The 10 Quickest Jets of 2024: The Fastest in the World

Before the movie Top Gun, kids dreamed of being astronauts or sports stars. But after the release of the film, everyone wanted to be pilots in high-tech fighter jets.

Our gallery provides information about the 10 fastest jet planes in the world and their history.

Strap in and get your sick bags ready as we take to the skies to see which jet is the fastest.

10 – F-22 Raptor

An F-22 Raptor flies over Kadena Air Base, Japan on a routine training mission.Photo by Sergeant Major Andy Dunaway/U.S. Air Force

The F-22 Raptor is a single-seat stealth fighter with a top speed of Mach 2.25 and long-range cruise capability. Its stealth capabilities are so advanced that it’s not allowed to be sold outside the United States. Despite its speed and stealth, it has been overshadowed by the F-35 Lightning II jet. Only 187 were built, making it rare to see in the air.

9 – MiG-29 Fulcrum

Bangladesh Air Force MiG-29 with full afterburner.Photo credit: Bangladesh Air Force/Wikipedia

The MiG-29 was built by the Soviet Union and has a top speed of Mach 2.3. Despite its age, it’s still used in many countries around the world.

8 – F-14 Tomcat

An F-14D Tomcat flies over the Persian Gulf region. Photo by Sergeant Rob Tabor/USAF

The F-14 has a top speed of Mach 2.34 and has been in service for over 30 years.

7 – MiG-23 Frogger

An aerial view of a Soviet-era MiG-23 jet in flight.Photo credit: U.S. Air Force

The MiG-23 has a top speed of Mach 2.35 and is known for its agility. Over 5,000 were built and it is still in use today.

6 – Sukhoi Su-27 Flanker

Sukhoi Su-27 demonstrating its capabilities at the MAKS-2005 air show.Photo credit: Dmitry Pichugin/Wikipedia

The Sukhoi Su-27 has a top speed of Mach 2.35 and is known for its excellent range and flight maneuverability. It remains in production more than 40 years after its introduction.

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Source: www.sciencefocus.com

Giant sea scorpions, the largest insects, were all predators.

All pterosaur eurypterids (sea scorpions), giant aquatic arthropods with large claws, were considered apex predators, but some scientists believe that certain species are not predatory because their claws are weak. suggested. New research reveals that their claws were stronger and were only used to capture prey. Other appendages chewed it up. Fossils found in the pterosaur eurypterids show that some species specialized in lightly armored crustaceans and fishes, but most species specialized in heavily armored fishes.

Size of sea scorpions (Euripterids) over time.pterosaur eurypterid Jachelopterus (Background), the largest arthropod of all time, and a eurypterid of the Hibertopteridae family. Siltoctenus (Foreground) The size of a human (an average British male) compared to the silhouette of its eurypterid relatives. Image credit: Simon Powell.

Sea scorpions (family Eurypteridae) are ancient aquatic creepy crawlers (arthropods) that lived long before the dinosaurs, from 467 million to 253 million years ago.

These include the “pterygoids” (428 to 391 million years ago), which had large, fearsome claws. Grows up to 2.5 meters longthe biggest bug that ever existed.

An extinct millipede called Arthropleura was It is claimed that it is even largerHowever, if the length of 12 to 14 preserved body segments is 76 cm, the body length of an animal with 32 segments is (76/12 x 32), which is just over 2 m (excluding the head).

All pterosaurs, eurypterids, were thought to have been ferocious apex predators. tyrannosaurus About their time.

Later, some scientists believed that pterygoid claws acutiramus It could only catch and slice weak, soft-bodied prey, and its eyesight wasn't sharp enough Becoming a predator.It has been demoted from the top echelon of predators and even a label is attached “Pussycat”.

According to new research, nails acutiramus It was much more robust. Suggestions that they would snap were based on incorrect assumptions.

The apparent lack of an “elbow joint” doesn't hurt either. This was at the base of the nail. Also, the claws were used only for catching prey. If it had more powerful mouthparts in the groin, it would kill or chew it up.

It doesn't matter that their eyesight is poor either. Their prey is large, and some non-predatory insects (such as bees and butterflies) have eye indicators similar to arthropods that were considered predators.

Computer modeling and experiments with robotic swimming eurypterids also show that pterosaurs were slower swimmers than expected. They were so large that relatively small swim paddles could not provide sufficient propulsion, so a flat tail (telson) served both as a rudder and as propulsion.

Analysis of the types of fossils found with pterygomorphs also suggests that: acutiramus It specializes in lightly armored crustaceans (called foliaceans) and pterophytes. Eretopterus Therodont fish and pterigotus and Jachelopterus About the more heavily armored placoderm fish.

Evidence of predation (claw marks) and fossilized feces (coprolites) confirm that some eurypterids ate armored fish, trilobites, and even other eurypterids.

Previous studies have generally dismissed suggestions that Eurypteridae influenced the evolution of early vertebrates (fish) in a predator-prey arms race, but this new study This suggests that pterosaurs and other eurypterids probably had some influence on the evolution of early vertebrates.

The evolutionary relationships of pterygoids have also changed. Their shape, vision, fossil associations, ecology, and stratigraphic record all indicate that: acutiramus It was more basic Jachelopterus and pterigotus.

This is the largest arthropod in history (Jachelopterus lenaniae) It is now estimated to be about 2.6 meters long, 10 centimeters longer than previous estimates. The biggest bug is now a little bigger.

this paper will appear in Earth Science Bulletin.

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S. J. Brady. 2023. Paleoecology of the pterygoid eurypterids: Pladicnia and paleontological assemblages. Earth Science Bulletin 98(4); doi: 10.3140/bull.geosci.1891

Source: www.sci.news

Fermi’s Time-Lapse Tour: A One-of-a-Kind View of the Gamma-Ray Sky

new movies from NASA's Fermi mission shows the intensity of gamma rays, the highest energy form of light, with energies of over 200 million electron volts (MeV), detected by Fermi's Large Area Telescope between August 2008 and August 2022 . For comparison, visible light has an energy of 2 to 3 electrons. bolt. Lighter colors indicate the location of more intense gamma ray sources.

“The Milky Way's bright, steady gamma-ray glow is punctuated by intense flares of near-light-speed jets that last for days, powered by the supermassive black hole at the center of the distant galaxy.” Dr. Digel said. Staff Scientist at SLAC National Accelerator Laboratory.

“These dramatic eruptions can appear anywhere in the sky, occurred millions to billions of years ago, and their light is just reaching Fermi as we see it. ”

“The first thing you see in a movie is a steady arc of light across the screen,” said Dr. Judy Racusin, a research scientist at NASA's Goddard Space Flight Center.

“It's our sun, and its apparent motion reflects the Earth's annual orbital motion.”

Most of the time, Fermi's Large Area Telescope (LAT) picks up faint glimpses of the Sun due to the influence of accelerated particles called cosmic rays. When they come into contact with the sun's gases or the light it emits, gamma rays are produced.

But sometimes, the sun suddenly brightens up in a powerful eruption called a solar flare, temporarily making our star one of the brightest sources of gamma rays in the sky.

The Fermi team created an all-sky time-lapse movie using 14 years of data acquired by Fermi's large-area telescope. Image credit: NASA Goddard Space Flight Center/DOE/LAT Collaboration.

“The new film depicts the sky from two different perspectives,” the astronomers said.

“The rectangular view shows the entire sky with the galaxy's center in the middle.”

“This highlights the central plane of the Milky Way, which glows with gamma rays produced from cosmic rays striking interstellar gas and starlight.”

“Many other sources are also scattered, such as neutron stars and supernova remnants.”

“Above and beyond this central band, we look out beyond our galaxy and into a wider universe studded with bright, rapidly changing light sources.”

“Most of these are actually distant galaxies that are better seen from a different perspective, centered around our galaxy's north and south poles.”

“Each of these galaxies, called blazars, has a central black hole with the mass of more than a million suns.”

“Somehow, black holes produce jets of matter that move at very high speeds. Using a blazar, we can see one of these jets almost directly below us, enhancing their brightness and variability. Masu.”

“This fluctuation indicates that something has changed in these jets,” Dr. Raksin said.

“We monitor these sources regularly and alert other telescopes, both in space and on the ground, when something interesting is happening.”

“We need to catch these flares quickly before they disappear, and the more observations we can collect, the better we can understand these events.”

Fermi plays a key role in a growing network of missions working together to capture these changes as they unfold in space.

“Many of these galaxies are very distant,” the researchers said.

“For example, the light from the blazar known as 4C +21.35 has been traveling for 4.6 billion years. This means that the flare-ups we see today actually happened when the sun and solar system began to form. means.”

“Other bright blazars are more than twice as far away, providing an impressive snapshot of black hole activity across cosmic time.”

“Many short-lived events that Fermi studies, such as gamma-ray bursts, the most powerful cosmic explosions, cannot be seen in time-lapse.”

“This is the result of processing data over several days to sharpen the image.”

Source: www.sci.news

Huge Neutron Stars Could Have Cores Composed of Unconfined Quark Matter

The core of a neutron star contains the highest density of matter in the universe. This highly compressed matter can undergo a phase transition in which nuclear matter dissolves into unconfined quark matter, releasing its constituent quarks and gluons. However, it is currently unknown whether this transition occurs inside at least some physical neutron stars. In a new study, physicists from the University of Helsinki, the University of Stavanger, the Flatiron Institute, and Columbia University quantified this possibility by combining information from astrophysical observations and theoretical calculations.

Artist's impression of a neutron star. Image credit: Sci.News.

Neutron stars are extreme astrophysical objects containing the densest matter found in the modern universe.

It has a radius of about 10 km (6 miles) and a mass of about 1.4 solar masses.

“A long-standing unresolved question concerns whether the enormous central pressure of a neutron star can compress protons and neutrons into a phase called cold quark matter. In this exotic state, individual protons and neutrons no longer exist. We don’t,” said Professor Aleksi Vuorinen of the University of Helsinki.

“The quarks and gluons that make them up are instead freed from typical color confinement and can move almost freely.”

In a new paper, Professor Vuorinen and colleagues provide the first quantitative estimate of the possibility of a core of quark matter existing inside a massive neutron star.

They showed that quark matter is almost inevitable in the most massive neutron stars, based on current astrophysical observations. The quantitative estimates they extracted put the likelihood in the 80-90% range.

For there to be a small chance that all neutron stars are composed only of nuclear matter, the change from nuclear matter to quark matter must occur through a strong primary phase similar to the phenomenon in which liquid water turns to ice. Must be a metastasis.

This type of rapid change in the properties of neutron star matter could destabilize the star in such a way that even the formation of a tiny quark matter core could cause the star to collapse into a black hole.

An artist's impression of the various layers inside a giant neutron star. The red circle represents a significant amount of quark matter core. Image credit: Jyrki Hokkanen, CSC.

“A key element in deriving the new results is a series of large-scale supercomputer calculations that utilize Bayesian inference, a branch of statistical deduction that estimates the likelihood of various model parameters through direct comparison with observed data. “, the authors explained.

“We demonstrate that the Bayesian component allows us to derive new limits on the properties of neutron star matter, approaching the so-called conformal behavior near the center of the most massive and stable neutron stars.”

Dr. Joonas Nettila from the University of Helsinki added: “It is interesting to see specifically how each new neutron star observation improves the ability to estimate the properties of the neutron star material.” .

“Being able to compare theoretical predictions with observations and constrain the possibility of quark-matter nuclei requires hundreds of supercomputers,” said Jonas Hirvonen, a doctoral student at the Flatiron Institute and Columbia University. “We had to spend tens of thousands of CPU hours.”

“We are very grateful to the Finnish Supercomputer Center CSC for providing us with all the necessary resources.”

of paper It was published in the magazine nature communications.

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E.Annara other. 2023. Strongly interacting matter exhibits unconfined behavior in massive neutron stars. Nat Commune 14, 8451; doi: 10.1038/s41467-023-44051-y

Source: www.sci.news

A Peculiar Tale: California Forever, the Impromptu Metropolis of Tech Tycoons

A road sign near a property recently purchased by Flannery Associates near Rio Vista, California.

Josh Edelson/AFP via Getty Images

For the past six years, a mysterious group called Flannery Associates has been buying up swaths of farmland in Solano County, north of San Francisco.now it has Plans to build a city on an area of ​​more than 200 square kilometers have been made public, and the name of the project has been revealed. california forever.

Jan Sramek, CEO of the business, said: work Investors include venture capitalist Marc Andreessen and LinkedIn co-founder Reid Hoffman. They are…

Source: www.newscientist.com

Unusual ‘Sad Trombone’ Effect Detected in Radio Burst from Space

allen telescope array

Seth Szostak/SETI Institute

Short, powerful bursts of radio waves from space are becoming increasingly bizarre. Astronomers discovered 35 of these bursts from a single object with a pattern unlike anything seen before.

sophia sheikh Researchers at California's SETI Institute and colleagues observed the object, a fast radio burst (FRB) called FRB 20220912A, during 541 hours of observation with the Allen Telescope Array in California. In each of this burst from his Fed, they discovered a phenomenon called “sad trombone”…

Source: www.newscientist.com

Alabama’s Plan to Use Nitrogen Gas for Execution: A Little-Known Method

Alabama has announced it will use nitrogen gas in an upcoming execution. This would make the state the first to use such a method as officials struggle with a shortage of lethal injection drugs. Legal challenges are on the horizon as the matter is under consideration.

While Alabama is eager to use nitrogen, details of the protocol remain under wraps, with some information on how the process works being kept from the public. Death row inmate Kenneth Eugene Smith noted his lack of access to unredacted state protocols that explain how the process works, alongside other inmates under the sentence.

In addition to the novelty of Smith’s case, he is also a rare survivor of a failed execution attempt from last year. Smith, convicted for his role in the 1988 murder of a preacher’s wife, Elizabeth Sennett, remains awaiting execution with the proposed nitrogen method set for January. In light of unsuccessful attempts to execute Smith using lethal injection, the state agreed to try an alternative method.

Read more about this story hereNBCNews.com Watch Harry Jackson NOW on NBC News NOW Fridays at 5pm ET/4pm CT.

Although lethal injection remains Alabama’s primary method of execution, the state authorized the use of nitrogen in 2018 and aims to use it in Smith’s case. With many questions remaining and the state’s questionable track record, critics argue that the decision to use an untested method won’t win public trust.

This month, Smith’s lawyers argued before a federal judge that the use of nitrogen hypoxia violates the Constitution’s ban on cruel and unusual punishment. An anesthetist testifying on Smith’s behalf expressed concerns about possible adverse effects on Smith’s health, such as vomiting, suffocation, or going into a vegetative state.

Source: www.nbcnews.com

ALMA discovers earthquake-like ripples in the disk of an old barred spiral galaxy

astronomer using Atacama Large Millimeter/Submillimeter Array ALMA observed disk bending waves in BRI 1335-0417, the oldest known spiral galaxy, more than 12 billion years old. This unprecedented observation reveals the galaxy’s dynamic growth pattern, showing the motion of a vertically oscillating disk similar to ripples in a pond. This study is the first time such a phenomenon has been detected in an early galaxy.

This simulation shows how the galactic disk is disturbed and seismic ripples propagate throughout the disk. Image credit: Brand-Hawthorne & Tepper-Garcia, University of Sydney.

Bar structures play an important role in driving galaxy evolution and forming disk structures.

In galaxies, axisymmetric stellar bars exert a gravitational torque on the gas, driving it toward the galactic center and forming concentrated stellar structures such as bulges and core disks.

This process may also promote the accretion of gas onto black holes, which are observed as active galactic nuclei.

Bars can also cause radial migration of gas and stars, which is essential for explaining the stellar kinematics observed in galaxies similar to the Milky Way.

“Thanks to a cutting-edge telescope called ALMA, we have been able to observe the ancient galaxy BRI 1335-0417 in greater detail,” said lead author Dr Takafumi Tsukui, an astronomer at the Australian National University.

“In particular, we were interested in how gas moves within and across galaxies.”

“Gas is a key component for star formation and provides important clues about how galaxies actually drive star formation.”

In this case, Dr. Tsukui and his colleagues were not only able to capture the movement of gas around BRI 1335-0417, but also revealed the formation of seismic waves, a first for this type of early galaxy.

The galaxy’s disk moves similar to the ripples in a pond after a stone is thrown into it.

ALMA detected emission from carbon ions in the galaxy BRI 1335-0417. Image credit: ALMA / ESO / NAOJ / NRAO / T. Tsukui & S. Iguchi, doi: 10.1126/science.abe9680.

“The vertical oscillatory motion of the disk is due to external factors, such as new gas flowing into the galaxy or contact with other small galaxies,” Tsukui said.

“Both possibilities would bombard the galaxy with new fuel for star formation.”

“Furthermore, our study revealed rod-like structures within the disk.”

“The galactic rods can destroy gas and transport it towards the center of the galaxy.”

“The bar discovered at BRI 1335-0417 is the most remote known structure of its kind.”

“Taken together, these results point to the dynamic growth of young galaxies.”

“We know that early galaxies formed stars at much faster rates than modern galaxies,” said co-author Dr Emily Wisnioski, also from the Australian National University.

“This is also true for BRI 1335-0417, which has a similar mass to our Milky Way galaxy but forms stars hundreds of times faster.”

“We wanted to understand how gas is supplied to keep up with this rapid rate of star formation.”

“Spiral structures are rare in the early Universe, and exactly how they form remains unknown.”

“This study also provides important information about the most likely scenario.”

“While it is impossible to directly observe the evolution of galaxies, our observations only provide snapshots, so computer simulations can help piece together the story.”

of findings will appear in Royal Astronomical Society Monthly Notices.

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Takafumi Tsukui other. 2024. Disk bending waves detected in a barred spiral galaxy at redshift 4.4. MNRAS 527 (3): 8941-8949; doi: 10.1093/mnras/stad3588

Source: www.sci.news

New Fossil Discovery Shows Baleen Whales Adapted to Large Bodies in Cold Southern Waters for the First Time

Baleen whales (mysterious animals) are the largest animals on Earth. How they achieved such enormous sizes is still debated, and research to date has focused primarily on when they grew, rather than where they grew. was. Paleontologists now report on the remains of a toothless baleen whale (chaeomysticete) from South Australia. At an estimated length of 9 meters, it is the largest baleen whale from the early Miocene. Analysis of body size over time shows that ancient baleen whales in the Southern Hemisphere were larger than those in the Northern Hemisphere.

Mysterious gigantism from the early Miocene. Image credit: Ruairidh Duncan

It was previously thought that the onset of the Ice Age in the Northern Hemisphere about 3 million years ago triggered the evolution of truly gigantic baleen whales.

The new study, led by Dr James Rule of Monash University and the Natural History Museum in London, reveals that this evolutionary size jump did, in fact, occur as early as 20 million years ago, and in the exact opposite direction in the southern hemisphere. I made it.

The major discovery came from a study of 16- to 21-million-year-old fossils held in Museum Victoria’s collection.

This specimen, the anterior end of the lower jaw of a large edentulous baleen whale, was discovered in 1921 on a cliff face on the banks of the Murray River in South Australia, but was largely unrecognized in collections.

In their study, Dr. Ruhl and colleagues explain how whales evolved to be larger in the southern hemisphere rather than the northern hemisphere, and that whales have been larger in the southern hemisphere throughout their evolutionary history (about 20 million to 30 million years). It was shown that

The discovery highlights the vital importance of the Australian and wider Southern Hemisphere fossil record in putting together a global picture of whale evolution.

The Murray River whale fossil confounds that theory, although previous leading theories were based primarily on fossils found in the northern hemisphere.

“The Southern Hemisphere, and Australia in particular, has always been overlooked as a frontier for fossil whale discovery,” says Dr Eric Fitzgerald, a palaeontologist at Museums Victoria Research Institute.

“Like the Murray River whale, the fossil whale discoveries in the south have shaken up whale evolution, giving us a more accurate, truly global picture of what was happening in the oceans in ancient times. .”

Researchers have discovered that the tip of a baleen whale’s jaw can expand depending on its body size.

They estimated the baleen whale to be about 9 meters long.

“The largest whales alive today, such as the blue whale, reach the length of a basketball court,” Dr. Ruhl said.

“About 19 million years ago, Murray River whales were nine meters long, already a third of this length. So baleen whales were well on their way to becoming ocean giants.”

of result will appear in Proceedings of the Royal Society B.

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James P. Rule other. 2023. A huge baleen whale emerges from its cold cradle in the south. Procedure R. Soc. B 290 (2013): 20232177; doi: 10.1098/rspb.2023.2177

Source: www.sci.news

A new species of toad has been found living in African volcanoes

Scientists have identified a new genus and species of true toad from a single specimen found in a high-altitude forest. mount kenya, an extinct volcano in Kenya and the second highest mountain in Africa after Kilimanjaro. Contrary to the popular belief that most of Kenya’s amphibians arose after volcanic activity subsided millions of years ago, this new species is related to the Kenya volcanic toad (Kenya Phrynoides vulcanis) – Its origins may date back as far as 20 million years, making it considerably older than the volcanic formation of Mt Kenya itself.

artistic performance Kenya Phrynoides vulcanis (A), dorsal view of the left hand of the holotype (B), and photographs of the dorsal (C) and ventral (D) sides of the holotype before preservation. Image credit: Liedtke other., doi: 10.1093/zoolinnean/zlad160.

Dr Simon Loader, lead curator of vertebrates at the Natural History Museum, London, said: ‘Many of Kenya’s mountains are volcanic or geologically relatively new, so discovering ancient lineages that have lasted for millions of years is unlikely. It’s amazing.”

“It’s a real challenge to figure out how it got here.”

“We can’t say for sure, but it seems likely that they were once more widespread, and as the climate has changed over the past tens of millions of years, they have tracked their way through tropical forests, with their final destinations being the mountaintops. It was ‘Mt Kenya’. ”

The discovery of Kenya’s volcanic toads calls into question the concept of the Kenya interval, a term used to describe the striking contrast in amphibian diversity between Kenya and its neighboring countries.

Ethiopia and Tanzania have long been hotspots for amphibian biodiversity, but Kenya’s geological history and frequency of tectonic activity make it a difficult place for these organisms to thrive.

unique features Kenya Phrynoides vulcanis This suggests that the Kenyan Interval may not be as simple as previously believed.

When this toad was first discovered in Mount Kenya’s pit in 2015, it already seemed very different from the species normally seen in the area.

“We were really surprised to see this animal. It looked nothing like anything we had seen before, but it was similar to what we know and call the Tanzanian animal. Ta” Churamiti MaridadiIt is a forest tree toad that lives in the Ukaguru Mountains rainforest,” said National Museums of Kenya curators Dr Patrick Maronza and Dr Victor Wasonga.

Kenya Phrynoides vulcanisDistinctive features include its small size, more frog-like body, and distinctive green and brown markings.

Genetic and morphological differences from other known toad species have led to its recognition at the genus level.

Clues from physical features such as enlarged fingertips suggest it may be a climber.

Its thumb has a sharp tip known as a nuptial spine found in many male frogs and toads, which helps the male grasp the female and encourage reproduction.

“The forest toad found in the mountains of East Africa is unusual and does not resemble typical toads,” said Dr. Hendrik Müller, a researcher at Martin Luther University Halle-Wittenberg.

“More interestingly, some individuals are known to have an unusual reproductive strategy called ovoviviparity.”

“In ovoviviparity, the eggs hatch inside the female’s body. This means that the chicks are born from the mother as small toads, rather than as tadpoles.”

This finding is reported in the following article: paper inside Zoological journal of the Linnean Society.

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H. Christoph Liedtke other. A new species of toad discovered from Mount Kenya sheds light on the biogeography of East Africa’s mountains. Zoological journal of the Linnean Society, published online on November 7, 2023. doi: 10.1093/zoolinnean/zlad160

Source: www.sci.news

Different Forms and Varieties of Eating Disorders

Eating Disorders: The Basics debunks the stereotype that eating disorders only affect a certain group of people and emphasizes their universal impact and the need for comprehensive, early treatment and support. I am.

According to eating disorder experts, eating disorders affect everyone, regardless of race, gender, or age.

Medical experts say the myth that only thin, white, wealthy girls develop eating disorders is preventing other patients from receiving diagnosis and treatment.

Psychiatrist Janet Treasure, general practitioner Dr Elizabeth McNaught and therapist Jess Griffiths (all survivors of eating disorders) agree that this stereotype is not true for other people, including black women and men. She says it means she has a hard time asking for help.

They urge clinicians to treat all eating disorders as serious, even those that don’t involve weight loss, such as purging.

The importance of early intervention and comprehensiveness in treatment

Professor Treasure, Dr McNaught and Jess from King’s College London also highlight the importance of early intervention to save lives and the important role of fathers in helping girls recover.

their books Eating disorders: the basics – TV presenter Strictly Winner Stacey Dooley – For schools, health care workers, and families.

This guide details common risk factors, different types of eating disorders, the latest treatments, and provides advice for families on how to support their loved one’s recovery.

“Eating disorders are often thought of as affecting thin, white, affluent girls. But they lack true discrimination about who they affect,” the authors write. states.

“Other groups, such as men, racial minorities, transgender people, and people from disadvantaged socio-economic backgrounds, can remain in our communities struggling with eating disorders for years untreated. There is a gender.

“It is also important to recognize that all eating disorders are serious and all eating disorders deserve treatment and support.

“It doesn’t have to be a lifelong or fatal disease, but it can often be due to lack of preparedness and lack of awareness of symptoms in people who are underweight.”

Recognize the universal impact of eating disorders

Problematic behaviors related to eating food are common around the world. These can occur at any stage of life and affect everyone, regardless of race, gender, or age.

eating disorder Based on the latest evidence on anorexia, bulimia, bulimia, and other conditions.

The guide also features real-life stories from people who have developed eating disorders, as well as letters of hope to support those still suffering.

These stories include those of patients who were told they were not sick enough to need help.

Despite the risks and pain associated with her condition, Carla Lisette said her purging disorder would only be taken seriously if it met the criteria for anorexia.

Furthermore, she added: “Although most people with purge disorder do not become underweight, that does not mean they are at a healthy weight for their bodies or that they are not harming themselves. It doesn’t even mean it. The purge could be deadly.”

In the letter, Christina Taylor was told she was “too healthy” to be helped, even though she drank excessively and felt sick 10 times a day.

“This (receiving the letter) was one of the most invalidating experiences of my life. I truly felt that there was no point in continuing this way.”

Professor Treasure and his co-authors say other challenges remain when it comes to eating disorders, including:

  • Food poverty, ultra-processed foods, and less sharing of home-cooked meals. These are among the environmental factors behind eating disorders.
  • Men often face societal pressure to “be manly.” This can create further secrecy about one’s disorder and create barriers to receiving treatment.
  • Body mass index (BMI) may not be useful in many situations. The authors state that the risk of poor health is related to the degree of weight loss, not absolute body weight. Some people may have a “normal” BMI but still be at risk for serious physical harm.
  • Fathers and partners may feel left out, as if eating disorders are “women’s work”, or siblings may be seen as too young to be involved. However, the authors say it plays an important role in supporting your loved one’s recovery.

References: Eating Disorders: The Basics, by Elizabeth McNaught, Janet Treasure, and Jess Griffiths.
DOI: 10.4324/9781003342762

Source: scitechdaily.com

The impact of chip-integrated lasers on the field of photonics

Chip-scale ultrafast mode-locked laser based on nanophotonic lithium niobate.Credit: Alireza Marandi

Researchers have developed a compact mode-locked laser integrated into a nanophotonic platform that can generate ultrafast light pulses at high power. This breakthrough in the miniaturization of MLL technology has the potential to significantly expand photonics applications.

Innovation in mode-locked laser technology

Setting out to improve a technology that typically requires bulky benchtop equipment, Quishi Guo and colleagues have miniaturized a mode-locked laser (MLL) with an integrated nanophotonics platform to the size of an optical chip. This result shows promise for the development of ultrafast nanophotonics systems for a wide range of applications.

Possibility of small MLL

Model-locked lasers (MLLs) can generate coherent ultrashort pulses of light at very fast speeds on the order of picoseconds to femtoseconds. These devices have enabled numerous techniques in the field of photonics, including extreme nonlinear optics.photon Microscopy and optical computing.

However, most MLLs are expensive, power-hungry, and require bulky, separate optical components and equipment. As a result, the use of ultrafast photonic systems has generally been limited to benchtop laboratory experiments. Furthermore, so-called “integrated” MLLs aimed at driving nanophotonics platforms have significant limitations, such as low peak power and lack of controllability.

Breakthrough advances in nanophotonics MLL integration

Through hybrid integration of semiconductor optical amplification chips and novel thin-film lithium niobate nanophotonic circuits, Guo other. We created an optical chip-sized integrated MLL.

According to the authors, this MLL generates ultrashort light pulses of about 4.8 picoseconds at about 1065 nanometers with a maximum output of about 0.5 watts. This is the highest output pulse energy and peak power of any MLL integrated into a nanophotonics platform.

Furthermore, the researchers show that the repetition rate of the integrated MLL can be tuned over a range of about 200 MHz and that the coherence properties of the laser can be precisely controlled, creating a fully stable on-chip nanophotonic frequency comb source. provided a path to.

Learn more about this breakthrough advancement below.

Reference: “Ultrafast mode-locked lasers in nanophotonic lithium niobate” Qiushi Guo, Benjamin K. Gutierrez, Ryotosekine, Robert M. Gray, James A. Williams, Luis Ledezma, Luis Costa, Arkadev Roy, Selina Zhou, Mingchen Liu, and Alireza Marandi, November 9, 2023; science.
DOI: 10.1126/science.adj5438

Source: scitechdaily.com

NASA’s Rotating Explosive Rocket Engine Takes Flight with 3D Printing Technology

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Engineers at NASA’s Marshall Space Flight Center in Huntsville, Alabama, successfully completed a 251-second high-temperature combustion test of a full-scale rotary explosion rocket engine combustor in fall 2023, achieving more than 5,800 pounds of thrust. Credit: NASA

NASAMarshall Space Flight Center tested a 3D-printed Rotating Explosive Rocket Engine (RDRE) for more than four minutes and was able to generate significant thrust. This test is essential for deep space missions and represents a step forward in NASA’s development of an efficient propulsion system for the Moon. Mars vision.

NASA has achieved a new benchmark in the development of an innovative propulsion system called the Rotating Explosive Rocket Engine (RDRE). Engineers at NASA’s Marshall Space Flight Center in Huntsville, Alabama, tested his new 3D-printed RDRE for 251 seconds (or over four minutes) and were able to generate more than 5,800 pounds of thrust.

This type of sustained burn emulates the typical requirements for a lander touchdown or deep space burn that could set a spacecraft on a course from the Moon to Mars, the center said. said Thomas Teasley, lead Marshall combustion equipment engineer.

RDRE’s first high-temperature fire test was conducted in Marshall in the summer of 2022 in partnership with In Space LLC and Purdue University (Lafayette, Indiana). The test generated more than 4,000 pounds of thrust for nearly a minute. The main objective of the latest tests was to extend the combustor to different thrust classes, support all types of engine systems, and maximize the diversity of missions it can deliver, from landers to upper stages to supersonics. Teasley said the key is to better understand how to increase the Reverse propulsion is a deceleration technique that has the potential to land larger payloads, and even humans, on the surface of Mars.

Test stand video taken at NASA’s Marshall Space Flight Center in Huntsville, Alabama, shows the ignition of a full-size rotary-explosion rocket engine combustor that ignited for a record 251 seconds and achieved more than 5,800 pounds of thrust. It is shown.

“RDRE significantly increases design efficiency,” he said. “This shows we are getting closer to developing lightweight propulsion systems that will allow us to send more mass and payloads into deep space, a critical component for NASA. From the moon to Mars vision. “

Engineers at NASA’s Glenn Research Center in Cleveland; Venus Aerospace, Houston, Texas, is working with NASA Marshall to identify ways to scale the technology for higher performance.

RDRE is managed and funded by the Game Changing Development Program within NASA’s Space Technology Mission Directorate.

Source: scitechdaily.com

Transforming NASA’s ISS Resupply with Revolutionary Technology



Illustration of Sierra Space’s first dream chaser, DC#1 (Tenacity). The Dream Chaser spacecraft developed by Sierra Space for NASA is gearing up for a demonstration mission to the ISS in 2024, with a focus on cargo delivery and in-orbit certification. .Credit: Sierra Space

NASA Sierra Space’s Dream Chaser spacecraft is scheduled for a demonstration flight to the ISS in 2024, carrying cargo transport and various on-orbit tests to ensure operational readiness for future missions. be exposed.NASA and Sierra Space are making progress toward the maiden flight of the company’s Dream Chaser spacecraft. international space station. The unmanned cargo spaceplane is scheduled to begin demonstration missions to orbital complexes in 2024 as part of NASA’s commercial resupply services.

Dream chaser and shooting starManufactured by Sierra Space, Louisville, Colorado, the Dream Chaser cargo system consists of two main elements: the Dream Chaser spacecraft and the Shooting Star cargo module. As a lifting body spacecraft, Dream Chaser is designed to be reused up to 15 times. HL-20 spacecraft It was developed at NASA’s Langley Research Center in Hampton, Virginia.Shooting Star, a spaceplane cargo module companion, is designed to support the transportation and disposal of pressurized and unpressurized cargo to the space station. The cargo module can only be used once and is disposed of before reentry.

The Dream Chaser system will be mounted on a ULA (United Launch Alliance) Vulcan Centaur rocket from Space Launch Complex 41 at Cape Canaveral Space Force Station in Florida, inside a 5-meter fairing. It can be launched by folding its wings. Fairing panels protect the spacecraft during ascent, but are discarded once it reaches orbit. Dream Chaser’s cargo module and wing-mounted solar arrays will be deployed during an autonomous rendezvous with the space station. In the event of disaster, Dream Chaser is designed to be ready for launch within as little as 24 hours.

NASA and Sierra Space are making progress toward the company’s Dream Chaser spacecraft’s maiden flight to the International Space Station. The unmanned cargo spaceplane is scheduled to begin demonstration missions to orbital complexes in 2024 as part of NASA’s commercial resupply services.Credit: Sierra SpaceMission overview

During the first flight, Sierra Space will conduct an in-orbit demonstration to qualify Dream Chaser for future missions. Teams from NASA Kennedy Space Center in Florida, NASA Johnson Space Center in Houston, and Dream Chaser Mission Control Center in Louisville, Colorado will monitor the flight. Sierra Space flight controllers will control the Dream Chaser spacecraft at the launch pad until it is handed over to NASA Kennedy’s Sierra Space ground operations team after landing.

The far-field demonstration will be conducted outside the vicinity of the space station before the spacecraft enters the invisible 2.5-by-1.25-by-1.25-mile (4-by-2-by-2-kilometer) boundary around the ellipsoid. . Rotating laboratory. These demonstrations are required before Dream His Chaser enters joint operations with his NASA team at Mission Control Center in Houston. These include demonstrating postural control, translational movements, and aborting functions.

Near-field demonstrations must be performed in close proximity to the space station, and include activation and use of light detection and ranging (LIDAR) sensors, responding to commands sent from the space station, retreating from the station in response to commands, and initially This includes maintaining proximity. 1,083 feet (330 meters) from the station, then 820 feet (250 meters), and finally 98 feet (30 meters). After the successful completion of the demonstration, Dream Chaser will move towards the space station.

As Dream Chaser approaches the orbiting laboratory, it will eventually park approximately 38 feet (11.5 meters) from the space station, where the station’s crew will use the Canadarm2 robotic arm to maneuver the spacecraft in front of the team on the ground. Hold on to the cargo module fixtures. Attach the cargo module to the earth-facing port of the Unity or Harmony module.

Dream Chaser will carry more than 7,800 pounds of cargo on its first flight to the International Space Station. On future missions, Dream Chaser is designed to remain on station for up to 75 days and deliver up to 11,500 pounds of cargo. Cargo can be loaded onto the spacecraft up to 24 hours before launch. Dream Chaser can return more than 3,500 pounds of cargo and experimental samples to Earth, and more than 8,700 pounds of trash can be disposed of during reentry using its cargo module.return to earthDream Chaser will remain on the space station for approximately 45 days before being uninstalled using Canadarm2. After departure, the spacecraft can land within 11 to 15 hours at the earliest, with the possibility of landing daily if weather conditions permit.

Dream Chaser’s landing weather criteria typically require crosswinds of less than 17.2 mph (15 knots), headwinds of less than 23 mph (20 knots), and tailwinds of less than 11.5 mph (10 knots). Thunderstorms, lightning, or rain within a 20-mile radius of the runway or 10 miles along the approach path are not acceptable conditions for landing. Detailed flight rules help controllers determine whether a landing opportunity is favorable.

A combination of Dream Chaser’s 26 Reaction Control System thrusters ignites, sending the spacecraft out of orbit. Dream Chaser re-entered Earth’s atmosphere and glided in the style of NASA’s Space Shuttle to a runway landing at Kennedy Launch and Landing Facility, becoming the first spacecraft to land at the facility since the Space Shuttle’s last flight in 2011. becomes.Once Dream Chaser is powered down after landing, the Sierra Space ground operations team will transport Dream Chaser to the Space Systems Processing Facility for necessary inspections, unload remaining NASA cargo, and prepare for the next mission. let’s start doing ….Sierra Space (formerly Sierra Nevada Corporation) was selected in 2016 as NASA’s third commercial cargo replenishment spacecraft to service the International Space Station.


Source: scitechdaily.com

Apple Ex-Employee’s iPhone Keyboard Hack Simplifies Screen Use

Here are some easy ways to impress the people at Genius Bar. A former Apple employee shares an easy-to-do keyboard hack that makes inputting numbers, especially numbers, smoother for users. In TikTok clip Viewed 17 million times technologist-turned-musician Tyler Morgan shows off features hidden in plain sight that allow you to do things like numeric keyboard shortcuts. He also introduced a fun “Harry Potter” command that Siri uses to turn the flashlight on and off. Just say “Lumos” (a Hogwarts spell that creates light on the tip of a wizard’s wand, etc.) and your iPhone’s flashlight will turn on. Conversely, if you say “Knox,” the light on your wand will go out and your flashlight will magically go out. Users can also ask Siri to identify songs playing in the background. Morgan said in another video additionally proven We recommend taking a screenshot of the entire web page, not just a portion of what’s on your screen. After you take a shot, there is an option to create and save a PDF in the top right part of your iPhone screen. Just tap Entire Page on the right side of the Screen tab. Keyboard hacks to try today Here are some easy iPhone keyboard hacks that are worth trying. AFP (via Getty Images) A simple and very effective way to enable Caps Lock on your iPhone keyboard is to double-tap the uppercase up arrow symbol. This will allow you to type uppercase letters until you turn the feature off. If you press and hold a letter, you can easily see different versions of the accented letter on top of the letter without having to install an international keyboard. Morgan’s tips also include a convenient way to display the numeric keyboard and automatically revert to the alphabet keys after use. Just press and hold the “123” tab in the bottom left corner while viewing the alphabet. When you enter a number, the screen temporarily changes to a numeric keypad, and when you release “123” it returns to letters. Here are some easy ways to get the most out of your iPhone’s keyboard. Dear Grease – Stock.adobe.com Also, if you accidentally press and hold the wrong number or symbol, keep your finger on the screen and slide it to change it to the number or symbol you actually want. Another useful tip is that if you hold down the spacebar, the cursor will move freely and easily through large groups of text like a mouse.

Source: nypost.com

New study sheds light on the visual masking phenomenon, unraveling the mystery of “invisibility”

A new study has revealed how visual masking, a phenomenon in which rapid succession of images leads to unconscious image processing, occurs in both humans and mice. This study highlights the role of the cortex in conscious perception and provides important insights into the brain’s visual processing mechanisms.

Delve into the mysterious optical illusions and science of visual masking.

Recent research published in natural neuroscience Visual masking is a phenomenon that plays an important role in how we perceive things, or rather how we don’t “see” them. This study not only revealed aspects of conscious perception in the brain, but also demonstrated that this phenomenon occurs in both humans and mice.

Visual masking occurs when a person does not consciously recognize an image because another image is displayed in rapid succession. For effective masking, the first image must appear and disappear quickly, followed by her second image within about 50 milliseconds.

Groundbreaking research in visual perception

Allen Institute researcher Dr. Sean Olsen and his colleagues have delved into the science behind this optical illusion and shown for the first time that it also occurs in mice. After training the mice to report what they saw, the researchers were also able to pinpoint the specific areas of the brain needed for the visual masking illusion to work.

“This is an interesting observation, that what exists in the world is not accurately reflected in your perception,” Olsen said. “Like other optical illusions, we think this tells us something about how the visual system works and, ultimately, the neural circuits underlying visual perception.”

Exploring the brain’s role in visual recognition

Scientists discovered this strange phenomenon in the 19th century, but why and how the human brain does this remains a mystery.

The study narrows down the parts of the brain involved in perceiving the world around us, said Dr. Christoph Koch, a Distinguished Fellow at the Allen Institute who led the study with Dr. Olsen and Dr. Sam Gale. Ta. , a scientist at the Allen Institute.

When a rain of photons hits our retina, the information follows a predetermined path from the eyeball through several different areas of the brain and into the highly-processed areas of the cortex, the wrinkled outermost shell of the brain. It ends with Previous research on visual masking has led scientists to believe that neurons in early parts of the brain, in the retina and its pathways, are activated even when a person is unaware that they are looking at an image. I know. In other words, your brain sees things without your knowledge.

From mouse to human: parallel recognition

To explore where unconscious sensations turn into conscious perceptions and actions, scientists first taught 16 mice to move a small mouse in the direction of a rapidly flashing image in exchange for a reward if they chose the correct direction. I trained him to spin a Lego wheel. The scientists then added different masking images on either side of the screen immediately after the target image. Adding a mask prevented the animal from performing the task correctly. This means that the animal can no longer recognize the original target image.

Visual masking had never been tested in mice before, so the research team had to create a task for mice, in which the images and the way they were displayed were different from those used in previous human studies. I meant that. To confirm that the optical illusion they showed to rodents was also relevant to us, the research team tested it on 16 people (using keystrokes instead of a wheel). It turns out that human perception (or lack thereof) and mouse perception of this particular visual masking illusion are very similar.

This result implies that conscious perception is occurring in the visual cortex or in higher regions of the cortex downstream. This is consistent with the general sentiment in the field that the cortex is the seat of conscious cognition in mammals, including us, Koch said.

Reference: “Visual cortex is required for posterior masking in mice” by Samuel D. Gale, Chelsea Stroder, Corbett Bennett, Stefan Mihalas, Christoph Koch, and Sean R. Olsen, November 13, 2023 Day, natural neuroscience.
DOI: 10.1038/s41593-023-01488-0

Source: scitechdaily.com

Researchers identify unique species of seal in the Arctic

This scientific study used satellite transmitters, population counts, and DNA analysis of tissue samples to describe the special Kangi ringed seal in the Ilulissat Icefjord. Here, a satellite transmitter is attached to the seal’s back.Credit: Pinngortitaleriffik – Greenland Institute of Nature Research

Local hunters in the Icefjord near Ilulissat are familiar with a special type of ringed seal known as the Kangia seal. Kangia seals vary in size and appearance, being significantly larger than the common Arctic ringed seal, and with markedly different fur colors and patterns. Recent scientific research has revealed that this distinctive seal has been genetically separated from Arctic seals over a long period of over 100,000 years.

Exploring the natural wonders of the Arctic can be difficult. Extreme weather and vast distances often hinder researchers’ quest to uncover nature’s mysteries.

However, a research project led by Greenlandic and Danish researchers has succeeded in describing a new species of ringed seal that lives in an ice fjord near Ilulissat in West Greenland. A unique natural area on the UNESCO World Heritage List.

The results were recently published in a prestigious scientific journal. molecular ecology.

Kangia ringed seals are larger than the typical Arctic ringed seal, and their fur is a different color and has more distinctive markings.Credit: Pinngortitaleriffik – Greenland Institute of Nature Research

small population

For years, researchers worked with local hunters to trap seals in nets and attach small satellite transmitters to their backs. As the seals flew, satellite transmitters sent messages about the seal’s location.

“We found that the Kangia seals mainly stayed within the ice fjords. We were able to count the seals from the plane, so we estimated that there was only about one seal. There are 3,000 special Kangi ringed seals,” said Akual Rosing Asvid, a senior researcher at the Greenland Institute for Nature Research Pingoltitalerifik and one of the researchers who supported the study. .

Color and pattern of the fur of the Kangia ringed seal (left) and a typical Arctic ringed seal (right).Credit: Pinngortitaleriffik – Greenland Institute of Nature Research

Their small population is very unusual compared to the typical Arctic ringed seal, which is huge and often travels thousands of kilometers around the North Pole in search of food.

isolated for thousands of years

The researchers also took small tissue samples from the captive seals. The samples were sent for genetic analysis to determine the seal’s identity. DNA The results revealed that Kangia ringed seals are genetically distinct from typical Arctic ringed seals.

Kangia ringed seals live in the Ilulissat Icefjord, which is a UNESCO World Heritage Site due to its spectacular and unique nature.Credit: Pinngortitaleriffik – Greenland Institute of Nature Research

However, where and how the Kangia ringed seal became isolated from other Arctic ringed seals and why it acquired new special biological characteristics remains a mystery.

Perhaps other arctic fjords also have special seals

The study highlights that there is still much we don’t know about the biodiversity of the Arctic and its potential to adapt to climate change and human activities.

“There are many other fjords in the Arctic that have not yet been studied in detail, and ringed seals may also carry new genetic mutations in these areas,” said Rune Dietz, professor at Aarhus University’s School of Ecological Sciences. Point out. he participated in the research.

Reference: “Evolutionarily distinct ringed seals of the Ilulissat Icefjord” Aqqalu Rosing-Asvid, Ari Löytynoja, Paolo Momigliano, Rikke Guldborg Hansen, Camilla Hjorth Scharff-Olsen, Mia Valtonen, Juhana Kammonen, Rune Dietz, Frank Farsø Rigét, Steve By H Ferguson, Christian Leidersen, Kit M. Kovacs, David M. Holland, Jukka Jarnvall, Petri Auvinen, Morten Tange Olsen, October 19, 2023. molecular ecology.

DOI: 10.1111/mec.17163

Source: scitechdaily.com