Interstellar Comets Become Only the Third Known Visitors Beyond Our Solar System

Astronomers are laying out welcome mats for newly discovered visitors making their way through our solar system.

This particular object is categorized as a comet and marks only the third confirmed interstellar visitor in recorded history to traverse our cosmic neighborhood.

The comet, named 3i/Atlas, poses no threat to Earth, maintaining a distance of about 150 million miles while it accelerates. As reported by NASA.

This interstellar comet was initially discovered on Tuesday by The final alert system for the asteroid’s terrestrial impact (Atlas) located in Rio Hartado, Chile. The research telescope, funded by NASA, is actually two telescopes from Hawaii and one in Chile, in addition to a fourth in South Africa, all dedicated to scanning the sky multiple times nightly for asteroids that could threaten Earth.

Researchers examined archived data from three different Atlas telescopes and Zwick temporary facilities at the Palomar Observatory in California, uncovering observations that would corroborate the findings. Other telescopes worldwide have also joined the initiative, as stated by NASA.

“ESA’s planetary defenders are currently monitoring an object provisionally known as #A11PL3Z, utilizing telescopes from around the globe,” the European Space Agency announced in a post on X this Wednesday.

Interstellar Comet 3i/Atlas.
David Rankin/Saguaro Observatory

The comet is located around 420 million miles away and is rapidly traveling from the direction of the constellation Sagittarius. NASA commented in a blog post regarding the findings. Sagittarius is a prominent constellation in the Southern Hemisphere and indicates the center of the Milky Way galaxy.

The agency noted that 3i/Atlas will make its closest approach to the sun around October 30th, passing roughly 130 million miles away, close to Mars’ orbit.

NASA indicated that the comet will remain observable from ground-based observatories until September, providing scientists with the opportunity to gather additional details about these cosmic visitors, including their size. After September, 3i/Atlas will be too close to the sun for telescopes to observe, but it is expected to become visible again in early December, as it reemerges on the far side of the sun.

The upcoming months will present a rare chance to study these celestial tourists traveling through the solar system. The first confirmed interstellar object, observed in 2017 by the University of Hawaii’s Pan-Starrs1 telescope, was the rocky body named “Oumuamua” (Hawaiian for first visitor), notable for its reddish hue and elongated cigar-like shape. As noted by NASA.

The only other known interstellar visitor is 2i/Borisov, a comet discovered in 2019 by amateur astronomer Gennady Borisov.

Source: www.nbcnews.com

A11PL3Z: The Interstellar Comet 3i/Atlas Traversing Our Solar System

Comet 3i/Atlas is the third interstellar object detected in the solar system

E. Guido, M. Rocchetto, J. Ferguson

Interstellar objects have been observed speeding through the solar system, prompting both amateur and professional astronomers globally to direct their telescopes toward them, refining their orbital models to confirm their status as visitors from other stars.

The comet was initially designated A11PL3Z and marks the third documented interstellar object. The first, ‘Oumuamua, was identified in October 2017, shortly after its closest approach to Earth. Its bizarre acceleration sparked numerous theories, including the possibility that it might be an alien spacecraft. The second interstellar object, Comet Borisov, was discovered in 2019, allowing for more extensive observations early in its journey through the solar system.

The A11PL3Z was first detected by NASA’s Asteroid Terrestrial Impact Last Alert System (ATLAS). Earlier images of the object, once overlooked, were identified in data collected on June 14. New observations are underway in Chile and beyond through the Deep Random Survey. The Minor Planet Center—charged with the observation and reporting of such entities—has now officially named it 3I/ATLAS, acknowledging both its classification as the third interstellar object and the discoverers.

The object measures approximately 20 km wide and is estimated to move at around 60 km per second, gradually accelerating due to the sun’s gravitational pull. By October, it will reach its closest point to the Sun, passing within two astronomical units (twice the distance from Earth to the Sun) before swinging away and exiting our solar system.

The anticipated trajectory of 3i/Atlas marks its position as only the third interstellar object to be recorded in the solar system

CSS, D. Rankin

This creates a limited window for studying 3i/Atlas, although its visibility offers more time for observation compared to other interstellar entities. “They move through the solar system at astonishing speeds,” states Mark Norris from the University of Central Lancashire, UK. “It’s a race against time to learn as much as we can about them.”

Unfortunately, the technology needed to launch missions to intercept and investigate these celestial visitors remains out of reach, according to Norris. “Even if we started today, it would be too late,” he concludes. However, this may evolve soon, as the European Space Agency (ESA) aims to deploy a comet interceptor mission into space in 2029, where it will await encounters with newly discovered comets and interstellar bodies.

For now, astronomers must depend on existing telescopes to observe 3i/Atlas from a distance. “As we can track it until the end of the year, we have sufficient time to refine its trajectory, and there’s still time to focus the spectrometer on it,” mentions Richard Moisle. Our team is already eager to pinpoint the earliest possible observations. Everyone is highly enthusiastic and ready for what’s ahead.”

World Capital of Astronomy: Chile

Explore the breathtaking astronomical sites in Chile. Visit advanced observatories and marvel at the breathtaking clear night skies.

Topic:

Source: www.newscientist.com

A11PL3Z: Interstellar Travelers Discovered Racing Through the Solar System

SEI 257609617

The predicted trajectory of A11PL3Z marks it as the third interstellar object observed in the solar system

CSS, D. Rankin

Potential interstellar bodies are now observed zipping through our solar system, and both amateur and professional astronomers globally are racing to direct telescopes towards these phenomena, refine their trajectory models, and ultimately validate their status as visitors from another star.

The object provisionally named A11PL3Z represents the third interstellar entity detected to date. The asteroid ‘Oumuamua was first seen in October 2017, just three days after it passed closest to Earth, and its unusual acceleration sparked a variety of hypotheses, including the possibility of it being an alien spacecraft. The second identified object, Comet Borisov, was observed in 2019, allowing for closer examination given its early passage through the solar system.

A11PL3Z was first identified by the Deep Random Survey in Chile, a group of amateur astronomers. However, a review of earlier observations by other teams revealed that it was initially spotted on June 14 by NASA’s Asteroid Terrestrial-impact Last Alert System (ATLAS). It is estimated to measure approximately 20 km in width and is currently traveling at around 66 km/s, accelerating as it gets pulled in by solar gravity. In October, it will reach its closest point to the Sun, passing within two astronomical units (the Earth is twice the distance from the Sun) before swinging away and exiting the solar system.

This provides a limited window for studying A11PL3Z, though it’s more than that available for previous interstellar objects, which were seen hurtling towards the solar system. “These objects move through the solar system at incredible speeds,” remarks Mark Norris from the University of Central Lancashire. “They are quite transient, which restricts our ability to learn about them.”

Sadly, the prospect of sending missions to intercept and study A11PL3Z is beyond the reach of current technology, notes Norris. “If we were to launch a mission today, it would be too late,” he states. However, the European Space Agency (ESA) is planning a comet interceptor mission set for launch in 2029, which would remain in space to await the arrival of newly discovered comets and possibly interstellar objects.

For the time being, astronomers are relying on existing telescopes to observe A11PL3Z from a distance. “We anticipate we will be observing it by the end of the year, giving us ample time to prepare our spectrometers once we finalize the trajectory,” shares Richard Moisle. When will our observers discern its visibility? There’s a palpable excitement as everyone is prepared and looking forward to this opportunity.

At the time of this writing, over 100 observations of A11PL3Z have already been logged, and the Minor Planet Center—the official body responsible for monitoring and reporting such celestial entities—is expected to confirm its interstellar classification later today.

Topics:

Source: www.newscientist.com

The Great Multivitamin Myth: How Pills Can Harm Your Immune System

The immune system is intricate, consisting of a vast network of cells, proteins, and organs that serve as the body’s primary defense against infections. Given its vital role, it’s essential to maintain its health.

So, how can you achieve that? Similar to other crucial bodily functions, numerous supplements and products claim to enhance your immune system’s performance. However, the reality is that your body may not require these so-called enhancements. In fact, it often functions best when left to its natural processes.

Misconceptions About Immune Boosting

The idea of vitamins that “boost” immunity can be quite misleading. In theory, the immune system is self-sufficient and operates optimally if you maintain a healthy lifestyle.

Moreover, “boosting” the immune system is a somewhat ambiguous notion. Simply increasing the quantity of immune cells or similar components in your body may not be beneficial and could potentially be harmful.

Consider your immune system as a finely tuned machine, operating at peak efficiency as long as it receives proper maintenance. Attempts to push this machine into overdrive may lead to overheating or malfunction.

The same principle applies to the immune system; an overstimulated immune response can inadvertently attack healthy cells, resulting in autoimmune disorders.

“The immune system can typically maintain its own balance. As long as you adhere to a relatively healthy lifestyle, no additional enhancement is necessary,” stated Dr. Bobby Cherayil, author of The Logic of Immunity, in an episode of BBC Science Focus.

“This includes a nutritious diet, sufficient sleep, regular physical activity, and avoiding harmful practices such as smoking or excessive alcohol consumption.”

Though a decline in lifestyle can affect our immune system, this deterioration is gradual, often requiring severe circumstances for visible infection to occur.

“A diet lacking essential nutrients or severe vitamin deficiencies can negatively impact your immune system, but such deficiencies are generally quite extreme.”

Risks Associated with Vitamin Supplements

If you maintain a healthy lifestyle—eating well, sleeping adequately, and exercising regularly—what risk is there in taking supplements aimed at enhancing your immune system?

Often, the risks are minimal, with the primary concern being the lack of effectiveness. The body can only absorb a certain amount of vitamins, and excess amounts typically pass through the body and are expelled in urine.

This applies mainly to water-soluble vitamins; however, vitamins A, D, E, and K do not leave the system so easily, and an excess can lead to toxicity. For instance, too much vitamin D can cause nausea, weakness, and may ultimately lead to bone and kidney pain if left untreated.

Many immune-boosting supplements are categorized as “multivitamins,” which encompass various vitamins and minerals in a single tablet or capsule.

A significant study associated multivitamins with a high rate of placebo effects. Research indicates no significant health statistics difference from a control group.

Clinical trials revealed no notable variation in mental or physical health outcomes between those taking multivitamins and those who were not. However, individuals consuming multivitamins often believe these products contribute positively to their health.

The danger is that individuals might assume multivitamins can substitute for other health-boosting practices, leading to neglect in other health areas such as maintaining a balanced diet.

Long-term effects of excessive vitamin intake remain less understood, with some studies suggesting a connection between multivitamin use and increased risk of cancer, heart failure, or cardiovascular issues.

Research indicates risk may increase with age. A study from the University of Minnesota found that among over 38,000 women aged 62 and older, those taking supplements had a 2.4% higher mortality risk.

This area of research continues to evolve, and not all studies reach such dire conclusions. For instance, another study found no significant correlation between multivitamin use and overall mortality rates.

Vitamins Have Their Place…for Some

For many, a healthy lifestyle is all that’s needed to keep the immune system in optimal condition. However, there are individuals with significant vitamin deficiencies that require attention.

Globally, over 2 billion people lack essential vitamins, and certain demographic groups may require additional support.

Vitamin supplements can be beneficial, particularly for older adults who struggle with chewing or swallowing. This is also true for pregnant individuals or those with digestive issues (always consult a healthcare professional).

Ultimately, the immune system remains a highly advanced, self-regulating entity. For the average person, it functions effectively on its own. Immune-boosting supplements may not pose significant risks, but they often result in “expensive urine.”


About Our Expert, Bobby Cherayil

Cherayil is an associate professor of Pediatrics at Harvard University and author of The Logic of Immunity. His research focuses on the immune system and its response to infection and inflammation.

Read More:

Source: www.sciencefocus.com

Webb Discovers Two Young Exoplanets in the YSES-1 System

Astronomers utilizing the NASA/ESA/CSA James Webb Space Telescope have discovered a silicate cloud in the atmosphere of the exoplanet YSES-1C and a disk in the evasion facility surrounding the planet YSES-1B.

Artist rendering of the YSES-1 system, featuring a central sun-like star, YSES-1B with its dusty evasive disc (right), and YSES-1C’s atmospheric silicate clouds. Image credit: Ellis Bogut.

YSES-1 is a solar-type star located approximately 309 light-years away in the constellation of Masca.

Also referred to as TYC 8998-760-1 or 2mass J13251211-6456207, this star is roughly equivalent in mass to our Sun but is only 16.7 million years old.

The system comprises two planets, YSES-1B and YSES-1C.

These planets orbit their parent star at distances of 160 and 320 AU, making them more distant from their star than Jupiter and Saturn are from the Sun.

YSES-1B and C could exhibit redder hues compared to other exoplanets (or brown dwarfs), indicating distinct atmospheric properties.

While the system has been observed with various telescopes before the Webb, comprehensive observations were not achievable prior to the Webb program.

“Directly imaged exoplanets are the only types we can truly photograph,” stated Dr. Ebert Nazkin, a postdoctoral researcher at Trinity College Dublin.

“Typically, these exoplanets are younger, hotter from their formative layers, and astronomers observe this heat in the thermal infrared spectrum.”

Utilizing Webb’s spectroscopic capabilities, Dr. Nasedkin and his team obtained detailed spectra of the planets YSES-1B and YSES-1C.

These observations include the first direct detection of atmospheric silicate clouds on YSES-1C, validating prior hypotheses regarding its atmospheric structure.

These silicate clouds likely contain iron, which might contribute to rainfall on the planet.

Astronomers estimate that the cloud particles are less than 0.1 μm in size.

“Upon observing a smaller, more distant companion identified as YSES-1C, I detected a silicate cloud signature in the mid-infrared,” Dr. Nasedkin remarked.

“Composed primarily of sand-like particles, this represents the strongest silicate absorption feature documented in an exoplanet.”

“We believe this is connected to the planet’s youth. Younger planets tend to have slightly larger radii, and this expanded atmosphere enables clouds to absorb more light emitted by the planet.”

“We were able to employ detailed modeling to uncover the chemical makeup of these clouds as well as the size and shape of the cloud particles.”

The team also identified silicate disks surrounding YSES-1B, marking a rare observation of a substellar companion exoplanet.

This finding suggests that YSES-1B may be a relatively recently formed planet.

The discoveries enhance our understanding of the early stages of planetary formation and atmospheric development.

“The planets within the YSES-1 system are so widely separated that current formation theories cannot explain them. The discovery of distinct silicate clouds around YSES-1C and additional findings of small, hot, dusty materials around YSES-1B introduces further mystery and complexity regarding how planets form and evolve.”

The team’s results will be featured in the journal Nature this week.

____

kkw hoch et al. Silicate cloud and evasive agent disks in the YSES-1 exoplanet system. Nature Published online on June 10th, 2025. doi:10.1038/s41586-025-09174-w

Source: www.sci.news

Discovery of a Compact Binary System: A Neutron Star Orbiting Within Another Star

This binary system comprises a PSR J1928+1815 along with a rapidly spinning millisecond pulsar known as the Helium Star Companion.



The AI impression of the compact binary system. Image credit: Gemini AI.

The millisecond pulsar consists of rapidly rotating neutron stars that emit radio waves.

These stars attain remarkable rotational velocities by harvesting material from surrounding stellar groups.

The development of such exotic binary systems remains partially understood, as it encompasses a range of complex processes.

The theory suggests that binary systems may undergo a common envelope phase, where a star orbits within the outer layer of its companion.

If the companion in this evolutionary phase is a neutron star, the theory indicates that the outer layer will be swiftly ejected, resulting in a binary system of recycled pulsars and stripped helium stars.

In the recent study, Dr. Zonglin Yang, a national astronomer at the Chinese Academy of Sciences, along with colleagues, examined the millisecond pulsar PSR J1928+1815.

Utilizing data from a high-speed 500-meter aperture spherical radio telescope, they discovered that the pulsar has a spin period of 10.55 ms and resides in a close binary system with companion helium stars, completing an orbit every 3.6 hours.

They employed a stellar model to demonstrate that this system originated following an unstable mass transfer from companion stars to neutron stars, leading to the formation of a common envelope around both stellar objects.

The neutron star approached the core of the other star, ejected the outer envelope, and released energy, resulting in a tightly bound binary system.

“The companion star has a mass between 1.0 and 1.6 solar masses, obscuring the pulsar approximately 17% of its orbit and is undetectable at other wavelengths, suggesting it is likely a stripped helium star,” the authors noted.

“We interpret this system as having recently undergone a common envelope phase to create compact binaries.”

“Such systems are thought to be rare, yet we anticipate the existence of others,” they added.

“We estimate that there could be between 16 and 84 undiscovered examples within the Milky Way.”

The findings are documented in a paper published in the journal Science.

____

Zl Yang et al. 2025. A pulsar helium star compact binary system formed by common envelope evolution. Science 388 (6749): 859-863; doi: 10.1126/science.ado0769

Source: www.sci.news

Tianwen-2: China’s Upcoming Missions to Two Rocky Bodies in the Solar System

Artist impressions of Earth’s semi-satellite Kamo`oalewa, designated as the initial target for the Tianwen-2 mission

Addy Graham/University of Arizona

China is making final preparations to launch a spacecraft aimed at exploring asteroids and comets, seeking to gain insights into these celestial bodies in our solar system.

The Tianwen-2 mission, orchestrated by the China National Space Agency (CNSA), plans to collect 100 grams of samples from the asteroid Chuan West and return them to Earth. Following the sample retrieval, the probe will utilize Earth’s gravity to propel itself towards the comet 311P/Panstarrs, which will be observed remotely.

The mission is set for launch from the Xichang Satellite Launch Center in Sichuan Province on May 29th. While NASA’s Osiris-Rex and JAXA’s Hayabusa missions have previously returned asteroid samples, this marks China’s inaugural asteroid mission, including the return of rock samples, and potentially the first mission aimed at a unique type of celestial body known as quasi-satellites.

Quasi-satellites, like Kamo`oalewa, do not orbit the Earth in a traditional manner; instead, they follow orbits around the Sun that are similar to Earth’s, creating an oval path relative to our planet. This intriguing scenario has led scientists to theorize that this may be a remnant lunar mass ejected by an asteroid impact millions of years ago.

In contrast, 311P/Panstarrs has an asteroid-like orbit, encircling the Sun within the asteroid belt between Mars and Jupiter, yet possesses a tail that gives it a comet-like appearance. This is believed to be composed of dust and debris shed from its nucleus.

The CNSA has previously indicated that 311P/Panstarrs is a “living fossil,” crucial for studying the early material composition, formation processes, and evolutionary history of the solar system. Tianwen-2 aims to enhance our understanding of both Kamo`oalewa and 311P/Panstarrs. However, the findings will not be available immediately, as the spacecraft is expected to reach 311P/Panstarrs by 2034, and the Kamo`oalewa samples are anticipated to return to Earth in the latter half of 2027.

It remains uncertain what extent the CNSA will share these findings. Leah-Nani Alconcel from the University of Birmingham, UK, mentions that the mission outline is known but lacks detailed information. One of the objectives may involve examining the differences between asteroids and comets to gain better insights into the diverse bodies of our solar system; however, specific details remain elusive.

In her previous experience with CNSA’s Double Star Satellite, Alconcel expressed concerns about the institution’s ability to provide substantial scientific data. She states, “It was incredibly challenging to negotiate with [the CNSA]. There is no public repository for this data.”

She describes the mission as ambitious, noting that Kamo`oalewa is in a rotating behavior. Navigation algorithms may require powerful computing resources to process images and sensor data sent back to Earth for calculations. “If we always opt for favorable and stable objects, we won’t gain much knowledge,” she warns. “There are numerous potential challenges ahead.”

The CNSA has not responded to requests for comment from New Scientist.

Topics:

Source: www.newscientist.com

Astronomers Discover Massive Molecular Hydrogen Clouds Close to the Solar System

Recently identified by astronomers, this newly discovered molecular cloud is one of the largest structures in the sky and is among the closest to the Sun and Earth ever detected.

The EOS Cloud is situated at the boundary of your local bubble—a region populated by large gases within the solar system. Image credits: Thomas Müller, HDA & MPIA/Thavisha Dharmawardena, NYU.

Molecular clouds consist of gas and dust, primarily composed of hydrogen, the most prevalent molecule in the universe and essential for the formation of all known stars and planets.

Additionally, these structures harbor other molecules, including carbon monoxide.

Traditional detection methods for molecular clouds often involve wireless and infrared observations, which readily capture the chemical signatures of carbon monoxide.

However, Blakely Burkhart, an astrophysicist from Rutgers University in New Brunswick, and his team took a different approach.

“This is the first molecular cloud discovered by directly seeking out the distant ultraviolet radiation of molecular hydrogen,” Dr. Burkhart stated.

“Our data revealed glowing hydrogen molecules detected through fluorescence in distant ultraviolet light. This cloud truly shines in the dark.”

The new molecular cloud, named EOS, was located approximately 300 light-years from Earth and can be viewed here.

It resides at the periphery of a local bubble, a region filled with gases surrounding the solar system.

Astronomers estimate that these crescent clouds are immense, spanning about 40 months across the sky and having a mass approximately 3,400 times that of the Sun.

They are projected to dissipate within 6 million years.

According to the research team, the EOS cloud poses no threat to Earth or the solar system.

Its proximity offers a unique opportunity to explore the properties of structures within the interstellar medium.

The interstellar medium, composed of gas and dust, fills the space between stars in the galaxy and is a key source for new star formation.

“When you look through a telescope, you observe the solar system in its formative phase, but the exact process remains unclear,” Dr. Burkhart explained.

“The discovery of EOS is thrilling because it allows us to directly measure how molecular clouds form and dissolve, as well as how galaxies transform interstellar gas and dust into stars and planets.”

The EOS Cloud was identified using data from the FIMS-Spear Far-ultraviolet spectrograph aboard the Korean satellite STSAT-1.

“Utilizing distant UV fluorescence technology could redefine our understanding of the interstellar medium, uncover hidden clouds across the galaxy, and even push our exploration further back to the very edge of the universe’s inception.”

The findings are reported in a study published today in the journal Nature Astronomy.

____

B. Burke Hart et al. Dark molecular clouds near local bubbles revealed via H2 fluorescence. Nature Astronomy. Published online on April 28, 2025. doi:10.1038/s41550-025-02541-7

Source: www.sci.news

Twin stars could be brought into orbit by planets similar to tattoos beyond our solar system

new Like a tattoo Planets outside the solar system may orbit two The failed starScientists reported Wednesday.

Around 120 light years away, the exoplanet appears to be walking an unusual path around two brown d stars, whipping at the right angle. Brown dwarfs are sometimes called failed stars because they are lighter than stars but heavier than giant gas planets. The light year is nearly 6 trillion miles.

The brown dwarf pair was first discovered a few years ago. Scientists have noticed that twins celebrate each other, so they are always partially blocked when viewed from Earth.

In a new analysis, researchers found that brown dwarves were changing their movements. This is a habit that is more likely to occur when you go around each other on your own. This study was published in the journal Science Advances.

Scientists know more than 12 planets orbiting two stars, like the desert planets that burn the fictional “Star Wars” engulfed by the double sunsets that Luke Skywalker calls home.

Possible trajectories of exoplanet around two brown dwarfs.
L.calçada / eso via ap

The strange orbit of the new planet makes it stand out. But it’s not spy directly. Scientists say more research is needed to make sure it’s there and figure out its mass and trajectory.

“I still didn’t bet on my life that there was a planet,” said Simon Albrecht, an astrophysicist at Alfs University, who hadn’t played a role in the new research.

Investigating these eccentric bodies will help us understand how states beyond our solar system produce planets that are very different from our own, says Thomas Beycroft, a research author at the University of Birmingham.

The twin-star circling planet “has been in sci-fi for decades before we know that it can even exist in real life,” he said.

Source: www.nbcnews.com

Strange vertical orbits of an exoplanet observed around a binary brown dwarf system

Impression of the artist in the unusual orbit around the brown dwarf of ExoPlanet 2M1510 (AB)B

ESO/L. Calsada

It was first revealed that a pair of rare stars have equally rare companions, exoplanets that rush into orbit vertically.

Astronomers may think they know what the normal thing is about stars and planets, but they say, “But the universe is very diverse.” Amaury Triaud At the University of Birmingham, UK. He and his colleagues unexpectedly discovered evidence of rare constructs while analyzing data collected by a very large Chilean telescope.

The two stars are brown d stars. This means that they are small and very dim because they cannot maintain fusion and are often referred to as failed stars or subseber ral objects. They follow orbit and continue to cover each other when viewed from Earth. Researchers have previously observed only one brown d-star binary.

Triaud and his colleagues carefully analyzed the new binary system to determine the mass of the stars and their movements, and unexpectedly strange signals were found in the data. Ultimately, the only physical scenario that can explain it is that of a planet-sized object orbiting two stars, following an ellipse perpendicular to the star’s orbit.

Triaud says that vertical orbit is not entirely unheard of, but he and his colleagues never expected to see it in this context. “Brown dwarfs are rare. Brown dwarf pairs are rare. Covering a pair of brown dwarfs is even more unusual and faint, making it difficult to measure,” he says. “That was a surprise. In a system that is ideal and not rare in itself, there is this configuration.”

Twenty years ago, such a structure was considered science fiction, but now it has become a scientific fact. Katherine Brandel At Oxford University. “This is a truly beautiful outcome,” she says. Details of the impending orbit of the two stars make a strong claim that this “harmonograph of the sky” is authentic. By studying how they eat each other, we can identify more details about this unique trio’s moves going forward, Blundell says.

Researchers would like to learn more about the exoplanet named 2M1510(AB)B, but can be compared to a fictional tattoo. Star Warsa desert world orbiting two suns. However, the two suns on the 2M1510(AB)B dimming and get exposed to the surface with something similar to the double dose of moonlight.

topic:

Source: www.newscientist.com

BYD, a Chinese EV manufacturer, claims their new rapid charging system could rival the speed of filling up a gas tank

BYD, a Chinese electric vehicle (EV) maker, has announced plans to construct a charging network across China. This network aims to enable EVs to charge as quickly as refilling with gasoline.

Founder Wang Chuanfu revealed the “supere platform” at a home event in Shenzhen on Monday. This platform will support a peak charging speed of 1,000 kW, allowing cars to travel 400 km on a five-minute charge.

BYD’s 1,000 kW charging speed is double that of Tesla superchargers, offering faster charging speeds than before in the industry. Fast charging technology is crucial for increasing EV adoption.

Tesla, already struggling, saw its shares drop 15% on March 10, prompting concerns for owner Elon Musk. The company faces challenges in meeting sales targets and producing self-driving cars, with increasing competition from more affordable EV models from Chinese companies like BYD.

Tesla stocks dropped 4.8% on Wall Street, marking an eighth consecutive weekly decline. Baron.

Wang emphasized the goal of reducing EV charging times to match gasoline vehicle refueling times. The new charging architecture will debut with the Han L Sedan and Tang L SUV, priced from 270,000 yuan ($37,330).

BYD plans to build over 4,000 ultra-fast charging stations to support the new platform, but no specific timeline for construction was provided. Previously, BYD owners relied on public charging poles from other manufacturers or third-party operators.

While Tesla has been offering superchargers in China since 2014, other Chinese EV companies like NIO, Li Auto, Xpeng, and Zeekr have also established charging facilities.

BYD’s sales primarily come from plug-in hybrids, with aims to sell 5-6 million units this year.

Reuters and

Source: www.theguardian.com

White dwarf binary system linked to irregular radio signals

Astrophysicists have discovered ILT J110160.52+552119.62, a recently discovered temporary radio source, and that the arrival of that approximately one minute pulse with a periodicity of 125.5 minutes is a red-white, white-white dwarf binary system with orbital periods that match the orbital period observed when two stars are observed when they are engaging.

Artistic illustration showing radioactive pulses emitted by the binary star system: white d star orbit around a red d star. Image credits: Daniëlle Futselaar/Artsource.nl.

In recent years, astronomers have detected radio pulses from sources in the Milky Way that last from seconds to minutes.

These pulses differ from what you would expect from known pulsars that produce pulses on the order of milliseconds.

Furthermore, unlike radiopulsars, these so-called long-term transients (LPTs) are periodic on timescales ranging from minutes to hours.

There have been some hypotheses regarding the origin of these novel pulses, but evidence is scarce.

“There are several highly magnetized neutron stars or magnetores known to exhibit radio pulses in periods of a few seconds,” said Charles Kilpatrick, a northwestern astrophysicist.

“Some astrophysicists also claim that the source is spinning and can emit pulses at regular time intervals, so radio emissions are only shown when the source rotates towards us.”

“I know now that at least some long-term radio transients come from binary.”

“We hope this motivates radio astronomers to localize new classes of sources that could arise from neutron stars or magnetoresistance binaries.”

In their study, Dr. Kilpatrick and colleagues focused on periodic radio signals from transient radio sources designated as ILT J110160.52+552119.62 (ILT J1101+5521);

New imaging techniques were used to detect some of these radio pulses in data collected by low frequency arrays (LOFAR).

Behaving like a large radio camera, the telescope can pinpoint the exact location of the radio source in the sky.

According to the team, the Object is about 1,600 light years away in the Ursa major's constellation.

Follow-up observations with multiple mirror telescopes of 6.5 m diameter in Arizona and the Texas Hobby and Everly telescope showed that the ILT J1101+5521 is not a single flashing star, but two stars that cause pulses together.

A white dwarf in orbit around the two stars, the red war star, brings a common center of gravity into orbit every 125.5 minutes.

Researchers say there are two possibilities for the way stars produce unusually long radio pulses.

Potentially, radio bursts can be emitted from the strong magnetic field of a white dwarf or generated by the interaction of a white dwarf and its stellar companion magnetic field.

However, further observation is required to make this clear.

“Thanks to this discovery, we know that compact objects other than neutron stars can produce bright radio emissions,” says Dr. Kaustub Rajwade, an astronomer at Oxford University.

Discoveries are reported in a paper It's published in the journal today Natural Astronomy.

____

I. de Ruiter et al. Sporadicated radio pulses from white dwarf binaries during orbit. Nut AthlonPublished online on March 12, 2025. doi:10.1038/s41550-025-02491-0

Source: www.sci.news

First Operating System for Quantum Networks Successfully Created

Qnodeos is an operating system that allows you to connect different types of quantum computers.

Studio Oostrum/Blijft Eigendom Van Fotograaf

Researchers created the first operating system for quantum networks, making it easier to link quantum computers to each other.

“By building only hardware, we make quantum networks useless.” Stephanie Wenner At Delft University of Technology in the Netherlands. She has been working on connecting quantum computers to a network for a long time. This allows for the exchange of information very safely and perform calculations in new ways, but this requires understanding of the technical nity-gritty of each device involved. Together with her colleagues, Wehner has now developed a way to run quantum networks more universally.

The operating systems the team has built are software that allows you to control devices within a quantum network regardless of the type of qubit or qubit that make them. Such control devices become more difficult due to the fact that networked quantum computers receive both quantum information from other quantum computers and traditional signals from classical computers that serve the interface.

To demonstrate that an operating system called Qnodeos can handle both, researchers tested it on two types of quantum computers and several different tasks. They used two quantum computers made from specially processed diamonds and another quantum computer made from electric charged atoms. Using these two types of quantum hardware, researchers ran a delegated quantum computing test program, similar to using laptops to perform calculations in the cloud. We also tested the ability of Qnodeos to handle multitasking by running two programs at once.

Joe Fitzsimmons At the Quantum Computing Startup Horizon Quantum, based in Singapore and Ireland, it states that this is a major advance in laying the foundations of the quantum internet. He says, “If you start to take the idea of ​​seriously building a general-purpose quantum network, there's a lot to do,” and the new operating system will lead to a long list of things to develop next, such as routing protocols.

Wehner says that Qnodeos development is like creating coloring pages. They outline all the shapes and struggle to color them all. For example, the work raised the question of how to write a scheduling program for quantum networks. “This wasn't even on my radar before, but now I'm very excited,” she says.

topic:

Source: www.newscientist.com

Potential long-term consequences of measles: immune system memory loss and encephalitis

Measles is not just a rash and fever.

The outbreak of the disease in West Texas has sent 29 people, most of them, to hospitals, as they continue to grow. Two people have died, including a six-year-old child.

It remains to be seen how many people have become ill in the outbreak. There have been at least 223 confirmed cases, but experts believe hundreds more people may have been infected since late January. As public health officials try to slow the spread of the highly contagious virus, some experts are worried about long-term complications.

Measles is different from other childhood viruses that come and go. In severe cases, it can cause pneumonia. According to the Centers for Disease Control and Prevention, approximately one in 1,000 patients develop encephalitis or encephalitis or encephalitis, with one or two deaths in 1,000 people.

This virus can wipe out the immune system, a complication known as “immune amnesia.”

When you get sick with a virus or bacteria, the immune system has the ability to form memories that can quickly recognize and respond to pathogens if they are encountered again.

Measles targets cells in the body, such as plasma cells and memory cells, and contains their immunological memory, and destroys some of them in the process.

“No one can escape this,” said Dr. Michael Mina, a vaccine expert and a former professor of epidemiology at the Harvard Chan School of Public Health.

In a 2019 survey, Mina and his team discovered that measles infections can be wrecked from anywhere 11% to 73% of human antibody stockpiledepends on how serious the infection is. This means that if people had 100 antibodies to Chicken Pox before they developed measles, they would be left at just 50 after measles infection, potentially catching them and getting sick.

Iwasakimon, professor of immunology at Yale University School of Medicine, said: You forget who the enemy is. ”

Virtually everyone who contracts measles weakens the immune system, but some are hit harder than others.

“There's no world where you get measles and it won't destroy some [immunity]He said. “The problem is that it will destroy enough to have clinical impact.”

In a previous study in 2015, Mina presumed that the virus was a virus before vaccination, when measles was common It may be related to half of childhood deaths due to infectionmainly from other diseases such as pneumonia, sepsis, diarrheal diseases, meningitis.

Researchers found that after measles infection, the immune system was suppressed almost immediately and remained intact for two to three years.

“Immune amnesia begins as soon as the virus replicates in them [memory] Cells,” Mina said.

The best protection against serious complications is the measles vaccine. Two doses of the vaccine are 97% effective in preventing infection.

What is “immune amnesia”?

Our bodies are constantly exposed to a variety of bacteria and viruses in our environment. Over time, our immune system learns to remember a particular intruder and can take action immediately if we find something that doesn't belong to our body.

“Children are in contact with all sorts of microorganisms, and most of those encounters have not led to illness,” said Dr. Adam Ratner, pediatrician and director of the Department of Pediatric Infectious Diseases at NYU Langone Health. “Children often recover and have memories, so if they see the same strain of the virus that causes diarrhea, they will be the second disease they are exposed to.”

With immune amnesia, he said that if people are exposed to strains of the same virus again, their bodies will act as if it was the first time they had it and they don&#39t have that robust protection.

This means that the measles virus can destroy the immunity that people have accumulated over time, such as pneumonia, colds, flu, bacteria, and more that can cause other pathogens.

Mina elicited a comparison with HIV, saying that the level of immunosuppression in severe measles infection can be compared to HIV that has not been treated for years. However, he warned that HIV affects various parts of the immune system, and that people&#39s immune systems can ultimately recover from measles.

How does measles destroy the immune system?

Highly contagious viruses can destroy long-lived plasma cells that are present in the bone marrow and are essential to the immune system. Cells are like factories that expel antibodies to protect us from intruders entering our bodies.

“It&#39s almost like bombing a sacred city,” Mina said.

Measles also targets cells in our body, called memory cells. This is a cell that remembers what intruders look like, allowing the immune system to quickly identify and fight them in the future.

When you breathe a virus, it is enveloped in cells called macrophages. Macrophages function as “trojan horses” to collect viruses in lymph nodes, Iwasaki said.

Once there, the virus can bind and destroy these memory cells, wiping away some of our built-in immunity in the process.

“one time [memory cells] As it is excluded, we basically no longer have any memory of those specific pathogens, so we are more susceptible to most infectious diseases that are unrelated to measles,” Iwasaki said.

Will the immune system recover?

The way your body begins to regain immune memory after being surrounded by measles is to be exposed to other viruses and bacteria, get sick again, and boost your immune system.

Such immunity can be relearned, but University of Pennsylvania immunologist John Welley says that while such immunity can be relearned, he is particularly susceptible to other infectious diseases.

“As every parent of a daycare child knows, if you&#39’re building a lot of immunity at the time, you’re suffering through it,” Welley said.

Mina relearned our immunity and compared it to why babies seem to get sick frequently.

“The illness a baby gets is not because the baby is more vulnerable, because they don&#39t have the same immunological memory set yet,” he said. “They have to spend several years accumulating it through exposure, which is kind of what people experience after measles.”

How Measles Causes Brain Inflammation

What&#39s even more frightening is an untreated measles complication called subacute sclerosing pan encephalitis (SSPE), a brain disease that can occur for more than a decade, which is fatal after someone recovers from an infection.

For poorly understood reasons, the measles virus can cause persistent infections and lead to brain damage, leading to cognitive decline, coma, and death.

Researchers believe that SSPE was once considered rare, but is more common than realization. a Review of measles cases in California From 1998 to 2015, SSPE cases were found to occur at a higher rate than expected among children who were not vaccinated.

Dr. Bessie Gibberge, a pediatric infectious disease expert at Northwest Medicine, said the disease is progressive and symptoms occur at normal stages.

“It can start with just a change in personality and a change in behavior,” she said. In children, it can be as subtle as worse performance in school.

The disease then progresses and can eventually lead to seizures and abnormal movements, Siebarghese said. Finally, parts of the brain that regulate vital signs such as breathing, heart rate, and blood pressure can be damaged and can lead to death.

There is no cure for this disease and is almost always fatal. Patients usually survive 1-3 years after diagnosis. In the US, there are usually four to five cases each year, which can be underestimated, says Ratner of Nyu Langone Health.

“It’s probably more common than we think because it’s not always diagnosed,” he said. “But as these outbreaks become more common, I think we will clearly see more cases of SSPE.”

Source: www.nbcnews.com

Possible Hierarchical Triple System in Kuiper Belt Object Altjira

Altozillaalso known as the 2001 UQ18, is located outside the solar system, 6 billion km (3.7 billion miles), or 44 times the distance between the Earth and the Sun.



This artist’s concept illustrates one of the possible scenarios for Kuiper Belt’s Altjira system. Image credits: NASA/ESA/Joseph Olmsted, Stsci.

“The Hubble images show two Kuiper Belt Objects (KBOs) about 7,600 km (4,700 miles) apart,” says Meianelsen, an astronomer at Brigham Young University and a colleague.

“However, Altjira’s repeated observations of the unique cooperative movement show that the inner object is indeed two bodies very close to each other.

“In small, far-flung objects, we need to discover that the separation between the two inner members of the system is part of the pixels of Hubble’s camera, using non-imaging methods.”

Astronomers gathered data from the Hubble and WM Keck Observatory for 17 years of observation baselines and looked at the trajectory of objects outside the Altjira system.

“Over time, the direction of the trajectory of the outer object changes, indicating that the inner object is either very elongated or in fact one of two separate objects,” says Dr. Dalin Lagoziczin of Brigham Young University.

“The triple system was perfect when putting Hubble data into different modeling scenarios,” Nelsen added.

“Other possibilities are that the inner object is a contact binary, so close that two separate bodies touch each other, or in fact, oddly flat as pancakes.”

Of the 40 identified binary objects in the Kuiper belt, of another system, Lempoit is known to be triple.

“Now, Altjira and Lempo are likely triples, so they are more likely to be looking for a population of three-body systems formed by the same situation, rather than a strange ball,” the astronomer said.

“But building that evidence requires time and repeated observation.”

The only Kuiper Belt objects explored in detail are PL Pun and the small object Arrocos that NASA’s New Horizons mission visited in 2015 and 2019, respectively.

New Horizons showed that Arrokoth is a contact binary. This means that in the case of KBO, two objects that have moved close to each other are currently touched or merged, often in the form of peanuts.

“Altozilla is the “cous” of Arokos, a member of the Kuiper Belt Objects of the same group,” Dr. Lagozin said.

“The Altjira is 10 times the Arocos, which is 200 km (124 miles) wide.”

“There is no mission that Altozilla plans to fly to get Arrocos level details, but there are other upcoming opportunities to further study the intriguing system,” Nelsen said.

“Altozilla is entering the season of the eclipse, where the outer body passes in front of the central body.”

“This will continue for the next 10 years and give scientists a great opportunity to learn more about it.”

Team’s paper It was published in Journal of Planetary Science.

____

Maia A. Nelsen et al. 2025. Beyond the point square. IV. The Transneptinian object Altjira is a hierarchical triple, possibly discovered by non-kipler movements. planet. SCI. j 6, 53; doi:10.3847/psj/ad864d

Source: www.sci.news

How to View the Alignment of Every Planet in the Solar System This Week

Artists’ impressions of the solar system

Shutterstock/Vadim Sadovski

All of our solar system planets line up in the night sky once this week. This extraordinary celestial event will see the sky scattered with seven visible planets in what is called a great planet alignment, or what is called a “planet parade.”

The eight planets in our solar system first formed from the same disc of debris around the sun, thus bringing the sun into orbit on roughly the same plane. The lines that line this plane appear along the zodiac when the sun crosses the daytime sky, as the sun crosses the daytime sky, appear all along the zodiac when the planets appear in the sky. The orbit is slightly tilted, so it’s not the perfect line of the planet, but it’s pretty close.

This is less obvious than during planetary alignment. Normally, only a few planets share the night sky, but the unusual alignment of all seven planets will be visible around a few nights, around February 28, depending on your location.

The best time to see is right after sunset, and you will have the opportunity to see all the planets arching in the sky, but all of them are near the horizon except Mars, Jupiter and Uranus. These three will continue to stroll all night, but by the time the sky is completely dark, Mercury and Saturn will sink below the horizon, and Neptune and Venus will soon follow.

The main thing that prevents such alignments from being invisible all the time is the difference in orbital periods between planets, except for the weather. Mercury closest to the Sun takes about 88 Earth days to complete its orbit, but Neptune, most of the distant planets, takes nearly 165 Earth years.

It is only possible to have a large alignment if the planets are all relatively far from the Sun, so they can be seen at night, so they are all in roughly the same half of the sky, so they can be seen at the same time. It’s a coincidence of an astonishing trajectory. Sometimes there are multiple large alignments per year, sometimes even if there are no more than one year, it can pass. A similar event is not scheduled to occur until 2040.

“It’s great to see the interest that Planet Parade is creating.” David Armstrong At the University of Warwick, UK. “It’s all great to be involved in astronomy, look up at the sky and evaluate the wonders of our solar system. I encourage anyone interested in going out and looking at the planets with their own eyes if they get the chance in the next few days.”

Additional Reports by Alex Wilkins

topic:

Source: www.newscientist.com

Astronomers Report Our Solar System Surpassed the “Radcliffe Waves” in the Miocene Era

As our solar system orbits the Milky Way, we encounter a variety of environments, including dense regions of interstellar media. These encounters can increase the flow of interstellar dust into the solar system and the Earth's atmosphere, exposing parts of the solar system to interstellar mediums. The discovery of new galactic structures, such as the Radcliffe waves over the 9,000 Wright years, raises the question of whether the Sun encountered any of them. New research shows that the solar system trajectories intersected with the waves of Radcliffe in the Orion star-forming region 15 to 12 million years ago (Miocene era). In particular, this period coincides with the mid-Miocene climate transition on Earth, providing an interdisciplinary connection with paleoclimatology.

Radcliffe wave visualization. Image credit: Alyssa Goodman/Harvard University.

When the solar system brings the Milky Way into orbit, we encounter a variety of galactic environments with different interstellar densities, including hot voids, fronts of supernova blasts, and cold gas clouds.

The passage of the sun through dense regions of interstellar media can affect the solar system in several ways.

For example, pressure enhancement compresses the heliosphere and exposes parts of the solar system to cold, dense interstellar media.

Furthermore, the amount of interstellar dust mounted on the Earth's atmosphere can increase, potentially enhancing the delivery of radioactive isotopes such as iron-60 through dust grains.

Radcliffe's waves are narrow sinusoidal gas structures and consist of many known star-forming cloud complexes, including CMA, Orion, Taurus, Perseus, Cephaus, North American Nebula, and Cygnus.

With an estimated mass of 3 million people, this gas structure appears to vibrate consistently like a moving wave and is thought to be part of the Milky Way spiral structure.

Dr. Efrem Macconi, a doctoral student at the University of Vienna, said:

“Our Sun encountered a higher gas density region as it passed through the waves of Radcliffe in the Orion constellation.”

Using data from ESA's Gaia mission and spectroscopic observations, Dr. Maconi and his colleagues identified the passage of the solar system through the Radcliffe Wave in the Orion area.

“The findings are based on previous works identifying Radcliffe's waves,” said Professor Joanne Albes of the University of Vienna.

“We passed the Orion area as well as famous star clusters like NGC 1977, NGC 1980 and NGC 1981.”

“The area is easily visible in the winter sky in the Northern Hemisphere and in the summer in the Southern Hemisphere.”

“Look for Orion Constellation and Orion Nebula (Messier 42) – our solar system has come from that direction!”

“The increased dust from this galaxy encounter may have had some effects.”

“It could potentially leave traces of radioactive elements from supernovas in the geological record that permeate the Earth's atmosphere.”

“Current technologies may not be sensitive enough to detect these traces, but future detectors may make it possible.”

This study shows that the solar system passing through the Orion region occurred around 18.2 to 11.5 million years ago, with the most likely time between 148 and 12.4 million years ago.

This time frame is in good agreement with the mid-Miocene climate transition, and is a major shift from warm variable climate to cool climates, leading to the establishment of a continental-scale prototype Antarctic ice sheet composition.

This study raises the possibility of a link between past crossings of the solar system through galaxy neighbours and Earth's climate through interstellar dust, but the authors need further investigation of the causal relationship. It emphasizes that there is.

“The basic processes responsible for the mid-Miocene climate transition have not been fully identified, but available reconstructions are most likely to be long-term reductions in atmospheric greenhouse gas carbon dioxide concentrations. It suggests that it is a high explanation.

“However, our research highlights that interstellar dust associated with the crossing of Radcliffe's waves has affected the Earth's climate and may have played a potential role during this climate change. Masu.”

“To change the Earth's climate, the amount of extraterrestrial dust on Earth needs to be much larger than what previous data suggests.”

“Future research explores the importance of this contribution. This past climate change and current climate change is comparable as this past climate change is unfolding over a timescale of hundreds of thousands of years. It is important to note that we do not do that.”

“In contrast, the evolution of global warming today has been happening at an unprecedented rate for decades to centuries due to human activity.”

study Published in the journal Astronomy and Astrophysics.

____

E. Machoni et al. 2025. Passing through the solar system through the waves of Radcliffe in the mid-Miocene. A&A 694, A167; doi: 10.1051/0004-6361/202452061

Source: www.sci.news

Astronomers Possibly Found the Swiftest Exoplanet System on Record

Candidate planetary systems detected by microlens method are thought to travel at least 540 km (1.2 million mph) per 540 km.



Impressions of the superniputin exoplanet artist orbiting a low-mass star near the center of our Milky Way galaxy. Image credits: NASA/JPL-Caltech/R. Hurt, Caltech-IPAC.

“I think this is the so-called Super Neptune world orbiting a low-mass star at the distance between Venus and Earth's orbit,” University of Maryland, College Park, NASA Goddard. At the Space Flight Center.

“The star is so weak that it is outside its habitable zone. If so, it will be the first planet ever discovered orbiting a fast star.”

The system was first discovered indirectly in 2011 thanks to the microlens event MOA-2011-BLG-262.

“Microlenses occur because a large amount of presence distorts the fabric of space-time,” the astronomer explained.

“Whenever an intervening object appears to drift near a background star, light from the star curve passes through space-time, distorted around nearby objects.”

“If the alignment is particularly close, the distortion around the object behaves like a natural lens and can amplify the light of the background star.”

In MOA-2011-BLG-262, microlens signals revealed pairs of celestial bodies.

Astronomers have determined relative masses (one is about 2,300 times heavier than the other), but their exact mass depends on how far they are from the Earth.

“It's easy to determine the mass ratio,” said Dr. David Bennett, a senior research scientist at the Goddard Space Flight Center at the University of Maryland, College Park and NASA.

The MOA-2011-BLG-262 Discovery Team has a microlens object that is about 20% of the stars, about 29 times heavier than Earth, or Jupiter's mass with Exomoon. They suspected it was one of roughly four times more illicit planets.

To understand which explanations were more likely, Dr. Terry, Dr. Bennett and his colleagues searched data from the Keck Observatory in Hawaii and the Gaia satellite at the ESA.

If the pair are illegitimate Exoplanets and Exomoons, they will not look effective – dark objects lost in the black space of the universe.

Researchers discovered a strong suspect about 24,000 light years away and put it in the bulge of the Milky Way galaxy.

By comparing the position of the stars in 2011 and 2021, they calculated its speed.

But that's its 2D motion. If it's heading towards us or away from us, it must be moving even faster.

Its true speed may increase to the galaxy's escape speed exceeding 600 km/s (1.3 million mph) per second.

If so, the planetary system is destined to traverse intergalactic space for millions of years to come.

“To make sure the newly identified star is part of the system that caused the 2011 signal, we looked again in another year and it moved the right amount and moved in the right direction. And I want to see where it is. We've detected a signal,” Dr. Bennett said.

“If a high-resolution observation indicates that the stars remain in the same position, it can be sure that it is not part of the system that caused the signal,” says Aparna Bhatacharya at the University of Maryland. The doctor said. College Park and NASA's Goddard Space Flight Center.

“That means the Rogue Planet and the Exomoon model are preferred.”

Team's paper It was released this week Astronomy Journal.

____

Sean K. Terry et al. 2025. A candidate high-speed peeling system for galaxy swelling. AJ 169, 131; doi:10.3847/1538-3881/ad9b0f

Source: www.sci.news

Planets of the Solar System

In the southwestern sky, Venus shines the brightest and is easy to spot. Saturn can be seen below Venus, but as the days progress, the other visible planets become harder to spot, sinking lower in the sky each day after sunset. Jupiter can be found in the southern part of the evening sky, while Mars appears in the eastern sky. Mercury should also be visible to the naked eye, but it is challenging to find due to its proximity to the sun.

By February 24th, mercury will be further from the sun, making it easier to spot after sunset near Saturn in the western sky.

For skywatchers with binoculars and telescopes, Uranus and Neptune can also be spotted with dedication, patience, and a Starchart, according to Faherty.

NASA refers to this event as the “Planet Parade,” where multiple bright planets are visible simultaneously overhead. This phenomenon occurs when all planets in our solar system orbit the sun on relatively flat disc-shaped planes, akin to cars on a racetrack. Each planet orbits the sun at different rates, resulting in them lining up in the sky at different points, like cars on a track.

The planetary parade will continue until February, with more opportunities to view multiple bright planets in the sky in the months and years ahead, including instances of four planets lining up before sunrise in late August, five planets before sunrise in October 2028, and five planets after sunset in February 2034.

Faherty sees this event as a great educational opportunity for newcomers to explore the universe in an engaging way, as the sky is always changing and full of surprises.

Source: www.nbcnews.com

UK welfare system AI prototype criticized for its “misguided launch,” say officials

According to the Guardian, ministers have halted or abandoned at least six artificial intelligence prototypes for welfare systems, indicating that Prime Minister Kia Starmer’s efforts to improve government efficiency are facing challenges.

It has been revealed that these AI prototypes were not advanced to enhance staff training, improve job center services, expedite disability benefits payments, and update communication systems. Officials acknowledge the importance of “thorough testing” to ensure the expandability and reliability of the AI system.

While two of the discarded prototypes were highlighted as successful tests in the latest annual report by the Department of Labor Pensions (DWP), A-Cubed aimed to assist staff in guiding job seekers and Igents to expedite disability benefits for millions of people.

The Prime Minister emphasized the role of AI in transforming public services and urged ministers to prioritize the introduction and growth of AI in each ministry and agency. However, Ada Loveless’s Associate Director, Imougen Parker, highlighted the importance of learning from failures and ensuring that the reality of AI aligns with rhetoric.

The use of AI in welfare systems by DWP has not been disclosed in the government’s algorithm transparency registry, raising concerns about transparency and accountability in the use of AI technology.

While officials have acknowledged that AI technology may play a role in future system developments, they stress the importance of thorough testing before implementation. This indicates the challenges faced by the Labour Party in their efforts to revolutionize public services through AI.

Peter Kyle, the Secretary of State for Science, Innovation, and Technology, announced plans to utilize AI for transforming public services and improving economic productivity. Director Laura Gilbert highlighted the importance of learning from failures and continuing to explore new opportunities for impact.

The DWP officials emphasized the importance of scalability and reliability in AI products and acknowledged the need for thorough testing before implementing AI systems. However, concerns remain about transparency and the potential impact of AI on inequality and fairness in the welfare field.

The government spokesperson highlighted the short-term nature of concept demonstration projects and the importance of learning from these projects to inform future implementations. The government aims to follow a “Scan, Pilot, Scale” approach outlined in the AI opportunity action plan to harness the full potential of AI in transforming public services.

Source: www.theguardian.com

New Discovery: Long-period Giant Exoplanet Found in Multiplanetary System WASP-132

WASP-132 is a unique multiplanet system in that both the inner rocky planet and the newly discovered outer giant planet are in a system that includes a hot Jupiter planet. This suggests that hot Jupiter migrated via a rare dynamically cooled mechanism and helps further our understanding of how hot Jupiter systems form and evolve. .

The WASP-132 system includes hot Jupiter (in the foreground), an inner super-Earth (passing in front of the orange host star), and the cold planet WASP-132d. Image credit: Thibaut Roger, University of Geneva.

A hot Jupiter is a planet with a mass similar to Jupiter, but it orbits closer to its star than Mercury, which orbits the Sun.

Because there is not enough gas or dust for these giant planets to form where they are observed, the established theory is that they originate far from their stars and are not planets. They move inward as the system evolves.

Until now, it was thought that hot Jupiter was orbiting the star alone, as other planets in the system were ejected as it moved toward the star.

Two extra planets in the WASP-132 planetary system now cast doubt on this theory.

“The WASP-132 system is an excellent laboratory for studying the formation and evolution of multiplanetary systems,” said Dr. François Bouchy, an astronomer at the Geneva Observatory.

“The discovery of hot Jupiters alongside inner super-Earths and distant giants challenges our understanding of the formation and evolution of these systems.”

“This is the first time I have observed such a configuration.”

Hot Jupiter WASP-132b orbits its parent star every 7.1 days. Super Earth WASP-132c orbits the star in just 24 hours and 17 minutes.

The newly discovered ice giant, named WASP-132d, will orbit its host star for five years.

Dr David Armstrong from the University of Warwick said: “Finding planets inside the hot interior of Jupiter is particularly rare, so the detection of an inner super-Earth was exciting.”

“We conducted an intensive campaign using state-of-the-art instruments to characterize its mass, density and composition, revealing a planet with a similar density to Earth.”

“The discovery of this planet adds further complexity to the WASP-132 system, as the movement of hot Jupiter towards the host star due to dynamic perturbations destabilizes the orbits of the other two planets.”

“This suggests a more stable, ‘cooler’ migration path for hot Jupiter in the protoplanetary disk that surrounds young stars and is the site of planet formation.”

Regarding this discovery, paper Published in today’s magazine astronomy and astrophysics.

_____

nolan greaves others. 2025. Discovery of a cold giant planet and measurement of the mass of a hot super-Earth in the multiplanetary system WASP-132. A&A 693, A144; doi: 10.1051/0004-6361/202348177

Source: www.sci.news

Study Shows Octopus Arm Nervous System is Sectioned into Parts

Controlling octopus motion is a very complex issue. Each of its eight arms is a muscular hydrostat, a soft-bodied structure without a rigid skeleton that moves with nearly infinite degrees of freedom. Additionally, the arm is packed with hundreds of suction cups, each of which can change shape independently. Despite this complexity, octopuses effectively control behavior along the length of a single arm, across all eight arms, and between suckers. In a new study, scientists at the University of Chicago show that the circuits in the nervous system that control the movements of an octopus' arms are subdivided, allowing this extraordinary creature to explore its environment, grasp objects, and capture prey. discovered that he could precisely control his arms and suction cups.

Octopus at USC Wrigley Marine Science Center on Catalina Island. Image credit: University of Southern California.

“If you're going to create a nervous system that controls dynamic movements like this, that's a good way to set it up,” said Clifton Ragsdale, a professor at the University of Chicago.

“We think this is a feature that evolved specifically in soft-bodied cephalopods with suckers for insect-like movements.”

Each arm of an octopus has an extensive nervous system, with more neurons connected across all eight arms than in the animal's brain.

These neurons are concentrated in large axial nerve cords (ANCs) that snake back and forth as they travel along the arm, forming an extension above each sucker with each bend.

The study authors wanted to analyze the structure of the ANC and its connections with the musculature of the arm. California two-spotted octopus (Octopus bimacroides)a small species native to the Pacific Ocean off the coast of California.

They tried to view a thin circular cross-section of the arm under a microscope, but the sample kept falling off the slide.

They tried peeling the arm lengthwise and got lucky, leading to an unexpected discovery.

Using cell markers and imaging tools to track structures and connections from the ANC, they found that neuronal cell bodies are packed into columns that form corrugated pipe-like segments.

These segments are separated by gaps called septa, through which nerves and blood vessels connect to nearby muscles.

Nerves from multiple segments connect to different regions of the muscle, suggesting that these segments work together to control movement.

“If you think about this from a modeling perspective, the best way to set up a control system for this very long, flexible arm is to break it up into segments,” said Cassady Olson, a graduate student at the University of Chicago. states.

“There has to be some communication between the segments. I can imagine that helping smooth the movement.”

The sucker nerves also exit the ANC through these septa and are systematically connected to the outer edge of each sucker.

This indicates that the nervous system sets up a spatial or topographic map of each sucker.

Octopuses can move their suction cups independently and change their shape.

The suckers are also packed with sensory receptors that allow the octopus to taste and smell things it touches. This is the same as combining your hands, tongue, and nose.

The researchers believe that the suckers (what they called maps) facilitate this complex sensorimotor ability.

To see if this kind of structure is common to other soft-bodied cephalopods, the researchers also Long-tailed squid (Dorytheutis Pileyi)common in the Atlantic Ocean.

These squid have eight arms and two tentacles with octopus-like muscles and suckers.

The tentacles have long stalks without suction cups, and at the end are clubs with suction cups.

While hunting, squid can shoot out tentacles and catch prey with clubs equipped with suckers.

Using the same process to study long strips of squid tentacles, we found that the ANC in the suckerless stem was unsegmented, but the club at the end was segmented in the same way as in the octopus. .

This suggests that the segmented ANC was built specifically to control all types of dexterous sucker-equipped appendages in cephalopods.

However, squid tentacle clubs have fewer segments per sucker, probably because they do not use suckers for sensation like octopuses do.

Squids rely on sight to hunt in the open ocean, while octopuses roam the ocean floor and use their sensitive arms as tools for exploration.

Octopuses and squids diverged more than 270 million years ago, but the similarities in how some of their appendages are controlled by suction cups and the differences in others are a question of how evolution always best resolves them. It shows you how to find a solution.

“An organism with insect-like, sucker-containing appendages needs the right kind of nervous system,” Professor Ragsdale says.

“Different cephalopods have come up with segmented structures, the details of which vary depending on environmental demands and hundreds of millions of years of evolutionary pressure.”

of study Published in a magazine nature communications.

_____

C.S. Olson others. 2025. Neuronal segmentation in the cephalopod arm. Nat Commune 16, 443;doi: 10.1038/s41467-024-55475-5

Source: www.sci.news

Advancements in Research Shed Light on Habitability of Oceanic Worlds in Our Solar System and Beyond

In a new paper, planetary researchers from Texas A&M University and the University of Washington introduce a new thermodynamic concept called centotectics to investigate the stability of liquids under extreme conditions. This is important information for determining the habitability of icy moons and oceanic exoplanets.

Europa's surface stands out in this newly reprocessed color view. Image scale is 1.6 km per pixel. North of Europe is on the right. Image credit: NASA / JPL-Caltech / SETI Institute.

Exploration of icy ocean worlds represents a new frontier in planetary science, with a focus on understanding the potential of these environments to support life.

New research is addressing fundamental questions in this field. Under what conditions can liquid water remain stable on these distant frozen bodies?

The authors provide an important framework for interpreting data from planetary exploration activities by defining and measuring the cenotect, the absolute minimum temperature at which a liquid remains stable under various pressures and concentrations.

This research combines their expertise in cryobiology with their expertise in planetary science and high-pressure water ice systems.

Together, they developed a framework that bridges the disciplines to tackle one of the most fascinating challenges in planetary science.

2016 artist concept for the European Clipper spacecraft. As spacecraft development progresses, the design changes. Image credit: NASA/JPL-Caltech.

“The launch of NASA's Europa Clipper, the largest planetary exploration mission ever launched, ushered us into a decades-long era of exploration of the frigid ocean world,” said Dr. Baptiste Journeau, a planetary scientist at the University of Washington. It's coming in,” he said.

“Measurements from this and other missions will tell us the depth of the ocean and its composition.”

“Laboratory measurements of liquid stability, particularly the lowest possible temperature (a newly defined cenotect), combined with the mission results will help us determine how habitable the solar system's cold, deep oceans are, and how likely they will ultimately be. It will be possible to completely constrain what the temperature will be.''The fate would be when the moon or planet cools down completely. ”

“The study of icy worlds is a particular priority for both NASA and ESA, as evidenced by the spate of recent and upcoming spacecraft launches,” said Dr. Matt Powell-Palm, a planetary scientist at Texas A&M University. Ta.

“We hope to help Texas A&M provide intellectual leadership in this area.”

of paper Published in the Journal on December 18, 2024 nature communications.

_____

A. Zaris others. 2024. On the equilibrium limit of liquid stability in pressurized water systems. nut community15;doi: 10.1038/s41467-024-54625-z

Source: www.sci.news

Binary star system found in close proximity to the central black hole of the Milky Way galaxy

Using data from ESO’s Very Large Telescope (VLT) and the Keck Telescope, astronomers detected a binary star system in the S star cluster near Sagittarius A*, the supermassive black hole at the center of the Milky Way. I discovered it. This is the first time that a binary star has been discovered near a supermassive black hole.

This image shows the location of binary star D9 orbiting Sagittarius A*, the supermassive black hole at the center of the Milky Way. Image credit: ESO / Peißker et al. / S. Guizard.

Sagittarius A* is orbited by fast stars and dusty objects collectively known as the S cluster.

Binary star systems (two stars gravitationally bound to each other around a common center of mass) are predicted to exist within the S cluster, but have not been detected so far.

Previous studies have suggested that such stars are unlikely to be stabilized by their interactions with Sagittarius A*.

“Black holes are not as destructive as we think,” says Florian Peisker, an astronomer at the University of Cologne.

“Our findings show that some binaries can temporarily thrive even under disruptive conditions.”

The newly discovered binary star, named D9, is estimated to be just 2.7 million years old.

Due to the strong gravity of the nearby black hole, it will probably merge into a single star within just a million years, a very short time for such a young system.

“This only provides a short window on the cosmic timescale for observing such binary star systems, but we succeeded,” said Dr. Emma Bordier, also from the University of Cologne. Ta.

“The D9 system shows clear signs of gas and dust surrounding the star, suggesting it may be a very young system that must have formed near a supermassive black hole. ” said Dr. Michal Zajacek. Astronomer at Masaryk University and the University of Cologne.

The most mysterious of the S clusters are the G objects, which behave like stars but look like clouds of gas and dust.

It was while observing these mysterious objects that the research team discovered a surprising pattern in D9.

“This result sheds new light on what the mysterious G-objects are,” the authors said.

“They may actually be a combination of binaries that have not yet merged and leftover material from stars that have already merged.”

“Planets often form around young stars, so this discovery allows us to speculate about their existence,” Dr. Pisker said.

“It seems like it’s only a matter of time before planets are detected at the center of the galaxy.”

a paper This discovery was published in today’s magazine nature communications.

_____

F. Peisker others. 2024. A binary star system in the S star cluster near the supermassive black hole Sagittarius A*. Nat Commune 15, 10608; doi: 10.1038/s41467-024-54748-3

Source: www.sci.news

AI system used to detect UK benefits fraud exposed for bias | Universal Credit

The Guardian has uncovered that artificial intelligence systems utilized by the UK government to identify welfare fraud exhibit bias based on individuals’ age, disability, marital status, and nationality.

A review of a machine learning program used to analyze numerous Universal Credit payment claims across the UK revealed that certain groups were mistakenly targeted more frequently than others.

This revelation came from documents published under the Freedom of Information Act by the Department for Work and Pensions (DWP). A “fairness analysis” conducted in February of this year uncovered a significant discrepancy in outcomes within the Universal Credit Advance automated system.

Despite previous claims by the DWP that the AI system had no discrimination concerns, the emergence of this bias raises important questions about its impact on customers.

Concerns have been raised by activists regarding the potential harm caused by the government’s policies and the need for transparency in the use of AI systems.

The DWP has been urged to adopt a more cautious approach and cease the deployment of tools that pose a risk of harm to marginalized groups.

The discovery of disparities in fraud risk assessment by automated systems may lead to increased scrutiny of the government’s use of AI, emphasizing the need for greater transparency.

The UK public sector employs a significant number of automated tools, with only a fraction being officially registered.

The lack of transparency in the use of AI systems by government departments has raised concerns about potential misuse and manipulation by malicious actors.

The DWP has stated that their AI tools do not replace human judgment and that caseworkers evaluate all available information when making decisions related to benefits fraud.

Source: www.theguardian.com

Scientists find a new exoplanet in Kepler-51 system

Kepler-51 is a 500-million-year-old G-type star that hosts four low-density planets. new paper Published in astronomy magazine.

This diagram shows the Kepler-51 planetary system. Image credit: NASA / ESA / L. Hustak, J. Olmsted, D. Player & F. Summers, STScI.

Kepler-51 It is located approximately 2,615 light years away in the constellation Cygnus.

The star, also known as KOI-620, was already known to host three Saturn-sized “superpuff” exoplanets: Kepler-51b, c, and d.

First discovered by NASA's Kepler Space Telescope in 2012, these worlds have orbital period ratios close to 1:2:3 (45, 85, and 130 days, respectively).

It is several times more massive than Earth and has a hydrogen/helium atmosphere.

“Superpuff planets are very unusual in that they have very low masses and very low densities,” says Penn State astronomer Jessica Libby Roberts.

“The three planets known so far orbiting the star Kepler-51 are about the same size as Saturn, but only a few times the mass of Earth, making them as dense as cotton candy. ”

“We think they have small cores and huge atmospheres of helium hydrogen, but we don't know how these strange planets formed and how their atmospheres developed. It remains a mystery why the star was not blown away by the intense radiation of the young star.

“We had planned to use Webb to study one of these planets to answer these questions, but now we have to describe the fourth, low-mass planet in the system.”

To examine evidence of Kepler-51e, the fourth planet in the system, astronomers conducted extensive passes over 14 years from a variety of facilities, including the Webb, Apache Point Observatory telescopes, and Penn State Davey Laboratory telescopes. We utilized a timing dataset.

“We conducted a so-called 'brute force' search, testing different combinations of planet properties to find a four-planet model that explains all transit data collected over the past 14 years.” said Kento Masuda, an astronomer at Osaka University.

“We found that the signal is best explained if Kepler-51e has a mass similar to the other three planets and follows a fairly circular orbit of about 264 days. That's to be expected.”

“Other possible solutions we've found include larger planets in wider orbits, but we think that's unlikely.”

It is unclear whether Kepler-51e is also a superpuff planet, as researchers have not observed Kepler-51e transiting the Sun and therefore cannot calculate its radius or density.

According to the team, a wide range of demographics (

“Superpuff planets are fairly rare, and when they do occur, they tend to be unique in planetary systems,” said Penn State astronomer Jessica Libby Roberts.

“If explaining how three superpuffs formed in one star system wasn't enough of a challenge, now we have to explain a fourth planet, whether it's a superpuff or not. And we can't rule out the possibility that there are more planets in this system.”

“Kepler-51e's orbit is slightly larger than Venus and just inside the star's habitable zone, so there could be a lot more going on beyond that distance if we take the time to look.”

“Continuing to observe variations in transit timing could help us discover planets further away from their stars, which could aid in the search for planets that may harbor life.”

_____

Kento Masuda others. 2024. The fourth planet in the Kepler-51 system revealed by fluctuations in transit timing. A.J. 168, 294; doi: 10.3847/1538-3881/ad83d3

Source: www.sci.news

Astrophysicists discover that black hole-hosting binary star V404 Cygnus is part of a triple system

V404 Cygnus, an X-ray binary star that hosts a low-mass black hole, has a wide echelon with a tertiary companion at least 3,500 astronomical units (AU) away from the inner binary, according to MIT astrophysicists. It is said to be part of a triple star.

V404 SIGNI. Image credit: Verge others., doi: 10.1038/s41586-024-08120-6.

V404 Cygni is located approximately 7,800 light-years away in the constellation Cygnus.

This system first attracted attention more than 80 years ago, during the 1938 nova explosion.

Another eruption occurred in 1989 and was discovered by the Japanese X-ray satellite Ginga and high-energy instruments aboard the Mir space station.

The 1989 explosion, known as Nova Cygnus 1989, was pivotal in the study of black holes.

Until then, astronomers had known of only a handful of objects that could be black holes, and V404 Cygnus was one of the most likely candidates.

V404 Cygnus is known to host a central stellar-mass black hole in the act of consuming a small star that spirals very close to the black hole every 6.5 days. This is a configuration similar to most binary star systems.

But new research suggests there's a second star orbiting the black hole, albeit much further away.

“Most black holes are thought to be formed by violent explosions of stars, but this discovery helps cast doubt on that,” said Kevin Burge, a researcher at the Massachusetts Institute of Technology (MIT). Ta.

“This system is very interesting for the evolution of black holes, and also raises the question of whether triples exist.”

Artist's impression of V404 Cygnus: The central black hole (black dot) is consuming a nearby star (orange object on the left), while the second star (white flash at the top) is far away orbiting a distance of Image credit: Jorge Lugo.

Burge and his colleagues estimate that the third companion star orbits the V404 Cygnus black hole every 70,000 years.

The fact that black holes appear to exert a gravitational pull on distant objects raises questions about the origins of black holes themselves.

Black holes are thought to be formed by violent explosions of dying stars. This is a process known as a supernova, in which a star releases a huge amount of energy and light in one final burst before collapsing into an invisible black hole.

But the team's findings suggest that if the newly observed black hole had originated from a typical supernova, the energy released before it collapsed would have kicked loosely bound objects around it. It suggests that it might have been.

So the second outer star shouldn't be hanging around yet.

Instead, the authors believe that the V404 Cygnus black hole formed through a more gentle process of direct collapse, in which the star simply collapsed and formed the black hole without a final, dramatic flash. I think it might be.

Such a benign origin poses little impediment to loosely bound, distant objects.

Because V404 Cygnus contains a very distant star, this suggests that the black holes in this system were born through a more gradual, direct collapse.

And while astronomers have observed more violent supernovae for centuries, this triple system may be the first evidence of a black hole formed from this more gentle process.

In addition to providing clues about the black hole's origin, the outer star also revealed the age of the system.

Astrophysicists observed that the outer star happened to be in the process of becoming a red giant, a stage that occurs at the end of a star's life.

Based on this star's evolution, they determined that the outer star was about 4 billion years old.

Considering that the neighboring stars were born at about the same time, they conclude that the components of the binary star are also 4 billion years old.

“This has never been done before with old black holes,” Dr. Burge says.

“Thanks to this discovery, we now know that V404 Cygnus is part of a triple star. It may have formed by direct collapse, and it formed about 4 billion years ago.”

of findings Published in this week's magazine nature.

_____

KB barge others. The black hole low-mass X-ray binary V404 Cygnus is part of a wide triple. naturepublished online October 23, 2024. doi: 10.1038/s41586-024-08120-6

Source: www.sci.news

Allen Telescope Array seeks radio signatures of technology from TRAPPIST-1 system

The TRAPPIST-1 system is a compact system of at least seven exoplanets that are similar in size to Earth. Astronomers from Pennsylvania State University and the SETI Institute spent 28 hours scanning the system for signs of alien radio technology using the Allen Telescope Array. This project marks the longest single-target search for radio signals from TRAPPIST-1. Although astronomers found no evidence of extraterrestrial technology, their work introduced new ways to search for wireless techno-signatures in the future.

This artist's impression shows a surface view of one of the exoplanets in the TRAPPIST-1 planetary system. Image credit: ESO / M. Kornmesser / Spaceengine.org.

TRAPPIST-1 is an ultracool dwarf star located 38.8 light-years away in the constellation Aquarius.

This star is barely larger than Jupiter and has only 8% the mass of the Sun. It rotates rapidly and produces an energetic flare of ultraviolet light.

TRAPPIST-1 is the home planet of seven transit planets named TRAPPIST-1b, c, d, e, f, g, and h.

All of these planets are the same size or slightly smaller than Earth and Venus, and have very short orbital periods of 1.51, 2.42, 4.04, 6.06, 9.21, 12.35, and 20 days, respectively.

Presumably they are all tidally locked, meaning that the same side of the planet always faces the star, just as the same side of the moon always points towards the Earth. This creates a persistent night side and a persistent day side for each planet in TRAPPIST-1.

Three of the planets, TRAPPIST-1e, f, and g, are located in the star's habitable zone, meaning they may have an environment suitable for life.

“The TRAPPIST-1 system is relatively close to Earth and has detailed information about the planet's orbit, making it an excellent natural laboratory for testing these technologies,” said Penn State graduate student Nick Tasei said.

“The methods and algorithms we developed for this project could eventually be applied to other star systems, increasing the likelihood of finding regular communications between planets beyond our solar system (if they exist). ).

Tusay and his colleagues focused on a phenomenon called interplanetary occultations.

These occultations occur when one planet moves in front of another. If intelligent life exists in that star system, it is possible that radio signals sent between the planets could leak and be detected from Earth.

Astronomers used the upgraded Allen Telescope Array to scan a wide range of frequencies, looking for narrowband signals that could be a possible sign of alien technology.

They filtered through millions of potential signals and narrowed it down to about 11,000 candidates for further analysis.

They detected 2,264 of these signals during the predicted interplanetary occultation period. However, none of the signals were of non-human origin.

New features of the Allen Telescope Array include advanced software to filter signals, helping researchers separate possible alien signals from those on Earth.

They believe that improving these techniques and focusing on phenomena such as interplanetary occultations could increase the chances of detecting alien signals in the future.

Although scientists did not find any alien signals this time, they plan to continue refining their search techniques and exploring other star systems.

Future explorations using larger and more powerful telescopes could help scientists detect even fainter signals and expand our understanding of the universe.

“This study shows that we are getting closer to detecting radio signals similar to those we send into space,” Tusey said.

“Most searches assume some kind of intent, such as a beacon, because our receivers have a sensitivity limit to the minimum transmit power above what we transmit unintentionally.”

“But with better instruments, such as the upcoming Square Kilometer Array, we may soon be able to detect signals from alien civilizations communicating with our spacecraft.”

of the team result will appear in astronomy magazine.

_____

Nick Tasei others. 2024. TRAPPIST-1 wireless technology signature search using the Allen Telescope Array. A.J.in press. arXiv: 2409.08313

Source: www.sci.news

Hubble captures twin stars in R Aquarii binary system

Astronomers using the NASA/ESA Hubble Space Telescope have created a unique time-lapse of R Aquari's dynamic behavior from observations spanning 2014 to 2023.



The two stars in the R Aquarii binary system are approximately 1.6 billion miles apart. Image credits: NASA / ESA / Matthias Stute / Margarita Karovska / Davide De Martin / Mahdi Zamani / N. Bartmann, ESA, Hubble.

Located 650 light years away, R Aquary is a so-called symbiotic binary, consisting of two stars surrounded by a large, dynamic cloud of gas.

Such binaries contain two stars in an unequal and complex relationship: a white dwarf and a red giant.

In a disturbing act of stellar cannibalism, white dwarfs are stripping material from their larger companions.

Suffering red giants and unstable white dwarfs occasionally eject material in strange eruptions, loops, and trajectories.

“The twisted outflow of stars makes the region look like an out-of-control lawn sprinkler,” Hubble astronomers said in a statement.

“This dramatically shows how the universe redistributes the products of nuclear energy that form deep inside stars and are jetted out into space.”

“Aquarius R belongs to a class of double stars called symbiotic stars,” they added.

“The host star is an aging red giant star, and its companion star is a compact, burnt-out star known as a white dwarf.”

“The red giant star is mira variable It is more than 400 times larger than the Sun. ”

“The expanded monster star pulsates, changes temperature, and changes brightness by a factor of 750 over a period of approximately 390 days.”

“At its peak, the star is blindingly bright, about 5,000 times brighter than the Sun.”

“When the white dwarf comes closest to the red giant star during its 44-year orbit, it gravitationally sucks out hydrogen gas.”

“This material accumulates on the surface of the dwarf star until spontaneous nuclear fusion occurs, causing the surface to explode like a giant hydrogen bomb.”

“After the explosion, the fueling cycle begins again.”

“This explosion causes geyser-like filaments to erupt from the core, forming strange loops and trajectories as the plasma emerges as a streamer.”

“The plasma is twisted by the force of the explosion and guided upwards and outwards by a strong magnetic field.”

“The outflow appears to be folded into a spiral pattern.”

“Plasma is ejecting into space at more than 1.6 million km (1 million miles) per hour, which is fast enough to travel from Earth to the Moon in 15 minutes.”

“The filament glows in visible light because it is energized by intense radiation from the star.”

Source: www.sci.news

‘Sustainable Startups Struggle to Fix Broken Food System as Venture Capital Seeks Return on Investment’

Andrew Carter and Adam DiMartino launched Smallhold in 2017 with a goal of providing mushrooms to more people. Carter believed that mushrooms are highly sustainable in terms of water, waste, plastic use, and emissions. Over the years, Smallhold has successfully introduced specialty mushrooms like shiitake, green oysters, and trumpet mushrooms to grocery stores and households across America.

As mushrooms gained popularity as a symbol of sustainability during the pandemic, Smallhold found success and attention from the media, resulting in a valuation of $90 million. Despite starting in a Brooklyn shipping container, the brand expanded rapidly with farms in New York, Texas, and California, selling in 1,400 stores nationwide.

Smallhold’s co-founders, DeMartino and Carter, believe in promoting sustainability and reducing waste in the food industry. However, the company faced challenges when the founders resigned, leading to Smallhold filing for bankruptcy. Although the brand was acquired and reorganized, it struggled to maintain its original vision, closing farms and reducing staff.

For entrepreneurs, Smallhold’s journey serves as a lesson on finding a niche beyond sustainability and ensuring economic sustainability. While the company focused on unique mushroom varieties and sustainable practices, it also built a strong brand through aesthetics and social media. It’s crucial for startups to deliver quality products, maintain profitability, and avoid excessive reliance on venture capital.

In the evolving landscape of food startups, lessons can be learned from Smallhold’s experience. By combining sustainability with quality, variety, and branding, companies can attract customers and thrive in the market. Innovating in the food industry requires a balance between financial responsibility and sustainability goals, defining success on your own terms.

Source: www.theguardian.com

Research Indicates Sun-like Star-shaped Outer Solar System Approached Billions of Years Ago

At least 140 million Sun-like stars in our Milky Way galaxy may have experienced similar stellar flybys, according to a new study by astrophysicists from the Jülich Research Centre and Leiden University.

Snapshot of a flyby of an ancient star. Blue-green particles indicate TNOs injected into the planetary region by the flyby. The perturbation star passed through the disk at perihelion distance 110 AU, on the right side of the picture. Image courtesy of Pfalzner others., doi: 10.1038/s41550-024-02349-x.

The planets in our solar system accumulated from a disk of dust and gas orbiting the young Sun.

Thus, the planets move in circular orbits close to a common plane.

About 3,000 small bodies have been observed orbiting the Sun beyond Neptune. Surprisingly, most of them move in eccentric or inclined orbits.

Therefore, some force must have lifted these trans-solar objects (TNOs) out of the disk in which they formed and significantly altered their orbits.

“When we think about the solar system, we usually think of it ending with Neptune, the outermost known planet,” said Dr Susanne Pfalzner, astrophysicist at the Jülich Research Centre and lead author of the paper.

“However, thousands of objects are known to travel beyond the orbit of Neptune.”

“It is even suspected that there are tens of thousands of objects over 100 kilometers in diameter.”

“Surprisingly, many of these TNOs travel on eccentric orbits that are inclined with respect to the common orbital plane of the planets in our solar system.”

In this study, Dr. Falzner and her colleagues compared the properties of observed TNOs with thousands of flyby simulations to determine specific properties of stellar flybys that could potentially reproduce all of the different TNO populations, their locations, and relative abundances.

They Found A flyby of a 0.8 solar mass star at a distance of 110 AU could explain the inclined and highly eccentric orbits of known TNOs.

“We can even infer the orbits of very distant objects, such as Sedna, a dwarf planet discovered in the outermost solar system in 2003,” Dr Pfalzner said.

“There are also objects moving in orbits that are almost perpendicular to the planet's orbit.”

“Such flybys could even explain the orbits of two objects moving in the opposite direction to the planet: 2008 KV42 and 2011 KT19.”

“The best match we found in our simulations for the outer solar system today is a star that is slightly lighter than our Sun, about 0.8 times its mass,” said Dr Amis Govind, also of the Jülich research centre.

“It traveled about 16.5 billion kilometers from the Sun, which is about 110 times the distance between Earth and the Sun and just under four times the distance to the outermost planet, Neptune.”

Astrophysicists were surprised Found The irregular moons orbiting the giant planets in the solar system in distant, inclined, and eccentric orbits are actually TNOs that were launched into the inner solar system by close passes of their stars.

“Some of these objects could have been captured as moons by giant planets,” said Dr Simon Portegies Zwart, an astrophysicist at Leiden University.

“This would explain why the outer planets in our solar system have two different types of moons.”

“In contrast to regular moons, which orbit their planets in circular orbits close to the planet, irregular moons orbit their planets at greater distances in inclined, elongated orbits.”

“Until now, there has been no explanation for this phenomenon.”

“The beauty of this model is its simplicity. With just one source, it answers several outstanding questions about our solar system,” Dr Pfalzner said.

_____

Susanne Falzner othersOrbits of flybys of stars that formed the outer solar system. Nat AstronPublished online September 4, 2024; doi: 10.1038/s41550-024-02349-x

Susanne Falzner others2024. A close flyby of a star could inject an irregular moon from outside the solar system. Apu JL 972, L21;doi:10.3847/2041-8213/ad63a6

Source: www.sci.news

Research indicates TRAPPIST-1 system developed through a two-stage formation process

TRAPPIST-1 is an ultracool dwarf star located 38.8 light-years away in the constellation Aquarius that hosts seven planets. The period ratios of the neighboring planets are closer as they move away from the star: 8:5, 5:3, 3:2, 3:2, 4:3, 3:2. This compact resonant configuration is a clear indication of disk-driven migration, but the desired outcome of such an evolution would be the establishment of a first-order resonance, rather than the higher-order resonances observed in the inner system. Astronomer Gabriele Pichierri of the California Institute of Technology and his colleagues explain the orbital configuration of the TRAPPIST-1 system with a model that is largely independent of the specific disk migration and orbital circularization efficiency. Two key elements of the team's model are that, along with the migration, the inner boundary of the protoplanetary disk retreated over time, and that the TRAPPIST-1 system initially separated into two subsystems.

This artist's rendering shows TRAPPIST-1 and its planets as seen on the surface. Image courtesy of NASA / R. Hurt / T. Pyle.

“When all we had to analyse was the solar system, we could simply assume that planets formed where we see them today,” Dr Pichieri said.

“But when the first exoplanet was discovered in 1995, we had to rethink this assumption.”

“We're developing better models of how planets form and how they come to be oriented in the way that we found them.”

Most exoplanets are thought to form from a disk of gas and dust around a newly formed star, and then migrate inwards, approaching the inner boundary of this disk.

This results in a planetary system assembled much closer to the host star than is the case in our solar system.

In the absence of other factors, planets tend to move away from each other at characteristic distances based on their mass and the gravitational force between them and their host star.

“This is the standard transition process,” Dr. Pichieri said.

“The positions of the planets form resonances between their respective orbital periods. If you divide the orbital period of one planet by the orbital period of its neighbor, you get a simple integer ratio like 3:2.”

For example, if one planet takes two days to orbit a star, the next planet further away takes three days.

If the second planet and a more distant third planet were also in 3:2 resonance, the third planet's orbital period would be 4.5 days.

“The exoplanets behave nicely in simpler predicted resonances, so to speak,” Dr Pichieri said.

“But the inner ones have slightly more exciting resonances. For example, the orbital ratio of planets b and c is 8:5, and the ratio of c and d is 5:3.”

“This subtle difference in the outcome of TRAPPIST-1 assembly is puzzling and represents a unique opportunity to tease out in detail what other processes were at work in its assembly.”

“Moreover, most planetary systems are thought to have begun in such resonances, but have experienced significant instabilities during their lifetimes before we observe them today.”

“Most planets would become unstable or collide with each other, and everything would be in chaos. For example, our solar system was affected by such instability.”

“But we know there are some systems that are more or less pristine specimens that have remained stable.”

“They effectively represent a record of its entire dynamical history, and we can try to reconstruct it. TRAPPIST-1 is one of them.”

The challenge then was to develop a model that could explain the orbits of the TRAPPIST-1 planets and how they got to their current configuration.

The resulting model suggests that the inner four planets evolved alone within the originally predicted 3:2 resonant chain.

As the disk's inner boundary expanded outward, the orbits loosened from the tighter 3:2 linkage into the configuration observed today.

The fourth planet was originally located on the inner boundary of the disk and moved outward with the disk, but was pushed back inward at a later stage when three more outer planets joined the planetary system.

“By observing TRAPPIST-1, we were able to test an exciting new hypothesis about the evolution of planetary systems,” said Dr Pichieri.

“TRAPPIST-1 is very interesting because it's a very complex, long chain of planets, and it's a great example for testing alternative theories about the formation of planetary systems.”

of Survey results Published in a journal Natural Astronomy.

_____

G. Pichieri othersDuring the recession of the inner edge of the disc, the TRAPPIST-1 system forms in two steps. Nat AstronPublished online August 20, 2024, doi: 10.1038/s41550-024-02342-4

Source: www.sci.news

Study Suggests Egypt’s Pyramid of Djoser Could Have Been Constructed Using an Innovative Hydraulic Lift System

The Pyramid of Djoser, also known as the Step Pyramid, is believed to be the oldest of the seven great pyramids, built around 4,500 years ago.



Map of the Saqqara Plateau showing the waterway from the Gisr el-Mudir Dam (left) to the water treatment plant near the Pyramid of Djoser. The water is then routed to the pyramid's network of pipes to power the hydraulic elevators. Image courtesy of Landreau. others., doi: 10.1371/journal.pone.0306690.

The Pyramid of Djoser, built around 2680 BC at Saqqara in Egypt, is considered a major milestone in monumental architecture.

This revealed for the first time two important innovations: the pyramidal shape of the pharaoh's tomb and the use of only perfectly finished stones in the masonry.

In fact, the ability to extract, lift and precisely stack millions of stones is also revolutionary.

Such were the complex and visible achievements of King Djoser that his architect, vizier and great priest of Ra, Imhotep, was deified during the New Kingdom.

In a new interdisciplinary analysis, Dr. Xavier Landreau of the CEA Palaeotechnical Institute and his colleagues have found that hydraulic lifts may have been used in the construction of the pyramid.

Based on their mapping of nearby watersheds, the authors found that one of Saqqara's large unexplained structures, the Gisr el-Mudir Enclosure, has the characteristics of a check dam intended to capture sediment and water.

Additionally, a series of compartments dug into the ground outside the pyramid may have acted as water treatment plants, allowing sediment to settle as water passed through each compartment.

This would have allowed the water to flow into the pyramid's columns themselves, and its upward force could have carried the building stones along.

More research is needed to understand how water flowed through the tunnels and how much water was present on the land at that point in Earth's history.

However, archaeologists suggest that while other building methods such as ramps may have been used to construct the pyramids, if there was enough water a hydraulic lift system may have been used to support the building process.

“The internal structure of the step pyramid is found to be consistent with a previously unreported mechanism for hydraulic build-up,” the researchers said.

“The ancient builders may have used sediment-free water from the south side of the dry moat to raise the stones from the center of the pyramid in a volcanic fashion.”

“The ancient Egyptians are famous for being pioneers and masters of hydraulics, including irrigation canals and barges for transporting megaliths.”

“This research opens up a new field of research into the use of water power to build the massive structures erected by the Pharaohs.”

of study Published online in the journal PLoS One.

_____

X. Landreau others2024. On the possibility of using hydropower to aid in the construction of the Step Pyramid at Saqqara. PLoS One 19 (8): e0306690; doi: 10.1371/journal.pone.0306690

Source: www.sci.news

Is it possible to embark on a space journey with the entire solar system?

Dead Planets Society is a podcast that explores wild ideas for manipulating the universe and tests their impact on the laws of physics, from splitting the moon to triggering doomsday events with gravitational waves. apple, Spotify Or visit our podcast page.

The thrilling adventure begins: In the season finale of Dead Planets Society, hosts Chelsea Whyte and Leah Crane propel Earth on a cosmic journey through our solar system.

Of course, sending Earth into space without its home planet would result in a dark, frigid voyage that would extinguish all life on Earth. And without anyone to witness the wonders of the universe, the journey would be meaningless. That’s why we need to bring the Sun along. The other planets are just a bonus.

Naturally, relocating the Sun is a monumental task, especially in terms of maintaining the orbits of the planets around it. This is where astrophysicists Jay Farihi and researchers from University College London come to the rescue in the episode.

One proposed solution is to construct a colossal warp drive, a self-contained space-time bubble that moves by distorting the space ahead of it. However, these theoretical devices are known for potentially enabling faster-than-light travel, and the key to keeping all planets tethered to the Sun is moving at a slow pace. Unfortunately, we have yet to figure out how to build such a device.

Another idea involves placing a black hole just ahead of the Sun to give it a slight boost – the black hole would then need to move along with the Sun, or alternatively, a series of black holes could traverse the Solar System in a cosmic relay race.

While these notions may seem far-fetched, there are more plausible concepts – though still improbable – such as deploying giant solar sails or inserting an unbreakable tube into the Sun to release high-pressure plasma jets.

The universe offers countless destinations that our hosts would love to explore with our now navigable solar system, ranging from star clusters to nebulae to supermassive black holes – all it requires is a few technological breakthroughs to make it a reality.

topic:

Source: www.newscientist.com

Minister issues apology for data breach in Northern Ireland special education system

The education secretary of Northern Ireland has issued a sincere apology after the personal information of over 400 individuals who volunteered to assist with a review of special needs education was accidentally leaked.

The breach was discovered when the Department of Education mistakenly sent a spreadsheet to 174 individuals, containing the names, email addresses, and job titles of 407 people interested in participating in the review of special educational needs events in Northern Ireland.

The spreadsheet included comments from several individuals.

The department has requested the 174 recipients to delete the information they received and has confirmed that this has been done.

Many affected individuals have reported their concerns to authorities regarding the data breach.

Education Secretary Paul Givhan stated, “The Department of Education takes data protection seriously and deeply regrets this incident. We apologize to all those impacted and have informed them about the breach.”

Givan has ordered an internal audit department to conduct a thorough investigation into the data leak to prevent such incidents in the future.

An initial report has been submitted to the Information Commissioner’s Office, and updates will be provided as the investigation progresses.

This data breach is not the first in Northern Ireland, as a similar incident occurred last year involving the Police Service of Northern Ireland.

Around 5,000 officers and staff from PSNI took legal action after personal details of approximately 9,500 employees were mistakenly disclosed in response to a Freedom of Information request.

The leaked information included employee last names, initials, ranks, grades, workplaces, and departments, and was later discovered to have reached dissident republicans.

Source: www.theguardian.com

Technology: Can AI truly be the solution to our ailing healthcare system?

circle
What if AI isn’t as great as we thought? What if its potential has been exaggerated to the point of being dangerous? Leading cancer experts in the NHS are raising concerns that the health service’s excessive focus on new technology is jeopardizing patient safety. As reported in our recent article:


Cancer experts warn that “innovative solutions” like new diagnostic tests are being falsely hailed as a “magic bullet” for the cancer crisis, but fail to address the root cause of cancer as a systemic issue.

The authors note that a common misconception among NHS leaders is that new technologies can eliminate inequalities, when in reality, technologies like AI can create additional hurdles for those with low digital and health literacy.

“We advise against adopting a technology-centric approach without a thorough evaluation of equity,” concludes the paper.

The Lancet Oncology publication argues for a back-to-basics strategy for cancer treatment. Their suggestions include increasing staff numbers, refocusing research on traditional areas such as surgery and radiation therapy, and establishing dedicated units for technology transfer to ensure proven treatments are integrated into routine care.

AI may divert attention from these critical improvements. While the technology holds much promise for the future, experts are concerned that hype about future advancements may detract from necessary present-day changes.

The paper describes AI as the latest iteration of “bionic duckweed,” a concept introduced by Stian Westlake in 2020 to highlight the use of future technologies to oppose current investments.
(Read More)

Source: www.theguardian.com

UK think tank calls for system to track misuse and failures in Artificial Intelligence

The report highlighted the importance of establishing a system in the UK to track instances of misuse or failure of artificial intelligence. Without such a system, ministers could be unaware of alarming incidents related to AI.

The Centre for Long Term Resilience (CLTR) suggested that the next government should implement a mechanism to record AI-related incidents in public services and possibly create a centralized hub to compile such incidents nationwide.

CLTR emphasized the need for incident reporting systems, similar to those used by the Air Accident Investigation Branch (AAIB), to effectively leverage AI technology.

According to a database compiled by the Organisation for Economic Cooperation and Development (OECD), there have been approximately 10,000 AI “safety incidents” reported by news outlets since 2014. These incidents encompass a wide range of harms, from physical to economic and psychological, as defined by the OECD.

The OECD’s AI Safety Incident Monitor also includes instances such as a deepfake of Labour leader Keir Starmer and incidents involving self-driving cars and a chatbot-influenced assassination plot.

Tommy Shafer-Shane, policy manager at CLTR and author of the report, noted the critical role incident reporting plays in managing risks in safety-critical sectors like aviation and healthcare. However, such reporting is currently lacking in the regulatory framework for AI in the UK.

CLTR urged the UK government to establish an accident reporting regime for AI, similar to those in aviation and healthcare, to address incidents that may not fall under existing regulatory oversight. Labour has promised to implement binding regulations for most AI incidents.

The think tank recommended the creation of a government system to report AI incidents in public services, identify gaps in AI incident reporting, and potentially establish a pilot AI incident database.

In a joint effort with other countries and the EU, the UK pledged to cooperate on AI security and monitor “AI Harm and Safety Incidents.”

CLTR stressed the importance of incident reporting to keep DSIT informed about emerging AI-related risks and urged the government to prioritize learning about such harms through established reporting processes.

Source: www.theguardian.com

What If the Earth Was the Center of the Solar System?

Dead Planets Society is a podcast that takes some crazy ideas for how to tinker with the universe and tests their effects against the laws of physics, from snapping the moon in half to causing doomsday events with gravitational waves. apple, Spotify Or check out our podcast page.

By the end of the 16th century, pretty much everyone knew that the Earth revolved around the Sun, not the other way around. This was a huge blow to those who thought the Earth was the center of the universe, but the Dead Planets Society is here to ease their disappointment. Yes, we're trying to revive geocentrism.

Putting Earth at the center of the solar system requires more than just fudging the math: The Sun is much more massive than our puny planet, so forcing it to orbit the Sun would be nearly impossible, so hosts Chelsea White and Leah Crane would have to make some major changes to the solar system as we know it.

In this episode, Andy Rivkin Researchers at Johns Hopkins University in Maryland say the only way to make Earth an Earth-centered solar system would be to make it the most massive thing around – which would have some strange effects, assuming it doesn't collapse the planet into a black hole.

First, the Moon would have to speed up to maintain its orbit, orbiting the Earth in an hour or so before it would break apart. If the remaining planets didn't speed up too, they would all crash into the new giant Earth within a decade or two. The Earth's extra mass could also disrupt other nearby stars, causing them to start attracting it to Earth. A victorious Earth-centered solar system might not last long, but it would certainly come to a dramatic end.

topic:

Source: www.newscientist.com

Is an aging NASA probe redefining the limits of our solar system?

NASA’s New Horizons spacecraft is hurtling out of our solar system at incredible speed. It’s currently about 8 billion kilometers from the Sun, and by the time you finish reading this article, it will be thousands of kilometers further into the frigid darkness. Space is lonely; even the giant planet Jupiter is just a tiny speck.

New Horizons is best known for getting the first proper glimpses of the dwarf planet Pluto in 2015, which it had previously only seen as a faint smudge. It also taught us a lot about the outer solar system and the tiny frozen worlds that float there. “It’s really been an Alice in Wonderland kind of story,” says Alan Stern, the mission’s principal investigator. “It’s been a magical experience, and we’ve made some amazing discoveries.”

But the dream isn’t over yet, because New Horizons may make a surprise final move. In early 2024, one of New Horizons’ detectors recorded an unexpected increase in the amount of dust it encountered. That material could have been created by collisions between rocky fragments, and astronomers now suspect that there may be many objects beyond the rubble-strewn Kuiper Belt, often considered the edge of the solar system. If so, the boundaries of the solar system would need to be redrawn, calling into question models of the formation of the solar system.

Stern and his colleagues are clearly hoping to take advantage of the rover’s unique location to learn more about this unexplored wilderness while they still can. “This is…

Source: www.newscientist.com

Astronomers find parallel jets and disks around nearby multiple star system

Astronomers Atacama Large Millimeter/Submillimeter Array (ALMA) Mid-infrared measuring instrument (mm) NASA/ESA/CSA James Webb Space Telescope A twin disk and parallel jets were discovered in the young star system WL20.

Barsoni othersTwin disks and jets erupting from a pair of young stars in WL20. Image credit: NSF / NRAO / B. Saxton / NASA / JPL-Caltech / Harvard-Smithsonian CfA.

WL20 It is located in the Rho Ophiuchus Molecular Cloud Complex, more than 400 light years from Earth.

“What we found was absolutely surprising,” said Dr Mary Barthony, lead author of the study.

“We've known about the WL20 system for some time, but what caught our attention was that one of the stars in the system appeared to be much younger than the others.”

“Using MIRI and ALMA together, we were able to see that this one star is actually two stars next to each other.”

“Each of these stars was surrounded by a disk, and each disk emitted a jet parallel to the others.”

ALMA and Webb's MIRI observe very different parts of the electromagnetic spectrum.

Used together, they allowed astronomers to discover these hidden twins in the stellar system's radio and infrared wavelengths: ALMA found the disk, and MIRI found the jet.

They analyzed archived ALMA data to reveal the composition of the disk, and MIRI data to reveal the chemical composition of the jet.

They also analyzed high-resolution images, revealing the size of the massive disk – about 100 times the distance between Earth and the Sun.

“Without MIRI we would never have known these jets even existed, which is amazing,” Dr Barthony said.

“ALMA's high-resolution observations of the disks surrounding the two newly observed stars reveal the structure of the disks.”

“Someone looking at this ALMA data and not knowing there are twin jets would think it's a big edge-on disk with a hole in the middle, rather than two edge-on disks and two jets. That's pretty remarkable.”

Combining multi-wavelength data from ALMA and Webb revealed the complex processes involved in the formation of several stellar systems.

“We plan to take advantage of ALMA's future upgrades, such as the broadband sensitivity upgrade, to continue unlocking the mysteries surrounding the birth of stars and planetary systems,” the researchers said.

They are, result in 244th Meeting of the American Astronomical Society In Madison, Wisconsin.

_____

Mary Barthony others2024. Twin jets and twin discs: JWST MIRI and ALMA discoveries in the young WL20 multiple star system. 224 AustraliaAbstract #253

Source: www.sci.news