Astronomers find the farthest merging quasar pair ever recorded

Astronomers have discovered a pair of merging quasars observed just 900 million years after the Big Bang. Not only is this the most distant pair of merging quasars ever found, but it’s also the first pair identified during a period in the history of the universe known as the “cosmic dawn.”



This image taken with the Subaru Telescope’s HyperSupreme-Cam shows a pair of quasars in the process of merging, HSC J121503.42-014858.7 (C1) and HSC J121503.55-014859.3 (C2). Image courtesy NOIRLab / NSF / AURA / TA Rector, University of Alaska Anchorage & NSF NOIRLab / D. de Martin, NSF NOIRLab / M. Zamani, NSF NOIRLab.

The dawn of the universe lasted from about 50 million to 1 billion years after the Big Bang.

During this period the first stars and galaxies began to appear and the dark universe was filled with light for the first time.

The appearance of the first stars and galaxies marked the beginning of a new era in the formation of the universe, known as the Reionization Epoch.

The epoch of reionization that occurred during the cosmic dawn was a period of cosmic transition.

About 400 million years after the Big Bang, ultraviolet light from the first stars, galaxies, and quasars spread throughout the universe, interacting with intergalactic matter and beginning a process called ionization, which stripped electrons from the universe’s primordial hydrogen atoms.

The reionization epoch is a crucial period in the history of the universe, marking the end of the cosmic dark ages and sowing the seeds of the large structures we observe in the local universe today.

To understand exactly what role quasars played during the reionization period, astronomers are interested in discovering and studying quasars that existed during this earlier, distant era.

“The statistical properties of quasars during the reionization stage can tell us a lot, including the progress and origin of reionization, the formation of supermassive black holes at the dawn of the universe, and the earliest evolution of the quasars’ host galaxies,” said Dr Yoshiki Matsuoka, an astronomer at Ehime University.

About 300 quasars have been discovered during the reionization period, but none have been found in pairs.

But as Dr. Matsuoka and his team were reviewing images taken with the Subaru Telescope’s HyperSupreme-Cam, a faint red spot caught their eye.

“While screening images for potential quasars, we noticed two similar, very red sources next to each other. This discovery was pure coincidence,” Dr Matsuoka said.

The distant quasar candidates are contaminated by many other sources, including foreground stars and galaxies and gravitational lensing, so the authors were unsure whether they were quasar pairs.

To confirm the nature of these objects, named HSC J121503.42-014858.7 and HSC J121503.55-014859.3, the team carried out follow-up spectroscopic measurements using the Faint Object Camera and Spectrograph (FOCAS) on the Subaru Telescope and the Gemini Near-Infrared Spectrograph (GNIRS) on the Gemini North Telescope.

The spectra obtained by GNIRS resolved the light emitted by the source into its constituent wavelengths and were crucial for characterizing the properties of the quasar pair and its host galaxy.

“GNIRS observations have shown that quasars are too faint to be detected in near-infrared light, even with the largest ground-based telescopes,” said Dr Matsuoka.

This allowed astronomers to deduce that some of the light detected in the visible wavelength range comes not from the quasar itself, but from ongoing star formation in its host galaxy.

The two black holes were also found to be enormous, with masses 100 million times that of the Sun.

This, combined with the presence of a bridge of gas extending between the two quasars, suggests that the two quasars and their host galaxies are undergoing a major merger.

“The existence of merging quasars during the reionization period has long been predicted, but this has now been confirmed for the first time,” said Dr Matsuoka.

This discovery paper In Astrophysical Journal Letters.

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Yoshiki Matsuoka others2024. Discovery of twin quasars merging at z = 6.05. Apu JL 965, L4; doi: 10.3847/2041-8213/ad35c7

Source: www.sci.news

How social media and screen time impact young people: The reality

“Put that phone away!” Most parents have yelled something similar to this at their children, usually resulting in a shocked look on the child’s face.

In recent years, the spread of smartphones and social media has led us to spend more time in front of screens. Children are no exception. The COVID-19 pandemic has led to a significant increase in children’s screen time due to lockdowns and school closures.

There are many frightening claims about excessive screen time for children and teens: that it harms their mental health, leading to depression, eating disorders and even suicide; that it cuts into time they could be spending on socializing and exercise, making them feel lonely and less physically fit; and more. In short, the fear is that spending too much time on digital devices is ruining our children’s lives, with the tech companies who design the apps that keep us hooked being complicit. It’s no wonder that governments around the world are considering restricting screen time for under-18s.

Yet a closer look at the evidence does not support this overwhelmingly negative view. This does not mean that the tech giants are harmless and that further regulation is not needed. But it does mean that we need to think more carefully about what healthy screen time looks like for young people, and how we can make the online world the most accessible to them. So here is your guide to what we actually know about the impact of screens and social media.

One thing is clear in this complex field: children and young people, like the rest of us, spend a lot of time in front of screens.

Source: www.newscientist.com

Self-driving cars are typically safer than humans in most scenarios, but struggle around curves

Self-driving car driving through downtown San Francisco

Jason Doi Photography/Getty Images

Self-driving cars may be safer than human drivers in everyday situations, but the technology struggles more than humans in dark places and when turning, according to the largest accident research study to date.

The findings come at a time when self-driving cars are already on the roads in some US cities, and GM-owned Cruise is set to resume testing of driverless cars. Pedestrian dragging incident The March incident prompted California to suspend its license, but Google spinoff Waymo has been gradually expanding its robot taxi operations in Austin, Los Angeles, Phoenix and San Francisco.

“It is important to improve the safety of self-driving cars at dawn, dusk or when turning,” he said. Ding Sheng Xuan “Key strategies include strengthening weather and lighting sensors and effectively integrating sensor data,” say researchers from the University of Central Florida.

Ding and his colleagues Mohamed Abdel AtiA team from the University of Central Florida collected data from California and the National Highway Traffic Safety Administration (NHTSA) on 2,100 crashes involving vehicles equipped with some degree of autonomous or driver-assistance technology, as well as more than 35,000 crashes involving unassisted human drivers.

The researchers then used statistical matching techniques to find pairs of accidents that occurred under similar circumstances, with common factors such as road conditions, weather, time of day, whether the accident happened at an intersection or on a straight road, etc. The researchers focused their matching analysis on 548 autonomous vehicle accidents reported in California, excluding less automated vehicles equipped only with driver assistance systems.

Abdel Aty said the overall results suggest that self-driving cars are “generally safer in most situations.” But the analysis also found that self-driving cars are five times more likely to crash when driving at dawn and dusk than human drivers, and are almost twice as likely to crash when making turns.

One obstacle to research is that “the database of autonomous vehicle accidents is still small and limited,” Abdel Aty said. He and Din cited the need for “enhanced autonomous vehicle accident reporting,” a major caveat that independent experts agree with.

“I think this is an interesting, but very early, step in measuring the safety of self-driving cars.” Missy Cummings Cummings, of George Mason University in Virginia, said the number of self-driving car accidents is “too small to make blanket conclusions about the safety of these technologies,” and warned about biased reporting by self-driving car makers. During her time at NHTSA, Cummings said, video footage of accidents didn’t always match the manufacturers’ explanations, which tended to place the blame on the human driver. “When you looked at the actual videos, they told a completely different story,” she said.

He said some minor collisions may not be reported to police, so that factor needs to be taken into account when comparing accidents involving self-driving cars with those involving human drivers. Eric Teo Virginia Insurance Institute for Highway Safety, 2017 study Early testing of Google’s self-driving cars found that only three out of 10 accidents made it into police reports.

“Neither California nor NHTSA require comprehensive data reporting on the testing and deployment of autonomous vehicles,” Cho Junfeng “Autonomous vehicles, and especially robotaxis, often operate in specific regions and environments, making it difficult to generalize research findings,” the Arizona State University researchers said.

topic:

  • artificial intelligence/
  • Driverless cars

Source: www.newscientist.com

Paleontologists Uncover Secrets of ‘Elgin Marvel’ Fossil

The “Elgin Marvel” fossil is a block of reddish sandstone containing a natural cast of a Permian skull and jaw. Dicynodonts It was discovered in the Hopeman Sandstone Formation near Elgin, Scotland. According to a new study, the specimen Gordonia traquairi A type of dicynodont that lived between 254 and 252 million years ago, when the Earth was made up of a single land mass called Pangaea.

Artist image Gordonia traquairi Image courtesy of Scott Reed.

Gordonia traquairi It belongs to a group of extinct species known as dicynodonts, and is characterized by its stocky body, beak, and tusks.

This organism lived relatively shortly before the end-Permian extinction (the Great Dying), the worst mass extinction event in history, which occurred about 252 million years ago and wiped out much of life on Earth.

The Elgin Marvel specimen is one of the best-preserved in a series of fossils collected near Elgin in northeast Scotland.

These are collectively known as the Elgin reptiles. Gordonia traquairi are closely related to mammals.

In the new study, paleontologist Heidi George of the University of Edinburgh and her colleagues performed micro-CT scans of the cavities the animal carved into the sandstone before the bones deteriorated.

The scan produces a three-dimensional representation of the skull anatomy, including details of the brain.

These insights help us understand animal behavior and the biology behind it, providing clues about the evolution of this and other species.

Gordonia traquairi The fossil shares many physical characteristics with similar remains found in China, indicating that dicynodonts were diversifying around the world just before the devastating extinction.

The Elgin reptile is the only known example of this type of fossil from Western Europe.

Palaeontologists hope that the increasing use of micro-CT scanning as a tool to study fossils in detail, combined with the trend toward open sharing of data, will provide opportunities to add to the body of knowledge in the field.

“The Elgin Marvel is a fascinating fossil of an ancient mammal relative that is one of the best-preserved of the world-famous Elgin reptiles,” Dr. George said.

“Most of these famous fossils were discovered more than a century ago, but it’s only recently that new techniques have revealed more detail and provided valuable insights into their skull and brain anatomy and lineage.”

“It’s hard to imagine, but about 250 million years ago Scotland was a desert covered with sand dunes. Gordonia “God was in control of the world,” says Professor Steve Brusatte of the University of Edinburgh.

“By studying them, we can learn about some of the earliest stages of our own evolution.”

This study paper In Zoological Journal of the Linnean Society.

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Heidi George others Micro-CT data reveal new information about the craniomandibular and neuroanatomy of dicynodonts. Gordonia (Therapsid: Heterodontida) Lived in the Late Permian of Scotland. Zoological Journal of the Linnean Society Published online June 18, 2024; doi: 10.1093/zoolinnean/zlae065

Source: www.sci.news

Astronomers observe the reawakening of a supermassive black hole

In December 2019, a little-known galaxy called SDSS 1335+0728, located 300 million light-years away in the constellation Virgo, suddenly started glowing brighter than ever before. To understand why, astronomers used data from multiple space and ground-based observatories to track the changes in the galaxy's brightness. They concluded that they were witnessing the sudden awakening of the supermassive black hole at its center.

This artist's impression shows the black hole drawing in the surrounding gas, growing a disk of material that lights up the galaxy. Image credit: ESO/M. Kornmesser.

“Imagine observing a distant galaxy for years and it always seemed quiet and inactive,” said Dr Paula Sánchez Sáez, astronomer at ESO and the Millennium Astrophysics Institute.

“Suddenly, the brightness of its central core began to change dramatically, which is not a typical phenomenon we've seen before.”

This is what happened to SDSS 1335+0728, which has been classified as having an active galactic nucleus (AGN) after brightening dramatically in December 2019.

Galaxies can suddenly brighten due to events such as supernova explosions or tidal disruption, but these changes in brightness usually only last for a few tens or, at most, a few hundred days.

SDSS 1335+0728 continues to grow brighter, more than four years after it was first observed “lighting up.”

What's more, the changes detected in the galaxy are unlike anything seen before, suggesting alternative explanations to astronomers.

Dr Sáez and his colleagues sought to understand these brightness changes by combining archival data with new observations from several facilities, including the X-SHOOTER instrument on ESO's Very Large Telescope.

Comparing data taken before and after December 2019, we found that SDSS 1335+0728 now emits much more light in ultraviolet, visible and infrared wavelengths, and the galaxy also began emitting X-rays in February 2024.

“This kind of action is unprecedented,” Dr. Saez said.

“The most concrete option to explain this phenomenon is that we are seeing the galactic core starting to show activity,” added Dr Lorena Hernández García, an astronomer at the Millennium Institute for Astrophysics and Valparaíso University.

“If this is the case, it would be the first time that we have observed the activation of a massive black hole in real time.”

“Supermassive black holes are normally dormant and cannot be seen directly,” said Dr Claudio Ricci, an astronomer at the Diego Portales University and the Kavli Institute for Astronomy and Astrophysics at Peking University.

“In the case of SDSS 1335+0728, we were able to observe a massive black hole awakening and suddenly absorbing the surrounding gas, becoming extremely bright.”

“This process has never been observed before,” Dr. Garcia said.

“Previous studies have reported that dormant galaxies become active after a few years, but this is the first time that the process of black hole awakening itself has been observed in real time.”

“This could also happen to Sagittarius A*, the supermassive black hole at the centre of our Milky Way galaxy, but we don't know how likely this is to happen.”

“Regardless of the nature of the fluctuations, SDSS 1335+0728 will provide valuable information about how black holes grow and evolve,” said Dr. Sáez.

“We hope that instruments like MUSE on the VLT and the upcoming MUSE on the Extremely Large Telescope (ELT) will hold the key to understanding why galaxies are brightening.”

of study Published in a journal Astronomy and Astrophysics.

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P. Sanchez Aes others2024 SDSS1335+0728: The awakening of the universe about 1 billion years ago6 M_sun Black hole. A&Ain press; doi: 10.1051/0004-6361/202347957

Source: www.sci.news

First Class of U.S. Climate Corps Sworn in at White House

The Biden administration announced on Tuesday that the United States Climate Corps is a federal program focused on training young individuals in clean energy, environmental protection, and climate resilience. AmeriCorps, the federal agency overseeing the program, plans to swear in 9,000 members by the end of the month. Due to virtual meeting room limitations, the swearing-in will take place at multiple events over the next few weeks, with the next event scheduled for June 25.

“I want young people to understand the significance of this moment,” said Maggie Thomas, special assistant for climate change to President Joe Biden. “This is about addressing the climate crisis and empowering this generation to take charge of their future.”

Ultimately, 20,000 young people will participate in the program. Various paid positions are available through federal, state, and local partnerships with employment durations ranging from two months to over a year, all funded by the federal government.

The focus of these positions is on connecting vulnerable communities to renewable energy grids and supporting local community initiatives, such as securing grant funding and reducing wildfire risks in forests.

The White House views this program as a dual-purpose initiative to address immediate climate change impacts and equip young individuals with the necessary skills for careers in clean energy and climate-resilient industries.

The U.S. Climate Corps, founded by John F. Kennedy, emphasizes the importance of community involvement in climate action and offers multiple pathways for individuals to engage in environmental efforts.

This initiative, originating from Franklin D. Roosevelt’s Civilian Conservation Corps, signifies a significant step toward combating climate change and creating a sustainable economy. President Biden’s executive order regarding climate crisis highlights the administration’s commitment to addressing environmental challenges.

For further information and opportunities to join the program, visit the official website.

Source: www.nbcnews.com

Do plants possess intelligence? | Science News

of Tall goldenrod (Solidago altissima)a North American species of the goldenrod family Asteraceaecan recognize other nearby plants without touching them by sensing the proportion of far-red light reflected from their leaves. When goldenrod is eaten by herbivores, it adapts its response based on whether other plants are nearby. Are such flexible, real-time adaptive responses a sign of plant intelligence?

In the context of behavioral ecology, plant responses to environmental stressors are increasingly being studied. This is especially true for plant responses to herbivores, which mediate direct and indirect defense and tolerance. These seemingly adaptive changes in plant defense phenotypes in the context of other environmental conditions have prompted discussion of such responses as intelligent behavior. In their paper, Kessler and Mueller explore the concept of plant intelligence and some of its predictions regarding chemical signaling in plant interactions with other organisms. Image courtesy of Becky.

“There are over 70 published definitions of intelligence, and even within specific fields there is no consensus on what it is,” says chemical ecologist Professor André Kessler. Cornell University.

“Many people believe that intelligence requires a central nervous system, and that electrical signals act as the medium for information processing.”

“Some plant biologists equate the plant's vascular system with a central nervous system, arguing that there is some centralized entity within the plant that allows it to process and respond to information.”

But Kessler and his colleague, Michael Mueller, a doctoral student at Cornell University, disagree.

“Although electrical signals are clearly seen in plants, there is no solid evidence of any homology with the nervous system, but the question is how important they are to the plant's ability to process environmental signals,” Professor Kessler said.

To make the case for plant intelligence, the authors narrowed the definition down to its most basic element: the ability to solve problems toward a specific goal based on information obtained from the environment.

As a case study, Kessler points to previous research looking at goldenrod and its response to being eaten by pests.

When beetle larvae feed on goldenrod leaves, the plant releases chemicals that let the insects know the plant is damaged and a poor food source.

These airborne chemicals, called volatile organic compounds (VOCs), are also absorbed by nearby goldenrod plants, causing them to develop their own defenses against the beetle larvae.

In this way, goldenrod attracts herbivores to nearby areas, dispersing damage.

In 2022, Professor Kessler and his co-authors Experiments were conducted To show that Solidago altissima They can also detect a higher proportion of far-red light reflected from the leaves of nearby plants.

If nearby plants are feeding on goldenrods by beetles, the goldenrod will grow faster in an effort to withstand the herbivores, but it will also start producing defensive compounds that help the plant fight off the pests.

In the absence of neighboring plants, plants do not accelerate their growth when eaten, and their chemical response to herbivores is significantly different, but they can still survive a significant amount of herbivore attack.

“This fits into our definition of intelligence: plants change their standard behaviour in response to information they receive from the environment,” Professor Kessler says.

“Neighboring goldenrods also become intelligent when they detect VOCs that signal the presence of pests.”

“Volatile emissions from nearby areas are a harbinger of future herbivore occurrence.”

“They can use cues from the environment to predict future situations and act accordingly.”

“Applying the concept of intelligence to plants could generate new hypotheses about the mechanisms and functions of plant chemical communication and may even change people's ideas about what intelligence actually means.”

“The latter idea is timely because artificial intelligence is a hot topic right now. For example, at least for now, artificial intelligence doesn't solve problems toward a goal.”

“Artificial intelligence is not even intelligent according to our definition of intelligence. Artificial intelligence is based on patterns it identifies from the information it has access to.”

“The idea that interests us comes from mathematicians in the 1920s who proposed that plants might function like beehives.”

“In this case, each cell acts like an individual bee, and the whole plant resembles a hive.”

“That means the plant brain is the whole plant, without any central coordination.”

“Instead of electrical signals, chemical signals are transmitted throughout the superorganism.”

“Work by other researchers has shown that all plant cells have a wide range of light spectrum recognition and sensory molecules to detect very specific volatile compounds emanating from nearby plants.”

“They can sniff out their environment with great precision, and as far as we know, all cells can do that.”

“Cells may be specialized, but they all recognize the same things, communicate through chemical signals, and trigger collective responses in growth and metabolism.”

“The idea is very appealing to me.”

Team paper Published in the journal Plant signaling and behavior.

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Andre Kessler & Michael B. Mueller. Induced resistance to herbivores and intelligent plants. Plant signaling and behaviorPublished online April 30, 2024, doi: 10.1080/15592324.2024.2345985

Source: www.sci.news

Astronomers say that a near, warm Neptune has a sulfurous atmosphere

The warm Neptunian exoplanet, called GJ 3470b (Gliese 3470b), is 96 light years away and orbits a 2 billion year old red dwarf star in the direction of the constellation Cancer.

Artist's impression of the warm-Neptunian exoplanet GJ 3470b. Image courtesy of the University of Wisconsin-Madison Department of Astronomy.

First discovered in 2012, GJ 3470b is the lightest and coolest (over 325 degrees Celsius, or 600 degrees Fahrenheit) exoplanet containing sulfur dioxide.

The compounds are likely a sign of active chemistry taking place in the planet's atmosphere, as radiation from a nearby star explosively breaks down hydrogen sulfide components, which then seek out new molecular partners.

“We never expected to see sulfur dioxide on such a small planet, so finding this new molecule in an unexpected place is exciting because it gives us new ways to understand how these planets formed,” said Professor Thomas Beatty of the University of Wisconsin-Madison.

“And small planets are particularly interesting because their composition depends heavily on how the planet-formation process happened.”

Prof Beatty and his colleagues hope that by observing what exoplanets contain, they can shed light on the principles of planet formation and do just that.

“The discovery of sulphur dioxide on a small planet like GJ 3470b adds another important item to the list of ingredients for planet formation,” Prof Beatty said.

In the case of the GJ 3470b, there are also other interesting features that could help round out that recipe.

The planet orbits the star and passes nearly over the star's pole, meaning that it orbits at a 90 degree angle to the expected orbit of a planet in this system.

The moon is also incredibly close to its star, close enough that light from the star would blow a lot of GJ 3470b's atmosphere out into space.

The team says the planet may have lost around 40% of its mass since it formed.

The misaligned orbit suggests that GJ 3470b was once somewhere else in the system, and at some point, the planet became caught in the gravity of another planet, pulling it into a new orbit and eventually settling in a different neighborhood.

“The migration history that led to this polar orbit and how it has lost so much mass are things we don't typically know about other exoplanet targets that we study,” Prof Beattie said.

“These are important steps in the recipe that created this particular planet, and they help us understand how planets like this one are made.”

“Further analysis of the components remaining in the planet's atmosphere may help us understand why planets like GJ 3470b became so appetizing.”

This month, the authors 244th Meeting of the American Astronomical Society In Madison, Wisconsin.

Source: www.sci.news

Paris heatwave raises concerns for Olympic hopefuls

summary

  • A group of Olympic hopefuls has expressed concern about the heat during the games in Paris.
  • Olympic organizers say they are preparing for tough conditions, including scheduling events to avoid heat.
  • A study has found that Paris is one of the European capitals most vulnerable to heatstroke concerns.
  • Heatwaves could cause temperatures to rise by up to seven degrees Celsius since 2003 A study published in November.

Leading up to the Paris Olympics, athletes are raising concerns about the scorching summer temperatures and the impact of climate change on their competitiveness and safety in sports.

In a recent report by climate advocacy and sports organizations in the UK and US, 11 athletes have highlighted the environmental challenges at the upcoming Olympics and the long-term implications for sporting competitions in a warming world.

Report The average temperature in Paris during the Olympics is projected to be over 5.5 degrees higher than in 1924, the last time the city hosted the event.

Athlete Jamie Ferndale, a former GB Olympic rugby sevens team member, expressed concerns about the extreme heat in Paris potentially affecting athletes’ performance.

“When temperatures reach 30 to 35 degrees Celsius, it becomes quite dangerous,” Ferndale said. “With six games in three days, athletes don’t have enough time to cool off between matches.”

Olympic organizers are taking measures to combat the heat, scheduling events strategically to minimize exposure and implementing heat-response tools to ensure safety, according to an International Olympic Committee spokesperson.

Local organizers for Paris 2024 have stated that France’s meteorological service will be closely monitoring temperatures, and adjustments to competition dates can be made if needed. Free water will also be available to spectators to help combat the heat.

Paris, being one of the European capitals most vulnerable to heat waves, is focusing on reducing the carbon footprint of the Olympics. Geothermal cooling and natural ventilation will be used in the athletes’ village, which will serve as permanent housing post-Olympics.

Athlete Pragnya Mohan raised concerns about the lack of air conditioning potentially affecting athletes’ recovery rate. However, the Paris 2024 committee assured that temperatures in athlete accommodations would be significantly lower than outside, and portable cooling units would be available for rent.

Discus thrower Sam Mathis questioned the feasibility of hosting Summer Olympics during the hottest times of the year, considering the challenges posed by extreme heat. Research has shown that heat-related illnesses have affected athletes in past Olympics, prompting the need for climate-conscious measures.

Investments in sustainable practices, such as cleaning up the Seine, building bike lanes, and planting shade trees, demonstrate Paris’ commitment to reducing emissions and adapting to future climate challenges.

Deputy Mayor Emmanuel Gregoire stressed the urgency of making changes to protect people from the dangers of extreme heat in everyday life.

Source: www.nbcnews.com

Rare nothosaurus fossil discovered in New Zealand

The 246-million-year-old specimen is the geologically oldest marine reptile to inhabit the Southern Hemisphere.

This image shows a nothosaurus swimming along the ancient Antarctic coast of what is now New Zealand about 246 million years ago (during the Triassic Period). Image courtesy of Stavros Kundromichalis.

“Reptiles dominated the seas millions of years before dinosaurs dominated the land,” said Dr Benjamin Kear from the Museum of Evolution at Uppsala University and his colleagues.

“The most diverse and geologically longest-surviving group are the sauropods, with an evolutionary history spanning more than 180 million years.”

“This group included the long-necked plesiosaurs. Nothosaurus was their distant ancestor.”

“Nothosaurus could grow up to 7 metres (23 feet) in length and swam using four paddle-like limbs. It had a flattened skull with a web of narrow, conical teeth that it used to catch fish and squid.”

The 246-million-year-old Nothosaurus fossil was discovered in 1978 in rocks found along a major tributary of the Balmacaan River at the foot of Mount Harper in the Harper Ranges of New Zealand's central South Island.

“The New Zealand nothosaurus is more than 40 million years older than the oldest sauropod fossil yet found in the Southern Hemisphere,” said Dr Keir, lead author of the paper. paper Published in the journal Current Biology.

“We show that these ancient marine reptiles lived in shallow coastal environments rich in marine life within the Antarctic Circle at that time.”

“The oldest nothosaurus fossils date back to about 248 million years ago and were found along an ancient low-northern latitude belt that stretched from the remote northeastern to northwestern edges of the Panthalassa superocean.”

“The origin, distribution and timing of the arrival of nothosaurs in these remote areas remain a matter of debate.”

“Some theories suggest that they migrated along Arctic coastlines, swam through inland seas, or used ocean currents to cross the Panthalassa superocean.”

Morphology and biogeographical context of the earliest sauropod-finned fish in the Southern Hemisphere. Image courtesy of Kear others., doi: 10.1016/j.cub.2024.03.035.

New fossils discovered in New Zealand overturn these long-held assumptions.

“Using a time-calibrated evolutionary model of the global distribution of sauropods, we show that nothosaurs originated near the equator and then rapidly spread north and south at the same time that complex marine ecosystems were being re-established after the great extinction that marked the beginning of the Age of Dinosaurs,” Dr Kear said.

“The beginning of the age of the dinosaurs was marked by extreme global warming, which allowed these marine reptiles to thrive in Antarctica.”

“This also suggests that the ancient polar regions were likely routes for their earliest global migration, similar to the epic transoceanic journeys undertaken by modern whales.”

“There are surely fossils of long-extinct sea monsters still waiting to be discovered in New Zealand and other parts of the Southern Hemisphere.”

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Benjamin P. Kear others2024. Earliest southern sauropods reveal early globalization of marine reptiles. Current Biology 34(12):562-563; doi: 10.1016/j.cub.2024.03.035

Source: www.sci.news

New bird-like dinosaur unearthed by paleontologists in Argentina

A new genus and species of Unenraghiin dinosaur has been identified by Argentine paleontologists. DiuqinrechiguanaeThe discovery fills a large gap in the theropod dinosaur fossil record.

Reconstructing your life DiuqinrechiguanaeImages/Photos Courtesy: Porfiri others., doi: 10.1186/s12862-024-02247-w.

Diuqinrechiguanae It lived on Earth during the Santonian stage of the Cretaceous period, 86 to 84 million years ago.

This species Unenraghiina subfamily of long-snouted proto-avian theropods within the family Dromaeosauridae.

“The Unenraghiin was a carnivorous dinosaur from the Gondwana continent. Paraves“It is a clade that includes birds and their closest non-avian theropod relatives,” said Dr Juan Porfiri of the National University of Comahue in Buenos Aires and his colleagues.

“The fossil record of Unenlagineidae comes primarily from Argentina, where the greatest number of specimens and the most complete skeletons have been found, but other material at least tentatively assigned to Unenlagineidae has been found in Brazil, Chile, Colombia, and Antarctica.”

“A small, flying Malagasy theropod Lahonavis Ostromi Depending on the particular phylogenetic hypothesis adopted, they are often considered to be non-enragine.

“The Unenraginae are most often interpreted as early-diverging dromaeosaurids, but others consider these theropods to be a separate proto-avian clade (Unenragiiidae).”

“They are an important clade for understanding the origin of birds because they are closely related phylogenetically to birds.”

“But unfortunately, most species are only represented by fragmentary fossils.”

DiuqinrechiguanaeA fragmentary but related skull was found. Bajo de la Culpa Formation Neuquén province, Patagonia, Argentina.

“The specimen was collected in the province of Neuquén, from the isthmus between the southeastern shore of the Balearic Lake and the northwestern shore of Lake Mari-Menuco,” the paleontologists said.

According to the authors: Diuqinrechiguanae It is the first species of Unenraghiine dinosaur to be discovered in the Bajo de la Culpa Formation.

“The Bajo de la Culpa Formation provides fossils that comprehensively represent a diverse and important group of paleontological species,” the researchers said.

“Vertebrate fossils are abundant and often well preserved, including snakes, lizards, turtles, crocodylomorphs, indeterminate pterosaurs, ornithopods, titanosaur sauropods, non-avian theropods, and bird fossils.”

Diuqinrechiguanae It fills a gap of at least 15 million years in the Unenra Guinness fossil record (conservative estimates are 90-75 million years, perhaps more).

“This new species adds to the South American Unenraguines fossil record by filling a large gap in their temporal distribution,” the researchers said.

“Saved elements Diuqinrechiguanae It is morphologically distinct from corresponding bones in other Unenraginian species, including an accessory plate on the most posterior sacral vertebral neural arch, unique paired foramina in the most posterior sacral and anterior coccygeal neural arches, a humerus with a distally positioned distal lateral deltoid ridge, and several conditions that appear intermediate between the humerus and the humerus. Unenragia spp. and the very large Unenraghiines Austroraptor Kabazai. “

“Combined with gaps in the strata spanning millions of years, Diuqinrechiguanae These anatomical differences support the validity of the new species, which are geologically older and newer Unenlagines, respectively.”

“Furthermore, the humerus Diuqinrechiguanae The type specimen retains two conical tooth impressions, indicating that the remains were eaten by another tetrapod, possibly a crocodylomorph, mammal, or theropod (perhaps a megaraptor, as represented by teeth found at the same site, or perhaps another non-enraginean individual of the same species).”

Discovery Diuqinrechiguanae It has been reported paper In the journal BMC Ecology and Evolution.

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JD Porfiri others. 2024. Diuqinrechiguanae A new genus and species of the subfamily Unenraginae (Theropoda: Hypopoda) from the Bajo de la Culpa Formation (Neuquén Group, Upper Cretaceous), Neuquén Province, Patagonia, Argentina. BMC Ecolevo 24, 77; doi: 10.1186/s12862-024-02247-w

Source: www.sci.news

Observing a humanoid robot driving a car at a very slow pace

Humanoid robots that can drive cars may one day be used as chauffeurs, but their creators acknowledge that this could be at least 50 years away.

Most driverless cars work completely differently than a human driver, using artificial intelligence and custom mechanical systems to directly control the steering wheel and pedals. This approach is much more efficient and simpler than using a humanoid robot to drive, but it needs to be customized for each specific car.

Kento Kawarazuka Professor Takeru Sato of the University of Tokyo and his team have developed a humanoid robot called “Musashi” that can drive a car just like a human. Musashi has a human-like “skeleton” and “muscles,” and is equipped with cameras in both eyes and force sensors in its limbs. An artificial intelligence system determines the movements required to drive the car and responds to events such as changes in the color of traffic lights and people cutting in front of the car.

Currently, robots can only perform a limited range of driving tasks, such as going straight or turning right, at speeds of around 5km per hour on non-public roads. “The pedal speed and car speed are not high, and the car handling is also not as fast as a human,” Kawarazuka said.

Musashi is a humanoid robot that operates cars just like a human would.

Kento Kawarazuka et al. 2024

But Kawarazuka hopes that as the system is improved it could be used in any car, which could be useful when humanoid robots are routinely produced. “I’m not looking 10 or 20 years out, I’m looking 50 or 100 years out,” he says.

“This research could be of interest to people developing humanoid robots, but it doesn’t tell us much about autonomous driving.” Jack Stilgoe “Self-driving cars cannot and should not drive like humans. Because the technology doesn’t need to rely on limbs and eyes, it can rely on digital maps and dedicated infrastructure to find safer, more convenient ways to navigate the world,” say researchers at University College London.

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Source: www.newscientist.com

How to Recognize and Conquer Body Dysmorphic Disorder

If you have ever set a goal to change your appearance, know that you are not alone. Approximately 43% of UK adults aim to lose weight. For some, this goal may lead to more extreme methods such as cosmetic or plastic surgery.

However, when does this desire for self-improvement become problematic? About 3% of the general population may develop a condition known as body dysmorphic disorder (BDD), where individuals have a constant urge to alter their physical appearance.

Individuals with BDD perceive significant flaws or defects in their appearance that may not be as noticeable to others. For example, Rebecca, a 36-year-old woman, believes she has a “moon face” due to acne scars, while Tyson, a 17-year-old, works out excessively because he feels too skinny. Despite reassurances from others, they continue to struggle with their self-perception.

BDD is not a new phenomenon and has been recognized since 1891. Factors such as genetics, brain function, and adverse childhood experiences can contribute to the development of BDD. Society’s focus on appearance can exacerbate this condition, as attractive individuals often receive social advantages.

Social media has also played a role in heightening BDD prevalence, with filters, editing tools, and curated content leading to unrealistic beauty standards. Excessive social media use has been linked to increased BDD symptoms and a desire for cosmetic procedures.

People with BDD often engage in extreme behaviors to alter their appearance, such as mirror gazing, excessive grooming, or seeking cosmetic treatments. However, studies have shown that cosmetic surgery may not provide lasting relief for individuals with BDD, and their symptoms may worsen post-surgery.

Cognitive behavioral therapy with exposure and response prevention (CBT-ERP) is a recommended treatment for BDD, offering relief for up to 70% of individuals. It is essential for cosmetic surgeons to identify BDD in patients before performing procedures to prevent further distress.

Instead of fixating on appearance, individuals can focus on engaging in hobbies, limiting mirror time, and taking breaks from social media to improve self-esteem. Developing a broader sense of self-worth beyond physical appearance is key to overcoming BDD.

*Names and descriptions do not reflect actual clients.

Source: www.sciencefocus.com

Hubble Space Telescope Discovers a Massive Binary Protostar within the RCW 7 Nebula

RCW 7 is located in the constellation Puppis, about 5,300 light years from Earth.



This Hubble image shows the nebula RCW 7. Image courtesy of NASA/ESA/Hubble/J. Tan, Chalmers University, University of Virginia.

“Nebulae are regions of space that are rich in the raw materials needed to form new stars,” the Hubble astronomers said.

“Due to the effects of gravity, some of these molecular clouds collapse and merge into protostars surrounded by a rotating disk of remaining gas and dust.”

“In the case of RCW 7, the protostar forming here is particularly massive, emitting intense ionizing radiation and a powerful stellar wind that propelled the star into a “H II region“.

“The H II regions are filled with hydrogen ions. HI refers to regular hydrogen atoms, and H II is hydrogen that has lost an electron.”

“Ultraviolet rays from the massive protostar excite the hydrogen, which then emits light that gives the nebula its soft pink glow.”

In RCW 7, the researchers IRAS 07299-1651.

“IRAS 07299-1651 still resides within a cocoon of glowing gas, in clouds swirling towards the top of the nebula,” the researchers said.

To expose this star and its sibling, the new image was created from separate exposures taken in the near-infrared region of the spectrum. Hubble’s Wide Field Camera 3 (WFC3).

“This massive protostar is most bright in ultraviolet light, but it also emits a lot of infrared light that penetrates much of the surrounding gas and dust and can be seen by the Hubble Telescope,” the scientists said.

“Many of the other large visible stars in this image are not part of the nebula, but are located between the nebula and the solar system.”

Assuming a circular orbit, IRAS 07299-1651 is estimated to have a minimum total mass of 18 times that of the Sun and a maximum period of 570 years.

“The formation of the H II region marks the beginning of the end of the molecular cloud,” the authors said.

“Over just a few million years, radiation and winds from the massive stars gradually disperse the gas, and this dispersion continues as the most massive stars end their lives in supernova explosions.”

“Only a small portion of this gas will be absorbed by new stars within the nebula, while the rest will spread throughout the galaxy and eventually form new molecular clouds.”

Team Investigation result Published in a journal Natural Astronomy.

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Y. Chan others2024. Dynamics of a giant binary star at birth. Nat Astron 3, 517-523; doi: 10.1038/s41550-019-0718-y

Source: www.sci.news

What was the speed of life’s recovery from the end-Permian mass extinction?

Think back to the last time you put together a puzzle. How long did it take you to connect the first piece? Did you aim for the edge pieces, or did you look for random pairs? Now imagine that the puzzle pieces are fossils of marine creatures that lived in ancient oceans. How would you put the pieces together? Which animals appeared first, and how long did they live for? This is the “puzzle” paleontologists face when studying the fossil record.

Researchers studying the fossil record have found that a mass extinction occurred at the end of the Permian Period 250 million years ago, leaving the oceans largely empty. They propose that the Earth's higher temperatures and changes in water chemistry killed 80% of marine life, ending the Paleozoic Era. Sometime later, during the Triassic Period, marine communities were reorganized to include a diversity of organisms similar to those found in today's oceans. As such, scientists believe that Triassic marine life is a precursor to modern marine ecosystems.

Paleontologists initially thought that marine animals recovered slowly from this extinction, because complex fossil ecosystems were only discovered 10 million years later. More recently, researchers have found diverse marine animal fossils just 3 million years after this mass extinction. However, these studies leave a gap of 3 million years between the mass extinction and the appearance of modern-like marine life in the earliest Triassic period.

An international team of researchers hypothesized that a collection of fossils in southern China called the Guiyang Biota could help fill in this gap: These ancient animals were covered in deep-sea sand, forming a layer of exceptionally well-preserved fossils, LagerstätteLagerstätten often form in calm undersea environments that can preserve delicate animal parts like bones and scales. Based on their location and their position within the rocks, the team proposed that the Guiyang fossils date to the Early Triassic period.

The scientists explained that the fossils at the site included animals across all five levels of the food chain, including 10 species of bony fish, two species of shrimp, lobsters, sponges, eels, and plankton. They found that fish ate lobsters, which ate clams, which ate plankton, which ate algae, which provided energy, forming a complete modern-day marine community. The scientists suggested that these fossils may be younger than the oldest diverse fossil ecosystem scientists have ever unearthed from the Early Triassic Period.

The researchers used three methods to determine the age of the Guiyang fossils: First, they looked at the eel-like creature's teeth. ConodontsThey only lived during certain periods in Earth's history, and the researchers found that conodont teeth from the southern China fossils belonged to Triassic conodonts, supporting their original dating estimates.

Second, the researchers measured chemical signals. Carbon isotopesfound in the rock walls surrounding the fossils. Scientists have measured carbon isotopes in rocks throughout Earth's history. By matching the increases and decreases in carbon isotopes in rocks to patterns of carbon isotopes from different periods in the rock record, researchers can estimate the age of the rocks. They found that the carbon isotopes in the Guiyang rocks matched the patterns of carbon isotopes in rocks from the Early Triassic Period, further supporting the Triassic age of the fossils.

Finally, the researchers needed to establish a precise age for the Guiyang rocks to determine how rapidly the fossil assemblage developed after the mass extinction event. They used a dating method based on the radioactive decay of uranium into lead. U-Pb datingIt is found in minerals extracted from two volcanic ash layers in the rock wall.

The team explained that these ash layers were located just below and just above the fossil layers in the rocks, meaning they fell just before and just after the fossils formed. U-Pb dating determined that the fossils were between 250.79 and 250.92 million years old. The team interpreted these dates as indicating that the marine creatures lived only 10,000 to 1 million years after their extinction 250 million years ago.

From the Triassic Lagerstätte fossils, the researchers concluded that marine ecosystems recovered quickly from the end-Permian extinction, re-establishing complete food chains within one million years of the mass extinction. The researchers propose that this diverse group of organisms thrived during a cold period in the warming Triassic environment. The researchers suggest that future researchers should examine whether a short period of cool weather allowed these organisms to survive the heat, or whether other factors, such as favorable ocean chemistry, were involved.


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Source: sciworthy.com

The correct and incorrect way to pet a cat

Wondering how to best pet a cat? The answer might surprise you. Although petting is often considered a bonding activity, not all cats enjoy it.

As Dr. Lauren Finca, a cat behavior expert from Nottingham Trent University, explains: “While some cats may like being petted, most cats may not be thrilled with our typical petting methods. Cats tolerate petting due to the positive relationship with their owners, including treats, food, and affection.”

“Cats are not naturally social or tactile animals, so when it comes to petting, it’s important to keep in mind their preferences,” advises Finca.

It’s essential to pay attention to your cat’s body language to understand their comfort levels with petting. Avoid areas like the lower back and belly, as touching these spots can make cats feel threatened due to their exposed vital organs.

According to Finca, early socialization and handling play a significant role in a cat’s tolerance for petting. Each cat’s preferences may vary, so it’s crucial to observe their reactions and adjust accordingly.

A cat displaying positive body language (notice the raised tail) © Getty

Watch out for signs of negative arousal in cats, such as turning away, freezing, or abrupt grooming behaviors. Cats may subtly communicate their discomfort through tail movements, ear positions, or body language.

What’s the best way to pet a cat?

When petting a cat, focus on areas like the cheeks, chin, and base of the ears, where cats enjoy being touched. Look for signs of positive excitement like purring, rubbing, and tail wagging to ensure your cat is comfortable.

Remember Dr. Finca’s guidelines for petting, known as CAT:

  • C: Give your cat choice and control during interactions, allowing them to approach you for petting.
  • A: Pay attention to your cat’s behavior and body language to recognize signs of discomfort or the need for a break.
  • T: Think about where you’re touching the cat, focusing on areas they enjoy and avoiding sensitive spots like the tail and belly.

By following these guidelines, you can ensure a positive petting experience for both you and your feline friend.

About Dr. Lauren Finca

Dr. Lauren Finca is a feline behavior expert at Nottingham Trent University with over a decade of experience in cat research. She collaborates with organizations like Battersea Dogs and Cats Home, ICatCare, and ISFM on various behavioral and welfare projects.

Source: www.sciencefocus.com

Science debunks 7 common myths about your reality

Our perception of reality is quite limited because we evolved on the African plains 3 million years ago. Our senses were shaped to help us survive in that environment, with eyes that can detect approaching predators and ears that can hear the rustling of grass.

Although our senses have given us a basic understanding of the world, they also deceive us at times. The majority of nature remains hidden from us, and things are not always as they appear.

Here are a few examples of things that seem obvious but are not necessarily true:

1. The Earth is flat

Many ancient peoples believed the Earth was a disk. – Photo credit: Alamy

While the Earth may appear flat, evidence such as ships disappearing over the horizon and the curved shadow of the Earth on the Moon during a lunar eclipse point to its spherical nature. Observations like the first circumnavigation of the globe also support the round Earth theory.

Proving the Earth’s size involved measurements and calculations, with early estimates by Eratosthenes aligning closely with modern figures.

2. The stars revolve around the Earth

It may seem logical that stars move around a stationary Earth, but evidence such as artillery deviations and the Foucault pendulum disproves this. The invention of the pendulum provided physical proof of the Earth’s rotation.

3. Living things are designed to suit their habitats

The apparent design in nature is often attributed to mutations and natural selection rather than intentional design. DNA plays a crucial role in the adaptation of organisms to their environments.

4. Your time is the same as everyone else’s

Speeds close to the speed of light and strong gravitational fields (such as near a black hole) distort time. – Photo credit: Science Photo Library

The concept of time is influenced by speed and gravity, as demonstrated by Einstein’s theories. Time dilation occurs in different gravitational fields, impacting the flow of time.

5. The moon won’t fall

Newton’s insights about gravity and orbital mechanics explain why the moon stays in orbit rather than falling to the Earth. Objects in free fall experience weightlessness due to the effect of gravity.

6. Stars are tiny dots on the celestial sphere

The Milky Way galaxy contains over 100 billion stars. – Photo credit: Getty

The apparent size of stars is deceiving, with parallax observations revealing their true distance and magnitude. Spectral analysis further confirms the nature of stars as distant suns.

7. We can know what the universe is like “now”

The concept of “now” is complex in a universe where light travels slowly through vast distances. Observations of distant objects reflect their past states, allowing us to study the history of the universe but not its current state.

Source: www.sciencefocus.com

You may be lacking in fiber intake, which could accelerate aging

Research indicates that a lack of dietary fiber may result in accelerated brain aging, potentially contributing to the prevalence of Alzheimer’s disease and dementia. Expert nutritionists, such as Dr. Emily Leeming and Nutritional Psychologist Kimberly Wilson, presented this theory at the Cheltenham Science Festival.

In fact, dementia, a condition characterized by memory loss, is described as a model of accelerated brain aging by Wilson. This highlights the importance of dietary fiber for brain health and overall well-being.

Most adults in the UK are not consuming enough fiber, falling short of the recommended intake of 30g per day for optimal health. This deficiency poses a risk factor for various health conditions, including cognitive decline and neurodegenerative diseases.

According to Leeming and Wilson, consuming fiber-rich foods is essential for brain protection. Fiber is metabolized by gut bacteria, producing short-chain fatty acids that play a crucial role in maintaining the integrity of the blood-brain barrier. These fatty acids help prevent the passage of harmful substances into the brain.

If you are not getting enough fiber in your diet, Leeming suggests incorporating fiber-rich foods like rye bread, beans, nuts, and vegetables. Additionally, consuming dark chocolate and root vegetables with the skin on can help boost your fiber intake.

By increasing fiber consumption, individuals can support their gut health, manage blood sugar levels, and reduce the risk of chronic diseases. Leeming and Wilson emphasize the importance of fiber for overall health and well-being.

Our experts, Kimberly Wilson and Dr. Emily Leeming, have extensive experience in nutrition and psychology, respectively. Wilson is a licensed psychologist and author, while Leeming is a Registered Dietitian and Research Fellow with a focus on the gut microbiome.

Source: www.sciencefocus.com

Study indicates that Earth’s inner core started decelerating in 2010

The movement of Earth’s inner core has been a topic of debate in the scientific community for the past 20 years, with some studies suggesting that the inner core rotates faster than the Earth’s surface. However, a new study has presented clear evidence that the inner core started to slow down around 2010 and is now moving at a slower pace compared to the Earth’s surface.

king othersIt shows that Earth’s inner core gradually super-rotated from 2003 to 2008, then repeated a slower rotation 2-3 times along the same path from 2008 to 2023. Image by USC Graphic/Edward Sotelo.

“When I first saw the earthquake records suggesting this change, I was puzzled,” said John Bedale, a professor at the University of Southern California.

“But when we found 24 more observations showing the same pattern, the result was inevitable.”

“The inner core is slowing down for the first time in decades.”

“Other scientists have recently proposed similar or different models, but our latest work offers the most plausible solution.”

The inner core is believed to be rotating and moving relative to the Earth’s surface, as it is now moving slightly slower than Earth’s mantle after about 40 years of moving faster.

Compared to the rates observed over the past few decades, the inner core is now slowing down.

The inner core is a solid iron-nickel sphere surrounded by a liquid iron-nickel outer core.

Located more than 4,828 km (3,000 miles) beneath the Earth’s surface, the inner core is roughly the size of the Moon and poses a challenge for researchers as it cannot be visited or directly observed.

Scientists rely on seismic waves from earthquakes to study the movement of the inner core.

In contrast to previous studies, Professor Vidale and his team used waveforms and repeating earthquakes in their research.

Repeating earthquakes are seismic events that occur in the same location and produce identical earthquake records.

The study analyzed recorded seismic data from 121 repeating earthquakes around the South Sandwich Islands between 1991 and 2023, as well as data from Soviet and nuclear tests from the early 1970s and other studies on the inner core.

“The slowing down of the inner core is attributed to the churning of the liquid iron outer core that surrounds it. This churning creates a gravitational pull from the Earth’s magnetic field and the dense region of the rocky mantle above,” Prof Vidale explained.

“We can only speculate on how these changes in the inner core’s movement will impact the Earth’s surface.”

“The retreat of the inner core could briefly alter the length of the day. This alteration lasts for milliseconds and is almost imperceptible amid the noise of the ocean and atmosphere,” he added.

The study was published in the journal Nature.

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Wang others Retrograde motion of the inner core due to reversal of seismic waveform changes. Nature. Published online June 12, 2024, doi: 10.1038/s41586-024-07536-4

Source: www.sci.news

NASA successfully restores Voyager 1 spacecraft to regular scientific operations

Voyager 1 Due to technical issues, scientific observations are being carried out for the first time. Happened November 2023.

Voyager 1 launched from NASA's Kennedy Space Center in Florida on September 5, 1977, 16 days after its twin, Voyager 2. This artist's concept drawing depicts one of NASA's twin Voyager spacecraft. Image courtesy of NASA/JPL-Caltech.

Voyager 1 stopped transmitting readable science and engineering data to Earth on November 14, 2023, even though mission controllers were able to confirm that the spacecraft was still receiving commands and was otherwise operating normally.

In April 2024, they prompted Voyager 1 to begin transmitting engineering data containing information about the spacecraft's health and condition, partially resolving the problem.

On May 19, they carried out the second stage of the repair process and sent commands to the spacecraft to begin transmitting science data.

Two of the four scientific instruments immediately returned to normal operating mode.

The other two instruments required additional work, but all four are now returning usable science data.

The four instruments will study plasma waves, magnetic fields and particles.

This infographic highlights major milestones of NASA's Voyager missions, including visiting four outer planets and escaping the heliosphere, a protective bubble of magnetic fields and particles generated by the Sun. Image courtesy of NASA/JPL-Caltech.

The twin Voyager probes are NASA's longest-serving missions and the only spacecraft to have explored interstellar space.

Launched in 1977, both probes traveled to Jupiter and Saturn, with Voyager 1 traveling faster and reaching Jupiter and Saturn first.

Together, they have revealed a lot about the solar system's two largest planets and their moons.

Voyager 1 is more than 24 billion km (15 billion miles) from Earth, and Voyager 2 is more than 20 billion km (12 billion miles) from Earth.

The probe will celebrate its 47th anniversary of operation later this year.

“Voyager 1 and 2 are the only spacecraft to directly sample interstellar space, the region outside the heliosphere – the protective bubble of magnetic fields and solar wind created by the Sun,” NASA engineers said.

“Voyager 1 has resumed science, but additional minor operations are required to remove the effects of the problem.”

“Among other tasks, we will resynchronize the timing software in the spacecraft's three onboard computers to ensure commands are executed at the right time.”

“We will also be maintaining the digital tape recorder that records the plasma wave instrument data that is sent back to Earth twice a year.”

Source: www.sci.news

Quantum entanglement used by physicists to measure Earth’s rotation

Physicists at the University of Vienna have used a maximally entangled quantum state of light paths in a large interferometer to experimentally measure the speed of the Earth’s rotation.

Silvestri othersThey have demonstrated the largest and most precise quantum-optical Sagnac interferometer to date, sensitive enough to measure the Earth’s rotation rate. Image courtesy of Marco Di Vita.

For over a century, interferometers have been key instruments for experimentally testing fundamental physical questions.

They disproved the ether as a light-transmitting medium, helped establish the theory of special relativity, and made it possible to measure tiny ripples in space-time itself known as gravitational waves.

Recent technological advances allow interferometers to work with a variety of quantum systems, including electrons, neutrons, atoms, superfluids, and Bose-Einstein condensates.

“When two or more particles are entangled, only the overall state is known; the states of the individual particles remain uncertain until they are measured,” said co-first author Dr. Philip Walther and his colleagues.

“Using this allows us to get more information per measurement than we would without it.”

“But the extremely delicate nature of quantum entanglement has prevented the expected leap in sensitivity.”

For their study, the authors built a large fiber-optic Sagnac interferometer that was stable with low noise for several hours.

This allows the detection of entangled photon pairs with a sufficiently high quality to exceed the rotational precision of conventional quantum-optical Sagnac interferometers by a factor of 1000.

“In a Sagnac interferometer, two particles moving in opposite directions on a rotating closed path reach a starting point at different times,” the researchers explained.

“When you have two entangled particles, you get a spooky situation: they behave like a single particle testing both directions simultaneously, accumulating twice the time delay compared to a scenario where no entanglement exists.”

“This unique property is known as super-resolution.”

In the experiment, two entangled photons propagated through a 2 km long optical fiber wound around a giant coil, creating an interferometer with an effective area of ​​more than 700 m2.

The biggest hurdle the team faced was isolating and extracting the Earth’s stable rotation signal.

“The crux of the problem lies in establishing a measurement reference point where light is not affected by the Earth’s rotation,” said Dr Raffaele Silvestri, lead author of the study.

“Since we can’t stop the Earth’s rotation, we devised a workaround: split the optical fiber into two equal-length coils and connect them through an optical switch.”

“By switching it on and off, we were able to effectively cancel the rotation signal, which also increased the stability of larger equipment.”

“We’re basically tricking light into thinking it’s in a non-rotating universe.”

The research team succeeded in observing the effect of the Earth’s rotation on a maximally entangled two-photon state.

This confirms the interplay between rotating reference systems and quantum entanglement, as described in Einstein’s special theory of relativity and quantum mechanics, and represents a thousand-fold improvement in precision compared to previous experiments.

“A century after the first observations of the Earth’s rotation using light, this is an important milestone in that the entanglement of individual quanta of light is finally in the same region of sensitivity,” said co-first author Dr Haokun Yu.

“We believe that our findings and methods lay the foundation for further improving the rotational sensitivity of entanglement-based sensors.”

“This could pave the way for future experiments to test the behaviour of quantum entanglement through curves in space-time,” Dr Walther said.

Team work Published in a journal Scientific advances.

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Raffaele Silvestri others2024. Experimental Observation of Earth’s Rotation through Quantum Entanglement. Science Advances 10(24); doi: 10.1126/sciadv.ado0215

Source: www.sci.news

Realigning the UK’s Climate Strategy: Strategies for the Next Government

Climate activists protest outside the Houses of Parliament in London in March.

Andrea Domeniconi/Alamy

This week, more than 400 climate scientists from UK research institutes published an open letterAhead of the general election on 4 July, he called on UK political parties to commit to stronger climate action in the next Parliament.

Their demands included a “credible” carbon reduction strategy for the country, during an election campaign where there has been little in-depth discussion about the UK's transition to net zero.

Why are scientists worried? After all, the UK has one of the most ambitious climate targets in the world – a legally binding target to reach net-zero emissions by 2050 – and has halved its greenhouse gas emissions since 1990.

But the truth is that the UK's race to net zero has slowed in recent years, with annual emissions Half the rate needed to achieve the intermediate goal.

While great progress has been made in decarbonizing the electricity supply, with around half of all electricity now generated from zero-carbon sources, other sectors are lagging behind. The Committee on Climate Change, the UK government's climate advisers, say that outside the electricity sector, the rate of emissions reductions needs to quadruple over the next seven years for the UK to meet its commitment to cut emissions by 68% by 2030. I said in OctoberHe warned it was “unlikely” the UK would get there under current plans.

“There's a real sense of frustration in the climate science community,” he said. Emily Schuckberg “We are yet to see the level of response that is required,” said a Cambridge University researcher who co-authored the scientists' letter.

The slow progress means problems are piling up, waiting for the next administration to tackle them.

Transportation and Buildings

By the end of the decade, emissions from surface transport – roads, rail and ships – need to fall by around 4 million tonnes of carbon dioxide equivalent, four times the rate of reduction over the past decade. Electric car sales may be growing strongly, but sales of electric vans and trucks are sluggish, and the number of public charging points is not growing fast enough to keep up with the volume of electric vehicles travelling. Meanwhile, public transport use has fallen sharply during the COVID-19 pandemic, It's not back to the previous level.

Getting the transport sector to net zero will require more than just convincing everyone to buy electric cars, Michael Pollitt The Cambridge researchers say that reducing the number and size of cars is a key part of the puzzle. “We need more…and electric vehicles.

When it comes to buildings, home heating is the biggest pain point. Around 23 million homes in the UK are heated by gas boilers. By the middle of the century, all of these homes will need to be heated with zero-carbon energy sources, and it is expected that most will switch to heat pumps.

But the pace of the transition is too slow: just 69,000 heat pumps will be installed in UK homes in 2022, far short of the target of 600,000 per year by 2028. Part of…addition, increasing the affordability and efficiency of heat pumps will be crucial for decarbonizing home heating.

It is urgent to solve these problems. Nick Air One Oxford professor who signed the open letter said that a gas boiler installed in 2035 would still be heating homes in 2050. “For heat pumps and cars, we need to be pretty much sorted by the early 2040s, which means we need to get very serious about it in the 2030s,” he said.

That's why the UK government's inaction over the last decade, when it should have been focusing on preparing industry for mass adoption, is so worrying.

Agriculture and Aviation

Beyond heat, power and transport, tougher choices lie ahead. For example, emissions from agriculture and land use have remained almost unchanged for a decade, but need to be reduced by 29% by 2035. Achieving these reductions will likely require actions…

“The biggest challenge is starting to implement policies and regulations that will affect people's daily lives.” Leo Mercer “If policies are not communicated well, people will react quite strongly,” said the professor at the London School of Economics.

Alongside its domestic challenges, the UK needs to rebuild its reputation on the international stage: under former Prime Minister Boris Johnson, the UK hosted the COP26 climate summit and led international coalitions on deforestation, methane and electric vehicles.

However, progress on climate change measures in the UK has slowed, cuts in international aid and climate diplomacy; Britain's international reputation has suffered, and the government's decisions to approve new fossil fuel projects in the UK while urging lower-income countries to “move away” from fossil fuels have also antagonized the British public.

Unless a country like the UK can demonstrate that net zero is achievable and desirable as a national strategy, it will face an uphill battle to persuade lower-income countries to cut emissions, which is why it is crucial the UK restores its reputation as a climate leader in the next parliament, he says.

Next year, countries are due to submit new commitments under the Paris Agreement to reduce greenhouse gas emissions by 2035. “So this is a pivotal moment for the international community,” she said. “This parliament will be crucial…cing in the 2030s,” he said.

What each party is proposing

So which party can take action on the scale needed to get the UK back on track? All the major parties agree on the need to reach net zero by mid-century, and Labour and the Conservatives are remarkably in agreement on the need for renewable energy, particularly offshore wind.

But Labour has made an eye-catching promise to deliver a fully decarbonised electricity grid by 2030. Adam Bell A former senior UK government official at Stonehaven, a British consultancy, said the target was “highly ambitious” and would push government agencies to the limits of their capabilities. [Labour] It could be even more ambitious.”

But for Eyre, a credible climate manifesto should also include ambitious targets in the areas where the UK is seriously off track: home energy efficiency, heat pump adoption, industrial emissions, land use, solar power and electric vehicles. “It's not a matter of doing one or two of them,” Eyre says. “We need to do them all.”

Many experts privately doubt that the major parties have policy programmes with the pace and scale needed to get to net zero by 2050. Absent that, looking for enthusiasm for the challenges ahead may be the next best way to gauge a party's credibility. In Eyre's eyes, the next UK government is embarking on a “10-year plan on the scale of the introduction of the steam engine.” “If you don't have a positive vision yourself, you're not going to sell it to the public,” he says.

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Source: www.newscientist.com

Amazing Discovery: JWST Uncovers Abundance of Supernovae in Early Universe

Many of the circled objects represent previously unknown supernovae.

Collaboration between NASA, ESA, CSA, STScI and JADES

Astronomers using the James Webb Space Telescope (JWST) have discovered a surprising number of supernovae in the distant universe, including some of the most distant yet seen. Their discoveries increase the number of known supernovae in the early universe by a factor of ten.

The researchers imaged the same small patch of sky twice, in 2022 and 2023, and found 79 new supernovae. “It’s actually very small, about the size of a grain of rice held at arm’s length,” the researchers said. Christa DeCourcy “We’ve spent more than 100 hours on JWST,” said Dr. [observing] I took my time with each image, which gives them a lot of depth.”

Astronomers then compared the two images with each other and with previous photos of the same area taken by the Hubble Space Telescope, looking for bright spots that appear in one image but not the other.

These specks are relatively faint stars that shone brightly before fading in bright supernova explosions. Some of them are candidates for the most distant supernovae ever found, although their distances have yet to be confirmed. And one of them is definitely the most distant one ever seen. This star exploded when the universe was only about 1.8 billion years old.

Such supernovae would have produced the heavy elements that are now widespread throughout the universe, so they would have had lower concentrations of these elements than modern supernovae. “The universe at this early stage was fundamentally different from what has been explored in the past by the Hubble Space Telescope and especially ground-based surveys,” he said. Justin Pierre “This is really new territory that JWST is breaking into,” he said during a presentation at the Space Telescope Science Institute in Maryland, where observations could help shed light on what the first stars were like.

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  • Performer/
  • James Webb Space Telescope

Source: www.newscientist.com

UK election: Realigning the next government’s climate strategy for success

Climate activists protest outside the Houses of Parliament in London in March.

Andrea Domeniconi/Alamy

This week, more than 400 climate scientists from UK research institutes published an open letterAhead of the general election on 4 July, he called on UK political parties to commit to stronger climate action in the next Parliament.

Their demands included a “credible” carbon reduction strategy for the country, during an election campaign where there has been little in-depth discussion about the UK's transition to net zero.

Why are scientists worried? After all, the UK has one of the most ambitious climate targets in the world – a legally binding target to reach net-zero emissions by 2050 – and has halved its greenhouse gas emissions since 1990.

But the truth is that the UK's race to net zero has slowed in recent years, with annual emissions Half the rate needed to achieve the intermediate goal.

While great progress has been made in decarbonizing the electricity supply, with around half of all electricity now generated from zero-carbon sources, other sectors are lagging behind. The Committee on Climate Change, the UK government's climate advisers, say that outside the electricity sector, the rate of emissions reductions needs to quadruple over the next seven years for the UK to meet its commitment to cut emissions by 68% by 2030. I said in OctoberHe warned it was “unlikely” the UK would get there under current plans.

“There's a real sense of frustration in the climate science community,” he said. Emily Schuckberg “We are yet to see the level of response that is required,” said a Cambridge University researcher who co-authored the scientists' letter.

The slow progress means problems are piling up, waiting for the next administration to tackle them.

Transportation and Buildings

By the end of the decade, emissions from surface transport – roads, rail and ships – need to fall by around 4 million tonnes of carbon dioxide equivalent, four times the rate of reduction over the past decade. Electric car sales may be growing strongly, but sales of electric vans and trucks are sluggish, and the number of public charging points is not growing fast enough to keep up with the volume of electric vehicles travelling. Meanwhile, public transport use has fallen sharply during the COVID-19 pandemic, It's not back to the previous level.

Getting the transport sector to net zero will require more than just convincing everyone to buy electric cars, Michael Pollitt The Cambridge researchers say that reducing the number and size of cars is a key part of the puzzle. “We need more radical thinking about intercity transport, including prioritising lanes for small vehicles and dramatically reducing the size and weight of vehicles,” they say. “If people can travel in significantly smaller cars and public transport, that's the route to net-zero transport.”

When it comes to buildings, home heating is the biggest pain point. Around 23 million homes in the UK are heated by gas boilers. By the middle of the century, all of these homes will need to be heated with zero-carbon energy sources, and it is expected that most will switch to heat pumps.

But the pace of the transition is too slow: just 69,000 heat pumps will be installed in UK homes in 2022, far short of the target of 600,000 per year by 2028. Part of the problem is finances: heat pumps are much more expensive to install than gas boilers, and they are often more expensive to run as well, due to an additional levy on grid costs. “We absolutely have to get the price of heat pumps down,” Porritt says. “Unless the price of heat pumps comes down significantly, they will be a major obstacle to decarbonising heating.”

It is urgent to solve these problems. Nick Air One Oxford professor who signed the open letter said that a gas boiler installed in 2035 would still be heating homes in 2050. “For heat pumps and cars, we need to be pretty much sorted by the early 2040s, which means we need to get very serious about it in the 2030s,” he said.

That's why the UK government's inaction over the last decade, when it should have been focusing on preparing industry for mass adoption, is so worrying. “We know what needs to be done,” Eyre says, “but the last two years in particular have been a period of no real action being taken.”

Agriculture and Aviation

Beyond heat, power and transport, tougher choices lie ahead. For example, emissions from agriculture and land use have remained almost unchanged for a decade, but need to be reduced by 29% by 2035. Achieving these reductions will likely require actions to change the way people eat. Similarly, reducing aviation emissions will require actions to curb demand, such as taxes on frequent flyers.

“The biggest challenge is starting to implement policies and regulations that will affect people's daily lives.” Leo Mercer “If policies are not communicated well, people will react quite strongly,” said the professor at the London School of Economics.

Alongside its domestic challenges, the UK needs to rebuild its reputation on the international stage: under former Prime Minister Boris Johnson, the UK hosted the COP26 climate summit and led international coalitions on deforestation, methane and electric vehicles.

However, progress on climate change measures in the UK has slowed, cuts in international aid and climate diplomacy; Britain's international reputation has suffered, and the government's decisions to approve new fossil fuel projects in the UK while urging lower-income countries to “move away” from fossil fuels have also antagonized the British public.

Unless a country like the UK can demonstrate that net zero is achievable and desirable as a national strategy, it will face an uphill battle to persuade lower-income countries to cut emissions, which is why it is crucial the UK restores its reputation as a climate leader in the next parliament, he says. Katerina Brandmeyer At Imperial College London.

Next year, countries are due to submit new commitments under the Paris Agreement to reduce greenhouse gas emissions by 2035. “So this is a pivotal moment for the international community,” she said. “This parliament will be crucial not only to ensuring delivery in the UK, but also to raising ambition globally.”

What each party is proposing

So which party can take action on the scale needed to get the UK back on track? All the major parties agree on the need to reach net zero by mid-century, and Labour and the Conservatives are remarkably in agreement on the need for renewable energy, particularly offshore wind.

But Labour has made an eye-catching promise to deliver a fully decarbonised electricity grid by 2030. Adam Bell A former senior UK government official at Stonehaven, a British consultancy, said the target was “highly ambitious” and would push government agencies to the limits of their capabilities. [Labour] It could be even more ambitious.”

But for Eyre, a credible climate manifesto should also include ambitious targets in the areas where the UK is seriously off track: home energy efficiency, heat pump adoption, industrial emissions, land use, solar power and electric vehicles. “It's not a matter of doing one or two of them,” Eyre says. “We need to do them all.”

Many experts privately doubt that the major parties have policy programmes with the pace and scale needed to get to net zero by 2050. Absent that, looking for enthusiasm for the challenges ahead may be the next best way to gauge a party's credibility. In Eyre's eyes, the next UK government is embarking on a “10-year plan on the scale of the introduction of the steam engine.” “If you don't have a positive vision yourself, you're not going to sell it to the public,” he says.

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Source: www.newscientist.com

The Dangers of Overlooked Fatigue on Your Sleep and Ways to Combat It

You’ve probably experienced this scenario before: after a long day, feeling mentally and physically drained, all you want to do is crawl into bed and sleep.

However, your brain, the most powerful biological supercomputer in the universe, decides to play tricks on you. Instead of allowing you to rest, it keeps you wide awake, with thoughts racing through your mind at lightning speed.

So why does this happen? Why does it prevent us from sleeping when we need it the most? The answer is simple: when you’re too tired, your brain overrides the signals for sleep and keeps you awake.

If you’ve heard of being “over-fatigued” before, it’s often used to describe babies who become agitated and unsettled from being awake too long, leading to sleep disturbances and stress.

Similarly, adults can experience the same issues when unaddressed emotions interfere with the body’s natural sleep processes. The longer you stay fatigued, the more challenging it becomes to fall asleep.

Fortunately, there are ways to break this cycle. In the sections below, we’ll explore what causes excessive fatigue and share three scientifically proven steps to combat it for good.


Excessive fatigue impacts your sleep quality

Being overly tired is a paradoxical situation. When you’re physically and mentally drained, your brain is actually overstimulated and in a state of hyperarousal, making it difficult to transition to sleep.

This hyperarousal state affects essential functions that promote sleep, particularly hindering the buildup of sleep pressure in the brain.

Sleep pressure refers to the buildup of neurochemicals and hormones that increase throughout the day, signaling your body’s need for rest.

“Interestingly, as sleep pressure rises, the brain can become more excitable,” explains Professor Matt Jones, a Neuroscientist at the University of Bristol. “The neurons in the cerebral cortex tend to fire more frequently as wakefulness increases.”

“The primary theory is that sleep helps reset sleep pressure, preventing the brain from becoming overly excited and metaphorically ‘exploding!'”

When you’re vigilant and overwhelmed by racing thoughts, this process of resetting the brain for sleep is disrupted, particularly impacting the locus ceruleus area in the brainstem.

“In times of hyperarousal, the activity in this brain region remains high, impeding the transition to sleep and resisting mechanisms that facilitate falling asleep,” Jones clarifies.

Furthermore, persistent fatigue and sleep deprivation can exacerbate troubling thoughts, making it harder to sleep the following night.

“A study in 2019 found that individuals with insomnia were more likely to ruminate about recent embarrassing events and have disrupted sleep compared to healthy sleepers,” he explains.

“Insomniacs might even become hypersensitive to their heartbeat, showing how an unrested brain struggles to ignore irrelevant stimuli,” Jones adds.

“A well-rested brain can filter out unnecessary information, but insomnia disrupts this process, leading to increased mental strain,” he concludes.

©Getty

Strategies to prevent excessive fatigue

When you’re too tired and key brain regions remain hyperaroused while trying to sleep, essential processes for rest are disrupted.

Dr. Alex Scott, a Psychology lecturer at Keele University, explains that in today’s society, people struggle to regulate their emotions and process daily experiences effectively due to various distractions.

“At the end of the day, we are less inclined to deal positively with our emotions, often exaggerating worries and ruminating in bed,” he shares.

Scott suggests that when fatigued, individuals tend to use unhealthy coping mechanisms, like rumination and blame-shifting.

If rumination proves ineffective for alleviating fatigue, Scott recommends the following three strategies:

1. Avoid counting sheep

Paradoxically, trying too hard to fall asleep can make it even harder. Instead of using traditional methods like counting sheep, Scott encourages individuals to understand that sleep is an automated process that cannot be forced.

“Focus on processing your emotions through exercises like a worry journal,” Scott advises.

2. Maintain a worry diary

Although it may seem tedious, journaling your worries can significantly improve sleep quality for those with sleep issues, according to Scott.

Before bedtime, write down all your concerns in a journal, allowing you to acknowledge them and develop strategies to address them the next day.

“The act of writing down your worries may help you rationalize them and temporarily set them aside, promoting better sleep,” Scott explains.

3. Establish a bedtime routine

Creating a relaxation routine before bed, ideally starting an hour before sleep, can help alleviate mental fatigue and prepare your mind for rest.

“Engage in activities like reading, mindfulness, or journaling during this time to unwind and avoid associating your bed with worries,” Scott suggests.

Learn more about our experts

Professor Matt Jones: A Neuroscientist at the University of Bristol, delving into the science of sleep, memory, and decision-making. His research has been featured in numerous academic journals, such as Frontiers in Neurology, Sleep, and the Neuroscience Journal.

Dr. Alex Scott: As a Psychology lecturer at Keele University, Scott explores the relationship between sleep and mental health issues. His work has been published in esteemed journals like the British Journal of Health Psychology and the British Medical Journal.

Source: www.sciencefocus.com

Astronomers find parallel jets and disks around nearby multiple star system

Astronomers Atacama Large Millimeter/Submillimeter Array (ALMA) Mid-infrared measuring instrument (mm) NASA/ESA/CSA James Webb Space Telescope A twin disk and parallel jets were discovered in the young star system WL20.

Barsoni othersTwin disks and jets erupting from a pair of young stars in WL20. Image credit: NSF / NRAO / B. Saxton / NASA / JPL-Caltech / Harvard-Smithsonian CfA.

WL20 It is located in the Rho Ophiuchus Molecular Cloud Complex, more than 400 light years from Earth.

“What we found was absolutely surprising,” said Dr Mary Barthony, lead author of the study.

“We've known about the WL20 system for some time, but what caught our attention was that one of the stars in the system appeared to be much younger than the others.”

“Using MIRI and ALMA together, we were able to see that this one star is actually two stars next to each other.”

“Each of these stars was surrounded by a disk, and each disk emitted a jet parallel to the others.”

ALMA and Webb's MIRI observe very different parts of the electromagnetic spectrum.

Used together, they allowed astronomers to discover these hidden twins in the stellar system's radio and infrared wavelengths: ALMA found the disk, and MIRI found the jet.

They analyzed archived ALMA data to reveal the composition of the disk, and MIRI data to reveal the chemical composition of the jet.

They also analyzed high-resolution images, revealing the size of the massive disk – about 100 times the distance between Earth and the Sun.

“Without MIRI we would never have known these jets even existed, which is amazing,” Dr Barthony said.

“ALMA's high-resolution observations of the disks surrounding the two newly observed stars reveal the structure of the disks.”

“Someone looking at this ALMA data and not knowing there are twin jets would think it's a big edge-on disk with a hole in the middle, rather than two edge-on disks and two jets. That's pretty remarkable.”

Combining multi-wavelength data from ALMA and Webb revealed the complex processes involved in the formation of several stellar systems.

“We plan to take advantage of ALMA's future upgrades, such as the broadband sensitivity upgrade, to continue unlocking the mysteries surrounding the birth of stars and planetary systems,” the researchers said.

They are, result in 244th Meeting of the American Astronomical Society In Madison, Wisconsin.

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Mary Barthony others2024. Twin jets and twin discs: JWST MIRI and ALMA discoveries in the young WL20 multiple star system. 224 AustraliaAbstract #253

Source: www.sci.news

FDA advises updating COVID-19 vaccine to target KP.2 variant

The Food and Drug Administration on Thursday recommended that pharmaceutical companies develop coronavirus vaccines targeting the KP.2 strain, a descendant of the highly contagious JN.1 variant that began spreading widely in the United States this winter. The announcement comes just one week after an FDA advisory committee unanimously recommended updating COVID-19 vaccines in the fall to target the JN.1 variant or its descendants.

After the vote, there was disagreement between committee members and Dr. Peter Marks, the agency’s top vaccine regulator, over which strain the agency should choose. Most committee members expressed a preference for JN.1, but Dr. Marks favored choosing a newer strain like KP.2. “We’re paying an incredibly high premium for the mRNA vaccines to get the freshest vaccine,” Marks said, likening getting the vaccine to buying milk at the store.

The FDA said it had initially advised drugmakers on June 6 to target the JN.1 variant, but the agency continues to monitor circulating strains and “based on the latest available data and recent increases in COVID-19 cases in areas of the country, the FDA has further determined that the JN.1 lineage is preferred for improved vaccines,” with the KP.2 strain preferred “when possible,” the FDA said.

The JN.1 is hardly in circulation in the United States. Centers for Disease Control and Prevention As of Saturday, KP.2 accounted for 22.5% of new coronavirus cases in the U.S., while its sister variant, KP.3, accounted for 25% of new cases.

The FDA’s decision allows pharmaceutical companies to begin manufacturing and distributing the vaccine, which is expected to be used as part of COVID-19 vaccination campaigns this fall.

Three pharmaceutical companies, Pfizer, Moderna, and Novavax, are producing coronavirus vaccines. Pfizer and Moderna’s vaccines are mRNA-based, while Novavax’s vaccine is protein-based. Because protein-based vaccines take a long time to produce, Novavax has indicated that it will not be able to produce the KP.2 vaccine by the fall. Instead, it plans to distribute the JN.1 vaccine that it has already produced.

This is the third time the vaccine has been updated to target circulating strains. The process of selecting the next vaccine is becoming more routine, similar to the annual influenza vaccination update, with vaccinologists selecting the strains in the spring and then conducting vaccination campaigns in the fall.

At the advisory committee meeting, the pharmaceutical company presented data showing that compared to current vaccines that target the variant XBB.1.5, which is not currently in circulation, the JN.1 vaccine should generate higher levels of antibodies against circulating virus strains.

The committee did not recommend who should get the latest vaccine, leaving that to the CDC, which will be holding its own advisory committee meeting later this month.

Source: www.nbcnews.com

DeSantis Policies Impact Summer Weather

As summer approaches in the Northern Hemisphere, Florida is already facing extreme weather conditions. Storms have hit South Florida, bringing heavy rain and causing severe flooding in cities like Miami, Fort Lauderdale, and Sarasota. This comes after an early-season heatwave pushed temperatures above triple digits. All of this is happening as forecasters predict a particularly active hurricane season.

These events are all exacerbated by climate change, a reality that clashes with the current state politics in Florida. Governor Ron DeSantis has become known for his opposition to addressing climate change, with recent legislation deprioritizing climate change in the state’s energy policy. This goes against the scientific consensus that these extreme events are linked to climate change.

DeSantis has also signed bills that prevent cities and counties from implementing measures to protect against heat-related illnesses in the workplace. This leaves workers vulnerable as Florida faces a warmer-than-normal summer.

Experts argue that DeSantis’ policies are out of sync with climate science and hinder efforts to protect people from the impacts of climate change. The state’s refusal of federal funding for climate change initiatives further complicates efforts to address the issue.

While some Republicans are beginning to take climate change more seriously, it remains a divisive issue. Former President Donald Trump and DeSantis have downplayed the threat of climate change, aligning themselves with a stance that dismisses the urgency of addressing it.

Despite these challenges, climate change advisers stress the importance of taking action to protect communities from the impacts of global warming. It is crucial for states like Florida to prioritize mitigation measures to safeguard against the worsening effects of the climate crisis.

Source: www.nbcnews.com

Cooling fabric reduces heat transfer from pavements and buildings in urban areas with high temperatures

A scorching hot day in Bucharest, Romania, June 2019

lcv / Alamy

In the future, city dwellers could beat the heat with clothes made from new fabrics that keep them cool.

Made from plastic material and silver nanowires, the fabric is designed to keep you cool in urban environments by using the principle of radiative cooling, a natural process in which objects radiate heat back into space.

The material selectively emits a narrow band of infrared light that allows it to escape the Earth’s atmosphere, while at the same time blocking radiation from the sun and from surrounding structures.

Jo Bo-jun, a researcher from the University of Chicago, Illinois, and his team say the material “is more than half [the radiation]” from buildings and the ground,” he says.

Some cooling fabrics and building materials already use this radiative cooling principle, but most of their designs don’t take into account radiation from the sun or infrared radiation from structures like buildings and pavements, and they assume the materials are oriented horizontally against the sky, like roof panels, rather than vertically like clothing worn by a person.

Such designs “work well when they face something cooler, like the sky or a field,” Su says, “but not when they face an urban heat island.”

Xu and his colleagues designed a three-layered fabric: the inner layer is made from common clothing fabrics like wool or cotton, and the middle layer is made up of silver nanowires that reflect most of the radiation.

The top layer is made of a plastic material called polymethylpentene, which does not absorb or reflect most wavelengths and emits a narrow band of infrared light.

In outdoor tests, the fabric remained 8.9°C (16°F) cooler than regular silk fabric and 2.3°C (4.1°F) cooler than a broad-spectrum radiation-emitting material. When tested against the skin, the fabric was 1.8°C (3.2°F) cooler than cotton fabric.

Su said this slight difference in temperature could theoretically increase the amount of time a person can comfortably be exposed to heat by up to a third, but that this has yet to be tested.

“It’s always been difficult to make this material practical as a fiber.” Aswath Raman, the UCLA researcher added that the study is a good example of applying the physical principles of radiative cooling to a practical material. Other materials with similar properties could also be used on vertical surfaces in buildings, he said.

Science
DOI: 10.1126/science.adl0653

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Source: www.newscientist.com

Malaria drug shows promise in treating polycystic ovary syndrome

The malaria drug artemisinin is extracted from the plant wormwood.

Frederick J. Brown/AFP via Getty Images

A drug already used to treat malaria may also be effective in treating polycystic ovary syndrome (PCOS).

A small study of 19 women with PCOS found that the commonly used drug artemisinin improved menstrual cycle regularity and reduced high testosterone levels that are common in PCOS patients.

The underlying cause of PCOS is unknown, but it is linked to several hormonal imbalances, including excess testosterone produced by the ovaries, which can lead to symptoms like irregular menstrual periods, infertility, and increased acne and body hair.

Affected people also tend to have reduced sensitivity to insulin, the hormone that regulates sugar, which leads to weight gain and exacerbates the hormonal imbalance.

Currently, PCOS patients are treated individually depending on their symptoms, for example undergoing laser treatments to remove body hair or taking birth control pills to regularize menstruation.

While investigating the effects of various drugs on fat cells in mice, Chi Kun Tang Researchers at Fudan University in Shanghai, China, found that artemisinin reduced symptoms in mice with PCOS-like conditions.

His team then gave 19 women with PCOS artemisinin for three months and found that all of them experienced a drop in testosterone levels, and most also saw a reduction in another substance called anti-Müllerian hormone. Associated with PCOSTwelve of the participants also experienced more regular menstrual cycles after taking the drug.

In other studies using mouse and human cells, the team found that artemisinin could reduce testosterone production in the ovaries.

Stephen Franks The Imperial College London researcher says that although the 19 women had a healthy BMI on average, weight loss tends to reduce PCOS symptoms, suggesting that artemisinin may work through another mechanism: improving insulin sensitivity. “If the results are as positive in a randomized trial as they are in this pilot study, it would be exciting,” he says.

Elisabeth Stener-Victorin Researchers at the Karolinska Institutet in Stockholm, Sweden, say the fact that artemisinin is already generally safe when used to treat malaria means that it could soon be repurposed as a new treatment for PCOS.

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Source: www.newscientist.com

Australia Unearths New Flying Reptile Fossil

Australian paleontologists have discovered the fossilized skeleton of a previously unknown Anhangeria pterosaur, dating back 100 million years.

Reconstructing your life Haliskia petersenii Image courtesy of Gabriel N. Ugueto.

The newly identified pterosaur species lived in what is now northeastern Australia's state of Queensland during the Early Cretaceous period, about 100 million years ago.

Scientific Name Haliskia petersenii This flying reptile had a premaxillary crown and curved teeth.

It also had a long wingspan of about 4.6 metres (15.1 feet).

Haliskia petersenii “About 100 million years ago, when much of central-west Queensland was underwater and covered by a vast inland sea, and on Earth where the southern Victoria coastline is now, it would have been a fearsome predator,” said Adele Pentland, a PhD student at Curtin University.

Fossilized remains Haliskia petersenii Kevin Petersen, curator of the Kronosaurus Corner Museum, in November 2021 Toule back formation Of the Eromanga Basin.

Haliskia petersenii “The fossil is 22 per cent complete, more than twice as complete as the only other partial pterosaur skeleton found in Australia,” Mr Pentland said.

“The specimen includes a complete lower jaw, the tip of the upper jaw, 43 teeth, vertebrae, ribs, both wing bones and part of a leg.”

“There are also very thin and delicate throat bones present, indicating the presence of a muscular tongue, which would have been useful when eating fish and cephalopods.”

Pentland and colleagues Anhangeria is a group of pterosaurs known to have lived all over the world, including in what is now Brazil, Britain, Morocco, China, Spain, and the United States.

“The global nature of the Anhang-area pterosaurs, and in particular their success across Gondwana (e.g. in the Eromanga and Araripe basins), may have been made possible by niche partitioning within this clade,” the paleontologists said.

“However, rigorous testing of this hypothesis will require multiple locations and better time constraints.”

“Additional data on this clade are available Haliskia petersenii ” sheds light on the palaeoecology of Anhangeria pterosaurs and highlights the taxonomic diversity of these flying reptiles from the Cretaceous of Australia.”

Team paper Published in the journal Scientific Reports.

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A.H. Pentland others. 2024. Haliskia petersenii A new Anhangelian pterosaur that lived in the early Late Cretaceous of Australia. Scientific Reports 14, 11789; doi: 10.1038/s41598-024-60889-8

Source: www.sci.news

Researchers are releasing faux birds into simulated aircraft for study

Mid-air collision

To find out whether air taxi passengers need to worry about collisions with birds, a number of tests were carried out by a German emergency program.

Colliding a real air taxi with a real bird would be complicated and dangerous, so perfection was impossible, so experimenters made do by dropping artificial “bird bullets” onto a rigged metal plate that allowed them to measure the force of the impact.

Aditya Devta and Isabelle Metz of the German Aerospace Center and Sophie Armani of the Technical University of Munich described these violent encounters as follows: Preprint paper(Thanks to reader Mason Porter for pointing this out.)

This study was, necessarily, a rough step toward definitively answering the big questions.

The report said the bird shots were dropped manually and faced various challenges, including “inconsistency and lack of repeatability” due to human involvement. Future efforts should “eliminate human involvement and [so as to] “Improve the accuracy and repeatability of force measurements.”

Collision in the middle of the track

Speaking of experiments involving birds and flying taxis, have you heard of the moose and bullet train experiment? Yong Peng and his colleagues from Central South University in China began investigating what happens when these heavy animals meet at high speed.Analysis of moose movement trajectory after collision between bullet train and moose” “.

The questions go beyond the initial simple collision: the scientists mention two possible complications: “If the moose lies on the tracks after the collision, it could increase the risk of train derailment” and “if the moose is thrown into the air during the collision, it could strike and damage the pantograph, disrupting train operation.”

Previous investigations have relied on mathematical simulations using finite element methods and less-heavy experiments, using fresh beef muscle tissue (from cows, not elk) and a type of stress-strain testing machine called a “split-Hopkinson pressure bar.”

Essentially, the force of the impact “depends on the area of contact between the train and the moose,” the scientists report.

Regarding these complexities, the report states: “The moose will not be pushed aside by the V-shaped locomotive and derail, and the moose will not be thrown into the air to the height of the pantograph, causing no damage to the Shinkansen pantograph.”

The study suggests something bigger is on the way: “Only a scenario of a train crossing the tracks at 110km/h hitting a moose was simulated, which cannot fully reflect the risk of a train-moose collision. Therefore, further speeds and attitudes are needed to enhance ongoing research.”

Feeling cheeky

Slowly and gently, new findings about sources are coming in from readers. These concern the off-label use of ketchup and other sticky foods to make electrocardiogram (ECG) electrodes work better (Feedback, May 25).

Brian Leffin Smith adds a musical note: “You don’t need human skin to test whether ketchup electrodes are better than regular gel electrodes. I have equipment that applies a low voltage to plant leaves (or anything else) and converts the varying current into a MIDI signal that can be sent to a computer or synthesizer to play sounds… Anyway, in a statistically insignificant but anecdotally and culinarily interesting test, I found that low-salt ketchup placed between an ECG electrode and a chili leaf produced a fairly high E, while the proper gel placed on the adjacent leaf produced a G. I thought this might be useful, but now I don’t think so.”

Dave Hardy makes a point about practicality: “In the early 1970s, my GP said that gel was ridiculously expensive, but that strawberry jam would work just as well. I don’t know if he tried a range of options or just used what he had on hand (this was in the Falkland Islands).”

Death of a Star

It is surprising how few people are hailed as “famous pathologists.” news The paper reported on the death of one of them: “Dr. Cyril Wecht, the prominent pathologist who argued that more than one shooter killed JFK, has died at age 93.”

One of the first celebrated pathologists, Bernard Spilsbury (1877-1947), helped establish London’s reputation as a hotbed of fascinating and intricate murder mystery investigations.

Royal College of Physicians RevealedAfter his death, he said that Spilsbury’s career had been a truly dramatic one: “The famous Crippen trial in which he was involved [William] Wilcox’s attempts to prove that the murders were committed with hyoscine hydrobromide first attracted him to public attention, and he lamented it at every trial he subsequently attended, which no doubt accounted for his stern and cold demeanor towards all but his closest friends.

Spilsbury’s attitude was by no means contemptible. One aspect of the job of dissecting a corpse is the terrible stench of rotting bodies, which can put off sensitive people. Spilsbury was not a sensitive person in this respect. His colleagues were amazed at how enthusiastic he was about dissecting a corpse. Obituary To put it politely, it was an “olfactory disorder.”

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

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Neutron stars merging form heavy elements, scientists find

Since the 1920s, Edwin Hubble Ever since it was discovered that the universe is expanding, astrophysicists have been asking themselves the question, “Where does matter come from?” In the Big Bang theory, a possible explanation, not a TV show, astrophysicists propose that the universe began with an explosion, a single hot, dense point expanding, then cooling down to transform from pure energy into solid matter. But that origin story ends with the two smallest elements: hydrogen and helium. Not everything in the universe is made of these two elements, leaving scientists with a new question: “Where does other matter come from?”

The emergence of nuclear physics in the early 20th century gave astronomers their first big clue. Researchers studying stars noted that stars are very bright and require a large source of energy to produce that much light. Nuclear physicists, including Albert Einstein and his famous E = mc2 The equations showed that one of the most powerful sources of energy in the universe is the smashing of smaller atoms together to create larger ones – nuclear fusion. And that's exactly what stars do in the hot, dense regions at their centers, called “nuclear fusion.” coreBut there's a limit to this process in stars — specifically, iron, which is the 26th of the 92 naturally occurring elements. Stars create energy by colliding elements with each other, but elements bigger than iron need to generate more energy than they can give off, which is why elements heavier than iron, like gold and uranium, remain unexplained.

Researchers have discovered the next clue in a massive, bright stellar explosion in the night sky. SupernovaIt turns out that massive stars, more than 10 times the size of the Sun, burn up their accumulated elements to fuse rapidly. These stars not only shine, but also run out of energy to hold themselves together, exploding and scattering their outer layers of elements in all directions. This is a supernova explosion. For decades, astrophysicists thought that heavy elements were created from a chaotic mixture of light elements and free energy. However, careful observation of supernovae has shown that the amount of heavy elements produced in the explosion is less than what is needed to explain the abundance of heavy elements in the universe.

Astrophysicists got the final clue in 2017 when the Laser Interferometer Gravitational-Wave Observatory detected the first binary neutron star (BNS) merger. RaigoThe final stage in the life cycle of a massive star, between 10 and 25 times the mass of the Sun, is Neutron StarDuring this stage, the star's core collapses, and the electrons and protons in atoms get so close together that they fuse into neutrons. Two neutron stars orbiting each other collide, scattering debris into the surrounding galaxy. Researchers propose that this phenomenon could provide the energy and matter needed to fuse heavy elements into the heaviest naturally occurring elements.

Researchers from Peking University and Guangxi University wanted to test whether BNS mergers could produce elements heavier than iron. Because the event is extremely rare, occurring only a few dozen times per year across our galaxy, they couldn't just point their telescopes into space and hope for luck. Instead, they used advanced nuclear physics software to simulate a BNS merger.

The researchers gave their simulations specific initial conditions, such as what atoms were present in the stars when the collision began, the rates of nuclear reactions and decay, the number of electrons mixing, and the sizes of the colliding neutron stars. They then mathematically described how temperature, volume, and pressure relate to matter. Equation of stateIt simulates the effects of the collision and calculates what elements would be formed and released into space.

The team found that these BNS mergers could produce huge amounts of very heavy elements, between 300 and 30,000 times the mass of the Sun, which is 10 to 1,000 times the amount produced by supernovae. The team believes that this result could explain the abundance of heavy elements observed in the Galaxy in relation to other cosmic effects, e.g. Galactic WindHowever, the researchers acknowledged that their findings cannot explain the abundance of all heavy elements, especially those at the lower end of the atomic mass range they studied. They explained that these elements are probably still being created in the cores of collapsing stars, but suggested that future researchers should further test this hypothesis.


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Source: sciworthy.com

Accidental Broadcast of NASA Astronaut Medical Training

NASA had to reassure the public that there was no emergency on the International Space Station after audio from a medical training drill was mistakenly played during a livestream on Wednesday night.

The regularly scheduled livestream was interrupted at 6:28pm ET by an unidentified speaker, apparently a flight surgeon, communicating with the ISS crew about what to do for the commander, who was suffering from severe pressure illness.

The speaker advised crew members to “check the pulse again” before placing the injured astronaut in a spacesuit filled with pure oxygen. She said any treatment was “the best treatment” and better than nothing.

“Unfortunately, Commander's prognosis is relatively uncertain,” she said.

“I'm concerned that there are people with severe DCS,” she said. [decompression sickness] He “hits” and tells the crew to get him suited up as quickly as possible.

She mentions that there is a hospital in San Fernando, Spain, with a hyperbaric treatment facility, apparently implying that she would order an emergency evacuation of the space station.

But after stirring up fear among space enthusiasts listening in, NASA revealed that this scenario wasn't real: All crew members aboard the ISS were safely asleep at the time.

NASA said there was “no emergency on board the International Space Station.”

“At approximately 5:28 p.m. CDT, audio was broadcast on NASA's livestream from a ground-based simulated audio channel indicating the crew member was experiencing symptoms associated with decompression sickness,” NASA said in a statement. X's message.

“The audio was inadvertently transmitted from an ongoing simulation in which crew and ground teams were training for various scenarios in space and is not related to an actual emergency,” NASA said in a statement.

“The International Space Station crew was asleep at the time. All crew members are healthy and safe, and tomorrow's spacewalk will begin as scheduled at 8 a.m. EDT,” it added.

The emergency training came after two astronauts aboard Boeing's Starliner spacecraft successfully docked with the ISS last week.

Source: www.nbcnews.com

Shocking Revelation: The Dark Truth behind Mayan Human Sacrifice

The ancient Maya civilization of Central America has fascinated scholars for centuries with its incredible astronomical calendar and magnificent step pyramids.

But alongside their glorious culture, they are also associated with another dark cultural phenomenon: human sacrifice. And according to recent research, very It's certainly dark.

New findings from an analysis of ancient DNA from the ancient Maya city of Chichen Itza suggest that many of those sacrificed were children, including a high proportion of identical twins.

El Castillo, also known as the Temple of Kukulkan, is the centerpiece of the Chichen Itza ruins in the Yucatan state of Mexico. – Image credit: Johannes Krauss

Published in a journal NatureThe study looked at human bones found in a xultun, or underground cistern, located near a large sinkhole known as the Sacred Cenote.

Radiocarbon dating (when scientists use decaying radioactive carbon to estimate the age of organic remains) suggests that the chultun was used between the early 7th century AD and the mid-12th century AD.

“The only people in Chultung were children between the ages of three and six.” Dr. Rodrigo BarqueraThe lead author of the study is BBC Science Focus“Until now, we haven't had the opportunity to report the sex of these individuals because when they are that young, you can't determine their biological sex based on the bones alone.”

Moving quickly on from how bleak a hole filled with 100 children looks, DNA evidence revealed that all 64 people tested were male, and about 25% were close relatives, including two sets of identical twins.

The chance of having identical twins is about 1 in 250, so two sets of male twins in such a small sample size is unusual.


Barquera explained that twins had a special meaning to the Mayans because one of their most important myths involves heroic twins who defeat the king of the underworld.

The team believes that unlike other sacrificial rituals that were intended as offerings, the sacrifice of identical male twins may have been undertaken to honour the existence of hero twins.

Detail of the reconstructed stone tzonpantli (skull house) at Chichen Itza. – Image courtesy of Christina Wariner

While that's not great news for identical twins in Mayan culture, as Barquera says, it would have been a huge honor for the family: “It was more like, 'Wow, the gods or the powers that be have chosen us to be the guardians of these children who will one day participate in this magical ceremony.'”

“We know this because the site has been there for over 500 years. This isn't something that happened once or twice; it's been a widely held belief for at least five centuries,” he said.

Next, Barcela and his team hope to confirm their findings by comparing them with other similar archaeological sites.

About our experts

Rodrigo Barquera He is a postdoctoral researcher in the Archaeogenetics department at the Max Planck Institute for Evolutionary Anthropology in Leipzig. He has authored nearly 200 academic research papers, which have been published in such renowned journals as: Nature and Nature Communications Biology.


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Source: www.sciencefocus.com

Amateur astronomers find speedy L-type subdwarf star in our cosmic neighborhood

At an estimated distance of 140 parsecs (457 light years), the L-type subdwarf star CWISE J124909+362116.0 (J1249+36 for short) has a total velocity of at least 600 km/s, exceeding the local galactic escape velocity. Remarkably, the star may have been ejected from a globular cluster in the outer reaches of the Milky Way sometime in the past 10 to 30 million years.

A simulation of the hypothetical J1249+36 white dwarf binary ends with the white dwarf star exploding in a supernova. Image courtesy of Adam Makarenko / WM Keck Observatory.

J1249+36 was first discovered by a citizen scientist. Backyard Worlds: Planet 9 Program.

The star immediately stood out as its speed across the sky was initially estimated to be around 600 km/s.

This speed is fast enough for the star to escape the gravity of the Milky Way, making it a potential hypervelocity star.

To better understand the properties of J1249+36, Professor Adam Burgasser of the University of California, San Diego, and his colleagues used the W. M. Keck Observatory to measure its infrared spectrum.

These data revealed that the object is a rare L-type subdwarf star, a class of stars with an extremely low mass and temperature.

Spectral data and imaging data from multiple ground-based telescopes allowed the team to precisely measure J1249+36's position and velocity in space, and predict its orbit within the Milky Way galaxy.

“What makes this source so interesting is that its speed and orbit suggest it is moving fast enough to escape the Milky Way,” Professor Burgasser said.

The researchers focused on two scenarios to explain J1249+36's unusual orbit.

In the first scenario, J1249+36 was originally a low-mass companion to a white dwarf.

If a companion star is in a very close orbit with a white dwarf, it can transfer mass, causing periodic explosions called novae. If the white dwarf gathers too much mass, it can collapse and explode as a supernova.

“In this type of supernova, the white dwarf is completely destroyed, so the companion star is freed to fly away at the orbital velocity it was originally moving at, plus a bit of a supernova blast,” Prof Burgasser said.

“Our calculations show that this scenario holds true. However, because the white dwarf no longer exists and the remnants of the explosion that probably occurred millions of years ago have already dissipated, we have no conclusive evidence that this is its origin.”

In the second scenario, J1249+36 was originally a member of a globular cluster, a tightly bound group of stars that is immediately recognizable by its distinctive spherical shape.

The centers of these clusters are predicted to contain black holes with a wide range of masses.

These black holes can also form binary systems, and such systems prove to be great catapults for any star that happens to get too close to them.

“When a star encounters a black hole binary, the complex dynamics of this three-body interaction can cause the star to be thrown out of the globular cluster,” said Dr Kyle Kremer, an astronomer at the University of California, San Diego.

The scientists ran a series of simulations and found that, on rare occasions, these types of interactions can cause low-mass subdwarf stars to be ejected from globular clusters and follow orbits similar to the one observed in J1249+36.

“This is a proof of concept, but we don't actually know which globular cluster this star is from,” Dr Kremer said.

“By tracking J1249+36 back in time, we find that it lies in a very crowded part of the sky that may be hiding undiscovered star clusters.”

To determine whether one of these scenarios, or some other mechanism, can explain J1249+36's orbit, the team wants to take a closer look at its elemental composition.

For example, the explosion of a white dwarf star could produce heavy elements that could pollute J1249+36's atmosphere as they escape.

Stars in the Milky Way's globular clusters and satellite galaxies also have unique presence patterns that could shed light on the origins of J1249+36.

“We're basically looking for a chemical fingerprint that will pinpoint exactly what system this star came from,” says Roman Gerasimov, also of the University of California, San Diego.

“Whether J1249+36's high-speed movement is the result of a supernova, a chance encounter with a black hole binary, or some other scenario, its discovery offers astronomers a new opportunity to learn more about the history and dynamics of the Milky Way.”

The astronomers discovery this week's 244th Meeting of the American Astronomical Society In Madison, Wisconsin.

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Adam Burgasser others2024. A superfast L-type subdwarf star passes near the solar system. 224 AustraliaAbstract #3

Source: www.sci.news

Greek Island of Aegina reveals ancient workshop where 3,600-year-old purple dye was made

Coloured dyes were essential commodities in the Mediterranean region during the Late Bronze Age.



Berger and his colleagues unearthed a purple dye factory at site K10 (marked in red) outside Colonna, Aegina, during the Bronze Age. Image courtesy of Berger others., doi: 10.1371/journal.pone.0304340.

of The small island of Aegina It is located in the middle of the Saronic Gulf, between Attica, the Peloponnese and the central Aegean Sea.

The island has played an important role in the cultural history of the Aegean for thousands of years.

From the Neolithic to the Byzantine period (6th millennium BC to the 10th century AD), Aegina's main settlement was located on a small, well-protected promontory on the northwest coast called Cape Colonna.

During the 2nd millennium BC, this densely built and heavily fortified settlement reached the height of its economic prosperity and culture.

Representative monuments, outstanding finds and rich tombs indicate an economically stable and complex social system integrated into inter-regional trade networks and emerging cultures in the Middle and Late Bronze Age Aegean.

in New paper In the journal PLoS OneDr. Lydia Berger from the Université Paris-Lodron de Salzburg and her colleagues describe the remains of a 16th century BC purple dye workshop at Aegina Colonna.

The existence of this workshop is inferred from three main pieces of evidence: purple pigment preserved on pottery shards believed to be remnants of dye containers, dyeing tools such as grinding stones and waste pits, and crushed shells of marine snails harvested for the pigment.

Analysis of the chemical composition of shells and pigments indicates that the workshop mainly produces Mediterranean snails. Murex striped dye (Hexagonal column trunk).

Excavations at the site also uncovered numerous burnt bones of young mammals, mainly piglets and lambs.

Archaeologists hypothesize that these may be the remains of animals that were ritually sacrificed as sacred offerings to protect the dye-producing areas. This practice is known from other cultural sites, but the exact relationship of these bones to dye production is not yet entirely clear.

The site provides valuable insight into the tools and processes of Mycenaean purple dye production.

Further investigations may reveal more information about the scale of dye production at Aegina Colonna, details of procedures at the site, and the use of this dye in regional trade.

“The discovery for the first time of a remarkably large amount of well-preserved pigment, a large amount of crushed mollusc shells and several functional installations allows detailed insights into the production of purple dye on the Greek island of Aegina around 3,600 years ago,” the researchers said.

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L. Burger others2024. More than just a colour: Archaeological, analytical and procedural aspects of Late Bronze Age purple dye production at Cape Colonna, Aegina. PLoS One 19(6):e0304340;doi:10.1371/journal.pone.0304340

Source: www.sci.news

Citizens in Georgia rally against proposed construction of major monkey breeding facility in their community.

Residents are expressing concerns about the facility itself and the potential for monkeys to escape, which has occurred in the past. Similar incidents have been reported at other facilities in the United States, including one operated by Oregon Health & Science University. In Portland, there have been no reports of harm to nearby residents,

“We’re facing a jungle – the noise, the smell, the risk of disease,” stated Penny Reynolds, who resides across the street from the land designated for the Bainbridge facility.

Safer Human Medicine has reassured residents that they take all necessary precautions to ensure that all waste remains on-site and is sent to the city’s wastewater treatment plant, and that most of the noise is contained on-site with no detectable odors.

Greg Westergaard, the CEO of monkey breeder Alpha Genesis, mentioned that establishing a monkey facility entails significant effort.

“It would involve extensive training and infrastructure,” he explained. “There will be unpleasant odors and wastewater from cleaning.”

Residents of Bainbridge point to the backgrounds of several executives at Safer Human Medicine, two of whom previously held leadership roles at companies that were under investigation, as a reason to be skeptical of their efforts.

CEO of Safer Human Medicines, Jim Harkness, is the chief operating officer of Envigo. He recently pleaded guilty. Thousands of dogs were abandoned, leading to a $35 million fine. Former Chief Operating Officer Kurt Derfler has left Charles River Laboratories. The Department of Justice issued a subpoena The probe was part of an inquiry into the potential smuggling of wild monkeys from Cambodia, and Charles River Laboratories stated at the time that any concerns about its involvement were “unwarranted.”

Neither Mr. Harkness nor Mr. Derfler faced individual charges related to those incidents.

Safer Human Medicine declined an interview request. “Envigo was functioning under unprecedented circumstances brought on by the pandemic,” they said in an email. They also stated that “we have been committed to operating responsibly and ethically in this field for decades and will continue to do so.”

Long-tailed macaques, also known as crab-eating macaques, are climbing the pillar in Indonesia in 2023.Chaidir Mahyudin/AFP via Getty Images file

Safer Human Medicine has stated that they do not use wild-caught macaques. Herpes BThe macaques will be sourced from Asia, but the specific location has not been disclosed.

Community activism in Bainbridge has made an impact. What was initially promoted as a “significant investment” is now overseen by Rick McCaskill, executive director of the Bainbridge and Decatur County Development Authority. Approximately $400 million and 260 jobs Things took a turn quickly. Following pushback from the community, Bainbridge leaders decided in February to Withdraw support for the Safer Human Medicine Project.

“The division and fear within the community seemed to outweigh the benefits of the project,” McCaskill remarked.

Monkeys used for research are housed at seven national primate research centers, each with its own breeding colonies, as well as other facilities across the country. While the national primate research centers mostly utilize rhesus macaques, pharmaceutical companies tend to prefer long-tailed macaques, which Safer Human Medicine intends to use.

Animal testing for drug development was formerly mandatory in the United States, but President Joe Biden will lift the ban in 2022. FDA Modernization Act 2.0 Signed into LawAllow non-animal options where possible. Several members of Congress voted this year to The bill was submitted. We advocate for a shift away from animal testing.

“There are various alternatives available today, such as AI, computer models, and organs on chips,” stated Jim Newman, spokesperson for the American Association for Medical Progress, a group that supports animal testing when necessary, “but current options can only reduce the number of animals to a certain extent.”

An artist’s rendering of a monkey enclosure proposed for Bainbridge, Georgia.Safer Human Medicines

Currently, researchers still rely on monkeys for certain tests, and some animal researchers cite a U.S. Shortage of long-tailed macaques — Imports reportedly dropped by over 20% in 2020 due to China halting exports, leading to a surge in prices of long-tailed macaques.

Safer Human Medicine believes that their proposed facility can address the monkey shortage, intending to start with 500 to 1,000 monkeys and then expand. They stated that the facility would be funded by industry and private donors in the US, without specifying them.

The extent of opposition from local residents to the facility remains unclear. Some local politicians who opposed the facility lost recent elections, but it is uncertain if their defeat was linked to their stance.

Nevertheless, Faircloth asserted that her group has no intention of backing down.

“If we don’t stand up for our rights, they will walk all over us,” she declared. “And we can’t allow that to happen.”

Source: www.nbcnews.com

Compensation Claims for $32 billion Over Russia’s Carbon Emissions During Ukraine War

A building damaged by a drone strike in Kiev in October 2022

Roman Fritzina/Associated Press/Alamy

A group of climate experts estimates that the first two years of Russia's war in Ukraine will result in greenhouse gas emissions equivalent to about 175 million tonnes of carbon dioxide.

The extra warming caused by these emissions will lead to extreme weather events around the world, with impacts estimated at $32 billion.

Ukraine intends to add these climate-related costs to the list of damages for which Russia is responsible and for which it seeks compensation.

“This will be an important pillar in the compensation case we are building against Russia,” Ukrainian Minister of Environmental Protection and Natural Resources Ruslan Strylets said in a statement.

“These are the costs to economies and societies caused by extreme weather events due to emissions-driven climate change,” said Leonard de Klerk, a climate businessman and founder of the War Greenhouse Gas Accounting Initiative.

The group today Fourth evaluation The report estimated the impact of the war from February 2022 to February 2024. It found that rebuilding bombed-out buildings, roads and other infrastructure was the biggest source of emissions, accounting for almost a third of the 175 million tonnes – a figure that also includes reconstruction that has yet to take place.

The remaining third is a direct result of the war, with fuel use accounting for the largest proportion.

About 14% of the total is due to passenger airlines having to reroute flights to avoid Russia and Ukraine. For example, a flight from Tokyo to London now travels over Canada instead of Russia, increasing flight times from 11 to 15 hours.

About 13 percent is due to an increase in wildfires recorded on satellite imagery, which is due not only to weapons-fired fires but also an end to fire management in occupied territories, the assessment said.

In most cases, there is a great deal of uncertainty around the figures as there are no official figures to rely on, and instead the group must rely on open source assessments and figures from past conflicts.

There's also the issue of how far to go in assessing the cascading effects of war: “We try to be as comprehensive as possible,” de Klerk says, “but at the same time, there are limitations. Some effects are too remote or too hard to quantify.”

Estimating how much damage additional emissions will cause (known as the social cost of carbon) is another tricky area: “The science of trying to put a monetary value on future damages is still developing,” says de Klerk.

The estimated figure of $32 billion Based on 2022 research The social cost of carbon is about $185 per tonne of CO2.

If this amount, which is growing every day, were to be paid, De Klerk thinks that one part should be sent to Ukraine to be used for measures such as reforestation and helping to capture some of the carbon, while the other part should go to the countries most affected by global warming, probably through the existing system. Green Climate FundBut where that money will go is a political decision that has yet to be resolved.

Low-income and small island nations have fought for decades to establish the principle that high-income countries with large greenhouse gas emissions should compensate them for loss and damage caused by their emissions. A loss and damage fund was finally established last year as part of an international climate agreement.

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Source: www.newscientist.com

The unexpected impact of weight loss drugs on your mental wellbeing and cognitive function

ADDICTIVE STOCK CREATIVES/Alamy; AdoBe Stock

Kathy Schwartz had been sober for 10 years, but battling cravings was a daily struggle. “They were always in my head,” she said. But last June, the cravings subsided.

After being prescribed the weight-loss drug semaglutide, she not only lost nearly 30 kilos over 10 months, but also eliminated her desire for drinks or pills. “The cravings went away, and I didn’t realize that was a side effect,” Schwartz says. Amazingly, the depression and anxiety that had previously hit her in waves also subsided.

Schwartz isn’t the only one to have had this experience: New research is showing that semaglutide drugs like Ozempic and Wegovy, as well as other diabetes and weight-loss drugs that mimic gut hormones released after eating, can have surprising benefits for brain and mental health.

Though it’s still early days, evidence suggests that these drugs could potentially be repurposed to treat depression, anxiety, addiction, and even certain eating disorders, as well as neurological diseases like Parkinson’s and Alzheimer’s. What’s more, these benefits appear to be mediated not simply through weight loss, but through a direct effect on the brain.

The history of drugs like Ozempic dates back to the 1970s and 1980s, when researchers discovered them. A gut hormone called glucagon-like peptide 1 has been discovered. When GLP-1 was injected into rodents in the lab, it was able to stimulate insulin secretion. Even more amazingly, these animals started to eat less and lose weight. We now know that this hormone leads to an increased feeling of fullness.

Semaglutide, etc.

Today, there are drugs that mimic…

Source: www.newscientist.com