diff --git "a/raw_rss_feeds/https___www_space_com_feeds_all.xml" "b/raw_rss_feeds/https___www_space_com_feeds_all.xml" --- "a/raw_rss_feeds/https___www_space_com_feeds_all.xml" +++ "b/raw_rss_feeds/https___www_space_com_feeds_all.xml" @@ -10,8 +10,101 @@
As the shutdown continues into its second month, many federal employees are furloughed. Some, however, keep working (mostly without pay at the moment), because they're considered critical to the continued operation of the nation's functions, like the delivery of the mail.
Thankfully for the NASA astronauts aboard the International Space Station (ISS), their wellbeing falls into the category of "protection of life and safety," which NASA is tasked with maintaining while the government's doors are closed.
Like all federal agencies, NASA has had to severely cut back on its day-to-day activities, as more than 15,000 NASA civil servants have been furloughed since Oct. 1. Only essential personnel deemed "necessary to protect life and property" are granted "excepted" status, according to NASA's shutdown guidance. This includes astronauts in space and the technicians in mission control on the ground who support them.
For the most part, life aboard the ISS has continued as usual. The Expedition 73 crew currently occupying the space station have spent the past month conducting microgravity research and other experiments on their rotation and performing scheduled maintenance.
Of the seven astronauts currently living on the ISS, three are from the Russian space agency Roscosmos — Sergey Ryzhikov, Alexey Zubritsky and Oleg Platonov — and another is Japan's Kimiya Yui, from Japan.
The remaining three are NASA's Jonny Kim, Zena Cardman and Mike Fincke. Like their international counterparts, they've continued pulling their fair share of the chores in space. They just aren't getting paid for it. Like every other federal employees forced to work during the shutdown, they will later receive backpay compensation for the time they're currently putting in.
This past week, for example, Japan's new HTV-X1 cargo spacecraft launched and rendezvoused with the ISS. All three NASA astronauts were on hand for that capture and were scheduled to help unload its cargo on Friday (Oct. 31).
One thing NASA's astronauts aren't doing is updating their social media feeds or other lines of public communication. Yui, though, has been filling that gap. Over the last month, he has posted stunning views of Earth that have included the HTV-X arrival, comet Lemon above the thin line of Earth's atmosphere, and auroras from space.
今日は、少し違ったレンズでレモンさんを撮影してみました。ISSは地上から約400km上空ですので、地上がまだ夜でも、ISSでは既に陽が昇ってきます。彗星が太陽に近づく事で、ISSからの撮影機会がとても短くなってきました。HTV-X君のお迎えに集中する様にレモンさんが気を遣ってくれているのかも笑。 pic.twitter.com/4Ng456jOpZOctober 26, 2025
おはようございます!今日は、皆さんに特別見て頂きたい景色があり、仕事を早めに進めて、時間を作りつつ撮影しました。「きぼう」の窓から撮影した写真としては、歴代でも5本の指に入る絶景ではないでしょうか?自画自賛です笑(今日は、ISSが普段とは違う姿勢になったので窓の景色も変化しました) pic.twitter.com/a07yWavRbiOctober 14, 2025
NASA has also classified work on the agency's Artemis moon program as critical and therefore continues work to launch the four-astronaut Artemis 2 mission around the moon as early as February 2026.
While work on Artemis has progressed, the continued shutdown may put a strain on agency resources as more and more employees are forced to work without pay. Delays could push the mission's hopeful February target date further into the launch window, which extends through April.
And any delay to Artemis 2 could be bad news for the timeline of Artemis 3, which will be NASA's first mission to land astronauts on the lunar surface since the end of the Apollo program in the 1970s. China, too, has aspirations of landing astronauts (or, as China calls them, "taikonauts") on the moon, and NASA and U.S. lawmakers have repeatedly stressed the importance of winning this new "moon race."
]]>The International Space Station is one of the most remarkable achievements of the modern age. It is the largest, most complex, most expensive and most durable spacecraft ever built.
Its first modules were launched in 1998. The first crew to live on the International Space Station – an American and two Russians – entered it in 2000. Nov. 2, 2025, marks 25 years of continuous habitation by at least two people, and as many as 13 at one time. It is a singular example of international cooperation that has stood the test of time.
Two hundred and ninety people from 26 countries have now visited the space station, several of them staying for a year or more. More than 40% of all the humans who have ever been to space have been International Space Station visitors.
The station has been the locus of thousands of scientific and engineering studies using almost 200 distinct scientific facilities, investigating everything from astronomical phenomena and basic physics to crew health and plant growth. The phenomenon of space tourism was born on the space station. Altogether, astronauts have accumulated almost 127 person-years of experience on the station, and a deep understanding of what it takes to live in low Earth orbit.
If you've ever seen photos of the inside of the International Space Station, you've probably noticed the clutter. There are cables everywhere. Equipment sticks out into corridors. It doesn’t look like Star Trek's Enterprise or other science fiction spacecraft. There’s no shower for the crew, or a kitchen for cooking a meal from scratch. It doesn’t have an area designed for the crew to gather in their downtime. But even without those niceties, it clearly represents a vision of the future from the past, one where humanity would live permanently in space for the first time.
November 2025, by coincidence, also marks the 10th anniversary of my team's research on the space station, the International Space Station Archaeological Project. The long history of habitation on the space station makes it perfect for the kind of studies that archaeologists like my colleagues and me carry out.
We recognized that there had been hardly any research on the social and cultural aspects of life in space. We wanted to show space agencies that were already planning three-year missions to Mars what they were overlooking.
We wanted to go beyond just talking to the crew about their experiences, though we have also done that. But as previous studies of contemporary societies have shown, people often don't want to discuss all their lives with researchers, or they’re unable to articulate all their experiences.
Astronauts on Earth are usually trying to get their next ride back to space, and they understandably don't want to rock the boat. Our research provides an additional window onto life on a space station by using archaeological evidence: the traces of human interactions with the objects and built spaces of the site.
The problem, of course, is that we can't go to the station and observe it directly. So we had to come up with other ways to capture data. In November 2015, I realized that we could use the thousands of photos taken by the crew and published by NASA as a starting point. These would allow us to track the movement of people and things around the site over time, and to map the behaviors and associations between them.
In 2022, the International Space Station Archaeological Project also carried out the first archaeological fieldwork off the Earth, an experiment designed by my collaborator, Alice Gorman. We asked the crew to document six sample locations in different modules by taking photos of each one every day for two months.

We learned that the crew of the International Space Station is a lot like those of us on Earth – perhaps unsurprising, since they live 95% or more of their lives here with the rest of us. They decorate the walls of the station with pictures, memorabilia and, on the Russian side, religious items, the way you might put photos and souvenirs on your refrigerator door to say something about yourself and your family. They make birthday cakes for their colleagues. They love to snack on candy or other special foods that they selected to be sent.
Unlike the rest of us, however, they live without much freedom to make choices about their lives. Their days are governed by lengthy procedures overseen by Mission Control, and by lists of items and their locations.
Crew members do show some signs of autonomy, though. They sometimes create new uses for different areas. They used a maintenance work station for the storage of all kinds of unrelated things, just because it has a lot of Velcro for holding items in place. They have to come up with solutions for storing their toiletry kits because that kind of affordance wasn’t considered necessary by the station’s designers 30 or 40 years ago.
We discovered that despite the international nature of the station, most areas of it are highly nationalized, with each space agency controlling its own modules and, often, the activities going on in each one. This makes sense, since each agency is responsible to their own taxpayers and needs to show how their money is being spent. But it probably isn't the most efficient way to run what is the most expensive building project in the history of humanity.
In our latest research, we tracked changes in scientific activity, which we found has become increasingly diverse, by documenting the use of specialized experimental equipment. This work was the result of questions from one of the companies competing to build a commercial successor to the International Space Station in low Earth orbit.
The company wanted to know if we could tell them what facilities their customers were likely going to need. Of course, understanding how people have used different parts of a site over time is a typical archaeological problem. They are using our results to improve the experiences of their crews.
Similar archaeological studies of contemporary issues here on Earth can also make future lives better, whether by studying phenomena such as migration, ethnonationalism or ecological issues.
In this way, we and other contemporary archaeologists are charting a new future for studying the past, a path for our discipline that lies alongside our traditional work of investigating ancient societies and managing heritage resources. Our International Space Station work also demonstrates the relevance of social science research for solving all kinds of problems – even ones that seem to be purely technical, like living in space.
You can read the original article here.
]]>Sunday (Nov. 2) marked the 25th anniversary of continuous human occupation of the International Space Station (ISS), which has carved out a spot in the history books as one of our species' grandest (and most expensive) technological achievements.
Don't save any confetti for a semicentennial celebration, however — the ISS is in its home stretch. NASA and its partners plan to deorbit the aging outpost toward the end of 2030, using a modified, extra-burly version of SpaceX's Dragon cargo capsule to bring it down over an uninhabited stretch of ocean.
And not just any stretch — the "spacecraft cemetery," a patch of the Pacific centered on Point Nemo, which is named after the famous submarine captain in Jules Verne's 1871 novel "Twenty Thousand Leagues Under the Sea."
"This remote oceanic location is located at coordinates 48°52.6′S 123°23.6′W, about 2,688 kilometers [1,670 miles] from the nearest land — Ducie Island, part of the Pitcairn Islands, to the north; Motu Nui, one of the Easter Islands, to the northeast; and Maher Island, part of Antarctica, to the south," officials with the U.S. National Oceanic and Atmospheric Administration wrote in a brief Point Nemo explainer.
That remoteness explains Point Nemo's appeal to mission planners, who have ditched several hundred big spacecraft there over the decades: If there's no land nearby, there's virtually no chance that chunks of falling, flaming hardware could harm people, buildings or other infrastructure. (You'd have to be a pretty unlucky sailor to get hit in the spacecraft cemetery).
And some pieces of the ISS are likely to survive its blazing reentry.
"NASA engineers expect breakup to occur as a sequence of three events: solar array and radiator separation first, followed by breakup and separation of intact modules and the truss segment and finally individual module fragmentation and loss of structural integrity of the truss," agency officials wrote in an FAQ about the ISS transition plan.
"As the debris continues to re-enter the atmosphere, the external skin of the modules is expected to melt away and expose internal hardware to rapid heating and melting," they added. "Most station hardware is expected to burn up or vaporize during the intense heating associated with atmospheric re-entry, whereas some denser or heat-resistant components like truss sections are expected to survive reentry and splash down within an uninhabited region of the ocean."

This analysis is informed by the reentry behavior of other large spacecraft, such as the Soviet-Russian space station Mir and NASA's Skylab, agency officials explained. The final days of these two orbiting outposts hold some lessons for mission planners, especially as Earth orbit gets more and more crowded.
Russia steered Mir down to a controlled reentry near Point Nemo in March 2001. NASA tried to ditch Skylab over the Indian Ocean in July 1979 but didn't quite manage it; charred pieces of the station dropped onto a swath of Western Australia, and the town of Esperance famously fined NASA $400 for littering.
The 107-foot-long (33-meter-long), 130-ton Mir remains the largest vehicle ever to fall to Earth over the spacecraft cemetery (or anywhere else, for that matter), but the ISS will break that mark: It's about as long as a football field and weighs 460 tons.
]]>India launched a huge and powerful communications satellite for its navy early Sunday morning (Nov. 2).
The CMS-03 spacecraft, also known as GSAT-7R, lifted off atop a Launch Vehicle Mark-3 (LVM3) rocket from Satish Dhawan Space Centre Sunday at 6:56 a.m. EST (1056 GMT; 5:26 p.m. local time in India).

The LVM3 deployed the 9,700-pound (4,400-kilogram) CMS-03 into geostationary transfer orbit about 16 minutes after lifting off. It was the heaviest communications satellite ever launched to GTO from Indian soil, according to ISRO.
The spacecraft will eventually settle into geostationary orbit, a circular path that lies 22,236 miles (35,786 kilometers) above Earth. At this altitude, orbital speed matches our planet's rotational speed, allowing spacecraft there to "hover" over one patch of Earth continuously.
Geostationary orbit is therefore a popular destination for spy satellites and communications craft like CMS-03. The new satellite will serve as a key link for the Indian Navy, taking this mantle from GSAT-7, which launched in 2013.
"With upgraded payloads, GSAT-7R or CMS-03 is designed to expand secure, multi-band communications for the Navy’s growing blue-water operations," the Times of India wrote. "CMS-03 will provide real-time communication for naval operations, air defence and strategic command control across a wide oceanic and terrestrial region."

Sunday's launch was the eighth overall for the LVM3, which debuted in December 2014. The rocket's previous flight was in July 2023, when it successfully sent India's robotic Chandrayaan-3 mission to the moon's south polar region.
The 143-foot-tall (43.5-meter-tall) LVM3 is India's most powerful rocket. It can haul 17,600 pounds (8,000 kgs) to low Earth orbit, according to its ISRO specifications page.
]]>SpaceX just launched a satellite that could help pave the way for a private space station in the very near future.
A Falcon 9 rocket lifted off from Cape Canaveral Space Force Station in Florida today at 1:09 a.m. EDT (0509 GMT), on a multi-satellite rideshare mission that SpaceX calls Bandwagon-4.
Among the 18 payloads on board the Falcon 9 is Haven Demo, a pathfinder for Haven-1, the private space station that California company Vast Space plans to launch to Earth orbit next year.

"The first step in our iterative approach towards building next-generation space stations, Haven Demo will test critical systems for Haven-1, including propulsion, flight computers and navigation software," Vast wrote in a description of the satellite.
Vast's Haven-1 will launch to low Earth orbit (LEO) atop a Falcon 9, perhaps as soon as the second quarter of 2026. If that schedule holds, Haven-1 — which can support up to four astronauts at a time — will be the first standalone private space station in human history.
The other 17 payloads that went up today will be operated by South Korea's Agency for Defense Development (ADD), the Berlin-based company Exolaunch, Turkey's Fergani Space, the weather-forecasting outfit Tomorrow Companies and Starcloud, which aims to build data centers in space.
The Falcon 9's first stage came back to Earth as planned today about eight minutes after launch, touching down at Cape Canaveral's Landing Zone-2. It was the third flight for this particular booster, according to SpaceX.
The rocket's upper stage, meanwhile, continued carrying the 18 payloads to orbit. It will deploy them over an hour-long stretch that begins about 12 minutes after liftoff with the separation of ADD's Korea 425 satellite.
As its name suggests, Bandwagon-4 was the fourth mission in SpaceX's Bandwagon series to lift off. The company also operates another rideshare program called Transporter, which has 14 launches to its name to date.
Bandwagon-4 was the 140th Falcon 9 launch of 2025 already. More than 70% of the rocket's missions this year have been dedicated to building out Starlink, SpaceX's huge and ever-growing broadband megaconstellation.
]]>This inspiring PBS science documentary utilizes cinematic recreations and advanced CGI alongside more than a quarter-century of NASA archival footage to tell the complete story of this extraordinary human endeavor.
Per the official description, it's "an immersive experience that places viewers inside the cramped modules and spacewalks, to experience the claustrophobia, wonder, and split-second decisions that defined life aboard humanity's most remote outpost."
"What's remarkable about the stories that 'Operation Space Station' tells is the way they remind us that the potential for disaster is a constant companion for the astronauts and how time and again, through innovative ideas and productive collaboration, they averted disaster," said NOVA Co-Executive Producer Chris Schmidt. "Over 25 years of continual habitation, not a single life was lost aboard the ISS. It's a testament to the courage and dedication of every astronaut and engineer. This film is comprehensive, emotional, and cinematic, and a real inside look at how humanity can thrive under extreme conditions."

The initial chapter, "High-Risk Build," examines the ISS construction process and considers the astounding engineering achievement it was. NOVA's synopsis explains how "every step of this ambitious project unfolded against the backdrop of a merciless vacuum, dangerous radiation, and extreme temperatures."
A second chapter, "Science and Survival," reveals unexpected challenges that the crew encountered once the ISS was finished. Astronauts deliver memories of danger and heroism, "from the time astronaut Luca Parmitano's helmet filled with water while on a spacewalk, to the time a software glitch on a new module propelled the entire station to spin out of control."

Besides its past and present history, the docuseries ends by peering into the ISS's future as its journey is scheduled to conclude in 2030, when it is sadly de-orbited down into the Pacific Ocean.
"When you see the challenges that these astronauts had to overcome, you realize how thin the margin for error really is," said Executive Producer Dan Chambers. "These moments aren't just highlighting technical failures – they're showing people solving impossible problems, in the harshest environment we know of, with physics, chemistry, and sheer will."
"Operation Space Station: High-Risk Build" debuts Nov. 5, 2025 at 9 p.m. ET on PBS. "Operation Space Station: Science and Survival" drops Nov. 12, 2025, at 9 p.m. ET. Both will stream at PBS.org/NOVA, NOVA's YouTube channel, and the PBS Documentaries Prime Video Channel.
]]>
The sun is getting into the Halloween spirit once again. NASA's Solar Dynamics Observatory (SDO) captured a hauntingly festive view of our star on Oct. 28, looking like a cosmic jack-o'-lantern grinning down at Earth.
In the image, captured by SDO's Atmospheric Imaging Assembly (AIA), dark coronal holes and bright active regions combine to form what appears to be glowing eyes, a nose and a mischievous smile carved across the solar surface.
That "mouth" however, is more than just a decoration. It's actually a vast coronal hole, an area on the sun's surface where the magnetic field opens up, allowing charged particles (solar wind) to stream freely into space. This particular hole is currently spewing a high-speed solar wind stream toward Earth, which could spark minor (G1) to moderate (G2) geomagnetic storm conditions from Oct. 28 through Oct. 29, according to space weather forecasters.
If geomagnetic storm conditions intensify, auroras can spread beyond their usual polar locations, into mid-latitudes. 22 years ago this week, the infamous Halloween storms of 2003 saw a barrage of powerful solar eruptions trigger spectacular auroras and disrupt satellites and power systems worldwide.
SDO has been watching the sun since 2010, providing continuous, high-resolution views that help scientists understand how the sun's magnetic energy drives space weather, which in turn affects our lives here on Earth.
This isn't the first time the observatory has spotted a spooky face on the sun. Back in 2014, it captured this eerie jack-o'-lantern-like grin.

The X-59 is NASA's experimental new jet built to break the sound barrier without generating the thunderous sonic booms typically associated with supersonic flight.
After taxiing out of the U.S. Air Force's (USAF) Plant 42 facility, the X-59 took off from the Palmdale Regional Airport in California today (Oct. 28) at 10:13 a.m. EDT (1413 GMT), according to aircraft tracker Flightradar24. The airport and USAF facility share a runway.
X-59 unrestricted climb! pic.twitter.com/8vzeMZJoqmOctober 28, 2025
Videos and photos were posted to social media by aircraft spotters and photographers, showing the radically elongated X-59 taking off before flying north out of Palmdale. Photographer Jarod Hamilton caught the X-59 as it left the ground, making a steep climb into the air above the Mojave Desert.

NASA did not announce the flight publicly ahead of time. Following the flight, acting NASA administrator Sean Duffy praised the test flight in a Lockheed Martin statement. The X-59 was designed by NASA and built by Lockheed Martin at the company's storied Skunk Works facility in Palmdale.
"X-59 is a symbol of American ingenuity. The American spirit knows no bounds. It's part of our DNA – the desire to go farther, faster, and even quieter than anyone has ever gone before," Duffy said. "This work sustains America's place as the leader in aviation and has the potential to change the way the public flies."
Lockheed Martin's statement adds that the X-59 "performed exactly as planned" during its first flight.

Based on the X-59's track, it appears the X-plane flew oval-shaped "racetrack" patterns over the U.S. Air Force's Edwards Air Force Base for just over an hour before landing at the facility.
NASA's Armstrong Flight Research Center is located at the base. After this first flight, the X-59 will now reside at Armstrong, where it will undergo a testing campaign that will involve flying the jet over microphones placed throughout the desert and trailing other aircraft equipped with special air sensors through its shockwaves .

The X-59 was designed from the wheels up to be able to fly faster than the speed of sound without producing loud sonic booms, which can be disruptive to people on the ground below. Because of those booms, supersonic flight has been prohibited above land within a certain distance of the U.S. since 1973.

But NASA hopes to change that. If the X-59 can prove that "quiet" supersonic flight is possible, the restrictions on breaking the sound barrier above the populated U.S. could someday be lifted, allowing commercial supersonic flight. The high speeds of supersonic travel could also be a huge boon for disaster relief, medical transport and other industries.
To that end, President Trump issued an Executive Order earlier this year instructing the Federal Aviation Administration (FAA) to begin taking steps to repeal the prohibition on supersonic flight over the United States.
Several U.S. companies are also innovating aircraft aimed at ushering in a new era of supersonic travel. In January 2025, Colorado-based Boom Supersonic's XB-1 jet broke the sound barrier for the first time, marking the first time an independently-developed commercial aircraft achieved supersonic flight over the continental United States.
Editor's note: This story was updated on Oct. 29 to include comment from acting NASA administrator Sean Duffy and Lockheed Martin.
]]>Siddharth Patel, a 12-year-old who lives in London, Ontario (west of Toronto), spotted two possible asteroids in September as part of a citizen science program that partners with NASA, according to the Toronto Star.
The two suspected space rocks are called 2024 RX69 and 2024 RH39 and are cataloged in the Minor Planet Center, which is a branch of the International Astronomical Union that reports and tracks asteroids and other small, naturally occurring space objects.
Siddharth told the Star he pursues his love of astronomy — he's been using a telescope since age five, supported by parents with no space background — after finishing school activities.
"Space was not really taught in schools," he said. "I really started doing things about space after I came back from school, because school is the academic time. And after that is the time when I pursue my interests and dreams."
While confirming the asteroids' orbits may take as long as a decade, Patel has another big project on his mind: becoming an astronaut. He recently joined the youth-focused Royal Canadian Air Cadets to learn how to fly a plane, the Star reported. This is following the pathway of notable Canadian Space Agency astronauts such as Jeremy Hansen (who will fly around the moon as part of NASA's Artemis 2 mission next year) and Chris Hadfield, the first Canadian to command the International Space Station.
Siddharth found the asteroids through the International Astronomical Search Collaboration, which uses images from the Hawaiian Pan-STARRS facility and the Arizona-based Catalina Sky Survey for asteroid searches. While Siddharth's two space rocks reside in the main asteroid belt between Mars and Jupiter, the collaboration can also find near-Earth asteroids and trans-Neptunian objects (which orbit the sun beyond Neptune), according to NASA.
The provisional asteroid discoveries aren't Siddharth's only space accolades. His image of Comet C/2023 A3 (Tsuchinshan-ATLAS) alongside the Milky Way received the People's Choice Award in DarkSky International's 2025 Capture the Dark photography contest.
"I love taking photos through my telescopes," Siddharth told the Canadian Broadcasting Corp. "When I go to somewhere dark, or someplace that has lots of stars, it really ignites my sense of wonder. I've learned how mysterious space really is."
The method, developed by researchers at the State University of Campinas in Brazil, uses images of dune surfaces to estimate the force acting on each grain of sand. By combining laboratory experiments, computer simulations and artificial intelligence (AI), the team generated detailed force maps that reveal the physics of dune formation.
Dunes, particularly crescent-shaped "barchan" dunes, form wherever wind or water flows over loose sand — from deserts and seabeds on Earth to the dusty plains of Mars. Scientists can track their movement to infer prevailing winds and environmental conditions, but measuring the forces driving each grain’s motion has, until now, been impossible, according to a statement from the university.
"To measure the force acting on each grain, you'd need to place a tiny accelerometer on each one, which simply doesn't exist," the researchers said in the statement.
To overcome this challenge, the team recreated miniature underwater dunes in a laboratory setting and ran detailed 3D simulations to calculate the exact forces acting on each grain. They then trained a convolutional neural network — a form of AI used for image recognition — to link dune images with corresponding "force maps" from the simulations. Once trained, the AI could infer the distribution of forces directly from visual data. When tested on new images, it accurately predicted the forces at play, even for dune shapes it hadn't seen before.
"Any granular system that can be seen in an image — whether ice, salt or synthetic particles — can be analyzed as long as there’s a simulation capable of accurately reproducing the behavior of the material," Renato Miotto, a postdoctoral researcher and lead author of the study, said in the statement.
The ability to extract such detailed physical information from images alone could have wide-ranging applications. On Earth, it may help engineers better predict coastal erosion, river sediment transport or the behavior of granular materials in industrial systems. This can also be applied to other planets imaged from orbit, like Mars, whose dunes evolve under the same basic physics as those on Earth.
"In the case of Mars, it’s possible to infer, from widely available images, the intensity of winds in the past and the evolution of dunes in the future," Erick Franklin, professor and co-author of the study, said in the statement.
This method therefore offers a new window into studying the Red Planet's atmospheric history and surface evolution. Their findings were published Aug. 1 in the journal Geophysical Research Letters.
]]>The detection of the baby black holes and information about the four parent black holes that forged them came courtesy of ripples in spacetime, or gravitational waves, caused by the violent cosmic events that gave birth to them. Those waves were registered by the LIGO (Laser Interferometer Gravitational-Wave Observatory), Virgo, and KAGRA (Kamioka Gravitational Wave Detector) gravitational wave detectors.
The LIGO-Virgo-KAGRA collaboration detected the first merger, designated GW241011, on Oct. 11, 2024. It was the result of a black hole with around 17 times the mass of the sun crashing into its partner black hole with a mass around seven times that of our star. The event was calculated to have happened around 700 million light-years from Earth. Decoding the resultant gravitational wave signal revealed a couple of things: The masses of the black holes involved as well as the fact that the larger of the pair is one of the most rapidly spinning black holes ever observed.
Less than one month after this groundbreaking detection, on Nov. 11, 2024, the gravitational wave instruments "heard" another newborn black hole screaming after the violent collision of its progenitors. This signal, GW241110, originated from a collision between black holes with 16 and eight times the mass of the sun and occurred about 2.4 billion light-years away. This signal revealed that one of the black holes involved was spinning in the opposite direction of its orbit around the other black hole, the first time such a characteristic has been seen for merging binary black holes.

"Each new detection provides important insights about the universe, reminding us that each observed merger is both an astrophysical discovery but also an invaluable laboratory for probing the fundamental laws of physics," Carl-Johan Haster, an assistant professor of astrophysics at the University of Nevada, Las Vegas (UNLV), said in a statement. "Binaries like these had been predicted given earlier observations, but this is the first direct evidence for their existence."
Both events indicate the existence of so-called second-generation black holes.
"GW241011 and GW241110 are among the most novel events among the several hundred that the LIGO-Virgo-KAGRA network has observed," Stephen Fairhurst, LIGO Collaboration spokesperson and a Cardiff University professor, said in the statement. "With both events having one black hole that is both significantly more massive than the other and rapidly spinning, they provide tantalizing evidence that these black holes were formed from previous black hole mergers."
The idea that the detected black holes are second-generation comes from the difference in size between the larger black holes and their smaller companions in the two mergers. The more diminutive black holes appear to have been almost half the mass of their companions. The orbit-opposing orientation of the larger black hole's spin in the merger that produced the signal GW241110 is also evidence of a prior merger having produced that dominant black hole.
The process of black hole growth by collision after collision is known as "hierarchical merger." This is believed to occur in densely populated regions like star clusters, where black holes are more likely to meet and coalesce over and over again, resulting in subsequently larger black holes.

GW241011 offers scientists the opportunity to probe the limits of Albert Einstein's 1915 theory of gravity, general relativity, from which the concept black holes and gravitational waves both emerged.
For instance, the rapid rotation of the black hole involved in this particular merger deforms the object, and that leaves a unique impression in the gravitational waves it emits. This means that this event can be compared to general relativity and the predictions physicist Roy Kerr made using Einstein's theory concerning rotating black holes. The black holes of GW241011 conformed to Kerr's solution to general relativity, the study team explains, helping verify it as well as Einstein's magnum opus theory itself in extreme circumstances. This includes confirming for the third time within a gravitational wave signal (GW241011) the "hum" of a higher harmonic, akin to the overtones of musical instruments.
The LIGO-Virgo-KAGRA collaboration also thinks these gravitational wave signals could be key to unlocking something predicted but never before seen — something outside the limits of general relativity.
Plus, the two black hole mergers behind these signals have the potential to reveal more about an unrelated scientific field: particle physics.
Scientists can use rapidly rotating black holes to test the hypothesized existence of ultralight bosons, or particles that exist beyond the Standard Model of particle physics. Should they exist, ultralight bosons should draw the rotational energy from spinning black holes. How much energy these particles extract and how much they slow black holes down is dependent on their mass.
The revelation that the progenitor black hole of the merger behind GW241011 is still rotating at a rapid rate after millions (or even billions) of years since the merger that created it seems to rule out a range of ultralight boson masses.

"The detection and inspection of these two events demonstrate how important it is to operate our detectors in synergy and to strive to improve their sensitivities," Francesco Pannarale, co-chair of the Observational Science Division of the LIGO-Virgo-KAGRA Collaborations and professor at Sapienza University of Rome, said. "The LIGO and Virgo instruments taught us yet some more about how black hole binaries can form in our universe, as well as about the fundamental physics that regulates them at the very essence.
"By upgrading our instruments, we will be able to dive deeper into these and other aspects with the increased precision of our measurements."
The team's research was published on Tuesday (Oct. 28) in the Astrophysical Journal Letters.
]]>