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Revolutionary Study Reveals Sagittarius A* Formed from Ancient Black Hole Merger

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Discover how researchers have uncovered evidence that Sagittarius A*, the supermassive black hole at the heart of the Milky Way, likely formed from a merger of two black holes. This groundbreaking study sheds light on the dynamics of our galaxy and the universe.


Unveiling the Origins of Sagittarius A*

Researchers from the University of Nevada, Las Vegas, have unveiled compelling evidence suggesting that the supermassive black hole known as Sagittarius A*, located at the center of the Milky Way, likely formed from a cataclysmic merger between two supermassive black holes. This discovery adds a new dimension to our understanding of black hole formation and the dynamics of our galaxy.

The Size and Significance of Sagittarius A*

Sagittarius A* is an enormous entity, weighing approximately 4.3 million times the mass of the sun and situated 27,000 light-years from Earth. It is widely believed that nearly every large galaxy, including Andromeda and Messier 87, harbors a supermassive black hole at its core. The mechanisms behind their formation generally fall into two categories: the accumulation of surrounding matter or the merging of existing black holes.

Insights from the Event Horizon Telescope

Recent data from the Event Horizon Telescope reveal that Sagittarius A* rotates at an unexpectedly high rate, with its rotation misaligned from the Milky Way's angular momentum. The researchers propose that these peculiar traits can be attributed to a significant merger that occurred approximately 9 billion years ago, during which a smaller dwarf galaxy collided with the Milky Way, resulting in the fusion of their supermassive black holes. This groundbreaking study, published in Nature Astronomy, utilizes advanced computer simulations to model the merger's effects, providing insights that could influence future gravitational wave observations, particularly with the upcoming LISA observatory set to launch in 2035.

  • The study's findings emphasize the importance of understanding supermassive black hole mergers, as they can shed light on the evolution of galaxies and the universe as a whole. The proposed merger scenario, with a mass ratio of 4:1, aligns with the observed rotational characteristics of Sagittarius A*, offering a plausible explanation for its current state. As researchers continue to explore the cosmos, the implications of these discoveries could lead to revolutionary advancements in astrophysics and our comprehension of the universe's history.
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Refs: | Aljazeera |

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