Sunbirds may look similar to hummingbirds — small, iridescent birds with thin bills — but it turns out the two are only distantly related. Sunbirds live primarily in Africa, Asia and Australia, and have a unique way to slurp up nectar. Unlike hummingbirds, which use minute movements in their bills to sip nectar, sunbirds use their tongues as a straw. published in Current Biology, a team led by researchers at the �������� showed that these long-billed birds can change the pressure at the base of their tongues to create suction that moves nectar through their tongues and into their mouths, a novel mechanism never before seen in vertebrates. The researchers used multiple techniques — including high-speed video of sunbirds drinking red-dyed nectar from transparent artificial flowers — to demonstrate this phenomenon across multiple sunbird species as well as build a mathematical model that describes how it works. Sunbirds pollinate the flowers they drink from, and researchers are interested in understanding how different sunbird species’ plant preferences affect the plant-pollinator networks across continents.

For more information, contact lead author , who completed this research as a UW doctoral student in biology, at david_cuban@brown.edu.����

The other UW co-author is . A full list of co-authors and funding is included . Related stories in and .��

Seattle Fault gets 5,000 more years of sleep��

Just over 1,100 years ago an on the Seattle fault rocked — and reshaped — the Puget Sound region. It lifted the sea floor and sent a powerful tsunami through the sound. Researchers have estimated that this fault, which runs east to west beneath the middle of the city, will produce a large earthquake every 5,000 years or so. However, , recently published in Geology, pushes that estimate back to 11,000 years. The researchers extended this window by scouring submerged shorelines for evidence of significant elevation changes. The geological record at these sites dates back 11,000 years, but they only found evidence of one major earthquake. This information could be useful to those making seismic hazard maps, which help people understand the risks associated with different regions. Although other regional faults and the imposing pose more imminent risks to residents, the main Seattle fault doesn’t appear to be ready for rupture anytime soon.

For more information, contact lead author , UW research scientist of Earth and space sciences, at edav@uw.edu.

The other UW co-author is . A full list of co-authors and funding is included in the paper. Related story in .

The PNW has many rivers, but no system for gauging landslide dam risk

Scientists have a new tool for estimating lesser known hazards in the Pacific Northwest: and outburst floods. Landslides along rivers can block the flow of water downstream, creating a lake just above the slide area. Most landslide dams fail within 10 days, releasing trapped water in an outburst flood, which can be devastating. Last fall, 20 people died after in Taiwan. published in Natural Hazards and Earth System Sciences, UW researchers debut a mathematical approach to mapping landslide dam hazards based on valley width and projected slide size. When they applied the tool to a mountain range in Oregon, they found that roughly one-third of rivers in the study area were susceptible to landslide dams, with risk increasing in mountainous areas. If a landslide dam does form, alleviating pressure by for water to escape can help prevent flooding. Identifying high risk areas can help guide emergency response efforts following storms, earthquakes and other events that increase landslide risk.

For more information, contact lead author , UW doctoral student of Earth and space sciences, at pmmorgan@uw.edu.

The other UW co-author is . A full list of co-authors and funding is .

Rubin observatory expected to spot many ‘imminent impactor’ asteroids

Small asteroids — those 1 to 20 meters in diameter —�� hit the Earth 35-40 times per year, though they’re very rarely spotted by telescopes before impact. That could soon change: published in The Astrophysical Journal, UW astronomers calculate that the Simonyi Survey Telescope at the NSF-DOE Vera C. Rubin Observatory could discover one to two Earth-impacting asteroids annually , roughly doubling the number currently logged. The researchers expect Rubin to discover these asteroids an average of 1.5 days before impact, which is more warning time than ever before. Advance notice is extremely valuable in the case of larger asteroids that could be a threat to people or infrastructure. Because the Rubin Observatory is located in the Southern Hemisphere, it will likely discover many Earth impactors that existing asteroid surveys — concentrated in the Northern Hemisphere — miss.

For more information, contact lead author Ian Chow, a UW graduate student of astronomy, at chowian@uw.edu.

Other UW co-authors are Mario Jurić, Joachim Moeyens, Aren N. Heinze and Jacob A. Kurlander. A full list of co-authors is included .

Many marine microbes share a genetic toolbox for fixing supper at sea

Researchers have now identified a set of genes that allow some bacteria to process a compound, called homarine, that is abundant in the ocean and appears to play a key role in nutrient cycling. Phytoplankton produce loads of homarine, but scientists weren’t sure what became of it until now. In a recent study published in Nature Microbiology, researchers found a set of genes present in common and far-flung bacteria that convert homarine into glutamic acid, an essential building block for life. This suggests that homarine may be a vital and overlooked resource and highlights the importance of bacteria in stabilizing marine ecosystems. Previous studies also found that homarine serves as and helps small crabs . The UW team will continue studying homarine to better understand how it fits into the broader ecological landscape.

For more information, contact senior author , a UW professor of oceanography, at aingalls@uw.edu.��

The other UW co-authors are , , , , , and �� A full list of co-authors and funding is

Mammals and dinosaurs coexisted on Earth until . Despite the devastation, some animals survived, including rodent-like mammals in the Cimolodon genus. These creatures are part of , a group that arose during the Jurassic Period and survived over 100 million years before going extinct. Studying these animals helps researchers better understand how mammals survived the mass extinction event and then diversified into the variety of mammals around today.

A research team led by the �������� has identified a new species in the Cimolodon genus from a fossil the team discovered at a research site in Baja California. The researchers estimate that this fossil is about 75 million years old. The new species, named Cimolodon desosai, was about the size of a golden hamster, the researchers said. It likely scampered on the ground and in trees and ate fruits and insects.

The researchers April 22 in the Journal of Vertebrate Paleontology.

“The genus Cimolodon was a pretty common mammal during the Late Cretaceous, the last epoch of the Age of Dinosaurs. Cimolodon fossils have been found throughout western North America, from western Canada down through Mexico,” said senior author , a UW professor of biology and curator of vertebrate paleontology at the Burke Museum. “This new species, Cimolodon desosai, was ancestral to the species that survived the extinction event. It and its descendants were relatively small and omnivorous — two traits that were advantageous for surviving.”

When Wilson Mantilla and his team discovered the fossil in 2009, they found teeth, a skull, jaws and parts of the skeleton, including a femur and an ulna.

“It’s very hard to find fossils at this site compared to other areas,” Wilson Mantilla said. “At first, my field assistant found just a little tooth poking out. If he had just found that, I would have been over the moon. But then when we looked inside the crack of the rock, we could see there was more bone.”

The fact that the researchers uncovered more than just teeth for C. desosai means that they can better understand its size and shape and how it likely moved. It also helps fill out the picture of this genus and the habitat in which it lived, and contributes to a better understanding of the multituberculate group in general.

The researchers used digital imaging and a tool called micro-computed tomography, or micro-CT, to get high resolution images of the fossil. Then the team compared the teeth of C. desosai to those of its cousins in the Cimolodon genus to establish it as a new species.

“That far back in time everything is named based on their tooth characteristics,” Wilson Mantilla said. “If you find a skeleton that’s missing teeth, sometimes it’s hard to attach it to a name.”

The team named this species after Michael de Sosa VI, the field assistant who first found it, because de Sosa died while they were still analyzing the fossil.

“He was a great field assistant, and he was like a little brother to me,” Wilson Mantilla said. “It’s a great specimen to be associated with.”

Additional co-authors are , UW doctoral student in biology, at the University of Rhode Island; Yue Zhang, who completed this research as a UW postdoctoral fellow in biology; Meng Chen, who completed this research as a UW doctoral student in biology; and and at the Universidad Nacional Autónoma de México.

This research was funded by UC MEXUS-CONACYT, Dirección General de Asuntos del Personal Académico PAPIIT IN111209-2, the UW College of Arts and Sciences, the UW Department of Biology and the American Philosophical Society.

For more information, contact Wilson Mantilla at gpwilson@uw.edu.

As far as research subjects go, it’s not always easy to find common ground with a single-celled bacterium. Yet the more studies his model bacteria, , the more he sees surprising commonalities between their behavior and our own as humans.

“It was mortifying to be stumped for so long by what appeared to be completely counterintuitive behavior only to realize that I engage in exactly the same behavior everyday,” said Wiggins, an associate professor of both physics and bioengineering at the ��������.��

Scientists in use experiments and modeling to understand the global principles that govern gene expression, and protein abundance in particular. In in Science Advances, Wiggins’ team discovered that A. baylyi cells amass huge surpluses of essential proteins, rather than taking the seemingly more efficient approach of making just enough to survive. UW News chatted with Wiggins to learn about the remarkably relatable reason for this puzzling behavior.

This work grew out of a mystery you and your team uncovered. Tell us about that mystery.

Paul Wiggins: Genes are the blueprints for proteins — we say they “code for proteins.” A. baylyi has a number of genes that code for proteins that we know are essential for cell growth. But we didn’t know exactly what each of these proteins do. In 2016, we were attempting to uncover these proteins’ specific functions in collaboration with the . To do this we disrupted each gene so that the cells couldn’t make any more protein — they were left with a now dwindling supply of whatever they’d previously made. Then we would watch the cells under a microscope to determine when and how cellular processes would fail.��

As an example, we knocked out a gene that coded for a protein that we found was responsible for cell wall synthesis — it makes the protein-sugar chainmail that prevents the cells from rupturing, or lysing. And you can watch the video we recorded to see what happened: The cells grew and divided for a while, but then all of a sudden they inflated and just popped.

In that example, something strange happened. We would expect the cell walls to start to fail almost immediately after the disruption happened because every time the cells divide, the remaining protein is divided among the offspring cells, so pretty quickly there wouldn’t be enough to sustain the new cell walls. However, growth continued, one generation after another, before the cells finally failed after four rounds of division!

Why did it take so long? Gene after gene showed the same pattern. We realized that each cell must have made a ton of extra proteins — far more than it needed. So after we knocked out that essential gene, the cell was able to run on fumes for a while — and was even able to pass stores of that protein on to its offspring. That finding was initially a huge surprise. We all expected, naively, that if a cell only needed a few copies of a protein to function, it would only make a few — anything more would be a waste of resources and energy. It’d be like taking a seven-day trip and packing 30 pairs of socks. And yet, this behavior seemed to be common for lots of essential genes.��

What do you think is the cause of this protein overabundance?

PW: Baking is a good analogy. If you want to make an apple pie, you probably only buy as many apples as you need for that recipe. But you keep a large quantity of salt in your pantry. You might only need a teaspoon of salt to make any given meal, but none of us go to the store and buy salt a teaspoon at a time. Salt is so cheap and easy to store that, relative to the cost of other ingredients in your meal, it’s basically free to keep in large quantities. And critically, you don’t want to run out of salt when you’re cooking.��

We demonstrated that something analogous is happening in A. baylyi cells for most of the essential genes. Only about 30% of a cell’s essential genes code for proteins that are “expensive” in that the cells need these proteins in large numbers. It would be very costly to, say, double an already large number. These are the apples in our apple pie analogy — the cell makes just enough of those proteins to get by.��

The remaining 70% of essential genes, however, code for proteins that the cell does not need in large numbers. In fact, relative to that other 30%, the cell needs so few of these proteins that it’s basically free to produce a bunch of extras. Doubling the production of those proteins, say from 30 to 60 copies, is a drop in the bucket if the cell’s overall budget is three million proteins. So the cell says, “Screw it, it’s virtually free. Let’s make extra so we don’t run out.” In some cases a cell might make 10 times more protein than it will ever need.

Why is this strategy useful for the cells?

PW: This overabundance strategy is important because otherwise a cell might fail to produce enough of something critical. Protein synthesis is an imprecise process — cells sometimes make a little more or a little less of things than they’re programmed to make. Some essential proteins are made at such low numbers that any deviation from the plan could leave a cell with zero copies of that protein. This is less of a problem for essential proteins that are made in much higher numbers.��

How do these findings support or challenge previous ideas about how cells function?

PW: Depending on who you talk to, this is either definitely wrong or completely obvious. On the one hand, it’s a really ingrained idea that organisms are always optimizing everything, which would naively suggest that cells should make exactly what they need — no more, no less. However, this is clearly not the case. Other studies have observed these kinds of protein surpluses in cells before, but it wasn’t appreciated quite how wide-spread this phenomenon was. Previously researchers proposed that overabundance might be a hedge against changing conditions — maybe cells are stockpiling proteins in case times get tough. We’re suggesting that it’s a hedge against the cells failing to make the right number of essential proteins.

Co-authors include , a UW postdoctoral researcher of physics; Teresa W. Lo and , former UW doctoral students of physics; , a UW graduate student of physics; and , a UW postdoctoral researcher of laboratory medicine and pathology.

This research was funded by the National Science Foundation and the National Institutes of Health.

For more information, contact Wiggins at pwiggins@uw.edu.��

�������� professor of physics and UW research professor emeritus are part of an international team that won the 2026 . The $3 million award is shared among roughly 400 scientists, including 18 other researchers from the UW team. It celebrates decades of work to better understand the muon — a subatomic particle with anomalous properties. This collaborative effort could ultimately lead to the discovery of entirely new particles.

“A remarkable aspect of these experiments is that it took the collective talents and experience of scientists and engineers from particle, nuclear, atomic, optical, accelerator and theoretical physics communities to work coherently toward one single goal,” Hertzog said. “Together, we measured a property of the muon that encapsulates almost everything we know about modern physics from relativity to quantum mechanics to the zoo of particles that govern the fundamental forces that shape our world.”

The were established in 2012 to recognize research achievements in life sciences, fundamental physics and mathematics.��

Muons, short-lived subatomic particles, are created for experiments by particle accelerators. They exist for a fraction of a second before decaying into electrons and even tinier particles called neutrinos. During their short life, muons exhibit magnetic properties that deviate slightly from the – the leading theory that describes the particles and forces that make up the universe, along with anything that exists that has not yet been discovered.

The experiments recognized by the Breakthrough Prize represent 60-plus years of work to find out exactly how far the muon’s magnetism strays from Standard Model predictions. The first experiments began in 1959 at the, also called CERN.��

Hertzog’s group at the University of Illinois was involved in a later experiment at the in the mid-1990s. He joined the faculty at UW in 2010 and helped develop a new experiment at (Fermilab) that in 2025 with record-setting precision.��

While Hertzog and others have now completed their experimental measurements, theorists�� continue to refine the predictions of the Standard Model. In time, the gap between theory and experiment — where the muon currently hovers — may vanish or persist. If the muon’s properties never fit the Standard Model, physicists may need to explore entirely new theories.��

“No matter where the final theory settles, the comparison with our experiment will have important consequences and give us deep insight into the heart of matter,” Hertzog said.

Many UW physicists have been recognized by Breakthrough Prizes since the prizes’ inception, including a banner year in 2021 that also featured a win in the life sciences category by Nobel Prize laureate , a UW professor of biochemistry.

“The Breakthrough Prize has previously recognized UW physicists for work that deepened our understanding of gravity, dark energy and dark matter,” said , UW divisional dean of natural sciences in the College of Arts and Sciences. “This latest recognition is a testament to the value of large-scale collaborative physics research and we are very proud of the accomplishments of all of the UW faculty, postdocs and students who contributed to this effort.”

A full list of current UW researchers recognized by the 2026 prize . Learn about other UW wins at the Breakthrough Prize here.��

For more information, contact Victor Balta at balta@uw.edu.

The Ecological Society of America on Wednesday awards. , a �������� assistant professor of environmental and forest science, was named an Early Career Fellow, which recognizes scientists for contributions to advancing and applying ecological knowledge within eight years of completing a doctorate.

Willing studies how microbes respond, and help plants cope with, environmental change. focuses on fungi and other microbes living near plant roots. Much like the gut microbiome, these communities play a critical role in plant nutrition, immune function and overall forest health.

Willing’s lab focuses on understanding these communities and how they are shifting with climate change. Her research integrates methods from various scientific disciplines to gain insight into the ecosystem-wide impact of fungi.

“I work across pretty diverse fields, from fungal ecology to plant and forest ecology,” Willing said. “Integrating everything together is challenging, but I think it’s a critical intersection to study right now and this award is a nice acknowledgement of that.”

As a Faculty Fellow, Willing also collaborates with federal, state and tribal agencies to incorporate fungi into climate adaptation planning.

Many of her lab’s projects examine responses to climate change. For example, one of Willing’s current grad students is studying fungi in post-fire ecosystems.

Some fungal groups are fire-adapted, meaning that they can withstand wildfire better than others. After wildfire, the soil often becomes hydrophobic, which causes water to run off the surface instead of soaking in. This increases the risk of erosion, among other consequences. Fungi help seedlings to establish and stabilize the soil by helping it retain water.

Early findings from her lab indicate that prolonged fire suppression, a stewardship strategy intended to minimize wildfire impacts, can limit microorganisms fire tolerance, which then exacerbates the damage caused by a fire.

“There are lots of different nuances that we’re really just starting to understand,” Willing said.

She hopes this work can help inform future forest management practices. Although there are many mushroom enthusiasts in the Pacific Northwest, Willing is one of few scientists in the region studying how these organisms fold into broader ecosystems.

Most of the data on microbial communities was collected within the past 20 years or so, which makes it difficult to gauge how these organisms are responding to climate change. Another project in Willing’s lab involves conducting genetic analyses on preserved plant specimens to establish a baseline for fungal health.

“Our understanding of what fungal and bacterial communities were like before the onset of rapid warming is really limited,” Willing said.

Building this baseline will help researchers see how microbial communities are evolving and reveal management opportunities.

Without fungi, life on Earth couldn’t exist as we know it. Dead logs and fallen leaves would simply accumulate, with nothing to break them down and return their nutrients to the soil.

“Fungi are involved in everything,” Willing said. “In the cycle of life, they are at the beginning, helping plants to take root across every ecosystem on Earth, and at the end, helping to create lush soils for future life to flourish.”

ESA will acknowledge and celebrate fellows during a ceremony on July 27 at the annual meeting in Salt Lake City. Early Career Fellows are elected for five years.

For more information about her work, contact Willing at willingc@uw.edu.

Unfortunately for science fiction fans, desert worlds outside our solar system are unlikely to host life, according to new research from ��������. Scientists show that an Earth-sized planet needs at least 20 to 50% of the water in Earth’s oceans to maintain a critical natural cycle that keeps water on the surface.

Scientists believe that there are billions of planets outside our solar system. More than are confirmed, but only some of them are candidates for life. The search for life has focused on planets in the “,” a sweet spot that is neither too close nor too far from a central star. Planets in this zone are considered viable because they can maintain liquid surface water.

“When you are searching for life in the broad landscape of the universe with limited resources, you have to filter out some planets,” said lead author , a UW doctoral student of Earth and space sciences.

Water, although essential, does not guarantee the existence of life. With this study, researchers worked to further narrow the search by investigating planets with just a small amount of water.

“We were interested in arid planets with very limited surface water inventory — far less than one Earth ocean. Many of these planets are in the habitable zone of their star, but we weren’t sure if they could actually be habitable,” White-Gianella said.

The team’s results, , show that habitability hinges on the geologic carbon cycle — a water-driven process that exchanges carbon between the atmosphere and interior over millions of years, stabilizing surface temperatures.

Carbon dioxide, which comes from volcanoes in a natural system, accumulates in the atmosphere before falling back to Earth dissolved in rainwater. Rain erodes and chemically reacts with rocks on the Earth’s surface and runoff transports carbon to the ocean, where it sinks to the seafloor. Plate tectonics drives carbon-rich oceanic plates below continental land. Millions of years later, carbon resurfaces as mountains form.

If water levels drop too low for rainfall, carbon removal — from weathering — can’t keep up with emissions from volcanic eruptions and carbon dioxide levels in the atmosphere spike, trapping water. Rising temperatures evaporate the remaining surface water, initiating runaway warming that makes the planet too hot to support life.

“So that unfortunately makes these arid planets within habitable zones unlikely to be good candidates for life,” White-Gianella said.

Although scientists have instruments that can measure surface water, rocky exoplanets are difficult to observe directly. In this study, the researchers ran a series of complex simulations to better understand how water might behave in these desert worlds.

Previous efforts to model the carbon cycle focused on cooler, perhaps wetter planets. The models factored in evaporation from sunlight, but didn’t include other drivers, such as wind. White-Gianella adapted existing models to drier planets by refining evaporation and precipitation estimates.

“These sophisticated, mechanistic models of the carbon cycle have emerged from people trying to understand how Earth’s thermostat has worked — or hasn’t — to regulate temperature through time,” said senior author , a UW assistant professor of Earth and space sciences.

However, the function of the geologic carbon cycle on arid planets was largely unexplored. The results show that even planets that form with surface water could lose it, transitioning from potentially habitable to uninhabitable due to carbon cycle disruption.

One such planet exists far closer to home: Venus. The planet of love is roughly the same size as Earth, likely formed around the same time and may have started with a similar amount of water.

Yet today, the surface of Venus rivals the temperature of a wood-fired pizza oven. Standing on the surface would feel like being crushed by 10 blue whales, White-Gianella said.

Many theories attempt to explain why Earth and Venus are so different. White-Gianella and Krissanen-Totton propose that Venus, being closer to the sun, may have formed with slightly less water than Earth, which imbalanced the geologic carbon cycle. As surface temperatures rose with atmospheric carbon dioxide levels, Venus lost its water — and any life it may have hosted.

Upcoming missions to Venus will attempt to understand what happened to the planet and whether it ever hosted life. The findings could also offer insight into planets much farther away.

“It’s very unlikely that we will land something on the surface of an exoplanet in our lifetime, but Venus — our nextdoor neighbor — is arguably the best exoplanet analog,” White-Gianella said.

The researchers hope that results from future missions will help validate the results of their modeling.

“This has implications for a lot of the potentially habitable real estate out there,” Krissanen-Totton said.

This study was funded by the National Science Foundation, the NASA Astrobiology Program and the Alfred P. Sloan Foundation.

For more information, contact White-Gianella at hasktw@uw.edu or Krissanen-Totton at joshkt@uw.edu.��

Weasels are small carnivores with a long body and short legs. They also have a stout skull and sharp teeth. These creatures, along with ferrets and minks, make up the Mustelinae subfamily.

Until now, researchers believed that the oldest fossils from this family were from Poland and Germany, dating back to about 3.5 million years ago in the . But a fossil discovered in Teruel, Spain, has doubled that estimate, dating back to the late , around 6.5 million years ago.

The research team, including , a �������� principal research scientist in the biology department, has identified this fossil as belonging to a new species, named Galanthis baskini. The researchers estimate that this creature was about 5 ounces, comparable in size to the smallest living carnivoran today, the or Mustela nivalis. Much like the modern weasel, G. baskini was also likely a carnivore, based on its teeth.

The team in Palaeontology.

“This study begins to uncover the evolutionary history of modern weasels, specifically, why do they have unique small, elongated bodies compared to all other mammals?” said Law, who is also an affiliate curator at the UW Burke Museum of Natural History and Culture. “We had hypothesized that events during the mid- to late-Miocene — both the expansion of open habitats, such as grasslands, and the diversification of rodents — would have allowed weasels to evolve bodies that were small and flexible enough to chase rodent prey in small crevices underground. G. baskini is exciting because it confirms that weasels were present in the Late Miocene. And it’s pretty cool that G. baskini was the size of the least weasel — that means small weasels were already around more than 6 million years ago.”

To compare this fossil to other weasel family members, the researchers used a combination of classical comparative anatomy with advanced analytical techniques, such as micro-computed tomography, or micro-CT. Micro-CT allowed the team to three-dimensionally reconstruct the internal structure of teeth and jaws as well as observe anatomical features that were not externally visible.

“The new genus, Galanthis, is named after a figure from Greek mythology who was transformed into a weasel, symbolizing the fossil’s significance as representing the origin of the weasel family and the lineage leading to modern species,” said senior author , assistant professor of paleontology at Complutense University of Madrid.

The fossils come from excavations carried out in the 1990s in the Teruel area of Aragón, Spain.

“This research is a clear example of the remarkable richness of Aragón’s fossil record of mammals, recognized worldwide,” said co-author , professor at the University of Zaragoza. “Our team has been contributing for decades to excavations and the study of fossil mammals.”

The study also revises the classification of another fossil of a similar age discovered in China. This fossil has now been assigned to the genus Zdanskyictis.

The next step, the researchers said, will be to find new fossils that help reconstruct in greater detail the early evolution of weasels and their relatives.

“Ideally, we will find an entire skeleton of a fossil weasel,” Law said. “That way we can actually quantify just how elongate these ancient weasels were and when body elongation actually evolved.”

A full list of co-authors and funding .

For more information, contact Law at cjlaw@uw.edu.��

Adapted from a release from Complutense University of Madrid.

Even on a campus like the ��������’s — home to particle accelerators, wave tanks and countless other bespoke pieces of equipment — the machinery in the stands out. Take the dilution fridge, a large, white, cylindrical device that can cool a small chamber to one hundredth of a kelvin above absolute zero — the coldest possible temperature in the universe.��

“This is the coldest fridge money can buy,” said , a UW assistant professor of electrical and computer engineering and the former director of the lab, which goes by the nickname QT3. “When it’s running, the chamber inside this device is about 100 times colder than outer space. At that temperature, it’s much easier to study and manipulate a material’s quantum properties.”

The lab also houses a photon qubit tabletop lab: a nondescript set of boxes, lasers and lenses that can demonstrate the “spooky” — a term scientists actually use — phenomenon known as quantum entanglement, where two particles appear to communicate instantaneously with each other despite being physically apart.

Or there’s the lab’s latest acquisition, the scanning tunneling microscope, which can image individual atoms within a solid material, allowing researchers to study the structure of materials at the smallest scales.

An interdisciplinary group of researchers has been marshalling resources and expertise to create QT3 for three years, and now, the lab is opening its doors as a unique one-stop shop resource for quantum researchers and educators at the UW.

“The idea of this lab is to improve access to quantum hardware,” Parsons said. “It’s rather hard to acquire equipment like this. And there are a lot of researchers that may have good ideas that they want to test, but don’t have the resources yet for their own equipment. So we’re inviting researchers, initially from across campus, but also from other universities and from industry, to come in and test their ideas. This can be a hub for quantum experts to share their ideas and collaborate.”

The lab also boasts hardware that can demonstrate known quantum principles and techniques, making it useful for students in quantum fields. In addition to the entanglement device, Parsons’ students developed a machine that can suspend charged particles — in this case, tiny grains of pollen — in midair using electric fields. Researchers use the same technique to trap single atoms and manipulate their quantum properties, making the lab’s ion-trapping machine good practice for more complex work.

Some students even work at the lab through an undergraduate staffing program, and have helped install instrumentation, write code to power equipment and build parts for custom microscopes. The program provides yet another avenue for students to get hands-on experience with unusual machinery and techniques.��

“Quantum mechanics is inherently counterintuitive, and that makes it a powerful teaching tool,” Parsons said. “In the QT3 lab, students will encounter systems where their everyday intuition breaks down, and they must rely on careful reasoning and experimentation instead. They learn how to debug when results don’t match expectations, how to test simple cases and how to build understanding about hardware step by step.”

The cosmically cold dilution fridge remains something of a centerpiece, even as the lab fills up with specialized equipment. The extreme environment within the device strips heat, light and other stray energy away from materials, allowing researchers to observe the peculiar quantum properties that remain. One such property is superposition, or the ability of a particle like an electron to maintain multiple mutually exclusive properties at the same time. Scientists use superposition to create a powerful, tiny piece of technology: a quantum bit, or qubit.��

“Traditional computers use bits, which can only be one or zero. A qubit, on the other hand, we can make one plus zero,” Parsons said. “It’s both at the same time, and only when we measure it do we find out which one it is. We can use this unusual property to build a new class of computers that excel at tasks like communications and encryption.”

QT3 is part of a collaborative effort to solidify UW as a leader in quantum research and applications. Most of the lab hardware was funded by a congressional earmark championed by Senator Maria Cantwell’s office. Departmental funding from across the College of Engineering and the College of Arts and Sciences helped rehab the lab space. The National Science Foundation provided seed funding for the instructional lab equipment.

The UW has also spent the past decade investing heavily in faculty with quantum expertise.

“Very few places have expertise across the full quantum stack, from materials up to algorithms,” said , a UW professor of physics and founder of QT3. “The UW has quantum faculty in electrical and mechanical engineering, physics, computer science, materials science and chemistry. Our faculty work on superconducting qubits, spin defects, photons, trapped ions, neutral atoms and topological qubits. Our advantage is the breadth of our investment.”

The lab is now available to researchers and students across the UW, and private companies are encouraged to reach out about partnering. Parsons has already used the lab to teach a graduate-level class in electrical and computer engineering for students who included employees from Boeing, Microsoft and quantum computing company IonQ. The lab is hiring for a full-time manager to maintain the equipment and help users make the most of the facility.��

“Here in academia, we can improve the building blocks for applied technologies like quantum computing, and then transfer those learnings to industry for further scaling,” Parsons said.

For more information, contact Parsons at mfpars@uw.edu.

New evidence suggests that a disease-causing tapeworm that has been spreading across the United States and Canada has arrived in the Pacific Northwest. The tapeworm, called Echinococcus multilocularis, lives as a parasite in coyotes, foxes and other canid species and can cause severe disease if passed to domestic dogs or humans.

E. multilocularis has long been recognized as a public health threat in parts of the Northern hemisphere, including Europe and Asia, but was considered extremely rare in North America until approximately 15 years ago, when cases in humans and dogs began cropping up in Canada and the midwestern U.S., indicating that the parasite was spreading.

This study, led by �������� researchers, is the first to detect E. multilocularis in a wild host on the west coast of the contiguous U.S. Researchers surveyed 100 coyotes in the Puget Sound region, and found E. multilocularis in 37 of them. The results were .

“This parasite is concerning because it has been spreading across North America. There have been numerous cases of dogs getting sick, and a handful of people have also picked up the tapeworm,” said lead author , who recently graduated from the UW with a doctorate in environmental and forest science. “The fact that we found it here in one-third of our coyotes was surprising, because it wasn’t found anywhere in the Pacific Northwest until earlier this year.”

When E. multilocularis infects an animal or person, it causes cancer-like cysts to form in the liver and sometimes other organs. If untreated, infection can be fatal.

However, not all carriers become sick. E. multilocularis has a complex life cycle that involves multiple hosts. Canids, which host adult parasites, can support thousands of worms in their intestines without becoming sick. The worms shed eggs that are then passed in their feces.

Rodents — another host — become infected by eating food contaminated with coyote feces. Once consumed, the parasite eggs migrate to the liver and form cysts, ultimately weakening or killing the rodents. The parasite’s life cycle begins again when coyotes prey upon infected rodents.

Humans and domestic dogs are categorized as accidental hosts. Humans may pick up the parasite by consuming tapeworm eggs — in food that is contaminated with coyote or dog feces, for example — and can develop a disease called , characterized by slow-growing metastatic cysts. Symptoms may not appear for five to 15 years after exposure, which complicates diagnosis and treatment.

Alveolar echinococcosis is considered the third most important food-borne illness globally, and one of the top 20 neglected tropical diseases by the World Health Organization. Many countries have developed robust protocols for tracking it.

Domestic dogs that are exposed to E. multilocularis may or may not become sick, depending on where the parasite is in its life cycle at exposure. It is more common for dogs to carry the parasite and shed eggs without developing disease, but dogs that are exposed to parasite eggs may develop the same cancer-like cysts as other infected animals.

“To minimize the risk of dogs getting infected with E. multilocularis, owners should not let them prey on rodents or scavenge their carcasses,” said co-author , an associate professor and director of the Parasitology Diagnostic Laboratory at the Texas A&M University College of Veterinary Medicine and Biomedical Sciences.

Owners can also give dogs preventative medication for worms and ticks and ensure routine veterinary care, which should include diagnostic tests for parasites, Verocai said.

Although the researchers found E. multilocularis in more than one-third of local coyotes tested, there is little evidence of the infection spreading to other hosts. One study in Washington, Oregon and Idaho since 2023, five of which were in Washington. Few human cases have been reported in the U.S., and none on the West Coast.

“The reason that it’s so high in coyotes is because they are regularly eating raw rodents, and that is the primary way for them to get infected. Most domestic dogs are not eating the raw livers of wild rodents,” Hentati said.

Before the uptick in the 2010s, there were several reports of E. multilocularis on remote islands in northwestern Alaska. Those cases were caused by a parasite with different origins than the current outbreak. Genetic analysis pins the earlier cases to a tundra variant while these recent cases are driven by a more infectious variant with European origins. The coyotes in this study carried the newer variant, now thought to be the predominant variant in the U.S. and Canada.

Neither Canada nor the U.S. require dogs to undergo deworming upon arrival, which may explain the spread. Previous studies also proposed that E. multilocularis could have come over in red foxes imported for hunting 100 years ago, but no one knows for sure.

“The main takeaway is that Echinococcus multilocularis is here, it’s pretty prevalent in the local coyote population and people should be aware of potential risks,” Hentati said.

Co-authors include , lab manager at UW; , UW doctoral graduate in environmental and forest science; , a UW professor of environmental and forest science; , a UW associate professor of aquatic and fishery science; of the College of William and Mary; Erika Miller of Sound Data Management; of DePaul University; and of UC Berkeley. This study was funded by The National Science Foundation and the �������� Hall Conservation Genetics Fund.

For more information, contact Hentati at yhentati26@gmail.com.

Using preliminary data from the Simonyi Survey Telescope at the NSF–DOE Vera C. Rubin Observatory, scientists have discovered over 11,000 new asteroids in our solar system. The findings were confirmed by the International Astronomical Union’s Minor Planet Center (), and include hundreds of distant worlds beyond Neptune as well as 33 previously unknown near-Earth objects.

The discoveries — Rubin Observatory’s largest asteroid haul yet — were made using data from the observatory’s early optimization surveys and processed with software developed at the ��������’s . The new findings are a powerful preview of the observatory’s transformative impact on solar system science.

“This first large submission after is just the tip of the iceberg and shows that the observatory is ready,” said , a UW professor of astronomy and leader of Rubin’s solar system team, which is located at the UW. “What used to take years or decades to discover, Rubin will unearth in months. We are beginning to deliver on Rubin’s promise to fundamentally reshape our inventory of the solar system and open the door to discoveries we haven’t yet imagined.”

The submission to MPC comprises approximately 1 million observations, taken over the span of a month and a half, of over 11,000 new asteroids and more than 80,000 already known asteroids, including some that had previously been observed but were later “lost” because their orbits were too uncertain to predict their future locations. The new batch adds to roughly 1,500 asteroids previously discovered by Rubin as part of its First Look project.

The newly discovered near-Earth objects, or NEOs, are small asteroids and comets whose closest approach to the sun is less than 1.3 times the distance between Earth and the sun. None of the new NEOs pose a threat to Earth. Once in full operation, Rubin is expected to reveal an additional nearly 90,000 new NEOs, some of which may be potentially hazardous. By enabling early detection and continuous monitoring of these objects, Rubin will be a powerful tool for planetary defense.

The dataset also contains roughly 380 trans-Neptunian objects (TNOs) — icy bodies orbiting beyond Neptune. Two of the newly discovered TNOs — provisionally named and — have been found to be on extremely large and elongated orbits. At their most distant points, these two objects reach roughly 1,000 times farther away from the sun than the Earth is, placing them among the 30 most distant known asteroids.

A total of 12,700 asteroids discovered with Rubin are shown here during the 1.6 years of observation. The discoveries come in three bursts: 73 were discovered during the first early test observations using Rubin’s Commissioning Camera in late 2024; 1,514 were discovered during First Look observations in April and May 2025; and the recent 11,000 asteroids were discovered in Rubin’s early optimization surveys in Summer 2025.

The discoveries were enabled by Rubin Observatory’s unique combination of a large mirror, the world’s most powerful astronomical digital camera, and highly sophisticated, software-driven pipelines developed at the UW that can detect faint, fast-moving objects against a crowded sky. These capabilities will allow Rubin to build the most detailed census of our solar system ever, and the resulting discoveries will help scientists work out the story of the solar system’s history.

“Rubin’s unique observing cadence required a whole new software architecture for asteroid discovery,” said , a UW research scientist of astronomy who, together with UW astronomy graduate student , built the software that detected them. “We built it, and it works. It seems pretty clear this observatory will revolutionize our knowledge of the asteroid belt.”

Particularly striking is the rapid growth of the TNO population. The 380 candidates discovered by Rubin in less than two months adds to the 5,000 discovered over the past three decades. As with less distant asteroids, finding the TNOs depended critically on developing new sophisticated algorithms.

“Searching for a TNO is like searching for a needle in a field of haystacks — out of millions of flickering sources in the sky, teaching a computer to sift through billions of combinations and identify those that are likely to be distant worlds in our solar system required novel algorithmic approaches,” said , a senior astrophysicist at the Harvard & Smithsonian Center for Astrophysics and former director of the Minor Planet Center, who spearheaded the work on the TNO discovery pipeline.

“Objects like these offer a tantalizing probe of the solar system’s outermost reaches, from telling us how the planets moved early on in the solar system’s history, to whether a hitherto undiscovered ninth large planet may still be out there,” said , a research scientist at the Harvard-Smithsonian Center for Astrophysics who, with Holman, developed the algorithms to detect distant solar system objects with Rubin data.

The verification of this large group of discoveries enables the entire global community to access the data, refine orbits and begin analysis immediately. And these 11,000-some asteroids are just the start. Once the decade-long Legacy Survey of Space and Time () begins later this year, scientists expect Rubin to discover this many asteroids every two to three nights during the early years of the survey. This will ultimately triple the number of known asteroids and increase the number of known TNOs by nearly an order of magnitude.

Rubin Observatory is jointly operated by NSF NOIRLab and SLAC.

For more information, contact Jurić at mjuric@uw.edu.��

This story was adapted from a .

Operations of the Vera C. Rubin Observatory are funded by the U.S. National Science Foundation and the U.S. Department of Energy’s Office of Science.

Other team members include , a former DiRAC postdoctoral fellow at the UW, now at the Institute for Astronomy, Geophysics and Atmospheric Sciences of the University of São Paulo; , a UW research software engineer and B612 Asteroid Institute team member who earned his doctorate in astronomy at the UW; , a former UW postdoctoral researcher in astronomy, now at the University of Illinois Urbana-Champagne; and at Princeton University.