NASA

A collaboration between NASA and the Indian Space Research Organisation, NISAR will use synthetic aperture radar to monitor nearly all the planet’s land- and ice-covered surfaces twice every 12 days.Credit: NASA/JPL-Caltech NASA will provide live coverage of launch activities for NISAR (NASA-ISRO Synthetic Aperture Radar), which is set to lift off at 8:10 a.m. EDT (5:40 p.m. IST), Wednesday, July 30, from Satish Dhawan Space Centre on India’s southeastern coast. A collaboration between NASA and the Indian Space Research Organisation (ISRO), the first-of-its-kind satellite will lift off aboard an ISRO Geosynchronous Satellite Launch Vehicle on a mission to scan nearly all the Earth’s land and ice surfaces twice every 12 days. Watch live coverage of the launch on NASA+ and the agency’s YouTube channel. Learn how to watch NASA content through a variety of platforms, including social media. With its two radar instruments — an S-band system provided by ISRO and an L-band system provided by NASA — the NISAR mission will provide high-resolution data to help decision-makers, communities, and scientists monitor major infrastructure, agricultural fields, and movement of land and ice surfaces. Hailed as a critical part of a pioneering year for United States – India civil space cooperation by President Trump and Prime Minister Modi during their visit in Washington in February, the NISAR launch will advance U.S. – India cooperation and benefit the U.S. in areas such as agriculture and preparation and response to disasters like hurricanes, floods, and volcanic eruptions. NASA’s mission coverage is as follows (all times Eastern and subject to change based on real-time operations): Monday, July 28 12 p.m. – Prelaunch teleconference with the following participants: Karen St. Germain, director of Earth science, NASA Headquarters Gerald Bawden, NISAR program scientist, NASA Headquarters Shanna McClain, Disasters program manager, NASA Headquarters Phil Barela, NISAR project manager, NASA Jet Propulsion Laboratory (JPL) Marco Lavalle, NISAR deputy project scientist, NASA JPL The teleconference will stream on JPL’s YouTube Channel. Members of the media may ask questions via phone during the teleconference. To register, media must provide their name and affiliation by 4 p.m. on Sunday, July 27, to Rexana Vizza at: rexana.v.vizza@jpl.nasa.gov. Questions may also be asked via social media with the hashtag #AskNISAR. Wednesday, July 30 7 a.m. – Launch coverage begins on NASA+ and YouTube. The launch broadcast begins from NASA’s Jet Propulsion Laboratory in Southern California, where the U.S. portion of the mission is managed. Follow launch events on NASA’s NISAR blog. Watch, Engage on Social Media You can also stay connected by following and tagging these accounts: X: @NASA, @NASAEarth, @NASAJPL Facebook: NASA, NASA Earth, NASA JPL Instagram: @NASA, @NASAEarth, @NASAJPL Additional Resources The NISAR press kit features deeper dives into the mission as well as its science and technology. Explore NISAR videos as well as NISAR animations and b-roll media reel. The NISAR mission is the first joint satellite mission between NASA and ISRO, marking a new chapter in the growing collaboration between the two space agencies. The launch of NISAR, years in the making, builds on a strong heritage of successful programs, including Chandrayaan-1 and the recent Axiom Mission-4, which saw ISRO and NASA astronauts living and working together aboard the International Space Station for the first time. Learn more about the mission at: https://science.nasa.gov/mission/nisar -end- Elizabeth Vlock / Karen Fox Headquarters, Washington 202-358-1600 elizabeth.a.vlock@nasa.gov / karen.c.fox@nasa.gov Andrew Wang / Jane J. Lee Jet Propulsion Laboratory, Pasadena, Calif. 626-379-6874 / 818-354-0307 andrew.wang@jpl.nasa.gov / jane.j.lee@jpl.nasa.gov Share Details Last Updated Jul 23, 2025 LocationNASA Headquarters Related TermsNISAR (NASA-ISRO Synthetic Aperture Radar)Earth Science DivisionJet Propulsion LaboratoryScience Mission Directorate View the full article

4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) An image of Betelgeuse, the yellow-red star, and the signature of its close companion, the faint blue object.Data: NASA/JPL/NOIRlab. Visualization: NOIRLAB. A century-old hypothesis that Betelgeuse, the 10th brightest star in our night sky, is orbited by a very close companion star was proved true by a team of astrophysicists led by a scientist at NASA’s Ames Research Center in California’s Silicon Valley. The research published in The Astrophysical Journal Letters in the paper “Probable Direct Imaging Discovery of the Stellar Companion to Betelgeuse.” Fluctuations in the brightness and measured velocity of Betelgeuse, the closest red supergiant star to Earth, had long presented clues that it may have a partner, but the bigger star’s intense glow made direct observations of any fainter neighbors nearly impossible. Two recent studies by other teams of astronomers reignited the companion star hypothesis by using more than 100 years of Betelgeuse observations to provide predictions of the companion’s location and brightness. If the smaller star did exist, the location predictions suggested that scientists had a window of just a few months to observe the companion star at its widest separation from Betelgeuse, as it orbited near the visible edge of the supergiant. After that, they would have to wait another three years for it to orbit to the other side and again leave the overpowering glow of its larger companion. Searches for the companion were initially made using space-based telescopes, because observing through Earth’s atmosphere can blur images of astronomical objects. But these efforts did not detect the companion. Steve Howell, a senior research scientist at Ames, recognized the ground-based Gemini North telescope in Hawai’i, one of the largest in the world, paired with a special, high-resolution camera built by NASA, had the potential to directly observe the close companion to Betelgeuse, despite the atmospheric blurring. Officially called the ‘Alopeke speckle instrument, the advanced imaging camera let them obtain many thousands of short exposures to measure the atmospheric interference in their data and remove it with detailed image processing, providing an image of Betelgeuse and its companion. Howell’s team detected the very faint companion star right where it was predicted to be, orbiting very close to the outer edge of Betelgeuse. “I hope our discovery excites other astrophysicists about the robust power of ground-based telescopes and speckle imagers – a key to opening new observational windows,” said Howell. “This can help unlock the great mysteries in our universe.” To start, this discovery of a close companion to Betelgeuse may explain why other similar red supergiant stars undergo periodic changes in their brightness on the scale of many years. Howell plans to continue observations of Betelgeuse’s stellar companion to better understand its nature. The companion star will again return to its greatest separation from Betelgeuse in November 2027, a time when it will be easiest to detect. Having found the long-anticipated companion star, Howell turned to giving it a name. The traditional star name “Betelgeuse” derives from Arabic, meaning “the hand of al-Jawza’,” a female figure in old Arabian legend. Fittingly, Howell’s team named the orbiting companion “Siwarha,” meaning “her bracelet.” Photo of the constellation Orion, showing the location of Betelgeuse – and its newfound companion star.NOIRLab/Eckhard Slawik The NASA–National Science Foundation Exoplanet Observational Research Program (NN-EXPLORE) is a joint initiative to advance U.S. exoplanet science by providing the community with access to cutting-edge, ground-based observational facilities. Managed by NASA’s Exoplanet Exploration Program, NN-EXPLORE supports and enhances the scientific return of space missions such as Kepler, TESS (Transiting Exoplanet Survey Satellite), Hubble Space Telescope, and James Webb Space Telescope by enabling essential follow-up observations from the ground—creating strong synergies between space-based discoveries and ground-based characterization. NASA’s Exoplanet Exploration Program is located at the agency’s Jet Propulsion Laboratory. To learn more about NN-EXPLORE, visit: https://exoplanets.nasa.gov/exep/NNExplore/overview Share Details Last Updated Jul 23, 2025 Related TermsAstrophysicsAmes Research CenterAmes Research Center's Science DirectorateAstrophysics DivisionExoplanet Exploration ProgramGeneralScience & ResearchScience Mission Directorate Explore More 4 min read NASA Tests 5G-Based Aviation Network to Boost Air Taxi Connectivity Article 1 hour ago 3 min read NASA Tests Mixed Reality Pilot Simulation in Vertical Motion Simulator Article 3 hours ago 2 min read Radio JOVE Volunteers Tune In to the Sun’s Low Notes As the Sun approaches the most active part of its eleven-year magnetic cycle this summer,… Article 5 hours ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

4 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA researcher Darren Nash monitors experimental communications equipment on NASA’s Pilatus PC-12 during a flight test over NASA’s Glenn Research Center in Cleveland on April 17, 2025.NASA/Sara Lowthian-Hanna NASA engineers are exploring how the technology used in existing cellphone networks could support the next generation of aviation. In April and May, researchers at NASA’s Glenn Research Center in Cleveland built two specialized radio systems to study how well fifth-generation cellular network technology, known as 5G, can handle the demands of air taxi communications. “The goal of this research is to understand how wireless cellphone networks could be leveraged by the aviation industry to enable new frontiers of aviation operations,” said Casey Bakula, lead researcher for the project, who is based at Glenn. “The findings of this work could serve as a blueprint for future aviation communication network providers, like satellite navigation providers and telecommunications companies, and help guide the Federal Aviation Administration’s plan for future advanced air mobility network requirements in cities.” Instead of developing entirely new standards for air taxi communications, NASA is looking to see if the aviation industry could leverage the expertise, experience, and investments made by the cellular industry towards the development of reliable, secure, and scalable aviation networks. If 5G networks could provide an “80% solution” to the challenge, researchers can focus on identifying the remaining 20% that would need to be adapted to meet the needs of the air taxi industry. NASA researchers Darren Nash, left, and Brian Kachmar review signal data captured from experimental communications equipment onboard NASA’s Pilatus PC-12 on April 17, 2025.NASA/Sara Lowthian-Hanna 5G networks can manage a lot of data at once and have very low signal transmission delay compared to satellite systems, which could make them ideal for providing location data between aircraft in busy city skies. Ground antennas and networks in cities can help air taxis stay connected as they fly over buildings, making urban flights safer. To conduct their tests, NASA researchers set up a system that meets current 5G standards and would allow for future improvements in performance. They placed one radio in the agency’s Pilatus PC-12 aircraft and set up another radio on the roof of Glenn’s Aerospace Communications Facility building. With an experimental license from the Federal Aviation Administration (FAA) to conduct flights, the team tested signal transmissions using a radio frequency band the Federal Communications Commission dedicated for the safe testing of drones and other uncrewed aircraft systems. During testing, NASA’s PC-12 flew various flight patterns near Glenn. The team used some of the flight patterns to measure how the signal could weaken as the aircraft moved away from the ground station. Other patterns focused on identifying areas where nearby buildings might block signals, potentially causing interference or dead zones. The team also studied how the aircraft’s angle and position relative to the ground station affected the quality of the connection. These initial tests provided the NASA team an opportunity to integrate its new C-Band radio testbed onto the aircraft, verify its basic functionality, and the operation of the corresponding ground station, as well as refine the team’s test procedures. The successful completion of these activities allows the team to begin research on how 5G standards and technologies could be utilized in existing aviation bands to provide air-to-ground and aircraft-to-aircraft communications services. Experimental communications equipment is secure and ready for flight test evaluation in the back of NASA’s Pilatus PC-12 at NASA’s Glenn Research Center in Cleveland on April 17, 2025. NASA/Sara Lowthian-Hanna In addition to meeting these initial test objectives, the team also recorded and verified the presence of propeller modulation. This is a form of signal degradation caused by the propeller blades of the aircraft partially blocking radio signals as they rotate. The effect becomes more significant as aircraft fly at the lower altitudes air taxis are expected to operate. The airframe configuration and number of propellers on some of the new air taxi models may cause increased propeller modulation effects, so NASA researchers will study this further. NASA research will provide baseline performance data that the agency will share with the FAA and the advanced air mobility sector of the aviation industry, which explores new air transportation options. Future research looking into cellular network usage will focus on issues such as maximum data speeds, signal-to-noise ratios, and synchronization between aircraft and ground systems. Researchers will be able to use NASA’s baseline data to measure the potential of new changes or features to communications systems. Future aircraft will need to carry essential communications systems for command and control, passenger safety, and coordination with other aircraft to avoid collisions. Reliable wireless networks offer the possibility for safe operations of air taxis, particular in cities and other crowded areas. This work is led by NASAs Air Mobility Pathfinders project under the Airspace Operations and Safety Program in support of NASA’s Advanced Air Mobility mission. NASA Pilot Mark Russell emerges from NASA’s Pilatus PC-12 after mobile communication tests at NASA’s Glenn Research Center in Cleveland on April 17, 2025. NASA/Sara Lowthian-Hanna Share Details Last Updated Jul 23, 2025 Related TermsArmstrong Flight Research CenterAeronauticsAir Mobility Pathfinders projectAir Traffic SolutionsAirspace Operations and Safety ProgramAmes Research CenterDrones & YouGlenn Research CenterLangley Research CenterNASA Aircraft Explore More 3 min read NASA Tests Mixed Reality Pilot Simulation in Vertical Motion Simulator Article 2 hours ago 4 min read GRUVE Lab The GRUVE (Glenn Reconfigurable User-Interface and Virtual Reality Exploration) Lab is located within the GVIS… Article 5 hours ago 4 min read GVIS History As part of NASA Glenn’s Scientific Computing and Visualization Team, the GVIS Lab has a… Article 5 hours ago Keep Exploring Discover More Topics From NASA Missions Humans in Space Climate Change Solar System View the full article

Damian Hischier of the National Test Pilot School in Mojave, California, takes part in testing of a virtual reality-infused pilot simulation in the Vertical Motion Simulator (VMS) at NASA’s Ames Research Center in California’s Silicon Valley on May 30, 2025. NASA/Brandon Torres-Navarrete Commercial companies and government agencies are increasingly pursuing a more immersive and affordable alternative to conventional displays currently used in flight simulators. A NASA research project is working on ways to make this technology available for use faster. Mixed reality systems where users interact with physical simulators while wearing virtual reality headsets offer a promising path forward for pilot training. But currently, only limited standards exist for allowing their use, as regulators have little to no data on how these systems perform. To address this, NASA’s Ames Research Center in California’s Silicon Valley invited a dozen pilots to participate in a study to test how a mixed-reality flight simulation would perform in the world’s largest flight simulator. “For the first time, we’re collecting real data on how this type of mixed reality simulation performs in the highest-fidelity vertical motion simulator,” said Peter Zaal, a principal systems architect at Ames. “The more we understand about how these systems affect pilot performance, the closer we are to providing a safer, cost-effective training tool to the aviation community that could benefit everyone from commercial airlines to future air taxi operators.” A National Test Pilot student observes the mixed-reality pilot simulation in the VMS at Ames on May 30, 2025.NASA/Brandon Torres-Navarrete Mixed reality blends physical and digital worlds, allowing users to see physical items while viewing a desired simulated environment. Flight simulators employing this technology through headset or a similar setup could offer pilots training for operating next-generation aircraft at a reduced cost and within a smaller footprint compared to more traditional flight simulators. This is because pilots could rely more heavily on the visuals provided through the headset instead of large embedded visual displays in a physical motion simulator. During the testing – which ran May 23-30 – pilots donned a headset through which they could see the physical displays and control sticks inside the Vertical Motion Simulator (VMS) cab along with a virtual cockpit overlay of an electric vertical take-off and landing vehicle through the head-mounted display. When the pilots looked toward their windscreens, they saw a virtual view of San Francisco and the surrounding area. Pilots performed three typical flight maneuvers under four sets of motion conditions. Afterward, they were asked to provide feedback on their level of motion sickness while using the head-mounted display and how well the simulator replicated the same movements the aircraft would make during a real flight. An initial analysis of the study shows pilots reported lower ratings of motion sickness than NASA researchers expected. Many shared that the mixed-reality setup inside the VMS felt more realistic and fluid than previous simulator setups they had tested. As part of the test, Ames hosted members of the Federal Aviation Administration Civil Aerospace Medical Institute, which studies factors that influence human performance in aerospace. Pilots from the National Test Pilot School attended a portion of the testing and, independent from the study, evaluated the head-mounted display’s “usable cue environment,” or representation of the visual cues pilots rely on to control an aircraft. Peter Zaal (left), observes as Samuel Ortho (middle) speaks with a National Test Pilot student during the mixed reality pilot simulation in the Vertical Motion Simulator at Ames on May 30, 2025. NASA will make the test results available to the public and the aviation community early next year. This first-of-its-kind testing – funded by an Ames Innovation Fair Grant and managed by the center’s Aviation Systems Division – paves the way for potential use of this technology in the VMS for future aviation and space missions. View the full article

JAXA (Japan Aerospace Exploration Agency)/Takuya Onishi In this photo from June 28, 2025, Expedition 73 flight engineer Jonny Kim and former NASA astronaut and director of human spaceflight at Axiom Space Peggy Whitson work together inside the International Space Station’s Destiny laboratory module setting up hardware for cancer research. The hardware is used to culture patient-derived cancer cells, model their growth in microgravity, and test a state-of-the-art fluorescence microscope. Results of this study may lead to earlier cancer detection methods, development of advanced cancer treatments, and promote future stem cell research in space. Whitson returned to Earth on July 15, 2025, with fellow Axiom Mission 4 crew members ISRO (Indian Space Research Organisation) astronaut Shubhanshu Shukla, ESA (European Space Agency) project astronaut Sławosz Uznański-Wiśniewski of Poland, and Hungarian to Orbit (HUNOR) astronaut Tibor Kapu of Hungary. They completed about two and a half weeks in space. Image credit: JAXA (Japan Aerospace Exploration Agency)/Takuya Onishi View the full article

As the Sun approaches the most active part of its eleven-year magnetic cycle this summer, NASA volunteers have been watching it closely. Now they’ve spotted a new trend in solar behavior that will have you reaching for your suntan lotion. It’s all about something called a “Type II” solar radio burst: “Type II solar radio bursts are not commonly detected in the frequency range between 15 to 30 megahertz,” said Prof. Chuck Higgins, Co-founder of Radio JOVE. “Recently, we’re seeing many of them in that range.” Let’s unpack that. Our Sun often sprays powerful blasts of radio waves into space. Heliophysicists classify these radio bursts into five different types depending on how the frequency of the radio waves drifts over time. “Type II” solar radio bursts seem to come from solar flares and enormous squirts of hot plasma called coronal mass ejections. Now, Thomas Freeman, an undergraduate student at Middle Tennessee State University, and other volunteers working on NASA’s Radio JOVE project have observed something interesting about these Type II bursts: they are now showing up at lower frequencies—somewhere in between FM and AM radio. What does it mean? It means our star is full of surprises! These Radio JOVE observations of the Sun’s radio emissions during solar maximum can be used to extend our knowledge of solar emissions to lower frequencies and, therefore, to distances farther from the Sun. Radio JOVE is a NASA partner citizen science project in which participants assemble and operate radio astronomy telescopes to gather and contribute data to support scientific studies. Radio JOVE collaborated with SunRISE Ground Radio Lab, organized teams of high school students to observe the Sun, and recently published a paper on these Type II solar radio bursts. Learn more and get involved! A Type II solar radio burst on April 23rd, 2024, seen as the gently sloping yellow band drifting from 17:49 to 18:02 UTC in the 15-30 MHz radio frequency-time spectrogram. Credit: Tom Ashcraft, Lamy, NM Share Details Last Updated Jul 23, 2025 Related Terms Citizen Science Heliophysics Explore More 2 min read Bring NASA Science into Your Library! Article 2 days ago 4 min read NASA to Launch SNIFS, Sun’s Next Trailblazing Spectator July will see the launch of the groundbreaking Solar EruptioN Integral Field Spectrograph mission, or… Article 6 days ago 6 min read NASA’s TRACERS Studies Explosive Process in Earth’s Magnetic Shield Article 7 days ago View the full article

The Moon photographed from the International Space Station, pictured in between exterior International Space Station hardware (Credit: NASA). NASA is seeking proposals from U.S. companies about innovative Moon and Mars proximity relay communication and navigation capabilities as the agency aims to use private industry satellite communications services for emerging missions. On July 7, NASA issued a Request for Proposals, soliciting advanced industry concepts to establish high-bandwidth, high-reliability communications infrastructure between the lunar surface and an Earth-based operations control center, along with concepts that establish a critical communications relay on the Martian surface and transfer data between Mars and the Earth. “These partnerships foster important advancements in communications and navigation,” said Greg Heckler, deputy program manager for capability development within NASA’s SCaN (Space Communications and Navigation) Program. “It allows our astronauts, our rovers, our spacecraft – all NASA missions – to expand humanity’s exploration of the Moon, Mars, and beyond.” NASA’s request directly supports the agency’s long-term vision of an interoperable space communication and navigation infrastructure that enables science, exploration, and economic development in space. NASA, as one of many customers, will establish a marketplace that supports cost-effective commercial services involving communication needs on and around the Moon and Mars. Responses are due by 5 p.m. EDT, Wednesday, Aug. 13. NASA’s SCaN Program serves as the management office for the agency’s space communications and navigation. More than 100 NASA and non-NASA missions rely on SCaN’s two networks, the Near Space Network and the Deep Space Network, to support astronauts aboard the International Space Station and future Artemis missions, monitor Earth’s weather, support lunar exploration, and uncover the solar system and beyond. Learn more about NASA’s SCaN Program at: https://www.nasa.gov/scan News Media Contact: Claire O’Shea Headquarters, Washington 202-358-1100 claire.a.o’shea@nasa.gov View the full article

4 Min Read GRUVE Lab The CAVE in the GRUVE Lab is capable of running highly immersive VR experiences through powerful projectors, mirrors, an infrared motion tracking system, and active-shutter glasses. Credits: NASA About The GRUVE (Glenn Reconfigurable User-Interface and Virtual Reality Exploration) Lab is located within the GVIS Lab. It is home to the CAVE, which is predominantly used for mission scenarios and to tour virtual environments of NASA facilities. GRUVE Lab VisualizationUsers virtually explore a facility at NASA’s Glenn Research Center in Cleveland.NASA GRUVE Lab DemonstrationA user analyzes a visualization of a prototype structure.NASA GRUVE Lab VisualizationA user analyzes a visualization of a prototype structure that will be used for a fire experiment on the Moon.NASA GRUVE Lab VisualizationA Graphics and Visualization Lab (GVIS) intern in the Cave Automatic Virtual Environment (CAVE).NASA GRUVE Lab TourA user takes a virtual tour of a facility at NASA’s Glenn Research Center in Cleveland.NASA How GRUVE Works GRUVE allows multiple people to view a visualization in 3D together. These visualizations include 3D models of NASA facilities and intricate images created from collected data. Powerful projectors and mirrors, in combination with an infrared motion tracking system and active-shutter glasses, allow viewers to view 3D models and data in perfect perspective. 3D models effectively pop off the screen and remain proportional no matter where the user with the pair of tracking glasses moves in the environment. The CAVE can be driven by either a Windows or Linux computer system, enabling the team to use the best environment for a given problem and software tool. The CAVE setup immerses the user in 3D visualizations through walls on all sides, projectors from above, tracking cameras, and mirrors hidden behind the facade.Visbox, Inc. Benefits of GRUVE The CAVE’s technology provides a unique advantage for researchers, scientists, engineers, and others. Seeing and analyzing forces and data that would otherwise not be viewable to the human eye allows the observer to understand their subject matter in more detail. Benefits of GRUVE to research include: Providing an immersive environment: with large screens to fill peripheral vision and stereoscopic projection for a real sense of three-dimensional space, more parts of the brain are engaged, and the user is better able to understand problems and solve them faster More effective collaboration: the ability to see each other in the virtual reality environment makes GRUVE better for collaboration than traditional VR technology Seeing complex data and flows in 3D: this makes it easier for both experts and non-experts to understand the data Providing greater resolution and larger display size: this allows details to be displayed without losing their context Delivering faster and more accurate manipulation and viewing of models, including CAD data, with fewer errors: this results in a faster time to market and less re-work All members of NASA Glenn may use GRUVE for their projects. Applications of Immersive 3D Environments Fluid dynamics analysis (CFD) Point cloud data, e.g., LiDAR Virtual design reviews Virtual manufacturing testing Computer Aided Design (CAD) 3D imaging data Training and education Virtual procedures Biomedical research Molecular dynamics Virtual building walkthroughs Showroom “theater” Education and outreach Building Information Management (BIM) Big data and data mining Cybersecurity data analysis Safety systems analysis Microfocus CT scan data Electron microscopy 3D photos and videos Data Types Supported Point cloud data Volume data Computational fluid dynamics (CFD) Computer Aided Design (CAD) Molecular dynamics GRUVE Hardware Linux CAVE node Windows 10 CAVE node CAVE wall Stereo glasses Audio system Tracking system Wand Software Available in the GRUVE Lab The Windows node attached to the GRUVE Lab runs middleware software, which enables Unity-developed applications to run in the CAVE. This greatly expands the number of VR applications that can be run. Vrui VR Toolkit-based applications such as LiDAR viewer and 3D visualizer VMD – Visual Molecular Dynamics ParaView COVISE– Collaborative Visualization and Simulation Environment Other Visualization Devices The GVIS Lab maintains a large collection of computing, visualization, and user interaction devices including: Virtual reality display devices Head-mounted displays Room-scale CAVE Augmented reality head-mounted displays 3D displays Psuedo-3D displays Pepper’s Ghost display Persistence of Vision (POV) LED display Light field technology- based displays Projection devices for projected AR Natural user interface devices Hand gesture recognition devices Motion capture devices Cameras for mixed reality Computing hardware High-end laptops High-end desktops High-end tablets and smartphones Cameras Stereo 3D camera 180/360 camera Flight simulators 3D printers All these devices are available for employees to try and test for possible application to their work. A Graphics and Visualization Lab (GVIS) intern in the Cave Automatic Virtual Environment (CAVE).NASA Contact Us Need to reach us? You can send an email directly to the GVIS Team (GRC-DL-GVIS@mail.nasa.gov) or to the team leader, Herb Schilling (hschilling@nasa.gov). Share Details Last Updated Jul 23, 2025 LocationGlenn Research Center Related TermsGlenn Research CenterNASA Centers & Facilities Explore More 5 min read NASA Advances Pressure Sensitive Paint Research Capability Article 3 weeks ago 1 min read Gateway Space Station in 3D Article 11 months ago 5 min read Augmented Reality Speeds Spacecraft Construction at NASA Goddard Article 1 year ago Keep Exploring Discover More Topics From NASA Want to Go on a Simulated Mission to the Moon? Aeronautics STEM Glenn University Student Design Challenges NASA at Home: Virtual Tours and Apps View the full article

4 Min Read GVIS History As part of NASA Glenn’s Scientific Computing and Visualization Team, the GVIS Lab has a storied visual and technological history. Credits: NASA GVIS: the ICARE Era In 1982, a $20 million supercomputer was brought to NASA Glenn. Scientists at NASA Glenn were becoming increasingly reliant on computer simulations to test their experiments. Advancements in computer technology allowed a different type of testing environment — one that revolved around virtual models and data over physical observation. The benefits of this method included a decrease in costs, a decrease in associated risk, faster turnaround, and more data. High Definition Video System (HDVS)A High Definition Video System (HDVS) in the early Graphics and Visualization Lab (GVIS). NASA High Definition Video System (HDVS) in the LabNASA employee in early Graphics and Visualization Lab (GVIS) setup, containing High Definition Video Systems (HDVS). NASA Early Graphics and Visualization Lab (GVIS)Early Graphics and Visualization Lab (GVIS) setup, which housed original analog processing hardware. NASA Cray 1-S/2200 SupercomputerThe original Cray 1-S/2200 Supercomputer in the Research and Analysis Center in 1982.NASA But this method of experimentation created a problem: With data-point counts somewhere in the millions, it was a challenge for scientists to even begin to look at their own collected data. In short, there was simply too much data to be analyzed. To solve this problem, NASA Glenn built the Interactive Computer Aided Research Engineering system (ICARE) in the center’s Research Analysis Center. Taking up several rooms, consisting of 22 total workstations, and costing a grand total of $20 million, the ICARE system was a way for scientists to examine their data through the aid of supercomputer visualizations. Using both graphical and modular methods, ICARE’s visualizations revealed and shared information in ways that traditional methods could not match. The construction and implementation of the ICARE system was revolutionary to both the center and NASA as a whole. Before 1982, NASA already had an established interest in powerful computers; however, the ICARE system took NASA into the era of supercomputing. ICARE also brought increased attention to the value and power of scientific visualization. Original Processing HardwareOriginal analog Graphics and Visualization Lab (GVIS) processing hardware.NASA ICARE RoomAn ICARE room in the Research and Analysis Center. NASA 1980s VisualizationA typical 1980s visualization at NASA’s Glenn Research Center in Cleveland.NASA GRAPH3DGRAPH3D was an innovative technology in the 1980s that supported shaded surfaces and had a rich set of user-friendly commands.NASA The Creation of GVIS In 1989, it was time for an upgrade. NASA Glenn wanted the latest scientific visualization technology and techniques for its scientists, so the center expanded the Research Analysis Center to make room for the new Graphics and Visualization Lab (GVIS). The GVIS Lab acquired cutting-edge graphics technology, including studio-quality TV animation and recording equipment, stereographic displays, and image processing systems. Later, the High-Performance Computing Act of 1991 provided funding and opportunities to add high-speed computing, virtual reality, and collaborative visualization to its fleet of tools. The secure supercomputing space that would eventually become the Graphics and Visualization Lab (GVIS), shown in 1989.NASA During this period, the GVIS Lab was responsible for assisting NASA Glenn scientists who needed help visualizing their data. The lab was also tasked with inventing new visualization techniques and promoting NASA Glenn’s activities though tours, videos, and other outreach programs. Some of the techniques the lab developed included particle tracking, iso-surface contours, and volume visualization. Tour guests included school children, corporate VIPs, local and national politicians, TV news media, and researchers from other national labs. Using state-of-the-art recording and editing hardware, the GVIS Lab regularly shared work both inside and outside of NASA. As other labs and researchers began to gain access to their own scientific visualization tools, the GVIS Lab shifted its focus to experimenting with virtual reality- and augmented reality-based visualizations. Jay HorowitzJay Horowitz saw the Graphics and Visualization Lab (GVIS) through its creation and early years at NASA’s Glenn Research Center in Cleveland. NASA Cray X-MP-2 SupercomputerThe Cray X-MP-2 Supercomputer that replaced the 1-S. NASA Early Research and Analysis CenterThe Research and Analysis Center pre-expansion. NASA Research and Analysis CenterThe Research and Analysis Center after the expansion. The Graphics and Visualization Lab (GVIS) is in the upper left corner. NASA Lewis Advanced Cluster Environment (LACE)The Advanced Computational Concepts Lab’s (ACCL) Lewis Advanced Cluster Environment (LACE) in 1993. NASA Mobile Aeronautics Education Laboratory (MAEL) VR Flight SimulatorSetup showing location of the various equipment used in the Mobile Aeronautics Education Laboratory (MAEL) VR Flight Simulator.NASA Mobile Aeronautics Education Laboratory (MAEL) VR Flight SimulatorMAEL (Mobile Aeronautics Education Laboratory) trailer’s flight simulator supported multi-screen panoramic views or head-tracked Head Mounted Displays (HMDs). NASA WrightSimApollo 13 flight director Gene Kranz watches Jim Lovell pilot WrightSim. NASA 100 Years of Flight Gala CelebrationJohn Glenn talks to a Graphics and Visualization Lab (GVIS) programmer during the 2003 “100 Years of Flight Gala Celebration” event at NASA’s Glenn Research Center in Cleveland. NASA VR TreadmillThe concept of the VR treadmill was used to test if duplicating a visual-motor linkage was feasible for long-duration spaceflight. NASA 2000s VisualizationTurn-of-the-century Graphics and Visualization Lab (GVIS) model. NASA 2000s VisualizationTurn-of-the-century Graphics and Visualization Lab (GVIS) model. NASA 2000s Visualization Turn-of-the-century Graphics and Visualization Lab (GVIS) model. NASA Aeroshark ClusterThe Advanced Computational Concepts Lab’s (ACCL) Aeroshark Cluster in 2001. NASA Early 2000s Graphics and Visualization Lab (GVIS)The turn-of-the-century Graphics and Visualization Lab (GVIS), shown in 2004. NASA Advanced Communications Environment (ACE) ClusterThe Advanced Computational Concepts Lab’s (ACCL) Advanced Communications Environment (ACE) Cluster in 2005. NASA Early Computer Automatic Virtual Environment (CAVE)A Graphics and Visualization Lab (GVIS) team member demonstrating the old Computer Automatic Virtual Environment (CAVE). NASA Current Computer Automatic Virtual Environment (CAVE)A Graphics and Visualization Lab (GVIS) intern in the Computer Automatic Virtual Environment (CAVE). NASA GVIS Now Today, the GVIS Lab has the same mission that it had in 1989: to apply the latest visualization and human interaction technologies to advance NASA’s missions. The team takes pride in pushing the limits of scientific visualization and computer science, helping fellow researchers make sense of their data, and inspiring the next generation through demonstrations and presentations. Computational technology has come a long way since the days of ICARE, but GVIS has continued to explore current and cutting-edge technologies. In addition to scientific visualization and experimental computational technologies, the GVIS Lab now also specializes in virtual design, interactive 3D simulations, natural user interface development, applications of computer science, and mission scenario visualizations. The team uses the latest edition of 3D programs and VR devices to experiment with how these systems can be used to visualize data, pushing their input and output capabilities. With all this technology, GVIS also supports the visualization of a wide variety of 3D data and models such as CAD, point clouds, and volume data. Additionally, the lab is capable of high-impact data visualization, web-based visualization, time-accurate data representation, and designing and testing CAD models in virtual reality. The Graphics and Visualization Lab (GVIS) team attends a STEM outreach event at the Cleveland Museum of Natural History.NASA Public Engagement Outside of the lab, GVIS has a longstanding history of taking its technology demonstrations across the city, throughout the country, and around the world. The team has extensive experience organizing, presenting, and facilitating STEM-based educational outreach for a variety of different events and venues. Inside the lab, GVIS supports the education and career exploration of its high school and college interns through mentorship, community engagement opportunities, and access to cutting-edge technology. STEM Engagement EventVisitors interact with the Graphics and Visualization Lab (GVIS) team while attending Score with STEM, an event organized by the Cleveland Cavaliers. NASA/GRC/Jef Janis STEM Engagement EventA visitor interacts with a Graphics and Visualization Lab (GVIS) team member while attending Dino Days at the Cleveland Museum of Natural History. NASA STEM Engagement EventA Graphics and Visualization Lab (GVIS) Intern interacts with visitors at a STEM outreach event. NASA STEM Engagement EventGraphics and Visualization Lab (GVIS) team members attend Women in Aviation Day organized by Women in Aviation International (WAI). NASA GRUVE Lab ToursThe Graphics and Visualization Lab (GVIS) team provides tours of NASA labs and facilities. NASA GVIS Lab ToursA Graphics and Visualization Lab (GVIS) team member demonstrates VR visualizations. NASA GRUVE Lab ToursVisitors interact with a visualization through the CAVE environment at the Graphics and Visualization Lab (GVIS). NASA Contact Us Need to reach us? You can send an email directly to the GVIS Team (GRC-DL-GVIS@mail.nasa.gov) or to the team leader, Herb Schilling (hschilling@nasa.gov). Share Details Last Updated Jul 23, 2025 Related TermsGlenn Research CenterNASA Centers & Facilities Explore More 3 min read 1942: Engine Roars to Life in First Test at Future NASA Glenn Article 1 year ago 2 min read NASA Glenn History Includes Contributions of Women in Aerospace Research Article 3 years ago 3 min read NASA Uses Cleveland Landmark for Microgravity Research in the 1960s Article 3 years ago Keep Exploring Discover More Topics From NASA Explore NASA’s History Glenn Historic Facilities This collection of webpages was created to document some of the historic facilities formerly located at NASA's Glenn Research Center… Glenn Historic Preservation NASA History Series View the full article

When a reservoir conduit cannot be closed, thousands of cubic feet of water can roar through uncontrolled, threatening public safety, irreplaceable reservoir storage, and power generation. Seal Team Fix invites engineers, fabricators, and creative problem-solvers to stop that torrent in its tracks. Your mission: design a rapid-deploying, temporary seal that can be deployed to a submerged 3- to 25-ft diameter conduit opening, accommodate differential pressure, and achieve a 95–98 % flow reduction – without leaning on trash racks or other non-structural surfaces. The competition unfolds in three phases: a short-format concept white paper, a funded prototype build, and a lab-scale hydraulic demonstration. Award: $575,000 in total prizes Open Date: July 22, 2025 Close Date: October 14, 2025 For more information, visit: https://www.herox.com/SealTeamFix View the full article

4 min read NASA, JAXA XRISM Satellite X-rays Milky Way’s Sulfur An international team of scientists have provided an unprecedented tally of elemental sulfur spread between the stars using data from the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft. Astronomers used X-rays from two binary star systems to detect sulfur in the interstellar medium, the gas and dust found in the space between stars. It’s the first direct measurement of both sulfur’s gas and solid phases, a unique capability of X-ray spectroscopy, XRISM’s (pronounced “crism”) primary method of studying the cosmos. “Sulfur is important for how cells function in our bodies here on Earth, but we still have a lot of questions about where it’s found out in the universe,” said Lía Corrales, an assistant professor of astronomy at the University of Michigan in Ann Arbor. “Sulfur can easily change from a gas to a solid and back again. The XRISM spacecraft provides the resolution and sensitivity we need to find it in both forms and learn more about where it might be hiding.” A paper about these results, led by Corrales, published June 27 in the Publications of the Astronomical Society of Japan. Watch to learn how the XRISM (X-ray Imaging and Spectroscopy Mission) satellite took an unprecidented look at our galaxy’s sulfur. XRISM is led by JAXA (Japan Aerospace Exploration Agency) in collaboration with NASA, along with contributions from ESA (European Space Agency). NASA’s Goddard Space Flight Center Using ultraviolet light, researchers have found gaseous sulfur in the space between stars. In denser parts of the interstellar medium, such as the molecular clouds where stars and planets are born, this form of sulfur quickly disappears. Scientists assume the sulfur condenses into a solid, either by combining with ice or mixing with other elements. When a doctor performs an X-ray here on Earth, they place the patient between an X-ray source and a detector. Bone and tissue absorb different amounts of the light as it travels through the patient’s body, creating contrast in the detector. To study sulfur, Corrales and her team did something similar. They picked a portion of the interstellar medium with the right density — not so thin that all the X-rays would pass through unchanged, but also not so dense that they would all be absorbed. Then the team selected a bright X-ray source behind that section of the medium, a binary star system called GX 340+0 located over 35,000 light-years away in the southern constellation Scorpius. This composite shows a section of the interstellar medium scientists X-rayed for sulfur using the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission). X-ray binary GX 340+0 is the blue dot in the center. The composite contains a blend of imagery in X-rays (represented in deep blue), infrared, and optical light.DSS/DECaPS/eRosita/NASA’s Goddard Space Flight Center This composite shows a section of the interstellar medium scientists X-rayed for sulfur using the Japan-led XRISM (X-ray Imaging and Spectroscopy Mission). The X-ray binary 4U 1630–472 is highlighted at the center. The composite contains a blend of imagery in X-rays (represented in deep blue), infrared, and optical light.DSS/DECaPS/eRosita/NASA’s Goddard Space Flight Center Using the Resolve instrument on XRISM, the scientists were able to measure the energy of GX 340+0’s X-rays and determined that sulfur was present not only as a gas, but also as a solid, possibly mixed with iron. “Chemistry in environments like the interstellar medium is very different from anything we can do on Earth, but we modeled sulfur combined with iron, and it seems to match what we’re seeing with XRISM,” said co-author Elisa Costantini, a senior astronomer at the Space Research Organization Netherlands and the University of Amsterdam. “Our lab has created models for different elements to compare with astronomical data for years. The campaign is ongoing, and soon we’ll have new sulfur measurements to compare with the XRISM data to learn even more.” Iron-sulfur compounds are often found in meteorites, so scientists have long thought they might be one way sulfur solidifies out of molecular clouds to travel through the universe. In their paper, Corrales and her team propose a few compounds that would match XRISM’s observations — pyrrhotite, troilite, and pyrite, which is sometimes called fool’s gold. The researchers were also able to use measurements from a second X-ray binary called 4U 1630-472 that helped confirm their findings. “NASA’s Chandra X-ray Observatory has previously studied sulfur, but XRISM’s measurements are the most detailed yet,” said Brian Williams, the XRISM project scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “Since GX 340+0 is on the other side of the galaxy from us, XRISM’s X-ray observations are a unique probe of sulfur in a large section of the Milky Way. There’s still so much to learn about the galaxy we call home.” XRISM is led by JAXA (Japan Aerospace Exploration Agency) in collaboration with NASA, along with contributions from ESA (European Space Agency). NASA and JAXA developed Resolve, the mission’s microcalorimeter spectrometer. Download images and videos through NASA’s Scientific Visualization Studio. By Jeanette Kazmierczak NASA’s Goddard Space Flight Center, Greenbelt, Md. Media Contact: Alise Fisher 202-358-2546 alise.m.fisher@nasa.gov NASA Headquarters, Washington Facebook logo @NASAUniverse @NASAUniverse Instagram logo @NASAUniverse Share Details Last Updated Jul 23, 2025 EditorJeanette Kazmierczak Related TermsGoddard Space Flight CenterAstrophysicsStarsThe UniverseX-ray AstronomyX-ray BinariesXRISM (X-Ray Imaging and Spectroscopy Mission) View the full article

Explore This Section Perseverance Home Mission Overview Rover Components Mars Rock Samples Where is Perseverance? Ingenuity Mars Helicopter Mission Updates Science Overview Objectives Instruments Highlights Exploration Goals News and Features Multimedia Perseverance Raw Images Images Videos Audio More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 2 min read Feeling the Heat: Perseverance Looks for Evidence of Contact Metamorphism NASA’s Mars Perseverance rover acquired this image of the boulders along the contact at Westport, using its Mastcam-Z Left Camera, one of a pair of cameras located high on the rover’s mast. The rover acquired the image on July 10, 2025 — Sol 1560, or Martian day 1,560 of the Mars 2020 mission — at the local mean solar time of 11:23:38. NASA/JPL-Caltech/ASU Written by Melissa Rice, Professor of Planetary Science at Western Washington University Following a short break for the July 4th holiday, Perseverance drove westward to a site called “Westport,” where the clay-bearing “Krokodillen” unit meets an olivine-bearing rock formation. It is possible that the olivine-rich rocks are an intrusive igneous unit, meaning they could have formed when molten magma from deep within Mars got pushed upwards and cooled under the surface. If that’s the case, Westport could preserve a dramatic moment in Mars’ history when hot, molten material intruded into existing rock formations. Those intrusive processes are common on Earth, and the heat of the intruding magma can fundamentally alter the surrounding geology through a process called “contact metamorphism.” The heat from the intrusion will “bake” nearby rocks, creating new minerals and potentially new environments for microbial life. Conversely, the intrusive rocks get rapidly “chilled” where they meet preexisting solid rock formations. At Westport, Perseverance is looking for evidence that the Krokodillen rocks at the contact were baked, and that the olivine-bearing rocks at the contact were chilled. Images from the Mastcam-Z instrument reveal that the contact is littered with intriguing dark, rubbly rocks alongside lighter-toned, smooth boulders. Both rock types are proving challenging to study. The dark fragments are too small and rough for Perseverance’s standard abrasion techniques, but the rover cleared off the surface of a rock called “Holyrood Bay” with its gas Dust Removal Tool (gDRT). Perseverance also tried to abrade a nearby boulder named “Drake’s Point,” but the rock shifted to the side, causing the abrasion to stop short. The science questions here are compelling enough, however, that Perseverance will keep trying to look within the rocks at this important boundary. Share Details Last Updated Jul 22, 2025 Related Terms Blogs Explore More 3 min read Curiosity Blog, Sols 4607-4608: Deep Dip Article 1 hour ago 3 min read Curiosity Blog, Sols 4604-4606: Taking a Deep Breath of Martian Air Article 10 hours ago 2 min read Curiosity Blog, Sols 4602-4603: On Top of the Ridge Article 4 days ago Keep Exploring Discover More Topics From NASA Mars Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited… All Mars Resources Explore this collection of Mars images, videos, resources, PDFs, and toolkits. Discover valuable content designed to inform, educate, and inspire,… Rover Basics Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a… Mars Exploration: Science Goals The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four… View the full article

Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home 3 min read Curiosity Blog, Sols 4607-4608: Deep Dip NASA’s Mars rover Curiosity acquired this image, looking toward the upper slopes of Mount Sharp, using its Left Navigation Camera (Left Navcam) on July 20, 2025. Curiosity captured the image on Sol 4605, or Martian day 4,605 of the Mars Science Laboratory mission, at 18:58:26 UTC. NASA/JPL-Caltech Written by Deborah Padgett, MSL OPGS Task Lead at NASA’s Jet Propulsion Laboratory Earth planning date: Monday, July 21, 2025 Curiosity continues our exploration of the fractured boxwork terrain on the slopes of Mount Sharp. After a successful 5-meter drive (about 16 feet), our rover is resting in a hollow on its way to a boxwork ridge viewpoint. Over the weekend, Curiosity began an atmospheric observation with the SAM instrument, which will continue into today’s plan. Because the SAM instrument is complex and powerful, it uses a great deal of energy when it operates, causing what we call a “deep dip” in the battery charge level. This means that we have to wait a bit after the SAM observations complete for the battery to recharge enough for Curiosity to observe its surroundings with other science instruments, or move its arm or wheels. For this reason, the plan today does not include a drive, and contact science at this location will be done on the second sol of the plan. On Sol 4607, Curiosity will begin the day with SAM atmospheric composition activity, which will run for several hours. After it finishes, we will use the rover’s navigation camera to perform a cloud altitude observation, looking for cloud shadows on the upper reaches of Mount Sharp, and clouds drifting by overhead at the zenith. Overnight, Curiosity’s battery will recharge, allowing us to perform a targeted science block on the morning of Sol 4608. This starts with Navcam observations of dust opacity across the floor of Gale Crater, then a measurement of dust in the air toward the Sun with Mastcam. Curiosity then turns Mastcam toward the ridge ahead to obtain a 15×1 mosaic on target “Cueva De Los Vencejos Y Murcielagos (Cave of Swifts and Bats).” Afterwards, Mastcam will look back along Curiosity’s tracks, hoping to see freshly broken rocks and determine the texture of disturbed ground. Next, ChemCam’s laser spectrograph will zap a nodular rock pillar named for the famous high-altitude “Lake Titicaca” bordering Bolivia and Peru. A second ChemCam observation with the RMI telescopic camera will study stratigraphy on the Mishe Mokwa butte with a 5×2 image mosaic. Mastcam will finish off this science block by looking at the pits left behind by the ChemCam laser on target “Lake Titicaca.” In the afternoon, Curiosity’s arm will reach out to brush the dust from the bedrock target “La Tranquita,” then observe it with the MAHLI microscopic imager and APXS. MAHLI and APXS will also investigate plate-like rock formations at target “Aqua Dulce.” A third target with more complex rock structures dubbed “Paposo,” after a natural monument along the Pacific Coast of northern Chile, will be imaged only by MAHLI. The next morning will include another targeted science block. Curiosity will then drive away toward the next viewpoint in the boxwork terrain of Mars. For more Curiosity blog posts, visit MSL Mission Updates Learn more about Curiosity’s science instruments Share Details Last Updated Jul 22, 2025 Related Terms Blogs Explore More 3 min read Curiosity Blog, Sols 4604-4606: Taking a Deep Breath of Martian Air Article 9 hours ago 2 min read Curiosity Blog, Sols 4602-4603: On Top of the Ridge Article 4 days ago 2 min read Curiosity Blog, Sols 4600-4601: Up and Over the Sand Covered Ramp Article 7 days ago Keep Exploring Discover More Topics From NASA Mars Mars is the fourth planet from the Sun, and the seventh largest. It’s the only planet we know of inhabited… All Mars Resources Explore this collection of Mars images, videos, resources, PDFs, and toolkits. Discover valuable content designed to inform, educate, and inspire,… Rover Basics Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a… Mars Exploration: Science Goals The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four… View the full article

Explore This Section Science Uncategorized NASA eClips STEM Student… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 3 min read NASA eClips STEM Student Ambassadors Light Up CNU’s 2025 STEM Community Day More than 2,000 curious visitors from Newport News and the surrounding Hampton Roads region of Virginia flocked to Christopher Newport University (CNU) on May 31, 2025 for their annual STEM (Science, Technology, Engineering, & Mathematics) Community Day, and the NASA eClips team from the National Institute of Aerospace’s Center for Integrative STEM Education (NIA-CISE) made sure every one of them left with their eyes—and imaginations—fixed on the Sun. At the heart of the NASA eClips exhibit were NIA’s STEM Student Ambassadors—a team of carefully selected high school students from the Tidewater region of Virginia who underwent extensive training with NASA eClips educators during the summer of 2024. These bright, enthusiastic young leaders are passionate about communicating about and advocating for STEM. The STEM Student Ambassador program is made possible through a Coastal Virginia STEM Hub grant from the Virginia General Assembly and is already having an impact. Throughout the day, the Ambassadors engaged learners of all ages with two creative, hands-on experiences that connected STEM and the arts: Chalk Corona – Using black construction paper and vibrant chalk, participants recreated the Sun’s corona—the super-hot, gaseous “crown” that’s visible during a total solar eclipse. While they shaded and smudged, the Ambassadors explained why the corona is so important to solar research and handed out certified solar viewers for safe Sun-watching back home. Pastel Auroras – Visitors also discovered how solar wind, storms, and coronal mass ejections (aka Sun “sneezes”) spark Earth’s dazzling auroras. Guided by the Ambassadors, budding artists layered pastels to capture swirling curtains of light, tying recent mid-Atlantic aurora sightings to real-time space weather. Throughout the day, the Ambassadors’ energy was contagious, turning complex heliophysics into hands-on fun and opening eyes to the opportunities and careers that await in STEM. Judging by the smiles—and the dusting of chalk and pastels—NASA eClips’ presence was, quite literally, the “crowning” touch on an unforgettable community celebration of STEM. 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 Two STEM Student Ambassadors engage a young girl while she creates her own Pastel Aurora artwork. Share Details Last Updated Jul 22, 2025 Editor NASA Science Editorial Team Related Terms Opportunities For Students to Get Involved Science Activation The Sun Explore More 2 min read GLOBE-Trotting Science Lands in Chesapeake with NASA eClips Article 1 day ago 6 min read NASA’s TRACERS Studies Explosive Process in Earth’s Magnetic Shield Article 6 days ago 3 min read NASA Citizen Science and Your Career: Stories of Exoplanet Watch Volunteers Doing NASA Science brings many rewards. But can taking part in NASA citizen science help… Article 6 days ago Keep Exploring Discover More Topics From NASA James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Perseverance Rover This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial… Parker Solar Probe On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona… Juno NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to… View the full article

After months of work in the NASA Spacesuit User Interface Technologies for Students (SUITS) challenge, more than 100 students from 12 universities across the United States traveled to NASA’s Johnson Space Center in Houston to showcase potential user interface designs for future generations of spacesuits and rovers. NASA Johnson’s simulated Moon and Mars surface, called “the rock yard,” became the students’ testing ground as they braved the humid nights and abundance of mosquitoes to put their innovative designs to the test. Geraldo Cisneros, the tech team lead, said, “This year’s SUITS challenge was a complete success. It provided a unique opportunity for NASA to evaluate the software designs and tools developed by the student teams, and to explore how similar innovations could contribute to future, human-centered Artemis missions. My favorite part of the challenge was watching how the students responded to obstacles and setbacks. Their resilience and determination were truly inspiring.” Tess Caswell and the Rice Owls team from Rice University test their augmented reality heads-up display at Johnson Space Center’s Rock Yard in Houston on May 19, 2025.NASA/James Blair Students filled their jam-packed days not only with testing, but also with guest speakers and tours. Swastik Patel from Purdue University said, “All of the teams really enjoyed being here, seeing NASA facilities, and developing their knowledge with NASA coordinators and teams from across the nation. Despite the challenges, the camaraderie between all the participants and staff was very helpful in terms of getting through the intensity. Can’t wait to be back next year!” John Mulnix with Team Cosmoshox from Wichita State University presents the team’s design during the Spacesuit User Interface Technologies for Students (SUITS) exit pitches at Johnson on May 22, 2025.NASA/David DeHoyos “This week has been an incredible opportunity. Just seeing the energy and everything that’s going on here was incredible. This week has really made me reevaluate a lot of things that I shoved aside. I’m grateful to NASA for having this opportunity, and hopefully we can continue to have these opportunities.” At the end of test week, each student team presented their projects to a panel of experts. These presentations served as a platform for students to showcase not only their technical achievements but also their problem-solving approaches, teamwork, and vision for real-world application. The panel–composed of NASA astronaut Deniz Burnham, Flight Director Garrett Hehn, and industry leaders–posed thought-provoking questions and offered constructive feedback that challenged the students to think critically and further refine their ideas. Their insights highlighted potential areas for growth, new directions for exploration, and ways to enhance the impact of their projects. The students left the session energized and inspired, brimming with new ideas and a renewed enthusiasm for future development and innovation. Burnham remarked, “The students did such a great job. They’re all so creative and wonderful, definitely something that can be implemented in the future.” Gamaliel Cherry, director of the Office of STEM Engagement at Johnson, presents the Artemis Educator Award to Maggie Schoonover from Wichita State University on May 22, 2025.NASA/David DeHoyos NASA SUITS test week was not only about pushing boundaries; it was about earning a piece of history. Three Artemis Student Challenge Awards were presented. The Innovation and Pay it Forward awards were chosen by the NASA team, recognizing the most groundbreaking and impactful designs. Students submitted nominations for the Artemis Educator Award, celebrating the faculty member who had a profound influence on their journeys. The Innovation Award went to Team JARVIS from Purdue University and Indiana State University, for going above and beyond in their ingenuity, creativity, and inventiveness. Team Selene from Midwestern State University earned the Pay it Forward Award for conducting meaningful education events in the community and beyond. The Artemis Educator Award was given to Maggie Schoonover from Wichita State University in Kansas for the time, commitment, and dedication she gave to her team. “The NASA SUITS challenge completes its eighth year in operation due to the generous support of NASA’s EVA and Human Surface Mobility Program,” said NASA Activity Manager Jamie Semple. “This challenge fosters an environment where students learn essential skills to immediately enter a science, technology, engineering, and mathematics (STEM) career, and directly contribute to NASA mission operations. These students are creating proposals, generating designs, working in teams similar to the NASA workforce, utilizing artificial intelligence, and designing mission operation solutions that could be part of the Artemis III mission and beyond. NASA’s student design challenges are an important component of STEM employment development and there is no better way to learn technical skills to ensure future career success.” The week serves as a springboard for the next generation of space exploration, igniting curiosity, ambition, and technical excellence among young innovators. By engaging with real-world challenges and technologies, participants not only deepen their understanding of space science but also actively contribute to shaping its future. Each challenge tackled, each solution proposed, and each connection formed represents a meaningful step forward; not just for the individuals involved, but for humanity as a whole. With every iteration of the program, the dream of venturing further into space becomes more tangible, transforming what once seemed like science fiction into achievable milestones. Are you interested in joining the next NASA SUITS challenge? Find more information here. The next challenge will open for proposals at the end of August 2025. The 2025 NASA SUITS teams represent academic institutions across the United States.NASA/David DeHoyosView the full article

Curiosity Navigation Curiosity Home Mission Overview Where is Curiosity? Mission Updates Science Overview Instruments Highlights Exploration Goals News and Features Multimedia Curiosity Raw Images Images Videos Audio Mosaics More Resources Mars Missions Mars Sample Return Mars Perseverance Rover Mars Curiosity Rover MAVEN Mars Reconnaissance Orbiter Mars Odyssey More Mars Missions Mars Home NASA’s Mars rover Curiosity acquired this image, looking south across the large boxwork structures, using its Left Navigation Camera on July 17, 2025. A series of ridges and hollows forms the dramatic topography in the foreground, while the distant buttes expose additional sedimentary structures. Curiosity acquired this image on Sol 4602, or Martian day 4,602 of the Mars Science Laboratory mission, at 17:49:18 UTC. NASA/JPL-Caltech Written by Lauren Edgar, Planetary Geologist at USGS Astrogeology Science Center Earth planning date: Friday, July 18, 2025 Curiosity has started to investigate the main exposure of the boxwork structures! What was once a distant target is now on our doorstep, and Curiosity is beginning to explore the ridges and hollows that make up this terrain, to better understand their chemistry, morphology, and sedimentary structures. I was on shift as Long Term Planner during this three-sol weekend plan, and the team put together a very full set of activities to thoroughly investigate this site — from the sky to the sand. The plan starts with Navcam and Mastcam observations to assess the amount of dust in the atmosphere, followed by a large Mastcam mosaic to characterize the resistant ridge on which the rover is parked. ChemCam will also acquire a LIBS observation on a target named “Vicuna” to assess the chemistry of a well-exposed vein. The team chose this parking location to characterize the chemistry and textures of this topographic ridge (to compare with topographic lows), so the next part of the plan involves contact science using APXS and MAHLI to look at different parts of the nodular bedrock in our workspace, at targets named “Totoral” and “Sillar.” There’s also a MAHLI observation of the same vein that ChemCam targeted. The second sol involves more Mastcam imaging to look at different parts of this prominent ridge, along with a ChemCam LIBS observation on top of the ridge, and a ChemCam RMI mosaic to document the sedimentary structures in a distant boxwork feature. Navcam will also be used to look for dust devils. Then Curiosity will take a short drive of about 5 meters (about 16 feet) to explore the adjacent hollow (seen as the low point in the foreground of the above Navcam image). After the drive we’ll take more images for context, and to prepare for targeting in Monday’s plan. After all of this work it’s time to pause and take a deep breath… of Martian atmosphere. The weekend plan involves an exciting campaign to look for variations in atmospheric chemistry between night and day. So Curiosity will take an overnight APXS atmospheric observation at the same time that two instruments within SAM assess its chemical and isotopic abundance. On the third sol Curiosity will acquire a ChemCam passive sky observation, leading to a great set of atmospheric data. These measurements will be compared to even more atmospheric activities in Monday’s plan to get the full picture. As you can imagine, this plan requires a lot of power, but it’s worth it for all of the exciting science that we can accomplish here. The road ahead has many highs and lows (literally), but I can’t wait to see what Curiosity will accomplish. The distant buttes remind us that there’s so much more to explore, and I look forward to continuing to see where Curiosity will take us. For more Curiosity blog posts, visit MSL Mission Updates Learn more about Curiosity’s science instruments Explore More 2 min read Curiosity Blog, Sols 4602-4603: On Top of the Ridge Article 4 days ago 2 min read Curiosity Blog, Sols 4600-4601: Up and Over the Sand Covered Ramp Article 6 days ago 2 min read Curiosity Blog, Sols 4597-4599: Wide Open Spaces Article 6 days ago Keep Exploring Discover More Topics From NASA Mars Mars Resources Explore this page for a curated collection of Mars resources. Rover Basics Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a… Mars Exploration: Science Goals The key to understanding the past, present or future potential for life on Mars can be found in NASA’s four… View the full article

Credit: NASA Senegal will sign the Artemis Accords during a ceremony at 2 p.m. EDT on Thursday, July 24, at NASA Headquarters in Washington. Brian Hughes, NASA chief of staff, will host Maram Kairé, director general of the Senegalese space agency (ASES), and Abdoul Wahab Haidara, ambassador of Senegal to the United States, along with other officials from Senegal and the U.S. Department of State. This event is in-person only. Media interested in attending must RSVP no later than 10 a.m. on Thursday, July 24, to: hq-media@mail.nasa.gov. NASA’s media accreditation policy is online. The signing ceremony will take place at the James E. Webb Memorial Auditorium at NASA Headquarters in the Mary W. Jackson building, 300 E. Street SW in Washington. In 2020, during the first Trump Administration, the United States, led by NASA and the State Department, joined with seven other founding nations to establish the Artemis Accords, responding to the growing interest in lunar activities by both governments and private companies. The accords introduced the first set of practical principles aimed at enhancing the safety, transparency, and coordination of civil space exploration on the Moon, Mars, and beyond. Senegal is the 56th country to sign the Artemis Accords since their inception. The Artemis Accords are grounded in international law and represent the best practices and norms of responsible behavior that NASA and its partners have supported, including the public release of scientific data. Learn more about the Artemis Accords at: https://www.nasa.gov/artemis-accords -end- Bethany Stevens / Elizabeth Shaw Headquarters, Washington 202-358-1600 bethany.c.stevens@nasa.gov / elizabeth.a.shaw@nasa.gov Share Details Last Updated Jul 22, 2025 EditorJessica TaveauLocationNASA Headquarters Related TermsArtemis AccordsOffice of International and Interagency Relations (OIIR) View the full article

NASA/Carla Thomas NASA’s X-59 quiet supersonic research aircraft completed its first low-speed taxi test at U.S. Air Force Plant 42 in Palmdale, California, on July 10, 2025. This marked the first time the one-of-a-kind experimental aircraft has ever moved under its own power.  During the test, engineers and flight crews monitored the X-59 as it moved across the runway, working to validate critical systems like steering and braking. The taxiing represents the start of the X-59’s final series of ground tests before first flight.  The X-59 is the centerpiece of NASA’s Quesst mission, which aims to demonstrate quiet supersonic flight by reducing the loud sonic boom to a quieter “thump.” Image Credit: NASA/Carla Thomas View the full article

NASA Glenn Research Center’s Thermal Energy Conversion Branch team and the University of Leicester’s Space Nuclear Power team pose for a photo at the center in Cleveland following a successful test in January 2025.Credit: NASA/Jef Janis To explore the unknown in deep space, millions of miles away from Earth, it’s crucial for spacecraft to have ample power. NASA’s radioisotope power systems (RPS) are a viable option for these missions and have been used for over 60 years, including for the agency’s Voyager spacecraft and Perseverance Mars rover. These nuclear batteries provide long-term electrical power for spacecraft and science instruments using heat produced by the natural radioactive decay of radioisotopes. Now, NASA is testing a new type of RPS heat source fuel that could become an additional option for future long-duration journeys to extreme environments. Historically, the radioisotope plutonium-238 (plutonium oxide) has been NASA’s RPS heat source fuel of choice, but americium-241 has been a source of interest for the past two decades in Europe. In January, the Thermal Energy Conversion Branch at NASA’s Glenn Research Center in Cleveland and the University of Leicester, based in the United Kingdom, partnered through an agreement to put this new option to the test. One method to generate electricity from radioisotope heat sources is the free-piston Stirling convertor. This is a heat engine that converts thermal energy into electrical energy. However, instead of a crankshaft to extract power, pistons float freely within the engine. It could operate for decades continuously without wear, as it does not have piston rings or rotating bearings that will eventually wear out. Thus, a Stirling convertor could generate more energy, allowing more time for exploration in deep space. Researchers from the University of Leicester — who have been leaders in the development of americium RPS and heater units for more than 15 years — and NASA worked to test the capabilities of a Stirling generator testbed powered by two electrically heated americium-241 heat source simulators. “The concept started as just a design, and we took it all the way to the prototype level: something close to a flight version of the generator,” said Salvatore Oriti, mechanical engineer at Glenn. “The more impressive part is how quickly and inexpensively we got it done, only made possible by a great synergy between the NASA and University of Leicester teams. We were on the same wavelength and shared the same mindset.” Salvatore Oriti, mechanical engineer in the Thermal Energy Conversion Branch at NASA’s Glenn Research Center in Cleveland, adjusts the Stirling testbed in preparation for testing at the center in January 2025.Credit: NASA/Jef Janis The university provided the heat source simulators and generator housing. The heat source simulator is the exact size and shape of their real americium-241 heat source, but it uses embedded electric heaters to create an equivalent amount of heat to simulate the decay of americium fuel and therefore drive generator operation. The Stirling Research Lab at Glenn provided the test station, Stirling convertor hardware, and support equipment. “A particular highlight of this (testbed) design is that it is capable of withstanding a failed Stirling convertor without a loss of electrical power,” said Hannah Sargeant, research fellow at the University of Leicester. “This feature was demonstrated successfully in the test campaign and highlights the robustness and reliability of an Americium-Radioisotope Stirling Generator for potential future spaceflight missions, including long-duration missions that could operate for many decades.” The test proved the viability of an americium-fueled Stirling RPS, and performance and efficiency targets were successfully met. As for what’s next, the Glenn team is pursuing the next version of the testbed that will be lower mass, higher fidelity, and undergo further environmental testing. “I was very pleased with how smoothly everything went,” Oriti said of the test results. “Usually in my experience, you don’t accomplish everything you set out to, but we did that and more. We plan to continue that level of success in the future.” For more information on NASA’s RPS programs, visit: https://science.nasa.gov/rps Explore More 2 min read GLOBE-Trotting Science Lands in Chesapeake with NASA eClips On June 16-17, 2025, 50 students at Camp Young in Chesapeake, Virginia traded their usual… Article 19 hours ago 6 min read 5 Things to Know About Powerful New U.S.-India Satellite, NISAR Article 21 hours ago 3 min read NASA-Derived Textiles are Touring France by Bike Article 4 days ago View the full article

The crew of NASA’s SpaceX Crew-10 mission pictured aboard the International Space Station. From left to right: JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, NASA astronauts Anne McClain and Nichole Ayers, and Roscosmos cosmonaut Kirill Peskov.Credit: NASA Media are invited to hear from NASA’s SpaceX Crew-10 during a news conference beginning at 10:40 a.m. EDT, Friday, July 25, from the International Space Station. NASA astronauts Anne McClain and Nichole Ayers, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov will discuss their upcoming return to Earth on the agency’s YouTube channel. Media interested in participating must contact the newsroom at NASA’s Johnson Space Center in Houston no later than 5 p.m., Thursday, July 24, at 281-483-5111 or jsccommu@mail.nasa.gov. To ask questions, media must dial into the news conference no later than 10 minutes prior to the start of the call. A copy of NASA’s media accreditation policy is online. Crew-10 joined the Expedition 72 crew when arriving to the station in March. Throughout Expedition 72 and into Expedition 73, the crew aboard the space station contributed to hundreds of experiments, including testing expanded capabilities of existing hardware for pharmaceutical production in space, investigating how cells sense gravity, which is an important aspect of space biology, and examining the effects of microgravity on protein yields in microalgae, a potential source for life support, fuel, and food on long-duration missions. The crew will depart the space station after the arrival of Crew-11 and a handover period. Ahead of Crew-10’s return, mission teams will review weather conditions at the splashdown sites off the coast of California prior to departure from station. The mission is part of NASA’s Commercial Crew Program, which provides reliable access to space, maximizing the use of the station for research and development and supporting future missions beyond low Earth orbit by partnering with private companies to transport astronauts to and from the space station. Follow updates on the Crew-10 mission at: https://www.nasa.gov/blogs/crew-10 -end- Claire O’Shea Headquarters, Washington 202-358-1100 claire.a.o’shea@nasa.gov Courtney Beasley Johnson Space Center, Houston 281-483-5111 courtney.m.beasley@nasa.gov Share Details Last Updated Jul 21, 2025 LocationNASA Headquarters Related TermsHumans in SpaceCommercial CrewISS ResearchOpportunities For International Participants to Get Involved View the full article

Portrait of Dr. Makenzie Lystrup, director of NASA’s Goddard Space Flight Center in Greenbelt, Maryland.Credit: NASA On Monday, NASA announced Dr. Makenzie Lystrup, director of NASA’s Goddard Space Flight Center in Greenbelt, Maryland, is set to leave the agency on Friday, Aug. 1. As center director of Goddard, a role she has held since April 2023, Lystrup also was responsible for guiding the direction and management of multiple other NASA field installations including Wallops Flight Facility in Virginia, Katherine Johnson Independent Verification & Validation Facility in West Virginia, the White Sands Complex in New Mexico, and the Columbia Scientific Balloon Facility in Texas. “Having served in a variety of science and aerospace civilian and government roles in her career, Makenzie has led development of, and/or contributed to a variety of NASA’s priority science missions including successful operations of our James Webb Space Telescope and Imaging X-Ray Polarimetry Explorer, as well as development of the agency’s Roman Space Telescope, and more,” said Vanessa Wyche, acting NASA associate administrator. “We’re grateful to Makenzie for her leadership at NASA Goddard for more than two years, including her work to inspire a Golden Age of explorers, scientists, and engineers.” Throughout her time at NASA, Lystrup led Goddard’s workforce, which consists of more than 8,000 civil servants and contractors. Before joining the agency, Lystrup served as senior director for Ball’s Civil Space Advanced Systems and Business Development, where she managed new business activities for NASA, National Oceanic and Atmospheric Administration (NOAA), and other civilian U.S. government agencies as well as for academia and other science organizations. In addition, she served in the company’s Strategic Operations organization, based in Washington where she led Ball’s space sciences portfolio. Prior to joining Ball, Lystrup worked as an American Institute of Physics – Acoustical Society of American Congressional Fellow from 2011 to 2012 where she managed a portfolio including technology, national defense, nuclear energy, and nuclear nonproliferation. Lystrup also has served on boards and committees for several organizations to include the University Corporation for Atmospheric Research, International Society for Optics and Photonic, the University of Colorado, and the American Astronomical Society. She was named an American Association for the Advancement of Science fellow in 2019 for her distinguished record in the fields of planetary science and infrared astronomy, science policy and advocacy, and aerospace leadership. Lystrup also served as an AmeriCorps volunteer focusing on STEM education. Lystrup holds a bachelor’s in physics from Portland State University and attended graduate school at University College London earning her doctorate in astrophysics. She was a National Science Foundation Astronomy & Astrophysics Postdoctoral Research Fellow spending time at the Laboratory for Atmospheric & Space Physics in Boulder, Colorado, and University of Liege in Belgium. As a planetary scientist and astronomer, Lystrup’s scientific work has been in using ground- and space-based astronomical observatories to understand the interactions and dynamics of planetary atmospheres and magnetospheres – the relationships between planets and their surrounding space environments. Following Lystrup’s departure, NASA’s Cynthia Simmons will serve as acting center director. Simmons is the current deputy center director. For more information about NASA’s work, visit: https://www.nasa.gov -end- Cheryl Warner / Kathryn Hambleton Headquarters, Washington 202-358-1600 cheryl.m.warner@nasa.gov / kathryn.hambleton@nasa.gov Katy Mersmann Goddard Space Flight Center, Greenbelt, Md. 301-377-1724 katy.mersmann@nasa.gov Share Details Last Updated Jul 21, 2025 EditorJessica TaveauLocationNASA Headquarters Related TermsGoddard Space Flight CenterLeadership View the full article

5 min read Preparations for Next Moonwalk Simulations Underway (and Underwater) The north polar region of Jupiter’s volcanic moon Io was captured by the JunoCam imager aboard NASA’s Juno during the spacecraft’s 57th close pass of the gas giant on Dec. 30, 2023. A technique called annealing was used to help repair radiation damage to the camera in time to capture this image. Image data: NASA/JPL-Caltech/SwRI/MSSS Image processing by Gerald Eichstädt An experimental technique rescued a camera aboard the agency’s Juno spacecraft, offering lessons that will benefit other space systems that experience high radiation. The mission team of NASA’s Jupiter-orbiting Juno spacecraft executed a deep-space move in December 2023 to repair its JunoCam imager to capture photos of the Jovian moon Io. Results from the long-distance save were presented during a technical session on July 16 at the Institute of Electrical and Electronics Engineers Nuclear & Space Radiation Effects Conference in Nashville. JunoCam is a color, visible-light camera. The optical unit for the camera is located outside a titanium-walled radiation vault, which protects sensitive electronic components for many of Juno’s engineering and science instruments. This is a challenging location because Juno’s travels carry it through the most intense planetary radiation fields in the solar system. While mission designers were confident JunoCam could operate through the first eight orbits of Jupiter, no one knew how long the instrument would last after that. Throughout Juno’s first 34 orbits (its prime mission), JunoCam operated normally, returning images the team routinely incorporated into the mission’s science papers. Then, during its 47th orbit, the imager began showing hints of radiation damage. By orbit 56, nearly all the images were corrupted. The graininess and horizontal lines seen in this JunoCam image show evidence that the camera aboard NASA’s Juno mission suffered radiation damage. The image, which captures one of the circumpolar cyclones on Jupiter’s north pole, was taken Nov. 22, 2023. NASA/JPL-Caltech/SwRI/MSSS Long Distance Microscopic Repair While the team knew the issue may be tied to radiation, pinpointing what, specifically, was damaged within JunoCam was difficult from hundreds of millions of miles away. Clues pointed to a damaged voltage regulator that is vital to JunoCam’s power supply. With few options for recovery, the team turned to a process called annealing, where a material is heated for a specified period before slowly cooling. Although the process is not well understood, the idea is that the heating can reduce defects in the material. “We knew annealing can sometimes alter a material like silicon at a microscopic level but didn’t know if this would fix the damage,” said JunoCam imaging engineer Jacob Schaffner of Malin Space Science Systems in San Diego, which designed and developed JunoCam and is part of the team that operates it. “We commanded JunoCam’s one heater to raise the camera’s temperature to 77 degrees Fahrenheit — much warmer than typical for JunoCam — and waited with bated breath to see the results.” Soon after the annealing process finished, JunoCam began cranking out crisp images for the next several orbits. But Juno was flying deeper and deeper into the heart of Jupiter’s radiation fields with each pass. By orbit 55, the imagery had again begun showing problems. “After orbit 55, our images were full of streaks and noise,” said JunoCam instrument lead Michael Ravine of Malin Space Science Systems. “We tried different schemes for processing the images to improve the quality, but nothing worked. With the close encounter of Io bearing down on us in a few weeks, it was Hail Mary time: The only thing left we hadn’t tried was to crank JunoCam’s heater all the way up and see if more extreme annealing would save us.” Test images sent back to Earth during the annealing showed little improvement the first week. Then, with the close approach of Io only days away, the images began to improve dramatically. By the time Juno came within 930 miles (1,500 kilometers) of the volcanic moon’s surface on Dec. 30, 2023, the images were almost as good as the day the camera launched, capturing detailed views of Io’s north polar region that revealed mountain blocks covered in sulfur dioxide frosts rising sharply from the plains and previously uncharted volcanos with extensive flow fields of lava. Testing Limits To date, the solar-powered spacecraft has orbited Jupiter 74 times. Recently, the image noise returned during Juno’s 74th orbit. Since first experimenting with JunoCam, the Juno team has applied derivations of this annealing technique on several Juno instruments and engineering subsystems. “Juno is teaching us how to create and maintain spacecraft tolerant to radiation, providing insights that will benefit satellites in orbit around Earth,” said Scott Bolton, Juno’s principal investigator from the Southwest Research Institute in San Antonio. “I expect the lessons learned from Juno will be applicable to both defense and commercial satellites as well as other NASA missions.” More About Juno NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Juno mission for the principal investigator, Scott Bolton, of the Southwest Research Institute in San Antonio. Juno is part of NASA’s New Frontiers Program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington. The Italian Space Agency, Agenzia Spaziale Italiana, funded the Jovian InfraRed Auroral Mapper. Lockheed Martin Space in Denver built and operates the spacecraft. Various other institutions around the U.S. provided several of the other scientific instruments on Juno. More information about Juno is at: https://www.nasa.gov/juno News Media Contact DC Agle Jet Propulsion Laboratory, Pasadena, Calif. 818-393-9011 agle@jpl.nasa.gov Karen Fox / Molly Wasser NASA Headquarters, Washington 202-358-1600 karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov Deb Schmid Southwest Research Institute, San Antonio 210-522-2254 dschmid@swri.org 2025-091 Share Details Last Updated Jul 21, 2025 Related TermsJunoJet Propulsion LaboratoryJupiterJupiter Moons Explore More 6 min read 5 Things to Know About Powerful New U.S.-India Satellite, NISAR Article 2 hours ago 6 min read Meet Mineral Mappers Flying NASA Tech Out West Article 2 weeks ago 3 min read NASA Aircraft, Sensor Technology, Aid in Texas Flood Recovery Efforts Article 2 weeks ago Keep Exploring Discover Related Topics Missions Humans in Space Climate Change Solar System View the full article

Explore This Section Science Earth Science GLOBE-Trotting Science Lands… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 2 min read GLOBE-Trotting Science Lands in Chesapeake with NASA eClips On June 16-17, 2025, 50 students at Camp Young in Chesapeake, Virginia traded their usual summer routines for microscopes. The NASA eClips team from the National Institute of Aerospace Center for Integrative STEM Education (NIA-CISE) taught two engaging lessons focused on macroinvertebrates and plankton, with a surprising star of the show – mosquitoes! Camp Young, a Title I camp program serving students from Norfolk Public Schools, provides year-round, environmental science-based learning. The NASA eClips’ visit reinforced their mission to help students explore their environment on the Elizabeth River while seeing its place in the Earth System. The lessons, designed for students in grades 3 through 8, were inspired by NASA’s GLOBE (Global Learning and Observations to Benefit the Environment) program, which encourages people around the world to collect and share environmental data as ‘citizen scientists’. This is where mosquitos stole the show! The lesson focuses on how these tiny insects can serve as indicators of climate and habitat change. By identifying mosquito larvae and understanding their breeding environments, students contributed to the bigger picture of global health and environmental monitoring, right from their own backyard. During this experience, Camp Young’s stunning waterfront on the Elizabeth River was turned into a living laboratory. With phytoplankton nets, petri dishes, and sample jars in hand, campers ventured into the field to collect real environmental data, bringing their findings back to a cabin-turned-classroom to analyze them with scientific tools, including microscopes provided by the NASA eClips team. Rather than just reading about ecosystems and the kinds of scientific questions that arise within them, students got to experience them firsthand and experience real science in the field. “It’s one thing to talk about microscopic marine organisms,” one instructor noted, “but it’s another thing entirely when students can actually see them swimming in a droplet from the river.” 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 A student collects a stagnant water sample, looking for mosquito eggs and larvae. Share Details Last Updated Jul 21, 2025 Editor NASA Science Editorial Team Related Terms Earth Science Opportunities For Students to Get Involved Science Activation Explore More 3 min read NASA Citizen Science and Your Career: Stories of Exoplanet Watch Volunteers Doing NASA Science brings many rewards. But can taking part in NASA citizen science help… Article 5 days ago 4 min read NASA SCoPE Summer Symposium Celebrates Early Career Scientists and Cross-Team Collaboration Article 6 days ago 4 min read Linking Satellite Data and Community Knowledge to Advance Alaskan Snow Science Article 1 week ago Keep Exploring Discover More Topics From NASA James Webb Space Telescope Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the… Perseverance Rover This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial… Parker Solar Probe On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona… Juno NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to… View the full article

On July 19, 2013, in an event celebrated the world over, NASA’s Cassini spacecraft slipped into Saturn’s shadow and turned to image the planet, seven of its moons, its inner rings, and, in the background, our home planet, Earth.NASA/JPL-Caltech/SSI On July 19, 2013, NASA’s Cassini spacecraft had a rare opportunity to image Saturn and, far in the background, Earth. This image spans about 404,880 miles (651,591 kilometers) across. With the Sun’s powerful and potentially damaging rays eclipsed by Saturn itself, Cassini’s onboard cameras were able to take advantage of this unique viewing geometry. They acquired a panoramic mosaic of the Saturn system that allows scientists to see details in the rings and throughout the system as they are backlit by the sun. This mosaic is special as it marks the third time our home planet was imaged from the outer solar system; the second time it was imaged by Cassini from Saturn’s orbit; and the first time ever that inhabitants of Earth were made aware in advance that their photo would be taken from such a great distance. Before the mission ended in 2017, Cassini was already a powerful influence on future exploration. Lessons learned during Cassini’s mission are being applied in NASA’s Europa Clipper mission. The mission uses an orbital tour design derived from the way Cassini explored Saturn. Launched in 2024, Europa Clipper will reach Jupiter in April 2030 and make dozens of flybys of the planet’s icy moon to determine whether there are places below the surface that could support life. Learn more about this unique image. Image credit: NASA/JPL-Caltech/SSI View the full article

NISAR: Tracking Earth’s Changing Surface (Official NASA Trailer)