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A second black hole at the Milky Way's center would have significant implications for our understanding of the galaxy and the universe as a whole. It could help explain the formation and evolution of galaxies, and shed light on the mysterious nature of black holes.
This second black hole was identified through observations of the orbit of a star called S62, which showed unusual deviations that could only be explained by the presence of a massive object, possibly a second black hole, at the Milky Way's center.
Based on current observations, the second black hole is estimated to have a mass of about 100,000 times that of our sun, making it a "supermassive" black hole. It also appears to have a highly elongated and tilted orbit, which is unusual for a black hole in the Milky Way's center.
If confirmed, this second black hole could challenge our current theories about the structure and dynamics of the Milky Way. It could also have implications for the distribution of dark matter in the galaxy and the formation of its spiral arms.
More observations and data analysis will be needed to confirm the existence of this second black hole and determine its exact properties. Future studies using advanced telescopes and technologies may also provide more insight into the nature of this potential black hole.