Scientists from NASA, analyzing data collected by the Fermi Telescope, have made a discovery that turned out to be completely unexpected. The telescope recorded gigantic flashes of incredibly high-energy radiation coming from beyond the Milky Way. This discovery has sparked the interest of researchers and raises new questions about the origins of the universe.
The flashes that were observed are different from typical gamma-ray radiation. Scientists are not certain of their source, but they speculate that it may be related to gamma-ray radiation. This mysterious phenomenon could be the key to better understanding the beginnings of our universe.
Cosmic Microwave Background radiation (CMB), which is a remnant of the early universe, is well-known to scientists. Anyone with an old television set can observe it as “static” on the screen. However, analysis of the data collected by the Fermi Telescope has revealed completely random and unexpected bursts of immense energy that do not originate from our galaxy.
Now, scientists face two tasks. The first is to identify the source of these powerful bursts, which may be challenging due to the space beyond the Milky Way. The second task is to find a theoretical explanation that does not contradict existing theories about the Cosmic Microwave Background radiation. These discoveries mark another step towards answering fundamental questions about the origins of the universe.
FAQ:
What is the Big Bang Theory?
The Big Bang Theory is a scientific model that describes the beginning and evolution of the universe. It posits that the universe originated from a single point of concentrated energy and has been expanding since.
What is gamma-ray radiation?
Gamma-ray radiation is very high-energy electromagnetic waves. It originates from violent and powerful phenomena such as supernova explosions or nuclear reactions.
What is the Cosmic Microwave Background radiation?
The Cosmic Microwave Background radiation (CMB) is the remnant of the Big Bang and still exists in the universe today. It is a faint form of electromagnetic radiation that serves as one of the key pieces of evidence for the Big Bang Theory.
Source: NASA (https://www.nasa.gov)
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