What is a dark galaxy?
The dark galaxy is a cluster of dark matter that cannot be visually observed because the matter does not distribute or does not affect visible light. The presence of such galaxies was supposed to be physics and astronomers who believed that the presence of these phenomena was a critical part of some theories explaining the nature of the universe. Their monitoring proved to be a problem because of their invisible nature, but the international team in 2005 managed to identify one with the help of a radio telescope. This discovery was an important development in the field of astrophysics.
According to theorists, most of the universe is actually composed of dark matter that can create gravity -bound galaxies that have more mass over time. At some point, they would theoretically reach the point of reversal, midwife and other objects to create a full -fledged galaxy. This theory is supported by the research of galaxies with unusually young stars; Scientists suspect that Thgalaxie ESE actually existed for billions of years in the form of darkthe matter.
Collecting gases and mass in a dark galaxy can still affect the surrounding objects, which is one way to see one. Scientists looking for dark galaxies were looking for visible galaxies that behave unusually, as if there was a gravitational move that could affect their shape and size. Another method of finding these elusive phenomena involves searching for signatures with a telling with a radio telescope. Although the dark galaxy does not appear in the visible spectrum, the gases it contains may emit radio waves that betray its presence.
In addition to being a general cosmological interest, the dark galaxy is an important theory and finding for physics. Theorists believed that they had to exist because they support the most general model of how the universe has created and it continues to change over time. Finding a real sample created support for their theories and also explained some phenomena inThe universe that wouldn't make sense if there were no dark galaxies.
Scientists continue to seek more evidence of dark galaxies using observations of different points in space and careful data analysis. Each dark galaxy must be confirmed before it is officially announced, and to ensure that observers do not make a notification based on defective or incomplete information. This may be a slow international process, as peers check findings in their own viewing devices and check the methods used in the initial finding.