How Early Humans Revolutionized Their Toolkits 200,000 Years Ago: Key Changes and Innovations

Changes in predator populations may have driven early humans to develop innovative tools

Raul Martin/MSF/Science Photo Library

Approximately 200,000 years ago, a decline in megafauna may have compelled early humans to transition from heavy stone tools to more lightweight hunting kits designed for smaller prey. A recent study supports the notion that this change in hunting strategy could have sparked a rise in cognitive capabilities among our ancestors.

For over a million years, various early human species relied on heavy stone tools such as axes, kitchen knives, scrapers, and stone balls. These robust tools were essential for hunting and butchering large herbivores, including extinct relatives of modern elephants, hippos, and rhinos.

Between 400,000 and 200,000 years ago, archaeological evidence shows a notable increase in smaller, sophisticated tools alongside the fading of traditional heavier tools. Our species, Homo sapiens, emerged during this timeframe.

Circa 200,000 years ago, heavy stone tools vanished from the archaeological record of the Levant, while the presence of diverse, lightweight masonry toolkits—like blades and precision scrapers—increased.

Research led by Vlad Litov, a professor at Tel Aviv University, revealed a correlation between these technological advancements and a significant decline in large herbivores, potentially due to overhunting.

The researchers analyzed archaeological findings from 47 sites across the Levant, spanning the Paleolithic period, which lasted from around 3.3 million years ago to 12,000 years ago. Their analysis of dated stone artifacts in relation to animal remains uncovered a compelling trend.

Findings indicate a drastic reduction in the biomass and specimen count of giant herbivores exceeding 1,000 kilograms correlating with the disappearance of heavy tools 200,000 years ago. Conversely, the availability of smaller prey increased alongside more sophisticated small tools.

Supporting the connection between tool technology and prey type, the researchers noted that sturdy stone tools were still in use in regions with abundant large game, such as southern China, until about 50,000 years ago.

Heavy-duty tools and their evolution to lightweight alternatives used by early humans

Vlad Litov et al., Institute of Archaeology, Tel Aviv University

Previous theories suggested that advancements in technology stemmed from increasing intelligence and creativity due to evolutionary pressures. However, Litov and his research team propose a different perspective: reliance on smaller prey may have catalyzed the evolutionary growth of larger brains in modern humans.

“As large herbivores dwindled, humans increasingly depended on smaller prey, necessitating varied hunting strategies, advanced planning, and the implementation of lightweight, intricate toolsets,” states Litov. “This cognitive evolution was a byproduct of adapting to new prey types, rather than the initial driver of this adaptive transformation.”

“There is more to this adaptation than merely prey size,” says Seri Shipton from University College London. He notes preliminary evidence indicating mass hunting of medium-sized ungulates like horses and bison, with signs of enhanced cognitive abilities and planning emerging during the Middle Paleolithic.

Nicolas Tessandier from the French National Center for Scientific Research also maintains some reservations. “Human adaptation to new fauna underscores adaptability rather than mere intelligence,” he posits. “Producing powerful tools for hunting large herbivores was equally astute.”

Litov recognizes that prior research has shown advanced cognitive functions present early in human evolution, notably in the development of Homo erectus around two million years ago. However, he emphasizes that switching from large to smaller prey had major consequences for human society. A single ancient elephant carcass could sustain a group of about 35 hunter-gatherers for months. As these high-calorie resources vanished, reliance on smaller prey reduced the yield per animal.

“Energetically, we had to gather numerous smaller ungulates, such as fallow deer, to replace the loss of one elephant,” explains Litov. This shift likely stimulated diverse cognitive and behavioral changes, including cooperative hunting strategies, advanced techniques, and enhanced social collaboration and organization. “Such adaptations may have contributed to the evolution of larger brains in later species, including Neanderthals and Homo sapiens,” he adds.

“In my view, the decline in large prey familiar to hominins likely intensified competition among groups,” asserts Shipton. “It was probably an iterative process where the reduction of larger prey prompted cognitive shifts that facilitated access to smaller prey.”

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Astronomers Uncover Massive Hydrogen Reservoirs Surrounding Early Galaxies

Astronomers from the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) have discovered colossal hydrogen halos, known as Lyman-alpha nebulae, surrounding over 30,000 galaxies dating back 10 to 12 billion years. This groundbreaking finding indicates that the essential materials for galaxy formation were far more plentiful than previously believed.



A giant halo of hydrogen gas, as revealed by HETDEX data and captured in deep imaging from the NASA/ESA/CSA James Webb Space Telescope. This ancient star system, 11.3 billion years old, radiates from the collective light of its myriad galaxies, with the brightest areas highlighted in red. Image credit: Erin Mentuch Cooper, HETDEX/NASA/ESA/CSA/STScI.

Hydrogen gas presents a unique challenge to astronomers, as it doesn’t emit light independently.

However, when located near energy-emitting objects—like galaxies packed with stars radiating UV light—hydrogen can glow due to this energy.

Detecting hydrogen halos demands significant time and precision, as the specialized instruments needed are often in high demand.

Previous astronomical surveys have identified some of these halos but typically focused only on the most luminous and extreme examples.

Furthermore, targeted observations of early galaxies are often too zoomed in, leading to the omission of larger halos.

HETDEX’s observations are actively filling this observational gap. This research uses the Hobby-Eberly Telescope at McDonald Observatory to map over 1 million galaxies and deepen our understanding of dark energy.

“We collected nearly half a petabyte of data, not just on these galaxies, but also on the intergalactic space,” stated Dr. Karl Gebhardt, the principal investigator of HETDEX and chair of the astronomy department at the University of Texas at Austin.

“Our observations encompass a sky area capable of hosting more than 2,000 full moons. The extent is extraordinary and unprecedented.”

“The Hobby-Eberly Telescope ranks among the largest telescopes worldwide,” Dr. Dustin Davis, a HETDEX scientist and postdoctoral fellow at UT Austin, remarked.

“HETDEX’s instruments yield 100,000 spectra per observation, providing a vast quantity of data and a treasure trove of exciting discoveries on the horizon.”

To locate hydrogen halos, astronomers examined the brightest 70,000 of the 1.6 million early galaxies cataloged by HETDEX.

Utilizing supercomputers at the Texas Advanced Computing Center, they assessed how many showed signs of surrounding halos.

According to the research team, these halos can span tens to hundreds of thousands of light-years across.

Some appear as simple, football-shaped clouds enveloping individual galaxies, while others take on irregular forms housing multiple galaxies.

“These formations are intriguing,” said Erin Mentaci-Cooper, HETDEX data manager and researcher at UT Austin.

“They resemble giant amoebas with tentacles extending into the cosmos.”

Results of this study were published on March 11, 2026, in a paper in the Astrophysical Journal.

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Erin Mentouch Cooper et al. 2026. Lyα Nebula in HETDEX: The largest statistical census connecting Lyα halos and blobs across cosmic noon. APJ 1000, 38; doi: 10.3847/1538-4357/ae44f3

Source: www.sci.news

Perseverance Uncovers Nickel-Rich Rocks on Mars: Insights into Early Martian Chemistry

Exciting findings from the Neretva Canyon—a prehistoric river channel that once flowed to Mars’ Jezero Crater—uncover significant concentrations of nickel in 3 billion-year-old sediments. These patterns mirror mineral formations found on Earth, often linked to microbial activity.



Nickel detected in bright magnesium sulfate veins in Jezero Crater on Mars, supporting its genuine origin. Image credit: Manelski et al., doi: 10.1038/s41467-026-70081-3.

“The Perseverance rover landed in Mars’ Jezero Crater in February 2021 aimed at exploring ancient habitable environments and collecting core samples for future return to Earth during a planned Mars sample return mission,” stated Dr. Henry Manerski from Purdue University and his research team.

“Jezero is a Noachian impact crater, approximately 45 km in diameter, dating back 3.8 to 4 billion years, that once housed a lake, as supported by its two inlet valleys, delta fan formations, and an outlet valley on the eastern side.”

“Since its landing, Perseverance has traversed the igneous crater floor, ascended western alluvial fan deposits, crossed olivine- and carbonate-rich margins, and entered the western inlet valley known as the Neretva Valley.”

In their comprehensive study, Dr. Manerski and colleagues employed lasers, infrared spectrometers, and X-ray spectrometers onboard Perseverance to analyze 126 sedimentary rock samples and eight rock surfaces in the Neretva Valley.

They discovered nickel in 32 rocks at concentrations reaching up to 1.1% by weight, marking the highest level ever recorded in Martian rock.

The team noted that nickel tends to occur alongside iron sulfide compounds and sulfate minerals resulting from the breakdown of rocks such as jarosite and acanite.

Researchers drew parallels between the nickel-rich iron sulfide arrangements found in the Neretva Valley and the composition and structure of pyrite, an iron sulfide mineral observed in sedimentary rocks worldwide.

Iron sulfide found in Earth’s sedimentary rocks is predominantly produced by the anaerobic respiration of microorganisms that utilize sulfate in the presence of iron-rich minerals.

Previous investigations identified iron sulfide in the Neretva Valley, coinciding with organic carbon compounds and suggested these may have originated from biological sources.

“Although, such formations can also arise from non-biological processes,” the scientists noted.

“Our current research hasn’t provided evidence of any organisms being present.”

“Nickel is a vital element in the enzymes of many ancient archaeal and bacterial species, playing crucial roles in energy production, carbon fixation, and organic matter decomposition.”

“The identification of nickel-rich rocks implies that if life existed on early Mars, nickel was potentially available in forms usable by these organisms.”

“The nickel may stem from the breakdown of igneous rocks or from nickel-rich meteorites.”

“More research is essential to pinpoint the source of nickel in the Neretva Gorge and to examine its relationship with organic matter at this location.”

Results from this study were published in this week’s issue of Nature Communications.

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HT Manerski et al. 2026. Strong nickel enrichment coexists with redox and organic interactions in Neretva Canyon on Mars. Nat Commun 17, 2705; doi: 10.1038/s41467-026-70081-3

Source: www.sci.news

Early Miocene Fossils: Uncovering Missing Links in Ape Family Evolution

Paleontologists have recently uncovered a groundbreaking genus and species of fossil monkey known as Maslipithecus mograensis, which inhabited northern Egypt approximately 17 to 18 million years ago. This discovery challenges previous notions, indicating that the evolutionary ancestors of modern apes and humans may have emerged at the intersection of Africa and Eurasia, rather than in East Africa.



Reconstruction of the life of Maslipithecus mograensis. Image credit: Mauricio Anton.

The current consensus among scientists is that the earliest great apes, known as pedunculated hominids, originated in the Africa-Arabia region during the Oligocene epoch over 25 million years ago. These species diversified and migrated into Eurasia by the Miocene epoch, approximately 14 to 16 million years ago.

However, the origin of modern apes, encompassing all existing species and their last common ancestor, remains elusive due to the scarcity and wide dispersion of relevant fossils from this period.

This uncertainty is compounded by the fragmented fossil record in Africa, where significant discoveries are predominantly localized to a few areas, leaving numerous potential ancient habitats of Miocene apes unexplored.

“Historically, the early Miocene fossil record documenting the evolution of hominids was mainly derived from sites in East Africa, with only long-tailed macaque fossils identified in contemporary North African locations,” stated Showrouk al-Ashkar, a paleontologist from Mansoura University, along with collaborating researchers from Egypt and the United States.

The newly discovered fossil, which dates back to 17 to 18 million years ago, was found in the Wadi Mogra region of northern Egypt.

Named Maslipithecus mograensis, this species significantly enhances our comprehension of the diversity and evolution of early apes during a crucial period when Afro-Arabia began to connect with Eurasia, facilitating the species’ dispersal from Africa.

“Although the fossil remains consist mainly of the lower jaw, they exhibit a unique combination of features not found in other known apes from this era,” the research team reported.

“These features include notably large canines and premolars, molars characterized by rounded and finely textured chewing surfaces, and exceptionally robust jaws,” they continued.

“Collectively, these traits indicate that Maslipithecus mograensis was adapted for dietary versatility,” they added.

Researchers interpreted the masticatory anatomy of this species as indicative of a flexible diet, largely comprising fruits, but capable of processing harder food items like nuts and seeds when necessary.

To ascertain the position of Maslipithecus mograensis within the human evolutionary lineage, scientists employed a modern Bayesian “advanced dating” method, combining both anatomical features and fossil ages to estimate evolutionary relationships and divergence times.

The findings imply that this new species represents a stem hominin closely linked to the lineage that ultimately led to all modern apes.

This discovery reinforces the hypothesis that the origins of modern apes may lie within northern Afro-Arabia, the Levant, or the eastern Mediterranean.

“We dedicated five years to searching for fossils of this nature, as an in-depth examination of the early ape family tree revealed significant gaps, with North Africa serving as that missing piece,” remarked Hesham Salam, a paleontologist at Mansoura University.

For further details, refer to the results published in the journal Science.

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Shoruk F. Al Ashkar et al. 2026. An early Miocene ape living at the biogeographic crossroads of African and Eurasian hominids. Science 391 (6792): 1383-1386; doi: 10.1126/science.adz4102

Source: www.sci.news

Colorado Residents Encounter Unprecedented Early Water Restrictions

Residents of Colorado are facing unprecedented water restrictions due to a historic snow drought and extreme heat wave.

On Wednesday, Denver Water announced the need for a 20% reduction in water usage, urging residents to disable automatic irrigation systems until mid-May and limiting tree and shrub watering to just twice a week.

Todd Hartman, a spokesperson for Denver Water, stated, “The situation is dire. If conditions don’t improve, we might have to limit water use to only one day a week in the coming months.”

This marks the first instance in 2023 that Denver Water has imposed restrictions.

Colorado’s snowpack peaked at critically low levels on March 12, about a month earlier than usual, subsequently diminishing during the recent widespread heat wave affecting nearly all Western states.

Peter Goble, Colorado’s assistant state meteorologist, noted, “Current snowpack levels are at their lowest since at least 1981, with approximately 40% of the snowpack lost since March 12 due to heat.” He added, “The situation resembles conditions typically seen in late April or early May.”

These water restrictions signal a worrying trend for many states in the West as officials strive to combat extensive drought conditions. Nearly every snow basin in the Mountain West is experiencing unprecedented winter temperatures, resulting in severely diminished water supplies. For more information, visit the US Drought Monitor. The reduced snowpack raises the risk of severe wildfires, diminishes hydroelectric power generation, and imposes additional restrictions on farmers.

Hartman remarked that communities east of the Rocky Mountains and along Colorado’s frontier are facing similar challenges as Denver.

Members of the Aurora City Council are also contemplating similar water restrictions. Current reservoir levels are about 58%, according to the city’s website. A water shortage emergency was declared on March 20 after a significant spike in consumption was reported in Erie.

Gabi Ray, the town spokeswoman, expressed concern that Erie is at risk of exhausting its water supply due to many residents watering their lawns early due to unseasonably high temperatures.

“We were on track to run out of water within just a day, which is why this is such an emergency,” she stated.

Erie officials have urged local residents to cease using irrigation systems immediately.

Goble reported that the recent heatwave has broken numerous temperature records across Colorado, often by significant margins.

“I can’t recall ever witnessing so many records fall during a single heatwave,” he noted. “For instance, in Fort Collins, last Saturday reached 91 degrees, breaking the old March record of 81 degrees, and this wasn’t just a one-time occurrence.”

Skiers at Breckenridge Ski Resort this month as temperatures soar.
Michael Ciaglo/Getty Images

Denver Water, serving approximately 1.5 million residents in and around Denver, sources about half of its water from the Upper Colorado River and South Platte River basins. Recent reports indicate that the snowfall for the latter is approximately 42% of normal levels, while the former stands at 55%.

Overall, Denver Water’s reservoirs are currently about 80% full, which is only slightly below the usual levels.

“That’s positive news,” Hartman commented. “However, with such low snowpack, we can’t rely on substantial runoff to refill the reservoirs.”

Essentially, the snowpack, serving as a natural reservoir, is largely depleted and won’t be replenished until late spring and summer when runoff typically peaks.

In Erie, officials plan to deploy smart meters to monitor residential water usage closely, implementing measures to enforce water conservation over the coming week. Ray stated that public works crews will actively patrol neighborhoods for active sprinklers.

“Residents may feel frustrated by our stringent measures, but they might not fully grasp the consequences of inaction,” Ray emphasized. “We’re facing a serious emergency where taps could run dry. Essential services, including hospitals, schools, and fire hydrants, will be affected.”

While restrictions on outdoor watering may be lifted soon, Ray anticipates more limitations will be enforced this spring and summer.

Source: www.nbcnews.com

Powerful Jaws of Early Triassic Cyclidan Crustaceans: A Deep Dive into Ancient Marine Life

Paleontologists have unveiled a fascinating new species of enigmatic ciclidan crustacean, identified from three exceptionally preserved specimens hailing from China’s Early Triassic Guiyang biota.



Yunnanosiculus fortis. Image credit: Sun et al., doi: 10.1002/spp2.70052.

The Cyclidae represent a unique group of arthropods that first emerged during the Carboniferous period and persisted until the late Cretaceous period.

Despite their significance, their fossil record is scant, as most findings only display the carapace (hard shell) of these creatures, with many anatomical features remaining elusive.

“Cyclida is an arthropod order integral to the Guiyang biota,” explains Dr. Xiaoyuan Sun from the China University of Geosciences, alongside collaborators from China and the United States.

“This specialized group of crustaceans originated in the Mississippi Sea (359-323 million years ago) and went extinct during the Maastrichtian (73-66 million years ago) of the Late Cretaceous Period.”

“They’re classified as crustaceans due to distinctive traits such as antennae, mandibles, and maxillae.”

“Sadly, our comprehension of ciclidan crustaceans remains limited because of their rarity in the fossil record.”

Typically, only the robust carapace is preserved, with the antennae and limbs being scarcely found.

The newly identified ciclidan species, designated Yunnanosiculus fortis, thrived during the late Dinerian period of the early Triassic, around 251 million years ago.

It is described based on three specimens sourced from the Daye Formation in Guizhou Province, China.

These fossils unveil an oval carapace featuring narrow, smooth margins, well-defined antennae, and seven pairs of thoracic segments.

Significantly, one specimen retains a pair of robust lower jaws, an exceptionally rare feature in ciclidan fossils.

The holotype’s carapace measures approximately 19.8 mm long by 14.7 mm wide, with the lower jaw spanning about 1.7 mm long and 0.8 mm wide.

Microscopic X-ray fluorescence analysis revealed elevated levels of calcium and phosphorus within the mandible and other structures, indicating they were thick and heavily calcified.

Yunnanosiculus fortis boasted a notably sturdy oval lower jaw,” the research team stated.



Holotype of Yunnanosiculus fortis. Scale bar – 2 mm. Image credit: Sun et al., doi: 10.1002/spp2.70052.

This remarkable discovery broadens the known geographic range of Early Triassic cichlidans.

Previously, fossils from this era were primarily registered from Madagascar and select regions of Europe.

The new species signifies the oldest record of cichlidans located in the eastern Tethyan area.

“The identification of this new species from China enhances our understanding of the paleogeographical distribution of Early Triassic cichlidans,” the researchers noted.

“Early Triassic cyclidans demonstrate widespread distribution across Madagascar, Europe, and China.”

“However, by the Late Triassic, their presence was predominantly limited to Europe.”

These fossils also provide insights into the evolutionary trajectory of these enigmatic creatures.

By examining the morphological data from Yunnanosiculus fortis, scientists reconstructed morphospace—an approach to analyze the diversity of body morphology within cichlidans and other related species.

The findings indicate that cichlidans underwent significant diversification early in their history during the Carboniferous period, with a gradual reduction in disparity in later geologic periods.

This pattern corroborates the “initial burst” model of evolution, where groups diversify rapidly soon after emerging, followed by a phase of slow evolutionary change.

This discovery further enriches our understanding of ecosystems following the Permian-Triassic mass extinction, which eradicated over 80% of marine life.

The fossil evidence from the Guiyang biota and other Early Triassic sites suggests that complex marine communities might have been reinstated earlier than initially believed.

By revealing new anatomical details and extending the geographic record of cichlidans, Yunnanosiculus fortis offers valuable insights into the recovery and evolution of marine life during one of Earth’s most chaotic periods.

“The addition of new species and the re-evaluation of the chronological paleogeography of Triassic cichlids illustrate that early Triassic cichlids were the most broadly distributed, with a gradual decline in distribution thereafter,” the authors concluded.

“This trend mirrors the global distribution of ammonoid and other marine invertebrate species during the Early Triassic and may relate to the reduction of environmental gradients in varying latitudinal zones post-Permian-Triassic mass extinction.”

The groundbreaking discovery of Yunnanosiculus fortis is discussed in the research paper published in the journal Paleontology Papers.

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Sun Xiaoyuan et al.. 2025. A new Induan (Early Triassic, Dinerian) cichlidan crustacean discovered from the Guiyang biota. Paleontology Papers 11 (6): e70052; doi: 10.1002/spp2.70052

Source: www.sci.news

Record-Breaking Early Heatwave Hits California and the Southwest

This week, much of the western United States is experiencing a summer-like heatwave in March, with temperatures soaring across California and the Southwest, raising significant climate concerns.

Forecasters predict high temperatures exceeding 90 degrees Fahrenheit will blanket Southern California and reach triple digits in parts of Arizona and Nevada. On Monday, about 39 million residents were placed under heat warnings, with expectations for the heatwave to intensify as the week progresses.

The National Weather Service attributes this “unusually rapid” heatwave to a unique atmospheric pattern characterized by a dome of high pressure settling over the West, trapping heat and humidity.

“We anticipate daily record ties and new records emerging throughout Southern California, the desert Southwest, and the Great Basin over the next few days,” the agency noted in their Monday short-term forecast. “These rising temperatures are paving the way for even more extreme and widespread record heat later this week.”

In Los Angeles, temperatures are expected to reach the mid to upper 90s this week, peaking at 98 degrees on Thursday. In Phoenix, readings could soar to 105 degrees by Thursday, while southern Nevada cities might hit 107 degrees, marking an exceptionally hot start to the year.

“Temperatures will be more than 20 degrees above normal, making it feel more like early June than mid-March,” the Las Vegas Weather Bureau stated in a recent post on X.

Cities likely to break monthly temperature records in the coming days include San Francisco, Los Angeles, Sacramento, and Palm Springs in California, alongside Phoenix and Tucson in Arizona, Las Vegas, Salt Lake City, Albuquerque, Colorado Springs, and Denver in Colorado.

Heat domes occur when a powerful, persistent area of high pressure hovers over land, effectively trapping hot air.

This week’s heatwave is especially concerning due to its unusual timing and extended duration. The Bureau of Meteorology cautioned that this heat dome might be “one of the strongest we’ve observed for this time of year,” with little relief expected until late next week.

While linking specific extreme weather events directly to climate change remains challenging, studies indicate that heatwaves are becoming more frequent, intense, and prolonged as global temperatures rise.

Extended periods of extreme heat pose significant risks to vulnerable populations, including children, the elderly, and individuals with pre-existing health conditions, especially as they adjust to summer-like climates.

The National Weather Service San Diego office warned, “Moderate to severe heat risk is expected. Please stay safe, especially for those without air conditioning. Avoid outdoor activities during peak heating hours.” They shared this announcement via X on Sunday.

This March heatwave has further worsened the West’s ongoing snow drought, diminishing the region’s already low snowpack and increasing concerns about wildfire risks and water availability for the upcoming months.

As the West faces soaring temperatures, a major winter storm is impacting the upper Midwest and Upper Great Lakes, with heavy snowfall anticipated in Wisconsin and Michigan on Monday. More than 120 million residents from the Mississippi Valley to New England also face wind warnings, with potential for damaging winds and tornadoes in areas like Pennsylvania, New Jersey, and Washington, D.C.

Simultaneously, Hawaii has been battered by a powerful atmospheric river, bringing continuous rain and resulting in widespread flash flooding and landslides over the past five days.

Source: www.nbcnews.com

How Early Howler Monkeys Adapted to Leaf-Based Diets 13 Million Years Ago

Discoveries of the Fossilized Jaw of an Ancient Monkey Species Stiltonia victoriae unveil insights from Colombia’s La Victoria Formation, indicating that early primates in South America adapted to leaf consumption, which enabled them to grow larger and explore new ecological niches. This remarkable find may also provide clues about the timeline of when this lineage developed the anatomical traits responsible for the powerful howls seen in today’s howler monkeys.



Howler monkey wearing a cloak (Alouatta palliata) in Panama. Image credit: Ariel Rodriguez-Vargas / CC BY 4.0.

The ancient primate Stiltonia victoriae thrived in what is now Colombia during the Miocene epoch, approximately 13 million years ago.

Dr. Siobhan Cook, a researcher from Johns Hopkins University, stated, “Prior to this discovery, there was no evidence indicating that South American primates consumed leaves.”

This research helps address crucial questions about ecological evolution in one of the Earth’s most biodiverse regions.

“What evolutionary changes occurred in the Amazon rainforest during the existence of these monkeys?”

In their recent study, Cook and colleagues investigated two fossilized mandibles of Stiltonia victoriae from Colombia’s La Victoria Formation in the Tatacoa Desert.

The findings indicate when this ancient monkey developed the ability to eat leaves, expanding its diet beyond fruit. This adaptation enabled it to grow larger and lessen food competition among howler monkeys and other primate species in ancient ecosystems.

“Millions of years ago, ancient monkeys traversed trees in what is now the Tatacoa Desert, once inhabited by wetland grasses, forests, and riverbanks,” said Dr. Cook.

These monkeys coexisted with long-extinct fauna in the Amazon basin, including giant sloths and armored armadillos.

“Before this, fossil findings were scarce. With Stiltonia victoriae, we could only glean knowledge from a few facial and cranial bone fragments,” Cook remarked.

“The latest discoveries not only shed light on their biodiversity and dietary habits but may also provide insight into when howler monkeys developed their distinctive ‘howl’, the loudest vocalization among land mammals.”

The structure of the jaws indicated a broad and deep mandibular body, which may have allowed the hyoid bone to protrude, similar to modern howler monkeys, potentially enabling their iconic calls.

“However, we are still uncertain about their exact behavior,” Dr. Cook added.

Paleontologists employed scans of the jaw fossils to create a 3D model for detailed analysis.

From the structure of the mandibular molars, researchers determined the dietary patterns, size, and distinguishing features of Stiltonia victoriae, comparing it against 3D models of other South American primate fossils, including Stiltonia tatakoensis, a known ancestor of howler monkeys.

They also closely examined the jaws of modern howler monkey ancestors and their relatives, such as spider monkeys and woolly gibbons residing in rainforests.

“Like modern howler monkeys, Stiltonia victoriae possessed relatively large molars with protrusions to act as ‘scissors’ for efficiently grinding carbohydrates, an adaptation common in leaf-eating primates,” said Dr. Cook.

Through their research, the body weight of Stiltonia victoriae was reconstructed, revealing these monkeys weighed between 17 and 22 pounds (8 to 10 kg).

Dr. Cook highlighted, “Previous South American monkeys in the fossil records were significantly smaller. This suggests that for the first time, these monkeys had access to abundant food sources, primarily leaves, enabling them to evolve into a heavier ecological niche.”

This discovery marks the emergence of a large and diverse group of primates in South America.

“We can now accurately trace the origins of various modern lineages.”

These findings will be published in the journal Paleoanthropology.

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Siobhan B. Cook et al. 2026. Mandibular specimen of Stiltonia victoriae from La Victoria Formation, La Venta, Colombia. Paleoanthropology 1: 148-170; doi: 10.48738/2026.iss1.3992

Source: www.sci.news

Ancient 275-Million-Year-Old Amphibian Relative with Twisted Jaw Redefines Diet of Early Quadrupeds

A groundbreaking discovery in paleontology has unveiled a new genus and species of Permian archaic tetrapods, identified from fossilized jawbones found in Brazil. Named Tanika amnicola, this intriguing amphibian relative showcases unique horizontal teeth and abrasive, file-like surfaces. This suggests that ancient tetrapod vertebrates may have begun experimenting with plant consumption much earlier than previously thought.



Tanika amnicola. Image credit: Vitor Silva.

Tanika amnicola thrived in the southern regions of the Gondwana supercontinent during the early Permian period, approximately 275 million years ago.

Tanika amnicola has captivated researchers,” says Dr. Jason Pardo, a paleontologist at the Field Museum.

“We were intrigued by an unusual twist in its jaw that we were determined to understand.”

“For years, we speculated whether this was a variant, but with nine jaw samples now extracted, all exhibiting this distinctive twist—some exceptionally well preserved—it’s clear this was characteristic of the species, not a deformity,” he added.

Tanika amnicola represents a pedunculated tetrapod lineage, the oldest subset of tetrapods that eventually diversified into two major groups: those laying eggs outside of aquatic environments and those that lay eggs in water.

Modern reptiles, birds, and mammals descend from the branches that evolved to lay watertight eggs on land, while contemporary amphibians, like frogs and salamanders, represent tetrapod relatives that require moist environments for their eggs.

Nonetheless, some pedunculated tetrapods persisted even after more modern variations evolved, with Tanika amnicola being a notable example.

“In essence, Tanika amnicola survived as a remnant of the pedunculated tetrapod lineage long after newer tetrapods emerged. Its appearance is somewhat akin to that of a platypus—a true living fossil,” remarked Dr. Pardo.

Many aspects of Tanika amnicola‘s anatomy still puzzle scientists.

“The isolated jawbones we’ve discovered are remarkably unique and distinctive,” stated Dr. Ken Angielczyk, curator of paleomammalogy at the Field Museum.

“However, until we find a skull or additional bones definitively connected to these jaw samples, we cannot conclusively ascribe other nearby bone fragments to Tanika amnicola.”

Yet, the jawbone alone is revealing, demonstrating the rarity of this creature.

“Run your tongue across your lower teeth. Do you feel the tops pointing towards the roof of your mouth?” they explained.

“In Tanika amnicola, the lower jaw twists, with teeth projected sideways rather than upwards.”

“Conversely, the portion of the jaw facing the tongue in Tanika amnicola angles upward, towards the roof of the mouth.”

“The jawbone is adorned with numerous small teeth, known as denticles, creating a grinding surface akin to a cheese grater.”

Scientists hypothesize that the teeth and dental arrangements in the upper jaw harmonized with those in the lower jaw.

“We theorize that the lower jaw’s teeth would rub against similar teeth in the upper mouth,” Pardo explained.

“This grinding action suggests a distinctive feeding method predominantly aimed at plant material.”

“Based on dental morphology, we believe Tanika amnicola was likely an herbivore, consuming plants at least occasionally,” remarked Dr. Juan Carlos Cisneros from the Federal University of Piauí.

“It’s astonishing that a quadrupedal creature like Tanika amnicola existed, especially considering most of its tetrapod relatives primarily consumed meat, indicating an evolved adaptation to a plant-based diet.”

The peer-reviewed findings are published in the journal Proceedings of the Royal Society B.

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Jason D. Pardo et al.. 2026. A quadrupedal organism with an anomalous jaw structure living during the early Permian period in Brazil. Proc Biol Sci 293 (2066): 20252106; doi: 10.1098/rspb.2025.2106

Source: www.sci.news

Astronomers Uncover Hidden Structure of the Early Universe: Breakthrough Discoveries Explained

Astronomers have utilized spectral data from the Hobby-Eberly Telescope at McDonald Observatory to construct the most intricate 3D map of faint cosmic structures dating back 9 to 11 billion years, unveiling galaxies and intergalactic gas previously undetectable by telescopes.



A line intensity map showcasing the distribution of excited hydrogen in the universe approximately 10 billion years ago. The stars denote areas where HETDEX has identified galaxies. The inset simulates the structure after optimizing the data by reducing background noise. Image credit: Maja Lujan Niemeyer / Max Planck Institute for Astrophysics / HETDEX / Chris Byrohl / Stanford University.

“Studying the early Universe reveals how galaxies have evolved into their current forms and the role that intergalactic gas plays in this transformation,” stated Dr. Maya Lujan Niemeyer, an astronomer at the Max Planck Institute for Astrophysics and Ludwig Maximilian University of Munich, and a key member of the Hobby-Eberly Telescope’s Dark Energy Experiment (HETDEX).

“Many objects from this epoch are faint and challenging to observe due to their vast distances,” she continued.

“Through a technique known as line intensity mapping, this innovative map enhances our understanding of these objects, adding complexity and depth to this crucial era of cosmic history.”

Although line intensity mapping is not a novel methodology, this is the first instance it has been employed to visualize Lyman alpha emissions with such exceptional precision across an extensive dataset.

The HETDEX project harnesses the capabilities of the Hobby-Eberly Telescope to catalog over 1 million luminous galaxies to decode the mysteries of dark energy.

What differentiates this project is its extensive measurement scope, equivalent to observing more than 2,000 full moons and amassing a colossal dataset of over 600 million spectra across an expansive area of the sky.

“We leverage only a fraction of our data—approximately 5%,” remarked Dr. Karl Gebhardt, principal investigator of HETDEX and an astronomer at the University of Texas at Austin.

“This leaves significant potential for future research utilizing the remaining data.”

“While HETDEX captures images of the entire sky, only a small subset of the collected data comprises sufficiently bright galaxies for our research,” noted Dr. Lujan Niemeyer.

“These galaxies are merely the beginning. In the vast expanses in between, lies an entire ocean of light awaiting discovery.”

To construct this groundbreaking map, astronomers employed a supercomputer at the Texas Advanced Computing Center to meticulously analyze approximately half a petabyte of HETDEX data.

Using the coordinates of luminous galaxies already detected by HETDEX, they inferred the positions of fainter galaxies and adjacent glowing gas.

Due to the gravitational forces that cause matter to cluster, the existence of one bright galaxy implies the presence of nearby celestial objects.

“This allows us to utilize known galaxy positions as reference points to ascertain distances to fainter celestial entities,” explained Dr. Eiichiro Komatsu, HETDEX scientist and astronomer at the Max Planck Institute for Astrophysics.

“The resultant map emphasizes regions surrounding bright galaxies while providing intricate details of the areas in between.”

“Simulation models exist for this cosmic era, yet they remain hypothetical; they do not represent the actual universe.”

“We now possess a foundational understanding that allows us to verify whether the astrophysics underlying these simulations holds true.”

For more on these remarkable findings, published on March 3, 2026, in the Astrophysical Journal.

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Maya Lujan Niemeyer and others, 2026. Lyα intensity mapping in HETDEX: Galaxy-Lyα intensity cross-power spectrum. APJ 999, 177; doi: 10.3847/1538-4357/ae3a98

Source: www.sci.news

How Skin, Lung, and Intestinal Inflammation Could Signal Early Onset of Alzheimer’s Disease

Amyloid plaques in the brain are a defining feature of Alzheimer’s disease, but what if the roots of the condition start elsewhere in the body?

Alamy

Alzheimer’s disease has traditionally been believed to originate in the brain. However, comprehensive genomic analysis indicates that inflammation in distant organs such as the skin, lungs, or intestines may initiate the condition, potentially decades before noticeable memory decline occurs. This shift in understanding could shed light on why Alzheimer’s treatments have been largely ineffective. Current drugs intervene too late; a focus on early-stage inflammation in peripheral organs may be crucial.

“As neuroscientists, we tend to focus on the brain, but this study highlights that the brain is interconnected with the body, and changes elsewhere can impact brain function,” states Donna Wilcock from Indiana University, not involved in the study. “Although Alzheimer’s is a brain disorder, we must consider the entire body when discussing its genesis.”

To explore the genetic underpinnings of Alzheimer’s disease, researchers including Cesar Cunha from Denmark’s Novo Nordisk Foundation Basic Metabolic Research Center analyzed genetic data from the European Alzheimer’s and Dementia Biobank, encompassing over 85,000 individuals with the disease and approximately 485,000 without it. They also evaluated gene activity in 5 million single cells across 40 body regions and 100 brain regions.

The study scrutinized 1,000 genes linked to an increased Alzheimer’s disease risk, surprisingly finding these genes were more abundant in organs like the skin, lungs, and digestive system than in the brain. “It was counterintuitive at first because the expression of these risk genes in brain cells seemed low,” notes Cunha. “Our continued analysis revealed their primary presence in other body parts.”

Many of these Alzheimer’s risk genes are tied to immune regulation and are particularly abundant in barrier tissues like the skin and lungs, which defend against bacteria and toxins through inflammatory responses. “This suggests that Alzheimer’s might initiate due to inflammation in these peripheral organs,” Cunha explains. Genetic variations may even dictate the extent of inflammation and its impact on brain health. Hence, individuals with a family history of Alzheimer’s could be more vulnerable to the disease amidst infections or inflammatory episodes.

Interestingly, the highest expression of these gene variants occurs when individuals reach ages 55 to 60. Inflammation during this period seems likely to trigger Alzheimer’s, corroborated by long-term studies from Hawaii. Inflammatory markers rise in individuals in their late 50s, with those in their 70s and 80s exhibiting increased Alzheimer’s likelihood. “A person could suffer from lung inflammation due to a viral infection at age 55, which might initiate Alzheimer’s 30 years later, but the exact mechanisms remain elusive,” Cunha remarks.

Rezanur Rahman, a researcher at QIMR Berghofer Medical Research Institute, has identified a genetic mutation associated with Alzheimer’s that appears concentrated in the skin and lungs. More research is essential to understand their functional role in symptom progression, Rahman states. “Association does not imply causation.”

Nonetheless, findings imply that individuals with various inflammatory conditions—such as eczema, cold sores, pneumonia, periodontal disease, Lyme disease, syphilis, diabetes, high blood pressure, and intestinal infections—may face heightened Alzheimer’s disease risk in the future. This correlation is particularly robust when inflammation occurs in middle age, around ages 45 to 60, aligning with Cunha’s insights.

Previously, the brain was deemed immune-privileged and largely unaffected by inflammatory processes elsewhere in the body. Bryce Vissel from St. Vincent’s Hospital in Sydney, Australia, among those who first proposed inflammation as a trigger for Alzheimer’s, acknowledges that while initially contentious, new evidence supports that peripheral inflammation from infections or injuries may indeed instigate the disease.Infection or injury can affect brain function.

When inflammation occurs, immune cells are activated, releasing signaling proteins like cytokines that can cross into the brain via the bloodstream. An unpublished study by Vissel and his team indicates that cytokines may disrupt neuronal connections, potentially leading to memory impairment.

Concurrently, research has shown that the blood-brain barrier becomes more permeable with age, allowing inflammatory cytokines and immune cells easier access, which might elucidate why inflammation poses more of a risk during mid-life compared to youth, Cunha notes.

Current theories posit that Alzheimer’s disease stems from the accumulation of misfolded beta-amyloid and tau proteins within the brain. Yet, treatments aimed at eliminating these proteins have yielded minimal success, indicating that such accumulation might be a symptom rather than the core issue. “We’ve been trying to treat the result of the disease, not its cause,” Cunha argues.

Cunha likens this to past mistakes in obesity treatments, which initially targeted excess fat directly, failing until genetic research revealed that mutations connected with obesity are often highly expressed in the brain, disrupting appetite and energy balance. This led to the development of the weight-loss medication semaglutide (marketed as Ozempic and Wegovy), which modulates brain pathways to curb appetite.

If Alzheimer’s originates from peripheral inflammation, its treatment would necessitate a paradigm shift, Cunha asserts. Data indicate that midlife vaccinations may offer protective benefits against Alzheimer’s disease. A recent Californian study revealed that adults receiving both doses of the shingles vaccine recommended for individuals aged 50 and older were 50% less likely to develop Alzheimer’s by age 65. Another investigation found that those aged 50 and older treated with the Bacillus Calmette-Guérin (BCG) vaccine for bladder cancer had a 20% reduced risk of onset.

This phenomenon might arise as vaccines bolster the aging immune system and mitigate inflammation, suggests Wilcock. “At age 55, we should invigorate our immune systems and remind them to stay active, as most vaccinations occur in childhood.”

Beyond vaccinations, several lifestyle interventions have been shown to diminish inflammation and avert Alzheimer’s disease. These include adopting a Mediterranean diet, limiting alcohol consumption, exercising, quitting smoking, and managing blood pressure and cholesterol levels.

Professor Cunha emphasizes that the challenge lies in convincing fellow neuroscientists to recognize peripheral inflammation as a potential contributor to Alzheimer’s disease. “I’ve encountered skepticism at academic conferences, being told, ‘If you aren’t focusing on amyloid, you’re not studying Alzheimer’s disease,'” he shares. “After decades entrenched in amyloid research, adapting one’s perspective can be daunting.”

Topics:

Source: www.newscientist.com

How Early Humans Created Symbol Systems Before Writing: Uncovering Prehistoric Communication

Approximately 40,000 years ago, early humans in Europe created a sophisticated system of geometric symbols. These symbols are believed to represent an intentional, repeatable form of communication that transcends mere decoration. Discover more in a recent study published in Proceedings of the National Academy of Sciences.



Movable artefact featuring geometric symbols from the Swabian Aurignacian culture. Image credit: Christian Bentz & Ewa Dutkiewicz, doi: 10.1073/pnas.2520385123.

According to researchers Christian Benz from the Universities of Saarland and Passau, and Eva Dutkiewicz from the National Museum in Berlin, “Around 45,000 years ago, modern humans migrated into eastern and central Europe.”

During this migration, they encountered Neanderthals, their distant relatives.

In a period of rapid population turnover, modern humans produced a variety of movable artifacts, including tools and figurines crafted from materials such as ivory, bone, and antler.

These artifacts date back to the early Upper Paleolithic and are part of the Aurignacian technocomplex.

Numerous objects adorned with geometric symbols have been discovered, particularly in France’s Dordogne region, Germany’s Swabian Jura, and Belgian archaeological sites.

The researchers examined a collection of 260 mobile Aurignacian artifacts found in caves in the Swabian Jura.

These remarkable items, made from mammoth ivory, bone, and horn, date between 43,000 and 34,000 years ago.

Artifacts include tools, beads, musical instruments, and figurines representing both animals and humans, many etched with sequences of geometric signs—dots, lines, crosses, and more.

The scientists emphasized, “The inhabitants of these caves produced specialized tools for cutting meat, processing animal hides, and crafting clothing and ropes during this period.”

They also pioneered the flute, the first musical instrument made from bone and ivory.

Utilizing information theory and quantitative linguistics, the authors analyzed over 3,000 geometric symbols from the artifacts.

They assessed characteristics like repetition, diversity, and overall information density within the engraved symbols.

Dr. Benz noted, “While many theories exist, there has been minimal empirical research on the measurable properties of these symbols.”

The results revealed intriguing findings. Statistically, these Paleolithic symbols differ significantly from modern writing, which usually favors less repetition and denser information.

However, they bear a resemblance to Protocuneiform, the earliest known accounting symbols from Mesopotamia, used about 5,500 years ago.

This similarity doesn’t indicate that Ice Age Europeans had a writing system, as true writing encodes spoken language, while the Aurignacian symbols do not.

Instead, these artifacts illustrate a stable, traditional system for visually storing and conveying information without language.

The placement of symbols matters; figurines, particularly ivory ones, display a greater complexity and denser arrangement than everyday tools.

Specific symbols were exclusive to certain subjects, with dots frequently appearing on human and feline figures, while crosses were found on mammoths and horses, but never on human forms.

This pattern indicates a shared set of rules passed down through generations.

Researchers noted that unlike precuneiform, which evolved into a comprehensive script as ancient societies grew more complex, the structure of the Aurignacian symbol system remained remarkably consistent over roughly 10,000 years.

Dr. Benz stated, “Our analysis reveals that these symbol sequences have no correlation to contemporary writing systems, which represent spoken language and feature high information density.”

In contrast, the symbols found in archaeological artifacts often showcase repetitive patterns: cross, cross, cross, line, line, line, a hallmark absent in spoken language.

“Our findings also indicate that Paleolithic hunter-gatherers developed symbols with an information density statistically akin to the earliest proto-cuneiform tablets from ancient Mesopotamia, which emerged 40,000 years later.”

Proto-cuneiform symbols exhibit a similar repetitive quality, with individual symbols appearing at consistent rates, showcasing comparable complexity.

This discovery supports the growing consensus among archaeologists that symbolic communication likely evolved gradually through systems aimed at recording numbers, events, or social knowledge, rather than emerging suddenly as writing.

Some symbols may have tracked seasonal patterns, hunting data, or ritual concepts, though their precise meanings remain elusive.

Dr. Dutkiewicz added, “Modern humans have the benefit of thousands of years of accumulated knowledge that was unavailable to our ancestors. However, anatomically, Stone Age humans may have possessed cognitive abilities akin to ours.”

“The capacity to record and share information was crucial for Paleolithic humans, possibly enhancing their ability to coordinate groups and improve survival strategies.”

“They were adept craftsmen, evident in the portability of many of these artifacts, which often fit seamlessly in the palm of the hand, reminiscent of proto-cuneiform tablets.”

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Christian Benz and Eva Dutkiewicz. 2026. Early humans developed a traditional symbol system 40,000 years ago. PNAS 123 (9): e2520385123; doi: 10.1073/pnas.2520385123

Source: www.sci.news

Discovering Diverse Marine Amphibian Communities: Early Triassic Fossils Uncovered in Australia

Recent findings from museum collections in Australia and the United States showcase the incredible diversity of the Western Australian trematosaurid temnospondyl, underscoring how early marine amphibians proliferated across the continent shortly after the end-Permian mass extinction.



Ancient marine amphibians Erythrobatrachus (foreground) and Aphanelamma (background) traversed the northern coast of modern-day Western Australia 250 million years ago. Image credit: Pollyanna von Knorring, Swedish Museum of Natural History.

“The catastrophic end-Permian mass extinction and severe global warming gave rise to modern marine ecosystems at the dawn of the Mesozoic Era, around 252 million years ago,” stated Dr. Benjamin Kjaer from the Swedish Museum of Natural History and his colleagues.

“This significant evolutionary milestone marked the early emergence of sea-going tetrapods (limbed vertebrates), including amphibians and reptiles that quickly established themselves as dominant aquatic apex predators.”

“To date, the earliest sea monster fossils have primarily been documented in the Northern Hemisphere.”

“In contrast, the fossil record from the Southern Hemisphere remains geographically sparse and inadequately understood.”

Paleontologists recently analyzed marine amphibian fossils from the renowned Kimberley region of Western Australia’s far north.

“These fossils were uncovered during scientific expeditions in the early 1960s and 1970s,” the researchers noted.

“The specimens were subsequently distributed to various museum collections across Australia and the United States.”

“The results of this research were initially published in 1972, identifying a single species of marine amphibian, Erythrobatrachus nooncambahensis, named after skull fragments discovered at Noonkumba Farm, east of Derby in the Kimberley region.”

“Unfortunately, the original fossil of Erythrobatrachus has since been lost over the past 50 years.”

“This prompted a survey of international museum collections, leading to the rediscovery and reanalysis of these ancient marine amphibian remains in 2024.”

According to scientists, Erythrobatrachus is classified within the trematosaurid family of temnospondyls.

“Trematosaurids bore a superficial resemblance to crocodiles and were related to modern salamanders and frogs, reaching lengths of up to 2 meters (6.6 feet),” the researchers explained.

“These fossils hold significant importance as they were found in rocks deposited as coastal sediments less than a million years after the end-Permian mass extinction.”

“Thus, they represent the oldest currently recognized groups of Mesozoic marine tetrapods in geological terms.”

However, detailed investigations revealed that the skull fragments of Erythrobatrachus were not unified but belonged to at least two distinct types of trematosaurids: Erythrobatrachus and another species from the well-known genus Aphanelamma.

“Examination of Erythrobatrachus using advanced 3D imaging indicated the skull measured approximately 40 centimeters (16 inches) when intact, suggesting it was a robust, broad-headed apex predator,” the authors stated.

“Conversely, Aphanelamma were similar in size but featured elongated snouts adapted for catching smaller fish.”

“Both types of trematosaurids occupied the water column yet targeted different prey within the same habitat.”

“Furthermore, the fossils of Erythrobatrachus are uniquely found in Australia, while Aphanelamma has been discovered in similarly aged deposits across regions like the Scandinavian Arctic, Svalbard, the Far East, Pakistan, and Madagascar.”

“The Australian trematosaurid fossils provide evidence that these early Mesozoic marine tetrapods not only radiated swiftly into various ecological niches but also dispersed globally along the coastal margins of interconnected supercontinents during the initial two million years of the dinosaur epoch.”

The team’s study was recently published in the Journal of Vertebrate Paleontology.

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Benjamin P. Care and colleagues. Revision of Trematosauridae Erythrobatrachus nooncambahensis: A mysterious marine vertebrate assemblage from the Lower Triassic of Western Australia. Journal of Vertebrate Paleontology, published online on February 22, 2026. doi: 10.1080/02724634.2025.2601224

Source: www.sci.news

Early Homo Species First Appeared in the Jordan Valley Over 1.9 Million Years Ago

New Study Reassesses the Age of the Jordan Valley Ubaydiya Layer: Dating Back Approximately 2 Million Years, Comparable to Georgia’s Dmanisi Ruins. This Research May Mark a Critical Moment in Human Evolution, Indicating That Early Humans with Advanced Tool-Making Skills Expanded into New Environments Much Earlier Than Previously Believed.

Artist’s reconstruction of Homo erectus. Image credit: Yale University.

The Ubaydiya ruins are situated in Israel’s Jordan Valley, nestled between Menahemia village and Beit Zerah kibbutz.

Discovered in 1959, this site has yielded a distinctive Ature hatchet but only a few human remains.

“The Ubaydiya Formation has been a focus of research for years, offering early evidence of the Acheulean culture, recognized by its large, double-sided stone tools, often found alongside a diverse array of fauna, including species from Africa and Asia,” remarked Ali Matmon, a professor at the Hebrew University of Jerusalem.

“Yet, determining the precise age of this site has posed a considerable challenge over the decades.”

“Historically, researchers estimated Ubaydiya’s age to be between 1.2 and 1.6 million years, based on relative chronology.”

To ascertain the site’s true age, researchers employed three independent dating techniques: magnetic stratigraphy, uranium-lead (U-Pb) dating of mollusc shells, and cosmogenic isotope burial dating.

“Cosmogenic isotope burial dating measures rare isotopes generated when cosmic rays strike rocks on Earth’s surface,” explained the research team.

“Once buried, these isotopes decay at a known rate, effectively beginning a geological clock that indicates how long they have been underground.”

“We also analyzed remnants of Earth’s ancient magnetic field preserved in lake sediments at the site,” they added.

“As sediment settles, it locks in the orientation of the planet’s magnetic field at that time.”

“By correlating these magnetic signatures with known historical reversals in Earth’s magnetic field, we established that this formation emerged during the Matsuyama period, over 2 million years ago.”

“We also examined the fossils of melanopsis, utilizing U-Pb dating to determine the age of shells and freshwater snails within the sediment, which helped us establish the minimum age of the layer where the stone tools were discovered.”

“Overall, our findings indicate an age much earlier than previously anticipated.”

Double-sided stone tool excavated from the Ubaydiya site in Israel. Image credit: Omri Barzilai.

The team’s results indicate that the Ubaydiya site is at least 1.9 million years old, significantly older than prior estimates.

“This new chronology suggests that Ubaydiya is roughly contemporaneous with the renowned Dmanisi site in Georgia, implying that our ancestors migrated to different regions simultaneously,” the scientists noted.

“Additionally, this suggests that both simpler Oldowan and more advanced Acheulean stone tool-making techniques began their migration from Africa as various hominin groups explored new terrains.”

This groundbreaking study is published in the Quaternary Science Review.

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A. Matmon et al. 2026. The Complex History of Radiation Exposure Burials in the Dead Sea Rift Valley and the Recycling of Pleistocene Sediments Affecting the Age of the Acheulian Site Ubaydiya. Quaternary Science Review 378: 109871; doi: 10.1016/j.quascirev.2026.109871

Source: www.sci.news

Four Astronauts Arrive at Space Station Following Early Departure of Previous Crew

Four new crew members, including two from the United States, received a warm welcome upon their arrival at the International Space Station (ISS) on Saturday.

The spacecraft, transporting NASA astronauts Jessica Meir and Jack Hathaway, European Space Agency astronaut Sophie Adenot, and Russian cosmonaut Andrei Fezyaev, docked with the ISS at 3:16 p.m. ET.

“Everyone arrived safely. We have been looking forward to this moment for a long time,” commented Sergei Kud Sverchkov, a current member of the Russian Federation’s Roscosmos crew on board.

The Dragon spacecraft was propelled into orbit by a SpaceX Falcon 9 rocket early Friday morning.

“We’re thrilled to be here and ready to get to work,” Meir said after meeting the ISS crew. “We made it. We’re here. We love you.”

Later, Adenot mentioned how much she enjoyed the journey.

“It was quite a ride, but it was a lot of fun,” she remarked. “Seeing the Earth from above is mesmerizing; you can’t distinguish any lines or boundaries.”

They arrived at an unusually quiet orbital laboratory.

Originally, the four crew members were expected to overlap in space with the departing team on Mission Crew 11. However, that group had to return to Earth early due to medical issues. (NASA has maintained privacy regarding the identities of the affected astronauts.)

The Crew-11 astronauts departed on January 14, leaving behind NASA astronaut Chris Williams and Russian cosmonauts Kudo Sverchkov and Sergei Mikayev on the ISS.

The four new arrivals will be designated Crew 12, increasing the ISS’s occupancy to seven astronauts.

“Floating in zero gravity is an incredible experience,” Hathaway said after greeting fellow passengers. “The journey was fantastic, shared with great friends from Crew 12.”

A time-exposure shot of a SpaceX Falcon 9 rocket launch from Pad 40 at Cape Canaveral Space Force Station on Friday.
John Rau/AP

The crew launched from SpaceX’s Falcon 9 rocket at 5:15 a.m. ET from Cape Canaveral Space Force Station, Florida.

NASA delayed the launch by two days due to high winds affecting the flight path earlier in the week. The agency continuously monitors weather conditions for safe ascent and emergency scenarios.

Recently, a Falcon 9 incident during an unmanned mission to deploy SpaceX’s Starlink satellites prompted NASA to review safety findings before this launch.

Following the Feb. 2 incident, SpaceX paused launches for an investigation with the Federal Aviation Administration (FAA). The FAA later permitted SpaceX to resume operations, successfully deploying Starlink satellites thereafter.

NASA officials confirmed in a recent press conference that there have been no significant issues while the ISS has been understaffed, allowing a relaxed timeline for the arrival of new crew members.

“We anticipate additional support soon, but will launch when ready,” stated Dina Contera, NASA’s deputy director of ISS programs at the Johnson Space Center.

Crew-12 members, from left, Andrei Fezyaev, Jack Hathaway, Jessica Meir, and Sophie Adenot during a press conference at NASA.
NASA

The Crew-12 mission members are slated to stay at the ISS for approximately eight months, where they will conduct scientific research including food production in space, examine how microgravity impacts blood flow, and study bacteria linked to pneumonia. NASA states these endeavors will enhance research for future missions to the Moon and Mars and will provide benefits for humanity on Earth.

This mission marks Hathaway and Adenot’s first spaceflight, while Fezyaev is on his second journey. Meir has previously spent 205 days aboard the ISS starting in July 2019 and made history with fellow astronaut Christina Koch during NASA’s first all-female spacewalk. They are also part of the Artemis II lunar orbit mission set to launch in March.

On Saturday, Meir expressed her surprise at the collaborative spirit that has turned the ISS into a beacon of human achievement.

“This represents a commitment from five nations, underpinned by trust, collaboration, and powered by science, innovation, and curiosity that has been upheld for decades,” she stated before entering the ISS. “Looking back at Earth from these windows, we are reminded that cooperation is not just possible, but essential. There are no borders in space, and hope transcends all.”

Source: www.nbcnews.com

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.

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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.

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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.

_____

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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Source: www.newscientist.com

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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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