Space & Satellites
SpaceX Launches Three Space Weather Satellites for Solar Storm Monitoring
SpaceX launched NASA and NOAA spacecraft to Lagrange Point 1, enhancing solar storm prediction and protection of critical infrastructure.

SpaceX Launches Three Critical Space Weather Monitoring Spacecraft: A New Era in Solar Storm Prediction and Protection
On September 24, 2025, SpaceX successfully launched three sophisticated space weather monitoring spacecraft aboard a Falcon 9 rocket, marking a significant milestone in humanity’s ability to predict and protect against solar storms and space weather events. The mission, launched at 7:30 a.m. EDT from NASA’s Kennedy Space Center in Florida, carried NASA’s Interstellar Mapping and Acceleration Probe (IMAP), NASA’s Carruthers Geocorona Observatory (CGO), and NOAA’s Space Weather Follow-on (SWFO-L1) spacecraft to their destination at the sun-Earth Lagrange Point 1, approximately 930,000 miles from Earth. This launch represents the convergence of decades of scientific research, technological advancement, and growing recognition of space weather as a critical threat to modern civilization’s infrastructure.
IMAP alone, with its investment of roughly $600 million and ten advanced scientific instruments, underscores the substantial commitment to understanding the complex interactions between solar activity and Earth’s protective magnetic environment. The successful deployment of these three complementary observatories establishes a new frontier in space weather prediction capabilities, providing enhanced protection for astronauts, satellites, power grids, and the countless technologies that underpin contemporary society.
This mission not only advances scientific research but also strengthens operational infrastructure, ensuring that both public and private sectors are better equipped to manage the risks posed by space weather. As society becomes ever more reliant on space-based assets and interconnected technologies, such initiatives are increasingly vital for economic stability and public safety.
Mission Overview and Launch Details
The September 24, 2025 launch was a carefully orchestrated deployment of three distinct but complementary space weather monitoring systems. SpaceX’s Falcon 9 rocket lifted off from Launch Complex 39A at NASA’s Kennedy Space Center, carrying all three spacecraft on a shared trajectory toward the sun-Earth Lagrange Point 1 (L1), a gravitationally stable location ideal for continuous solar observation. The launch was timed for optimal deployment and benefited from favorable weather conditions.
The deployment sequence was meticulously planned: IMAP was released into an interplanetary transfer orbit approximately 84 minutes after launch, followed by SWFO-L1 just over six minutes later, and CGO thirteen minutes after that. This staggered schedule ensured that each spacecraft could achieve its specific orbital requirements while minimizing potential interference during early mission phases.
Highlighting the mission’s technical prowess, the Falcon 9’s first stage booster landed safely on the “Just Read the Instructions” droneship, demonstrating the reliability and cost-effectiveness of reusable rocket technology. This was the 120th Falcon 9 flight of 2025, with SpaceX’s continued dominance in commercial space launches largely attributed to its reusable systems and the growing demand for satellite deployment.
“Humanity has only ever existed inside our protective magnetosphere, and as we travel beyond that protective shield, whether it be to the moon or to Mars, the actionable information from missions like IMAP will keep our astronauts safe.” — NASA’s Nicky Fox, Science Mission Directorate
The Three Spacecraft and Their Scientific Objectives
NASA’s Interstellar Mapping and Acceleration Probe (IMAP)
IMAP is the flagship of this mission, representing a $600 million investment in probing the boundaries of our solar system and the processes governing particle acceleration in the heliosphere. It carries ten scientific instruments designed to address the composition and properties of the local interstellar medium, the evolution of regions where solar wind and interstellar medium interact, and particle acceleration processes. IMAP’s compact design, just 2.4 meters in diameter and 0.9 meters in height, houses advanced imaging systems capable of mapping energetic neutral atoms across a broad energy spectrum.
Key instruments include IMAP-Lo, IMAP-Hi, and IMAP-Ultra, each targeting different energy ranges to provide comprehensive data on the interactions at the edge of the heliosphere. The spacecraft also features a magnetometer system and specialized particle detectors, enabling it to study both solar wind and interstellar particles in unprecedented detail. IMAP is expected to take about 108 days to reach its operational position at L1, with a planned mission duration of three to five years.
IMAP builds upon a scientific legacy stretching back to the Voyager missions and the Interstellar Boundary Explorer (IBEX), promising more frequent and higher-resolution data that will refine our understanding of the solar system’s outer boundaries and the mechanisms driving space weather.
NASA’s Carruthers Geocorona Observatory (CGO)
CGO focuses on Earth’s exosphere, the outermost layer of the atmosphere, extending from about 375 miles to 6,200 miles above the surface. Named after Dr. George Carruthers, a pioneer in ultraviolet astronomy, CGO utilizes two far ultraviolet (FUV) cameras to study the geocorona’s shape, density, and response to space weather events. Its main scientific goals are to map the geocorona’s response to solar storms and to understand the sources and behavior of hydrogen in the upper atmosphere.
With a mass of 240 kilograms, CGO will operate from L1 for two years, continuously monitoring the hydrogen-rich frontier that shields Earth from solar wind. Insights from CGO will improve models of atmospheric loss and space weather impacts, with implications for both Earth and comparative planetology.
This mission continues the work begun by Carruthers’ Apollo 16 Far Ultraviolet Camera/Spectrograph, updating his foundational research with modern technology and persistent observation capabilities.
NOAA’s Space Weather Follow-on (SWFO-L1)
SWFO-L1 is NOAA’s next-generation operational space weather monitoring system, designed to provide real-time observations and early warnings for infrastructure protection. From its L1 vantage point, SWFO-L1 will deliver continuous data on solar wind properties, magnetic fields, and energetic particles, supporting critical sectors such as electric power, aviation, and satellite operations.
This spacecraft enables the retirement of aging satellites and enhances NOAA’s ability to provide timely alerts and forecasts. Its mission addresses the growing need for uninterrupted space weather data as society becomes increasingly dependent on vulnerable technologies.
NOAA and NASA share responsibilities for SWFO-L1, with NOAA managing requirements and data dissemination, while NASA and commercial partners handle development, testing, and launch. This collaborative model ensures that operational needs are met with cutting-edge technical solutions.
“SWFO-L1 will serve as an early warning beacon, helping protect our electric grid, aviation, and satellite industries from the unpredictable nature of space weather.”
Space Weather: Understanding the Threat and Economic Impact
Space weather, encompassing solar flares, coronal mass ejections, and geomagnetic storms, poses a documented threat to modern infrastructure. Effects range from power grid failures to satellite disruptions and impaired GPS navigation. The economic stakes are high; a 2017 NOAA report examined impacts on satellites, electric power, aviation, and navigation systems, highlighting the potential for cascading failures across entire economies.
Insurance industry analyses, such as those by Lloyd’s of London, estimate that a severe space weather event could result in global economic losses ranging from $1.2 trillion to $9.1 trillion, with North America particularly vulnerable. In the United States alone, studies have projected that an extreme blackout scenario could cost nearly $42 billion per day, not including international supply chain losses. The manufacturing sector is especially exposed, but the ripple effects would touch nearly every aspect of daily life.
Historical precedent for such events exists, most notably in the 1859 Carrington Event, which disrupted global telegraph systems. Modern society’s reliance on electricity and digital communications means that a similar event today would have far more devastating consequences. Recent research suggests there is a 12% probability of a Carrington-scale event occurring within the next decade, making robust space weather monitoring and forecasting an urgent priority.
“The potential cost of a major solar storm blackout in the US could reach $42 billion per day, with additional losses from global supply chain disruptions.”
Technological Innovation and Mission Significance
This mission showcases advancements in spacecraft miniaturization, instrument integration, and international collaboration. IMAP’s ten instruments, packed into a compact 900-kilogram platform, reflect progress in electronics and systems engineering. The deployment of three complementary spacecraft to L1 allows for multi-faceted observation, enhancing both scientific discovery and operational monitoring.
IMAP’s real-time data link will provide approximately 30 minutes of advance warning for incoming solar radiation events, an essential capability for protecting astronauts and sensitive technologies. CGO’s continuous monitoring of the geocorona will improve atmospheric models, while SWFO-L1’s operational focus ensures that NOAA can deliver timely alerts to critical industries.
The mission’s collaborative framework, involving NASA, NOAA, Princeton University, Johns Hopkins Applied Physics Laboratory, and 27 international partners, demonstrates a model for future large-scale scientific and operational missions. The integration of real-time data and advanced instrument suites sets a new standard for space weather monitoring, with direct benefits for both research and societal resilience.
“Space weather prediction is no longer just a scientific pursuit, it’s an economic and national security imperative.”
Conclusion
The successful launch and deployment of IMAP, CGO, and SWFO-L1 mark a transformative leap in our ability to monitor and predict space weather. These spacecraft will provide continuous, high-quality data that enhances both our scientific understanding of the heliosphere and our operational capacity to protect vital infrastructure and human life.
As society’s dependence on space-based technologies grows, the insights and warnings delivered by these missions will become increasingly crucial. Looking ahead, the data collected will inform next-generation prediction systems, support safe human exploration beyond Earth’s magnetosphere, and help safeguard the global economy from the unpredictable forces of our Sun.
FAQ
What is the main purpose of the IMAP mission?
IMAP’s primary goal is to study the boundary of the heliosphere and the processes that govern particle acceleration, improving our understanding of how solar and interstellar phenomena affect space weather near Earth.
Why is the Lagrange Point 1 (L1) chosen for these missions?
L1 offers a stable gravitational point between Earth and the Sun, providing an unobstructed, continuous view of solar activity and allowing real-time monitoring of space weather conditions.
How does space weather impact daily life and the economy?
Space weather can disrupt electric power grids, satellites, aviation, GPS, and communications systems, with the potential for large-scale economic losses and critical infrastructure failures.
How will these new spacecraft improve space weather prediction?
By providing real-time, high-resolution data from multiple vantage points, the new spacecraft will enable earlier warnings and more accurate forecasts, helping to mitigate the impacts of solar storms.
Who manages and operates these missions?
NASA and NOAA share management responsibilities, with contributions from international partners, universities, and commercial entities ensuring robust scientific and operational outcomes.
Sources: NASA Press Release
Photo Credit: NOAA
Space & Satellites
Space Nuclear Power Faces Logistical and Economic Barriers, DRACO Canceled
Experts say space nuclear power challenges are logistical and economic, not technical. DRACO canceled; focus shifts to nuclear reactors in space and on the Moon.

This article summarizes reporting by Aerospace America.
For decades, the aerospace industry has recognized the immense potential of space nuclear power. Despite possessing the foundational technical knowledge since the 1960s, modern spacecraft continue to rely predominantly on chemical propulsion and solar arrays. A recent workshop at the May 2026 AIAA ASCEND event in Washington, D.C., sought to unpack this enduring paradox.
According to reporting by Aerospace America, a panel of aerospace and policy experts concluded that the primary barriers to deploying nuclear reactors in space are no longer technical. Instead, the industry is grappling with logistical, economic, and systemic hurdles that have repeatedly stalled progress.
The recent cancellation of the highly publicized Demonstration Rocket for Agile Cislunar Operations (DRACO) program in mid-2025 serves as a stark, real-world validation of these expert assessments, demonstrating how shifting economic landscapes can ground even the most ambitious nuclear initiatives.
The Illusion of Technical Barriers
During the ASCEND workshop, hosted by Brian Weeden of The Aerospace Corporation, panelists emphasized the extensive capital and time already invested in space nuclear research. Bhavya Lal, a professor at the RAND School of Public Policy, highlighted that the United States has spent 60 years and over $20 billion proving that the technology itself is viable.
“The technology has never been the bottleneck. What has failed each time is the system around the reactor,” Lal stated, according to the workshop coverage.
Lal further explained that these systemic failures include shifting mission scopes, a lack of political continuity, and unstable leadership architectures that prevent long-term projects from reaching the launch pad.
Stagnation Since the Space Race
The historical context of space nuclear power underscores the panel’s frustrations. During the Cold War, the U.S. heavily researched and successfully ground-tested nuclear thermal rockets through initiatives like the NERVA program. However, as reported by Aerospace America, these programs were ultimately scrapped due to changing political administrations and budget cuts following the Apollo era.
Tabitha Dodson, a program manager at the DARPA Defense Sciences Office, noted the resulting stagnation in the field during her panel remarks.
“The United States hasn’t really evolved our nuclear space technology since the fifties or sixties,” Dodson remarked at the event.
Dodson added that current research priorities have had to pivot toward radioisotope power systems and direct-energy power conversion systems to maintain momentum in a risk-averse funding environment.
Economic Realities and the DRACO Cancellation
The intersection of aerospace engineering and economic viability was brought into sharp focus with the recent fate of the DRACO program. Initiated in 2020 as a joint effort between DARPA, NASA, Lockheed Martin, and BWX Technologies, DRACO aimed to test a nuclear thermal rocket in orbit by 2027. Nuclear thermal propulsion was projected to be two to three times more efficient than chemical propulsion, potentially halving the travel time to Mars.
The Impact of Commercial Launch Costs
In June 2025, DARPA officially canceled the DRACO program. According to public statements from DARPA deputy director Rob McHenry, the decision was driven entirely by economics rather than technical failure.
The rapid decrease in commercial launch costs, largely propelled by the heavy-lift capabilities of companies like SpaceX, fundamentally altered the financial equation. The massive research and development costs required to perfect nuclear thermal propulsion could no longer be justified by a positive return on investment when chemical launches had become so inexpensive.
Current Mandates and the Path Forward
Despite the setbacks in nuclear propulsion, the push for nuclear power generation in space remains robust. Current executive mandates have established ambitious timelines, aiming for a functional nuclear reactor in space by 2028 and a working reactor on the lunar surface by 2030. These systems are considered critical for supporting long-term lunar habitats and deep-space exploration missions.
Balancing Ambition and Safety
Aaron Miles, Coordinator for Strategic Capabilities at the White House Office of Science and Technology Policy, discussed these targets at the ASCEND workshop. He emphasized the administration’s focus on setting goals that push the industry forward without ignoring logistical realities.
“Lunar surface reactor development efforts and in-space reactor efforts can benefit each other,” Miles noted regarding the dual mandates.
To meet these goals while navigating strict regulatory and safety hurdles, modern programs are utilizing High-Assay Low-Enriched Uranium (HALEU). Furthermore, contemporary reactor designs ensure that fission is only initiated once the system is safely in orbit, mitigating the historical public fears and international treaty complications associated with launching nuclear material.
AirPro News analysis
We observe that the pivot from nuclear propulsion (like the canceled DRACO program) to stationary nuclear surface power reflects a pragmatic maturation of the aerospace sector. While reusable chemical rockets have decisively won the current launch economics battle, sustained deep-space habitats and lunar bases will undeniably require the continuous, high-density energy that only nuclear reactors can provide. The looming 2028 and 2030 mandates will serve as a critical test of whether the U.S. government and its commercial partners can finally overcome the systemic inertia and political discontinuity described by the ASCEND panelists.
Frequently Asked Questions
What was the DRACO program?
The Demonstration Rocket for Agile Cislunar Operations (DRACO) was a joint U.S. government and industry program initiated in 2020 to develop and test a nuclear thermal rocket by 2027. It was canceled in June 2025 due to shifting economic priorities and the falling cost of commercial chemical rocket launches.
Why is nuclear power needed in space?
While solar panels and chemical batteries are sufficient for operations near Earth, deep-space exploration and permanent lunar or Martian habitats require reliable, high-density power sources that can operate continuously without sunlight or frequent resupply.
What is HALEU?
High-Assay Low-Enriched Uranium (HALEU) is a type of nuclear fuel that provides a balance between high energy output and safety, making it a preferred choice for modern space reactor designs to comply with international regulations and safety standards.
Sources
Photo Credit: Aerospace America
Space & Satellites
SpaceX Secures $4.16B Contract for Space-Based Airborne Targeting
SpaceX awarded $4.16B by U.S. Space Force to develop SB-AMTI satellite constellation for global airborne threat detection by 2028.

This article summarizes reporting by DefenseScoop.
The U.S. Space Force has awarded SpaceX a $4.16 billion Other Transaction Authority (OTA) agreement to accelerate the development of the Space-Based Airborne Moving Target Indicator (SB-AMTI) program. According to reporting by DefenseScoop, the May 29, 2026, award aims to deploy a constellation of satellites capable of continuously detecting, tracking, and targeting airborne threats, including aircraft, drones, and cruise missiles, globally from space.
This multi-billion dollar contract highlights a strategic shift by the Pentagon to move critical surveillance capabilities from vulnerable airborne platforms to a more resilient space-based architecture. The Space Force expects to field an initial constellation by 2028, providing the Joint Force with an early operational capability.
SpaceX’s selection is part of a broader competitive procurement strategy. According to the source material, the aerospace company is one of nine vendors selected in April 2026 to compete for the SB-AMTI program. The Space Force anticipates issuing multiple awards to other vendors in the coming year to maintain a diverse industrial base.
The Shift from Air to Space
Retiring Legacy Airborne Systems
Historically, the U.S. military has relied on airborne warning and control system (AWACS) aircraft, such as the aging E-3 Sentry and the retired E-8 JSTARS, to execute moving target indicator missions. However, DefenseScoop reports that as adversaries develop increasingly sophisticated anti-access/area-denial (A2/AD) systems, these large, slow-moving aircraft have become highly vulnerable in contested airspace.
To address these operational blind spots, the Space Force is developing SB-AMTI to complement traditional airborne sensing. While the Air Force is currently procuring the E-7 Wedgetail to replace the E-3 Sentry, following congressional intervention to save the E-7 program from budget cuts, the Pentagon’s long-term goal is to transition the bulk of AMTI tasks into the space domain for enhanced survivability.
“To compliment traditional airborne sensing, the requirement for a layered, highly resilient tracking architecture is evident.”
Contract Details and Strategic Context
Funding and the “Golden Dome” Framework
The $4.16 billion OTA agreement tasks SpaceX with building an interconnected “system-of-systems” that combines space-based sensors, secure communication links, and ground processing to track moving airborne targets in real-time. To support this architecture, the Space Force has requested $7 billion to begin the formal procurement of SB-AMTI in fiscal year 2027, though DefenseScoop notes these funds are contingent upon Congress passing a reconciliation bill.
The SB-AMTI program is also a critical component of President Donald Trump’s proposed “Golden Dome” missile defense initiative. This framework aims to create a multi-layered defense system spanning ground, air, and space to detect and intercept airborne threats. The military is fast-tracking the SB-AMTI program to ensure the defensive system can meet its 2028 operational target.
“By focusing these capabilities to the space domain, we are providing the Joint Force with sustained battlespace awareness of contested airspace.”
SpaceX’s Growing Defense Portfolio
A Week of Multi-Billion Dollar Awards
This latest contract cements SpaceX’s position as a dominant player in U.S. national security. According to the provided research, the SB-AMTI award arrives just days after the Space Force granted SpaceX a separate $2.29 billion contracts on May 26, 2026, for the Space Data Network Backbone program, which will provide satellite communications for future missile interceptors.
In a single week, SpaceX secured nearly $6.45 billion in defense contracts. This surge in government backing coincides with industry reports indicating that SpaceX is preparing for an initial public offering (IPO) that could value the company at over $1.5 trillion.
Future Milestones and Parallel Programs
Looking Toward 2035
The Space Force has outlined an aggressive timeline for its space-based surveillance initiatives. Following the projected 2028 deployment of the initial SB-AMTI satellite constellation, the military anticipates operating second- and third-generation systems by 2035.
In parallel, the Space Force is developing the Space-Based Ground Moving Target Indicator (SB-GMTI) program to track ground-based targets. DefenseScoop reports that this complementary system is currently in the research-and-development phase.
“We will not leverage any one single provider; instead, we are partnering with a highly diversified pool of traditional and non-traditional vendors…”
AirPro News analysis
At AirPro News, we observe that the rapid succession of multi-billion dollar OTA agreements awarded to SpaceX underscores a fundamental shift in Pentagon procurement. By utilizing Other Transaction Authority agreements, the Space Force is bypassing traditional, often sluggish acquisition processes to field critical capabilities on an accelerated timeline. This is particularly vital given the 2028 target for the “Golden Dome” initiative.
Furthermore, the explicit linkage of the SB-AMTI program to national missile defense suggests that space-based sensing is no longer viewed merely as a support function, but as the primary nervous system for future combat operations. While the Space Force publicly emphasizes vendor diversity, noting that SpaceX is just one of nine companies selected for the vendor pool, the sheer financial volume of SpaceX’s recent awards indicates that the industrial base for national security space is heavily reliant on a few highly capable mega-constellation providers.
Frequently Asked Questions
What is the SB-AMTI program?
The Space-Based Airborne Moving Target Indicator (SB-AMTI) is a U.S. Space Force initiative designed to deploy a constellation of satellites capable of detecting, tracking, and targeting airborne threats globally from space.
How much is the SpaceX contract worth?
The U.S. Space Force awarded SpaceX a $4.16 billion Other Transaction Authority (OTA) agreement for the SB-AMTI program on May 29, 2026.
When will the SB-AMTI system be operational?
The Space Force projects the deployment of an initial SB-AMTI satellite constellation by 2028, with second- and third-generation systems anticipated by 2035.
Sources
Photo Credit: Starbase Texas
Space & Satellites
NASA X-59 Set for First Supersonic Flight in June 2026
NASA’s X-59 experimental aircraft will make its first supersonic flight in June 2026 to test quiet supersonic technology and reduce sonic booms.

NASA’s experimental X-59 aircraft is preparing to cross a historic aviation threshold. According to an official press release from the space agency, the quiet supersonic research aircraft is scheduled for its first supersonic flight in early June 2026. This milestone marks a critical phase in NASA’s Quesst (Quiet SuperSonic Technology) mission, which seeks to demonstrate that an aircraft can break the sound barrier without producing a disruptive sonic boom.
Since its maiden flight in October 2025, the X-59 has successfully completed 14 subsonic test flights, according to NASA’s project data. The upcoming tests will transition the aircraft into a rigorous “envelope expansion” phase. By gathering precise acoustic data, NASA ultimately hopes to provide federal and international regulators with the evidence needed to reconsider the 53-year-old ban on commercial supersonic flight over land.
To prepare for these high-stakes flights, the X-59 team has recently accelerated its testing cadence. NASA reports that in late April 2026, the ground crew and flight team successfully executed two test flights in a single day for the first time, demonstrating the aircraft’s growing reliability.
The Quesst Mission and Envelope Expansion
Pushing Toward Mach 1.4
The initial supersonic test scheduled for early June 2026 will see the X-59 cross the sound barrier, exceeding 630 mph, at an altitude of approximately 43,000 feet. Following this initial breakthrough, NASA plans to push the aircraft toward its ultimate “mission conditions.” Official specifications dictate a target cruising speed of Mach 1.4 (approximately 925 mph) at an altitude of 55,000 feet.
In the agency’s press release, Cathy Bahm, Project Manager for NASA’s Low Boom Flight Demonstrator, emphasized the importance of this testing phase:
“What comes next is the first time this one-of-a-kind aircraft will fly supersonic. We are starting toward the mission conditions test point that X-59 was designed for.”
Bahm further noted that completing the first mission-conditions flight is a significant milestone, as it allows the team to verify that the aircraft performs safely in its intended environment.
Engineering a “Quiet Thump”
Unconventional Design and Testing Methodology
The X-59 was built by Lockheed Martin Skunk Works under a $247.5 million contract awarded by NASA in 2018. To achieve its acoustic goals, the aircraft features a highly unconventional design. According to project specifications, the nose accounts for nearly a third of the aircraft’s total length. This elongated structure is engineered specifically to scatter shock waves before they can merge into a loud sonic boom.
Because of this unique aerodynamic shape, the cockpit lacks a forward-facing windshield. Instead, NASA equipped the X-59 with a high-resolution External Vision System (XVS), which feeds live camera footage to an in-cockpit monitor to allow pilots to navigate safely.
NASA test pilot Jim ‘Clue’ Less detailed the cautious approach the flight team is taking during this envelope expansion phase:
“From here on out, once we’re airborne, we can increase speed and increase altitude in small, measured chunks, looking at things as we go and not getting ahead of ourselves.”
During these initial supersonic flights, the public will not yet hear the anticipated “quiet thump.” NASA states that the X-59 will be accompanied by a traditional F-15 chase plane equipped with a specialized shock-sensing probe. The traditional sonic boom produced by the F-15 will obscure the X-59’s quieter acoustic signature from observers on the ground.
AirPro News analysis
We view the upcoming June 2026 flights as a pivotal moment not just for NASA, but for the broader commercial aviation industry. In 1973, the Federal Aviation Administration (FAA) banned commercial supersonic flights over U.S. land due to severe noise pollution. For historical context, the retired Concorde produced a sonic boom of about 105 to 110 Effective Perceived Noise Level in decibels (EPNdB). NASA’s target for the X-59 is a mere 75 EPNdB, roughly equivalent to the sound of a car door closing 20 feet away.
If the current Phase 1 envelope expansion is successful, NASA will move to Phase 2 (Acoustic Validation) later in 2026, utilizing a 48-kilometer-long array of 125 sonic boom recorders in the Mojave Desert. Phase 3 will involve flying the aircraft over selected U.S. communities to gather public feedback. We believe that this methodical, data-driven approach is the most viable pathway for the aerospace sector to establish new noise standards and potentially unlock a new era of overland commercial supersonic travel.
Frequently Asked Questions (FAQ)
What is the NASA X-59?
The X-59 is an experimental research aircraft developed by NASA and Lockheed Martin as part of the Quesst mission. It is designed to fly faster than the speed of sound without producing a loud sonic boom, reducing the noise to a quiet “thump.”
When is the X-59’s first supersonic flight?
According to NASA, the aircraft is scheduled to make its first supersonic flight in early June 2026, crossing the sound barrier at an altitude of approximately 43,000 feet.
Why does the X-59 have no forward windshield?
To prevent shock waves from merging into a sonic boom, the X-59 requires an exceptionally long, pointed nose, which obstructs forward visibility. Pilots use an External Vision System (XVS), a network of cameras and screens, to see directly in front of the aircraft.
Sources
Photo Credit: NASA
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