Texas faces devastating wildfires amidst climate emergency

Unusually warm temperatures, dry grass, and a sudden strong wind cold front combined to create the conditions for the devastating wildfires that raged through parts of Texas this week.

The winds that sparked wildfires in the Texas Panhandle came at the perfect time for destruction, “like a hurricane hitting land at high tide,” said Texas climatologist John Nielson Gammon. Ta. He added that hot, dry temperatures, which may be promoted by climate change, helped create the conditions for these fires to start.

On Monday, temperatures reached the mid-80s in some parts of the state's arid region and several wildfires began burning.

The next day, arctic air swept in from the north on a severe cold front. Winds on either side of that front could exceed 50 miles per hour, causing flames to roar through the dormant grass, Nielsen-Gammon said. The cold front arrived in the late afternoon when wind speeds were highest and changed direction as it passed, maximizing the rate of fire spread.

It is not clear how the fire started.

Firefighters work at the scene of the Smokehouse Creek Fire near Amarillo in the Texas Panhandle on Tuesday.
Hanazuka Fire Department

“The timing of the weather during the day was probably the worst,” Nielsen-Gammon said. “If wildfires were to occur, these weather patterns would occur.”

The fire spread through the area so quickly that firefighters had little chance to extinguish it.

“Those fires were, all things considered, very fast-moving for a wildfire. We've seen speeds in the 5 to 10 mph range,” said National Weather Service meteorologist in Amarillo. Christian Rangel said. “The strong winds really helped push them around and get them out of control.”

The region's topography also plays a role, with open land facilitating fire establishment and rapid spread, while making firefighting difficult.

Although the area is mostly flat, it is characterized by “broken terrain” with sand and grass that makes it difficult to access, said Luke Canclairs, chief of forecasting services for the Texas A&M Forest Service. It can be difficult to do so. As a result, once a fire hit the plains, it was difficult to extinguish it quickly.

“A fire moving at about 8 miles per hour may not sound that fast, but when you have a large fire front and you're trying to contain a large area, it can far outpace the firefighting effort,” Kankleerts said. .

The Texas Panhandle is used to in-the-face winds and roller-coaster temperatures. But the fires would not have been as likely to occur if it weren't for unseasonably warm temperatures and dry conditions made more likely by climate change.

“This particular event would not have been as devastating had it happened at the same time several decades ago,” Nielsen-Gammon said. “These high temperatures can occur early in the season and usually occur when the grass is dormant, so there is a lot of dry fuel available.”

John Abatzoglou, a climatologist at the University of California, Merced, said wind was the biggest factor in the size of the nearly 1 million-acre fire, according to the federal government's wildfire tracking website Inchweb.

“This is primarily a wind-driven fire,” Abatzoglou said, adding that the role of climate change is “more subtle than we generally think.”

Abatzoglou said winds initially blew from the west, spreading the fire in the shape of an oval on the map, but then turned about 90 degrees and began pushing that line southward.

Abatzoglou said there is little hard evidence about how climate change is changing wind speeds.

Temperatures in the Borger area near where the fire started reached 85 degrees Fahrenheit on Monday, the news agency said. National Weather Service data.

Rangel said the Amarillo forecast area “has set records at many weather stations,” with relative humidity readings below 20 percent in many parts of the state and the landscape on the verge of flaming. added.

Source: www.nbcnews.com

Top 10 Groundbreaking Medical Advancements: Pure Moments of Eureka captured in Photos

The history of science is filled with moments of discovery, those “Eureka” moments when a theory is proven or a breakthrough is achieved. The latest image competition at Great Ormond Street Hospital, titled ‘A Moment of Discovery’, celebrates these breakthroughs.

Staff from Great Ormond Street Children’s Hospital NHS Foundation Trust (GOSH) and its partners have submitted images capturing significant milestones in research. The public voted on the three most popular images shortlisted by a panel of experts via social media.

The shortlisted images range from colorful micrographs to cartoon illustrations, offering a glimpse into the research conducted at GOSH. It is hoped that this research will lead to new treatments for rare and complex conditions, transforming the lives of children and young people with serious illnesses.

The winning image, taken by PhD student Giada Benedetti at the Zayed Pediatric Rare Disease Research Center (ZCR), shows exploding intestinal organoids revealing their inner workings.

Organoids are small three-dimensional tissue cultures derived from stem cells that can mimic different organs like the heart and liver in the human body.

In honor of Rare Disease Day on February 29, all winning and shortlisted images will be displayed at an event at the Zayed Pediatric Rare Disease Research Center.

Selected as a finalist – my lungs are on fire

These lung “mini-organs,” or organoids, were grown from stem cells to replicate the complexity of lungs. The image showcases cell nuclei in blue, cell membranes in red, and moving hair-like structures called cilia in yellow/orange. Photo courtesy of Giuseppe Cala at GOSH.

Shortlist – Active Glial Cells

The image showcases nerve helper cells, known as glial cells, with long fibrous structures that transport nutrients and oxygen to surrounding nerve cells. Photo courtesy of Lucien Bonfante at GOSH.

Finalist – Light of Life

The image shows the spinal cord of a zebrafish embryo with different neurons generated through asymmetric division. Photo courtesy of Atachapon Theppichaiyanond at GOSH.

Source: www.sciencefocus.com

The Purpose of Leap Year 2024: Understanding the Reason Behind It

It may surprise you, but the universe isn’t perfect, at least not from a human perspective. One clear example of this imperfection is the existence of leap years like 2024.

What is a leap year?

By definition, a leap year occurs every four years, adding an extra day to make the year 366 days long instead of the usual 365. This extra day falls on February 29th rather than the typical February 28th.

Why do leap years occur?

The discrepancy between a year (Earth’s orbit around the sun) and a day (Earth’s rotation) drives the need for leap years to align our calendar with the Earth’s journey around the sun. This misalignment accumulates over time, necessitating the addition of leap years to keep our calendar in sync with the seasons.

“Leap years play a crucial role in aligning our calendar with the Earth’s orbit around the sun,” explains Dr. Minjae Kim, a Research Fellow in Astrophysics at the University of Warwick.

The Julian calendar introduced by Julius Caesar in 46 BC added a day every four years, but it slightly overcorrected the discrepancy between the solar year and the calendar year. Reforms led to the Gregorian calendar in 1582, which provides rules for determining leap years, reducing the error rate to about one day every 3000 years.

Celebrities with leap year birthdays

  • Jack Rousma: NASA astronaut born on February 29, 1936.
  • Ja Rule: American rap legend born on February 29, 1976.
  • Pedro Sanchez Perez-Castechon: Prime Minister of Spain born on February 29, 1972.
  • Karen Jones: American competitive swimmer born on February 29, 1984.

Is it possible to create the perfect calendar?

Despite efforts to improve calendars, there is no perfect solution due to the dynamic nature of space. The concept of time harmonizing with natural rhythms is temporary, as our days get longer and Earth’s orbit changes over long timescales. For now, the Gregorian calendar remains adequate.

About our experts

Dr. Minjae Kim: Research Fellow in the Department of Physics at the University of Warwick, focusing on planetary science and dust signatures in debris disks around stars.

Dr. James McCormack: Assistant Professor in the Astronomy and Astrophysics Group at the University of Warwick, specializing in transiting exoplanets and the European Space Agency’s PLATO mission.

Source: www.sciencefocus.com

Webb unveils stunning new images of NGC 1559

NASA/ESA/CSA’s James Webb Space Telescope has captured new images of barred spiral galaxy NGC 1559.

This Webb image shows barred spiral galaxy NGC 1559, located approximately 32 million light-years away in the constellation Reticulata. Image credits: NASA / ESA / CSA / Webb / A. Leroy / J. Lee / PHANGS Team.

NGC 1559 is situated about 32 million light-years away in the southern constellation Rechi.

Also known as LEDA 14814, ESO 84-10, and IRAS 04170-6253, this galaxy was first observed in 1826 by Scottish astronomer James Dunlop.

NGC 1559 features extensive spiral arms filled with star formation and is receding from us at a speed of approximately 1,300 km/s.

It has a mass of around 10 billion solar masses, which may seem substantial, but it’s almost 100 times less than the mass of our Milky Way galaxy.

“NGC 1559 exhibits a massive spiral arm of active star formation moving away from us at 1,300 kilometers per second,” explained the Webb astronomers.

“Although NGC 1559 appears to be close to the Large Magellanic Cloud, one of the nearest clouds in the sky, this is merely a perspective illusion.”

“In reality, NGC 1559 is not physically near the Large Magellanic Cloud in space. It is actually isolated, lacking any nearby galactic companions or members of galaxy clusters.”

Images of NGC 1559 are composed of data from Webb’s two instruments: Mid-infrared measuring instrument (Miri) and near infrared camera (NIRCam).

“MIRI captures the glow of interstellar dust particles that trace the interstellar medium fueling future star formation,” the astronomers elaborated.

“NIRCam reflects starlight and reveals young stars hidden behind vast amounts of dust.”

“This instrument also detects emission from ionizing nebulae around young stars.”

The image of NGC 1559 was taken by the PHANGS team as part of Webb’s observation of 55 galaxies using instruments such as the Atacama Large Millimeter/Submillimeter Array (ALMA) and the NASA/ESA Hubble Space Telescope.

“By combining Webb’s unique view of dust and stars with data from these other facilities, we can delve into the detailed processes of star birth, life, and death in galaxies across the universe. Our goal is to gain new insights into this phenomenon,” stated the researchers.

“This program is also part of a Treasury Department initiative, allowing immediate access to the data for the scientific community and the general public,” they added.

“This enables us to conduct more research at a faster pace.”

Source: www.sci.news

NASA’s DART mission may have reshaped the asteroid moon Dimorphos

On September 26, 2022, NASA’s Double Asteroid Redirection Test (DART) mission successfully impacted Dimorphos, the natural satellite of the near-Earth binary asteroid Didymos. New numerical simulations show that the DART impact triggered global deformation and resurfacing of Dimorphos.

The asteroid moon Dimorphos was seen by NASA’s DART spacecraft 11 seconds before impact. His DRACO imager aboard DART captured this image from a distance of 68 km (42 miles). This image was the last one to include all dimorphos in the field of view. Image credit: NASA/Hopkins Applied Physics Laboratory.

DART was a planetary defense mission that demonstrated the possibility of using kinetic impactors to alter the orbits of asteroids.

The collision was successful and highly effective, resulting in Dimorphos’ orbital period around Didymus being shortened from its original 11 hours and 55 minutes to 33 minutes.

The LICIACube Unit Key Explorer (LUKE) instrument aboard the cubesat took images of the system between 29 seconds and 320 seconds after impact, showing the ejecta stream and other debris that spread for several kilometers from the impact site. revealed a complex pattern.

Furthermore, the dramatic brightening of the Didymos system due to solar illumination of the ejected impact ejecta was observed by ground-based and space-based telescopes for many weeks after the impact.

These three Hubble images capture the breakup of Dimorphos when it was intentionally collided by DART on September 26, 2022. The top panel, taken two hours after impact, shows the ejecta cone (estimated at 1,000 tons of dust). The center frame shows dynamic interactions within the Didymos-Dimorphos binary system that begin to distort the cone of ejecta patterns approximately 17 hours after impact. The most notable structure is a rotating windmill-shaped feature. The windmill is connected to Didymus’s gravitational pull. In the bottom frame, Hubble captures debris being pushed back into the comet-like tail by the pressure of sunlight on tiny dust particles. This spreads out into a column of debris, with the lightest particles traveling fastest and furthest away from the asteroid. The mystery deepens after Hubble recorded the tail splitting into two for several days. Image credit: NASA/ESA/STScI/Jian-Yang Li, PSI/Joseph DePasquale, STScI.

In a new study, University of Bern scientist Sabina Raducan and colleagues use realistic constraints on the mechanical and compositional properties of dimorphos, informed by DART’s initial results, to create a state-of-the-art impact The DART impact was modeled using physical code.

The simulations that best match observations of the impact suggest that Dimorphos is weakly cohesive, similar to asteroids Bennu and Ryugu, and lacks large rocks on its surface.

The researchers suggest that Dimorphos may be a pile of debris formed by the rotational shedding and re-accumulation of material ejected from Didymos.

Their model also suggests that DART’s impact may not have created an impact crater, but instead may have changed the shape of the moon as a whole, a process known as global deformation, which could have been caused by material from within. It also indicates that it may have caused the resurfacing of Dimorphos.

The discovery provides further insight into the formation and characteristics of binary asteroids and could have implications for future exploration, including ESA’s Hera mission and asteroid deflection efforts.

“ESA’s future Hera mission may discover reformed asteroids rather than well-defined craters,” the authors concluded.

their paper It was published in the magazine natural astronomy.

_____

SD Raducan other. Physical properties of the asteroid Dimorphos obtained from the DART impact. Nat Astron, published online on February 26, 2024. doi: 10.1038/s41550-024-02200-3

Source: www.sci.news

Magnetic particles transform water droplets into skilled tightrope walkers

New technology allows water droplets to be guided precisely around obstacle courses to trigger chemical reactions

Jonathan Knowles/Getty Images

By placing tiny magnetic particles inside ordinary water droplets, you can turn them into liquid acrobats. Droplets can climb steps, jump over obstacles, and initiate chemical reactions. This level of control could be useful for drug delivery and the creation of more complex lab-on-a-chip technologies.

Fan Shilin He and his colleagues at Sun Yat-sen University in China created a surface with tiny grooves and covered it with a superhydrophobic, or wet-resistant, varnish. They know that a water droplet resting on such a groove can spontaneously jump up due to the pressure difference between the bottom of the droplet, which is deformed by the small groove, and the rounded and less constrained top part. I did.

The researchers wanted to create this pressure difference on demand. They added small magnetic particles to each droplet and placed an electromagnet beneath the groove. When the electromagnet was turned on, some of the particles, or droplets, were drawn into the groove. When I turned it off, the water droplet shape bounced and flew upwards as if from a slingshot.

Using this technique, the team was able to enable droplets to hop down millimeter-scale stairs and overcome small obstacles. The researchers were also able to direct a droplet into the narrow space between two wires and connect a circuit to light a light bulb.

Xiao Yan Researchers from China’s Chongqing University say this is a creative way to control pressure-based droplet jumps and could become a valuable tool for precisely transporting chemical droplets. It has said.

In one experiment, researchers plunged and mixed droplets into a liquid chemical sample under a microscope lens, allowing them to observe the resulting chemical reaction from start to finish. Another experiment involved mixing two droplets with a third in a closed box, which would have been ruined if the researchers had had to open the box to let air in. The reaction was initiated remotely.

Such precise chemical control can be applied to drug delivery. Huang hopes the technology will also advance “lab-on-a-chip” technology, an effort to miniaturize complex biochemical experiments that typically require a lot of space and glassware. He proposes a “lab-on-stacked chip” in which droplets jump vertically between levels to generate many reactions in parallel.

topic:

  • chemistry /
  • fluid mechanics

Source: www.newscientist.com

Causes and Occurrences of Total Solar Eclipses

A solar eclipse is a surprising cosmic coincidence that causes the moon to appear as large as the sun.

Chance Bush/Albuquerque Journal (via AP)

People travel thousands of miles to see a solar eclipse. There’s nothing like darkness falling and the excitement ripple through the crowd. A total solar eclipse will soon grace the skies in parts of Central America and North America, and some places outside the total path will be able to see a partial solar eclipse. So now is the perfect time to ask what exactly a solar eclipse is.

When one celestial object is hidden from view by another celestial object moving between them, astronomers call the event an “occultation.” Strictly speaking, a total solar eclipse is the occultation of the sun by the moon.

A total solar eclipse occurs when the moon and sun line up perfectly, with the moon moving in front of the sun and blocking nearly all of the sun’s light. From the path of totality, or the area of ​​the Earth where a total solar eclipse is visible, the sun almost disappears. This part of the eclipse can last up to 7.5 minutes. The solar eclipse on April 8th will last 4 minutes and 27 seconds.

What causes solar eclipses?

There are many different types of solar eclipses, but all occur when the moon passes in front of the sun, blocking some or all of the light seen from certain parts of the Earth. By pure cosmic coincidence, the moon is about 400 times smaller than the sun, but the sun is about 400 times farther away, so the moon and sun appear to be the same size in the sky. When the two line up perfectly during the new moon phase, when the moon is between the Earth and the sun, the moon can block all of the sun’s light. This is a total solar eclipse.

During a solar eclipse, the moon casts two shadows. The central part of the shadow where light does not reach is called the umbra. The outer partial shadow is known as the penumbra. Only light coming from part of the sun’s disk can reach here. During a total solar eclipse, the path of totality is land within the umbra. On April 8, the road will be 185 kilometers wide and will cross North America from Mexico through the United States and Canada. However, the total path can be as narrow as 150 kilometers. The penumbra covers a much larger area and a partial solar eclipse can be seen in those locations.

Conceptual Imagery Lab at NASA Goddard Space Flight Center

What types of solar eclipses are there?

A partial solar eclipse occurs when the moon blocks only part of the sun’s light. This occurs when the viewer is within the penumbra. Before and after totality, you can see the moon slowly eclipsing the sun in a partial solar eclipse. However, because the moon’s central shadow completely misses the Earth, only a partial solar eclipse may be visible from anywhere on Earth.

An annular solar eclipse occurs when the moon’s elliptical orbit moves it farther from Earth than normal, blocking most of the sun’s light but leaving behind a so-called ring of fire. A hybrid solar eclipse occurs when some parts of the world see a total solar eclipse, while other parts see an annular solar eclipse. Total solar eclipses, hybrid solar eclipses, and annular solar eclipses are all types of “central” solar eclipses, meaning that the umbra is projected somewhere on Earth.

Solar eclipse in 2024

On April 8th, a total solar eclipse will pass over Mexico, the United States, and Canada. Our special series covers everything you need to know, from how and when to see a solar eclipse to the strangest solar eclipse experience of all time.

How often do solar eclipses occur?

Every year, anywhere from two to five solar eclipses are visible somewhere around the world. A total solar eclipse occurs on average every 18 months. However, in certain locations on Earth, the portion of the Earth where a total solar eclipse is visible is so small that a total solar eclipse is only seen about once every 400 years.

What is a lunar eclipse?

A lunar eclipse occurs when the moon moves through the shadow that Earth casts in space. These events always occur during a full moon when the moon is on the opposite side of Earth’s sun. But they don’t happen every full moon because our moon’s orbit is tilted around the Earth compared to Earth’s orbit around the sun.

Do solar eclipses always occur in pairs?

A solar eclipse occurs when the Earth, Sun, and Moon line up (a so-called syzygation), so a solar eclipse is always accompanied by a lunar eclipse two weeks before and after it. This year, a lunar eclipse will occur on March 24th, two weeks before the solar eclipse on April 8th. However, it will be a penumbral lunar eclipse, meaning only the Earth’s outer shadow will hide the moon.

topic:

  • solar eclipse/
  • solar eclipse 2024

Source: www.newscientist.com

The Surprising Influence of Your Skin on Your Well-being and Longevity

woman applying body cream

Shutterstock/Rawpixel.com

In winter, the backs of your hands can become dry, red, and cracked. Maybe you find yourself applying more moisturizer. Otherwise, itching and pain can be a big hindrance.

Cracked skin is annoying and uncomfortable, but it's not as serious as something like high blood pressure. However, that assumption may not hold, as with skin aging.

Growing evidence suggests that skin damage can have knock-on effects on other parts of the body, causing inflammation, muscle and bone loss, and even cognitive decline. The more your skin deteriorates, the faster the rest of your skin ages. This new perspective means that our skin not only reflects the signs of aging, but also contributes to it. There's even preliminary evidence that taking better care of your skin may slow down the negative effects of aging and improve your overall health.

Our skin is one of the first areas of our body to show signs of aging. Especially in active areas such as the outer corners of the eyes, wrinkles may increase and age spots may appear. Although these changes may seem to be literally skin deep, the importance of the skin to the rest of the body should not be underestimated. “The skin is the largest organ in the body,” he says. wendy borag At Augusta University in Georgia, USA.

And it's not just the size. Skin is essential for survival. The outer layer of the epidermis is impermeable to water, so body fluids, the source of life, are not lost to the air. If someone causes damage to a large area…

Source: www.newscientist.com

I discovered the reason behind the distinct flavor of oranges

Many compounds contribute to orange flavor

Photography/Shutterstock

Chemical analysis revealed 26 compounds responsible for orange’s distinctive flavor. This discovery will help plant scientists create disease-resistant orange hybrids that are just as tasty as the original variety.

In recent decades, citrus greening disease, also known as Huanglongbing, has devastated citrus production around the world. orange (Citrus sinensis) say they are particularly affected by this disease Anne Plott at the American Horticultural Research Institute in Florida.

Plotto and his colleagues wanted to see if it was possible to create a hybrid that was resistant to citrus greening disease while retaining the characteristic orange flavor.

To identify the chemicals responsible for this flavor, researchers analyzed 179 juice samples from a variety of citrus fruits, including oranges and mandarins.Citrus reticulata), three-leaf mandarin orange (Citrus trifoliata) and its hybrids. Trained citrus testers also tried each sample and rated how much it tasted like orange juice.

They found that the strongest orange-flavored juices all contained 26 specific compounds. Seven of these compounds are a type of chemical called esters, which seem to be the key to differentiating the taste of oranges from tangerines.

Plott and her team then conducted genetic analysis of the fruit and discovered genes involved in the synthesis of all seven esters they named. C. sinensis alcohol acyltransferase 1.

“This gene is expressed more in varieties that produce more esters,” team members say jen fan at the University of Florida.

The research could eventually help create disease-resistant hybrids with a rich orange flavor, Plott said. “This discovery may allow us to screen citrus hybrid seedlings early to get the desired orange flavor, rather than waiting 10 to 15 years for the trees to bear fruit,” she said. says.

topic:

Source: www.newscientist.com

Slowing Alzheimer’s Disease Progression: How Light and Sound Can Remove Toxins from the Brain

Cross-section of a mouse brain highlighting neurons that appear to release molecules that increase toxin clearance

Tsai Laboratory/MIT Picower Laboratory

A new explanation has emerged for why an experimental treatment for Alzheimer’s disease that involves flickering sounds and lights may help slow cognitive decline. This frequency appears to strengthen the brain’s waste processing network, helping to remove beta-amyloid and other toxic proteins that contribute to memory and concentration issues.

“Once we understand the mechanism, we can probably understand how to further optimize this whole concept and improve its effectiveness,” he says. Cai Li Hui at Massachusetts Institute of Technology.

The treatment involves exposure to light that flashes at a frequency of 40 times per second, or 40 hertz, and to a bass sound, also at 40 hertz. Typically, stimulation is given for one hour per day.

The key to this new approach is that large networks of brain cells naturally fire in sync with each other at different frequencies, known as brain waves. Brain waves around 40 Hz are common when people are concentrating and forming or accessing memories.

In 2016, Tsai’s team wondered if 40Hz stimulation could enhance cognitive performance in Alzheimer’s patients, since visual or auditory stimulation at a certain frequency is known to enhance brain waves at that same frequency. I decided to investigate.

Their group and other researchers have shown that this reduces amyloid accumulation in mice with Alzheimer’s disease and has cognitive benefits. Small trial in people with this condition, an even larger trial is underway. However, it is unclear how this treatment works, and another idea is that it boosts the function of immune cells in the brain.

Well, the special light and sound appears to work by enhancing the function of the brain’s drainage system, also known as the glymphatic system.

In the latest study, Tsai’s team conducted a series of experiments to study the mechanism of treatment in mice that were genetically modified to have amyloid buildup that normally occurs with age and to have worse memory than typical mice. carried out.

As expected, when the animals were exposed to light and sound, the amount of amyloid decreased. The new findings were that during treatment, the amount of cerebrospinal fluid entering the brain increased, and the amount of waste fluid leaving the brain through the glymphatic vessels increased.

This appears to occur because nearby blood vessels pulsate more, which may help glymph fluid flow through the blood vessels, allowing more water to flow into the glymph system.

The research team also found that the activity of a particular type of brain cell known as an interneuron appears to cause an increase in glymph flow by releasing a molecule called vasoactive intestinal peptide. When the research team chemically blocked the production of this molecule, the treatment no longer accelerated amyloid clearance.

Miken Nedergaard A professor at the University of Rochester in New York who helped discover the glymphatic system says the discovery is consistent with what we already know about it. “The brain, blood, and cerebrospinal fluid are all contained within the skull. When the blood volume expands, the brain tissue cannot be compressed, so the cerebrospinal fluid volume must also move.”

In the accompanying article natural medicineDr. Nedergaard says that a better understanding of the mechanisms of toxin removal in the brain “could be the key to unlocking that.” [their] Treatment Possibilities.”

topic:

Source: www.newscientist.com

80% of microplastics can be removed from tap water by boiling it.

Most microplastics in tap water can be removed by boiling.

Yuri Nedopekin/Alamy

Boiling tap water before use can remove at least 80 percent of the potentially harmful small plastic particles it contains.

Nanoplastics and microplastics (NMPs) are pieces of plastic such as polystyrene, polyethylene, and polypropylene that range in diameter from 0.001 to 5 millimeters. Although the health effects are still being studied, researchers suspect they may be harmful to humans.

Eddie Zen and colleagues from China's Jinan University took samples of tap water and measured levels of NMP and found that the average concentration was 1 milligram per liter. The samples were then boiled for 5 min and then cooled. NMP levels were then remeasured and found to have decreased by more than 80%.

“NMP intake from boiled water consumption was estimated to be two to five times lower than the daily intake from tap water,” Zeng said. “This simple but effective boiling water strategy can 'decontaminate' NMPs from household tap water and potentially harmlessly reduce human exposure to NMPs through water consumption.”

Zeng said NMP was removed by being incorporated into the crystalline structure of limescale, which is formed from calcium in the water. Hard water, which contains more calcium, removed more particles than soft water, which contains less calcium.

Bringing water to its boiling point was a major contributing factor to how efficiently these crystal structures were created. “Boiling water has several other benefits, including killing bacteria and parasites and removing traces of heavy metals,” he says.

“The way they demonstrated how things are deposited through the boiling process was amazing,” he says. caroline goshott lindsay At the University of Glasgow, UK. But the world should seek to solve the problem of microplastics in drinking water long before they reach homes, she added. “We should consider modifying drinking water treatment plants to remove microplastics,” she says.

topic:

Source: www.newscientist.com

Greenland’s melting ice could trigger a heat wave in Europe this year

Melting ice in Greenland could worsen extreme weather across Europe

REDA & CO srl/Alamy

Europe's 10 hottest and driest summers in the past 40 years have all come after a particularly large amount of fresh water was released from the Greenland ice sheet, meaning southern Europe will experience an especially hot summer this year. Maybe you are doing it.

They say this link occurs because the excess meltwater triggers a series of amplifying feedbacks that affect the strength and position of the atmospheric jet stream over Europe. Marilena Ortmans At the UK National Marine Centre.

“2018 and 2022 were the most recent examples,” she says. 2022 saw extreme heat and numerous bushfires across Europe, with high temperatures reaching 40°C (104°F) in parts of the UK for the first time.

These feedback effects, on top of the underlying warming trend from fossil fuel emissions, mean Europe will become even hotter and drier in coming decades as the melting of the Greenland ice sheet accelerates. Then Mr. Ortmans says:

“This is on top of the warming that is already happening due to increases in greenhouse gases,” she says.

Hotter heat waves and drier droughts are expected as the planet warms, but in some regions, such as Europe, recent heat waves and droughts have been even more extreme than climate modeling projects. Several studies have linked these extreme events to changes in the strength and position of the Arctic jet stream. The Arctic jet stream is a band of upper-level winds whose location and strength have a significant impact on weather.

But it's not clear what causes these changes, Ortmans says. Now, she and her colleagues are analyzing weather observations from the past 40 years, and the results show that extreme weather is ultimately the result of a period of increased ice melt in Greenland. It is said that there is.

“Observational statistical associations are very powerful,” she says.

The excess meltwater leads to a shallow layer of freshwater that extends south of the North Atlantic Ocean. This layer does not easily mix with the warm, salty ocean water below, causing the ocean surface to be colder than normal in winter.

This makes the gradient between this colder water and warmer water further south even more extreme, strengthening the weather front aloft. As a result, wind patterns strengthen, pushing warm water flowing northward, the North Atlantic Current, further north than usual. This further amplifies the temperature gradient.

“The front that forms between an area of ​​cold fresh water and an area of ​​warm ocean water is the main source of energy for storms,” ​​she says.

In a 2020 study, Ortmans suggested: This process leads to an increase in storms. during one winter.

Now, Oltmans' team suggests that these winter changes have lasting effects into the following summer. “Two years after the freshwater anomaly occurred, we are still seeing significant signs,” she says.

The researchers found that stronger temperature gradients lead to stronger jet streams across Europe, making the weather in southern Europe even hotter and drier. Then, as the unusually cold water recedes, the jet stream moves north, bringing hot, dry weather to northern Europe.

“We have discussed the individual links in this feedback chain before,” Ortmans says. “What we did in this study is bring these links together.”

Computer models miss this chain of feedback because they don't include factors such as large fluctuations in meltwater from year to year, she says.

“The association between Atlantic freshwater anomalies and subsequent European summer weather proposed in this study is interesting and relevant to current scientific research on long-term predictions of summer weather, especially “If that relationship holds true for future summers,” he says. adam scaife He works on long-term forecasts at the UK Met Office.

“I think this study is somewhat convincing,” he says. Fei Luo At the Singapore Climate Research Center. But when it comes to predicting summer weather, looking at the previous year's snowmelt isn't as helpful as looking at winter weather conditions, Luo said.

But Oltmans is confident enough to predict that Europe will experience more heatwaves and droughts in the coming years as Greenland's ice melts further in the summer of 2023. “I think southern Europe will experience strong heat anomalies this summer,” she says.

These are likely to become even more powerful in 2025, after which they will begin to impact Northern Europe. “We expect Northern Europe to experience another strong heatwave and drought, not this year, but in the next few years.”

topic:

Source: www.newscientist.com

Prohibiting social media use for children does not address the root issues.

When considering the most effective way to protect children’s mental health, the idea of banning social media often comes up. Recent events in the UK, such as the tragic murder of Brianna Gee, have reignited discussions on the dangers of social media for children. However, scientific evidence does not strongly support the notion that social media directly causes mental health issues in children.

Social media has been around for quite some time and has brought many positive aspects to the lives of young people. It allows them to connect with others, pursue their interests, and show support in times of tragedy. Studies have shown that increased social media use does not necessarily decrease life satisfaction for most children.

While it may seem that social media is linked to a decrease in life satisfaction for some adolescents, the opposite is not always true. Evidence supporting the idea of social media addiction in children is limited. Without a clear causal relationship between social media use and mental health issues, banning social media for children may not be the solution.

Are most children addicted to social media and smartphones?

Using the term “addiction” in reference to social media and smartphone use may be misleading. While some children may develop bad habits related to their use, it does not necessarily constitute a true addiction. Weaning children off social media is often easier than addressing addictive behaviors related to substances.

Is it possible that a social media ban will actually be enforced?

Enforcing a ban on social media for children poses many challenges, both legally and morally. Children have rights to access and enjoy social media, and restricting their access may infringe on these rights. Past attempts to ban social media use, such as South Korea’s “Cinderella Law,” have shown limited effectiveness in improving children’s well-being.

How can children develop a healthy relationship with screens?

As parents, it is important to guide children in developing a healthy relationship with screens, including social media. Teaching them to self-regulate their behavior and manage their screen time can prepare them for adulthood. Simply banning social media may not address the underlying issues of human behavior and the attention economy.

Source: www.sciencefocus.com

VLT spots metallic scar on surface of white dwarf

A dynamically active planetary system orbits a significant portion of the white dwarf. These stars often exhibit surface metals accreted from a disk of debris. However, the complete journey of a planetesimal from its star-grazing orbit to its final dissolution in its host star is poorly understood. In a new paper, Astrophysics Journal Letter astronomers report the discovery that stars exist that are contaminated with cold metals. WD 0816-310 It cannibalized heavy elements from a planetary body as large as the dwarf planet Vesta.

WD 0816-310 is a magnetic white dwarf star located 63 light-years away in the constellation Papis. Image credit: L. Calçada / ESO.

Dr Stefano Vanullo, an astronomer at the Armagh Observatory and Planetarium, said: 'It is common for some white dwarfs – slowly cooling embers of stars like our Sun – to cannibalize parts of planetary systems. known,” he said.

“Now we find that the star's magnetic field plays a key role in this process, causing scars on the white dwarf's surface.”

The metal signatures the researchers observed on WD 0816-310 are concentrations of metal imprinted on the white dwarf's surface.

Professor Jay Farihi of University College London said: “These metals come from fragments of a planet the size of, or possibly even larger than, Vesta, which at about 500 kilometers in diameter is the second largest asteroid in the solar system. I have proven that.”

To observe WD 0816-310, astronomers FORS2 equipment upon ESO's super large telescope (VLT).

They also relied on archival data from VLT. X shooter instrument This is to confirm the survey results.

The authors noticed that the strength of the metal detections changed as the star rotated, indicating that the metals were concentrated in specific areas on the white dwarf's surface, rather than being spread smoothly across the surface. Suggests.

They also found that these changes were synchronized with changes in the white dwarf's magnetic field, indicating that this metallic scar is located at one of its magnetic poles.

Taken together, these clues indicate that the magnetic field funneled metal into the star, creating the scar.

“Surprisingly, the material was not evenly mixed on the star's surface, as theory predicted. Instead, this scar was a concentrated patch of planetary material that guided falling debris. “We've never seen anything like this before,” said John Landstreet, a professor at Western University.

“ESO offers a unique combination of capabilities needed to observe faint objects like white dwarfs and make sensitive measurements of the star's magnetic field,” Vanullo said.

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Stefano Vanullo other. 2024. Discovery of magnetically induced metal accretion on contaminated white dwarfs. APJL 963, L22; doi: 10.3847/2041-8213/ad2619

Source: www.sci.news

Webb uncovers incredible black hole in the ancient cosmos

Using the NASA/ESA/CSA James Webb Space Telescope, astronomers observed a very red quasar-like object. A2744-QSO1 Its color suggests that A2744-QSO1's black hole lies behind a thick veil of dust obscuring much of its light. The researchers also measured the black hole's mass (40 million solar masses) and found it to be much more massive compared to its host galaxy than what has been seen in more localized examples. . This discovery suggests that it may represent the missing link between black hole seeds and the first luminescent quasars.



A composite color image of A2744-QSO1. Image credit: Furutaku other, doi: 10.1038/s41586-024-07184-8.

“We were very excited when Webb started transmitting its first data,” said Dr. Lukas Furtak, a postdoctoral researcher at Ben-Gurion University of the Negev.

“As we were scanning the data coming in for the UNCOVER program, three very compact objects with red flowers stood out to us.”

“Because of its 'red dot' appearance, we immediately suspected it to be a quasar-like object.”

“Using a numerical lensing model we built for the Abell 2744 galaxy cluster, we found that the three red dots are multiples of the same background light source seen when the universe was just 700 million years old. “We determined that it must be an image of Adi Zitlin, also from Ben-Gurion University in the Negev.

“Analysis of the object's color shows that it is not a typical star-forming galaxy,” said Professor Rachel Bezanson, an astronomer at the University of Pittsburgh.

“This further supports the supermassive black hole hypothesis.”

“Together with its compact size, it became clear that this was probably a supermassive black hole, but it was still different from other quasars discovered earlier.”

The astronomers then analyzed the JWST/NIRSpec spectrum of A2744-QSO1.

“The spectrum was just shocking,” said Professor Ivo Rabe of Swinburne University of Technology.

“The spectrum obtained by combining the signals from the three images and the lens magnification corresponds to 1,700 hours that Webb observed the object without a lens, making it the deepest spectrum Webb obtained for a single object in the early universe. Masu.”

“Using the spectrum, we were able to not only confirm that this red compact object is a supermassive black hole and measure its precise redshift, but also estimate its mass based on the width of its emission line. We were able to get a solid estimate,” Dr. Furtak said.

“The gas orbits the black hole's gravitational field, achieving extremely high velocities not seen in other parts of the galaxy.”

“Due to the Doppler shift, the light emitted from the accreting material is redshifted on one side and blueshifted on the other side, depending on its velocity.”

“This makes the emission lines in the spectrum wider.”

But this measurement brought yet another surprise. The black hole's mass appears to be disproportionately large compared to the mass of its host galaxy.

“All the light in that galaxy would have to fit within a small region about the size of a modern star cluster,” said Dr. Jenny Green, an astronomer at Princeton University.

“The source's gravitational lensing magnification provided an exquisite constraint on size.”

“Even if you pack all possible stars into such a small region, the black hole will end up being at least 1% of the total mass of the system.”

“In fact, it has now been discovered that several other supermassive black holes in the early Universe exhibit similar behavior, which provides insight into the growth of black holes and host galaxies, and the interactions between them. This provides some interesting insights, but this is not well understood.”

Astronomers do not know whether such supermassive black holes grow from the remains of stars, for example, or perhaps from material that collapsed directly into black holes in the early universe.

“In some ways, this is an astrophysical chicken-and-egg problem,” says Professor Zitlin.

“Currently we don't know whether galaxies or black holes formed first, how big the first black holes were, and how they grew.”

“Recently, many more such 'little red dots' and other active galactic nuclei have been detected in the Webb, so we hope to have a better idea soon.”

of the team result appear in the diary Nature.

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LJ Furutak other. High black hole-to-host mass ratio in the lensed AGN of the early Universe. Nature, published online on February 14, 2024. doi: 10.1038/s41586-024-07184-8

Source: www.sci.news

Small Fish in the Cyprinidae Family Can Produce Sounds Over 140 dB, Say Ichthyologists

Danionella cerebrumThis translucent fish species, only 12 mm long, produces high-amplitude sounds exceeding 140 dB (1 µPa relative at a distance of 1 body length). This is comparable to a jet engine taking off at a distance of 100 meters.



Danionella cerebrum It has a pair of extrinsic indirect muscles that house the drumming cartilage. When the sonic muscles contract, they pull the fifth rib forward, pulling on the cartilage and increasing tension. When the cartilage is suddenly released, it rapidly impinges on the swim bladder, producing a short, loud pulse. Bursts of pulses are produced by bilateral alternating or unilateral muscle contractions. In summary, this mechanism allows for loud, stereotypical sounds elicited in structured sequences, making it unique for vertebrate acoustic communication and ultrafast skeletal locomotion that exceeds the limitations of muscle contraction velocity. It will be a solution. Image credit: Ralf Britz, Senckenberg Natural History Collections.

“Oyster oyster shrimp can make crackling noises of up to 250 dB with their claws,” he said. Dr. Ralph Blitzichthyologist at the Senckenberg Natural History Collection.

“The flightless kakapo’s mating call can reach 130 dB, and elephants can make up to 125 dB of noise with their trunks.

“Fish, on the other hand, are generally considered to be fairly quiet members of the animal kingdom.”

“But certain fish species can be surprisingly noisy. For example, male redfin midshipmanfish attract females with an audible vibrato of about 100 Hz and 130 dB.”

In a new study, Dr. Blitz and his colleagues looked into Danionella cerebruma small teleost fish with the smallest brain of any known vertebrate.

“This small fish can emit over 140dB of sound at a distance of 10-12mm, which is comparable to the noise of a plane taking off at a distance of 100m, which is highly unusual for such a fish. 'It's a small size,' Dr. Blitz said.

“We sought to understand how the fish manage this and what mechanisms are involved in this outcome.”

Using a combination of high-speed video, microcomputed tomography, gene expression analysis, and differential methods, the researchers discovered that: Danionella cerebrum Males have unique sound-producing equipment, including drumming cartilage, specialized ribs, and fatigue-resistant muscles.

“This device accelerates the drumming cartilage with a force of more than 2,000g and slams it against the swim bladder, producing rapid and loud pulses,” Dr. Blitz said.

“These pulses chain together to produce calls for bilateral alternating or unilateral muscle contractions.”

Due to its small size and lifelong light transmission, Danionella cerebrum It is a new model organism for biomedical research.

This species lives in the shallow, murky waters of Myanmar.

“It is likely that competition between males in this visually restricted environment contributed to the development of specialized mechanisms for acoustic communication,” Dr Blitz said.

The results of this study cast doubt on the conventional concept that the speed of skeletal movement in vertebrates is limited by muscle movement.

“Understanding unusual adaptations Danionella cerebrum “This extends our knowledge of animal locomotion and highlights the remarkable diversity of propulsion mechanisms in different species,” the authors said.

“This contributes to a broader understanding of evolutionary biology and biomechanics.”

“Sounds made by others are Danionella The species has not yet been studied in detail. It would be interesting to know how their sound production mechanisms differ and how those differences relate to evolutionary adaptations. ”

“Combined with its lifelong transparency, this genus Danionella This provides a unique opportunity to compare the neural mechanisms underlying sound production between different species. ”

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

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Verity ANO Cook other. 2024. A superfast sound production mechanism in one of the smallest vertebrates. PNAS 121 (10): e2314017121; doi: 10.1073/pnas.2314017121

Source: www.sci.news

Where and when can you view the solar eclipse of 2024?

In a total solar eclipse, the moon blocks the sun’s light.

Scott Sadie/tahoelight.com/Alamy

A total solar eclipse is coming to North America. On April 8, the moon will pass between the Earth and the sun, perfectly aligned to block the entire disk of the sun in a phenomenon called totality. It will be visible from a strip of land that stretches from Mexico across the United States into Canada.

The eclipse will begin in the Pacific Ocean, about halfway between North America and New Zealand, and will begin to be visible off the west coast of Mexico at 8:42 a.m. local time. It begins as a partial solar eclipse, with the moon slowly moving to cover more and more of the sun. The totality event was first observed in Mexico at 9:38 a.m. local time.

As the sun and moon move across the sky, the eclipse will be visible over a 185-kilometre-wide area of land known in the United States as totality. It will pass through 13 states, from Texas to Maine, and enter southern Ontario, Canada. The last place to see the eclipse on land will be Newfoundland, where the sun’s visibility will return to normal at 5:16 p.m. local time.

The duration of totality varies by location, from less than 2 minutes to nearly 4.5 minutes. This is because the moon’s orbit around the Earth is not a perfect circle, and neither is the Earth’s orbit around the sun, so the distances between the three bodies change throughout the day.

Solar eclipse in 2024

On April 8th, a total solar eclipse will pass over Mexico, the United States, and Canada. Our special series covers everything you need to know, from how and when to see a solar eclipse to the strangest solar eclipse experience of all time.

During a total solar eclipse, the moon’s shadow moves across the ground at speeds of over 2400 kilometers per hour, forming a dark patch that darts along the ground. In this shadow, the temperature drops rapidly and the sky becomes strangely dark, making planets and stars visible even during the day. Total solar eclipses are important to scientists because they provide a rare opportunity to measure the outermost layer of the sun, called the corona. This tenuous layer is much fainter than the Sun’s disk, making it difficult to observe normally.

Viewers in areas just outside the total path will also be able to see the eclipse, but it will only be partial, with the moon covering a smaller portion of the sun. A partial solar eclipse will last about 3 hours. Partial solar eclipses, which include the period just before and after a total solar eclipse, must be viewed through a special solar filter. Such filters are available in the form of eclipse glasses. However, regular sunglasses do not provide sufficient protection for the viewer’s eyes. Do not look directly at the sun without a solar filter, even during a partial solar eclipse.

If you don’t have eclipse glasses, don’t despair. A partial solar eclipse can still be seen, just not directly. You can use any object with holes, such as a colander or paper with pinholes, to project an image in the shape of an eclipse onto a screen or onto the ground. Even between the leaves of the trees the ground is speckled with strange sunlight that changes like a crescent moon.

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Source: www.newscientist.com

Eco-friendly dyeing method for denim could lessen the environmental impact of jeans

Harmful chemicals are used to dye jeans blue

Getty Images

A new technique that dyes denim using chemicals that turn blue in sunlight could reduce the environmental impact of jeans production.

Blue denim is dyed with indigo. Indigo is a compound that was once extracted from plants, but is now usually synthesized. Harmful chemicals such as sodium dithionite are required to dissolve indigo in water so that it can be used for dyeing. These chemicals produce toxic fumes that can harm the health of textile workers and can also cause toxic pollution of wastewater.

now, Ditte Hededam Werner Researchers at the Technical University of Denmark have instead developed a new process that uses a natural precursor of indigo called indican.

“Indican is also a natural product, so it's not artificial or weird,” says Hededam-Werner. “But the good thing about this is that it's soluble, so you can basically just soak the fabric, which you can't do with indigo. So many harsh chemicals simply This made it a very attractive solution to this problem because it could be omitted.”

However, there is one important drawback. Indican is colorless, so the compound must be converted to indigo after being applied to the material. One way to do this is to leave it in the sun for a few hours.

“I don't know if consumers like it or not, but if you wear Indian-soaked jeans in the sun, they turn blue over time,” says Hededam-Werner. “You think it's a gimmick, don't you? You can do it.”

The research team has discovered two methods that can provide the faster, more reproducible results required by modern manufacturing. One method uses plant enzymes and the other uses electric light.

Using light is a simpler process that reduces the environmental impact of dyeing by 73% compared to using indigo. European Commission indicators It takes into account carbon emissions, land use, water consumption, and ozone layer depletion. Using enzymes led to even greater reductions of 92%.

Hededam-Werner said that with further research, the process could become cheaper and more efficient, but major obstacles still stand in the way, not least of which is the production of the 4 billion pairs needed. The aim is to establish a supply chain for 80,000 tons of Indican. Number of jeans manufactured each year.

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Source: www.newscientist.com

Artificial Intelligence creates personalized 3D printed prosthetic eyes

A man with artificial eyes not made by AI

Stephen Bell, Ocupeye Ltd.

Prosthetic eyes designed with artificial intelligence and 3D printing could benefit more people by requiring 80% less time for human experts compared to traditional manufacturing methods. Small trials also suggest that this approach leads to adequate prostheses in most cases.

For example, in the UK, Approximately 1 in 1,000 people wears a prosthetic eye., it takes a highly trained ophthalmologist to take an impression of the eye socket. Many people wearing such prostheses also have orbital implants that replace lost eye volume and create a surface to which muscles can be reattached, allowing natural eye movement. Masu. A prosthesis is placed over this to give it a natural appearance.

The standard process for making a prosthetic limb takes about eight hours; Johan Reinhardt Researchers at the Fraunhofer Institute for Computer Graphics in Darmstadt, Germany, have developed a method to automatically design and 3D print an implant that fits into a wearer's eye socket and aesthetically matches the remaining eye. .

“It's more comfortable to do an optical scan than to have someone pour this alginate.” [mould-making material] It seems difficult to make an impression on the eye socket, especially for children. [sit through] This is the procedure,” Reinhardt said.

In the new process, an optical coherence tomography scanner uses light to create a 3D model of a person's missing eye, so the back of the prosthesis can be designed to fit snugly. A color image of the remaining eye is also taken to ensure an aesthetic match.

The data is collected into an AI model, a design is created, and then 3D printed on a machine that can operate at a resolution of 18 billion droplets per cubic centimeter.

Once the prosthesis is printed, a human eye doctor can polish and adjust it for the perfect fit. This task takes only 20% of the time of the existing process.

3D printed prosthetic eye designed by AI

Johann Reinhardt, Fraunhofer IGD

In a trial of 10 people at Moorfields Eye Hospital in London, only two people found these prostheses did not fit properly. Neither has orbital implants, which Reinhardt says poses problems for scanners and AI designers.

The team hopes to improve the process to significantly reduce the cost required to create convincing prosthetics and make them available to more people. However, Reinhardt says it is unlikely that future prosthetics will be created without human experts.

“We think of this like a tool for ophthalmologists,” he says. “So this is not going to replace an eye doctor, but it's a new process that they can use, and we think it's going to give them better results in terms of appearance.”

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Source: www.newscientist.com

An undisclosed ice base uncovers ethereal cosmic particles in Antarctica

Scientists have faced a challenge for nearly a century: How do you detect the undetectable, like the elusive neutrino? But now, in a groundbreaking discovery, neutrinos from elsewhere in the Milky Way have been detected for the first time, shedding light on a new era of neutrino astronomy.

The discovery of neutrinos has opened up new possibilities, and researchers like Steve Sclafani from the University of Maryland are excited about this new frontier. Neutrinos, the second most abundant elementary particles in the universe, are notoriously difficult to detect due to their elusive nature. When Austrian physicist Wolfgang Pauli proposed their existence in the 1930s, he thought they could never be detected, but he was proven wrong in 1956.

The discovery of neutrinos from outside the Milky Way was made possible by the IceCube Neutrino Observatory, a massive telescope located near the South Pole. By detecting high-energy neutrinos from distant galaxies, scientists are uncovering the mysteries of cosmic particle accelerators. These accelerators, like supermassive black holes, can provide clues about the origins of cosmic rays and other cosmic phenomena.

Small particles, huge targets

The IceCube detector, operated by a collaboration of scientists from around the world, works by detecting Cherenkov radiation emitted when high-energy neutrinos interact with the ice. This innovative approach allowed researchers to distinguish Milky Way neutrinos from other background signals, leading to the detection of hundreds of neutrinos over a 10-year period.

By studying the distribution of these neutrinos, scientists hope to learn more about the origins of cosmic rays and other high-energy phenomena in our galaxy. With plans to expand the IceCube observatory and improve detection methods, the future of neutrino astronomy looks promising.

Birth of neutrino astronomy

The detection of high-energy neutrinos from the Milky Way marks a new era in astronomy, providing researchers with a unique tool to study cosmic phenomena. By tracking these neutrinos back to their sources, scientists hope to uncover the mechanisms behind cosmic particle accelerators and other cosmic mysteries.

Neutrino astronomy offers a new perspective on the universe, allowing researchers to peer into the heart of energetic and turbulent environments near supermassive black holes. This discovery opens up a whole new window on the universe, providing invaluable insights into the workings of the cosmos.

New perspective

Neutrino astronomy has the potential to revolutionize our understanding of the universe, offering a rare glimpse into the inner workings of cosmic particle accelerators and other energetic phenomena. By studying the origins of high-energy neutrinos, researchers can uncover the mysteries of the cosmos and explore new frontiers in astrophysics. Exciting times lie ahead for neutrino astronomy, with new discoveries and advancements on the horizon.

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About our experts

Mirko Hünefeld from Dortmund University of Technology and Steve Sclafani from the University of Maryland are leading scientists in the field of neutrino astronomy. Their contributions to the IceCube observatory have helped advance our understanding of the universe and unlock new insights into cosmic phenomena.

Source: www.sciencefocus.com

Unusual Fish with Mouth that Extends to Resemble a Trunk

A hinged mouth that extends its proboscis to feed at the bottom of the aquarium.

Alison Evans

Found only in rivers and forest ponds in West Africa, this fish has a protruding trunk-like snout that allows it to suck in food or breathe air like a snorkel.

hinge(Fractolemus ansorgii) has what biologists call an expandable proboscis, a tubular structure that can be folded onto the head and extended upward or downward. The lips of the proboscis are lined with tooth-like structures made of keratin, which the fish uses to scrape up algae and other debris.

Alison Evans Researchers at George Washington University in Washington, D.C., used dissection, videography, and CT scans to uncover the jaw's complex structure.

Unlike all other fishes, where the jaw joint is located at the back of the mouth, the hinge mouse's jaw joint is located at the front of the head. The lower jaw is tipped back and pointed toward the throat. The upper jaw is connected to the lower jaw by ligaments and is part of the proboscis. “You can think of the upper jaw more or less hanging onto the skin of the proboscis,” Evans says. This is why the structure can extend far from the head.

Hingemouths offer “a novel mechanical solution to a ubiquitous challenge faced by all fish: how to acquire food in viscous fluid media,” Evans says.

She also observed the fish swimming up to the surface and using its proboscis “like a snorkel” to suck in air. This can be a useful feature in forest pools where oxygen levels can be low.

Scientists aren't sure how hinges evolved because fossil evidence is scant. “The family, fractoremus“The family Quneridae is thought to have originated in the mid-Cretaceous period, but no intermediate forms have yet been found in the fossil record,” says Evans.

“The most important thing for me is that scientists remain curious about the world’s little weirdos,” she says.

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Source: www.newscientist.com

This ‘zombie’ cannibal star was caught feasting on his siblings

White dwarfs, known as “man-eating stars” by scientists, are not just a concept from a Stephen King novel set in space. They are born through the process of swallowing surrounding planets and asteroids, leaving visible scars.

Researchers have made a groundbreaking discovery in solving the mystery of these cannibal stars by finding traces of metal on the surface of one such white dwarf star for the first time ever.

“We’ve never seen anything like this before,” said study co-author John Landstreet, a professor at Western University in Canada. These findings are reported in the Astrophysics Journal Letter.

The white dwarf in question, WD 0816-310, is now the size of Earth and is the remnants of a star that was once as large as the Sun.

Using the Very Large Telescope (VLT) at the European Southern Observatory in Chile, researchers detected the concentrated metals on the scar of the cannibal star using the VLT’s FORS2 instrument, often referred to as the “Swiss Army Knife.”


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Experts believe that a planet or asteroid disintegrated as it neared the white dwarf, forming a ring of debris around the dead star. WD 0816-310 then consumed part of this debris ring, leaving behind traces of specific chemicals on its surface, akin to evidence of food theft around a child’s mouth.

Additionally, scientists observed variations in the strength of metal detections on the star as it rotated, resembling changes in the magnetic field.

It was discovered that the magnetic field drew these metallic elements into the man-eating star, concentrating them at its poles and creating a distinctive “scar” in those areas.

These observations provide valuable insights into the composition of exoplanets and shed light on how stars interact with planetary systems even after their “death,” showcasing that WD 0816-310 is not just a “man-eating” star but also a “zombie” star.

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Source: www.sciencefocus.com

Hubble Observes NGC 1841 Globular Cluster

This new image from the NASA/ESA Hubble Space Telescope shows the globular star cluster NGC 1841 in the Large Magellanic Cloud.



This Hubble image shows the globular cluster NGC 1841 about 162,000 light-years away in the constellation Mensa. The color images include ultraviolet, optical, and near-infrared observations from both Hubble's Wide Field Camera 3 (WFC3) and Survey Altitude Camera (ACS). Three filters were used to sample different wavelengths. Color is obtained by assigning different hues to each monochromatic image associated with an individual filter. Image credits: NASA / ESA / Hubble / A. Saragedini / F. Niederhofer.

NGC1841 It is located approximately 162,000 light years away in the constellation Mensa.

The cluster is discovered It was proposed by British astronomer John Herschel on January 19, 1836.

Also known as ESO 4-15, this galaxy is part of the Large Magellanic Cloud, a satellite galaxy of our Milky Way.

“Satellite galaxies are galaxies that are gravitationally bound in orbit around a larger host galaxy,” Hubble astronomers said in a statement.

“While we usually think of our galaxy's closest galactic companion as the Andromeda galaxy, it would be more accurate to say that the Andromeda galaxy is the closest galaxy that does not orbit the Milky Way.”

“In fact, our galaxy is orbited by dozens of known satellite galaxies much closer than Andromeda, the largest and brightest of which is the Large Magellanic Cloud, which is easily visible to the naked eye even from the southern hemisphere. can.”

Globular clusters, such as NGC 1841, are very old systems of stars bound together by gravity into a single structure about 100 to 200 light-years in diameter.

These objects contain hundreds of thousands, or perhaps millions, of stars. The large mass in the cluster's rich stellar center pulls the stars inward, forming a star ball.

These are among the oldest objects known in the universe, relics from the earliest era of galaxy formation.

It is believed that all galaxies contain globular clusters. There are at least 150 such objects in our Milky Way galaxy.

“There are many globular star clusters in the Large Magellanic Cloud,” the astronomers said.

“These objects lie somewhere between open clusters (much less dense and tightly bound) and small, compact galaxies.”

“Increasingly sophisticated observations have revealed that the stellar populations and other characteristics of globular clusters are diverse and complex, but how these dense clusters form is poorly understood. yeah.”

“But all globular clusters have a certain consistency. They are so stable that they can persist for long periods of time, and therefore can be very old.”

“This means that globular clusters often contain large numbers of very old stars, making them similar to 'fossils' in the sky.”

“Just as fossils provide insight into the early development of life on Earth, globular clusters like NGC 1841 provide insight into the very early formation of stars in galaxies.”

Source: www.sci.news

Study finds that butterfly and moth genomes have remained remarkably stable over 250 million years of evolution

This stability exists despite the incredible diversity in wing patterns, sizes, and caterpillar morphology across more than 160,000 species worldwide today, according to one study. new paper It was published in the magazine natural ecology and evolution.



lissandra belargas. Image credit: Eric Silvestre.

Butterflies and moths (in order) Lepidoptera) make up 10% of all described animal species and are extremely important pollinators and herbivores in many ecosystems.

In a new study, Professor Mark Blaxter and colleagues from the Wellcome Sanger Institute set out to understand the processes driving the evolution of chromosomes in this highly diverse group.

They analyzed and compared more than 200 high-quality chromosome-level genomes of butterflies and moths.

They identified 32 ancestral chromosomal components; Merian element Thanks to the work of pioneering 17th century entomologist Maria Sibylla Merian, most butterfly and moth species have remained intact since their last common ancestor more than 250 million years ago.

With the exception of a single ancient fusion event between two chromosomes that led to the 31 chromosomes found in most species today, the chromosomes of most modern species correspond directly to these ancestral Merian elements.

Researchers discovered that not only are chromosomes incredibly stable, but the order of genes within them is also stable.

They discovered several species with small changes, mainly involving the fusion of small autosomes and sex chromosomes. This highlights the role of chromosome length as a driver of evolutionary change.

However, scientists believe that the blue butterfly (lissandra) and the group containing cabbage butterflies (Pieris) ignored these genomic structure constraints.

These groups underwent large-scale chromosomal reshuffling, including large-scale chromosome reshuffling through chromosome breakage and fission and fusion.

This study improves our understanding of the factors that lead to genetic diversity in these insects. This will guide efforts to protect and conserve specific species facing unique challenges and environmental changes related to climate change.

“The chromosomes of most butterflies and moths living today can be directly traced back to 32 ancestral Merian elements that existed 250 million years ago,” said Dr. Charlotte Wright, researcher at the Wellcome Sanger Institute. said.

“It is surprising that even though the species has diversified extensively, its chromosomes have remained surprisingly intact.”

“This calls into question the idea that stable chromosomes may limit species diversification. Indeed, this feature may be the basis for building diversity. We We hope to find clues about rare groups that have circumvented these rules.”

“Studies like this that allow us to delve into these evolutionary processes are only possible through efforts like the Darwin Tree of Life Project, which generate high-quality, publicly available genome assemblies,” Blaxter said. the professor said.

“We are stepping up these efforts with Project Psyche, where we aim to sequence all 11,000 butterfly and moth species in Europe in collaboration with collaborators across the continent.”

“As important pollinators, herbivores, and food sources in a variety of ecosystems, and as powerful indicators of ecosystem health, a deeper understanding of the biology of butterflies and moths through Project Psyche will This will be useful for future research on adaptation and speciation for biodiversity conservation.”

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CJ light other. Comparative genomics reveals the dynamics of chromosome evolution in Lepidoptera. Nat Ecole Evol, published online on February 21, 2024. doi: 10.1038/s41559-024-02329-4

Source: www.sci.news

Radcliffe waves found to exhibit oscillations by astronomers

Our Sun is within 300 parsecs (about 1,000 light-years) of a 2,700-parsec (about 9,000 light-years) long sinusoidal dense gas cloud known as the Radcliffe wave. The wavy shape of this structure was discovered using 3D dust mapping, but initial kinematic investigations of its oscillatory motion were inconclusive. Radcliffe waves oscillate in the plane of the Milky Way galaxy, radiating away from the galaxy's center, according to a new study.

Radcliffe waves next to the sun (yellow dot) in a cartoon model of the Milky Way. The blue dots are a group of baby stars.The white line is the theoretical model by Konietzka other. It describes the current shape and movement of the wave. The magenta and green lines show how the waves will move in the future. Image credit: Ralf Konietzka / Alyssa Goodman / Worldwide Telescope.

“By using the movement of baby stars born in gas clouds along Radcliffe waves, we can track the movement of the natal gas and show that the Radcliffe waves are actually rippling,” says Ralph.・Dr. Konietzka said. He is a student at Harvard University and the Smithsonian Center for Astrophysics.

In 2018, astronomers mapped the 3D location of a stellar nursery in the sun's galactic neighborhood.

By combining new data, ESA's Gaia Mission Using a data-intensive “3D dust mapping” technique, they noticed an emerging pattern, leading to the discovery of the 2020 Radcliffe wave.

“This is the largest coherent structure that we know of, and it's in our immediate vicinity,” said Dr. Katherine Zucker, an astronomer at the Harvard University & Smithsonian Center for Astrophysics.

“It's been there all along. We just didn't know it because we weren't able to build high-resolution models in 3D to show the distribution of gas clouds near the Sun.”

Although the 3D dust map clearly showed that Radcliffe waves were present, sufficient measurements were not available at the time to confirm whether the waves were moving.

But in 2022, astronomers used a new release of Gaia data to assign 3D motion to young star clusters in Radcliffe waves.

By understanding the location and movement of the clusters, they were able to confirm that the entire Radcliffe wave was indeed undulating, moving like what physicists call a “traveling wave.”

“Traveling waves are the same phenomenon you see in sports stadiums, where people take turns standing and sitting to do waves,” Konietzka said.

“Similarly, star clusters along Radcliffe waves move up and down, creating patterns that travel through the galaxy's backyard.”

“In the same way that fans in a stadium are pulled back into their seats by Earth's gravity, Radcliffe waves are oscillated by the Milky Way's gravity.”

No one yet knows what causes Radcliffe waves or why they behave the way they do.

“Now we can test all the different theories about why the waves formed in the first place,” Dr. Zucker said.

“Those theories range from the explosion of a giant star called a supernova to disturbances outside the galaxy, such as a dwarf satellite galaxy colliding with the Milky Way,” Konietzka added.

“It turns out we don't need significant dark matter to explain the motion we observe.”

“The gravity of ordinary matter is enough to move waves.”

Furthermore, the discovery of this oscillation has raised new questions about the predominance of these waves in both the Milky Way and other galaxies.

Radcliffe waves appear to form the backbone of the Milky Way's closest spiral arms, so the ripples in these waves may be due to the oscillations of galactic spiral arms in general, making galaxies even more dynamic than previously thought. It may suggest that you are doing something.

“The question is: What causes the displacement that causes the ripples that we see?” said Professor Alyssa Goodman, an astronomer at Harvard University and the Smithsonian Center for Astrophysics.

“And does it happen throughout the galaxy? In every galaxy? Does it happen sometimes? Does it happen all the time?

of result appear in the diary Nature.

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R. Konietzka other. Radcliffe waves are oscillating. Nature, published online on February 20, 2024. doi: 10.1038/s41586-024-07127-3

Source: www.sci.news

New Moons Found Around Uranus and Neptune by Astronomers

The three newly discovered moons (S/2023 U1, S/2002 N5, and S/2021 N1) are the faintest ever discovered around Uranus and Neptune using ground-based telescopes.



Discovery image of Uranus’ moon S/2023 U1 using the Magellan Telescope on November 4, 2023. Image credit: Scott Sheppard.

The new Uranian moon, tentatively named S/2023 U1, was first discovered by astronomers at the Carnegie Institution for Science on November 4, 2023. Scott Sheppard using the Magellan Telescope at the Las Campanas Observatory.

At just 8 km (5 miles), it is probably the smallest of Uranus’ moons. It takes 680 days to circumnavigate the ice giant.

S/2023 U1 will eventually be named after a character from a Shakespeare play, following Uranus’ outer moon naming conventions.

This discovery brings the total number of moons on this giant icy planet to 28.

Dr. Sheppard also used the Magellan telescope to discover S/2002 N5, the brighter of two newly discovered Neptune moons.

The moon’s diameter is about 23 km (14.3 miles), and it takes almost nine years to circumnavigate the ice giant.

The dimmer moons of Neptune were discovered by Dr. Sheppard and his colleagues using the Subaru telescope.

The star, named S/2021 N1, is about 14 km (8.7 miles) in diameter and has an orbital period of almost 27 years.

S/2002 N5 and S/2021 N1 were both first seen in September 2021.

Both have enduring names based on the 50 Nereid sea goddesses from Greek mythology.

“The orbit around Neptune of S/2002 N5 is determined using observations from 2021, 2022, and 2023, indicating that it was discovered near Neptune in 2003, but is still orbiting the planet. “We were able to trace it back to an object that was lost before it was confirmed,” Sheppard said.

S/2023 U1, S/2002 N5, and S/2021 N1 have far-flung, eccentric, and inclined orbits that occurred when Uranus and Neptune were formed from rings of dust and debris surrounding them, or it suggests that they were captured by the gravity of these planets shortly after our sun is in its infancy.

All giant planets in our solar system, regardless of their size or formation process, have a similar composition of outer moons.

“Even Uranus, which is tilted sideways, has a moon population similar to other giant planets orbiting the sun,” Dr. Sheppard said.

“And Neptune, which likely captured the distant Kuiper Belt object Triton, an event that could disrupt its lunar system, has an outer moon that looks similar to its neighbors. “

This new moon also indicates the existence of a dynamic orbital group of outer moons around Uranus and Neptune, similar to those seen around Jupiter and Saturn.

At Uranus, S/2023 U1 has an orbit similar to Caliban and Stefano.

At Neptune, S/2021 N1 has an orbit similar to Psamate and Neso, and S/2002 N5 has an orbit similar to Thao and Laomedeia.

These groupings suggest that the once larger parent moon was shattered, perhaps by a past collision with a comet or asteroid, leaving shattered debris in an orbit similar to the original larger moon. There is.

Many small lunar fragments are likely present in these groups, but they are generally too small to be efficiently observed with current technology.

These groupings of moons indicate that the early solar system was a very chaotic place, with constant movement and collisions between different objects.

Source: www.sci.news

Cretaceous Dinosaurs with Armored Bodies had Two Cheek Horns

A new genus and species of ankylosaurid dinosaur have been identified from two specimens discovered in southeastern China.

type specimen of Datai Inliangis Rebuilt on site. The head, neck, and thorax of the specimen were discovered and extracted from a single block. Image credit: Xing other., doi: 10.18435/vamp29396.

named Datai Inliangisthe newly discovered dinosaur species roamed the Earth during the Late Cretaceous period, about 96 million to 90 million years ago.

ancient beast was a member strongosaursa group of club-tailed armored dinosaurs that reached a peak of diversity in the latest Cretaceous period.

“Ankylosaurids are iconic armored dinosaurs that characterized the terrestrial vertebrate fauna of Asia and Laramidia (western North America) during the Late Cretaceous period,” said a paleontologist from the China University of Geosciences. Rida Singh And my colleagues.

“The earliest members of this clade are known from the Early Late Cretaceous of Asia, but there is little consensus on how they relate to anatomically derived and chronologically younger forms. are not obtained.”

“In southeastern China, Cretaceous red sand beds extend into a basin from Zhejiang to Guangdong.”

“However, horizons corresponding to the early Late Cretaceous remain poorly sampled.”

Two well-preserved immature skeletons Datai Inliangis It was collected from the Zhoutian Formation in southeastern China.

The specimens were found combined, with one head placed on top of the other, representing slightly different stages of the ontogeny of the skeleton.

“This is the first definitive vertebrate skeleton, let alone an armored dinosaur skeleton, excavated from the Ganzhou Formation,” the paleontologists said.

According to the authors: Datai Inliangis It is characterized by having two cheekbones/square zygomatic angle.

“The primary horn develops in the posteroventral horn of the skull and projects posterolaterally,” the researchers explained.

“There is a small attached horn just in front of this that hides the jaw joint when viewed from the side.”

“Morphologically, it is intermediate to older Asian ankylosaurids (e.g. crichton pelta and Giyumperta) and derived post-Cenomanian ankylosaurines (e.g. pinacosaurus),” they added.

“Phylogenetic analyzes broadly support this assessment.”

“The new species will either be placed in the Asian ankylosaurine subfamily, which is close to the lineage of the derived taxon, or it will form a sister lineage.” pinacosaurus

“Based on these insights, Datai This genus represents an important addition to the Early Late Cretaceous vertebrate fauna of southeastern China and highlights the region's future potential for a better understanding of the origins and early evolution of ankylosaurids. ”

of discovery is reported in Vertebrate anatomy, morphology, and paleontology.

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L. Shin other. 2024. A new armored dinosaur with double cheek horns that lived in the early Late Cretaceous of southeastern China. Vertebrate anatomy, morphology, and paleontology 11; doi: 10.18435/vamp29396

Source: www.sci.news

Delta Airlines offers eclipse viewing flight as airlines seek to profit from solar phenomenon

Passengers who book special Delta flights will have the opportunity to witness the total solar eclipse in April from a unique perspective at 30,000 feet.

The airline revealed on Monday that it will be offering flights from Dallas-Fort Worth to Detroit on April 8, allowing passengers to maximize their time within the eclipse’s “total path.”

The eclipse is anticipated to be a significant event as it travels through various populated areas of North America, including parts of Mexico, the continental United States, and eastern Canada. In the U.S. alone, millions of sky gazers from Texas to Maine will have the chance to witness this rare astronomical occurrence.

A solar eclipse happens when the moon moves between the Earth and the sun, temporarily blocking the sun’s light. Within the approximately 100-mile-wide strip known as the Path of Totality, observers will witness the moon completely obscuring the sun, creating a darkened afternoon sky.

Delta Airlines is providing eclipse enthusiasts with another option to experience the April event. The flight announced on Monday will be the airline’s second full charter scheduled for April 8. The initial flight from Austin, Texas to Detroit was announced on February 19 and sold out within 24 hours, according to the company.

The Austin to Detroit flight (Delta Flight 1218) is on an A220-300 aircraft, departing from Texas at 12:15pm Central Time and arriving in Detroit at 4:20pm Eastern Time.

The flight from Dallas-Fort Worth to Detroit (Delta Flight 1010) is operated on a large A321neo plane, departing Texas at 12:30 PM (Central Time) and landing in Detroit at 4:20 PM (Eastern Time).

While the flights are designed to maximize time within the total path, they are subject to potential changes due to factors like weather conditions and air traffic control.

For detailed booking information, visit the following website: Delta.com.

The upcoming solar eclipse is poised to be a major draw for travel and tourism, with many businesses already capitalizing on it. Hotels are offering special solar eclipse packages, while state tourism departments are organizing various events tied to the cosmic phenomenon.

During the April eclipse, the total path will traverse through states like Texas, Oklahoma, Arkansas, Missouri, Illinois, Kentucky, Indiana, Ohio, Pennsylvania, New York, Vermont, New Hampshire, and Maine. In certain areas of Michigan and Tennessee, totality may be visible if weather conditions are clear.

In other parts of the continental U.S., observers will witness a partial solar eclipse, where the moon appears to “take a bite” out of the sun and only partially obscures it in the sky.

To safely observe the eclipse, use eclipse glasses or a pinhole projector to avoid eye damage. Never look directly at the sun during a solar eclipse, even when it is partially or mostly covered by the moon.

Source: www.nbcnews.com

Can Wasabi Aid in Preserving Ancient Egyptian Papyrus Artifacts?

Ancient Egyptian papyrus scrolls can be damaged by fungi

Paul Williams / Alamy

Wasabi steam is powerful enough to kill fungi growing on painted papyrus pieces without damaging the fragile craft or altering the appearance of the vibrant colors.

A unique disinfection strategy could help archaeologists and museums preserve documents written on paper made from the papyrus plant, which has been used for thousands of years in ancient Egypt, Greece, and the Roman Empire. “Biological degradation of papyrus is a global problem,” he says. Hanadi Saada At the Grand Egyptian Museum in Egypt.

Fungi can damage delicate papyrus, but some disinfectants can be harmful as well. So Sarda and his colleagues are researching less irritating, “greener” treatments. In this experiment, a paste of wasabi (a popular Japanese seasoning derived from a plant related to horseradish and mustard) was mixed and placed on aluminum foil next to a papyrus sample.

Instead of risking historic papyrus artifacts, researchers prepared replicas for experiments. Samples of modern papyrus were painted in different colors such as red, yellow, and blue and heated in an oven at 100°C (212°F) for 120 days to simulate the natural aging of papyrus over 1000 years. . Finally, they were exposed to several fungal species known to parasitize archaeological papyri.

After 3 days, wasabi treatment removed the fungal contamination without affecting the pigments of the papyrus samples. A follow-up test 1 month later showed the same results.

Current papyrus storage methods include folders lined with special blotting material to protect against changes in humidity, which it says is a “passive method to prevent fungal growth and deterioration.” I am. jessica byler At the Penn Museum in Pennsylvania.

However, Beiler acknowledges that using standard methods does not always guarantee fungal prevention, and that is why “our team of conservators is working to improve the environment in the field of conservation.” I'm interested in learning more about innovative technology.”

A team at the Grand Egyptian Museum is planning to use wasabi treatment on archaeological papyri. The researchers also plan to test whether the spicy condiment is equally effective at disinfecting other crafts made of wood, paper and textiles.

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Source: www.newscientist.com

The Surprising Noisemaking Abilities of Tiny Fish

Danionella celebraum male fish

Ralph Blitz/Senkenberg Dresden

One of the world’s smallest fish, measuring just 12 millimeters long, it can make a sound as loud as a firecracker at more than 140 decibels.

Danionella cerebrum It is a small fish that lives in small rivers along the Bago Yoma Mountains in Myanmar.it is smallest known brain of all vertebrates in the world.

“We study this fish primarily for neuroscience because it’s so small and transparent,” he says. verity cook Charité, Faculty of Medicine, University of Berlin, Germany. But the fish are so loud, she says, that she can hear the pulsating sound just by walking in front of the tank.

To investigate how these tiny fish make this sound, Cook and his colleagues gathered groups of three or four fish into small tanks and shot high-speed video.

When a fish makes a sound, the ribs next to the swim bladder (organs that control the buoyancy of the swim bladder) are pulled by special muscles into a small hollowed cartilage area.

“There’s a lot of tension in this contraction,” Cook said. “When it is released rapidly, [the rib] When you hit the swim bladder, it makes a drum sound. “

Based on gene expression analysis, these specialized muscles are more resistant to fatigue than other muscles in the fish, and are therefore able to produce more hits in a row.

It’s unclear why these fish make so much noise. D. cerebrum They typically live in murky, murky waters and may have evolved this behavior to help find each other when visibility is poor, Dr Cook said.

“But the fact that only males make sounds suggests that it is related to aggressive behavior towards other males and mating behavior with females,” she says.

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Source: www.newscientist.com

The emotional impact of live music finally explained

Elton John to perform at Glastonbury Festival in June 2023

Matt Crossic/Alamy

Hearing live music can be more moving than listening to a recording of the same song. This is because the parts of the brain associated with emotional processing become more active.

Sasha Frewholz from the University of Zurich in Switzerland, composed 12 pieces of music, each 30 seconds long. Half were written with the purpose of conveying negative emotions such as sadness or anger. These are slower than the rest of the songs, are less harmonious, contain more minor chords, and were written to evoke positive emotions.

They then recruited 27 people with no musical training and asked them to listen to these 12 songs twice. The first performance was performed by a live pianist, and the second performance was played to the participants as a recording.

The order of hearing was randomly assigned, with 30 seconds of silence in between. Participants did not know when they were listening to a recording or a live performance.

While listening to music, they lay in an MRI scanner so the team could monitor their brain activity. The pianist was told to adjust the volume and speed of the piece according to this activity. For example, if participants showed little activity in response to positive music, they may have played louder.

“Recorded music does not adapt to the listener's response, but live pianists often adapt their music to the audience to get the best response from the audience,” says Frewholz.

The researchers found that live performances of both negative and positive pieces consistently caused brain activation in the left amygdala, an area of ​​the brain strongly associated with assigning sensory stimuli such as sounds to specific emotions. was found to lead to an increase in

The recorded songs, on the other hand, activated activity in the left amygdala much less and more inconsistently. This matched how emotionally participants rated each piece of music after the experiment.

The findings show that live music enhances our emotional responses, perhaps because of its free-flowing, dynamic nature, Fruhholz says.

The researchers hope to repeat the experiment with a larger audience in a concert setting. “When you go to a live concert, you're not alone,” Fruhholz says. “This intense emotional experience is also a social experience.”

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Source: www.newscientist.com

Searching for the exomoon: Investigating a moon orbiting a distant planet

Many years ago, at that time david kipping When he lived in London, he would walk home through the city and look up at the moon. For astronomers, its dimly glowing presence was a nightly source of inspiration. “It reminded us that satellites are waiting for us around exoplanets,” he says. “It made sense that we should look for them.”

It would be exciting to discover an exomoon, a natural satellite of a world outside our solar system. First, the moon may play a key role in determining the habitability of its host planet by dampening its wobble and promoting a stable climate, in the same way it did for Earth. there is. There may also be strange and wonderful configurations, such as a lunar ring or a moon with its own moon. But the most interesting thing is that some of them may be more suitable for life than exoplanets.

Kipping, now at Cornell University in New York, is part of a small community of astronomers exploring solar moons. At least statistics are on your side. About 5,500 exoplanets have been discovered so far, some of which may have dozens of moons. The problem is that it’s not easy to prove its existence. Two previous sightings of Kipping have been hotly debated.

But now there’s hope on the horizon, with many new ways to explore these objects, from monitoring rogue planets that have abandoned their stars to monitoring exoplanets’ gravitational wobbles. Armed with these new technologies, and new telescopes also in development, the Moon will…

Source: www.newscientist.com

Supplements containing resistant starch could assist in weight loss

Raw oats are a natural source of resistant starch

Mark Oliver/Alamy

Supplements containing resistant starch, a type of carbohydrate that takes time to digest, helped people moderately lose weight in a small trial.

Resistant starch is naturally found in beans, whole grains, raw oats, and green bananas, and is also formed when common starchy foods like potatoes, pasta, and rice cool after cooking.

Resistant starch comes in several different forms, but what they have in common is that the structure of the molecule means that it is not easily digested and absorbed in the small intestine.

Therefore, the starch reaches further into the intestine, into the large intestine, where it is digested by bacteria. This means that starch is classified as a prebiotic.

Although some previous studies have suggested that this starch can help with weight loss, Lihuatei Researchers from the Shanghai Jiao Tong University School of Medicine in China studied its effects on gut bacteria.

Researchers asked 37 overweight people to consume sachets of starch mixed with water twice a day before meals. For eight weeks they were given resistant starch, and for a further eight weeks they were given packets containing regular starch as a comparison. Participants were also provided with three balanced meals a day and various health indicators were measured.

After consuming resistant starch for eight weeks, people lost an average of 2.8 kilograms, while regular starch had no effect on weight. Resistant starch causes less rise in blood sugar levels after meals and is considered to be good for health.

Stool samples revealed that while people consumed resistant starch, the numbers of several bacterial species increased in their intestines. When these bacteria were transplanted into mice fed a high-fat diet, they appeared to have a weight-loss effect.

Rebecca McManamon A spokesperson for the British Dietetic Association said the trial was too small to be conclusive, but the results were plausible. “These outcomes are natural,” she says.

However, some people with irritable bowel syndrome may feel bloated and uncomfortable when they eat resistant starch, as the bacteria produce gas as they break down, she says.

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  • carbohydrates/
  • weight loss

Source: www.newscientist.com

First images from civilian lunar lander capture historic moon landing

A privately built spacecraft on the moon has sent back new photos from the lunar surface. The images captured the spacecraft’s much-lauded descent and the moment it rolled over shortly after landing.

The Odysseus lander, built by Houston-based Intuitive Machines, touched down on the moon on February 22, making it the first commercial ship to reach the moon’s surface and the first U.S. ship to reach the moon in more than 50 years. It made history as a spaceship.

The Odysseus Lunar Module took this image about 35 seconds after it rolled over on its approach to the landing site.
Intuitive machine via AP

The next day, Intuitive Machines announced that Odysseus had rolled over as it landed near a crater called Malapart A near the moon’s south pole. Company officials said the 14-foot-tall lander was operational, but part of the rover’s antenna was pointing toward the ground, limiting its ability to communicate with flight controllers on Earth. Ta.

with update MondayIntuitive Machines said it was continuing to communicate with the spacecraft, adding that flight controllers “will collect data until the lander’s solar panels are no longer exposed to light.”

Company officials said they expect to be able to communicate with Odysseus until Tuesday morning, based on the positions of the Earth and the moon. The lander was originally expected to spend about a week collecting data on the lunar surface before the lunar night begins and the spacecraft powers down.

In its latest update, the company announced that Odysseus’ instruments detected nine safe landing sites within the target zone near the moon’s south pole. The moon’s south pole region has long intrigued scientists because water ice is thought to be relatively abundant in permanently shadowed craters.

Source: www.nbcnews.com

Bizarre White Dwarf Leaves Metallic Marks Following Consumption of Planet

Artist’s impression of WD 0816-310. Astronomers have discovered scars imprinted on the surface left when a star swallows a planet.

ESO/L. Calzada

Astronomers have discovered a white dwarf star with strange metallic scars on its surface. The scar likely formed when the star tore apart and ate a small planet in its orbit.

Researchers often find white dwarfs with traces of metal in their atmospheres that came from planets that fell into the star. It has long been thought that metals should be evenly distributed across the surfaces of these so-called contaminated white dwarfs; Jay Farihi Researchers at University College London have discovered a strange concentration of metal debris.

Researchers monitored the star, called WD 0816-310, for two months using the Very Large Telescope in Chile. They discovered that the white dwarf had an opaque piece of metal on top of one of its magnetic poles, blocking some of the star’s light as it rotated. This position indicates that material may have been funneled into the star by its magnetic field. “This is the same process that causes auroras on Earth: charged particles follow magnetic fields to the surface,” Farihi said.

The planet that WD 0816-310 destroyed was small, probably about the same size as the solar system’s asteroid Vesta, which is about 525 kilometers in diameter. Its interior is now prominently displayed on its host star, which could make it relatively easy to study what its geochemistry was like before it was engulfed. Such studies may even be one of the best ways to observe small worlds outside our solar system, even after they disappear.

And there may be many other stars that have been similarly damaged. “When we find something outlandish, it’s often because they all looked that way and we just weren’t asking the right questions,” Farihi says. “This is the first, but it probably won’t be the last.” In fact, researchers have already discovered two white dwarfs that appear to have similar scars. If we go back and observe similar stars over and over again, we may discover even more stars.

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Source: www.newscientist.com

Recognizing gender disparities in the brain is crucial for mental well-being

we heard it all. Men's brains are larger and have better spatial awareness. Women's brains are adapted for multitasking and emotional intelligence. Stereotypes about how sex influences behavior abound, and as increasingly sophisticated brain-scanning technology emerges, claims about such inconsistencies are becoming more apparent.

But as we discovered in our feature on the human brain (“Your Amazing Brain: 10 Challenging Questions That Uncover Amazing New Discoveries About the Human Brain”), men's and women's behaviors, interests, We are trying to identify the biological reasons for population differences in . The issue of occupation is a delicate debate that includes not only sex but also gender, and has never been resolved.

Still, we should keep trying. In particular, if there really are gender-related brain differences, this would have a major impact on our health. That's because many pathologies related to the brain and neural branches affect men and women at different rates and in different ways. For example, women have higher rates of depression, anxiety, and eating disorders. Men have higher rates of autism and attention deficit hyperactivity disorder.

There are many possible reasons for this imbalance in the gender ratio. For example, autism may be underdiagnosed among girls, or typical behaviors may manifest differently. Similarly, biological factors may make women more susceptible to depression because they tend to have lower incomes or because men are less likely to seek help for mental health problems. .

However, brain differences between the sexes may also exist. If so, the photo is not yet complete. These may not be due to direct genetic or sex hormonal effects, but may be due to the way society generally treats men and women differently throughout their lives.

Elucidating all of this could shed light on the mechanisms behind these symptoms and lead to better treatment strategies. After all, this is not a competition between male and female brains, but an initiative that has the potential to help everyone.

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Source: www.newscientist.com

How to Safely Watch the Rare “Ring of Fire” Eclipse

A total solar eclipse is set to pass over North America in April, offering millions of skywatchers the rare chance to witness the afternoon sky briefly darken and a “ring of fire” appear overhead. The upcoming April 8 solar eclipse is expected to be a significant event, as its path will traverse parts of Mexico, the continental United States, and eastern Canada. Weather permitting, skywatchers in 15 states in the US will have the opportunity to see the moon almost completely block the sun, casting its shadow in a fiery circle and creating a halo effect in the sky. In all other states in the continental US, viewers will witness a partial solar eclipse where the moon appears to partially obscure the sun.

Here is everything you need to know about the upcoming total solar eclipse.

How to safely view a solar eclipse

It is crucial not to look directly at the sun during a solar eclipse, even if it is partially or mostly covered by the moon. Special eclipse glasses or a pinhole projector are necessary to safely view the eclipse and prevent eye damage. Sky observers should never look at the Sun through binoculars, telescopes, or camera lenses without a solar filter installed. Using Eclipse glasses is essential, as failure to do so can result in serious eye damage. NASA advises taking proper precautions. During the total solar eclipse when the moon completely blocks the sun, it is safe to view with the naked eye, but at all other times, eclipse glasses are required.

What is a solar eclipse?

A solar eclipse occurs when the sun, moon, and earth align, with the moon passing in front of the sun to temporarily block its light. The moon can either completely obscure the sun in a total solar eclipse or partially block its light in a partial solar eclipse.

Who can see it?

This eclipse is rare because it will cross populated areas of the United States compared to other recent total solar eclipses. NASA estimates that approximately 31.6 million people will live within the 160-mile-wide total path, with an additional 150 million living within 200 miles of the path. The eclipse will pass through various states in the US and enter Canada through provinces such as Ontario, Quebec, and New Brunswick.

While the most spectacular views will be within the total eclipse path, there are still opportunities for people across the continent to witness the astronomical event. A partial solar eclipse will be visible in all 48 states of the continental US, and NASA will stream a live view of the total solar eclipse online.

When will it happen?

The timing and duration of totality will vary by location, with some areas experiencing darkness and the “ring of fire” for up to 4 minutes and 28 seconds. Various resources online, including NASA, NationalEclipse.com, and timeanddate.com, provide information for planning and expectations on the day of the eclipse.

Specific timings for some populous cities along the path of totality are as follows:

Dallas: Partial eclipse begins at 12:23 PM CT. Totality begins at 1:40 PM CT. Totality ends at 1:44 PM CT. Partial eclipse ends at 3:02 PM CT.

Little Rock, AR: Partial eclipse begins at 12:33 PM CT. Totality begins at 1:51 PM CT. Totality ends at 1:54 PM CT. Partial eclipse ends at 3:11 PM CT.

Cleveland: Partial eclipse begins at 1:59 PM ET. Totality begins at 3:13 PM ET. Totality ends at 3:17 PM ET. Partial eclipse ends at 4:29 PM ET.

Buffalo, New York: Partial eclipse begins at 2:04 PM ET. Totality begins at 3:18 PM ET. Totality ends at 3:22 PM ET. Partial eclipse ends at 4:32 PM ET.

Lancaster, New Hampshire: Partial eclipse begins at 2:16 PM ET. Totality begins at 3:27 PM ET. Totality ends at 3:30 PM ET. Partial eclipse ends at 4:38 PM ET.

Source: www.nbcnews.com

The Search for Extraterrestrial Life: A Comprehensive Guide to Everything You Need to Know about Extraterrestrials

Currently, there is a high level of excitement in the quest for extraterrestrial life. This field, known as astrobiology, combines biology, chemistry, planetary science, and astronomy to explore the possibility of life beyond Earth.

While microbial life forms like bacteria are expected to be the most common in the Milky Way, there is a chance that some planets could support more complex life forms such as plants and animals. Recent advancements in extremophiles, exoplanets, and robotic exploration have increased optimism among astrobiologists for discovering signs of life beyond Earth.

List three reasons why astrobiologists are optimistic about finding extraterrestrial life.

1. Extremophile microorganisms

The adaptability of life on Earth, especially extremophiles, showcases the limits of life in extreme environments. These microorganisms thrive in harsh conditions like hydrothermal vents, glaciers, acidic volcanic water, and high radiation zones, offering insights into potential habitable extraterrestrial environments.

Image credit: Getty

2. Exoplanets

Discovery of exoplanets orbiting distant stars has expanded the search for potentially habitable worlds. Small, rocky, Earth-like planets orbiting within the habitable zone of their stars offer promising locations for extraterrestrial life. Future space telescopes are expected to detect biosignatures, such as oxygen, indicating potential life forms.

3. Exploration of the solar system by robots

Advances in robotic technology have enabled probes to explore planets and moons in our solar system, revealing environments that could support life. From Mars to Europa and Enceladus, these missions provide valuable data on habitable conditions and the possibility of extraterrestrial life.

Where in the solar system could extraterrestrial life exist?

Various celestial bodies within our solar system, including Venus, Mars, Europa, Enceladus, and Titan, offer potential environments for extraterrestrial life. Whether in subsurface oceans or unique atmospheres, these locations raise interesting questions about the existence of life beyond Earth.

Do aliens have intelligence?

While astrobiology primarily focuses on single-celled life and biosignatures, the possibility of more complex life forms and intelligent beings in the galaxy is still an intriguing topic. Despite efforts to detect signs of intelligent life, no definitive evidence has been found yet.

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Source: www.sciencefocus.com

Guide to Viewing the 2024 Snow Moon: Witness the Final Full Moon of Winter

The upcoming full moon in February 2024, known as the snow moon, will be the second one of the year. Despite being a micromoon this month, it signifies the end of winter and the coming of spring.

Wondering when is the best time to witness this full snow moon in the UK? How close is the micromoon? And the current constellation of the moon? Here is everything you need to know about the full moon in February 2024.

If you want to enjoy a clear night sky, explore our beginner’s guide to astronomy. To get familiar with some unique constellations, this guide is the perfect starting point.

Interested in capturing beautiful moon photos? Check out our practical moon photography guide that is filled with expert advice from astrophotographers and even BBC Night Sky presenter Pete Lawrence. Whether you are a beginner or an advanced user, we have tutorials to suit your needs.


When will we see the snow moon in 2024?

If the skies are clear, the snow moon will be visible in the early morning and evening on February 24, 2024, across the UK, US, and other parts of the world.

The peak illumination of the full moon in February will happen at 12:30 PM GMT. For viewers in the UK, this means that the moon will be fully illuminated during the day when it is below the horizon. However, it will still appear “full” when it rises at night and for a few days after.

In London, the Snow Moon will rise in the east-northeast on February 24 at 5:27pm GMT and set in the west-northwest at 7:32 a.m. on February 25th.

In New York, the Snow Moon will rise in the east-northeast on February 24 at 5:55 pm ET and set in the western sky at 7:18 am on February 25th.

In Seattle, the Snow Moon will rise in the east-northeast on February 24 at 6:07 pm PST and set in the west at 7:40 a.m. on February 25th.

What’s unique about the 2024 Snow Moon?

This year’s Snow Moon is special for two reasons. First, it falls on the day before the moon reaches its apogee, making it the smallest full moon of the year. Secondly, it coincides with the Lunar New Year celebrations, including the Lantern Festival.

On February 24th, National Tortilla Day is also celebrated in the US, giving you another reason to toast the full moon with chips and dip.

When is the best time to view the 2024 Snow Moon?

The best time to observe the snow moon is in the evening of February 24th, just after sunrise, or before moonset on the morning of February 24th. The moon will be closest to full illumination and low on the horizon in both cases.

In London, the moon will set at 7:21 a.m. GMT on the morning of February 24th, offering a picturesque sight low on the horizon. And if you wait until evening, the moon will rise at 5:27pm GMT on February 24th, just after sunset.

The Earth’s counterclockwise rotation means that the moon will appear to move across the sky from left to right in the Northern Hemisphere and from right to left in the Southern Hemisphere at a rate of 15 degrees per hour.

Why is February’s full moon called the snow moon?

February is one of the coldest months of the year in the Northern Hemisphere due to the cooling effects of winter and the sun’s lower angle. The snow moon gets its name from the significant snowfall experienced in the US, Canada, and Europe during this time.

What constellation is the moon in?

On February 22nd, the Moon will be in Cancer, and by the full moon, it will have moved into Leo, situated between Regulus and Keltan. Three days later, the moon will shift to Virgo, followed by Libra from March 1st.

Is the snow moon a supermoon?

No, the February 2024 snow moon is not a supermoon, as it will be a micromoon. Supermoons occur when the moon is closest to Earth, known as perigee, making it appear larger and brighter in the sky.

How far away is the moon?

During apogee on February 25, the moon will be 406,312 km (252,470 miles) away from Earth, making it the smallest full moon of 2024. The farthest point of the moon from Earth will be on October 2, 2024, at 406,516 km (252,597 miles) during a new moon.

What causes a full moon?

A full moon occurs when the side facing Earth is fully illuminated by the sun, as the Earth is positioned between the Sun and the Moon. This alignment, known as “syzygy,” only lasts for a moment but signifies a full moon in the lunar cycle.

The moon’s cycle lasts about 29.53 days, with the full moon marking the midpoint. The sun and moon balance each other during a full moon, with the moon appearing full all night but technically only being “full” for a brief moment.

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Source: www.sciencefocus.com

Misconceptions about prostate cancer: What we need to know

Recent news about King Charles’ prostate issues and subsequent cancer diagnosis has raised awareness of such health issues nationwide. Although the king is not diagnosed with prostate cancer, his efforts to raise awareness among older men have been widely appreciated.

The charity Prostate UK is using billboards to encourage men across the country to assess their cancer risk and consult their GP if they experience symptoms like frequent or difficult urination. However, prostate cancer is a complex and subtle condition.


The prostate, located below the bladder, tends to enlarge with age. The urethra, the tube draining urine from the bladder to the outside, passes through it. When the prostate enlarges, it can put pressure on the urethra, causing symptoms like dribbling and increased frequency of urination. This condition is quite common.

Similarly, prostate cancer is also common. Autopsy studies show that 36% of whites and 51% of African Americans develop prostate cancer in their 70s. There are even cases of prostate cancer found in 5% of men under 30 in autopsy studies. However, not all forms of prostate cancer are equally dangerous, with some being harmless and others potentially fatal.

How dangerous is prostate cancer?

Prostate cancer accounts for around 4% of male deaths in the UK, with approximately 12,000 people dying from it each year. The challenge lies in finding treatments that do not cause further harm, as treatments like surgery and radiation therapy can lead to side effects such as erectile dysfunction and incontinence.

The lack of an accurate way to differentiate between aggressive and non-aggressive tumors is a major problem. The PSA test, developed in the 90s, was introduced to monitor men’s response to prostate cancer treatment. However, the increasing number of diagnoses did not correspond to a reduction in mortality rates.

In the US, the Preventive Services Task Force has offered recommendations for or against PSA screening. While screening may slightly reduce prostate cancer deaths, it can also lead to unnecessary testing and treatments for non-fatal conditions.

To avoid unnecessary treatment, the “watchful waiting” approach has been effective in managing localized prostate cancer with low mortality rates. In the UK, the National Screening Committee does not recommend PSA screening for prostate cancer.

Research suggests that identifying harmful cancers through prostate screening MRI scans may be a viable solution, although more evidence is needed to assess its impact on reducing deaths without overtreatment.


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Source: www.sciencefocus.com