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Taking Carbon Science Out of Orbit

EOS - Wed, 11/12/2025 - 13:59
Editors’ Highlights are summaries of recent papers by AGU’s journal editors. Source: AGU Advances

What better way to study an entire planet’s monthly exchange of CO2 between the atmosphere, oceans, and land than to position a satellite in space that measures these swings in the atmosphere’s CO2 on a daily basis? We’ve had that tool, NASA’s Orbiting Carbon Observatory-2 (OCO-2), since 2014, and it has yielded an impressive body of science, demonstrating the impacts of natural and human-induced changes in emissions and sinks of CO2, including large-scale fires, ocean warming, and the economic shutdown during the COVID-19 pandemic.

The monthly growth rate of global atmospheric CO2 (ppm yr-1) measured by the OCO 2 satellite‐ (black line) demonstrates a relationship with the Earth’s global surface temperature increase (relative to the preindustrial baseline; red dashed line). The fossil CO2 emissions (black dashed line) are interpolated annual values (also expressed as ppm yr-1), which dipped during the pandemic of 2020, but have resumed growing since then. Credit: Pandey [2025], Figure 1a

In addition to unprecedented frequency of global CO2 measurements, it also provides spatial resolution that enables attribution to changes of sources and sinks across latitudes and continents. This science is driven, in part, by concerns about climate change, but even if we take climate out of the equation to remove political implications, the basic science of understanding the Earth’s carbon cycle has advanced tremendously by this extraordinary tool in space.

Pandey [2025] likens the possible premature decommissioning of this satellite to removing stethoscopes from medical doctors’ toolkits, and yet that is precisely what the current U.S. Administration’s proposed 2026 budget would do. This commentary elegantly describes what has been learned from the OCO-2 mission and how it can inform policy; it should be mandatory reading for anyone, from members of Congress to their constituents, who could possibly influence funding for the OCO-2 mission.

Citation: Pandey, S. (2025). Taking Earth’s carbon pulse from space. AGU Advances, 6, e2025AV002085. https://doi.org/10.1029/2025AV002085

—Eric Davidson, Editor, AGU Advances

Text © 2025. 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.

When Cascadia Gives Way, the San Andreas Sometimes Follows

EOS - Wed, 11/12/2025 - 13:56

Successfully predicting earthquakes sounds like a dark art.

However, new research hints it may be possible: Sediment cores extracted from the Pacific seafloor suggest that two major fault systems along the western coast of the United States and Canada might be partially synchronized. After an earthquake on the southern part of the Cascadia subduction zone, an earthquake soon after on the northern part of the San Andreas fault appears to occur roughly half of the time, the new findings reveal. These results, published in Geosphere, provide evidence of stress triggering, which has long been invoked to explain how activity on one fault might lead to activity on another nearby.

Fault zones persist across wide swaths of our planet, but the one that stretches onshore and offshore from California to British Columbia, Canada, is particularly complex. The vertical strike-slip San Andreas fault, in the south, intersects the Cascadia subduction zone off the coast of Northern California at a point known as the Mendocino Triple Junction.

There’s an amalgam of different types of large, active faults, and the Mendocino Triple Junction itself is migrating northward, said Chris Goldfinger, an earthquake geologist at Oregon State University in Corvallis. “It’s a very complicated situation.”

Earthquake Here, Earthquake There

Researchers have long wondered whether the northern region of the San Andreas fault and the southern part of the Cascadia subduction zone might be affecting one another. The idea isn’t far-fetched: Scientists know that earthquakes, which result from sudden releases of stored-up energy on a fault, relieve stress on one part of a fault but often do not make that stress disappear. “When it ruptures, [a fault] relieves the local stress. But then it transfers stress to other things around it,” said Goldfinger. Such stress transfer could, in turn, trigger activity on another nearby fault.

In 2008, Goldfinger and his colleagues published a study of earthquakes along the northern San Andreas and Cascadia subduction zone. To determine when the earthquakes happened, the team used radiocarbon dating of turbidites, which are sedimentary deposits left on the seafloor when ground shaking causes underwater landslides. The researchers found several apparent pairs of earthquakes that seemed to have occurred around the same time—that is, within decades or centuries of one another. However, the significant age uncertainties precluded drawing any definitive conclusions about paired earthquakes, Goldfinger said.

Mysterious Turbidites

Since then, Goldfinger and his collaborators have obtained more turbidite records from sediments in the ocean and also analyzed inland sediments from places like Lake Merced near San Francisco. With those new data, which stretch back roughly 3,100 years, in hand, the team returned to the question of paired earthquakes. The researchers also revisited a mystery that had been bothering them since the late 1990s: Why did some turbidites collected from near the Mendocino Triple Junction appear to be upside down?

“They had all of the sand at the top, which is not where it should be.”

Turbidites are layers of sand, mud, clay, and silt that typically are coarsest near the bottom and become finer grained at the top. That’s because gravity causes the coarsest particles—the sand—to settle out first and smaller particles to be deposited later as the current slows down. But many of the turbidite beds recorded in cores from near the Mendocino Triple Junction appear to be capped with sand, rather than finer sediment. That’s unexpected, said Goldfinger. “They had all of the sand at the top, which is not where it should be.”

It’s taken more than 2 decades for the team to finally arrive at an explanation for those anomalous turbidites.

They are, in fact, two turbidite beds, Goldfinger and his colleagues concluded. The sand on top is actually a second turbidite bed formed close to an earthquake source whose finer particles were carried away and deposited at more distant locations.

The researchers furthermore inferred that these so-called doublet turbidites were created by two different earthquakes occurring on different fault systems—one in the Cascadia subduction zone and one on the San Andreas fault. The tip-off was that the occurrence of doublet turbidites systematically decreases with increasing distance from the Mendocino Triple Junction. The San Andreas–derived turbidite beds fade away to the north, and Cascadia-derived turbidite beds fade away to the south. That’s expected because shaking from San Andreas earthquakes will be weaker the farther north one goes and shaking from Cascadia earthquakes will correspondingly be weaker the farther south one goes.

“These doublets should fade in a specific way, and they do,” said Goldfinger.

The team found that slightly more than half of the 18 turbidites they studied in the southern Cascadia subduction zone were closely associated in time with turbidites from the northern San Andreas. In those 10 cases, the median ages of the earthquakes inferred from radiocarbon measurements differed from their associated quake on the other fault system by roughly 60 years, which is about equal to the data’s uncertainty. Eight of those pairs furthermore exhibited a doublet structure, indicating that they occurred especially close together in time.

The similar timing and unique stacking pattern of the doublets suggest that Cascadia earthquakes generate regional stresses that trigger subsequent earthquakes on the northern San Andreas fault.

These findings convincingly demonstrate that the northern San Andreas and the southern Cascadia subduction zone are at least partially synchronized, said Kathryn Materna, a geophysicist at the University of Colorado Boulder not involved in the work. “Seeing half of them correlated on opposite sides of the triple junction is a pretty striking correlation,” she said. Because these faults tend to unleash earthquakes at different rates, there’s no reason their events should line up closely in time, said Materna. “They’re different systems with different recurrence intervals.”

Patiently Ducking and Covering

“The best fit to the data, by far, is to have Cascadia go first.”

Goldfinger and his colleagues believe that in cases of paired earthquakes, Cascadia is the one leading the charge. “The best fit to the data, by far, is to have Cascadia go first,” said Goldfinger.

Understanding why will take some modeling work. It’d also be interesting to dig into whether a Cascadia event of a certain magnitude is necessary to unleash shaking on San Andreas, he said. “It makes sense that there must be a triggering threshold.”

These findings suggest that a large Cascadia earthquake might be followed by ground shaking on the San Andreas. But ducking and covering after Cascadia lets loose could require some patience. The timing between paired earthquakes likely varies substantially, Goldfinger said. “It could be anything from minutes to decades.”

—Katherine Kornei (@KatherineKornei), Science Writer

Citation: Kornei, K. (2025), When Cascadia gives way, the San Andreas sometimes follows, Eos, 106, https://doi.org/10.1029/2025EO250419. Published on 12 November 2025. Text © 2025. 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.

Speedy Flyby Adds New Organics to Enceladus’s “Primordial Soup”

EOS - Wed, 11/12/2025 - 13:54

In 2008, NASA’s now-departed Cassini spacecraft made its fastest flyby of Enceladus, the moon of Saturn that’s spewing its subsurface ocean into space. A new analysis of data from that flyby has revealed a bevy of complex organic compounds that hadn’t been detected before and confirmed the origin of several previously known organics. The speed at which the flyby occurred, a zippy 18 kilometers per second, helped convince the researchers that the organics truly originated from Enceladus’s interior ocean and were not a product of postejection space weathering.

When combined with the slate of previously detected organic compounds, “these new organics could support chemical networks or chemical pathways that potentially could lead to biologically relevant compounds,” said Nozair Khawaja, lead researcher on this discovery and a planetary scientist at Freie Universität Berlin in Germany.

Connecting Chemistries

Enceladus emits plumes of water from its subsurface ocean through icy cracks near its south pole. Enough material has been released into space to create a ring around Saturn called the E ring. During its 13 years exploring the Saturn system, Cassini collected and analyzed multiple samples from the E ring and discovered a wide variety of organic and inorganic molecules, including aromatics and oxygen-bearing species, that hinted at complex chemistry happening within Enceladus.

“If you capture some particles in the E ring, that means, indirectly, you are sampling the subsurface ocean.”

“If you capture some particles in the E ring, that means, indirectly, you are sampling the subsurface ocean,” Khawaja said.

However, planetary scientists have debated whether all of the organic compounds discovered in E ring material could truly be traced back to the Enceladean ocean. After all, material sits in the E ring for years, and the material’s chemistry may have been altered through exposure to radiation from Saturn and the solar system, a process called space weathering.

Material ejected from Enceladus creates Saturn’s E ring, imaged here by Cassini in 2006. Credit: NASA/JPL/Space Science Institute

But Cassini didn’t just fly through Saturn’s rings. It also flew directly through Enceladus’s plumes. During those flybys, the spacecraft’s onboard Cosmic Dust Analyzer (CDA) collected and measured spectra from freshly ejected material. Grains of material entered the CDA collector and shattered into chemical constituents—mostly water ice with smatterings of other molecules. The CDA measured chemical spectra and reported what those grains were made of.

The trouble is that water molecules are very sticky, Khawaja explained. After shattering, ice molecules quickly cluster around and shield other molecules from detection. The slower the grains traveled through the instrument, the less time CDA had to spot those other compounds, which were the ones that scientists were most interested in decoding.

Previous analyses of Enceladus and E ring flybys, most of which occurred at relative speeds less than 12 kilometers per second, detected five of the six elements essential for Earth’s biology—the CHNOPS elements—but other materials remained elusive.

Speed Is Everything

Luckily, Cassini’s fifth Enceladus flyby was particularly speedy. Plume material traveled through the CDA at 18 kilometers per second. Analysis of data from that flyby, conducted by Khawaja and his team, revealed that the freshly ejected ice grains contained many of the same compounds that had previously been found in E ring material.

New models suggest that organic molecules could originate in hydrothermal vents at the base of Enceladus’s ocean, float upward toward the bottom of the moon’s ice shell, and condense onto ice grains as they travel through vents, before being ejected into space. Credit: NASA/JPL-Caltech

“These new particles, they were very young in age and very fresh material,” Khawaja said. “That means, if we observe in these fresh grains the same compounds [seen] in the E ring grains, which are months or many years old, that means that those compounds are actually coming from the subsurface of Enceladus.”

Because the material collected in this flyby did not have time to be altered by space radiation, these chemical commonalities “effectively rule out” space radiation or another process external to Enceladus as the source of complex organic material in the E ring and Enceladus’s ocean, explained Alexander Berne.

The results “indicate that endogenic processes, such as hydrothermal activity, i.e., energy-releasing interactions between silicate rock and water, form the observed chemistry,” Berne said. “This hydrothermal activity is potentially a key process for sustaining metabolic reactions to support astrobiology within Enceladus,” like black smokers near Earth’s mid-ocean ridges. Berne, a planetary scientist at the California Institute of Technology in Pasadena, was not involved with this research.

New Ingredients in the Soup

The swiftness of this particular flyby also enabled the CDA to measure the spectra of several previously undetected complex organic compounds before they were shielded behind an icy curtain. These compounds, including oxygen- and nitrogen-bearing species, aryls, alkenes, and ethyls, strengthen the theory that they were generated through geochemical processes at the base of the Enceladean ocean.

“The new compounds confirm that organics are present in the subsurface ocean and may indicate more complex, potentially hydrothermal processes there,” said Larry Esposito, a planetary scientist at the University of Colorado Boulder who was not involved with this research. “The new findings are consistent with the likely habitability of the ocean, which may resemble a complex organic ‘primordial soup.’”

These results were published in Nature Astronomy in October.

Khawaja cautioned that these newly detected organics do not mean that life exists in Enceladus’s ocean or that life is an inevitable result of mixing together this primordial soup. Continued analysis of archival Cassini data, bolstered by future laboratory experiments, could reveal the many potential outcomes of this chemical mixture and could piece together its origin story.

—Kimberly M. S. Cartier (@astrokimcartier.bsky.social), Staff Writer

Citation: Cartier, K. M. S. (2025), Speedy flyby adds new organics to Enceladus’s “primordial soup,” Eos, 106, https://doi.org/10.1029/2025EO250416. Published on 12 November 2025. Text © 2025. 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.

Light pollution: The silent threat to the planet that's easily solved

Phys.org: Earth science - Wed, 11/12/2025 - 10:00
New research has revealed for the first time the full extent of how "Artificial Light At Night" (ALAN) is increasing carbon released by plants and animals across continents—without any increase in the carbon they absorb. The result is reduced carbon storage in ecosystems—which has major implications for climate models and global carbon budgets.

Understanding boulders' influence on snow melt and watersheds could improve northern region climate modeling

Phys.org: Earth science - Tue, 11/11/2025 - 21:25
Thanks to their use of a unique methodology, a McGill-led research team has obtained new insights into how boulders affect snow melt in mountainous northern environments, with implications for local water resources.

How to make AMOC model experiments more realistic

Phys.org: Earth science - Tue, 11/11/2025 - 20:04
Melting ice in the Arctic is causing an increasing amount of freshwater to enter the North Atlantic, which is expected to result in a weakening of the Atlantic overturning circulation. However, many modeling studies make unrealistic assumptions about how this water enters the ocean. A new study published in Ocean Modelling shows that the timing, location, and source of freshwater input can have a considerable impact on its eventual fate and should therefore be taken into account in future model experiments.

Editorial Board

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s):

High-precision zircon geochronology constrains early Permian exhumation of the deep Adriatic crust in the western Italian Alps

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Marco Filippi, Federico Farina, Maria Ovtcharova, Fabiola Caso, Manuel Roda, Chiara Benedetta Piloni, Michele Zucali

Structural controls on simultaneous earthquake clustering and normal fault synchronization

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): F. Iezzi, C. Sgambato, G. Roberts, Z. Mildon, J. Robertson, J. Faure Walker, I. Papanikolaou, A.M. Michetti, S. Mitchell, R. Shanks, R. Phillips, K.J.W. McCaffrey, E. Vittori

Evolution of frictional properties, permeability and elastic parameters due to surface roughness changes during fault maturation in laboratory shear experiments

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Agathe Eijsink, Clay Wood, Chris Marone, Parisa Shokouhi, Jacques Rivière, Derek Elsworth

Interactions between syn-rift magmatism and tectonic extension at intermediate rifted margins

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Peng Yang, Marta Pérez-Gussinyé, Shaowen Liu, Javier García-Pintado, Gudipati RaghuRam

Concentric ionospheric currents driven by teleseismic rayleigh waves from the 2011 Tohoku Earthquake

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Hui Wang, Gary Egbert, Baojia Song, Fangyuan Ma

A machine learning-based V-in-olivine oxybarometer for characterizing oxygen fugacity in lunar and terrestrial basalts

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Guang-Shao Wang, Zhong-Jie Bai, Wen-Jun Hu, Jian-Feng Gao, Wei-Guang Zhu, Ying-Xiong Bai

The role of submarine volcanism in atmospheric chemistry

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): M. Colombier, M. Bonifacie, M. Brenna, A. Burke, C. Cimarelli, S.J. Cronin, P. Delmelle, D.B. Dingwell, K-U. Hess, M. Huebsch, T. Kula, F. Latu’ila, Y. Lavallée, G.W. Mann, T.A. Mather, J. Paredes-Mariño, T. Plank, B. Scheu, Y-J Sun, Z. Taracsák

Rivers of change: the Tethyan Himalaya records how the Gondwanide orogeny altered Late Triassic global climate

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Zhen Li, Pengfei Li, Gideon Rosenbaum, Peter A. Cawood, Qiang Wang, Chao Yuan, Jun Shen

Acceleration of Wilson cycles over time: insights from detrital zircon Hf isotope records

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Zhen-Xin Li, Ross N. Mitchell, Peter A. Cawood, Xuan-Qiao Liu, Lei Qin, Shao-Bing Zhang, Yong-Fei Zheng

Comets and carbonaceous chondrites delivered noble gases to the Moon

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): William S. Cassata, Rita Parai, Lars E. Borg, Charles K. Shearer

Sub-centennially resolved reconstruction of surface temperature on High Arctic Svalbard for the past 13,000 years

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Sher-Rine Kong, Willem G.M. van der Bilt, Pål T. Mørkved, Lars Wörmer, Katarzyna Hasal, William J. D’Andrea

Preaccretionary origin of clay minerals in CI chondritic objects? Insights from the Orgueil clay mineralogy and iron oxidation state

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): J.-C. Viennet, K. Amano, L. Delbes, B. Lavina, F. Hubert, S. Bernard, S. Yaroslavtsev, D. Bessas, A. Chumakov, J.-P. Celse, M. Gounelle, L. Remusat, M. Roskosz

Rifting a post-orogenic continental crust: Insights from the South China Sea

Earth and Planetary Science Letters - Tue, 11/11/2025 - 19:11

Publication date: 1 December 2025

Source: Earth and Planetary Science Letters, Volume 671

Author(s): Fan Zhou, Laetitia Le Pourhiet, Manuel Pubellier, Matthias Delescluse

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