NASA Supports GoAERO University Awardees for Emergency Aircraft Prototyping

NASA Supports GoAERO University Awardees for Emergency Aircraft Prototyping

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Preparations for Next Moonwalk Simulations Underway (and Underwater)

Artist illustration of the Aircraft Harmony, one of the GoAEROs prize competition winners..
Artist’s concept of an emergency response flyer from a team at Texas A&M University and Oklahoma State University, one of 14 university teams that received NASA-supported GoAERO awards in 2025.
Texas A&M University and Oklahoma State University

With support from NASA, the international GoAERO Prize competition recently announced funding for 14 U.S. university teams to build innovative new compact emergency response aircraft. 

The teams will develop prototype versions of Emergency Response Flyers, aircraft intended to perform rescue and response missions after disasters and in crisis situations. The flyers must be designed to deliver a first responder, evacuate victims, provide emergency medical supplies, and aid in humanitarian efforts. Teams will bring their test aircraft to a fly-off expected in 2027. 

These awards will provide students with an opportunity that might have otherwise been difficult – a chance to design and build potentially lifesaving aircraft.

koushik datta

koushik datta

NASA Project Manager

“These awards will provide students with an opportunity that might have otherwise been difficult – a chance to design and build potentially lifesaving aircraft,” said Koushik Datta, University Innovation Project manager in NASA’s Aeronautics Research Mission Directorate at NASA Headquarters in Washington. “At NASA, we’re looking forward to seeing how these young innovators can contribute to our mission to advance futuristic aviation technologies that can benefit first responders and the public.” 

With support from NASA’s University Innovation Project, GoAERO named 14 awardee teams at the following universities: 

  • Auburn University, in Leeds, Alabama  
  • California Polytechnic University, in Pomona  
  • Carnegie Mellon University, in Pittsburgh  
  • Embry-Riddle Aeronautical University, in Daytona Beach, Florida 
  • Georgia Institute of Technology, in Atlanta 
  • North Carolina Agricultural & Technical State University, in Greensboro  
  • North Carolina State University, in Raleigh 
  • The Ohio State University, in Columbus  
  • Penn State University, in State College  
  • Purdue University, in West Lafayette, Indiana  
  • Saint Louis University  
  • Texas A&M University, in College Station, and Oklahoma State University, in Stillwater  
  • University of Texas, Austin  
  • Virginia Tech, in Blacksburg 

Student teams can utilize the funds to purchase parts, materials, batteries, and other components for building their aircrafts. 

When naming the university awardees, GoAERO – in partnership with Boeing, RTX, and Honeywell – also announced 11 winners of Stage 1 of its competition. These include teams from the private sector and universities. These awardees were selected to build full- or smaller-scale flyers for evaluation. Eight entries will be selected for the next round of Stage 2 awards. The GoAERO Prize is still accepting new teams.  While prizes are awarded at Stage 1 and Stage 2, teams do not need to win prizes to continue on to the next stage or compete in the final fly-off.  

In addition to the University Innovation Project support for the university teams, NASA has partnered with GoAERO through a non-funded Space Act Agreement to provide U.S. teams with mentorship, educational opportunities, and access to specialized software tools. 

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Last Updated

Feb 11, 2025

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Lillian Gipson
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Sols 4447–4449: Looking Back at the Marker Band Valley

Sols 4447–4449: Looking Back at the Marker Band Valley

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Sols 4447–4449: Looking Back at the Marker Band Valley

A dim, grainy, grayscale, exaggerated wide-angle photograph from the Martian surface shows two large buttes on the curved horizon, with very rough terrain leading from there to the image foreground. The ground is covered in rocks of all sizes, many large and sharply angled. A rover wheel is visible in the lower left corner of the image, with tracks in the soil leading away from it.
NASA’s Mars rover Curiosity captured this image of its workspace using the rover’s Rear Hazard Avoidance Camera (Rear Hazcam) on sol 4447 — or Martian day 4,447 of the Mars Science Laboratory mission — on Feb. 8, 2025, at 13:54:13 UTC.
NASA/JPL-Caltech

Earth planning date: Friday, Feb. 7, 2025

We are continuing our merry way alongside “Texoli” butte, heading toward the boxworks feature in the distance, our next major waypoint. This is a series of large-scale ridges, which appear from orbital data to be a complex fracture network.  

Of course, we don’t actually expect to get there until late fall 2025, at the earliest. Our drives are long right now (the weekend plan has a 50-meter drive, or about 164 feet) but we are still taking the time to document all of the wonderful geology as we go, and not just speeding past all of the cool things! 

As Conor mentioned in Wednesday’s blog, power is becoming a challenge right now. Those of us in the northern hemisphere might be thinking (eagerly anticipating!) about the return of Spring but Mars is heading into colder weather, meaning we need to use more power for warming up the rover. However, we are also in a very interesting cloud season (as Conor mentioned), so the environmental theme group (ENV) are keen to do lots of imaging right now. This means very careful planning and negotiating between ENV and the geology theme group (GEO) to make the most of the power we do have. Luckily, this plan has something for everyone. 

The GEO group was handed a weekend workspace containing a jumble of rocks — some layered, some not. None of the rocks were very large but we were able to plan APXS and MAHLI on a brushed rock surface at “Aliso Canyon” and on a small, flat unbrushed target, “Bridge to Nowhere,” close to the rover. ChemCam will use the LIBS laser to shoot three bedrock targets, sampling regular bedrock at “Newcomb,” some cracked bedrock at “Devore” and some of the more layered material at “Rubio Canyon.” Mastcam will document the ChemCam LIBS targets. In addition to the cloud imaging, we have lots of other imaging in this plan. We are in position right now to look back down at the “Marker Band Valley,” which we first entered almost a thousand sols ago! Before we go too much further along the side of Texoli butte and lose sight of the Marker Band Valley for some time, both ChemCam and Mastcam will take advantage of this to image the Marker Band Valley and the “Marker Band.” Other images include ChemCam remote images of cap rocks in the distance and two Mastcams of near-field (i.e., close to the rover) troughs.

Written by Catherine O’Connell-Cooper, Planetary Geologist at University of New Brunswick

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Feb 10, 2025

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Mount Everest from Space

Mount Everest from Space

A view of Mount Everest and the surrounding area from space. White snow can be seen on mountains; valleys and shadows appear blue-gray.
This view from space shuttle Columbia shows Mount Everest, which reaches 29,028 feet in elevation (8,848 meters), along with many glaciers. Mount Everest is to the left of the V-shaped valley.
NASA

Crew aboard space shuttle Columbia captured this image of Mount Everest on Nov. 30, 1996, during the STS-80 mission. STS-80, the final shuttle flight of 1996, was highlighted by the successful deployment, operation, and retrieval of two free-flying research spacecraft.

See more photos from this mission.

Image credit: NASA

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Monika Luabeya

NASA Awards Launch Service Task Order for Pandora Mission

NASA Awards Launch Service Task Order for Pandora Mission

The letters NASA on a blue circle with red and white detail, all surrounded by a black background
Credit: NASA

NASA has selected SpaceX of Starbase, Texas, to provide the launch service for the agency’s Pandora mission, which will study at least 20 known exoplanets and their host stars to find out how changes in stars affect our observations of exoplanet atmospheres.

The selection is part of NASA’s Venture-Class Acquisition of Dedicated and Rideshare (VADR) launch services contract. This contract allows the agency to make fixed-price indefinite-delivery/indefinite-quantity awards during VADR’s five-year ordering period, with a maximum total value of $300 million across all contracts.

During its one-year primary mission, Pandora will observe each exoplanet 10 times, observing for 24 hours each visit. It will capture critical data about the planet and its host star during transits, an event where a planet crosses in front of the star it orbits.

The satellite will use an innovative 17-inch (45-centimeter)-wide all-aluminum telescope to simultaneously measure the visible and near-infrared brightness of the host star and obtain near-infrared spectra of the transiting planet. This will allow scientists to cleanly separate star and planetary signals, knowledge that will enhance observations from NASA’s James Webb Space Telescope and future missions searching for habitable worlds, like the agency’s Habitable Worlds Observatory.

Pandora is a joint effort between NASA’s Goddard Space Flight Center in Greenbelt, Maryland, and Lawrence Livermore National Laboratory in California. The Astrophysics Pioneers program, from the Astrophysics Division at NASA Headquarters in Washington, funds Pandora and other astrophysics science missions using smaller, lower cost hardware and payloads. NASA’s Launch Services Program, based at the agency’s Kennedy Space Center in Florida, manages the VADR contract.

To learn more about NASA’s Pandora mission, visit:

https://science.nasa.gov/mission/pandora

-end-

Tiernan Doyle
Headquarters, Washington
202-358-1600
tiernan.doyle@nasa.gov

Patti Bielling
Kennedy Space Center, Florida
321-501-7575
patricia.a.bielling@nasa.gov

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Tiernan P. Doyle

Station Science Top News: Feb. 7, 2025

Station Science Top News: Feb. 7, 2025

Measuring water loss from space

This study showed that the International Space Station’s ECOSTRESS instrument estimates of evapotranspiration (transfer of water to the atmosphere from Earth’s surface and plants) are comparable to ground-based reference values. This finding suggests space measurements could provide guidance for improved water management on large scales.

Worsening droughts due to climate change require better water management. Evapotranspiration is a critical part of the hydrologic cycle, but data are lacking on local water conditions and demands. California’s Eastern Municipal Water District uses the ground-based California Irrigation Management Information System to track evapotranspiration, but it has limited spatial coverage and consistency. Space-based estimates could be better and more consistent.

The International Space Station's ECOSTRESS instrument is shown outside of the space station.
The ECOSTRESS instrument, the white box in the center, is visible on the outside of the station.
NASA

Four-legged robotic retrievers

Space station crew members successfully located and retrieved an object in a simulated Mars environment using a remotely controlled four-legged robot, Bert. Legged robots could provide the ability to explore and survey different extraterrestrial surfaces on future missions.

On uneven lunar and planetary surfaces, robots with legs could explore areas inaccessible to wheeled rovers. Surface Avatar, an investigation from ESA (European Space Agency), evaluated remote control of multiple robots in space, providing information on how human operators respond to physical feedback (such as feeling a bump when a robot arm makes contact) and identifying challenges for orbit-to-ground remote operation of robots. The German Aerospace Center is developing Bert.

ESA astronaut Samantha Cristoforetti practices maneuvers for the Surface Avatar investigation.
ESA astronaut Samantha Cristoforetti practices maneuvers for the Surface Avatar investigation.
NASA

Technology supports atmospheric studies

Researchers found that the Compact Thermal Imager (CTI) on the space station produced scientifically useful imagery of atmospheric phenomena, including gravity waves, clouds, and volcanic plumes. This technology could change current practices and instrument design for remote sensing of Earth from space.

The CTI is mounted on hardware for Robotic Refueling Mission 3, which tested technology for the robotic transfer and storage of cryogenic fluids in microgravity. The station’s orbit provides near-global coverage and CTI has reduced size, energy use, and cost. Its images can measure fires, ice sheets, glaciers, and snow surface temperatures on the ground and the transfer of water from soil and plants into the atmosphere.

Two astronauts install experimental hardware on the space station.
NASA astronaut Anne McClain and CSA astronaut David Saint-Jacques installing the RRM3 hardware.
NASA

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Linda E. Grimm