Department of Astronomy – UW News /news Wed, 14 Oct 2026 19:35:32 +0000 en-US hourly 1 https://wordpress.org/?v=6.9.10 UW researcher who studies ‘big and weird stars’ named next editor-in-chief of astronomy journals /news/2026/10/14/emily-levesque-profile-astronomy/ Wed, 14 Oct 2026 19:35:32 +0000 /news/?p=93626 A bright illustrated star against a starfield
An artist’s rendering of the red supergiant star Betelgeuse as it ejects stellar dust into space, which led to a peculiar dip in the star’s observed brightness in 2019. UW astronomer Emily Levesque specializes in “big and weird stars� and studied Betelgeuse’s “great dimming.� Photo: NASA

It all started with Halley’s Comet.

was a toddler in 1986, the last time the was visible to the naked eye. One night, her family kept her up late to try and spot it above their home in East Taunton, Massachusetts.

“I was fussy and tired until they pointed up,â€� Levesque recalled, “and then all of a sudden I just went, ‘W³ó´Ç²¹â€™.â€�

Levesque’s career interests followed a trend after that.

“People would ask me what I wanted to be when I grew up, and I would say, ‘Well, I’m going to be a ballerina or an astronomer,’ or ‘I’m going to be a firefighter or an astronomer,’ or ‘a violinist or an astronomer’,â€� she said.

Levesque’s childhood infatuation stuck. Today she is a professor of astronomy at the ÌìÃÀÓ°ÊÓ´«Ã½ who studies “big and weird stars.â€� She’s authored two textbooks on and , as well as general-interest on astronomy. And in 2027, she will become the next editor-in-chief of the American Astronomical Society’s portfolio of academic journals, making her the first woman to serve at the helm of six of astronomy’s busiest and most prestigious research outlets.

“I published my very first research paper in The Astrophysical Journal more than 20 years ago as an undergrad,� Levesque said. “The AAS Journals have played such an enormous role in the history of astronomy and in so many of our careers, and my predecessors have established an incredibly high standard of care and commitment in how the journals are run. I’m excited and honored to become the next steward of that legacy.�

Levesque became interested in stars as a child, and she carried her enthusiasm through to a degree in physics from MIT. Her first research project there brought her to the in Flagstaff, Arizona, where she studied — a star so large that one would engulf Mercury, Venus, Earth, Mars and Jupiter if it were placed where our sun is.

“I got really interested in these huge, unstable stars — they die explosive, spectacular deaths as supernovae, and leave behind mysterious things like black holes,� Levesque said. “We tend to think of stars as just big round balls of gas. But when you look closer, they turn into these brain-bending objects that stretch our ability to comprehend the universe.�

Headshot for Emily Levesque
Levesque Photo: ÌìÃÀÓ°ÊÓ´«Ã½

From MIT, Levesque hopscotched to a doctoral program at the University of Hawaii, a postdoctoral fellowship at the University of Colorado, Boulder and then, in 2015, an appointment at the UW. Along the way, her taste in stars has only gotten stranger: At the UW she studies hypothesized oddities called (TZOs), which are red supergiants with for cores. While in Colorado, Levesque and collaborators . Today, much of her work at the UW is dedicated to finding more possible TZOs and understanding how they might form — though their existence still isn’t a sure thing.

“We could absolutely be wrong,â€� Levesque said. “Other researchers have published papers since our initial discovery arguing that TZOs couldn’t possibly be stable, or that the star we found wasn’t actually a TZO. Still others have published papers saying, ‘We looked closer at your candidate and we think it really is a TZO.’ So it’s a subject of debate, which I think is great. If we made a mistake, I desperately want someone to find it.â€�

Levesque has been involved with the American Astronomical Society Journals for 10 years. She’s currently serving as a science editor, which entails running the journals’ peer review process, matching submissions with reviewers and shepherding drafts through to publication.

“Getting involved with the journals has been a great way to support the astronomy community on a large scale,� Levesque said. “The AAS Journals are such a great resource in our field, so working with them is really impactful. Plus, it helps me keep tabs on the latest science.�

The editor-in-chief role, though, is a much larger proposition.

“It’s a big job,� Levesque said. “It is essentially a full-time position. But I like the idea of getting to devote so much of my time and attention to this.�

When she officially steps into the role next fall, Levesque will navigate a critical and chaotic moment for academic research and publishing. She sees twin challenges ahead for the journals: remaining solvent in the dicey landscape of federal funding, and managing a firehose of paper submissions unleashed with the help of artificial intelligence.

“We’re certainly seeing lots of papers that are auto-generated junk,� Levesque said. “But there’s also a huge uptick in people simply being able to do research faster or to write down their research faster. We’re figuring out how to manage the influx of papers and deciding what constitutes appropriate use of AI.�

Levesque betrays no intimidation about juggling her faculty position with the new leadership role at the journal. She’s letting friends and family be overwhelmed on her behalf.

“When I tell people that I’m moving into this role, there’s sort of this look of like, ‘Oh my gosh, you’re going to be dealing with funding disasters and AI is going to upend everything, isn’t this terrifying?’â€� Levesque laughed. “In this landscape, the AAS Journals are more important than ever. It’s never been easier to generate and share information, but it’s also never been harder to trust information. Publishing is a crucial part of how our field shares trustworthy science, so for me it’s worth the effort.â€�

For more information, contact Levesque at emsque@uw.edu.

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UW faculty, researchers and students earn recognition from the Berkeley Prize, Marconi Society and National Science Foundation /news/2026/09/21/uw-faculty-researchers-and-students-earn-recognition-from-the-berkeley-prize-marconi-society-and-national-science-foundation/ Mon, 21 Sep 2026 17:03:33 +0000 /news/?p=93261

Recent recognition of the ÌìÃÀÓ°ÊÓ´«Ã½ includes a Berkeley prize recognizing research on ancient galaxies, a 2026 Marconi Society Paul Baran Young Scholar Award for a doctoral student, and an NSF CAREER Award supporting research on the brain circuits that drive social behavior.

UW astronomer is part of team that receives Berkeley prize for study of ancient galaxies

, UW postdoctoral scholar in astronomy, is part of a team of astronomers who received the 2027 Lancelot M. Berkeley–New York Community Trust Prize for Meritorious Work in Astronomy.Ìý

Khullar is one of 60 astronomers who make up the UNCOVER team, an international collaboration built to study tens of thousands of galaxies, black holes and star clusters. The Berkeley Prize recognized the UNCOVER team for its work using the to study galaxies behind “Pandora’s Cluster,â€� a massive galaxy cluster. The large mass of this cluster causes it to act as a powerful magnifying glass, bending the light from faraway background galaxies.Ìý

Deep imaging and spectroscopy of this gravitational lens have enabled the UNCOVER project team to identify and characterize distant galaxies from some of the earliest stages of our universe.Ìý

“This team award is a genuine recognition of the incredible work that this new collaboration has conducted, spearheaded by early career astronomers,� Khullar said. “I am fortunate to have played a small part in contributing to studying the first galaxies in the universe which have paused star formation — systems called quiescent galaxies.�

Awarded annually since 2011 by the American Astronomical Society (AAS), the Berkeley prize recognizes research that advances the field of astronomy. The prize includes a monetary award and an invitation to give the closing plenary lecture at the AAS winter meeting in January.

This story was adapted from a press release by AAS.

UW doctoral student receives 2026 Marconi Society Paul Baran Young Scholar AwardÌý

, a doctoral student in the UW Department of Electrical & Computer Engineering, was , which recognizes exceptional early-career researchers advancing the future of information and communications technology.Ìý

A researcher in the Paul G. Allen School of Computer Science & Engineering’s Mobile Intelligence Lab, Itani works with , a UW professor of computer science and engineering, to develop AI-poweredÌý devices that give users greater control over what they hear. The technology could allow someone wearing earbuds or hearing aids to amplify specific voices or sounds they want to focus on while reducing unwanted background noise.Ìý

That ability couldÌýmakeÌý listeningÌýmore customizable, from following a conversation in a crowded restaurant to better distinguishing important sounds in noisy environments. Itani and his collaborators are currently advancing systems designed to enable this kind of real-time “superhumanâ€� hearing on earbuds and hearing aids.Ìý

“I feel like I’ve hit a niche that’s going to be so transformational,â€� Itani said, noting that the technology could eventually reach billions of devices. “It’s going to change the way we hear the world.â€�Ìý

Because of that potential reach, Itani said he feels a responsibility to continue advancing the technology and its ability toÌýimpactÌýpeople’sÌý lives.Ìý

Itani and his collaborators have also launchedÌýHearvanaÌýAI to commercialize their research. He and his fellow honorees will be formally recognized at the Marconi Awards Gala & Institute Forums, held Nov. 4–6 in San Francisco.ÌýÌý

UW assistant professor of psychology and neuroscience receives NSF CAREER Award to study brain circuits driving social behaviorsÌý

Sama Ahmed, UW assistant professor of psychology and neuroscience, received a 2026 National Science Foundation CAREER Award of more than $1.4 million.Ìý

The NSF CAREER Award is the agency’s most prestigious honor for early-career faculty, recognizing those with the potential to become academic leaders in both research and education.Ìý

With the award, Ahmed and his team will study the brain circuits behind “proceptivity” — the active behaviors animals use to pursue and engage potential mates. Using fruit flies, the most complex organism with a fully mapped brain and a species with well-studied social behaviors, the researchers will use advanced genetic and imaging tools in the Ahmed Lab to watch how different neural networks in the brain talk to each other in real time.Ìý

Instead of looking at how the brain does one thing at a time, Ahmed’s team tracks how the nervous system switches between responding to external social cues and actively generating social behaviors. Understanding how the brain juggles these competing choices helps researchers understand how more complex brains — including our own — prioritize information and decide when to act.Ìý

“I’ve always wanted to understand how our brains generate and respond to social signals,â€� Ahmed said, adding that the CAREER Award opens a new way for his lab to investigate that question.Ìý

The project will also provide research training opportunities for high school, undergraduate and graduate students and support the development of open-source computational tools and STEM modules focused on coding and automated behavioral tracking. The award will also allow Ahmed to create a new Course-based Undergraduate Research Experience (CURE), where students will use technologies such asÌýconnectomicsÌýand optogenetics to investigate questions that, as Ahmed put it, “nobody has answered yet.â€�Ìý

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UW researchers lead and support new ‘AI-for-Science’ Genesis Mission awards /news/2026/09/08/uw-researchers-lead-and-support-new-ai-for-science-genesis-mission-awards/ Tue, 08 Sep 2026 17:00:02 +0000 /news/?p=93074 image of bronze "W" framed by blooming trees
UW researchers are leading and collaborating on a number of research projects as part of Phase 1 in the U.S. Department of Energy Genesis Mission. Photo: Dennis Wise/ÌìÃÀÓ°ÊÓ´«Ã½

ÌìÃÀÓ°ÊÓ´«Ã½ researchers are leading and collaborating on four research projects as part of Phase 1 in the U.S. Department of Energy (DOE) , a national initiative to build an AI-for-science ecosystem which accelerates breakthroughs in energy, discovery science and national security.Ìý

The DOE awarded a total of 278 Genesis Mission awards for projects that involve more than 300 participating institutions, including DOE and National Nuclear Security Administration national laboratories, universities and companies. As part of the Genesis Mission, awardees will have access to the Genesis Mission Platform, which includes AI frameworks, advanced AI models from industry partners, and high-performance computing resources across DOE’s National Laboratories and partner facilities.Ìý

“The Genesis Mission represents the kind of bold, collaborative approach needed to accelerate the complex scientific and technological breakthroughs required in our rapidly changing world,” said UW Vice Provost for Research . “Its emphasis on bringing together diverse expertise and cutting-edge technology with strategic partnerships highlights the important role universities play in driving innovation for the nation.”Ìý

The UW-supported Genesis projects span disciplines including advanced sensing technologies, protein design for microelectronic applications, and astronomy data infrastructure, demonstrating the broad potential of AI to accelerate scientific discovery.Ìý

, assistant professor of electrical and computer engineering, received a Genesis award to develop neuromorphic terahertz imaging technology for next-generation augmented reality systems. Ìý

“Neuromorphic terahertz imagers, or brain-inspired imaging in the terahertz band, give us superhuman vision to see through optically obscured media in real time by combining sensing and computation in a single piece of hardware. The Genesis Mission award supports our research in developing the hardware for the neuromorphic terahertz imager, as well as creating a digital twin of the entire system to train imaging models before implementing them on the actual hardware. This is an important step for future terahertz imaging systems on augmented reality hardware,” Naghavi said. Ìý

Building on research conducted in UW’s , the project brings together collaborators at Texas A&M University, the University of Utah, ChipNexus and NVIDIA to integrate sensing and computation directly within imaging hardware. By reducing the amount of data that must be transferred between sensors and processors, the technology could enable lightweight, low-cost augmented reality headsets capable of seeing through visually obscured materials in real time while operating with far lower power consumption than conventional systems.ÌýÌý

, director of the , and his colleagues are contributing to two Phase I Genesis Mission projects that apply advances in protein design and artificial intelligence to challenges beyond traditional biomedical applications.Ìý

One project, BIND (Biophysics-Informed Learning of Coordination for Metalloprotein Design), led by the Lawrence Livermore National Laboratory, seeks to develop an AI framework for designing selective metal-binding proteins. The project leverages quantum chemistry, structural biology, machine learning and high-throughput experimentation to advance the computational design strategies of next-generation rare earth element binders. ÌýThese advancements will catalyze change in critical mineral recovery, radionuclide management and environmental monitoring, while advancing DOE priorities in predictive biosystems design. Ìý

The second project, led by Pacific Northwest National Laboratory, will develop an AI-guided loop for the design, fabrication and evaluation of microelectronic devices. The team will leverage proteins designed to assemble on van der Waals substrates to modulate their properties and organize charge carriers within the synthesized hybrid materials, integrating deep-learning protein models with AI-guided material synthesis and characterization, device fabrication and measurements, and circuit-level performance evaluation to create an iterative design process that improves molecules, materials, and device design. Ìý

Both IPD projects demonstrate how UW-developed protein design technologies are expanding into new areas of chemistry, materials science, and advanced manufacturing. “The Genesis Mission award provides necessary support to develop data that will vastly improve our models, an essential next step in delivering advances for key global challenges,â€� Baker said.ÌýÌý

, director of the and founding director of the and , a researcher at DiRAC, are partnering with researchers at Carnegie Mellon University to help develop infrastructure that will make it easier for astronomers to combine and analyze data from a wide range of observatories and scientific instruments. Ìý

Their project will expand data formats and analysis platforms to support images, spectra, data cubes and other forms of astronomical data while enabling seamless access to information distributed across cloud and high-performance computing systems. The goal is to remove technical barriers that often slow scientific discovery and make large, multimodal datasets more accessible for AI research. Ìý

“We want the plumbing to be boring so the astronomy can be spectacular,” Caplar said.Ìý

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New galactic simulations narrow the hunt for dark matter /news/2026/08/27/stellar-streams-dark-matter-simulation/ Thu, 27 Aug 2026 16:03:49 +0000 /news/?p=92927 Bright multicolored lines wrap around a rendering of the Milky Way galaxy.
Most galaxies are likely surrounded by long filaments of orbiting stars known as stellar streams. In a new study from the ÌìÃÀÓ°ÊÓ´«Ã½, astronomers simulated stellar streams — pictured here as multicolored streaks — as they orbited virtual host galaxies to test a leading theory about how dark matter might influence the streams’ shape. The results could help researchers separate true evidence of dark matter from false positives. Credit: Visualization by Arpit Arora and Adrian Price-Whelan. Milky Way image credit: Stefan Payne-Wardenaar.

Most of the stars in sit neatly on a flat plane. But the space around our galaxy is much more chaotic. Rogue bands of stars called “� orbit the Milky Way much like planets in our solar system orbit the sun.

Astronomers have long been fascinated by the possibility that stellar streams could indirectly reveal the presence of , that mysterious theorized substance that doesn’t interact with light or normal matter — except via gravity. However, a new ÌìÃÀÓ°ÊÓ´«Ã½ study casts doubt on a leading theory linking dark matter and stellar streams, and raises new questions about both galactic phenomena.

“Dark matter makes up most of the mass in the universe and forms the scaffolding that galaxies grow on, but we still don’t know what it is,â€� said co-author , a UW assistant professor of astronomy. “The Milky Way is one of the best laboratories we have for figuring that out, and stellar streams are one of the sharpest tools inside it.â€�

in The Astrophysical Journal.

Take a stellar stream tour

Use the visualizer below to explore some of the simulated stellar streams from the study. Click and drag the image to rotate the view. Scroll to zoom. Click or tap the gear icon to access variables like number of streams, rotation rate and more. Use the icon in the lower lefthand corner to go fullscreen.

A stellar stream forms when a group of stars crashes into a galaxy and becomes ensnared by its gravity. As the stars orbit the galaxy, its gravity stretches the cluster into a . Most galaxies host stellar streams, though the Milky Way’s are the most visible to astronomers. 

In our galaxy, most stellar streams we can see are irregular — gaps and kinks interrupt an otherwise uniform smear of stars. Many astronomers believe that those irregularities could signal the gravitational tug from small clumps of dark matter, called subhalos. If there are indeed subhalos sprinkled throughout the galaxy, studying the aberrations in stellar streams could teach us about the composition of dark matter.

The new study was an effort to understand the role that the host galaxy — rather than the dark matter clumps within it — plays in shaping stellar streams. Astronomers simulated four Milky Way-sized galaxies without any dark matter clumps, then peppered them with roughly 15,000 stellar streams. After five billion simulated years, the team observed irregularities in nearly every stellar stream.

“In our simulations, the host galaxies alone caused the same kinds of irregularities that we observe in real stellar streams,� said lead author , a UW postdoctoral scholar in astronomy. “Now that we can predict what the host galaxy does on its own, we can start isolating the part that dark matter is responsible for.�

The cause of the irregularities was the structure of the galaxies themselves. In each simulated galaxy, stars were spread somewhat unevenly across the disc, creating areas of greater and lesser density to mimic the composition of a real galaxy like ours. As the simulated streams of stars passed through denser regions of space, they were bent and torn by the irregular gravitational landscape.

Arora expected the host galaxies to impart some irregularities on the streams, but the sheer number caught him off guard.

“We found that almost all of the streams had some sort of structural variation,â€� Arora said. “So this idea that streams are naturally thin and smooth wasn’t really necessarily true.â€�

A grid of orange wiggly lines set against a plain black backdrop
A selection of virtual stellar streams shows the variety of bends, wiggles, kinks and gaps that the simulations produced. Out of roughly 15,000 streams, only 70 were featureless. Credit: Arora et. al/The Astrophysical Journal

The simulation generated wiggles, kinks, spurs, branches, gaps and clumps; some streams were totally torn apart by the gravitational froth of their host galaxies. Streams orbiting closer to the galactic core were thrown into dense clumpy regions of space more often, where they acquired more irregularities. Out of the 15,000 streams spread across the four host galaxies, only 70 remained perfectly smooth after five billion years. 

The results might seem disheartening, but the UW team believes they chart a clear and exciting course for the future of dark matter research. Arora wants to include dark matter clumps in the next simulation to see whether they produce stellar stream irregularities that are distinct from those caused by the host galaxy alone. 

There may also be opportunities to check simulations against new observations: the is , which will help astronomers build a taxonomy of stream features and — hopefully — discover fingerprints of dark matter.

“Sadly there’s no magic wand to reveal the structure of dark matter,â€� said , a research assistant professor of astronomy at the UW. “Streams are complex systems, but they’re still the most interesting way to study the dark matter close to home.â€� 

Co-authors from the UW astronomy department include , a postdoctoral fellow; , an undergraduate student; and and , graduate students.

A complete list of co-authors is .

This research was funded by the Gordon and Betty Moore Foundation.

For more information, contact Arora at arora125@uw.edu.

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NASA’s Hubble shows star formation in Andromeda galaxy winding down /news/2026/08/03/nasa-hubble-andromeda-galaxy-star-formation/ Mon, 03 Aug 2026 18:43:44 +0000 /news/?p=92703 A photo of a galaxy with two inset boxes highlighting a red region and a blue region
NASA’s Hubble Space Telescope has provided a detailed view of millions of stars in the Andromeda galaxy. Regions that have experienced recent star formation (1) appear significantly bluer than regions with less recent star formation (2). Photo: NASA, ESA, Benjamin Williams (UW), Zhuo Chen (UW), L. Clifton Johnson (Northwestern); Image Processing: Joseph DePasquale (STScI)

A new study using data from NASA’s found that star formation in the nearby Andromeda galaxy has undergone a 500-million-year decline, with an even steeper drop in the last 40 million years. Andromeda, a spiral galaxy comparable in size to our Milky Way, is close enough to be seen with the unaided eye from areas with dark skies. Located about 2.5 million light-years from Earth, practically our cosmic backyard, Andromeda is close enough for astronomers to examine its stellar populations in detail and learn about the past of galaxies like our own.

July 27 in .

To reach this conclusion, the researchers combined data from two Hubble surveys: the and the . Together, these two surveys mapped two-thirds of the disk of Andromeda in ultra-sharp detail. In total, the team measured about 200 million individual stars across the galaxy, giving them a detailed picture of Andromeda’s past activity.

“We need to measure the individual stars because they are the fossil record of the galaxy’s formation,â€� said , a research professor of astronomy at the ÌìÃÀÓ°ÊÓ´«Ã½ and a co-author on the study. “Hubble is the only telescope that can give you high enough spatial resolution in the blue part of the spectrum over a large enough area to be able to do that in Andromeda.â€�

Massive stars are bluer and short-lived, while less massive stars are redder and longer-lived. As a result, areas that have experienced recent star formation tend to have a larger fraction of blue stars, while areas with less recent star formation typically have a redder population. The team divided the Andromeda images into thousands of squares, spanning 300 light-years on each side, and determined the history of star formation within each parcel to gain a comprehensive view of the galaxy’s past.

Previous research showed the Andromeda galaxy experienced a dramatic burst of star formation about 2 billion years ago, likely due to a past interaction or merger with another galaxy. Since that time, star formation has been steadily declining.

This movie, created from an analysis of data from NASA’s Hubble Space Telescope, demonstrates how the rate of star formation in the Andromeda galaxy has declined over the past 500 million years. Brighter colors indicate where star formation was highest during a given time. Credit: Visualization: Tobin Wainer (UW); Image Processing: Joseph DePasquale (STScI); Video: NASA, ESA, STScI, Gregory Bacon (STScI)

Astronomers measure the rate of star formation in terms of the mass, or amount of gas and dust, converted into stars per year. The researchers calculated that, 500 million years ago, Andromeda formed stars at a rate of about one solar mass per year. However, the formation rate dropped to about half that by 40 million years ago. The current rate has plummeted even farther, to about one-fifth the mass of our Sun per year.

The team also examined whether that decline was consistent across the galaxy or concentrated in certain areas. They found that much of the recent star formation has occurred in a star-forming ring located about 32,000 light-years from the galaxy’s center. As a result, much of the decline they measure is driven by decreasing activity within that ring.

The decline is likely to be a natural winding down from its previous, more active state.

“It’s just like after running a marathon, sometimes you’ve got to take a bit of a breather,â€� said lead author , a UW graduate student in astronomy.Ìý

The team also investigated whether there was any connection between the decrease of activity in Andromeda and its proximity to the satellite galaxy Messier 32, or M32. The M32 galaxy is separated from Andromeda by about 16,000 light-years in the plane of the sky; however, its 3D location in space is uncertain. As a result, astronomers are unsure if or when it might have interacted with Andromeda in the past.

“One of the major motivations for this program was to probe potential interactions between M32 and Andromeda’s disk,� said co-author , a UW postdoctoral scholar in astronomy.

Survey data from the Panchromatic Hubble Andromeda Southern Treasury allowed the team to study the history of star formation in Andromeda near M32. They found that this area showed signs of decreased star formation compared with other regions. The timing of this decrease, which this study finds began roughly 60 million years ago, could help constrain when the M32 galaxy interacted with Andromeda’s disk.

“We can’t explicitly say that we are seeing a decrease in star formation because of M32. But it’s right there, and it’s definitely the most likely suspect,� Wainer said.

The team plans to continue analyzing the Hubble data and combine it with data from ground-based observatories to gain additional insights into the history of Andromeda.

“There’s a strong scientific value to this archival data,â€� said co-author , a professor of astronomy and astrophysics at University of California Santa Cruz. “Andromeda is important because it’s a neighbor that is close enough that we can see it in great detail while also getting a global perspective.â€�Ìý

An even greater global perspective is likely to come from NASA’s Nancy Grace Roman Space Telescope after it launches as early as Sunday, Aug. 30. Roman’s gigantic field of view can cover at least 100 times as much area as Hubble at near-infrared wavelengths in a single observation. A newly approved will image the entirety of Andromeda’s disk and areas of its surrounding halo, allowing astronomers to measure hundreds of millions of stars and enabling groundbreaking new science.

Hubble is a project of international cooperation between NASA and the European Space Agency.Ìý

UW co-authors include , professor emerita of astronomy and , and , former UW graduate students in astronomy.

A complete list of co-authors is .

This research was funded by NASA.

For more information, contact Wainer at tobinw@uw.edu.

This story was adapted from a press release by .

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UW researchers join national effort to streamline AI-driven cosmology /news/2026/07/22/ai-cosmology-genesis-mission/ Wed, 22 Jul 2026 18:17:53 +0000 /news/?p=92624 A dense view of many stars and galaxies
A view of the cosmos captured by the Simonyi Survey Telescope at the NSF-DOE Vera C. Rubin Observatory. A new collaboration between the ÌìÃÀÓ°ÊÓ´«Ã½ and Carnegie Mellon University will create shared tools that allow researchers to work across massive, distributed datasets — such as those created by the Rubin Observatory — to accelerate discoveries about the universe. Photo: NSF–DOE Vera C. Rubin Observatory

Researchers at the ÌìÃÀÓ°ÊÓ´«Ã½ and partners at Carnegie Mellon University are collaborating with the U.S. Department of Energy’s on a new project to help scientists use artificial intelligence to better understand the universe.

Modern astronomy is producing more data than ever before. Powerful telescopes — like the — and other instruments around the world are collecting detailed information about billions of stars, galaxies and other cosmic objects. These observations help researchers investigate some of the biggest mysteries in science, including the nature of dark matter and dark energy, how the universe evolved over time and what it is made of.

But there is a challenge: Much of the data from those projects is stored in different formats, housed at different institutions and difficult to combine. As a result, scientists often spend significant time preparing data before they can begin analyzing it.

“The scientific opportunities and the data analysis challenges are incredible,� said , head of physics at Carnegie Mellon University.

The new effort, led by Mandelbaum and funded by the U.S. Department of Energy’s , will create a shared data service to allow researchers to seamlessly access and combine information from multiple astronomy experiments. Rather than moving massive datasets from one location to another, the system will allow the data to remain where it is stored while making it available through a central platform.

“A new generation of telescopes and surveys will each change the way we understand our universe,� said co-investigator , a UW professor of astronomy and director of the eScience Institute. “But it is when we bring these data together to look at the universe from a unified perspective that these discoveries will be truly transformative.�

The data infrastructure developed as part of this project will be available to the astronomical community at the SLAC-hosted Rubin Observatory’s U.S. Data Facility and via the American Science Cloud, which integrates the nation’s most advanced high-performance computing systems, scientific facilities, data resources and production capabilities into a single, coordinated AI-driven system. The project extends the UW’s investments in Rubin Observatory and the UW , which are supported by Charles and Lisa Simonyi and led by and .Ìý

The infrastructure also will support a growing area of AI known as foundation models. These AI systems are trained on large and diverse datasets, enabling them to recognize patterns and connections that might otherwise go unnoticed.

In astronomy, foundation models could help researchers analyze many different types of observations at once, including images, measurements of light from distant objects and records of how those objects change over time. By bringing these data sources together, scientists hope to uncover new insights about the universe more quickly and efficiently.

Ultimately, the team hopes to transform the vast collections of astronomical data being gathered today into a long-lasting scientific resource, helping researchers answer some of humanity’s most fundamental questions about the origin, evolution and makeup of the universe.

Other UW co-investigators include , a research scientist and engineer in astronomy. Other co-investigators include , director of engineering for the LINCC project and , senior staff scientist at SLAC and at Stanford’s/SLAC’s Kavli Institute for Particle Astrophysics and Cosmology.

Additional modeling will be provided by Francois Lanusse of the French National Centre for Scientific Research. Their work is an extension of the Schmidt Sciences-supported LINCC Frameworks program, a partnership led jointly by CMU and the UW.

This story was adapted from a press release by .

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ArtSci Roundup: Summer 2026 /news/2026/07/08/artsci-roundup-summer-of-2026/ Wed, 08 Jul 2026 19:36:20 +0000 /news/?p=92308 ArtSci Roundup title and illustration, image

Come curious. Leave inspired.

Wherever you are, the ÌìÃÀÓ°ÊÓ´«Ã½ offers opportunities to learn and connect with the ideas, people, and research shaping our world. This summer, visit campus for the latest exhibitions at the Henry Art Gallery and Burke Museum of Natural History and Culture, or join us from anywhere through recorded lectures, podcasts, virtual experiences, and more. As a public university, we’re proud to share the knowledge, creativity, and discoveries of the UW with communities near and far.

.


If You’re in Seattle:

SUMMER EVENTS:

Wild Seattle book coverJuly 7 | (Arboratum Foundation)
Meet Seattle-based author, journalist, and photographer Roddy Scheer and learn about his new book, Wild Seattle: Explore the Amazing Nature in and Around the Emerald City.

July 11 | (Harry Bridges Center for Labor Studies)
Harry Bridges Center for Labor Studies at the ÌìÃÀÓ°ÊÓ´«Ã½ for a day packed with labor history, organizing strategies, and labor research with the Seattle labor community. How are racism and capitalism related, and how have workers confronted them, past and present? Come ready to learn, discuss, and organize!

Assembly Art Fair Seattle 2026 posterJuly 22 – 26 | (School of Art + Art History + Design)
Assembly is a new invitational contemporary art fair organized by a cohort of Seattle’s leading galleries. Founding members include Traver Gallery, led by School of Art + Art History + Design alum Sarah Traver (BFA ’02), and Greg Kucera Gallery. The fair’s inaugural edition will take place at the West Canal Yards. It will bring together galleries from across the Western US with their curatorial programs, artists, and collectors.

July 23 – 26 | Ìý(ArtsUW)
Seattle Art Fair, a one-of-a-kind showcase for the vibrant arts community of the Pacific Northwest, and a leading destination for the best in modern and contemporary art, returns for its tenth edition. The Fair brings together the region’s strong collector base, the Pacific Northwest’s top museums and institutions, and an array of innovative public programming.

Through July 24 – Book Club | The Frozen River by Ariel Lawhon (UW Alumni Association)
Readers’ Choice! Bundle up for an historical mystery set in 18th-century Maine. The body of a local man is found in the frozen Kennebeck River. Martha Ballard, the local midwife, suspects that this death is not an accident — and her detailed diaries of local life are full of clues. Will she weather the scandals unleashed by her pursuit of the truth? Inspired by historic events!

July 25 | (Burke Museum of Natural History and Culture)
Walk around the ÌìÃÀÓ°ÊÓ´«Ã½ campus with Dr. Susan Pavel to learn more about native plants and how you can use them to dye textiles. In this workshop, learn about the native plants around the Burke Museum and how they can be used. Hear about the dyeing process and see samples of native plant dyes. Leave this workshop with the information to do your own natural dyeing at home! Takeaways include: a sample card of a natural dye from a native plant.

August 6 |Ìý(Burke Museum of Natural History and Culture)
Admission to the Burke Museum is FREE, and the museum is open until 8 p.m. on the first Thursday of every month. Get closer to the daily work happening in the Burke Museum’s visible collections storage, labs, and workrooms during Free First Thursday.

August 27 | (Henry Art Gallery)
Celebrate the opening of new exhibitions featuring newly acquired prints by Helen Frankenthaler, collection objects that explore the politics of the everyday, a solo exhibition by artist Joiri Minaya, and the unveiling of a new mural project! Plus music and drinks!

 

SEPTEMBER EVENTS:

Defending Animals, Disappointing People book coverSeptember 14 | (Philosophy)
Drawing on care ethics and relational philosophy, Karen S. Emmerman develops relational vegan ecofeminism, a framework that takes animals’ moral standing seriously while also acknowledging the emotional, cultural, and familial stakes woven into human traditions. Rather than treating veganism as a simple matter of ethical prioritization, Emmerman shows that refusing a grandmother’s lovingly prepared chicken soup, or rejecting a family hunting tradition, carries profound relational weight. These moments produce “moral remaindersâ€� of lingering hurt, regret, or estrangement that persists even when we make the best ethical choice. Emmerman’s book is a ground-breaking exploration of what happens when caring deeply about animals places us in conflict with the people we love. She’ll be joined in conversation by Amy Reed-Sandoval.ÌýFree.

SIn the Range of Fire & Ice book covereptember 16 | (Burke Museum of Natural History and Culture)
In this event, David B. Williams will be in conversation with local journalist Mary Ann Gwinn, about his new book. Blending human and natural history into a vivid portrait of one of North America’s most dynamic landscapes, In the Range of Fire and Ice is a lively, groundbreaking exploration of Washington’s Cascade Range. Drawing on conversations with anthropologists, park rangers, ecologists, and climate scientists, as well as firsthand experience, award-winning author David B. Williams brings readers into the mountains to uncover stories etched in the landscape over millennia.

Image of Just Hear Me Out bookcover

September 17 | (Philosophy)
UW Prof. Colin Marshall is joined by UW Assoc. Prof. José Jorge Mendoza for a lively conversation about Marshall’s new book, Just Hear Me Out. In Just Hear Me Out, Marshall describes a persuasive method that is both effective and ethical. Rather than share a flurry of tips on how to win friends and influence people, Marshall invites us to take up persuasion as fundamentally civil work, good for both our conscience and our communities. Real-world persuaders such as Jane Addams, Daryl Davis, and Fred Rogers show us an ethical route, he argues, to changing hearts through patience, respect, and compassion. Hosted at the University Bookstore. Free.

September 24 | (Burke Museum of Natural History and Culture)
Samuel Elwitt (1834-1919) was a prolific and highly accomplished Tsimshian carver from the Kitselas First Nation. Partially paralyzed from an early age, Elwitt worked as a full-time artist and relied on carving and painting as his primary source of income for his entire life. Despite a multitude of Elwitt’s spoons, model poles, bowls, and headdresses being present in some of the world’s most notable museums, including the British Museum, American Museum of Natural History, Canadian Museum of History, and the Museum of Anthropology at UBC, most Northwest Coast scholars have never heard of this pivotal artist. This presentation by Vancouver-based museum anthropologist and writer Christopher W. Smith retraces his efforts over the last 18 years to untangle the historic intersectional discrimination and inconsistent museum cataloguing practices that led to this important artist being left out of the Northwest Coast art historical canon. In his presentation, Smith will share key biographical details on Elwitt, historic photos, notable works, and the defining features of Elwitt’s unique carving and painting styles with the audience. Smith will also discuss the important roles that formal attribution, archival research, and online museum databases have played in the return of this information back to Elwitt’s home community and descendants. Free.

Picture of artist's work of post-it notes

September 24 | (Henry Art Gallery)
Every night for almost two decades, artist Clare Johnson has drawn and written on a post-it to save a small piece of each ending day. Currently including over 6,500 sticky notes and growing nightly, this sprawling yet deeply intimate work honors what normal communication can’t—all the separate times held within ourselves, endlessly overlapping, collapsing, and refocusing. As part of Art + Culture Week and in conjunction with the exhibition Day-to-Day: Rhythm, Routine, Resistance, join Johnson at the Henry for a talk and hands-on activity exploring personal histories and practices of everyday making. Free.

September 25 | (Burke Museum of Natural History and Culture)
Join in for an introduction to a moving meditation called Qi Gong. Participants will learn a practice called T’ai Chi Chih, which is a series of 19 movements and one closing posture. Benefits of Qi Gong include improved balance, increased energy, and greater mental clarity. Free.

September 30 | (Art + Art History + Design)
Celebrate the 2026 MFA Show at the Jacob Lawrence Gallery. The exhibition runs from September 30 through November 7. Free.

Image of Gyetk book coverSeptember 30 | (Burke Museum of Natural History and Culture)
Authors Spencer Greening and Rachel Greening discuss their new book, Gyetk: Coastal Fusion and Ancestral Knowledge from a Ts’msyen Kitchen.ÌýGyetk (pronounced gy-e-tk and meaning “to feed the peopleâ€�) immerses readers into the rich food traditions, knowledge, and relationships that have sustained the Ts’msyen (Tsimshian) people for millennia along the Pacific Northwest Coast. Drawing from the authors’ lived experiences practicing a land-based lifestyle, as well as their backgrounds in Indigenous food sovereignty, health and well-being, and cultural research, Gyetk weaves together modern culinary fusion, traditional knowledge, and scholarly insight. Through 60 beautifully photographed recipes, the book follows the Ts’msyen seasonal round, weaving together ancestral foodways, traditional ecological knowledge, dietetic perspectives, and thoughtful harvesting practices — inviting readers to feast in relationship with the natural world.

(Biology)
Wednesdays, noon to 4 pm / 2nd and 4th Saturdays, 10 am – 2 pm
For nearly 70 years, the Biology Greenhouse at the ÌìÃÀÓ°ÊÓ´«Ã½ has played a vital role in research and teaching. Whether focusing on plant-pollinator interactions, paleoclimatology, or other biological questions, the teaching collection has enhanced and inspired UW biological research. Visit the 4 Collection rooms and browse through an amazing diversity of plant species from around the world. Free.

 

EXHIBITIONS:

Opening July 5 | Ìý(Henry Art Gallery)

Art piece by Helen Frankenthaler
Helen Frankenthaler
Ramblas, 1987-88, Ed. 11/75
Six color lithograph, drypoint, and etching
© 2024 Helen Frankenthaler Foundation, Inc. / Artists Rights Society (ARS), New York / Ediciones Polígrafa, S.A., Barcelona

By the age of thirty-two, Helen Frankenthaler (1928—2011) had established herself in a white male-dominated art world as one of the leading American Abstract Expressionist painters of the twentieth century. Her distinctive “soak-stain� technique—applying thinned paint onto unprimed canvases on the floor to produce watercolor-like effects—introduced chance as an integral part of her artistic process. Printmaking, a technical process involving chemistry, collaboration, and repetition, might appear at odds with the spontaneity and physicality of her painting.

Opening July 11 |
(Henry Art Gallery)
This exhibition brings together contemporary artworks across media that explore the poetics and politics of everyday life. Using the day-to-day as both material and subject, these works explore how the ordinary and seemingly incidental can become a powerful source for artistic inquiry, critical reflection, and imagination.

Opening July 18 | (Henry Art Gallery)
Richard Learoyd’s (U.K., b. 1966)Ìýlarge-scale photograph of a dead grey reef shark in the Henry’s permanent collection. This photograph draws from lineages of scientific photography and still life across media, resulting in a picture that surfaces entanglements between traditions of imaging and practices of extraction from land, people, and other living creatures. Reflections from members of the UW community across Art History, Anthropology, and Marine Biology will examine these intersecting histories and contexts.

Art by joiri minaya
Joiri Minaya (U.S., b. 1990). Container #7, 2020. Archival pigment print. Courtesy of the artist. Photo: Joiri Minaya.

Opening July 25 | (Henry Art Gallery)
Joiri Minaya (b.1990, New York City; raised in the Dominican Republic) is a multidisciplinary artist who examines the Tropics as a constructed place and identity. As both performer and saboteur, Minaya challenges misrepresentations that reduce tropical geographies and their inhabitants to imagined fantasies of the colonial imagination. In her work, she reclaims Afro-Indigenous narratives of resistance, ancestral knowledges, and regenerative practices—especially those rooted in plant and botanical traditions.

Through August 30 | (Burke Museum of Natural History and Culture)
Journey through the seasonal cycle of weaving, from gathering materials and spinning wool to dyeing with natural ingredients and weaving intricate designs. Along the way, learn firsthand from weavers and gain insight into the deep cultural and scientific knowledge embedded in every strand. Related Article by the Seattle Times:

As you enter the exhibit, you’ll see baskets, tumplines, and raw materials — all part of the first phase of the weaving process: gathering. Ancestral weavings — some on loan and returning to Coast Salish territory for the first time in a century — are displayed alongside contemporary creations by the co-curators.

exhibition photo, image
Eric-Paul Riege: ojo|-|oÌ�lÇ«Ì� [Installation view, Henry Art Gallery, ÌìÃÀÓ°ÊÓ´«Ã½, Seattle. 2026]. Photo: Jueqian Fang.

(Henry Art Gallery)
ojo|-|o�lǫ� (pronounced oh-ho hol-ohn) is an exhibition of recent and newly commissioned work by Diné artist Eric-Paul Riege (b. 1994, Na’nízhoozhí [Gallup, New Mexico]) that includes sculpture, textile, collage, and video, activated by moments of performance. Across this work, Riege combines customary Diné practices of weaving, silversmithing, and beading with contemporary cultural forms, exploring Diné cosmology, the history of Euro-American trading posts in and adjacent to the Navajo Nation, and the notion of “authenticity� as a value marker of Indigenous art and craft.

ART AROUND SEATTLE:

Volunteer Park: (Henry Art Gallery)
The title, Soft Services, is a phrase drawn from the artist’s research and interviews with members of the activist community, in reference to the care efforts made during the height of the AIDS crisis. At the time, the rare opportunity arose to use the Ryan White (CARE Act) monies towards “soft services”—aspects of support deemed assistive but not strictly necessary and as such not covered by traditional healthcare (massage, meal trains, dog walking, etc.) Through this installation, Bass explores the notion of what true care means, what we define as essential versus optional, and who has access to it, questions of heightened importance at this moment of crisis and recovery.

Detailed views of ‘A walk in the neighborhood,’ a new public art commission installed at the Judkins Park light rail station.
Photo courtesy Sound Transit

Judkins Park Sound Transit: Ìý(School of Art + Art History + Design)
“A Walk in the Neighborhood,� a public art installation by Barbara Earl Thomas, ’73, ’77, is the culmination of 12 years of creative development. It features illustrated glass panels that serve as dividers and windbreaks on the terminal platform. The imagery features people and elements from the neighborhood rendered in Thomas’s cut-paper style.

Through August 8 | ARTS at King Street Station: Ìý(School of Art + Art History + Design)
Vivian Cho is a visual designer and animator based in Seattle whose work includes themes of identity, nature, and digital nostalgia. Their practice is driven by curiosity and a love for experimentation, often exploring ways to synthesize 2D and 3D digital art with analog techniques. A recent graduate of the ÌìÃÀÓ°ÊÓ´«Ã½â€™s Visual Communication Design program, Vivian has previously worked as a motion design intern at Netflix and a visual designer at the Jacob Lawrence Gallery. Currently, they are a staff designer at ARCADE NW Publishing, while also continuing to develop their independent practice and personal design and animation projects. Related article by ÌìÃÀÓ°ÊÓ´«Ã½ Magazine: .

Engage with the ÌìÃÀÓ°ÊÓ´«Ã½ from Anywhere:

SUMMER READS:

Ìý(Department of English)
Discover the latest books and creative achievements from the Department of English faculty.

(Department of English)
From captivating novels and memoirs to poetry, scholarship, and more, this collection showcases the breadth of alumni publications.

PODCASTS:

(Communication)
Lost Credits is a podcast that emerged from a single question: what happened to all of the Black girls that used to occupy our screens? Each episode invites listeners into the quest of two friends to find answers. Hosts Dr. Timeka Tounsel (UW Communication associate professor) and Dr. Ashleigh Greene Wade (Digital Studies, University of Virginia) draw on their expertise as Black feminist media scholars to offer fascinating insights about popular culture and the inner workings of Hollywood. Together, they examine Black girls’ representation in late-twentieth-century and new-millennium entertainment media. With equal doses of fan criticism and educational content, Lost Credits is designed for Black culture enthusiasts as well as students and teachers.

(School of Art + Art History + Design)
UW Professor Karen Cheng joins host and Design alum Jason Tselentis (MFA 2004), Head of Design at Winthrop University, to discuss Working Girl (1988). They discuss the cinematography, Harrison Ford’s character, and other movies that would pair well with Working Girl for a potential double feature.

"Ways of Knowing" podcast image
“Ways of Knowing”

Ways of Knowing, Season 2 (College of Arts & Sciences)
Faculty in the College of Arts & Sciences are facilitating critical conversations in the classroom and the sound booth! The second season of “Ways of Knowing,� a podcast collaboration with The World According to Sound, spotlights eight Arts & Sciences faculty members whose research shapes our knowledge of the world in real time—from digital humanities to mathematics to AI.

(Astronomy)
Researchers at the Large Hadron Collider in Switzerland have announced that they discovered a new subatomic particle. Roughly four times more massive than a standard proton, this short-lived piece of matter called Ξcc�(Xi-cc-plus) is like an extra-heavy proton, researchers say. Physicist Hassan Jawahery joins Host Flora Lichtman to unpack how the particle was found, and what its discovery means for theoretical physics. Then, astronomer Eric Bellm describes a new alert system that could flag potentially significant changes in the southern night sky in real time. On its first night of testing at the Rubin Observatory in Chile, the system fired off 800,000 alerts.

Ìý(Jackson School of International Studies)
Launched in 2021 with UW Professor Daniel Bessner and writer Derek Davison, “American Prestige,� the winner of the 2025 Signal Awards “silver� medal, offers an in-depth analysis of U.S. foreign policy and international affairs, and has featured guests such as actor Morgan Spector and HuffPost senior diplomatic correspondent Akbar Shahid Ahmed.

(Biology)
This is a podcast centered around the humans who study the myriad biological processes that shape our world, specifically, the humans who are students and faculty in the Department of Biology at the ÌìÃÀÓ°ÊÓ´«Ã½. They are scientists who study everything from the ways cells move through complex tissues to ancient communities of long-extinct mammals, from the ways plants interact with their surroundings to the ways bats fly and hummingbirds feed. Plunge into the vast world of biology, where students share paths to becoming scientists and the lessons they have learned along the way.

Podcast:ÌýÌý(School of Drama)
A lively and opinionated cultural history of the Broadway Musical that tells the extraordinary story of how Immigrants, Jews, Queers, African-Americans, and other outcasts invented the Broadway Musical, and how they changed America in the process. In Season One, host David Armstrong traces the evolution of American Musical Theater from its birth at the dawn of the 20th Century, through its mid-century “Golden Age�, and right up to its current 21st Century renaissance; and also explores how musicals have reflected and shaped our world — especially in regard to race, gender, sexual orientation, and equality.

STREAMING 2025-26 LECTURES AND PERFORMANCES:

The World (Cup) Comes to Seattle Lecture Series (Jackson School of International Studies)
The Global Sports Lab hosts an online series of talks and discussions featuring local and global experts to discuss the geopolitical, local, and sporting implications of the 2026 FIFA Men’s World Cup in Seattle.


  • Presented by Sean Jacobs, Professor and Director of the Graduate Program in International Affairs at The New School, and Martha Saavedra, former Associate Director of the Center for African Studies at UC Berkeley.

  • Presented by César Wazen, Director of the International Affairs Office at Qatar University.
  • picture of the seattle skyline
    Presented by Mary V. Harvey, Chief Executive at the Center for Sport and Human Rights; Maya Mendoza-Exstrom, Board Member of the SeattleFWC26 Local Organizing Committee, Chief Business Officer of Seattle Reign Football Club, and Chief Operating Officer of Seattle Sounders Football Club; Leo Flor, Chief Legacy Officer of the SeattleFWC26 Local Organizing Committee; and Anita Ramasastry, Henry M. Jackson Professor of Law and Director of the Sustainable International Development Graduate Program at the ÌìÃÀÓ°ÊÓ´«Ã½ School of Law.

  • Presented by Niki Akhavan, Associate Professor and Chair of the Department of Media and Communication Studies at The Catholic University of America.

  • Presented by Teresa Mosqueda, Councilmember of the Metropolitan King County Council, and Anita Ramasastry, Barer Chair and Professor of Law at the ÌìÃÀÓ°ÊÓ´«Ã½.

  • Presented by Stéphane Mourlane, Senior Lecturer, Aix-Marseille University; Yvan Gastaut, Lecturer, University of Côte d’Azur; and Paul Dietschy, Professor, Marie and Louis Pasteur University.

  • Presented by Abdullah Al-Arian, Associate Professor of History, Georgetown University in Qatar.

  • Presented by Jen Barnes, Co-Chair of the Pride+ Match Impact Committee with SEA2026 and founder and CEO of both Rough & Tumble Pub and Salmon Bay FC.
Picture of David Baker
David Baker

Ìý(Physics)
Building on the Department’s longtime commitment to public scholarship, the lecture series brings renowned scientists to UW to offer free lectures on exciting advances in physics with the goal of fostering an appreciation of science and technology in our community:


  • Nobel laureate David Baker discusses advanced protein design software and its use in developing molecules to address challenges in medicine, technology, and sustainability.

  • Dr. John Martinis, recipient of the 2025 Nobel Prize in Physics, presents “Prehistoric quantum bits: experiments testing the fundamental physics of superconducting quantum devices.â€�

Image to promote the History Lecture Series Power & Punishment

Ìý(History)
Incarceration is a hotly debated topic in the United States, a country that has one of the highest rates of incarceration in the world. Looking at the practice from a historical perspective, what can incarceration teach us about who we were and who we are now? What might histories of incarceration, and the histories of those who have been incarcerated, tell us about power dynamics, belonging, exclusion, struggle, and hope across societies in the past and present? The 2026 History Lecture Series explores the practice of incarceration, tracing its evolution from antiquity to our modern world.

(Communication)
Kathleen Hall Jamieson is the Elizabeth Ware Packard Professor of Communication at the Annenberg School for Communication at the University of Pennsylvania, the Walter and Leonore Annenberg Director of the Annenberg Public Policy Center at the University of Pennsylvania, and the cofounder of the fact-checking site FactCheck.org and its science subsite, SciCheck. In this lecture, Dr. Jamieson argues that scientists and science communicators would be well served by using a “mental models� approach to simultaneously increase consequential knowledge and reduce public susceptibility to misconceptions about controversial climate and health findings. By engaging audiences with visual, verbal, or animated models, this approach fosters an understanding of science that audiences can draw on to recognize and reject consequential misconceptions.

(Department of English)
Nationally-acclaimed poet and critic Ange Mlinko lecture, “When Poets Say Nothing,� addresses the use of a negative mode in poetry, called apophasis or the apophatic. Her title itself is a clever pun that operates on several levels. Poets have always been accused of saying nothing much, of course. William Butler Yeats describes this accusation as a professional hazard; to be a poet is to “[b]e thought an idler by the noisy set / Of bankers, schoolmasters, and clergymen / The martyrs call the world.� On a different level, though, it is equally true that poets themselves invoke the negative to create distinct artistic and intellectual effects from those of positive language. As Mlinko noted, the apophatic is historically connected to theology, with figures from the ancient world, such as Saint Augustine of Hippo, urging that a correct human understanding of God must always be tempered by humility. Humans cannot understand the divine, writes Augustine; if you think you understand something, you can be sure it is not God. Poets say nothing when nothing is precisely the thing that needs to be said.

(Department of Psychology)
Dr. Cynthia Berg presents a perspective on self- and social-regulation that guides her work across the lifespan. In addition to talking about transition points across the lifespan where coordination of self- and social-regulation are linked to diabetes outcomes — across adolescence, in young adulthood, and in late adulthood — she identifies interventions that help to optimize the coordination of self- and social-regulation.

(School of Art + Art History + Design)
Visual Communication Design faculty members Karen Cheng, Annabelle Gould, Chad P. Hall, and Kristine Matthews give a series of short presentations reflecting on the designers, projects, and ideas that have shaped their practices and design values—from their time as students through their early careers. Their selections ranged from foundational texts on typography to inventive works, such as annual reports that document a designer’s year through charts and graphs. Watch the presentation recording to learn from these creative influencers.

UW School of Music Performances
Performances and more from the ÌìÃÀÓ°ÊÓ´«Ã½ School of Music.

Browse the full list of the UW School of Music’s


By bringing top minds from around the world to the ÌìÃÀÓ°ÊÓ´«Ã½ to teach and speak to the public, the UW Graduate School’s Office of Public Lectures takes big ideas and discoveries into the community and brings the community into scholarly life.


  • This talk invites audiences to explore five distinct perspectives on the political and cultural impact of the tournament—offering a more nuanced, thought-provoking look at what the World Cup means for Seattle and the world.

  • From winning two Olympic gold medals and a World Cup championship to enduring a career-ending concussion that left her “temporarily totally disabledâ€� and forced her to pawn her Olympic medals, Briana Scurry delivers a raw and inspiring account of resilience. With unflinching candor, she guides audiences through the soaring highs and devastating lows of her journey—sharing a story of triumph, adversity, and ultimate redemption. Along the way, Scurry reflects on soccer’s global influence and the enduring significance of the World Cup, offering a deeply personal perspective on the sport that shaped her life and legacy.

  • Based on Alexis Pauline Gumbs’ forthcoming book of poetic indexes, this interactive poetic lecture explores the life, teaching, and artwork of color theorist Alma Thomas. Engaging themes of audience, intimacy, abstract expressionist art, and the dynamic relationship between Black women’s creativity and the process of being Earth, the lecture invites participants into a rhythmic dialogue of form, meaning, and presence.

  • In the shadow of an empire, in a world on fire, what if we could imagine — and build — otherwise? Crip feminist technoscience teaches us how to wield disabled, mad, neuroexpansive, crip, sick people’s wisdom as a vital tool for surviving now and thriving then. Disabled people know intimately how to strategically leverage legal and policy tools and know precisely the limitations of these tools and frameworks.

  • While World War I is often framed as a European conflict, its most far-reaching consequences were profoundly felt far beyond Europe’s borders. In the Middle East, the war sparked a sweeping political crisis that ultimately led to the collapse of the Ottoman Empire. In its wake, the European victors imposed new borders and mandates, carving the region into fragmented zones of imperial control and influence. But this was not merely a story of unchecked colonial dominance. In the postwar moment, a spectrum of fluid, intersecting anti-colonial movements emerged. Palestine became a key site in these struggles, as a racialized order of settler-colonial capitalism took shape under British rule. This talk locates those movements within the broader transition from British to American imperial ascendancy, contending that the political history of the region must be understood as integral to the global history of fossil capitalism. Moving beyond frameworks centered solely on empire, the talk examines how anti-colonial actors envisioned their futures within a rapidly transforming global system—even as new hierarchies of race, empire, and capital were being redefined.

  • This talk explores the idea that the endurance of the rule of law in the United States relies not solely on the provisions of the Constitution—its structural framework, the institutions it established, or the rights it enshrines—but fundamentally on the character of its citizens. Qualities such as public-spiritedness, tolerance, moderation, empathy, mutual respect, a sense of fair play, and, ultimately, intelligence, honor, and decency form the foundation of constitutional democracy.

  • Join this lecture on reviving MLK’s vision of the beloved community—where inclusion, cultural goodwill, and nonviolence expand democracy beyond voting. Discover how these values can bridge today’s deep divides and strengthen the soul of American civic life.

  • Healthcare can be challenging for anyone—but for older LGBTQ individuals, the barriers are often deeper and more complex. This engaging talk explores how thoughtful, inclusive communication can transform healthcare experiences, making every person feel truly seen, heard, and respected. Join us to learn how the words we choose and the ways we listen can foster trust, reduce disparities, and build a system that cares for everyone with dignity.

  • Is artificial intelligence on the brink of world domination? Have tech giants created autonomous thinking machines? Will AI render authors, artists, and other creatives obsolete? Are we entering an era where computers surpass humans in every way?

  • In this powerful and deeply personal talk, Dr. Uché Blackstock explores the legacies that have shaped her journey—both personal and institutional. She reflects on following in her mother’s footsteps to medical school, a path that made Dr. Blackstock and her twin sister the first Black mother-daughter legacy at the institution.

(Simpson Center for the Humanities)
The Katz Distinguished Lectures Playlist offers a rich, ever-growing archive to explore from anywhere, inviting you to engage with a wide range of thought-provoking topics.


  • Why do we turn to the past in order to confront the crises of the present? Michael Rothberg approaches this question from the perspective of “comparison controversies,” which occur when impassioned public debates emerge from provocative historical comparisons. Since October 7, 2023, political speeches, protests, magazine articles, and social media posts have generated controversy by connecting recent events in Israel and Gaza to the Holocaust. In this talk, Rothberg will consider post-October 7 examples in relation to a larger context of comparison controversies and a longer trajectory of Holocaust memory to reflect more generally on the possibilities and pitfalls of historical analogy.

  • The production and promotion of so-called “AIâ€� technology involves dehumanization on many fronts: the computational metaphor valorizes one kind of cognitive activity as “intelligence,â€� devaluing many other aspects of human experience while taking an isolating, individualistic view of agency, ignoring the importance of communities and webs of relationships. Meanwhile, the purpose of humans is framed as labeling data or as interchangeable machine components. Data collected about people is understood as “ground truthâ€� even while it lies about those people, especially marginalized people. In this talk, Bender will explore these processes of dehumanization and the vital role that the humanities have in resisting these trends by painting a deeper and richer picture of what it is to be human.

(Astronomy)
What will Rubin Observatory discover that no one’s expecting? Neil deGrasse Tyson and comedian Chuck Nice learn and answer cosmic queries about the Vera Rubin Observatory, the Legacy Survey of Space and Time (LSST), and our next big tool to uncover more about the universe with Zeljko Ivezic, Director of Rubin Observatory Construction.


ArtSci Roundup goes monthly!

The ArtSci Roundup is your guide to connecting with the UW—whether in person, on campus, or on your couch.

Previously shared on a quarterly basis, those who sign up for the Roundup email will receive them monthly, delivering timely updates and engaging content wherever you are. Check the roundup regularly, as events are added throughout the month. Make sure to check out the ArtSci On Your Own Time section for everything from podcasts to videos to exhibitions that can be enjoyed when it works for you!

In addition, if you like the ArtSci Roundup, sign up to receive a monthly notice when it’s been published.

Do you have an event that you would like to see featured in the ArtSci Roundup? Connect with Lauren Zondag (zondagld@uw.edu).uw.edu).

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Rubin Observatory begins landmark 10-year timelapse of night sky /news/2026/06/30/rubin-observatory-legacy-survey-space-time-lsst/ Tue, 30 Jun 2026 18:27:57 +0000 /news/?p=92274 A dense, colorful starfield
A field of stars in the constellation Lupus captured by the Simonyi Survey Telescope at the NSF–DOE Vera C. Rubin Observatory. The faint, glowing clouds spread across the image are galactic cirrus: clouds of interstellar gas and dust that can be seen in the foreground of the Milky Way galaxy. The original image is a whopping 1.7 gigapixels in size, a scale made possible by the Rubin Observatory’s 3,200-megapixel camera, the largest digital camera in the world. Photo: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA

From a mountaintop in Chile, under clear dark skies, the Simonyi Survey Telescope at the NSF–DOE Vera C. Rubin Observatory has officially begun the Legacy Survey of Space and Time (). The 10-year survey will create the most comprehensive, cinematic record of the universe in history. Over the next decade, Rubin will observe the entire southern sky every few nights to create an ultra-wide, ultra-high-definition time-lapse record of our universe.Ìý

“The decision to officially begin the LSST was made after a period of system optimization and a careful operational review of technical readiness, data system performance and scientific validation,â€� said , a ÌìÃÀÓ°ÊÓ´«Ã½ professor of astronomy and head of LSST. “The ÌìÃÀÓ°ÊÓ´«Ã½ Rubin team played a central role in optimizing the observatory and helping prepare it for the start of full survey operations.â€�

The Simonyi Survey Telescope’s unique design combines enormous light-collecting power, the ability to move rapidly across the sky and a wide field of view. The attached 3,200-megapixel camera — the largest digital camera in the world — is now capturing a new, detailed image approximately every 40 seconds. Using a telescope with this speed and sensitivity, Rubin is capable of catching faint objects and fleeting events with reliability and consistency every night.

Over the next decade, Rubin will illuminate a treasure trove of discoveries: pulsating stars, supernova explosions, the fossil record of galaxies, clues to the mysteries of dark energy and dark matter, and entirely new phenomena we’ve never seen before. Some cosmic processes unfold slowly, unpredictably or incredibly rarely, which is why a 10-year survey is essential. By returning to each point in the sky about 800 times over a decade, Rubin data will provide the scientific community with deep, time-rich views needed to uncover subtle events, capture moving objects and study the accelerating expansion of the universe.

This milestone follows the Rubin First Look event that took place in June 2025, which was followed by final commissioning work, an operational readiness review and the beginning of the alert stream.

Each night, Rubin collects approximately 10 terabytes of data and produces as many as seven million alerts of changes in the night sky. These alerts stream to : automated systems that sort and classify these changes so scientists can act quickly. UW researchers led by , research associate professor of astronomy, developed the alert pipeline.

“Astronomers have already used Rubin’s public alerts to discover and follow up hundreds of transient phenomena during the early optimization period,â€� Bellm said. “We can expect many more exciting discoveries with the start of the full survey.â€�

Not only is Rubin helping to unlock the mysteries of the distant universe, it is also the most powerful solar system discovery machine ever built. By taking about a thousand images every night, Rubin is compiling a detailed census of our solar system, including millions of asteroids and comets. In just a month and a half, during early optimization surveys, Rubin discovered over 11,000 never-before-seen asteroids, including 33 near-Earth objects and 380 trans-Neptunian objects.

Rubin combines a wide view of the sky with the ability to detect extremely faint objects. With this capability, Rubin can reveal details of the cosmos across an enormous range of scales, from distant galaxies, to individual stars, to the wispy clouds of dust spread throughout our galaxy. Photo: NSF–DOE Vera C. Rubin Observatory/NOIRLab/SLAC/AURA

When the LSST is complete, the final dataset will contain billions of objects with trillions of measurements, all accessible through regular data releases. This is the first time so much astronomical data will be available to so many people, opening the door to new kinds of discovery by both scientists and the public. Rubin invites anyone in the world to engage with its data and explore the dynamic universe in ways never before possible.

“It is amazing and humbling to be here at this time and place as we start the Legacy Survey of Space and Time, after more than two decades of incredible work by our dedicated team,� said Bob Blum, director of Rubin Observatory at NSF NOIRLab. “Rubin Observatory is for everyone; the LSST will change how we do astronomy and astrophysics, allowing researchers anywhere to participate in cutting-edge science.�

Visit to follow the status of the LSST in real time.

Rubin Observatory is jointly operated by NSF NOIRLab and SLAC. Observatory operationsÌýare funded by the U.S. National Science Foundation and the U.S. Department of Energy’s Office of Science.

For more information, contact Ivezić at ivezic@astro.washington.edu.

This story was adapted from a press release by .

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June research highlights: Air quality inequity, ultrafast chemistry, cigar galaxy, more /news/2026/06/30/june-research-highlights-air-quality-inequity-ultrafast-chemistry-cigar-galaxy-more/ Tue, 30 Jun 2026 17:29:57 +0000 /news/?p=92268
This high-resolution image of Messier 82, also known as the Cigar galaxy because of its elliptical shape, provides the most detailed look yet at the one-of-a-kind galaxy. Photo: NASA, ESA, CSA, Adam Smercina (STScI, Tufts), Thomas Williams (University of Manchester); Image Processing: Alyssa Pagan (STScI)

New images of cigar-shaped M82 galaxy capture millions of stars

The Messier 82 galaxy, known as M82 or the Cigar galaxy, has long fascinated researchers with its astronomical rate of star formation — approximately 10 times faster than the Milky Way. Researchers have pored over grainy, low-resolution, images taken by previous generations of telescopes, which weren’t powerful enough to see through the thick cloud of dust surrounding the galaxy. The , however, can pierce straight through with extremely sharp vision. That enabled a team of astronomers from multiple institutions, including NASA and the UW, to capture new high-resolution images. Posted June 23, the images include more than 16.5 million individual stars and provide the clearest look yet at M82’s , the flattened central hub that contains most of the galaxy’s stellar mass. That could help scientists understand how M82 formed and for how long it has been producing stars so prodigiously.

For more information, contact team member a UW research professor of astronomy, at benw1@uw.edu.

All images are included in NASA’s


New study maps pollution disparities by state and sector across almost 20 years

Air quality in the United States has improved markedly since the landmark Clean Air Act passed in 1970. However, the gains have not been equally shared: Today, communities of color and low-income communities are exposed to disproportionately more air pollution than the overall population. In in Science Advances, UW researchers created the first comprehensive map cataloging how air quality inequity has changed per state and economic sector from 2002 to 2019. The study confirmed that, despite improvements in overall air quality, pollution tends to be concentrated in Black, Hispanic and low-income communities. The findings include specific state-level opportunities for improvement across 11 sectors — for example, disparities in construction-related emissions in Florida increased significantly during the study period. The findings and resulting database could help policymakers across the country prioritize environmental justice projects.

For more information, contact senior author , UW professor of civil and environmental engineering at jdmarsh@uw.edu.

The other UW co-authors are , , and . A full list of co-authors is .Ìý


Researchers observe ultrafast chemistry happening in real time

Molecules are not static. Instead, they are having little dance parties — their atoms wiggle and twist around in space. Occasionally, upon receiving a burst of energy, the bonds holding atoms together in a molecule can break and reform with the atoms in a different configuration. While the number of atoms stays the same, the orientation of these atoms determines a molecule’s chemical properties — an important part of its identity. In , a UW-led team witnessed firsthand, and for the first time, a molecule turning into its “alter ego.” The researchers observed a hydrogen atom, also known as a proton, jump to a new position by bonding to a different atom in the same molecule. This process, which happens within a few millionths of billionths of a second, is important for various fundamental processes, including photosynthesis, and when DNA acquires mutations. To understand why, and how, this happens so fast, the researchers developed a new tool that probes molecular structure on an ultrafast timescale. They were able to use this technology to detect how the molecule’s wiggles allowed the proton transfer to happen. These findings will help researchers test existing theories about these ultrafast chemical dynamics and develop new molecules for clean energy processes.

For more information, contact senior author , UW professor of chemistry, at mkhalil@uw.edu.ÌýÌýÌý

Co-authors , and completed this work while at the UW. Funding information is .


Random events leave lasting signature on the atmospheric methane record, new study shows

Methane is a powerful greenhouse gas with a complicated life cycle. It’s released into the atmosphere by both natural and industrial processes, and there are multiple pathways by which it’s broken down. Recently, atmospheric methane levels have reached record highs but the rate of accumulation has been somewhat inconsistent over time. To understand why, researchers are looking at climate records preceding the industrial era, via ice cores. These deep cylinders of glacial ice document slow swings in atmospheric methane levels spanning decades, or even centuries. This pattern is typically associated with gradual climate change, but in , UW researchers show that it doesn’t have to be. Instead, they reveal that short-term, random events, such as fires or changes in wetlands, can spark gradual shifts. Not only does this clarify the historical record, but it also adds nuance to modern trends.

For more information, contact senior author , UW doctoral student of atmospheric and climate science at emei@uw.edu.

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

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April research highlights: Sunbird tongues, Seattle fault, inbound asteroids, more /news/2026/04/28/april-research-highlights-sunbird-tongues-seattle-fault-inbound-asteroids-more/ Tue, 28 Apr 2026 16:07:03 +0000 /news/?p=91471 Sunbirds use their tongues as straws

The team took high-speed video of sunbirds drinking from transparent artificial flowers. Shown here are two views — a macro video of the sunbird drinking (top) and a close-up of its tongue inside the “flower” (bottom). The nectar in these flowers is dyed red so that it’s easy to see it going into the birds’ tongues. Credit: Cuban et al./Current Biology

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 ÌìÃÀÓ°ÊÓ´«Ã½ 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.ÌýÌý

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


Seattle Fault gets 5,000 more years of sleepÌý

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

This landslide occurred in December 2025 within the study area. It destroyed multiple houses and crashed into the Siletz river, partially blocking but not damming it. This work was motivated by concerns about similar landslides damming narrower sections of the river. Photo:

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 —Ìý 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

The various shapes shown in the circle are phytoplankton, from the Strait of Juan de Fuca, under a microscope. Most species pictured are diatoms, many of which likely produce homarine. Photo: Anitra Ingalls

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.Ìý

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

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