How Shifting Induction Time to Early Morning Can Reduce Labor Duration by 6 Hours

For an efficient labor, opt for induction early in the morning.

Yulia Burmystrova/Getty Images

Innovative research indicates that the optimal time for labor induction is early in the morning. This approach aligns with our natural circadian rhythms, potentially shortening labor duration and decreasing the likelihood of C-sections.

“This cost-effective strategy enhances the birthing experience for mothers, newborns, and healthcare providers alike,” notes Hanne Hoffman from Michigan State University.

Across the UK, US, and Australia, approximately one-third of all births are induced, utilizing medication or artificial methods instead of allowing labor to commence spontaneously. Induction generally mitigates the risk of stillbirth, especially when the baby is overdue or facing developmental issues. Another indication for induction is when the water breaks prematurely, heightening the risk of infection.

However, induced labor can often be longer than natural labor. “I know individuals who underwent labor induction and endured two lengthy days of it; I was astonished by their prolonged and painful experiences,” Hoffman shares.

This prompted Hoffman, who investigates circadian rhythms—our body’s natural oscillations—to contemplate whether a specific time of day is ideal for labor induction. “We observe that natural childbirth follows a circadian rhythm, with uterine contractions peaking in the late evening and deliveries primarily occurring at night,” she adds. This timing may have evolved as it offers a safer environment, reducing predator threats.

To further explore this, Hoffman and her team analyzed data from over 3,000 induced deliveries at Michigan hospitals from 2019 to 2022. They discovered that the shortest labor duration was for those induced between 3 a.m. and 9 a.m. For instance, inductions at 5 a.m. averaged 15 hours, while those at 11 p.m. took around 21 hours—an extension of six hours. Those induced in the morning also faced lower chances of emergency C-sections.

The early morning advantage may stem from heightened uterine receptor sensitivity to oxytocin during this timeframe, a crucial hormone that stimulates uterine contractions during childbirth. For inductions, a synthetic oxytocin is typically administered. “When a doctor initiates labor with a substantial dose of oxytocin, you may, in essence, be capitalizing on your body’s internal morning oxytocin boost and intensifying labor,” explains Satchidananda Panda from the Salk Institute for Biological Studies in San Diego, California.

The findings suggest that women with a higher BMI or first-time mothers benefit significantly from early morning inductions. The research team now aims to delve into the biological mechanisms behind these outcomes.

While organizing all labor inductions between 3 a.m. and 9 a.m. may not be feasible for all hospitals, prioritizing first-time mothers and patients with higher BMI could be beneficial, Hoffman posits.

Crucially, this study indicated no medical complications arising from early morning inductions. “We observed no rise in NICU admissions,” emphasizes Rene Cortese from the University of Kansas Medical Center. “This study sends a vital message: while one risk is diminished, no new risks are introduced.”

The research team is eager to conduct additional studies to validate that assigning early morning delivery actually enhances outcomes. “We need to establish a proof-of-concept study to replicate this finding,” shares Hoffman.

Other chronotherapy approaches, which adjust medical interventions based on circadian rhythms, are being explored across oncology, cardiology, and psychiatry, with recent findings indicating that administering cancer treatments before 3 p.m. can improve patient survival rates.

Topics:

  • Pregnancy and Childbirth/
  • Circadian Rhythm

Source: www.newscientist.com

Discovering the Five Sleep-Wake Profiles: Why Staying Up Late and Waking Early Isn’t Enough for Optimal Health

A groundbreaking study conducted by researchers at McGill University indicates that human sleep patterns, or chronotypes, exist on a broader biological spectrum. Each subtype is linked to distinct health and behavioral traits, challenging the conventional ‘early riser vs. night owl’ classification.

Zhou et al. The study identifies five distinct biological subtypes, each related to various behavioral patterns and health conditions. Image credit: Wok & Apix.

Chronotype refers to the specific time during the 24-hour cycle when an individual naturally feels the most alert or is prepared for sleep.

Previous research has often associated late-onset chronotypes with health issues, yet the findings have frequently been inconsistent.

“Instead of asking if night owls face greater risks, it may be more insightful to explore which specific night owls are at risk and why,” explains Dr. Yue Zhou, a researcher at McGill University.

Utilizing AI technology, Zhou and colleagues analyzed brain scans, questionnaires, and medical records from over 27,000 adults in the UK Biobank.

Their findings uncovered three night owl subtypes and two early riser groups.

One early riser subtype exhibited the fewest health issues, while the other was more closely linked to depression.

Night owls performed better on cognitive assessments but faced difficulties in emotional regulation.

One night owl group was prone to risk-taking behaviors and cardiovascular challenges, while another group showed higher tendencies for depression, smoking, and heart disease.

“These subtypes are not merely characterized by their sleep times,” stated Dr. Danilo Buzdok from McGill University.

“They represent a complex interaction of genetic, environmental, and lifestyle factors.”

Instead of categorizing sleep types as good or bad, the researchers emphasize how risks and strengths are distributed differently among the five profiles.

A nuanced comprehension of sleep profiles can clarify why identical sleep schedules impact individuals differently, promoting research and sleep support that transcends a one-size-fits-all methodology.

“In today’s digital age and post-pandemic world, sleep patterns are more diverse than ever,” remarks Zhou.

“Recognizing this biological diversity may ultimately lead to more personalized strategies for sleep, work schedules, and mental health support.”

For further details, refer to the published findings in the Journal on December 22, 2025, Nature Communications.

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L. Joe et al. (2025). Potential brain subtypes of chronotypes reveal unique behavioral and health profiles across population cohorts. Nat Commune 16, 11550; doi: 10.1038/s41467-025-66784-8

Source: www.sci.news

How Early Cancer Treatment Before 3 PM Can Increase Patient Survival Rates

Timing Cancer Treatment: A Simple Yet Effective Intervention

Kenneth K. Lam/ZUMA Press/Alamy

The first randomized controlled trial investigating the timing of cancer immunotherapy has revealed that administering treatment earlier in the day may significantly enhance patient survival rates.

Human cells and tissues operate on a 24-hour cycle, known as the circadian rhythm, influencing various bodily functions including mood, metabolism, and immune response.

Numerous observational studies have indicated that cancer patients receiving checkpoint inhibitors (a class of immunotherapy drugs that empower the immune system to combat cancer) earlier in the day show a lower risk of disease progression and mortality.

Recently, Francis Levy and his team at the University of Paris-Saclay, France, conducted the first randomized controlled trial focused on chronotherapy—timing treatments based on circadian rhythms—utilizing both chemotherapy and immunotherapy.

In this study, 210 patients diagnosed with non-small cell lung cancer were given four doses of either pembrolizumab or sintilimab, two checkpoint inhibitors that function similarly.

Every three weeks, half of the participants received their doses before 3 p.m., while the others received treatments later. All patients also received chemotherapy immediately after each immunotherapy session. Chemotherapy targets rapidly dividing cells and is believed to have a lesser connection to circadian rhythms than immunotherapy.

This timing was strictly adhered to during the initial four cycles of the combined immunochemotherapy treatments. Following this period, all participants continued receiving the same medications until their tumors advanced or no longer responded, but without specific timing guidelines. Previous research suggests that the first four cycles are crucial, as noted by team member Zhang Yongchang from Central South University, China.

Participants were monitored for an average of 29 months post-initial treatment. Results showed that those treated before 3 p.m. had a median survival of 28 months, compared to 17 months for those treated later in the day. “The results are dramatically positive,” Levy stated. “Survival time nearly doubles.”

“When we compare our findings to significant trials that resulted in new drug approvals, such large effects are rarely observed,” noted Pasquale Innominato from the University of Warwick, UK. He emphasized that the study demonstrates a definitive link between treatment timing and survival outcomes, deeming it solid evidence of causation.

This dramatic improvement may be attributed to T cells, a type of immune cell targeted by checkpoint inhibitors, which tend to accumulate near tumors in the morning and gradually enter the bloodstream later. Administering immunotherapy earlier could position T cells closer to tumors, enabling more effective destruction, according to Levy.

Levy also emphasized the need for further studies to explore if more precise timing, such as 11 a.m., offers additional advantages compared to broader scheduled treatments. Innominato pointed out that having flexibility in timing is advantageous for busy healthcare facilities.

Further investigation is necessary to determine whether managing the timing of chemoimmunotherapy beyond the first four cycles yields greater benefits, Levy mentioned. Individual variability could also play a critical role; for example, a morning person may have different immune responses compared to a night owl.

Whether these findings apply to various cancer types remains an open question. Innominato anticipates similar results in other tumors commonly treated with immunotherapy, like skin or bladder cancers, but tempered his expectations for tumors such as prostate or pancreatic cancers that often resist treatments.

Topics:

Source: www.newscientist.com

Neanderthal and Early Human Interbreeding Across Wide Regions: What the Evidence Shows

Artist’s Impression of Neanderthal Life

Christian Jegou/Science Photo Library

Homo sapiens and Neanderthals likely interbred across a vast region, extending from Western Europe to Asia.

Modern humans (Homo sapiens) and Neanderthals (Homo neanderthalensis) exhibited mixed ancestry, with most non-Africans today possessing Neanderthal DNA, approximating 2% of their genome. Neanderthals also engaged in interbreeding, leading to a lineage shift in the Y chromosome influenced by Homo sapiens.

Despite increasing knowledge about the timing of this hybridization, the specific regions and scales of these interactions long remained a mystery. Ancestors of Neanderthals departed Africa around 600,000 years ago, migrating toward Europe and Western Asia. The first evidence of Homo sapiens moving from Africa includes skeletal remains from sites in modern-day Israel and Greece, dating to approximately 200,000 years ago.

Evidence suggests that Homo sapiens contributed genetically to the Neanderthal population in the Altai Mountains around 100,000 years ago. However, the primary wave of migration from Africa occurred over 60,000 years ago. Recent studies utilizing ancient genomic data indicate that significant gene flow between Homo sapiens and Neanderthals began around 50,000 years ago, with findings documented in studies of 4000 and 7000 gene transfers.

This interaction is thought to have primarily taken place in the eastern Mediterranean, although pinpointing the exact locations remains challenging.

To investigate, Matthias Karat and his team from the University of Geneva analyzed 4,147 ancient genetic samples from over 1,200 locations, with the oldest dating back approximately 44,000 years. They studied the frequency of genetic mutations (introgression alleles) originating from Neanderthal DNA that were passed down through hybridization.

“Our objective was to use Neanderthal DNA integration patterns in ancient human genomes to determine the sites of hybridization,” Carlat explains.

Findings revealed that the proportion of transferred DNA increased gradually as one moved away from the eastern Mediterranean region, plateauing approximately 3,900 kilometers westward into Europe and eastward into Asia.

“We were surprised to identify a distinct pattern of increasing introgression rates in the human genome, likely linked to human expansion from Africa,” Carlat notes. “This increase toward Europe and East Asia allows us to estimate the parameters of this hybrid zone.”

Computer simulations showed a hybrid zone potentially spanning much of Europe and the eastern Mediterranean, extending into western Asia.

Interbreeding Zone between Neanderthals and Homo sapiens

Lionel N. Di Santo et al. 2026

“Our findings suggest a continuous series of interbreeding events across both space and time,” notes Carlat. “However, the specifics of mating occurrences in this hybrid zone remain unknown.”

This hybrid zone encompasses nearly all known Neanderthal remains found across Western Eurasia, with the exception of the Altai region.

“The extensive geographical breadth of the putative hybrid zone suggests widespread interactions among populations,” states Leonard Yasi from the Max Planck Institute for Evolutionary Anthropology in Leipzig, Germany.

Notably, the Atlantic periphery—including western France and much of the Iberian Peninsula—was not part of the hybrid zone, despite the established presence of Neanderthals in these regions. Currat suggests that interbreeding may not have occurred here or may not be reflected in the analyzed genetic samples.

“This study reveals ongoing interactions between modern humans and Neanderthals over extensive geographical areas and extended periods,” adds Yasi. The hybrid zone may extend further, though limited ancient DNA sampling in regions like the Arabian Peninsula complicates assessment of its reach.

“This pivotal research challenges the notion that interbreeding occurred only in one area of West Asia with a singular Neanderthal population (not represented in existing genetic samples). Homo sapiens appear to have dispersed from Africa in increasing numbers across expanding territories, likely outcompeting smaller Neanderthal groups they encountered throughout most of the recognized Neanderthal range,” comments Chris Stringer from the Natural History Museum in London.

Topics:

  • Neanderthal Man/
  • Ancient Humans

Source: www.newscientist.com

Ancient Wooden Tool: The Oldest Known Stick Shaped by Early Humans

Reconstruction of a Paleolithic woman crafting wooden tools

Credit: G. Prieto; K. Harvati

Remarkably, some of the oldest known wooden tools have been unearthed in an open-pit mine in Greece, dating back 430,000 years. These artifacts were likely crafted by an ancient human ancestor, potentially related to Neanderthals.

Archaeologists note that prehistoric wooden artefacts are “extremely rare.” According to Dirk Leder from the Lower Saxony Cultural Heritage Office in Hannover, Germany, any new findings in this area are highly valued.

Evidence suggests our extinct relatives may have utilized wooden tools for millions of years. “This could be the oldest type of tool ever used,” states Katerina Harvati from the University of Tübingen, Germany. Unfortunately, the preservation of wooden artifacts is often poor, hindering our understanding of their use.

Harvati and her team discovered the tool at a site called Marathusa 1, originally confirmed in 2013 in the Megalopolis Basin of southern Greece. The open-pit lignite mine revealed sediment layers that are nearly a million years old, offering unprecedented access to date and research, as mentioned by researcher K. Harvati.

From 2013 to 2019, excavations yielded not only tools but also the skeleton of a straight-tusked elephant (Paleoloxodon antiquus), indicating a rich archaeological context with evidence of activity, including more than 2,000 stone tools and remains of varied flora and fauna, depicting an ancient lakeshore ecosystem.


To date Marathusa 1, researchers relied on various methods, including analyzing fossil footprints and historical changes in the Earth’s magnetic field. By 2024, they confirmed that the artefacts are around 430,000 years old, a time marked by challenging climatic conditions—the gravest ice age of the Pleistocene in Europe. The Megalopolis Basin likely provided refuge due to its relatively temperate climate.

The archaeological team identified two significant wooden tools among the 144 artifacts. The first, an 81 cm long pole made from alder, exhibits marks indicative of intentional shaping. One end appears rounded, possibly serving as a handle, while the other is flattened, hinting at potential use for digging underground tubers or perhaps for butchering elephant carcasses. Harvati admits uncertainty about its exact application.

Mysterious second wooden tool from Marathusa 1

Credit: N. Thompson; K. Harvati

The second tool remains enigmatic, measuring just 5.7 cm in length and made from willow or poplar. It also shows signs of intentional shaping after the bark was removed. According to Harvati, this represents a completely new type of wooden tool. While it might have served to modify stone tools, the specific purpose remains a mystery.

Reeder points out that while the first tool is a clear example of wooden craftsmanship, questions remain about the functionality of the second. “Is this a complete item or part of something larger?” he muses.

No hominid remains have been found at Marathusa 1. Given its age, it predates our species and is likely too early even for Neanderthals. “The prevailing hypothesis suggests this site might be associated with pre-Neanderthal humans or Homo heidelbergensis. However, Harvati cautions against making definitive conclusions, noting that Greece was frequented by various hominin groups.

Other ancient wooden tools, like the Clacton spear discovered in Britain, are estimated to be about 400,000 years old, while a wooden spear from Schöningen, Germany, has been dated using multiple methods to around 300,000 years. The only tools that predate those found at Marathusa 1 are from Kalambo Falls in Zambia, which date back 476,000 years and resemble remains of larger structures or buildings.

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Revolutionary Cosmological Simulations Illuminate Black Hole Growth in the Early Universe

Revolutionary simulations from Maynooth University astronomers reveal that, at the onset of the dense and turbulent universe, “light seed” black holes could swiftly consume matter, rivaling the supermassive black holes found at the centers of early galaxies.

Computer visualization of a baby black hole growing in an early universe galaxy. Image credit: Maynooth University.

Dr. Daksar Mehta, a candidate at Maynooth University, stated: “Our findings indicate that the chaotic environment of the early universe spawned smaller black holes that underwent a feeding frenzy, consuming surrounding matter and eventually evolving into the supermassive black holes observed today.”

“Through advanced computer simulations, we illustrate that the first-generation black holes, created mere hundreds of millions of years after the Big Bang, expanded at astonishing rates, reaching sizes up to tens of thousands of times that of the Sun.”

Dr. Louis Prowl, a postdoctoral researcher at Maynooth University, added: “This groundbreaking revelation addresses one of astronomy’s most perplexing mysteries.”

“It explains how black holes formed in the early universe could quickly attain supermassive sizes, as confirmed by observations from NASA/ESA/CSA’s James Webb Space Telescope.”

The dense, gas-rich environments of early galaxies facilitated brief episodes of “super-Eddington accretion,” a phenomenon where black holes consume matter at a rate faster than the norm.

Despite this rapid consumption, the black holes continue to devour material effectively.

The results uncover a pivotal “missing link” between the first stars and the immense black holes that emerged later on.

Mehta elaborated: “These smaller black holes were previously considered too insignificant to develop into the gigantic black holes at the centers of early galaxies.”

“What we have demonstrated is that, although these nascent black holes are small, they can grow surprisingly quickly under the right atmospheric conditions.”

There are two classifications of black holes: “heavy seed” and “light seed.”

Light seed black holes start with a mass of only a few hundred solar masses and must grow significantly to transform into supermassive entities, millions of times the mass of the Sun.

Conversely, heavy seed black holes begin life with masses reaching up to 100,000 times that of the Sun.

Previously, many astronomers believed that only heavy seed types could account for the existence of supermassive black holes seen at the hearts of large galaxies.

Dr. John Regan, an astronomer at Maynooth University, remarked: “The situation is now more uncertain.”

“Heavy seeds may be rare and depend on unique conditions for formation.”

“Our simulations indicate that ‘garden-type’ stellar-mass black holes have the potential to grow at extreme rates during the early universe.”

This research not only reshapes our understanding of black hole origins but also underscores the significance of high-resolution simulations in uncovering the universe’s fundamental secrets.

“The early universe was far more chaotic and turbulent than previously anticipated, and the population of supermassive black holes is also more extensive than we thought,” Dr. Regan commented.

The findings hold relevance for the ESA/NASA Laser Interferometer Space Antenna (LISA) mission, set to launch in 2035.

Dr. Regan added, “Future gravitational wave observations from this mission may detect mergers of these small, rapidly growing baby black holes.”

For further insights, refer to this paper, published in this week’s edition of Nature Astronomy.

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D.H. Meter et al. Growth of light seed black holes in the early universe. Nat Astron published online on January 21, 2026. doi: 10.1038/s41550-025-02767-5

Source: www.sci.news

Astrophysicists Discover ‘Little Red Dot’ as Early Universe’s Young Supermassive Black Hole

Astrophysicists from the University of Copenhagen have discovered that the enigmatic “little red dots” visible in images of the early universe are rapidly growing black holes shrouded in ionized gas. This groundbreaking finding offers significant insights into the formation of supermassive black holes after the Big Bang.



The small red dot is a young supermassive black hole encased in a dense ionized cocoon. Image credits: NASA / ESA / CSA / Webb / Rusakov et al., doi: 10.1038/s41586-025-09900-4.

Since the launch of the NASA/ESA/CSA James Webb Space Telescope in 2021, astronomers globally have been studying the red spots that appear in regions of the sky corresponding to the universe just a few hundred million years after the Big Bang.

Initial interpretations ranged from unusually massive early galaxies to unique astrophysical phenomena that challenged existing formation models.

However, after two years of extensive analysis, Professor Darach Watson and his team from the University of Copenhagen have confirmed that these points represent young black holes surrounded by a thick cocoon of ionized gas.

As these black holes consume surrounding matter, the resulting heat emits powerful radiation that penetrates the gas, creating a striking red glow captured by Webb’s advanced infrared camera.

“The little red dot is a young black hole, approximately 100 times less massive than previously estimated, encased in a gas cocoon and actively consuming gas to expand,” stated Professor Watson.

“This process generates substantial heat, illuminating the cocoon.”

“The radiation that filters through the cocoon provides these tiny red dots with their distinctive color.”

“These black holes are significantly smaller than previously thought, so there’s no need to introduce entirely new phenomena to explain them.”

Despite being the smallest black holes ever detected, these objects still weigh up to 10 million times more than the Sun and measure millions of kilometers in diameter, shedding light on how black holes accelerated their growth during the early universe.

Black holes typically operate inefficiently, as only a small fraction of the gas they attract crosses the event horizon. Much is blown back into space as high-energy outflows.

However, during this early phase, the surrounding gas cocoon serves as both a fuel source and a spotlight, enabling astronomers to observe a black hole in intense growth like never before.

This discovery is crucial for understanding how supermassive black holes, such as the one at the center of the Milky Way, grew so quickly in the universe’s first billion years.

“We observed a young black hole in a growth spurt at a stage never documented before,” Professor Watson remarked.

“The gas-dense cocoon around them supplies the rapid growth fuel they require.”

For more details, see the findings featured in this week’s edition of Nature.

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V. Rusakov et al. 2026. A small red dot like a young supermassive black hole inside a dense ionized cocoon. Nature 649, 574-579; doi: 10.1038/s41586-025-09900-4

Source: www.sci.news

NASA Astronaut Exits Space Station Early Over Health Concerns, Resulting in Droplets Falling

Four astronauts successfully returned to Earth early Thursday morning, concluding an eventful and extraordinary week in space. The crew made an early departure from the International Space Station as a result of medical issues that emerged during their mission.

NASA astronauts Zena Cardman, Mike Finke, Japanese astronaut Kamiya Yui, and Russian cosmonaut Oleg Platonov made a splashdown in the Pacific Ocean near San Diego at 3:41 a.m. ET after an 11-hour journey.

“On behalf of SpaceX and NASA, welcome home, Crew-11,” mission controllers communicated to the astronauts shortly after the Dragon capsule’s touchdown.

This return marks a historic moment, being the first instance in the ISS’s 25-year history where a mission was terminated early due to medical complications.

On Thursday, SpaceX’s Crew Dragon Endeavor spacecraft splashed down in the Pacific Ocean near San Diego, California.
NASA

Out of respect for medical privacy, NASA has not disclosed the identities of the crew members involved or specific details surrounding the medical incident. The situation remains stable and is not deemed an emergency.

NASA Administrator Jared Isaacman stated in a recent press conference that the early return decision was made with an emphasis on precaution.

The medical issue led to the cancellation of a planned spacewalk scheduled for January 8, during which Cardman and Finke were set to perform modifications outside the ISS.

The recovery team approaches the Dragon capsule.
NASA

Prior to leaving the space station, Finke reassured that he and his colleagues were “stable, safe, and well cared for.”

“This decision was made to facilitate proper medical evaluation in a controlled environment with complete diagnostic capabilities,” Finke mentioned in a statement on LinkedIn. “While it’s bittersweet, it’s the right call.”

The astronauts returned in the same SpaceX Dragon capsule that had transported them to the ISS.

The return mission proceeded without incident, with air traffic controllers reporting favorable weather conditions at the landing site off the California coast. The capsule’s drogue and main parachutes deployed successfully just before landing, ensuring a safe splashdown.

NASA’s Crew 11 Endeavor spacecraft during recovery efforts.
NASA

SpaceX recovery teams promptly arrived to assess the capsule and ensure it was safe to open the hatch. Dolphins were also spotted joyfully swimming in the vicinity.

The Crew-11 astronauts spent 165 days aboard the space station. For Cardman and Platonov, this represents their first spaceflight, while Yui has now completed her second journey. Finke has successfully finished four missions in total.

The astronauts were scheduled to stay on the ISS until late February but returned early, leaving only three crew members onboard: NASA’s Chris Williams and Russian cosmonauts Sergei Kud-Sverchkov and Sergei Mikayev.

Inside the International Space Station’s Kibo Experiment Module: NASA astronaut Mike Finke, Roscosmos cosmonaut Oleg Platonov, NASA astronaut Zena Cardman, and JAXA astronaut Kamiya Yui.
NASA/AP

The next crew rotation for the space station is expected to launch by February 15, but NASA is exploring options for an expedited flight. Nonetheless, Williams is likely to be the only NASA astronaut responsible for U.S. scientific experiments and operations at the station for several weeks to come.

Source: www.nbcnews.com

SEO-Optimized Title: “The Late Ordovician Mass Extinction: How It Laid the Foundation for the Evolution of Early Fish”

A significant enigma in vertebrate evolution—why numerous major fish lineages appeared suddenly in the fossil record tens of millions of years post their presumed origins—has been linked to the Late Ordovician mass extinction (LOME). This insight comes from a recent analysis conducted by paleontologists at the Okinawa Institute of Science and Technology Graduate University. The study reveals that the LOME, occurring approximately 445 to 443 million years ago, instigated a parallel endemic radiation of jawed and jawless vertebrates (gnathostomes) within isolated refugia, ultimately reshaping the early narrative of fishes and their relatives.

Reconstruction of Sacabambaspis jamvieri, an armored jawless fish from the Ordovician period. Image credit: OIST Kaori Seragaki

Most vertebrate lineages initially documented in the mid-Paleozoic emerged significantly after the Cambrian origin and Ordovician invertebrate biodiversity. This temporal gap is often attributed to inadequate sampling and lengthy ghost lineages.

However, paleontologists Kazuhei Hagiwara and Lauren Saran from the Okinawa Institute of Science and Technology Graduate University propose that the LOME may have fundamentally transformed the vertebrate ecosystem.

Utilizing a newly compiled global database of Paleozoic vertebrate occurrences, biogeography, and ecosystems, they identified that this mass extinction coincided with the extinction of stylostome conodonts (extinct marine jawless vertebrates) and the decline of early gnathostomes and pelagic invertebrates.

In the aftermath, the post-extinction ecosystems witnessed the initial definitive emergence of most major vertebrate lineages characteristic of the Paleozoic ‘Age of Fish’.

“While the ultimate cause of LOME remains unclear, clear changes before and after the event are evident through the fossil record,” stated Professor Saran.

“We have assimilated 200 years of Late Ordovician and Early Silurian paleontology and created a novel database of fossil records that will assist in reconstructing the refugia ecosystem,” Dr. Hagiwara elaborated.

“This enables us to quantify genus-level diversity from this era and illustrate how LOME directly contributed to a significant increase in gnathostome biodiversity.”

LOME transpired in two pulses during a period marked by global temperature fluctuations, alterations in ocean chemistry—including essential trace elements—sudden polar glaciation, and fluctuations in sea levels.

These transformations severely impacted marine ecosystems, creating post-extinction ‘gaps’ with reduced biodiversity that extended until the early Silurian period.

The researchers confirmed a previously suggested gap in vertebrate diversity known as the Thalimar gap.

Throughout this time, terrestrial richness remained low, and the surviving fauna consisted largely of isolated microfossils.

The recovery was gradual, with the Silurian period encompassing a 23-million-year recovery phase during which vertebrate lineages diversified intermittently.

Silurian gnathostome lineages displayed gradual diversification during an early phase when global biodiversity was notably low.

Early jawed vertebrates appear to have evolved in isolation rather than rapidly dispersing into ancient oceans.

The researchers noted that gnathostomes exhibited high levels of endemism from the outset of the Silurian period, with diversification occurring primarily in certain long-term extinction reserves.

One such refuge is southern China, where the earliest conclusive evidence of jaws is present in the fossil record.

These primitive jawed vertebrates remained geographically restricted for millions of years.

Turnover and recovery following LOME paralleled climatic fluctuations similar to those at the end of the Devonian mass extinction, including prolonged epochs of low diversity and delayed dominance of jawed fishes.

“For the first time, we discovered the entire body fossil of a jawed fish directly related to modern sharks in what is now southern China,” Dr. Hagiwara noted.

“They remained concentrated in these stable refugia for millions of years until they evolved the capability to migrate across open oceans to new ecosystems.”

“By integrating location, morphology, ecology, and biodiversity, we can finally understand how early vertebrate ecosystems restructured themselves after significant environmental disruptions,” Professor Saran added.

“This study elucidates why jaws evolved, why jawed vertebrates ultimately became widespread, and how modern marine life originated from these survivors rather than earlier forms like conodonts and trilobites.”

For more information, refer to the study published on January 9th in Scientific Progress.

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Kazuhei Hagiwara & Lauren Saran. 2026. The mass extinction that initiated the irradiation of jawed vertebrates and their jawless relatives (gnathostomes). Scientific Progress 12(2); doi: 10.1126/sciadv.aeb2297

Source: www.sci.news

NASA Schedules Astronauts’ Early Departure from ISS Amid Medical Concerns

NASA has announced plans to return four astronauts from the International Space Station (ISS) earlier than initially scheduled due to a crew member’s health issue encountered in orbit.

According to a statement released by NASA late Friday, the undocking from the ISS is set to take place by 5 p.m. ET on Wednesday, weather permitting at the designated splashdown site off California’s coast.

This marks the first occasion in the 25-year history of the ISS that a mission has been interrupted due to a medical incident in space.

While NASA confirmed a medical issue arose earlier this week, specific details regarding the crew member’s condition or identity have not been disclosed, citing medical privacy regulations.

During a news conference on Thursday, agency officials reassured that the situation is stable, and the decision for early departure is a precautionary measure rather than an emergency evacuation.

NASA Administrator Jared Isaacman stated, “After consulting with Chief Medical Officer Dr. J.D. Polk and agency leaders, we concluded that it’s best for the astronauts to return Crew-11 ahead of schedule.”

The returning crew includes NASA astronauts Zena Cardman and Mike Finke, Japanese astronaut Kamiya Yui, and Russian cosmonaut Oleg Platonov. Crew-11 was initially slated to reach the ISS in early August and remain in the laboratory until late February.

The astronauts will return in the same SpaceX Dragon capsule that transported them to the ISS. If all goes as planned, undocking will occur Wednesday night, with an expected splashdown in the Pacific Ocean around 3:40 a.m. Thursday.

NASA and SpaceX will provide further updates on the precise landing time and location as it gets closer to the undocking.

Post Crew-11’s departure, NASA will maintain one astronaut aboard the ISS to oversee U.S. scientific experiments and operations. Flight engineer Chris Williams launched aboard a Russian Soyuz spacecraft on November 27th and will be joined by Russian cosmonauts Sergei Kud-Sverchkov and Sergei Mikayev.

The next crew is scheduled to launch to the ISS in mid-February, with NASA considering enhancements to this mission, known as Crew-12.

Source: www.nbcnews.com

NASA to Return Space Station Astronauts Early Due to Medical Concerns

NASA has announced that four astronauts aboard the International Space Station (ISS) will return to Earth over a month early due to medical issues. This unprecedented evacuation marks the first of its kind in the ISS’s 25-year history.

Due to medical privacy regulations, NASA refrained from disclosing specific details, including the identities of the affected astronauts and the nature of their medical conditions. However, officials confirmed that the overall situation remains stable.

Speaking at a recent news conference, NASA Administrator Jared Isaacman stated that the astronauts are expected to return home in the coming days. An exact timeline for undocking and landing has not yet been provided.

“After consulting with Medical Officer of Health Dr. J.D. Polk and leadership across the agency, we believe returning Crew-11 early is in the best interest of the astronauts,” Isaacman said in a statement.

Inside the International Space Station.
NASA

Isaacman noted that further updates would be available within the next 48 hours.

The Crew-11 team evacuating the ISS consists of NASA astronauts Zena Cardman and Mike Finke, Japanese cosmonaut Kamiya Yui, and Russian cosmonaut Oleg Platonov. They had originally arrived in early August with plans to stay until late February.

Dr. Polk reassured the public that the situation is stable, clarifying that the decision to evacuate was made for the well-being of the astronauts, not due to an emergency.

“While the ISS is equipped with sophisticated medical technology, it cannot match the complete resources of a hospital emergency department for thorough patient evaluations,” Polk explained. “In this case, there were multiple medical events which necessitated a careful assessment of the astronauts’ health.”

NASA first made the medical concerns public on Wednesday, when it was revealed that Cardman and Finke were deferring a scheduled spacewalk.

Following the early return of Crew-11, NASA will operate with just one astronaut on the ISS, who will oversee ongoing U.S. scientific operations. Flight engineer Chris Williams launched aboard a Russian Soyuz spacecraft on November 27, accompanied by Russian cosmonauts Oleg Platonov, Sergei Kud-Sverchkov, and Sergei Mikayev.

The subsequent crew is slated to launch to the ISS in mid-February, but Isaacman indicated that NASA may evaluate enhancements for this upcoming mission, known as Crew-12.

This week’s developments present Isaacman’s first significant challenge since taking office on December 18.

Source: www.nbcnews.com

Evidence Suggests Early Humans Began Hunting Elephants 1.8 Million Years Ago

Homo heidelbergensis hunting elephant

Ancient Humans Hunting Elephants—Evidence of Slaughtering Animals 1.8 Million Years Ago

Natural History Museum/Scientific Photography Library

Hunting an elephant is a formidable challenge, necessitating advanced tools and teamwork, offering an abundant source of protein.

A research team led by Manuel Dominguez-Rodrigo from Rice University in Texas suggests that ancient humans may have accomplished this feat approximately 1.78 million years ago in Tanzania’s Olduvai Gorge.

“Around 2 million years ago, our ancestors consistently consumed smaller game like gazelles and waterbucks but did not target larger prey,” says Dominguez-Rodrigo.

Later findings from Olduvai Gorge indicate a significant shift. This valley, abundant with both animal and human fossils formed over the past 2 million to 17,000 years, shows a marked increase in elephant and hippopotamus remains around 1.8 million years ago. However, establishing conclusive evidence of human involvement in hunting remains elusive.

In June 2022, Dominguez-Rodrigo and his team discovered what may be an ancient elephant slaughterhouse at Olduvai.

The site, dubbed the EAK site, revealed partial remains of an extinct elephant species, Elephas reki, surrounded by an array of stone tools that were much larger and sturdier than those utilized by hominins 2 million years ago. Dominguez-Rodrigo posits these tools were likely crafted by the ancient hominin Homo erectus.

“These include Pleistocene knives, known for their sharpness even today,” he notes, emphasizing their potential for butchering tasks.

Dominguez-Rodrigo and his colleagues believe these stone tools facilitated elephant slaughter. Some limb bones appear to have fractured shortly after the elephant’s demise, indicating the bones were still fresh or “green.” Unlike scavengers like hyenas that can strip meat, they can’t shatter the dense bone shafts of mature elephants.

“We discovered numerous bones in the field with fresh fractures, pointing to human use of hammer stones for processing,” he states. “These ‘green’ fractured bones are widespread in the 1.7-million-year-old landscape and bear distinct impact marks.”

However, there is a scarcity of cut marks on bones, which typically indicate butchering practices to extract meat.

It remains uncertain whether humans actively hunted the elephants or merely scavenged existing carcasses.

“What we can confirm is that they disassembled the bones—or portions of them—leaving behind tools and bones as evidence,” affirms Dominguez-Rodrigo.

He adds that the transition to hunting elephants wasn’t merely due to advancements in stone tools, but also hinted at an increase in social structure and cultural development among hominin groups.

However, Michael Pante, a researcher at Colorado State University, remains skeptical of the findings.

Pante contends that the evidence for human exploitation of this individual elephant is weak. The interpretation relies heavily on the proximity of stone tools and elephant remains, as well as the inferred fractures created by human attempts to access bone marrow.

Pante asserts that the earliest definitive evidence of hippo, giraffe, and elephant hunting in Olduvai dates back to around 80,000 years ago, as shown in the research of the 1.7-million-year-old HWK EE site.

“In contrast to the EAK site, the bones at HWK EE exhibit cut marks and are associated with thousands of other bones and artifacts within an archaeological context,” he explains.

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How El Niño Triggered Famine in Early Modern Europe: Uncovering the Climate Crisis’ Impact

Impact of El Niño on Crop Failures

El Niño’s Impact on European Agriculture: Crop Failures and Price Hikes

Public Domain

El Niño, a climate phenomenon affecting the Pacific Ocean region, significantly influenced the economy and climate of Europe, resulting in widespread famine from 1500 to 1800.

During El Niño, the warming of ocean waters in the central and eastern Pacific disrupts trade winds, which leads to altered global rainfall patterns. The cooling phase, known as La Niña, and the oscillation between these two phases is referred to as the El Niño Southern Oscillation (ENSO).

This climatic variation poses severe risks in tropical and subtropical areas, notably in Australia, where it can lead to droughts and wildfires, and in the Americas, where it causes increased rainfall.

However, until recently, the focus on El Niño’s effects on Europe was minimal. Emil Esmaili from Columbia University and his research team studied records from 160 famines in early modern Europe, correlating them with El Niño and La Niña data derived from tree rings.

The findings revealed that over 40% of famines in Central Europe during this era were directly linked to El Niño events.

El Niño typically increases rainfall in the region, which can lead to excess soil moisture, resulting in crop failures. Though it did not directly trigger famine in other European areas, it raised the likelihood of famine occurrences by 24% across all nine regions studied.

To better understand this correlation, Esmaili’s team assessed grain and fish prices, discovering that El Niño significantly drove up food prices throughout Europe for several years.

Researchers, including David Yubilaba from the University of Sydney, indicate that ENSO events can still lead to food insecurity and malnutrition in low-income households in regions such as South Asia, Southeast Asia, Oceania, and parts of Africa.

While El Niño continues to influence the climate in Europe, its impact on food security is expected to be less severe today. “Modern agricultural practices are now more resilient, weather forecasting has greatly improved, and markets have become more consolidated,” says Ubilaba.

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Mysterious Blob in Early Universe Heats Up: Unraveling the Mystery Behind It

Galaxy Cluster SPT2349-56

This galaxy cluster must be much, much colder than it actually is.

Lingxiao Yuan

Recent discoveries about young galaxy clusters, such as SPT2349-56, are transforming our understanding of how these colossal structures formed and evolved in the early universe. Interestingly, the gas within SPT2349-56 is significantly hotter and denser than anticipated, posing intriguing questions for researchers.

Zhou Daizhi and their team at the University of British Columbia utilized the Atacama Large Millimeter/submillimeter Array (ALMA) in Chile to investigate this galaxy cluster. Their findings revealed that the gas at the cluster’s center reaches temperatures of tens of millions of degrees Celsius.

“The sun’s surface temperature is just a few thousand degrees Celsius, making this region much hotter,” Zhou notes. “Our conservative estimates indicate temperatures five to ten times higher than expected based on simulations, which is surprising since such hot gas was thought to exist only in clusters billions of years old.”

Located in the early universe, approximately 1.4 billion years after the Big Bang, SPT2349-56 is unlike any other known cluster of its age. Zhou explains, “This gas should still be relatively cold and in small quantities, as these nascent clusters are still in the process of accumulating gas and heating up.” However, SPT2349-56 seems to be more mature than anticipated.

The unusual heating could stem from the presence of particularly active galaxies within the cluster, with at least three galaxies emitting massive jets of energy. These jets, combined with intermittent star formation bursts, might be heating the gas rapidly, challenging previous assumptions.

“This discovery opens a new window into understanding stages of cluster evolution that we have not observed before,” Zhou emphasizes. The research team plans additional observations to locate more hot young clusters like SPT2349-56, with the hope of unraveling the complexities of galaxy formation.

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Fossil Analysis Sheds Light on Early Human Walking Evolution: Expanding the Debate

Comparison of Sahelanthropus fossils with chimpanzees and humans

Sahelanthropus: Fossil comparison with chimpanzees and humans

Williams et al., Sci. Adv. 12, eadv0130

The long-standing debate regarding whether our earliest ancestors walked on knuckles like chimpanzees or stood upright like modern humans may be closer to resolution, yet skepticism remains.

Scott Williams and researchers at New York University recently reanalyzed fossil remains of Sahelanthropus tchadensis, indicating that this species possessed at least three anatomical features suggesting it was our earliest known bipedal ancestor.

The journey to this conclusion has been extensive.

Fossilized remains of a skull, teeth, and jawbone from approximately 7 million years ago were first identified in 2002 in Chad, north-central Africa. The distinctive features of this ancient species, including its prominent brow ridge and smaller canine teeth, were quickly acknowledged as diverging from ape characteristics.

Analyzing the skull’s anatomy suggests it was positioned directly over the vertebrae, analogous to other upright, bipedal hominins.

In 2004, French scientists uncovered the femur and ulna associated with the Sahelanthropus skull from Chad. However, it wasn’t until 2020 that researchers claimed the femur exhibited curvature similar to that of non-bipedal great apes.

Since then, scholarly debate has fluctuated. For instance, in 2022, researchers Frank Guy and Guillaume Daver of the University of Poitiers argued for anatomical features of the femur that indicate bipedalism. In 2024, Clement Zanoli and colleagues from the University of Bordeaux countered, suggesting Guy and Daver’s assertions were flawed, as the anatomical characteristics of bipedalism may also appear in non-bipedal great apes.

Lead study author Williams started with a “fairly ambivalent” stance on Sahelanthropus.

His team investigated the femur’s attachment point for the gluteus maximus muscle, finding similarities to human femur anatomy.

They also compared the femur and ulna size and shape; while similar in size to chimpanzee bones, they aligned more closely with human proportions.

Additionally, they identified the “femoral tuberosity,” a previously overlooked feature of Sahelanthropus.

“We initially identified it by touch, later confirming it with 3D scans of the fossil,” Williams shared. “This bump, present only in species with a femoral tubercle, contrasts smooth areas found in great apes and plays a critical role in mobility.”

This area serves as an attachment point for the iliofemoral ligament, the strongest ligament in the human body. While relaxed when seated, it tightens during standing or walking, securing the femoral head in the hip joint and preventing the torso from tilting backward or sideways.

However, Williams expressed doubts about whether this study would fully end the conversation about how Sahelanthropus moved.

“We are confident Sahelanthropus was an early bipedal hominin, but we must recognize that the debate is ongoing,” Williams noted.

In response to a recent paper, Guy and Daver issued a joint statement asserting that humans likely began walking on two legs by 2022: “This reaffirms our earlier interpretations about Sahelanthropus adaptations and locomotion, suggesting habitual bipedalism despite its ape-like morphology.”

They acknowledged that only new fossil discoveries could unequivocally conclude the matter.

John Hawkes, a professor at the University of Wisconsin-Madison, also endorsed the new findings, noting their implications for understanding the complex origins of the hominin lineage.

“It may be deceptive to perceive Sahelanthropus as part of a gradual evolution towards an upright posture. It reveals crucial insights into these transformative changes,” Hawkes commented.

However, Zanoli contended, stating, “Most of the evidence aligns Sahelanthropus with traits seen in African great apes, suggesting its behavior was likely a mix between chimpanzees and gorillas, distinct from the habitual bipedalism of Australopithecus and Homo.

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Massive Black Holes: Potential Remnants from the Early Universe Explained

Primordial black holes likely formed shortly after the Big Bang.

Shutterstock/Mohd. Afuza

An exceptionally massive black hole from the early universe may represent a type of exotic starless black hole first theorized by Stephen Hawking.

In August, Boyuan Liu and his team from the University of Cambridge used the James Webb Space Telescope (JWST) to uncover a peculiar galaxy named Abell 2744-QSO1. This ancient galaxy, dating back 13 billion years, harbored a black hole around 50 million times the mass of our Sun but hosted extremely few stars.

“This contradicts traditional theories which dictate that stars must form prior to or simultaneously with black holes,” Liu explained. Typically, black holes are believed to evolve when massive stars exhaust their fuel and undergo gravitational collapse.

Liu and his team conducted initial simulations suggesting that QSO1 might have originated as a primordial black hole—an exotic concept introduced by Stephen Hawking and Bernard Carr in 1974. Unlike conventional black holes, primordial black holes are thought to form from density fluctuations shortly after the Big Bang.

While most primordial black holes likely evaporated by the time of the JWST’s observations, some might have persisted, evolving into larger black holes like QSO1.

Although Liu and his team’s calculations align broadly with their observations, they remain relatively simple and do not factor in the intricate interactions among primordial black holes, gas clouds, and stars.

Now, the authors have employed advanced simulations to investigate how primordial black holes grew in the universe’s infancy. They analyzed how gas dynamics influenced the formation of early primordial black holes and how interactions with newly formed and dying stars affected them.

Their predictions about the black hole’s ultimate mass and the heavy elements present in it are congruent with the findings from QSO1.

“It’s not conclusive, but it represents a compelling possibility,” Liu stated. “These observations suggest that established black hole formation theories may not fully explain the phenomenon, making the notion of a significant primordial black hole in the early universe increasingly plausible.”

Simulations indicate that primordial black holes could be a feasible origin for QSO1, according to Roberto Maiorino, a team member involved in the discovery of black holes. “The alignment of their predicted properties with those of QSO1, in terms of black hole mass, stellar mass, and chemical composition, is both intriguing and promising.”

However, standard models of primordial black holes typically predict that their maximum mass should be around a million solar masses, while Maiorino pointed out that QSO1 is 50 times larger. “Nevertheless, it’s plausible that these primordial black holes are densely concentrated, allowing them to merge and grow rapidly,” he noted.

A further challenge arises from the requirement that for a primordial black hole to initially collapse, a burst of high-energy radiation, like that from a nearby supernova, is essential; however, no potential sources have been identified near QSO1, according to Maiorino.

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New Evidence Suggests Early Use of Bows and Arrows by Homo Sapiens in Europe for Hunting

In a newly published paper in this month’s iScience, researchers from the University of Tübingen and their collaborators present an interdisciplinary study of ancient stone and bone projectile points associated with Homo sapiens from the Lower Paleolithic era (40,000 to 35,000 years ago). This comprehensive research uses a blend of experimental ballistics, detailed measurements, and use-wear analysis, revealing that some of these prehistoric artifacts correspond not just to hand-thrown spears and javelin darts but also potentially to bow-propelled arrows.

Evidence suggests early humans may have used bows, arrows, and spear throwers in the Upper Paleolithic period. Image credit: sjs.org / CC BY-SA 3.0.

For decades, it was commonly believed that weapon technology evolved linearly, transitioning from hand-held spears to spear-throwing and eventually to bows and arrows.

However, lead researcher Keiko Kitagawa and her team at the University of Tübingen challenge this notion, arguing for a more complex evolution of weapon technology.

“Direct evidence of hunting weapons is rarely identified in the archaeological record,” they noted.

“Prehistoric hunting weapons encompassed a range from hand-held thrusting spears ideal for close-range hunting, to javelins and bow-headed arrows suitable for medium to long-range engagements.”

“The earliest known instances of such tools include wooden spears and throwing sticks, dating back 337,000 to 300,000 years in Europe.”

“Spear-throwing hooks first appeared during the Upper Solutrean period (around 24,500 to 21,000 years ago), gaining prominence in the Magdalenian culture of southwestern France (approximately 21,000 years ago), with nearly 100 specimens documented.”

Bows and arrows, however, have only surfaced from well-preserved sites like Mannheim-Vogelstang and Stermol in Germany, dated to about 12,000 years, and Lilla Roschulz-Mosse in Sweden, approximately 8,500 years, indicating they are significantly younger than other projectile technology.

Comparison of archaeological specimens from the Aurignac site with experimental examples from Vogelherd, Istritz, and Manot. Image credit: Kitagawa et al., doi: 10.1016/j.isci.2025.114270.

The authors propose that early modern humans may have concurrently experimented with various projectile technologies, adapting to diverse ecosystems and prey types.

The analysis reveals that the damage patterns on these ancient projectile points corresponded with what is expected from arrows shot from bows, as well as from spears and darts.

“We emphasize Upper Paleolithic bony projectiles, including split bases and megabases made from antler and bone, predominantly discovered in Aurignacian environments in Europe and the Levant, between 40,000 and 33,000 years ago,” the researchers explained.

“Our goal is to determine if the wear patterns and morphometry can identify the types of weapons associated with Aurignacian bone projectile tips.”

This discovery aligns with previous archaeological findings indicating that bows and arrows were utilized in Africa as far back as 54,000 years ago, predating earlier estimates and some of Europe’s archaeological record.

Importantly, the researchers do not assert that Homo sapiens invented the bow simultaneously across all regions, nor do they claim the bow was the only weapon used.

Instead, their findings suggest a rich technological diversity during the initial phases of human migration into new territories.

“Our study highlights the intricate nature of reconstructing launch technologies, which are often made from perishable materials,” the researchers stated.

“While it is impossible to account for all variables affecting the properties of the armature and resulting wear, we aspire to implement future experimental programs aimed at deepening our understanding of the projectiles that form a crucial component of hunter-gatherer economies.”

_____

Keiko Kitagawa et al. suggest that Homo sapiens may have utilized bows and arrows for hunting as early as the Upper Paleolithic period in Eurasia. iScience published online on December 18, 2025. doi: 10.1016/j.isci.2025.114270

Source: www.sci.news

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

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



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

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

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

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

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

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

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

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

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

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

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

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

_____

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

Source: www.sci.news

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

Gas ball with a black hole

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

Shutterstock / Nazarii_Neshcherenskyi

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

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

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

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

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

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

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

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

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

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

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

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

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Astronomers Uncover Direct Evidence of Supermassive Stars in the Early Universe

Astronomers utilizing the NASA/ESA/CSA James Webb Space Telescope have identified the chemical signature of a protostar with a mass between 1,000 and 10,000 times that of the Sun in GS 3073, an early galaxy with a redshift of 5.55 (approximately 1 billion years post-Big Bang).



A primordial supermassive star in the early universe. Image credit: Gemini AI.

In 2022, it was suggested by astronomers that supermassive stars formed naturally within turbulent flows of rare cold gas during the early universe, thus accounting for the existence of quasars less than a billion years after the Big Bang.

“Our recent finding helps to unravel a cosmic enigma that has persisted for two decades,” stated Dr. Daniel Whalen of the University of Portsmouth.

“GS 3073 offers the first observational proof of these colossal stars.”

“These astronomical behemoths would have radiated intensely for a brief period before collapsing into enormous black holes, leaving behind chemical imprints detectable billions of years later.”

“Much like Earth’s dinosaurs, they were massive and rudimentary, with lifespans spanning just 250,000 years—an ephemeral moment in cosmic time.”

The cornerstone of this discovery involved assessing the nitrogen-to-oxygen ratio in the GS 3073 galaxy.

This galaxy presents a nitrogen-to-oxygen ratio of 0.46, significantly exceeding what can be accounted for by any known type of star or stellar explosion.

“Chemical abundances serve as the universe’s fingerprints, and the pattern from GS 3073 is unlike that produced by typical stars,” remarked Dr. Devesh Nandal, an astronomer at the University of Virginia, Harvard University, and the Smithsonian Center for Astrophysics.

“This unprecedented nitrogen concentration aligns with a single known source: protostars that are thousands of times more massive than the Sun.”

“This suggests that the first generation of stars included genuine supermassive objects that contributed to the creation of early galaxies and may have planted the seeds for contemporary supermassive black holes.”

The researchers performed modeling of stars with masses between 1,000 and 10,000 solar masses to predict their evolution and the elements they would produce.

They identified a specific mechanism for generating substantial nitrogen. (i) These colossal stars fuse helium, forming carbon in their cores. (ii) Carbon seeps into the outer shell, where hydrogen is undergoing fusion. (iii) Carbon merges with hydrogen, resulting in nitrogen through the carbon/nitrogen/oxygen (CNO) cycle. (iv) Convection disseminates nitrogen throughout the star. (v) Eventually, this nitrogen-rich material is expelled into space, enriching the surrounding gas.

This mechanism spans millions of years during the star’s helium burning phase, leading to the excess nitrogen observed in GS 3073.

The team’s models predict that upon demise, these massive stars do not explode. Instead, they collapse directly into gigantic black holes with masses reaching thousands of solar masses.

Interestingly, GS 3073 harbors an actively feeding black hole at its core, which could potentially be the remnant of one of these supermassive first stars.

If validated, this would simultaneously clarify two mysteries: the origin of nitrogen and the formation of black holes.

The study also revealed that this nitrogen signature is exclusive to specific mass ranges.

“Stars below 1,000 solar masses or above 10,000 solar masses do not generate chemical patterns suitable for this signature, indicating a ‘sweet spot’ for such enrichment,” scientists noted.

of study Published in Astrophysics Journal Letter.

_____

Devesh Nandal others. 2025. A protostar between 1000 and 10,000 MSun created a nitrogen surplus in GS 3073 at z = 5.55. APJL 994, L11; doi: 10.3847/2041-8213/ae1a63

Source: www.sci.news

The First Evidence of Fire-Making by Early Humans in Britain

Artistic representation of sparks from flint and pyrite

Craig Williams, Trustee of the British Museum

Approximately 400,000 years ago, Neanderthals or their ancestors in Britain struck flint with pyrite, repeatedly igniting fires in the same location. Archaeologists believe this is the earliest evidence of human fire-making discovered to date.

Early humans may have opportunistically utilized fire for around 1.5 million years, likely benefiting from naturally occurring fires caused by events like lightning strikes.

Starting around 400,000 years ago, signs of more extensive fire usage grew in Europe, yet direct evidence indicates that humans gained the ability to control fire only around 50,000 years ago.

Nick Ashton from The British Museum reported three crucial findings from the Burnham Quarry site in Suffolk: pyrite, charred deposits, and a heat-damaged hatchet.

Pyrite holds significant importance in humanity’s fire history, as striking it with flint can produce sparks capable of igniting dry materials. However, pyrite does not naturally occur near quarries, implying that early humans must have transported it. “Pyrite is crucial,” Ashton states.

Additionally, the reddish sediment left by these fires is vital, according to him. Combustion alters the iron minerals present in the deposits, consequently changing their magnetic characteristics. Laboratory tests indicate that the reddish clay layer may have experienced firing events more than a dozen times, suggesting that humans revisited and ignited fires in this area repeatedly.

Heating flint facilitates its shaping into sharp tools, but excessive heat can lead to its shattering, as evidenced by the hatchet discovered at Burnham. Tests indicated it exceeded 700 degrees Celsius, prompting Mr. Ashton to believe it had inadvertently been heated.

Excavations at a disused quarry in Burnham, UK

Jordan Mansfield, Road to Ancient Britain Project.

Ashton notes that there’s accumulating evidence suggesting humans half a million years ago possessed a range of cultural and technological abilities, including making and using fire.

“Early Neanderthals, along with other modern human species, were far more capable than we often acknowledge,” Ashton says. “Starting a fire is no simple task; it necessitates understanding pyrite’s origin, its properties when used with flint, and selecting the right tinder to create a flame.”

John Gowlett at The University of Liverpool has stated that recent findings make it “highly plausible” that individuals 400,000 years ago were not just aware of fire but likely utilized it daily.

“Early humans were indeed familiar with fire, but the mere discovery of a burnt object associated with a tool doesn’t automatically indicate human control over it,” he explains. “If a location shows signs of repeated human occupation accompanied by multiple indicators of fire, that presents compelling evidence of human control, as natural fires seldom occur in the same place repeatedly.”

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Severe Heat Impacts Children’s Early Learning

Extreme heat and poverty can hinder child development

Riccardo Renato Niels Mayer/Alamy

Research indicates that young children exposed to extreme heat typically exhibit a reduced vocabulary, with fewer words, letters, and numbers understood, suggesting that global warming could negatively affect early human development.

Specifically, when average monthly maximum temperatures reached 32°C (90°F) or higher, children aged 3 and 4 were 2.8 to 12.2 percent less likely to meet developmental benchmarks compared to those in environments with maximum temperatures below 26°C (79°F).

“This marks the first instance in literature demonstrating that excessive heat influences not just physical health but also developmental capabilities,” stated Jorge Quartas from New York University.

Quartas and his team analyzed data from 19,600 children surveyed by UNICEF across Georgia, Gambia, Madagascar, Malawi, Sierra Leone, and the State of Palestine, referencing the early childhood development index. They assessed children’s abilities in naming letters, reading simple words, and recognizing numbers from 1 to 10.

The researchers correlated this data with climate records while adjusting for variables such as poverty, maternal education, and baseline temperatures. Notably, even temperatures of 30°C (86°F) began to adversely affect literacy and numeracy skills, with heat also impeding children’s social, emotional, and physical development to a lesser degree.

“Minor effects in early childhood can become more pronounced over time,” Quartas explains. For instance, children who struggle with number recognition might find it challenging to learn math concepts, potentially falling behind academically.

Heat-related stress remains the primary cause of weather-related fatalities, claiming nearly 500,000 lives annually. A recent rapid assessment estimated that the heatwave in June and July was responsible for 2,300 deaths across 12 European cities, primarily occurring among those aged 65 and older.

The findings also revealed that the impacts of heat extend even to prenatal periods. For instance, temperatures of 33 degrees Celsius (91 degrees Fahrenheit) during early pregnancy correlated with a 5.6% reduction in the likelihood of successful childhood development.

Children from poorer, urban households with limited access to water resources were found to be more heavily affected by the heat. “Climate change and excessive heat serve as amplifiers of existing threats,” Quartas articulated. “These children are already at a disadvantage.”

Nonetheless, the study may not comprehensively address barriers such as violence and political instability, which can also impede childhood development, as noted by Giulia Pescarini from the London School of Hygiene and Tropical Medicine.

Further investigations are needed to clarify how heat impacts development, she suggests, noting that low-income households might lack air conditioning, and parents may experience increased stress during heat events.

Pescarini emphasizes that a better understanding of who is affected and how can aid in developing adaptive strategies to support these vulnerable groups.

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Source: www.newscientist.com

Three Key Factors That Likely Shaped the Moon’s Formation in Earth’s Early History

The moon may have had a more intricate formation than previously believed.

NASA/NOAA

Recent theories suggest that multiple collisions with Earth might better elucidate the Moon’s origin than the traditionally accepted single massive impact 4.5 billion years ago, potentially addressing one of its greatest enigmas.

Tracing the Moon’s origin has proven challenging. The prevailing theory is that it formed early in the solar system’s evolution due to a catastrophic collision between Earth and Theia, a Mars-sized body, and its formation likely originated closer to the sun than Earth’s current position. This impact would have expelled debris that ultimately coalesced into the large natural satellite we recognize today. At that period, matter around the sun was highly intermixed, making collisions frequent.

However, this prevailing model encounters complications, as the chemical compositions of Earth and the Moon are remarkably similar, suggesting that the Moon should retain more material from Theia than our planet does. “This presents a significant dilemma for the standard model,” comments Philip Carter, a researcher at the University of Bristol, UK.

Carter and his team propose a paradigm shift, suggesting that a series of impacts with Earth over millions of years may provide a more coherent explanation for the compositional similarities between Earth and the Moon. They propose that three or more significant impacts in the early solar system, involving bodies from the size of the modern Moon to those approaching Mars in size, could account for the Moon’s creation as we observe it today.

In this revised model, each impact creates smaller moons, known as microsatellites, orbiting Earth. Over eons, these smaller bodies would progressively merge under gravitational attraction, forming a singular large entity. “They will be drawn to one another and collide,” explains Carter. “The probability of sustaining a stable system with multiple large moonlets is exceedingly low.”

Previous models also posited multiple impacts as the origin of the Moon; however, they typically required a more rigorous series of impacts than this current framework. “After three significant collisions, we introduced sufficient mass into orbit to form a full Moon,” stated Carter.

Robert Citron, a researcher at the Southwest Research Institute in Colorado, suggests that fewer impacts might be more favorable since too many collisions could displace smaller satellites from Earth’s orbit and hinder Moon formation. However, as more impacts occur, the compositional alignment between Earth and the Moon increases, accurately reflecting their current similarities. “When multiple impacts are involved, you are averaging out more influencing factors,” Citron notes.

The unique relationship between Earth and the Moon underscores the necessity of understanding the Moon’s formation. “It is a remarkably distinctive satellite,” Citron emphasizes. “Its size relative to Earth is vast, whereas the moons of Mars appear minuscule in comparison to Mars, and the moons of gas giants are diminutive compared to their planets.”

Establishing which hypothesis is correct necessitates more intricate modeling to assess the impact’s intensity on Earth and the volume of material expelled. Carter remarks, “Calculating all these details remains exceedingly complex.” He adds, “Personally, I prefer the multi-impact model over the traditional single-impact theory.”

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Source: www.newscientist.com

Fossils from Venezuela Uncover the Early Origins of Anaconda Giants

The anaconda is among the largest surviving snake species in the world. Typically, its length ranges from 4 to 5 meters, although exceptional cases can reach up to 7 meters. A recent study conducted by paleontologists on giant anaconda fossils from South America suggests that these tropical reptiles achieved their maximum size approximately 12.4 million years ago and have maintained their large dimensions continuously since then.

Green anaconda (Eunectes murinus). Image credit: MKAMPIS / CC BY-SA 4.0.

“Current snakes display a broad spectrum of body lengths, averaging about 1 meter, with sizes ranging from 10 centimeters for the smallest leptotyphloid thread snakes to roughly 7 meters for anacondas.” Eunectes Andrés Alfonso Rojas, a PhD student at the University of Cambridge, and his colleagues state:

“Within the Eunectes genus, the green anaconda (Eunectes murinus) is the largest species, averaging 4 to 5 meters in length, with maximum recorded lengths of 6 to 7.2 meters.”

“Limited fossil findings from Brazil, Colombia, Peru, and Venezuela suggest that the evolutionary timeline of anacondas dates back to the mid-to-late Miocene.”

“However, our understanding of the body size of early anacondas, which coexisted with massive crocodilians, turtles, ungulates, and xenartranians, remains scarce.”

In their research, the authors examined 183 fossilized anaconda spines representing at least 32 snakes discovered in the state of Falcón, Venezuela.

By integrating these measurements with fossil data from various South American locations, they concluded that ancient anacondas measured 4 to 5 meters in length, similar to today’s anacondas.

“While other species, including giant crocodiles and colossal turtles, have become extinct since the Miocene—likely due to declining global temperatures and reduced habitats—giant anacondas have persisted. They demonstrate remarkable adaptability,” noted Alfonso Rojas.

“The analysis of fossils indicates that anacondas’ body size evolved significantly soon after their emergence in tropical South America around 12.4 million years ago, and this size has remained consistent ever since.”

The researchers cross-verified their estimates using an alternative method known as ancestral state reconstruction, employing snake family trees to estimate the length of giant anacondas and related modern species like tree boas and rainbow boas.

This method corroborates the notion that when anacondas first appeared in the Miocene, their average size was 4 to 5 meters.

Anacondas inhabit swamps, marshes, and substantial rivers, such as the Amazon. During the Miocene, northern South America resembled the contemporary Amazon region, allowing anacondas to thrive in wider areas than seen today.

Nonetheless, the current environment still offers ample food sources, including capybaras and fish, and suitable habitats that support the continued growth of modern anacondas.

As snakes are particularly sensitive to temperature changes, it was previously believed that anacondas might have grown even larger during earlier warm periods.

“This finding is unexpected, as ancient anacondas were thought to have reached lengths of 7 to 8 meters,” remarked Alfonso Rojas.

“However, we found no evidence supporting the existence of larger snakes during the Miocene, even when global temperatures were higher.”

These findings were published recently in the Journal of Vertebrate Paleontology.

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Andres F. Alfonso-Rojas et al. Early origins of gigantism in anacondas (Serpentes: Eunectes) revealed by the fossil record. Journal of Vertebrate Paleontology published online on December 1, 2025. doi: 10.1080/02724634.2025.2572967

Source: www.sci.news

Supermassive Dark Matter Stars Could Be Hidden in the Early Universe

Exotic stars may be fueled by dark matter

remote vfx/getty images

We might be observing the earliest indications of peculiar stars that harness dark matter. These dark stars could provide explanations for some of the universe’s most enigmatic entities, and offer insights into the actual nature of dark matter itself.

Standard stars are birthed when a gas cloud collapses, leading to a core dense enough to initiate nuclear fusion. This fusion generates significant heat and energy, radiating into the surrounding gas and plasma.

Dark stars could have emerged in a similar fashion during the universe’s infancy, a period of higher density which also saw a notably concentrated presence of dark matter. If a gas cloud collapsing into a star contains substantial dark matter, it may begin to collide and dissipate prior to nuclear fusion, generating enough energy to illuminate the dark star and halt further collapse.

The process leading to the formation of dark stars is relatively straightforward, and currently, a team led by Katherine Freese from the University of Texas at Austin is exploring its potential outcome.

In an ordinary large star, once the hydrogen and helium are depleted, it continues fusing heavier elements until it runs out of energy and collapses into a black hole. The more mass the star contains, the quicker this transition occurs.

However, the same is not true for dark stars. “By incorporating dark matter into a star roughly the mass of the Sun, and sustaining it through dark matter decay rather than nuclear means, you can continuously nourish the star. Provided it receives enough dark matter, it won’t undergo the nuclear transformations that lead to complications,” explains George Fuller, a collaborator with Freese at the University of California, San Diego.

Despite this, general relativity imposes a limit on how long dark matter can preserve these unusual giants. Albert Einstein’s theory suggests that an object’s gravitational field does not increase linearly with mass; instead, gravity intensifies the gravitational force. Ultimately, an object may reach a mass at which it becomes unstable, with minor variations overpowering its gravitational pull and resulting in a collapse into a black hole. Researchers estimate this threshold for a dark star is between 1,000 and 10 million times the Sun’s mass.

This mass range makes supermassive dark stars prime candidates for addressing one of the early universe’s profound mysteries: the existence of supermassive black holes. These giants were spotted relatively early in the universe’s history, but their rapid formation remains a puzzle. One prevailing theory posits that they didn’t arise from typical stars, but rather from some colossal “seed.”

“If a black hole weighs 100 solar masses, how could it possibly grow to a billion solar masses in just a few hundred million years? This is implausible if black holes were formed solely from standard stars,” asserts Freese. “Conversely, this situation changes significantly if the origin is a relatively large seed.” Such faint stars could serve as those seeds.

Yet, the enigmas of the early universe extend beyond supermassive black holes that dark stars could elucidate. The James Webb Space Telescope (JWST) has unveiled two other unforeseen object types, referred to as the little red dot and the blue monster, both appearing at substantial distances. The immediate hypothesis for these is that they are compact galaxies.

However, like supermassive black holes, these objects exist too far away and too early in universal history for simple formation explanations. Based on observations, Freese and her associates propose that both the little red dot and the blue monster may represent individual, immensely massive dark stars.

If they indeed are dark stars, they would display particular clues in their light. This aspect pertains to specific wavelengths that dark stars should ostensibly absorb. Normal stars and galaxies dense with them are too hot to capture that light.

Freese and colleagues have found possible indicators of this absorption in initial JWST observations of several distant entities; however, the data is too inconclusive to confirm its existence. “Currently, of all our candidates, two could potentially fit the spectrum: a solitary supermassive dark star or an entire galaxy of regular stars,” Freese notes. “Examining this dip in the spectrum, we’re convinced it points to a dark star rather than a conventional star-filled galaxy. But for now, we only possess a faint hint.”

While it remains uncertain if we have definitively detected a dark star, this development marks progress. “It isn’t a definitive finding, but it certainly fuels motivation for ongoing inquiries, and some aspects of what JWST has been examining seem to align with that direction,” remarks Dan Hooper from the University of Wisconsin-Madison.

Establishing whether these entities are genuinely dark stars necessitates numerous more observations, ideally with enhanced sensitivity; however, it remains ambiguous whether JWST can achieve the level of detail required for such distant galaxies or dark stars.

“Confirming the existence of dark stars would be a remarkable breakthrough,” emphasizes Volodymyr Takistov from the High Energy Accelerator Research Organization in Japan. This could facilitate new observational avenues into foundational physics. This is particularly true if dark stars are recognized as seeds for supermassive black holes. Freese, Fuller, and their team deduced that the mass at which a black hole collapses correlates with the mass of the dark matter particle annihilating at its center, implying that supermassive black holes could serve as metrics to evaluate or at least restrict dark matter properties. Of course, validating the existence of dark stars is the first priority. “Even if these entities exist, their occurrence is rare,” Hooper states. “They are uncommon, yet significant.”

Exploring the Mysteries of the Universe: Cheshire, England

Join some of the brightest minds in science for a weekend dedicated to unraveling the universe’s mysteries, featuring a tour of the legendary Lovell Telescope.

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Source: www.newscientist.com

Mysterious Footprint Indicates Another Early Human Relative Coexisted with Lucy

In a recent breakthrough regarding human evolution, researchers have unveiled that a peculiar foot unearthed in Ethiopia is from a yet-to-be-identified ancient relative.

The findings, released on Wednesday in the journal Nature, indicate the foot dates back approximately 3.4 million years and likely bears similarities to Lucy, another ancient human relative who inhabited the region around the same period.

However, scientists have revealed that Burtele’s foot, named after the site in northeastern Ethiopia where it was discovered in 2009, is distinctly different.

The fossil of Bartel’s foot has an opposable thumb akin to that of humans, suggesting its owner was a proficient climber, likely spending more time in trees compared to Lucy, according to the study.

Elements of Brutere’s foot discovered in Ethiopia in 2009.
Johannes Haile Selassie/Arizona Institute of Human Origins (via AFP)

For many years, Lucy’s species was believed to be the common ancestor of all subsequent hominids, serving as a more ancient relative to humans, including Homo sapiens, in contrast to chimpanzees.

Researchers were unable to confirm that the foot belonged to a novel species until they examined additional fossils found in the same vicinity, including a jawbone with twelve teeth.

After identifying these remains as Australopithecus deiremeda, they determined that Bartele’s feet were from the same species.

John Rowan, an assistant professor of human evolution at the University of Cambridge, expressed that their conclusions were “very reasonable.”

“We now have stronger evidence that closely related, yet adaptively distinct species coexisted,” Rowan, who was not part of the study, communicated in an email to NBC News on Thursday.

The research also examined how these species interacted within the same environment. The team, led by Johannes Haile Selassie of Arizona State University, suggested that the newly identified species spent considerable time in wooded areas.

The study proposed that Lucy, or Australopithecus afarensis, was likely traversing the open land, positing that the two species probably had divergent diets and utilized their habitats in distinct ways.

Various analyses of the newly found tooth revealed that A. deiremeda was more primitive than Lucy and likely fed on leaves, fruits, and nuts, the study indicated.

“These distinctions suggest they are less likely to directly compete for identical resources,” remarked Ashley Los Angeles-Wiseman, an assistant professor at the Macdonald Institute of Archaeology at the University of Cambridge.

In an email on Thursday, Wiseman highlighted the significant implications of this discovery for our understanding of evolution, stating that it “reminds us that human evolution is not a linear progression of one species evolving into the next.”

Instead, she asserted, it should be viewed as a branching family tree with numerous so-called “cousins” existing simultaneously, each adopting various survival strategies. “Did they interact? We may never know the answer to that,” she concluded.

Rowan also noted that as the number of well-documented species related to humans increases, so do the inquiries concerning our ancestry. “Which species were our direct ancestors? Which species were our close relatives? That’s the challenge,” he remarked. “As species diversity ascends, so too do the avenues for plausible reconstructions of how human evolution unfolded.”

Wiseman cautioned that definitive species classifications should rely on well-preserved skulls and fossil fragments belonging to multiple related individuals. While the new study bolsters the case for A. deiremeda, it “does not dismiss all other alternative interpretations,” she stated.

Source: www.nbcnews.com

Astronomers Simulate Formation of Early Star Clusters – Sciworthy

The universe has undergone significant changes. Examining the contrasts between the universe as we perceive it today and its origin nearly 14 billion years ago is a crucial area of study for astrophysicists and cosmologists. Their focus is primarily on the first billion years following the Big Bang, when the first stars and galaxies began to emerge, marking the dawn of the universe. This was the initial phase when celestial objects began to emit light on their own rather than merely reflecting the remnants of the Big Bang, and it was also the first occurrence when elements heavier than helium started forming via nuclear fusion in stars.

In a recent study, a group of scientists utilized computer simulations to explore what star clusters looked like during the dawn of the universe. Their objective was to create models of star and galaxy formation that could be confirmed by new observations made by the JWST. This approach will enhance astronomers’ understanding of galaxy formation in the early universe, particularly the influence of galaxies on dark matter, which remains enigmatic, during the birth of the first stars from cosmic dust.

The research employed a cosmological simulation code called Arepo to recreate the dawn of the universe within a three-dimensional box measuring 1.9 megaparsecs on each side. This size converts to 60 quintillion kilometers or 40 quintillion miles. Within this box, the simulation contained 450 million particles representing early elemental matter, including hydrogen, helium, various isotopes, ions, and molecules that formed together. Additionally, it incorporated particles simulating known dark matter, which is affected by gravity but does not interact with other forces. When these aggregates of particles coalesced and surpassed a specific mass threshold known as jeans mass, the code indicated the formation of a star.

The team aimed to identify where the simulated stars and particles formed structures like star clusters, galaxies, and galaxy clusters. They implemented a method to group particles that were sufficiently adjacent to be considered connected, utilizing a friend of friends algorithm. By executing multiple iterations of this algorithm in the simulated universe—some focused on dark matter and others on ordinary matter such as stars, dust, and gas—the researchers sought to ascertain the arrangement of matter in the early universe.

The resulting simulated clusters were found to have dimensions comparable to actual clusters observed by astronomers in the early universe. However, no real clusters with metal-rich stars matching those in the simulations have yet been identified. Furthermore, the number of stars present in the simulated cluster was consistent with previous observations of distant star clusters recorded by the JWST. Many simulated star clusters were unstable, indicating they were not fully bound by their internal gravity. The team also found that as stable star clusters began merging into larger structures, such as galaxies, they became unstable once more.

An unexpected finding emerged from the study. The friend-of-a-friend algorithm produced varying results when assessing dark matter versus ordinary matter. The discrepancy reached up to 50%, implying that an algorithm targeting dark matter might detect only half the objects identified by an algorithm focused on regular matter. This variance depended on the mass of the identified star clusters or galaxies, particularly evident for objects within a moderate size range of 10,000 to 100,000 solar masses and very low masses around 1,000 solar masses.

The researchers could not ascertain the reasons behind this phenomenon, suggesting their simulations might be overly simplistic for accurately representing all conditions present during the universe’s dawn. Notably, they mentioned the absence of newly formed stars ejecting materials into space in their simulations. Consequently, they proposed treating their discovery as an upper limit on the frequency of star-like and, by extension, star-containing objects forming in the early universe. Their results might illustrate instances in nature where star formation occurs extremely efficiently, yet sorting out the roles of all involved processes remains necessary.

The conclusion drawn was that cosmic dawn clusters could have coalesced to create the foundations of modern galaxies or possibly evolved into the luminous cores of later galaxies. Additionally, the simulated clusters appeared to be strong candidates for forming medium-sized black holes, the remnants of which may be detectable with deep-space telescopes.


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Source: sciworthy.com

Ancient DNA May Transform Our Understanding of Iceland’s Early Settlers

While historical accounts claim that Ingólfr Arnarson was the first Norse settler to reach Iceland in the 870s, this assertion might not hold true.

Public domain

Norsemen may have arrived in Iceland as much as 70 years earlier than previously believed, and their arrival might not have been the environmental catastrophe often depicted.

Traditionally, it’s stated that Iceland saw its first settlement in the 870s. This early migration is frequently viewed as an ecological calamity brought on by Viking raiders and Norse settlers who cleared the forests for fuel, construction materials, and arable land. Today, less than 2 percent of the country is still forested.

Finding concrete evidence regarding the arrival of these early settlers has been challenging. Archaeologists have discovered an ancient wooden longhouse, estimated to be from around 874 AD, located near Stódvarfjordur in eastern Iceland. This old longhouse is thought to have been a summer dwelling established in the 800s, though this finding has yet to be documented in scientific journals.

Currently, Eske Willerslev, a professor at the University of Copenhagen, and his team examined environmental DNA (eDNA) gathered from sediment cores drilled in Lake Tjörnin, an area in central Reykjavík, one of Iceland’s earliest and continuously inhabited locations, to identify which species existed and their timestamps. They analyzed volcanic ash layers, alongside radiocarbon dating and plutonium isotope assessments, to develop a timeline from about 200 AD up to contemporary times, integrating known historical events.

A significant marker in their research is the Randonham tephra layer, formed from volcanic ash deposited during eruptions around 877 AD. The bulk of evidence indicating human habitation in Iceland is found above this layer, indicating subsequent settlement.

“The signs beneath the tephra provide compelling evidence for earlier human activity,” Comments Chris Callow from the University of Birmingham, UK, who did not participate in the research.

Willerslev and his colleagues postulate that humans may have arrived as early as 810 AD. This inference is based on an observed rise in levoglucosan, a compound linked to biomass burning, and a subsequent increase in sewage-related viruses.

“If it were 850, I wouldn’t have been so surprised, but 810 represents rapid Viking expansion in the North Atlantic,” Callow remarks. “Overall, this aligns with our suspicions, but a date as early as 810 remains contentious.”

While piecing together a thorough environmental history of the region is noteworthy, the evidence supporting such an early arrival remains questionable. Kathryn Catlin from Jacksonville State University in Alabama stated, “The sewage biomarkers only show a slight increase around 800, nothing until 1900. Where are the indicators of sewage and human activity in between?” She also pointed out that while biomass burning could imply human presence, natural occurrences like lightning could also ignite fires.

Willerslev and his colleagues opted not to conduct interviews. New Scientist also noted that the settlers’ arrival corresponded with an uptick in local biodiversity. Genetic data imply they brought grazing animals, cultivated hay, and grew barley on a small scale for brewing purposes.

In contrast to the widespread narrative of swift deforestation, eDNA from pollen samples revealed that birch and willow trees expanded during the settlement era. Notably, birch pollen grains rose fivefold between 900 and 1200 AD, a shift researchers believe may have been influenced by settlers managing the area to protect timber and fuel sources.

“This significantly contradicts earlier claims that Vikings arrived in Iceland and immediately caused environmental destruction,” Katrin stated.

Although sheep, cattle, pigs, and horses do not appear in considerable numbers until decades after the initial settlement, Willerslev and his colleagues propose this lag may stem from the 20-year period required to build up detectable herds in eDNA records.

Callow posits another explanation: the first inhabitants may have only visited during the summer months for walrus ivory, possibly arriving without many animals. “They could have intended to hunt a few walruses and return home,” he suggested.

eDNA indicators imply the significant loss of biodiversity, including birch and willow trees, didn’t transpire until after 1200. Willerslev and his team associate this decline with the cooler climate associated with the Little Ice Age, rather than direct effects from settlers. This marked a period of colder temperatures from approximately 1250 to around 1860, compounded by volcanic eruptions and storm surges.

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Source: www.newscientist.com

Mysterious Brazilian Fossil Reveals Widespread Presence of Lichens in the Early Devonian Period

Paleontologists have discovered a specimen dating back 410 million years: cavernous cavernosa nanum. This lichen is one of the oldest and most extensively distributed in the fossil record and was found in Brazil’s Paraná Basin, specifically within the Ponta Grossa Formation.

Artistically reconstructed cavernous cavernosa nanum from the Early Devonian, depicting high-latitude sedimentary systems of the Paraná Basin. Image credit: J. Lacerda.

The colonization of land and the evolution of complex terrestrial ecosystems rank among the most significant evolutionary milestones in the history of life.

This phenomenon greatly affected terrestrial and marine ecosystems, leading to the sequestration of atmospheric carbon dioxide, enhanced weathering, nutrient absorption in oceans, soil formation, and the emergence of major groups of terrestrial animals.

It is well-established that early plants played a crucial role in land colonization, particularly in establishing the first plant communities.

The earliest records of ancient land plants appear in the form of cryptospores from the Middle Ordovician, around 460 million years ago. The first macrofossils of vascular plants are found in Silurian deposits dating from approximately 443 to 420 million years ago.

Despite this, the specific role and presence of lichens during various stages of terrestrialization remain uncertain.

cavernous cavernosa nanum displays a partnership of fungi and algae akin to modern lichens,” noted Dr. Bruno Becker Kerber from Harvard University.

“Our research illustrates that lichens are not merely peripheral organisms; they were vital pioneers in reshaping Earth’s terrain.”

“They contributed to the soil formation that enabled the colonization and diversification of plants and animals on land.”

Morphology and internal structure of cavernous cavernosa nanum. Image credit: Becker-Kerber et al., doi: 10.1126/sciadv.adw7879.

Findings indicate that ancient lichens originated in the cold polar regions of the Gondwana supercontinent, now known as parts of modern-day South America and Africa.

cavernous cavernosa nanum is a remarkable fossil, preserved in an incredible state. Essentially, they are mummified with their organic matter intact,” remarked Professor Jochen Brocks from the Australian National University.

“In simple plants, the tough component is cellulose. In contrast, lichens are unique; they consist of chitin, the same material that gives insects like beetles their strength.”

“Chitin contains nitrogen. In our analyses, cavernous cavernosa nanum yielded an unprecedented nitrogen signal.”

“Such clear results are rare. It was a true Eureka moment.”

“Today, lichens continue to be vital in soil creation, nutrient recycling, and carbon capture in extreme environments spanning from deserts to the polar regions.”

“Yet, due to their delicate structure and infrequent fossil records, their origins remain elusive.”

“This research underscores the necessity of blending traditional techniques with innovative technology,” explained Dr. Nathalie L. Alchira, a researcher at the Synchrotron Light Institute in Brazil.

“Preliminary measurements enabled us to identify crucial areas of interest and collect 3D nanometer imaging for the first time, unveiling the intricate fungal and algal networks that define cavernous cavernosa nanum as a true lichen.”

The team’s study was published in this week’s edition of Scientific Advances.

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Bruno Becker-Kerber et al. 2025. The role of lichens in the colonization of terrestrial environments. Scientific Advances 11(44); doi: 10.1126/sciadv.adw7879

Source: www.sci.news

Paleontologists Uncover New Early Triassic Coelacanth Species

Chinese paleontologists have identified a new species of Coelacanth, Whiteia anniae, based on two fossil specimens. This breakthrough expands the geographic presence of the genus Whiteia, marking the oldest record of this genus in Asia, which predates the earliest known pyloid coelacanth in this continent by 9 million years.



Whiteia anniae Right side view, holotype. Image credit: Dai et al., doi: 10.1038/s41598-025-20229-w.

“Coelacanths are a fascinating group of sarcopterygian fishes, with two extant marine species from the genus Latimeria,” stated lead author Dr. Guan Hui Shu, a paleontologist at the Institute of Vertebrate Paleontology and Paleoanthropology, Chinese Academy of Sciences, and colleagues.

“This group first appeared in the Early Devonian, peaked in taxonomic diversity during the Early Triassic, but saw a decline starting in the Middle Cretaceous.”

“Coelacanths play a crucial role in evolutionary biology due to their distinctive physiological and anatomical characteristics, as well as their resilience through four major extinction events over hundreds of millions of years.”

The discovery of Latimeria previously ignited discussions on how this unusual lobe-finned fish relates to the evolution of terrestrial animals.

“Given their evolutionary stability, coelacanths have long been viewed as one of the most morphologically conservative vertebrate groups.”

“However, some research, particularly those focusing on Triassic fossils, indicate that coelacanth body shapes exhibit greater diversity than previously recognized.”

“Recent discoveries of new species around the globe continue to yield significant insights into the evolution of coelacanths.”

The newly identified species, Whiteia anniae, lived during the Smithian stage of the Early Triassic, approximately 249 million years ago.

This fish belongs to the genus Whiteia, an extinct group of coelacanths that were previously known from Madagascar, South Africa, Canada, and Greenland, but not from Asia.

“As the first record in Asia, this new finding from the Early Triassic dramatically broadens the geographic distribution of the genus Whiteia and is a significant addition to our understanding of the evolution of this major Triassic coelacanth lineage,” stated the paleontologists.

Two specimens of Whiteia anniae were discovered in Late Triassic marine deposits at Maoshankou in Anhui Province, China.

Fossil evidence suggests that this coelacanth measured between 41 and 46 centimeters in length, making it notably larger than other named species within its genus.

“Previously reported Whiteia species from the Early Triassic were typically small, ranging from 11.5 to 27 cm in length, and a slender body shape was once believed to be a defining characteristic of the genus,” the researchers explained.

“While there has been a recent trend of recovery, the Whiteia giganteus (estimated to exceed 100 cm in length) from Texas illustrates a period in which the genus achieved larger body sizes during the Late Triassic in North America.”

“The recovery of Whiteia anniae provides an intriguing example of a smaller species, in contrast to larger relatives in Europe, Africa, and North America.”

The team’s study was published on October 17th in the journal Scientific Reports.

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QH.Large et al. 2025. A new species of coelacanth (Actinistia, Sarcopterygii) from the Early Triassic period of Anhui Province, China. Scientific Reports 15, 36320; doi: 10.1038/s41598-025-20229-w

Source: www.sci.news

Physicists Suggest a Cosmic ‘Knot’ Could Have Influenced the Early Universe Briefly

Knots are prevalent in various fields of mathematics and physics today. A collaborative team of Japanese and German physicists proposes the existence of a “knot-dominated epoch” in the universe’s early days, suggesting that knots were essential building blocks during this time. This intriguing hypothesis can be investigated through gravitational wave observations. Additionally, they theorize that the conclusion of this period will involve the collapse of the knot due to quantum tunneling, leading to an Asymmetry between matter and antimatter in space.



Model proposed by Eto et al.. It suggests a brief, knot-dominated epoch when these intertwined energy fields outweighed everything else, a scenario that can be investigated through gravitational wave signals. Image credit: Muneto Nitta / Hiroshima University.

Mathematically, knots are defined as closed curves embedded in three-dimensional space and can be found not just in tying neckties but across numerous scientific disciplines today, as noted by Lord Kelvin.

Although his theory postulated that atoms are knots of etheric vortices was ultimately refuted, it sparked advancements in knot theory and its application in multiple areas of physics.

“Our study tackles one of the core mysteries of physics: why the universe is predominantly composed of matter rather than antimatter,” remarked Professor Munehito Nitta, a physicist at Hiroshima University and Keio University.

“This question is crucial as it relates directly to the existence of stars, galaxies, and ourselves.”

“The Big Bang was expected to produce equal amounts of matter and antimatter, with the intent that each particle would annihilate its counterpart, leaving only radiation.”

“Yet, the universe is overwhelmingly composed of matter, with only trace amounts of antimatter.”

“Calculations indicate that to achieve the matter we see today, only one extra particle of matter is needed for every billion matter-antimatter pairs.”

“Despite its remarkable achievements, the Standard Model of particle physics fails to resolve its inconsistencies.”

“That prediction is significantly off.”

“Unraveling the origin of the slight excess of matter, a phenomenon known as baryogenesis, remains one of the greatest unresolved enigmas in physics.”

By merging the measured baryon number minus lepton number (BL) symmetry with the Peksey-Quinn (PQ) symmetry, Professor Nitta and his associates demonstrated that the knot could have spontaneously formed in the early universe, resulting in the observed surplus.

These two well-studied extensions to the standard model address some of its most confounding gaps.

PQ symmetry offers a solution to the strong CP problem, which explains the absence of the small electric dipole moments that theories predict for neutrons, simultaneously introducing axions, a leading candidate for dark matter.

BL symmetry, conversely, elucidates why neutrinos, elusive particles that can seamlessly pass through entire planets, possess mass.

Maintaining the PQ symmetry globally, rather than merely measuring it, safeguards the delicate axion physics that addresses the strong CP problem.

In physics, “measuring” a symmetry implies allowing it to operate freely at any locale and moment in time.

However, this regional freedom requires nature to introduce new mechanisms for force transmission to clarify the equations.

By acknowledging BL symmetry, the researchers not only validated the existence of heavy right-handed neutrinos (crucial for averting anomalies in the theory and central to the primary burr formation model) but also incorporated superconducting behavior, likely providing the magnetic foundation for some of the universe’s earliest knots.

As the universe cooled following the Big Bang, its symmetry may have fractured through a series of phase transitions, leaving behind string-like defects called cosmic strings, which some cosmologists theorize may still persist.

Even though thinner than a proton, a cosmic string can stretch across a mountain.

As the universe expanded, these writhing filaments would twist and intertwine, preserving traces of the primal conditions that once existed.

The breakdown of BL symmetry formed a flux tube string, while PQ symmetry resulted in a flux-free superfluid vortex.

This contrast renders them compatible.

The BL flux tube grants the Chern-Simons coupling of the PQ superfluid vortex a point of attachment.

This coupling subsequently channels the PQ superfluid vortex into the BL flux tube, counteracting the tension that might otherwise disrupt the loop.

The outcome is a metastable, topologically locked structure known as a knot soliton.

“No prior studies had simultaneously considered these two symmetries,” notes Professor Nitta.

“In a way, our good fortune lay in this. By integrating them, we uncovered a stable knot.”

While radiation diminishes energy as waves traverse through space and time, knots exhibit properties akin to matter and dissipate energy far more gradually.

They subsequently surpassed all other forms, heralding an era of knot domination, where their energy density eclipsed that of radiation in the universe.

However, this dominance was short-lived. Ultimately, the knot succumbed to quantum tunneling, an elusive process where particles slip through energy barriers as though they were nonexistent.

This decay yielded heavy dextral neutrinos, a consequence of the inherent BL symmetry within its framework.

These colossal, elusive particles eventually transformed into lighter and more stable variations that favored matter over antimatter, shaping the universe we recognize today.

“Essentially, this decay releases a cascade of particles, including right-handed neutrinos, scalar particles, and gauge particles,” explained Dr. Masaru Hamada, a physicist at the German Electron Synchrotron Institute and Keio University.

“Among them, right-handed neutrinos are particularly noteworthy since their decay can inherently generate a discrepancy between matter and antimatter.”

“These massive neutrinos decompose into lighter particles, such as electrons and photons, sparking a secondary cascade that reheats the universe.”

“In this manner, they can be regarded as the ancestors of all matter in the universe today, including our own bodies, while knots might be considered our forebears.”

Once the researchers delved into the mathematics underlying the model—analyzing how efficiently the knot produced right-handed neutrinos, the mass of those neutrinos, and the degree of heat generated post-collapse—the observed matter-antimatter imbalance naturally emerged from their equations.

Rearranging the equations, with an estimated mass of 1012 gigaelectronvolts (GeV) for heavy dextral neutrinos, and assuming that most energy retained by the knot was utilized to generate these particles, the model yielded a natural reheating temperature of 100 GeV.

This temperature fortuitously coincides with the final opportunity for the universe to produce matter.

Should the universe cool beyond this point, the electroweak reactions that convert neutrino discrepancies into matter would cease permanently.

Reheating to 100 GeV may have also reshaped the cosmic gravitational wave spectrum, shifting it toward higher frequencies.

Forthcoming observatories such as Europe’s Laser Interferometer Space Antenna (LISA), the United States’ Cosmic Explorer, and Japan’s Decihertz Interferometer Gravitational-Wave Observatory (DECIGO) may someday detect these subtle tonal variations.

Dr. Minoru Eto, a physicist at Yamagata University, Keio University, and Hiroshima University, remarked, “The cosmic string is a variant of topological soliton, an entity defined by a quantity that remains unchanged regardless of how much it is twisted or stretched.”

“This characteristic not only guarantees stability but also indicates that our results are not confined to the specifics of the model.”

“While this work is still theoretical, we believe it represents a significant advancement towards future development, as the foundational topology remains constant.”

Although Lord Kelvin initially proposed that knots were fundamental components of matter, the researchers assert that their findings present the first realistic particle physics model in which knots could significantly contribute to the origin of matter.

“The next step involves refining our theoretical models and simulations to more accurately forecast the formation and collapse of these knots, connecting their signatures with observable signals,” said Professor Nitta.

“In particular, upcoming gravitational wave experiments like LISA, Cosmic Explorer, and DECIGO will enable the testing of whether the universe indeed experienced a knot-dominated era.”

The team’s work appears in the journal Physical Review Letters.

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Minoru Eto et al. 2025. Tying the Knot in Particle Physics. Physics. Pastor Rhett 135, 091603; doi: 10.1103/s3vd-brsn

Source: www.sci.news

Studies Suggest the 1-Million-Year-Old Yunxian Fossil Is an Early Hominid

Different varieties of Homo, such as Homo Longhi, coexisted during the mid-Pleistocene era. The debate over whether these fossilized humans represent distinct species continues. The 1-million-year-old Yunxian 2 skulls from China are crucial for understanding the beginnings of Homo. In a recent study, paleontologists applied cutting-edge technology to recover and reconstruct the distorted Yunxian 2 fossils. Their findings indicate that this skull exhibits both primitive and advanced features in a mosaic pattern. Team analysis proposes that it belongs to an early Asian branch of Homo Longhi, which is closely related to Denisovan and is a significant part of the clade leading to Homo sapiens.

Reconstruction of Homo Longhi in its habitat. Image credit: Chuang Zhao.

Fossil evidence indicates the presence of multiple forms of Homo during the mid-Pleistocene period.

A significant portion of what we know about human evolution and archaic humanity is based on fossil skulls.

Nonetheless, many specimens from this time are damaged or deformed, creating uncertainty in species classification.

For instance, three human skulls from the Yunxian site in China, dating back nearly a million years, exhibit a mix of primitive traits.

The two already known Yunxian fossils, Yunxian 1 and 2, both show distortion. The newly discovered Yunxian 3 skull is still under analysis.

In this recent study, Dr. Xiaobo Feng, affiliated with Shanghai University and Huqiaotech University, along with his research team from the Yunxian Man Site’s Garden Team Laboratory, utilized advanced CT scanning and digital reconstruction methods to address the compression and distortion present in Yunxian 2.

The team’s analysis reveals a blend of previously unidentified primitive and derived characteristics, suggesting that this fossil belongs to the Asian Homo Longhi clade, closely related to Homo sapiens, which may include Denisovan traits.

Individuals within the Homo Longhi clade display distinctive traits, such as a larger cranial capacity, narrower eye spacing, a pronounced graveller depression, and a lower elongated frontal bone, all of which are evident in the Yunxian 2 fossils.

Researchers further posit that the Yunxian fossil is likely the oldest within the Homo Longhi clade, making it particularly significant.

“With geological ages ranging from 0.94 to 1.1 million years, Yunxian is closely aligned with the theoretical origins of the Longhi and Sapiens clades,” the team stated.

“Phylogenetically, it is nested within the Homo Longhi clade. However, its mosaic characteristics retain some plesiomorphic traits seen in Homo Erectus and Homo Elgustar. While Kabwe and Petralona show shared apomorphic traits, Homo Longhi and Homo sapiens may exhibit transitional functions close to the clade’s origin.”

“The narrow temporal gap between Yunxian and the deeper Longi nodes suggests a swift, early diversification of the Longi clades, similar to those of Sapiens and Neanderthals.”

A study detailing these findings will appear in the journal Science this week.

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Xiaobo Feng et al. 2025. The phylogenetic position of the Yunxian head in relation to Homo Longhi and Denisovan. Science 389 (6767): 1320-1324; doi: 10.1126/science.ado9202

Source: www.sci.news

Early Findings Indicate Elevated Risk of Colon Cancer in Long-Distance Runners

Researchers may have identified a potential connection between extreme endurance running and colorectal cancer, as nearly half of marathon and ultra-marathon participants have undergone screening.

Initial research assembled 100 long-distance runners aged 35-50 for colonoscopy, though these findings have not yet been peer-reviewed.

Close to 50% were found to have polyps (growths), with 15% diagnosed with advanced adenomas—growths that are likely to progress to cancer.

In contrast, recent studies indicate that only about 4.5 to 6 percent of adults in their late 40s from the general population have these advanced adenomas. However, it’s important to note that these studies included significantly larger sample sizes.

“I was quite concerned when I observed a group of ultra-marathon runners in their 30s diagnosed with stage 4, very advanced colorectal cancer,” said Dr. Timothy Cannon, who led the study at the Inova Schar Cancer Institute in Virginia. BBC Science Focus.

“They reported experiencing bleeding and convulsions post-race. At least one or two mentioned that they were told this was normal following their runs.”

Such symptoms can result from ischemic colitis, where blood flow is diverted from the colon to supply oxygen to the legs and other muscles during intense activity. This can lead to swelling and bleeding but typically resolves spontaneously.

Dr. Cannon speculated whether repeated cycles of damage and healing could create conditions conducive to cancer development.

Blood flow to the legs deprives the intestines of oxygen.

“There is currently no evidence that ischemic colitis directly causes cancer,” he stated. “However, it’s not difficult to imagine the potential outcomes. When numerous cells die and regenerate chaotically, there are ample chances for DNA replication errors.”

Alternative explanations exist as well. Endurance athletes are known to possess distinct gut microbiota compared to non-runners, and they often consume considerable amounts of ultra-processed foods, such as bottled energy drinks.

Dr. Cannon’s team is preparing to compare the gut bacteria of runners with and without adenomas to that of non-runners.

The findings were presented at the American Society of Clinical Oncology’s annual meeting, yet researchers cautioned that these are merely preliminary results, necessitating further investigation. They also highlighted that the screening study lacked a control group of non-runners.

“This leans more toward hypothesis than definitive answers,” Cannon remarked.

“I definitely don’t want people to walk away thinking exercise is harmful because it is beneficial overall. The inquiry is whether high levels of exercise could elevate the risk of colon cancer—and I believe they might.”

Read more:

  • Running slowly may be essential for a healthier, longer lifespan. Here’s why
  • What are the limits of human endurance?
  • The astonishing truth about how running can alter one’s perception of time

Source: www.sciencefocus.com

Initiating HRT During Early Menopause Could Lower Alzheimer’s Risk in Women

A decrease in estrogen during menopause may affect cognitive function

Elena Popova/Getty Images

Commencing hormone replacement therapy (HRT) within five years of the onset of postmenopause appears to decrease the likelihood of developing Alzheimer’s disease. In contrast, starting HRT later in life may have adverse effects, indicating that the timing of the therapy is crucial for its impact on the brain.

Women face a greater risk of developing Alzheimer’s, particularly after menopause, compared to men. This heightened risk may be linked to reduced estrogen levels, which play vital roles in brain energy regulation and inflammation. Consequently, HRT has surfaced as a potential method to reduce Alzheimer’s risk following menopause. However, research on its effectiveness has produced mixed outcomes.

To investigate this, Fnu Vaibhav Pandit Bagwat Deira Sharma from Health Science University in India and his team analyzed 53 studies encompassing over 8.4 million postmenopausal participants regarding Alzheimer’s disease prevalence.

In a randomized controlled trial, participants receiving HRT exhibited, on average, a 38% greater risk of developing Alzheimer’s compared to those not on HRT. Conversely, observational studies suggested a 22% reduction in Alzheimer’s risk among HRT users.

Vaibhav presented these findings at a meeting with the American Nerve Association in Maryland on September 15th, noting that the disparity is likely age-related. Most subjects in the randomized trial were over 65, while those in observational studies tended to be younger. Further analysis revealed that individuals who initiated HRT within five years post-menopause had a decreased risk of Alzheimer’s by 32% over a follow-up period ranging from five years to others that consumed their lifetime.

“This transition during menopause represents a neurological shift,” stated Roberta Brinton from the University of Arizona, who was not part of the research. As estrogen levels decline, the brain seeks alternative energy sources. There is some evidence suggesting that this reallocation may utilize compounds meant for brain function while sacrificing others, leading to potential neurodegeneration. She posits that HRT may either initiate or halt this transition during menopause. However, if the brain has already undergone this shift, HRT may be ineffective.

“More research is essential to clarify this perplexity,” remarked Vaibhav. Without a clearer comprehension of HRT’s impact, he warns that “women may miss out on advantages, and some may inadvertently face harm.”

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Source: www.newscientist.com

In a 100-Mile Race, the Wealthy Gain an Early Advantage

Getty Images on Unsplash+

I am a centenarian. Not too long ago, reaching this milestone was a rarity, often only mentioned in local newspapers. Yet today, it’s an aspiration that many can achieve. Recently, Japan celebrated reaching a remarkable count of 100,000 centenarians, marking a significant milestone. By 2015, nearly half a million people globally surpassed the age of 100, with projections suggesting this number could reach 3.7 million by 2050.

This increase is largely due to advancements in healthcare and a better understanding of longevity. What the human body requires to thrive has become clearer. I’ve also learned how to enhance my own chances of living to a hundred. In our special issue, you will discover insights into diet, travel, and mindset that could help you celebrate a century with your own birthday cake.

However, individual choices have their limits; a stark reality exists between life expectancy and health status among different socio-economic groups. Those residing in the wealthiest areas of the UK now enjoy nearly 18 healthier additional years compared to those in less affluent communities, accounting for significant disparities among men and women over a decade. A recent The Lancet report indicated that the gap in life expectancy among demographics in the U.S. widened from 12.6 years in 2000 to 20.4 years in 2021, with Asian Americans living the longest and Native Americans the shortest. The divide continues to widen. In 2020, high-ranking Hindus saw their life expectancy drop by 1.3 years, while Indian Muslims experienced a loss of 5.4 years. These statistics are alarming. Access to nutritious foods, secure housing, and healthcare must be prioritized to address the growing inequality.


By 2050, the global centenarian population is expected to reach 3.7 million.

As we push for enhancements in longevity, it’s essential to hold our politicians accountable to combat this escalating inequality. Achieving a life to 100 should be a goal accessible to all, not just the affluent.

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Source: www.newscientist.com

Early Neanderthals Pursued Ibex on Steep Mountain Terrain

Ibex can navigate gracefully across steep mountain terrains

Serge Goujon/Shutterstock

Nearly 300,000 years ago, Neanderthals had already devised strategies for hunting goats on vertical cliffs and managing them in well-structured camps.

Typically recognized for ambushing large animals in flat meadows and forests of Western Europe, Neanderthals seemed to adapt to the hilly landscapes of Eastern Europe by incorporating the lightweight ibex into their hunting practices. Early humans skinned these animals in nearby caves, but only after the bones had been covered and fractured. Stephen Milosevic from the University of Belgrade in Serbia.

“The approach to hunting ibex is entirely distinct since they inhabit robust, steep, and barren terrains,” he explains. “Now we observe primitive Neanderthals who barely distinguish themselves as a separate species, already utilizing an ecological niche previously unexploited by humans.”

Neanderthals evolved approximately 400,000 years ago, yet most of our knowledge stems from sites in Western Europe that are under 150,000 years old. According to Marie Helen Monsel, who was not involved in this research at the National Museum of Natural History in Paris, it’s crucial to uncover clues that can bridge the gaps in our understanding of Neanderthal timelines, habitats, and cultures.

In 2017, archaeologists uncovered evidence that Neanderthals inhabited the layers of Belikabaranica Cave in Serbia, which date back roughly 290,000 years, making it the oldest remains of Neanderthals found in Eastern Europe.

Since that discovery, Milosevic and his colleagues have excavated hundreds of stone tools and analyzed the bone fragments of approximately 30,000 animals within the cave. Almost three-quarters of these fragments are less than two centimeters long, with the majority traceable to ibex and red deer hunted in spring and summer, indicating that Neanderthals likely resided in the cave seasonally.

Some bones, particularly those from the legs of larger deer, exhibited burn marks and were cracked open. This suggests that these early Neanderthals may have liquefied the bones, leaving remnants scattered on the walls surrounded by the grease that fueled their fires. Others may have shown signs of tendon harvesting for use in ropes or nets.

The deer remains indicate the presence of older youths and adults, pointing to selective hunting practices that would promote herd survival, according to Milosevic. However, ibex were hunted at all life stages. Neanderthals seemed to be “novices” when it came to hunting goats, implying they likely relied on sharp sticks and rudimentary traps. “They must have experienced a significant number of failed attempts,” he notes.

Apart from these favored food sources, researchers have also found several remains from wild boars, cave bears, wolves, foxes, leopards, and even various birds.

The arrangement of the bones in various sections of the cave indicates a clear division of tasks. For instance, the hearth was located centrally, with discarded bones stacked behind it, while the entrance appeared to function as a tool workshop.

In summary, the findings suggest “notable cognitive flexibility,” states Jose Carrion from the University of Murcia in Spain. “This confirms that Neanderthals are creative problem-solvers who effectively navigate complex habitats with ingenuity and skill. Neanderthals were indeed human. They were intellectual, social, and highly adaptable.”

“The discoveries from Baranica provide a glimpse of Neanderthals who not only display resilience but are experimenting with strategies and social structures typically associated with later periods,” commented Antonio Rodriguez Hidalgo from the Archaeological Institute in Merida, Spain. “This reminds us that Neanderthal sophistication is not a gradual developement but rather a deep-rooted flame that ignited early in human history.”

Neanderthals, ancient humans, cave art: France

Join new scientist Kate Douglas on an enchanting journey through time as she explores significant Neanderthal and Upper Paleolithic sites across southern France, from Bordeaux to Montpellier.

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Source: www.newscientist.com

Fossils from the Early Cretaceous Period at the Swiss Museum

Paleontologists have identified a new species within the extinct turtle genus Craspedochelys, based on some remarkable fossil shells and subsequent bones discovered in Colombia.



Artistic reconstruction of Craspedochelys Renzi and the shallow marine ecosystem it inhabited. The flip-like shape of the forelimbs is inspired by the most complete known specimen of Thalassemys bruntrutana. Image credit: Juan Guilard.

Craspedochelys Renzi thrived during the early Cretaceous Hauterivian period, approximately 132 to 125 million years ago.

This ancient species belonged to the Thalassocheridia, a group of marine-adapted turtles from the Jurassic and Cretaceous eras.

“Throughout their evolutionary journey, various unrelated turtle groups have developed adaptations for marine and coastal habitats,” says Dr. Edwin Alberto Cadena, a paleontologist at the Smithsonian Tropical Research Institute of Natural History.

“One such group is the Thalassocheridia, traditionally classified into three Jurassic families: Eurysternidae, Plesiochelyidae, and Thalassemydidae, which have complex and often debated phylogenetic relationships.”

“Among these families, the ‘Plesiochelyidae’ is particularly diverse, encompassing at least ten species across four different genera: Craspedochelys, Plesiochelys, Portlandomys, and Tropidemys.”

“The shells of ‘Plesiochelyids’ can be distinguished from other thalassocheridians by their large size (40-55 cm in shell length), with adults lacking the thyroid cortex of the hanging skin, typically displaying only a thick layer of fontanel in the center.”



Craspedochelys Renzi is characterized by a distinct shell featuring several occipital bones. Image credits: Cadena et al. , doi: 10.1186/s13358-025-00394-1.

The fossil specimen of Craspedochelys Renzi was first discovered by Swiss geologist Otto Lenz during a field expedition in the Cunja de Cuisa region of Guazila Province, Colombia, in the 1950s.

This specimen included partial shells measuring 25.5 cm long and 23.1 cm wide, along with hind limb bones and caudal vertebrae.

It was later stored in the paleontological collection of the Naturhistorisches Museum Basel in Switzerland, where it remained unnoticed for over 60 years among the fossil invertebrate collection.

“Geological evidence connects these specimens to shallow marine sediments from the Moina Formation, dating to the Hauterivian,” the paleontologist explained.

This fossil represents the youngest known occurrence of Thalassocheridians globally during the Hauterivian, and it is the second record from a non-European group.

“The discovery of Craspedochelys Renzi will greatly enhance our understanding of Thalassocheridians, particularly the ‘Plesiochelyidae’, expanding their geographical range to North Gondwana and temporal range to the Hauterivian,” the researchers stated.

“This find underlines the significance of reevaluating historical collections and the potential for future discoveries in less explored areas such as northern South America.”

“The existence of Craspedochelys Renzi in the Moina Formation further underscores the intricate paleobiogeographic history of early Cretaceous coastal habitats and marine turtles.”

“It also offers new perspectives on the evolutionary dynamics of Thalassocheridia and the still unresolved, unstable phylogenetic relationships within the group, which necessitates further detailed investigation in future research.”

The discovery of Craspedochelys Renzi is discussed in a paper published in the Swiss Journal of Palaeontology.

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ea. Cadena et al. 2025. The first occurrence of the “Plesiochelyidae” turtle in the early Cretaceous period of South America. Swiss J Palaeontol 144, 52; doi:10.1186/s13358-025-00394-1

Source: www.sci.news

Study Reveals Asteroid Sample Composition Mirrors Early Solar System Elements

The initial bodies that formed in the solar system gathered materials from stars, presolar molecular clouds, and protozoan debris. Asteroids that have not experienced planetary differentiation retain evidence of these significant materials. Nevertheless, geological processes such as hydrothermal changes can significantly modify their composition and chemistry. In a recent study, researchers scrutinized the elemental and isotopic composition of samples from the asteroid Bennu, uncovering the origin and nature of the materials associated with its parent body.

This mosaic image of the asteroid Bennu consists of 12 images collected on December 2, 2018 by a 15-mile (24 km) Polycam instrument at Osiris-Rex. Image credit: NASA/NASA’s Goddard Space Flight Center/University of Arizona.

“Our analysis shows that Bennu’s elemental composition closely resembles that of the sun,” stated LLNL scientist Greg Brennecka.

“This indicates that the materials obtained from Bennu provide a valuable reference to the initial arrangement of the entire solar system.”

“Notably, Bennu has remained largely untouched by intense heat, which would alter some of its original ingredients.”

Researchers continue to investigate how planets form, and determining the initial composition of the solar system is akin to gathering a recipe for a cake.

“With that recipe, we gain insight into how all these elements interacted to create the solar system and, ultimately, the Earth and its living beings,” Dr. Brennecca remarked.

“If we aim to understand our origins, the composition of our solar system serves as a fundamental starting point.”

Outer view of the Osiris-Rex sample collector. Sample material for the asteroid can be seen in the center right. Image credits: NASA/Erika Blumenfeld/Joseph Aebersold.

The Osiris-Rex mission by NASA has introduced new possibilities by returning pristine samples to Earth while avoiding contamination from our planet.

LLNL scientist Quinn Shollenberger commented:

“We cannot tackle the significant question of ‘origins’ without a sample on Earth.”

“One of our objectives is to ascertain which elements of the periodic table and their percentages contributed to the solar system’s inception. Bennu can help us uncover this,” noted LLNL scientist Jan Render.

To achieve these findings, researchers ground the asteroid material into fine powders and dissolved them in acid.

This mixture was then analyzed with a series of mass spectrometers to determine the concentrations of most elements within the periodic table.

From these results, scientists have sorted the samples by elements and successfully analyzed the isotopic ratios of several.

“I work at a National Laboratory that boasts remarkable analytical capabilities with state-of-the-art equipment,” shared LLNL scientist Josh Winpenny.

“It is quite rare to have all these functions consolidated in one place, allowing us to make optimal use of these valuable materials.”

“NASA’s Johnson Space Center researcher Dr. Anne Nuguen stated:

“We discovered stardust grains with compositions predating our solar system, organic materials likely formed in interstellar space, and high-temperature minerals that originated close to the sun.”

“All these components were transported over to the region that formed Bennu’s precursor asteroids.”

Survey results published in the journal Natural Astronomy.

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JJ Burns et al. Diversity and origin of materials accumulated by Bennu’s pro-asteroids. Nat Astron Published online on August 22, 2025. doi:10.1038/s41550-025-02631-6

Source: www.sci.news

Paleontologists Uncover Early Signs of Human-Maternal Interbreeding

Paleontologists at the National Museum d’Historel in Tel Aviv University and Delige University, France, have reported a fascinating discovery involving a combination of Neanderthal and Homo sapiens skeletal features in a 5-year-old child found in 1931 at Skhūl Cave, located on Mount Carmel, Israel.

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

Mugarat Es Skhūl (Skhūl Cave) was uncovered in 1928 by Theodore McConne and Dorothy Garrod on Mount Carmel, Israel.

The excavation revealed skeletal remains of seven adults and three children, alongside isolated bones linked to 16 additional individuals associated with the Fauna and Musteria tool industry.

The fossils belong to Homo sapiens, or “anatomically modern humans,” dating back approximately 140,000 years to the end of the Mid Pleistocene.

The initial discoveries in the cave were of children aged three to five years.

A recent study led by Professor Israel Hirschkowitz of Tel Aviv University indicates that the child’s skull resembles the overall shape of Homo sapiens, particularly in the skull vault, with inner ear structures characteristic of the intracranial blood supply system and features of the mandible akin to Neanderthals.

“This finding highlights the earliest known human fossils exhibiting morphological traits from both of these groups,” he stated.

“This study indicates that the skeleton of the five-year-old child is a result of ongoing genetic intermingling with the local Neanderthal and Homo sapiens populations,” he added.

“Genetic research over the last decade has demonstrated that these two groups exchanged genes,” remarked Professor Hirschkowitz.

“Even today, 40,000 years after the last Neanderthals vanished, 2-6% of our genomes can be traced back to Neanderthals,” he continued.

“However, these gene exchanges occurred much later, between 60,000-40,000 years ago. In this case, we are addressing human fossils from 140,000 years ago.”

Traditionally, Neanderthals were thought to have evolved in Europe and migrated to Israeli territories approximately 70,000 years ago due to advancing glaciers.

A 2021 study revealed that early Neanderthals inhabited Israeli lands around 400,000 years ago.

This type of human is referred to as “Nescher Ramra.” Homo might have interbred with Homo sapiens, a group that began migrating out of Africa around 200,000 years ago – and according to findings from the current study, they did breed.

The children from Skhūl Cave represent the earliest fossil evidence of the social and biological bonds formed between these two groups over thousands of years.

Ultimately, local Neanderthals dwindled as they were absorbed into the Homo sapiens population, similar to Neanderthals in later Europe.

“The fossils we researched are the earliest known tangible proof of mating between Neanderthals and Homo sapiens,” Professor Hirschkowitz commented.

“In 1998, child skeletons were unearthed in Portugal, displaying features from both human groups.”

“However, that skeleton, known as the ‘Lapedo Valley Child,’ dates back just 28,000 years.”

Historically, anthropologists have attributed the fossils found in Skhūl Cave, alongside those from the Caffze cave near Nazareth, to early groups of Homo sapiens.

“Current research reveals that some fossils from the Skhūl cave are indeed the product of continuous genetic intermingling with local and ancient Neanderthal populations of Homo sapiens,” he concluded.

Survey results were published in the journal on June 14th, l’anthropologie.

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Bastien Bouvier et al. 2025. New analysis of Skhūl child’s neurological and mandible: taxonomic conclusions and cultural implications. l’anthropologie 129(3): 103385; doi: 10.1016/j.anthro.2025.103385

Source: www.sci.news

Early Cretaceous Iguanodontian Dinosaurs Could Strike Their Sails

A new genus and species of sailed Iguanodontian dinosaurs has been discovered from a partial skeleton unearthed in the Wessex Formation on the Isle of Wight, England.

Restoration of Istiorachis macarthurae. Image credit: James Brown.

Named Istiorachis macarthurae, this new dinosaur species thrived in what is now England during the early Cretaceous period, approximately 125 million years ago.

These ancient creatures were part of a large, widely distributed group of herbivorous dinosaurs known as iguanodontians.

“Iguanodontia represented a highly successful clade of Ornithischian dinosaurs,” said Jeremy Lockwood, a paleontologist from the University of Portsmouth and the Museum of Natural History in London.

“By the end of the Cretaceous, they dominated the dinosaur fauna of Laurasia, alongside the hadrosaurid family, including Edmontosaurus legatus and Parasaurolophus walkeri.”

“While diversity among iguanodonts was low during the late Jurassic, it surged in the early Cretaceous.”

The most notable characteristic of Istiorachis macarthurae is a series of elongated spines along its back and tail, which formed a large sail-like structure.

“Evolution often favors the extravagant over the practical,” Lockwood commented.

“The precise function of such structures has been debated for years; however, while they may serve purposes from heat regulation to fat storage, visual signaling—perhaps for sexual display—seems the most plausible explanation in this context.”

“In modern reptiles, such sail structures are often more pronounced in males, indicating that these traits may have evolved to attract mates or intimidate rivals.”

“We hypothesize that Istiorachis macarthurae may have done something similar.”

Paleontologists closely examined the fossilized bones to determine the purpose of the sails.

By creating a comprehensive database of similar dinosaur backbones through direct observations, photographs, scientific illustrations, and reconstructions, they were able to investigate the evolutionary history of the back structure in this new Iguanodontian family tree.

This helped identify broader trends in the evolution of these sails.

“These methods allow us not only to explain the fossil evidence but also to test hypotheses about their function,” Lockwood noted.

“We demonstrated that Istiorachis macarthurae‘s spines were not only taller but also more exaggerated compared to typical Iguanodon features, making it an ideal candidate for traits arising through sexual selection.”

Istiorachis macarthurae illustrates a broader evolutionary pattern.

Research indicates that the lengthening of neural spines in the Iguanodon lineage began in the late Jurassic period, becoming more common in the early Cretaceous.

However, true hyperelongation, which surpasses four times the height of the spine body, remains rare.

Similar displays can be observed in present-day reptiles, such as various lizard species, where elaborate crests and sails often communicate health and strength to potential mates.

Istiorachis macarthurae is a prime example,” Lockwood said.

The findings were published in the journal Paleontology Papers this week.

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Jeremy A. F. Lockwood et al. 2025. The origin of neural spine elongation in Iguanodontian dinosaurs and the osteology of the new sail-backed dinosaur (Dinosaur, Ornithischia) from the Cretaceous Wealden group in England. Paleontology Papers 11(4): E70034; doi: 10.1002/spp2.70034

Source: www.sci.news