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Fossils unearthed in China suggest that the End-Permian mass extinction, which wiped out around 80% of life on Earth nearly 252 million years ago, may not have been as catastrophic for plant life. This period, known as the “Great Dying,” saw extreme volcanic activity from the Siberian Traps, leading to drastic increases in carbon dioxide levels, severe global warming, and ocean acidification. While marine ecosystems suffered a near-total collapse, new evidence indicates that some terrestrial plant life endured the crisis. A site in present-day northeastern China has revealed fossilized remains of gymnosperm forests and ferns, pointing to a region where vegetation managed to persist despite the mass extinction event.

Evidence from Rock Layers in Xinjiang

According to a study published in Science Advances, researchers examined rock formations in Xinjiang, China, that date back to the period of the Great Dying. Lead author Wan Yang, a professor of geology and geophysics at Missouri University of Science and Technology, stated in an interview with Live Science that mass plant extinction was not observed in this region. The rock layers contained fossilised spores and pollen, showing a gradual shift in plant species rather than a sudden collapse and regrowth. Yang highlighted that this finding challenges the assumption that land ecosystems suffered the same level of devastation as marine environments during this period.

Climate and Location Played a Role

The research suggests that regions with humid climates and access to water bodies may have served as refuges for plant life. Similar patterns have been observed in South America and Africa, where high-latitude locations appear to have provided more stable conditions for vegetation. Josefina Bodnar, a paleobotanist at the National University of La Plata in Argentina, who was not involved in the study, explained to Live Science that plants possess survival adaptations such as deep-rooted structures and long-lasting seeds, which may have helped them endure extreme conditions.

A Different Impact on Land and Sea

The study also supports the idea that land ecosystems experienced a crisis rather than complete extinction. Robert Gastaldo, an emeritus professor of geology at Colby College, stated that the term “extinction” may not accurately describe what occurred on land. He pointed out that while marine life had no escape from ocean acidification, terrestrial organisms could migrate to more temperate regions or adapt to changing conditions.

Lessons from Earth’s Past

The End-Permian extinction has drawn scientific attention due to its parallels with modern climate change. Research has shown that greenhouse gas emissions from volcanic activity during that time reached levels comparable to those expected from human activity by the end of this century. Devin Hoffman, a researcher at University College London, told Live Science that studying past climate crises could offer insight into the potential long-term impacts of rising atmospheric carbon dioxide levels today. Gastaldo further noted that the geological record serves as a historical account of how extreme environmental shifts have affected life on Earth, providing valuable context for current climate concerns.

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James Webb Space Telescope Reveals Stunning Hourglass Nebula LBN 483 in Unmatched Detail

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James Webb Space Telescope Reveals Stunning Hourglass Nebula LBN 483 in Unmatched Detail

A striking nebula shaped by the dynamic interactions of two young stars has been observed in unprecedented detail by the James Webb Space Telescope (JWST). The structure, identified as Lynds 483 (LBN 483), is located approximately 650 light-years away. The nebula’s intricate shape is a result of powerful outflows generated by the formation of a binary star system. As material from a collapsing molecular cloud feeds these stars, bursts of gas and dust are expelled, shaping the surrounding nebulosity into a striking hourglass-like formation. The interaction of these stellar winds and jets with surrounding matter continues to sculpt the nebula over time, providing valuable insight into the mechanisms of star formation.

Star Formation and Nebular Evolution

According to reports, the two protostars at the core of LBN 483 play a crucial role in shaping the nebula. The presence of a lower-mass companion star, identified in 2022 through observations by the Atacama Large Millimeter/submillimeter Array (ALMA), suggests complex interactions within the system. Material accreted onto the stars periodically fuels energetic outflows, which in turn crash into the surrounding gas and dust. The JWST’s infrared imaging has revealed intricate structures within these lobes, including dense pillars and shock fronts where ejected material meets older expelled gas.

Impact of Magnetic Fields on Nebular Shape

Radio observations from ALMA have detected polarised emissions from cold dust within the nebula. These emissions indicate the presence of a magnetic field, which influences the direction and structure of the outflows. The study highlights a distinct 45-degree kink in the field at a distance of approximately 1,000 astronomical units from the stars. This deviation is attributed to the migration of the secondary star over time, altering the system’s angular momentum and consequently shaping the nebular outflows.

Implications for Star Formation Studies

LBN 483 presents a unique opportunity for astronomers to study star formation outside of massive stellar nurseries such as the Orion Nebula. The nebula’s isolation allows researchers to examine the formation process without interference from external stellar activity. Findings from this study contribute to refining theoretical models of star formation by integrating real observational data into numerical simulations. Scientists continue to analyse such systems to gain a deeper understanding of how stars, including the Sun, evolved from collapsing clouds of gas billions of years ago.

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Microlightning in Water Droplets Could Explain the Origin of Life on Earth

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Microlightning in Water Droplets Could Explain the Origin of Life on Earth

Life on Earth may have emerged not from a single, dramatic lightning strike but through countless tiny electrical discharges occurring in water droplets. Research indicates that microlightning, generated by crashing waves or waterfalls, could have led to the formation of essential organic molecules. Scientists have long debated how life began, with theories suggesting that lightning interacting with early atmospheric gases may have created crucial compounds. However, new findings suggest that small electrical charges produced in water spray could have played a key role in the process, offering an alternative explanation to the widely known Miller-Urey hypothesis.

Organic Molecules Formed Without External Electricity

According to the study published in Science Advances, water droplets subjected to a mixture of gases believed to be present in Earth’s early atmosphere resulted in the formation of organic molecules. The research, led by Richard Zare, the Marguerite Blake Wilbur Professor of Natural Science at Stanford University, explored how water spray generated electrical charges capable of forming carbon-nitrogen bonds—essential for life. Postdoctoral scholars Yifan Meng and Yu Xia, along with graduate student Jinheng Xu, contributed to the study, which challenges the idea that lightning strikes were necessary to initiate the chemical reactions leading to life.

Microlightning and Chemical Reactions in Water Droplets

The research team discovered that water droplets of varying sizes developed opposite electrical charges when dispersed. Larger droplets typically carried a positive charge, while smaller ones were negatively charged. When these oppositely charged droplets came into proximity, tiny electrical sparks—termed “microlightning” by Zare—were observed. These discharges were captured using high-speed cameras, revealing flashes of energy powerful enough to drive chemical reactions.

When room-temperature water was sprayed into a gas mixture containing nitrogen, methane, carbon dioxide, and ammonia—compounds believed to be abundant on early Earth—organic molecules such as hydrogen cyanide, glycine, and uracil were produced. These findings suggest that microlightning from water droplets may have contributed significantly to the formation of life’s building blocks, without the need for large-scale lightning strikes.

A New Perspective on Life’s Origins

Zare stated in Tech Explore that water droplets in constant motion—whether crashing into rocks or dispersing into the air—could have repeatedly generated these microelectric discharges. This mechanism, he explained, may resolve challenges associated with the Miller-Urey hypothesis, which has been criticised for its reliance on infrequent lightning events over vast oceans.

Beyond its implications for the origins of life, the study also aligns with previous research from Zare’s team on the reactivity of water droplets. Prior investigations have demonstrated how divided water can spontaneously generate hydrogen peroxide and contribute to ammonia production. He emphasised that while water is often perceived as chemically passive, when broken into tiny droplets, it becomes highly reactive, capable of driving significant chemical transformations.

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NASA’s Space Station Research Aids Lunar Missions With Key Technologies

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NASA’s Space Station Research Aids Lunar Missions With Key Technologies

Scientific research aboard the International Space Station continues to contribute to lunar exploration, with recent experiments supporting advancements in space weather studies, navigation, and radiation-resistant computing. Firefly Aerospace’s Blue Ghost Mission-1 successfully landed on the Moon on 2 March 2025, carrying three experiments influenced by space station research. These include the Lunar Environment Heliospheric X-ray Imager (LEXI), the Radiation Tolerant Computer System (RadPC), and the Lunar Global Navigation Satellite System (GNSS) Receiver Experiment (LuGRE). Insights from these investigations are expected to enhance future Moon missions by improving technology resilience and space-based navigation.

X-ray Studies Enhance Understanding of Space Weather

According to reports, LEXI has been designed to study Earth’s magnetosphere and its interaction with solar wind. The instrument, which operates similarly to the Neutron Star Interior Composition Explorer (NICER) mounted on the International Space Station, has been calibrated using the same X-ray star. By analysing X-rays emitted from Earth’s upper atmosphere, LEXI is expected to provide valuable data on space weather effects, which could assist in protecting future lunar infrastructure.

Radiation-Tolerant Computing Technology Tested on the Moon

As per reports, the RadPC experiment is assessing how computers can withstand and recover from radiation-related faults. Prior to deployment on Blue Ghost, a radiation-tolerant computing system was tested aboard the space station, where an algorithm was developed to detect and address potential hardware failures. RadPC has been designed to identify faulty components and repair them autonomously, with its findings anticipated to aid the development of more resilient computing systems for deep-space missions.

GNSS Signals Successfully Received on the Lunar Surface

Reports indicate that the LuGRE experiment has detected GNSS signals at an unprecedented distance from Earth. On the space station, the Navigation and Communication Testbed (NAVCOM) has been evaluating backup navigation solutions that could serve as alternatives when GNSS signals are weak or unavailable. This research is expected to contribute to the development of reliable navigation methods for future lunar missions.

The International Space Station remains integral to advancing space research, with its experiments continuing to inform and refine technologies for long-term lunar exploration.

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