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NASA’s Artemis campaign aims to propel astronauts, scientific experiments, and essential payloads into deep space, utilising the Space Launch System (SLS). The upcoming Artemis IV mission will introduce the Block 1B variant of the SLS, equipped with an upgraded Exploration Upper Stage (EUS). The enhanced system will enable the transportation of larger payloads, including the Orion spacecraft and the Lunar I-Hab module, developed by the European Space Agency (ESA), which will serve as a critical component of the Gateway lunar space station.

Structural Innovations for Deep Space Missions

According to NASA reports, a key structural component of the SLS Block 1B, the payload adapter, has undergone significant development at the Marshall Space Flight Center in Huntsville, Alabama. Designed to accommodate a variety of payloads, the adapter consists of eight composite panels reinforced with an aluminium honeycomb core and secured by aluminium rings. Engineers have employed structured light scanning technology to ensure precise construction, eliminating the need for traditional, costly tooling during assembly.

Flexible Manufacturing Approach

As per NASA, the structured light scanning method has reduced costs while increasing adaptability, allowing engineers to modify adapter dimensions based on mission requirements. Brent Gaddes, Lead for the Orion Stage Adapter and Payload Adapter at NASA Marshall, stated in an official NASA release that the approach enables rapid design adjustments for different payload sizes without requiring extensive retooling. He explained that should a larger or smaller adapter be required, the structured light scanning system would allow quick modifications without significant resource expenditure.

Testing and Load Capacity Verification

Reports indicate that an engineering development unit of the payload adapter has been tested to withstand three times the expected load. A separate qualification unit is also being developed to meet NASA’s structural standards for composite materials. The payload adapter, designed in a conical shape, differs from historically tested cylindrical structures, making rigorous testing essential.

Future Prospects in Lunar and Martian Exploration

NASA’s Artemis programme aims to establish sustainable lunar exploration capabilities, providing critical data for future crewed missions to Mars. The SLS, combined with the Gateway lunar station, advanced spacesuits, and human landing systems, forms the foundation of deep space exploration efforts. Findings from ongoing structural testing will contribute to NASA’s database on spacecraft component resilience, offering insights that will benefit both governmental and commercial aerospace sectors.

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NASA Solves Black Hole Jet X-ray Mystery with IXPE’s Polarization Powers

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May 9, 2025

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NASA Solves Black Hole Jet X-ray Mystery with IXPE’s Polarization Powers

The blazar BL Lacertae, a giant black hole with jets, facing the earth, have made scientists curious about how X-rays are generated in such extreme conditions for a while. NASA’s Imaging X-ray Polarimetry Explorer or IXPE now might have been able to solve the mystery. By a collaboration with radio and optical telescopes and using polarisation measurements of X-ray, IXPE’s produced results indicates that the interaction between fast-moving electrons and photons might be the reason for X-ray emission in such conditions.

Evidence of Compton Scattering

According to the IXPE’s findings, high optical to X-ray polarization ratio indicates that Compton scattering might be the mechanism of X-ray generation. There are two possible and competing explanations of X-ray emission in blazar jets. One saying if the X-rays in the black hole jets are highly polarised, then the X-rays are generated from interactions between photons while the other says a low polarisation indicates X-ray formation by electron-photon interaction.

Leveraging IXPE’s unique X-ray polarisation measuring ability, scientists conducted a focused observation on BL Lac in November 2023. During this period, BL Lac’s optical polarization peaked at 47.5%, the highest recorded for any blazar. Yet IXPE found the X-ray polarization to be much lower, capped at 7.6%. This contrast supports the Compton scattering and possibly irradicates the photon-based explanation.

Milestone for blazar studies

“This was one of the biggest mysteries about supermassive black hole jets,” said Iván Agudo, lead author of the study and astronomer at the Instituto de Astrofísica de Andalucía – CSIC in Spain. The discovery validates IXPE’s mission, launched in December 2021 to study X-ray polarization.

Astrophysicist Enrico Costa, called it one of IXPE’s most significant achievements. Yet, this is just the beginning. Project scientist Steven Ehlert noted the need to observe more blazars, as their emissions vary over time. With IXPE, astronomers are now better equipped to explore these powerful cosmic jets.

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SpaceX Falcon 9 Successfully Launches 28 Starlink Satellites to Orbit From Florida

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May 9, 2025

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SpaceX Falcon 9 Successfully Launches 28 Starlink Satellites to Orbit From Florida

SpaceX continued its rapid-fire Starlink deployment campaign on Tuesday night (May 6), lofting 28 more internet satellites to orbit atop a Falcon 9 rocket from Florida’s Cape Canaveral Space Force Station. The launch itself took place at 9:17 p.m. EDT (0117 GMT on May 7) from Launch Complex-40, marking the company’s 53rd Falcon 9 launch of 2025 and the 36th dedicated Starlink mission this year. The payload offers worldwide internet connectivity by adding to SpaceX’s swiftly expanding array of over 7,200 Starlink satellites in low Earth orbit.

As per a Space.com report, B1085, the reusable first-stage booster, executed a perfect main engine cut about 2.5 minutes after launch, then stage separation and a retrograde burn to stop its descent. Roughly eight minutes after launch, B1085 successfully landed on the autonomous drone ship, stationed in the Atlantic Ocean. The mission was the seventh flight for this particular booster, which had previously supported two other Starlink missions.

The Falcon 9‘s upper stage continued into orbit and deployed the 28 Starlink satellites roughly one hour after launch. These newly deployed units will spend several days adjusting their positions before integrating into the broader Starlink network, which now blankets most of the globe except the polar regions. Each satellite, compact but equipped with large solar arrays, forms part of the larger web responsible for delivering high-speed satellite internet.

The May 6 launch demonstrates how quickly SpaceX is moving to meet its broadband goals. In addition to Falcon 9 missions, the company has performed two Starship test flights this year to demonstrate development progress in both satellite launch and heavy-lift capability.

An expanding constellation would finally bring reliable internet coverage to remote locations around the world. The drive to offer a reliable internet connection to remote sites globally reflects a commitment to putting the world more in reach.

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Asteroid Vesta May Be a Fragment of a Lost Planet, Say Scientists

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May 9, 2025

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Asteroid Vesta May Be a Fragment of a Lost Planet, Say Scientists

Asteroid Vesta, long considered a stalled protoplanet, may actually be a massive fragment of a larger world that once existed in our solar system. New findings based on gravity-field mapping and spin-rate data suggest Vesta lacks the dense core typically found in differentiated planetary bodies. The discovery challenges previous assumptions, drawn from NASA’s Dawn mission in 2012, that classified Vesta as an embryonic planet. Now, scientists report that Vesta might have been ejected from a differentiated world in a massive collision 4.5 billion years ago, upending ideas about the development of planets and asteroids.

New Gravity Data Suggests Vesta Is Debris from a Destroyed Planet, Not a Protoplanet

As per a new study published in Nature Astronomy on April 23, 2025, Vesta does not quite match the former model. Refined calibration methods polished the radio Doppler signals, confirming the absence of a metal-rich core, which was inconsistent with earlier work. Seth Jacobson of Michigan State University, who led the research, stated the new interpretation marks a major shift in planetary science. While Vesta’s basaltic, volcanic surface still indicates geological activity, its internal uniformity contradicts the expectations of a body that once underwent full differentiation.

This paradox has caused scientists to reconsider the asteroid’s heritage. One scenario is that Vesta started to differentiate but never got very far. But data from meteorites called howardite-eucrite-diogenites (HEDs), thought to have come from Vesta, show no signs of such incomplete differentiation. Jacobson and his team instead favour the explanation that Vesta was formed from material blasted off a fully developed planet during an ancient planetary collision, which could also illustrate its volcanic surface without requiring it to have a dense core.

The results not only question Vesta’s identity but also suggest a possibility of a more general theory: that other asteroids could also be pieces of shattered planets. NASA’s Psyche and ESA’s Hera missions, planned for the next decades, intend to do such gravity investigations, which could ultimately confirm this new view. Jacobson noted that Vesta’s composition could even hint at a shared origin with Earth or other early planets, a hypothesis that may reshape asteroid science entirely.

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