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A New Study into Dark Matter in the Bullet Cluster Could Disprove its Existence
Dark Matter (DM), that mysterious matter that accounts for 85% of the Universe’s mass, continues to fascinate and puzzle scientists. While we are unable to resolve it in visible light, its influence can be seen in the rotational curves of galaxies, Dark Matter halos, and the gravitational lenses they cause. The Bullet Cluster, consisting of two colliding galaxy clusters located about 3.7 billion light-years from Earth, is of particular interest to astronomers searching for DM. The reason being that gravitational lensing studies are claimed to provide strong evidence for its existence.
When examining the Bullet Cluster, scientists noted that galaxies located beyond it appeared distorted, the result of the cluster’s gravity warping spacetime around it.
Using the James Webb Space Telescope (JWST), an international team of researchers analyzed new data and existing images to gain new insight into this cluster. According to their analysis, there is an alternative explanation for the observed effects of the cluster that does not involve DM at all. Their findings could force astronomers to reevaluate what was considered to be some of the most compelling evidence for DM.
The collision that created the Bullet Cluster occurred around 4 billion years ago, when two clusters containing hundreds of galaxies collided at speeds of over 2,500 km/s (1,550 mps). While galaxy clusters contain stars in the trillions, the majority of their visible matter consists of gas located between star systems – aka. the interstellar medium (ISM). During the collision, the two gas clouds experienced frictional forces as they passed through each other, causing them to both heat up and slow down. These gas clouds are visible today as diffuse patches that glow brightly in the X-ray spectrum.
*Image from the James Webb Space Telescope of the inner region of the Bullet Cluster. © Image: NASA/ESA/CSA/STScI/CXC/Caltech/IPAC*
However, the galaxies in the two clusters passed through each other without incident, since the distance between individuals stars was so great that they were able to fly past each other. As a result, the two clusters were separated from the interstellar gas they carried with them. In the Webb image (shown above), the hot gas clouds appear in pink, while the distribution of dark matter appears in blue. Cluster 1 is visible to the left of the left-most gas cloud, while Cluster 2 is just to the right of the right one. These four structures form the entirety of the Bullet Cluster.
Another thing that is clear from the image is how galaxies beyond the cluster appear distorted and crescent-shaped. Strangely, the galaxy clusters show the strongest lensing effect, despite their relatively low mass. Meanwhile, the two luminous clouds, where the greatest mass should be concentrated, show a comparatively weak effect. This suggests that there is additional matter hidden in these galaxies that astronomers cannot detect.
According to current theories, DM interacts with normal matter only through gravity, and not through the other fundamental forces (electromagnetism, the weak and strong nuclear forces). Because of this, it is not slowed down by friction and would not be separated from the galaxy clusters. The data also supports another interpretation: Modified Newtonian Dynamics (MOND), the cosmological model that does away with DM entirely. To this day, MOND has been considered something of a fringe theory because it cannot explain phenomena such as the Bullet Cluster.
“However, we show in our study that, on the contrary, the Bullet Cluster is actually particularly consistent with the MOND scenario,” said HISKP researcher Dong Zhang, the lead author and the one who carried out a large proportion of the calculations. “If massive stars eventually burn up, they become neutron stars or black holes. Like dark matter, both are invisible and can only be detected by the huge gravitational forces that they exert.”
Artist’s impression of “ghost galaxies” within the Milky Way’s Dark Matter Halo. Credit: NASA, ESA, and T. Brown and J. Tumlinson (STScI)
As HISKP Professor Pavel Kroupa, a co-author on the study, added:
This observation has so far been considered evidence of the existence of dark matter. The remnants of massive stars take on the role of dark matter to a certain extent in the MOND scenario. Even in the standard model, which assumes the existence of dark matter, its postulated quantity would have to be significantly reduced – by around half.
Additionally, new data from Webb have enabled more precise calculations of the number of stars and heavy elements in both clusters. Dr. Indranil Banik of the Institute of Cosmology and Gravitation at the University of Portsmouth (another co-author) showed that the newly calculated numbers of stars and other objects can account for the observed gravitational lensing effect. This new data and insight into the Bullet Cluster have cast doubt on a key piece of evidence for DM and made for a more compelling case for MOND.
Further Reading: Universität Bonn, Physics Review D
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Two Million X-Ray Sources, and One Cluster That Doesn’t Fit
Clusters are the largest gravitationally bound things in the universe, thousands of galaxies held together in a vast reservoir of hot gas, gas so hot it glows in X-rays rather than visible light. But they do not stop at a tidy, neat edge. They taper away into the surrounding darkness, and they are still being fed, drawing in fresh material along enormous threads of gas that run between them like the strands of a web. Those outskirts are the interesting part, because they are where the universe is still assembling itself. They are also very faint, which is why so little is known about them.
The eROSITA telescope, launched in 2019 aboard the joint Russian and German Spektrum-RG mission, has now published its second major data release. Built from three complete surveys of the sky, DR2 contains close to two million X-ray sources across the western half of the sky, about twice as many as the first release. Roughly 1.9 million are point like, mostly stars and feeding supermassive black holes. Some 64,000 are extended: galaxy clusters, nearby galaxies and the shredded remains of supernovae.

Galaxy cluster A3266 in X-rays, linked by a filament of hot gas to a neighbouring galaxy group. The Bonn team measured the faint outer glow for the first time and found gas hotter and denser than the models predict (Credit : Jakob Dietl/Uni Bonn/eROSITA-DE)
Within that haul, Thomas Reiprich and Jakob Dietl at Bonn’s Argelander Institute went after a single object. A3266 is a massive cluster connected by a filament of gas to a neighbouring group of galaxies, and their team became the first to measure the faint X-ray glow in its outer reaches.
Our current theories of how cosmic structure formed match what eROSITA sees, that’s reassuring. The interesting news is in the detail, where they don’t quite match. The gas in the outskirts and in the filament runs hotter and denser than predicted, and contains comparatively little in the way of heavy elements.

The Perseus cluster, one of the brightest X-ray objects in the sky. The diffuse glow is gas hot enough to shine in X-rays, and it holds more mass than all the cluster’s stars together (Credit : X-ray: NASA/CXC/SAO/V. Olivares et al.; Optical/IR: DSS; H-alpha: CFHT/SITELLE; Image Processing: NASA/CXC/SAO/N. Wolk)
Heavy elements, anything past hydrogen and helium, are manufactured inside stars and flung out when those stars die. Gas that is short of them has therefore never spent much time near a galaxy, which marks it as relatively pristine material arriving from the wider cosmic web rather than something expelled from the cluster itself. Yet it’s warmer and denser than models predict for gas of that kind. The two facts pull against each other, and reconciling them means adjusting our picture of how matter actually falls into a cluster: how quickly it heats, how thoroughly it mixes with what is already there and how much enriched gas the galaxies push back out to meet it.
Before eROSITA, the only X-ray survey of the whole sky came from ROSAT in 1990, so astronomers waited the best part of three decades for a successor. And eROSITA itself has been in safe mode since February 2022, with no return to science operations. There is a lesson in that about the value of surveying everything, whether or not you know yet what you are looking for.
Source : Homing In on the X-Ray Sky
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L.A. reaches deal on cost recovery for 2028 Olympics, amid warnings

A divided Los Angeles City Council finalized a deal with organizers of the 2028 Summer Olympic Games aimed at controlling the city’s costs during the global event, amid complaints that the protections don’t go far enough.
On a 10-4 vote, the council approved the Enhanced City Resources Master Agreement, which lays out the process for the city to seek reimbursement for the services it provides during the Games.
City Administrative Officer Matt Szabo said the agreement sets up additional financial safeguards, by allowing the city to tap a $270-million contingency fund set up by LA28, the privately run Olympic organizing committee, if outstanding costs remain.
Still, some on the council warned that taxpayers could wind up on the hook for $1 billion in police and other public safety costs if LA28 incurs serious losses.
“This fails to provide any safeguards for Los Angeles taxpayers and most assuredly risks the city’s fiscal stability,” Councilmember Monica Rodriguez said after voting against the agreement. Councilmembers Eunisses Hernandez, Ysabel Jurado and Nithya Raman, who is running against Mayor Karen Bass, also were opposed.
Critics of the Games have long voiced concern about the risks that surround the event.
If LA28 incurs massive financial losses, the city would cover the first $270 million. The state would absorb the next $270 million. After that, the city’s general fund, which pays for basic services, would cover any remaining shortfall.
The city’s negotiating team said L.A.’s political leaders committed the city roughly a decade ago to serve as a financial backstop for the Games, as part of the contract that made L.A. the host city.
“We are providing you today as many protections as we can, given the reality that if it is not financially successful, it does fall onto us,” Szabo said. “So there is nothing we could propose today or tomorrow or next year that would eliminate that risk.”
The council, in a flurry of votes, sidelined proposals from Councilmembers Imelda Padilla, Hernandez and Raman that were billed as a way to reduce the risk facing the city.
LA28 spokesperson Jacie Prieto Lopez, in a statement, said the newly approved agreement delivers on the committee’s commitment to “execute a safe, secure and fiscally responsible Games that benefit Los Angeles for decades to come.”
Under the terms approved by the council, LA28 would pay the city ahead of the Games for services that are ineligible for reimbursement from the federal government, such as street sweeping and deployment of traffic officers.
The terms around police protection are more complicated.
The city would first seek reimbursement from the federal government for law enforcement services, particularly in high-security zones, Szabo said. If the government fails to cover the cost of security in those areas, the city would seek all or a portion of LA28’s contingency funds to make up difference, he said.
Last year, President Trump signed the One Big Beautiful Bill Act, setting aside $1 billion for state and local governments for security, planning and other costs associated with the Games.
Some council members have voiced concerns that the federal government might not follow through on its commitment, or that only a fraction of those funds would make their way to L.A., one of several Southern California communities slated to host Olympic competitions.
In April, Rodriguez sent LA28 a letter warning the city’s public safety costs could easily blow past $1 billion if there is an emergency or major weather event.
City Controller Kenneth Mejia, in an interview, said he intends to use his office to look into LA28’s finances in the run-up to the Games. He also argued that the deal to secure the Olympics was a bad one from the beginning.
“We’re already locked into a huge financial liability. This was one of our big chances to throw in protections for the city and also provide that transparency,” said Mejia, who opposed the agreement.
If LA28 makes money on the Games, the organizing committee would be barred from distributing that surplus to any organization until it has covered its financial obligations to the city, according to the terms approved Wednesday by the council.
Szabo, appearing before the council, acknowledged that the city faces a financial risk. If LA28 does experience a financial loss, it first would tap its own $330-million contingency fund, he said.
After that, LA28 and the city would have access to a second, $270-million contingency fund set up to protect taxpayers, he said.
“Is that a likely scenario? We don’t believe so,” Szabo said. “Their reports thus far have suggested that they are meeting their targets on their sponsorships and on other revenues, and we want them to continue to hit their targets.”
Those arguments haven’t satisfied an array of activists, who urged the council to rewrite the agreement.
“LA28 has no incentive to keep the city from being forced into bankruptcy,” said Chris Tyler, spokesperson for Strategic Actions for a Just Economy, a nonprofit that advocates for low-income communities in L.A.
Under a deal reached in 2021, LA28 must reimburse the city for services that go beyond what would be provided on a normal day in key parts of the city, such as Exposition Park, the Sepulveda Basin and parts of downtown L.A.
The organizing committee is obligated to create a $270-million contingency fund that can be distributed as a surplus if the Games make money or cover any losses in the event of a shortfall.
The proposal approved Wednesday calls for the five-year-old agreement to be amended to ensure that those contingency funds can be used to cover the city’s costs in the event that other funds aren’t available.
The city and LA28 were supposed to have a draft agreement on the cost recovery process completed by October. A draft document did not surface until June.
City negotiators now head into another round of talks with LA28 on the precise level of services needed at the Convention Center, Venice Beach, Dodger Stadium and other locations. Those venue agreements must be completed in July 2027.
Under the terms approved Wednesday, the two sides must reach an accord on the cost of those additional services by October 2027.
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