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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.

Astronomy often reveals the universe in slow motion. Galaxies drift apart over billions of years, stars evolve over millions, and planetary systems assemble over spans so vast that human observers usually see only the end results. Yet every once in a while, the cosmos offers a fleeting glimpse of something far more dynamic. NASA’s Hubble Space Telescope has captured such a moment near the bright star Fomalhaut, observing what appears to be the aftermath of a massive collision between two large bodies in a distant planetary system. It is a rare cosmic accident caught almost in real time, and it offers scientists an extraordinary opportunity to study how planetary systems evolve through violence as much as through calm.

Fomalhaut itself is not an obscure star. Located roughly twenty-five light-years away in the constellation Piscis Austrinus, it is one of the brightest stars visible in Earth’s night sky. Astronomers have long known that Fomalhaut is surrounded by a vast disk of debris composed of dust, ice, and rocky fragments. Such debris disks are thought to be the leftover building materials of planetary systems, similar to the asteroid belt and Kuiper Belt in our own Solar System. Within these disks, countless objects—from dust grains to planet-sized bodies—move along intersecting paths, occasionally colliding and reshaping the architecture of the system.

For years, astronomers suspected that something unusual was happening inside the Fomalhaut system. In 2008, Hubble captured images of what appeared to be a faint object moving within the debris disk, initially thought to be a possible exoplanet. However, as scientists continued to observe the region over the following years, the object behaved strangely. Instead of remaining compact like a planet, it gradually expanded and faded. The mysterious cloud appeared to grow larger while becoming dimmer, suggesting that it was not a solid body at all, but rather an expanding cloud of dust created by a catastrophic collision.

The idea that Hubble might have witnessed the aftermath of a massive collision between two planetary building blocks was both surprising and exciting. Planetary collisions are thought to be common during the early stages of solar system formation. Our own Moon likely formed when a Mars-sized body struck the young Earth billions of years ago. But observing such an event directly in another star system has proven extraordinarily difficult. The distances involved, combined with the relatively small size of planetary bodies, usually make these collisions invisible to telescopes. What Hubble saw near Fomalhaut may represent the first clear observation of the debris from a large-scale collision unfolding over time.

Understanding this event requires both scientific insight and remarkable engineering. The Hubble Space Telescope, launched in 1990 and operating more than 500 kilometers above Earth, was designed to observe the universe without the distortions caused by Earth’s atmosphere. Its 2.4-meter mirror collects light with extraordinary clarity, and its suite of cameras and spectrographs allows astronomers to study objects across multiple wavelengths. Over the decades, upgrades performed by astronauts during servicing missions transformed Hubble into one of the most capable astronomical observatories ever built.

The observations of the Fomalhaut collision relied on Hubble’s ability to capture extremely high-contrast images. Observing faint structures near bright stars is notoriously difficult because the star’s glare overwhelms nearby objects. To overcome this problem, Hubble uses a technique called coronagraphy. A coronagraph blocks the intense light from a star, allowing astronomers to see faint material orbiting nearby. With this method, Hubble was able to reveal the faint expanding cloud of debris around Fomalhaut.

By comparing images taken over several years, scientists noticed that the dust cloud was moving outward and expanding. Careful analysis showed that the cloud’s growth was consistent with the debris from a collision between two large objects, likely hundreds of kilometers in diameter. When such bodies collide at high speeds—often several kilometers per second—the impact releases enormous energy. Instead of forming a single merged object, the bodies can shatter, producing a spray of fragments and dust that expands outward into space.

Computer models helped researchers reconstruct what might have happened. In the dense debris disk surrounding Fomalhaut, two large planetesimals—primitive building blocks of planets—may have crossed paths. The collision would have instantly vaporized or shattered large portions of both bodies, sending material outward in a rapidly expanding cloud. Over time, radiation from the star and interactions with surrounding dust gradually disperse the debris, causing the cloud to expand and fade until it eventually becomes indistinguishable from the background disk.

What makes the Fomalhaut event so compelling is that it offers a glimpse of the chaotic processes that shape planetary systems. Planet formation is often described as a gradual process in which small particles stick together and slowly grow into larger bodies. Yet collisions play an equally important role. Throughout the history of a planetary system, impacts can destroy worlds as easily as they create them. Asteroids collide, planetary embryos merge, and occasionally entire planets can be reshaped or even obliterated.

Observations like this one help astronomers understand how often such events occur and how they influence the final arrangement of planets. The Fomalhaut debris disk is thought to resemble the early Solar System billions of years ago, when Earth, Mars, and the other rocky planets were still forming. Watching a collision unfold in that distant system is almost like peering back into our own planet’s past.

The event also highlights the importance of long-term observations. Hubble did not capture a single dramatic explosion. Instead, it recorded subtle changes over many years, allowing scientists to piece together the story gradually. The expanding cloud revealed itself through patience and persistence, reminding us that astronomy often advances through careful observation rather than sudden discovery.

Even after more than three decades in orbit, Hubble continues to produce groundbreaking science. Its ability to track faint objects over long periods makes it uniquely suited to studying phenomena like the Fomalhaut collision. Newer observatories such as the James Webb Space Telescope may provide additional insights by observing the system in infrared wavelengths, where warm dust and debris are easier to detect.

For now, the expanding cloud around Fomalhaut remains a rare window into the violent processes that shape planetary systems. It reminds us that the serene appearance of the night sky hides a universe filled with collisions, transformations, and dramatic events. Somewhere in the distant reaches of that system, two ancient bodies met in a catastrophic encounter, scattering fragments across space. And thanks to the engineering triumph of the Hubble Space Telescope, humanity has been able to witness the aftermath of that cosmic crash unfolding light-years away.

Video credit: NASA Goddard

The microgravity research sector crossed $4 billion in market value during early 2026, according to industry analysis published in March. This milestone reflects growing commercial interest in conducting scientific experiments and manufacturing processes in orbital environments where gravity’s effects are dramatically reduced.

Commercial satellite launches have accelerated at approximately 15 percent annually, according to the same analysis, creating expanded infrastructure for payload deployment and in-orbit operations. The convergence of more launch opportunities and increased research interest is driving investment in dedicated commercial space platforms.

The International Space Station remains the primary venue for microgravity research, hosting experiments from NASA, ESA, JAXA, and commercial customers. However, private stations planned for launch later in the decade will add significant capacity. Companies including Axiom Space, Voyager Space, and Orbital Reef are developing commercial orbital outposts designed specifically for research and manufacturing.

Research conducted in microgravity spans multiple disciplines. Protein crystallization experiments have demonstrated improved crystal quality compared to Earth-based methods, potentially accelerating pharmaceutical development. Materials processing leverages the absence of convection and sedimentation to create novel alloys and optical components. Biological studies examine how organisms adapt to spaceflight, providing insights relevant to long-duration human space missions.

The United Kingdom opened a microgravity research centre in Swansea in March 2026, joining a growing list of national programs supporting orbital science. Space Forge, a UK-based company, successfully generated plasma in orbit in late 2025, demonstrating conditions necessary for advanced crystal growth aboard commercial spacecraft. Such capabilities could eventually enable manufacturing processes impractical on Earth.

Defense contractors have also increased investment in orbital research, driven by applications including advanced materials for aircraft and spacecraft, sensors for surveillance systems, and fundamental physics investigations. The intersection of commercial and defense interests is creating a broader industrial base for space-based research.

The $4 billion figure encompasses launch services, orbital platform operations, experiment hardware, and downstream data analysis. Market researchers project continued growth as more commercial stations come online and as pharmaceutical and materials companies demonstrate returns on orbital research investments. Whether the sector maintains current growth rates will depend partly on launch cost trends and the success of early commercial station deployments.

NASA Administrator Jared Isaacman announced sweeping changes to the Artemis program in late February 2026, reshaping the path to lunar exploration. The overhaul aims to restore momentum, reduce technical risk, and establish a sustainable cadence for crewed lunar missions. Industry partners have largely endorsed the streamlined approach, though aligning the extensive SLS supply chain and workforce to the new plan presents implementation challenges.

The revised plan standardizes hardware configurations, adds a critical integrated systems test flight, increases launch cadence to roughly one SLS mission every 10 months, and maintains the target for the first crewed lunar landing in 2028, potentially with two landings that year.

Artemis II remains the immediate priority. The first crewed Orion flight will loop around the Moon, with launch now targeted for April 2026. The SLS upper stage, known as ICPS, was rolled back to the Vehicle Assembly Building after a helium leak caused by a dislodged seal in the quick-disconnect system was identified during preparations. Repairs required special access platforms in High Bay 3, with rollout to Launch Pad 39B projected around March 19, 2026. It was during this repair period that Isaacman announced the comprehensive replan.

The most significant change affects Artemis III. Originally planned as the first crewed lunar landing in 2027, the mission has been reconfigured as an all-up systems test in low Earth orbit. Orion will rendezvous and dock with one or both commercial Human Landing Systems, SpaceX’s Starship HLS and Blue Origin’s Blue Moon MK2, validating in-space operations, life support, propulsion, docking interfaces, and Axiom Space’s lunar EVA suits. The mission explicitly mirrors Apollo 9, which tested the lunar module in Earth orbit before Apollo 11’s moon landing. This approach eliminates the high-risk direct jump to surface operations without prior integrated testing.

Artemis IV will deliver the first crewed lunar landing in early 2028, with Artemis V following later that year for a second touchdown and initial outpost development. NASA intends to sustain at least one crewed landing per year thereafter, building toward an enduring lunar presence.

To achieve this faster tempo, the agency is standardizing future SLS flights on a near-Block 1 configuration, canceling the planned Exploration Upper Stage and associated Block 1B upgrades. Production lines will focus on repeatable, high-rate manufacturing to rebuild workforce muscle memory. The replacement for the ICPS will be Centaur V, confirmed through a NASA contract award.

Isaacman framed the changes as a return to fundamentals. He emphasized standardizing vehicle configuration, increasing flight rate, and progressing through objectives in a phased approach, describing it as the approach that achieved the near-impossible in 1969 and would enable its repetition. The overhaul adds one mission, reduces technical risk, and establishes a sustainable cadence capable of supporting long-term lunar infrastructure rather than isolated flags-and-footprints achievements.

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.

New scientific analysis suggests NASA’s Artemis 2 mission should not launch until the second half of 2026 due to elevated solar superflare activity. Dr. Ignacio Jose Velasco Herrera published findings indicating the Sun is experiencing a period of increased superflare risk that could pose radiation hazards to astronauts aboard the Orion spacecraft.

The research identifies mid-2025 through mid-2026 as a period of elevated superflare probability. The Sun’s current activity cycle has produced several powerful solar eruptions, and the analysis suggests the peak danger period coincides with Artemis 2’s planned launch window. Superflares represent extreme versions of normal solar eruptions, capable of releasing enormous amounts of radiation into space.

While Earth’s atmosphere protects terrestrial life from solar radiation, astronauts in deep space face potentially dangerous exposure levels. The Orion spacecraft provides substantial radiation shielding, including a storm shelter design for solar particle events. However, mission planners must balance the benefits of the lunar flyby mission against the risks of heightened radiation exposure.

The four Artemis 2 astronauts continue training regardless of the launch schedule. Commander Reid Wiseman, Pilot Victor Glover, and Mission Specialists Christina Koch and Jeremy Hansen have progressed through extensive preparation for the first crewed lunar flyby since Apollo 8. NASA will review the superflare analysis in coming months before finalizing the launch timeline.

Artemis 2 represents the first crewed flight of NASA’s post-Apollo lunar program. The mission will send the Space Launch System rocket and Orion spacecraft on a trajectory that loops around the Moon before returning to Earth. Success would pave the way for Artemis 3, which aims to land astronauts on the lunar surface, the first human Moon landing since 1972.

The solar activity concern adds to existing schedule pressures for the Artemis program. The SLS rocket and Orion spacecraft have experienced development delays, and the ground systems at Kennedy Space Center require extensive preparation for crewed launches. The mission originally targeted 2024 but has slipped multiple times.

Solar activity forecasting has improved considerably in recent decades, but predicting specific superflare events remains challenging. Scientists can identify periods of elevated risk based on solar cycle patterns and sunspot activity, but the exact timing and magnitude of individual events cannot be predicted precisely. This uncertainty informs the recommendation to avoid the entire elevated-risk period rather than attempting to time a specific launch window.

The Sun’s current activity cycle is among the most vigorous in recorded history. Space weather events have already affected satellite operations and ground-based infrastructure, highlighting the practical importance of understanding solar behavior. For human spaceflight, the stakes are even higher, as astronauts cannot shelter from cosmic radiation as easily as electronic systems can be hardened.

NASA’s approach to space weather has evolved following lessons from earlier programs. The agency maintains space weather forecasting capabilities and has developed procedures for protecting crew during solar events. For Artemis 2, the decision whether to delay involves weighing these protective measures against the risks of operating during a known period of elevated activity.

The Artemis program represents humanity’s most ambitious lunar exploration effort in decades. The success of Artemis 2 as a crewed shakedown flight is critical to subsequent missions, including lunar surface operations and eventually Mars missions. Ensuring crew safety during this foundational flight takes precedence over maintaining an aggressive schedule.