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Bigger, Better Catalog Unveils Half a Billion Celestial Objects
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By NASA
A funky effect Einstein predicted, known as gravitational lensing — when a foreground galaxy magnifies more distant galaxies behind it — will soon become common when NASA’s Nancy Grace Roman Space Telescope begins science operations in 2027 and produces vast surveys of the cosmos.
This image shows a simulated observation from NASA’s Nancy Grace Roman Space Telescope with an overlay of its Wide Field Instrument’s field of view. More than 20 gravitational lenses, with examples shown at left and right, are expected to pop out in every one of Roman’s vast observations. A journal paper led by Bryce Wedig, a graduate student at Washington University in St. Louis, Missouri, estimates that of those Roman detects, about 500 from the telescope’s High-Latitude Wide-Area Survey will be suitable for dark matter studies. By examining such a large population of gravitational lenses, the researchers hope to learn a lot more about the mysterious nature of dark matter.Credit: NASA, Bryce Wedig (Washington University), Tansu Daylan (Washington University), Joseph DePasquale (STScI) A particular subset of gravitational lenses, known as strong lenses, is the focus of a new paper published in the Astrophysical Journal led by Bryce Wedig, a graduate student at Washington University in St. Louis. The research team has calculated that over 160,000 gravitational lenses, including hundreds suitable for this study, are expected to pop up in Roman’s vast images. Each Roman image will be 200 times larger than infrared snapshots from NASA’s Hubble Space Telescope, and its upcoming “wealth” of lenses will vastly outpace the hundreds studied by Hubble to date.
Roman will conduct three core surveys, providing expansive views of the universe. This science team’s work is based on a previous version of Roman’s now fully defined High-Latitude Wide-Area Survey. The researchers are working on a follow-up paper that will align with the final survey’s specifications to fully support the research community.
“The current sample size of these objects from other telescopes is fairly small because we’re relying on two galaxies to be lined up nearly perfectly along our line of sight,” Wedig said. “Other telescopes are either limited to a smaller field of view or less precise observations, making gravitational lenses harder to detect.”
Gravitational lenses are made up of at least two cosmic objects. In some cases, a single foreground galaxy has enough mass to act like a lens, magnifying a galaxy that is almost perfectly behind it. Light from the background galaxy curves around the foreground galaxy along more than one path, appearing in observations as warped arcs and crescents. Of the 160,000 lensed galaxies Roman may identify, the team expects to narrow that down to about 500 that are suitable for studying the structure of dark matter at scales smaller than those galaxies.
“Roman will not only significantly increase our sample size — its sharp, high-resolution images will also allow us to discover gravitational lenses that appear smaller on the sky,” said Tansu Daylan, the principal investigator of the science team conducting this research program. Daylan is an assistant professor and a faculty fellow at the McDonnell Center for the Space Sciences at Washington University in St. Louis. “Ultimately, both the alignment and the brightness of the background galaxies need to meet a certain threshold so we can characterize the dark matter within the foreground galaxies.”
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This video shows how a background galaxy’s light is lensed or magnified by a massive foreground galaxy, seen at center, before reaching NASA’s Roman Space Telescope. Light from the background galaxy is distorted, curving around the foreground galaxy and appearing more than once as warped arcs and crescents. Researchers studying these objects, known as gravitational lenses, can better characterize the mass of the foreground galaxy, which offers clues about the particle nature of dark matter.Credit: NASA, Joseph Olmsted (STScI) What Is Dark Matter?
Not all mass in galaxies is made up of objects we can see, like star clusters. A significant fraction of a galaxy’s mass is made up of dark matter, so called because it doesn’t emit, reflect, or absorb light. Dark matter does, however, possess mass, and like anything else with mass, it can cause gravitational lensing.
When the gravity of a foreground galaxy bends the path of a background galaxy’s light, its light is routed onto multiple paths. “This effect produces multiple images of the background galaxy that are magnified and distorted differently,” Daylan said. These “duplicates” are a huge advantage for researchers — they allow multiple measurements of the lensing galaxy’s mass distribution, ensuring that the resulting measurement is far more precise.
Roman’s 300-megapixel camera, known as its Wide Field Instrument, will allow researchers to accurately determine the bending of the background galaxies’ light by as little as 50 milliarcseconds, which is like measuring the diameter of a human hair from the distance of more than two and a half American football fields or soccer pitches.
The amount of gravitational lensing that the background light experiences depends on the intervening mass. Less massive clumps of dark matter cause smaller distortions. As a result, if researchers are able to measure tinier amounts of bending, they can detect and characterize smaller, less massive dark matter structures — the types of structures that gradually merged over time to build up the galaxies we see today.
With Roman, the team will accumulate overwhelming statistics about the size and structures of early galaxies. “Finding gravitational lenses and being able to detect clumps of dark matter in them is a game of tiny odds. With Roman, we can cast a wide net and expect to get lucky often,” Wedig said. “We won’t see dark matter in the images — it’s invisible — but we can measure its effects.”
“Ultimately, the question we’re trying to address is: What particle or particles constitute dark matter?” Daylan added. “While some properties of dark matter are known, we essentially have no idea what makes up dark matter. Roman will help us to distinguish how dark matter is distributed on small scales and, hence, its particle nature.”
Preparations Continue
Before Roman launches, the team will also search for more candidates in observations from ESA’s (the European Space Agency’s) Euclid mission and the upcoming ground-based Vera C. Rubin Observatory in Chile, which will begin its full-scale operations in a few weeks. Once Roman’s infrared images are in hand, the researchers will combine them with complementary visible light images from Euclid, Rubin, and Hubble to maximize what’s known about these galaxies.
“We will push the limits of what we can observe, and use every gravitational lens we detect with Roman to pin down the particle nature of dark matter,” Daylan said.
The Nancy Grace Roman Space Telescope is managed at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, with participation by NASA’s Jet Propulsion Laboratory in Southern California; Caltech/IPAC in Pasadena, California; the Space Telescope Science Institute in Baltimore; and a science team comprising scientists from various research institutions. The primary industrial partners are BAE Systems, Inc. in Boulder, Colorado; L3Harris Technologies in Melbourne, Florida; and Teledyne Scientific & Imaging in Thousand Oaks, California.
By Claire Blome
Space Telescope Science Institute, Baltimore, Md.
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Last Updated Jun 12, 2025 EditorAshley BalzerContactAshley Balzerashley.m.balzer@nasa.govLocationNASA Goddard Space Flight Center Related Terms
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By Space Force
The Air Force Aid Society, AFAS, announced a series of bold changes aimed at better supporting the evolving needs of Airmen, Guardians, and their families.
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By European Space Agency
Video: 00:02:27 2025 marks a landmark year for Europe’s ‘bridge between Earth and space’. The European Space Agency’s Estrack satellite tracking network turns 50.
Since its inception in 1975, Estrack – ESA’s global network of ground stations – has formed the vital communication bridge between satellites in orbit and mission control at the European Space Operations Centre (ESOC) in Darmstadt, Germany.
Now comprising six stations spanning six countries, Estrack has grown into a strategic asset for Europe, enabling communication with spacecraft, transmitting commands and receiving scientific data.
The network keeps an eye on satellites no matter their location: tracking them across Earth orbit, voyaging to comets or asteroids, keeping station at the scientifically important Sun-Earth Lagrange points, and deep into our Solar System. It even keeps tabs on European launchers as they soar into orbit, ensuring no rocket is ever out of reach.
Fittingly, this celebration of technological excellence coincides with the 200th birthday of Johann Strauss II and the 50th anniversary of ESA. To honour this convergence of milestones, ESA and the Vienna Tourist Board are orchestrating a unique mission: broadcasting The Blue Danube Waltz to its destined home among the stars.
Don’t miss the live concert of the Wiener Symphoniker (Vienna Symphony Orchestra) on Saturday, 31 May. The event will start at 20:30 CEST and the transmission from ESA’s Cebreros antenna will occur at 21:30 CEST.
The live stream can be followed via space.wien.info and the Vienna Instagram channel.
Waltzing celebration for half a century of European satellite tracking
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By European Space Agency
As the new Biomass satellite settles into life in orbit following its launch on 29 April, ESA has released its most extensive satellite-based maps of above-ground forest carbon to date. Spanning nearly two decades, the dataset offers the clearest global picture yet of how forest carbon stocks have changed over time.
Developed through ESA’s Climate Change Initiative, this new long-term record integrates data from multiple satellite missions – and will soon be further enhanced by data from the Biomass mission itself.
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By NASA
Explore This Section Science Science Activation Building for a Better World:… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 6 min read
Building for a Better World: Norfolk Students Bring STEM to Life with NASA Partnership
At Norfolk Technical Center in Norfolk, Virginia, carpentry students in Jordan Crawford’s first-year class aren’t just learning how to measure and cut wood—they’re discovering how their skills can serve a greater purpose.
When the NASA Science Activation program’s NASA eClips project—led by the National Institute of Aerospace’s Center for Integrative Science, Technology, Engineering, and Mathematics (STEM) Education (NIA-CISE)—needed help building weather instrument shelters for local schools, Norfolk Public Schools’ Career and Technical Education (CTE) team saw an opportunity to connect students to something bigger than the classroom. The shelters are used to house scientific equipment that K–12 students rely on to collect data using GLOBE (Global Learning and Observations to Benefit the Environment) protocols—a set of standardized, internationally recognized methods for gathering environmental data such as temperature, soil moisture, and cloud cover. These observations contribute to a global citizen science database, giving young learners a meaningful role in real-world environmental research.
Originally, shelters were being ordered from a national supplier to support GLOBE training sessions for teachers in GO (Growth & Opportunity) Virginia Region 5, an economic development region. These training sessions were funded through a generous grant from the Coastal Virginia STEM Hub (COVA STEM Hub), which supports regional collaboration in STEM education. But when the supplier couldn’t keep up with demand, Norfolk Public Schools CTE Specialist Dr. Deborah Marshall offered a bold solution: why not have local students build them?
That’s when the project truly took off. Under the guidance of Jordan Crawford, students took on the challenge of building 20 high-quality shelters in spring 2024, following precise construction plans provided through the GLOBE Program. Materials were funded by the COVA STEM grant, and the students rolled up their sleeves to turn lumber into lasting educational tools for their community.
“As an instructor, you look for opportunities that challenge your students, allow them to do things bigger than themselves, and let them see a project through from start to finish,” Crawford said. “This project allowed my students to hone existing skills and build new ones, and I saw incredible growth not just in craftsmanship but in teamwork. The most rewarding part was seeing the impact of their work in real schools.”
And the students rose to the occasion—taking pride in their work, learning advanced techniques, and developing new confidence. One of the most challenging parts of the build involved crafting the louvers—angled slats on the sides of the shelters needed for proper air circulation. Student Zymere Watts took the lead in designing and building a jig to make sure the louvers could be cut uniformly and precisely for every unit.
“Building the weather shelters was a fun and challenging task that pushed me to strive for perfection with each one,” said student Amir Moore. “After completion, I was delighted to see the faces of the people who were proud and happy with what we built.”
“It was an extreme pleasure working on this project. I would love to work with NIA again,” added LaValle Howard. “I am proud to be a part of this vocational school and team.”
Jaymyson Burden agreed: “It was fun and great to be exposed to the carpentry realm and install them in the real world. It was gratifying to know what we have done has an impact.”
After completing the shelters, the students volunteered to install them at seven Hampton City Schools. Their work completed the full circle—from building the shelters in their carpentry classroom to setting them up where younger students would use them to collect real environmental data.
Their dedication did not go unnoticed. The team was invited to NASA’s Langley Research Center for a behind-the-scenes tour of the NASA Model Shop, where they met Sam James, a Mechanical Engineering Technician and Fabrication Specialist. James showed the students how the same kind of craftsmanship they’d used is essential in the creation of tools and components for NASA missions. They also learned about NASA summer internships and discovered that their hands-on skills could open doors to exciting careers in STEM fields.
“It was an honor to help where we were needed,” said student Josh Hunsucker. “Assembling these gave us a new perspective on the importance of duplication and how each step impacts the result. We’re happy to help wherever or whenever we’re needed—it provides a learning experience for us.”
Kyra Pope summed it up: “It’s been a great amount of work over the past few months, but it pays off—especially when you’re giving back to the community.”
According to Dr. Sharon Bowers, Associate Director and Senior STEM Education Specialist for NIA-CISE, the project demonstrates what’s possible when regional partners come together to empower students and educators alike. “The financial support from COVA STEM Hub supported sustained educator professional learning within our STEM learning ecosystem. Work with the Norfolk Technical Center truly made this a real-world, problem-solving experience. This is just the beginning for more collaborative work that will bring the region together to engage educators and learners in authentic STEM learning experiences.”
This collaboration wasn’t just about building boxes to house thermometers. It was about building bridges—between technical education and science, between high school students and their futures, and between local classrooms and global research. With each shelter they crafted, the students created something that will outlast them, reminding others—and themselves—of what’s possible when learning is hands-on, meaningful, and connected to the world beyond school walls.
Thanks to Betsy McAllister, NIA’s Educator-in-Residence from Hampton City Schools, for her impactful contributions and for sharing this story. The NASA eClips project provides educators with standards-based videos, activities, and lessons to increase STEM literacy through the lens of NASA. It is supported by NASA under cooperative agreement award number NNX16AB91A and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn
Carpentry students from the Norfolk Technical Center install a digital, multi-day, minimum/maximum thermometer in the GLOBE instrument shelter. Share
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