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IBM NASA Surya AI Model Enhances Solar Storm Prediction Accuracy

IBM and NASA unveil Surya, an AI model improving solar storm forecasts by 16% to protect technology and infrastructure globally.

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Revolutionary AI Model Surya Transforms Solar Storm Prediction and Technology Protection Through NASA-IBM Partnership

The development of the Surya Heliophysics Foundation Model marks a pivotal moment in the advancement of space weather prediction. By harnessing artificial intelligence and over a decade of continuous solar observation data, IBM and NASA have created an unprecedented capability for forecasting solar storms, events that pose significant threats to global technology infrastructure. Announced in August 2025, this collaboration has yielded the first foundation model tailored to heliophysics, achieving a 16% improvement in solar flare classification accuracy and providing visual predictions of flare locations up to two hours in advance. The potential economic impact of major solar storms is immense, with global losses estimated at $2.4 trillion over five years, underscoring the necessity of accurate prediction systems for safeguarding satellites, power grids, and communication networks. By releasing this 366-million parameter model as open source, IBM and NASA have democratized access to advanced space weather forecasting, empowering researchers worldwide to build upon NASA’s extensive Solar Dynamics Observatory (SDO) dataset and create specialized applications.

The Surya model’s open-source nature, performance breakthroughs, and technical innovations not only represent a leap forward in scientific capability but also signal a new era of interdisciplinary collaboration. The model’s development and deployment have implications for global resilience, economic stability, and the future of AI-driven scientific discovery.

Background on Solar Weather and Space Storms

Solar weather, driven by the Sun’s dynamic magnetic and plasma processes, is a major natural hazard for modern technology. The Sun’s nuclear fusion core generates complex magnetic fields, occasionally releasing charged particles and electromagnetic radiation in the form of solar flares and coronal mass ejections (CMEs). When these phenomena reach Earth, they can disrupt satellites, power grids, and communications networks.

The significance of solar storms became widely recognized after the 1859 Carrington Event, which caused global telegraph failures and electrical fires. Today, the stakes are exponentially higher, as our dependence on electronic systems and interconnected infrastructure leaves us more vulnerable to space weather. The launch of NASA’s Solar Dynamics Observatory in 2010 represented a turning point, providing high-frequency, multi-wavelength solar observations that form the backbone of modern predictive efforts.

Solar activity follows an 11-year cycle, with peak periods producing frequent and intense storms. The classification system for solar flares, C, M, and X classes, reflects their increasing intensity, with X-class flares posing the greatest risk. The physical mechanisms behind these events involve the reconfiguration of magnetic field lines in the Sun’s corona, releasing vast amounts of energy that can travel through space at extraordinary speeds.

“If a Carrington-level event occurred today, the technological and economic impacts would be orders of magnitude greater than in the 19th century.”

The Economic Stakes of Space Weather Protection

The economic vulnerability to space weather has grown with the proliferation of satellite-dependent systems and digital infrastructure. According to Lloyd’s of London, a severe solar storm could expose the global economy to losses between $1.2 trillion and $9.1 trillion, with North-America, Europe, and Asia-Pacific facing the greatest risks. These projections reflect the interconnectedness of global power grids, telecommunications, and financial systems.

Electric power grids are particularly susceptible; geomagnetically induced currents from CMEs can overload transformers and trigger cascading failures. The 1989 Quebec blackout, caused by a geomagnetic storm, left millions without power and resulted in significant economic losses, a scenario that could be far worse today. Satellite operators face risks from radiation and charging effects, with past events leading to satellite failures and service disruptions.

The aviation industry is also exposed, especially on polar routes where communication blackouts and increased radiation can force costly rerouting. Telecommunications and GPS services, which underpin everything from agriculture to finance, can be degraded or disabled during severe storms. NOAA’s economic analyses estimate that space weather forecasting services help the electric power industry avoid losses ranging from $111 million to $27 billion, depending on the severity of the event.

“Space weather forecasting is not just a scientific endeavor, it’s an economic imperative for modern society.”

Technical Innovation Behind the Surya AI Model

Surya represents a technological leap in the application of AI to solar physics. The model, named after the Sanskrit word for “sun,” features 366 million parameters and a spatiotemporal transformer architecture designed to handle the massive scale and complexity of solar observation data. Its training relied on nine years of SDO data, encompassing multiple channels and instruments that capture the Sun’s behavior in unprecedented detail.

Key innovations include spectral gating and long-short range attention mechanisms, allowing the model to capture both fine spatial details and long-term temporal dynamics. Surya is the first heliophysics foundation model to use time advancement as a pretext task, enabling it to learn the physics of solar evolution by predicting changes in solar structures over time. This is further enhanced by autoregressive rollout tuning, which improves prediction accuracy over extended timeframes.

The model’s development required specialized computational infrastructure, provided by the National Science Foundation and NVIDIA, to process petabytes of high-resolution data. Surya’s architecture supports parameter-efficient fine-tuning, allowing researchers to adapt it for tasks such as active region segmentation, solar wind forecasting, and EUV spectra prediction.

“Surya’s ability to learn the Sun’s rotation and magnetic dynamics directly from data is a breakthrough for AI-driven scientific discovery.”

Performance Capabilities and Breakthrough Results

Surya’s performance sets new benchmarks in space weather prediction. Testing shows a 16% improvement in solar flare classification accuracy over previous methods, a substantial gain in a field where accuracy directly translates to protection for critical infrastructure. The model can provide visual predictions of flare locations up to two hours in advance, giving operators more time to take protective action.

The model’s versatility extends to forecasting solar wind speeds up to four days ahead and predicting the emergence of active regions that often precede major flares. Its ability to forecast EUV spectra across 1,343 channels enables more accurate modeling of atmospheric and satellite drag conditions, benefiting both scientific research and operational planning.

Surya’s architecture allows it to generalize across multiple applications, with zero-shot evaluations demonstrating its capability to forecast solar dynamics and flare events without task-specific fine-tuning. This broad applicability reduces the resources required for specialized research and operational deployment.

“Surya’s foundation model approach accelerates research and operational forecasting, setting a new standard for space weather science.”

Strategic Partnership Between IBM and NASA

The IBM-NASA partnership exemplifies the power of public-private collaboration in scientific innovation. Building on a broader initiative to develop foundational AI models for Earth and space science, the Surya project leverages IBM’s expertise in AI architecture and NASA’s deep domain knowledge in solar physics. This collaboration has produced not only technical breakthroughs but also new models for interdisciplinary research.

Key figures such as Juan Bernabé-Moreno of IBM and Kevin Murphy of NASA have emphasized the transformative potential of AI for space science. The partnership draws on expertise from multiple institutions, including NASA’s Goddard Space Flight Center, the Jet Propulsion Laboratory, the Southwest Research Institute, and others, ensuring that Surya meets both scientific and operational requirements.

The project’s open-source approach and integration with platforms like Hugging Face and GitHub reflect a commitment to transparency and global collaboration. By making Surya accessible to researchers worldwide, IBM and NASA are fostering a more inclusive and innovative scientific community.

Open Source Accessibility and Democratic Research

Surya’s open-source release is a significant departure from proprietary AI development. By publishing the model and its datasets on platforms such as Hugging Face, GitHub, and IBM’s TerraTorch, IBM and NASA have enabled researchers everywhere to access, modify, and extend Surya for their own applications. This approach supports reproducibility, accelerates innovation, and lowers barriers for institutions with limited resources.

The availability of curated datasets and benchmarks (SuryaBench) simplifies the process of developing and evaluating new heliophysics applications. Educational institutions are already incorporating Surya into curricula, ensuring that the next generation of researchers gains practical experience with advanced AI models.

The open-source model also supports commercial innovation, allowing companies to develop new services for satellite operations, power grid management, and space weather forecasting. This democratization of technology aligns with broader trends in open science and public-private partnership.

Conclusion

The Surya Heliophysics Foundation Model represents a major advancement in space weather prediction, offering improved accuracy, longer lead times, and broad applicability across scientific and operational domains. Its development through the IBM-NASA partnership demonstrates the potential of AI to address critical vulnerabilities in modern infrastructure while advancing fundamental scientific understanding.

As Surya’s capabilities are integrated into global space weather monitoring systems and adapted for new applications, the model’s open-source nature will ensure that its benefits are widely shared. The future of space weather science is likely to be shaped by continued collaboration, technological innovation, and the democratization of advanced predictive tools, transforming solar storms from unpredictable threats into manageable risks.

FAQ

What is the Surya Heliophysics Foundation Model?
Surya is an open-source AI model developed by IBM and NASA to predict solar storms and related space weather events, using high-resolution solar observation data.

How accurate is Surya compared to previous models?
Surya improves solar flare classification accuracy by 16% over earlier methods and can provide visual predictions up to two hours in advance.

Why is space weather prediction important?
Accurate space weather prediction is vital for protecting satellites, power grids, telecommunications, and GPS systems from disruptions caused by solar storms, which can have significant economic and safety impacts.

Is the Surya model available to the public?
Yes, Surya and its datasets are available as open source on platforms like Hugging Face and GitHub, enabling global access for research and development.

What are the future implications of Surya’s release?
Surya’s success paves the way for more advanced, collaborative, and open approaches to space weather prediction, with potential benefits for scientific research, industry, and global infrastructure protection.

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Photo Credit: IBM

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Commercial Space

Dawn Aerospace Aurora Spaceplane to Support Astral Materials

Dawn Aerospace will conduct up to 100 microgravity flights for Astral Materials using the Aurora spaceplane from Oklahoma starting 2028.

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Astral Materials has selected Dawn Aerospace to conduct up to 100 microgravity test flights using the Aurora spaceplane to accelerate the development of next-generation semiconductor manufacturing hardware. The campaign, announced on September 1, 2026, will operate out of the Infinity One Oklahoma Spaceport in Burns Flat, Oklahoma.

In a press release issued on September 1, 2026, Dawn Aerospace detailed the agreement, which leverages the rapid reusability of the Aurora spaceplane to provide high-cadence microgravity testing. Astral Materials plans to use these flights to refine its microgravity furnace hardware. The system is designed to reduce gravity-driven defects, such as convection and sedimentation, during the growth of semiconductor crystals. These materials have potential applications in photonics, quantum computing, and high-power electronics.

Rapid iteration in suborbital flight

The Aurora spaceplane is designed to reach a top speed of Mach 3.7 and a maximum altitude of 100 kilometers, providing payloads with up to 127 seconds of microgravity per flight. According to the manufacturers, the vehicle supports a four-hour turnaround time between flights. This operational tempo allows researchers to conduct multiple tests within a single day.

Astral Materials Chief Technology Officer Jiya Janowitz highlighted the value of this cadence for hardware development, noting that payloads can be recovered in approximately 45 minutes.

“We can test an idea, recover it in around 45 minutes, make an adjustment on the ground and test it again later that same day. That kind of rapid iteration has never existed for microgravity manufacturing, and it fundamentally changes how quickly we can develop our technology.”

Astral Materials Chief Executive Officer Dr. Jessica Frick stated that the Aurora spaceplane provides a practical pathway to validate manufacturing systems before scaling to commercial production in orbit, where longer-duration microgravity is available.

Commercial operations and Oklahoma infrastructure

Commercial flight operations for the Astral Materials campaign are slated to begin in 2028 at the Infinity One Oklahoma Spaceport. The Oklahoma Space Industry Development Authority (OSIDA) welcomed the partnerships in an official social media statement on September 1, 2026, emphasizing the state’s focus on attracting high-cadence commercial spaceflight operations.

This agreement follows an April 16, 2026, announcement in which Dawn Aerospace and OSIDA launched the Suborbital Spaceplane Challenge. That initiative offered United States researchers up to 25 flights aboard the Aurora spaceplane to stimulate utilization of the Oklahoma facility.

Dawn Aerospace Chief Executive Officer Stefan Powell noted that routine access is required to transition microgravity manufacturing from a scientific curiosity to a viable industry, comparing the need for rapid experimentation to previous industrial revolutions.

AirPro News analysis

The partnership between Dawn Aerospace and Astral Materials highlights a critical gap in the current space manufacturing ecosystem. While orbital platforms like the International Space Station offer long-duration microgravity, the cost and lead times associated with orbital launches prohibit the rapid trial-and-error necessary for hardware development. Suborbital spaceplanes like Aurora serve as an essential stepping stone. By providing brief but frequent periods of microgravity, these vehicles allow companies to validate complex systems before committing to expensive orbital deployments.

We note a minor discrepancy in Dawn Aerospace’s published materials regarding the commencement of operations at the Oklahoma site. The main announcement targets 2028 for commercial flights, while the company’s boilerplate text references 2027. Regardless of the exact start date, establishing a reliable suborbital testbed will be vital for the commercial viability of in-space manufacturing applications.

Sources: Dawn Aerospace

Photo Credit: Dawn Aerospace

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Space & Satellites

NASA X-59 Completes 25th Flight, Enters Acoustic Validation

NASA’s X-59 quiet supersonic aircraft finished initial envelope expansion and moves to acoustic validation for the Quesst mission.

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The National Aeronautics and Space Administration (NASA) X-59 quiet supersonic experimental aircraft completed its 25th test flights on August 21, 2026, validating aerodynamic models and clearing the way for the program’s critical acoustic validation phase.

In a press release issued on September 4, 2026, the agency confirmed the milestone marks the conclusion of initial envelope expansion for the centerpiece of the Quesst mission. The X-59 is designed to cruise faster than the speed of sound while producing a muted sonic thump rather than a disruptive sonic boom. Data collected during the upcoming flight phases will be shared with U.S. and international regulators to inform new noise thresholds, which could eventually lead to the lifting of the ban on commercial supersonic flight over land.

Flight envelope expansion and performance

During the 72-minute test flight originating from NASA’s Armstrong Flight Research Center in Edwards, California, the X-59 reached a speed of Mach 1.2 and an altitude of 49,000 feet. The flight followed a rapid envelope expansion campaign over the summer. The aircraft achieved its first supersonic flight on June 5, 2026, and reached its target cruise conditions of Mach 1.4 (924 mph) and 55,000 feet on June 12, 2026.

NASA Test Pilot Nils Larson described the test flights as “exciting but uneventful,” noting that the aircraft “likes to fly fast.”

The initial 25 flights focused on proving the airworthiness and baseline performance of the unique airframe, which was built by prime contractor Lockheed Martin and powered by a General Electric GE-F414 engine.

“Through our ongoing flight tests with the X-59, we’ve gained invaluable insights into both the aircraft’s performance and the unique challenges of the aircraft design,” said Cathy Bahm, Project Manager for the NASA Low Boom Flight Demonstrator project. “Each test point has validated our models and predictions, and it has strengthened our confidence in the aircraft’s performance.”

Transitioning to acoustic validation

With baseline performance established, the Quesst mission will now shift focus to measuring the sound produced by the aircraft. During the acoustic validation phase scheduled for later this year, NASA will utilize ground- and air-based tools to measure the sonic thumps generated by the X-59 at supersonic cruise speeds.

The objective is to verify that the physical aircraft meets the low-boom design targets established by computer modeling.

“This is the phase we’ve been working toward,” said Larry Cliatt, Acoustic Validation Technical Lead for the NASA Quesst mission. “Building and flying a brand-new aircraft is an extraordinary accomplishment, but the next phase is where the real research begins.”

Cliatt noted that the acoustic validation campaign will be complex and demanding. The tools and methods used to design the X-59 will be put to the test, potentially forming the foundation for future commercial supersonic aircraft development.

AirPro News analysis

The successful completion of the X-59’s initial flight test phase marks a pivotal transition for the Quesst mission. We view the upcoming acoustic validation phase as the true test of the program’s value to the broader aerospace industry. While building a supersonic demonstrator is a significant engineering feat, the X-59 is fundamentally a data-gathering tool. If the acoustic measurements match NASA’s models, the agency will possess the empirical evidence required by the Federal Aviation Administration (FAA) and the International Civil Aviation Organization (ICAO) to establish noise-based certification standards. Establishing these standards is the mandatory first step toward opening overland routes to a new generation of commercial supersonic aircraft.

Sources: NASA Quesst Blog

Photo Credit: NASA

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Space & Satellites

NASA Awards Blue Origin $700M Mars Telecommunications Contract

NASA selected Blue Origin to build the Mars Telecommunications Orbiter on its Blue Ring platform for up to $700 million.

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The National Aeronautics and Space Administration (NASA) has awarded Blue Origin a firm-fixed-price contract valued at up to $700 million to develop the Mars Telecommunications Network (MTN). The agreement, finalized on September 1, 2026, tasks the aerospace manufacturer with delivering a dedicated Mars Telecommunications Orbiter (MTO) by December 31, 2028, to replace the agency’s aging interplanetary relay infrastructure.

In a press release issued on September 2, 2026, Blue Origin confirmed the orbiter will be built on its Blue Ring spacecraft platform. The new network is designed to provide continuous, high-speed communications for future robotic and crewed missions under NASA’s broader Moon to Mars exploration strategy. The Space Communications and Navigation (SCaN) program expects the MTO to become operational in Mars orbit by 2030.

Replacing legacy Mars infrastructure

NASA’s current communications relay at the Red Planet relies heavily on legacy spacecraft, specifically the Mars Odyssey launched in 2001 and the Mars Reconnaissance Orbiter launched in 2005. The MTN contract aims to establish a modern, high-bandwidth foundation for sustained exploration in the coming decades. NASA officials stated the award marks a milestone in the agency’s strategy to expand communications and navigation services beyond Earth and the moon.

The competition for the MTN contract, initiated via a request for proposal in May 2026, was restricted by the July 2025 budget-reconciliation package. Bidding was limited to the eight companies that participated in the 2024 and 2025 commercial Mars sample return studies. Funding for the project was authorized by Congress through the Working Families Tax Cut Act.

Blue Ring platform and technical specifications

Blue Origin will utilize its Blue Ring spacecraft architecture for the MTO. The platform features hybrid solar electric and chemical (SEP-Chem) propulsion, enabling it to deploy multiple payloads and establish infrastructure ahead of human arrival. The spacecraft can carry a payload exceeding 1,000 kilograms to Mars orbit.

Production of the MTO is underway at Blue Origin’s dedicated manufacturing facility in Huntsville, Alabama. The facility is currently sized to produce four Blue Ring vehicles per year. The MTO will also feature a 20-kilogram dedicated payload capacity available for science instruments or deployable cubesats.

“MTO is the backbone of America’s Mars exploration program for the next decade and beyond and will provide the reliable communications capacity that will keep future robotic and human missions connected to each other and to Earth,” said Tory Bruno, President of Blue National Security.

Bruno added that the contract award validates the company’s development of the Blue Ring platform, noting that the hardware is ready for this specific mission profile.

AirPro News analysis

We view this $700 million contract as a critical validation of Blue Origin’s Blue Ring spacecraft program and its broader pivot toward deep space infrastructure. By securing a foundational role in the Mars Telecommunications Network, Blue Origin positions itself as an essential utility provider for all future NASA Mars operations. The aggressive delivery timeline of December 31, 2028, will test the production capabilities of the Huntsville facility, but successfully deploying the MTO would cement the company’s status as a primary contractor for interplanetary logistics.

Sources: Blue Origin

Photo Credit: Blue Origin

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