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Widening beaches make California 500 acres bigger than it was 40 years ago

Phys.org: Earth science - Fri, 02/06/2026 - 16:20
Southern California's beaches have grown more than 500 acres over the past four decades despite being one of the most heavily urbanized and dammed coastal regions in the world, according to a new study conducted by researchers at the University of California, Irvine, the U.S. Geological Survey and other institutions. The conventional wisdom-challenging revelation about coastal erosion and replenishment is the subject of the study published recently in Nature Communications.

How the Spring Thaw Influences Arsenic Levels in Lakes

EOS - Fri, 02/06/2026 - 14:08
Source: Journal of Geophysical Research: Biogeosciences

From 1948 to 1953, a gold mine called Giant Mine released about 5 tons of arsenic trioxide per day into the environment around Yellowknife, Northwest Territories, Canada. Emissions declined from the 1950s until the mine closed in 2004, but the surrounding landscape remains highly contaminated with arsenic.

Little et al. recently studied how the spring thaw influences arsenic levels in four Yellowknife area lakes and how phytoplankton populations alter arsenic biogeochemistry during this transition period. The researchers sampled each lake twice per year in 2022 and 2023: once in late April, before the beginning of the spring thaw period, and once 7–10 days later, when the thaw had begun but the ice was still thick enough to safely walk on, making sample collection feasible.

Sammy’s, Handle, Frame, and Jackfish lakes spanned a gradient of arsenic contamination levels when measured before the thaw in 2022—from 5.5 micrograms per liter in Sammy’s Lake to 350 micrograms per liter in Frame Lake. In Handle, Frame, and Jackfish lakes, arsenic levels went down as the spring thaw began, but Sammy’s Lake followed the opposite trend. The difference likely lies in how much arsenic the lakes contained to begin with. With Sammy’s Lake starting at such a low level, arsenic from meltwater exacerbated the contamination. In the other three lakes, the concentration of arsenic in meltwater was lower than or similar to the starting concentration in the lake, so meltwater diluted the contamination.

Arsenic exists mostly in two oxidation states: arsenite and the less toxic, less mobile arsenate. Because arsenate is more stable under oxic conditions, the influx of highly oxygenated snow and ice meltwater during the spring thaw period was accompanied by a predictable shift in the predominant form of arsenic in the lakes.

The winter of 2022 was significantly colder than 2023, with the difference reflected in the thickness of the ice: 76–130 centimeters in 2022 compared with 65–72 centimeters in 2023. The warm winter did not alter the final arsenic concentration or speciation in the water at the end of the thaw. However, an increase was observed in plankton communities in more mature life stages and in taxa that are more competitive in warmer conditions. This result is important, the authors say, because late winter and spring thaw plankton community dynamics set the stage for the following open-water season. (Journal of Geophysical Research: Biogeosciences, https://doi.org/10.1029/2025JG009231, 2026)

—Saima May Sidik (@saimamay.bsky.social), Science Writer

Citation: Sidik, S. M. (2026), How the spring thaw influences arsenic levels in lakes, Eos, 107, https://doi.org/10.1029/2026EO260051. Published on 6 February 2026. Text © 2026. AGU. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

Primordial Impact May Explain Why the Moon Is Asymmetrical

EOS - Fri, 02/06/2026 - 14:07

Until 1959, nobody on Earth had ever seen our Moon’s farside. Thanks to gravitational tidal forces, the lunar nearside always faces us, so it was surprising for everyone to learn that the other half of the Moon looks strikingly different. Not only that, but subsequent observations showed the lunar farside has a thicker surface than the nearside, and its rocks have different compositions.

And nobody knows exactly why.

However, some scientists think the solution to the mystery involves a site known as the South Pole–Aitken (SPA) basin, which was created by an asteroid impact early in the solar system’s history. A new study published in the Proceedings of the National Academy of Sciences of the United States of America draws from surface samples returned by the Chang’e-6 (pronounced CHAHNG-ua) robotic probe. The samples contain minuscule differences in chemical and isotopic composition that indicate the ancient impact may have vaporized part of the Moon’s interior, enough to account for the differences between the near- and farsides.

“Chang’e-6 currently provides the only samples returned from the lunar far side,” said planetary geochemist Heng-Ci Tian ( 田恒次) of the Institute of Geology and Geophysics at the Chinese Academy of Sciences, Beijing, in an email to Eos. Comparing these samples to those collected by previous Chang’e probes and the Apollo missions, Tian and his colleagues determined the impact did more than just make a big crater: It reshuffled the geological components of the lunar mantle. In particular, they looked at isotopes of moderately volatile substances such as potassium that vaporize at relatively low temperatures, rather than more abundant, low-mass elements like hydrogen and oxygen.

If this hypothesis holds up under further scrutiny, it would not only tell us about our Moon’s history and origins but help us understand planetary evolution in general.

As with Earth, the Moon’s mantle—the relatively plastic layer of minerals between the crust and core—is the source of the magma that once powered volcanoes. The nearside is marked by ancient volcanic flows, known as “mares” (pronounced MAR-ays) or “seas,” which are largely absent on the farside.

“Our study reveals that the SPA basin impact caused [evaporation] of moderately volatile elements in the lunar mantle,” Tian said. “The loss of these volatile elements likely suppressed magma generation and volcanic eruptions on the far side.”

If this hypothesis holds up under further scrutiny, it would not only tell us about our Moon’s history and origins but help us understand planetary evolution in general. After all, Earth’s surface is constantly renewed by plate tectonics and hydrologic processes, but other worlds such as Mars and Venus are less dynamic, and much of what is going on inside is still mysterious.

“There’s so many uncertainties as to really what happened [when SPA formed] and how it would’ve affected the interior,” said Kelsey Prissel, a planetary scientist at Purdue University in Indiana who was not involved in the study. She pointed out that different geophysical processes like crystallization and evaporation lead to different populations of isotopes. The new study, which shows a larger fraction of certain isotopes in the SPA region than on the lunar nearside, therefore provides strong evidence that the farside mantle was partially vaporized long ago.

“Previous studies have shown that impacts alter the composition and structure of the lunar surface and crust, but our study provides the first evidence that large impacts play an important role in planetary mantle evolution,” Tian said.

It Came from the Farside!

The SPA basin is one of the biggest impact craters in the solar system, so huge it doesn’t even look like a crater: It stretches all the way from the lunar South Pole to the Aitken crater (hence the name) at approximately 16°S latitude. Researchers determined it formed about 4.3 billion years ago—not long, in cosmic terms, after the Moon was born. Interestingly, it is also almost directly antipodal to a cluster of volcanoes on the lunar nearside, which suggested to some scientists the features might be related.

However, the farside is harder to study. Humanity’s first view came only in 1959 with the uncrewed Soviet Luna 3 orbiter, and none of the Apollo missions landed there. Robotic spacecraft have mapped the entire Moon in detail, but the Chang’e-4 probe achieved humanity’s first farside landing in 2019. Chang’e-6 landed in the SPA basin on 1 June 2024 and returned the first (and so far only) samples from the lunar farside to Earth on 25 June.

“[If] you looked at this data 20 years ago, [the samples] would all look the same.”

The next phase in the study was comparing the chemical makeup and isotopes in these rocks to their nearside counterparts collected by the Apollo astronauts and the Chang’e-5 mission. In particular, Tian and his colleagues looked at potassium (K), rare-earth elements, and phosphorous, collectively known as KREEP, which are possibly related to mantle composition. As the researchers noted in their paper, if the SPA impact vaporized materials in the Moon’s mantle, it might also have redistributed KREEP-rich minerals from the farside to the nearside. Testing this hypothesis required doing very sensitive laboratory measurements that weren’t possible in the Apollo era.

“Having the far side samples is brand-new no matter what,” Prissel said. “But looking at these really fine differences between isotopes is something we haven’t been able to do forever. [If] you looked at this data 20 years ago, [the samples] would all look the same.”

Prissel’s point highlights the interdependency of different branches of planetary science: Understanding the Moon’s interior requires studying samples, performing laboratory experiments on them (or on analog materials), and running theoretical models. These new results will inform the next set of experiments and modeling, as well as guide future lunar sample return missions.

“We plan to analyze additional volatile isotopes to verify our conclusions,” Tian said. “We will combine these with numerical modeling to further evaluate the global effects of the SPA impact.”

—Matthew R. Francis (@BowlerHatScience.org), Science Writer

Citation: Francis, M. R. (2026), Primordial impact may explain why the Moon is asymmetrical, Eos, 107, https://doi.org/10.1029/2026EO260050. Published on 6 February 2026. Text © 2026. The authors. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

How gold is formed in China's Tianshan mountains

Phys.org: Earth science - Fri, 02/06/2026 - 13:30
A new study led by Prof. Xiao Wenjiao from the Xinjiang Institute of Ecology and Geography of the Chinese Academy of Sciences sheds light on the ore-forming process and key mechanisms of the gold deposit in the South Tianshan of northwest China. The research was published in the Geological Society of America Bulletin on Jan. 20.

Satellite imagery of the 24 January 2026 landslide on Gunung Burangrang in Indonesia

EOS - Fri, 02/06/2026 - 09:47

Imagery is now available that shows the aftermath of 3.1 km long landslide that killed about 90 people in West Bandung.

On 24 January 2026, a major landslide occurred on the flanks of Gunung Burangrang (Mount Burangrang) in West Bandung, Indonesia. The search has been long and painstaking, but it is thought that 92 people were killed. There were 23 reported survivors.

AFA Channel has posted some very good drone footage of the landslide to Youtube (excuse the dramatic music and the incorrect headline):-

Planet Labs have also captured a good satellite image of the site. I have overlain this onto the Google Earth DEM:-

Satellite image of the 24 January 2026 landslide on Gunung Burangrang in Indonesia. Image copyright Planet Labs, used with permission.

By way of comparison, this is the site prior to the landslide (image from February 2025):-

Google Earth image of the site of the 24 January 2026 landslide on Gunung Burangrang in Indonesia.

And here is a slider to allow a comparison between the images:-

This appears to have been a deep-seated, probably structurally-controlled failure on high, very steep slopes of Gunung Burangrang, which has then transitioned into a channelised flow. There is considerable entrainment along the track. The landslide is about 3.1 km long and up to 150 m wide.

There has been considerable discussion in Indonesia about the role of logging and mining in the causation of these large landslide events, but in this case neither are apparent in the source area. Institut Teknologi Bandung has a nice article about causation of this landslide, which notes that the underlying geology is volcanic. Loyal readers of this blog will recognise the frequency with which intense rainfall triggers devastating landslides in volcanic materials.

Acknowledgement

Many thanks to the wonderful people at Planet Labs for providing access to the satellite imagery.

Return to The Landslide Blog homepage Text © 2026. The authors. CC BY-NC-ND 3.0
Except where otherwise noted, images are subject to copyright. Any reuse without express permission from the copyright owner is prohibited.

2018 Kīlauea earthquake may have stalled fault's slow slip for decades

Phys.org: Earth science - Thu, 02/05/2026 - 20:21
The magnitude 6.9 earthquake that took place in 2018 on the south flank of Kīlauea on the Island of Hawaiʻi may have stalled episodes of periodic slow slip along a major fault underlying the volcano, according to a new study by scientists at the U.S. Geological Survey.

How intertidal sediment stratification regulates coastal nutrient fluxes

Phys.org: Earth science - Thu, 02/05/2026 - 20:05
A research team led by Prof. Xiao Kai from the Yantai Institute of Coastal Zone Research of the Chinese Academy of Sciences has systematically elucidated the transformation and transport processes of nutrients in intertidal groundwater. The team employed a combined methodological approach, including multi-depth groundwater sampling, dynamic monitoring, stable isotope tracing, and multivariate statistical analysis. Their findings, published in the Journal of Hydrology, provide scientific evidence to deepen understanding of the terrestrial drivers of nearshore eutrophication.

Modelization of the MiniCaLMa neutron monitor based on Geant4 and Garfield++

Publication date: 1 February 2026

Source: Advances in Space Research, Volume 77, Issue 3

Author(s): Alberto Regadío, Juan José Blanco, J. Ignacio García Tejedor, Carlo Luis Guerrero, Du Toit Strauss

Nonlinear shock and solitary wave structures in nonplanar non-Maxwellian plasmas

Publication date: 1 February 2026

Source: Advances in Space Research, Volume 77, Issue 3

Author(s): Shakir Ullah, Abdullah Alshehab, Muhammad Shohaib, Huda Alfannakh, Najeh Rekik

Global map catalogs 459 rare continental mantle earthquakes since 1990

Phys.org: Earth science - Thu, 02/05/2026 - 19:00
Stanford researchers have created the first-ever global map of a rare earthquake type that occurs not in Earth's crust but in our planet's mantle, the layer sandwiched between the thin crust and Earth's molten core. The new map will help scientists learn more about the mechanics of mantle earthquakes, in turn opening a window into the complexities and triggers for all earthquakes.

Scientists explain why methane spiked in the early 2020s

Phys.org: Earth science - Thu, 02/05/2026 - 19:00
A combination of weakened atmospheric removal and increased emissions from warming wetlands, rivers, lakes, and agricultural land increased atmospheric methane at an unprecedented rate in the early 2020s, an international team of researchers report today in the journal Science.

Understanding the hazard potential of the Seattle fault zone: It's 'pretty close to home'

Phys.org: Earth science - Thu, 02/05/2026 - 17:52
In the Pacific Northwest, big faults like the Cascadian subduction zone located offshore, get a lot of attention. But big faults aren't the only ones that pose significant hazards, and a new study investigates the dynamics of a complex fault zone that runs right under the heart of Seattle.

Snowball Earth: Ancient Scottish rocks reveal annual climate cycles

Phys.org: Earth science - Thu, 02/05/2026 - 17:20
Scientists at the University of Southampton have uncovered evidence from ancient rocks that Earth's climate continued to fluctuate during its most extreme ice age—known as Snowball Earth. During the Cryogenian Period, between 720 and 635 million years ago, it has long been believed that Earth's climate entirely shut down.

Unlocking the 'black box' of Grand Canyon's water supply

Phys.org: Earth science - Thu, 02/05/2026 - 15:36
Every year at Grand Canyon National Park, millions of visitors from all over the world stop at one of a dozen water spigots. Most people are on a rim, seeing the canyon's majesty for the first time, when they step off the trail to refill a water bottle. Others are deep in the belly of the canyon, sweaty and tired, facing a hike up in punishing heat, filling their reservoirs and dumping water over their heads to avoid dehydration and heat stroke.

Capturing gravity waves: Scientists break 'decades of gridlock' in climate modeling

Phys.org: Earth science - Thu, 02/05/2026 - 15:05
Global climate models capture many of the processes that shape Earth's weather and climate. Based on physics, chemistry, fluid motion and observed data, hundreds of these models agree that more carbon dioxide in the atmosphere leads to hotter global temperatures and more extreme weather. Still, uncertainty remains around how seasonal weather patterns and atmospheric systems like the jet stream will respond to global warming. Some of this uncertainty stems from the way models approximate the effects of relatively short-lived, small-scale phenomena known as gravity waves.

Seamounts promote expansion of oxygen minimum zone in western Pacific, researchers discover

Phys.org: Earth science - Thu, 02/05/2026 - 14:32
Seamounts and the oxygen minimum zone (OMZ) are two typical deep-sea habitats that often coexist. However, determining whether the "seamount effect" alters OMZ structure through marine stratification, thereby influencing the deep-sea hypoxic environment and carbon sink processes, remains unconfirmed.

Meet the Mysterious Electrides

EOS - Thu, 02/05/2026 - 14:22

This story was originally published by Knowable Magazine.

For close to a century, geoscientists have pondered a mystery: Where did Earth’s lighter elements go? Compared to amounts in the Sun and in some meteorites, Earth has less hydrogen, carbon, nitrogen and sulfur, as well as noble gases like helium—in some cases, more than 99 percent less.

Some of the disparity is explained by losses to the solar system as our planet formed. But researchers have long suspected that something else was going on too.

Recently, a team of scientists reported a possible explanation—that the elements are hiding deep in the solid inner core of Earth. At its super-high pressure—360 gigapascals, 3.6 million times atmospheric pressure—the iron there behaves strangely, becoming an electride: a little-known form of the metal that can suck up lighter elements.

Electrides, in more ways than one, are having their moment.

Study coauthor Duck Young Kim, a solid-state physicist at the Center for High Pressure Science & Technology Advanced Research in Shanghai, says the absorption of these light elements may have happened gradually over a couple of billion years—and may still be going on today. It would explain why the movement of seismic waves traveling through Earth suggests an inner core density that is 5 percent to 8 percent lower than expected were it metal alone.

Electrides, in more ways than one, are having their moment. Not only might they help solve a planetary mystery, they can now be made at room temperature and pressure from an array of elements. And since all electrides contain a source of reactive electrons that are easily donated to other molecules, they make ideal catalysts and other sorts of agents that help to propel challenging reactions.

One electride is already in use to catalyze the production of ammonia, a key component of fertilizer; its Japanese developers claim the process uses 20 percent less energy than traditional ammonia manufacture. Chemists, meanwhile, are discovering new electrides that could lead to cheaper and greener methods of producing pharmaceuticals.

Today’s challenge is to find more of these intriguing materials and to understand the chemical rules that govern when they form.

Electrides at High Pressure

Most solids are made from ordered lattices of atoms, but electrides are different. Their lattices have little pockets where electrons sit on their own.

Normal metals have electrons that are not stuck to one atom. These are the outer, or valence, electrons that are free to move between atoms, forming what is often referred to as a delocalized “sea of electrons.” It explains why metals conduct electricity.

The outer electrons of electrides no longer orbit a particular atom either, but they can’t freely move. Instead, they become trapped at sites between atoms that are called non-nuclear attractors. This gives the materials unique properties. In the case of the iron in Earth’s core, the negative electron charges stabilize lighter elementsat non-nuclear attractors that were formed at those super-high pressures, 3,000 times that at the bottom of the deepest ocean. The elements would diffuse into the metal, explaining where they disappeared to.

In an experiment, scientists simulated the movement of hydrogen atoms (pink) into the lattice structure of iron at a temperature of 3,000 degrees Kelvin (2,727 Celsius), at pressures of 100 gigapascals (GPa) and 300 GPa. At the higher pressure (right) an electride forms, as indicated by the altered distribution of the hydrogen observed within the iron lattice — these would represent the negatively charged non-nuclear attractor sites to which hydrogen atoms bond, forming hydride ions. Duck Young Kim and his coauthors think that the altered hydrogen distribution at higher pressure in these simulations is good evidence that an electride with non-nuclear reactor sites forms within the iron of Earth’s core. Credit: Knowable Magazine, adapted from I. Park et al./Advanced Science 2024

The first metal found to form an electride at high pressure was sodium, reported in 2009. At a pressure of 200 gigapascals (2 million times greater than atmospheric pressure) it transforms from a shiny, reflective, conducting metal into a transparent glassy, insulating material. This finding was “very weird,” says Stefano Racioppi, a computational and theoretical chemist at the University of Cambridge in the United Kingdom, who worked on sodium electrides while in the lab of Eva Zurek at the University at Buffalo in New York state. Early theories, he says, had predicted that at high pressure, sodium’s outer electrons would move even more freely between atoms.

The first sign that things were different came from predictions in the late 1990s, when scientists were using computational simulations to model solids, based on the rules of quantum theory. These rules define the energy levels that electrons can have, and hence the probable range of positions in which they are found in atoms (their atomic orbitals).

Simulating solid sodium showed that at high pressures, as the sodium atoms get squeezed closer together, so do the electrons orbiting each atom. That causes them to experience increasing repulsive forces with one another. This changes the relative energies of every electron orbiting the nucleus of each atom, Racioppi explains—leading to a reorganization of electron positions.

This graphic shows alternative models for metal structures. At left is the structure at ambient conditions, with each blue circle representing a single atom in the metallic lattice consisting of a positively charged nucleus surrounded by its electrons. The electrons can move freely throughout the lattice in what is known as a “sea of electrons.” Earlier theories of metals at high pressures assumed a similar structure, with even greater metallic characteristics (top, right), but more recent modeling shows that in some metals like sodium, at high pressure the structure changes (bottom, right) to a system in which the electrons are localized (dark blue boxes) between the ionic cores (small light blue circles)—an electride. This gives the structure very different properties. Credit: Knowable Magazine, adapted from S. Racioppi and E. Zurek/Ar Materials Research 2025

The result? Rather than occupying orbitals that allow them to be delocalized and move between atoms, the orbitals take on a new shape that forces electrons into the non-nuclear attractor sites. Since the electrons are stuck at these sites, the solid loses its metallic properties.

Adding to this theoretical work, Racioppi and Zurek collaborated with researchers at the University of Edinburgh to find experimental evidence for a sodium electride at extreme pressures. Squeezing crystals of sodium between two diamonds, they used X-ray diffraction to map electron density in the metal structure. This, they reported in September 2025, confirmed that electrons really were located in the predicted non-nuclear attractor sites between sodium atoms.

Just the Thing for Catalysts

Electrides are ideal candidates for catalysts—substances that can speed up and lower the energy needed for chemical reactions. That’s because the isolated electrons at the non-nuclear attractor sites can be donated to make and break bonds. But to be useful, they would need to function at ambient conditions.

Several such stable electrides have been discovered over the last 10 years, made from inorganic compounds or organic molecules containing metal atoms. One of the most significant, mayenite, was found by surprise in 2003 when material scientist Hideo Hosono at the Institute of Science Tokyo was investigating a type of cement.

Mayenite is a calcium aluminate oxide that forms crystals with very small pores—a few nanometers across—called cages, that contain oxygen ions. If a metal vapor of calcium or titanium is passed over it at high temperature, it removes the oxygen, leaving behind just electrons trapped at these sites—an electride.

Unlike the high-pressure metal electrides that switch from conductors to insulators, mayenite starts as an insulator. But now its trapped electrons can jump between cage sites (via a process called quantum tunnelling)—making it a conductor, albeit 100 to 1,000 times less conductive than a metal like aluminum or silver. It also becomes an excellent catalyst, able to surrender electrons to help make and break bonds in reactions.

By 2011, Hosono had begun to develop mayenite as a greener and more efficient catalyst for synthesizing ammonia. Over 170 million metric tons of ammonia, mostly for fertilizers, is produced annually via the Haber-Bosch process, in which metal oxides facilitate hydrogen and nitrogen gases reacting together at high pressure and temperature. It is an energy-intensive, expensive process—Haber-Bosch plants account for some 2 percent of the world’s energy use.

The company estimates that this will avoid 11,000 tons of CO2 emissions annually—about equal to the annual emissions of 2,400 cars.

In Haber-Bosch, the catalysts bind the two gases to their surfaces and donate electrons to help break the strong triple bond that holds the two nitrogen atoms together in nitrogen gas, as well as the bonds in hydrogen gas. Because mayenite has a strong electron-donating nature, Hosono thought mayenite would be able to do it better.

In Hosono’s reaction, mayenite itself does not bind the gases but acts as a support bed for nanoparticles of a metal called ruthenium. First, the nanoparticles absorb the nitrogen and hydrogen gases. Then the mayenite donates electrons to the ruthenium. These electrons flow into the nitrogen and hydrogen molecules, making it easier to break their bonds. Ammonia thus forms at a lower temperature—300 to 400° C—and lower pressure—50 to 80 atmospheres—than with Haber-Bosch, which takes place at 400 to 500° C and 100 to 400 atmospheres.

In 2017, the company Tsubame BHB was formed to commercialize Hosono’s catalyst, with the first pilot plant opening in 2019, producing 20 metric tons of ammonia per year. The company has since opened a larger facility in Japan and is setting up a 20,000-ton-per year green ammonia plant in Brazil to replace some of the nation’s fossil-fuel-based fertilizer production. The company estimates that this will avoid 11,000 tons of CO2 emissions annually—about equal to the annual emissions of 2,400 cars.

There are other applications for a mayenite catalyst, says Hosono, including a lower-energy conversion of CO2 into useful chemicals like methane, methanol or longer-chain hydrocarbons. Other scientists have suggested that mayenite’s cage structure also makes it suitable for immobilizing radioactive isotope waste in nuclear power stations: The electrons could capture negative ions like iodine and bromide and trap them in the cages.

Mayenite has even been studied as a low-temperature propulsion system for satellites in space. When it is heated to 600°C in a vacuum, its trapped electrons blast from the cages, causing propulsion.

Organic Electrides

The list of materials known to form electrides keeps growing. In 2024, a team led by chemist Fabrizio Ortu at the University of Leicester in the UK accidentally discovered another room-temperature-stable electride made from calcium ions surrounded by large organic molecules, together known as a coordination complex.

“You put something in a milling jar, you shake it really hard, and that provides the energy for the reaction.”

He was using a method known as mechanical chemistry—“You put something in a milling jar, you shake it really hard, and that provides the energy for the reaction,” he says. But to his surprise, electrons from the potassium he had added to his calcium complex were not donated to the calcium ion. Instead, what formed “had these electrons that were floating in the system,” he says, trapped in sites between the two metals.

Unlike mayenite, this electride is not a conductor—its trapped electrons do not jump. But they allow it to facilitate reactions that are otherwise hard to get started, by activating unreactive bonds, doing a job much like a catalyst. These are reactions that currently rely on expensive palladium catalysts.

The scientists successfully used the electrideon a reaction that joins two pyridine rings—carbon rings containing a nitrogen atom. They are now examining whether the electride could assist in other common organic reactions, such as substituting a hydrogen atom on a benzene ring. These substitutions are difficult because the bond between the benzene ring carbon and its attached hydrogen is very stable.

There are still problems to sort out: Ortu’s calcium electride is too air- and water-sensitive for use in industry. He is now looking for a more stable alternative, which could prove particularly useful in the pharmaceutical industry to synthesize drug molecules, where the sorts of reactions Ortu has demonstrated are common.

Still Questions at the Core

There remain many unresolved mysteries about electrides, including whether Earth’s inner core definitely contains one. Kim and his collaborators used simulations of the iron lattice to find evidence for non-nuclear attractor sites, but their interpretation of the results remains “a little bit controversial,” Racioppi says.

Sodium and other metals in Group 1 and Group 2 of the periodic table of elements—such as lithium, calcium and magnesium—have loosely bound outer electrons. This helps make it easy for electrons to shift to non-nuclear attractor sites, forming electrides. But iron exerts more pulling power on its outer electrons, which sit in differently shaped orbitals. This makes the increase in electron repulsion under pressure less significant and thus the shift to electride formation difficult, Racioppi says.

Electrides are still little known and little studied, says computational materials scientist Lee Burton of Tel Aviv University. There is still no theory or model to predict when a material will become one. “Because electrides are not typical chemically, you can’t bring your chemical intuition to it,” he says.

“The potential is enormous.”

Burton has been searching for rules that might help with predictions and has had some success finding electrides from a screen of 40,000 known materials. He is now using artificial intelligence to find more. “It’s a complex interplay between different properties that sometimes can all depend on each other,” he says. “This is where machine learning can really help.”

The key is having reliable data to train any model. Burton’s team only has actual data from the handful of electride structures experimentally confirmed so far, but they also are using the kind of modeling based on quantum theory that was carried out by Racioppito create high-resolution simulations of electron density within materials. They are doing this for as many materials as they can; those that are confirmed by real-world experiments will be used to train an AI modelto identify more materials that are likely to be electrides — ones with the discrete pockets of high electron density characteristic of trapped electron sites. “The potential,” says Burton, “is enormous.”

—Rachel Brazil (@rachelbrazil.bsky.social), Knowable Magazine

“This article originally appeared in Knowable Magazine, a nonprofit publication dedicated to making scientific knowledge accessible to all. Sign up for Knowable Magazine’s newsletter.” Read the original article here.

AI to track icebergs adrift at sea in boon for science

Phys.org: Earth science - Thu, 02/05/2026 - 10:00
British scientists said Thursday that a world-first AI tool to catalog and track icebergs as they break apart into smaller chunks could fill a "major blind spot" in predicting climate change.

Upper Crustal Anisotropy in the Southeastern Termination of the Zagros Mountains and Qeshm Island

Geophysical Journal International - Thu, 02/05/2026 - 00:00
SummaryWe investigate upper crustal seismic anisotropy in the southeastern termination of the Zagros Mountains and Qeshm Island through shear wave splitting analysis on the aftershock records of 3 local earthquakes: the 2006 Tiab earthquake (Mw = 6) in the north of the Main Zagros Reverse Fault (MZRF), the 2006 Fin event (Mw = 5.9) in SE Zagros, and the 2005 Qeshm Island event (Mw = 5.8). The results show that north of the MZRF in the Faryab region, the local anisotropy as measured by fast axis orientations of the shear waves, is mainly controlled by crustal structures such as fault shear fabrics or plane fractures around a set of orthogonal active strike-slip faults of a dominantly NE-SW strike. Stress-induced anisotropy caused by fluid-filled microcracks aligned with local maximum horizontal compression seems to be of minor importance. In the vicinity of the MZRF and the Zendan-Minab-Palami Fault, another major fault of the region, local anisotropy is controlled by the structural fabric developed by those faults. Far from the faults, the fast orientations rotate to become aligned with the regional compressional stress. The MZRF is located on an old subduction suture, and it seems that the metamorphic or mylonite fabrics that prevail in this part have shaped the anisotropic structure in the upper crust. In the Simply-Folded Belt of the Zagros and in Qeshm Island, where the deformation of the upper crust is younger, local anisotropy is mostly stress-induced, and the role of fault structures, even though the region is affected by extensive and complex sets of active faulting, is relatively minor. The intensity of anisotropy, as witnessed by splitting delay times, decreases from the metamorphic belt north of the MZRF, to the deformation front in Qeshm Island. This observation is in agreement with the decrease in the accumulated deformation from north to south everywhere in the Zagros. Crustal anisotropy in the Zagros does not show large-scale uniform patterns, rather, it varies over relatively small distances. This is partly due to the fact that both stress-induced and structurally-controlled anisotropies are at work, and partly because of the short-distance variations of the modern stress field in the Zagros.

Single and Multi-Objective Optimization of Distributed Acoustic Sensing Cable Layouts for Geophysical Applications

Geophysical Journal International - Thu, 02/05/2026 - 00:00
SummaryWe present a systematic approach to optimise distributed acoustic sensing (DAS) fibre-optic cable layouts using global optimisation techniques. Our method represents cable geometries using splines, enabling efficient exploration of layouts while respecting physical deployment constraints. The use of evolutionary algorithms enables single and multi-objective optimisation, taking into account complex design constraints such as terrain, accessibility, exclusion zones, cable length, and coupling-related or local site effects, while allowing efficient parallelisation of the optimisation process. We demonstrate the approach on a real-world case study, optimising the layout of a DAS cable for monitoring slope stability in the Cuolm da Vi area of Switzerland. We adapt design criteria for seismic source location problems, and for ambient noise surface wave tomography, to account for the unique characteristics of DAS, such as directional sensitivity patterns. The results show significant potential for improvements in source location accuracy and surface wave tomographic resolution by optimising cable layouts, highlighting the potential of this approach for optimising DAS deployments in various geophysical applications.

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