Saturday, 21 March 2026

NASA Selects University Finalists for Technology Concepts Competition

Banner image for the 2026 RASC-AL Competition with a space/moon background and an astronaut showing a reflection of Mars in the visor. The RASC-AL wordmark is included, and text reads ‘2026 RASC-AL / Revolutionary Aerospace Systems Concepts – Academic Linkage.
Image Credit: National Institute of Aerospace

NASA selected 14 university teams from across the nation as finalists in the 2026 Revolutionary Aerospace Systems Concepts – Academic Linkage (RASC-AL) Competition. This NASA challenge tasks students to design innovative concepts that could further human life and work on the Moon, Mars, and beyond. The competition links academia and the aerospace community, fostering innovation, collaboration, and workforce development in support of NASA’s long-term exploration goals.

“The innovation and technical depth demonstrated this year are exemplary of the next generation of aerospace leaders,” said Daniel Mazanek, RASC-AL program sponsor and senior space systems engineer from NASA’s Langley Research Center in Hampton, Virginia. “The strongest teams demonstrated not only creativity, but also the disciplined analysis and systems engineering required to develop credible solutions for space exploration challenges facing the agency.”

The 2026 RASC-AL competition invited university teams to develop technically rigorous proposals addressing one of four mission themes: Communications, Position, Navigation, and Time (CPNT) Architectures for Mars Surface Operations; Lunar Surface Power and Power Management and Distribution (PMAD) Architectures; Lunar Sample Return Concepts; and Lunar Technology Demonstrations Leveraging Common Infrastructure. Each topic reflects relevant areas of exploration technology development aligned with NASA’s Artemis program and long-term human missions to Mars.

The 2026 RASC-AL Finalists are:

CPNT Architectures for Mars Surface Operations

  • Massachusetts Institute of Technology
    MELIORA: Mars Exploration Layered Infrastructure for Operations, Research, and Advancement
  • University of Texas, Austin
    Project Pharos
  • Virginia Polytechnic Institute and State University
    The Mars Pylon Network (MPN)

Lunar Surface Power and Power Management and PMAD Architectures

  • Dartmouth College
    FLORA: Flywheel for Lunar Operations – Redundancy Architecture
  • Embry-Riddle Aeronautical University, Daytona Beach
    Project AUREVO: Advanced Utilization of Resources for Energy & Viability Off-Earth
  • Massachusetts Institute of Technology
    Exploration-Class Lunar Integrated Power SystEm (ECLIPSE)
  • University of Hawaii, Manoa with University of Hawaii, Hilo
    Project PETAL: Power Energy Transfer Architecture for the Lunar surface

Lunar Sample Return Concept

  • South Dakota State University
    SELENE: Sample Extraction of Lunar Elements for Network Entry
  • Texas A&M University
    TAMU NOVA Lunar Mission
  • University of Michigan
    LASSO – Lunar Autonomous Sample Staging Operations

Lunar Technology Demonstrations Leveraging Common Infrastructure

  • Massachusetts Institute of Technology
    CHEESEBURGER: CLPS-enabled Highly-autonomous End-to-End isru-System Evaluations to Build Understanding and Resilient Growth by Experimenting with Regolith
  • University of Illinois, Urbana-Champaign with Ecole Supérieure d’Ingénieurs Léonard de Vinci
    MATRIX: Mining and Advanced Transformation of Regolith for Infrastructure and eXpansion
  • University of Maryland
    Project LILI: Lunar Infrastructure & Landing Innovation
  • University of Texas, Austin
    Demonstration of Up-scalable Surface Treatment for Earth-Moon Economy (DUSTEE)

Each team submitted an initial proposal paper and a two-minute video presentation, which were evaluated by a review panel of NASA and aerospace industry experts.

“The RASC-AL competition challenges students to address many of the same technical and operational questions we encounter working on Artemis, from surface infrastructure to mobility and resource utilization,” added Dr. Christopher Jones, RASC-AL program sponsor and chief technologist for the Systems Analysis and Concepts Directorate at NASA Langley.  “The concepts developed through the competition help expand NASA’s thinking as we plan and refine future exploration missions.”

As finalists, each team will further develop their concept into a comprehensive technical paper and oral presentation, culminating in an in-person showcase beginning on June 2 at the 2026 RASC-AL Forum in Cocoa Beach, Florida. During the Forum, students will present their work to NASA leaders, industry professionals, and fellow finalist teams, gaining valuable feedback and professional experience in systems-level mission design. The top-performing teams at the forum will be recognized for technical merit, innovation, and presentation excellence.

NASA’s RASC-AL Competition is administered by the National Institute of Aerospace. The RASC-AL Competition is sponsored by NASA’s Strategy and Architecture Office within the Exploration Systems Development Mission Directorate, by NASA’s Space Technology Mission Directorate, and by the Systems Analysis and Concepts Directorate at NASA Langley. The NASA Tournament Lab, part of the Prizes, Challenges, and Crowdsourcing Program in the Space Technology Mission Directorate, manages the challenge.

For more information about RASC-AL, visit RASCAL.nianet.org.



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Smiles and Spacesuits

Chris Williams, an astronaut, is wearing a white spacesuit and helmet. He is facing the camera, but his body is turned to the right of the image. His arms are extended in front of him.
NASA/Zena Cardman

NASA astronaut Chris Williams smiles at the camera during a spacesuit fit verification on Jan. 2, 2026, inside the International Space Station’s Quest airlock. This procedure confirms that the spacesuit is airtight and properly configured, assesses comfort and mobility, and helps prevent potential safety risks.

Williams and fellow NASA astronaut Jessica Meir completed an approximately seven-hour and two-minute spacewalk on March 18, 2026. The pair did tasks that will enable the future installation of roll-out solar arrays. These arrays will provide additional power for the orbiting laboratory, supporting critical systems and its safe, controlled deorbit.

Learn more about station activities on the International Space Station blog.

Image credit: NASA/Zena Cardman



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Friday, 20 March 2026

NASA Exploration, Science Inspire “Project Hail Mary” Film

At right, a man in a blue flight suit with patches on it takes a selfie with his cell phone. He is in the photo, as well as panel members and the large audience. They are in an auditorium. In the far background, there is a NASA "meatball" insignia and the letters "JPL" on the wall.
NASA astronaut Kjell Lindgren takes a selfie with the people behind “Project Hail Mary” and the audience during a panel about the movie at NASA’s Jet Propulsion Laboratory on Feb. 25, 2026.
NASA/Dan Goods

Real-life space exploration and big-screen science fiction will converge on Friday. As NASA prepares to launch Artemis II, the first crewed mission under the agency’s Artemis program and another step toward sending the first astronauts – Americans – to Mars, the fictional film “Project Hail Mary” premiere will take audiences on a journey into deep space.

The agency provided guidance throughout filming, and also is participating in activities related to the release of the film to connect the agency’s missions, innovations, and discoveries to the public through pop culture.

“Space exploration captures the public’s imagination, and collaboration between science and storytelling brings that sense of discovery to a wider audience,” said Will Boyington, associate administrator for the Office of Communications at NASA Headquarters in Washington. “Inspiring the next generation, whether through rocket launches or sci-fi movies, helps build the talent and support that underpin American leadership in space.”

NASA’s communications personnel provided informal consultation about human spaceflight and science during the making of the movie, and experts from the agency in astrobiology and astrophysics, which are major themes in “Project Hail Mary,” answered questions about these topics during the making of the film. Agency advisors are listed in the credits.

On the movie set, the agency provided an in-person consultation between NASA astronaut Kjell Lindgren and actor Ryan Gosling, who plays an astronaut in the movie. NASA also facilitated brand use guidance and clearance for the agency’s “meatball” and “worm” logos featured in the film. 

NASA’s activities related to the movie even reached beyond Earth. In between conducting research and demonstrating new technologies, Expedition 74 crew members living and working aboard the International Space Station, including NASA astronauts Chris Williams, Jessica Meir, and Jack Hathaway, screened “Project Hail Mary” while in orbit.

Artemis II crew members, NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen, who will help make what once was science fiction a reality through their upcoming deep space launch, are expected to have an opportunity to view “Project Hail Mary” while in quarantine. They are preparing to explore more of the Moon for scientific discovery, economic benefits, and to build on our foundation for the first crewed missions to Mars.

Learn more about the agency’s missions on NASA’s website:

https://www.nasa.gov

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Mar 20, 2026
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NASA Simulations Improve Artemis II Launch Environment

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NASA Simulations Improve Artemis II Launch Environment

This simulation of the Artemis I launch shows how the Space Launch System rocket’s exhaust plumes interact with the air, water, and the launchpad. Colors on surfaces indicate pressure levels—red for high pressure and blue for low pressure. The teal contours illustrate where water is present.
Credits: NASA/Chris DeGrendele, Timothy Sandstrom

Airflow around rockets as they travel from Earth into space can have a dramatic impact on a mission, which is why NASA used advanced simulations to provide the best possible launch conditions for the Artemis II test flight around the Moon. 

To better understand the Artemis Space Launch System (SLS) rocket’s flight environment, engineers turned to a NASA-developed tool called the Launch, Ascent, and Vehicle Aerodynamics (LAVA) framework. The software addresses computational fluid dynamics, the flow behavior of gases and liquids. 

Using data from the 2022 Artemis I launch, researchers at NASA’s Ames Research Center in California’s Silicon Valley used LAVA to simulate complex interactions between the rocket plume and a system that pumps water to suppress sound during launch. The system protects the rocket and other equipment from potentially damaging sound waves. 

Comparing simulations with and without the sound suppression system activated revealed that the water effectively reduces pressure waves from sound, but exhaust gases from the rocket could also redirect water, causing significant pressure increases in certain areas of the launchpad.   

The LAVA simulations improved NASA’s understanding of the plume interaction with the Artemis mobile launcher platform. Using this knowledge, aerospace engineers at NASA’s Kennedy Space Center in Florida refined the design plume pressures and adapted the launch platform to endure those pressures for Artemis II, NASA’s first mission with crew aboard the SLS and Orion spacecraft. 

NASA will release LAVA in the coming weeks to the aerospace community and accelerate innovation by enabling U.S. companies and researchers to run complex simulations and optimize designs for aircraft and rockets. NASA has hosted a seminar on using LAVA with more about the tool’s capabilities. 

The work on LAVA is supported through NASA’s Transformational Tools and Technologies project, which develops new computational capabilities to help predict aerospace vehicle performance. The project is part of NASA’s Transformative Aeronautics Concepts Program under the Aeronautics Research Mission Directorate.  

NASA’s decades of aeronautics research expertise strengthens its space missions, using tools like wind tunnel testing, advanced software development, and other innovations to enhance safety and reliability. 

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NASA Glenn Opens Applications for Free Summer Engineering Institute

Three High School Engineering Institute students are centered in the foreground of the image working on a small vehicle with large red plastic wheels. There are two more students in the background working on their own identical vehicle.
Students collaborate on a hands‑on STEM project, assembling and testing components during the NASA Glenn High School Engineering Institute at NASA’s Glenn Research Center on July 18, 2025.
NASA/Sara Lowthian-Hanna

NASA’s Glenn Research Center in Cleveland is hosting the 2026 NASA Glenn High School Engineering Institute this July. The hands-on learning experience is designed to help high school students prepare for a future in the aerospace workforce.  

Rising high school juniors and seniors can submit applications for this summer program beginning Friday, March 20, through Friday, May 1. 

The institute will immerse students in NASA’s work while providing essential career readiness tools to help them in future science, technology, engineering, and math-focused academic and professional pursuits.  

Throughout the five-day program, students will use authentic NASA mission content and work alongside Glenn’s technical experts to gain a deeper understanding of the engineering design process, develop practical engineering solutions to real-world challenges, and test prototypes to answer questions in key mission areas: 

  • Acoustic dampening – How can we reduce noise pollution from jet engines? 
  • Power management and distribution – How can we develop a smart power system for future space stations? 
  • Simulated lunar operations – Can we invent tires that don’t use air? 

How to Apply: 
To be considered for the 2026 NASA Glenn High School Engineering Institute, applicants must submit a complete application package no later than May 1, 2026, at 11:59 p.m. ET. 

Program Dates 
Selected students will participate in one of the following weeklong sessions:

  • Session 1: July 13-17, 2026 
  • Session 2: July 20-24, 2026 
  • Session 3: July 27-31, 2026 

Eligibility and Application Requirements 
To be eligible for this program, students must:  

  • Be entering 11th or 12th grade for the 2026-2027 academic year
  • Have a minimum 3.2 GPA, verified by their school counselor 
  • Submit a letter of recommendation from a teacher 
  • Be a U.S. citizen

Questions about the institute should be directed to GRC-Ed-Opportunities@mail.nasa.gov.  

For information about NASA Glenn, visit:  

https://www.nasa.gov/glenn

-end- 

Heather Roe 
NASA Glenn Research Center, Cleveland
216-695-7292
heather.m.roe@nasa.gov



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Restless Kīlauea Launches Lava and Ash

The heat signature from an eruption at Kilauea glows yellow and orange in the volcano’s summit crater.
March 10, 2026

Kīlauea has entered its second year of episodic activity after reawakening in December 2024. Since then, the Hawaiian volcano has gone through dozens of bouts of lava fountaining, each lasting several hours to several days.

Activity ramped up once again on March 10, 2026, for episode 43 of the eruption. From approximately 9 a.m. to 6 p.m. local time that day, lava spewed from two active vents on the southwest side of Halema‘uma‘u Crater, adding to the ever-thickening layer of fresh basaltic rock in the summit caldera. The flareup also featured the highest lava fountains of the current eruption, estimated at 1,770 feet (540 meters). Meanwhile, ash and other airborne debris fell on communities up to 50 miles (80 kilometers) away.

About 4 hours after fountaining subsided, the Landsat 9 satellite passed over the Island of Hawai‘i. This image shows shortwave infrared and near-infrared data, acquired with the satellite’s OLI (Operational Land Imager) at 10:20 p.m. local time on March 10 (08:20 Universal Time on March 11), revealing heat emanating from the still-sizzling lava. That information is layered over a composite of daytime Landsat images and a digital elevation model.

An estimated 16 million cubic yards (12 million cubic meters) of lava erupted during the episode, according to the Hawaiian Volcano Observatory (HVO), bringing the total volume erupted across all episodes since December 2024 to close to 325 million cubic yards (250 million cubic meters). Over the same period, the depth of lava in the crater has increased by about 300 feet (90 meters).

While lava remained confined to the summit area, other erupted material traveled much farther. Images captured by satellites orbiting over the area during the daytime showed a volcanic plume drifting northeast from the vents. Volcanic gas and ash reached a maximum height in the atmosphere of more than 30,000 feet (9,100 meters) above sea level, the HVO said. The aviation color code was elevated to red during the eruption, and several flights at the airport in Hilo were canceled, according to news reports.

Volcanic fragments up to several inches in diameter fell along the north rim of the caldera and in adjacent communities. The hazards and accumulation of debris caused the temporary closure of Highway 11 and the evacuation of visitors from parts of Hawaiʻi Volcanoes National Park. Smaller particles were carried farther: people reported ash and Pele’s hair falling tens of miles to the north and east of Kīlauea, including in Hilo, Keaʻau, and other communities on the coast. Volcanic debris is an eye, skin, and respiratory irritant, the HVO warned, and it may affect water quality for those using rainwater catchment systems.

NASA Earth Observatory image by Michala Garrison, using Landsat data from the U.S. Geological Survey. Story by Lindsey Doermann.

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The heat signature from an eruption at Kilauea glows yellow and orange in the volcano’s summit crater.

March 10, 2026

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Thursday, 19 March 2026

NASA’s Roman Observatory Passes Final Major Prelaunch Tests

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

NASA’s Nancy Grace Roman Space Telescope team recently blasted the observatory with extreme sound, shook it, and listened to its electronic hum. Roman passed all three assessments, which aimed to confirm that the observatory will withstand launch conditions and function as expected in space. The achievement keeps the mission on track for launch as early as this fall.

“All of the testing went smoothly and progress is well ahead of schedule,” said Jack Marshall, the Roman observatory integration and testing lead at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “The team has done a great job putting the observatory together, and the tests show that everything is lining up with expectations.”

Many people in white gowns observe as the Roman observatory is pushed through an enormous doorway. The observatory is surrounded by a protective clear "tent."
Technicians move NASA’s Nancy Grace Roman Space Telescope into an acoustics chamber for environmental testing at the agency’s Goddard Space Flight Center.
NASA/Jolearra Tshiteya
Many people in head-to-toe white suits surround the Roman observatory, which is on a small white platform and surrounded in a clear protective "tent."
Technicians place the Roman observatory on an air barge to safely move it between testing facilities.
NASA/Sydney Rohde (Rocz)
The Roman observatory, surrounded in a clear protective "tent," lowers onto a testing platform.
The Roman observatory moves onto a shaker table for vibration testing.
NASA/Jolearra Tshiteya
A woman in a white hard hat aims a camera up at a raised platform, onto which the Roman observatory is being lowered. Several people in hard hats surround the observatory to facilitate the process.
Technicians prepare for Roman’s vibration test to begin.
NASA/Jolearra Tshiteya
A creative style photo capturing movement of people in white gowns. Their appearances are blurred and look almost spectral. Behind them through an open doorway, the Roman observatory sits in a tall room. The observatory is encased in a clear protective structure.
Technicians move the Roman observatory into the acoustics chamber.
NASA/Jolearra Tshiteya

In January, the team set up an absorbent panel around the observatory for an electromagnetic interference test. This special configuration is designed to block external radio signals and absorb reflections inside the test facility.

Engineers powered on all of Roman’s electronics and measured the signals they generated, closely monitoring for any errors. Too much electrical noise could interfere with the observatory’s ability to detect faint infrared signals, but Roman passed with flying colors.

The team moved on to vibration testing in February. “Each time the observatory traveled between test facilities, it was placed in a custom-made portable clean room to protect it from contamination that could otherwise compromise scientific performance once in space,” said Joel Proebstle, a mechanical systems engineer who led the vibration and acoustic tests at NASA Goddard.

Engineers tested the observatory on a large shaker table to simulate the vibrations it will experience during launch, gradually building to higher frequencies. “Try to imagine sitting on that rocket and feeling all those vibrations,” said Cory Powell, the Roman structural analyst lead at NASA Goddard. “We simulated the shaking that the launch vehicle will produce to ensure the components and connections will all remain intact.”

In early March, the team conducted an acoustic test. The test took place in a state-of-the-art sound booth, where engineers ramped up the volume to 138 decibels — about as loud as a jet engine from 100 feet away.

“If you’ve ever been at a concert with an extremely loud bass, that load you felt was acoustic energy,” Powell said. “Now think about how loud a launch is. The acoustics can produce very high loads on a large structure like Roman.”

This video showcases some of NASA’s Nancy Grace Roman Space Telescope team’s major accomplishments during the second half of 2025, culminating in the completion of the observatory.
NASA’s Goddard Space Flight Center

Roman has now returned to the large clean room at Goddard where it will undergo a final series of smaller tests. The next one aims to replicate the shock Roman will experience shortly after launch when the observatory separates from the rocket. Then the team will deploy all of the elements that will initially be stowed (including the solar panels, “visor,” antenna, and “sunblock” shield), to verify that they’ll still work correctly even after launch and rocket separation.

Early this summer, the observatory will be transported to NASA’s Kennedy Space Center in Florida for launch preparations. There, engineers will verify that the observatory arrived fully intact and begin prepping the rocket — a SpaceX Falcon Heavy. The team expects Roman to be ready for launch within a few months after the observatory’s arrival at NASA Kennedy.

“We have a great team, great leadership, and with our successful testing we continue to set the standard for staying within budget and schedule while balancing difficult challenges,” Powell said. “Meeting cost and schedule commitments without compromise to technical standards is a major point of pride for the Roman team.”

Explore a 3D model of the Roman observatory

To learn more about the Roman mission, visit:

www.nasa.gov/roman

By Ashley Balzer
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Media contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, Md.
301-286-1940

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Last Updated
Mar 19, 2026
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Australia’s “Red Centre” Turns Green

January 21, 2026
March 10, 2026
Central Australia’s desert landscape appears predominantly rusty red.
Central Australia’s desert landscape appears predominantly rusty red.
NASA Earth Observatory / Lauren Dauphin
Central Australia’s desert landscape shows widespread green vegetation across areas that are typically red.
Central Australia’s desert landscape shows widespread green vegetation across areas that are typically red.
NASA Earth Observatory / Lauren Dauphin

The town of Alice Springs lies near Australia’s geographic center, in a region often called the “Red Centre” for the rusty hue of its desert landscape. After weeks of heavy rainfall in February and March 2026, however, vast areas of desert and surrounding mountains turned lush and green. 

The MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Terra satellite captured this image (right) of the southern part of Australia’s Northern Territory on March 10, 2026. For comparison, the left image shows the same area in January 2026, before the onset of heavy rains.

The area’s landscape typically appears red due to the oxidation of iron-rich rock. During periods of sufficient rainfall, water begins to flow in previously dry riverbeds, and dormant vegetation springs to life. February 2026 brought more than enough water to the Northern Territory for the transformation to occur—an area average of 239 millimeters (9 inches)—marking the territory’s third-wettest February on a record that dates back to 1900, according to the Bureau of Meteorology.

Beyond the transformation visible from above, the rainfall also caused disruptions on the ground. Thunderstorms earlier in the month produced enough rain to cause water levels on the Todd River and other area rivers to quickly rise, while flash flooding in Alice Springs uprooted trees and left some people stranded, according to news reports. Later in the month, heavy rains returned as another tropical low stalled over central Australia for nearly a week, causing flooding that prompted officials to declare a natural disaster.

As of late March, more extreme weather was on the way for Australia with the approach of Tropical Cyclone Narelle. Bureau of Meteorology forecasts called for severe storm impacts to reach northern Queensland by late on March 19 or March 20. Flooding watches and warnings also extended inland, including to Alice Springs, where past storms have already saturated river catchments.  

NASA Earth Observatory image by Lauren Dauphin, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Story by Kathryn Hansen.

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Central Australia’s desert landscape appears predominantly rusty red.

January 21, 2026

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Central Australia’s desert landscape shows widespread green vegetation across areas that are typically red.

March 10, 2026

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NASA Selects University Finalists for Technology Concepts Competition

Image Credit: National Institute of Aerospace NASA selected 14 university teams from across the nation as finalists in the 2026 Re...