NASA's New Supercomputer Simulation Reveals Supermassive Black Holes in Spiral



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The NASA astrophysicists team has established a dramatic prediction of what happens when two supermassive black holes meet.

NASA's latest simulation helps researchers better understand how supermassive black holes work. These black holes often weigh millions, even billions of times more than our Sun, but little is known about what happens if they collide.

With the help of a supercomputer, researchers at the Goddard Space Flight Center finally have an idea of ​​what two black holes of this size would do if they interacted. The team used the physical effects established by Albert Einstein's theory of general relativity. According to NASA, the gases in these systems would primarily ignite ultraviolet rays and X-rays.

"We know that galaxies with central supermassive black holes are combining at any time in the universe, but we only see a small fraction of galaxies, two of which are close to their center," said Scott Noble, Astrophysicist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "The pairs we see are not emitting strong gravitational wave signals because they are too far apart. Our goal is to identify, with light alone, even narrower pairs from which gravitational wave signals could be detected in the future. "

The NASA team also reminded us of this rather disturbing information. Almost all galaxies the size of the Milky Way or larger have a supermassive black hole in their heart. For decades, NASA has observed these

Noble and the rest of the Goddard team published their analysis of the simulation in a recent edition of The astrophysical journal.

NASA's New Supercomputer Simulation Reveals Supermassive Black Holes in Spiral

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