Scientists harness bottled ‘lightning’ to generate essential ingredients for life

Nitrogen is an essential element for life and is an integral part of DNA and proteins. Most of the nitrogen on Earth exists in the atmosphere as gaseous nitrogen, denoted as N.2 However, most organisms cannot directly use nitrogen. In modern ecosystems, some microorganisms have specialized enzymes that convert nitrogen into nitrogen.2 It converts gases into a form that other living things can use. Fixed nitrogen These microorganisms Nitrogen fixing bacteria.

But 3 to 4 billion years ago, during a period in Earth's history called the Archean Era, life had not yet evolved and no nitrogen-fixing organisms existed, so scientists studying the origin of life are faced with a classic chicken-and-egg problem: life needed nitrogen to evolve, but before life evolved, there were no microorganisms to convert nitrogen into nitrogen.2 Let's turn gas into something we can use! So where did life get its nitrogen from before there were nitrogen-fixing organisms?

Researchers recently hypothesized that early life on Earth may have obtained fixed nitrogen from lightning. They propose that the high energy of a lightning spark could react with oxygen and N.2 Fixing atmospheric nitrogen2 The gas is converted into other usable forms of nitrogen. Nitrogen oxides.

Geologists have studied the sedimentary rock record to understand nitrogen throughout Earth's history, but they had no way to distinguish lightning-derived nitrogen in rocks from other ancient sources of nitrogen. To explore whether lightning provided fixed nitrogen to early life, researchers led by Dr. Patrick Barth created “lightning” in a jar and tested whether it would react with nitrogen.2 It emitted gases and produced nitrogen oxides that had an identifiable signal.

To simulate lightning, the researchers used electrodes in glass flasks filled with different gas mixtures: To mimic modern-day Earth, Barth and his colleagues used a flask with a composition similar to our current atmosphere, containing 85 percent nitrogen.2 They also used flasks containing an atmosphere similar to that of Archean Earth, which scientists believe was about 83% nitrogen.20% oxygen, 16% carbon dioxide.

The researchers added 50 milliliters (about a quarter cup) of water to the bottom of each flask to allow any nitrogen oxides and other compounds produced during the reaction to dissolve in the water. They discharged each experimental flask to about 50 kilovolts for 15 to 60 minutes — nearly 10 times the voltage of an electric car battery.

The research team developed a device called Quadrupole Gas AnalyzerThey measured the nitrogen compounds in the gases coming out of each flask before and after they were ignited. They found that in the modern experiment, more fixed nitrogen was dissolved in the water than in the gas. But in the Archean experiment, the fixed nitrogen was split almost equally between the water and the gas.

After each reaction, the researchers placed the flask of water into an apparatus that measured the weight of the nitrogen atoms. Gas Source Mass SpectrometerThey explained that nitrogen atoms exist in two main forms with different masses, called isotopes. 14The N isotope is lighter and more abundant in nature, 15The N isotope is heavier and less common. The researchers used mass spectrometer data to calculate the ratios of nitrogen isotopes in the lightning-fixed nitrogen samples. They compared these nitrogen isotope ratios to those in rocks that are 3.1 to 3.8 billion years old to see if there was a match.

The researchers found that the nitrogen isotope ratio of the lightning-produced nitrogen was about 0.1% to 1% lighter than that of the rocks, and suggested that this difference in nitrogen isotopes indicates that most of the nitrogen in the Archean rocks was not produced by lightning.

The researchers also used the lightning flash rate on modern Earth to predict the amount of nitrogen oxides that lightning would produce per year. They estimated that the annual lightning flash rate alone could not have provided enough nitrogen to support ecosystems on early Earth. They explain that there was even less lightning in the Archean than there is today, so even less nitrogen was available to support early life.

The researchers concluded that lightning was not the main source of available nitrogen for early life. Because nitrogen-fixing organisms must have evolved very early in Earth's history, life did not need to rely solely on lightning, they suggested. However, one of the 3.7-billion-year-old rock samples showed nitrogen isotope ratios similar to lightning-fixed nitrogen, leading the researchers to speculate that small amounts of fixed nitrogen from lightning may have supported early life. Furthermore, the researchers suggested that the lightning-fixed nitrogen isotope ratios obtained in this study could be used to investigate how nitrogen is fixed on other planets in the solar system.


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Source: sciworthy.com

Regular walking may extend your period of time pain-free in your back

Back pain is a common discomfort that can be difficult to shake once it sets in. Researchers suggest a simple way to make back pain more manageable and potentially extend the time between episodes.

Over 600 million people worldwide suffer from back pain, with studies showing that 7 out of 10 individuals experience a relapse within a year after recovery. This makes back pain a major cause of disability globally (source).

The Spine Pain Research Group at Macquarie University in Australia conducted a study indicating that regular walking can help treat back pain. They suggest that some current exercise recommendations may not be suitable or practical due to cost or supervision requirements (source).


A recent study published in the journal Lancet focused on 701 adults who had recovered from low back pain lasting at least 24 hours. Participants were assigned to a personalized walking program, physical therapy sessions, or a control group with no treatment (Dr. Mark Hancock).

The researchers observed that the walkers experienced less back pain, reduced the need for medical assistance, and halved their sick leave. The time between episodes nearly doubled from 112 days to 208 days.

Dr. Hancock believes walking’s benefits come from gentle motion and muscle strengthening, as well as stress-relieving effects. While some experts agree that low-intensity exercise like walking can help with back pain, others suggest the study’s findings may not be groundbreaking.

In conclusion, while walking may not be a quick fix for back pain, it is a recommended low-intensity exercise that can provide relief over time. It’s important to keep moving and gradually improve rather than sitting still and doing nothing.

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Source: www.sciencefocus.com

Today is the summer solstice in 2024 – what causes the longest day of the year and when does it occur?

Summer is here, officially starting today with the Northern Hemisphere experiencing more daylight than anywhere else. This marks the 2024 summer solstice, a significant day that has been celebrated for thousands of years. Whether for religious ceremonies or casual barbecues, the longest day of the year is a cause for celebration.

If you’re unsure about the summer solstice and its importance, especially at places like Stonehenge, we’re here to provide some clarity.

When is the Summer Solstice in 2024?

The summer solstice in 2024 falls on Thursday, June 20th at 9:51 pm BST (4:50 pm EDT New York time, 1:50 pm PDT Los Angeles time). Keep in mind that the summer solstice occurs at a specific moment, signifying the start of astronomical summer when the Northern Hemisphere faces the Sun directly.

It’s the longest day of the year, providing the most hours of sunshine in 2024. Expect at least 16 hours of sunlight in the UK and US. This is one of the two solstices each year, with the second occurring in December. The summer solstice always falls between June 20 and 22, coming a day earlier this year compared to 2023.


When are Sunrise and Sunset on the Summer Solstice?

On Thursday, June 20th, the sunrise in London, England is at 4:43 am BST, and the sunset is at 9:21 pm BST. Sunrise and sunset times may vary slightly depending on your location in the UK or US.

  • Summer solstice sunrise in New York City: 5:25 a.m. EDT.
  • Summer solstice sunset in New York City: 8:31 pm EDT.
  • Summer solstice sunrise in Austin, Texas: 6:30 am CDT.
  • Summer solstice sunset in Austin, Texas: 8:36 pm CDT.
  • Summer solstice sunrise in Los Angeles: 5:42 am PDT.
  • Summer solstice sunset in Los Angeles: 8:08 pm PDT.

While today is the longest day of the year, it doesn’t necessarily have the earliest sunrise or the latest sunset. The exact dates for these phenomena vary based on your latitude. In areas around the 40th parallel north, the earliest sunrise of the year occurred around June 14th, with the latest sunset around June 27th.

“This slight difference occurs because the Earth orbits the Sun in a slight ellipse, not a circle.” Dr. Darren Baskill“It’s a very exciting time for us,” says astrophotographer and astronomy lecturer at the University of Sussex. BBC Science Focus.

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What is the Summer Solstice?

The summer solstice occurs when the Sun reaches its highest point in the sky, directly hitting the Northern Hemisphere. This axis tilt of about 24 degrees causes opposite seasons in the Northern and Southern Hemispheres, with the summer solstice marking the longest day of the year. As the Earth orbits the Sun in an ellipse, the perihelion (closest point to the Sun) occurs in January, while the aphelion (farthest point) occurs in July.

Due to the Earth’s tilt, sunlight falls directly on the Northern Hemisphere during the summer solstice. In the Southern Hemisphere, this marks the shortest day of the year, or winter solstice. – Image credit: Getty

Although the summer solstice is the longest day of the year, peak temperatures usually occur in July or August as the Earth continues to release absorbed heat. The tilt of the Earth’s axis, not its distance from the Sun, causes the change in seasons.

Why is the Earth Tilted?

The Earth’s tilt resulted from significant impacts during the solar system’s formation 4.5 billion years ago. The current tilt allows for regions where the sun never sets during the summer solstice, like in the Arctic. This tilt contributes to the variety of seasons experienced on Earth.

How is the Summer Solstice Celebrated Around the World?

Celebrations of the summer solstice take place worldwide, from the Swedish midsummer festivities to Stonehenge in England. Stonehenge, built thousands of years ago, aligns with the rising sun on the summer solstice, attracting hundreds to witness the event every year.

Starting in the late Middle Ages, Swedes began the tradition of erecting a Midsummer pole and dancing around it. The custom of decorating the pole with flowers and greenery was called a “maja”, which also came to be called a Maypole. – Image credit: Getty

What is the Difference Between the Equinox and the Summer Solstice?

Equinoxes mark the change of seasons with equal day and night lengths, occurring in spring and autumn. Solstices, on the other hand, focus on sunlight, with the summer solstice being the longest day of the year in the Northern Hemisphere.

Do Other Planets Have Solstices?

Every planet in the solar system has solstices due to axial tilts. Earth’s tilt is pronounced compared to other planets like Venus or Jupiter. Mars, similar to Earth, experiences seasons but with longer durations due to its elliptical orbit.

Upcoming Summer Solstice Dates and Times, BST

  • 2025: June 21, 3:42 AM
  • 2026: June 21, 9:24 AM
  • 2027: June 21, 3:10 p.m.
  • 2028: June 20, 9:01 p.m.
  • 2029: June 21, 2:48 AM
  • 2030: June 21, 8:31 AM

About Our Experts

Darren Baskill is an Outreach Officer and Lecturer in the School of Physics and Astronomy at the University of Sussex. They have a background in astronomy and have contributed to various projects in the field.


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Source: www.sciencefocus.com

New study finds solid wood surfaces exhibit natural antiviral characteristics

In a recent study, researchers from the University of Jyväskylä and the University of Eastern Finland examined the antiviral properties of different types of wood, including coniferous and deciduous trees, against coronaviruses and enteroviruses.

Shroff othersScots pine and Norway spruce were found to have excellent antiviral activity, especially against enveloped viruses, with onset within 10-15 minutes. In contrast, other hardwoods showed mixed efficacy, and oak showed effectiveness against enteroviruses. Image courtesy of Schroff. others., doi: 10.1021/acsami.4c02156.

Since ancient times, wood has played a vital role in tools, utilities, and construction.

The 20th century witnessed a depletion of wood resources, prompting the emergence of alternatives like plastics and metals for interior surfaces and fixtures.

A growing concern for sustainability and the unique qualities of wood has led to a resurgence in its use across various applications.

The 21st century has brought new health challenges, including viral outbreaks like SARS and COVID-19, emphasizing the importance of surface hygiene.

Viruses can persist on surfaces as fomites, with enveloped viruses having shorter survival times compared to non-enveloped viruses.

Wood has been known for its antibacterial and antifungal properties, but its antiviral capabilities were not thoroughly explored until this study.

Researchers investigated how different types of wood affect the infectivity of enveloped and non-enveloped viruses.

The study found that certain types of wood could significantly reduce viral infectivity within hours, showcasing their potential as natural antiviral materials.

Their research paper was published in the journal ACS Applied Materials & Interfaces.

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Reference: Sailey Shroff et al. (2024). Inactivation of coronaviruses and enteroviruses on solid wood surfaces depending on wood species. ACS Applied Materials & Interfaces, 16(23), 29621-29633. doi:10.1021/acsami.4c02156

Source: www.sci.news

NGC 1546 Spotted by Hubble Space Telescope

The NASA/ESA Hubble Space Telescope has captured its first images since changing to an alternate operating mode that uses just a single gyroscope to help control and orient the telescope.

This Hubble Space Telescope image shows NGC 1546, a spiral galaxy about 52.5 million light-years away in the constellation Doradus. Image courtesy of NASA / ESA / Hubblr / STScI / David Thilker, JHU.

Hubble I input it On May 24, 2024, we will pause science observations and go into safe mode due to ongoing gyroscope issues.

Over the past six months, the gyroscope has frequently returned inaccurate measurements, causing multiple interruptions to science operations.

This allowed Hubble astronomers to transition from a three-gyroscope operating mode to observing with only one gyroscope, allowing for more consistent science observations and preserving the other working gyroscope for future use.

“Hubble’s new images of the spectacular galaxy NGC 1546 prove that the telescope’s new, more stable pointing mode is a complete success,” said Dr. Jennifer Weissman, Hubble’s senior project scientist at NASA’s Goddard Space Flight Center.

“We’re poised for many years of discovery to come, looking at everything from our solar system to exoplanets to distant galaxies.”

“Hubble plays a vital role in NASA’s astronomy toolkit.”

NGC 1546 It is a spiral galaxy 52.5 million light years Beyond the constellation of Dorado.

Also known as ESO 157-12, IRAS 04134-5611, and LEDA 14723, the galaxy is approximately 50,000 light years Across.

It was discovered on December 5, 1834 by British astronomer John Herschel.

“The orientation of the galaxy makes a backlit dust band highly visible some distance above the galaxy’s nucleus,” said Dr Weissman and his colleagues.

“This dust absorbs light from the core, making the core red and the dust appear rusty brown.”

“The core itself glows brightly with a yellowish light, indicating that it is an old population of stars.”

“Bright blue regions of active star formation shine through the dust.”

“You can also see several background galaxies, including an edge-on spiral galaxy just to the left of NGC 1546.”

A color image of NGC 1546 can be found at Hubble’s Wide Field Camera 3 (WCF3).

“The WCF3 instrument captured this image as part of a joint observing program between the Hubble Space Telescope and the NASA/ESA/CSA James Webb Space Telescope,” the astronomers said.

“The program also uses data from the Atacama Large Millimeter/submillimeter Array (ALMA), which allows us to look at how stars form and evolve in great detail and at many wavelengths.”

“This image represents one of the first observations made with Hubble since transitioning to a new pointing mode that will allow for more consistent science observations.”

“We expect the Hubble Space Telescope will conduct most of its science observations in this new mode and continue its groundbreaking observations of the universe.”

Source: www.sci.news

New research reveals deeper insights into the genetic factors influencing coffee consumption

Coffee is one of the most widely consumed beverages. In a new study, scientists from the University of California, San Diego and others conducted a genome-wide association study (GWAS) of coffee intake among US-based 23andMe participants. They investigated genetic correlations and conducted a phenotype-wide association study across hundreds of biomarkers, health, and lifestyle traits, and compared their results with the largest GWAS of coffee intake from UK Biobank.

Coffee drinking is an inherited habit and carries a certain amount of genetic load. Image courtesy of Sci.News.

“To create the GWAS, we collected genetic data and self-reported coffee consumption,” said lead author Dr. Hayley Thorpe, a researcher at Western University and the University of Guelph.

“Our goal was to identify associations between genes known to be associated with coffee consumption and health-related traits and conditions.”

“We used these data to identify regions in the genome that are associated with a higher or lower likelihood of drinking coffee.”

“And then we identify the genetics and biology that underlie coffee consumption.”

“Many people are surprised that coffee consumption has genetic effects,” said co-author Abraham Palmer, PhD, a research scientist at the University of California, San Diego.

“From previous papers, we had good reason to suspect that there was a gene that influenced coffee intake.”

“So it wasn’t a surprise to us that in both cohorts we looked at, there was statistical evidence that this is a genetic trait.”

“In other words, the specific genetic variants we inherit from our parents influence how much coffee we drink.”

“The genetic influence on coffee consumption was the first of two questions we wanted to answer,” said Sandra Sanchez Loij, PhD, a research scientist at the University of California, San Diego and senior author of the paper.

“The second thing is what coffee lovers really want to know: Is drinking coffee good or bad? Does drinking coffee have positive health consequences or not?”

The group’s genome-wide association study of 130,153 US-based 23andMe study participants, compared with a similar UK Biobank database (334,649 British individuals), found consistent positive genetic associations between coffee consumption and adverse health outcomes such as obesity and drug use.

A positive genetic association is a link between a particular gene variant (genotype) and a particular condition (phenotype).

Conversely, a negative genetic association would be a clear protective trait that would thwart the onset of the disease.

When it comes to mental illness, the findings are more mixed.

“For example, if you look at the genetics of anxiety disorders, bipolar disorder and depression, in the 23andMe data, they tend to be positively correlated with the genetics of coffee consumption,” Dr. Thorpe said.

“However, in UK Biobank we see the opposite pattern of negative genetic correlation, which is not what we expected.”

“There were other instances where the 23andMe sets did not match the UK Biobank, but the biggest discrepancies were for psychiatric disorders.”

“It’s common in this field to combine similar datasets to increase research power. This information tells us pretty clearly that combining these two datasets was not a smart idea. And we ended up not doing so.”

“Mixing databases can mask effects, leading researchers to erroneous conclusions, or even cancel each other out.”

“There are a few ideas as to how the differences in results could have arisen. First, the studies were comparing apples with oranges,” Dr. Sánchez Loisi said.

“For example, the 23andMe survey asks, ‘How many 5-ounce (cup-sized) cups of caffeinated coffee do you drink per day?’ Compare this to UK Biobank’s, ‘How many cups of coffee do you drink per day (including decaffeinated coffee)?'”

“The study did not take into account the variety of ways coffee is presented, beyond serving size and whether it’s caffeinated or decaffeinated.”

“We know that in the UK instant coffee is generally preferred, whereas in the US ground coffee is more commonly preferred,” Dr Thorpe said.

“And then there’s the Frappuccino, the American fad of drinking coffee loaded with added sugar,” Dr. Sánchez Loij added.

“There are other caffeinated drinks out there and, particularly in the UK Biobank context, tea was not included in the GWAS that looked solely at coffee,” Dr Palmer said.

“GWAS shows that the genotype-phenotype relationship is more different than that between coffee and tea.”

“Genetics influences a lot of things. For example, it influences your height.”

“And these things would probably play out in the same way whether you lived in the US or the UK. But coffee is a decision people make.”

“Coffee comes in many forms, from instant to Frappuccino, and is consumed within different cultural norms in different places,” Dr Sánchez Loij said.

“Someone with one genotype may end up with a completely different phenotype if they live in the UK and the US.”

“And that’s exactly what the data tells us, because in the case of height, behavior doesn’t really matter, but behavior and selection in the environment affect it in different ways. So genotype-environment interactions complicate the picture.”

Team paper Published in the journal Neuropsychopharmacology.

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HHA Soap othersGenome-wide association study of coffee consumption in UK/US participants of European descent revealed cohort-specific genetic associations. NeuropsychopharmacologyPublished online April 17, 2024, doi: 10.1038/s41386-024-01870-x

Source: www.sci.news

Discovery of Silver and Bronze Coin Hoard from Gallus Revolt Unearthed in Israel

Jewish Revolt Constantius Gallus, alias Gallus' RebellionThe Roman Civil War of 351-354 AD broke out during the Roman Civil War and was the last Jewish revolt against Rome.

Bronze and silver coins from the 4th century AD found at Lod in central Israel. Image courtesy of the Israel Antiquities Authority.

The 1,650-year-old treasure was discovered by archaeologists from the Israel Antiquities Authority (IAA). rodcentral Israel.

The treasury contains 94 silver and bronze coins dating from 221 to 354 AD.

“The most recent coins date to the period of Gallus' revolt (351-354 AD),” the IAA archaeologists said.

“Documentary evidence for the revolt is scarce, but there are documents that document the destruction of major Jewish communities, such as Lod, Tzipori, and Tiberias, by the armies of Constantine Gallus.”

Also found were impressive stone and marble artifacts, inscriptions in Greek, Hebrew and Latin, and inscriptions bearing the names of Jewish men of priestly descent.

“This is probably a magnificent Jewish building where the city's elders lived,” said IAA archaeologists Shahar Crispin and Mol Wiesel.

“We know from Talmudic texts that Lod was the most important center for the Jews after the destruction of the Second Temple in Jerusalem.”

“Famous 'Sages of Rod' include Rabbi Eliezer ben Horcanos, Rabbi Tarfon, Rabbi Akiva and Rabbi Yossi Hagalili.”

“The building, destroyed down to its foundations, is a clear indication that the rebellion was forcibly put down with violence and brutality, and was not merely a localized uprising as previous studies have claimed.”

“This is the only evidence so far of the scope and power of this rebellion in Lod, which is in the heart of the country.”

“It is difficult to determine whether this magnificent building was used as a synagogue, a study hall, a meeting place for the elders, or all three functions combined,” said IAA professor Joshua Schwartz.

“What is clear, however, is that the size of the buildings, the coin deposits, and the assemblage of archaeological finds produced by the excavations fit well with the description of Lod/Diospolis as depicted in both Jewish and non-Jewish sources as a center of Torah-faithful Jewish life during the Mishnaic and Talmudic periods.”

“Lod's role as a leading community with elders continued from the time of its destruction until this moment, when it was brutally destroyed in the Gallus Rebellion.”

“The incredible finds made here reinforce our commitment to researching and protecting Rod's history and rich heritage,” said IAA director Eli Escuse.

“Together with the city's new exhibition centre with its beautiful rod mosaics, we will bring this building into public awareness.”

Source: www.sci.news

Preventing Back Pain Through Regular Walking

Being active has many health benefits

Sergio Azenha/Alamy

People who suffer from recurring back pain appear to be able to avoid the discomfort for longer by taking regular walks.

Over 600 million people worldwide I feel pain in this part of my back, Initially resolved but often recursDespite this high prevalence, little research has been done on its prevention. Tash Pocovy At Macquarie University, Sydney, Australia.

Pocobi and her colleagues wanted to find an affordable, relatively accessible way to prevent pain recurrence, so they designed “Walk-Back,” the first controlled trial of its kind.

The researchers selected 701 people aged between 20 and 82 years old living across Australia who had experienced and recovered from back pain in the previous six months, without any specific diagnosis such as fracture or infection.

On average, participants experienced 33 episodes of back pain each that interfered with their daily activities and lasted at least 24 hours. None of the participants went for recreational walks or participated in any kind of exercise program to manage their pain.

The scientists asked 351 participants to create an individualized walking program with the help of a physical therapist, with the goal of gradually increasing their walking to 30 minutes a day, five days a week, within six months. The program was unique to each participant to ensure they could stick to it, Pocovy said. After 12 weeks, participants were walking an average of 130 minutes a week.

Pocoví said her intention was to also inform people about the latest scientific knowledge about back pain and reassure them that moving with the supervision of a physical therapist is safe. “A history of back pain can lead many people to avoid or fear moving,” she said.

The remaining 350 volunteers received no such education or walking program recommendations. Pocobi and her team followed all of the participants for up to three years. Regardless of which group they were in, participants were free to receive additional treatment for their pain.

On average, subjects in the treatment group experienced their first recurrence of activity-limiting back pain 208 days after starting the study, compared with 112 days in the control group.

Additionally, half of the control group sought other interventions, such as massage or chiropractic care, compared with only 36% of those who participated in the walking and education program, but the latter group was more likely to experience minor exercise-related complications, such as sprains.

“I think this is probably a useful tool that clinicians can use and patients can use when they go to the clinician,” Pocoví says.

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Source: www.newscientist.com

Study shows wave activity causing erosion along the coastlines of Titan’s largest lakes and oceans

Titan, Saturn’s largest moon, is the only known planet other than Earth that still retains liquid water. Liquid hydrocarbons fed by rain from Titan’s thick atmosphere form rivers, lakes, and oceans, most of which are found in the polar regions. In a new study, a team of MIT geologists surveyed Titan’s coastline and found that the moon’s large lakes and oceans were likely formed by waves.

Artist’s rendering of the surface of Saturn’s largest moon, Titan. Image by Benjamin de Bivort, debivort.org / CC BY-SA 3.0.

The existence of waves on Titan has been a somewhat controversial topic ever since NASA’s Cassini spacecraft discovered liquid puddles on Titan’s surface.

“Some people who have looked for evidence of waves haven’t seen any waves at all and have said, ‘The ocean is as smooth as a mirror,'” said Dr. Rose Palermo, a geologist with the U.S. Geological Survey. “Others have said they saw some roughness in the water but didn’t know if it was caused by waves.”

“Knowing whether there is wave activity in Titan’s oceans can provide scientists with information about the moon’s climate, including the strength of the winds that generate such waves.”

“Wave information could also help scientists predict how the shape of Titan’s ocean will change over time.”

“Rather than looking for direct signs of wave-like features in Titan images, we wanted to take a different approach and see if just looking at the shape of the coastline could tell us what it is that is eroding the coast.”

Titan’s oceans are thought to have formed when rising waters flooded a landscape crisscrossed by river valleys.

The researchers zeroed in on three scenarios for what happened next: no coastal erosion, wave-driven erosion, and uniform erosion caused by either dissolution, where liquids passively dissolve coastal material, or a mechanism where the coast gradually peels away under its own weight.

They simulated how different coastline shapes would change under each of the three scenarios.

To simulate wave erosion, the researchers took into account a variable called “fetch,” which describes the physical distance from one point on the shoreline to the other side of a lake or ocean.

“Wave erosion depends on the height and angle of the waves,” Dr Palermo said.

“We used the fetch to estimate wave height because the bigger the fetch, the further away the wind will blow and the bigger the waves will be.”

Cassini observed Titan’s surface with microwaves and found several grooves that are deep canyons filled with liquid hydrocarbons, including Vid Fulmina, a branching network of thin lines in the upper left quadrant of the image. Image credit: NASA / JPL-Caltech / ASI.

To test how coastline shape would differ between the three scenarios, the scientists started with a simulated ocean area with a flooded river valley all around it.

For wave erosion, we calculated the fetch distance from every point along the coastline to every other point and converted that distance to wave height.

They then ran simulations to see how waves would erode the original shoreline over time.

They compared this to how the same coastline would change due to erosion caused by uniform erosion.

The authors repeated this comparative modelling for hundreds of different initial shoreline configurations.

They found that the shape of the termini varies greatly depending on the underlying mechanism.

Most notably, uniform erosion produced a bulging shoreline that was evenly distributed all around, even in flooded river valleys, whereas wave erosion smoothed out portions of the shoreline exposed primarily to long downstream distances, leaving the flooded valleys narrow and rough.

“Although the initial coastline was the same, we found that uniform erosion and wave erosion resulted in very different final shapes,” Dr Perron said.

“Although it looks like a flying spaghetti monster because of the flooded river valley, the endpoints created by the two types of erosion are very different.”

This image is a composite of images taken during two flybys of Titan in 2006. A large circular feature near the center of Titan’s disk may be the remnant of a very old impact basin. The mountain range southeast of the circular feature and the long, dark linear feature northwest of the old impact site may be the result of deformation of Titan’s crust caused by energy released when the impact occurred. Image credit: NASA/JPL/University of Arizona.

Dr. Perron and his colleagues verified their results by comparing their simulation results with actual lakes on Earth.

They found the same shape differences between Earth’s lakes known to have been eroded by waves and those affected by homogeneous erosion, such as dissolved limestone.

Their modelling revealed distinct and distinctive shapes depending on the mechanism by which the shoreline evolved.

So they wondered: Where does Titan’s coastline fit into these distinctive shapes?

In particular, they focused on four of Titan’s largest and best-mapped oceans: Kraken Mare, which is comparable in size to the Caspian Sea; Ligeia Mare, which is larger than Lake Superior; Punga Mare, which is longer than Lake Victoria; and Lake Ontario, which is about 20% the size of the land-based lake of the same name.

The researchers used Cassini’s radar images to map the coastlines of each of Titan’s oceans, and then applied their model to the coastlines of each ocean to see which erosion mechanisms best explain their shape.

They found that all four oceans fit closely to the wave-induced erosion model, meaning that waves created the closest coastlines to Titan’s four oceans.

“We found that when the shoreline is eroding, its shape is more consistent with wave-driven erosion than uniform erosion or no erosion,” Dr Perron said.

Scientists are trying to figure out how strong Titan’s winds would need to be to churn up waves strong enough to repeatedly scrape away the shoreline.

They also hope to learn from the shape of Titan’s coastline which direction the winds primarily blow from.

“Titan shows us that this case is completely pristine,” Dr. Palermo said.

“It may help us learn more fundamental things about how coasts erode without human influence, which in turn may help us better manage coastlines around the world in the future.”

of Investigation result Published in today’s journal Scientific advances.

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Rose V. Palermo others2024. Evidence of wave erosion on Titan’s coast. Scientific advances 10(25); Source: 10.1126/sciadv.adn4192

Source: www.sci.news

Scientists Study Pest-Killing Fungus by Collecting Sexually-Excited Zombie Cicadas

With their bulging red eyes and alien-like mating sounds, periodical cicadas may seem scary and weird, but some of them are speed-freak, sex-crazed zombies that have been hijacked by super-sized fungi.

West Virginia University mycology professor Matt Casson, his 9-year-old son Oliver, and graduate student Angie Macias have been tracking a pesky fungus called Massospora cicadina, the only fungus on Earth that can hijack an animal’s body to make amphetamines (a drug known as speed)—and sure enough, it’s taking over cicadas, increasing their sex drive and spreading a parasite that’s transmitted sexually.

“They’re zombies, totally at the mercy of the fungus,” says John Cooley, a cicada researcher at the University of Connecticut.

The fungus has the largest genome of any known fungus—about 1.5 billion base pairs, Casson says, making it about 30 times longer than any common fungus we know—and while the periodical cicada lives underground for 17 years (13 years in the southern U.S.), its spores typically remain underground as well.

“It’s been a mycological oddity for a long time,” says Casson, “and it has the largest genome, produces wild compounds, keeps its host active, and has a whole host of other strange characteristics.”

Matt Cusson, a professor of mycology at West Virginia University, dissects fungal tissue from the posterior abdomen of a female periodical cicada infected with the fungus Massospora cicadina.Carolyn Custer/AP

This year, Casson decided to ask people to send him infected cicadas from around the country, and despite his injured leg, he, his son, and Mathias traveled from West Virginia to the Morton Arboretum outside Chicago, where they reported a fungus that takes over the lower half of the cicada’s body, discarding its reproductive organs and replacing them with a rather conspicuous mass that’s white, sticky but flaky. The spores then spill out like salt from a shaker.

Infected cicadas can be hard to spot.

Ten seconds after jumping off the golf cart, Macias was in the trees, looking around. She triumphantly raised the semi in the air and shouted, “I got it!”

“That was just luck,” Oliver complained.”

“Luck, eh? Good luck,” Macias replies.

Ten seconds later, Oliver spotted another bird in the bushes next to him, and a little later the photographer spotted a third.

Casson is tracking the only bacteria on Earth that produces amphetamines in living organisms when it takes control of them.Carolyn Custer/AP

Kasson and his small team collected 36 infected cicadas during a quick trip around Chicago, and another 200 or so have been sent in from elsewhere. He’s still waiting for the results of an RNA analysis of the fungus.

Some cicada experts estimate that one in every 1,000 periodical cicadas is infected with the fungus, but that’s just a guess, says Gene Kritsky, a biologist at Mount St. Joseph University who has written a book about the fungus. This year’s unique double appearanceHe said the numbers could be skewed because healthy cicadas tend to stay higher in trees.

“This year’s fungal situation is business as usual and not particularly unusual,” Cooley said in an email.

Scientists debate whether the fungus burrows deep underground and then infects the cicadas that emerge after 13 or 17 years, or whether it infects newly hatched larvae as they make their way underground for more than a decade.

The fungus isn’t a parasite that kills its host, but rather needs to keep it alive, Casson said. Infected cicadas will try to mate with other cicadas, spreading the spores to their mates/victims. Males may also become hypersexual and pose as females to lure and infect other males, Casson said.

Test tubes containing live periodical cicadas infected with the fungus Massospora cicadina await field processing at the Morton Arboretum in Lisle, Illinois, on June 6, 2024.Carolyn Custer/AP

A related species of the fungus that infects annual cicadas in the West also produces psychoactive compounds in the cicadas that are more similar to hallucinogens like magic mushrooms, Kasson said. That’s why some people, even experts, confuse the amphetamines produced by infected 17- and 13-year cicadas with the highly hallucinogenic compounds in the annual insects, he said.

Either way, don’t try this at home. The cicada itself is edible, Not many people are infected.

Out of scientific curiosity, Casson experimented on one during this emergence, ensuring that it was taken from the body of a female, which was more sterile.

“It was really bitter,” Cason said, explaining that she quickly rinsed her mouth. “It tasted like poison.”

Source: www.nbcnews.com

Introducing smartphones gradually is more beneficial for children than banning them completely

“Let’s take cell phones out of schools.” “Social media is harmful to teens.”

Such messages are being broadcast around the world and appear to have reached a peak in recent days. In the UK, concerns about the harms of social media and screen time have led to Smartphone Free Children Campaign A government crackdown on smartphone use in schools has also begun, and ministers are considering banning the sale of smartphones to anyone under 16. Meanwhile, in the United States, Surgeon General Vivek Murthy this week called for social media platforms to require cigarette-style warning labels.

More than 40% of American children own a smartphone by age 10, and the concern is Excessive screen use can lead to health problemsThese include obesity, sleep disorders, depression and anxiety.

Certainly, some studies have documented this link, but as we explain in our feature, The Truth About How Social Media and Screen Time Affect Young People, the evidence that screen time causes widespread harm to children is not as strong or clear as some claim.

While we figure out the details, we must protect our children, especially those who are most vulnerable to the harmful influences of smartphones and social media. But depriving them entirely would be the wrong move.

The smarter approach is to give children access, even from an early age, in a controlled and measured way.

Imagine what a smartphone utopia might look like: It would be done in stages: instead of giving kids access to the entire internet at first, we’d allow them access to walled gardens, like kid-friendly TV channels.

In such a world, we would allow limited messaging with strict moderation that loosens with age, the system would allow parents access that diminishes over time, and all of this would be combined with ongoing digital literacy classes.

Smartphones, social media, and screens will continue to be a part of our children’s lives, no matter how many warning labels they carry, and now is the time to think seriously about how we give our kids the tools they need to navigate the realities of growing up online.

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Source: www.newscientist.com

The Methane Ocean on Saturn’s Moon Titan is Causing Coastal Erosion

Titan's liquid hydrocarbon ocean may have waves

NASA/JPL-Caltech/University of Arizona/University of Idaho

Saturn's largest moon, Titan, has rocky coastlines around its methane seas and lakes that appear to have been carved out by waves, and a NASA mission launching in 2028 may be able to get a closer look.

Titan is the only body in the solar system other than Earth that has liquid on its surface. It has lakes and oceans made of hydrocarbons such as liquid methane, ethane, and other organic molecules. Scientists think that winds in Titan's thick, nitrogen-rich atmosphere drive the waves in these lakes, but this has never been observed directly because Titan's atmosphere is too hazy to see through.

now, Rose Palermo Researchers from the U.S. Geological Survey in Florida and their colleagues found that the shape of Titan's coastline is best explained by the presence of waves that have eroded the ocean surface over eons.

Palermo and his team looked at the shorelines around Titan's largest oceans and lakes, including Kraken Mare and Ligeia Mare, and compared them to coastlines on Earth with known origins, such as Lake Rotoef in New Zealand, which initially formed by floods and later was eroded by waves. The team then created different simulations of Titan's oceans, including those in which the shores were eroded by waves or by dissolving their edges.

Photographed by NASA's Cassini spacecraft, Ligeia Mare on Saturn's moon Titan has a variety of edges that appear to have been carved by waves.

NASA/JPL-Caltech/ASI/Cornell

The researchers found that images of Titan's coastline, best depicted by wave simulations, resemble Earth's wave-eroded coastlines.

“It's still tentative, but I'm very excited about it.” Ingo Muller-Vodarg The Imperial College London researchers say that although the study did not observe waves themselves, it is very strong evidence that waves exist. Dune-like structures.

The only way to truly verify that waves exist is to send a spacecraft to the surface, like NASA's Dragonfly drone mission, scheduled to launch in 2028, Mueller-Vaudergues said.

Studying Titan's coastlines may also help us understand how the first coasts on Earth formed, Palermo says: “Titan is a unique laboratory for studying coastal processes because it is not influenced by humans or plants. It's a place where we can study coasts only as physical processes.”

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Source: www.newscientist.com

Is an aging NASA probe redefining the limits of our solar system?

NASA’s New Horizons spacecraft is hurtling out of our solar system at incredible speed. It’s currently about 8 billion kilometers from the Sun, and by the time you finish reading this article, it will be thousands of kilometers further into the frigid darkness. Space is lonely; even the giant planet Jupiter is just a tiny speck.

New Horizons is best known for getting the first proper glimpses of the dwarf planet Pluto in 2015, which it had previously only seen as a faint smudge. It also taught us a lot about the outer solar system and the tiny frozen worlds that float there. “It’s really been an Alice in Wonderland kind of story,” says Alan Stern, the mission’s principal investigator. “It’s been a magical experience, and we’ve made some amazing discoveries.”

But the dream isn’t over yet, because New Horizons may make a surprise final move. In early 2024, one of New Horizons’ detectors recorded an unexpected increase in the amount of dust it encountered. That material could have been created by collisions between rocky fragments, and astronomers now suspect that there may be many objects beyond the rubble-strewn Kuiper Belt, often considered the edge of the solar system. If so, the boundaries of the solar system would need to be redrawn, calling into question models of the formation of the solar system.

Stern and his colleagues are clearly hoping to take advantage of the rover’s unique location to learn more about this unexplored wilderness while they still can. “This is…

Source: www.newscientist.com

Rare Titan Arum blooms in Kew Gardens emitting scent of rotten flesh

June 18th, Corpse Flowers at Kew Gardens

Sebstian Kettley/RBG Cue

This gorgeous, but smelly, corpse flower bloomed on June 18th. Royal Botanic Gardens, KewIn London however it tends to be only for a short period, lasting only 24 to 36 hours.

Corpse Flower (Amorphophallus titanium) also known as Titan Aramgets its name from the foul smell it gives off, resembling rotting meat, which is so strong it can be heard for hundreds of metres. The smell is produced to attract rare pollinating insects, such as flesh flies and carrion beetles, to the short-lived flowers, and must be strong enough to do its job during the short period the plant is in flower, because the plant may not flower again for many years.

Strictly speaking, this up to 3 metre tall plant isn’t one flower, but many. The inner inflorescence, or spadix, emerges from a purple, pleated collar called a bract and looks like a yellow obelisk. The inflorescence, or cluster of flowers, lies in the protected area between the bract and the spadix.

If you happen to see and smell it, the smell may not be what you expect: it can change during the flower’s short lifespan and can smell like rotting flesh, as well as pleasant excrement or warm garbage.

This rare plant is endemic to the rainforests of the Indonesian island of Sumatra, but is cultivated in many botanical gardens around the world for its beauty and the crowds it attracts when it blooms. The first time it is known to flower outside of Sumatra was in 1889 at Kew Botanical Gardens.

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Source: www.newscientist.com

The glassy gel is as rigid as plastic and can extend up to seven times its original length.

SEI 209347890

Glassy gels are a new class of materials that are as stiff as plastic but extremely stretchy.

Meishan Wang, North Carolina State University

When you think of gel, you might imagine something sludgy, but the new gel-like material has been engineered to be strong and transparent like glass, yet flexible enough to stretch to almost seven times its original length.

Michael Dickey The North Carolina State University researchers say they discovered the “glassy gel” when student Meishan Wang was experimenting with ionic liquids and kept finding unexpected mechanical properties. The material they came up with is more than 50 percent liquid, yet it's as strong as the plastic in water bottles, and it's also highly stretchable and sticky. “It has a lot of great properties,” Wang says.

Each glassy gel is made up of long molecules called polymers mixed with ionic liquid (essentially liquid salt). The gels are transparent solids that can withstand up to 400 times atmospheric pressure, yet easily stretch up to 670 percent. Dickey says this could make them suitable for building soft robotic grippers or for 3D printing deformable materials.

He and his colleagues created glassy gels from mixtures of several polymers and liquid salts, and found that their strength and stretchability depended on the exact ratios used.

“By simply changing the ratio of the two materials, we can make something as stretchy as a rubber band or as hard as glass,” Dickey says.

This is because the material's stretchability comes from the ionic liquid depositing in the spaces between the stiff polymer molecules, pushing them apart, while its strength comes from electrostatic attraction between the charged particles in the liquid and the polymer, which prevents the particles from moving apart completely.

The glassy gel is also capable of self-repair; cuts or breaks can be repaired by applying heat, causing the molecules at the broken edges to rejoin. Richard Hoogenboom Researchers at Ghent University in Belgium say the technique could be useful in some cases where traditional plastics are used, but that the formulations may need to be tweaked to only soften at high enough temperatures to avoid accidental softening.

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Source: www.newscientist.com

The Revelation of Why Some Individuals Have Greater Resistance to the Novel Coronavirus

Volunteers were exposed to coronavirus as part of a scientific study

Koto Feja/Getty

By intentionally exposing people to the coronavirus that causes COVID-19, scientists have been able to understand why some people appear to be immune to infection.

As part of the first human COVID-19 challenge study conducted in 2021, an international group of researchers looked at 36 healthy people who had not tested positive for SARS-CoV-2 and had not been vaccinated.

The ancestral SARS-CoV-2 strain was sprayed into their noses. Nasal and blood samples were taken from 16 of the participants before exposure and then six to seven times over the next 28 days. All were also tested for SARS-CoV-2 twice daily.

Participants were split into three groups, team members said. Sarah Teichmann The study was conducted at the Cambridge Stem Cell Institute. In one group, six participants tested positive in both daily tests for more than two days and also had symptoms. In another group, three participants tested positive in one of two daily tests but not in the other and did not have symptoms, but for less than two days. In the final group, seven participants consistently tested negative for coronavirus.

In total, the researchers sequenced more than 600,000 blood and nasal cells across all subjects.

In the second and third groups, the researchers found that participants were producing more interferon (a substance that helps the immune system fight infection) in their blood in front of the nasopharynx (the top of the nose at the back of the throat where the nasal samples were taken). The interferon response was actually higher in the noses of participants in the second group than in the third group, Teichmann says.

These groups also did not have active infections within the immune cells T cells and macrophages, team members say. Marko Nikolic At University College London.

The results showed that high levels of gene activity HLA-DQA2 Exposure to SARS-CoV-2 helped prevent persistent infection.

Nikolic hopes that this discovery will improve understanding of the cellular responses involved in preventing COVID-19 and aid in the development of vaccines and treatments.

“With its carefully controlled design and real understanding of 'time zero' when infection occurs, this study will serve as a unique resource of previously uninfected SARS-CoV-2 participants to measure subsequent immune responses,” the study said. Jose Ordovas Montanez Harvard Stem Cell Institute

But most people have been exposed to “a true mosaic of SARS-CoV-2 variants,” not just the ancestral variant used in the study, so the results may not reflect cellular responses outside the testing environment, he says.

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Source: www.newscientist.com

What’s the real health impact of supermarket bread, as determined by obesity experts

When discussing diet and nutrition, opinions can often be divisive and passionate. Recently, I found myself in the middle of a debate surrounding supermarket bread that sparked unexpected backlash.

The controversy began after I wrote an article on “ultra-processed foods” (UPF). These foods are products of industrial processes that are difficult to replicate at home, including sweetened drinks, prepackaged foods, and most supermarket breads. In the UK, around 50% of our daily calories come from UPF (source).


UPF has garnered a negative reputation for several reasons. Firstly, these foods tend to be low in protein and fiber, making them easily digestible and calorically dense. Secondly, the processing of UPF often strips away natural flavors, leading to high amounts of added sugar, salt, and fat to enhance taste. Lastly, there are concerns that excessive consumption of UPF may lead to various health issues (British Medical Journal).

While the negative effects of UPF are well-documented, the term itself is vague, encompassing a wide range of foods from heavily processed items to minimally altered products like mass-produced supermarket bread.

In a response to my article, it was argued that real sourdough bread made through lactobacterial fermentation may offer health benefits that are lacking in supermarket bread. It was also noted that supermarket bread tends to be higher in salt and sugar, leading to potential weight gain.

While artisanal sourdough may provide some advantages over supermarket bread, it’s essential to consider the accessibility of such premium products to a broader demographic.

A balanced discussion on the prevalence of UPF in our food supply is necessary, but the demonization of supermarket bread, a staple for many households, may be unwarranted without substantial evidence of harm.

Source: www.sciencefocus.com

Webb Reveals the Inner Workings of the Crab Nebula

The NASA/ESA/CSA James Webb Space Telescope has provided stunning new images of the Crab Nebula, containing the highest-quality infrared data yet available to help astronomers investigate the detailed structure and chemical composition of this supernova remnant.

Webb's detailed analysis of the Crab Nebula's structure has helped astronomers continue to evaluate the leading theories about the origin of supernova remnants. Image credit: NASA/ESA/CSA/STScI/T. Temim, Princeton University.

The Crab Nebula is the result of a supernova explosion observed in 1054 AD by Chinese, Japanese, Arab and Native American astronomers.

Bright enough to be seen in amateur telescopes, this beautiful nebula lies 6,500 light-years away in the constellation Taurus.

Also known as Messier 1, NGC 1952, or Taurus A, the galaxy was first identified in 1731 by British astronomer, physician, and electrical researcher John Bevis.

In 1758, French astronomer Charles Messier rediscovered the faint nebula while searching for comets, and later added it to his celestial catalog as a “false comet” named Messier 1.

The nebula got its name from an 1844 drawing by Irish astronomer Lord Rosse.

The Crab Nebula is extremely unusual: its atypical composition and extremely low explosion energy had previously led astronomers to believe it was an electron-capture supernova, a rare type of explosion that occurs from a star with a less-evolved core made of oxygen, neon, and magnesium, rather than the more common iron nucleus.

Previous studies have calculated the total kinetic energy of the explosion based on the volume and velocity of the current ejecta.

Astronomers have estimated that the explosion had a relatively low energy (less than one-tenth the energy of a typical supernova) and that the source star's mass was in the range of eight to ten times that of the Sun, lying on the fine line between stars that undergo violent supernova explosions and those that do not.

However, there are contradictions between the electron capture supernova theory and observations of the Scorpio Nebula, especially the observed rapid motion of the pulsar.

In recent years, astronomers have also come to understand more about iron-collapse supernovae, leading them to believe that these types of supernovae could also produce low-energy explosions if the star's mass is low enough.

To reduce uncertainties about the nature of the Crab Nebula's protostar and explosion, Tee Temim of Princeton University and his colleagues used Webb's spectroscopy capabilities to zero in on two regions within the Crab Nebula's inner filament.

Theory predicts that due to the different chemical composition of the cores of electron capture supernovae, the abundance ratio of nickel to iron (Ni/Fe) should be much higher than that measured in the Sun, which contains these elements from earlier generations of stars.

Studies in the 1980s and early 1990s used optical and near-infrared data to measure the Ni/Fe ratios in the Crab Nebula and recorded high Ni/Fe abundances that seemed to favor an electron capture supernova scenario.

With its sensitive infrared capabilities, the Webb Telescope is currently advancing research into the Crab Nebula.

The study authors leveraged Webb's spectroscopic capabilities. Milli (mid-infrared instrument) to measure nickel and iron emission lines to get a more reliable estimate of the Ni/Fe abundance ratio.

They found that while this ratio is still high compared to the Sun, it is only slightly higher and much lower than previous estimates.

The revised value is consistent with electron capture, but does not exclude the possibility of iron-collapse explosions from low-mass stars as well.

High-energy explosions from more massive stars would produce Ni/Fe ratios closer to the solar abundance.

Further observational and theoretical work will be needed to distinguish between these two possibilities.

Webb extracted spectral data from two small regions within the Crab Nebula to measure abundances, and also observed the remnant's larger environment to understand the details of synchrotron radiation and dust distribution.

The images and data collected by MIRI allowed astronomers to isolate dust emissions within the Crab Nebula and map them in high resolution for the first time.

“By mapping the warm dust emissions with Webb and combining it with data on cold dust particles from NASA's Herschel Space Telescope, we have created a comprehensive picture of the dust distribution, with the outermost filaments containing relatively warm dust and cold particles spread out near the center,” the team said.

a paper The paper on the survey results is Astrophysical Journal Letters.

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Teatemimu others2024. JWST analysis of the Crab Nebula: Ni/Fe abundance constraints on pulsar winds, dust filaments, and explosion mechanisms. Apu JL 968, L18; Source: 10.3847/2041-8213/ad50d1

Source: www.sci.news

New study suggests Jupiter’s Great Red Spot may not be the permanent feature reported by Cassini

Jupiter’s Great Red Spot is perhaps the best-known atmospheric feature and a popular icon among the solar system’s objects. Its large oval shape, contrasting red color, and long lifespan make it easily visible with a small telescope. A new study led by scientists from the University of the Basque Country, based on historical measurements of its size and motion, shows that the present-day Great Red Spot was probably first reported in 1831 and is not a permanent spot observed by Giovanni Domenico Cassini and others between 1665 and 1713.



The Permanent Spot (PS) and the early Great Red Spot (GRS): (a) drawing of the PS by GD Cassini on 19 January 1672, (b) drawing by S. Swave on 10 May 1851, showing the GRS area as a clear ellipse bounded by a depression (depicted by a dashed red line). (c) photograph taken by AA Common on 3 September 1879 using a 91 cm reflecting telescope at Ealing (London). The GRS appears as a clear "dark" ellipse because it is red and the photographic plate is sensitive to violet-blue wavelengths. (d) photograph taken at Lick Observatory on 14 October 1890 using a yellow filter. All figures show astronomical images of Jupiter (south at top, east at left) to preserve the notes on the drawings. Image courtesy of Sánchez-Lavega others., doi: 10.1029/2024GL108993.

Jupiter’s Great Red Spot is the largest and longest-lasting known vortex of any planet in the solar system.

The formation mechanism that produced this feature is unknown, and its longevity is controversial.

It was also unclear whether the Great Red Spot was the dark oval nicknamed the “Eternal Spot” that astronomer Giovanni Domenico Cassini and others reported between 1665 and 1713.

“Speculation about the origin of the Great Red Spot dates back to the first telescopic observations by Giovanni Domenico Cassini, who in 1665 discovered a dark oval at the same latitude as the Great Red Spot, which he named a permanent spot, because it was observed by Cassini and other astronomers until 1713,” said Professor Agustin Sánchez Lavega from the University of the Basque Country.

“For the next 118 years, traces of it were lost, and it was only after 1831 that S. Schwabe again observed a clear, almost elliptical structure at the same latitude as the GRS. This can be considered the first observation of the present-day GRS, possibly of the infant GRS.”

“Since then, the Great Red Spot has been regularly observed by telescopes and by various space probes that have visited the planet up to the present day.”

In their study, the authors analysed the change in the size of the Great Red Spot over time, its structure, and the behaviour of two meteorological structures, the former permanent spot and the Great Red Spot.

To do so, they used historical sources dating back to the mid-17th century, shortly after the telescope was invented.

“Based on our measurements of its size and motion, we infer that it is highly unlikely that the current Great Red Spot is the permanent spot observed by Cassini,” Professor Sanchez LaVega said.

“The permanent spot probably disappeared sometime between the mid-18th and 19th centuries, which would put the lifespan of the red spot at least 190 years.”

“The Red Spot, which in 1879 measured 39,000 kilometres along its longest axis, has now shrunk to about 14,000 kilometres and is becoming rounder at the same time.”

“Furthermore, since the 1970s, several space missions have studied this weather phenomenon in detail.”

“Recently, various instruments on the Juno spacecraft in orbit around Jupiter have shown that the Great Red Spot is shallow and thin compared to its horizontal length. Its vertical length is about 500 km.”

To understand how this giant whirlpool formed, the astronomers ran numerical simulations using two complementary models of the behavior of thin vortices in Jupiter’s atmosphere.

Powerful winds prevail on this giant planet, flowing along parallels that alternate in direction and latitude.

To the north of the Great Red Spot, winds blow westward at 180 km/h, while to the south, winds blow in the opposite direction, eastward at 150 km/h.

This creates huge north-south shear in the wind speed, which is the fundamental element that allows vortices to grow internally.

The study explored a variety of mechanisms to explain the formation of the Great Red Spot, including the eruption of a giant superstorm like those rarely observed around its twin planet Saturn, or the merging of several smaller vortices caused by sheared winds.

The results show that although anticyclones form in both cases, their shapes and dynamic characteristics are different from those of the present-day Great Red Spot.

“We believe that if one of these anomalies had occurred, it, or its effects in the atmosphere, would have been observed and reported by astronomers at the time,” Prof Sanchez Lavega said.

In a third set of numerical experiments, the researchers investigated how the GRS may arise from known instabilities in the winds that they believe could produce elongated cells that surround and trap the GRS.

Such cells were early red spots, the proto-Great Red Spot, whose subsequent shrinkage would give rise to the compact, rapidly rotating Great Red Spot observed in the late 19th century.

The formation of large elongated cells has already been observed during the emergence of other major vortices on Jupiter.

“In our simulations, thanks to supercomputers, we were able to find that elongated cells are stable when they rotate around the Great Red Spot at the speed of Jupiter’s winds, which is what you would expect to form due to this instability,” said Dr Enrique García Melendo, an astronomer at the Polytechnic University of Catalonia.

Using two different numerical models, the scientists concluded that if the GRS rotated slower than the surrounding winds, it would break up and the formation of a stable vortex would be impossible.

And if it were very high, the properties of the primordial Great Red Spot would be different from those of the current Great Red Spot.

“Future studies will aim to reconstruct the Great Red Spot’s shrinkage over time and elucidate in more detail the physical mechanisms underlying its persistence,” the authors wrote.

“At the same time, we try to predict whether the Great Red Spot will collapse and disappear when it reaches its size limit, as happened with Cassini’s permanent spot, or whether it will remain stable at its size limit and persist for many years.”

of result Published in a journal Geophysical Research Letters.

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Agustin Sanchez Lavega others2024. Origin of Jupiter’s Great Red Spot. Geophysical Research Letters 51(12):e2024GL108993; doi:10.1029/2024GL108993

Source: www.sci.news

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.

topic:

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