The Surprising Connection Between Family Size and Aging: How the Number of Children Affects Your Youthfulness

As a father who gazes at my weary reflection each morning before the school rush, I can confidently assert that our children indeed age us. However, research reveals a more intricate relationship between parenthood and aging.

Becoming a parent induces substantial physiological changes, known as maternal matrescence and paternal patrescence.

These terms encompass the physical, cognitive, emotional, and social transformations that come with parenting, many of which are understood.

Major hormonal shifts, including decreased testosterone and increased oxytocin during and after birth, are thought to be biological adaptations that foster parental attentiveness and facilitate bonding with children.

Similar adjustments occur in our brains, which may slightly shrink and restructure.

However, research indicates that these changes can elevate some parents’ risks for stress and postpartum mental health issues.

Telomere length, the protective caps on your DNA, is a key indicator of health – Image courtesy of Getty Images

In the early parenting years, biological aging pathways are significantly affected. Stressors such as sleep deprivation and financial strain may lead to shorter telomeres, the protective caps at the ends of our DNA.

Shorter telomeres are associated with increased risks of cardiovascular diseases, dementia, and premature mortality. Thanks for the added stress, kids!

Chronic stress can elevate inflammation and hormones like cortisol, resulting in long-term health complications.

Yet, as any fatigued parent would note, it’s just a phase. Research suggests that, over time, parents may actually enjoy a slightly longer life expectancy compared to non-parents.

Data from Sweden indicates that this advantage may emerge post-60, with fathers enjoying a two-year lead and mothers experiencing a marginally decreased advantage.

What accounts for this phenomenon? Researchers believe the social and emotional support received from adult children plays a significant role.

Other powerful factors also influence longevity, such as income level. Parents in low-income households typically experience higher stress, leading to life expectancies that are 10 years shorter in comparisons between income groups.

Additionally, factors such as the number of children and the timing of their births can impact outcomes. A recent study from the University of Helsinki found that giving birth between the ages of 24 and 38 is linked to more favorable aging and longevity.

The study also indicated that women with two to three children tend to have longer lifespans, while those with four or more children may face accelerated biological aging and shorter lifespans.

This could reflect the biological demands of pregnancy and the challenges of managing multiple young children.

Conversely, previous research suggests a slight positive correlation between longevity and the number of children for men. But honestly, two is enough for me—thank you very much.


This article addresses the question posed by Amir Ali from Colchester: “Are my children aging me?”

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Reduce Your Risk of Death by 28%: Drink 5 Cups of This Hot Beverage Daily

Exploring the health benefits of hot drinks is a complex task, so brew yourself a cup while we delve into the science. Many studies have examined the health impacts of various hot beverages, but their findings can be difficult to compare due to the diversity of drinks and their effects.

Fortunately, some hot drinks are consistently linked to positive health outcomes, especially when consumed regularly.

Let’s kick things off with coffee. It ranks just behind water as one of the most popular beverages globally. Research shows that individuals who enjoy one or two cups of coffee daily may experience longer lifespans.

Furthermore, studies on Asian populations indicate that those consuming five cups of coffee a day have a 28% lower risk of all-cause mortality. The polyphenols in coffee are believed to contribute significantly to these health benefits.

These antioxidant-rich compounds combat inflammation and oxidative stress, which are linked to various diseases, including cardiovascular and neurodegenerative issues. While caffeine may have similar effects, individual responses can vary greatly.

Green tea provides numerous health benefits – Image courtesy of Getty Images

Next up is green tea, renowned for its health advantages. Research confirms that regular consumption can lower the risks of cancer, heart disease, and all-cause mortality.

The health-promoting properties are largely attributed to polyphenols, particularly epigallocatechin gallate (EGCG). A 2025 meta-analysis revealed that regular intake of EGCG may aid in cancer prevention.

If you’re a fan of black tea, you’re not alone; it’s prevalent in many Western cultures. While it may be less potent than coffee or green tea, black tea still offers notable health benefits.

Research indicates that black tea can help reduce blood pressure and LDL cholesterol, with regular consumption linked to slower cognitive decline in later life. A study utilizing UK Biobank data found that drinking two or more cups daily can decrease all-cause mortality risk by 9 to 13% here.

Importantly, the myth that adding milk to tea negates its health benefits has largely been debunked.

Let’s not forget about herbal teas, which often boast powerful polyphenols. Some have been shown to positively impact health as well.

For instance, peppermint tea may alleviate IBS symptoms, chamomile tea can enhance sleep quality, and hibiscus tea has been linked to lower blood pressure.

As for the traditional hot toddy, science has yet to thoroughly investigate its effectiveness against cold symptoms. Hot liquids can assist in clearing nasal passages, while honey may help suppress coughs, and the vitamin C from lemons may offer some benefits, making this drink feel “subjectively medicinal.”


This article addresses the question posed by Jodi Whitehead from Warmington: “What is the best hot drink for health?”

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Experts Reveal Shocking Findings: Do Cats Truly Help Humans in Need?

Meet Stubby, a remarkable stray Boston Terrier crossbreed who became a hero during World War I. Serving in the U.S. Army, Stubby bravely warned soldiers of gas attacks and helped locate the wounded.

Stubby served for 18 months and participated in 17 battles, making him one of the most decorated dogs in military history. He was awarded a gold medal, two Purple Hearts, and even received a promotion to sergeant.

While history is filled with stories of canine heroes, one must wonder: where are the feline counterparts?

The answer? They’re likely lounging comfortably on the radiator.

Cats have a reputation for being aloof and self-centered. To investigate their tendencies to help humans, researchers at Eötvös Loránd University in Budapest, Hungary conducted an intriguing experiment. In this study, they observed interactions between a cat, a dog, and a 2-year-old child.

The experiment was conducted in a home setting where unsuspecting participants watched human scientists hide various items. These included uninteresting dish scrubbers and engaging toys or food.

After hiding the objects, the scientist observed how the “witnesses” reacted—whether the child’s parents or the pet owners would seek assistance.

In a performance worthy of an Oscar, the caregiver expressed frustration, repeatedly saying, “Oh, I can’t find it! What should I do?” But would the witnesses lend a hand?

Regardless of the item, over 75% of dogs and toddlers pointed towards or fetched the hidden objects without any special training. They simply seemed eager to help.

Need a reliable helper? A dog is your best bet! – Image courtesy of Getty Images

Cats, however, rarely “help” unless their owners are directly involved. The only time a cat may show interest is when a treat or toy is missing, and even then, only 40% of them approach the hidden object.

This leads to an interesting question: Do cats not understand the problem, or do they simply choose not to care? If it’s the former, they may be unaware; if it’s the latter, they might be seen as selfish.

Personally, I lean towards the latter conclusion since my cat seems to know everything but chooses not to assist. Nonetheless, this behavior may not even be entirely her fault.

Unlike dogs, whose ancestors, the gray wolf, were inherently sociable, domestic cats evolved from solitary wild ancestors. Human intervention led to selective breeding for both physical and behavioral traits.

While we have successfully bred selflessness into dogs, a naturally social species, we have not replicated this trait in cats.

The takeaway? If you misplace your keys, don’t expect your cat to be your helper—ask your dog instead.


This article addresses the question: “How selfish are cats?” (submitted by Thomas King of Leicester).

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Newly Discovered Long-Necked Dinosaur Species Identified in Thailand

Paleontologists in northeastern Thailand have discovered a new species of mamenchisaurid sauropod dinosaur, revealing that this group of colossal dinosaurs, once believed to be primarily located in East Asia, also inhabited mainland Southeast Asia.



Reconstruction of a herd of Uragasaurus carasinensis in the Late Jurassic forests of Thailand, featuring rhymphorhynchoid pterosaurs and metricanthosaurid theropods. Image credit: Pakorn Chotchaiyaporn.

This newly identified dinosaur species, dubbed Uragasaurus carasinensis, thrived in what is now Thailand during the Late Jurassic period, approximately 150 to 145 million years ago.

Uragasaurus is part of the Mamenchisauridae family, renowned for their exceptionally long necks.

While Mamenchisauridae were common in China during the Middle to Late Jurassic, their presence in areas outside of China remains scarce.

“Mamenchisauridae represents a significant clade of non-neosauropod eusauropods from the Middle to Late Jurassic of East Asia,” said Dr. Apirut Nirupanapan of Mahasarakham University and his colleagues.

“Members of this clade are characterized by elongated cervical vertebrae with advanced pneumatic features, distinguishing them from other eusauropods, particularly in derived taxa.”

“Despite these traits evolving in various Cretaceous neosauropod lineages, including eupods and titanosaurs, they make interpreting the relationships within mamenchisaurids intricate, adding to the ongoing uncertainty regarding their phylogenetic placement among sauropods.”

The fossil record for mamenchisaurs is predominantly found in China, especially in the Sichuan Basin, where the Shaximi Formation provides an abundance of well-preserved Jurassic vertebrate fossils.

Uragasaurus carasinensis is primarily known from a single, remarkably preserved anterior dorsal vertebra, located just behind the dinosaur’s neck.

This specimen was unearthed from the Phu Noi Fossil Site within the Phu Kradung Formation, which is notable for yielding a rich diversity of Jurassic vertebrate fossils in Southeast Asia.

This vertebra, cataloged as PRC 460, was excavated alongside various other sauropod bone fragments, although these were not conclusively linked to the same individual.

Phylogenetic analysis places Uragasaurus carasinensis near the basal node of the mamenchisaurid family tree, indicating it may be one of the early diverging members of this group.

This discovery enriches the limited list of mamenchisaurids found outside of China, suggesting a broader geographic range and a more intricate evolutionary narrative than previously recognized.

The identification of Uragasaurus carasinensis marks “the first formally named mamenchisaurid from Thailand,” according to the paleontologists involved.

“This also extends the geographic reach of Mamenchisauridae into mainland Southeast Asia, further affirming that this clade was widespread across East Asia during the Late Jurassic,” they concluded.

“The presence of closely related taxa in China implies possible faunal connections throughout the East Asian continent during this era.”

“Comparative studies with more distantly located taxa highlight the complex paleobiogeographic dynamics of sauropods during the Jurassic-Cretaceous transition, but the limited fossil record complicates detailed reconstructions of dispersal pathways.”

“The phylogenetic positioning of Uragasaurus carasinensis at the base of Mamenchisauridae accentuates the morphological diversity present among the clade’s early divergent members.”

“Ongoing discoveries from the Phu Kradung Formation and other Jurassic sites in Southeast Asia could unveil critical insights into the initial evolutionary history and biogeographical dispersal of mamenchisaurid sauropods.”

The discovery of Uragasaurus carasinensis is detailed in a study published in the journal Scientific Reports.

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A. Nirupanapan et al. 2026. A new mamenchisaurid sauropod from the lower Phu Kradung Formation in the Upper Jurassic of northeastern Thailand. Scientific Reports 16, 21205; doi: 10.1038/s41598-026-49822-3

Source: www.sci.news

Revived Human Retinas Show Light Response 10 Hours Post-Mortem

Preserving Retinal Function Outside the Body: A Breakthrough for Transplantation

Michael Lutz/Alamy

Recent studies show that human eyes can function outside the body for up to 10 hours after death, doubling previous records. By supplying blood and oxygen to donor eyes, researchers have ensured that the eyes can still respond to light, maintaining structural integrity and health.

“This study marks a significant advance toward the potential for whole-eye transplantation,” states Thomas Johnson of Johns Hopkins University in Baltimore, Maryland, who was not involved in the research. “Achieving a mild response outside the body is a remarkable milestone.”

Over 1 million people in the UK experience blindness or low vision. Irreversible eye conditions like age-related macular degeneration impact the retina, the light-sensitive tissue at the back of the eye.

Progress has been made in transplantation techniques. Corneal transplants enhance vision for patients with damaged corneas; however, treating the retina remains challenging due to its connection to the central nervous system.

In 2023, a partial face transplant and a full eye transplant were performed, but vision restoration was not achieved—a significant hurdle. The retina is vulnerable to degeneration due to oxygen deprivation, known as ischemia. Johnson explains, “Even brief periods of ischemia may cause permanent damage to light-sensitive neurons and circuits.”

Eimear Byrne from Barcelona University of Science and Technology led researchers who aimed to mitigate this damage by replicating the conditions donor eyes encounter in the body.

They developed a system that channels blood through a flexible tube into the ophthalmic artery, nourishing the eye and surrounding tissues. The Eyes-in-Care-Box utilizes sensors to deliver oxygenated solution, ensuring optimal pressure and flow.

The researchers tested their technique on six donors, where one eye was perfused, while the other was not. Results indicated that the perfused eyes maintained retinal structure and cellular health for up to 24 hours, contrasted with rapid deterioration in the non-perfused eyes.

After perfusing 36 additional eyes, they found that 15 exhibited electrical light responses akin to those in living humans—lasting up to 10 hours post-mortem, double the previous average of five hours. Although other scientists made similar discoveries in 2022, the reasons for the limited response in 21 eyes remain unclear.

A significant challenge persists: regenerating the severed fibers of the optic nerve to connect with the brain’s visual center. Johnson highlights, “Without this regeneration, the donor eye cannot relay vision to the recipient’s brain.”

While this new research does not resolve that issue, maintaining healthy eye metabolism after death may facilitate future strategies for vision restoration and enhance donor eyes’ resilience to ischemic damage.

Many organizations are investigating potential interventions to promote optic nerve regrowth. “Now is the perfect time to integrate these promising strategies for whole-eye transplantation,” Johnson expresses.

Byrne’s team suggests the Eyes-in-Care box could also allow for testing vision-related treatments on human eyes instead of alternative animal models. “This technology has significant potential for advancing the understanding of biology and pathology, as well as developing new in vitro models for testing drugs and other treatments,” Johnson asserts. “These results will be directly applicable to human diseases and biology.”

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Source: www.newscientist.com

Demonstrating How Special Relativity Distorts Chemical Bonds: New Findings Revealed

Electrons in heavy atoms like bismuth

In some heavy atoms like bismuth (crystalline form), electrons move at relativistic speeds

Image Credit: savva_25/Shutterstock

Albert Einstein’s special theory of relativity has reshaped our understanding of chemical bonds within molecules, a phenomenon now observed for the first time by researchers.

Special relativity elucidates how moving at near-light speeds affects the experience of space and time, extending even to electrons within certain heavy atoms. These high-speed electrons behave similarly to those found in particle accelerators and spacecraft.

Wang Laisheng and colleagues at Brown University in Rhode Island undertook a groundbreaking study that challenges conventional views on chemical bonding in charged molecules composed of bismuth and carbon.

In the studied molecule, bismuth and carbon are interconnected via three bonds. Researchers anticipated one bond would be of the “sigma” type while the other two would be “pi” bonds. The distinction between these bond types is rooted in the quantum nature of electrons, which are not solid masses but are instead “smeared” over a space, determining bond formation based on their spatial overlap.

During experiments, Wang and his team mapped electron distributions across the molecule, analyzing its bonding configuration. Contrary to expectations, they found the electron distributions indicative of two unique combinations of sigma and pi bonding shapes. “These bonds exhibit characteristics inconsistent with traditional definitions,” Wang notes. “They defy conventional Sigma and Pi classifications.”

His collaborator, Kirk Peterson, from Washington State University, calculated that this unusual mix arises from strong electromagnetic interactions, where electrons near the bismuth nucleus exhibit relativistic speeds—a phenomenon never before captured experimentally.

“Studying heavy elements presents unique challenges; quality experimental data is scarce,” Peterson mentions. “It’s a rare opportunity to compare advanced theoretical models with empirical data in such a fascinating way.”

Wang emphasized that key to their success was cooling the molecules before observation, significantly reducing noise and excitation, leading to more accurate results.

“The methodology employed is the pinnacle of both experimental and theoretical research,” states Pekka Pyykkö from the University of Helsinki, Finland.

This relativistic restructuring of bismuth-carbon bonding could revolutionize how organobismuth compounds are utilized in chemical reactions. Indeed, recent studies from the Max Planck Institute for Coal Research in Germany demonstrate that relativistic effects enhance the catalytic properties of this heavy metal in chemical processes.

Professor Wang and his team aim to replicate this experiment using a similar element from the periodic table to investigate when special relativity disrupts traditional chemical bond structures.

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Source: www.newscientist.com

Exploring the Chemistry of Giant Exoplanet Beta Pictoris b: Insights from Astronomers

Using the advanced GRAVITY+ instrument at ESO’s Very Large Telescope Interferometer (VLTI), astronomers have measured the carbon isotope ratio in the atmosphere of the young exoplanet Beta Pictoris b, offering groundbreaking insights into the formation of giant planets.

Artist’s impression of a gas giant exoplanet within the disk of Pictoris Beta. Image credit: L. Calçada / ESO.

Beta Pictoris b, discovered in November 2008 via ESO’s Very Large Telescope, is a gas giant resembling Jupiter but with a mass between 9 and 13 times greater.

This exoplanet orbits its host star Pictoris Beta at a distance eight times greater than that between the Earth and the Sun.

The host star is also accompanied by at least two planets and a circumstellar disk filled with gas and dust, which could ultimately evolve into an icy body torus similar to the Kuiper belt in our solar system.

In this recent research, Antonia von Stauffenberg, a Ph.D. student at the Max Planck Institute for Astronomy, and her team sought to explore the origins and possible atmospheric variability of Beta Pictoris b.

They employed the cutting-edge GRAVITY+ instrument for their observations.

“We utilized a method developed years ago to determine the planetary formation location within its disk,” the researchers detailed.

“By analyzing the relative abundance of two carbon isotopes (C) trapped in carbon monoxide (CO) gas of Beta Pictoris b’s atmosphere, we can deduce whether the planet formed inside or outside the disk’s icy regions.”

“As radiation from the host star heats the disk from its center, it directly correlates to how far from the star the planet formed.”

The temperature boundary at which gas condenses into ice is commonly referred to as the snow line.

“Isotopes contain the same number of positively charged protons but differ in neutrons, such as carbon-12 (12C) and carbon-13 (13C).

“Despite their differing masses, their chemical properties are similar.”

“In cosmic contexts, carbon often exists in combinations with oxygen, appearing as 12CO and 13CO molecules.”

“Interestingly, past assessments of the 12CO/13CO diagnostic yield were conducted using the original GRAVITY setup, resulting in relatively low ratios.”

“We suspected that the original GRAVITY instrumentation was insufficient for resolving key signals in this dataset and advised caution in interpreting the results.”

“Following the rationale above, preliminary findings suggest Beta Pictoris b likely formed in the outer disk, beyond the snowline, by accumulating CO ice instead of gaseous CO.”

“Yet, positioned approximately 10 astronomical units from its star, Beta Pictoris b orbits within the disk’s transition zone between the host star and the snowline, where gas predominately comprises CO.”

“If these results hold true, they imply that Beta Pictoris b may have migrated across the disk during its formation.”

Astronomers also detected subtle variations in magnetic flux from the planet over time.

“While statistically insignificant, the primary variation closely corresponds to the planet’s rotation period of approximately 8.7 hours,” the researchers noted.

“If confirmed, this could indicate the presence of clouds or chemical processes in Beta Pictoris b’s atmosphere, but further sensitive observations are essential.”

“The proposed restoration plan for the gas giant’s birthplace necessitates new, precise measurements of the 12CO/13CO abundance, clearly indicating a position in the warmer inner zones of its natal planet-forming disk.”

“Moreover, this ratio aligns well with values typically found in the interstellar medium extending across our solar system and the Milky Way.”

“The majority of the 12 young gas giant planets assessed for CO ratios displayed comparable values.”

“This consistency may actually signal challenges, as carbon isotope abundances appear to provide minimal diagnostic value when determining a planet’s location relative to its host star.”

“The probable explanation is that fluctuations during planet formation are too subtle to be captured effectively by our proposed methodology.”

“This suggests that 12CO/13CO ratios may not provide specific insights into individual planet-forming environments.”

“Consequently, we are likely overlooking essential physical factors influencing the chemistry of CO ice in planet-forming disks.”

“Hence, the 12CO/13CO ratio may not shed substantial light on the distinction between gaseous environments and regions abundant in CO ice.”

“At this moment, this wide-orbiting gas giant remains reluctant to disclose its origins.”

“We require innovative tools capable of differentiating between planet formation scenarios, and GRAVITY+ could significantly contribute to identifying and evaluating these scenarios.”

The findings are published in today’s issue of Astronomy and Astrophysics.

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A. von Stauffenberg et al. 2026. 13CO and potential variations in β Pictoris b using GRAVITY+. A&A 711, L2; doi: 10.1051/0004-6361/202660275

Source: www.sci.news

Revolutionizing Thermodynamics: A 200-Year Old Mathematics Rewritten

close-up of a marble illustrating thermodynamics

Examining thermodynamics through the lens of marbles and shadows offers fresh insights into this established theory.

Priscila Zambotto/Getty Images

The theory of thermodynamics has significantly advanced our understanding of various devices, particularly engines, for over two centuries. However, its mathematical framework has often been criticized for lacking precision. Currently, researchers are reinforcing the foundation of this seminal theory, incorporating modern mathematical approaches to describe quantum fields more effectively.

Thermodynamics remains one of the most pertinent branches of physics in daily life. Its evolution was propelled by engineers aiming to enhance the performance of heat engines—basic devices exemplified by ubiquitous technologies such as car engines and refrigerators.

Despite its success, thermodynamics has historically struggled with mathematical rigor. Brian Roberts from the London School of Economics has embarked on a mission to reconstruct thermodynamic principles using innovative mathematical concepts rooted in geometry and quantum field theory—an approach that deviates significantly from traditional teachings.

The cornerstone of Roberts’ new methodology is “gauge theory,” which addresses characteristics of entities that are typically unobservable or unmanageable.

A straightforward example featuring a marble rolling on a surface serves to clarify this theory. Although each marble appears identical, their centers conceal different colors.


Gauge theory delineates a mathematical terrain defined by the numbers governing the marbles’ movements—referred to as “observable” space—and an alternative domain, known as “bundle” space, which contains hidden information about the internal colors of each marble.

These two mathematical realms are profoundly interconnected; the observable space serves as a projection of the unobservable bundle space. According to Roberts, this concept parallels the phenomenon of illuminating an object: even if the object itself remains concealed, its properties can still be inferred by observing its projection—its shadow.

Roberts proposes that this framework may be instrumental in examining thermodynamics since the discipline also encompasses both visible and hidden quantities.

“Thermodynamics has two levels,” he explains. “Some levels are more accessible, allowing for work extraction—akin to movable pistons in an engine. Others are less overt, like the heat generated or lost within a system, which cannot be manipulated directly.” He identifies this as a concealed contribution to energy.

This distinction is not emphasized in conventional thermodynamics where “work” and “heat” are treated equivalently, aiding in the total energy calculations of an object. However, for Roberts, recognizing the concealed aspects of thermodynamic energy permits aligning thermodynamics with gauge theory structures inside bundle space.

This innovative perspective offers a pathway to harness foundational principles established in other physics domains relating to gauge theory, ultimately leading to a comprehensive grasp of thermodynamics.

For instance, crucial thermodynamic concepts such as temperature and entropy can be articulated through specific projections from bundle space to observable space. Roberts contends that this geometric definition of entropy is more intuitive, facilitating its application across diverse systems, from engines to black holes.

Furthermore, gauge structures have connections to experiments in the quantum theory of electromagnetic fields. Roberts anticipates that a similar interplay may emerge within thermodynamics. Preliminary investigations involving specific molecular junctions hint at a thermodynamic version of the Aharonov-Bohm effect—an iconic experiment in which charged particles seem to encounter a hidden magnetic field.

Roberts presented this work at the Basics of Physics conference held on June 16 in Irvine, California.

Lucas Cerelli, a professor at the Federal University of Goiás in Brazil, expressed admiration for Roberts’ concept, emphasizing its compatibility with evolving efforts to decode thermodynamics in the quantum framework as a gauge theory.

With the application of gauge theory to quantum phenomena, thermodynamics presents even greater complexities. Cerelli cautions, “I have reservations about quantum thermodynamics, given the multitude of definitions regarding heat and work. Establishing a rigorous mathematical framework could yield a consistent and unique understanding.”

Cerelli and his team have been pursuing this by leveraging gauge theory, reportedly achieving success in reconciling some outcomes of standard quantum thermodynamics.

A significant challenge ahead for both quantum and classical thermodynamics will be integrating these with Albert Einstein’s special theory of relativity. Fortunately, Cerelli asserts, gauge mathematics may offer advantages over traditional methodologies.

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Source: www.newscientist.com

Impact of Cold Shock in Warming Oceans on Large Marine Animals | Sciworthy

In March 2021, the remains of over 260 marine animals from 81 distinct species were found washed ashore in South Africa. Scientists are investigating whether this alarming occurrence was linked to substantial temperature drops caused by a process known as coastal upwelling, where deep, cold water rises to the surface, leading to rapid cooling.

While climate change is warming ocean temperatures, it is also intensifying coastal upwelling, potentially disrupting marine megafauna. Researchers focused on two rapidly warming boundary currents—the Agulhas Current in southern Africa and the East Australian Current in eastern Australia—to evaluate how these changes in upwelling zones could lead to more frequent and severe cold shock events affecting species like sharks.

To understand the events that occurred in March 2021, the scientists analyzed satellite data on sea surface temperatures and collected hourly temperature records from loggers to track subsurface temperature variations. They discovered that coastal sea temperatures plummeted by up to 7°C (12°F), dropping from 24°C (75°F) to below 17°C (63°F) within a mere 48 hours. Simultaneously, subsurface temperatures decreased more than 9°C (16°F) over 24 hours.

Bull sharks, which experience physiological stress at temperatures below 19°C (66°F), were likely pushed beyond their thermal tolerance limit during this cold shock event, potentially by over 5°C (10°F).

The research team equipped 66 bull sharks—41 in the Agulhas Current and 25 in the East Australian Current—with acoustic and satellite transmitters to monitor their responses in relation to lower thermal limits. Acoustic tags track shark movements via underwater receivers, while satellite tags log temperature and depth data for extended periods.

Data analysis revealed significant findings: prolonged low temperatures hindered sharks’ physiological recovery, resulting in some migrating to shallower depths in search of warmth, though cooling can occur too swiftly for them to adapt.

Wind records from the South African Weather Service indicated that strong easterly winds, which triggered upwelling, preceded the 2021 event. The correlation of cooling temperatures, fierce winds, and marine animal deaths suggests that coastal upwelling was a critical factor in this die-off.

Examining 41 years of sea surface temperature data, researchers employed mathematical models to assess the frequency and intensity of these rapid cooling incidents. Their results demonstrated that such events can persist longer than the usual one to three days, with the March 2021 incident lasting a full seven days.

The frequency and intensity of these cold shock events have notably escalated in recent decades, leading to more extreme temperature reductions than typically seen in just 24 hours. Their conclusions indicate that the 2021 marine die-off is indicative of a broader trend where warm ocean conditions allow species migration, yet intensified upwelling can suddenly expose marine life to life-threatening cold events, a phenomenon termed climate bait and switch.

The researchers concluded that climate change is likely reinforcing coastal upwelling processes, pushing marine megafauna beyond their thermal limits, despite initial warming benefits. These findings shed light on a crucial aspect of climate change, emphasizing how temperature fluctuations and upwelling can directly affect species survival. The implications of this research could prove vital for predicting future responses of marine ecosystems to changing ocean conditions.


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Source: sciworthy.com

New Injection Reduces Chromosomal Errors in Older Women’s Eggs by 50%

Cells displaying signals for excess chromosomes

Department of Clinical Cytogenetics, Addenbrookes Hospital/Scientific Photo Library

Issues with human eggs, such as aneuploidy (having too many or too few chromosomes), can lead to miscarriages, unsuccessful IVF treatments, or genetic conditions like Down syndrome. Recent research has unveiled a potential solution: a single injection into the egg can significantly mitigate these issues, promising to enhance IVF success rates for women of advanced age.

“This discovery could revolutionize the field,” says Marcos Iuri Ruth Kullman Niro Franz, Ph.D., from Reproductive Medicine in Porto Alegre, Brazil, who was not involved in the study. “This could be the first instance of demonstrating the feasibility of correcting the primary issues behind IVF failures.”

During meiosis, egg and sperm cells typically lose exactly half of their genetic material. This ensures that, upon fertilization, a complete genome is formed. However, irregularities may occur, resulting in sperm or egg cells having an incorrect amount of genetic material, known as aneuploidy.

Aneuploidy affects approximately 10-25% of eggs and its prevalence increases with age, starting from the early 30s. “By the late 30s, over 65% of eggs are aneuploid,” mentions Agata Zielinska from the German biotech company Ovo Labs, during her presentation at the European Society of Human Reproduction and Embryology conference in London on July 6th.

Clinicians may screen IVF embryos for aneuploidy in couples at high risk of miscarriage or IVF failure. However, for many couples, genetic conditions—such as those leading to Down syndrome—can only be identified through blood tests and ultrasounds in the first trimester. Until now, there were limited methods to prevent aneuploidy.

Recent findings by Zielinska and her team indicate that levels of a protein called Shugosin-1 are significantly diminished in older mice and humans compared to their younger counterparts. Shugoshin-1 plays a crucial role during meiosis, ensuring that chromosome pairs line up correctly in immature egg cells, maintaining the molecular integrity that holds each chromosome pair together.

Upon fertilization, these paired chromosomes separate, with one half forming a mature egg cell while the other is discarded. In older eggs, the integrity of this glue deteriorates, resulting in improper chromosome separation before fertilization and leading to aneuploidy.

To investigate the potential for Shugoshin-1 supplementation to preserve chromosome integrity and reduce aneuploidy, researchers collected 111 spare immature eggs from over 30 women aged 22 to 43 undergoing IVF or egg storage.

The study involved injecting mRNA coding for Shugoshin-1 into selected eggs, while others from the same donor remained untreated. Results showed that 53% of untreated eggs exhibited premature chromosome separation, compared to only 29% of those treated. For women over 35, the untreated egg aneuploidy rate averaged 65%, while the treated eggs averaged only 44%. Though the reduction wasn’t statistically significant due to sample size, researchers remain optimistic.

Further experiments showed that this treatment avoided aneuploidy in mouse eggs, allowing them to fertilize and produce healthy offspring without side effects in either mouse or human studies. “We achieved live births in mice, indicating that this approach does not disrupt any phase of embryonic development nor compromise the health of the pups,” Zielinska informed the conference attendees.

Current research focuses on testing the effects of Shugoshin-1 in humans, necessitating adjustments to traditional IVF methods to utilize immature instead of mature eggs—a change that is expected to be smoothly implemented, according to Zielinska.

She envisions that the treatment, dubbed “EmbryoProtect,” will provide a cost-effective option to enhance IVF success rates for older women. “The goal is to make this treatment affordable compared to a full IVF cycle,” Zielinska states. “By significantly boosting IVF success rates, we aim to reduce the number of attempts needed to conceive, especially for women over 35, who typically have lower success rates.”

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Source: www.newscientist.com

Exploring the Surprising Physics Behind Lugworm Waste: Fascinating Insights!

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The Physics of Defecation

News Editor Alexandra Thompson of the University of Amsterdam explains the intriguing origin of the poop emoji — Hoe de poep-emoji zijn vorm kreeg, which translates to “how the poop emoji got its shape.”

For those unfamiliar with emojis beyond smileys, the poop emoji stands out. It’s typically depicted as a conical mound resembling coiled feces. Emojipedia describes it in a relatable manner, comparing it to “soft serve ice cream.” However, during this heat wave, that imagery takes on a rather unsavory twist.

If you watched the 2017 animated film The Emoji Movie, you might recall the poop emoji as a notable character, voiced by none other than Patrick Stewart, known for his Stentorian delivery.

A recent study published in Nature Communications in April explores the physics behind lugworm feces. The authors describe how various animals, including earthworms and some mammals, produce coiled poop, much like the emoji itself. This shape emerges from “the coiling of a ‘rope’ of fluid falling onto a hard surface,” influenced by gravity, inertia, and viscosity.

Remarkably, lugworms defy conventional defecation by ejecting waste upward. They inhabit U-shaped burrows on sandy beaches within the intertidal zone, positioning their anus just below the burrow entrance. At low tide, they expel waste upward, leaving marks on the sandy flat.

Despite their unconventional method, lugworms still produce coiled poop. They accomplish this against the odds of “buckling instability,” indicating their evolutionary mechanism is effective.

Unlike animals that defecate downwards, where the drop height is vital, the coil’s radius is determined solely by material properties and rope shape. The researchers elaborated on this mathematics, noting their model can also explain the curling behavior of other substances, such as rice noodles and spaghetti. The elegance of these findings demonstrates the universe’s remarkable design.

Bayeux Tapestry Queue

The art of queuing and optimizing it for fairness and efficiency presents intriguing mathematical challenges. For example, when a train runs late, should it receive priority—possibly delaying others—or wait? Determining the fairest approach for passengers while maximizing the rail system’s efficiency remains a complex question.

History enthusiast and Managing Editor Kelsey Hayes recently faced a virtual queue while attempting to access early ticket sales for the British Museum’s Bayeux Tapestry exhibit, scheduled to run for the first time in the UK in 900 years. Kelsey, a museum member, received an email in early June promoting pre-sales two weeks before the general public.

The email urged her to “register to reserve” a spot, leading Kelsey to comment on the seemingly pointless exercise. However, she soon encountered an online queue with “over 1,400 people and a 20-minute wait.”

This exercise was a tactic to ensure members organized their login details to prevent registration or password issues later. If you know Kelsey or Feedback, waiting 20 minutes to reset passwords is not typical.

Two weeks later, when member reservations became available, Kelsey reported, “It took us four hours in line to secure a time slot.” She would be furious to discover that likely the Bayeux Tapestry wasn’t crafted in a bayou, nor is it technically a tapestry.

Not My Bag

Feedback often pokes fun at hubris, so we’re excited to present news of a bag made from a patented substance known as “T-Rex Leather.” However, it didn’t sell at the Paris auction in June. Initially expected to fetch over $500,000, the bid ultimately fell short.

This unique bag was likely produced using preserved collagen from a Tyrannosaurus rex femur, but here’s the catch: true leather is derived from the animal’s skin, and this “T-Rex Leather” did not come from a Tyrannosaurus skin.

Collagen is the primary protein found in skin, but recreating Tyrannosaurus skin entails an intact Tyrannosaurus genome to grow skin cells. Unfortunately, the oldest preserved DNA is only 2 million years old, while Tyrannosaurus went extinct 66 million years ago.

Without the DNA or a complete genome, growing Tyrannosaurus skin cells is impossible. While we can speculate this bag’s failure to sell may relate to its questionable provenance, we can’t overlook the likelihood that its outdated color played a significant role.

Have a story for Feedback?

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Source: www.newscientist.com

The Top 4 Must-Watch Sci-Fi Series of 2026: A Comprehensive Guide

Anastasia's fame in Dark Forest takes its toll as Irina follows a decisive lead. Anna Maxwell Martin stars in 'Star City' now streaming on Apple TV.

Anna Maxwell Martin delivers a standout performance as Raskova in ‘Star City’

Image Credit: Apple TV

In the realm of sci-fi television during the first half of 2026, the landscape presents a mixed bag of offerings. While some series shine brightly, others struggle to make a lasting impression. A standout among them is Star City, a gripping alternate-history thriller that delves into the Soviet space program, featuring characters evading KGB interrogators and navigating harrowing space perils.

Other shows this season offered great moments but came with their own challenges. Take, for instance, Fallout, which faced an uneven start in the new year after three episodes. Set against the backdrop of a nuclear nightmare, the series follows privileged individuals seeking refuge in underground “vaults” as others struggle to survive the harsh conditions above ground.

Fans are thrilled to see the heroes return in Fallout Season 1! From the vault dweller Lucy to the mechanic-enhanced soldier Max, and the irradiated gunslinger known as the Ghoul, drama unfolds. Max grapples with his allegiances to the Brotherhood of Steel while Lucy, despite her past experiences in Season 1, ends up wasting her time with dynamics that don’t seem to evolve.

The Ghoul, however, is a bright spot in Fallout Season 2, showcasing impressive character depth and charisma. His backstory is rich, with hints of Westerns woven into his life narrative, making his character unforgettable as he navigates pre-nuclear disaster intrigues.

Another series, Paradise, had the monumental task of living up to its acclaimed first season, where significant twists shook the foundations of power and governance post-civilization collapse. Despite this, its second season manages to explore new elements, including a subplot surrounding a long-lost wife and the tensions of surviving in a dystopian world.


In Star City, real-life rocket engineer Sergei Korolev survives, enabling the Soviet Union to eclipse the United States in the moon landing.

Overall, Paradise yields mixed results, adding a ghoul character and a complex villain-turned-Secret Service agent storyline that may feel cheesy but keeps viewers engaged. It creatively uses various sci-fi tropes better than many current series.

For All Mankind presents a fascinating alternate reality where the US and USSR are in a fierce race to colonize space. Despite being set in 2012, the show imagines characters who live on Mars and attempt to access Titan to uncover extraterrestrial life.

The narrative centers on the Baldwin family, primarily Ed, a disgruntled Apollo-era astronaut, navigating the complexities of life on Mars. However, the new season disappointingly skims over the pivotal conflict between Mars and Earth, which many had anticipated.

Fortunately, For All Mankind expands its universe through a spin-off from Star City. The divergence in timelines begins with Sergei Korolev’s survival, allowing a different trajectory for the Soviet space program. This spin-off features Anastasia Belikova, the first female cosmonaut on the moon, as she grapples with political tension from the KGB surrounding her fellow cosmonauts, particularly with the chilling performance by Anna Maxwell Martin.

For anyone seeking a compelling sci-fi series to watch in 2026, For All Mankind comes highly recommended.

Topics:

  • Science Fiction/
  • Television Series

Source: www.newscientist.com

Insects of 500 Million Years Ago: Why They Preferred Turning Right

Fossil of Spriggina floundersi

The right-turned Spriggina floundersi insect is preserved as a left-turned fossil.

Photo Credit: Scott Evans/AMNH

The 555-million-year-old worm, known as Spriggina floundersi, showcases a tendency to turn to the right, potentially providing evidence of the earliest known example of handedness.

Although these ancient organisms lacked limbs, which would prevent them from being classified as left- or right-handed in the conventional sense, the development of a directional preference implies a complex nervous system.

This behavioral trait still exists among free-roaming, nomadic species today. However, until this groundbreaking discovery, researchers believed handedness did not emerge until the Cambrian period, around 541 million years ago.

Scott Evans, a researcher at the American Museum of Natural History in New York, and his colleagues examined 100 fossilized specimens of the flatworm-like Spriggina floundersi, collected over decades in South Australia.

These ancient organisms thrived during the Ediacaran period, when multicellular life forms first became abundant. This era preceded the Cambrian explosion, a time of remarkable diversification among animal life, characterized by the appearance of various new species.

Fossils of Spriggina suggest that these creatures inhabited shallow seas approximately 500 million years ago, foraging for food on or near the ocean floor, moving in a characteristic side-to-side motion.

“We have analyzed about 50 specimens of Spriggina. The evidence indicates these fossils display a definitive curve,” said Evans. Interestingly, twice as many fossils were found curving to the left as those to the right, suggesting the original organism predominantly curved to the right due to the mirror-like preservation of its shapes.

“This finding appears statistically significant and aligns with current biologist studies on handedness across species,” explains Evans. Some specimens exhibit multiple bends on both sides, indicating their ability to bend in either direction, which is logical for avoiding circular motion while navigating.

While the majority seem to indicate right-handedness, it remains challenging to discern absolute handedness distinctions. “Imagine counting 100 people waving with one hand. You can determine that more are waving with their right hand, but you cannot definitively conclude who is right- or left-handed,” Evans elaborates.

These discoveries underscore that many fundamental traits shared among numerous modern animals, including locomotion, bilateral symmetry, and handedness, first emerged during the Ediacaran period, according to Evans.

During the Cambrian period, these early organisms built upon these fundamental traits, evolving greater complexity, such as the development of legs for more efficient movement, and gradually becoming more similar to familiar animal groups today. “This is noteworthy because it reinforces that the Cambrian, while crucial in the history of animal evolution, was not a sudden appearance of life but rather a continuation and refinement of structures established back in the Ediacaran,” Evans explains.

“The observation of handedness and its relation to functional asymmetries in the fossil record offers deep insights into the evolutionary history of these behaviors,” concludes Russell Bicknell at Flinders University in Adelaide, Australia.

Topics:

Source: www.newscientist.com

Study Reveals Night Owls Eat Less at Breakfast and More at Midnight: Key Insights on Eating Habits

New research reveals that night owls may face a higher risk of obesity and slower metabolism due to their tendency to consume a significant portion of daily calories late at night. This study focused on women of European and Pacific descent living in New Zealand.



Research by van der Merwe et al. examined the link between chronotype and dietary habits, meal timing, body composition, and metabolic indicators in healthy women of European and Pacific descent in New Zealand. Image credit: RitaE.

Humans generally organize their sleep and wake patterns within a 24-hour cycle based on personal preferences.

These preferences are known as chronotypes, impacting not only sleep and wake times but also meal timing.

Morning people typically wake and sleep several hours earlier than night owls.

Understanding your chronotype can provide insight into your eating habits.

“Are you an early riser or a night owl? An early riser is classified as a morning chronotype, while a night owl prefers later bedtimes and wake-up times,” says Professor Roseanne Kruger from Massey University and Griffith University.

“Chronotype has significant effects on our food preferences, behaviors, and metabolic health.”

The study monitored 287 healthy women from European and Pacific Islander backgrounds in New Zealand.

Participants completed extensive questionnaires on sleep patterns, maintained a 5-day food diary, underwent body composition scans, and provided fasting blood samples for metabolic analysis.

Results showed over half the participants were classified as intermediate chronotypes, 34% as night owls, and 12% as morning owls.

The average BMI for night owls was 31.4 compared to 26.1 for morning and intermediate chronotypes.

Night owls displayed higher total body fat and a higher android-to-gynoid fat ratio, which is linked to abdominal fat accumulation.

Although total daily food intake was similar, meal timings were significantly different.

Morning types consumed most of their energy, protein, carbohydrates, and fats before 10 a.m., whereas night owls ingested more nutrients after 8 p.m.

This trend was most pronounced among night owls with higher body fat percentages.

Night owls tended to eat less in the morning but compensated by consuming more energy and fats during late-night hours.

Compared to morning types, night owls had lower intakes of various nutrients essential for a healthy diet, including fiber, vitamins A and E, folate, calcium, magnesium, potassium, and iodine.

While night owls consumed less caffeine and alcohol, their overall energy and carbohydrate intake was slightly higher.

Metabolic health assessments indicated these dietary habits were linked to poorer health outcomes.

Evening chronotypes exhibited elevated levels of triglycerides, insulin, glycated hemoglobin, and leptin, alongside lower levels of HDL (the “good” cholesterol) and the appetite-regulating hormone ghrelin.

Correlation analysis further suggested that increased energy intake during the morning was associated with higher HDL cholesterol and lower insulin and glycated hemoglobin levels.

Conversely, higher energy consumption in the evening correlated with elevated triglyceride, insulin, and glycated hemoglobin levels.

“The total energy intake was consistent across both morning and night owls,” the researchers noted.

“However, night owls ate significantly less between 3 a.m. and 9:59 a.m. but consumed more between 8 p.m. and 2:59 a.m., which was the reverse for morning owls.”

“This night-time eating pattern correlates with increased body fat percentage, abdominal fat, and elevated blood sugar and lipid levels.”

“Eating during night hours, when the body is naturally inclined to fast, contributes to food storage rather than consumption, heightening the risk of obesity and associated health issues.”

For more details, refer to the study published on July 7, 2026, in Frontiers in Nutrition.

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Karlian van der Merwe et al. 2026. Associations Between Chronotype and Dietary Intake, Meal Timing, Body Composition, and Metabolic Biomarkers. Frontiers in Nutrition 13; doi: 10.3389/fnut.2026.1862060.

Source: www.sci.news

Webb Telescope Uncovers the Hidden Heart of Centaur A: A Deep Dive into Cosmic Mysteries

Celebrating four years of groundbreaking research, the NASA/ESA/CSA James Webb Space Telescope has successfully navigated the dense dust of the colossal galaxy Centaurus A. This exploration has unveiled its vibrant core, intricate dust lanes, and millions of stars that illuminate the remnants of an ancient galactic collision.



A stunning ground image of Centaurus A from ESO (top left) providing context for the near-infrared and mid-infrared perspectives captured by Webb. Image credit: ESO / NASA / ESA / CSA / STScI / A. Pagan, STScI.

Centaurus A, a massive galaxy located in the southern constellation of Centaurus, is also recognized as NGC 5128, LEDA 46957, ESO 270-9, and Caldwell 7. This galaxy stands out as one of the brightest celestial objects in the Southern Hemisphere’s night sky.

Discovered on April 29, 1826, by Scottish astronomer James Dunlop, Centaurus A is positioned approximately 13 million light-years away, making it the closest active galactic nucleus to Earth.

Astronomers believe that Centaurus A originated as an elliptical galaxy that underwent a dramatic collision with a smaller spiral galaxy, resulting in the distinctive shape observed today.

“At the heart of Centaurus A lies a supermassive black hole that actively consumes surrounding matter,” stated the Webb astronomers. “This black hole simultaneously emits powerful jets, releasing vast energy and shaping the galaxy’s structure.”

“Centaurus A bears the marks of a tumultuous history, including a significant collision with another galaxy that occurred approximately 2 billion years ago,” they continued. “The aftermath is still evident in its unique architecture and ongoing star formation.”

Previous visible-light observations using the NASA/ESA Hubble Space Telescope were unable to penetrate the dusty region at the center of Centaurus A. However, NASA’s retired Spitzer Space Telescope managed to reveal large-scale structures in the infrared without distinguishing individual stars.

Now, the Webb Space Telescope provides unparalleled clarity and depth, bringing to light the inner workings of the galaxy, star by star.

“Webb’s mid-infrared vision showcases the galaxy’s intricate dust structure, displaying complex patterns that surprise and intrigue astronomers,” researchers noted. “A distorted parallelogram-like band traverses the galaxy’s center, with fragments of matter extending outward like cosmic clouds.”

The prominent ‘S’-shaped feature captured in Webb’s MIRI (Medium Infrared Instrument) image is particularly unusual, prompting questions that require further investigation: What birthed this shape? How does the black hole influence it? Is it impacted by the merger-induced star formation?

Many red spots in MIRI images represent dusty stars or stellar nurseries, where aging stars are ejecting material or new stars are forming. This dust serves as the essential building block for future generations of stars and planets, playing a critical role in the life cycle of galaxies.

With its high resolution, Webb now permits scientists to examine Centaurus A star by star, even within its previously obscured central region.

“The ‘grainy’ appearance in images from Webb, particularly evident in the combined MIRI and NIRCam (Near-Infrared Camera) views, illustrates a densely packed region of individual stars that together narrate the galaxy’s history,” researchers explained. “Webb’s observations of Centaurus A transform it into a case of galactic archaeology.”

“Each star discovered contributes to reconstructing a timeline of significant events: the formation of old stars, periods of reduced activity, explosive star formation during collisions, and stars emerging from gas stirred up in the aftermath,” they concluded. “Collectively, these findings chart the evolution of galaxies.”

Source: www.sci.news

Discovering Shared Lifestyles: Neanderthals and Homo Sapiens Coexisted in an Ancient Turkish Cave

Recent discoveries in the Üçağızlı II cave along the stunning Mediterranean coast of Turkey reveal comprehensive records suggesting that the cultural transition from Neanderthals to modern humans was far more fluid than previously recognized.

A group of Neanderthals in a cave. Image credit: Tyler B. Tretsven.

“During the mid-to-late Pleistocene, the Levant served as a crucial corridor for the dispersal of our species, homo sapiens, between Africa and Eurasia,” stated Kyoto University archaeologist Naoki Morimoto and colleagues.

“Evidence of early human settlement in the Levant and sporadic expansions into Eurasia is supported by hominid fossils sourced from Misliya Cave (approximately 180,000 years ago), Kafze and Sukfur Cave (around 100,000 years ago), and Apidima Cave (about 200,000 years ago).

“Various models have been proposed concerning events outside Africa; a prevailing hypothesis suggests multiple dispersals between 130,000 and 80,000 years ago were followed by significant migrations out of Africa approximately 60,000 years ago, which ultimately led to the genetic evolution of modern human populations.”

“There is a substantial lack of fossil data from the period corresponding to the large-scale migration out of Africa, which leaves many questions unanswered regarding homo sapiens.”

“Key questions focus on the tempo, mode, and behavioral context of interactions between homo sapiens and homo neanderthalensis.”

“The Levant remains one of the few regions where both modern humans and Neanderthals coexisted.”

In the Üçağızlı II cave, located in the northern tip of the Levant near the Orontes River, archaeologists uncovered an intricate series of artifacts, including teeth, stone tools, animal remains, and shells, dating from approximately 77,000 to 47,000 years ago.

Teeth analysis indicated that the oldest layer (77,000 to 59,000 years ago) contained Neanderthal dentition, while the upper layer (59,000 to 47,000 years ago) held early human remains attributed to homo sapiens.

What fascinated archaeologists was not merely the change in species but the persistence of behavioral patterns.

Both Neanderthals and modern humans crafted remarkably similar stone tools influenced by the Middle Paleolithic, or Mousterian, tradition, employed similar hunting methods for wild goats, fallow deer, roe deer, and wild boar, and collected the same marine snail shells, Columbella rustica, likely utilized for decoration rather than sustenance.

Some of these shells displayed indications of intentional perforations or color alterations from heat exposure, implying that both species regarded shells as symbolic or decorative items rather than food sources.

Carved stone artifacts and other manuports (objects brought to the site but not utilized) were also present throughout the site, revealing shared traditions across species.

“Our findings illustrate a profound level of cultural interchange,” emphasized Dr. Morimoto.

“These two distinct yet closely related human groups were not only adapted to the same environment but likely shared symbolic values.”

The researchers assert that their results differ markedly from patterns seen at other archaeological sites, such as France’s Mandolin Cave, where distinct layers show alternating settlements of modern humans and Neanderthals.

In contrast, Üçağızlı II cave exhibits cultural continuity that transcends biological change, indicating ongoing close interactions between the two species in this region.

“The findings from Üçağızlı II cave fill significant gaps in global archaeological and paleontological records and have the potential to transform our understanding of how early human species interacted, communicated, and shared their environments,” the scientists concluded.

Discover the full findings in the upcoming issue of Proceedings of the National Academy of Sciences.

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Ismail Baykara and colleagues. 2026. Long-term cultural continuity from Neanderthals to modern humans in Üçağızlı II cave in the northern Levant. PNAS 123 (29): e2609061123; doi: 10.1073/pnas.2609061123

Source: www.sci.news

Euclid Unveils the Oldest Quasar Ever Discovered in History

Astronomers utilizing the ESA’s Euclid Space Telescope have made a groundbreaking discovery of 31 ancient quasars dating back to when the universe was only 670 million to 800 million years old. Among these celestial objects, EUCL J172902.75+641018.1 has set a remarkable record as the most distant quasar ever identified.



This collage showcases 15 of the 31 newly discovered quasars by ESA’s Euclid Space Telescope. EUCL J172902.75+641018.1 and EUCL J125308.55+705432.3 are featured in the first row, first and second from the left, respectively. Image credit: ESA / Euclid / Euclid Consortium / NASA / Euclid Science Ground Segment / Antoine Basset, CNES.

Quasars are among the universe’s brightest and most energetic entities, fueled by supermassive black holes at the centers of galaxies.

Dr. Damin Yang, an astronomer from Leiden University, noted, “These early quasars trace back to the universe’s infancy. By locating and examining them, we can delve deeper into one of astrophysics’ greatest mysteries: how these colossal systems formed and evolved so rapidly.”

He further stated, “Previously known early quasars were merely the tip of the iceberg—rare, luminous outliers that were easier to detect.”

“We hadn’t identified a sufficient number of quasars from this early epoch to study them collectively,” Dr. Yang explained.

The recent findings by Euclid have changed the narrative, capturing a significant portion of the ancient quasar population, beyond just the bright exceptions.

This discovery introduces 12 new quasars with redshifts greater than 7, corresponding to the universe’s first 770 million years.

The oldest quasars from this batch, EUCL J172902.75+641018.1 and EUCL J125308.55+705432.3, feature redshifts of 7.77 and 7.69, respectively, establishing new records for the oldest known quasars.

Both quasars are located over 13 billion light-years away and appeared in the universe’s first 670 million years.

ESA researcher Dr. Antonio La Marca commented, “This finding more than doubles our knowledge of extremely ancient quasars.”

“It took astronomers over a decade to discover the initial 10 quasars with redshifts above 7, but Euclid has already surpassed that within a year.”

“The Euclid research team is conducting the first true examination of the quasar population from the universe’s early days.”

This represents a significant milestone toward gaining a more fundamental understanding of these enigmatic objects.

For more in-depth information, a research paper detailing the discovery has been published in this week’s edition of Astronomy and Astrophysics.

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D. Yang et al. 2026. Euclid: 31 new quasars discovered with 6.6 < z < 7.8. A&A 711, A104; doi: 10.1051/0004-6361/202658883

Source: www.sci.news

Hayabusa 2 Delivers Breathtaking Close-Up Images of Asteroid Bird Ship During Flight

On July 5, 2026, the Japan Aerospace Exploration Agency’s (JAXA) Hayabusa2 spacecraft achieved a groundbreaking milestone by completing its first asteroid encounter during its extended mission. The spacecraft passed near a fascinating two-lobed asteroid close to Earth, known as Torifune. It successfully captured and transmitted stunning close-up visual and thermal images.



This image of the near-Earth asteroid Tryphne was taken on July 5, 2026, with the ONC-T instrument aboard JAXA’s Hayabusa2 spacecraft. Image credit: JAXA / University of Tokyo / Chiba Institute of Technology / Tokyo University of Science / AIST / Paris Observatory / IAC.

Launched in 2014, JAXA’s Hayabusa2 was initially designed to explore the carbon-rich near-Earth asteroid Ryugu, which holds primordial material from the solar system’s formation. Upon arrival in 2018, the spacecraft spent over a year mapping Ryugu and deployed a small “hopping” lander along with the German-made MASCOT lander for sample collection.

In April 2019, Hayabusa2 initiated a daring experiment by firing a copper projectile into Ryugu, creating an artificial crater. Researchers aimed to gather samples shielded from billions of years of space weathering.

The spacecraft later descended to collect freshly excavated material, which, when analyzed after the return capsule landed in Australia in 2020, revealed water-bearing minerals, organic molecules, and compounds that provide insights into the early solar system’s chemical makeup, dating back 4.6 billion years.

In a remarkable twist, unlike many missions that conclude after returning their samples, Hayabusa2 continued its journey.

After releasing its sample capsule, the spacecraft resumed its engines for a long-term mission to visit the near-Earth asteroid 1998 KY26 in 2031.

On its path, Hayabusa2 performed a high-speed flyby of the small asteroid Tryphne, also referred to as 2001 CC21, scheduled for 2026.



This thermal image of the asteroid Tryphne was captured on July 5, 2026, by the TIR instrument aboard JAXA’s Hayabusa 2 spacecraft. Image credit: JAXA / Maebashi Institute of Technology / Chiba Institute of Technology / University of Aizu / Hokkaido University of Education / National Institute of Advanced Industrial Science and Technology.

The flyby occurred at 6:30 PM on July 5, Japan time, with Hayabusa2 approaching the asteroid at an impressive speed of approximately 5 kilometers per second.

The spacecraft utilized its Optical Navigation Camera (ONC-T) to capture visible-light images, revealing Torifune as an asteroid with dual elongated lobes reminiscent of a snowman.

“Observations with NIRS3 (near-infrared spectrometer), TIR (thermal infrared imager), and LIDAR (light detection and ranging) instruments were conducted an hour before the closest approach,” mission members reported.

“Data collection continued right up until the nearest point of approach, but no observations were made post-encounter,” they added.

“Currently, only a portion of the data collected by scientific instruments has been transmitted to Earth. The remaining data will be shared during upcoming operations.”

Source: www.sci.news

Why Occam’s Razor is No Longer Effective: Tips to Refine Your Truth-Seeking Journey

Explore the latest science news, technology, health, and environmental developments on our website and magazine.

The ancient Greek astronomer Ptolemy conceived that the planets and the sun revolved around the Earth, based on the limited knowledge of his era. Every observation that contradicted this notion required a slight adjustment to the theory until Nicolaus Copernicus radically redefined the understanding of our solar system. He proposed that all planets orbit the sun, igniting a scientific revolution that transformed our comprehension of the universe.

Throughout history, simpler theories have often evolved into accepted knowledge. Special relativity emerged victoriously over the concept of the luminous ether, and continental drift gained clarity through shared fossils found across distant continents, rather than imagined land bridges. This aligns with Ockham’s razor, attributed to the 14th-century monk William of Ockham, advocating for the simplest explanation that aligns with the facts.

But what if scientific advancement doesn’t always adhere to simplicity? What if starting with complexity, instead, broadens our understanding and reveals concealed structures?

Cognitive scientist and philosopher Marina Dubova from the Santa Fe Institute in New Mexico suggests that Ockham’s razor is merely one of several guidelines that may cloud our quest for genuine reality. Through computer simulations and microscopic explorations, Dubova applies principles of psychology and cognition to challenge existing scientific paradigms, revealing the fluidity of our assumptions about truth-seeking.

As we advance toward a future where automation in science is likely, these insights could prove instrumental in shaping the development of “AI scientists.” New Scientist reached out to Dubova to discuss the hazards of integrating antiquated concepts into contemporary science, how maximizing real-world interactions can enhance learning speed, and the fundamental implications this holds for the essence of science itself.

Thomas Luton: What is the Occam’s Razor Principle, and how do scientists implement it?

Marina Dubova: Occam’s Razor inherently promotes simplicity in explanations. Students across diverse scientific fields, myself included, are often instructed to commence with the most straightforward theory. If discrepancies arise in the data, additional variables can be introduced, but the initial approach should always be the simplest. Scientists apply this in varied contexts, favoring explanations with minimal assumptions or fewer causative mechanisms. Sometimes, less adaptable explanations are preferred for making specific predictions.

Is this simplistic approach unique to science, or do we all tend to do this?

Evidence suggests that when prompted to clarify various phenomena, humans gravitate towards broad, simplistic explanations. Research conducted by psychologist Tania Lombroso at Princeton University revealed that individuals often prefer explanations invoking fewer causes that adequately account for most data. For instance, participants asked to diagnose an alien showcasing two symptoms preferred a singular ailment encompassing both symptoms, rather than suggesting two different diseases for each symptom, even when the latter presented as more likely.

Is there empirical evidence supporting the notion that Occam’s Razor promotes scientific progress?

My research examined these theoretical concepts using computational models. In this study, an AI agent formed a foundational representation based on limited datasets, generating theories with minimal variables, while others constructed more intricate frameworks. For example, an agent with access to three significant variables might create an explanation with a thousand. Surprisingly, agents prioritizing complexity sometimes performed predictions as well as—or even better than—those favoring simplicity, challenging many entrenched assumptions held by scientists regarding our understanding of the world.

You implied that there are multiple theories that can mislead us, not just Occam’s Razor?

Indeed, another common guideline suggests that experiments should arise from existent theories. In studying extraterrestrial life or human memory phenomena, researchers often formulate a theory to conduct theory-based experiments. An example is Arthur Stanley Eddington’s 1919 solar eclipse expedition, specifically tailored to verify general relativity’s prediction of starlight bending due to the Sun’s gravity, forcing a choice between conflicting hypotheses of Einstein and Newton.

Images of a solar eclipse taken in 1919 confirmed Albert Einstein’s theory of general relativity, showcasing stars near the Sun appearing slightly displaced due to gravitational lensing.

Royal Astronomical Society Scientific Photo Library

Is the pursuit of reason in science misguided?

Similar computational models create agents that resolve discrepancies using targeted experiments. Another approach involves testing theories for validation, which can introduce confirmation bias. Further exploratory strategies include randomly selecting novel experiments.

Which theoretical approach yielded the most effective theories?

Agents employing exploratory strategies, whether randomness or novelty-driven, produced the most accurate theories about the underlying truth. Our surprising findings prompted additional experiments to revalidate our results.

Have you witnessed similar behaviors in actual scientists?

Yes. We engaged neuroscientists to utilize brain imaging and lesions in deciphering the underlying causal structures of a model brain. Although they succeeded in their task, some showed difficulty in adapting their preconceived notions. For instance, when regions governing multiple functions were evident, some neuroscientists insisted on the existence of distinct areas for each ability, reflecting the tendency to maintain rigid hypotheses even in the face of contrary evidence.

What insights should scientists draw from your research?

Current scientific institutions often inhibit inquiry. It’s crucial to acknowledge that our theories can shape decision-making and limit our exploration of reality. This range of theories—from general relativity to chemical structures—guides and enhances our progress but can also obstruct our understanding of objective reality.

Are scientific revolutions sufficient for overcoming erroneous concepts?

Though scientific revolutions yield significant breakthroughs, will it take countless years to overturn established notions? A more exploratory approach may accelerate discoveries.

Can you provide examples of how simplistic theories led to misconceptions?

Consider advancements in neuroscience, which has shifted to viewing the brain as an integrated network rather than a collection of isolated regions tasked with specific functions. A similar shift in genetics challenges the notion of single-gene traits, revealing a more complex interplay of multiple genes and environmental influences in establishing traits.

One might argue that simpler initial ideas have at least served as a starting point for understanding complex phenomena.

Given our cognitive limitations, such simplifications are somewhat inevitable. However, AI can initiate explorations into higher-dimensional complexities that were previously inconceivable.

This phenomenon is evident in statistical learning, a field that analyzes data interactions. A noteworthy discovery termed “double descent of generalization” illustrates that larger models might have unexpected performance advantages. Historically, it was believed that minimizing environmental details was essential for optimal model performance. Recent findings indicate a reduction in error rates as models grow more complex, suggesting that they excel in predicting unseen data by emphasizing broader representations over mere memorization.

Does this influence the training of AI scientists?

We need robust discussions on which components of the scientific method merit preservation and which need reevaluation. Was our previous scientific approach our best effort given cognitive constraints? Understanding this is critical as we transition toward automating scientific processes; without it, established biases and blind spots may scale up.

What do your findings indicate about the nature of science?

The goal of science is to comprehend reality and expand our knowledge of the world. However, numerous perspectives must be employed to adequately investigate phenomena. Philosopher Haseok Chan from Cambridge University describes this as maximizing our contact with reality. Scientific inquiry often resembles tactile exploration rather than purely visual observation. Engaging with various elements of reality allows us to extract unique insights and understanding.

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Using Seawater for Cloud Seeding: A Solution to Prevent Super El Niño Events

Cloud Brightening and Climate Engineering

Innovative cloud brightening using ship exhaust particles could be a climate change solution

NASA Earth Observatory

Short-term geoengineering strategies, like enhancing cloud brightness over the eastern Pacific, have the potential to mitigate El Niño’s impacts and safeguard the global economy, potentially saving trillions of dollars. However, these interventions may disrupt natural cycles, leading to uneven consequences.

El Niño is a climate phenomenon where weakened easterly winds allow warm water from the western Pacific to flow eastward, raising global temperatures significantly and impacting economic growth.

Currently, a strong El Niño, possibly a “super” El Niño, is observed in the eastern Pacific. However, climate models indicate that future warming might be mitigated through ocean cloud brightening, a geoengineering method.

This method involves dispersing tiny seawater droplets into the atmosphere beneath low-level stratocumulus clouds. As the number of droplets increases, the clouds become whiter, reflecting more sunlight back into space.

If the cloud brightness is enhanced in the Niño 3.4 region, it could disrupt the feedback loop that sustains El Niño. This leads to a decrease in sea surface temperatures, reinforcing trade winds that push warm water back to the western Pacific, resulting in colder water surfacing in the eastern Pacific.

“By brightening ocean clouds, we can effectively prevent the cascading effects from escalating,” states Jessica Wang, a researcher from the University of California, San Diego. “We’re beginning to reverse the cycle.”

Wang’s team drew inspiration from Australia’s catastrophic 2019-2020 bushfires, followed by La Niña, a climate pattern that cools global temperatures. Their research proposes that smoke particles from these fires inadvertently enhanced cloud brightness, cooling the eastern Pacific and prolonging the “triple bottom” La Niña from 2020 for three consecutive winters.

The study assessed the impact of cloud brightness on past Super El Niño events (1997-1998 and 2015-2016) and found that increasing seawater spray for nine months could reduce the temperature rise in the Niño 3.4 region from over 2 degrees Celsius to slightly above 1 degree Celsius. This would effectively shorten the El Niño event significantly.

However, implementing this hypothetical cloud-brightening mission would require an estimated 2,400 ships spraying seawater—a scale beyond current nozzle technology. Nonetheless, this intervention could downgrade a super El Niño to a moderate one.

Despite starting only in June, as El Niño conditions began to develop, Wang expressed surprise at the impact observed.

Meanwhile, Matt Collins, a researcher from the University of Exeter, cautioned that such results may not be applicable in real-world scenarios. Warming oceans typically lead to the dissipation of lower clouds, intensifying warming through feedback loops.

“Models suggesting stronger cloud feedback necessitate higher aerosol injection,” he warned. “The experiment may have reached its operational capacity.”

Wang acknowledged potential unintended consequences, as simulations only predict impacts for up to two years. In both scenarios assessed, La Niña approached promptly after El Niño, with the 2015-2016 cycle producing stronger cooling periods, due in part to diminished rainfall during strong La Niña events, which contributed to widespread starvation.

Nevertheless, she affirmed the approach merits further exploration. Unlike long-term geoengineering strategies aimed at cooling the Earth, short-term measures can be paused without incurring drastic temperature spikes.

“This study paves the way for innovative geoengineering research focused on climate change and El Niño mitigation,” Wang emphasized. “It holds significant potential as it avoids long-term risks.”

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Enhancing Fertility: How Softening the Ovaries Can Improve Reproductive Health

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Light micrograph illustrating a cross-section of a follicle containing an immature egg. The immature egg (orange) is enveloped by a fluid-filled cavity (light pink) and granulosa cells (dark pink), which supply nutrients and hormones.

Steve Gschmeisner/Science Photo Library

Recent studies indicate that by softening ovarian tissue, it may be possible to enhance fertility rates. A novel drug aimed at reducing organ hardness more than doubled conception rates and increased litter sizes five-fold in older, subfertile rats. While human trials are necessary, these findings spark optimism that similar interventions could aid older women in conception.

Female fertility significantly declines in the mid-30s. However, in regions like England and Wales, many delay childbirth, often until later in life. The quantity and quality of a woman’s immature eggs decrease with age, supported by evidence that ovarian stiffness increases over time, affecting egg development and quality negatively.

In a study led by Wang Shixuan, researchers at Huazhong University of Science and Technology analyzed protein levels in the ovaries of women aged 18 to 28, 35 to 42, and 47 to 52, all with a history of gynecological cancer that did not impact the ovaries after removal.

The findings revealed an increase in a protein called interleukin-11 in aging ovaries. This protein activates fibroblasts, connective tissue cells that produce collagen, contributing to ovarian stiffness. Learn more about the causes of ovarian stiffness.

The research team also genetically modified mice to resist interleukin-11, resulting in reduced ovarian stiffness and increased ovulation compared to unmodified mice.

Subsequently, the researchers tested an experimental drug to inhibit interleukin-11 production by silencing its gene, administering it to 36-week-old mice, analogous to humans in their late 30s or early 40s, twice weekly for a month.

Results demonstrated a 36% decrease in ovarian firmness compared to untreated controls. Conception rates increased from 25% to 50%, and average litter sizes grew from three to five calves. Similarly, in aged rats, conception rates improved from 20% to 50%, with litter sizes increasing fivefold from one to five.

Francesca Duncan from Northwestern University in Illinois remarks that this intervention may yield comparable results in premenopausal women, noting that interleukin-11 levels also rise with age in human ovaries. However, she cautions that findings are based on women with a cancer history, leaving questions about its effect on individuals without such health concerns.

Additional studies are needed, as indicated by Barbara Vanderheiden of the University of Ottawa, who suggests potential broader benefits for women’s health. “Preserving fertility and extending ovarian function could mitigate menopause effects like osteoporosis and heightened heart disease risks,” she notes.

The goal is to deliver the drug directly to the ovaries ahead of human trials. So far, no adverse effects have been observed in mice and rats. Yet, Duncan warns of risks since interleukin-11 is present in various human tissues. “Considering the pivotal role of ovarian egg cells in future generations, drug safety protocols targeting the ovaries must be exceptionally stringent,” she states.

Questions remain about the duration required for the drug to enhance reproductive outcomes. “While reducing ovarian stiffness could be feasible,” Vanderheiden states, “short-term treatments show limited data on their long-term positive or negative impacts.”

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Link Between Certain Moisturizers and Hair Loss: What Scientists Don’t Understand

Some dermatologists are exploring the connection between skin care products and rising rates of frontal fibrosing alopecia (FFA)—a condition characterized by hair loss at the front of the scalp, predominantly affecting postmenopausal women.

A recent 2023 study suggests that FFA may be linked to facial products containing moisturizers, particularly sunscreens, based on data compiled from nine different studies.

Cases of FFA have surged in the last two decades, especially in Europe and the United States, sparking further investigation into environmental factors alongside genetic and hormonal influences.

One hypothesis is that certain ingredients in leave-on products may penetrate the skin surrounding hair follicles, inciting an immune response that can gradually damage hair follicles over time.

However, proving this link remains challenging due to the methodologies of existing studies. For instance, two UK studies found that in 2016 and 2017, researchers analyzed small cohorts of individuals with FFA. In the first study, 100 women suffering from FFA utilized more sunscreen compared to 105 women without hair loss.

Similarly, in the second study, 17 men with FFA reported using sunscreen (and sunscreen-containing moisturizers) significantly more than 73 men without symptoms.

Factors influencing hair loss can be interconnected – Image courtesy of Getty Images

While these findings may appear compelling, Thai researchers approached the topic with caution. In a 2021 survey, they examined 250 Asian women, of which 50 had FFA and 100 experienced significant hair loss or thinning. It was noted that individuals with hair loss employed more moisturizers and sunscreen compared to the control group.

Nonetheless, this kind of research can only indicate correlations rather than establish causation.

Another possibility is that individuals who first observe hair thinning become more focused on their appearance and may increase their usage of skin care products, rather than those products being the source of the issue.

Furthermore, sun exposure itself could also play a role, with increased sunscreen use potentially reflecting greater time spent outdoors.

A more effective way to determine the relationship would involve randomly assigning participants without hair loss to either use specific skin care products or avoid them entirely. However, is such testing ethical if these products contribute to hair loss?

For now, the majority of experts concur that the evidence is insufficient to warrant the avoidance of sunscreen, which is vital for skin cancer prevention.

The British Association of Dermatologists indicates that while the exact cause of FFA remains unknown, possible contributing factors include genetics, immune responses, and hormonal changes.


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Success of In Vitro Fertilization: Advancements in Lambs Born from Highly Immature Eggs

IVF Sheep Experiment

Groundbreaking IVF Study Results in Five Healthy Lambs

Photo by Laurence Winram

An innovative approach to in vitro fertilization (IVF) has successfully led to the birth of a healthy lamb. This method involves maturing immature eggs in a lab setting and marks a significant milestone in reproductive technology for large animals. The implications of this study may increase the availability and success rates of IVF treatments for women facing infertility issues, particularly those with ovaries compromised by cancer therapies.

“This is a monumental advancement,” says Stein Christensen, a professor at Copenhagen University Hospital who was not part of the research.

This study builds on over three decades of previous research, which first showed the potential of IVF in mice, as outlined in this live birth study. “Reproductive processes in sheep are more comparable to humans than in mice,” explains Dr. Manjushree Boob, whose clinic in Maharashtra, India, was not involved in the research.

Conventional IVF requires a series of daily hormone injections for one to two weeks that stimulate immature eggs to mature in the ovaries. Typically, only about 6 to 8 out of 10 mature eggs fertilize successfully, leading to implantation challenges, with only a 20% success rate for live births.

Due to these low success rates, attention is turning to the potential of utilizing immature eggs. Women are born with hundreds of thousands of eggs, but this count declines throughout their lives. Each menstrual cycle sees the maturation of a single follicle that releases an egg during ovulation.

In recent research, Helen Picton and her team at the University of Leeds collected numerous immature follicles from sheep. They utilized a blend of reproductive hormones and growth factors, such as follicle-stimulating hormone, to promote growth and maturation, achieving approximately 60% maturation of the eggs.

About 30% of these matured eggs were successfully fertilized, leading to embryos implanted in 18 sheep. This resulted in the birth of a female lamb in early 2024, along with four additional lambs earlier this year. Notably, the female lamb has also given birth to two offspring this year. Mr. Picton shared these findings at the European Society of Human Reproduction and Embryology conference in London on July 7th.

The outcomes of this research suggest that this novel technique could significantly enhance egg availability for fertilization and improve conception rates, as noted by Christensen. However, it may need to complement standard IVF practices, which could complicate the process and lead to higher costs.

Picton pointed out that while this approach shows promise, it is unlikely to become standard practice due to the invasive nature of follicle retrieval, which is more complicated than collecting mature eggs through conventional IVF.

Nonetheless, this method could greatly assist women whose ovaries have been adversely affected by cancer treatments. While doctors typically remove and freeze ovarian tissue to preserve fertility before treatment, this process carries risks, including the possibility of reintroducing cancer cells during transplantation. Picton emphasized that retrieving immature eggs poses fewer risks, as cancer primarily affects surrounding tissues.

Before widespread use, further research is necessary to determine if human eggs matured using this method are viable for fertilization. Christensen stated that upcoming studies are expected in the next few years, and, if they yield positive results, small-scale trials could aim for healthy live births. However, obtaining ethical approval may take 5 to 10 years. It is crucial that such studies demonstrate that benefits clearly outweigh any associated risks for future parents and their children.

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Why Erwin Schrödinger’s 1944 Classic ‘What is Life?’ Remains a Timeless Science Essential

New Scientist - Science news and insights by expert journalists covering developments in science, technology, health, and the environment.

What is Life? Is It Still Impactful?

Erwin Schrödinger, a pioneer of modern quantum science, articulated in his 1944 book that scientists should contribute to their fields as a form of nobility. In What Is Life?, he invites readers to delve into the world of living organisms, moving away from the focus on inanimate atoms that brought him fame. Over approximately 90 pages, he transitions from one area of expertise to another, producing an influential work in popular science during the 20th century.

Based on a series of lectures delivered in Dublin in 1943, What Is Life? maintains a conversational tone while occasionally reflecting on deeper philosophical questions. However, Schrödinger’s core dilemma is framed within the parameters of physics: “How can phenomena occurring within living organisms be explained through physics and chemistry?”

To explore this, Schrödinger employs a physicist’s rationale. What Is Life? begins with a discussion on the minuscule and abundant building blocks of life and how they adhere to statistical physics principles. He clarifies that while physicists can derive averages from large collections, individual behavior remains unpredictable.

The laws of physics indicate that systems trend towards disorder and exhibit fluctuations. Yet, living organisms display remarkable order, akin to the intricate mechanisms of a clock. Schrödinger is captivated, noting that even minimal “genetic material” enables consistent reproduction and trait transmission, a phenomenon that poses questions in his analysis.

Written before the full understanding of DNA’s structure, Schrödinger contemplates the composition of this genetic material. Drawing from his studies on mutation inheritance and linking it to quantum concepts, he reflects on the possibilities of this genetic solidity and its quantum stability. His principal claim is that living entities require “negative entropy” to sustain order, necessitating a continual draw of organization from their environment. Schrödinger asserts that fully unraveling this enigma might demand new physics laws.

Published in 1944, What Is Life? garnered significant attention, inspiring numerous physicists to pivot towards biology. It frequently features in “best of” lists, appealing to general readers, yet chemists and biologists were less enthusiastic.

Nobel Prize laureate Max Perutz examined the extensive contemporary work that Schrödinger might have referenced for his inquiries. He noted that Schrödinger’s confusion about the regeneration of small genetic materials during cell division could have been mitigated with a better understanding of the roles of involved enzymes. Perutz also criticized the concept of negative entropy.

Recently, author Philip Ball indicated that Schrödinger might have gained deeper insight by engaging with ideas connecting entropy and information—such as Leo Szilard’s 1929 solution to Maxwell’s Demon paradox, where rising disorder is seemingly countered.

Despite valid criticisms, as a physicist, I find myself more aligned with Schrödinger’s perspective than those entrenched in modern genetics. In conversations with biophysicists, echoes of What Is Life? resound. Just last year, a researcher shared his ambitions to establish new physical laws addressing living systems. Another scholar sensibly noted, “If you’re in equilibrium, you’re dead,” capturing Schrödinger’s sentiments from the 1940s.

In 2021, biophysicist Rob Phillips at the California Institute of Technology asserted that What Is Life? should be viewed as “a manifesto on the frontiers of physics, signifying that every new phenomenon demands innovative concepts and ultimately results in new laws.” I concur. Although Schrödinger’s grasp of biology and chemistry was incomplete, his physicist’s intuition remains relevant.

Are physicists best equipped to decipher the precise mechanisms that distinguish the living from inanimate matter? It’s a philosophical question that future research may illuminate. This duality of excitement and frustration was poignantly addressed by Schrödinger over 80 years ago, grappling with the same challenges we face today.

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How Histamine Affects Allergies and Boosts Memory Function

Polarized light micrograph of histamine crystals

Polarized light micrograph of histamine crystals

Alfred Pasieka/Science Photo Library

Individuals suffering from hay fever understand that histamine stimulates an immune response in various parts of the body. Interestingly, recent research shows that histamine plays a distinct role in the brain, where elevated levels can enhance memory accuracy by approximately 10%.

“We believe it enhances something known as excitement associated with novelty,” explains
Michael Colwell from Oxford University. “It affects how alert we are when encountering new stimuli in our environment.”

There’s substantial evidence that the brain contains receptors specifically for histamine. “These receptors are concentrated around areas crucial for learning and memory,” Colwell notes. Animal studies further support the correlation between
histamine and learning.

This link may clarify some side effects associated with early antihistamines, as elaborated in
academic research. “Many older antihistamines penetrated the brain,” Colwell explains. “Consequently, they appeared to impair memory, which is a common issue for long-term users.”

But what happens when histamine levels rise in the brain? Previously, there was no method to examine this in humans until Colwell and his team discovered that an existing narcolepsy medication, pitolisant, could achieve this. It binds to histamine-3 receptors, raising histamine levels throughout the brain.


In their study, the team enlisted 60 volunteers, administering pitolisant to half of them, while the others received a placebo. MRI scans revealed that subjects treated with pitolisant exhibited enhanced connectivity between the histamine-producing regions and the hippocampus, an essential area for memory. These volunteers were also 11% more accurate in recalling learned information during scanning.

However, Colwell cautions against using pitolisant as a “smart drug.” “It significantly impacts sleep, and I suspect that prolonged use might ultimately worsen memory.”

Roland Seifert
from Hannover Medical University in Germany suggests the rarity of pitolisant misuse as a cognitive enhancer, given the difficulty in accessing it. He emphasizes that findings in animal models likely reflect similar trends in humans, signaling potential for targeting histamine receptors in treating neurological disorders.

Those using pitolisant for genetic conditions such as narcolepsy or Prader-Willi syndrome have reported increased alertness.
Holger Stark, who collaborated on the drug’s development at Heinrich-Heine University in Düsseldorf, states, “In cases where cognitive function suffers due to illness, pitolisant has shown promise in reversing cognitive decline and enhancing alertness. However, in most scenarios, the goal was to normalize function rather than to exceed typical cognitive levels.”

The dual effects of histamine in the body illustrate evolution’s resourcefulness. “This reflects how economical the human body can be,” Colwell concludes.

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How Extreme Heat Impacts Your Body and Effective Strategies for Relief

Passengers on the London Underground during the heatwave on June 26th

Guy Bell / Alamy

The June heatwave that gripped Europe shattered records and followed a similarly intense heatwave just weeks earlier in May. A new wave of extreme heat is now underway, with temperatures in the UK soaring to 34°C (93°F).

To gain insights into the repercussions of this extreme weather, I visited the Environmental Extremes Laboratory at the University of Brighton, situated adjacent to Brighton & Hove Albion Football Club’s stadium. This institute collaborates with athletes to evaluate their fitness under extreme conditions. Within just 10 minutes inside the heat chamber, I realized that the increasing frequency and intensity of heatwaves means that many, like myself, are unprepared.

The heat chamber is designed to replicate the high temperatures, humidity, and oxygen levels found in environments like Mexico City’s elevated World Cup stadium or urban areas experiencing heatwaves.

“Heatwaves are a permanent reality, and we must proactively prepare individuals for frequent bouts of extreme heat, not just as isolated incidents,” emphasized lab director Neil Maxwell during my visit.

Inside the chamber, with a temperature set to 35°C (95°F) and a humidity of 50%, reminiscent of London’s conditions during the June heatwave, my vital signs were monitored through a fingertip pulse meter for heart rate and oxygen levels, with skin temperature measured via an infrared thermometer. I was also prompted to assess my perceived warmth and activity level.


Upon entering the chamber, the heat engulfed me, creating an immediate sensation of anxiety about what awaited me for the sake of science.

To mimic outdoor activity, I was instructed to walk on a treadmill set to a 1% incline. Despite my efforts, high humidity hindered the cooling process, making even this moderate exertion arduous.

After only 5 minutes, my skin temperature climbed from 33°C to over 36°C. Maxwell explained that this was my body’s attempt to regulate temperature by directing warm blood to the skin.

Reporter Alec Lune in the heat chamber at the University of Brighton’s Environmental Extremes Laboratory.

Bill Norton

My heart rate surged from 72 beats per minute to 81 bpm as my body strained to compensate for the loss of hydration, making my blood thicker and my heart work harder.

After an exhausting 10 minutes, I felt fatigue set in, with my heart rate peaking at 95 bpm. Dizziness washed over me as Maxwell guided me off the treadmill and into a chair.

“You’re not acclimatized to the heat,” he remarked, noting that even those in good health could face risks.

Maxwell handed me a strawberry popsicle, its delightful flavor not only refreshing but serving to cool my body from within. He then instructed me to soak my hands in chilled water, targeting the blood vessels in areas rich with arteries and capillaries for quicker cooling.

“This method helps us reduce core body temperature swiftly,” Maxwell explained.

Even something as simple as a cold shower can be effective. If the water is too cold, blood vessels may constrict; however, research by Maxwell and his team indicates that only a small segment of the UK population actively takes preventative measures against heat exposure. He noted my own oversight of coming without a water bottle, even on a scorching day.

For long-term solutions, Maxwell emphasizes the importance of improving heat tolerance through strategies such as aerobic exercises like jogging, which enhances the heart’s efficiency in regulating blood flow to the skin. The lab housed a sauna tent to illustrate that regular sauna sessions can rapidly expand blood vessels and promote increased sweating. Furthermore, these sessions help to maintain electrolyte levels while reducing sweat salt concentration.

“The focus must shift; heat is often viewed as detrimental. However, we need to acknowledge that controlled heat exposure may have therapeutic benefits,” Maxwell advised.

Upon returning home, I was met with a headache, a heightened sense of heat, and significant thirst, reinforcing my intent to incorporate regular sauna visits into my routine. As for jogging, I’ll strive to stay consistent.

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China’s Tianwen-2 Spacecraft Successfully Reaches Earth’s Quasi-Moon After 1 Billion Kilometer Journey

On July 2, 2026, the Tenbun-2 spacecraft made a remarkable approach, coming within just 20 km (12.4 miles) of the near-Earth asteroid 2016 HO3. As one of the seven identified Earth quasi-satellites, this celestial body has sparked a science campaign in preparation for the final sample return attempt.



Tianwen-2 captured this image of 2016 HO3 on July 2, 2026, from roughly 20 km away. Image credit: CNSA.

Discovered on April 27, 2016, by the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) at Haleakala Observatory in Hawaii, 2016 HO3—also known as Kamo’olewa (Hawaiian for “vibrating celestial fragment”)—is approximately 30 meters (98 feet) in diameter and has a one-year orbital period.

“Of all known near-Earth asteroids, 2016 HO3 is a unique co-orbital object with Earth,” stated Dr. Rongqiao Zhang and colleagues from the Lunar Exploration and Space Engineering Center.

“As a quasi-Earth satellite, its orbital period closely matches Earth’s, enabling low-energy transfers and maintaining a stable distance of approximately 0.1-0.3 astronomical units (AU) from Earth. This allows for optimal tracking, control, and communication.”

“Its unusual orbital characteristics, mysterious origin, and poorly understood physical properties make this satellite a strong candidate for addressing fundamental questions about the origins of Earth’s quasi-satellites and the dynamic evolution of their orbits.”

“Orbital dynamics models suggest that the current quasi-satellite state began around 100 years ago and is expected to continue for about 300 years,” researchers noted.

Currently, 2016 HO3 holds the title of the closest quasi-satellite to Earth (minimum distance 0.2 AU, with stable dynamics not exceeding 0.3 AU) and is the most stable target of its kind.

Possible origins for this asteroid include local formation, gravitational capture, or ejection from the lunar surface due to a collision with another celestial body.

2016 HO3 serves as the primary target for the China National Space Administration (CNSA) Tianwen-2 small celestial body exploration mission.

“Launched from the Xichang Satellite Launch Center on May 29, 2025, using a Long March 3B/G2 rocket, Tianwen-2 represents China’s commitment to planetary exploration,” researchers said.

China’s planetary exploration initiative, dubbed the Astronomical Project, outlines an ambitious vision that encompasses a series of four flagship missions: Tianwen-1 for Mars, Tianwen-2 for small celestial objects, Tianwen-3 for returning Martian samples, and Tianwen-4 for exploring the Jupiter system.

Notably, Tianwen-2 serves dual purposes: conducting in-orbit observations and sample collection from the near-Earth asteroid 2016 HO3, while also investigating the subsequent main-belt comet 311P.

After a 400-day journey covering about 1 billion kilometers (600 million miles), Tianwen-2 approached within approximately 20 kilometers of 2016 HO3 on July 2, 2026.

“During its journey, Tianwen-2 executed a series of deep space maneuvers and mid-course adjustments,” mission scientists reported.

“The spacecraft identified the asteroid on June 6, performed acquisition control from a distance of 30,000 km on June 7, and achieved co-orbital flight by June 19, when it was within 2,000 km.”

“Using the optical navigation data, we refined the asteroid’s ephemeris, improving positional accuracy to just a few kilometers compared to hundreds based solely on ground observations.”

Tianwen-2 is now set to enter a more detailed scientific investigation phase, characterizing the asteroid’s shape, surface composition, and internal structure, laying the groundwork for future sample collection.

Source: www.sci.news

Scientists Uncover Four New Genetic Strains of Cacao in Peru: A Breakthrough for Chocolate Production

In a comprehensive study of 390 traditional cacao trees representing Amazonian varieties, researchers discovered four previously unidentified genetic lineages. Notably, two of these lineages exhibited ancestry linked to exceptional flavor potential, opening up new avenues for growers and artisanal chocolate makers.

Motilal et al. Cacao samples were collected from eight departments in Peru. Image credit: Fernando Granier.

Cacao (Theobroma cacao) is a valuable outcrossed understory tree species native to the Amazon basin, primarily known for its economically significant beans.

These beans are essential in the multibillion-dollar chocolate industry and are utilized in various food and cosmetic applications, making cocoa an important agricultural commodity.

Cacao farming is a vital livelihood for millions of smallholder farmers in tropical regions and plays a critical role in global trade and the economies of producing nations.

In Peru, the world’s 8th largest cocoa producer, over 80,000 farmers rely on cocoa production as of 2024.

Many farms in Peru cultivate wild and semi-wild cacao varieties that have remained largely unchanged by breeding or genetic engineering.

Prior research indicated that native cacao trees in Peru and other countries can be classified into 10 genetic groups based on their similarities. Each tree may belong to a pure group or a combination of several groups.

However, recent studies have challenged this 10-group framework, with few focused specifically on Peru.

In a groundbreaking study, Dr. Lambert Motilal of the Cocoa Research Center at the University of St. Augustine of the West Indies, alongside colleagues, examined the genetic diversity of 390 wild and semi-wild cacao trees from indigenous farms across various Peruvian regions.

The researchers concentrated on single nucleotide polymorphisms (SNPs)—single-letter variations in the DNA of individual trees—to assess genetic diversity and relationships, thus categorizing them into genetically similar groups.

This analysis unveiled four previously unrecognized genetic groups in addition to the existing ten. While some trees were classified into pure groups, others were mixed.

Findings revealed that different areas of Peru exhibit unique genetic traits, showcasing fine-scale geographical variations in the genetic structure of cultivated cacao trees.

Remarkably, two of the four newly identified groups possess ancestry suggesting they may yield particularly high-quality, flavorful beans, according to the researchers.

This research also shed light on the ancestry of a notable cacao variety known as CCN51, which is cultivated for its high yields and disease resistance, gaining increasing economic significance.

The results indicate that Peru possesses unique genetic resources ripe for exploration regarding desirable traits in the cocoa and chocolate industries.

“Our study highlights that while Peru’s cacao trees share a common genetic foundation, each region maintains a distinct genetic identity, allowing for the identification of four entirely new cacao lineages,” the authors stated.

“This research not only transforms our understanding of Peru’s genetic landscape but also equips us with invaluable resources for conservation and the premium chocolate market.”

“One particularly rewarding aspect was engaging directly with trees on indigenous farms spanning eight diverse sectors, from the lush lowlands of Amazonas to the Andean foothills.”

“It was enlightening to realize these invaluable genetic treasures are not confined to laboratory settings but are genuinely thriving in farmers’ backyards, awaiting proper characterization and value for the premium market.”

Findings are part of a study featured in this week’s issue of PLoS ONE.

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LA Motilal et al. 2026. The genetic structure of traditional cacao reveals four new genetic lineages in indigenous regions of the Peruvian Amazon. PLoS One 21 (7): e0351690; doi: 10.1371/journal.pone.0351690

Source: www.sci.news

Groundbreaking Jurassic Fossil Sheds Light on How Birds Evolved from Dinosaurs and Lost Their Tails

Chinese paleontologists have recently identified a new species of small Jurassic bird, offering fresh insights into the evolution of avian anatomy. The short tail of this bird provides compelling evidence that early birds transitioned from the long, dinosaur-like tails to a more compact coccyx, facilitating the development of flight.



Reconstruction of Jenhernis Buyu. Image credit: Chung-Tat Cheung.

Modern birds are distinguished among vertebrates by their short tails, which comprise a fused bony structure known as the coccyx. This structure anchors the tail feathers and plays a crucial role in flight.

Unlike their dinosaur ancestors, which had long, bone-rich tails made up of numerous vertebrae, the evolution of birds involved a significant transformation that remains poorly understood due to the scarcity of fossils illustrating intermediate stages.

The newly discovered bird species, Jenhernis Buyu, appears to play a critical role in this evolutionary puzzle.

Dr. Zhou Zhonghe, a paleontologist at the Institute of Vertebrate Paleontology and Paleoanthropology of the Chinese Academy of Sciences, states, “Evolutionary biologists have often suggested that a transitional species with a shortened but not fully fused bony tail is biologically improbable, as long-tailed and short-tailed birds appeared nearly simultaneously in the early fossil record without clear intermediates.”

The holotype specimen of Jenhernis Buyu was discovered in 2024 in the Nanyuan Formation near Yangyuan Village in Zhenghe County, Fujian Province, China. This fossil dates back 148 to 150 million years, during the late Jurassic period, a time when some of the earliest bird species began to diversify.

This discovery represents the fourth taxonomic group of birds linked to what paleontologists refer to as the Zhenghe fauna. Notably, Baminornis has also contributed to our understanding, although it is represented by an incomplete specimen.

Estimations based on the circumference and length of the femur suggest that Jenhernis Buyu weighed between 74 to 163 grams, making it smaller than the previously known smallest bird, Archeopteryx.

“To our knowledge, this is the smallest adult non-pygostyle theropod known to date,” the research team stated.



Holotype specimen of Jenhernis Buyu. Image credit: Wang et al., doi: 10.1126/sciadv.aeb5202.

Jenhernis Buyu is notable for having only 15 vertebrae in its tail, whereas other early avian relatives often possess more than 30 separate, non-fused vertebrae.

The peculiar box-shaped last two coccyges feature anatomical characteristics also found in distant dinosaur relatives like Codypteryx, challenging previously held beliefs about tail shortening and caudal column fusion occurring simultaneously.

“This anatomical diversity illustrates a stepwise evolutionary transition. In the evolution of early birds, the reduction and shortening of vertebrae occurred prior to the fusion of the caudal column,” explained Dr. Ming Wang from the Institute.

The analysis indicates that Jenhernis Buyu was uniquely adapted compared to other nearby Jurassic birds, which suggests it did not thrive in arboreal or terrestrial habitats.

The researchers assert, “The body size, skeletal structure, and ecological niches of the symbiotic Zhenghe birds differ significantly, providing undeniable evidence of extensive adaptive radiation occurring by the end of the Jurassic period.”

This groundbreaking discovery contributes to settling longstanding debates regarding the timing of the initial diversification of early avian species.

For more details, refer to their study published in this month’s issue of Scientific Progress.

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Wang Ming et al. 2026. Jurassic Birds Unveil the Gradual Evolution of the Avian Coccyx. Scientific Progress 12(27);doi: 10.1126/sciadv.aeb5202

Source: www.sci.news

Chris Packham: ‘I Would Sacrifice Myself to a Tyrannosaurus’ – A Bold Statement on Conservation

Chris Packham presents a replica skull of Dorudon atrox, an ancient dolphin relative, in the documentary series Evolution.

Chris Packham features the skull of Dorudon atrox, a vital ancient dolphin relative in his new series Evolution.

Credit: BBC Studios/Freddie Claire

Evolution is an engaging five-part series featuring broadcaster and naturalist Chris Packham as he reveals the fascinating evolutionary histories of five charming animals. From elephants to ostriches, he guides viewers to the last common ancestor of all life on Earth, using innovative CGI to introduce significant ancestors along the journey.

In an exclusive interview with New Scientist, Chris discusses his ambition to utilize groundbreaking science and stunning visuals to transform our perception of nature from mere affection to genuine appreciation.

Penny Sarche: Chris, congratulations on your new show! What drew you to the project and its theme of evolution?

Chris Packham: We thrive on challenges. Our previous series, Earth, tackled immense time scales and complex events. It captivated audiences, and we realized we could delve into something equally intricate: evolution. This series tackles a concept recognized for its complexity by focusing on five iconic animals, narrating stories about locomotion, intelligence, feeding, and reproduction.

We learned invaluable lessons from Earth. Starting from the first cell to modern-day species, we abandoned traditional classroom methods for a more relatable approach. This allowed us to craft compelling narratives that engage our audience on a personal level, encouraging them to share newfound knowledge.

I found the exploration into each animal’s evolutionary journey fascinating. For instance, with bats, we examine their adaptation to flight, as well as the reasons behind their unique feeding habits.

People are often surprised by simple yet profound questions. We tend to overlook childhood curiosities once we grow up. However, revisiting fundamental questions about nature, like why the sky is blue, can be just as thrilling as uncovering scientific facts.

Another essential aspect is showcasing how these significant animals symbolize evolutionary milestones. CGI enables us to reconstruct elements that were only conceptualized before or known through fossil records. Observing phenomena like gills evolving into jaws reminds us of the wonders of nature.

For example, bats consume half their body weight nightly. Understanding their adaptations, including their ear’s role in feeding, illustrates the marvels of evolution.

It was illuminating to see these concepts brought to life. During my studies, I encountered dusty fossils and theory-laden textbooks. Now, blending CGI with scientific data adds a fresh angle!

Science is a perpetually evolving field. We’ve taken the opportunity to present new understandings through this series. We don’t claim to possess all the answers; instead, we acknowledge various perspectives from scientific communities, adding depth to our storytelling.

Chris Packham alongside a Baird’s Tapir in Costa Rica, featured in Evolution

Credit: BBC Studios/Freddie Claire

How does a deeper understanding of evolution enhance our love for wildlife?

Many misunderstand evolution as a finality. Humans are remarkable—inventive, creative, and resilient. Evolution is ongoing and encompasses all life, reminding us we are part of nature and reliant on it.

It’s imperative we increase our awareness, as human actions harm both nature and ourselves. We must truly care for the environment. Sir David Attenborough has profoundly engaged audiences, instilling deep connections to wildlife, but it’s time to transition from mere affection to vital care. Knowledge fosters appreciation.

If you could time travel for a moment, what would you wish to witness?

I’ve always admired the Tyrannosaurus rex as a child—large and ferocious, yet ultimately extinct. As a kid, I never envisioned understanding its appearance. Today, we have immense paleontological discoveries redefining our knowledge about this creature, including its color and behavior. If given five minutes in a time machine, I’d love to see it live—and possibly experience it firsthand.

What a fascinating thought!

That would indeed be an amusing epitaph!

Chris Packham with a rock monitor lizard in South Africa

Credit: BBC Studios/Will Edwards

I appreciate that Evolution isn’t solely focused on renowned species. It also showcases modern relatives and analogues of significant ancestors. Do you have a favorite?

I was captivated by a small velvet worm. Although I had only seen them in books and documentaries, encountering one in person was remarkable.

I found the lungfish equally intriguing. I’ve read extensively about them but never seen footage.

Ah, the lungfish! It’s incredibly unique with its slimy texture and articulated limbs resembling tentacles. Engaging with scientists behind the scenes was particularly enlightening as they shared their insights. We even discussed lungfish for about two hours—I could easily write a dedicated show about them!

You often incorporate science into Spring Watch. Do you believe there’s merit in embedding scientific insights into broader nature programs?

My passion for research ignited early, leading me to publish work before even attending university. Mentors from the scientific community have enriched my understanding, making my collaboration with Spring Watch particularly valuable.

Spring Watch allows us to explore species familiar to the public, such as swallows. A fascinating experiment showed that swallows prefer white feathers for nest lining. This choice is essential because certain bacteria break down specific materials, resulting in higher hatching success rates. Intertwining relatable examples fosters greater connection and understanding among audiences.

I hope viewers leave Evolution feeling inspired and contemplative about the essence of evolution. It’s vital to appreciate the richness of life on this planet and the role we play in its ongoing journey. The opportunities presented by evolution are remarkable—but do we truly want to jeopardize this incredible legacy?

Evolution premieres in the UK on July 13th on BBC Two and BBC iPlayer.

Topics:

Source: www.newscientist.com

Is Time a Construct of Universal Calculations?

What if the universe is just one big computer?

What if the universe was just one big computer?

NASA/ESA/J. Lee and pro500/Shutterstock

Below is an excerpt from our Lost in Space and Time newsletter. Every month, we share fascinating insights from around the globe. You can subscribe to Lost in Space and Time here.

My colleagues and I often joke about time’s illusion. “Oh, did I miss the deadline?” But what if time itself isn’t real? How can 40 years feel like mere moments? If extraterrestrial observers were to gaze at Earth now, would they witness an age of dinosaurs or merely an expanse of molten rock? Clearly, our perception of time is complex.

Yet, there’s a profound truth in this humor. It’s not that time is fictional; rather, our understanding of it is superficial. This sentiment resonates with physicists and philosophers who have contemplated time for centuries. Numerous theories exist, yet a definitive explanation remains elusive.

I posed this question to Stephen Wolfram, an esteemed physicist and computer scientist who has developed influential computational tools. His ambitious initiative, the Wolfram Physics Project, aims to redefine physics through computation instead of the conventional mathematical frameworks. This project has stirred debate within the scientific community. Wolfram’s premise—viewing the universe as one massive computer—could potentially unravel the mysteries of time, its forward motion, and our inability to foresee the future. I spoke with him to delve deeper into this concept.

Leah Crane: What is time?

Stephen Wolfram: Time is fundamentally an act of calculation.

Leah Crane: And that’s a wrap! Have a great day.

Time has puzzled physicists and philosophers for centuries

Vernon Leach / Alamy

Seriously, can you elaborate?

The perception of time is fundamentally the ongoing calculation of the universe’s continuous state.

Is it comparable to stacking images in a flipbook to simulate movement?

In a manner, yes, but it’s more intricate. Each state is computed sequentially from the preceding state over time. A question arises: if clear rules govern these computations, why can’t we predict outcomes? Why do we experience the relentless flow of time? The answer lies in the concept I’ve termed computational irreducibility.

What does irreducibility mean, and how does it inhibit time travel or future predictions?

Knowing a system’s foundational rules doesn’t guarantee its predictability. Traditionally, in mathematical sciences, one can derive future states from these rules. However, for many systems, the complexity of the calculations necessitates running each step, revealing the evolution of the system over time. Irreducible calculations compel you to traverse every step; shortcuts are non-existent.

Can you provide a tangible example of a computation that’s not reducible?

Consider calculating the digits of pi. Although there’s a defined method, you cannot reach the 1200th digit without calculating the preceding 1199 digits.

So it’s akin to navigating a staircase in the dark, where each step reveals the next?

Precisely. Climbing unpredictable stairs in the dark presents challenges. Predictability is integral to our experiences and how we navigate the world.

Thus, irreducible calculations resemble climbing a complex staircase in darkness, requiring focus without skipping steps and precluding time travel and future predictions. Is human nature inherently bounded?

Human observers have limited computational capabilities. For instance, deciphering an encrypted message demands exhaustive trials to find the plaintext. In scenarios involving computationally irreducible processes, we are unable to execute the entirety of calculations; our cognitive resources are finite. Predicting what occurs after a billion steps is simply beyond our mental capacity.

When calculating time, you cannot skip some steps

Alex Lynch / Alamy

If I had enhanced computational prowess, could I predict the future?

Should a computer execute computations faster than the universe itself, then theoretically, yes. However, our current computers are constructed from the universe’s materials, limiting their predictive capabilities.

Is this framework deterministic, where everything is entirely predetermined? How does humanity and free will fit in?

In deterministic contexts, knowing a system’s rules can imply predictability. However, if a computation is irreducible, the only way to ascertain outcomes is through executing the computation. You cannot outrun the system; experiencing it is essential for understanding.

This presents a duality: it illustrates the limits of science but also highlights the significance of experiencing time. The passage of time indicates that we engage in irreducible calculations, imbuing our experiences with meaning.

Your insights suggest our existence transcends the notion of superdeterminism. Even if free will is debatable, this ambiguity is vital to our experience?

Even within frameworks that suggest determinism, the nuances of decision-making remain significant. We might be subject to rules, yet our choices hold weight. Simple rules can yield complex outcomes. Imagining free will independent of existing laws paves the way for the universe to function arbitrarily. Failure in scientific inquiry would follow from such randomness. Thus, to establish consistent laws, we must acknowledge their inherent limitations.

Conclusively, if foundational laws govern reality, does the concept of free will lose its relevance?

Indeed, once definitive laws govern the universe, the broader concept of free will dissipates. The intriguing inquiry remains: why do we perceive free will? Computational irreducibility might elucidate this; predicting future actions undermines the perception of agency, portraying us as passengers within a predetermined narrative.

Topic:

Source: www.newscientist.com

Peter Scholl’s Algorithm: Is It Really a Threat to the Internet? Here’s Why He’s Not Concerned

Peter Shor: The Innovator Behind the Quantum Algorithm

Christopher Harting

“Is he the Beyoncé of this event?” a young woman asked beside me. As we observe a crowd of bearded men in orange sweaters, getting a glimpse of him feels akin to viewing the Mona Lisa—a momentary, fleeting encounter. “His algorithm is revolutionary,” remarked a colleague, capturing quick snapshots with attendees who were taking selfies and getting conference badges autographed.

I’m currently at the Quantum.Tech World conference in Boston, where Peter Schor is the headliner. Schor is renowned in the quantum computing sphere, thanks to his notable invention, known as Schor’s algorithm.

During the 1990s, Schor was a visionary at Bell Laboratories in New Jersey. At the time, quantum computing was an emerging research topic that piqued his interest after attending a seminar presented by quantum pioneer Umesh Vazirani. He posed questions about the advantages quantum computers held over classical ones, which led him to wonder about practical applications.

Over six transformative months, he pinpointed a significant problem—factoring large numbers—and engineered a solution for quantum computers. Thus, Schor’s algorithm was born, a breakthrough that “could disrupt everything.” This pivotal contribution motivated researchers to push forward with the real construction of quantum computers.

Modern cryptography heavily relies on the challenge of factoring large numbers. As long as classical computers struggle with this task, our digital data—ranging from emails to banking records—remains secure. However, a quantum computer utilizing Schor’s algorithm can efficiently tackle this problem. In fact, a sufficiently powerful quantum computer could leverage this algorithm to decrypt even the most secure data.

Yet, in a rare moment of calm at the conference’s makeshift lounge, Schor expressed that he isn’t overly concerned. “We have robust methods for post-quantum cryptography; we just need to implement them.” He cautioned, “It will be a substantial challenge.”

Fortunately, well-documented encryption techniques exist that can withstand his algorithm.Organizations like the National Institute of Standards and Technology (NIST) are already establishing quantum-resistant encryption standards. However, adapting to these methods is a daunting and costly endeavor. For large entities like banks or hospitals, it may take years to audit their systems for vulnerabilities, followed by an equally lengthy process to update their infrastructure and software.

Peter Schor in an orange sweater, signing a conference badge.

Karmela Padavic-Callaghan

Time is of the essence. While current quantum computers are still in their developing stages, lacking the power to execute Schor’s algorithm, there have been remarkable advancements in both hardware and software in recent years. Major tech companies like Google are aiming for a 2029 target to finalize the transition to post-quantum cryptography. Furthermore, U.S. President Joe Biden recently issued a presidential order mandating that all high-value government systems achieve similar transitions by 2031.

“Quantum computers are still experimental, but they won’t remain that way for long,” Schor asserts. He commends the significant strides made by researchers to enhance the size and computational capabilities of quantum computers. The collaborative efforts in academia and industry to improve error correction in quantum systems have been impressive, according to Schor.

He clarifies a common misconception: not everything a classical computer does can be replicated faster by a quantum computer. “I don’t expect quantum systems to predict the stock market,” he states.

In Schor’s perspective, quantum computing should focus on a limited set of questions. Beyond cryptography, he emphasizes simulating complex systems related to quantum mechanics, chemistry, and biomedicine, alongside tackling certain optimization challenges. He expresses particular enthusiasm for optimization algorithms, which he believes have often been overlooked.

However, he candidly acknowledges that creating genuinely useful quantum algorithms thus far has proven to be an uphill battle. “It’s not that we aren’t intelligent enough to design superior algorithms; it may simply be that quantum computers will only be applicable for a narrow range of tasks,” he muses.

Final thoughts lead to a question about what could help advance understanding in the field. “Engaging with real quantum computers to explore their limitations and potential is vital,” he advises. “However, mastering quantum mechanics and computer science is a daunting task—it requires a great deal of dedication.”

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Source: www.newscientist.com

How Salt Batteries Will Transform Electric Vehicles and Grid Storage Solutions

CATL’s Sodium-Ion Battery at the Exhibition

VCG/VCG (via Getty Images)

On February 5, a black sedan sped down an icy road in northern China at 95 km/h when a tire burst, creating a plume of white smoke in the -32°C air. Remarkably, the vehicle coasted to a stop without hitting the snow. This demonstration aimed to showcase Changan’s new electric vehicle lineup, which includes the first mass-produced EV equipped with sodium-ion batteries, proving its endurance in severe conditions.

Changan’s Nevo AO6 model features a new generation of advanced sodium-ion batteries from leading energy storage company CATL and is slated for release later this year.

Most rechargeable batteries rely on lithium, a valuable mineral, while sodium-ion batteries utilize a more plentiful and cost-effective resource: salt. If sodium-ion technology can match the performance of lithium-based batteries at a lower cost, it could challenge lithium’s market dominance, potentially leading to a variety of battery chemistries customized for specific devices.

“This is just the beginning of the battery revolution. We will see various new batteries targeting specific segments,” says Maria Crespo-Rivadeneira from Queen Mary University of London. “Sodium is paving the way for a future beyond lithium.”

The first sodium-ion battery was developed by Ford in 1966, but serious advancements in this technology have surged in the last 15 years due to increased demand for electrification in power grids and vehicles. While both types of batteries operate on similar mechanisms, sodium-based batteries have sodium dissolved in the electrolyte instead of lithium, and they utilize differing electrode materials.

However, sodium is three times heavier than lithium; hence, a sodium-ion battery with equivalent storage capacity will weigh significantly more. This characteristic has long limited its application to grid storage and small EVs with shorter ranges.

Multiple sodium-ion grid storage facilities have been established in China, Germany, and the U.S. General Motors, the largest automobile manufacturer in America, has partnered with startup Peak Energy to expand this technology. Peak Energy provides sodium-ion batteries for data centers to store energy during cheaper electricity periods. Additionally, Eleven Energy has begun supplying household sodium-ion batteries in the UK.

Recent studies indicate that the specifications of sodium-ion batteries have progressed sufficiently for them to enter the broader EV market. A recent study by Moritz Schutte at Aachen University in Germany found Hina’s sodium-ion batteries to be comparable to Tesla’s lithium-ion batteries in most aspects, albeit still a third heavier.

CATL claims that their sodium-ion batteries achieve an energy density of 175 watt-hours per kilogram, making them competitive with low-cost lithium iron phosphate batteries from companies like Tesla. Schutte also noted that while sodium-ion batteries currently fail to compete with lithium batteries on price, this may change as the market grows.

“Sodium-ion batteries scale rapidly,” he explains. “Production costs are continuously decreasing. Material advancements are occurring with each generation, and it’s uncertain where this will lead regarding energy density.”

Sodium also presents ecological advantages. The extraction of lithium is both energy-intensive and environmentally costly. Since China dominates lithium supply chains, geopolitical tensions, such as those involving Taiwan, could disrupt availability. Furthermore, lithium ions experience slower movement through the electrolyte at low temperatures, which can lead to diminished device performance. In contrast, sodium ions exhibit lower heat generation during electrochemical reactions, enhancing safety and stability.

CATL reported that during cold testing in northern China, their sodium-ion EV batteries retained 90% capacity at -40°C (-40°F). Even when cut in half, the batteries functioned without catching fire, continuing to supply energy to a bulb.

Elliot Richards, an EV video blogger from Shanghai, noted that sodium-ion batteries have been dubbed “lithium killers.” While lithium may remain prominent in luxury vehicles, sodium could become the go-to choice for budget-friendly EVs, vehicles optimized for extreme weather, cargo trucks, energy grids, and home energy solutions.

“We may underestimate the impact this will have on our daily lives,” he remarks. “Owning an EV will become more cost-effective than a traditional combustion vehicle, and integrating batteries in homes will be significantly cheaper, which will reduce the overall energy costs for consumers.”

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Source: www.newscientist.com

Artemis II Astronaut Jeremy Hansen Steps Down from Full-Time Mission Role

On Monday, Canadian astronaut Jeremy Hansen announced his resignation from his full-time position with the Canadian Space Agency, following his groundbreaking journey around the Moon on NASA’s Artemis II mission.

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Hansen, aged 50, expressed in an Instagram post his intent to transition from his role at the Canadian Space Agency, emphasizing that this change is “far from a departure.” He characterized his new position as “an intentional launching pad,” designed to maintain avenues for creative and continued support of Canada’s vital space initiatives.

He will maintain his service as a reservist in the Royal Canadian Air Force.

“I extend my gratitude to the Canadian Armed Forces, CSA, NASA, our international partners, and my family,” Hansen stated. “Thank you, Canadians, for believing that when our country sets its sights high, we can achieve greatness. The mission continues.”

Notably, Hansen has dedicated 32 years to the Royal Canadian Air Force and 17 years to the CSA as an astronaut, according to the CSA.

In 2013, he participated in a unique caves program, spending six days living underground, as reported by the CSA. In 2014, he engaged in another pioneering venture, Nemo19, where he spent seven days working aboard the Aquarius underwater laboratory, according to a CSA release. Hansen made history in 2017 as the first Canadian to lead NASA’s astronaut class, training astronauts from both the United States and Canada.

“Through his dedicated service in the Royal Canadian Air Force and pivotal contributions to Canada’s space endeavors, Hansen has embodied the pinnacle of Canadian leadership and excellence,” stated Canadian Defense Minister David J. McGuinty. “His legacy will inspire future generations to explore careers in science, innovation, and discovery.”

In April, Hansen participated in NASA’s Artemis II mission alongside three American astronauts, marking the first crewed flight to the Moon in over half a century.

The mission crew set several records, becoming the first humans to travel such a distance from Earth and to witness the entire far side of the Moon with their own eyes, as well as the first astronauts to experience a solar eclipse from lunar territory.

In an interview with NBC News while in space, Hansen conveyed, “I feel immensely humbled.” He added, “The sight of us four out here is absolutely overwhelming.”

He remarked that the visuals of Earth and the Moon captured during the mission don’t do justice to the awe-inspiring views experienced by the astronauts firsthand.

“While those photos are wonderful,” he emphasized, “the reality here transcends anything you could capture.”

Source: www.nbcnews.com

5 Charts Illustrating the Growing Dangers of Heatwaves

Paramedics assist in loading a patient into an ambulance amid the 2022 heatwave in Barcelona, Spain.

Image credit: Angel Garcia/Bloomberg via Getty Images

The recent heatwave in May set alarming monthly temperature records across Europe, with June marking the hottest month ever recorded in Western Europe. As we enter July, another heatwave unfolds, highlighting a concerning trend—just 50 years ago, such extreme heat in June would have been virtually unheard of. However, the impact of global warming is making heat waves more frequent, prolonged, and intense.

Tragically, heat is recognized as the deadliest climate hazard, claiming the lives of around 500,000 individuals annually. Even if we achieve net-zero emissions tomorrow, this number is likely to rise due to the already elevated levels of carbon dioxide driving up global temperatures.

As Hugh Montgomery, a leading researcher at University College London, states, “This is just the beginning.” He emphasizes the ongoing severity of this situation, indicating that prolonged heat will have significant long-term consequences.

Interestingly, outside the tropics, the annual occurrence of temperatures exceeding 32°C has increased by an average of 12 days over the last fifty years. Europe, which is warming most rapidly, typically experiences intense heat stress beginning in June and extending into September—sometimes even starting as early as May.

This trend results in a growing number of individuals facing extreme heat days and heatwaves. North America, Europe, South America, and parts of Africa are now enduring up to 50 additional days of severe heat stress compared to the 1970s.

Neil Maxwell from the University of Brighton notes, “The longer a heatwave persists and the more frequent they become, the longer individuals remain in a heightened physiological state.” Such conditions can lead to increased inflammatory responses, ultimately contributing to elevated stress levels in affected individuals.

Before the year 1998, severe nighttime heat stress was rare; however, temperatures at night are now rising in regions like Western Europe, with rates increasing twice as fast as overall global warming.

The lack of cool nighttime temperatures—defined as below 20 degrees Celsius—impairs sleep quality. Persistent hot environments make it difficult for individuals to fall asleep and attain deep sleep stages. Additionally, sleep deprivation over successive nights can diminish reaction times, escalates anxiety, and increase stress levels.

In 2022, Europe faced its hottest summer on record, triggering destructive events such as wildfires across France, Portugal, and Spain. Notably, Italy’s longest river, the Po, experienced severe drought conditions, revealing remnants of wartime ships as water levels plummeted in the Danube. The UK recorded temperatures surpassing 40°C (104°F) for the first time ever.

Dreadfully, over 60,000 deaths were attributed to these extreme temperatures, with Mediterranean countries like Italy, Greece, and Spain experiencing the highest mortality rates. These nations, home to some of the oldest populations, are at a heightened risk, given that aging bodies are more sensitive to heat and vulnerable to chronic illnesses.

Montgomery warns, “Heat triggers an inflammatory response, instigating various detrimental biological reactions in the body. This exposure can be directly harmful, particularly for those already unwell.”

Since the 1970s, Europe has witnessed a 73% increase in the frequency of heat stress days followed by tropical nights, defined as exceeding 20°C. This phenomenon, referred to as “complex events,” prevents bodies from cooling down overnight, exacerbating heat stress.

Moreover, the prevalence of prolonged heat stress is rising in Europe, while Africa is now nearly three times more likely to endure extreme heat for extended periods throughout the year.

While leaders, including former US President Donald Trump, have pledged to plant millions of trees while simultaneously increasing CO2 emissions, urban forests can significantly mitigate heat. Trees not only provide shade but also release moisture into the air through evaporation, cooling their surroundings. Neighborhoods with abundant tree cover are 10°C cooler than those without.

Despite various cities initiating tree-planting initiatives to combat heat, research indicates that many areas still fall below a 30% canopy cover, insufficient to effectively counteract the urban heat island effect. More than 90% of buildings in major cities like Paris and London remain beneath this threshold.

Topics:

  • Climate Change/
  • Extreme Weather

Source: www.newscientist.com

How Changes in Ovarian Identity After Menopause Contribute to Inflammation

Ovaries’ Vital Role in Postmenopausal Health

Magic Mine/Getty Images

Recent research indicates that ovaries may have a significant impact on postmenopausal health, contradicting the belief that they become completely inactive after menopause. Studies show that immune cells infiltrate the ovaries of aging mice, linking these organs to chronic postmenopausal inflammation.

“We assumed the ovaries fulfilled their purpose after reproduction,” stated Francesca Duncan from Northwestern University. “Our findings were quite unexpected.”

In March, Duncan and her team published a study that explored the protein profiles of postmenopausal women aged 50 to 75. Contrary to their expectations of uniformity, they discovered that the molecular signatures of the ovaries evolve dramatically over time, challenging the notion of their inactivity.

To delve deeper, Duncan’s team is analyzing mouse ovaries, focusing on tissue and gene expression at different life stages: young (2 months), reproductive (18 months), and post-reproductive (24 months). Despite lacking menstrual cycles, aging mice experience a decline in egg reserves leading to irregular cycles, similar to human menopause. “We recognize that the hormonal changes mirror what happens in humans as they age,” Duncan noted.

Initial findings confirmed some expectations; older ovaries exhibited a loss of egg-producing follicles and increased scarring. However, the study also found heightened gene activity associated with inflammation and immune response as aging progressed. The number of immune cells, including T cells and macrophages, rose in tandem with age.

Further investigation is crucial to clarify the implications of these changes for immunity and overall health. Duncan suggests this transformation in the ovaries might indicate a loss of reproductive function coupled with an increase in immune activity, which may not be beneficial. “As ovaries transition, there could be an uptick in inflammatory signaling that interacts with other bodily systems,” she explained.

While the current study focuses on mice, Diana Laird and her team at UCSF propose that similar immune modifications may be occurring in human ovaries, based on shared reproductive traits across species. “Both our species cease cyclical activity once the ovarian supply is depleted. Other phenomena, like fibrosis and altered nerve supply, are also present,” she asserted.

Although the rationale behind this evolutionary change in older mice remains unclear, it may have historically provided a survival advantage by enabling immune cell reservoirs at a time when fewer individuals lived to old age. Today, however, it poses risks of inflammation and autoimmune disorders.

This research prompts a reevaluation of the ovaries’ importance post-menopause. Although typically seen as dormant, they continue to release hormones like androgens, crucial for maintaining bone density and libido. Laird emphasized the need for more in-depth studies, linking immune changes in the ovaries to increased inflammation and conditions like rheumatoid arthritis after menopause. “This emphasizes the necessity for detailed investigations into the post-reproductive ovary’s cellular and molecular components,” she concluded.

Topics:

Source: www.newscientist.com

How Changes in Ovarian Identity Post-Menopause Contribute to Inflammation

Postmenopausal Health

Significance of Ovaries in Postmenopausal Health

Image Credit: Magic Mine/Getty Images

The traditional view held that after menopause, ovaries become dormant, but recent findings suggest these organs may contribute to postmenopausal inflammation.

Francesca Duncan from Northwestern University states, “We believed the ovaries had fulfilled their role after reproduction, yet our discoveries were quite unexpected.”

In a recent study published in March, Duncan and her team analyzed ovarian protein structures in women aged 50 to 75, expecting uniformity across samples. Conversely, they found that molecular signatures significantly changed over the decades, indicating a dynamic rather than static organ.

To explore these changes further, Duncan’s team investigated mouse ovaries, examining tissues and gene expression across various age groups: young (2 months), reproductive age (18 months), and post-reproductive (24 months).

Unlike humans, mice do not have menstrual cycles. Instead, their endometrial lining is reabsorbed. Also, while humans experience menopause, mouse fertility gradually declines with age, leading to irregular cycles. Duncan explains, “The decline in fertility and hormonal function mirrors what we see in aging mice.”


Expectedly, older ovaries showed a loss of egg-producing follicles and increased scarring. Moreover, genes responsible for reproduction and hormone production, specifically estradiol (a form of estrogen), were less active. However, genes linked to inflammation and immune activity were notably more active, with an increase in immune cells such as T cells and macrophages in aging ovaries.

Further investigation is needed to discern the implications of these findings for immune function and overall health. Duncan suggests that this might indicate a transformation in ovarian identity rather than an enhancement in immune capacity. “Ovaries seem to lose reproductive functions while gaining immune functions, which may not be beneficial,” she adds.

The phenomenon of chronic low-grade inflammation in aging tissues may involve the release of inflammatory molecules from the ovaries post-reproduction. Duncan remarks, “This shift in biological function could signal communication with other body systems, although its significance remains uncertain.”

Professor Diana Laird at the University of California, San Francisco posits that similar immune transformations may occur in humans, alluding to known reproductive similarities between species. “Both humans and mice cease cycling after their egg supply depletes, and experience similar changes like fibrosis and increased nerve distribution,” she notes.

While the rationale behind immune changes in older mice is still unclear, Laird suggests these adaptations might have offered an evolutionary advantage for surviving longer. However, such changes could also contribute to inflammation and autoimmune disorders under modern living conditions.

This study underscores the evolving role of ovaries post-menopause. While generally healthy, ovaries still release androgens, which help maintain bone density and libido. Laird asserts this research contributes to a growing understanding of how immune changes in ovaries may lead to increased inflammation, associated with conditions like rheumatoid arthritis in postmenopausal women. “This discovery emphasizes the need for comprehensive studies on the cellular and molecular aspects of post-reproductive ovaries,” she concludes.

Topics:

Source: www.newscientist.com

Unveiling History: 3,000 Artifacts from Stone Age to WWII Discovered by Archaeologists in Dutch Valley

Over 3,000 archaeological artifacts, spanning from the Stone Age to World War II, have been unearthed in the Nieuwe Drostendiep river valley in the Netherlands. This discovery emphasizes the historical significance of waterways in attracting human activity.

Among these artifacts, 600 items of exceptional importance highlight the valley’s role as a hub for trade, sustenance, and even spiritual practices, according to experts.







Currently, environmental restoration initiatives are taking place in the Nieuwe Drostendiep river valley between Slín and Oosterhesselen, located in the northern Drenthe region. During these efforts, archaeologists meticulously examined the upper soil layers, leading to the discovery of numerous historic items such as Stone Age tools, Bronze Age artifacts, and jewelry dating from 200 BC to the early Middle Ages.

Notable finds include a gold ring from the 3rd or 4th century AD and a fibular pin from the 10th or 11th century AD, used historically to fasten clothing. Objects from more recent histories, including artifacts from the Eighty Years’ War (1568-1648) and World War II, were also uncovered.

All discoveries were made around the New Drostendiep valley – Credit: Getty

The research team is astounded by the sheer number and diversity of artifacts, many of which are in excellent condition. These items were found in relatively undisturbed soil layers, ensuring their preservation.

Professor David Bridgeland from Durham University, who researches human evolution and environmental interaction, noted that: “Rivers supplied essential resources like water and food, attracting both predators and livestock, while also preserving historical evidence.”

Yvonne Turenhout, an executive member overseeing the project, expressed pride in the rich history and stunning landscapes of Drenthe province. She stated that these extraordinary discoveries further highlight the region’s significance.

The artifacts are currently not open for public viewing as researchers are still cleaning, cataloging, and studying them. Officials are contemplating an exhibition and exploring ways to provide digital access to parts of the collection.

Read more:

The featured image of the ring is for illustrative purposes only and was not found in the Nieuwe Drostendiep.

Source: www.sciencefocus.com

Discovering Jupiter’s Future: Giant Exoplanet Orbiting White Dwarf Star Provides Insights into Planetary Evolution

Astronomers employing NASA/ESA/CSA’s James Webb Space Telescope have successfully analyzed the atmosphere of a giant exoplanet, WD1856+534, which orbits a white dwarf star. These groundbreaking findings provide insight into the ultimate fate of giant planets surrounding stars with masses akin to our Sun.



WD 1856b is a gas giant planet orbiting its star 50 times closer than Earth does the Sun. Image credit: NASA/ESA/CSA/Ralf Crawford, STScI.

“Most stars, including our Sun, eventually exhaust their fuel, leaving behind a white dwarf,” noted Dr. Ryan McDonald, an astronomer at the University of St. Andrews, along with colleagues.

“The implications of this stellar evolution on orbiting planets remain largely unclear.”

“Multiple planet candidates have been discovered around white dwarfs, suggesting that planets can endure the transition period when stars evolve into red giants before becoming white dwarfs.”

“However, there is still limited knowledge regarding the atmospheric composition of such planets.”

The new study focused on WD1856b, identified in 2020 by astronomers using NASA’s TESS and Spitzer Space Telescopes.

This exoplanet boasts a radius of 0.9 times that of Jupiter and a mass between 4.3 and 10.9 times Jupiter’s mass.

It orbits the 10-billion-year-old white dwarf star WD 1856+534, which is situated 80 light-years away in the Draco constellation.

“This planet is approximately the same size as Jupiter, while the white dwarf star it orbits is the size of Earth, making this planet seven times larger than its star,” Dr. McDonald stated.

Utilizing Webb’s Near Infrared Spectrometer (NIRSpec), astronomers detected hydrocarbons and aerosols, including methane, in WD 1856b’s atmosphere.

They also measured thermal radiation emanating from the planet’s night side.

“We observed tiny cloud particles and clear indications of hydrocarbons (possibly methane),” shared Cornell University astronomer Victoria Boehm. “This marks the first instance of observing the atmosphere of a planet transiting a dead star.”

“We have recently executed four additional observations of WD 1856b with Webb to delve deeper into the chemistry of its atmosphere, and we’re eager to analyze the results.”



Webb evaluated the composition of WD 1856b as it transited in front of the star, revealing signs of methane. Image credit: NASA/ESA/CSA/Joseph Olmsted, STScI.

Researchers estimate that the planet’s atmosphere has a temperature ranging from 390-412K, significantly higher than the expected temperature of a giant planet (160K).

This heating likely transpired between 3 billion and 5.5 billion years after the star converted into a white dwarf.

In this context, the planet would have initially occupied a wider orbit, safeguarding it from the star during its cataclysmic red giant phase, only to eventually move to its current position.

“As the planet migrated inward, interactions with the white dwarf’s formidable gravity would have induced a significant temperature spike, which has been decreasing ever since,” stated Dr. Christopher O’Connor of Northwestern University.

“The primary question is how WD 1856b evolved into its current state, and there are two prevailing theories.”

“One hypothesis suggests the planet was engulfed by its dying host star and somehow persisted within.”

“The alternative theory posits that the movement was influenced by gravitational dynamics of other bodies within the system.”

The white dwarf is part of a triple star system, where its companion star may play a role in shaping WD 1856b’s orbital path.

In approximately 5 billion years, our Sun will exhaust its hydrogen fuel, expanding to over 100 times its current dimensions, entering the red giant phase.

Following this, it will shed its outer layers, ultimately becoming a white dwarf.

Mercury, Venus, and potentially Earth may be obliterated during this transition.

However, the fates of outer planets, particularly gas giants, remain uncertain.

“We typically rely on telescopes to examine the past, but for the first time, we can observe what may happen to exoplanets around remnants of Sun-like stars,” Dr. McDonald remarked.

“It’s akin to employing a time machine to glimpse into the distant future of our own solar system.”

For further details, see the findings outlined in this week’s edition of Nature.

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RJ McDonald et al. 2026. Aerosols and hydrocarbons in the atmosphere of a white dwarf star. Nature 655, 76-80; doi: 10.1038/s41586-026-10514-7

Source: www.sci.news

New Research Reveals Ancient Americans as Specialized Hunters of Large Animals

A recent study reveals that the earliest human cultures in the Americas were not simply opportunistic foragers. Instead, they were specialized big game hunters who dedicated their lives to hunting large animals like mammoths, elephant-like gomphotheres, and giant ground sloths—true Ice Age giants.



Paleoindians hunting glyptodonts, relatives of armadillos from the Pleistocene. Illustrated by Heinrich Harder, 1920.

For decades, archaeologists have debated whether Paleoindians focused on hunting megafauna or adopted a generalist lifestyle, consuming a diverse diet that included small game, fish, plants, and shellfish based on their environment.

In recent years, many scientists have leaned toward a generalist perspective. However, a new study led by the University of Alaska Fairbanks contradicts this notion.

Ben Potter, a professor at the University of Alaska Fairbanks, stated, “One of the competing theories is dietary generalization, which advocates for utilizing a wide variety of resources varying by region.”

“The other theory posits megafauna specialization, concentrating on a select few large-bodied prey.”

In this groundbreaking study, researchers analyzed 50 sites across three regions: Eastern Beringia (ancient Alaska, circa 14,000 to 13,300 years ago), the Clovis Culture of North America (approximately 13,400 to 12,800 years ago), and the Fishtail Projectile Point Culture of South America (roughly 12,900 to 11,600 years ago).

Together, these cultures represent the oldest known human societies extending across the Western Hemisphere.

By assessing factors such as species richness, minimum population size, and edible biomass, scientists discovered that megafauna constituted 83% to 88% of the meat and fat consumed by these groups.

Woolly mammoths dominated Beringia diets, while Columbian mammoths were prevalent in North America, and giant ground sloths along with gomphotheres were staples in South America.

While small animals were present in many locales, they provided minimal nutritional value.

“Evaluating culinary expertise involves more than identifying the number of specific animals at ancient campsites,” notes Professor Potter.

“If early humans were dietary generalists, the most common animals would be reflected more frequently in their campsites.”

“Mammoths and ground sloths were relatively rare in the environment, yet they dominate the archaeological record.”

“Conversely, rabbits and rats, despite being numerous, are seldom found in the record.”

The authors also cite independent evidence: chemical analysis of the Clovis-era child, Anzick-1, showed that about 96% of the mother’s proteins were derived from megafauna, primarily mammoths.

In addition to their diets, these early groups exhibited traits characteristic of professional hunters. They led highly mobile lifestyles rather than establishing fixed homesteads, and there was scant evidence of plant-processing tools such as grindstones.



Maps and dietary analysis illustrating how three Paleoindian cultures, East Beringian, Clovis, and Fishtail Projectile Point, specialized in hunting megaherbivores across the Western Hemisphere from about 14,000 to 11,600 years ago. Image credit: Ben Potter.

Professor Potter elaborated: “The focus on large edible herbivores explains the remarkable similarity in early toolkits found from California to Maine and across South America.”

“Hunters targeting the same type of animals across vastly different landscapes did not need to modify their methods to adapt to local conditions.”

“Archaeological findings included tools specifically designed for hunting large game, such as large fluted projectiles and specialized equipment for slaughtering.”

There was a significant absence of fishing tools and implements for processing plants.

This emphasis on large prey facilitated the rapid human expansion from Alaska to South America.

Typically, when hunter-gatherers venture into unfamiliar regions, it can take many generations to fully understand the local terrain, hunt smaller game, and identify edible plants. However, relying on large mammals alters this dynamic.

“Mammoths, for instance, were widespread, traversing vast territories,” stated Matt Uhler, a professor at the University of Alaska Fairbanks.

“In effect, expert hunter-gatherers utilized their knowledge of megaherbivores like mammoths to expand across continents faster than they would have if they had to learn about every local ecosystem.”

The researchers hypothesize that this specialization in hunting large herbivores may have significantly impacted ecological networks, contributing to the mass extinction of Ice Age megafauna as these cultures migrated southward.

Mammoths and horses vanished from Alaska around 13,300 years ago, coinciding with the earliest known human occupations.

In North America, Clovis-era megafauna disappeared by 12,800 years, while gomphotheres and giant ground sloths lingered in South America until approximately 11,600 years ago.

“This pattern of arrival, proliferation, and extinction may have repeated itself, each time progressing further south, making a compelling case for human hunting as the primary catalyst for megafauna extinctions, with climate change possibly exacerbating the situation,” Professor Potter concluded.

“Megaherbivores reproduce slowly, occupy expansive territories, and lack natural predators as adults.”

“They likely did not possess the learned wariness that technologically advanced hunter-gatherers exhibited.”

For more information, see the study published in the Journal on July 1, 2026, in Scientific Progress.

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Ben A. Potter et al. 2026. Hemispheric-scale evidence for early Paleoindian megaherbivore specialization. Scientific Progress 12(27); doi: 10.1126/sciadv.aef9628

Source: www.sci.news