OrbitalHub

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Early on the morning of September 24, 2025, a SpaceX Falcon 9 rocket thundered off Pad 39A at Kennedy Space Center, carrying into space a powerful trio: NASA’s Interstellar Mapping and Acceleration Probe (IMAP), the Carruthers Geocorona Observatory, and NOAA’s SWFO-L1 (Space Weather Follow On – Lagrange 1). The launch marked a bold new chapter in humanity’s efforts to monitor and understand the Sun’s influence across the solar system. The weather was nearly perfect—a 90 percent favorable forecast—and the three spacecraft were stacked together in a “cosmic carpool” bound for a vantage point some 1.6 million kilometers from Earth, at the L1 Lagrange point between the Sun and Earth.

IMAP is the centerpiece of the mission package. Designed to probe the boundary of the heliosphere—the region where the solar wind collides with the interstellar medium—it will sample energetic particles streaming outward from the Sun and inward from beyond, charting the invisible frontier that shields our solar system from cosmic rays. Its array of ten instruments includes devices to detect solar wind electrons, energetic ions, interstellar dust, and magnetic fields, among others. IMAP will also provide near–real-time data useful for space weather prediction, offering up to thirty minutes of advance warning for harmful solar radiation events.

Accompanying IMAP is the Carruthers Geocorona Observatory, a smaller NASA payload dedicated to observing the Earth’s exosphere—the tenuous outermost layer of our atmosphere. From its L1 vantage point, Carruthers will use ultraviolet imaging to monitor the geocorona’s glow, revealing how it responds to solar storms and seasonal changes. The mission is named in honor of George Carruthers, a pioneering space physicist and ultraviolet astronomer.

Meanwhile, NOAA’s SWFO-L1 is the operational arm of this venture, designed for continuous, real-time space weather monitoring. With instruments including a solar wind plasma sensor, magnetometer, and coronagraph, SWFO-L1 will keep watch on solar emissions and storms that could affect Earth’s satellites, communications networks, power grids, and crewed missions beyond low Earth orbit.

Following liftoff, the mission deployment sequence unfolded about 83 minutes later, with IMAP separating first, followed by Carruthers and SWFO-L1 in carefully timed intervals. Engineers expected to receive IMAP’s first signal roughly ten minutes after deployment, while Carruthers’ communications would follow about half an hour later. All spacecraft are destined for halo orbits around L1, providing unobstructed views of solar activity and the heliosphere’s edge.

This launch is more than a technological feat—it’s a leap toward safeguarding life and infrastructure on Earth, as well as deepening our knowledge of how the Sun, Earth, and the galaxy interact. In the coming months and years, IMAP, Carruthers, and SWFO-L1 will collectively map invisible space weather dynamics, chart the Sun’s magnetic bubble, monitor the Earth’s exosphere, and provide vital data for future human missions venturing beyond our planet.

Video credit: NASA/SpaceX

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On August 26, 2025, SpaceX finally pushed its Starship system through a full, ambitious test flight that many in the space-community had long awaited. After a series of earlier mishaps and scrapped attempts, the tenth integrated flight test marked a turning point: the vehicle performed a full-duration ascent burn, reached its planned velocity, deployed test payloads, and survived a fiery reentry before splashing down as intended.

The flight began from Starbase, Texas, with the Super Heavy booster igniting all 33 Raptor engines for launch. After climbing to altitude, Starship’s upper stage (Ship 37) separated and ignited its six engines, continuing on a suborbital trajectory.

During its coast phase, it deployed eight Starlink simulator payloads—marking the first time Starship successfully released a mock satellite mass during a test flight.

The upper stage also accomplished a Raptor engine relight in space, a key demonstration for future deorbit or orbit-raising maneuvers.

As the vehicle reentered Earth’s atmosphere, Starship faced some stress and damage—particularly in the aft skirt and in sections of its heat-shield and flaps.

Despite these challenges, the spacecraft managed a controlled “flip” maneuver, guiding itself nose-first toward the splashdown zone in the Indian Ocean.

Meanwhile, the booster executed a series of burns to reverse course, though it intentionally disabled one of its center engines during the landing burn as part of testing engine-out capability. It hovered briefly over the water before cutting engines and splashing in the Gulf of Mexico, where it broke up on impact.

While not perfect, Flight 10 delivered on many of its critical test objectives. The mission pushed Starship closer to full reusability, validated maneuvers needed for future missions, and restored confidence in the system after earlier failures.

The success of payload deployment and engine relighting in space stand out as especially important steps for upcoming missions to orbit and beyond. Challenges remain—especially refining heat-shield durability, improving structural margins during reentry, and achieving consistent booster recoveries. But the trajectory is now clearer: if the lessons from Flight 10 are applied well, Starship may well be on its way to realizing SpaceX’s goals for lunar, Martian, and deep-space missions.

Video credit: SpaceX

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Axiom Mission 4 (Ax-4) is currently unfolding as a landmark mission in the ongoing expansion of commercial spaceflight. Organized by Axiom Space, in partnership with NASA and SpaceX, Ax-4 is the fourth private astronaut mission to the International Space Station (ISS) and is part of NASA’s Commercial Low Earth Orbit Development program. As the line between government and private spaceflight continues to blur, Ax-4 is demonstrating what multinational, commercially driven space exploration looks like in practice.

Ax-4 launched aboard a SpaceX Falcon 9 rocket from Launch Complex 39A at NASA’s Kennedy Space Center in Florida, carrying the Crew Dragon Freedom spacecraft. After a successful launch and orbital insertion, the spacecraft docked with the ISS, beginning an approximately two-week mission in low Earth orbit.

The Ax-4 crew is led by Peggy Whitson, a former NASA astronaut and Axiom’s Director of Human Spaceflight. Whitson, who holds the U.S. record for cumulative days in space, brings unmatched experience and leadership to the mission. She is joined by three private astronauts representing the emerging generation of global space explorers:

Shubhanshu Shukla (India), a payload specialist and biomedical researcher.

Sławosz Uznański-Wiśniewski (Poland), a European Space Agency (ESA) reserve astronaut and nuclear physicist.

Tibor Kapu (Hungary), a flight and aerospace engineer.

Together, the crew represents a powerful combination of scientific, medical, and operational expertise, with participation from multiple national space programs and agencies.

Ax-4 plays a vital role in the commercialization of low Earth orbit. It serves as a live test case for integrating international and non-agency astronauts into the ISS framework—something that NASA sees as essential to its future LEO strategy. The mission supports NASA’s plan to transition routine orbital operations to commercial providers by the end of the decade, freeing government resources for Artemis missions and Mars exploration.

Furthermore, Ax-4 directly contributes to Axiom Space’s long-term vision of building Axiom Station, a free-flying commercial space station currently under development. Lessons from Ax-4—ranging from crew logistics to science payload management—inform Axiom’s engineering and operational planning for launching its first module, which will initially attach to the ISS before eventually separating into an independent platform.

This mission also sets a precedent for international inclusion in crewed spaceflight. Shubhanshu Shukla’s participation highlights India’s growing role in the commercial space sector, while Sławosz Uznański-Wiśniewski represents a step forward for ESA’s reserve astronaut program. Tibor Kapu’s presence underscores Hungary’s commitment to reentering human spaceflight after decades of absence.

The international nature of Ax-4 reinforces Axiom Space’s role as a facilitator of access to orbit for nations that lack launch capabilities or domestic astronaut corps. By enabling sovereign astronauts to fly as mission specialists, Axiom broadens the scope of participation in space exploration and science.

As Ax-4 continues, the mission is collecting critical data—not just from its scientific payloads, but from the structure and coordination of commercial spaceflight itself. The success of this mission will help define best practices for future mixed-nationality crews, commercial research operations, and astronaut training.

Looking forward, Axiom Mission 5 (Ax-5) is already in planning for 2025, expected to feature even more ambitious goals in terms of duration, research, and international collaboration. As commercial spaceflight moves from novelty to infrastructure, missions like Ax-4 will be remembered as formative efforts that redefined how, and by whom, space is explored.

Video credit: NASA

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Honeybee Robotics, a subsidiary of Blue Origin, contributed two innovative instruments—LISTER and LPV—to Firefly Aerospace’s Blue Ghost Mission 1, which successfully landed on the Moon in March 2025 as part of NASA’s Commercial Lunar Payload Services (CLPS) program. These instruments are pivotal in advancing our understanding of the Moon’s thermal properties and developing efficient regolith sampling techniques for future lunar exploration.

LISTER: Lunar Instrumentation for Subsurface Thermal Exploration with Rapidity

LISTER is designed to measure the heat flow from the Moon’s interior, providing insights into the Moon’s thermal evolution and internal structure. By assessing how heat escapes from the lunar interior, scientists can infer details about the Moon’s composition and geological history.

LISTER is a collaborative effort between Honeybee Robotics and Texas Tech University. It employs a sophisticated pneumatic drill capable of penetrating up to 3 meters into the lunar regolith. At every 0.5-meter interval, the drill pauses to deploy a custom-built thermal probe that measures temperature gradients and thermal conductivity at various depths. LISTER weighs approximately 4.3 kilograms.

During its operation on the lunar surface, LISTER successfully drilled into the regolith and collected thermal data at multiple depths. These measurements are crucial for understanding the Moon’s internal heat flow and contribute to models of its thermal and geological evolution. The data also aid in assessing the Moon’s suitability for future human habitation and resource utilization.

LPV: Lunar PlanetVac

LPV is a technology demonstration aimed at efficiently collecting lunar regolith samples. Its success is vital for future missions that require in-situ resource utilization or sample return capabilities.

LPV is installed on one of the Blue Ghost lander’s legs. It utilizes a burst of compressed gas to dislodge and propel regolith particles into a collection chamber. Capable of collecting particles up to 1 centimeter in diameter. Features a tube that transports the collected material to onboard instruments for analysis or storage.

LPV successfully demonstrated its ability to collect and transfer lunar soil samples using its gas-driven mechanism. The efficient and contamination-free sampling process validates LPV’s potential for future missions that aim to analyze or return lunar materials to Earth. Its performance also provides valuable data for refining regolith collection techniques in low-gravity environments.

Blue Ghost Mission 1, which landed in Mare Crisium, carried a total of ten NASA payloads, including LISTER and LPV. The mission operated for a full lunar day (~14 Earth days), during which all instruments performed their designated tasks. The successful deployment and operation of LISTER and LPV not only achieved their scientific objectives but also demonstrated the viability of these technologies for future lunar exploration endeavors. Their contributions are instrumental in paving the way for sustained human presence on the Moon and the development of lunar resources.

Video credit: Blue Origin

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SpaceX’s Fram2 mission, launched on March 31, 2025, from Kennedy Space Center, marked a historic milestone as the first human spaceflight to orbit over Earth’s polar regions. This privately funded mission, led by cryptocurrency entrepreneur Chun Wang, featured a diverse international crew and aimed to advance scientific research and exploration.

The mission’s name, Fram2, pays homage to the Norwegian exploration ship Fram, symbolizing a new era of polar exploration—this time from space. The spacecraft completed multiple orbits over both the North and South Poles, providing unprecedented views and data.

The crew members are:

Chun Wang (Mission Commander): A Maltese entrepreneur of Chinese origin and founder of F2Pool, Wang financed the mission.

Jannicke Mikkelsen (Capsule Commander): A Norwegian cinematographer specializing in extreme environments.

Rabea Rogge (Pilot): A German robotics researcher and the first German woman in space.

Eric Philips (Mission Specialist & Medical Officer): An Australian polar explorer and guide.

All crew members were civilians with backgrounds in exploration and science, emphasizing the mission’s pioneering spirit.

The Fram2 mission conducted 22 experiments focusing on:

Human Physiology: Including the first X-ray of a human in space and studies on blood flow restriction to mitigate muscle and bone loss in microgravity.

Radiation Exposure: Assessing the effects of increased cosmic radiation encountered in polar orbits.

Biological Studies: Attempting to cultivate oyster mushrooms in space as a potential food source.

Atmospheric Phenomena: Observing aurora-like events such as STEVE and green emissions using high-resolution cameras.

Educational Outreach: The “Fram2Ham” amateur radio project connected with students worldwide, promoting STEM education.

Mission Highlights

Historic Polar Orbit: Fram2 was the first crewed mission to achieve a polar orbit, offering unique perspectives of Earth’s poles.

International Collaboration: The diverse crew underscored the global nature of modern space exploration.

Scientific Contributions: The mission’s experiments provided valuable data for future long-duration spaceflights.

Cultural Significance: Artifacts such as a piece of the original Fram ship’s deck and a Stephen Hawking Medal were carried onboard, bridging past and future explorations.

Fram2’s success demonstrates the potential of private missions to contribute meaningfully to space science and exploration. By achieving a polar orbit, the mission opened new avenues for Earth observation and research. The data collected will inform future missions, particularly those targeting long-duration travel to destinations like Mars. Moreover, the mission’s emphasis on international cooperation and educational outreach sets a precedent for inclusive and globally beneficial space endeavors.

Video credit: SpaceX

Asteroid (52246) Donaldjohanson is a small but significant body located in the main asteroid belt between Mars and Jupiter. Though it may not have the fame of larger or more compositionally unique asteroids, Donaldjohanson stepped into the scientific spotlight thanks to its pivotal role in NASA’s ambitious Lucy mission — a 12-year journey to explore the Trojan asteroids that share Jupiter’s orbit. Before Lucy reaches its primary Trojan targets, it first encountered Donaldjohanson, making it a key object of study in humanity’s effort to understand the solar system’s early history.

Discovery

Asteroid Donaldjohanson was discovered on March 2, 1981, by astronomer Schelte “Bobby” Bus at the Siding Spring Observatory in Australia. Initially designated 1981 EQ5, the asteroid was later named in honor of Dr. Donald Johanson, the paleoanthropologist best known for co-discovering the fossilized remains of Australopithecus afarensis, famously known as Lucy, in Ethiopia in 1974.

This naming decision was particularly meaningful to NASA, as their Lucy spacecraft, launched in 2021, carries a similar goal: to uncover the fossils of the solar system—namely, the Trojan asteroids, which are thought to be leftover building blocks from planetary formation. Naming the asteroid after Johanson creates a poetic link between the exploration of human origins and the origins of our solar system.

Location and Characteristics

Donaldjohanson resides in the inner region of the main asteroid belt, at a semi-major axis of approximately 2.39 astronomical units (AU) from the Sun. Its orbit is relatively circular and stable, with a low eccentricity and inclination, placing it within the Erigone asteroid family, a large group of stony asteroids in the inner main belt.

Though smaller and less well-studied than some of its larger neighbors, Donaldjohanson’s value lies in its convenience and timing—it is perfectly positioned to serve as a flyby target for the Lucy spacecraft en route to the outer solar system.

The Lucy Mission Flyby

NASA’s Lucy spacecraft has successfully completed a flyby of asteroid Donaldjohanson, providing unprecedented insights into this intriguing celestial body. Lucy performed a close flyby at a distance of approximately 600 miles (960 kilometers), capturing detailed images and data.

The flyby is particularly exciting because very few main belt asteroids have been visited by spacecraft, and each one offers a new data point in understanding the diversity and history of these primitive bodies. By studying Donaldjohanson, Lucy will help bridge the scientific gap between the inner and outer asteroid populations.

During the flyby, Lucy used its three onboard science instruments — L’LORRI (a long-range imager), L’Ralph (a visible and infrared spectrometer), and L’TES (a thermal emission spectrometer) — to examine Donaldjohanson’s surface geology, composition, and thermal properties. In addition to gathering scientific data, the flyby allowed engineers to practice operating the spacecraft’s pointing, tracking, and data-gathering systems ahead of the more complex Trojan encounters.

The flyby revealed that Donaldjohanson is a contact binary asteroid, characterized by two lobes connected by a narrow neck, resembling a peanut or a barbell. This structure suggests a history of two separate bodies gently colliding and merging. The asteroid measures about 8 kilometers in length and 3.5 kilometers at its widest point, larger than previously estimated.

Donaldjohanson’s surface exhibits a complex geology with varying crater densities between its lobes, indicating a diverse collisional history. These observations provide valuable data on the processes that shaped such bodies and, by extension, the early solar system. The successful flyby serves as a critical rehearsal for Lucy’s upcoming encounters with Trojan asteroids near Jupiter, scheduled between 2027 and 2033.

Looking Ahead

While Donaldjohanson is not the primary target of Lucy’s mission, the asteroid plays an essential role in validating the mission’s capabilities and providing early science returns. Its proximity and well-known orbit make it an ideal testbed. Moreover, the data collected during the flyby will contribute to our broader understanding of asteroid families, space weathering, and solar system evolution.

After the 2025 encounter, Lucy will go on to visit eight Trojan asteroids, including Eurybates, Polymele, Leucus, Orus, and the binary pair Patroclus and Menoetius. These objects are expected to reveal new insights into the formation of the gas giants and the migration of planets during the early stages of solar system development.

In this grand journey, asteroid Donaldjohanson acts as the first stepping stone—a humble but crucial waypoint on the path to uncovering our solar system’s ancient past. As such, it not only honors the legacy of scientific discovery associated with its namesake but also propels forward the exploration of space’s most enduring mysteries.