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Preparations for Next Moonwalk Simulations Underway (and Underwater) This image shows about 1.5% of Euclid’s Deep Field South, one of three regions of the sky that the telescope will observe for more than 40 weeks over the course of its prime mission, spotting faint and distant galaxies. One galaxy cluster near the center is located almost 6 billion light-years away from Earth. ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre, E. Bertin, G. An-selmi

With contributions from NASA, the mission is looking back into the universe’s history to understand how the universe’s expansion has changed. 

The Euclid mission — led by ESA (European Space Agency) with contributions from NASA — aims to find out why our universe is expanding at an accelerating rate. Astronomers use the term “dark energy” to refer to the unknown cause of this phenomenon, and Euclid will take images of billions of galaxies to learn more about it. A portion of the mission’s data was released to the public by ESA on Wednesday, March 19.

This new data has been analyzed by mission scientists and provides a glimpse of Euclid’s progress. Deemed a “quick” data release, this batch focuses on select areas of the sky to demonstrate what can be expected in the larger data releases to come and to allow scientists to sharpen their data analysis tools in preparation.

The data release contains observations of Euclid’s three “deep fields,” or areas of the sky where the space telescope will eventually make its farthest observations of the universe. Featuring one week’s worth of viewing, the Euclid images contain 26 million galaxies, the most distant being over 10.5 billion light-years away. Launched in July 2023, the space telescope is expected to observe more than 1.5 billion galaxies during its six-year prime mission.

The entirety of the Euclid mission’s Deep Field South region is shown here. It is about 28.1 square degrees on the sky. Euclid will observe this and two other deep field regions for a total of about 40 weeks during its 6-year primary mission. ESA/Euclid/Euclid Consortium/NASA; image processing by J.-C. Cuillandre, E. Bertin, G. An-selmi

By the end of that prime mission, Euclid will have observed the deep fields for a total of about 40 weeks in order to gradually collect more light, revealing fainter and more distant galaxies. This approach is akin to keeping a camera shutter open to photograph a subject in low light.

The first deep field observations, taken by NASA’s Hubble Space Telescope in 1995, famously revealed the existence of many more galaxies in the universe than expected. Euclid’s ultimate goal is not to discover new galaxies but to use observations of them to investigate how dark energy’s influence has changed over the course of the universe’s history.

In particular, scientists want to know how much the rate of expansion has increased or slowed down over time. Whatever the answer, that information would provide new clues about the fundamental nature of this phenomenon. NASA’s Nancy Grace Roman Space Telescope, set to launch by 2027, will also observe large sections of the sky in order to study dark energy, complementing Euclid’s observations.

The locations of the Euclid deep fields are shown marked in yellow on this all-sky view from ESA’s Gaia and Planck missions. The bright horizontal band is the plane of our Milky Way galaxy. Of the two regions highlighted at bottom right, Euclid’s Deep Field South is the one at left.ESA/Euclid/Euclid Consortium/NASA; ESA/Gaia/DPAC; ESA/Planck Collaboration Looking Back in Time

To study dark energy’s effect throughout cosmic history, astronomers will use Euclid to create detailed, 3D maps of all the stuff in the universe. With those maps, they want to measure how quickly dark energy is causing galaxies and big clumps of matter to move away from one another. They also want to measure that rate of expansion at different points in the past. This is possible because light from distant objects takes time to travel across space. When astronomers look at distant galaxies, they see what those objects looked like in the past.

For example, an object 100 light-years away looks the way it did 100 years ago. It’s like receiving a letter that took 100 years to be delivered and thus contains information from when it was written. By creating a map of objects at a range of distances, scientists can see how the universe has changed over time, including how dark energy’s influence may have varied.

But stars, galaxies, and all the “normal” matter that emits and reflects light is only about one-fifth of all the matter in the universe. The rest is called “dark matter” — a material that neither emits nor reflects light. To measure dark energy’s influence on the universe, astronomers need to include dark matter in their maps.  

Bending and Warping

Although dark matter is invisible, its influence can be measured through something called gravitational lensing. The mass of both normal and dark matter creates curves in space, and light traveling toward Earth bends or warps as it encounters those curves. In fact, the light from a distant galaxy can bend so much that it forms an arc, a full circle (called an Einstein ring), or even multiple images of the same galaxy, almost as though the light has passed through a glass lens.

In most cases, gravitational lensing warps the apparent shape of a galaxy so subtly that researchers need special tools and computer software to see it. Spotting those subtle changes across billions of galaxies enables scientists to do two things: create a detailed map of the presence of dark matter and observe how dark energy influenced it over cosmic history.

It is only with a very large sample of galaxies that researchers can be confident they are seeing the effects of dark matter. The newly released Euclid data covers 63 square degrees of the sky, an area equivalent to an array of 300 full Moons. To date, Euclid has observed about 2,000 square degrees, which is approximately 14% of its total survey area of 14,000 square degrees. By the end of its mission, Euclid will have observed a third of the entire sky.

The dataset released this month is described in several preprint papers available today. The mission’s first cosmology data will be released in October 2026. Data accumulated over additional, multiple passes of the deep field locations will also be included in the 2026 release.

More About Euclid

Euclid is a European mission, built and operated by ESA, with contributions from NASA. The Euclid Consortium — consisting of more than 2,000 scientists from 300 institutes in 15 European countries, the United States, Canada, and Japan — is responsible for providing the scientific instruments and scientific data analysis. ESA selected Thales Alenia Space as prime contractor for the construction of the satellite and its service module, with Airbus Defence and Space chosen to develop the payload module, including the telescope. Euclid is a medium-class mission in ESA’s Cosmic Vision Programme.

Three NASA-supported science teams contribute to the Euclid mission. In addition to designing and fabricating the sensor-chip electronics for Euclid’s Near Infrared Spectrometer and Photometer (NISP) instrument, JPL led the procurement and delivery of the NISP detectors as well. Those detectors, along with the sensor chip electronics, were tested at NASA’s Detector Characterization Lab at Goddard Space Flight Center in Greenbelt, Maryland. The Euclid NASA Science Center at IPAC (ENSCI), at Caltech in Pasadena, California, supports U.S.-based science investigations, and science data is archived at the NASA / IPAC Infrared Science Archive (IRSA). JPL is a division of Caltech.

For more information about Euclid go to:

science.nasa.gov/mission/euclid/

News Media Contact

ESA Media Relations
media@esa.int

Calla Cofield
Jet Propulsion Laboratory, Pasadena, Calif.
626-808-2469
calla.e.cofield@jpl.nasa.gov

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Details Last Updated Mar 19, 2025 Related Terms

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This compressed, resolution-limited gif shows the view of lunar sunset from one of the six Stereo Cameras for Lunar-Plume Surface Studies (SCALPSS) 1.1 cameras on Firefly’s Blue Ghost lander, which operated on the Moon’s surface for a little more than 14 days and stopped, as anticipated, a few hours into lunar night. SCALPSS was taking images every 10 minutes during the sunset. The bright, swirly light moving across the surface on the top right of the image is sunlight reflecting off the lander. Images taken by SCALPSS 1.1 during Blue Ghost’s descent and landing, as well as images from the surface during the long lunar day, will help researchers better understand the effects of a lander’s engine plumes on the lunar soil, or regolith. The instrument collected almost 9000 images and returned 10 GB of data. This data is important as trips to the Moon increase and the number of payloads touching down in proximity to one another grows. The SCALPSS 1.1 project is funded by the Space Technology Mission Directorate’s Game Changing Development program. SCALPSS was developed at NASA’s Langley Research Center in Hampton, Virginia, with support from Marshall Space Flight Center in Huntsville, Alabama.

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Sols 4481-4483: Humber Pie NASA’s Mars rover Curiosity acquired this image using its Front Hazard Avoidance Camera (Front Hazcam) on March 14, 2025 — sol 4480, or Martian day 4,480 of the Mars Science Laboratory mission — at 08:53:19 UTC.NASA/JPL-Caltech

Written by Michelle Minitti, Planetary Geologist at Framework

Earth planning date: Friday, March 14, 2025

The rover successfully arrived at the “Humber Park” outcrop which, on this fine “Pi Day” on Earth, we could convince ourselves looked like a pie with a sandy interior and a rough and rocky crust. We can only hope our instruments are as excited to tuck into this outcrop as the Curiosity team is to eat our pizzas and favorite pies (for me, pumpkin) this afternoon and evening. 

MAHLI gets a big serving of rock structures from the Humber Park “crust” with three separate imaging targets. One observation, at the target “Yerba Buena Ridge,” covers structures expressed across the front of the outcrop in the above image. A second target, “Sepulveda Pass,” has intriguing texture that warranted multiple flavors of stereo imaging. The final target, which MAHLI shared with APXS, was “South Fork.” It was the clearest place to put APXS down on the rough bedrock blocks. 

ChemCam also feasted on rock chemistry from an array of targets with different textures. “Ridge Route” covered a low-lying bedrock slab with the fine layering we have seen consistently through the sulfate unit, while “Toyon Canyon” covered a lumpier portion of the Humber Park outcrop above Yerba Buena Ridge. The “Mount Lawlor” target was a mix of Ridge Route and Toyon Canyon — layered, but on a high-standing portion of the outcrop that also had some unusual chains of pits. ChemCam added two long distance mosaics on “Gould Mesa” to the menu, which captured a variety of structures on this impressive butte about 100 meters ahead of the rover. 

Mastcam focused on covering the whole of Humber Park with a stereo mosaic but also added small mosaics across a trough in the sand and a bedrock block with potential cross bedding at “Rancho Los Feliz.” Because just imaging this side of Humber Park was not enough, Mastcam and Navcam worked closely with the rover drivers to plan a mid-drive mosaic of the other side of the outcrop so we fully capture Humber Park’s “crust.”

Our environmental observations were not just pie in the sky but will help us monitor the chemistry of and the amount of dust in the atmosphere, and record clouds and dust devils crossing above and around us.

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NASA astronauts Nick Hague, Suni Williams, Butch Wilmore, and Roscosmos cosmonaut Aleksandr Gorbunov land in a SpaceX Dragon spacecraft in the water off the coast of Tallahassee, Florida on March 18, 2025. Hague, Gorbunov, Williams, and Wilmore returned from a long-duration science expedition aboard the International Space Station. Credit: NASA/Keegan Barber

NASA’s SpaceX Crew-9 completed the agency’s ninth commercial crew rotation mission to the International Space Station on Tuesday, splashing down safely in a SpaceX Dragon spacecraft off the coast of Tallahassee, Florida, in the Gulf of America.

NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore, and Roscosmos cosmonaut Aleksandr Gorbunov, returned to Earth at 5:57 p.m. EDT. Teams aboard SpaceX recovery vessels retrieved the spacecraft and its crew. After returning to shore, the crew will fly to NASA’s Johnson Space Center in Houston and reunite with their families.

“We are thrilled to have Suni, Butch, Nick, and Aleksandr home after their months-long mission conducting vital science, technology demonstrations, and maintenance aboard the International Space Station,” said NASA acting Administrator Janet Petro. “Per President Trump’s direction, NASA and SpaceX worked diligently to pull the schedule a month earlier. This international crew and our teams on the ground embraced the Trump Administration’s challenge of an updated, and somewhat unique, mission plan, to bring our crew home. Through preparation, ingenuity, and dedication, we achieve great things together for the benefit of humanity, pushing the boundaries of what is possible from low Earth orbit to the Moon and Mars.”

Hague and Gorbunov lifted off at 1:17 p.m. Sept. 28, 2024, on a SpaceX Falcon 9 rocket from Space Launch Complex 40 at Cape Canaveral Space Force Station in Florida. The next day, they docked to the forward-facing port of the station’s Harmony module. Williams and Wilmore launched aboard Boeing’s Starliner spacecraft and United Launch Alliance Atlas V rocket on June 5, 2024, from Space Launch Complex 41 as part of the agency’s Boeing Crew Flight Test. The duo arrived at the space station on June 6. In August, NASA announced the uncrewed return of Starliner to Earth and integrated Wilmore and Williams as part of the space station’s Expedition 71/72 for a return on Crew-9. The crew of four undocked at 1:05 a.m. Tuesday to begin the trip home.

Williams and Wilmore traveled 121,347,491 miles during their mission, spent 286 days in space, and completed 4,576 orbits around Earth. Hague and Gorbunov traveled 72,553,920 miles during their mission, spent 171 days in space, and completed 2,736 orbits around Earth. The Crew-9 mission was the first spaceflight for Gorbunov. Hague has logged 374 days in space over his two missions, Williams has logged 608 days in space over her three flights, and Wilmore has logged 464 days in space over his three flights.

Throughout its mission, Crew-9 contributed to a host of science and maintenance activities and technology demonstrations. Williams conducted two spacewalks, joined by Wilmore for one and Hague for another, removing a radio frequency group antenna assembly from the station’s truss, collecting samples from the station’s external surface for analysis, installing patches to cover damaged areas of light filters on an X-ray telescope, and more. Williams now holds the record for total spacewalking time by a female astronaut, with 62 hours and 6 minutes outside of station, and is fourth on the all-time spacewalk duration list.

The American crew members conducted more than 150 unique scientific experiments and technology demonstrations between them, with over 900 hours of research. This research included investigations on plant growth and quality, as well as the potential of stem cell technology to address blood diseases, autoimmune disorders, and cancers. They also tested lighting systems to help astronauts maintain circadian rhythms, loaded the first wooden satellite for deployment, and took samples from the space station’s exterior to study whether microorganisms can survive in space.

The Crew-9 mission was the fourth flight of the Dragon spacecraft named Freedom. It also previously supported NASA’s SpaceX Crew-4, Axiom Mission 2, and Axiom Mission 3. The spacecraft will return to Florida for inspection and processing at SpaceX’s refurbishing facility at Cape Canaveral Space Force Station, where teams will inspect the Dragon, analyze data on its performance, and begin processing for its next flight.

The Crew-9 flight is part of NASA’s Commercial Crew Program, and its return to Earth follows on the heels of NASA’s SpaceX Crew-10 launch, which docked to the station on March 16, beginning another long-duration science expedition.

The goal of NASA’s Commercial Crew Program is safe, reliable, and cost-effective transportation to and from the space station and low Earth orbit. The program provides additional research time and has increased opportunities for discovery aboard humanity’s microgravity testbed for exploration, including helping NASA prepare for human exploration of the Moon and Mars.

Learn more about NASA’s Commercial Crew Program at:

https://www.nasa.gov/commercialcrew

-end-

Amber Jacobson / Joshua Finch
Headquarters, Washington
202-358-1100
amber.c.jacobson@nasa.gov / joshua.a.finch@nasa.gov

Kenna Pell / Sandra Jones
Johnson Space Center, Houston
281-483-5111
kenna.m.pell@nasa.gov / sandra.p.jones@nasa.gov

Steve Siceloff / Stephanie Plucinsky
Kennedy Space Center, Florida
321-867-2468
steven.p.siceloff@nasa.gov / stephanie.n.plucinsky@nasa.gov

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Details Last Updated Mar 19, 2025 EditorJessica TaveauLocationNASA Headquarters Related Terms

• Humans in Space
• Commercial Crew
• Expedition 72
• International Space Station (ISS)
• ISS Research
• Space Operations Mission Directorate

After delivering ten NASA science and technology payloads to the near side of the Moon through NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign, Firefly Aerospace’s Blue Ghost Mission 1 lander captured this image of a sunset from the lunar surface. Credit: Firefly Aerospace

After landing on the Moon with NASA science and technology demonstrations March 2, Firefly Aerospace’s Blue Ghost Mission 1 concluded its mission March 16. Analysis of data returned to Earth from the NASA instruments continues, benefitting future lunar missions.

As part of NASA’s CLPS (Commercial Lunar Payload Services) initiative and Artemis campaign, Firefly’s Blue Ghost lunar lander delivered 10 NASA science and technology instruments to the Mare Crisium basin on the near side of the Moon. During the mission, Blue Ghost captured several images and videos, including imaging a total solar eclipse and a sunset from the surface of the Moon. The mission lasted for about 14 days, or the equivalent of one lunar day, and multiple hours into the lunar night before coming to an end.

“Firefly’s Blue Ghost Mission 1 marks the longest surface duration commercial mission on the Moon to date, collecting extraordinary science data that will benefit humanity for decades to come,” said Nicky Fox, associate administrator, Science Mission Directorate at NASA Headquarters in Washington. “With NASA’s CLPS initiative, American companies are now at the forefront of an emerging lunar economy that lights the way for the agency’s exploration goals on the Moon and beyond.”

All 10 NASA payloads successfully activated, collected data, and performed operations on the Moon. Throughout the mission, Blue Ghost transmitted 119 gigabytes of data back to Earth, including 51 gigabytes of science and technology data. In addition, all payloads were afforded additional opportunities to conduct science and gather more data for analysis, including during the eclipse and lunar sunset.

“Operating on the Moon is complex; carrying 10 payloads, more than has ever flown on a CLPS delivery before, makes the mission that much more impressive,” said Joel Kearns, deputy associate administrator for exploration, Science Mission Directorate, NASA Headquarters. “Teams are eagerly analyzing their data, and we are extremely excited for the expected scientific findings that will be gained from this mission.”

Among other achievements, many of the NASA instruments performed first-of-their-kind science and technology demonstrations, including:

• The Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity  is now the deepest robotic planetary subsurface thermal probe, drilling  up to 3 feet and providing a first-of-its kind demonstration of robotic thermal measurements at varying depths.
• The Lunar GNSS Receiver Experiment acquired and tracked Global Navigation Satellite Systems (GNSS) signals, from satellite networks such as GPS and Galileo, for the first time enroute to and on the Moon’s surface. The LuGRE payload’s record-breaking success indicates that GNSS signals could complement other navigation methods and be used to support future Artemis missions. It also acts as a stepping stone to future navigation systems on Mars. 
• The Radiation Tolerant Computer successfully operated in transit through Earth’s Van Allen belts, as well as on the lunar surface into the lunar night, verifying solutions to mitigate radiation effects on computers that could make future missions safer for equipment and more cost effective.
• The Electrodynamic Dust Shield successfully lifted and removed lunar soil, or regolith, from surfaces using electrodynamic forces, demonstrating a promising solution for dust mitigation on future lunar and interplanetary surface operations.
• The Lunar Magnetotelluric Sounder successfully deployed five sensors to study the Moon’s interior by measuring electric and magnetic fields. The instrument allows scientists to characterize the interior of the Moon to depths up to 700 miles, or more than half the distance to the Moon’s center.
• The Lunar Environment heliospheric X-ray Imager captured a series of X-ray images to study the interaction of the solar wind and Earth’s magnetic field, providing insights into how space weather and other cosmic forces surrounding Earth affect the planet. 
• The Next Generation Lunar Retroreflector successfully reflected and returned laser light from two Lunar Laser Ranging Observatories, returning measurements allowing scientists to precisely measure the Moon’s shape and distance from Earth, expanding our understanding of the Moon’s inner structure. 
• The Stereo Cameras for Lunar Plume-Surface Studies instrument captured about 9,000 images during the spacecraft’s lunar descent and touchdown on the Moon, providing insights into the effects engine plumes have on the surface. The payload also operated during the lunar sunset and into the lunar night.
• The Lunar PlanetVac was deployed on the lander’s surface access arm and successfully collected, transferred, and sorted lunar soil using pressurized nitrogen gas, demonstrating a low-cost, low-mass solution for future robotic sample collection.
• The Regolith Adherence Characterization instrument examined how lunar regolith sticks to a range of materials exposed to the Moon’s environment, which can help test, improve, and protect spacecraft, spacesuits, and habitats from abrasive lunar dust or regolith.

The data captured will benefit humanity in many ways, providing insights into how space weather and other cosmic forces may impact Earth. Establishing an improved awareness of the lunar environment ahead of future crewed missions will help plan for long-duration surface operations under Artemis.

To date, five vendors have been awarded 11 lunar deliveries under CLPS and are sending more than 50 instruments to various locations on the Moon, including the lunar South Pole and far side.

Learn more about NASA’s CLPS initiative at:

https://www.nasa.gov/clps

-end-

Alise Fisher 
Headquarters, Washington
202-617-4977
alise.m.fisher@nasa.gov

Natalia Riusech / Nilufar Ramji
Johnson Space Center, Houston
281-483-5111
nataila.s.riusech@nasa.gov / nilufar.ramji@nasa.gov

Antonia Jaramillo
Kennedy Space Center, Florida
321-501-8425
antonia.jaramillobotero@nasa.gov

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Details Last Updated Mar 19, 2025 LocationNASA Headquarters Related Terms

• Commercial Lunar Payload Services (CLPS)
• Artemis
• Blue Ghost (lander)
• Johnson Space Center
• Kennedy Space Center
• Marshall Space Flight Center
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A group of attendees of the joint NASA-USGS workshop, Planetary Subsurface Exploration for Science and Resources, gathers for a photo at NASA’s Ames Research Center on Feb. 11, 2025. Workshop participants discussed observations, technologies, and operations needed to support new economies for terrestrial and off-world resources, including critical minerals.NASA/Brandon Torres Navarrete

NASA and the U.S. Geological Survey (USGS) welcomed a community of government, industry, and international partners to explore current technology needs around natural resources – both on Earth and “off world.” During a workshop held in February at NASA’s Ames Research Center in California’s Silicon Valley, participants discussed technologies that will improve the ability to detect, assess, and develop resources, such as critical minerals and water ice to be found on our Moon, other planets and their moons, and asteroids.

More than 300 attendees, taking part in person and virtually, worked to define the elements needed to find and map resources beyond Earth to support the growing space economy. These include sensors to image the subsurface of planetary bodies, new platforms for cost-effective operations, and technologies that enable new concepts of operation for these systems.

Scientific studies and measurements of off-world sites will be key to detecting and characterizing resources of interest, creating an important synergy with technology goals and helping to answer fundamental science questions as well.

The workshop was the third in a series called Planetary Subsurface Exploration for Science and Resources. By leveraging the expertise gained from decades of resource exploration on this planet and that of the space technology and space mission communities, NASA and USGS aim to spark collaboration across industry, government, and academia to develop new concepts and technologies.

Participants in the NASA-USGS off-world resources workshop take part in a panel review of technology opportunities, Feb. 13, 2025, at NASA’s Ames Research Center. The panelists were Dave Alfano, chief of the Intelligent Systems Division at NASA’s Ames Research Center in California’s Silicon Valley (left); Rob Mueller, a senior technologist and principal investigator in the Exploration Research and Technology Programs Directorate at NASA’s Kennedy Space Center in Florida; Christine Stewart, CEO at Austmine Limited in Australia; Gerald Sanders, in-situ resource utilization system capability lead for NASA’s Space Technology Mission Directorate based at NASA’s Johnson Space Center in Houston; and Jonathon Ralston, Integrated Mining Research Team lead at Australia’s Commonwealth Scientific and Industrial Research Organisation. NASA/Brandon Torres Navarrete

NASA's SpaceX Crew-9 members pose together for a portrait inside the vestibule between the International Space Station and the SpaceX Dragon crew spacecraft.

NASA/Nick Hague

NASA astronauts Butch Wilmore, Nick Hague, and Suni Williams, and Roscosmos cosmonaut Aleksandr Gorbunov – the members of NASA’s SpaceX Crew-9 mission – smile at the camera in this Feb. 19, 2025, photo. While aboard the International Space Station, Hague, Williams, and Wilmore completed more than 900 hours of research between more than 150 unique scientific experiments and technology demonstrations during their stay aboard the orbiting laboratory.

Wilmore, Hague, Williams, and Gorbunov are set to return to Earth on Tuesday, March 18, with splashdown set for approximately 5:57 p.m. EDT.

Watch NASA’s Crew-9 return coverage at 4:45 p.m. EDT Tuesday on NASA+.

Image credit: NASA/Nick Hague

As part of NASA’s Advanced Capabilities for Emergency Response Operations flight tests in November 2024, Overwatch Aero flies a vertical takeoff and landing aircraft in Watsonville, California.Credit: NASA

NASA will conduct a live flight test of aircraft performing simulated wildland fire response operations using a newly developed airspace management system at 9 a.m. PDT on Tuesday, March 25, in Salinas, California.

NASA’s new portable airspace management system, part of the agency’s Advanced Capabilities for Emergency Response Operations (ACERO) project, aims to significantly expand the window of time crews have to respond to wildland fires. The system provides the air traffic awareness needed to safely send aircraft – including drones and remotely piloted helicopters – into wildland fire operations, even during low-visibility conditions. Current aerial firefighting operations are limited to times when pilots have clear visibility, which lowers the risk of flying into the surrounding terrain or colliding with other aircraft. This restriction grounds most aircraft at night and during periods of heavy smoke.

During this inaugural flight test, researchers will use the airspace management system to coordinate the flight operations of two small drones, an electric vertical takeoff and landing aircraft, and a remotely piloted aircraft that will have a backup pilot aboard. The drones and aircraft will execute examples of critical tasks for wildland fire management, including weather data sharing, simulated aerial ignition flights, and communications relay.

Media interested in viewing the ACERO flight testing must RSVP by 4 p.m. Friday, March 21, to the NASA Ames Office of Communications by email at: arc-dl-newsroom@mail.nasa.gov or by phone at 650-604-4789. NASA will release additional details, including address and arrival logistics, to media credentialed for the event. A copy of NASA’s media accreditation policy is online.

NASA’s ACERO researchers will use data from the flight test to refine the airspace management system. The project aims to eventually provide this technology to wildland fire crews for use in the field, helping to save lives and property. This project is managed at NASA’s Ames Research Center in California’s Silicon Valley.

For more information on ACERO, visit:

https://go.nasa.gov/4bYEzsD

-end-

Rob Margetta
Headquarters, Washington
202-358-1600
robert.j.margetta@nasa.gov

Hillary Smith
Ames Research Center, Silicon Valley
650-604-4789
hillary.smith@nasa.gov

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Details Last Updated Mar 18, 2025 EditorJessica TaveauLocationNASA Headquarters Related Terms

• Ames Research Center
• Advanced Capabilities for Emergency Response Operations
• Aeronautics
• Aeronautics Research Mission Directorate
• Flight Innovation

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Media are invited to meet leaders in the space community during the 62nd annual Goddard Space Science Symposium, taking place from Wednesday, March 19, to Friday, March 21, at Martin’s Crosswinds in Greenbelt, Maryland. The symposium will also be streamed online.

Hosted by the American Astronautical Society (AAS) in conjunction with NASA’s Goddard Space Flight Center in Greenbelt, the symposium examines the current state and future of space science and space exploration at large by convening leading minds across NASA, other government agencies, policy, academia, and industry – collectively navigating a path forward by identifying the opportunities and challenges ahead.

This year’s theme, “Pathways and Partnerships for U.S. Leadership in Earth and Space Science,” highlights the evolving collaborative landscape between the public and private sectors, as well as how it is helping the United States remain and grow as a leading space power. 

“Earth and space science are complex by nature, with a growing list of public and private enterprises carving out their space,” said Christa Peters-Lidard, co-chair of the symposium planning committee and Goddard’s director of sciences and exploration. “It’s an exciting time as we work to determine the future trajectory of space exploration in this new era, and the Goddard Space Science Symposium is an instrumental tool for gathering the insights of leading experts across a broad spectrum.”

AAS President Ron Birk and Goddard Deputy Center Director Cynthia Simmons will deliver the symposium’s opening remarks on March 19, followed by panels on enabling science and exploration from the Moon to Mars and navigating space science and exploration policy. Greg Autry, associate provost for space commercialization and strategy at the University of Central Florida, will deliver the keynote address. The first day will conclude with an industry night reception.

The second day of the symposium on Thursday, March 20, will feature panels on enhancing U.S. economic leadership through science, the Habitable Worlds Observatory, and the confluence of public science and the private sector. Gillian Bussey, deputy chief science officer for the U.S. Space Force, will serve as the luncheon speaker.

Panels on the third and final day, March 21, will discuss integrating multi-sector data to advance Earth and space science, the Heliophysics Decadal Survey, and the space weather enterprise. Mark Clampin, acting deputy associate administrator for the NASA Science Mission Directorate, will provide the luncheon address.

Media interested in arranging interviews with NASA speakers should contact Jacob Richmond, Goddard acting news chief.

For more information on the Goddard Space Science Symposium and the updated program, or to register as a media representative, visit https://astronautical.org/events/goddard.

For more information on NASA’s Goddard Space Flight Center, visit https://www.nasa.gov/goddard.

Media Contact:
Jacob Richmond
NASA’s Goddard Space Flight Center, Greenbelt, Md.

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Details Last Updated Mar 18, 2025 EditorJamie AdkinsLocationNASA Goddard Space Flight Center Related Terms

• Goddard Space Flight Center

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

Skylab 3 astronauts witnessed many spectacular sights during their 858 orbital trips around the Earth in the summer of 1973. One involved watching powerful Hurricane Ellen take shape off the West African coast. “There’s a nice storm down there. She looks pretty big. She’s got a lot of clouds,” said astronaut Alan L. Bean upon viewing the storm from Skylab’s low-Earth orbit.

Knowing they were witnessing something of interest to meteorologists on Earth, Bean and his fellow Skylab crew members captured stereo photographs of the storm using cameras aboard the space station. Meteorologists later used these images, which provided three-dimensional data, to help them understand how the clouds in tropical systems formed and functioned.

This image of Hurricane Ellen was taken by Skylab astronauts in September 1973. Unscheduled weather observations that relied on the judgement and actions of Skylab astronauts captured valuable research data for scientists.NASA

Like the Skylab 3 crew’s photographs of Hurricane Ellen, the lightning observations of Skylab 4 astronaut Edward G. Gibson were also used by meteorologists to understand regional weather phenomena. While gazing down at a storm over South America’s Andes Mountains, Gibson noted that the thunderstorm he observed generated recognizable lightning patterns over a 500-square-mile region.

“A few things impressed me here: one is the fact that they could go off simultaneously or near simultaneously over a large distance—sympathetic lightning bolts, if you will, analogous to sympathetic flares on the sun. And that we do get periods of calm between periods of very high activity. Some sort of collective phenomenon appears to be at work,” Gibson recalled.

This photograph of Edward G. Gibson, Skylab 4 science pilot, was taken at Kennedy Space Center, Florida on November 8, 1973, before his November 16 launch to Skylab. Meteorologists were very interested in the regional lightning patterns he witnessed while aboard the space station.NASA

The photographs of Hurricane Ellen and Gibson’s notes about lightning patterns are just two of many valuable meteorological observations and recordings astronauts made during Skylab’s three crewed missions. All told, astronaut-conducted Earth studies provided important regional, also known as mesoscale, weather data that improved storm forecasting.

Along with providing valuable data to meteorologists, the notable findings of the Skylab astronauts supported the argument of the era’s scientists and mission planners who insisted that there was no adequate replacement for intelligent human observers in space.

Perhaps the authors of Living and Working in Space: A History of Skylab  put it best when they wrote: “Man’s ability to discriminate, to select the important features of a wide vista, and to respond effectively to unexpected events constituted his greatest contribution to orbital investigations.”

Read more about how Ed Gibson's lightning observations impacted weather forecasting Read the NASA publication Skylab Explores the Earth Share

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Atomic Layer Processing Coating Techniques Enable Missions to See Further into the Ultraviolet

Astrophysics observations at ultraviolet (UV) wavelengths often probe the most dynamic aspects of the universe. However, the high energy of ultraviolet photons means that their interaction with the materials that make up an observing instrument are less efficient, resulting in low overall throughput. New approaches in the development of thin film coatings are addressing this shortcoming by engineering the coatings of instrument structures at the atomic scale.

Researchers at the NASA Jet Propulsion Laboratory (JPL) are employing atomic layer deposition (ALD) and atomic layer etching (ALE) to enable new coating technologies for instruments measuring ultraviolet light. Conventional optical coatings largely rely on physical vapor deposition (PVD) methods like evaporation, where the coating layer is formed by vaporizing the source material and then condensing it onto the intended substrate. In contrast, ALD and ALE rely on a cyclic series of self-limiting chemical reactions that result in the deposition (or removal) of material one atomic layer at a time. This self-limiting characteristic results in a coating or etchings that are conformal over arbitrary shapes with precisely controlled layer thickness determined by the number of ALD or ALE cycles performed.

The ALD and ALE techniques are common in the semiconductor industry where they are used to fabricate high-performance transistors. Their use as an optical coating method is less common, particularly at ultraviolet wavelengths where the choice of optical coating material is largely restricted to metal fluorides instead of more common metal oxides, due to the larger optical band energy of fluoride materials, which minimizes absorption losses in the coatings. Using an approach based on co-reaction with hydrogen fluoride, the team at JPL has developed a variety of fluoride-based ALD and ALE processes.

(left) The Supernova remnants and Proxies for ReIonization Testbed Experiment (SPRITE) CubeSat primary mirror inside the ALD coating facility at JPL, the mirror is 18 cm on the long and is the largest optic coated in this chamber to-date. (right) Flight optic coating inside JPL ALD chamber for Pioneers Aspera Mission. Like SPRITE, the Aspera coating combines a lithium fluoride process developed at NASA GSFC with thin ALD encapsulation of magnesium fluoride at JPL. Image Credit: NASA-JPL

In addition to these metal-fluoride materials, layers of aluminum are often used to construct structures like reflective mirrors and bandpass filters for instruments operating in the UV.  Although aluminum has high intrinsic UV reflectance, it also readily forms a surface oxide that strongly absorbs UV light. The role of the metal fluoride coating is then to protect the aluminum surface from oxidation while maintaining enough transparency to create a mirror with high reflectance.

The use of ALD in this context has initially been pursued in the development of telescope optics for two SmallSat astrophysics missions that will operate in the UV: the Supernova remnants and Proxies for ReIonization Testbed Experiment (SPRITE) CubeSat mission led by Brian Fleming at the University of Colorado Boulder, and the Aspera mission led by Carlos Vargas at the University of Arizona. The mirrors for SPRITE and Aspera have reflective coatings that utilize aluminum protected by lithium fluoride using a novel PVD processes developed at NASA Goddard Space Flight Center, and an additional very thin top coating of magnesium fluoride deposited via ALD.

Team member John Hennessy prepares to load a sample wafer in the ALD coating chamber at JPL. Image Credit: NASA JPL

The use of lithium fluoride enables SPRITE and Aspera to “see” further into the UV than other missions like NASA’s Hubble Space Telescope, which uses only magnesium fluoride to protect its aluminum mirror surfaces. However, a drawback of lithium fluoride is its sensitivity to moisture, which in some cases can cause the performance of these mirror coatings to degrade on the ground prior to launch. To circumvent this issue, very thin layers (~1.5 nanometers) of magnesium fluoride were deposited by ALD on top of the lithium fluoride on the SPRITE and Aspera mirrors. The magnesium fluoride layers are thin enough to not strongly impact the performance of the mirror at the shortest wavelengths, but thick enough to enhance the stability against humidity during ground phases of the missions. Similar approaches are being considered for the mirror coatings of the future NASA flagship Habitable Worlds Observatory (HWO).

Multilayer structures of aluminum and metal fluorides can also function as bandpass filters (filters that allow only signals within a selected range of wavelengths to pass through to be recorded) in the UV. Here, ALD is an attractive option due to the inherent repeatability and precise thickness control of the process. There is currently no suitable ALD process to deposit aluminum, and so additional work by the JPL team has explored the development of a custom vacuum coating chamber that combines the PVD aluminum and ALD fluoride processes described above. This system has been used to develop UV bandpass filters that can be deposited directly onto imaging sensors like silicon (Si) CCDs. These coatings can enable such sensors to operate with high UV efficiency, but low sensitivity to longer wavelength visible photons that would otherwise add background noise to the UV observations.

Structures composed of multilayer aluminum and metal fluoride coatings have recently been delivered as part of a UV camera to the Star-Planet Activity Research CubeSat (SPARCS) mission led by Evgenya Shkolnik at Arizona State University. The JPL-developed camera incorporates a delta-doped Si CCD with the ALD/PVD filter coating on the far ultraviolet channel, yielding a sensor with high efficiency in a band centered near 160 nm with low response to out-of-band light.

A prototype of a back-illuminated CCD incorporating a multi-layer metal-dielectric bandpass filter coating deposited by a combination of thermal evaporation and ALD. This coating combined with JPL back surface passivation approaches enable the Si CCD to operate with high UV efficiency while rejecting longer wavelength light. Image credit: NASA JPL

Next, the JPL team that developed these coating processes plans to focus on implementing a similar bandpass filter on an array of larger-format Si Complementary Metal-Oxide-Semiconductor (CMOS) sensors for the recently selected NASA Medium-Class Explorer (MIDEX) UltraViolet EXplorer (UVEX) mission led by Fiona Harrison at the California Institute of Technology, which is targeted to launch in the early 2030s. 

For additional details, see the entry for this project on NASA TechPort

Project Lead: Dr. John Hennessy, Jet Propulsion Laboratory (JPL)

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Depending on where you stand at the lunar South Pole, you may experience temperatures of 130°F (54°C) during sunlit periods, or as low as -334°F (-203°C) in a permanently shadowed region. Keeping crews comfortable and tools and vehicles operational in such extreme temperatures is a key challenge for engineers at Johnson Space Center working on elements of NASA’s Artemis campaign.

Abigail Howard is part of that innovative team. Since joining Johnson in 2019, she has conducted thermal analysis for projects including the lunar terrain vehicle (LTV), pressurized rover, VIPER (Volatiles Investigating Polar Exploration Rover), and Gateway – humanity’s first lunar space station. Her work explores how different materials and components respond to different temperatures and how to manage heat transfer in products and structures.

She currently serves as the passive thermal system manager for the Extravehicular Activity and Human Surface Mobility Program, leading a small team of thermal analysts. Together, they provide expertise on passive thermal design, hardware, modeling, and testing to vendors and international partners that are developing rovers and tools for human exploration of the lunar surface.

Abigail Howard posing in front of a mockup of VIPER (Volatiles Investigating Polar Exploration Rover), which she worked on as a thermal analyst for three years. Image courtesy of Abigail Howard

Howard said her sudden shift from thermal analysis engineer to thermal system manager involved a steep learning curve. “Every day was like drinking through a firehose. I had to learn very quickly about systems engineering tasks, project phases, and leadership, while also learning about many new thermal approaches and designs so that I could provide good insight to project leadership and program vendors and partners,” she said. “Having a good group of senior engineers and friends to lean on and building up my team helped me get through it, but the single most important thing was not giving up. It gets easier and persistence pays off!”

Abigail Howard (left) and Brittany Spivey (right) after presenting their poster at the 2022 International Symposium for Materials in the Space Environment in Leiden, the Netherlands. Image courtesy of Abigail Howard

Howard feels fortunate to have worked on many interesting projects at NASA and presented her work at several conferences. Top achievements include watching her first NASA project launch successfully on Artemis I and supporting the LTV Source Evaluation Board as the thermal representative. “Something I’m really proud of is obtaining funding for and managing a test that looked at thermal performance of dust mitigation for spacecraft radiators,” she added.

Abigail Howard removes lunar dust simulant from a tray holding radiator test coupons during a test to evaluate thermal performance of radiators with integrated Electrodynamic Dust Shield for dust mitigation. Image courtesy of Abigail Howard

She believes interesting and challenging work is important but says the biggest determinant to professional success and satisfaction is your team and your team lead. “Having a really great team and team lead on Gateway thermal taught me the kind of leader and teammate I want to be,” she said.

Howard encourages fellow members of the Artemis Generation to not let imposter syndrome get in their way. “Focus on the evidence of your abilities and remember that no one is in this alone,” she said. “It’s okay to ask for help.”

Many spiral galaxies have bars across their centers.

NASA’s Office of STEM Engagement at Johnson Space Center offers Texas high school students a unique gateway to the world of space exploration through the High School Aerospace Scholars (HAS) program. This initiative gives juniors hands-on experience, working on projects that range from designing spacecraft to planning Mars missions. 

Nearly 30 participants who have been hired by NASA in the past five years are HAS alumni. Their stories highlight the program’s impact on students—inspiring innovation, fostering collaboration, unlocking their potential as they move forward into STEM careers. 

Discover how the HAS experience has shaped these former students’ space exploration journey.  

Jaylon Collins: Designing the Future of Spaceflight 

Jaylon Collins always knew he wanted to study the universe but HAS shifted his perspective on what a STEM career could be. 

“HAS brought a newfound perspective on what my STEM career could look like, and that shift led me to where I am today,” Collins said. “The coursework, NASA-led seminars, and space exploration research showed me that I could do direct design work to aid humanity’s exploration of the cosmos. I didn’t want to only learn about our universe—I wanted to help explore it.” 

Jaylon Collins with his parents at the University of Texas at Austin after being accepted as a student class of 2028.

“HAS showed me that a career in STEM doesn’t require a label, only your passion,” Collins said. “I saw that STEM could lead to endless career paths, and the guide was whatever I was most passionate about.” 

He saw firsthand how engineers tackle the challenges of spaceflight, from designing spacecraft to solving complex mission scenarios. His strong performance in the program earned him an invitation to Moonshot, a five-day virtual challenge where NASA scientists and engineers mentor students through an Artemis-themed mission. His team developed a Mars sample return mission, an experience that taught him valuable lessons in teamwork. 

“We combined our knowledge to design solutions that fit our mission profile, and I learned how problem-solving goes beyond the obvious tools like math and science,” he said. “Instead, it entails finding unique methods that trade off certain elements to bolster others and finding the optimal solution for our problem. HAS taught me to listen more than talk and take constructive feedback to create a solid plan.”

Now studying aerospace engineering at the University of Texas at Austin, Collins credits HAS with building his professional network and opening doors to NASA internship opportunities. 

“I learned so much from seminars, my peers, and my Moonshot mentors about not only my academic future but also my prospective career,” he said. “My HAS experience has granted me a web of internship opportunities at NASA through the Gateway Program, and I hope that I can leverage it soon in L’Space Academy’s Lucy Internship.” 

Jaylon Collins at Johnson Space Center with the 2024 astronaut graduate class. 

Collins hopes to contribute to NASA’s mission by developing solutions for deep space travel. Beyond that, he wants to inspire the next generation. 

“I believe that the goal of universal knowledge is to reverberate the passions I have onto other curious dreamers,” he said. “Having mentors who teach the curious is the way we progress and innovate as a society, and I am dedicated to being one of those mentors one day.” 

Erin Shimoda: Guiding Astronauts to Safety 

Erin Shimoda’s path to becoming an aerospace engineer did not start with a clear vision of her future. Growing up in a family full of engineers and scientists, she was already on the STEM path, but she did not know where to focus. HAS changed that. 

“HAS exposed me to so many different things that an aerospace engineer does,” she said. “I learned about the history of humans in space, NASA’s missions, how to design 3D models, how to apply equations from math class to real-life scenarios.” 

During the program’s summer experience, she and her team designed a mission to send humans to Mars. She credits the program with inspiring her to earn an aerospace engineering degree. 

Official portrait of Erin Shimoda. NASA/Josh Valcarcel

The HAS program also reshaped her understanding of what a STEM career could look like. “My mentors were incredible. They talked about their projects with such energy and passion. It made me want to feel that way about my own work,” she said. “I didn’t realize before how exciting and innovative working in STEM could be.” 

Shimoda said every person she met through HAS was inspiring. “Just knowing that those people existed and worked at NASA helped push me to persevere and succeed in my undergraduate career. I had plenty of bumps in the road, but I had a goal in mind that others had achieved before me, so I knew I could, too.” 

One of the biggest lessons she took from the program was the power of collaboration. In high school, she often felt like she was carrying the load on group projects, which left her with a negative view of working on a team. HAS changed that perspective. 

“During HAS, everyone was very passionate about accomplishing our goal, so I was consistently supported by my peers,” she said. “That’s so true at NASA, too. Not one single person can build an entire mission to the Moon. We’re all so passionate about accomplishing the mission, so we always support each other and strive for excellence.”

Shimoda also saw firsthand how diverse perspectives lead to better results. “There are many ways to come to a solution, and not every solution is right,” she said. “Collaboration leads to innovation and better problem-solving.” 

Erin Shimoda stands in front of a presentation on the Launch Abort System for NASA’s Orion spacecraft and Space Launch System rocket.NASA/Robert Markowitz

Now, Shimoda plays a key role in NASA’s Orion Program, ensuring astronaut safety through comprehensive ascent abort planning and procedures, and supporting Artemis recovery operations. She works on guidance, navigation, and control, predicting where the crew module and recovery hardware will land so teams—including the U.S. Navy—are in the right place at the right time. 

“It’s exciting because we get to go ‘in the field’ on a U.S. Navy ship during training. Last year, I spent a week on a Navy ship, and seeing everything come together was incredible,” she said. 

Her advice for students exploring STEM? “Try every opportunity possible! I joined almost every club imaginable. When I saw the HAS poster in front of my high school’s library, I thought to myself, ‘Well, I’m not in anything space-related yet!’ and the rest is history.” 

Looking ahead, she is eager for what is to come. “I’m especially excited for Artemis III, where I’ll be directly involved in recovery operations,” Shimoda said. “I hope that all this work propels us to a future with a sustained human presence on the Moon.” 

Hallel Chery: Aspiring Astronaut and Emerging Leader 

Hallel Chery is a high school senior who will pursue a degree in mechanical engineering and materials science at Harvard College, with her sights set on becoming both an engineer and an astronaut.  

She completed all three stages of HAS: the online course, the virtual Moonshot challenge, and the five-day on-site experience at Johnson. Balancing the program with academics and leading a school-wide tutoring club pushed her limits—but also broadened her confidence. 

“I learned that I could take on a tremendous amount of work at one time,” she said. “This realization has helped me become more ambitious in my future plans.” 

A portrait of Hallel Chery during her time in the High School Aerospace Scholars program.

Moonshot was her proving ground. Tasked with redesigning a module for NASA’s future Gateway lunar space station, she led a team of eight HAS scholars—none of whom she had met before—through an intense, weeklong mission. Their work was presented to NASA scientists and engineers and her group landed among the top teams in the challenge. 

“The experience strengthened my confidence in my abilities as a leader,” said Chery. “I learned that I thrive under pressure and am well prepared to tackle any challenge, technical or interpersonal, no matter how difficult it is.” 

“Moonshot exposed me for the first time to true, deep teamwork,” she said. “Interacting almost non-stop with the same people over one week in a high stakes situation truly taught me about the dynamics of how teams work, the value of teamwork, and being an effective leader. This, coupled with the program’s emphasis on the importance of teamwork have firmly ingrained in me the essentiality of this core NASA value.”  

While at Johnson, Chery toured the Space Vehicle Mockup Facility, watched astronauts suit up at the Neutral Buoyancy Laboratory, and visited the Mission Control Center. “Spending only a few days at Johnson, I can truly say that as an aspiring astronaut, being there felt just like home,” Chery said.  

Hallel Chery in a spacesuit mockup at Johnson Space Center.

“Because of HAS, I directly visualize myself working in a team to solve the problems I wanted to tackle instead of primarily focusing on the individual accomplishments that will solve them,” she said. “The program taught me how essential teamwork is to effective problem solving and innovation.” 

 The advice she has for the next generation is to keep exploring and to answer the question: What do you want to contribute for the good of the world? 

HAS also introduced her to professional networking early in her academic career. Engaging with NASA professionals provided insight into the agency’s work culture and internship opportunities. 

Now, as she prepares for her future in mechanical engineering and materials science, Chery is determined to apply what she has learned. 

She is particularly grateful for the mentorship of NASA consultant Gotthard Janson, who provided encouragement and guidance throughout the HAS journey.  

“The opportunity to connect with great professionals like him has provided additional wisdom and support as I grow through my academic and professional career,” she said.  

Looking ahead, Chery aims to design space habitats, create innovative exercise solutions, and develop advanced materials for use in space.  

“I want to help propel humanity forward—on Earth, to the Moon, Mars, and beyond—while inspiring others in the Artemis Generation,” she said. “Building and launching my rocket at Johnson felt like launching my future—one dedicated to contributing to NASA and humanity.” 

Johnson Space Center will showcase its achievements at the Texas Capitol for Space Day Texas on Tuesday, March 25. The High School Aerospace Scholars program will have a booth, and NASA will have interactive exhibits highlighting the programs and technologies that will help humanity push forward to the Moon and Mars.

Learn more about NASA’s involvement here.

LOCATION: Texas State Capitol – Austin, Texas SUBJECT: Space Day activities at the Texas State Capitol in Austin, Texas PHOTOGRAPHER: Lauren HarnettNASA

March 17, 2025

NASA is heading back to the state capitol in March for Space Day Texas, a recognition of achievements throughout Texas and a look ahead to the impact future human space exploration has on the Lone Star state.

The two-day schedule of events and exhibits focusing on exploration, astronauts, and science, technology, engineering, and math education will include astronaut visits, interactive exhibits, and legislative proclamations.

NASA’s Johnson Space Center in Houston will share its accomplishments on the Capitol grounds from 9 a.m. to 4 p.m. CDT Tuesday, March 25, joining academic and commercial partners from across the state to share Texas’ blueprint for expanding humanity’s frontier in space.

On Monday, March 24, exhibits will feature the Texas High School Aerospace Scholars program at the University of Texas Elementary Charter school, along with NASA Johnson’s Office of STEM Engagement, Orion program, and Lockheed Martin. Interactive events will feature NASA STEM engagement programs and hands-on exhibits.

At 10 a.m. Tuesday, March 25, proclamations celebrating NASA’s 25th anniversary of continuous human presence on the International Space Station, the High School Aerospace Scholars program, and the continued progression of the Artemis campaign through NASA’s commercialization of cargo, crew, landers, spacesuits, and rovers will be read in the Texas House and Senate chambers, respectively. Following the proclamations, an Artemis II crew astronaut will participate in a live question and answer session on the front steps of the Capitol.

NASA’s impact in Texas is strong. NASA Johnson has served as the iconic site for some of the greatest moments in American history, from landing humans on the Moon to assembling the International Space Station.

For more than 60 years, NASA has led the world in human space exploration. Today, it is testing technologies on the Space Station that will help humanity push forward to the Moon and Mars. NASA’s workforce in Texas includes more than 10,000 aerospace employees and more than $2 billion in contracts and federal salaries in 2024.

Learn more about NASA Johnson and its impact in Texas at:

https://www.nasa.gov/johnson

-end-

Kelly Humphries

Johnson Space Center, Houston

281-483-5111

kelly.o.humphries@nasa.gov

Students, mentors, and team supporters donning team colors watch robots clash on the playing field at the FIRST Robotics Los Angeles regional competition in El Segundo on March 16. NASA/JPL-Caltech

Robots built by high schoolers vied for points in a fast-moving game inspired by complex ocean ecosystems at the FIRST Robotics Los Angeles regional competition.

High school students who spent weeks designing, assembling, and testing 125-pound rolling robots put their fast-moving creations into the ring over the weekend, facing off at the annual Los Angeles regional FIRST Robotics Competition, an event supported by NASA’s Jet Propulsion Laboratory in Southern California.

Four of the 43 participating teams earned a chance to compete in April at the FIRST international championship tournament in Houston, which draws winning teams from across the country.

Held March 14 to 16 at the Da Vinci Schools campus in El Segundo, the event is one of many supported by the nonprofit FIRST (For Inspiration and Recognition of Science and Technology), which pairs students with STEM professionals. Teams receive the game rules, which change every year, in January and sprint toward competition, assembling their robot based on FIRST’s specifications. The global competition not only gives students engineering experience but also helps them develop business skills with a range of activities, from fundraising for their team to marketing.

For this year’s game, called “Reefscape,” two alliances of three teams competed for points during each 2½-minute match. That meant six robots at a time sped across the floor, knocking into each other and angling to seed “coral” (pieces of PVC pipe) on “reefs” and harvesting “algae” (rubber balls). In the final seconds of each round, teams could earn extra points if their robots were able to hoist themselves into the air and dangle from hanging cages, as though they were ascending to the ocean surface.

The action was set to a bouncy soundtrack that reverberated through the gym, while in the bleachers there were choreographed dancing, loud cheers, pom-poms, and even some tears.

The winning alliance was composed of Warbots from Downey’s Warren High School, TorBots from Torrance’s South High School, and West Torrance Robotics from Torrance’s West High School. The Robo-Nerds of Benjamin Franklin High in Los Angeles’ Highland Park and Robo’Lyon from Notre Dame de Bellegarde outside Lyon, France, won awards that mean they’ll also get to compete in Houston, alongside the Warbots and the TorBots.

NASA and its Robotics Alliance Project provide grants for high school teams across the country and support FIRST Robotics competitions to encourage students to pursue STEM careers in aerospace. For the L.A. regional competition, JPL has coordinated volunteers — and provided coaching and mentoring to teams, judges, and other competition support — for 25 years.

For more information about the FIRST Los Angeles regional, visit:

https://cafirst.org/frc/losangeles/

News Media Contact

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

2025-037

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Details Last Updated Mar 17, 2025 Related Terms

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A SpaceX Falcon 9 rocket carrying the company's Dragon spacecraft is launched on NASA’s SpaceX Crew-10 mission to the International Space Station with NASA astronauts Anne McClain and Nichole Ayers, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov onboard, Friday, March 14, 2025, from NASA's Kennedy Space Center in Florida. NASA’s SpaceX Crew-10 mission is the tenth crew rotation mission of the SpaceX Dragon spacecraft and Falcon 9 rocket to the International Space Station as part of the agency’s Commercial Crew Program. McClain, Ayers, Onishi, and Peskov launched at 7:03 p.m. EDT from Launch Complex 39A at NASA Kennedy to begin a six-month mission aboard the orbital outpost.