NASA - Breaking News
10 Years of Students Helping NASA Grow Space Food with Growing Beyond Earth
3 min read
10 Years of Students Helping NASA Grow Space Food with Growing Beyond Earth Students from 71 Classrooms engaged with NASA scientists to learn about how their Growing Beyond Earth research is contributing to feeding astronauts for long distance space travel.Nearly 1,250 middle and high school students from 71 schools around the world joined Fairchild Tropical Botanic Garden for the Growing Beyond Earth (GBE) Student Launch Chat with the Scientists, marking an inspiring milestone in the program’s 10th anniversary year.
The live session, held in collaboration with NASA, connected classrooms directly with Dr. Gioia Massa and Trent M. Smith, senior leaders of NASA Kennedy Space Center’s Space Crop Production team. Students heard firsthand how their classroom experiments are helping NASA identify and grow the best crops for future astronauts on long-duration missions to the Moon and Mars.
“Our students are contributing to real NASA science,” said one participating teacher. “It’s incredibly motivating for them to know their data could influence what astronauts eat in space someday.”
Connecting Classrooms with NASA ScienceGrowing Beyond Earth, led by Fairchild Tropical Botanic Garden in Miami, Florida, brings authentic NASA research into classrooms in a way that few science programs can. For more than a decade, the 83-acre botanic garden – renowned for its conservation, education, and research programs – has worked hand-in-hand with NASA to advance understanding of food production in space.
Students use specially designed plant growth chambers to test how different crops perform under conditions that mimic spacecraft environments. The data they collect are shared with NASA scientists, who use the findings to refine ongoing space crop production research.
Since the program’s inception, more than 120,000 students across 800+ classrooms have tested over 250 plant cultivars, with five student-tested crops already grown aboard the International Space Station.
Cultivating the Future STEM (Science, Technology, Engineering, & Mathematics) WorkforceThe Growing Beyond Earth project exemplifies the mission of NASA’s Science Activation (SciAct) program, which connects NASA Science with people of all ages and backgrounds in ways that activate minds and promote a deeper understanding of our world and beyond, with the ultimate Vision: To increase learners’ active participation in the advancement of human knowledge. By engaging students as active participants in cutting-edge research, projects like GBE not only advance NASA’s goals but also cultivate curiosity, creativity, and confidence in the next generation of scientists and explorers. This year’s GBE Student Launch Chat celebrated that impact, showing how student research from classrooms around the globe contributes to the future of space exploration.
“When students see themselves as part of NASA’s mission, they realize science isn’t something distant, it’s something they can do,” said Dr. Massa. Teacher Espy Rodriguez from Hialeah Senior High School said, “It made their [her students] projects matter. I think it gave the kids a real sense of community. We are far, but we are one.” By growing plants, analyzing data, and sharing results with NASA, these students are helping humanity prepare for life beyond Earth, proving that the seeds of tomorrow’s discoveries are being planted in today’s classrooms.
GBE is supported by NASA under cooperative agreement award number 80NCCS2M0125 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/.
Share Details Last Updated Nov 21, 2025 Editor NASA Science Editorial Team Location Kennedy Space Center Related Terms Explore More 6 min read NASA Fuels Discovery from Earth to Sky: One Crayon at a TimeArticle
1 day ago
5 min read Helio Highlights: October 2025
Since we all have a relationship with the Sun, it is important to learn about…
Article
2 months ago
2 min read OSDR and PSI Unveil New Consolidated Website
Article
2 months 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…
Hubble Captures Puzzling Galaxy
This NASA/ESA Hubble Space Telescope image features a galaxy that’s hard to categorize. The galaxy in question is NGC 2775, which lies 67 million light-years away in the constellation Cancer (the Crab). NGC 2775 sports a smooth, featureless center that is devoid of gas, resembling an elliptical galaxy. It also has a dusty ring with patchy star clusters, like a spiral galaxy. Which is it: spiral or elliptical — or neither?
Because we can only view NGC 2775 from one angle, it’s difficult to say for sure. Some researchers classify NGC 2775 as a spiral galaxy because of its feathery ring of stars and dust, while others classify it as a lenticular galaxy. Lenticular galaxies have features common to both spiral and elliptical galaxies.
Astronomers aren’t certain of exactly how lenticular galaxies come to be, and they might form in a variety of ways. Lenticular galaxies might be spiral galaxies that merged with other galaxies, or that have mostly run out of star-forming gas and lost their prominent spiral arms. They also might have started out more like elliptical galaxies, then collected gas into a disk around them.
Some evidence suggests that NGC 2775 merged with other galaxies in the past. Invisible in this Hubble image, NGC 2775 has a tail of hydrogen gas that stretches almost 100,000 light-years around the galaxy. This faint tail could be the remnant of one or more galaxies that wandered too close to NGC 2775 before being stretched apart and absorbed. If NGC 2775 merged with other galaxies in the past, it could explain the galaxy’s strange appearance today.
Most astronomers classify NGC 2775 as a flocculent spiral galaxy. Flocculent spirals have poorly defined, discontinuous arms that are often described as “feathery” or as “tufts” of stars that loosely form spiral arms.
Hubble previously released an image of NGC 2775 in 2020. This new version adds observations of a specific wavelength of red light emitted by clouds of hydrogen gas surrounding massive young stars, visible as bright, pinkish clumps in the image. This additional wavelength of light helps astronomers better define where new stars are forming in the galaxy.
What is BioSentinel?
Editor’s Note: This article was updated Nov. 21, 2025 shortly after BioSentinel’s mission marked three years of operation in deep space.
Astronauts live in a pretty extreme environment aboard the International Space Station. Orbiting about 250 miles above the Earth in the weightlessness of microgravity, they rely on commercial cargo missions about every two months to deliver new supplies and experiments. And yet, this place is relatively protected in terms of space radiation. The Earth’s magnetic field shields space station crew from much of the radiation that can damage the DNA in our cells and lead to serious health problems. When future astronauts set off on long journeys deeper into space, they will be venturing into more perilous radiation environments and will need substantial protection. With the help of a biology experiment within a small satellite called BioSentinel, scientists at NASA’s Ames Research Center, in California’s Silicon Valley, are taking an early step toward finding solutions.
To learn the basics of what happens to life in space, researchers often use “model organisms” that we understand relatively well. This helps show the differences between what happens in space and on Earth more clearly. For BioSentinel, NASA is using yeast – the very same yeast that makes bread rise and beer brew. In both our cells and yeast cells, the type of high-energy radiation encountered in deep space can cause breaks in the two entwined strands of DNA that carry genetic information. Often, DNA damage can be repaired by cells in a process that is very similar between yeast and humans.
Conceptual graphic of a radiation particle causing a double-stranded DNA break.BioSentinel set out to be the first long-duration biology experiment to take place beyond where the space station orbits near Earth. BioSentinel’s spacecraft is one of 10 CubeSats that launched aboard Artemis I, the first flight of the Artemis program’s Space Launch System, NASA’s powerful new rocket. The cereal box-sized satellite traveled to deep space on the rocket then flew past the Moon in a direction to orbit the Sun. Once the satellite was in position beyond our planet’s protective magnetic field, the BioSentinel team triggered a series of experiments remotely, activating two strains of the yeast Saccharomyces cerevisiae to grow in the presence of space radiation. Samples of yeast were activated at different time points throughout the six- to twelve-month mission.
One strain is the yeast commonly found in nature, while the other was selected because it has trouble repairing its DNA. By comparing how the two strains respond to the deep space radiation environment, researchers will learn more about the health risks posed to humans during long-term exploration and be able to develop informed strategies for reducing potential damage.
During the initial phase of the mission, which began in December 2022 and completed in April 2023, the BioSentinel team successfully operated BioSentinel’s BioSensor hardware – a miniature biotechnology laboratory designed to measure how living yeast cells respond to long-term exposure to space radiation – in deep space. The team completed four experiments lasting two-weeks each but did not observe any yeast cell growth. They determined that deep space radiation was not the cause of the inactive yeast cells, but that their lack of growth was likely due to the yeast expiring after extended storage time of the spacecraft ahead of launch.
Although the yeast did not activate as intended to gather observations on the impact of radiation on living yeast cells, BioSentinel’s onboard radiation detector – that measures the type and dose of radiation hitting the spacecraft – continues to collect data in deep space.
Jesse Fusco, left, and James Milsk, right, at the BioSentinel command console at the Multi-Mission Operations Center at NASA’s Ames Research Center in Silicon Valley. The team is receiving spacecraft telemetry at the three-year timepoint since the mission launched on Artemis I. BioSentinel continues to fly in its heliocentric orbit, now more than 48 million miles from Earth. NASA/Don RicheyNASA has extended BioSentinel’s mission to continue collecting valuable deep space radiation data in the unique, high-radiation environment beyond low Earth orbit.
The Sun has an 11-year cycle, in which solar activity rises and falls in the form of powerful solar flares and giant eruptions called coronal mass ejections. As the solar cycle progresses from maximum to a declining phase, scientists expect strong solar activity to continue through 2026, with some of the strongest storms seen during this declining phase. These events send powerful bursts of energy, magnetic fields, and plasma into space which causes the aurora and can interfere with satellite signals. Solar radiation events from particles accelerated to high speeds can also pose a threat to astronauts in space.
Built on a history of small-satellite biologyThe BioSentinel project builds on Ames’ history of carrying out biology studies in space using CubeSats – small satellites built from individual units each about four inches cubed. BioSentinel is a six-unit spacecraft weighing about 30 pounds. It houses the yeast cells in tiny compartments inside microfluidic cards – custom hardware that allows for the controlled flow of extremely small volumes of liquids that will activate and sustain the yeast. Data about radiation levels and the yeast’s growth and metabolism will be collected and stored aboard the spacecraft and then transmitted to the science team back on Earth.
A reserve set of microfluidic cards containing yeast samples will be activated if the satellite encounters a solar particle event, a radiation storm coming from the Sun that is a particularly severe health risk for future deep space explorers.
BioSentinel’s microfluidics card, designed at NASA’s Ames Research Center in Silicon Valley, California, will be used to study the impact of interplanetary space radiation on yeast. Once in orbit, the growth and metabolic activity of the yeast will be measured using a three-color LED detection system and a dye that provides a readout of yeast cell activity. Here, pink wells contain actively growing yeast cells that have turned the dye from blue to pink color.NASA/Dominic Hart Multiple BioSentinels will compare various gravity and radiation environmentsIn addition to the pioneering BioSentinel mission that will traverse the deep space environment, identical experiments take place under different radiation and gravity conditions. One ran on the space station, in microgravity that is similar to deep space, but with comparatively less radiation. Other experiments took place on the ground, for comparison with Earth’s gravity and radiation levels. These additional versions show scientists how to compare Earth and space station-based science experiments – which can be conducted much more readily – to the fierce radiation that future astronauts will encounter in space.
Taken together, the BioSentinel data will be critical for interpreting the effects of space radiation exposure, reducing the risks associated with long-term human exploration, and confirming existing models of the effects of space radiation on living organisms.
Milestones- December 2021: The BioSentinel ISS Control experiment launched to the International Space Station aboard SpaceX’s 24th commercial resupply services mission.
- January 2022: The BioSentinel ISS Control experiment began science operations aboard the International Space Station.
- February 2022: The BioSentinel ISS Control experiment began ground control science operations at NASA Ames.
- June 2022: The BioSentinel ISS Control experiment completed science operations. The hardware was returned to Earth in August aboard SpaceX’s CRS-25 Dragon.
- October 2022: The BioSentinel ISS Control experiment completed ground control science operations at NASA Ames.
- Nov. 16, 2022: BioSentinel launched to deep space aboard Artemis I.
- Dec. 5, 2022: BioSentinel began science operations in deep space.
- Dec. 19, 2022: BioSentinel began ground control science operations at NASA Ames.
- Nov. 16, 2024: BioSentinel marks two years of continuous radiation observations in deep space, now more than 30 million miles from Earth.
- Nov. 16, 2025: BioSentinel marks three years of continuous radiation observations in deep space, now more than 48 million miles from Earth.
Partners:
- NASA Ames leads the science, hardware design and development of the BioSentinel mission.
- Partner organizations include NASA’s Johnson Space Center in Houston and NASA’s Jet Propulsion Laboratory in Southern California.
- BioSentinel is funded by the Mars Campaign Development (MCO) Division within the Exploration Systems Development Mission Directorate at NASA headquarters in Washington.
- BioSentinel’s extended mission is supported by the Heliophysics Division of NASA’s Science Mission Directorate at NASA headquarters in Washington, the MCO, and the NASA Electronic Parts and Packaging Program within NASA’s Space Technology Mission Directorate at NASA Headquarters in Washington.
Learn more:
- NASA story: NASA’s BioSentinel Studies Solar Radiation as Earth Watches Aurora (Sept. 2024)
- NASA story: NASA Extends BioSentinel’s Mission to Measure Deep Space Radiation, Aug. 2023
- NASA story: First Deep Space Biology Experiment Begins, Follow Along in Real-Time, Dec. 2022
- NASA story: BioSentinel Underway After Successful Lunar Flyby, Nov. 2022
- NASA story: Artemis I to Launch First-of-a-Kind Deep Space Biology Mission, Aug. 2022
- NASA video: Why NASA is Sending Yeast to Deep Space, Feb. 2022
- NASA podcast: “Houston We Have a Podcast,” Deep Space Biology, Jan. 2022
- NASA blog: All Artemis I Secondary Payloads Installed in Rocket’s Orion Stage Adapter, Oct. 2021
- NASA blog; NASA Prepares Three More CubeSat Payloads for Artemis I Mission. Jul. 2021
- NASA story: NASA’s BioSentinel Team Prepares CubeSat For Deep Space Flight, Apr. 2021
- NASA in Silicon Valley podcast episode: Sharmila Bhattacharya on Studying How Biology Changes in Space, Mar. 2018
- NASA story: For Holiday Celebrations and Space Radiation, Yeast is the Key, Dec. 2018
For researchers:
- NASA Space Station Research Explorer: BioSentinel ISS Control Experiment
- NASA technical webpage: BioSentinel
For news media:
- Members of the news media interested in covering this topic should reach out to the NASA Ames newsroom.
25 Years of Scientific Discovery Aboard the International Space Station
November marks 25 years of human presence aboard the International Space Station, a testament to international collaboration and human ingenuity. Since the first crew arrived on Nov. 2, 2000, NASA and its partners have conducted thousands of research investigations and technology demonstrations to advance exploration of the Moon and Mars and benefit life on Earth.
Researchers have taken advantage of the unique microgravity environment to conduct experiments impossible to replicate on Earth, transforming research across disciplines. More than 4,000 experiments have pushed the boundaries of science, sparked discoveries, and driven scientific breakthroughs.
“25 years ago, Expedition 1 became the first crew to call the International Space Station home, beginning a period of continuous human presence in space that still continues to this day,” said NASA acting administrator Sean Duffy. “This historic milestone would not have been possible without NASA and its partners, as well as every astronaut and engineer who works to keep the lights on in low Earth orbit.”
To celebrate a quarter century of innovation in microgravity, NASA is highlighting 25 scientific breakthroughs that exemplify the station’s enduring impact on science, technology, and exploration.
Building the road to the Moon and Mars The waxing crescent moon appears just above the Earth’s atmosphere as the International Space Station orbits the Earth.NASANASA uses the space station as a proving ground to develop new systems and technologies for missions beyond low Earth orbit.
- Navigation, communication, and radiation shielding technologies proven aboard the space station are being integrated into spacecraft and missions to reach the Moon and Mars.
- Robotic systems, for example a robotic surgeon and autonomous assistants, will expand available medical procedures and allow astronauts to dedicate time to more crucial tasks during missions far from Earth.
- Astronauts have used recycled plastic and stainless steel to 3D print tools and parts. The ability to 3D print in space lays the groundwork for on-demand repair and fabrication during future deep space missions where resupply isn’t readily available.
- From the deployment of the first wooden satellite to laser communications and self-healing quantum communications, the space station is a proving ground for cutting-edge space technologies.
Why this matters:
Humanity’s push to the Moon and Mars begins with discoveries in low Earth orbit. From demonstrating how astronauts can live, work, and repair equipment off Earth to testing life-support systems and advanced materials, every innovation aboard the station helps to advance NASA’s Artemis and other exploration initiatives and brings humanity closer to thriving beyond our planet.
Sustaining life beyond Earth NASA astronauts Jessica Watkins, front, and Bob Hines, back, work on XROOTS aboard the International Space Station. This experiment used the station’s Veggie facility to test soilless hydroponic and aeroponic plant growth.NASAAs NASA prepares to return humans to the Moon through the Artemis program and push onward to Mars, sustaining life beyond Earth is more critical than ever.
- Astronauts have grown more than 50 species of plants in space, including tomatoes, bok choi, romaine lettuce, and chili peppers.
- Advanced life support systems are capable of recycling up to 98% of water in the U.S. segment aboard the space station, the ideal level needed for exploration missions.
- Crew health data shows how space affects the brain, vision, balance and control, and muscle and bone density, guiding strategies to maintain astronaut performance during extended missions and improve health on Earth.
- Researchers have sequenced DNA in orbit and are advancing techniques to enable real-time assessment of microbial life in space, which is essential to maintaining astronaut health.
Why this matters:
By growing food, recycling water, and improving medical care in space, NASA is paving the way for future long-duration missions to the Moon and Mars while revolutionizing agriculture and medicine back home.
Helping humanity on Earth Pharmaceutical crystals grown aboard the International Space Station are shown after returning to Earth.RedwireResearch aboard the orbiting laboratory not only pushes humanity farther into the cosmos but can help address complex human health issues on the ground. By providing a platform for long-term microgravity research, the space station fosters breakthroughs that yield direct benefits to people on Earth.
- Research aboard the space station provides new insights to develop treatments for diseases like cancer, Alzheimer’s, Parkinson’s, and heart disease by revealing how microgravity alters cellular functions.
- New developments in medicine for cancer, muscular dystrophy, and neurodegenerative diseases have come from growing protein crystals in microgravity with larger, more organized structures.
- High quality stem cells can be grown in greater quantities in space, helping to develop new regenerative therapies for neurological, cardiovascular, and immunological conditions.
- Pioneering efforts in 3D bioprinting, which uses cells, proteins, and nutrients as source material, have produced human tissue structures such as a knee meniscus and heart tissue, a major step toward manufacturing organs in space for transplant patients on Earth.
- Researchers are using miniaturized tissue models to observe how space affects tissues and organ systems, offering new ways to develop and test medicines to protect astronauts on future missions and improve treatments on Earth.
- Photos taken by astronauts have supported emergency response to natural disasters, such as hurricanes, with targeted views from space.
- Instruments mounted on the space station protect critical space infrastructure and provide data on the planet’s natural patterns by measuring Earth’s resources and space weather.
Why this matters:
Microgravity research is moving us closer to manufacturing human organs in space for transplant and revealing new ways to fight cancer, heart disease, osteoporosis, neurodegenerative disease, and other serious illnesses that affect millions of people worldwide. The station also serves as an observation platform to monitor natural disasters, weather patterns, and Earth’s resources.
Understanding our universe Artist concept of operations inside NASA’s Cold Atom Laboratory aboard the International Space Station.NASAThe space station offers scientists an unparalleled vantage point to learn about the fundamental behavior of the universe. By studying cosmic phenomena typically blocked or absorbed by Earth’s atmosphere and observing physics at an atomic level, researchers can probe mysteries impossible to study from Earth.
- Data from X-ray telescopes on the space station’s exterior have been featured in more than 700 research publications, helping to improve our understanding of collapsing stars, black holes, and ripples in the fabric of space-time.
- Researchers have recorded billions of cosmic events, helping scientists search for antimatter and dark matter signatures in space.
- Scientists have created and studied the fifth state of matter on the space station, allowing researchers to use quantum science to advance technology like space navigation, satellite operations, and GPS systems on Earth.
Why this matters:
Research aboard the space station is helping us unravel the deepest mysteries of our universe, from the smallest quantum particles to the most powerful cosmic explosions. Observations of collapsing stars and black holes could inspire new navigation tools using cosmic signals and expand our grasp of space-time. Studies of antimatter and dark matter bring us closer to understanding the 95% of the universe invisible to the human eye. Creating the fifth state of matter in space unlocks new quantum pathways that could transform technology on Earth and in space.
Learning new physics This image shows a flame ignited as part of the Flame Design investigation on the International Space Station.NASAPhysical processes behave differently in microgravity, offering scientists a new lens for discovery.
- Engineers can design more efficient fuel and life support systems for future spacecraft thanks to studies of fluid boiling, containment, and flow.
- Analyzing gels and liquids mixed with tiny particles in space helps researchers fine-tune material compositions and has led to new patents for consumer products.
- The discovery of cool flames in space, a phenomenon difficult to study on Earth, has opened new frontiers in combustion science and engine design.
Why this matters:
Breakthroughs in fundamental physics aboard the space station drive innovation on Earth and advance spacecraft fuel, thermal control, plant watering, and water purification systems. Research in soft materials is improving products in medicine, household products, and renewable energy, while cool flames studies may lead to cleaner, more efficient engines.
Enabling global access to space NASA astronaut Nichole Ayers talks on a ham radio with students from Lakeside Junior High School in Springdale, Arkansas. Ayers answered questions from the students about her experience living and working aboard the International Space Station.NASASince 2000, the space station has opened doors for private companies, researchers, students, and astronauts around the world to participate in exploration and help propel humanity forward to the Moon and Mars.
- The space station is a launchpad for the commercial space economy, enabling private astronaut missions and hosting hundreds of experiments from commercial companies, giving them the chance to strengthen their technologies through in-orbit research, manufacturing demonstrations, and innovation.
- CubeSats deployed from the space station enable students and innovators around the world to test radio antennas, small telescopes, and other scientific demonstrations in space.
- More than one million students have engaged with astronauts via ham radio events, inspiring the next generation to participate in science, technology, engineering, and mathematics.
- More than 285 crew members from more than 25 countries have visited humanity’s longest-operating outpost in space, making it a symbol of global collaboration.
Why this matters:
The space station has enabled the space economy, where commercial research, manufacturing, and technology demonstrations are shaping a new global marketplace. NASA and its international partners have established a leadership position in low Earth orbit, creating new opportunities for industry and paving the way for exploration missions to the Moon, Mars, and beyond.
Learn more about the research aboard the International Space Station at:
Revisit the 20th anniversary for more information.
Keep Exploring Discover More Topics From NASA International Space Station: 25 YearsNovember 2, 2025, marked a historic milestone: 25 years of continuous human presence aboard the International Space Station.
Latest News from Space Station Research
Space Station Research and Technology
Humans In Space
Hubble Seeks Clusters in ‘Lost Galaxy’
- Hubble Home
- Overview
- Impact & Benefits
- Science
- Observatory
- Team
- Multimedia
- News
- More
2 min read
Hubble Seeks Clusters in ‘Lost Galaxy’ This NASA/ESA Hubble Space Telescope image features the spiral galaxy NGC 4535. ESA/Hubble & NASA, F. Belfiore, J. Lee and the PHANGS-HST TeamToday’s NASA/ESA Hubble Space Telescope image features the spiral galaxy NGC 4535, which is situated about 50 million light-years away in the constellation Virgo (the Maiden). Through a small telescope, this galaxy appears extremely faint, giving it the nickname ‘Lost Galaxy’. With a mirror spanning nearly eight feet (2.4 meters) across and its location above Earth’s light-obscuring atmosphere, Hubble can easily observe dim galaxies like NGC 4535 and pick out features like its massive spiral arms and central bar of stars.
This image features NGC 4535’s young star clusters, which dot the galaxy’s spiral arms. Glowing-pink clouds surround many of these bright-blue star groupings. These clouds, called H II (‘H-two’) regions, are a sign that the galaxy is home to especially young, hot, and massive stars that blaze with high-energy radiation. Such massive stars shake up their surroundings by heating their birth clouds with powerful stellar winds, eventually exploding as supernovae.
The image incorporates data from an observing program designed to catalog roughly 50,000 H II regions in nearby star-forming galaxies like NGC 4535. Hubble released a previous image of NGC 4535 in 2021. Both the 2021 image and this new image incorporate observations from the PHANGS observing program, which seeks to understand the connections between young stars and cold gas. Today’s image adds a new dimension to our understanding of NGC 4535 by capturing the brilliant red glow of the nebulae that encircle massive stars in their first few million years of life.
Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubbleMedia Contact:
Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD
Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.
Hubble Science Highlights
Hubble Images
Hubble News
Europa Clipper Captures Uranus With Star Tracker Camera
NASA/JPL-Caltech Photojournal Navigation Downloads Europa Clipper Captures Uranus With Star Tracker Camera
PNG (128.99 KB)
Description
NASA’s Europa Clipper captured this image of a starfield — and the planet Uranus — on Nov. 5, 2025, while experimenting with one of its two stellar reference units. These star-tracking cameras are used for maintaining spacecraft orientation. Within the camera’s field of view — representing 0.1% of the full sky around the spacecraft — Uranus is visible as a larger dot near the left side of the image.
Figure A is an annotated version of the image with Uranus and several background stars labeled. NASA/JPL-Caltech Figure B is an animated GIF made of a pair of images taken 10 hours apart. In this version, Uranus can be seen moving very slightly, relative to the background stars. NASA/JPL-CaltechAt the time the images were taken, Europa Clipper was about 2 billion miles (3.2 billion kilometers) from Uranus. The spacecraft is currently en route to the Jupiter system to study the icy moon Europa.
Europa Clipper launched in October 2024 and will arrive at the Jupiter system in 2030 to conduct about 50 flybys of Europa. The mission’s main science goal is to determine whether there are places below Europa’s surface that could support life. The mission’s three main science objectives are to determine the thickness of the moon’s icy shell and its surface interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission’s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet.
For more information about Europa and Europa Clipper, go to: https://science.nasa.gov/mission/europa-clipper/
Keep Exploring Discover More Topics From Photojournal
Photojournal
Search Photojournal
Photojournal’s Latest Content
Feedback
NASA’s Quesst Mission Marks X-59’s Historic First Flight
NASA’s X-59 quiet supersonic research aircraft took off for its historic first flight on Oct. 28, 2025, at 11:14 a.m. EDT from Lockheed Martin Skunk Works in Palmdale, California. The one-of-a-kind aircraft flew for 67 minutes before landing and taxiing to NASA’s Armstrong Flight Research Center in Edwards, California.
NASA test pilot Nils Larson flew the X-59 up to an altitude of about 12,000 feet and an approximate top speed of 230 mph, precisely as planned. The plane’s landing gear remained down during the entire flight, a common practice for experimental aircraft flying for the first time.
Now that the X-59’s first flight is in the books, the team is focused on preparing for a series of test flights where the aircraft will operate at higher altitudes and supersonic speeds. This test flight phase of NASA’s Quesst mission will ensure the X-59 meets performance and safety expectations.
Through the Quesst mission, NASA aims to usher in a new age of quiet supersonic flight, achieved through the unique design and technology of the X-59 in future supersonic transport aircraft.
Image Credit: NASA/Lori Losey
NASA’s Scott Tingle to Serve as Agency’s Chief Astronaut
NASA named astronaut Scott Tingle as chief of the Astronaut Office at the agency’s Johnson Space Center in Houston, effective Nov. 10. A decorated spaceflight veteran and former captain in the United States Navy, Tingle has logged more than 4,500 flight hours in 51 different aircraft and served as a flight engineer aboard the International Space Station.
As chief astronaut, Tingle is responsible for managing astronaut resources and operations. He also will help develop astronaut flight crew operations and make crew assignments for future human spaceflight missions, including Artemis missions to the Moon.
“Our Johnson Space Center team congratulates Scott on his selection as chief of the Astronaut Office. We wish him well as he takes on this new and exciting leadership role,” said Johnson Space Center Director Vanessa Wyche. “I extend my sincerest thanks to Joe Acaba, for his dedicated service to the Astronaut Office, as he completed the tremendous task of preparing our astronaut corps for daring missions to and from the International Space Station and integrated their expertise and space knowledge to develop and test future technologies, software, and procedures making space travel safer and more attainable for our nation’s explorers.”
A native of Randolph, Massachusetts, Tingle was selected as a NASA astronaut in 2009. He holds a bachelor’s degree in mechanical engineering from Southeastern Massachusetts University and a master’s degree in mechanical engineering from Purdue University in West Lafayette, Indiana.
Tingle most recently served as a flight engineer aboard the space station, spending more than six months in orbit during Expedition 54/55. He was the flight engineer and United States Operational Segment lead for the mission, which launched from the Baikonur Cosmodrome aboard a Soyuz spacecraft on Dec. 17, 2017, and concluded with landing on June 3, 2018. Since returning to Earth, he has supported the Astronaut Office in various roles, including mission support, technical leadership, and crew readiness activities.
Before coming to NASA, Tingle worked for The Aerospace Corporation in El Segundo, California, where he served as a technical staff member supporting the company’s propulsion department. He was commissioned as a naval officer in 1991 and went on to complete a distinguished career, earning the rank of captain before retiring. Follow Tingle on X.
Tingle succeeds NASA astronaut Joe Acaba, who had served as chief of the Astronaut Office since February 2023. Acaba has transitioned to the center director’s staff, where he provides technical advice on mission planning and strategy at NASA Johnson. In this new role, he leads the center’s alignment with NASA’s strategic plan and human spaceflight priorities, supports the agency’s STEM workforce goals, and advances collaboration with commercial space, academia, and other government partners as NASA continues its exploration beyond low Earth orbit.
Learn more about the International Space Station:
https://www.nasa.gov/international-space-station
-end-
Shaneequa Vereen
Johnson Space Center, Houston
281-483-5111
shaneequa.y.vereen@nasa.gov
NASA Celebrates Five Years of Artemis Accords, Welcomes 3 New Nations
October marked the fifth anniversary of NASA and the original founders signing the Artemis Accords, as well as the recognition of Hungary, Malaysia and the Philippines joining the expanding coalition dedicated to the peaceful exploration of space. The number of countries involved now totals 59.
“NASA welcomes the newest signatories, whose participation strengthens the global commitment to responsible exploration,” said acting NASA Administrator Sean Duffy. “Their decision to sign the Artemis Accords affirms a shared commitment to safe, transparent, and peaceful exploration — at a time when others seek to weaponize the final frontier. Together we are building the foundation for the Golden Age of space exploration.”
Both Malaysia and the Philippines signed the Artemis Accords as part of President Trump’s visit to Kuala Lumpur for the annual Association of Southeast Asian Nations Summit. The separate signings were announced by the White House on Oct. 26.
Foreign Minister Péter Szijjártó of Hungary signed the Artemis Accords on Oct. 22 while in Washington during an official visit, in the lead up to President Trump’s meeting with Prime Minister Viktor Orbán.
Hungary’s signing came three months after Hungarian to Orbit (HUNOR) astronaut Tibor Kapu launched to space in a mission aboard a SpaceX Dragon spacecraft to the International Space Station. The private astronauts, part of the NASA-supported Axiom Mission 4 crew, spent about two weeks conducting science, outreach, and commercial activities, alongside NASA astronauts.
Five years of progress
On Oct. 13, 2020, during the first Trump Administration, the United States, led by NASA and the U.S. Department of State, joined with seven other founding nations to establish the Artemis Accords, responding to the growing interest in lunar activities by both governments and private companies.
Since then, the Artemis Accords have grown into an international coalition. What began with a handful of founding nations has multiplied with seven countries signing in 2025 alone. The surge in participation highlights an increased global commitment to shaping a safe, peaceful, and prosperous future in space.
In September, NASA co-chaired the Artemis Accords Principals’ Meeting in Sydney alongside the space agencies of Australia and the United Arab Emirates. The gathering brought together dozens of signatory nations to deepen dialogue and strengthen shared commitments to the sustainable and responsible use of space. Global space leaders discussed the following topics:
- Non-interference in each other’s space activities, including transparency on expected launch dates, general nature of activities, and landing location
- Orbital debris mitigation
- Interoperability of systems for safer and more efficient operations
- Release of scientific data
At the meeting, NASA committed to hosting an Artemis Accords workshop in 2026 for signatories focused on transparency and the sharing of data. The agency has taken additional steps since the accords were established to release more information about lunar missions, promoting openness and preventing harmful interference.
The progress made by signatories, and their continued commitment to implementing the accords’ principles, is essential to advancing sustainable exploration of the Moon under the Artemis campaign, Mars, and beyond. Following a call to Artemis Accords signatories, four CubeSats from South Korea, Saudi Arabia, Argentina, and Germany, will fly on Artemis II.
More nations are expected to sign the accords in the months and years ahead, as NASA and its partners continue to advance the principles of the accords.
Learn more about the Artemis Accords at:
https://www.nasa.gov/artemis-accords
Share Details Last Updated Nov 20, 2025 LocationNASA Headquarters Related TermsNASA Sets Coverage for Crew Launch to Join Station Expedition
NASA astronaut Chris Williams will launch aboard the Roscosmos Soyuz MS-28 spacecraft to the International Space Station on Thursday, Nov. 27, accompanied by cosmonauts Sergey Kud-Sverchkov and Sergei Mikaev, where they will join the Expedition 73 crew advancing scientific research.
Williams, Kud-Sverchkov, and Mikaev will lift off at 4:27 a.m. EST (2:27 p.m. Baikonur time) from the Baikonur Cosmodrome in Kazakhstan. Live launch and docking coverage will be available on NASA+, Amazon Prime, and the agency’s YouTube channel. Learn how to watch NASA content through a variety of platforms, including social media.
After a two-orbit, three-hour trip to the orbital complex, the spacecraft will automatically dock to the station’s Rassvet module at approximately 7:38 a.m. Shortly after, hatches will open between Soyuz and the space station.
Once aboard, the trio will join NASA astronauts Mike Fincke, Zena Cardman, and Jonny Kim, JAXA (Japan Aerospace Exploration Agency) astronaut Kimiya Yui, and Roscosmos cosmonauts Sergei Ryzhikov, Alexey Zubritsky, and Oleg Platonov.
NASA’s coverage is as follows (all times Eastern and subject to change based on real-time operations):
Thursday, Nov. 27
3:30 a.m. – Launch coverage begins on NASA+, Amazon Prime, and YouTube.
4:27 a.m. – Launch
6:45 a.m. – Rendezvous and docking coverage begins on NASA+, Amazon Prime, and YouTube.
7:38 a.m. – Docking to the space station
9:50 a.m. – Hatch opening and welcome remarks coverage begins on NASA+, Amazon Prime, and YouTube.
10:10 a.m. – Hatch opening
Williams, Kud-Sverchkov, and Mikaev will spend approximately eight months aboard the space station as Expedition 73/74 crew members, before returning to Earth in summer 2026. This will be the first spaceflight for Williams and Mikaev, and the second for Kud-Sverchkov.
During his stay aboard station, Williams will conduct scientific research and technology demonstrations aimed at advancing human space exploration and benefiting life on Earth. He will help install and test a new modular workout system for long-duration missions, support experiments to improve cryogenic fuel efficiency and grow semiconductor crystals in space, and assist NASA in designing new re-entry safety protocols to protect crews during future missions.
For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs that are not possible on Earth. The station is a critical testbed for NASA to understand and overcome the challenges of long-duration spaceflight and to expand commercial opportunities in low Earth orbit. As commercial companies concentrate on providing human space transportation services and destinations as part of a robust low Earth orbit economy, NASA is focusing its resources on deep space missions to the Moon as part of the Artemis campaign in preparation for future human missions to Mars.
Learn more about International Space Station research and operations at:
-end-
Joshua Finch / Jimi Russell
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / james.j.russell@nasa.gov
Sandra Jones / Joseph Zakrzewski
Johnson Space Center, Houston
281-483-5111
sandra.p.jones@nasa.gov / joseph.a.zakrzewski@nasa.gov
What’s Up: November 2025 Skywatching Tips from NASA
Mars and Mercury get close for a conjunction, the Leonid meteor shower delights, and Saturn’s rings are…disappearing?
Skywatching Highlights- Nov. 12: A conjunction between Mars and Mercury
- Nov. 16-18: Leonid meteor shower peak viewing
- Nov. 23: Saturn’s rings disappear
Mars and Mercury have a cozy conjunction, the Leonid meteor shower delights, and Saturn’s rings are…disappearing?
That’s What’s Up for November.
Conjunction:Mars and Mercury will cozy up together in the night sky just after sunset on November 12th.
The planets will experience what is known as a conjunction, meaning they appear close together in the sky from our view (even though in real life, Mars and Mercury are well over 100 million miles apart).
But you can see these two long distance pals close together if you look slightly southwest just after sunset in the early evening sky on November 12th.
NASA/JPL-CaltechMars will be just to the right above Mercury, and you’ll know it’s Mars by its distinctive reddish-orange color.
Leonid Meteor Shower:The Leonid meteor shower will sparkle across the skies this month, peaking on November 17th.
NASA/JPL-CaltechWhile the meteor shower stretches from November 3rd through December 2nd, it will be at its most visible late on the night of November 16th into the dawn of November 17th, even into the early morning of November 18th.
Look for meteors coming from the shower’s radiant point within the constellation Leo in the eastern sky.
With dark skies, you might see 10-15 meteors per hour with this shower which happens when we travel through the debris trailing the comet 55P/Tempel-Tuttle.
Saturn’s rings disappearSaturn’s rings will disappear from view this November!
Saturn orbits the sun leaning at an angle of 26.7 degrees. This means that from our view, its rings shift up and down over time.
On November 23, Saturn will be angled in such a way that its rings face us, and since they are so thin they’ll just disappear from view.
Alan Friedman/avertedimagination.comBut don’t worry, the rings aren’t gone from view forever. As the planet continues to orbit, its rings will gradually become more visible again.
Conclusion + Moon PhasesHere are the phases of the Moon for November.
NASA/JPL-CaltechYou can stay up to date on all of NASA’s missions exploring the solar system and beyond at science.nasa.gov.
I’m Chelsea Gohd from NASA’s Jet Propulsion Laboratory, and that’s What’s Up for this month.
Keep Exploring Discover More Topics From NASA
What’s Up
Skywatching
Galaxies
Stars
NASA Fuels Discovery from Earth to Sky: One Crayon at a Time
6 min read
NASA Fuels Discovery from Earth to Sky: One Crayon at a Time Student interns help kids color in data to learn more about the far side of the Moon while visiting the Goddard Space Flight Center Visitor Center. Photo Credit: NASA Earth to SkyA collaboration between the NASA Earth Science Education Collaborative (NESEC) and Earth to Sky (ETS) – an exciting, growing partnership between NASA, the National Park Service, and other federal, state, and local organizations – is facilitating the implementation of a simple, yet incredibly effective activity that will help millions of national park visitors connect with NASA Earth and space science.
The Color-a-Pixel activity, developed by NESEC, transforms complex satellite imagery into accessible, collaborative art projects. Incorporating this simple technique into ETS science communication training programs demonstrates to park interpreters and outdoor educators how NASA’s view from space can enhance millions of visitor experiences at parks, refuges, and nature centers.
“This low-tech activity is powerful because of its simplicity,” explains ETS Space Science Coordinator Brandi Stewart, “All you have to do is pick up a crayon, follow the easy number guides, and discover the stories that NASA satellites are telling us about our world and beyond.”
The Color-a-Pixel activity begins with selecting satellite imagery from NASA missions like Landsat, the Mars Reconnaissance Orbiter (MRO), or the Lunar Reconnaissance Orbiter (LRO). Using technology developed by NESEC’s lead organization, the Institute for Global Environmental Strategies, these images are converted into a 3’ by 2’ poster of numbered squares, each corresponding to one of 120 standard Crayola crayon colors.
Earth to Sky demonstrates the magnetic appeal of this activity by setting it up for the rangers and educators during workshops. With a bit of explanation, participants immediately jump in, eager to reveal the imagery and data shown through the pixels.
“It becomes a group mission that, by the end of the training, the image will be fully colored in and complete. It’s been a great teambuilding and stress-relieving activity for our participants,” states Geneviève de Messières, Earth to Sky Program Lead.
When applied to public lands communication efforts, this activity becomes a tool for interpretive messaging. While visitors work on completing the image, park rangers can weave in scientific concepts, environmental change stories, and space exploration connections. This activity also drives home that satellite imagery is more than just a pretty picture – each pixel is also data that scientists use to better understand Earth and other worlds throughout our solar system.
Bringing Space Down to EarthSome ways that Earth to Sky has implemented the activity at special events on public lands include:
- Death Valley Dark Sky Festival, California: Visitors were invited to color Landsat imagery of Earth’s Badwater Basin and MRO imagery of Mars’ Belva Crater. As they colored, Earth to Sky outreach specialists made connections between finding signs of water on the dry landscapes in both locations.
- Park After Dark, Minnesota: During this urban event hosted by Mississippi River & National Recreation Area in Minneapolis St. Paul, attendees worked together to color topographical maps of both the Moon’s familiar near side and its mysterious far side, using data from NASA’s Lunar Reconnaissance Orbiter. The striking differences that emerged through their coloring sparked questions about why the Moon’s two hemispheres appear so dramatically different, leading to rich discussions about lunar formation and geological change.
- Patuxent Wildlife Refuge Open House, Maryland: Just miles from the urban centers of Baltimore and Washington DC, the Color-a-Pixel activity helped local community members visualize something they could feel but not easily see: the refuge’s role as a “cool island” in an urban heat landscape. Visitors colored Landsat imagery of the refuge and surrounding neighborhoods while examining heat maps showing temperature differences between developed areas and the protected green space. The activity helped residents understand the refuge’s importance beyond wildlife habitat.
All of these activities are available on the Institute for Global Environmental Strategies (IGES) website in a pre-generated format ready for printing.
A Colorful CollaborationThe collaboration between NESEC and Earth to Sky brings complex scientific concepts to diverse audiences in engaging and relevant ways. Earth to Sky’s community of practice –now including more than 2,000 interpreters and environmental educators – reaches millions of visitors annually across the country’s parks, refuges, and nature centers.
Theresa Schwerin, who leads NESEC, noted that Color-a-Pixel originally started as a simple idea for a tabletop activity to use at conferences and public events. “I wanted something hands-on that could draw people in and start conversations as simple as ‘these beautiful NASA images from space are data’ and talk about different NASA missions and how they are relevant to people’s lives. There’s also an opportunity to invite the public to contribute to NASA science by participating in citizen science projects … [some of which] can fill in the details of the pixels with information that complements NASA’s view from space.”
Andrew Clark, a data scientist and engineer at IGES, created the Color-a-Pixel poster generator, which has gone through several iterations to make it more effective. Schwerin noted, “I’ve used this at several public events. Kids will jump right in, with parents watching over their shoulders. Soon enough, the entire family is coloring together and asking questions about the image and NASA. I am thrilled about our collaboration with Earth to Sky that is taking this even further.”
As environmental challenges increasingly affect public lands, this collaboration helps visitors understand these issues through NASA’s unique perspective from above. The activity also introduces learners of all ages to the broader value of NASA’s Earth science missions alongside its more well-known space exploration endeavors.
Continuing to Color Outside the LinesLooking ahead, the Earth to Sky partnership plans to continue using this activity in each new place they host a training. Most recently, Earth to Sky shared the activity with 417 visitors to the Goddard Space Flight Center Visitor Center, where local families colored in topographical Moon maps to prepare for International Observe the Moon Night. Additionally, a recording of a recent Color-a-Pixel webinar with NESEC’s Theresa Schwerin is available on the Earth to Sky website for interpreters and informal educators interested in implementing this place-based activity. Free registration is required to access this (and dozens of other) webinar recordings.
The success of this collaboration demonstrates how seemingly simple activities – enhanced with NASA science – can create meaningful learning experiences that resonate with visitors long after they leave a park or refuge.
For interpreters, educators, or NASA enthusiasts interested in bringing the Color-a-Pixel activity to their own sites or events, pre-generated activities are available in the gallery at: https://strategies.org/color-a-pixel-pregenerated.
NASA science is helping humanity discover new perspectives on both our home planet and the universe beyond, one crayon at a time. 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/.
Share Details Last Updated Nov 20, 2025 Editor NASA Science Editorial Team Related Terms Explore More 5 min read Helio Highlights: October 2025Since we all have a relationship with the Sun, it is important to learn about…
Article
2 months ago
4 min read From City Lights to Moonlight: NASA Training Shows How Urban Parks Can Connect Communities with Space Science
Article
2 months ago
3 min read NASA Helps Connect Astronomers and Community Colleges Across the Nation
Article
2 months 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…
NASA Progresses Toward Artemis II Moon Mission
As 2026 nears, NASA continues moving forward to launching and flying Artemis II, the first crewed mission under the Artemis campaign, no later than April next year.
NASA’s Orion spacecraft, complete with its launch abort system escape tower, is now integrated with the SLS (Space Launch System) rocket in the Vehicle Assembly Building (VAB) at the agency’s Kennedy Space Center in Florida. Following Orion stacking, teams completed testing critical communications systems between SLS and Orion, and confirmed the interfaces function properly between the rocket, Orion, and the ground systems, including end-to-end testing with the Near Space Network and Deep Space Network, which aid in communications and navigation.
“NASA remains focused on getting ready to safely fly four astronauts around the Moon and back,” said acting NASA Administrator Sean Duffy. “Our mission will lay the groundwork for future missions to the lunar surface and to Mars.”
In the coming weeks, engineers and the Artemis II crew will conduct the first part of a Countdown Demonstration Test at Kennedy, a dress rehearsal for launch day. The crew will don their Orion crew survival system spacesuits and venture to their rocket before being secured inside Orion, which the crew recently named Integrity, simulating the final moments of the countdown. Because the rocket and spacecraft are not yet at the launch pad, the crew will board Orion inside the VAB. The test will serve as a final verification of the timeline for the crew and supporting teams on the ground. A second part of the test, preparing for an emergency at the launch pad, will occur after the rocket and spacecraft roll out to Launch Pad 39B.
NASA astronaut Christina Koch, Artemis II mission specialist, and the remaining Artemis II crew members walk on the crew access arm of the mobile launcher in the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida on Tuesday, Aug. 12, 2025. NASA/Kim ShiflettThe Artemis II crew and ground personnel responsible for launching and flying the mission are preparing to conduct additional integrated simulations across teams and facilities to prepare for any scenario that could arise as the crew of four launches from Florida and flies their approximately 10-day mission.
NASA astronauts Reid Wiseman, Victor Glover, and Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen, have a busy schedule over the next several months reviewing procedures for all phases of flight until their preparations are second nature, practicing for different mission scenarios, and maintaining their familiarity with every element of their spacecraft.
Through Artemis, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and build the foundation for the first crewed missions to Mars.
NASANASA’s Quesst Mission Marks X-59’s Historic First Flight
NASA’s X-59 quiet supersonic research aircraft took off for its historic first flight on Oct. 28 at 11:14 a.m. EDT from Lockheed Martin Skunk Works in Palmdale, California. The one-of-a-kind aircraft flew for 67 minutes before landing and taxiing to NASA’s Armstrong Flight Research Center in Edwards, California.
NASA test pilot Nils Larson flew the X-59 up to an altitude of about 12,000 feet and an approximate top speed of 230 mph, precisely as planned. The plane’s landing gear remained down during the entire flight, a common practice for experimental aircraft flying for the first time.
Now that the X-59’s first flight is in the books, the team is focused on preparing for a series of test flights where the aircraft will operate at higher altitudes and supersonic speeds. This test flight phase of NASA’s Quesst mission will ensure the X-59 meets performance and safety expectations.
Through the Quesst mission, NASA aims to usher in a new age of quiet supersonic flight, achieved through the unique design and technology of the X-59 in future supersonic transport aircraft.
Share Details Last Updated Nov 20, 2025 EditorMaria WerriesContactKristen Hatfieldkristen.m.hatfield@nasa.gov Related Terms Explore More 1 min read X-59 First Flight Media Resources Article 7 hours ago 5 min read NASA’s X-59 Completes First Flight, Prepares for More Flight Testing Article 1 day ago 3 min read NASA, Industry Weave Data Fabric with Artificial IntelligenceAir taxis and drones navigate different flight zones with NASA-inspired system
Article 3 days ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
Aeronautics
QuesstQuesst is NASA's mission to demonstrate how the X-59 can fly supersonic without generating loud sonic booms and then survey…
Integrated Aviation Systems Program
NASA, Aerospace Corporation Study Sharpens Focus on Ammonia Emissions
6 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Researchers used data taken in March 2023 by an airborne imaging spectrometer to map ammonia emissions in the Imperial Valley. Produced by agricultural activities as well as geothermal processes, ammonia is a precursor to particulate matter, which can cause adverse health outcomes when inhaled.NASA/JPL-CaltechThe pungent gas contributes to fine airborne particulate pollution, which endangers human health when inhaled and absorbed in the bloodstream.
A recent study led by scientists at NASA’s Jet Propulsion Laboratory in Southern California and the nonprofit Aerospace Corporation shows how high-resolution maps of ground-level ammonia plumes can be generated with airborne sensors, highlighting a way to better track the gas. A key chemical ingredient of fine particulate matter — tiny particles in the air known to be harmful when inhaled — ammonia can be released through agricultural activities such as livestock farming and geothermal power generation as well as natural geothermal processes. Because it’s not systematically monitored, many sources of the pungent gas go undetected.
Published in Atmospheric Chemistry and Physics in October, the study focuses on a series of 2023 research flights that covered the Imperial Valley to the southeast of the Salton Sea in inland Southern California, as well as the Eastern Coachella Valley to its northwest. Prior satellite-based research has identified the Imperial Valley as a prolific source of gaseous ammonia. In the study, scientists employed an airborne sensor capable of resolving ammonia plumes with enough detail to track their origins: Aerospace Corporation’s Mako instrument is an imaging spectrometer that observes long-wave infrared light emitted by areas of Earth’s surface and atmosphere 6 feet (2 meters) across.
Using the instrument, which can detect ammonia’s chemical signature by the infrared light it absorbs, the authors found elevated levels of the gas near several sources, including agricultural fields, livestock feedlots, geothermal plants, and geothermal vents. Measurements in parts of the Imperial Valley were 2½ to eight times higher than in Coachella Valley’s Mecca community, which had ammonia concentrations closer to background levels.
Though not toxic on its own in low concentrations, ammonia is a precursor to particulate matter, also known as aerosol or particle pollution. It reacts with other gases to form solid ammonium salt particles small enough to penetrate the bloodstream from the lungs. Particles under 2.5 micrometers in diameter — also known as PM2.5 — are associated with elevated rates of asthma, lung cancer, and cardiovascular disease, among other negative health outcomes.
“Historically, more attention has focused on primary sources of PM2.5, such as auto emissions. But with significant reductions in those emissions and increasingly stringent air quality standards, there is growing interest in understanding secondary sources that form particles in the air from precursor gases,” said Sina Hasheminassab, lead author of the paper and a research scientist at JPL. “As an important precursor to PM2.5, ammonia plays a key role, but its emissions are poorly characterized and undermonitored.”
Rising ammonia
Previous satellite-based studies have shown rising levels of atmospheric ammonia, both globally and in the continental United States. That research revealed broad trends, but with spatial resolution on the order of tens of miles, the measurements were only sufficient to identify variation over areas of hundreds of square miles or more.
The chemical behavior of ammonia also poses a particular monitoring challenge: Once emitted, it only stays in the atmosphere for hours before reacting with other compounds. In contrast, carbon dioxide can remain in the air for centuries.
Planes and satellites can provide an overview of sources and the geographic distribution of emissions at a given moment. Although satellites offer wider and more recurrent coverage, airborne instruments, being closer to the source, produce higher-resolution data and can focus on specific locations at designated times.
Those proved to be the right capabilities for the recent study. Researchers flew Mako over the Imperial and Eastern Coachella valleys on the mornings and afternoons of March 28 and Sept. 25, 2023, and took concurrent measurements on the ground with both a fixed monitoring station in Mecca operated by the South Coast Air Quality Management District (AQMD) and a mobile spectrometer developed at the University of California, Riverside.
“The goal was to show that this technique was capable of delivering data with the required accuracy that aerosol scientists and potentially even air quality regulatory bodies could use to improve the air quality in those regions,” said David Tratt, a senior scientist at Aerospace Corporation and coauthor of the paper. “We ended up with maps that identify multiple sources of ammonia, and we were able to track the plumes from their sources and observe them coalescing into larger clouds.”
Distinct plumes
During the flights, the team collected data over the southeastern coast of the Salton Sea, which straddles Riverside and Imperial counties. There, Mako revealed small plumes coming from geothermal fumaroles venting superheated water and steam that react with nitrogen-bearing compounds in the soil, releasing ammonia.
Farther to the southeast, the results showed several geothermal power plants emitting ammonia, primarily from their cooling towers, as part of their normal operations.
Farther southeast still, the researchers spotted ammonia emissions, a byproduct of animal waste, from cattle farms in the Imperial Valley. During the March 28 flight, a plume from the largest facility in the study area measured up to 1.7 miles (2.8 kilometers) wide and extended up to 4.8 miles (7.7 kilometers) downwind of the source.
‘Very large puzzle’
As part of the study, AQMD’s Mecca monitoring station recorded seasonal changes in ammonia concentrations. Given the few sources in the area, the researchers surmised that winds during certain months tend to blow the gas from Imperial Valley to the Coachella Valley.
The study underscores the benefits of detailed spatial information about ammonia emissions, and it partly informed the agency’s decision in July to expand its ammonia-monitoring network and extend the life of the Mecca station.
As a precursor to PM2.5, ammonia is “one piece of a very large puzzle” that, for Coachella Valley residents, includes vehicle emissions, desert dust, and agricultural activities, said Payam Pakbin, manager of the Advanced Monitoring Technologies Unit at AQMD and a paper coauthor.
“These communities want to know the contributions of these sources to the air quality they’re experiencing,” he added. “Findings like these help our agency better prioritize which sources require the most attention and ultimately guide our focus toward those that are the highest priority for achieving emission reductions in this community.”
NASA Studies Wildflowers From the Air NASA Maps Critical Minerals With High-Altitude Aircraft NASA Helps Spot Wine Grape Disease From the SkiesNews Media Contacts
Andrew Wang / Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
626-379-6874 / 626-840-4291
andrew.wang@jpl.nasa.gov / andrew.c.good@jpl.nasa.gov
2025-129
Share Details Last Updated Nov 20, 2025 Related Terms Explore More 2 min read SARP 2025 Closeout Article 1 day ago 9 min read SARP East 2025 Atmospheric Chemistry Group Article 1 day ago 10 min read SARP East 2025 Terrestrial Fluxes Group Article 1 day ago Keep Exploring Discover Related Topics Explore Earth ScienceFrom its origins, NASA has studied our planet in novel ways, using a fleet of satellites and ambitious airborne and ground-based…
Earth Science at WorkNASA Earth Science helps Americans respond to challenges and societal needs — such as wildland fires, hurricanes, and water supplies…
Earth Science Data
Earth Science MissionsIn order to study the Earth as a whole system and understand how it is changing, NASA develops and supports…
Celebrating 25 Years of Humanity in Space
In 2025, NASA and its international partners celebrate 25 years of continuous human presence aboard the International Space Station. Since November 2, 2000, more than 290 people from 26 countries have lived and worked aboard the orbiting laboratory, conducting thousands of experiments that have advanced science and technology on Earth and paved the way for Artemis missions to the Moon and future journeys to Mars.
Beyond its role as a science platform, the station has been a bridge—connecting cultures, sparking creativity, and inspiring generations. The memories of Johnson Space Center employees reflect how the orbiting laboratory is not only an engineering marvel but also a deeply human endeavor.
Christopher Brown – Advancing Life Support Systems for Future Exploration
Christopher Brown (center) receives the Rotary National Award for Space Achievement alongside NASA astronaut Sunita Williams. NASA/James BlairAs a space station Environmental Control and Life Support System (ECLSS) integrator, Christopher Brown’s role has been ensuring astronauts have clean air and water. ECLSS removes carbon dioxide from the air, supplies oxygen for breathing, and recycles wastewater—turning yesterday’s coffee into tomorrow’s coffee. Today, these systems can recover nearly 98% of the water brought to the station.
His proudest memory was commissioning regenerative life support systems and raising a symbolic toast with the crew while on console in mission control. He also helped activate the Water Storage System, saving crew time and improving operations on station. For Brown, these milestones were vital steps toward future long-duration missions beyond Earth.
Stephanie Sipila – The Heart of Microgravity Research
NASA astronaut Kate Rubins works on the Cardinal Heart study, which seeks to help scientists understand the aging and weakening of heart muscles in the search for new treatments for astronauts and people on Earth. NASA/Mike HopkinsStephanie Sipila, now integration manager for NASA’s Extravehicular Activity and Human Surface Mobility Program, began her career as a mechanical and robotic systems instructor for the orbital outpost. Her favorite experiment, Engineered Heart Tissues, studies microgravity’s effect on the human heart to help develop new treatments for cardiovascular disease. She recalls NASA astronaut Sunita Williams running the Boston Marathon on a treadmill aboard station, becoming the first person to complete the race in space and showing how astronauts stay connected to Earth while living on orbit.
Sipila also highlights the Spacesuit Art Project, an initiative that turned artwork from children with cancer into spacesuits flown to and worn aboard the orbital outpost during live downlinks, connecting science, art, and hope — and raising awareness of cancer research conducted aboard the orbital outpost.
Liz Warren – Where Exploration Meets Humanity
NASA astronaut Jack Fischer wearing the Unity spacesuit painted by patients at MD Anderson Cancer Center in Houston. NASA/Randy BresnikSpace station Associate Chief Scientist Liz Warren has seen firsthand how the Spacesuit Art Project uplifted children on Earth. During Expedition 52, she watched astronaut Jack Fischer wear a suit covered in artwork created by young cancer patients, including his own daughter, a survivor. “It was incredibly touching to note the power of art and inspiration. Human spaceflight requires fortitude, resilience, and teamwork—so does fighting childhood cancer,” Warren said.
Her memories also extend to her time as an operations lead for NASA’s Human Research Program, which uses research to develop methods to protect the health and performance of astronauts in space to prepare for long-duration missions. While out for a weekend run, Warren received a call from the Payload Operations and Integration Center in Huntsville, Alabama. An astronaut on station, following a prescribed diet for a research study, wanted to swap out a food item. Warren coordinated with her support team and relayed the decision back to orbit—all while continuing her run. The moment, she recalls, underscored the constant, real-time connection between astronauts in space and teams on the ground.
Adam Baker – Checkmate: Space Debris Cleanup
Flight Director Chris Edelen, left, and capsule communicator Jay Marschke discuss their next chess move during a match with NASA astronaut Greg Chamitoff, Expedition 17 flight engineer aboard the space station.NASA/Robert MarkowitzAs an aerospace engineer, Adam Baker helped track experiments and spacecraft operations from mission control. Baker remembers when mission control played a live chess match with astronaut Greg Chamitoff during Expedition 17, a moment that showed the unique ways the station connects crews in orbit with people on Earth. His favorite technical project, though, was the RemoveDebris small satellite, deployed from the station in 2018 to test technologies for cleaning up space junk. “Knowing these experiments could one day help keep the orbital environment safe made it even more meaningful,” he said.
Michael McFarlane – Training for Success
Engineers run simulations inside Johnson’s Systems Engineering Simulator during a shuttle-to-station docking simulation.Smiley Pool/Houston ChronicleAs chief of the Simulation and Graphics Branch, Michael McFarlane prepared astronauts for space station assembly missions using high-fidelity simulators. “My greatest memory is seeing the station grow as we successfully executed assembly missions that looked very much like what we analyzed and trained for in our ground-based simulations,” he said.
A Legacy of Ingenuity and Community
Date: 10-31-2023 Location: Bldg 30 MCC, ISS MER Subject: Mission Evaluation Room (MER) Halloween Celebration “MERloween” Photographer: James BlairNASA/James BlairIn the Mission Evaluation Room, engineers not only troubleshoot in real time but also celebrate milestones with traditions like “MERloween,” where controllers dress in space-themed costumes to honor the year’s lessons learned.
NASA’s SpaceX Dragon Freedom spacecraft splashed down in the Gulf of America, off the coast of Tallahassee, Florida, returning Crew-9 to Earth on March 18, 2025. NASA/Keegan BarberFor social media consultant Mark Garcia, sharing the station story with the public has been the highlight of his career. His favorite moment was watching NASA’s SpaceX Crew-9 splash down in 2025, greeted by dolphins in the Gulf of America. “I love writing about the science aboard the station that benefits people on Earth,” he said.
For 25 years, the International Space Station has shown what humanity can accomplish together. The lessons learned aboard will guide Artemis missions to the Moon and future journeys to Mars—ensuring the next 25 years are built on innovation, resilience, and the human spirit.
NASA’s X-59 Completes First Flight, Prepares for More Flight Testing
5 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)After years of design, development, and testing, NASA’s X-59 quiet supersonic research aircraft took to the skies for the first time Oct. 28, marking a historic moment for the field of aeronautics research and the agency’s Quesst mission.
The X-59, designed to fly at supersonic speeds and reduce the sound of loud sonic booms to quieter sonic thumps, took off at 11:14 a.m. EDT and flew for 67 minutes. The flight represents a major step toward quiet supersonic flight over land.
“Once again, NASA and America are leading the way for the future of flight,” said acting NASA Administrator Sean Duffy. “The X-59 is the first of its kind, and a major breakthrough in America’s push toward commercial air travel that’s both quiet and faster than ever before. Thanks to the X-59 team’s innovation and hard work, we’re revolutionizing air travel. This machine is a prime example of the kind of ingenuity and dedication America produces.”
Following a short taxi from contractor Lockheed Martin’s Skunk Works facility, NASA X-59 test pilot Nils Larson approached U.S. Air Force Plant 42’s runway in Palmdale, California, where he completed final system checks and called the tower for clearance.
NASA’s X-59 quiet supersonic research aircraft cruises above Palmdale and Edwards, California, during its first flight, Tuesday, Oct. 28, 2025. The aircraft traveled to NASA’s Armstrong Flight Research Center in Edwards, California.NASA/Lori LoseyThen, with a deep breath, steady hands, and confidence in the labor of the X-59’s team, Larson advanced his throttle, picking up speed and beginning his climb – joining the few who have taken off in an experimental aircraft for the first time.
“All the training, all the planning that you’ve done prepares you,” Larson said. “And there is a time when you realize the weight of the moment. But then the mission takes over. The checklist starts. And it’s almost like you don’t even realize until it’s all over – it’s done.”
The X-59’s first flight went as planned, with the aircraft operating slower than the speed of sound at 230 mph and a maximum altitude of about 12,000 feet, conditions that allowed the team to conduct in-flight system and performance checks. As is typical for an experimental aircraft’s first flight, landing gear was kept down the entire time while the team focused on ensuring the aircraft’s airworthiness and safety.
The aircraft traveled north to Edwards Air Force Base, circled before landing, and taxied to its new home at NASA’s Armstrong Flight Research Center in Edwards, California, officially marking the transition from ground testing to flight operations.
“In this industry, there’s nothing like a first flight,” said Brad Flick, center director of NASA Armstrong. “But there’s no recipe for how to fly an X-plane. You’ve got to figure it out, and adapt, and do the right thing, and make the right decisions.”
NASA’s X-59 quiet supersonic research aircraft flies above Palmdale and Edwards, California, on its first flight Tuesday, Oct. 28, 2025. The aircraft traveled to NASA’s Armstrong Flight Research Center in Edwards, California, where it will begin flight testing for NASA’s Quesst mission, which aims to demonstrate quiet supersonic flight over land.NASA/Jim RossHistoric flight
The X-59 is the centerpiece of NASA’s Quesst mission and its first flight connects with the agency’s roots of flying bold, experimental aircraft.
“The X-59 is the first major, piloted X-plane NASA has built and flown in over 20 years – a unique, purpose-built aircraft,” said Bob Pearce, NASA associate administrator for the Aeronautics Research Mission Directorate. “This aircraft represents a validation of what NASA Aeronautics exists to do, which is to envision the future of flight and deliver it in ways that serve U.S. aviation and the public.”
NASA Armstrong has a long history of flying X-planes that pushed the edges of flight. In 1947, the X-1 broke the sound barrier. More than a decade later, the X-15 pushed speed and altitude to new extremes. Starting in the 1960s, the X-24 shaped how we understand re-entry from space, and in the 1980s the X-29 tested forward-swept wings that challenged aerodynamic limits.
Each of those aircraft helped answer a question about aeronautics. The X-59 continues that tradition with a mission focused on sound – reducing loud sonic booms to sonic thumps barely audible on the ground. The X-59 was built for one purpose: to prove that supersonic flight over land can be quiet enough for public acceptance.
NASA test pilot Nils Larson steps out of the X-59 after successfully completing the aircraft’s first flight Tuesday, Oct. 28, 2025. The mission marked a key milestone in advancing NASA’s Quesst mission to enable quiet supersonic flight over land.NASA/Genaro VavurisNext steps
Getting off the ground was only the beginning for the X-59. The team is now preparing the aircraft for full flight testing, evaluating how it will handle and, eventually, how its design will shape shock waves, which typically result in a sonic boom, in supersonic flight. The X-59 will eventually reach its target cruising speed of about 925 mph (Mach 1.4) at 55,000 feet.
The aircraft’s design sits at the center of that testing, shaping and distributing shock-wave formation. Its engine is mounted on top of the fuselage – the main body of the aircraft – to redirect air flow upward and away from the ground.
The cockpit sits mid-fuselage, with no forward-facing window. Instead, NASA developed an eXternal Vision System – cameras and advanced high-definition displays that allow the pilot to see ahead and below the aircraft, which is particularly critical during landing.
These design choices reflect years of research and modeling – all focused on changing how the quieter sonic thump from a supersonic aircraft will be perceived by people on the ground.
NASA’s goal is to gather community response data to support the development of new standards for acceptable levels of sound from commercial supersonic flight over land. To do this, NASA will fly the X-59 over different U.S. communities, collecting ground measurement data and survey input from residents to better understand people’s perception of the X-59’s sonic thump.
“Most X-planes only live in the restricted airspace here on center,” Flick said. “This one is going to go out and fly around the country.”
When the X-59 lifted off the ground for the first time, it carried a piece of NASA’s history back into the air. And with it, a reminder that advancing aeronautics remains central to NASA’s mission.
Share Details Last Updated Nov 19, 2025 EditorDede DiniusContactNicolas Cholulanicolas.h.cholula@nasa.govLocationArmstrong Flight Research Center Related Terms Explore More 41 min read 2025-2026 DWU: High School Engineering Challenge Article 2 months ago 12 min read 2025-2026 DWU: Middle School Aviation Challenge Article 2 months ago 4 min read NASA Flights Study Cosmic Ray Effects for Air, Future Space Travelers Article 2 months ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
Humans in Space
Climate Change
Solar System
SARP 2025 Closeout
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) SARP students peer into the cockpit onboard NASA’s P-3 aircraft, during research flights for the 2025 Student Airborne Research Program (SARP) internship. NASA/Milan LoiaconoIn August 2025, 47 students from NASA’s Student Airborne Research Program (SARP) culminated a summer of science by presenting their research to an audience of mentors, professors, family, friends, and NASA personnel.
SARP is a summer internship for undergraduate students, hosted in two cohorts: this year SARP West operated out of Guardian Jet Center and University of California, Irvine in Southern California, while SARP East operated out of Wallops Flight Facility and Virginia Commonwealth University in Virginia.
SARP randomly assigns students into one of four research disciplines, to encourage interdisciplinary collaboration and give them the opportunity to work outside of their usual field. Each discipline is led by a faculty researcher who is an expert in their field, and supported by a graduate mentor. This year, SARP research topics spanned three spheres: atmosphere, biosphere, and hydrosphere, covered between the two cohorts.
The beauty of Earth science lies in its interconnectedness. As a student who primarily researches atmospheric science, stepping out of my comfort zone to explore something new was truly eye-opening, and I am incredibly grateful for the experience.Nimay mahajan
2025 SARP West student
Over the course of two months, students learned more about NASA’s Airborne Science Program and Earth Science through lectures led by SARP faculty and guest speakers from NASA and the Earth science community, engaged in Earth science data collection while flying onboard Dynamic Aviation’s B-200 and NASA’s P-3 aircraft, and participated in field trips to perform ground sampling fieldwork. Students also visited NASA’s Jet Propulsion Laboratory, Goddard Space Flight Center, and NASA Headquarters. The program also includes other enriching opportunities such as visiting the University of California San Diego’s WAVElab and Virginia Commonwealth University’s Rice Rivers Center.
Students were also provided the opportunity to attend introductory programming sessions and receive hands-on support from a coding mentor to develop and strengthen their experience with code, and incorporate code in their research project.
SARP really made me realize that science is bigger than all of us, but it needs every one of us – even those just stepping into the scientific world – to contribute. Every effort, no matter how big or small, is a step forward in a mission greater than any one individual.TJ Ochoa Peterson
2025 SARP East student
To watch videos of these student’s presentations, read their research abstracts, or see more photos from the summer, please follow the links below.
2025 SARP East Research Presentations The 2025 SARP East Aerosols Group poses in front of the Dynamic Aviation B-200 aircraft, parked in a hangar at NASA’s Wallops Flight Facility in Virgina. During the internship, students spend a week engaged in Earth science data collection and learning from instruments specialists while flying onboard both the B-200 and NASA’s P-3 aircraft.NASA/Milan Loiacono Watch the Atmospheric Chemistry Group Presentations Watch the Ecohydrology Group Presentations Watch the Oceans Group Presentations Watch the Terrestrial Fluxes Group Presentations View the SARP East Photo Gallery 2025 SARP West Research Presentations The students and faculty of the 2025 Student Airborne Research Program (SARP) pose in front of NASA’s P-3 aircraft.NASA/Milan Loiacono Watch the Aerosols Group Presentations Watch the Land Group Presentations Watch the Oceans Group Presentations Watch the Whole Air Sampling (WAS) Group Presentations View the SARP West Photo Gallery About the AuthorMilan LoiaconoScience Communication SpecialistMilan Loiacono is a science communication specialist for the Earth Science Division at NASA Ames Research Center.
Share Details Last Updated Nov 19, 2025 Related Terms Keep Exploring Discover More Topics From NASAMissions
Humans in Space
Climate Change
Solar System
SARP East 2025 Atmospheric Chemistry Group
9 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The 2025 SARP East Atmospheric Chemistry Group poses in front of the Dynamic Aviation B-200 aircraft, parked in a hangar at NASA’s Wallops Flight Facility in Virginia. During the internship, students spend a week engaged in Earth science data collection and learning from instruments specialists while flying onboard both the B-200 and NASA’s P-3 aircraft.NASA/Milan Loiacono Return to 2025 SARP CloseoutFaculty Advisor:
Stacey Hughes, University of New Hampshire
Graduate Mentor:
Katherine Paredero, Georgia Institute of Technology
Atmospheric Chemistry Group Introduction Faculty Advisor Stacey Hughes and Graduate Mentor Katherine Paredero Kaylena Pham Spooky Swamps: How Methane Emission Rates and Their Spatial Variability Differ Between the Great Dismal Swamp and the Alligator RiverKaylena Pham, University of Southern California
Wetlands represent a dominant natural source of methane emissions to the atmosphere through methanogenesis, a process that produces methane in nutrient-depleted anoxic sediments, or as a result of decomposition. In coastal wetlands, particularly brackish regimes such as the Alligator River, severe storms and rising sea levels intensify saltwater intrusion inland. This leads to expansive vegetation death and the formation of ghost forests, large areas of dead standing vegetation. The widespread forest loss caused by salinization suggests elevated methane emissions in areas with vegetation stress through increased rates of decomposition from plant death. Previous research has not yet considered ghost forests when estimating methane emissions in wetlands, leading us to explore emission concentrations across two wetlands with similar vegetation compositions: the Great Dismal Swamp and Alligator River.
In this work, we utilized in-situ measurements collected aboard the Dynamic Aviation B-200 aircraft during the NASA Student Airborne Research Program (SARP) 2025 flight campaign. Methane and carbon monoxide measurements were determined using a PICARRO Gas Concentration Analyzer. This data was then linked with Normalized Difference Vegetation Index (NDVI) imagery from the Terra satellite’s Moderate Resolution Imaging Spectroradiometer (MODIS) instrument. With these two datasets, we studied how vegetation stress influences methane emissions. We observed greater vegetation stress in the Alligator River compared to the Great Dismal Swamp. Furthermore, the Alligator River has wider methane concentration variability occurring over areas with greater vegetation stress. In contrast, methane measurements over the Great Dismal Swamp have narrower distributions and less vegetation stress. This comparison of wetlands in differing vegetative states suggests a potential link between ecosystem stress and elevated methane emissions in wetland environments. Interestingly, despite these differences, the Great Dismal Swamp had a slightly higher mean methane concentration (2.11 ppm) compared to the Alligator River (1.96 ppm). Our results emphasize the importance of improving our understanding of what types of vegetation conditions lead to methane enhancements over wetland regimes.
Carson Turner Calculating Methane Flux Over the Great Dismal Swamp Using the Mass Balance TechniqueCarson Turner, University of North Dakota
Methane is one of the most potent greenhouse gases in the atmosphere, with a warming potential approximately 28 times larger than carbon monoxide. When examining the Global Methane Budget, wetlands are the largest natural source of methane accounting for 20-40% of global methane emissions. Wetland methane emissions have been shown to present the highest uncertainty due to both a lack of in-situ measurements to compare with models as well as a lack of understanding of how different conditions, like soil moisture and air temperature, affect methane emissions. This study looks specifically at The Great Dismal Swamp (GDS), located on the border of southeast Virginia and northeast North Carolina, to study emissions over the region using data collected on flights conducted as part of the Student Airborne Research Program (SARP) in the summer of 2025. A PICARRO Gas Concentration Analyzer was used to collect high frequency methane and carbon monoxide measurements. The two research flights followed similar flight paths around the GDS, on the 23rd and 24th of June. Methane flux was then calculated using the mass balance approach for each flight. Methane flux values were measured at 0.037 kg/s and 0.603 kg/s for the 23rd and 24th respectively. A similar study on wetlands in northern Sweden and Finland found an average methane flux value of 5.56 kg/s. A decreased methane flux value was observed on the flight day associated with higher temperatures, which is contrary to previous research on the relationship between methane emissions and temperature. Future work includes utilizing these flux measurements to improve our understanding of methane emissions from wetlands in models and further explore the relationship between methane emissions and soil moisture.
Alek Libby Comparative Analysis of Urban Ozone Chemistry in Baltimore, Richmond, and NorfolkAlek Libby , Florida State University
Urban ozone pollution remains a significant air quality concern in many U.S. cities. Ground-level ozone is not directly emitted but forms through photochemical reactions involving volatile organic compounds (VOCs) and nitrogen oxides (NOₓ) in the presence of sunlight—especially during the summer when incoming solar radiation is enhanced. The National Ambient Air Quality Standard set by the EPA for tropospheric ozone is 70 ppb, which is measured as an 8-hour average. Though exceedances of said standard have declined nationwide, understanding how emission composition varies across metropolitan areas remains critical. This study investigates the VOC makeup and ozone formation dynamics of three Mid-Atlantic urban environments: Baltimore, Richmond, and Norfolk. In-situ Whole Air Samples (WAS) were collected onboard the Aviation Dynamics B200 aircraft during the 2024 NASA Student Airborne Research Program (SARP) Campaign. Gas chromatography was used to quantify the VOC composition of each sample. Additional airborne data from CAFE and CANOE instruments provided measurements of formaldehyde (HCHO) and nitrogen dioxide (NO₂), respectively. This study looked at measurements collected below the boundary layer and within urban beltways to assess regional ozone production potential. Results showed that Baltimore exhibited significantly lower levels of key anthropogenic VOCs, particularly n-butane, i-pentane, and n-pentane. VOC/NOₓ ratios placed Richmond and Norfolk in NOₓ-limited regimes, while Baltimore fell within the transitional zone—supported by HCHO/NO₂ ratios averaging at 2.44 in Baltimore versus 5.14 and 5.09 in Norfolk and Richmond. Baltimore continues to experience notably more ozone exceedance days than Norfolk and Richmond, which is likely related to elevated NO₂ levels in the area. While reducing VOCs may help, these findings suggest that NOₓ reductions are likely more effective for mitigating ozone in the Baltimore area. Future work might replicate this analysis using the 2025 SARP dataset, which was collected on hot, stagnant days that are favorable for ozone production.
Hannah Suh Characterization of Volatile Organic Compound (VOC) Sources in the Baltimore areaHannah Suh, University of California, Santa Cruz
Volatile organic compounds (VOCs) play a key role in tropospheric photochemistry, as they react with nitrogen oxides (NOx) in sunlight to produce tropospheric ozone (O3). Both VOCs and tropospheric O3 can have negative impacts on air quality and human health. Understanding the sources of VOCs in urban areas such as Baltimore is essential for informing future air quality policies. In this study, in-situ VOC measurements collected onboard the Aviation Dynamics B200 aircraft during the NASA Student Airborne Research Program (SARP) were analyzed to characterize potential emission sources in the Baltimore area. VOC datasets from two flights from June 24th that flew over that location were investigated. This flight data was collected using aircraft instruments on the Aviation Dynamics B200, primarily the Whole Air Sampler (WAS). WAS canisters were later processed in lab using gas chromatography, which identified the different VOC mixing ratios in the air. VOCs ratios along with Positive Matrix Factorization (PMF), which reduces an inputted data matrix to separate out potential emission source contributions, were compared to each other to consider the most notable sources of VOCs in the Baltimore area. A total of six sources were looked at through PMF for this region. The top three sources seem to align with oil and natural gas, biogenic, and vehicular emissions. Chemical signature ratios indicate the presence of mixed plumes of both industrial and urban emissions, with many significant correlations with ethyne. These results point towards oil and natural gas industries, biogenic sources, and urban sources like vehicles as primary contributors to VOC signature ratios in the Baltimore area. A logical next step for this research would be to compare VOC signature ratios across multiple years to assess temporal trends.
Aashi Parikh Characterizing VOC Emissions from Chemical Plant Plumes in Hopewell, VAAashi Parikh, Boston University
Hopewell, VA is home to a cluster of major chemical facilities, whose emissions have raised concerns in neighboring communities about air pollution and health disparities. While there is information about the historical pollution in Hopewell, few studies provide a comprehensive analysis of volatile organic compounds (VOCs). This study investigates the distribution of VOCs in Hopewell’s industrial corridor and
In-situ whole air samples (WAS) were collected aboard the Aviation Dynamics B200 during the NASA Student Airborne Research Program in June 2024. In this study, samples collected at Hopewell were compared to the rest of the flight. The values were separated by chemical families, and enhancements were identified. The analysis showed that Hopewell had significant levels of aromatics, with 60 ppt of benzene, 119 ppt of toluene, and 47 ppt of styrene, which are VOCs linked to respiratory illness, neurological disorders, reproductive issues, and cancer. Aromatics observed over Hopewell were approximately 5x higher than that of the remaining flight path. According to the EPA, these carcinogenic compounds have no safe threshold for chronic exposure. As such, long-term exposure to these compounds can pose health risks. These findings reinforce existing health outcome disparities in the region, such as elevated cancer rates, and raise concerns about the exposure of nearby communities. Underserved communities are disproportionately being impacted by such health risks in Hopewell. Future research will evaluate VOC concentrations over Hopewell in 2025 and compare them to the 2024 baseline established in this study, providing insight into whether emissions reductions have occurred and if regulatory or community-driven interventions are showing impact.
Return to 2025 SARP Closeout Share Details Last Updated Nov 19, 2025 Related Terms Explore More 2 min read SARP 2025 Closeout Article 5 hours ago 10 min read SARP East 2025 Terrestrial Fluxes Group Article 5 hours ago 10 min read SARP East 2025 Oceans Group Article 5 hours agoSARP East 2025 Terrestrial Fluxes Group
10 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The 2025 SARP East Terrestrial Fluxes Group poses in front of the Dynamic Aviation B-200 aircraft, parked in a hangar at NASA’s Wallops Flight Facility in Virginia. During the internship, students spend a week engaged in Earth science data collection and learning from instruments specialists while flying onboard both the B-200 and NASA’s P-3 aircraft.NASA/Milan Loiacono Return to 2025 SARP CloseoutFaculty Advisors:
Lisa Haber, Virginia Commonwealth University
Brandon Alveshere, Virginia Commonwealth University
Graduate Mentor:
Kayla Preisler, University of Arizona
Terrestrial Fluxes Group Introduction Rice Rivers Center Director Chris Gough and Graduate Mentor Kayla Preisler Quinn Koch Monitoring Postfire Ecosystem Recovery With Spectral Indices and Eddy-Covariance Flux TowersQuinn Koch, University of California, Los Angeles
Fire is a common ecological disturbance in forest ecosystems, leading to changes in forest structure and function that have implications for the Earth’s carbon budget. Observations of post-fire carbon fluxes provide insight into the trajectory of forest recovery and its future as a carbon sink. Eddy-covariance flux towers measure high frequency greenhouse gas exchange between forests and the atmosphere, yielding measurements of net ecosystem exchange (NEE), gross primary productivity (GPP), and ecosystem respiration (Reco). While flux towers are the gold standard for quantifying ecosystem scale fluxes, vegetation indices derived from remote sensing are highly correlated with tower flux data and may provide broader spatial scale understanding of how carbon fluxes vary following fire and other disturbances. The objective of our study is to examine the relationship between tower carbon flux data and NASA Landsat-derived spectral indices at five sites in the United States and Australia that were disturbed by severe fire. Specifically, we evaluated changes following fire in two Landsat-derived spectral indices, Normalized Difference Vegetation Index (NDVI) and Normalized Burn Ratio (NBR), examining whether spectral indices paralleled temporal variation in NEE, GPP, and Reco. We found that the recovery of spectral indices outpaced the recovery of NEE and GPP at sites that experienced severe fire, highlighting how lags in structural and functional responses to disturbance may decouple vegetation indices from carbon fluxes. This suggests that a temporal lag should be considered when using vegetation indices as a proxy for carbon fluxes in post-fire ecosystems compared to unburned systems. This analysis represents a small snapshot of ecosystems worldwide; therefore, continuing to monitor these trends at future burned flux tower sites will be crucial to further understanding this relationship.
Sara Typrin Characterizing Forest Response Pathways in the Blackwater National Wildlife RefugeSara Typrin, Carleton College
Coastal forests along the Chesapeake Bay are rapidly becoming marshes due to sea level rise and extreme weather events. Predicting these ecosystem shifts is essential for climate adaptation responses. Previous studies have employed Normalized Difference Vegetation Index (NDVI) time series trends to characterize the resilience of coastal ecosystems; however, few have assessed NDVI variation trends within the Chesapeake Bay coastal region, where rates of sea level rise far exceed the global average. This study examines the spatial distribution of forest response pathways in relation to elevation within Maryland’s Blackwater National Wildlife Refuge and the surrounding Eastern Shore region. We used the Landsat 8 record (2014-2024) to extract NDVI values for areas classified as upland forest. We calculated trends in NDVI and NDVI variation using Kendall’s τ (rank correlation) to characterize each 30m pixel into one of four ecosystem shift trajectories: abrupt transition, gradual transition, recovering, or stable. We found that 14.7% of the study area is in abrupt transition, 27.4% in gradual transition, 17.3% is in recovery, and 40.6% is stable. Mapping these regions qualitatively shows that in the BNWR, areas closer to the coast tend to experience abrupt or gradual transitions, and areas farther from the coast are typically stable or in recovery. Recovering forests have higher and more variable elevations than other pathways in a subset of BNWR’s southwest region. Future work can examine how elevation and distance to the coast relate to forest response pathways at a regional scale.
Austin Jeffery Structural Characteristic Variation Between Upland Forests and Forested WetlandsAustin Jeffery, The University of Texas at Austin
Forested wetlands are important for regulating the Earth’s climate, cycling nutrients, and providing vital habitats, but are far less studied than upland forests. Prior work in upland forests has illustrated that canopy structural traits vary widely within and across forest types, and that these traits affect crucial ecosystem functions and services such as primary production and carbon sequestration. However, how canopy structure varies within and across forested wetlands has not been thoroughly explored. This study uses waveform lidar data collected during the 2024 SARP East flight campaigns over the Chesapeake Bay region using the LVIS (Land, Vegetation, and Ice Sensor) airborne platform. The LVIS Facility L2 Geolocated Surface Elevation and Canopy Height Products were used to investigate how canopy structure varies across forested wetlands and to compare canopy structural variation between forested wetlands and upland forests. To analyze the data, each lidar granule was first divided into upland and wetland forests by overlaying the granules over a USGS NLCD land use map and a USFS forest type map. Then, 20 plots were created of 100 granules each based on four tree species and whether it was an upland forest or forested wetland plot. Two upland and two wetland species were used with 5 plots each. Then, the data were used to assess variation in structural characteristics, including canopy height and vertical complexity, among forested wetlands and upland forests. The analysis resulted in a significant statistical difference between forested wetlands and upland forests structural characteristics. Additionally, forested wetlands showed a general larger variance in canopy structural complexity suggesting variation in canopy height, canopy density, layering, and forest age. This study serves as a benchmark for LiDAR-based structural characterization of forested wetlands, and informs management and conservation of forested wetlands in the mid-Atlantic region.
Ellery Moore Arctic Ecosystem Carbon Dynamics: Comparing Greenhouse Gas Measurements in Alaska and Northern Canada Using MODIS Satellite Data and Atmospheric Flask SamplesEllery Moore, Colby College
As global temperatures continue to warm, the International Panel on Climate Change (IPCC) has called attention to thawing permafrost as a potential tipping point leading to “irreversible” change to Earth’s ecosystems. Currently, permafrost holds an estimated 1,400 Pg of carbon, which will be released primarily as greenhouse gases (GHGs), methane (CH4), and carbon dioxide (CO2), through microbial activity as temperatures continue to rise, thus exacerbating the atmospheric GHG effect and further warming. In Alaska and Northern Canada, permafrost underlies most of the land, with regions determined by the percentage of frozen soil: continuous (90-100%) and discontinuous (50-90%). Upon examination of spatial maps, the continuous region tends to correspond to the tundra ecosystem, and the discontinuous region to the boreal forest ecosystem. We quantified the permafrost regions using Moderate Resolution Imaging Spectroradiometer (MODIS) derived Normalized Difference Vegetation Index (NDVI) and land surface temperature (LST). In this study, we aim to determine if CO2 and CH4 concentration measurements differ between the two ecosystems using atmospheric flask samples collected during the Arctic Boreal Vulnerability Experiment (ABoVE) in 2017. Overall, the results showed a positive correlation between NDVI and LST, with the boreal forest characterized by higher NDVI and LST than the tundra. Additionally, higher CO2 concentrations were associated with lower NDVI and LST. However, when separating the samples into the two ecosystems, no difference was seen in their diurnal cycles. In general, CH4 measurements did not show a clear relationship with NDVI and LST, but predominantly higher measurements were seen in the tundra when separating the samples by ecosystem. The different CH4 concentrations could be influenced by other environmental sources not considered in this study, such as thermokarst lakes and anthropogenic factors. Further work to differentiate the ecosystems and confirm findings can be done by examining soil moisture samples and comparing permafrost active layer thicknesses. Additionally, to better understand the rates of carbon release, eddy covariance measurements could be examined between the tundra and boreal forest over time.
Rayyane Matonding San Francisco BVOC Emissions: The Role of Urban Vegetation in HCHO/NO2 RatiosRayyane Matonding, University of San Francisco
Biogenic Volatile Organic Compounds (BVOCs) influence local air quality, especially during summer when emissions and photochemical activity peak. BVOCs can oxidize to form ground level ozone, which poses respiratory health risks. Formaldehyde (HCHO), a key photooxidation product of BVOCs, serves as a useful proxy for biogenic emissions in remote sensing studies. Likewise, nitrogen dioxide (NO2) indicates combustion-related activity and anthropogenic VOC influence. This study examines the relationship between urban tree cover and BVOC-related ozone formation using the HCHO to NO2 photochemical regime, which reflects the balance between biogenic and anthropogenic sources. HCHO and NO2 data were obtained from NASA’s TEMPO instrument, and tree cover data from SF OpenData. San Francisco was selected due to its urban greening efforts, high anthropogenic emissions, and prevalence of invasive tree species. Two neighborhoods were selected, Sunnyside with approximately 22 percent canopy cover and Potrero Hill with approximately 2 percent canopy cover, to compare temporal trends in HCHO to NO2 ratios using time series plots. These neighborhoods were chosen based on the availability of hyperlocal weather data, which allowed for more localized atmospheric analysis. No consistent relationship between tree cover and HCHO to NO2 ratios was observed, except during 15:11 and 18:11 on June 18, 2024, which may be associated with elevated photolysis. When weather variables such as zonal wind, meridional wind, and temperature were included in the analysis, no significant correlations were found. Further research should include other cities, additional time periods, and tree species information.
Emmanuel Kaiser-Veyrat Vegetation Traits to Methane Fluxes: A Machine Learning Approach Across Diverse WetlandsEmmanuel Kaiser-Veyrat, Cornell University
Wetlands are the largest and most uncertain biological source of CH4, a greenhouse gas with 56 times the radiative forcing of CO2 over a 20-year time horizon. Given the spatiotemporal constraints of these dynamic ecosystems for consistent on-site observations, remotely sensed vegetation indices (VIs) offer a scalable approach to capturing the biophysical and biochemical conditions that govern CH4 exchanges. However, their reliability in wetland environments is challenged by signal saturation in dense vegetation as well as spectral mixing of water, soil, and plants. Seeking to quantify these limitations, we employ the machine learning algorithm, Random Forest Regressor (RFR), to answer the question: Can remotely sensed vegetation traits predict CH4 fluxes across freshwater and saltwater marshes? VIs from the Index DataBase are derived from the Landsat Collection 2 Level-2 products for Landsat-7 ETM+ and Landsat-8 OLI. The FLUXNET-CH4 Community Product yields 17 wetland sites across the contiguous U.S. with daily mean methane flux values spanning some or all of the 2011 to 2018 interval. Generalized flux footprints were computed for every site adopting a uniform approach scaling fetch with increasing measurement height. Extracting feature importances from RFR, we found the Green Vegetation Moisture Index (GVMI) to consistently outperform all other indices, including two meteorological covariates measured from flux tower sites: air temperature and shortwave radiation. Grouping the VIs into five categories (moisture and water, greenness and productivity, structure and soil, pigments, and burn), we found that moisture and water indices consistently scored higher in feature importance than all other categories combined.
