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A New Research into Darkish Matter within the Bullet Cluster May Disprove its Existence

July 4, 2026
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A New Research into Darkish Matter within the Bullet Cluster May Disprove its Existence
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Darkish Matter (DM), that mysterious matter that accounts for 85% of the Universe’s mass, continues to fascinate and puzzle scientists. Whereas we’re unable to resolve it in seen mild, its affect could be seen within the rotational curves of galaxies, Darkish Matter halos, and the gravitational lenses they trigger. The Bullet Cluster, consisting of two colliding galaxy clusters situated about 3.7 billion light-years from Earth, is of specific curiosity to astronomers looking for DM. The reason is that gravitational lensing research are claimed to supply sturdy proof for its existence.

When analyzing the Bullet Cluster, scientists famous that galaxies situated past it appeared distorted, the results of the cluster’s gravity warping spacetime round it.
Utilizing the James Webb Space Telescope (JWST), a global workforce of researchers analyzed new knowledge and current photographs to achieve new perception into this cluster. In accordance with their analysis, there may be an alternate rationalization for the noticed results of the cluster that doesn’t contain DM in any respect. Their findings may pressure astronomers to reevaluate what was thought-about to be a few of the most compelling proof for DM.

The collision that created the Bullet Cluster occurred round 4 billion years in the past, when two clusters containing a whole bunch of galaxies collided at speeds of over 2,500 km/s (1,550 mps). Whereas galaxy clusters include stars within the trillions, nearly all of their seen matter consists of gasoline situated between star programs – aka. the interstellar medium (ISM). In the course of the collision, the 2 gasoline clouds skilled frictional forces as they handed by means of one another, inflicting them to each warmth up and decelerate. These gasoline clouds are seen right now as diffuse patches that glow brightly within 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 *Picture from the James Webb Area Telescope of the inside area of the Bullet Cluster. © Picture: NASA/ESA/CSA/STScI/CXC/Caltech/IPAC*

Nevertheless, the galaxies within the two clusters handed by means of one another with out incident, because the distance between people stars was so nice that they have been in a position to fly previous one another. In consequence, the 2 clusters have been separated from the interstellar gasoline they carried with them. Within the Webb picture (proven above), the new gasoline clouds seem in pink, whereas the distribution of darkish matter seems in blue. Cluster 1 is seen to the left of the left-most gasoline cloud, whereas Cluster 2 is simply to the best of the best one. These 4 buildings type everything of the Bullet Cluster.

One other factor that’s clear from the picture is how galaxies past the cluster seem distorted and crescent-shaped. Surprisingly, the galaxy clusters present the strongest lensing impact, regardless of their comparatively low mass. In the meantime, the 2 luminous clouds, the place the best mass must be concentrated, present a relatively weak impact. This implies that there’s extra matter hidden in these galaxies that astronomers can’t detect.

In accordance with present theories, DM interacts with regular matter solely by means of gravity, and never by means of the opposite basic forces (electromagnetism, the weak and robust nuclear forces). Due to this, it’s not slowed down by friction and wouldn’t be separated from the galaxy clusters. The info additionally helps one other interpretation: Modified Newtonian Dynamics (MOND), the cosmological mannequin that does away with DM solely. To at the present time, MOND has been thought-about one thing of a fringe idea as a result of it can’t clarify phenomena such because the Bullet Cluster.

“Nevertheless, we present in our examine that, quite the opposite, the Bullet Cluster is definitely significantly in keeping with the MOND situation,” stated HISKP researcher Dong Zhang, the lead writer and the one who carried out a big proportion of the calculations. “If large stars finally fritter away, they turn out to be neutron stars or black holes. Like darkish matter, each are invisible and may solely be detected by the large 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) Artist’s impression of “ghost galaxies” inside the Milky Approach’s Darkish Matter Halo. Credit score: NASA, ESA, and T. Brown and J. Tumlinson (STScI)

As HISKP Professor Pavel Kroupa, a co-author on the examine, added:

This remark has to date been thought-about proof of the existence of darkish matter. The remnants of large stars tackle the function of darkish matter to a sure extent within the MOND situation. Even in the usual mannequin, which assumes the existence of darkish matter, its postulated amount must be considerably decreased – by round half.

Moreover, new knowledge from Webb have enabled extra exact calculations of the variety of stars and heavy parts in each clusters. Dr. Indranil Banik of the Institute of Cosmology and Gravitation on the College of Portsmouth (one other co-author) confirmed that the newly calculated numbers of stars and different objects can account for the noticed gravitational lensing impact. This new knowledge and perception into the Bullet Cluster have solid doubt on a key piece of proof for DM and made for a extra compelling case for MOND.

Additional Studying: Universität Bonn, Physics Review D



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