Defense technology company Anduril Industries announced on March 11, 2026, that it has signed a definitive agreement to acquire ExoAnalytic Solutions, a firm specializing in space situational awareness and missile defense tracking. The acquisition will significantly expand Anduril’s presence in the space surveillance market and support the company’s ambitions in national security capabilities.
ExoAnalytic Solutions, based in Orange County, California, provides satellite and missile tracking services to government and commercial customers. The company operates a network of sensors capable of detecting, tracking, and cataloging objects in Earth orbit. This capability has become increasingly important as concerns grow about orbital congestion, potential collisions, and the militarization of space.
Anduril plans to fully absorb ExoAnalytic, adding approximately 130 employees to its space sector workforce. The company stated that the acquisition will significantly scale the impact available for national security missions. The deal aligns with broader Pentagon interests in enhancing space-based surveillance and tracking capabilities.
The acquisition comes amid heightened U.S. government focus on space domain awareness. The Department of Defense maintains the United States Space Surveillance Network, which tracks objects larger than approximately 10 centimeters in low Earth orbit and larger objects at greater distances. Commercial providers like ExoAnalytic supplement government capabilities with additional sensor networks and data analysis services.
Anduril has positioned itself as a defense technology disruptor, developing autonomous systems, sensors, and software for military applications. The company has expanded rapidly in recent years, pursuing contracts across multiple domains including air defense, maritime surveillance, and now space operations.
The deal also reflects growing interest in space-based assets for missile defense and early warning purposes. ExoAnalytic’s tracking capabilities can support detection of missile launches, trajectory prediction, and assessment of reentry vehicles. These functions align with U.S. missile defense architecture and have gained urgency given evolving global threat landscapes.
Industry analysts note that consolidation in the space surveillance market reflects broader trends in defense contracting, where established primes and emerging technology companies are competing to provide capabilities for next-generation military space systems. Anduril’s acquisition of ExoAnalytic positions the company to compete for contracts related to the U.S. Space Force’s space surveillance and tracking requirements.
The announcement did not disclose financial terms of the acquisition. Anduril stated that ExoAnalytic will continue operating from its current locations while integrating into Anduril’s broader platform and capabilities portfolio.
SpaceX has completed cryoproof testing of the Starship upper stage assigned to the next flight, designated Ship 39, moving the company closer to its first Starship launch of 2026. During testing the week of March 7, 2026, engineers examined the vehicle’s redesigned propellant system and its structural strength, including squeeze tests that mimic the forces involved in future ship catches by the Mechazilla arms at Starbase in Texas.
CEO Elon Musk stated on social media that the launch is approximately four weeks away, targeting April 2026 for Flight 12. This marks another delay from earlier projections, as the company continues to refine the vehicles and procedures necessary for the massive fully-stacked Starship system.
The testing conducted in early March represented one of the final major milestones before the launch authorization process begins. SpaceX has pursued an aggressive testing schedule with Starship, using each flight to gather data and implement improvements for subsequent vehicles. Ship 39 incorporates several design changes from earlier test articles, particularly in the propellant storage and delivery systems that are critical to achieving the vehicle’s performance goals.
Starship consists of two stages: the Super Heavy booster and the Starship upper stage. Together, the system stands approximately 123 meters tall and uses liquid methane and liquid oxygen as propellants. The vehicle is designed to be fully reusable, with both stages intended to return to Earth for refurbishment and reflight. This reusability is central to SpaceX’s vision for dramatically reducing the cost of accessing space.
The company has conducted six full-stack Starship flights to date, with varying degrees of success. Each mission has provided engineering data that informed modifications to later vehicles. The program has progressed from initial short hops to increasingly complex maneuvers, including attempts at booster catches using the tower-based Mechazilla system.
SpaceX operates Starship from its Starbase facility in Boca Chica, Texas, where the company has constructed extensive production and launch infrastructure. The location on the Gulf Coast provides access to convenient launch trajectories and recovery areas. The company has also received approval to launch Starship from Kennedy Space Center Launch Complex 39A for future missions.
NASA’s Artemis program depends on a human-rated version of Starship serving as the lunar lander for Artemis III and subsequent missions. The space agency selected Starship for this critical role based on its technical capabilities and development progress. Continued successful testing of the SpaceX system remains important to NASA’s lunar exploration timeline.
The upcoming Flight 12 will represent another step in SpaceX’s iterative development approach, gathering additional data on vehicle performance and operational procedures. The company has not announced specific objectives for the mission beyond the standard goals of testing flight characteristics and system reliability.
On March 16, 2026, the space community marks the 100th anniversary of Dr. Robert H. Goddard’s historic first flight of a liquid propulsion rocket. This milestone represents one of the most significant moments in the history of rocketry, comparable to the Wright Brothers’ first powered airplane flight at Kitty Hawk in 1903. The anniversary provides an opportunity to reflect on Goddard’s pioneering contributions and their lasting impact on modern space exploration.
Goddard launched the world’s first liquid-fueled rocket in Auburn, Massachusetts, on that March morning in 1926. The rocket climbed 41 feet and traveled 184 feet in just 2.5 seconds before landing. While modest by today’s standards, this flight demonstrated the fundamental principle that would enable humanity to reach space. From 1930 to 1941, Goddard continued developing increasingly sophisticated rockets, eventually achieving altitudes of 2,400 meters, approximately 1.5 miles, while refining guidance systems, welding techniques, insulation, and propulsion components.
The advances in rocket propulsion, guidance, and control that Goddard pioneered throughout the 1920s and 1940s formed the foundation for virtually every modern launch vehicle and in-space propulsion system. Communications satellites, human spaceflight, the Apollo Moon landings, robotic exploration of the solar system, space astronomy, the Space Shuttle, Earth observation satellites, space stations, GPS navigation, and orbital space tourism all trace their technological lineage to Goddard’s early work in liquid propulsion.
Alan Stern, planetary scientist and leader of NASA’s New Horizons mission to the Kuiper Belt, wrote about the significance of Goddard’s contributions in Aerospace America. Stern noted that it is profoundly regrettable that Goddard’s pioneering work was largely unappreciated during his lifetime. Goddard passed away in 1945, before witnessing the rapid advancement of rocketry in the 1950s and 1960s that led to satellites, human space travel, and eventually Moon landings.
Today, with a century of progress and perspective since that first flight, the space community can more clearly appreciate the profound and pivotal nature of Goddard’s contributions. The Goddard Centennial offers an occasion for celebration across the global space community, including space companies, government agencies, professional societies, and educational institutions.
Throughout March 2026, rocket clubs across the United States, including the National Association of Rocketry, the Tripoli Rocketry Association, and the American Rocketry Challenge, will launch rockets to honor Goddard’s achievements. Events are planned at the original launch site in Auburn, Massachusetts, and at the Hanover Theatre and Conservatory in Worcester. These celebrations provide opportunities to share the significance of Goddard’s contributions with the public, students, and future generations of engineers and scientists.
Goddard’s legacy extends beyond his technical achievements. His perseverance against doubters and critics, his inventive approach to engineering challenges, and his dedication to advancing the field of rocketry continue to inspire those working in space exploration today. As the industry looks toward the next century of spaceflight, Goddard’s example reminds practitioners of the importance of persistence, innovation, and technical rigor.
The Roman Space Telescope was conceived with an ambitious goal: to observe vast regions of the sky with the clarity of a space telescope while capturing an enormous field of view. Previous missions such as Hubble and the James Webb Space Telescope excel at examining small patches of sky with extraordinary detail. Roman, by contrast, is designed to combine high resolution with panoramic scale. Its observations will reveal patterns in the structure of the universe that cannot be seen when focusing on individual objects alone.
The mission itself is built around the idea that the universe contains more than meets the eye. For nearly a century, astronomers have known that the visible matter—stars, planets, gas, and dust—accounts for only a small fraction of the cosmos. Most of the universe appears to be made of mysterious components known as dark matter and dark energy. Dark matter exerts gravitational influence but emits no detectable light. Dark energy, even more mysterious, seems to drive the accelerated expansion of the universe itself. Roman’s mission is to help uncover the nature of these invisible forces.
The engineering behind Roman reflects the scale of its ambitions. At the heart of the telescope sits a 2.4-meter primary mirror, similar in size to the one used on Hubble. However, Roman pairs that mirror with an instrument designed to capture images across an enormous portion of the sky. Its Wide Field Instrument is the largest camera ever sent into space for astronomical observation, composed of an array of advanced infrared detectors that together create a massive imaging mosaic. Each image Roman captures will cover an area of sky about one hundred times larger than a typical Hubble image, while still maintaining comparable resolution.
The spacecraft will operate from a stable orbit around the Sun–Earth L2 Lagrange point, roughly 1.5 million kilometers from Earth. This location provides a thermally stable environment, minimal interference from Earth’s atmosphere, and a continuous view of deep space. It is the same region where the James Webb Space Telescope operates, and it offers an ideal vantage point for long-term astronomical surveys. From this distant perch, Roman will quietly collect vast amounts of data, building a map of the universe that extends across billions of light-years.
Roman’s ability to survey the sky on such a grand scale is essential for studying dark matter. Although dark matter cannot be observed directly, its presence reveals itself through gravity. One of the most powerful tools for detecting it is gravitational lensing, a phenomenon predicted by Einstein’s theory of general relativity. When light from distant galaxies passes near massive structures such as galaxy clusters, the curvature of spacetime bends the light’s path. This bending subtly distorts the shapes of background galaxies. By measuring these distortions across millions or even billions of galaxies, astronomers can reconstruct the distribution of dark matter that caused the lensing effect.
This technique requires enormous statistical power. A single galaxy’s distortion is tiny and easily masked by noise or natural variation. But when measurements are repeated across vast areas of sky, patterns begin to emerge. Roman’s wide field of view allows it to collect the massive datasets required to trace the cosmic web—the vast network of dark matter filaments that connect galaxies and clusters throughout the universe. With Roman’s observations, scientists will be able to map the invisible scaffolding upon which galaxies form and evolve.
Dark energy presents an even deeper challenge. Observations over the past few decades have revealed that the expansion of the universe is accelerating. Instead of slowing down under the influence of gravity, cosmic expansion is speeding up. This discovery led scientists to propose the existence of dark energy, a mysterious form of energy permeating space itself. Yet its nature remains unknown.
Roman will investigate dark energy through several complementary methods. One approach involves measuring the large-scale distribution of galaxies across cosmic time. By mapping how galaxies cluster together, astronomers can track how structures grow as the universe evolves. If dark energy influences the expansion of space, it will also influence how quickly galaxies gather into clusters and filaments.
Another method involves observing distant supernovae, particularly Type Ia supernovae, which serve as cosmic distance markers. Because these stellar explosions have nearly uniform brightness, they allow astronomers to measure how far away their host galaxies are. By comparing distance measurements with the galaxies’ redshifts—the stretching of light caused by cosmic expansion—scientists can determine how the expansion rate of the universe has changed over billions of years.
Roman’s wide surveys will detect thousands of such supernovae, dramatically improving the statistical precision of these measurements. Combined with gravitational lensing studies and galaxy mapping, the telescope will provide multiple independent ways of probing dark energy’s influence.
The telescope will also contribute to the search for exoplanets through gravitational microlensing, an observational technique that detects planets when their gravity briefly magnifies the light of distant stars. While this aspect of the mission is not directly related to dark matter or dark energy, it demonstrates Roman’s versatility as a survey instrument capable of exploring multiple frontiers of astrophysics.
Perhaps the most exciting aspect of Roman’s mission is its potential for discovery. When astronomers open a new window on the universe, unexpected phenomena often follow. Hubble revealed distant galaxies that challenged existing theories of cosmic evolution. Webb has already begun uncovering surprising details about the earliest galaxies. Roman’s surveys, covering enormous areas of sky with unprecedented precision, may reveal entirely new cosmic structures or patterns that reshape our understanding of the universe.
The telescope stands as a tribute to Nancy Grace Roman’s vision. During the early years of NASA, she advocated for space-based astronomy at a time when many believed ground telescopes were sufficient. Her efforts helped pave the way for Hubble and for the entire field of modern space astronomy. The telescope that now bears her name continues that legacy by pushing the boundaries of what we can measure and understand.
When Roman begins its mission, it will not simply observe the universe—it will chart it. The telescope will map the invisible architecture of dark matter, measure the subtle fingerprints of dark energy, and provide astronomers with an unprecedented dataset describing the large-scale structure of the cosmos.
In doing so, Roman will help humanity confront one of the greatest mysteries in science: that most of the universe is made of something we cannot see. Yet by carefully measuring the light from distant galaxies, by tracing the curvature of spacetime itself, and by building a detailed map of cosmic structure, the telescope may bring us closer than ever to understanding the hidden forces shaping the universe.
In the history of astronomy, certain instruments do more than gather light — they reshape perspective. The Hubble Space Telescope revealed a universe of breathtaking clarity and depth. The James Webb Space Telescope opened a new infrared frontier, peering into the earliest epochs of galaxy formation. And now, standing on the shoulders of those giants, NASA’s Nancy Grace Roman Space Telescope prepares to widen our cosmic view in a way no space observatory has done before.
Named after Nancy Grace Roman, NASA’s first Chief of Astronomy and one of the architects of the Hubble program, the Roman Space Telescope is built on a bold premise: if we want to understand the structure and fate of the universe, we must not only see deeply — we must see broadly. Roman is not designed to zoom in on a single galaxy with exquisite detail. Instead, it is built to survey immense swaths of the sky with Hubble-level sharpness, combining resolution and scale in a way that has never before been achieved.
At the heart of Roman is a 2.4-meter primary mirror — the same diameter as Hubble’s — but paired with a field of view nearly one hundred times larger. That combination defines the mission. Where Hubble sees a small patch of sky in exquisite detail, Roman will see vast cosmic landscapes with comparable clarity. It is as though we have replaced a telescope’s keyhole view with a panoramic window.
The mission has two central scientific pillars. The first is to investigate the nature of dark energy, the mysterious force driving the accelerated expansion of the universe. The second is to conduct a census of exoplanets through gravitational microlensing, extending our knowledge of planetary systems far beyond what current techniques allow. Together, these goals address some of the most profound questions in modern astrophysics: What is the universe made of? How did it evolve? And how common are worlds like our own?
The engineering behind Roman reflects the demands of those ambitions. The telescope’s Wide Field Instrument is its primary scientific eye, operating in near-infrared wavelengths. This wavelength range is critical because it allows astronomers to observe distant galaxies whose light has been stretched, or redshifted, by cosmic expansion. The instrument consists of eighteen state-of-the-art infrared detectors arranged in a mosaic, creating a detector array of enormous scale and sensitivity. Each exposure captures a sky area equivalent to dozens of Hubble images stitched together — except it happens all at once.
The spacecraft itself is designed for precision and stability. Roman will operate in a Sun-Earth L2 orbit, approximately 1.5 million kilometers from Earth. This location provides a thermally stable environment, continuous sunlight for solar power, and a steady observational platform free from Earth’s shadow. Maintaining exquisite pointing accuracy is essential; even slight jitter would compromise measurements of subtle cosmic distortions. Advanced reaction wheels, gyroscopes, and fine guidance sensors work together to ensure the telescope holds its gaze with extraordinary steadiness.
One of Roman’s most important capabilities is its ability to measure weak gravitational lensing. According to Einstein’s general theory of relativity, mass bends spacetime, and light traveling through that curved spacetime follows the distortion. When light from distant galaxies passes near massive structures such as galaxy clusters or dark matter halos, its path is subtly altered. By statistically analyzing the shapes of millions of galaxies across vast areas of sky, Roman will map the invisible distribution of dark matter and trace how cosmic structures have grown over billions of years.
This mapping is essential for understanding dark energy. The rate at which cosmic structures form and evolve is influenced by the balance between gravity, which pulls matter together, and dark energy, which pushes space apart. Roman will measure this balance with unprecedented statistical power, surveying thousands of square degrees of sky and collecting data from billions of galaxies. The resulting dataset will refine our understanding of cosmic expansion and test whether dark energy behaves like Einstein’s cosmological constant or something more exotic.
At the same time, Roman will search for planets in a way unlike any previous mission. Most exoplanet discoveries have relied on transit photometry, observing the dimming of a star as a planet crosses its face, or radial velocity measurements that detect the gravitational tug of an orbiting planet. Roman’s microlensing survey will instead exploit a phenomenon predicted by general relativity: when a foreground star passes in front of a more distant background star, its gravity magnifies the background star’s light. If the foreground star hosts a planet, that planet can create a distinctive, temporary signature in the magnified light curve.
This technique is uniquely sensitive to planets at greater distances from their stars, including cold, Earth-mass planets and even free-floating planets that drift through space unbound to any star. Roman is expected to discover thousands of new worlds, filling in a region of planetary parameter space that remains largely unexplored. In doing so, it will help astronomers build a more complete picture of planetary system formation and diversity.
Roman will also carry a coronagraph instrument, a technology demonstration designed to block out the light of a star and directly image faint nearby exoplanets. While primarily experimental, the coronagraph will test technologies essential for future missions aimed at imaging Earth-like planets and analyzing their atmospheres for signs of habitability or life.
Perhaps what makes Roman most exciting is the scale of its data. It is not simply another observatory; it is a survey engine. The volume of information it will collect will fuel research for decades, enabling discoveries not yet imagined. Just as the Hubble Deep Field revealed galaxies that challenged cosmological models, Roman’s wide-field surveys are likely to uncover unexpected structures, rare objects, and statistical anomalies that reshape theoretical frameworks.
In many ways, the Roman Space Telescope represents the maturation of space astronomy. It is not designed solely for spectacle, though it will undoubtedly produce stunning images. It is built for measurement — precise, repeatable, statistically robust measurement. It embodies a shift from isolated observations to cosmic cartography.
When Roman opens its wide eye to the sky, it will not simply extend our reach deeper into space. It will expand our view sideways, revealing the structure of the universe at scales we have only begun to comprehend. In doing so, it will continue a legacy that Nancy Grace Roman herself helped establish: that by investing in bold, carefully engineered observatories, we do more than observe the cosmos — we learn to understand our place within it.
The American Institute of Aeronautics and Astronautics has released a groundbreaking report identifying ten technologies that will fundamentally reshape aerospace operations, manufacturing, and services over the next two decades. The comprehensive study, titled “Technologies Transforming Aerospace,” draws on insights from over 700 aerospace professionals and nearly two dozen senior technology leaders across industry, academia, and government. This represents the most extensive survey of its kind, capturing the collective wisdom of the aerospace community on the technologies that will define the future of flight and opening new frontiers in how we think about aviation and space exploration. The findings represent a consensus view of where the industry is heading.
Leading the list is AI-Aided Advanced Design and Engineering, which promises to revolutionize how aircraft and spacecraft are conceived and optimized. Machine learning algorithms can now explore design spaces that would take human engineers centuries to examine, leading to more efficient structures, improved aerodynamics, and innovative configurations that were previously unimaginable. This technology is already accelerating development cycles and reducing the cost of bringing new aerospace vehicles from concept to certification. The implications for the industry are profound, potentially democratizing aerospace design by making advanced tools accessible to smaller organizations that previously lacked the resources for extensive simulation and testing.
Alternative Aviation Fuels and Electric Aircraft represent the industry’s response to the imperative of decarbonization. As climate concerns intensify and regulatory pressure increases, aerospace engineers are developing propulsion systems that dramatically reduce carbon emissions. Electric aircraft, once considered science fiction, are now transitioning from experimental prototypes to viable commercial platforms for short-haul routes. The technology is maturing rapidly, with several manufacturers announcing plans for regional electric aircraft within the decade. This represents a fundamental shift in how we think about aircraft propulsion and could eventually transform the entire aviation industry.
Fully Reusable Launch Systems continue to transform the economics of space access. The success of SpaceX’s Falcon 9 has proven the concept, and numerous companies worldwide are developing their own reusable rockets. This technology is democratizing space, making it accessible to smaller nations and private companies that previously could not afford launch services. The economic implications are profound, potentially reducing launch costs by an order of magnitude and enabling entirely new categories of space-based applications that were previously economically unfeasible. The space economy is expanding rapidly as a result.
High-Temperature Materials and Hypersonic Propulsion are enabling the next generation of military and civilian aircraft capable of traveling at incredible speeds. Hypersonic vehicles that can traverse the globe in hours are moving from laboratory concepts to operational systems, potentially revolutionizing air travel and strategic capabilities. The materials required to survive the extreme temperatures generated by hypersonic flight represent a significant engineering challenge that is now being overcome through advances in ceramics, composites, and thermal management systems. This technology could compress international travel times dramatically and reshape global connectivity.
In-Space Manufacturing and Space Nuclear Power and Propulsion represent the frontier technologies that will enable permanent human presence beyond Earth. Manufacturing products in the microgravity environment of orbit opens possibilities impossible on our planet, from advanced materials to pharmaceuticals that cannot be produced in terrestrial environments. Nuclear propulsion could reduce travel times to Mars from months to weeks, making deep space exploration more practical and safe. These technologies remain in earlier stages of development but hold tremendous promise for the future of space exploration and could fundamentally change humanity’s relationship with the solar system.
The remaining technologies on the list Quantum Computing and Sensing, and Pilotless Aircraft round out a picture of an industry undergoing rapid transformation. Quantum computing will accelerate the development of all other technologies by enabling calculations currently impossible with classical computers, potentially revolutionizing everything from materials science to mission planning. Pilotless aircraft will transform both military and civilian aviation, potentially making air travel safer and more efficient while raising important questions about the role of human operators in aviation. The social and regulatory implications of this technology will be as significant as the technical ones.
The report emphasizes that these technologies are not developing in isolation but are converging to create unprecedented capabilities. The synergies between artificial intelligence, advanced materials, and new propulsion systems are creating opportunities that none of these technologies could achieve alone. For aerospace professionals and enthusiasts alike, this report provides a roadmap for understanding the technological landscape that will shape the next twenty years of aviation and space exploration. The future of aerospace is being written today, and these technologies will be the chapters that define it.
The convergence of these technologies also raises important questions about workforce development and education. As the aerospace industry transforms, the skills required for success are evolving rapidly. Engineers and technicians will need to become proficient in artificial intelligence, advanced materials science, and new propulsion technologies. Universities and training programs are already adapting their curricula to prepare the next generation of aerospace professionals for this transformed industry. The workforce implications are as significant as the technological ones.
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