Scientists puzzled by mysterious ‘chirps’ in space

The melodious high-pitched sound of birdsong is not something typically associated with the vastness of space, usually serving as a delightful indication of the arrival of spring. However, to the surprise of many, scientists at China’s Beijing Aviation University have recently stumbled upon a similar occurrence over 100,000 kilometers away from Earth.

Through the analysis of data collected from NASA’s Magnetospheric Multiscale (MMS) satellite, researchers have pinpointed a phenomenon referred to as “chorus waves,” which consist of bursts of electromagnetic radiation traveling along Earth’s magnetic field lines.

If one were to venture into space, this sound would remain unheard due to the absence of air for sound waves to propagate. Interestingly, upon conversion into an audio signal for examination, this “chirp” is actually the auditory representation of these waves.

https://c02.purpledshub.com/uploads/sites/41/2025/01/Space-chirps-v2.mp4
“Twitter” confirmed in space

So, what exactly causes these electromagnetic chirps? Contrary to expectations, it is not a celestial songbird. In reality, chorus waveforms are relatively common. However, the peculiarity lies in their location, as highlighted by their distance from Earth.

The energy transfer induced by chorus waves prompts electron acceleration to speeds nearing that of light, crucial for the formation of Earth’s radiation belts which shield against the sun’s energetic particles.

While these accelerated particles contribute to the magnificent aurora borealis, they are also dubbed “killer electrons” due to the hazards they pose to satellites, astronauts, and crucial communication systems.

Typically, these waves are found around 51,000 km (32,000 miles) away, in a region influenced by the “magnetic dipole effect,” defining the Earth’s magnetic field with north and south poles.

However, a 2016 study published in nature unveiled that for the first time, these chorus waves have been observed at distances up to 165,000 km (103,000 miles) from Earth, in regions where the magnetic field is distorted and dipole effects are absent.

Furthermore, these waves exhibit similar properties to those closer to Earth, lasting around 0.1 seconds with frequencies reaching nearly 100Hz (akin to the noise of a revving car engine).

Chorus waves are part of the complex magnetic field system that causes auroras – Photo credit: Getty

Why is this discovery significant? It indicates that Earth’s environmental conditions are not prerequisites for wave generation as previously assumed by scientists.

“Though this finding does not refute existing theories… it certainly prompts a deeper investigation,” remarked Professor Richard Horne, head of space weather at the British Antarctic Survey, not involved in the study.

“The unexpected presence of chorus waves in this region calls for further exploration in areas where the Earth’s magnetic field displays substantial deviations from the dipole.”

Chorus waves play a vital role in shielding Earth from solar storms, yet they also pose potential dangers. Enhanced understanding of these waves can lead to better protective measures.

Horne expressed that this breakthrough “will significantly enhance our comprehension of these waves and refine our capacity to forecast them.”

read more:

Source: www.sciencefocus.com

The mysterious process of fog formation

Fog consists of water vapor molecules that float as tiny water droplets in the air but remain near the ground. Essentially, fog is a cloud touching the Earth’s surface, forming similar to clouds. High humidity plays a significant role in fog formation, and depending on its rate and temperature, fog can appear and vanish suddenly.

Water in its vapor state is transparent and invisible. The higher the air’s temperature, the greater its kinetic energy, allowing more water molecules to exist as vapor.

When warm, moisture-rich air cools abruptly, the water molecules slow down too much to maintain their vapor form and combine into small liquid droplets. These droplets, while still small enough to float in air currents, appear opaque as light reflects off the air-water interface.

radiation fog

Radiation fog © Dan Bright

Radiation fog forms on the ground during calm, clear nights when heat absorbed by the Earth’s surface during the day radiates into the air. As the heat rises, the air near the surface cools until it becomes saturated.

Cold air holds less water vapor than warm air, causing the water vapor to condense into fog. Radiation fog typically dissipates as the ground warms up again, but it can persist all day in the winter.

Radiation fog is also known as shallow fog or ground fog when it occurs in a narrow layer below average eye level on land and below about 10 meters at sea.

valley fog

Valley Fog © Dan Bright

Valley fog develops at the bottom of valleys as cold, dense air settles and condenses to form fog. It is restricted to local terrains like hills and mountains and can persist for several days.

advection fog

Advection fog © Dan Bright

Advection fog forms when horizontal winds push warm, moist air onto cold surfaces, leading to fog formation through condensation. This phenomenon is common at sea, where warm tropical air interacts with cold water. Advection fog can cover large areas, with the Golden Gate Bridge in San Francisco Bay often obscured by it.

Sea fog, a type of advective fog, occurs when warm, moist air descends from land into chilly oceans, or when warm fronts clash with cold ocean currents. The northeast coast of the UK is particularly prone to sea fog due to the cold waters of the North Sea.

uphill fog

Uphill fog © Dan Bright

Uphill fog, a type of hill fog, occurs when moist air is pushed up a slope, hill, or mountain by wind, cooling and condensing to form fog as it descends down the slope.

evaporation fog

Evaporative fog © Dan Bright

Evaporative fog is akin to advection fog, forming when cold air passes over moist land or warm water. When warm water evaporates into the lower atmosphere, it warms the air, causing it to rise. This upward movement of warm, moist air mixes with cooler air until reaching 100% humidity, resulting in fog formation. Evaporative fog is commonly observed at lakes, ponds, and outdoor pools.

Why does altitude affect temperature?

Consider the atmosphere as consisting of air masses. The higher an air parcel, the less compressed it is due to the weight of the atmosphere above, allowing for greater volume. This expansion requires energy, leading to sacrifice of thermal energy and a decrease in temperature.

Does sound travel further on foggy days?

“Sound propagates through the air as pressure waves move air molecules back and forth. In fog, water droplets scatter more sound energy, attenuating the sound and reducing the distance it can travel,” explains physicist Robert Matthews.

However, the complete impact of fog formation conditions on sound travel is not fully resolved. “On warm, highly humid days, smaller droplets have minimal effect on sound waves,” he adds.

“Moist air, being denser than dry air, allows sound waves to travel more effectively and be heard over greater distances,” Matthews further explains.

Does sound travel farther on foggy days? ©Getty Images

About our expert Professor Robert Matthews

After completing his physics studies at Oxford, Robert ventured into science writing. He currently serves as a visiting professor of science at Aston University.

Explore more about fog:

Submitted by: Rich French, London

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Source: www.sciencefocus.com

Mysterious X-ray oscillations detected in supermassive black hole by XMM-Newton

In 2018, astronomers discovered that the corona of 1ES 1927+654, an actively accreting black hole with 1.4 million solar masses located in a galaxy some 270 million light-years away, suddenly disappeared and reassembled several months later. I observed that. The short but dramatic outage was the first of its kind in black hole astronomy. Now, astronomers using ESA's XMM-Newton Observatory have captured the same black hole exhibiting even more unprecedented behavior. They detected X-ray flashes from 1ES 1927+654 at a steadily increasing clip. Over a two-year period, the frequency of millihertz vibration flashes increased from every 18 minutes to every 7 minutes. This dramatic speed-up of X-rays has never been observed from a black hole before.



In this artist's concept, material is stripped from a white dwarf (bottom right sphere) orbiting within the innermost accretion disk surrounding the supermassive black hole of 1ES 1927+654. Image credit: NASA/Aurore Simonnet, Sonoma State University.

Black holes are a prediction of Albert Einstein's theory of general relativity. They are gravitational monsters that trap any matter or energy that crosses their “surface,” a region of spacetime known as the event horizon.

In its final descent into the black hole, a process known as accretion, the doomed material forms a disk around the black hole. The gas in the accretion disk heats up and emits primarily ultraviolet (UV) light.

The ultraviolet light interacts with the cloud of electrically charged gas or plasma that surrounds the black hole and accretion disk. This cloud is known as the corona, and the interaction energizes the ultraviolet light and amplifies it into X-rays, which can be captured by XMM Newton.

XMM-Newton has been observing 1ES 1927+654 since 2011. Back then, everything was very normal.

But things changed in 2018. As the X-ray corona disappeared, the black hole erupted in a massive explosion that seemed to disrupt its surroundings.

The coronavirus gradually returned, and by early 2021, it seemed like normal conditions had returned.

However, in July 2022, XMM Newton began observing its X-ray output fluctuating at a level of about 10% on timescales of 400 to 1,000 seconds.

This type of fluctuation, called quasi-periodic oscillations (QPO), is notoriously difficult to detect in supermassive black holes.

“This was the first sign that something strange was going on,” said Dr. Megan Masterson. Student at MIT.

The oscillations could suggest that a massive object, such as a star, is embedded in the accretion disk and rapidly orbiting the black hole on its way to being swallowed.

As an object approaches a black hole, the time it takes to orbit decreases and the frequency of its oscillations increases.

Calculations revealed that the orbiting object was probably the remains of a star known as a white dwarf, had about 0.1 times the mass of the Sun, and was moving at an astonishing speed.

It was completing one orbit of the central monster, covering a distance of about 100 million km, about every 18 minutes. Then things got even weirder.

Over nearly two years, XMM Newton showed an increase in the strength and frequency of the vibrations, but not as much as the researchers expected.

They assumed that an object's orbital energy is being emitted as gravitational waves, as prescribed by the theory of general relativity.

To test this idea, they calculated when the object crossed the event horizon, disappeared from view, and stopped oscillating. It turns out to be January 4, 2024.

“Never in my career have I been able to predict anything so accurately,” says Dr. Erin Kara of MIT.

In March 2024, XMM Newton observed it again and the oscillations were still present.

The object was currently traveling at about half the speed of light, completing an orbit every seven minutes.

Whatever was inside the accretion disk, it stubbornly refused to be swallowed up by the black hole.

Either something more than gravitational waves is at play, or the entire hypothesis needs to be changed.

Astronomers also considered other possibilities for the origin of the vibrations.

Remembering that the X-ray corona disappeared in 2018, they wondered if this cloud itself was vibrating.

The problem is that there is no established theory to explain such behavior, so there is no clear path to take this idea further, so they go back to the original model and realize there is a way to fix it. I did.

“If the black hole has a white dwarf companion, the gravitational waves produced by the black hole could be detected by LISA, an ESA mission scheduled to launch within the next 10 years in partnership with NASA.” said Masterson.

team's paper will appear in journal nature.

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Megan Masterson others. 2025. Millihertz oscillations near the innermost orbit of a supermassive black hole. naturein press. arXiv: 2501.01581

Source: www.sci.news

New Research Explores Mysterious Qualities of Liquid Brine Found on Mars

Mars is at the extreme of salt water stability. And only the combination of the most favorable environmental conditions and the salt with the lowest eutectic temperature could stabilize brine, at least temporarily, on the surface of Mars, one researcher says. new research Published in Proceedings of the National Academy of Sciences.

This image of an impact crater in the Sirenum Fossai region of Mars was taken by NASA's Mars Reconnaissance rover on March 30, 2015. The crater is approximately 3,300 feet (1 km) wide and appears to be relatively recent due to its sharp edges and wells. -Stored emissions. The steep inner slopes are carved by canyons and contain slope lines that may recur on the equator-facing slopes. Image credit: NASA / JPL / University of Arizona / Alfred McEwen.

Liquid water is an important prerequisite for a habitable planet. However, the combination of Mars' low temperatures, atmospheric pressure, and water vapor pressure means that any liquid water found on Mars would likely freeze, boil, or evaporate quickly, making it unlikely that Mars exists. .

However, paleontologists continue to insist that liquid water exists on Mars.

Of particular interest is the discovery of seasonal black stripes called repeat slope lines.

These features appear in some places on Mars when temperatures rise above -23 degrees Celsius (-10 degrees Fahrenheit) and disappear when it gets colder.

They are often described as possibly being associated with liquid water.

The new study puts a damper on the idea that liquid water is likely to be found soon in Mars' recurring slopes, permafrost, or salt water.

“If we look closely at RSL, its behavior is consistent with a sand or dust flow, and water is not required for RSL formation,” said lead author Dr. Vincent Chevrier, a researcher at the University of Arkansas. said.

Other researchers believe that brine, a highly salty solution like Earth's oceans, may hold the key to finding liquid water on Mars.

Salt water can freeze at much lower temperatures, and Mars is rich in salt.

Among these salts, perchlorate appears to be the most promising because of its extremely low eutectic temperature (the temperature at which the melting point of the mixture is lower than that of the single components).

For example, calcium perchlorate brine freezes at -75 degrees Celsius (-14 degrees Fahrenheit), but the average surface temperature near the equator of Mars is -50 degrees Celsius (-58 degrees Fahrenheit), so theoretically This suggests that there may be zones where calcium coagulates. Perchlorate water can remain liquid, especially underground.

Dr. Chevrier and his colleague, Dr. Rachel Srank of the Lunar and Planetary Institute, then considered all the arguments for and against brine that could form a stable liquid.

“A variety of limiting factors, including the relatively small amount of most promising salts, water vapor pressure, and ice position, strongly limit the amount of brine present at the surface and in the shallow subsurface,” the researchers said. Ta.

“And even if saline waters formed, they would still remain uninhabitable by terrestrial standards.”

“Despite these drawbacks and limitations, there is always a possibility that Martian life adapted to these salt waters and some terrestrial life could survive in them. This is a planetary protection consideration because there is a possibility that

“Therefore, detecting brine in situ remains a key objective for Mars exploration.”

The next hurdles ahead, the authors say, are improving the equipment needed to detect small amounts of brine, better identifying the best places to look for brine, and conducting more experiments under Martian conditions. It is suggested that this is to enable room measurements to be carried out.

“Despite our best efforts to prove otherwise, Mars remains a cold, dry, and completely uninhabitable desert,” Chevrier said.

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Vincent F. Chevrier and Rachel A. Slank. 2024. The elusive nature of liquid brine on Mars. PNAS 121 (52): e2321067121;doi: 10.1073/pnas.2321067121

Source: www.sci.news

Authorities report dozens of deaths from mysterious disease in Congo

A mysterious illness with flu-like symptoms has claimed the lives of dozens of people in the Democratic Republic of Congo, as reported by the country’s health authorities.

As of Tuesday, the unknown disease has resulted in the death of 79 people and the sickness of 376 individuals, according to the country’s Ministry of Public Health, Hygiene and Social Security.

In a statement regarding X, the ministry stated that the origin of the disease is “still unknown” and was first identified in Kwango province in southwestern Congo.

Symptoms reported include fever, headache, stuffy nose, cough, difficulty breathing, and anemia.

According to Reuters and Associated Press, local authorities have warned that the death toll could potentially rise to 143.

The Ministry of Health emphasized that the remains of those who have died with similar symptoms should not be handled without the involvement of authorized health authorities. They urged the public to report any suspicious illnesses or unusual deaths, avoid large gatherings, and follow basic hygiene practices like washing hands with soap and water.

Emergency public health officials are being deployed to the affected area, as confirmed by the ministry.

The World Health Organization, in response to the reports of the unidentified illness, stated to NBC News that they are collaborating with local authorities and have dispatched a team to collect samples for laboratory testing.

The U.S. Centers for Disease Control and Prevention, with offices in Congo, is aware of the situation and is providing technical support to a rapid response team sent by the local emergency operations center.

Source: www.nbcnews.com

Hubble Captures Mysterious Spiral Galaxy Edge-On

NASA has released a surprising image of the unusual edge-on spiral galaxy UGC 10043 taken by the Hubble Space Telescope.

This Hubble image shows UGC 10043, an unusual spiral galaxy located about 150 million light-years away in the constellation Serpens. Image credits: NASA / ESA / Hubble / R. Windhorst / W. Kiel.

UGC 10043 It is located in the constellation Serpens, about 150 million light years from Earth.

Also known as IRAS 15464+2201 or LEDA 56094, this galaxy is one of the somewhat rarer spiral galaxies. Viewed from the side.

“We see galactic disks as sharp lines through space, with pronounced dust lanes along them,” Hubble astronomers said in a statement.

“This dust is spread throughout UGC 10043's spiral arm, but when viewed from the side it appears very thick and cloudy.”

“I can see some lights, too.” Active star forming region In your arms, shining from behind the dust. ”

“Surprisingly, we can also see that the center of the galaxy has a bright, almost egg-shaped bulge that towers far above and below the disk.”

“All spiral galaxies have such a bulge as part of their structure, containing stars that orbit the center of the galaxy in paths above and below the spiral disk.”

“This is a feature that isn't usually obvious in pictures of galaxies.”

“The unusually large size of this bulge compared to the galaxy's disk is likely due to UGC 10043 sucking up material from nearby dwarf galaxies.”

“This may also be why the disc warps, causing one end to bend up and the other end to bend down.”

The color image of UGC 10043 was created from separate exposures taken in the visible and near-infrared regions of the spectrum. Hubble's advanced survey camera (ACS) and Wide field planetary camera 2 (WFPC2).

Two filters were used to sample different wavelengths.

Color is obtained by assigning different hues to each monochromatic image associated with an individual filter.

“Like most full-color images published by Hubble, this image is a composite of multiple individual snapshots taken by Hubble at different times and capturing different wavelengths of light,” the astronomers said. Explained.

“What is remarkable about this image is that the two sets of Hubble data used were collected 23 years apart, in 2000 and 2023.”

“Hubble's longer lifespan not only allows us to generate new and better images of old targets.”

“It also provides a long-term archive of data, making it increasingly useful to astronomers.”

Source: www.sci.news

Early universe reveals mysterious supermassive galaxy

Astronomers using the NASA/ESA/CSA James Webb Space Telescope have determined that within the first billion years after the Big Bang, three supermassive galaxies with a mass roughly the same as our own Milky Way already existed. I discovered that there is. The discovery, part of the JWST/FRESCO survey, shows that stars in the early universe grew much more rapidly than previously thought, casting doubt on existing models of galaxy formation.

Three red monster galaxies discovered by Webb. Image credits: NASA / CSA / ESA / M. Xiao & PA Oesch, University of Geneva / G. Brammer, Niels Bohr Institute / Dawn JWST Archive.

Until now, it was thought that all galaxies formed gradually within large halos of dark matter.

Dark matter halos trap gas (atoms and molecules) in gravitationally bound structures.

Typically, up to 20% of this gas is converted into stars within a galaxy.

But new discoveries cast doubt on this view, revealing that giant galaxies in the early universe may have grown much more rapidly and efficiently than previously thought.

“The problem of ‘impossible’ giant galaxies in the aftermath of the Big Bang has puzzled astronomers since the first images of the web,” said Dr Ivo Rabe, an astronomer at Swinburne University of Technology.

“This is like finding a 100 kg infant. Webb has proven that monsters roam the early universe.”

While most of the sources found in the FRESCO survey fit existing models, astronomers also discovered three surprisingly massive galaxies with stellar masses comparable to today’s Milky Way galaxy. .

They are named “red monsters” because of their high dust content and their distinctive red color in web images.

These form stars nearly twice as efficiently as their subsequent lower-mass counterparts and galaxies.

“These findings raise new questions about galaxy formation theory, especially the problem of ‘too many, too big’ galaxies in the early Universe,” said Dr. Rabe.

“Current models cannot explain why star formation occurs so efficiently so early in the universe.”

“The general assumption is that an exploding star or a supermassive black hole kills star formation and blows out the candle.”

“I have no doubt that future observations of the web will provide clues about what we are missing.”

Professor Stein Weitz, an astronomer at the University of Bath, said: “Finding three such gigantic beasts among the specimens poses an interesting puzzle.”

“Many processes of galactic evolution tend to introduce rate-limiting steps in how efficiently gas turns into stars, but somehow this red monster quickly bypassed most of these hurdles. It seems there is.”

“These results show that galaxies in the early Universe may form stars with unexpected efficiency,” said Dr. Mengyuan Xiao, an astronomer at the University of Geneva.

“Studying these galaxies in more detail will provide new insights into the conditions that shaped the early days of the universe.”

“The Red Monster is just the beginning of a new era in the exploration of the early universe.”

“That’s the great thing about astronomy: we’re always surprised by new discoveries,” Professor Weitz said.

“Already in the first few years, Webb has thrown us some curveballs.”

“In multiple ways, we show that some galaxies mature rapidly during the first chapters of the universe’s history.”

a paper Survey results are published in a magazine nature.

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M. Xiao others. The formation of supermassive galaxies accelerates during the first billion years. naturepublished online on November 13, 2024. doi: 10.1038/s41586-024-08094-5

Source: www.sci.news

China and the US race to study neutrinos, the mysterious ‘ghost particles’ of the cosmos

Trillions of neutrinos pass through our bodies every second. The sun produces them through nuclear fusion. The same goes for nuclear power plants. Some come from supernova explosions in space. Neutrinos are paired with antineutrinos, which scientists believe mirror the behavior of neutrinos.

As such, JUNO is designed to capture antineutrinos, specifically the antineutrinos emitted by two nuclear power plants located approximately 53 miles from the observatory.

The 13-story JUNO sphere will be filled with a special liquid called a scintillator and submerged in a cylinder of purified water, said project leader Wang Yifang, director of the China Institute of High Energy Physics.

When the antineutrinos pass through the liquid, they trigger a chemical process that produces a brief burst of light that can be picked up by sensors inside the sphere.

“This event will cause a flash that will last only about 5 nanoseconds, and we hope to capture it with thousands of photomultiplier tubes surrounding the sphere,” he says, as a worker behind him says, Mr. Wang, wearing a helmet, spoke while installing the doubler. “We hope to catch 60 events per day.”

Thanks to its approach, JUNO should be able to measure differences in antineutrino masses about 10 times more accurately than previous instruments.

First of three new neutrino observatories

JUNO is part of China’s ambitious efforts to become a global scientific powerhouse. In a speech this year, President Xi Jinping laid out plans to transform the country into a science and technology superpower by 2035.

October 11th, workers at the bottom of JUNO.Eric Baclinao/NBC News

JUNO is expected to be the first of three next-generation neutrino observatories to open over the next decade, making it a kind of spearhead in a new era of physics. In Japan, the Hyper-Kamiokande Observatory is scheduled to open in 2027. And a U.S.-backed program called the Deep Neutrino Experiment (DUNE) calls for particle accelerators to send beams of neutrinos underground from Illinois to North Dakota starting in 2027. 2031.

The three upcoming observatories are both complementary and competitors, as they all plan to use different techniques to detect particles. Each project involves extensive international collaboration aimed at advancing the field, creating new spin-off technologies and training a new wave of scientists.

“When you start these experiments, it’s not unlikely that you’ll observe something unexpected,” said Chris Marshall, an assistant professor of physics at the University of Rochester who works on the DUNE project. “Trying to unravel these very complex effects will require multiple experiments measuring things in different ways.”

The ability of each observatory to answer important physics questions depends in part on how well researchers can collaborate between and among projects. But there is growing concern among some scientists around the world that rising geopolitical tensions between the United States and China, and the resulting deterioration in their scientific relations, could hinder progress. are.

In recent years, the United States has pursued policies to prevent Chinese scientists from bringing American-based technology to the country and to prevent China from poaching its scientific stars.

Wang said the U.S. is denying visa applications for 2022 and 2023 without explanation and limiting U.S. involvement in JUNO.

“In science, cooperation and competition are good, but it can’t be all about competition,” he said.

On October 11, Mr. Wang pointed out to journalists the underlying characteristics of JUNO’s domain.Eric Baclinao/NBC News

U.S.-based scientists also said they have found new obstacles to cooperation with Chinese scientists.

“From the U.S. side, it’s becoming increasingly difficult to obtain funding for collaborations with Chinese colleagues,” Patrick Huber, director of the Center for Neutrino Physics at Virginia Tech, said in an email. It has also become much more difficult for our Chinese colleagues to obtain U.S. visas.” .

“It’s not impossible to collaborate with Chinese scientists, but it’s becoming increasingly difficult,” said Ignacio Taboada, a physics professor at the Georgia Institute of Technology who directs an existing neutrino observatory in Antarctica. “I’m working on it,” he said.

Solving the mystery of neutrinos

The data generated by JUNO could go a long way toward solving important mysteries about how and why neutrinos change shape more than other elementary particles.

Neutrinos can oscillate, or transform, between three so-called “flavors” during their travels: muon, tau, and electron. For example, the sun sends electron neutrinos toward Earth, but they can also arrive as muon neutrinos. When neutrinos interact (which rarely happens), they settle on a particular flavor.

Additionally, scientists believe that neutrinos travel as one of three different mass states, and that state helps determine the likelihood of a neutrino interacting as a particular flavor. However, it is not yet clear which state has the largest population.

Scientists also found that neutrinos and antineutrinos may deform differently as they travel, and that those differences may account for some of the imbalance in the physics between matter and antimatter in the universe. I think there is.

Journalists take photos at the top of JUNO’s sphere on October 11th.Eric Baclinao/NBC News

If so, learning more about the masses and oscillations of neutrinos and antineutrinos will help researchers find a missing page in the Standard Model of physics (the rulebook of particles and their interactions), or something that has never been known before. This could help researchers understand whether missing particles or forces are having invisible effects. role.

“Our beautiful theory of reality, the Standard Model, is not the final theory,” said Sergio Bertolucci, an Italian particle physicist and DUNE co-spokesperson. “It turns out that we need to know more about neutrinos to answer things that the standard model can’t answer.”

Wang hopes JUNO will win the race to determine the neutrino mass hierarchy before the United States and other countries.

“We just want to be good scientists. In science, being first is most important. There’s nothing to be second,” he said. “As a scientist, I can’t always be a follower. I want to have my own thing.”

Entrance to the Jiangmen Underground Neutrino Observatory in China.Eric Baclinao/NBC News

If JUNO explains the neutrino mass story before DUNE comes online, the U.S.-led project will be able to measure that question differently and confirm JUNO’s results.

DUNE’s plan is to measure neutrinos as they leave the Illinois facility, then travel 800 miles around Earth, where they can interact and oscillate. If the neutrinos arrive in South Dakota and can be detected, scientists could compare the flavor combinations of the neutrinos at the beginning and end of their journey. However, the project experienced delays and cost overruns.

“JUNO’s uniquely rich dataset, alone or in combination with other experiments, will play a key role in determining bulk orders by 2030,” said Professor Pedro Ochoa said in physics and astronomy from the University of California, Irvine.

However, several scientists involved in neutrino observation projects acknowledged that it is impossible to predict how much benefit the research will actually bring to Earth. They suggested that in the future, new technologies could be spun off, driving innovation in data-intensive computing and advancing particle accelerator science.

“We can’t make electric light by improving candles, so we need to take a step forward. We need a break,” said John C., a particle physicist at the U.S. Department of Energy’s Brookhaven National Laboratory and co-spokesperson for the DUNE project. Mary Bishai says. “Basic research inherently creates discontinuities.”

Wang put it another way, saying his work is driven by pure curiosity: “I work in ‘useless’ science.”

Source: www.nbcnews.com

Webb finds mysterious cosmic question mark in distorted galaxy formation

Seven billion years ago, the universe’s star formation boom began to slow. What did our Milky Way galaxy look like at that time? Astronomers using the NASA/ESA/CSA James Webb Space Telescope have discovered a clue in the form of a cosmic question mark, the result of an unusual alignment in space spanning several light-years.



Galaxy cluster MACS-J0417.5-1154 is so massive that it warps the fabric of space-time and distorts the appearance of galaxies behind it. This phenomenon is known as gravitational lensing. This natural phenomenon magnifies distant galaxies, sometimes causing them to appear multiple times in the image, as Webb saw here. Two distant interacting galaxies (a spiral galaxy seen face-on and a dusty red galaxy seen edge-on) appear multiple times, tracing a familiar shape across the sky. Active star formation and the remarkably perfect spiral shape of the galaxy seen face-on indicate that these galaxies are just beginning to interact. Image credit: NASA/ESA/CSA/STScI/V. Estrada-Carpenter, Saint Mary’s University.

“There are only three or four known examples of similar gravitational lensing configurations in the observable universe, so this discovery is exciting as it demonstrates the power of Webb and suggests that we may find more like it in the future,” said Dr Guillaume Despres, from St Mary’s University.

The region has previously been observed by the NASA/ESA Hubble Space Telescope, but Webb was the first to spot the dusty red galaxy forming an intriguing question mark shape.

This is because the wavelengths of light that Hubble detects are trapped in space dust, while longer wavelengths of infrared light pass through Webb’s instruments and can be detected.

Astronomers used both telescopes to observe the galaxy cluster. MACS-J0417.5-1154The cluster is so large that it distorts the fabric of space-time, acting like a magnifying glass.

This will allow astronomers to see clearer details of the much more distant galaxies behind the cluster.

But the same gravitational effects that expand galaxies also cause distortions, which can result in galaxies appearing spread out in an arc across the sky, or appearing multiple times.

This optical illusion in space is called gravitational lensing.

The red galaxy Webb uncovered, along with the spiral galaxy it interacts with, previously detected by Hubble, is magnified and distorted in an unusual way that requires a special and rare alignment between the distant galaxy, the lens, and the observer — something astronomers call hyperbolic umbilical gravitational lensing.

This explains five images of the galaxy pair seen in the Webb image, four of which trace the top of the question mark.

The question mark points are, from our perspective, unrelated galaxies that happen to be in the right place and spacetime.

In addition to developing a case study for Webb, Niris Noting the ability of their infrared imaging device and slitless spectrometer to detect star formation locations in galaxies billions of light years away, the research team also couldn’t help but notice the shape of the question mark.

“This is really cool. I got interested in astronomy when I was younger because I saw amazing images like this,” said Dr Marcin Sawicki, also from Saint Mary’s University.

“Knowing when, where and how star formation occurs in galaxies is crucial to understanding how galaxies have evolved throughout the history of the universe,” said Dr Vicente Estrada Carpenter from Saint Mary’s University.

“The results show that star formation is widespread in both. The spectral data also confirm that the newly discovered dusty galaxy is located at the same distance as the frontal spiral galaxy, suggesting that the two are probably starting to interact.”

“Both galaxies in the question mark pair show several dense regions of active star formation, likely the result of the gas in the two galaxies colliding.”

“But neither galaxy seems particularly disturbed, so perhaps we are seeing the beginning of an interaction.”

“These galaxies, seen billions of years ago when star formation was at its peak, are similar in mass to the Milky Way at that time,” Dr Sawicki said.

“Thanks to Webb, we can now study what our galaxy was like in its teenage years.”

Team paper Published in Monthly Bulletin of the Royal Astronomical Society.

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Vicente Estrada Carpenter others2024. CANUCS JWST/NIRISS We will use grism spectroscopy to investigate when, where and how star formation occurs in a pair of galaxies at cosmic noon. MNRAS 532 (1): 577-591; doi: 10.1093/mnras/stae1368

This article is based on a press release provided by NASA.

Source: www.sci.news

New study uncovers common, mysterious I motif structure in human genome DNA

The so-called i-motif is a knot-like DNA structure that forms in the nuclei of human cells and is thought to provide important genome control. Garvan Institute of Medical Research Other studies have used immunoprecipitation and next-generation sequencing to identify i-motif structures in human DNA.

Peña Martinez othersIn total, we observed 53,000 i-motifs across three human cell lines (MCF7, U2OS, and HEK293T). Image courtesy of Peña Martínez. others., doi: 10.1038/s44318-024-00210-5.

The I motif is a DNA structure that differs from the iconic double helix shape.

These form when runs of cytosine letters on the same DNA strand pair up with each other to form a four-stranded twisted structure that juts out from the double helix.

In 2018, scientists at the Garvan Institute of Medical Research were the first to successfully directly visualize i-motifs inside living human cells, using new antibody tools they developed to recognise and bind to the i-motifs.

The new study expands on these findings by using the antibody to identify the location of i-motifs throughout the genome.

“In this study, we have mapped more than 50,000 i-motif sites in the human genome that are found in all three cell types we looked at,” said Professor Daniel Crist from the Garvan Institute of Medical Research, lead author of the study.

“This is a surprisingly high number for a DNA structure whose presence in cells was once a matter of debate.”

“Our findings confirm that the i-motif is not just an object of laboratory study, but is widespread and likely plays an important role in genome function.”

The researchers found that i-motifs are not scattered randomly, but are concentrated in important functional regions of the genome, including those that control gene activity.

“We found that the i-motif is associated with genes that are highly active at specific times in the cell cycle,” said lead author Cristian David Peña Martinez, PhD, also of the Garvan Medical Institute.

“This suggests that it plays a dynamic role in regulating gene activity.”

“We also discovered that i-motifs are formed in the promoter regions of cancer genes. For example, MYC Oncogenes encode one of cancer’s most notoriously ‘untreatable’ targets.”

“This opens up exciting opportunities to target disease-related genes through i-motif structures.”

“The widespread presence of the i-motif near these 'holy grail' sequences implicated in hard-to-treat cancers opens up new possibilities for novel diagnostic and therapeutic approaches,” said study co-author Sarah Kummerfeld, PhD, a researcher at the Garvan Medical Institute.

“It may be possible to design drugs that target the i-motif to affect gene expression, potentially expanding current treatment options.”

Team result Published in EMBO Journal.

_____

Christian David Peña Martinez othersi-motif structures are widely distributed in human genomic DNA. Embo JPublished online August 29, 2024, doi: 10.1038/s44318-024-00210-5

Source: www.sci.news

The solution to the mysterious link between clouds and climate

Eric S. Neitzel Fireground Communications LLC/AdobeStock

Central Park Reservoir is one of the few places in New York City to get a good view of the clouds. Looking north from the reservoir’s edge, there’s a large gap between the buildings that lets you see the clouds rolling in from the harbor. Meteorologist Kara Lamb suggested we try our hand at cloud watching here.

At the time, the sky is full of fluffy cumulus clouds beneath a ceiling of altostratus. One of them looks a lot like a whale. But Lam, who studies clouds at Columbia University in New York, doesn’t think they’re so strange. “Clouds are fascinating because they’re cool to look at,” he says. “But I think about clouds in terms of climate” – understanding how the sunlight they reflect and the heat they trap beneath them affect the Earth’s temperature.

What the casual cloud watcher might not know is that clouds are the biggest unknown in predicting future climate change to determine how this balance will change in a warming world. If we double carbon dioxide from pre-industrial levels, will the world get a manageable 1.5°C warming or a hellish 4.5°C warming? The biggest source of this uncertainty is our lack of understanding of clouds.

But researchers are making progress. Lamb is looking at ice crystals in the clouds, which play a surprisingly large role in influencing the climate. Some researchers are using cloud chambers, and are planning to set up cloud chambers…

Source: www.newscientist.com

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

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

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

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

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


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

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

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

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

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

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

About our experts:

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

For more information, visit the University of Sussex website.

Source: www.sciencefocus.com

Study reveals that Pompeii disaster survivors were killed by a second mysterious force

During the eruption of Mount Vesuvius in 79 A.D., residents were trapped under ash and rock, unable to escape. Surprisingly, a new study shows that some people did survive, only to meet their end later due to a different natural disaster.

The eruption covered the city in ash and rock particles for 18 hours, preserving the Roman inhabitants in a protective shell of solidified ash. However, experts discovered two skeletons in a house buried on top of the ash, rather than beneath it, indicating a massive earthquake as the cause of death.

Researchers investigating the house, Casa dei Pittori al Lavoro, noticed the absence of typical volcanic signs in the excavation near Vesuvius. Further examination revealed that the two men found in the house, around 50 years old, suffered severe injuries and were crushed by a collapsing wall due to the earthquake.

Scientists have discovered two skeletons in the ruins of a building in Pompeii and concluded that the cause of death was the collapse of a wall caused by an earthquake. – Image courtesy of Pompeii Archaeological Park

Residents who survived the initial eruption likely thought they were safe and attempted to flee, only to be met with powerful earthquakes. The combination of volcanic and seismic effects made it difficult to study the coincident earthquakes occurring at that time.

Researchers suggest that seismic activity during the eruption played a significant role in the destruction of Pompeii and may have affected the decisions made by its inhabitants facing imminent death.

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Source: www.sciencefocus.com

Dark energy could be even more mysterious than previously believed

The choice to name a new project the Dark Energy Spectroscopic Instrument (DESI) may come across as presumptuous. Dark energy, you see, is completely unseen; it does not emit any detectable light for a spectrometer to analyze. In fact, dark energy has never been directly observed and has managed to evade capture despite efforts made using the most advanced telescopes and detectors available.

As far as we understand it, dark energy is invisible, uniformly spread throughout space, does not interact with matter or light, and serves the sole purpose of accelerating the universe’s expansion through a mechanism that remains a mystery to us.

So, with the recent announcement of DESI’s initial data release, are we witnessing a shift in our comprehension of dark energy, as promised?

In the search for elusive dark energy, our observations offer limited insights: dark energy merely stretches space-time. To investigate different theories about dark energy, we must examine how this stretching occurred over cosmic time.

One method is to observe the universe’s expansion history, while another involves examining how matter accumulated within galaxies and clusters at various junctures in the universe’s past.

Efforts to measure the expansion rate often involve constructing a precise 3D map of the universe’s matter. By studying the spectra of light, we can determine how much it has stretched due to the universe’s expansion. By combining this information with accurate physical distances, we gain valuable insights into the universe’s evolution.

DESI’s new model has stirred speculation by proposing that dark energy may have a more intricate history than previously believed. If these indications prove to be accurate, they could revolutionize our understanding of not just the universe’s past, but also its eventual fate.

The Concordance Model of Cosmology outlines the prevailing model of the universe and its components. In this model, dark energy is viewed as a cosmological constant, providing a minimal flexibility to every part of space.

DESI and other surveys commonly report their dark energy findings in terms of an “equation of state” parameter denoted as w. A value of w = -1 is expected if dark energy behaves as a cosmological constant. Any deviation from this value implies a different characteristic for dark energy.

The recent DESI findings present a puzzling scenario: while a constant w of -1 aligns well with the results, a scenario where w is variable suggests a different interpretation. When combined with data from other sources, these results hint at a changing w, implying a varying impact of dark energy on the universe over time.

While the implications of these findings remain uncertain, they raise intriguing possibilities about the future course of the universe and the role of dark energy within it. Though still preliminary, these results suggest that dark energy may continue to surprise us in unforeseen ways in the future.

Source: www.sciencefocus.com

There is a possibility that dark energy is even more mysterious than previously believed.

Naming a new project the Dark Energy Spectroscopic Instrument (DESI) may come across as overly confident. This is because dark energy is undetectable and cannot be examined or analyzed through traditional methods like spectroscopy. Despite numerous attempts, dark energy has never been directly observed and remains a mystery in the realm of astrophysics.

Dark energy is believed to be a uniform force throughout the universe that does not interact with matter or light in any discernible way. Its primary function is to expand space at an accelerating rate, a process that baffles scientists due to its unknown underlying mechanism.

The recent release of data from DESI has sparked interest and debate in the scientific community. This project aims to shed light on the behavior of dark energy by mapping the expansion history of the universe. By studying the motion of galaxies and measuring the stretching of light emitted from distant objects, researchers can gain insights into the evolution of the cosmos.

The current prevailing model of cosmology suggests that dark energy exists as a static cosmological constant, affecting the fabric of space uniformly. However, DESI’s findings hint at a more complex history for dark energy, challenging conventional theories about its nature and implications for the future of the universe.

As researchers delve deeper into the mysteries of dark energy, they may uncover new discoveries that challenge existing paradigms and push the boundaries of our understanding of the cosmos. The DESI project represents an important step towards unraveling the enigma of dark energy and its profound impact on the universe.

Source: www.sciencefocus.com

Solution found for mysterious deaths of black-headed gulls in Denmark

Pet participation

What exactly can dogs offer cities? The answer is coming soon.

Reader Dorothy Sheckler informed Feedback that Brad D. Lee of the University of Kentucky will be presenting his views at the Soil & Water Conservation Association conference in Myrtle Beach, South Carolina, on July 22, 2024. What will Lee’s presentation topic be?Nutritional contributions of pet dogs in urban peri-urban environments” “.

Tensions may be palpable during the talks, as the host city announced that dogs will only be allowed on beaches this summer before 10 a.m. and after 5 p.m., and owners “must pick up and properly dispose of their feces.”

Mussel-bound Death

Through investigation and international cooperation, two preserved bodies that had long been forgotten were rediscovered.

Keith Moeliker, a biologist who studies surprising animal behavior (he discovered homosexual necrophilia in mallards, according to feedback on February 10, 2024), tells us what happened.

“The fate of Denmark’s black-headed gulls is dramatic.Chroicocephalus ridibundus“In 1952 a seagull stepped on a freshwater clam,” he writes, “and the clam closed its valve and refused to let go. The proof, of the seagull (now dead) with the clam still attached to its right foot, was found in an old photograph I found in the depths of the Internet.”

Mölliker learned that the photo was taken at the Hunting and Forestry Museum in Hörsholm, eastern Denmark. In 2017, the museum moved to and became part of another institution, the Green Museum in Auning, western Denmark. As is often the case with large and diverse museum collections, some treasures were safely stored but largely unnoticed. Mölliker got in touch with the Green Museum curator, who picked up the twin objects (officially named JSH 05542) from their resting place on a long shelf in a heavily refrigerated building.

“In April 2024, I was allowed to observe the black-headed gull in the museum’s collection storage facility and was able to take this photograph,” Moeliker continues (see below). “There I learned more: the gull had not died embracing the mussels, but had been shot together with the mussels near Solo on Zealand. [Denmark]Another special item from the same Danish collection is JHS 05924, the leg of a herring gull that was found trapped inside a half-open tin can in 1954.”

Mustache denial

Feedback consulted with native Iranian (or, in the ChatGPT era, human, if you prefer) translators to solve this puzzling mystery. Several recent studies published in Iranian research journals use strange wording in their titles. Here are three examples:

Analysis of the economic diplomacy of the Islamic Republic of Iran in international relations with emphasis on the rule of negation of the moustache“, published in Strategic Studies of Jurisprudence and Law.

A jurisprudential explanation of the show of force and the build-up of Iran’s military defense capabilities, approaching the rule of mustache negation“, published in Protection and Security Research.

The role of the moustache ban in the Islamic Republic’s foreign policy and international relationsPublished in ” Iranian Journal of Political Sociology.

Each paper is written in a mixture of Persian and Arabic, and includes a synopsis written in English, which includes a reference to “Moustache” as well as each title.

Why the moustache? Feedback’s language consultant was astonished. “Because the translator of the paper is a complete idiot!! The word for “path” in Arabic is [of doing something]’ is sometimes called SavilePersian [Farsi], Sybil It means “mustache.” The translator might just be Google.

The world will now find out what impact these moustache-twirling papers will have on international diplomatic relations.

Mustache measurement

While pursuing the intricacies of mustache negation rules, Feedback stumbled upon a (possibly unrelated) study published in 1982:Survival curves and growth rates of mustache populationsThe paper, written by Cliff Frohlich and Ruth Buskirk, reports measurements of “three previously unstudied characteristics of mustaches: hair length distribution, hair growth rate, and rate of hair shedding or weathering,” all of which were measured on “unshaven mustaches of 30-year-old Caucasian men.”

Eleven years later, Frohlich cited Mustache’s paper, studyPublished in Journal of Geophysical Research: Solid Earthdiscussed the subtle mathematical aspects of measuring earthquake strength. He noted that, like mustache growth, “earthquakes are just one of many phenomena for which a logarithmic plot of number versus magnitude is approximately a straight line.”

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

Do you have a story for feedback?

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

Source: www.newscientist.com

Scientists are baffled by the discovery of a mysterious cosmic sphere in the universe

Discovered by chance in 2019, Odd radio circles (ORCs) are circular regions of faint radio radiation with bright edges that are not visible to optical, infrared, ultraviolet, and X-ray wavelengths.

Some ORCs contain galaxies at their centers, while others do not, but what sets them apart is their size, which is significantly larger than normal galaxies. Some ORCs display a double ring structure, while others have a single ring. There are also some with internal arc-like structures that might be linked to galaxies surrounded by bubbles of radio emission.

While objects with high spherical symmetry are common in the universe, ORCs appear to be distinct from them all, prompting astronomers to classify them as a new type of object.


ORCs could potentially be a type of spherical shock wave generated by fast radio bursts, gamma-ray bursts, or neutron star mergers. If this is the case, they must be extremely ancient to have grown to such a large size.

Alternatively, they may be associated with material jets emanating from the central regions of radio galaxies, but explaining their size and the absence of central objects in all galaxies is challenging.

One intriguing theory suggests that ORCs are created by the fusion of two supermassive black holes in a central galaxy. The available data also support the idea that the shell is caused by a “shock termination” of high-energy particle winds from the central “starburst” galaxy.

Another hypothesis proposes that the ORC is the throat of a “wormhole,” a theoretical passage through spacetime. However, astronomers have yet to agree on the true nature of ORC.

This article addresses the question (by Bradford’s Brendan Owens): “What are strange radio circles?”

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Mars Express uncovers mysterious ‘spider’ near ‘Inca City’ on Martian outskirts

ESA’s Mars Express spacecraft found obvious traces of spider. They are scattered in the south pole region of Mars.

This image of an Inca city on Mars was taken on February 27, 2024 by the high-resolution stereo camera on board ESA’s Mars Express spacecraft. Image credit: ESA / DLR / FU Berlin.

“The Martian ‘spiders’ are not actual spiders, but form when spring sunlight falls on layers of carbon dioxide deposited during the dark winter,” said a member of the Mars Express team.

“Sunlight turns the carbon dioxide ice at the bottom of the layer into gas, which then accumulates and breaks through the ice sheet above.”

“During Mars’ spring, the gas explodes, dragging black material down to the surface as it progresses and shattering layers of ice up to a meter thick.”

“The resulting gas, laden with black dust, erupts through cracks in the ice in the form of tall fountains and geysers, before falling down and sinking to the surface.”

This creates a dark spot 45 m to 1 km (148 to 3,280 ft) in diameter.

This same process carves a distinctive “spider-shaped” pattern beneath the ice. Therefore, these black spots are evidence that a spider may be lurking underneath.

“Dark spots can be seen throughout the Mars Express image. But most of them can be seen as small specks in the dark region on the left, located just on the outskirts of a part of Mars called Inca City.” said the researchers.

“The reason for this name is no mystery: the network of linear, almost geometric ridges recalls Inca ruins.”

More formally known as Angustus Labyrinth. Inca City was discovered in 1972 by NASA’s Mariner 9 spacecraft.

“We still don’t know exactly how Inca cities formed. Sand dunes may have turned to stone over time,” the scientists said.

“Perhaps materials such as magma or sand are seeping through fractured sheets of Martian rock. Alternatively, the ridges could be ‘eskers,’ tortuous structures associated with glaciers.”

“The ‘walls’ of Inca cities appear to be part of a larger circle, 86 km (53.5 miles) in diameter.”

Scientists suspect that Inca City is located inside a large crater formed when rocks from space collided with the planet’s surface.

“This impact may have caused the fault to ripple in the surrounding plains, which was then filled with rising lava and then worn away over time,” the researchers said.

Source: www.sci.news

Webb delves into the mysterious depths of Messier 82

Astronomers using the NASA/ESA/CSA James Webb Space Telescope discovered the central starburst of Messier 82 (M82, NGC 3034, or Cigar Galaxy), a starburst irregular galaxy 12 million light-years away in the constellation A new image of the area was taken. of Ursa Major.

Messier 82 was observed by the NASA/ESA Hubble Space Telescope in 2006, showing a spiral disk, shredded clouds, and hot hydrogen gas right next to the galaxy. The NASA/ESA/CSA James Webb Space Telescope observed the center of Messier 82, capturing the structure of the galactic wind in unprecedented detail and revealing the characteristics of individual stars and star clusters. Image credits: NASA / ESA / CSA / Hubble / Webb / STScI / A. Bolatto, UMD.

Messier 82 is located approximately 12 million light years away. It can be seen high in the northern sky in spring, in the direction of Ursa Major in the north.

First discovered by German astronomer Johann Erath Bode in 1774, this galaxy is approximately 40,000 light-years in diameter.

Messier 82 is also called the Cigar Galaxy because of its elongated elliptical shape caused by the tilt of its star-like disk with respect to our line of sight.

This galaxy is famous for its unusually high rate of new star formation, with stars being born 10 times faster than the Milky Way.

Astronomer Alberto Borat and his colleagues at the University of Maryland led Webb's research. NIRCam (Near Infrared Camera) We will aim our instrument at the center of Messier 82 to closely observe the physical conditions that promote the formation of new stars.

“Messier 82 is thought to be the prototype of a starburst galaxy and has attracted a variety of observations over the years,” Borat said.

“Both the Spitzer Space Telescope and the Hubble Space Telescope have observed this target. With Webb's size and resolution, we can observe this star-forming galaxy and see all of this beautiful new detail.”

“Star formation remains a mystery because it is shrouded by a curtain of dust and gas, which poses an obstacle to observing this process.”

“Fortunately, Webb's ability to see into the infrared can help us navigate these ambiguous situations.”

“Furthermore, these NIRCam images of the center of the starburst were obtained using instrumental mode, which prevents very bright light sources from overwhelming the detector.”

“Even in this infrared image, dark brown dust tendrils are visible throughout Messier 82's bright white core, but Webb's NIRCam has revealed a level of detail that was historically hidden.”

“If you look closely toward the center, small green specks indicate areas of concentrated iron, most of which are supernova remnants.”

“The small red spots indicate regions where hydrogen molecules are illuminated by radiation from nearby young stars.”

“This image shows the Webb's force,” said Dr. Rebecca Levy, an astronomer at the University of Arizona.

“All the white dots in this image are stars or star clusters. We can start to distinguish between all of these small point sources, which will allow us to get an accurate count of all the star clusters in this galaxy. Masu.”

If you look at Messier 82 at slightly longer infrared wavelengths, you'll see clumpy tendrils, shown in red, extending up and down the galactic plane. These gaseous streamers are galactic winds blowing out from the starburst's center.

One of the research team's areas of focus was understanding how this galactic wind, caused by rapid star formation and subsequent supernovae, originates and affects the surrounding environment.

By resolving Messier 82's central region, astronomers were able to investigate where the winds originate and gain insight into how hot and cold components interact in the wind. .

Webb's NIRCam instrument was well-suited to tracking the structure of the galactic wind via radiation from sooty chemical molecules known as polycyclic aromatic hydrocarbons (PAHs).

PAHs can be thought of as very small dust particles that survive at low temperatures but are destroyed at high temperatures.

Much to the team's surprise, Webb's observations about PAH emissions highlight previously unknown fine structures in the galactic wind.

This emission, depicted as a red filament, moves away from the central region where the center of star formation is located.

Another unexpected finding was the similarity between the structure of the PAH emission and the structure of the hot ionized gas.

“It was unexpected that the release of PAHs resembled ionized gases,” Dr. Borat said.

“PAHs are not thought to survive very long when exposed to such strong radiation fields, so they are probably constantly being replenished.”

“This casts doubt on our theory and indicates the need for further investigation.”

team's paper will be published in astrophysical journal.

_____

Alberto D. Borat other. 2024. Observation of starbursts by JWST: Emission of polycyclic aromatic hydrocarbons at the root of the M 82 galactic wind. APJ, in press. arXiv: 2401.16648

Source: www.sci.news

The mysterious glow of Venus evades detection by computers, but not by the human eye

“Ash light” or AL is a faint mysterious glow or hue seen in the night hemisphere of Venus. It is often compared to Earthshine, the reflected light that illuminates the far side of the Moon.

First described by Italian astronomer Giovanni Riccioli in 1643, AL has been observed many times since then, but its faint, ephemeral, and elusive nature has prevented serious research. It’s here.

Even more problematic, AL has so far only been detected by the human eye, and no scientific instruments, either earth-based or space-based, have recorded this phenomenon.

Some authorities have declared this phenomenon to be an illusion, perhaps an eye contrast effect or even an “expectation bias.” Some have suggested that a defect in the equipment could explain the phenomenon. Light scattering, optical aberrations, background sky brightness, weather, etc.

But there are enough reliable reports about AL that some scientists can offer an explanation. These include reflected light from Earth, auroras, “airglow” radiation, lightning, and infrared (thermal) radiation from Venus’ atmosphere.

Most of these explanations are ignored for some reason. However, there is ample evidence that not only ultraviolet light from the sun, but also high-energy solar wind particles can excite oxygen atoms in Venus’ atmosphere.

This creates a pale green glow similar to that seen in the aurora borealis on Earth. However, the process is somewhat different because auroras on Earth are caused by Earth’s magnetic field interacting with solar particles, whereas Venus has no appreciable magnetic field.

It remains to be seen whether this explanation can explain all or some of the AL observations. Therefore, the long-standing mystery of AL may still turn out to be an illusion.

This article is an answer to the question (asked by Herman Townsend of Liverpool): “What is Ashen Light?”

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Can you guess the mysterious lost 80’s hit song that everyone is talking about? | Music

I
The song is only 17 seconds long and sounds like 80’s Genesis playing at the bottom of a pool. But this bouncy but sonically degraded snippet of pop has become one of the internet’s biggest and most enduring musical mysteries.

This clip was uploaded in 2021 by a person named Carl92 who wanted to see if anyone could identify it. “I don’t remember its origins,” he wrote on his site called WatZatSong, adding, “I found it among a bunch of very old files on a DVD backup… it feels kind of nostalgic.” But even after this 17-second sample of his was posted on his Reddit, a powerful pop culture spirit is rarely lost, not a single person was able to identify the song or the artist.

This quest captured people’s imaginations. Last June it was my own subreddit – Named after the song’s unofficial title “Everyone Knows That (Ulterior Motives)”, or EKT, and currently has approximately 27,000 members. And recently, TikTok has become popular, with predictable results. Users flooded me with unhelpful comments like “Have you tried Shazaming?” which is like telling someone who lost their keys to check their pockets.

Bass, a music journalist from the Netherlands, is one of the subreddit’s moderators. He attributes the explosion in this exploration to a cultural shift. “We live in an age where knowledge is freely available and music can be consumed with few restrictions,” he says. “Music that was lost in the pre-internet era can be very interesting to young people because it’s something very foreign to them and they can’t easily look up songs.”

20 year old content creator with fame kylie bogley is one such convert. “We’re in the prime of a lost medium that will be viewed with great fondness in the future, and I’m grateful to be a part of it,” she says.

She is EKT. “Lost Wave” This movement collects dusty and forgotten songs, perhaps recorded from the radio or buried in folders of old MP3s, and attempts to give them names and artists. “There is another unconfirmed song and it is called “The most mysterious song on the internet‘ The mystery has remained unsolved for nearly 20 years. But I think EKT has outgrown its popularity,” says Bogley. “I don’t think it’s possible that we can’t find an artist.”

One obstacle is that the sound quality is so poor that no one can fully agree with the lyrics. There is even some doubt as to whether the singer is male or female. However, internet sleuths have identified the drum machine and synthesizer used for this song, most likely a LinnDrum and a Yamaha DX7. This narrows down the release date to his 1983 years and beyond. They also analyzed the background frequencies and figured out the format of the DVD. Apparently Carl92 was playing. Beyond that, forensic analysis was unable to locate it.

Dozens of similar-sounding artists (Roxette, Savage Garden, the one who sang the theme song for the Pokémon TV series) have all been asked if it’s their song, but no luck was. Unsurprisingly, misinformation also spread. Bass recalled a Redditor he claimed to have heard at a McDonald’s in Poland. “This person fabricated an email from a company to trick the search community into believing we were trying to find a song,” he says. “I think that’s the point of creativity.”


This song may have been an unreleased demo or an advertising jingle. Bass’ theory is that the piece was created in the United States for a movie or advertisement and “ended up on his VHS tape.” Someone had been recording audio in his room with his VHS tape playing in the background, backed up the file to his DVD, and forgot about it. ” Some think it may have come from Japan. Searchers are now trying to contact an unknown singer named White Mike Johnny Grove, who has a “strikingly similar voice,” Bogley said. Please pay attention to this column.

As for Carl 92, he disappeared, probably out of fear that online detectives would search him for clues. Some say he must have staged the whole thing, but maybe it’s some of the music he generated using his AI? If so, he could have directed tens of thousands of people. You’ve succeeded in destroying it. However, there is no evidence that he was not real. The despondent tone of his near-final message, which came just a few months after he posted EKT, certainly rings true. “It’s a dead end,” he wrote. “I just lost interest in that song.” But the rest of the world is just getting started.

Source: www.theguardian.com

Scientists puzzled by mysterious burst of intergalactic radio waves hitting Earth.

It may be hard to miss, but unimaginably strong bursts of cosmic radiation happen possibly a thousand times every day. They are bright enough to overwhelm our radio telescopes from billions of light-years away.

However, fast radio bursts (FRBs) were not detected until 2007. Despite over a decade of investigation, they remain one of the most intriguing mysteries in astrophysics. Recent research offers new and promising clues about their origins, while also revealing why these space phenomena are so perplexing in the first place.

When FRBs were first discussed in seminars, the big question wasn’t “What astrophysical cause is causing this?” Instead, it was, “Isn’t this just a mechanical failure?”

FRBs last about 1 millisecond and spread out in frequency in a manner very similar to a blip from a pulsar. But the problem is, they don’t come from any known pulsars, they don’t repeat like pulsars, and they’re clearly much more powerful than any pulsar pulses we’ve seen before.



To make matters worse, for many years the only telescope that observed FRBs was the Parkes Observatory in Australia. The debate became even more heated when it turned out that some of the FRB-like bursts observed by Parkes did not come from astronomical sources.

These bursts, called “peritons,” were always suspected to be of terrestrial origin. But clever detective work by astronomers solved the case. Dr. Emily Petrov and her colleagues showed that Periton had a strong correlation with local lunchtime. In reality, radiation leaked from the observatory’s microwave when the door opened too early.

It was eventually revealed that the FRBs were indeed from far away in space. More radio telescopes were configured to record very short bursts of radio waves, and detection rates began to skyrocket.

Those bursts came from all over the sky, suggesting they didn’t originate in our galaxy. In the first decade after the discovery, theorists produced a huge number of papers explaining the possible origins of the bursts.

In 2012, repeated FRBs were discovered, ruling out origins requiring complete destruction, such as supernovae. It was soon discovered that there were many more repeated bursts, mostly occurring at irregular intervals.

As more outbursts are discovered, there is growing evidence that FRBs may be associated with extraordinarily powerful magnetars: neutron stars that rotate in extremely strong magnetic fields.

Recent evidence suggests that at least some FRBs originate from nearby spiral galaxies rather than elliptical galaxies.

Astronomers will need to continue collecting clues, looking for suggestive patterns in the data, and eagerly awaiting observational upgrades that will allow them to pinpoint the FRBs’ local environment.

Whatever the outcome, the fast radio burst is a great example of the fact that in science, when we look at the universe in new and different ways, we almost always discover something surprising that no one had ever thought to look for.

Source: www.sciencefocus.com

Potential Discovery of the Lightest Black Hole Ever Seen: A Mysterious Object

Artist's impression of a pulsar orbiting a black hole – one possible interpretation of the mysterious binary star system

Daniel Hutseller (artsource.nl)

Some 40,000 light-years away, a strange object could be either the heaviest neutron star or the lightest black hole ever seen, and it resides in a mysterious celestial void that astronomers have never directly observed. .

Neutron stars form when a star runs out of fuel and collapses due to gravity, creating a shock wave called a supernova and leaving behind an extremely dense core. Astrophysical calculations show that these nuclei must remain below a certain mass, about 2.2 times the mass of the Sun, or they will collapse further to form a black hole.

However, black holes have only been observed to have a mass more than five times that of the sun, leaving a gap in scale between neutron stars and black holes. Gravitational-wave observatories have observed several dense objects in this gap, but astronomers have never discovered them with conventional telescopes.

now, Ewan Barr Researchers at Germany's Max Planck Institute for Radio Astronomy discovered an object with 2.5 times the mass of the Sun by observing pulsars orbiting around it. A pulsar is a neutron star that emits pulses of light at regular millisecond intervals due to a strong magnetic field.

As predicted by Albert Einstein's theory of relativity, pulsars emit light with great regularity, but very large nearby objects can distort these rhythms. Dr. Barr and his team were able to calculate the mass of the pulsar's partner by observing the pulsar's pulses for more than a year using his MeerKAT radio telescope in South Africa.

“What we've discovered in this binary system appears to go beyond that [upper limit for neutron star mass]This suggests that there is some new physics going on here and that this is either a new type of star, or simply a black hole, the lightest stellar-mass black hole yet discovered. “There will be,” Barr said.

Pulsars are located in globular clusters, which are dense regions of stars and some rare objects that can pass close to each other. These unusual interactions could explain the mysterious object, Barr said.

If it's a black hole, researchers will be able to test theories of gravity that weren't possible before. “A pulsar is just a ridiculously accurate measuring device in orbit around a black hole, but it's not going anywhere. It's going to be around for the next billion years,” Barr says. “So this is an incredibly stable and natural test bed for investigating the physics of black holes.”

“If it's a neutron star, it would be more massive than any neutron star we've ever seen,” he says. Christine Dunn At Durham University, UK. “This actually tells us about the ultimate density that a star can support before it collapses under its own gravity and becomes a black hole. We need to understand the physics of matter at such extreme densities. I don't know what the limits are.”

Barr and his team plan to observe the pulsar with other telescopes over the next few years, looking for clues about what the object is. If it were a black hole, we would see the pulsar's orbit change over time, as the black hole dragged through spacetime around it, much like a ship dragging a small boat behind it. Or if it's a neutron star, more sensitive instruments might be able to detect the light.

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Source: www.newscientist.com

Potentially the heaviest neutron star ever observed found in mysterious object

A neutron star is the collapsed core of a massive star

www.science.org/doi/10.1126/science.adg3005

Some 40,000 light-years away, a strange object could be either the heaviest neutron star or the lightest black hole ever seen, and it resides in a mysterious celestial void that astronomers have never directly observed. .

Neutron stars form when a star runs out of fuel and collapses due to gravity, creating a shock wave called a supernova and leaving behind an extremely dense core. Astrophysical calculations show that these nuclei must remain below a certain mass, about 2.2 times the mass of the Sun, or they will collapse further to form a black hole.

However, black holes have only been observed to have a mass more than five times that of the sun, leaving a gap in scale between neutron stars and black holes. Gravitational-wave observatories have observed several dense objects in this gap, but astronomers have never discovered them with conventional telescopes.

now, Ewan Barr Researchers at Germany's Max Planck Institute for Radio Astronomy discovered an object with 2.5 times the mass of the Sun by observing pulsars orbiting around it. A pulsar is a neutron star that emits pulses of light at regular millisecond intervals due to a strong magnetic field.

As predicted by Albert Einstein's theory of relativity, pulsars emit light with great regularity, but very large nearby objects can distort these rhythms. Dr. Barr and his team were able to calculate the mass of the pulsar's partner by observing the pulsar's pulses for more than a year using his MeerKAT radio telescope in South Africa.

“What we've discovered in this binary system appears to go beyond that [upper limit for neutron star mass]This suggests that there is some new physics going on here and that this is either a new type of star, or simply a black hole, the lightest stellar-mass black hole yet discovered. “There will be,” Barr said.

Pulsars are located in globular clusters, which are dense regions of stars and some rare objects that can pass close to each other. These unusual interactions could explain the mysterious object, Barr said.

If it's a black hole, researchers will be able to test theories of gravity that weren't possible before. “A pulsar is just a ridiculously accurate measuring device in orbit around a black hole, but it's not going anywhere. It's going to be around for the next billion years,” Barr says. “So this is an incredibly stable and natural test bed for investigating the physics of black holes.”

“If it's a neutron star, it would be more massive than any neutron star we've ever seen,” he says. Christine Dunn At Durham University, UK. “This actually tells us about the ultimate density that a star can support before it collapses under its own gravity and becomes a black hole. We need to understand the physics of matter at such extreme densities. I don't know what the limits are.”

Barr and his team plan to observe the pulsar with other telescopes over the next few years, looking for clues about what the object is. If it were a black hole, we would see the pulsar's orbit change over time, as the black hole dragged through spacetime around it, much like a ship dragging a small boat behind it. Or if it's a neutron star, more sensitive instruments might be able to detect the light.

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Source: www.newscientist.com

Porous iceberg on Saturn’s moon Titan may be a mysterious ‘magical island’

Infrared image of Saturn’s icy moon Titan

NASA/JPL-California Institute of Technology/Stephane Le Mouelik, Virginia Pasek

Saturn’s moon Titan is home to strange “magical islands” that appear and disappear over hours to weeks. These so-called islands are actually porous, sponge-like masses of snow that can slowly fill with liquid before sinking.

Titan’s thick atmosphere is filled with complex organic molecules that can clump together and fall to the moon’s surface like snow. Sintin Yu Researchers at the University of Texas at San Antonio thought that snow could be the cause of the magical islands. To test their idea, they took advantage of what we know about these atmospheric compounds and how they are expected to interact with Titan’s oceans.

Titan’s liquid is methane, not water, so any solids on the surface of these oceans would normally be expected to sink quickly. Water molecules tend to stick together and displace other substances, but methane easily sticks to other molecules, so the surface tension of a pool of liquid methane is very low.

“Water molecules just love themselves by excluding certain molecules,” he says. michael marasca from NASA’s Jet Propulsion Laboratory in California was not involved in the study. “But if you put methane on the same surface, it will start crawling all over the place.” That means Titan’s methane oceans and lakes should immediately swallow up any solids that are expected to float. It means that.

But that clearly won’t happen on the magical island, which appeared as a temporary bright spot in observations from the Cassini spacecraft. “For us to see magical islands, they cannot float briefly and then immediately sink,” Yu said in the paper. statement. “You have to stay afloat for a while, but not forever.”

Researchers have found a solution to this problem. When large amounts of snow accumulate on the coast, they can form sponge-like, porous ice. Once these porous “icebergs” separated from the land, they could float in Titan’s oceans for long enough to rival Cassini’s observations. The researchers calculated that this would work if the sponge-like structure contained enough free space (at least about 25 to 50 percent, depending on the exact composition of the ice).

However, this does not mean that these mysterious islands are definitely porous icebergs. “We’re narrowing down different scenarios for the magical island, but we don’t know the answer yet,” Malasca says. Other possible explanations include nitrogen gas bubbles, waves caused by wind or solid ocean deposits. However, this provides evidence that Titan’s temporary islands may actually be suspended matter from this strange world’s atmosphere.

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Source: www.newscientist.com

Radio Bursts from Distant Galaxies: A Mysterious Phenomenon

Artist's impression of the path of a fast radio burst (not to scale) FRB 20220610A

M. Kohnmesser/European Southern Observatory

The unexplained flash of radio waves that reached Earth in 2022 originated from a small group of galaxies about 8 billion light-years away. This discovery expands our understanding of how mysterious fast radio bursts (FRBs) form.

To date, astronomers have discovered more than 1,000 FRBs. FRBs are strange bursts of high-frequency electromagnetic radiation that cross the sky in just a few milliseconds. Some events repeat and are detected as blinking multiple times. The main explanation is that FRBs are produced by powerful spinning stars known as magnetars, highly magnetized spinning stars left behind after a massive star explodes as a supernova.

About 50 FRBs have been identified as the source of the Milky Way and other galaxies. But in 2022, astronomers discovered the most distant and powerful FRB yet: non-recurring FRB 20220610A, which dates back to when the universe was just 5 billion years old.

alexa gordon A team of researchers from Northwestern University in Illinois followed up on this finding. Researchers discovered in April 2023 using the Hubble Space Telescope that FRB 20220610A originates from a small dwarf galaxy. This galaxy was part of a compact group of seven galaxies so small that the entire galaxy fit within the Milky Way. “This is a very unusual system,” Gordon says. “At this distance of his FRB, only about 0.1 to 1 percent of galaxies belong to compact groups.”

Such groups are thought to be active regions of star formation. This supports FRB's explanation of magnetars, as they probably form early in a galaxy's evolution when hot, massive stars explode. In compact groups, “galaxies are interacting fairly frequently,” Gordon says. This triggers star formation consistent with what is seen in his FRB study, produced by newer, near-Earth sources.

This work was uploaded to the arXiv preprint server late last year and was also presented at today's presentation. Meeting of the American Astronomical Society in New Orleans.

This discovery further expands the types of environments in which FRBs are known to exist. “The majority are in star-forming spiral galaxies,” Gordon says. “But he also found FRBs in galaxy clusters, dwarf galaxies, and globular clusters. The addition of 'compact groups' to this list shows that we are finding his FRBs in a variety of locations.” Here's another example. ”

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Source: www.newscientist.com

New, Mysterious Species of Moth Discovered in Europe by Scientists

Myrrhatia arcuata, a newly discovered moth species in Europe reveals gaps in our knowledge about European Lepidoptera. Its unique characteristics and the mysteries surrounding its habitat and adaptations highlight the need for continued research in this field. Above is an adult male Myrrhatia arcuata. Credit: Hausmann et al.

The order Lepidoptera, which consists of butterflies and moths, is known to number approximately 11,000 individuals.
seed and is considered well researched. However, the discovery of new genera and species in the Geometrid family suggests there is still much to learn. The results of this study were recently published in the journal Zookey. What is the name of the moth? Myrrhatia arcuata The discovery, by a team of researchers from Germany, Austria, and the United Kingdom, is one of the most remarkable discoveries in Lepidoptera in recent decades.

UFOs from decades ago

Source: scitechdaily.com