How Ancient Crater Lakes Fostered Ideal Conditions for Earth’s Earliest Oxygen-Breathing Life

Groundbreaking research has unveiled the presence of stromatolites—layered structures created by microbial communities—within a 42,000-year-old asteroid crater in South Korea. This significant finding suggests that an ancient post-impact lake acted as an “oxygen oasis,” providing a vital habitat for early life.

A detailed analysis of stromatolites and lake sediments at the Hapcheon impact crater indicates that these formations may represent the oldest fossilized evidence of oxygen-producing microbial life on early Earth. Image credit: Lim et al., doi: 10.1038/s43247-026-03206-7.

“Stromatolites, which are layered organic sedimentary structures, have been identified as some of the earliest evidence of life on Earth, dating back approximately 3.5 billion years to the early Archean era,” stated lead author Dr. Jaesoo Lim and colleagues from the Korea Institute of Earth Science and Mineral Resources.

These layered structures form through the trapping and binding of sediment particles by microbial activity or through mineral precipitation triggered by microbial metabolic processes.

In the northwestern section of Hapcheon Crater, the research team discovered numerous stromatolites, each measuring between 10 to 20 centimeters in diameter.

“Geochemical analysis of the stromatolites unveiled crucial features, including traces of extraterrestrial materials and surrounding rock, as well as indications of alteration due to hydrothermal activity,” the researchers explained.

The inner layer exhibits a stronger hydrothermal signal, suggesting formation during an earlier, hotter phase.

“These findings collectively support the idea that stromatolites evolved in hydrothermal lakes that gradually decreased in temperature after the impact event,” they added.

Analysis indicates that the Hapcheon collision occurred roughly 42,300 years ago.

This discovery sheds light on the Great Oxidation Event, a significant period around 2.4 billion years ago when Earth’s atmospheric oxygen levels surged,” the scientists noted.

The impact-induced hydrothermal lake likely provided a unique habitat for oxygen-producing microorganisms to flourish.

Such environments have been referred to by the research team as “oxygen oases.”

The study also raises the prospect of similar habitats existing on early Mars.

Since Mars is believed to have had water-filled impact craters in its early history, these cratered environments could serve as promising sites in the search for signs of past life.

“This research presents the first comprehensive evidence that stromatolites can form in hydrothermal lakes generated by asteroid impacts,” Lim remarked.

“Such conditions may have favored the development of early microbial ecosystems.”

For more details, refer to the study published in the Journal, Communication Earth and Environment, on April 16, 2026.

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J. Lim et al. 2026. Discovery of stromatolite formation in post-impact hydrothermal lake environments and its significance for early Earth. Communication Earth and Environment 7, 334; doi: 10.1038/s43247-026-03206-7

Source: www.sci.news

Research Reveals Earth’s First Organisms Used Molybdenum for Biochemical Processes

A groundbreaking study reveals that approximately 3.4 billion years ago, during the Archean Era, ancient microbes were not only reliant on molybdenum—a rare metal at the time—but also explored the use of tungsten. This discovery has the potential to transform how astrobiologists search for extraterrestrial life.

Early Earth. Image credit: Peter Sawyer/Smithsonian Institution.

Geochemical evidence indicates that the concentration of molybdenum in early Earth’s anoxic oceans was extremely limited; however, modern organisms are largely dependent on this essential element.

Previous theories proposed that life initially utilized tungsten before transitioning to molybdenum as it became more abundant.

Professor Betül Kaçar from the University of Wisconsin-Madison and her research team aimed to test this hypothesis.

“The transition metal molybdenum presents a puzzling evolutionary narrative in relation to biological systems,” the researchers stated.

“Molybdenum plays a significant role in vital biogeochemical processes involving carbon, nitrogen, and sulfur, which previous studies suggest have deep-rooted evolutionary histories.”

In their research, the authors analyzed genome databases to pinpoint species with genes responsible for molybdenum transport, storage, and enzymatic functions.

They applied a technique known as phylogenetic matching to trace the evolutionary lineage of molybdenum- and tungsten-utilizing proteins within the current tree of life.

Moreover, they investigated the mechanisms of molybdenum movement and utilization within living cells, focusing on intracellular transport from uptake to catalysis.

Simultaneously, they explored the historical context of biological tungsten use for similar functions.

The researchers compiled existing data regarding molybdenum’s prevalence over time and found that, despite its scarcity, ancient microorganisms on Earth found ways to utilize it, dating back to between 3.3 and 3.7 billion years ago.

“Counterintuitively, geochemical records suggest that the abundance of molybdenum on early Earth was significantly lower billions of years ago, particularly prior to the emergence of oxygenic photosynthesis,” noted Dr. Aya Cross, a student at the University of Wisconsin-Madison.

“Yet, life persisted in evolving biochemical pathways that depended on molybdenum, despite its limited availability.”

“These processes have been passed down to modern organisms.”

“Understanding the elemental dependencies of early life could aid astrobiologists in identifying other planets capable of supporting life,” Professor Kaçar remarked.

“This study illustrates that a lack of an element in the environment doesn’t negate the potential for life to adapt and exploit it in innovative ways.”

“Life exhibits remarkable adaptability, and insights like these remind us that the quest for extraterrestrial life may necessitate considering possibilities previously unimagined.”

A research paper detailing these findings was published in the latest edition of Nature Communications.

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AS Cross et al. 2026. The biological utilization of molybdenum and tungsten dates back 3.4 billion years. Nat Commun 17, 3943; doi: 10.1038/s41467-026-72133-0

Source: www.sci.news

Understanding Earth’s Slow Magnetic Field Reversal: Should You Be Concerned?

What Causes the Earth’s Magnetic Field?

The Earth’s magnetic field originates from moving charges. In a typical bar magnet, these moving charges are electrons orbiting in atoms. However, inside the Earth, the magnetic field is produced by electrons in circulating flows of molten iron.

The exact processes are not fully understood. Essentially, the hot material in the Earth’s outer liquid iron core expands and rises as it becomes less dense than its surroundings. As it cools, it should sink again; yet, Earth’s rotation complicates this process.

Consequently, fluid circulation occurs around the core, generating friction between the various layers, similar to a plastic comb rubbing against a nylon sweater. It’s this movement of charges that ultimately creates the Earth’s magnetic field.

Thus, two essential factors for planetary magnetism are a liquid core and rotation. This is evident because, despite Venus being nearly the size of Earth and having a liquid core, it lacks a significant magnetic field due to its slow rotation speed of once every 243 Earth days.

Why Do the Earth’s Magnetic Poles Move?

Tracking the true position of magnetic north is essential for accurate navigation – Credit: Alamy

The Earth’s magnetic field resembles that of a bar magnet with distinct north and south poles; however, the processes that generate it are complex and lead to fluctuations in the magnetic poles.

Historically, the North Pole has shifted approximately 15 km (9 miles) annually. Since the 1990s, this acceleration has intensified, with the pole currently moving towards Siberia at a rate of about 55 kilometers (34 miles) per year. Speculatively, this shift might signal an impending magnetic reversal, where the magnetic north and south poles swap positions—an event recorded 171 times over the past 71 million years.

Satellite observations suggest that these movements arise from competing clusters of unusually strong magnetic fields deep within the Earth. Despite various theories, the exact reasons for the reversal of Earth’s poles remain uncertain.

What Happens If the Magnetic Field Disappears?

Auroras visualize magnetic fields that protect us from harmful radiation – Credit: Getty

Scientists discovered the concept of magnetic reversal by studying fields on either side of the Mid-Atlantic Ridge, where molten rock emerges and solidifies. As it does so, crystals align with the Earth’s magnetic field, leaving a historical record of reversals.

The reversal is believed to take place over a period of 1,000 to 10,000 years, during which the magnetic field can shrink to zero before re-emerging with the opposite polarity. This process implies that there may be extended periods when Earth had no magnetic field.

This absence poses risks for life, as the magnetic field extends far into space, creating a protective bubble that shields the Earth’s surface from harmful solar wind particles and cosmic rays.

These particles usually funnel toward the poles, resulting in stunning auroras. Without this protective shield, the increase in radiation could elevate mutation rates in living cells and potentially lead to cancer in various organisms. Despite these challenges, life has withstood many such magnetic field events.

How Stable Is Earth’s Magnetic Field?

Earth’s core is as hot as the sun’s surface – Credit: Getty

The reliance of the Earth’s magnetic field on electrical currents flowing through molten material means that the field is inherently variable. This variability is evident in the current movement of the magnetic north pole, while the south pole’s movement is less pronounced.

Nonetheless, it’s crucial to recognize that the magnetic field remains relatively stable 99.9% of the time. This stability has played a key role in protecting life on Earth for nearly 3.8 billion years.

How Do Animals Use Magnetic Fields for Navigation?

Pigeons can sense Earth’s magnetic field, enhancing their incredible homing instincts – Credit: Getty

Many animals exhibit remarkable navigation abilities, leading to the hypothesis that they possess a magnetic sense to detect magnetic field lines. However, identifying the underlying mechanisms has proven challenging.

In the 1970s, American researcher Richard Blakemore observed that certain single-celled organisms responded to magnetic fields, leading biologists to discover that these organisms contain small sacs of magnetic iron oxide or sulfide.

Currently, Noboru Ikeya and Jonathan Woodward from the University of Tokyo have demonstrated that magnetic fields can induce chemical changes affecting cell behavior. They found that the presence of a magnet could alter cellular chemicals by up to 3.5%, shedding light on the connection between magnetic fields and biological responses.

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Source: www.sciencefocus.com

Artemis II Astronauts Experience Moon’s Gravity: Stronger Than Earth’s Pull

Breaking News: The Artemis II astronaut crew has officially joined the ranks of the lunar space exploration community.

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The crew’s Orion capsule entered the Moon’s gravitational influence at 12:41 a.m. ET on Monday, marking a significant moment as they navigate an area dominated by the moon’s gravity.

“This represents a critical milestone in our mission,” stated NASA Flight Director Rick Henfling during a recent press conference.

The Moon’s sphere of influence is a mathematical boundary, not a tangible one, which indicates an astronaut’s proximity to the lunar body.

This milestone is a major achievement for NASA, marking the first human entry into the Moon’s sphere of influence since Apollo 17 in 1972.

On Sunday, astronauts shared images of their “last glimpse of Earth before approaching the moon,” capturing the planet as a distant crescent through the Orion spacecraft’s window.

The Artemis II astronauts—Reed Wiseman, Christina Koch, Victor Glover, and Canadian astronaut Jeremy Hansen—began their Sunday with a special wake-up message from Apollo 16 astronaut Charlie Duke.

“John Young and I landed on the moon in 1972 with a lunar module we named Orion,” Duke shared in a recorded message. “It’s exciting to see a new kind of Orion leading the way for humans to return to the moon.”

Artemis II crew members (from left) Jeremy Hansen, Reid Wiseman, Christina Koch, and Victor Glover respond to reporter questions on Thursday.
NASA

The astronauts tested newly designed spacesuits for this flight, essential for both launch and emergency situations.

Orange spacesuits are worn during launch and can provide a breathable atmosphere for up to six days in case the Orion capsule loses pressurization, as highlighted by NASA.

The Orion spacecraft conducted a crucial 14-second engine burn on Sunday to maintain an accurate orbit around the moon. Although correction burns were planned for other dates, this was the first time one was required since leaving Earth’s orbit.

“Orion demonstrated a precise orbit, so the initial two corrections were unnecessary,” Henfling explained.

The crew will orbit the moon on Monday, reaching an approximate distance of 452,760 miles from Earth, a new record for human distances traveled from home. They are poised to surpass the Apollo 13 crew’s record of 248,655 miles.

During their lunar flyby, Wiseman, Koch, Glover, and Hansen will dedicate about seven hours to observing and photographing the moon, starting at 2:45 p.m. ET. They will explore never-before-seen areas of the moon’s surface.

NASA will deliver live coverage of the flyby starting at 1 p.m. ET.

NASA estimates the Orion spacecraft will reach a distance of 4,070 miles from the moon’s surface at its closest approach around 7 p.m. ET.

The astronauts will utilize two Nikon D5 cameras and one Nikon Z9 camera to capture stunning imagery during their mission.

Focusing on 30 scientific objectives, crew members will investigate the Oriental Basin, a 3.8 billion-year-old crater formed by a large impactor. The approximately 600-mile-wide basins on both sides of the moon harbor geological features that provide insight into ancient impacts, as per NASA.

The crew will also examine the Hertzsprung basin located on the moon’s far side. Unlike the well-preserved Oriental Basin, the 400-mile-wide crater showcases features affected by subsequent lunar impacts, providing a unique opportunity to compare lunar topographical changes over time.

To guide their observations, the crew will employ advanced software tools designed for scientific targets.

Kelsey Young, Artemis II’s lunar science director, noted the busy schedule but emphasized the need for flexibility. “They are scientists on a mission and are encouraged to deviate from the agenda if something compelling captures their attention,” she stated.

Towards the end of their lunar viewing period, astronauts will witness a solar eclipse lasting approximately one hour from their vantage point in space. This eclipse will begin at 8:35 PM ET, obstructing light from the Orion capsule’s perspective.

During this time, the moon will appear predominantly dark, offering astronauts the chance to observe the sun’s corona and detect flashes from meteoroids impacting the lunar surface.

Astronauts will also photograph other visible planets during the eclipse, including Mercury, Venus, Mars, and Saturn, as mentioned by Young.

“This crew stands at the forefront of lunar exploration, with the unparalleled opportunity to view the moon from a unique perspective,” she added.

“This is exploration,” Young concluded. “We have received valuable data from orbiting spacecraft, but these subtle observations are what we truly need to uncover new discoveries.”

Source: www.nbcnews.com

New Theory: Earth’s Formation from Two Distinct Solar Rings

Early solar system model

New Models Suggest Flawed Understanding of Early Solar System

Image Credit: Panther Media Global / Alamy

The formation of the inner solar system may not align with previous scientific beliefs. Traditionally, researchers posited that rocky planets emerged from a singular disc of dust and debris originating from the early solar system. However, groundbreaking new simulations indicate the possible existence of two distinct disks.

Models relying on a single disk or ring of material surrounding the young Sun tend to fall short in replicating several observable features of our solar system. For instance, Earth’s unique rock composition suggests a blend of two different types, which raises questions about their originating from a singular ring. Moreover, single-ring models often render Mercury and Mars disproportionately large while placing Venus and Earth too closely together, leading to composition similarities between Earth and Mars that seem out of place.

Bill Bottke, along with his team at Colorado’s Southwest Research Institute, conducted a series of sophisticated simulations exploring how planets could evolve from a shared reservoir of material. Yet they faced persistent challenges.

“For six months, we tried different simulations without success,” Bottke explained during a recent presentation at the Lunar and Planetary Science Conference held in Texas on March 16th. “In a moment of desperation, we considered testing a second reservoir and discovered that this approach yielded a viable model for creating terrestrial planets, while addressing many of the outstanding concerns.”

The optimal model proposed involved two separate disks: one situated about half the current distance from the Sun to Earth and the other approximately 1.7 times that distance. The simulation resulted in planets of proper size and distance.

This theory also aligns with the compositions of the Earth, Moon, and Mars. “We believe Earth predominantly formed from material sourced from the inner solar system, with only a minor contribution from outside,” noted Jan Hermann, who delivered a related presentation the same day at the Max Planck Institute for Solar System Research in Germany. In contrast, Mars appears to have formed mainly from the outer disk, explaining the contrasting compositions of the two planets.

Nonetheless, some researchers express concern that this model relies on very specific initial conditions that may not be entirely understood. “Small alterations in the shape of the disk can significantly affect the outcome of where terrestrial planets are positioned,” Bottke cautioned.

Current efforts are focused on refining the model and exploring additional factors that may influence solar system formation. “We’re investing considerable computational resources to examine every logical possibility,” Bottke indicated. If successful, this new perspective could illuminate various solar system enigmas, from anomalous asteroids to mysterious lunar rocks.

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Source: www.newscientist.com

Top Ocean Predators Thrive Even After Earth’s Largest Mass Extinction

Artwork of Hibodus Sharks

Artwork of Hibodus sharks—predators from the late Permian period that outlasted mass extinctions.

Credit: Christian Darkin/Science Photo Library

The largest mass extinction in history led to the loss of over 80% of marine life. Remarkably, certain ecosystems continued to thrive, and various species, including apex predators, managed to survive this catastrophic event.

This research indicates that the survival of specific ecosystems was influenced by their unique species compositions. A similar pattern may be observed in today’s marine ecosystems, which are under significant threat from climate change.

Approximately 252 million years ago, the end-Permian extinction was likely triggered by extensive volcanic eruptions in present-day Siberia, causing rapid global warming and diminishing ocean oxygen levels. Notably, some groups, like trilobites and eurypterids (sea scorpions), faced total extinction, while others experienced dramatic losses. In the aftermath, new species groups emerged, including dinosaurs and ichthyosaurs.

Despite the extinction of numerous species, researchers speculate that ecosystems may have become less complex. A functioning ecosystem relies on diverse interdependent species—plants that produce energy, herbivores that consume them, and predators that eat herbivores. Top predators may face extinction as they depend on prey for survival. Thus, a significant extinction event, such as the one at the end of the Permian, would simplify ecosystems.

To investigate this hypothesis, Baran Kalapunar and a team from the University of Leeds assessed preserved remains from seven marine ecosystems globally, both before and after the extinction. They analyzed the ecosystem structures based on the species present. Kalapunar declined to provide an interview as the study is yet to undergo peer review.

Even with species losses reaching 96%, five of the seven ecosystems sustained at least four trophic levels.

In regions, particularly near the poles, slow-moving herbivores caused the most significant damage, while free-swimming organisms, such as fish, were less severely impacted.

Ecosystem recovery varied based on proximity to the equator. Tropical ecosystems were primarily populated by low-trophic-level species, while those nearer to the poles experienced the addition of trophic levels as fish predators relocated away from extreme heat near the equator.

These findings imply that present-day marine ecosystems also respond differently to climate change and other anthropogenic impacts.

“I’m not aware of any other study that encompasses so many regions,” states Peter Roopnarine from the California Academy of Sciences in San Francisco. He concurs with the conclusions that many ecosystems sustain trophic levels despite extinctions, as previous smaller-scale studies indicated.

However, Roopnarine cautions against placing too much emphasis on the specifics of researchers’ ecosystem models. The fossil record does not clarify which organisms survived and which did not, requiring researchers to combine all photosynthetic organisms together without predicting outcomes if these species became extinct. “These findings are firmly supported by the fossil record, yet it remains incomplete,” he remarks.

Dinosaur Fossil Discovery in Mongolia’s Gobi Desert

Join an exciting expedition to unearth dinosaur fossils in Mongolia’s Gobi Desert, one of the world’s top paleontological locations.

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Source: www.newscientist.com

Are Aliens Picking Up Earth’s Radio Waves? – Cyworthy Insights

Radio signals are a fundamental element of the first contact subgenre in science fiction. Carl Sagan’s Contact features a compelling narrative that centers around Liu Cixin’s discovery of encrypted radio signals from the planet Vega. Another notable work, The Three-Body Problem by Vince Gilligan, explores the ramifications of a scientist establishing covert radio contact with extraterrestrial beings. The story of Pluribus focuses on the consequences of scientists following instructions transmitted to Earth through radio signals. What is the likelihood of us receiving alien radio signals, or vice versa?

A team of researchers from Pennsylvania State University and the California Institute of Technology delved into this intriguing question. They identified radio signals as a critical component in the quest for intelligent extraterrestrial life. Astronomers have established that intelligent species, like humans, can create machines that both generate and detect radio signals.

The research team specifically focused on a subset of radio transmissions from Earth that relay signals between ground stations and spacecraft located far from our planet. This system is known as NASA’s Deep Space Network, or DSN. It comprises three sites located in the United States, Spain, and Australia, each featuring 70-meter (230 feet) and 34-meter (112 feet) radio antennas.

The detectability of signals from these antennas depends on several factors, including the strength of the signal, the duration of the observation, the bandwidth of the signal, and the required distinction from background noise. Using a formula based on the typical input power of DSN signals, the researchers calculated the possible distance at which extraterrestrial intelligence could detect signals from Earth. They assumed that the telescope used by an alien civilization would have specifications similar to those of Earth’s signals. Using the observation time of the Green Bank Telescope of 30 minutes, they estimated that signals could be detected within a radius of approximately 7 parsecs, equating to 200 trillion kilometers or 100 trillion miles, which is only about 0.02% of the Milky Way’s diameter.

Following this analysis, the astronomers posed two related questions: First, from which direction in the sky is Earth likely to be detected by radio signals? Second, in what direction are the planetary systems most likely to send radio signals to detect extraterrestrial life?

To answer the first question, the researchers examined the distribution of DSN signals transmitted from Earth to various satellites and telescopes, including the James Webb Space Telescope (JWST). By comparing the DSN patterns to those that extraterrestrial intelligence might generate, astronomers could identify where distant observers are most likely to detect signals from Earth. They utilized publicly available DSN schedules to map the sky and assess where and when antennas were transmitting radio signals.

Their findings revealed that a significant portion of Earth’s radio signals emanate from spacecraft like the Advanced Composition Explorer, the Deep Space Climate Observatory, and the Solar Heliosphere Observatory, primarily along the Sun’s apparent path in the sky, known as the ecliptic. Remarkably, up to 79% of Earth’s deep space radio signals are within 5° of the ecliptic, with minor but notable peaks directed towards Mars, Mercury, Jupiter, Saturn, and the JWST.

These insights bring several implications for the search for extraterrestrial intelligence. First, astronomers should prioritize scanning for radio signals from distant planetary systems, especially where exoplanets transit between Earth and their host star. This could increase the likelihood of capturing stray signals from alien civilizations directed at their own satellites and probes positioned near the ecliptic.

Second, astronomers should focus efforts during times when exoplanets orbiting their stars pass behind one another. This increases the probability that a distant observer might detect Earth’s signals to 12%. If alien civilizations are broadcasting signals towards stars resembling Jupiter or Mars, there are substantial chances of detection.

Lastly, as most of Earth’s deep space radio signals are concentrated near the ecliptic, astronomers should particularly investigate stars positioned close to this ecliptic plane. These stars are more likely to be recipients of signals from Earth, and they may even be attempting to reply. Following this strategy, the researchers identified 128 star systems within a seven parsec radius of Earth where civilizations possessing intelligence could potentially detect signals from Earth through DSN communications and vice versa. Therefore, for the most promising avenue in the search for extraterrestrial life, attention should be directed along the path of the Sun.


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Ganymede’s Aurora Patch: Discovering Similarities with Earth’s Aurora Physics

Scientists from the United States, Europe, and China utilized the Ultraviolet Spectrometer (UVS) on NASA’s Juno spacecraft to meticulously map the auroral patch structure on Ganymede, Jupiter’s moon, revealing similarities to Earth’s auroras. Their groundbreaking research indicates that interactions between magnetic fields and charged particles could be the universal driver of auroras, enhancing our understanding of magnetospheres across the solar system.

Artist’s concept of the aurora borealis on Jupiter’s moon Ganymede. Image credits: NASA/ESA/G. Bacon, STScI/J. Saur, University of Cologne.

Ganymede stands out as the only known moon to possess its intrinsic magnetic field, creating a miniature magnetosphere nested within the vast magnetosphere of Jupiter.

The auroral emissions primarily stem from oxygen at wavelengths of 130.4 nm and 135.6 nm, triggered by precipitating electrons.

In a recent groundbreaking study, researcher Philippe Gusbin from the University of Liège and his team examined ultraviolet observations of Ganymede conducted on June 7, 2021, by the Juno spacecraft.

They identified multiple auroral spots in Ganymede’s leading downstream hemisphere.

These patches typically measure about 50 km in size, with brightness levels soaring to around 200 Rayleigh.

“Auroras on Ganymede are driven by the precipitation of electrons into its thin oxygen atmosphere,” explained Gusbin.

“Previous observations of Ganymede’s auroras were limited in detail due to the spatial constraints of ground-based methods, which couldn’t resolve the fine structures commonly observed in planetary auroras.”

The morphology and scale of Ganymede’s auroras closely resemble the auroral ‘beads’ found on Earth prior to magnetospheric substorms and in Jupiter during ‘dawn storms.’

The lack of a similar patch in the southern hemisphere could stem from observational geometry, but it may also reflect an asymmetry tied to Ganymede’s location in Jupiter’s plasma disk.

“Auroral ‘beads’ are also present in the auroras of Earth and Jupiter, where they correlate with substorms and dawn storms—major magnetospheric reorganizations that release significant energy and induce intense auroral activity,” noted Dr. Alessandro Moirano, a postdoctoral researcher at the University of Liège and the National Institute of Astrophysics in Rome.

This discovery implies that similar physical processes may govern magnetospheres, despite variations in scale and environmental conditions.

“Juno’s close flyby of Ganymede lasted under 15 minutes, and it will not revisit Ganymede, leaving us unsure about the frequency of these patches or how they may evolve,” remarked Dr. Bertrand Bonfont, an astrophysicist at the University of Liège.

“Fortunately, ESA’s JUICE mission is currently en route to Jupiter and is set to arrive in 2031. This mission will conduct detailed observations of Ganymede.”

“Equipped with a similar ultraviolet spectrometer to that of Juno, this spacecraft will facilitate long-term observations that could reveal more about the evolution of Ganymede’s aurora and potentially uncover new mysteries.”

For further reading, refer to a paper published in Astronomy and Astrophysics.

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A. Moirano et al. 2026. High spatial resolution ultraviolet observations of Ganymede’s aurora patches by Juno. Constraints on the magnetospheric source region. A&A 706, L16; doi: 10.1051/0004-6361/202558379

Source: www.sci.news

Uncovering Hidden Bacteria: How They Thrive in Earth’s Deep Soils – Sciworthy

Beneath the Earth’s surface lies a largely unexplored ecosystem known as the critical zone. This unique area of soil stretches from the Earth’s surface to the base of the groundwater zone, acting as a dynamic interface where rock, water, air, and life converge. Despite their low content of carbon and nutrients compared to surface soils, the microbial communities found in these deep soils are remarkably diverse. Scientists are still uncovering how these microorganisms manage to thrive under such nutrient-scarce conditions.

To explore how microbes survive in the critical zone, researchers focused on a little-known group of bacteria identified globally in deep soils. Known as CSP1-3 Gate, these bacteria were first discovered in 2006 within a geothermal system in Yellowstone National Park. Since then, they have been found in various oxygen-limited and nutrient-poor environments, yet their exact role and characteristics remain mysterious.

Researchers collected soil samples from seven deep soil cores spanning 20 meters (approximately 65 feet) in Shaanxi province, China, and western Iowa, USA. By extracting and sequencing environmental DNA from these samples, they pieced together draft genomes of the microorganisms inhabiting these depths. Through metagenomic analyses, they aim to uncover where CSP1-3 microbes live, their dietary habits, their nutrient cycling processes, and the adaptations that facilitate their survival.

Analysis revealed CSP1-3 bacteria were abundant in deeper soils, comprising over 10% of all microorganisms found in 30 out of 86 soil layers below 5 meters (16 feet). In some layers, such as those at 17 meters (56 ft) and 22 meters (72 ft) deep, CSP1-3 accounted for up to 60% of the microbial population. Using DNA copy-counting methods, researchers estimated that nearly 50% of CSP1-3 cells in these deep soils were actively replicating.

Based on the assembled metagenomes, the research indicated that CSP1-3 bacteria utilize a flexible metabolism to thrive in deep soils. They identified genes that allow these bacteria to alternate between two methods of obtaining energy: autotrophy, which involves producing their own food, and heterotrophy, which entails consuming organic matter from their environment. This adaptability, referred to as mixotrophy, allows them to respond to varying nutrient availability.

Additionally, researchers uncovered genes enabling CSP1-3 bacteria to utilize diverse energy sources such as carbon monoxide (CO) and diatomic hydrogen (H2), both prevalent in deep soils. They also identified genes allowing these microbes to generate energy under varying oxygen conditions, providing an advantage in environments where oxygen levels fluctuate. Genes related to sugar synthesis, such as trehalose, contribute further to their endurance in resource-limited conditions, alongside genes linked to carbon, nitrogen, and sulfur management.

The team analyzed 521 genomes from diverse environments globally, including aquatic habitats, topsoil, and deep soil, to trace the evolutionary lineage of CSP1-3. Genome analysis indicated that these bacteria’s ancestors originated in aquatic settings before transitioning to topsoil and ultimately to deep soil, with significant genomic changes that augmented their carbohydrate and energy metabolism to facilitate adaptation to terrestrial ecosystems.

The researchers concluded that CSP1-3 bacteria are evolutionarily suited to thrive in deep, nutrient-poor soils due to their specialized metabolism and low-energy survival strategies. They posited that CSP1-3 plays a crucial role in energy and nutrient cycling, potentially influencing global environmental processes by enhancing soil fertility and nutrient availability, thereby stabilizing deep soil ecosystems. The ability of these microorganisms to utilize gaseous energy in nutrient-deficient environments offers compelling insights into their survival strategies under extreme conditions, contributing to ongoing planet protection efforts. However, further investigations are necessary to fully comprehend how these deep soil microbes impact soil chemistry and ecosystem functions over time.


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Massive Heat Within Earth’s Core May Have Disrupted the Magnetic Field

Earth's Magnetic Field Representation

Earth’s Magnetic Field Extends Thousands of Kilometers into Space

Getty Images/iStockphoto

Recent studies reveal that two massive, enigmatic rock formations beneath Africa and the Pacific Ocean may play a crucial role in generating Earth’s magnetic field. These formations could have contributed to the field’s destabilization over millions of years.

Scientists have long been aware of these continent-sized rock blocks, which stretch nearly 1000 kilometers from the outer core to the upper mantle. They exhibit unique properties that slow seismic wave passage, although their depth complicates measurements, making precise differentiation challenging.

Andrew Biggin, a researcher from the University of Liverpool, explored Earth’s magnetic field for insights. This protective magnetic field, created over billions of years by molten iron convection in the core, extends thousands of kilometers into space, shielding our planet from solar winds and cosmic radiation.

The magnetic field’s shape is influenced by the heat energy transfer from the hot core to cooler zones. Biggin and his team theorized that analyzing changes in the magnetic field could unveil details about heat movement within the Earth’s core.

To trace the evolution of the magnetic field, researchers compared ancient volcanic rock records that captured magnetic orientations over millions of years. They simulated the heat flow in the core with and without the influence of large hot rock masses, correlating results with actual magnetic measurements.

Findings indicated that simulations incorporating these rock blocks aligned most closely with ancient magnetic data. “These convection simulations can reproduce notable features of the core’s magnetic field only when considering significant variability in heat flow at the core’s upper layer,” says Biggin.

This implies that these hot regions have likely maintained higher temperatures than their surroundings for millions of years, leading to diminished heat exchange between the core and mantle. Such discrepancies in heat flow may have significantly contributed to the creation and stabilization of the Earth’s magnetic field.

While many geologists view the Earth’s magnetic field evolution as symmetrical over time, Biggin’s research revealed inherent asymmetries in ancient fields, likely instigated by these rock formations. This discovery could refine how geologists interpret the movement of ancient rocks and reveal changes in Earth’s deep structure over time, according to Biggin.

If accurate, these temperature contrasts in the rock formations could also exist in the upper outer core, potentially detected through seismic wave analysis.

However, Sanne Kottar from Cambridge University expresses skepticism. “Mapping core variations is extremely challenging due to the vast mantle material we must analyze before accessing the core,” she explains.

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Source: www.newscientist.com

Fossil Discovery Sheds Light on the Origins of Earth’s First Fish

Paleontologists from Australia and China have conducted two groundbreaking studies on the fossilized remains of a remarkable Devonian lungfish. Utilizing advanced imaging technology, they have unearthed previously overlooked anatomical details, significantly enhancing our understanding of early vertebrate evolution. Their findings have been published in the Canadian Journal of Zoology and the journal Current Biology.



Paleolophus yunnanensis, a unique lungfish species that thrived in southern China’s waters 410 million years ago. Image credit: Brian Choo, Flinders University.

In a recent study, lead researcher Alice Clement, a paleontologist at Flinders University, investigates The Mystery of Kainokara, a fossil known from a single specimen found in the Late Devonian Gogo Formation of Western Australia.

“New research, including the analysis of previously neglected specimens, is gradually uncovering the rich diversity of lungfishes found in Australia’s significant fossil sites,” said Dr. Clement.

“One particularly enigmatic specimen originates from Australia’s earliest ‘Great Barrier Reef’, a Devonian reef located in the Kimberley region of northern Western Australia.”

“When first described in 2010, this unusual specimen was so perplexing that the authors speculated it might represent an entirely new type of fish never documented in science.”

“Using advanced scanning techniques, we developed comprehensive digital images of both the external and internal structures of the skull, revealing the complexity of this fascinating lungfish’s brain cavity.”

“In fact, we confirmed that earlier interpretations may have been from an upside-down perspective.”

“We were also able to compare the well-preserved inner ear region with other lungfishes,” noted Flinders University paleontologist Hannah Thiele.

“This provides an essential data point in the rich collection of lungfish and early vertebrate species.”

“This research enhances our understanding of the evolutionary progression of these ancient lobe-finned fishes, both in Gondwana and globally.”

In a separate study, Flinders University paleontologist Brian Chu and colleagues reveal a newly discovered species of lungfish from the Devonian period in China, Paleolophus yunanensis.

“The discovery of Paleolophus yunanensis offers unprecedented insight into the transitional phase between the early appearance of lungfish and their extensive diversification millions of years later,” said Dr. Chu.

“At this time, this group was just beginning to develop unique feeding adaptations that would serve them well throughout the remainder of the Devonian period and into the present.”

“Lungfish, including the ancient lineage found in Queensland, Australia, have fascinated researchers due to their close evolutionary relationship with tetrapods, the four-limbed vertebrates that include humans.”

“The distinctive skull of the newly discovered lungfish from 410-million-year-old rock formations in Yunnan offers crucial insights into the rapid evolutionary changes during the Early, Middle, and Late Devonian periods.”

“The new specimens exhibited both similarities and differences compared to the earliest known specimens, such as Diabolepis fossils from southern China and uranolophus found in locations like Wyoming and Australia.

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Hannah S. Thiele et al., deciphering The Mystery of Kainokara from the Late Devonian Gogo Formation, Australia. Canadian Journal of Zoology, published online January 28, 2026. doi: 10.1139/cjz-2025-0109

Tuo Qiao et al., 2026. New fish fossil sheds light on the rapid evolution of early lungfish. Current Biology 36 (1): 243-251; doi: 10.1016/j.cub.2025.11.032

Source: www.sci.news

How Two Massive Clumps of Superheated Material Influence Earth’s Magnetic Field

Two colossal, ultra-hot rock formations, positioned 2,900 kilometers beneath the Earth’s surface in Africa and the Pacific Ocean, have influenced Earth’s magnetic field for millions of years, according to groundbreaking research led by Professor Andy Biggin from the University of Liverpool.



Giant superheated solid masses at the Earth’s mantle base impact the liquid outer core. Image credit: Biggin et al., doi: 10.1038/s41561-025-01910-1.

Measuring ancient magnetic fields and simulating their generation presents significant technical challenges.

To explore these deep Earth features, Professor Biggin and his team used paleomagnetic data in conjunction with advanced Earth Dynamo simulations. The flow of liquid iron in the outer core generates Earth’s magnetic field, akin to a wind turbine producing electricity.

Numerical models reconstructed critical insights about magnetic field behavior over the past 265 million years.

Even with supercomputers, conducting these long-term simulations poses enormous computational challenges.

The findings showed that temperature at the upper layer of the outer core is not uniform.

Instead, localized hot areas are accompanied by continent-sized rock structures exhibiting significant thermal contrasts.

Some regions of the magnetic field were found to remain relatively stable over hundreds of millions of years, while others displayed considerable changes over time.

“These results indicate pronounced temperature variations in the rocky mantle just above the core, suggesting that beneath hotter regions, liquid iron in the core may be stagnant, rather than flowing intensely as observed beneath colder areas,” Professor Biggin stated.

“Gaining such insights into the deep Earth over extensive timescales enhances the case for utilizing ancient magnetic records to comprehend both the dynamic evolution and stable properties of deep Earth.”

“These discoveries also bear significant implications for understanding ancient continents, including the formation and breakup of Pangea, and could help address long-standing uncertainties in ancient climate studies, paleontology, and natural resource formation.”

“It has been hypothesized that, on average, Earth’s magnetic field acts as a perfect bar magnet aligned with the planet’s rotation axis in these regions.”

“Our findings suggest that this may not be entirely accurate.”

This study is published in today’s edition of Nature Earth Science.

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AJ Biggin et al. Inhomogeneities in the mantle influenced Earth’s ancient magnetic field. Nature Earth Science published online on February 3, 2026. doi: 10.1038/s41561-025-01910-1

Source: www.sci.news

How Mars’ Gravity May Influence Earth’s Ice Age Cycles

Composite photo of Mars

Mars’ Significant Impact on Earth’s Climate

Credit: NASA/JPL/Malin Space Science Systems

Despite Mars being smaller than Earth, it profoundly affects Earth’s climate cycle. Understanding how smaller planets influence the climates of exoplanets is crucial for assessing their potential for habitability.

According to Stephen Cain, researchers at the University of California, Riverside, discovered this phenomenon by simulating various scenarios to analyze Mars’ effect on Earth’s orbit across different masses, from 100 times its current mass to its complete removal. “Initially, I was skeptical that Mars, only one-tenth the mass of Earth, could so significantly affect Earth’s cycles. This motivated our study to manipulate Mars’ mass and observe the effects,” says Cain.

Earth’s climate is influenced by long-term cycles tied to its orbital eccentricity and axial tilt. These cycles are dictated by the gravitational forces of the Sun and other planets, determining significant climate events such as ice ages and seasonal shifts.

One crucial cycle, referred to as the Grand Cycle, spans 2.4 million years, involving the elongation and shortening of Earth’s orbital ellipse. This directly influences the amount of sunlight reaching Earth’s surface, thus controlling long-term climate changes.

The research indicates that eliminating Mars would not only remove the Grand Cycle but also another essential eccentricity cycle lasting 100,000 years. “While removing Mars wouldn’t completely halt ice ages, it would alter the frequency and climate impacts associated with them,” Cain explains.

As Mars’ simulated mass increases, the resulting climate cycles become shorter and more intense. However, a third eccentricity cycle, enduring approximately 405,000 years, remains predominantly influenced by Venus and Jupiter’s gravitational pulls, illustrating that while Mars is notably influential, it is not the only player.

Mars also affects Earth’s axial tilt, which oscillates over about 41,000 years. Cain and colleagues observed that Mars seems to stabilize these cycles—more mass leads to less frequent cycles, while a smaller Mars results in more frequent ones.

The precise impact of Mars’ absence or increased mass on Earth remains speculative, but it would undoubtedly lead to changes. The pursuit of Earth-like exoplanets with climates suitable for life continues, underscoring the need to evaluate the influence of smaller planets more thoroughly. “A comprehensive understanding of exoplanet system architectures is essential for predicting possible climate changes on these worlds,” warns Sean Raymond from the University of Bordeaux, France.

However, deciphering these structures can be challenging. “This serves as a cautionary note: small planets like Mars may wield a greater influence than we realize, making it imperative not to overlook these difficult-to-detect celestial bodies,” concludes Cain.

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Source: www.newscientist.com

How Plate Tectonics, Not Volcanoes, Shaped Earth’s Climate Over the Last 540 Million Years

A revealing new study challenges traditional beliefs by showing that mid-ocean ridges and continental rifts, rather than volcanic eruptions, significantly influence atmospheric carbon fluctuations and long-term climate change in Earth’s geological history.

Cryogenic Earth. Image credit: NASA.

Over the past 540 million years, Earth’s climate has gone through dramatic shifts, alternating between icy icehouse conditions and warm greenhouse phases.

Icehouse conditions prevailed during key geological periods, including the Late Ordovician, Late Paleozoic, and Cenozoic eras.

Notably, warmer periods were associated with increased atmospheric carbon dioxide, while declines in greenhouse gases led to global cooling and extensive glaciation.

Research conducted by Ben Mather and a team at the University of Melbourne reconstructed carbon movements between volcanoes, oceans, and the deep Earth over the past 540 million years.

“Our findings challenge the long-accepted view that volcanic chains formed by tectonic plate collisions are the primary natural source of Earth’s atmospheric carbon,” Dr. Mather stated.

“Instead, it appears that carbon emissions from deep-sea crevices and mid-ocean ridges, driven by tectonic movements, have been crucial in shaping the transitions between icehouse and greenhouse climates throughout most of Earth’s history.”

“For example, we discovered that carbon released from volcanoes in the Pacific Ring of Fire only emerged as a significant carbon source in the last 100 million years, prompting us to reevaluate current scientific understanding.”

This study presents the first robust long-term evidence indicating that Earth’s climate change is primarily driven by carbon released at divergent plate boundaries rather than convergent ones.

“This insight not only reshapes our understanding of past climates but will also enhance future climate models,” Dr. Mather noted.

By integrating global plate tectonics reconstructions with carbon cycle models, the research team traced the storage, release, and recycling of carbon as continents shift.

Professor Dietmar Müller from the University of Sydney remarked, “Our findings illustrate how variations in carbon release from plate spreading influenced long-term climate shifts, clarifying historical climate changes, such as the late Paleozoic ice ages, the warm Mesozoic greenhouse world, and the rise of present-day Cenozoic icehouses.”

This research holds vital implications for understanding the ongoing climate crisis.

“This study contributes to the growing body of evidence that atmospheric carbon levels are a significant factor driving major climate shifts,” Dr. Mather emphasized.

“Comprehending how Earth managed its climate historically underscores the extraordinary pace of current climate change.”

“Human activities are releasing carbon at a staggering rate, far surpassing any natural geological processes previously recorded.”

“The climate balance is tipping alarmingly fast.”

For more on this groundbreaking research, you can view the findings published in the journal Communication Earth and Environment.

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B.R. Mather et al. 2026. Carbon emissions along divergent plate boundaries influence climate shifts between icehouses and greenhouses. Communication Earth and Environment 7, 48; doi: 10.1038/s43247-025-03097-0

Source: www.sci.news

Ancient Volcanoes: Understanding Low Greenhouse Gas Emissions in Earth’s History

Arc volcanoes like Sakurajima releasing carbon dioxide

Arc-shaped volcanoes like Japan’s Sakurajima release carbon dioxide from the Earth’s interior

Asahi Shimbun via Getty Images

New research suggests that the impact of volcanoes on Earth’s climate may not be as ancient as previously believed.

The Earth’s climate has experienced shifts between “icehouse” and “greenhouse” conditions, largely dictated by greenhouse gas levels like carbon dioxide.

Volcanic arcs, including significant eruptions from mountain ranges such as Japan’s, release CO2 from deep within the Earth. Recent findings indicate that dinosaurs became a substantial source of carbon emissions only towards the end of their reign, approximately 100 million years ago, according to Ben Mather and his team from the University of Melbourne.

This correlates with the emergence of phytoplankton featuring calcium carbonate scales in the oceans approximately 150 million years ago. When these organisms perish, they deposit large amounts of calcium carbonate on the ocean floor.

As tectonic plates shift, these significant reservoirs of carbon are pushed into the mantle and recycled into the Earth’s molten core via a process known as subduction.

“Most of the carbon derived from plankton on the subducting oceanic plate mixes into the melt interior, but a portion is released through volcanic arcs,” explains Mather.

Before the emergence of scaly plankton, volcanic arc emissions contained relatively lower levels of CO2, according to Mather.

Through modeling, Mather and colleagues examined tectonics’ long-term impact on the carbon cycle over the past 500 million years. They discovered that much of the carbon stored within Earth throughout its history was released through crustal fractures in a process termed rifting, not primarily through volcanic arcs.

Rifting, a geological process where continents separate, can occur on land (as in the East African Rift) or along mid-ocean ridges.

“As tectonic plates separate, they effectively ‘roof off’ parts of the molten Earth,” Mather states. “This process generates new crust at mid-ocean ridges, releasing carbon.” The amount of carbon entering the atmosphere from continental fractures and mid-ocean ridges relies on the cracks’ length and the rate at which they separate, a process that has remained relatively stable. However, emissions from volcanic arcs have surged in the last 100 million years due to new carbon reservoirs formed by plankton.

Currently, Earth is in a temporary warm phase called an interglacial period, nested within a larger ice age that began 34 million years ago. One reason for the persistent cold phases is that phytoplankton sequester substantial amounts of carbon from the ocean, depositing it on the sea floor. Although volcanic emissions are rising, they still pale in comparison to the carbon stored by phytoplankton and that sequestered through tectonic movements.

According to Alan Collins and his team from the University of Adelaide, modeling studies like this are crucial for comprehending how volcanic and tectonic activities have influenced climate patterns over geological timescales.

“The composition of marine sediments has shifted as new organisms evolved, utilizing diverse elements, including the rise of calcium carbonate-based zooplankton,” Collins emphasizes.

Reference journal: Nature Communications Earth and Environment, DOI TK

Explore the Land of Fire and Ice: Iceland

Embark on an unforgettable journey through Iceland’s breathtaking landscapes. Experience volcanic and geological marvels by day, and chase the mesmerizing Northern Lights by night (October).

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Source: www.newscientist.com

Data Reveals 2025 as Earth’s Third Hottest Year on Record

According to Copernicus, the European Union’s climate monitoring service, last year ranked as the third warmest on record in modern history.

This finding aligns with existing trends; Copernicus data reveals that the last 11 years have consistently been the warmest in history.

In 2025, the average global temperature soared to approximately 1.47 degrees Celsius (2.65 degrees Fahrenheit) above the baseline period from 1850 to 1900. This reference period is significant as it predates the industrial era, marking a time before extensive carbon emissions entered our atmosphere.

“Annual surface temperatures exceeded average levels across 91 percent of the globe,” stated Samantha Burgess, head of climate strategy at the European Center for Medium-Range Forecasts, which operates Copernicus. “The primary contributor to these record temperatures is the accumulation of greenhouse gases, largely from fossil fuel combustion.”

Under the 2015 Paris Agreement, global leaders committed to limiting warming to 1.5 degrees Celsius above pre-industrial levels. However, this goal appears increasingly unachievable as temperatures have neared or surpassed this threshold for three consecutive years.

Mauro Facchini, director of Earth Observation at the European Commission’s Directorate-General for Defense, Industry, and Space, noted at a press conference: “A three-year average temperature exceeding 1.5 degrees Celsius compared to pre-industrial levels is a milestone we never anticipated.” He emphasized the urgent need to address climate change.

A woman shields herself from the scorching sun near the Colosseum in Rome during July.
Tiziana Fabi/AFP via Getty Images File

The U.S. government is anticipated to unveil its 2025 climate metrics on Wednesday. NASA provides its reports separately from the National Oceanic and Atmospheric Administration, owing to differing methodologies in calculating average annual temperatures, which often leads to variations in findings.

Nevertheless, the overarching trend is unmistakable: the planet is warming at an alarming rate, possibly faster than scientists had predicted.

Europe faces bleak climate data, compounded by the U.S. administration’s aggressive moves to roll back climate regulations and retreat from international efforts to mitigate warming.

Last week, the Trump administration announced its withdrawal from the United Nations Framework Convention on Climate Change, diminishing the U.S. role in global climate change discussions. Additionally, plans to withdraw support from the Intergovernmental Panel on Climate Change, which produces crucial reports on climate change impacts, were made public.

The United States is set to officially leave the Paris Agreement later this month, following a one-year waiting window.

A child enjoys a refreshing mist under a fog system in Milan during July.
Luca Bruno / AP File

President Donald Trump has labeled climate change “the work of con artists,” and his administration has actively sought to downplay critical climate reports such as the National Climate Assessment. Efforts are underway to reduce the Environmental Protection Agency’s ability to regulate greenhouse gas emissions, a primary cause of global warming.

Simultaneously, steps are being taken to promote the coal industry, including ordering coal-fired power plants to continue operations (coal is notorious for generating significant greenhouse gas emissions). The administration is also attempting to reverse many of the Biden administration’s climate initiatives, including subsidies for electric vehicles.

According to preliminary findings from Rhodium Group, an independent research firm monitoring U.S. emissions, climate pollution in the United States is projected to rise by approximately 2.4% in 2025. This increase may not stem directly from President Trump’s policies, as many regulations are yet to be implemented. The rise is likely due to high natural gas prices, growth in energy-intensive data centers, and particularly cold winters.

Rhodium Group anticipates that U.S. emissions will eventually decrease as renewable energy sources become more economically feasible compared to fossil fuels. However, the expectation of emission reductions is now less optimistic than prior to Trump’s administration.

The greenhouse gases that trap heat are intensifying weather patterns, resulting in more extreme conditions and increasing the likelihood of heavy rainfall, heatwaves, and flooding.

Last year emerged as the third-costliest year for weather-related disasters, an analysis by the nonprofit organization Climate Central revealed. In 2025, it was reported that 23 meteorological events inflicted damages surpassing $1 billion, resulting in 276 fatalities and $115 billion in total damages.

In Fleurance, France, a pharmacy thermometer indicates a scorching 45 degrees Celsius, equivalent to 113 degrees Fahrenheit.
Isabel Souliment / Hans Lukas, from Reuters file

While greenhouse gas emissions remain the principal driver of rising global temperatures, natural fluctuations also contribute. La Niña patterns, characterized by colder-than-average water in the central Pacific, generally lead to lower global temperatures, while El Niño events can raise them.

Though the La Niña pattern emerged in late 2025, NOAA scientists expect a return to neutral conditions early this year.

Source: www.nbcnews.com

Researchers Say Europa’s Spider-Like Structures Mirror Earth’s Lake Stars

Europa, Jupiter’s frigid moon, is an oceanic environment that stands out as a key player in the quest for extraterrestrial life. Its surface is characterized by various landforms believed to originate from salty water sources beneath its icy crust, potentially making it the most accessible body of liquid water in the solar system. Notably, the asterisk-shaped “spider” located in the center of Manannan Crater was identified during NASA’s Galileo mission. Planetary scientists have recently introduced a novel hypothesis regarding the formation of this spider-like structure, drawing on morphological analysis and initial analog modeling. They propose that it may have formed through a process akin to the creation of dendritic “lake stars,” a seasonal phenomenon observed in frozen terrestrial ponds and lakes.



Damkhan Alla topographic map of Manannan. Image credit: McCune et al., doi: 10.3847/PSJ/ae18a0.

“The spider-like feature may have resulted from an eruption of molten salt water following the Manannan impact,” explains Dr. Elodie Lesage from the Planetary Science Institute.

“This presents an opportunity to understand the subsurface characteristics and the salt water composition at the impact’s time.”

Dr. Lesage and colleagues are also researching similar “spiders” on Mars, which are tree-like formations in the regolith near the planet’s south pole.

Their findings on Mars have been applied to other celestial bodies, including Europa.

Martian spiders develop as a result of gases escaping beneath a seasonal dry ice layer; however, the Europa study speculates that the “asterisk-shaped” features could have emerged post-impact.

“Lake stars are radial branching designs that occur when snow accumulates on a frozen lake, creating holes in the ice due to the snow’s weight, allowing water to flow through and spread out energetically,” stated Dr. Lauren McCune from the University of Central Florida and NASA’s Jet Propulsion Laboratory.

“We believe a similar process could have happened on Europa, with subsurface brine erupting after the impact and dispersing through the porous surface ice.”

The research team has informally designated the Europa feature as Damhan Alla, which translates to “spider” in Irish, differentiating it from Martian spider formations.

To validate their hypothesis, they studied lake stars in Breckenridge, Colorado, and conducted field as well as lab experiments using a cryogenic glovebox equipped with a Europa ice simulator cooled by liquid nitrogen.

“In our experiments where we passed water through these simulants at various temperatures, we observed similar star-like formations even at extremely low temperatures (-100 degrees Celsius or -148 degrees Fahrenheit), lending support to the idea that such mechanisms could occur on Europa after the impact,” Dr. McCune remarked.

Scientists also created models showing how the saltwater beneath Europa’s surface would react following an impact, including an animation illustrating the process.

While observations of Europa’s icy features are primarily reliant on images captured by the Galileo spacecraft in 1998, the researchers aim to explore this further with high-resolution images from NASA’s Europa Clipper mission, anticipated to arrive at the Jupiter system in April 2030.

“Although lake stars offer significant insights, terrestrial conditions differ vastly from those on Europa,” Dr. McCune notes.

“Earth possesses a nitrogen-rich atmosphere, while Europa’s environment features extremely low pressures and temperatures.”

“This investigation combined field data and laboratory trials to better simulate Europa’s surface conditions.”

The team will further examine how low-pressure systems affect the formation of these landforms and explore whether such structures can form beneath Europa’s icy crust, akin to how flowing lava generates smooth, rope-like textures known as pahoehoe on Earth.

While the primary focus was geomorphology, this discovery sheds light on subsurface activity and habitability, crucial for future astrobiological studies.

“By employing numerical modeling of saline reservoirs, we assessed the potential depth of the reservoir (up to 6 km, or 3.7 miles below the surface) and its longevity (potentially several thousand years post-impact),” Dr. Lesage stated.

“This data is invaluable for upcoming missions investigating viable ecosystems beneath ice shells.”

The team’s results were published in Planetary Science Journal.

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Lauren E. McCune et al. 2025. A lake star as an Earth analogue of Europa’s Manannan Crater Spider feature. Planet. Science. J 6,279; doi: 10.3847/PSJ/ae18a0

Source: www.sci.news

Three Key Factors That Likely Shaped the Moon’s Formation in Earth’s Early History

The moon may have had a more intricate formation than previously believed.

NASA/NOAA

Recent theories suggest that multiple collisions with Earth might better elucidate the Moon’s origin than the traditionally accepted single massive impact 4.5 billion years ago, potentially addressing one of its greatest enigmas.

Tracing the Moon’s origin has proven challenging. The prevailing theory is that it formed early in the solar system’s evolution due to a catastrophic collision between Earth and Theia, a Mars-sized body, and its formation likely originated closer to the sun than Earth’s current position. This impact would have expelled debris that ultimately coalesced into the large natural satellite we recognize today. At that period, matter around the sun was highly intermixed, making collisions frequent.

However, this prevailing model encounters complications, as the chemical compositions of Earth and the Moon are remarkably similar, suggesting that the Moon should retain more material from Theia than our planet does. “This presents a significant dilemma for the standard model,” comments Philip Carter, a researcher at the University of Bristol, UK.

Carter and his team propose a paradigm shift, suggesting that a series of impacts with Earth over millions of years may provide a more coherent explanation for the compositional similarities between Earth and the Moon. They propose that three or more significant impacts in the early solar system, involving bodies from the size of the modern Moon to those approaching Mars in size, could account for the Moon’s creation as we observe it today.

In this revised model, each impact creates smaller moons, known as microsatellites, orbiting Earth. Over eons, these smaller bodies would progressively merge under gravitational attraction, forming a singular large entity. “They will be drawn to one another and collide,” explains Carter. “The probability of sustaining a stable system with multiple large moonlets is exceedingly low.”

Previous models also posited multiple impacts as the origin of the Moon; however, they typically required a more rigorous series of impacts than this current framework. “After three significant collisions, we introduced sufficient mass into orbit to form a full Moon,” stated Carter.

Robert Citron, a researcher at the Southwest Research Institute in Colorado, suggests that fewer impacts might be more favorable since too many collisions could displace smaller satellites from Earth’s orbit and hinder Moon formation. However, as more impacts occur, the compositional alignment between Earth and the Moon increases, accurately reflecting their current similarities. “When multiple impacts are involved, you are averaging out more influencing factors,” Citron notes.

The unique relationship between Earth and the Moon underscores the necessity of understanding the Moon’s formation. “It is a remarkably distinctive satellite,” Citron emphasizes. “Its size relative to Earth is vast, whereas the moons of Mars appear minuscule in comparison to Mars, and the moons of gas giants are diminutive compared to their planets.”

Establishing which hypothesis is correct necessitates more intricate modeling to assess the impact’s intensity on Earth and the volume of material expelled. Carter remarks, “Calculating all these details remains exceedingly complex.” He adds, “Personally, I prefer the multi-impact model over the traditional single-impact theory.”

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Source: www.newscientist.com

Coral Reefs Triggered Major Global Warming Events in Earth’s History

Corals construct their skeletons from calcium carbonate, releasing carbon dioxide as a byproduct.

Reinhard Dirscherl/Alamy

For the last 250 million years, coral reef systems have been crucial to the Earth’s climate, but perhaps not in the manner you might assume.

Coral reefs generate excess carbon dioxide because the formation of calcium carbonate, which constitutes coral skeletons, involves the release of greenhouse gases.

Certain plankton species utilize calcium carbonate to form their shells, and when these organisms perish, the mineral becomes buried on the ocean floor. In ecosystems dominated by coral, calcium and carbonate ions that typically nourish deep-sea plankton are rendered inaccessible.

Tristan Salles and his team at the University of Sydney conducted a modeling study on the interactions among shallow corals and deep-sea plankton over the last 250 million years, incorporating reconstructions of plate tectonics, climate simulations, and variations in sediment contribution to the ocean.

They determined that tectonic activity and geographic features foster periods with extensive shallow continental shelves, which provide optimal conditions for reef-building corals, thereby disrupting the coral-plankton dynamics.

As the area covered by coral reefs diminishes, calcium and alkali levels accumulate in the ocean, enhancing plankton productivity and increasing the burial of carbonate in the deep ocean. This shift contributes to lower CO2 concentrations and cooler temperatures.

The study revealed three significant disruptions in the carbon cycle over the past 250 million years. During these events—specifically in the Mid-Triassic, Mid-Jurassic, and Late Cretaceous—extensive coral reefs consumed vast amounts of calcium carbonate, resulting in notable ocean temperature increases.

Once the balance between shallow-sea corals and deep-sea plankton is disrupted, realignment can require hundreds of thousands to millions of years, noted Salles.

“Even if the system recovers from a significant crisis, achieving equilibrium will be a prolonged process, significantly extending beyond human timelines,” Salles elaborated.

On a brighter note, Salles observes that corals excel at absorbing excess nutrients to aid in reef building, even if planktonic nutrient growth gets excessive.

Currently, human-induced carbon dioxide emissions are driving unprecedented global warming and ocean acidification, endangering both corals and plankton, according to Salles. While the outcomes remain uncertain, the potential impact on ecosystems could be catastrophic.

“The feedback mechanisms we modeled span deep time and may not be relevant today. The current rate of change is too rapid for carbonate platform feedbacks to maintain similar significance.”

Alexander Skiles from the Australian National University in Canberra remarks that this research illustrates a “profoundly interconnected feedback cycle between ecosystems and climate.”

He suggested that while species are presumed to evolve and adapt to the climatic conditions dictated by “immutable physical and chemical processes,” it is increasingly evident that certain species are actively shaping the climate itself, leading to co-evolutionary feedback loops.

“Beyond corals, ancient microbial colonies like stromatolites have significantly influenced atmospheric carbon regulation,” Skiles pointed out.

“It is well-recognized that carbon is accelerating climate warming at an alarming rate. Corals contribute to this dynamic over extensive geological time, which may elucidate fluctuations between warmer and cooler periods.”

Source: www.newscientist.com

Experts Suggest Earth’s Prehistoric Oceans Might Not Have Been Blue

Our planet has hosted oceans for approximately 3.8 billion years, but their current blue appearance is relatively recent. Research indicates that it hasn’t always been this way.

In the ocean’s depths today, the water appears blue because it absorbs longer wavelengths of sunlight, particularly those at the red end of the spectrum.

This absorption allows shorter, bluer wavelengths to penetrate further and scatter back into our eyes. Billions of years ago, various colors may have masked the blue waters.

During that era, the earliest life forms emerged in the oceans, particularly unicellular cyanobacteria. These organisms were crucial in shaping our planet’s habitability by capturing sunlight energy through photosynthesis, resulting in Earth’s first oxygen availability.

Researchers in Japan have recently developed a computer model demonstrating that the initial oxygen released by cyanobacteria reacted with dissolved iron in the seawater, leading to the formation of oxidized iron that turned the ocean’s surface green.

Moreover, early cyanobacteria likely adapted to thrive in the greenish water.

In their study, scientists engineered cyanobacteria that possess a specific type of photosynthetic pigment responsive to green light, known as phycoerythrobilin.

Japanese researchers created a model showing how early cyanobacteria’s oxygen interacted with dissolved iron, resulting in a green ocean surface. – Image credit: Getty Images

In contrast, most current plants utilize red and blue light through chlorophyll pigments.

In laboratory settings, these modified cyanobacteria were cultivated in tanks filled with green water, revealing a phenomenon that also occurs naturally.

The waters surrounding Iwo Jima in Japan are naturally high in iron oxide, imparting a unique green hue. The cyanobacteria prevalent along its coastlines possess pigments that make use of elevated green light levels.

This study suggests that exobiologists searching for extraterrestrial life should not only consider blue liquid water but also various shades of green that may hint at primitive life forms.


This article addresses the inquiry (by Philip Burke of Somerset): “Has the sea always been blue?”

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Astronomers Unveil Moon Concealed in Earth’s Shadow

Astronomers have identified a peculiar “moon” that casts a shadow on Earth as it navigates through space. Dubbed quasi-moons, these entities don’t orbit our planet in a traditional manner, yet they maintain proximity as they travel around the sun.

According to a new study published in the American Astronomical Society Research Notes, this space rock may have been a companion to Earth for as long as 60 years.

The object, identified as 2025 PN7, is small enough that it might have evaded earlier detections. While its exact dimensions remain uncertain, researchers estimate it to be around 30 meters (98 feet) in diameter—approximately the wingspan of a typical short-haul airliner—making it the tiniest known quasi-moon associated with Earth.







“With rapid technological progress, we’re identifying near-Earth objects faster than ever,” said Dr. Darren Baskill, an astronomy lecturer at the University of Sussex, in BBC Science Focus. “The sensitivity of digital cameras has improved, allowing us to detect these faint objects, and computers can effectively process vast data sets.”

At its closest approach, this object comes within 300,000 km (186,400 miles) of Earth. Usually, it remains about 384,000 km (238,600 miles) away, but its horseshoe-shaped orbit can take it as far as 297 million km (185 million miles) from our planet.

Consequently, it’s only detectable when nearby, as occurred in August 2025, when researchers from Spain’s Complutense University of Madrid spotted it from the PanSTARRS Observatory in Hawaii.

Upon reviewing historical records, scientists identified it as a potential Earth companion for decades.

“The primary question is, where did 2025 PN7 originate?” Baskill noted. “At its closest, 2025 PN7 will be roughly the same distance from Earth as the Moon, providing insights into the Moon’s possible origin.

“Another clue can be observed on a clear night: the Moon is full of craters. Each impact casts debris into the atmosphere, and some material may escape the Moon’s gravity and be launched into space.”

Moon’s craters offer clues to the origin of space rocks – Photo credit: Getty

Another hypothesis suggests that the space rock originated in the asteroid belt, but Baskill states, “It’s challenging to gather sufficient light from such a moving object to determine its chemical composition and origin.”

He further added, “Astronomers must be patient and wait to observe PN7 when it’s at its brightest, closest to Earth.”

2025 PN7 is just one of seven quasi-satellites currently orbiting near Earth. The other is the space rock Kamooarewa, which is the target of China’s Tianwen-2 mission. Launched in May 2025, Tianwen-2 aims to collect samples from asteroids to understand more about Earth’s origins and asteroid formation.

“These near-Earth objects, due to their occasional close passes, might become prime targets for the inaugural mining operations beyond Earth, or even enter Earth’s atmosphere,” Baskill remarked.

PN7 will remain in existence until 2085 when it will be pulled from orbit by gravitational forces.

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Source: www.sciencefocus.com

Breathtaking Images Showcase the Battle to Safeguard Earth’s Diverse Biodiversity

Malaysian tropical longhorn beetle

Kim Hee Yu

“It had an unusual expression, reminiscent of an alien, but it wasn’t hostile. It remained motionless on the branch throughout,” said Kim Hui Yu, the photographer of the long-eared longhorn beetle during a family visit to Gunung Jerai on Malaysia’s west coast.

A light bulb inside the mosquito net drew invertebrates during the night. In the morning, she selected the most vibrant ones for photographs. “I want to raise awareness that every creature, even the tiniest, has its place. So we must protect our forests.”

The image titled alien is one of eight featured in the Natural History Museum’s 2025 Biodiversity Exhibit. Visit the Wildlife Photographer of the Year exhibition, opening in London on October 17th. The collection includes images from past contests.

The exhibit also showcases a large map illustrating biodiversity levels based on the Biodiversity Intact Index developed by museum researchers.

4 month old black rhino calf

Hilary O’Leary

Hannah McCartney, who oversees the contest, emphasizes the significant influence of images. The aim is to motivate viewers to notice and act. A prime example includes Innocent Betrayed by Hilary O’Leary, showcasing a four-month-old black rhino calf interacting with an anti-poaching scout, captured while the calf was lost in the brush.

Berchtesgaden National Park in the German Alps

marc graff

high and wild, captured by Mark Graf, presents a different perspective on the potential losses of nature. This shot shows trees and rocks emerging from sunlit clouds within Berchtesgaden’s national park.

Intimate moments between harlequin toads

Jaime Culeblas

Jaime Culebras’ happy couple captures mating harlequin toads in Colombia’s Sierra Nevada de Santa Marta National Natural Park, home to numerous endangered species.

Caitlin Woods, marine ranger off Lord Howe Island

Justin Gilligan

rich reflections by Justin Gilligan captures marine ranger Caitlin Woods snorkeling among the vibrant seaweed off Lord Howe Island, located between Australia and New Zealand.

Interspecies showdown

Morgan Heim

A close encounter between a pygmy rabbit and a stink bug, both found in rabbit burrows, was captured in burrow mate by Morgan Heim in the Columbia Basin, Washington.

Red kite takes off in the UK

owen hearn

flight path: Owen Hearn’s image juxtaposes the close-up of a red kite with a distant airplane silhouette. This pivotal photo was taken at a Bedfordshire site once selected as London’s third major airport, a project halted due to public opposition. Currently, this location offers a unique vantage point for wildlife photography. While the red kite population has dramatically recovered following its near extinction due to historical persecution, Britain remains one of the most depleted nations in terms of wildlife.

Life beneath the ice off the coast of Antarctica

Laurent Ballesta

Laurent Ballesta’s pyramid of life illustrates the biodiversity thriving beneath East Antarctica’s ice, featuring giant ribbon worms and starfish.

The Wildlife Photographer of the Year competition is celebrating its 61st year, with judges evaluating a record 60,000 entries, compared to just 341 in 1965. Winners will be revealed on October 14th.

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Echoes of Rock: A Personal Exploration of Earth’s Geological History

The rocks lining Britain’s Jurassic Coast are roughly 185 million years old

James Osmond/Alamy

Whispers of Rock
Anjana Khatwa, Bridge Street Press (UK). Basic Books (USA, releasing November 4th)

Stones are often overlooked. How frequently do we consider the materials beneath our feet, or the origins of the beach pebbles we idly collect?

And how often do we recognize the role of geology when discussing nature and our pressing discussions about climate change? Any efforts towards addressing climate change and the future of our planet must include our relationship with the elements that constitute our world.

We are fortunate to gain insights from geoscientist Anjana Khatwa through her latest book, Whispers of Rock: Stories from Earth. This work, described as “an exhilarating journey through deep time,” is a heartfelt tribute that is sure to resonate with readers. Khatwa has dedicated a significant part of her life to promoting an understanding of geology, providing the scientific detail that highlights her profound knowledge.

In this book, she methodically covers topics such as the formation of mountains, craters, and slate, interspersing fascinating anecdotes. For instance, the iconic Taj Mahal of India, a symbol of love, was constructed from ivory-white Makrana marble that dates back approximately 2 billion years, originating from ancient landmass collisions. This complex genesis involved tectonic shifts, cyanobacteria, photosynthesis, and calcium carbonate, all coming together to create the stones used in this magnificent structure.

Once the scientific framework is laid down, Khatwa breathes life into the narrative of rocks and minerals, transforming it into a sensory experience far removed from the geology classes of my past. She invites readers to appreciate the negative spaces carved in Petra, Jordan, which form breathtaking structures and the unexpected beauty found within. She describes the markings on the stone as remnants of an ancient river, illustrating her deep connection to these geological marvels, becoming a “keeper of the stories of time.”


A recipe that involved tectonic movements, photosynthesis, and more resulted in the marble utilized in the Taj Mahal.

Khatwa’s passion for stones began in her childhood, walking on solidified lava flows in southeastern Kenya. Throughout her book, she takes readers on a global journey, including her hometown of Dorset, England, where she enjoyed 20 years of geological history at the Jurassic Coast World Heritage Site.

This adventure reveals how rocks have shaped her life and the lives of many others. We explore the colossal sarsen stones of Stonehenge in England, delve into the science and folklore of New Zealand’s Ponamu greenstone, and trace the socio-political history of the Black Belt, a fertile region in the American South shaped by cotton plantations after the removal of indigenous communities.

However, what truly distinguishes this book is Khatwa’s personal narrative. She openly addresses the lack of diversity in the environmental sector in the UK and shares her experiences as a mother, imparting a sense of vulnerability along the journey.

She reflects on how she was “transformed by the whiteness of my working environment” and came to realize that her cultural and spiritual identity often took a backseat to her scientific persona. This book is essential reading for anyone grappling with that duality or wishing to understand it better. We stand with Khatwa as she navigates the space between belonging and the feeling of being an outsider.

Whispers of Rock is packed with such insight that it requires contemplation after each chapter. Khatwa is also intentionally provocative, acknowledging that the intersection between science and spirituality may make some readers uncomfortable, as it challenges their preconceived notions. Yet, this provocative approach sparks a genuinely enlightening exploration.

Dhurti Shah is a freelance journalist based in London.

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Source: www.newscientist.com

The Mystery of Earth’s Ancient Frozen Nuclei Unveiled: Discovering the Reasons Behind Their Existence

We may finally understand what caused the inner core of the Earth to freeze.

The inner core is a sphere of iron approximately 2,400 km (1,500 miles) in diameter, enveloped by a molten outer core. Its growth is responsible for generating the Earth’s magnetic field, which shields the planet from harmful solar radiation. However, the precise process by which the core first crystallized has remained unclear.

Recent research published in Nature Communications suggests a mechanism that hinges on deep Earth chemistry. By utilizing advanced computer simulations, scientists examined how various factors influence the freezing of iron under extreme pressure and temperature at the planet’s center.

They found that incorporating carbon allows iron to solidify under realistic conditions, positioning it as a key component in understanding the ingredients that contributed to the formation of the inner core billions of years ago.

“By investigating how Earth’s inner core formed, we gain insights not only into the planet’s history,” said Dr. Alfred Wilson from the University of Leeds, who led the study.

“We get rare insights into the chemistry of a region that we can never physically reach, and we can only speculate on how it might change in the future.”

The inner core lies deep within the planet, beneath layers of rock and magma – Credit: Getty Images/EPS Vector

At the extreme pressures found 5,000 km beneath our feet, iron doesn’t simply freeze when it drops below its melting point; it requires “super-cooling” of the crystals before they form. Pure iron must be cooled to as low as 1,000°C (1832°F), resulting in a significantly larger core than the one we see today.

New computer modeling indicates that the presence of carbon alters this equation. With less than 4% carbon in the mix, iron can crystallize at much lower temperatures, producing a core that aligns with seismic observations.

Scientists believe that the Earth’s center likely continues to host a mixture of elements. However, this research firmly highlights the critical role of carbon in one of geology’s greatest mysteries.

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Source: www.sciencefocus.com

Experts Predict Continued Recovery of the Earth’s Ozone Layer for Decades Ahead

The ozone layer has shown significant improvement, with the Antarctic ozone holes in 2024 being smaller than in prior years. New Report from the World Meteorological Organization (WMO).

This map depicts the size and shape of the Antarctic ozone hole on October 5th, 2022. Image credit: Earth Observatory by Joshua Stevens/NASA.

The depth of the Antarctic ozone hole in 2024 (which typically appears every spring) was below the average levels measured from 1990 to 2020, with the maximum ozone mass deficit recorded on September 29th at 46.1 million tons.

From 2020 to 2023, it remained smaller than a significantly larger hole.

Its development was relatively gradual, with ozone depletion slowing by September, followed by a quicker recovery after reaching the maximum deficit.

“This consistent progression is considered a strong indicator of early recovery in the Antarctic ozone holes,” stated WMO experts.

The alarm was initially sounded by scientists in 1975 when the WMO reported “changes in the ozone layer due to human activities and certain geophysical factors.”

If current policies remain in effect, the latest assessment for 2022 indicates that the ozone layer is projected to return to 1980 levels (prior to the appearance of ozone holes) around 2066, 2045 in the Arctic, and globally by 2045.

“Despite the significant success of the Montreal Protocol over the years, this effort remains ongoing, and continuous monitoring of stratospheric ozone and ozone-depleting substances is essential,” experts noted.

“WMO’s scientific research on the ozone layer spans decades,” remarked Celeste Sauro, WMO executive director.

“It relies on trust, international collaboration, and a commitment to free data exchange—fundamental principles of the world’s most successful environmental agreements.”

“To date, the Montreal Protocol has resulted in over 99% reduction in the production and consumption of controlled ozone-depleting substances used in refrigeration, air conditioning, fire foam, and even hairsprays.”

“Consequently, the ozone layer is on course to recover to 1980 levels by the middle of this century, significantly lowering the risk of ecosystem damage from skin cancer, cataracts, and UV overexposure.”

Source: www.sci.news

Mars Once boasted a Thicker Atmosphere Than Earth’s Today

Modern Mars has a minimal atmosphere

NASA/JPL/USGS

Mars’ atmosphere may have once been far thicker, providing a protective layer against the frequent asteroid impacts that destroyed other celestial bodies.

Our solar system began forming around 4 billion years ago, and by that time, Mars was nearly fully developed. The planet existed within a vast reservoir of hot gas and dust swirling around a youthful sun, known as the solar nebula, which some planets absorbed into their atmosphere. However, it was believed that as the solar nebula dissipated, Mars would lose this gas, resulting in a thinner atmosphere.

Recently, Sarah Jollett from Paris’ Collège de France and her team propose that Mars retained this gas for a longer period, forming a primordial atmosphere akin to a sustained soup.

Shortly after the nebula receded, it was believed that the orbits of significant planets like Jupiter and Saturn influenced each other, subsequently disturbing the paths of comets and asteroids that headed towards the inner solar system, impacting rocky planets. While chemical signatures of these impacts can be found on Earth, evidence on Mars remains limited.

“All terrestrial planets faced bombardments from comets during this time, and Mars was no exception, so we should observe remnants of this cometary assault on Mars,” Jollett stated at the Europlanet Science Congress held on September 11th in Helsinki, Finland.

Jollett and her colleagues suggest that the dense, hydrogen-rich atmosphere during this era may have diluted comet material that was available for absorption by Mars. By running simulations of the early solar system, they estimated the potential amount of material impacting Mars and compared it to the detectable quantity. They deduced that the original Martian atmosphere had a mass equivalent to 2.9 bars, around three times the atmospheric pressure we experience on the surface today.

However, this atmosphere dissipated relatively swiftly over about a million years, according to Raymond Pierre Hambart from Oxford University, who was not involved in the study. This loss primarily occurred before liquid water could come to the surface of Mars. The necessary clear atmospheric conditions, rich in carbon dioxide, were likely not present in that thick primordial atmosphere.

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The Extinction of a Dinosaur: A Dramatic Transformation of Earth’s Landscape

Large dinosaurs such as Titanosaurus significantly influenced their ecosystems

Christian Jegou/Science Photography Library

The extinction of dinosaurs had profound consequences for Earth, leading to significant alterations in the planet’s landscapes, including shifts in river systems.

There is a clear distinction between various rock formations in North America before and after the end of the dinosaurs during the Cretaceous-Paleogene (K-PG) extinction event approximately 66 million years ago, triggered by the Chicxulub asteroid impact in the Yucatan Peninsula.

For example, the Green Gray Mudstone, recognized as the Hell Creek Formation from the dinosaur period, transitions into the more vivid pajama-striped layers of the Fort Union Formation, which hosts many lignite-rich charcoals from plant material that surfaced with the rise of mammals.

This transition was initially attributed to the direct impacts of asteroid strikes, such as increased rainfall. However, Luke Weaver from the University of Michigan and his team propose another explanation.

They examined floodplain areas in the western United States, revealing abrupt geological changes around the K-PG boundary, particularly in the Williston Basin, stretching across parts of Wyoming, Montana, and the Dakotas.

The multifaceted colorful layers from the Post-dinosaur period are believed to be deposits formed by rising water levels, creating temporary ponds. However, Weaver and his colleagues did not find supporting literature on water level changes during this era.

“There’s no evidence of extremely high water tables or particularly wet conditions,” he says. While there was an intrusion of seawater inland, the nearest instance occurred at least 300,000 years after the K-PG boundary.

Weaver’s team argues that significant sandstone layers formed post-K-PG boundary are indicative of large, stable rivers, known as Point Bar deposits, instead of temporary pond deposits. These layers can exceed 10 meters in thickness, reflecting the stability of these rivers.

Researchers attribute these findings to the extinction of dinosaurs. They propose that, like today’s large herbivores, dinosaurs were ecological engineers, disrupting vegetation, trampling, and grazing seedlings, inhibiting new plant growth.

“These creatures were colossal compared to modern fauna,” Weaver notes. For instance, while a contemporary elephant weighs around 5,000 kilograms, a Triceratops could weigh at least double that.

As they moved through and destroyed vegetation, the rivers would have flooded periodically instead of winding through forests. This change ultimately led to the expansion of marshy mudstone, according to Weaver. Once the dinosaurs vanished, tree roots stabilized the sediments, allowing water to flow through a meandering riverbed, thus creating point bars.

“This illustrates a landscape where biology plays a crucial role,” Weaver observes. Animals, he argues, significantly modify their environments, much like humans have drastically altered Earth’s landscapes.

Christopher Doughty from Northern Arizona University believes this perspective better explains the observed geological transformations than earlier theories. “In contemporary studies where large animals are removed from ecosystems, tree cover significantly increases,” he mentions. “With the extinction of dinosaurs, there were no longer large animals capable of uprooting trees. This led to a decrease in herbivory and reduced the disturbance of seedlings giving rise to robust tree growth.”

However, Cat Schroder from the University of New Mexico remains skeptical. “While there seems to be a correlation between large dinosaurs and open nutritional landscapes, causality hasn’t been established yet,” she says. “Forests thrived before, during, and after the age of dinosaurs.”

Doughty is using isotopic analysis of fossil leaves to investigate how forest structures have shifted since the dinosaurs went extinct.

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Strata Review: Unveiling the Captivating Narratives in Earth’s “Boring” Layered Rocks

Rock layers reveal insights into our planet’s deep past, such as these in Canada

Paul Andreassen/Alamy

hierarchy
Laura Poppick (WW Norton)

The narrative of Earth is one of transformation. Over 4.5 billion years, our planet has evolved from a scorching mass of molten rock and poisonous gases into a temperate and vibrant habitat teeming with diverse life forms. This evolution was punctuated by pauses, restarts, and cataclysmic events, as the intricate biogeochemical processes shaped the most extraordinary phases in Earth’s history.

Our understanding of this vast tale is largely thanks to rocks. They preserve the chronology of events that contributed to the surface’s stratification through various deposits. This intricate ordering is understood through hierarchies, and the scientific discipline dedicated to interpreting them is known as stratigraphy.

In Strata: A Story from Deep Time, journalist Laura Poppick delves into this nuanced science of rock interpretation, offering insights on how planets respond to and recover from periods of upheaval. “Through these layers, we glimpse ancient versions of our planet, gaining contextual awareness as we traverse through the present,” she observes.

Poppick highlights several transformative periods in Earth’s history, selecting four key episodes. The first examines the development of oxygen-rich atmospheres, tracking the evolution of photosynthesizing microorganisms and significant oxidative events that led to mass extinctions around 2.4 billion years ago.

The second segment discusses “Snowball Earth,” a period approximately 720 million years ago when many regions are believed to have frozen over. Following this, she explores the advent of mud and the subsequent rise of vegetation. Finally, the Mesozoic era, dominated by dinosaurs, records atmospheric carbon dioxide levels much higher than today’s due to volcanic activity, offering a framework to understand planetary responses to climate shifts.


Sedimentary rocks maintain a distinct layer system that clearly records the events that have shaped our planet’s surface.

Throughout each episode, Poppick introduces geologists working to unravel the numerous unanswered questions regarding the timing and causes of these changes. She visits significant geological sites, from Newfoundland to the Australian Outback, where one can observe the strata that articulate these narratives.

The recurring theme emphasizes the importance of paying attention to rocks. To an untrained observer, they may appear ordinary; however, Poppick reminds us that “a trained eye discerns physical and chemical indicators—proxies—that reveal the characteristics of our planet during the formation of these rocks.” She underscores the value of geologists’ expertise.

This book is a remarkable attempt to make stratigraphy engaging. At times, it falters, and Poppick’s fragmented writing style led me to lose the thread of the narrative.

Her comparisons of geological transformations to human-centric changes sometimes felt uneasy. For instance, she likens the Mesozoic greenhouse climate to modern carbon emissions, though the historical era’s temperatures were so extreme that such analogies may be misleading, even at optimistic emission projections.

Another limitation lies in the currently incomplete nature of geoscience. Some of the pivotal questions raised by Poppick—including the true cause of Snowball Earth—remain unresolved or are subject to debate among different factions. By the end, I was left with a sense of uncertainty about what can be definitively stated. Yet, that unpredictability might be intrinsic to geology itself. “Nothing is immutable in stone as our understanding of geology continues to evolve, just like the rocks,” Poppick states.

Nevertheless, the book effectively captures the grandeur of the story embedded in rocks. It does so particularly well by showing how seemingly mundane observations about rocks can lead directly to profound insights into Earth’s history. Such revelations illuminate the stratigraphic process as Poppick examines overlooked outcrops, encouraging us to perceive the rocks in our surroundings with renewed appreciation.

“Hierarchies are, in many ways, love letters from a maturing Earth,” she argues. This book abundantly reveals the reasons to uncover the secrets they hold.

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Climate Change Feedback Loops Are Degrading Earth’s Carbon Sinks

Wildfires in Greece are diminishing the Earth’s natural carbon sink

Thanassis Stavrakis/AP Photo/Alamy

Climate change is increasingly compromising the ability of the Earth’s natural carbon sinks to absorb excess carbon dioxide. This results in greenhouse gases emitted by human activity lingering in the atmosphere, contributing to further warming.

These feedback loops account for roughly 15% of the rise in CO2 levels since 1960, according to Pierre Friedlingstein from the University of Exeter, UK.

The land and oceans serve as carbon sinks, absorbing nearly half of the extra CO2 produced by humans. While higher CO2 levels can enhance plant growth, leading to greater CO2 uptake by vegetation, extreme temperatures, droughts, and wildfires associated with global warming can counteract this CO2 fertilization effect.

Friedlingstein is part of the Global Carbon Project, which aims to clarify the amounts of CO2 being emitted, how it is absorbed by different sources, and how this process evolves over time. Previously, his research team used climate models to project a 27% increase in land sinks in the absence of drought or other feedbacks.

His latest estimates have adjusted this figure to 30%, as he shared at the Exeter Climate Conference last month. He mentioned that ocean sinks also increase CO2 by 6% without feedback effects.

Together, land and oceans contribute over 15% of atmospheric CO2. Since 1960, CO2 levels have surged to around 100 parts per million (ppm), indicating that 15 ppm can be traced back to the feedback effects impacting the sinks. “The sink hasn’t collapsed, but its recovery is slow,” Friedlingstein noted.

There remains uncertainty regarding the sink’s capacity, as David Armstrong McKay from the University of Sussex has observed. “It aligns with expectations, but it’s not encouraging news that we’re marginally off what we projected,” McKay stated. “As warming intensifies, it will challenge land sinks’ adaptability to increased CO2, with extreme events like the recent El Niño-enhanced drought hampering the positive effects on vegetation growth.”

The pressing question is what will unfold next. With the rise in warming, droughts, and fires, research has indicated that land sinks have made minimal net CO2 contributions in the past two years.

This has raised concerns that the effectiveness of land sinks might significantly decrease in the near future, opposing the gradual decline most climate scientists anticipate.

Nonetheless, Friedlingstein referred to these short-term fluctuations as “blips” that may not accurately predict future trends. “What we should focus on is the long term,” he emphasized.

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Niger Probes $5 Million Sale of Earth’s Largest Martian Rock

Dakar, Senegal – the largest meteorite discovered on Earth – a 54-pound (25 kilograms) rock that fetched over $5 million at a New York auction last month, setting a world record.

However, in a West African nation where rusty red rocks have been excavated from the Sahara desert, authorities have initiated an investigation into what they describe as “illegal international trafficking,” suggesting it may have been smuggled from the country.

Here’s what you should know about meteorites and legal controversies:

How was it discovered

According to Sotheby’s, the rock, designated NWA 16788, was dislodged from the surface of Mars by a massive asteroid collision and journeyed 140 million miles (225 million kilometers) to Earth.

It was uncovered in the Sahara, northwest Niger by an unnamed meteorite hunter in November 2023, as per the auction house’s report. The identities of buyers remain undisclosed.

In the arid regions of the Sahara like Niger, meteorite hunting is on the rise. While meteorites can fall anywhere on Earth, the Sahara has emerged as a prime location for their discovery due to its climate, which is conducive to conservation.

Hunters often seek space rocks to sell to collectors and scientists. The most coveted and valuable meteorites are from Mars and the Moon.

As reported by the Heritage Academic Journal, the rock was sold to international dealers and eventually made it to a private gallery in Italy. Last year, a team of scientists from the University of Florence examined the rock to determine its structure and origins before it fell to Earth.

The meteorite was briefly showcased in Rome before appearing at the New York auction last month.

Why Niger is investigating

Following the sale, Niger raised concerns about how the meteorite was made available for auction.

Last month, the Niger government launched an inquiry into the discovery and sale of meteorites, stating that it resembles “illegal international trafficking.”

Last week, President Abdullah Hamanetiani halted the export of precious stones, semi-precious stones, and meteorites to ensure proper traceability.

In a statement to the Associated Press, Sotheby’s maintained that the meteorite was exported from Niger and transported in line with all applicable international regulations.

“In selling this item, all necessary documentation was obtained at each stage of the journey, consistent with best practices and the requirements of the involved countries,” the statement indicated.

Niger authorities did not respond to inquiries from the Associated Press.

What international law says

Patti Garstenblis, a cultural heritage attorney and expert on illegal trade, noted that rare minerals like meteorites are recognized as cultural property under the UNESCO Cultural Property Treaty, which both Niger and the United States have ratified.

However, Garstenbliss pointed out that Niger needs to establish ownership and that the meteorite was stolen.

“I doubt Niger could reclaim the meteorite if it wasn’t stolen and was properly declared upon entering the U.S.,” she stated to the Associated Press.

Paleontologist Paul Sereno, who has spent years uncovering dinosaur fossils in Niger’s Sahara, is advocating for the return of the nation’s cultural and natural heritage, including meteorites.

“When laws clearly state that rare minerals like meteorites are cultural artifacts, unique and valuable items cannot just be claimed without consideration for the country,” he told the AP.

“We are no longer in a colonial era,” he added.

In certain countries, including Morocco, a major source of meteoritic specimens for international markets, if an object is found on their territory, compensation is required. Nonetheless, due to the expansive desert regions and the informal trading networks, enforcement remains challenging.

Source: www.nbcnews.com

Unlocking the Mysteries of Earth’s Extraordinary Deep Biosphere: Our Next Great Frontier

Microbial life thrives in this thermal vent in the Pacific Ocean

Galih/Alamy

Within the Earth
Karen G. Lloyd (Princeton University Press)

While many shelves are filled with titles about forests, oceans, and deserts, the deep biosphere, an important and intriguing habitat beneath our feet, is often overlooked. Despite a few notable exceptions, literature on ecosystems ranging from the Amazon to Antarctica largely ignores this underground world.

Not anymore. Within the Earth: Discover the Strangest Life on Earth by Karen G. Lloyd serves as a crucial field guide to the underground life we’ve started to uncover. “In fact, we have yet to find the limits of where life ceases to exist,” she states.

The general unawareness of the deep biosphere’s existence reflects our surface-centric worldview. However, Lloyd, a microbial biogeochemist at the University of Tennessee, Knoxville, argues that learning about this life can profoundly change our understanding of existence itself.

She defines the deep biosphere as areas below the seafloor or beneath land where life thrives without sunlight, the primary energy source for most surface organisms. These environments encompass a variety of metabolic processes, from methane production arising from decomposed plants beneath a few centimeters of marsh mud to chemical processes with microbes three kilometers underground.

Discussing these microorganisms, she notes, “It’s as if there are millions of small, low-energy suns scattered throughout the Earth’s crust, each supporting its own underground ecosystem.”

How much life is present? It’s difficult to say. However, Lloyd contends that all estimates are likely underestimated. One claim suggests that marine sediments alone could hold 2.9 x 1029 cells, potentially twice as many as those in continental fractures and pores, presenting astonishing figures.

Advances in genetic sequencing and field research are illuminating these rich ecosystems. Lloyd helps researchers differentiate between microbial species and deduce metabolic functions through DNA alone. This is especially helpful since many deep-dwelling bacteria and archaea have proven impossible to cultivate in surface laboratories.

It’s like a movie. Be careful not to slip on the volcanic glass shards. Don’t fall into the acid lake!

The fieldwork section discusses how scientists obtain new DNA samples—whether from hydrothermal vents, excavated continental rocks, or dripping water in deep mines. “To understand limits, one sometimes must become the explorer,” Lloyd notes.

Through engaging prose, she recounts her adventures tracking microorganisms from the high deserts of the Andes to the perilous peaks of Costa Rican volcanoes. These stories resemble scenes from action films—caution is essential to avoid slipping on volcanic glass fragments or falling into acid lakes!

Fortunately, this book transcends a mere expedition narrative. It features an extensive and approachable explanation of the chemistry that enables a deep biosphere. Although the equations involved can be complex, Lloyd adeptly guides readers to grasp the chemical frameworks that support these creatures living on the “edge of energy.”

To facilitate this challenging learning curve, she draws parallels between surface ecosystems and our dietary habits to illuminate the underground world. For instance, bacteria that metabolize sulfides are likened to “couch potatoes,” competing with methane-producing “freeloaders” by preserving hydrogen, a universal nutrient—a dramatic ecological narrative reminiscent of the Serengeti. Sulfate-reducing agents in Svalbard’s fjords “have access to a permanently stocked refrigerator.” Engaging and thrilling, her exploration of biogeochemistry is no small feat.

However, the highlight of Lloyd’s book is her assertion that certain forms of deep life may possess a sluggish metabolism, allowing individuals to survive for thousands, or even millions of years. These “eonophiles” (once confirmed to have extraordinarily long life spans) “redefine our preconceived notions about the nature of life,” she asserts. Truly, these lifestyles are alien, and how fortunate we are to uncover more about them right here on Earth!

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Surviving and Thriving in One of Earth’s Most Hostile Environments

Marine tube worms in deep-sea habitats

The deep-sea environment is largely dominated by marine tube worms

Institute of Deep Sea Science and Engineering, CAS

Over 9,500 meters of ecosystems fueled by chemicals from tectonic plate interactions have been uncovered beneath the northwest Pacific Ocean.

“Their resilience and beauty captivated me,” says Mengrand Du from the Chinese Academy of Sciences in Sanya. “The striking crimson tentacles unfurl like delicate blossoms of the trench.”

Du and her team undertook 24 dives between July 8 and August 17, 2024, exploring 2,500 kilometers west of the Krill Kamchatka trench and Aleutian trench, at depths ranging from 5,800 to 9,533 meters. In a frozen section beyond 6,000 meters deep, the Hadal zone experiences crushing pressure and is devoid of light.

This region is referred to as the Hadal biosphere, which derives energy from nutrients descending from surface photosynthesis or exists via chemical bonds relying on chemicals as energy sources.

Taxonomic and genetic data gathered during the dives indicated that many organisms in the Hadal zone utilize compounds such as hydrogen sulfide and methane, which are released through fault lines formed as tectonic plates slide against each other.

“We have discovered a chemically-synthesized community thriving at an astonishing depth of 9,533 meters,” Du states. These findings, made during 19 dives, illustrate their extensive distribution.

The chemically-driven community was primarily composed of bivalve mollusks and marine tube worms known as ciboglinid polychaetes. Some populations consisted of thousands of individuals, sprawling for kilometers.

Numerous bivalve mollusks are also present.

Institute of Deep Sea Science and Engineering, CAS

A notable characteristic of many of these organisms is their dependence on chemical energy rather than sunlight, according to Du. “While other organisms, such as sea cucumbers and amphipods, might inhabit greater depths, they cannot harness chemicals like hydrogen sulfide for energy and must rely on organic matter instead.”

This finding indicates “the deepest and most extensive known chemical synthesis community on our planet.”

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Ancient Rocks Reveal the First Signs of Earth’s Structural Activity

The Pilbara Craton in Western Australia features rocks that date back 3.5 billion years.

Elizabeth Czitronyi / Alamy

Rocks from Australia reveal that tectonic plates were shifting as far back as 3.5 billion years ago, a breakthrough that alters our understanding of the onset of plate tectonics over subsequent hundreds of millions of years.

Currently, along with roughly eight major hard rock plates on Earth’s surface, several smaller plates are interacting with the softer rock layer beneath. When these plates’ edges grind against one another, it can lead to sudden geological upheavals, such as earthquakes, and gradual processes like mountain range formation.

However, there is disagreement among geologists regarding the configurations of these ancient plates and their movements. Some researchers claim to have found indications of tectonic activity as far back as 4 billion years ago when the planet was significantly hotter; others argue that more compelling evidence is noted after 3.2 billion years ago.

Much of this data derives from the chemical compositions of rocks, which suggest past movements. Despite this, records detailing the interactions of early plates remain scarce, which is regarded as critical evidence supporting plate tectonics.

Recently, Alec Brenner and his team from Yale University claim to have uncovered substantial evidence of relative plate movement dating back 3.5 billion years in the eastern Pilbara Craton of Western Australia. They traced the magnetic orientation of rocks aligned with Earth’s magnetic field, observing shifts similar to how a compass needle changes direction when the ground moves.

Brenner and colleagues initially dated the rock using radioisotope analysis, establishing that at certain times, the rock’s magnetism remained unchanged. By observing this magnetization shift, they demonstrated that the rock mass progressively moved at a rate of several centimeters each year. They compared these findings to similarly examined rocks in the Barberton Greenstone Belt in South Africa, which exhibited no such movement.

“This suggests that some type of plate boundary must exist between these two regions to accommodate that relative movement,” remarked Brenner during his presentation at the Goldschmidt Geochemical Conference in Prague, Czech Republic, on July 9.

“Approximately 3.8 billion years ago, the Pilbara plate transitioned from medium to high latitudes, eventually reaching proximity to Earth’s magnetic poles and, possibly millions of years later, to the latitude of Svalbard.”

“If two plates are moving relative to one another, there must be various dynamic interactions happening between them,” noted Robert Hazen from the Carnegie Institute of Science in Washington, DC. “It cannot be an isolated event.”

Nonetheless, multiple interpretations exist regarding the underlying causes of this movement, according to Hazen. The variability in plate movement rates adds to the confusion, and existing data could align with various theories regarding Earth’s interior structure at that time.

At the very least, this discovery indicates the presence of structural boundaries, according to Michael Brown from the University of Maryland. However, he argues that the nature of rock movement appears dissimilar to contemporary understanding of plate tectonics. “Essentially, the Pilbara plate moved to higher latitudes to prevent stagnation, which is atypical within any current plate structural model.”

Brown posits that this aligns with the theory suggesting the Earth’s crust consisted of numerous smaller plates propelled by a thermal mantle plume during that period. He believes the remnants of these small plates examined by Brenner and his team provide evidence of movement; however, due to their limited representation of the crust, they may not accurately reflect broader Earth movements.

Brenner’s team also discovered indications that the Earth’s magnetic field underwent reversals around 3.46 billion years ago. Unlike today’s magnetic field reversals, which occur every million years, these ancient magnetic shifts seemed to happen much more frequently, over spans of tens of millions of years. This could imply a fundamentally different set of energies and mechanisms at play, as noted by Brenner.

Hazen emphasized that the scarcity of magnetic data leads to ongoing debates about the state of Earth’s magnetic field during that era of its evolution. “I believe this discovery raises the bar significantly,” he asserts. “It represents a vital breakthrough in understanding early magnetic reversals, shedding light on the core’s geomechanics in ways previously unexplored.”

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Source: www.newscientist.com

Unique Plants Aid in Reconstructing Ancient Earth’s Climate

Smooth equestrian plants have split stems

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The peculiar plants that existed since the dawn of terrestrial animals can process water to remarkable extremes, resembling water from metstones more than typical groundwater. Not only do they play a crucial role in today’s ecosystems, but their fossilized remnants also provide insights into Earth’s ancient climate and hydrological systems during the age of dinosaurs.

Almost every oxygen atom in water contains eight neutrons, though some rare heavy isotopes possess nine or ten neutrons. When water evaporates, lighter isotopes do so more readily than their heavier counterparts, leading to predictable shifts in their ratios. Researchers can utilize this information to trace the origin of a specific water sample, determining whether it originated from groundwater, fog, or the rate at which it traversed through plants and the humidity levels experienced by those plants in the past.

Nevertheless, due to the minimal presence of heavier isotopes, acquiring reliable data on how these ratios fluctuate can be quite challenging, making it hard for scientists to draw definitive conclusions.

During examinations of water samples from desert flora and fauna, Zachary Sharp from the University of New Mexico and his colleagues discovered discrepancies between the observed data and the anticipated outcomes based on laboratory models.

Sharp and his team believe they have addressed the issue through a remarkable plant known as horsetail, which has been on Earth since the Devonian period approximately 400 million years ago and features segmented, hollow stems. “It’s a tall cylinder with countless holes, evenly spaced, a marvel of engineering,” states Sharp. “We couldn’t replicate this design in our lab.”

As water flows through each segment of the horsetail stem, it undergoes a process of repeated distillation. Sharp and his colleagues collected water samples at various points along the smooth idiot stem (Equisetum) cultivated near the Rio Grande in New Mexico.

By the time the water reaches the top of the stem, its isotopic composition markedly differs from other terrestrial waters. “If you encounter this sample, I suspect it originates from metstone, as it doesn’t come from Earth. [The oxygen isotope ratios],” Sharp remarked during a presentation at the Goldschmidt Geochemical Conference in Prague, Czech Republic, on July 7.

These horsetail analyses enable Sharp and his team to ascertain the variations in the water’s isotopic ratios under near-ideal conditions, allowing them to enhance model accuracy with these values.

By reassessing desert plant data with these refined models, previously inexplicable observations suddenly made sense. Sharp posits that these findings could illuminate other challenging observations, especially in arid regions.

Reaching heights of 30 meters, far surpassing today’s descendants, ancient horsetails provide even more extreme isotopic ratios and could serve as a key to understanding ancient water systems and climates, according to Sharp. Small, sand-like grains known as plant stone threads within horsetail stems can endure to the present day and may feature unique isotopic signatures influenced by atmospheric humidity. This factor affects the evaporation rate. “This could serve as a paleofat meter [humidity indicator]—how fascinating,” Sharp concludes.

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Source: www.newscientist.com

Fresh Challenge: Lowering Earth’s Temperature


Unwanted Thoughts

Sometimes our minds become cluttered with confusing thoughts. What can we do when we’re unable to release them? Here are some tips to manage these thoughts and soothe your mind:

Pups vs. Parenting

In recent years, many individuals have opted for furry companions over raising children. When it comes to achieving happiness, which is preferable: owning a dog or raising a child?

Asteroids and the Apocalypse

Meet the dedicated scientists, astronomers, and mathematicians who tirelessly monitor the skies, keeping a watchful eye on asteroids that could threaten our world.

Feelings of Isolation

Loneliness encompasses the negative emotional state we experience when we lack sufficient personal time. While social interactions are essential, carving out quality time for yourself can significantly lower stress levels.

Plus

  • Eliminate Fluoride from US Water: US Health Secretary Robert F. Kennedy Jr. has urged the CDC to cease recommendations for water fluoridation. Dental experts express concerns about potential impacts on oral health. Explore the facts.
  • Cyborg Advancements: Imagine a future where humans possess extraordinary strength, enhanced vision, and the ability to fly—it may sound far-fetched, but it’s already in progress. Discover the leading “cyborg technology” that will soon be commercially available.
  • Q&A: This month’s burning questions answered! Can animals become intoxicated? What’s the best way to use a defibrillator? What are tufted ground squirrels? How much exercise do you require? Do you really control my blood pressure? What if a Super Collider were built around the moon? What’s the ideal sleeping position? How do you combat compassion fatigue? Are there other sites akin to Stonehenge? And more…

Issue 421 Available on Tuesday, July 8th, 2025

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Source: www.sciencefocus.com

How Ancient Mass Extinctions Revealed Earth’s Evolution into a Super Greenhouse

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Current forest die-offs due to global warming resemble those from the Permian and Triassic extinction events.

Ina Fassbender/AFP via Getty Images

Following a dramatic increase in carbon dioxide levels 252 million years ago, the death of forests resulted in enduring climate alterations, with the greenhouse effect persisting for millions of years.

Researchers striving to comprehend this phenomenon, which triggered the largest mass extinction in Earth’s history, caution that ongoing greenhouse gas emissions may lead to similar outcomes.

The extinction events of the Permian and Triassic are believed to have been triggered by extensive volcanic activity in what is now Siberia, elevating atmospheric CO2 concentrations.

The planet’s surface temperature soared by as much as 10°C, with average temperatures in the equatorial regions climbing to 34°C (93°F)—a rise of 8°C above the current average.

These extreme conditions persisted for roughly 5 million years, causing over 80% of marine species and upwards of 70% of terrestrial vertebrate families to become extinct, according to some estimates.

Although some scientists have recently posited that these mass extinction events may have limited effects on terrestrial ecosystems, Andrew Meldis from the University of Adelaide expresses confidence that life was nearly extinguished 252 million years ago.

“Small pockets of life might survive mass extinctions in isolated enclaves, but many areas within the Permian-Triassic fossil record reveal a complete ecosystem collapse,” notes Meldis.

He and his team scrutinized the fossil record to investigate why the Super Greenhouse event, which drives mass extinction, lasted five million years—far longer than the 100,000 years predicted by climate models.

The findings revealed that vast expanses of forests, originally with canopies of around 50 meters, were supplanted by resilient underground flora, typically ranging from 5 cm to 2 meters in height. Additionally, peat marshes, significant carbon storage ecosystems, vanished from tropical areas.

Employing computer models of Earth’s climatic and geochemical systems, researchers indicated that the depletion of these ecosystems contributes to elevated CO2 levels persisting for millions of years. This predominantly occurs because vegetation plays a crucial role in weathering, the mechanism that extracts carbon from the atmosphere and sequesters it in rocks and soil over extensive timescales.

With atmospheric CO2 levels rising rapidly, the parallels to the present are striking, asserts Meldis. As temperatures escalate, tropical and subtropical forests may find it increasingly challenging to adapt, potentially surpassing thresholds where vegetation ceases to maintain climate equilibrium.

Meldis explains that simply restoring former ecosystems will not lead to a “ping-pong effect.” He emphasizes that the atmosphere cannot be swiftly rejuvenated after the loss of the equatorial forest.

“You’re not transitioning from an ice house to a greenhouse and then back; the Earth will find a new equilibrium, which may differ significantly from prior states,” he elaborates.

Catlin Maisner, a researcher at the University of New South Wales—who was not involved in the study—describes reconstructing these events as analogous to “trying to assemble a jigsaw puzzle with many missing pieces,” yet acknowledges the team’s arguments as “plausible.”

However, she notes considerable uncertainty regarding oceanic processes during this period. “The ocean harbors far more carbon than land and atmosphere combined, and we still lack a comprehensive understanding of how marine biology, chemistry, and physical circulation were affected during that event,” cautions Meissner.

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  • Paleontology

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Source: www.newscientist.com

Canada’s Nuvvuagittuq Greenstone Belt Contains Fragments of Earth’s Oldest Crust, Research Reveals

Geologists have found significant evidence indicating the preservation of Hadean Rocks, with an age of 4.16 billion years. The Nuvvuagittuq Greenstone Belt offers a rare glimpse into the early Earth.



Canadian Nuvvuagittuq Green Stone Belt. Image credit: Jonathan O’Neill.

The earliest geological history of Earth remains largely unclear due to the scarcity of rocks and minerals from the Hadean period (over 4.3 billion years ago).

These ancient materials are often altered or destroyed as the planet’s crust undergoes continual recycling through various geological processes.

“One potential survivor of the Hadean era crustal rock is the Nuvvuagittuq Greenstone Belt,” stated Dr. Christian Saul, a senior author from the University of Ottawa and his colleagues.

“However, this perspective is contentious. Some researchers argue that the isotopic data backing these estimates might instead reflect later geological mixing rather than the true age of the layers.”

“If proven to be of Hadean origin, the Nuvvuagittuq Greenstone Belt would represent the oldest known preserved rock sequence on Earth.”

“This could yield critical insights into early geology and possible environments for the emergence of life.”

To refine the age of the Nuvvuagittuq Greenstone Belt, researchers concentrated on specific types of ancient rock intrusions known as metagabbro within the belt.

These intrusions intersect with ancient basaltic rocks, enabling the authors to utilize combined uranium-lead (U-Pb) dating to determine the minimum age limits of older layers, along with both short and long-lived samarium-neodymium (Sm-Nd) isotopic analysis.

Sm-Nd data yielded a consistent age of approximately 4.16 billion years, irrespective of the sample location or mineral composition.

The convergence of both isotope systems producing the same age in rocks with clear evidence of magma differentiation strongly supports their Hadean era crystallization.

This is in accordance with the Hadean Eon surviving within the Nuvvuagittuq Greenstone Belt.

“Studying these rocks allows us to trace back to the origins of our planet,” noted Dr. Jonathan O’Neill, a researcher at the University of Ottawa.

“This will enable us to gain a better understanding of how the first continent formed and help reconstruct the environment in which life emerged.”

Survey results published in the journal Science.

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C. Sole et al. 2025. Evidence of Hadean Mafic invasion in the Canadian Nuvvuagittuq Greenstone Belt. Science 388 (6754): 1431-1435; doi: 10.1126/science.ads8461

Source: www.sci.news

These Rocks May Be the Final Remnants of Earth’s Early Crust

Canadian Nuvvuagittuq Green Stone Belt may contain the world’s oldest rock

Jonathan O’Neill

About four billion years ago, magma from Earth’s mantle intruded the primitive crust of a nascent planet. Over the next period, nearly all of the planet’s early crust melted back into the mantle, leaving behind a small remnant near the site of this intrusion that still exists today.

This remnant is part of the Nuvvuagittuq Greenstone Belt along Hudson Bay’s coast in Canada. Recent analyses of the rock’s radioisotope signatures have sparked debates among geologists about whether it is indeed the oldest rock on Earth or simply very ancient.

In a study published in 2008, Jonathan O’Neill from the University of Ottawa and his team posited that the surrounding rocks could be as old as 4.3 billion years, dating back to the Hadean eon—just a few hundred million years after Earth’s formation.

While there have been discoveries of older mineral grains, these ancient Hadean rocks provide critical insights into Earth’s formative years, possibly shedding light on geological enigmas like the onset of plate tectonics and early ocean compositions.

The method used for dating the rocks has drawn controversy, particularly regarding the claimed age of 4.3 billion years. Traditionally, old rocks are dated utilizing a robust mineral known as zircon, but these volcanic rocks lack zircon. “No one can date these rocks using the popular techniques,” O’Neill remarks.

Instead, researchers analyzed the isotopes of neodymium and samarium within the rock. As samarium decays, it generates different isotopes of neodymium at predictable rates, allowing the ratio of isotopes to serve as a “clock” marking the time since the rock crystallized from magma. Interestingly, two isotopes of samarium can decay at differing rates, acting as two parallel chronometers. Disagreement arose among researchers about whether the rock was genuinely Hadean, as the two clocks provided inconsistent age estimates.

“I’m not convinced that most of the early Earth research community agrees,” states Richard Walker at the University of Maryland.

Currently, O’Neill’s team is assessing the neodymium and samarium isotopes in the rock formations dating back 4.3 billion years. By definition, such intrusions are younger than the surrounding rock layers, implying that dating an intrusion yields the minimum age for the enclosing rocks.

Detailed view of the Canada Nuvvuagittuq Green Stone Belt

David Hutt/Alamy

In the findings, the two chronological indicators tell the same tale, indicating the rocks’ age to be approximately 4.16 billion years. “Both clocks yield identical results,” O’Neill states. This consistency bolsters the theory that the surrounding rocks were indeed solidified during the Hadean eon, making them potentially the only known remnants of Earth’s ancient crust.

“I believe they present the strongest argument possible,” asserts Graham Pierson from the University of Alberta, Canada.

“The simplest interpretation of this data is that these represent the oldest rocks on Earth,” says Jesse Reimink at Pennsylvania State University. Nevertheless, he cautions that this may not be the final word on the subject, stating, “When it comes to the oldest rocks and minerals, absolute certainty is hard to come by.”

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Source: www.newscientist.com

The Earth’s Sensitivity to Greenhouse Gases is Greater Than We Realized

Climate change might be even more severe than previously estimated

kapook2981/getty images

The Earth’s climate appears to be more responsive to the pollution caused by greenhouse gases than previously assumed, making it harder to keep global temperature increases below 2°C.

This is concerning news for global efforts to combat climate change, according to Gunnar Myhre from Cicero International Climate Research Centre in Norway.

Researchers have long been aware that releasing greenhouse gases into the atmosphere can lead to climate warming with widespread consequences. However, the extent of potential warming due to these emissions remains uncertain. Specifically, how sensitive is the Earth’s climate to this pollution?

The primary uncertainty arises from how clouds react to warming atmospheres, as shifts in cloud systems could exacerbate warming through feedback loops.

Most predictions regarding warming by the century’s end are derived from climate models that incorporate various sensitivity assumptions. The model utilized by the Intergovernmental Panel on Climate Change indicates that if atmospheric concentrations double compared to pre-industrial levels, warming could range between 2°C and 5°C, prompting organizations to adopt a median estimate of 3°C.

Myhre and his team sought to align climate model predictions with satellite data showing the Earth’s energy imbalance—a measure of excess heat within our climate system, reflecting its sensitivity levels.

They discovered that less sensitive climate models, which suggest that the Earth’s climate is more resistant to greenhouse gas emissions, did not align with satellite data collected since the turn of the millennium. According to Myhre, models asserting that the Earth’s climate is less resistant to these gases are “more common.” He added, “Models predicting minimal warming are increasingly rare.”

The findings challenge the reliability of climate models forecasting warming below 2.9°C with doubled greenhouse gas concentrations. Instead, the data imply that warming beyond this threshold is more probable for the same level of pollution.

This has been corroborated by recent record-high temperatures observed both on land and in the sea since 2023, described as “strong climate feedback” in the atmosphere by Myhre.

A more sensitive climate necessitates a quicker reduction in emissions to maintain the same temperature trajectory. In essence, the world must accelerate decarbonization efforts to meet its climate commitments.

Johannes Kuas from the University of Leipzig in Germany argues that the study presents a “very plausible contention” that the Earth is indeed more sensitive to global warming than some models suggest, stating it “reduces the margin” for model estimations that scientists should follow. “It highlights the urgent need for political action against climate change,” he emphasized.

Richard Allen from the University of Reading in the UK notes that “natural climate change” could also be part of the narrative, by pointing out that satellite records date back only to 2001. Nevertheless, he describes the study as “rigorous” and adds, “there is further evidence that simulations predicting less warming are increasingly unrealistic in the long-term.”

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Source: www.newscientist.com

Hidden Plumes in Earth’s Mantle May Drain Heat from the Core

The Al Haja Mountains of Oman

l_b_photography/shutterstock

Researchers have discovered the first known “ghost plume” beneath Oman, suggesting a column of hot rock rising from the lower mantle with no visible volcanic activity on the surface.

The mantle plume is a mysterious intrusion of molten rock believed to transfer heat from the core-mantle boundary to the Earth’s surface, sometimes occurring beneath the heart of continental plates, as seen in regions like Yellowstone and East Africa. Notably, “these scenarios typically feature surface volcanoes,” states Simone Pilia from King Fahd University of Petroleum and Minerals in Saudi Arabia. Oman lacks such volcanic indicators.

Pilia first hypothesized the existence of this “accidental” plume while examining new seismic data from Oman. The analysis revealed that seismic waves from distant earthquakes travel more slowly through a cylindrical region beneath eastern Oman, indicating it is less dense than surrounding materials due to elevated temperatures.

Additional independent seismic assessments identified critical boundaries where Earth’s deep minerals undergo changes that align with the hot plume’s characteristics. This evidence suggests the plume extends over 660 km from the surface.

The presence of these plumes also explains why the region continues to elevate despite geological compression, a process where the crust is squeezed together. This discovery fits models that explain alterations in Indian tectonic plate movements.

“The more evidence we collected, the more convinced we became it was a plume,” remarks Pilia, who has named this geological feature the “Dinni plume” after her son.

“It’s plausible that this plume exists,” agrees Saskia Goes at Imperial College London, adding that this study is “thorough.” Nevertheless, she emphasizes that identifying narrow plumes is notoriously challenging.

If verified, the existence of a “ghost plume” trapped within Oman’s relatively thick rocky layers suggests there might be others. “We are confident that the Dinni plume is not alone,” says Pilia.

If multiple hidden plumes exist, it could indicate that heat from the core is transferring more readily through the mantle in these regions, influencing our understanding of Earth’s evolutionary history.

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Source: www.newscientist.com