Scientists may have finally caught their first glimpse of dark matter, a mysterious substance that makes up 27% of the universe's mass-energy budget. The discovery, made by Japanese astrophysicist Tomonori Totani, claims to provide direct evidence for the existence of this invisible entity.
Totani analyzed data from NASA's Fermi Gamma-ray Space Telescope and spotted a pattern of gamma rays that matched the shape of dark matter halos surrounding galaxies. If true, this finding would mark a major breakthrough in understanding one of the most enduring unsolved puzzles in astrophysics.
Dark matter was first proposed by Swiss astronomer Fritz Zwicky in the 1930s, after he observed that distant galaxies were spinning faster than their visible mass could account for. Since then, scientists have searched for dark matter particles using a variety of methods, including ground-based detectors and space-based telescopes, but so far have come up empty-handed.
One popular theory suggests that dark matter is composed of weakly interacting massive particles (wimps), which are heavier than protons but interact very little with normal matter. When two wimps collide, they can annihilate each other, releasing gamma rays in the process. Totani's discovery appears to be consistent with this prediction.
However, experts caution that more work is needed to confirm the finding and rule out alternative explanations for the signal. Justin Read, an astrophysicist at the University of Surrey, noted that similar signals have not been detected from other regions of space, such as dwarf galaxies. Kinwah Wu, a theoretical astrophysicist at UCL, urged caution, saying that while Totani's analysis is encouraging, it is still too early to declare a major breakthrough.
If Totani's finding is confirmed, it would have significant implications for our understanding of the universe and the nature of dark matter. The discovery of this elusive substance could finally help explain why galaxies rotate faster than they should, and potentially shed light on some of the biggest mysteries in modern astrophysics.
Totani analyzed data from NASA's Fermi Gamma-ray Space Telescope and spotted a pattern of gamma rays that matched the shape of dark matter halos surrounding galaxies. If true, this finding would mark a major breakthrough in understanding one of the most enduring unsolved puzzles in astrophysics.
Dark matter was first proposed by Swiss astronomer Fritz Zwicky in the 1930s, after he observed that distant galaxies were spinning faster than their visible mass could account for. Since then, scientists have searched for dark matter particles using a variety of methods, including ground-based detectors and space-based telescopes, but so far have come up empty-handed.
One popular theory suggests that dark matter is composed of weakly interacting massive particles (wimps), which are heavier than protons but interact very little with normal matter. When two wimps collide, they can annihilate each other, releasing gamma rays in the process. Totani's discovery appears to be consistent with this prediction.
However, experts caution that more work is needed to confirm the finding and rule out alternative explanations for the signal. Justin Read, an astrophysicist at the University of Surrey, noted that similar signals have not been detected from other regions of space, such as dwarf galaxies. Kinwah Wu, a theoretical astrophysicist at UCL, urged caution, saying that while Totani's analysis is encouraging, it is still too early to declare a major breakthrough.
If Totani's finding is confirmed, it would have significant implications for our understanding of the universe and the nature of dark matter. The discovery of this elusive substance could finally help explain why galaxies rotate faster than they should, and potentially shed light on some of the biggest mysteries in modern astrophysics.