such a wealth of novel life forms. “As we explore more, discovering diverse gene variants becomes almost inevitable,” notes Leopold Parts at the Wellcome Sanger Institute in the UK.

Nevertheless, Basecamp promotes the notion that all newly discovered materials might hold value. It’s not alone in this sentiment. “This is among the most thrilling advances I’ve encountered in quite some time,” remarks Nathan Frey, a machine learning researcher at Genentech, a US biotech firm. He emphasizes that most AI biology projects focus on algorithm improvement or generating additional lab data rather than venturing out to collect samples directly from nature.

However, skepticism arises regarding whether this database will yield the meaningful advancements the company aspires to achieve. For starters, it remains uncertain how much this newfound diversity in proteins reflects valuable new functions like enzymes and proteins that can degrade plastic useful for gene editing. “They must demonstrate that this novelty has practical utility,” cautions Parts.

Moreover, if the new genes significantly differ from known genes, Overmann expresses doubts about how easily existing tools can predict functionality or how such data can be utilized for training new models. “I can’t discern the functions of most of my genes,” he states. The company may have created a valuable new repository of biological data, but in traditional lab settings, even the most advanced AI may still face challenges in interpretation.

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Source: www.newscientist.com

Can Reusable Rockets Mitigate the Risks of Solar Geoengineering?

Rockets can transport cooling aerosols to high altitudes

Kevin Dietsch/Getty Images

Reusable rockets designed to deliver sun-reflecting aerosols into the upper stratosphere could help cool the planet. However, this fleet of climate-modifying rockets presents its own challenges.

The increase in global temperatures has led to a surge in research on solar geoengineering, a controversial method aimed at cooling the Earth by reflecting sunlight. The most recognized technique, known as stratospheric aerosol injection (SAI), entails continuously releasing reflective particles, such as sulfur dioxide, into the stratosphere.

Typically, researchers believe that aerosols will be released from cargo aircraft flying at around 20 km high. Climate models suggest that this could offset warming caused by rising greenhouse gas levels. Nonetheless, it also presents numerous other climate risks, some of which are unknown.

One significant concern is that the aerosols absorb sunlight, warming the stratosphere itself, even while surface temperatures cool. Because of wind patterns, aerosols tend to cluster in the tropical stratosphere, resulting in more warming than in other areas of the atmosphere. This can disrupt jet streams and circulation patterns that influence global weather.

Aerosols may also hasten ozone depletion caused by chlorine, potentially postponing the recovery of ozone holes over Antarctica by as much as 50 years.

Pengfei Yu from Jinan University in China and his team explored whether injecting aerosols at much greater heights—50 kilometers in the upper stratosphere—would change these dynamics. They discovered that high-altitude injections could yield greater cooling benefits than lower altitude methods, as aerosols persist longer, particularly at the poles. This additional height also prevents the aerosols from warming the lower stratosphere until they reach the poles, avoiding the harmful heating in the tropical stratosphere.

Finally, researchers found that these aerosols interact with another chemical that depletes ozone, which results in only a five-year delay in ozone recovery. “We weren’t aware that [injecting at] 50 kilometers offered such a different perspective,” says Yu.

Since planes cannot reach nearly 50 km, researchers propose using rockets. They estimate that deploying 80 reusable, hydrogen-powered rockets every other day could inject between 3 million and 8 million tonnes of aerosols annually, which they say falls within current technological capabilities.

While this scenario may be theoretically feasible, it is likely to be significantly more complex than traditional SAI approaches, according to Douglas McMartin at Cornell University in New York. Some advantages, such as preventing warming in the tropical stratosphere, can be more easily achieved by focusing on higher latitudes instead of high altitudes.

“It may rise higher in the atmosphere for increased efficiency, but the costs are astronomical in comparison,” he states.

Moreover, the high-altitude method does not fully mitigate many risks associated with solar geoengineering, including the rapid temperature increase that could follow if injection ceases. “What happens if the rockets fail on the ground?” Yu questions. “That’s a legitimate concern.”

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Source: www.newscientist.com

Helgorand: Exploring the Past and Future of Quantum Physics on a Tiny Island

Helgoland Island occupies a nearly mythical position in quantum mechanics history

Shutterstock/Markus Stappen

Having attended numerous scientific conferences, the recent one on Helgoland Island, marking a century of quantum mechanics, stands out as one of the most peculiar, in a positive sense.

This tiny German island, stretching less than a kilometer in the North Sea, exudes the ambiance of a coastal resort. Even during summer, its charm wanes, giving way to the scent of quaint streets filled with souvenir shops, fish eateries, and ice cream stalls. Picture cutting-edge experimenters in Quantum Technologies casually mingling after discussions at the town hall beside a miniature golf course—it’s quite an experience.

Our purpose here becomes evident as we stroll along the cliffside road, where a bronze plaque commemorates physicist Werner Heisenberg’s purported invention of quantum mechanics in 1925. While it sounds intriguing, it’s an embellishment; Heisenberg merely outlined some concepts here. The more recognized formulation came from Erwin Schrödinger in early 1926, who introduced wave functions to predict quantum system evolutions.

Nonetheless, this year clearly holds significance as we commemorate a century of quantum mechanics. Regardless of how much of Helgoland’s narrative stems from Heisenberg’s own embellishments—he recounted his breakthrough there several years later—this “Remote Control Island” serves as a unique venue for celebratory gatherings.

And what a celebration it is! It’s almost surreal to witness such a congregation of renowned quantum physicists. Among them are four Nobel laureates: Alain Aspect, David Wineland, Anton Zeilinger, and Serge Haroche. Collectively, they’ve validated the bizarre aspects of quantum mechanics, showcasing how the characteristics of one particle can instantaneously influence another, no matter the distance. They’ve also developed techniques to manipulate individual quantum particles, crucial for quantum computing.

In my view, these distinguished individuals would concur that the younger generation is poised to delve deeper into the implications of quantum mechanics, transforming its notoriously counterintuitive essence into new technologies and a better understanding of nature. Quantum mechanics is renowned for encompassing multiple interpretations of its mathematical framework concerning reality, with many seasoned experts firmly entrenched in their perspectives.

Helgoland’s plaque honors Werner Heisenberg’s role in quantum mechanics

Philip Ball

This divisive sentiment was noticeable during Zeilinger and Aspect’s evening panel discussion. Jill’s Brothers pioneered quantum cryptography at the University of Montreal.

In fairness to the veterans, their theories emerged under considerable skepticism from their peers, particularly regarding the significance of examining such foundational concerns. They navigated an era where “silent calculations” were prevalent—a term coined by American physicist David Mermin to describe how it was frowned upon to ponder the implications of quantum mechanics beyond merely solving the Schrödinger equation. It’s no wonder they developed thick skins.

In contrast, younger researchers seem more pragmatic in their approach to quantum theories, often adopting various interpretations as tools to address specific challenges. Elements of the Copenhagen interpretation and the multiverse theory are intertwined, not as definitive claims about reality, but as frameworks for analysis.

The new wave of researchers, such as Vedika Khemani from Stanford University, are actively bridging condensed matter physics and quantum information. I heard her highlight the evolution from storing information on magnetic tapes in the 1950s to the crucial error correction techniques in today’s quantum computing.

Quantum mechanics applications are on the rise, with theorists also stepping up their game. For instance, Flaminia Giacomini at the Federal Institute of Technology in Zurich spoke about her pursuit of reconciling the granular quantum realm with the smooth continuous world required for quantum gravity, offering profound insights into the essence of quantum mechanics.

While some may consider this exploration to be veering into the realm of speculation, as seen in string theory attempts, Giacomini asserted, “There is no experimental evidence that gravity should be quantized.” Hence, empirical validation remains elusive, despite a wealth of theoretical discourse.

Excitingly, there are plans to test hypotheses in the not-so-distant future. For instance, examining whether two objects can entangle purely through gravitational interactions is a goal. The difficulty is ensuring the objects are substantial enough to exert meaningful gravitational pull while being sufficiently small to demonstrate quantum characteristics. Several speakers expressed confidence in overcoming this hurdle within the next decade.

The conference revealed the interconnectedness of quantum theories and experiments: perturbing one aspect inevitably influences others. Gaining a nuanced understanding of quantum gravity through delicate experiments involving trapped particles could shed light on black hole information paradoxes and inspire innovative ideas for quantum computing and the nature of quantum states.

Ultimately, achieving progress in any of these areas appears promising for uncovering the enduring questions that have fascinated Heisenberg and his contemporaries. What occurs when we measure quantum particles? However, rather than perceiving it as a repetitive struggle, it’s clear that quantum mechanics is much more sophisticated and intriguing than the founders ever envisaged.

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Source: www.newscientist.com

How Your Overlooked Memories Shape Your Decisions Today

When recalling memories, neural activity is sparked in different brain regions

Nopparit/Getty Images

Even forgotten memories appear to influence our behavior.

“People often perceive memories as something to reflect on or contemplate,” says Nick Turk Brown from Yale University, who was not involved in this research. “However, we don’t spend our days lost in past memories. We work, parent, and have fun. Our memories continuously shape our actions; I believe 95% of our cognitive processes operate in this unseen manner.”

Memory can be described in various ways. One perspective focuses on self-reported recollections, like what someone had for dinner yesterday or details about their seventh birthday. Another way to conceptualize memory involves the persistent networks of brain cells known as engrams, which create the biological representation of experiences we have memorized.

Many researchers have long believed that forgetting a memory implies the disappearance of its related engrams. However, studies on mice suggest that forgotten memories endure even when they cannot be consciously retrieved.

In a study led by Tom Willems from the University of Bern, Switzerland, 40 participants briefly viewed 96 pairs of images, including human faces and objects like guitars and staplers.

The researchers then monitored the participants’ brain activity while testing their memory of whether two images had been paired 24 hours prior, using high-resolution functional magnetic resonance imaging. Participants were also asked if they remembered seeing the images together, if they were uncertain, or if they were just guessing.

When they confidently recalled the images, participants correctly chose the paired images 87% of the time in both tests. Conversely, those who could not recall what they had seen managed to achieve about a 50% accuracy rate.

Participants uncertain of their memory estimated correctly 57% of the time after both 30 minutes and 24 hours, suggesting that this group may still retain some memory of the associations.

Interestingly, when guessers made the right choice, their brain activity patterns mirrored those of participants who confidently remembered, particularly in the relevant hippocampal regions.

During a follow-up test after 24 hours, individuals who believed they had forgotten remained active in the hippocampus, while those who recognized the images exhibited activity in the anterior cingulate gyrus of the neocortex.

As Amy Milton from Cambridge University states, “I suggest that the shift of memory activity to the neocortex is associated with recall, but it remains unclear whether this change is a cause or a result of what is remembered.”

Nevertheless, the findings align with a predominant theory of memory function, known as Standard Integration Theory, as explained by Turk Brown. This theory proposes that memories are initially formed in the hippocampus and later consolidated in the neocortex during sleep for long-term storage.

This research highlights a potential separation between the memories we consciously access and the associated engrams in the brain, according to Turk-Browne. “This offers a fascinating illustration of the subtle, automatic, and pervasive influence of hippocampal memories on behavior.”

“Essentially, what they propose is that some memories don’t have to be consciously searched for in order to influence behavior later,” Milton explains.

She expresses no surprise that strong memory traces can shape our actions without our conscious awareness, referencing the phenomenon of priming. Seeing or hearing something can subtly prompt specific responses without us discerning the reasons.

However, priming occurs in various brain regions, such as the prefrontal cortex, and as Turk-Browne notes, it typically produces only transient effects lasting seconds or minutes.

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Source: www.newscientist.com

Physicists Unveil Heaviest Known Proton-Luminescent Isotope: Astatine-188

At the Accelerator Laboratory of the University of Zibaskira in Finland, physicists utilized a gas-filled recoil separator focal plane spectrometer to observe two attenuation events of the newly discovered isotope astatin-188 (188At), which is composed of 85 protons and 103 neutrons.

Kokkonen et al. Report the discovery of the new nucleus 188At, which is the heaviest proton-emitting isotope known to date.

“Proton emission is a rare type of radioactive decay where the nucleus releases protons, moving toward stability,” explained Henna Kokkonen, a doctoral researcher at Zibaskira University.

“This new nucleus is currently the lightest known isotope of astatin, 188At, containing 85 protons and 103 neutrons.”

“Studying this type of exotic nucleus is exceedingly challenging due to its brief lifespan and low production cross-section. Therefore, precise techniques are essential.”

“The nuclei were produced through fusion deposition reactions by irradiating natural silver targets with a 84Sr ion beam,” added Dr. Kare Auranen of Zibaskira University.

“The detection of the new isotopes was made possible using the Ritu Recoil separator’s detector setup.”

In addition to the experimental findings, the physicists expanded theoretical models to interpret the collected data.

According to the team, 188At can be likened to a strong explosion, resembling “the shape of a watermelon.”

“The nuclear properties suggest a shift in the behavior of the binding energy of valence protons,” Kokkonen stated.

“This is attributed to unprecedented interactions with heavy nuclei.”

“Isotopes are rare globally, and this marks the second occasion I’ve had the chance to make history.”

“All experiments pose challenges, and it is rewarding to conduct research that enhances our understanding of the fundamental limits of matter and nuclear structure.”

The authors intend to refine the current uncertainties and half-life of the attenuation energy by further theoretical exploration of charged particle-damped heavy nuclei, observing the evolution of their shapes, and examining additional decay events of 188At.

“Equally intriguing is the study of the collapse of a currently unknown nuclear isotope 189At, which could be a proton-emitting nucleus, an aspect we have yet to explore in future experiments,” they concluded.

Their paper was published in the journal Nature Communications.

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H. Kokkonen et al. 2025. New Proton Emitter 188At signifies unprecedented interactions in heavy nuclei. Nat Commun 16, 4985; doi:10.1038/s41467-025-60259-6

Source: www.sci.news

These Unusual “Bears” Have the Power to Halt Aging—Here’s What We’re Discovering

Commonly referred to by fans as “water bears” or “moss pigs,” the tardigrade is arguably the cutest microscopic creature on Earth.

These tiny beings have even been sent to the International Space Station. Scientists have successfully launched them into the vacuum of space.

Remarkably, they survived for days without air, water, or any protection from intense solar radiation, showcasing their resilience. Researchers believe these little animals possess extraordinary survival capabilities.

In extreme situations, tardigrades enter a state known as cryptobiosis, essentially drying out and halting their metabolism.

Once conditions improve and water is reintroduced, they can rehydrate and start functioning again as if nothing ever happened.

Recent research has revealed new insights into these remarkable organisms. For instance, scientists have identified a protein called “DSUP” that shields their DNA from radiation, acting like molecular armor.

Researchers from the University of Stuttgart have provided evidence supporting the “sleeping beauty” hypothesis.

This theory posits that in their dormant state, tardigrades may not only pause their metabolism but also their biological clocks.

They survived for days without air, water, or protection from intense solar radiation. – Image credits: Scientific Photo Library via Sebastian Kauritzki/Getty Images

Interestingly, water bears that undergo freezing thrive for twice as long while awake compared to a control group that never sleeps.

In their natural habitats, tardigrades might only be active for a few months, yet they can enter a state of suspended animation and survive for decades.

A 2024 study focused on the recently discovered tardigrade, Hypsibius henanensis, which provided further insights.

The research revealed a gene responsible for producing betalain, which counteracts the damaging effects of ultraviolet rays.

Additionally, they uncovered proteins that enhance DNA repair mechanisms. The next step is to determine whether these proteins offer protection across any of the 1,300 known tardigrade species.


This article answers the question posed by Madison Halladay: “Why are tardigrades so indestructible?”

Please email us to submit your questions Question @sciencefocus.com or Message Facebook, Twitter or Instagram Page (don’t forget to include your name and location).

Check out our ultimate Fun facts for more amazing science content.


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Cyanocoronene Discovered: Astronomers Find 7-Ring Polycyclic Aromatic Hydrocarbons in TMC-1

Polycyclic aromatic hydrocarbons (PAHs) are believed to be the most prevalent class of organic compounds in the universe, yet their lifecycle in interstellar media remains poorly understood. Recently, astronomers using NSF’s Green Bank telescopes identified cyanocoronene (C24H11CN), the largest PAH discovered in space, located within the starless cloud core TMC-1.



Cyanocoronene, composed of seven interconnected benzene rings and cyano groups, is a region known for its abundant chemistry and was discovered in the cold, dark molecular cloud TMC-1, recognized as a new cradle for star formation. Image credits: NSF/AUI/NSF/NRAO/P.VOSTEEN.

Cyanocoronene is a derivative of coronene, often regarded as a prototype compact PAH due to its stability and distinctive structure.

PAHs are thought to play a crucial role in the chemistry that captures a significant portion of the universe’s carbon and contributes to star and planet formation.

Until this discovery, only smaller PAHs had been identified in space, making this finding a significant leap in understanding size limits.

“Each new detection brings us closer to understanding the origins of the complex organic chemistry in the universe, and possibly the building blocks of life,” says Dr. Gabi Wentzel, an astronomer at the Center for Astrophysics at MIT and Harvard & Smithsonian.

Dr. Wentzel and her team first synthesized cyanocoronene in the laboratory and recorded its unique microwave spectrum using advanced spectroscopic methods.

Equipped with this molecular fingerprint, the astronomers searched data from the Green Bank telescope, the primary instrument for the Gotham project (GBT observations of TMC-1: GBT observations of aromatic molecules).

They identified several spectral lines of cyanocoronene, confirming its presence with a statistical significance of 17.3 sigma, a robust detection by astronomical standards.

Cyanocoronene is currently the largest individual PAH molecule found in interstellar space, featuring 24 carbon atoms in its core structure (excluding the cyano group).

The quantity of cyanocoronene detected is comparable to that of smaller PAHs previously identified, challenging the notion that larger molecules are rare in the universe.

This indicates that even more complex aromatic molecules may be prevalent in the cosmos.

“The presence of such a large, stable PAH lends support to the idea that these molecules can serve as significant reservoirs of carbon and potentially facilitate the formation of new planetary systems throughout their lifecycle,” the researchers stated.

“The quantum chemical analysis in this study reveals that the reaction between coronene and CN radicals enables the efficient formation of cyanocoronene in cold space conditions.

“This implies that even prior to star formation, there can be chemical processes that establish complex organic matter.”

“The discovery of cyanocoronene not only adds new chapters to the narrative of astrochemistry but also reinforces the PAH hypothesis. It suggests that these molecules are responsible for the enigmatic infrared emission zones scattered throughout the universe.”

“Additionally, it establishes a direct link between interstellar clouds, meteoroids, and asteroid chemistry, implying that organic molecules present in our solar system might have originated in similar environments long before the Sun was born.”

The scientists presented their Survey results on June 11th at the AAS246, 246th Summer American Astronomical Association.

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Gabi Wenzel & Gotham Collaboration. 2025. Discovery of 7-ring PAH cyanocoronene (C24H11CN) from Gotham observation of TMC-1. AAS246 Summary #75

Source: www.sci.news

Astronomers Map the Distribution of Ordinary Matter Across the Universe

Astronomers are making significant strides in comprehending how matter behaves and interacts in space utilizing fast radio bursts (FRB). They have found that over three-quarters of the universe’s ordinary material is concealed within sparse intergalactic gases, and they have also identified the furthest FRB event recorded to date.

This artist’s concept illustrates the density regions and red blank areas of the universe’s web in blue. Image Credit: Jack Madden/Illustristng/Ralf Konietzka/Liam Connor, CFA.

For many years, it has been established that at least half of the normal, predominantly proton-based baryonic material in the universe has gone unaccounted for.

Previous approaches by astronomers employed methods like X-ray and ultraviolet observations to gather significant clues regarding this missing mass, which manifests as extremely thin warm gases between galaxies.

The challenge arises from the high-temperature, low-density gas that remains mostly invisible to most telescopes, leaving scientists unable to assess its presence or distribution.

This is where FRBs come into play – brief, intense radio signals emitted by distant galaxies that researchers have recently demonstrated could measure baryonic matter in space, although its location remained a mystery until now.

In the latest study, scientists examined 60 FRBs, with the most distant FRB recorded at 1,174 million light-years (FRB 20200120E) from Messier 81 and reaching up to 9.1 billion light-years (FRB 20230521b).

This enabled them to pinpoint the missing material within intergalactic spaces or the intergalactic medium (IGM).

“The ‘baryon problem’ was never in doubt,” stated Dr. Liam Connor, an astronomer at the Harvard & Smithsonian Center for Astrophysics. “The issue has always been about its location. Now with FRBs, we’ve established that three-quarters of it exists between galaxies in the cosmic web.”

By analyzing the delays in each FRB signal as it traveled through space, Dr. Connor and his colleagues tracked the gaseous medium along its path.

“FRBs function like flashlights in space, illuminating the intergalactic medium. By accurately gauging how the light slows down, we can assess this medium, whether it’s starkly visible or barely detectable,” Dr. Connor explains.

The findings are revealing—approximately 76% of the universe’s baryonic matter resides within the IGM.

Additionally, about 15% is found in galaxy halos, with a minor fraction embedded within stars and cool galactic gases.

This distribution aligns with predictions made by advanced cosmological simulations, yet this is the first instance of direct confirmation.

“This marks a triumph for contemporary astronomy,” noted Dr. Vikram Ravi, an astronomer from California.

“Thanks to FRBs, we are now approaching a new understanding of the universe’s structure and composition.”

“These brief flashes enable us to trace the invisible baryonic matter filling the expansive voids between galaxies,” he added.

“Baryons are pulled into galaxies by gravity; however, supermassive black holes and supernova explosions can expel them back into the IGM, cooling cosmic temperatures when they spiral out of control,” commented Dr. Connor.

“Our findings indicate that this feedback mechanism is effective, suggesting gas must be displaced from galaxies into the IGM.”

The team’s results are published today in the journal Nature Astronomy.

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L. Connor et al. Gas-rich cosmic web unveiled by the partition of missing baryons. Nature Astronomy Published online on June 16th, 2025. doi:10.1038/s41550-025-02566-y

Source: www.sci.news

Paleontologists Discover Early Jurassic Ikchosaurus Fossils in British Columbia

The partial skeleton discovered in the Fernie Formation in British Columbia, Canada, in 1916, represents a new genus and species of an extinct marine reptile named Ichaosaurus, as stated by an international group of paleontologists.



Photos and interpretation of Fernatator Prentisai skeleton in side view on the left. Image credit: Massare et al.

Fernatator Prentisai existed in North America during the early Jurassic Epoch, approximately 109 million years ago.

“Ichthyosaurs—marine reptiles that superficially resemble dolphins—were prominent marine predators from the early Triassic (Olenek) to the beginning of the late Cretaceous (Cenomanian),” noted Professor Judy Massare from SUNY College.

“They were the dominant large predators of the Triassic and early Jurassic seas.”

“Many partial and complete skeletal remains of early Jurassic ichthyosaurs have been collected, primarily from England and Germany.”

“The early Jurassic Ektisaurus in North America is considered rare,” they emphasized.

“Hence, the discovery of partial skeletal remains from western Canada is significant.”



Excavation of Fernatator Prentisai skeleton. The podium is incomplete, but the additional parts that were lost have since been preserved. T. Prentice At Light, WR Wilson, the general manager of CNP Coal Company, is on the left. Photo taken around 1916, between the Elk River, Morrissey, and Fernie, British Columbia. Photographer unknown. Image credit: Massare et al.

The skeleton of Fernatator Prentisai was found by T. Prentiss in the summer of 1916 while fishing on the Elk River in British Columbia, Canada.

“This specimen represents the most complete ichthyosaur known from the early Jurassic in North America and is one among several ichthyosaur specimens known from the Fernie Formation in western Canada,” the paleontologist remarked.

This new species is a medium-sized ichthyosaur, measuring 3-4 m (10-13 feet) in length, with a distinct combination of features.

“As preserved, the entire skeleton measures 2.8 m long, which includes an impression of the front of the podium,” the researcher added.

“In life, this skeleton likely reached approximately 3.5 m in length, possibly even 4 m.”

“Despite the poor preservation, there is enough identifiable morphology to justify the designation of a new genus and species,” they noted.

“It is characterized by a tall, bar-like orbital, short straight jugals that do not extend beyond the anterior or posterior of the orbit, a long, narrow anterior process of the maxilla, and a cora-like body with a broad curved outer end and a deep anterior region, among other features.”

Fernatator Prentisai symbolizes a sparse record of early Jurassic ichthyosaurs, validated from the Early Jurassic in Canada, and is a significant addition to ichthyosaur taxonomy.

A paper detailing this discovery has been published in the June 2025 issue of the journal Paldicola.

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Judy A. Massare et al. 2025. The most complete early Jurassic ichthyosaur from North America. Paldicola 15(2): 86-99

Source: www.sci.news

Nature Unveils the “Black Box” of Science by Releasing Peer Review Files

Nature of science journals aims to highlight the complexities of academic publishing.

In an editorial released on Monday, the journal revealed it will include a peer review file with the papers it plans to publish. This will grant reviewers insight into the behind-the-scenes process where authors respond to revisions.

Publishing peer review files has been an option in Nature since 2020, but as of Monday, it has become a standard practice.

“Our goal is to demystify what many refer to as the ‘black box’ of science and clarify how research papers are developed. This aims to enhance transparency and foster trust in the scientific process. We believe that publishing peer reviewer reports enriches scientific communication and contextualizes how results and conclusions are reached.”

Opening the peer review process is becoming increasingly common among scientific journals, but Nature stands out as one of the largest and most influential in adopting this practice.

Peer review occurs once scientific research is submitted to a reputable journal, where field experts evaluate the work for issues such as flawed inferences, poor research practices, and data errors. These external experts provide feedback to journal editors and authors, known as the Judge Report.

“Peer review enhances the quality of the paper,” the editorial states. “The dialogue between authors and reviewers should be regarded as a significant component of the scientific record, crucial to research andits dissemination.”

Nature’s updated process automatically publishes judge reports and author responses. Journal practices evolve particularly when public trust in science wanes; a Pew Research Center poll indicates that trust in scientists fell approximately 10 percentage points from 2019 to 2024, with only 45% of Americans considering scientists to be effective communicators.

Michael Eisen, a former editor of the scientific journal Elife and a proponent of reforming the scientific publishing process, believes Nature’s decision marks a significant step towards greater transparency in the field.

“It’s valuable for the public to witness the process,” Eisen stated. “Much of the criticism stems from misunderstanding, which often arises from a lack of transparency surrounding scientific processes.”

Eisen suggests this move could help skeptics recognize the rigorous scrutiny applied to critical topics.

“For instance, if people observe the thorough examination vaccine-related studies undergo, it can help them better understand and assess the context of scientific findings,” Eisen noted.

At the same time, this transparency may help to mitigate the sensationalism often associated with striking findings.

“It may help dispel the notion that once a paper is published, it is infallible and that all questions have been resolved,” Eisen added.

He also mentioned that Nature could publish reviewer comments on manuscripts that were ultimately rejected.

“The truly transformative step would be to disclose reviews for all submitted papers,” Eisen remarked. “While it’s insightful to understand the questions raised in reviews of accepted papers, it is equally important to see why certain papers were rejected by the journal.”

Source: www.nbcnews.com

Milky Way Black Holes Could Be Rotating at Their Limit

SEI 255742397

Image of Sagittarius A*, the black hole at the center of the Milky Way galaxy

EHT

At the core of our Galaxy lies an extraordinary rotating entity: a black hole that appears to be spinning near its maximum velocity.

Michael Jansen from Radboud University in the Netherlands and his team investigated black holes in the center of the Milky Way, specifically Sagittarius A*, utilizing data gathered by a collective network known as the Event Horizon Telescope (EHT). To tackle the intricacies of the data, they opted for artificial intelligence methods.

Initially, they simulated approximately one million black holes using established mathematical models, a computational endeavor that necessitated millions of hours on supercomputers. These simulations served as training data for a type of AI known as neural networks, enabling them to assess the properties of black holes based on empirical observations. Subsequently, they fed the AI with data on Sagittarius A* collected by the EHT throughout 2017.

The AI determined that Sagittarius A* is rotating at 80-90% of its theoretical maximum speed. It also indicated to the researchers that none of the currently available magnetic field models adequately describe the characteristics of this black hole, highlighting the need for additional mathematical modeling. Janssen notes that earlier studies had merely narrowed down the potential characteristics of Sagittarius A*, such as its rotation speed and surrounding magnetic fields, while this new methodology has refined those estimates.

Dimitrios Psaltis from Georgia Tech in Atlanta remarked that some of the findings were unexpectedly counterintuitive. Previous analyses had not clarified whether black hole spins could be accurately discerned from EHT data.

While earlier research suggested that Sagittarius A* might be spinning at significant speeds,
Mizuno Yuishi from Zhejiang University in Shanghai, China, noted that there is still room for enhancement in the computational models applied in this new analysis. “Our theoretical model is still not perfect,” he acknowledged.

However, both Mizuno and Psaltis agree that integrating AI into the study of exotic cosmic entities like black holes is increasingly essential. “We possess a wealth of data and numerous models, and we require a contemporary approach to merge the two,” Psaltis states. “This is precisely where machine learning proves to be transformative.”

Yet, this integration presents unique challenges, as AI work necessitates verification to mitigate potential inaccuracies and errors in subsequent analysis.

Janssen and his team have conducted numerous verification checks, including testing the AI with specially designed simulation data. They are also evaluating data from subsequent EHT operations and will be analyzing new findings from observatory results, he explains.

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Source: www.newscientist.com

Prospectors Explore Hydrogen Resources along the US Continental Divide

New Scientist Explores Hydrogen Wells in Kansas

Hyterra/Adler Gray

Excavation rigs often stir curiosity in fields dotted with grazing cattle. Although we are in Kansas, these rigs proudly display both American and Australian flags, indicating the origins of their owner. Hyterra, an Australian company, has been exploring for natural hydrogen fuels lurking in deep fractures of North America.

“I believe behind us is the kitchen where hydrogen is produced,” said Avon McIntyre, the company’s executive director. The surge in activity has drawn numerous businesses to the Midwest, positioning eastern Kansas as a pivotal area in the global quest for “geological hydrogen.”

This tale began about 1.3 billion years ago when the continent that is now North America began to fragment into two parts. While the continent eventually stopped separating, the fracture left a 2,000-kilometer-long mark of iron-rich mantle rock. Presently, this cleft lies buried beneath farms and ranches in the Midwest.

In eastern Kansas, older oil and gas wells have recorded high concentrations of hydrogen as solid rocks surrounding these fractures are pushed near the surface. To explore potential harvesting, several companies have secured hydrogen drilling rights over more than 100,000 hectares in the region, according to McIntyre’s analysis of public court documents. Hyterra and its competitor Koloma are advancing their efforts by drilling deeper into the earth.

“It’s like a gold rush, with everyone eager to find it,” stated Kristen Delano from the Colorado-based company Coloma. While she refrained from disclosing their drilling locations in Kansas, she noted that public opinion has indicated their recent excavations. Additional companies, such as the Australian firm Top End Energy, are acquiring mineral rights based solely on where Koloma is active.

“There has been considerable discussion within the community,” remarked Shawn McIntyre, who has no relation to Hyterra’s executive director. As a rancher from Waterville, Kansas, he has leased thousands of acres for hydrogen drilling. “This could revitalize the industry in small towns that have suffered economically in this region.”

The global pursuit of underground hydrogen escalated following updated assessments of global reserves several years ago. Companies investigating gas deposits are hopeful that it could become an alternative to the fossil fuels currently dominating heavy industry, fertilizer production, and electricity generation. “Natural hydrogen fits seamlessly into that narrative,” stated Jay Calbus from the Kansas Geological Survey. “If we are sitting atop a substantial supply of hydrogen that can be harnessed… it could transform not only the state but also the wider region, and the nation.”

As Avon McIntyre and I traverse the muddy terrain to the drilling platform southwest of Manhattan, Kansas, he shouts above the din of the rig, “It’s crucial to understand what’s happening down there.”

The company hypothesizes that water from the underground aquifer interacts with iron-rich mantle rocks within the Middle Continent fractures, resulting in the production of hydrogen through a process known as meandering. This reaction generates hydrogen molecules in the water, which subsequently migrate to the surrounding rocks.

This year, plans include drilling five exploratory wells aimed at identifying hydrogen concentrations along subsurface rises in bedrock known as Nemahalridge. Earlier reports revealed that the first well, drilled at a prominent location on this ridge, recorded hydrogen concentrations of 96%.

Currently, the second well is deepening, surpassing 1600 meters and operating continuously. At the rig, workers sift through the mud, which contains granite scraps from the excavated hole, extracting gas from the liquid for analysis.

In the Mud Shack, a makeshift office at the site’s periphery, a team of contractors monitors and reports in real-time the gas composition from varying depths of the well. While gas levels remained low in solid rock, hydrogen concentrations began measuring over 800 parts per million.

“[The first well] had an impressive peak, but this one is continuously producing hydrogen,” noted Hyterra’s Josh Whitcom.

While these measurements alone carry limited meaning, more precise evaluations require gas samples sent from the site. Moreover, high hydrogen concentrations do not indicate how much gas can actually be extracted or the duration of flow.

Even if hydrogen ultimately flows from any of these wells, numerous questions remain, such as how it will be isolated from other gases, transported, stored, and who will be its consumers.

However, McIntyre is thrilled by the detection of hydrogen and encourages the crew to work through the night. “Our goal is to gather information,” he stated. “And now we have some.”

Topic:

Source: www.newscientist.com

Judges Evaluate Legality of Trump Administration Cuts at the National Institutes of Health

On Monday, a federal judge in Boston ruled that the termination of grants from the National Institutes of Health signals the end of efforts aimed at diversity-related research topics. Trump’s administration has claimed this decision was “invalid and illegal,” citing discrimination against racial minorities and the LGBTQ community.

US District Judge William Young stated in a non-judicial trial that the NIH breached federal law by capriciously canceling over $1 billion in research grants linked to diversity, equity, and inclusion initiatives.

Judge Young indicated he is reinstating grants awarded to organizations that advocated for such initiatives in democratically led states. He also mentioned that as the case unfolds, more significant decisions might follow.

“This amounts to racism and discrimination against the American LGBTQ community,” remarked Young, a Republican appointee of President Ronald Reagan. “Government discrimination is profoundly wrong; I urge the court to prohibit it, and I will take action in due course.”

Discussing the end of grants for research addressing racial minority issues, Young expressed from the bench that he has “never witnessed such blatant racism” in his 40 years on the bench.

“You judge people of color based on their skin,” he stated concerning the Trump administration. “The Constitution does not permit that.”

The Department of Health and Human Services, representing the NIH and its parent organization, has not responded promptly to requests for statements.

Rachel Meelopol from the American Civil Liberties Union, who represents the grant recipients in the lawsuit, mentioned that Young’s ruling impacts hundreds of grants. The plaintiffs include the American Public Health Association and 16 states led by Massachusetts.

The NIH, the world’s premier funder of biomedical and behavioral research, has terminated approximately 2,100 research grants worth about $9.5 billion and an additional $2.6 billion in contracts since President Donald Trump took office in January. I signed on to protest the cuts last week.

These funding cuts reflect Trump’s broader agenda to reshape the government, reduce federal expenditures, and eliminate support for DEI programs and transgender healthcare. Another federal judge has temporarily blocked the administration’s plan to reduce 10,000 jobs across the NIH and other health agencies.

Trump has also enacted a series of executive orders mandating that institutions ensure grant funding does not support “gender ideology” and puts an end to what the administration deems “discriminatory” DEI programs. Conservative critics argue that these DEI initiatives unfairly target white individuals and others.

Aligned with Trump’s policy objectives, the NIH has directed staff to cease grant funding for research on DEI programs, issues facing transgender individuals, COVID-19 vaccine hesitancy, and funding beneficial to universities in China.

The trial presided over by Young on Monday focused on just a portion of the claims in the consolidated litigation regarding the funding cuts. He intends to consider additional claims later.

Young indicated he would allow political parties to present further evidence before making decisions regarding these claims and determine whether to restore grants beyond those allocated to the plaintiffs.

The cessation of NIH grants, coupled with delays in grant approvals and renewals, has reverberated across universities nationwide, many of which now face the loss of significant portions of their research budgets.

As a result, universities have initiated employment freezes, travel restrictions, reduced class sizes, furloughs, and layoffs.

Numerous universities depend on NIH grants for the majority of their research funding. For instance, Washington University, recognized as the top public institution for biomedical research, reported receiving roughly 1,220 grants from the NIH, totaling about $648 million last year, as per court documents.

Students and faculty at universities have expressed concerns that the funding confusion could lead to brain drain from the United States, as researchers increasingly seek positions abroad. This slowdown also threatens long-term research initiatives, including projects focused on banking and studying the brains of Alzheimer’s patients.

The Trump administration has aimed to reduce other critical research funding sources.

In February, US District Judge Angel Kelly halted regulations that severely restricted government payments for indirect research costs, including equipment, maintenance, utilities, and support staffing. The administration projected that this action would eliminate $4 billion in funding for research institutions.

Source: www.nbcnews.com

Ministry Time Review: An Amazing Time Travel Novel Blending Thriller and Romance

John Franklin’s Fateful Ship Erebus: A 19th Century Painting, Confined to Ice

Pictorial Press Ltd/Alamy

Time Saving
Kaliane Bradley (scepter (UK); A Dedicated Leader Press (US)

Reading various novels for work can sometimes be challenging, especially when you want to find something captivating. However, Time Saving by Kaliane Bradley instantly drew me in with its engaging prologue. It was a brief glimpse into the life of a man sprinting through the snow, hearing his ship signal him. This offered plenty of intrigue for what was to come.

This month’s selection for the New Scientist Book Club has been a resounding success since its release last year. The narrative follows a young civil servant who unexpectedly applies for a mysterious position involving time travel, a concept kept under wraps, allowing individuals from the past to journey to the present.

These “visitors” require support, which is where our unnamed heroine comes in as a caretaker, dubbed a “bridge.” She is assigned to Commander Graham Gore, living with him and assisting him in adjusting to modern life.

New Scientist Book Club

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This is not solely a narrative about time travel; it meticulously explores whether the government would permit time travelers to integrate into society alongside civil servants. The novel confidently posits that, for this reader, it could have crafted Sally without delving into excessive particulars.

One of the intriguing aspects of the story is that Gore is rooted in reality, having been a genuine figure that many remain unaware of. He was the first officer of John Franklin’s ill-fated expedition to the Arctic and met his demise around 1847 or 1848. While the specifics of his final hours remain uncertain, the novel takes a creative approach by transporting him to contemporary London just before his death.

Modern London is full of men from the lost world. But Gore is a resilient and capable officer.

Bradley’s depiction of Gore exemplifies the art of storytelling. She brings him to life with such precision that he appears as a tangible, charismatic individual—rarely do we encounter characters so vividly portrayed in literature.

The vibrant interaction between our young bureaucrat and this spirited officer of the Colonial Royal Navy unfolds within the context of a future version of London, where many individuals from the past now inhabit. Once again, Gore’s resilience shines, highlighting that he is adaptable, making for the most enjoyable segments of the narrative where they learn from one another.

The plot transitions from romance to thriller, composing about 40% sci-fi, 40% romantic comedy, and 20% thriller. I found the initial segment significantly more engaging, though I questioned whether the thriller conclusion would hold up. However, this does not overshadow the fact that the book offers a delightful reading experience, perfect for those looking for fun.

At the conclusion of the novel, Bradley includes a photograph of Gore. Having grown fond of his fictional counterpart, it was a poignant moment to connect with the real historical figure. According to Bradley’s PostScript, he was regarded as “a remarkably fine officer with a kind temperament.”

This beloved, memorable officer represents a captivating twist in history that deserves a place in a bestselling novel nearly two centuries later. Bradley has undoubtedly fashioned a most endearing hero.

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I recommend Emily as well…

The Persian Boy
Maryle Noh (Virago Modern Classics)

While this is not science fiction, it resurrects another historical character—Alexander the Great—through the perspective of Bagoa, a young Persian boy in bondage. For me, this book, along with its precursor, provides all I need to know about Alexander.

Emily H. Wilson is the former editor of New Scientist and the author of the Sumerian trilogy set in ancient Mesopotamia. The series’ final installment, Ninshuval, will be released in August. Connect with her at emilyhwilson.com or follow her on X @emilyhwilson and Instagram @emilyhwilson1

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Using Psychology to Boost Your Confidence in a Swimsuit

Bird's-eye perspective of a bustling beach, Praia de Nazaré, Europe, Portugal. ShutterStock ID 2189816843; Order Form: -; Job: -; Client: -; Other: -

Are these vacationers experiencing “seasonal body image dissatisfaction”?

Shutterstock/Puyalroyo

While winter still lingers in the Northern Hemisphere, we’re nearing the summer solstice. The sun overhead signifies one thing: a surge of lifestyle articles and social media posts encouraging you to “get your beach body ready.”

A friend of mine recently shared his anxiety about summer for this exact reason. “I’ve even stopped trying to get a six-pack,” he confessed. “But I feel really self-conscious without my shirt on.”

This conversation piqued my curiosity about whether this sentiment is widespread. I soon discovered several recent studies addressing “Seasonal Body Image Dissatisfaction,” along with strategies to combat it.

Scott Griffith and his team at the University of Melbourne conducted a groundbreaking study involving 823 gay and bisexual men globally. They found that over 70% reported significant physical dissatisfaction during summer, more so than in any other season, attributing it to societal pressures from the media and the increased exposure of their bodies.

These findings align with a recent analysis of 12 million social media posts from 2020 to 2023, revealing that expressions of self-loathing peaked in July, with similar trends noted for December in both hemispheres.

If any of this resonates with you, it may be beneficial to explore research on mindful self-compassion. This concept emphasizes three core aspects: recognizing that one’s struggles are universal, developing a mindful awareness of our experiences, and refraining from getting lost in negative thoughts and emotions.

Personally, I would love to see a rise in “body-neutral movements” on social media. Unlike “body-positive exercise,” which aims to celebrate our flaws, body neutrality prioritizes bodily function over appearance.

Forthcoming research by Raeanna Kilby and Kristin Mickelson of Arizona State University suggests that body neutrality may more effectively decrease self-objectification compared to body positivity. Jameela Jamil advocates for this perspective, stating, “My body is not an advertising board for others. It’s not something for them to judge, nor for me to judge… I focus on enjoying life to the fullest.”

This summer, my goals are centered on health, happiness, and friendships—the true #gains.

David Robson is an award-winning science writer and author of “The Law of Connection: 13 Social Strategies that Change Your Life.”

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Proba-3: Stunning Image Captures the First Artificial Solar Eclipse

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The sun’s corona appears as it would to the human eye during a solar eclipse, but through a green filter.

ESA/proba-3/aspiics

The synchronized movement of the twin satellites has produced the first artificial solar eclipse in space, revealing the burnt corona of the sun in remarkable detail.

The ProBA-3 mission, launched last December, is operated by the European Space Agency (ESA) and consists of two satellites positioned 150 meters apart.

One of the satellites, known as Occulter, features 1.4-meter wide discs made from carbon fiber and plastic, effectively blocking sunlight coming from the second satellite, Coronagraph. The alignment accuracy of the satellites is within one millimeter for capturing images.

In March, the satellites autonomously synchronized for extended periods, providing lengthy exposures of the solar eclipse. ESA scientists can stitch these exposures together to generate a comprehensive image of the solar corona, the outermost layer of the sun’s atmosphere.

“When I first viewed these images, it was unbelievable,” says Damien Galano from ESA. “But shortly after, it transformed into an incredible sense of achievement and pride for all our hard work.”

The image above captures the visible light of the corona, resembling how it would appear to the human eye but through a green filter.

This image illustrates the light emitted from electron-depleted iron in the most heated sections of the corona.

ESA/proba-3/aspiics

The Proba-3 satellite camera also captures light frequencies linked to specific elements within the solar corona, exemplified by the dark green image above.

“We can clearly see the substantial achievements made during COVID,” remarks Galano.

The sun’s corona shown in polarized white light, artificially tinted to look violet.

ESA/proba-3/aspiics

The image above illustrates the sun’s corona, artificially colored purple in polarized white light. This technique allows scientists to distinguish the polarized light from the hot corona from that scattered by interplanetary dust.

These images were primarily captured to verify the ProBA-3 mission’s functionality. When fully operational, they will take pictures of the artificial food every 19.6 hours.

This will enhance our comprehension of solar corona physics, and according to Galano, it will also improve understanding of solar winds and coronal mass ejections that influence space weather.

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A Fruit and Vegetable-Rich Diet May Enhance Sleep Quality

A recent study conducted by researchers at the University of Chicago School of Medicine and Columbia University revealed that increasing fruit and vegetable intake to five cups daily, as recommended by dietary guidelines, is linked to a 16% enhancement in sleep quality.



Borge et al. Increasing fruit and vegetable intake during the day was found to be associated with improved sleep that same night. Image credit: Guillermo Gavilla.

Observational studies have shown that diets of high quality correlate with better sleep quality.

Despite this, a deeper comprehension of this relationship is essential, as dietary changes could represent novel and natural methods for enhancing sleep.

“We have been striving to maximize our lives,” stated Dr. Esla Tasari, director of the Sleep Center at the University of Chicago.

“The temporal associations and objectively measured outcomes from this study are significant in addressing gaps in crucial public health knowledge.”

Earlier observational research indicated that higher consumption of fruits and vegetables was connected to improved self-reported overall sleep quality, but this latest study is the first to establish a temporal link between specific daily food choices and objectively measured sleep quality.

Healthy young adults in this study recorded their daily food intake through an app and wore wrist monitors to allow researchers to obtain objective measurements of their sleep patterns.

The researchers focused on sleep fragmentation, which indicates the frequency of awakenings during sleep or transitions into deep sleep throughout the night.

They discovered that meal choices had significant correlations with differences in sleep quality the following night.

Participants consuming more fruits and vegetables during the day experienced deeper, more uninterrupted sleep that night, similar to those who included healthy carbohydrates like whole grains.

Based on their findings and statistical modeling, scientists estimate that those who adhere to the CDC’s recommendation of five cups of fruits and vegetables per day could see a 16% improvement in sleep quality compared to those who do not consume these foods.

“A 16% difference is substantial,” said Dr. Tasari.

“It’s remarkable that such significant changes can be detected within just 24 hours.”

Future studies will aim to establish causal relationships, expand the findings to diverse populations, and explore the underlying mechanisms of digestion, neurology, and metabolism that may clarify the positive effects of fruits and vegetables on sleep quality.

Nevertheless, based on current evidence, the authors strongly recommend maintaining a diet rich in complex carbohydrates, fruits, and vegetables for optimal long-term sleep health.

“They are making a difference,” remarked Dr. Marie Pierre St. Onge, director of the Center for Sleep and Circadian Research at Columbia University Irving Medical Center.

“Minor adjustments can impact your sleep. It’s empowering to know better rest is within your control.”

The study was published in the journal Sleep Health this month.

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Header L. Boge et al. We anticipate that increased daytime intake of fruits and vegetables will lead to less disrupted nighttime sleep in younger adults. Sleep Health Published online on June 11th, 2025. doi: 10.1016/j.sleh.2025.05.003

Source: www.sci.news

Hubble Space Telescope Reveals New Images of NGC 4449

Astronomers utilizing the NASA/ESA Hubble Space Telescope have captured remarkable new images of the Dwarf Starburst Galaxy NGC 4449.



This Hubble image illustrates NGC 4449, a galaxy of dwarf stars located roughly 12.5 million light years away within the Canes constellation. Image credits: NASA/ESA/Hubble/E. Sabbi/D. Calzetti/A. Aloisi.

NGC 4449 is situated about 12.5 million light years away in the constellation of Canes.

Also known as Caldwell 21, Leda 40973, or UGC 7592, this galaxy is approximately 20,000 light-years in age.

NGC 4449 was first identified by German-born British astronomer William Herschel on April 27, 1788.

This galaxy is part of the M94 Galaxy group and is in close proximity to the local group that contains our Milky Way.

“NGC 4449 is a dwarf galaxy, meaning it is significantly smaller than our Milky Way and contains fewer stars,” a Hubble astronomer remarked.

“However, its small size is deceptive; NGC 4449 is prolific in star formation.”

“This galaxy is referred to as a Starburst galaxy because it produces new stars at a rate much higher than would be expected for its size.”

“While most Starburst Galaxies primarily produce stars in their centers, NGC 4449 is scattered with bright young stars throughout its structure.”

Astronomers believe this global surge in star formation has resulted from interactions between NGC 4449 and its neighboring galaxies.

“Due to its proximity, NGC 4449 offers a valuable opportunity for Hubble to investigate how intergalactic interactions influence new star formation,” they noted.

The new color image of NGC 4449 is derived from Hubble observations utilizing the Advanced Cameras for Surveys (ACS) and the Widefield Camera 3 (WFC3) across the UV, near-infrared, and optical segments of the spectrum.

Seven filters were employed to capture various wavelengths, assigning different hues to each monochrome image linked to the specific filters.

“The Hubble images of NGC 4449 were previously released in 2007,” the researchers stated.

“This updated version includes several additional wavelengths of light gathered by Hubble through multiple observational programs.”

“These programs encompass groundbreaking science, ranging from exploring the history of star formation in NGC 4449 to mapping galaxies with the brightest, hottest, and most extensive stellar structures.”

Source: www.sci.news