Solar maximum increases chances of auroras.

overview

  • A recent flurry of solar storms suggests the Sun is at its peak as part of an 11-year cycle.
  • The active period is likely to continue into next year, and more auroras may appear.
  • Next month, NASA will take an up-close look at solar activity as the Parker Solar Probe makes its closest approach to the sun ever.

The sun is awake.

Earth’s star has become more active in recent months, with giant flares erupting from the surface and streams of plasma and charged particles spewing into space. Several solar storms have been directed towards our planet, causing intense magnetic storms and the dazzling glow of the aurora borealis.

Experts say a storm of solar explosions after years of relative calm and calm is a sure sign that the star has entered a busy phase of its natural cycle, or solar maximum.

The active period is likely to continue into next year, with the potential for more solar storms and spectacular aurora borealis.

“This is definitely the season for major solar storms,” ​​said Kelly Kolek, a program scientist in NASA’s Heliophysics Division. “I think we’ll see the sky lit up again by the northern lights.”

Aurora photographed over Kiruna, Sweden on March 7th.
Leon Neal/Getty Images File

Later this month, NASA will get a close-up look at intense solar activity when the agency’s Parker Solar Probe makes its closest approach ever to the sun on December 24th.

The spacecraft is on an orbit that swoops to within 3.86 million miles of the Sun’s surface. This is closer than any other artifact in history. It is predicted that it could fly through the sun’s plasma plumes and fly into the star’s active regions.

“If you think of an American football field, if the Earth is on one side and the sun is on the other side, this is like going to the sun’s 4-yard line,” Kolek said.

Parker Solar Probe after heat shield installation in a clean room in Titusville, Florida, 2018.
Johns Hopkins APL / Ed Whitman / NASA

The Parker Solar Probe was launched in 2018 with a mission to study the sun’s atmosphere, an extremely hot region known as the corona. Last month, the car-sized spacecraft flew nearby in a maneuver that helped slingshot Venus closer to the sun.

Kolek said the spacecraft’s close encounters could provide valuable insights, especially if there are active sunspot regions (temporary features that appear as dark scratches on the sun’s surface) along its path. He said there is. Such observations could help researchers better understand how the sun’s activity rises and falls.

Solar cycles typically last about 11 years, as the Sun’s magnetic activity moves from periods of low to high magnetic activity. When a star emerges from its calm phase, or solar minimum, and reaches the peak of its solar cycle, its magnetic poles reverse and it enters solar maximum, increasing activity and erupting more frequently and violently.

The main way scientists know when the Sun has reached its maximum is by monitoring the formation of sunspots. As the sun spins, its magnetic field undulates, becoming distorted and tighter in some areas, Kolek said. This creates sunspots, which appear as dark specks in telescope images.

A huge, bright coronal loop traces magnetic field lines over the Sun’s active region in 2018.
Solar Dynamics Observatory / NASA

“The sun is a magnetic sphere, but it’s not a solid solid body, so as it rotates, its magnetic field gets twisted,” Kolek said.

the number of sunspots It increases steadily as the star moves towards its solar maximum. Once a significant decline is observed, researchers can define the beginning and end of a period of activity.

In some sunspot regions, the magnetic field can be about 2,500 times stronger than Earth’s magnetic field. According to NASA. Over time, sunspots can release vast amounts of stored magnetic energy in the form of solar storms.

This year, two major solar storms (one in May and one in early October) painted the night sky in bright pinks, greens, and purples as far south as Texas and Alabama. It surprised sky watchers. NASA said the May event was the strongest geomagnetic storm to hit Earth in the past 20 years.

On May 10th, a solar storm hit the Scottish National Monument in Edinburgh.
Jacob Anderson/AFP – Getty Images File
On October 10, the Northern Lights illuminate the desert sky of the Tonto National Forest northeast of Phoenix.
Michael Chou / USA Today Network

Auroras occur when clouds of charged particles ejected from the Sun during solar storms collide with Earth’s magnetic field and interact with atoms and molecules in Earth’s upper atmosphere. The colorful display is a beautiful byproduct of that process and is usually only seen at high latitudes. But during periods of high solar activity, the light can wander farther south than usual.

However, there may also be negative consequences. Strong magnetic storms can cause problems for astronauts in space and for GPS systems and satellites in orbit.

Source: www.nbcnews.com

Why Do We Engage in Self-Destructive Behavior and How to Stop it: Insights from Psychologists

Self-sabotage (also called “self-handicapping” by psychologists) is intentionally doing something that can harm your chances of success. academic ability testperformance at work, sportsor relationships.

For example, let’s say you intentionally don’t rehearse your work presentation. Or let’s say you have a running race coming up and you decide not to train for it. In a relationship, you might start ignoring your partner’s texts, even if you’re happy with the relationship.

In all these cases, behaving this way may sound strange and self-defeating. However, research suggests that there is a logic to self-destruction. It’s something people often do as a way to protect their self-esteem and reduce their fear of failure or abandonment.

For example, let’s say you deliberately fail to prepare for a presentation at work, and as a result, your presentation goes very poorly. The reason for your failure may be that you didn’t prepare, rather than the presentation saying something fundamental about you as a person or your skills. Similarly, if you come in last in a running race, you can ignore your misfortune and attribute it to not training at all.

If you ignore your partner’s messages, and they decide to break up with you, you can take that rejection not as a sign that they don’t like you anymore, but as a sign that you’ve been ignoring them. You can blame the facts. Or choose to go out with someone else.

In other words, self-sabotage is a way to protect your ego by having the perfect excuse in case of failure or rejection.

People who fear failure or have low self-esteem are more likely to engage in this type of self-sabotage. In the short term, it may make you feel better about yourself, and it’s a way to protect your image in the eyes of others. However, this is not a recommended strategy. Because in the long run, of course, it’s going to be something like this. increase the likelihood of failure or rejection.

How to stop self-sabotage

If you really want to give a good presentation, you better prepare. I should have trained to win the race. And if you really want to be with your partner, you shouldn’t make them angry by ignoring their messages.

If you’re stuck in a habit of self-sabotage, it will take time to break it, but a healthier approach is within reach. One useful strategy is the so-called “Master Mindset”This includes viewing challenges as opportunities to learn and improve, rather than as deep judgments about your unique skills and worth. If you give your best at a work presentation or a running race and it doesn’t go perfectly, think about how you can do it better next time.

Another helpful strategy is to practice. self-pityThis includes treating yourself with the same kindness you would treat a close friend or relative, and recognizing that your worth does not depend on any particular opinion or outcome of a relationship.

If you feel close to a romantic partner, get used to that feeling of vulnerability and know that even if the relationship ends someday, it doesn’t mean you are inherently broken or unlovable. Remind yourself.

read more:

  • Will being too kind hinder your life?
  • Why some people don’t feel shame, according to psychologists
  • The Ultimate Anxiety Guide: The 6 Biggest Questions About Anxiety Answered by Psychologists
  • Why do I always cry when I watch movies on a plane?

Asked by: Samantha Osborne via email

To submit a question, please email questions@sciencefocus.com (remember to include your name and location)

Source: www.sciencefocus.com

You might be cleaning your reusable water bottle incorrectly

Observing people around your local park, office, or city center, you will likely see many individuals using reusable water bottles. This trend has become a fashion statement and a social connector, in addition to being an environmentally conscious choice. According to NHS health guidelines, drinking 6-8 glasses of water per day from reusable bottles can reduce environmental impact by cutting down on single-use plastic consumption.

However, while using a water bottle is seen as a positive and healthy choice for the planet, there are hidden risks associated with not cleaning them properly. A study by WaterFilterGuru revealed that if water bottles are not cleaned regularly, they can harbor bacteria and mold on their surfaces, leading to potential health issues if consumed.

What is living in your water bottle?

Water, even from a kitchen faucet, is not sterile and can promote bacterial growth within a few days of filling a bottle. Storing water at room temperature can increase microbial growth, while refrigeration can help reduce the proliferation of microorganisms. Microorganisms in water bottles can come from the water itself, but most are transferred from the consumer’s body or surrounding environment.

Various microorganisms found in water bottles include skin and oral bacteria such as Staphylococcus and Streptococcus, which are normally harmless but can cause infections if ingested. Additionally, water bottles can harbor gut bacteria like Escherichia Coli, which can lead to gastrointestinal issues if consumed. Pregnant women, children, the elderly, and those with weakened immune systems are particularly vulnerable to illnesses caused by contaminated water.

The type of liquid used in water bottles also influences microbial growth, with sugary or nutrient-rich drinks creating an optimal environment for bacteria and mold. Even carbonated water, while having antibacterial properties, requires regular cleaning to prevent the accumulation of harmful pathogens.

How to clean a water bottle

Regular cleaning of reusable water bottles is essential to prevent the buildup of bacteria and mold. Washing the bottle with hot water and detergent, letting it soak, and ensuring complete drying can help maintain hygiene. For heavily soiled bottles, a vinegar-water solution can be used for deeper cleaning. It is recommended to clean bottles and accessories like lids and straws after each use or at least several times a week to avoid contamination.

While proper hygiene practices are important to prevent illness, our immune systems are resilient and have evolved to protect us from various pathogens. By maintaining cleanliness and regular cleaning routines, we can continue to enjoy the benefits of using reusable water bottles while staying healthy.

Source: www.sciencefocus.com

As hurricane season wraps up, scientists explore surprising trends

overview

  • The Atlantic hurricane season officially ends Saturday.
  • The pattern of activity surprised forecasters. The season was busy early on, with strong storms occurring later in the season, but quiet during what is normally considered the peak period.
  • Climate change has most likely caused the observed storms to become more intense.

A bizarre and devastating hurricane season officially came to an end Saturday, and forecasters are looking into its many surprises.

Philip Klotzbach, a Colorado State University meteorologist who specializes in Atlantic hurricane forecasting, said, “Every year there are one or two things that bother me, but this year there were more than usual.” he said.

Most forecasters are predicting a very active hurricane season as early as April, and the National Oceanic and Atmospheric Administration has released its best forecast ever.

In the end, there were 18 named storms, 11 hurricanes, and 5 major hurricanes. Although this was at the low end of the range most forecasters expected, it was still above normal and a “very active” season.

What surprised researchers was how strange the season unfolded. It got off to a roaring start in June when Hurricane Beryl became the first Category 5 storm to be observed in the Atlantic Ocean. But from mid-August to early September, everything went quiet. The season typically reaches its peak around September 10th. But it was the first time since 1968 that no named storm formed during those weeks.

Just when researchers thought their predictions were wrong, storm activity picked up again and Hurricanes Helen and Milton struck, causing billions of dollars in damage.

Hurricane Milton made landfall in the Gulf of Mexico on October 8th.
NOAA/NESDIS/Star

“The normal seasonal cycle has been reversed,” Klotzbach said. “What was striking to me was that it was like a switch was flipped, completely off, then completely on. For Helen, nothing happened, and for East Atlantic and Milton, The storm continued.”

Researchers are studying what causes this strange pattern to better understand the factors that cause hurricanes and improve future predictions.

Researchers predicted this spring's hurricane season would be busy and dangerous because of record-high ocean temperatures in the Atlantic Ocean and the possibility that La Niña, a pattern of natural fluctuations, could take hold. Ta. Ocean heat provides fuel for hurricanes and can intensify them faster. La Niña is associated with hurricanes because it often reduces atmospheric stability.

“Early on, we thought it was going to be our busiest season on record,” Klotzbach said.

Although ocean temperatures remained at or near record highs in the North Atlantic, La Niña events did not develop as strongly, said Matthew Rosen, chief hurricane forecaster at the NOAA Climate Prediction Center, a division of the National Weather Service. Krans said.

A combination of other factors most likely contributed to the alarming stagnation in activity.

Approximately 60% of hurricanes occur as a result of Africa's tropical monsoon season. draws moisture into an area called the Sahel. However, this year's monsoon developed elsewhere.

“The monsoon reached so far north and was so strong that it reached areas that hadn't had rain in 45 years,” Rosencrans said, adding that this change had weakened the development of tropical cyclones. Ta.

Rosencrans said another climate pattern, called the Madden-Julian Oscillation, a group of storms that pass near the equator, also likely contributed, with storm development slowing in early September and then later in the month. It is said that hurricanes are starting to occur.

Researchers will spend the winter examining which factors had the most influence through climate and weather models.

“This is an opportunity to learn, to observe systems and let the Earth teach us something new,” he said.

Despite a mid-season interruption due to a tropical storm, 2024 set several records. According to a review published by Klotzbach, five hurricanes have made landfall in the continental United States, tied for the second-highest number in history.

Destroyed and damaged buildings in the aftermath of Hurricane Helen's flooding in Batcave, North Carolina, on October 8.
Tama Mario/Getty Images File
On September 28, heavy rains from Hurricane Helen caused record flooding and damage in Asheville, North Carolina.
Melissa Sue Gerrits/Getty Images File

Helen was the most powerful hurricane to hit Big Bend, Florida. Since September 25th, seven hurricanes have formed in the Atlantic Ocean, the most on record.

Hurricane Milton set a record for tornado warnings in Florida, spawning dozens of tornadoes.

Research suggests climate change has worsened Helen and Milton's symptoms. Both hurricanes underwent a rapid intensification process, with their sustained wind speeds increasing by at least 35 miles per hour over a 24-hour period. This trend is becoming more common as global temperatures rise.

Additionally, scientists studying the effects of climate change on weather have discovered that: Rainfall amounts for single-day events like Milton are currently about 20% to 30% higher due to climate change.. Researchers, in collaboration with the World Weather Attribution project, determined that Milton's wind speeds were likely 10% stronger due to the effects of climate change. The group had similar results during Hurricane Helen.

A destroyed home in Lakewood Park, Florida, on October 10th.
Giorgio Vieira/AFP – Getty Images File

According to a report published by Climate Central, a nonprofit organization that tracks climate change, all 11 of this year's Atlantic hurricanes An additional 9 to 28 miles per hour due to human-induced global warmingmainly due to the record-breaking warmth of the ocean.

Rosenkrans said research generally does not suggest that the number of named storms (winds of 39 miles per hour or more) will change with climate change. However, a larger proportion of named storms are expected to become hurricanes, with the majority of those hurricanes reaching Category 4 or 5. That was the case this year as well.

Source: www.nbcnews.com

The hidden radioactive waste problem lies at the core of achieving net zero emissions

A dog chased a ball past me at full speed across the open fields of Seascale Beach, Cumbria. The beach is surrounded by a small park, rows of shops, and houses, with tall chimneys and large rectangular buildings visible on a vast industrial site as you walk north.

Close to Seascale Beach is the Sellafield complex, a 2 square mile nuclear facility located 5 km away. Sellafield is home to most of the UK’s radioactive nuclear waste and the world’s largest store of plutonium.

I visited Sellafield earlier this year to learn about the management of Britain’s nuclear waste. It was an eye-opening and expensive lesson in dealing with hazardous material with no clear plan.

Sellafield played a crucial role in producing plutonium during the Cold War. The current cleanup operation involves processing and storing spent nuclear fuel, cooling and stabilizing it, then storing it in silos covered with steel and concrete.

Initially, safe long-term storage was not a priority, leading to waste being disposed of from decades ago. The process of moving waste from dilapidated silos to more modern stores is ongoing.

Read More:

  • Meet the rebels building fusion reactors in your neighborhood
  • Where next for nuclear energy?
  • Why do nuclear fission and fusion both release energy?

A recent report by the National Board of Audit highlighted that Sellafield is still in the early stages of the cleanup mission, expected to last until 2125 with an estimated cost of £136bn, showcasing uncertainty about the exact tasks and timeline.

The plan for the most dangerous nuclear waste is to bury it deep underground in a geological disposal facility (GDF). Finding a suitable location involves not just solid rock but also a willing community.

Three communities are currently in discussion about building a GDF facility, with experts believing it to be the best option. Several countries are also working on similar facilities.

The complexity of site selection may delay the facility’s opening until the 2040s or 2050s, amidst a push for new nuclear power to reduce emissions and reach net zero.

As we navigate through the challenges of nuclear waste management, experts like Professor Claire Corkhill from the University of Bristol play a crucial role in advancing our understanding of radioactive waste.


About our expert Professor Claire Corkhill

Claire is Professor of Mineralogy and Radioactive Waste Management in the School of Earth Sciences at the University of Bristol.

Her work has been published in magazines material, nature, and ceramics.

Read More:

  • Nuclear fusion: Inside the construction of the world’s largest tokamak
  • Instant Genius Podcast: The race to bury nuclear waste in hidden bunkers
  • Sticky atoms and devastating iron: The strange science behind nuclear fusion

Source: www.sciencefocus.com

Incredible Scientific Phenomenon of Rainbow Clouds

During midwinter, under the right conditions, the polar sky can be transformed into a colorful spectacle by shimmering clouds.

These rainbow clouds, also known as “nacre clouds” due to their resemblance to iridescent shells, are an incredibly rare atmospheric phenomenon.

Scientifically referred to as “polar stratospheric clouds,” they exist at much higher altitudes in the atmosphere compared to typical clouds. While most clouds are found below 10 km above the Earth’s surface, rainbow clouds form in the lower stratosphere, between 15 and 25 km in altitude.

In the usually dry stratosphere, temperatures dropping below -80°C can cause sparse water molecules to form small ice crystals that eventually gather to create a cloud. These tiny ice crystals scatter sunlight, producing a dazzling rainbow effect and a pearlescent appearance.

Due to their high altitudes, the curvature of the Earth allows sunlight from below the horizon to hit and reflect off the underside of these clouds, illuminating them at dawn and dusk.

Rainbow clouds formed from pure water crystals are the thickest and most vivid, while those formed from air pollutants like nitric acid can result in thin, less impressive clouds. The latter type of cloud is associated with the degradation of the Antarctic ozone layer.

To witness rainbow clouds, consider visiting Antarctica during winter or look up at the sky around sunrise or sunset in parts of Norway, Sweden, Finland, Alaska, or even Scotland. These breathtaking phenomena are a result of unique atmospheric conditions.

This article addresses the question posed by Ollie Peterson via email: “What causes rainbow clouds?”

If you have any inquiries, please contact us at: questions@sciencefocus.comor reach out to us on Facebook, Twitteror Instagram (please include your name and location).

Explore more:

Source: www.sciencefocus.com

New study reveals that one human lineage experienced an increase in brain size

A recent study conducted by researchers at the University of Reading and the University of Durham has revealed that the increase in relative brain size, known as encephalization, during the seven million years of human evolution was a result of incremental changes within individual species.

Modern humans, Neanderthals, and other recent relatives on the human family tree evolved large brains much more rapidly than earlier species. Image credit: SINC / Jose Antonio Peñas.

“One of the most striking evolutionary changes in human evolution, closely linked to the unique cognitive and behavioral characteristics of humans, is the increase in brain size,” explained lead author Thomas Puschel and his colleagues.

“The question of encephalization in human evolution has been a topic of debate, with various studies comparing the brain capacities of different hominin species and exploring adaptive mechanisms that might have influenced differences in brain size among hominins. Our research proposes

“Some argue for a gradual growth pattern over time, while others suggest a pattern of rapid increases followed by periods of stagnation.”

“Certain studies support a combination of both models, while others claim that they are indistinguishable.”

In their recent study, the authors compiled the largest dataset of ancient human fossils spanning seven million years and utilized advanced computational and statistical methods to identify gaps in the fossil record.

These innovative approaches have provided the most comprehensive understanding to date of the evolution of brain size over time.

“This study has completely altered our perception of how the human brain evolved,” noted study co-author Professor Chris Venditti.

“Previously, it was believed that brain size varied significantly between species, like upgrading to newer computer models.”

“However, our study reveals a pattern of steady, incremental ‘software updates’ occurring within each species over millions of years.”

This study challenges the traditional notion that certain species, such as Neanderthals, remained unchanged and were unable to adapt, suggesting instead that the increase in brain size was a gradual and continuous driving force in evolution. It underscores the significance of changes.

“Major evolutionary shifts do not always require dramatic events,” Pushel stated.

“They can result from making small incremental improvements over time, akin to the learning and adaptation processes observed today.”

The researchers also identified a notable pattern: larger-bodied species tend to have larger brains, but the variation observed within individual species does not consistently correlate with body size.

Hence, the evolution of brain size over long evolutionary timescales spanning millions of years has been influenced by factors distinct from those observed within individual species, underscoring the complexities of evolutionary pressures on brain size. It’s remarkable.

“The reasons behind the evolution of large brains in humans are a key aspect of human evolution,” added study co-author Dr. Joanna Baker.

“Through analyzing the brain and body sizes of various species over millions of years, we have demonstrated that the characteristic large brains of humans primarily emerged through gradual changes within individual species. This became evident.”of study On November 26, 2024, Proceedings of the National Academy of Sciences.

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Thomas A. Puschel others. 2024. The increase in human brain size was revealed by intraspecific encephalization. PNAS 121 (49): e2409542121;doi: 10.1073/pnas.2409542121

Source: www.sci.news

Study: Ancient Central European Peasants Lived Equally 8,000 Years Ago

There are no signs of population stratification in the Linear Pottery Culture (LBK) communities that first spread agriculture across much of Europe, according to a new study led by scientists at the University of Vienna and Harvard University. He said he couldn’t see it.

The manual labor of prehistoric central European women was more demanding than the rowing of today’s boat crews.

“The expansion of agriculture in Central Europe occurred in the 6th millennium BC,” said Dr. Pere Gelabert of the University of Vienna and colleagues.

“Within a few generations, Balkan farmers expanded down the Danube Valley into what is now France and eastward into what is now Hungary and Ukraine.”

“The cultural footprint of peasants is homogeneous across this region, which spans thousands of kilometers, but the lack of genetic data from multiple families makes it difficult to understand whether these communities lived on social equality. It has become difficult to assess which individuals have migrated and migrated across continents. “

In the study, Dr. Gelabert and co-authors sequenced and analyzed the genomes of 250 LBK individuals and other extensive datasets.

“The LBK people expanded over hundreds of kilometers in just a few generations,” Dr. Gelabert said.

“We found distant relatives in Slovakia and others in western Germany, more than 500 miles away.”

“In this study, we report for the first time that families in the study sites of Nitra in Slovakia and Polgar Ferencí Hat in Hungary do not differ in terms of the food they consume,” said Dr. Ron Pignasi, a researcher at the institute. said. University of Vienna.

“This suggests that the people living at these Neolithic sites were not stratified based on family or biological sex, understood as differences in access to resources and space. No signs of inequality are detected.”

The LBK culture came to an end around 5000 BC, and various theories have been proposed for its demise.

Some say this period was a period of social and economic crisis, often associated with widespread incidents of violence.

“One of the most famous incidents was the Asparn Schretz massacre in Lower Austria, where more than 100 people were recovered from a ditch,” the researchers said.

“This site, along with Herxheim in Germany, is one of the largest known assemblages of people who were violently murdered during the early Neolithic period, and the skeletons show signs of violence and multiple fractures.”

“Our in-depth genetic studies of the Asparn Schretz people show that fewer than 10 people are genetically related, making it unlikely that this genocide represents a single population. This casts doubt on the hypothesis that there is a

“Previous anthropological studies have noted an underrepresentation of young women, but the new data further support the complete absence of relatives.”

“The large number of children among the victims opens the door to different interpretations of this remarkable event of Neolithic violence.”

of findings Published in a magazine nature human behavior.

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P. Gelabert others. Social and genetic diversity among the first farmers of central Europe. Nat Hum Behavepublished online on November 29, 2024. doi: 10.1038/s41562-024-02034-z

Source: www.sci.news

Unlocking the Mystery of Dinosaur Dominance: Fossilized Poop Holds Clues

We now know that dinosaurs were large reptiles that ruled the Earth, but scientists have always been curious about why it took them 30 million years to reach their peak. New research on fossilized poop and vomit may have found the answer – food.

According to the study, carnivorous dinosaurs like Tyrannosaurus may owe their massive size to their plant-eating ancestors. If these herbivores hadn’t consumed so many plants, researchers suggest that dinosaurs might not have evolved into the colossal creatures we know today.

The fossilized poop and vomit, dated back to about 230 to 200 million years ago, provide insights into the ancient food web. By studying over 500 fossils, scientists identified various prey items from beetles to bones, shedding light on the evolving food chains during the Triassic period.

By combining this information with climate data and other fossils, researchers gained valuable knowledge about the prehistoric environment and the species that coexisted with dinosaurs on Earth.

“Sometimes seemingly ordinary fossils hold extraordinary information that is invaluable,” said study co-author Dr. Martin Kvarnström from Uppsala University in Sweden, as reported by BBC Science Focus.

Co-author Dr. Grzegorz Niedzwicki added, “Understanding the dietary habits of early dinosaurs can offer insights into their success as a group and the importance of predator-prey relationships in shaping Earth’s evolutionary history.”

The study, featured in Nature magazine, analyzed digestive samples from south-central Poland, providing clues about the Late Triassic period and the changes in vegetation during that time.

By employing advanced scanning techniques, researchers were able to visualize intricate details of the fossils, unveiling significant discoveries about the size and distribution of vertebrate populations before the dominance of dinosaurs.

Scientists scanned more than 500 fossils for the study. – Illustration: Qvarnström et al., Nature, 2024

This research model opens up opportunities to explore ancient species in different regions worldwide, emphasizing the importance of analyzing fossilized remains beyond just skeletal findings.

“We aim to highlight the significance of saprolites in reconstructing ancient ecosystems, moving beyond their conventional perception as mere curiosities,” noted Kvarnström.

“While everyone focuses on fossilized skeletons, it is the organic remains that provide crucial insights into the ancient ecological dynamics,” added Niedzwicki.

About our experts:

Dr. Martin Kvarnström, a researcher at Uppsala University, specializes in using fossils to study reptilian diets, particularly dinosaurs.

Dr. Grzegorz Niedzwicki, also a researcher at Uppsala University, focuses on the early evolution of dinosaurs and quadrupeds.

Read more:

Source: www.sciencefocus.com

Two hominin species lived together in Kenya 1.5 million years ago

Paleoanthropologists have discovered 1.5 million-year-old footprints of two very different species of humans. homo erectus and Paranthropus boisei — at the same location near Lake Turkana in Kenya.

A 3D computerized model of the surface of an area near Lake Turkana in Kenya shows fossil footprints. Paranthropus boisei (vertical footprint) separate footprint homo erectus Form a vertical path. Image credit: Kevin Hatala / Chatham University.

Hominin is a term that describes a subdivision of the larger category known as Hominidae.

The hominid family includes all extinct and living organisms that are thought to belong to the human lineage that emerged after we separated from our great ape ancestors. This is thought to have happened about 6 to 7 million years ago.

Paleoanthropologists have long hypothesized that: homo erectus and Paranthropus boisei They coexisted.

According to the fossil record, homo erectus It lasted another million years.

Paranthropus boiseiHowever, they became extinct within a few hundred thousand years. Scientists don’t know why.

Both species had an upright posture and bipedal gait, and were very agile. We still know little about how these coexisting species interacted culturally and reproductively.

“Footprints are important because they fall into the category of trace fossils, which includes footprints, nests, and burrows,” said Craig Feibel, a professor at Rutgers University.

“Trace fossils are not parts of living things, but they provide evidence of behavior. Fossil body parts, such as bones and teeth, are evidence of past life, but they are easily displaced by water and predators. ”

This is a reconstruction by the artist homo erectus. Image credit: Yale University.

Professor Feibel and his colleagues discovered footprints from 1.5 million years ago. homo erectus and Paranthropus boisei Near Lake Turkana in Kenya.

“By being on the same surface and forming closely together over time, these two species are located at the edge of the lake and use the same habitat,” Professor Feibel said.

“Skeletal fossils have long provided the primary evidence for studying human evolution, but new data from fossil footprints reveals fascinating details about the evolution of human anatomy and locomotion. , giving further clues about ancient human behavior and the environment,” said Dr. Kevin Hatala. , a researcher at Chatham University.

“Fossil footprints are interesting because they provide a vivid snapshot of our fossil relatives coming to life.”

“These types of data can help us understand how living individuals millions of years ago moved through their environments, interacted with each other, and potentially interacted with other animals. Masu.”

“That's something you can never get from bones or stone tools.”

Paranthropus boisei. Image credit: © Roman Yevseyev.

The authors used a new method they recently developed that allows them to perform 3D analysis to distinguish one footprint from another.

“Biological anthropology is always interested in finding new ways to extract behavior from the fossil record, and this is a great example,” said Dr. Rebecca Ferrell, program director at the National Science Foundation.

“The team used state-of-the-art 3D imaging technology to create a completely new way to observe footprints, which will help us understand human evolution and the role of cooperation and competition in shaping our evolutionary journey. It will help.”

of findings Published in today's diary science.

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Kevin G. Hatala others. 2024. Footprint evidence of locomotor diversity and common habitats in early Pleistocene hominids. science 386 (6725): 1004-1010;doi: 10.1126/science.ado5275

Source: www.sci.news

New review highlights the numerous health benefits of staying well-hydrated

Drinking enough water can help with weight loss and prevent kidney stones as well as migraines, urinary tract infections, and low blood pressure, according to a new systematic review of 18 randomized clinical trials.

A systematic review of 18 randomized clinical trials found that interventions that increased water intake (or decreased intake in some studies) were associated with statistically significant increases in weight loss and reductions in kidney stone events. A single study suggested benefits related to migraine prevention, urinary tract infections, diabetes management, and lower blood pressure, but did not reach statistical significance. Image credit: Günther.

Water is a major component of the human body and is considered an essential nutrient that cannot be produced in sufficient quantities through metabolism.

The National Academy of Medicine recommends a daily fluid intake of approximately 13 8-ounce cups for men and 9 cups for women.

A common public health recommendation is to drink 8 cups of water per day, but the evidence supporting this is not clear.

Determining a single optimal daily water intake is a difficult concept, given the wide variation in body weight, activity levels, and health status at the population level, and the numerous mechanisms that regulate water balance.

Because of the known negative effects of dehydration, behavioral factors and hydration status have been widely studied in relation to health conditions.

Professor Benjamin Breyer of the University of California, San Francisco, and colleagues aimed to summarize the evidence from randomized clinical trials on the effects of increasing daily water intake on health-related outcomes.

“We wanted to take a closer look at such a ubiquitous and simple intervention, as the evidence is not clear and the benefits are not well established,” Professor Breyer said.

“Although the amount of rigorous research turned out to be limited, there were statistically significant benefits in some specific areas.”

“To our knowledge, this is the first study to broadly evaluate the benefits of water intake on clinical outcomes.”

Researchers have found the most evidence supporting drinking water to prevent kidney stones and lose weight.

Drinking 8 cups of water a day significantly reduced the chance of kidney stones recurring.

Some studies have found that drinking about 6 glasses of water a day can help adults lose weight.

However, a study of adolescents found that drinking just over 8 cups of water a day had no effect.

Still, encouraging people to drink water before meals is a simple and inexpensive intervention that could have significant benefits, given the rise in obesity.

Other studies have shown that water can help prevent migraines, manage diabetes and low blood pressure, and prevent urinary tract infections.

Adults with recurring headaches felt better after drinking more water for three months.

Drinking about 4 more cups of water a day helped diabetics with elevated blood sugar levels.

Drinking an additional 6 cups of water per day also helped women with recurrent urinary tract infections. The number of infected people has decreased and the time between infections has increased.

And drinking more water helped young people with low blood pressure.

“Dehydration has been shown to be particularly harmful for people with a history of kidney stones or urinary tract infections,” says Professor Breyer.

“On the other hand, people who sometimes suffer from frequent urination may benefit from drinking less alcohol. There is no one-size-fits-all approach when it comes to water consumption.”

of the team paper Published in a magazine JAMA network open.

_____

Nizar Hakam others. 2024. Results of randomized clinical trials testing changes in daily fluid intake: a systematic review. JAMA Net Open 7 (11): e2447621;doi: 10.1001/jamanetworkopen.2024.47621

Source: www.sci.news

Astronomers find scorching-hot Neptune close to TOI-3261

Orbit of newly discovered exoplanet TOI-3261 (also known as TIC 358070912) is an inactive main sequence star located 300 parsecs (978.5 light years) away in the constellation Hydra.

Artist's concept of the super-hot Neptunian exoplanet TOI-3261b. Image credit: NASA/JPL-Caltech/K. Miller, Caltech & IPAC.

The radius of this newly discovered exoplanet, named TOI-3261b (TIC 358070912b), is 3.82 Earth's radius.

Its mass is 30.3 times that of Earth, more than twice the median mass of Neptune-sized planets in longer orbits.

To determine these properties, astronomer Emma Nabby from the University of Southern Queensland and her colleagues used data from NASA's Exoplanet Survey Satellite (TESS), the Las Cumbres Observatory's Global Telescope, and the ESPRESSO and HARPS instruments. I used

“In our measurements, TOI-3261b is exactly hot neptune desert “The planets are so rare that their rarity evokes images of desolate landscapes,” the astronomers said in a statement.

“This type of exoplanet is similar in size and composition to our own Neptune, but it orbits very close to its star.”

The planet orbits its parent star, TOI-3261, every 21 hours.

Such a narrow orbit has so far allowed the planet to belong to the same group as only three other ultrashort-period, high-temperature Neptunes: LTT-9779b, TOI-849b, and TOI-332b.

“TOI-3261b has proven to be an ideal candidate for testing new computer models of planet formation,” the researchers said.

“One reason hot Neptunes are so rare is that it's difficult to maintain a thick gaseous atmosphere in the immediate vicinity of the star.”

“Because stars are massive, they exert a large gravitational force on surrounding objects and can strip away layers of gas surrounding nearby planets.”

“It also releases a lot of energy and blows away the gas layer.”

“Both of these factors mean that a hot Neptune like TOI-3261b may have started out as a much larger Jupiter-sized planet and then lost most of its mass.”

The TOI-3261 system is about 6.5 billion years old, and the planet began as a much larger gas giant, the researchers said.

“But it likely lost mass in two ways: by photoevaporation, where energy from the star causes gas particles to dissipate, and by gravity from the star, which strips layers of gas from the planet. tidal separation,” the scientists said.

“It's also possible that the planet formed further away from the star, where both of these effects would be less strong and it would be able to maintain an atmosphere.”

“The planet's remaining atmosphere is one of its most interesting features and will likely invite further atmospheric analysis, perhaps helping to elucidate the formation history of this hot Neptunian desert dweller.”

“TOI-3261b's density is about twice that of Neptune, indicating that the lighter parts of the atmosphere have been removed over time, leaving only the heavier components,” the researchers added.

“This suggests that the planet must have started out with a variety of elements in its atmosphere, but at this stage it's difficult to know exactly what they are.”

This finding is reported in the following article: paper Published in astronomy magazine.

_____

Emma Naby others. 2024. Survival in the Hot Neptunian Desert: Discovery of the ultrahot Neptune TOI-3261b. A.J. 168, 132; doi: 10.3847/1538-3881/ad60be

Source: www.sci.news

Ancient Footprints Reveal Two Human Relative Species Coexisted Together

overview

  • Ancient footprints discovered in Kenya belong to two different species of human relatives who walked on the same ground at the same time, a study has found.
  • This coat of arms is thought to belong to the species Homo erectus and Paranthropus boisei.
  • This discovery raised questions about what kind of relationship and interaction the two species had.

A newly discovered set of footprints in Kenya provides the first evidence that two different species of ancient human relatives walked on the same ground at the same time 1.5 million years ago.

Researchers involved in the discovery say the footprints belong to the species Homo erectus and Paranthropus boisei, and were left within hours to days of each other, meaning that when the two crossed paths, reveals new mysteries about what happened.

According to research on this discovery, Published in Science on Thursdaythe footprints were buried in dry mud near a lake in northern Kenya, and were buried in deposits of prominent fossil sites. By analyzing the print shapes and strike patterns, the researchers found that the two sets were different. They concluded that the best explanation was that two different species left the footprints.

This research advances anthropologists and paleontologists’ understanding that ancient human relatives likely interacted and coexisted. This also raises the question of what kind of relationship these species had.

“We think these individuals, the two species that were there, were probably aware that there were members of another species nearby. They saw each other and thought each other was a member of another species. “This raises the question of what that interaction was,” said Kevin Hatala, an associate professor of biology at Chatham University and lead author of the study. “Were they competitors? Were they totally okay with each other there?”

Previously discovered fossil skeletons of Homo erectus and Paranthropus boisei indicated that both species lived in the area at some point, but the new discovery provides evidence of a direct duplication.

Research team members excavate to reveal footprints.
Neil T. Roach / Harvard University

It also shows that the two species walked on two legs in very different ways.

Although both Homo erectus and Paranthropus boisei are related to humans, they have very different characteristics and their fates in the human evolutionary tree took very different paths.

Homo erectus had an anatomy similar to humans from the neck down. This species may have used stone tools and cooked over fire. Its members probably had a varied diet that included meat.
The species eventually spread to Asia, Indonesia, and other regions, and survived for more than a million years after the newly discovered footprints were made.It last appeared in the fossil record just over 100,000 years ago..

“Many have considered themselves to be as good candidates as our direct ancestors,” Hatala said. “They seem to be a very successful species.”

Paranthropus boisei, on the other hand, featured a smaller brain, huge masticatory muscles, and large molar teeth. William Harcourt Smith, an associate professor of anthropology at Lehman College who was not involved in the study, said the species eats difficult-to-eat foods like hard nuts or grinds hard, poor-quality foods like shrubs. It is highly likely that they evolved in this way.

This species did not persist on Earth as long as Homo erectus.

“They probably went extinct not very long after that, within the next few hundred thousand years,” Hatala said, referring to the time of the footprints. He added that no one knows exactly what happened, but it’s possible that environmental changes may have restricted the animal’s specialized diet.

The footprints were first discovered in 2021 at a site called Koobi Fora while researchers were excavating other fossils. This location has become a fossil hotspot. The uplifted rocks expose older sedimentary layers on the surface, giving researchers access to the bones of ancient humans and other animals.

The following year, researchers unearthed about a dozen footprints that appeared to be walking in a line, and later discovered other footprints running at right angles.

“We think these footprints were created in the mud of this lakeshore environment. Something happened that brought sediment on top of it. It could have been deposited by a small flood or by rising water levels. “It’s possible that something was brought in and the footprints were formed and quickly buried,” Hatala said.

The muddy footprints were not trampled by other animals and showed no signs of cracking before being buried in the sand. Researchers said that means they were separated from each other within hours or days.

“The sediment protected them, prevented them from cracking, and allowed them to remain in the geological record,” Hatala said.

He and his co-authors believe that the two species may have been able to coexist in this region because their diets were very different. It is possible that they competed for resources and were in a hostile relationship. This species appears to have lived in the same area for hundreds of thousands of years.

Harcourt Smith, a research paleontologist at the American Museum of Natural History, said the researchers’ analysis was sound and the site was unique.

“I want to emphasize how unusual it is that a site like this exists, how special it is, and the great opportunity we have to find out more,” he said.

Broadly speaking, over the past seven million years of evolution, it has become increasingly clear that different ancient human species interacted in different habitats, Harcourt-Smith added. The evolutionary path to modern humans is full of side branches and species, such as Paranthropus boisei, which represent evolutionary dead ends.

“Human evolution is complex and messy, and there are many experiments being done. It’s not a straight line,” he said.

Over the past few decades, scientists have developed genetic and archaeological evidence showing that: Humans, Denisovans, and Neanderthals overlapped and sometimes interbred. Although the new study does not mention interbreeding, it does provide a clearer picture that even older species overlapped and had more interactions than previously understood.

The researchers completed their work at the Koobi Fora site, photographing and recording the footprints in a variety of ways before concealing them for future generations, said Craig, another author of the research paper.・Mr. Feibel said.

“The footprints need to be carefully refilled with non-damaging sediment to prevent erosion,” he says.


Source: www.nbcnews.com

Ancient footprints reveal how early human species lived together

Footprints thought to have been left by an individual of Paranthropus boisei

Neil T. Roach

Preserved footprints in Kenya appear to record two different species of ancient humans walking along the same muddy lake shore, perhaps within days of each other. This is one of the most dramatic pieces of evidence ever discovered that multiple human species once coexisted in the world.

“It's really unusual to find evidence of two different species walking on that surface,” he says. Kevin Hatala at Chatham University in Pittsburgh, Pennsylvania.

footprints Discovered in 2021 Kobi Fora, Kenya, near the eastern shore of Lake Turkana. They were first discovered by team member Richard Loki. Turkana Basin Research Institute“Originally, there was a team of Kenyans working there,” Hatala says.

The researchers discovered a track consisting of 12 footprints preserved in a layer of dry sand and silt (see image above). This was apparently left behind by one person walking in a straight line. Near the main group were also three isolated prints that appeared to have been made by three different individuals. The lack of mud cracks or signs of overprinting with other tracks indicates that these prints were all made at about the same time. “These sites are probably capturing times ranging from minutes to days,” Hatala says.

This deposit was determined to be approximately 1.52 million years old. Isolated footprints are similar to footprints left by modern humans. Your heel touches the ground first, then your foot rolls forward and you push off with the sole of your foot. Hatala and his colleagues suggest that these may have been fabricated. homo erectusis known to have lived in this area.

In contrast, continuous trajectories were created by flatter-footed hominins. Hatala and his colleagues suggest that this could be Paranthropus boiseianother type of hominin that lived in this area.

The footprint fossil on the left, with its deeper heel marks, is thought to have been made by Homo erectus, and the more flat-footed fossil on the right is thought to have been made by Paranthropus boisei.

Kevin Hatala/Chatham

“With footprints, you can never be 100% sure who made them,” he says. Ashley Wiseman from University College London was not involved in the study but, H. erectus and P.Boisei. They are the only humans whose remains have been found preserved in this area, “so we can make an informed guess that it is these two individuals.”

If the track was really made by humans, P.Boisei Wiseman said the specimen appears to have been walking on two legs. The bones of the skull, arms, and legs are paranthropus“We've never found a skull associated with the rest of the skeleton,” she says, meaning little is known about their bodies beyond their heads, and the way they walk remains a mystery. The trajectory will be changed, saying, “This is clear evidence that it was walking on two legs.''

These two species were very different. H. erectus It was one of the earliest members of our genus, homo. They had larger brains than early humans and were the first clade to travel outside of Africa. in contrast, P.Boisey They had large teeth and jaws, small brains, and were apparently adapted to eating chewy foods like grasses and sedges.

Hatala and his team then looked at other known footprints found in the same area and at the same time and found that they appeared to match either species. “Similar patterns have been seen at other sites, which may span more than 100,000 years,” he says. “These two species appear to have coexisted with each other in this same familiar landscape for a very long time.”

“If they were able to coexist for more than 100,000 years, we speculate that there was probably a low to neutral level of competition,” Hatala says. Previous research suggests that the two people were eating different foods. Unlike P.Boisei, H. erectus It is thought that they had a varied diet, including hunting large animals.

“Both could carve out their own existence within this shared landscape,” Hatala says. Subsequent changes in the environment may have had an effect. P.Boisei Potentially extinct, yet more adaptable H. erectus Survived.

topic:

  • evolution/
  • evolution of humanity

Source: www.newscientist.com

The bonding power of Cheerios leads to creation of innovative robot

A Cheerios-inspired robot that emits alcoholic fuel using fluorescent dye.

Jackson K. Wilt et al. 2024

The same phenomenon as beetles floating on a pond and Cheerios growing in clusters. You can combine them inside a cereal bowl to make a small floating robot.

One such effect, the Marangoni effect, occurs when a fluid with a low surface tension spreads rapidly across the surface of a fluid with a high surface tension. To take advantage of this effect, stenus There are beetles that have evolved to fly around ponds by secreting a substance called stenusin, and toy boats that run on soap.

To explore how engineers can use this, jackson wilt Harvard University and his colleagues 3D printed round plastic pucks about 1 centimeter in diameter. Each had an air chamber for buoyancy and a small fuel tank containing 10 to 50 percent alcohol, which has a lower surface tension than water. The alcohol gradually leaks out of the pack and the pack moves across the surface of the water.

The researchers used alcohol, which evaporates, as fuel, unlike soap, which ends up contaminating the water and ruining the Marangoni effect. It turns out that the stronger the alcohol, the better the results. “The beer would be pretty bad,” Wilt says. “Vodka is probably the best thing you can use. Absinthe…that's a lot of propulsion.” At top speed, the robot moves at 6 centimeters per second, and some experiments propelled the puck for as long as 500 seconds. It has been confirmed that

By printing pucks with multiple fuel outlets and gluing them together, researchers can also create larger devices that can make wide curves or rotate in place. Using multiple packs also allows researchers to study the “Cheerios effect,” where cereals and other similar floating objects cluster together. This occurs because they form a meniscus, or curved surface, in the fluid, and these surfaces are attracted to each other.

Wilt said 3D printed devices could be useful in education to help students intuitively understand concepts related to surface tension, but could also be carefully designed to produce more complex and elegant behavior. If this technology is developed, it can be expected to be applied to environmental and industrial processes.

For example, if there is a substance that needs to be dispersed throughout the environment and also acts as a suitable fuel, the robot can automatically disperse it around it. “Say you have a body of water that needs to release a chemical and you want it to be distributed more evenly, or say you have a chemical process that needs to deposit material over time,” Wilt says. . “I feel like there's some really interesting behavior here.”

topic:

Source: www.newscientist.com

Lessons from history: Strategies for defeating a wild emu

COP load of this

As COP29, the latest round of international climate negotiations, struggles in Azerbaijan, Feedback watches bemused from afar. We have previously covered several COPs and are still on most of the relevant mailing lists. So, as I write this on November 18th, we know that the Climate Action Network's Fossil of the Day is South Korea. That's because South Korea single-handedly blocked a deal by high-income countries to end oil and gas subsidies. Yes, that's enough.

Holding a conference dedicated to reducing greenhouse gas emissions in a country as heavily dependent on fossil fuel exports as Azerbaijan was always likely to backfire. Feedback believed that diplomacy was about understanding other people's motives, but apparently no one could reconcile what the Azerbaijani government wanted. Soon, President Ilham Aliyev announced that oil and gas “gift from god'', the country's chief negotiator was photographed saying in his opening speech. Apparently they are arranging it A meeting to discuss fossil fuel trading.

Then the conference actually started – or rather, it didn’t really start. On the first day, work stalled within the first hour as several countries objected to the rest of the meeting's agenda. This is how I spent my first day Renegotiating the agendawhile the delegates sat around with nothing to do. Still, climate change is not an urgent problem.

Feedback would like to think things are only uphill from here, but the experience of the past decade suggests otherwise. And I still get shivers when I think about the last night of one of the COPs we attended. It was well past the evening, so the agreement was signed and the party was supposed to start. But then we see young diplomats carrying stacks of take-out pizza boxes into the negotiating room, and we realize that even in the best case scenario, we'll be there until the early hours of the morning. I noticed. Feedback does not endorse this experience or any cases of caffeine addiction associated with it.

Find your inner villain

News Editorial Assistant Alexandra Thompson calls our attention to a brilliantly titled paper about the psychology research repository PsyArXiv.What it means to be a true badass: An experimental investigation of a commonplace concept.”. Its authors, Briana Nguyen and Michael Prinzing, set out to explain what we mean when we say someone is a “bad person.” It's not clear, since both Genghis Khan and Malala Yousafzai could be called villains, but “they are about as different as you can imagine,” they say. Well, quite a bit.

Researchers used a series of online surveys to find out what kinds of people were counted as bad guys and what kinds of people were not. From this, it became clear that “badass'' is a two-layered concept. It has a superficial meaning of being physically strong or having a “fearsome presence.” But there's also a deeper inner meaning about “moral resilience and courage.”

According to the author, Yousafzai embodies this inner evil, while Khan embodies more of the external evil. Feedback is less certain. We read a biography of Khan by John Mann, and he showed remarkable courage in a difficult situation. Still, the distinction between inner and outer badasses sounds plausible.

Feedback sometimes enjoys this kind of research, which delves into the subtle meanings of everyday terms, in quiet moments. A classic example is Harry Frankfurt's book About bullshit. Frankfurt was a philosopher who distinguished between lying (telling a falsehood with the purpose of clearly misleading someone) and bullshit (telling a lie, regardless of its truth or falsity, in order to serve one's own purpose).

About bullshit is useful to read because it explicitly states what we all implicitly understand. Once the concept is clear, it's easier to find examples, which is why June's paper was frankly titled.ChatGPT is bullshit“It's also great to have a term that is accurate and allows for the overused swear words. We think Frankfurt was the worst.

emu in flight

On November 15th, CBS News published twowild and untrainedAn emu (are there other types?) has escaped in South Carolina. They had apparently escaped three months earlier, but their escape didn't garner any attention until 43 monkeys escaped from a medical research facility in the same state. As of November 18th, Six of the monkeys remained at large.. Faced with hordes of marauding monkeys on the run, journalists began looking for similar stories and found (or rather, didn't find) rogue emus.

Feedback doesn't get any lower than at your local police department.Not EMU-SED“However, we would like to reiterate the following point. matthew downhour About Blue Sky: “Okay, if you didn't want them to get out of control and be irresponsible, why did you name them like that?“?That's a good question because the emus' names are Thelma and Louise.

If US authorities are unable to recapture the bird, they may take notes from the Australians. fought a famous short war against wild emus in 1932. surely, The emu decisively won the conflict.But failure is the best teacher.

Have a story for feedback?

You can email your article to Feedback at feedback@newscientist.com. Please enter your home address. This week's and past feedback can be found on our website.

Source: www.newscientist.com

Could fossilized excrement unlock the secrets of dinosaur dominance on Earth?

We now know that dinosaurs were giant reptiles that dominated the Earth, but scientists have long wondered why it took them 30 million years to reach their peak. New research on their fossilized poop and vomit may have found the answer suggests that there was food in their waste.

Carnivorous dinosaurs like tyrannosaurus may have their herbivore ancestors to thank for their enormous size. The researchers propose that if these plant-eating animals hadn’t ingested so many plants, dinosaurs might not have evolved into the giant creatures we know today.

The fossilized poop and vomit, known as bromalite or copralite, dates back to around 230 to 200 million years ago, a time long before the reign of the tyrannosaurus and the Chicxulub asteroid impact that led to the extinction of dinosaurs.

Scientists reconstructed a “food web” from the undigested meals of early dinosaurs, revealing the intricate relationships between different species during the Triassic period. By scanning over 500 fossils, they found evidence of various organisms, including beetles, bones, and partially digested fish.

Combining this information with climate data and other fossils provided insights into the diverse flora and fauna coexisting with dinosaurs on Earth.

“Sometimes seemingly ordinary fossils contain remarkable information that cannot be found anywhere else,” said Dr. Martin Kvarnström, a study co-author from Uppsala University in Sweden, as reported by BBC Science Focus.

Dr. Grzegorz Niedzwicki, another co-author from Uppsala University, added, “Understanding the diet of early dinosaurs may help us grasp why this group thrived. The evolution of life on Earth hinges on predator-prey dynamics and feeding habits.”

A study published in Nature analyzed digestive samples from south-central Poland during the Late Triassic period when the region was part of the Pangea supercontinent.

According to experts, increased volcanic activity and humidity favored the growth of moisture-loving plants during this time, potentially influencing the evolution of dinosaurs.

The study utilized advanced scanning techniques to reveal detailed information from the fossils, highlighting changes in vertebrate populations leading up to the dominance of dinosaurs.

The researchers aim to apply this model to study ancient species in other regions and emphasize the importance of fossilized waste in reconstructing ancient food webs.

“Everyone is focused on finding fossilized skeletons, but it’s the waste that offers valuable insights into events from millions of years ago,” remarked Niedzwicki.

About our experts:

Dr. Martin Kvarnström is a researcher at Uppsala University in Sweden, focusing on using fossils to understand reptile diets, including dinosaurs.

Dr. Grzegorz Niedzwicki, also from Uppsala University, specializes in the early evolution of dinosaurs and other quadrupeds.

Read more

Source: www.sciencefocus.com

Analysis of fossilized stomach contents provides insight into the origins of dinosaurs

Swedish and Polish paleontologists are using hundreds of fossilized fecal and vomit samples from the Polish Basin in central Europe to reconstruct the rise of dinosaurs to play a dominant role in Earth’s ancient ecosystems. I investigated.



Bone-crushing archosaur fecal fossil smoke, smoke In the background is reconstruction. Image credit: Grzegorz Niedzwiedzki.

The fossil record shows that dinosaurs evolved during the mid-Triassic period (247 to 237 million years ago).

However, the dominance of dinosaurs in terrestrial ecosystems was not seen until the early Jurassic period, about 30 million years later.

Although many non-dinosaur tetrapods (four-limbed vertebrates) were expelled during this period, questions remain as to why dinosaurs came to dominate the ecosystem.

“The real detective work is piecing together ‘who ate who’ in the past,” said Martin Kvarnström, a paleontologist at Uppsala University.

“Being able to examine what animals ate and how they interacted with their environment helps us understand what enabled dinosaurs to be so successful.”

Dr. Kvarnström and his colleagues reconstructed the food web using more than 500 fossilized remains of digestive material (such as feces and vomit), known as bromalite, collected from the Polish Basin, which spans the Late Triassic to Early Jurassic period. We investigated this transition by constructing a.

“The research material was collected over a period of 25 years,” said Dr. Grzegorz Niedrzywicki, a paleontologist at Uppsala University and the Polish Geological Institute.

“It took years to piece everything together and paint a coherent picture.”

“Our study is innovative because we chose to understand the ecology of early dinosaurs based on their dietary preferences.”

“There were a lot of surprising discoveries along the way.”

Analysis of these remains (including 3D imaging of internal structures to reveal undigested food content) is compared to the existing fossil record, along with climate and botanical data, to determine the size and presence of vertebrates during this period. We estimated the change in quantity.

These data indicate that non-dinosaur tetrapods replaced omnivorous ancestors of early dinosaurs that evolved into the first carnivorous and herbivorous dinosaurs towards the end of the Triassic.

Researchers now believe that environmental changes associated with increased volcanic activity may have led to a greater variety of plant prey, which in turn led to the emergence of larger and more diverse herbivore species. Suggests.

This led to the evolution of even larger carnivorous dinosaurs by the beginning of the Jurassic period, completing the transition to dinosaur dominance within the ecosystem.

This analysis sheds light on the emergence of dinosaur dominance within the Polish Basin ecosystem.

“Our findings support the idea that stochastic processes and competitive advantage enabled dinosaurs’ great evolutionary success,” the authors said.

“Dinosaurs gradually achieved supremacy over 30 million years of evolution.”

“The processes illustrated by the Polish data may explain global patterns and shed new light on the emergence of environmentally dominated dinosaur dominance and gigantism that persisted until the mass extinction at the end of the Cretaceous.” We suggest that there is a

team’s paper Published in a magazine nature.

_____

M. Kvarnström others. Digestive content and food webs record the advent of dinosaur supremacy. naturepublished online on November 27, 2024. doi: 10.1038/s41586-024-08265-4

Source: www.sci.news

Archaeologists Find North Americans Made Needles from Bones of Canids, Cats, and Hares

A 12,900-year-old bone needle discovered at the La Preure site in Wyoming, USA, was made from fox bone. rabbit. This could include felines such as bobcats, pumas, lynx, and even the now extinct American cheetah. New research from the University of Wyoming shows that the bones of these animals are sized to make bone needles, remain attached to fur sewn into intricate clothing, and are readily available within campgrounds. It is said to have been used by early Paleoindian gatherers at La Prele.

La Prele Bone Needle and Needle Preform Reconstruction and Comparison Micro-CT Scan of Animal Specimens. Image credit: Pelton others., doi: 10.1371/journal.pone.0313610.

la prele Early Paleoindian mammoth trapping site and campground on a tributary of the North Platte River near Douglas, Wyoming.

Ten seasons of excavation in four major blocks yielded tens of thousands of artifacts related to a single occupation.

Among the wide variety of artifacts recovered from the site so far are fragments of 32 bone needles.

“Our study identifies for the first time the species and possible elements from which Paleoindian people produced bone needles with eyes,” said Wyoming State Archaeologist Spencer Pelton and colleagues.

“Our results provide strong evidence that tailored clothing is produced using bone needles and fur from fur-bearing animals.”

“These garments partially enabled the dispersal of modern humans into northern latitudes and, ultimately, the colonization of the Americas.”

In their study, Dr. Pelton and his colleagues examined bone needle fragments taken from the La Prele site.

The researchers used peptides (short chains of amino acids) obtained from these artifacts to identify animals known to have existed during the Paleoindigenous period, which refers to the prehistoric period of North America between 13,500 and 12,000 years ago. peptide.

As a result of the comparison, it was concluded that the bones of the red fox are bones. Bobcat, puma, lynx, or American cheetah. At La Preure, hares and rabbits were used to make needles.

“Despite the importance of bone needles in explaining the global dispersal of modern humans, archaeologists have not identified the materials used to make bone needles, making this important cultural innovation “This limits our understanding of the

Previous research has shown that to cope with the cold temperatures of northern latitudes, humans likely created tailored clothing with tightly sewn seams that provided a barrier against the elements.

There is little direct evidence of such clothing, but there is indirect evidence in the form of bone needles and the bones of fur owners whose fur was used for clothing.

“Wearing such clothing allowed modern humans to extend their range into areas that were previously inaccessible due to the threat of hypothermia and death from exposure. '' said the scientists.

“How did the people of La Prele Ruins obtain fur-bearing animals?

“It was probably a trap, not necessarily looking for food.”

“Our results are a reminder that foragers used animal foods for a wide range of non-subsistence purposes, and that the mere presence of animal bones at an archaeological site need not indicate a diet. ”

“Combined with a review of comparable evidence from other North American Paleoindian sites, our results suggest that early Paleoindians of North America had direct access to fur-bearing predators, probably by traps, and that It represents some of the most detailed evidence ever discovered regarding Indian clothing.

of findings Published in a magazine PLoS ONE.

_____

SR Pelton others. 2024. Early Paleoindians used canids, felines, and hares to produce bone needles at the La Prele site in Wyoming, USA. PLoS ONE 19 (11): e0313610;doi: 10.1371/journal.pone.0313610

Source: www.sci.news

Astronomers witness Jupiter’s ephemeral dark polar ellipse in ultraviolet light

Earth-sized ovals at Jupiter's north and south poles, visible only at ultraviolet (UV) wavelengths, appear and disappear at seemingly random intervals, according to a study led by astronomers at the University of California, Berkeley.

False-color ultraviolet image of the entire planet showing a hood or cap of hydrocarbon fog covering the south pole. The edge of the arctic hood is visible at the top. Image credit: Troy Tsubota and Michael Wong, University of California, Berkeley.

Jupiter's dark ultraviolet ellipses are mostly located directly beneath bright auroral bands at each pole, similar to Earth's northern and southern lights.

This spot absorbs more ultraviolet light than the surrounding area, so it appears darker in images from the NASA/ESA Hubble Space Telescope.

In annual images of the planet taken by Hubble between 2015 and 2022, dark ultraviolet ellipses appear 75% of the time at the south pole, but only in one in eight images taken at the north pole. A dark oval will appear.

The dark ultraviolet ellipses suggest that unusual processes are occurring in Jupiter's strong magnetic field. This magnetic field propagates all the way to the poles and deep into the atmosphere, much deeper than the magnetic processes that produce auroras on Earth.

The dark ultraviolet ellipse was first detected in the 1990s by Hubble at the North and South poles, and later also at the North Pole by NASA's Cassini spacecraft, which flew close to Jupiter in 2000, but received little attention.

In a new analysis of Hubble images, University of California, Berkeley undergraduate student Troy Tsubota and his colleagues found that the oval shape is a common feature of Antarctica. They counted eight Southern Ultraviolet Dark Ovals (SUDOs) between 1994 and 2022.

In all 25 Hubble Earth maps showing Jupiter's north pole, only two northern ultraviolet dark ellipses (NUDOs) were found.

Most of the Hubble images were taken as part of the Outer Planet Atmospheres Legacy (OPAL).

“In the first two months, we realized that these OPAL images were kind of a gold mine. We quickly built this analysis pipeline and asked what we could get by sending all the images. We were able to confirm that,” says Tsubota.

“That's when we realized we could actually do good science and real data analysis and have conversations with our collaborators about why these things appear.”

The authors also aimed to determine the cause of these areas of dense fog.

They theorized that the dark ellipse was likely being stirred up from above by a vortex created when the planet's magnetic field lines rub at two very far apart locations. One is the friction in the ionosphere and the Earth's sheet, the rotational motion of which has previously been detected using ground-based telescopes. Hot ionized plasma around the planet emitted by the volcanic moon Io.

The vortex rotates fastest within the ionosphere and gradually weakens as it reaches deeper layers.

Like a tornado landing on dusty ground, the deepest parts of the vortex stir up the hazy atmosphere, creating the dense patches observed by astronomers.

It is unclear whether the mixing will dredge more haze from below or create additional haze.

Based on their observations, researchers believe that the oval shape may form over about a month and disappear within a few weeks.

Astronomer Dr Shih Zhang said: “The dark elliptical haze is 50 times thicker than typical concentrations. This is because this haze is due to the dynamics of the vortex, rather than a chemical reaction caused by high-energy particles from the upper atmosphere. This suggests that it is likely to have been formed by At the University of California, Santa Cruz.

“Our observations show that the timing and location of these high-energy particles do not correlate with the appearance of the dark ellipses.”

This discovery, which the OPAL project was designed to discover, will reveal how the atmospheric dynamics of the solar system's giant planets differ from what we know on Earth. .

“Studying the connections between different atmospheric layers is extremely important for all planets, whether exoplanets, Jupiter, or Earth,” said Dr. Michael Wong, an astronomer at the University of California, Berkeley.

“We see evidence of processes connecting everything throughout the Jovian system, from internal dynamos to satellites, plasma torii, ionospheres, and stratospheric haze.”

“Finding these examples helps us understand the entire planet.”

of study Published in a magazine natural astronomy.

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TK Tsubota others. Jupiter's ultraviolet to dark polar ellipse shows the connection between the magnetosphere and atmosphere. Nat Astronpublished online on November 26, 2024. doi: 10.1038/s41550-024-02419-0

This article is adapted from the original release by the University of California, Berkeley.

Source: www.sci.news

NASA astronaut Suni Williams reveals her Thanksgiving plans from space

Astronauts aboard the International Space Station are ready to break Thanksgiving bread in orbit.

NASA astronaut Suni Williams said she and her fellow crew members will be taking the day off to celebrate.

“I’m packing a lot of Thanksgiving-y food,” Williams said Wednesday in an interview with NBC News. “Smoked turkey, cranberries, apple cobbler, green beans and mushrooms, and mashed potatoes.”

She added that she plans to attend the Macy’s Thanksgiving Day Parade before dining with American and Russian colleagues.

Williams has been living and working on the International Space Station for almost six months. She and fellow NASA astronaut Butch Wilmore arrived at the orbiting outpost in early June as test pilots for the first manned flight of Boeing’s Starliner space capsule.

The two were scheduled to stay on the ISS for only about a week, then return to Earth on the Starliner. However, problems with the spacecraft kept them in orbit for months longer than expected. Wilmore and Williams are scheduled to return home in February in a SpaceX Crew Dragon capsule.

Starliner’s difficult mission was a dramatic, months-long story for NASA and Boeing. But Williams said she doesn’t feel like she’s “stranded” in space.

“Our control team and management always had the option of us returning home,” she said. “Yes, we came here on the Starliner. We’re coming back on the Dragon, but there was always a plan for how we were going to get home.”

In the last few weeks, NASA dodged the rumors Williams reportedly suffered from health problems while in space. Although some news articles suggested that the astronauts had lost significant weight, the agency’s medical director said on Nov. 14 that the health of Williams and others on board the space station was He said the condition was good.

Williams told NBC News that he is enjoying his time in orbit and is in good spirits.

“We feel good, we exercise and we eat properly,” she said. “We’re having a lot of fun here, too. So people are worried about us. Really, don’t worry about us.”

June 5, Suni Williams and Butch Wilmore of Cape Canaveral, Florida.
Chris O’Meara / AP File

Despite problems that occurred during Starliner’s voyage (mainly thruster and helium leaks), the capsule returned to Earth without a crew on September 7th. Williams said he wished he had been able to see Starliner’s mission to completion.

She added that Boeing and NASA would not hesitate to send Starliner into space again if they ironed out the problems that arose during the test flight.

“It might not be tomorrow because we need to incorporate some of the lessons we learned,” she said. “But once we knew we were on the right path, we fixed some of the issues we had — absolutely.”

Source: www.nbcnews.com

Parts of the US may be able to see the Northern lights this Thanksgiving

Thanksgiving might bring cool and rainy weather to many parts of the country, but a solar storm could offer some Americans a chance to witness the beauty of the Northern Lights.

Thanks to a filament eruption on Monday, a mild to moderate geomagnetic storm is expected on Thursday and Friday, as the sun releases a cloud of high-energy plasma towards Earth, as reported by the National Oceanic and Atmospheric Administration (NOAA).

This eruption has the potential to illuminate the night sky in the U.S. with shades of green, red, and purple over the Thanksgiving holiday.

The brightness of the aurora and how long it will be visible depends on the strength of the solar storm and whether it reaches G1 or G2 conditions, according to NOAA meteorologist Mike Betwi.

Residents in states like Washington, Montana, Dakota, Minnesota, Wisconsin, Michigan, and Maine are in prime locations to witness the Northern Lights this weekend, with those in northern parts of Idaho, Wyoming, New York, Vermont, and New Hampshire also having a chance, based on NOAA’s predictions.

NOAA experts anticipate that the Northern Lights will likely be visible from Thursday evening until early Friday morning, but it’s uncertain when and where the sky will light up during the geomagnetic storm. You can monitor the latest activity and forecasts using NOAA’s Aurora Dashboard and experimental tools.

Optimal viewing conditions will be in areas with clear skies, although cloudy weather in the Northeast, much of New England, and near the Great Lakes could obstruct the view.

Unlike a previous strong solar storm earlier this year, experts do not anticipate major disruptions to communication systems in the U.S. unless the storm intensifies unexpectedly, according to Betwi.

The aurora borealis is typically visible at high altitudes, but a significant solar storm can cause it to be visible in areas much farther south than usual.

These solar storms occur when coronal mass ejections from the Sun send large plasma clouds into space, which when directed towards Earth, interact with the planet’s magnetic field and upper atmosphere, resulting in the glowing auroras.

NOAA is gearing up for the expected peak in solar activity next July, which is why the aurora has been visible further south multiple times this year.

Source: www.nbcnews.com

The detrimental effects of banning frightening concepts may outweigh the sense of security it provides

Yuichiro Chino/Getty Images

In 1818, Mary Shelley invented a technology that has been used for both good and bad in the centuries since. It's called science fiction.

Although you might not think that literary genres count as technology, science fiction has long been a tool for predicting and critiquing science. Shelley’s Frankenstein Considered by many to be the first serious science fiction novel, it was so powerful that South Africa banned it in 1955. This story set the formula with a story that still serves today as a warning against unintended consequences.

As far as we know, the exact science that the eponymous Victor Frankenstein used to create is impossible. But today researchers can restore dead human brains to something resembling life. Experiments are underway to restart cell activity (but importantly not consciousness) after death to test its effectiveness in treating conditions such as Alzheimer's disease (see “Fundamental treatments that bring people back from the brink of death”).

It reminds me of many science fiction stories that feature similar scenarios and I can’t help but imagine what will happen next. The same is true for the study reported in “1000 people’s AI simulation accurately reproduces their behavior.” In this study, researchers used the technology behind ChatGPT to recreate the thoughts and actions of specific individuals with surprising success.

The team behind this work blurs the lines between fact, fiction, and what it means to be human.

In both cases, the teams behind this research are blurring the lines between fact, fiction, and what it means to be human, and their research is being conducted under strong ethical oversight. We are deeply aware that there are ethical concerns in the details. It was announced early on. But now that the technology is proven, there is nothing to stop more violent groups from attempting the same thing without oversight, potentially causing significant damage.

Does that mean the research should be banned for fear of it falling into the wrong hands, as Shelley’s book was? Far from it. Concerns about technology are best addressed through appropriate evidence-based regulation and swift punishment of violators. When regulators go too far, they miss out on not only the technology but also the opportunity to criticize and debate it.

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Source: www.newscientist.com

Deep sea affected by ocean acidification

Deep sea coral reefs are at risk of acidification

Howard Chu/Alamy Stock Photo

Ocean acidification is penetrating to depths of 1,500 meters, posing new threats to creatures such as sea butterflies, sea snails and cold-water corals.

The ocean is the largest natural sink of carbon dioxide, absorbing about a quarter of our annual emissions. The uptake of CO2 makes the ocean surface more acidic, which affects sensitive ecosystems such as coral reefs. But until now, researchers didn’t know how far acidification was reaching the deep ocean.

jens daniel müller Researchers at the Federal Institute of Technology Zurich in Switzerland have developed a 3D reconstruction of how CO2 moves through the ocean, based on global measurements of ocean currents and other circulation patterns. They used this model to estimate how the carbon dioxide absorbed by the ocean has affected deep-sea acidity since 1800, around the beginning of the industrial revolution.

They found clear acidification signals down to 1,000 meters deep in most of the ocean. In some regions, such as the North Atlantic, where the powerful Atlantic Meridional Overturning Current (AMOC) transports carbon from the surface to the deep ocean, acidification was observed down to 1500 meters. Some pockets of deep water, which are more acidic in nature, showed even more acidification than the surface. Their high natural acidity reduces their ability to absorb added CO2, Mueller says.

This is more or less what researchers expected would happen as the oceans absorbed more carbon dioxide. Wang Hongjie at the University of Rhode Island. “But it’s another thing to actually see the data coming in that affirms this.”

Remarkably, about half of all acidification since 1800 has occurred since 1994, as CO2 emissions have increased exponentially. “We’re seeing this progress be quite rapid,” Muller says.

The scale of acidification is sufficient to threaten the survival of a wide range of life in the oceans. Chiropods such as sea snails and sea butterflies are particularly at risk because their shells are made of calcium, which dissolves when water becomes too acidic. Increasing acidification has doubled the number of areas where it is difficult for cold-water corals to survive.

And ocean acidification will continue as seawater absorbs more carbon dioxide. “Even if we were able to stop carbon dioxide emissions immediately, we would still see ocean acidification processes inland for hundreds of years,” Muller said.

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Source: www.newscientist.com

Ancient Mars: Evidence of Hydrothermal Activity Uncovered by Meteorite

Scientists from Curtin University and the University of Adelaide analyzed 4.45 billion-year-old zircon particles from a famous Martian meteorite called North West Africa 7034 (NWA 7034) to determine the geochemistry of the water-rich fluid. They found a “fingerprint.”

Northwest Africa 7034. Image credit: NASA.

NWA 7034 weighs approximately 320 grams and is a regolith breccia from Mars.

This meteorite, better known as Black Beauty, was discovered in Morocco's Sahara desert in 2011.

NWA 7034 contains the oldest Martian igneous material ever discovered (approximately 4.45 billion years old).

Dr Aaron Cavosy from Curtin University said: “This discovery opens new avenues for understanding not only the past habitability of Mars, but also the ancient Martian hydrothermal systems associated with magmatic activity.” Ta.

“We used nanoscale geochemistry to detect elemental evidence of Martian hydrothermal waters 4.45 billion years ago.”

“Hydrothermal systems are essential for the development of life on Earth, and our findings show that Mars also had water, a key component of a habitable environment, during its early history of crustal formation.” It suggests that.

“Through nanoscale imaging and spectroscopy, the research team identified the elemental pattern of this unique zircon, including iron, aluminum, yttrium, and sodium.”

“These elements were added when zircon formed 4.45 billion years ago, suggesting that water was present during early magmatic activity on Mars.”

The authors show that water was present in the early pre-Noachian period before about 4.1 billion years ago, even though the Martian crust withstood massive meteorite impacts that caused large-scale surface deformation. showed.

“A 2022 Curtin study on the same zircon particle found that it had been 'shocked' by a meteorite impact, making it the first and only known shocked zircon from Mars. “It turns out,” Dr. Kavosie said.

“This new study identifies telltale signatures of water-rich fluids when the particles formed and provides geochemical markers of water in the oldest known Martian crust. This brings us one step closer to understanding early Mars.”

of findings appear in the diary scientific progress.

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Jack Gillespie others. 2024. Zircon trace element evidence of early hydrothermal activity on Mars. scientific progress 10(47);doi: 10.1126/sciadv.adq3694

Source: www.sci.news

Equipment deployed by NASA’s European Clipper spacecraft

NASA’s European Clipper, the largest spacecraft the agency has ever developed for a planetary mission, is already 20 million kilometers (13 million miles) from Earth.

An artist’s concept for NASA’s Europa Clipper shows the spacecraft silhouetted on the surface of Jupiter’s icy moon Europa, with the magnetometer boom fully deployed on top and the antenna for the radar instrument pointing out from the solar array. It’s growing. Image credit: NASA/JPL-Caltech.

Europa Clipper launched from NASA’s Kennedy Space Center in Florida on October 14, 2024.

The spacecraft is hurtling toward the Sun at 35 kilometers per second (22 miles per second).

Europa Clipper will travel 2.9 billion kilometers (1.8 billion miles) to reach Jupiter in 2030 and begin a series of 49 flybys in 2031, collecting data using an array of instruments. , will tell scientists whether the icy moon and its interior ocean influenced the icy moons. Conditions necessary for life to exist.

For now, the information mission teams are receiving from the spacecraft is strictly engineering data, telling them how the hardware is working.

Immediately after launch, Europa Clipper deployed a giant solar array extending the length of a basketball court.

Next on the list was the magnetometer boom, which unwound from a canister attached to the spacecraft body and stretched 8.5 meters (28 feet) in length.

To ensure that all boom deployments went well, the team used data from three magnetometer sensors.

Once the spacecraft reaches Jupiter, these sensors will measure Europa’s surrounding magnetic field, confirming the existence of an ocean believed to lie beneath the moon’s icy crust, and telling scientists about its depth and salinity. I’ll let you know.

After the magnetometer, the spacecraft deployed several antennas for radar instruments.

Four high-frequency antennas extend laterally from the solar array, forming what appear to be two long poles, each 17.6 m (57.7 ft) long.

Eight rectangular very high frequency antennas, each 2.76 m (9 ft) long, were also deployed, two on each of the two solar arrays.

“This is an exciting time for the spacecraft to complete these important deployments,” said Jordan Evans, a researcher at NASA’s Jet Propulsion Laboratory and project manager for Europa Clipper.

“Most of what the team is focused on right now is understanding the small, interesting things in the data that help us understand the behavior of the spacecraft on a deeper level. It’s really good to see that. That’s it.”

The remaining seven devices will be powered on and off throughout December and January so engineers can check their health.

Some instruments, including visible imagers and gas and dust mass spectrometers, will remain under protective covers for the next three years or so to prevent potential damage from the Sun while Europa Clipper was in the inner solar system. I plan to make it.

Once all equipment and engineering subsystems are checked out, the mission team will shift its focus to Mars.

On March 1, 2025, Europa Clipper will reach Mars’ orbit and begin orbiting Mars, using Mars’ gravity to gain speed.

The mission navigator has already completed one course correction maneuver to keep the spacecraft on the correct course as planned.

On Mars, as a test run, the rover’s thermal imager will be turned on to take multicolor images of Mars.

They also plan to collect data on the radar equipment so engineers can verify that it is working as expected.

The spacecraft is scheduled to perform another gravity assist in December 2026 and swoop down to Earth before making the remainder of its long journey to the Jupiter system.

At that time, the magnetometer measures the Earth’s magnetic field and calibrates the instrument.

Source: www.sci.news

The Rise of Dinosaurs Told through Fossilized Feces

A plant-eating sauropod dinosaur that evolved in a humid environment during the early Jurassic period.

Marcin Ambrozik

The contents of feces and vomit from 200 million years ago are helping to show how dinosaurs conquered the world at the beginning of the Jurassic period.

Whole insects embedded in various shapes and sizes of well-preserved plants, bones, fish parts, and even ancient animal feces show that dinosaurs varied in comparison to other groups of animals. This suggests that dinosaurs were able to survive in the ecosystem thanks to their wide-ranging diet. This led to their further growth and eventually led to the establishment of a “land dynasty.” Martin Kvarnström At Uppsala University, Sweden.

Fossil evidence shows that the first dinosaurs had prominent hip joints that placed their legs underneath their bodies like mammals, rather than sprawling sideways like lizards. More than 230 million years ago During the Triassic. For tens of millions of years, these early dinosaurs blended into a landscape filled with many other types of reptiles. But by about 200 million years ago, dinosaurs had essentially taken over the Earth, around the time most other reptiles disappeared during the end-Triassic extinction.

What led to this dominance remains somewhat of a mystery. Kvarnström and his colleagues suspected that important clues might be hidden in the bromalites (fossilized feces and vomit) of dinosaurs and other animals. So they Polish Geological Institute collected by a prior research group from eight locations in Poland between 1996 and 2017.

The research team estimated the age of each bromalite based on the layer of sediment in which it was found, and determined its size, which ranges from a few millimeters to a “fairly large fecal mass,” and the animals that may have produced it. A suitable shape was used. The researchers then 3D scanned the fossil to examine its contents. “We noticed that it was clogged with food debris,” Kvarnström says.

Coprolites, or fossilized feces, of herbivorous dinosaurs containing plant remains

Grzegorz Niedzwicki

Combining the known fossil record and past climate information, researchers determined that the emergence of dinosaurs occurred in several different stages. First, the omnivorous ancestors of early dinosaurs began to outnumber non-dinosaurs. They then evolved into the first carnivorous and plant-eating dinosaurs.

At that point, increased volcanic eruptions and movement of tectonic plates caused flooding and waterway development. The resulting humidity and related changes in climate likely led to a wider range of plants and the evolution of larger and more diverse herbivorous dinosaurs. On the other hand, animals other than dinosaurs (such as dicynodonts, which eat plants weighing up to 1 ton) Lisowisia, Their feces contained mainly coniferous debris and they were less able to adapt to changes in vegetation.

As herbivorous dinosaurs grew larger, so did their predators. By the beginning of the Jurassic period, about 30 million years after the first dinosaurs appeared, the transition to a dinosaur-dominated world was complete, Kvarnström says.

“This study shows how climate primarily affected dominant plants, which created opportunities for new herbivores at certain points in time,” he says. michael benton from the University of Bristol, UK, was not involved in the study.

Although it's difficult to be sure that the researchers matched the scat to the right animal, the discovery nonetheless suggests that the dinosaur species had already expanded significantly in South America before major climate change. This confirms earlier research, he says. “But it took the end-Triassic mass extinction for the final stage of the takeover to begin.”

for emma dunn The study, conducted at Germany's Friedrich-Alexander University, helps answer long-standing questions about the emergence of dinosaurs. “It's not every day that a fossil poop is published in such an influential journal,” said Dunn, who was not involved in the study. “This is obviously interesting, but it's also very useful for understanding prehistoric environments. So if you think of the evolution of early dinosaurs like a jigsaw puzzle with pieces missing, there are new It’s just a lot of pieces thrown in.”

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Source: www.newscientist.com

Diamond storage breaks records by holding data for millions of years

Diamond can store data stably for a long time

University of Science and Technology of China

The famous marketing slogan that diamonds are forever may be just a slight exaggeration for diamond-based systems that can store information for millions of years. Now, researchers have developed a system with a record-breaking storage density of 1.85 terabytes per cubic centimeter.

Previous technology used laser pulses to encode data onto diamond, but due to its higher storage density, a diamond optical disc with the same capacity as a standard Blu-ray could hold approximately 100 terabytes of data (Blu-ray). (equivalent to approximately 2,000 rays). It lasts much longer than the typical Blu-ray lifespan of just a few decades.

“Once the internal data storage structure is stabilized using our technology, diamond can achieve an extraordinary lifetime of millions of years of data retention at room temperature without requiring maintenance,” he says. Wang Ya at the University of Science and Technology of China in Hefei.

Wang and his colleagues conducted their research using tiny pieces of diamond, just a few millimeters long, but say future versions of the system could use rapidly spinning diamond discs. Their method used ultrafast laser pulses to knock some of diamond’s carbon atoms out of place, leaving single-atom-sized empty spaces, each exhibiting a stable brightness level.

By controlling the laser’s energy, the researchers were able to create multiple empty spaces at specific locations within the diamond, and the density of those spaces influenced the overall brightness of each site. . “The number of free spaces can be determined by looking at the brightness, so the stored information can be read,” Wang says.

The team then saved the images, including a colorful painting by artist Henri Matisse. cat with red fish And a series of photographs taken by Eadweard Muybridge in 1878, showing a rider on a galloping horse, maps the brightness of each pixel to the brightness level of a specific region within a diamond. The system stored this data with over 99% accuracy and completeness.

This preservation method is not yet commercially viable because it requires expensive lasers, high-speed fluorescence imaging cameras, and other devices, Wang said. But he and his colleagues hope that the diamond-based system can eventually be miniaturized to fit in a space the size of a microwave oven.

“In the short term, government agencies, research institutes, and libraries with a focus on archives and data preservation may be eager to adopt this technology,” he says.

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Source: www.newscientist.com

NASA to investigate subterranean ocean of Uranus’ moon

Some of the icy moons in the Jupiter and Saturn systems appear to have oceans of liquid water inside them. Although our knowledge of Uranus' moons is more limited, future tours of the Uranian system may be able to detect subsurface oceans. To plan for this, we need to understand how the internal structure of satellites, with and without oceans, relates to observable quantities. New research from the University of Texas Geophysical Institute and the University of California, Santa Cruz shows it may be possible to diagnose the presence or absence of liquid water oceans inside some of Uranus' moons, including Miranda and Ariel. There is, Umbriel, and it is thought that this, combined with measurements of the gravitational field, may provide comprehensive constraints on the internal structure and history of Uranus' moons.

Uranus' four major moons, Ariel, Umbriel, Titania, and Oberon, may have oceanic layers. Salty seas, or salty seas, are found beneath the ice and above water-rich and dry rock layers. Miranda is too small to retain enough heat in the ocean layer. Image credit: NASA/JPL-Caltech.

When NASA's Voyager 2 flew by Uranus in 1986, it took grainy photos of the large icy moon.

Now, NASA plans to send another spacecraft to Uranus, this time equipped to see if those icy moons hide oceans of liquid water.

The mission is still in the early planning stages, but planetary researchers are preparing by building a new computer model that can be used to detect oceans beneath the ice using only the rover's cameras.

Their computer model works by analyzing the moon's tiny vibrations, or wobbles, as it orbits its parent planet.

From there, you can calculate how much water, ice, and rock is inside. A small wobble means the moon is mostly solid, while a large wobble means its icy surface is floating in an ocean of liquid water.

When combined with gravity data, the model calculates the depth of the ocean and the thickness of the overlying ice.

Dr. Doug Hemingway, a planetary scientist at the University of Texas Geophysical Institute, said: “If we find that Uranus' moons have an inland ocean, it means there are a huge number of potentially habitable worlds across the galaxy. It may mean,” he said.

“The discovery of oceans of liquid water on Uranus' moons will change our thinking about the range of possibilities for life.”

All large moons of the solar system, including the moons of Uranus, are tidally locked.

This means that the same side always faces the parent planet while orbiting, as the gravity matches their rotation.

However, this does not mean that the satellite's rotation is completely fixed; all tidally locked satellites will oscillate back and forth during their orbit.

Determining the extent of the wobble is key to learning whether Uranus' moons have oceans, and if so, how large.

A satellite with an ocean of liquid water splashing inside will wobble more than one that is entirely solid. However, even the largest oceans experience only small wobbles. The moon's rotation can shift by just a few hundred feet as it passes through its orbit.

This is still enough for a passing spacecraft to detect it. In fact, this technique was previously used to confirm that Saturn's moon Enceladus has an internal ocean.

To find out whether the same technique would work on Uranus, Dr. Hemingway and his colleague Dr. Francis Nimmo of the University of California, Santa Cruz performed theoretical calculations on Uranus's five moons, using a variety of the most I came up with a plausible scenario.

Detecting smaller oceans means the spacecraft will need to get closer or carry more powerful cameras.

“The next step is to extend the model to include measurements from other instruments and see how this improves the interior of the satellite,” Dr. Hemingway said.

of the team work Published in a magazine Geophysical Research Letters.

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DJ Hemingway and F. Nemo. 2024. Search for the underground ocean inside Uranus's moon using balance and gravity. Geophysical Research Letters 51 (18): e2024GL110409;doi: 10.1029/2024GL110409

This article is a version of a press release provided by the University of Texas.

Source: www.sci.news

Archaeologists Uncover Possible 2,100-Year-Old Temple in Egypt

Archaeologists have uncovered an entrance to a large stone temple in an ancient Egyptian town, Athribis, near the modern city of Sohag.



The south tower of the Athribis pylon and the hill behind it. It is believed that there is a sanctuary here. Image credit. Marcus Müller, Athribis Project.

“The entrance to the temple in the rock appears to lie beneath a still-untouched pile of rubble behind it,” said archaeologists Professor Christian Reitz and Dr Markus Müller from the University of Tübingen.

“Since 2022, we have been working with Mohamed Abdelbadia of the Egyptian Antiquities Authority and the Egyptian team at Asribis to excavate the large stone temple.”

“Excavations have been underway since 2012 to reveal an ancient temple district built between 144 BC and 138 AD.”

“The width of the complex was a total of 51 meters, and the monumental temple entrance towers were each 18 meters high.”

“Today there is only about five meters left. The rest was sacrificed to quarrying,” they added.

“Thanks to the fallen coins, the removal of this stone may have taken place in 752 or shortly thereafter.”

Archaeologists also discovered a relief of a king offering a sacrifice to the lion-headed goddess Lepit and her son Kolantes.

A newly discovered hieroglyphic inscription reveals for the first time which king was responsible for the decoration of the pylon, and perhaps also for its construction: Ptolemy VIII in the 2nd century BC.

“We unexpectedly encountered a previously unknown chamber in the northern tower,” the researchers said.

“We used air cushions, wooden scaffolding and rollers to remove ceiling blocks weighing approximately 20 tonnes.”

“We found a chamber about 6 meters long and 3 meters wide.”

“It was a storage room for temple utensils and was later used to store amphora.”

“A corridor led to the room through a pylon, allowing access from outside.''

“This entrance is also decorated with reliefs and hieroglyphs,” they added.

“Once again we see the goddess Lepit, but on the opposite door frame the fertility god Min is depicted, along with two very rarely depicted beings, the falcon-headed decan (who can measure the hours of the night) It is accompanied by a star.

“Unique in Egyptian temple architecture is the second door in the façade of the pylon, which opens onto a previously unknown staircase that led to the upper floors on at least four floors. It has now been destroyed and further storage rooms may be rebuilt there.”

“Finely smoothed limestone blocks in vertically cut rock facades may belong to rock sanctuaries,” says Professor Wrights.

“The finds over 3 meters high and the typical decorations at the top of the temple, such as the cobra frieze, indicate that there may have been a door behind the temple.”

Source: www.sci.news

Astronomers reveal new main-belt comet mistaken for active asteroid

456P/Panstars, an active main-belt asteroid first discovered in 2021, is repeatedly active, and its activity is linked to volatile ice formations, according to new observations from the Magellan-Baade and Lowell Discovery telescopes. It is likely that this is caused by sublimation.



456P/PanSTARS image taken on October 3, 2024 with the Magellan Baade Telescope in Chile and with the Lowell Discovery Telescope in Arizona on October 26, 2024. At the center of each image is the comet’s head or nucleus, the tail extends to the right. Image credits: Scott S. Sheppard / Carnegie Institution for Science / Audrey Thirouin, Lowell Observatory / Henry H. Hsieh, Planetary Science Institute.

“Main-belt comets are icy objects found in the asteroid belt between Mars and Jupiter, rather than outside the cold solar system, where icy objects would normally be expected,” said Henry Hsieh, senior scientist at the Planetary Science Institute.

“They have comet-like features, such as tails that extend away from the sun and fuzzy clouds as the sun’s heat evaporates the ice.”

These objects were first discovered in 2006 at the University of Hawaii by Dr. Hsieh and his then-doctoral supervisor, Professor David Jewitt.

“Main-belt comets belong to a larger group of Solar System objects known as active asteroids, which look like comets but have asteroid-like orbits in the warm inner Solar System,” the astronomers said.

“This large group includes not only objects that emit dust from evaporated ice, but also objects that have clouds or tails of ejected dust from collisions or rapid rotation.”

“Both main-belt comets and active asteroids in general are still relatively rare, but scientists are discovering them.”

456P/PANSTARRS was discovered as P/2021 L4 (PANSTARRS) through observations by Pan-STARRS1 on June 9 and 14, 2021, and observations by Canada, France, and Hawaii telescopes on June 14, 2021.

Dr. Hsieh and his co-authors observed the object twice in October 2024 using the Magellan-Baade Telescope and the Lowell Discovery Telescope, establishing its status as a main-belt comet.

“This object is not just an asteroid that experienced a one-off event, but is essentially an active icy object, like other comets in the outer solar system,” Hsieh said.

If 456P/PANSTARRS’s activity is due to something other than ice evaporation, its tail would be expected to appear only once, randomly, and not repeatedly as it approaches the Sun.

On the other hand, icy objects heat up every time they approach the sun, and the evaporated ice is carried away with the dust.

As the object moves away from the sun and cools, it ceases to be active.

Observations of repeated dust ejection activity during their approach to the Sun are currently considered the best and most reliable method of identifying main-belt comets.

“Confirmed main-belt comets are still largely unknown,” Dr. Xie said.

“We want to grow the population so we can understand more clearly what its broader characteristics are, such as its size, active period, and distribution within the asteroid belt. We will be able to better utilize them to track ice within the asteroid belt and across the solar system.”

of findings Published in American Astronomical Society Research Notes.

_____

Henry H. Shea others. 2024. Recurrence activity of main belt comet 456P/Panstars (P/2021 L4) confirmed. Resolution memo AAS 8,283;doi: 10.3847/2515-5172/ad90a6

This article is a reprint of a press release provided by the Planetary Science Institute.

Source: www.sci.news

The impact of artificially stopping your period on your body

People with a uterus experience menstruation about once every 28 days for approximately 40 years of their lives.

Menstruation goes beyond just blood. It’s common for 84% of women to experience menstrual pain regularly. Severe menstrual pain can lead women to miss numerous days of education or work each month. Additionally, periods are costly, with an estimated lifetime cost of around 4,800 pounds (approximately $6,100).

Given these challenges, it’s only natural to want to stop menstruation. While periods may naturally cease during pregnancy, breastfeeding, or menopause, many women in the UK opt to stop their menstrual cycles using hormonal contraception.

Contraceptive pills, implants, and hormonal coils work by releasing hormones that prevent ovulation. Without an egg being released or the lining of the uterus thickening for pregnancy, menstruation, which occurs due to shedding of this lining, typically stops when it ceases to grow.

“There’s nothing harmful about not having a menstrual cycle,” affirms Dr. Nicola Tempest, a researcher and gynecologist at Liverpool Women’s Hospital. “Taking hormones doesn’t detract from your body’s wellbeing.”

But are there any drawbacks to not having periods?

For individuals with regular menstrual cycles (not taking hormonal contraceptives), the sudden absence of periods may signify underlying health issues.

While the occasional missed period isn’t typically worrisome, a prolonged absence of periods after having regular cycles could indicate potential problems such as early menopause or polycystic ovarian syndrome.

Tempest notes that individuals with such conditions may require hormone medication as part of their treatment, which could help in diagnosing these conditions along with other associated symptoms, even if periods have ceased due to birth control pills.

There may be certain side effects associated with hormonal contraceptives, such as a slight increase in the risk of breast, liver, and cervical cancer with long-term use. However, Tempest emphasizes that prolonged use of birth control also reduces the risk of endometrial and ovarian cancer.

In her view, menstruation is not an indispensable aspect of a person’s health. “If you wish to forego menstruation, you have that choice,” she states.

This article addresses the question “Can I stop my period?” posed by Veronica Nielson via email.

If you have any queries, please reach out to us via email: questions@sciencefocus.comor connect with us on Facebook, ×or Instagram (please include your name and location).

Explore more interesting fun facts Discover more fascinating science insights.

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Meet our experts:

Dr. Nicola Tempest I am a clinical researcher and gynecologist at Liverpool Women’s Hospital. Her research includes chronic pelvic pain, exercise and reproduction, and endometriosis.

Source: www.sciencefocus.com

Hubble Space Telescope Spots Spiral of Condensation in NGC 2090

Astronomers using the NASA/ESA Hubble Space Telescope have taken surprising new photos of spiral galaxy NGC 2090.

This Hubble image shows NGC 2090, a spiral galaxy located south of the constellation Columba, about 40 million light-years away. Color images were created from separate exposures taken in the ultraviolet, visible, and near-infrared regions of the spectrum using Hubble's Wide Field Camera 3 (WFC3). This is based on data obtained through six filters. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / D. Tilker.

NGC2090 It is a spiral galaxy located south of the constellation Columba.

Also known as ESO 363-23, IRAS 05452-3416, LEDA 17819. discovered It was announced by Scottish astronomer James Dunlop on October 29, 1826.

“NGC 2090 is notable as part of a group of galaxies being studied. Hubble's Extragalactic Distance Scale Key Project“This study aimed to determine a new, state-of-the-art value for the Hubble constant, one of the main scientific goals of the then-new telescope,” Hubble astronomers said in a statement.

“NGC 2090's contribution was to calibrate the Tully-Fisher (TF) distance method by observing Cepheid variable stars in the galaxy.”

“Cepheid-based measurements from a 1998 study estimated the distance of NGC 2090 to be 37 million light-years.”

“Latest measurements in 2020 using the TF method place NGC 2090 slightly further away, at 40 million light-years.”

Before and after that project, NGC 2090 has been well studied as a very prominent nearby example of star formation.

It has been described as a cotton-like spiral, meaning a spiral galaxy with a speckled, dusty disk and flaky or no visible arms.

“This Hubble image gives a good indication of why NGC 2090 received such a description, with its spiral arms looking like lanes of light winding through the dust,” the astronomers said. said.

“NGC 2090 remains an active galaxy, with clusters of star formation in various stages of evolution spread throughout the disk.”

“Investigating star formation and the movement of matter within galaxies was the motivation for these Hubble observations taken in October of this year.”

“Likewise, Hubble's partner in space astronomy, NASA/ESA/CSA's James Webb Space Telescope, also scouted this galaxy to add infrared data to the picture of galaxy evolution.”

Source: www.sci.news

Nanopasta: The World’s Thinnest Spaghetti Emerges

The world's thinnest spaghetti is only 372 nm wide, which is about 1/200th the width of a human hair.

Britton others. Using a scanning electron microscope, they scanned the mat with a focused beam of electrons and created images based on the patterns of electrons that were deflected, or bounced away. The individual strands are too thin to be clearly captured by any form of visible light camera or microscope. Image credit: Beatrice Britton/Adam Clancy.

Beatrice Britton, a researcher at University College London, and her colleagues said: “This novel nanopasta is not intended as a new food product, but rather that strands of ultra-thin material called nanofibers have a wide range of uses in medicine and industry. It was made with usage in mind.”

“Nanofibers made from starch are particularly promising and could be used in dressings to aid wound healing and as scaffolds for bone regeneration and drug delivery.”

“But they rely on starches that are extracted and purified from plant cells, a process that requires a lot of energy and water.”

“A more environmentally friendly method is to create nanofibers directly from starch-rich raw materials, such as the flour that pasta is made from.”

To create the spaghetti, which is just 372 nm in diameter, the authors used a technique called electrospinning. In this technique, a thread of flour and liquid is pulled through the tip of a needle by an electric charge.

“To make spaghetti, you push a mixture of water and flour through metal holes,” says Adam Clancy, a researcher at University College London.

“In our study, we did the same thing, except we charged the flour mixture and forced it through. It's literally spaghetti, but much smaller.”

The new nanopasta forms a mat of nanofibers about 2 cm in diameter that is visible to the eye, but the individual strands are too thin to be clearly captured by any form of visible light camera or microscope. Therefore, its width was measured using a scanning electron microscope.

Professor Gareth Williams, from University College London, said: “Nanofibers, such as those made from starch, are highly porous and therefore show potential for use in wound dressings.”

“Additionally, nanofibers are also being investigated for use as scaffolds for tissue regrowth because they mimic the extracellular matrix (the network of proteins and other molecules that cells build to support themselves). .”

“Starch is a promising material to use because it is abundant and renewable. Starch is the second largest source of biomass on Earth after cellulose, and it is biodegradable, so it can be broken down in the body,” Clancy said. the doctor said.

“However, refining starch requires a lot of processing. We have shown that a simple method of making nanofibers using wheat flour is possible.”

“The next step is to investigate the properties of this product.”

“We want to know, for example, how quickly it breaks down, how it interacts with cells, and whether we can produce it at scale.”

In electrospinning, the needle containing the mixture and the metal plate on which the mixture is deposited form the two ends of the battery.

When a charge is applied, the mixture flows out of the needle and onto the metal plate, completing the circuit.

Electrospinning with starch-rich raw materials, such as refined flour, is more difficult than with pure starch because impurities (proteins and cellulose) increase the viscosity of the mixture, making it impossible to form fibers.

The researchers used flour and formic acid instead of water. This is because formic acid breaks down the giant helical stacks that make up starch.

This is because the layers of helices stuck together are too large to be the building blocks of nanofibers.

When the noodles fly through the air and reach the metal plate, the formic acid evaporates.

The scientists also had to carefully warm the mixture for several hours and then slowly cool it to the right consistency.

“As the newly developed material is composed of fibers formed by extruding and drying flour, it could be defined as pasta, breaking the previous record for the thinnest pasta runga by about 1,000 the researchers concluded.

their paper appear in the diary Nanoscale advances.

_____

Beatrice Britton others. Nanopasta: Electrospinning white flour nanofibers. nanoscale advancepublished online October 30, 2024. doi: 10.1039/D4NA00601A

Source: www.sci.news

How can we solve the planet’s plastic pollution crisis?

plastic waste in indonesia

PA Image/Alamy

The world currently generates more than 50 million tonnes of “mismanaged” plastic waste each year, and some researchers predict that this flood of plastic pollution will double by mid-century. But he also said that if countries could agree to adopt four key policies during this period. This number could be reduced by 90 per cent if this week's global plastics deal is negotiated.

Plastic pollution ultimately chokes land and sea ecosystems. “This affects every level of the food chain, from phytoplankton cells to humans,” he says. Sarah-Jeanne Royer at the University of California, San Diego. Plastics also account for about 5% of greenhouse gas emissions.

That's why most of the world's countries are meeting this week in Busan, South Korea, to hammer out the final details of a global treaty to end plastic pollution. By 2022, 175 countries have already agreed to adopt a legally binding treaty For the past two years, we have been debating what exactly we should require, with particular disagreements over setting limits on production of new plastics.

To make the discussion more clear, douglas mcquarley The researchers at the University of California, Santa Barbara, used an artificial intelligence model trained on economic data to test how the policies they were considering would affect global plastic pollution. “I wasn't sure that [eliminating plastic pollution] It was actually possible,” McCauley said. “But it turns out we can get pretty close.”

They predict that under current conditions, plastic pollution is expected to almost double by 2050, reaching between 100 million and 139 million tonnes. However, all four policy combinations are still on the bill. Current draft treatywas sufficient to reduce this by over 90%.

The most influential of these was the mandate that plastic products contain at least 40% recycled material. This rule alone will cut plastic pollution in half by mid-century. Mr McCauley said this effect was significant because it would reduce demand for newly made or “virgin” plastics, while also stimulating demand for recycled materials. “Suddenly, there was a huge global recycling market.”

But recycling alone wasn't enough. “If our goal is to eliminate plastic pollution, we need to address it throughout its lifecycle,” he says. Further reductions would have required limiting virgin plastic production to 2020 levels. According to the model, this production cap would have reduced plastic pollution by about 60 million tons per year by mid-century. This change also had the biggest impact on greenhouse gas emissions from plastic production, as the extraction of fossil fuels and conversion into virgin plastics involves processes with large emissions.

A third policy would spend $50 billion on waste management, roughly equal to the production cap, especially if these funds go to low-income countries with poor infrastructure and where plastic pollution is most severe. reduced pollution. “When we start talking about global finance, [the amount of money needed] It’s not that big,” McCauley said. “Building a sanitary landfill is different from building a port.”

Plastic waste is increasing, and while some is recycled or destroyed, the majority is “mismanaged” and piles up as plastic pollution.

A. Samuel Pottinger et al.

Finally, a small tax on plastic packaging has reduced pollution by tens of millions of tons. The researchers based this estimate on case studies of how people reduced their plastic use in response to similar taxes. 5 cents fee Regarding disposable plastic bags in Washington DC. Funds raised through such taxes could also be used to pay for other changes, such as building waste management infrastructure or improving recycling systems.

Royer, who was not involved in the study, said he thinks all of these policies will help. Reducing the use of single-use plastics, such as shopping bags and plastic forks, through taxes or bans could also make a difference, she says. “If you look at plastic pollution in general, 40% of the plastic produced is single-use.”

However, she points out that local rules alone will never solve the problem. California, for example, banned some single-use plastic bags a decade ago and this year banned all such bags. But most of the plastic pollution that washes up on our shores comes from outside the state, with California's plastic waste typically washing ashore from Asia across the Pacific or being left behind by fishing. “There are no borders,” Royer says.

This is where the World Treaty comes into play. Researchers explore how different policies around the world can reduce three things: the amount of poorly managed plastic waste, the production of new plastics, and plastic-related greenhouse gas emissions. I showed you. By combining the four key policies seen in the graph below, all three measures reduced, specifically mismanaged waste, by 91%.

Researchers estimated the impact of different policies to reduce plastic

Source: www.newscientist.com

Webb Reveals a Fresh Perspective on the Sombrero Galaxy

sharp resolution Web’s mid-infrared device (MIRI) focuses on details of the outer ring of the Sombrero Galaxy, providing insight into how dust is distributed.

This web image shows the Sombrero Galaxy. Image credit: NASA/ESA/CSA/STScI.

The Sombrero Galaxy is located approximately 28 million light-years away in the constellation Virgo.

This spiral galaxy, also known as Messier 104, M104, or NGC 4594, was discovered by French astronomer Pierre Méchain on May 11, 1781.

It is about 49,000 light-years in diameter, about one-third the size of our Milky Way galaxy.

The Sombrero galaxy has a very large central bulge and a supermassive black hole.

We are looking directly at the galaxy, at an angle of 6 degrees south of its face. Its dark dusty path dominates the view.

“The clumpy nature of the dust, in which MIRI detects carbon-containing molecules called polycyclic aromatic hydrocarbons, may indicate the presence of young star-forming regions,” Webb astronomers said in a statement.

“But unlike some of the galaxies studied with Webb, such as Messier 82, which has 10 times as many stars as the Milky Way, the Sombrero galaxy is not a special hotbed of star formation.”

“The Sombrero ring produces less than 1 solar mass per year of stars, compared to about 2 solar masses per year for the Milky Way.”

“The supermassive black hole at the center of the Sombrero galaxy, also known as an active galactic nucleus (AGN), is fairly docile, even at a massive 9 billion solar masses,” the researchers noted.

“Classified as a low-luminosity AGN, it slowly chews up material falling from the galaxy while emitting bright and relatively small jets.”

“Also, there are about 2,000 globular clusters within the Sombrero galaxy, which are collections of hundreds of thousands of old stars held together by gravity,” the researchers said.

“This type of system acts as a pseudo-laboratory for astronomers to study stars. There are thousands of stars in one system of the same age but with different masses and other properties, making it difficult to compare It’s an interesting opportunity for research.”

“In the MIRI images, galaxies of different shapes and colors are scattered across the cosmic background.”

“The different colors of these background galaxies can tell astronomers about their properties, such as their distance.”

Source: www.sci.news

Japanese researchers discover a new species of pterosaur

Paleontologists have announced the discovery of a new species of Quetzalcotorin azhdarchopterosaur. Nippotherus mifunensis from the Late Cretaceous of Japan.

Restoration of life in the giant azhdarchid group, Quetzalcoatlus nothropi foraging in the Cretaceous fern steppe. Image credit: Mark Witton / Darren Naish.

Pterosaurs were highly successful flying reptiles (not dinosaurs, as is commonly misunderstood) that lived between 210 and 65 million years ago.

They were the first flying vertebrates on Earth, with birds and bats appearing much later.

Some pterosaurs, like the giant azhdarchids, were the largest flying animals in history, with wingspans exceeding 9 meters (30 feet) and a standing height comparable to modern giraffes.

“Pterosaurs, the earliest vertebrate group to achieve powered flight, exhibit remarkable morphological diversity, with a fossil record that spans from the Late Triassic to the Cretaceous-Paleogene boundary. '' said Dr. Naoki Ikegami of the Mifune Dinosaur Museum and Dr. Naoki Ikegami of the University of São Paulo. Rodrigo Pegas and his friends.

“The pterosaur skeleton's fragile air bones make its fossil record particularly irregular and uneven.”

“Most well-preserved, relatively complete archaeological sites are confined to a few Lagerstätten around the world. In contrast, most other deposits that yield pterosaurs are typically fragments. generate a typical sample.

“For one thing, there are very few records of pterosaurs in Japan, so every artifact has special significance.”

“The first pterosaur specimen discovered in Japan came from the Ezo Group in Hokkaido, and is representative of an indeterminate pterosaur species consisting of a femur, metatarsals, foot phalanges, and part of the caudal vertebrae. It is.”

6th cervical vertebra Nippoterus mifunensis. Image credit: Zhou others., doi: 10.1016/j.cretres.2024.106046.

The newly identified species is Quetzalcoatrinae a subfamily of the pterosaur family Azhdarchidae.

“Azhdarchids represent a very special clade of pterosaurs, particularly notorious for containing some of the largest flying creatures in history, with wingspans of 10 to 11 meters (33 to 36 feet).” Quetzalcoatlus nothropi, aramburgiania philadelphia and Hatzegopteryx tanbema'' said the paleontologists.

“The azhdarchid clade, most prominently characterized by elongated cervical vertebrae with reduced neural spines, is widely distributed in Turonian to Maastrichtian pterosaur communities around the world.”

“They represent the most diverse and widespread group of pterosaurs during the Late Cretaceous.”

named Nippoterus mifunensis the new species lived in what is now Japan about 90 million years ago (late Cretaceous period).

Nippoterus mifunensis “This is the first nominally Japanese pterosaur species,” the researchers said.

“This new species exhibits many Quetzalcoat line characteristics and bears a striking resemblance to the unnamed Burcant azhdarchid of Mongolia's Turonian-Coniacian.”

Part of the 6th cervical vertebra Nippotherus mifunensis It was produced from an outcrop of the Mifune Group near Amagi Dam in Mifune Town, Kumamoto Prefecture, Kyushu.

“The specimen was found in a 30-centimeter (12-inch) thick layer of coarse lenticular sandstone, nestled between two tuff layers, in the middle of the upper formation of the Mifune Group,” the scientists said. said.

their paper Published in this month's magazine Cretaceous research.

_____

Zhou Xuanyu others. Re-evaluation of azhdarchoid pterosaur specimens from the Mifune Group, Late Cretaceous of Japan. Cretaceous researchpublished online on November 16, 2024. doi: 10.1016/j.cretres.2024.106046

Source: www.sci.news

Disputed COP29 deal highlights deteriorating climate cooperation

When COP29 President Mukhtar Babayev stepped up to the podium on Sunday morning at the closing session of the Baku Climate Summit, he had two speeches ready. According to sources who spoke to Reuters on condition of anonymity, one speech was prepared in anticipation of a much-anticipated deal, while the other was prepared in case of a deadlock after the summit collapsed. It was seen as a contingency plan.

An official from the COP29 Presidency revealed that negotiations were tough until the last minute to secure the Baku breakthrough, but they were still preparing for various outcomes. The final speech was being crafted to address different possibilities.

Ultimately, without giving his detractors a chance to react, Babayev succeeded in pushing through a $300 billion funding plan to assist developing countries in handling the escalating costs of global warming over the next decade, earning praise for his efforts.

He lauded the agreement as a significant achievement and criticized skeptics, labeling them as “wrong,” along with many individuals targeted by the climate deal accused of being grossly inadequate.

The audience was already aware that Babayev was preparing for a mixed outcome at the divisive Baku summit, signaling that negotiations were unlikely to proceed smoothly.

Concerns about the imminent withdrawal of the United States from global climate cooperation, geopolitical tensions, and the surge of isolationist politics that have sidelined climate change in many nations’ priorities had lowered expectations for the deal.

An activist holds up a globe balloon during a protest at the United Nations Climate Change Conference COP29 in Baku, Azerbaijan, on November 21.
Maxim Shemetov/Reuters

Potential obstacles loomed large over Baku. The coming months will continue to cast a shadow over global efforts to address climate change as Brazil gears up to host a major conference next year in the Amazon rainforest city of Belem. The world will then embark on a multi-year plan for deeper emissions cuts and building climate resilience.

Trump Effect

One major factor clouding the negotiations in Baku was the impending return of Donald Trump as the President of the United States, the world’s largest economy, historically the largest emitter of greenhouse gases, and a significant producer of oil and gas, who has been a climate change skeptic.

President Trump, due to take office again in January, had vowed to withdraw the US from the global Paris climate accord, repeating his stance from his previous term and dismissing climate change as a hoax.

Negotiators at the Baku conference noted that while the US delegation contributed to developing a climate finance agreement, the country was unable to play the high-profile leadership role seen in previous climate summits. Doubts persisted about the administration’s commitment to honoring the agreement.

“As far as the United States is concerned, the voters have spoken, and that’s where we stand. We are unsure of their intentions,” stated South Africa’s Environment Minister Dion George.

US officials attending COP29 tried to assure global partners that even if President Trump withdraws from the international process, market forces, federal subsidies, and state mandates will continue driving the deployment of renewable energy.

Furthermore, conflicts in Ukraine and the Middle East diverted global attention towards security and energy availability, compelling many governments to tighten their budgets, making it challenging to secure larger climate finance amounts, noted observers.

“Given the current political climate, maintaining climate finance at its current level is an uphill battle,” remarked Joe Thwaites, a senior adviser at the Natural Resources Defense Council.

The pledged $300 billion annually by 2035 would theoretically triple the previous commitments of rich countries to provide $100 billion by 2020. Rich countries’ reluctance to offer further funding and the pressure to reach agreements amidst political turmoil disappointed least developed countries and small island states left out of negotiations at the Baku conference.

At one point during the summit’s final stages, the negotiating bloc representing these nations staged a walkout in protest, leading to a delay in reaching an agreement.

Representatives from Marshall Islands and India voiced their dissatisfaction with the climate finance deal, highlighting the reluctance of developed countries to fulfill their responsibilities, setting the stage for challenges at COP30 in Brazil.

“This could prove contentious in Belém. Brazil must find a way to rebuild trust,” remarked Oscar Soria, head of the Common Initiative focused on global financial reform.

Source: www.nbcnews.com

The complexity of Viking expansion into the North Atlantic was underestimated.

Vikings played a prominent role among the peoples of the North Atlantic, and the populations founded by them might be expected to be genetically similar and homogeneous. New research suggests that the Icelandic and Faroese people had distinctly different founding fathers. This result is consistent with a scenario in which the male population of the Faroe Islands was formed by a more diverse population from the more diverse Scandinavian population than from neighboring Icelanders. Furthermore, this study conclusively shows that there is no evidence of post-founder admixture between the Faroese and Icelandic gene pools.

The Faroe Islands consist of an archipelago of 18 small islands located in the North Atlantic Ocean between southern Norway, Iceland, and Scotland. As a result of their demographic history and relative geographical isolation, the Faroe Islands, like other North Atlantic island populations, are genetically homogeneous compared to mainland populations. Historical and archaeological sources report that the Faroe Islands were settled around 800 AD by Vikings, primarily from western Norway. However, increasing evidence suggests that these islands were settled earlier, perhaps by Celtic monks or other people from the British Isles. Carbon dating of peat moss and barley grain supports two pre-Viking periods of settlement, approximately 300-500 AD and 500-700 AD. More recently, scientists detected sheep DNA in archaeological deposits from 500 AD, and based on modern whole-genome data, the original founding of the Faroe Islands occurred between 50 and 300 AD. estimated that it may have been two to three centuries earlier than previously thought. Based solely on archaeological findings. Image credit: Oscar CR

From the 8th century to about 1050 AD, Vikings roamed the Atlantic in longships all the way to Newfoundland, Labrador, and Greenland, as well as exploring the Mediterranean and Eurasia.

Among the places they are known to have settled are the Faroe Islands, an archipelago of 18 islands in the North Atlantic Ocean.

They probably weren’t the first. Archaeologists have found evidence that these islands have been inhabited since about 300 AD, perhaps by Celtic monks or other people from the British Isles.

However, according to Fairinga Sagawritten around 1200, a Viking chieftain called Grimur Kamban settled in the Faroe Islands between about 872 and 930 AD. But where in Scandinavia did Grimur and his followers come from?

“We have strong evidence here that the Faroe Islands were colonized by a diverse group of male settlers from multiple Scandinavian populations,” said University of Louisville researcher Dr. Christopher Tillquist. .

In this study, Dr. Tillquist and his colleagues genotyped 12 “short tandem repeat” (STR) loci on the Y chromosome of 139 men from the Faroese islands of Bordoloi, Streymoy, and Suzloj.

They assigned each man to the most likely haplogroup. Each haplogroup has a different known distribution across Europe today.

They compared the genotype distribution to that found in 412 men from Norway, Sweden, Denmark, Iceland, and Ireland.

This allowed the team to reconstruct the source population of the founders of the Viking population.

Advanced analysis showed that the Faroe Islands sample range was similar to the broader Scandinavian genotype range, whereas the Icelandic genotypes were different.

The authors also developed a powerful and innovative genetic method called “variational distance from modal haplotype” to analyze SNP (single nucleotide polymorphism) variation within STRs.

This has led to the “founder effect” (vestiges of random loss of diversity during historical colonization by a small number of people) that remains in the genetic composition of male populations in the Faroe Islands and Iceland today. was able to clarify.

“Scientists have long thought that the Faroe Islands and Iceland were settled by similar Nordic peoples,” Dr Tillquist says.

“However, our new analysis showed that these islands were founded by people belonging to different gene pools within Scandinavia.”

“One group of diverse Scandinavian origins settled in the Faroe Islands, while a more genetically distinct group of Vikings colonized Iceland. They had separate genetic characteristics that continue to this day. Masu.”

“Despite their geographic proximity, there appears to have been no subsequent interbreeding between these two populations.”

“Our findings show that Viking expansion into the North Atlantic was more complex than previously thought.”

“Each longship that sailed to these distant islands carried a different genetic heritage, and not just Vikings.”

“We can now trace the separate journeys of conquest and settlement, revealing a more nuanced story of Viking exploration than is told in history books.”

of findings appear in the diary frontiers of genetics.

_____

Alison E. Mann others. 2024. Genetic evidence points to distinct patrilineal colonization of the Faroe Islands and Iceland. front. Genet 15;doi: 10.3389/fgene.2024.1462736

Source: www.sci.news

Astronomers conduct simulations of undetected asteroids within our galaxy

Astronomers discover large planets around other stars more often than small planets.whether to measure The gravitational pull of an exoplanet on its host starobserve How much starlight do exoplanets block?or Take a photo of the exoplanet itselfObservation methods for exoplanets are biased toward planets with masses twice the mass of Earth, or 12 septillion kilograms or more. But astronomers know that small planets exist. It's just harder to find because the smaller the planet, the more accurate equipment is needed.

Astronomers call planets smaller than Earth: sub-earth or asteroid. Current telescopes are bad at finding these tiny planets, so astronomers rely on simulations to determine how they behave. A team of astronomers studied the conditions of a hypothetical planetary system containing only asteroids. They argued that understanding where asteroids are likely to appear in large numbers will allow scientists to better understand how common these types of planets are.

To obtain a representative sample of the right conditions for planetary systems to form, astronomers simulation codeGenerate models of exoplanets similar to actual observations. Using this code, the team ran 33 sets of 1,000 simulations, each set with different starting parameters. Most stars in the Milky Way are in that size range, so they simulated a system containing stars ranging from 1/2 to 5 times the mass of the Sun. They ran all but the last two sets of simulations over a billion years of simulation time.

The first set was their point of comparison. This demonstrated that the code would produce a system containing asteroids given the same conditions as a solar system in which planets smaller than Earth are known to exist. In the next set of eight, they varied the mass of the host star, the spread of mass within the disk of matter's starting point, and the ratio of gas to dust in the system. The astronomers then ran four sets of experiments varying the period during which the asteroid could accumulate new material, ranging from 320,000 to 32 million years. The researchers ran 16 more sets, varying the amount of dust the system needed to start with, from exactly the same mass of Earth to 10,000 times the mass of Earth.

The astronomers' last four sets of simulations varied depending on the host star's mass, which ranges from 1.5 to 5 times the mass of the Sun. They ran their two largest sets on shorter timescales than the rest because large stars burn out their fuel faster and have shorter lifetimes than smaller stars. At the end of a star's life, it expands, sometimes quite dramatically. Scientists used these sets to find scenarios in which the star swallows the asteroid as it expands, and scenarios in which the star survives.

The researchers noted that computing power limits the scope of the simulation, as certain systems cannot perform calculations on more than 1,000 objects at once. Also, ice and rock were not allowed to accumulate at the edges of the system, as they do in real star systems. They said these factors limit the accuracy of models of planet formation processes and long-term system dynamics, respectively.

Overall, the research team found that asteroids should be extremely abundant in the universe. They found that under the parameters they studied, systems consisting of only planets between 1 and 110 million times the mass of Earth could “easily form.” They suggested that estimates of how often planets form around stars may significantly underestimate the actual frequency of planets.

Astronomers have found that the most important factor determining how large an asteroid becomes is the amount of dust it can initially form. But they also found that systems containing only small planets stop forming when the initial available dust exceeds 100 times the mass of Earth. Their final conclusions dealt with the outermost asteroids of certain systems, which are more than 10 times the distance from Earth to the Sun. They found that although these planets rarely grow larger than small moons, they can survive the star's inevitable expansion and persist for billions of years after the star's expansion.


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Source: sciworthy.com