Thursday, October 8, 2026

Defense News: Wearable counter‑drone tech enters frontline service across US, Ukraine and IDF units

Wearable counter‑drone tech enters frontline service across US, Ukraine and IDF units


The wearable counter‑drone kit, deployed by Ukrainian troops and IDF forces and integrated into US Army exercises under EUCOM as top US commander warns troops will be ‘hunted’ by autonomous systems

By Anna Aharonheim, Jerusalem Post, October 6, 2026

https://www.jpost.com/defense-and-tech/article-910744

Skylock's Wearable Kit counter-drone solution (photo credit: Autonomous Guard)


Autonomous Guard’s Wearable Kit counter-drone system has been used by Ukrainian troops and undergone operational testing with the US Army in Europe and maneuvering forces in Gaza by the IDF, Defense & Tech by The Jerusalem Post.

The system is a compact RF detection and jamming device that can detect hostile drones up to two kilometers away, providing early warning for units on the move. Its jamming capability extends to three kilometers, enabling forces to disrupt drone operations before the aircraft reaches visual range. It provides directional alerts, allowing troops to take cover or reposition before a drone identifies their location.

When interception is required, SkyLock’s RF guns, which are handheld jamming devices that do not require precise aiming, can be used to neutralize incoming drones. The company says this combination of early warning and rapid response is designed to reduce exposure during reconnaissance and targeting cycles.

SkyLock’s Sky Spotter Pro, a wearable system used at higher command levels such as battalion forward command posts, allows operators to preload friendly drone data during mission planning, reducing false alarms and improving identification accuracy. This helps troops distinguish between hostile and friendly platforms.

The Wearable kit seen on troops in Ukraine, helps warfighters detect hostile drones (credit: Courtesy)

Sky Spotter Pro can detect drones at ranges of up to five kilometers, or three kilometers in complex terrain. It can also identify the drone operator's location, enabling units to direct fire and close the operational loop more quickly. Additionally, SkyLock provides a wearable module that identifies friendly drones to prevent accidental interception.

Wearable counter‑UAS systems have seen widespread use in the Russia‑Ukraine conflict, where both sides rely heavily on small drones for reconnaissance and targeting. According to Autonomous Guard, interest in wearable systems is increasing among militaries, police forces, border units, and prison services.

The system has been sold to hundreds of US Army operations in the US European Command (EUCOM) and other combatant commands worldwide, including Ukraine’s Armed Forces. In July, EUCOM tested the system during a large-scale exercise in Germany. The Defense Post reported that participants included the 2nd Cavalry Regiment, a 4,800-person agile unit stationed at the Rose Barracks in Vilseck that specializes in a full spectrum of operations in support of EUCOM and the NATO alliance.

As AI‑enabled drones are becoming more resilient to jamming, defense officials say wearable counter‑UAS systems are likely to play a growing role in infantry protection by providing mobile coverage in environments where aerial threats are persistent, adaptive, and increasingly autonomous.

Russian drone flies in the sky over the city after a Russian drone strike, amid Russia's attack on Ukraine, in Kyiv, Ukraine November 2, 2024. (credit: REUTERS/GLEB GARANICH)

‘Hunted by autonomous systems’

In a keynote address at the Air, Space and Cyber Conference in Maryland in September, chairman of the Joint Chiefs of Staff Gen. Dan Caine said US forces should assume they will be “hunted by autonomous systems, jammed across the spectrum, and tracked in real time,” citing lessons from the Russia‑Ukraine war. 

According to a report in DefenseScoop, Caine said FPV drones equipped with AI‑enabled computer vision can now continue toward targets even when GPS signals or control links are disrupted.  

“We have to transition the joint force to be prepared to fight and win our future wars by generating and delivering lethality at scale with an agile, optimized, high-low mix of combat capabilities to give the young members of the 2.8 million-member all-volunteer joint force the tools that they need before they need them,” Caine said.

Referring to the Russia-Ukraine war, Caine said that the life expectancy of a new Russian recruit on the frontline in certain areas was as little as 20-30 minutes.

“Think about that. This is what happens when low-cost precision [weaponry] is fielded fast, adapted quickly, and scaled across the battlefield. The price of lethal exchange is decreasing day over day,” he said.

“In the future fight, advantage will go to the side that can see first, who can understand first, decide first, and act first, and along the way be a learning organization,” Caine said, adding that “AI is here now and it’s already changing the way militaries see, sense, decide and act.”

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Radio galaxy from 12.5 billion years ago may be most powerful ever found

VLASS image of TXS 2354+015. The red cross marks the position of the optical source. Credit: arXiv (2026). DOI: 10.48550/arxiv.2609.28632

Astronomers have confirmed a powerful radio galaxy from nearly 12.5 billion years ago. The source, TXS 2354+015, was originally identified as a high-redshift candidate from its characteristic drop in optical light, and follow-up spectroscopy placed it at a redshift of 4.946. Their paper was posted to the arXiv preprint server


Radio-loud AGNs

When material falls onto a galaxy's central supermassive black hole, the resulting accretion activity can power an active galactic nucleus (AGN) and launch powerful relativistic jets of plasma, producing large amounts of radio waves. Such a galaxy is called a radio-loud active galactic nucleus (RLAGN). The energy that the jets carry can influence star formation in the galaxy and heat its surrounding gas.

This "AGN feedback" is incorporated in simulations to correctly predict the number of galaxies in the universe. Such powerful galaxies in the early universe—called high-z RLAGNs—tend to mark the locations of the most massive, earliest-forming galaxies and galaxy clusters.

However, the central black hole and surrounding regions of most powerful early-universe RLAGNs are hidden by a bubble of dusty gas, with only the radio jet able to escape and be seen directly. In particular, a 2024 study suggests as many as 90% of these sources at redshifts greater than 3.5 might be hidden in the ultraviolet and optical bands. Because they are obscured, they are difficult to find and confirm spectroscopically.

Optical cutouts in the five Subaru HSC SSP survey bands. The white circle marks the position of the candidate HzRG. Right plot: AB magnitudes in the five HSC-SSP bands. Credit: arXiv (2026). DOI: 10.48550/arxiv.2609.28632

Missing radio galaxies

The dominant approach to hunting radio sources, which identifies unusually steep spectra, appears to miss a large portion of the true population. To work around this, astronomers instead combined deep optical imaging with radio catalogs, searching for galaxies whose light showed the telltale "dropout" signature of extreme distance. This is known as the Lyman-break technique: Intervening clouds of neutral hydrogen absorb ultraviolet light, causing the galaxy's observed optical spectrum to drop off abruptly at these high redshifts.

In this work, the team led by Barbara Balmaverde of the INAF Astrophysical Observatory of Turin combined deep optical imaging from Subaru's Hyper Suprime-Cam Subaru Strategic Program survey with radio catalogs such as TGSS at 150 MHz and VLASS at 3 GHz to find radio sources whose optical counterparts show the characteristic "dropout" feature within the redshift range of 4.5 to 5.3, when the universe was 1.1 billion to 1.3 billion years old.

In their search, they found an interesting candidate, TXS 2354+015, whose optical spectrum showed a prominent Lyman-alpha emission line. They verified the redshift using a second, fainter emission line. Based on the emission line position, the team confirmed the redshift at 4.946, when the universe was less than 1.2 billion years old. This makes it the second-most-distant radio galaxy ever found.

They also checked whether this was a chance alignment. The precise positional match between optical and radio data, the extremely rare radio brightness and the expected ratio between the radio and optical emission all supported the conclusion that this is a genuine radio source with an optical counterpart.

The most powerful of all

When researchers calculated its intrinsic radio power, TXS 2354+015 turned out to be more powerful than any other known high-redshift radio galaxy in the existing literature. Its estimated radio power at 500 MHz exceeds the previous record-holder from a 2008 census. "TXS 2354+015, thus, appears to be the most powerful radio galaxy known to date," the team writes in the paper.

Researchers also estimated a possible host galaxy mass of around 2 trillion solar masses. This number makes it one of the brightest galaxies known. "This estimate is clearly plagued by several large uncertainties, in particular by the age of the stellar population," the team notes.

Researchers found that TXS 2354+015 does not meet the usual ultra-steep-spectrum selection criteria. Its discovery through the optical dropout method supports the idea that the standard radio selection technique is incomplete, likely missing a meaningful fraction of the true obscured radio galaxy population in the early universe.

https://phys.org/news/2026-10-radio-galaxy-billion-years-powerful.html

Monday, October 5, 2026

An Alien Civilization Lived on Mars. But a Nuclear Disaster Wiped It Out, a Controversial Theory Claims.

 https://www.popularmechanics.com/science/a73939479/mars-aliens-nuclear-theory/


So why haven’t we seen evidence of it?


  • John Brandenburg—a plasma physicist at an aerospace development company—argues that there was an alien civilization on Mars.
  • He cites data from NASA’s Curiosity rover, claiming that xenon levels on the Red Planet indicate a nuclear disaster wiped the population out.
  • Brandenburg’s theory poses striking questions in the broader search for extra terrestrial life; namely: How would we know if another civilization already came and went?

The aliens were next door, and somebody killed them. That’s the story plasma physicist John Brandenburg, PhD, tells about Mars. His theory suggests that a civilization built monuments on our neighboring planet before nuclear explosions wiped it out. He also argues that humanity must investigate—because we could face the same danger. 

In his 2014 Journal of Cosmology paper, Brandenburg presents Martian chemistry and supposed ruins as evidence of a planetary massacre. Both the journal’s editorial standards and Brandenburg’s theory itself have drawn criticism from other scientists. But the decisive question is whether his proposed explanation fits the measurements he provides. Dismissing the alleged attack leaves another question worth asking. If a civilization had flourished somewhere in our solar system and disappeared billions of years before we started looking, what would remain? Could we send a rover across its former home without ever knowing what had been there?

 Brandenburg—who did not respond to requests for an interview—argues that we’ve already found evidence of nuclear explosions in Mars’s atmosphere, focusing particularly on the Red Planet’s xenon measurements. Xenon comes in several forms, called isotopes, each with different numbers of neutrons in their atoms. Timothy Swindle, PhD—a professor emeritus and director emeritus at the University of Arizona’s Lunar and Planetary Laboratory—explains that radioactive decay and reactions caused by radiation can add to that mix. If an explosion produced the xenon on Mars, scientists would expect to find those isotopes in certain proportions. 

Some of the evidence Brandenburg referenced comes from pieces of Mars that landed here on Earth. NASA’s Curiosity, a car-sized rover that landed on Mars in August 2012, gave scientists a way to check these meteorite findings against the atmosphere of our celestial neighbor itself.

“My battery is low and it’s getting dark.” In 2019, those final words shook the internet when NASA announced that Curiosity’s predecessor—Opportunity—shut down after more than a decade of exploring Mars. But was the rover’s last transmission as poetic as this heart-wrenching line seems to be? Sadly, no. The quote is taken out of context; in actuality, it’s a Tweet from a science journalist who was summarizing accounts of Opportunity’s last moments. What really occurred was a cocktail of unfortunate circumstances. Data from Opportunity told the team that it was low on battery, and a blinding sandstorm was incoming. Scientists instructed Opportunity to hunker down through the storm and conserve energy. After the weather cleared, they were unable to make contact with the rover again. But perhaps the internet’s favorite probe—the one that “lived” for years in isolation so that it could send information back to Earth—deserves the cinematic ending we imagine for it.

The “spacecraft measurements by Curiosity match those in one class of Martian meteorites quite closely,” Swindle says, apart from small differences in isotopes Brandenburg doesn’t discuss. Older rocks, on the other hand, tell a somewhat different story. Allan Hills 84001, a Martian meteorite found in Antarctica in 1984, contains a slightly different xenon mix, Swindle says, “suggesting that the atmosphere may have changed over billions of years.” And when asked if the xenon measurements support Brandenburg’s explosion claim, Swindle disagrees. “In a word, no,” he says.

Brandenburg focuses on the unusually high proportion of xenon-129 in Mars’s atmosphere. A nuclear explosion could produce it, but its presence alone hardly clinches the case. Swindle says the problem becomes clearer when you look at how Brandenburg tries to recreate the full Martian xenon pattern. In the 2014 paper, Brandenburg starts with the isotope mix found in Earth’s atmosphere, then calculates what would happen if xenon measured after nuclear tests were added to it. He adds just enough of the nuclear-test xenon to bring xenon-129 up to the level measured on Mars. That isotope is bound to match because Brandenburg used it to set the proportions.

Several other isotopes also appear to line up. But Swindle points out that fission, the splitting of atomic nuclei that causes a nuclear explosion, doesn’t produce four of them. Their agreement says only that Mars’s starting xenon looks similar to Earth’s, not that an explosion occurred. The meaningful test is whether the mixture also matches the other isotopes that fission does produce. It doesn’t. The fit gets progressively worse among the heavier isotopes. At xenon-136, Swindle says Brandenburg’s plotted mixture contains 50 percent more than the amount measured on Mars. “Normally, if you can’t match it to within a few percent, it’s not a good match at all,” he says.

Swindle also identifies an internal contradiction. Brandenburg invokes a shift toward lighter fission products to explain xenon-129. Swindle says that shift should produce progressively less xenon as you move from isotope 131 to 132, 134, and 136. But Brandenburg’s calculated mixture already predicts too much of those heavier isotopes compared to the amounts measured in Mars’s atmosphere, and the gap gets larger with each one. “The mismatch is in the opposite direction,” Swindle says.

There’s another possible source of xenon-129. Radioactive iodine-129 decays into it naturally, although that explanation brings its own timing problem. Half of the iodine-129 decays every 15 million years, so most of it would have disappeared early in Mars’s history. The difficult part, Swindle says, is coming up with a timeline in which Mars released so much decay-produced xenon-129 after the planet had already lost most of its atmosphere.

Here, it’s important to distinguish between Brandenburg’s 2014 and 2023 papers. In the more recent work, he uses different xenon comparisons. The paper was published by Scientific Research Publishing—an organization included on librarian Jeffrey Beall’s archived list of potentially predatory resources. Swindle’s criticism addresses the comparisons in the 2014 paper, not the newer analysis.

Brandenburg also sees another clue supporting his explosion theory in the ratio of argon-40 to argon-26 on Mars, which is higher than it is on Earth. He argues that Mars must have received an unusual dose of argon-40. However, Swindle says that considering the actual amounts of these isotopes paints a different picture. Per gram of planet, Mars’s atmosphere has only about 2 percent as much argon-36 as Earth’s, and it also has less argon-40. In other words, the ratio is high because Mars has so little argon-36, not because it has an unexplained surplus of argon-40. All things considered, Swindle would not say an ancient explosion was impossible. He calls the isotopic evidence “very, very weak.”

Outside scientists have other ideas about what may have happened to Mars’s xenon. In their 2024 Science Advances study, “Impact sculpting of the early martian atmosphere,” Oliver Shorttle and his colleagues used laser-driven shocks and computer models to study the effects of objects colliding with early Mars. They found that repeated collisions during the solar system’s first 200 to 300 million years of existence could’ve knocked xenon out of the planet’s atmosphere. The lighter xenon isotopes escaped more easily than the heavier ones, changing the balance of what remained. That could explain much of the pattern scientists measure today, although the study doesn’t explain the extra xenon-129 at the center of Brandenburg’s argument.

What we do know is that Mars once had rivers and lakes, and researchers have found ways to explain how they dried out—without nuclear devastation. Measurements from NASA’s MAVEN spacecraft show how solar wind and radiation stripped away atmospheric gas on Mars. Some of the water went into the rocks and may still be there, bound up in minerals in the planet’s red crust. This put the estimated amount of water at 30 to 99 percent of the planet’s original conditions, according to a 2021 study published in Science. Having water makes Mars a place worth searching for life, but it doesn’t tell us if anything lived there.

Any microbes living on Mars might’ve had somewhere to go as the surface dried out, perhaps underground, where conditions could have allowed them to survive. But Brandenburg is asking us to imagine inhabitants who built things, which is a much bigger leap. “We see zero evidence of ancient technological species in the Solar System,” says Jason Wright, PhD, a Pennsylvania State University astronomy and astrophysics professor and director of the school’s Extraterrestrial Intelligence Center.

Wright points to Gavin Schmidt and Adam Frank’s 2018 Silurian Hypothesis paper, which asks how an earlier industrial civilization might register in Earth’s geological record. (Though it doesn’t make an argument that one existed.) Wright says we might have only a few million years before the evidence becomes too hard to recognize as something a civilization left behind. The paper also considers chemical signatures that might outlast recognizable artifacts.

On Mars, Wright imagines a rover discovering an unmistakably technological device buried in sand. However, erosion complicates its survival. “Many artifacts that we, or our ancestors, considered to be durable may not persist for million-year timescales,” says Jacob Haqq-Misra, PhD, an astrobiologist and senior research investigator at Blue Marble Space, a nonprofit research institute based in Seattle.

Haqq-Misra suggests machine learning could help search high-resolution Martian imagery for anomalies. Recognition would require investigation with experts in natural planetary processes. “We should investigate all anomalies, but we should not assume all anomalies are evidence of aliens,” he says. A strange feature could eventually reveal an ordinary explanation or something scientifically new. The investigation has value even when the anomaly turns out to have a natural cause.

Brandenburg’s 2014 paper turns his alleged catastrophe into a warning about hostile civilizations. He proposes human exploration to help humanity avoid a similar fate. But Wright rejects the premise that cosmic silence necessarily requires an explanation: “The Fermi paradox isn’t really a problem that demands an answer.” Interstellar travel is difficult, and we have done limited searching.

Likewise, the Great Filter—a proposed obstacle to life’s advancement—need not exist. Wright cautions that nuclear war would not necessarily eliminate all human life, much less establish a universal fate. “We regularly project our own existential fears onto hypothetical aliens,” he says.

Haqq-Misra offers a possibility without a massacre: “Another civilization could have even visited the solar system long ago, with few if any traces left behind.” Civilizations might miss one another in space and time.

Understanding what alien traces could look like is worthwhile. However, before we treat Mars as a warning, the isotope mix predicted by Brandenburg’s proposed explosion needs to match what we actually found there. As is the case with all of our search for extraterrestrial life thus far, the question still remains: Are we—and have we always been—truly alone in the cosmos?

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Saturday, October 3, 2026

Astronomers find the lightest double neutron star system ever seen

www.techexplorist.com/astronomers-find-lightest-double-neutron-star-system-seen/105674/

Astronomers have just unveiled a remarkable discovery: a compact double neutron star (DNS) system unlike any seen before. The pulsar PSR J1856–0039, detected with China’s Five-hundred-meter Aperture Spherical Radio Telescope (FAST), is rewriting what we know about the extremes of stellar physics and gravitational theory.

Neutron stars are the extremely compact remnants left behind after the explosive demise of very large (massive) stars as supernovae. As long as these neutron stars are in a binary system with each other, they provide scientists with a unique opportunity to test Albert Einstein’s Theory of General Relativity and observe the catastrophic collisions that result in the generation of gravitational waves.

PSR J1856-0039 represents a unique example of a double neutron star (DNS) system. The pulsar component of PSR J1856-0039 rotates once every 23.4 milliseconds, which places it in the category of “mildly recycled.” The pulsar component of PSR J1856-0039 rotates once every 23.4 milliseconds, which places it in the category of “mildly recycled.”

Remarkably, this is the least massive of all the DNS discovered to date, with a total mass of 2.49 solar masses. In addition, the companion neutron star has a mass of 1.185 solar masses and is among the least massive neutron stars ever detected.

Determining the birth population of double neutron stars

Using high-precision measurements of PSR J1856–0039’s pulse arrival times, researchers were able to measure many of the relativistic effects that exist in this system. For instance, the orbital decay of this system is occurring at a rate of approximately 1.28 x 10^-12 seconds/second, which is consistent with the predicted decay due to gravitational wave emission.

The periastron precession, which is the movement of the point on the orbit that comes closest to the center, is occurring at 17.6 degrees per year; this is a very typical effect seen in relativity. The Einstein delay, a slight delay in the pulsar signals, provides evidence of how space-time has been warped.

Additionally, it appears as though the measured rate of orbital decay agrees with the prediction made by general relativity with an error of less than one percent, providing some of the strongest support for Einstein’s theory.

This pair of neutron stars is expected to collide and combine within 82 million years. Depending on whether the system slows down rapidly enough during the collision process to remain stable as a single neutron star, or if the system collapses into a black hole, these collisions are the power sources for several of the most energetic events in the universe, such as short gamma-ray bursts, and the production of heavy elements such as gold and platinum.

Colliding neutron stars could shed light on universal mysteries

Discoveries such as PSR J1856-0039 offer a valuable opportunity to test relativity in a real-world setting, pushing the limits of our knowledge of gravity. Additionally, such discoveries help researchers refine their models of gravitational-wave signals, which are required for detectors such as LIGO and Virgo.

These systems offer insights into the formation and evolution of neutron stars. They also reveal why some are unusually light. They also reveal the ultimate fate of compact pairs, whether they survive as stable neutron stars or collapse into black holes.

Long-term observations of PSR J1856-0039 may also test the validity of Lense-Thirring Precession, a very subtle phenomenon in which the rotation of a body creates a “dragging” effect on its surrounding spacetime. Detection of such an effect would provide another great validation of Einstein’s Theory of Relativity.

Journal Reference:

  1. Z. L. Yang et al., Relativistic Effects of PSR J1856–0039 Double Neutron Star System in a 2.36-Hour Compact Orbit, Physical Review Letters (2026). DOI: 10.1103/hmjp-htd1

Friday, October 2, 2026

Space News: SpaceX's Starship engine failure could cause problem for NASA's 2028 moon mission objectives

SpaceX's Starship engine failure could cause problem for NASA's 2028 moon mission objectives

A longer delay would pose not only a greater setback to SpaceX's commercial ambitions to rapidly expand its Starlink broadband satellite network, but its pivotal role in NASA's Artemis moon program.

By Reuters, September 29, 2026


The SpaceX Starship and Super Heavy v3 Booster lift off on its 13th test flight from the SpaceX launch complex in Starbase, Texas, U.S., July 24, 2026. (photo credit: REUTERS/STEVE NESIUS)

The Starship engine failure that nearly foiled the orbital debut of SpaceX's next-generation spacecraft on its 14th uncrewed test flight may complicate NASA's ability to meet its time frame for astronaut missions to the moon.

Starship, designed in part to carry large payloads to space, is one of two vehicles vying to become the first craft that NASA will use as early as 2028 to land humans on the moon and bring them safely home, a feat last achieved in 1972 at the end of the Apollo era.

While Starship accomplished a number of key objectives in its latest test launch from Texas on Monday, the mission was cut short by several hours after a malfunction of its propulsion system.

Despite the unexpected shutdown of one of its three main Raptor engines following Starship separation from its lower-stage booster rocket, flight controllers proceeded with sending the spacecraft to orbit for its first-ever commercial satellite deployment.

Determining what caused the engine glitch remains critical to SpaceX's bottom line. But the stakes are potentially higher for NASA, as a Starship moon-landing vehicle would rely on the same engine system for transporting astronauts through space to and from the lunar surface.


NASA astronaut and Artemis II Commander Reid Wiseman takes a moment during the seven-hour lunar observation period where the crew reported to the ground team their observations including color nuances, which will help enhance scientific understandings of the Moon, April 6, 2026. (credit: NASA/HANDOUT VIA REUTERS)
How big a blow to Starship's development progress the engine snafu becomes depends on whether it turns out to be "a one-off failure of a single part" or points to a larger design problem that requires upgrades "across the fleet," said Dean Sladen, an aerospace engineer for Accu Components.

"Any engine fix that holds up the next flights, including the planned attempt to catch the ship with the launch tower's arms (after re-entry), eats into that schedule," he said.

NASA and SpaceX did not immediately respond to Reuters requests for comment.

'The real pressure is the moon'

A longer delay would pose not only a greater setback to SpaceX's commercial ambitions to rapidly expand its Starlink broadband satellite network, but its pivotal role in NASA's Artemis moon program.

"The real pressure is the moon. NASA needs Starship for Artemis III," an Earth-orbit test mission targeted as soon as next summer as a rehearsal flight for the program's actual first crewed lunar landing, Sladen said.

Raptor engine and propulsion-system issues have contributed to several previous Starship setbacks, including an engine that failed to ignite as planned during Starship's 12th flight in May. The methane-fueled engines are among the most complex and expensive components on the rocket.

During some previous flights, SpaceX scrubbed plans to test-ignite the Raptor engine in space. But all of the engines successfully fired during ascent on Starship's 13th flight in July.

SpaceX, the newly public venture founded by Elon Musk near Los Angeles in 2002, is competing with Blue Origin, the rival rocket company from fellow entrepreneur Jeff Bezos, to usher in an era of lunar exploration under NASA's Artemis program.

While SpaceX was originally contracted to provide the first crewed lunar lander for Artemis, the head of the US space agency, Jared Isaacman, said in April that NASA would go with whichever lander was ready to fly first. NASA saw the added competition as healthy for progress in light of mounting delays in Starship's test flight program.

NASA hopes to return to the moon's surface by 2028

NASA officially aims to return astronauts to the moon's surface by 2028 - a target widely seen as overly ambitious - to get there ahead of China, which plans a crewed lunar landing by 2030.

A functioning lunar landing craft also will be needed for the precursor Artemis III mission, as early as summer 2027, to test rendezvous and docking manoeuvres in low Earth orbit.

SpaceX is developing a Human Landing System based on its Starship vessel, a towering stainless-steel vehicle far larger than any moon lander built before. Blue Origin is building its own Blue Moon lander, relying on a more traditional design philosophy.

If ready, both landers are likely to participate in the Artemis III mission, demonstrating orbital maneuvers using their in-space engines.

Isaacman went public with the competing lander strategy days after completion of NASA's Artemis II mission sending astronauts around the moon and back in what was the first crewed launch of NASA's Space Launch System rocket, built by Boeing and Northrop Grumman, and the Orion capsule, made by Lockheed Martin.

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