Under the influence of gravity, over time the dense central part of a galaxy will tend to collapse inward and form a supermassive black hole. This process is believed to occur due to the accumulation of mass within the galactic center, resulting from the merging of smaller galaxies and the accretion of matter.
As the central part of a galaxy collapses, the gravitational forces increase, causing the matter to be compressed to extreme densities. This compression results in the formation of a supermassive black hole, which is a region in space with an incredibly high gravitational pull that even light cannot escape from.
The presence of a supermassive black hole at the center of a galaxy has significant implications for its evolution. The gravitational influence of the black hole can affect the orbits of nearby stars and gas, leading to the formation of a central bulge and a disk-like structure around it. Additionally, the black hole can release tremendous amounts of energy as matter falls into it, leading to the creation of active galactic nuclei and other energetic phenomena.
In summary, under the influence of gravity, the dense central part of a galaxy will collapse and form a supermassive black hole, which shapes the structure and evolution of the galaxy.
Under the influence of gravity, over time the dense central part of a galaxy will do what
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