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SpaceX’s next-generation Starship spacecraft exploded minutes after liftoff in an uncrewed test flight from South Texas on Thursday, cutting short a key step in Elon Musk’s development of a rocket vessel to eventually take humans to the moon and Mars.

The flight test was the first for Starship mounted atop the company’s new Super Heavy rocket, and the first launch ever for that lower-stage booster, which SpaceX has touted as the most powerful launch vehicle on Earth.

Even though the two-stage rocket ship made it less than halfway to the edge of space, climbing to just under 25 miles (40 km), the flight achieved a primary objective of getting the new vehicle off the ground at liftoff despite some of its engines failing.

While SpaceX officials were heartened by the outcome, the mission fell short of reaching several objectives.

The plan was for Starship to soar into space at least 90 some miles (150 km) above Earth before it would re-enter the atmosphere and plunge into the Pacific near Hawaii.

But SpaceX said in a statement afterward that the spacecraft “experienced multiple engines out” during its ascent, then “lost altitude and began to tumble,” before the “flight termination system was commanded on both the booster and the ship.”

Musk, SpaceX’s founder, chief executive and chief engineer, had appeared eager to temper expectations in remarks made Sunday that downplayed the odds of a successful first flight. SpaceX President Gwynne Shotwell told a conference in February that the “the real goal is to not blow up the launch pad.”

By that measure, the debut flight of Starship with its booster rocket represented a milestone in SpaceX’s ambition of sending astronauts back to the moon and ultimately to Mars, as a major partner in Artemis, NASA’s newly inaugurated human spaceflight program.

NASA chief Bill Nelson congratulated SpaceX on Twitter, saying, “every great achievement throughout history has demanded some level of calculated risk, because with great risk comes great reward.”

Launch, then fiery ‘disassembly’

The two-stage rocket ship, standing taller than the Statue of Liberty at 394 feet (120 meters), blasted off from the company’s Starbase spaceport on the southern tip of Texas along the Gulf Coast east of Brownsville. SpaceX hoped, at best, to pull off a 90-minute debut flight into space but just shy of Earth orbit.

A live SpaceX webcast showed the rocket ship rising from the launch tower into the morning sky as the Super Heavy’s Raptor engines roared to life in a ball of flame and billowing clouds of exhaust and water vapor.

But less than four minutes into the flight, the upper-stage Starship failed to separate as designed from the lower-stage Super Heavy, and the combined vehicle was seen tumbling end over end before blowing apart.

The pad and surrounding area were cordoned off well in advance of the test, SpaceX said. Any debris from the explosion should have landed over the water in areas placed off-limits by the U.S. Coast Guard.

The spacecraft reached a peak altitude of about 24 miles (39 km) before its fiery disintegration, SpaceX said. The company also noted that the rocket reached the critical launch point of maximum aerodynamic pressure before appearing to lose control.

SpaceX officials on the webcast hailed the liftoff as a welcome accomplishment.

A throng of SpaceX workers shown during the webcast watching a livestream together at the company’s headquarters near Los Angeles cheered wildly as the rocket cleared the launch tower – and again when it blew up.

‘Learned a lot’

Musk, shown seated in the Starbase mission control room in Boca Chica, Texas, wearing a headset, said on Twitter afterwards that the next Starship test launch would be in a few months.

“Congrats @SpaceX team on an exciting test launch of Starship! Learned a lot for next test launch,” he tweeted. Musk, who purchased Twitter last year for $44 billion, is also CEO of electric carmaker Tesla Inc.

SpaceX principal integration engineer John Insprucker, one of the webcast commentators, said the experience would provide a wealth of data to inform further flight tests.

The road to Thursday’s accident has not been without previous tests and setbacks.

A stationary test firing of the Super Heavy while bolted to a platform managed to ignite just 31 Raptor engines in February, and an earlier static firing test in July 2022 ended with the vehicle’s engine section exploding.

Before that, SpaceX had test-launched prototypes of Starship’s top half in five short flights to an altitude of 6 miles (9.7 km), seeking to perfect its return landing capability. All but one crashed in flames.

The spectacular nature of Thursday’s loss of the first fully integrated Starship-and-booster vehicle during its introductory launch further highlighted challenges SpaceX faces moving beyond its workhorse Falcon 9 rocket, the centerpiece of the company’s satellite launch business.

Still even a textbook test flight would have by design ended with crash landings of both portions of the spacecraft at sea.

The Super Heavy and Starship were each designed as reusable components, capable of flying back to Earth for soft landings in a maneuver that has become routine in dozens of missions for SpaceX Falcon 9 rockets.

For Thursday’s launch, however, the flight plan called for the lower stage to fall into the Gulf of Mexico after separating from the upper stage, which would have come down in the Pacific Ocean near Hawaii after achieving nearly one full Earth orbit.

© Thomson Reuters 2023


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A Nearby Supernova May End Dark Matter Search, Claims New Study

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A Nearby Supernova May End Dark Matter Search, Claims New Study

The pursuit of understanding dark matter, which comprises 85 percent of the universe’s mass, could take a significant leap forward with a nearby supernova. Researchers at the University of California, Berkeley, led by Associate Professor of Physics Benjamin Safdi, have theorised that the elusive particle known as the axion might be detected within moments of gamma rays being emitted from such an event. Axions, predicted to emerge during the collapse of a massive star’s core into a neutron star, could transform into gamma rays in the presence of intense magnetic fields, offering a potential breakthrough in physics.

Potential Role of Gamma-Ray Telescopes

The study was published in Physical Review Letters and revealed that the gamma rays produced from axions could confirm the particle’s mass and properties if detected. The Fermi Gamma-ray Space Telescope, currently the only gamma-ray observatory in orbit, would need to be pointed directly at the supernova, with the likelihood of this alignment estimated at only 10 percent. A detection would revolutionise dark matter research, while the absence of gamma rays would constrain the range of axion masses, rendering many existing dark matter experiments redundant.

Challenges in Catching the Event

For detection, the supernova must occur within the Milky Way or its satellite galaxies—an event averaging once every few decades. The last such occurrence, supernova 1987A, lacked sensitive enough gamma-ray equipment. Safdi emphasised the need for preparedness, proposing a constellation of satellites, named GALAXIS, to ensure 24/7 sky coverage.

Axion’s Theoretical Importance

The axion, supported by theories like quantum chromodynamics (QCD) and string theory, bridges gaps in physics, potentially linking gravity with quantum mechanics. Unlike neutrinos, axions could convert into photons in strong magnetic fields, providing unique signals. Laboratory experiments like ABRACADABRA and ALPHA are also probing for axions, but their sensitivity is limited compared to the scenario of a nearby supernova. Safdi expressed urgency, noting that missing such an event could delay axion detection by decades, underscoring the high stakes of this astrophysical endeavour.

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

Intelligent extraterrestrial civilisations might be utilising stars as massive interstellar vehicles to explore the galaxy, according to a theory proposed by Clement Vidal, a philosopher at Vrije Universiteit Brussel in Belgium. His research suggests that alien species could potentially accelerate their binary star systems to traverse vast cosmic distances. While such a concept is purely hypothetical and unproven, Vidal’s recent paper, which has not undergone peer review, raises intriguing possibilities about advanced extraterrestrial engineering.

Concept of Moving Star Systems

The study was published in the Journal of the British Interplanetary Society. As per a report by LiveScience, the idea revolves around the notion that alien civilisations, instead of building spacecraft for interstellar travel, might manipulate entire star systems to travel across the galaxy. Vidal highlights binary star systems, particularly those involving neutron stars and smaller companion stars, as ideal candidates. Neutron stars, due to their immense gravitational energy, could serve as anchors for devices designed to propel the system by selectively ejecting stellar material.

Vidal explained in the paper that uneven heating or manipulation of magnetic fields on a star’s surface could cause it to eject material in one direction. This process would create a reactionary thrust, propelling the binary system in the opposite direction. The concept provides a way to travel while preserving planetary ecosystems, making it a theoretically viable method for species reliant on their home systems.

Known Examples with High Velocities

Astronomers have identified hypervelocity stars, such as the pulsars PSR J0610-2100 and PSR J2043+1711, which exhibit high accelerations. While their movements are believed to be natural phenomena, Vidal suggests they could be worth further investigation to rule out potential artificial influences.

This theory adds an unconventional angle to the search for intelligent life, expanding possibilities beyond traditional methods of exploration like searching for signals or probes. The research underscores the importance of considering advanced and unconventional methods aliens might employ to navigate the galaxy.

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

NASA’s Hubble Space Telescope has provided new insights into the young star FU Orionis, located in the constellation Orion. Observations have uncovered extreme temperatures in the inner region of its accretion disk, challenging current models of stellar accretion. Using Hubble’s Cosmic Origins Spectrograph and Space Telescope Imaging Spectrograph, astronomers captured far-ultraviolet and near-ultraviolet spectra, revealing the disk’s inner edge to be unexpectedly hot, with temperatures reaching 16,000 kelvins—almost three times the Sun’s surface temperature.

A Star’s Bright Outburst Explained

First observed in 1936, FU Orionis became a hundred times brighter in months and has remained a unique object of study. Unlike typical T Tauri stars, its accretion disk touches the stellar surface due to instabilities. These are caused by the disk’s large mass, interactions with companion stars, or material falling inwards. Lynne Hillenbrand, a co-author from Caltech, in a statement said that the ultraviolet brightness seen exceeded predictions, revealing a highly dynamic interface between the star and its disk.

Implications for Planet Formation

As per a report by NASA, the study holds significant implications for planetary systems forming around such stars. The report further quoted Adolfo Carvalho, lead author of the study, saying that while distant planets in the disk may experience altered chemical compositions due to outbursts, planets forming close to the star could face disruption or destruction. This revised model provides critical insights into the survival of rocky planets in young star systems, he further added.

Future Investigations on FU Orionis

The research team continues to examine spectral emission lines in the collected data, aiming to map gas movement in the star’s inner regions. Hillenbrand noted that FU Orionis offers a unique opportunity to study the mechanisms at play in eruptive young stars. These findings, published in The Astrophysical Journal Letters, showcase the ongoing value of Hubble’s ultraviolet capabilities in advancing stellar science.

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