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By NASA
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
El piloto de pruebas de la NASA Nils Larson inspecciona el avión de investigación F-15D de la agencia en el Centro de Investigación de Vuelo Armstrong de la NASA en Edwards, California, antes de un vuelo de calibración para una sonda de detección de impactos de campo cercano recién instalada. Montada en el F-15D, la sonda está diseñada para medir las ondas de choque generadas por el silencioso avión supersónico X-59 durante el vuelo. Los datos ayudarán a los investigadores a comprender mejor cómo se comportan las ondas de choque en las proximidades de la aeronave, apoyando la misión Quesst de la NASA para permitir vuelos supersónicos silenciosos sobre tierra.NASA/Steve Freeman El piloto de pruebas de la NASA Nils Larson inspecciona el avión de investigación F-15D de la agencia en el Centro de Investigación de Vuelo Armstrong de la NASA en Edwards, California, antes de un vuelo de calibración para una sonda de detección de impactos de campo cercano recién instalada. Montada en el F-15D, la sonda está diseñada para medir las ondas de choque generadas por el silencioso avión supersónico X-59 durante el vuelo. Los datos ayudarán a los investigadores a comprender mejor cómo se comportan las ondas de choque en las proximidades de la aeronave, apoyando la misión Quesst de la NASA para permitir vuelos supersónicos silenciosos sobre tierra.NASA/Steve Freeman El avión de investigación F-15D de la NASA realiza un vuelo de prueba cerca de Edwards, California, con una sonda de detección de impactos de campo cercano. Idéntica a una versión previamente volada que estaba prevista como reserva, esta nueva sonda captará datos de ondas de choque cerca del X-59 mientras vuela a velocidad más rápida que la del sonido apoyando la misión Quesst de la NASA.NASA/Jim Ross El avión de investigación F-15D de la NASA realiza un vuelo de prueba cerca de Edwards, California, con una sonda de detección de impactos de campo cercano. Idéntica a una versión previamente volada que estaba prevista como reserva, esta nueva sonda captará datos de ondas de choque cerca del X-59 mientras vuela a velocidad más rápida que la del sonido apoyando la misión Quesst de la NASA.NASA/Jim Ross Read this story in English here.
Cuando se prueba un avión de última generación de la NASA, se necesitan herramientas especializadas para realizar pruebas y capturar datos, pero si esas herramientas necesitan mantenimiento, hay que esperar hasta que se reparen. A menos que tengas un respaldo. Por eso, recientemente la NASA ha calibró una nueva sonda de deteccíon de impactos para capturar datos de ondas de choque cuando el silencioso avión de investigación supersónico X-59 de la agencia inicie sus vuelos de prueba.
Cuando un avión vuela más rápido que la velocidad del sonido, produce ondas de choque que viajan a través del aire, creando fuertes estampidos sónicos. El X-59 desviará esas ondas de choque, produciendo sólo un silencioso golpe supersónico. En las últimas semanas, la NASA ha completado los vuelos de calibración de una nueva sonda de detección de impactos de campo cercano, un aparato en forma de cono que captará datos sobre las ondas de choque que generará el X-59.
Esta sonda está montada en un avión de investigación F-15D que volará muy cerca del X-59 para recopilar los datos que necesita la NASA. La nueva unidad servirá como la sonda de campo cercano principal de la NASA, con un modelo idéntico desarrollado por la NASA el año pasado actuará como reserva montada en otro F-15B.
Las dos unidades significan que el equipo del X-59 tiene una alternativa lista en caso de que la sonda principal necesite mantenimiento o reparaciones. Para pruebas de vuelo como las del X-59, donde la recopilación de datos es crucial y las operaciones giran en torno a plazos ajustados, condiciones meteorológicas y otras variables, las copias de respaldo de los equipos críticos ayudan a garantizar la continuidad, mantener los plazos y preservar la eficiencia de las operaciones.
“Si le ocurre algo a la sonda, como una falla en unsensor, no hay una solución fácil,” explica Mike Frederick, investigador principal de la sonda en el Centro de Investigación de Vuelos Armstrong de la NASA en Edwards, California. “El otro factor es el propio avión. Si uno necesita mantenimiento, no queremos retrasar los vuelos del X-59.”
Para calibrar la nueva sonda, el equipo midió las ondas de choque de un avión de investigación F/A-18 de la NASA. Los resultados preliminares indicaron que la sonda captó con éxito los cambios de presión asociados a las ondas de choque, de acuerdo con las expectativas del equipo. Frederick y su equipo ahora están revisando los datos para confirmar que se alinean con los modelos matemáticos en tierra y cumplen las normas de precisión requeridas para los vuelos X-59.
Los investigadores de la NASA en Armstrong se están preparando para vuelos adicionales con las sondas principal y de respaldo en sus aviones F-15. Cada avión volará a velocidad supersónico y recopilará datos de las ondas de choque del otro. El equipo está trabajando para validar tanto la sonda principal como la de respaldo para confirmar la redundancia total;en otras palabras, asegurarse de que tengan un respaldo fiable y listo para usar.
Artículo Traducido por: Priscila Valdez
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Last Updated May 13, 2025 EditorDede DiniusContactNicolas Cholulanicolas.h.cholula@nasa.gov Related Terms
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By NASA
Teams at NASA’s Michoud Assembly Facility in New Orleans move a liquid hydrogen tank for the agency’s SLS (Space Launch System) rocket into the factory’s final assembly area on April 22, 2025. The propellant tank is one of five major elements that make up the 212-foot-tall rocket stage. NASA/Steven Seipel NASA completed another step to ready its SLS (Space Launch System) rocket for the Artemis III mission as crews at the agency’s Michoud Assembly Facility in New Orleans recently applied a thermal protection system to the core stage’s liquid hydrogen tank.
Building on the crewed Artemis II flight test, Artemis III will add new capabilities with the human landing system and advanced spacesuits to send the first astronauts to explore the lunar South Pole region and prepare humanity to go to Mars. Thermal protection systems are a cornerstone of successful spaceflight endeavors, safeguarding human life, and enabling the launch and controlled return of spacecraft.
The tank is the largest piece of SLS flight hardware insulated at Michoud. The hardware requires thermal protection due to the extreme temperatures during launch and ascent to space – and to keep the liquid hydrogen at minus 423 degrees Fahrenheit on the pad prior to launch.
“The thermal protection system protects the SLS rocket from the heat of launch while also keeping the thousands of gallons of liquid propellant within the core stage’s tanks cold enough. Without the protection, the propellant would boil off too rapidly to replenish before launch,” said Jay Bourgeois, thermal protection system, test, and integration lead at NASA Michoud. “Thermal protection systems are crucial in protecting all the structural components of SLS during launch and flight.”
In February, Michoud crews with NASA and Boeing, the SLS core stage prime contractor, completed the thermal protection system on the external structure of the rocket’s liquid hydrogen propellant fuel tank, using a robotic tool in what is now the largest single application in spaceflight history. The robotically controlled operation coated the tank with spray-on foam insulation, distributing 107 feet of the foam to the tank in 102 minutes. When the foam is applied to the core stage, it gives the rocket a canary yellow color. The Sun’s ultraviolet rays naturally “tan” the thermal protection, giving the SLS core stage its signature orange color, like the space shuttle external tank.
Having recently completed application of the thermal protection system, teams will now continue outfitting the 130-foot-tall liquid hydrogen tank with critical systems to ready it for its designated Artemis III mission. The core stage of SLS is the largest ever built by length and volume, and was manufactured at Michoud using state-of-the-art manufacturing equipment. (NASA/Steven Seipel) While it might sound like a task similar to applying paint to a house or spraying insulation in an attic, it is a much more complex process. The flexible polyurethane foam had to withstand harsh conditions for application and testing. Additionally, there was a new challenge: spraying the stage horizontally, something never done previously during large foam applications on space shuttle external tanks at Michoud. All large components of space shuttle tanks were in a vertical position when sprayed with automated processes.
Overall, the rocket’s core stage is 212 feet with a diameter of 27.6 feet, the same diameter as the space shuttle’s external tank. The liquid hydrogen and liquid oxygen tanks feed four RS-25 engines for approximately 500 seconds before SLS reaches low Earth orbit and the core stage separates from the upper stage and NASA’s Orion spacecraft.
“Even though it only takes 102 minutes to apply the spray, a lot of careful preparation and planning is put into this process before the actual application of the foam,” said Boeing’s Brian Jeansonne, the integrated product team senior leader for the thermal protection system at NASA Michoud. “There are better process controls in place than we’ve ever had before, and there are specialized production technicians who must have certifications to operate the system. It’s quite an accomplishment and a lot of pride in knowing that we’ve completed this step of the build process.”
The core stage of SLS is the largest NASA has ever built by length and volume, and it was manufactured at Michoud using state-of-the-art manufacturing equipment. Michoud is a unique, advanced manufacturing facility where the agency has built spacecraft components for decades, including the space shuttle’s external tanks and Saturn V rockets for the Apollo program.
Through Artemis, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and build the foundation for the first crewed missions to Mars.
For more information on the Artemis Campaign, visit:
https://www.nasa.gov/feature/artemis/
News Media Contact
Jonathan Deal
Marshall Space Flight Center, Huntsville, Ala.
256-544-0034
jonathan.e.deal@nasa.gov
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By NASA
Explore This Section Science Science Activation Take a Tour of the Cosmos with… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 4 min read
Take a Tour of the Cosmos with New Interactives from NASA’s Universe of Learning
Ready for a tour of the cosmos? NASA’s Universe of Learning has released a new, dynamic way for lifelong learners to explore NASA’s breathtaking images of the universe—ViewSpace interactive Image Tours. ViewSpace has an established track record of providing museums, science centers, libraries, and other informal learning environments with free, web-based videos and digital interactives—like its interactive Image Sliders. These new Image Tours are another unique experience from NASA’s Universe of Learning, created through a collaboration between scientists that operate NASA telescopes and experts well-versed in the most modern methods of learning. Hands-on, self-directed learning resources like these have long been valued by informal learning sites as effective means for engaging and intriguing users with the latest discoveries from NASA’s space telescope missions—while encouraging lifelong learners to continue their passionate exploration of the stars, galaxies, and distant worlds.
With these new ViewSpace Image Tours, visitors can take breathtaking journeys through space images that contain many exciting stories. The “Center of the Milky Way Galaxy” Tour, for example, uses breathtaking images from NASA’s Hubble, Spitzer, and Chandra X-ray telescopes and includes eleven Tour Stops, where users can interact with areas like “the Brick”—a dense, dark cloud of hydrogen molecules imaged by Spitzer. Another Tour Stop zooms toward the supermassive black hole, Sagittarius A*, offering a dramatic visual journey to the galaxy’s core.
In other tours, like the “Herbig-Haro 46/47” Tour, learners can navigate through points of interest in an observation from a single telescope mission. In this case, NASA’s James Webb Space Telescope provides the backdrop where lifelong learners can explore superheated jets of gas and dust being ejected at tremendous speeds from a pair of young, forming stars. The power of Webb turns up unexpected details in the background, like a noteworthy distant galaxy famous for its uncanny resemblance to a question mark. Each Interactive Image Tour allows people to examine unique features through videos, images, or graphical overlays to identify how those features have formed in ways that static images alone can’t convey.
These tours, which include detailed visual descriptions for each Tour Stop, illuminate the science behind the beauty, allowing learners of all ages to develop a greater understanding of and excitement for space science, deepening their engagement with astronomy, regardless of their prior experience. Check out the About the Interactives page on the ViewSpace website for a detailed overview of how to use the Image Tours.
ViewSpace currently offers three Image Tours, and the collection will continue growing:
Center of the Milky Way Galaxy:
Peer through cosmic dust and uncover areas of intense activity near the Milky Way’s core, featuring imagery from the Hubble Space Telescope, Spitzer Space Telescope, and the Chandra X-ray Observatory.
Herbig-Haro 46/47:
Witness how a tightly bound pair of young stars shapes their nebula through ejections of gas and dust in an image from the James Webb Space Telescope.
The Whirlpool Galaxy:
Explore the iconic swirling arms and glowing core of a stunning spiral galaxy, with insights into star formation, galaxy structure, and more in a Hubble Space Telescope image.
“The Image Tours are beautiful, dramatic, informational, and easy to use,” explained Sari Custer, Chief of Science and Curiosity at Arizona Science Center. “I’m excited to implement them in my museum not only because of the incredible images and user-friendly features, but also for the opportunity to excite and ignite the public’s curiosity about space.”
NASA’s Universe of Learning is supported by NASA under cooperative agreement award number NNX16AC65A 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/about-science-activation/
Select views from various Image Tours. Clockwise from top left: The Whirlpool Galaxy, Center of the Milky Way Galaxy, Herbig-Haro 46/47, detail view in the Center of the Milky Way Galaxy. Share
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Last Updated May 13, 2025 Editor NASA Science Editorial Team Related Terms
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By NASA
8 Min Read NASA Telescopes Tune Into a Black Hole Prelude, Fugue
The first sonification features WR124, an extremely bright, massive star. Here, the star is shown in a short-lived phase preceding the possible creation of a black hole. NASA released three new pieces of cosmic sound Thursday that are associated with the densest and darkest members of our universe: black holes. These scientific productions are sonifications — or translations into sound — of data collected by NASA telescopes in space including the Chandra X-ray Observatory, James Webb Space Telescope, and Imaging X-ray Polarimetry Explorer (IXPE).
This trio of sonifications represents different aspects of black holes and black hole evolution. WR124 is an extremely bright, short-lived massive star known as a Wolf-Rayet that may collapse into a black hole in the future. SS 433 is a binary, or double system, containing a star like our Sun in orbit with either a neutron star or a black hole. The galaxy Centaurus A has an enormous black hole in its center that is sending a booming jet across the entire length of the galaxy. Data from Chandra and other telescopes were translated through a process called “sonification” into sounds and notes. This new trio of sonifications represents different aspects of black holes. Black holes are neither static nor monolithic. They evolve over time, and are found in a range of sizes and environments.
WR 124
Credit: X-ray: NASA/CXC/SAO; Infrared: (Herschel) ESA/NASA/Caltech, (Spitzer) NASA/JPL/Caltech, (WISE) NASA/JPL/Caltech; Infrared: NASA/ESA/CSA/STScI/Webb ERO Production Team; Image processing: NASA/CXC/SAO/J. Major; Sonification: NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida) The first movement is a prelude to the potential birth of a black hole. WR124 is an extremely bright, short-lived massive star known as a Wolf-Rayet at a distance of about 28,000 light-years from Earth. These stars fling their outer layers out into space, creating spectacular arrangements seen in an image in infrared light from the Webb telescope. In the sonification of WR124, this nebula is heard as flutes and the background stars as bells. At the center of WR124, where the scan begins before moving outward, is a hot core of the star that may explode as a supernova and potentially collapse and leave behind a black hole in its wake. As the scan moves from the center outward, X-ray sources detected by Chandra are translated into harp sounds. Data from NASA’s James Webb Space Telescope is heard as metallic bell-like sounds, while the light of the central star is mapped to produce the descending scream-like sound at the beginning. The piece is rounded out by strings playing additional data from the infrared telescopic trio of ESA’s (European Space Agency’s) Herschel Space Telescope, NASA’s retired Spitzer Space Telescope, and NASA’s retired Wide Image Survey Explorer (WISE) as chords.
SS 433
Credit: X-ray: (IXPE): NASA/MSFC/IXPE; (Chandra): NASA/CXC/SAO; (XMM): ESA/XMM-Newton; IR: NASA/JPL/Caltech/WISE; Radio: NRAO/AUI/NSF/VLA/B. Saxton. (IR/Radio image created with data from M. Goss, et al.); Image Processing/compositing: NASA/CXC/SAO/N. Wolk & K. Arcand; Sonification: NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida) In the second movement of this black hole composition, listeners can explore a duet. SS 433 is a binary, or double, system about 18,000 light-years away that sings out in X-rays. The two members of SS 433 include a star like our Sun in orbit around a much heavier partner, either a neutron star or a black hole. This orbital dance causes undulations in X-rays that Chandra, IXPE, and ESA’s XMM-Newton telescopes are tuned into. These X-ray notes have been combined with radio and infrared data to provide a backdrop for this celestial waltz. The nebula in radio waves resembles a drifting manatee, and the scan sweeps across from right to left. Light towards the top of the image is mapped to higher-pitch sound, with radio, infrared, and X-ray light mapped to low, medium, and high pitch ranges. Bright background stars are played as water-drop sounds, and the location of the binary system is heard as a plucked sound, pulsing to match the fluctuations due to the orbital dance.
Centarus A
Credit: X-ray: (Chandra) NASA/CXC/SAO, (IXPE) NASA/MSFC; Optical: ESO; Image Processing: NASA/CXC/SAO/K. Arcand, J. Major, and J. Schmidt; Sonification: NASA/CXC/SAO/K.Arcand, SYSTEM Sounds (M. Russo, A. Santaguida) The third and final movement of the black hole-themed sonifications crescendos with a distant galaxy known as Centaurus A, about 12 million light-years away from Earth. At the center of Centaurus A is an enormous black hole that is sending a booming jet across the entire length of the galaxy. Sweeping around clockwise from the top of the image, the scan encounters Chandra’s X-rays and plays them as single-note wind chimes. X-ray light from IXPE is heard as a continuous range of frequencies, producing a wind-like sound. Visible light data from the European Southern Observatory’s MPG telescope shows the galaxy’s stars that are mapped to string instruments including foreground and background objects as plucked strings.
For more NASA sonifications and information about the project, visit https://chandra.si.edu/sound/
These sonifications were led by the Chandra X-ray Center (CXC), with support from NASA’s Marshall Space Flight Center and NASA’s Universe of Learning program, which is part of the NASA Science Activation program. The collaboration was driven by visualization scientist Kimberly Arcand (CXC), astrophysicist Matt Russo, and musician Andrew Santaguida (both of the SYSTEM Sounds project), along with consultant Christine Malec.
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science from Cambridge Massachusetts and flight operations from Burlington, Massachusetts. NASA’s Universe of Learning materials are based upon work supported by NASA under cooperative agreement award number NNX16AC65A to the Space Telescope Science Institute, working in partnership with Caltech/IPAC, Center for Astrophysics | Harvard & Smithsonian, and NASA’s Jet Propulsion Laboratory.
The agency’s IXPE is a collaboration between NASA and the Italian Space Agency with partners and science collaborators in 12 countries. The IXPE mission is led by Marshall. BAE Systems, Inc., headquartered in Falls Church, Virginia, manages spacecraft operations together with the University of Colorado’s Laboratory for Atmospheric and Space Physics in Boulder.
To learn more about NASA’s space telescopes, visit:
https://science.nasa.gov/universe
Read more from NASA’s Chandra X-ray Observatory Learn more about the Chandra X-ray Observatory and its mission here:
https://www.nasa.gov/chandra
https://chandra.si.edu
Visual Description
This release features three sonifications related to black holes, presented as soundtracks to short videos. Each sonification video features a composite image representing a different aspect of the life of a black hole. These images are visualizations of data collected by NASA telescopes. During each video, a line sweeps through the image. When the line encounters a visual element, it is translated into sound according to parameters established by visualization scientist Kimberly Arcand, astrophysicist Matt Russo, musician Andrew Santaguida, and consultant Christine Malec.
The first sonification features WR124, an extremely bright, massive star. Here, the star is shown in a short-lived phase preceding the possible creation of a black hole. At the center of the composite image is the large gleaming star in white and pale blue. The star sits at the heart of a mottled pink and gold cloud, its long diffraction spikes extending to the outer edges. Also residing in the cloud are other large gleaming stars, glowing hot-pink dots, and tiny specks of blue and white light. In this sonification, the sound activation line is an ever-expanding circle which starts in the center of the massive star and continues to grow until it exits the frame.
The second sonification features SS 433, a binary star system at the center of a supernova remnant known as the Manatee Nebula. Visually, the translucent, blobby teal nebula does, indeed, resemble a bulbous walrus or manatee, floating in a red haze packed with distant specs of light. Inside the nebula is a violet streak, a blue streak, and a large bright dot. The dot, represented by a plucking sound in the sonification, is the binary system at the heart of the nebula. In this sonification, the vertical activation line begins at our right edge of the frame, and sweeps across the image before exiting at our left.
The third and final sonification features Centaurus A, a distant galaxy with an enormous black hole emitting a long jet of high-energy particles. The black hole sits at the center of the composite image, represented by a brilliant white light. A dark, grainy, oblong cloud cuts diagonally across the black hole from our lower left toward our upper right. A large, faint, translucent blue cloud stretches from our upper left to our lower right. And the long, thin jet, also in translucent blue, extends from the black hole at the center toward the upper lefthand corner. In this sonification, the activation line rotates around the image like the hand of a clock. It begins at the twelve o’clock position, and sweeps clockwise around the image.
News Media Contact
Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
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Lane Figueroa
Marshall Space Flight Center, Huntsville, Alabama
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lane.e.figueroa@nasa.gov
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Last Updated May 08, 2025 EditorBeth RidgewayLocationMarshall Space Flight Center Related Terms
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Explore Hubble Science Hubble Space Telescope NASA’s Hubble Pinpoints… Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 7 Min Read NASA’s Hubble Pinpoints Roaming Massive Black Hole
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the collision with a star followed by an explosion detected in X-ray as well as Hubble Space Telescope visible-light observations. Credits:
Artwork: NASA, ESA, STScI, Ralf Crawford (STScI) Like a scene out of a sci-fi movie, astronomers using NASA telescopes have found “Space Jaws.”
Lurking 600 million light-years away, within the inky black depths between stars, there is an invisible monster gulping down any wayward star that plummets toward it. The sneaky black hole betrayed its presence in a newly identified tidal disruption event (TDE) where a hapless star was ripped apart and swallowed in a spectacular burst of radiation. These disruption events are powerful probes of black hole physics, revealing the conditions necessary for launching jets and winds when a black hole is in the midst of consuming a star, and are seen as bright objects by telescopes.
The new TDE, called AT2024tvd, allowed astronomers to pinpoint a wandering supermassive black hole using NASA’s Hubble Space Telescope, with similar supporting observations from NASA’s Chandra X-Ray Observatory and the NRAO Very Large Array telescope that also showed that the black hole is offset from the center of the galaxy.
The paper will be published in an upcoming issue of The Astrophysical Journal Letters.
This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 2) A wayward star gets swept up in the black hole’s intense gravitational pull; 3) The star is stretched or “spaghettified” by gravitational tidal effects; 4) The star’s remnants form a disk around the black hole; 5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy’s nucleus, where an even more massive black hole dwells. Artwork: NASA, ESA, STScI, Ralf Crawford (STScI) Surprisingly, this one million-solar-mass black hole doesn’t reside exactly in the center of the host galaxy, where supermassive black holes are typically found, and actively gobble up surrounding material. Out of approximately 100 TDE events recorded by optical sky surveys so far, this is the first time an offset TDE has been identified. The rest are associated with the central black holes of galaxies.
In fact, at the center of the host galaxy there is a different supermassive black hole weighing 100 million times the mass of the Sun. Hubble’s optical precision shows the TDE was only 2,600 light-years from the more massive black hole at the galaxy’s center. That’s just one-tenth the distance between our Sun and the Milky Way’s central supermassive black hole.
This bigger black hole spews out energy as it accretes infalling gas, and it is categorized as an active galactic nucleus. Strangely, the two supermassive black holes co-exist in the same galaxy, but are not gravitationally bound to each other as a binary pair. The smaller black hole may eventually spiral into the galaxy’s center to merge with the bigger black hole. But for now, it is too far separated to be gravitationally bound.
A TDE happens when an infalling star is stretched or “spaghettified” by a black hole’s immense gravitational tidal forces. The shredded stellar remnants are pulled into a circular orbit around the black hole. This generates shocks and outflows with high temperatures that can be seen in ultraviolet and visible light.
“AT2024tvd is the first offset TDE captured by optical sky surveys, and it opens up the entire possibility of uncovering this elusive population of wandering black holes with future sky surveys,” said lead study author Yuhan Yao of the University of California at Berkeley. “Right now, theorists haven’t given much attention to offset TDEs. “I think this discovery will motivate scientists to look for more examples of this type of event.”
This is a Hubble Space Telescope image of distant galaxy that is host to the telltale signature of a roaming supermassive black hole. Science: NASA, ESA, STScI, Yuhan Yao (UC Berkeley); Image Processing: Joseph DePasquale (STScI) A Flash in the Night
The star-snacking black hole gave itself away when several ground-based sky survey telescopes observed a flare as bright as a supernova. But unlike a supernova, astronomers know that this came from a black hole snacking on a star because the flare was very hot, and showed broad emission lines of hydrogen, helium, carbon, nitrogen, and silicon. The Zwicky Transient Facility at Caltech’s Palomar Observatory, with its 1.2-meter telescope that surveys the entire northern sky every two days, first observed the event.
“Tidal disruption events hold great promise for illuminating the presence of massive black holes that we would otherwise not be able to detect,” said Ryan Chornock, associate adjunct professor at UC Berkeley and a member of the ZTF team. “Theorists have predicted that a population of massive black holes located away from the centers of galaxies must exist, but now we can use TDEs to find them.”
The flare was seemingly offset from the center of a bright massive galaxy as cataloged by Pan-STARRS (Panoramic Survey Telescope and Rapid Response System), the Sloan Digital Sky Survey, and the DESI Legacy Imaging Survey. To better determine that it was not at the galactic center, Yao’s team used NASA’s Chandra X-ray Observatory to confirm that X-rays from the flare site were also offset.
It took the resolving power of Hubble to settle any uncertainties. Hubble’s sensitivity to ultraviolet light also allows it to pinpoint the location of the TDE, which is much bluer than the rest of the galaxy.
This is a combined Hubble Space Telescope/Chandra X-Ray Observatory image of a distant galaxy that is host to the telltale signature of a roaming supermassive black hole. Both telescopes caught a tidal disruption event (TDE) caused by the black hole eating a star. Science: NASA, ESA, STScI, Yuhan Yao (UC Berkeley); Image Processing: Joseph DePasquale (STScI) Origin Unknown
The black hole responsible for the TDE is prowling inside the bulge of the massive galaxy. The black hole only becomes apparent every few tens of thousands of years when it “burps” from capturing a star, and then it goes quiet again until its next meal comes along.
How did the black hole get off-center? Previous theoretical studies have shown that black holes can be ejected out of the centers of galaxies because of three-body interactions, where the lowest-mass member gets kicked out. This may be the case here, given the stealthy black hole’s close proximity to the central black hole. “If the black hole went through a triple interaction with two other black holes in the galaxy’s core, it can still remain bound to the galaxy, orbiting around the central region,“ said Yao.
An alternative explanation is that the black hole is the surviving remnant of a smaller galaxy that merged with the host galaxy more than 1 billion years ago. If that is the case, the black hole might eventually spiral in to merge with the central active black hole sometime in the very far future. So at present, astronomers don’t know if it’s coming or going.
Erica Hammerstein, another UC Berkeley postdoctoral researcher, scrutinized the Hubble images as part of the study, but did not find any evidence of a past galaxy merger. But she explained, “There is already good evidence that galaxy mergers enhance TDE rates, but the presence of a second black hole in AT2024tvd’s host galaxy means that at some point in this galaxy’s past, a merger must have happened.”
Specialized for different kinds of light, observatories like Hubble and Chandra work together to pinpoint and better understand fleeting events like these. Future telescopes that will also be optimized for capturing transient events like this one include the National Science Foundation’s Vera C. Rubin Observatory and NASA’s upcoming Nancy Grace Roman Space Telescope. They will provide more opportunities for follow-up Hubble observations to zero in on a transient’s exact location.
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The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
ZTF is a public-private partnership, with equal support from the ZTF Partnership and from the U.S. National Science Foundation.
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Six panel illustration of Black Hole TDE AT2024tvd
This is a six-panel illustration of a tidal disruption event around a supermassive back hole.
Black Hole TDE AT2024tvdu00a0
This is a Hubble Space Telescope image of a distant galaxy that is host to the telltale signature of a roaming supermassive black hole.
Black Hole TDE AT2024tvd (Hubble + Chandra)
This is a combined Hubble Space Telescope/Chandra X-Ray Observatory image of a distant galaxy that is host to the telltale signature of a roaming supermassive black hole.
Black Hole TDE AT2024tvd Compass Image
This is a combined Hubble Space Telescope/Chandra X-Ray Observatory image of a distant galaxy that is host to the telltale signature of a roaming supermassive black hole.
Black Hole Tidal Disruption Event
This is a video animation of a tidal disruption event (TDE), an intense flash of radiation caused by the supermassive black hole eating a star. The video begins by zooming into a galaxy located 600 million light-years away.
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Last Updated May 08, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center
Contact Media Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov
Ray Villard
Space Telescope Science Institute
Baltimore, Maryland
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Hubble Space Telescope Astrophysics Astrophysics Division Black Holes Chandra X-Ray Observatory Galaxies Goddard Space Flight Center
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