NASA News
San Francisco’s Patchwork Streets
An astronaut aboard the International Space Station took this picture of downtown San Francisco and nearby communities on May 27, 2026. The image captures two of the region’s iconic bridges. The Golden Gate Bridge connects the northern San Francisco Peninsula with Marin County to the north, while the San Francisco-Oakland Bay Bridge spans the bay toward Oakland to the east.
Read more about this photograph on Earth Observatory.
Text credit: Kathryn Hansen
Image credit: NASA
Experience the Launch of NASA’s Roman Space Telescope
Are you ready for a new view of the universe? The Nancy Grace Roman Space Telescope will reveal distant worlds, dark energy, and the structure of the cosmos, and we want you to be a part of it!
Digital creators and social media users are invited to register to our NASA Social for the Nancy Grace Roman Space Telescope launch. Roman is NASA’s next flagship astrophysics mission, designed to explore everything from our outer solar system to the edge of the observable universe. This mission is scheduled to launch on Aug. 30, 2026, aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida.
Are you passionate about social media and communications? Do you love to create content for an audience? Are you a fan of new, unique experiences? If you said yes, this NASA Social event is for you! This is your opportunity to be on the front lines of this historic mission.
The NASA Social event will take place over two days, including the day of launch. A maximum of 50 digital creators will be selected to attend this two-day event and will be given access similar to news media.
NASA Social participants will have the opportunity to:
- Tour NASA’s Kennedy Space Center
- Learn directly from astrophysics subject matter experts
- Meet fellow digital creators and social media users
- Spend time with members of NASA’s social media team
- View the launch of the Nancy Grace Roman Space Telescope
NASA Social events are intended for members of the public. Current or former NASA civil servants, NASA contractors, NASA interns, and individuals or organizations currently under contract to provide products or services to NASA are not eligible to apply or participate in NASA Social events.
NASA Social registration for the Roman launch opens on this page on Monday, June 15 and the deadline to apply is at 11:59 p.m. EDT on Sunday, June 28. All applications will be considered on a case-by-case basis.
Do I need to have a social media account to register?
Yes. This event is designed for people who:
- Actively use multiple social networking platforms and tools to disseminate information to a unique audience.
- Regularly produce new content that features multimedia elements.
- Have the potential to reach a large number of people using digital platforms.
- Reach a unique audience, separate and distinctive from traditional news media and/or NASA audiences.
- Must have an established history of posting content on social media platforms.
- Have previous postings that are highly visible, respected, and widely recognized.
Users are encouraged to follow @NASARoman for Roman updates on X, Facebook, and @NASAGoddard and @NASAUniverse on Instagram. Updates and information about the event will be shared on X via @NASA_Events
How do I register?
Registration for this event opens Monday, June 15 and closes at 5 p.m. EDT on Sunday, June 28. Registration is for one person only (you) and is non-transferable. Each individual wishing to attend must register separately. Each application will be considered on a case-by-case basis.
Can I register if I am not a U.S. citizen?
Yes, this event is open for all to apply.
When will I know if I am selected?
After registrations have been received and processed, an email with confirmation information and additional instructions will be sent to those selected. We expect to send the first notifications on XX and waitlist notifications on XX.
What are NASA Social credentials?
All NASA social applications will be considered on a case-by-case basis. Those chosen must prove through the registration process they meet specific engagement criteria.
If you do not make the registration list for this NASA Social, you still can attend the launch off site and participate in the conversation online. Find out about ways to experience a launch at https://www.nasa.gov/kennedy/see-a-launch-up-close/.
What are the registration requirements?
Registration indicates your intent to travel to NASA Kennedy and attend the two-day event in person. You are responsible for your own expenses for travel, accommodation, food, and other amenities.
The schedule of events and special guest appearances are subject to change without notice. NASA is not responsible for loss or damage incurred as a result of attending. NASA, moreover, is not responsible for loss or damage incurred if the event is canceled with limited or no notice. Please plan accordingly.
Kennedy is a government facility. Those who are selected may need to complete additional steps to receive clearance to enter the secure areas.
IMPORTANT: Those without proper identification cannot be admitted.
For United States Citizens:
You will be required to present a REAL ID compliant identification or valid U.S. passport PLUS one of the following:
Acceptable documents to accompany federal or state identification:
- U.S. Passport
- Unexpired Employment Authorization Card (Form I-688A)
- Unexpired Employment Authorization Document issued by DHS that contains a photograph (Form I-688B)
- Driver’s license or ID card issued by a state or outlying possession of the United States provided it contains a photograph or information such as name, date of birth, gender, height, eye color, and address
- ID card issued by federal, state, or local government agencies or entities, provided it contains a photograph or information such as name, date of birth, gender, height, eye color, and address
- School ID card with a photograph
- Voter’s Registration Card
- Military Dependent’s ID Card
- U.S. Military card or draft record
- U.S. Coast Guard Merchant Mariner Card
- Native American Tribal Document
- U.S. Social Security Card issued by the Social Security Administration (other than a card stating it is not valid for employment)
- Original or Certified copy of birth certificate issued by a state, county, municipal authority, or outlying possessions of the United States bearing an official seal
- U.S. Citizen ID Card (Form I-197)
- ID Card for use of Resident Citizens of the United States (Form I-179)
- Unexpired employment authorization document issued by DHS (other than those listed previously)
For Foreign Nationals:
- Same items required of U.S. Citizens (SSN only when applicable)
- Unexpired foreign passport, with I-551 stamp or attached Form I-94 indicating unexpired employment authorization
- Passport number and registration date
- Citizenship
- Driver’s license issued by a Canadian Government authority
For Legal Resident Aliens:
- Same items required of U.S. Citizens, and:
- Permanent Resident Card or Alien Registration Receipt Card with photograph (Form I-551)
- Unexpired Temporary Resident Card (Form I-688)
- Certification of Birth Abroad issued by the Department of State (Form FS-545 or Form DS-1350)
The REAL ID Act was passed by Congress in 2005 to establish minimum security standards for state-issued driver’s licenses and identification cards.
All registrants must be at least 18 years old.
What if the launch date changes?
Hundreds of different factors can cause a scheduled launch date to change multiple times. The launch date will not be official until after the Flight Readiness Review. If the launch date changes prior to the review, NASA may adjust the date of the NASA Social accordingly to coincide with the new target launch date, and will notify registrants of any changes via email.
If the launch is postponed, attendees will be invited to attend a later launch date. If the launch is postponed beyond 72 hours, the NASA Social event may be canceled.
NASA Social attendees are responsible for any additional costs they incur related to any launch delay. We strongly encourage participants to make travel arrangements that are refundable and/or flexible.
What if I cannot come to the Kennedy Space Center?
If you cannot come to NASA Kennedy and attend in person, you should not register for the NASA Social. Join the conversation by following @NASARoman on X and Facebook, and @NASAGoddard and @NASAUniverse on Instagram. You can watch the launch at nasa.gov/live. NASA will provide regular launch and mission updates on @NASA.
If you cannot make this NASA Social, don’t worry; NASA is planning many other NASA Social events in the near future at various locations! Check for updates on NASA Socials.
Pumice Rafts Encroach on Admiralty Islands
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NASA to Cover 34th SpaceX Resupply Mission Space Station Departure
NASA and its international partners are set to receive scientific research samples and hardware as a SpaceX Dragon spacecraft is scheduled to depart the International Space Station on Tuesday, June 16, for its return to Earth.
Watch NASA’s live undocking coverage beginning at 11:45 a.m. EDT on NASA+, Amazon Prime, and the agency’s YouTube channel. Learn how to watch NASA content through a variety of online platforms, including social media.
The Dragon spacecraft will undock from the forward port of the station’s Harmony module at about 12:05 p.m., after receiving a command from SpaceX ground controllers. The spacecraft then will fire its thrusters to move safely away from the orbiting complex.
Following a June 16 departure, the spacecraft will reenter Earth’s atmosphere on Wednesday, June 17, before splashing down off the coast of California at approximately 5:08 a.m. PDT. NASA will not stream the splashdown but will post updates on its space station blog.
Dragon will return to Earth with thousands of pounds of cargo, carrying samples that could shape future space exploration and life on Earth. Research returning includes bioprinted organ and cartilage tissue, data on improving cryogenic fuel storage for future space missions, and DNA‑inspired materials to develop new cancer treatments. The returning hardware includes an ocular imaging device used to monitor crew members’ eye health, an absorbent bed that filters trace contaminants from cabin air, and a separator pump from the waste and hygiene compartment.
Loaded with nearly 6,500 pounds of crew cargo and science experiments, Dragon arrived at the station on May 17 after launching two days earlier on a Falcon 9 rocket from Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida.
For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs not possible on Earth. The space station helps NASA understand and overcome the challenges of human spaceflight, expand commercial opportunities in low Earth orbit, and build on the foundation for long-duration missions to the Moon, as part of the Artemis program, and to Mars.
Get breaking news, images, and features from the space station on Instagram, Facebook, and X.
Learn more about International Space Station research and operations at:
https://www.nasa.gov/international-space-station
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Jimi Russell
Headquarters, Washington
202-358-1100
james.j.russell@nasa.gov
Leah Cheshier
Johnson Space Center, Houston
281-483-5111
leah.d.cheshier@nasa.gov
Black Eye Galaxy
This March 20, 2026, image of Messier 64, or the Black Eye Galaxy, is a composite view from NASA’s Hubble Space Telescope and James Webb Space Telescope. It shows Messier 64 captured at near- and mid-infrared wavelengths by Webb, while Hubble’s image shows the galaxy in ultraviolet, visible, and near-infrared light.
Messier 64 is characterized by its bizarre internal motion. The gas in the outer regions of this spiral galaxy is rotating in the opposite direction from the gas and stars in its inner regions. This strange behavior may be the result of a merger between M64 and a satellite galaxy over a billion years ago.
Image credit: NASA, CSA, ESA, F. Belfiore (European Southern Observatory – Germany), J. Lee (Space Telescope Science Institute), A. Leroy (The Ohio State University), and D. Thilker (The Johns Hopkins University); Processing: Gladys Kober (NASA/Catholic University of America)
Hubble Sees Swarm of Galaxies
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Hubble Sees Swarm of Galaxies This NASA Hubble Space Telescope image features the galaxy cluster MACS0329-0211. NASA, ESA, M. Postman (STScI); Image Processing: G. Kober (NASA/Catholic University of America)Looking somewhat like a swarm of bees returning to their hive, this NASA Hubble Space Telescope image features the galaxy cluster MACS0329-0211. Galaxy clusters like MACS0329-0211 are important signposts in the story of how the structure of the universe evolved, and are the ultimate telescopic lenses, placing gravitationally lensed galaxies from the earliest stages of the universe into our view.
Zoom into this galaxy swarm and you will find large, oval-shaped elliptical galaxies, and thin spiral and lenticular galaxies viewed from the edge. We can also see the full, face-on view of spiral galaxies and their curving spiral arms. The image’s upper-right quadrant holds faint arcs of distant galaxies gravitationally lensed by the cluster’s massive gravity. The largest of these arcs appears above the bright oval shape of a giant elliptical galaxy. Closer inspection of the image’s center reveals several bright-white intersecting curves that appear as a distorted figure eight. This may be another distant galaxy whose light was magnified and distorted by this massive cluster’s gravity.
Hubble looked at MACS0329-0211 as part of an observing program of X-ray bright galaxy clusters. Researchers used Hubble’s two main cameras, the Advanced Camera for Surveys and its Wide Field Camera 3, to gather data visible and infrared light from the cluster. Hubble’s ability to see such a broad spectrum of light makes it a valuable tool in understanding the very nature of these galaxy clusters.
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Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
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NASA Award Boosts Space Technology Research Capabilities
NASA is introducing a new funding opportunity to accelerate academic research and technology development. The Minority University Research and Education Project Space Technology Artemis Research (M‑STAR) application window opened Thursday and will remain open through 11:59 p.m. EDT on Tuesday, Aug. 11.
The research funded through this award supports the agency’s priorities for exploring the Moon, Mars, and deep space, while strengthening eligible institutions in the future of space exploration. Through M-STAR, institutions are encouraged to grow their scientific and engineering capabilities, enhance faculty and student engagement in aerospace research, and expand their ability to compete for future federal and commercial research awards.
Administered by NASA’s Office of STEM Engagement, this initiative contributes to NASA’s Space Technology Mission Directorate, and supports the agency’s broader mission to develop innovative technologies that improve space transportation, human exploration, robotic discovery, and the growing space economy.
NASA’s Office of STEM Engagement fosters an ecosystem across education, industry, and government to cultivate a well‑prepared talent pool, while the agency’s Space Technology Mission Directorate develops the transformative space technologies that enable future NASA missions and ensure U.S. leadership in aerospace. Together, they accelerate mission readiness by aligning cutting edge technological innovation with the workforce needed to carry it forward.
For complete eligibility information, help session registration, and to submit an M-STAR proposal, visit:
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NASA’s Chandra Discovers Possible Supernova Remnant in Galactic Center
Using data from NASA’s Chandra X-ray Observatory, astronomers may have found a supernova remnant in an intriguing neighborhood in the middle of our galaxy. A paper describing these new findings published in The Astrophysical Journal.
Supernova remnants are the expanding remains of exploded stars and provide elements – like iron, oxygen, and silicon – that are critical for the formation of planets and for life as we know it to form and flourish.
This new supernova remnant, if confirmed, would be one of the closest ever discovered to the supermassive black hole at the central region of the Milky Way galaxy, an exotic region crammed with massive stars, long threads of magnetic fields and dense clouds of gas orbiting rapidly around the Galactic Center.
Astronomers may have uncovered a new supernova remnant in a star-forming region near the center of the Milky Way galaxy using data from Chandra and XMM-Newton. If confirmed, this would be one of the closest supernova remnants to the supermassive black hole in the Galactic Center. This image shows the region where the evidence was found, which contains X-rays from Chandra and XMM-Newton, radio data from the MeerKAT telescope in South Africa, and an optical image from the Pan-STARRS telescopes in Hawaii. X-ray: NASA/CXC/UCLA/Z. Zhu et al.; ESA/XMM-Newton; Optical: PanSTARRS; Radio: MeerKAT; Infrared (JWST): NASA/ESA/CSA/STScI; Image Processing: NASA/CXC/SAO/L. Frattare and P. EdmondsA new composite image of this region contains X-rays from Chandra and ESA’s (European Space Agency’s) XMM-Newton mission (shown in blue) as well as radio data from the MeerKAT telescope (shown in red) in South Africa. These have been combined with an optical image from the Pan-STARRS telescopes in Hawaii (red, green, and blue). The plane of the galaxy runs horizontally from left to right in the image, and the central black hole is off to the left of the image.
The evidence for the new supernova remnant, located about 26,000 light-years from Earth, comes from X-ray data from Chandra and XMM-Newton. The X-ray data reveals a “blob” of X-ray emission that may come from the remains of a massive star that self-destructed as a supernova, buried within the larger cloud of expanding gas.
The location of this suspected supernova remnant in the image is labeled with a circle.
It is in a bubble of gas that has had electrons stripped away from hydrogen – called an “H II region” – surrounding a massive, young star. This bubble is a bright source of radio emission called Sagittarius C.
If this is indeed a supernova remnant, then it is expanding at about two million miles per hour and is at least about 1,700 years old. Previously, observations with NASA’s now-retired SOFIA (Stratospheric Observatory for Infrared Astronomy) mission had shown evidence for an expanding shell of gas surrounding Sagittarius C. This gave astronomers a hint that a stellar explosion had occurred in the same spot.
The long filaments seen in the radio image are caused by energetic particles travelling along magnetic fields that are mostly directed perpendicular to the plane of the galaxy.
The nuclear fusion engines of stars create elements from hydrogen and helium that were abundant at the beginning of the universe. When stars explode at the end of their lives as supernovae, they send these newly synthesized elements into interstellar space and provide material for the next generation of stars and planets.
The team of astronomers searched the X-ray data for signs of increased amounts of key elements in the remnant, which would have been caused by the stellar explosion blasting them into space. While they did not see an enhancement, this could imply that the stellar debris has already mixed with the surrounding gas.
An alternative explanation for the X-ray blob is that the hot gas comes from a collection of massive stars in the region. The authors of the recent study don’t think this explanation is likely, because the X-ray emission from the blob is more than ten times brighter than the X-ray emission of large, known stellar clusters with bright, massive stars.
An additional image shows data from NASA’s James Webb Space Telescope added to the X-ray and radio data. The light blue color represents infrared light from gas in the H II region, and the darker blue depicts X-rays from the supernova remnant candidate, on the right side of the image. X-rays near the center of the image are associated with the H II region, possibly caused by material blown away by massive stars that has heated gas to millions of degrees, producing X-rays.
Sagittarius C, close-up image adding NASA’s James Webb Space Telescope data to the X-ray and radio data.The study’s authors are Zhenlin Zhu and Mark Morris of the University of California, Los Angeles; Gabriele Ponti of Italy’s National Institute for Astrophysics; and Ping Zhou of Nanjing University in China.
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
Visual DescriptionThis release features a composite image of colorful, overlapping clouds, which suggests to astronomers that a supernova remnant may be buried in gas near the center of our Milky Way galaxy.
Set against a backdrop packed with distant stars and other specks of light are two distinct, overlapping clouds. The larger, visually dominant cloud, is red and multifaceted. It has an irregular shape, and features patches of different textures, including pockets that resemble wispy smoke, tangles of faint red veins, and clear streaking lines. This large cloud of expanding gas represents radio data from the MeerKAT telescope in South Africa.
Overlapping with that red cloud is a cloudy blue blob representing X-ray data from NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton. Astronomers suggest that this blue blob of X-ray emissions is the remains of a massive star destroyed by a supernova.
Read more from NASA’s Chandra X-ray Observatory
To learn more about NASA’s Chandra mission, visit:
https://science.nasa.gov/chandra
News Media ContactMegan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
mwatzke@cfa.harvard.edu
Joel Wallace
Marshall Space Flight Center, Huntsville, Alabama
256-544-0034
joel.w.wallace@nasa.gov
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I Am Artemis: Elkin Norena
Listen to this audio excerpt from Elkin Norena, resident management officer, NASA’s Space Launch System Program:
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Your browser does not support the audio element.NASA’s Elkin Norena has helped the agency launch more than a dozen space shuttle missions – that’s more than a dozen crews to low Earth orbit and more than a dozen historic missions. They were missions that helped build the International Space Station, that provided a final servicing mission to the Hubble Space Telescope, and that performed critical science experiments that improved life right here on Earth.
Today, he continues that work as the manager of the Resident Management Office for SLS at NASA’s Kennedy Space Center in Florida, helping launch America’s rocket – the SLS (Space Launch System) – and the Orion spacecraft with its international quartet of astronauts on the Artemis II mission to fly by the Moon and return home.
Elkin Norena, who serves as an SLS resident management officer at NASA’s Kennedy Space Center in Florida, stands in front of an RS-25 engine.NASAAs resident manager, Norena provides onsite SLS support for NASA’s Exploration Ground Systems team that is responsible for preparing, stacking, testing, and launching SLS and Orion. He is also the eyes and ears for the SLS Program, providing an avenue of communications back to the program, which is managed at NASA’s Marshall Space Flight Center in Huntsville, Alabama.
It is the continuation of a childhood dream to be part of space exploration.
“When I was a kid in New Jersey, I watched a space shuttle launch in class one day,” said Norena. “When I watched the power of launch and the brave astronauts going to explore, I knew I had to be a part of that one day. I wanted to become an astronaut.”
The dream to join the space program led the Colombia native to the University of Central Florida in Orlando, where he majored in computer engineering, just miles from the Space Coast and in view of space shuttle launches like the ones he once watched on TV.
When that clock ticks down to T-10 minutes, everybody’s just waiting. You wait for the automated system to kick in. You hold your breath and watch the clock go down to T-0. Then BOOM, launch happens, and you know it was all worth it.Elkin Norena
Resident management officer, NASA Space Launch System Program
Following college, he joined NASA contractor United Space Alliance at NASA Kennedy, and in 2008 he joined the NASA Kennedy team as a civil servant, working on the same spacecraft that inspired him to pursue the space program as a child.
“I started off in the Space Shuttle Program as an electrical engineer. Then I moved into the firing room for 17 different shuttle missions as a flight termination engineer. It was exciting to be part of all those missions and build the International Space Station,” Norena said.
The Milky Way stretches above Dry Tortugas National Park in Florida. Elkin NorenaUsing those experiences, he became one of the original SLS team members. He was a part of the teams that successfully launched Artemis I and II and is now critical to the upcoming Artemis III mission.
Away from the launch pad, Norena’s hobbies orbit around his teenage daughters, participating in their activities. He also keeps a keen eye on space and is an avid astrophotographer.
“I love capturing the Milky Way! I’ve traveled to Utah, New Mexico, Arizona, and all across the western United States,” he said. “A great spot that’s closer for me is Dry Tortugas National Park beyond Key West.”
No matter how he explores space, Norena believes Artemis II is more than just a mission.
“This is historic. I grew up watching the shuttle missions, learning about Apollo, and wanting to be part of those Moon missions. We built the space station. The space shuttle explored space and technology on many levels,” he said. “Now, it’s our turn with Artemis to get back to the Moon, and this time to stay there. I’m excited to be part of the generation that does that.”
About the AuthorWilliam BryanCommunication Strategist Share Details Last Updated Jun 11, 2026 EditorLee MohonContactJonathan Dealjonathan.e.deal@nasa.govLocationMarshall Space Flight Center Related Terms Explore More 3 min read I Am Artemis: Doug Parkinson Article 5 months ago 4 min read I Am Artemis: Jacki Mahaffey Article 5 months ago 3 min read I Am Artemis: Lili VillarrealLili Villarreal fell in love with space exploration from an early age when her and…
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NASA Robotic Tech Demo Will Advance Prototype Gamma-Ray Detectors
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NASA Robotic Tech Demo Will Advance Prototype Gamma-Ray DetectorsA new type of gamma-ray sensor developed by NASA, called AstroPix, will take part in a robotic arm demonstration on the agency’s upcoming Fly Foundational Robots mission, set to launch in late 2027.
Gamma rays are the highest-energy form of light. Scientists observe them coming from events like lightning in Earth’s atmosphere, powerful solar flares from our Sun, and cosmic collisions in distant galaxies. The sensors on the AstroPix technology demonstration are designed to measure gamma rays between 20,000 and 700,000 electron volts. For comparison, visible light’s energy falls between 2 and 3 electron volts.
Current NASA missions, including the Fermi Gamma-ray Space Telescope and Neil Gehrels Swift Observatory, also observe gamma rays, including those with even higher energies.
But for energies between 500,000 to 1 million electron volts, existing detectors are less sensitive. This range is where many powerful explosions called gamma-ray bursts shine the brightest. It’s also where astronomers expect to see the strongest glow from the most massive and distant active galaxies powered by black holes. By stacking AstroPix detectors in future missions, scientists could bridge this gap and improve observations of these cosmic objects to better understand the processes that create and drive them.
“The Fly Foundational Robots spacecraft is also a technology demonstration, so the projects were a good fit for each other,” said Dan Violette, an AstroPix team member and post-doctoral fellow at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We need to thoroughly test AstroPix’s performance before we can use the sensors in future science missions. We’ve flown comparable technologies on a scientific balloon mission, and the current prototype eventually will be part of a sounding rocket payload. Many of those flight opportunities only reach near space, though. It’s not often that technology demonstrations like ours can find a ride into orbit.”
Each AstroPix chip has four silicon pixel gamma-ray detectors. Each of these detectors incorporates 1,225 pixels. AstroPix detectors, which are developed by NASA’s Goddard Space Flight Center in Greenbelt, Md., function similarly to the sensors in cellphone cameras except they are sensitive to gamma-ray light. Image courtesy of Argonne National LaboratoryEach AstroPix chip contains four silicon pixel gamma-ray detectors, and each detector incorporates 1,225 pixels. The chips function similarly to the sensors in cell phone cameras.
The AstroPix Satellite Technology dEmonstration Payload, also known as A-STEP, will be hosted within the Fly Foundational Robots mission’s Orbital Replacement Unit, a movable module built by Rocket Lab Robotics. Rocket Lab Robotics also will provide a robotic arm that will pick up and reposition the unit during flight and perform in-orbit operations as part of a robotic servicing demonstration. The A-STEP payload will collect its data following the repositioning. Astro Digital will provide the spacecraft.
The Orbital Replacement Unit was designed to support power and data interfaces for a payload, but the original plan called for the robotic arm to reposition the module without one. As mission development progressed, however, the Fly Foundational Robots team identified an opportunity to further maximize the mission’s value by integrating an additional technology demonstration that could fit within the 11.8-inch (30-centimeter) cube.
“The unit already had the volume, power, and data needed to support the AstroPix team’s design,” said Bo Naasz, senior technical lead, In-space Servicing, Assembly, and Manufacturing in the Space Technology Mission Directorate at NASA Headquarters in Washington. “One of our major goals with Fly Foundational Robots is to demonstrate robotic changeout of payloads in orbit, enabling upgrades or improvements to satellites and space instruments at a fraction of the cost of a full mission. Allowing AstroPix to complete its own technology demonstration in orbit is a bonus.”
NASA’s Fly Foundational Robots mission will be hosted aboard a spacecraft provided by Astro Digital of Littleton, Colo., as shown in this artist’s concept. The robotic arm, provided by Motiv Space Systems in Pasadena, Calif., will perform a technology demonstration in orbit, including picking up and moving a small box containing the agency’s AstroPix gamma-ray sensors. Rocket Lab RoboticsThe AstroPix team is working to deliver their hardware this September, and it will be integrated into the Fly Foundational Robots payload before final integration onto the spacecraft. The Orbital Replacement Unit will hold the chips and all the associated electronics needed to provide power, and collect and transmit data during flight.
NASA’s Fly Foundational Robots mission is funded through the Space Technology Mission Directorate’s ISAM portfolio, managed at NASA Goddard. Rocket Lab Robotics will supply the mission’s robotic arm system through a NASA Small Business Innovation Research Phase III award. Astro Digital will host the orbital flight test of the arm through NASA’s Flight Opportunities program, managed at NASA’s Armstrong Flight Research Center in Edwards, California. The development of AstroPix was supported by NASA’s Astrophysics Division in the Science Mission Directorate at NASA Headquarters, through the agency’s Astrophysics Research and Analysis Program, and funded through the Nancy Grace Roman Technology Fellowship.
To learn more, visit:
By Jeanette Kazmierczak
Goddard Space Flight Center, Greenbelt, Md.
Soccer Meets Space Science
A soccer ball floats in microgravity in this March 2, 2026, picture from the International Space Station. The space station crew tested soccer balls to study how internal mass affects motion and stability in microgravity. The findings have improved understanding of how embedded technologies, including match-ball sensors, can influence performance during play.
Through research aboard the International Space Station and technology developed for exploration, NASA continues to demonstrate how discoveries made for space can benefit people on Earth—including athletes and fans participating in the world’s most popular sport.
Image credit: NASA
NASA’s Career Technical Education Day Highlights Technical Careers
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Preparations for Next Moonwalk Simulations Underway (and Underwater) Students participate in a hands-on robotics demonstration during Career Technical Education Day at NASA’s Langley Research Center in Hampton, Virginia. NASA/Mark KnoppAt NASA, remaining a global leader in exploration and innovation includes having a skilled
and dedicated workforce. Technicians play a critical role in advancing the agency’s
research and missions, applying hands-on expertise across engineering, fabrication,
electronics, and countless other technical fields.
To help cultivate the next generation of technical talent, NASA’s Office of STEM Engagement
hosted Career Technical Education Day recently at NASA’s Langley Research Center in
Hampton, Virginia. One hundred high school and community college students from Virginia
and North Carolina attended, eager to explore the technical career paths that help drive
NASA’s work.
“Many students picture NASA as only astronauts or engineers and therefore never consider
a career at NASA to be within their reach,” said Bonnie Murray, lead for the Office of STEM
Engagement at NASA Langley. “Bringing students from local career and technical
education programs to Langley allows them the opportunity to see technicians at work,
hear the pathways those technicians followed, and understand how the skills they are
developing in their related classes have a place in the NASA workforce.”
The event opened with remarks from NASA Langley’s Steve Gayle, who traced his path from
an engineering technician co-op in the center’s Fabrication Division and a graduate of
Langley’s Engineering Technician Apprentice Program to his current role as acting
associate director. Gayle encouraged students to embrace challenges, think critically, stay
curious, and create their own opportunities as they pursue their career goals.
“We need young, bright minds,” Gayle said. “At NASA, we rely on skilled hands-on
professionals — technicians who operate our wind tunnels, apply their skills in our
fabrication shops, and use their electronics knowledge to design, test, and build critical
systems.”
Throughout the day, students toured several of Langley’s world-class facilities, including
the historic Landing and Impact Research Facility and one of the center’s wind tunnels. At
each stop, they received a behind-the-scenes look at the spaces where NASA technicians
build, test, and refine the tools and technologies that support the agency’s missions. The
technicians spoke with students about their work, their career paths, and the skills needed
to excel in technical roles.
Hands-on demonstrations and interactive activities lead by NASA technicians and
aerospace industry partners helped students connect their classroom experience with
real-world applications. Whether observing fabrication techniques, seeing instrumentation
up close, or engaging with engineering demonstrations, participants experienced how
STEM and technical skills directly translate into meaningful careers.
“Through events such as this, NASA seeks to prepare students for aerospace careers
through experiences and investments that strengthen research capacity, build technical
expertise, and expand reach in alignment with agency missions and needs,” Murray said.
The event ended with a career panel moderated by NASA astronaut Joe Acaba, associate
director of mission and strategy at NASA’s Johnson Space Center in Houston and former
math and science teacher. The panel featured four Langley technician apprentices who
shared insights into their roles and the value of strong foundational skills in technical
fields.
“A basic grasp of how software, systems, and even everyday items function goes a long way
as you progress in your technician journey,” said Wyatt Healy, mechanical engineering
technician apprentice at NASA Langley. “When you have those fundamentals down,
learning the more advanced concepts becomes much easier. It doesn’t happen overnight,
but with a strong foundation, the sky is the limit.”
By connecting students with NASA professionals, facilities, and hands-on experiences, the
event showcased a broad range of opportunities available in technical careers. It also
underscored NASA’s commitment to building a strong, skilled workforce equipped to
support the agency’s mission and tackle the challenges of tomorrow.
For more information about opportunities to connect students with NASA’s mission, work, and people, visit:
https://www.nasa.gov/learning-resources
Brittny McGraw
NASA Langley Research Center
Missions
Humans in Space
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NASA, USGS Scientists Go Rock Hounding in California’s High Desert
Equipped with rock picks and hand lenses, a team of geoscientists deployed to the Mojave Desert recently to investigate a tantalizing “fingerprint” detected by a NASA sensor. Their target: a cache of topaz hiding in plain sight.
The geologists weren’t searching for gem-grade treasure. Rather, the presence of topaz could hint at a more valuable deposit below of something known as porphyry copper.
One of the world’s primary sources of copper, these deposits are left behind when magma and hot water from deep underground course through Earth’s crust, chemically transforming the surrounding rock. This tends to occur where one tectonic plate dives below another, known as a subduction zone, such as the North American Cordillera, which stretches from the Canadian Rockies to western Mexico.
California’s high desert stretches below a bright spring sky in April 2026. NASA and USGS scientists are using airborne remote sensing to home in on potential sources of critical minerals here and across the Western U.S.NASA/JPL-CaltechIn addition to copper — the third most used metal in the world after steel and aluminum — the deposits can hold other critical minerals like molybdenum and tellurium, which are used in everything from steelmaking to solar panels. Finding the deposits isn’t easy. Geologists look for topaz because it forms under the same volcanic conditions.
For the team in the Mojave, the goal was to collect more evidence. That would require boots on the ground and a heavy bag of samples. The scientists who converged on the site included three experts from the U.S. Geological Survey (USGS) and Robert Green of NASA’s Jet Propulsion Laboratory in Southern California.
“What we’re doing out here is geologic CSI,” said Green, referring to the investigative TV show, as he split open a weathered red rock to expose a sparkling core. “We’re looking for clues to reconstruct what happened here.”
Three-dimensional image cubes illustrate the volume of data captured by NASA imaging spectrometers. The front face shows an aerial view of the Mojave Desert. The colorful side panels reveal what no eye or camera can detect: the spectral fingerprints of minerals present in every pixel.NASA/JPL-Caltech Next-generation mineral mappingThe sensor that detected the topaz deposit on public land near Barstow, California, was built at JPL. Called AVIRIS, short for Airborne Visible Infrared Imaging Spectrometer, it analyzes reflected sunlight and can be used to identify chemicals and minerals by their unique spectral fingerprint. The technology was pioneered in the early 1980s by a team that included Green, and space-hardened versions have explored the Moon, Mars, and other rocky bodies in the solar system in the decades since.
While its cousins study distant worlds aboard spacecraft, the AVIRIS line of sensors is advancing Earth science from aircraft. The latest model, AVIRIS-5, recently took to the skies for the first time as part of the NASA-USGS Geologic Earth Mapping Experiment (GEMx). The goal of GEMx is to identify sources of critical minerals across the American West, including in the waste rock of active and legacy mines. It is led by the USGS as part of its larger, nationwide initiative.
Carrying next-generation sensors, a high-altitude NASA ER-2 aircraft takes off from the agency’s Armstrong Flight Research Center in Edwards, California, on March 31, 2026, to support the GEMx mineral mapping campaign.NASA/Carla ThomasSince 2023, GEMx flights have covered more than 386,000 square miles (1 million square kilometers) of American soil, including most of California.
Ground-truthing the sensor data can entail hot field work, scrambling over steep crags to uncover samples for lab analysis. While testing has confirmed the topaz discovery, determining if the Mojave site overlies a porphyry copper deposit will require intensive investigation using ground-penetrating equipment. But the AVIRIS finding shows how advanced NASA airborne sensing can help lead geologists to the metaphorical needle in a haystack, even in heavily explored Southern California.
“People have been prospecting this area for generations,” said Erik Tharalson, a USGS geologist. “But there’s a lot more to discover.”
High flyerFrom the beginning, the GEMx mineral mapping campaign has been enabled by one of the highest-flying aircraft in NASA’s fleet: the ER‑2. It deployed on March 31 from NASA’s Armstrong Flight Research Center in Edwards, California, to Colorado Springs Airport in Colorado.
“We deployed to Colorado Springs to maximize flight time for data collection needed in Colorado, Utah, New Mexico, Arizona, and Texas,” said John McGrath, ER‑2 project manager at NASA Armstrong.
By the conclusion of this deployment on June 5, the aircraft had completed 26 flights totaling more than 125 hours. Soaring at about 65,000 feet, the ER-2 can fly at high altitudes that allow it to collect broad‑area, high‑resolution spectral measurements in a single pass, supporting researchers studying mineral composition and surface processes.
In 2025, the aircraft flew 36 science missions, collecting more than 7 billion measurements over 200 flight hours. The data has contributed to the largest airborne surface mineralogy dataset gathered in a single NASA-USGS campaign.
The GEMx survey is led and funded by the USGS Earth Mapping Resources Initiative. Earth MRI is modernizing mapping the nation’s surface and subsurface to find new, critical, and other minerals. It is a partnership effort with 45 state geological surveys, federal agencies, private industry, tribes, universities, and others. The initiative will capitalize on both the technology developed by NASA for spectroscopic imaging, as well as the USGS expertise in analyzing the datasets, conducting field work, and deriving critical mineral information from them.
To learn more about GEMx visit:
https://science.nasa.gov/mission/gemx/
Media Contacts
Andrew Wang / Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 818-393-2433
andrew.wang@jpl.nasa.gov / andrew.c.good@jpl.nasa.gov
Written by Sally Younger
2026-037
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NASA to Preview Katalyst Mission to Boost Swift Spacecraft’s Orbit
NASA will host an audio-only media teleconference at 11 a.m. EDT, Wednesday, June 17, to preview the Katalyst Space mission to boost the orbit of NASA’s Neil Gehrels Swift Observatory.
Katalyst’s robotic servicing spacecraft, called LINK, will attempt to rendezvous with Swift and raise its altitude, extending its science mission lifespan and advancing a key capability for the future of space exploration. The LINK spacecraft will launch on Northrop Grumman’s Pegasus XL rocket later this month from Kwajalein Atoll in the Marshall Islands.
Media interested in participating by phone must RSVP no later than two hours before the start of the call to Amy Barra at: amy.l.barra@nasa.gov. NASA’s media accreditation policy is available online.
Audio of the media teleconference will stream on the agency’s website at:
Participants in the media teleconference include:
- Shawn Domagal-Goldman, division director, Astrophysics, NASA Headquarters in Washington
- Brad Cenko, principal investigator, Swift, NASA’s Goddard Space Flight Center in Greenbelt, Maryland
- Kieran Wilson, principal investigator, LINK, Katalyst Space
- Robert Lamontagne, vice president, strategic partnerships, Katalyst Space
- Wes Collier, vice president, launch systems, Northrop Grumman
The Swift mission, which launched in 2004, leads NASA’s fleet of telescopes in studying changes in the high-energy universe, like gamma-ray bursts, which are the most powerful explosions in the cosmos. When a rapid, sudden event takes place in the sky, Swift serves as a “dispatcher,” providing critical information that allows other “first responder” missions to follow up to learn more about how the universe works.
After 21 years, Swift’s low Earth orbit has begun to rapidly decay because of increased solar activity. Rather than allowing the observatory to re-enter Earth’s atmosphere, as many missions do at the end of their lifetimes, NASA is using this opportunity to advance U.S. spacecraft servicing technology. In September 2025, NASA awarded a contract to Katalyst to mount a robotic servicing mission for Swift in less than a year. The mission will use LINK to rendezvous with Swift and boost it to a higher altitude, demonstrating a key capability for the future of space exploration. The mission is targeted for launch in June from Kwajalein Atoll, Marshall Islands.
Learn more about the mission to boost Swift’s orbit at:
https://science.nasa.gov/mission/swift/swift-boost-mission/
-end-
Karen Fox / Alise Fisher
Headquarters, Washington
202-385-1287 / 202-358-2546
karen.c.fox@nasa.gov / alise.m.fisher@nasa.gov
Amy Barra
Wallops Flight Facility, Wallops Island, Va.
757-824-1579
amy.l.barra@nasa.gov
Air Pollution’s Daily Pulse Over the Northeast
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Curiosity Blog: Sols 4913-4919: Planetary explorers, freewheeling to the Yardang unit!
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Curiosity Blog: Sols 4913-4919: Planetary explorers, freewheeling to the Yardang unit! Navcam image from sol 4916 showing the rough drive direction. The yardang unit can be seen as a series of pale coloured hills in the centre of the image, at the very back. NASA/JPL-CaltechWritten by Catherine O’Connell-Cooper, APXS Strategic Planner and Payload Uplink/Downlink Lead, University of New Brunswick, Canada
Earth planning day: Friday, June 5th, 2026
In a very broad sense, Curiosity has two modes of doing science – one centred around a defined science campaign (such as the recent boxwork campaign) and the other as we move between campaigns. During a science campaign, with a very defined start and end location, every image and every workspace is carefully choregraphed to make sure we hit all of our science goals for the campaign. This is a lot of pressure!
But in between campaigns, the emphasis moves to driving towards the next major campaign. Our next major stop is the yardang unit, a series of intriguing wind sculpted, pale coloured hills which you can just see in the distance in the cover image for this blog. The rover planners (RPs) sometimes make our drives as long as they can and we drive as far as we can go, other times we stop a little short to look at interesting looking workspaces as we go. As part of the APXS team, I loved being part of the boxwork campaign and getting all the information we needed there … but as a geologist, there is something very special about this kind of exploring, the sense of being a planetary explorer, ambling along to see what the rocks will show us.
So we continue southwards, trundling over laminated bedrock which varies from predominantly pale coloured laminated bedrock to bands with abundant thin flaky, darker coloured, layers and patches. Some of the rocks stick out at strange angles, which make planning drives more challenging. This past week there has been abundant dark layers interbedded with the more dominant pale coloured rock, both in place and in fragments around the workspace. APXS and MAHLI characterized some of this darker material, for example at “Rio Bio Bio” and “Placilla de Caracoles” and some of the paler material at the brushed targets “La Primavera” and “Los Quemados.” ChemCam also analyzed both types of rocks along the way.
We are busily acquiring Mastcam and ChemCam LD-RMI (“Long Distance Remote Micro Imager”) images of everything even remotely interesting – and there are lots and lots of cool features around here. The wide open landscape here allows us to image features from several different angles and distances, such as “Mira Flores,” a small erosional outlier seen from a distance in this image and closer up here. Another great example is the “Kimsa Chata” trough which shows some amazing sedimentary structures, which may help us to determine if this was a desert or a lake or maybe something in between, such as a desert with some water moving through.
The Environmental Theme Group continues to populate each plan with environmental monitoring activities. Activities varied from dust devil monitoring in Gale crater to looking at levels of dust in the skies overhead. The weekend drive is planned to take us further into that drive distance shown in the cover image, to an area where the contrast between dark and light bedrock is more pronounced, and just beyond that, to an area which looks very smooth, with no jutting out blocks. From where we sit today, its impossible to say what it is but that is the fun of exploring – who knows what we will find? Stay tuned to find out over the coming weeks.
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NASA Awards Contract for Construction Services in California
NASA has selected multiple small businesses for the Western Regional Multiple Award Construction Contract, which supports a broad range of facility enhancement, modernization, and sustainment work at NASA’s Armstrong Flight Research Center in Edwards, California, NASA’s Ames Research Center in California’s Silicon Valley, and other federal agencies in the region.
The contract provides general construction, modification, maintenance and repair, and demolition services, as well as new construction of buildings and facilities that incorporate Leadership in Energy and Environmental Design practices and building information modeling to support efficient and sustainable project execution.
The indefinite-delivery/indefinite-quantity, firm-fixed-price contract is a follow-on to the agency’s previous regional construction contract and has a potential value of $450 million over a five‑year period.
Contract awardees are:
- Abide International Inc.
- Able Heating and Air Conditioning
- Anderson Burton Construction Inc.
- Anna Lisa Luna Construction
- Barkley Andross Corporation
- Bibro Construction Company Inc.
- CM Construction Services
- CMS Construction Inc.
- FASONE
- G‑1 Lead Builders JV LLC
- Gideon USA
- Good‑men Roofing & Construction Inc.
- Groundlevel Construction Inc.
- IPI Construction Inc.
- Innovative Project Solutions Inc.
- Ironwood Commercial Builders Inc.
- J.I. Garcia Construction Inc.
- JG Contracting
- Lead Builders Inc.
- Martinez Construction Services
- MX Construction Inc.
- OCS Construction Services Inc.
- Patricia I. Romero Inc., doing business as Pacific West Builders
- Gustav Keoni, doing business as Precision Construction
- Prime MIK JV LLC
- Spectrum Builders and Renovations Inc.
- Sea Pac Engineering Inc.
- Sergent Construction
- Souza Construction Inc.
- TLI Construction Inc.
For more information about NASA and agency programs, visit:
-end-
Jennifer Dooren / Jessica Taveau
Headquarters, Washington
202-358-1600
jennifer.m.dooren@nasa.gov / jessica.c.taveau@nasa.gov
Dede Dinius
Armstrong Flight Research Center, Edwards, Calif.
661-276-5701
darin.l.dinius@nasa.gov
NASA, NOAA to Hold Joint Session at 23rd Symposium on Operational Environmental Satellite Systems
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Submit your abstract for “Advancing Weather and Environmental Science Through NASA and NOAA Commercial Satellite Data Programs,” a joint session hosted by NASA’s Commercial Satellite Data Acquisition (CSDA) program, in partnership with the NOAA National Environmental Satellite, Data, and Information Service (NESDIS) Commercial Data Program (CDP).
The session is part of the 23rd Symposium on Operational Environmental Satellite Systems, which will take place at the 2027 American Meteorological Society (AMS) Annual Meeting January 10-14 in Denver, Colorado. It will examine the growing capabilities of commercial Earth observation providers that are creating new opportunities to advance weather research, operational forecasting, and environmental science applications.
NASA’s CSDA program and NESDIS’s CDP collaborate to expand federal access to commercial satellite data and accelerate its use in both research and operational applications.
The CSDA program supports the scientific community by evaluating and acquiring diverse commercial datasets, including optical, Synthetic Aperture Radar, Global Navigation Satellite System Radio Occultation and Reflectometry, methane, precipitation, and Digital Elevation/Terrain Models for modeling, hazard monitoring, climate studies, and applied research.
Similarly, the CDP operationalizes commercial space-based environmental data, with demonstrated impacts from assimilated observations in weather forecasting and space weather applications. It also conducts pilot projects and transitions the piloted data to operations.
Together, the CSDA and CDP strengthen the nation’s weather enterprise by enabling innovative research, closing observational gaps, and integrating commercial data into real-world forecasting and decision support applications.
To submit an abstract or for additional information about the abstract submission process, visit the symposium’s website.
NASA Equips Astronauts, Industry with Robotic Intelligence
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) In the Integrated Mobile Evaluation Testbed for Robotics Operations facility at Johnson Space Center, PickNik robotic control software proved its prowess in tasks like passing cargo transfer bags through a hatch and placing them in storage bins, in anticipation of work NASA would like robots to carry out during the later Artemis missions.Credit: NASAAs NASA plans long-term missions on the Moon, the agency could use robots to perform routine tasks, allowing crew members to dedicate more time to science and exploration. However, robotic motion control requires complex technology and advances in features like robotic decision-making and object recognition.
These are the challenges a Boulder, Colorado-based robotics company is teaming up with NASA to overcome.
PickNik Inc. recently worked with Shaun Azimi, who leads the Dexterous Robotics team at NASA’s Johnson Space Center in Houston, and other agency roboticists. The team tested software that enabled a robotic arm to recognize a spacecraft hatch, then turn the latch, grasp the handle, and open the door. The arm then was able to transfer cargo bags between the hatch and a bin.
The work was carried out in NASA Johnson’s new Integrated Mobile Evaluation Testbed for Robotics Operations with funding from NASA’s Small Business Innovation Research program.
PickNik designed and refined the robotic software, called MoveIt Pro, with support from early government investments. Commercially released in 2023, MoveIt Pro has found a significant customer base.
Automotive company BMW is using the software on its robotic assembly lines. A company called Lightspeed is using MoveIt Pro to program huge robotic arms that build modular “panels” for constructing affordable housing. Another company, known as Hivebotics, used MoveIt Pro to automate its flagship product, a cleaning robot.
Ezra Brooks, principal software engineer at PickNik, said the 35-person company might not have a product without NASA’s early support. Robotic software requires years of research and development to refine algorithms and create a commercial product. NASA enabled much of that foundational work.
NASA’s technological advancements unlock key capabilities for missions at the Moon and beyond while benefiting commercial industries on Earth. For 50 years, NASA has documented the everyday benefits of space technology through the agency’s Spinoff publication. To learn more about the project, visit: https://go.nasa.gov/49CNSi7
Read More Share Details Last Updated Jun 10, 2026 Related Terms Explore More 3 min read NASA-Supported Space Tech Advances Earthly Construction Article 4 weeks ago 4 min read Hello Universe: NASA’s Next-Gen Space Processor Undergoes Testing Article 4 weeks ago 3 min read NASA Heat Shield Technology Enables Space Industry Growth Article 4 months ago Keep Exploring Discover Related TopicsTechnology Transfer & Spinoffs
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