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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

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

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



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

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

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

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

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

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

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

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

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

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

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

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

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



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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Discovering the Origins of Spider Fangs: Tracing Ancient Marine Life Back to 518 Million Years Ago



Urocodia equalis

is an early Cambrian marine predator from China’s Chengjiang biota, notable for preserving the earliest evidence of chelicerae. This unique structure is a precursor to the fangs of spiders and pincers of scorpions.



Artist’s impression of Urocodia equalis, a marine predator that roamed Cambrian seas around 518 million years ago. Image credit: Xiaodong Wang.

Spiders, scorpions, and ticks belong to a significant group of invertebrates known as chelicerates, which includes over 100,000 described species.

Characterized by articulated limbs and an external skeleton, these creatures are particularly known for their specialized limbs, called chelicerae, used for capturing prey.

The earliest fossil records of chelicerae emerged not from terrestrial habitats but from marine organisms inhabiting Cambrian seas over 500 million years ago.

In a groundbreaking study, paleontologists examined Urocodia equalis from the renowned Chengjiang Fossil Site in Yunnan Province, China.

This diminutive creature measures just 2 to 3 centimeters and features large, stalked eyes, a segmented skeleton, and articulated limbs extending from its elongated body.

“The Urocodia equalis was part of an ancient ecosystem with over 200 species thriving in the ocean more than 500 million years ago,” stated Professor Mark Williams from the University of Leicester.

“These excellently preserved fossils offer invaluable insights into the early evolution of life on Earth.”

Utilizing X-ray tomography, Professor Williams and his team conducted an in-depth analysis of Urocodia equalis, uncovering much of its soft tissue still intact.

The scans revealed small, scissor-like limbs located behind the eyes, representing an early evolutionary version of the chelicerae that later developed into the fangs of spiders and pincers of scorpions.

“During our X-ray tomography analysis, we discovered soft anatomy that had remained buried for millions of years, including these fascinating scissor-like limbs,” remarked Professor Yu Liu, a paleontologist at Yunnan University and the University of Leicester.

“This fossil is particularly intriguing as it is a distant ancestor of chelicerates like scorpions and spiders.”

Urocodia equalis‘s legs also exhibit features similar to gills, a respiratory adaptation still observed in modern horseshoe crabs.

This discovery extends the fossil record of this unique trait, providing a rare glimpse into the origins of one of evolution’s most successful hunting adaptations that emerged in ancient oceans.

Urocodia equalis has a seven-segmented head with a sclerotized lower mouth, pincer-like appendages, and bilobed body appendages equipped with overlapping exit valves,” noted the paleontologists.

“These scissor-like appendages illustrate a transitional structure between a multi-segmented appendage and a true chelicera; mega keiran represents the origin of book gills.”

Further details of these findings are published in the latest issue of Nature.

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Y. Liu et al., Urokodia: Shedding light on the origin of chelicerae and their book gills. Nature, published online July 1, 2026. doi: 10.1038/s41586-026-10713-2

Source: www.sci.news

Discovering the World’s Smallest Marsupial: Unveiling Four Distinct Species

Australian scientists have uncovered that what was previously considered a single widespread species of Planigal is actually four distinct species, including a newly identified species that thrives exclusively on the rocky slopes of Kakadu National Park.



Revised distribution of the four Planigale species complex previously classified as Planigale ingrami. Image credit: Umbrello et al., doi: 10.1093/zoolinnean/zlag082.

Planigals, small marsupials primarily feeding on insects, are known for their flat skulls which allow them to fit into narrow crevices in their habitats.

These unique creatures inhabit various terrestrial environments across Australia and New Guinea, with nine species now recognized.

Among them, Planigale ingrami holds the title of the world’s smallest marsupial, weighing an average of just 4.2 g (as little as 2.6 g) and measuring 5.7 cm from head to body.

A recent study by researchers from the Western Australian Museum and Queensland University of Technology, led by Dr. Lynette Umbrello, utilized genetic analysis and museum specimens to reveal the complex Planigale ingrami species classification, introducing Planigale tea ray and unveiling two unclassified lineages.

The team analyzed DNA samples from over 220 individuals combined with detailed measurements of skull and body proportions, derived from collections in natural history museums across Australia.

“This study leveraged historical samples to identify species that might never be documented in contemporary settings,” Dr. Umbrello noted.

“We undertook thorough genetic sampling and morphological analysis of Planigal specimens from museum collections throughout Australia.

“Our data integration approach, termed integrative taxonomy, enabled us to identify species previously grouped under a single classification.”

The researchers delineated three distinct lineages among the studied samples, including Planigale ingrami.

“We re-listed Planigale subtilissima, previously thought to belong to: Planigale ingrami, as a separate species,” Dr. Umbrello remarked.

“Furthermore, the subspecies Planigale ingrami brunea was reassigned to its original classification.”

“We also discovered a completely new species: Planigale petrophila.

Planigale petrophila (commonly known as the Arnhem Plateau Planigal) is distinguished from its relatives by several characteristics.

While most Planigal species prefer lowland clay soils, this species is adapted to rocky cliff environments.

Significantly larger than its closest relatives, it boasts the longest tail recorded for any Planigal, surpassing its body length.

Planigale petrophila is a medium-sized Planigal with a notably flat skull and an exceptionally long tail,” the scientists explained.

“It uniquely features the longest tail of any genus member (8.05-9.19cm), outstripping even the larger Planigale novaeguineae specimens (from New Guinea) that reach 8 cm.”

Currently, only three specimens of Planigale petrophila are known, all collected within a close range of 12 km in Kakadu National Park, with the latest one documented in 2004 — none have been observed since.

The researchers highlighted the concerning decline of native mammal populations in Kakadu, urging an immediate conservation assessment.

Planigale petrophila is undoubtedly rare among Australian Planigals, with just three specimens identified and its known habitat limited to a small area of the sandstone plateau and rocky slopes in Kakadu National Park,” Dr. Umbrello stated.

The only other Planigal recorded in Kakadu National Park is Planigale maculata, which occupies lowlands and basins rather than sandstone plateaus.

Planigale petrophila is distinctive for its notably longer tail compared to other Planigal species, and exhibits larger body-to-skull ratios than its genetically closest relatives.”

“Our findings suggest Planigale petrophila may be threatened,” added Dr. Andrew Baker from Queensland University of Technology and Queensland Museum.

“Given the limited geographical area where Planigale petrophila has been identified, along with the alarming declines observed in other mammal species in Northern Australia, we strongly recommend an urgent conservation assessment.”

“This species is known from only three specimens collected within 12 km and has not been encountered since 2004.”

“Accurate classification and taxonomy are vital for conservation efforts to ensure appropriate management strategies are implemented.”

“This information plays a crucial role in establishing the conservation status of this new mammal, especially considering the broader decline in Kakadu and other native species in Australia.”

The team’s results will be published in the Zoological Journal of the Linnean Society.

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Lynette S. Umbrello et al. 2026. Disentangling the Onagaplanigale (Dassuriidae: Planigale ingrami) Species Complex: Four Species Revealed Using Integrated Taxonomy. Zoological Journal of the Linnean Society 207 (2): zlag082; doi: 10.1093/zoolinnean/zlag082

Source: www.sci.news

Discovering Earth’s First Land Animals: Surprising Facts Beyond Amphibians

A paleontologist from the Field Museum of Natural History has unveiled new insights into the fossilized remains of a baby embolomere, a crocodile-like predator that inhabited ancient rivers and swamps between 350 million and 280 million years ago. Contrary to previous beliefs, these early vertebrates did not resemble tadpoles during their infancy.



New fossil evidence suggests that embolomeres did not undergo the same metamorphosis as modern amphibians, contradicting the notion that amphibians, reptiles, and mammals evolved from tadpole-like ancestors. Image credit: Berit Godling.

“Many of us learned a simplified version of evolution in high school: that fish evolved into amphibians, which then led to reptiles, and finally to mammals,” said Jason Pardo, a paleontologist at the Field Museum.

“Our research indicates that this fundamental premise—that the first four-legged vertebrates developed like amphibians—is incorrect.”

In their recent study, Dr. Pardo and colleague Dr. Arjan Mann analyzed well-preserved fossil quadrupeds from Mason Creek Lagerstätte, Illinois, known for its exceptional soft tissue specimens.

“Mason Creek is one of the world’s best fossil sites for soft tissue and delicate small fossils,” remarked Dr. Mann.

“The fossils from Mason Creek serve as a time capsule, allowing us to gain insights that were previously thought impossible.”

Embolomeres could grow over 3 meters (10 feet) as adults and were fearsome apex predators in ancient rivers, lakes, and swamps from 350 million years ago (Carboniferous period) to 280 million years ago (Permian period).

The Mason Creek specimen offers a striking contrast; though the baby is just a few centimeters long, it provides enough evidence to challenge century-old scientific assumptions.

Notably, researchers observed that embolomere offspring lacked crucial characteristics associated with amphibian tadpoles, such as external frilled gills.

No evidence of true metamorphosis was found in these early tetrapods, despite the major changes that occur during the larval stage in modern amphibians.

Instead, the life cycles of these initial tetrapods appear to resemble those of humans or fish more than they do those of amphibians.

“We examined a range of species representing various lineages throughout the fish-to-tetrapod transition and found no evidence resembling a tadpole,” Pardo stated.

“If there are no tadpoles, then metamorphosis cannot exist.”

“If creatures like embolomeres did not display tadpole morphology or undergo true amphibian metamorphosis, then the widely accepted theory that reptiles and mammals evolved from amphibian-like ancestors must be reconsidered.”

“The narrative that metamorphosis facilitated the transition of animals from water to land is no longer valid. It’s become obsolete.”

For further details, refer to the findings published in Science.

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Jason D. Pardo & Arjan Mann. 2026. Direct development of stalk tetrapods through the fin-to-limb transition. Science 392 (6804): 1292-1296; doi: 10.1126/science.aeb7635

Source: www.sci.news

Discovering Four Generations of Stars in the Globular Cluster Tarzan 5: A Breakthrough by Astronomers

Globular clusters are traditionally known to host a single, ancient population of stars. However, groundbreaking data from the NASA/ESA/CSA James Webb Space Telescope and the NASA/ESA Hubble Space Telescope has confirmed the presence of two distinct star populations within the ancient star system Terzan 5. Once classified merely as a globular cluster, Terzan 5 now also shows evidence of two recent rounds of star formation.



This Webb/NIRCam image showcases the star cluster Terzan 5. Image credit: NASA/ESA/CSA/Webb.

Terzan 5, discovered in 1968 by Armenian-Turkish-French astronomer Agop Terzan, is located approximately 19,000 light-years away in the constellation Sagittarius.

Also known as ESO 520-27 and 2MASX J17480455-2446441, this star system is home to hundreds of thousands of varied stars.

Nesting within the inner bulge of the Milky Way, Terzan 5 exhibits many characteristics reminiscent of globular clusters, yet significant findings emerged in 2009 revealing two distinct star populations.

A 2016 study using Hubble provided crucial age estimates: one population formed around 12 billion years ago, pre-dating the Milky Way, while the other emerged approximately 5 billion years ago, shortly before Earth’s formation. This complex history suggests Terzan 5’s evolution diverges from typical globular clusters.

Dr. Giorgia Zullo, a student at the University of Bologna, remarked, “Webb’s new near-infrared observations, in conjunction with Hubble’s archival data, present a clearer narrative of Terzan 5’s history.”

Studying Terzan 5 presents challenges due to its dense star environment and substantial dust cover within the galaxy.

Webb’s infrared capabilities enable astronomers to penetrate this dust, allowing for a comprehensive cataloging of both faint and distant stars.

By analyzing the colors and brightness of the stars, researchers can categorize them based on different ages and chemical compositions.

Webb successfully measured these essential properties for all visible stars, including those in Terzan 5 and unrelated foreground stars.

To distinguish Terzan 5’s stars, researchers leveraged Hubble’s long-term observations. The varying intervals between Hubble’s 12-year exposures allowed them to track tiny stellar movements, known as proper motion, helping to identify which stars are part of Terzan 5 versus those belonging to the Milky Way’s bulge.

By integrating findings from both Webb and Hubble, researchers found compelling evidence for two additional stellar populations, one dating back 3.8 billion years and another 2.5 billion years old.

They also determined the ages of the known stellar populations with remarkable precision, revealing formation timelines between 12.5 billion and 4.7 billion years ago.

The existence of these four distinct generations of stars suggests that Terzan 5 likely interacted with another celestial object, potentially a globular cluster or giant molecular cloud, enriching it with gas and dust to spark a second round of star formation.

Observations made using the W.M. Keck Observatory and ESO’s Very Large Telescope indicate that Terzan 5 hosts a unique stellar population.

Dr. R. Michael Rich, an astronomer at UCLA, noted, “As these populations age, the clusters preserve a fossil record of progressive heavy element enrichment from supernovae.”

Terzan 5 has managed to retain essential raw materials, allowing for the formation of multiple star generations.

There is substantial evidence that Terzan 5 witnessed a powerful supernova explosion that produced heavier elements, which were subsequently dispersed amongst the following generations of stars.

In less massive systems, the explosive force could have expelled residual gases and dust, thereby releasing the resultant elements.

Terzan 5’s progenitor possessed enough mass to sustain ejection, enabling new star generations to take shape over billions of years.

The results indicate that Terzan 5 likely remains from a significantly larger star system that formed around 12.5 billion years ago.

This cluster is remarkable in its survival without merging or fully blending with the Milky Way’s bulge.

Professor Francesco Ferraro from the University of Bologna explains, “For some reason, this extraordinary cluster formed separately from the bulge and was not obliterated during the bulge’s formation.”

“Terzan 5 is considered a bulge fossil fragment, resembling the primordial mass that contributed to bulge formation.”

For further details, consult this study published in Astronomy and Astrophysics.

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G. Zullo et al. 2026. Terzan 5’s multi-age stellar population revealed by JWST. A&A 709, A212; doi: 10.1051/0004-6361/202659349

Source: www.sci.news

Discovering an Early Prototype of Stonehenge: The Secrets of an Ancient Monument

Reenactment of Summer Solstice Celebrations in Bulford

Marijane Porter, Wessex Archaeology

Ancient Stone Age societies in Britain constructed wooden monuments to mark the summer solstice approximately 500 years before the iconic stone circles at Stonehenge were established.

Stonehenge also aligns with the summer solstice, hinting that the wooden structures may have inspired its creation. This discovery represents one of the earliest manifestations of monuments dedicated to celestial events in Britain.

“What we have now is substantial evidence that these communities were able to track the sun’s movement,” stated Phil Harding from Wessex Archaeology, who led the excavation project during a press conference unveiling the findings.

Stonehenge, completed at the end of the Stone Age, during the Neolithic era, is situated on Salisbury Plain, England. It encompasses an outer ring of vertical sarsen stones topped with horizontal lintels, alongside a smaller inner circle of vertical bluestone and additional stones. This oldest section dates back to around 3100 BC, with further constructions extending until 1600 BC.

Notably, certain standing stones appear meticulously positioned to align with the summer solstice sunrise and the opposite sight for the winter solstice sunset, with construction of these associated stones occurring around 2500 BC.

Harding and his team unearthed the remnants of a 500-year-old monument near Bulford, roughly five kilometers northeast of Stonehenge, in a location initially designated for a military base housing 5,000 soldiers. Prior to construction, Wessex Archaeology carried out excavations from 2015 to 2017.

The research team identified several pits containing fluted pottery created by late Neolithic cultures. Radiocarbon dating suggests the pottery dates back to around 2950 BC, with 40 samples clustered closely in time. “This site was occupied for a relatively brief period,” Harding explained, estimating an occupancy span of about a decade.

Acknowledging its significance, Susan Greaney from the University of Exeter, who was not involved in the study, remarked, “This is a crucial Middle Neolithic settlement.”

Pottery Unearthed in Bulford, England

Wessex Archaeology

Two pits found at Bulford displayed distinct shapes: tapering sides that transitioned from 1.2 meters wide to just 0.5 meters, lacking pottery but filled with chalk rubble. Harding concluded these were postholes that once supported upright timbers, with one containing rowan charcoal.

Positioned approximately 120 meters apart, the postholes’ alignment directed towards the northeast, roughly 48.1 degrees—a significant angle for summer solstice sunrises. Harding expressed his enthusiasm, remarking, “I was genuinely thrilled.”

Wessex Archaeology enlisted Fabio Silva, a skyscape archaeologist with Stone x Sky, to analyze the posthole arrangements further. Through a 3D landscape reconstruction, Silva concluded that the alignment of the postholes correlated effectively with ancient midsummer sunrises, allowing for a discrepancy of just about one degree.

Silva noted, “This slight variation makes sense considering the potential diameter of wooden pillars, which could have reached 50 centimeters. Accounting for this width, the alignment remains impressive.” He stated, “The chance of this being coincidental is less than 0.5 percent.”

“A rough orientation might suffice for the rituals conducted at such sites,” suggested A. Cesar González Garcia from Spain’s National Research Council, highlighting the community’s long-standing interest in cosmological phenomena.

Evidently, ancient ruins in the vicinity provide indications that early societies tracked the sun, albeit with varying precision. As Matt Leivers of Wessex Archaeology affirmed, “Since the dawn of Neolithic communities, the sun has consistently influenced their ceremonial structures.”

Greaney reiterated that numerous wooden monuments were similarly oriented, with the Bulford site contributing to the narrative of early monumental architecture. For instance, nearby Larkhill features a Neolithic enclosure from approximately 3700 BC, predating Bulford and Stonehenge. Its entrance faces northeast, allowing for full sunrise visibility over Sidbury Hill on midsummer mornings, as noted by Leavens.

Topic:

Source: www.newscientist.com

Discovering a New Duck-Billed Dinosaur Species Unearthed in Romania

A collaborative effort by an international team of Romanian, Hungarian, and Italian paleontologists has led to the identification of a new genus and species of herbivorous duck-billed dinosaur, discovered from an incomplete skeleton in the Hersheg Basin, located in the Carpathian Mountains of present-day Romania.



Cryptohadros Kallaiae. Image credit: Tibor Pecsics.

Cryptohadros Kallaiae inhabited our planet during the Maastrichtian period of the Late Cretaceous, approximately 70 million years ago.

This dinosaur belongs to the Hadrosauridae family, which includes iconic duck-billed dinosaurs and their relatives.

The holotype specimen of this species was uncovered in continental deposits at the vertebrate site of Fantanelle-3, near the village of Valioara, within the Denshu-Siura Formation in Romania.

This region is renowned among paleontologists for its unique and rare dinosaur fossils.

“Complete skeletons, including cranial elements, vertebrae, and limb bones, are incredibly rare in the Haseg Basin, particularly for hadrosaur fossils,” stated paleontologist Dr. Attila Sisi from ELTE Eötvös Lorand University.

“Most sites yield only isolated bone elements, often mistakenly attributed to known dinosaur groups, despite lacking definitive features.

The skeleton of Cryptohadros Kallaiae is a partial specimen comprising the skull, rib fragments, caudal vertebrae, and parts of the hind limbs.”

Nevertheless, this fragmentary material was sufficient to distinguish the new species from other known dinosaurs, particularly from Thelmatosaurus transsylvanicus, a duck-billed dinosaur that has been misidentified for over a century.

This discovery suggests that at least two closely related duck-billed dinosaurs coexisted in the region during the Late Cretaceous.

“The morphological similarities with Thelmatosaurus are significant, indicating a close relationship,” remarked János Magyar, a PhD student at ELTE Eötvös Lorand University and the Hungarian Museum of Natural History.

“The differences largely pertain to the morphology of the skull elements.”

The researchers classified Cryptohadros Kallaiae, Thelmatosaurus transsylvanicus, and Tethyshadros from Italy as part of a newly recognized evolutionary group known as Telmatosauridae, a distinct lineage that evolved in southeastern Europe’s island environments.

“Our phylogenetic analysis reveals close relationships among all known Late Cretaceous hadrosaurids in southeastern Europe, including Thelmatosaurus, Tethyshadros, and Cryptohadros,” the researchers concluded.

“Furthermore, this analysis identifies several distinct evolutionary lineages of hadrosaurids within the European archipelago during the Late Cretaceous, suggesting multiple dispersal events between Asia and Europe during this period.”

The findings on Cryptohadros Kallaiae are detailed in a study published in the Journal of Systematic Paleontology.

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Janos Magyar et al. 2026. A new early Maastrichtian “duck-billed” dinosaur from the Haseg Basin (Densus-Siura Formation, Romania) documents a unique clade of non-hadrosaurid hadrosaurids from the southeastern Late Cretaceous European archipelago. Journal of Systematic Paleontology 24(1); doi: 10.1080/14772019.2025.2607800

Source: www.sci.news

Discovering the Hidden Truth: Amazon’s Short-Eared Dog More Common Than Previously Believed

Discover the short-eared dog (Aterocynus microtis): A rare canid thriving in Bolivia and Peru. This elusive species, often referred to as the world’s least-known canid, flourishes in the pristine high-altitude forests of Latin America. Learn more in the official research article.

According to Dr. Robert Wallace and his colleagues at the Wildlife Conservation Society, “The short-eared dog, also known as the ghost dog, is likely the least understood medium-to-large mammal in the neotropics, and its habitat distribution remains largely unknown.”

Recent analyses reveal that short-eared dogs are forest specialists. Studies in southern Peru indicate they prefer terra firma, or highland forests, far from rivers.

Previously, Bolivia recorded only six localities, four museum specimens, and two field sightings by trained biologists. However, extensive efforts to document mammal distribution have uncovered more habitats for this fascinating species.

Between 2001 and 2024, researchers conducted 34 camera trap surveys in the Greater Madidi Tambopata landscape and the Llanos de Moxos biocultural landscape, resulting in 4,635 photographs depicting 594 independent short-eared dog events across 21 of 34 camera trap surveys.

Dr. Wallace stated, “This research demonstrates the power of modern conservation techniques like camera trapping, providing valuable insights into one of the Amazon rainforest’s least-known species.”

Camera traps have unveiled the distinct features of the short-eared dog: a dark, dense coat ranging from blackish-gray to reddish-brown, a prominent head with tiny rounded ears, short legs, and a bushy tail. Remarkably, they possess partially webbed feet, a trait unique among Amazonian canids.

Despite their mythic reputation, new findings suggest that short-eared dogs are more common than previously believed, with capture rates estimating around 15 individuals per 100 square kilometers.

Active primarily during daylight hours, with peak activity between 6 a.m. and 12 p.m., short-eared dogs are true forest specialists, thriving in untouched highland forests, which explains their elusive nature.

Given their dependence on intact forest ecosystems, the conservation of short-eared dogs hinges on the establishment and effective management of protected areas. Researchers found that their relative abundance was significantly higher in protected areas and indigenous territories compared to unprotected zones.

According to the authors, “The most critical management strategy is to safeguard the Amazon forest canopy through the creation and effective management of protected regions, paired with sustainable practices in indigenous lands.” This knowledge illustrates how short-eared dogs are quietly flourishing in the dense forests of Bolivia and Peru, emphasizing the urgent need for habitat protection.

This important study was published in Neotropical Biology and Conservation on March 27, 2026.

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RB Wallace et al. 2026. Delivering Insights: Short-Eared Dog (Aterocynus microtis) Distribution and Ecology in Bolivia. Neotropical Biology and Conservation 21 (1): 49-66; doi: 10.3897/neotropical.21.e183324

Source: www.sci.news

Discovering the Secrets: How the Pyramids Were Built Revealed

The remarkable ability of ancient Egyptians to construct the Great Pyramid of Giza, without modern machinery, has fascinated and puzzled scholars for decades.

Recent insights from researcher Vicente Luis Rosell Roig suggest a resolution to this long-standing mystery. He provides mathematical evidence to support his claims: Nature. Roig proposes that an innovative system of spiral, uneven ramps was utilized to transport the massive stones used in the construction.

As Egypt’s largest pyramid, the Great Pyramid of Giza was erected around 2560 BC as a tomb for Pharaoh Khufu. This monumental structure comprises approximately 2.3 million stone blocks, each weighing between 2.5 to 15 tons.










For the pyramid to be completed within Khufu’s 27-year reign, a stone block would need to be placed every three minutes on average. However, debates continue over how this colossal structure was achieved in such a short time.

Some theories propose the use of external lamps, although such ramps would require significant materials, with no substantial archaeological evidence to support these claims.

Alternatively, another theory posits that a single ramp may have been built into the pyramid, spiraling upwards and filled from the top down as construction progressed.

However, Roig’s mathematical modeling suggests that using a single ramp would extend the construction time to nearly 50 years.

Instead, he argues for the use of four concave ramps spiraling around the pyramid simultaneously, each starting from distinct points near the base. His computer-generated model indicates that this method could align with the 27-year completion timeframe.

4-lamp parallel IER configuration (3D rendering). Image credit: npj Heritage Science (npj Herit. Sci.)

“This is a fascinating explanation regarding the structure of the pyramids,” remarked Dr. Roland Enmarch, a reader in Egyptology at the University of Liverpool. “Further verification with more evidence and scans of the structural anomalies at the corners where the ramp direction would have suddenly changed is necessary.”

“Nevertheless, it appears quite plausible. The Great Pyramid of Giza is neither the oldest nor the last pyramid, which may also provide insights into the construction of other pyramids.”

Read more:

Source: www.sciencefocus.com

Discovering Europe’s Half-Ton Cow Ancestors: Four Million Years Ago

A nearly complete bovine skeleton discovered at the early Pliocene site of Camp dels Ninotz in northeastern Spain has unveiled that the ancestors of modern buffaloes and cows had reached impressive sizes long before humans inhabited the continent.



Paleo-artistic reconstruction of the early Pliocene environment around Lake Camp Dels Ninotz. Image credit: Mauricio Anton.

“Cows play a vital role in many contemporary ecosystems and human agriculture, particularly species within the Bovini tribe, such as bison, buffalo, and cattle,” stated Dr. Leonardo Solberg from the Leibniz Institute for Evolutionary and Biodiversity Sciences and his colleagues.

“However, due to the scarcity of well-preserved early fossils, their evolutionary origins and relationships with close relatives remain largely unknown.”

The study involved the examination of at least 14 human remains excavated from the Camp dels Ninotz site in Spain.

Researchers identified the specimen as Parabos tineresi, one of five buffalo-like species that thrived in Europe during the early Pliocene.

The largest of these animals is estimated to have weighed nearly 500 kg, making it smaller than most existing bovine species but larger than other similar bovid species of the period.

This indicates an early stage of body size increase in the bovine lineage, possibly as an adaptation to the changing climate and environment that characterized continental Europe during the Pliocene.

Their anatomy suggests a preference for moist, plant-rich environments, aligning with researchers’ understanding of the water-abundant ecosystem at the Camp dels Ninotz site.

Researchers argue that the early Pliocene marked the dawn of large cattle, but the exact evolutionary connection between cattle and cows remains unclear. The status of Parabos also remains ambiguous.

Comparative studies suggest that Parabos could either represent early members of the Bovini tribe or more modern relatives of the related Tragoportacini lineage, which was eventually supplanted by true water buffalo, cattle, and bison.

Future research focusing on the anatomy and ecology of Parabos will clarify their place in the bovine evolutionary narrative.

“The Camp dels Ninotz bovid is one of the most exquisite fossils from the European Pliocene,” remarked the researchers.

“The exceptional preservation of these specimens allows for a deeper understanding of their anatomy and, consequently, the ecology of the continent’s earliest large bovids.”

“Studying these fossils presented both challenges and rewards.”

“The extraordinary preservation and richness of the findings have provided us an unprecedented wealth of data for this ancient geological period, offering a new perspective on the world before humans.”

The study has been published in the journal PLoS ONE.

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L. Solberg et al. 2026. First or last dynasty? Parabos tineresi and the evolution of Eurasian bovidae during the early Pliocene. PLoS ONE 21 (6): e0340256; doi: 10.1371/journal.pone.0340256

Source: www.sci.news

Ötzi’s Frozen Remains: Discovering Metabolically Active Microorganisms in Ancient Ice

Ötzi’s Preservation Conditions

South Tyrol Archaeological Museum/Eurac Research/Marion Lafogler

Recent research suggests that some microorganisms in the 5,300-year-old remains of Ötzi the Iceman may be metabolically active, despite his long-term ice preservation.

Ötzi’s mummified remains were discovered in 1991, as they melted from a glacier in the Alps near the Austria-Italy border. He is estimated to have lived between 3350 and 3120 BC. Over the last 35 years, studies of his remains revealed significant insights, including his probable dark complexion and baldness, and the fact that he had numerous tattoos. An arrow wound in his shoulder indicates he was murdered.

Ötzi is currently housed at the South Tyrol Archaeological Museum in Bolzano, Italy, under conditions that replicate those of his original icy environment: -6°C (21°F) with 99% relative humidity.

Researchers, including Frank Meixner from the Eulac Institute Mummy Research Institute, analyzed skin swabs, tissue fragments, and thawed water samples from Ötzi, collected in 1992, 2010, and 2019. They compared these to soil and ice samples from the discovery site in the 1990s.

Both ancient and modern microorganisms have been identified in Ötzi, with some possibly remaining metabolically active. “We can differentiate between Ötzi’s endogenous gut bacteria and those that entered his body from the environment after death,” Meixner explains.

Metagenomic analysis of internal tissues conducted by the research team has revealed specialized bacteria that thrive in mammalian intestines without oxygen, such as Treponema and Kineotrix. The extent of DNA damage in these bacteria suggests they were living in Ötzi’s body during his lifetime.

The diverse range of microbes found in Ötzi’s gut may reflect the varied diets of Chalcolithic humans, contrasting with those of modern Western societies, according to Meixner.

Additionally, the samples contained bacteria from the Pseudomonas genus, commonly found in soil and water. The DNA damage observed indicates these bacteria likely belong to an ancient microbial community at the discovery site.

The research team identified cold-tolerant or psychrophilic yeasts in Ötzi’s external samples: Phenoripheria, Graciojima, Gofojima, and Murakia.

Analysis indicated that these yeasts are also ancient microorganisms. Notably, the presence of Graciojima increased from 2010 to 2019, suggesting it may be metabolically active or capable of reproduction under current storage conditions.

Reconstructed Image of Ötzi

South Tyrol Archaeological Museum/Augustin Ochsenreiter

“This is compelling evidence that Graciojima has colonized the mummy post-mortem,” states Nikolai Oskolkov, although he’d like additional data points to ensure results are not influenced by experimental conditions.

The increasing prevalence of yeast is intriguing, as noted by Damra Kaptan from the University of Stavanger, Norway. “Determining if it’s active will require us to check for RNA produced from the yeast DNA,” she elaborates. “It’s possible the yeast was dormant or partially activated during thawing.”

Some yeasts possess enzymes capable of breaking down proteins and collagen, which could potentially harm the mummies; however, researchers found no evidence of such damage.

The research team also identified microorganisms containing genes that can degrade the toxic compound phenol. Professor Meixner suggests this may be linked to treatments applied to the mummy in the 1990s aimed at controlling mold growth. “When Ötzi was discovered, there was already active mold, and he was treated with phenol,” he explains. “This could have strengthened the microbiome.”

Overall, the study indicates that Ötzi is not merely a biological time capsule, but rather a complex ecosystem formed from the inheritance of his gut microbes, the glacial environment, and over 30 years of preservation. “Given these microbes have been associated with the mummy from the start, should we consider them as part of his biological makeup?” questions Meixner.

He recommends ongoing genomic monitoring, including checks for activity signs like RNA and metabolites, to determine if the microbial community is awakening and affecting Ötzi’s tissue. If this occurs, scientists may need to reassess storage conditions to mitigate microbial activity.

Topic:

Source: www.newscientist.com

Discovering a Meteorite in Africa: Evidence of a Lost Giant Protoplanet Unveiled

Discover the fascinating North West Africa (NWA) 12774, an Angrite meteorite found in the Sahara Desert of Mauritania. This rare fragment offers compelling evidence that large planetary bodies were formed and subsequently destroyed during the chaotic early years of our solar system.



Artist’s impression of the protoplanetary disk surrounding HD 107146. Image credit: A. Angelich / NRAO / AUI / NSF.

“It’s hard to believe that the world was once this vast,” remarked Dr. Aaron Bell, the lead author of the study.

“We know it exists because some of its fragments have landed on Earth.”

“These meteorites contain evidence of a distinct evolutionary path for early planet formation.”

In their research, Bell and colleagues studied a sample of the NWA 12774 Angrite meteorite.

“Angrites are among the oldest known volcanic rocks in the solar system, having formed within a few million years of the solar system’s inception around 4.56 billion years ago,” the researchers explained.

“They are also extremely rare; of the more than 80,000 meteorites discovered on Earth, only 68 are classified as angrite.”

“What makes angrites particularly intriguing is their unique chemistry. Unlike Earth, Mars, and other rocky planets, angrites contain very little silicon dioxide or silica, which are major components of virtually all known terrestrial planets.”

“Therefore, scientists previously believed that angrites originated from small asteroids, planets with a radius of less than 200 km (124 miles).”

However, researchers found that NWA 12774 includes clinopyroxene, a mineral typically encountered in Earth’s crust and mantle.

This clinopyroxene is notably rich in aluminum, suggesting that the rock formed under immense pressure deep within its parent body.

Scientists reconstructed the conditions necessary for NWA 12774 to form.



X-ray image of NWA 12774. Image credit: Aaron Bell / CU Boulder.

Surprisingly, the aluminum-rich clinopyroxene requires pressures of at least 17.5 kbar, which is significantly higher than the crushing pressure at the bottom of the Mariana Trench (around 1 kilobar).

This level of pressure wouldn’t be feasible within a small asteroid.

Calculations indicate that the progenitor of the Angrite must have had a radius of at least 1,000 km (621 miles).

Additional clues about the meteorite suggest even more astonishing possibilities.

The crystals in NWA 12774 retain sharp edges and distinct chemical patterns, which would have been erased if formed deep underground.

This implies that the crystals likely originated at a relatively shallow depth in a much larger parent body.

In this case, the original planet could have a radius greater than 1,800 km (1,118 miles), making it comparable in size to Earth’s moon or approaching a Mars-sized body with a radius of 3,300 km (2,050 miles).

“We have numerous understudied meteorites still in storage, indicating there may be more protoplanets yet to be discovered,” says Bell.

“It remains uncertain what led to the demise of the protoplanet. One possibility is a catastrophic event in the early solar system that shattered it, with its fragments providing materials for the formation of other terrestrial planets, including Earth.”

“The materials forming the matrix of angrites differ fundamentally from those of Earth and Mars.”

“This divergence indicates distinct evolutionary pathways in the formation of planets during the early solar system,” Dr. Bell concluded.

For more insights, check out the study published online on April 10 in the journal Earth and Planetary Science Letters.

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Aaron S. Bell et al. 2026. High-pressure clinopyroxene from Northwest Africa 12774 and new global pressure evidence for an angritic parent body the size of a planetary embryo. Earth and Planetary Science Letters 685: 120029; doi: 10.1016/j.epsl.2026.120029

Source: www.sci.news

Discovering Toothless Bipedal Crocodile Relatives from 212 Million Years Ago in New Mexico

Paleontologists have unveiled a groundbreaking discovery: a new bipedal shubosaur archosaur, Rubble Jascus Expetatus, found in New Mexico. This finding enriches our understanding of the diverse prehistoric creatures that inhabited North America over 200 million years ago during the Triassic period.



Rubble Jascus Expetatus traversed its prehistoric environment on two legs, equipped with tiny arms and a beak-like structure devoid of teeth. Image credit: Jorge Gonzalez / NHMLAC Dinosaur Institute.

Rubble Jascus Expetatus belongs to the newly classified Shubosauridae family, which consists of ancient crocodilian relatives resembling bipedal theropod dinosaurs.

“Shubosauridae represents a unique group of Triassic poposauriforms found in western North America and Argentina,” explained Dr. Alan Turner of Stony Brook University and his team.

“These agile, bipedal, toothless creatures demonstrate a remarkable convergence with the ornithomimid theropod dinosaurs that thrived in the Cretaceous period.”

Currently, three recognized species of shubosaurs include Shubosaurus inexpectatus from the Cooper Canyon Formation in Texas, Ephigia ochiferae from the Coelophysis Quarry at the Chinle Formation in northern New Mexico, and Syrossuchus longiservicus found in the Lower Ischigualasto Formation of western Argentina.

Rubble Jascus Expetatus effectively bridges the fossil timeline between Shubosaurus inexpectatus and Ephigia ochiferae.

This fossil, estimated at around 212 million years old, was excavated from the Hayden Quarry in the Chinle Formation fossil forest of northern New Mexico, USA, yielding significant partial skeletons and other fossilized remains.

Paleontologists note that Rubble Jascus Expetatus exhibits minimal differences compared to its relatives, reinforcing a trend of remarkable skeletal conservatism within the Shubosauridae family.

“The anatomical similarities between the skeletal remains of these species suggest that this morphological consistency has persisted within the Shubosauridae of western North America for at least 10 million years,” the researchers stated.

Rubble Jascus Expetatus aligns well with the hypothesis of morphological conservatism and fits within the known stratigraphic range of North American shubosaurs.”

This discovery further supports the hypothesis that shubosaurs were primarily endemic to western North America, suggesting a unique pattern distinguishing them from many other rare Triassic reptile groups.

“Our phylogenetic analysis positions this shubosaur within the same clade as two other North American shubosaurs, reinforcing the concept of an endemic group of small, bipedal, toothless forms in the southwestern United States,” the researchers concluded.

The findings are detailed in a paper published in the May 26th edition of the Journal of Vertebrate Paleontology.

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Alan H. Turner et al. New Shubosaurid (Archosaur, Poposauridae) unearthed from the Late Triassic (Norian) Hayden Quarry in New Mexico, USA Journal of Vertebrate Paleontology, Published online on May 26, 2026. doi: 10.1080/02724634.2026.2618182

Source: www.sci.news

Discovering Dental History: The First Known Dentist Was a Neanderthal

Neanderthal dentistry may have been remarkably advanced, according to a recent study led by scientists from the Russian Academy of Sciences in St. Petersburg.

This study examined a 59,000-year-old molar tooth discovered in Chagyrskaya Cave, Russia, featuring a deep central hole.

Archaeologists believe that the tooth was intentionally punctured with a sharp tool to treat an infection and alleviate pain.

This represents the oldest known dental evidence, dating back over 40,000 years and surpassing previous findings from about 14,000 years ago in Italy, which were previously considered the first examples of dental treatment by Homo sapiens.

“What surprised me was that the owner of this tooth understood exactly what was causing the pain and intuitively knew it could be alleviated,” remarked the first author, Dr. Aliza Zubova from the Peter the Great Museum of Anthropology and Ethnology, Russian Academy of Sciences.

“Neither Neanderthals nor even later modern humans have encountered anything like this before.”










To investigate the treatment of this tooth, archaeologists utilized a method known as microtomography to capture highly detailed X-rays. This analysis revealed microscopic grooves on the tooth’s surface.

Researchers performed experiments on modern human teeth, attempting to replicate similar holes and markings using techniques accessible to Neanderthals.

Neanderthal tooth labeled Chagyrskaya 64, photographed from five angles – Image credit: Zubova et al., 2026, PLOS One, CC-BY 4.0

Senior author Dr. Kseniya Korobova from the Siberian branch of the Russian Academy stated that these experiments showcased the technical proficiency of the procedures, involving the removal of carious tissue via deep holes in the tooth.

“It’s important to remember that we couldn’t fully replicate the real-life conditions,” she noted. “The inflammation and swelling in the oral cavity would have introduced additional challenges during the procedure.”

She emphasized that the mouth is a “complex area to work,” necessitating “manual dexterity, patience, and a caregiver to keep the head still.”

Remarkably, all of this was achieved without anesthesia. Thus, while the patient likely experienced pain, archaeologists believe the method effectively alleviated tooth discomfort.

Second author Dr. Lydia Zotkina remarked, “What astonishes me is the incredible willpower this Neanderthal must have possessed.”

“This finding is a striking illustration of how archaeological evidence allows us to gain insights into past lives, revealing the strength and resilience of these individuals. Every visit to the dentist now reminds me of that Neanderthal.”

For Zubova, this research contributes to a growing body of evidence indicating that Neanderthals provided care for one another regularly.

“Historically, Neanderthals have been viewed as more primitive than modern humans, making their care for Middle Paleolithic community members an exception,” she explains.

“As evidence accumulates, it increasingly suggests that Neanderthals cared for the sick and infirm just like modern humans.”

Read more:

Source: www.sciencefocus.com

Discovering Humanity’s First Tools: The Evolution of Simple Containers

Oil lamp discovered in Lascaux cave, France

Oil Lamp Discovered in Lascaux Cave, France

Sémhur CC BY-SA 4.0

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In the iconic opening of 2001: A Space Odyssey, the first tool is presented as a club, used not only for hunting prey but also in the dramatic leap through time. This perspective suggests that the earliest tools served primarily as weapons.

This interpretation also extends to early stone tools. Round stones were employed for striking, while sharper stones were utilized for cutting and penetrating. We envision these primitive implements used for breaking, hunting, and lethal purposes.

Yet, early humans likely employed various tools crafted from other materials, particularly plant-based materials like wood, which, unfortunately, are less likely to be preserved. The Stone Age may well have also been the Vegetative Age (refer to Sophie Verdugo’s insightful 2024 article).

This opens up intriguing possibilities, particularly regarding the concept of containers. Imagine if the first tool was an object capable of carrying or storing valuable items.

As paleoanthropologist Mark Kissel from Appalachian State University notes, “Containers resolve a multitude of challenges,” emphasizing their critical role in early human existence. His team has developed an extensive database of prehistoric containers, encompassing hundreds of examples spanning over 100,000 years, though this likely represents only a small fraction of what once existed. “Containers were essential for humanity’s success,” Kissel asserts.

Exploring Prehistoric Containers

Compiling a comprehensive database of ancient containers is a daunting task. Kissel and his colleagues dedicated over a year to scouring scientific literature for examples, using a broad range of terminology to identify various types of containers, faced with the realization that they had to cease their efforts and recently published their findings in a study in the Journal of Human Archaeology on April 8th.

Determining what qualifies as a container posed another challenge. They opted for a wide definition: “Any object that functions as a container (holding contents and acting as a barrier) and can be transported by humans.”

This broader definition includes items not conventionally viewed as containers, such as spoons, which can also transport materials. Notably, examples of early lamps comprise small rock slabs with hollows to hold and burn animal fat. A renowned specimen from the Lascaux Caves in France is carved from red sandstone and features a handle.

Other containers might include hollow bones; for instance, tubes crafted from swan wing bones may have been utilized for needle transport. Similarly, robust ostrich eggs were likely employed in Africa for carrying water on lengthy journeys. Rock art raises further possibilities, depicting vessels and net-like objects found in Gennersdorf, Germany.

Fragment of Engraved Ostrich Eggshell Container from South Africa

Texier et al. 2013

The research team ultimately cataloged 793 mobile containers, exploring examples from the Pleistocene epoch, which spans 2.58 million years to 11,700 years ago; however, all findings seem to date back no further than 500,000 years.

Conventionally, archaeologists believed containers emerged in the last 10,000 years, closely tied to the agricultural revolution and the advent of pottery, attributed to the rise of agrarian societies that needed to store surplus food. Hunter-gatherer societies were thought to lack such surplus and mobility would render pots easily breakable.

However, Kissel argues this notion has largely been overturned, suggesting a more gradual and fragmented transition from prehistory to the Neolithic era. Evidence indicates that some indigenous Australian groups crafted pottery over 2,000 years ago; simultaneously, early gatherers in the Amazon, dating back 10,000 years, left pottery shards behind, with signs of ceramic production in China as early as 18,000 years ago.

This evolution implies a gradual development of containers over time. Kissel maintains, “It’s beneficial to observe containers along a spectrum.”

While container origins reach deep into our past, it’s worth noting that non-human primates like great apes do not utilize them; instead, they might use leaves as sponges to draw water. Kissel suggests this fundamental difference speaks volumes about human evolution.

The oldest container identified in their database is a bark tray or dish, unearthed at Kalambo Falls in Zambia, estimated to be between 400,000 to 500,000 years old. Kalambo Falls has showcased remarkably preserved wooden artifacts, including a structure potentially dating back 476,000 years. However, dating for the bark tray remains inconclusive.

This reveals a significant challenge Kissel’s team faced: numerous artifacts were excavated long ago, resulting in vital information obscured in outdated texts, often inaccessible online. The Kalambo Falls tray was excavated in the 1950s by archaeologist John Desmond Clarke, with minimal records available today.

Despite observable trends within the dataset, Kissel emphasizes they primarily reflect the archaeological record’s limitations rather than definitive prehistoric facts. Astonishingly, 87.8 percent of the identified containers were discovered in Europe, a statistic Kissel attributes to the extensive archaeological endeavors in that region rather than implying that Europe was the cradle for container innovation. Interestingly, the dataset’s oldest containers hail from Africa.

Furthermore, only two vessels in their records exceed 100,000 years old; nevertheless, Kissel posits that hominins likely employed containers far earlier than documented. Such artifacts may be undiscovered or have undergone degradation.

As Kissel puts it, a clearer understanding of how integral containers have been to human existence is emerging. In Europe, where archaeological research is robust, many examples persist despite conservation issues, indicating their necessity for human survival.

The Role of Containers in Human Evolution

One of Humanity’s Oldest Tools Remains in Use

Ron Giling/Alamy

Kissel theorizes that one of the initial applications of containers might have been for carrying infants in slings. Many anthropologists—especially women—have championed this concept for decades.

Great apes like chimpanzees typically carry their infants clinging to their bodies. However, as humans evolved with less body hair and an increased reliance on bipedal locomotion, baby carriers would have become essential for carrying helpless newborns. Millions of years ago, Australopithecus likely utilized slings, implying that even Lucy, a representative of Australopithecus afarensis, may have carried an infant snugly.

While these concepts are not groundbreaking, their prominence is gradually increasing, largely due to their early association with feminist interpretations of prehistory, which faced skepticism.

In 1976, anthropologists Nancy Tanner and Adrian Zillman posited that the earliest tools may have been baskets, utilized primarily by women for carrying food. Their work challenged the misconception of prehistoric male dominance, introducing a more nuanced portrait that included women’s contributions.

Feminist journalist Elizabeth Fisher echoed similar themes in her 1979 book, Creation of Woman: Evolution of Sexuality and Formation of Society, where she argued that the earliest cultural inventions likely included containers for gathered products.

Mystery writer Ursula Le Guin influenced the narrative surrounding containers with her Carrier-Bag Theory of Fiction, emphasizing that without a vessel, food remains unattainable, and even the simplest container allows for preservation during adverse conditions.

Le Guin advocated for a reassessment of historical narratives, advocating narratives of community, nurturing, and environmental stewardship alongside tales of conflict. She asserted the necessity of fostering alternate narratives to enrich our understanding of humanity’s journey.

As this exploration unfolds, it’s important to track the data. There’s increasing evidence that humanity’s distinctiveness lies not only in intelligence, creativity, or aggression but in our capabilities for empathy and social connection. When isolated from one another, human beings face a notably higher risk of extinction due to the lack of cooperative networks.

Our survival as a species hinges on collaboration and sharing, as exemplified by the way one might offer a piece of their food stores to a friend in need using a homemade container.

Topics:

  • Archaeology/
  • Ancient Humans

Source: www.newscientist.com

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

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

Shutterstock/Stephen Ray Chapman

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

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

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

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

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

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

Eternal Challenges in Mathematics

Founding members of the Bourbaki Group gathered in France in 1935

Charmet/Bridgeman Image Archive

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

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

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

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

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

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

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

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

Emerging Mathematical Challenges

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

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

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

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

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

Topic:

Source: www.newscientist.com

Discovering Distant Galaxies: A Guide to Planet Search – Sciworthy

In the realm of Star Wars, alien heroes confront villains wielding planet-destroying superweapons “a long time ago in a galaxy far, far away.” But what do scientists truly understand about alien planets in galaxies far beyond our own? These fascinating worlds are known as extragalactic exoplanets. Assuming the Milky Way galaxy is akin to other galaxies, it is predicted to harbor similar worlds. Yet, many galaxies remain distant, rendering modern exoplanet observation techniques inadequate for their detection.

Recently, astronomers studied a stream of over 700,000 stars potentially absorbed by the Milky Way from the Sagittarius Dwarf Galaxy. Given their remoteness, the team investigated if any of these stars hosted large exoplanets orbiting close to Earth, specifically hot Jupiters, which are generally easier to identify.

The researchers established three criteria for narrowing down their star selection. First, each star must be sufficiently bright as observed by a transiting exoplanet probe like TESS to ensure high accuracy in their data processing software. Second, each star should possess at least a 50% likelihood of originating from the Sagittarius Dwarf Galaxy, based on motion and position measurements from the Gaia mission. Finally, the radius of each star needed to be less than twice that of the Sun to simplify the search for planets around smaller stars. These criteria helped refine the list to approximately 20,000 candidate stars.

Subsequently, the team utilized a software package to analyze public TESS catalog data, specifically the Eleanor TESS-Gaia light curve, also known as TGLC. Using these tools, they plotted the brightness of each star over time on a graph termed the light curve. The astronomers searched for periodic brightness dips, indicating an exoplanet passing in front of the star. This process eliminated several thousand stars affected by optical interference, refining their sample size to just over 15,000 stars.

To detect hot Jupiters, the team looked for brightness dips occurring at intervals of 14 hours to 10 days, the typical orbital periods for these planets. They employed geometric calculations to derive the radius of each exoplanet based on the proportion of starlight obscured. Candidates with dips corresponding to objects with radii more than twice that of Jupiter were excluded, as these dips likely resulted from orbiting companion stars rather than true exoplanets.

Among the examined stars, the most promising candidate for a hot Jupiter was identified as TIC 92223525. The researchers estimated that it could host an exoplanet with a radius 1.76 times that of Jupiter and an orbital period of 7.2 days. However, closer inspection of the star’s light curve indicated contamination from a neighboring star, TIC 92223526. The periodic brightness variations from this companion star mimicked those of an exoplanet, leading to a false positive in the initial screening. Consequently, the research team had to dismiss this candidate, leaving no confirmed exoplanets from their study.

The researchers drew significant conclusions from their inability to identify hot Jupiters within the Sagittarius Dwarf star sample. They estimated that if more than 1% of these stars hosted hot Jupiters, detecting at least one in a sample of over 15,000 stars would have been very probable. This limits the occurrence rate of hot Jupiters to around 1%. If accurate, future exoplanet-hunting endeavors may necessitate exploring over 11,000 stars to discover one, with reasonable scientific uncertainty suggesting at least 80,000 stars may need to be examined.

While this survey of the Sagittarius Dwarf yielded no conclusive results, the research team encourages subsequent researchers to continue their exploration of the Sagittarius Dwarf and other star streams from different galaxies. Scientists have identified over 20 such streams within the Milky Way. Investigations into these stellar streams may lead to the discovery of the first extragalactic planets or offer insights into whether other galaxies produce fewer hot Jupiters than our own. Let’s hope none of them stumble upon an extragalactic Death Star!


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Discovering the Unusual Secrets of Uranus’ Rings: New Insights Revealed

Uranus viewed from the Hubble Space Telescope

Uranus as Observed by the Hubble Space Telescope

Credit: Erich Karkoschka, NASA and the University of Arizona

While the rings of Uranus may appear similar visually, their compositions reveal surprising differences. Understanding these rings is critical for uncovering the mysteries of Uranus’s unique and dynamic system.

The outer rings of Uranus, known as the Mu and New rings, are notably dark and challenging to observe given their vast distance. Researchers, including Imke de Pater from the University of California, Berkeley, utilized nearly 20 years of data from the Keck Telescope, Hubble Space Telescope, and James Webb Space Telescope to conduct a thorough analysis.

The team discovered that the outermost ring, Mulling, appears blue, suggesting it consists of minute ice grains. Conversely, the New ring takes on a reddish hue, rich in dust and complex organic molecules known as thorin.

The ice particles within Mulling likely originate from Uranus’s small moon, Mab, implying that Mab is composed of ice rather than rock, unlike other neighboring moons. However, the mechanism by which these tiny ice fragments escaped Mab to form the ring remains uncertain.

This scenario shares similarities with Saturn’s E ring, which is sustained by the icy moon Enceladus, known for its substantial water plumes. In contrast, Mab, which measures approximately 12 kilometers in diameter, is not expected to produce similar plumes.

“We don’t anticipate plumes on small moons like Mab, though the comparisons are intriguing,” says Tracy Becker, a researcher at the Southwest Research Institute in Texas who was not involved in the study. Instead, it is probable that micrometeorites have collided with Mab’s surface, propelling ice grains into space.

It is not surprising that the New ring is laden with dust, yet the rocky bodies responsible for this dust have yet to be identified, suggesting they are relatively small. The researchers also noted that the brightness of the New ring fluctuated over time—its brightness was halved between 2003 and 2006. This may indicate a significant collision event prior to 2003, causing a temporary increase in brightness.

The key question is not just why the two rings differ so significantly but why the objects that contribute to them exhibit such variance, despite orbiting similar regions around Uranus. “All rocky bodies might originate from a moon that fragmented, but Mab stands apart,” De Pater remarked. “This points back to the origins of the entire system and historical events.” Mab might be debris from a larger moon of Uranus, yet the factors that led to this process remain unclear.

“We are able to add two or three critical pieces to the puzzle that enrich our understanding of the Uranus system,” Becker emphasized. “This suggests that the puzzle is far more complex than we previously believed and that additional pieces are necessary for a complete understanding of the system.”

Topics:

Source: www.newscientist.com

Discovering a Unique Hyperdimensional State of Matter: Beyond 2D and 3D Dimensions

Graphene sheets are 2D, but some thin materials may not fit neatly into that category.

Alfred Pasieka/Science Photo Library

Researchers have identified a groundbreaking quantum state of matter that operates beyond traditional two- or three-dimensional characteristics, unveiling novel mechanics in electron movement.

Physicists categorize matter states by analyzing electron mobility within various materials, driven by factors like atomic structure and arrangement.

In a magnetic field, thin materials experience a distinct electron behavior; electrons trace a small circular path, funneling currents toward the material—a phenomenon known as the Hall effect. In magnetic substances, electron trajectories are more intricate, leading to diverse manifestations of this effect.

Wang Lei and his research team at Nanjing University have made an unexpected finding: they’ve discovered a new variant, termed the Transdimensional Anomalous Hall Effect (TDAHE).

While examining electrons in a thin material structured from carbon atoms arranged in a diamond-like pattern to create highly efficient electrical currents, they observed unusual electron behaviors upon magnetization.

“The TDAHE discovery was astonishing; it’s a phenomenon not previously documented in other materials nor predicted by existing theories,” Wang states. Measuring the raw data took nearly a year, indicating the complexity of this new effect.

The unexpected finding was that their material exhibited Hall effect characteristics under two mutually perpendicular magnetic fields. This discovery was significant because it demonstrated electrons performing loop motions both horizontally and vertically, despite the material’s minimal thickness.

Initially, Wang’s team suspected experimental errors, yet repeated tests verified their measurements. Additional samples yielded consistent results, leading to a groundbreaking conclusion: in carbon materials only 2 to 5 nanometers thick, the electrons were exhibiting unprecedented behaviors.

Due to the material’s ambiguous dimensionality, the researchers coined the term “hyperdimensional” to describe the new electronic states that do not adhere to the traditional 2D or 3D frameworks. “We aim to express that this finding introduces a novel regime beyond the well-explored dimensions,” explains Wang.

Andrea Young from the University of California, Santa Barbara, notes that this new state is distinctive because its mathematical portrayal of electron states lacks symmetry in three different aspects, setting it apart from analogous states. He emphasizes that the material’s thickness is secondary to its unique characteristics.

Young likens the newly identified state to a “quarter metal,” indicating that its asymmetry constrains electron behavior compared to conventional metals.

Wang’s team is now eager to delve further into hyperdimensional physics across various materials, utilizing advanced tools, including diamond-based magnetic field sensors, to explore this unprecedented state.

Topics:

Source: www.newscientist.com

Discovering the Uniqueness of Chemically Unique Stars: Insights from Cyworthy

Stars primarily consist of two elements: hydrogen and helium. These elements, along with lithium, were the only ones present during the Big Bang approximately 14 billion years ago. When the first stars exploded, they released their primordial elements along with heavier elements produced through
nuclear fusion.

In astronomy, all elements heavier than hydrogen and helium are referred to as
metals.
Chemists, however, use different terminology. Subsequent generations of stars, including our Sun, formed in clouds of gas and dust enriched with metals like carbon, oxygen, magnesium, and silicon. Scientists estimate that modern stars contain between 1% and 5% metals by mass.

While astronomers have found no solid evidence suggesting that stars significantly differ in metal content, some stars display unique chemical signatures. The light emitted by stars can be analyzed through their
spectrum,
revealing the presence of various elements. Each element emits a distinct light pattern, allowing astronomers to ascertain the abundance of each element, especially in a star’s outer layers. The prevailing theory suggests that chemically unique stars might not contain more metals than the average star; instead, the metals in their interiors are thought to be more distributed throughout their outer layers.

A research team from the
American Association of Variable Star Observers
at Masaryk University in the Czech Republic recently studied 85 chemically unique stars to better understand their behaviors and classifications. Their research relied on the
CP Star General Catalog published in 2009, focusing on categorizing these stars into four classes:
CP1,
CP2,
CP3, and
CP4.
CP1 stars exhibit strong spectral patterns of iron and other heavy elements, while CP2 stars show strong patterns of silicon, chromium, strontium, and europium. CP3 stars reveal patterns of mercury and manganese, and CP4 stars have either unusually weak or strong helium patterns.

The team compiled a list of 85 stars for observation, utilizing the BRIght Target Explorer (
BRITE
), a constellation that monitors brightness variations. The BRITE constellation consists of five satellites equipped with telescopes and cameras sensitive to red or blue light. Over several days, the team monitored each star.

Out of the observed stars, 74 exhibited variations in brightness, potentially due to fluctuating surface metal content creating dark spots that appeared and disappeared from our viewpoint as the stars rotated. Interestingly, six of these stars demonstrated brightness changes across multiple time periods—an unexpected result since rotation alone would typically not cause such variability. Comparisons with data from the Transiting Exoplanet Survey Satellite
TESS revealed that all six stars had been misclassified as chemically unusual.

The remaining 11 chemically unique stars displayed no apparent periodic brightness changes, suggesting they may be stationary. While the research team noted that some CP1 and CP3 stars do not rotate, they also found instances where CP2 and CP4 stars, which are expected to rotate, appeared stationary. They proposed two possible explanations for this phenomenon:
one is the potential misclassification of these stars, requiring a deeper analysis of their spectra, and the other is a slower rotation speed, exceeding 50 days, making them hard to differentiate from stationary stars.

The research team emphasized the need for astronomers to reconsider historical star classifications, particularly as technology advances and more space telescopes become available. This approach will enable future researchers to extract improved data from existing research archives and catalogs. Furthermore, they advocated combining long-term monitoring by small satellites with TESS data to refine classifications, unveil misclassified objects, and delve deeper into the structural and behavioral mechanisms of chemically unusual stars.


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Discovering Two Earth-Sized Planets in the TRAPPIST-1 System: A Distinct Divide Between Day and Night

Recent observations by the James Webb Space Telescope reveal startling climate details of two exoplanets, TRAPPIST-1b and TRAPPIST-1c, showcasing extreme daily temperatures and freezing nights, which may hinder their prospects for habitability.

An artist’s view of an exoplanet within the TRAPPIST-1 system, which is located 38.8 light-years from Earth. These planets, similar in size and temperature to Venus and Earth, showcase unique orbital dynamics. Image credit: M. Kornmesser / ESO.

Red dwarfs, which are smaller and cooler than our Sun, account for over 75% of the stars in the Milky Way galaxy.

Research indicates that Earth-sized planets are particularly abundant around these faint stars, raising intriguing questions about the potential for life on such distinctly different worlds.

TRAPPIST-1 is one such star system currently under scrutiny.

Discovered back in 2017, this fascinating system resides 38.8 light-years away in the constellation Aquarius.

It features seven transiting planets: TRAPPIST-1b, c, d, e, f, g, and h.

These planetary bodies are either comparable to or slightly smaller than Earth and Venus, and all possess notably short orbital periods.

“The TRAPPIST-1 system is a remarkable discovery: seven planets with Earth-like masses orbiting a single star,” stated Emmeline Bolmont, an astronomer at UNIGE.

“At least three of these planets lie within the star’s habitable zone, allowing for the presence of liquid water on their surfaces.”

“This system serves as an ideal environment for comparative planetology, helping us unravel the mysteries of planetary habitability and life development around red dwarfs.”

Dr. Bolmont and her research team utilized the NASA/ESA/CSA James Webb Space Telescope to study the two inner planets, TRAPPIST-1b and TRAPPIST-1c.

“Although red dwarfs and their planetary systems are commonplace, their environments don’t guarantee the potential for life,” the team noted.

“These stars emit intense ultraviolet radiation and high-energy particles that can erode planetary atmospheres, jeopardizing any existing life forms.”

“Furthermore, planets within a red dwarf’s habitable zone orbit very closely to the star, leading to a tidal lock effect that results in one side experiencing perpetual daylight while the other is in constant darkness.”

This illustration depicts the TRAPPIST-1 star and its planets reflected on its surface. Image credit: NASA / R. Hurt / T. Pyle.

By analyzing the light emitted from the star and the two planets, astronomers accurately determined the surface temperatures on both the day and night sides of TRAPPIST-1b and TRAPPIST-1c.

Daytime temperatures exceed 200 degrees Celsius for TRAPPIST-1b and nearly 100 degrees Celsius for TRAPPIST-1c, while at night, temperatures plummet below -200 degrees Celsius.

This extreme temperature disparity implies minimal energy transfer between the planet’s sides, indicating an absence of a significant atmosphere.

Even if these planets formed with atmospheres, harsh stellar conditions would likely have stripped them away entirely.

The team concluded that the lack of dense atmospheres on TRAPPIST-1b and c supports the theory that intense stellar radiation is crucial in shaping planetary evolution in such systems.

“TRAPPIST-1 acts as a vital reference point,” Dr. Bolmont mentioned. “Our theoretical models suggest that the outer planets may retain atmospheres, unlike the inner planets, similar to Mercury’s situation near our Sun.”

“We are eager to advance our exploration of the TRAPPIST-1 system in future studies.”

The findings were published on April 3rd in Nature Astronomy.

_____

M. Gillon et al. “No thick atmosphere around TRAPPIST-1 b and c from JWST thermal phase curve.” Nat Astron 3 April 2026. doi: 10.1038/s41550-026-02806-9

Source: www.sci.news

Discovering Hidden Fossils: Uncovering Secrets of Pre-Mass Extinction Oceans

Discoveries of Radiolarian Fossils in a Rock Sample

Provided by Jonathan Aitchison

A minuscule pellet of ancient rock, measuring only half the size of a rice grain, has unveiled 20 microscopic fossils from eight distinct species, including several previously unknown types. This significant discovery enhances our knowledge of the second-largest mass extinction known to science, while demonstrating how innovative analytical techniques can uncover neglected segments of the fossil record.

Jonathan Aitchison, a professor at the University of Queensland in Australia, was pivotal in extracting these pellets from rocks gathered in late 2018 from the Sichuan Basin in China, located approximately 300 kilometers south of Xi’an. These rocks date back 445 million years, situating them just prior to the late Ordovician mass extinction, ranked as the second most severe extinction event in the last half billion years.

The pellets contained eight species of radiolarians—single-celled plankton characterized by silica shells that continue to inhabit oceans today.

The discovered fossils encompass five genera, four families, and three orders, including a newly identified species named Haplotaniatum woufengensis.

The fossils are remarkably well-preserved, with both external and internal structures perfectly encased in asphalt, creating flawless impressions.

Patrick Smith, from the New South Wales Geological Survey in Sydney, Australia, remarked that the fossils were formed before the extinction event escalated.

“The quantity and diversity of fossils indicate that marine ecosystems, especially microscopic plankton communities, thrived just prior to the extinction,” Smith stated. “Ordovician oceans were significantly more biologically diverse than previously understood, especially on a microscopic scale. These fossils showcase a vibrant plankton community during a pivotal moment of environmental upheaval in Earth’s oceans.”

Traditionally, researchers have studied small fossils by using acid to dissolve surrounding rock, a process Aitchison notes is highly destructive.

In contrast, the study employed advanced X-ray technology (from the Australian Nuclear Science and Technology Organization’s synchrotron in Melbourne) to scan the rock pellets, yielding high-resolution 3D images of the contained fossils within seconds.

“Growing up, I was fascinated by ads for X-ray glasses that could see through objects,” Aitchison commented. “Now, I can ‘see’ these radiolarian plankton directly within the rocks without needing to remove them.”

“This represents the most significant technological advancement in my career,” he added.

Professor Aitchison concluded that the extensive life forms discovered in such a limited sample size imply that the marine biodiversity found in other Late Ordovician rocks might be “significantly underestimated.”

Smith emphasizes that a key takeaway from this study is that numerous fossils remain to be explored worldwide, “not due to a lack of specimens, but because our traditional methods are insufficient for detection and recovery.”

Topics:

Source: www.newscientist.com

Discovering New Forms of Matter Hidden in the Depths of Uranus and Neptune

Recent computational simulations indicate that icy giant planets like Uranus and Neptune may contain quasi-one-dimensional superionic carbon hydrides. This groundbreaking discovery could change how scientists perceive planetary interiors.



Diagram depicting hexagonal hydrocarbon compounds anticipated under conditions similar to those in Neptune. In this framework, carbon forms the outer helical chain (yellow), while hydrogen forms the inner helical chain (blue), aligning with the quasi-one-dimensional superionic behavior suggested by simulations. Image credit: Cong Liu.

Density measurements of Uranus and Neptune reveal that these colossal planets possess an unusual, hot, icy interlayer situated beneath an atmospheric envelope of hydrogen and helium, and above a rocky core.

While these layers are believed to comprise water, methane, and ammonia, extreme internal conditions likely result in exotic phases.

The physics associated with these high-pressure, high-temperature regions can lead to unconventional states of matter, prompting theorists and experimentalists to predict and recreate the phenomena they might encounter.

Dr. Cong Liu and colleagues at the Carnegie Institution for Science employed advanced computing and machine learning to conduct quantum physics simulations of hydrogenated carbon at pressures ranging from about 5 million to 30 million times atmospheric pressure (5-3,000 gigapascals) and temperatures of 4,000-6,000 K.

These simulations indicated the development of an ordered hexagonal framework where hydrogen atoms traverse helical paths, resulting in a quasi-one-dimensional superionic state.

Superionic materials are remarkable as they exist in a unique state between solids and liquids. Atoms of one type maintain their crystal arrangement, while atoms of another type gain mobility.

“This newly predicted carbon-hydrogen phase is particularly noteworthy because the movement of atoms isn’t entirely three-dimensional,” explained Dr. Ronald Cohen, also from the Carnegie Institution for Science.

“Rather, hydrogen preferentially migrates along distinct helical paths contained within the organized carbon structure.”

The direction of this atomic motion significantly influences heat and electrical transport within the planet’s interior.

This behavior has implications for understanding internal energy redistribution, electrical conductivity, and potentially the generation of magnetic fields in ice giants.

Additionally, this discovery broadens our comprehension of how simple compounds behave under extreme conditions and suggests that even basic systems can remarkably organize into complex phases.

“Carbon and hydrogen are prevalent in planetary materials, yet their combined behavior under giant planetary conditions remains poorly understood,” Dr. Liu remarked.

These findings are published in a study in Nature Communications dated March 16th.

_____

C. Liu et al. “Prediction of thermally driven quasi-one-dimensional superionic state of hydrogenated carbon under giant planetary conditions.” Nat Commun, published online on March 16, 2026. doi: 10.1038/s41467-026-70603-z

Source: www.sci.news

Discovering a Jurassic Ichthyosaur Fossil: A Major Find in Cuba

Discovering the Most Complete Ichthyosaur Skeleton in Cuba



An ophthalmosaurid ichthyosaur. Image credit: Dmitri Bogdanov / CC BY 3.0.

Paleontologists recently unearthed the most complete **ichthyosaur skeleton** ever found in western Cuba, deep within a **limestone cave**. This significant discovery was made in 2023 at the river cave known as **El Cuajani**, part of the Viñales Geopark and National Park.

The exposed skeletal remains feature a **U-curved vertebral column**, multiple associated ribs, isolated vertebrae, and a hindlimb.

“The specimen is preserved in rock slabs that form the ceiling of the river cave, specifically known as **Cueva del Ictiosario**, located approximately 60 meters from the entrance,” shared Dr. Manuel Iturralde Vinent from the Cuban Academy of Sciences, collaborating with experts from Cuba, Argentina, Poland, and the US.

This remarkable fossil dates back to the **Tithonian period** of the late Jurassic era, roughly **145 million years ago**. Previously, most records of Cuban ichthyosaurs were limited to older Oxford deposits.

“This fossil stands out as the most complete ichthyosaur retrieved from Cuba,” the paleontologists remarked. “It significantly extends the temporal record of **island ichthyosaurs**, which previously only included the Oxford specimen.”



Partial skeleton of El Cuajani ichthyosaur. Image credit: Iturralde-Vinent et al., doi: 10.1080/02724634.2025.2609717.

The **El Cuajani ichthyosaur**, as researchers have informally dubbed it, has yet to be classified into a specific species, but its anatomical features suggest connections to the **Ophthalmosauridae** family.

“The morphology of the hind limbs resembles that of Tithonian **platypterigin ophthalmosaurids**, such as Caprisaurus bonapartei and Aegylosaurus leptospondylus,” they explained.

Scientists believe this ancient creature thrived in **deep ocean** environments. The **Caribbean Seaway** served as a vital oceanic corridor, linking distant regions of the Jurassic world.

“The Caribbean Seaway played a crucial role in promoting the dispersal of marine species between Europe, the Gulf of Mexico, and the Pacific Ocean from the Late Jurassic,” the researchers stated.

“This corridor has a Triassic to early Jurassic heritage, rooted in the intercontinental rifts of Pangea, which should not be confused with the early Caribbean basin.”

“The El Cuajani ichthyosaur adds to the growing body of Tithonian ichthyosaur discoveries in this area, potentially enriching our understanding of the biogeographic history of this group,” the researchers concluded.

For further reading, refer to their research paper published in the February 6th issue of the Journal of Vertebrate Paleontology.

_____

Manuel Iturralde-Vinent et al.. A partial skeleton of an ichthyosaur (Ophthalmosauridae) excavated from the Tithonian (late Jurassic period) in western Cuba. Journal of Vertebrate Paleontology published online on February 6, 2026. doi: 10.1080/02724634.2025.2609717

Source: www.sci.news

Discovering Saturn’s Warped Magnetic Shield: Insights into an Alien World

Recent archival data from ESA’s Cassini mission reveals that Saturn’s magnetic bubble is asymmetrically shaped, influenced not only by the solar wind but also by Saturn’s rapid rotation and the material emitted by its moons.



A diagram illustrating Saturn’s magnetosphere configuration affected by solar wind and rapid rotation. Image credit: Xu et al., doi: 10.1038/s41467-026-69666-9.

Saturn’s magnetosphere serves as a shield, protecting the planet from highly charged particles in the solar wind.

Its magnetic footprint is vast, spanning over 10 times the width of Saturn.

A study led by Professor Andrew Coates from University College London analyzed six years of Cassini data to precisely locate Saturn’s cusp, the point where magnetic fields bend towards the planet’s poles and charged particles descend into its atmosphere.

The researchers discovered that this cusp is displaced to the right from the sun’s perspective, typically found between 1 PM and 3 PM (akin to a clock face), compared to the 12 PM position seen on Earth.

This asymmetry is attributed to Saturn’s rapid rotation, which completes a cycle in just 10.7 hours, along with the dense plasma environment resulting from its moons, especially Enceladus.

These factors contribute to pulling the magnetic field lines to the right, though further simulations are needed for validation.

Enceladus, known for its icy plumes erupting from subsurface oceans, holds potential for extraterrestrial life. Saturn’s diverse environment is particularly intriguing as it is slated to be the focus of a significant ESA mission launching in the 2040s.

“The cusp allows the solar wind direct access into the magnetosphere,” states Professor Coates.

“Understanding the location of Saturn’s cusp is crucial for mapping its entire magnetic bubble.”

“Gaining deeper insights into Saturn’s environment is increasingly important as we prepare for missions returning to Saturn and its moon Enceladus.”

“These findings invigorate our enthusiasm for future explorations.”

“This time, we will search for signs of habitability and potential life.”

“The study supports the long-held theory that the rapid rotation of gas giants like Saturn, coupled with their active moons, displaces the solar wind, shaping their magnetospheres differently than Earth’s.”

“This suggests that gas giants like Saturn have unique magnetospheric behaviors compared to Earth.”

“Enceladus is a significant contributor to this dynamic, emitting substantial water vapor that ionizes and infuses the magnetosphere with heavy plasma, further influenced by Saturn’s rotation.”

“The contrasts between Saturn’s and Earth’s magnetic structures imply a fundamental process governing solar wind interactions among different planets,” explains Professor Zhonghua Yao from the University of Hong Kong.

“Comprehensive observations of Earth elucidate its mechanisms, while comparative studies across planets unveil fundamental laws applicable to understanding other celestial environments, including exoplanets.”

“By integrating Cassini’s observations with simulations, we illustrate how Saturn’s rapid rotation and Enceladus’s plasma emissions contribute to the asymmetric global distribution of cusps,” says researcher Dr. Yang Xu from Southern University of Science and Technology.

“We aim for this research to serve as a crucial reference for future explorations of Jupiter and Saturn’s environments.”

Results were published in the journal Nature Communications.

_____

Y. Shu et al. Asymmetric distribution of Saturn’s cusps at dawn and dusk. Nat Commun. 1861, 17th 2023. doi: 10.1038/s41467-026-69666-9

Source: www.sci.news

Discovering WASP-189b: Superhot Jupiter Reveals Star’s Chemical Makeup, Astronomers Find

Astronomers utilizing the Immersion Grating Infrared Spectrometer (IGRINS) at the International Gemini Observatory’s Gemini South Telescope have made groundbreaking discoveries regarding WASP-189b’s atmospheric composition. Their findings indicate that the planet’s elemental composition closely aligns with that of its host star, offering compelling evidence that the planet inherits its chemical makeup from the protoplanetary disk from which it formed.

Artist’s impression of super-hot Jupiter. Image credit: Sci.News.

WASP-189, classified as a 730-million-year-old A-type star, is located 322 light-years away in the constellation Libra.

Also known as HD 133112, this star is significantly larger than our Sun and boasts a temperature exceeding 2,000 degrees Celsius.

First discovered in 2018, WASP-189b is a gas giant that orbits its star at a distance roughly 1.6 times that of Jupiter.

This exotic planet lies about 20 times closer to its star than Earth is to the Sun, completing an orbit in a mere 2.7 days.

According to Arizona State University graduate student Jorge Antonio Sanchez and colleagues, “Superhot Jupiter has temperatures sufficient to vaporize rock-forming elements, such as magnesium, silicon, and iron. This presents a unique opportunity to observe these elements through spectroscopy, a technique that identifies chemicals by analyzing light spectra.”

The astronomers harnessed the IGRINS instrument to capture high-resolution thermal emission spectra of WASP-189b.

They successfully identified neutral iron, magnesium, silicon, water, carbon monoxide, and hydroxyl groups within the exoplanet’s atmosphere.

“The IGRINS data reveals that WASP-189b exhibits a magnesium to silicon ratio identical to that of its host star,” they noted.

This pivotal finding offers the first observational evidence supporting a commonly held hypothesis regarding planetary formation, paving the way for deeper insights into exoplanet creation and evolution.

Gas giants like WASP-189b are believed to possess outer gas layers whose chemical makeup is heavily influenced by the protoplanetary disk from which they originated.

Researchers suspect that the ratio of rock-forming elements in the protoplanetary disk mirrors that of the host star, as they formed from the same primordial matter cloud.

This inferred chemical connection between a star and its surrounding planets is frequently utilized to model the composition of rocky exoplanets.

Previously observed only within our solar system, this link has now been directly documented on distant planets.

“WASP-189b represents a critical observational milestone in understanding terrestrial planet formation, as it allows for measurable quantities to confirm the similarities in stellar composition and the proportion of rocky materials that form alongside planets,” Sanchez stated.

Dr. Michael Rhine, an astronomer at Arizona State University, added, “Our study showcases the capabilities of ground-based, high-resolution spectrometers to analyze key species like magnesium and silicon, two essential elements in rocky planet formation. This advancement opens a new frontier in exoplanet atmospheric studies.”

The findings of this research were published in a paper in the journal Nature Communications on February 18, 2026.

_____

JA Sanchez et al. 2026. The magnesium to silicon ratio in the exoplanet’s atmosphere. Nat Commune 17, 2902; doi: 10.1038/s41467-026-69610-x

Source: www.sci.news

Revealing the Shroud of Turin: Discovering DNA from Humans, Plants, and Animals

Shroud of Turin

The Shroud of Turin is inscribed with an image of a man believed to resemble Jesus Christ.

Public Domain/Art Collection 2/Alamy

Recent DNA analysis has revealed a wide array of animal, plant, and human contaminants on the Shroud of Turin, complicating the narrative surrounding this enigmatic relic that is claimed to be the burial cloth of Jesus Christ from over 2,000 years ago.

Spanning 4.4 meters in length and 1.1 meters in width, the Shroud stands as one of the most infamous and controversial Christian artifacts globally. It was first documented in France in 1354, and has since resided at the Basilica of St. John the Baptist in Turin, Italy, for nearly 5 centuries.

In 1988, scientists utilized radiocarbon dating and accelerator mass spectrometry to conclude that the Shroud was created between 1260 and 1390, thereby raising questions about its association with Jesus. Nonetheless, this late medieval dating remains a point of contention among some Christian scholars.

In 2015, Gianni Barcaccia and a team at the University of Padova in Italy analyzed samples taken from the Shroud in 1978 and proposed that the cloth might have originated from India.

Currently, Mr. Barcaccia, who opted not to be interviewed, leads a renewed study re-examining the 1978 samples. His team has uncovered diverse DNA from both medieval and modern sources preserved within the Shroud.

The genetic material includes DNA from domesticated animals like cats, dogs, chickens, cows, goats, sheep, pigs, and horses, as well as wild species such as deer and rabbits.

The researchers also identified several fish species, including mullet and Atlantic cod, along with marine crustaceans and insects like flies and skin mites.

Common plant DNA found in the Shroud consists of carrots, various wheat types, peppers, tomatoes, and potatoes—likely introduced to Europe post-exploration of Asia and the Americas.

However, pinpointing the timeline of these contamination events remains elusive.

Human DNA samples were traced back to many individuals who handled the Shroud, including the 1978 sampling team. The researchers noted, “The Shroud’s contact with multiple individuals complicates the possibility of identifying its original DNA.”

Almost 40% of the human DNA is of Indian origin, which may stem from historical trade routes or Romans importing linen from areas near the Indus Valley, Barcaccia and his team noted.

“The DNA evidence on the Shroud of Turin indicates that it may have been significantly exposed in the Mediterranean region, and the fabric may indeed have been produced in India,” they concluded.

Anders Goeterström from Stockholm University noted that while early studies date the Shroud to the 13th century, this timeframe is widely accepted in the scientific community. “Although there’s ongoing debate regarding the 1988 radiocarbon date, most researchers consider it robust,” he stated.

Goeterström remains skeptical about the cloth’s Indian origins, asserting, “There’s currently no evidence to suggest that the Shroud is anything other than a French artifact from the 13th or 14th century.”

“As a significant relic, the Shroud has its own history, which may be more fascinating than the unsupported legendary narratives,” he concluded.

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Source: www.newscientist.com

Discovering the Oldest Known Dog: Unraveling the Genetic History of Our Canine Companions

Ancient Evidence of Dog Care in Punarbashi, Turkey, dating back 15,800 years.

Credit: Kathryn Killackey

A groundbreaking discovery at a 15,800-year-old archaeological site in Turkey has revealed the oldest known evidence of dog domestication. Genetic studies indicate that our canine companions were already widespread across Europe 14,300 years ago, during a time when humans were primarily hunter-gatherers and agriculture had yet to develop.

Determining the precise timeline for dog domestication is complex, especially due to the genetic similarities shared between Canis lupus familiaris (domestic dogs) and Canis lupus (gray wolves). Initially, it was believed that the earliest dogs dated back to around 10,900 years ago. However, earlier fossils resembling dogs have been found, as far back as 33,000 years ago, indicating the presence of ancestral dogs that were not fully domesticated.

To further examine the history of dogs, Dr. Lachie Scarsbrook and his team at the University of Oxford analyzed genetic material from various early dog-like remains unearthed at different archaeological sites in Europe.

The oldest confirmed dog remains were discovered at the Pinarbaş Ruins in central Anatolia, Turkey, dating back to the Upper Paleolithic period (15,800 years ago). These findings are currently the earliest direct evidence of dog existence, with more substantial evidence emerging around 5,000 years ago.

“By at least 15,800 years ago, dogs possessed physical and genetic traits akin to modern breeds,” noted Scarsbrook.

Researchers genetically verified that remains from Gough’s Cave, located in Somerset, England, belonged to a dog that lived approximately 14,300 years ago. The genetic cohesiveness between these two ancient dogs suggests a shared ancestor, a phenomenon that sparked intrigue among researchers, given the geographical distance between the cultures associated with these dogs.

The genome analysis indicates that these two Paleolithic dogs originated from a population that traversed across Europe between 18,500 and 14,000 years ago.

Despite their impressive range, Scarsbrook notes, “It’s unlikely dogs traveled across Europe independently.” Instead, the researchers propose that the Epigravettian culture played a role in their introduction, as evidenced by past archaeological findings indicating ancient human interactions.

14,300-Year-Old Dog Jawbone from Gough’s Cave, England

Credit: Natural History Museum

During significant periods, these ancient peoples migrated from the Italian peninsula into Western Europe and southeast into Turkey, fostering interactions that likely resulted in cultural and technological exchanges.

Dogs provided hunter-gatherers with enhanced hunting capabilities, protection from predators, and warmth during chilly nights, according to Scarsbrook.

Research at Gough’s Cave and the Pinarbaş ruins indicates the nature of ancient human-dog relationships. “These findings highlight the foundations of modern human-dog interactions,” states team member William Marsh from the Natural History Museum in London.

Isotope analysis has revealed that the Pinarbash community not only fed their dogs fish but also consumed it, indicating a profound bond between humans and canines. Dogs were buried similarly to humans, pointing to symbolic treatment of these animals about 15,000 years ago, notes Marsh.

At Gough’s Cave, the mixed diet of humans and dogs suggests a connection rich in symbolism. Instead of typical burial practices, some cultures there appear to have practiced ritual cannibalism, with evidence of bones showing mutilation marks and carvings.

Interestingly, similar markings were discovered on a dog jawbone from Gough’s Cave, suggesting parallels in treatment between humans and dogs, positing emotional ties as well, per Marsh. “They undoubtedly felt bonded to these animals, but the complexity of these expressions remains hard to interpret,” he reflects.

Scarsbrook hypothesizes that the domestication of dogs began during the Last Glacial Maximum, roughly 26,000 to 20,000 years ago. “Circumstances were dire for both wolves and humans in northern Eurasia during this period, pushing them southward and compelling interactions that may have initiated a unique companionship,” he states.

Exploring the Origins of Humanity Through Prehistoric Times in South-West England

Join a gentle walking tour that delves deep into the Neolithic, Bronze Age, and Iron Age, allowing you to immerse yourself in the rich heritage of early humans.

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Neanderthals Used Birch Tar as a Natural Antibiotic: Discovering Ancient Medical Practices

Recent research highlights that birch bark tar—historically recognized as a natural tool adhesive—can effectively inhibit harmful bacteria like: Staphylococcus aureus. This suggests that Neanderthals may have utilized it to treat wounds and manage infections during the Ice Age.

Neanderthals likely employed birch tar for various applications, including wound care. Siemsen et al. confirmed that birch tar possesses selective antibacterial properties and effectively inhibits Staphylococcus aureus.

Birch tar is frequently discovered at Neanderthal sites, where it is known to have served as an adhesive for crafting tools.

Recent inquiries suggest that Neanderthals may have had additional uses for this versatile substance.

For instance, indigenous communities in Northern Europe and Canada have utilized birch tar to treat injuries. Increasing evidence indicates that Neanderthals also engaged in various medicinal practices.

To explore the medicinal capabilities of birch tar, Dr. Tjaark Siemssen and his team from the Universities of Cologne and Oxford extracted tar from birch tree bark, particularly species identified at Neanderthal sites.

The researchers employed multiple extraction techniques, including distillation in clay pits and condensation on stone surfaces—methods that Neanderthals could also have accessed.

All tested tar samples showcased effectiveness in inhibiting bacterial growth against various strains, including the notorious Staphylococcus bacteria responsible for wound infections.

These findings not only reinforce the efficacy of indigenous medicinal practices but also lend credence to the possibility that Neanderthals used birch tar for therapeutic purposes.

The researchers note that birch tar, alongside other available plants, may serve additional roles, such as an insect repellent.

Further investigations into the diverse applications of these natural substances will enrich our understanding of Neanderthal culture.

“Our findings demonstrate that birch tar produced by Neanderthals and early humans possesses notable antibacterial properties,” the researchers stated.

“This discovery has significant implications for how Neanderthals managed disease burdens during the last Ice Age and contributes to the expanding knowledge of medicine among early human communities.”

“Integrating research in indigenous pharmacology and experimental archaeology enhances our understanding of the medical practices of our early ancestors and their closest relatives.”

“Moreover, this paleopharmacological research could assist in rediscovering antibiotic treatments as we confront a rising crisis of antimicrobial resistance.”

“The intricate processes involved in birch tar production are noteworthy.”

“Each stage of production was a sensory journey, and the challenge of cleaning tar from my hands after hours by the fire was a central experience every time.”

For more detailed insights, refer to the study published in the journal PLoS ONE.

_____

T. Ziemsen et al. 2026. Antibacterial properties of experimentally produced birch tar and its medicinal efficacy in the Pleistocene. PLoS One 21 (3): e0343618; doi: 10.1371/journal.pone.0343618

Source: www.sci.news

Discovering a Mysterious Magma and Sulfur Planet Hidden in the Milky Way

Recent findings on L 98-59d, part of the five-planet system L 98-59, indicate that this intriguing exoplanet may host an extensive global magma ocean, effectively trapping sulfur deep within its interior. This discovery introduces a previously unidentified category of extraterrestrial worlds.

Artist’s impression of planetary system L 98-59. Image credit: Mark A. Garlick / markgarlick.com.

The distant L 98-59 system lies approximately 34.5 light-years away in the southern constellation Bootes.

Known as TOI-175 or TIC 307210830, this bright M dwarf star has a mass roughly one-third that of the Sun.

This intriguing planetary system features at least three transiting planets and two non-transiting planets: L 98-59b, L 98-59c, L 98-59d, L 98-59e, and L 98-59f.

L 98-59d completes an orbit around its parent star every 7.5 days and is about 1.6 times larger than Earth, receiving approximately four times the radiant energy of our planet.

A recent study led by astronomer Harrison Nichols from the University of Oxford aimed to reconstruct the planetary history of this super-Earth, tracing its evolution from its formation nearly 5 billion years ago.

By correlating telescope observations with comprehensive physical models of the planet’s interior and atmosphere, the research team gained insights into the planet’s deep geological processes.

The findings suggest that L 98-59d possesses a mantle of molten silicate similar to Earth’s lava, underpinned by a vast global magma ocean that extends for thousands of kilometers.

This massive molten reservoir enables L 98-59d to store significant amounts of sulfur within its interior over geological timescales.

Moreover, the magma ocean assists in retaining a hydrogen-rich atmosphere laden with sulfur compounds like hydrogen sulfide, which is typically lost to space due to X-ray radiation emitted by the host star.

Over billions of years, the interplay between its molten interior and atmosphere has sculpted L 98-59d into the striking world observed today.

Researchers propose that L 98-59d may represent the inaugural example of a newly identified category of gas-rich sulfur exoplanets that sustain long-lived magma oceans. If validated, this could greatly expand our understanding of planetary diversity in the galaxy.

“This discovery highlights that the current classifications of small planets may be overly simplistic,” remarked Dr. Nichols.

“While this molten world is unlikely to support life, it showcases the vast array of planets beyond our solar system. What other types of celestial bodies remain undiscovered?”

For more details, refer to the study published in today’s edition of Nature Astronomy.

_____

H. Nichols et al. Evolution of a volatile-rich molten super-Earth L 98-59d. Nat Astron, published online March 16, 2026. doi: 10.1038/s41550-026-02815-8

Source: www.sci.news

Discovering Unique Mobius Strip-Inspired Molecules: Unveiling Their Extraordinary Shapes

Representation of electrons in a half Möbius molecule

Representation of Electrons in a Half Möbius Molecule

IBM Research and the University of Manchester

Recent discoveries by chemists reveal an intriguing new molecular structure, which exceeds the complexity of a traditional Möbius strip.

A Möbius strip is a twisted shape that requires an object, like an ant, to traverse it twice to return to its original side.

Igor Roncevic and his team at the University of Manchester have uncovered a more complex half-Möbius molecular structure. This breakthrough could revolutionize the manipulation of molecular shapes and topologies for various applications.

“This molecule is entirely novel and unexpected. Not only is it captivating that we have synthesized a molecule with unconventional topology, but we have also verified that such a structure is feasible, which was previously unconsidered,” he states.

To synthesize the molecule, the researchers combined 13 carbon atoms and two chlorine atoms into a ring on a gold substrate at ultra-low temperatures. Utilizing advanced atomic force and scanning tunneling microscopes, they precisely controlled individual atoms and analyzed the electron properties. Here, electrons do not remain rigidly attached but are diffused in a localized region, resembling tiny waves of matter.


The interactions among these electrons induced unprecedented twists within the molecule. A hypothetical quantum particle would need to revolve around the structure four times to return to its starting point.

Researchers demonstrated the ability to toggle the molecular state from left-handed to right-handed or to untwist it through small electromagnetic pulses. This innovation allows chemists to engineer molecular topology on demand.

To comprehend the newly discovered molecule and its potential existence, the researchers employed simulations on classical computers and an IBM quantum computer. Electron interactions are essential for introducing twists in molecules, which are challenging to simulate accurately on traditional platforms. However, quantum computers, built upon interacting quantum entities, can perform these simulations with greater precision, Roncevic notes.

According to team members, this research illustrates how quantum computing can tackle real-world chemistry challenges. Ivano Tavernelli from IBM emphasizes this point.

“This groundbreaking experiment integrates multiple facets of organic chemistry, surface science, nanoscience, and quantum chemistry,” asserts Gemma Solomon from the University of Copenhagen.

“This is an exciting endeavor that effectively translates abstract topological ideas into the field of molecular chemistry,” adds Kenichiro Itami from RIKEN, Japan, noting the technical significance of the research.

Kim Dong Ho, a professor at Yonsei University in South Korea, highlights the potential applications of shape-switchable molecules in sensor technology, indicating that they could toggle states in response to magnetic fields.

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Source: www.newscientist.com

Ganymede’s Aurora Patch: Discovering Similarities with Earth’s Aurora Physics

Scientists from the United States, Europe, and China utilized the Ultraviolet Spectrometer (UVS) on NASA’s Juno spacecraft to meticulously map the auroral patch structure on Ganymede, Jupiter’s moon, revealing similarities to Earth’s auroras. Their groundbreaking research indicates that interactions between magnetic fields and charged particles could be the universal driver of auroras, enhancing our understanding of magnetospheres across the solar system.

Artist’s concept of the aurora borealis on Jupiter’s moon Ganymede. Image credits: NASA/ESA/G. Bacon, STScI/J. Saur, University of Cologne.

Ganymede stands out as the only known moon to possess its intrinsic magnetic field, creating a miniature magnetosphere nested within the vast magnetosphere of Jupiter.

The auroral emissions primarily stem from oxygen at wavelengths of 130.4 nm and 135.6 nm, triggered by precipitating electrons.

In a recent groundbreaking study, researcher Philippe Gusbin from the University of Liège and his team examined ultraviolet observations of Ganymede conducted on June 7, 2021, by the Juno spacecraft.

They identified multiple auroral spots in Ganymede’s leading downstream hemisphere.

These patches typically measure about 50 km in size, with brightness levels soaring to around 200 Rayleigh.

“Auroras on Ganymede are driven by the precipitation of electrons into its thin oxygen atmosphere,” explained Gusbin.

“Previous observations of Ganymede’s auroras were limited in detail due to the spatial constraints of ground-based methods, which couldn’t resolve the fine structures commonly observed in planetary auroras.”

The morphology and scale of Ganymede’s auroras closely resemble the auroral ‘beads’ found on Earth prior to magnetospheric substorms and in Jupiter during ‘dawn storms.’

The lack of a similar patch in the southern hemisphere could stem from observational geometry, but it may also reflect an asymmetry tied to Ganymede’s location in Jupiter’s plasma disk.

“Auroral ‘beads’ are also present in the auroras of Earth and Jupiter, where they correlate with substorms and dawn storms—major magnetospheric reorganizations that release significant energy and induce intense auroral activity,” noted Dr. Alessandro Moirano, a postdoctoral researcher at the University of Liège and the National Institute of Astrophysics in Rome.

This discovery implies that similar physical processes may govern magnetospheres, despite variations in scale and environmental conditions.

“Juno’s close flyby of Ganymede lasted under 15 minutes, and it will not revisit Ganymede, leaving us unsure about the frequency of these patches or how they may evolve,” remarked Dr. Bertrand Bonfont, an astrophysicist at the University of Liège.

“Fortunately, ESA’s JUICE mission is currently en route to Jupiter and is set to arrive in 2031. This mission will conduct detailed observations of Ganymede.”

“Equipped with a similar ultraviolet spectrometer to that of Juno, this spacecraft will facilitate long-term observations that could reveal more about the evolution of Ganymede’s aurora and potentially uncover new mysteries.”

For further reading, refer to a paper published in Astronomy and Astrophysics.

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A. Moirano et al. 2026. High spatial resolution ultraviolet observations of Ganymede’s aurora patches by Juno. Constraints on the magnetospheric source region. A&A 706, L16; doi: 10.1051/0004-6361/202558379

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

Discovering the Oldest Vertebrates: Unveiling Four Camera-Shaped Eyes

A groundbreaking study by paleontologists at Yunnan University reveals that two Myrodonidae fish species, which thrived in what is now China approximately 518 million years ago during the Cambrian period, possessed a unique vision system featuring two large lateral eyes alongside two smaller central eyes.

An artist’s reconstruction of the four-eyed Myllokunmingiid that navigated the ancient world. Image credit: Xiangtong Lei and Sihang Zhang.

This primitive jawless fish, known as Myllokunmingiid, existed during the Cambrian period, a time marked by rapid evolutionary advancements in body structures and sensory systems as a response to increased predation.

Considered the oldest known vertebrates, these fascinating creatures challenge our understanding of early vision.

In a recent study, Professor Peiyun Cong and colleagues investigated a newly discovered fossil of Myrocunminidae, expertly preserved at the renowned Sumjiang Fossil Bed in southern China.

“These fossils maintain remarkable detail in their eye structures,” stated Professor Cong.

“Initially, we focused on the large eye to outline its anatomy and were astonished to discover two fully functional small eyes nestled between them. The excitement of this finding was immense.”

Modern vertebrates primarily rely on two eyes for vision.

The pineal gland, a brain structure, plays a crucial role in sleep regulation by producing melatonin in response to light exposure.

Interestingly, some fish, amphibians, and reptiles retain the ability to detect light through what is commonly referred to as a “third eye.”

The discovery of two Myrocunminidae provides evidence that early vertebrates possessed a well-developed pair of image-forming eyes, rather than a simple light sensor.

“Our findings suggest that the pineal gland originated as an imaging eye,” remarked Professor Cong.

“Over time, these structures diminished in size, lost their vision capabilities, and assumed their modern function in sleep regulation.”

Using a high-powered microscope, researchers identified melanosomes—pigment-containing organelles crucial for vision—across all four Myrocunminidae orders.

Chemical analyses confirmed the presence of melanin, the same pigment utilized in contemporary vertebrate vision.

Circular formations resembling lenses indicate that these eyes had the capacity to detect light and form images, offering direct evidence of an advanced visual system in early vertebrates.

Professor Sarah Gabot from the University of Leicester emphasized, “Fossilized eyes are extremely rare. It’s remarkable that delicate structures like eyes can survive hundreds of millions of years.”

“However, under optimal conditions, such preservation is achievable, unveiling crucial insights into how extinct species perceived their environment.”

“We speculated that these Chinese fossil eyes might be remarkably preserved, demonstrating light-absorbing pigments in their retinas and lenses, revealing the visual acuity of our early ancestors.”

The Cambrian seas presented perilous conditions, with emerging large predators threatening the small, vulnerable early vertebrates.

Dr. Jacob Binther, a paleontologist at the University of Bristol, noted, “In such an environment, having four eyes may have provided these organisms with a broader field of vision essential for evading predators.”

This discovery elucidates long-held questions about the origin of the pineal gland, offering the oldest known evidence of a camera-like eye in the fossil record.

“This finding reshapes our understanding of vertebrate evolutionary history,” stated Dr. Binther.

“It turns out our ancestors were visually sophisticated beings capable of surviving in a hazardous world.”

The study also prompts a reevaluation of the established notion of the vertebrate “third eye.”

“These early vertebrates possessed not only a third eye, but intriguingly, a fourth eye as well,” concluded Dr. Binther.

This discovery is detailed in a paper published in the journal Nature on January 21, 2026.

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X Ray others. 2026. Four camera-shaped eyes found in the earliest Cambrian vertebrates. Nature 650, 150-155; doi: 10.1038/s41586-025-09966-0

Source: www.sci.news

Ancient Mariners: Discovering Remote Arctic Islands Over 4,000 Years Ago

Ruins on Isbjørne Island

Ancient Inuit Circular Tents Found on Isbjørne Island

Credit: Matthew Walls, Marie Christ, Pauline Knudsen

4,500 years ago, early humans embarked on a historic journey to a remote island off Greenland’s northwest coast. This daring expedition entailed crossing over 50 kilometers of open sea, marking one of the longest maritime voyages by Arctic indigenous peoples.

Archaeologists assert that these intrepid sailors were the first to reach these isolated islands. Notably, John Derwent from the University of California, Davis, contributed insights but was not involved in this study.

In 2019, Matthew Walls and a team from the University of Calgary, Canada, explored the Kittisut Islands, also known as the Carey Islands, located northwest of Greenland. These islands lie within the Pikiarasorsuaq polynya—an open ocean region surrounded by sea ice, which has been present for approximately 4,500 years.

The research focused on three main islands: Isbjörne, Mellem, and Nordvest, revealing five sites with a total of 297 archaeological features. The most significant findings were at Isbjörne beach terraces, where they uncovered the remnants of 15 circular tents, each with a central hearth and divided by stones. These distinctive “bilobed” structures are emblematic of the Paleo-Inuit—the first settlers of northern Canada and Greenland.

Radiocarbon dating of a long-billed murre’s wing bones found within one of the tent rings indicated they are between 4,400 and 3,938 years old. This confirms that humans occupied the Kittisut Islands shortly after the formation of the polynya.

“We have nesting colonies of long-billed murres,” Walls noted. The early settlers likely harvested their eggs and hunted them for food, and they likely pursued seals as well.

The Old Inuit had already reached Greenland at this time and likely journeyed to Kittisut from the west, covering a minimum distance of about 52.7 kilometers. However, due to prevailing winds and currents, they most likely set sail from a more northerly location, resulting in a longer, safer journey. To the west of Kittisut lies Ellesmere Island, which is further but presents challenging navigational conditions.

The only comparable journey known in Arctic prehistory was the 82-kilometer crossing of the Bering Strait from Siberia to Alaska, likely first accomplished over 20,000 years ago, with the Diomede Islands serving as a midway stopping point.

“Crossing that expanse required advanced watercraft,” Derwent emphasizes. The population on Kittisut likely necessitated larger vessels rather than single-person kayaks. “You can’t transport children and the elderly safely in a kayak,” he explained. The Old Inuit likely used larger boats capable of carrying nine or ten individuals.

Despite extensive studies, no boat wrecks have yet been uncovered on Kittisut Island, and few such finds exist in the Arctic region. “Their vessels would have been skin-on-frame designs similar to those utilized by later Inuit communities,” noted Walls.

The initial Paleo-Inuit settlers likely played a vital role in shaping the Kittisut ecosystem. By transporting marine nutrients onto land, they fertilized the barren soil, fostering plant growth on the islands. “There’s initially a diverse plant life there, reliant on human involvement in nutrient cycling between marine and terrestrial systems.”

Arctic Cruise with Dr. Russell Arnott: Svalbard, Norway

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Discovering the Universe’s Most Powerful Microwave Laser: A Revolutionary Breakthrough

Galaxy H1429-0028 Gravitational Lensing

This image combines views from the Hubble and Keck II telescopes. The diagonal galaxy in the foreground serves as a gravitational lens, causing a distorted image of the background galaxy H1429-0028.

Credit: NASA/ESA/ESO/WM Keck Observatory

Astronomers have identified an unprecedented microwave beam, akin to a laser, emitted from two colliding galaxies. This discovery, the brightest and most distant recorded, marks a significant milestone in our understanding of cosmic phenomena.

The generation of laser light involves stimulating atoms into a high-energy state. When photons interact with these excited atoms, they induce the release of additional photons, leading to a chain reaction. The result is a coherent light beam with uniform frequency.

Similarly, during galactic collisions, compressed gas triggers star formation and enhanced luminosity. As light travels through dust clouds, it can excite hydroxyl ions composed of hydrogen and oxygen into a high-energy state. When these ions are stimulated by radio waves, potentially from a supermassive black hole, they can release concentrated beams of microwave radiation known as masers.

Recently, Roger Dean and researchers from the University of Pretoria discovered the brightest and most distant maser in galaxy H1429-0028, approximately 8 billion light-years from Earth. Gravitational lensing, caused by a massive galaxy, distorts the light from H1429-0028, acting like a cosmic magnifying glass.

Using the MeerKAT telescope—a network of 64 radio telescopes working collaboratively—Dean and his team searched for galaxies abundant in hydrogen molecules emitting distinctive frequencies. When they focused on H1429-0028, they detected an unusually strong radiation signal, indicating the presence of powerful masers.

“Upon checking the frequency of 1667 megahertz, we immediately recognized a significant signal. What was once a mere observation transformed into a record-breaking discovery,” Dean recalls.

These extraordinary light emissions could be classified as gigamasers, far exceeding the brightness of typical megamasers found closer to the Milky Way, with an intensity approximately 100,000 times that of an ordinary star, tightly concentrated in a minuscule region of space.

Future enhancements, including the development of the South African Square Kilometer Array, will be capable of detecting even more distant masers, poised to revolutionize our understanding of cosmic history. As Matt Jarvis from Oxford University notes, these masers may offer insights into the merger processes of some of the universe’s earliest galaxies.

“To acquire accurate data about these ancient galactic mergers, we require continuous radio and infrared emissions, primarily sourced from heated dust enveloping forming stars,” Jarvis explains. “The intricate physical conditions needed to produce masers originate from these galactic collisions.”

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Discovering the Pioneers of Tool and Art Creation: Uncovering Human Innovation

Recent findings highlight the emergence of early mining and hunting tools.

Raul Martin/MSF/Science Photo Library

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In headlines about human evolution, terms like “oldest,” “earliest,” and “first” dominate. I’ve authored numerous articles featuring these phrases.

This isn’t just an attention-grabbing tactic; it serves a purpose. When researchers identify evidence suggesting a species or behavior predates previous estimates, it elucidates our understanding of timelines and causations.

For instance, it was once believed that all rock art originated no earlier than 40,000 years ago, attributed solely to Homo sapiens, as Neanderthals were thought to have vanished by then. New evidence suggests that some prehistoric art predates this threshold, indicating Neanderthal artistic expression.

The past month has unveiled a flurry of “earliest” discoveries, prompting reflections on the reliability of such timelines. How can we ascertain the true age of early technologies?


Let the Exploration Begin!

During excavations in southern Greece, archaeologists unearthed two wooden tools estimated to be about 430,000 years old—possibly the oldest known wooden tools. One is believed to be a drilling rod, while the function of the other remains uncertain.

These tools are closely dated to the previous record holders, including the Clacton spear from Britain, approximated at 400,000 years old, and wooden spears found in Schöningen, now reassessed to nearly 300,000 years old.

Bone tools also emerged in Europe during this epoch. For instance, in Boxgrove, England, remnants from an elephant-like creature, possibly a steppe mammoth, were fashioned into hammers. These elephant bones date back 480,000 years, marking the oldest known utilization of elephant bone in Europe. However, in East Africa, ancient humans were crafting tools from elephant bones over 1.5 million years ago—perhaps much earlier.

Shifting our chronological lens, a recent discovery in Xigou, central China, reported a collection of 2,601 stone artifacts dating between 160,000 and 72,000 years ago, featuring composite tools attached to wooden handles—possibly the earliest evidence of such technologies in East Asia.

Moreover, an archaeological revelation in South Africa indicated that 60,000 years ago, early humans employed poisoned arrows for hunting, as evidenced by five arrowheads lined with toxic plant fluids.

Each of these findings carries deeper implications.

Examining the Past

Traces of plant toxins discovered on arrow points

Marlize Lombard

The oldest verified wooden tools we have may not represent the absolute earliest. Preservation issues plague prehistoric wooden artifacts; they tend to decay, leading to gaps in the historical record.

According to Katerina Harbati, who directs the wooden tools excavation, people likely used such tools well before 400,000 years ago, but prior examples remain undiscovered.

Woodworking is simpler than stone crafting, and since chimpanzees can fashion rudimentary wooden tools, it is plausible that wooden tools represent humanity’s earliest technological forms. An unexpected finding of a million-year-old wooden tool, though astonishing, would not be entirely improbable.

Consequently, significant narratives on human technological advancements shouldn’t solely pivot on the age of the earliest wood tools. Confidence in tool usage timelines necessitates rigorous investigation into various age groups.

As for poisoned arrows, these are recognized as the earliest validated forms of poisoned arrowheads. Nonetheless, designs akin to contemporary poisoned arrows have been identified from tens of thousands of years ago. Like wood, poison’s organic nature leads to rapid decay.

We should be cautiously assured. Poison arrows exemplify composite technological advancements and emerged later in the evolutionary timeline, possibly not even tracing back to early hominids such as Ardipithecus or Australopithecus.

Turning to prehistoric art, we find a wealth of complexity.

Exploring Prehistoric Graffiti

Hand stencils from a cave in Indonesia

Ahdi Agus Oktaviana

While cave paintings are iconic, other forms like carvings and engravings offer their own challenges in dating. If a sculpture is buried in sediment, its age can usually be determined based on sediment analysis. However, dating cave art proves trickier. Charcoal-based works that are less than 50,000 years old offer more reliable carbon dating, whereas those beyond this window yield inconclusive results.

Recently, hand-painted stencils found in caves on Sulawesi island were dated to at least 67,800 years, competing with a similar stencil in Spain attributed to Neanderthals, arguably the oldest rock art known.

Notably, the phrase “at least” matters significantly in this context. Dating relies on surface rock layers created through mineral deposits, which are only minimally informative. The artworks beneath could be much older.

The goal here isn’t to assert that we lack all knowledge, but rather, we possess a wealth of understanding, much of it newly uncovered in the last two decades. We must strive for a coherent timeline in human evolution and cultural development while acknowledging uncertainties.

In paleontology, having numerous specimens enhances reliability. Instead of studying charismatic prehistoric animals like dinosaurs, paleontologists often focus on smaller organisms that leave abundant fossil records, enabling deeper insights into their evolutionary progress.

However, in human evolution, the fossil record is uneven. Individual hominid species may number in the dozens, yet the early specimens remain scarce, hindering our understanding of their longevity and geographical spread. The relationship between evolved species also eludes clarity amidst possible complicated derivations.

Conversely, stone tool records are extensive, dating back to the 3.3 million-year-old Lomekwean stone tools in Kenya. We might encounter even older tools. Early humans like Ororin (6-4.5 million years ago) and Ardipithecus (5.8-4.4 million years ago) likely spent most time in trees, making their tool-making unlikely.

Wooden tools present their own challenges. Our knowledge remains limited and fragmented, largely due to preservation issues. A reliable timeline for the evolution of wooden tools seems elusive.

When it comes to ancient art, the challenges are primarily technical. Preserved artworks are available, yet accurate dating techniques are limited. Creating a chronology for artistic development poses immense challenges, although advancements in technology may facilitate progress over time. With any luck, by retirement, I hope to have a clearer understanding of the evolution of ancient human artistic practices.

In essence, all narratives about human evolution are, to some degree, provisional. This holds true across paleontological studies, especially for narratives with more uncertainty. The timeline of non-avian dinosaur extinction is quite clear-cut; however, human evolution allows for more variability. Further excavations and improved dating methods should refine our understanding, but some uncertainties may remain.

Neanderthals, the Origins of Humanity, and Cave Art: France

From Bordeaux to Montpellier, embark on a fascinating journey through time as you explore southern France’s significant Neanderthal and Upper Paleolithic sites.

Topics:

  • Ancient Humans /
  • Our Human Story

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

Discovering the Shining Nebula: A Stellar Cradle of New Stars

Exploring Bella Junior’s Supernova, also referred to as RX J0852.0-4622 or G266.2-1.2, scientists have revealed the mysteries surrounding its explosive past. This ancient nebula, once a brilliant supernova, has perplexed researchers regarding its distance and the magnitude of its explosion. Recently, however, groundbreaking discoveries linked a newly formed star, Ve 7-27, with the remnants of Bella Junior. By utilizing the Multi-Unit Spectroscopic Explorer (MUSE) on the ESO’s Very Large Telescope, astronomers have captured unprecedented detailed images of Ve 7-27.



VLT/MUSE image of Ve 7-27. Image credit: ESO / Suherli et al.

“This is the first evidence ever connecting a newborn star to the remnants of a supernova,” stated Dr. Samar Safi Harb, an astrophysicist from the University of Manitoba.

“This discovery resolves a decades-long debate, enabling us to calculate the distance of Bella Junior, its size, and the true power of the explosion.”

By examining the gas emissions from Ve 7-27, Dr. Safi Harb and his team confirmed that it shares the same chemical signature as materials from the Vela Junior supernova.

This correlation established a physical connection between the two celestial bodies, allowing astronomers to accurately determine Bella Junior’s distance.

Both Ve 7-27 and Vela Junior are approximately 4,500 light-years away.

“The gas present in this young star mirrors the chemical composition of stars that exploded in the past,” remarked Dr. Safi Harb.

“Isn’t it poetic? Those same elements eventually contributed to Earth and now play a role in forming new stars.”

Recent findings indicate that Bella Junior is larger, more energetic, and expanding at a rate quicker than previously thought, marking it as one of the most potent supernova remnants in our galaxy.

“Stars are constructed in layers, much like onions,” Dr. Safi Harb explained. “When they explode, these layers are propelled into space.”

“Our research indicates that these layers are now becoming visible in the jets of nearby young stars.”

“This study not only solves an enduring astronomical enigma but also sheds light on stellar evolution, the enrichment of galaxies with elements, and how extreme cosmic events continue to shape our universe.”

This research was published today in a study featured in the Astrophysics Journal Letters.

Source: www.sci.news