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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

Source: www.sci.news

Ancient Canoe Uncovers Early Advances in Navigation Technology

More than 7,000 years ago, Neolithic people used technologically sophisticated boats to navigate the Mediterranean Sea, according to a new study.


The 7,300-year-old canoe Marmotta 1 is on display at the Museum of Civilization in Rome. It is a huge dugout canoe made from an oak trunk, approximately 10.43 meters long, 1.15 meters wide at the stern, and 0.85 meters wide at the bow. Depending on the part of the canoe, the height is 65 to 44 cm. Image credit: Gibaja other., doi: 10.1371/journal.pone.0299765.

Many of Europe's most important civilizations were born along the Mediterranean coast.

The Phoenicians, Greeks, Romans, and Carthaginians took advantage of the virtually enclosed sea to move quickly between islands along the coast.

At various times in history, the Mediterranean Sea has been a space of travel and a means of communication.

However, one of the major migration phenomena in history occurred during the Neolithic period, when rural societies began to spread around Europe and North Africa.

The beginning of the Neolithic period is recorded in the Near East around 10,000 BC, but communities from that region gradually occupied the entire Mediterranean Sea around 7500-7000 BC, reaching the coast of Portugal around 5400 BC.

In a new study, Dr. Juan Guibaja and colleagues from Spain's National Research Council dug out a tree from La Marmotta, a Neolithic lakeside village near Rome, Italy, between 5700 and 5100 BC. Five dugout canoes that were built were investigated.

Analysis revealed that the canoe was constructed from four types of wood, which is unusual for similar sites, and incorporated advanced construction techniques such as lateral reinforcement.

Three T-shaped wooden objects are also associated with one canoe, each with a series of holes that may have been used to secure ropes tied to sails or other nautical elements. there is.

These features, together with previous reconstruction experiments, indicate that these are seaworthy vessels, a conclusion supported by the presence of stone tools associated with nearby islands.

“These canoes are exceptional examples of prehistoric vessels, and their construction required a well-organized and specialized workforce, as well as a detailed understanding of structural design and wood properties,” the researchers said. said.

“The similarities between these canoes and modern navigation technology support the idea that many major advances in sailing took place during the early Neolithic period.”

“Direct dating of a Neolithic canoe discovered at La Marmotta reveals it to be the oldest in the Mediterranean and provides valuable insight into Neolithic navigation,” the study said. they added.

“Our research reveals the remarkable technological sophistication of early agricultural and pastoral communities, highlighting their woodworking skills and complex shipbuilding.”

of study Published in an online journal PLoS ONE.

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JF Gibaha other. 2024. The first Neolithic ship in the Mediterranean: the settlement of La Marmotta (Anguillara Sabazia, Lazio, Italy). PLoS ONE 19 (3): e0299765; doi: 10.1371/journal.pone.0299765

Source: www.sci.news

Webb uncovers incredible black hole in the ancient cosmos

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



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

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

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

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

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

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

“This further supports the supermassive black hole hypothesis.”

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

of the team result appear in the diary Nature.

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

Source: www.sci.news

An undisclosed ice base uncovers ethereal cosmic particles in Antarctica

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

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

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

Small particles, huge targets

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

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

Birth of neutrino astronomy

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

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

New perspective

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

read more:


About our experts

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

Source: www.sciencefocus.com

Webb uncovers massive inactive galaxy with mature stars in the ancient cosmos

The formation of galaxies through the stepwise hierarchical coassembly of baryons and cold dark matter halos is a fundamental paradigm underpinning modern astrophysics and predicts a significant decline in the number of giant galaxies in the early Universe. . Very massive quiescent galaxies have been observed 1 to 2 billion years after the Big Bang. These form between 300 million and 500 million years ago and are very limiting for theoretical models, as only some models can form massive galaxies this early. The spectrum of newly discovered quiescent galaxy ZF-UDS-7329 reveals features typical of much older stellar populations. Detailed modeling shows that the stellar population formed about 1.5 billion years ago, when dark matter halos with sufficient host mass had not yet assembled in the standard scenario. This observation may indicate the existence of an undetected early population of galaxies and potentially large gaps in our understanding of the nature of early stellar populations, galaxy formation, and/or dark matter.



This web image shows ZF-UDS-7329, a rare massive galaxy that formed very early in the universe. Image credit: Glazebrook other., doi: 10.1038/s41586-024-07191-9.

Galaxy formation is a fundamental paradigm underpinning modern astrophysics, and a significant decrease in the number of massive galaxies in the early universe is predicted.

Very large quiescent galaxies have been observed 1 to 2 billion years after the Big Bang, casting doubt on previous theoretical models.

Professor Carl Glazebrook, from Swinburne University of Technology, said: “We have been tracking this galaxy for seven years, observing it for hours with two of the largest telescopes on Earth to find out its age.” Ta.

“But it was too red and too faint to be measured. In the end, we had to go outside Earth and use the web to see its properties.”

“This was truly a team effort, from the infrared sky survey that began in 2010 to identifying this galaxy as an anomaly, and the many hours spent with the Keck Telescope and the Very Large Telescope. But we couldn’t confirm it, and finally, last year, we spent a lot of effort trying to figure out how to process the web data and analyze this spectrum.”

“We are now beyond the realm of possibility to have identified the oldest giant stationary monster deep in the universe,” said Dr Temmiya Nanayakkara, an astronomer at Swinburne University of Technology.

“This pushes the limits of our current understanding of how galaxies form and evolve.”

“The key question now is how do stars form so quickly, so early in the universe, and how do they form at a time when other parts of the universe are forming stars? “What kind of mysterious mechanism could cause it to suddenly stop forming?”

“Galaxy formation is determined primarily by how dark matter is concentrated.”

“The presence of these extremely massive galaxies in the early universe poses significant challenges to our standard model of cosmology.”

“This is because dark matter structures large enough to accommodate these massive galaxies are unlikely to have formed yet.”

“More observations are needed to help us understand how common these galaxies are and how massive they really are.”

“This could open new doors in our understanding of the physics of dark matter,” Professor Glazebrook said.

“Webb continues to discover evidence that massive galaxies form early.”

“This result sets a new record for this phenomenon. It’s very impressive, but it’s just one object. But we want to discover more. If I If we were to do this, it would seriously disrupt our understanding of galaxy formation.”

This finding is reported in the following article: paper Published in this week’s magazine Nature.

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K. Glazebrook other. A huge galaxy that formed stars at z ~ 11. Nature, published online on February 14, 2024. doi: 10.1038/s41586-024-07191-9

Source: www.sci.news

The Hubble Telescope uncovers countless faraway galaxies in the constellation Cetus

New infrared images taken with wide field camera 3 (WFC3) onboard the NASA/ESA Hubble Space Telescope shows dozens of galaxies in the constellation Cetus, including SDSS J020941.27+001558.4, SDSS J020941.23+001600.7, and HerS J020941.1+001557. Masu.

This Hubble image shows a variety of distant galaxies in the constellation Cetus. Most galaxies are very small, but there are also some larger galaxies and some stars that can be seen in detail. At its center is an elliptical galaxy with a bright nucleus and a wide disk. A reddish, distorted ring of light surrounds its center, thicker on one side. Small galaxies intersect the rings as bright spots. Image credits: NASA / ESA / Hubble / H. Nayyeri / L. Marchetti / J. Lowenthal.

“What are we looking at when we study this image?” Hubble astronomers said in a statement.

“A distant galaxy 19.5 billion light-years away from Earth? Or a much closer (relatively) tiny glowing red galaxy 2.7 billion light-years away? Or a third galaxy that appears to be much closer to the second galaxy? Is not it?”

“The answer, perhaps confusingly, is that we are considering all three.”

“More precisely, we see light emitted from all of these galaxies, even though the farthest galaxy from Earth is directly behind the first.”

“In fact, it's that very alignment that makes the particular visuals of this image possible.”

“The bright spot in the center of this image is one of our closest galaxies, known by a long (but informative) name. SDSS J020941.27+001558.4,” they said.

“Another bright spot above it appears to be intersected by a curved crescent of light, SDSS J020941.23+001600.7, is the second closest galaxy. ”

“And finally, that curved crescent of light itself is 'lensed' light from a very distant galaxy. Girlfriend J020941.1+001557

Her J020941.1+001557 light was bent by the gravity of the foreground galaxy and expanded into a circular shape called an Einstein ring.

“Einstein rings occur when light from a very distant object bends around a large intermediate object,” the astronomers said.

“This is possible because the fabric of the universe itself, spacetime, is bent by mass, and so is light traveling through spacetime.”

“This is too subtle to observe at a local level, but when dealing with the curvature of light on large astronomical scales, for example when light emitted from a galaxy bends around another galaxy or galaxy cluster, , may become clearly observable.”

“When the lensed object and the lensed object are aligned in such a way, the result is a unique Einstein ring shape, with a complete or partial ring around the lensed object, depending on the precision of the alignment. A circle of light appears.

“This partial Einstein ring is of particular interest because it was identified thanks to a citizen science project. space warp — means that the public made the discovery of this object possible. ”

Source: www.sci.news

New research uncovers the ‘visual masking’ phenomenon in animal behavior

A strange phenomenon called visual masking can reveal the time scale of perception, but its underlying mechanisms are not well understood.

Colored plots show neural activity recorded in mouse visual cortex (V1). Each row of tick marks represents the spikes of a different neuron. Although researchers can predict the target side from neural activity with near-perfect accuracy, animal subjects often get incorrect masked trials due to how brain regions downstream of V1 process this information. I am.Image credit: Gail other.

Have you ever wanted to make something invisible? It turns out your brain can do it.

Unfortunately, this is a limited superpower. In visual masking, we do not consciously recognize another image when it appears in rapid succession.

But the timing of those images is important. For masking to work, the first image must flash very quickly, and the second image must follow rapidly (on the order of 50 milliseconds).

Don't get me wrong, the first image doesn't stay in view very long, but it's definitely long enough to be recognizable without the second image or mask.

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

“This is an interesting observation, that your perception doesn't accurately reflect what exists in the world,” said Dr. Sean Olsen, a researcher at the Allen Institute.

“Like other optical illusions, we think this tells us something about how the visual system works and, ultimately, the neural circuits underlying visual perception.”

In a new study, Dr. Olsen and colleagues take a closer look at the science behind this bizarre illusion and show for the first time that it also occurs in mice.

When the mice were trained to report what they saw, they were also able to pinpoint the specific areas of the brain needed for the visual masking illusion to work.

Dr. Christoph Koch, also from the Allen Institute, said, “Our research has narrowed down the region of the brain responsible for perceiving the world around us.''

“What are the steps from the time the photons rain down on your retina to when you actually become consciously aware of what you’re seeing?”

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 the early part 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.

To explore where unconscious sensations turn into conscious perceptions and actions, scientists first asked 16 mice to move a small mouse in the direction of rapidly flashing images in exchange for a reward if they chose the correct direction. I trained him to spin a Lego wheel.

I 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.

Because visual masking had never been tested in mice before, the authors had to create a task for mice, in which the images and the way they were presented 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, they tested it on 16 people.

It turns out that human perception (or lack thereof) and mouse perception of this particular visual masking illusion are very similar.

The researchers then used a special technique known as optogenetics, which allowed them to quickly suppress activity in cells or areas throughout the brain with flashes of light.

They targeted this inhibition to the mouse's primary visual cortex, known as the first part of the cortex where visual information from the eyes enters higher cortical areas of the brain.

By turning off the primary visual cortex the moment the masking image appeared, they were able to completely block visual masking after the target image. Even though the masking image was visible, the mouse reverted to accurately locating the first image. the current.

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 idea in the field that the cortex is the seat of conscious cognition in mammals, including ourselves,” Dr. Koch said.

Although this study narrowed down the region responsible for conscious perception to the cortex, there are still many regions of the cortex that may be involved.

Further studies will need to silence these other areas to test their effects on visual masking tasks.

“We're starting to put some limits on where masking is occurring,” Dr. Olsen said.

“We think this is a good paradigm to track to track other areas that are listening to the primary visual cortex and essentially fusing the flow of target and mask information in the brain. Masu.”

of findings It was published in the magazine natural neuroscience.

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SD Gale other. Visual cortex is required for posterior masking in mice. nut neurosi, published online on November 13, 2023. doi: 10.1038/s41593-023-01488-0

Source: www.sci.news

New approach uncovers the complete chemical complexity of quantum decoherence

Rochester researchers have reported a strategy for understanding how molecules in completely chemically complex solvents lose their quantum coherence. This discovery opens the door to rational tuning of quantum coherence through chemical design and functionalization.

Credit: Annie Ostau de Lafon

This discovery can be used to design molecules with custom quantum coherence properties, laying the chemical basis for new quantum technologies.

In quantum mechanics, particles can exist in multiple states at the same time, which defies the logic of everyday experience. This property, known as quantum superposition, is the basis for new quantum technologies that promise to transform computing, communications, and sensing. However, quantum superposition faces a serious challenge: quantum decoherence. During this process, interaction with the surrounding environment disrupts the delicate superposition of quantum states.

Quantum decoherence challenges

To unlock the power of chemistry and build complex molecular architectures for practical quantum applications, scientists need to understand and control quantum decoherence so they can engineer molecules with specific quantum coherence properties. must be. To do so, we need to know how to rationally modify the chemical structure of molecules to modulate or alleviate quantum decoherence. To do this, scientists need to know the “spectral density,” a quantity that summarizes the speed at which the environment moves and the strength of its interactions with the quantum system.

A breakthrough in spectral density measurement

Until now, quantifying this spectral density in a way that accurately reflects molecular complexity has remained difficult in theory and experiment. However, a team of scientists has developed a way to extract the spectral density of molecules in a solvent using a simple resonance Raman experiment, a method that fully captures the complexity of the chemical environment.

A team led by Ignacio Franco, an associate professor of chemistry and physics at the University of Rochester, published their findings in Proceedings of the National Academy of Sciences.

Relationship between molecular structure and quantum decoherence

Using the extracted spectral density, we can not only understand how quickly decoherence occurs, but also determine which parts of the chemical environment are primarily responsible for decoherence. As a result, scientists can now map decoherence pathways and link molecular structure to quantum decoherence.

“Chemistry is built on the idea that molecular structure determines the chemical and physical properties of matter. This principle guides the modern design of molecules for medical, agricultural, and energy applications.” Using our strategy, we can finally begin to develop chemical design principles for emerging quantum technologies,” said Ignacio Gustin, a chemistry graduate student at the University of Rochester and lead author of the study.

Resonant Raman experiments: an important tool

The breakthrough came when the team realized that resonance Raman experiments provided all the information needed to study decoherence in its full chemical complexity. Although such experiments are routinely used to study photophysics and photochemistry, their usefulness for quantum decoherence had not been evaluated. The key insight was shared by David McCamant, an associate professor in the Department of Chemistry at the University of Rochester and an expert in Raman spectroscopy, and Jang Woo Kim, currently on the faculty at Chonnam National University in South Korea and an expert in quantum decoherence. This became clear from the discussion. He was a postdoctoral fellow at the University of Rochester.

Case study: Thymine decoherence

The researchers used their method to show for the first time how the superposition of electrons in thymine, one of the building blocks of humans, occurs. DNA, it takes only 30 femtoseconds (one femtosecond is one billionth of a billionth of a second) after absorbing ultraviolet light. They found that some vibrations within the molecule were dominant in the early stages of the decoherence process, while the solvent was dominant in the later stages. Furthermore, they found that chemical modifications to thymine significantly altered the decoherence rate, with hydrogen bonding interactions near the thymine ring resulting in more rapid decoherence.

Future implications and applications

Ultimately, the team’s research paves the way to understanding the chemical principles governing quantum decoherence. “We are excited to use this strategy to finally understand quantum decoherence in molecules of full chemical complexity and use it to develop molecules with robust coherence properties.” Franco said.

Reference: “Mapping the intramolecular electron decoherence pathway” by Ignacio Gustin, Chan Woo Kim, David W. McCamant, and Ignacio Franco, November 28, 2023. Proceedings of the National Academy of Sciences. DOI: 10.1073/pnas.2309987120

Source: scitechdaily.com

New Research Uncovers the Secrets of Sarcomeres

Diagram of interacting thick and thin filaments within cardiac sarcomeres based on structural cryo-electron tomography data. Credit: MPI of Molecular Physiology

Scientists have captured the first true-to-life 3D images of the thick filaments of a mammal’s heart muscle.

Atrial fibrillation, heart failure, and stroke are among the serious health conditions that can result from hypertrophic cardiomyopathy and are important factors in sudden cardiac death in people under 35 years of age.

“The heart muscle is the central engine of the human body. Of course, if you know how engines are made and how they work, it’s easy to repair a broken engine,” says Stefan Lunser. say. “At the beginning of our study of muscle, we were able to use cryo-electron microscopy to visualize the structure of key muscle components and how they interact.”

“But these were still images of proteins taken from living cells. We just don’t teach them much,” Rounser said.

through thick and thin

Skeletal and cardiac muscles contract through the interaction of two types of parallel protein filaments (thin and thick) within the sarcomere. Sarcomeres are subdivided into several regions called zones and bands, and these filaments are arranged in different ways.

Thin filaments are composed of F-actin, troponin, tropomyosin, and nebulin. Thick filaments are formed by myosin, titin, and myosin-binding protein C (MyBP-C). The latter can form bonds between filaments, while the so-called motor protein myosin interacts with thin filaments to generate force and muscle contraction.

Thick filament structures within relaxed cardiac sarcomeres. The image above shows a tomographic slice of a cardiac sarcomere. Thin filaments are marked with green marks, thick filaments with purple arrows. The middle image shows reconstructed thick filaments (purple) and thin filaments (green). The image below shows the structure of thin filaments spanning several sarcomere regions. Scale bar indicates 50 nm. credit:
Molecular Physiology MPI

Muscle research milestones

“If we want to fully understand how muscles work at the molecular level, we need to delineate their components in their natural environment. This is one of the biggest challenges in biological research today. and cannot be addressed using traditional experimental approaches,” says Rounser.

To overcome this obstacle, his team developed an electron cryo-tomography workflow specifically for examining muscle samples. The scientists flash-frozen mammalian heart muscle samples produced by his Gautel group in London at very low temperatures (-175°C). ).

3D structure of a sarcomere showing thick filaments (purple) and thin filaments (green). Credit: MPI of Molecular Physiology

This maintains moisture and microstructure, keeping it pristine. Next, a focused ion beam (FIB milling) is applied to thin the sample to a thickness of approximately 100 nanometers, ideal for transmission electron microscopy, and multiple images are acquired while tilting the sample along its axis. Masu. Finally, computational methods reconstruct his three-dimensional image in high resolution.

In recent years, Raunser’s group has successfully applied customized workflows and recently published two groundbreaking publications. They created the first high-resolution images of sarcomeres and, so far, a misty muscle protein called nebulin. Both studies investigated the 3D organization of muscle proteins in sarcomeres, such as how myosin binds to actin to control muscle contraction, and how nebulin binds to actin to stabilize it and its We provide unprecedented insight into the 3D organization of muscle proteins in sarcomeres, including what determines their length.

complete the picture

In the current study, scientists have created, for the first time, high-resolution images of the heart’s thick filaments spanning several regions of the sarcomere. “With a length of 500 nm, this makes it the longest and largest structure ever resolved by cryo-ET,” said Davide Tamborini of MPI Dortmund, lead author of the study. Masu.

Even more impressive is the new insight gained into the molecular organization of the thick filaments and, by extension, their function. The arrangement of myosin molecules depends on their position within the filament.

Scientists believe that this allows the thick filaments to sense and process a large number of muscle-regulating signals and adjust the strength of muscle contractions depending on the sarcomere area. They also revealed how titin chains run along the filament. Titin chains intertwine with myosin and serve as a scaffold for its assembly, likely regulating length-dependent sarcomere activation.

“Our goal is to one day paint a complete picture of sarcomeres. The images of thick filaments in this study are ‘only’ snapshots of the muscle in its relaxed state. “We want to analyze sarcomeres in different states, such as during contraction, to fully understand how they function and how they are regulated,” says Rounser.

Comparisons with samples from patients with muscle diseases will ultimately contribute to a better understanding of diseases such as hypertrophic cardiomyopathy and the development of innovative treatments.

Reference: “Structure of native myosin filaments in relaxed cardiac sarcomeres” Davide Tamborrini, Zhexin Wang, Thorsten Wagner, Sebastian Tacke, Markus Stabrin, Michael Grange, Ay Lin Kho, Martin Rees, Pauline Bennett, Mathias Gautel, Stefan Raunser, 2023 October 32nd Nature.
DOI: 10.1038/s41586-023-06690-5

Source: scitechdaily.com

Study uncovers long-term health hazards

New research reveals significant metabolic and health risks associated with long-term coconut oil supplementation, including hormonal changes, weight gain, and inflammation. Lead researcher Marcio Alberto Torsoni advises against consuming coconut oil blindly and recommends a moderate amount according to dietary guidelines.

Scientists at the State University of Campinas observed changes in eating patterns, weight gain, signs of anxiety, and increased inflammation in the brain, adipose tissue, and liver in mice.

Article published in Functional food journal We report on a research study in which oral administration of extra virgin coconut oil supplements to mice showed significant changes in eating habits, weight gain, anxiety levels, and inflammation in the central nervous system, adipose tissue, and liver.

Researchers also discovered that leptin, an important metabolic hormone, insulin The ability to activate cellular mechanisms involved in satiety and blood sugar control may be impaired, and biochemical mechanisms involved in fat synthesis may be stimulated.

Researcher insights

Marcio Alberto Torsoni, a researcher at the Institute of Metabolic Disorders, said: “The results of this study suggest that although the process occurs slowly and quietly, long-term coconut oil supplementation contributes to the development of obesity and related comorbidities. “This suggests that it may cause significant metabolic changes.” LabDiMe) is conducted at the Faculty of Applied Sciences of the State University of Campinas (FCA-UNICAMP), São Paulo State, Brazil. He holds a PhD in Functional and Molecular Biology and completed postdoctoral studies at the UNICAMP Faculty of Medicine and the University of Michigan, USA.

LabDiMe is part of the Obesity and Comorbidity Research Center (OCRC), one of FAPESP’s Research, Innovation, and Dissemination Centers (RIDCs), and the Center for Metabolic Programming and Perinatal Management (MPPM), which receives funding from the U.S. We are collaborating with National Institutes of Health (NIH (National Institutes of Health).

Animal fat and coconut oil risks

Excessive intake of animal fats is associated with an increased risk of: cardiovascular disease, as well as obesity and diabetes. One of the components of this diet is cholesterol, but this type of fat also contains saturated fatty acids, which can activate inflammatory processes through Toll-like receptor 4 (TLR-4) and cause disease. there is.

Saturated fatty acids are also available from other sources, such as plants. For example, it makes up 90% of the fat in coconut oil. Although short-chain fatty acids make up the majority and are beneficial as they reduce inflammation, the saturated fatty acids found in coconut oil are sufficient to activate inflammatory pathways and damage many different types of cells.

“Consumption of coconut oil, either as part of the regular diet or as a dietary supplement, has increased significantly in the population,” Torsoni says. The problem is that most of the time it is consumed without the guidance of a nutritionist who can adjust the daily intake according to the individual’s needs.

experimental model

To find out whether daily consumption of coconut oil over long periods of time could cause health problems, the research group used an animal model involving healthy mice that were given coconut oil daily for eight weeks. did. This amount of coconut oil is equivalent to about 1 soup spoon (13g) of calories per day, or 5% of the calories from saturated fat in the diet of an adult of appropriate weight for his or her age and height.

Torsoni said coconut oil should be used in small amounts as part of seasonings and sauces, preferably with fresh or minimally processed vegetables. This is also the advice of the Ministry of Health’s Dietary Guidelines for Brazilian Citizens, which also recommends “an appropriate and healthy diet that combines quantity and quality and meets the needs of variety, balance, moderation and enjoyment.” I am.

“Coconut oil is not recommended as a supplement to treat disease or restore health,” Torsoni says.

Reference: “CO 2 supplementation induces lipogenesis in adipose tissue, leptin and insulin resistance in healthy Swiss mice” Alana Carolina Costa Veras, Larissa da Silva Bruzasco, Ana Beatriz Profiro Lopes, Beatriz da Silva Franco, Written by Alessandro Spencer de Souza Holanda, Andrea Maculano Estevez, Marcian Milanski, Adriana Souza Torsoni, Leticia Martins Ignacio-Sousa, Marcio Alberto Torsoni, June 4, 2023. Functional food journal.
DOI: 10.1016/j.jff.2023.105600

This study was funded by the São Paulo Research Foundation.

Source: scitechdaily.com