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Fossil Discovery Sheds Light on the Origins of Earth’s First Fish

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Paleontologists from Australia and China have conducted two groundbreaking studies on the fossilized remains of a remarkable Devonian lungfish. Utilizing advanced imaging technology, they have unearthed previously overlooked anatomical details, significantly enhancing our understanding of early vertebrate evolution. Their findings have been published in the Canadian Journal of Zoology and the journal Current Biology.

Paleolophus yunnanensis, a unique lungfish species that thrived in southern China’s waters 410 million years ago. Image credit: Brian Choo, Flinders University.

In a recent study, lead researcher Alice Clement, a paleontologist at Flinders University, investigates The Mystery of Kainokara, a fossil known from a single specimen found in the Late Devonian Gogo Formation of Western Australia.

“New research, including the analysis of previously neglected specimens, is gradually uncovering the rich diversity of lungfishes found in Australia’s significant fossil sites,” said Dr. Clement.

“One particularly enigmatic specimen originates from Australia’s earliest ‘Great Barrier Reef’, a Devonian reef located in the Kimberley region of northern Western Australia.”

“When first described in 2010, this unusual specimen was so perplexing that the authors speculated it might represent an entirely new type of fish never documented in science.”

“Using advanced scanning techniques, we developed comprehensive digital images of both the external and internal structures of the skull, revealing the complexity of this fascinating lungfish’s brain cavity.”

“In fact, we confirmed that earlier interpretations may have been from an upside-down perspective.”

“We were also able to compare the well-preserved inner ear region with other lungfishes,” noted Flinders University paleontologist Hannah Thiele.

“This provides an essential data point in the rich collection of lungfish and early vertebrate species.”

“This research enhances our understanding of the evolutionary progression of these ancient lobe-finned fishes, both in Gondwana and globally.”

In a separate study, Flinders University paleontologist Brian Chu and colleagues reveal a newly discovered species of lungfish from the Devonian period in China, Paleolophus yunanensis.

“The discovery of Paleolophus yunanensis offers unprecedented insight into the transitional phase between the early appearance of lungfish and their extensive diversification millions of years later,” said Dr. Chu.

“At this time, this group was just beginning to develop unique feeding adaptations that would serve them well throughout the remainder of the Devonian period and into the present.”

“Lungfish, including the ancient lineage found in Queensland, Australia, have fascinated researchers due to their close evolutionary relationship with tetrapods, the four-limbed vertebrates that include humans.”

“The distinctive skull of the newly discovered lungfish from 410-million-year-old rock formations in Yunnan offers crucial insights into the rapid evolutionary changes during the Early, Middle, and Late Devonian periods.”

“The new specimens exhibited both similarities and differences compared to the earliest known specimens, such as Diabolepis fossils from southern China and uranolophus found in locations like Wyoming and Australia.

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Hannah S. Thiele et al., deciphering The Mystery of Kainokara from the Late Devonian Gogo Formation, Australia. Canadian Journal of Zoology, published online January 28, 2026. doi: 10.1139/cjz-2025-0109

Tuo Qiao et al., 2026. New fish fossil sheds light on the rapid evolution of early lungfish. Current Biology 36 (1): 243-251; doi: 10.1016/j.cub.2025.11.032

Source: www.sci.news

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

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Comparison of Sahelanthropus fossils with chimpanzees and humans

Sahelanthropus: Fossil comparison with chimpanzees and humans

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

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

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

The journey to this conclusion has been extensive.

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Explore the Origins of Humanity in South-West England

Join a gentle walking tour through the Neolithic, Bronze Age, and Iron Age, immersing yourself in early human history.

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Source: www.newscientist.com

AI Research Sheds Light on Why Super-Recognition Skills Excel in Face Identification

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They are salisbury novichok addict uncovering a murder suspect or even identifying a sexual predator. The research offers fresh insights into why superrecognizers excel at facial recognition.

Previous studies indicate that individuals with exceptional facial recognition skills observe more regions of the entire face compared to average individuals.

Recently, researchers have employed advanced AI techniques to reveal how this perspective enhances their capabilities.

“It’s not solely about seeing everything, it’s about using your vision intelligently,” stated the lead author of the study, Dr. James Dunn from UNSW Sydney.


In a recent article published in Proceedings of the Royal Society B: Biological Sciences, Dunn et al. highlight how they extracted eye-tracking data from a previous study involving 37 superrecognizers and 68 typical recognizers.

In their experiment, participants viewed both images of entire faces and segmented images focusing on the regions they were examining.

In this new research, the team utilized this data to reconstruct the visual information that was available to the participants’ eyes.

This “retinal information” was processed through a deep neural network (DNN), an AI system trained for facial recognition. Participants provided the AI with either a complete image of the same face they had seen or a different one.

In all instances, the AI generated a score indicating how closely the retinal information matched a given complete facial image.

The research team compared outcomes between typical participants and super-recognizers, along with data drawn from randomly chosen areas of the initial facial images.

The findings indicated that the AI system’s effectiveness improved as the visibility of the observed facial feature increased.

Moreover, across all levels of visibility, the AI performed optimally when relying on retinal data from superrecognizers.

“This suggests that variations in facial recognition capability are partly due to our active exploration and sampling of visual data, rather than just post-processing by the brain,” Dunn remarked.

The team then examined whether their findings simply indicated that superrecognizers looked at more areas of the face and gathered more data.

However, they discovered that even when the same amount of retinal information was captured, the AI performed better with data from super-recognizers.

“Their advantage lies not only in the quantity but also in the quality of information,” says Dunn. “They focus on areas that provide more identity cues, making each ‘pixel’ they select significantly more valuable for facial recognition.”

Dr. Rachel Bennett, a facial processing expert from Brunel University in London who was not involved in the study, praised the research.

“The key contribution to understanding super-recognition is that effective facial recognition isn’t only about examining specific areas or spending more time looking at the face. Super-recognizers explore not just larger areas, but also gather more advantageous data,” she asserted.

Dr. Alejandro Estudillo from Bournemouth University noted that the study was conducted by showing participants still images in highly controlled environments.

“It will be crucial to see if the same patterns emerge in more natural, dynamic contexts,” he said.

This study implies there are strategies to enhance facial recognition; however, it seems unlikely that anyone can train to become a super-recognizer.

“At present, we cannot determine if these eye movement patterns can be effectively trained,” Bennett remarked.

Dunn stated that research indicates super-recognition is likely influenced by genetics and is often inherited.

“Superrecognizers appear to instinctively identify the most crucial features. This is challenging to teach, as it differs from one face to another,” he explained.

Researchers have created a free test to help identify supercognitive traits: New South Wales face test.

Source: www.theguardian.com

Ultracold Clock Sheds Light on Quantum Physics’ Impact on Time

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What is the quantum nature of time? We may be on the verge of discovering it

Quality Stock / Alamy

How does time manifest for a genuine quantum entity? The most advanced clocks can rapidly address this query, enabling us to test various ways to manipulate and alter the quantum realm, thereby delving into the uncharted territories of physics.

The notion that time can shift originates from Albert Einstein’s special theory of relativity. As an object approaches the speed of light, it appears to experience time more slowly compared to a stationary observer. He expands upon this with a general theory of relativity, which demonstrates a similar temporal distortion in the presence of a gravitational field. Igor Pikovsky from the Stevens Institute in New Jersey and his team aim to uncover whether a similar effect occurs within the microscopic quantum landscape, utilizing ultra-cold clocks constructed from ions.

“The experiments we’ve performed until now have always focused on classical time, disregarding quantum mechanics,” says Pikovsky. “We’ve observed a regime where conventional explanations falter with an ion clock,” he continues.

These clocks consist of thousands of ions cooled to temperatures nearing absolute zero via laser manipulation. At such low temperatures, the quantum state of an ion and its embedded electrons can be precisely controlled through electromagnetic forces. Thus, the ticks of an ion clock are governed by the electrons oscillating between two distinct quantum states.

Since their behavior is dictated by quantum mechanics, these instruments provided an ideal platform for Pikovsky and his colleagues to investigate the interplay between relativistic and quantum phenomena on timekeeping. Pikovski mentions that they’ve identified several scenarios where this blending is evident.

One example arises from the intrinsic fluctuations inherent in quantum physics. Even at ultra-low temperatures, quantum objects cannot be completely static and instead must oscillate, randomly gaining or losing energy. Team calculations indicated that these fluctuations could lead to extended clock time measurements. Although the effect is minute, it is detectable in current ion clock experiments.

The researchers also mathematically analyzed the behavior of ions in a clock when “compressed,” resulting in “superpositions” of multiple quantum states. They found that these states are closely linked to the motion of the ions, influenced by their internal electrons. The states of ions and electrons are interconnected at a quantum level. “Typically, experiments necessitate creative methods to establish entanglements. The intriguing aspect here is that it arises organically,” explains team member Christian Sanner from Colorado State University.

Pikovski asserts that it is intuitive to think that quantum objects existing in superposition cannot simply perceive time linearly, though this effect has yet to be experimentally confirmed. He believes it should be achievable in the near future.

Team member Gabriel Solch from the Stevens Institute of Technology mentions that the next step is incorporating another crucial aspect of modern physics: gravity. Ultra-cold clocks can currently detect temporal extensions caused by significant variations in the Earth’s gravitational pull, such as when elevated by a few millimeters, but the exact integration of these effects with the intrinsic quantum characteristics of the clock remains an unresolved question.

“I believe it is quite feasible with our existing technology,” adds David Hume from the U.S. National Institute of Standards and Technology, Colorado. He highlights that the primary challenge is to mitigate ambient disturbances affecting the clock to ensure it doesn’t overshadow the effects suggested by Pikovsky’s team. Successful experiments could pave the way for exploring unprecedented physical phenomena.

“Such experiments are thrilling because they create a platform for theories to interact in a domain where they could yield fresh insights,” remarks Alexander Smith at St. Anselm College, New Hampshire.

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Source: www.newscientist.com

New Tektite Discovery Sheds Light on 11-Million-Year-Old Asteroid Impact in Australia

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Tektite forms almost pure glass (with minimal crystalline inclusions) when space debris impacts the Earth, causing surface materials to melt and be ejected hundreds or thousands of kilometers away.

Map of Ananguite strown field based on Tektite location. Image credit: Musolino et al. , doi: 10.1016/j.epsl.2025.119600.

“Tektite is a specific type of glass formed by impacts, recognized particularly for its distribution across extensive spray fields far from the source crater,” stated Professor Fred Jordan from Curtin University and his team.

“The widespread distribution in Central Europe (14 million years ago), North America (35 million years ago), the Ivory Coast (1 million years ago), and from China to Australia (780,000 years ago) has been traced back to the spread originating from Central Europe, known for four distinct scattered fields located in Central America (800,000 years ago).

“The corresponding tektites include Moldavites, Bediasite-Georgiaite, Ivorites, Australiasites, and Belizites, respectively.”

A newly identified type of Tektite, called Ananguite, has been found primarily in South Australia.

“Discovering a new Tektite field is akin to opening a new chapter in Earth’s tumultuous geological history,” remarked Professor Jourdan.

“These glasses are indigenous to Australia and reveal ancient impact events previously unknown to us.”

“Each piece acts as a small time capsule from the depths of our planet’s history.”

“What adds intrigue to these findings is that, despite the considerable impact, the crater has yet to be located.”

“Understanding when and how frequently large asteroids strike Earth can also assist in evaluating the risk of future impacts, which is vital for planetary defense.”

Photos of six Tektites studied by Musolino et al. Scale bar – 2 mm. Image credit: Musolino et al. , doi: 10.1016/j.epsl.2025.119600.

“The glasses differ from all previously known tektites,” noted PhD candidate Annam Solino from AIX-Marseille University.

“These tektites are distinct due to their unusual chemistry and an approximate age of 11 million years.”

“They indicate a shock event that is completely separate from the fields associated with well-known Australian tektites.”

“While Australian tektites formed roughly 780,000 years ago and have spread across the globe, these tektites are significantly older and suggest major impacts that were previously overlooked.”

The team’s research paper was published in the journal Earth and Planetary Science Letters.

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Anna Musolino et al. 2025. Australia’s new tektite spray field dates back 11 million years, originating from a volcanic arc impact crater. Earth and Planetary Science Letters 670:119600; doi:10.1016/j.epsl.2025.119600

Source: www.sci.news

Ancient Protein Analysis Sheds New Light on the Rhino Family Tree

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Paleontologists have extracted ancient enamel protein sequences from fossilized teeth of epiacaratherium sp., a nasal bacteria that thrived in the High Arctic of Canada between 240 and 21 million years ago (early Miocene). This recovered sequence enabled researchers to ascertain that this ancient rhino diverged from other syoxidants during the mid-Eocene Oligocene period, approximately 410-250,000 years ago. Additionally, the findings illuminate the distinctions between two principal subfamilies of rhinocerotinae and Rhinocerotinae, indicating a more recent division of bone development around 340-22 million years ago.

Reconstruction of three extinct rhinoceros species: foreground features a Siberian unicorn (Elasmotherium sibiricum), accompanied by two Merck rhinos (Stephanorhinus kirchbergensis); In the distant background is a wooly rhino (Coelodonta antiquitatis). Image credit: Beth Zaiken.

Dr. Mark Dickinson and his team from York University investigated the teeth of epiacaratherium sp. They utilized a method known as chiral amino acid analysis, which aids in understanding how these proteins were preserved over time.

By assessing the degree of proteolysis and comparing it with previously studied rhino material, they confirmed that the amino acids originated from the teeth themselves, not from subsequent contamination.

“It’s astounding that these techniques allow us to revisit the past and delve deeper,” Dr. Dickinson remarked.

“Armed with our understanding of ancient proteins, we can now pose intriguing new questions regarding the evolution of ancient life on Earth.”

The rhinoceros holds particular significance as it is currently categorized as an endangered species. Exploring its extensive evolutionary history offers vital insights into how past environmental shifts and extinctions have influenced present biodiversity.

Historically, scientists have depended on the morphology of fossils or, more recently, ancient DNA (aDNA) to reconstruct the evolutionary narratives of long-extinct species.

Nonetheless, aDNA typically does not last more than a million years, constraining its utility in unraveling deep evolutionary history.

Although ancient proteins have been detected in Miocene fossils, previous samples extending back over 4 million years had been constrained to roughly the last 10 million years—full sequences were necessary for robust reconstructions of evolutionary lineages.

The latest research significantly broadens this temporal scope, indicating that proteins may endure across extensive geological timescales under optimal conditions.

“Success in analyzing ancient proteins from such old specimens provides fresh perspectives for scientists globally, who possess remarkable fossils in their collections,” stated Dr. Fazeera Munier of York University.

“This crucial fossil aids our understanding of the distant past.”

The results were published in the journal Nature this week.

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RS Patterson et al. Phylogenetically significant proteins from the early Miocene era. Nature Published online on July 9, 2025. doi:10.1038/s41586-025-09231-4

Source: www.sci.news

Webb Sheds New Light on the Structural Evolution of Disk Galaxies

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Modern disk galaxies frequently display distinct thin and thick disks. The mechanisms driving the formation of these two discs and the timeline of their emergence are still unanswered questions. To investigate these issues, astronomers examined various epochs (statistical samples of 111 edge-on disk galaxies dating back up to 11 billion years, or approximately 2.8 billion years post-Big Bang) utilizing archived data from the NASA/ESA/CSA James Webb Space Telescope.

Webb/nircam composite images of a quarter of the team’s samples were sorted by increasing redshift. Image credit: Tsukui et al., doi: 10.1093/mnras/staf604.

Present-day disk galaxies often comprise extensive, star-rich outer disks alongside thin, star-like disks.

For instance, the thick discs of the Milky Way reach approximately 3,000 light-years in height, while the thin discs are roughly 1,000 light-years thick.

But what mechanisms lead to the formation of this dual disk structure?

“The thickness of high redshift discs, or unique measurements from the early universe, serve as benchmarks for theoretical research that can only be conducted using Webb,” states Takagi, an astronomer at the Australian National University.

“Typically, older, thicker disk stars are dim, while the younger, thinner disk stars dominate the galaxy.”

“However, Webb’s exceptional resolution allows us to observe and highlight faint older stars, enabling us to distinguish between two disk structures in a galaxy and measure their thickness separately.”

Through an analysis of 111 edge-on targets over cosmological time, astronomers studied both single-disc and double-disc galaxies.

The findings indicate that galaxies initially form a thick disk, which is followed by the formation of a thin disk.

The timing of this process is contingent on the galaxy’s mass: high-mass, single-disk galaxies transitioned to two-disk structures around 8 billion years ago.

In contrast, a thin disk emerged about 4 billion years ago within low-mass, single-disk galaxies.

“This is the first time we’ve resolved a thin star disk at such a high redshift,” remarked Dr. Emily Wysnioski from the Australian National University.

“The novelty becomes evident when observing the onset of thin star disks.”

“It was astonishing to witness a thin star disk from 8 billion years ago, and even further back.”

To elucidate the transition from a single thick disk to a dual-disk structure, as well as the timing differences between high-mass and low-mass galaxies, researchers expanded their investigation beyond the initial edge-on-galaxy samples. They examined data showing the movement of gases from large millimeter/sub-millimeter arrays (ALMAs) in Atacama and ground surveys.

By considering the movement of the galaxy’s gas disks, they found their results aligned with the “turbulent gas disk” scenario.

In this framework, the turbulent gas disks of the early universe catalyze intense star formation, leading to the creation of thick star disks.

As stars form, they stabilize the gas disks, diminishing turbulence and consequently resulting in thinner disks.

Larger galaxies can convert gas into stars more efficiently and thus calm down more quickly than their lower-mass counterparts, leading to the formation of the earlier thin disk.

“This study delineates structural differences between thin and thick discs, but we aim to explore further,” Dr. Tsukui mentioned.

“We look to incorporate the types of information typically acquired from nearby galaxies, such as stellar movement, age, and metallicity.”

“By doing so, we can bridge insights from both nearby and distant galaxies, enhancing our understanding of disk formation.”

Survey results were published in Monthly Notices of the Royal Astronomical Society.

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Takagi Tsukui et al. 2025. The emergence of thin and thick discs of galaxies across the history of the universe. mnras 540(4): 3493-3522; doi: 10.1093/mnras/staf604

Source: www.sci.news

Hubble sheds light on atmospheric composition and dynamics of Uranus

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The 20-year Hubble study of Uranus provides valuable data to help you understand the atmospheric dynamics of this distant ice giant. This serves as a proxy for studying the deformation of similar sizes and compositions.

The image sequence shows changes in Uranus over the past four years when Hubble’s STIS instrument observed Uranus over 20 years. Over that period, astronomers saw Uranus season as the Antarctic region (left) entered winter shadows, and the Arctic region (right) brightened, and began to become more direct view as summer approached the north. The top row of visible light shows how Uranus’ colours look to the human eye, as can be seen by even amateur telescopes. In the second line, false-colored images of the planet are assembled from visible and near-infrared light observations. The color and brightness correspond to the amount of methane and aerosol. Both of these quantities were indistinguishable before STI first targeted Uranus in 2002. Generally, the green area has less methane than the blue area, and the red area does not show methane. The red area is in the limbs, where the stratosphere of Uranus is almost completely free of methane. The two bottom rows show the latitudinal structures of aerosols and methane, inferred from those visible from 1,000 different wavelengths (colors) to near-infrared. In the third row, bright areas show cloudy conditions, while dark areas show clearer conditions. In the fourth row, the bright areas show depleted methane, and the dark areas show the total amount of methane. At mid- and low-latitude latitudes, aerosol and methane depletion has a unique latitude structure that has changed little over 20 years of observation. However, in polar regions, aerosol and methane depletion behave very differently. In the third row, aerosols near the Arctic show a dramatic increase, becoming very dark in the early days of the Northern Spring and very bright in recent years. It appears that aerosols also disappear in their left limbs when solar radiation disappears. This is evidence that solar radiation alters aerosol haze in Uranus’s atmosphere. On the other hand, methane depletion appears to remain very high in both polar regions throughout the observation period. Image credits: NASA/ESA/Erich Karkoschka, LPL.

Uranus is a giant ice planet about four times the diameter of Earth.

It has a hydrogen and helium feel and has a bit of methane that gives it a blue tint.

Uranus lies to its side and rotates, its magnetic field is biased – it tilts at the center 60 degrees from its axis.

When Voyager 2 passed Uranus in 1986, it provided a close-up snapshot of the planet facing sideways. What it saw resembled a bland blue-green billiard ball.

In comparison, Hubble recorded the story of 20 years of seasonal changes from 2002 to 2022.

During that period, it was used by a team of astronomers led by Dr. Erich Karkoschka of the University of Arizona and Dr. Larry Slomovsky and Dr. Pat Free of the University of Wisconsin. Hubble Space Telescope Imaging Spectrometer (stis) Draw an accurate picture of Uranus’ atmosphere structure.

Researchers observed Uranus four times in 20 years: 2002, 2012, 2015, and 2022.

They found that unlike gas giants Saturn and Jupiter, methane was not evenly distributed on Uranus.

Instead, it is heavily depleted near the pole. This depletion remained relatively constant for 20 years.

However, the structure of aerosols and hazes changes dramatically, and brightens significantly in the Arctic region as the planet approaches the northern summer solstice in 2030.

Uranus takes Earth age just over 84 years to complete the single orbit of the Sun.

Therefore, for over 20 years, the team has seen the spring almost north to make the Northern Pole shine directly in 2030, before shining the equator of Uranus.

“Hubble’s observations suggest a complex atmospheric circulation pattern for Uranus during this period,” the scientists said.

“The data most sensitive to methane distribution shows polar inundation and upwelling in other regions.”

Source: www.sci.news

New research sheds light on the biological characteristics of megalodon

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Megatooth shark, Otodus Megalodonthe iconic shark is primarily represented by the enormous teeth of the Neogene fossil record, but the lack of well-preserved skeletal hampers an understanding of various aspects of its biology. In the new study, paleontologists reassessed some of their biological properties using a new approach, based on known vertebral specimens. Otodus Megalodon 165 species of extinction and 10 orders of living sharks. Their results show that Otodus Megalodon Their bodies were thin and could have reached about 24.3 m in length.

Otodus Megalodon It was extinct 3.6 million years ago. Image credit: Alex Boersma/PNAS.

Otodus MegalodonIt is also called Carcharocles MegalodonThis is a giant megatooth shark that lived in the oceans of the world from 23 to 3.6 million years ago.

This creature is usually portrayed as a super-sized monster in popular culture, with a recent example of science fiction films.

“Otodus Megalodon A professor, colleagues and colleagues at DePaul University said:

“Several vertebrae, pracoid scales, and tessellated cartilage fragments have also been reported to date.”

“However, the lack of a complete fossil specimen has led to uncertainty regarding the true size of this prehistoric shark.”

In their study, the authors examined incomplete vertebral specimens of Otodus MegalodonIt is composed primarily of trunk vertebrae, 11.1 m from the Miocene of Belgium. It was also a specimen of 165 species of extinction and living Neotheratia sharks.

“Assuming that Otodus Megalodon If there was a body plan that matched the majority of sharks, we determined that their head length and tail length accounted for about 16.6% and 32.6% of the total length, respectively,” they said.

“Because the Belgian specimen is 11.1 m, its head and tail were calculated to be about 1.8 m and 3.6 m in length, respectively, which specifically results in an estimated total length of 16.4 m. Otodus Megalodon Individual. “

“The largest vertebrae in a Belgian specimen is 15.5 cm in diameter, but estimated Otodus Megalodon Vertebrae with a diameter of 23 cm have been reported from Denmark. ”

“If a Danish vertebra represents the largest vertebra in the body, that individual could have measured approximately 24.3 m in length.”

Based on a comparison of their body proportions, they have a body shape Otodus Megalodon It probably looked like a modern lemon shark on the surface (Negaprion Brevillo Stris), has a slender body than the great white sharks of modern times.

They also have huge modern sharks, such as whale sharks.Rhincodon Types) And the shark was exposed (Cetorhinus Maximus), like many other giant aquatic vertebrates like whales, they have slender bodies, as their large stubborn bodies are hydrodynamically inefficient for swimming.

In contrast, dark white sharks that become even more severe as they grow can grow larger, but are not huge (below 7 m) due to hydrodynamic constraints.

“Our new research solidified that idea. Otodus Megalodon “We've been working hard to get the better of our team,” said Phillip Sternes, educator at SeaWorld San Diego.

“What distinguishes our research from all previous papers on body size and shape estimation Otodus Megalodon Jakewood, a doctoral student at Florida Atlantic University, added:

According to the team, it is 24.3 m long. Otodus Megalodon It weighs approximately 94 tons and estimates of cruising speeds of 2.1-3.5 km/h.

“The growth patterns recorded in Belgian vertebral specimens are Otodus Megalodon A newborn about 3.6-3.9 m long was given birth to a newborn, and the embryos were nourished through egg-eating behavior,” the author said.

“A known fossil record with newly inferred additional growth patterns Otodus Megalodon And the white shark lineage supports the idea that the rise of the great white shark likely played a role in the ultimate end mise about five million years ago. Otodus Megalodon For competition. ”

“Many interpretations we have made are still tentative, but they are data-driven and serve as a reasonable reference point for future research into the biology of Otodus MegalodonProfessor Shimada said.

study Published online in the journal Palaeontologia Electronica.

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Shimada Mana et al. 2025. Reassessment of the size, shape, weight, cruising speed and growth parameters of extinct megatooth sharks; Otodus Megalodon (Lamniformes: Otodontidae), and new evolutionary insights into its giants, life history strategies, ecology, and extinction. Palaeontologia Electronica 28(1): A12; doi: 10.26879/1502

Source: www.sci.news

Discovery of new bird fossils from China sheds light on early evolution of avian species

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Paleontologists have excavated fossilized remains of two Jurassic bird species in the area of Zenge County, Fujian Province, southeastern China. These 149 million-year-old fossils exhibit early appearances of highly derived bird characteristics, and together with fossils of another bird from the same region, they have the early origins of the birds and the early Jurassic. It suggests bird radiation.

Baminornis Zhenghensis. Image credit: Chuang Zhao.

“Birds are the most diverse group of terrestrial vertebrates,” says Professor Min Wang. Paleontology and Paleontology of Vertebrates The Chinese Academy of Sciences and colleagues said in a statement.

“Specific macroevolutionary studies suggest that their early diversification dates back to the Jurassic period.”

“However, the earliest evolutionary history of birds has long been obscure by highly fragmented fossil records. Archeopteryx Being the only widely accepted Jurassic bird. ”

“nevertheless Archeopteryx It was closely similar, especially due to its distinctive long reptile tail, as it had feathered wings. This is in stark contrast to the short-tailed morphology of modern and Cretaceous birds. ”

“Recent research questions about Aviaran's status. Archeopteryx classifies it as a deinonychosaurian dinosaur, a sister group of birds. ”

“This raises the question of whether there is a clear record of Jurassic birds.”

In their new study, Professor Wang and co-authors discovered and investigated two early bird fossils that were part of the so-called Zhenghe Biota.

One of these birds named Baminornis Zhenghensis the earliest known short-tailed bird.

“Baminornis Zhenghensis The end of the short tail in a complex bone called Pygostyle is a characteristic that can also be observed in living birds,” the paleontologist said.

“Previously, the oldest record of short-tailed birds was from the early Cretaceous period.”

“Baminornis Zhenghensis It is the only Jurassic and the oldest short-tailed bird ever discovered, pushing back the appearance of this derivative bird's distinctive features for nearly 20 million years. ”

According to the team, Baminornis Zhenghensis It also represents one of the oldest known birds.

“A step back and reconsidering the uncertainty of the phylogenetics Archeopteryx we don’t doubt it Baminornis Zhenghensis said Dr. Zhonghe Zhou of the Institute for Vertebrate Paleontology and Paleontology at the Chinese Academy of Sciences.

The second unnamed bird is represented by a single fossilized fullcula (wishbone).

“Our results support this introduction to Furcula ornithuromorpha a diverse group of Cretaceous birds,” the researchers said.

Team's work It was published in the journal today Nature.

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R. Chen et al. 2025. The first short-tailed bird from the late late Jurassic period in China. Nature 638, 441-448; doi:10.1038/s41586-024-08410-z

Source: www.sci.news

New study sheds light on amino acid metabolism and transport in tea plants

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High concentrations of free amino acids in tea leaves are important for tea’s flavor and health functions, but their biosynthesis, transport and turnover in the tea plant have remained unknown.

A practical model of nitrogen assimilation, amino acid synthesis, transport, and decomposition/recycling in tea plants. Image courtesy of Yu others., doi: 10.1093/hr/uhae060.

“Amino acids are essential for plant growth and have a significant impact on the flavor and health benefits of tea,” Professor Zhao Jian Hunan Agricultural University and colleagues.

“Especially the tea trees Camellia sinensis exhibits a unique amino acid profile that contributes to its distinctive taste and nutritional value.”

“Although the importance of amino acids such as theanine and glutamine (Gln) is known, the detailed dynamics of their synthesis, transport and degradation in tea plants remain unknown.”

“These challenges require intensive research to be carried out to understand the complex metabolic pathways and spatial distribution of amino acids within the tea plant.”

In the study, Professor Zhao and his co-authors analyzed the spatial dynamics of amino acid biosynthesis, transport and turnover in tea plants.

“This study provides a detailed analysis of the metabolic pathways and gene expression that control these processes,” the researchers said.

“By understanding these mechanisms, we hope to improve tea cultivation and enhance the quality of tea beverages.”

“This study revealed that nitrogen assimilation occurs mainly in the roots, where glutamate, theanine and arginine (Arg) are actively synthesized. These amino acids are then transported through the plant’s vascular system.”

“Transcriptome analysis revealed that genes involved in Arg synthesis are highly expressed in roots, whereas genes involved in Arg transport and degradation are expressed in stems and young leaves. This indicates that there is a sophisticated amino acid management system within the plant.”

“One of the key findings is the role of the CsGSIa gene, which is crucial for the synthesis, transport and recycling of amino acids.”

“Overexpression and knockdown experiments of CsGSIa in transgenic tea plants demonstrated significant effects on the levels of Gln and theanine.”

“The study also revealed that Arg, Gln, glutamic acid (Glu), and theanine are the major amino acids transported through xylem sap, facilitating long-distance nitrogen transport from roots to leaves.”

“Our findings provide a detailed map of amino acid metabolism in the tea plant, which is of vital importance for both basic science and applied agricultural practice,” Dr Zhao said.

“Understanding these metabolic pathways opens up new possibilities for breeding tea varieties with enhanced flavor and health benefits.”

The team’s findings have important implications for the tea industry.

“By elucidating the pathway of amino acid metabolism, our study paves the way for the development of tea plants with higher contents of beneficial amino acids, enhancing both flavour and nutritional value,” the researchers said.

“These insights can be applied to breeding programs and cultivation practices to produce superior tea varieties.”

“Furthermore, understanding these metabolic processes can help us develop strategies to improve nitrogen use efficiency, contributing to more sustainable and productive tea farms.”

of study Published in the journal Horticultural Research.

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Shuwei Yu others2024. Analysis of spatial dynamics of biosynthesis, transport and metabolism of major amino acids in tea plants (Camellia sinensis). Horticultural Research 11(5):uhae060; doi:10.1093/hr/uhae060

Source: www.sci.news

New research on Zinc sheds light on the link between loud noise and hearing loss

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Exposure to loud noises, such as at music festivals, can worsen your hearing

Sergei Ilnitsky/EPA-EFE/Shutterstock

Exposure to loud noises can disrupt zinc levels in the inner ear, potentially affecting hearing, a study in mice suggests. Treatments that reduce this could be used to treat or prevent such damage, for example, if taken before a rock concert.

Loud noises can cause cells in the inner ear die. Although it has long been known that this affects hearing, the mechanisms behind it are less clear.

Thanos Tsonopoulos Researchers at the University of Pittsburgh, Pennsylvania, thought it might have something to do with free-moving zinc, which plays an important role in the neurotransmission of our senses.

Most of the zinc in the body is bound to proteins, but the rest acts as communication signals between organs, especially the brain, Tsonopoulos says. The highest concentration of free zinc in the body is in the cochlea, the snail-shaped structure in the inner ear that converts vibrations into electrical signals, which are then interpreted as sound.

To learn more, Tzounopoulos and colleagues tested free zinc levels in young mice that had been genetically engineered to produce biological markers that indicate the transport of free zinc throughout the body.

Tsonopoulos said mice exposed to 100 decibels of noise, about the same level as a bulldozer or motorcycle, for two hours straight developed significant hearing loss within the next 24 hours.

The researchers found that these mice had higher amounts of free zinc between and around the cells of the cochlea after the blast compared to before the blast and compared to a group of control mice that did not hear the loud noise. I discovered that

“There is a very strong upregulation of zinc, not only in terms of quantity but also in terms of regional spatial extent,” he says. “It goes everywhere.”

Tsonopoulos said the zinc appears to be released from specific cells in the cochlea after it is separated from the proteins to which it is normally bound. Free zinc ultimately causes cell damage and disrupts normal communication between cells, he says.

To see if lowering free zinc levels could protect hearing, Tsonopoulos and his team injected another group of mice with a compound that scavenged zinc into their abdomens or administered a slow-release drug into the inner ear. It was treated by placing an implant. The mice then listened to the same loud sound for two hours. Both groups experienced significant reductions in hearing loss.

With further research, zinc-capturing tablets, IV drugs, or slow-release implants could one day help prevent or treat inner ear damage caused by noise trauma, Tsonopoulos says.

“You can go to concerts, you can go to battle, you can take drugs,” he says. “Or, if you have an accident, you might have these compounds in your ER. [emergency room] We will give it to you to reduce the damage. ”

Future research should also determine how long after exposure to noise people can benefit from such zinc trap therapy, team members say. Amantha Satyaalso at the University of Pittsburgh.

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Source: www.newscientist.com

New study sheds light on the visual masking phenomenon, unraveling the mystery of “invisibility”

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A new study has revealed how visual masking, a phenomenon in which rapid succession of images leads to unconscious image processing, occurs in both humans and mice. This study highlights the role of the cortex in conscious perception and provides important insights into the brain’s visual processing mechanisms.

Delve into the mysterious optical illusions and science of visual masking.

Recent research published in natural neuroscience Visual masking is a phenomenon that plays an important role in how we perceive things, or rather how we don’t “see” them. This study not only revealed aspects of conscious perception in the brain, but also demonstrated that this phenomenon occurs in both humans and mice.

Visual masking occurs when a person does not consciously recognize an image because another image is displayed in rapid succession. For effective masking, the first image must appear and disappear quickly, followed by her second image within about 50 milliseconds.

Groundbreaking research in visual perception

Allen Institute researcher Dr. Sean Olsen and his colleagues have delved into the science behind this optical illusion and shown for the first time that it also occurs in mice. After training the mice to report what they saw, the researchers were also able to pinpoint the specific areas of the brain needed for the visual masking illusion to work.

“This is an interesting observation, that what exists in the world is not accurately reflected in your perception,” Olsen said. “Like other optical illusions, we think this tells us something about how the visual system works and, ultimately, the neural circuits underlying visual perception.”

Exploring the brain’s role in visual recognition

Scientists discovered this strange phenomenon in the 19th century, but why and how the human brain does this remains a mystery.

The study narrows down the parts of the brain involved in perceiving the world around us, said Dr. Christoph Koch, a Distinguished Fellow at the Allen Institute who led the study with Dr. Olsen and Dr. Sam Gale. Ta. , a scientist at the Allen Institute.

When a rain of photons hits our retina, the information follows a predetermined path from the eyeball through several different areas of the brain and into the highly-processed areas of the cortex, the wrinkled outermost shell of the brain. It ends with Previous research on visual masking has led scientists to believe that neurons in early parts of the brain, in the retina and its pathways, are activated even when a person is unaware that they are looking at an image. I know. In other words, your brain sees things without your knowledge.

From mouse to human: parallel recognition

To explore where unconscious sensations turn into conscious perceptions and actions, scientists first taught 16 mice to move a small mouse in the direction of a rapidly flashing image in exchange for a reward if they chose the correct direction. I trained him to spin a Lego wheel. The scientists then added different masking images on either side of the screen immediately after the target image. Adding a mask prevented the animal from performing the task correctly. This means that the animal can no longer recognize the original target image.

Visual masking had never been tested in mice before, so the research team had to create a task for mice, in which the images and the way they were displayed were different from those used in previous human studies. I meant that. To confirm that the optical illusion they showed to rodents was also relevant to us, the research team tested it on 16 people (using keystrokes instead of a wheel). It turns out that human perception (or lack thereof) and mouse perception of this particular visual masking illusion are very similar.

This result implies that conscious perception is occurring in the visual cortex or in higher regions of the cortex downstream. This is consistent with the general sentiment in the field that the cortex is the seat of conscious cognition in mammals, including us, Koch said.

Reference: “Visual cortex is required for posterior masking in mice” by Samuel D. Gale, Chelsea Stroder, Corbett Bennett, Stefan Mihalas, Christoph Koch, and Sean R. Olsen, November 13, 2023 Day, natural neuroscience.
DOI: 10.1038/s41593-023-01488-0

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Active Matter Theory sheds new light on longstanding biological enigmas

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November 22, 2023A team of scientists has developed a new algorithm to solve theoretical equations for active materials, deepening our understanding of living materials. This research is of vital importance in biology and computational science, paving the way for new discoveries in cell morphology and the creation of artificial biological machines. Advanced open-source supercomputer algorithms predict the patterns and dynamics of living matter and enable exploration of its behavior across space and time. Biological materials are made up of individual components, such as tiny motors that convert fuel into motion. This process creates a pattern of movement, guiding the shape of the material itself through a consistent flow driven by constant energy consumption. Such permanently driven substances are called “active substances.”

How cells and tissues work can be explained by active matter theory, a scientific framework for understanding the shape, flow, and form of living matter. Active matter theory consists of many difficult mathematical equations. Scientists from Dresden’s Max Planck Institute for Molecular Cell Biology and Genetics (MPI-CBG), the Dresden Center for Systems Biology (CSBD), and the Dresden University of Technology have developed an algorithm implemented in open-source supercomputer code. For the first time, you can solve active matter theory equations in realistic scenarios. These solutions bring him a big step closer to solving his century-old mystery of how cells and tissues acquire their shape, and to designing artificial biological machines. 3D simulation of active substances in a dividing cell-like geometry. Credit: Singh et al. Physics of Fluids (2023) / MPI-CBG

Biological processes and behaviors are often highly complex. Physical theory provides a precise and quantitative framework for understanding physical theories. Active matter theory provides a framework for understanding and explaining the behavior of active substances, which are materials made up of individual components that can convert chemical fuels (“food”) into mechanical forces. The development of this theory was led by several Dresden scientists, including Frank Uricher, director of the Max Planck Institute for Complex Systems Physics, and Stefan Grill, director of MPI-CBG. These physical principles allow us to mathematically describe and predict the dynamics of active organisms. However, these equations are very complex and difficult to solve. Therefore, scientists need the power of supercomputers to understand and analyze living matter. There are various ways to predict the behavior of active materials, including by focusing on small individual particles, by studying active materials at the molecular level, and by studying active fluids on a larger scale. These studies help scientists understand how active substances behave at different scales in space and time. Scientist in the research group of Dresden University of Technology Ivo Sbalzarini Professor at the Dresden Center for Systems Biology (CSBD), research group leader at the Max Planck Institute molecular cell The Dean of the Department of Biology and Genetics (MPI-CBG) and Computer Science at the Technical University of Dresden has now developed a computer algorithm to solve the active substance equation. Their research was published in the journal fluid physics and it appeared on the cover. They present an algorithm that is capable of solving complex equations for active materials in three-dimensional and complex-shaped spaces.

“Our approach can handle a variety of shapes in three dimensions over time,” says research mathematician Abhinav Singh, one of the study’s first authors. He continued, “Even when the data points are not regularly distributed, our algorithm employs a novel numerical approach that works seamlessly for complex biologically realistic scenarios, and the theoretical equations Using our approach, we can finally understand the long-term behavior of active materials in both mobile and non-mobile scenarios in order to predict dynamic scenarios. Additionally, theory and simulation can be used to program biological materials and create engines at the nanoscale to extract useful work.” The other first author, Philipp Suhrcke, holds a master’s degree in computational modeling and simulation from the Technical University of Dresden. “Thanks to our research, scientists can predict, for example, the shape of tissues and when biological materials will become unstable or dysregulated, leading to growth and disease. This has far-reaching implications for our understanding of mechanisms.”

The scientists implemented the software using the open source library OpenFPM. This means that others can use it freely. OpenFPM was developed by his Sbalzarini group to democratize large-scale scientific and technical computing. The authors first developed a custom computer language that allows computational scientists to write code for a supercomputer by specifying mathematical formulas that let the computer do the work of writing the correct program code. As a result, you no longer have to start from scratch every time you write code, effectively reducing code development time in scientific research from months or years to days or weeks, greatly increasing productivity.

Because the study of three-dimensional active materials has significant computational demands, using OpenFPM the new code is scalable on shared and distributed memory multiprocessor parallel supercomputers. This application is designed to run on powerful supercomputers, but can also be run on regular office computers to study 2D materials. Ivo Sbalzarini, the study’s lead researcher, summarizes: All this has been integrated into a tool for understanding her three-dimensional behavior of living matter. Our code, which is open source, scalable, and able to handle complex scenarios, opens new avenues in active materials modeling. This could ultimately lead to an understanding of how cells and tissues acquire their shape, addressing fundamental questions in morphogenesis that have puzzled scientists for centuries. There is a gender. But it may also be useful for designing artificial biological machines with minimal components.

References: “Numerical solver for three-dimensional active fluid dynamics and its application to active turbulence” by Abhinav Singh, Philipp H. Suhrcke, Pietro Incardina, and Ivo F. Sbalzarini, October 30, 2023. fluid physics. DOI: 10.1063/5.0169546 This research was funded by the Federal Ministry of Education and Research (Bundesministerium f€ur Bildung und Forschung, BMBF), the Federal Center for Scalable Data Analysis and Artificial Intelligence, ScaDS.AI, and Dresden/Leipzig. The computer code supporting the results of this study is publicly available in the 3Dactive-hydynamics github repository at: https://github.com/mosaic-group/3Dactive-hydrodynamic sThe open source framework OpenFPM is available at: https://github.com/mosaic-group/openfpm_pdataRelated publications for embedded computer languages https://doi.org/10.1016/j.cpc.2019.03.007https://doi.org/10.1140/epje/s10189-021-00121-x (function (d, s, id) {var js, fjs = d.getElementsByTagName (s) [0]; if (d.getElementById (id)) return; js = d.createElement (s); js.id = id; js.src = “https://connect.facebook.net/en_US/sdk.js#xfbml=1&version=v2.6”; fjs.parentNode.insertBefore (js, fjs); } (document, ‘script’, ‘facebook-jssdk’));

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