The most powerful explosions in the universe are caused by the births of black holes rather than dense neutron stars called magnetars, new evidence confirms.
Gamma-ray bursts are blasts of high-energy radiation that arrive at Earth from all directions.
Bursts lasting longer than 2 seconds are thought to be related to the collapse of massive stars that fire out jets of matter at near light speed, emitting copious radiation in the process. When the jets happen to be pointed at Earth, they send a volley of gamma rays our way.
But exactly how these jets are generated is still unclear. If the star collapses to form a rapidly spinning neutron star with a powerful magnetic field, called a magnetar, it could violently stir up matter around it to produce jets.
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Alternatively, if the star collapses to form a black hole, the jets might arise from the interaction of the black hole with matter spiralling into it. Either way, the tremendous rotational energy of the black hole or neutron star is thought to power the jets.
One way to distinguish between the two possibilities is to measure the total energy of the blast. The energy of a rotating object depends on its mass, and there is a limit to how heavy neutron stars can get before they collapse to black holes. There is no limit on the mass of black holes, however, so they could provide more energy than neutron stars.
Now, of the University of California, Berkeley, and colleagues have analysed four of the most powerful gamma-ray bursts detected by NASA’s Fermi Gamma-ray Space Telescope.
“These are among the most energetic GRBs ever seen,” says team member Alex Filippenko, also of the University of California, Berkeley.
The most poweful of the bursts, called GRB 090926A, released about 1.4 x 1052 ergs in jets. Neutron stars should be able to produce no more than 3 x 1052 ergs, with only a fraction of their energy going into jets. So the researchers argue that this burst, along with the three others, must be due to black holes instead.
of the University of California, Santa Cruz, says this is an “exciting result” for pinning down the source of the most powerful gamma-ray bursts. But he adds: “This does not mean that magnetars don’t make some or even most GRBs – only that they have difficulty producing the most energetic.”
The researchers reported their findings on Wednesday at a in Annapolis, Maryland.
![Astronomers have long known that understanding how star clusters come to be is key to unlocking other secrets of galactic evolution. Stars form in clusters, created when clouds of gas collapse under gravity. As more and more stars are born in a collapsing cloud, strong stellar winds, harsh ultraviolet radiation and the supernova explosions of massive stars eventually disperse the cloud, and their light can bear down on other star-forming regions in the galaxy. This process is called stellar feedback, and it means that most of the gas in a galaxy never gets used for star formation. Researching how star clusters develop can answer questions about star formation at a galactic scale. Now, the state of the art has been further developed with both Hubble and Webb working together to provide a broad-spectrum view of thousands of young star clusters. An international team of astronomers has pored over images of four nearby galaxies from the FEAST observing programme (#1783), trying to solve this mystery. Their results show that it is the most massive star clusters that clear away their gaseous shroud the fastest, and begin lighting their galaxy the earliest. The team identified nearly 9000 star clusters in the four galaxies in different evolutionary stages: young clusters just starting to emerge from their natal clouds of gas, clusters that had partially dispersed the gas (both from Webb images), and fully unobstructed clusters visible in optical light (found in Hubble images). With Webb???s ability to peer inside the gas clouds, they were able to then estimate the mass and age of each cluster from its light spectrum. This image shows a section of one of the spiral arms of Messier 51 (M51), one of the four galaxies studied in this work, as seen by Webb???s Near-Infrared Camera (NIRCam). The thick clumps of star-forming gas are shown here in red and orange, representing infrared light emitted by ionised gas, dust grains, and complex molecules such as polycyclic aromatic hydrocarbons (PAHs). Within these gas complexes, each tens or hundreds of light years across, Webb reveals the dense, extremely bright clusters of massive stars that have just recently formed. The countless stars strewn across the arm of the galaxy, many of which would be invisible to our eyes behind layers of dust, are also laid bare in infrared light. [Image description: A large, long portion of one of the spiral arms in galaxy M51. Red-orange, clumpy filaments of gas and dust that stretch in a chain from left to right comprise the arm. Shining cyan bubbles light up parts of the gas clouds from within, and gaps expose bright star clusters in these bubbles as glowing white dots. The whole image is dotted with small stars. A faint blue glow around the arm colours the otherwise dark background.]](https://images.newscientist.com/wp-content/uploads/2026/05/13114322/SEI_296271016.jpg)


