Paleontologists discover significant discrepancies in growth patterns between ancient and modern mammals from the Jurassic era

In a new study, paleontologists used synchrotron X-ray tomography of annual growth in dental cementum from fossil mammals belonging to three Jurassic animal groups to elucidate the origin of mammalian growth patterns that are intrinsically linked to mammals being warm-blooded.

Jurassic forest mammals. Image courtesy of © Zhao Chuang.

“This is the first time we've been able to reconstruct the growth patterns of early mammals in such detail,” said Dr Elise Newnham, a postdoctoral researcher at Queen Mary, University of London and the University of Bonn.

“By studying the spacing and texture of these growth rings, we can not only tell us how fast they grew at different stages of their life, but also make inferences about their metabolism and overall lifespan.”

The study calls into question previous assumptions about the growth patterns of our mammalian ancestors and the idea that these animals may have grown in a way similar to modern mammals.

Instead, the study answers a question raised by similar recent studies of early mammalian ancestors: when did modern mammalian life cycles evolve?

The researchers found that the first signs of modern mammalian growth patterns — high growth rates in young animals that stop at puberty — began in the earliest true mammals about 130 million years ago, compared with relatively little change throughout their lives in previously evolved mammalian forms.

However, like mammals, these animals grow slower and live much longer than modern small mammals such as mice and mice, with a maximum lifespan of 8 to 14 years.

The timing of this change in growth rate, combined with changes in tree-ring structure, indicates when these animals reached puberty and possibly sexual maturity.

“These data suggest that while all living small mammals reach sexual maturity within a few months of birth, the earliest mammals took several years to reach sexual maturity, supporting the results of a recent study on one of our study animals. Cruxatodon” Dr Pam Gill, a researcher at the Natural History Museum and University of Bristol, said:

“What's more, we find that this long, drawn-out life history was common to early mammals throughout the Jurassic Period.”

“Our results suggest that distinctive mammalian life history traits, such as high metabolic rate and extended parental care, evolved gradually over millions of years,” Dr Newnham said.

“The Jurassic period appears to have been a pivotal period in this evolution.”

The researchers used a technique called synchrotron X-ray tomography to image tiny growth rings in fossilized root cementum, the bone tissue that attaches teeth to the jaw. These rings are similar to those found in trees, but on a microscopic scale.

By counting the growth rings and analysing their thickness and texture, they were able to reconstruct the growth patterns and lifespan of the extinct animals.

“This work is a great example of how new technologies are revolutionizing our understanding of the distant past,” said Professor Thomas Martin from the University of Bonn.

“By closely examining these fossilized teeth, we can gain valuable insight into the lives of organisms that lived millions of years ago.”

“We are incredibly excited to be involved in this project,” said researcher Dr Jen Bright, from the University of Hull.

“Putting Jurassic fossils in a particle accelerator (synchrotron) to reconstruct the past sounds like science fiction, but it's actually possible!”

of Investigation result Published in a journal Scientific advances.

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Ellis Newham others2024. Origin of mammalian growth patterns during the Jurassic mammalian radiation. Scientific advances 10(32); doi: 10.1126/sciadv.ado4555

Source: www.sci.news

Struggling to find the perfect gift for your teenager? Discover the top tech gifts for teens in 2024

When it comes to choosing gifts for teenagers, gift cards are often the go-to option. With new technology constantly emerging, it can be challenging to find products that are both worth buying and will be loved by your teen.

Our list features a variety of fantastic tech gifts for teenagers, from cutting-edge gadgets for amazing selfies to popular items that can transform a regular bedroom into the ultimate teen hideaway. These products cater to every budget and level of tech knowledge – you don’t have to be a tech expert to enjoy these innovative devices.

These tech gifts are truly inspiring.

If you know a teenager who’s into science, don’t miss out on these amazing science gifts for teens.

Best Tech Gifts for Teens

Adding a color-changing LED light strip can instantly elevate a dull bedroom into a vibrant, multi-colored space. Perfect for adding a touch of excitement to a sleepover, gaming session, or just a relaxing night at home. This LED light strip may be one of the best tech gifts for teenagers.

Philips Hue Series Tapo is a well-known name in smart LED strips, and this version of Tapo is a great budget-friendly choice.

Setting up is easy – simply stick the strips on shelves, screens, or other bedroom furniture. The strips are five meters long and can be cut to any desired size. Use the Tapo app to select preset lighting moods, effects, and timers to automatically control the multicolored LEDs. It works over standard home Wi-Fi and is compatible with Alexa and Google Assistant for voice control.

For more gift ideas, check out our guide to the best sci-fi games.

Latest Philips Hue Lightstrip deals:

Tapo Light Strip Latest Deals:

Insta360 X3

At first glance, this small gadget may seem expensive, but its impressive features speak for themselves.

The Insta360 X3 features a 5.7K 360° camera with useful functions like image stabilization, horizon lock, and HDR mode. With the extended selfie stick, the camera intelligently edits your footage to provide a unique third-person perspective, almost like having your personal videographer.

Don’t miss out on the best instant cameras for more photo gift ideas.

While the camera captures the action in 360°, you have the freedom to choose the best angle for your video.

Additional features include:

  • 8K quality 360° time lapse video
  • Automatically saves 15 or 30 seconds of footage before hitting the shutter button
  • Convenient automated editing and live 360° streaming allow viewers to see from every angle
  • Focus on a single person, animal, or moving object and keep it centered in the frame.
  • Waterproof up to 10m, extendable to 50m with a diving case (sold separately)

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Crosley Voyager Portable Turntable

A portable record player like the Crosley Voyager makes a fun and unique gift for teenagers. Music enthusiasts will appreciate having a stylish turntable in their room.

This turntable’s portability is a standout feature – easily pack it up and take your music with you to parties, vacations, and other gatherings.

Despite its vintage look, the turntable is equipped with modern features: Built-in stereo speakers and Bluetooth for streaming music from your phone, plus a headphone jack for private listening. The turntable also offers three speed settings for playing traditional records.

The Crosley Voyager is an affordable turntable option. If you’re unsure about it, explore our top record players currently available.

While you’re here, check out the best sunrise alarm clocks too.

Mini projector

A portable projector is a must-have for sleepovers or movie nights at home. Whether your teen has a TV in their room or not, this gadget will enhance their viewing experience with a projection size of up to 210 inches.

This is also perfect for PlayStation and Xbox enthusiasts.

While projectors can be pricey, this one offers a balance of affordability and quality. Highly rated by customers, it supports Full HD with 7500 lumens and allows you to choose your preferred projection size from 35 inches to 210 inches, from a distance of 3.7 feet from the wall.

Featuring built-in Hi-Fi speakers, it also has an audio-out port for connecting external speakers or headphones. Once set up, you can connect your phone, tablet, laptop, or gaming console to enjoy TV shows, movies, and photos (some devices may require an HDMI cable).

Explore our guide for the best projectors for your home for more options.

Ultimate Ears BOOM 3 Wireless Bluetooth Speaker

There are few speakers that deliver both style and sound quality, but the Ultimate Ears Boom 3 manages to do just that. With its unique “unicorn” appearance, this speaker stands out from the crowd. It also boasts impressive technical specifications.

The Boom 3 is fully waterproof, allowing you to play music underwater for 30 minutes, and it floats to the surface when released, making pool parties even more enjoyable. Moreover, if your recipient or their friends own other Ultimate Ears speakers, you can link up to 150 of them to synchronize music in one location.

This speaker delivers 360° sound and is made with a highly elastic material used in motorcycle jackets and firefighting gear. Ultimate Ears has conducted over 25 durability tests, ensuring it can withstand even the most energetic users.

The rechargeable battery provides up to 15 hours of playtime on a full charge. Power Up Dock for a seamless charging experience. For speaker options, explore our selection of portable speakers, shower speakers, or noise-canceling headphones.

Auraglow LED USB Wall or Tabletop Word Clock

Looking for a great gift under £25? Consider this unique clock from Auraglow. Instead of traditional numbers, this clock displays the time in 5-minute intervals. LEDs light up the relevant letters on a black panel to indicate the time.

The clock comes with a USB cable for connecting to various power sources, and you can add an adapter for more flexibility. It can be wall-mounted with a hanging slot or propped up on a desk or shelf thanks to its flat base.

If black isn’t your style, the clock is also available in copper. Explore our guides for the best wireless phone chargers, power banks, portable chargers, and charging stations for more useful tech ideas.

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Apexel 10-in-1 Cell Phone Camera Lens Kit

For Instagrammers, photographers, or selfie enthusiasts, a smartphone lens attachment is an ideal choice if you want to enhance your phone’s camera capabilities without investing in a new camera. This set, with 10 different lens attachments stored in a convenient pouch, is compatible with most smartphones and tablets, including iPhone, Samsung, Huawei, and Sony models.

The kit includes macro, wide-angle, and telephoto lenses, along with fun accessories like a fisheye lens, a star filter, a kaleidoscope attachment, and even a polarizing filter to reduce glare and reflections for sunny days.

Source: www.sciencefocus.com

Discover abandoned navigation aids that guided planes in the past

VOR NVS is located on the edge of the village of Navas del Rey in Spain

Ignacio Evangelista

These isolated structures were once vital pillars of aviation navigation, but are little known today due to their remote location. Ignacio Evangelista’s The stunning shot highlights these beacons, known as VORs (Very High Frequency Omnidirectional Range Stations), and the role they play in charting routes in the skies for aircraft.

VOR CMA

Ignacio Evangelista

VORs are essentially giant antennas that send out radio signals from remote locations to help planes locate and stay on course by flying from VOR to VOR. You can think of the signals as “breadcrumbs,” Evangelista says. The separation is necessary to avoid broadcast interference between VORs.

Stations like the ones mentioned here are disappearing as they are increasingly being replaced by satellite-based GPS, but while GPS is a more accurate means of navigation, VORs provide a backup during events like solar storms and GPS interference that could wreak havoc without them, Evangelista said.

Vol Brai

Ignacio Evangelista

Their locations are public, so anyone can find the remaining VORs simply by using a GPS — “an interesting technical gyre,” in Evangelista’s words — which prompted him to document some of the more photogenic stations before they disappear forever.

Seen from above, the first two stations are in Spain: VOR NVS, located on the edge of the village of Navas del Rey, 50km from Madrid, VOR CMA, 1.5km from the village of Calamocha, and the last one, VOR BRY, located on the edge of the French village of Bray-sur-Seine.

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Source: www.newscientist.com

Scientists discover unknown species of armadillo

of Cricket Armadillo (Dasypus novemucinctus) There are actually four different species, including a previously undescribed endemic species. Guiana ShieldAccording to a new study.



Guiana Navajo Armadillo (Dasypus guianensisImage courtesy of Quentin Martinez, https://quentinmartinez.fr.

Armadillos are New World placental mammals. CingulataAlong with anteaters and sloths, they form part of a superclade that dates back 100 million years ago. Xenomorphs.

The cricket armadillo The most widely distributed xenarthropod species Across the Americas.

Recent studies suggest that it consists of four distinct lineages whose taxonomic status is unclear.

“It has been widely believed that the cricket armadillo ranges from northern Argentina to southern Illinois, but in recent years some scientists have presented evidence that it is in fact a complex of several different species,” said Dr. Frédéric Delschuk, research director at the CNRS.

“By studying the DNA of armadillos across their range, we were able to perform a very detailed genomic analysis and become convinced that there are in fact four different species of armadillos.”

“Under the new classification, armadillos found in the United States should be called Mexican long-legged armadillos,” added Dr Anderson Feijo, a researcher at the Field Museum.

“In addition, a new species of Guiana Navajo armadillo (Dasypus guianensis) is the first armadillo described in the past 30 years.

In this study, the researchers analyzed the mitochondrial and nuclear genomes. Dasypus Armadillos were sampled throughout their range.

A combination of genetic data and physical characteristics led them to conclude that cricket armadillos are actually four genetically distinct species.

Thus, some subspecies within this species have come to be recognized as species in their own right.

The armadillo found in Mexico and the United States was formerly a subspecies of Mexican wolfnow just Mexican wolf: Mexican long-legged armadillo.

Subspecies Window StratusThe species that inhabits the central part of its range is now a distinct species, and its original name was Novemucinctas Currently limited to South America.

Meanwhile, the data showed that another branch of the armadillo phylogenetic tree did not belong to any of these three existing groups.

The area of ​​northeastern South America known as the Guiana Shield is home to the newest armadillo species. Dasypus guianensis.

The new armadillo is slightly larger than the other three species, has a hairless shell, a robust domed skull and additional bones in its spine.

Overall, however, to the untrained eye, these four species appear very similar.

“It's nearly impossible to tell in the field,” Dr Delsac said.

a paper The findings were published in the journal. Systematic biology.

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Mathilde Barthes othersExon capture museomics deciphers a cricket armadillo species complex and identifies a new species endemic to the Guiana Shield. Systematic biologyPublished online June 22, 2024, doi: 10.1093/sysbio/syae027

Source: www.sci.news

The Power of Music to Discover the Universe’s Hidden Secrets

Music and physics are two disciplines that transcend mere study to become intertwined aspects of human creativity. This hidden harmony between music and physics has been acknowledged by luminaries such as Albert Einstein, who expressed a longing for music had he not pursued physics.

As someone who navigates both fields, I have uncovered deeper connections between them. My journey began in the Bronx, where the worlds of hip hop and science collided in unexpected ways. Later, while studying at Imperial College London, I witnessed the fusion of artistic expression and scientific inquiry in Brian Eno’s studio.

This intersection between art and science inspired me to explore further and led me to write the book “Physics Jazz.” Through this exploration, I delved into the commonalities between music and physics, from improvisation to quantum uncertainty.

My passion for sharing these discoveries prompted the creation of the course “Jazz in Modern Physics” at Brown University, bridging the gap between disciplines and offering students a new way to appreciate the symphony of the universe through mathematics and melody.

Believing in the transformative power of education, I founded the “Sound + Science” after-school program to provide underserved students with an opportunity to explore the fusion of music and physics through hands-on experimentation and collaboration.

This fusion of art and science celebrates human ingenuity and the interconnectedness of the universe. In embracing this harmonious blend, we can unlock the mysteries of the universe and delve into the depths of the human soul.

Source: www.sciencefocus.com

Scientists Discover Unique Characteristics of Rare Element Promethium

Promethium is extremely rare, with only about 0.5 kg occurring naturally in the Earth’s crust at any one time.

Conceptual art depicts the rare earth element promethium in a vial surrounded by organic ligands. Image courtesy of Jacqueline DeMink / Thomas Dyke / ORNL.

[DiscoveredattheClintonLaboratoryin1945promethium is a lanthanide element with the symbol Pm and atomic number 61.

Named after the mythical Titan who brought fire to mankind, the name symbolizes human endeavor.

Despite their use in medical research and long-life nuclear batteries, some of their properties remain poorly understood.

“The aim of this project was to explore and gain new knowledge about this extremely rare element,” he said. Oak Ridge National Laboratory.

Dr. Ivanov and his colleagues prepared a chemical complex of promethium, allowing them to characterize it in solution for the first time.

Thus, they uncovered the secrets of this element through a series of meticulous experiments.

“Promethium was the last lanthanide discovered and has been the most difficult to study because it has no stable isotopes,” said Dr. Ilya Popovs, also of Oak Ridge National Laboratory.

“There are thousands of papers on lanthanide chemistry without promethium. It was a glaring flaw in the science as a whole,” said Dr. Santa Giansone-Popova of Oak Ridge National Laboratory.

“Scientists could only guess at most of its properties. Now we can actually measure some of them.”

The researchers linked, or chelated, radioactive promethium with a special organic molecule called a diglycolamide ligand.

The researchers then used X-ray spectroscopy to determine the properties of the complex, including the lengths of the chemical bonds between promethium and neighboring atoms — a scientific first and a long-missing part of the periodic table of elements.

Unlike other rare earth elements, synthetic promethium has no stable isotopes and is therefore only available in very small quantities.

For their research, the scientists produced the isotope promethium-147, which has a half-life of 2.62 years, in sufficient quantity and purity to study its chemical properties.

Remarkably, they were the first to demonstrate the signature of lanthanide contraction in solution for the entire lanthanide series, including promethium, atomic number 61.

Lanthanide contraction is a phenomenon in which elements with atomic numbers 57 through 71 become smaller than expected.

As the atomic number of these lanthanides increases, the radius of their ions decreases.

This contraction results in unique chemical and electronic properties as the same electric charge is confined to a shrinking space.

The authors obtained a clear promethium signal, which allowed them to better define the shape of the trend across the series.

“It’s really amazing from a scientific point of view. When I got all the data I was blown away,” Dr Ivanov said.

“This contraction of chemical bonds accelerates along the atomic series, but slows down significantly from promethium onwards.”

“This is a major breakthrough in understanding the chemical bonding properties of these elements and their structural changes along the periodic table.”

“Among other things, this achievement will ease the difficult task of isolating these valuable elements,” said Dr. Jansonne Popova.

“Our team has been working for a long time to isolate the entire series of lanthanides, but promethium was the last puzzle piece. It’s been very challenging.”

“With today’s advanced technology, we can’t use all these lanthanides as a mixture, because we have to separate them first.”

“This is where shrinkage becomes really important. It basically allows you to separate them, which is still pretty difficult.”

“All of the technological marvels of our time contain these rare earth elements in some form,” Dr Popovs said.

“We’re adding the missing link.”

Team paper Published in today’s journal Nature.

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D.M. Driscoll othersObservation of promethium complexes in solution. NaturePublished online May 22, 2024, doi: 10.1038/s41586-024-07267-6

Source: www.sci.news

Scientists discover a previously unknown species of fake scorpion trapped in 50-million-year-old amber

Paleontologists have reported fossils of a new genus and species of pseudoscorpion from the Eocene Cambay amber of western India.



Geogaranya variensis. Image credit: Agnihotri other, doi: 10.26879/1276.

pseudo scorpion It is the earliest order of arthropods to colonize Earth’s land during the early Devonian period.

This diverse order accounts for more than 3% of all known arachnid species.

“Pseudoscorpions are an ancient lineage of terrestrial arachnids that are morphologically similar to real scorpions, but lack the tail and stinger,” said Dr. Priya Agnihotri of DST’s Birbal Sahni Institute of Paleosciences and colleagues.

“Certain families have unique venom devices in the serrated digits of their palps, which evolved independently of the venom devices of scorpions and spiders.”

“Recent research also supports the inclusion of pseudoscorpions as a sister group to scorpions.”

“Due to their delicate bodies and small size, these fossils are mainly found in amber deposits around the world rather than in sediments,” they added.

“Forty-nine pseudoscorpion species have been recorded from Eocene Baltic amber and Rovno amber.”

Newly discovered pseudoscorpion species belongs to the small scorpion family Goridae.

named Geogaranya variensis showing strong similarities with extant genera. Geogalypus From Sri Lanka, India, and New Guinea.

“The Geogarypidae family is one of a group of bark-dwelling and leaf litter-dwelling species similar to the Geogarypidae family. Gallipidae It has a distinctive subtriangular carapace and eyes located near the leading edge,” the paleontologist said.

“This family includes more than 70 species with habitats suitable for tropical and subtropical regions, some of which have been reported from temperate biomes.”

“Geogarypidae are more common in Baltic and Rovno amber, and there are some records from Cretaceous Burmese amber.”

“Unlike the sparse record of fossils, their modern-day counterparts have been recorded in all major biogeographic regions, including Europe, Central Asia, North America, and North Africa.”

Amber from Cambay from 50 million years ago. Geogaranya variensis It was discovered in the open-pit Valia lignite mine, part of the Cambay Shale Formation, in the Cambay Basin of Gujarat, India.

“The Cambay Shale Formation overlies the Deccan Trap, and below it is the Paleocene to lower Eocene Vagadkol Formation,” the researchers said.

According to the team: Geogaranya variensis It is one of the smallest known adult pseudoscorpion fossils in amber from the Cambay Basin.

This discovery further strengthens the biodiversity of bark-dwelling arthropods identified in Eocene amber from western India.

“The discovery of the smallest known adult pseudoscorpion in Cambay Basin amber aligns it with fossil taxa recorded in Baltic Sea amber and Bitterfeld amber that survived the early Eocene. “This provides insight into similar bark-dwelling arthropod taxa,” the scientists concluded.

“Scanning electron microscopy studies revealed diagnostic features in the fossils, such as abnormally enlarged palps. This strengthened Foresy’s idea that species from non-arboreal habitats could be mistakenly This suggests that it may have been carried in amber and had a connection to a flying host.”

discovery of Geogaranya variensis is reported in paper in diary Old Trogia Electronica.

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priya agnihotri other. 2024. A new genus and species of fossil pseudoscorpion (Arachnida: Pseudoscorpiones) discovered in Eocene amber from western India. Old Trogia Electronica 27 (2):a26; doi: 10.26879/1276

Source: www.sci.news

Researchers Discover Oldest Evidence of Earth’s Magnetic Field in Greenland

Recovering ancient records of the Earth's magnetic field is difficult because the magnetization of rocks is often reset by heating during burial due to tectonic movements over a long and complex geological history. Geoscientists from MIT and elsewhere have shown that rocks in West Greenland's Isua supercrustal zone have experienced three thermal events throughout their geological history. The first event was the most important, heating rocks to 550 degrees Celsius about 3.7 billion years ago. His two subsequent phenomena did not heat the region's northernmost rocks above 380 degrees Celsius. The authors use multiple lines of evidence to test this claim, including paleomagnetic field tests, metamorphic mineral assemblages across the region, and temperatures at which the radiometric ages of observed mineral assemblages are reset. They use this body of evidence to argue that an ancient record of Earth's magnetic field from 3.7 billion years ago may be preserved in the striated iron layer at the northernmost edge of the magnetic field. .

Earth's magnetic field lines. Image credit: NASA's Goddard Space Flight Center.

In a new study, Professor Claire Nicholls from the University of Oxford and colleagues examined a range of ancient iron-bearing rocks from Isua, Greenland.

Once locked in place during the crystallization process, iron particles effectively act as tiny magnets that can record both the strength and direction of a magnetic field.

Researchers found that 3.7 billion-year-old rocks exhibited magnetic field strengths of at least 15 microteslas, comparable to modern magnetic fields (30 microteslas).

These results provide the oldest estimates of the strength of Earth's magnetic field derived from whole rock samples, providing a more accurate and reliable estimate than previous studies using individual crystals.

“It's very difficult to extract reliable records from rocks this old, so it was really exciting to see the primary magnetic signals start to emerge when we analyzed these samples in the lab,” Professor Nichols said. said.

“This is a very important step forward in our efforts to understand the role of ancient magnetic fields in the creation of life on Earth.”

Although the strength of the magnetic field appears to remain relatively constant, the solar wind is known to have been significantly stronger in the past.

This suggests that surface protection from the solar wind may have strengthened over time, thereby allowing life to leave the protection of the oceans and migrate to the continents.

The Earth's magnetic field is created by the mixing of molten iron within a fluid outer core, driven by buoyancy as the inner core solidifies, forming a dynamo.

During the early stages of Earth's formation, a solid inner core had not yet formed, leaving unanswered questions about how the initial magnetic field was maintained.

These new results suggest that the mechanisms driving Earth's early dynamo were as efficient as the solidification processes that generate Earth's magnetic field today.

Understanding how the strength of Earth's magnetic field has changed over time is also key to determining when Earth's interior solid core began to form.

This helps us understand how fast heat is escaping from the Earth's deep interior, which is key to understanding processes such as plate tectonics.

A key challenge in reconstructing Earth's magnetic field back in time is that any event that heats rocks can change the preserved signal.

Rocks in the Earth's crust often have long and complex geological histories that erase information about previous magnetic fields.

However, the Isua supercrustal zone has a unique geology, sitting on a thick continental crust and protected from extensive tectonic movements and deformation.

This allowed scientists to build clear evidence for the existence of magnetic fields 3.7 billion years ago.

The results may also provide new insights into the role of magnetic fields in shaping the development of Earth's atmosphere as we know it, particularly regarding the release of gases into the atmosphere.

“In the future, we hope to expand our knowledge of Earth's magnetic field before oxygen increased in the Earth's atmosphere about 2.5 billion years ago by examining other ancient rock sequences in Canada, Australia, and South Africa. “We believe that this is the case,” the authors said.

“A better understanding of the strength and variability of ancient Earth's magnetic field will help determine whether the planet's magnetic field was important for harboring life on the planet's surface and its role in the evolution of the atmosphere. Masu.”

of study Published in Geophysical Research Journal.

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Claire IO Nichols other. 2024. Possible Archean record of geomagnetism preserved in the Isua supercrustal zone of southwestern Greenland. Geophysical Research Journal 129 (4): e2023JB027706; doi: 10.1029/2023JB027706

Source: www.sci.news

Astronomers discover large ejection of dipolar material from NGC 4383

A large number of stars are born in the center NGC4383where a unique galaxy is located 74 million light years It is located beyond the constellation Coma. The largest lose mass through powerful winds over their lifetime, eventually exploding into violent supernovae. These stellar winds and supernovae drag away some of NGC 4383's gas reservoir. The bright red filaments indicate hydrogen gas ejected at least 20,000 light-years from the galaxy. This process controls the rate at which stars form within the galaxy, as this gas is carried away from the galactic center rather than remaining to form the next generation of stars.

watt other. We mapped the chemical composition and motion of NGC 4383's outflow in detail, providing insight into the mechanisms that caused the dramatic outflow seen in this image from ESO's Very Large Telescope.Image credit: ESO / Watts other.

Gas outflow is important for controlling the rate and duration at which galaxies continue to form stars.

The gas ejected by these explosions can pollute the space between stars within galaxies and even between galaxies, becoming permanently suspended in the intergalactic medium.

Dr Adam Watts, an astronomer at the University of Western Australia's node at the International Radio Center, said: “This outflow is the result of a powerful stellar explosion at the center of the galaxy, potentially spewing out huge amounts of hydrogen and heavy elements. There is a gender,” he said. Astronomical Research (ICAR).

“The mass of gas released is equivalent to more than 50 million suns.”

“Spills are very difficult to detect, so very little is known about the physics of spills and their properties.”

“The ejected gas is extremely rich in heavy elements, providing a unique insight into the complex process by which metals mix with hydrogen in the ejected gas.”

“In this particular case, oxygen, nitrogen, sulfur and many other chemical elements were detected.”

astronomers are muse (Multi-unit Spectroscopic Explorer) Turn on the instrument ESO's super large telescope (VLT) Created a high-resolution map of NGC 4383 in northern Chile.

Data were collected as part of VLT/MUSE's larger program MAUVE (MUSE and ALMA Unveiling the Virgo Environment).

“We designed MAUVE to investigate how physical processes, such as gas outflow, help stop star formation in galaxies,” said West, also at the International Center for Radio Astronomy Research (ICRAR). said Professor Barbara Catinella of the Australian University of Nord.

“NGC 4383 was our first target because we thought something very interesting might be happening, and the data exceeded all expectations.”

“In the future, we hope that MAUVE's observations will reveal in great detail the importance of gas outflow in the local universe.”

team's paper Published in Royal Astronomical Society Monthly Notices.

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Adam B. Watts other. 2024. Mauve: A 6 kpc bipolar outflow launched from NGC 4383, one of the most Hi-rich galaxies in the Virgo cluster. MNRAS 530 (2): 1968-1983; doi: 10.1093/mnras/stae898

Source: www.sci.news

Paleontologists Discover New Species of Massive Triassic Ichthyosaur

Ichthyotitan severnensis It lived in the Triassic seas around 202 million years ago and may have grown over 25 meters (82 feet) long.



Ichthyotitan severnensis. Image credit: Gabriel Uguet.

Ichthyosaurs are dolphin-like marine reptiles known from hundreds of fossils from the time of the dinosaurs.

These creatures ranged in size from less than a meter to over 20 meters (65 feet) in length.

All animals gave birth to live young in the sea, and some had giant eyes and so-called warm-blooded physiology, and some were fast swimmers and deep divers.

“Ichthyosaurs first evolved during the early Triassic period, about 250 million years ago,” said Dr Dean Lomax and colleagues from the Universities of Bristol and Manchester.

“Within a few million years, some ichthyosaurs evolved to reach lengths of 15 meters or more, and by the late Triassic period (about 200 million years ago), the largest fish, including the newly described ichthyosaurs. The dragon has evolved. Ichthyotitan severnensis

“But this reign didn’t necessarily last long. Some species of ichthyosaurs continued to roam the oceans for millions of years, but these ‘giant ichthyosaurs’ It is thought to have become extinct during the Tatami-Jurassic extinction event. And this unique group of marine reptiles never reached such a world again. Huge size.”

two fragmentary jaw bones Ichthyotitan severnensis Collected from the uppermost layer of the Triassic period Westbury Mudstone Formation Located in Somerset, England.

Based on the length of the fossil, the new species could have been a whopping 25 meters long, or twice as long as a city bus.

“In 2018, my team studied and described a giant jawbone, and we were hopeful that one day another jawbone would be revealed,” Dr. Lomax said.

“The new specimen is more complete and better preserved, showing that there are two large bones (called quadrilateral bones) with unique shapes and structures.”

“It’s quite amazing to think that gigantic ichthyosaurs, the size of blue whales, were swimming in the seas around Britain during the Triassic period.”

“These jaw bones provide intriguing evidence that perhaps someday the complete skull or skeleton of these giants may be discovered. You never know.”

discovery of Ichthyotitan severnensis is explained in paper in diary PLoS ONE.

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DR Lomax other. 2024. The last giant: new evidence of a giant Late Triassic (Rhaetian) ichthyosaur from Britain. PLoS ONE 19 (4): e0300289; doi: 10.1371/journal.pone.0300289

Source: www.sci.news

Students Implicated in Cyber Fraud After Police Discover Involvement in Massive Phishing Site

Police have uncovered a disturbing trend among university students, who are resorting to cyber fraud to boost their income. They have managed to infiltrate a large phishing site on the dark web that has defrauded tens of thousands of individuals.

The site, known as LabHost, has been operational since 2021 and serves as a hub for cyber fraud, enabling users to create realistic-looking websites mimicking reputable companies like major banks. It has ensnared 70,000 users globally, including 70,000 individuals in the UK.

Victims unknowingly provided sensitive information, which was then used to siphon money from their accounts. The perpetrators behind the site profited by selling this stolen data on the dark web to other fraudsters.

According to the Metropolitan Police, the primary victims fall within the 25-44 age bracket, with a significant portion of their activities carried out online.

Law enforcement authorities have apprehended one of the alleged masterminds behind the site, along with 36 other suspects detained in the UK and abroad. The arrests were made at various airports in Manchester, Luton, Essex, and London.

British police are facing mounting pressure to demonstrate their effectiveness in combating the rising tide of cyber fraud.

Despite the relatively small impact of dismantling this particular site, the police intend to dismantle additional cyber fraud operations to undermine the confidence of criminals who believe they can act with impunity.

While fraud and cybercrime present considerable challenges for law enforcement agencies, they often compete for resources with other policing priorities, such as safeguarding children and enhancing women’s safety.

LabHost managed to amass significant amounts of sensitive data, including 480,000 debit or credit card numbers and 64,000 PIN numbers, generating over £1 million in membership fees from 2,000 individuals who paid in cryptocurrency.

The company lured users with tutorial videos on committing crimes using the site and on utilizing new consumer products. It promised quick installation of software in five minutes and offered “customer service” in case of any issues.

DI Oliver Richter noted the shift in cyber fraud from requiring technical skills like coding to now being accessible to individuals ranging from late teens to late 20s, many of whom are college students.

He expressed concern that these users may not fully grasp the risks and consequences of their actions, assuming anonymity and ease of operation.

Following the dismantling of the site, 800 users received warnings that the police were aware of their activities.

Detective Inspector Helen Rance, head of the Metropolitan Police’s cybercrime unit, described the LabHost bust as a sophisticated operation targeting those who have commercialized fraudulent activities. She highlighted collaboration with 17 factions globally, both in the public and private sectors.

She emphasized the success of penetrating the service, identifying the perpetrators, and understanding the scale of their illicit operations.

Source: www.theguardian.com

Astronomers discover colorful ‘glory’ in the atmosphere of WASP-76b

Using data from ESA's Extraterrestrial Planet Characterization Satellite (CHEOPS) and several other ESA and NASA missions, astronomers detected signs of extraterrestrial planets. Rainbow-like “glory effect” In the atmosphere of super-hot Jupiter WASP-76b. This effect occurs when light is reflected from a cloud composed of a completely homogeneous but so far unknown material. This “glory effect” is common on Earth, but it has only been discovered once on another planet, Venus. If confirmed, this first extrasolar glory would reveal more about the nature of this puzzling exoplanet and hold exciting lessons about how to better understand strange, distant worlds.

Artist's impression of WASP-76b's atmospheric rainbow-like “glory effect.” Image credit: ESA.

WASP-76b is the superhot planet Jupiter located 640 light-years away in the constellation Pisces.

First discovered in 2016, this exoplanet orbits the F-type star WASP-76 once every 1.8 days.

WASP-76b is tidally locked to its star. It takes about the same amount of time to rotate around its axis as it does to orbit its parent star.

On the day side, the planet receives thousands of times more radiation from its star than Earth receives from the Sun.

Temperatures on the dayside can exceed 2,400 degrees Celsius (4,352 degrees Fahrenheit), high enough to vaporize metals. However, nighttime temperatures are much cooler at 1,316 degrees Celsius (2,400 degrees Fahrenheit).

Here, the elements that form Earth's rocks melt and evaporate, condensing on the slightly cooler night side and creating iron clouds that drip rain of molten iron.

But astronomers have been puzzled by the apparent asymmetry, or oddity, of WASP-76b's “limbs,” the outermost regions seen as it passes in front of its host star.

“WASP-76b is being 'inflated' by the intense radiation from its star,” said Dr. Monica Rendl, an astronomer at the University of Geneva.

“That means it's 10% less massive than our cousin Jupiter, but almost twice the size.”

“The important thing to keep in mind is the incredible scale of what we are witnessing,” says ESA astronomer Dr Matthew Standing.

“WASP-76b is a very hot gas giant planet hundreds of light years away, likely raining molten iron. Despite the chaos, we detected potential signs of glory. It seems like it's an incredibly weak signal.''

In this study, the authors analyzed data from a variety of ESA and NASA missions, including CHEOPS, TESS, Hubble, and Spitzer.

CHEOPS intensively monitored WASP-76b as it passed in front of and around a Sun-like star. After making her 23 observations over three years, the data showed a surprising increase in the amount of light emanating from the planet's eastern “terminator,” the boundary where night and day meet. .

This allowed astronomers to disentangle the signal and constrain its origin.

“This is the first time that such a sudden change in the brightness of an exoplanet, its 'phase curve', has been detected,” said Dr. Olivier Demanjon, an astronomer at the Spanish Institute of Astronomical Sciences in Portugal.

“This discovery led to the hypothesis that this unexpected glow may be caused by a strong, locally anisotropic (direction-dependent) reflection, or glow effect.”

“Never before have we seen such colorful concentric rings on an extrasolar object,” said Dr Thomas Wilson, an astronomer at the University of Warwick.

“Therefore, if future studies confirm the glory of this first exoplanet, WASP-76b will be a truly unique object, providing insight into the atmospheres of distant exoplanets and how habitable they may be. It’s a beautiful tool for understanding.”

Confirmation of the glory effect means that the cloud, which is made up of perfectly spherical droplets, has lasted at least three years or is constantly replenished.

For these clouds to persist, the atmospheric temperature must also remain stable over time. This is an interesting and detailed insight into what's going on with WASP-76b.

Importantly, being able to detect such subtle wonders at great distances will teach scientists and engineers how to detect other less visible but important phenomena. For example, sunlight reflecting off liquid lakes and oceans is a requirement for habitability.

“More evidence is needed to say conclusively that this interesting 'extra light' is a rare glory,” said Dr Teresa Luftinger, project scientist for ESA's upcoming Ariel mission.

“Follow-up observations by the NIRSPEC instrument aboard the NASA/ESA/CSA James Webb Space Telescope could do just that. Or perhaps ESA’s upcoming Ariel mission will prove its existence.” We may even discover brighter colors shining from other exoplanets.”

a paper The survey results were published in a magazine astronomy and astrophysics.

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ODS demansion other. 2024. Asymmetry in the atmosphere of superhot Jupiter WASP-76b. A&A 684, A27; doi: 10.1051/0004-6361/202348270

Source: www.sci.news

Discover the message NASA is sending to Europa, Jupiter’s icy moon.

Illustration of NASA’s Europa Clipper spacecraft

NASA/JPL-California Institute of Technology

In October, NASA’s Europa Clipper spacecraft will begin a journey to explore Jupiter’s icy moon Europa (imagined above).

NASA has asked METI International, the scientific organization I lead, to leverage our expertise in trying to make contact with extraterrestrial intelligence by creating a symbolic engraved tantalum plate on a spacecraft. We asked them to help us create a message, a greeting from one water world to another.

We helped create two parts of the message. First, we collected a globally representative sample of recordings of water words in 103 languages. Each language is displayed as a waveform on the outside of the panel (pictured above) that protects sensitive scientific equipment.

On the other, inward-looking side (see below), we designed the scientific part of the message. This refers to water in terms of the “water hole,” a frequency band between the hydrogen and hydroxyl (combining to form water) emission lines in the radio spectrum where many of the early searches for intelligence beyond Earth took place. I’m explaining.

Other parts of the internal message include: Drake equation to estimate the number of extraterrestrial civilizations in the galaxy. Microchips containing the names of 2.6 million supporters will be added soon.and Poet Laureate of the United States Ada Limon’s Poem to Europa ends like this. “O second moon, we too / are made of water, of a vast, beckoning ocean… / of the need to call out in the darkness.” The European Clipper will fly to Jupiter in April 2030. We are planning to enter the orbit of

douglas vacochChairman of Ministry of Economy, Trade and Industry International

topic:

  • Jupiter/
  • space exploration

Source: www.newscientist.com

Physicists discover first natural unconventional superconductor

Solid state chemistry has led to the creation of numerous materials with unique properties not found in nature. For instance, the high-temperature superconductivity of copper oxide compounds known as cuprates is so distinct from the superconductivity of naturally occurring metals and alloys that it is often referred to as “unconventional.” Unconventional superconductivity is also present in other synthetic compounds like iron-based superconductors and heavy fermion superconductors. Physicists at Ames National Laboratory have uncovered strong evidence of unconventional superconductivity in synthetic samples of Rh17S15, a mineral that exists in nature as miassite.



Miasite is one of only four minerals found in nature that act as a superconductor when grown in the laboratory, and is the only mineral ever known to exhibit unconventional superconductivity in its clean synthetic form. It is the only mineral that exists. Image credit: Paul Canfield.

Superconductivity is the ability of a material to conduct electricity without any loss of energy.

Superconductors have various applications including medical MRI machines, power cables, and quantum computers.

Conventional superconductors are well understood but have low critical temperatures.

The critical temperature is the highest temperature at which a material displays superconductivity.

In the 1980s, scientists discovered unconventional superconductors with significantly higher critical temperatures, all of which were manufactured in a lab, challenging the notion that unconventional superconductivity is not a natural occurrence, as stated by Ruslan Prozorov, a researcher at Ames National Laboratory.

“Miasite is a fascinating mineral due to its intricate chemical composition,” he added.

Continued efforts to grow miasite crystals as part of a broader exploration into compounds combining elements with high melting points and volatile elements have led to the discovery of unconventional superconductors in the Rh-S system.

Professor Paul Canfield highlighted the unique process of growing crystals at low temperatures with minimal vapor pressure in elements like Rh, contrary to pure elements found in nature.

Further tests confirmed that miasite functions as an unconventional superconductor, enhancing the understanding of superconductors.

For more information on this discovery, refer to the article published in Communication Materials.

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H. Kim et al. 2024. Nodal superconductivity in miasite Rh17S15. Communication Materials 5, 17; doi: 10.1038/s43246-024-00456-w

Source: www.sci.news

Brain researchers discover cold sensors in mice

Neuroscientists at the University of Michigan have identified thermoreceptors that mediate the sensation of cold in somatosensory neurons.

GluK2 KO mice have a defect in cold sensing.Image credit: Kai other10.1038/s41593-024-01585-8.

“The field began elucidating such temperature sensors more than 20 years ago with the discovery of a heat-sensing protein called TRPV1,” said Professor Sean Hsu of the University of Michigan.

“While various studies have discovered proteins that sense hot, warm, and even cold temperatures, we have not identified any proteins that sense temperatures below about 15 degrees Celsius (60 degrees Fahrenheit).”

In 2019, scientists discovered The world's first cold receptor protein Caenorhabditis elegans a millimeter-long nematode species that the lab is studying as a model system for understanding sensory responses.

Because the gene that codes for it is Caenorhabditis elegans This protein is evolutionarily conserved across many species, including mice and humans, and this discovery was a starting point for testing cold sensors in mammals. Glutamate ion channel receptor kainate type subunit 2 (GluK2).

In a new study, Professor Xu and colleagues tested that hypothesis in mice with the deficiency. GluK2 Because of the gene, the GluK2 protein could not be produced.

Through a series of experiments testing animals' behavioral responses to temperature and other mechanical stimuli, they found that mice responded normally to hot, warm, and cold temperatures, but not to harmful cold.

GluK2 is primarily found in neurons in the brain, where it receives chemical signals and facilitates communication between neurons.

However, it is also expressed by sensory neurons in the peripheral nervous system (outside the brain and spinal cord).

“We found that this protein serves a completely different function in the peripheral nervous system, processing temperature cues instead of cold-sensing chemical signals,” said Dr. Bo Duan from the University of Michigan.

of GluK2 This gene has relatives across the evolutionary tree, going back to single-celled bacteria.

“Bacteria don't have brains, so why have they evolved a way to receive chemical signals from other neurons?” Professor Xu said.

“But the need to sense its environment, and perhaps both temperature and chemicals, will be very strong.”

“Thus, I suspect that temperature sensing is an ancient function, at least for some of these glutamate receptors, that was eventually adopted as organisms evolved more complex nervous systems. .”

of result appear in the diary natural neuroscience.

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W. Kai other. The kainate receptor GluK2 mediates cold sensing in mice. nut neurosi, published online on March 11, 2024. doi: 10.1038/s41593-024-01585-8

Source: www.sci.news

Physicists at CERN Discover Intriguing New Decay Mode of Mesons

Physicists from LHCb collaboration at CERN’s Large Hadron Collider (LHC) have made the first observation of the collapse of the Bc+ meson. This results in a J/ψ charm-anticharm quark bound state (consisting of two heavy quarks, b and c) and a pair of pions π+π0. This new decay process shows a contribution from an intermediate particle, the ρ+ meson, which forms for a short time and then decays into π+π0 pairs.



September 2016, LHCb experimental cave at LHC IP8. Image courtesy of CERN.

The Bc+ is the heaviest meson and decays only through weak interactions due to the decay of one heavy constituent quark.

It decays into an odd number of optical hadrons, and J/ψ (or another attractive and anti-attractive quark-bound state called Charmonia) has been intensively studied and found to be in remarkable agreement with theoretical predictions.

The decay of Bc+ to J/ψ and π+π0 pairs is the simplest decay to charmonium and even-numbered optical hadrons.

This has never been observed before. The main reason for this is that in the LHC proton-proton collision environment, it is very difficult to accurately reconstruct low-energy π0 mesons through their decay into a pair of photons.

“Accurate measurements of the Bc+→J/ψπ+π0 decay will allow us to better understand its possible contribution as a background source for the study of other decays of Bc mesons and rare decays of B0 mesons,” said the LHCb physicist.

From a theoretical point of view, J/ψ and the decay of Bc into an even number of pions are closely related to the decay of the τ lepton into an even number of pions and the e+e- annihilation into an even number of pions.

Accurate measurements of e+e- annihilation into two pions in the ρ mass region (like the Bc decay discussed here) are possible using the Fermilab G-2 experiment, which measures the anomalous magnetic dipole moment of the muon and is important for interpreting the results. The annihilation of low-energy e+e- into hadrons is an important source of uncertainty in g-2 measurements.

The ratio of the probability of a new decay to the probability of a decay from Bc+ to J/ψπ+ has been calculated by various theorists over the past 30 years.

Now these predictions can finally be compared with experimental measurements. Most predictions agree with the new result 2.80±0.15±0.11±0.16.

The large number of b quarks produced in LHC collisions and the excellent detectors allow LHCb researchers to study the formation, decay, and other properties of Bc+ mesons in detail.

“Since the discovery of the meson by the Tevatron Collider’s CDF experiment, 18 new Bc+ decays (with more than 5 standard deviations) have been observed, all from the LHCb,” the researchers said.

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LHCb collaboration. 2024. Observation of B+c→J/ψπ+π0 collapse. arXiv: 2402.05523

Source: www.sci.news

Peruvian researchers discover new species of miniature deer

Pudera Carlae is the first deer species to be discovered in the 21st century and the first from the New World in over 60 years. Learn more about it here.

Pudera Carlae. Image credit: Sernanp.

The newly described deer species, Pudera Carlae, belongs to the Neotropical deer family, Odokoileini.

“Some questions regarding the phylogeny and taxonomy of Odocoileini, a group of 18 recognized extant species currently assigned to seven genera, remain unclear,” said Dr. Guillermo Delaire of the University of South Australia and his colleague.

“The few available phylogenetic analyzes indicate that some genera are not monophyletic and that species richness within groups is underestimated.”

“One genus that has both problems is the stocky, short-legged dwarf deer, Pudu

“It has two species, the Northern Pudu (Pudu Mephisto File) from Peru, Ecuador, and Colombia, and the Southern Pudu (Pudupuda) from southern Chile and neighboring Argentina.”

In a new study, the authors found that the Pudu Mephisto File species are actually two different species.

“One is distributed north of the Huancabamba depression from the northernmost part of Peru to the north (Ecuador and Colombia), while the other is endemic in Peru south of the Huancabamba depression and does not have a name yet, so we propose naming it Pudera Carlae

“This is the first extant deer species described in the 21st century and the first discovered in the New World in over 60 years.”

The researchers also found that the Pudupuda type species of Pudu are not related to the two northern Pudu species.

“We revalidate the genus Pudera and assign the latter two species to it.”

The team’s paper was published in the mammal journal this month.

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Javier Barrio et al. Extant deer species first described in the 21st century and their reexamination Pudera (Artiodactyla). mammal journal, published online March 1, 2024. Doi: 10.1093/jmammal/gyae012

Source: www.sci.news

Astronomers discover floating crystals preventing cooling in high-mass white dwarf stars

Astronomers have proposed a new theory to explain why a mysterious population of white dwarfs has stopped cooling for at least 8 billion years.

This diagram shows a white dwarf and the moon. Image credit: Giuseppe Parisi.

White dwarfs are the remains of stars without a nuclear energy source that gradually cool over billions of years, eventually freezing from the inside out to a solid state.

Recently, it was discovered that a population of frozen white dwarfs maintains a constant brightness for a period comparable to the age of the universe, indicating the existence of an unknown, powerful energy source that inhibits cooling.

“We find that the classical picture that all white dwarfs are dead stars is incomplete,” said astronomer Dr Simon Bruin from the University of Victoria.

“To stop these white dwarfs from cooling, we need some way to generate additional energy.”

“We didn’t know how this happened, but now we have an explanation for this phenomenon.”

The researchers say that in some white dwarfs, the dense plasma inside them doesn’t just freeze from the inside out.

Instead, the solid crystals that form when frozen tend to float because they are less dense than the liquid.

As the crystals float upwards, the heavier liquid moves downwards.

As heavy material is transported toward the star’s center, gravitational energy is released, and this energy is enough to interrupt the star’s cooling process for billions of years.

Dr Antoine Bedard, an astronomer at the University of Warwick, said: “This is the first time this transport mechanism has been observed in any type of star, and it’s very interesting because it’s not every day that a completely new astrophysical phenomenon is discovered.”

“We don’t know why this happens in some stars and not others, but it’s probably due to the star’s composition.”

“Some white dwarfs are formed by the merger of two different stars,” Dr Bruin said.

“When these stars collide to form white dwarfs, the star’s composition changes, allowing the formation of floating crystals.”

White dwarfs are routinely used as an indicator of age, and the cooler a white dwarf is, the older it is considered to be.

However, the extra delay in cooling seen in some white dwarfs means that some stars at certain temperatures may be billions of years older than previously thought.

“This new discovery will not only require a revision of astronomy textbooks, but will also require a reexamination of the processes astronomers use to determine the age of stellar populations,” Dr. Blouin said.

of the team paper Published in today’s diary Nature.

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A. Bedard other. Buoyant crystals stop the white dwarf from cooling. Nature, published online March 6, 2024. doi: 10.1038/s41586-024-07102-y

Source: www.sci.news

Astronomers discover the heaviest supermassive black hole pair ever measured

Astronomers are gemini north telescope measured a binary supermassive black hole located within the elliptical galaxy B2 0402+379.

Artist's impression of the supermassive black hole binary in elliptical galaxy B2 0402+379. Image credit: NOIRLab / NSF / AURA / J. daSilva / M. Zamani.

The pair of compact objects at the center of B2 0402+379 are the only supermassive black hole binaries ever resolved in enough detail that both objects can be seen separately.

It holds the record for the smallest distance ever directly measured – just 24 light years.

While this close separation portends a strong merger, further research reveals that the pair has been stuck at this distance for more than 3 billion years, raising questions. What is the holdup?

To better understand the dynamics of this system and its stalled merger, Stanford University professor Roger Romani and his colleagues turned to archival data from Gemini North. Gemini multi-object spectrometer (GMOS) This allowed them to determine the speed of stars near the black hole.

“The excellent sensitivity of GMOS allowed us to map the increasing velocity of stars as they approach the center of the galaxy. This allowed us to estimate the total mass of black holes present there.” Professor Romani said.

The authors estimate that the binary star's mass is a whopping 28 billion times that of the Sun, making the pair the most massive binary black hole ever measured.

This measurement not only provides valuable background on the formation of binary systems and the history of their host galaxies, but also confirms the long-held belief that the mass of supermassive binary black holes plays a key role in preventing potential mergers. This supports the theory.

“The data archive provided by the International Gemini Observatory holds a goldmine of untapped scientific discoveries,” said Dr. Martin Still, NSF program director for the International Gemini Observatory.

“Measuring the mass of this extreme supermassive binary black hole is an awe-inspiring example of the potential impact of new research exploring its rich archive.”

Understanding how this binary formed can help predict if and when it will merge. Also, some clues indicate that the pair formed through multiple galaxy mergers.

First, B2 0402+379 is a “fossil cluster,” meaning it is the result of an entire galaxy cluster's worth of stars and gas merging into a single giant galaxy.

Additionally, the presence of two supermassive black holes, coupled with their large combined mass, suggests that they resulted from the merger of multiple smaller black holes from multiple galaxies.

After galaxies merge, supermassive black holes do not collide head-on. Instead, they start slingshotting each other as they settle into a certain trajectory.

Each time a black hole passes, energy is transferred from it to the surrounding stars.

Losing their energy, the pair are dragged together, and gravitational radiation takes over, merging them just a few light years away.

This process has been observed directly in pairs of stellar-mass black holes, first documented by the detection of gravitational waves in 2015, but has never been observed in binaries of supermassive black holes.

With new knowledge about the system's extremely large mass, astronomers concluded that it would take a very large number of stars to slow down the binary enough to make its orbits so close together. .

In the process, the black hole seems to have blown away almost all the material around it, depleting the galaxy's center of stars and gas.

The merger of the two companies stalled in the final stages, as there was nothing left to further slow the companies' trajectory.

“Galaxies with lighter black hole pairs usually seem to have enough stars and mass to quickly merge the two,” Professor Romani said.

“The pair is so massive that we needed a lot of stars and gas to get the job done. But binaries scour the galaxy for such material, causing it to stagnate, making it impossible for our research to do so.” has been made accessible.”

It remains to be determined whether the pair will overcome stasis and eventually merge on a timescale of millions of years, or remain in orbit forever in limbo.

If they merged, the resulting gravitational waves would be 100 million times more powerful than those produced by the merger of stellar-mass black holes.

The pair could potentially conquer that final distance via another galactic merger. In that case, additional material, or potentially a third black hole, could be injected into the galaxy, slowing the pair's orbits enough for a merger.

However, given that B2 0402+379 is a fossil cluster, further galaxy mergers are unlikely.

“We're looking forward to tracking the core of B2 0402+379 to find out how much gas is present,” said Tirth Surti, an undergraduate at Stanford University.

“This should give us more insight into whether supermassive black holes may eventually merge or remain stuck as binaries.”

of result will appear in astrophysical journal.

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Tirth Surti other. 2024. Central kinematics and black hole mass of 4C+37.11. APJ 960, 110; doi: 10.3847/1538-4357/ad14fa

Source: www.sci.news

Revolutionary Method for Ending Pregnancy Nausea Quickly: Discover the Morning Sickness Cure

We have all experienced vomiting at some stage in our lives. Whether it’s due to a nasty bout of food poisoning or the well-known norovirus that infects the population episodically. And we can all agree that it’s scary.

But imagine what it would do to you physically, mentally, and emotionally if you were to expect constant nausea and vomiting at a critical stage in your life.this is the reality for them
4 in 5 women experience nausea and vomiting during pregnancy. Even mild cases can cause unpleasant symptoms such as nausea, loss of appetite, and vomiting.

for 3% of women develop a condition called hyperemesis gravidarum.things get worse and require hospitalization and treatment.

According to the Office for National Statistics, in 2022 this will result in: 20,000 women hospitalized.



But until recently, little was known about the causes of nausea and vomiting during pregnancy. Anecdotal evidence suggests that the more nausea and vomiting you have, the healthier your pregnancy, and even suggests that it is related to the number of babies you have.

However, real-world evidence shows this is not true. In fact, nausea and vomiting can vary widely in severity and pattern during pregnancy.

Often referred to as “morning sickness,” nausea and vomiting during pregnancy can occur at any time of the day or night. Usually it’s worse for the first 12 weeks, then it calms down. However, for many women, it lasts throughout the pregnancy.

Read more about women’s health:

However, after more than 20 years of research in this field, a breakthrough has been made that identifies a causal relationship. This was promoted by Dr. Malena Fezo, a geneticist at the Keck School of Medicine at the University of Southern California.

Fezo was inspired to pursue this career after suffering from severe nausea and vomiting during her second pregnancy in 1999. She was unable to eat or drink without vomiting, and she rapidly lost weight and became so weak that she could no longer stand or walk.

However, doctors were skeptical that she might be exaggerating her symptoms to get attention. Fezo was eventually hospitalized and she miscarried at 15 weeks.

Fezo will conduct genetic research on previously pregnant women in collaboration with 23andMe, a private company that allows individuals to send samples of their DNA to determine health status and insights into their ancestry. did.

She identified a link with a woman who suffered from severe nausea and vomiting during pregnancy (requiring an intravenous fluid). and a variant of the gene encoding a protein named GDF15, a hormone that acts on the brain stem.

This association pinpointed the need for further research to understand the role of GDF15 protein in pregnancy.

GDF15 is secreted by the placenta during the first two trimesters of pregnancy. It also likely plays a role in preventing the mother from biologically rejecting the baby, which is essential to allowing the pregnancy to continue. However, GDF15 has been shown to regulate physiological body weight and appetite through the brain. This substance is produced in excess in cancer patients who suffer from severe appetite and weight loss.

In addition to previous research, research led by Fejzo and the University of Cambridge Professor Stephen O'Rahilly We found that the level of GDF15 was high. Seen in women with severe nausea and vomiting during pregnancy. However, the effects of this hormone appear to depend on the woman's susceptibility and her exposure to GDF15 before pregnancy. Women who received higher levels of exposure before pregnancy had higher levels of the GDF15 hormone but did not have symptoms of nausea or vomiting.

It has been hypothesized that long-term exposure to GDF15 before pregnancy may have a protective effect and reduce a woman’s sensitivity to the hormonal surge caused by fetal development.

This exposure relationship is very unique and provides more understanding and knowledge as well as the potential that women may be desensitized by increasing their exposure to hormones before pregnancy. It also suggests possible treatments. Just like some people treat food allergies with controlled exposure therapy.

Many of the common symptoms affecting women, such as nausea and vomiting during pregnancy, are poorly understood despite their very high incidence. Women’s healthcare is not a niche, and there is much to understand and learn through this type of research.

Read more:

Source: www.sciencefocus.com

Robot explores deep sea to discover new species with dodecahedral design

Robot dodecahedron mounted on a submersible (circled area)

brennan phillips

The robotic dodecahedron can capture fragile deep-sea animals, collect tissue samples, and build three-dimensional scans of the creatures, potentially speeding up the cataloging of deep-sea life. Up to 66% of marine species are still unknown to science.

brennan phillips RAD2 Sampler and colleagues at the University of Rhode Island have developed the RAD2 Sampler, which is designed to be mounted on any submersible to collect fresh tissue samples in situ from living animals. They hope this will reveal more about the creature than existing techniques, which are typically exposed to stress when pulled up from the depths.

RAD2 is a dodecahedron with an internal volume large enough to hold a basketball. It can be folded and unfolded on command to temporarily capture organisms for detailed examination and take small tissue samples that are stored directly on board the submarine for later genetic analysis. It is designed to.

The ultimate goal is to take a small biopsy and release the animal relatively unscathed, but RAD2's current technique (called tissue cutting) is “a little more crude,” Phillips said.

RAD2 has already been tested on two expeditions, collecting up to 14 tissue samples a day at a depth of around 1200 meters. “We could get small pieces of tissue, and sometimes we could get whole animals,” he says. “It depended on how big it was. So I can't say we've been able to release the animal unharmed after that, but we're moving towards that.”

The robot sampler is also equipped with a 4K resolution video camera to capture high-quality footage of the animal in motion, and a virtual model of the animal is constructed by various 3D scanning devices. In the future, Phillips said, he might be able to put sensors on each of his 12 sides of the dodecahedron and take different measurements of living things at once.

Phillips called other sampling methods “outdated” and said they essentially require people to manually put things into jars for later analysis, or use submersibles to do the same thing. Masu.

Preservation at the point of collection using RAD2 improves the quality of tissue samples and also allows researchers to detect which genes are expressed, further informing animal behavior and physiology. Phillips said it could shed some light. “This is a luxury item,” he says. “This is the best you can get with this animal, better than anyone we’ve ever had.”

eva stewart Researchers at the University of Southampton in the UK say that while digital data on deep-sea life can be a useful tool for research, there is no substitute for capturing and preserving entire samples.

“There are thousands of type specimens here. [at the university]” says Stewart.Some of them were collected by Swedish scientists carl linnaeusShe died in 1778 and says: Once you have the specimen, you are done. Even as our science changes, we can keep coming back to it. ”

But Stewart said underwater scans are useful for gelatinous and other delicate animals that are difficult to collect intact, and for how the creatures behave in their natural environment, rather than after being hoisted onto the deck of a boat. I agree that it may be helpful to understand.

“We've been conducting research to examine gene expression in sea cucumbers because we want to understand how sea cucumbers behave when they're stressed or affected by things like climate change,” says Stewart. he says. “But when you collect them and bring them to the surface, it's stressful. So being able to harvest tissue from them in a more natural way means you know what their natural baseline is, so they can It means we may be able to see more clearly what happens when placed in different environments.”

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Source: www.newscientist.com

Discover the Thrills of Prince of Persia: Lost Crown – Conquer a New Gaming Empire

FA gigantic statue, frozen at the moment of destruction, is fixed above the entrance to Mount Kahu. In mid-autumn, fragments of shattered granite heads hang. In the castle’s intricate, trap-filled hallways, some characters haven’t aged a day in 100 years, while characters who arrived hours before you have already died of old age. Time does not follow normal rules in the Fortress’ cursed halls. If you want to complete Prince of Persia: The Lost Crown, you’d better learn that lesson quickly.

These quirks of time lend themselves well to a game that reimagines and combines multiple generations of a series dating back to 1989. Developer Jordan Mechner’s original Prince of Persia was his 2D platformer that had you navigating a castle filled with fake floors, guillotines, and swords. -Swirl the guards around to fight the Grand Vizier. Meanwhile, in the hands of developer Ubisoft, later reimaginings of the series saw the titular hero gain the ability to control time, suspending and reversing time to solve puzzles in 3D worlds, and more. I was able to avoid the trap. With The Lost Crown, Ubisoft returns to the side-view perspective of early games while incorporating the time-lapse powers of later titles, creating a vast labyrinthine world littered with enemies and traps to overcome. is created.

Labyrinth…Prince of Persia: The Lost Crown. Photo: Ubisoft

You play Sargon, one of Persia’s legendary defenders, as you hunt down Prince Ghassan and his captors. You follow the group up to Cuff Mountain. The kidnappers aim to force the prince to abdicate there. You must reach the prince before they do. Sargon can jump through holes, swing from pillar to pillar, and jump between the walls of narrow shafts to climb the levels of the Calf, but even this athletic ability only allows him access to a small portion of the fortress. In many cases, you will be faced with gaps that are too large. Ledges too high to jump, ledges too high to grab, locked doors too far to attack with your sword. But as you discover the secrets of the mountain and defeat more bosses, you learn how to run through the air, double jump, and fix your body to a point in space from which you can teleport back. Combine these powers and you’ll be able to perform intricate aerial acrobatics and explore all-new districts of Calf.

The Lost Crown is a reimagining of Prince of Persia as a Metroidvania, and the series feels at home in the genre’s ever-expanding universe. You repeat the same areas of the map over and over again, discovering new secrets in old rooms thanks to the powers you acquire. Treasure chests that were previously out of reach will fall into your hands, locked doors will open before your eyes, and bosses that were too fast or too strong will also become vulnerable to your attacks.

That said, The Lost Crown has a tough difficulty curve, with later platforming sections and bosses requiring you to memorize tough attack patterns and develop the reflexes to pull off complex combinations of jumps, dodges, and parries. is required. Hitting these skill walls can be a frustrating experience, especially in a game where the joy comes from putting together uninterrupted acrobatics and combos of attacks.

However, the moment you encounter a frustrating blocker, you can explore other parts of the calf. Finding new power usually opens up opportunities across the mountain, not just one area. You can also upgrade Sargon’s weapons to make them more powerful, purchase health potion upgrades, and change the configuration of your amulet. These unlockable items allow you to enhance your hero’s abilities, for example increasing his health when he is at low health or reducing the damage he takes from poison attacks. If you find a boss that you can’t defeat, it’s comforting to know that you can make the fight easier by replacing some of the amulets you bring into battle.

Prince of Persia: The Lost Crown is not a sequel or prequel to other games, but a new journey for the series, and its first step is a leap of faith. Not only are the most notable elements of the series’ various iterations (setting, traps, time forces, combat) all naturalized in this new form, but they are also the best of the newly selected games. That means you can play it like one of the games. This genre is as good a game as Metroid Dread or Hollow Knight, not an imitation of them. It’s been 13 years since the last completely new Prince of Persia game. If this is a new direction, I’m excited to see where it lands.

Prince of Persia: The Lost Crown will be released on PC, PS4/5, Switch and Xbox platforms on January 18th for £50.

Source: www.theguardian.com

Researchers Discover the Root Cause of a Historic, Lethal Climate Shift Millions of Years in the Past

Scientists have linked mass extinctions and climate change over the past 260 million years to massive volcanic eruptions and Earth’s astronomical cycles. The study highlights the role of CO2 emissions in climate change and reveals a complex relationship between Earth’s geology and position in space that is distinct from modern anthropogenic climate change.

New research reveals that Earth’s geological history is tied not only to the planet’s interior, but also to its astronomical movements.

The team of scientists concluded that it has occurred over the past 260 million years and that the mass extinction of life caused during these periods was primarily caused by large-scale volcanic eruptions and the resulting environmental crisis.

The analysis published in the magazine earth science reviews indicate that these eruptions released large amounts of carbon dioxide into the Earth’s atmosphere, resulting in extreme greenhouse climate warming and creating lethal or deadly conditions on Earth.

Astronomical cycles and Earth’s climate

Importantly, these phenomena occur every 26 to 33 million years and coincide with significant changes in the orbits of the solar system’s planets, which follow the same periodic pattern, the researchers added.

“Earth’s geological processes, long thought to be strictly determined by events inside the planet, may actually be controlled by the solar system and Earth’s astronomical cycles. milky way Galaxy,” says Professor Michael Lampino. new york university Department of Biology and senior author of the paper. “Importantly, these forces have converged many times in Earth’s past to predict dramatic changes in climate.”

The researchers, including Ken Caldeira of the Carnegie Institution for Science and geologist Sederia Rodriguez of Barnard College, say their conclusions are unrelated to climate change in the 20th and 21st centuries, and that scientists believe that human It warns that it shows that it is caused by activity. The last studied pulse of volcanic eruptions occurred about 16 million years ago.

But they added that the analysis nevertheless supports the well-established impact of carbon dioxide emissions on climate warming.

Volcanic eruptions and geological phenomena

Researchers have identified Continental Flood Basalt (CFB) eruptions, the largest volcanic eruptions on Earth with lava flows covering nearly 500,000 square miles, and other major geological events over the past 260 million years. focused. These include ocean anoxic events (periods during which the Earth’s oceans are depleted of oxygen, thereby producing toxic water) and the hyperthermal climate pulse, a sudden increase in global temperature and the resulting ocean and periods of mass extinction of non-marine life. .

They found that CFB eruptions frequently coincided with these other deadly geological phenomena, revealing the larger impact of volcanic activity. Its relevance to astronomy is evidenced by its regular, multimillion-year cycles of volcanic activity and extreme weather events, and its similarities with the known orbital periods of the Earth in our solar system and Milky Way galaxy.

The authors found that the correspondence between geological and astrophysical cycles was too close to be a mere coincidence. The big problem they were left with was how The astronomical movements of the planets disrupt the geological engines inside the Earth.

“This is an unexpected connection and predicts a convergence of both astronomy and geology. Events that occur on Earth occur within the context of our astronomical environment,” Rampino said. Observe.

References: “Periods of ~32.5 My and ~26.2 My in correlated episodes of continental flood basalts (CFBs), hyperthermal climate pulses, anoxic oceans, and mass extinctions over the past 260 My years: geological and astronomical cycles. Relationships” by Michael R. Rampino, Ken Caldeira, and Cederia Rodriguez, September 25, 2023. earth science reviews. DOI: 10.1016/j.earscirev.2023.104548

Source: scitechdaily.com

Researchers discover new method for treating life-threatening liver condition

New research reveals the role of omega-3 fatty acids in the fight against non-alcoholic steatohepatitis (NASH)

Using innovative analytical techniques, researchers determined that omega-3 targets betacellulin, a protein that contributes to liver fibrosis. This discovery opens new avenues for NASH drug research and highlights the importance of omega-3s in the diet for liver health.

A recent study conducted by Oregon State University revealed new insights into how certain polyunsaturated fatty acids, particularly omega-3s, fight serious liver conditions. This discovery paves the way for research into new drugs for nonalcoholic steatohepatitis (NASH), for which there is currently no FDA-approved treatment.

Scientists including Natalia Shulzhenko, Andrei Morgan, and Donald Jump at Oregon State University used a technique known as multiomic network analysis to find that omega-3 supplements can be used to treat nonalcoholic steatohepatitis. This mechanism involves betacellulin, a protein growth factor that contributes to liver fibrosis and other serious liver conditions.

The results of this research have recently been published in EMBO molecular medicine. NASH is associated with a disease known as metabolic syndrome, and it is crucial to understand the role of omega-3s in the fight against NASH.

In this study, scientists used both a mouse model and human liver transcriptome data to determine that omega-3 PUFAs reduce, or downregulate, betacellulin in both mice and humans with NASH. This discovery not only significantly advances our understanding of how NASH begins and progresses, but also opens new doors for pharmaceutical research. Researchers say the discovery of betacellulin as a new drug target may help explore precision medicine approaches to NASH treatment and liver cancer prevention by using specific omega-3 PUFAs.

In addition to dietary supplements, omega-3 PUFAs can be found in cold-water fatty fish such as salmon and mackerel, as well as in some nuts, seeds, and vegetable oils. Omega-3 PUFAs are essential fatty acids that are not produced by the body but must be obtained from the diet.

Reference:

Jyothi Padiadpu, Manuel Garcia-Jaramillo, Nolan K Newman, Written by Jacob W Pederson, Richard Rodrigues, Zhipeng Lee, Sekhavir Singh, Philippe Monnier, Giorgio Trinchieri, Kevin Brown, Amiran K. Zutsev, Natalia Shulzhenko, Donald B. Jump, Andrei Morgan, 2023 October 20th, EMBO molecular medicine. DOI: 10.15252/emm.202318367

Jyoti Padyap, a postdoctoral fellow in the OSU College of Pharmacy, is the study’s lead author. Other Oregon State researchers who contributed to the paper were Nolan Newman, Richard Rodriguez, Sehajivir Singh, Manuel Garcia-Jaramillo, Jacob Pederson, Jipeng Li, Philip Monnier, and Kevin Brown.

This research was supported by a grant from the National Institute of Diabetes and Digestive and Kidney Diseases, part of the National Institutes of Health.

Source: scitechdaily.com

Researchers discover the science behind our increased appetite for certain foods

Researchers have made an interesting discovery about the impact of advanced glycation end products (AGEs) found in prepared foods on hunger and health. AGEs, which are produced during cooking processes like baking and frying, enhance the appeal of food but also have negative effects on our well-being. Studies using nematodes have shown that AGEs lead to increased consumption and reduced lifespan, emphasizing the importance of choosing healthier food options.

Scientists at Buck have identified a mechanism that may explain why consuming delicious yet unhealthy food increases our desire to eat more. Overeating and weight gain can result from various factors, including the ready availability of flavorful, high-calorie foods. The researchers at Buck have found that AGEs, a type of chemical found in processed and prepared foods, contribute to increased hunger and a decreased ability to make healthy food choices. This research sheds light on the reasons behind our testing abilities for these foods.

According to Pankaj Kapahi, the lead author of the research study, “This research involving tiny worms has significant implications for human dietary choices and our tendency to overeat certain foods.” He added, “Modern processed foods rich in AGEs are tempting to eat, but we know very little about their long-term effects on our health.” The study was recently published in the journal eLife.

An evolutionary perspective suggests that humans have evolved mechanisms that encourage us to consume as much food as possible when it is readily available. This is because excess calories are stored as fat, which can be utilized during periods of fasting. The preference for flavorful foods, particularly those high in sugar, has been favored by natural selection. However, the mechanisms that make it difficult to resist such foods have remained unclear. AGEs are metabolic byproducts that occur naturally during sugar metabolism in cells but are also formed during cooking processes and are found in many processed foods. AGEs provide the appealing brown color that occurs during cooking, making food more appetizing and harder to resist.

While the Maillard reaction, which occurs when sugars and proteins interact with heat, is well-known for making food taste good, it can have detrimental effects on the body. The resulting AGEs cause inflammation and oxidative damage, which contribute to various health issues such as blood vessel stiffness, high blood pressure, kidney disease, cancer, and neurological problems. Accumulation of these metabolic byproducts in different organs is likely one of the main factors in the aging process of organs and organisms overall. It is due to these harmful effects that researchers are studying the impact of AGEs on health.

Even tiny worms used in the Kapahi lab were not immune to the allure and harm of AGEs. Researchers observed that these chemicals not only caused diseases and reduced lifespan but also increased the worms’ appetite for the same substances. The researchers aimed to understand the underlying mechanism by which AGEs promote excessive eating. Through their study, they identified a signaling pathway mediated by specific AGE molecules that promotes feeding and neurodegeneration. They also found that worms lacking the ability to process even naturally occurring AGEs had significantly shorter lifespans. The study is now expanding to mice, where researchers will investigate the relationship between AGEs and fat metabolism.

Understanding this signaling pathway may provide insights into overeating caused by modern diets rich in AGEs. This research highlights the role of AGE accumulation in diseases such as obesity and neurodegeneration and its association with the global rise in age-related diseases.

The key takeaway from their work is a profound realization that our food intake is often controlled by the food itself. To address this, the researchers have personally changed their diets, practicing intermittent fasting to allow the body to utilize fat instead of sugar. They also recommend consuming whole grains to maintain stable glucose levels and utilizing moist heat instead of dry cooking methods, such as steaming or frying. Adding acids when cooking, like when grilling, slows down the formation of AGEs.

In conclusion, this study provides valuable insights into the impact of AGEs found in processed and prepared foods on hunger, overeating, and overall health. It highlights the need for individuals to be conscious of their dietary choices and opt for healthier alternatives to reduce the negative effects of AGE accumulation in the body.

Source: scitechdaily.com