Latest news with #ASKAP
New York Post
3 hours ago
- Science
- New York Post
Astronomers baffled by mystery object flashing signals at Earth every 44 minutes: ‘Like nothing we've ever seen'
The truth is out there. Astronomers say they're stunned by an unidentified object flashing strange signals from deep space. The object, named ASKAP J1832-0911, was detected by the Australian Square Kilometre Array Pathfinder (ASKAP) and NASA'S Chandra X-ray observatory — the world's most powerful X-ray telescope. 'It is unlike anything we have seen before,' Andy Wang, an astronomer at Curtin University in Perth, Australia, declared in a statement published this week. ASKAP J1832-0911 emits pulses of radio waves and X-rays for two minutes every 44 minutes, according to the experts, who documented their findings in Nature journal. An image of the sky showing the region around ASKAP J1832-0911. Ziteng Wang, ICRAR ASKAP J1832-0911 has been classified as a 'long-period transient' or 'LPT' — a cosmic body that emits radio pulses separated by a few minutes or a few hours. Wang and has team theorize that the object could be a dead star, but they don't know why it 'switches on' and 'switches off' at 'long, regular and unusual intervals,' reports. 'ASKAP J1831-0911 could be a magnetar (the core of a dead star with powerful magnetic fields), or it could be a pair of stars in a binary system where one of the two is a highly magnetised white dwarf (a low-mass star at the end of its evolution),' Wang wrote. 'However, even those theories do not fully explain what we are observing,' he added. 'This discovery could indicate a new type of physics or new models of stellar evolution.' Wang and his team hope to detect similar another using radio waves and the Chandra X-ray observatory, saying a subsequent discovery will help them learn more about the nature of such LPTs. An artist's illustration of NASA's Chandra X-ray Observatory in space. NASA/CXC & J. Vaughan, NASA/CXC & J. Vaughan It's not the only space discovery to hit headlines and spark conversation in recent weeks. Earlier this month, Cambridge University Press revealed that astronomers had detected a signal extracted from interstellar noise that could be a sign of active biology on another planet. 'Astronomers have detected the most promising signs yet of a possible biosignature outside the solar system, although they remain cautious,' a press release from the prestigious publisher read.
Indian Express
8 hours ago
- Science
- Indian Express
Scientists baffled by unknown space object that emits X-ray and radio waves every 44 minutes
Scientists have discovered a strange object in space, which they say behaves 'like no other seen before.' Located in the Milky Way, around 15,000 light years away from Earth, the mysterious object ASKAP J1832-0911 is sending pulses of radio waves and X-rays for two minutes straight every 44 minutes. First discovered by NASA's Chandra X-ray Observatory, ASKAP J1832-0911 belongs to a class of objects called 'long period radio transients' (also known as LPT), which emit intense radio waves over tens of minutes. NASA says that these waves are thousands of times longer than the length of repeated variations seen in pulsars, which are rapidly spinning neutron stars. According to team leader and Curtin University researcher Zieng (Andy) Wang, 'Discovering that ASKAP J1832-0911 was emitting X-rays felt like finding a needle in a haystack. The ASKAP radio telescope has a wide field view of the night sky, while Chandra observes only a fraction of it. So, it was fortunate that Chandra observed the same area of the night sky at the same time.' Discovered in 2022, LPTs are cosmic bodies that emit radio pulses every few minutes or hours. In the last few years, astronomers have come across 10 LPTs, but say that ASKAP J1832-0911 is unlike any other. Using Chandra, scientists have discovered that ASKAP J1832-0911 also emits 'regularly varying' X-rays every 44 minutes, making it the first long-period radio transient object to do so. As of now, there is no explanation as to how or why LPTs generate these signals and why they 'switch on' and 'switch off' at long, regular and irregular intervals. However, researchers believe that ASKAP J1832-0911 is a dead star, but don't know what type it is. Some say that it could be a magnetar, which is the core of a dead star, while others assume that it could be a pair of stars where one of the two is a highly magnetised dwarf.
Time of India
a day ago
- Science
- Time of India
Rare space object blasts X-rays and radio waves every 44 minutes
Astronomers have detected a rare space object that emits powerful bursts of energy in both radio and X-ray wavelengths every 44 minutes. The object, known as ASKAP J1832-0911 , lies around 15,000 light-years away in the Milky Way and is the first of its kind to show such behaviour across both ends of the electromagnetic spectrum. Long-period transients (LPTs) a recently identified class of cosmic bodies typically emit brief pulses of radio waves separated by hours or minutes. But until now, none had been observed producing X-ray emissions . ASKAP J1832-0911 has changed that, emitting energy levels far beyond anything previously recorded in this category. 'This object is unlike anything we have seen before,' said Dr Ziteng (Andy) Wang, lead author of the study and a researcher at Curtin University, part of the International Centre for Radio Astronomy Research (ICRAR). The findings were published this week in *Nature*. A lucky observation by Taboola by Taboola Sponsored Links Sponsored Links Promoted Links Promoted Links You May Like Giao dịch CFD với công nghệ và tốc độ tốt hơn IC Markets Đăng ký Undo ASKAP J1832-0911 was initially detected via radio signals by the Australian Square Kilometre Array Pathfinder (ASKAP), operated by CSIRO on Wajarri Yamaji Country. By sheer coincidence, NASA's Chandra X-ray Observatory happened to be surveying the same region of sky at the same time, enabling astronomers to match the radio pulses with bursts of X-ray radiation. 'Discovering that ASKAP J1832-0911 was emitting X-rays felt like finding a needle in a haystack,' said Dr Wang. 'The ASKAP telescope has a broad view of the sky, but Chandra focuses on a much smaller region, so the overlap was a matter of great fortune.' Since the first LPT was discovered in 2022, around ten more have been identified. But none has demonstrated behaviour as intense and regular as ASKAP J1832-0911. New Physics on the horizon? Astronomers suspect ASKAP J1832-0911 could be either an ageing magnetar a type of dead star with extremely strong magnetic fields or a binary system containing a magnetised white dwarf, the remnant of a low-mass star. 'ASKAP J1831-0911 could be a magnetar, or it could be a pair of stars in a binary system where one is a highly magnetised white dwarf,' Wang explained. 'However, even those theories do not fully explain what we are observing. This discovery could indicate a new type of physics or new models of stellar evolution.' A doorway to more discoveries According to Professor Nanda Rea from the Institute of Space Science (ICE-CSIC) and the Institute of Space Studies of Catalonia (IEEC), the discovery suggests ASKAP J1832-0911 may be the first of many similar objects. 'Finding one such object hints at the existence of many more,' Rea said. 'The discovery of its transient X-ray emission opens fresh insights into their mysterious nature.'
Yahoo
a day ago
- General
- Yahoo
'One of the most geometrically perfect': What is this mysterious sphere deep in the Milky Way galaxy?
When you buy through links on our articles, Future and its syndication partners may earn a commission. There's no shortage of round celestial objects in our universe. Planets, moons and stars all exhibit lovely spherical shapes. But astronomers recently spotted a mysteriously circular orb deep in the Milky Way galaxy — and it's certainly none of these things. This celestial bubble, discovered by astrophysicist Miroslav Filipović of Western Sydney University, is likely a supernova remnant (SNR), an expanding shell of gas and dust formed by shockwaves from a massive stellar explosion. SNRs aren't uncommon, but this particular example showcases numerous anomalies, including its astonishingly round shape. For that shape, Filipović and his team named SNR Teleios, the Greek word for "perfect." Filipović discovered Teleios — officially designated G305.4–2.2 — by accident, scanning through new images taken by the radio telescope Australian Square Kilometre Array Pathfinder (ASKAP). ASKAP is currently surveying the entire southern hemisphere sky. "I was looking at these images as they became available, searching for anything interesting, or not seen before, and came across Teleios," Filipović told "Its perfectly circular shape was unusual, and so I investigated further." Using data from ASKAP and the Murchison Widefield Array, Filipović and his team estimate that Teleios spans either about 46 light-years across at a distance of about 7,175 light-years from Earth, or about 157 light-years across at a distance of about 25,114 light-years from Earth. (Judging such vast distances in space is difficult.) Regardless of the size and distance of Teleios, though, the SNR's near-perfect symmetry is extraordinary. Its shape was quantified with a circularity score of 95.4%, placing it among the most symmetric known SNRs. While idealized models suggest SNRs remnants should be circular, reality often paints a more chaotic picture. "'Typical' SNR shapes vary dramatically, either from asymmetries in the initial explosion, or disruption from expanding into a non-perfect environment, or a number of other interfering factors," says Filipović. "What makes Teleios' shape so remarkable is that it displays none of these asymmetries; it effectively looks like an explosion that has happened with almost perfect initial parameters and with almost no disruption while expanding." So, what could explain such an undisturbed evolution? According to Filipović, it likely comes down to location. Teleios lies 2.2 degrees below the Galactic Plane, where interstellar gas and dust are significantly more sparse. This environment may have allowed the remnant to expand while remaining largely undisturbed for thousands of years. Teleios' shape is only one of the unusual characteristics of this SNR. Adding to the mystery, Teleios emits only in radio wavelengths, with a hint of hydrogen-alpha emissions. "Most SNRs are visible at another frequency. They either emit at optical, infrared, or X-ray frequencies as well," says Filipović. "The fact that we don't see that here is quite confusing. It could be that the temperatures are not high enough to produce this emission, or that Teleios is old enough that the optical emission has faded, but the radio emission is still present." Related Stories: — Hundreds of supernova remnants remain hidden in our galaxy. These astronomers want to find them— Mysterious cosmic lights turn out to be 2 undiscovered supernova remnants— Watch 2 gorgeous supernova remnants evolve over 20 years (timelapse video) This lack of emissions poses challenges to determining the type of supernova that produced Teleios. The most likely scenario is a Type Ia supernova, which occurs in binary star systems in which a white dwarf consumes enough mass of its companion star to explode violently. Alternatively, Teleios' origin might be Type Iax supernova, which is similar to a Type Ia supernova but one that leaves behind a "zombie" star. But Teleios's observable data doesn't fit either model perfectly. As it goes with newfound objects in the universe, researchers have a lot more to study to unravel all of Teleios's mysteries. Fortunately, there's no better time to study SNRs. "These are the 'golden days' for radio astronomy as the new instruments, such as ASKAP and MeerKAT, are opening windows for new discoveries," says Filipović. A paper on the findings has been submitted to the Publications of the Astronomical Society of Australia, and is presently available on preprint server arXiv.
Daily Maverick
a day ago
- Science
- Daily Maverick
X-rays have revealed a mysterious cosmic object never before seen in our galaxy
After the initial discovery, we began follow-up observations using telescopes around the world, hoping to catch more pulses. With continued monitoring, we found the radio pulses from ASKAPJ1832 arrive regularly — every 44 minutes. This confirmed it as a new member of the rare long-period transient group. In a new study published today in Nature, we report the discovery of a new long-period transient — and, for the first time, one that also emits regular bursts of X-rays. Long-period transients are a recently identified class of cosmic objects that emit bright flashes of radio waves every few minutes to several hours. This is much longer than the rapid pulses we typically detect from dead stars such as pulsars. What these objects are, and how they generate their unusual signals, remains a mystery. Our discovery opens up a new window into the study of these puzzling sources. But it also deepens the mystery: the object we found doesn't resemble any known type of star or system in our galaxy – or beyond. Watching the radio sky for flickers There's much in the night sky that we can't see with human eyes but can detect when we look at other wavelengths, such as radio emissions. Our research team regularly scans the radio sky using the Australian SKA Pathfinder (ASKAP), operated by CSIRO on Wajarri Yamaji Country in Western Australia. Our goal is to find cosmic objects that appear and disappear (known as transients). Transients are often linked to some of the most powerful and dramatic events in the universe, such as the explosive deaths of stars. In late 2023, we spotted an extremely bright source, named ASKAP J1832-0911 (based on its position in the sky), in the direction of the galactic plane. This object is located about 15,000 light years away. This is far, but still within the Milky Way. A dramatic event After the initial discovery, we began follow-up observations using telescopes around the world, hoping to catch more pulses. With continued monitoring, we found the radio pulses from ASKAPJ1832 arrive regularly — every 44 minutes. This confirmed it as a new member of the rare long-period transient group. But we did not just look forward in time — we also looked back. We searched through older telescope data from the same part of the sky. We found no trace of the object before the discovery. This suggests something dramatic happened shortly before we first detected it — something powerful enough to suddenly switch the object 'on'. Then, in February 2024, ASKAPJ1832 became extremely active. After a quieter period in January, the source brightened dramatically. Fewer than 30 objects in the sky have ever reached such brightness in radio waves. For comparison, most stars we detect in radio are about 10,000 times fainter than ASKAPJ1832 during that flare-up. A lucky break X-rays are a form of light that we can't see with our eyes. They usually come from extremely hot and energetic environments. Although about 10 similar radio-emitting objects have been found so far, none had ever shown X-ray signals. In March, we tried to observe ASKAPJ1832 in X-rays. However, due to technical issues with the telescope, the observation could not go ahead. Then came a stroke of luck. In June, I reached out to my friend Tong Bao, a postdoctoral researcher at the Italian National Institute for Astrophysics, to check if any previous X-ray observations had captured the source. To our surprise, we found two past observations from NASA's Chandra X-ray Observatory, although the data were still under a proprietary period (not yet public). We contacted Kaya Mori, a research scientist at Columbia University and the principal investigator of those observations. He generously shared the data with us. To our amazement, we discovered clear X-ray signals coming from ASKAPJ1832. Even more remarkable: the X-rays followed the same 44-minute cycle as the radio pulses. It was a truly lucky break. Chandra had been pointed at a different target entirely, but by pure coincidence, it caught ASKAPJ1832 during its unusually bright and active phase. A chance alignment like that is incredibly rare — like finding a needle in a cosmic haystack. Still a mystery Having both radio and X-ray bursts is a common trait of dead stars with extremely strong magnetic fields, such as neutron stars (high-mass dead stars) and white dwarfs (low-mass dead stars). Our discovery suggests that at least some long-period transients may come from these kinds of stellar remnants. But ASKAPJ1832 does not quite fit into any known category of object in our galaxy. Its behaviour, while similar in some ways, still breaks the mould. We need more observations to truly understand what is going on. It is possible that ASKAPJ1832 is something entirely new, or it could be emitting radio waves in a way we have never seen before. DM
