The dinosaur history of Wales illuminated by 205-million-year-old bone bed

The recently discovered Late Triassic bonebed at Labanock in South Wales is a storm deposit that preserves a rich coastal marine biota, including a diverse range of fish and marine reptiles.



A view of the cliff face at Labanock Point from the eastern end of the beach shows how the red mudstones of the Williton Member (Marcia Mudstone Formation) transition upward into the bedded shales of the Westbury Formation. Image courtesy of Evans others., doi: 10.1016/j.pgeola.2024.05.001.

“The new bone beds paint a picture of a tropical island that was frequently battered by storms, washing material from the surrounding areas on land and at sea into the tidal zone,” said paleontologist Owain Evans from the University of Bristol.

“This means that from just one fossil bed, we can reconstruct a complex ecosystem containing a wide variety of marine reptiles, such as underwater ichthyosaurs, plesiosaurs, and placodonts, as well as land-based dinosaurs.”

The discovery was made at Labanock Head, near Cardiff and Penarth in South Wales, where dark shale and limestone cliffs reveal an ancient, shallow sea.

Several layers contain deposits of bones, including the remains of fish, sharks, marine reptiles, and occasionally dinosaurs.

“I grew up in Cardiff and have been visiting Penarth beach all my life but I'd never noticed any fossils,” Ms Evans said.

“And the more I read, the more amazing it became.”

“Local geologists have been collecting the bones since the 1870s, and most of them are in the National Museum of Wales in Cardiff.”

“The Labanock collection dates back to the 19th century and many parts of the bone bed have been collected over many years,” said Dr. Cindy Howells, curator of palaeontology at the National Museum Wales.

“The presence of dinosaur remains at the site ensures that it will remain one of the most important sites for palaeontology in Wales.”

The paleontologists also unearthed the remains of a placodont osteoderm and a coelacanth throat bone.

“Coelacanth and other placodont fossils are relatively rare in the UK, which makes this find all the more remarkable,” said Dr. Chris Duffin, a palaeontologist at the University of Bristol and the Natural History Museum in London.

“Just these two fossils alone, Rhaetian What would it have been like in England?”

“The amount of dinosaur fossils found at Labanoc is extremely exciting and provides an opportunity to study a complex and often mysterious period in dinosaur evolutionary history,” said Professor Michael Benton, from the University of Bristol.

“We are a big Plateosaurus “Similar animals and several other bones possibly belonging to a predatory theropod were found.”

of Investigation result Appears in Proceedings of the Association of Geologists.

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Owain Evans othersA microvertebrate from the basal Rhaetian bone bed (Late Triassic) at Lavanock, South Wales. Proceedings of the Association of GeologistsPublished online May 23, 2024; doi: 10.1016/j.pgeola.2024.05.001

Source: www.sci.news

Research reveals crows can distinguish up to four sounds.

Carrion crow (Crow) It can count up to four times based on visual and auditory cues and control the number of times it vocalizes. study Published in the journal Science.

Carrion crow (Crow). Image courtesy of Andreas Nieder.

Counting out loud (e.g., reciting 1, 2, 3, etc.) requires an understanding of quantity and controlled, purposeful vocalization.

Humans use language to count and communicate quantity symbolically, which is a complex skill developed during childhood.

Before acquiring symbolic counting, where specific words are associated with specific quantities, infants produce several sounds that correspond to the quantities of objects they see and use these sounds as acoustic counting to communicate the corresponding numbers.

This early human behavior reflects a non-symbolic capacity shared with animals.

Some animals have demonstrated the ability to distinguish between different numbers of objects and communicate information through different numbers of vocalizations.

However, it is unclear whether animals other than humans have the ability to count by intentionally making a specific number of vocalizations.

“The carrion crow, a member of the songbird group, is known not for the beauty of its song but for its incredible learning ability,” Professor Andreas Nieder, researcher University of Tübingen.

“For example, previous studies have shown that birds understand counting.”

“Plus, they have incredible vocal control. They can control exactly whether or not they're going to chirp.”

In this study, Professor Nieder and his co-authors investigated whether carrion crows can control the rate at which they vocalize and solve complex vocal response tasks.

The researchers trained three crows to produce one to four vocalizations in response to both visual (colored numbers) and auditory (distinct sounds) cues associated with numerical values.

On each trial, birds were required to produce a target number of vocalizations and indicate the end of the vocalization sequence by pecking the target.

The researchers found that crows can successfully and purposefully produce a specific number of vocalizations in response to specific cues, a level of control that has not yet been observed in other animals.

The birds used a non-symbolic approximate number system and planned the number of vocalizations before initiating them.

Further analysis showed that the timing and characteristics of the first vocalization predicted the number of subsequent vocalizations, and different acoustic features of the vocalizations indicated their number in a given sequence.

“Our results show that humans are not the only ones who can do this,” Professor Nieder said.

“In principle, this could enable advanced communication with crows.”

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Diana A. Liao othersThe year is 2024. Crows “count” the number of cries they make. Science 384(6698):874-877; doi:10.1126/science.adl0984

Source: www.sci.news

New research reveals insights into childhood stress in Neanderthals and Paleolithic humans

Neanderthal life has been portrayed as historically highly stressful, shaped by constant pressure to survive in harsh ecological conditions, which may have contributed to their extinction. In a new study, paleoanthropologists analyzed the frequency of dental enamel hypoplasia, an indicator of growth impairment due to early life stress, in the largest sample of Neanderthals and Upper Paleolithic humans. Their findings support similar overall stress levels in both groups, but show that there are species-specific patterns in the distribution of its occurrence. They found that the likelihood of growth impairment increased during the weaning process in Neanderthal children and culminated in intensity after weaning, whereas growth impairment in Upper Paleolithic children was limited to the time of weaning and significantly decreased after its expected completion. These results may reflect differences in parenting and other behavioral strategies between the two species, including some that may be advantageous for long-term survival in modern humans.

Neanderthal family. Image courtesy of the Field Museum.

“Neanderthals have traditionally been depicted as living highly stressful lives, including pressures to survive in the harsh and highly variable ecological conditions of Pleistocene Eurasia, which have been thought to have contributed to their extinction,” said Dr Laura Rimmer from the University of Tübingen and her colleagues.

“Modern Upper Paleolithic humans faced similar environmental conditions, but it is generally assumed that they were better equipped to buffer such pressures through their behavioral repertoire.”

“This includes strategies such as greater flexibility and efficiency in resource use and more complex social organisation and networks.”

“Their behavioral repertoire is thought to have given modern humans a competitive advantage over Neanderthals during the Upper Paleolithic, allowing them to survive while Neanderthals became extinct.”

“However, several recent studies have cast doubt on this view, arguing that Neanderthals and modern Upper Paleolithic humans lived similarly stressful lives.”

For the study, the researchers analyzed the enamel of 423 Neanderthal teeth and 444 Upper Paleolithic human teeth.

The researchers investigated early life stress in these individuals by identifying thin horizontal grooves in the enamel that previous studies have demonstrated are associated with early life stressors such as illness, infection, malnutrition, nutritional deficiencies and trauma.

The researchers found that the overall likelihood of enamel defects was similar in the teeth of Neanderthals and modern Upper Paleolithic humans.

“However, we observed that the distribution of dental enamel defects varied across developmental stages: in modern humans, enamel defects were more likely to occur around the time of weaning,” Dr Rimmer said.

In Upper Paleolithic humans, enamel defects were more likely to occur around the age when weaning was estimated to have occurred (between 1 and 3 years) than after the estimated weaning period.

In Neanderthals, enamel defects began to appear during weaning (around 1 year of age), peaked during late weaning (between 2 and 4 years of age), and then tended to decrease.

Scientists hypothesize that the stress experienced by Upper Paleolithic human children during weaning may have been due to increased energy demands that increased their risk of malnutrition.

They propose that Late Paleolithic humans may have helped to reduce developmental stress in their offspring after weaning through strategies such as encouraging long-term dependency on parents, using resources more efficiently and providing offspring with access to food.

They suggest that these strategies may not have been used by Neanderthals, which may have contributed to the long-term survival advantage of modern humans compared to Neanderthals.

“Modern humans may have gained an advantage over Neanderthals by providing better support for their young during these difficult times, such as by protecting them for longer or by providing a better food supply,” said Dr Shireen El-Zaatari, a researcher at the University of Tübingen.

“Neanderthals lived in a particularly cold and harsh climate, which is often said to have led to their extinction.”

“But because over a period of time Neanderthals and modern humans were exposed to the same climatic conditions, we are investigating other explanations.”

of study Published in a journal Scientific Reports.

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LS Rimmer others2024. Differences in childhood stress between Neanderthals and early modern humans reflected in impaired dental enamel growth. Scientific Reports 14, 11293; doi: 10.1038/s41598-024-61321-x

Source: www.sci.news

Scientists say orange peel could be a crucial factor in enhancing cardiovascular health

A study by researchers from the University of Florida, Texas State University, and the United States Department of Agriculture suggests that an extract of the polar fraction of orange peel, which contains a compound called feruloylputrescine, may reduce cardiovascular disease.

Lee othersThe inhibitory effects of orange peel polar fraction (OPP) and orange peel non-polar fraction (OPNP) on the production of trimethylamine (TMA) and trimethylamine N-oxide (TMAO) in response to L-carnitine treatment were compared. In vivo and In vitro.

Recent studies have shown that some gut bacteria may contribute to the development of cardiovascular disease.

During digestion, gut bacteria produce trimethylamine N-oxide (TMAO) when certain nutrients are ingested, and levels of TMAO can help predict future cardiovascular disease.

In a new study, Dr. Yu Wang from the University of Florida and colleagues investigated the potential of orange peel extract to reduce the production of TMAO and trimethylamine (TMA).

They tested two types of extracts: a polar fraction and a non-polar fraction.

To obtain the polar fraction, they extracted orange peels using polar and non-polar solvents.

“Think of a salad dressing. The things that are in the water and vinegar section are polar compounds. The things that are in the oil section, away from the water, are non-polar compounds,” says Dr. Wang.

“The solvents we used are not exactly the same as water and oil, but they have a similar polarity.”

The authors found that extracts of the non-polar fraction of orange peel effectively inhibited the production of harmful chemicals.

The researchers also identified a compound in the polar fraction extract of orange peel called feruloylputrescine, which also significantly inhibited the enzyme involved in TMA production.

“This is a novel discovery that highlights a previously unrecognized potential health benefit of feruloylputrescine in reducing the risk of cardiovascular disease,” Dr Wang said.

“The discovery regarding orange peel is significant because five million tonnes of orange peel are produced annually in orange juice production nationwide.”

“About 95 percent of Florida oranges are used for juice. About half of the peels are used to feed cows. The rest are discarded.”

“But the FDA considers natural orange peel extract to be safe for human consumption, so we're looking to get more out of the peel.”

“These findings suggest that orange peels, which are often discarded as waste in the citrus industry, could be repurposed into valuable health-promoting compounds, such as ingredients in dietary supplements and foods,” Dr Wang said.

“Our study paves the way for the development of functional foods enriched with these bioactive compounds, providing a new therapeutic strategy for heart health.”

of result Appears in Journal of Agricultural and Food Chemistry.

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Hana Lee others2024. Discovery of novel bioactive compounds from the polar fraction of orange peel and their inhibition of trimethylamine and trimethylamine N-oxide by a metabolomic approach. In vitro and In vivo Assay: Feruloylputrescine inhibits trimethylamine by suppressing the cntA/B enzymes. Journal of Agricultural and Food Chemistry 72(14):7870-7881; doi:10.1021/acs.jafc.3c09005

Source: www.sci.news

Webb focuses on irregular galaxy NGC 4449

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have captured stunning new photos of NGC 4449, located in the constellation Canes Venatici.



This Webb/MIRI/NIRCam image shows the center of irregular galaxy NGC 4449. Image credit: NASA / ESA / CSA / Webb / A. Adamo, Stockholm University / FEAST JWST Team.

NGC 4449 It is located about 12.5 million light years away in the constellation Canes Venatici.

Also known as Caldwell 21, LEDA 40973, and UGC 7592, the galaxy has a diameter of about 20,000 light-years.

NGC 4449 discovered It was discovered on April 27, 1788 by German-born British astronomer William Herschel.

It is part of the M94 galaxy group, lie It is near the Local Group that hosts our Milky Way galaxy.

“NGC 4449 has been forming stars for billions of years, but star formation is occurring at a much higher rate today than in the past,” astronomer Webb said.

“Such unusually explosive and intense star formation activity is called a starburst, and NGC 4449 is therefore known as a starburst galaxy.”

“Indeed, at the current rate of star formation, the gas supply required for star formation will last only another billion years or so.”

“Starbursts typically occur in the centres of galaxies, but NGC 4449 shows more widespread star formation activity, with very young stars observed both in the galaxy's core and in the outflow that surrounds it.”

“The current widespread starburst is likely caused by an interaction or merger with a smaller companion star.”

“Indeed, star formation in NGC 4449 is likely influenced by interactions with several nearby stars.”

“NGC 4449 resembles a primitive star-forming galaxy that grew by merging and accreting with smaller stellar systems,” the researchers added.

“NGC 4449 is close enough for us to observe it in great detail, making it an ideal laboratory for studying what happened during the formation and evolution of galaxies in the early universe.”



This Webb/NIRCam image shows the irregular galaxy NGC 4449. Image courtesy of NASA / ESA / CSA / Webb / A. Adamo, Stockholm University / FEAST JWST Team.

NGC 4449 was observed as part of the FEAST (Feedback in Emerging extrAgalactic Star cluSTers) survey.

The image is MIRI on the Web (mid-infrared measuring instrument) and NIR Cam (Near infrared camera) equipment.

“Infrared observations reveal the galaxy's crawling tentacles of gas, dust and stars,” the astronomers said.

“The bright blue dots reveal countless individual stars, while the bright yellow regions spread across the galaxy show concentrated active stellar nurseries where new stars are forming.”

“The orange-red areas show the distribution of a type of carbon-based compound known as polycyclic aromatic hydrocarbons (PAHs). The MIRI F770W filter is particularly well suited to imaging these important molecules.”

“The bright red spots correspond to hydrogen-rich regions that have been ionized by radiation from newly formed stars.”

“The diffuse gradient of blue light around the central region indicates the distribution of old stars.”

“The compact light blue regions within the red ionized gas are concentrated mainly in the outer regions of the galaxy and represent the distribution of young star clusters.”

Source: www.sci.news

Incredible Discovery: Giant Short-Faced Kangaroo Fossil Unearthed in Australia

Palaeontologists from the Victoria Museum Research Institute and other institutions have discovered Cymostenurus occidentalis Fossils of a eastern grey kangaroo, a species of giant short-faced kangaroo that lived in Australia until about 42,000 years ago, have been discovered in Nightshade Cave in Gunaikurnai County, north of the town of Buchan in eastern Victoria, Australia.

Short-faced kangaroo They appear in the Australian fossil record around 10 to 15 million years ago, when tropical rainforests began to give way to drier habitats.” Said Dr Tim Ziegler, Collections Manager at Museum Research Victoria;

“They especially diversified during the Late Pleistocene, about 500,000 years ago, during the transition to our present-day arid climate.”

“But in a wave of extinction around 45,000 years ago, they disappeared from the entire continent, along with up to 85% of Australia's large animals.”

49,400-year-old skeleton of a giant short-faced kangaroo Cymostenurus occidentalis It was discovered in Nightshade Cave in Victoria.

The animal's skull was discovered by a local cave group in 2011, and just 10 years later, the individual's skeleton below the skull was discovered by expert paleontologists.

“The skull had a deep snout, robust jaws and teeth, characteristic of a short-faced kangaroo,” Dr Ziegler explained.

“Behind it there were many more bones. It was amazing to see the vertebrae, shoulders, hips, limbs and thin rib cage. Many of the bones had not been moved at all and were still in their original position. This was one animal, not just bones scattered randomly. It felt like the Holy Grail of fossils.”

Cymostenurus occidentalisImage credit: Nellie Pease / ARC CoE CABAH / CC BY-SA 4.0 Deed.

According to the team, the discovery was made at a young age. Cymostenurus occidentalis.

“This is a further distinction from other species of this animal as it is a juvenile rather than an adult kangaroo,” Dr Ziegler said.

“The teeth had barely worn down, the skull had not yet fused, and the ends of the limbs had not yet joined together.”

“Based on the size of its limbs, we estimate its weight to be around 80 kilograms, which is roughly the weight of an average human. However, as an adult, it may have been half that size.”

The specimen consists of 150 preserved bones and is the most complete fossil skeleton ever found in a Victorian cave.

This fossil, along with others from Nightshade Cave, are now permanently housed and cared for at the Melbourne Museum.

“The skeleton we found has a perfectly intact spinal column, providing new insights that aren't possible from isolated bones,” Dr Ziegler said.

“Thanks to the detailed 3D model, this nearly complete skeleton can be studied from anywhere in the world.”

“A key idea under investigation is whether the Stenulin kangaroo was striding rather than hopping.”

Source: www.sci.news

Study confirms recent volcanic activity on Venus

Using radar data NASA’s Magellan Project Planetary scientists have detected volcano-related flow features in two different regions of Venus: on the western slope of Sif Mons and in western Niobe Planitia.

This image shows the Schiffmons region with active volcanic areas highlighted in red. Image courtesy of Davide Sulcanese, IRSPS – Università d’Annunzio.

Venus’s thick atmosphere makes it difficult to make direct observations of the planet’s surface.

However, although global radar mapping performed by the Magellan spacecraft in the 1990s showed that Venus’s surface is covered with many volcanoes and was likely formed by extensive volcanic activity in the past, the role of volcanism in Venus’s geological present remained unclear.

However, 2023 Magellan data confirmed evidence of more recent activity from one volcanic vent on the planet’s surface.

In the new study, Davide Sulcanese, a researcher at D’Annunzio University, and his colleagues analyzed two sets of Magellan radar data taken in 1990 and 1992 to look for evidence of volcanic activity.

They found surface changes that could indicate volcanic activity in two areas with volcanic-related features: on the western slope of Mount Sif and in western Niobe Planitia.

After analyzing a range of possible causes, the authors suggest that these fluctuations were likely caused by fresh lava flows.

They suggest that not only is Venus currently a geologically active planet, but that volcanic activity is currently quite widespread.

They also suggest that volcanic activity on Venus is comparable to that on Earth, indicating that Venus is more volcanically active than previously thought.

Artist’s impression of an erupting volcano on Venus. Image courtesy of ESA / AOES Medialab.

“These maps suggest that Venus may be much more volcanically active than previously thought,” Dr Sulcanese said.

“Analysis of lava flows observed at two locations on Venus suggests that volcanic activity on Venus may rival that on Earth.”

“We interpret these signals as flows along the slopes and volcanic plains that, like fluids, may bypass obstacles such as shield volcanoes,” added Dr Marco Mastrogiuseppe, a researcher at Sapienza University of Rome.

“After ruling out other possibilities, we determined that the best interpretation is that these are new lava flows.”

“These new findings about Venus’s recent volcanic activity provide compelling evidence for the types of regions NASA’s upcoming VERITAS mission should target when it arrives at Venus,” said Dr. Suzanne Smrekar, a research scientist at NASA’s Jet Propulsion Laboratory and VERITAS principal investigator.

“Our spacecraft has a suite of approaches to identify surface changes with much more comprehensiveness and resolution than Magellan’s images.”

“Finding evidence of activity even in the low-resolution Magellan data has great potential to revolutionize our understanding of this mysterious world.”

of result Published in this week’s journal Natural Astronomy.

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D. Sulcanese othersEvidence of ongoing volcanic activity on Venus revealed by Magellan radar. Nat AstronPublished online May 27, 2024, doi: 10.1038/s41550-024-02272-1

Source: www.sci.news

The long, prehensile tail of the extinct North American porcupine

New World porcupines originated in South America and dispersed into North America between 4 and 3 million years ago. Today, prehensile tail porcupines live in the tropical forests of Central and South America. In contrast, North American porcupine (Erethizon Dorsatum) It is thought to be adapted to temperate forests at higher latitudes, with a larger body, shorter tail, and a diet that includes bark. paper Published in this week's journal Current BiologyPalaeontologists have described functionally important features of the skeleton of an extinct porcupine. Erethizon PoeriThe oldest nearly complete porcupine skeleton recorded in North America, discovered in Florida from the Early Pleistocene.

North American porcupines differ from their southern counterparts in that they have more fur, a shorter tail, and a larger build.

Porcupines are a type of rodent whose ancestors probably originated in Africa more than 30 million years ago.

Their descendants subsequently migrated overland to parts of Asia and Europe, but the journey to South America is a particularly defining event in mammalian history.

They probably crossed the Atlantic Ocean on rafts at a time when Africa and South America were much closer than they are today.

They were the first rodents to set foot on the continent, where they evolved into familiar groups such as guinea pigs, chinchillas, capybaras, and porcupines.

Some were gigantic – lumbering, mouse-like creatures up to five feet long, with tiny brains and weighing less than a plum – and a close relative of the extinct capybara that grew to the size of a cow.

Porcupines have evolved to remain relatively small and adapt to life in the trees of the lush tropical rainforests of South America.

Now they move through the tree canopy using long fingers with blunt, sickle-shaped claws perfectly angled to grip branches.

Many birds have long, prehensile tails that can support their body weight and help them climb trees and pick fruit.

Despite its impressive track record of migration, South America was a dead end for millions of years.

North and South America are separated by a vast ocean passage with rapids, which most animals could not cross, with a few notable exceptions.

Beginning about 5 million years ago, the Isthmus of Panama rose above sea level, separating the Pacific and Atlantic oceans.

Millions of years later, this land bridge would become the equivalent of an ancient, congested highway, allowing traffic to flow in both directions.

Prehistoric elephants, sabre-toothed tigers, jaguars, llamas, peccaries, deer, skunks and bears migrated from North America to South America.

Also joining us on the reverse journey were four species of ground sloths, an oversized armadillo, fearsome birds, capybaras and even marsupials.

The two groups had radically different fates. The mammals that migrated south did relatively well, and many successfully colonized their new tropical environments and have survived to the present day. But the lineages that moved north into colder environments almost entirely went extinct. Only three species remain today: the giant armadillo, the Virginia opossum, and the North American porcupine.

South American porcupines have a formidable coat of hollow, overlapping quills that provide considerable defense but little in the way of thermoregulation.

North American porcupines replaced this with a mixture of insulating hairs and long, needle-like hairs that they erect when they sense danger. They also had to change their diet, which led to a change in the shape of their jaws.

“When their favorite foods disappear in the winter, they'll nibble at tree bark and eat the soft tissue underneath. It's not the tastiest food, but it’s better than nothing,” says Natasha Vitek, a research scientist at the Florida Museum of Natural History.

“This type of feeding appears to have been selected for a particular jaw structure that enhances the ability to grind teeth.”

“They also lost their tails, which they used to prehensile. North American porcupines still love climbing trees, but it’s not their forte.”

“Museum specimens often show signs of healed fractures, likely caused by falls from trees.”

In the new study, Vitek and his colleagues examined an exceptionally well-preserved skeleton of an extinct species of porcupine from Florida, US.

“It's very unusual to find a fossil skeleton like this, which includes not only the skull and jaw, but also many other bones from other parts of the body,” said Dr. Jonathan Block, curator of vertebrate paleontology at the Florida Museum of Natural History.

“This will give us a more complete picture of how extinct mammals interacted with their environment.”

“We quickly realized that it was different from modern North American porcupines in that it had a specialized tail for grasping branches.”

The researchers were confident that by comparing the fossil skeleton with modern porcupine bones they could pinpoint its identity.

“The results were surprising: the fossil lacked the reinforced jaws for gnawing at bark, but had a tail adapted for prehensile functions, making it more similar to South American porcupines,” Vitek said.

“But other features, such as the shape of the middle ear bones and the shape of the lower front and back teeth, bore stronger similarities to North American porcupines.”

When all the data was combined, the analyses consistently gave the same answer.

Fossils Erethizon Poeriis an extinct species of North American porcupine, and this group has a long history that likely began before the formation of the Isthmus of Panama.

But questions remain about how many species in this group once existed and why they became extinct.

“One of the things our study leaves unresolved is whether these extinct species were the direct ancestors of today’s living North American porcupines,” Vitek said.

“It’s possible that porcupines have invaded temperate zones twice — once along the Gulf Coast and once in the West — but we’re not there yet.”

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Natasha S. Vitek othersAn extinct North American porcupine with a South American tail. Current BiologyPublished online May 27, 2024; doi: 10.1016/j.cub.2024.04.069

Source: www.sci.news

Researchers sequence genome of pineapple mint | Sci.News

The researchers: Pineapple Mint (Mint)This herb is highly valued for its unique aroma and medicinal properties.

Pineapple Mint (Mint) is cultivated worldwide for its unique aroma and commercial value. Image credit: Yang others., doi: 10.1093/hr/uhae022.

Genus MintThis plant, known as mint, is a type of herb with a strong scent. Lamiaceae.

This versatile plant contains a variety of components, including essential oils and non-essential compounds, making it suitable for a wide range of uses.

Mint Essential oils have a long history of medicinal use as digestive aids and pain relievers. Essential oils have a wide range of biological activities, including antioxidant, antibacterial, antiradiation, anticancer, and antihypertensive properties.

Pineapple mint is a cultivated variegated variety of apple mint.

It grows as a wild plant all over the world and is widely used in the medical field due to its many therapeutic properties.

“Despite their importance, understanding the genetic basis of these traits remains Mint “This gene is very unique, characterized by high heterozygosity and numerous structural mutations,” said Qi Song, PhD, of Chengdu University of Traditional Chinese Medicine, and his colleagues.

“Comprehensive research Mint “Sequencing the genome was essential to uncover the genetic factors that influence its unique characteristics.”

In this study, the researchers succeeded in generating the first high-quality, haplotyped genome assembly of pineapple mint, with a genome size of 414.3 Mb and 31,251 coding genes.

By integrating data from different sequencing platforms, we resolved two complete haplotype assemblies with nearly complete annotated telomeres and centromeres.

Remarkably, they uncovered 41,135 structural variations, including deletions, insertions, duplications, and translocations, many of which affect genes involved in terpenoid biosynthesis.

One important finding is that piperitenone oxide dominates among the volatile compounds produced by pineapple mint, in contrast to menthol, which is more common in other plants. Mint seed.

The authors identified three genes. Isopiperitenone reductase We identified ISPR, a key enzyme in menthol biosynthesis, but found that its low transcription level likely led to the accumulation of piperitenone oxide instead.

“The completion of the gap-free genome Mint “This is an important milestone in plant genomics,” Dr. Song said.

“This comprehensive genetic map provides a basis for investigating the molecular mechanisms underlying pineapple mint's unique properties, which may lead to innovative applications in medicine and agriculture.”

of result Published in the journal Horticultural Research.

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Hanting Yang others2024. Haplotyped gap-free genome assembly provides new insights into monoterpenoid diversification. Mint “Variegata”. Horticultural Research 11(3):uhae022; doi:10.1093/hr/uhae022

Source: www.sci.news

Scientists Successfully Sequence Genome of Extinct Little Bushmower

Scientists at Harvard University and elsewhere have used ancient DNA recovered from fossil bones on New Zealand’s South Island to identify the tiny bushmower.Anomalopteryx didiformisIt is one of nine species of flightless birds that once roamed the forested islands of New Zealand.

Moas fed on trees and shrubs in the forest understory. Image by Heinrich Harder.

There are currently nine recognized species of extinct New Zealand moas, which belong to the infraclass Aves. PaleognathomorphaThese include flightless ratites (ostriches, emus, cassowaries, kiwis, rheas, moas and elephant birds) and flying shorebirds and skylarks.

The extinction of all moa species is thought to have occurred shortly after Polynesian migration to New Zealand in the 13th century, and is the result of direct human exploitation combined with anthropogenic land-use change and impacts associated with invasive species.

“New Zealand’s extinct moa is our Taonga “It’s a species that has fascinated generations of New Zealand children,” said Dr Nick Lawrence, a palaeontologist at the University of Otago who was not involved in the study.

“Since the advent of ancient DNA, we’ve learned a lot more about the nine moa species that call Aotearoa home, but there are still many questions that remain unanswered.”

“Having the nuclear genome of the male little bush moa is the first step in exploring more deeply what makes moas so special. Even though it’s still in draft form, it’s about 85% complete.”

In the new study, Harvard researcher Scott Edwards and his colleagues assembled the complete mitochondrial and nuclear genomes of a male moa by sequencing ancient DNA and comparing it with the high-quality genome of the closely related emu.

They first calculated that the size of the moa nuclear genome was approximately 1.07 to 1.12 billion bases.

By analyzing the genetic diversity of the mitochondrial genome, the researchers estimated the bushmore’s long-term population to be approximately 237,000 individuals.

“Reconstructing the genome of a species like the tiny bushmore is difficult because there is only so much degraded ancient DNA to recover,” said Dr Gillian Gibb, a researcher at Massey University who was not involved in the study.

“In the case of moas, an additional challenge exists because the closest extant species with high-quality genomes to compare with diverged about 70 million years ago.”

“Despite these challenges, we have been able to recover a large portion of the genome, providing insight into moa evolution.”

The authors also investigated genes involved in the moa’s sensory biology and concluded that the bird probably has an extensive sense of smell and ultraviolet (UV) receptors in its eyes.

“This new study uses the genome to estimate the little bushmouse population at around 240,000 individuals, a number that is probably too high and the authors acknowledge it is a rough estimate,” Dr Lawrence said.

“Ecological estimates of moa are Motu “The (country) has a bird population of between 2 and 10 birds per square kilometre, with a total population of between 500,000 and 2.5 million birds.”

“The genome also shows that the little bush moa had a complex olfactory repertoire, which is consistent with what is seen in the moa skull.”

“Moas could also see in the ultraviolet spectrum, which may have helped them to find food, such as brightly colored truffle-like fungi, that they may have dispersed.”

“Moas, like other birds, are sensitive to bitter foods.”

“Moas are the only birds that have completely lost their wings,” added Prof Paul Schofield from the Canterbury Museum, who was not involved in the study.

“In this new paper, we also take a closer look at the big mystery of how this happened, concluding that it is not due to the loss of genes responsible for wing development, as previously suggested.”

“The paper also found that despite having an abnormal arrangement of the olfactory cortex in the brain, moas had normal avian olfactory abilities.”

of study Published in the journal Scientific advances.

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Scott V. Edwards others2024. Nuclear genome assembly of the extinct flightless bird, Little Bushmoore. Scientific advances 10(21); doi: 10.1126/sciadv.adj6823

Source: www.sci.news

New species of Ceratosaurus unearthed by paleontologists

Cinderella Longipes It is the first ceratopsian species known from the Early Cretaceous of Asia, extending the geological range of the dinosaur group Ceratopsia on the continent by 40 million years.



Cinderella Longipesreference specimen (b) and holotype (cj). Image courtesy of Averyanov. others., doi: 10.1098/rspb.2024.0537.

The newly discovered dinosaur species lived in what is now Siberia between 121 and 113 million years ago (the Early Cretaceous period).

Named Cinderella LongipesThe ancient creature is estimated to have been 2.5 metres (8.2 feet) long.

it is Noasauridaean extinct family and group of small carnivorous dinosaurs. Ceratopsians.

“Ceratopsians were the first major lineage of theropod dinosaurs to achieve taxonomic diversity and a wide geographic distribution,” said Dr. Alexander Averyanov from the Institute of Zoology and his colleagues.

“They were probably distributed worldwide during the Late Jurassic, but were pushed out of the northern continents by other theropod groups and underwent a secondary radiation in the Cretaceous on Gondwana, where they became the dominant predators and survived until the end of the Cretaceous.”

AbelisauroideaThe most diverse ceratosaurid clade, the Acanthosaurus genus, is known from the Cretaceous of Europe, where it is probably represented by secondary dispersals, but in Asia no ceratosaurids are known from the Late Jurassic onwards.

Fragmentary skeleton Cinderella Longipes Fossils including cervical vertebrae, pectoral girdle, humerus, and hind limbs were excavated at the Shestakovo 1 locality in the Ilek Formation of Western Siberia.

Cinderella Longipes Share unique hind leg proportions Elaphrosaurus and Limusaurus“This suggests improved running ability,” the paleontologists said.

“These species show ostrich-like foot specializations, with a large third metatarsal and a greatly reduced second metatarsal.”

“In contrast, all other fast-running non-avian theropod dinosaurs have arc metatarsals, with the third metatarsal being greatly reduced proximally.”

According to the authors: Cinderella Longipes This is about 40 million years younger than the youngest recorded Asian ceratosaur to date.

Cinderella Longipes It was part of a rare vertebrate group dominated by advanced ceratopsian dinosaurs. Psittacosaurus sibiricus“However, it also includes groups of tetrapods long extinct elsewhere, such as stem salamanders, protosuchian and chartegosuchian crocodylomorphs, tritylodontian synapsids, and docodontian mammalomorphs,” the researchers said.

Team work Published in a journal Proceedings of the Royal Society B.

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Alexander O. Averyanov others2024. Asia's last ceratopsid: a new noasaurid dinosaur from the Early Cretaceous Siberian Great Refuge. Proc. R. Soc. B 291 (2023): 20240537; doi: 10.1098/rspb.2024.0537

Source: www.sci.news

Study suggests ellagic acid as a promising dietary option for non-alcoholic fatty liver disease

Ellagic acid is a polyphenolic, non-flavonoid compound found naturally in a variety of fruits, including pomegranates, raspberries, strawberries, and grapes, as well as nuts, including pistachios, pecans, walnuts, and acorns.

Senavirasna othersResearchers are investigating the effects of ellagic acid, an antioxidant found in pomegranates, raspberries, strawberries, grapes and nuts, in preventing and potentially reversing the damage caused by fatty liver disease. Image courtesy of Engin Akyurt.

Obesity is epidemic in many parts of the world and contributes to increasing rates of non-alcoholic fatty liver disease (NAFLD).

This rapidly expanding epidemic is the most common chronic liver disease worldwide.

The prevalence of NAFLD increased from 25.24% in 2015 to 29.38% in 2021.

NAFLD represents a range of pathologies from simple fatty liver (nonalcoholic fatty liver, NAFL) to nonalcoholic steatohepatitis (NASH), which can progress to more severe conditions including fibrosis.

Currently, no cure exists for the long-term management of NAFLD/NASH, but dietary interventions containing several polyphenolic compounds have been investigated for the treatment of NASH. Ellagic acid is one such compound.

“Ellagic acid, found in a variety of foods including raspberries, pomegranates, blackberries and pecans, is widely known for its antioxidant properties but has also demonstrated anti-inflammatory, anti-fibrotic and anti-cancer properties,” said researcher Lois Balmer and doctoral student Tarani Senaviratna, both from Edith Cowan University.

“Ellagic acid stands out as a remarkable polyphenolic compound with a wide range of pharmacological properties that may be promising for the treatment of various chronic diseases, including NAFLD.”

“Edible plants containing ellagic acid and its derivatives are recognized as valuable functional foods that promote human health due to their pleiotropic biological effects.”

“Furthermore, evidence suggests that ellagic acid may exert synergistic therapeutic effects when combined with other antioxidant dietary supplements, making it a potential candidate for combination therapy.”

The authors were involved in a previous pilot study investigating the effects of several polyphenolic compounds on NAFLD, with ellagic acid showing the most promise in reducing inflammation.

“Ellagic acid exerts its hepatoprotective properties mainly through scavenging free radicals, modulating cytokine production, and regulating lipid metabolism,” the researchers said.

“Ellagic acid, a potent antioxidant, combats reactive oxygen species (ROS) and activates the NrF2 pathway to reduce oxidative stress and protect the liver.”

“Surprisingly, ellagic acid also inhibits the Nf-kB and MAPK pathways, reducing inflammation during NAFLD/NASH.”

“Evidence also shows that ellagic acid can lower both triglyceride and cholesterol levels and combat de novo lipogenesis, a significant risk factor in the progression of NASH.”

“Test-tube findings suggest that ellagic acid has the ability to reduce fibrosis.”

“Urolithins, the main microbial metabolites of ellagic acid, have been shown to improve the gut microbiota in several mouse models of obesity.”

“Specifically, Urolithin A has been shown to lower LDL and increase HDL levels and is also involved in improving lipid metabolism through gene regulation, while Urolithin C activates the hepatic AMPK pathway, countering the pathophysiology of NAFLD.”

“While the health benefits of ellagic acid and urolithins in NAFLD/NASH are being debated, their biological effects on the liver are still poorly understood.”

“Given that lipid metabolism, oxidative stress, inflammation, and insulin resistance play a role in the development of NASH, the results of this review suggest that ellagic acid may be a potential dietary intervention for NASH, potentially suppressing and even reversing the pathological symptoms of NAFLD/NASH.”

of study Published in the journal Antioxidants.

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Tarani Senavilasna others2024. Elucidation of the therapeutic effects of ellagic acid on nonalcoholic fatty liver disease and nonalcoholic steatohepatitis. Antioxidants 13(4):485; doi:10.3390/antiox13040485

Source: www.sci.news

Hubble Space Telescope Shines Light on Stunning Spiral Galaxy NGC 4731

The NASA/ESA Hubble Space Telescope captured this stunning image of a barred spiral galaxy called NGC 4731.

This Hubble Space Telescope image shows NGC 4731, a barred spiral galaxy about 43 million light-years away in the constellation Virgo. Image courtesy of NASA / ESA / Hubble / D. Thilker.

NGC 4731 It is located in the constellation Virgo, about 43 million light years from Earth.

Also known as IRAS 12484-0607, LEDA 43507, and UGCA 302, it is classified as a barred spiral galaxy.

“Barred spiral galaxies outnumber regular spiral and elliptical galaxies combined, making up about 60 percent of all galaxies,” the Hubble astronomers said.

“The bar-like structure we see is the result of the orbits of stars and gas in our galaxy aligning, forming dense regions where individual stars move in and out over time.”

“This is the same process that maintains the spiral arms of our galaxy, but in the case of barred galaxies it's a bit more mysterious. As spiral galaxies mature they seem to form a bar at their centre, which explains the large number of bar structures we see today. But later on the bar can also be lost if the accumulated mass along it becomes unstable.”

“The orbital patterns and gravitational interactions of galaxies support the bar-like structure of the galaxy, transporting matter and energy and promoting star formation.”

“Indeed, the observing program studying NGC 4731 seeks to investigate this flow of matter within the galaxy,” they added.

beginning discovered Discovered on April 25, 1784 by German-born British astronomer William Herschel, NGC 4731 has a diameter of about 80,000 light years.

With LEDA 43526 Galaxy, Forms Holm 472, a pair of interacting galaxies.

NGC 4731 is also a member of the NGC 4697 galaxy group. Located Near the Virgo Supercluster.

“Beyond the bar, NGC 4731's spiral arms extend far beyond the scope of this close-up Hubble image,” the astronomers said.

“The galaxy's elongated arms are thought to be the result of gravitational interactions with other nearby galaxies in the Virgo Cluster.”

The color image of NGC 4731 includes ultraviolet, near-infrared, and optical observations. Hubble's Wide Field Camera 3 (WFC3).

Six filters were used to sample different wavelengths, and color was generated by assigning a different hue to each monochromatic image associated with an individual filter.

“The richness of color reveals the galaxy's swirling gas clouds, dark dust bands, bright pink star-forming regions, and most notably, its long, luminous arms stretching out behind it,” the researchers said.

Source: www.sci.news

Astronomers document extraterrestrial exoplanets

The new catalogue, created as part of the TESS-Keck survey, includes 126 strange planets outside our solar system, ranging from unusual worlds with extreme environments to those that could potentially support life as we know it.

Artist's impression of the 126 planets in the new TESS-Keck survey catalog is based on data such as planet radius, mass, density, and temperature. Question marks represent planets that need more data for full characterization. Image courtesy of W. M. Keck Observatory/Adam Makarenko.

“Relatively few known exoplanets have had both their mass and radius measured,” said Steven Kane, professor at the University of California, Riverside, and principal investigator of the TESS-Keck survey. paper Published in Astrophysical Journal Supplement.

“Combined, these measurements tell us what the planet is made of and how it formed.”

“With this information, we will be able to answer the question of where our solar system fits in the grand scheme of other planetary systems.”

Professor Kane and his colleagues analysed more than 13,000 radial velocity (RV) measurements to calculate the masses of 120 confirmed planets and six candidate planets spread across the northern sky.

“These RV measurements allow astronomers to detect and characterize these exoplanetary systems,” said astrophysicist Ian Crossfield of the University of Kansas.

“When we see a star wobbling back and forth in a regular pattern, we can infer the presence of orbiting planets and measure their masses.”

Several planets discovered in the TESS-Keck survey stand out as touchstones for improving astronomers' understanding of the diverse ways planets form and evolve.

in Related Papers In Astronomical JournalAstronomers have announced the discovery of two new planets orbiting a sun-like star.

The first is a sub-Saturnian planet with a mass and radius intermediate between Neptune and Saturn.

“There's been some debate about whether sub-Saturn planets are truly rare or whether we're just bad at finding them,” said Michelle Hill, a graduate student at the University of California, Riverside.

“So planet TOI-1386b is an important addition to this planetary group.”

TOI-1386b takes just 26 days to orbit its star, while its neighbour, a planet with a mass similar to that of Saturn, takes 227 days to orbit the same star.

in Related ArticlesThe researchers described TOI-1437b, a planet about half the size of Neptune that orbits a sun-like star every 19 days.

“Planets smaller than Neptune and larger than Earth are the most common worlds in our galaxy, but they don't exist in our solar system,” said Daria Pidhorodetka, a graduate student at the University of California, Riverside.

“With each new discovery, we are reminded of how diverse the universe is, and that our place in it may be more unique than we can understand.”

The catalog also contains detailed descriptions of planets that, unlike the Sun, orbit extremely short distances around their stars.

One is so close to the orange dwarf that it completes an orbit in less than 12 hours.

“TOI-1798c orbits its star so quickly that a year on the planet lasts less than half an Earth day,” said Alex Polansky, a graduate student at the University of Kansas.

“Because these planets are so close to their stars, they are extremely hot and receive more than 3,000 times the radiation that Earth receives from the Sun.”

“Being in this extreme environment means that the planet is likely losing any atmosphere it may have originally formed.”

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Alex S. Polanski other2024. TESS-Keck Survey. XX. Uniform RV analysis of 15 new TESS planets and all survey targets. AppJS 272, 32; Source: 10.3847/1538-4365/ad4484

Michelle L. Hill other2024. TESS-Keck Survey. XIX. Warm transiting sub-Saturn-mass and non-transiting Saturn-mass planets orbiting solar analogues. AJ 167, 151; Source: 10.3847/1538-3881/ad2765

Daria Pidhorodetka other. 2024. TESS-Keck Survey. XXII. TOI-1437 in Near-Neptune Orbit. arXiv: 2405.12448

Source: www.sci.news

New research indicates that caterpillars are able to detect predatory wasps through the emission of static electricity.

Predatory wasps are electrically charged and emit electric fields, and their larvae respond to these fields with defensive behaviour, according to a new study from the University of Bristol.

Sam J. England and Daniel Robert discovered that some terrestrial animals can sense the electric fields emitted by electrostatically charged predators and use this sensation to mount defensive actions. These photos show the four animal species examined in the study: (A) A Cinnabarga larva (Tilia jacobae) Taking a defensive posture. (B) The larva of a rare transpiration moth (Terrorcrus Rekens) in a defensive coiled position. (C) The larva of the European peacock butterfly (Aglais), (D) a predatory common hornet in the middle of a defensive maneuver (HornetImage credit: Sam J. England & Daniel Robert, doi: 10.1073/pnas.2322674121.

“Many animals naturally build up static electricity on their bodies as they move around in their environment, and we knew that static electricity can push or pull on other charged objects,” said researcher Sam England, from the University of Bristol.

“In particular, we knew that insect hairs can be moved by electric fields emitted by electrostatically charged objects, in the same way that an electrically charged balloon can move hair on the head.”

“This got us thinking: What if prey animals like caterpillars could detect predators by sensing the electric fields emitted by the predators?”

“Could the static electricity of a predator like a wasp be enough to alert the caterpillar to the approach of the wasp, by pushing and pulling on the caterpillar's sensory hairs?”

Dr England and his colleague, Professor Daniel Robert, from the University of Bristol, measured how much static electricity the wasps and caterpillars had picked up by passing them through a static sensor.

The researchers then fed these charge values ​​into a computational model to mathematically predict how strong the electric field would be as the wasp approached the larvae on the plant.

When the caterpillars reacted defensively to these conditions, they were able to determine whether it was sensory hairs that were detecting the electricity by using a laser to detect tiny vibrations and measuring how much the hairs moved in response to electric fields of different frequencies.

The results are concerning because they show that the caterpillars are also sensitive to the frequencies of electric fields emitted by power lines and other electronic devices.

This means that humans may be filling the environment with electrical “noise” that interferes with animals' ability to detect predators.

Dr England continued: “We now feel it is extremely urgent to assess whether introducing a new type of sensory pollution – electrical noise – is interfering with the ability of caterpillars, and other animals, to detect predators.”

Almost all terrestrial animals seem to accumulate static electricity, so this static sense may be widespread, and the discovery that static electricity plays a role in these ecological interactions would open up an entirely new dimension to our understanding of how animals sense each other, and more generally, how and why animals evolve in certain ways.

“Our study suggests that terrestrial animals may be able to use static electricity as a predator-detection cue,” Dr England said.

“This is likely an ability that is particularly widespread in insects and small animals such as spiders and scorpions.”

“This study provides the first example of an animal detecting predators by sensing static electricity emitted by the predator.”

“This reveals a new dimension of predator-prey interactions on land, but also suggests a previously unnoticed way in which we may be negatively impacting wildlife by introducing sources of electrosensory pollution.”

of study Published in Proceedings of the National Academy of Sciences.

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Sam J. England & Daniel Robert. 2024. Prey can detect predators via airborne electroreception. PNAS 121(23):e2322674121; doi:10.1073/pnas.2322674121

Source: www.sci.news

Scientists Discover Unique Characteristics of Rare Element Promethium

Promethium is extremely rare, with only about 0.5 kg occurring naturally in the Earth’s crust at any one time.

Conceptual art depicts the rare earth element promethium in a vial surrounded by organic ligands. Image courtesy of Jacqueline DeMink / Thomas Dyke / ORNL.

[DiscoveredattheClintonLaboratoryin1945promethium is a lanthanide element with the symbol Pm and atomic number 61.

Named after the mythical Titan who brought fire to mankind, the name symbolizes human endeavor.

Despite their use in medical research and long-life nuclear batteries, some of their properties remain poorly understood.

“The aim of this project was to explore and gain new knowledge about this extremely rare element,” he said. Oak Ridge National Laboratory.

Dr. Ivanov and his colleagues prepared a chemical complex of promethium, allowing them to characterize it in solution for the first time.

Thus, they uncovered the secrets of this element through a series of meticulous experiments.

“Promethium was the last lanthanide discovered and has been the most difficult to study because it has no stable isotopes,” said Dr. Ilya Popovs, also of Oak Ridge National Laboratory.

“There are thousands of papers on lanthanide chemistry without promethium. It was a glaring flaw in the science as a whole,” said Dr. Santa Giansone-Popova of Oak Ridge National Laboratory.

“Scientists could only guess at most of its properties. Now we can actually measure some of them.”

The researchers linked, or chelated, radioactive promethium with a special organic molecule called a diglycolamide ligand.

The researchers then used X-ray spectroscopy to determine the properties of the complex, including the lengths of the chemical bonds between promethium and neighboring atoms — a scientific first and a long-missing part of the periodic table of elements.

Unlike other rare earth elements, synthetic promethium has no stable isotopes and is therefore only available in very small quantities.

For their research, the scientists produced the isotope promethium-147, which has a half-life of 2.62 years, in sufficient quantity and purity to study its chemical properties.

Remarkably, they were the first to demonstrate the signature of lanthanide contraction in solution for the entire lanthanide series, including promethium, atomic number 61.

Lanthanide contraction is a phenomenon in which elements with atomic numbers 57 through 71 become smaller than expected.

As the atomic number of these lanthanides increases, the radius of their ions decreases.

This contraction results in unique chemical and electronic properties as the same electric charge is confined to a shrinking space.

The authors obtained a clear promethium signal, which allowed them to better define the shape of the trend across the series.

“It’s really amazing from a scientific point of view. When I got all the data I was blown away,” Dr Ivanov said.

“This contraction of chemical bonds accelerates along the atomic series, but slows down significantly from promethium onwards.”

“This is a major breakthrough in understanding the chemical bonding properties of these elements and their structural changes along the periodic table.”

“Among other things, this achievement will ease the difficult task of isolating these valuable elements,” said Dr. Jansonne Popova.

“Our team has been working for a long time to isolate the entire series of lanthanides, but promethium was the last puzzle piece. It’s been very challenging.”

“With today’s advanced technology, we can’t use all these lanthanides as a mixture, because we have to separate them first.”

“This is where shrinkage becomes really important. It basically allows you to separate them, which is still pretty difficult.”

“All of the technological marvels of our time contain these rare earth elements in some form,” Dr Popovs said.

“We’re adding the missing link.”

Team paper Published in today’s journal Nature.

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D.M. Driscoll othersObservation of promethium complexes in solution. NaturePublished online May 22, 2024, doi: 10.1038/s41586-024-07267-6

Source: www.sci.news

Ancient settlement uncovered in Chile dates back 12,500 years

About 12,440 to 12,550 years ago, hunter-gatherers regularly returned to Chile’s Lake Taguatagua to hunt an ancient elephant relative called Gomphotherium and exploit other local resources, according to a team led by archaeologists from the Pontificia Catholic University of Chile.

Taguatagua 3 site, Chile: (A) Burning evidence spatially associated with Gomphothery cervical vertebrae and skull fragments. (B) Sacral and caudal vertebrae, intervertebral disks, and unfused hipbone segments. Note the distance between the first sacral vertebra and its disk. (C) End scraper from the site. (D) Core debitage from the site spatially associated with Gomphothery remains. Image courtesy of Labarca others., doi: 10.1371/journal.pone.0302465.

There are several known archaeological sites in the area. Lake Taguatagua Located in central Chile, it is one of the oldest known sites of human habitation in the Americas.

In a new study, Dr Rafael Labarca from the Pontificia Catholic University of Chile and his colleagues discovered an ancient hunter-gatherer camp dating back to the Late Pleistocene epoch, between 12,440 and 12,550 years ago.

The site, named Taguatagua 3, contains fossils of the Gomphosele, an extinct species closely related to the elephant.

Butchery marks on bones, stone tools and other evidence indicate that Taguatagua 3 was a temporary camp set up to process large carcasses.

During the camp’s short existence, other activities were also carried out, including the processing of other foods, as evidenced by the charred remains of plants and small animals such as frogs and birds.

Fossilized cactus seeds and bird egg shells suggest that the camp was inhabited, especially during the dry season.

Numerous archaeological sites from a similar period are now known to exist in the area, suggesting that Lake Tagua-Tagua was a recurring hunting and food-scavenging site for Late Pleistocene people thanks to abundant and predictable local resources.

“The area was an important location along the route of mobile groups at the time and the temporary camp may have hosted regular meetings between these groups,” the archaeologists said.

Further investigation of this archaeologically rich area will continue to provide insight into the migration and survival strategies of early humans in South America.

“Taguatagua 3 contributes to a greater understanding of how early humans adapted to the rapidly changing environment of central Chile during the Late Pleistocene,” the researchers said.

of Investigation result Published online in the journal PLoS One.

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R. Labarca others2024. Taguatagua 3: A new Late Pleistocene settlement in a highly suitable site for lacustrine habitat in central Chile (34°S). PLoS One 19(5): e0302465; doi: 10.1371/journal.pone.0302465

Source: www.sci.news

New Study Reveals Australian Marsupials Are More Afraid of Humans Than Other Predators

Researchers from the University of Tasmania and Western University have conducted experiments to show that Australian marsupials such as kangaroos and wallabies are most afraid of human “super predators,” fleeing from them 2.4 times more frequently than from other predators.



Recent experiments have demonstrated that carnivores and ungulates from Africa, Asia, Europe, and North America fear human “superpredators” much more than they do other predators. Australian mammals have been the focus of research into predator ignorance because they are suspected of exhibiting atypical responses. To experimentally test whether Australian mammals are also most afraid of humans, McGann others quantified responses of four native marsupials (eastern grey kangaroo, Bennett’s wallaby, Tasmanian pademelon, and brushtail possum) and taught fallow deer to playback predator (human, dog, Tasmanian devil, wolf) or non-predator control (sheep) vocalizations. Image courtesy of Pen_ash.

There is a widespread fear of humans among wildlife in Africa, Asia, Europe, and North America, reflecting the reality that humans are “super-predators,” far more dangerous than other predators worldwide.

Australian marsupials have been traditionally seen as naive to predators, based on their reactions to non-human threats.

“Our results significantly contribute to the growing body of experimental proof that wildlife globally view humans as the most feared predators on the planet,” stated Professor Liana Zanetto of Western University, a co-senior author of the study published in the journal Nature Proceedings of the Royal Society B.

“The strong fear of humans found in this study, as well as in similar recent experiments, is expected to have significant ecological repercussions, as additional research indicates that fear itself can reduce wildlife populations and that fear of humans can lead to cascading effects on multiple species across entire regions.”

To conduct their study, Professor Zanette and colleagues designed a hidden automated camera-speaker system in a sheep pasture in central Tasmania known as the Bowfront.

The five species they observed (eastern grey kangaroo, Bennett’s wallaby, Tasmanian pademelon, brushtail possum, and fallow deer) are the most prevalent native herbivores in the area.

As the animals came close (about 10 meters, 30 feet), the cameras captured their responses to non-threatening stimuli such as calm human speech, a barking dog, growling Tasmanian devil, howling wolf, or bleating sheep.

Native marsupials reacted by fleeing more frequently when exposed to the sound of their next most feared predator (dogs) compared to human voices, and were over twice (2.4 times) more likely to flee from humans (44.3% vs. 18.6% of trials).

These findings present conservation challenges but also offer insights for managing native marsupials in regions where they are overpopulated.

“Global studies have shown that humans kill prey at a much higher rate than other predators, making us ‘super-predators,’ and the intense fear of our presence in all wildlife species aligns perfectly with our inherent deadliness,” noted Professor Zanette.

“Humans are the ‘invisible killer.’ We may not perceive ourselves as the primary predator, let alone the most dangerous, but wild animals clearly see us for what we truly are.”

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Catherine McGann et al. 2024. Fear of human “super-predators” in Australia’s native marsupials and invasive deer. Proceedings of the Royal Society B 291 (2023): 20232849; doi: 10.1098/rspb.2023.2849

Source: www.sci.news

Research reveals that Mycenaean armor was created for extended battles

A 3,500-year-old Mycenaean bronze suit of armour discovered in the Greek village of Dendra may have been used in combat and not just for ritual purposes as previously thought.



Volunteer Marines wearing replica Dendra armor during a mock battle during a demonstration study. Image credit: Andreas Flouris / Marija Marković.

One of the oldest armors discovered in Europe is a 3,500-year-old suit of armor found near the village of Dendra, a few kilometers from ancient Mycenae in southern Greece.

Since its discovery in 1960 by a team of Greek and Swedish archaeologists, it has been unclear whether it was ceremonial clothing or gear suitable for combat.

This question has important implications for understanding warfare in Late Bronze Age Europe, yet there is no historical record of the use of this style of armour.

In a new study, Professor Andreas Floris from the University of Thessaly and his colleagues combined historical and experimental evidence to investigate the combat suitability of Dendra armour.

The researchers recruited 13 volunteers from the Greek Marine Corps, outfitted them with replica Dendra armour and Bronze Age weapons, and had them carry out 11 hours of simulated Bronze Age combat protocols.

This battle simulation was developed based on the historical records of Homer. Iliad Additionally, we add physiological and environmental evidence to approximate the typical diet, activities, and operations of a Mycenaean army.

Testing has shown that the replicated Dendra Armor does not restrict a warrior's combat capabilities, nor does it place undue strain on the wearer.

These results suggest that Dendra armour was battle-hardened and that the Mycenaeans' powerful influence on Mediterranean history was due in part to their armour technology.

To complement these results, the authors developed freely available software that allows for the simulation of combat conditions and allows testing the hypothetical effectiveness of the armor in more diverse scenarios.

“The armour worn by our volunteers had the same dimensions as the Bronze Age originals and weighed roughly the same,” Professor Floris said.

“We also monitored calorie intake based on the Homeric diet (about 4,443 calories), which Iliad“It linked calorie expenditure and the stress placed on the volunteers' bodies in typical Greek summer temperatures of 30-36°C.”

“As the 11-hour combat protocol began, we measured heart rate, oxygen consumption, core body temperature, fluid loss and muscle function.”

“We found that this armor allows complete flexibility of movement and does not place undue physiological stress on the body.”

“This means that, despite previous views that classified the armour as ceremonial clothing, it could have been worn for extended periods during battle by healthy individuals.”

“Sixty years have passed since the discovery of Dendra armour, and we now know that, although seemingly cumbersome, it was not only flexible enough to permit nearly all of a warrior's movements on foot, but also durable enough to protect the wearer from most blows.”

of result Published online in the journal PLoS One.

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AD Floris others2024. Analysis of Greek prehistoric full-body armour combat based on physiological principles: a series of studies using thematic analysis, human experiments and numerical simulations. PLoS One 19(5): e0301494; doi: 10.1371/journal.pone.0301494

Source: www.sci.news

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New research indicates that following a Mediterranean diet may alleviate anxiety and lower stress levels

Researchers from the University of the Sunshine Coast and the University of South Australia have discovered in a recent study that following a Mediterranean diet is linked to lower severity of anxiety and stress-related symptoms in older Australians living in the community. Despite this, there was no observed connection with depressive symptoms. The study also found that specific components of the Mediterranean diet, such as reduced consumption of sugary beverages and increased intake of fruits, nuts, and legumes, were independently associated with lower levels of anxiety symptoms.



The Mediterranean diet is inversely associated with the severity of anxiety and stress-related symptoms.

Anthony Villani, a researcher from the University of the Sunshine Coast, and his team investigated the correlation between adherence to a Mediterranean diet and the severity of depression, anxiety, and stress-related symptoms in older adults. A total of 294 older adults with an average age of 70.4 years who lived independently in Australia participated in the study.

The results showed that adherence to the Mediterranean diet was associated with lower levels of anxiety and stress-related symptoms, but not depressive symptoms. Furthermore, specific dietary components like low intake of fruits, nuts, legumes, and sugar-sweetened beverages were linked to decreased severity of anxiety and stress-related symptoms.

Dr. Anthony Villani noted, “These foods were key indicators in a study of more than 300 older Australians.” Additionally, he mentioned that individuals following a Mediterranean-style diet high in fruits, vegetables, legumes, nuts, seeds, fish, and olive oil had lower intensity of anxiety symptoms.

He continued, “Higher consumption of legumes and nuts, along with lower intake of sugary beverages, showed the most significant impact on reducing anxiety and stress. Nuts and legumes are rich in fiber, healthy fats, and antioxidants, which can have positive effects on brain health through gut health and inflammation reduction.”

The study, which controlled for various factors associated with poor mental health, emphasized the importance of a healthy diet in maintaining good mental health. It also highlighted the need for further research to explore the mental health benefits of the Mediterranean diet in older adults.

Published in Nutrients, the findings of the study are significant for understanding the relationship between diet and mental health in older populations.

_____

Lisa Allcock et al. 2024. Adherence to a Mediterranean diet is inversely associated with anxiety and stress, but not depression: a cross-sectional analysis of community-dwelling older Australians. Nutrients 16(3):366; doi: 10.3390/nu16030366

Source: www.sci.news

Illinois Unearths Remarkable 308-Million-Year-Old Fossil of Spiny Spider

The forests of the Late Carboniferous Period (about 300-320 million years ago) were home to a wide variety of arachnids. In addition to the familiar spiders, harvestmen, and scorpions, there were other strange kinds of spider-like animals. new paper this month, paleontology journal a pair of paleontologists explained. douglas sarachne echinopod a large spider-like arachnid with highly spiny legs (presumably to deter predators) from the world-famous Mason Creek fossil site in Illinois, USA.



douglas sarachne echinopod. Image credit: Paul Selden and Jason Dunlop, doi: 10.1017/jpa.2024.13.

douglas sarachne echinopod “It comes from Illinois' famous Mason Creek and is approximately 308 million years old,” said Dr. Paul Selden, a paleontologist at the University of Kansas and the Natural History Museum in London.

“This compact arachnid, about 1.5 cm long, has surprisingly strong, spiny legs, and is completely unlike any other known arachnid, living or extinct.”

“Coal measurements are an important source of information about fossil arachnids and represent the first time in Earth's history that most living groups of arachnids arose together. However, the fauna remains quite different from what it is today. It was different.”

Dr Jason Dunlop, a paleontologist at the Berlin Museum of Nature, said: 'Spiders are a fairly rare group, only known from primitive lineages at the time, and they are similar to a variety of long-extinct arachnids and these. They shared a shared ecosystem.”

douglas sarachne echinopod is a particularly striking example of one of these extinct forms. ”

“Although this fossil's highly spiny legs are reminiscent of modern harvesters, its body structure is quite different from harvesters and other known arachnid groups.”

douglas sarachne echinopod The researchers discovered that it does not belong to any known order of Araneidae.

“Unfortunately, we can't see details such as the mouth parts, so it's difficult to say exactly which group of arachnids are our closest relatives,” Dr Selden said.

“It may belong to a broader group that includes spiders, whip spiders and whip scorpions.”

“Whatever their evolutionary similarities, these spiny arachnids likely come from a time when arachnids were experimenting with different body plans.”

“Some of these later became extinct, probably shortly after the Mason Creek era, during the so-called 'Carboniferous rainforest collapse,' when coal forests began to fragment and disappear. Or perhaps these strange arachnids are hanging on until the mass extinction at the end of the Permian?”

Specimen douglas sarachne echinopod It was discovered in clay and ironstone concretions by Bob Macek in the 1980s.

Macek introduced a common method of cracking stones by leaving them outdoors in water over the winter, allowing frost to penetrate the natural cracks in the stones along the fossil-containing surface.

A sharp hammer blow split the stone along a plane, exposing the fossil.

Around 1990, David Douglas acquired a specimen from Bob, at which point it became part of the David and Sandra Douglas Collection and was displayed in the Douglas Family Museum of Prehistoric Life.

In 2023, when it became clear that the specimen was a new species, David Douglas donated it to the Field Museum of Natural History for study.

“Genus name douglas sarachne We recognize the Douglas family,” Dr. Dunlop said.

“after that, echinopods “Refers to the animal's unique and distinctive spiny legs.”

_____

Paul A. Selden and Jason A. Dunlop. A remarkable spiny arachnid from Mason Creek Lagerstätte, Pennsylvania, Illinois. paleontology journal, published online on May 17, 2024. Doi: 10.1017/jpa.2024.13

Source: www.sci.news

Ancient Norwegian archaeologist uncovers Stone Age leader’s visage

The skeletal remains of a 4,000-year-old Scandinavian man were discovered in 1916. Hitla island, Norway.

The male Hitra was approximately 169 cm tall, had blond hair and blue eyes. Image courtesy of Thomas Foldberg/Åge Hojem/NTNU University Museum.

“In 1916, the road up the hill to the Fausland farm on the island of Hitra was being renovated using gravel from the coast along the deepest part of Balmsfjorden,” said Dr. Birgitte Skarr of the NTNU University Museum. a colleague said.

“Suddenly, the workers noticed human bones among the sand and stones.”

“The bones belonged to an approximately 25-year-old man who died at the end of the Stone Age, 4,000 years ago.”

“He is believed to have drowned. At the time of his death, the sea level would have been 12.5 meters higher than it is now, and the site of his discovery would have been at a depth of 4 meters.”

Archaeologists also found and studied a Hitraean dagger and arm guard.

“The arm guard is a rectangular bone with two holes that would have been attached to the wrist of the bow hand,” they said.

“The guard protects your wrist from the impact of the bowstring when you shoot an arrow.”

“These pieces of equipment may indicate that he was a warrior.”

“It is impossible to determine whether the drowning was the result of a fight or an accident,” Dr. Skarr said.

“What we do know is that the Hitraeans lived in a very turbulent time.”

“Up until that point, most people lived as hunter-gatherers, and agriculture only became fully established in Norway at the end of the Stone Age, during the time of the Hitra people.”

“Although elements of agriculture had been introduced earlier in southern and eastern Norway, agriculture was first established during this period in central Norway, along the coast of western Norway, and in northern Norway.”

“We believe that agriculture was introduced by settlers who came to Norway to obtain more land, and they were willing to use weapons to do so.”

“So we have to expect violent clashes between the people who were already living here and the newcomers.”

“New people brought new knowledge to the country, not just about animal husbandry and agriculture, but also about other ways of organizing society.”

“They lived in a class society, had different worldviews, different religions, and large networks that spanned Europe.”

“This knowledge led to major political, economic, and social changes.”

“There is still much we don’t know about this dramatic period in Scandinavian history, and research continues.”

“His DNA is currently being analyzed at the Lundbeck Foundation Geogenetics Center at the University of Copenhagen.”

Source: www.sci.news

Stunning images of NGC 4689 captured by Hubble

Astronomers using the NASA/ESA Hubble Space Telescope have captured sharp images of NGC 4689, a jewel-bright spiral galaxy in the constellation Coma.



This Hubble image shows spiral galaxy NGC 4689 located 52 million light-years away in the constellation of Coma. Image credits: NASA / ESA / Hubble / D. Tilker / J. Lee / PHANGS-HST Team.

NGC 4689 It is located approximately 52 million light-years away in the constellation Kamina.

“Of the 88 constellations officially recognized by the International Astronomical Union (IAU), Coma has the distinction of being the only constellation named after a historical figure. Queen Berenice II of Egypt” explained the Hubble astronomer.

“The Latin word ‘coma’ refers to her hair, meaning that NGC 4689 can be said to be present in the Queen’s hair.”

“Some of Berenice’s contemporaries may have meant this quite literally; her court astronomer believed that Berenice’s lost locks had been destroyed by God (“among the stars”). It was given this name because there is a story that it was thought to have been placed in It is the constellation of Coma. ”

NGC 4689 is discovered It was proposed by German-born British astronomer William Herschel on April 12, 1784.

Also known as LEDA 43186 or UGC 7965, this galaxy is a member of the Virgo Cluster, a group of more than 2,000 galaxies.

NGC 4689 is tilted 36 degrees and can be viewed almost head-on.

The new images of the galaxy were created from separate exposures taken in the ultraviolet, visible, and near-infrared spectral regions. Hubble’s Wide Field Camera 3 (WFC3).

This is based on data obtained through a gender filter. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter.

“This image was created using two sets of observations taken in 2019 and 2024, both as part of a program to observe multiple ‘nearby’ galaxies.” Astronomy said the people.

The 2024 observing program is an interesting example of how Hubble, a relatively old but highly productive telescope, can support the work of the technologically cutting-edge Webb Telescope. ”

“Observations collected by Webb change our understanding of how galaxies change and evolve over time by providing data of unprecedented detail and clarity. It will be.”

“But thanks to their complementary capabilities, new observations from Hubble (such as those used to create new images) can aid the work being done using the Web.”

“In this case, the Hubble data were collected to better understand the stellar populations of nearby galaxies, which is critical to understanding the evolution of galaxies.”

“NGC 4689 therefore plays an important role in advancing our understanding of how all galaxies evolve.”

Source: www.sci.news

Cyprus settled by hunter-gatherers much earlier than previously believed

With persistent stories of isolation, inaccessibility, and unattractiveness, one of the eastern Mediterranean islands was first populated by an influx of agricultural populations from the mainland under demographic pressures. It is generally considered to be a Neolithic phenomenon that began with. New research led by Professor Corey Bradshaw from Flinders University shows Cyprus may have been settled by hunter-gatherers by about 14,000 to 13,000 years ago, earlier than previously recognized. . This process must have involved a small number of large-scale migration events (hundreds to thousands of people), which infers the intentions and organization of these early humans.



Bradshaw uses the latest archaeological data, afterthought climate projections, and demographic models of age structure to other. They demonstrate evidence of an early arrival on Cyprus (14,257-13,182 years ago), within two to three major events occurring within 100 years, to ensure the risk of extinction is low. They expected a large group (1,000 to 1,375 people) to arrive.Image credit: Bradshaw other., doi: 10.1073/pnas.2318293121.

In researching when Cyprus was first occupied by humans, Professor Bradshaw and his colleagues discovered that the large Mediterranean islands were an attractive and preferred destination for Paleolithic people.

Their findings contradict previous research that suggested Mediterranean islands would have been inaccessible and inhospitable for Pleistocene hunter-gatherer societies.

Archaeologists used archaeological data, climate estimates, and demographic modeling to uncover Cyprus's early people.

Analysis of archaeological dating from the 10 oldest sites across Cyprus suggests that first human habitation dates between 14,257 and 13,182 years ago, which is longer than previously thought. It is also much older.

“The islands were then rapidly settled. Climate modeling shows that this early hominin population was able to survive in tandem with increases in temperature, precipitation, and environmental productivity sufficient to sustain large hunter-gatherer populations. “We show that this is the case,” the researchers said.

Based on demographic models, we believe that large groups of hundreds to thousands of people arrived in Cyprus over two or three major migration events within 100 years.

“This settlement pattern suggests systematic planning and the use of advanced vessels,” Professor Bradshaw said.

Within 300 years, or 11 generations, Cyprus' population grew to a median of 4,000 to 5,000 people.

Dr Theodora Muzio, an archaeologist at James Cook University and the University of Cyprus, said: “This result suggests that Cyprus, and perhaps other Mediterranean islands, were more likely to be inhospitable places for Paleolithic hunter-gatherer societies. “This suggests that it would have been an attractive destination.”

“The dispersal and settlement of humans in Cyprus and other eastern Mediterranean islands was due to rapid climate change, with coastal regions inundated by post-ice age sea level rise and farmers forced to move to new locations. , it is argued that this is due to demographic pressures on the mainland, an area of ​​necessity rather than choice.”

“This interpretation has arisen as a result of significant gaps in the archaeological record of Cyprus, resulting from differences in the preservation of archaeological materials, bias in preservation, uncertainties associated with dating, and limited DNA evidence. '' said Australian Museum of Archaeology's archaeologist Dr Christian Liebmeyer. Australian Biodiversity and Heritage Research Council Center of Excellence, German Institute of Archaeology, and James Cook University.

“Our research, based on more archaeological evidence and advanced modeling techniques, changes that.”

“New findings highlight the need to reconsider the question of early human migration in the Mediterranean and test the validity of the perceived early settlement dates in the light of new technologies, field survey methods and data. ' said Professor Bradshaw.

Regarding this research, paper Published in Proceedings of the National Academy of Sciences.

_____

Corey J.A. Bradshaw other. 2024. Demographic models predict the onset of the late Pleistocene and rapid expansion of pre-agro-pastoralism in Cyprus. PNAS 121 (21): e2318293121; doi: 10.1073/pnas.2318293121

Source: www.sci.news

Astronomers Find Milky Way Center is Ventilated

Astronomers using NASA's Chandra X-ray Observatory have discovered an “exhaust vent” that directs hot gas away from Sagittarius A*, the supermassive black hole at the center of the Milky Way galaxy. The vent is about 26,000 light-years from Earth and is connected to a previously discovered chimney-like structure perpendicular to the galactic plane. Chandra's data shows a cylindrical tunnel that helps collect gas towards the outer edge of the Milky Way. The results reveal how the Milky Way's black hole takes in and rejects matter.

This image shows a region near the center of the Milky Way galaxy in X-rays and radio waves. At the bottom of the image, near the center, there are knots of shiny, tangled material that resemble paint splatters. This is the brightest region in the image and contains the supermassive black hole at the center of the galaxy known as Sagittarius A*. The bottom third of the image looks like an angry firestorm. Red and orange stripes were scattered in all directions, as if the embers of a fire had crackled and shot into the air all at once. A flame-like structure is licking from the right side towards the center. Most of the image is injected with a wispy blue cloud indicating his X-rays detected by Chandra. In some places, wispy blue clouds appear to form balls of blue-green light, known as dust rings. They are caused by X-rays from a bright X-ray source reflecting off the dust around them. These dust rings resemble underwater lights glowing in a cloudy pool at night. Rising from Sagittarius A* in the center of the image is a pillar of blue light called a chimney. This chimney of hot gas is surrounded by a red cloud filled with stars, appearing as a small red speck. Near the top of the blue pillar is a light blue stripe surrounded by an illustrated gray box. This line is called the chimney exhaust. Immediately to the left is another illustrated box showing a close-up image of the chimney vent that Chandra observed.Image credits: NASA / CXC / Chicago Space / Mackey other. / NRF / SARAO / MeerKAT / SAO / N. Walk.

The chimney begins at the center of the Milky Way and stands perpendicular to the galaxy's spiral disk.

Astronomers previously identified the chimney using X-ray data from NASA's Chandra mission and ESA's XMM Newton mission.

The radio emissions detected by the MeerKAT radio telescope show the influence of the magnetic field surrounding the gas in the chimney.

The latest Chandra data reveals several X-ray ridges nearly perpendicular to the galactic plane.

Astronomers believe these are cylinder-shaped tunnel walls that help collect hot gas as it moves upwards along the chimney and away from the center of the galaxy. .

The newly discovered vent is located near the top of a chimney about 700 light-years from the center of the galaxy.

“We suspected that the magnetic field was acting as a chimney wall, allowing hot gases to rise through it like smoke,” said Dr. Scott McKee, an astronomer at the University of Chicago.

“I just discovered an exhaust near the top of the chimney.”

Astronomers believe the vent formed when hot gas rising through the chimney collided with cooler gas in its path.

The brightness of the exhaust wall in X-rays is caused by the shock wave created by this collision, similar to the sonic boom from a supersonic airplane.

The left side of the exhaust port is thought to be particularly bright because the upwardly flowing gas hits the tunnel wall at a more direct angle and with more force than other areas.

The researchers believe that the hot gas originates from a series of events in which material falls into Sagittarius A*, then erupts from the black hole, sending gas upward along the chimney and out the exhaust vent. I think it is most likely that it did.

However, it is not known exactly how often black holes are fed.

Previous studies have shown that dramatic X-ray flares occur every few hundred years at or near the central black hole, so that these flares send hot gases upward through the exhaust vent. may play an important role in pushing up.

Astronomers also estimate that Sagittarius A* tears apart and swallows a star approximately every 20,000 years.

Such an event would lead to a powerful and explosive release of energy, much of which would rise through the chimney vent.

Dr Mark Morris, an astronomer at the institute, said: 'We don&#39t know whether this energy and heat is caused by a large amount of material being thrown into Sagittarius A* at once. It&#39s like being thrown into it.” University of California, Los Angeles.

“Alternatively, it could result from multiple small loads being fed into the black hole, similar to kindlings thrown in periodically.”

Particles and energy within the vents provide clues about the origins of two mysterious and much larger structures near the center of the Milky Way. Fermi bubbles observed in gamma-rays by NASA&#39s Fermi Gamma-ray Space Telescope, and eROSITA bubbles detected by NASA&#39s Fermi Gamma-ray Space Telescope. ESA&#39s eROSITA X-ray telescope.

These are both pairs of structures that extend thousands of light-years away from the center of our galaxy.

These provide important information about past explosive activity near the center of the galaxy.

Both the Fermi and eROSITA bubbles are aligned along the direction of the chimney and a second X-ray chimney that starts at the center of the galaxy and points in the opposite direction.

The funnel effect of the exhaust near the top of the chimney keeps the hot gases concentrated as they move upwards, which can promote the formation of a bubble agglomerate structure.

“The origin of the Fermi and eROSITA bubbles is one of the greatest mysteries facing the study of high-energy radiation from the Milky Way,” said Dr. Gabriele Ponti, an astronomer at Italy&#39s National Institute of Astrophysics.

“We discovered small structures that may play a major role in the creation of these giant bubbles.”

a paper Regarding the survey results, astrophysical journal.

_____

Scott C. McKee other. 2024. X-rays from the central “exhaust” of the chimney at the center of the galaxy. APJL 966, L32; doi: 10.3847/2041-8213/ad3248

Source: www.sci.news

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Arup, a British engineering firm, duped out of £20m in deepfake scam

Arup, a British engineering firm, fell victim to a deepfake scam when an employee mistakenly transferred HK$200 million (approximately 20 million yen) to criminals during an artificial intelligence-generated video call.

Reports from Hong Kong police in February revealed that an employee of an unnamed company was duped into sending a large sum of money in a fraudulent call impersonating a company executive.

Arup confirmed that they were the company involved and had reported the incident to the Hong Kong police earlier this year. They admitted that fake audio and video had been used in the fraud.

The company stated, “Our financial stability and business operations remained unaffected, and there was no compromise to our internal systems.”

Arup’s global chief information officer, Rob Greig, mentioned that the organization faces frequent cyberattacks, including deepfakes, as seen in this incident.

Greig emphasized the need for increased awareness regarding the sophistication of cyber attackers, especially after Arup’s experience.

A report from the Financial Times newspaper first identified Arup as the target of the scammers.

Arup, known as one of the world’s leading consulting engineering firms, employs over 18,000 individuals and is recognized for its involvement in projects like the Sydney Opera House and London’s Crossrail transport scheme.

Another recent case involving a deepfake scam targeted WPP CEO Mark Read, as reported by The Guardian last week.

Hong Kong police disclosed that employees transferred HK$200 million in total to five local bank accounts in 15 transactions during a video conference call where the perpetrators posed as senior company officials.

The investigation into the scam is ongoing, but no arrests have been made yet, with the case classified as “obtaining property by deception.”

Source: www.theguardian.com

Fresh research offers new understanding of baobab’s evolutionary past

The iconic baobab, also known as the upside-down tree or tree of life, is most likely native to Madagascar, according to a new study.

Baobab tree in Senegal. Image credit: Viajesunion2.

genus AdansoniaThis plant, better known as the baobab or “Mother of the Forest,” has fascinated botanists, tourists, naturalists, and passersby for centuries.

Perhaps the earliest record of humans marveling at these amazing trees can be traced back to the ancient Egyptians around 2,300 BC.

Their grotesque appearance, gigantic size, reputed longevity, and diverse uses have made baobabs one of the most charismatic species on Earth.

Embedded in folklore and tradition, baobabs have inspired countless works of art and have been associated with human settlements and cultures for thousands of years.

Adansonia consisting of Eight morphologically distinct species: one distributed throughout Africa, one in northwestern Australia, and six endemic to Madagascar.

However, the origin of baobabs has been debated for many years due to a lack of fossil evidence.

“Our study reveals new insights into baobab speciation patterns and shows how climate change has influenced baobab distribution and speciation patterns over millions of years.” said Dr Ilia Leech, researcher at the Royal Botanic Gardens, Kew.

Dr. Leach and his colleagues conducted genomic analyzes of all eight baobab tree species and combined these datasets with ecological analyses.

As a result of the analysis, Adansonia They originated about 41 million years ago and diversified about 20 million years ago.

The researchers found that the historical population dynamics of baobabs are closely linked to both interspecific competition and geological changes in Madagascar, particularly changes in sea level.

Based on data including phylogenetic relationships, gene flow, and genetic diversity of different baobab species, they believe that the hypothesis of mainland Africa and Madagascar as the center of origin for baobabs is the most reasonable explanation for the current data. suggests providing. Australia.

The discovery also allowed scientists to reassess the baobab's conservation strategies and current status.

For example, they suggest that two endangered baobab species in Madagascar should be assigned higher conservation status. Adansonia Suarezensis and Adansonia grandidieri.

High levels of inbreeding, low genetic diversity, and population declines all mean these endangered species lack resilience to ecological perturbations and could be seriously threatened by climate change. It suggests that.

“We are thrilled to be part of this project that uncovers patterns of baobab speciation in Madagascar and the subsequent remarkable long-distance dispersal of two species, one to Africa and one to Australia. I was delighted,” said Professor Andrew Leach, a researcher at Queen Mary University. London.

“This has been accompanied by the evolution of some interesting pollination syndromes involving hawkmoths, lemurs and bats.”

of study It was published in the magazine Nature.

_____

JN. One other. Baobab tree prominence in Madagascar. Nature, published online April 19, 2024. doi: 10.1038/s41586-024-07447-4

Source: www.sci.news

Marine scientists confirm that killer whales only take one breath during a dive

To collect information on the animals’ behaviors, Professor Andrew Treitz and his team at the University of British Columbia utilized drone footage and biological data from tags attached to 11 northern and southern resident killer whales in Queen Charlotte Sound, Queen Charlotte Strait, Johnston Strait, and Strait of Juan de Fuca along the British Columbia coast.



Still image from UAV drone video showing data logger placement and breathing. Image credit: McRae et al., doi: 10.1371/journal.pone.0302758.

“Orcas are like sprinters; they lack the endurance for deep and prolonged dives like blue or humpback whales,” Professor Treitz noted.

Research revealed that killer whales predominantly spend their time off the coast of British Columbia, engaging in shallow dives lasting less than a minute.

An adult male recorded the longest dive time of 8.5 minutes.

By determining that the whales took only one breath during the dive, researchers could calculate their oxygen consumption rates per minute for adults and juveniles.

This information contributes to estimating the energy expenditure of killer whales and their daily fish consumption needs.

University of British Columbia student Tess McRae stated, “This will aid in understanding if killer whales, especially the endangered southern population, are obtaining sufficient food. It’s a critical aspect.”

The orcas in the study took 1.2 to 1.3 breaths per minute at rest, increasing to 1.5 to 1.8 breaths per minute while moving or hunting.

For comparison, humans typically take around 15 breaths per minute at rest and 40 to 60 breaths per minute during physical activity.

“It’s akin to holding your breath, rushing to the grocery store, shopping, and returning before being able to breathe again,” explained Dr. Beth Volpoff, a postdoctoral researcher at the University of British Columbia.

Published findings in the online journal PLoS ONE.

_____

TM McRae et al. 2024. Killer whale breathing rate. PLoS ONE 19 (5): e0302758; doi: 10.1371/journal.pone.0302758

Source: www.sci.news

Hubble Space Telescope finds three-star system in Taurus

The Hubble team has released an astonishing image. NASA/ESA Hubble Space Telescope of the triple star system HP Tau.

About 550 light-years away in the constellation Taurus, three dazzling stars, HP Tau, shine brightly from the cavity of a reflection nebula in a new Hubble image. Image credit: NASA / ESA / G. Duchene, University of Grenoble I / Gladys Kober, NASA and Catholic University of America.

HP Tau is a triple star system located approximately 550 light-years away in the constellation Taurus.

The system, also known as EPIC 247592463, TIC 118521708, or IRAS 04328+2248, consists of the variable stars HP Tau, HP Tau G2, and HP Tau G3.

HP Tau is one of the stars. T Taurus a type of young variable star that has not yet begun nuclear fusion but is beginning to evolve into a hydrogen-fueled star similar to the Sun.

“T Tauri stars tend to be less than 10 million years old, compared to our Sun, which is about 4.6 billion years old, but they formed when they were shrouded in clouds of dust and gas. “They are often discovered as they are,” Hubble astronomers said.

“Like other variable stars, HP Tau's brightness changes over time.”

“The T Tauri star is known to have periodic and random fluctuations in brightness.”

“Random fluctuations can be caused by chaotic conditions in a developing young star, such as instability in the accretion disk of dust and gas around the star, material from that disk falling into the star and being consumed, and flares on the star's surface. It may be due to the nature of

“The periodic changes may be due to giant sunspots rotating in and out of view.”

“Clouds of gas and dust glow with reflected light as they orbit the star.”

“Reflection nebulae do not themselves emit visible light, but they shine when light from nearby stars reflects off gas and dust, much like fog illuminated by a car's headlights.”

Hubble studied the HP-tau system as part of its study of protoplanetary disks, disks of material around stars that coalesce into planets over millions of years.

Source: www.sci.news

As heat waves loom, cities innovate to protect residents and prevent casualties.

In North Carolina, for instance, Ward and colleagues have assisted counties in formulating heat preparedness plans to identify their most vulnerable residents.

He emphasized that government officials should approach the rise in heat and humidity in a similar manner to how they handle hurricanes, tornadoes, and other emergencies.

“Emergency management and public health officials are already well-prepared for various extreme weather events, but they are not as well-prepared for heat-related incidents,” Ward explained.

The events of last summer raised concerns, she noted.

“It was a Category 5 heat event,” Ward explained. “The severity of what we experienced last summer was enough to bring attention to this issue.”

Research indicates that climate change is leading to an increase in the frequency, duration, and intensity of heatwaves worldwide. Last year marked the hottest year on record, and the warming trend continues. According to the European Union’s Copernicus Climate Change Agency, April saw World temperature records being set for 11 consecutive months.

Forecasts suggest that temperatures will be higher than usual across much of the United States in the next three months, as per the National Oceanic and Atmospheric Administration’s predictions. According to the National Oceanic and Atmospheric Administration.

Ward expressed optimism that cities were taking the threat of heatwaves seriously, although significant challenges lie ahead. Securing funding for preparing for extreme heatwaves, particularly in rural regions, is a major challenge.

Addressing the root social issues that exacerbate during heatwaves, such as homelessness, soaring energy costs, and economic disparities, is an even greater challenge.

However, Ward remains hopeful that the experiences of last summer have motivated some local governments to take action.

“Moving forward, I would like to see a stronger emphasis on preventive measures to reduce these exposures in the first place, so we are not constantly in response mode,” she stated.

Source: www.nbcnews.com

Discovery of ancient star in Milky Way halo estimated to be 12-13 billion years old by astronomers

Astronomers at the Massachusetts Institute of Technology have discovered very old stars in the Milky Way’s halo, a cloud of stars that covers the entire disk of our galaxy. These objects formed between 12 and 13 billion years ago, when the first galaxies were beginning to form. Researchers believe that each star once belonged to its own dwarf galaxy, which was later absorbed into the larger but ever-growing Milky Way, making them known as small accreting star systems (SASS). It’s called a star.



Artist’s concept of the Milky Way galaxy. Image credit: Pablo Carlos Budassi / CC BY-SA 4.0.

“Given what we know about galaxy formation, these oldest stars should definitely exist,” says MIT professor Anna Froebel.

“They are part of our cosmic family tree. And now we have a new way to find them.”

As they discover similar SASS stars, Professor Froebel and his colleagues hope to use them as analogues of ultrafaint dwarf galaxies, which are thought to be some of the first living galaxies in the universe.

These galaxies remain intact today, but they are too distant and faint for astronomers to study in detail.

SASS stars may once have belonged to similar primitive dwarf galaxies, but they are now located within the Milky Way and are much closer, making them more accessible for understanding the evolution of ultrafaint dwarf galaxies. This could be the key.

“Now we can look for more brighter analogs in the Milky Way and study their chemical evolution without chasing these very faint stars,” Professor Froebel said.

The low chemical abundances of these stars suggest that they first formed between 12 and 13 billion years ago.

In fact, their low chemical signature was similar to what astronomers had previously measured for several ancient, ultra-dark dwarf galaxies.

Are the team’s star players from similar galaxies? And how did they come to exist in the Milky Way?

Based on a hunch, scientists studied the orbital patterns of stars and how they move across the sky.

The three stars are located in different locations throughout the Milky Way’s halo and are estimated to be about 30,000 light-years from Earth.

When astronomers used observations from ESA’s Gaia satellite to trace the movement of each star around the galaxy’s center, they noticed something strange. All three stars appeared to be in motion, compared to most of the stars in the main disk, which move like cars on a race track. Wrong way.

In astronomy, this is known as retrograde motion, and is information that the object was once accreted or pulled in from elsewhere.

“The only way to get a star wrong from other members is if you throw it the wrong way,” Professor Froebel says.

The fact that these three stars orbit in a completely different way than the rest of the galactic disk or halo, combined with the fact that their chemical abundances are low, suggests that these stars are actually It was strongly argued that it was ancient and once belonged to an earlier era, a small dwarf galaxy that fell into the Milky Way at a random angle and continued its stubborn orbit billions of years later.

The authors were interested in whether retrograde motion was a feature of other ancient stars in the halo that astronomers had previously analyzed, and they looked at the scientific literature and found similarly low strontium and barium contents, discovered 65 other stars that appear to be moving in retrograde motion as well. Galaxy flow.

“Interestingly, they are all traveling very fast, hundreds of kilometers per second, in opposite directions,” Professor Froebel said.

“They’re on the run! We don’t know why it happened, but this is the piece of the puzzle we need and we never expected it when we started.”

Researchers are keen to find other ancient SASS stars, and now have a relatively simple recipe for doing so. First, they look for stars with low chemical abundance, then track their orbital patterns for signs of retrograde motion.

Researchers hope this method will uncover a small but significant number of the universe’s oldest stars, out of the more than 400 billion stars in the Milky Way.

“I really enjoyed working with three female undergraduates. It was a first for me,” said Professor Froebel.

“This is just an example of the MIT way. It is. And anyone who says, ‘I want to participate,’ can do so, and good things happen.”

team’s paper Published in Royal Astronomical Society Monthly Notices.

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Hilary Diane Anders other. 2024. The oldest star with a small amount of neutron-capturing elements and originating from an ancient dwarf galaxy. MNRAS 530 (4): 4712-4729; doi: 10.1093/mnras/stae670

Source: www.sci.news

Physicists Investigate True Tauonium: The Heaviest and Smallest QED Atom

Quantum Electrodynamics (QED) Atoms are composed of unstructured point-like lepton pairs held together by electromagnetic forces.



An artist's impression of a true tauonium. Image credit: Fu other., doi: 10.1016/j.scib.2024.04.003.

QED atom “Like hydrogen, which is formed from protons and electrons, it is formed from lepton pairs through electromagnetic interactions,” said physicist Jinghan Hu of Peking University and colleagues.

“Their properties have been studied for things like testing QED theory, fundamental symmetries, gravity, and exploring physics beyond the Standard Model.”

“The first QED atom was discovered in 1951. It was in a bonded state and was named positronium.”

“The second one, discovered in 1960, was in a captive state and was named Muonium.”

“No other QED atoms have been discovered in the past 64 years.”

“A new collider is proposed to discover true muonium, which decays to its final state with electrons and photons,” they said.

“The heaviest and smallest QED atoms are tauonium, ditauonium, or true tauonium

in new paper in a diary science bulletinphysicists introduce a new method to identify true tauonium.

“Tauonium, which consists of tauon and its antiparticle, has a Bohr radius of only 30.4 femtometers, which is about 1/1741 times smaller than the Bohr radius of a hydrogen atom,” the researchers said.

“This means that tauonium can test the fundamental principles of quantum mechanics and QED on a smaller scale, providing a powerful tool for exploring the mysteries of the microscopic world of matter.”

“We will observe taunium by collecting data at 1.5 ab-1, which is close to the threshold for tauon pair production, in an electron-positron collider and selecting signal events containing charged particles accompanied by undetected neutrinos carrying away energy. We have demonstrated that the significance exceeds 5σ.

“This provides strong experimental evidence for the presence of tauonium.”

“We also found that by using the same data, the accuracy of measuring the tau lepton mass can be improved to an unprecedented level of 1 keV, two orders of magnitude higher than the best accuracy achieved in current experiments.”

“This result not only contributes to the accurate verification of the electroweak theory in the Standard Model, but also has profound implications for fundamental physics questions such as the universality of leptonic flavors.”

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Jin Hung Fu other. A new method for determining the heaviest QED atoms. science bulletin, published online on April 4, 2024. doi: 10.1016/j.scib.2024.04.003

Source: www.sci.news

Juno captures the reddest object in the solar system: Amalthea

NASA’s Juno spacecraft captured these views of the small red moon Amalthea and its parent planet during a flyby on March 7, 2024.

These views of Jupiter, captured by Juno on March 7, 2024, during its 59th flyby of the giant planet, offer a good look at Jupiter’s colorful bands and swirling storms, including the Great Red Spot. can. Image credit: NASA / JPL-Caltech / SwRI / MSSS / Gerald Eichstädt.

Amalthea, also known as Jupiter V, is Jupiter’s third moon in order of distance from the gas giant.

Discovered in 1892 by American astronomer Edward Emerson Barnard, the Moon is irregular and measures approximately 250 x 146 x 128 km (155 x 91 x 80 miles).

Amalthea orbits Jupiter at a distance of 181,400 km (112,717 miles) and takes 0.498 Earth days to complete one orbit.

Each time it orbits Jupiter, it rotates once on its axis, always keeping the same side facing the planet.

Amalthea is the reddest object in the solar system and appears to emit more heat from the Sun than it receives.

This is likely due to the fact that the moon’s core contains electrical currents as it orbits within Jupiter’s strong magnetic field.

Alternatively, the heat could be due to tidal forces.

These images from Juno show Jupiter’s small moon Amalthea. Image credit: NASA / JPL-Caltech / SwRI / MSSS / Gerald Eichstädt.

“Amalthea is potato-shaped and lacks the mass to pull it into a sphere,” the Juno scientists said.

“In 2000, NASA’s Galileo spacecraft revealed several surface features, including impact craters, hills, and valleys.”

“Amalthea orbits Jupiter inside the orbit of Io. Io is the innermost of Jupiter’s four large moons and takes 0.498 Earth days to orbit.”

“At the time the first of these two images was taken, Juno was approximately 265,000 kilometers above Jupiter’s clouds and at a latitude of approximately 5 degrees north of the equator,” the researchers added.

“Citizen scientist Gerald Eichstedt created these images using raw data from Juno’s JunoCam instrument and applied processing techniques that enhance the clarity of the images.”

Source: www.sci.news

Study shows ability to capture solar radiation at 1,922 degrees Fahrenheit

As the world focuses on decarbonizing power and transportation, reducing heat emissions from industrial processes remains a challenge. Although using solar energy is an attractive alternative, current solar converters have poor performance and are expensive when process temperatures above 1,000 degrees Celsius (1,832 degrees Fahrenheit) are required. In a new study, scientists at ETH Zurich show that the heat-trapping effect caused by exposing common translucent materials (such as quartz or water) to solar radiation absorbs sunlight by suppressing radiation losses at high temperatures. We have shown how the viability of the photoreceiver can be increased. They demonstrated this effect experimentally at industrially relevant temperatures of 1,050 degrees Celsius (1,922 degrees Fahrenheit).

Casati other. The solar capture effect was experimentally demonstrated at temperatures as high as 1,050 degrees Celsius. They performed stagnation experiments under concentrated thermal radiation and achieved a steady-state temperature difference of about 600 degrees Celsius between the absorber and the outer surface by using quartz as a volumetric absorption medium.Image credit: Casati other., doi: 10.1016/j.device.2024.100399.

“To tackle climate change, we need to decarbonize energy in general,” said Dr. Emiliano Casati, a researcher at ETH Zurich.

“Electricity can only be thought of as energy, but in reality, about half of that energy is used as heat.”

Glass, steel, cement, and ceramics are at the heart of modern civilization, essential to the construction of everything from car engines to skyscrapers.

However, manufacturing these materials requires temperatures in excess of 1,000 degrees Celsius and relies heavily on the combustion of fossil fuels for heat. These industries account for approximately 25% of global energy consumption.

Researchers have been exploring clean energy alternatives using solar receivers that concentrate and store heat with thousands of sun-tracking mirrors.

However, this technology has difficulty transmitting solar energy efficiently at temperatures above 1,000 degrees Celsius.

To increase the efficiency of solar receivers, Dr. Casati and his colleagues turned to translucent materials such as quartz that can trap sunlight. This is a phenomenon called the thermal trap effect.

The researchers created a heat-trapping device by attaching synthetic quartz rods to opaque silicon disks as energy absorbers.

When the device was exposed to an energy flux equivalent to 136 solar rays, the absorber plate reached a temperature of 1,050 degrees Celsius, while the other end of the quartz rod remained at 600 degrees Celsius (1,112 degrees Fahrenheit).

“Previous studies have only been able to demonstrate heat-trapping effects up to 170 degrees Celsius (338 degrees Fahrenheit),” Dr. Casati said.

“Our research shows that solar heat capture works not only at low temperatures, but also at temperatures well above 1,000 degrees Celsius. This is very important to demonstrate its potential in real-world industrial applications. is.”

The scientists also simulated the heat-trapping efficiency of quartz under various conditions using a heat transfer model.

The model showed that the heat trap achieves the target temperature at a lower concentration with the same performance, or the same concentration and higher thermal efficiency.

For example, a state-of-the-art (unshielded) receiver has an efficiency of 40% at 1,200 degrees Celsius (2,192 degrees Fahrenheit) and a concentration of 500 suns.

A 300 mm quartz shielded receiver achieves 70% efficiency at the same temperature and concentration.

A concentration of at least 1,000 suns is required for equivalent performance with an unshielded receiver.

The authors are currently optimizing the heat trapping effect and investigating new applications of the method. So far, their research is promising.

By studying other materials, such as various fluids and gases, even higher temperatures could be reached.

They also noted that the ability of these translucent materials to absorb light and radiation is not limited to solar radiation.

“Energy issues are fundamental to the survival of our society,” Dr. Casati said.

“Solar energy is readily available and the technology already exists.”

“To truly accelerate industry adoption, we need to demonstrate the economic viability and benefits of this technology at scale.”

The team's results were published online today. journal device.

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Emiliano Casati other. Captures solar heat over 1,000℃. device, published online on May 15, 2024. doi: 10.1016/j.device.2024.100399

Source: www.sci.news

Scientists say large-scale language models and other AI systems are already capable of fooling humans

In a new review paper published in journal pattern, researchers claim that various current AI systems are learning how to deceive humans. They define deception as the systematic induction of false beliefs in the pursuit of outcomes other than the truth.


Through training, large language models and other AI systems have already learned the ability to deceive through techniques such as manipulation, pandering, and cheating on safety tests.

“AI developers do not have a confident understanding of the causes of undesirable behavior, such as deception, in AI,” said Peter Park, a researcher at the Massachusetts Institute of Technology.

“Generally speaking, however, AI deception is thought to arise because deception-based strategies turn out to be the best way to make the AI ​​perform well at a given AI training task. Deception helps them achieve their goals.”

Dr. Park and colleagues analyzed the literature, focusing on how AI systems spread misinformation through learned deception, where AI systems systematically learn how to manipulate others.

The most notable example of AI deception the researchers uncovered in their analysis was Meta's CICERO, an AI system designed to play the game Diplomacy, an alliance-building, world-conquering game.

Meta claims that CICERO is “generally honest and kind” and has trained it to “not intentionally betray” human allies during gameplay, but the data released by the company shows that CICERO is “generally honest and kind” and has trained itself not to “intentionally betray” human allies during gameplay. It was revealed that he had not done so.

“We found that meta AI is learning to become masters of deception,” Dr. Park said.

“Meta successfully trained an AI to win at diplomatic games, while CICERO ranked in the top 10% of human players who played multiple games; We couldn’t train the AI.”

“Other AI systems can bluff professional human players in a game of Texas Hold’em Poker, fake attacks to beat an opponent in a strategy game called StarCraft II, or fake an opponent’s preferences to gain an advantage. Demonstrated ability to perform well in economic negotiations.

“Although it may seem harmless when an AI system cheats in a game, it could lead to a “breakthrough in deceptive AI capabilities'' and lead to more advanced forms of AI deception in the future. There is a sex.”

Scientists have found that some AI systems have even learned to cheat on tests designed to assess safety.

In one study, an AI creature in a digital simulator “played dead” to fool a test built to weed out rapidly replicating AI systems.

“By systematically cheating on safety tests imposed by human developers and regulators, deceptive AI can lull us humans into a false sense of security,” Park said. Ta.

The main short-term risks of deceptive AI include making it easier for hostile actors to commit fraud or tamper with elections.

Eventually, if these systems are able to refine this anxiety-inducing skill set, humans may lose control of them.

“We as a society need as much time as possible to prepare for more sophisticated deception in future AI products and open source models,” Dr. Park said.

“As AI systems become more sophisticated in their ability to deceive, the risks they pose to society will become increasingly serious.”

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Peter S. Park other. 2024. AI Deception: Exploring Examples, Risks, and Potential Solutions. pattern 5(5):100988; doi: 10.1016/j.patter.2024.100988

Source: www.sci.news

478-Million-Year-Old Fossil Illuminates the Diversity and Evolution of Early Euchelidae

Euchericherata A large group of arthropods that includes horseshoe crabs, scorpions, spiders, mites, ticks, and the extinct sea scorpions and snails. Abundant cetapedites The new species of Euchelycerate, which lived in what is now Morocco during the Early Ordovician period 478 million years ago, bridges the gap between modern and Cambrian species.

rebuilding the life of Abundant cetapedites. Image credit: Elissa Sorojsrisom.

“Modern scorpions, spiders, and horseshoe crabs belong to a vast lineage of arthropods that appeared on Earth about 540 million years ago,'' said Lorenzo Lustri, a paleontologist at the University of Lausanne. Ta.

“More precisely, they belong to the subphylum, chelicerates, which includes organisms equipped with pincers used specifically for biting, grasping prey, and injecting venom, and therefore chelicerates ( Euchelicerata+Pycnogonida). But what is the ancestor of this very special group?

“This question has puzzled paleontologists ever since the study of ancient fossils began.”

“Among early arthropods, it has been impossible to identify with certainty which forms share enough similarities with modern species to be considered ancestral.”

“The mystery is further complicated by the dearth of available fossils from the critical period between 505 million and 430 million years ago. This has made genealogical research easier. must.”

Abundant cetapedites. Image credit: Lustri other., doi: 10.1038/s41467-024-48013-w.

Dr. Rustri and his co-authors collected fossils of euchelicerate from the 478-million-year-old Fezouata Shale in Morocco, and found that the modern-day euchelicerate and the Cambrian (505 million-year-old) We identified a new species that binds the eucheris cerate.

with scientific name Abundant cetapeditesthe body length of this species was 0.5-1 cm.

“This animal makes it possible for the first time to trace the entire lineage of Euchelicerates, from the appearance of early arthropods to modern spiders, scorpions and horseshoe crabs,” Dr Rustri said.

“Initially, we just wanted to describe this fossil and give it a name.”

“I had no idea it would hold so many secrets.”

“It was therefore an exciting surprise to discover, after careful observation and analysis, that it also fills an important gap in the evolutionary tree of life.”

“Yet, this fossil has not yet revealed all its secrets,” he added.

“Indeed, some of its anatomical features allow for a deeper understanding of the early evolution of the eucherycerate group and perhaps link other fossil forms to this group, the similarities of which are still hotly debated. It is even possible.”

of result appear in the diary nature communications.

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L. Rustri other. 2024. Late Ordovician syndiphosrines reveal the diversity and evolution of early euchelicerates. Nat Commune 15, 3808; doi: 10.1038/s41467-024-48013-w

Source: www.sci.news

Can you trust a robot to care for your cat?

Created by scientists and explosion theory artists from the University of Nottingham cat royale is a multispecies world centered around a custom-built enclosure where three cats and a robotic arm coexist for six hours a day during a 12-day installation period.

Professor Steve Benford from the University of Nottingham and colleagues said: “Robots are finding a place in everyday life, from cleaning houses to mowing the lawn, shopping around hospitals and delivering parcels.”

“In doing so, they will inevitably have interactions and encounters with animals.”

“They could be companion animals, pets that share a home, guide dogs that help people navigate public places, but they could also be wild animals.”

“Often these encounters are unplanned and incidental to the robot’s primary mission, such as navigating a world inhabited by cats riding Roombas, guide dogs confused by delivery robots, and lawn mowing robots. Such as a hedgehog.”

“But it could also be intentional. We could also design robots to serve animals.”

“Little is known about how to design robots for animals, even though such encounters are inevitable, whether planned or not. Can you do that?

“We present Cat Royale, a creative quest to design a domestic robot to enrich cats’ lives through play.”

schneiders other. It suggests we need more than carefully designed robots to care for cats. In addition to human interaction, the environment in which the robot operates is also important. Image credit: Schneiders other., doi: 10.1145/3613904.3642115.

Cat Royale was unveiled at the World Science Festival in Brisbane, Australia in 2023, has been touring ever since, and just won a Webby Award for its creative experience.

The installation centers around a robotic arm that provides activities to make cats happier, including dragging a “mouse” toy along the floor and raising a feathered “bird” into the air. , which included feeding the cat treats.

The team then trained the AI to learn which games cats liked best so they could personalize their experience.

“At first glance, this project is about designing a robot that can play with cats and enrich the lives of families,” Professor Benford says.

“But beneath the surface, we are exploring the question of what it takes to entrust robots to care for our loved ones, and in some cases, ourselves.”

By working with Blast Theory to develop and study Cat Royale, researchers gained important insights into robot design and interaction with cats.

They had to design a robot that would pick up toys and deploy them in a way that excited the cats, all while learning which games each cat liked.

They also designed an entire world for the cat and robot to live in, providing a safe space for the cat to observe and sneak around the robot, and decorating it so that the robot had the best chance of spotting the approaching cat. did.

This means that robot design involves not only engineering and AI, but also interior design.

If you want to bring a robot into your home to take care of your loved ones, you will likely need to redesign your home.

Dr Ike Schneiders, a researcher at the University of Nottingham, said: ‘As we learned through Cat Royale, to create a multi-species system where cats, robots and humans are all taken into account, you simply need to design robots. That’s not enough.”

“We needed to ensure the animal’s health at all times, while also ensuring that the interactive installation would attract a global (human) audience.”

“Many factors were considered in this, including the design of the enclosure, the robot and its underlying systems, the different roles of the humans, and of course the selection of the cat.”

The authors announced their results in CHI 2024 meeting in Honolulu, Hawaii.

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Ike Schneiders other. Design multispecies worlds for robots, cats, and humans. CHI ’24: Proceedings of the CHI Conference on Human Factors in Computing Systems. article #593; doi: 10.1145/3613904.3642115

Source: www.sci.news

Scientists mapping Ceres’ cold traps

The dwarf planet Ceres has permanently shadowed regions in its polar regions, and these regions are interesting, similar to Mercury and the Moon. Ceres’ permanently shadowed regions were mapped by NASA’s Dawn spacecraft, and thanks to scattered sunlight, bright deposits were discovered in parts of the permanently shadowed regions. To understand more clearly the nature of Ceres’ cold-trapped ice deposits, researchers from the Planetary Science Institute and NASA’s Goddard Space Flight Center are investigating the nature of the crater, which forms a permanently shadowed region. An improved shape model was constructed.

A permanently shadowed region in the arctic region of Ceres. The color indicates the maximum inclination at which the position will be shaded throughout the trajectory. Image credit: Schorghofer other., doi: 10.3847/PSJ/ad3639.

“For Ceres, the story began in 2016, when the Dawn spacecraft, then orbiting around Ceres, glimpsed these permanently dark craters and saw bright ice deposits in some of them. “, said lead author and researcher Dr. Norbert Schorhofer. At the Planetary Science Institute.

“The 2016 discovery raised a mystery: many of the polar craters on Ceres are in shadow all year round, which lasts 4.6 Earth years on Ceres, so it remains extremely cold, but the ice Only a few of these craters hold deposits.”

“Soon, another discovery provided a clue as to why: Tides from the Sun and Jupiter cause Ceres’ axis of rotation to oscillate back and forth every 24,000 years.”

“When the Earth’s axial tilt is high and the seasons are strong, only a few craters remain in shadow throughout the year, and these craters contain bright ice deposits.”

To determine how big a shadow was inside the crater thousands of years ago, scientists created a digital elevation map and used it to perform ray-tracing calculations to cast images onto the crater’s floor. Theoretically reconstructs the shadows created by shadows.

The results are only as reliable as the digital shape model on which they are based. Note that the bottoms of these craters are always in shadow, so it is not easy to measure their depth.

NASA’s Dawn spacecraft has a very sensitive camera on board that was able to identify features on the shadowed crater floor.

Stereo images of sunny areas are often used to create digital elevation maps of sunny regions, but creating elevation maps of shaded terrain is a challenge that has rarely been addressed to date.

As part of their research, the authors developed a new technique to reconstruct heights even in shadowed parts of stereo image pairs.

These improved elevation maps can be used for ray tracing to predict the extent of cold, permanently shaded areas.

These more accurate maps yielded surprising results. The last time, about 14,000 years ago, when Ceres’ axial tilt reached its maximum, the crater on Ceres did not remain in shadow forever, and the ice within the crater quickly entered space. It must have sublimated.

“Then there is only one plausible explanation left: the ice deposits must have formed more recently,” Scholghofer said.

“The results suggest that all of these ice deposits were accumulated within the past 6,000 years.”

“That’s a surprisingly young age considering Ceres’ age is well over 4 billion years.”

“Ceres is an ice-rich body, but very little of this ice is exposed on the surface. The only exposed ice is in the aforementioned polar craters and a few small patches outside the polar regions. However, Ice is everywhere at shallow depths, so even small dry impactors can cause some of that ice to evaporate.”

“About 6,000 years ago, an asteroid fragment may have impacted Ceres, creating a temporary water atmosphere.”

“Once a water atmosphere was created, the ice would condense in the frigid crater, forming the bright deposits we still see today.”

“Alternatively, the ice deposits could have formed by an avalanche of ice-rich material. This ice would survive only within the cold, shaded crater.”

“In any case, these events are very recent on an astronomical time scale.”

The researchers also investigated the possibility that other types of ice besides water ice were trapped in these unusual craters on Ceres.

On our moon, some of the polar craters are so cold that even carbon dioxide ice and some other chemical species can remain inside them for billions of years.

Because Ceres is farther from the Sun, its polar craters are expected to be even colder than those on the Moon.

Scientists have calculated the temperature inside Ceres’ polar crater, something that has never been done before.

The answer was surprising. These craters are cold enough to hold water ice, but too warm to hold other common types of ice. Two circumstances contribute to this.

First, Ceres’s axial tilt is currently 4 degrees, higher than the Moon’s 1.5 degrees, allowing sunlight to hit more of the crater rim and scattering more light onto the crater floor.

Second, Ceres has no permanently shadowed craters in the immediate vicinity of its north pole, unlike the moon, which has one crater almost exactly at its south pole.

For these reasons, temperatures on Ceres are not as cold as on parts of the moon’s surface.

“Whatever the history of ice accumulation, it does not result from events much older than human civilization,” Dr. Scholghofer said.

of findings will appear in Planetary Science Journal.

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Norbert Schorghofer other. 2024. History of Ceres cold traps based on sophisticated geometric models. planet. Science. J 5(99); doi: 10.3847/PSJ/ad3639

Source: www.sci.news