Astronomers spot galaxy shaped like the Milky Way but much bigger
Astronomers have observed a galaxy dating to an earlier epoch in the universe's history that surprisingly is shaped much like our Milky Way - a spiral structure with a straight bar of stars and gas running through its centre- but much bigger, offering new insight into galactic formation.
The distant galaxy, called J0107a, was observed as it appeared 11.1-billion years ago, when the universe was about a fifth of its age today. The researchers used data from the Chile-based Atacama Large Millimeter/submillimeter Array (Alma) and Nasa's James Webb Space Telescope to study the galaxy.
They determined the galaxy's mass, including its stars and gas, was more than 10 times greater than that of the Milky Way, and it was forming stars at an annual rate about 300 times greater. J0107a was, however, more compact than the Milky Way.
"The galaxy is a monster galaxy with a high star formation rate and plenty of gas, much more than present day galaxies," said astronomer Shuo Huang of the National Astronomical Observatory of Japan, lead author of the study published this week in the journal Nature.
"The discovery," said study co-author Toshiki Saito, an astronomer at Shizuoka University in Japan, "raises the important question: How did such a massive galaxy form in such an early universe"?
While a few galaxies undergoing star formation at a similar rate to J0107a exist in today's universe, almost all are in the process of a galactic merger or collision. There was no sign of such circumstances involving this galaxy.
J0107a and the Milky Way have some commonalities.
Hashtags

Try Our AI Features
Explore what Daily8 AI can do for you:
Comments
No comments yet...
Related Articles


Daily Maverick
5 hours ago
- 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


Eyewitness News
5 hours ago
- Eyewitness News
The hunt for mysterious 'Planet Nine' offers up a surprise
PARIS - It's an evocative idea that has long bedevilled scientists: a huge and mysterious planet is lurking in the darkness at the edge of our solar system, evading all our efforts to spot it. Some astronomers say the strange, clustered orbits of icy rocks beyond Neptune indicate that something big is out there, which they have dubbed Planet Nine. Now, a US-based trio hunting this elusive world has instead stumbled on what appears to be a new dwarf planet in the solar system's outer reaches. And the existence of this new kid on the block could challenge the Planet Nine theory, the researchers have calculated. Named 2017 OF201, the new object is roughly 700 kilometres (430 miles) across according to a preprint study, which has not been peer-reviewed, published online last week. That makes it three times smaller than Pluto. But that is still big enough to be considered a dwarf planet, lead study author Sihao Cheng of New Jersey's Institute for Advanced Study told AFP. - Distant traveller - The object is currently three times farther away from Earth than Neptune. And its extremely elongated orbit swings out more than 1,600 times the distance between the Earth and the Sun, taking it into the ring of icy rocks around the solar system called the Oort cloud. It goes so far out, it could have passed by stars other than our Sun in the past, Cheng said. During its 25,000-year orbit, the object is only close enough to Earth to be observed around 0.5 percent of the time, which is roughly a century. "It's already getting fainter and fainter," Cheng said. The discovery suggests "there are many hundreds of similar things on similar orbits" in the Kuiper Belt beyond Neptune, Cheng said. After taking a risk spending more than half a year sorting through a difficult dataset in search of Planet Nine, Cheng said he was "lucky" to have found anything at all. The researchers are requesting time to point the James Webb, Hubble and ALMA telescopes at their discovery. But Sam Deen, a 23-year-old amateur astronomer from California, has already been able to track the dwarf planet candidate through old datasets. "OF201 is, in my opinion, probably one of the most interesting discoveries in the outer solar system in the last decade," Deen told AFP. - What about Planet Nine? - The icy rocks discovered in the Kuiper belt tend to have a clustered orbit going in a particular direction. Two decades ago, astronomers proposed this was due to the gravitational pull of a world up to 10 times larger than Earth, naming it Planet Nine and kicking off a debate that has rumbled since. It is also sometimes called Planet X, a name proposed for a hypothetical world beyond Neptune more than a century ago. Back in 1930, astronomers were searching for Planet X when they discovered Pluto, which became our solar system's ninth planet. But Pluto turned out to be too tiny -- it is smaller than the Moon -- and was demoted to dwarf planet status in 2006. There are now four other officially recognised dwarf planets, and Cheng believes 2017 OF201 could join their ranks. When the researchers modelled its orbit, they found it did not follow the clustered trend of similar objects. This could pose a problem for the Planet Nine theory, but Cheng emphasised more data is needed. Samantha Lawler of Canada's University of Regina told AFP that this "great discovery" and others like it mean that "the original argument for Planet Nine is getting weaker and weaker". The Vera Rubin Observatory, which is scheduled to go online in Chile this year, is expected to shed light on this mystery, one way or another. Deen said it was discouraging that no sign of Planet Nine has been found so far, but with Vera Rubin "on the horizon I don't think we'll have to wonder about its existence for much longer". For Cheng, he still hopes that this huge planet is out there somewhere. "We're in an era when big telescopes can see almost to the edge of the universe," he said. But what is in our "backyard" still largely remains unknown, he added.


Daily Maverick
7 hours ago
- Daily Maverick
Musk aiming to send uncrewed Starship to Mars by end of 2026
Musk presented a detailed Starship development timeline in a video posted online by his Los Angeles area-based rocket company, SpaceX, a day after saying he was departing the administration of U.S. President Donald Trump as head of a tumultuous campaign to slash government bureaucracy. The billionaire entrepreneur had said earlier that he was planning to scale back his role in government to focus greater attention on his various businesses, including SpaceX and electric car and battery maker Tesla Inc TSLA.O. Musk acknowledged that his latest timeline for reaching Mars hinged on whether Starship can accomplish a number of challenging technical feats during its flight-test development, particularly a post-launch refueling maneuver in Earth orbit. The end of 2026 would coincide with a slim window that occurs once every two years when Mars and Earth align around the sun for the closest trip between the two planets, which would take seven to nine months to transit by spacecraft. Musk gave his company a 50-50 chance of meeting that deadline. If Starship were not ready by that time, SpaceX would wait another two years before trying again, Musk suggested in the video. The first flight to Mars would carry a simulated crew consisting of one or more robots of the Tesla-built humanoid Optimus design, with the first human crews following in the second or third landings. Musk said he envisioned eventually launching 1,000 to 2,000 ships to Mars every two years to quickly establish a self-sustaining permanent human settlement. NASA is currently aiming to return humans to the surface of the moon aboard Starship as early as 2027 – more than 50 years after its last manned lunar landings of the Apollo era – as a stepping stone toward ultimately launching astronauts to Mars sometime in the 2030s. Musk, who has advocated for a more Mars-focused human spaceflight program, has previously said he was aiming to send an unmanned SpaceX vehicle to the red planet as early as 2018 and was targeting 2024 to launch a first crewed mission there. The SpaceX founder was scheduled to deliver a livestream presentation billed as 'The Road to Making Life Multiplanetary' from the company's Starbase, Texas, launch site on Tuesday night, following a ninth test flight of Starship that evening. But the webcast was canceled without notice after Starship spun out of control and disintegrated in a fireball about 30 minutes after launch and roughly halfway through its flight path without achieving some of its most important test goals. Two preceding test flights in January and March failed in more spectacular fashion, with the spacecraft blowing to pieces on ascent moments after liftoff, raining debris over parts of the Caribbean and forcing scores of commercial jetliners to change course as a precaution. Musk shrugged off the latest mishap on Tuesday with a brief post on X, saying it produced a lot of 'good data to review' and promising a faster launch 'cadence' for the next several test flights.