Jump to content

NASA Opportunities Fuel Growth and Entrepreneurship for Bronco Space Club Students


Recommended Posts

  • Publishers
Posted

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Two men adjust the lens on the Bronco Ember technology
The Bronco Space team assembles its Bronco Ember technology, which uses a short-wave infrared camera with AI to improve early wildfire detection.
Credit: Bronco Space

NASA’s public competitions can catalyze big changes – not just for the agency but also for participants. Bronco Space, the CubeSat laboratory at California State Polytechnic University in Pomona, California, matured more than just space technology as a result of winning funds from NASA’s TechLeap Prize competition. It grew from its roots in a broom closet to a newly built lab on campus, expanding its capacity to mature space technologies long into the future.

The TechLeap Prize seeks to rapidly identify and develop space technologies through a series of challenges that each address a specific technology need for NASA and the nation. In addition to a cash prize, winners receive access to a suborbital or orbital flight opportunity on a commercial flight platform. Bronco Space won $500,000 in the inaugural TechLeap Prize, Autonomous Observation Challenge, launched in 2021. The challenge sought small spacecraft technologies that could autonomously detect, locate, track, and collect data on transient events on Earth and beyond. The team, made up of both undergraduate and graduate students, developed and launched a wildfire detection system called Bronco Ember, which used a short-wave infrared camera with AI (artificial intelligence) to improve early wildfire detection.

Zachary Gaines was an undergraduate student when he participated in the first challenge through TechLeap with Bronco Space. He has since graduated and now supervises the lab at Cal Poly Pomona. Gaines notes how the prize gave the team flexibility to invest in their lab and expand the university’s technology development and maturation capabilities.

“Because TechLeap gave us prize money rather than a grant, we had the freedom to invest those funds,” said Gaines. “If we want to make a real-world impact, which we always want to do, we needed a real lab with equipment. Thanks to TechLeap, we now have space in an innovation village right outside of campus.”

In 2022, Gaines was also involved in Bronco Space’s second time participating in TechLeap as part of the first Nighttime Precision Landing Challenge. The competition sought sensing systems to detect surface hazards from at least 250 meters high and process the data in real-time to generate a terrain map suitable for a spacecraft to land safely in the dark. As one of three winners eligible to receive up to $650,000 each, Bronco Space developed a system using a light projector to create an initial geometry map for landing. The system then uses LIDAR (light detection and ranging) along with advances in computer vision, machine learning, robotics, and computing to generate a map that reconstructs lunar terrain.

A 3D image of a suburban neighborhood, with single family homes on a street that circles the neighborhood.
A demo of the 3D digital “twin” app created by PRISM Intelligence for NASA’s Entrepreneurs Challenge.
Credit: Bronco Space

From the experience with TechLeap, Gaines and other team members formed the small business Pegasus Intelligence and Space, now PRISM Intelligence, and participated in another challenge – NASA’s Entrepreneurs Challenge. This competition seeks the development and commercialization of lunar payloads and climate science through an entrepreneurial and venture lens to advance the Agency’s science exploration goals. The company’s technology, also called PRISM, is a 3D digital map of the world that uses AI to make the “twin” world searchable. The challenge encouraged Gaines and the PRISM team to bridge the gap between available data and consumer end-users. PRISM was a Round 2 winner of the challenge, receiving a share of the $1 million prize as well as exposure to external funders and investors.

Gaines traces the success of PRISM back to his first TechLeap experience: “The company wouldn’t have happened if we hadn’t done TechLeap. It helped me understand how to develop technologies for industry.”

The company and the university continue to secure NASA support. In December 2023, Cal Poly Pomona was selected to receive a two-year funded cooperative agreement through NASA’s University SmallSat Technology Partnership.

“When people invest in your ideas and continue to support them, they help you get smarter and increase your understanding of people’s needs,” said Gaines. “Building technologies with the goal of a real-world impact is really motivating.”

A young man sits on an A-frame ladder inspecting a large piece of technology, a sensing system developed by Bronco Space. The technology appears mostly silver with a pointed top with a silver sphere near the top and a gold-and-solver sphere near the bottom visible from the technology's framed exterior
Members of Bronco Space developed a sensing system that generates a map for precise spacecraft landing as part of NASA’s second TechLeap competition.
Credit: Bronco Space

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • By NASA
      1 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      Will the Sun ever burn out?

      Well, the Sun, just like the stars we see at night, is a star. It’s a giant ball of super hot hydrogen.

      Gravity squeezes it in and it creates energy, which is what makes the Sun shine. Eventually, it will use up all of that hydrogen. But in the process, it’s creating helium. So it will then use the helium. And it will continue to use larger and larger elements until it can’t do this anymore.

      And when that happens, it will start to expand into a red giant about the size of the inner planets. Then it will shrink back down into a very strange star called a white dwarf — super hot, but not very bright and about the size of the Earth.

      But our Sun has a pretty long lifetime. It’s halfway through its 10-billion-year lifetime.

      So the Sun will never really burn out, but it will change and be a very, very different dim kind of star when it reaches the end of its normal life.

      [END VIDEO TRANSCRIPT]

      Full Episode List

      Full YouTube Playlist
      Share
      Details
      Last Updated May 15, 2025 Related Terms
      Science Mission Directorate Heliophysics Heliophysics Division The Solar System The Sun The Sun & Solar Physics Explore More
      4 min read Eclipses, Auroras, and the Spark of Becoming: NASA Inspires Future Scientists
      In the heart of Alaska’s winter, where the night sky stretches endlessly and the aurora…
      Article 16 hours ago 6 min read NASA Observes First Visible-light Auroras at Mars
      On March 15, 2024, near the peak of the current solar cycle, the Sun produced…
      Article 19 hours ago 6 min read NASA’s Magellan Mission Reveals Possible Tectonic Activity on Venus
      Article 19 hours ago Keep Exploring Discover Related Topics
      Missions
      Humans in Space
      Climate Change
      Solar System
      View the full article
    • By NASA
      Explore This Section Science Science Activation Eclipses, Auroras, and the… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science   4 min read
      Eclipses, Auroras, and the Spark of Becoming: NASA Inspires Future Scientists
      In the heart of Alaska’s winter, where the night sky stretches endlessly and the aurora dances across the sky in a display of ethereal beauty, nine undergraduate students from across the United States were about to embark on a transformative journey. These students had been active ‘NASA Partner Eclipse Ambassadors’ in their home communities, nine of more than 700 volunteers who shared the science and awe of the 2024 eclipse with hundreds of thousands of people across the country as part of the NASA Science Activation program’s Eclipse Ambassadors project. Now, these nine were chosen to participate in a once-in a lifetime experience as a part of the “Eclipses to Aurora” Winter Field School at the University of Alaska Fairbanks. Organized by the Astronomical Society of the Pacific and NASA’s Aurorasaurus Citizen Science project, supported by NASA, this program offered more than just lectures—it was an immersive experience into the wonders of heliophysics and the profound connections between the Sun and Earth.
      From January 4 to 11, 2025, the students explored the science behind the aurora through seminars on solar and space physics, hands-on experiments, and tours of cutting-edge research facilities like the Poker Flat Research Range. They also gained invaluable insight from Athabaskan elders, who shared local stories and star knowledge passed down through generations. As Feras recalled, “We attended multiple panels on solar and space physics, spoke to local elders on their connection to the auroras, and visited the Poker Flat Research Range to observe the stunning northern lights.”
      For many students, witnessing the aurora was not only a scientific milestone, but a deeply personal and emotional experience. One participant, Andrea, described it vividly: “I looked to the darkest horizon I could find to see my only constant dream fulfilled before my eyes, so slowly dancing and bending to cradle the stars. All I could do, with my hands frozen and tears falling, I began to dream again with my eyes wide open.” Another student, Kalid, reflected on the shared human moment: “Standing there under the vast Alaskan sky… we were all just people, looking up, waiting for something magical. The auroras didn’t care about our majors or our knowledge—they brought us together under the same sky.”
      These moments of wonder were mirrored by a deeper sense of purpose and transformation. “Over the course of the week, I had the incredible opportunity to explore auroras through lectures on solar physics, planetary auroras, and Indigenous star knowledge… and to reflect on these experiences through essays and presentations,” said Sophia. The Winter Field School was more than an academic endeavor—it was a celebration of science, culture, and shared human experience. It fostered not only understanding but unity and awe, reminding everyone involved of the profound interconnectedness of our universe.
      The impact of the program continues to resonate. For many students, that one aurora-lit week in Alaska became a turning point in the focus of their careers. Sophia has since been accepted into graduate school to pursue heliophysics. Vishvi, inspired by the intersection of science and society, will begin a program in medical physics at the University of Pennsylvania this fall. And Christy, moved by her time at the epicenter of aurora research, has applied to the Ph.D. program in Space Physics at the University of Alaska Fairbanks—the very institution that helped spark her journey. Their stories are powerful proof that the Winter Field School didn’t just teach—it awakened purpose, lit new paths, and left footprints on futures still unfolding.
      Eclipse Ambassadors is supported by NASA under cooperative agreement award number 80NSS22M0007 and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn/about-science-activation/
      Participants at the Winter Field School are enjoying the trip to Anchorage, AK. Andy Witteman Share








      Details
      Last Updated May 14, 2025 Editor NASA Science Editorial Team Related Terms
      Science Activation Auroras Eclipses Opportunities For Students to Get Involved Explore More
      4 min read Take a Tour of the Cosmos with New Interactives from NASA’s Universe of Learning


      Article


      1 day ago
      6 min read What NASA Is Learning from the Biggest Geomagnetic Storm in 20 Years


      Article


      5 days ago
      6 min read Building for a Better World: Norfolk Students Bring STEM to Life with NASA Partnership


      Article


      4 weeks ago
      Keep Exploring Discover More Topics From NASA
      James Webb Space Telescope


      Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…


      Perseverance Rover


      This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial…


      Parker Solar Probe


      On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona…


      Juno


      NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to…

      View the full article
    • By NASA
      6 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      This artist’s concept shows the Moon’s hot interior and volcanism about 2 to 3 billion years ago. It is thought that volcanic activity on the lunar near side (the side facing Earth) helped create a landscape dominated by vast plains called mare, which are formed by molten rock that cooled and solidified. NASA/JPL-Caltech Analyzing gravity data collected by spacecraft orbiting other worlds reveals groundbreaking insights about planetary structures without having to land on the surface.
      Although the Moon and the asteroid Vesta are very different, two NASA studies use the same technique to reveal new details about the interiors of both.
      In the lunar study, published May 14 in the journal Nature, researchers developed a new gravity model of the Moon that includes tiny variations in the celestial body’s gravity during its elliptical orbit around Earth. These fluctuations cause the Moon to flex slightly due to Earth’s tidal force — a process called tidal deformation — which provides critical insights into the Moon’s deep internal structure.
      Using their model, the researchers produced the most detailed lunar gravitational map yet, providing future missions an improved way to calculate location and time on the Moon. They accomplished this by analyzing data on the motion of NASA’s GRAIL (Gravity Recovery and Interior Laboratory) mission, whose spacecraft, Ebb and Flow, orbited the Moon from Dec. 31, 2011, to Dec. 17, 2012.
      These views of the Moon’s near side, left, and far side were put together from observations made by NASA’s Lunar Reconnaissance Orbiter. NASA/JPL-Caltech In a second study, published in the journal Nature Astronomy on April 23, the researchers focused on Vesta, an object in the main asteroid belt between Mars and Jupiter. Using NASA’s Deep Space Network radiometric data and imaging data from the agency’s Dawn spacecraft, which orbited the asteroid from July 16, 2011, to Sept. 5, 2012, they found that instead of having distinct layers as expected, Vesta’s internal structure may be mostly uniform, with a very small iron core or no core at all.
      “Gravity is a unique and fundamental property of a planetary body that can be used to explore its deep interior,” said Park. “Our technique doesn’t need data from the surface; we just need to track the motion of the spacecraft very precisely to get a global view of what’s inside.”
      Lunar Asymmetry
      The lunar study looked at gravitational changes to the Moon’s near and far sides. While the near side is dominated by vast plains — known as mare — formed by molten rock that cooled and solidified billions of years ago, the far side is more rugged, with few plains.
      NASA’s Dawn mission obtained this image of the giant asteroid Vesta on July 24, 2011. The spacecraft spent 14 months orbiting the asteroid, capturing more than 30,000 images and fully mapping its surface. NASA/JPL-Caltech/UCLA/MPS/DLR/IDA Both studies were led by Ryan Park, supervisor of the Solar System Dynamics Group at NASA’s Jet Propulsion Laboratory in Southern California, and were years in the making due to their complexity. The team used NASA supercomputers to build a detailed map of how gravity varies across each body. From that, they could better understand what the Moon and Vesta are made of and how planetary bodies across the solar system formed.
      Some theories suggest intense volcanism on the near side likely caused these differences. That process would have caused radioactive, heat-generating elements to accumulate deep inside the near side’s mantle, and the new study offers the strongest evidence yet that this is likely the case.
      “We found that the Moon’s near side is flexing more than the far side, meaning there’s something fundamentally different about the internal structure of the Moon’s near side compared to its far side,” said Park. “When we first analyzed the data, we were so surprised by the result we didn’t believe it. So we ran the calculations many times to verify the findings. In all, this is a decade of work.”
      When comparing their results with other models, Park’s team found a small but greater-than-expected difference in how much the two hemispheres deform. The most likely explanation is that the near side has a warm mantle region, indicating the presence of heat-generating radioactive elements, which is evidence for volcanic activity that shaped the Moon’s near side 2 billion to 3 billion years ago.
      Vesta’s Evolution
      Park’s team applied a similar approach for their study that focused on Vesta’s rotational properties to learn more about its interior.  
      “Our technique is sensitive to any changes in the gravitational field of a body in space, whether that gravitational field changes over time, like the tidal flexing of the Moon, or through space, like a wobbling asteroid,” said Park. “Vesta wobbles as it spins, so we could measure its moment of inertia, a characteristic that is highly sensitive to the internal structure of the asteroid.”
      Changes in inertia can be seen when an ice skater spins with their arms held outward. As they pull their arms in, bringing more mass toward their center of gravity, their inertia decreases and their spin speeds up. By measuring Vesta’s inertia, scientists can gain a detailed understanding of the distribution of mass inside the asteroid: If its inertia is low, there would be a concentration of mass toward its center; if it’s high, the mass would be more evenly distributed.
      Some theories suggest that over a long period, Vesta gradually formed onion-like layers and a dense core. But the new inertia measurement from Park’s team suggests instead that Vesta is far more homogeneous, with its mass distributed evenly throughout and only a small core of dense material, or no core.
      Gravity slowly pulls the heaviest elements to a planet’s center over time, which is how Earth ended up with a dense core of liquid iron. While Vesta has long been considered a differentiated asteroid, a more homogenous structure would suggest that it may not have fully formed layers or may have formed from the debris of another planetary body after a massive impact.
      In 2016, Park used the same data types as the Vesta study to focus on Dawn’s second target, the dwarf planet Ceres, and results suggested a partially differentiated interior.
      Park and his team recently applied a similar technique to Jupiter’s volcanic moon Io, using data acquired by NASA’s Juno and Galileo spacecraft during their flybys of the Jovian satellite as well as from ground-based observations. By measuring how Io’s gravity changes as it orbits Jupiter, which exerts a powerful tidal force, they revealed that the fiery moon is unlikely to possess a global magma ocean.
      “Our technique isn’t restricted just to Io, Ceres, Vesta, or the Moon,” said Park. “There are many opportunities in the future to apply our technique for studying the interiors of intriguing planetary bodies throughout the solar system.”
      News Media Contacts
      Ian J. O’Neill
      Jet Propulsion Laboratory, Pasadena, Calif.
      818-354-2649
      ian.j.oneill@jpl.nasa.gov
      Karen Fox / Molly Wasser
      NASA Headquarters, Washington
      202-358-1600
      karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
      Share
      Details
      Last Updated May 14, 2025 Related Terms
      Vesta Dawn Earth's Moon GRAIL (Gravity Recovery And Interior Laboratory) Jet Propulsion Laboratory Planetary Science Small Bodies of the Solar System The Solar System Explore More
      7 min read Webb’s Titan Forecast: Partly Cloudy With Occasional Methane Showers
      Saturn’s moon Titan is an intriguing world cloaked in a yellowish, smoggy haze. Similar to…
      Article 3 hours ago 5 min read NASA’s Europa Clipper Captures Mars in Infrared
      Article 2 days ago 5 min read NASA’s Webb Reveals New Details, Mysteries in Jupiter’s Aurora
      NASA’s James Webb Space Telescope has captured new details of the auroras on our solar…
      Article 2 days ago Keep Exploring Discover Related Topics
      Missions
      Humans in Space
      Climate Change
      Solar System
      View the full article
    • By NASA
      NASA Glenn Research Center senior materials research engineer Kim de Groh, who conducted research for Hubble Space Telescope servicing missions, shared her experiences during a presentation at Great Lakes Science Center, home of the NASA Glenn Visitor Center, in Cleveland on Thursday, May 8, 2025. Credit: NASA/Dennis Brown  April 24 marked the 35th anniversary of the launch of NASA’s Hubble Space Telescope. The iconic space observatory remains a household name —the most well-recognized and scientifically productive telescope in history. Engineers at NASA’s Glenn Research Center in Cleveland played a significant role in how the telescope functions today.  
      NASA’s Glenn Research Center researchers Kim de Groh, left, and Joyce Dever conducted research for Hubble Space Telescope servicing missions. De Groh shared her experiences during a presentation at Great Lakes Science Center, home of the NASA Glenn Visitor Center, in Cleveland on Thursday, May 8, 2025. Credit: NASA/Sara Lowthian-Hanna  NASA Glenn researchers assisted in all five Hubble servicing missions by testing damaged insulation, determining why it degraded in space, and recommending replacement materials.  
      One of those researchers, Kim de Groh, senior materials research engineer, shared some of that research in a special presentation at Great Lakes Science Center, home of the NASA Glenn Visitor Center, in Cleveland on May 8. She chronicled her Hubble experience with a presentation, a show-and-tell with samples directly from the telescope, and a Q&A addressing the audience’s Hubble-related questions. 
      Return to Newsletter Explore More
      1 min read NASA Glenn Hosts Slovenian Delegation and Ohio Governor’s Office
      Article 48 seconds ago 1 min read Specialty NASA Glenn License Plates Available  
      Article 1 min ago 1 min read NASA Glenn Shows Students Temperature-Cooling Technology
      Article 2 mins ago View the full article
    • By NASA
      NASA Glenn Research Center’s Associate Director Larry Sivic, front row, third from left, joins in a group photo with Slovenian government officials and representatives from the Ohio Governor’s Office during a visit to the center on Friday, April 11, 2025. Credit: NASA/Jef Janis  NASA’s Glenn Research Center in Cleveland hosted a delegation of Slovenian government officials and representatives from the Ohio Governor’s Office on April 11. NASA Glenn leadership provided the group with an overview of the center’s vital role within the agency. The delegation also visited key space-related and aeronautics facilities, including tours of the Zero Gravity Research Facility, Simulated Lunar Operations Laboratory, and Icing Research Tunnel. 
      Republic of Slovenia Minister of Defense Borut Sajovic and Ambassador of the Republic of Slovenia to the United States Iztok Mirosic headed the delegation. Joe Zeis, who is the senior advisor for Aerospace and Defense for the Office of the Governor, and Tobias Engel, who is with the Ohio Department of Development International Affairs, also attended. 
      Facility Manager Dennis Eck, second from left, points out features of NASA Glenn Research Center’s Icing Research Tunnel to a delegation of Slovenian government officials and representatives from the Ohio Governor’s Office during a tour to the center on Friday, April 11, 2025. Credit: NASA/Jef Janis  The Slovenia Space Office — under the Ministry of the Economy, Industry, and Sport — coordinates Slovenia’s space activities within ESA (European Space Agency). Slovenia recently became a member state of ESA, enabling more international opportunities for Slovenian scientists and engineers. Last year, Slovenia joined the Artemis Accords, which provides a common set of principles to enhance the governance of the civil exploration and use of outer space, as the 39th participant.  
      Return to Newsletter Explore More
      1 min read NASA Glenn Engineer Highlights Research for Hubble Servicing Missions 
      Article 21 seconds ago 1 min read Specialty NASA Glenn License Plates Available  
      Article 1 min ago 1 min read NASA Glenn Shows Students Temperature-Cooling Technology
      Article 2 mins ago View the full article
  • Check out these Videos

×
×
  • Create New...