Category: 7. Science

  • Detecting Water Ice And Vapor Disks Originating From Icy Planetary Bodies Around White Dwarfs With Future PRIMA Observations

    Detecting Water Ice And Vapor Disks Originating From Icy Planetary Bodies Around White Dwarfs With Future PRIMA Observations

    Schematic showing the distribution of the modeled volatile gas (e.g., water vapor) disk and water ice disk around a WD. The rocky dust disk and their observationally inferred properties are also summarized. — astro-ph.EP

    Observations of atmospheres of polluted white dwarfs provide insights into the elemental composition of accreted exoplanets and exo-asteroids.

    However, they poorly constrain the abundance of ice-forming volatile elements due to the properties of white dwarf atmospheres. Instead of focusing solely on atmospheric observations, we propose observing circumstellar water ice and vapor disks formed by the tidal disruption of icy bodies using the future PRobe far-Infrared Mission for Astrophysics (PRIMA) far-infrared enhanced survey spectrometer.

    PRIMA has the potential to measure volatile abundances in colder circumstellar regions inaccessible by shorter-wavelength observations. We employ a simple disk emission model with disk parameter ranges inferred from previous observations and disk evolution simulations. We find the 44-μm water ice feature promising for observing icy disks.

    For white dwarfs within 60 pc, 1-hour PRIMA observations could detect water ice with a mass above 1020 g, representing a potential lower limit of circumstellar disk mass. Water vapor rotational lines also abundantly emerge within the PRIMA wavelength coverage, and 5-hour observations for white dwarfs within 20 pc could detect water vapor with a total disk mass ≳1020 g, depending on the H2/H2O ratio. 19 metal polluted white dwarfs within 20 pc and 210 within 60 pc could be optimal targets for water vapor and ice observations, respectively.

    Ayaka Okuya, Hideko Nomura

    Comments: 19 pages, 7 figures, published in JATIS. This paper is part of the JATIS special issue focused on the PRobe Infrared Mission for Astrophysics (PRIMA) probe mission concept. The issue is edited by Matt Griffin and Naseem Rangwala (JATIS VOL. 11, NO. 3 | July 2025)
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Instrumentation and Methods for Astrophysics (astro-ph.IM); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2509.01697 [astro-ph.EP] (or arXiv:2509.01697v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2509.01697
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    Journal reference: J. Astron. Telesc. Instrum. Syst. 11(3), 031607 (2025)
    Related DOI:
    https://doi.org/10.1117/1.JATIS.11.3.031607
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    Submission history
    From: Ayaka Okuya
    [v1] Mon, 1 Sep 2025 18:17:26 UTC (957 KB)
    https://arxiv.org/abs/2509.01697
    Astrobiology,

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • An Analysis Of The Radius Gap In A Sample Of Kepler, K2 And TESS Exoplanets Orbiting M Dwarf Stars

    An Analysis Of The Radius Gap In A Sample Of Kepler, K2 And TESS Exoplanets Orbiting M Dwarf Stars

    Distribution of the derived planetary radii as a function of insolation, along with the associated KDE. — astro-ph.EP

    Planetary radii are derived for 218 exoplanets orbiting 161 M dwarf stars. Stellar radii are based on an analysis of APOGEE high-resolution near-IR spectra for a subsample of the M-dwarfs; these results are used to define a stellar radius-MKs calibration that is applied to the sample of M-dwarf planet hosts.

    The planetary radius distribution displays a gap over Rp∼1.6-2.0 R, bordered by two peaks at Rp∼1.2-1.6 R⊕ (super-Earths) and 2.0-2.4 R (sub-Neptunes). The radius gap is nearly constant with exoplanetary orbital period (a power-law slope of m=+0.01+0.03−0.04), which is different (2-3σ) from m∼−0.10 found previously for FGK dwarfs.

    This flat slope agrees with pebble accretion models, which include photoevaporation and inward orbital migration. The radius gap as a function of insolation is approximately constant over the range of Sp∼20-250 S⊕. The Rp-Porb plane exhibits a sub-Neptune desert for Porb<2d, that appears at Sp>120 S, being significantly smaller than Sp>650 S found in the FGK planet-hosts, indicating that the appearance of the sub-Neptune desert is a function of host-star mass.

    Published masses for 51 exoplanets are combined with our radii to determine densities, which exhibit a gap at ρp∼0.9ρ, separating rocky exoplanets from sub-Neptunes. The density distribution within the sub-Neptune family itself reveals two peaks, at ρp∼0.4ρ and ∼0.7ρ. Comparisons to planetary models find that the low-density group are gas-rich sub-Neptunes, while the group at ρp∼0.7ρ likely consists of volatile-rich water worlds.

    Fábio Wanderley, Katia Cunha, Verne V. Smith, Diogo Souto, Ilaria Pascucci, Aida Behmard, Carlos Allende Prieto, Rachael L. Beaton, Dmitry Bizyaev, Simone Daflon, Sten Hasselquist, Steve Howell, Steven R. Majewski, Marc Pinsonneault

    Comments: Submitted to ApJ
    Subjects: Earth and Planetary Astrophysics (astro-ph.EP); Solar and Stellar Astrophysics (astro-ph.SR)
    Cite as: arXiv:2509.01930 [astro-ph.EP] (or arXiv:2509.01930v1 [astro-ph.EP] for this version)
    https://doi.org/10.48550/arXiv.2509.01930
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    Submission history
    From: Fábio Carneiro Wanderley
    [v1] Tue, 2 Sep 2025 03:56:15 UTC (13,697 KB)
    https://arxiv.org/abs/2509.01930
    Astrobiology,

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  • Searching For Missing Interstellar Oxygen In The Far-infrared

    Searching For Missing Interstellar Oxygen In The Far-infrared

    Efficiency factors of crystalline ice grains with carbon inclusions for grain radii of 1 (red), 2 (blue), 5 (green), and 10 µm (brown). The inclusion fraction is set as 0.1. (a) The solid lines indicate the extinction efficiency factors in the 3 µm region. The scattering and absorption efficiency factors for a 2 µm grain are also shown with the dotted and dashed lines. (b) Absorption efficiency factors in the FIR. The colors are the same as in (a). — astro-ph.EP

    Study of interstellar elemental depletion poses an important problem in the interstellar matter that at least a quarter of the total oxygen (∼160 ppm relative to hydrogen) is not accounted for in any known form of oxygen in the translucent or dense interstellar medium (ISM).

    Detailed analysis of the absorption feature of water ice at 3 μm suggests that one fifth of the missing oxygen may reside in 3 μm-sized water ice grains. However, the 3 μm feature becomes complex and weak for grains larger than 3 μm, and thus the NIR spectroscopy is not the best means to study the presence of large ice grains reliably.

    Here we show that sensitive observations of the far-infrared (FIR) features of water ice at 44 and 62 μm enable us to constrain the amount of crystalline water ice grains up to 5 μm or even larger sizes unambiguously. Oxygen is one of the key elements in the ISM chemistry, and [O I] 63 μm is a dominant cooling line in the neutral ISM. Understanding the actual form of the missing oxygen in the ISM is crucial for the study of the ISM and star-formation process.

    To detect the FIR features of the crystalline water ice over the expected strong continuum, a sensitive FIR spectrograph represented by PRIMA/FIRESS is indispensable. Since the feature is broad, the low spectral resolution of R∼130 is sufficient, but accurate relative calibration better than 1% is required.

    Takashi Onaka, Itsuki Sakon, Takashi Shimonishi, Mitsuhiko Honda

    Comments: This paper is part of the JATIS special issue focused on the PRobe Infrared Mission for Astrophysics (PRIMA) probe mission concept. The issue is edited by Matt Griffin and Naseem Rangwala (JATIS VOL. 11 NO. 3 | July 2025)
    Subjects: Astrophysics of Galaxies (astro-ph.GA); Instrumentation and Methods for Astrophysics (astro-ph.IM)
    Cite as: arXiv:2509.01846 [astro-ph.GA] (or arXiv:2509.01846v1 [astro-ph.GA] for this version)
    https://doi.org/10.48550/arXiv.2509.01846
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    Journal reference: Journal of Astronomical Telescopes, Instruments, and Systems, 11, 031602 (2025)
    Related DOI:
    https://doi.org/10.1117/1.JATIS.11.3.031602
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    Submission history
    From: Takashi Onaka
    [v1] Tue, 2 Sep 2025 00:08:09 UTC (405 KB)
    https://arxiv.org/abs/2509.01846
    Astrobiology,

    Explorers Club Fellow, ex-NASA Space Station Payload manager/space biologist, Away Teams, Journalist, Lapsed climber, Synaesthete, Na’Vi-Jedi-Freman-Buddhist-mix, ASL, Devon Island and Everest Base Camp veteran, (he/him) 🖖🏻

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  • Partnership Between Algae And Bacteria Reveals Secrets Of Evolution

    Partnership Between Algae And Bacteria Reveals Secrets Of Evolution

    Chain of the symbiotic diatom with its N2 fixing cyanobacterial symbiont. In the brightfield (top) the symbiont is inconspicuous inside the host, whereas with epi-fluorescence (bottom) the filaments of the symbionts (arrows) are easily distinguished. Credit Images by Dr. Vesna Grujcic.

    The microscopic alliance between algae and bacteria offers rare, step-by-step snapshots of how bacteria lose genes and adapt to increasing host dependence. This is shown by a new study led by researchers from Stockholm University, in collaboration with the Swedish University of Agricultural Sciences and Linnaeus University, published in Current Biology.

    In some of the most nutrient-poor waters of our oceans, tiny partnerships are hard at work keeping life going. These partnerships, called symbioses, are between microscopic algae known as diatoms and a specific bacteria called cyanobacteria that can take nitrogen from the air and convert it into a form that living things can use.

    In some of these symbioses, the cyanobacteria belong to the genus Richelia, and their main role is to supply nitrogen to their diatom hosts. The diatom hosts are highly active photosynthesizers. Photosynthesis is the metabolic process common to all plants, algae, and some bacteria which use sunlight energy to reduce carbon dioxide (CO2) into chemical energy, usually in the form of sugars.

    A continuum of integration

    How the Richelia physically interact with their diatom hosts vary widely. Some Richelia live attached to the outside of their host, others live in the space between the diatom’s outer cell wall (called a frustule) and inner cell membrane, and some live fully inside. This “continuum” of integration reflects different stages of the partnerships and provides researchers with a unique opportunity to examine the evolutionary process at these different time points of their relationship.

    “In general, as symbionts become more dependent on their hosts, they become more integrated into the host, for example, live inside the host cell, and start to lose genomic information that is redundant with their hosts,” explains co-author, Professor Rachel Foster at Stockholm University.

    Genomes in transition

    Using a comparative genomics approach, postdoctoral researcher Dr. Vesna Grujcic identified that several genomic features of the different Richelia reflect key transitional stages in the evolutionary process.

    “As Richelia become more dependent to their hosts, the set of genes they carry changes a lot. We can see which genes disappear and which stay – giving us a rare view of how these partnerships evolve step by step. Moreover, by comparing Richelia to other nitrogen-fixing cyanobacterial symbionts, we found both shared patterns of gene loss and unique changes that reflect each lineage’s evolutionary path,” says Vesna Grujcic.

    “What excites me most with this research is that different steps on the way to a fully integrated symbiont exist at the same time. This allowed us to study the genetics behind how evolution towards a lifestyle characterized by complete dependence of the symbiont on its host happened,” says Daniel Lundin, from Linnaeus University.

    Grujcic led the pangenome analysis, identifying the set of genes shared by all Richelia (the core genome) as well as the accessory genes that differ between species. Together with Maliheh Mehrshad from the Swedish University of Agricultural Sciences, Grujcic also examined patterns of genome reduction, the size and distribution of spaces between genes known as intergenic spacers, and the extent of pseudogenization – when genes accumulate mutations and lose their function.

    “The level of integration between Richelia and their hosts affects not only genome size and gene content, but also the proportion of coding regions – the parts of DNA that carry instructions for making proteins. Looking at the non-coding DNA, such as the intergenic spacers and broken genes that no longer work (pseudogenes), also tells us a lot about their evolutionary journey,” says Maliheh Mehrshad.

    Coding and noncoding fractions reflect genome degradation stages in Richelia symbionts
    Genome statistics were calculated for the four Richelia genomes derived from the cultures and ten MAGs (Figure 2; Table S1; Figure S1). There is a direct correlation between genome size and GC content in the Richelia spp.: endobionts possess smaller genomes and lower GC content (3.39 Mb ± 0.34 and 34.03% ± 0.88%) compared with periplasmic symbionts (5.17 Mb ± 0.78 and 39% ± 0.07%) and the epibiont (5.98 Mb and 40%) (Figure 2A; Table S1). The number and percentage of coding sequences (CDSs) follows a similar trend where genomes of endobionts have fewer CDSs (2,038 ± 175; 56% ± 4.81%) compared with periplasmic symbionts (6,029 ± 1,548; 67% ± 1.50%) and the epibiont (4,954; 76.09%) (Figures 2B, 2C, and S1A; Table S1).

    The role of ‘jumping genes’

    Another interesting result came from the work of the researcher Theo Vigil-Stenman, a former postdoc at Stockholm University, who characterized all the insertion sequences and transposons – pieces of DNA known as “jumping genes” because they can move genetic information within the genome.

    The researchers had earlier noticed that the genome of the partially integrated symbiont which lives wedged between the outer cell wall of the diatom and the inner cell membrane, only had a slightly smaller genome than the symbiont that attaches to the outside of the host diatom and was missing similar metabolic pathways as the most internal symbiont. Typically, genome size decreases as symbionts become more integrated, or live further inside their respective hosts.

    “We didn’t understand why it could maintain this genome size despite lacking several functional metabolic pathways,” reflects Foster. ”Theo Vigil-Stenman identified that these partially integrated symbiont genomes were full of insertion sequences which inflated their genome size.”

    A model for studying evolution in action

    The research group suggest that these diatom-Richelia symbioses represent a valuable model for studying symbiont genome evolution. The work offers a unique glimpse into evolution in action, as there are few known examples of symbioses caught in transitional stages. Such comparative analysis is rare among planktonic systems and places the diatom–Richelia partnership alongside other notable models of symbiosis.

    Much remains however to learn about how living in symbioses has impacted the evolutionary trajectory of the host diatom genomes and how such models of N2 fixing symbioses can be used in other fields. For example, can such systems lend valuable insights to synthetic biology for making N2-fixing crops?

    Stepwise genome evolution from a facultative symbiont to an endosymbiont in the N2-fixing diatom-Richelia symbioses, current biology

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  • Complete brain activity map revealed for the first time in mice – Neurology

    Complete brain activity map revealed for the first time in mice – Neurology

    The first complete activity map of the brain has been unveiled by a large international collaboration of neuroscientists including at UCLA Health. 

    The International Brain Laboratory (IBL) researchers published their findings today in two papers in Nature, revealing insights into how decision-making unfolds across the entire brain in mice at the resolution of single cells. This brain-wide activity map challenges the traditional hierarchical view of information processing in the brain and shows that decision-making is distributed across many regions in a highly coordinated way.

    “This is the first time anyone has produced a full, brain-wide map of the activity of single neurons during decision-making. The scale is unprecedented as we recorded from over half a million neurons across mice in 12 labs, covering 279 brain areas, which together represent 95% of the mouse brain volume. The decision-making activity, and particularly reward, lit up the brain like a Christmas tree,” explained Professor Alexandre Pouget, Co-Founder of IBL and Group Leader at the University of Geneva.

    Brain-wide map showing 75,000 analysed neurons lighting up during different stages of decision-making. Credit: International Brain Laboratory

    The brain map was made possible by a major international collaboration of neuroscientists from multiple universities across Europe and the US. Officially launched in 2017, IBL introduced a new model of collaboration in neuroscience that uses a standardized set of tools and data processing pipelines shared across multiple labs, ensuring data reproducibility. This visionary approach, supported by Wellcome and the Simons Foundation, draws inspiration from large-scale collaborations in physics and biology, such as CERN and the Human Genome Project.

    “We’d seen how successful large-scale collaborations in physics had been at tackling questions no single lab could answer, and we wanted to try that same approach in neuroscience. The brain is the most complex structure we know of in the universe and understanding how it drives behavior requires international collaboration on a scale that matches that complexity,” commented Professor Tom Mrsic-Flogel, Director of the Sainsbury Wellcome Centre at UCL and one of the core members of IBL.

    Researchers across 12 labs used state-of-the-art electrodes for simultaneous neural recordings, called Neuropixels probes, to measure brain activity while mice were carrying out a decision-making task. In the task, a mouse sits in front of a screen and a light appears on the left or right side. The mouse then responds by moving a small wheel in the appropriate direction to receive a reward. 

    However, in some trials, the light is so faint that the animal must guess which way to turn the wheel. The mouse uses how often the light has appeared on the left or right previously to help them make this guess. These challenging trials therefore allowed the researchers to study how prior expectations influence perception and decision-making. 

    The first paper, “A brain-wide map of neural activity during complex behaviour,” showed that decision-making signals are surprisingly distributed across the brain, not localized to specific regions. This adds to a growing number of studies that challenge the traditional hierarchical model of brain function and emphasizes that there is constant communication across brain areas during decision-making, movement onset, and even reward. This brain-wide activity means that neuroscientists will need to take a more holistic, brain-wide approach when studying complex behaviors in future.

    The second paper, “Brain-wide representations of prior information,” showed that prior expectations, our beliefs about what is likely to happen based on our recent experience, are encoded throughout the brain. Surprisingly, these expectations are not only found in cognitive areas, but also brain areas that process sensory information and control actions. For example, expectations are even encoded in early sensory areas such as the thalamus, the brain’s first relay for visual input from the eye. This supports the view that the brain acts as a prediction machine, but with expectations encoded across multiple brain structures playing a central role in guiding behavior responses. These findings could have implications for understanding conditions such as schizophrenia and autism, which are thought to be caused by differences in the way expectations are updated in the brain. 

    “The efforts of our collaboration generated fundamental insights about the brain-wide circuits that support complex cognition; this is really exciting and a major step forward relative to the “piecemeal” approach (1-2 brain areas at a time) that was previously the accepted method in the field. Moreover, our team took rigor and reproducibility very seriously. We developed an entire task force that leveraged our unique, multi-lab approach to determine the extent to which our efforts at standardization enhanced reproducibility. My hope going forward is that both our scientific discoveries and our new insights on reproducibility will have an impact in the field,” commented Dr. Anne Churchland, professor of Neurobiology at the University of California, Los Angeles (UCLA) and one of the core members of IBL.

    “Traditionally, neuroscience has looked at brain regions in isolation. Recording the whole brain means we now have an opportunity to understand how all the pieces fit together. This was too big of a project for any one lab, and a collaboration on this scale was only possible because of the dedication and talent of our staff scientists, who are the best in the business,” commented Dr Kenneth Harris, Professor of Quantitative Neuroscience at UCL and one of the core members of IBL.

    “It’s immensely gratifying to see the IBL deliver the first brain-wide map of neural activity with such high spatial and temporal resolution. The map describes the activity of over 650,000 individual neurons with single-spike resolution. This activity underlies the brain’s sensory and motor activity that constitutes a decision. The map is a fantastic resource that is already being mined by myriad scientists, and yielding unexpected discoveries. It’s a great success for team science and open science,” commented Dr Matteo Carandini, Professor of Visual Neuroscience at UCL and one of the core members of IBL.

    Looking ahead, the team at IBL plan to expand beyond their initial focus on decision-making to explore a broader range of neuroscience questions. With renewed funding in hand, IBL aims to expand its research scope and continue to support large-scale, standardized experiments. As per the IBL model, it will continue to share its tools, data pipelines and platforms with the global scientific community to democratize and accelerate science and enhance data reproducibility.

    “The brain-wide map is undoubtedly an impressive achievement, but it marks a beginning, not the grand finale. The IBL has shown how a global team of scientists can unite, pushing each other beyond comfort zones into uncharted territories no single lab could reach alone. For me, working within the IBL meant constantly confronting the limits of my own knowledge while learning from the extraordinary expertise of colleagues. The IBL has set the highest standards for sharing high-quality data, tools, and resources to accelerate scientific progress. Now, the next horizon is to extend this collective expertise to the entire community. We envision diverse groups of scientists joining IBL to pursue their own projects, leveraging the unique expertise of the IBL staff and benefiting from the open exchange of data and ideas that only large-scale collaboration can offer,” commented Tatiana Engel, Associate Professor at Princeton University and one of the core members of IBL.

    All data from these studies, along with detailed specifications of the tools and protocols used for data collection, are openly accessible to the neuroscience community for further analysis and research. Summaries of these resources can be viewed and downloaded on the IBL website under the sections: DataToolsProtocols

    This research was supported by grants from Wellcome (209558 and 216324), the Simons Foundation, The National Institutes of Health (NIH U19NS12371601), the National Science Foundation (NSF 1707398), the Gatsby Charitable Foundation (GAT3708), and by the Max Planck Society and the Humboldt Foundation.

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    Read the full papers in Nature

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  • From 370 Million Miles Away, NASA Heats Up a Spacecraft’s Camera to Fix It

    From 370 Million Miles Away, NASA Heats Up a Spacecraft’s Camera to Fix It

    How do you revive an unreliable camera aboard a spacecraft 370 million miles from Earth? Give it the equivalent of a swift whack — or what NASA calls a “thermal kick.”

    This remote-controlled procedure was performed on the Juno spacecraft’s JunoCam before it made a critical flyby of Jupiter’s volcanic moon, Io.

    Jupiter’s Hellish Radiation Belts

    Jupiter is surrounded by one of the most intense radiation belts in the universe. Spacecraft like Juno, which has been orbiting the gas giant since 2016, are constantly bombarded by energetic particles that can fry even the most radiation-hardened electronics.

    Fortunately, NASA equipped Juno’s critical systems with a protective titanium radiation vault — save for one key instrument outside this shielding, the JunoCam.

    A New Tool in NASA’s Toolbox

    The camera was expected to survive eight orbits, but it managed to hold on for over 45 orbits before showing signs of degradation. By orbit 56, its images were corrupted by streaks and noise, courtesy of a radiation-fried voltage regulator.

    Due to the probe’s distance from Earth, traditional repair was out of the question. Instead, NASA’s engineers came up with an unconventional solution widely used in metallurgy: annealing. NASA first commanded JunoCam’s heater to raise its temperature to 77°F and then to the max. What followed was a waiting game.

    “On-the-Fly” Deep Space Repairs

    The gamble eventually paid off, with the JunoCam sending factory-fresh images of Io’s towering sulfur dioxide-coated mountains and active volcanic fields, proving that even delicate, radiation-damaged components can be resurrected through remote-controlled annealing.

    As Juno’s principal investigator, Scott Bolton, puts it, thermal annealing has given them a new tool in their toolbox. It could extend the lifespan of billion-dollar interplanetary missions as well as safeguard military and commercial satellites in Earth orbit.

    Image credit: Vadim Sadovski/Shutterstock

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  • How a fracturing supercontinent forged rare volcanic rocks

    How a fracturing supercontinent forged rare volcanic rocks

    To the untrailed eye, a rock on the side of the road is just that: a lowly rock. To geologists, they are time capsules chock full of data from some of our planet’s most turbulent days. Now, scientists are unraveling a dramatic story secreted away in rare, roughly 800 million-year-old volcanic rocks called carbonatites. Uncovered deep within central Australia, these seemingly unremarkable rocks are telling geologists about a time when continents ripped violently apart.

    Core samples and isotope-dating of the metal-rich carbonatites recently discovered in Australia’s Northern Territory indicate that the rocks traveled near the Earth’s surface between 830 and 820 million years ago. During this time, the ancient supercontinent Rodinia was breaking apart. Rodinia incorporated almost all of Earth’s landmasses for about 450 million years during the Proterozoic Eon (2.5 billion to 541 million years ago), over a billion years before the last supercontinent, Pangaea, formed.

    As tectonic plates ripped apart Rodinia about one billion years ago, magma rose up from the Earth’s shifting mantle. Eventually, that magma cooled, crystalized, and solidified creating these rare Australian carbonatites.

    “This tectonic setting allowed carbonatite magma to rise through fault zones that had remained open and active for hundreds of millions of years, delivering metal-rich melts from deep in the mantle up into the crust,” study University of Göttingen geochemist Maximilian Dröllner explained in a statement. In other words, these rocks are likely straight from the Earth’s deep middle layer. Dröllner is also the co-author of a recent study published in the journal Geological Magazine that describes the rocks.

    Magma or lava-made rocks, known as igneous rocks, are common across the world. But carbonites like these are few and far between.

    “Carbonatites are rare igneous rocks known to host major global deposits of critical metals such as niobium and rare earth elements,” added study co-author and geologist Chris Kirkland. “But determining when and how they formed has historically been difficult due to their complex geological histories.”

    Cathodoluminescence images of selected zircon grains from various samples, illustrating different degrees of primary structure modification. CREDIT: Dröllner et al. 2025.

    To unlock their stories, the team used high-resolution imaging to reconstruct over 500 million years of geological events that the rocks experienced. With this approach, the team pinpointed that the carbonatites formed 830 and 820 million years ago. The imaging and isotope analysis also helped the team separate when the rocks went through more subtle changes versus the more dramatic events, such as when Rodina was tearing apart and magma shot up to the Earth’s surface.

    These carbonatites also contain one of the world’s oldest deposits of an important metal called niobium. Nobium is a silvery metal that is highly resistant to both heat and corrosion. As such, it is useful for producing high-strength steel and clean energy technologies.

    “These carbonatites are unlike anything previously known in the region and contain important concentrations of niobium, a strategic metal used to make lighter, stronger steel for aircraft, pipelines, and EVs, and a key component in some next-generation battery and superconducting technologies,” said Dröllner.

    The team’s research sheds new light on how these rare, metal-rich magmas can reach Earth’s surface. Even though this carbonatite deposit is billions of years old, it could still play a role in protecting our planet’s future for hundreds of years to come.

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  • Brain tumours in mice grow more slowly when starved of key amino acid

    Brain tumours in mice grow more slowly when starved of key amino acid

    A highly lethal type of brain tumour often steals key nutrients to aid its aggressive growth — a habit that can be exploited to slow the cancer’s spread, scientists have found1.

    Experiments show that many brain tumours called glioblastomas grab serine, a crucial amino acid, from their environment rather than synthesizing it themselves: a metabolic Achilles’ heel. The scientists fed mice with certain kinds of glioblastoma a diet that lacked serine and found that the rodents’ tumours, unable to get their fix the usual way, grew more slowly. The animals also lived longer.

    The paper “represents a big advance in the field”, says Sheila Singh, a neurosurgeon–scientist at McMaster University in Hamilton, Canada, who was not involved with the work. “They’ve actually found a metabolic vulnerability of glioblastoma that can be exploited with a therapeutic strategy.”

    The work was published on 3 September in Nature.

    Ruthless disease

    Glioblastomas invade brain tissue with lightning speed and almost always regrow after treatment, which typically involves surgery and a combination of chemotherapy and radiation. Most people who are diagnosed with this type of cancer survive only 1–2 years.

    Tumours filch sugar and other resources from their hosts. Cancers then use this loot to run their own metabolic pathways — the network of chemical processes that turn food into useful molecules — doing “whatever it takes to grow and grow and grow,” says study co-author Andrew Scott, a cancer neuroscientist at the University of Michigan in Ann Arbor.

    To understand how that strategy works for glioblastomas, the authors of the Nature paper studied eight people who underwent surgery to remove their brain tumours. During surgery, physicians infused the participants with sugar molecules that were labelled with a particular carbon isotope. The researchers then analysed samples of the participants’ tumours and surrounding brain tissue.

    By tracking the isotopes, the team found that some glioblastomas use sugar that is taken from their surroundings to make materials such as the basic ingredients for DNA. This helps tumours to grow wildly.

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  • New catalysis method can generate a library of novel molecules for drug discovery

    New catalysis method can generate a library of novel molecules for drug discovery

    Underpinning these biologically active compounds is the carbon-carbon bond, the backbone of all organic chemistry, holding together biomolecules like proteins and DNA. Understanding how and where to make or break these bonds can yield powerful, novel molecules and compounds.

    There are a number of ways to facilitate reactions that create carbon bond-based structures. Yang’s UCSB team, with counterparts in University of Pittsburgh computational organic chemistry professor Peng Liu’s research group, propose a combinatorial process that uses enzymes and sunlight-harvesting catalysts to produce novel molecular scaffolds with rich and well-defined stereochemistry, or 3D shapes.

    “Enzymes are nature’s privileged catalysts,” Yang said. Having evolved alongside their substrates over vast timescales, enzymes are generally powerful, efficient and specific with the molecules they work upon. However, these natural catalysts work on only a select number of substrates under certain conditions. Synthetic catalysts, meanwhile, can be broad and diverse, and function under a wide range of conditions but are not as efficient and as selective as enzymes.

    The method seeks to leverage the best of both worlds: the efficiency and selectivity of enzymes with the versatility of synthetic catalysts. In a process of concerted chemical reactions, the photocatalytic reaction generates reactive species that participate in the larger enzymatic catalysis cycle to ultimately produce six novel products via carbon-carbon bond formation with outstanding enzymatic control.

    “Through enzyme-photocatalyst cooperativity, using a radical mechanism, we developed novel multicomponent biocatalytic reactions which were both unknown in chemistry and biology,” Yang said. “These enzymes are surprisingly general and can function on a wide range of substrates. This allowed us to carry out one of the most complex multicomponent enzymatic reactions my team has developed.”

    Research in this project was also conducted by Chen Zhang, Jun Zhou and Silvia M. Rivera at UCSB; Pei-Pei Xie and Turki M. Alturaifi at the University of Pittsburgh; and collaborators James Finnegan and Simon Charnock at Prozimix Ltd. in the UK.

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  • Earth’s core has ‘reversed’ its rotation. What does that mean for us?

    Earth’s core has ‘reversed’ its rotation. What does that mean for us?

    This article originally appeared on our sister publication PC-WELT and was translated and localized from German.

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