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From Suriname to Space: Rohit Goeptar Shares His Journey to NASA

18 June 2026 at 20:06
Rohit Goeptar, an electromagnetic/radio frequency analyst with NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida, reviews a radio frequency link budget analysis for NASA’s Nancy Grace Roman Space Telescope from his office. Goeptar is among the engineers and technicians sworn in as new NASA civil servants as part of NASA Administrator Jared Isaacman’s workforce directive to restore technical core competencies within the civil servants ranks.
NASA/Amanda Griffin

Rohit Goeptar was born into a poor family in Suriname, South America, the kind where both parents work three jobs and they still can only provide food and shelter for their family. At around age six, his family moved to California to start a new life. Only two years later, he moved back to South America with his father while his mother stayed in the United States and remarried. When he was 13, he became a U.S. citizen and he and his brothers returned to live with their mother in California. 

At 19, Goeptar joined the U.S. Marine Corps where he spent six years as a technical operator. During one deployment to the Philippines, Goeptar helped set up communication systems for individuals who needed to contact their loved ones after a typhoon ripped through entire towns.  

“I was lost, the Marine Corps gave me an opportunity,” Goeptar recalled.  

While the Marines taught him useful skills, his life had not been the easiest. He lost not one, but two, fathers to suicide, and a short first marriage ended with him being unhoused on the streets of Kissimmee, Florida, for six months. But Goeptar eventually found his way.   

As with most underdog stories, there was another person in the shadows behind his rise to success.  

“Your brain works in mysterious ways,” his now wife told him a short while after they met. She then filled out college applications for him, and he eventually applied to NASA’s Kennedy Space Center in Florida.  

While raising three kids, going to school full-time pursuing a computer engineering and electrical engineering degree simultaneously, Goeptar got the call that changed his life. 

“In spring 2025, I was driving to pick my son up from school when a gentleman from Kennedy calls, telling me he’s seen my resume and do I have time for a quick interview,” Goeptar recounted. 

He pulled on the side of the road and took part in an impromptu job interview. 

Two weeks later, he had an in-person interview with others from Kennedy and two weeks after that, he had a contractor badge at America’s premier spaceport.  

After starting as an intern under the Expendable Launch Vehicle Integrated Support, or ELVIS, contract, then moving to part-time until he graduated from the University of Central Florida (UCF) in Orlando, then full-time at the beginning of 2026, Goeptar was one of the ELVIS contractors who applied and were picked up to become civil servants recently. 

Rohit Goeptar, an electromagnetic/radio frequency analyst with NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida, reviews a radio frequency link budget analysis for NASA’s Nancy Grace Roman Space Telescope with a colleague.
NASA/Amanda Griffin

Now an employee of NASA’s Launch Services Program, Goeptar works with electromagnetic interference, electromagnetic compatibility, and radio frequency. It is his job throughout the entirety of the mission to analyze and ensure avionic boxes or anything electrically powered doesn’t interfere with any other systems. He also ensures independent systems are compatible when brought together. And finally, he conducts model radio frequency link analysis for different rockets and science demonstrations payloads. These may belong to NASA or commercial partners, and he is responsible for ensuring uninterrupted communication with the ground. In his short time at Kennedy, Goeptar has worked on Sentinel-6B, JPSS-4 (Joint Polar Satellite System), and IMAP (Interstellar Mapping and Acceleration Probe) missions.  

And as far as his wife’s assessment that his brain works differently, he proved that within a year at Kennedy when he noticed an analytical issue his team wasn’t tracking. Once a rocket launches, it does a pitch, yaw, and roll. The analysis the team had been conducting didn’t account for this movement, which meant it wasn’t as accurate as it could be. He presented his solution to the team lead, and it now enables NASA data and partner data to be much more in sync. 

“There is no greater feeling, being able to serve. It’s more than serving the public, it’s serving our country. It’s serving the future of our country,” Goeptar said with tears brimming in his eyes. “Being able to give back to that same government that gave me an opportunity to be where I’m at today. There’s no greater feeling than that.” 

Meanwhile, Goeptar’s 11-year-old takes most of the credit for his landing at the space center, a NASA enthusiast, his son believes he spoke it into existence. 

Rohit Goeptar and children
Rohit Goeptar, an electromagnetic/radio frequency analyst with NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida, poses for a photograph with his children.
NASA/Rohit Goeptar

“One day he wants to become an astronaut,” Goeptar said with joy on his face. “And I told him I will guide him until the day that I die. Maybe my last mission could be the one my son flies on. I’m not going to stop until that day happens.” 

Rohit’s positive streak continues as he recently was accepted into electrical engineering master’s programs at both Johns Hopkins University, and UCF.  

Learn more about NASA’s missions online: 

https://www.nasa.gov 

The post From Suriname to Space: Rohit Goeptar Shares His Journey to NASA appeared first on NASA Science.

From Suriname to Space: Rohit Goeptar Shares His Journey to NASA

18 June 2026 at 20:06
Rohit Goeptar, an electromagnetic/radio frequency analyst with NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida, reviews a radio frequency link budget analysis for NASA’s Nancy Grace Roman Space Telescope from his office. Goeptar is among the engineers and technicians sworn in as new NASA civil servants as part of NASA Administrator Jared Isaacman’s workforce directive to restore technical core competencies within the civil servants ranks.
NASA/Amanda Griffin

Rohit Goeptar was born into a poor family in Suriname, South America, the kind where both parents work three jobs and they still can only provide food and shelter for their family. At around age six, his family moved to California to start a new life. Only two years later, he moved back to South America with his father while his mother stayed in the United States and remarried. When he was 13, he became a U.S. citizen and he and his brothers returned to live with their mother in California. 

At 19, Goeptar joined the U.S. Marine Corps where he spent six years as a technical operator. During one deployment to the Philippines, Goeptar helped set up communication systems for individuals who needed to contact their loved ones after a typhoon ripped through entire towns.  

“I was lost, the Marine Corps gave me an opportunity,” Goeptar recalled.  

While the Marines taught him useful skills, his life had not been the easiest. He lost not one, but two, fathers to suicide, and a short first marriage ended with him being unhoused on the streets of Kissimmee, Florida, for six months. But Goeptar eventually found his way.   

As with most underdog stories, there was another person in the shadows behind his rise to success.  

“Your brain works in mysterious ways,” his now wife told him a short while after they met. She then filled out college applications for him, and he eventually applied to NASA’s Kennedy Space Center in Florida.  

While raising three kids, going to school full-time pursuing a computer engineering and electrical engineering degree simultaneously, Goeptar got the call that changed his life. 

“In spring 2025, I was driving to pick my son up from school when a gentleman from Kennedy calls, telling me he’s seen my resume and do I have time for a quick interview,” Goeptar recounted. 

He pulled on the side of the road and took part in an impromptu job interview. 

Two weeks later, he had an in-person interview with others from Kennedy and two weeks after that, he had a contractor badge at America’s premier spaceport.  

After starting as an intern under the Expendable Launch Vehicle Integrated Support, or ELVIS, contract, then moving to part-time until he graduated from the University of Central Florida (UCF) in Orlando, then full-time at the beginning of 2026, Goeptar was one of the ELVIS contractors who applied and were picked up to become civil servants recently. 

Rohit Goeptar, an electromagnetic/radio frequency analyst with NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida, reviews a radio frequency link budget analysis for NASA’s Nancy Grace Roman Space Telescope with a colleague.
NASA/Amanda Griffin

Now an employee of NASA’s Launch Services Program, Goeptar works with electromagnetic interference, electromagnetic compatibility, and radio frequency. It is his job throughout the entirety of the mission to analyze and ensure avionic boxes or anything electrically powered doesn’t interfere with any other systems. He also ensures independent systems are compatible when brought together. And finally, he conducts model radio frequency link analysis for different rockets and science demonstrations payloads. These may belong to NASA or commercial partners, and he is responsible for ensuring uninterrupted communication with the ground. In his short time at Kennedy, Goeptar has worked on Sentinel-6B, JPSS-4 (Joint Polar Satellite System), and IMAP (Interstellar Mapping and Acceleration Probe) missions.  

And as far as his wife’s assessment that his brain works differently, he proved that within a year at Kennedy when he noticed an analytical issue his team wasn’t tracking. Once a rocket launches, it does a pitch, yaw, and roll. The analysis the team had been conducting didn’t account for this movement, which meant it wasn’t as accurate as it could be. He presented his solution to the team lead, and it now enables NASA data and partner data to be much more in sync. 

“There is no greater feeling, being able to serve. It’s more than serving the public, it’s serving our country. It’s serving the future of our country,” Goeptar said with tears brimming in his eyes. “Being able to give back to that same government that gave me an opportunity to be where I’m at today. There’s no greater feeling than that.” 

Meanwhile, Goeptar’s 11-year-old takes most of the credit for his landing at the space center, a NASA enthusiast, his son believes he spoke it into existence. 

Rohit Goeptar and children
Rohit Goeptar, an electromagnetic/radio frequency analyst with NASA’s Launch Services Program at the agency’s Kennedy Space Center in Florida, poses for a photograph with his children.
NASA/Rohit Goeptar

“One day he wants to become an astronaut,” Goeptar said with joy on his face. “And I told him I will guide him until the day that I die. Maybe my last mission could be the one my son flies on. I’m not going to stop until that day happens.” 

Rohit’s positive streak continues as he recently was accepted into electrical engineering master’s programs at both Johns Hopkins University, and UCF.  

Learn more about NASA’s missions online: 

https://www.nasa.gov 

NASA Testing Advanced Capabilities for Moon, Mars Rovers

18 June 2026 at 19:19
A white four-wheeled rover with a rectangular head on its mast projects a red glow onto a dark desert landscape. Pink and yellow hues indicate the sun has set behind a distant mountain range, while the top of the frame remains blue.
Developed at NASA’s Jet Propulsion Laboratory, ERNEST (Exploration Rover for Navigating Extreme Sloped Terrain) is used in a desert field test to help refine mobility hardware and autonomy software that could be used for a potential future long-range lunar rover mission.
A white four-wheeled rover on the left side of the frame casts a long shadow across barren, brown ground toward the lower right. A few low, scrubby plants dot the desert landscape and mountains rise in the far distance under a pale blue sky.
During the field test, which took place in March 2026 in the Colorado Desert of Southern California, the JPL team deployed ERNEST at all times of the day — including dusk, dawn, and nighttime, when lighting conditions create long shadows like those seen on the Moon’s polar regions.

On a bleak stretch of the Colorado Desert in Southern California, a compact four-wheeled rover recently trundled about 16 miles (26 kilometers) with minimal intervention from the team of engineers trailing it. Called ERNEST (Exploration Rover for Navigating Extreme Sloped Terrain), this prototype is being used by NASA to advance both robotic autonomy and the ability to traverse challenging landscapes.

Developed at NASA’s Jet Propulsion Laboratory in Southern California, ERNEST is 4 feet (1.2 meters) long. Not only can it lift each of its mesh wheels to get past obstacles that would stymie Curiosity and Perseverance, NASA’s six-wheeled Mars rovers, but the prototype also has enhanced independent decision-making capabilities. These mobility and autonomy advances could be infused into future missions that will venture to previously inaccessible areas of the Red Planet or the Moon.

ERNEST serves as a testbed for a potential future lunar rover mission requiring high speeds and extreme distances. In a recent field test, the prototype traveled 16 miles over the course of 37 hours, going an order of magnitude above the top speed at which NASA’s current Mars rovers can navigate. Credit: NASA/JPL-Caltech

In the field, ERNEST served as a testbed for a potential future lunar mission requiring higher speeds and much greater mileage than can be accomplished by current rovers. This technology could be used to inform future designs for exploration efforts on the Moon and beyond.

“This testing is helping us refine the mobility hardware and autonomy software to navigate extreme distances across a wide range of terrain and lighting conditions anticipated on the Moon,” said Issa Nesnas, a principal technologist at JPL who led the recent testing as head of autonomy for a NASA mission concept for a potential future long-range lunar rover.

Against a pitch-black background sky in which a handful of white stars are visible, two men stand on either side of a 4.5-foot-tall white rover, which is lit up by the glow from their headlamps as they set up the illuminators on the robot’s mast.
Engineers from JPL set up illuminators after transporting ERNEST for a pre-sunrise test during a seven-day desert field campaign.
NASA/JPL-Caltech

Nesnas’ team is using ERNEST to demonstrate it is possible to build a rover that’s twice as big as the prototype and capable of a long-distance Moon mission. During the recent campaign, ERNEST traveled at speeds up to 0.6 mph (1 kph) over 37 hours of driving, across seven days of intermittent testing. That’s an order of magnitude above the top speed Perseverance and Curiosity can navigate.

“You could do a science road trip across the Moon — or Mars — with this vehicle,” said James Keane, a JPL planetary scientist working on lunar missions.

The initial goal of the team that developed ERNEST was mechanical: to design a relatively simple, low-cost rover that advances the trusted rocker-bogie suspension system featured on every Mars rover since NASA’s Sojourner. This passive system keeps relatively constant weight on all six wheels, thanks to pivot points and struts that enable each one to adapt to the changing surface.

The mobility and autonomy advances developed at JPL for the ERNEST prototype rover could be infused into future NASA missions to previously inaccessible areas of the Red Planet or the Moon. Credit: NASA/JPL-Caltech

On ERNEST, the active suspension lets the rover manage weight distribution among its wheels. Two powered joints in front articulate a gimbal that allows the rover to drive using different gaits like squirming, wheel-walking, and obstacle-climbing. With a clutch mechanism, it can switch between active and passive suspension, which is less terrain capable but more energy efficient. With four steerable wheels, it can drive in any direction, including sideways.

“We started by postulating that we could do better in designing a planetary surface robotic mobility system,” said Hari Nayar, a JPL principal technologist leading the ERNEST team. “While the rocker-bogie system has been very successful over the past 30 years, there’s been a lot of research in that time on mobility and understanding terrain interaction.”

Before arriving at today’s version of ERNEST, the team built two earlier prototypes, each about 2 feet (0.6 meters) long, to test 11 active suspension configurations. In a trailer filled with lunar regolith simulant, they ran experiments at different slope angles over several months before landing on a final design.

Then the team scaled up, including adding a rectangular head mounted on a 4.5-foot-tall (1.4-meter-tall) mast. The hardware was completed in September 2024, but the rover still needed a human operator to joystick it, sending commands to instruct the rover on how to move over obstacles.

In order to train the rover to think on its own, the ERNEST team turned to reinforcement learning, a type of artificial intelligence where the robot learns by interacting with its environment. The Dynamics and Real-Time Simulation Laboratory at JPL developed a high-fidelity virtual testing environment that replicates the rover’s behavior. The team fed the simulator data collected by engineers who documented the response of the actual rover hardware to a variety of terrain types. On a high-performance computing cluster, the team ran many simulations at once, sometimes completing thousands of hours of tests over a single weekend.

After months of virtual training, the ERNEST team was ready to see if the rover could use its new autonomous algorithms to figure out how to drive over terrain features that would halt a passive-suspension rover. They set up an obstacle course with sand ripples, rubble piles, steps, and steep slopes in JPL’s Mars Yard, an outdoor terrain proving ground. Then they watched as the rover maneuvered the terrain on its own. Since then, ERNEST has completed many such courses.

Nayar’s team is starting a new autonomy project which involves integrating the rover’s ability to determine when and how to use its active suspension with longer-range intelligent navigation. The goal is to enable ERNEST to plan an efficient path so that it can tackle surmountable obstacles and circumnavigate hazardous ones. These capabilities could contribute to potential future rover missions encountering formidable landscapes on Mars or more rugged areas of the Moon.

Work on ERNEST began in 2022 was initially supported by JPL internal research and development funds. It is currently funded by NASA’s Mars Exploration Program and the agency’s Exploration Science Strategy and Integration Office in its Science Mission Directorate at NASA Headquarters in Washington. Caltech in Pasadena, California, manages JPL for NASA.

Media Contacts

Karen Fox / Molly Wasser
NASA Headquarters, Washington
240-285-5155 / 240-419-1732
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov   

Melissa Pamer
Jet Propulsion Laboratory, Pasadena, Calif.
626-314-4928
melissa.pamer@jpl.nasa.gov

2026-040

The post NASA Testing Advanced Capabilities for Moon, Mars Rovers appeared first on NASA Science.

NASA Testing Advanced Capabilities for Moon, Mars Rovers

18 June 2026 at 19:19
A white four-wheeled rover with a rectangular head on its mast projects a red glow onto a dark desert landscape. Pink and yellow hues indicate the sun has set behind a distant mountain range, while the top of the frame remains blue.
Developed at NASA’s Jet Propulsion Laboratory, ERNEST (Exploration Rover for Navigating Extreme Sloped Terrain) is used in a desert field test to help refine mobility hardware and autonomy software that could be used for a potential future long-range lunar rover mission.
A white four-wheeled rover on the left side of the frame casts a long shadow across barren, brown ground toward the lower right. A few low, scrubby plants dot the desert landscape and mountains rise in the far distance under a pale blue sky.
During the field test, which took place in March 2026 in the Colorado Desert of Southern California, the JPL team deployed ERNEST at all times of the day — including dusk, dawn, and nighttime, when lighting conditions create long shadows like those seen on the Moon’s polar regions.

On a bleak stretch of the Colorado Desert in Southern California, a compact four-wheeled rover recently trundled about 16 miles (26 kilometers) with minimal intervention from the team of engineers trailing it. Called ERNEST (Exploration Rover for Navigating Extreme Sloped Terrain), this prototype is being used by NASA to advance both robotic autonomy and the ability to traverse challenging landscapes.

Developed at NASA’s Jet Propulsion Laboratory in Southern California, ERNEST is 4 feet (1.2 meters) long. Not only can it lift each of its mesh wheels to get past obstacles that would stymie Curiosity and Perseverance, NASA’s six-wheeled Mars rovers, but the prototype also has enhanced independent decision-making capabilities. These mobility and autonomy advances could be infused into future missions that will venture to previously inaccessible areas of the Red Planet or the Moon.

ERNEST serves as a testbed for a potential future lunar rover mission requiring high speeds and extreme distances. In a recent field test, the prototype traveled 16 miles over the course of 37 hours, going an order of magnitude above the top speed at which NASA’s current Mars rovers can navigate. Credit: NASA/JPL-Caltech

In the field, ERNEST served as a testbed for a potential future lunar mission requiring higher speeds and much greater mileage than can be accomplished by current rovers. This technology could be used to inform future designs for exploration efforts on the Moon and beyond.

“This testing is helping us refine the mobility hardware and autonomy software to navigate extreme distances across a wide range of terrain and lighting conditions anticipated on the Moon,” said Issa Nesnas, a principal technologist at JPL who led the recent testing as head of autonomy for a NASA mission concept for a potential future long-range lunar rover.

Against a pitch-black background sky in which a handful of white stars are visible, two men stand on either side of a 4.5-foot-tall white rover, which is lit up by the glow from their headlamps as they set up the illuminators on the robot’s mast.
Engineers from JPL set up illuminators after transporting ERNEST for a pre-sunrise test during a seven-day desert field campaign.
NASA/JPL-Caltech

Nesnas’ team is using ERNEST to demonstrate it is possible to build a rover that’s twice as big as the prototype and capable of a long-distance Moon mission. During the recent campaign, ERNEST traveled at speeds up to 0.6 mph (1 kph) over 37 hours of driving, across seven days of intermittent testing. That’s an order of magnitude above the top speed Perseverance and Curiosity can navigate.

“You could do a science road trip across the Moon — or Mars — with this vehicle,” said James Keane, a JPL planetary scientist working on lunar missions.

The initial goal of the team that developed ERNEST was mechanical: to design a relatively simple, low-cost rover that advances the trusted rocker-bogie suspension system featured on every Mars rover since NASA’s Sojourner. This passive system keeps relatively constant weight on all six wheels, thanks to pivot points and struts that enable each one to adapt to the changing surface.

The mobility and autonomy advances developed at JPL for the ERNEST prototype rover could be infused into future NASA missions to previously inaccessible areas of the Red Planet or the Moon. Credit: NASA/JPL-Caltech

On ERNEST, the active suspension lets the rover manage weight distribution among its wheels. Two powered joints in front articulate a gimbal that allows the rover to drive using different gaits like squirming, wheel-walking, and obstacle-climbing. With a clutch mechanism, it can switch between active and passive suspension, which is less terrain capable but more energy efficient. With four steerable wheels, it can drive in any direction, including sideways.

“We started by postulating that we could do better in designing a planetary surface robotic mobility system,” said Hari Nayar, a JPL principal technologist leading the ERNEST team. “While the rocker-bogie system has been very successful over the past 30 years, there’s been a lot of research in that time on mobility and understanding terrain interaction.”

Before arriving at today’s version of ERNEST, the team built two earlier prototypes, each about 2 feet (0.6 meters) long, to test 11 active suspension configurations. In a trailer filled with lunar regolith simulant, they ran experiments at different slope angles over several months before landing on a final design.

Then the team scaled up, including adding a rectangular head mounted on a 4.5-foot-tall (1.4-meter-tall) mast. The hardware was completed in September 2024, but the rover still needed a human operator to joystick it, sending commands to instruct the rover on how to move over obstacles.

In order to train the rover to think on its own, the ERNEST team turned to reinforcement learning, a type of artificial intelligence where the robot learns by interacting with its environment. The Dynamics and Real-Time Simulation Laboratory at JPL developed a high-fidelity virtual testing environment that replicates the rover’s behavior. The team fed the simulator data collected by engineers who documented the response of the actual rover hardware to a variety of terrain types. On a high-performance computing cluster, the team ran many simulations at once, sometimes completing thousands of hours of tests over a single weekend.

After months of virtual training, the ERNEST team was ready to see if the rover could use its new autonomous algorithms to figure out how to drive over terrain features that would halt a passive-suspension rover. They set up an obstacle course with sand ripples, rubble piles, steps, and steep slopes in JPL’s Mars Yard, an outdoor terrain proving ground. Then they watched as the rover maneuvered the terrain on its own. Since then, ERNEST has completed many such courses.

Nayar’s team is starting a new autonomy project which involves integrating the rover’s ability to determine when and how to use its active suspension with longer-range intelligent navigation. The goal is to enable ERNEST to plan an efficient path so that it can tackle surmountable obstacles and circumnavigate hazardous ones. These capabilities could contribute to potential future rover missions encountering formidable landscapes on Mars or more rugged areas of the Moon.

Work on ERNEST began in 2022 was initially supported by JPL internal research and development funds. It is currently funded by NASA’s Mars Exploration Program and the agency’s Exploration Science Strategy and Integration Office in its Science Mission Directorate at NASA Headquarters in Washington. Caltech in Pasadena, California, manages JPL for NASA.

Media Contacts

Karen Fox / Molly Wasser
NASA Headquarters, Washington
240-285-5155 / 240-419-1732
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov   

Melissa Pamer
Jet Propulsion Laboratory, Pasadena, Calif.
626-314-4928
melissa.pamer@jpl.nasa.gov

2026-040

💾

Engineers from NASA’s Jet Propulsion Laboratory are field-testing advanced capabilities for potential future Moon and Mars rovers. In the Colorado Desert nea...

AI/ML STIG Leadership Council Nominations Are Open!

18 June 2026 at 18:42

AI/ML STIG Leadership Council Nominations Are Open!

Nominate yourself or a colleague to join the leadership council of the NASA AI/ML Science and Technology Interest Group (STIG). We welcome early-career researchers (graduate students, postdocs, and early-career scientists) broadly interested in AI and astronomy. Duties are light: suggesting speakers and helping run remote seminars by sending reminders and introducing the speaker.

https://docs.google.com/forms/d/e/1FAIpQLSc5ccFmCWEw-fDmkjlldeUvSK81f6M_2DauycSif3GN3rw9tw/viewform

As we begin planning the next iteration of the NASA Artificial Intelligence and Machine Learning Science and Technology Interest Group (AI/ML STIG) seminar series, we are expanding our leadership council and would love your help. We are writing to invite you to nominate yourself or a colleague to join.

We are especially looking for early-career researchers, including graduate students, postdocs, and early-career scientists, who are broadly interested in the intersection of AI and astronomy. You do not need to be an expert across the whole field; curiosity and a willingness to help the community learn matter most.

The organizational duties are light. Council members help suggest speakers and run the remote seminars, which mainly means sending email reminders and introducing the speaker. It is a great way to meet people across the field and to help shape a series that reaches the NASA community and beyond.

Two themes will anchor next year’s series:

  1. Agentic AI for Astrophysics. How LLM agents and multi-agent systems can accelerate astronomical research, from literature and data analysis to simulation and discovery workflows.
  2. AI and Astronomy in the US: Initiatives, Funding, and Broader Impacts. The wider landscape of AI in astronomy, including national initiatives, funding opportunities, AI pedagogy, the ethics and philosophy of AI in science, and ways AI can support NASA priorities such as ASTRA.

Please use this Google form to nominate yourself or someone else by the end of next week (extended to 27 June 2026).

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post AI/ML STIG Leadership Council Nominations Are Open! appeared first on NASA Science.

TODAY: Planning for the Future of Astrophysics & the ASTRA Initiative, 18 June 2026

18 June 2026 at 18:03

TODAY: Planning for the Future of Astrophysics and the ASTRA Initiative, June 18th, 2026

10:00am – 11:30am PT

Dear Astrophysics Strategic Technology & Research Accelerator (ASTRA) community members this serves as a reminder for those attending AAS248. This session is in-person only.

AAS248 Block Schedule: https://submissions.mirasmart.com/AAS248/Itinerary/EventDetail.aspx?evt=70

Summary

NASA’s astrophysics fleet of observatories push the limits of human vision and understanding, exploring the most profound questions of our existence while driving innovations that transform the extraordinary into the everyday and reinforce U.S. leadership in space. This special session, organized by the NASA Astrophysics Division, will provide insight into the ASTRA Initiative, share initial findings from the May 2026 Innovation for Astrophysics Missions Workshop, and will discuss plans for the September 2026 Astrophysics community science (Ad ASTRA) workshop. Talks will be followed by a panel to address questions from the community.

TimeSessionLocation
10:00am ‑ 11:30amSpecial Session: Planning for the Future of Astrophysics and the ASTRA Initiative Pasadena Convention Center ‑ 
Ballroom G

ASTRA Initiative Special Session

TimeTopicSpeaker
10:00am ‑ 10:10amIntroduction from the NASA Astrophysics Division DirectorShawn Domagal‑Goldman, NASA HQ
10:10am ‑ 10:25amThe ASTRA Initiative: Overview & Path ForwardJessica Gaskin, NASA HQ
10:25am ‑ 10:40amInnovation for Astrophysics Workshop: Initial FindingsKendra Short, JPL
10:40am ‑ 10:55amAd ASTRA Community Science WorkshopPeter Kurczynski, NASA/GSFC
10:55am ‑ 11:30amPanel DiscussionFrancesca Civano, NASA/GSFC

Wishing you the best,

Dr Ron Gamble
Cosmic Origins Support Scientist, NASA GSFC

Dr Bernard Kelly
PhysCOS Support Scientist, NASA GSFC

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post TODAY: Planning for the Future of Astrophysics & the ASTRA Initiative, 18 June 2026 appeared first on NASA Science.

TODAY! NASA’s Big Science, Small Missions

16 June 2026 at 16:58

TODAY! NASA’s Big Science, Small Missions

16 June 2026

Tuesday, June 16th, 2026
1:00pm – 2:30pm

For Cosmic Origins at AAS, please visit the link below. 

https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/cosmic-origins-at-aas-248-june-2026

Splinter Session: NASA’s Big Science, Small Missions

Tuesday, June 16th, 1:00pm – 2:30pm ET, 10:00am -11:30am PT (Hybrid Session)

For remote participation, please look for the “Join the Session” link above the agenda on the Cosmic Origins at AAS website.

High-Impact Science
Smarter, Faster, Together

Agenda

Organizers: Swara Ravindranath (NASA/GSFC), Emily Witt (JHU)

TimeTopicSpeaker
10:00am ‑ 10:05amWelcomeSwara Ravindranath (NASA/GSFC)
10:05am ‑ 10:15amFORTIS Sounding RocketEmily Witt (JHU)
10:15am ‑ 10:25amBlackCAT CubeSatAbe Falcone (Pennsylvania State University)
10:25am ‑ 10:35amSunRISE CubeSat ConstellationJoseph Lazio (University of Michigan)
10:35am ‑ 10:45amSPHEREx Medium Explorer MissionRoberta Paladini (IPAC/Caltech)
10:45am ‑ 10:55am Landolt Pioneer MissionPeter Kurczynski (NASA/GSFC)
10:55am ‑ 11:05amNon-Traditional Path to MissionsSanchayeeta Borthakur (Arizona State University)
11:05am ‑ 11:10amBREAK
11:10am ‑ 11:30amPanel DiscussionSwara Ravindranath (NASA/GSFC, moderator) Panelists: Drew Miles (Caltech), Pablo Saz Parkinson (NASA HQ), Joseph Lazio (University of Michigan), Abe Falcone (Pennsylvania State University), David Ardila (JPL)
American Astronomical Society

The 248th Meeting of the AAS

The 248th AAS meeting (joint with the High Energy Astrophysics and the Laboratory Astrophysics Divisions) will be held 14-18 June 2026 in Pasadena, California.

Learn More
Black line art with letters on a white background
American Astronomical Society (AAS)

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post TODAY! NASA’s Big Science, Small Missions appeared first on NASA Science.

Department of Health and Human Services Digital Stockpile & Manufacturing Response Network Challenge

16 June 2026 at 15:39
Alexandre – stock.adobe.com

NASA’s Center of Excellence for Collaborative Innovation (CoECI) assists in the use of crowdsourcing across the federal government. CoECI’s NASA Tournament Lab offers the contract capability to run external crowdsourced challenges on behalf of NASA and other agencies.

Sponsored by the Administration for Strategic Preparedness and Response (ASPR), a division of the U.S. Department of Health and Human Services (HHS), this prize competition seeks forward-thinking solutions to strengthen the nation’s ability to rapidly produce and distribute critical medical supplies during public health emergencies and supply chain disruptions. Through three challenge phases, participants will develop an innovative conceptual systems design using technologies and frameworks that advance the future of resilient medical manufacturing, logistics, and digital coordination capabilities.

Phase 1: Participants will submit:

  • 8-page submission paper
  • 3-minute Pitch video
  • Blueprint supporting the key capabilities and structure of the solution

Submissions will be evaluated per challenge Judging Criteria. Following the Judge evaluation period, up to 8 Finalists will receive a $5,000 prize each and be invited to the hybrid (in-person and virtual) Pitch Event at ASPR headquarters in Washington, DC. Up to 3 Winners from the Pitch Event will receive a $150,000 prize each and be invited to the innovation development phase.

Phase 2: Two developmental milestones will monitor solution development and will include $75,000 additional prizes for each milestone complete (up to $150,000 in total milestone prize payments).

Phase 3: At the end of the development milestone period, up to 3 teams may be invited to the final Live Validation Event to test their solution under applicable real-world simulations and compete for a total prize purse up to $1,100,000.

‍Total Prizes: Up to $2.04 Million

Challenge Launch: June 15, 2026

Phase 1 Submissions Due: August 28, 2026

For more information, visit: https://www.expeditionhacks.com/challenges/digital-stockpile-challenge

The post Department of Health and Human Services Digital Stockpile & Manufacturing Response Network Challenge appeared first on NASA Science.

Department of Health and Human Services Digital Stockpile & Manufacturing Response Network Challenge

16 June 2026 at 15:39
Alexandre – stock.adobe.com

NASA’s Center of Excellence for Collaborative Innovation (CoECI) assists in the use of crowdsourcing across the federal government. CoECI’s NASA Tournament Lab offers the contract capability to run external crowdsourced challenges on behalf of NASA and other agencies.

Sponsored by the Administration for Strategic Preparedness and Response (ASPR), a division of the U.S. Department of Health and Human Services (HHS), this prize competition seeks forward-thinking solutions to strengthen the nation’s ability to rapidly produce and distribute critical medical supplies during public health emergencies and supply chain disruptions. Through three challenge phases, participants will develop an innovative conceptual systems design using technologies and frameworks that advance the future of resilient medical manufacturing, logistics, and digital coordination capabilities.

Phase 1: Participants will submit:

  • 8-page submission paper
  • 3-minute Pitch video
  • Blueprint supporting the key capabilities and structure of the solution

Submissions will be evaluated per challenge Judging Criteria. Following the Judge evaluation period, up to 8 Finalists will receive a $5,000 prize each and be invited to the hybrid (in-person and virtual) Pitch Event at ASPR headquarters in Washington, DC. Up to 3 Winners from the Pitch Event will receive a $150,000 prize each and be invited to the innovation development phase.

Phase 2: Two developmental milestones will monitor solution development and will include $75,000 additional prizes for each milestone complete (up to $150,000 in total milestone prize payments).

Phase 3: At the end of the development milestone period, up to 3 teams may be invited to the final Live Validation Event to test their solution under applicable real-world simulations and compete for a total prize purse up to $1,100,000.

‍Total Prizes: Up to $2.04 Million

Challenge Launch: June 15, 2026

Phase 1 Submissions Due: August 28, 2026

For more information, visit: https://www.expeditionhacks.com/challenges/digital-stockpile-challenge

IR STIG PRIMA Seminar, 22 June 2026

16 June 2026 at 00:56

IR STIG PRIMA Seminar

Infrared Science and Technology Interest Group

Over the next few months, our talk series will be highlighting research from PRIMA’s Working Groups, with this talk focusing on dust properties in galaxies in the nearby universe.  Stay tuned as well for overview talks this fall that highlight PRIMA’s PI science in the areas of Protoplanetary Disks and the Evolution of Dust and Metals. 

IR STIG about IR STIG PRIMA Seminar

Location

Virtual

Dates

22 June 2026
9:00am PT / 12:00pm ET

Community

IR STIG

Type

Seminar

Speaker

Bogdan Pastrav (Institute of Space Science)

Seminar Connection

Please visit the P-CAST webpage https://prima.ipac.caltech.edu/page/p-cast for a link to join and to see all of our upcoming speakers!

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post IR STIG PRIMA Seminar, 22 June 2026 appeared first on NASA Science.

AGN SIG Spotlight Series, 23 June 2026

16 June 2026 at 00:41

AGN SIG Spotlight Series Seminar

Active Galactic Nuclei Science Interest Group

AGN SIG about AGN SIG Spotlight Series Seminar

Location

Virtual

Dates

23 June 2026
1:00pm ET / 10:00am PT

Community

AGN SIG

Type

Seminar

Our Spotlight Series highlights recent advances in AGN science, with a strong emphasis on participation from early-career researchers, and includes plenty of time for community discussion following the presentations. 

Central Shocks and Metal-Enriched Outflows: A New View of AGN Feedback

Speaker

Peixin Zhu (Harvard University)

Abstract

The growth of galaxies and their central supermassive black holes (SMBHs) is tightly linked. However, the exact impact of active galactic nuclei (AGNs) feedback on the host galaxy is still uncertain, with different observations suggesting AGNs enhance, suppress, or do not affect the host galaxy star formation rate. Resolving these controversies requires proper treatment of shocks, which are known to exist with AGN-driven outflow and yet are difficult to distinguish from AGN emission. In my talk, I will present a new theoretical three-dimensional diagram built for integral-field spectroscopy that cleanly separates star formation, AGN, and shock-dominated spaxels. Furthermore, these separation results can be combined with theoretical diagnostics to map the spatial distribution of gas-phase metallicity, ionization parameter, and gas pressure within these galaxies. After applying this new technique to 8 nearby Seyfert galaxies, we reveal that AGN and star formation coexist in the galaxy center, and fast shocks are present at the base of AGN outflows in some galaxies. We also find that outflowing gas is systematically metal-enhanced relative to adjacent star-forming rings. I will discuss how these results refine the picture of AGN feedback and the implications for nuclear enrichment and gas transport.

Investigating AGN Feeding and Feedback Through Circumnuclear Gas Kinematics in NGC 3079 and NGC 1068

Speaker

Dr. Ming-Yi Lin (University of Toledo)

Abstract

Studying gas kinematics in the circumnuclear regions (< 100 pc) of nearby AGNs on spatial scales of <10 pc provides insights into gas transport toward the supermassive black hole (SMBH) and the impact of AGN feedback in both radiative and kinetic forms. The kinematics of cold molecular gas are observed with radio interferometers (ALMA and NOEMA), while the warm molecular gas in the near-IR are studied using adaptive optics (AO)-assisted integral field spectrographs (IFS; Keck/OSIRIS). In this talk, I will use NGC 1068 and NGC 3079, two nearby Compton-thick AGNs, as pilot targets to discuss two distinct types of molecular outflows located at distances of ~40 pc from the SMBH: a cooling-efficient, momentum-driven outflow and a cooling-inefficient, energy-driven outflow. I will also present the discrepancy between Bondi accretion prescriptions and observationally constrained mass accretion rates.

Seminar Connection

Zoom Registration, you will receive connection details by email after registration: https://zoom.us/j/97689874465?pwd=XZNUqr19oopa1LfD7hgln1aQ2vbnT2.1

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Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post AGN SIG Spotlight Series, 23 June 2026 appeared first on NASA Science.

TODAY COR at AAS 248 | Everything but Exoplanets

15 June 2026 at 17:56

Everything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory

Monday, June 15th, 10:00am -11:30am PT

This is your reminder to join the Cosmic Origins community members as they present their science and talk about relevant topics of interest across the astrophysics landscape!

For Cosmic Origins at AAS, please visit the link below. 

https://science.nasa.gov/astrophysics/programs/cosmic-origins/community/cosmic-origins-at-aas-248-june-2026

Special Session: Everything but Exoplanets: The Transformative General Astrophysics of the Habitable Worlds Observatory

Highlights from Cosmic Origins Science Interest Groups (SIGs) and Science Analysis Groups (SAGs).

TimeTopicSpeaker
10:20am – 10:30amSpatially Resolved UV Spectroscopy Science Analysis Group in Support of HWOEmily Witt (JHU)
10:30am – 10:40amInvestigating the NIR Discovery Space of the Habitable Worlds Observatory: Updates from the Red Limit Science Analysis GroupKyle Cooke (University of Louisville)
10:40am – 10:50amOpening the OVI Window to Reveal the Diffuse Cosmic Ecosystem with HWOSanchayeeta Borthakur (Arizona State University)
11:00am -11:10amHWO Science Interest Group: Keeping the Community Connected to HWOJessie Christiansen (Caltech/IPAC)

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Sign Up
Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.

The post TODAY COR at AAS 248 | Everything but Exoplanets appeared first on NASA Science.

Experience the Launch of NASA’s Roman Space Telescope 

15 June 2026 at 15:28
8 Min Read

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.

APPLY NOW 

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. 

The post Experience the Launch of NASA’s Roman Space Telescope  appeared first on NASA Science.

UK unveils sweeping social media ban for users under 16

15 June 2026 at 15:36
The ban would apply to a range of social media platforms, including Snapchat, TikTok, YouTube, Instagram, Facebook, and X.

Experience the Launch of NASA’s Roman Space Telescope 

15 June 2026 at 15:28
8 Min Read

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.

APPLY NOW 

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 11:59 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 July 17 and waitlist notifications on July 22. 

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. 

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