Feed aggregator

Researchers find smaller amounts of microplastics in southern Narragansett Bay

Phys.org: Earth science - Wed, 11/26/2025 - 15:32
It's safe to say Rhode Islanders have a symbiotic relationship with Narragansett Bay.

The Land Beneath Antarctica’s Ice Might Be Full of Water

EOS - Wed, 11/26/2025 - 14:28

In Antarctica, beneath the ice, there is liquid water—and potentially a lot of it. That’s the takeaway from new research that used seismographic instruments to probe the still largely unstudied boundary between Antarctica’s bedrock and its ice sheet.

Previous hydrological studies and modeling work have found evidence of lakes and rivers beneath the Antarctic Ice Sheet, though much remains unknown about the region.

Now, using an array of seismic sensors, researchers from Stony Brook University have added more data points to the map of subglacial Antarctica, finding evidence of a layer of water-saturated sediments or rock under the ice. That layer could have implications for models of Antarctic groundwater systems, as well as for future movements of the ice sheet as it slides toward the ocean.

Looking Beneath the Ice with Earthquakes

The data, which will be presented at AGU’s 2025 Annual Meeting, come from an array of more than 600 seismic sensors strung in two long lines totaling about 600 kilometers near the South Pole, put there over the course of two field seasons in Antarctica. The sensors listen for seismic waves that travel through the upper layers of Earth and into the ice sheet.

Those waves carry the signatures of every medium through which they’ve traveled, said Weisen Shen, a geoscientist at Stony Brook University and a paper coauthor. To isolate that information, the researchers applied a mathematical technique called a receiver function to remove the waves’ source information, leaving only the signatures of what they moved through on their journey to the sensor.

In their data from beneath the South Pole, in a region known as the Pensacola-Pole Basin, the researchers found a very low velocity layer, where seismic waves travel too slowly for the conducting medium to be bedrock or ice.

While the authors can’t say exactly what this layer looks like, Shen said the best explanation is a layer of water-saturated sediments or sandstone, likely hundreds of meters thick.

“Anything we can do to try and enhance our knowledge of what’s going on…is just going to help us try and narrow down this really bizarre landscape underneath the ice.”

“We believe…there must be some aquifer system, a groundwater system, that must be preserved beneath the ice,” he said.

The water there could even be connected to groundwater elsewhere in Antarctica, Shen noted. If so, water might be moving around beneath the surface of Antarctica through hydrologically linked basins, and perhaps even out to the ocean.

That scenario could have implications for sea level rise, but, as University of Waterloo glaciologist Christine Dow pointed out, we know far too little to say for sure. In her own modeling, Dow, who wasn’t affiliated with the research, said it appears these basins aren’t connected to the ocean.

“But these are models based on our current knowledge of where’s frozen and where’s not under the Antarctic,” she said. “Perhaps this new information will change that.”

Dow welcomed new data on the mostly uncharted landscape of subglacial Antarctica, where scientists have evidence of lakes, rivers, and groundwater interacting in complex ways, but little hard evidence of the continent’s topography.

“Anything we can do to try and enhance our knowledge of what’s going on…is just going to help us try and narrow down this really bizarre landscape underneath the ice,” she said.

More Questions Than Answers

One question the new data raise is where the heat energy needed to melt the water comes from, noted Hanxiao Wu, a Ph.D. candidate at Stony Brook University and the paper’s first author. It could come from geothermal heat from below, friction caused by the movement of ice at the surface, or some combination of both.

One takeaway from the research is that estimates of geothermal heat flux below Antarctica may need to be bumped upward, Dow said. Models of ice sheet movement and evolution may also need to change to accommodate hundreds of meters of water-saturated sediments. “That’s a game changer,” Dow said.

Should there turn out to be more water beneath Antarctica than previously thought, and should that water move greater distances and in greater amounts, sea levels could rise beyond current predictions, Shen said. It’s too early, however, to estimate any of these probabilities with much certainty, he cautioned.

Right now, Shen and his fellow researchers are focused on improving their dataset and seeking collaborations with other geophysicists to map out the implications of their findings. Wu traveled back to Antarctica for the 2025–2026 field season, where the team is adding another line of seismic sensors to increase coverage and working on tracking the array to better understand changes in snow surface elevation.

In the future, they hope to add additional data from satellites, magnetotelluric surveys, and fiber-optic cables for a more comprehensive look at the ice pack and its underbelly, perhaps as part of the 5th International Polar Year in 2032.

What the scientists will find is unknown. But with millions of square miles of land underneath the ice, the potential for discovery is appropriately vast.

—Nathaniel Scharping (@nathanielscharp), Science Writer

Citation: Scharping, N. (2025), The land beneath Antarctica’s ice might be full of water, Eos, 105, https://doi.org/10.1029/2025EO250435. Published on 26 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.

Some Summer Storms Spit Sooty Particles into the Stratosphere

EOS - Wed, 11/26/2025 - 14:24

Powerful summertime thunderstorms are injecting particulate matter from wildfires and additional moisture into the stratosphere—a layer of the atmosphere scientists have long thought was mostly pristine.

“The lower stratosphere almost looked more like a smoke cloud.”

A new study, published in Nature Geoscience, detailed these findings, which could have implications for Earth’s ozone layer and atmospheric circulation, especially as the climate continues to warm.

“We as atmospheric scientists have this preconceived notion that [the stratosphere] is a really stable, clean area of our atmosphere. We don’t think about it being perturbed all that often,” said Dan Cziczo, an atmospheric scientist at Purdue University and a coauthor of the new study. 

But in the new observations, “the lower stratosphere almost looked more like a smoke cloud,” he said.

Stratospheric Science

North America’s monsoon season starts when warm, moisture-laden air from the Gulf of Mexico collides with the Rocky Mountains. This process can create powerful summer storms familiar to those living in the U.S. Midwest.

If those storms get powerful enough, some clouds “overshoot,” or extend multiple kilometers above the troposphere and into the stratosphere—a cold, thin layer of Earth’s atmosphere beginning at about 12,000 meters (39,000 feet) above sea level.

This overshoot happens often in the United States: There are about 50,000–100,000 overshooting storms each summer, though some last only a minute or two, said Ken Bowman, an atmospheric scientist at Texas A&M University and a coauthor of the new study. 

Bowman is the lead scientist of a 6-year project called Dynamics and Chemistry of the Summer Stratosphere (DCOTSS) that is investigating these overshooting storms. 

To study overshooting storms, DCOTSS researchers use a unique aircraft called Earth Resources 2, or ER-2, which was built by NASA and flies as high as 22,860 meters (75,000 feet)—higher than 95% of the Earth’s atmosphere. Cziczo and his team used DCOTSS data from 31 May to 27 June 2022, an active fire season in the United States, for their new study. The data came from flights over the U.S. Midwest and Great Plains that specifically targeted overshooting storms. 

Their observations showed an unexpected amount of biomass-burning particles in the lower stratosphere during periods affected by overshooting clouds.

“Once we got the aircraft into the stratosphere, we just found it to be littered with these biomass-burning particles, particles from wildfires,” Cziczo said. There had been previous evidence from flights in 2002 that biomass-burning particles existed in the stratosphere, but not to this extent—Cziczo and his team found particles as high as 4 kilometers into the stratosphere, about 4 times higher than previous detection.

The new study “is really the first time people have seen a really large contribution from smoke in the lower stratosphere,” said Brian Toon, an atmospheric scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder who was not involved in the new study. 

“When you add lots of water vapor, it changes a lot of things.”

Cziczo explained that powerful storm clouds pick up smoke, either directly from burning areas or from smoke already mixed into the troposphere, then “spit” that smoke out into the stratosphere after clouds build up and cross the boundary between the two layers. Virtually all the observed biomass-burning particles were probably transported by overshooting storms, as there are no other likely mechanisms for the particles to enter the stratosphere, Bowman said.

The particles the team observed in the lower 4 kilometers of the stratosphere will likely stay suspended there for months.

The researchers didn’t have a way to track exactly where the particles they observed originated. But wildfires across the United States and Canada in the summer of 2022 were a likely source: “We just have to sort of infer that it was the smoke that was in the Midwest,” Cziczo said.

In addition to the biomass-burning particles, the overshooting storms brought a lot of moisture to the stratosphere. As the ER-2 aircraft flew through overshooting clouds, instruments on board detected additional water, sometimes taking the stratosphere’s usual 4 or 5 parts per million of water up to 20 or 30 parts per million. 

Such an influx of water can affect the chemistry, heating, and cooling of the stratosphere, but more research is needed to figure out exactly how. “When you add lots of water vapor, it changes a lot of things,” Bowman said.

Atmospheric Alterations

The combined forces of stronger storms and more wildfires could make the occurrence of these sooty particles in the stratosphere more likely as the climate continues to warm. 

Additional biomass-burning particles in the stratosphere could have consequences for Earth’s ozone layer. Particles provide additional surface area for the stratosphere’s gas molecules to stick to, encounter other gas particles, and react. Many of these reactions over time can damage the ozone layer, a shield of ozone molecules that protects Earth from too much ultraviolet radiation from the Sun.

“It’s important to make sure we understand this so that we can see what might happen in the future.”

“This is not a paper to panic about,” Bowman said. “But as the number of wildfires increases, which it’s likely to continue doing, we’ll get more biomass-burning particles in the stratosphere. And as the climate warms up, it’s likely that the amount of overshooting convection is going to increase, so that’s going to put more material into the stratosphere.”

The findings also raise numerous questions about how additional particles in the stratosphere might affect Earth’s other atmospheric processes. Additional dark, sooty particles could heat the atmosphere, which could change its dynamics or even blur the typically stark boundary between the troposphere and the stratosphere.

“It’s important to make sure we understand this so that we can see what might happen in the future,” Bowman said.

—Grace van Deelen (@gvd.bsky.social), Staff Writer

Citation: van Deelen, G. (2025), Some summer storms spit sooty particles into the stratosphere, Eos, 106, https://doi.org/10.1029/2025EO250443. Published on 26 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.

New framework unveiled for climate-resilient shores

Phys.org: Earth science - Wed, 11/26/2025 - 01:20
Canada has a marine coastline twice as long as any other country and shares four Great Lakes with the United States. A new report warns that without coordinated planning, coastal communities face increasing flooding and erosion as climate change accelerates.

Muography for structural characterization of volcanoes: a case study at Mount Unzen, Japan

Geophysical Journal International - Wed, 11/26/2025 - 00:00
SummaryDestabilization of volcanic edifices can generate debris avalanches with catastrophic impacts on their environment. We present the first high-resolution muography of Mount Unzen, Japan, conducted to characterize the structure of lava lobes formed on the volcano’s summit and flank during the 1990-1995 eruption. A multi-wire-proportional-chamber-based muon tracking system was operated for 203 days. The obtained high-resolution muographic image shows the internal density structure of Mount Unzen with a spatial resolution of 12 meters. Mean densities were respectively measured as 2,470 kg m−3 and 2,290 kg m−3 for the base rock and a fracture zone, and both were consistent with the results of prior drilling and sampling experiments. The mean density of lava lobes was measured significantly lower value of 1,570 kg m−3, indicating post-eruptive structural weakening. A comparison between the time-series of muographically measured density-lengths and daily precipitation records suggest that rainfall-induced gravitational destabilization did not occur during the observational period. This work demonstrates that long-term (multi-year) muon monitoring of the lava lobes can provide valuable complementary information for volcanic stability assessments.

Global Finite-Frequency Tomography of the 220-km Discontinuity

Geophysical Journal International - Wed, 11/26/2025 - 00:00
SummaryThe asthenosphere is a weak layer in the upper mantle that supports the movement of the overriding tectonic plates and facilitates mantle convection. In this study, we compile a global dataset of SS precursors reflected at the base of the asthenosphere, also known as the 220-km discontinuity. The global dataset includes the oceanic SS precursors from Sun & Zhou (2025a) and new measurements with bounce points in continental regions. Similar to the oceanic dataset, the continental SS precursors are observed on about 45% of the SS waves, with bounce points distributed across all tectonic regions — from orogeny belts to stable cratons. We image the depth of the discontinuity at a global scale using finite-frequency tomography. In oceanic regions, the depth of the 220-km discontinuity agree well with the previous study, with discontinuity depth structure characterized by alternating linear bands of shallow and deep anomalies that roughly follow seafloor age contours. In continental regions, the variations are not spatially oscillatory but are instead much broader, with prominent perturbations associated with convergent plate boundaries. The base of the asthenosphere is shallow along the southern border of the Eurasian plate, from the Mediterranean region to Southeast Asia. Shallow discontinuity anomalies are also observed in the continental interiors – in Eurasia, from the northern Tian Shan through Mongolia to eastern Siberia, and in North America east of the Rocky Mountains. These anomalies form a linear structure roughly parallel to the Pacific subduction zones. The average depth of the discontinuity, as well as the velocity contrast across the interface, is globally consistent across both oceans and continents, with an average depth of approximately 251 km and a velocity increase of about 7%. Given that the continental lithosphere has been cooling for much longer than the oceanic lithosphere, the observed consistency in the average depth of the discontinuity implies that secular cooling does not significantly impact the thermal structure at the base of the asthenosphere.

Optimizing data usage in regional body wave tomography by using asynchronous network data and relative sensitivity kernels: an example from Patagonia

Geophysical Journal International - Wed, 11/26/2025 - 00:00
SummaryA very frequent approach for studying lithospheric processes is to deploy temporary seismological networks in dedicated areas and to map the mantle structures with different approaches. One of them is the well-established relative travel time body wave tomography. Different circumstances often lead to a non-uniform deployment of stations both in space and time, and a wish to combine data which have been acquired asynchronously. This is the situation in Patagonia where two distinct seismic experiments provide complementary seismic data over the region covering the Patagonia slab window. Combining these data in one regional relative body wave tomography is however problematic as the two data sets are a priori with respect to two different reference models. In this contribution, we show that the number of finite-frequency relative travel time residuals varies very strongly from station to station for this data set, violating the assumption implicit in relative travel time tomography of a unique reference model due to an even data distribution for all events. We demonstrate the superiority of the inversion using relative sensitivity kernels compared with a traditional approach with absolute kernels and event terms. A resolution test proves how this is crucial for resolving the important issue of the eastern extent of the slab window. In addition, we discuss potential issues related to interference of the direct phases with core phases when measuring finite-frequency travel time residuals by cross-correlation of waveforms in necessarily relatively large time windows. We also briefly outline our preferred strategy for performing crustal correction, keeping in mind that finite-frequency residuals require frequency-dependent crustal corrections.

Harnessing sedimentary reverberations: A joint inversion approach for enhanced crustal imaging

Geophysical Journal International - Wed, 11/26/2025 - 00:00
SummaryP-wave receiver functions (RFs), which utilize P-wave conversions to probe subsurface structures, face significant challenges in sedimentary environments. Specifically, strong reverberations generated by ultra-low-velocity sedimentary layers distort RF waveforms and obscure crustal signals, posing challenges for robust shallow crustal imaging. We develop a novel Bayesian joint inversion framework that simultaneously utilizes three complementary datasets—reverberant receiver functions, dereverberated receiver functions, and surface wave dispersion—to address this challenge. Our approach employs Unscented Kalman Inversion, a derivative-free method that efficiently handles nonlinear joint inversion problems. Synthetic tests demonstrate that our joint inversion recovers sediment thickness and Moho depth with uncertainties of ±0.50 km and ±1.0 km, respectively. Application to real data from the Songliao Basin verifies the approach, successfully reconstructing sediment thickness and Moho depth beneath sedimentary cover. This methodology demonstrates potential for advancing crustal investigations in complex sedimentary settings, such as continental rift basins and oceanic margins, where sedimentary sequences of variable thickness often obscure deeper structures.

The world's little-known volcanoes pose the greatest threat

Phys.org: Earth science - Tue, 11/25/2025 - 23:20
The next global volcanic disaster is more likely to come from volcanoes that appear dormant and are barely monitored than from the likes of famous volcanoes such as Etna in Sicily or Yellowstone in the US.

Thermal infrared characterization of spatially unresolved resident space objects: Prospects from analytical two-component modeling

Publication date: Available online 19 November 2025

Source: Advances in Space Research

Author(s): Stephen Catsamas, Sarah Caddy, Michele Trenti, Benjamin Metha, Simon Barraclough, Robert Mearns, Airlie Chapman, Rachel Webster

Adaptive Gaining-Sharing Knowledge Region Coverage Planning for Multi-Stratospheric Airships in Complex Environments

Publication date: Available online 19 November 2025

Source: Advances in Space Research

Author(s): Xing-han Liu, Ming Zhu, Yi-fei Zhang, Tian Chen

VOH-Net: Vision-Optimized Hybrid Network for Deep Learning-Based Phase Unwrapping

Publication date: Available online 19 November 2025

Source: Advances in Space Research

Author(s): Saoussen Djeddi, Tarek Bentahar, Riad Saidi, Yacine Belhocine

Prediction of thermospheric CO<sub>2</sub> emission using Machine Learning Technique

Publication date: Available online 19 November 2025

Source: Advances in Space Research

Author(s): Tikemani Bag, Yasunobu Ogawa, V. Sivakumar, Swati Garg

Three decades of GNSS-derived geocenter motion: disentangling geophysical signal from systematic errors

Publication date: Available online 19 November 2025

Source: Advances in Space Research

Author(s): Radosław Zajdel, Kyriakos Balidakis, Adrian Nowak, Tomasz Kur, Krzysztof Sośnica, Jan Douša

Investigating the Signature of Thunderstorm-Generated Gravity Waves on Low-Latitude Ionospheric Dynamics

Publication date: Available online 19 November 2025

Source: Advances in Space Research

Author(s): Akshay S. Patil, Rani P. Pawar, Aditi D. Yadav, Dada P. Nade, T. Dharmaraj, Sanjay V. Pore, Sambhaji M. Pawar, Sunil D. Pawar

Storm-time hourly morphologies of Equatorial Ionization Anomaly (EIA) crests along 110-125<sup>o</sup>E meridian during 2013 St Patrick’s Day geomagnetic storm

Publication date: Available online 19 November 2025

Source: Advances in Space Research

Author(s): A.O. Akala, B. Olugbon, P.O. Amaechi, O.J. Oyedokun, J.A. Ayangbemi, E.O. Oyeyemi, Y. Otsuka

Two centuries of tree rings reveal hydroclimatic patterns and mega-drought impacts in China's Central Water Tower

Phys.org: Earth science - Tue, 11/25/2025 - 18:06
The Qinling-Bashan Mountains (QBMs) serve as an important boundary between southern and northern China and are dubbed China's Central Water Tower (CCWT). However, the spatiotemporal structures and dynamics of the summer hydroclimate, as well as the water vapor sources and mechanisms in this CCWT during the peak and most concentrated precipitation period, which is crucial for forest growth, crop yield, and water management, remain unclear.

Earth system models overstate carbon removal: New findings suggest nitrogen fixation is 50% lower than thought

Phys.org: Earth science - Tue, 11/25/2025 - 17:41
High levels of atmospheric carbon dioxide intensify climate change, but high carbon dioxide levels can also stimulate plant growth. Plant growth removes carbon dioxide from the atmosphere, partially mitigating the effects of climate change. However, plants only grow faster in the presence of high levels of carbon dioxide if they can also acquire enough nitrogen from the atmosphere to do so.

Earthquakes shake up Yellowstone's subterranean ecosystems

Phys.org: Earth science - Tue, 11/25/2025 - 15:31
Up to 30% of life, by weight, is underground. Seismic activity may renew the energy supply for subterranean ecosystems. Published in PNAS Nexus, Eric Boyd and colleagues chronicled the ecological changes in subsurface microbial communities that took place after a swarm of small earthquakes rattled the Yellowstone Plateau Volcanic Field in 2021.

Uranus’s Small Moons Are Dark, Red, and Water-Poor

EOS - Tue, 11/25/2025 - 14:13

The solar system’s oddball planet has some pretty odd moons, too. The first infrared spectra of Uranus’s small inner moons, which will be presented on 18 December at the 2025 AGU Annual Meeting in New Orleans, have shown that their surfaces are much redder, much darker, and more water-poor than the larger moons orbiting far from the planet.

“We were trying to see how these properties varied across the rings and moons,” said Matt Hedman, a planetary scientist at the University of Idaho in Moscow and a coauthor on the research. “We didn’t have a lot of information about their spectra before because they’re hard to observe.”

The new observations also revealed that some moons were not quite where they should have been, highlighting how much more astronomers have to learn about the dynamics of the Uranian system.

Small, Dark, and Red

In 1986, Voyager 2 flew past Uranus in humanity’s only visit to the system. At that time, astronomers knew only of the planet’s five major moons and a handful of rings. Voyager 2 discovered 11 more moons and was able to roughly measure their sizes. Since then, scientists have used ground- and space-based telescopes to discover more than a dozen additional satellites, bringing Uranus’s moon total to 29.

Many of the more recently discovered moons are pretty tiny, from Sycorax at 150 kilometers across to Mab and Cupid at just 10 kilometers. Most of them also orbit within or just outside Uranus’s ring system, close to the much brighter planet.

All of these properties have made it tricky for astronomers to learn more about the smallest Uranian moons. That’s where the infrared powerhouse James Webb Space Telescope (JWST) comes in.

This diagram shows the orbital distances of Uranus’s inner moons and rings, to scale. Uranus is placed at the top of the diagram. Click image for larger version. Credit: Ruslik0/Wikimedia Commons, Public Domain

“Part of what makes JWST particularly good for this compared to, say, Hubble and other optical telescopes, is that in the infrared, Uranus is much fainter, so you can see the things orbiting it way more easily,” Hedman explained. What’s more, all of the spectral features the team was interested in, like water ice, occur at wavelengths that JWST can observe.

The researchers observed Uranus at several infrared wavelengths in February and got a deep look at the inner portions of the planetary system. They wanted to characterize the known small moons and search for new ones. They did discover a previously unknown moon, temporarily named S/2025 U1, orbiting just outside the epsilon ring.

Those observations also provided the first information on the infrared brightnesses of the smallest moons, many of which have remained elusive since the Voyager flyby.

“Most of the rings and inner moons show very similar properties,” Hedman said. They tend to be much redder, darker, and more water-poor when compared with the larger outer moons Miranda, Ariel, Umbriel, Titania, and Oberon.

“And then there’s Mab,” Hedman added.

The new spectra show that Mab’s surface is bluer and more water-rich than the other inner moons, said Jacob Herman, a physics graduate student at the University of Idaho and lead author on the research. In fact, its surface spectrum looks very similar to Miranda’s, the major moon that orbits closest to the rings and to Mab. Miranda’s jigsaw surface suggests a messy history.

“There is still much to be discovered about Uranus’s small inner moons, particularly regarding their origin, composition, and long-term orbital stability.”

Did the two moons encounter each other sometime during Uranus’s chaotic past? Could that encounter be related to Uranus’s mu ring, which is likely generated by material sloughing off Mab? Hedman hopes that future observations or a long-term mission to Uranus will provide those answers.

“These new measurements significantly expand our current knowledge, revealing, for instance, striking variations in the composition and reflectivity of the surfaces of moons such as Mab, Cupid, and Perdita,” said Jadilene Xavier, an astrophysicist at São Paulo State University in Guaratinguetá, Brazil, who was not involved with this research.

“There is still much to be discovered about Uranus’s small inner moons, particularly regarding their origin, composition, and long-term orbital stability,” Xavier said. “More precise data on their density, three-dimensional shape, and surface properties would be essential to determine whether these moons are fragments produced by collisions, captured objects, or primordial remnants associated with the formation of Uranus’s ring system.”

Just a Little Bit Off

Because Voyager 2 spent only a short time visiting Uranus, it could provide only limited information about the small moons’ orbital periods and distances, sometimes with large uncertainties. When the researchers compared the moons’ current positions with the positions predicted by Voyager 2 data, some of the moons were not where they seemingly should have been.

“Perdita was quite a bit off,” Herman said. “And there’s also Cupid, which was surprising.” The positions of Cordelia, Ophelia, Cressida, and Desdemona were also off, but not by much. The team is still trying to figure out whether the differences are just a matter of having more precise observations of these tiny objects or if there are unknown dynamics in play.

“These new observations are quite useful for improving our understanding of the inner Uranian system, especially its orbital dynamics.”

“These new observations are quite useful for improving our understanding of the inner Uranian system, especially its orbital dynamics,” said Matija Ćuk, who researches solar system dynamics at the SETI Institute in Mountain View, Calif.

Ćuk, who was not involved with this research, pointed out that Cordelia and Ophelia shepherd Uranus’s epsilon ring, Cressida and Desdemona are part of a pack of moons with chaotic orbits, and Perdita is known to interact with another moon, Belinda. “So the fact that these [five] moons are not in their predicted positions is valuable for understanding the system, but I wouldn’t say it’s unexpected,” Ćuk said.

These observations hint at just how many mysteries Uranus is still hiding.

“For a dynamicist like me,” Ćuk said, “knowing the precise masses of these moons would be ideal, because then we could predict their future interactions and also estimate with some confidence how stable they are on long timescales.”

Hedman and their team plan to observe the Uranian system again with JWST, are looking through archived and technical images, and hope to establish long-term monitoring to better understand the moons’ dynamics and possibly estimate their masses. The researchers are also leaning on their colleagues who simulate planetary orbits to better understand how Uranus’s moons and rings might be influencing each other.

“It’s a very dynamic and interconnected system,” Herman said.

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

Citation: Cartier, K. M. S. (2025), Uranus’s small moons are dark, red, and water-poor, Eos, 106, https://doi.org/10.1029/2025EO250442. Published on 25 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.

Theme by Danetsoft and Danang Probo Sayekti inspired by Maksimer