Conversation with Kathy Willis: Utilizing the therapeutic properties of plants to alleviate anxiety and enhance overall health

We all know that being in nature is good for our health and mental wellbeing. But how does its magic work? For example, how do we explain research showing that patients who had gallbladder surgery and had a green view from their hospital windows spent less time in nature afterwards? They recovered three times faster and required far fewer painkillers than those simply staring out of a brick wall.?

It was this mystery that led botanist Kathy Willis on her latest mission. Former scientific director of the Royal Botanic Gardens, Kew, London, and now professor of biodiversity at St Edmund Hall, Oxford University, she says the discovery has changed her life. In her new book, Good NatureIn this article, she explores a growing body of research that illuminates what happens to our brains and bodies when we connect with nature. Though we tend to think of ourselves as a visual species, it turns out the benefits we derive from our other senses — smell, hearing, touch, and the mysterious “hidden senses” — are just as impressive, and sometimes even more so. There's still much to discover, but as she says, New ScientistWe have already learned many things that can improve our lives.

Kate Douglas: What happens when you observe nature?

Kathy Willis: It induces different pathways in our body. Lowers heart rate and blood pressure, Decreased stress hormones such as adrenaline And our Brainwave activity There is an increase in areas that indicate we are in a calmer, more clear minded state.

Are there any “natural” colors we should look for?

Looking at physiological indicators of calmness, Green and white leavesand Yellow or white flowers

Source: www.newscientist.com

The Mechanisms of Anticipating the Beat Drop in Your Brain

We are able to enjoy music because of our ability to recognize musical boundaries.

NDAB Creativity/Shutterstock

We may finally understand how the brain processes beat drops: People use two distinct brain networks to predict and identify the transitions between musical segments.

Musical boundaries – the moments when one part of a composition ends and another begins – are important to enjoying music, especially in the Western musical tradition. Without them, he says, your favorite hits can sound like a monotonous, random stream of notes, “like reading a text without punctuation.” Ibarra Burnat Perez At the University of Jyväskylä, Finland.

To understand how the brain processes musical boundaries, she and her colleagues analyzed brain activity while listening to 36 adults listen to instrumental pieces from three different genres: Adios Nonino Astor Piazzolla, an American progressive metal band Stream of consciousness Dream Theater and Russian Ballet Classics of Spring Festival Works by Igor Stravinsky. All of the listeners had attended school in Finland, and half of them considered themselves semi-professional or professional musicians.

The researchers found that just before musical boundaries, a brain network they call the early auditory network activates in anticipation of the end of a musical phrase. This network primarily involves auditory regions located in the posterior, or back, outer region of the brain called the cortex.

Another network becomes active during and after musical transitions. This network, called the border-transition network, is characterized by increased activity in auditory areas toward the middle and anterior, or front, parts of the cortex. Perez says that this change in brain activity between the two regions is similar to how the brain understands the difference between sentences in a language.

During and after the musical boundary, several brain regions, including the right ventrolateral prefrontal cortex, which is involved in complex cognitive tasks and decision-making, deactivate, suggesting that the brain redirects attention and resources to integrating new musical information as a new segment begins, Perez says.

Musicians and non-musicians also used these two brain networks differently. For example, musicians relied on brain regions important for higher-order auditory processing and integration, which may reflect a more specialized approach to understanding musical boundaries, Perez says. Non-musicians, on the other hand, showed greater connectivity across broader brain regions, indicating a more general approach.

In addition to shedding light on how the brain processes music, Perez says, these findings could also help develop music therapy for people who have difficulty comprehending language. For example, incorporating elements of musical boundaries into speech transitions (such as matching syllables to a melody) might make sentences easier to understand, she says.

topic:

Source: www.newscientist.com

Huge Search Yields Zero Results, Dealing Another Blow to Dark Matter

Source: www.newscientist.com

Venus Express discovers surprising rise in deuterium to hydrogen ratio in Venus’ mesosphere

Venus is often called Earth's twin, but its current surface conditions are very different from Earth's and are not suitable for life to exist: not only cannot liquid water exist due to the extreme temperatures and pressures beneath the thick cloud layer, but more importantly, there is almost no water in Venus' atmosphere. Solar Occultation Observatory in Infrared (SOIR) On ESA's Venus Express spacecraftPlanetary researchers have discovered an unexpected increase in the abundance of two variants of the water molecule.2O and HDO, and their ratio HDO/H2O in Venus' mesosphere. This phenomenon calls into question our understanding of Venus' water history and its possible past habitability.

Venus in true colors, processed from Mariner 10 images. Image credit: Mattias Malmer / NASA.

Currently, the temperature on Venus is about 460 degrees Celsius and the pressure is almost 100 times that of Earth.

The atmosphere is extremely dry, covered with thick clouds of sulfuric acid and water droplets, and most of the water resides beneath and within these cloud layers.

However, it is possible that Venus once contained as much water as Earth does.

“Venus is often called Earth's twin planet because its size is similar to Earth's,” says Dr. Hiroki Kario of Tohoku University.

“Despite the similarities between the two planets, their evolutionary processes are different. Unlike Earth, the surface conditions on Venus are extreme.”

Survey of H abundance2O and its deuterated isotope HDO (isotope) reveal insights into the history of water on Venus.

It is generally accepted that Venus and Earth originally had similar HDO/H2O ratio.

However, the ratio observed in Venus' entire atmosphere (below altitude 70 km) was 120 times higher, indicating a significant increase in deuterium over time.

This enrichment occurs primarily when solar radiation breaks down isotopes of water in the upper atmosphere, producing hydrogen (H) and deuterium (D) atoms.

Hydrogen atoms have a small mass and are therefore prone to escaping into space, so HDO/H2The O ratio gradually increases.

To understand how much hydrogen and deuterium has been released into space, it is important to measure the amount of isotopes in water at altitudes where hydrogen and deuterium are broken down by sunlight (above the clouds at altitudes of 70 km or more).

Dr. Caryu et al.2O and HDO increase between 70 and 110 km altitude, and HDO/H2In this range, the O ratio increases by an order of magnitude, reaching levels more than 1,500 times higher than in Earth's oceans.

“The proposed mechanism to explain these findings is the reaction of hydrated sulfuric acid (H2So4) aerosols,” the researchers said.

“These aerosols form just above the clouds, where temperatures drop below the dew point of sulfuric acid water, leading to the formation of deuterium-rich aerosols.”

“These particles rise to high altitudes and evaporate due to rising temperatures, releasing a much higher proportion of HDO compared to non-HDO.2“oh.”

“The steam is then conveyed downwards and the cycle begins again.”

“This study highlights two important points,” they added.

“First, altitude changes play an important role in pinpointing the location of deuterium and hydrogen reservoirs.”

“Second, the increase in HDO/H2The O ratio ultimately increases the release of deuterium, influencing the long-term change in the D/H ratio.”

“These findings encourage us to incorporate highly dependent processes into models to make accurate predictions about the evolution of D/H.”

“Understanding the evolution of Venus' habitability and water history can help us understand what makes a planet habitable and inform how to ensure Earth doesn't follow in its twin's footsteps.”

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

_____

Arnaud Mahieu others2024. Unexpected increase in deuterium to hydrogen ratio in the Venus mesosphere. PNAS 121 (34): e2401638121; doi: 10.1073/pnas.2401638121

Source: www.sci.news

UGC 3478 observed by the Hubble Space Telescope

Stunning new images taken by the NASA/ESA Hubble Space Telescope show spiral galaxy UGC 3478 in great detail.

This Hubble Space Telescope image shows UGC 3478, a spiral galaxy located 128 million light-years away in the constellation Camelopardalis. Image credit: NASA / ESA / Hubble / M. Koss / A. Barth.

3478 posts It is located in the constellation Camelopardalis and is approximately 128 million light years away from Earth.

Also known as LEDA 19228, INTREF 304, IRAS 06280+6342, Seyfert galaxyA type of galaxy centered around an active galactic nucleus (AGN).

“If you look at the long, star-filled spiral arms and the dark threads of dust that crisscross them, your eye may be drawn to a bright spot at the center of UGC 3478,” the Hubble astronomers said.

“This spot is the core of a galaxy, and there's something very special about it: it's a growing massive black hole, what astronomers call an AGN.”

“As with other active galaxies, the brightness seen here hides a supermassive black hole at the galaxy's centre,” the researchers added.

“A disk of gas spirals into this black hole, and as the material collides and heats up, it emits extremely intense radiation.”

“The spectrum of this radiation includes hard X-ray emission, which makes it clearly distinguishable from stars in the galaxy.”

“Despite the strong brightness of the compact central region, the surrounding galactic disk is still clearly visible, making it a Seyfert galaxy.”

“Astronomers know that many active galaxies are far away from Earth because their nuclei are so bright that they stand out next to other fainter galaxies.”

“Located 128 million light-years away, UGC 3478 is Earth's very own neighbour,” the astronomers said.

The new image of UGC 3478 is Hubble's Advanced Camera for Surveys (ACS) is in the near infrared and optical parts of the spectrum.

Two 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 data used to create this image come from Hubble Space Telescope surveys of nearby powerful AGNs discovered in such relatively high-energy X-rays and are expected to help us understand how galaxies interact with their central supermassive black holes,” the researchers said.

Source: www.sci.news

Astronomers find a rare hot Neptune that defies convention

The number of planets in our solar system used to be limited to only eight, excluding Pluto. These include Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, and Neptune, often remembered by the phrase “My cultured mother served us nachos.” However, with the discovery of exoplanets since 1992, the list has expanded dramatically. These exoplanets, such as PSR B1257+12 b and 51 Pegasus b, have added to the existing planets, making it challenging for students to remember them all.

Scientists have observed a pattern among exoplanets concerning their masses, distances from their stars, compositions, and other factors. Interestingly, there are very few planets with masses similar to Earth and Jupiter orbiting very close to their stars, with less than 5% of Earth’s distance from the Sun.

Research indicates that the scarcity of what they call “Hot Neptunes” might be due to the evolution of large planets. As gas giants grow, they either become comparable in size to Jupiter or lose their outer gas layers, leaving behind a rocky core like Earth’s size. Furthermore, astronomers have recently discovered new exoplanets, TOI-2374 b and TOI-3071 b, in what they refer to as Neptune’s desert.

These exoplanets stand out due to their proximity to their stars, with TOI-2374 b having a mass 56 times that of Earth and TOI-3071 b being 68 times the Earth’s mass. Despite their extreme surface temperatures, the exoplanets have not evaporated, possibly due to their high metal contents.

The observations of these exoplanets provide valuable insights for future research and exploration, potentially shedding light on unexplored phenomena in Neptune’s desert.


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Source: sciworthy.com

Matching dinosaur footprints found in Africa and South America by paleontologists

A team of paleontologists led by Southern Methodist University has discovered more than 260 dinosaur footprints from the Early Cretaceous period in Brazil and Cameroon, marking a place where land dinosaurs were last able to travel freely between South America and Africa millions of years before the two regions split apart.

Theropod dinosaur footprints discovered in the Souza Basin in northeastern Brazil. Image credit: Ismar de Souza Carvalho/SMU.

Africa and South America began to separate about 140 million years ago, causing fissures in the Earth's crust called rifts to form along pre-existing weaknesses.

As the crustal plates beneath South America and Africa moved apart, magma from the Earth's mantle rose to the surface, forming new oceanic crust as the continents moved away from each other.

And eventually the South Atlantic Ocean filled the gap between these two continents.

Evidence of some of these major events was evident between the two sites, where paleontologists from Southern Methodist University discovered footprints of three-toed theropod, sauropod and ornithischian dinosaurs dating back 120 million years. Louis Jacobs and his colleagues.

“We determined that, in terms of age, the prints are similar,” Dr Jacobs said.

“From a geological and plate tectonic point of view, they are similar. In terms of shape, they are almost identical.”

Theropod dinosaur footprints discovered in the Kum Basin in northern Cameroon. Image by Ismar de Souza Carvalho/SMU.

The researchers found the footprints in the Borborema region of northeastern Brazil and the Kum Basin in northern Cameroon, more than 6,000 kilometers (3,700 miles) apart.

“Dinosaurs left their mark on a single supercontinent called Gondwana, which separated from Pangaea 120 million years ago,” Dr Jacobs said.

“One of the newest and narrowest geological connections between Africa and South America was an elbow in northeastern Brazil that borders the present-day coast of Cameroon along the Gulf of Guinea.”

“Because the two continents were contiguous along that narrow stretch, animals on either side of the connection could potentially migrate across it.”

“Before the continental connection between Africa and South America was severed, rivers flowed and lakes formed in their drainage basins,” he said.

“The plants provided food for herbivores, supporting the food chain. Muddy deposits left in rivers and lakes contain dinosaur footprints, including those of carnivores, providing evidence that these river valleys may have provided special migration routes for life to cross the continents 120 million years ago.”

_____

This article is based on a press release provided by Southern Methodist University.

Source: www.sci.news

Pneumatic tubes are making a surprising comeback for this unexpected reason

Do you remember the days when pneumatic tubes were used for fast delivery of packages, mail, and important documents? Despite being touted as the future of delivery technology in shows like Futurama and Star Trek, pneumatic tubes started to disappear with the rise of the Internet, online purchasing, and improved communication methods.

Surprisingly, pneumatic tubes are now making a high-tech comeback, primarily in hospitals where they are used for quick, hygienic, and safe transportation of samples and sensitive information within large buildings.

How did the pneumatic tube come about?

The idea of pneumatic tubes initially included plans for a mass transit system where people would travel through tubes at high speeds using jets of air. While this idea didn’t fully materialize, some unique uses of pneumatic tubes included sending messages across tables in a Berlin bar and transporting various items like money, parts, and even fish in different industries.

Why are they returning?

Even though pneumatic tubes fell out of use in many areas, hospitals have continued to utilize them for efficient internal transfers. The modern version of pneumatic tube systems is highly automated, allowing for quick deliveries of samples and medicines within hospital premises.

Aside from hospitals, pneumatic tubes have found applications in waste disposal systems, such as the one on Roosevelt Island in New York, where these tubes whisk away trash at high speeds, eliminating the need for trucks and crews for garbage collection.

Overall, the pneumatic tubing market is expected to grow in the coming years, with valuations increasing and projects being built worldwide in various industries like dairy farms, cannabis dispensaries, and more.

It’s fascinating to see how technology that originated in the 1850s is making a comeback in the modern world.

Source: www.sciencefocus.com

The Cognitive Benefits of Owning Cats and Dogs: How Your Pets Can Prevent Cognitive Decline

As we age, our cognitive abilities, such as memory, language, and attention, tend to decline, and scientists have yet to find a way to prevent this decline.

However, there are steps you can take to slow down this decline, and recent scientific studies suggest that owning a pet could be one of them.


For instance, in a 2022 study conducted by US researchers, they examined the cognitive abilities of 1,369 older individuals covered by Medicare health insurance over a six-year period.

About half of the participants owned pets, and the researchers observed that those who owned pets experienced a slower decline in cognitive abilities compared to non-pet owners.

Furthermore, within the pet-owning group, those who had pets for a longer period performed better on the cognitive tests.

The English Longitudinal Study of Ageing (ELSA) has been tracking the aging process in people over 50 for over 25 years, helping scientists explore the positive effects pets have on the brain.

According to survey results released last year, owning a pet has been linked to slowing down cognitive decline, particularly in individuals who live alone.

Living alone can contribute to a faster decline in cognitive function and a higher risk of dementia, but having a pet appears to help mitigate these risks.

While there is still much to learn about brain health and aging, owning a pet could be a practical approach to maintaining mental sharpness as we grow older.

This article addresses the question posed by George Grainger from Truro: “Can owning a pet really slow down cognitive decline?”

If you have any inquiries, please contact us at the email provided below. For additional information, you can reach out to us via Facebook, Twitter, or Instagram (please include your name and location).

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Source: www.sciencefocus.com

According to scientific research, the most effective way to handle insults is by

The saying goes, “Sticks and stones may break my bones, but words can never hurt me.” But that’s not true. Criticism and rejection It produces brain activity that is indistinguishable from actual pain. Essentially, insults cause pain.

Insult is a complex concept. Has been studied for a long timeIt turns out that the impact of an insult depends not only on who gives it but also on who receives it.

Thus, when it comes to simple insults (insults that have no social or historical significance), the “target” has a great deal of control over the outcome.



And there are plenty of scientifically-recognized ways to successfully defuse an insult or reverse its effects.

One is to attribute category membership to the insulter, making him or her appear as a lower-status, more vulnerable to ridicule.

Someone says, “Your hair is weird,” and you respond, “OK, grandma, calm down,” and you put them in the “old, unfashionable, out of date” category, making them look even worse, especially if they’re a guy in his 20s and there’s no way they could be your grandma.

Some people recommend finding something the insulter says about themselves and highlighting it.

They say, “I don’t know why. [your attractive partner] If they ask you, “Shall I explain it to you? In crayons?”, they mean to insult you, but their response comes across as an admission that they are easily confused.

And then there is co-constructed critique, which takes the insult and builds on it, which de-fans the insult.

“You’re fat!” they say. You say, “I hope so, I’ve spent enough money to get here.”

There are countless other counter-attacks, but they all revolve around a central theme of not empowering the insulter, not elevating the insulter’s status, and maintaining control of the narrative and the interaction.

This article is a response to a question emailed to me by Archie Fox: “What’s the best way to respond to an insult?”

If you have any questions, please send them to the email address below. For further information, please contact:or send us a message Facebook, Xor Instagram Page (be sure to include your name and location).

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NASA reveals astronauts stranded in space will wait for SpaceX spacecraft instead of returning in Boeing capsule.

NASA announced on Saturday that SpaceX will bring home the two astronauts who have been stranded on the International Space Station since early June due to issues with Boeing’s spacecraft. Astronauts Butch Wilmore and Suni Williams will return to Earth aboard SpaceX’s Crew Dragon spacecraft instead of the Boeing Starliner spacecraft. This decision follows months of uncertainty within the space agency regarding the safe return of the crew members on a mission initially planned to last eight days.

The problems with the Starliner spacecraft have posed a significant setback for Boeing’s space program, which has been struggling to keep up with SpaceX. The Starliner program was already over budget and behind schedule before the launch of Wilmore and Williams in June.

Top NASA officials, led by Administrator Bill Nelson, held a formal review in Houston and based their decision on the results of tests conducted in orbit and on the ground. The announcement to choose SpaceX for the astronauts’ return was made during a press conference at NASA’s Johnson Space Center.

Although the return plans have been finalized, Wilmore and Williams will remain on the space station for approximately six more months before coming back in February. NASA revealed that two seats on SpaceX’s next launch, Crew 9, will be left empty to accommodate the astronauts on their return journey.

The Crew 9 mission is scheduled to launch on September 24 from NASA’s Kennedy Space Center in Florida. Meanwhile, the troubled Starliner spacecraft will return to Earth without its crew.

Source: www.nbcnews.com

Fires persist on the Pacific Crest Trail, leading to closures and evacuations

The Pacific Crest Trail (PCT) is facing increasing challenges due to wildfires and their aftermaths, making sections of the trail hazardous and leading to sudden road closures. Long-distance hikers are experiencing significant environmental transformations as wildfires ravage the area, while rural communities near the trail are stepping up to assist hikers during wildfire emergencies.

According to Riley, wildfires are becoming more frequent and unpredictable, affecting a larger number of trails, users, and communities. The PCT, which traverses diverse terrains like the Mojave Desert, Sierra Nevada Mountains, and Cascade Mountains, attracts thousands of long-distance hikers and hundreds of thousands of day hikers annually.

However, the combination of global warming-induced extreme temperatures and decades of aggressive fire suppression has led to intense wildfire seasons altering the landscape along the PCT. Climate change effects are noticeable along the trail, with local weather scientist John O’Brien remarking, “This is an extended tour of climate history.”

Trail crews on the Pacific Crest Trail pass through burned areas of the Eagle Creek Fire in the Columbia River Gorge near Portland, Oregon, in 2018.Jamie Hale/The Oregonian via The Associated Press

Apart from fire risks, climate change is intensifying water scarcity along the trail and affecting wildlife populations. Glacial retreat in higher elevations is exposing more slippery rock, while river levels are peaking earlier in the season, leading to hazardous crossings.

Hikers like Karen Altergott have faced extreme weather conditions, from heavy late-season snowfall to intense heat waves, prompting concerns about the impact on health. Altergott emphasized the need for preparedness and flexibility when dealing with changing trail conditions.

Karen Altergott.Courtesy of Karen Altergott

The PCT community is coming together to tackle these challenges, with the Pacific Crest Trail Association releasing a smartphone app to help hikers navigate wildfire closures. Local “trail angels” are also stepping up to provide aid, transport, and support to stranded hikers during emergencies.

Becky Wade and her partner Jeff McCabe.Courtesy of Becky Wade

Becky Wade and Jeff McCabe, who have experienced evacuations due to wildfires, exemplify the importance of community support. Their efforts in assisting hikers around fire-affected areas highlight the crucial role of local residents in ensuring hiker safety along the PCT.

Although wildfires and their aftermath present challenges, hikers like Will Geolis attest to the enduring value of the PCT experience. While adapting to changing trail conditions is necessary, the trail’s community and scenic beauty remain priceless.

Joris aptly sums up the essence of the PCT experience, emphasizing that it’s the people and the journey that truly matter, rather than completing a continuous hike along the trail.

Source: www.nbcnews.com

Super-Earths and Sub-Neptunes have significantly higher water content than previously believed

Water is a key component of exoplanets, and its distribution – on the surface or deep inside – has a fundamental impact on the planet’s properties. A new study suggests that for Earth-sized planets and planets with more than six times Earth’s mass, the majority of water resides deep within the planet’s core.



Most of the water isn’t stored on the surface of exoplanets, but deep within their cores and mantles. Image courtesy of Sci.News.

“Most of the exoplanets known to date are located close to their stars,” said Professor Caroline Dohn of ETH Zurich.

“That means they consist mainly of hot worlds with oceans of molten magma that haven’t yet cooled enough to form a solid mantle of silicate rock like Earth’s.”

“Water is very soluble in these magma oceans, unlike, say, carbon dioxide, which quickly outgasssssssssssss and rises into the atmosphere.”

“The iron core is beneath a molten silicate mantle. So how does water partition between the silicates and the iron?”

“It takes time for the iron core to form. Most of the iron is initially contained in the hot magma soup in the form of droplets.”

“The water trapped in this soup binds to these iron droplets and together they sink to the center. The iron droplets act like a lift force, being carried downward by the water.”

Until now, such phenomena were known to occur only under moderate pressures, which also exist on Earth.

It was not known what would happen on larger planets with higher internal pressures.

“This is one of the key findings of our study,” Professor Dorn said.

“The larger and more massive the planet, the more likely the water is to be integrated into the core, together with the iron droplets.”

“Under certain circumstances, iron can absorb up to 70 times more water than silicates.”

“But because of the enormous pressure at the core, the water no longer exists in the form of water molecules, but in the form of hydrogen and oxygen.”

The research was sparked by an investigation into the Earth’s water content, which four years ago led to a startling result: the Earth’s surface oceans contain only a tiny fraction of the planet’s total water.

More than 80 of Earth’s oceans may be hidden within it.

This is shown by simulations that calculate how water would have behaved under conditions when the Earth was young, so experiments and seismological measurements are compatible.

New discoveries about the distribution of water within planets will have a dramatic impact on the interpretation of astronomical observational data.

Astronomers can use telescopes in space and on Earth to measure the weight and size of exoplanets under certain conditions.

They use these calculations to create mass-radius diagrams that allow them to draw conclusions about the planet’s composition.

“Ignoring water solubility and distribution, as has been done in the past, can lead to a massive underestimation of the water volume, by up to a factor of ten,” Prof Doern said.

“There’s a lot more water on the planet than we previously thought.”

The distribution of water is also important if we want to understand how planets form and develop: any water that sinks to the core will remain trapped there forever.

However, dissolved water in the mantle’s magma ocean can degas and rise to the surface as the mantle cools.

“So if we find water in a planet’s atmosphere, there’s probably even more water in its interior,” Prof Dorn said.

Water is one of the prerequisites for life to develop, and there has long been speculation as to whether water-rich super-Earths could support life.

Calculations have since suggested that too much water could be detrimental to life, arguing that on such a watery world, an alien layer of high-pressure ice would prevent vital exchange of materials at the interface between the ocean and the planet’s mantle.

Current research has come to a different conclusion: Most of the water on super-Earths is locked away in their cores, rather than on their surfaces as previously assumed, so planets with deep aqueous layers are probably rare.

This has led astronomers to speculate that planets with relatively high water content could potentially form habitable environments like Earth.

“Their study sheds new light on the possibility that worlds rich enough in water to support life may exist,” the authors said.

of study Published in the journal Natural Astronomy.

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H. Luo othersThe interior as the main water reservoir of Super-Earths and Sub-Neptunes. Nat AstronPublished online August 20, 2024; doi: 10.1038/s41550-024-02347-z

Source: www.sci.news

New insights into the evolutionary origins of tardigrades from Cretaceous amber fossils

Tardigrades are a diverse group of microinvertebrates widely known for their remarkable ability to survive. Molecular clocks suggest that tardigrades diverged from other panarthropods (arthropods, tardigrades, velvet worms, and lobopods) before the Cambrian, but the fossil record is extremely poor. Now, paleontologists have described a new species of tardigrade and redescribed previously known species. readBoth are from Canadian Cretaceous amber.

Artistic Restoration read (Top) and Aerobius dactylus (Bottom) A hypothetical fossilization environment. Image courtesy of Franz Anthony.

First discovered in 1773, tardigrades are a diverse group of microscopic invertebrates best known for their ability to survive in extreme environments.

Also known as tardigrades or moss pigs, these creatures can live up to 60 years and grow to a size of up to 0.5mm. They are best seen under a microscope.

They can survive up to 30 years without food or water, and can survive temperatures as low as -272°C and as high as 150°C for a few minutes, and as low as -20°C for decades.

Tardigrades can withstand pressures ranging from nearly zero atmospheres in outer space to 1,200 atmospheres at the bottom of the Mariana Trench, and can also tolerate radiation levels of up to 5,000-6,200 Gy.

They survive by entering a state of suspended animation called biostasis, using proteins that form a gel inside the cells and slow down vital processes.

“Tardigrades are microscopic invertebrates characterized by a compact body shape with lobopod legs with four pairs of claws, and are closely related to the clawed pterygota and euarthropods. Panarthropods“Harvard doctoral student Mark Mapalo and his colleagues said:

“Tardigrades are widely known for having several species with cryptobiotic capabilities that allow them to survive extreme conditions such as the vacuum of space, ionizing radiation and freezing temperatures. Tardigrades are also found in marine, freshwater and terrestrial habitats around the world.”

“Despite their ubiquity in the modern biosphere, tardigrades have a notoriously poor fossil record, and research into their macroevolution, such as the origin of their body shape, the timing of their terrestrialization, and the acquisition of their cryptic abilities, is limited.”

“Currently, only four fossil crown-group tardigrades are known, all preserved as amber inclusions, but only two of these have an established taxonomic position relative to extant tardigrades.”

Aerobius dactylusImages/Photos: Mapalo others., doi: 10.1038/s42003-024-06643-2.

For the study, the authors looked at a piece of amber containing a tardigrade fossil that was discovered in Canada in the 1960s. read and what was presumed to be another tardigrade, which was virtually unexplained at the time.

Using confocal laser scanning microscopy, a technique commonly used to study cell biology, the researchers were able to examine the microscopic structure of the tardigrade fossils in astonishing detail.

This study read It has been identified as a new species in the Tardigrade family tree, Aerobius dactylus.

“Both were found in the same Cretaceous amber, which means that these tardigrades coexisted with dinosaurs,” said Dr Javier Ortega-Hernández of Harvard University.

read The seven claws are well preserved, and those that curve towards the body are smaller than those that curve away from it, a pattern seen in modern tardigrades.”

“The second, previously unidentified specimen had claws of equal length on each of the first three pairs of legs, but the outer claws on the fourth leg were longer.”

Both species serve as important calibration points for an analysis called a molecular clock analysis, which helps scientists estimate important evolutionary timing.

For example, new research suggests that modern tardigrades likely branched off during the Cambrian period, more than 500 million years ago.

The study also sheds light on the origins of tardigrades' remarkable ability to survive extreme environments by entering a state of torpor.

“This study estimates that this survival mechanism likely evolved during the middle to late Palaeozoic and may have played a key role in helping tardigrades survive the end-Permian mass extinction, one of the most severe extinction events in Earth's history,” Dr Ortega-Hernández said.

of result Published in a journal Communication Biology.

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MA Mapalo others2024. Inclusions in Cretaceous amber shed light on evolutionary origins of tardigrades. Communication Violet 7, 953; doi: 10.1038/s42003-024-06643-2

Source: www.sci.news

Hot Gulf of Mexico experiences unusually calm hurricane season

summary

  • Despite warm ocean temperatures, hurricane season is on a lull.
  • This season is expected to be much more active than usual and is off to a record-breaking start.
  • Still, the unofficial peak of hurricane season is on September 10, so scientists wouldn’t be surprised if cyclonic activity picks up again soon.

The Gulf of Mexico is scorching hot, but hurricane season is on a lull (at least temporarily) — a surprise to researchers who say there’s a lot brewing in the Atlantic, but no storms are showing up on radar.

The National Hurricane Center said on Friday No tropical cyclone activity expected for at least a week.

“Nothing is happening, which is extremely quiet and odd given the warm temperatures in the Atlantic and the La Niña climate pattern,” said Philip Klotzbach, a meteorologist at Colorado State University who specializes in seasonal hurricane forecasting in the Atlantic basin. “It’s a head-scratching situation right now.”

The La Niña weather phenomenon that scientists are predicting will develop this fall is closely linked to hurricanes, as is warming water in the Atlantic Ocean, with ocean heat content in the Gulf of Mexico at its highest since 2013, according to data from the University of Miami.

Sea surface temperatures in the North Atlantic are trending about 1.8 degrees above normal. According to the University of Maine’s Climate Reanalysis InstrumentThis trend is especially evident in the Gulf of Mexico.

Warmer oceans increase hurricane energy through heat, increasing the risk of storms intensifying rapidly.

“We have plenty of fuel. It’s not going to hinder our season,” Klotzbach said.

Hurricane season begins on June 1 and ends on November 30. Hurricane scientists had predicted this year’s hurricane season would be record-breaking, but it got off to a record-breaking start in June with Hurricane Beryl being the first Category 4 storm to form in the Atlantic. Then, the slow-moving Hurricane Debbie dumped incredible rain on several southeastern states in early August. But since then, it’s been relatively quiet.

Steve Bowen, chief scientific officer at global reinsurance broker Gallagher Re, said weather trends off the coast of West Africa, including a strengthening monsoon, may have prevented tropical storms from developing in the Atlantic basin.

But that may not last long: The unofficial peak of hurricane season is September 10.

“I wouldn’t be surprised if we get what’s called a backloading season with pretty good activity through September, October, and possibly November,” Bowen said.

Although things have calmed down recently, scientists believe this season has been quite active so far.

“We’ve already had two landfalls in the United States,” Bowen said. “Typically, the first major hurricane doesn’t form until August 31st. … Just looking at the statistics, we’re well ahead of normal.”

Source: www.nbcnews.com

Neolithic architects utilized scientific understanding to construct massive megalithic structures.

Inside the monument known as Mengadolmen in Spain

Miguel Angel Blanco de la Rubia

Neolithic people appear to have understood advanced concepts from sciences such as physics and geology, and used this knowledge to build megalithic monuments in southern Spain.

The dolmen, called Menga Dolmen, was built between 3600 and 3800 BC and is one of the oldest megalithic structures in Europe. The covered enclosure is made of 32 large stones, some of which are the largest ever used for such a structure. The heaviest stone weighs over 130 tonnes, more than three times the heaviest stone at Stonehenge in England, which was built more than 1000 years later.

“[In the Neolithic Period]”It must have been an impressive experience to experience these huge stone structures,” he said. Leonardo Garcia San Juan He studied at the University of Seville in Spain. “It still moves me. It still makes an impression on me.”

García Sanjuan and his colleagues are now conducting a detailed geological and archaeological analysis of the stones to deduce what knowledge Menga's builders needed to construct the monument in the city of Antequera.

Paradoxically, they found that the rock was a type of relatively brittle sandstone, meaning that it was at high risk of breaking, but the team found that they could compensate for that risk by shaping the rock, locking it into a very stable overall structure.

Neolithic people would have needed some way to make the stones fit together very snugly, Garcia-Sanjuan says. “It's like Tetris,” he says. “The precision, and how tightly each stone is fastened to each other, forces you to think they had some concept of angles, even if it was just rudimentary.”

The researchers also discovered that the 130-ton stone, laid horizontally on top to form part of the roof, has a raised surface in the middle and slopes down at the edges, which helps distribute forces in the same way an arch does and strengthens the roof, Garcia-Sanjuan says. “To our knowledge, this is the first time the principle of the arch has been documented in human history.”

The purpose of the mengas is unknown, but they were positioned to create unique light patterns inside them during the summer solstice, and the stones are protected from water damage by layers of carefully pounded clay, supporting evidence of their builders' knowledge of architecture and engineering.

“They knew about geology and the properties of the rocks they were working with,” Garcia San Juan says. “When you put all of this together — engineering, physics, geology, geometry, astronomy — you get what you call science.”

There are other Neolithic structures in France of a similar size to Menga, but less is known about how it was built, Garcia San Juan said. “To date, Menga is unique both in the Iberian peninsula and in Western Europe.”

“What's surprising is how sophisticated it is.” Susan Greaney “This architectural understanding of how weight is distributed is something I've never seen anywhere before,” says Professor David Schneider of the University of Exeter in the UK. But, she adds, this may be a testament to an understanding of architecture and engineering rather than an understanding of science.

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Source: www.newscientist.com

Mpox: Understanding the Fatality Rate and Treatment Options of the Virus

Health workers assess a suspected case of MPOX in North Kivu province, Democratic Republic of Congo.

Arlette Basij/Bloomberg via Getty Images

Mpox, formerly known as monkeypox, is currently in the midst of an outbreak in the Democratic Republic of Congo (DRC) and neighboring countries, with the surge in cases being blamed in part on a new variant that is thought to be more deadly than the variant of the Mpox virus that caused a global outbreak in 2022. But there are treatments that may help.

How deadly is MPOX?

Studies have shown that the mortality rate among people infected with the currently circulating lineage I variant of MPOX is approximately 1-2%. 11 percentThe variation in reported mortality rates is probably due to differences in affected populations and problems with disease surveillance, Lilith Whittles At Imperial College London.

For example, infants and children with underdeveloped immune systems may be more likely than adults to develop serious, even fatal, infections, and people with suppressed immune systems, such as those with HIV, may also be more susceptible, she says.

Additionally, some areas have little access to health care and limited surveillance for MPOX. As a result, health care providers only catch the most severe cases and miss milder cases, making the death rate appear higher than it actually is. If MPOX symptoms are increasingly misdiagnosed as other illnesses, like measles or chickenpox, more cases will go undetected, Whittles says.

In fact, most deaths from MPOX occur due to complications such as sepsis, where infection enters the bloodstream and causes organ failure, and inflammation caused by the MPOX virus that damages the lungs, he said. Piero Oriaro At Oxford University.

What are the MPOX treatment options?

In the Democratic Republic of Congo and neighboring countries where the current outbreak is occurring, there are few treatments specific to MPOX. Instead, doctors focus on treating symptoms, which usually last two to four weeks, such as reducing fever and headaches with paracetamol (acetaminophen) and cleaning skin lesions to prevent bacterial infections, he said. Jean-Claude Udahemka At the University of Rwanda.

In the UK and US, doctors can use the antiviral drug Tecovirimat to treat people with severe smallpox. Originally developed to treat smallpox, its use against the disease was based on animal studies in which it improved survival rates compared to a placebo. Tecovirimat works by binding to a protein on the surface of both variola and smallpox that the virus uses to attack. Freeing itself from infected cells spreads to other cells.

Doctors in the United States and the United Kingdom can also treat MPOX with other antiviral drugs, such as brincidofovir and cidofovir. Protecting mice from lethal doses of the mpox virus. Both brincidofivir and cidofovir Interfering with enzymes Used by viruses to replicate their genome.

Another treatment, known as VIGIV, involves injecting people with smallpox with antibodies against smallpox taken from people who have had the smallpox vaccine, thus strengthening their immune response to the virus.

How effective is mpox treatment in humans?

Animal studies suggest that these treatments may be effective against MPOX, but their effectiveness in humans is unknown. Early results from a recent randomized controlled trial (best medical evidence) in the Democratic Republic of Congo suggest that tecovirimat does not accelerate the progression of MPOX. Healing of painful lesions in children and adults infected with lineage I variants of MPOX.

Nonetheless, the researchers found that the MPOX mortality rate for participants who received the antiviral drug was 1.7 percent, an improvement over the 3.6 percent mortality rate typically seen in the Democratic Republic of Congo. But this can be partly explained by the fact that participants in the trial received close care in hospital, Oriaro says.

Ultimately, better treatments and a better understanding of MPOX's lethality will be essential to protect people, especially in the Democratic Republic of Congo, from the ongoing epidemic. Lucille Blumberg She is a researcher at the University of Pretoria in South Africa. “There's a lot of work to be done,” she says.

topic:

  • virus/
  • Infection

Source: www.newscientist.com

State media reports show that Chinese scientists are using lunar soil to produce water

Chinese scientists have made a groundbreaking discovery in producing large amounts of water using lunar soil collected from the 2020 mission, as reported by state-run CCTV on Thursday.

The Chang’e-5 mission in 2020 marked a significant milestone in collecting lunar samples after a 44-year hiatus. Scientists from the Chinese Academy of Sciences found high amounts of hydrogen in minerals present in the lunar soil. When heated to extreme temperatures, this hydrogen reacts with other elements to generate water vapor, according to China Central Television.

CCTV reported, “After extensive research and verification over three years, a new method has been identified for producing significant quantities of water from lunar soil. This discovery is anticipated to play a crucial role in designing future lunar research and space stations.”

This finding could have significant implications for China’s long-standing ambition to establish a permanent lunar base, amid the race between the United States and China to explore and exploit lunar resources.

On August 26, 2021, a small vial containing lunar soil brought back from the moon by China’s lunar probe Chang’e-5 was placed in Beijing.Ren Hui/VCG via Getty Images file

NASA Administrator Bill Nelson has expressed concerns about China’s rapid progress in space exploration and the potential risk of Beijing controlling valuable lunar resources.

According to state media, the new technique can yield approximately 51-76 kilograms of water from one ton of lunar soil, enough to fill over 100 500ml bottles or sustain the daily water needs of 50 individuals.

China aims for its recent and upcoming lunar missions to establish a basis for constructing the International Lunar Research Station (ILRS), a collaborative project with Russia.

The Chinese space agency’s plan includes establishing a lunar “base station” at the moon’s south pole by 2035, followed by a lunar orbiting space station by 2045.

This discovery coincides with ongoing experiments by Chinese scientists on lunar samples obtained from the Chang’e-6 probe in June.

While the Chang’e-5 mission collected samples from the moon’s near side, Chang’e-6 gathered lunar soil from the far side, perpetually hidden from Earth.

The significance of lunar water surpasses sustaining human settlement; NASA’s Nelson mentioned to NPR in May that moon water could be utilized to produce hydrogen fuel for rockets, potentially fueling missions to Mars and beyond.

Source: www.nbcnews.com

The World’s Leading AI Expert Predicts a Strange 2050

Ray Kurzweil is a prominent figure in the field of artificial intelligence, with over 60 years of experience. He has achieved many milestones in AI development, such as inventing the first commercially available large vocabulary speech recognition software. Kurzweil’s expertise in AI was recognized with the National Medal of Technology by President Bill Clinton in 1999 and his induction into the National Inventors Hall of Fame in 2002.

In addition to his practical accomplishments, Kurzweil is known for his accurate predictions about future technologies. His book “The Singularity is Near,” published in 2005, explored the rapid advances in computing and AI, predicting the future impact of AI on society. In his follow-up book, “The Singularity is Approaching,” Kurzweil delves into how AI will reshape our lives.

Kurzweil forecasts significant changes ahead, particularly in the realm of artificial general intelligence (AGI). He believes AGI will surpass human abilities in various cognitive tasks, potentially becoming available by 2029. The pace of technological advances in AI is accelerating exponentially, with Kurzweil emphasizing the need to prepare for the evolution of AI.

Another groundbreaking prediction by Kurzweil is the potential end of aging through advancements in healthcare and technology. He envisions a future where aging can be slowed down or prevented entirely, with life expectancy increasing significantly. Kurzweil’s optimistic outlook extends to the integration of AI with human intelligence by 2050, creating a new form of intelligence through the merging of human brains with computers.

As a futurist, author, and inventor, Ray Kurzweil continues to shape the conversation around AI and its impact on society. His visionary insights invite us to consider the possibilities and challenges that lie ahead in the ever-evolving landscape of artificial intelligence.

Source: www.sciencefocus.com

Get ready for an influx of tarantulas in the US: Here’s what you need to know

Reports suggest that Americans are set to witness a peculiar and somewhat alarming occurrence as swarms of tarantulas are poised to invade certain regions of the country.

Despite the ominous connotations associated with this event, it is actually a normal annual happening where thousands of spiders are on the lookout for mates, particularly in Colorado, Texas, New Mexico, and Arizona.

Naturally, one might feel inclined to take action upon witnessing such a spectacle, but how challenging is it to manage these swarms? And what level of threat do they truly pose?

What’s prompting the spider swarms?

The appearance of swarms of animals and insects typically indicates two main reasons: migration or mating. In the case of American tarantulas, it is primarily due to the latter. It is an intriguing scenario distinct from what we might typically envision.

“Every year, male tarantulas come out in search of a mate, while females remain in their burrows releasing pheromones to attract males,” stated Lauren Davidson, an entomologist at the Houston Museum of Natural Science. “It’s a fascinating phenomenon that occurs based on weather conditions and geographical location.”

Male tarantulas usually have a short lifespan solely for the duration of the mating season, with only mature males actively seeking a mate. Upon detecting a female’s pheromones, the male tarantula initiates a mating ritual by drumming near the entrance of her burrow. If the female is receptive, she will come out to meet him.


Wondering where you might encounter these males? Tarantula mating season varies across different regions; for instance, mating in Texas typically occurs in early summer, while in Colorado and New Mexico, it can extend until October.

Davidson notes, “The timing is consistent each year, and these events are often unnoticed by urban residents. It’s a cyclical process that occurs at night due to tarantulas being nocturnal.”

Though it may appear to be migration, the spiders are primarily in search of mates within close proximity to their usual habitats, generally traveling no more than a kilometer from home.

Encountering a tarantula: What to do?

While encounters with tarantulas may be rare, it is not impossible. If you do come across one, remain calm as these spiders are harmless. Despite their intimidating size, their venom is similar to that of a bee sting and bites are infrequent. Tarantulas typically avoid human contact and resort to kicking out irritating hairs if threatened.

Direct contact with these hairs can cause itchiness and irritation, but one would need to be in close proximity to the spider for that to occur. Davidson reassures, “Many people travel to witness these tarantulas as they are docile creatures and safe to handle.”


About our expert

Lauren Davidson: Associate Curator of Entomology at the Houston Museum of Natural Science and Manager of the Cockrell Butterfly Center. Davidson has authored several children’s books focusing on entomology education.

Read more:

Source: www.sciencefocus.com

Here’s why scientists are planning to construct a massive “bioreservoir” on the moon

Life on Earth has faced various threats over millions of years, from asteroids to pandemics to climate change. According to the IPCC, nearly one in five terrestrial species is at risk of extinction by 2100 due to rising global temperatures.

Marine life is also in peril, with coral reefs disappearing rapidly. Dr. Mary Hagedorn, a coral reef expert, has been working on cryopreserving coral to ensure its survival and potential reintroduction into ecosystems.

Her innovative idea involves creating a lunar biorepository to store frozen cell samples of key species for ecosystem reconstruction. The moon’s cold temperatures and protection from radiation make it an ideal location for such a vault.

The focus is on preserving fibroblasts, which can be reprogrammed into different cell types, including stem cells for cloning. This initiative aims to safeguard Earth’s ecosystems and potentially support future human space exploration, such as Mars missions.


While the concept may seem futuristic, the team has already begun freezing cell samples from species like the starry goby for testing. The ultimate goal is to send diverse genetic samples to the lunar vault to ensure the preservation of essential species.

Creating a biorepository on the moon presents logistical challenges but could be achievable with NASA’s support and funding. Future generations might benefit from this innovative approach to conservation and space exploration.


Dr. Mary Hagedorn and Professor Ian Crawford are leading experts in this field, with a focus on conservation, lunar science, and astrobiology. Their research and work contribute to the understanding of ecosystems and the future of space exploration.

  • Learn more about the UK mission to the Moon
  • Discover how to build a moon base

Source: www.sciencefocus.com

Physicists Witness the First Observation of Antihyperhydrogen 4

Physicists from the STAR Collaboration have observed an antimatter hypernucleus, antihyperhydrogen-4, consisting of an antihypernucleus, an antiproton, and two antineutrons, in nuclear collisions at the Relativistic Heavy Ion Collider (RHIC) at the U.S. Department of Energy's Brookhaven National Laboratory.

Artistic representation of antihyperhydrogen-4 produced in the collision of two gold nuclei. Image courtesy of the Institute of Modern Physics.

“What we know in physics about matter and antimatter is that, apart from the opposite charge, antimatter has the same properties as matter – the same mass, the same lifetime before decaying, and the same interactions,” said Junlin Wu, a graduate student at Lanzhou University and the China Institute of Modern Physics.

“But in reality, our universe is made up of antimatter rather than matter, even though equal amounts of matter and antimatter are thought to have been created during the Big Bang about 14 billion years ago.”

“Why our universe is populated with matter remains a question, and we don't yet have a complete answer.”

“The first step in studying the asymmetry between matter and antimatter is to discover new antimatter particles. This is the basic idea of ​​this research,” added Dr Hao Qiu, a researcher at the Institute of Modern Physics.

STAR physicists had previously observed atomic nuclei made of antimatter produced in RHIC collisions.

In 2010, they detected an antihypertriton, the first example of an antimatter nucleus containing a hyperon, a particle that contains at least one strange quark rather than just the light up and down quarks that make up ordinary protons and neutrons.

Just a year later, STAR physicists broke that massive antimatter record by detecting antihelium-4, the antimatter equivalent of a helium nucleus.

Recent analysis suggests that antihyperhydrogen 4 may also be feasible.

But detecting this unstable antihypernucleus is a rare event: all four components (one antiproton, two antineutrons and one antilambda) need to be ejected from the quark-gluon soup produced in the RHIC collision in just the right place, in the same direction and at just the right time, briefly becoming bound together.

“It's just a coincidence that these four component particles appear close enough together in the RHIC collision that they can combine to form an antihypernucleus,” said Brookhaven National Laboratory physicist Lijuan Luan, one of the STAR collaboration's co-spokespeople.

To find antihyperhydrogen-4, STAR physicists studied the trajectories of particles produced when this unstable antihypernucleus decays.

One of these decay products is the previously detected antihelium-4 nucleus, and the other is a simple positively charged particle called a pion (pi+).

“Antihelium-4 had already been discovered with STAR, so we used the same methods as before to pick up those events and reconstruct them with the π+ track to find these particles,” Wu said.

“It is simply by chance that these four component particles emerge from the RHIC collision close enough together to combine to form an antihypernucleus,” said Dr. Lijuan Luan, a research scientist at Brookhaven National Laboratory.

RHIC's collisions produce huge amounts of pions, and physicists have been sifting through billions of collision events to find the rare antihypernuclei.

The antihelium-4 produced by the collision can pair up with hundreds or even a thousand pi+ particles.

“The key was to find an intersection point where the trajectories of the two particles had a particular characteristic – a collapse vertex,” Dr. Luan said.

“That is, the collapse apex must be far enough away from the collision point that the two particles could have originated from the decay of an antihypernucleus that formed shortly after the collision of the particle originally produced in the fireball.”

STAR researchers worked hard to eliminate the background of all other potential collapse pair partners.

Ultimately, their analysis found 22 candidate events with an estimated background count of 6.4.

“That means that about six of what appear to be antihyperhydrogen-4 decays could just be random noise,” said Emily Duckworth, a doctoral student at Kent State University.

Subtracting that background count from the 22, physicists can be confident that they have detected about 16 actual antihyperhydrogen-4 nuclei.

The results were significant enough to allow scientists to make a direct comparison between matter and antimatter.

They compared the lifespan of antihyperhydrogen 4 to that of hyperhydrogen 4, which is made from normal matter variants of the same building blocks.

They also compared the lifetimes of another matter-antimatter pair, antihypertritons and hypertritons.

Neither difference was significant, but the authors were not surprised.

“This experiment tested a particularly strong form of symmetry,” the researchers said.

“Physicists generally agree that this symmetry breaking is extremely rare and is not an answer to the imbalance of matter and antimatter in the universe.”

“If we saw this particular breaking of symmetry, we would basically have to throw a lot of what we know about physics out the window,” Duckworth said.

“So in a way it was reassuring that symmetry still worked in this case.”

“We agree that this result provides further confirmation that our model is correct and marks a major step forward in the experimental study of antimatter.”

Team work Published in a journal Nature.

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STAR Collaboration. Observation of the antimatter hypernucleus antihyperhydrogen 4. NaturePublished online August 21, 2024, doi: 10.1038/s41586-024-07823-0

This article is based on an original release from Brookhaven National Laboratory.

Source: www.sci.news

A new carnivorous dinosaur species discovered in Kyrgyzstan

New genus and species of large theropod dinosaur named Alpkaraqsh Kyrgyzics. It was discovered in the Middle Jurassic Barabansai Formation in the northern Fergana Basin of Kyrgyzstan.

Reconstructing your life Alpkaraqsh Kyrgyzics.Image credit: Joschua Knüppe.

Alpkaraqsh Kyrgyzics roamed the Earth during the Callovian Period of the Jurassic Period, between 165 and 161 million years ago.

This ancient predator was 7 to 8 metres (23 to 26 feet) long and had highly prominent “eyebrows” on a part of the skull behind the eye sockets, called the postorbital bone, which indicates the presence of horns in this area.

Alpkaraqsh Kyrgyzics belongs to Metriacanthosauridae, a group of medium- to large-sized allosauroid theropod dinosaurs characterized by high, arched skulls, elongated, dish-like neural spines, and slender hind limbs.

“Theropod dinosaurs are well-known predators, similar to modern birds,” said Professor Oliver Rauhut from the SNSB – Bayerische Staatssammlung für Paläontologie und Geology and his colleagues.

“A wide variety of theropods are known from the Mesozoic Era, the age of dinosaurs.”

“Just as lions today live mainly in Africa and tigers only in Asia, for example, Allosaurus was widespread throughout North America and southwestern Europe during the Jurassic, but a similarly sized Allosaurus lived in China.”

However, the region between Central Europe and East Asia was previously unknown, and no large carnivorous dinosaurs from the Jurassic period were previously known to have been found in this vast area.”

Two specimens of Alpkaraqsh Kyrgyzics were recovered from the top Barabansai Formation in Kyrgyzstan, Jalal-Abad, near the city of Tashkumil.

“While the type specimen represents a subadult individual, the smaller specimen is a juvenile, indicating that it probably lived in groups,” the paleontologists said.

Alpkaraqsh Kyrgyzics is the first diagnosable theropod species from the Jurassic of Central Asia in western China.

We suggest that metriocanthosaurid dinosaurs originated in Southeast Asia during the Late Early or Early Middle Jurassic and rapidly became the dominant group of apex theropod predators in many ecosystems on the continent during the Jurassic.

Alpkaraqsh Kyrgyzics “The discovery of a metriacanthosaurid dinosaur fossil isn’t necessarily a surprise, but it fills a major gap in our knowledge of Jurassic theropods,” Prof Rauhut said.

“This discovery provides important new insights into the evolution and biogeography of these animals.

This discovery paper issued this month in the Zoological Journal of the Linnean Society.

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Oliver W. M. Rauhut others A new theropod dinosaur from the Callovian-Balabansai Formation of Kyrgyzstan. Zoological Journal of the Linnean Society 201(4):zlae090;doi:10.1093/zoolinnean/zlae090

Source: www.sci.news

Your Brain May Have Mutated in Unexpected Ways

Fragments of mitochondrial DNA can be added to the cell's main genome

wir0man/Getty Images

Mutations in which DNA from energy-producing mitochondria is mistakenly added to a cell's main genome were thought to be extremely rare. Now, studies of brain tissue show that such mutations occur in all of us, and their numbers may be a factor in ageing.

“Not only are they present, but they are abundant in the dorsolateral prefrontal cortex, an area of ​​the brain associated with cognitive abilities.” Ryan Mills At the University of Michigan.

In human cells, almost all of the DNA (about 6 billion letters) resides in the nucleus, but the energy-producing organelles called mitochondria have their own tiny genome of about 16,600 letters.

That's because mitochondria were once free-living bacteria with their own large genome. In the roughly 2 billion years since those bacteria formed a symbiotic relationship with our distant ancestors, most of the original bacterial genome has been lost or transferred to the main genome in the nucleus.

This evidence of transfer has led biologists to know for a long time that fragments of mitochondrial DNA could somehow find their way into the nucleus and then be added to the main genome. But this kind of mutation was thought to be very rare, Mills says. Over the past few years, work by his team and others has shown that this isn't as uncommon as we thought. At least in cancer cells.

Mills and his colleagues showed that these types of mutations also occur in non-cancerous cells by sequencing the DNA of brain tissue samples taken from 1,200 people during post-mortem examinations.

Although another team took the samples and sequenced them, Mills and his colleagues looked for mutations that add mitochondrial DNA to the nuclear genome. “We were just curious,” Mills says.

Not only did they find such mutations, but they also found that they were more prevalent in people who, on average, died younger.

It's not clear whether these mutations are just a symptom of aging or a cause of it, Mills says. “The jury is still out,” he says. “But if you take the entire mitochondrial sequence and put it somewhere in the genome, it's hard for me to believe that it wouldn't have an effect.”

topic:

Source: www.newscientist.com

Many climate policies are ineffective in mitigating climate change

Most political efforts to tackle climate change have had little effect

Shutterstock

Most climate policies fail to significantly reduce emissions and have little effect on halting climate change, meaning governments must work harder to find ways to actually make a difference.

Nicholas Koch Researchers from the Mercator Institute for the Global Commons and Climate Change in Berlin found this by assessing the impact of 1,500 climate policies implemented in 41 countries across six continents between 1998 and 2022.

The researchers began by using machine learning to identify moments when a country's emissions fell significantly compared to a control group of other countries not included in the analysis. They found 69 such emissions “breaks” and compared them to a database compiled by the Organisation for Economic Co-operation and Development (OECD) that tracks what climate policies were enacted and when.

Matching policy shifts with changes in emissions is not an exact science, but the team was able to identify 63 of these changes as being due to one or more policy interventions that took place within a two-year period before or after the change, to account for lagged or anticipated effects.

Each of the 63 breaks reduced carbon dioxide emissions by between 600 million and 1.8 billion tonnes, but the researchers found that overall, most climate policies have fallen far short of this level of success. “There are many policies that have not led to significant reductions in emissions, and more policies do not necessarily lead to better outcomes,” Koch said.

Many policies fail because they are too specific, he says. For example, governments might subsidize the purchase of new electric cars, but most cars on the road are not electric, so the impact is minimal. One measure that seems to be very effective is a total ban, for example stopping the use of coal for electricity generation, but these are always used in conjunction with others, making it hard for the team to identify whether they work in isolation.

Politicians are looking for a one-size-fits-all policy mix, but they're out of luck: there's nothing that works for all sectors. Pricing seems to be the most effective tool, especially in reducing emissions in commercial industries, but it's not the only solution, Koch says. “We've found that the most frequently used policy tools – subsidies and regulations – are not enough,” he says. “Only in combination with price-based tools like carbon prices, energy taxes, can we achieve significant emissions reductions.” In other words, people will only reduce their emissions if it hurts their wallets.

“A key value of this paper is that it identifies clear changes in emissions in specific sectors and countries.” Matthew Patterson The researcher, from the University of Manchester in the UK, points out that the OECD's database of policy change has some limitations because the government documents it draws from are not reported consistently around the world, but he says it is the best available for the purposes of this study.

“We've known for some time that climate policies work best in combination, but this study gives us more specific information about which combinations work and in what circumstances,” Patterson says. This will allow us to more aggressively pursue these “breaks” to address the emissions gap and create the policy combinations that most effectively address emissions.

Marion Dumas Researchers at the London School of Economics and Political Science say that while the study should be useful to policymakers, looking first at emissions trends – or the results – and then working backwards to understand the causes may not capture the full reality of policy interventions.

“This is a very interesting approach, but there is a lot of uncertainty as to how to simulate the likely outcomes. [emissions] “You need to map out the trajectory and then identify the tipping points,” Dumas said, adding that a two-year gap around the tipping point may be too short and underestimates the real impact of more gradual, longer-term policy changes.

“It's important not to overinterpret the headline results, which suggest that very few policies will reduce emissions.” Robin Rambo The researchers, from Imperial College London, say small emissions reductions that their team's methods didn't detect could add up to big differences.

Of course, a larger issue in identifying the most effective measures is that policymaking doesn't take place in a vacuum, and specific policies must be acceptable to the general public. “The political dynamics will determine whether that combination can be implemented in any given country or sector,” Patterson says.

“We know this is going to be very difficult politically,” Koch said, “but the good news is that in general it's possible to put policies in place to achieve these very ambitious goals.”

topic:

  • Climate change measures/
  • Carbon Emissions

Source: www.newscientist.com

The Importance of Saving the Chandra Space Telescope

Chandra X-ray Observatory

NASA/CXC & J. Vaughan

On July 23, 1999, just a few months before I enrolled in college, NASA’s Space Shuttle Columbia launched with a precious cargo. Not only was it carrying a crew led by the first woman, Eileen Collins, its primary purpose was to launch the Chandra X-ray Observatory, a new flagship space telescope. Chandra This was the heaviest payload ever carried by a NASA space shuttle and turned out to be one of the last two missions completed by Columbia before it tragically exploded after launch on February 1, 2003.

Chandra is the first, and so far only, NASA mission named after a person of color. The late theoretical astrophysicist and Nobel Prize winner Subramanian Chandrasekhar was called Chandra by his friends and family. Chandrasekhar, whose last name means “crown of the moon,” made many important contributions to astrophysics. His most important work was discovering the Chandrasekhar limit, the maximum mass a white dwarf remnant can have before it collapses into a black hole.

It's fitting that an X-ray telescope mission should be named after a scientist who has spent his life thinking about the physics of black holes, as X-ray telescopes play a key role in black hole research. X-rays are high-energy light waves, which means they are produced in extremely energetic environments, such as those around black holes, where extreme distortions of space-time cause strong gravitational forces to accelerate particles to extremely high speeds. In other words, when we look at the universe through the lens of X-ray astronomy, rather than the visible wavelengths of traditional telescopes, we see an entirely different universe.

Importantly, X-ray astronomy can't be done from the Earth's surface, because it's blocked by the Earth's atmosphere. That's good for human health, but not so good for astronomers. Chandra is therefore a reminder of just how important it is to keep low Earth orbit debris-free, so we can safely launch space telescopes that perform tasks that are simply beyond the control of the Earth.

I feel like I have grown up with Chandra. And not just because I attended college at Chandra headquarters, now known as the Center for Astrophysics (CfA) in Massachusetts, and was often mistakenly called “Chandra”. One of my lab projects as an undergraduate was to adjust the light-gathering part of Chandra's backup camera. The following year, I wrote my undergraduate thesis under the guidance of Martin Elvis, an expert in X-ray astronomy. My research focused on the particle winds that fly out of galaxies that contain supermassive black holes. I used Chandra data to analyze what structures these galaxies take. It is true that Martin's letter helped me secure admission to at least one PhD program. In other words, without Chandra, my career may never have begun.

I am one of thousands of scientists in the fields of physics and astronomy who can tell similar stories of how Chandra data was the foundation of the early stages of their careers, or how they have dedicated their lives to using Chandra to explore the mysteries of the universe. Laura Lopez Ohio State University has used Chandra for many years to study supernovae. Daniel Castronow a staff scientist at CfA, is doing the same thing. The three of us were postdoctoral fellows at MIT and are from a generation that grew up on the power of the Chandra X-ray Observatory.

Now, after 25 years in orbit, Chandra is under threat – not the reality of space debris and aging equipment, but the political climate. US President Joe Biden's appointees to head NASA recently tried to scale back the project, but the scientific community worked with Congress to save the mission. But things will never be the same. A compromise proposal, which has not yet been signed into law, would drastically cut Chandra's funding and limit its scientific scope. Notably, there is no scientific basis for opposing the plan. Recommendations They have an army of expert advisers, but NASA has cut funding it had already promised to scientists, leaving PhD students and postdocs without enough money to cover living expenses.

Chandra deserves better. And so does its global audience. Thanks to Chandra, we have discovered new neutron stars and learned about their interiors. Our knowledge of black holes has blossomed. We have gained a deeper understanding of stellar life cycles and the history of our galaxy. We have been able to study galaxy clusters and learn how dark matter is distributed within them, putting the Milky Way in context. There is still time to save Chandra, a monument to human ingenuity. The fact that it is still going strong after 25 years should be celebrated and it should be honoured by the continuation of the mission.

Chanda's Week

What I'm Reading

My friend is Andrea Kindried. From Slavery to the Stars: A Personal Journey And it's beautiful.

What I'm seeing

I've seen some classic episodes Star Trek: The Next Generation Like “Remember Me”.

What I'm working on

I am developing a new course that prepares students to understand science in a social context..

Chanda Prescod Weinstein is an associate professor of physics and astronomy and a faculty member of women's studies at the University of New Hampshire. Her latest book is A Disordered Universe: A Journey into Dark Matter, Space-Time, and Dreams Deferred.

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Source: www.newscientist.com

Interested in dark love stories? A study could be just for you

Pathological dating

People with a craving for pathological romance could, if they so wished, write algorithms to select attractive, pathological prospective spouses or recreational dating partners.

Driven by curiosity, Coltan Scribner, inventor of the Morbid Curiosity Scale (Feedback, November 19, 2022), has explored new uses for the tool. He and two colleagues have study explains that “behavioral attraction predicts mating interest among morbidly curious women” toward men with risky personalities.

They cite previous research that shows those “women are aware of the potential costs associated with such men.” The new study aims to help those women, stating: “Despite the potential costs of men high on the dark triad, it may be beneficial for women with pathological curiosity to develop a preference for such men to fulfill short-term mating goals.

The study doesn’t delve into the obvious business potential here. Feedback envisions a new era dedicated to the making and use of morbid gadgets. Perhaps brighter days lie ahead for this industry, originally called “computer dating.”

(For those interested, Scribner has also created a simple way to measure where you stand on the scale: a free online Morbid curiosity test Before we begin, we’re told that “‘morbid’ doesn’t mean curiosity is bad, it simply refers to the fact that the topic is related to death in some way.”

The limits of curiosity

What are the limits of your curiosity? Is there a foolproof, easy way to find out? Here’s a test.

The feedback includes a copy of a paper published by Subhash Chandra Shaw and his colleagues. Indian Army Medical Journal The title of the study and your response may tell you something about yourself.

This paper is Missing anus: don’t miss it“”.

Talking about politics

Some politicians seek success through extremely eloquent speeches, which give them a momentary sense of persuasion.

Feedback noticed a similarity between the flashy but empty speeches of these politicians and the flashy but empty texts generated by ChatGPT and similar artificial intelligence computer programs.

Michael Townsen-Hicks, James Humphreys and Joe Slater of the University of Glasgow in the UK said: ChatGPT is bullshit“”teeth, Ethics and Information Technology They argue that “describing AI misinformation as bullshit is a more useful and accurate way to predict and discuss the behavior of these systems.” As a classic example of bullshit, the team cites a political candidate saying certain things simply because those words “might create a positive impression on potential voters.”

The feedback at least celebrates the skill of politicians who, like ChatGPT, can deliver endless streams of easy-to-swallow but indigestible chatter. In some countries, some of the most successful ChatGPT-esque politicians also display a visual counterpart to their words, a momentarily plausible physical aspect: they adorn their heads with ChatGPT-esque hair, or what might be mistaken for hair for a moment. There is little published research on why and how this happens.

It’s not such a small thing

Feedback continues its quest to create a list of trivial psychic powers, with Aline Berry confessing and professing that she has a trivial psychic power, which may not be trivial at all.

She writes, “I believe I have a superpower that I’ve taken for granted my whole life: when someone complains that they’re looking around for something, I usually find it within five minutes. Somehow, like Sherlock Holmes, I filter out the obvious things they no doubt see and focus on the lost item that’s camouflaged in such a way that it can easily be overlooked if not seen.”

“Recently, a friend of mine asked me for help after frantically searching for her car keys all morning. I stopped, looked around, realized there was no point in looking everywhere, and asked her if she’d looked in the fridge. Her eyes lit up – she’d placed her keys on something cold to remind herself to take them with her, but promptly forgot.”

Another skill emerged during her childhood: “I started a new school a few weeks late and was given a geometry problem. I had never studied geometry before and didn’t know any of the rules. So I looked at a graph and wrote the answer down. I was right. The teacher accused me of cheating and gave me a problem that I had drawn myself, that no one had seen. I wrote the right answer again. As punishment, the teacher gave me ten problems that had to be solved the right way. I didn’t know the correct rules, so I was happy when I got the news that I was going to a different school.”

A whirlwind of interest

An exercise in dimensional scaling. Which is more powerful: a) a storm in a teacup, or b) a storm in a teapot? An experiment is the real way to answer this question. Survey your colleagues (at least 50 people) and submit the three survey results (number of respondents, storm, and tempest) to Swirl of interest, c/o Feedback.

Marc Abrahams is the founder of the Ig Nobel Prize ceremony and co-founder of the journal Annals of Improbable Research. He previously worked on unusual uses of computers. His website is Impossible.

Do you have a story for feedback?

You can submit articles for Feedback by emailing feedback@newscientist.com. Please include your home address. This week’s and past Feedback can be found on our website.

Source: www.newscientist.com

Basic memory allows a blob of jelly to play Pong

Pong is a simple video game

Interphoto/Alamy

Inanimate blobs of ion-laden jelly can play computer games Pong And it will continue to improve over time: The researchers are planning further experiments to see if it can handle more complex calculations, and hope that it could eventually be used to control robots.

Inspired by past research into playing with brain cells in a dish Pong, Vincent Strong So he and his colleagues at the University of Reading in the UK decided to try a tennis-like game with simpler materials. They mixed ions into a water-filled polymer material so that it responded to electrical stimuli. When an electric current was passed through the material, those ions migrated to the current source, dragging water with them and causing the gel to swell.

In their experiments, the researchers used a standard computer to Pong They then used a 3 x 3 electrode grid to send electric currents to different points in the hydrogel to simulate ball movement, while a second electrode grid measured the concentration of ions in the hydrogel, which a computer interpreted as instructions for where to move the paddle.

The researchers found that not only was the hydrogel playable, but that with practice, accuracy improved by up to 10 percent and rallies also lasted longer.

The hydrogel expands faster than it contracts, and expands more slowly even when a constant electric current is applied.These properties allow the gel to record signals of expansion, creating a sort of rudimentary memory, the researchers say.

“Instead of just knowing what happened moment by moment, it's remembering the movement of the ball throughout the entire game,” Strong said, “so it's not just experiencing where the ball is right now, but the entire movement of the ball. It's like a black-box neural network that remembers how the ball behaves, how it moves, what it's doing.”

A polymer gel sandwiched between electrodes that deliver electrical current and measure ion levels

Vincent Strong et al. 2024

Strong said that while the hydrogel is much simpler than neurons in the brain, experiments have shown it can perform similar tasks. He believes the hydrogel could be used to develop new algorithms that would allow regular computers to perform tasks with minimal resources, making problem solving more efficient. But the hydrogel could also become an analog computer itself.

“I wouldn't rule out putting something like a hydrogel inside a robot brain,” Strong says. “That sounds interesting, and I'd like to see it. But the practicality of that is… I don't know yet.”

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Source: www.newscientist.com

First private spacewalk to be featured in SpaceX’s Polaris Dawn mission

A groundbreaking space mission known as Polaris Dawn is set to take off next week with four private citizens on board. The mission is expected to feature the first ever spacewalk conducted entirely by a civilian crew.

The commander of the mission is billionaire entrepreneur Jared Isaacman, who is also the founder and CEO of Shift4, a payment processing company. Polaris Dawn is the first of three spaceflights funded and organized by Isaacman in collaboration with SpaceX, collectively known as the Polaris Program. This will be the first private SpaceX mission to reach orbit in 2021.

The crew of three includes pilot Scott Kidd-Poteet, a retired Air Force Lt. Col., and SpaceX engineers Sarah Gillis and Anna Menon. They will be venturing into space aboard SpaceX’s Crew Dragon capsule on a Falcon 9 rocket for a planned five-day mission.

One of the highlights of the mission will be a spacewalk on the third day, where two crew members will exit the capsule via cables and spend up to 20 minutes in space. This is a historic moment as until now, spacewalks have been carried out exclusively by astronauts from government space agencies.

During the spacewalk, the Crew Dragon capsule will be fully exposed to the vacuum of space at an altitude of 435 miles above Earth. To prepare for this event, all four astronauts will don SpaceX-designed spacesuits for testing and future long-duration missions.

The mission aims to inspire people to dream big and push the boundaries of human exploration beyond Earth. The crew, including Isaacman, have undergone extensive training over the past two years in preparation for this momentous journey.

In addition to conducting science experiments and testing technology during the mission, the crew will also raise funds for St. Jude Children’s Research Hospital, continuing Isaacman’s philanthropic efforts in space.

Details regarding the cost, objectives, and timeline of future Polaris flights have not been disclosed by Isaacman at this time.

Source: www.nbcnews.com

Humpback whales employ unique tools for their tasks

Humpback whale (Megaptera novaegangliae) Whales build so-called “bubble nets” as tools to hunt, but researchers from the University of Hawaii and the Alaska Whale Foundation have found that these marine animals not only build bubble nets, but also manipulate these unique tools in a variety of ways to maximize food intake in their Alaskan feeding grounds. This novel study sheds light on a behavior critical to whale survival and makes a compelling case for including humpback whales among the rare animals that manufacture and use unique tools.

Although some animal species use tools to forage, only a few manufacture or modify tools. Humpback whales are one of these rare species, as they manufacture bubble net tools while foraging. Using animal tags and unmanned aerial system technology, Sabo others. Investigating the bubble nets made by solitary humpback whales (Megaptera novaegangliae) while feeding on krill in the Pacific Ocean, whale nets in southeast Alaska. They demonstrate that the nets are composed of internal tangential loops, suggesting that the whales actively control the number of loops, the size and depth of the net, and the horizontal spacing of adjacent bubbles. They argue that the whales adjust structural elements of the net to increase the amount of prey they catch in a single lunge by an average of seven-fold. Image credit: Szabo others., doi: 10.1098/rsos.240328.

“Many animals use tools to find food, but few actually make or modify their own tools,” says Lars Bader, a professor at the University of Hawaii.

“We discovered that solitary humpback whales in southeast Alaska build complex bubble webs to capture krill.”

“These whales expertly blow bubbles in patterns that form nets with internal loops, actively controlling details such as the number of loops, the size and depth of the net, and the spacing of the bubbles.”

“This method allows them to catch up to seven times as many prey in one feeding dive without expending any extra energy.”

“This impressive behaviour puts humpback whales in a rare group of animals that make and use their own tools to hunt.”

The marine mammals known as cetaceans include whales, dolphins and porpoises and are notoriously difficult to study.

Advances in research tools are making it easier to track and understand whale behaviour, and in this case, Professor Bader and his colleagues used specialised tags and drones to study the whale's movements from above and below the water.

“We attached non-invasive suction cup tags to whales in southeast Alaska and flew drones over humpback whales as they hunted alone in bubble nets to collect data on their underwater movements,” said Dr William Goff, also from the University of Hawaii.

“The tools are great, but it takes practice to hone them.”

“Whales are a difficult group to study and successful tracking with tags and drones requires skill and precision.”

“This little-studied foraging behavior is unique to humpback whales.”

“It's really amazing to see these animals in their natural habitat, doing things that only a handful of people get to see.”

“And then it's rewarding to be able to go back to the lab and look at the data and find out what they're doing underwater after they're out of sight.”

a paper The study was published in the journal Royal Society Open Science.

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A. Sabo others2024. Solitary humpback whales manufacture bubble nets as a tool to enhance prey intake. R. Soc. Open Science 11(8):240328;doi: 10.1098/rsos.240328

This article is based on a press release provided by the University of Hawaii.

Source: www.sci.news

Research indicates TRAPPIST-1 system developed through a two-stage formation process

TRAPPIST-1 is an ultracool dwarf star located 38.8 light-years away in the constellation Aquarius that hosts seven planets. The period ratios of the neighboring planets are closer as they move away from the star: 8:5, 5:3, 3:2, 3:2, 4:3, 3:2. This compact resonant configuration is a clear indication of disk-driven migration, but the desired outcome of such an evolution would be the establishment of a first-order resonance, rather than the higher-order resonances observed in the inner system. Astronomer Gabriele Pichierri of the California Institute of Technology and his colleagues explain the orbital configuration of the TRAPPIST-1 system with a model that is largely independent of the specific disk migration and orbital circularization efficiency. Two key elements of the team's model are that, along with the migration, the inner boundary of the protoplanetary disk retreated over time, and that the TRAPPIST-1 system initially separated into two subsystems.

This artist's rendering shows TRAPPIST-1 and its planets as seen on the surface. Image courtesy of NASA / R. Hurt / T. Pyle.

“When all we had to analyse was the solar system, we could simply assume that planets formed where we see them today,” Dr Pichieri said.

“But when the first exoplanet was discovered in 1995, we had to rethink this assumption.”

“We're developing better models of how planets form and how they come to be oriented in the way that we found them.”

Most exoplanets are thought to form from a disk of gas and dust around a newly formed star, and then migrate inwards, approaching the inner boundary of this disk.

This results in a planetary system assembled much closer to the host star than is the case in our solar system.

In the absence of other factors, planets tend to move away from each other at characteristic distances based on their mass and the gravitational force between them and their host star.

“This is the standard transition process,” Dr. Pichieri said.

“The positions of the planets form resonances between their respective orbital periods. If you divide the orbital period of one planet by the orbital period of its neighbor, you get a simple integer ratio like 3:2.”

For example, if one planet takes two days to orbit a star, the next planet further away takes three days.

If the second planet and a more distant third planet were also in 3:2 resonance, the third planet's orbital period would be 4.5 days.

“The exoplanets behave nicely in simpler predicted resonances, so to speak,” Dr Pichieri said.

“But the inner ones have slightly more exciting resonances. For example, the orbital ratio of planets b and c is 8:5, and the ratio of c and d is 5:3.”

“This subtle difference in the outcome of TRAPPIST-1 assembly is puzzling and represents a unique opportunity to tease out in detail what other processes were at work in its assembly.”

“Moreover, most planetary systems are thought to have begun in such resonances, but have experienced significant instabilities during their lifetimes before we observe them today.”

“Most planets would become unstable or collide with each other, and everything would be in chaos. For example, our solar system was affected by such instability.”

“But we know there are some systems that are more or less pristine specimens that have remained stable.”

“They effectively represent a record of its entire dynamical history, and we can try to reconstruct it. TRAPPIST-1 is one of them.”

The challenge then was to develop a model that could explain the orbits of the TRAPPIST-1 planets and how they got to their current configuration.

The resulting model suggests that the inner four planets evolved alone within the originally predicted 3:2 resonant chain.

As the disk's inner boundary expanded outward, the orbits loosened from the tighter 3:2 linkage into the configuration observed today.

The fourth planet was originally located on the inner boundary of the disk and moved outward with the disk, but was pushed back inward at a later stage when three more outer planets joined the planetary system.

“By observing TRAPPIST-1, we were able to test an exciting new hypothesis about the evolution of planetary systems,” said Dr Pichieri.

“TRAPPIST-1 is very interesting because it's a very complex, long chain of planets, and it's a great example for testing alternative theories about the formation of planetary systems.”

of Survey results Published in a journal Natural Astronomy.

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G. Pichieri othersDuring the recession of the inner edge of the disc, the TRAPPIST-1 system forms in two steps. Nat AstronPublished online August 20, 2024, doi: 10.1038/s41550-024-02342-4

Source: www.sci.news

Research shows that Clovis people utilized planted pikes for hunting large herbivores

Historical and ethnographic sources document that portable pole-hafted weapons, or spears, were used for hunting and defense against large game in North and South America, Africa, Eurasia, and Southeast Asia for several millennia during the Late Holocene. Given the dominance of large game in North America during the Late Pleistocene, centuries when Clovis points emerged and spread across much of the continent between 13,050 and 12,650 years ago, pole-hafted weapons may have been used for hunting large herbivores or for defense against large carnivores.

A Clovis point with distinctive grooved flake scars. Image courtesy of S. Byram.

“This ancient Native American design was a remarkable innovation in hunting strategy,” said Dr Scott Byrum, a researcher at the University of California, Berkeley.

“This unique indigenous technology provides a window into hunting and survival techniques that have been used for thousands of years in many parts of the world.”

The team's discovery may help solve a mystery that has plagued archaeological communities for decades: how North American communities actually used Clovis stone tools, the most commonly unearthed remains from the Ice Age.

Clovis Points are named after the town of Clovis, New Mexico, where they were first discovered about a century ago. Clovis Points are formed from rocks such as chert, flint, and jasper.

They range in size from the size of a person's thumb to the size of a medium-sized iPhone, and have a clearly defined, sharp edge and grooved indentations on either side of their base.

Thousands of fossils have been discovered across the United States, some of which have been unearthed within preserved mammoth skeletons.

“Clovis points are often the only part recovered from a spear,” said Dr. June Sunseri of the University of California, Berkeley.

“The elaborately engineered bone hafts at the ends of the weapons are sometimes found, but the wood at the bases of the spears, and the rosin and string that made them work as a complete system, have been lost over time.”

“Furthermore, research silos limit such systems thinking about prehistoric weaponry, and if stone experts are not bone experts they may not get the full picture.”

“We need to think beyond simple artifacts. The key here is looking at this as an engineered system that requires multiple types of expertise in our field and in other fields.”

Building tools into powerful and effective systems would have been a priority for communities 13,000 years ago.

Tools had to be durable; there were only a limited number of suitable rocks that people could use to cross the land.

They might travel hundreds of miles without obtaining a long, straight stick suitable for making a spear.

“So obviously you don't want to risk throwing or breaking your gear when you're not sure if you're going to catch the animal,” Dr Byrum said.

“People who analyse metal military artefacts know about it because it was used to halt horses in war.”

“But before that, it wasn't really known for other situations, like wild boar hunting or bear hunting.”

“It's a common theme in literature, but for some reason it hasn't been talked about much in anthropology.”

To evaluate their spear hypothesis, the researchers built a test platform to measure the force that the spear system could withstand before the tip broke off or the shaft stretched.

A low-tech, static version of an animal attack using reinforced replica Clovis point spears allowed us to test how different spears reach their breaking point and how their extension systems respond.

This builds on previous experiments in which researchers fired stone-tipped spears into clay and ballistic gel, which may have been as painful as a needle prick to a nine-tonne mammoth.

“The energy that a human arm can generate is completely different from the energy that a charging animal can generate. It's an order of magnitude different,” Dr Jun said.

“These spears were designed to protect the wielder.”

“The sophisticated Clovis technology, developed uniquely in North America, is a testament to the ingenuity and skill used by indigenous peoples to coexist with ancient lands and now-extinct megafauna,” said Kent Lightfoot, a professor at the University of California, Berkeley.

Team result Published in a journal PLoS One.

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RS Byram others2024. Clovis projectile points and foresharps subjected to reinforced weapon compression: modelling the encounter between Stone Age spears and Pleistocene megafauna. PLoS One 19 (8): e0307996; doi: 10.1371/journal.pone.0307996

This article is a version of a press release provided by the University of California, Berkeley.

Source: www.sci.news

The 1.5°C target may be out of reach, but climate action is still crucial

AP Photo/François Mori, File/Alamy

As a COP26 During climate change negotiations in Glasgow, UK, in November 2021, a new slogan entered the vocabulary: “Stay at 1.5°C.” The phrase, on everyone’s lips from politicians to climate scientists, was aimed at maintaining the goals set as part of the Paris Agreement at the COP six years ago.twenty oneIn hindsight, this ambition was probably already fizzling out, destined to remain merely an empty slogan.

New Scientist The argument began in 2022, when expert opinion did not reflect their personal views or the data we were seeing. Scientists felt trapped and unable to speak out because limiting warming to 1.5°C above pre-industrial levels is still possible according to the laws of physics, but not realistic given the political, social and economic upheaval.

Since then, there has been a growing recognition that 1.5°C is unattainable, but there was no frank discussion of what that meant. Now, for the first time, researchers have explicitly rejected that, saying that 1.6°C is the best we can hope for, and that higher temperatures are more likely (see “Best-case scenario for climate change now is 1.6°C warming”).

Will policymakers finally realize that platitudes and slogans are not enough to combat climate change? Promises to “maintain” these targets are meaningless if we do not achieve the only means of preventing rising temperatures — reducing emissions of carbon dioxide and other global-warming greenhouse gases to net zero.

Unfortunately, the phrase “net zero” is losing its original meaning as a description of atmospheric physics, and instead being used by many to mean “environmental policy I don’t like.” This is dangerous, because extreme temperature changes have locked us in a vicious cycle of emissions that only a net-zero energy system can break (see “Efforts to combat extreme temperatures are making the situation worse”). If we are to have any hope of limiting warming, we need to learn from the failure of “stay 1.5°C” and not let “net zero” become meaningless.

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Source: www.newscientist.com

COVID-19 vaccines may be less effective due to intestinal parasites

Duodenal hookworms (Ancylostoma duodenale) cause one of the most common intestinal parasitic infections worldwide.

Katerina Conn/Shutterstock

People with intestinal parasitic infections, quarter This has been suggested by experiments in mice infected with the parasite, which had significantly weaker immunity after receiving a COVID-19 vaccination compared to mice not infected with the parasite.

Previous studies have shown that people with intestinal parasitic infections have a weakened immune response to vaccines for diseases such as tuberculosis and measles because the parasites suppress the processes that vaccines trigger to confer immunity, such as activating pathogen-killing cells. Intestinal parasitic infections are most common in tropical and subtropical regions, where they often occur because of limited access to clean water and sanitation.

Scientists have not tested whether these pathogens reduce the effectiveness of COVID-19 vaccines. Michael Diamond Researchers at Washington University in St. Louis, Missouri, vaccinated 16 mice with a COVID-19 mRNA vaccine, half of which had been infected 12 days earlier with an intestinal parasite that lives only in rodents. They gave each mouse a booster shot three weeks after the first vaccination.

About two weeks after the booster shot, the researchers analyzed the animals' spleens to measure concentrations of CD8+ T cells, specialized white blood cells that are important for eliminating other cells infected with the SARS-CoV-2 virus. They found that the spleens of mice infected with the intestinal parasite had about half the number of cells as mice without the parasite, suggesting a weakened immune response to the vaccine.

The researchers repeated the vaccination process in another group of 20 mice, half of which were infected with the intestinal parasite, exposing them to the highly infectious Omicron variant of the SARS-CoV-2 virus. After five days, the lungs of vaccinated rodents infected with the intestinal parasite had, on average, about 20% more virus than uninfected ones.

These findings suggest that intestinal parasites may reduce the effectiveness of COVID-19 vaccines in people, but different types of intestinal parasites are known to affect immunity differently, the researchers say. Keke Fairfax The University of Utah researchers said it's unclear whether the parasite's infection in humans would have the same effect on vaccinating against COVID-19 as it did in mice, and the situation is further complicated by the fact that humans tend to harbor multiple types of intestinal parasites at the same time, they said.

Still, understanding how to alter the immune response to vaccination is important given the prevalence of parasitic infections, and these findings suggest that researchers may need to further evaluate the vaccine's effectiveness in parts of the world where a high proportion of the population is infected with intestinal parasites, Fairfax says.

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Source: www.newscientist.com

AI models do not learn in the same way humans do

AI programs quickly lose the ability to learn new things

Jiefeng Jiang/iStockphoto/Getty Images

The algorithms that underpin artificial intelligence systems like ChatGPT are unable to learn as they are used, forcing tech companies to spend billions of dollars training new models from scratch. This has been a concern in the industry for some time, but new research suggests there's an inherent problem with how the models are designed – but there may be a solution.

Most AI today is so-called neural networks, inspired by how the brain works, with processing units called artificial neurons. Typically, AI goes through distinct stages during its development: First, the AI ​​is trained, and its artificial neurons are fine-tuned by an algorithm to better reflect a particular dataset. Then, the AI ​​can be used to respond to new data, such as text inputs like those entered into ChatGPT. However, once a model's neurons are set in the training phase, they can no longer be updated or learn from new data.

This means that most large AI models need to be retrained when new data becomes available, which can be very costly, especially when the new dataset represents a large portion of the entire internet.

Researchers have wondered whether these models might be able to incorporate new knowledge after initial training, reducing costs, but it was unclear whether this was possible.

now, Shivhansh Dohare Researchers at the University of Alberta in Canada tested whether the most common AI models could be adapted to continually learn. The team found that when exposed to new data, a huge number of artificial neurons became stuck at a value of zero, causing the AI ​​models to quickly lose the ability to learn new things.

“If you think of it like a brain, it's like 90 percent of the neurons are dead,” D'Hare says. “You don't have enough neurons to learn with.”

Dhare and his team started by training their AI system from the ImageNet database, which consists of 14 million labeled images of simple objects like houses and cats. But instead of training the AI ​​once and then testing it multiple times to distinguish between the two images, as is the standard approach, they retrained the model for each image pair.

The researchers tested different learning algorithms in this way and found that after thousands of retraining cycles, the networks were unable to learn and their performance deteriorated, with many neurons becoming “dead” – that is, having a value of zero.

The team also trained the AI ​​to simulate the way ants learn to walk through reinforcement learning, a common technique that teaches an AI what success looks like and helps it figure out the rules through trial and error. They tried to adapt this technique to allow for continuous learning by retraining the algorithm after walking on different surfaces, but they found this also led to a significant decrease in learning ability.

The problem is inherent to the way these systems learn, D'Hare says, but there is a workaround: The researchers developed an algorithm that randomly turns on some neurons after each training round, which seems to mitigate the performance degradation. [neuron] “When it dies, you just bring it back to life,” D'Hare says, “and now it can learn again.”

The algorithm seems promising, but needs to be tested on larger systems before it can be trusted to be useful, he says. Mark van der Wilk At Oxford University.

“Solving continuous learning is literally a billion-dollar problem,” he says. “If you have a true comprehensive solution that allows you to continuously update your models, you can dramatically reduce the cost of training these models.”

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Source: www.newscientist.com

Children and teenagers experience varying symptoms from Long Corona

The impact of the long corona pandemic appears to vary by age

Damir Cudic/Getty Images

Symptoms of long COVID appear to be very different in young children and adolescents, and a better understanding of how the symptoms manifest could aid in diagnosis.

So far, most research on long-COVID has focused on adults, in part because of a “misconception that children can't get long-COVID,” he said. Rachel Gross At New York University.

Gross and his colleagues are currently following 751 children ages 6 to 11 and 3,109 children ages 12 to 17 whose parents say they had previously been infected with the SARS-CoV-2 virus.

The researchers defined long COVID as having at least one symptom that lasted more than a month, started or worsened during the COVID-19 pandemic, and was present at the time of the study.

Among young children, these symptoms primarily included sleep problems, difficulty concentrating, and abdominal problems such as pain, nausea, vomiting, and constipation.

The symptoms were uncommon among about 150 children of the same age who had not previously been infected, and were confirmed by the absence of antibodies against the virus in their blood samples.

In contrast, symptoms in the 1,300 uninfected young people typically included pain, fatigue and loss of smell or taste.

It's unclear why symptoms differ across different age groups, but Gross said it could be due to differences in hormones or immune systems, or that teenagers may simply be better able to vocalize their symptoms than younger kids. Danilo Buoncenzo A study from the Gemelli University Hospital in Rome, Italy. For example, a teenager may complain of fatigue, but a caregiver may only notice lingering symptoms in a younger child when they vomit.

Armed with this data, the researchers developed a score that ranks how likely a young person's symptoms are to have long-Covid. Currently, diagnosis depends on doctors ruling out other illnesses and recognizing that long-Covid can take many different forms. “Doctors would prefer a score or more objective criteria. Such a tool would definitely help clinicians at least recognize that a child may have long-Covid,” Buoncenso said.

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Source: www.newscientist.com

Latest Research Findings in BBC Science Focus Magazine

13,000 years ago, humans had to come up with creative ways to survive in icy environments. Recent studies suggest that their solutions were more inventive and brutal than previously thought: Ice Age hunters likely used weapons to impale prey such as mammoths and sabre-toothed tigers.

This discovery could potentially resolve a long-standing debate regarding the purpose of ancient tools known as Clovis points. These sharp rocks, made of materials like chert and flint, have been found throughout the United States in various sizes. While it was initially believed that Clovis points were used as spear tips by skilled hunters for hunting large animals like mammoths and bison, a new study suggests a different perspective.

Published in the journal PLoS One, the study conducted by archaeologists from the University of California, Berkeley proposes that these weapons were used to ensnare and wound charging animals, and possibly even defend against sabre-toothed cats.


So how did this hunting method work? Hunters likely positioned the sharpened spear in the ground at an angle, allowing the animal’s momentum to drive the spear deep into its body upon impact. This innovative technique provided a strategic advantage in hunting large animals, making it more effective than traditional spear-throwing.

“This ancient Native American design represents a significant advancement in hunting strategies,” stated Scott Byrum, a contributing researcher. John Myers, the lead author of the study, emphasized the importance of understanding ancient survival techniques that have been utilized worldwide for millennia.

To validate their findings, the researchers conducted experimental simulations of the hunting technique in addition to analyzing historical records and literature. This process led to a better understanding of how Clovis points were used to hunt mammoths during the Ice Age.

A replica of an ancient Clovis point shows distinctive flutes near its base. These may have been the weapons used to kill the mammoth. – Photo by Scott Byrum

Recreating this ancient hunting technique through experimental models enabled researchers to gain insight into the effectiveness and practicality of pike hunting. Byrum and his team aim to further test their theory by creating a simulated mammoth to assess the durability and impact of the Clovis point.

This method of impaling prey, known as pike hunting, has historical precedence in warfare and hunting practices. During the Ice Age, this technology was crucial for survival as it allowed hunters to reuse their weapons and avoid the challenge of finding suitable materials for crafting new spears in harsh winter conditions.

By discovering how Clovis points were utilized in hunting, researchers have shed light on the coexistence of early humans with large extinct animals. This new perspective highlights the innovative strategies employed by ancient hunters and deepens our understanding of human history.

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Source: www.sciencefocus.com

New Images of UGC 4879 Captured by Hubble Space Telescope

Hubble astronomers have released a stunning new image of the dwarf irregular galaxy UGC 4879, taken by the NASA/ESA Hubble Space Telescope.

This Hubble Space Telescope image shows irregular dwarf galaxy UGC 4879, about 3.6 million light-years away in the constellation Ursa Major. Image credit: NASA / ESA / Hubble Space Telescope / K. Chiboucas, NOIRLab and Gemini North / M. Monelli, Canarian Astrophysics Institute / Gladys Kober, NASA and Catholic University.

UGC 4879 is an irregular dwarf galaxy in the constellation Ursa Major.

Also known as VV124 and LEDA 26142, this galaxy is quite isolated.

It lies 3.6 million light years from our Milky Way galaxy and 3.9 million light years from the Andromeda galaxy.

Dwarf galaxy Leo A, located about 1.6 million light-years away, is UGC 4879's closest neighbor.

This isolation makes UGC 4879 an ideal laboratory to study primordial star formation, without the complications of interactions with other galaxies.

There are only two other galaxies in the Local Group that have a similar, though slightly lower, isolation to UGC 4879: DDO 210 and SgrDIG, which are located in the opposite direction from UGC 4879.

“UGC 4879 is an isolated dwarf galaxy that lies just outside our Local Group of galaxies,” Hubble astronomers said in a statement.

“Because of its isolation, we are studying UGC 4879 to determine whether it is an old, relatively undisturbed galaxy.”

“Theories suggest that the least massive dwarf galaxies may have formed first.”

“If UGC 4879 is a relic from the early universe, it may offer clues about the hierarchy and evolution of galaxies, galaxy clusters, and even the universe itself.”

This image of UGC 4879 combines data from two Hubble observing programs focused on learning more about how dwarf galaxies form and evolve.

Source: www.sci.news

Scientists are puzzled by mysterious object speeding through galaxy at over a million miles per hour

An object moving through space at close to 1 million miles per hour has been detected, moving so fast that it is leaving the Milky Way galaxy. Scientists are now trying to identify this mysterious object.

Currently located 400 light-years away, the object known as CWISE J1249 is unlikely to be a spacecraft due to its massive size. It is approximately 30,000 times the mass of Earth, making it about 8% of the mass of the Sun.

This unusual size places J1249 somewhere between a star and a planet, as described by Dr. Darren Baskill, a lecturer in astronomy at the University of Sussex. According to Dr. Baskill, stars moving at such high speeds are rare.

The object’s speed is so rapid that it could exit the Milky Way galaxy in just a few tens of millions of years, which is a short period considering stars’ long lifespans.


This massive object, flying at 0.001% of the speed of light, has the potential to escape the galaxy and venture into intergalactic space.

Discovered by citizen scientists contributing to NASA’s Backyard Worlds: Planet 9 project, J1249’s speed is approximately 2.6 times faster than any space probe ever launched.

A new study, pending peer review, confirms these findings and further characterizes the object discovered through the initiative.

The object, with an unusual composition compared to stars and brown dwarfs, may be the first star of its kind in the galaxy, based on NASA’s observations.

Researchers believe the high-speed movement of the object may be linked to a supernova explosion in a binary star system or encounters with black holes in a star cluster.

Dr. Baskill suggests that gravitational slingshots could explain the extreme speed of J1249, potentially originating from the galaxy’s dense center and accelerated through gravitational interactions.

About our experts:

Dr. Darren Baskill is an Outreach Officer and Lecturer at the University of Sussex School of Physics and Astronomy, with a background in organizing astronomy-related events and competitions.

For more information, visit the University of Sussex website.

Source: www.sciencefocus.com

New study finds that climate change influenced the demographics of prehistoric hunter-gatherers

Using the large number of human fossils found in Ice Age Europe, paleoanthropologists have identified a population turnover in Western Europe 28,000 years ago, isolation between western and eastern refugia between 28,000 and 14,700 years ago, and a bottleneck during the most recent Ice Age.

Artistic reconstruction of an Ice Age hunter-gatherer group. Image courtesy of Tom Björklund.

“Around 45,000 years ago, the first modern humans migrated into Europe during the Ice Age, marking the beginning of the so-called Late Paleolithic period,” said Dr Hannes Lassmann, a researcher at the University of Tübingen.

“These early populations continuously inhabited the European continent, even during the so-called Last Glacial Maximum about 25,000 years ago, a time when glaciers covered much of northern and central Europe.”

“Archaeologists have long debated how climate change and the resulting new environmental conditions affected the demographics of hunter-gatherers at the time.”

“The limited number of available fossils and the often poor molecular preservation for ancient DNA analysis have made it very difficult to draw conclusions about the influence of climatic factors on migrations, population growth, decline and extinction.”

Because teeth make up a large part of the fossil record and preserve genetic traits in their morphology, Dr. Rathman and his colleagues compiled a large dataset of 450 dentitions dating from 47,000 to 7,000 years ago.

They focused on morphological features of the teeth – small variations within the dentition, such as the number and shape of cusps on the crowns, the pattern of ridges and grooves on the chewing surfaces, and the presence or absence of wisdom teeth.

“Because these traits are heritable, they can be used to trace the genetic relationships of Ice Age humans without the need for well-preserved ancient DNA,” Dr Lassman said.

“These features are visible to the naked eye, so we also looked at hundreds of publicly available photographs of the fossils.”

The results show that between about 47,000 and 28,000 years ago, during the Middle Glacial Period, populations from Western and Eastern Europe were well connected genetically.

During the subsequent Late Glacial Period, between 28,000 and 14,700 years ago, the researchers found no genetic link between Western and Eastern Europe.

Furthermore, the analysis shows that both regions have experienced significant declines in population size and loss of genetic diversity.

“This dramatic population shift was likely caused by major climate change,” Dr Rathman said.

“Temperatures during this period fell to their lowest values ​​for the entire Upper Paleolithic, culminating in the Last Glacial Maximum, when ice sheets reached their maximum extent and covered large parts of northern and central Europe.”

“The worsening climate changed the vegetation from steppe to primarily tundra, affecting the habitat of prey animals and, consequently, the hunter-gatherers who depended on them.”

“Our findings support the long-held theory that humans were not only pushed southward by the advancing ice sheet but also isolated into isolated refugia with more favourable environmental conditions,” said Dr Judith Beier, also from the University of Tübingen.

Another notable finding of the study is the discovery that Western European populations became extinct during the transition from the Middle to Late Neoglacial and were replaced by new populations migrating from Eastern Europe.

After the Late Glacial Period, temperatures rose steadily again, the glaciers retreated, grassland and forest vegetation returned, and previously abandoned areas could be recolonized for the first time.

The team observed that during this period, the populations of Western and Eastern Europe, which had previously been isolated and significantly declining, began to grow again and migration between the regions resumed.

“Our new method makes it possible for the first time to reconstruct complex prehistoric demographic events using morphological data,” said researcher Dr Maria Teresa Vizzarri from the University of Ferrara.

“To our knowledge, this has never been accomplished before.”

“Our study provides important insights into the demographic history of Ice Age Europeans and highlights the profound impact that climatic and environmental change had on prehistoric human life,” Dr Lassmann said.

“If we want to tackle the complex environmental challenges of the future, we need to urgently learn from the past.”

of Survey results Published in the journal Scientific advances.

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Hannes Lassmann others2024. Human demography in Late Paleolithic Europe inferred from fossil dental phenotypes. Scientific advances 10(33);doi: 10.1126/sciadv.adn8129

This article has been edited based on the original release from the University of Tübingen.

Source: www.sci.news