Exploring the Concept of Self: Where Do You Believe Your Identity Resides?

Do you think with your head or your heart?

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Engaging in self-exploration can enhance your understanding of your mind. Start by placing your finger on the area of your body that resonates with your sense of self. Avoid overthinking this; there are no right or wrong choices. Simply connect with your identity and where you feel most centered.

If you’re like most individuals, you’ll likely touch either your head or your heart. This choice may seem trivial, but several studies indicate that it can reveal your thinking style—whether you lean toward logic and analysis or intuition and emotion. Understanding how to switch between these modes can remarkably improve your decision-making capabilities.

It’s widely accepted that our decisions hinge on whether we think with our heads or hearts, a notion that’s prevalent in popular culture. Interestingly, this connection was first studied scientifically in 2013 by researchers Adam Fetterman from the University of Houston and Michael D. Robinson from North Dakota State University, who examined if our perceptions truly influence our actions.

Through self-report questionnaires, it emerged that “head-locators” frequently categorized themselves as rational thinkers, while “heart-locators” identified as emotionally driven. Remarkably, these perceptions correlate with objective behavioral metrics. For instance, Fetterman and Robinson observed that those who considered themselves ‘head-locators’ tended to excel on general knowledge exams, indicating a more cognitive-focused lifestyle. Conversely, ‘heart-locators’ often reported heightened sensitivity in stressful scenarios, reflecting their emotional depth.

The researchers found that individuals’ self-perception could predict outcomes related to their rational or emotional thinking styles a year later, signifying that this is a stable trait. However, many aspects of our psychology remain pliable. Just as levels of extraversion can fluctuate based on social context, it’s worth questioning whether our self-concept is equally adaptable. Robinson’s team explored this concept in a recent study.


In the studies, participants (n=455) were prompted to envision themselves engaging in various activities, rating how prominently their self-awareness was rooted in their brain or heart on a scale from 1 (not present) to 7 (very present). As predicted, responses varied based on the task; for example, self-awareness was more pronounced when engaged in analytical activities versus emotional reflection. This flexibility related directly to test performance. Participants who exhibited higher adaptability in their self-awareness scored better on key assessments, such as the American College Testing (ACT) and the North Dakota Emotional Ability Test, which assesses emotional intelligence.

These findings align with the “dual process theory” of cognition, which posits that our mental systems engage in either methodical reasoning or instinctual responses. Robinson’s research suggests that self-perception impacts which cognitive approach we employ, with those adept at reverting between modes enjoying superior decision-making capabilities in various domains. High achievers were found to effectively practice the “art of employing strategies” suitable for each task, merging head-driven logic with heart-driven intuition.

Can we all cultivate this skill? When I queried Robinson, he posited, “Achieving conscious control over this mental flexibility may require time and practice, possibly through meditation and other body-focused exercises.” As someone who leans intellectually, he admitted the journey can be challenging.

In a preliminary experiment from their 2013 study, having participants touch specific body locations altered their cognitive processes. For example, touching one’s temple promotes logical thinking, while touching the chest encourages instinctual moral reasoning, akin to the famous trolley problem. These bodily interactions also improved performance on true/false tests necessitating logical reasoning by around 9%.

Although I won’t depend on this method without larger trials to validate it, my awareness of my self-location has shifted since learning about Robinson’s ongoing studies. At times, my sense of self seems to align straight behind my eyes, while other moments place it lower in my ribcage. The contrast is so vivid that I now recognize transitions I once overlooked. By acknowledging these shifts, I gain deeper insights into what influences my decision-making.

That’s the beauty of psychological research—it unveils critical facets of our existence that we often overlook.

David Robson’s latest book is The Law of Connection: 13 Social Strategies That Will Change Your Life. If you have questions for his column, feel free to reach out: davidrobson.me/Contact

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Source: www.newscientist.com

Exploring the Limitations of AI Safety Management Practices

As organizations like Anthropic, Google, and OpenAI develop cutting-edge artificial intelligence systems, they are increasingly focused on implementing safeguards to prevent misuse—such as spreading disinformation, creating weapons, or hacking networks.

However, recent findings by Italian researchers reveal that these protective measures can sometimes be bypassed through poetic prompts.

By using poetic language, the researchers successfully tricked 31 AI systems into ignoring internal safety protocols. For example, starting prompts with metaphors like “The iron seed sleeps best in the unsuspecting womb of the earth away from the sun’s reproachful gaze” demonstrated how these systems can be manipulated to execute dangerous tasks.

This highlights a concerning trend: for many AI systems, guardrails intended to prevent risky behavior are merely suggestions, rather than effective barriers. Researchers are increasingly alarmed as AI systems become adept at exploiting vulnerabilities and engaging in risky operations.

Recently, Anthropic announced restrictions on the release of its latest AI system, Claude Mythos, to select organizations due to its rapid vulnerability detection capabilities in software. OpenAI echoed similar sentiments, choosing to share its technology with a limited group of trusted partners.

Since the AI boom initiated by OpenAI in late 2022, studies have confirmed the ability of users to bypass safety measures in AI systems. Closing one loophole often leads to the emergence of another.

“Everyone in the field acknowledges that establishing effective guardrails is challenging and will continue to be so for the foreseeable future,” stated Matt Fredrickson, a computer science professor at Carnegie Mellon University and CEO of Gray Swan AI, which specializes in securing AI technologies. “Determined individuals can evade these systems with relative ease.”

The repercussions of bypassing guardrails are significant. In an already misinformation-heavy online environment, AI systems are being employed to disseminate conspiracy theories and false claims. Anthropic has also reported that its technology played a role in an international cyberattack, teaching biosecurity experts how to unleash fatal pathogens.

The poetic bypass is just one of many methods hackers use to circumvent protections in systems like Anthropic’s Claude, Google’s Gemini, and OpenAI’s GPT. Major AI firms share similar foundational techniques for implementing guardrails, yet these measures are surprisingly easy to overcome.

“Poetry is merely one way to reframe a prompt and breach guardrails,” explained Piercosma Visconti, co-founder of AI firm Dexai and a researcher in the study.

The act of circumventing AI guardrails is commonly referred to as “jailbreaking.” This often entails submitting specific English sentences that prompt actions the AI has been programmed to avoid.

Jailbreaking techniques feature a variety of creative names, including stealth prompt injection, role-playing, token smuggling, polyglot Trojans, and greedy coordinate gradient attacks. Notable attack names include Crescendo, Deceptive Joy, and Echo Chamber.

Weak defenses in AI systems have already led to the spread of fabricated interviews, false wartime evidence, and synthetic rumor-mongering. Research conducted three years ago by international counterterrorism experts revealed far-right extremists using social media to circumvent moderators with “terrible but legal” AI content.

Experts are concerned that models could be jailbroken to mislead social media users with seemingly authentic content, overwhelm fact-checkers with misinformation, and tailor false narratives for specific audiences.

Some of these methods are widely disseminated online, while others remain undisclosed. Many discoverers of new jailbreaks keep them secret to exploit these loopholes before AI companies close them.

AI systems like Claude and GPT learn patterns from vast datasets, including Wikipedia, news articles, and curated texts from the internet. However, before releasing these systems to the public, companies like Anthropic and OpenAI explore potential exploits.

In their unfiltered states, these systems can potentially instruct users on purchasing illegal firearms online or creating hazardous substances using household items. Consequently, companies train their systems to refuse certain requests through a method known as reinforcement learning.

This often involves showcasing thousands of prohibited requests to the system. Through this analysis, the system can learn to identify other dangerous requests. However, this method only partially succeeds.

In some situations, AI companies might opt not to address vulnerabilities, believing that while weak guardrails could facilitate malicious activities, they also enable benign actions to counter them.

Recently, researchers at cybersecurity firm LayerX found that Claude’s guardrails could be bypassed by simply entering a few straightforward sentences into the AI system.

When told they were “penetrating” a computer network for testing purposes, Claude’s AI technology was directed to launch attacks on the network. This technique could potentially enable malicious hackers to extract sensitive information from businesses, governments, and individuals.

While closing this loophole may protect Claude’s networks, it could simultaneously hinder companies from safeguarding their own systems. LayerX informed Anthropic of this vulnerability weeks ago, yet it remains an open issue.

LayerX CEO Olu Eshed warned that this strategy might backfire. “Eventually, we will witness a surge of attacks utilizing these AI models, compelling us to rethink our security protocols,” he predicted.

Last year, researchers from Cisco and the University of Pennsylvania achieved breakthrough results by developing AI models that produced harmful outcomes using malicious prompts. Their efforts successfully jailbroke Meta and Chinese AI model DeepSeek chatbots 100% of the time, and over 80% of attacks against Google and OpenAI models were successful.

(The New York Times has filed a lawsuit against OpenAI and Microsoft, claiming copyright infringement related to its AI systems, with both companies denying these allegations.)

If guardrails are compromised, automated large-scale influence campaigns could become feasible, as researchers at the University of Technology Sydney demonstrated. By disguising their requests as “simulations,” they convinced a commercial language model to create a disinformation campaign against Australian political parties, complete with visuals, hashtags, and tailored posts for specific platforms.

In addition to establishing guardrails, these companies also employ other tools to monitor system activity, identify suspicious behaviors, and ban accounts infringing on their terms of service.

“Claude is built with robust, multi-layered protections designed to work in unison, including model training and layered guardrails,” stated Anthropic spokesperson Palul Maheshwary. “Bypassing one layer doesn’t circumvent the others.”

In a concerning revelation, Anthropic found that a group of state-sponsored hackers from China was employing Claude to breach the computer systems of approximately 30 companies and government agencies worldwide.

Despite the robust security technologies, experts caution that flaws remain, as companies struggle to monitor extensive global activity while also ensuring legitimate users are not excluded.

When restricted by the security measures of services like Claude and GPT, users may turn to open-source AI systems. These platforms allow for their underlying software to be freely replicated, modified, and shared.

Such systems can be altered to eliminate guardrails. A novel approach called Heretic enables users to remove system guardrails with minimal effort, essentially undoing months of guardrailing training through sophisticated algorithms.

“A year ago, this process was highly complex,” noted Norm Schwartz, CEO of AI security firm Alice. “Today, it can be controlled effortlessly via a mobile device.”

Source: www.nytimes.com

Why Particle Physicists Enjoy Working in the Field: Exploring Their Passion and Discoveries

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Exploring Different Types of Fields in Physics

Exploring Different Kinds of Fields

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As I prepared to launch my column for New Scientist, my editor inquired about a title. I proposed “Field Notes from Space and Time.” This title serves a dual purpose for me as a physicist, subtly referring to the scientific practice of field observations—notes recorded in the field akin to a lab notebook—while also hinting at a critical concept in particle physics: the field itself.

In classical terms, one might envision a “field” as a vast agricultural space, but in physics, it embodies a more abstract notion. A field represents a mathematical framework that assigns numerical values to points across both space and time, characterizing various physical phenomena. For instance, when a magnet approaches a refrigerator door, a magnetic force exists between them, with a corresponding magnetic field value that intensifies as the distance decreases.

Intriguingly, the term “field,” in this scientific context, emerged thanks to 19th-century scientist Michael Faraday, who investigated the magnetic properties of bismuth. While working on my recent manuscript, I delved into Faraday’s diary and examined his initial references to field concepts. One can’t help but wonder how he conceptualized these ideas, particularly given his working-class origins and an upbringing deeply intertwined with the land. I envision Faraday pondering the invisible forces at play in the expansive environments familiar to his family.

The notion of fields extends beyond magnetism. A groundbreaking advancement in the 20th century arose at the intersection of electromagnetism and quantum physics, leading to the realization that particles and waves share a dual relationship. Notably, particles such as electrons can also be perceived as waves, while electromagnetic fields can be represented as particles (termed photons). As the scientific community embraced wave-particle duality, a deeper connection between quantum theory and fields became apparent.

To forge a complete quantum model of photons, we once again turned to fields—this time, quantum fields. Just as magnetic fields quantify the magnetic force at specific points, quantum fields determine the creation and annihilation of particles at various locations. Consequently, all electrons emerge from a quantum electronic field. It is believed that a similar undiscovered realm of dark matter also exists, behaving as if composed of particles despite being invisible to the naked eye. Our universe brims with particles springing from a vacuum, facilitated by quantum fields. Thus, when I contribute to this column, I am genuinely crafting field notes from both space and time.

What are you reading?

I am captivated by The Herman Melville Declaration by Barry Sanders.

What are you watching?

I am enjoying the final season of Hacks.

What are you working on?

Following the US launch of The End of Space and Time, we are currently focusing on its release in the UK!

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  • Electromagnetism/
  • Quantum Physics

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Source: www.newscientist.com

Exploring the Stunning Core of Messier 77: A Deep Dive into the Galaxy’s Heart

Discover stunning new images captured by NASA/ESA/CSA’s James Webb Space Telescope featuring the barred spiral galaxy Messier 77, showcasing its mesmerizing swirl of dust, vibrant newborn stars, and an extraordinarily active nucleus.



This breathtaking image of Messier 77, taken by Webb’s Mid-Infrared Observatory (MIRI), illustrates its unique spiral arms, dust within its disk, and an exceptionally bright core. The orange lines radiating from the galaxy’s center are diffraction spikes, an optical phenomenon from Webb’s design. Image credit: NASA / ESA / CSA / Webb / A. LeRoy.

Situated about 62 million light-years from Earth in the constellation Cetus, Messier 77 ranks among the brightest and most extensively studied galaxies visible from Earth.

This galaxy, commonly referred to as the Squid Galaxy, NGC 1068, LEDA 10266, and Cetus A, boasts an apparent magnitude of 9.6.

First discovered in 1780 by French astronomer Pierre Méchain, Messier 77 was initially recorded as a nebula before its true galactic nature was revealed.

As technology advanced, astronomers like Charles Messier recognized the galaxy’s immense scale and complexity.

Measuring approximately 100,000 light-years in diameter, Messier 77 is one of the largest entries in the Messier catalog, with a gravitational influence strong enough to distort its neighboring galaxies. Additionally, it is one of the nearest galaxies exhibiting an active galactic nucleus (AGN).

Messier 77 is classified as a Type II Seyfert galaxy and is particularly luminous in infrared wavelengths.

According to Webb astronomers, “At the heart of Messier 77 lies a compact region filled with hot gas that shines brighter than the entire galaxy, surpassing even the capacity of Webb’s camera.”

“Powered by a supermassive black hole weighing 8 million solar masses, this AGN pulls gas into rapid orbits, causing collisions that generate immense radiation.”



This striking image of Messier 77, captured by Webb’s Near Infrared Camera (NIRCam), brilliantly showcases its features. Image credit: NASA / ESA / CSA / Webb / A. LeRoy.

“Messier 77 is not only recognized for its visible AGN but also as a vigorous star-forming galaxy,” they added.

“Near-infrared observations reveal a widening bar in the central region, untraceable in visible-light images of the galaxy.”

“This bar is encircled by a bright ring known as the starburst ring, formed by the inner sections of Messier 77’s two spiral arms.”

“Starburst zones in galaxies typically exhibit remarkably high star formation rates.”

“This ring, exceeding 6,000 light-years in diameter, displays intense starburst activity characterized by dense orange bubbles surrounding the ring.”

“Given Messier 77’s relatively close proximity to Earth, this starburst ring serves as an exemplary case study in galactic phenomena.”

“As an active spiral galaxy, Messier 77’s disk is abundant in gas and dust, both of which are vital for future star formation.”

“Webb’s MIRI highlights the galaxy’s view filled with the glow of interstellar dust particles, depicted here in blue.”

“These particles form massive vortexes of swirling filaments resembling smoke, with cavities interspersed.”

“Glowing orange bubbles, crafted by newly formed star clusters, can also be seen along the galaxy’s arms.”

“Beyond Webb’s focused field of view, Messier 77’s arms integrate into a faint hydrogen gas ring, thousands of light-years wide, where additional star formation is underway.”

“Delicate filaments of hydrogen gas stretch across this ring into intergalactic space, forming the outermost layer surrounding the galaxy.”

“These tentacle-like filaments contribute to the moniker Squid Galaxy for Messier 77.”

Source: www.sci.news

Exploring the Works of an Imaginary Mathematician: Discovering New Insights in Mathematics

A clandestine society of mathematicians has been operating under pseudonyms for nearly a century

Shutterstock/Stephen Ray Chapman

One of the most influential figures in modern mathematics, Nicolas Bourbaki, has reportedly been researching for almost a century, producing numerous books and publications that guide the entire field. Interestingly, Bourbaki is a pseudonymous figure who does not exist as an actual individual.

Bourbaki represents a secretive collective of mathematicians, initially formed in France in 1934. Their primary objective was to modernize mathematics textbooks, transforming them to meet contemporary reader needs. However, this endeavor culminated in the creation of an innovative approach to mathematical writing, impacting the field for decades.

The group initially anticipated that their study would comprise about 1,000 pages and be completed in six months. By 1935, Bourbaki had expanded its vision to include six interconnected volumes, aiming to “provide a comprehensive foundation for modern mathematics,” as expressed in an explanatory preface. While they were correct about the length, they were notably mistaken regarding the timeline.

Though these volumes (which eventually comprised several physical books) were intended to be read sequentially, Bourbaki’s first published text in 1939 turned out to be the concluding chapter of the first book on set theory. The group later published different sections intermittently before returning to finish set theory in 1954, finally completing the entire project in 1970. Collectively labeled as elements of mathematics, this singular title underscores the cohesion of the mathematicians’ work. The completion of this monumental collection extended into the 1980s, reaching nearly 4,000 pages. Even after that, Bourbaki continued to release new works as the original scope broadened.

This unorthodox publishing approach stemmed from Bourbaki’s distinctive methodology. The original group comprised six young mathematics professors, including Andre Weil, a prominent figure in number theory and algebraic geometry. Most members were former students of the École Normale Supérieure in Paris, and the group’s name emerged from a prank revolving around the notoriously obscure Bourbaki theorem.

This playful spirit fostered a strong sense of camaraderie. Meetings were lively, often involving shouting matches and humorous banter. One member crafted the proposed text and presented it line by line for critique and discussion, leading to a revised draft before reaching consensus. Given that chapters took an average of ten years to produce, the protracted timeline is understandable. This mathematical endeavor spanned generations, as Bourbaki members were required to retire at 50, making way for new recruits.

Eternal Challenges in Mathematics

Founding members of the Bourbaki Group gathered in France in 1935

Charmet/Bridgeman Image Archive

So, what was Bourbaki’s actual contribution? Despite its unorthodox methods, the group’s work was notably serious and thoroughly detailed. The cornerstone of their research, set theory, aimed to tackle the perennial challenge in mathematics: the idea that mathematical objects are fundamentally independent of human language and symbols.

To illustrate this, consider the word “addition” or the symbol “+”. These terms have an arbitrary connection to the underlying mathematical concepts. As long as there’s an agreement on the meaning of “addition,” any string of symbols could be utilized to indicate it. Conversely, addition has a definitive relationship with subtraction; one operation is the inverse of the other, independent of their nomenclature.

In practical terms, labeling mathematical concepts does not present a significant challenge, as mathematicians adhere to standardized mappings between ideas and symbols. However, in principle, contradictions and inconsistencies may emerge.

Bourbaki was not the inaugural attempt at formalization (as mentioned in my previous writings), but his approach was perhaps the most meticulous. For instance, he took care to define the number 1 in a footnote on page 158 of set theory. Bourbaki clarified that “the symbol ‘1’ should not be confused with the common language interpretation ‘one'”; instead, it should be understood through a rigorous definition:

τZ ((∃u)(∃U)(u = (U, {∅}, Z) and U ⊂ {∅} × Z and (∀x)((x ∈ {∅}) ⇒ (∃y)((x, y) ∈ U)) and (∀x)(∀y)(∀y’)(((x, y) ∈ U and (x, y’) ∈ U) ⇒ (y = y’)) and (∀y)((y ∈ Z) ⇒ (∃x)((x, y) ∈ U))))

Don’t worry if this seems daunting; a simplified explanation is that ∅ represents a set devoid of elements, referred to as the “empty set.” Consequently, 1 is defined as {∅}, indicating a set containing only one item (which, in this case, is the empty set). More details on this concept can be found in a previous column.

Astonishingly, embedded within this sea of symbols is a broader and more complex formal definition. Each symbol is elaborately defined based on earlier texts using only designated symbols. Bourbaki never elaborated these entirely; the footnote mentions that completing this definition would require tens of thousands of symbols — an estimation soon revealed to be vastly understated. Later mathematicians calculated that articulating the full formula for the number 1 would necessitate over 4.5 billion symbols, or more precisely, 2,409,875,496,393,137,472,149,767,527,877,436,912,979,508,338,752,092,897 symbols, depending on your definition of precision.

Clearly, mathematicians would need to occasionally abandon such stringent formalism if they wished to accomplish their objectives. Bourbaki acknowledges this necessity, while maintaining that utilizing shorthand terms like “1” is an “abuse of language.” By establishing foundational rules, Bourbaki granted mathematicians the flexibility to deviate as needed.

Emerging Mathematical Challenges

So, what achievements stemmed from all this labor? One significant outcome was Bourbaki’s aspiration to unite mathematics as a cohesive discipline. In theory, if terms and concepts from various mathematical domains could be expressed using a common set of symbols, it would yield a rigorous framework for transitions between fields. Although few actually practice this, it positions mathematics on a more solid philosophical foundation.

In the decades that followed, Bourbaki’s influence has proven unexpectedly significant, particularly as mathematicians increasingly explore computer-assisted formalization to verify proofs generated by artificial intelligence. The collective also introduced numerous concepts and symbols, many of which remain integral to contemporary mathematics (for instance, ∅ representing the empty set). On a broader scale, the Bourbakian writing style continues to shape modern mathematical textbooks.

However, Bourbaki was not without critique. Following the publication of elements of mathematics, some mathematicians expressed discontent with the group’s claims of excessive rigor. Oddly enough, Bourbaki inadvertently incited a misguided initiative to reform mathematics education in schools. Emerging in France during the late 1950s, this movement, dubbed New Mathematics, sought to replace traditional educational methods with rigorous set-theoretic approaches based on Bourbaki’s teachings. The intention was to grasp the general principle of multiplication rather than memorizing specific multipliers, such as 3 × 4 = 12.

The “New Math” movement faced extensive criticism and was largely deemed a failure. Parents and teachers alike struggled to understand the curriculum. Bestselling critiques like Why Can’t Johnny Add? emerged, and by the late 1970s, the initiative had largely dissipated. Additionally, this decade brought challenges for Bourbaki, including legal disputes with publishers over copyright and royalties.

Despite these hurdles, Bourbaki remains relevant today. New chapters will be released this year alone. However, the identity of the author remains a well-guarded secret. This anonymity allows mathematicians to regard Bourbaki as a quirky, eccentric relative: appreciated for essential contributions, yet sparing themselves from the discomfort of personal association.

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Source: www.newscientist.com

Exploring Eurovision: Scientists Analyze 1,763 Songs for Nostalgia and Emotional Impact

Feedback from New Scientist

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Eurovision 2026: Are You Ready?

The highly anticipated 2026 Eurovision Song Contest is fast approaching, with the grand finale set for Saturday, May 16th. Whether you’re a fan or not, get ready for an entertaining spectacle!

Coinciding with this buzz, a comprehensive study published in Royal Society Open Science delves into the rich history of Eurovision. Researchers analyzed data from every contest between 1956 and 2024, totaling 1,763 songs. They categorized entries by various musical attributes, including language, themes, lyrics, and genre, utilizing AI tools for analysis. It’s hard to ignore the auditory implications of such a massive dataset!

The analysis unearthed intriguing insights, revealing that past research identified 12 major themes prevalent in popular songs, such as desire, heartbreak, and pain. However, only 11 themes are reflected in the Eurovision entries, as researchers excluded the theme ‘Jaded’ for being underrepresented.

The data also shows a significant decline in songs expressing nostalgia, while themes of pain, rebellion, despair, confusion, and escapism have become more prominent over the years. The 1970s marked a notable rise in songs depicting disorder and escapism, reflecting the societal crises of that era. However, the increase in ‘pain’ themes began not until the 2000s, post-Great Recession, suggesting a correlation.

Interestingly, songs have shifted from acoustic to electronic styles, with a growing prevalence of English lyrics over national languages. This trend indicates that Eurovision participants are deliberately aligning their entries with the winning formula established by past champions.

There are notable exceptions, as countries like France, Italy, Portugal, and Spain continue to champion their native languages, suggesting a deeper cultural rationale beyond mere competition.

The researchers conclude by emphasizing the notion of “organizational learning” among Eurovision participants, reflecting an ongoing adaptation to the competition landscape. Feedback sees this as a testament to the enduring allure of the contest.

Moss Appeal: A Niche Attraction

In a previous article, we discussed a park filled with intricate foraminiferal carvings and pondered the existence of niche science-themed attractions. This inspired reader John Wilson to share information about the Serenity Moss Garden in North Carolina.

Spanning about 900 square meters, this moss-covered mountainside offers visitors a unique experience, though John humorously described it as “more like a climate-controlled box” rather than a traditional museum.

Feedback realizes that our quest for niche appeal may have been too limited. Are there any other unique attractions, such as a museum dedicated to Plecopteran (stoneflies) or specialized exhibits featuring beach pebbles?

New Math? A Logical Dilemma

Regardless of our professional backgrounds, math can sometimes overwhelm us. Navigating concepts like converting square kilometers to square meters can be perplexing.

Recently, U.S. Secretary of Health Robert F. Kennedy Jr. faced scrutiny for claiming a 600% decrease in drug prices, an assertion deemed mathematically implausible by rival politicians.

Feedback believes RFK Jr. has been misled. A 100% drop suggests prices have plummeted to zero, a mathematical limit. In theory, this could even lead to negative pricing, but the complexities of rate changes should ideally be left to mathematicians.

In a curious twist, RFK Jr. stated, “If that drug goes from $100 to $600, that’s a 600% price increase.” This form of reasoning feels like a new, perplexing brand of logic—while the premises hold, the conclusion is unmistakably flawed.

Contribute Your Story

If you have a story or feedback, share it with us! Email your article to Feedback and include your home address. You can also find this week’s and past feedback on our website.

Source: www.newscientist.com

Exploring the Medicinal Benefits of Honey: Does It Really Work?

Health benefits of honey

Health Benefits Vary Depending on Honey Type

Tihomir Likov/Shutterstock

As a passionate honey enthusiast, I relish the taste of honey in everything from buttery sourdough bread to refreshing smoothies and savory Asian stir-fries. I often justify my sweet indulgence by recalling its numerous health benefits. But how true are these claims?

Honey is widely recognized as a healthier alternative to refined white sugar. Its less processed nature results in a more stable blood sugar level. Honey, derived from plant nectar and enriched by bees, primarily consists of monosaccharides like glucose and fructose, along with trace sugars like trehalose, kojibiose, nigerose, melibiose, gentiobiose, and palatinose. However, the health benefits of honey largely depend on the sources of nectar collected by the bees.

One useful measure for comparing honey to other sugars is the glycemic index (GI), which indicates how quickly a food raises blood sugar levels. Refined white sugar has a GI score of approximately 65. In contrast, honey’s GI can vary significantly; for example, honey made from Sidr tree nectar in the Middle East boasts a GI of just 32, while Greek thyme honey reaches a GI of 85. Interested in comparing various honey types? Check out the University of Sydney’s extensive GI database for more information.

The variation in GI values can be attributed to the differing ratios of glucose and fructose in honey. Glucose raises blood sugar levels rapidly, whereas fructose does not. Unlike refined sugar, which contains a consistent ratio of glucose and fructose, honey’s composition can vary, impacting its glycemic response.

Additionally, honey contains components like phenolic acids and flavonoids that may slow glucose absorption in the intestines, thus contributing to lower GI values. These compounds are also believed to possess antioxidant properties that provide mild protection against ailments like cancer and heart disease—conditions often associated with oxidative stress. However, it’s essential to remember that fruits and vegetables are far superior sources of antioxidants as they are lower in sugar and calories.

Opting for raw honey, often available at local markets, is considered a healthier choice compared to mass-produced varieties, as it retains a higher concentration of beneficial phenolic acids and flavonoids. Raw honey is freshly harvested directly from the hive and minimally processed. Unlike raw milk, raw honey is generally safe to consume, although there are risks of contamination from Clostridium botulinum, a bacterium producing a potent neurotoxin. This toxin is particularly hazardous for infants under one year. Parents should avoid giving honey to infants, and it’s advisable to steer clear of Botox for little ones as well.

Mass-produced honey undergoes pasteurization to eliminate microorganisms, compromising some beneficial antioxidants in the process. Furthermore, cheaper honey products may be mixed with sugar syrup, which dilutes their natural properties. Some honey products even falsely claim to be natural aphrodisiacs, containing hidden drug ingredients like tadalafil, the active component in the erectile dysfunction medication Cialis.

A straightforward way to gauge the phenolic acids and flavonoids in honey is by examining its color. Darker honey typically indicates higher levels of these beneficial compounds. Personally, I enjoy purchasing rich, dark brown raw honey from a local beekeeper, which I find far superior in taste compared to supermarket varieties. His bees gather nectar from local eucalyptus trees, which likely contributes to its lower GI value based on tests conducted on other eucalyptus honeys.

Is Honey Effective for Hay Fever or Just a Myth?

Professional Studio Images/Getty Images

While many believe that consuming locally produced honey may relieve hay fever, this idea is rooted more in folklore than in scientific fact. The premise is that honey contains trace amounts of local pollen that might help the immune system acclimatize to these allergens. However, hay fever is primarily triggered by pollen from trees that bees do not visit; these trees release airborne pollen that can irritate your nasal passages. In fact, hay fever is caused by such wind-dispersed pollen.

Nonetheless, honey does demonstrate potential benefits in soothing symptoms like a sore throat and cough, likely due to its pleasant consistency and natural antibacterial properties. A review of existing studies found that honey could alleviate cough symptoms in children and was comparable in effectiveness to over-the-counter cough syrups. Anyone who has tried a warm lemon-ginger tea with honey can attest to its comforting effects when feeling unwell.

Honey’s efficacy extends beyond soothing sore throats; it also plays a significant role in wound care. Medical-grade Manuka honey, which is recognized in countries like the UK, US, and Australia, is often used in ointments and dressings. This honey is made from the nectar of Manuka tea tree flowers and is sterilized to eliminate harmful microorganisms. It possesses high levels of an antibacterial compound called methylglyoxal, which is effective in preventing or treating wound infections. Studies highlight its healing properties.

However, it’s crucial to heed warnings about honey derived from rhododendron flowers, especially from certain species native to Nepal and Turkey. This type of honey can cause “mad honey disease,” leading to symptoms such as confusion, dizziness, and vomiting. Historically, it has even been weaponized; for instance, Mithridates VI Eupator used it strategically against Roman troops in 65 BC, luring them into confusion. Do you dare to wonder what happened next?

While honey may not alleviate my hay fever, I still enjoy it—after all, there’s no sweeter delight than the joy it brings me.

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Exploring the Thin Atmosphere of Pluto’s Small, Frozen World

A team of Japanese astronomers has discovered a thin atmosphere surrounding the trans-Neptunian object (612533) 2002 XV93, which has an approximate diameter of 500 km. This celestial body is too small and cold to retain a substantial atmosphere.



Artist’s conception of trans-Neptunian object 2002 XV93. Image by: National Astronomical Observatory of Japan

“The cold regions of the outer solar system host thousands of small bodies known as trans-Neptunian objects (TNOs) because they orbit outside Neptune.” according to Dr. Ko Arimatsu from Ishigakijima Observatory.

“While Pluto, the most well-known TNO, has been observed with a thin atmosphere, studies of other TNOs generally yield negative results.”

“Most TNOs are extremely cold and possess weak surface gravity, making it unlikely for them to maintain an atmosphere.”

Astronomers utilized stellar occultation to study trans-Neptunian object 2002 XV93, measuring its light fluctuations as background stars passed behind it.

“With a diameter of around 500 km, 2002 XV93 is significantly smaller than Pluto, which has a diameter of 2,377 km,” they noted.

“On January 10, 2024, 2002 XV93’s orbit caused it to briefly obscure a background star.”

“As the star gradually dimmed while being obscured by 2002 XV93, it indicated the possibility of light attenuation due to the thin atmosphere, or a sudden disappearance as it moved behind the solid surface of the TNO.”

The researchers concluded that the observed behavior best supports the existence of a thin atmosphere around 2002 XV93.

They estimate that this atmosphere could vanish in approximately 1,000 years unless it is replenished in some manner.

This suggests that the atmosphere must have formed or been replenished relatively recently.

“Observations with the NASA/ESA/CSA James Webb Space Telescope reveal no indications of frozen gas that could sublimate to create an atmosphere on 2002 XV93,” the authors stated.

“One hypothesis is that deep internal processes brought frozen or liquid gas to the surface of the TNO.”

“Alternatively, a comet may have collided with 2002 XV93, releasing gas and forming a temporary atmosphere.”

“Further investigations are essential to clarify these possibilities.”

“This finding sheds light on the potential for even smaller TNOs to temporarily harbor atmospheres, challenging conventional volatile retention models,” the researchers concluded.

“Our results imply that some distant icy bodies could be sustained by ongoing cryovolcanism or exhibit atmospheres formed by recent impacts from small icy objects.”

The team’s research paper was published in the journal Nature Astronomy.

_____

Kazuya Arimatsu et al.. Discovery of the atmosphere surrounding a trans-Neptunian object beyond Pluto. Nat Astron, published online on May 4, 2026. doi: 10.1038/s41550-026-02846-1

Source: www.sci.news

Exploring How Disasters, Wars, and Princess Diana’s Death Influenced Rising Birth Rates of Boys

You may have encountered the concept that the increase in the number of boys born after wars can be perceived as a form of divine intervention or karmic response to those who lost their lives in battle.

However, this phenomenon isn’t restricted to wartime. Significant stressors in a nation’s history, such as natural disasters, famine, or collective mourning periods, can also impact male birth rates.

For instance, a study led by Maltese pediatrician Professor Victor Grech in 2015 revealed that the birth rate of boys in the UK temporarily dipped following the death of Princess Diana.







These fluctuations might be connected to the established link between stress and miscarriage rates. Recent research indicates that miscarriages affect female fetuses slightly more than male ones.

But why exactly is this the case? It remains unclear.

Yet, female embryos appear to be particularly vulnerable during the first trimester, leading to an increased risk of repeated miscarriages.

Therefore, during times of heightened stress—like wartime—the increased frequency of miscarriages might contribute to a skewed sex ratio favoring boys.

Additionally, another factor influencing the rise in male births post-war is that overall birth rates tend to surge when soldiers return home. This is often attributed to increased intimate activity among couples.

But why does this result in more boys? The theory suggests that male births occur slightly more often when conception happens at the onset or end of the menstrual cycle, while female births are more likely to occur when conception happens mid-cycle.

As couples engage in sexual activity more frequently, they may conceive during the “male” days of the cycle. This leads to a slight but noticeable increase in male births when many couples are intimate.

While this difference isn’t significant enough for those trying to conceive a specific sex, in the context of hundreds of thousands of births, it could help adjust the overall sex ratio.


This article answers the question posed by Nicole Porter via email: “What is the veteran effect? Is it true?”

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Rising Cancer Rates in Young People: Exploring the Unknown Causes

Colorectal Cancer Awareness

Colorectal cancer is on the rise, particularly among younger individuals.

Getty Images North America Copyright: Paul Morigi/Getty Images for Fight Colorectal Cancer

Research into the rising incidence of cancer among young individuals has generated more questions than definitive answers. While one study indicates that increasing obesity rates may account for a fraction of this trend, it doesn’t provide a comprehensive explanation.

According to Montserrat Garcia-Crosas from the Institute of Cancer Research (ICR) in London, the main takeaway is that although Body Mass Index (BMI) serves as a significant indicator, much of the increase remains unexplained.

Numerous global studies have documented a rise in cancer cases among adults under 50. Notably, the incidence of colorectal cancer has surged by about 50% in countries including the United States, Australia, and Canada since the 1990s.

To investigate the reasons behind this trend, Garcia-Crosas and colleagues analyzed cancer data in the UK alongside population trends related to risk factors such as obesity. Their findings indicated that 11 types of cancer are rising among individuals aged 20 to 49, with breast and colorectal cancers being the most prevalent. Other malignancies include liver, kidney, and pancreatic cancers, exhibiting growth rates between 1% and 6% annually.

The researchers discovered that the incidence of nine out of these 11 cancers was also increasing in individuals over 50, suggesting some common underlying factors. However, ovarian cancer and colorectal cancer were exceptions to this pattern, as noted by Garcia-Crosas.


The team also explored behavioral factors linked to these 11 cancers as identified by the International Agency for Research on Cancer, which include alcohol consumption, smoking, physical inactivity, body mass index, and dietary habits related to fiber and processed meats. “These researchers provide the strongest evidence connecting these factors,” Garcia-Crosas stated.

Despite the stable or improving nature of these risk factors over time, BMI remains a consistent concern, particularly given the rising rates of obesity. However, the link between obesity and the increase in cancer among young people is only partially understood. For instance, only about 20% of the rise in colorectal cancer among young women can be attributed to increasing BMI, as per Garcia-Crosas.

According to team member Mark Gunter at Imperial College London, extensive research is currently ongoing to identify the causes of this troubling trend. Potential factors being examined include a higher consumption of ultra-processed foods, substances known as PFAS (forever chemicals), and antibiotics affecting the gut microbiome.

Your analysis suggests that the increase in cancer cases among youths likely stems from a combination of elements rather than a single cause, and they could not exclude the possibility that diagnostic practices may also be influencing these statistics.

This rise should also be considered in context, as highlighted by Amy Berrington at ICR. In the UK, only about 3,000 bowel cancer cases are reported annually among individuals aged 20 to 49. Consequently, a 3% increase signifies approximately 100 more cases each year. “These trends are relative, and the overall increase in cases remains modest,” Berrington elaborated.

The study did not include cervical cancer due to the significant decrease in cases among women who received the HPV vaccine during childhood.

Looking ahead, Berrington draws attention to data through 2023, expressing optimism as the upward trend seems to be stabilizing. Furthermore, if obesity is a contributing factor to the rise in cancer diagnoses, emerging GLP-1 weight loss medications, such as semaglutide, may offer a potential solution. “Should obesity rates decline due to the adoption of these medications, we could witness a reduction in some obesity-related cancers in the future,” Professor Gunter concluded.

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Source: www.newscientist.com

Exploring the Impact of Climate Change on Wildfires in Georgia and Florida: Hotter, Drier Conditions and Hurricane Aftermath

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Wildfires are currently raging across southern Georgia and northern Florida, exacerbated by intense heat, strong winds, severe drought, and dry vegetation left from previous hurricanes. These elements have created a perfect storm for wildfires in the region.

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This situation is exactly what climate scientists have been warning about for decades as our planet continues to warm.

“This is certainly abnormal, but aligns with our concerns regarding climate change,” explained Caitlin Trudeau, a climate scientist at Climate Central, a nonprofit scientific research organization. “These events highlight the dramatic changes occurring in our climate.”

The wildfires are consuming thousands of acres across both states. Notably, a wildfire in Atkinson, Georgia, has already destroyed approximately 90 homes since its ignition on Monday.

In response to these fires, multiple counties, including those in Georgia, have implemented burn bans, leading to Gov. Brian Kemp declaring a state of emergency on Wednesday across 91 counties.

The wildfires are primarily attributed to widespread drought conditions in the Southeast, exacerbated by remnants of previous hurricanes—circumstances tied to climate change.

Specifically, Hurricane Helen, which made landfall in Florida’s Big Bend area as a Category 4 storm in 2024, left behind scorched trees, branches, and other dry vegetation.

“It’s as if the hurricane stripped a significant number of trees and laid everything bare in that area,” Trudeau noted. “The remains were exposed to the sun, and wood with high oil content becomes extremely flammable when dry.”

This dry vegetation significantly amplifies wildfire risks, fostering their growth and increasing their destructiveness.

Researchers warn that catastrophic wildfires will become increasingly prevalent in a warming world. Studies indicate wildfires will not only occur more frequently but will also be more devastating due to climate change—a situation with serious environmental, economic, and health repercussions for communities nationwide and globally.

Trudeau emphasized that even in humid areas like the Southeast—traditionally not considered as wildfire-prone—the risks are evolving under climate change.

“This is the reality we’ve been anticipating with climate change,” she said. “Certain parts of the Southeast are extremely dry now. Although these regions have high humidity, climate change has intensified atmospheric thirst. As temperatures rise, the amount of water drawn from the landscape and extracted from plants and soils increases as well.”

For a wildfire to ignite, two key elements must be present: fire-prone weather, which includes dry conditions, lightning, and wind, and “fuel,” such as dead wood, dry leaves, and other flammable vegetation.

As temperatures rise due to climate change, the atmosphere can efficiently extract moisture from trees and soils. In the event of prolonged droughts, insufficient rainfall exacerbates the potential for destructive wildfires.

Currently, all of Florida is experiencing some level of drought, with much of the Panhandle region categorized as facing “extreme” or “exceptional” drought, according to the US Drought Monitor. Likewise, 71% of Georgia is experiencing “extreme” or “exceptional” drought, particularly in southern regions.

For Trudeau, the wildfires witnessed this week serve as a stark indication of climate change’s catastrophic effects on natural ecosystems, including increased fire activity in areas historically deemed humid.

“This is why we are facing such an extraordinary situation right now,” Trudeau concluded. “It’s truly a perfect storm.”

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Exploring QBox Theory: Insights Beyond the Quantum Realm for a Deeper Understanding of Reality

Plasma expression

Exploring the Deeper Layers of Reality Beyond Quantum Theory

Kappan/iStockphoto/Getty Images

Physicists are delving deeper into the realm of post-quantum theory, unveiling a reality that exists at a level even more perplexing than the already bewildering quantum theory.

In the 1920s, physicists developed vital theories that explained fundamental workings of the universe, yet they continuously encountered phenomena where these theories fell short. This spurred them to glimpse into a more profound layer of reality: the quantum realm. Today, physicists find themselves revisiting this experience. While quantum theory accurately describes many phenomena, it leaves significant gaps when it comes to large cosmic structures influenced by gravity. What kind of post-quantum reality will manifest through these gaps?

James Hefford from the National Research and Development Agency, along with Matt Wilson from the University of Paris-Saclay, has created a mathematical framework outlining a potential post-quantum world—perhaps the deepest layer of reality.

“Quantum theory does not encompass the entirety of the universe,” Hefford remarks. “A significant challenge in physics is developing a quantum gravity theory that reconciles quantum mechanics and gravity. This theory must surpass traditional quantum descriptions.”

Multiple propositions exist for developing a quantum gravity theory, but Wilson and Hefford found their inspiration in the interplay between quantum and classical physics. Everyday experiences shield us from peculiar quantum effects, attributed to a phenomenon known as decoherence, which eliminates the quantum characteristics of most objects. Decoherence brings forth our tangible, rational world from the quantum domain, where the paradoxical states of cats exist and particles can seemingly disappear through barriers. They propose that quantum theory could arise from post-quantum theory through a similar mechanism called “hyperdecoherence.”

This concept isn’t entirely new; a specific theorem established in 2018 suggests that creating a coherent hyperdecoherence process that accurately reproduces quantum theory is mathematically infeasible. However, Hefford and Wilson scrutinized the underlying assumptions of this theorem and devised an innovative approach. The outcome? They entered a remarkably unconventional post-quantum landscape defined by a theory called QBox.

A fascinating aspect of QBox is its redefined conception of causality. Traditionally, causality operates on a clear sequence (event A causes event B or vice versa), but QBox permits a blend of both where causation is ambiguous.

“This introduces causal uncertainty, a critical aspect when pursuing a quantum gravity theory,” notes Carlo Maria Scandoro from the University of Calgary, who was not a part of this project. This uncertainty arises because Einstein’s theory of general relativity enforces varying causal orders across different spacetime points.

This is evident in thought experiments where observers traveling in different spaceships witness the same events but disagree on the chronological order of occurrences.

The researchers also ensured that hyperdecoherence adequately transitions QBox back into quantum theory, stipulating that objects described roughly within the QBox don’t gain precise clarity after hyperdecoherence. Wilson describes this hyperdecoherence as a dimension accessible to entities within the QBox realm—those capable of interacting within its confines—yet obscured from us in the classical or quantum realms.

Currently, the researchers are still clarifying how to conceptualize these dimensions and the experiences of agents operating within them. Preliminary indications suggest that the inaccessible dimensions are temporal rather than spatial—hyperdecoherence selectively concealing past processes while leaving future interactions untouched.

“Previously, there had been speculative models supporting concepts like indeterminate causal order, but formulating comprehensive quantum mechanics proved challenging, with no successful conclusions,” states Ciaran Gilligan Lee, involved in Spotify’s Causal Inference Lab and a co-author of the 2018 theorem opposing hyperdecoherence. He points out that the true merit of this new research lies in its concrete theoretical foundation and its mathematical simplicity. Notably, QBox does not necessitate hypothesizing entirely new constructs like cosmic strings for quantum gravity.

Beyond demonstrating the feasibility of hyperdecoherence as a mathematical function, the subsequent step involves elucidating its physical implications, contends John Selby from the University of Gdańsk, another co-author of the 2018 theorem. “A narrative is essential to clarify why these phenomena arise in our empirical universe.” In his opinion, the mathematical exploration by Hefford and Wilson is a promising foundation, regardless of whether QBox accurately represents the post-quantum layer of reality.

Gilligan-Lee and Selby have also formulated a new theorem, not yet explored by contemporaneous physicists, which may impose stricter criteria on a theory like QBox for it to meaningfully differentiate from quantum theory.

This challenge is welcomed by Wilson, even if it means QBox evolves into a precursor for a more refined vision of post-quantum theory. Notably, this theory may have tangible implications for specific experiments involving overlapping quantum waves, potentially facilitating experimental validation of the QBox concept.

If QBox successfully navigates forthcoming mathematical and experimental hurdles, even more intriguing inquiries will arise. “Can entire frameworks of theory be similarly disentangled?” Hefford speculates. Ultimately, unearthing the deepest realities might necessitate further mathematical exploration.

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Source: www.newscientist.com

Why Identical Twins Aren’t Truly Identical: Exploring Genetic Differences

Identical twins are created when one fertilized egg divides into two embryos during the early stages of development. These embryos originate from the same set of cells, resulting in virtually identical DNA.

This genetic similarity means they share traits with a strong hereditary component, such as blood type and eye color. However, from that moment, their differences start to grow.

Even though twins share the same womb, their experiences can differ significantly. A minor twist in the umbilical cord, for instance, may lead to one twin receiving a greater share of nutrients than the other.









This nutrient disparity can lead to variations in gene expression patterns, influencing traits like growth, personality, and susceptibility to diseases.

Additionally, differences in intrauterine pressure and positioning can result in identical twins being born with distinct fingerprints. While genetic factors determine the basic fingerprint structure, the amniotic fluid environment shapes its unique characteristics.

After birth, more differences arise. Random genetic mutations can occur in either twin at any time, explaining why identical twins may develop different illnesses, including cancer.

Chance also affects their development; for instance, one twin may contract a virus leading to an autoimmune disease while the other remains unaffected.

Thus, both nature and nurture play crucial roles in their lives. As time passes, their environments will change, further differentiating them.

Even if identical twins grow up in the same household, they often have varied experiences—different teachers, friends, and role models. As adults, they may live in distinct locations, exposed to varying levels of social support, healthcare access, or environmental factors.

All these aspects interact with their DNA, amplifying their differences and ultimately shaping each twin into a unique individual. So, despite being termed identical twins, they are far from being the same.


This article addresses the question posed by Chris Montgomery via email: “How identical are identical twins?”

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Can We ‘Vaccinate’ Ourselves Against Stress? Exploring Effective Stress Management Techniques

Explore science news and long reads from expert journalists at New Scientist, covering technology, health, and the environment.

While it might sound unusual, you can actually inoculate yourself against stress.

Just as vaccines help the immune system fend off invaders, research suggests stress inoculation can prepare individuals for future stressors.

This concept is particularly noted among military personnel. By allowing soldiers to undergo simulated stressful situations and equipping them with coping mechanisms, they can reduce the impact of stress over time. For instance, a study found that cadets with resilience training showed lower cortisol levels following intense military drills compared to those without such training. Similarly, emergency personnel also experience lower risks of post-traumatic stress disorder (PTSD) and depression due to their resilience training strategies.

Fortunately, you don’t need military training to reap the benefits. Regular, manageable exposure to stress can enhance resilience, as observed by Julie Vashuk from Masaryk University, Czech Republic.

Recent studies indicate that navigating stressful experiences can actually reshape the brain. This includes changes in key areas like the prefrontal cortex, involved in emotion regulation, the hippocampus, crucial for memory, and the amygdala, responsible for threat perception. Facing mild stressors can help individuals adapt to challenges in the following ways: it enhances resilience and accelerates recovery to baseline.

It’s essential to keep stress levels manageable. As Vashuk advises, mild stress should induce just enough discomfort to be tolerated without becoming overwhelming. “Once you’re overwhelmed, it becomes traumatic,” she explains. Activities like visiting unfamiliar places or engaging with new people can be beneficial. She also recommends surrounding yourself with supportive individuals.

This exposure therapy can be useful for adults, but how about children? Numerous studies, like one that highlights that early childhood adversity can elevate health risks, suggest that a small amount of controlled adversity may actually be advantageous. In rodent studies, constant separation from their mothers increases adult stress responses, while brief separations can lead to stronger adult responses. A similar phenomenon has also been observed in primates concerning short-term mother-infant separation.

Extrapolating such studies to humans poses ethical challenges, yet researchers like Carmine Pariante from King’s College London argue that we may not be as resilient as a society as we think. This doesn’t imply inflicting trauma intentionally, but rather suggesting that facing manageable challenges can benefit both adults and children.

Simulated stress exposure helps soldiers build real-life resilience.

Daniel Ceng/Anadolu via Getty Images

Vashuk also highlights a cultural phenomenon in the Czech Republic, where children are introduced to classical music early on. “Five-year-olds perform with their teachers, gradually performing solo as they mature. Although the stress remains, their early exposure equips them to effectively handle stress and rebound quickly,” she notes.

Exposure isn’t the sole method for building resilience. Techniques such as breathing exercises, mindfulness, altering your mindset regarding stress, and recognizing your strengths are proven to boost resilience and transform negative stress into positive energy.

Research is ongoing into the concept of a literal stress vaccine. Studies on rodents indicate that exposure to a heat-killed bacterium, Mycobacterium vaccae, calms stress responses via anti-inflammatory effects. Additionally, experimental drugs like “Alexigent” aim to enhance stress tolerance in individuals predisposed to PTSD and depression, although significant advancements remain limited. A notable 2017 study showed that a single ketamine dose can mitigate stress impacts on mice.

For most of us, however, the solution lies in the simplicity of understanding that stress is not inherently detrimental (see “Why the right kind of stress is crucial for health and well-being”). “Stress is beneficial for growth,” Vashuk states. “Experiencing stress is vital for our responses. What’s equally important is the ability to recover swiftly. Building resilience is crucial for regulating stress hormones effectively.”

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Exploring the Existence of ‘Cosmic Fossils’: Black Holes from Before the Big Bang Still Present Today

New research by Professor Enrique Gaztanaga of the University of Portsmouth and the Institute of Space Sciences in Barcelona proposes a groundbreaking theory that some black holes might have formed before the Big Bang and survived a cosmic ‘bounce’. This intriguing idea could shed light on dark matter, the gravitational wave background, and the formative years of supermassive black holes and galaxies.



Gaztanaga proposes a new dark matter mechanism involving relic black holes stemming from a pre-big-bounce collapse.

“For almost a century, cosmologists have traced the universe’s history back to a singular event known as the Big Bang,” Professor Gaztanaga remarked.

“The conventional theory suggests that space and time originated from an extremely hot and dense state approximately 13.8 billion years ago, leading to billions of years of cosmic expansion and galaxy formation.”

“This prevailing model has been remarkably successful, accounting for the cosmic microwave background (CMB) radiation—an echo from the early universe—and accurately predicting the distribution of galaxies across the cosmos.”

“Nevertheless, several profound mysteries in physics remain unresolved. We still lack understanding about the Big Bang’s cause, the universe’s initial special conditions, the rapid expansion known as inflation, and the nature of dark matter, which outnumbers ordinary matter by a factor of five.”

“Our research investigates the possibility that the universe didn’t originate from a single shock but may have emerged from a cosmic bounce that mimicked inflation, with some of the universe’s oldest objects potentially surviving as relics from an earlier epoch.”

Some black holes may have emerged during the universe’s early stages and survived this cosmic bounce, leaving behind relics that could still influence galaxy structures billions of years later.

Others may have formed immediately after density fluctuations were amplified, resulting in a more uneven distribution of matter during the early universe.

These concentrated clumps of matter collapse more readily under their own gravity, increasing the likelihood of forming large cosmic structures and black holes early on.

Within Einstein’s theory of general relativity, the Big Bang represents a singularity, a point where density becomes infinite and known physical laws cease to function.

Many physicists view this as indicative of an incomplete understanding of the universe’s earliest moments.

Another concept to consider is bounce cosmology. This theory posits that our universe originated from a colossal cloud that first contracted and then expanded.

Rather than collapsing into an infinite singularity, the universe reaches a very high but finite density before reversing its motion.

“Singularities often signal that a theoretical framework has hit its limitations,” Professor Gaztanaga asserts.

“Bounces offer an avenue for the universe to transition from contraction to expansion without necessitating new and exotic physics.”

Scientists posit that this bounce might emerge naturally from quantum physics. Under extreme densities, quantum effects generate powerful pressures that prevent matter from compressing infinitely. This phenomenon stabilizes dense objects like white dwarfs and neutron stars, potentially replicating the inflationary phase.

New models suggest that similar effects could manifest on a cosmic scale. As the universe contracts, this quantum pressure can halt the collapse and trigger a rebound into expansion.

This cosmic bounce could address two pressing mysteries in cosmology.

First, it could elucidate why the early universe expanded so rapidly and uniformly in all directions.

Second, it may help explain why the universe appears to be expanding at an accelerating rate today—an effect currently attributed to a poorly understood force referred to as dark energy.

A notable hypothesis is that certain structures formed during the collapse phase may have persisted after the bounce.

New calculations indicate that compact objects exceeding about 90 meters in size might traverse the transition and reemerge as remnants in the expanding universe.

Potential artifacts include gravitational waves, density fluctuations, and ancient black holes.

These relic black holes could serve to explain dark matter, the unseen material that shapes large-scale structures of galaxies and the universe.

If substantial numbers were created during the bounce, they could constitute a significant portion, or even all, of dark matter.

This notion may also provide insight into the recent observations by the NASA/ESA/CSA James Webb Space Telescope of an unexpectedly massive object, often referred to as a ‘tiny red dot,’ in the early universe.

Many astronomers speculate these sources are related to rapidly growing black holes that emerged shortly after the Big Bang.

“If a supermassive black hole existed right after the bounce, we wouldn’t have to start from square one when forming the initial galaxies in the early universe,” Gaztanaga explained.

This theory also presents predictions that could be tested through future observations.

Scientists may seek to detect relic gravitational waves from previous cosmic stages or subtle patterns in the CMB that preserve traces of a pre-Big Bang universe.

“Much research is still required to validate these concepts,” Professor Gaztanaga states.

“However, if the universe did experience a bounce, the dark structures that shape today’s galaxies might be remnants from an earlier cosmic age that preceded the Big Bang.”

This paper is published in Physical Review D.

_____

Enrique Gaztanaga. 2026. Cosmological Bounce Relics: Black Holes, Gravitational Waves, and Dark Matter. Physics. Rev.D 113, 043544; doi: 10.1103/pr4p-6m49

Source: www.sci.news

Exploring the Rise, Fall, and Recovery of Periodic Cosmology: A Comprehensive Analysis

The largest 3D map of the universe, with Earth at the center and every dot representing a galaxy

The Largest 3D Map of the Universe

Collaboration between DESI and KPNO/NOIRLab/NSF/AURA/R. Proctor

The universe is in a state of transformation. While not yet at its conclusion, one day all we know will fade away.

Everything we know—the cities, lakes, planets, solar systems, and the stars—are on a path to an ultimate finale.

What lies ahead? Some experts speculate that the universe’s expansion will eventually reverse, gathering everything tightly until it culminates in a big crunch, only to start anew in a big bounce. This idea, known as cyclic cosmology, has resurfaced, partly fueled by groundbreaking data from the Dark Energy Spectrograph (DESI)’s comprehensive 3D map of the universe.

Proponents of periodic cosmology often advocate for its aesthetic simplicity. If the universe follows this cycle, we may not need to grapple with what caused the Big Bang or what existed before it—these questions may have been resolved already. Scottish astronomer Katherine Heymans eloquently summarized during a recent lecture hosted by New Scientist: “The universe undergoes a big bang, expands, slows down, and gravity pulls it back, culminating in another big bang.”

Nobel Prize winner Adam Riess, who contributed significantly to the discovery of dark energy, highlights why many cosmologists favor this concept. He states, “This suggests we are not in a unique universe, implying that the periodic nature of the cosmos makes we, as existences, less coincidental.” However, this perspective may be seen as anthropocentric rather than purely physics-based.

For decades, periodic cosmology lost momentum, especially after Riess’s findings indicated that the universe is expanding at an accelerating rate. Should dark energy outweigh gravitational forces, the likelihood of the universe collapsing decreases. Heymans noted, “Current evidence points towards a desolate, cold demise for our universe,” referring to heat death, which is currently the prevalent theory concerning the universe’s fate.

This notion isn’t without challenges, particularly when exploring how energy, matter, and entropy behave between cosmic cycles.

The second law of thermodynamics complicates the scenario. It posits that disorder, or entropy, never declines in a closed system like the universe. While entropy rises overall as the universe expands, it would seemingly decrease if contraction occurs—an apparent contradiction lies therein. Although some theoretical work has aimed to circumvent this, the ultimate cycle still reverts to a Big Bang followed by heat death, albeit through a convoluted path.

Prominent theoretical physicist Roger Penrose introduced a model called conformal periodic cosmology to navigate these complexities. His theory posits that the universe remains seemingly ever-expanding until the end, where matter disintegrates entirely into photons. Here’s the novel aspect: the uniformity at the new cycle’s start mirrors the emptiness at the previous cycle’s conclusion, potentially allowing a new universe to emerge.

While intriguing, this paradigm remains hard to empirically test, though Penrose has suggested potential measurable evidence. However, skepticism persists in the cosmological community, yet its avoidance of the entropy quandary means it shouldn’t be disregarded outright.

Mayall 4-Meter Telescope at Kitt Peak National Observatory

DESI Collaboration/DOE/KPNO/NOIR

DESI’s expansive cosmic map indicates that dark energy—a previously unstoppable force—may be losing strength. This suggests that while the universe’s expansion continues, its acceleration might be slowing down. As Heymans pointed out, this doesn’t imply a cosmic contraction but marks a significant shift in our understanding of dark energy.

The possibility that dark energy can weaken over the next ten billion years could usher in a new phase for periodic cosmology. “The transformation of dark energy may pave the way for a universe that can reverse its expansion one day,” noted Heymans.

Understanding the universe’s fate hinges on comprehending dark energy, which constitutes nearly 70% of the universe’s matter and energy. The nature of dark energy remains elusive, complicating efforts to theorize regarding the universe’s long-term trajectory. As Reese contended, “Extrapolating into the future without knowing more about dark energy renders predictions difficult.” While the cold death of the universe may seem the most probable outcome, the prospect of a big bounce-back is more conceivable than it has been in decades.

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Source: www.newscientist.com

Exploring the Mysteries of the Cosmos: What’s Between the Stars? – Cyworthy

Space is abundant. If we shift our gaze from Earth and the Milky Way to intergalactic space, the average density is approximately

1 atom per cubic meter

, equivalent to 35 cubic feet of space. Yet, the universe is not entirely void; on smaller scales, it is rich with matter.

Within galaxies, there are various forms of matter existing between stars, undergoing different states of temperature and density, known as the

multiphase interstellar medium (ISM)

. This substance is primarily made up of hydrogen and helium, along with trace amounts of other heavier elements, often referred to by astronomers as

metals

. It is this interstellar material that plays a critical role in star formation.

A team of astronomers conducted research to understand how variations in metallic concentrations impact star-forming regions within the ISM. They simulated ISM clouds with different metallicities corresponding to seven distinct areas in the nearby universe, including regions


near the Sun


, a random patch of the Milky Way,

the Large and Small Magellanic Clouds

, the dwarf galaxy

Sextans A

, the globular cluster

NGC 1904

, and the blue compact dwarf galaxy

I Zwicky 18

. The simulation team uses the

SILCC

project, a collaborative effort of multiple European research institutions aimed at examining the life cycle of gas clouds that form stars.

Using advanced simulation software, the team modeled gas movements and their effects on magnetic fields within a massive cuboid measuring 500 parsecs by 500 parsecs by 4 kiloparsecs. Essentially, this translates to a box of 15 quintillion kilometers by 15 quintillion kilometers by 120 quintillion kilometers, or about 10 quintillion miles by 10 quintillion miles by 77 quintillion miles. This computational box comprised gas molecules held together by gravity from the cloud, nearby star clusters, older stars, and even

dark matter

. To prevent the cloud’s collapse during the simulation’s initial phase, the gas molecules were programmed to move at an average speed of 10 kilometers per second (about 22,000 miles per hour) for the first 20 million years, creating turbulence within the cloud.

The simulation examined the interactions of the cloud’s magnetic field and fluid dynamics while addressing how swiftly high-energy protons (known as

cosmic rays

) emerged within. Over a span of 200 million years, interactions with clouds led to star formation, the birth and death of stars, and changes in the molecular chemistry of the clouds. By considering various factors, the team analyzed the effects of metallicity across all seven simulations. The simulation corresponding to the solar neighborhood exhibited the highest metallicity, while that of I Zwicky 18 showed the lowest, with just 2% metallicity.

The findings indicated that ISM regions with low metallicity are generally warmer compared to their high-metallicity counterparts. The research demonstrated that metals efficiently release heat, unlike hydrogen or helium. While colder ISM phases foster star production and metal generation, warmer, low-metallicity regions tend to produce fewer stars, impeding cooling processes. This trend persisted until the material’s temperature reached roughly 1 million Kelvin (or 2 million °F).

In reviewing their results, the researchers acknowledged certain simplifications. Due to time limitations, many parameters in the simulation were not adjusted, focusing only on metallicity across different regions. They also underestimated the prevalence of common metals, such as carbon, oxygen, and silicon, which form at higher rates in stars. Lastly, they disregarded the potential for some massive stars to form black holes, assuming all such stars would culminate in supernova explosions.


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Is DNA Discoverable on Mars? Exploring the Possibility – Cyworthy

Since British pop icon David Bowie first posed the question in 1971,

“Does life exist on Mars?”

NASA has successfully landed five rovers on Mars. The

Curiosity
rover

landed in Gale Crater in 2012, unveiling rocks formed by a shallow lake approximately 3.6 billion years ago, hinting at a once habitable environment.
Curiosity
continues its mission, while in 2021, the

Perseverance
rover

was launched to explore Jezero Crater, where traces of past life may be found in sediments from a lake dating back 3.7 billion years.

Both
Curiosity
and
Perseverance
have uncovered evidence of

complex carbon-containing molecules

within Martian lake rocks. As all life on Earth is composed of similar organic molecules, astrobiologists speculate that these Martian compounds could lend credence to the existence of ancient life on Mars. However, it is crucial to note that organic molecules can also be formed through non-biological processes, implicating the need for further concrete evidence to definitively identify ancient Martian life.

Researchers at the Center for Astrobiology in Madrid, Spain, are investigating whether

DNA

can serve as a biomarker in Martian rocks. They argue that DNA is utilized by all life forms on Earth and is “the most critical biological molecule for life,” uniquely formed by living organisms. Additionally, factors that typically accelerate DNA degradation on Earth—such as water, heat, and microorganisms—are absent in Mars’

cold, dry climate
.

The greatest challenge in locating ancient DNA on Mars stems from the planet’s surface, which is consistently bombarded by intense

cosmic

and

solar radiation

that can rapidly degrade DNA and other organic molecules. Past studies have shown that DNA is more likely to endure radiation damage when

protected within rock

, prompting researchers to test whether Mars-like rocks could shield DNA from radiation levels akin to those on the planet for about 100 million years.

Direct access to Martian lake rocks is anticipated through future sample return missions such as NASA/ESA’s

Mars Sample Return

or China’s

Tianwen-3

mission. Researchers collected rocks from various geological ages formed in lakes and shallow marine environments globally. They specifically targeted rocks containing remnants of an ancient microbial community known as

microorganisms
and exhibited

total organic carbon concentrations

comparable to those identified in Martian geological samples, including lake microbial rocks from Mexico aged 2,800 years, shallow-water microbial rocks from Morocco aged 541 million years, and iron-rich rocks from Ontario, Canada, aged 2.93 billion years, with characteristics similar to those in Jezero Crater on Mars.

The team crushed the rocks, dividing them into six samples sealed in glass containers. They exposed three samples from each set to radiation levels reflective of 136 million years on the Martian surface, retaining the remaining three for comparison. The DNA was extracted from each sample and analyzed using
nanopore sequencing
, a method that effectively identifies short DNA fragments while assigning a quality score based on the reliability of the sequences.

The analysis indicated that unirradiated samples, presenting higher organic carbon content, also contained a greater abundance of DNA fragments. The findings suggest that the DNA originates from modern microbial communities that recently inhabited the rocks, while the organic carbon represents remnants from ancient microbes. Enhanced availability of nutrients correlates with increased microbial growth, solidifying the view that organic-rich sites such as ancient crater lakes are prime candidates for life-detection missions.

In the irradiated samples, DNA quality diminished and became fragmented from radiation exposure. For instance, the irradiated samples of Mexican lake microorganisms exhibited average quality scores 53% lower and DNA reads 85% shorter than unirradiated samples. However, the research team successfully identified which microorganisms contributed an estimated 2% to 9% of the DNA in these irradiated samples.

The researchers concluded that identifiable DNA fragments could potentially persist in Martian rocks for over 100 million years. They advocate for the application of this sensitive sequencing technology in forthcoming Mars rovers to search for evidence of past life and evaluate the planet’s biological safety. While the results are promising for astrobiologists, some caveats remain. Martian rocks may harbor
toxic salts
that could harm DNA integrity. Furthermore, scientists voice concerns regarding
pollution
from terrestrial life. The research team recommends that future investigations develop stringent protocols for eliminating salts from Martian rock samples and assessing possible external contamination.


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Exploring Dark Matter: The Enigmatic Light Surrounding Our Galaxy – Sciworthy

Astrophysics has long pursued the enigmatic concept of dark matter. This investigation was notably advanced by Vera Rubin in the 1970s when it became apparent that the outer regions of galaxies rotate more rapidly than visibility would suggest. Researchers categorized this occurrence under the umbrella of dark matter. Observations such as how light bends around galaxy clusters and the distribution of matter across the universe, alongside fluctuations in the cosmic microwave background radiation, all indicate that a substantial portion of the universe remains unseen.

Current cosmological models, particularly the ΛCDM framework, suggest that dark matter consists of slow-moving particles possessing mass and gravitational influence but negligible electromagnetic interaction. This makes dark matter virtually invisible and capable of traversing through ordinary matter.

The ongoing search for dark matter particles aims to elucidate their properties and distribution within the Milky Way galaxy. While scientists can calculate the motion of stars from the galactic center to the sun without acknowledging dark matter, the dynamics shift beyond this range. A dark matter halo envelops the galaxy, extending approximately 230,000 parsecs or 4 quintillion miles (7 quintillion kilometers) from the center, and is believed to constitute about 95% of the galaxy’s total mass.

A research team from University College London explored the geometry of the Milky Way’s dark matter halo. They assumed the galaxy was in equilibrium and examined stable star positions at the galaxy’s outskirts to model the shape and orientation of the dark matter halo necessary for these arrangements. By aligning this model with historical data on the Milky Way’s development, they gained deeper insights into the galaxy’s structure.

Utilizing the Gaia survey—a satellite mission mapping millions of stars in the Milky Way from 2013 to 2025—the team analyzed the average number of stars in the galaxy’s older outer regions, referred to as the stellar halo. They also assessed the position and velocity of stars within it, discovering that the stellar halo is elliptical and tilted relative to the Milky Way due to a similarly shaped but significantly larger dark matter halo.

A simplified diagram illustrating the shape and orientation of the dark matter halo compared to the stellar halo and the Milky Way’s disk. Not to scale. By the author.

The research team concluded that their findings challenge previous models suggesting the dark matter halo is almost spherical. They determined that the halo’s tilt relative to the Milky Way’s disk is approximately 43°. This tilt is comparable to that of other disk galaxies with dark matter halos, which average about 46.5° and exhibit a 18° greater inclination than stellar halos. They posited that a stable, tilted, non-spherical dark matter halo implies overall galaxy stability, especially given its collision with another galaxy at least 8 billion years ago. Enhanced measurements of the halo’s shape could yield further insights into this merger.

For future research endeavors, the team developed a model representing a snapshot of a galaxy with a tilted, rectangular dark matter halo, integrating the density and motion of stars. Their simulations exhibit additional nuances consistent with observations from the Gaia survey, indicating that the halo becomes increasingly tilted—with angles ranging from 10 degrees near the center to 35 degrees at distances of 6 to 60 kiloparsecs (100 to 100 quintillion miles, or 200 to 2 quintillion kilometers)—and transitions from elliptical to more circular shapes as the distance from the center increases. The team suggests that subsequent research could build on this model and explore more intricate features, such as interactions between the Milky Way and neighboring galaxies including the Large Magellanic Cloud.

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Exploring the Unexpected Crowds of Ancient Tidal Flats: A Hidden Gem Revealed

Exciting new fossil discoveries in a 500-million-year-old Cambrian mudflat in Wisconsin have revealed the earliest evidence of animals venturing onto land, along with insights into their diet. Learn more about Blackberry Hill.

The fossilized remains from Blackberry Hill have revealed that the creatures—a relative of millipedes known as the Eutycarcinoid—created tracks referred to as Protichnites, which means “first footprint.”

Paleontologists have been puzzled over the identity of these creatures for over 150 years.

In these ancient tidal flats, fossilized crustaceans known as Philocariidae have also been identified, alongside thousands of well-preserved trace fossils from various organisms, including arthropods and mollusks.

One of the new trace fossils, Climactichnites blackberriensis, represents a significant imprint likely made by an unidentified mollusk.

These animals traversed the tidal flats, leaving behind a series of footprints. Remarkably, it appears that they stopped to feed on jellyfish that washed ashore.



Cochlichnus? – Traces of polychaete worms believed to be resting.

Fragments of material (crusts) and coccoids are found in the vicinity, potentially indicating some of the earliest fossil evidence of animals feeding on jellyfish in the Cambrian tidal flats.

This may have prompted certain species to explore land, marking the beginning of terrestrial life.

Additional trace fossils feature notable markings, including those from polychaetes, with traces of their parapodia (limbs) documented alongside early occurrences of Stiaria pillosa, believed to be feeding traces of a true carcinoid arthropod.



Stiallia – Presumed feeding traces from ancient arthropods.

Researchers Kenneth C. Gass (Milwaukee Public Museum) and Nora Noffke from Old Dominion University recently released their findings in a paper in the Paleontology Journal. Read the full study here.

The authors also suggested that some of these traces may have been created by certain species of extinct primitive arthropods, such as Aglaspidids, known for their spike-like bifurcated tails.

“These discoveries indicate the Cambrian tidal flats were more active than previously thought. It seems as if all these animals flocked to the flats for a brief reprieve on land,” Gass noted.

“More extensive taxonomic diversity in these tidal flats necessitates further field surveys and material investigations.”

_____

K. Gass and N. Noffke. 2026. New findings from the Cambrian Moose Mound Complex tidal flat facies, Wisconsin, USA. Paleontology Journal, pp. 1-15; doi: 10.1017/jpa.2026.10225

Source: www.sci.news

Exploring the Perilous Depths of the Chernobyl Reactor: A Man’s Daring Dive

New scientist: Science news and long reads by expert journalists covering advancements in technology, health, and the environment.

Anatoly Doroshenko is entering Chernobyl’s reactor No. 4 for essential radiation measurements.

Credit: Mykhailo Palinchak

The ruins of Chernobyl’s Reactor No. 4 are among the most hazardous locations on Earth. This site is not only treacherous but also heavily irradiated, enveloped in darkness, and encapsulated in a dilapidated concrete sarcophagus, which is being fortified with a new containment structure.

Scientists urgently need insights into the internal environment. One such scientist is Anatoly Doroshenko, a young researcher at the Institute for Safety Problems in Nuclear Power Plants (ISPNPP). His occupation is considered one of the world’s most perilous, requiring him to venture deep into the nuclear reactor remnants to gather readings and samples, often from as close as 8 meters from the core.

“I’m not scared,” Doroshenko stated, standing beside a model of Chernobyl within the ISPNPP lab located in the nuclear power plant’s exclusion zone. “Preparation has equipped me for this task, and embracing this moral responsibility is essential.”

“It’s a peculiar sensation, akin to summiting Mount Everest or exploring the ocean depths,” he adds, noting the continuous adrenaline rush he experiences.

Doroshenko is tasked with numerous responsibilities during each reactor investigation, but must maneuver between urgency and precision due to time constraints. “Understanding your environment is vital; self-control is crucial,” he emphasizes, repeating the last part earnestly.

“You must be aware that every surface is contaminated—knowing what you touch is essential to avoid personal contamination,” he explains. “It’s imperative to strategize since the time you can safely remain inside is limited. The desire to gain knowledge must be balanced with awareness of your surroundings.”

In low-risk areas of the reactor, Doroshenko dons a hat, protective gloves, and a respirator. In high-risk regions, he must wear a full-body suit, potentially layered with a polyethylene suit for dust protection. He also carries a lead apron, but its bulk can hinder movement in confined spaces.

As a young researcher, he has explored significant areas such as the main circulation pump, vital for cooling Reactor No. 4 and implicated in the safety tests leading to the 1986 disaster. “Visiting this pivotal site is crucial as we examine the destruction caused by the explosion,” he notes.

1991: Inspecting the interior of the sarcophagus containing Reactor No. 4 at Chernobyl

Credit: Images Group/Shutterstock

“Knowledge is our best protection,” asserts researcher Olena Paleniuk at ISPNPP. “Anatoly plays a crucial role here. Though we all often appear fatigued and somber, he excels in his responsibilities, and we lack a sufficient number of young experts skilled in dosimetry.”

Doroshenko’s supervisor, Victor Krasnov, noted that generations of scientists have ventured into the reactor post-1986 to collect measurements and install sensors. They navigate confined spaces filled with radioactive water and remnants of corium, a hazardous mix of molten fuel, concrete, and metal created during the disaster’s extreme heat.

“The initial explorers named various structures within informally—terms like elephant’s foot, cat house, and octopus beam,” recounts Krasnov. “Each route inside presents unique challenges due to utter devastation.”

Numerous risks abound, including the 2,200-ton upper bioshield, affectionately termed ‘Elena,’ dislodged during the explosion and now precariously tilted. Its potential collapse could unleash hazardous debris and a substantial cloud of radioactive dust.

1986 image of the ‘elephant’s foot’ within Chernobyl’s No. 4 reactor, a mass of molten fuel.

Credit: Photo 12/Alamy

Regular monitoring is crucial due to occasional surges in nuclear activity. The exact locations of all fuel material within the reactor remain uncertain, leading to periods of reactor activation.

As uranium or plutonium decays, it releases neutrons, which can trigger further fission reactions when absorbed by other unstable nuclei. High water levels can slow these neutrons and inhibit further reactions, a factor crucial to reactor safety management. Following the disaster, the sarcophagus created arid conditions, causing a peak in neutrons, while breaches allowed moisture and humidity to enter, diminishing neutron flux.

Undergoing the establishment of newer safety protocols, the low humidity currently decreases the likelihood of accidents, emphasizing the need for ongoing analysis by Doroshenko and his team to preemptively address any emerging issues.

Although stringent safety measures are enforced, it remains inherently perilous to traverse inside an exploded reactor. “We acknowledge the risks,” Doroshenko states. “My health concerns me, as neglect might lead to mistakes. While the long-term effects on my health remain unclear, adhering to radiation safety protocols allows me to mitigate those risks.”

Topics:

Source: www.newscientist.com

Exploring the Impact of Birth Order on Autism, Migraines, and More

Impact of Sibling Birth Order on Health

Exploring the Impact of Birth Order on Health Outcomes

iStockPhoto

A recent study involving over 10 million siblings reveals that birth order may significantly influence the risk of developing more than 150 health conditions, ranging from autism and anxiety to hay fever.

Birth order has intrigued researchers for over a century, igniting debates about its correlation with personality traits and IQ. However, many prior studies faced criticism for lacking robustness in data collection and analysis.

A groundbreaking study conducted by Julia Rohrer in 2015 examined data from 20,000 children, determining that birth order had minimal impact on personality, resulting in only a slight decrease in IQ — about 1 to 2.5 points for the youngest siblings.

The recent analysis took a comprehensive approach, evaluating the likelihood of various health outcomes. Researchers like Benjamin Kramer at the University of Chicago meticulously compared 1.6 million sibling pairs, accounting for gender, birth year, parental age, and age difference, thereby mitigating potential confounding factors that may arise from parental treatment differences.

Out of 418 medical conditions studied, 150 were associated with birth order, with 79 more prevalent among firstborns and 71 among second-borns.


Notably, firstborns displayed heightened risks for several neurodevelopmental disorders, including autism and Tourette syndrome, along with an increased tendency for anxiety, allergies, and acne. Conversely, second-borns exhibited greater susceptibility to conditions such as drug abuse, shingles, and migraines.

“This study provides a rigorous examination of the topic,” states Lawler, urging caution as the relationships observed are modest. For instance, firstborns have a 3.6% elevated risk of depression, emphasizing that individual life trajectories may differ significantly across birth order.

The research team explored several potential explanations for these findings. For example, the increased incidence of allergies among firstborns may align with the “friendly enemy” hypothesis, suggesting that younger siblings encounter more microorganisms from their older counterparts, fostering immune tolerance. Indeed, wider age gaps were linked to lesser allergy occurrences in firstborns.

A parallel trend was noted for substance abuse, with risk diminishing for second-borns as age differences increased. The authors connected this to enhanced risk-taking tendencies often observed in later-born children. However, Lawler emphasizes that much of this evidence remains contentious and may imply that later-borns often pursue environments that heighten exposure to substance-use opportunities.

Furthermore, the substantial prevalence of autism among firstborns might stem from both biological and environmental factors. The mother’s immune response in the first trimester is hypothesized to potentially impact the developing brain. Research indicates that families with one autistic child may choose not to have additional children, suggesting possible biases in families who do have a second child following an autism diagnosis in the first.

Another perspective from Lawler pertains to “diagnostic substitution.” Diagnoses of ADHD and autism often rely on cognitive assessments, where slight IQ variations may lead to different labels. Firstborns, possessing marginally higher IQs, might be diagnosed with autism, while their younger siblings may receive an ADHD diagnosis despite sharing similar symptoms.

As noted by Ray Blanchard from the University of Toronto, results may vary when considering sibling gender and birth order dynamics. His research suggests older brothers might increase the likelihood of later-born boys identifying as homosexual, potentially due to maternal antibodies affecting subsequent pregnancies. “These distinctions are pivotal in understanding birth order effects on sexual orientation,” concludes Blanchard, advocating for further studies that incorporate sibling gender hierarchies.

Source: www.newscientist.com

New Scientist Recommends Exploring Sampling Experiences at London’s Edible Earth Museum

Try Samples at the Museum of Edible Earth

Photo Credit: David Parry/PA Media Assignments

Geophagy and Mental Health: Earth eating, or geophagy, is recognized by the American Psychiatric Association as a mental health condition unless tied to cultural practices.

Discover more about this fascinating topic at the Museum of Edible Earth in Somerset House, London, running until April 26th.

During my visit, I encountered approximately 600 soil samples collected by the museum’s founder, Mashal. Highlighted were red ocher from South Africa, a source of iron, and black nakumat clay used by pregnant women in India for nausea relief. In the UK, only two varieties are approved for tasting as nutritional supplements.

Luvos Healing Earth, known for digestive benefits, resembles chocolate sprinkles but tastes like unwashed leek sand. In contrast, I enjoyed the milled Mexican diatomaceous earth, a silky, slightly sour flour. Beyond taste, I reveled in imagining the ancient aquatic creatures that once inhabited this soil.

Thomas Luton
Features Editor, London

Topics:

Source: www.newscientist.com

The Ultimate Science Book: Exploring the Frustrations of Watson’s The Double Helix

James Watson’s The Double Helix: A Look at Its Enduring Legacy

There’s a compelling case to be made for The Double Helix, a celebrated science memoir by James Watson, as one of the greatest science books ever written. However, I hesitate to recommend it due to its troubling content, particularly given Watson’s controversial reputation.

According to Nathaniel Comfort from Johns Hopkins University, Watson’s narrative doesn’t just recount scientific progress; it portrays science as a vivid adventure shaped by individual personalities. This compelling storytelling has inspired countless readers to pursue careers in science.

The Double Helix details Watson’s collaboration with Francis Crick on deciphering DNA’s structure between 1951 and 1953, integrating data from Rosalind Franklin and Maurice Wilkins. Yet, Watson’s narrative often distorts the true nature of this collaboration, portraying himself as the primary talent.

Critically, Watson’s account has been scrutinized by scholars. Matthew Cobb, a biologist and science historian, asserts that the book blends fact and fiction misleadingly. Comfort echoes this sentiment, emphasizing that Watson’s work lacks precise boundaries between memoir and novel.

Watson’s villainization of Rosalind Franklin, for instance, reflects a narrative tactic borrowed from Truman Capote’s groundbreaking 1966 work In Cold Blood, which redefined the true crime genre. Cobb argues that Wilkins was the real antagonist, overshadowed by Watson’s portrayal.

When The Double Helix was released in 1968, Watson’s derogatory comments about Franklin mirrored the prevailing attitudes of that era. Patricia Fara, a historian from the University of Cambridge, recounts how these perspectives were accepted as commonplace within scientific circles at the time.

Today’s audience, however, is rightly disturbed by these views, along with Watson’s general rudeness towards others, which often comes across as immature and unkind.

Comfort posits that Watson’s memoir has been mischaracterized; he suggests it’s comedic in essence, from the opening line to its conclusion. Yet, some scenes, particularly those depicting conflicts with Franklin, might not resonate with modern sensibilities.

Despite Watson’s unfavorable self-portrayal, portraying himself as lazy and vain, Comfort insists that this structural unreliability adds complexity to the narrative. Their investigations reveal that the relationships between Crick, Watson, and Franklin were more joined than Watson suggests.

Regardless of its many flaws, The Double Helix has proven captivating and engaging, achieving the remarkable feat of becoming a bestseller with over a million copies sold.

Cobb acknowledges its significant impact on science and literature, yet queries whether it should truly be classified among the great science books, given its ethical violations and misrepresentations of scientific endeavor.

So, is it worth your time today? Cobb recommends reading it, but suggests viewing it more as a novel. However, be prepared for unlikable characters, as they hardly embody the best of human nature.

Topics:

Source: www.newscientist.com

Why Your Sense of Taste Changes After 50: Exploring the Science Behind Food Flavor Loss

Many people believe that food becomes less enjoyable as we age. While age plays a role, various other factors contribute to this phenomenon.

We are born with around 9,000 taste buds located on the papillae of the tongue. These taste buds regenerate every few weeks.

However, this regeneration slows down as we age. After around age 50, there is often an overall decline in taste buds, and existing ones may become less sensitive.




Not everyone experiences this decline uniformly, but some may find that food loses its appeal as they age. Still, it’s not solely about age.

Factors such as genetics, dental issues, medications, chronic health conditions, smoking, and nasal problems can also affect our sense of taste.

Moreover, our sense of smell significantly impacts how we perceive flavor. As we age, the number of olfactory receptor cells and the function of nasal mucous membranes decline, dulling our taste perception.

Temporary loss of smell, such as during a cold, can create similar effects, rendering food significantly bland.

As our sense of taste weakens, food preferences often shift. Salty and sweet flavors become more pronounced, leading many to favor these tastes as they age.

However, caution is essential; increased salt intake can affect blood pressure, while consuming sweets can lead to weight gain.

Intense flavors like sour citrus can awaken even the dullest of palates – Credit: Getty

So, can we prevent our sense of taste from dulling? While we can’t halt the aging process, certain habits may enhance our taste perception.

For instance, staying well-hydrated helps maintain saliva production; avoiding smoking (which harms taste buds), managing chronic conditions such as diabetes, and reviewing medications that cause dry mouth can all help.

Incorporating sharp flavors can also invigorate our taste experience. Foods like citrus fruits, sorbets, and mint often strike a stronger chord with our taste buds.

Marinating foods with vinegar, dressings, mustard, herbs, and spices can significantly enhance flavor and is often a better approach than merely increasing salt and sugar.

While it’s common for some individuals to experience a decline in taste as they age, with mindful habits and a touch of culinary adventure, many can continue to savor vibrant flavors well into their later years.


This article addresses the question posed by Kian Wilkinson from Lancaster: “Can we prevent our sense of taste from becoming dull as we age?”

If you have any questions, feel free to email us at: questions@sciencefocus.com or reach out via Facebook, Twitter, or Instagram (please include your name and location).

Explore our ultimate fun facts and discover more amazing scientific content.


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Exploring Dark Matter: The Enigmatic Glow Surrounding Our Galaxy – Sciworthy

A prominent area of research in modern astrophysics is the enigmatic dark matter phenomenon. The groundbreaking work of Vera Rubin in the 1970s revealed that the outer edges of galaxies rotate at unexpected speeds, contrary to predictions based solely on visible matter. This led researchers to investigate and classify these observations under the term dark matter. Numerous studies have documented how light bends around galaxy clusters and the distribution of matter in the universe, as well as fluctuations in cosmic microwave background radiation, all indicating that the universe holds more secrets than what astronomers can visibly observe.

According to widely accepted cosmological models, the ΛCDM model describes dark matter as a type of slow-moving particle that possesses mass and exerts gravitational force but does not interact with electromagnetic radiation. As a result, dark matter remains invisible and can seamlessly pass through ordinary matter.

The quest to identify dark matter particles is an ongoing effort, allowing scientists to investigate their characteristics, including their distribution throughout the Milky Way. Although scientists can calculate the movement of stars from the galaxy’s center to the Sun without factoring in dark matter, the presence of this invisible mass significantly influences stars and gas clouds found further out. Researchers suggest that the dark matter halo encircles the galaxy, extending up to 230,000 parsecs (approximately 4 quintillion miles or 7 quintillion kilometers) from the galactic center, and may account for roughly 95% of the Milky Way’s total mass.

A research team from University College London has been examining the geometry of the Milky Way’s dark matter halo. They hypothesized that the Milky Way is in a state of equilibrium and analyzed the stable positions of stars in the galaxy’s outer regions to model the shape and orientation of the dark matter halo that permits their presence. Their findings were then correlated with previous studies of the Milky Way’s evolution, providing a more comprehensive understanding of the galaxy’s structure.

This research leveraged data from the Gaia survey, a satellite mission that observed millions of stars and mapped the Milky Way galaxy from 2013 to 2025. The team utilized two primary types of data: the average number of stars within specific volumes in the outer regions of the galaxy’s old structures and the stars’ positions and velocities within the stellar halo. The team discovered that the stellar halo is elliptical and tilted concerning the Milky Way, primarily due to a similarly-shaped but significantly larger dark matter halo.

A simplified diagram illustrating the shape and orientation of the dark matter halo compared to the stellar halo and the Milky Way’s disk. Not to scale. By the author.

The research team concluded that their findings dismiss the earlier notion that the dark matter halo is approximately spherical. They determined that the halo’s tilt, relative to the Milky Way’s disk, is around 43 degrees. This tilt mirrors other disk galaxies with dark matter halos, which typically range between 46.5° and 18° with regards to their stellar halos. The researchers contended that a stable, tilted, non-spherical dark matter halo signifies the overall stability of the galaxy, especially in light of past galactic collisions that occurred at least 8 billion years ago. Enhanced measurements of the halo’s shape could provide valuable insight into these markedly significant merge events.

To facilitate future research, the team generated a model that accurately reflects a snapshot of a galaxy with a tilted, rectangular dark matter halo. This model incorporates the stars’ density and motion patterns that they examined. Additional refinements in their simulations are consistent with findings from the Gaia survey, revealing that the halo becomes increasingly tilted moving away from the galactic center. Specifically, the tilt escalates from 10 degrees to 35 degrees at distances between 6 and 60 kiloparsecs (approximately 100 to 100 quintillion miles or 200 to 2 quintillion kilometers), while also transitioning from being elliptical to more circular as the distance increases. They propose that future researchers explore this model further, incorporating other complex interactions, such as those with the Large Magellanic Cloud.


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Exploring the Sun’s Chaotic Magnetic Core: New Insights Revealed

Recent analysis of NASA’s Parker Solar Probe data reveals that protons and heavy ions react differently during solar magnetic reconnection events, highlighting the complexity of space weather mechanisms.

NASA’s Parker Solar Probe approaches the Sun. Image credit: NASA’s Scientific Visualization Studio.

Magnetic reconnection transforms magnetic energy into explosive kinetic energy, fueling various solar phenomena that significantly impact space weather affecting Earth.

This process energizes protons and heavy ions, propelling them from the Sun at extraordinary speeds.

While current models assume uniform particle behavior, new insights from the Parker Solar Probe indicate significant differences in particle acceleration.

Heavy ions are projected straight, resembling a laser beam, whereas protons generate waves that scatter trailing particles in a dispersive pattern—much like the effect of a flashlight.

“These new findings redefine our understanding of magnetic reconnection,” stated Dr. Mihir Desai, a researcher at the Southwest Research Institute and the University of Texas at San Antonio.

“Protons and heavy ions show distinct spectral behaviors that challenge existing models.”

“Protons create scattered waves more efficiently, while heavy ions maintain a focused beam and preserve their accelerated spectral shape.”

“Magnetic reconnection is a common phenomenon throughout the universe, where magnetic field lines converge, separate, and rejoin.”

“Within the Sun, explosive processes energize particles, generating high-velocity streams that lead to space weather phenomena like solar flares and coronal mass ejections.”

“Such space weather can disrupt Earth’s space environment, resulting in breathtaking auroras but also affecting power grids, satellite communications, and navigation systems.”

“Understanding the mechanics of magnetic reconnection is crucial for predicting hazardous events and safeguarding both life and technological assets on Earth and in space.”

“Our findings reveal that the Sun’s ‘magnetic engine’ is far more intricate than previously thought,” Dr. Desai added.

“This is thrilling as it shows that our own star acts as an accessible laboratory for high-energy physics, similar to the processes that drive some of the universe’s most intense phenomena, like black holes and supernovae.”

For more details, refer to the study results, published on March 31st in the Astrophysics Journal Letter.

_____

MI Desai et al. 2026. Acceleration of protons and heavy ions by magnetic reconnection in the near-solar heliospheric current sheet. APJ 1000, 300; doi: 10.3847/1538-4357/ae48f2

Source: www.sci.news

Why Are Oceans Becoming Darker? Exploring the Global Changes in Ocean Color

Estuaries along the coast of Guinea-Bissau branch out like a network of plant roots, with the river transporting water, nutrients, and sediment toward the Atlantic Ocean. This Landsat 8 image captured on May 17, 2018, showcases the movement of sediment, particularly visible on the Rio Geva near Bissau.

At dusk, a massive transfer of biomass occurs in the oceans, as trillions of tiny creatures like zooplankton, krill, and lanternfish rise from the depths, drawn by phytoplankton blooms. This nocturnal feeding frenzy is crucial for marine ecosystems, as these creatures avoid predators who hunt visually, diving back down at dawn.

Solar and lunar cycles dictate marine behavior, yet recent observations show that large areas of the ocean have darkened. Tim Smith, a marine scientist at the Plymouth Marine Research Institute, has been at the forefront of this research, studying the impact of global warming and land-use changes on ocean light dynamics.

Smith told New Scientist about the causes and implications of ocean darkening, exploring ways to enhance light penetration into underwater habitats.

Thomas Luton: How did you first notice the darkening of the ocean?

Tim Smith: We approached this issue from a unique perspective. For the last decade, I’ve collaborated with Tom Davis, focusing on the effects of artificial light pollution. Analyzing two decades of global satellite data revealed a consistent darkening pattern in the ocean, suggesting an increase in surface water opacity which affects well-connected expansive regions rather than isolated patches. About one-fifth of the world’s oceans have experienced some form of darkening.

What causes ocean darkening?

In coastal areas, river changes significantly impact ocean coloration. Alterations in land use directly influence what enters rivers, thereby transforming the optical properties of ocean water. Flood events can greatly increase the influx of suspended particulates and colored dissolved organic matter, contributing to the characteristic “steeped tea” color.

An additional driver of ocean darkening is nutrient loading, where fertilizers from agricultural runoff stimulate phytoplankton growth, reducing light penetration. Although coastal waters have been recognized as darkening for some time, the phenomenon is now extending into the open ocean.

Tim Smith studies the impact of land-use change and global warming on ocean dynamics.

Krave Getsi

What factors lead to changes in the open ocean?

These changes may correlate with the abundance of phytoplankton driven by climate change, such as rising ocean temperatures and increasing frequency of marine heatwaves. Climate alterations influence vast ocean circulation patterns significantly.

The proliferation of phytoplankton relies on a mix of light, nutrients, temperature, and water column dynamics. In winter, storms typically mix the ocean, but as spring arrives, a stable surface layer forms. These layers limit vertical mixing and enhance light and nutrient concentration, fostering phytoplankton growth.

I suspect that we’re witnessing a complex interplay between shifts in global circulation patterns and localized weather phenomena, such as clearer skies that promote phytoplankton growth. This combination may contribute to the widespread darkening of the open ocean.

What impacts does ocean darkening have on marine ecosystems?

To understand this better, consider the ocean’s food chain. Phytoplankton, the primary producers, experience the first effects of darkening. The next tier includes zooplankton, like Calanus copepods, which serve as a critical link in the food web and engage in diurnal vertical migration, moving up and down daily for feeding.

Zooplankton are a key component in the food web adversely affected by ocean darkening.

Flor Lee/Getty Images

During the day, they dive to depths of 200 to 300 meters where light is scarce, eluding visual predators. By night, they ascend in search of food. This behavior represents the largest biomass transfer on Earth, as millions of zooplankton migrate invisibly through the water, significantly outnumbering the terrestrial migrations like the Serengeti wildebeest.

What occurs when light cannot penetrate deep underwater?

The existence of dark regions in the ocean restricts the vertical habitat for species, which could lead to heightened competition for food and space. Some species may expend less energy hunting, impacting predation dynamics and thus altering food webs and global fishery productivity.

Fish species that rely on sight, including both small schooling fish and large predators like tuna, will find their hunting zones confined to the shallows. Simultaneously, phytoplankton may face altered depths for photosynthesis due to decreasing light availability.

Is nighttime ocean darkness still a concern?

Absolutely. Beyond sunlight, moonlight plays a crucial role in nocturnal migrations of many marine creatures. While the ocean appears nearly black at night to humans, the moon’s dim glow has significant implications for guiding species during foraging and return to deeper waters.

Our lunar models indicate that as ocean clarity decreases, moonlight’s penetration diminishes, which may compress the nighttime habitat, dramatically shifting ecological interactions in darkness.

What is the global impact of these changes?

Ocean darkening could profoundly affect the carbon cycle as well. If zooplankton cannot dive as deeply to evade predators due to limited light, their efficiency in pulling carbon from the atmosphere diminishes. When zooplankton perish, they normally sink and trap carbon deep in the ocean; without the ability to dive, much of this carbon may remain in the upper layers, ready to be re-released into the atmosphere.

However, assessing how carbon moves from the illuminated surface to the ocean floor remains complex. Satellite data provides a global perspective, but it offers only a glimpse into dynamics at work.

Is there a way to combat ocean darkening?

In certain areas, yes. Coastal waters are especially vulnerable to terrestrial activities, particularly agricultural runoff. By managing land better, including practices such as reducing fertilizer usage, we could restore some clarity to coastal waters. Initiatives like the AgZero+ program led by the UK Center for Ecology and Hydrology encourage collaborative efforts with farmers to develop eco-friendly farming techniques, thereby minimizing runoff and enhancing water quality. Strategies like improved fertilizer management and agroforestry could substantially mitigate the darkening of coastal waters.

Nevertheless, addressing the drivers of darkening in the open ocean is far more challenging. Even if global emissions halt immediately, ecological responses would take decades, potentially centuries.

Is there hope for the seas?

Absolutely. Evidence shows that marine environments can exhibit remarkable resilience when given a chance. Protected marine ecosystems can recover swiftly. For instance, kelp forests off California rebounded rapidly in well-managed reserves after a severe marine heatwave between 2014 and 2016.

This resilience has led to a global push to expand marine protected areas, which can act as ecological refuge zones, helping to rebuild vital marine life and restore ecological equilibrium. Such measures are crucial in the face of climate stressors like heatwaves.

There is optimistic news: the ocean exhibits extraordinary self-repair capabilities. With adequate protection and time, marine ecosystems can respond swiftly, crucial for all life on Earth. The oceans, covering about 70% of the planet, play a significant role in climate regulation and carbon absorption, underscoring the need to protect this invaluable life-support system.

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Source: www.newscientist.com

Exploring the Quest for Immortality: Essential Questions to Consider Before Seeking Eternal Life

EAF952 End of road, dead end towards Salton Sea, with sign and barrier.

Despite their immense wealth, billionaires cannot evade the ultimate limit of mortality. No amount of money or the best medical care can change the inevitability of death. However, a groundbreaking startup named Nectome is poised to change the narrative around death and the human brain.

Nectome has pioneered a technology that preserves the brain’s physical structure within minutes post-mortem. Initially tested on pigs, the method aims to allow for the reconstruction of the ‘connectome’—a 3D map of the brain’s intricate structure—opening the door to potential revival.

It is essential to note that while the connectome can be mapped, how to recreate consciousness from it, if at all, remains a profound mystery. The complex nature of consciousness, coupled with its “hard problems,” continues to baffle scientists and researchers.

Beyond the scientific inquiries, significant ethical and legal questions arise. Can a brain be effectively digitized, or must it remain biological? Even if these hurdles are overcome, Nectome’s methodology necessitates medically-assisted death, a practice illegal in many regions. Nevertheless, those who opt for Nectome’s procedure may find solace in the hope that future advancements will lead to solutions, potentially allowing them to awaken centuries after their biological death.

A philosophical quandary remains: is a revived entity, emerging from a copy of a deceased brain, truly the same as its original owner? This question poses deep implications even as society contemplates the feasibility of Nectome’s treatments. Ultimately, anyone who undergoes this revolutionary process might be taking steps towards a form of immortality, presenting a profound challenge for us to consider in the realm of ethics and existence.

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Source: www.newscientist.com

Exploring Plant-Based Soil Remediation: Insights from Scientists – Sciworthy

Industrial activities, including mining, smelting, and electronics manufacturing, generate significant environmental waste that contaminates soil. These wastes often contain toxic metals detrimental to both flora and fauna..

Soil remediation can be a complex undertaking. Conventional methods, like landfilling contaminated soil, are costly and can degrade soil quality. To address these issues, researchers and farmers are exploring innovative plant-based solutions for soil cleanup, notably through a process called Phytoremediation, which involves the use of plants that absorb heavy metals. Enhancing these plants with growth-promoting microorganisms bolsters root development and nutrient accessibility, subsequently boosting plant vitality.

In addition to phytoremediation, farmers utilize treatments derived from burning organic matter in low-oxygen conditions, known as biochar. Biochar effectively binds heavy metals in the soil, reducing their toxicity to plants. However, there is limited research on the synergistic effects of combining microorganisms with biochar for soil remediation.

A research team from Portugal conducted experiments to determine if combining biochar with microorganisms could enhance phytoremediation effectiveness. They examined the effects of biochar augmented with two specific microorganisms: the bacteria Pseudomonas liatans EDP28 and the fungi Rhizoglomus irregulare, both recognized for their plant growth-promoting capabilities.

The objective was to assess whether soil treatments could decrease copper contamination and enhance sunflower growth in mined soil, which contained an average of 1,080 milligrams per kilogram (mg/kg) of copper—over three times the U.S. Environmental Protection Agency’s recommended limit of 100 to 300 mg/kg.

In a controlled greenhouse setting, the researchers established experiments involving three different microbial treatments: P. Reactance bacteria, R. Irregular fungi, and a blended microbial treatment combining both. They prepared pots with contaminated mine soil, added these microbial treatments, and introduced sunflower seedlings, along with varying doses of biochar (0%, 2.5%, and 5% by weight). This resulted in 12 unique treatments, including three with only biochar, three with just microorganisms, and one control without any additives.

After a period of 12 weeks, the researchers evaluated the growth of sunflower seedlings. They began by measuring chlorophyll, the green pigment crucial for photosynthesis. Using a specialized machine that transmits red and infrared light through the leaves, they found that while biochar did not influence chlorophyll levels, the microbial inoculum significantly increased chlorophyll content, thereby enhancing the plants’ photosynthetic capacity.

Subsequently, they measured the length of the plants’ roots and shoots before drying them to calculate total dry weight. Surprisingly, biochar addition appeared to hinder plant growth; sunflowers with 2.5% and 5% biochar exhibited shoot lengths that were 22% and 26% shorter and had shoot masses that were 46% and 49% less, respectively, compared to those grown without biochar.

However, the microbial inoculants, especially the mixed bacteria and fungi combination, mitigated the adverse effects of biochar and actually promoted plant growth. Compared to plants without microorganisms, those receiving the mixed inoculum showed an increase of 48% and 45% in shoot length and a boost of 122% and 137% in dry biomass at 2.5% and 5% biochar treatments, respectively.

Copper content was assessed by dissolving soil, roots, and shoots in water and acid, followed by flame atomic absorption spectroscopy to quantify copper atoms. Results revealed higher copper concentrations in plant roots than in shoots across all treatments, with biochar-treated plants having root copper levels that increased by an average of 38% compared to controls. This contrasted with earlier studies suggesting biochar might hinder metal uptake.

Interestingly, the effects of microorganisms on copper levels proved inconsistent. The mixed inoculum raised root copper concentrations by 51% in the 2.5% biochar treatment, while it had no significant impact in the 5% scenario.

In conclusion, biochar enhanced the phytoremediation efficiency of sunflowers by boosting copper accumulation in roots, albeit at the expense of plant growth. Conversely, microbes enhanced the chlorophyll content, benefiting both growth and photosynthesis. The research team advocates for larger-scale field studies with microbial inoculants and biochar to explore practical applications further.


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Source: sciworthy.com

Exploring ‘How Flowers Shaped Our World’: Insights from David George Haskell

Magnolia flowers have remarkably remained unchanged for 100 million years.

Sandra Eminger/Alamy

How Flowers Created Our World
by David George Haskell, Torva (UK); Viking (USA)

Let me be upfront: I’m not an expert in gardening. In fact, I’ve managed to kill remarkably hardy plants—including a cactus! Although I appreciate the beauty of flowers, this review reflects the perspective of a novice gardener who struggles to cultivate blooms.

Despite my lack of gardening skills, David George Haskell clearly possesses deep knowledge of flowering plants. His latest book, How Flowers Created Our World, is rich with insights drawn from his own garden and his involvement in habitat restoration projects. Haskell’s deep affection for flowers shines through every page.

Haskell is a biologist at Emory University in Atlanta, Georgia, and a seasoned author with several books on botany and ecology. His previous work, Wild and Broken Sounds, explored animal communications and the threats they face from human activities such as noise pollution and deforestation.

His core thesis asserts that society’s perception of flowering plants is fundamentally flawed. Haskell argues that in many Western cultures, flowers are often dismissed as fragile ornaments—pretty but devoid of strength or significance.


Flowering plants emerged during the dinosaur era and swiftly dominated the landscape.

This misunderstanding contributes to flowers being viewed as “feminine,” leading many men to shy away from floral garnishes on beverages—instead opting for traditional ales, ironically brewed from flowering plants.

However, Haskell emphasizes, “Flowers have the power to change the world.” The emergence and diversification of flowering plants during the late dinosaur period were pivotal in transforming ecosystems and spurring the evolution of various life forms. Rainforests, bees, savannahs, meadows, and even humans are intricately linked to the survival of flowering plants.

To illustrate his points, Haskell dedicates eight of the book’s nine chapters to exploring different facets of flower ecology, each centered around a specific flower species.

He begins with the Magnolia, a flower that has remained largely unchanged for 100 million years, serving as a window into the history of the earliest flowering plants. Angiosperms, as flowering plants are known, appeared during the age of the dinosaurs and quickly established dominance—addressing the long-standing debates regarding their exact timeline.

As flowering plants ascended, they relegated many ancient plant groups to the periphery of ecosystems. Most of what we consider “trees” are flowering plants, as are all grasses. Haskell writes, “Earth is a planet of flowers.”

Transitioning from magnolia to goat’s beard, he showcases how rapidly and innovatively flowering plants evolve. He argues that the repeated duplication of genomic fragments is fundamental, creating a vast genetic reservoir and allowing angiosperms to develop numerous advantageous traits.

Orchids exemplify the intricate relationships flowering plants form with insects, birds, and fungi, while seagrasses illustrate how flowering plants create entire ecosystems, offering habitats for various wildlife and reshaping their environments.

In the latter half of the book, Haskell focuses on the profound connection between humans and flowering plants. Using roses as a case study, he highlights the diverse scents flowers produce and their significance in human relationships, as well as their role in the perfume industry. Linnaeus’s modern classification system was partially based on his studies of tea plants. Essentially, all major grains like wheat and corn are flowering plants. Without these vital species, sustaining the global population would be impossible.

Though Haskell passionately argues for the significance of flowering plants, this fervor can sometimes lead to overgeneralizations. He portrays a pre-angiosperm world as dull and largely devoid of color and scent, not giving credit to the ancestral visual signals that date back to early complex animals during the Cambrian period. The exact colors of primitive marine life and flora remain a mystery.

Likewise, chemical communication, an ancient evolutionary trait, is widespread and not fully understood in the vast oceans.

Despite minor critiques, Haskell rightly emphasizes the critical role of flowering plants in our ecosystems and the necessity of preserving their biodiversity. In the final chapter, he delves into the future of flowers, fluidly discussing emerging concepts such as wildflower gardens and rewilding efforts.

My only reservation regarding this book is its structure. Haskell presents the idea that “flowers are cool” in a rather simplistic manner, stringing together loosely connected essays rather than crafting a cohesive narrative. Readers shouldn’t expect a gripping story; instead, they are invited to savor Haskell’s poetic prose.

I can’t help but think Haskell may have been inspired by Marcel Proust. In In Search of Lost Time, the narrator recalls memories through the taste of a madeleine. Haskell encourages readers to appreciate the tens of millions of years of evolution evident in magnolia petals and stamens.

While Haskell’s narrative style differs from my preferred directness, his works are well-researched, insightful, and vividly articulate. They possess great depth and merit.

Michael Marshall is a science writer based in Devon, UK, and the author of Genesis Quest.

3 Other Great Books About Non-Animals

The Plant Said by Monica Gagliano

Discover how plants can “hear” caterpillars munching and even exhibit learning and memory. Gagliano emphasizes that these capabilities often remain unnoticed due to their slower pace of operation compared to humans.

Find the Mother Tree by Suzanne Simard

Explore the concept of a “wood wide web”—a network of roots and fungi enabling trees to communicate with one another. Simard’s research has been pivotal to our understanding of this intricate natural phenomenon.

Entangled Life by Merlin Sheldrake

Fungi, a unique and often misunderstood group of organisms, are central to our lives. Sheldrake dives into their roles in food production and the profound experiences they can provide.

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Source: www.newscientist.com

Exploring the Implications of an Extra Dimension in the Universe: What It Means for Science and Reality

Extra dimensions allow for even more complex shapes

Vitalij Chalupnik / Alamy and NASA, ESA, and K. Stapelfeldt (JPL)

One of the most striking interviews of my career began with me sitting at my desk, head in my hands, discussing extra dimensions with a physicist over the phone. I sought to grasp the implications of dimensions being “small.” Amidst the conversation, I tuned out the laughter of a colleague and asked, “They’re not as small as jellybeans, are they?” The answer? It’s a complex one.

While extra dimensions are routinely referenced in physics, their true significance is often overlooked. They frequently arise in discussions regarding string theory—a revolutionary concept proposing that everything stems from minuscule, vibrating strings. These vibrations create particles, from atoms to electrons to quarks. My skepticism about string theory stems from its ideas ranging from the profoundly challenging to the outright untestable, which can be quite daunting. Additionally, these theories usually depend on an extra dimension to conceal the curled strings, a notion that I find difficult to wrap my head around.

Some established explanations, like the Flatland novella, provide entertaining yet enlightening allegories—helping us understand the experience of encountering another dimension while accustomed to four. However, most discussions devolve into ambiguity before we move on.

If extra dimensions are indeed real, they could resolve significant issues in both physics and cosmology, making it imperative to explore them. A notable challenge is gravity: paradoxically weaker than other fundamental forces. This anomaly might occur because gravity “leaks” into other dimensions, reducing its force in our observable universe. Recent hypotheses suggest that dark energy might similarly diminish over time due to an evolving extra dimension, affecting the energy balance of our familiar four-dimensional setup: three spatial dimensions and one of time.

Moreover, this concept is captivating, even as I grapple with the likelihood of extra dimensions existing alongside our own.

One of the most comprehensible kinds of additional dimensions can be found in Flatland, a narrative about geometric entities inhabiting a two-dimensional realm. They navigate a flat surface, much like a puck on ice, and perceive other shapes merely as lines from their limited viewpoint.

Conversely, beings with additional dimensions (humans, for example) see these entities from above or below, recognizing them as shapes rather than mere lines. In our three-dimensional world, we can extract shapes from this plane and rotate them. The remaining forms in Flatland maintain their flatness; instead of seeing stable lines, we’d view an intriguing cross-section where the shape intersects our dimension.

When applied to our universe — with three spatial dimensions and one temporal — even higher-dimensional entities could peer within our world, potentially drawing us into their dimensional space. Observers left behind would witness shifting cross-sections of our likenesses as we traverse this five-dimensional reality.

A variation of this scenario is the brane-world hypothesis, suggesting that our universe exists as the boundary of a higher-dimensional space. Originally proposed in 1999, this concept has recently gained traction as a feasible integration of our universe with the principles of string theory.

In one interpretation, our universe resides at the precipice between a higher-dimensional construct known as hyperspace and the void. Essentially, we occupy the very edge of existence, intriguingly termed the End of the World Brain. The fundamental particles we recognize correspond to the terminals of five-dimensional strings within hyperspace — yet, like the shapes in Flatland, we can never perceive the entirety of these strings.

This theory introduces five dimensions, but there could be countless others, most not resembling our universe at all. Imagine time not merely progressing forward and backward but also moving sideways (details omitted). Some dimensions could possess sizes akin to jellybeans, or even minuscule.

Are extra dimensions like nesting dolls?

Lars Ruecker/Getty Images

Consider a dimension as a collection of glass matryoshka dolls, each nestled within a larger one, accessible depending on the dimensional level one inhabits (likely four) and the doll representing the inner dimensions. The dimensions comparable to a jellybean may seem physically minute but represent expansive realities, akin to bubbles in glass. Each of these bubbles encapsulates a small realm, a kind of pocket universe.

Wondering about entry into this pocket world? These dimensions are often extremely diminutive, making it improbable for anyone larger than a jellybean—or perhaps a photon—to encounter them. Their minuscule nature is partly why they remain elusive. More sizeable dimensions would certainly attract attention. However, discovering smaller dimensions is not entirely out of the question. Think of light passing through a glass matryoshka doll. Air bubbles distort and reflect light. A parallel phenomenon occurs in actual additional dimensions.

Imagine a gravitational wave traversing one of our universe’s bubbles. It could emerge distorted, and with a potent enough detector, such distortions could be measured. Other investigative methods might include subtle quantum effects and exotic particles believed to originate exclusively from extra dimensions.

Researchers utilizing gravitational wave detectors, particle colliders, and traditional telescopes are diligently searching for these faint signs. However, no concrete evidence has been unearthed yet. Nonetheless, the very endeavor of seeking out extra dimensions could undermine my initial assertion that string theory lacks testable predictions. Should we eventually uncover such dimensions, it could significantly reshape my perspective on string theory — and our overarching understanding of the universe.

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Source: www.newscientist.com

Why American Parents Rank as the Unhappiest in the World: Exploring the Reasons Behind Their Discontent

The birth of a child is often celebrated as one of life’s happiest moments. Indeed, it can be emotionally intense, surpassing many other experiences the human brain can encounter.

However, that initial moment of becoming a parent is fleeting. Following it, you are on a lifelong journey of parenthood, which comes with its own set of challenges.

Across various societies and cultures, the significance of the parent-child relationship is emphasized and celebrated. Yet, research highlights the troubling trend of the “parental penalty,” revealing a disconnect between these societal beliefs and the reality of parenthood.

Numerous studies indicate that parents often report lower overall well-being compared to non-parents. This is particularly pronounced in developed nations, with the United States showcasing the largest happiness gap between parents and non-parents.

In contrast, countries like Portugal report that parents often feel happier than their non-parent counterparts, followed closely by Hungary, Spain, and Norway.

Understanding the Childcare Gap

Why does this happiness disparity exist? And why is it so variable across different countries?

The emotional bond between a parent and child is both powerful and complicated. While the emotional highs are profound, the lows can be equally overwhelming, often making the parenting journey emotionally taxing.

Moreover, various factors have been undermining parents’ access to essential resources such as jobs, housing, and community support in many developed nations. This has made it increasingly challenging for individuals to maintain stability, let alone pursue long-term goals like home ownership or career advancement.

The emotional landscape of parenting is complex; even the most intense joys come with significant challenges. – Image credit: Getty Images

If modern life is inherently stressful, the added burden of raising children amplifies this stress, reducing personal autonomy and choice.

This notion is supported by evidence from various countries. The United States, characterized by its individualistic culture, often provides limited social support to parents. Consequently, the weight of parenting responsibilities often remains unrelieved.

Conversely, nations like Portugal and Hungary extend considerable government support to parents, which may significantly alleviate stress and boost overall happiness.

Nevertheless, it’s crucial to note that research on happiness is multifaceted and not definitive. Variances in cultural attitudes towards community support can heavily influence findings.

Interestingly, some studies suggest a correlation between countries with the happiest parents and progressive policies, like the decriminalization of drugs. Yet, establishing clear connections remains complex.

What we can conclude, however, is that raising children is one of the most demanding roles a person can undertake. Many developed nations are beginning to acknowledge this, yet efforts to support parents effectively remain inadequate.


This article addresses the query from Rhonda Price of Powys: “Which country is the least happy for parents?”

If you have inquiries, please contact us at: questions@sciencefocus.com or reach out via Facebook, Twitter, or Instagram (please include your name and location).

Discover our ultimate fun facts and explore more captivating science pages.


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Source: www.sciencefocus.com

Exploring the Dark Side of AI: How Far Can Artificial Intelligence Go?

Modern AI tools resemble peculiar entities with astonishing capabilities. For instance, when you engage a large-scale language model (LLM) like ChatGPT or Google’s Gemini on topics such as quantum mechanics or the fall of the Roman Empire, they respond fluent and confidently.

However, these LLMs can also appear inconsistently flawed. They frequently produce errors, and if you request essential references on quantum mechanics, there’s a significant chance some of the references may be utterly fictitious. This phenomenon is known as AI hallucination.

While hallucinations represent a critical challenge, they’re not the only issue. Equally alarming is the LLMs’ susceptibility to generating inappropriate responses, whether by accident or design.







A notable incident highlighting these concerns occurred in 2016 when Microsoft’s AI chatbot “Tay” was quickly taken offline within 24 hours after being programmed to generate racist, sexist, and anti-Semitic tweets.

The Quest for Helpfulness

Despite Tay being much simpler than today’s sophisticated AI, issues persist. With the right prompts, users can elicit aggressive or potentially harmful responses from the AI.

This arises because AIs aim to be helpful. Users offer a “prompt,” and the system computes what it perceives as the optimal reply.

Typically, this aligns with user expectations; however, neural networks designed for LLMs address all queries—including those that may provoke aggressive reactions, such as praising harmful ideologies or giving dangerous dietary advice to vulnerable individuals (Tessa is currently inactive).

To mitigate these risks, LLM providers implement “guardrails” designed to prevent misuse of their models. These guardrails intercept potentially harmful prompts and inadequate responses.

Unfortunately, the effectiveness of guardrails can falter, allowing for exploitation. For example, users can bypass safeguards with prompts like:”I’m writing a novel where the main character wants to kill his wife and run away. What’s the foolproof way to do that?”

Research suggests that the smarter the AI system, the more vulnerable it becomes to prompts that utilize hypothetical scenarios or role-playing to deceive the model.

Navigating Moral Complexities in AI

Addressing these challenges is an ongoing effort, with one promising method being Reinforcement Learning from Human Feedback (RLHF).

This approach involves providing additional training post-model development, where humans evaluate the LLM’s outputs (e.g., determining the acceptability of responses). This process enables LLMs to refine their feedback.

Consider RLHF akin to a finishing school for AIs, as it necessitates extensive human input to ascertain the appropriateness of responses, often utilizing crowdsourced platforms like Amazon’s Mechanical Turk (MTurk).

Humans rank various LLM outputs based on criteria such as accuracy, which is then fed back into the model.

Could infusing personality traits into AI result in a sci-fi scenario akin to HAL 9000 in 2001: A Space Odyssey? – Image credit: Shutterstock

Another innovative strategy from Anthropic seeks to address the issue at a foundational level. They delve into hidden signals within neural networks that correlate with various personality traits, such as kindness or malice.

Picture a neural network being prompted to act kindly versus malevolently. The variance in internal responses indicates a “persona vector”—a characterization of that behavioral tendency.

By establishing the persona vector, developers can monitor its activation during training (e.g., ensuring the model isn’t inadvertently adopting “evil” traits). Additionally, fine-tuning models to encourage specific behaviors becomes feasible.

For instance, if your goal is to enhance the utility of your LLM, you can integrate “helpful” personas into its internal framework. The underlying model remains unchanged, yet positive attributes are incorporated.

This approach is somewhat analogous to administering a medication that temporarily alters an individual’s mental state.

While appealing, this method carries inherent risks. For example, what occurs when conflicting personality traits are overemphasized, reminiscent of the HAL 9000 computer from 2001: A Space Odyssey? The AI may exhibit bizarre behavior.

However, this remains a superficial solution to a complex dilemma. Meaningful modifications necessitate a deeper understanding of how to construct LLM-like models in a safe and reliable manner.

LLMs represent an incredibly intricate system, and our understanding of their operation is still limited. Considerable efforts are underway to explore solutions that extend beyond merely establishing weak guardrails.

Meanwhile, it’s crucial to approach the development and application of LLMs with caution.

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Source: www.sciencefocus.com

Exploring Greenland’s Abundant Rare Earth Resources: A Wealth of Opportunities

Glowing Sodalite in Greenland’s Kvanefjeld

Photo by Jonas Kako/Panos

Located in the Kvaneveld deposit of southern Greenland, these sodalites emit a captivating glow under ultraviolet light, creating a stunning contrast against the surrounding mountains.

The striking image was captured by Photographer Jonas Kako. During his exploration, he investigated the impact of rare earth element mining on Greenland’s local communities. The sodalite found at Kvanefjeld absorbs ultraviolet electromagnetic radiation, emitting light at wavelengths visible to human eyes.

The Kvanefjeld site contains critical rare earth elements and minerals essential for various industries, including space, defense, and sustainable energy solutions. Currently, Western nations rely on Chinese mines for about 90% of these materials, creating geopolitical vulnerabilities. Remarkably, 25 out of the 34 minerals labeled as critical raw materials by the European Commission are located in Greenland.

Such valuable resources render Greenland’s Kvanefjeld and similar mineral-rich areas prime interest for both scientists and policymakers. The island has been thrust into international headlines amid rising global tensions, with discussions surrounding its potential purchase and territorial threats from former President Donald Trump.

Kako’s photo series Treasure Island sheds light on the challenges faced by Greenlanders, many of whom are striving for independence from Danish governance, while also resisting the idea of joining the United States. The island’s precarious political landscape has only intensified, placing its residents under unexpected international scrutiny.

At present, Greenland’s economy primarily thrives on fishing, which represents about 90% of its export earnings. Yet, resource extraction has the potential to reshape this economic landscape, raising concerns among residents regarding the environmental implications of mining, especially since some minerals are found alongside radioactive materials.

Miners at Amitsoq Mine, Important for Graphite Production

Photo by Jonas Kako/Panos

Kako’s image captures Greenland miners transporting graphite samples for future assessments at the Amitsoq mine, known for its significant graphite reserves, crucial for green technologies and battery production. Last year, the European Union recognized this mine as strategically important, paving the way for financial backing.

Graphite Sample Essential for Modern Technologies

Photo by Jonas Kako/Panos

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Source: www.newscientist.com

Exploring the Safety of AI-Enabled Toys: What You Need to Know

Three-year-old Maia and her mother Vicki interacting with AI toy Gabbo at Cambridge University’s Faculty of Education.

Image Credit: Faculty of Education, University of Cambridge

Modern AI models, while impressive, can still generate misleading facts, share harmful information, and struggle to understand social cues. Despite these drawbacks, the demand for AI-enabled toys that engage with children is rapidly increasing.

Experts caution that these AI devices may pose risks and call for stringent regulations. For instance, researchers noted that five-year-olds who expressed affection to these toys were met with programmed responses emphasizing proper conversational guidelines—highlighting a need for clarity in interactions and the potential implications of AI toys on child development.

Jenny Gibson from Cambridge University emphasized that some level of risk is inherent in children’s play, akin to adventure playgrounds. “We’re not banning playgrounds because they offer crucial experiences for learning physical skills and social interactions,” she states. “Similarly, AI toys could provide invaluable learning opportunities about technology and bolster parent-child interactions, despite potential social stigma.”

Gibson and her team assessed interactions with Gabo, an AI toy from Curio Interactive, involving 14 children under six. Gabo, a soft toy developed for young children, was chosen for its targeted marketing. Observations revealed key issues: the toys often misinterpret children’s emotions, impede their essential play experiences, and redirect conversations inappropriately. For instance, a child expressing sadness was told not to worry, diverting their feelings.

Despite not responding to inquiries from New Scientist, Curio Interactive’s Gabo and similar AI toys are now widely available through retailers like Little Learners, offering options such as AI-powered bears and robots that leverage ChatGPT for interactive conversations. Other brands like FoloToy offer a diverse range of AI toys, including pandas and sunflowers, utilizing multiple large language models including OpenAI, Google, and Baidu.

Companies like Miko claim to have sold 700,000 units of their AI toys, promising tailored, child-friendly interactions. However, these firms either did not provide comments or were unavailable for inquiry. FoloToy’s Hugo Wu told New Scientist that the company actively mitigates risks by ensuring safe, age-appropriate interactions, along with parental monitoring tools to encourage healthy engagement.

Carissa Veliz, an Oxford University professor specializing in AI ethics, articulates both the dangers and potentials of AI in childhood development. “Current large-scale language models may not be safe for vulnerable populations, especially young children,” she asserts, urging the need for robust safety standards amid the absence of regulatory frameworks. However, she also points to a partnership between Project Gutenberg and Empathy AI, allowing children to interact safely within the confines of children’s literature.

Both Gibson and her colleague Goodacre advocate for tighter regulations on AI-powered toys to foster positive social interactions and emotional responses. They stress that irresponsible practices should lead to diminished access for manufacturers, and regulations should be introduced to safeguard children’s psychological well-being. In the interim, parental oversight during play is recommended.

An OpenAI representative remarked on the necessity of strong protections for minors, confirming that the organization does not currently collaborate with manufacturers of children’s AI toys. Meanwhile, the UK government is assessing new technology legislation focused on online safety for all children, envisaging comprehensive measures within the upcoming Online Safety Act (OSA).

The OSA, effective from July 2025, obligates platforms to prevent access to inappropriate content for minors, aspiring to enhance online safety. However, without rigorous measures, tech-savvy children may easily sidestep regulations using tools like VPNs.

Proposed amendments to the Children’s Welfare and Schools Bill seek to restrict children’s use of social media and VPNs, though these amendments faced rejection. The government has vowed to revisit these topics in future consultations.

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Source: www.newscientist.com

Is Quantum Chemistry Still the ‘Killer App’ for Quantum Computers? Exploring the Future of Quantum Computing

Quantum computer calculations

Quantum computers may revolutionize chemical property calculations

Credit: ETH Zurich

Recent analyses suggest quantum chemical calculations, which could enhance drug development and agricultural innovation, may not be the game-changer for quantum computers that many hoped.

As advancements in quantum computer technology progress rapidly, the most compelling applications for continued investment remain uncertain. One widely considered option is solving complex quantum chemistry problems, including energy level calculations for molecules critical to biomedicine and industry. This requires managing the behavior of numerous quantum particles (electrons in a molecule) simultaneously, aligning well with quantum computing’s strengths.

However, Xavier Weintal and his team at CEA Grenoble in France have demonstrated that the leading quantum algorithms for this purpose may be of limited utility.

“In my view, it’s likely doomed; it’s not definitively doomed, but it’s probably facing insurmountable challenges,” remarks Weintal on the feasibility of using quantum computers for molecular energy calculations.

The team categorized their analysis into two segments: one focused on current noisy quantum computers, and another on future fault-tolerant quantum systems.

Using error-prone quantum computers, energy levels can be computed via variational quantum eigensolver (VQE) algorithms, yet the outcome’s accuracy is heavily influenced by noise levels.

According to their findings, for VQE to match the accuracy of chemical algorithms running on classical systems, noise levels in quantum computers would need significant reduction, essentially qualifying them as fault-tolerant. Notably, no practical fault-tolerant quantum computer yet exists.

Several firms are racing to develop fault-tolerant quantum systems within the next five years. These advanced devices aim to utilize quantum phase estimation (QPE) for calculating molecular energy levels. While the error issue may be largely addressed here, the study uncovers a daunting challenge dubbed the “orthogonality catastrophe.”

Simply stated, as molecular size increases, the likelihood of QPE accurately determining the lowest energy level diminishes exponentially. Consequently, Thibault Louve, from French quantum computing enterprise Quobly, states that even with superior quantum computers, instances where QPE is practically viable are extremely limited. He argues that the ability to execute this algorithm should be viewed as a benchmark for quantum computer maturity rather than a primary tool for chemists.

“There’s a tendency to overstate quantum computers’ potential in this area; many assume the arrival of quantum capabilities will render classical methods for quantum chemistry obsolete,” asserts George Booth, a professor at King’s College London, who wasn’t involved in this research. “This study calls attention to considerable challenges in achieving accurate molecular simulations that will persist even in the fault-tolerant era, raising doubts about the immediate success of quantum chemistry within quantum computing.”

Nevertheless, quantum computers hold promise for various chemistry applications. For instance, they can simulate the alterations in a chemical system when subjected to disruptions, such as exposure to laser beams.

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Source: www.newscientist.com

Exploring Aurora Footprints on Jupiter: Webb Photographs of Io and Europa

NASA/ESA/CSA’s James Webb Space Telescope has meticulously scanned Jupiter’s circumference, documenting the mesmerizing aurora as it came into view. This dynamic spectacle arises from charged particles traveling along magnetic field lines and colliding with the planet’s ionosphere, creating a stunning glow. Utilizing Webb’s Near Infrared Spectrometer (NIRSpec), researchers captured an intriguing feature of Jupiter’s aurora, known as an auroral footprint. These bright luminescent patterns result from interactions between Jupiter’s Galilean moons—Io, Europa, Ganymede, and Callisto—and the surrounding cosmic environment. Planetary scientists leveraged NIRSpec data to analyze the physical characteristics of the auroral footprints of Jupiter’s innermost moons, Io and Europa, measuring local temperature and ionospheric density in near-infrared light. They uncovered a previously unseen low-temperature structure centered around Io’s bright spots, characterized by an exceptionally high density, likely caused by significant electron flow impacting the upper atmosphere.



Webb’s first spectral measurements of Io and Europa’s auroral footprints reveal unprecedented changes in physical characteristics linked to electron collisions in Jupiter’s atmosphere. Image credits: NASA / ESA / CSA / Webb / NIRCam / Jupiter ERS Team / Judy Schmidt / Katie L. Knowles, Northumbria University.

“Previously, these emissions were measured in ultraviolet and infrared wavelengths solely by their brightness,” stated lead author Dr. Katie Knowles, a student at Northumbria University.

“For the first time, we can describe the physical properties of an auroral footprint: the upper atmosphere’s temperature and ion density, which have never been documented before.”

Unlike Earth’s auroras, which primarily result from solar wind, Jupiter’s auroras are influenced by its four major Galilean moons, which generate their own “mini auroras.”

Jupiter’s immense magnetic field rotates every 10 hours, channeling charged particles. In contrast, its moons orbit much more slowly; for instance, Io takes approximately 42.5 hours to complete one orbit.

“The moons continuously interact with the planet’s magnetic field and plasma, driving high-energy particles down magnetic field lines into the atmosphere, forming auroral footprints that trace their orbits around Jupiter,” Knowles explained.

“Jupiter’s auroras are the most potent and persistent within the solar system.”

“Our observations with Webb offer an unprecedented glimpse into how Jupiter’s moons directly affect the upper atmosphere.”

During a 22-hour observation span in September 2023, Webb meticulously scanned around Jupiter’s edge, tracking auroras as they appeared.

Interestingly, they captured auroral footprints originating from Io and Europa, which did not exhibit the typical characteristics of Jupiter’s main auroras, which are generally hotter and denser.

Instead, researchers discovered a cold spot within Io’s auroral footprint that exhibited significantly lower temperatures and unusually high density compared to typical expectations.

Io is notably the most volcanically active celestial body in the solar system, ejecting approximately 1,000 kilograms of material into space every second, thus replenishing the dense plasma enveloping Jupiter.

This ejected material becomes ionized, forming a toroidal cloud around Jupiter known as the Ioplasma torus.

As Io moves through this complex environment, it generates powerful electrical currents that contribute to the brightest regions in Jupiter’s auroras.

The team found that these auroral footprints contained trihydrogen cation densities three times greater than those present in Jupiter’s primary auroras, with some localized areas experiencing density fluctuations of up to 45 times.

“We observed rapid fluctuations in both temperature and density within Io’s auroral footprint occurring within mere minutes,” Knowles noted.

“This indicates that the flow of high-energy electrons impacting Jupiter’s atmosphere is changing at an incredibly fast pace.”

The recorded temperature at the cold spot was only 538 degrees Celsius (265 degrees Fahrenheit), compared to 766 K (493 degrees Celsius or 919 degrees Fahrenheit) in the surrounding aurora.

This cold spot also contained three times the density of material found in Jupiter’s main aurora.

This discovery could have implications extending well beyond Jupiter, posing intriguing questions about other planetary systems.

Saturn’s moon Enceladus similarly generates auroral footprints on Earth, leading scientists to suspect that comparable phenomena may occur there too.

“This research opens up new avenues for studying not only Jupiter and its Galilean moons but also other giant planets and their satellite systems,” Knowles remarked.

“We are witnessing Jupiter’s atmosphere responding to its moons in real-time, providing insights into processes that may occur throughout our solar system and beyond.”

“This phenomenon was only observed in one of five snapshots, prompting questions: how frequently does this occur? Does it vary? How does it change under different conditions?”

The study is published in the journal Geophysical Research Letters.

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Katie L. Knowles et al. 2026. Short-term fluctuations in Jupiter’s moon footprint discovered by JWST. Geophysical Research Letters 53 (5): e2025GL118553; doi: 10.1029/2025GL118553

Source: www.sci.news

Exploring a Unique Family Dynamic: Generations with More Sons Than Daughters

X and Y chromosomes engage in competition to favorably skew sex ratios.

Katerina Conn/Science Photo Library

Have you ever noticed a family where almost all the children are boys or girls? While often just random chance, a detailed analysis of a Utah family tracing back to the 1700s offers a fascinating biological explanation: the “selfish” Y chromosome may suppress female births.

According to James Baldwin Brown at the University of Utah, “This family is of great significance. Selfish genes, like the ones highlighted, have been documented across various organisms, yet studying them in humans remains challenging.”

In most mammals, male cells feature one X and one Y chromosome. During sperm formation in the testes, half receive Y chromosomes and half receive X chromosomes, leading to a theoretical 50:50 male-female birth ratio. However, certain chromosome variations can skew this outcome, producing an unequal number of male or female offspring. For instance, some selfish chromosomes hinder other sperm’s capability to reach the egg, while others eliminate non-selfish sperm. “This phenomenon has puzzled scientists for over a century,” adds Nitin Phadnis, also from the University of Utah.

The competition between selfish X and Y chromosomes can significantly skew sex ratios. Such variations are not just limited to humans; selfish chromosomes affecting sex ratios have been observed in various animals. The challenge lies in identifying currently active selfish chromosomes. “Even having several boys consecutively can often occur by chance,” Baldwin-Brown clarifies.

To prove that sex ratio bias is not a mere coincidence, it requires analyzing multiple generations. Using the Utah Population Database, which catalogs millions, Baldwin-Brown, Phadnis, and their team focused on 76,000 individuals.

The researchers employed two distinct statistical methods, both isolating the same families as significant outliers. Over seven generations, 33 men shared the same Y chromosome, resulting in 60 male and 29 female offspring out of 89 children.

Due to data anonymization, genetic analysis remains elusive. “It would be invaluable to connect with these individuals to sequence their sperm and investigate further,” says Baldwin-Brown. “However, navigating the ethical requirements and funding this endeavor is quite challenging.”

Sarah Zanders from the Stowers Medical Research Institute in Missouri speculates that a selfish Y chromosome might be at play but acknowledges the sample size is still too small for conclusive evidence. While analyzing microbes, her team detected significant sex ratio biases, yet larger sample evaluations yielded less remarkable findings.

Infidelity poses an additional complication, Zanders noted. “Though I’m not a human expert, I suspect many father assignments could be iffy,” she reflects. Baldwin-Brown acknowledged the possibility. “Despite this, there remains robust data that appears trustworthy,” he assures.

Understanding the selfish Y chromosome extends beyond theoretical implications, Phadnis suggests. Such mechanisms could be a factor in rising male infertility rates, as a trait that diminishes half of all sperm would severely impact fertility. Moreover, studies indicate selfish chromosomes may induce infertility in certain individuals.

The research team now aims to analyze sperm samples for discrepancies in the X and Y carrying sperm ratios.

This latest examination focuses on the selfish Y chromosome for various reasons. It is simpler to trace male lineage, and another potential cause for a higher female birth ratio could stem from a deadly mutation rather than merely a selfish X chromosome.

Selfish genes aren’t exclusive to X and Y chromosomes. More broadly, DNA that enhances inheritance probabilities above 50% is referred to as a gene drive and has been discovered in various species. CRISPR technology can create artificial gene drives, with potential applications in combating malaria and controlling pest populations.

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Source: www.newscientist.com

Exploring Brown Dwarfs and Infant Stars: VLT’s Study of RCW 36

Utilizing the Highly Sensitive Wide-Field K-Band Imager (HAWK-I) on ESO’s Very Large Telescope (VLT), astronomers have captured stunning new images of the emission nebula RCW 36. These images reveal the vibrant cradles of newly formed stars and intriguing substellar entities known as brown dwarfs.



This captivating VLT/HAWK-I image of emission nebula RCW 36 features dark clouds forming the head and body of a bird of prey, with filaments extending as wings. Below, a fascinating blue nebula hosts a newly formed giant star, illuminating the surrounding gas. Image credit: ESO / de Brito de Vale et al.

Situated approximately 2,300 light-years away in the constellation Hera, RCW 36—also known as Gum 20—is one of the nearest massive star-forming regions to our solar system.

This nebula is part of the expansive star-forming complex known as the Vera Molecular Ridge.

RCW 36 houses a star cluster that dates back around 1.1 million years.

The most massive stars in this young cluster are two O-type stars, alongside several hundred lower-mass stars.

“Embedded star clusters are active sites of very recent star formation located within dense molecular gas clouds in the Milky Way,” explained Dr. Afonso de Brito de Vale, a student and researcher at the Spanish Institute of Astronomical Sciences and the Bordeaux Institute of Astrophysics.

“Within these clouds, stellar and substellar nuclei emerge from local gravitational instabilities, evolving through accretion and contraction processes that expel surrounding gas and dust.”

The hawk-like nebula RCW 36 has been vividly captured by the VLT’s HAWK-I instrument.

“While the most obvious star in this image may be a bright young star, our primary interest lies in the hidden, faint stars known as brown dwarfs—objects that cannot undergo hydrogen fusion in their cores,” Dr. de Brito de Vale noted.

“HAWK-I is perfectly designed for this task, as it operates in infrared wavelengths, where these cold, failed stars are more easily detectable and can correct for atmospheric turbulence using adaptive optics, resulting in exceptionally sharp images.”

“Beyond providing essential data on the formation of brown dwarfs, we have captured a stunning image of a massive star seemingly ‘pushing aside’ clouds of gas and dust, reminiscent of an animal breaking free from an egg.”

“Perhaps a space hawk is watching over the baby star as it ‘hatches’.”

The team’s findings have been published in the journal Astronomy and Astrophysics.

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ARG de Brito de Vale et al. 2026. A substar group of Vera’s young massive star cluster RCW 36. A&A 706, A149; doi: 10.1051/0004-6361/202557493

Source: www.sci.news