Category: 7. Science

  • Author defends addendum that sleuth says is ‘inadequate’ – Retraction Watch

    Author defends addendum that sleuth says is ‘inadequate’ – Retraction Watch

    A 23-year-old paper has received an addendum for “possible inadvertent errors” in the figures. But a sleuth says the update doesn’t address issues with the work. 

    The 2002 paper, which describes the behavior of Langerhans cells in normal and inflamed skin, was published in Nature Immunology and has been cited 774 times, according to Clarivate’s Web of Science. 

    The article received a correction in 2003 to replace two “incorrect” figures. Over 20 years later, PubPeer commenter “Archasia belfragei” flagged issues with different figures, noting in December that some PCR bands were “more similar than expected.”

    An addendum this April addressed the data errors, which, according to the notice, “may have occurred during the assembly of PCR measurements.” 

    Miriam Merad, lead author of the paper and now Chair of the Department of Immunology and Immunotherapy at Mount Sinai in New York, called the similarity between bands an “unfortunate mistake in assembling the PCR.” She told us “the PCR that was misassembled was measuring housekeeping genes, which are expressed by all cells” and were not the focus of the study. 

    The research was conducted at Irving Weissman’s lab at Stanford University in California. 

    But image expert and sleuth David Sanders told us the addendum is “inadequate in multiple senses.” While the correction applied to two proteins, the “problematic” data involve the expression of a third, he said. 

    “The argument that an image concerning protein expression … somehow justifies thoroughly flawed images of RNA levels is absurd,” Sanders said. The “extent and nature of the problems with the figures would, in my opinion, dictate that the article should have been retracted,” he added.

    Merad responded to Sanders’ concerns by emphasizing “there was no misconduct here.” 

    One of the paper’s authors, Harvard professor Amy Wagers, had another correction earlier this year to a 2023 paper in Nature Aging. The author correction addressed “potential duplication in two of the micrographs shown in the paper,” the January notice reads. Two of the probes were “unintentionally swapped” while the authors prepared images for the final submission of the paper. Wagers was one of 20 coauthors on this paper, which has been cited 37 times. She did not respond to email requests for comment.

    Wagers is the cochair of Harvard’s Department of Stem Cell and Regenerative Biology. In 2010, Wagers retracted a paper from Nature for data concerns. A postdoc in Wagers’ lab was dismissed after accepting responsibility for the “duplicated data and other inappropriate manipulations” cited in a retraction in 2011 from Blood.
    Lee Rubin, co-corresponding author and professor of stem cell and regenerative biology at Harvard, told us a coauthor of the paper discovered the mistake with the figures. “We are upset that we made the mistake but feel like we rectified it quickly and openly,” he said.


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  • Inouye Solar Telescope Sees Unprecedented Fine Details in Coronal Flare Loops

    Inouye Solar Telescope Sees Unprecedented Fine Details in Coronal Flare Loops

    Astronomers using the Visible Broadband Imager at NSF’s Daniel K. Inouye Solar Telescope captured dark coronal loop strands with unprecedented clarity during the decay phase of an X1.3-class flare on August 8, 2024. The loops averaged 48.2 km in width — perhaps as thin as 21 km — the smallest coronal loops ever imaged. This marks a potential breakthrough in resolving the fundamental scale of solar coronal loops and pushing the limits of flare modeling into an entirely new realm.

    A high-resolution image of the flare from the Inouye Solar Telescope, taken on August 8, 2024, at 20:12 UT. The image is about 4 Earth-diameters on each side. Labels of the different relevant regions of the image are added for clarity: flare ribbons (bright areas of energy release in the dense lower solar atmosphere) and an arcade of coronal loops (arcs of plasma outlining magnetic field lines that transport energy from the corona to the flare ribbons). Image credit: NSF / NSO / AURA.

    Coronal loops are arches of plasma that follow the Sun’s magnetic field lines, often preceding solar flares that trigger sudden releases of energy associated with some of these magnetic field lines twisting and snapping.

    This burst of energy fuels solar storms that can impact Earth’s critical infrastructure.

    Astronomers at the Inouye observe sunlight at the H-alpha wavelength (656.28 nm) to view specific features of the Sun, revealing details not visible in other types of solar observations.

    “This is the first time the Inouye Solar Telescope has ever observed an X-class flare,” said Dr. Cole Tamburri, an astronomer with the University of Colorado Boulder.

    “These flares are among the most energetic events our star produces, and we were fortunate to catch this one under perfect observing conditions.”

    Dr. Tamburri and colleagues focused on the razor-thin magnetic field loops (hundreds of them) woven above the flare ribbons.

    On average, the loops measured about 48 km across, but some were right at the telescope’s resolution limit.

    “Before Inouye, we could only imagine what this scale looked like,” Dr. Tamburri said.

    “Now we can see it directly. These are the smallest coronal loops ever imaged on the Sun.”

    The Inouye’s Visible Broadband Imager (VBI) instrument, tuned to the H-alpha filter, can resolve features down to 24 km.

    That is over two and a half times sharper than the next-best solar telescope, and it is that leap in resolution that made this discovery possible.

    “Knowing a telescope can theoretically do something is one thing,” said Dr. Maria Kazachenko, also from the University of Colorado Boulder.

    “Actually watching it perform at that limit is exhilarating.”

    While the original research plan involved studying chromospheric spectral line dynamics with the Inouye’s Visible Spectropolarimeter (ViSP) instrument, the VBI data revealed something unexpected treasures — ultra-fine coronal structures that can directly inform flare models built with complex radiative-hydrodynamic codes.

    “We went in looking for one thing and stumbled across something even more intriguing,” Dr. Kazachenko said.

    Theories have long suggested coronal loops could be anywhere from 10 to 100 km in width, but confirming this range observationally has been impossible — until now.

    “We’re finally peering into the spatial scales we’ve been speculating about for years,” Dr. Tamburri said.

    “This opens the door to studying not just their size, but their shapes, their evolution, and even the scales where magnetic reconnection — the engine behind flares — occurs.”

    Perhaps most tantalizing is the idea that these loops might be elementary structures — the fundamental building blocks of flare architecture.

    “If that’s the case, we’re not just resolving bundles of loops; we’re resolving individual loops for the first time,” Dr. Tamburri said.

    “It’s like going from seeing a forest to suddenly seeing every single tree.”

    The imagery itself is breathtaking: dark, threadlike loops arching in a glowing arcade, bright flare ribbons etched in almost impossibly sharp relief — a compact triangular one near the center, and a sweeping arc-shaped one across the top.

    “Even a casual viewer would immediately recognize the complexity,” Dr. Tamburri said.

    “It’s a landmark moment in solar science.”

    “We’re finally seeing the Sun at the scales it works on.”

    The team’s paper appears in the Astrophysical Journal Letters.

    _____

    Cole A. Tamburri et al. 2025. Unveiling Unprecedented Fine Structure in Coronal Flare Loops with the DKIST. ApJL, in press; doi: 10.3847/2041-8213/adf95e

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  • From NASA Citizen Scientist to Astronaut Training: An Interview with Benedetta Facini

    From NASA Citizen Scientist to Astronaut Training: An Interview with Benedetta Facini

    Titans Space Industries, a commercial space company, selected a new cohort of astronaut candidates this spring – and among them is NASA citizen scientist, Benedetta Facini. She has participated in not one, but many NASA citizen science projects: Cloudspotting on Mars, Active Asteroids, Daily Minor Planet, GLOBE, Exoasteroids and International Astronomical Collaboration (IASC). We asked her a few questions about her work with NASA and her path to becoming an astronaut candidate.

    Q: How did you learn about NASA Citizen Science?

    A: Through colleagues and social media, I often came across people talking about Citizen Science, and this immediately caught my curiosity. I did some online research on the subject, and I asked some colleagues already involved in it. Finally, I managed to find the way to participate by exploring the programs offered by NASA Citizen Science, which impressed me with their variety.

    Q: What would you say you have gained from working on these NASA projects?

    A: Curiosity in discovering new things and a lot of patience: many projects indeed require attention and, as mentioned, patience. I was pleased to discover that even NASA relies on “ordinary people” to carry out research, giving them the opportunity to learn new things using simple tools.

    I also gained hands-on experience in analyzing real data and identifying celestial objects to contribute to real research efforts. My favorite part was to learn to recognize the pattern of clouds in data collected by the Mars Climate Sounder on the Mars Reconnaissance Orbiter.

    I have learned the importance of international collaboration: I know many citizen scientists now, and interacting with them teaches me a lot every day. 

    Q. What do you do when you’re not working on citizen science?

    A: I am a student and a science communicator. I share my knowledge and enthusiasm through social media, schools, webinars around the world, and space festivals across Italy where I have the opportunity to engage with a wide audience, from young students to adults.

    Recently, I achieved a major milestone: I was selected as an Astronaut Candidate by the commercial space company, Titans Space Industries. I am thrilled to soon begin the basic training, which marks the first step toward realizing my dream of becoming an astronaut and contributing directly to human spaceflight and scientific research.

    Q. What do you need to do to become an astronaut?

    A: Gain as much experience as possible. During astronaut selection, not only academic achievements are evaluated, but also professional and personal experiences.

    Every skill can be useful during the selection process: the ability to work in a team, which is essential during space missions; survival skills; experience as a diver, skydiver, or pilot; knowledge of other languages; and the ability to adapt to different situations.

    I would also like to debunk a myth: you don’t need to be Einstein and fit as an Olympic level athlete; you just need to be good at what you do and be healthy.

    Q: How has citizen science helped you with your career?

    A: Citizen Science was very helpful for my career as a science communicator, as it gave me the opportunity to show people that anyone can contribute to the space sector. At the same time, it has allowed me to become a mentor and a point of reference for many students (mainly with the IASC project).

    The hands-on experience I gained in analyzing real data was also very helpful for my academic career, too. I had never had real data to work with before, and this experience proved extremely valuable for the practical courses in my physics degree program.

    Q. Do you have any advice you’d like to share for other citizen scientists or for people who want to become astronauts?

    A: For other citizen scientists my advice is to stay curious and persistent.

    Don’t be afraid to ask for help and interact with other colleagues because the goal of the NASA Citizen Science program is international collaboration and every small contribution can make a difference.

    For aspiring astronauts, my advice is to gain as much experience as possible. Academic results are important but hands-on skills, teamwork, adaptability, and real experiences are also important.

    Stay passionate and never lose your curiosity; the astronaut path is challenging; don’t give up after an eventual first rejection. You will always meet people trying to make you change your mind and your dream, even people from your family, but don’t stop in front of obstacles. The greatest regret is knowing you didn’t try to make your dream come true.

    Quoting my inspiration, Italian astronaut Paolo Nespoli: “You need to have the ability and the courage to dream of impossible things. Everyone can dream of things that are possible. Dream of something impossible, one of those things that, when you say it out loud, people look at you and say: “Sure, study hard and you’ll make it,” but deep down no one really believes it. Those are the impossible things that are worth trying to do!”

    Q: Thank you for sharing your story with us! Is there anything else you would like to add?

    A: I would like to thank the team behind NASA Citizen Science.

    These projects play a crucial role in keeping students’ passion for science alive and guiding them toward a potential career in this field.

    Knowing that I have contributed to helping scientists is incredibly motivating and encourages me and students around the world to keep going, stay curious, and continue pursuing our path in the science field.

    The opportunity to participate in these projects while learning is inspiring and it reinforces the idea that everyone, regardless of their background, can make a real impact in the scientific community.

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  • The NSF Inouye Solar Telescope delivers record-breaking images of solar flare, coronal loops

    The NSF Inouye Solar Telescope delivers record-breaking images of solar flare, coronal loops

    video: 

    A high-cadence, high-resolution movie of the flare captured by the Inouye Solar Telescope, sped up by 100x – both bright ribbons and dark overlying coronal loops are visible. The image is about 4 Earth-diameters on each side.


    view more 

    Credit: NSF/NSO/AURA

    MAUI, HI – AUGUST 25, 2025 — The highest-resolution images of a solar flare captured at the H-alpha wavelength (656.28 nm) ever captured may reshape how we understand the Sun’s magnetic architecture—and improve space weather forecasting. Using the U.S. National Science Foundation (NSF) Daniel K. Inouye Solar Telescope, built and operated by the NSF National Solar Observatory (NSO), astronomers captured dark coronal loop strands with unprecedented clarity during the decay phase of an X1.3-class flare on August 8, 2024, at 20:12 UT. The loops averaged 48.2 km in width—perhaps as thin as 21 km—the smallest coronal loops ever imaged. This marks a potential breakthrough in resolving the fundamental scale of solar coronal loops and pushing the limits of flare modeling into an entirely new realm. 

    Coronal loops are arches of plasma that follow the Sun’s magnetic field lines, often preceding solar flares that trigger sudden releases of energy associated with some of these magnetic field lines twisting and snapping. This burst of energy fuels solar storms that can impact Earth’s critical infrastructure. Astronomers at the Inouye observe sunlight at the H-alpha wavelength (656.28 nm) to view specific features of the Sun, revealing details not visible in other types of solar observations.

    “This is the first time the Inouye Solar Telescope has ever observed an X-class flare,” says Cole Tamburri, the study’s lead author who is supported by the Inouye Solar Telescope Ambassador Program while completing his Ph.D. at the University of Colorado Boulder (CU). The program is funded by the NSF and is designed to support Ph.D. students as they create a well-networked cohort of early-career scientists at U.S. Universities, who will bring their expertise in Inouye data reduction and analysis to the broader solar community. “These flares are among the most energetic events our star produces, and we were fortunate to catch this one under perfect observing conditions.”

    The team—which includes scientists from the NSO, the Laboratory for Atmospheric and Space Physics (LASP), the Cooperative Institute for Research in Environmental Sciences (CIRES), and CU—focused on the razor-thin magnetic field loops (hundreds of them) woven above the flare ribbons. On average, the loops measured about 48 km across, but some were right at the telescope’s resolution limit. “Before Inouye, we could only imagine what this scale looked like,” Tamburri explains. “Now we can see it directly. These are the smallest coronal loops ever imaged on the Sun.”

    The Inouye’s Visible Broadband Imager (VBI) instrument, tuned to the H-alpha filter, can resolve features down to ~24 km. That is over two and a half times sharper than the next-best solar telescope, and it is that leap in resolution that made this discovery possible. “Knowing a telescope can theoretically do something is one thing,” Maria Kazachenko, a co-author in the study and NSO scientist, notes. “Actually watching it perform at that limit is exhilarating.”

    While the original research plan involved studying chromospheric spectral line dynamics with the Inouye’s Visible Spectropolarimeter (ViSP) instrument, the VBI data revealed something unexpected treasures—ultra-fine coronal structures that can directly inform flare models built with complex radiative-hydrodynamic codes. “We went in looking for one thing and stumbled across something even more intriguing,” Kazachenko admits.

    Theories have long suggested coronal loops could be anywhere from 10 to 100 km in width, but confirming this range observationally has been impossible—until now. “We’re finally peering into the spatial scales we’ve been speculating about for years,” says Tamburri. “This opens the door to studying not just their size, but their shapes, their evolution, and even the scales where magnetic reconnection—the engine behind flares—occurs.”

    Perhaps most tantalizing is the idea that these loops might be elementary structures—the fundamental building blocks of flare architecture. “If that’s the case, we’re not just resolving bundles of loops; we’re resolving individual loops for the first time,” Tamburri adds. “It’s like going from seeing a forest to suddenly seeing every single tree.”

    The imagery itself is breathtaking: dark, threadlike loops arching in a glowing arcade, bright flare ribbons etched in almost impossibly sharp relief—a compact triangular one near the center, and a sweeping arc-shaped one across the top. Even a casual viewer, Tamburri suggests, would immediately recognize the complexity. “It’s a landmark moment in solar science,” he concludes. “We’re finally seeing the Sun at the scales it works on.” Something made only possible by the NSF Daniel K. Inouye Solar Telescope’s unprecedented capabilities.

    The paper describing this study, titled “Unveiling Unprecedented Fine Structure in Coronal Flare Loops with the DKIST,” is now available in The Astrophysical Journal Letters.

    ###

    About the U.S. NSF National Solar Observatory

    The mission of the NSF National Solar Observatory (NSO) is to advance knowledge of the Sun, both as an astronomical object and as the dominant external influence on Earth, by providing forefront observational opportunities to the research community.

    NSO built and operates the world’s most extensive collection of ground-based optical and infrared solar telescopes and auxiliary instrumentation— including the NSF GONG network of six stations around the world, and the world’s largest solar telescope, the NSF Daniel K. Inouye Solar Telescope—allowing solar physicists to probe all aspects of the Sun, from the deep solar interior to the photosphere, chromosphere, the outer corona, and out into the interplanetary medium. These assets also provide data for heliospheric modeling, space weather forecasting, and stellar astrophysics research, putting our Sun in the context of other stars and their environments.

    Besides the operation of cutting-edge facilities, the mission includes the continued development of advanced instrumentation both in-house and through partnerships, conducting solar research, and educational and public outreach. NSO is managed by the Association of Universities for Research in Astronomy, Inc. (AURA) under a cooperative agreement with NSF. For more information, visit nso.edu.

    Contact 

    For media inquiries, please contact: 

    Evan Pascual
    Communications Specialist
    U.S. NSF National Solar Observatory
    media@nso.edu


    Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.

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  • Supernova blast sculpts ghostly hand-shaped nebula in the cosmos (video)

    Supernova blast sculpts ghostly hand-shaped nebula in the cosmos (video)

    A glowing hand stretches across the cosmos, with its palm and fingers sculpted from the wreckage of a massive stellar explosion.

    The eerie structure is part of the nebula MSH 15-52, powered by pulsar B1509-58 — a rapidly spinning neutron star that is only about 12 miles (20 kilometers) in diameter. By combining radio data from the Australia Telescope Compact Array (ATCA) with X-rays from NASA’s Chandra X-ray Observatory, astronomers created a new view of the nebula, which spans over 150 light-years and resembles a human hand reaching toward the remains of the supernova — formally known as RCW 89 — that formed the pulsar at the heart of the image.

    “MSH 15–52 and RCW 89 show many unique features not found in other young sources,” according to a statement from the Chandra X-ray Observatory, releasing the new composite image. “There are, however, still many open questions regarding the formation and evolution of these structures.”

    The nebula MSH 15-52, which resembles a human hand with a palm and fingers pointing to the upper right in this view from NASA’s Chandra X-ray observatory. Near the center of the image is the pulsar B1509-58, a rapidly spinning neutron star that is only about 12 miles (19 km) in diameter. (Image credit: X-ray: NASA/CXC/Univ. of Hong Kong/S. Zhang et al.; Radio: ATNF/CSIRO/ATCA; H-alpha: UK STFC/Royal Observatory Edinburgh; Image Processing: NASA/CXC/SAO/N. Wolk)

    The central object, pulsar B1509-58, formed when a massive star ran out of fuel and collapsed before exploding as a supernova. The pulsar spins nearly seven times per second and has a magnetic field some 15 trillion times stronger than Earth’s. Despite its small size, it acts like a cosmic dynamo, accelerating particles to extreme energies and driving winds that carve the nebula into its hand-like form.

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  • Vibration Technique Boosts Lab-grown Tissue Safety

    Vibration Technique Boosts Lab-grown Tissue Safety

    Researchers in McGill’s Department of Mechanical Engineering have discovered a safe and low-cost method of engineering living materials such as tissues, organs and blood clots. By simply vibrating these materials as they form, scientists can dramatically influence how strong or, weak they become.

    The findings, published in the journal Advanced Functional Materials, could have a range of innovative applications, including in organ transplants, wound healing and regenerative medicine.

    Good vibrations

    The researchers used a speaker to apply controlled vibration, gently agitating the living materials during formation. By doing so, they found they could influence how cells organized and how strong or weak the final material became.

    The technique works across a range of soft cellular materials, including blood clots made from real blood and other human tissues.

    Aram Bahmani, study co-author and Yale postdoctoral fellow, conducted the research at McGill as a PhD student with Associate Professor Jianyu Li’s Biomaterials Engineering lab. Bahmani explained that strong, fast-forming blood clots are vital for use in emergencies like traumatic injuries. They’re also useful for people with clotting disorders.

    “On the other hand, the same approach could help design clots that break down more easily as necessary, helping to prevent dangerous conditions like stroke or deep vein thrombosis,” he added. “Mechanical nudging allows us to make the material up to four times stronger or weaker, depending on what we need it to do.”

    Why previous methods fell short

    Earlier approaches to shaping living tissues relied on physical forces like magnets or ultrasound waves. While promising, these methods often fail to replicate the complexity of real tissues, which contain billions of cells and have thick, three-dimensional structures. In addition, they are often limited to specific materials, can damage healthy tissues and sometimes trigger immune responses.

    The researchers’ study is the first to show that mechanical agitation, a very simple and widely accessible tool, can control the inner structure and performance of living materials in a “safe, scalable and highly tunable way.”

    From the lab bench to living systems

    To validate their findings, the team ran a series of tests to measure how vibration affected various cell-laden materials such as blood-based gels, plasma and seaweed-derived alginate. Using imaging and mechanical analysis, they assessed how broadly the method could be applied. Next, they tested the technique in animals.

    The results showed that the technique works when applied inside the body, without harming surrounding healthy tissues.

    Toward advanced medical technology

    Bahmani said he believes the simple method could one day be integrated into advanced medical devices or wound-healing techniques.

    “What makes this especially exciting is that our method is non-invasive, low-cost and easy to implement,” he said. “It does not rely on expensive machines or complex chemicals, meaning it could one day be built into portable medical devices, like a hand-held tool to stop bleeding, or a smart bandage that speeds up healing.”

    He noted that the method requires further testing, such as in irregular wounds or in combination with certain medications, before it can be used in real-life medical settings.

    “Moving toward clinical use will require miniaturizing the devices, optimizing settings for different medical scenarios and completing regulatory testing to ensure safety and effectiveness in humans,” he said.

    About this study

    “Engineering Highly Cellularized Living Materials via Mechanical Agitation” by Aram Bahmani, Jianyu Li et al was published in Advanced Functional Materials.

    The research was funded by the Canadian Institutes of Health Research, the NSERC/FRQNT NOVA Program, the Fonds de Recherche du Québec-Nature et Technologies Doctoral Scholarship, the Canada Research Chairs Program, the Centre de Recherche sur les Systèmes Polymères et Composites à Haute Performance and the McGill Faculty of Engineering.

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  • Tiny Waves, Big Impact: Study Finds New Way to Control Fluid in Space

    Tiny Waves, Big Impact: Study Finds New Way to Control Fluid in Space

    By changing the height of a partially submerged barrier in moving water, researchers Likun Zhang (right), senior scientist at the National Center for Physical Acoustics, and Zhengwu Wang, a doctoral student in physics, found that they can alter how much energy passes through that barrier. Photo by Clara Turnage/University Marketing and Communications 

    Likun Zhang, senior scientist at the National Center for Physical Acoustics and associate professor in the Department of Physics and Astronomy, led a research team studying how liquid waves move through barriers in low-gravity environments. Their results were published in Physical Review Letters 

    “In low-gravity cases like the space station, surface tension dominates everything,” said Zhengwu Wang, a fourth-year Ole Miss doctoral student in physics and co-author of the study. “The curvature of the water – the meniscus – is going to appear around structures, and we wanted to know how that meniscus would affect how waves move across barriers.” 

    When water meets a partially submerged barrier – think of a leaf on a pond – the surface tension of the liquid causes the liquid to curve upward where it meets the barrier; in this case, the leaf. Zhang and Wang’s research shows that this curve, called the meniscus, can be manipulated to reduce or increase the amount of energy that passes through that barrier.  

     

    “This is the first experiment studying this behavior in fluid, but it opens the door to new phenomena and new physics. This work is valuable because it shows a new way to control fluid for the first time.”  – Likun Zhang

    If the meniscus’ curve is slight, more energy passes through. But as the meniscus curves more steeply, it reduces the energy conveyed by the fluid.  

    A wave ripples through a tank of water in a laboratory.

    A wave travels through a tank in Likun Zhang’s laboratory at the National Center for Physical Acoustics. Submitted photo 

    “Our common sense tells us a barrier should block waves, but here we found certain meniscus shapes can make waves pass through more easily,” Zhang said. “Only a tiny, 1.5-millimeter change in the meniscus shape caused the transmission to drop from about 60% to just a few percent. Tiny meniscus, huge impact.” 

    Space travelers use liquids for all manner of applications: from fuel and water-recycling systems to life support and cooling systems. Being able to better control the fluid in these systems can make them more efficient and lighter – a key for space travel. 

    “These are really tiny effects in daily life, but they can have a huge impact in microgravity environments,” Wang said.  

    To conduct the experiment, the researchers simulated low gravity by generating small, frequent surface waves. Then, they placed a partial barrier in the path of those waves and used acoustics to measure the meniscus’ movement.  

    By changing the barrier’s height and using a surface coating to make it water-attracting or water-repelling, the researchers controlled the meniscus – and how much energy passed through the barrier.  

    A young man looks through a camera mounted in a track on a laboratory as another man watches.

    Zhengwu Wang (left) a doctoral student studying physics, adjusts his camera to best capture the movement of water through a barrier in microgravity-like conditions. Wang and Likun Zhang, senior scientist at the National Center for Physical Acoustics, recently published research on manipulating the flow of water through barriers in Physical Review Letters. Photo by Clara Turnage/University Marketing and Communications 

    As physicists, we are looking at very fundamental problems: the like problem of wave dynamics and barriers, Zhang said. But being able to control fluid behavior in low gravity is crucial – whether youre talking about water recycling systems or fuel tanks – because you cant rely on gravity to separate liquids and gases. 

    The applications could prove useful in earthbound manufacturing and biomedical engineering, too, where microfluidic devices move fluids through channels just millimeters wide, Zhang said. These devices range from printers to DNA chips to lab-on-a-chip technology 

    “This is the first experiment studying this behavior in fluid, but it opens the door to new phenomena and new physics,” he said. “This work is valuable because it shows a new way to control fluid for the first time.”  

    This material is based on work supported by the National Science Foundation grant no. 2306106. 

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  • McGill researchers develop safe, scalable vibration technique to improve lab-grown tissues | Newsroom

    McGill researchers develop safe, scalable vibration technique to improve lab-grown tissues | Newsroom

    Researchers in McGill’s Department of Mechanical Engineering have discovered a safe and low-cost method of engineering living materials such as tissues, organs and blood clots. By simply vibrating these materials as they form, scientists can dramatically influence how strong or, weak they become.

    The findings, published in the journal Advanced Functional Materials, could have a range of innovative applications, including in organ transplants, wound healing and regenerative medicine.

    Good vibrations

    The researchers used a speaker to apply controlled vibration, gently agitating the living materials during formation. By doing so, they found they could influence how cells organized and how strong or weak the final material became.

    The technique works across a range of soft cellular materials, including blood clots made from real blood and other human tissues.

    Aram Bahmani, study co-author and Yale postdoctoral fellow, conducted the research at McGill as a PhD student with Associate Professor Jianyu Li’s Biomaterials Engineering lab. Bahmani explained that strong, fast-forming blood clots are vital for use in emergencies like traumatic injuries. They’re also useful for people with clotting disorders.

    “On the other hand, the same approach could help design clots that break down more easily as necessary, helping to prevent dangerous conditions like stroke or deep vein thrombosis,” he added. “Mechanical nudging allows us to make the material up to four times stronger or weaker, depending on what we need it to do.”

    Why previous methods fell short

    Earlier approaches to shaping living tissues relied on physical forces like magnets or ultrasound waves. While promising, these methods often fail to replicate the complexity of real tissues, which contain billions of cells and have thick, three-dimensional structures. In addition, they are often limited to specific materials, can damage healthy tissues and sometimes trigger immune responses.

    The researchers’ study is the first to show that mechanical agitation, a very simple and widely accessible tool, can control the inner structure and performance of living materials in a “safe, scalable and highly tunable way.”

    From the lab bench to living systems

    To validate their findings, the team ran a series of tests to measure how vibration affected various cell-laden materials such as blood-based gels, plasma and seaweed-derived alginate. Using imaging and mechanical analysis, they assessed how broadly the method could be applied. Next, they tested the technique in animals.

    The results showed that the technique works when applied inside the body, without harming surrounding healthy tissues.

    Toward advanced medical technology

    Bahmani said he believes the simple method could one day be integrated into advanced medical devices or wound-healing techniques.

    “What makes this especially exciting is that our method is non-invasive, low-cost and easy to implement,” he said. “It does not rely on expensive machines or complex chemicals, meaning it could one day be built into portable medical devices, like a hand-held tool to stop bleeding, or a smart bandage that speeds up healing.” 

    He noted that the method requires further testing, such as in irregular wounds or in combination with certain medications, before it can be used in real-life medical settings.

    “Moving toward clinical use will require miniaturizing the devices, optimizing settings for different medical scenarios and completing regulatory testing to ensure safety and effectiveness in humans,” he said.

     

    About this study

    “Engineering Highly Cellularized Living Materials via Mechanical Agitation” by Aram Bahmani, Jianyu Li et al was published in Advanced Functional Materials.

    The research was funded by the Canadian Institutes of Health Research, the NSERC/FRQNT NOVA Program, the Fonds de Recherche du Québec–Nature et Technologies Doctoral Scholarship, the Canada Research Chairs Program, the Centre de Recherche sur les Systèmes Polymères et Composites à Haute Performance and the McGill Faculty of Engineering.

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  • Miles Below Earth’s Surface, Scientists Found A Giant Ecosystem Teeming With Life

    Miles Below Earth’s Surface, Scientists Found A Giant Ecosystem Teeming With Life

    Beneath our feet lies a hidden world of staggering scale, a deep ecosystem brimming with billions of microorganisms. Its astonishing diversity has earned it the nickname the “subterranean Galapagos” and suggests that its genetic richness may rival or even surpass life above ground.

    Presenting their work at the American Geophysical Union’s annual meeting in 2018, the researchers calculated the size of this mysterious treasure trove of life for the first time – and it was a lot bigger than they expected.

    They reported that approximately 70 percent of the total number of microbes on the planet live underground. In total, these microbes represent around 15 to 23 billion tonnes of carbon – hundreds of times greater than the carbon mass of all humans on the surface.

    Scientists have barely scratched the surface when it comes to describing these microorganisms. However, first glances suggest that the genetic diversity of life below the surface might be comparable to, or perhaps even exceed, life above the surface. This is why nicknamed the ecosystem the “subterranean Galapagos.”

    This unidentified nematode was found at the bottom of a gold mine in South Africa, some 1.4 kilometers below the surface.

    Image credit: Gaetan Borgonie/Extreme Life Isyensya, Belgium

    However, don’t expect any giant tortoises down there. Bacteria and their evolutionary cousins – archaea – seem to dominate beneath the surface, although the researchers also noted a fair number of eukarya down there too. For example, researchers described an unidentified nematode over 1.4 kilometers (0.8 miles) deep in a South African gold mine. 

    “Ten years ago, we had sampled only a few sites – the kinds of places we’d expect to find life,” Karen Lloyd, study author and Associate Professor of microbiology at the University of Tennessee, said in a statement in 2018.

    “Thanks to ultra-deep sampling, we know we can find them pretty much everywhere, albeit the sampling has obviously reached only an infinitesimally tiny part of the deep biosphere,” added Professor Lloyd.

    To reach the findings, the team brought together dozens of studies that looked at samples brought up from drilling between 2.5 and 5 kilometers (1.55 to 3.1 miles) into the Earth’s crust, both in the seafloor and the inland continents. Also, to their surprise, they discovered that the subsurface deep biosphere is almost twice the volume of all oceans.

    Subjected to intense heat, crushing pressures, no light, and scarcely any nutrients, this is hardly where you would expect to find a diverse bank of life. Nevertheless, the researchers said that this ecosystem could answer many questions about the limits of life on Earth – and beyond.

    “Our studies of deep biosphere microbes have produced much new knowledge, but also a realization and far greater appreciation of how much we have yet to learn about subsurface life,” added Rick Colwell, microbial ecologist at Oregon State University.

    “For example, scientists do not yet know all the ways in which deep subsurface life affects surface life and vice versa. And, for now, we can only marvel at the nature of the metabolisms that allow life to survive under the extremely impoverished and forbidding conditions for life in deep Earth.”

    An earlier version of this article was published in December 2018.

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  • New laser helps decode rare earth element samarium’s secret spectrum

    New laser helps decode rare earth element samarium’s secret spectrum

    Scientists in Germany have uncovered previously unknown properties of the rare Earth element samarium by developing a powerful new technique to investigate the internal structure of atoms.

    For the discovery, the research team at the Johannes Gutenberg University Mainz (JGU) and the Helmholtz Institute Mainz (HIM) applied an advanced laser-based technique known as dual-comb spectroscopy (DCS).

    The method, which enabled them to measure atomic spectra at a wide band of electromagnetic frequencies with high resolution and sensitivity, helped the team uncover hidden atomic transitions in the rare element.

    Samarium (Sm) is critical for producing high-performance samarium-cobalt (SmCo) permanent magnets used in electric vehicle motors and wind turbine generators.

    The findings also helped pave the way for ‘Spectroscopy 2.0,’ a next-generation platform designed as a ‘massively parallel spectroscopic tool’ capable of simultaneously performing many measurements.

    Breaking the limits

    Comprehending the internal structure of atoms is crucial to understanding the composition of matter and designing new experiments to explore fundamental physics. However, the energy-level structures of many atoms are still not fully explored, especially in the case of rare earths and actinides.

    Spectroscopy, which is based on the principle that electrons absorb or emit energy when they move between energy levels in an atom, is one of the most widely used methods for studying an atom’s structure.

    “High-resolution broadband spectroscopy is essential for precision measurements in atomic physics and the search for new fundamental interactions,” Razmik Aramyan, PhD student at the University of the study’s main author, explained.

    The whole experimental setup of the dual-comb spectroscopy.
    Credit: Razmik Aramyan

    Nevertheless, according to the PhD student, progress is often hindered by the challenge of measuring complex atomic spectra, as it is difficult to properly distinguish the sample’s signals and the limited range of wavelengths that instruments can detect.

    To overcome the challenges, Aramyan and his team utilized a method known as dual-comb spectroscopy (DCS), which is based on the 2005 Nobel-winning optical frequency comb technique.

    This method, where two synchronized comb lasers measure light frequencies with greater accuracy than conventional methods, allowed them to measure atomic spectra at a wide band of electromagnetic frequencies with high resolution and high sensitivity.

    Unlocking atomic secrets

    To detect weak signals with high precision, the team implemented multiple photodetectors to improve the signal-to-noise ratio. This made it possible to clearly identify the experimental data and determine the spectrum’s wavelengths.

    “This study introduces an enhanced multichannel DCS approach that combines a photodetector array with a novel scheme for resolving frequency ambiguities, enabling ambiguity-free, high-signal-to-noise-ratio broadband measurements,” Aramyan stated.

    The researchers described this as the first step toward ‘Spectroscopy 2.0’, a tool that will be used to perform spectroscopy of dense atomic and molecular spectra under intense magnetic fields.

    Since DCS is particularly well-suited to filling gaps in atomic data, the researchers recorded the spectrum of samarium vapor at different temperatures. They analyzed the spectral behavior at different samarium concentrations.

    When comparing the results, they were stunned to discover several previously undescribed samarium absorption lines. “This illustrates the potential of our method to uncover previously unknown atomic properties,” Aramyan said in a press release.

    According to the team, the findings open promising possibilities for massively parallel spectroscopy, including studies of atoms in pulsed, ultra-high magnetic fields.

    The study has been published in the journal Physical Review Applied.

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