Scientists have created the highest resolution map of the dark matter that threads through the universe—showing its influence on the formation of stars, galaxies and planets.
The research, including astronomers from Durham University, UK, tells us more about how this invisible substance helped pull ordinary matter into galaxies like the Milky Way and planets like Earth.
The findings, using new data from NASA’s James Webb Space Telescope (Webb), are published in the journal Nature Astronomy.
JWST has created a map of dark matter that is twice as good as anything we have had before, and it may help unravel some of the deepest mysteries of the universe
Between late 2019 and early 2020, the red supergiant Betelgeuse showed signs of weakening that led many to wonder whether its long-expected explosion into a supernova just a few hundred light-years from the Solar System might be imminent. Other ideas were put forward, and more recently, fresh data have shed new light on the question.
It’s well established that stars with masses greater than eight to ten times that of the Sun won’t end up as white dwarfs like our Sun will. Instead, they explode as type II supernovae, leaving behind a neutron star and sometimes, if the mass is high enough, a stellar black hole.
Located roughly 650 light-years from Earth in the constellation Orion, Betelgeuse is one of these stars, and it’s clearly nearing the end of its life. It sits in the red supergiant phase, outside the main sequence on the Hertzsprung–Russell diagram.
“This systematic deviation agrees with the boost factor that the AQUAL theory predicts for kinematic accelerations in circular orbits under the Galactic external field,” Chae says in the paper.
Similar to how the Newton-Einstein theory relies on the ever-elusive particle known as dark matter, MOND contains its own limitations and challenges. Chae’s study appears to be a big +1 in the pro column for Modified Newtonian Dynamics, but the theory is still just that—a theory. It will need much more observational support before it upends our modern understanding of gravity and the universe we inhabit.
The Dark Energy Survey Collaboration collected information on hundreds of millions of galaxies across the universe using the U.S. Department of Energy-fabricated Dark Energy Camera, mounted on the U.S. National Science Foundation Víctor M. Blanco 4-meter Telescope at CTIO, a program of NSF NOIRLab. Their completed analysis combines all six years of data for the first time and yields constraints on the universe’s expansion history that are twice as tight as past analyses.
The Dark Energy Survey (DES) is an international, collaborative effort to map hundreds of millions of galaxies, detect thousands of supernovae, and find patterns of cosmic structure that will help reveal the nature of the mysterious dark energy that is accelerating the expansion of our universe.
From 2013 to 2019, the DES Collaboration carried out a deep, wide-area survey of the sky using the 570-megapixel DOE-fabricated Dark Energy Camera (DECam), mounted on the NSF Víctor M. Blanco 4-meter Telescope at NSF Cerro Tololo Inter-American Observatory (CTIO) in Chile. For 758 nights over six years, the DES Collaboration recorded information from 669 million galaxies that are billions of light-years from Earth, covering an eighth of the sky.
Scientists analyzing data from heavy ion collisions at the Large Hadron Collider (LHC)—the world’s most powerful particle collider, located at CERN, the European Organization for Nuclear Research—have new evidence that a pattern of “flow” observed in particles streaming from these collisions reflects those particles’ collective behavior. The measurements reveal how the distribution of particles is driven by pressure gradients generated by the extreme conditions in these collisions, which mimic what the universe was like just after the Big Bang.
The research is described in a paper published in Physical Review Letters by the ATLAS Collaboration at the LHC. Scientists from the U.S. Department of Energy’s (DOE) Brookhaven National Laboratory and Stony Brook University played leading roles in the analysis.
The international team used data from the LHC’s ATLAS experiment to analyze how particles flow outward in radial directions when two beams of lead ions—lead atoms stripped of their electrons—collide after circulating around the 17-mile circumference of the LHC at close to the speed of light. The findings offer new insight into the nature of the hot, dense matter generated in these collisions—with temperatures more than 250,000 times hotter than the sun’s core. These extreme conditions essentially melt the protons and neutrons that make up the colliding ions, setting free their innermost building blocks, quarks and gluons, to create a quark-gluon plasma (QGP).
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That the universe began seems astonishing. What brought it about? What forces were involved? How did the laws of nature generate the vast expanse of billions of galaxies of billions of stars and planets in the structures that we see today? What new physics was involved? What more must we learn?
John Richard Gott III is a Professor of Astrophysical Sciences at Princeton University who is noted for his contributions to cosmology and general relativity.
0:00 Is universe basically a black hole? 1:10 Defining a black hole and the universe. 2:30 How would universe end up inside a black hole? 5:00 Explanations for how this may work. 6:35 Rotation and angular momentum. 8:05 What this could explain. 9:35 Counter evidence and why it’s probably not a black hole. 13:00 Rotation explanation using the cosmic web. 14:00 Conclusions.
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