Category: 7. Science

  • Research Reveals RNA Clump Formation and Dissolution Method

    Research Reveals RNA Clump Formation and Dissolution Method

    BUFFALO, N.Y. — Look inside a brain cell with Huntington’s disease or ALS and you are likely to find RNA clumped together.

    These solid-like clusters, thought to be irreversible, can act as sponges that soak up surrounding proteins key for brain health, contributing to neurological disorders.

    How these harmful RNA clusters form in the first place has remained an open question.

    Now, University at Buffalo researchers have not only uncovered that tiny droplets of protein and nucleic acids in cells contribute to the formation of RNA clusters but also demonstrated a way to prevent and disassemble the clusters.

    Their findings, described in a study published Thursday (July 2) in Nature Chemistry , uses an engineered strand of RNA known as an antisense oligonucleotide that can bind to RNA clusters and disperse them.

    “It’s fascinating to watch these clusters form over time inside dense, droplet-like mixtures of protein and RNA under the microscope. Just as striking, the clusters dissolve when antisense oligonucleotides pull the RNA aggregates apart,” says the study’s corresponding author, Priya Banerjee, PhD, associate professor in the Department of Physics, within the UB College of Arts and Sciences. “What’s exciting about this discovery is that we not only figured out how these clusters form but also found a way to break them apart.”

    The work was supported by the U.S. National Institutes of Health and the St. Jude Children’s Research Hospital.

    How RNA clusters form

    The study sheds new light on how RNA clusters form within biomolecular condensates.

    Cells make these liquid-like droplets from RNA, DNA and proteins — or a combination of all three. Banerjee’s team has researched them extensively, investigating their role in both cellular function and disease, as well as their fundamental material properties that present new opportunities for synthetic biology applications.

    The condensates are essentially used as hosts by repeat RNAs, disease-linked RNA molecules with abnormally long strands of repeated sequences. At an early timepoint, the repeat RNAs remain fully mixed inside these condensates, but as the condensates age, the RNA molecules start clumping together, creating an RNA-rich solid core surrounded by an RNA-depleted fluid shell.

    “Repeat RNAs are inherently sticky, but interestingly, they don’t stick to each other just by themselves because they fold into stable 3D structures. They need the right environment to unfold and clump together, and the condensates provide that,” says the study’s first author, Tharun Selvam Mahendran, a PhD student in Banerjee’s lab.

    “Crucially, we also found that the solid-like repeat RNA clusters persist even after the host condensate dissolves,” Mahendran adds. “This persistence is partly why the clusters are thought to be irreversible.”

    Preventing — and reversing — clusters

    The team was first able to demonstrate that repeat RNA clustering can be prevented by using an RNA-binding protein known as G3Bp1 that is present in cells.

    “The RNA clusters come about from the RNA strands sticking together, but if you introduce another sticky element into the condensate, like G3BP1, then the interactions between the RNAs are frustrated and clusters stop forming,” Banerjee says. “It’s like introducing a chemical inhibitor into a crystal-growing solution, the ordered structure can no longer form properly. You can think of the G3BP1 as an observant molecular chaperone that binds to the sticky RNA molecules and makes sure that RNAs don’t stick to each other.”

    In order to reverse the clusters, the team employed an antisense oligonucleotide (ASO). Because ASO is a short RNA with a sequence complementary to the repeat RNA, it was able to not only bind to the aggregation-prone RNAs but also disassemble the RNA clusters.

    The team found that ASO’s disassembly abilities were highly tied to its specific sequence. Scramble the sequence in any way, and the ASO would fail to prevent clustering, let alone disassemble the clusters.

    “This suggests our ASO can be tailored to only target specific repeat RNAs, which is a good sign for its viability as a potential therapeutic application,” Banerjee says.

    Banerjee is also exploring RNA’s role in the origin of life, thanks to a seed grant from the Hypothesis Fund. He is studying whether biomolecular condensates may have protected RNA’s functions as biomolecular catalysts in the harsh prebiotic world.

    “It really just shows how RNAs may have evolved to take these different forms of matter, some of which are extremely useful for biological functions and perhaps even life itself — and others that can bring about disease,” Banerjee says.

    /Public Release. This material from the originating organization/author(s) might be of the point-in-time nature, and edited for clarity, style and length. Mirage.News does not take institutional positions or sides, and all views, positions, and conclusions expressed herein are solely those of the author(s).View in full here.

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  • Astronomers reveal how infant galaxies appeared in early universe | National

    Astronomers reveal how infant galaxies appeared in early universe | National


























    Astronomers reveal how infant galaxies appeared in early universe | National | wyomingnewsnow.tv

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  • Chinese scientists propose 2033 Neptune orbiter mission

    Chinese scientists propose 2033 Neptune orbiter mission

    HELSINKI — Scientists are proposing China’s first ice giant mission, aiming to launch a radioisotope-powered spacecraft to orbit Neptune and study its enigmatic moon Triton.

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    Andrew Jones covers China’s space industry for SpaceNews. Andrew has previously lived in China and reported from major space conferences there. Based in Helsinki, Finland, he has written for National Geographic, New Scientist, Smithsonian Magazine, Sky… More by Andrew Jones


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  • Red Blood Cell Insight Boosts Artificial Blood Production

    Red Blood Cell Insight Boosts Artificial Blood Production


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    Scientists from the University of Konstanz and Queen Mary University of London have identified a key molecular trigger that facilitates a crucial step in the formation of red blood cells.

    The finding could advance research efforts into artificial blood production, the researchers say, though clinical applications remain distant.

    The research is published in Science Signaling.

    The role of CXCL12 in red blood cell formation

    Red blood cell production, known as erythropoiesis, naturally occurs in the bone marrow. Stem cells mature into erythroblasts, which then develop into erythrocytes (red blood cells). In the final phase of this development, erythroblasts expel their nucleus, creating more internal space for hemoglobin – a protein that enables oxygen transport. This process is unique to mammals.

    Although much is known about the maturation of stem cells into red blood cells, the mechanism prompting nuclear expulsion was unclear.

    The research team, led by Dr. Julia Gutjahr from the Institute of Cellular Biology and Immunology Thurgau at the University of Konstanz, has identified that the chemokine CXCL12 can initiate this step. 

    “We discovered that the chemokine CXCL12 found mainly in bone marrow can trigger such nucleus expulsion, albeit in an interplay with several factors. By adding CXCL12 to erythroblasts at the right moment, we were able to artificially induce the expulsion of their nucleus,” said Gutjahr.

    Mechanism reveals new function of chemokine receptors

    The study found that CXCL12 interacts with red blood cell precursors differently than it does with other cell types. While other cells migrate in response to CXCL12, erythroblasts internalize the molecule, even transporting it into the nucleus. This internal action enhances cell maturation and assists in nucleus expulsion.

    The research suggests that chemokine receptors may have intracellular roles in addition to their established function on the cell surface and may inform future techniques for improving the efficiency of artificial blood production.

    “Importantly, apart from immediate practical application for the industrial production of red blood cells, our results brought a completely new understanding of cell biological mechanisms involved in erythroblast responses to chemokines,” added senior study author Antal Rot, a professor of inflammation sciences in the William Harvey Research Institute at Queen Mary University of London.

    “While all other cells migrate when stimulated by CXCL12, in erythroblasts this signalling molecule is transported into the interior of the cell, even into the nucleus,” Rot continued. “There, it accelerates their maturation and helps to expel the nucleus. Our research shows for the first time that chemokine receptors not only act on the cell surface but also inside the cell, thus opening entirely new perspectives on their role in cell biology,”

    Challenges in sourcing cells for artificial blood

    Artificial blood production typically starts with stem cells derived from umbilical cord blood or bone marrow. These cells can achieve nucleus expulsion in approximately 80% of cases. However, the limited availability and high demand for these cells makes this approach insufficient for large-scale applications.

    Recent advancements in cell reprogramming have allowed for the transformation of other cell types into stem-like cells, which can then be guided to produce red blood cells. Yet, this method is slower and less efficient, with successful nucleus expulsion occurring in only 40% of cases.

    “Based on our new findings highlighting the key role of CXCL12 in triggering nuclear expulsion, we can expect that using CXCL12 should bring significant improvement in producing red blood cells from reprogrammed cells,” said Gutjahr.

    The research team hopes that new advances aiding large-scale artificial blood production could lead to immediate, meaningful improvements for patients.

    “Even though body cells are readily available, the lab-based production process will remain complex. But it would enable the targeted generation of rare blood types, help bridge shortages or allow individuals to reproduce their own blood for specialized treatments in many different diseases,” said Gutjahr.

    Reference: Gutjahr JC, Hub E, Anderson CA, et al. Intracellular and nuclear CXCR4 signaling promotes terminal erythroblast differentiation and enucleation. Sci Signal. 2025;18(891):eadt2678. doi: 10.1126/scisignal.adt2678

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  • Algae of polar origin may impact tropical ocean biogeochemistry, food webs

    Algae of polar origin may impact tropical ocean biogeochemistry, food webs

    image: 

    Polarella has only been isolated from polar regions, though through -omics techniques, we have been able to identify the genera in a tropical oxygen deficient zone. Our data suggests that as oxygen and light declines, Polarella shifts from a phototrophic lifestyle (green) to potential heterotrophy (orange). At depths where oxygen is depleted and light level extremely low, Polarella upregulates genes involved in the uptake of both inorganic and organic nutrients and stress response.


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    Credit: Birch Maxwell Lazo-Murphy designed the concept image and was finalized by the OLAR editorial office/graphic design team

    A tiny single-celled organism may have a big impact on how the world’s basic chemical building blocks cycle between living things and the non-living environment. Called Polarella, the algal genus was thought to be restricted to polar cap regions of Earth, but a team has revealed that it is abundant and influential in the Eastern Tropical North Pacific Ocean off the coast of Mexico.

     

    The researchers, based at the University of South Carolina (USC), published their findings on May 26 in Ocean-Land-Atmosphere Research.

     

    Polarella is a type of dinoflagellate that makes up a major portion of marine microbial communities and contributes significantly to global primary production, said first author Birch Maxwell Lazo-Murphy, a graduate student pursuing a Ph.D. in marine science in the laboratory of Xuefeng “Nick” Peng, the corresponding author and an assistant professor of in USC’s School of Earth, Ocean, and Environment.

     

    “Understanding the roles of free-living dinoflagellates — as opposed to those that live in symbiosis with other organisms — in dynamic environments is critical, as these habitats often harbor high microbial diversity and niche differentiation,” Lazo-Murphy said. “Gaining a deeper insight into these environments will enable more accurate predictions of how these globally important groups will respond to environmental changes.”

     

    One such dynamic environment in marine systems are oxygen-deficient zones (ODZs), where oxygen levels are so depleted that oxygen often can’t be detected even by state-of-the-art sensors. This results from a process called remineralization, which involves living matter decaying into its basic chemical building blocks. According to Lazo-Murphy and Peng, these zones account for less than 1% of the ocean area on Earth, yet they are responsible for losing 33% of biologically available nitrogen — which is critical for plant growth, human health and more — across the globe.

     

    “ODZs have been expanding in size in part due to anthropogenic warming, so the role of ODZs and their respective microbial communities in global nutrient cycling is becoming increasingly important,” Peng said.

     

    To better understand the specific microbial communities in these areas, including how they respond to change and potentially impact nutrient cycling, the researchers used a technique called metatranscriptomics. They collected seawater samples from the oxygen-rich surface, mid-depths and oxygen-depleted depths of the Eastern Tropical North Pacific Ocean, which houses the world’s largest ODZ. They extracted and sequenced genetic material, from which they identified the specific organisms present in each sample.

     

    “We found unexpectedly high relative contribution of Polarella, which is thought to have bipolar distribution, to the microbial communities in the Eastern Tropical North Pacific Ocean,” Lazo-Murphy said. “Once we established their abundance, we set out to understand the functions and gene expressions of Polarella, as well as their impacts on the nutrient cycles, in the ODZ.”

     

    Further analysis revealed increased expression of stress response genes in Polarella, ranging from the lowest stress in surface samples to the highest in samples from oxygen-depleted depths. The researchers also found that the closer to the surface, genes for photosynthesis — converting sunlight into energy — were more highly expressed. In addition, they found that, while the overall gene expression was low for Polarella from low-oxygen or oxygen-free areas, the genes involved in transporting organic and inorganic nutrients were more highly expressed. Lazo-Murphy said this suggests that Polarella has an opportunistic lifestyle, taking advantage of available resources wherever it exists.

     

    “Collectively, these findings suggest that Polarella thrives beyond polar regions and likely plays a more significant ecological and biogeochemical role in the ocean than previously recognized,” Lazo-Murphy said.

     

    The Simons Foundation Postdoctoral Fellowship in Marine Microbiology and the Simons Early Career Investigator in Aquatic Microbial Ecology and Evolution Award to Peng supported this research.


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  • NASA teaches Mars orbiter to roll over in quest to find Red Planet water

    NASA teaches Mars orbiter to roll over in quest to find Red Planet water

    The Mars Reconnaissance Orbiter (MRO) has learned to do backward rolls to give its onboard radar better opportunities to find water-ice beneath the red planet’s surface.

    “Not only can you teach an old spacecraft new tricks, you can open up entirely new regions of the subsurface to explore by doing so,” Gareth Morgan of the Planetary Science Institute and co-investigator on MRO’s Shallow Radar (SHARAD) instrument, said in a statement.

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  • Traffic Delays Ahead on Division Street for Three Weeks

    Traffic Delays Ahead on Division Street for Three Weeks

    ST. CLOUD (WJON News) — Road maintenance on Division Street in St. Cloud is going to cause some traffic headaches for the next three weeks.

    Crews will be doing planned maintenance between Highway 15 and County Road 81 near the Parkwood Cinema.

    The work starts on Monday and will last intermittently for up to three weeks.

    Drivers are urged to find an alternate route to minimize delays.

    WOW: 19 Exotic-Looking Animals Surprisingly Found in America

    While some are native and others arrived by accident, there are animals living quite happily in the U.S. that will make you say, “No way!” From seriously big cats to the pinkest bird you’ve ever seen, here are some of the most exotic creatures calling America home.

    Gallery Credit: Stephen Lenz

    Quiz: Do you know your state insect?

    Stacker has used a variety of sources to compile a list of the official state insect(s) of each U.S. state, as well as their unique characteristics. Read on to see if you can guess which insect(s) represent your state. 

    Gallery Credit: Andrew Vale

    LOOK: 30 fascinating facts about sleep in the animal kingdom

    Gallery Credit: Katherine Gallagher


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  • Hubble Spots More Than Hundred Galaxies in Abell 209

    Hubble Spots More Than Hundred Galaxies in Abell 209

    Abell 209 is a massive galaxy cluster located about 2.8 billion light-years away in the constellation of Cetus.

    This Hubble image shows Abell 209, a galaxy cluster located about 2.8 billion light-years away in the constellation of Cetus. The color image includes both optical and infrared observations from Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). Twelve filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / M. Postman / P. Kelly.

    Galaxy clusters contain thousands of galaxies of all ages, shapes and sizes.

    Typically, they have a mass of about one million billion times the mass of the Sun.

    At one point in time galaxy clusters were believed to be the largest structures in the Universe — until they were usurped in the 1980s by the discovery of superclusters, which typically contain dozens of galaxy clusters and groups and span hundreds of millions of light-years.

    However, galaxy clusters do have one thing to cling on to; superclusters are not held together by gravity, so galaxy clusters still retain the title of the biggest structures in the Universe bound by gravity.

    “Abell 209’s galaxies are separated by millions of light-years, and the seemingly empty space between the galaxies is actually filled with hot, diffuse gas that can be spotted only at X-ray wavelengths,” Hubble astronomers said in a statement.

    “An even more elusive occupant of this galaxy cluster is dark matter: a form of matter that does not interact with light.”

    “The Universe is understood to be comprised of 5% normal matter, 25% dark matter, and 70% dark energy,” they said.

    “Hubble observations like the ones used to create this image can help us answer fundamental questions about our Universe, including mysteries surrounding dark matter and dark energy.”

    “These investigations leverage the immense mass of a galaxy cluster, which can bend the fabric of spacetime itself and create warped and magnified images of background galaxies and stars in a process called gravitational lensing.”

    “While this image lacks the dramatic rings that gravitational lensing can sometimes create, Abell 209 still shows subtle signs of lensing at work, in the form of streaky, slightly curved galaxies within the cluster’s golden glow.”

    “By measuring the distortion of these galaxies, astronomers can map the distribution of mass within the cluster, illuminating the underlying cloud of dark matter.”

    “This information, which Hubble’s fine resolution and sensitive instruments help to provide, is critical for testing theories of how our Universe has evolved.”

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  • Chinese scientists develop non-invasive blood sodium tracker-Xinhua

    TIANJIN, July 7 (Xinhua) — A Chinese research team has developed a novel system to enable non-invasive and dynamic monitoring of blood sodium levels, which addresses critical needs in managing dehydration, kidney diseases and neuroendocrine disorders.

    Findings of the study, conducted by Tianjin University, were recently published in the international journal Optica.

    Terahertz radiation — positioned between microwave and mid-infrared bands — offers unique advantages for biomedical sensing: low energy usage, minimal tissue damage and high sensitivity to molecular changes. However, its strong absorption by water and limited penetration capabilities of biological tissues have hindered practical applications.

    The team’s breakthrough terahertz optoacoustic systems overcome the two challenges by emitting terahertz waves at frequencies resonant with sodium ions but screening out water absorption signals, according to the paper.

    This selectively excites sodium vibrations, generating ultrasound that are captured by transducers for analysis. The conversion to acoustic waves reduces scattering and attenuation, enabling deeper penetration through muscle and bone, as well as successful capture by ultrasound transducers.

    Led by Tian Zhen, a professor at Tianjin University, the team achieved label-free, continuous sodium monitoring with validated accuracy in live mice and human volunteers. Their approach promises a painless alternative to needle-based tests, with potential for clinical adoption.

    “The system holds promise beyond sodium monitoring,” said Li Jiao, a researcher on the team. “By leveraging terahertz characteristic absorption spectra, it could potentially detect other ions like potassium and calcium, as well as biomolecules such as sugars, proteins and enzymes — significantly expanding its clinical utility.”

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  • Double-detonation supernova may set universal candles alight • The Register

    Double-detonation supernova may set universal candles alight • The Register

    Astroboffins have found the first evidence of a double-detonated Type Ia supernova, which could explain why we have enough bright points of reference in the skies to plot our place in the universe.

    Data from the European Southern Observatory’s Very Large Telescope (VLT) on SNR 0509-67.5 – a supernova 160,000 light-years from Earth, caused when a white dwarf star hit critical mass and exploded – reveals that the elements created suggest something may have triggered the star to explode ahead of time.

    Supernovae like these are very luminous and referred to as “standard candles” in astronomy. As fixed points, they are used to measure the expansion of the universe, but there are a lot more of them than current theories would predict, and new data could explain why.

    “The explosions of white dwarfs play a crucial role in astronomy,” said Priyam Das, a PhD student at the University of New South Wales Canberra, Australia, who led the study on SNR 0509-67.5 published [PDF] in Nature Astronomy. “Yet, despite their importance, the long-standing puzzle of the exact mechanism triggering their explosion remains unsolved.”

    Type Ia explosions are thought to be caused when two white dwarf stars orbit closely and one accretes mass from another and grows to about 1.4 times the mass of our Sun. This is the Chandrasekhar limit, named after Nobel Prize-winning physicist Subrahmanyan Chandrasekhar, or the maximum mass of a stable white dwarf star. However, spectrographic data from the VLT shows signatures indicating the white dwarf could have detonated earlier due to an elemental collision.

    If a white dwarf collects enough helium, the second most abundant element in the universe, this can form a shell around the star and ignite, compressing it and causing an early eruption before the Chandrasekhar limit is reached. That could explain why we have so many points of reference.

    SNR 0509-67.5 supernova

    SNR 0509-67.5, a bright spot in the universe. Source: ESO

    “The classical ‘textbook’ wisdom of how Type Ia supernovae explode is that material is accreted onto a white dwarf star composed of carbon and oxygen,” Professor Friedrich Röpke at the Center for Astronomy of Ruprecht-Karls University told The Register.

    “It seems very difficult to grow a white dwarf star to the Chandrasekhar mass. Since these objects are very stable, a drastic event is needed for this. One scenario that was considered to be likely working is the double detonation, where the detonation in the helium shell surrounding the carbon-oxygen white dwarf star triggers the actual detonation of that star.”

    The elements we’re made of were formed in exploding stars, and Type Ia supernovae typically eject large amounts of iron. But what the VLT saw was expanding shells of more complex elements such as calcium and sulfur, suggesting the double-detonation idea is correct.

    “We are for the first time able to provide direct observational support for this (before only hypothetical) scenario,” Professor Röpke explained.

    “We see two shells of heavy elements that are produced by two subsequent and spatially separated detonations. Calcium is one of these elements and it can be observed well with our methods. So, it is a tracer of the double detonation structure, but similar double shell structures are also expected in other heavy elements produced in the detonations.” ®

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