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Millions of Stars in Cigar Galaxy
NASA’s James Webb Space Telescope recently observed edge-on starburst galaxy Messier 82 (M82), nicknamed the Cigar Galaxy. Webb’s new view of M82, added to archival data from NASA’s Hubble Space Telescope, gives us a more complete picture of this starburst galaxy. Because Webb can see infrared light, it is able to peer through clouds of dust and gas to see the shape of this edge-on galaxy, as well as approximately 16.5 million of its stars.
M82’s rapid star formation, thought to be the result of its merger with another galaxy, will only be a (relatively) brief period in its history. Ironically, the extreme star formation is causing plumes of material to be ejected above and below the disk of the galaxy – something that will disrupt future stellar birth.
Image credit: NASA, ESA, CSA, Adam Smercina (STScI, Tufts), Thomas Williams (University of Manchester); Image processing: Alyssa Pagan (STScI)
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NASA’s TESS Mission Reveals the “Puffiest” Planets Ever Found
Data from NASA’s TESS (Transiting Exoplanet Survey Satellite) mission has revealed two new “super-puff” planets, giant worlds so light that their density is comparable to cotton candy. Scientists calculate that these Jupiter-sized planets—named TOI-791 b and TOI-791 c—are the “puffiest” worlds ever found.
The planets orbit a Sun-like star named TOI-791 that is approximately 1,113 light years away from Earth. The TESS mission first detected the planets by watching for repeated dips in TOI-791’s brightness, a telltale sign that a planet is transiting, or passing in front of, a star. Further study revealed two large planets with unusual features.
TOI-791 b is nearly the same size as Jupiter but contains just 3.0 percent of Jupiter’s mass. TOI-791 c is even larger than Jupiter but contains just 5.9 percent of Jupiter’s mass.
“The main reason these planets are interesting to study is that we didn’t expect to see them at all,” said Jon Jenkins, the science lead for the Science Processing Operations Center at NASA’s Ames Research Center in California’s Silicon Valley, which provided the science-ready data from TESS analyzed in this study. “They represent a puzzle for us to solve about how giant planets like Jupiter and the super-puffs form.”
This graphic depicts the two giant planets orbiting the Sun-like star TOI-791 as compared to some of the planets in our solar system. These planets are roughly the size of Jupiter but a very tiny fraction of its mass. NASA’s TESS mission detected the shadows of these planets as they passed in front of their star. There is no direct imaging. Therefore, the appearance of the TOI-79 planets in this illustration are an artist’s interpretation. NASA / Daniel RutterThe newly found super-puffs also have unusually long orbits, with TOI‑791 b taking 139 days and TOI‑791 c taking 232 days to circle the host star. Such long-orbit planets are rare to find, needing long durations of telescope observation to capture and confirm their attributes. From its vantage point in high Earth orbit, TESS was able to gather 1,122 days of data on this planetary system over the course of seven years, giving the research team a wealth of data about the planetary system.
Further analysis found that TOI-791 b and TOI-791 c are locked in an orbital pattern that allows them to tug on each other gravitationally. As they orbit their host star, the planets alternate pulling on each other, affecting the timing of their transits across the host star. Scientists used that variation in orbital timing to calculate the planets’ masses, cementing their status as low density super-puffs.
“Only a handful of these super-puffy planets are known, and it is even rarer to find two in the same system,” said lead author George Dransfield of Oxford University’s Department of Physics in Oxford, England. “Their extremely low densities make them fascinating targets for understanding how planetary systems form and evolve.”
With further study, the super-puffs may have more to tell us about planetary evolution.
“Large planet formation is believed to drive the evolution of a planetary system, so further study of these Jupiter-size, but far less than Jupiter-mass, planets is of high value,” said Steve Howell, a NASA Ames research scientist who was involved in this study.
Scientists hope to learn more about the chemical makeup of the planets’ atmospheres, how their spin affects their shape, and how the tilt of their host star compares to their orbits. Deeper investigation could provide new insight into how TOI-791 b and TOI-791 c migrated through the planetary system during their development, whether their orbits were shaped by interactions with other planets, and how low-density super-puff planets form.
The study, published today in the Monthly Notices of the Royal Astronomical Society, was led by the University of Oxford, in collaboration with Université Côte d’Azur/Observatoire de la Côte d’Azur and the University of Birmingham.
NASA at the Ion: Orion Lessons from Artemis II Shape NASA’s Moon to Mars Path
Seven weeks after the Orion spacecraft returned four astronauts from humanity’s first crewed journey around the Moon since Apollo, Artemis II Orion Vehicle Manager Branelle Rodriguez reflected on the mission’s achievements and how it is shaping NASA’s return to the lunar surface and future missions to Mars.
Introduced by NASA’s Johnson Space Center Acting Director of Business Development and Technology Integration Monte Goforth, Rodriguez spoke at the Ion in Houston on May 28 as part of the NASA Stories at the Ion speaker series. Located in Houston’s Ion District, the innovation hub serves as a gathering place for entrepreneurs, researchers, and industry leaders working to advance technology and shape the future of industries ranging from aerospace to energy.
She shared an inside look at the mission she helped guide — as the Orion vehicle manager for Artemis II, Rodriguez has overseen the life of the spacecraft from end-to-end, through its development, production, execution of the mission, and currently, the post-mission work underway now that Orion is back at NASA’s Kennedy Space Center in Florida.
“This mission was very near and dear to my heart,” Rodriguez said. “It has not sunk in what this mission and what this accomplishment all means to us and humanity.”
From left: NASA’s Johnson Space Center Acting Director of Business Development and Technology Integration Monte Goforth, Artemis II Orion Vehicle Manager Branelle Rodriguez, and Director of the Rice Space Institute David Alexander.Launched April 1, Artemis II carried NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, along with CSA (Canadian Space Agency) astronaut Jeremy Hansen, on a 10-day voyage around the Moon inside the Orion spacecraft.
Using mission imagery and video, Rodriguez walked attendees through key milestones, including launch aboard NASA’s SLS (Space Launch System) rocket, operations in high-Earth orbit, a lunar flyby, and Orion’s return to Earth. She also shared views from Orion captured by the crew, including Earthrise, detailed images of the lunar surface, and a solar eclipse observed from deep space.
Artemis II successfully demonstrated Orion’s performance during its first crewed deep space mission. The mission tested Orion’s life support systems, crew interfaces, navigation, and reentry systems, providing data that will help teams prepare for upcoming Artemis missions. The crew also completed a manual piloting demonstration, evaluating Orion handling and proximity operations that will inform future rendezvous and docking activities.
“I think it really hit me at T-minus 10 seconds,” Rodriguez said. “That’s when we go into ‘terminal count,’ meaning there’s just no turning back.”
Rodriguez emphasized that Orion’s success on Artemis II was the result of global teamwork across NASA centers, industry partners, and international agencies. She highlighted the European Service Module, provided by ESA (European Space Agency), which supplies Orion with power, propulsion, oxygen, water, and other resources needed during flight. In the Orion Mission Evaluation Room at Johnson, more than 300 people supported the mission, monitoring spacecraft systems and standing ready to respond in real time. Among the mission’s more personal touches was Rise, Orion’s zero-gravity indicator. The plushie, created by a student through an Artemis II design competition, carried a memory card containing over 5.6 million names of space fans who signed up through NASA’s “Send Your Name with Artemis” effort.
“It is what the crew wanted – to bring all of us with them on this mission,” Rodriguez said.
The crew also designed the mission patch with a hidden detail: viewed from a distance, the artwork reads “all” – a deliberate tribute to everyone who made the mission a success.
“It is a village that makes this possible, absolutely,” she said. Looking ahead, Rodriguez discussed preparations underway for upcoming Artemis missions. Artemis III will test critical rendezvous and docking capabilities between Orion and commercial human landing systems in low Earth orbit and advance plans to return astronauts to the lunar surface. On June 9, NASA announced the Artemis III crew at Johnson Space Center in Houston, while hardware for future missions is already in production at Kennedy Space Center in Florida.
For Rodriguez, Artemis II demonstrated what is possible when thousands of people work toward a common goal, supporting NASA’s vision of a sustained presence at the Moon and, ultimately, human missions to Mars.
“It’s going to take time to build this all up,” Rodriguez said. “But we are off and running.”
Explore More 4 min read I Am Artemis: Jason PetersonJason Peterson’s responsibilities for NASA’s Artemis II mission went beyond his usual role as the…
Article 2 days ago 3 min read I Am Artemis: Elkin Norena Article 2 weeks ago 4 min read How NASA Science and Artemis Are Shaping the 2026 FIFA World Cup Article 2 weeks agoLa NASA compartirá los últimos avances del programa Base Lunar
Lea esta nota de prensa en inglés aquí.
El administrador de la NASA, Jared Isaacman, ofrecerá una conversación virtual el martes 30 de junio a las 2:30 p.m. EDT (hora del este) para compartir las novedades más recientes sobre los planes de la agencia para construir una base en la superficie de la Luna.
El administrador Isaacman y Carlos García-Galán, director del programa Base Lunar, hablarán sobre la próxima ronda de adjudicaciones para nuevas misiones de módulos de alunizaje y ofrecerán un avance de las próximas oportunidades a medida que la agencia avanza en la construcción de una presencia sostenida en la Luna.
La rueda de prensa se transmitirá por el canal de YouTube de la NASA (en inglés). Una repetición instantánea estará disponible en línea. Infórmese sobre cómo ver el contenido de la NASA en distintas plataformas, incluidas las redes sociales (información en inglés).
Para hacer preguntas de forma virtual durante el evento, los periodistas deberán confirmar su asistencia a más tardar a las 12:30 p.m. EDT (hora del este) del 30 de junio escribiendo a: hq-media@mail.nasa.gov. La política de acreditación de medios de la NASA está disponible en línea (en inglés).
La NASA avanza en el desarrollo de la Base Lunar, una iniciativa de exploración e infraestructura lunar a largo plazo diseñada para permitir una presencia humana sostenida y ampliar la actividad científica y comercial en la superficie de la Luna.
Como parte de una edad de oro de innovación y exploración, la NASA enviará astronautas en misiones cada vez más difíciles para explorar más de la Luna con fines de descubrimiento científico y beneficios económicos, y para continuar sentando las bases para las primeras misiones tripuladas a Marte.
Para obtener más información (en inglés) sobre los planes de la NASA para la Base Lunar, visite:
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NASA to Share Latest Moon Base Mission Progress
NASA Administrator Jared Isaacman will host a virtual conversation at 2:30 p.m. EDT, Tuesday, June 30, to share updates to NASA’s plans to build a Moon Base on the lunar surface.
Administrator Isaacman and Carlos García-Galán, Moon Base program manager, will discuss the next set of awards for new lunar lander missions and preview upcoming opportunities as the agency works toward building a sustained presence on the Moon.
The discussion will stream on NASA’s YouTube channel. An instant replay will be available online. Learn how to watch NASA content on a variety of platforms, including social media.
To ask a question virtually during the event, media must RSVP no later than 12:30 p.m., June 30 to: hq-media@mail.nasa.gov. NASA’s media accreditation policy is available online.
NASA is advancing development of the Moon Base, a long-term lunar exploration and infrastructure initiative designed to enable sustained human presence and expanded scientific and commercial activity on the lunar surface.
As part of the Golden Age of innovation and exploration, NASA will send astronauts on increasingly difficult missions to explore more of the Moon for scientific discovery, economic benefits, and to build on our foundation for the first crewed missions to Mars.
For more information about NASA’s Moon Base plans, visit:
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Roman Telescope Comes to Kennedy
In this June 21, 2026, photo, NASA’s Nancy Grace Roman Space Telescope arrives at the agency’s Kennedy Space Center in Florida aboard NASA’s Pegasus barge. After offloading and transportation to the spaceport’s Payload Hazardous Servicing Facility, Roman will undergo processing ahead of launch, targeted no earlier than Sunday, Aug. 30, 2026.
Named for NASA’s first chief astronomer and “mother of the Hubble Space Telescope,” Roman will offer a field of view over 100 times larger than Hubble’s to study up to a billion galaxies, directly image exoplanets and planet‑forming disks, and address fundamental questions about dark energy, exoplanets, and infrared astrophysics.
Image credit: NASA/Amber Jean Notvest
NASA’s HiRISE Captures Perseverance Marking a Milestone on Mars
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NASA’s Perseverance rover appears as a green speck on the Martian surface on June 13, 2026, a day before the robotic explorer marked a distance milestone, having traveled a full marathon (26.2 miles, or 42.195 kilometers) on the Red Planet. Perseverance reached that distance after five years and four months of driving — on the 1,890th Martian day, or sol, of its mission; the previous record holder, NASA’s Opportunity rover, took 11 years and two months to reach the same milestone.
This image was taken by NASA’s Mars Reconnaissance Orbiter (MRO) using its High-Resolution Imaging Science Experiment (HiRISE) camera. The rover’s tracks can be seen tracing the surface. The rover is in an area west of Jezero Crater that the science team is calling “Arbot.”
Figure AFigure A is the same image with a yellow circle indicating Perseverance.
Managed for NASA by Caltech, NASA’s Jet Propulsion Laboratory in Southern California manages operations of the Perseverance rover and MRO on behalf of the agency’s Science Mission Directorate as part of NASA’s Mars Exploration Program portfolio. Lockheed Martin Space in Denver built MRO and supports its operations. The University of Arizona, in Tucson, operates HiRISE, which was built by BAE Systems in Boulder, Colorado.
To learn more about these missions, visit:
https://science.nasa.gov/mars/
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Euclid View of Milky Way Heart Previews Core Survey by NASA’s Roman
A new look at the heart of our Milky Way galaxy by Euclid, an ESA (European Space Agency) mission with NASA contributions, overlaps with a region scientists will observe with NASA’s Nancy Grace Roman Space Telescope, launching later this summer. This sneak peek gives astronomers a major jumpstart on a core Roman survey, helping scientists learn more than they could from either telescope alone.
“This is the only time Euclid has paused its normal sky survey, which is mainly geared toward cosmology,” said Jason Rhodes, a senior research scientist at NASA’s Jet Propulsion Laboratory in Southern California. Rhodes serves as both the U.S. Euclid science lead and the NASA JPL Roman project scientist. “This takes a lot of work and planning, so it really has to be something with a high impact for science. Adding Euclid’s snapshot to Roman’s future survey will help us map our galaxy better and identify hard-to-find cosmic treasures like isolated black holes and rogue planets more easily.”
Euclid took one day out from its six-year prime mission to preview the area of sky that will be targeted by Roman’s Galactic Bulge Time-Domain Survey, which will provide one of the deepest views ever into the center of our galaxy. Though Euclid’s one-time observation is shallower and lacks some of the color detail Roman will see, it has similar resolution and covers a larger region — about 5 square degrees, or the sky area covered by about 25 full moons — since Roman’s survey area hadn’t yet been determined when the observation took place in March 2025.
This artist’s concept outlines the areas of the galactic core covered by Euclid (orange) and the future survey area of the Roman telescope (green). The Euclid observations more than cover Roman’s planned survey area because the Roman coverage wasn’t yet set in stone when Euclid imaged the area. The only exception is the portion right in the galactic center since Euclid’s visible light observations can’t pierce the thick dust in this region like Roman’s infrared vision will. NASA’s Goddard Space Flight CenterOver the course of its five-year primary mission, Roman will repeatedly image a smaller region (1.7 square degrees, or roughly the sky area covered by 8.5 full moons) to watch how hundreds of millions of stars and other objects change over short time periods. Monitoring these changes will reveal hordes of new planets, along with many other cosmic objects and phenomena. Stitching Euclid’s observation onto the front end of Roman’s collection will essentially extend the survey by two years (since Roman’s galactic bulge observations are set to begin in spring 2027), making even more science possible.
Mining hidden gems
Roman will watch for tiny surges in starlight that herald a microlensing event. This light-bending phenomenon occurs when a massive object like a star, planet, or black hole — any object with sufficient gravity — closely aligns with a background star from our vantage point. Light from the distant star curves as it travels through the warped space-time caused by the nearer object’s mass.
This image from Euclid (with color added using ground-based images) zooms in on the center of our Milky Way galaxy. The region gets its golden tone from myriad old, cool stars that have yellowish hues. Stars in this region are heavily crowded, so observing in this direction increases the likelihood of catching microlensing events. ESA/Euclid/Euclid Consortium/NASA, CFHT, image processing by J.-C. Cuillandre and E. Bertin (CEA Paris-Saclay)If the alignment is especially close, the nearer object acts like a cosmic lens, focusing and magnifying light from the background star.
“Most often, the lensing object is another star,” said Matthew Penny, an assistant professor at Louisiana State University, and co-lead of Euclid’s exoplanet science working group who has spent more than a decade simulating both Euclid and Roman data. “But Roman will also be able to detect planets orbiting them, and all kinds of weird objects that are nearly impossible to find any other way.”
Among those strange objects are black holes left behind after the most massive stars die. Astronomers think there should be about 100 million of these stellar-mass black holes in the Milky Way, but so far they’ve almost exclusively detected the invisible objects when they interact with a companion star. Yet most are thought to wander the galaxy alone. Roman will find them even when there’s nothing nearby to reveal their presence.
While microlensing events created by planets are typically hours or days long, black holes pack in so much mass that they can bend light over a larger region of space, creating much longer signals. That means astronomers may need to observe them for years to see the objects move out of alignment.
“The extra two years provided by Euclid give astronomers more time to watch the lens and source star drift apart, making it easier to identify the lens and measure its mass,” said Himanshu Verma, a postdoctoral researcher at Louisiana State University who has been analyzing Euclid images to help scientists predict and better understand the microlensing events Roman is expected to observe.
This image from the Advanced Camera for Surveys instrument on NASA’s Hubble Space Telescope is part of a 1.1-square-degree survey of the center of the Milky Way. Hubble’s full survey, which is made up of more than 350 individual images taken across about 14 months, is smaller but higher resolution than ESA’s Euclid observations and both overlap with the area Roman will cover. By capturing preview images years before Roman begins its microlensing search, Hubble and Euclid provide early reference points that will help astronomers measure the motions of stars and better characterize the planets and other objects Roman discovers.Adapted from Terry et al. 2026While most planet-hunting methods are best at finding scorching worlds tightly hugging their host star, microlensing is better at detecting worlds in orbits larger than Earth’s. That includes planets that whirl around their stars farther away than Neptune orbits the Sun and ones that have been kicked out of their original star systems altogether, now destined to roam the galaxy all alone.
“When Roman finds them, astronomers will be able to cross-reference Euclid’s earlier observations to look for stars near the lensing object, so we can confirm whether a planet is truly rogue or just orbiting very far from its host star,” said David Bennett, a senior research scientist and microlensing expert at the University of Maryland, College Park and NASA’s Goddard Space Flight Center.
Milky Way mapping
Scientists will also pair Euclid data with Roman’s Galactic Plane Survey. This observation program will reveal our home galaxy in unprecedented detail over an area about 400 times larger than the galactic bulge survey. In one month of observations spread across two years, the Roman survey will unveil tens of billions of stars and explore previously uncharted structures.
It’s tricky to study our own galaxy because it’s like trying to map the human body from inside a cell; there’s a lot of stuff in the way. Combining Euclid’s observations with Roman’s will let astronomers watch stars slowly move across the sky. Since stars in different parts of the Milky Way tend to follow different paths, this will help astronomers figure out which part of the galaxy those stars are in.
“One of the most exciting aspects of the Euclid observations is that they give us the chance to test and improve Milky Way models,” Penny said.
Euclid’s one-day detour offers a scientific payout that will last for years and shows how much more can emerge when telescopes team up.
“We’ve shown that these two telescopes can work together to do science that surpasses what either was originally designed for,” Rhodes said. “In doing so, we’ve established a model for future coordinated observations that can unlock far more discoveries than either mission could make alone.”
To learn more about the Roman mission, visit:
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Ashley is the lead science writer for NASA's Nancy Grace Roman Space Telescope.
Share Details Last Updated Jun 24, 2026 EditorAshley BalzerContactAshley Balzerashley.m.balzer@nasa.govLocationGoddard Space Flight Center Related Terms Explore More 7 min read Journey to Center of Milky Way With Upcoming NASA Roman Core Survey Article 5 months ago 6 min read Why NASA’s Roman Mission Will Study Milky Way’s Flickering Lights Article 3 years ago 6 min read NASA’s Roman Mission Preps to Unveil New Populations of Faraway Worlds Article 4 weeks ago Keep Exploring Discover More Topics From NASAMissions
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Career Spotlight: Electrician (Ages 14-18)
Electricity powers the world, and electricians are the ones who get it where it needs to go. An electrician is an expert who is trained to make sure electrical systems and equipment are installed safely and working correctly. Electricians are involved in a variety of systems, including power, lighting, communications, and more – anything that needs electricity to run.
While electricians ensure systems and equipment have the power they need, electrical technicians focus on building, modifying, or testing electronic devices.
What are some of the different types of work electricians and electrical technicians do at NASA?At NASA, electricians keep the lights on and the power flowing for rocket launches, scientific research, and everything in between. Their skills support engineers and scientists in building and testing spacecraft, aircraft, satellites, telescopes, and the equipment that makes human spaceflight possible. Electricians make sure all facilities and equipment have the power and functionality they need to be safe and ready to support NASA’s missions.
Electrical technicians at the agency help bring big ideas to life. They might build and wire control systems, connect tiny sensors to circuit boards, or write the software to make a device work in a specific way. They also test instruments in conditions that mimic space – extreme temperatures, intense vibrations, and even a vacuum – to make sure they will survive and perform well during their missions. Technicians use specialized tools, earn certifications, and work with incredible precision.
Being an electrician or electrical technician at NASA is careful, hands‑on work carried out with expertise. Because space hardware is headed to places like low-Earth orbit, the Moon, or even Mars, every detail has to be perfect.
What are the different certification levels for electricians?The information below is a general overview of the career path of an electrician. Specific guidelines for these roles vary from state to state. It’s important to look up the license requirements in your state.
- Apprentice electrician: This four-year job training program provides an entry into the industry. An apprentice works as an assistant to an experienced supervisor, gaining vital hands-on experience to move ahead as an electrician.
- Journeyman electrician: A journeyman is an electrician who has finished an apprenticeship, then passed a test. At this stage, the electrician is licensed and allowed to work without supervision.
- Master electrician: This is the highest certification possible for an electrician. Typically, a master electrician is someone who has completed approximately 4,000 hours as a journeyman, then passed a licensing exam. These electricians are qualified to work on complicated projects. They can also serve as supervisors for apprentices or journeymen following in their footsteps.
There are many options that provide the training needed to get started as an electrician or electrical technician.
Many community colleges, trade schools, and technical institutes offer a two-year program leading to an associate degree in electrical technology. Additionally, trade unions and apprenticeship programs provide real-world experience in the field.
Additionally, all branches of the U.S. military offer electronics training that may be transferrable to college credits or civilian certifications.
How can I start preparing today to become an electrician?It’s never too early to set the stage for an electrifying career! In high school, you can take courses in math, science, and technical education. At the same time, you can start learning about basic electrical concepts such as circuitry and safety.
Begin researching associate degree programs and apprenticeship opportunities so you can consider which pathway seems right for you. Weighing these options now will help you understand program requirements and ensure you’re ready to take the next step.
You can also gain useful experience through part-time work, or shadowing electricians on the job.
What skills will I need to be a successful electrician?Technical skills focus on the basics – how electricity works, how to stay safe, and how to read schematics and wiring diagrams. Some jobs also call for special hands‑on abilities, like soldering tiny components, putting together cables, or even having some familiarity with chemistry.
Being curious, open‑minded, and a good communicator matters, too. Any time you’re building or improving a device, you must understand who will use it and what they need it to do. Asking questions, sharing ideas, and being able to take feedback are essential to consistently building systems and devices that work well.
David McClaeb, electronic technician, NASA’s Goddard Space Flight Center in Greenbelt, Maryland Advice from NASA electricians and electronic technicians“As an aerospace technician, you have the opportunity to make a big difference. You can make a really big impact.” – Christopher Johnson, aerospace electrical engineering technician, NASA’s Kennedy Space Center in Florida
“What I wish I knew in high school is how many opportunities there are for electricians. I didn’t realize how big of a scale it really was. Everything needs electricity, and the sky’s the limit on what you can do with it. NASA needs electricians for everything from their testing campaigns to keeping their facilities running.” – Levi James, electrician apprentice, NASA’s Glenn Research Center at Armstrong Test Facility in Sandusky, Ohio
“It’s so gratifying when somebody comes in and says, ‘Hey, we want to build this, but it looks really difficult,’ and we say, ‘Yeah, it looks difficult, but we can do it’ – and we build it and then we hand it over to them, and then we’re on to the next thing. It’s a challenge, and I’m telling you, it is just so fun.” – David McClaeb, electronic technician, NASA’s Goddard Space Flight Center in Greenbelt, Maryland
Additional resources- Occupational Outlook for Electricians: Pay, Education, Job Outlook, and More (From the U.S. Bureau of Labor Statistics)
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Curiosity Blog, Sols 4927–4933: Let’s Drive to That Smooth Area
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Curiosity Blog, Sols 4927–4933: Let’s Drive to That Smooth Area NASA’s Mars rover Curiosity acquired this image showing a breathtaking diversity of polygons, veins, and other textural features waiting for investigation by the Mars Science Laboratory team. Curiosity captured the image using its Left Navigation Camera on June 17, 2026 – Sol 4928, or Martian day 4,928 of the Mars Science Laboratory mission – at 17:47:52 UTC. NASA/JPL-CaltechBy Susanne P. Schwenzer, Professor of Planetary Mineralogy at The Open University, UK
Earth planning date: Thursday, June 18, 2026
In the area Curiosity is currently exploring, the science team has mapped several areas with different-looking surface texture on the orbital images. If you wanted to have a look yourself at what there is to see, check the “Where is Curiosity?” map. You’ll discover different shades of orange and beige as well as more rough and more smooth-looking textures. This is what the geomorphologists in our team use to map the areas for exploration by the rover. Of course, we then supplement this all with ground-based images, including bespoke “drive direction imaging,” which is taken after each drive by the Mast Camera. Drive planning is done using a combination of all this information. So there shouldn’t be any surprises, right?
On Monday the team planned three sols in preparation for a Thursday planning to account for the U.S. federal holiday weekend. The workspace turned out to be a little spiky, so we could not find an area we could DRT. APXS still found one good bedrock target, “Rio Baker,” which also had MAHLI documentation. In addition, ChemCam investigated “Rica Aventura,” a textured bedrock, and “Tabebuia,” a darker-looking individual block, using its LIBS and conducted a passive spectral observation on a second dark float block called “Lago Ranco.” Of course, the team also wanted to look into the distance with ChemCam remote imaging, extending our investigation of the Cordillera base outcrop.
Imaging is always high on the list. In Monday’s plan Mastcam is looking into the modern dunes with the “Tacaza” mosaic, and with more mosaics looking forward to the future parking areas, some of which looked really smooth from that vantage point. We also continue our environmental and atmospheric observations looking for dust devils, the opacity of the atmosphere, and monitoring pressure and temperature. After all this, the rover drove about 35 meters (about 115 feet) to an area that looked really smooth in all images we had available at that point. So we were hoping for a good spot to deploy the DRT, but didn’t think we could be in for a surprise.
The drive ended exactly as planned, spot-on in the middle of that — from a distance — smooth-looking area. But when we opened the post-drive images on Thursday morning, we were all reacting with a lot of surprise. From up close, the parking spot looks anything but smooth. You can see the surprise in the title image of this blog. There are polygons, veins, lamination, and probably more, once we inspect the higher-resolution images taken today. “Higher-resolution” is the key for why we were in for such a surprise! The features are quite small, a few centimeters across, and therefore we could not see them in the orbital images or from a distance in our navigation and mast camera images. The camera resolution from a distance just isn’t enough to see them. But up close, the terrain revealed all its beauty! And I am sure there will be more in the even higher resolution of today’s MAHLI and ChemCam RMI imager images!
So, what did we plan after we caught our breath on Thursday? First, you guessed it, images, images, and more images. Mastcam takes a full panorama with its “left eye” and adds a range of closer-up mosaics with its higher-resolution “right eye.” In addition there is a ChemCam Remote Micro Imager image to document structures further afield at high resolution. ChemCam is investigating three targets using LIBS: “Rio Chimore” is a lighter-toned band; you can see some of those in the cover image of this blog, too. The other two LIBS targets are “Rio de Lava,” a vein target, and “Rio de Salta,” one of the polygons. APXS is also looking at the bedrock and the ridges, at the targets “Pampa Grande” and “Iquique Ridge.” MAHLI is having the above-mentioned close “hand lens” look. Let’s see what we will discover when we get those images.
Finally, Curiosity drove up the hill along very smooth-looking terrain that is just littered with tiny polygons. Let’s see if we are in for another surprise reverberating around all our offices — and across two continents, as I had the good fortune to be among the first ones, here in England (Or maybe it was our French ChemCam colleagues, who are in a time zone one hour ahead of me?). Whichever it is, this terrain has a lot to say about the geologic history of Mars!
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NASA Names Sean Gallagher as Chief Information Officer
NASA has selected Sean Gallagher as the agency’s chief information officer (CIO). In this role, he is responsible for the agency’s entire portfolio of Information Technology products and services. Gallagher has been serving in an acting capacity since January and his permanent role is effective immediately.
“Sean Gallagher’s leadership has been instrumental in strengthening NASA’s IT foundation and ensuring our workforce has the secure, modern tools needed to enable groundbreaking missions every day,” said NASA Deputy Administrator Matt Anderson. “As CIO, Sean will continue advancing the agency’s technology capabilities to support discovery, innovation, and mission success across NASA.”
Most recently, Gallagher also has served as the deputy chief information officer for Operations in the Office of the Chief Information Officer at NASA Headquarters in Washington, as well as a senior advisor for Transformation. This team provides services to tens of thousands of end users located in the U.S. and abroad in support of NASA missions, enabling discoveries, faster data sharing, increased workforce productivity, and more. Gallagher has worked with all NASA centers to implement efficient and effective IT operating models.
Previously, Gallagher was the CIO of NASA’s Glenn Research Center in Cleveland, leading IT initiatives for aeronautics, space, research and engineering, and test missions. He joined NASA in 2012 as Glenn’s deputy CIO and previously worked at Booz Allen Hamilton as a senior associate supporting a variety of federal, defense, and commercial customers.
Gallagher developed his leadership and management experience as a Signal Corps officer in the United States Army. He also served as a platoon leader managing the combat service support readiness of a tactical communications unit, a human resource manager for the 40th Signal Battalion, and as a network engineer for the 11th Signal Brigade. He has a bachelor’s degree in physics from John Carroll University and a master’s degree in computer information systems from the University of Phoenix.
For more information about NASA’s missions, visit:
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Camille Gallo / Cheryl Warner
Headquarters, Washington
202-358-1600
camille.m.gallo@nasa.gov / cheryl.m.warner@nasa.gov
CSDA Selects Eight Commercial Satellite Data Providers for On-Ramp 2 Contract Awards
NASA’s Commercial Satellite Data Acquisition program (CSDA) announced contract awards with eight commercial satellite data providers offering a range of data types to support the agency’s Earth science research and application goals.
The CSDA program On-Ramp 2 Multiple Award contract is a firm-fixed-price indefinite-delivery/indefinite-quantity (IDIQ) multiple-award contract with a maximum cumulative value of $476 million and a performance period through November 2028.
The CSDA IDIQ contract includes an on‑ramp provision that allows NASA to periodically reopen the solicitation, giving new vendors the opportunity to submit proposals. This mechanism also enables existing CSDA vendors to propose new data products, whether newly developed or derived from new instruments, that were not available during the original proposal period.
Newly Added Contract Holders
Vendor Sensor HydroSat Thermal Infrared Visible and Near-Infrared (VNIR) Ororatech Thermal Infrared – Medium Wavelength Infrared (MWIR) and Long Wavelength Infrared (LWIR) ImageSat Optical Multispectral Instrument (MSI) Satlantis Optical MSI / Greenhouse Gas (GHG) Emissions Kuva Space Hyperspectral – VNIR and Short Wavelength Infrared (SWIR) Wyvern Hyperspectral – VNIR Orbital Sidekick Hyperspectral – VNIR and SWIR Muon Space Global Navigation Satellite System – Radar (GNSS-R)Current CSDA Contract Holders with New Products
Vendor Sensor Airbus Optical MSI / Synthetic Aperture Radar (SAR) ICEYE SAR GHGSat GHG Emissions Planet Labs Optical MSI / Hyperspectral PlanetiQ Global Navigation Satellite System – Radio Occultation (GNSS-RO) Tomorrow.io Microwave Sounder“NASA’s Earth science community relies on a diverse suite of observations from spaceborne, airborne, and in situ assets to better understand our changing planet,” said CSDA Project Manager Dana Ostrenga. “The commercial providers added through this latest CSDA contract on-ramp complement NASA’s existing Earth observation capabilities and our current portfolio of commercial partners, expanding the range of data available for evaluation and use. Together, these observations provide researchers with a more comprehensive view of Earth’s atmosphere, land, oceans, cryosphere, and solid Earth, helping advance scientific discovery and applications that benefit our communities.”
Following issuance of the contract awards, the selected vendors’ data products will be made available to authorized CSDA data users via the Satellite Data Explorer (SDX), CSDA’s web-based data discovery and data access tool that allows approved users to search, discover, access, task, and download the data the program has acquired from its commercial partners.
The Vendor Selection ProcessThe award process begins with the CSDA issuing a request for proposals that is posted on Sam.gov, the U.S. government’s official system for managing federal contract proposals. Interested companies then submit proposals to enter into an IDIQ contract with CSDA. A Solicitation Evaluation Board is formed to determine whether the proposals are competitive and meet the CSDA’s technical requirements for continuous observations, orbit platforms, and data that aligns with NASA Earth Science Division (ESD) goals. The CSDA makes its selections from the proposals that meet the requirements and then submits them to NASA leadership for approval. Once approved, the contracts are then awarded and the companies are able to get their data evaluated by CSDA. Once the evaluations are complete, the commercial data providers can then compete for competitive task orders through CSDA.
About the CSDA ProgramNASA’s Earth Science Division (ESD) established the CSDA Program as the agency’s central mechanism for identifying, acquiring, and evaluating commercial Earth observation (EO) data. The program augments NASA’s and partner agencies’ Earth-observing capabilities by acquiring commercial satellite data that offer higher spatial resolution, increased revisit frequency, complementary measurement capabilities, and taskable observations. To learn more about the program, its commercial partners, data evaluation process, and more, visit the CSDA website.
Become an Authorized Data UserCommercial data discoverable through the SDX is made available to CSDA authorized data users. To become an authorized user, fill out the CSDA Program Data Authorization Form. Note: Use of SDX also requires an Earthdata Login.
58th Girl Scouts Unite Event
58th Girl Scouts Unite Event, July 23-25, 2026
Join NASA in the Exhibit Hall (Booth #206) for Hyperwall Storytelling by NASA experts. Full Hyperwall Agenda below.
Thursday, July 23
11:00AM – 11:15 AM From Daisy to NASA Engineer Barbara Hilton 11:15AM – 11:30 AM Exploring Mars, The Planet Next Door Lindsay Hays 11:30AM – 11:45 AM Get Ready With Me: Going to the Moon Naoma McCall 11:45Am – 12:00 PM NASA Is for Everyone! (talk about careers at NASA beyond science and engineering) Amy Kaminski 12:00PM – 12:15 PM Finding Asteroids Before They Find Us: Planetary Defense at NASA Kelly Fast
2:15 PM – 2:30 PM How to Nerd Your Way Into Science Communications Karen Romano Young 2:30 PM – 2:45 PM Earth: Exploring our home planet is a team effort Lesley Ott 2:45 PM – 3:00 PM TBD Jenny Mottar 3:00 PM – 3:15 PM The Journey Starts HERE: One CREW, Your HOME, Our MISSION Kaitlin Harbeck 3:15 PM – 3:30PM TBD – Artemis Overview Dominique Brewer 3:45 PM – 4:00 PM Social Media… For Science! Sofie Bates
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2026 ALA Hyperwall Schedule
2 min read
2026 ALA Hyperwall ScheduleAmerican Library Association (ALA) Annual Conference, June 25-29, 2026
Join NASA in the Exhibit Hall (Booth #2243) for Hyperwall Storytelling by NASA experts. Full Hyperwall Agenda below.
FRIDAY, JUNE 26
- 5:45 PM ——Roman Space Telescope Quiz! —— Peter Sooy
- 6:00 PM ——NASA’s Next Flagship is Launching Soon! Share in the Excitement with Roman Community Events —— Martha Irene Saladino
- 6:15 PM ——Open Science Resources for Libraries ——Amanda Adams
- 6:30 PM ——Launching NASA Earth Science Exhibits in Libraries Across America ——Eleanor Stokes
- 6:45 PM ——NASA Citizen Science Projects——Sarah Kirn
SATURDAY, JUNE 27
- 10:00 AM——Heliophysics Jeopardy!——Erin Mahoney
- 10:15 AM——NASA’s Next Flagship is Launching Soon! Share in the Excitement with Roman Community Events——Martha Irene Saladino
- 10:30 AM——Nancy Grace Roman: The Person——Courtney Lee
- 10:45 AM——Cosmic Canvas: Exploring the Process of Science Through Art and Astronomy——Tim Rhue
- 12:30 PM——Roman Space Telescope Quiz! —— Peter Sooy
- 1:00 PM——“Our Friend Orion” Children’s Book Reading——Lane Polak
- 2:30 PM——Heliophysics Jeopardy!——Erin Mahoney
- 3:00 PM——”The Adventure of Echo the Bat” Book Reading——Ginger Butcher
- 3:30 PM——Bring a NASA Solar System Ambassador to YOUR Library!——Danielle Diamond
- 3:45 PM——Journey Through the Heliosphere: The Sun-Earth System in Color——Christine Milotte
SUNDAY, JUNE 28
- 10:00 AM——Webb Space Telescope Quiz!——Peter Sooy
- 10:15 AM——Journey Through the Heliosphere: The Sun-Earth System in Color——Christine Milottet
- 10:30 AM——Science Explorer (SciX) Demo——Daniel Chivvis
- 10:45 AM——NASA Data and Open Science Quiz!——Adam Farragut
- 12:30 PM——Heliophysics Jeopardy!——Erin Mahoney
- 1:00 PM——“There and Back with EGS” Children’s Book Reading——Lane Polak
- 2:30 PM——Real NASA Research Projects Open to Everyone——Sarah Kirn
- 3:00 PM——Cosmic Canvas: Exploring the Process of Science Through Art and Astronomy——Tim Rhue
- 3:30 PM——NASA’s Next Flagship is Launching Soon! Share in the Excitement with Roman Community Events—— Martha Irene Saladino
- 3:45 PM——Journey Through the Heliosphere: The Sun-Earth System in Color——Milotte
MONDAY, JUNE 29
- 9:45 AM——Webb Space Telescope Quiz!——Peter Sooy
- 10:00 AM——“Hooray for SLS” Children’s——Lane Polak
- 10:30 AM——Bring a NASA Solar System Ambassador to YOUR Library!——Mark Benson
This is How NASA Flight Tests New Technology
Flight tests are a big part of how NASA turns breakthrough ideas into reality. From flying humans faster than the speed of sound to proving designs that helped shape the space shuttle, flight testing transforms bold concepts into safer, more efficient technologies that benefit the public.
“Flight tests are a way to safely and effectively prove new technology, which helps certification authorities certify equipment,” said Wayne Ringelberg, chief pilot at NASA’s Armstrong Flight Research Center in Edwards, California. “It helps industry iterate and make systems better, and it promotes research in areas where new ideas can be developed.”
For nearly 80 years, teams at NASA Armstrong have used flight testing in the Southern California desert to push the limits of aerodynamics and advance aviation. Thanks to that work, NASA-developed innovations are aboard every U.S. commercial aircraft and inside every control tower today.
“The space side of NASA uses flight test, too. Every mission, like Artemis II, is never routine,” Ringelberg said. “Everything we’re doing when flying a test mission is something new or different.”
NASA test pilots Jim Less, left, and Nils Larson walk away from a hangar at NASA’s Armstrong Flight Research Center in Edwards, California, on Thursday, Feb. 4, 2026. The pilots support the agency’s Crossflow Attenuated Natural Laminar Flow (CATNLF) project, which aims to lower fuel costs for future commercial aircraft by testing a scale-model wing designed to improve laminar flow.NASA/Christopher LC ClarkEvery NASA test flight — whether it’s studying new software, hardware, or the revolutionary technology of an experimental X-plane — relies on engineers, researchers, pilots, maintenance crew, control room operators, and many others working together.
“Experienced operators and engineers evaluate how things work in flight,” Ringelberg said. “Most new technologies are designed to work in a lab or can be tested in a wind tunnel or other facility, but you never really know how they’ll perform until you fly them.”
Preflight tests often include computer analysis, simulation, wind tunnel testing, and ground tests focused on an aircraft’s ability to withstand the forces of flight and the environments through which it may fly. After hardware or software is deemed safe to fly, researchers turn the mission over to the flight test team.
To support testing, NASA Armstrong maintains an aircraft fleet modified to create space for new hardware or instruments, as well as the ability to integrate new software. These aircraft are flying laboratories, and pilots are trained to accomplish experimental missions.
An F-15 research aircraft sits on the ramp at NASA’s Armstrong Flight Research Center in Edwards, California, on Tuesday, March 17, 2026. NASA pilots Jim Less, front seat, and Carrie Worth prepare for the flight. The agency’s Crossflow Attenuated Natural Laminar Flow (CATNLF) test article is attached to the bottom of the F-15. The project aims to lower fuel costs for future commercial aircraft by testing a scale-model wing designed to improve laminar flow.NASA/Carla EscamillaFor example, flight testing recently helped NASA gather critical data on laminar flow, or the smooth flow of air, over a wing. The work could lower fuel costs for future airliners. Computer modeling, wind tunnel tests, and other methods helped advance the research, but to find out even more about how the wing concept could reduce drag for future airliners, NASA used a scale model in actual flight.
NASA researchers strapped the Crossflow Attenuated Natural Laminar Flow (CATNLF) model wing to the belly of one of NASA Armstrong’s F-15s. The arrangement allowed them to collect all the information they would need without doing the extensive, costly modifications required to install a full-scale wing on an aircraft.
After a flight series is complete, engineers and researchers analyze the data. Did the instrument work as designed? Did the experimental aircraft perform safely at a high altitude? Did the software operate as planned? Each test raises its own set of questions to evaluate.
NASA continues working with academia, the Department of War, and industry partners to advance U.S. aviation through flight test and bring new benefits to the flying public.
Share Details Last Updated Jun 22, 2026 EditorDede DiniusContactTeresa Whitingteresa.whiting@nasa.gov Related Terms Explore More 9 min read ARMD Research Solicitations (Updated June 23) Article 11 hours ago 3 min read NASA’s Experimental Fabrication Branch Fuels Aircraft Innovation Article 1 day ago 5 min read NASA, USGS Scientists Go Rock Hounding in California’s High Desert Article 2 weeks ago Keep Exploring Discover More Topics From NASAMissions
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Hanging in the Balance
The Moon appears half-illuminated in this photo captured by the Artemis II crew on flight day 6. The terminator – the difference between light and darkness – provides a stark contrast and even greater perspective of the Moon’s rocky, uneven, and otherworldly surface features. The near side, which is what we can see from Earth, appears in the dark gray regions at the top of this image.
Revisit imagery from the Artemis II mission.
Image credit: NASA
ARMD Research Solicitations (Updated June 23)
9 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) NASA / Lillian Gipson/Getty ImagesTHIS PAGE WAS UPDATED ON JUNE 23, 2026
This Aeronautics Research Mission Directorate (ARMD) solicitations page compiles the opportunities to collaborate with NASA’s aeronautical innovators and/or contribute to their research to enable new and improved air transportation systems.
Most opportunities to participate in research are officially announced through the Web-based NASA Solicitation and Proposal Integrated Review and Evaluation System, better known as NSPIRES. You are encouraged to visit the NSPIRES web site, create an account, and sign up for automated email announcements.
Other types of collaborative opportunities, such as those involving Requests for Information or academic research contests, also are included on this page.
This ARMD Solicitations page has four major sections:
- Quick list of open solicitations with key dates listed.
- Current open solicitations with more details and helpful links.
- Closed solicitations in case it is helpful to see other examples of the kind of research opportunities NASA Aeronautics makes available.
- Summary of NASA’s Research Opportunities in Aeronautics (ROA) NASA Research Announcement (NRA) selection process.
August 3, 2026
Deadline for proposals on Open Fan Flight Demonstrations NRA
As part of NASA’s Advanced Air Vehicles Program, the Subsonic Vehicle Technologies and Tools project endeavors to advance knowledge, technologies, and concepts that enable accelerated introduction of radical aircraft and engine technologies across a range of vehicle classes.
This is achieved through partnerships with industry to ensure that these technologies are applicable to planned products to increase the chances of inclusion in future aircraft systems.
This research announcement solicits proposals for providing an open fan flight demonstration plan with optional accompanying risk reduction activities. The flight demonstration plan will inform the project of the scope of a possible future flight demonstration and provide insight into the roadmap, risk reduction areas, and areas of potential investment.
See the full research announcement text on SAM.gov.
Proposals Due: August 3, 2026, by 5:00 PM EDT
The Project F.I.R.E. team receives their “Future Game-Changer” award during the 2024 Gateways to Blue Skies forum held at NASA’s Ames Research Center in California. Gateways to Blue Skies is one of several Aeronautics Innovation Challenges open to the academic community.NASA / Brandon Torres Aeronautics Innovation Challenges – OPENNASA’s nationwide team of aeronautical innovators are committed to giving students of all ages opportunities to solve some of the biggest technical challenges facing the aviation community today. Through NASA-sponsored challenges and competitions, students representing multiple disciplines will put their skills to work by designing and building solutions to real-world problems.
See the Complete List of Challenges Currently Closed Solicitations NASA’s X-59 quiet supersonic research aircraft lifts off for its first flight Tuesday, Oct. 28, 2025, from U.S. Air Force Plant 42 in Palmdale, California. The aircraft’s first flight marks the start of flight testing for NASA’s Quesst mission, the result of years of design, integration, and ground testing and begins a new chapter in NASA’s aeronautics research legacy.NASA/Lori Losey NASA ARMD Aeronautics Flight Accelerator – CLOSEDNASA’s Aeronautics Research Mission Directorate is seeking information from U.S. industry, academia, and government organizations regarding potential partnerships for research, development, and flight testing under the Aeronautics Flight Accelerator initiative. NASA is requesting input on technologies, concepts, and flight test campaigns suitable for cost shared maturation leading to flight within the next three years. Areas of interest span subsonic (including vertical lift), supersonic, and hypersonic flight technologies.
THIS IS NOT A REQUEST FOR PROPOSAL. NO PROPOSALS SHOULD BE SUBMITTED.
RFI Release Date: April 7, 2026
Responses Were Due: May 7, 2026, 1:00PM Pacific Daylight Time (PDT)
For more detailed information, see the RFI listing on SAM.gov.
High school students visit the Glenn Research Center Manufacturing Facility and learn about careers in the STEM manufacturing field.NASA/Marvin Smith FY26 NASA Aerospace Skilled Technical Workforce Hubs (NAS_Hub) – CLOSEDThis opportunity seeks proposals to establish state or regionally focused Skilled Technical Workforce Hubs (NAS_Hubs) that will serve as strategic centers for developing and sustaining a skilled technical workforce aligned with aerospace industry and NASA mission needs. The NAS_Hub Notice of Funding Opportunity has been released and may be found in NASA’s Solicitation and Proposal Integrated Review and Evaluation System (NSPIRES) on the NAS_Hub landing page.
Key Dates
- Pre-Proposal Webinar: February 18, 2026, 2:00 to 3:00 p.m. ET
- Office Hours Session: March 3, 2026, 2:00 to 3:00 p.m. ET
- Proposal Deadline: March 23, 2026, at 11:59 p.m. ET
- Anticipated Award Notification: June 2026
About the Opportunity
The rapid expansion of the space economy and renewed national priorities in human space exploration have created an urgent demand for a robust skilled technical workforce—individuals in critical science- and engineering-based roles who do not require a bachelor’s degree. To address nationwide shortages and ensure U.S. competitiveness in aerospace and defense, NASA’s Office of STEM Engagement is launching the NASA Aerospace Skilled Technical Workforce Hubs (NAS_Hub) initiative.
Through this notice NASA seeks lead organizations to establish hubs that:
- Collaborate with aerospace employers to align education and training with industry-defined workforce needs.
- Partner with community colleges and high school Career and Technical Education programs to deliver hands-on, industry-aligned learning experiences.
- Coordinate with state or regional workforce development system.
- Build clear and sustainable employment pathways into high-demand aerospace technical careers.
NAS_Hubs will serve as focal points for aligning education, workforce, industry, and government partners to accelerate workforce readiness over a three-year period of performance.
Eligibility
Eligible applicants include:
- State, county, city, township, special district, and tribal governments
- Public and private institutions of higher education
- Nonprofit organizations
- For-profit organizations and small businesses
Proposals must include partnerships with, at a minimum:
- Three aerospace industry collaborators supporting NASA’s work
- Community college career and technical education program
- High school career and technical education program
- State or regional workforce development system
- NASA Center or other NASA facility
Award Information
- Maximum Annual Award: $500,000
- Maximum Total Award: $1,500,000 over three years
- Cost Sharing: Not required
How to Apply
Proposals must be submitted electronically via NSPIRES. Registration in NSPIRES and an active SAM.gov registration are required.
Pre-Proposal Webinar and Technical Assistance
NASA will host an interactive pre-proposal webinar for the NAS_Hub opportunity on Feb. 18, 2026, from 2:00 to 3:00 p.m. ET. This session will provide an in-depth overview of this funding opportunity, including program goals, eligibility requirements, proposal preparation guidance, and submission tips. Proposers will also have the opportunity to receive technical assistance and clarification from NASA staff. Prior to attending a webinar, proposers are strongly encouraged to review the full NAS_Hub notice and to check the NAS_Hub landing page in NSPIRES regularly for updates and additional guidance.
Please note that registration is required for the webinar. Connection details will be provided upon completion of registration. Webinar dates, times, registration links, and connection information will be posted on the NAS_Hub landing page in NSPIRES, which also will feature recordings and presentation materials from the webinar after the event for those unable to attend.
Office Hours Session
March 3, 2026, 2:00 to 3:00 p.m. ET
Last opportunity for questions prior to the proposal deadline. Join the office hours session here.
Contact Information
For technical assistance with NSPIRES
NSPIRES Help Desk available Monday–Friday, 8:00 AM–6:00 PM ET
(202) 479-9376
nspires-help@nasaprs.com
Program Contact
Maria Arredondo
Next Gen STEM Program Manager
NASA Office of STEM Engagement
Mary W. Jackson NASA Headquarters
Email: NAS_Hub@nasaprs.com
Advanced Capabilities for Emergency Response Operations RFI – CLOSEDView the full ACERO RFI announcement here.
NASA’s Advanced Capabilities for Emergency Response Operations (ACERO) project used this request for information to identify technologies that addressed current challenges facing the wildland firefighting community. NASA was seeking information on data collection, airborne connectivity and communications solutions, unmanned aircraft systems traffic management, aircraft operations and autonomy, and more. This would support development of a partnership strategy for future collaborative demonstrations.
Interested parties were requested to respond to this notice with an information package submitted via https://nari.arc.nasa.gov/acero-rfi no later than 4 pm ET, October 15, 2023. Submissions were accepted only from U.S. companies.
Advanced Air Mobility Mission RFI – CLOSEDView the full AAM RFI announcement here.
This request for information is being used to gather market research for NASA to make informed decisions regarding potential partnership strategies and future research to enable Advanced Air Mobility (AAM). NASA is seeking information from public, private, and academic organizations to determine technical needs and community interests that may lead to future solicitations regarding AAM research and development.
This particular RFI is just one avenue of multiple planned opportunities for formal feedback on or participation in NASA’s AAM Mission-related efforts to develop these requirements and help enable AAM.
The respond by date for this RFI closed on Feb. 1, 2025, at 6 p.m. EST.
ROA-2025 NRA Amendment 1 – CLOSEDAdvanced Air Vehicles Program Fellowship Opportunities
(View the full ROA-2025 NRA Amendment 1 text here.)
This announcement solicits proposals from accredited U.S. institutions for research training grants to begin the academic year. This Notice of Funding Opportunity is designed to support independently conceived research projects by highly qualified graduate students in disciplines needed to help advance NASA’s mission, thus affording these students the opportunity to directly contribute to advancements in STEM-related areas of study. These opportunities are focused on innovation and the generation of measurable research results that contribute to NASA’s current and future science and technology goals.
Research proposals are sought to address the key challenges summarized in the Elements section at the end of the Amendment 1 document, and which reference NASA’s Hypersonic Technology project.
Reflecting the Fiscal Year 2026 budget changes, the Transformational Tools & Technologies project opportunities originally described in this announcement were cancelled. Proposals citing this project will not be evaluated.
Notices of Intent are not required.
A budget breakdown for each proposal is required, detailing the allocation of the award funds by year. The budget document may adhere to any format or template provided by the applicant’s institution. Two pre-proposal teleconferences for potential proposers will be held and meeting links will be posted on NSPIRES.
Proposals were due by 5 p.m. EDT on June 11, 2025.
NASA Research Opportunities in AeronauticsCompetition for NRA awards is open to both academia and industry.
The current open solicitations for ARMD Research Opportunities are ROA-2024 and ROA-2025.
Here is some general information to know about the NRA process.
- NRA solicitations are released by NASA Headquarters through the Web-based NASA Solicitation and Proposal Integrated Review and Evaluation System (NSPIRES).
- All NRA technical work is defined and managed by project teams within these four programs: Advanced Air Vehicles Program, Airspace Operations and Safety Program, Integrated Aviation Systems Program, and Transformative Aeronautics Concepts Program.
- NRA awards originate from NASA’s Langley Research Center in Virginia, Ames Research Center in California, Glenn Research Center in Cleveland, and Armstrong Flight Research Center in California.
- Competition for NRA awards is full and open.
- Participation is open to all categories of organizations, including educational institutions, industry, and nonprofits.
- Any updates or amendments to an NRA is posted on the appropriate NSPIRES web pages as noted in the Amendments detailed below.
- ARMD sends notifications of NRA updates through the NSPIRES email system. In order to receive these email notifications, you must be a Registered User of NSPIRES. However, note that NASA is not responsible for inadvertently failing to provide notification of a future NRA. Parties are responsible for regularly checking the NSPIRES website for updated NRAs.
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Share Details Last Updated Jun 23, 2026 EditorJim BankeContactJim Bankejim.banke@nasa.gov Related TermsI Am Artemis: Jason Peterson
Jason Peterson’s responsibilities for NASA’s Artemis II mission went beyond his usual role as the range operations manager at NASA’s Stennis Space Center near Bay St. Louis, Mississippi.
For Peterson, working at NASA is a surreal full-circle moment.
“I grew up in DeLisle, Mississippi, right down the road from NASA,” said Peterson. “You would hear NASA testing, the windows would shake, and you knew they were out there. Not in a million years would I have ever dreamed I would work with NASA.”
His career journey took a few turns before reaching the space agency.
“I got out of school, welded, went to college and then to the Air Force. The path to NASA really started to develop from there,” said Peterson.
Peterson spent 24 years in the U.S. Air Force and Air National Guard, working in airfield and air-to-ground range operations, followed by a few years working as an aircraft dispatcher at Airbus Final Assembly Line.
Peterson credits his military experience with preparing him for the 12-to-16-hour workdays that helped bring the Artemis II test flight around the Moon and into view for audiences around the world.
He supported the team responsible for delivering video and communication feeds for the launch of NASA’s SLS (Space Launch System) rocket with the Artemis II crew aboard the Orion spacecraft, and then splashdown in the Pacific Ocean.
During the nearly 10-day mission, NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen completed a record-setting lunar flyby, taking them 252,756 miles at their farthest distance from Earth.
Aboard the USS John P. Murtha, Peterson was the first on the ship to spot the capsule returning with the crew.
“The sonic boom was the moment it truly hit me. Even though I was tracking the capsule, it did not fully register until then. Chills went down my neck and back. You realize our astronauts are coming home. It was an incredible and emotional moment.”JASON PETERSON
Range Operations Manager for NASA Stennis
Jason Peterson, NASA Stennis range operations manager, is shown with the Orion spacecraft aboard the USS John P. Murtha on April 13, 2026. Peterson was the first to spot the capsule returning with the Artemis II crew as he supported the team responsible for delivering video and communication feeds during splashdown operations. Credits: NASANASAPeterson operated one of six cameras providing live coverage by using a high‑resolution, multi‑sensor system with thermal capabilities. Using the ship’s heading and Orion’s predicted trajectory, he located the capsule within minutes and began tracking it.
Orion entered Earth’s atmosphere at about 400,000 feet above the planet’s surface, traveling nearly 35 times the speed of sound and about 1,956 statute miles from its splashdown point off the coast of California. Peterson tracked Orion from the release of the small parachutes that first slow and steady the capsule, through the main parachutes opening, and all the way to splashdown.
“You are fully locked in, keeping it centered, in focus, and steady,” said Peterson.
Peterson’s focus on the mission began weeks earlier at NASA’s Kennedy Space Center in Florida.
In the days leading to launch, Peterson worked with the team running full systems checks, staging communications gear, and preparing drones and fixed‑wing camera assets. He helped configure and operate the systems that ensured live video flowed from the launch pad, the crowds, and surrounding air and ground platforms.
On April 1, the launch day of Artemis II, the team unloaded and set up high‑resolution sensors, connection terminals, routers, monitors, fiber lines, and drone equipment. They flew drones to capture crowd scenes and aerial views before liftoff.
As the SLS rocket launched, Peterson’s full attention was on positioning the drone and maintaining the shot.
“There is not much time to step back and take in the moment, as you are concentrating on precision,” said Peterson.
As the mission got underway, Peterson and the team packed up, returned to the facility, and downloaded the day’s footage.
The Artemis II crew were more than halfway to the Moon as Peterson arrived in San Diego on April 4. In the days leading to splashdown, the team loaded and installed high‑fidelity cameras and supporting equipment, all to help the world witness a historic milestone when the Artemis II crew returned to Earth on April 10.
Next up will be Artemis III. NASA will launch four astronauts from NASA Kennedy aboard the Orion spacecraft on the SLS rocket. Building on the successful Artemis II crewed test flight in April, Artemis III will pave the way for future surface missions, with experts like Peterson helping every step of the way.
About the AuthorBo BlackCommunications Strategist Share Details Last Updated Jun 23, 2026 EditorCatherine Ragin Williams Related Terms Explore More 2 min read NASA Astronauts to Answer Questions from New Jersey Students Article 1 week ago 3 min read I Am Artemis: Elkin Norena Article 2 weeks ago 5 min read NASA’s Artemis II Moon Mission Research Continues on EarthResults from Artemis II’s science investigations will help support safe human exploration of deep space…
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