Most mission scientists would wince at the thought of their spacecraft being smashed to smithereens. But for those behind Nasa's Dart probe, anything short of total destruction will be chalked up as a failure. From a report: The $330m spacecraft is due to slam head-on into an asteroid about 11m kilometres above the Indian Ocean soon after midnight on Monday. The impact, at nearly seven kilometres a second, will obliterate the half-tonne probe, all in the name of planetary defence. Not that Dimorphos, the asteroid in question, poses any threat to humanity. The Dart, or double asteroid redirection test, is an experiment, the first mission ever to assess whether asteroids can be deflected should one ever be found on a collision course with Earth. A well-placed nudge could avert Armageddon, or so the thinking goes, and spare humans the same fate as the dinosaurs.

"It's a very complicated game of cosmic billiards," said Prof Alan Fitzsimmons, an astronomer and member of the Nasa Dart investigation team at Queen's University Belfast. "What we want to do is use as much energy [as we can] from Dart to move the asteroid." With telescopes constantly scanning the skies, scientists hope to have some notice if an asteroid were ever to present a major threat. "If we are able to see far enough in advance and know that an asteroid might be a problem, pushing it out of the way will be much safer than the big Hollywood idea of blowing it up," said Catriona McDonald, a PhD student at Warwick University. The Dart mission launched from Vandenberg space force base in November last year. On Monday night, mission controllers will hand control to Dart's software and let the probe steer itself into oblivion.

The Artemis I rocket will not have its third launch attempt on Tuesday as planned due to concerns over Tropical Storm Ian making its way toward Cuba and Florida. CNN reports: After meeting on Saturday morning, NASA's Artemis team decided to forgo the September 27 launch opportunity and is now preparing the mega moon rocket stack for rollback. "On Tuesday, Tropical Storm Ian is forecast to be moving north through the eastern Gulf of Mexico as a hurricane, just off the southwest coast of Florida. A cold front will also be draped across northern Florida pushing south," said CNN Meteorologist Haley Brink.

"The combination of these weather factors will allow for increased rain chances across much of the Florida peninsula on Tuesday, including the Cape Canaveral area. Showers and thunderstorms are forecast to be numerous and widespread across the region. Tropical storm-force winds from Ian could also arrive as early as Tuesday night across central Florida." Meanwhile, the Space Launch System rocket and Orion spacecraft continue to sit on the launchpad at Kennedy Space Center in Florida.

Team members continue to monitor the weather as they make a decision about when to roll the rocket stack back into the Vehicle Assembly Building at Kennedy. NASA will receive information from the US Space Force, the National Hurricane Center and the National Oceanic and Atmospheric Administration to inform their decision. [...] The rocket stack can remain at the pad and withstand winds up to 85 miles per hour (74.1 knots). If the stack needs to roll back into the building, it can handle sustained winds less than 46 miles per hour (40 knots). On Friday, the Artemis team said that October 2 was a backup launch date. But it's unlikely that a new launch date will be set until the rollback decision has been made.

An anonymous reader quotes a report from Ars Technica: In January this year, an undersea volcano in Tonga produced a massive eruption, the largest so far this century. The mixing of hot volcanic material and cool ocean water created an explosion that sent an atmospheric shockwave across the planet and triggered a tsunami that devastated local communities and reached as far as Japan. The only part of the crater's rim that extended above water was reduced in size and separated into two islands. A plume of material was blasted straight through the stratosphere and into the mesosphere, over 50 km above the Earth's surface. We've taken a good look at a number of past volcanic eruptions and studied how they influence the climate. But those eruptions (most notably that of Mount Pinatubo) all came from volcanoes on land. Hunga Tonga may be the largest eruption we've ever documented that took place under water, and the eruption plume contained unusual amounts of water vapor -- so much of it that it actually got in the way of satellite observations at some wavelengths. Now, researchers have used weather balloon data to reconstruct the plume and follow its progress during two circuits around the globe.

Your vocabulary word of the day is radiosonde, which is a small instrument package and transmitter that can be carried into the atmosphere by a weather balloon. There are networks of sites where radiosondes are launched as part of weather forecasting services; the most relevant ones for Hunga Tonga are in Fiji and Eastern Australia. A balloon from Fiji was the first to take instruments into the eruption plume, doing so less than 24 hours after Hunga Tonga exploded. That radiosonde saw increasing levels of water as it climbed through the stratosphere from 19 to 28 kilometers of altitude. The water levels had reached the highest yet measured at the top of that range when the balloon burst, bringing an end to the measurements. But shortly after, the plume started showing up along the east coast of Australia, which again registered very high levels of water vapor. Again, water reached to 28 km in altitude but gradually settled to lower heights over the next 24 hours.

The striking thing was how much of it there was. Compared to normal background levels of stratospheric water vapor, these radiosondes were registering 580 times as much water even two days after the eruption, after the plume had some time to spread out. There was so much there that it still stood out as the plume drifted over South America. The researchers were able to track it for a total of six weeks, following it as it spread out while circling the Earth twice. Using some of these readings, the researchers estimated the total volume of the water vapor plume and then used the levels of water present to come up with a total amount of water put into the stratosphere by the eruption. They came up with 50 billion kilograms. And that's a low estimate, because, as mentioned above, there was still water above the altitudes where some of the measurements stopped. The recent findings appear in a new study published in the journal Science.

A pair of researchers who previously identified what may be the first known interstellar meteor to impact Earth have now presented evidence of a second object that could have originated beyond the solar system, before it burned up in our planet's skies and potentially fell to the surface, according to a new study. Motherboard reports: Amir Siraj, a student in astrophysics at Harvard University, and astronomer Avi Loeb, who serves as Harvard's Frank B. Baird Jr. Professor of Science, suggest that a fast-moving meteor that burst into a fireball hundreds of miles off the coast of Portugal on March 9, 2017, is an "additional interstellar object candidate" that they call interstellar meteor 2 (IM2) in a study posted to the preprint server arXiv this week. The paper has not been peer-reviewed. In addition to their potential origin beyond the solar system, these objects appear to be extraordinarily robust, as they rank as the first- and third-highest meteors in material strength in a NASA catalog that has collected data about hundreds of fireballs.

"We don't have a large enough sample to say how much stronger interstellar objects are than solar system objects, but we can say that they are stronger," Siraj said in an email. "The odds of randomly drawing two objects in the top 3 out of 273 is 1 in 10 thousand. And when we look at the specific numbers relative to the distribution of objects, we find that the Gaussian odds are more like 1 in a million." This makes IM2 "an outlier in material strength," Loeb added in a follow-up call with Siraj. "To us, it means that the source is different from planetary systems like the solar system."

Loeb has attracted widespread attention in recent years over his speculation that the first interstellar object ever identified, known as 'Oumuamua, was an artifact of alien technology. Spotted in 2017, 'Oumuamua sped through the solar system and was up to a quarter-mile in scale, making it much larger than the interstellar meteor candidates identified by Siraj and Loeb, which are a few feet across. Loeb's claims of an artificial origin for 'Oumuamua have provoked substantial pushback from many scientists who do not consider a technological explanation to be likely. Loeb also thinks these interstellar meteor candidates could be alien artifacts, though he and Siraj present a mind-boggling natural explanation for the strangely robust objects in the study: The meteors may be a kind of interstellar shrapnel produced by the explosions of large stars, called supernovae. [...] Loeb, of course, is keeping his mind open. "We don't say, necessarily, that it is artificial," Loeb said in the call, referring to the supernovae explanation. But, he added, "obviously, there is a possibility that a spacecraft was designed to sustain such harsh conditions as passing through the Earth's atmosphere, so we should allow for that."

According to NASA, the James Webb Space Telescope has captured the clearest view of Neptune's rings in more than 30 years. From the report: Most striking in Webb's new image is the crisp view of the planet's rings -- some of which have not been detected since NASA's Voyager 2 became the first spacecraft to observe Neptune during its flyby in 1989. In addition to several bright, narrow rings, the Webb image clearly shows Neptune's fainter dust bands. "It has been three decades since we last saw these faint, dusty rings, and this is the first time we've seen them in the infrared," notes Heidi Hammel, a Neptune system expert and interdisciplinary scientist for Webb. Webb's extremely stable and precise image quality permits these very faint rings to be detected so close to Neptune.

Webb's Near-Infrared Camera (NIRCam) images objects in the near-infrared range from 0.6 to 5 microns, so Neptune does not appear blue to Webb. In fact, the methane gas so strongly absorbs red and infrared light that the planet is quite dark at these near-infrared wavelengths, except where high-altitude clouds are present. Such methane-ice clouds are prominent as bright streaks and spots, which reflect sunlight before it is absorbed by methane gas. Images from other observatories, including the Hubble Space Telescope and the W.M. Keck Observatory, have recorded these rapidly evolving cloud features over the years. More subtly, a thin line of brightness circling the planet's equator could be a visual signature of global atmospheric circulation that powers Neptune's winds and storms. The atmosphere descends and warms at the equator, and thus glows at infrared wavelengths more than the surrounding, cooler gases.

Neptune's 164-year orbit means its northern pole, at the top of this image, is just out of view for astronomers, but the Webb images hint at an intriguing brightness in that area. A previously-known vortex at the southern pole is evident in Webb's view, but for the first time Webb has revealed a continuous band of high-latitude clouds surrounding it. Webb also captured seven of Neptune's 14 known moons. Dominating this Webb portrait of Neptune is a very bright point of light sporting the signature diffraction spikes seen in many of Webb's images, but this is not a star. Rather, this is Neptune's large and unusual moon, Triton.

The Mars rover Perseverance was the subject of a new NASA briefing Thursday. CNET describes it as a celebration of this year's discovery of organic matter — in June NASA for the first time measured the total amount of organic carbon in Martian rocks — and a celebration of rock samples. (Specifically, the two samples collected from mudstone rock on Wildcat Ridge in Jezero Crater.) The rover's Sherloc instrument investigated the rock. (Sherloc stands for Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals.) "In its analysis of Wildcat Ridge, the Sherloc instrument registered the most abundant organic detections on the mission to date," NASA said.

Scientists are seeing familiar signs in the analysis of Wildcat Ridge. "In the distant past, the sand, mud and salts that now make up the Wildcat Ridge sample were deposited under conditions where life could potentially have thrived," said Perseverance project scientist Ken Farley in a statement. "The fact the organic matter was found in such a sedimentary rock — known for preserving fossils of ancient life here on Earth — is important."

Perseverance isn't equipped to find definitive evidence of ancient microbial life on the red planet. "The reality is the burden of proof for establishing life on another planet is very, very high," said Farley during the press conference. For that, we need to examine Mars rocks up close and in person in Earth labs. Perseverance currently has 12 rock samples on board, including the Wildcat Ridge pieces and samples from another sedimentary delta rock called Skinner Ridge. It also collected igneous rock samples earlier in the mission that point to the impact of long-ago volcanic action in the crater. NASA is so happy with the diversity of samples collected that it's looking into dropping some of the filled tubes off on the surface soon in preparation for the future Mars Sample Return campaign.... The mission is under development. If all goes as planned, those rocks could be here by 2033 .
The hope is that in 2033, Perseverance will meet the lander "and personally deliver the samples," the article quips. But in the meantime, Perseverance "could wander up the crater rim." And there's one more update about the smaller exploration vehicle that Peseverance carried to Mars.

"Its companion Ingenuity helicopter is in good health and expected to take to the air again."

On Sept. 26, the Double Asteroid Redirection Test (DART) mission will slam headfirst into a small asteroid in the name of planetary defense. "[S]cientists hope that should a dangerous asteroid threaten the planet in the future, a mission like DART could avert the disaster," reports Space.com. From the report: The theory goes that if scientists ever detected an asteroid on a collision course with Earth, an impactor probe could realign the orbit of the space rock, ensuring that it crossed Earth's path when our planet was a safe distance away. But scientists don't want to be working only from theory if the situation arises. That's where DART's dramatic destruction comes into play. The spacecraft will slam into a small asteroid called Dimorphos, which like clockwork orbits a larger near-Earth asteroid called Didymos every 11 hours and 55 minutes. (Neither asteroid poses any threat to Earth, and DART won't change that.) The DART impact should adjust the orbit of Dimorphos, cutting its circuit by perhaps 10 minutes.

Scientists on Earth will be spending weeks after the impact measuring the actual change in the moonlet's orbit to compare with their predictions. The work will refine scientists' understanding of how asteroids respond to impactors and help to tune any future missions to the necessary amount of orbital change. "This isn't just a one-off event," Nancy Chabot, the DART coordination lead at the Johns Hopkins University's Applied Physics Laboratory in Maryland, which runs the mission, said during the news conference. "We want to know what happened to Dimorphos, but more important, we want to understand what that means for potentially applying this technique in the future."

While the stakes are low compared to any scenario that would motivate a real asteroid-deflecting mission, the difficulty is the same. "This is incredibly challenging," Evan Smith, the deputy mission system engineer, said during the news conference, noting that the spacecraft will only be able to see Dimorphos itself about an hour and a half before impact. "This is a par-one course, so we're going in for the hit this time." And if something doesn't go according to plan? Mission personnel are pretty confident that, as long as the spacecraft hits its target, there should be something to see. "If DART collides with Dimorphos and then you don't see any orbital period change, this would be exceptionally surprising," Chabot said. "Just the amount of momentum that DART is bringing in on its own from the weight of the spacecraft slamming into Dimorphos is enough to shift its orbit in a measurable way."

SiFive is the first company to produce a chip implementing the RISC-V ISA.

They've now been selected to provide the core CPU for NASA's next generation High-Performance Spaceflight Computing processor (or HSPC), according to a SiFive announcement: HPSC is expected to be used in virtually every future space mission, from planetary exploration to lunar and Mars surface missions.

HPSC will utilize an 8-core, SiFive® Intelligence X280 RISC-V vector core, as well as four additional SiFive RISC-V cores, to deliver 100x the computational capability of today's space computers. This massive increase in computing performance will help usher in new possibilities for a variety of mission elements such as autonomous rovers, vision processing, space flight, guidance systems, communications, and other applications....

The SiFive X280 is a multi-core capable RISC-V processor with vector extensions and SiFive Intelligence Extensions and is optimized for AI/ML compute at the edge. The X280 is ideal for applications requiring high-throughput, single-thread performance while under significant power constraints. The X280 has demonstrated a 100x increase in compute capabilities compared to today's space computers..

In scientific and space workloads, the X280 provides several orders of magnitude improvement compared to competitive CPU solutions.
A business development executive at SiFive says their X280 core "demonstrates orders of magnitude performance gains over competing processor technology," adding that the company's IP "allows NASA to take advantage of the support, flexibility, and long-term viability of the fast-growing global RISC-V ecosystem.

"We've always said that with SiFive the future has no limits, and we're excited to see the impact of our innovations extend well beyond our planet."

And their announcement stresses that open hardware is a win for everybody: The open and collaborative nature of RISC-V will allow the broad academic and scientific software development community to contribute and develop scientific applications and algorithms, as well optimizing the many math functions, filters, transforms, neural net libraries, and other software libraries, as part of a robust and long-term software ecosystem.

America's Department of Agriculture and NASA recently announced the Artemis Moon Trees Program. After the first launch of its SLS super-heavy-lift launch vehicle, "the seeds carried on Artemis I will be grown into seedlings by the Forest Service and distributed to locations across the U.S."

But it's just part of a larger initiative. The U.S. government announced Friday that it's working with "a new coalition of space companies that will focus on increasing the space industry's capacity to meet the rising demand for the skilled technical workforce" — partly by inspiring and educating the next generation. This coalition includes Lockheed Martin, Northrop Grumman, Boeing, Blue Origin, Jacobs, L3Harris, Planet Labs PBC, Rocket Lab, Sierra Space, Space X and Virgin Orbit.

Long-time Slashdot reader theodp writes: Yesterday at the second convening of America's National Space Council, Vice President Kamala Harris announced "new commitments from the U.S. government, private sector companies, education and training providers, and philanthropic organizations to support space-related STEM initiatives to inspire, prepare, and employ the next generation of the space workforce..." according to a statement from the White House, "to address the challenges of today and prepare for the discoveries of tomorrow...."

Among those anchoring the Administration's efforts to increase the space industry's capacity to meet the rising demand for the skilled technical workforce is Amazon founder Jeff Bezos' space tourism company Blue Origin, which will be joined by industry partner Amazon to inspire youth to pursue space STEM careers. "Blue Origin's Club for the Future," the White House explains, "is launching Space Days to engage millions of students, teachers and school administrators in the excitement of space and space careers." Club for the Future, as reported earlier on Slashdot, is the Blue Origin founded-and-funded tax-exempt foundation that received the $28 million proceeds of a single auctioned ticket to accompany Bezos on Blue Origin's maiden 11-minute space tourism flight in June 2021. The nonprofit's mission is "to inspire future generations to pursue careers in STEM and to help invent the future of life in space."

The White House also announced that Amazon and Bezos-funded nonprofit Code.org "will highlight connections between computer science and space exploration in the 2022 Hour of Code. Students will have the opportunity to explore and develop coding skills through engaging, space-themed tutorials and create shareable projects. Through a collaboration with NASA, the U.S. Space Force, America's Department of Energy, and the U.S. Geological Survey, students will also learn about different careers and pathways for space careers in these agencies. Code.org reaches approximately 15 million students annually." Amazon reported in 2018 on its efforts to accelerate K-12 CS education in the U.S. with Code.org to "support the much-needed pipeline for workers who are well versed in computer science."
The coalition's other efforts include three pilot programs collaborating with community colleges, unions and others "to demonstrate a replicable and scalable approach to attracting, training and creating employment opportunities." Federal agencies and the Smithsonian Institute also launched a new web site with free space-related resources for K-12 educators which also promotes career awareness.

And NASA also released an educator resources hub that includes a LEGO Build to Launch Series — plus $4 million in educational grants.

When they examined decades-old blood samples from 14 NASA astronauts who flew Space Shuttle missions between 1998 and 2001, researchers found that samples from all 14 astronauts showed mutations in their DNA. Futurism reports: While these mutations are likely low enough not to represent a serious threat to the astronauts' long term health, the research underlines the importance of regular health screenings for astronauts, especially as they embark on longer missions to the Moon and beyond in coming years. The specific mutations, as identified in a new study published in the journal Nature Communications Biology, were marked by a high proportion of blood cells that came from a single clone, a phenomenon called clonal hematopoiesis. Mutations like this can be caused by exposure to excess ultraviolet radiation, and other forms of radiation including chemotherapy. In this case, researchers are suspicious that the mutations may have been the result of space radiation.

"Astronauts work in an extreme environment where many factors can result in somatic mutations, most importantly space radiation, which means there is a risk that these mutations could develop into clonal hematopoiesis," said lead author David Goukassian, professor of medicine at the Icahn School of Medicine at Mount Sinai, in a statement. The blood samples for this latest study were collected from 12 male and two female astronauts ten days before their flight and on the day of their landing. The samples were then cryogenically stored at -112 degrees Fahrenheit for around two decades. The mutations observed in the blood samples resemble the kind of somatic mutations we see in older individuals -- which is interesting on its own, considering the median age of the astronauts was only 42.

"Although the clonal hematopoiesis we observed was of a relatively small size, the fact that we observed these mutations was surprising given the relatively young age and health of these astronauts," Goukassian said. "The presence of these mutations does not necessarily mean that the astronauts will develop cardiovascular disease or cancer," he added, "but there is the risk that, over time, this could happen through ongoing and prolonged exposure to the extreme environment of deep space." Therefore, Goukassian and his team are recommending that NASA should regularly screen astronauts for these kinds of mutations.

NASA said Thursday that it is working to fix the issues that delayed the launch of its Artemis I moon rocket last week, and that it hopes to make another attempt later this month. CNBC reports: The space agency on Sept. 3 called off the second attempt to launch the mission after detecting a hydrogen leak as the Space Launch System (SLS) rocket was being fueled. The Artemis I mission represents the debut of the SLS rocket and the uncrewed Orion capsule it is carrying, for what is expected to be a more than month-long journey around the moon. NASA made several unsuccessful attempts during the launch countdown on Saturday to fix the leak.

During a press conference on Thursday, NASA officials said work at the launchpad is ongoing, with the agency's team aiming to complete the replacement of seals on the fueling system by the end of the day. NASA then hopes to conduct a tanking demonstration on Sept. 17 to verify the replacement work was successful. Assuming the work and testing are completed by then, NASA has requested new launch dates from the U.S. Space Force's Eastern Range -- which reviews and approves all missions that liftoff from Cape Canaveral region. The agency has asked to make launch attempts on Sept. 23 and Sept. 27.

An international team of scientists says it has discovered two new "super-Earth" type planets about 100 light-years away, one of which may be suitable for life. NPR reports: Unlike any of the planets in our solar system, the nearly 1,600 known super-Earths are larger than Earth, but lighter than icy planets like Uranus and Neptune. Researchers at Belgium's University of Liege announced Wednesday that they found another one while using Earth-based telescopes to confirm the existence of a different planet initially discovered by a NASA satellite in the same solar system.

NASA's satellite found planet LP 890-9b, which is about 30% larger than Earth and orbits its sun in just 2.7 days. ULiege researchers used their SPECULOOS (Search for habitable Planets EClipsing ULtra-cOOl Stars) telescopes in Chile and Spain to take a closer look at the planet with high-precision cameras. That's when the stargazers discovered another planet, LP 890-9c (renamed SPECULOOS-2c by the ULiege researchers), which is 40% larger than Earth and takes 8.5 days to orbit its sun. Francisco Pozuelos, a researcher at the Institute of Astrophysics of Andalusia and one of the main co-authors of the paper, said in a news release that the planet could be suitable to life despite being a mere 3.7 million miles from its sun. Earth, by comparison, is located over 93 million miles away from our sun. "Although this planet orbits very close to its star, at a distance about 10 times shorter than that of Mercury around our Sun, the amount of stellar irradiation it receives is still low, and could allow the presence of liquid water on the planet's surface, provided it has a sufficient atmosphere," Pozuelos said. "This is because the star LP 890-9 is about 6.5 times smaller than the Sun and has a surface temperature half that of our star."

With 8.8 million pounds of thrust, NASA's SLS would've been the most powerful rocket ever launched into space, notes the Orlando Sentinel.

But instead on Saturday morning, "NASA scrubbed its second attempt to launch the Artemis I mission into lunar orbit..." reports CNET. "During a press conference later in the day, Jim Free, an associate administrator at NASA Headquarters, said we shouldn't expect to see a third attempt within this launch period, which culminates Tuesday." (Though the mission manager the next launch attempt could be as late as mid-October.)

"This time, the culprit was a liquid hydrogen leak that showed up while the team was loading the rocket's core stage...." According to the space agency, the leak occurred "while loading the propellant into the core stage of the Space Launch System rocket" and that "multiple troubleshooting efforts to address the area of the leak, by reseating a seal in the quick disconnect where liquid hydrogen is fed into the rocket, did not fix the issue."

This is the second time the Artemis I mission has been delayed. Liftoff attempt No. 1 was scheduled for Monday, but launch director Charlie Blackwell-Thompson had to call a scrub then as well, because of an unyielding problem with what's known as an engine bleed test. (This process is meant to allow the engines to chill to the right temperature by releasing a small amount of the fuel).

"We were unable to get the engines within the thermal conditions required to commit to launch," Artemis mission manager Mike Sarafin said during a press conference on Tuesday. "In combination with that, we also had a bent valve issue on the core stage, and it was at that point that the team decided to knock off the launch attempt for that day."

Stefanie Waldek reports via Space.com: Led by the Massachusetts Institute of Technology (MIT), the Mars Oxygen In-Situ Resource Utilization Experiment (MOXIE) is a small instrument on the Perseverance rover that's designed to transform carbon dioxide, which comprises some 96% of the atmosphere on Mars, into breathable oxygen. Oxygen, of course, is crucial for a human mission to Mars. Since February 2021, the device has run seven times, each time producing about 0.2 ounces (6 grams) of oxygen per hour. That's on par with the abilities of small trees here on Earth.

MOXIE has now operated in a variety of conditions on Mars, both day and night, through all four seasons. The researchers expect that a version of the instrument approximately 100 times larger than MOXIE could potentially create breathable oxygen for future astronauts who visit the Red Planet. If explorers can't make their own oxygen on Mars, supplies from Earth would take up valuable mass on a spacecraft. Furthermore, MOXIE's products could also be used as an ingredient for rocket fuel -- pretty crucial to ensuring the mission isn't one-way. A rocket would need 33 to 50 tons (30 to 45 metric tons) of liquid oxygen propellant in order to launch humans off Mars. "This is the first demonstration of actually using resources on the surface of another planetary body, and transforming them chemically into something that would be useful for a human mission," MOXIE deputy principal investigator Jeffrey Hoffman, a professor of the practice in MIT's Department of Aeronautics and Astronautics and a former NASA astronaut, said in a statement. "It's historic in that sense."

The research has been published in the journal Science Advances.

A critical system aboard the probe was sending garbled data about its status. Engineers have fixed the issue but are still seeking the root cause. NASA reports: Engineers have repaired an issue affecting data from NASA's Voyager 1 spacecraft. Earlier this year, the probe's attitude articulation and control system (AACS), which keeps Voyager 1's antenna pointed at Earth, began sending garbled information about its health and activities to mission controllers, despite operating normally. The rest of the probe also appeared healthy as it continued to gather and return science data. The team has since located the source of the garbled information: The AACS had started sending the telemetry data through an onboard computer known to have stopped working years ago, and the computer corrupted the information.

Suzanne Dodd, Voyager's project manager, said that when they suspected this was the issue, they opted to try a low-risk solution: commanding the AACS to resume sending the data to the right computer. Engineers don't yet know why the AACS started routing telemetry data to the incorrect computer, but it likely received a faulty command generated by another onboard computer. If that's the case, it would indicate there is an issue somewhere else on the spacecraft. The team will continue to search for that underlying issue, but they don't think it is a threat to the long-term health of Voyager 1.

NASA delayed the debut launch of its new massive rocket due to an issue with one of its engines, dealing a temporary blow to the space agency's plan to return to the lunar surface. From a report: With Vice President Kamala Harris in attendance at Florida's Kennedy Space Center and a global audience watching online, the uncrewed Artemis I mission was called off at 8:34 a.m., one minute after its originally scheduled liftoff time. The launch missed its window after controllers were unable to resolve a temperature problem with one of the rocket's four main engines. The rocket and space capsule are in "a safe and stable configuration," NASA said Monday in a statement, adding that engineers were continuing to gather data.

The earliest available opportunity to try again is on Sept. 2, NASA said in a webcast while announcing the scrubbed launch. No decision has been made on rescheduling. Official confirmation of the delay came after the space agency spent the early morning hours investigating issues including a potential crack in material in the main body of the rocket as well as the temperature issue, officials said earlier Monday. Those came after engineers examined and resolved a suspected leak affecting the hydrogen tanking process.

United Launch Alliance has been developing a heavy-lift space vehicle since 2014 (with investment from the U.S. military) called the Vulcan Centaur.

So CNN reports that the ashes of the late Star Trek actress Nichelle Nichols "will head to deep space on a Vulcan rocket." Nichols' cremated remains will be aboard the first Celestis Voyager Memorial Spaceflight, which will launch from Cape Canaveral, Florida. Celestis, Inc., is a private company that conducts memorial spaceflights. Among the remains also aboard the flight will be the ashes of "Star Trek" creator Gene Roddenberry; his wife, Majel Barrett-Roddenberry, who played various roles in the show and films; and James Doohan, who played Montgomery "Scotty" Scott in the films and TV series....

The spaceflight will travel beyond NASA's James Webb Space Telescope and into interplanetary deep space. In addition to cremated remains, capsules onboard will also carry complete human genome DNA samples from willing participants.

People can participate in the flight — by having DNA or loved ones' remains in a spaceflight container — for a price starting at $12,500, and reservations close August 31. (Celestis offers other voyages that don't travel as far, but can cost less than $5,000.) Ahead of the flight's liftoff, Celestis will host a three-day event with mission briefings, an astronaut-hosted dinner, launch site tours, an on-site memorial service and launch viewing. All events will be shown via webcast, according to Celestis.
An announcement on the flight's site invites fans of Nichelle Nichols to "share your own story about how she inspired you and it will be sent into deep space aboard the first Celestis Voyager Memorial Spaceflight — the Enterprise Flight, launching later in 2022."

"Over the past year, nuclear fusion has inched closer to reality," the Washington Post reported Friday.

"Scientists are mere years from getting more energy out of fusion reactions than the energy required to create them, they said. Venture capitalists are pumping billions into companies, racing to get a fusion power plant up and running by the early 2030s. The Biden administration, through the Inflation Reduction Act and the Department of Energy, is creating tax credits and grant programs to help companies figure out how to deploy this kind of energy." (One fusion company's CEO argues that "Once the technology is shown to work, it's less risky, and the next buyer of that technology could get a commercial loan.")

But even with all this new excitement, challenges still remain, nuclear scientists warn: The U.S. energy grid would need a significant redesign for fusion power plants to become common. The price of providing fusion power is still too high to be feasible. "We're at a very exciting place," said Dennis G. Whyte, director of MIT's Plasma Science and Fusion Center. "But we also have to be realistic in the sense that it's still very hard...."

Phil Larochelle, a partner at the venture capital firm Breakthrough Energy Ventures, said private money is flowing into fusion at such high levels because scientific advancements, such as better magnets, have made cheap nuclear fusion a likelier possibility. Going forward, Larochelle noted that getting nuclear fusion to market probably will require formal cost-sharing programs with the government, which he said could be similar to how NASA is partnering with SpaceX for space travel innovation. "In both the U.S. and the U.K., there's now kind of new government programs and support for trying to get to a [fusion] pilot," he said. "It's a good kind of risk-sharing between public and private [sectors]."

Despite the growing government collaboration, Whyte said, a few challenges remain. The effects of climate change are increasingly irreversible, and the clock is ticking, he said, making fusion energy a crucial need. Companies will have to figure out how to deploy the technology widely. Doing it cheaply is most important, he said. "What I worry about is that we'll get to a system where we can't actually make it economically attractive fast enough," he added. Moreover, to create an electricity grid through which fusion technology provides large amounts of power, many things need to happen. Universities need to churn out scientists more capable of working on fusion technology. Fusion power companies need to build devices that create more energy than they consume. Scientific and manufacturing materials must be constructed in difficult ways if power plants want to scale.

"Can we get there?" Whyte asked. "I think we can if we get our act together in the right way. But there's no guarantee of that."

Space can be downright noisy in the right conditions, such as the hot gas surrounding the immense black hole at the center of the Perseus galaxy cluster, according to NASA. Motherboard reports: The agency recently tweeted an eerie audio clip that represents actual sound waves rippling through the gas and plasma in this cluster, which is 250 million light years from Earth. "The misconception that there is no sound in space originates because most space is a ~vacuum, providing no way for sound waves to travel," the agency tweeted. "A galaxy cluster has so much gas that we've picked up actual sound. Here it's amplified, and mixed with other data, to hear a black hole!"

Though the acoustic signals generated by the black hole were first identified in 2003 in data from NASA's Chandra X-ray Observatory, they have never been brought into the hearing range of the human ear -- until now. "In some ways, this sonification is unlike any other done before... because it revisits the actual sound waves discovered in data from NASA's Chandra X-ray Observatory," NASA said in a statement. "In this new sonification of Perseus, the sound waves astronomers previously identified were extracted and made audible for the first time." "As it turns out, the sound waves in their natural environment are a whopping 57 octaves below the note middle C, making this black hole a real cosmic baritone," adds Motherboard. "To make these tremors audible to humans, scientists raised their frequencies quadrillions of times (one quadrillion is a million billions, for perspective)."

The James Webb Space Telescope has snapped a pair of near-infrared photos showing Jupiter's polar auroras. "You can also see the planet's extremely faint rings and two of its smaller moons, Amalthea (the bright spot to the far left) and Adrastea (the dot at the left edge of the central ring)," notes Engadget. From the report: The pictures were taken using NIRCam's widefield view on July 27th. As for the trippy visuals? Astronomers created composites using several images produced with filters mapped to multiple colors (particularly visible in the image below). The Great Red Spot and other cloud formations are white as they reflect large amounts of sunlight. The observations should provide more insights into Jupiter's "inner life," according to the European Space Agency. That, in turn, could help scientists understand the behavior of gas giants beyond the Solar System.