Category: 7. Science

  • Peering Into a Starburst Galaxy With the JWST

    Peering Into a Starburst Galaxy With the JWST

    When it comes to star formation, not all galaxies are the same. Some are quenched, meaning they’ve depleted their star forming gas and form very few new stars. Some, like the Milky Way, are typical and form stars at an average rate. But some are extremely active, and form stars so readily they’re called starburst galaxies.

    Starburst galaxies experience episodes of pronounced star formation, where stellar superclusters containing 100,000 stars or more are born in the hundreds. These galaxies can form hundreds or even thousands of solar masses in stars each year. As a result, they’re extremely luminous, and can be brighter than the Sun by trillions of times in the infrared.

    The Cigar Galaxy (M82) is one of these starburst galaxies, and while its extreme luminosity is not apparent in optical light due to dust, the JWST can easily observe the galaxy’s abundant star formation in infrared.

    The JWST captured this image of M82 in shorter wavelengths with its NIRCam instrument. Some of the bright point sources are super star clusters that can contain 100,000 stars, and the Hubble identified about 200 of them in the galaxy. Astronomers use data in images like this to determine the galaxy’s star formation rate. Image Credit: NASA, ESA, CSA, STScI, A. Bolatto (UMD)

    Superclusters in M82 are responsible for much of the galaxy’s heightened luminosity. With around 100,000 stars, some of them have more stars than some globular clusters do.

    This image from a 2024 paper shows some of the superclusters in M82. Image Credit: Levy et al. 2024. ApJ. DOI 10.3847/2041-8213/ad7af3 This image from a 2024 paper shows some of the superclusters in M82. Image Credit: Levy et al. 2024. ApJ. DOI 10.3847/2041-8213/ad7af3

    Galaxies need abundant gas to become starburst galaxies, and M82 likely got an injection of gas by interacting gravitationally with its neighbor M81. The pair are orbiting one another about once every 100 million years. Those interactions have deformed M82 into its elongated cigar shape, and also sent gas from M82’s outer regions into its core, fueling its abundant star formation.

    M81 (left) and M82 (right) interact gravitationally and orbit one another once every 100 million years or so. The interactions have stretched the smaller M82 into a cigar shape, leading to its nickname, the Cigar Galaxy. The interactions are also triggering starburst episodes, evidenced by the filaments of red hydrogen gas. Image Credit: T.A. Rector (University of Alaska Anchorage) and NOIRLab/NSF/AURA/ M81 (left) and M82 (right) interact gravitationally and orbit one another once every 100 million years or so. The interactions have stretched the smaller M82 into a cigar shape, giving it the nickname the Cigar Galaxy. The interactions are also triggering starburst episodes, evidenced by the filaments of red hydrogen gas. Image Credit: T.A. Rector (University of Alaska Anchorage) and NOIRLab/NSF/AURA/

    Astronomers are interested in M82 and its neighbor because they’re like a laboratory for watching galaxy interactions. A 2024 paper used polycyclic aromatic hydrocarbon (PAH) emissions to reveal an intricate web of filaments and bubbles of gas created by supernovae. They also revealed M82’s galactic outflow. These outflows are another prominent feature of starburst galaxies.

    The leading JWST image also traces PAHs and they show the galactic outflows. They’re visible as elongated bright streaks emanating from the galactic center. PAHs are important in astronomy because they have strong emission features in the mid-infrared. They’re strongly correlated with cold molecular gas and help trace the movement of the gas.

    The leading JWST image clearly shows the galactic outflow winds from the galaxy's center. They're driven by the abundant formation of massive stars, and by supernova explosions. Image Credit: ESA/Webb, NASA & CSA, A. Bolatto. License: CC BY 4.0 INT The leading JWST image clearly shows the galactic outflow winds from the galaxy’s center. They’re driven by the abundant formation of massive stars, and by supernova explosions. Image Credit: ESA/Webb, NASA & CSA, A. Bolatto. License: CC BY 4.0 INT

    The outflows are created by the galaxy’s abundant star formation. The starburst activity produces thousands of stars much hotter and more massive than our Sun. These stars generate powerful stellar winds that drive gas away. Many of these stars will explode as supernovae, which also drives gas away. For these reasons, starburst galaxies don’t experience extreme star formation for much longer than about 100 million years before their gas supply is dissipated.

    However, M82 might be different. Due to repeated gravitational interactions with M81 in the future, M82 may go through cycles of abundant star formation and quenching. Astronomers think this has happened in the past. About 600 million years ago, it underwent a starburst phase, and the current phase was likely triggered between about 30 and 60 million years ago.

    M82 is only about 12 million light-years away, close for a galaxy. As a result, astronomers have focused a lot of attention on the starburst galaxy. It has been imaged repeatedly by the Hubble and other telescopes.

    Hubble captured this brilliant image of M82 that highlights the filaments of wind-borne gas in red. Image Credit: NASA, ESA and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI) and P. Puxley (National Science Foundation) Hubble captured this brilliant image of M82 that highlights the filaments of wind-borne gas in red. Image Credit: NASA, ESA and the Hubble Heritage Team (STScI/AURA); Acknowledgment: J. Gallagher (University of Wisconsin), M. Mountain (STScI) and P. Puxley (National Science Foundation)

    M82 will undergo many more starburst cycles in its future. But eventually, M82 and M81 will merge into one galaxy. That merger, in the far distant future, will likely trigger one massive, chaotic starburst event. Eventually that, too, will die down, and the resulting massive galaxy will settle into a quiet state.

    Continue Reading

  • Astronomers Discover Third-Ever Interstellar Object: 3I/ATLAS

    Astronomers Discover Third-Ever Interstellar Object: 3I/ATLAS

    After the interstellar asteroid 1I/ʻOumuamua and the interstellar comet 2I/Borisov, 3I/ATLAS is the third object and the second comet from outside the Solar System confirmed.

    This image, taken with the iTelescope.Net T72 telescope at Rio Hurtado, Chile, on July 2, 2025, shows the interstellar comet 3I/ATLAS. Image credit: Filipp Romanov / CC BY-SA 4.0.

    3I/ATLAS was discovered by the NASA-funded ATLAS (Asteroid Terrestrial-impact Last Alert System) survey telescope in Rio Hurtado, Chile, on July 1, 2025.

    Arriving from the direction of the constellation Sagittarius, the interstellar comet is currently located about 670 million km (420 million miles) away.

    “Since that first report, observations from before the discovery have been gathered from the archives of three different ATLAS telescopes around the world and the Zwicky Transient Facility at the Palomar Observatory in San Diego County, California,” NASA astronomers wrote in a statement.

    “These ‘pre-discovery’ observations extend back to June 14, 2025.”

    Also known as C/2025 N1 (ATLAS) and A11pl3Z, 3I/ATLAS is currently about 4.5 AU (670 million km, or 416 million miles) from the Sun.

    The comet poses no threat to Earth and will remain at a distance of at least 1.6 AU (240 million km, or 150 million miles).

    It will reach its closest approach to the Sun around October 30, 2025, at a distance of 1.4 AU (210 million km, or 130 million miles) — just inside the orbit of Mars.

    Its size and physical properties are being investigated by astronomers around the world.

    This diagram shows the trajectory of 3I/ATLAS as it passes through the Solar System. Image credit: NASA / JPL-Caltech.

    This diagram shows the trajectory of 3I/ATLAS as it passes through the Solar System. Image credit: NASA / JPL-Caltech.

    “If 3I/ATLAS’s brightness stems from reflecting sunlight at the typical albedo of order 10%, then its diameter of 20 km is about 100-200 times larger than the estimated length of ‘Oumuamua (and over a thousand times larger than ‘Oumuamua’s width) and about 50-100 times larger than the core of the comet Borisov,” Professor Avi Loeb, the head of the Galileo Project, founding director of Harvard University’s Black Hole Initiative, and director of the Institute for Theory and Computation at the Harvard-Smithsonian Center for Astrophysics, wrote in his blog.

    “If all three objects are rocks, then 3I/ATLAS’s mass is over ten million times larger than that of ‘Oumumua and at least a hundred thousand times larger than the core mass of Borisov.”

    “This is surprising because one expects high mass objects to be much rarer.”

    “Based on data about the main asteroid belt in the Solar System, one would expect millions of objects like ‘Oumuamua for each object on the mass scale of 3I/ATLAS.”

    3I/ATLAS should remain visible to ground-based telescopes through September 2025, after which it will pass too close to the Sun to observe.

    It is expected to reappear on the other side of the Sun by early December, allowing for renewed observations.

    “Based on its direction of motion, 3I/ATLAS appears to be coming at a retrograde orbit with an inclination of 175 degrees relative to the Earth’s orbital plane from the thin disk of stars in the Milky Way Galaxy,” Professor Loeb wrote.

    “In the coming months, we will learn much more about 3I/ATLAS’s properties based on data from multiple ground-based telescopes including the NSF/DoE Vera C. Rubin Observatory in Chile, as well as possibly from the NASA/ESA/CSA James Webb Space Telescope.”

    Continue Reading

  • Silent witnesses: corals pinpoint the start of deforestation in Borneo

    Silent witnesses: corals pinpoint the start of deforestation in Borneo

    image: 

    Massive coral in the Miri-Sibuti Coral Reef National Park.


    view more 

    Credit: Walid Naciri

    University of Leicester-led research has revealed the start of industrial deforestation of the Malaysian rainforest and its long-lasting impact on coastal ecosystems in the skeletons of corals.

    Published in Scientific Reports, they used coral cores obtained off the coast of Borneo in Southeast Asia to pinpoint the beginning of industrial deforestation and demonstrate the impact on marine ecosystems.

    The study brought together researchers from the UK, Malaysia, and Australia, including Professor Jens Zinke, Dr Arnoud Boom, and former Leicester PhD student Walid Naciri, from the University’s School of Geography, Geology and the Environment. The work was supported by a Royal Society Wolfson Fellowship awarded to Professor Zinke, and a PhD scholarship.. It builds upon the conclusions from a previously published pilot study where corals were found to be useful archives of past deforestation-induced sediment discharge.

    A solution to data scarcity

    Massive corals such as the ones used in this study can be used to fill gaps in environmental data, thanks to their ability to absorb a variety of trace elements found in surrounding seawater into their calcium carbonate skeleton during their growth. The measurement of these trace elements can then be linked to environmental conditions such as temperature, sediment, and hydrology.

    Lessons from the past

    Professor Zinke and former PhD student Hedwig Krawczyk, in association with local and international collaborators at Curtin University in Miri (Malaysia) and Perth (Australia), sampled coral cores using underwater pneumatic drills and obtained several metre-long cores from multiple coral colonies located at different distances from the main river mouth flowing into the coastal coral reef ecosystem, Miri-Sibuti Coral Reef National Park.

    During the COVID-19 pandemic, coral cores were sent to the John de Laeter Centre within Curtin University in Perth, Australia, for trace element analyses using a laser ablation inductively coupled mass spectrometer. Walid Naciri performed some analyses in collaboration with Kai Rankenburg while visiting in 2022, with the resulting data processed and analysed in Leicester.

    Professor Zinke, who led the project, explained: “The laser analysis focused on the ratio of trace elements barium and calcium (Ba/Ca) locked in coral skeletons because Ba is released from fine mud particles in river water once the river meets the salty ocean water. We use the coral Ba/Ca ratio as a proxy for sediment erosion long before any instrument was able to build a record.”

    Results of 100-year-long Ba/Ca records showed that sediment concentrations in surrounding reef waters remained low from the beginning to the middle of the 20th century. After 1950, records show an increase in Ba/Ca indicative of an increase in sediment discharge, which is linked with decreasing soil stability due to the start of industrial deforestation leading to enhanced soil erosion.

    Traces of organic carbon dissolved in river waters are now being studied by Leicester PhD student Hannah Kingsland to better understand interactions between tropical land and coastal ecosystems.

    Corals reveal long-lasting consequences of deforestation

    Former PhD student at Leicester Walid Naciri added: “Our findings allow us to make several conclusions: deforestation has an impact on the adjacent coastal system because Ba/Ca records show increasing trends, knowing pre-deforestation baseline conditions helped us to understand its impact, industrial deforestation started impacting coastal ecosystems around 1950, and assessments of deforestation impacts need to include all affected land-ocean ecosystems.

    “This study provides further motivation that local governments must strive to reduce deforestation by proposing alternative means of income for local populations while the global community eases demand on palm oil and pulpwood. These initiatives must be accompanied by tropical forest restoration in an effort to reduce sediment discharge, restore crucial ecosystems, and increase carbon uptake.”

    Dr Arnoud Boom, from the University of Leicester School of Geography, Geology and the Environment, said: “We have literally found a fingerprint for the onset and impact of industrial deforestation that led to enhanced soil erosion in Malaysian Borneo, affecting the Miri-Sibuti Coral Reef National Park. And all thanks to the massive corals which lived long enough to provide us with this record.”


    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.

    Continue Reading

  • Mounting case against notion that boys are born better at math — Harvard Gazette

    Mounting case against notion that boys are born better at math — Harvard Gazette

    Twenty years ago, cognitive psychologist Elizabeth Spelke took a strong position in an ongoing public debate.

    “There are no differences in overall intrinsic aptitude for science and mathematics among women and men,” the researcher declared.

    A new paper in the journal Nature, written by Spelke and a team of European researchers, provides what she called “an even stronger basis for that argument.” 

    A French government testing initiative launched in 2018 provided data on the math skills of more than 2.5 million schoolchildren over five years. Analyses showed virtually no gender differences at the start of first grade, when students begin formal math education. However, a gap favoring boys opened after just four months — and kept growing through higher grades.

    The results support previous research findings based on far smaller sample sizes in the U.S. “The headline conclusion is that the gender gap emerges when systematic instruction in mathematics begins,” summarized Spelke, the Marshall L. Berkman Professor of Psychology.

    Back in 2005, her position was informed by decades of work studying sensitivity to numbers and geometry in the youngest members of human society. 

    “My argument was, ‘OK, if there really were biological differences, maybe we would see them in the infancy period,’” recalled Spelke, who laid out her evidence in a critical review for the journal American Psychologist that year. 

    “We were always reporting on the gender composition of our studies, as well as the relative performance of boys and girls,” Spelke continued. “But we were never finding any differences favoring either gender over the other.”

    “The fact that there are no differences in infants could be because the abilities that show gender effects actually emerge during preschool.”

    The possibility remained that differences in skill or even motivation surface later in the lifecycle.

    “The fact that there are no differences in infants could be because the abilities that show gender effects actually emerge during preschool,” Spelke said.

    Recent years have found the psychologist applying her research on early counting and numeral-recognition skills via educational interventions, all analyzed and refined through randomized control experiments.

    One of the world’s most influential researchers on early learning, Spelke recently partnered with Esther Duflo, an MIT economics professor and Nobel laureate, to advise the Delhi office of the nonprofit Abdul Latif Jameel Poverty Action Lab (J-PAL). The group is working with the governments of four separate Indian states to develop and test math curricula for preschoolers, kindergartners, and first-graders. 

    Alongside her longtime collaborator, the cognitive neuroscientist Stanislas Dehaene, Spelke also serves as an adviser on the French Ministry of Education’s Scientific Council. The nationwide EvalAide language and math assessment was introduced with the council’s help in 2018. The project’s goal, Spelke explained, is establishing a baseline measure of every French child’s grasp of basic numeracy and literacy skills, while supporting the ministry in its commitment to implementing an evidence-based education for all French schoolchildren.

    Spelke co-authored the Nature paper with Dehaene and eight other researchers, all based in France. Specifically analyzed were four consecutive cohorts of mostly 5- and 6-year-olds entering school between 2018 and 2021. 

    As in many countries, French girls tested slightly ahead of French boys on language as they started first grade in the fall. But the gender gap was close to null when it came to math. 

    “That definitely connects to the earlier issue of whether there’s a biological basis for these differences,” Spelke argued.

    French first-graders were then reassessed after four months of school, when a small but significant math gap had emerged favoring boys. The effect quadrupled by the beginning of second grade, when schoolchildren were tested yet again.

    “It was even bigger in fourth grade,” said Spelke, noting that French children are now assessed at the start of even-number grades. “And in sixth grade it was bigger still.”

    For comparison, EvalAide results show the literacy gender gap was reduced by the first year’s four-month mark and changed far less as students progressed to higher grade levels.

    Why would a gender gap widen on math specifically as students accumulated more time in school? According to Spelke, the paper provides “only negative answers” concerning ideas about innate sex differences and social bias.  

    “If there was really a pervasive social bias, and the parents were susceptible to it,” she said, “we would expect boys to be more oriented toward spatial and numerical tasks when they first got to school.” 

    Delving further into the data yielded more results that caught the researchers’ interest. For starters, Spelke’s co-authors could disaggregate the findings by month of birth, with the oldest French first-graders turning 7 in January — nearly a year before their youngest classmates. The math gap was found to correlate not with age, but with the number of months spent in school. 

    Another noteworthy result concerned the COVID-19 pandemic, which wiped out the last 2.5 months of first grade for children who enrolled in fall 2019. “With less time in school, the amount of the gender gap grew by less than it did in the other years where there wasn’t a long school closure,” Spelke said.

    The 2019 cohort yielded one more striking result. Earlier that year, French schoolkids had placed at the very bottom of 23 European countries on the quadrennial Trends in International Mathematics and Science Study. That sparked a national conversation: How could France, birthplace of the great René Descartes, be trailing its peers in mathematics?

    In May 2019, the French Education Ministry, with the support of its Scientific Council, called for the introduction of more math curriculum during kindergarten. For the first time, an ever-so-slight gender math gap appeared that fall for those entering first grade. It hadn’t been there in 2018 but remained detectable in results from the 2020 and 2021 cohorts.

    The overall results, the most conclusive to date, suggest it’s time to shelve explanations based on biology or bias. Instead, it appears there’s something about early math instruction that produces gender disparities. 

    “We still don’t know what that is exactly,” said Spelke, who plans to spend much of her 2025-26 sabbatical year in France. “But now we have a chance to find out by randomized evaluations of changes to the curriculum.”


    Continue Reading

  • Astrophotographer snaps ‘once-in-a-lifetime’ shot of solar flare photobombing the ISS

    Astrophotographer snaps ‘once-in-a-lifetime’ shot of solar flare photobombing the ISS

    An astrophotographer has captured a stunning shot of a powerful solar flare photobombing the International Space Station (ISS) as the human-inhabited spacecraft appeared to zoom across the surface of our home star.

    Andrew McCarthy (aka Cosmic Background) snapped the incredible image on June 15 from a spot in the Sonoran Desert in Arizona. He was initially planning to photograph a standard “transit” photo of the ISS passing directly between Earth and the sun. However, as McCarthy was setting up his camera, he noticed that one sunspot — dubbed AR4114 — had begun to “flare to life,” he told Live Science.


    Continue Reading

  • NASA Reveals First-Ever Full Image of Peanut-Shaped Asteroid Donaldjohanson

    NASA Reveals First-Ever Full Image of Peanut-Shaped Asteroid Donaldjohanson

    Scientists with NASA’s Lucy mission are finally wrapping up the process of refining the data gathered by the spacecraft’s April 20 encounter with Donaldjohanson, an asteroid in our solar system’s main asteroid belt. And it’s, uh, as peanut-shaped as we first saw it. 

    Earlier this year, Lucy’s Long Range Reconnaissance Imager snapped an image of Donaldjohansson while quickly swooping past it, at a distance of about 600 miles (960 kilometers), with the smallest visible features measuring around 130 feet (40 meters) across—an impressive close-up, considering the overall scale of anything we observe in space. 

    Regrettably, the Sun’s position behind Lucy reduced the contrast of the asteroid’s smaller details. But the close visit is invaluable nevertheless, as it’s allowing scientists to carefully comb over the details of its surface after adjusting for the brightness. 

    A stereo image pair combining the last complete approach image (right) with a slightly clipped image taken 72 seconds later (left). Credit: NASA/Goddard/SwRI/Johns Hopkins APL/Brian May/Claudia Manzoni

    “Asteroid Donaldjohanson has strikingly complicated geology,” said Hal Levison, Lucy’s principal investigator, in an earlier press release about the asteroid. Donaldjohansson likely got its lumpy shape from a cosmic collision between two smaller objects around 150 million years ago. It’s a relatively common shape among smaller asteroids in the solar system, so what we learn from Donaldjohanson could inform our understanding of many other cosmic objects. 

    “As we study the complex structures in detail, they will reveal important information about the building blocks and collisional processes that formed the planets in our Solar System,” Levison added in the same release. 

    Donaldjohansson is not the main objective of the Lucy mission, whose itinerary is set for the eight Trojan asteroids that share Jupiter’s orbit around the Sun. Still, Lucy’s Donaldjohanson encounter—and the November 2023 flyby of asteroid Dinkinesh—is an excellent “dress rehearsal” for Lucy as it continues its journey toward the cooler, outer regions of the solar system, according to NASA’s Erin Morton in a statement earlier this week. 

    Lucy’s next milestone is set to occur in August 2027, when the spacecraft will finally start to explore the Jupiter Trojan asteroids in earnest—starting with Eurybates, a carbonaceous asteroid so big that it has its own satellite, Queta.

    Continue Reading

  • Studying Protoplanets and Protoplanetary Disks with the Habitable Worlds Observatory

    Studying Protoplanets and Protoplanetary Disks with the Habitable Worlds Observatory

    Substructures in protoplanetary disks, such as (a) spiral arms and (b) gaps, can inform the location and mass of protoplanets that shape these substructures (marked with arrows here; e.g., Dong & Fung 2017; Bae et al. 2018). Note: the panels displayed here use simulated data provided by Dong et al. (2015) for (a) and Bi & Lin (2024) for (b). — astro-ph.IM

    Since the discovery of the first exoplanet orbiting a Sun-like star, the confirmation of nearly 6000 exoplanets to date – and their diversity – has revolutionized our knowledge of planetary systems in the past three decades.

    Nevertheless, the majority of these planets are around mature stars (≳1 Gyr), where the planet birth environments have already dissipated. Indeed, we have only confirmed 2 forming planets (i.e., protoplanets; ≲10 Myr) residing in one single system. In comparison, we have imaged over 200 protoplanetary disks in the past decade, with many of them hosting substructures such as spirals and gaps which suggest the existence of protoplanets.

    To understand the early stages of planet formation, the Habitable Worlds Observatory (HWO) – with its high-contrast imaging and integral field spectroscopy capabilities – presents a unique opportunity to explore the demographics of the natal stages of planet formation and their birth environments.

    We propose to image protoplanets within substructured protoplanetary disks using HWO via direct imaging, and characterize them (i.e., protoplanets, protoplanetary disks, circumplanetary disks) using integral field spectroscopy and spectropolarimetry. This effort will dramatically extend current population of protoplanets, probing and characterizing over 200 protoplanets.

    By expanding the number of protoplanets by two orders of magnitude, these observations will test and refine planet formation theory and planet-disk interaction theory, and further motivate planet migration studies together with existing mature planets. The results will offer critical insight into planetary system formation and evolution, and help understand the origin of our own Solar System.

    Bin B. Ren

    Comments: 9 pages, 3 figures, 2 tables. HWO Science Case #SCDD-SSiC-8 for HWO25 proceedings
    Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); Earth and Planetary Astrophysics (astro-ph.EP)
    Cite as: arXiv:2506.24129 [astro-ph.IM] (or arXiv:2506.24129v1 [astro-ph.IM] for this version)
    https://doi.org/10.48550/arXiv.2506.24129
    Focus to learn more
    Submission history
    From: Bin Ren Dr.
    [v1] Mon, 30 Jun 2025 17:59:59 UTC (1,388 KB)
    https://arxiv.org/abs/2506.24129
    Astrobiology,

    Continue Reading

  • Adapting to UV: Integrative Genomic and Structural Analysis in Bacteria from Chilean Extreme Environments

    Adapting to UV: Integrative Genomic and Structural Analysis in Bacteria from Chilean Extreme Environments

    Isolation sites, genomic assembly characteristics, and ANI-based taxonomic assignment of three extremophilic bacterial isolates. (a–c) Representative sampling sites of bacterial isolates: (a) Atacama Desert, (b) Salar de Huasco, and (c) Antarctic soil. (d–f) Circular genome representations illustrating variability in genome size, contiguity, and genetic content: (d) Bacillus velezensis PQ169 (76 contigs, 4.18 Mb), (e) Pseudoalteromonas sp. AMH3-8 (single contig, 4.74 Mb), and (f) Rugamonas violacea T1-13 (171 contigs, 6.85 Mb). Rings (outer to inner) represent predicted CDSs, RNA genes (rRNA, tRNA, and tmRNA), GC content, and GC skew. — Int J Mol Sci via PubMed

    Extremophilic bacteria from extreme environments, such as the Atacama Desert, Salar de Huasco, and Antarctica, exhibit adaptations to intense UV radiation. In this study, we investigated the genomic and structural mechanisms underlying UV resistance in three bacterial isolates identified as Bacillus velezensis PQ169, Pseudoalteromonas sp. AMH3-8, and Rugamonas violacea T1-13.

    Through integrative genomic analyses, we identified key genes involved in DNA-repair systems, pigment production, and spore formation. Phylogenetic analyses of aminoacidic sequences of the nucleotide excision repair (NER) system revealed conserved evolutionary patterns, indicating their essential role across diverse bacterial taxa.

    Structural modeling of photolyases from Pseudoalteromonas sp. AMH3-8 and R. violacea T1-13 provided further insights into protein function and interactions critical for DNA repair and UV resistance. Additionally, the presence of a complete violacein operon in R. violacea T1-13 underscores pigment biosynthesis as a crucial protective mechanism.

    In B. velezensis PQ169, we identified the complete set of genes responsible for sporulation, suggesting that sporulation may represent a key protective strategy employed by this bacterium in response to environmental stress.

    Our comprehensive approach underscores the complexity and diversity of microbial adaptations to UV stress, offering potential biotechnological applications and advancing our understanding of microbial resilience in extreme conditions.

    Phylogenetic tree based on the amino acid sequences of UvrA, UvrB, and UvrC proteins (NER system). Multiple sequence alignment was performed using MUSCLE on the Phylogeny.fr platform, followed by tree construction with PhyML and visualization using TreeDyn. The resulting tree was further arranged and refined using the Interactive Tree of Life (iTOL v7) tool. The maximum likelihood method was employed with 1000 bootstrap replicates, where the node sizes reflect the level of bootstrap support. Each label includes the gene name, the bacterial species, and the corresponding NCBI accession number. Three environmental strains are highlighted: Bacillus velezensis PQ-169 (green), Pseudoalteromonas sp. AMH3-8 (yellow), and Rugamonas violacea T1-13 (purple). These strains, along with other extremophilic, UV-resistant, and pathogenic bacteria, were included to compare UvrA (red clade), UvrB (blue clade), and UvrC (green clade) variations under extreme environmental conditions. — Int J Mol Sci via PubMed

    Isolation sites, genomic assembly characteristics, and ANI-based taxonomic assignment of three extremophilic bacterial isolates. (a–c) Representative sampling sites of bacterial isolates: (a) Atacama Desert, (b) Salar de Huasco, and (c) Antarctic soil. (d–f) Circular genome representations illustrating variability in genome size, contiguity, and genetic content: (d) Bacillus velezensis PQ169 (76 contigs, 4.18 Mb), (e) Pseudoalteromonas sp. AMH3-8 (single contig, 4.74 Mb), and (f) Rugamonas violacea T1-13 (171 contigs, 6.85 Mb). Rings (outer to inner) represent predicted CDSs, RNA genes (rRNA, tRNA, and tmRNA), GC content, and GC skew. (g–i) Heatmaps depicting average nucleotide identity based on MUMmer (ANIm) analysis between each isolate and closely related reference strains, supporting definitive taxonomic assignment: (g) Bacillus velezensis PQ169, (h) Pseudoalteromonas sp. AMH3-8, and (i) Rugamonas violacea T1-13. Color gradients indicate similarity percentages, with red color representing higher ANI values, and blue lower values. — Int J Mol Sci via PubMed

    astrobiology, genomics, extremophiles,

    Continue Reading

  • An Unexpected Mineral Discovered In A Grain Of Asteroid Ryugu – astrobiology.com

    1. An Unexpected Mineral Discovered In A Grain Of Asteroid Ryugu  astrobiology.com
    2. A Fiery Mineral Found in an Icy Asteroid Baffles Scientists  SciTechDaily
    3. Asteroid Ryugu’s Latest Mineral Is As Weird As Finding “A Tropical Seed In The Arctic”  IFLScience
    4. Asteroid Ryugu May Have Experienced Unexpected Heating Events  Labroots
    5. Scientists baffled by discovery of unexpected mineral on asteroid Ryugu  India Today

    Continue Reading

  • A First Look At Rocky Exoplanets With JWST – astrobiology.com

    1. A First Look At Rocky Exoplanets With JWST  astrobiology.com
    2. Likely Saturn-Mass Planet Imaged by NASA Webb Is Lightest Ever Seen  NASA Science (.gov)
    3. James Webb First: Telescope Directly Images Young Saturn-Sized Exoplanet 110 Light-Years Away  Deccan Herald
    4. It’s official—NASA scientists have detected an unknown planet with 100 times the mass of Earth and a temperature that suggests possible habitable conditions  Unión Rayo
    5. “We’re Finally Hunting Aliens for Real”: James Webb Telescope Begins Deep-Space Search for Signs of Extraterrestrial Life  Rude Baguette

    Continue Reading