NASA’s Quesst Mission Marks X-59’s Historic First Flight

NASA’s Quesst Mission Marks X-59’s Historic First Flight

The X-59 is shown during its historic first flight flown by NASA test pilot Nils Larson.
NASA/Lori Losey

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.

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Maria Werries

NASA, Aerospace Corporation Study Sharpens Focus on Ammonia Emissions

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-Caltech

The 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.” 

News 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

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X-59 First Flight Media Resources

X-59 First Flight Media Resources

1 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

​Media Contact

Quesst Media Lead: Kristen Hatfield, 757-817-5522

First Flight Videos

First Flight Highlight Reel (1:43)

First Flight Extended B-Roll (7:39)

Articles

NASA’s X-59 Completes First Flight, Prepares for More Flight Testing

First Flight Images

NASA’s X-59 quiet supersonic research aircraft lifts off from the runway at U.S. Air Force Plant 42 in Palmdale, California. Its wheels are just slightly off the runway. Heat waves are visible off the back of the aircraft as it ascends under a clear sky. Rows of Joshua trees stretch toward the mountains in the background.
NASA’s X-59 quiet supersonic research aircraft lifts off for its first flight Tuesday, Oct. 28, 2025, from U.S. Air Force Plant 42 in Palmdale, California. The aircraft’s first flight marks the start of flight testing for NASA’s Quesst mission, the result of years of design, integration, and ground testing and begins a new chapter in NASA’s aeronautics research legacy.
NASA/Carla Thomas
NASA’s X-59 quiet supersonic research aircraft lifts off from the runway at U.S. Air Force Plant 42 in Palmdale, California. The nose is angled slightly upward, and the landing gear is down as it ascends under a blue sky. The tops of buildings are visible below, with mountains in the far background.
NASA’s X-59 quiet supersonic research aircraft lifts off for its first flight Tuesday, Oct. 28, 2025, from U.S. Air Force Plant 42 in Palmdale, California. The aircraft’s first flight marks the start of flight testing for NASA’s Quesst mission, the result of years of design, integration, and ground testing and begins a new chapter in NASA’s aeronautics research legacy.
NASA/Carla Thomas
NASA’s X-59 flies above the Mojave Desert against a blue sky. The aircraft’s long nose is angled slightly upward to the left, with its landing gear down. Layers of mountains are visible in the background. The aircraft is backlit, appearing to float as it ferries to NASA’s Armstrong Flight Research Center in Edwards, California.
NASA’s X-59 quiet supersonic research aircraft flies above Palmdale and Edwards, California, on its first flight Tuesday, Oct. 28, 2025. The aircraft will travel 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 Ross
NASA’s X-59 flies above the Mojave Desert with a NASA F-15 off its left wing. The X-59’s landing gear is down and below it the desert landscape stretches toward rows of windmills in front of mountains.
NASA’s X-59 quiet supersonic research aircraft flies above Palmdale and Edwards, California, on its first flight Tuesday, Oct. 28, 2025, accompanied by a NASA F-15 research aircraft. The F-15 monitored the X-59 during the flight as it 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 Ross
NASA’s X-59 is seen in flight, with a blue sky and mountains behind it and land below it. The aircraft’s long nose and distinct silhouette are visible as it ferries to NASA’s Armstrong Flight Research Center in Edwards, California 
NASA’s X-59 quiet supersonic research aircraft cruises above Palmdale and Edwards, California, during its first flight, Tuesday, Oct. 28, 2025. The aircraft will traveled to NASA’s Armstrong Flight Research Center in Edwards, California.
NASA/Lori Losey
The X-59 pulls onto the ramp at NASA’s Armstrong Flight Research Center. In front of the aircraft, the crew chief stands with arms raised to guide it in, while another flight crew member stands beside the aircraft. An audience is visible in the background near a large hangar.
The X-59 quiet supersonic research aircraft arrives at NASA’s Armstrong Flight Research Center in Edwards, California, following its first flight Tuesday, Oct. 28, 2025. The arrival marks the aircraft’s transition from ground testing to flight operations. Next, the aircraft will undergo scheduled maintenance followed by a series of additional test flights, gradually building toward its first supersonic flight.
NASA/Genaro Vavuris
Nils Larson steps down a ladder beside the X-59’s cockpit. He is wearing a tan flight suit with the aircraft parked on the ramp and its canopy open behind him.
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 Vavuris

More X-59 imagery is available in NASA’s Quesst Image Gallery

Historical Resources

Taxi Test B-Roll

Rollout of the X-59 Quesst Supersonic Plane Ceremony Jan. 12, 2024

Biographies

Peter Coen

Cathy Bahm

Brian Griffin

Nils Larson

Jim Less

Quesst Media Resources

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Lillian Gipson

I Am Artemis: Ethan Jacobs

I Am Artemis: Ethan Jacobs

3 Min Read

I Am Artemis: Ethan Jacobs

Colorado National Guard Chief Warrant Officer and military helicopter pilot Ethan Jacobs stands in the hangar bay at the High-Altitude Army National Guard Training Site near Gypsum, Colorado. NASA and the Colorado Army National Guard are partnering on a simulated lander flight training course for Artemis in the mountains of northern Colorado. Jacobs is the lead instructor and helped to develop the course.

Listen to this audio excerpt from Ethan Jacobs, a helicopter pilot and member of the Colorado Army National Guard developing a foundational flight training course for Artemis astronauts:

0:00 / 0:00

High above the Rocky Mountains, Ethan Jacobs is helping NASA preparing to land people on the Moon for the first time in more than 50 years. NASA will send astronauts to the lunar South Pole during the Artemis III mission and beyond. As part of their journeys, crew will travel in a human landing system that will safely transport them from lunar orbit to the lunar surface and back.

Jacobs, a chief warrant officer with the Colorado National Guard and helicopter pilot for 20 years, both privately, and with the U.S. Army active duty and National Guard, has been working with NASA to develop a foundational training course at the High-Altitude Army National Guard Aviation Training Site, near Gypsum, Colorado. The culmination of that work is a NASA-certified foundational training course for astronauts that exposes them to the challenges of vertical flight profiles and landing in extreme conditions.

The challenging conditions we fly in replicates – as much as possible here on Earth – some of the challenges astronauts will face when landing on the Moon.

Ethan Jacobs

Ethan Jacobs

Chief Warrant Officer, Colorado Army National Guard

Colorado’s challenging terrain, dusty and white-out conditions in certain places, and high desert landscape make it an ideal setting for replicating a lunar environment for flight. In addition, there can be flat light where there is little to no shadow, all of which can create visual illusions and challenge a crew’s sense of depth perception.

And a lot of the visual illusions the NASA astronauts training at the High-Altitude Army National Guard Aviation Training Site experience are eye-opening.

“I teach the astronauts how to distinguish slopes in degraded visual conditions because we normally judge slope by shadows and changes in vegetation color,” Jacobs said. “But these conditions in the Colorado mountains can be monochromatic, like on the Moon.”

On a typical flight in a UH-72 Lakota helicopter, Jacobs sits in the front with one astronaut crew member and another astronaut sits in the back. Jacobs trains the astronaut team on how best to identify and overcome visual and cognitive illusions while evaluating techniques and team dynamics. Working with NASA, Jacobs and his team have studied maps of the lunar terrain, then located similar landing zones in the Colorado mountains.

“The two-person astronaut crew has to work together, communicate, and navigate with real-world consequences,” Jacobs said. “Fuel is burning and they can’t press the pause button like in a simulator. I try to expose them to as many different conditions and various landing zones as possible.”

At the end of the day, adaptability is key to successfully landing in extreme conditions.

Ethan Jacobs

Ethan Jacobs

Chief Warrant Officer, Colorado Army National Guard

NASA recently certified the course, marking a milestone in preparing for the future Artemis III crew. Since 2021, astronauts with NASA and ESA (European Space Agency) have taken part in the high-altitude aviation course have proven to be receptive to the training and adaptable to expanding their piloting skills, Jacobs said.

Artemis astronauts will receive specialized training on the specific lander for their mission from NASA’s commercial providers, SpaceX and Blue Origin. The training course, along with simulators and specialized crew training, provides fundamental coursework that will allow Artemis astronauts to be best prepared to land on the lunar surface.

Through the Artemis campaign, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and to build the foundation for the first crewed missions to Mars for the benefit of all.

For more information about Artemis visit:

https://www.nasa.gov/artemis

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NASA Stennis Engineer Follows Family Footsteps into NASA’s Artemis Era

NASA Stennis Engineer Follows Family Footsteps into NASA’s Artemis Era

Huy Nguyen
Huy Nguyen is an electrical controls engineer at NASA’s Stennis Space Center, where his work has contributed to NASA’s Artemis program that will send astronauts to the Moon to prepare for future human exploration of Mars.
NASA/Danny Nowlin

Huy Nguyen grew up hearing about rocket engines and space flight around the family table. His parents worked for NASA’s Michoud Assembly Facility in New Orleans, and those early conversations eventually started his path to NASA’s Stennis Space Center near Bay St. Louis, Mississippi.

“They both created a household that allowed me to be curious and to be a problem solver,” Nguyen said.

The dinner conversations have come full circle as the New Orleans native finds himself applying that same curiosity and problem-solving mindset at NASA Stennis.

Nguyen is currently the electrical controls engineer for propulsion testing support areas, which include the NASA Stennis High Pressure Gas Facility and the High Pressure Industrial Water Facility.

“Both areas are considered the heart and powerhouse of testing,” Nguyen said.

His work involves two key challenges: maintaining legacy systems with hard-to-find replacement parts and modernizing them with robust control systems that offer better monitoring and maintenance capabilities. What energizes Nguyen most is bridging old and new technology by creating improved user interfaces and integrating modern controls with existing infrastructure.

“This is what excites me about my work,” he said.

One of the most exciting moments in Nguyen’s NASA career came with the successful Green Run test series at NASA Stennis for NASA’s Artemis campaign to return humans to the Moon.

The test series helped validate the first SLS (Space Launch System) core stage for the Artemis I test flight around the Moon, setting the stage for the Artemis II test flight when four astronauts will fly around the Moon in early 2026.

As the engineer overseeing controls operations for the NASA Stennis High Pressure Gas Facility and High Pressure Industrial Water Facility, Nguyen had a critical responsibility leading to the Green Run test series.

He ensured the complex systems ran flawlessly to supply helium, nitrogen, air, and water for SLS core stage testing.

It turned into a career highlight.

“It was a lot of work to set it up and then run it around the clock for 24 hours,” Nguyen recalled.

For an entire day, multiple systems had to operate in perfect harmony, supplying everything the massive SLS core stage needed for a sitewide stress test.

“Seeing everyone focused on a single goal like that was truly amazing,” he said.

Engineers, technicians, and support staff worked in shifts around the clock. Each person knew their role was essential to the mission’s success. It was the kind of teamwork his NASA parents likely witnessed countless times, and now Nguyen experienced it himself.

The 24-hour exercise helped make way for a historic milestone at NASA Stennis. The Green Run testing series reached its conclusion on March 18, 2021, when the SLS core stage fired its four RS-25 engines for a full mission duration of 8 minutes and 19 seconds. The final Green Run hot fire represented the most powerful propulsion test at the center in more than 40 years.

As NASA prepares for Artemis II, Nguyen’s work upgrading these critical facilities ensures NASA Stennis will remain ready to support humanity’s next giant leaps into deep space.

When Artemis II launches in 2026, Nguyen looks forward to watching the test flight around the Moon with his parents, who inspired him as a young boy, and his young nephews.

“My nephews are currently obsessed with cars and trucks, so I hope Artemis II will expose them to space travel,” Nguyen said.

Through the Artemis campaign, NASA will send astronauts to the Moon to prepare for future human exploration of Mars and inspire the next generation of explorers.

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LaToya Dean